CoRoT - Knowledge

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small changes in light flux. Corot is capable of detecting changes in brightness of about 1/10,000. Scientists can thus hope finding planets with a size of approximately 2 times that of the Earth with this method, a class of planet called Super-Earth; detection of Corot-7b, whose radius is 1.7 times that of the Earth has shown that these predictions were correct. CoRoT takes an exposure of 32 seconds duration, each 32 seconds, but the image is not fully transmitted to Earth because the data flow would be too large. The onboard computer performs an important work of data reduction: the field around each target star, previously selected by the exoplanets team, is defined on a certain number of pixels described by a particular mask, the sum all pixels within the mask is then performed and several exposures are added (usually 16, which amounts to an integration time of about 8 minutes) before sending this information to the ground. For some stars, considered particularly of interest, data of each exposure is transmitted every 32 seconds. Such a sampling of 32s or 512s is well suited to the detection of a planetary transit that lasts from a little less than an hour to several hours. A feature of this method is that it requires to detect at least three successive transits separated by two equal time intervals before one can consider a target as a serious candidate. A planet of orbital period

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does not mean the detection of a planet, but rather that of a binary star system, either one that corresponds to a grazing occultation of a star by the other, or that the system is close enough to a bright star (the CoRoT target) and the effect of transit is diluted by the light of this star; in both cases the decrease in brightness is low enough to be compatible with that of a planet passing in front of the stellar disk. To eliminate these cases, one performs observations from the ground using two methods: radial velocity spectroscopy and imaging photometry with a CCD camera. In the first case, the mass of the binary stars is immediately detected and in the second case one can expect to identify in the field the binary system near the target star responsible for the alert: the relative decline of brightness will be greater than the one seen by CoRoT which adds all the light in the mask defining the field of measurement. In consequence, the CoRoT exoplanet science team has decided to publish confirmed and fully characterized planets only and not simple candidate lists. This strategy, different from the one pursued by the

1147:, or an eclipsing fainter star very close to the target star, whose light, blended in the light curve, can reproduce transit-like events. A first screening is executed on the light curves, searching hints of secondary eclipses or a rather V-shaped transit, indicative of a stellar nature of the transits. For the brighter targets, the prism in front of the exoplanets CCDs provides photometry in 3 different colors, enabling to reject planet candidates that have different transit depths in the three channels, a behaviour typical of binary stars. These tests allow to discard 83% of the candidate detections, whilst the remaining 17% are screened with photometric and radial velocity follow-up from a network of telescopes around the world. Photometric observations, required to rule out a possible contamination by a diluted eclipsing binary in close vicinity of the target, is performed on several 1 m-class instruments, but also employs the 2 m 1885:): The relatively bright eclipsing system CoRoT 102918586 is a double-lined spectroscopic binary, observed by CoRoT, which revealed clear evidence of γ Doradus type pulsations. In addition to CoRoT photometry, a spectroscopic follow-up was performed which yielded the radial velocity curves, the component effective temperatures, the metallicity, and the line-of-sight projected rotational velocities. The eclipsing binary light curve analysis, combined with the spectroscopic results, provided system physical parameters with 1–2% accuracy while the comparison with evolutionary models led to constraints on the age of the system. After subtracting the best–fitting eclipsing binary model, the residuals were analyzed to determine the pulsation properties. The primary star pulsates with typical γ Dor frequencies and shows a period spacing consistent with high order g-modes of degree l=1. 1924:(also called Doppler boosting). This effect results from the variation in brightness of source approaching or moving away from the observer, with an amplitude proportional to the radial velocity divided by the speed of light. The periodic variation in the velocity of an orbiting star will thus produce a periodic beaming variation in the light curve. Such an effect can confirm the binary nature of a system even without any detectable eclipses nor transits. One of the main advantages of the beaming effect is the possibility to determine the radial velocity directly from the light curve but very different luminosities of the binary components are required and a single radial velocity curve can only be obtained as in an SB1 binary system. The out of eclipse variations were modeled with the BEER (Beaming Ellipsoidal Reflection) algorithm. 1875:: Tidally induced pulsations have been detected in the high eccentricity (e=0.29) and short period binary system HD 174884 consisting of two B stars. The upper panel of the figure shows the full light curve of the system. In the second panel tiny secondary eclipses are seen with a depth of about 1% of the depth of the primary eclipse. Actually the system is formed of stars of similar mass, size and temperature. Were the orbit circular, the eclipses would be similar in depth. However the orbit is highly eccentric and its orientation in space with respect to us is such that the secondary eclipse occurs when the stars are at a larger distance than at primary eclipse. The third panel of the figure shows the projection on the plane of the sky (i.e. the system as we see it) at different orbital phases. 1982:: the distance from the Earth to the Sun (150 million km), the mass of the Sun, the orbital period of the Earth (1 year); this implies that if the observing time is less a year, for example, the orbits of the detectable planets will be significantly smaller than that of the Earth. So, for CoRoT, due to the maximum duration of 6 months of observation for each star field, only planets closer to their stars than 0.3 Astronomic Units (less than the distance between the Sun and Mercury) can be detected, therefore generally not in the so-called habitable zone. The Kepler mission (NASA) has continuously observed the same field for many years and thus had the ability to detect Earth sized planets located farther from their stars. 4736: 1445:

helium. This region is rather thin and constitutes a sharp transition region, which induces a very subtle signature in the gravity modes frequency spectrum. Instead of a constant period spacing found in a homogeneous stellar model, periodic deviations from this constant value are expected in models affected by a sharp transition region. Moreover, the period of the deviations is directly related to the precise location of the sharp transition. This phenomenon has been detected in two hybrid B stars (showing at the same time acoustic β Cephei and gravity SPB modes): (1)

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undergoes, it always presents the same hemisphere to the star: as a consequence, the two hemispheres, the enlightened and the dark, exhibit an extreme contrast in temperature (2200K vs 50K) and a huge ocean of lava must occupy a large part of the hot side. A continent of water and nitrogen dioxide ices is probably occupying the dark side. CoRoT-7b was also the first case of a system discovered by CoRoT, with two super-Earths, one in transit the other not; radial velocity measurements have indeed led to the discovery of CoRoT-7c, a planet of 8.4 M

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frequency separation, second difference...). Transition zones introduce periodic deviations with respect to these regularities and the periods of the deviations are directly related to the precise location of the transition zones. These deviations were predicted by theory and were first observed in the Sun. Thanks to CoRoT they were also detected in the solar-like star HD 49933 and also in the red giant star HD 181907. In both cases the location of the helium ionization zone could be accurately derived.

747: 628:, in May 2007, just 3 months after the start of the observations. Mission flight operations were originally scheduled to end 2.5 years from launch but operations were extended to 2013. On 2 November 2012, CoRoT suffered a computer failure that made it impossible to retrieve any data from its telescope. Repair attempts were unsuccessful, so on 24 June 2013 it was announced that CoRoT had been retired and would be decommissioned; lowered in orbit to allow it to burn up in the atmosphere. 1548: 1301:

profile, the precise extent of the convective envelope and the location of the helium ionization zone. Despite enormous technical challenges, it was thus tempting to apply similar analyses to stars. From the ground this was only possible for stars close to the Sun such as α Centauri, Procyon, β Virginis... The goal is to detect extremely small light variations (down to 1 ppm) and to extract the frequencies responsible for these brightness fluctuations. This produces a

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Observed by CoRoT during an outburst of matter towards its circumstellar disk, which is typical of such stars, its frequency spectrum suffered drastic changes. Firstly dominated by acoustic modes the spectrum showed the appearance of gravity modes with amplitudes strictly in line with the outburst. Such a link between the nature of the excited modes and a dynamical phenomenon is of course a gold mine in the quest for the internal structure of Be stars.

2201: 1808:(PMS) δ Scuti stars and the confirmation of the existence of γ Doradus pulsations in PMS stars. Also the presence of hybrid δ Scuti/γ Doradus pulsations was confirmed in members of NGC 2264. The CoRoT observations included also the well known pre-main sequence pulsators, V 588 Mon and V 589 Mon, which were the first discovered members of this group of stars. The precision attained in the CoRoT light curves also revealed the important role of 1738:. The figure illustrates the behavior of the frequency versus time for two modes in the frequency spectrum of Chimera, a solar-like mode (top) and a β Cephei mode (bottom). The stochastic nature of the solar-like mode reveals itself in the instability of its frequency as time goes on and in the spread in frequency on several μHz. The contrast with the stability in frequency and the narrow frequency range of the β Cephei mode is striking. 47: 692: 1715: 4769: 4801: 15257: 781:, allowing up to 150 days of continuous observation. These observation sessions, called "Long Runs", allowed detection of smaller and long-period planets. During the remaining 30 days between the two main observation periods, CoRoT observed other patches of sky for a few weeks long "Short Runs", in order to analyze a larger number of stars for the asteroseismic program. After the loss of half the field of view due to 15269: 4744: 15245: 11840: 11176: 11501: 1536: 1369:, the spectacular time evolution of the frequency spectrum of a Be (emission lines B) star during an outburst, the first detection of a deviation from a constant period spacing in gravity modes in an SPB (Slowly Pulsating B) star. Interpreting those results opened new horizons in humanity's vision of stars and galaxies. In October 2009 the CoRoT mission was the subject of a special issue of 1863: 1314: 1773:

earliest phases in stellar evolution. Therefore, in December 2011 and January 2012, CoRoT was part of a large international observing campaign involving four space telescopes and several ground-based observatories. All instruments observed about 4000 stars in the young cluster NGC 2264 simultaneously for about one month at different wavelengths. The Canadian space mission

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periodically occurring minima that are different in depth and width, hence are semi-regular variables. With the CoRoT observations this class of objects could be established. Exciting insights into the earliest phases of stellar evolution also come from the comparison of the variability present in the optical light to that in the infrared and the X-ray regime.

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P.; Bouchy, F.; Cabrera, J.; Díaz, R. F.; Dvorak, R.; Erikson, A.; Guillot, T.; Hatzes, A.; Hébrard, G.; Mazeh, T.; Montagnier, G.; Ofir, A.; Ollivier, M.; Pätzold, M.; Rauer, H.; Rouan, D.; Santerne, A.; Schneider, J. (1 February 2014). "Transiting exoplanets from the CoRoT space mission XXV. CoRoT-27b: a massive and dense planet on a short-period orbit".

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of gravity-dominated modes are expected to be especially meaningful. Their detection for a large number of red giants could give us clues to establishing the extent of the extra-mixed region above the convective core during core hydrogen burning, but also the extent of the extra-mixed region during core helium burning, both mixing processes being

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tension. Similarly, stellar pulsation modes are characteristic of global stellar properties and of the internal physical conditions. Analyzing these modes is thus a way of probing stellar interiors to infer stellar chemical composition, rotation profiles and internal physical properties such as temperatures and densities.

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Bonomo, A. S; Santerne, A; Alonso, R; Gazzano, J.-C; Havel, M; Aigrain, S; Auvergne, M; Baglin, A; Barbieri, M; Barge, P; Benz, W; Bordé, P; Bouchy, F; Bruntt, H; Cabrera, J; Cameron, A. C; Carone, L; Carpano, S; Csizmadia, Sz; Deleuil, M; Deeg, H. J; Dvorak, R; Erikson, A; Ferraz-Mello, S; Fridlund,

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Barge, P; Baglin, A; Auvergne, M; Rauer, H; Léger, A; Schneider, J; Pont, F; Aigrain, S; Almenara, J.-M; Alonso, R; Barbieri, M; Bordé, P; Bouchy, F; Deeg, H. J; La Reza, De; Deleuil, M; Dvorak, R; Erikson, A; Fridlund, M; Gillon, M; Gondoin, P; Guillot, T; Hatzes, A; Hebrard, G; Jorda, L; Kabath, P;

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found on average between 200 and 300 cases of periodic events for each run, corresponding to 2–3% of the stars monitored. Of these, only 530 in total were selected as candidate planets (223 in the direction of the galactic anti-center and 307 towards the center). Only 30 of them were finally found to

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To find extra solar planets, CoRoT uses the method of transits detection. The primary transit is the occultation of a fraction of the light from a star when a celestial object, such as a planet, passes between the star and the observer. Its detection is made possible by the sensitivity of CCD to very

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The light curve of HD 174884. The upper panel shows the full light curve. The second panel is a blow-up where tiny secondary minima are visible (their depth is 1% of the deeper minimum). The third panel shows the projection on the plane of the sky (i.e. as we see the system) at different phases. From

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type objects. Previously to the CoRoT observations, T Tauri stars were known to either show sinusoidal light variations that are caused by spots on the stellar surface, or completely irregular variability that is caused by the gas and dust disks surrounding the young stars. AA Tauri type objects show

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Another unexpected CoRoT discovery was the presence of solar-like oscillations in massive stars. The small convective shell related to the opacity peak resulting from the ionization of iron group elements at about 200 000 K (iron opacity peak) could indeed be responsible for the stochastic excitation

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Many O stars have been observed by CoRoT. Among them HD 46150 and HD 46223 (members of the galactic cluster NGC 2264) and HD 46966 (member of the OB association Mon OB2) do not seem to pulsate, which is in agreement with stellar modeling of stars with similar global parameters. The frequency spectrum

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at work in layers where partial ionization of iron group elements produce a peak in opacity. In addition the most advanced of these stars present mixed modes i.e. modes with a g-character in deep layers and p-character in the envelope. Hydrogen burning takes place in a convective core surrounded by a

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Whether RGB or RC, these stars all have an extended convective envelope favorable to the excitation of solar-like oscillations. A major success of CoRoT has been the discovery of radial and long-lived non-radial oscillations in thousands of red giants in the exo field. For each of them, the frequency

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The presence of granulation was detected in the frequency spectrum of HD 49933. Analyses have been done with 3D hydrodynamical model atmospheres computed at solar and ten times smaller than solar metallicities. Here again the model with the lowest metallicity shows up to be closer to the observations

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Transition layers such as the helium ionization region or the lower boundary of the convective envelope in low mass and red giant stars also affect frequency spectra. In a structure devoid of such discontinuities, high order acoustic modes obey some regularities in their frequency distribution (large

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at work in layers where ionizations of iron group elements produces an opacity peak. In such stars, the convective core is surrounded by a region of varying chemical composition, the so-called μ-gradient region, left by the progressive withdrawal of the convective core as hydrogen is transformed into

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Parviainen, H.; Gandolfi, D.; Deleuil, M.; Moutou, C.; Deeg, H. J.; Ferraz-Mello, S.; Samuel, B.; Csizmadia, Sz; Pasternacki, T.; Wuchterl, G.; Havel, M.; Fridlund, M.; Angus, R.; Tingley, B.; Grziwa, S.; Korth, J.; Aigrain, S.; Almenara, J. M.; Alonso, R.; Baglin, A.; Barros, S. C. C.; Bordé, A. S.

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Pätzold, M; Endl, M; Csizmadia, Sz; Gandolfi, D; Jorda, L; Grziwa, S; Carone, L; Pasternacki, T; Aigrain, S; Almenara, J. M; Alonso, R; Auvergne, M; Baglin, A; Barge, P; Bonomo, A. S; Bordé, P; Bouchy, F; Cabrera, J; Cavarroc, C; Cochran, W. B; Deleuil, M; Deeg, H. J; Díaz, R; Dvorak, R; Erikson, A;

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Guenther, E. W; Díaz, R. F; Gazzano, J.-C; Mazeh, T; Rouan, D; Gibson, N; Csizmadia, Sz; Aigrain, S; Alonso, R; Almenara, J. M; Auvergne, M; Baglin, A; Barge, P; Bonomo, A. S; Bordé, P; Bouchy, F; Bruntt, H; Cabrera, J; Carone, L; Carpano, S; Cavarroc, C; Deeg, H. J; Deleuil, M; Dreizler, S; Dvorak,

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Ollivier, M; Gillon, M; Santerne, A; Wuchterl, G; Havel, M; Bruntt, H; Bordé, P; Pasternacki, T; Endl, M; Gandolfi, D; Aigrain, S; Almenara, J. M; Alonso, R; Auvergne, M; Baglin, A; Barge, P; Bonomo, A. S; Bouchy, F; Cabrera, J; Carone, L; Carpano, S; Cavarroc, C; Cochran, W. D; Csizmadia, Sz; Deeg,

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Tingley, B; Endl, M; Gazzano, J.-C; Alonso, R; Mazeh, T; Jorda, L; Aigrain, S; Almenara, J.-M; Auvergne, M; Baglin, A; Barge, P; Bonomo, A. S; Bordé, P; Bouchy, F; Bruntt, H; Cabrera, J; Carpano, S; Carone, L; Cochran, W. D; Csizmadia, Sz; Deleuil, M; Deeg, H. J; Dvorak, R; Erikson, A; Ferraz-Mello,

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Gandolfi, D; Hébrard, G; Alonso, R; Deleuil, M; Guenther, E. W; Fridlund, M; Endl, M; Eigmüller, P; Csizmadia, Sz; Havel, M; Aigrain, S; Auvergne, M; Baglin, A; Barge, P; Bonomo, A. S; Bordé, P; Bouchy, F; Bruntt, H; Cabrera, J; Carpano, S; Carone, L; Cochran, W. D; Deeg, H. J; Dvorak, R; Eislöffel,

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Fridlund, M; Hébrard, G; Alonso, R; Deleuil, M; Gandolfi, D; Gillon, M; Bruntt, H; Alapini, A; Csizmadia, Sz; Guillot, T; Lammer, H; Aigrain, S; Almenara, J. M; Auvergne, M; Baglin, A; Barge, P; Bordé, P; Bouchy, F; Cabrera, J; Carone, L; Carpano, S; Deeg, H. J; de la Reza, R; Dvorak, R; Erikson, A;

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Alonso, R; Auvergne, M; Baglin, A; Ollivier, M; Moutou, C; Rouan, D; Deeg, H. J; Aigrain, S; Almenara, J. M; Barbieri, M; Barge, P; Benz, W; Bordé, P; Bouchy, F; de la Reza, R; Deleuil, M; Dvorak, R; Erikson, A; Fridlund, M; Gillon, M; Gondoin, P; Guillot, T; Hatzes, A; Hébrard, G; Kabath, P; Jorda,

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The moderate number of exoplanets discovered by CoRoT (34 during the 6 years of operation), is explained by the fact that a confirmation should absolutely be provided by ground-based telescopes, before any announcement is made. Indeed, in the vast majority of cases, the detection of several transits

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typical of the star under scrutiny. Oscillation periods vary from a few minutes to several hours depending on the type of star and its evolutionary state. To reach such performances, long observing times devoid of day/night alternations are required. Space is thus the ideal asteroseismic laboratory.

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Gillon, M; Hatzes, A; Csizmadia, Sz; Fridlund, M; Deleuil, M; Aigrain, S; Alonso, R; Auvergne, M; Baglin, A; Barge, P; Barnes, S. I; Bonomo, A. S; Bordé, P; Bouchy, F; Bruntt, H; Cabrera, J; Carone, L; Carpano, S; Cochran, W. D; Deeg, H. J; Dvorak, R; Endl, M; Erikson, A; Ferraz-Mello, S; Gandolfi,

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Rauer, H; Queloz, D; Csizmadia, Sz; Deleuil, M; Alonso, R; Aigrain, S; Almenara, J. M; Auvergne, M; Baglin, A; Barge, P; Bordé, P; Bouchy, F; Bruntt, H; Cabrera, J; Carone, L; Carpano, S; de la Reza, R; Deeg, H. J; Dvorak, R; Erikson, A; Fridlund, M; Gandolfi, D; Gillon, M; Guillot, T; Guenther, E;

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Its orbital period (i.e. its local year) is very short since it lasts just 20.5 h; because the planet is very close to its star (an almost solar type star), its orbit is a mere 6 stellar radii. As the planet must be in synchronous rotation with its orbital motion because of the huge tidal forces it

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mission, where the candidates are regularly updated and made available to the public, is quite lengthy. On the other hand, the approach also increases the scientific return of the mission, as the set of published CoRoT discoveries constitute some of the best exoplanetary studies carried out so far.

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The stellar births and the stars' childhoods remain mostly hidden from us in the optical light because the early stars are deeply embedded in the dense molecular cloud from which they are born. Observations in the infrared or X-ray enable us to look deeper into the cloud, and learn more about these

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relatively close to us at a distance of about 1800 light years. Its age is estimated to be between 3 and 8 million years. At such a young age, the cluster is an ideal target to investigate many different scientific questions connected to the formation of stars and early stellar evolution. The CoRoT

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acting in the iron opacity peak zone were present side by side in the same star with pulsations stochastically excited by this very same zone. This is the reason why Kevin Belkacem, main discoverer of these solar-like oscillations in V1449 Aquilae, added a new baptismal certificate to this β Cephei

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frequency spectra of red giants brought new important discoveries. Small and subtle differences in seismic signatures allow us to distinguish RGB from RC stars notwithstanding their similar luminosities. This is now theoretically confirmed thanks to elaborate red giant modeling. The period spacings

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The age of a red giant is closely related to its former main sequence lifetime, which is in turn determined by its mass and metallicity. Knowing the mass of a red giant amounts to knowing its age. If the metallicity is known the uncertainty in age does not exceed 15%! Observational missions such as

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and collaborators noticed that both types of histograms were spitting images of one another, as can be seen in the histograms picture. Moreover, adding the knowledge of the distances of these thousands of stars to their galactic coordinates, a 3D map of this galaxy was drawn. This is illustrated in

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variations associated with acoustic pulsations of stars. This phenomenon allows calculation of a star's precise mass, age and chemical composition and will aid in comparisons between the sun and other stars. For this program, in each field of view there was one main target star for asteroseismology

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Cabrera, J; Bruntt, H; Ollivier, M; Díaz, R. F; Csizmadia, Sz; Aigrain, S; Alonso, R; Almenara, J.-M; Auvergne, M; Baglin, A; Barge, P; Bonomo, A. S; Bordé, P; Bouchy, F; Carone, L; Carpano, S; Deleuil, M; Deeg, H. J; Dvorak, R; Erikson, A; Ferraz-Mello, S; Fridlund, M; Gandolfi, D; Gazzano, J.-C;

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Bordé, P; Bouchy, F; Deleuil, M; Cabrera, J; Jorda, L; Lovis, C; Csizmadia, S; Aigrain, S; Almenara, J. M; Alonso, R; Auvergne, M; Baglin, A; Barge, P; Benz, W; Bonomo, A. S; Bruntt, H; Carone, L; Carpano, S; Deeg, H; Dvorak, R; Erikson, A; Ferraz-Mello, S; Fridlund, M; Gandolfi, D; Gazzano, J.-C;

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Following exhaustion of hydrogen in the core, the overall stellar structure drastically changes. Hydrogen burning now takes place in a narrow shell surrounding the newly processed helium core. While the helium core quickly contracts and heats up, the layers above the hydrogen-burning shell undergo

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Aigrain, S; Collier Cameron, A; Ollivier, M; Pont, F; Jorda, L; Almenara, J. M; Alonso, R; Barge, P; Bordé, P; Bouchy, F; Deeg, H; de la Reza, R; Deleuil, M; Dvorak, R; Erikson, A; Fridlund, M; Gondoin, P; Gillon, M; Guillot, T; Hatzes, A; Lammer, H; Lanza, A. F; Léger, A; Llebaria, A; Magain, P;

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Deleuil, M; Deeg, H. J; Alonso, R; Bouchy, F; Rouan, D; Auvergne, M; Baglin, A; Aigrain, S; Almenara, J. M; Barbieri, M; Barge, P; Bruntt, H; Bordé, P; Collier Cameron, A; Csizmadia, Sz; de la Reza, R; Dvorak, R; Erikson, A; Fridlund, M; Gandolfi, D; Gillon, M; Guenther, E; Guillot, T; Hatzes, A;

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Late Be type stars HD 181231 and HD 175869 are very rapid rotators, about 20 times more rapid than the Sun. Their seismic analysis seems to require a centrally mixed zone about 20% larger than what is expected from convection only. Another Be star, HD 49330, had a very exciting surprise in store.

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Tracing the mass of the planet versus the mass of the star (Figure), one finds that the CoRoT data set, with its lower scatter than other experiments, indicates a clear trend that massive planets tend to orbit massive stars, which is consistent with the most commonly accepted models of planetary

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and those which face a final supernova explosion. The impact on the chemical evolution of the galaxy is obvious. Physical reasons for this extra-mixing are various, either a mixing induced by internal rotation or a mixing resulting from convective bubbles crossing the convective core boundary to

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as well as the mixing efficiency are, however, difficult to assess. This additional mixing has very important consequences since it involves longer time scales for nuclear burning phases and may in particular affect the value of the stellar mass at the transition between those stars which end up

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Papers presenting the results of follow-up operations of planetary candidates in the IRa01, LRc01, LRa01, SRc01 fields have been published. In April 2019, a summary of the exoplanet search results have been published, with 37 planets and brown dwarves confirmed, and a further one hundred planet

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Later on solar-like oscillations were even discovered in a more massive O star member of the binary system HD 46149. Constraints coming from the binary nature of the system coupled with seismic constraints led to the determination of the orbital parameters of the system as well as to the global

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This CoRoT target is a β Cephei star whose frequency spectrum reveals high frequency and very small amplitude acoustic modes. A careful analysis has shown that they were solar-like oscillations excited by turbulent bubbles origination from this convective iron opacity peak zone or even from the

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Deleuil, M; Bonomo, A. S; Ferraz-Mello, S; Erikson, A; Bouchy, F; Havel, M; Aigrain, S; Almenara, J.-M; Alonso, R; Auvergne, M; Baglin, A; Barge, P; Bordé, P; Bruntt, H; Cabrera, J; Carpano, S; Cavarroc, C; Csizmadia, Sz; Damiani, C; Deeg, H. J; Dvorak, R; Fridlund, M; Hébrard, G; Gandolfi, D;

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One of the major successes of the CoRoT space mission has definitely been the detection of solar-like oscillations in stars slightly hotter than the Sun. As was previously done for the Sun, measurements of amplitudes and line widths in their frequency spectra resulted in new constraints in the

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and has been ongoing for a few decades by now. The solar surface helium abundance was derived very accurately for the first time, which has definitely shown the importance of microscopic diffusion in the solar structure. Helioseismology analyses have also unveiled the solar internal rotational

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On 8 March 2009 the satellite suffered a loss of communication with Data Processing Unit No. 1, processing data from one of the two photo-detector chains on the spacecraft. Science operations resumed early April with Data Processing Unit No. 1 offline while Data Processing Unit No. 2 operating

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could then be drawn and a totally unexpected and spectacular result came out when comparing these CoRoT histograms with theoretical ones obtained from theoretical synthetic populations of red giants in this galaxy. Such theoretical populations were computed from stellar evolution models, with

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Stars vibrate according to many different pulsation modes in much the same way that musical instruments emit a variety of sounds. Listening to an air on the guitar does not leave any doubt as to the nature of the instrument, and an experienced musician can even deduce the cords' material and

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containing a red giant and a B star was observed by CoRoT during two runs, which allowed us to fully cover the primary as well as the secondary eclipses. This system is presently being analyzed with the ultimate goal of bringing new constraints on the internal structure of the red giant in

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region of varying chemical composition and an envelope mostly radiative except for tiny convective layers related to partial ionization of helium and/or iron group elements. As in lower mass stars the extent of the fully or partially mixed region located just above the convective core

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data of stars in NGC 2264 allow us to study the interaction of recently formed stars with their surrounding matter, the rotation and activity of cluster members as well as their distribution, the interiors of young stars by using asteroseismology, and planetary and stellar eclipses.

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The primary contractor for the construction of the CoRoT vehicle was CNES, to which individual components were delivered for vehicle assembly. The CoRoT equipment bay, which houses the data acquisition and pre-processing electronics, was constructed by the LESIA Laboratory at the

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The rate of discoveries of transiting planets is dictated by the need of ground-based, follow-up observations, needed to verify the planetary nature of the transit candidates. Candidate detections have been obtained for about 2.3% of all CoRoT targets, but finding

4776:

The detection capabilities of Corot are illustrated by the figure D showing the depth of the transits measured for all candidates, depending on the period and the brightness of the star: there is indeed a better ability to detect small planets (up to 1.5 R

2204:

Artist's impression of CoRoT-7b, the first rocky Super-Earth ever discovered thanks to a good estimate of its size and mass and therefore its density. The image shows the ocean of lava that must exist on the hemisphere that faces the star. Author: Fabien

5579: 1219:

candidates still to be verified. Sometimes the faintness of the target star or its characteristics, such as a high rotational velocity or strong stellar activity, do not allow to determine unambiguously the nature or the mass of the planetary candidate.

1345:

are nice extras in addition to the main asteroseismic program. This exo field also turned out to be of incalculable richness in asteroseismic discoveries. During the first six years of its mission, CoRoT has observed about 150 bright stars in the

1089:. According to the press release announcing the first results, CoRoT's instruments are performing with higher precision than had been predicted, and may be able to find planets down to the size of Earth with short orbits around small stars. The 4747:

Diagram of the mass of the star as a function of the planetary mass for CoRoT planets (red) and the other planets discovered by the transit method (yellow). The line across CoRoT data indicates a trend: massive planets are found around massive

1093:

requires the detection of at least two transits, hence the planets detected will mostly have an orbital period under 75-day. Candidates that show only one transit have been found, but uncertainty remains about their exact orbital period.

712:

in size which corresponds to an angular pixel size of 2.32 arcsec. The CCDs are cooled to −40 °C (233.2 K; −40.0 °F). These detectors are arranged in a square pattern with two each dedicated to the planetary detection and

1619:

could of course widely benefit from these seismic gravities with the ultimate output of establishing the age-metallicity relation in this galaxy. Asteroseismology has crossed the doorstep of the structure and chemical evolution of this

1478:

of acoustic modes by turbulent convection. The frequency spectrum of HD 49933 was confronted to the stochastic excitation model developed by Samadi et al. Except at high frequencies, a good agreement can be reached by adopting a

4784:

The CoRoT planets cover the wide range of properties and features found in the disparate family of exoplanets: for instance, the masses of CoRoT planets cover a range of almost four orders of magnitude, as shown on Figure.

824:

as possible. In addition, in order to optimize the observations, the fields had to not be too sparse – fewer targets observed – or too crowded – too many stars overlapping. Several fields were observed during the mission:

1844:

type, were discovered during CoRoT runs. The eclipse phenomenon plays a key role since global parameters can immediately follow, bringing invaluable constraints, in addition to the seismic ones, to stellar modeling.

695:

The focal plane of CoRoT with its four full frame transfer CCD. The dark zone corresponds to the photo-sensitive area. Two CCDs are dedicated to the exoplanet programme and the two other ones to the asteroseismology

5583: 996:

range from 11 to 16 for the extrasolar planet study. In fact, stellar targets brighter than 11 saturated the exoplanets CCD detectors, yielding inaccurate data, whilst stars dimmer than 16 do not deliver enough

2227:

one, this is the first transiting temperate planet found known to be similar to those within the Solar System. At the time of the discovery, it was the second longest period exoplanet found in transit, after

1241:

of degree l and azimuthal order m. Some examples are presented here below with a color scheme in which blue (red) indicates contracting (expanding) material. The pulsation amplitudes are highly exaggerated.

1183:

is performed on the host star, in order to accurately determine the stellar parameters, from which further exoplanet characteristics can be derived. Such work is done with large aperture telescopes, as the

1084:

Before the beginning of the mission, the team stated with caution that CoRoT would only be able to detect planets few times larger than Earth or greater, and that it was not specifically designed to detect

1688:

shows that this star although rapidly rotating, which would favor extra-mixing, could be devoid of such a region. The magnetic field detected in this star could be the reason of this lack of extra-mixing.

12853: 2245:

CoRoT-10b, CoRoT-16b, CoRoT-20b, CoRoT-23b, four hot Jupiters which are on an eccentric orbits, despite circularization is theoretically predicted for such small orbits: this is a clear constraint on Q

12351: 1365:

in stars other than the Sun, the first detection of non-radial oscillations in red giant stars, the detection of solar-like oscillations in massive stars, the discovery of hundreds of frequencies in

1785:

measured at the same time the stars in the infrared (for 30 days) and the X-ray domains (for 300 kiloseconds). Ground-based observations were taken also at the same time, for example, with the ESO

808:, called CoRoTsky, with data about the stars located in these two patches of sky. This allowed selecting the best fields for observation: the exoplanet research program requires a large number of 1101:. The chances of seeing a planet transiting its host star is inversely proportional to the diameter of the planet's orbit, thus close in planets detections will outnumber outer planets ones. The 15447: 1097:

CoRoT should be assumed to detect a small percentage of planets within the observed star fields, due to the low percentage of exoplanets that would transit from the angle of observation of the

11032:

Csizmadia, Sz.; et al. (2015). "Transiting exoplanets from the CoRoT space mission: XXVIII. CoRoT-33b, an object in the brown dwarf desert with 2:3 commensurability with its host star".

4772:

Fig D. The timing and transit depth of all CoRoT planet candidates (courtesy A. Santerne). The size of the symbols indicates the apparent brightness of its parent star (small meaning faint).

12818: 2040:

was announced, which at the time was the smallest exoplanet to have its diameter confirmed, at 1.58 Earth diameters. The discoveries of a second non-transiting planet in the same system,

1777:

targeted the brightest stars in the cluster in the optical light, while CoRoT observed the fainter members. MOST and CoRoT observed NGC 2264 continuously for 39 days. The NASA satellites

11294: 10781:

Cabrera, J.; Csizmadia, Sz.; Montagnier, G.; Fridlund, M.; Ammler-von Eiff, M.; Chaintreuil, S.; Damiani, C.; Deleuil, M.; Ferraz-Mello, S.; Ferrigno, A.; Gandolfi, D. (1 July 2015).

1860:

for the orbital motion as well as for another long term variation were derived. This long period variation seems to originate from a periodic light attenuation by circumstellar dust.

8716:

Maceroni, C.; Cardini, D.; Damiani, C.; Gandolfi, D.; Debosscher, J.; Hatzes, A.; Guenther, E. W.; Aerts, C. (2010). "Eclipsing binaries with pulsating components: CoRoT 102918586".

785:

of Data Processing Unit No. 1 in March 2009, the observation strategy changed to 3 months observing runs, in order to optimize the number of observed stars and detection efficiency.

1072:(CSL) in Belgium, the IWF in Austria, the DLR (Berlin) in Germany and the ESA Research and Science Support Department. The 30 cm afocal telescope Corotel has been realized by 1684:. It would be extremely interesting to establish a relation between the extent of this zone and the rotation velocity and/or the magnetic field of the star. Seismic analysis of 2183:, being less massive than 25 Jupiter masses, is classified as an exoplanet. In an August 2010 paper, CoRoT detected the ellipsoidal and the relativistic beaming effects in the 14075: 14826: 11577: 10724:"The GAPS Programme with HARPS-N at TNG . XIV. Investigating giant planet migration history via improved eccentricity and mass determination for 231 transiting planets" 14176: 11433: 14673: 12743: 11696: 1571:

Introducing these seismic signatures, together with an estimation of the effective temperature, in the scaling laws relating them to the global stellar properties,

1564:

in the frequency spectrum as well as the large frequency separation between consecutive modes Δν could be measured, defining a sort of individual seismic passport.

14851: 8737:

Maceroni, C.; Montalbán, J.; Gandolfi, D.; Pavlovski, K.; Rainer, M. (2013). "CoRoT 102918586: a γ Doradus pulsator in a short-period eccentric eclipsing binary".

1317:

Dwarf and giant stars observed by CoRoT in the sismo and exo fields with some additional stars observed from the ground. From the work of members of the CoRoT team

5540: 10783:"Transiting exoplanets from the CoRoT space mission. XXVII. CoRoT-28b, a planet orbiting an evolved star, and CoRoT-29b, a planet showing an asymmetric transit" 10282:

Hebrard; et al. (2011). "Transiting exoplanets from the CoRoT space mission. XVIII. CoRoT-18b: A massive hot jupiter on a prograde, nearly aligned orbit".

1856:

interacting with its G star companion. Its observation by CoRoT provided an extremely high quality lightcurve. Global parameters could then be improved and new

14218: 8935:

Faigler, S.; et al. (2012). "Seven New Binaries Discovered in the Kepler Light Curves through the BEER Method Confirmed by Radial-velocity Observations".

1321:

At the beginning of the mission, two out of four CCDs were assigned to asteroseismic observations of bright stars (apparent magnitude 6 to 9) in the so-called

10722:

Bonomo, A. S.; Desidera, S.; Benatti, S.; Borsa, F.; Crespi, S.; Damasso, M.; Lanza, A. F.; Sozzetti, A.; Lodato, G.; Marzari, F.; Boccato, C. (1 June 2017).

11530: 11453: 10548:

Parviainen, H.; et al. (2014). "Transiting exoplanets from the CoRoT space mission XXV. CoRoT-27b: A massive and dense planet on a short-period orbit".

14958: 15635: 13800: 13506: 13482: 11403: 5514: 1060:

to complete. The design and building of the instruments were done by the Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA) de l'

15639: 14299: 13562: 12733: 11463: 11218: 1105:

is also biased toward large planets, since their very depth transits are more easily detected than the shallows eclipses induced by terrestrial planets.

1005:

with a radius two times larger than Earth, orbiting stars brighter than 14; it is also expected to discover new gas giants in the whole magnitude range.

10657:

Pallé, E.; Chen, G.; Alonso, R.; Nowak, G.; Deeg, H.; Cabrera, J.; Murgas, F.; Parviainen, H.; Nortmann, L.; Hoyer, S.; Prieto-Arranz, J. (1 May 2016).

1483:

ten times smaller than the solar metallicity. With the solar value on the contrary, disagreements in amplitudes can reach a factor 2 at low frequencies.

1130:

of the satellite is thus reduced by 50%, but without any degradation of the quality of the observations. The loss of channel 1 appears to be permanent.

15663: 15655: 15305: 12823: 1383:

Above the convective core where mixing of chemicals is instantaneous and efficient, some layers can be affected by partial or total mixing during the

14964: 14166: 12970: 6584: 5370: 1375:, dedicated to the early results of the probe. Below are some examples of breakthrough contributions to stellar astrophysics, based on CoRoT's data: 14952: 1718:

Frequency versus time for a solar-like mode (top) and a beta Cephei mode (bottom) in Chimera. From Kevin Belkacem, Frédéric Baudin and collaborators

1581: 1552: 1540: 15667: 11087: 16047: 15387: 14599: 13972: 12699: 10493:

Rouan, D.; et al. (2011). "Transiting exoplanets from the CoRoT space mission – XIX. CoRoT-23b: A dense hot Jupiter on an eccentric orbit".

8602:

Alencar, S.H.P.; et al. (2010). "Accretion dynamics and disk evolution in NGC 2264: a study based on CoRoT photometric observations".

15745: 14085: 12516: 8129:"Asteroseismology of the β Cephei star ν Eridani: massive exploration of standard and non-standard stellar models to fit the oscillation data" 2168:

became the first exoplanets to have its secondary eclipse detected in the optical, thanks to the high precision lightcurve delivered by CoRoT.

1664:

stars show that it is not obvious to derive a one-to-one extent of this extra-mixed zone. A rather large extent seems to be required to model

15750: 15702: 15492: 14055: 11878: 11304: 4826: 9723:

A. Léger; D. Rouan (2009). "Transiting exoplanets from the CoRoT space mission VIII. CoRoT-7b: the first Super-Earth with measured radius".

8439:

Zwintz, K.; et al. (2013). "Regular frequency patterns in the young δ Scuti star HD 261711 observed by the CoRoT and MOST satellites".

4739:

Distribution of CoRoT planets (red circles) in the Radius / Mass diagram. Yellow symbols are the other planets discovered by transit methods

1575:(seismic gravities), masses and radii can be estimated and luminosities and distances immediately follow for those thousands of red giants. 988:

The spacecraft monitored the brightness of stars over time, searching for the slight dimming that happens in regular intervals when planets

15880: 15791: 15659: 9277:

Schneider, J; Dedieu, C; Le Sidaner, P; Savalle, R; Zolotukhin, I (2011). "Defining and cataloging exoplanets: the exoplanet.eu database".

7956:"An asteroseismic study of the β Cephei star 12 Lacertae: multisite spectroscopic observations, mode identification and seismic modelling" 5681:

Deeg, H. G.; et al. (2009). "Ground-based photometry of space-based transit detections: Photometric follow-up of the CoRoT mission".

5006: 15907: 15671: 15631: 15611: 15533: 12793: 11711: 11428: 10977:

Bouchy, F.; et al. (2010). "Transiting exoplanets from the CoRoT space mission. XV. CoRoT-15b: A brown dwarf transiting companion".

4696: 4634: 4295: 4238: 4173: 4116: 4059: 3998: 3948: 804:. Both these "eyes" of CoRoT have been studied in preliminary observations carried out between 1998 and 2005, allowing the creation of a 13379: 10227:

Csizmadia; et al. (2011). "Transiting exoplanets from the CoRoT space mission XVII. The hot Jupiter CoRoT-17b: A very old planet".

9668:

Ferraz-Mello, S; Guenther, E; Gondoin, P; Den Hartog, R; et al. (2010). "Transiting exoplanets from the CoRoT space mission".

6464: 15903: 15647: 14234: 13339: 12415: 12407: 11843: 9956:

J; Erikson, A; Ferraz-Mello, S; Gazzano, J.-C; Gibson, N. B; et al. (2010). "Transiting exoplanets from the CoRoT space mission".

6488:

Benomar, O.; et al. (2010). "Spectrum analysis and seismic interpretation of a solar-like pulsator (HD 49933) observed by CoRoT".

4668: 4606: 4268: 4211: 4146: 4089: 4032: 3675: 1450: 1446: 1427: 1017:

as well as up to nine other targets. The number of observed targets have dropped to half after the loss of Data Processing Unit No. 1.

10068:

Gillon, M; Guenther, E. W; Guillot, T; Hatzes, A; Havel, M; et al. (2010). "Transiting exoplanets from the CoRoT space mission".

16022: 15939: 15919: 15915: 15849: 15766: 12890: 12843: 12190: 11388: 11376: 9115: 820:

are too shallow to be detectable. The asteroseismic program required stars brighter than magnitude 9, and to cover as many different

10338:

R; Erikson, A; Ferraz-Mello, S; Fridlund, M; Gandolfi, D; et al. (2012). "Transiting exoplanets from the CoRoT space mission".

9332:

Tsevi Mazeh; Simchon Faigler (2010). "Detection of the ellipsoidal and the relativistic beaming effects in the CoRoT-3 lightcurve".

5989:

Deleuil, Magali; Fridlund, Malcolm (2018). "CoRoT: The First Space-Based Transit Survey to Explore the Close-in Planet Population".

4331:

The following table illustrates brown dwarfs detected by CoRoT as well as non-transiting planets detected in the follow-up program:

2223:

CoRoT-9b, the first planet that has earned the epithet of a temperate planet. With 80% of Jupiter mass, and an orbit similar to the

15740: 15651: 15615: 12113: 11438: 11408: 11269: 10394:

Gillon, M; Guenther, E; Guillot, T; Hatzes, A; Jorda, L; et al. (2012). "Transiting exoplanets from the CoRoT space mission".

15988:

are underlined. Launch failures are marked with the † sign. Payloads deployed from other spacecraft are (enclosed in parentheses).

10124:

S; Fridlund, M; Gandolfi, D; Gillon, M; Guenther, E. W; et al. (2011). "Transiting exoplanets from the CoRoT space mission".

9500:

Hébrard, G; Jorda, L; Lammer, H; Léger, A; Llebaria, A; et al. (2008). "Transiting exoplanets from the CoRoT space mission".

7640:"An asteroseismic study of the Cephei star Ophiuchi: constraints on global stellar parameters and core overshooting" 7059:

Hekker, S.; et al. (2009). "Characteristics of solar-like oscillations in red giants observed in the CoRoT exoplanet field".

15799: 15770: 14201: 11211: 15205: 14916: 8849:

Maceroni, C.; et al. (2009). "HD 174884: a strongly eccentric, short-period early-type binary system discovered by CoRoT".

1333:, interesting science on stars was also obtained from the exoplanets channel data, where the probe records several thousands of 15833: 15298: 15248: 15114: 14186: 13880: 13625: 13131: 12439: 10180:

H. J; Deleuil, M; Diaz, R. F; Dvorak, R; Erikson, A; et al. (2012). "Transiting exoplanets from the CoRoT space mission".

10012:

D; Gazzano, J. C; Guenther, E; Guillot, T; Havel, M; et al. (2010). "Transiting exoplanets from the CoRoT space mission".

8549:

Zwintz, K.; et al. (2011). "PULSATIONAL ANALYSIS OF V 588 MON AND V 589 MON OBSERVED WITH THE MOST AND CoRoT SATELLITES".

6255:

Degroote, P.; et al. (2010). "Detection of frequency spacings in the young O-type binary HD 46149 from CoRoT photometry".

1516:. Once their central temperature reaches 100 10 K, helium starts burning in the core. For stellar masses smaller than about 2 M 1152: 1143:

transit events isn't enough to claim a planet discovery, since several configurations could mimic a transiting planet, such as

9900:

M; Gandolfi, D; Gillon, M; Guenther, E; Guillot, T; et al. (2010). "Transiting exoplanets from the CoRoT space mission".

6847:

Benomar, O.; et al. (2009). "A fresh look at the seismic spectrum of HD49933: analysis of 180 days of CoRoT photometry".

5037: 1434:

was submitted to CoRoT scrutiny and although not fully conclusive, new constraints were brought to the modeling of such stars.

14196: 13795: 12222: 12161: 11614: 11341: 7767: 6016: 621: 74: 5068: 2179:

and a planet." According to the definition of planet proposed by the owners of the exoplanet.eu database three years later,

16052: 15371: 14239: 13660: 13652: 13594: 12720: 9779:

Gillon, M; Guenther, E; Guillot, T; Guterman, P; et al. (2010). "Transiting exoplanets from the CoRoT space mission".

5736:

Santerne, A.; et al. (CoRoT radial velocity team) (2011). "Radial velocity follow-up of CoRoT transiting exoplanets".

5551: 1440:

More massive SPB (Slowly Pulsating B) stars show a frequency spectrum dominated by high order gravity modes excited by the

1397:

enter the radiative zone where they finally lose their identity (overshooting), or even some other poorly known processes.

1065: 15261: 4945: 13965: 13371: 13235: 13195: 11995: 11706: 11701: 9131:

Gaulme, P.; et al. (2010). "Possible detection of phase changes from the non-transiting planet HD 46375b by CoRoT".

9014:"Success for the first observations by the Corot satellite : An exoplanet discovered and first stellar oscillations" 7842:

Aerts, C (2006). "Discovery of the New Slowly Pulsating B Star HD 163830 (B5 II/III) from MOST Space-based Photometry".

1819:

stars and their interaction with their circumstellar matter using CoRoT data revealed the existence of a new class, the

16027: 16007: 15983:

Launches are separated by dots ( • ), payloads by commas ( , ), multiple names for the same satellite by slashes ( / ).

15828: 14607: 14484: 14332: 13291: 13019: 12707: 12532: 12238: 12137: 11832: 11346: 11204: 11191: 8247:"Seismic modelling of the late Be stars HD 181231 and HD 175869 observed with CoRoT: a laboratory for mixing processes" 6061:

Michel, E.; et al. (2008). "CoRoT Measures Solar-Like Oscillations and Granulation in Stars Hotter Than the Sun".

5249: 1426:

stars since the mass extension of the helium core formed during core hydrogen burning is increased. The sub-giant star

1237:

is the science which studies the vibration modes of a star. Each of these modes can be mathematically represented by a

10923: 9612:

Hatzes, A; Hébrard, G; Kabath, P; Jorda, L; et al. (2009). "Transiting exoplanets from the CoRoT space mission".

9556:

Mazeh, T; Moutou, C; Paetzold, M; Pinte, C; et al. (2008). "Transiting exoplanets from the CoRoT space mission".

15350: 15291: 15020: 14643: 14637: 14275: 13906: 12587: 11871: 11677: 11284: 11227: 6639:

Papics, P.I.; et al. (2012). "Gravito-inertial and pressure modes detected in the B3 IV CoRoT target HD 43317".

1580:

adopting various hypotheses to describe the successive generations of stars along the time evolution of this galaxy.

788:

In order to avoid the Sun entering in its field of view, during the northern summer CoRoT observed in an area around

8188:"Multisite spectroscopic seismic study of the β Cep star V2052 Ophiuchi: inhibition of mixing by its magnetic field" 6737:

Mazumdar, A.; et al. (2012). "Seismic detection of acoustic sharp features in the CoRoT target HD 49933".

608:

on 18 January 2007. Subsequently, the probe started to collect science data on 2 February 2007. CoRoT was the first

15272: 14990: 14679: 14060: 14050: 12758: 12431: 11274: 10934: 5446: 1962:

the semi-major axis of the elliptical orbit ) is linked to its orbital period by the second law of Kepler / Newton

1706:

HD 47129 on the contrary shows a peak with six harmonics in the frequency range expected from theoretical modeling.

1902:: One of the binary system observed by CoRoT is of particular interest since the less massive component is a late 708:. These CCDs are frame-transfer, thinned, back-illuminated designs in a 2,048 by 2,048 pixel array. Each pixel is 15002: 14070: 13815: 13299: 13259: 12808: 12788: 12773: 12611: 12492: 12343: 12327: 12295: 11801: 11791: 11716: 11468: 11299: 7773: 7169:

Kjeldsen, H.; Bedding, T.R. (1995). "Amplitudes of stellar oscillations: the implications for asteroseismology".

7004:

Ludwig, H.-G.; et al. (2009). "Hydrodynamical simulations of convection-related stellar micro-variability".

5100: 1509: 1355: 613: 405: 8494:

Zwintz, K.; et al. (2013). "γ Doradus pulsation in two pre-main sequence stars discovered by CoRoT".

5518: 16057: 15583: 15237: 15079: 14171: 13958: 13700: 13363: 13243: 12508: 12383: 12375: 12270: 12153: 12057: 12041: 11398: 11351: 11259: 9444:

L; Lammer, H; Léger, A; Llebaria, A; et al. (2008). "Transiting exoplanets from the CoRoT space mission".

9388:

Lammer, H; Llebaria, A; Loeillet, B; et al. (2008). "Transiting exoplanets from the CoRoT space mission".

7558:

Gillon, M.; et al. (2013). "WASP-64 b and WASP-72 b: two new transiting highly irradiated giant planets".

5186: 4841: 11443: 8070:"Asteroseismology of the β Cephei star ν Eridani: interpretation and applications of the oscillation spectrum" 7505:

Montalban, J.; et al. (2010). "Seismic Diagnostics of Red Giants: First Comparison with Stellar Models".

2198:, was the first confirmed rocky planet, with a density and composition which are close to those of the Earth. 1958:

to have a chance to detect three transits. The distance of the planet to the star ( which is characterized by

1168: 733:, had a launch mass of 630 kg, was 4.10 m long, 1.984 m in diameter and was powered by two solar panels. 16037: 13916: 13805: 13043: 13002: 12991: 12500: 12476: 12311: 11458: 11413: 11326: 5164: 2109:

In June 2011, during the Second CoRoT Symposium, the probe added ten new objects to the Exoplanet catalogue:

1727:

convective core. This is indeed a major discovery since it was the first time that pulsations excited by the

730: 8329:

Mahy, L (2009). "Early-type stars in the young open cluster NGC 2244 and in the Monoceros OB2 association".

14508: 13860: 13850: 13845: 13708: 13123: 12763: 11864: 11766: 9204: 6580:"Probing the properties of convective cores through g modes: high-order g modes in SPB and γ Doradus stars" 4853: 2255:

CoRoT-24b and c, the second planetary system discovered by CoRoT, with two small planets of 0.10 and 0.17 M

1307: 593:, discovered in 2009 which became the first exoplanet shown to have a rock or metal-dominated composition. 5378: 16032: 14842: 13896: 13778: 13766: 13522: 13514: 13498: 12484: 5626:

Almenara, J. M.; et al. (2009). "Rate and nature of false positives in the CoRoT exoplanet search".

1809: 1539:

Histograms of a synthetic red giant population (in red) and CoRoT red giant population (in orange). From

1408:

is illustrative of this extra-mixing problem. Its convective envelope is responsible for the presence of

254: 91: 13275: 1028:

with an altitude of 827 km . The first scientific observation campaign started on 3 February 2007.

680:

CCDs are defocused by 760μm toward the dioptric objective to avoid saturation of the brightest stars. A

15895: 15734: 15149: 14969: 14562: 14544: 14514: 14424: 14139: 14106: 14080: 13684: 13668: 13397: 13387: 13355: 13283: 13203: 13067: 12986: 12230: 12129: 11971: 11811: 11640: 10979: 10550: 10495: 10456: 10396: 10340: 10284: 10229: 10182: 10126: 10070: 10014: 9958: 9902: 9781: 9725: 9670: 9614: 9558: 9502: 9446: 9390: 9334: 9279: 9224: 9133: 9050: 8851: 8604: 8496: 8441: 8386: 8331: 8292: 8251: 8015: 7789: 7703: 7379: 7320:"Galactic archaeology: mapping and dating stellar populations with asteroseismology of red-giant stars" 7265: 7210: 7171: 7116: 7061: 7006: 6951: 6904: 6849: 6794: 6739: 6641: 6531: 6469: 6359: 6316: 6257: 5952: 5893: 5846: 5797: 5683: 5628: 5454: 5333: 5280: 2160:

Among the exoplanets CoRoT detected, one can highlight a subset with the most original features :

1903: 1644:

Massive variable main sequence stars have frequency spectra dominated by acoustic modes excited by the

1371: 1310:

level, CoRoT has provided a new vision of stars, never reached before by any ground-based observation.

15899: 12778: 8792:"CoRoT photometry and high-resolution spectroscopy of the interacting eclipsing binary AU Monocerotis" 6125:

De Ridder, J.; et al. (2009). "Non-radial oscillation modes with long lifetimes in giant stars".

1069: 16042: 15134: 14772: 14438: 14280: 14065: 13939: 13870: 13820: 12303: 11950: 11796: 11771: 11108:

Moutou, C.; Deleuil, M.; Guillot, T.; et al. (2013). "CoRoT: Harvest of the exoplanet program".

7263:

Miglio, A.; et al. (2009). "Probing populations of red giants in the galactic disk with CoRoT".

6694:

Roxburgh, I.W.; Vorontsov, S.V. (1998). "On the Diagnostic Properties of Low Degree Acoustic Modes".

6490: 4859: 4674: 4550: 4488: 3680: 3514: 3457: 3400: 3343: 3172: 3115: 3058: 2773: 2660: 2604: 2433: 2152:

As of November 2011, around 600 additional candidate exoplanets are being screened for confirmation.

1782: 1765: 1200: 1180: 797: 11140: 9186: 6792:

Miglio, A.; et al. (2010). "Evidence for a sharp structure variation inside a red-giant star".

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of 2.7° by 3.05°. The CoRoT optical path consisted of a 27 cm (10.6 in) diameter off-axis

15094: 13901: 13840: 11558: 10873:"Sub-stellar companions of intermediate-mass stars with CoRoT: CoRoT–34b, CoRoT–35b, and CoRoT–36b" 8013:

Aerts, C.; et al. (2011). "Seismic modelling of the β Cephei star HD 180642 (V1449 Aquilae)".

106: 85: 1920:: A binary system observed by CoRoT showed out of eclipses variations which were interpreted as a 1754:

During a 23-day observing run in March 2008, CoRoT observed 636 members of the young open cluster

15139: 14661: 14338: 14191: 14127: 13546: 13442: 13434: 12828: 11934: 11726: 11264: 5278:

Auvergne, M.; et al. (2009). "The CoRoT satellite in flight: Description and performances".

4814: 1778: 1475: 1212: 1196: 984:, from 6 July 2012 to 1 November 2012 - interrupted by the fatal failure which ended the mission. 605: 575: 14893: 10659:"The GTC exoplanet transit spectroscopy survey. III. No asymmetries in the transit of CoRoT-29b" 5400:

Deleuil, M.; Moutou, C.; Bordé, P. (2011). "The CoRoT Exoplanet program: status & results".

2259:. The two planets are of Neptune size, and orbit the same star and represent the first multiple 1412:. Comparing the observed frequency spectrum with that obtained from theoretical models of 1.19 M 15109: 14502: 13789: 13716: 13307: 12962: 12798: 12691: 12391: 12097: 11760: 11568: 11535: 11180: 11135: 5738: 4847: 4835: 4378: 4216: 3286: 3229: 2944: 2830: 2547: 2490: 2324: 1841: 1805: 1798: 1760: 1680:. This extra-mixed zone could even be absent in the structure of V1449 Aquilae (HD 180642) and 1449:

where an extra-mixing with a somewhat smooth shape is clearly required in the modeling and (2)

1148: 617: 31: 15795: 6527:"Seismic and spectroscopic characterization of the solar-like pulsating CoRoT target HD 49385" 2102:. The probe was also able to tentatively detect the reflected light at optical wavelengths of 14857: 14156: 13981: 12848: 12838: 12399: 12174: 11077: 7787:

Mazumdar, A (2006). "An asteroseismic study of the β Cephei star β Canis Majoris".

4949: 4735: 1330: 1123: 1115: 1061: 1040: 701: 665: 583: 415: 78: 17: 11910: 11002: 10946: 10808: 10749: 10684: 10627: 10573: 10518: 10469: 10419: 10363: 10307: 10252: 10205: 10149: 10093: 10037: 9981: 9925: 9804: 9748: 9693: 9637: 9581: 9525: 9469: 9413: 9357: 9302: 9247: 9156: 9013: 8874: 8760: 8627: 8519: 8464: 8409: 8354: 8305: 8264: 8038: 7812: 7716: 7581: 7434:"Gravity modes as a way to distinguish between hydrogen- and helium-burning red giant stars" 7402: 7288: 7233: 7194: 7139: 7084: 7029: 6974: 6927: 6872: 6817: 6762: 6707: 6664: 6554: 6372: 6329: 6280: 5965: 5916: 5869: 5810: 5706: 5651: 5477: 5303: 653:

specifically designed to block sunlight reflected by the Earth and a camera consisting of a

15195: 14899: 14743: 14625: 14393: 14375: 14326: 14149: 14144: 13921: 13810: 13227: 13211: 12954: 11585: 11316: 11127: 10998: 10942: 10804: 10745: 10680: 10623: 10569: 10514: 10465: 10415: 10359: 10303: 10248: 10201: 10145: 10089: 10033: 9977: 9921: 9847: 9800: 9744: 9689: 9633: 9577: 9521: 9465: 9409: 9353: 9298: 9243: 9152: 8954: 8870: 8813: 8756: 8680: 8623: 8568: 8515: 8460: 8405: 8350: 8301: 8260: 8209: 8140: 8091: 8034: 7977: 7918: 7861: 7808: 7742:"Asteroseismology of the β Cephei star HD 129929. Effects of a change in the metal mixture" 7712: 7661: 7620: 7577: 7524: 7455: 7398: 7341: 7284: 7229: 7190: 7135: 7080: 7025: 6970: 6923: 6868: 6813: 6758: 6703: 6660: 6603: 6550: 6499: 6412: 6368: 6325: 6276: 6202: 6134: 6080: 5961: 5912: 5865: 5806: 5757: 5702: 5647: 5473: 5419: 5299: 5014: 4453: 2398: 2055:

was announced. It's a long period planet (95.3 days) in an orbit close to that of Mercury.

1938: 1921: 1794: 1786: 1661: 1624:

Seismic signatures and extension of mixed zones during central hydrogen and helium burning:

1504:

whose radius and luminosity increase in time. These stars are now located on the so-called

1366: 1185: 1073: 989: 817: 673: 355: 9112: 5580:"Completion and delivery of equipment bay and camera to CNES mark major project milestone" 2276:

Light green rows indicate that the planet orbits one of the stars in a binary star system.

1416:

computed with and without additional mixing clearly excludes a model without extra mixing.

562:

mission which operated from 2006 to 2013. The mission's two objectives were to search for

8: 15503: 15330: 15319: 15315: 15179: 15124: 15119: 15089: 14928: 14887: 14875: 14869: 14756: 14568: 14538: 14397: 14369: 14270: 14001: 13772: 13751: 13724: 13466: 13011: 12858: 12635: 12287: 12065: 11806: 11748: 11279: 5891:

Carone, L.; et al. (2012). "Planetary transit candidates in the CoRoT LRa01 field".

4820: 1987: 1933: 1910:

with an estimated effective temperature of about 3000 K. The primary component is a 1.5 M

1733: 1586: 1521: 1238: 992:

their host star. In every field, CoRoT recorded the brightness of thousands stars in the

821: 801: 385: 251: 163: 11131: 9851: 8958: 8817: 8684: 8572: 8246: 8213: 8144: 8095: 7981: 7922: 7865: 7665: 7624: 7528: 7459: 7345: 6607: 6503: 6416: 6206: 6138: 6084: 5761: 5582:(Press release). Observatoire de Paris, CNES and CNRS-INSU. 30 June 2005. Archived from 5423: 760:

Please help update this article to reflect recent events or newly available information.

15762: 15412: 15283: 15169: 15074: 14881: 14818: 14691: 14575: 13855: 13732: 13554: 13219: 12813: 12753: 12595: 12214: 12206: 12105: 12073: 11963: 11721: 11660: 11153: 11117: 11041: 11014: 10988: 10884: 10794: 10735: 10704: 10670: 10639: 10613: 10585: 10559: 10530: 10504: 10431: 10405: 10375: 10349: 10319: 10293: 10264: 10238: 10191: 10161: 10135: 10105: 10079: 10049: 10023: 9993: 9967: 9937: 9911: 9881: 9816: 9790: 9760: 9734: 9705: 9679: 9649: 9623: 9593: 9567: 9537: 9511: 9481: 9455: 9425: 9399: 9369: 9343: 9314: 9288: 9259: 9233: 9168: 9142: 9035: 8970: 8944: 8886: 8860: 8831: 8803: 8772: 8746: 8717: 8698: 8670: 8639: 8613: 8584: 8558: 8531: 8505: 8476: 8450: 8421: 8395: 8366: 8340: 8227: 8199: 8168: 8109: 8081: 8050: 8024: 7995: 7967: 7936: 7908: 7877: 7851: 7824: 7798: 7679: 7651: 7593: 7567: 7540: 7536: 7514: 7487: 7445: 7414: 7388: 7359: 7331: 7300: 7274: 7245: 7219: 7180: 7151: 7125: 7096: 7070: 7041: 7015: 6986: 6960: 6913: 6884: 6858: 6829: 6803: 6774: 6748: 6719: 6676: 6650: 6621: 6593: 6540: 6446: 6292: 6266: 6234: 6192: 6158: 6104: 6070: 6022: 5994: 5928: 5902: 5855: 5773: 5747: 5718: 5692: 5663: 5637: 5489: 5463: 5409: 5315: 5289: 5231: 4806: 4359: 2305: 1816: 1703: 1302: 993: 777:

The satellite observed perpendicular to its orbital plane, meaning there were no Earth

669: 567: 15256: 10658: 8966: 7611:

Goupil, M. J.; Talon, S. (2009). "Seismic diagnostics of rotation for massive stars".

5844:

Cabrera, J.; et al. (2009). "Planetary transit candidates in CoRoT-LRc01 field".

1669: 97: 15911: 15643: 15376: 14649: 14550: 14448: 14431: 14409: 13578: 13163: 13155: 12882: 12874: 12728: 12081: 12008: 11942: 11605: 11494: 11381: 11157: 11059: 10904: 10822: 10763: 10696: 10435: 10109: 9997: 9941: 9873: 9597: 9172: 8974: 8826: 8791: 8702: 8588: 8580: 8480: 8222: 8187: 8153: 8128: 8104: 8069: 7990: 7955: 7931: 7896: 7763: 7674: 7639: 7479: 7418: 6723: 6616: 6579: 6438: 6226: 6150: 6096: 6026: 6012: 5319: 5235: 4953: 4446: 2391: 1836:

with non-radially pulsating members were observed by CoRoT. Some of them, which were

1203:

and possibly detect reflected light from the planet or the atmospheric compositions.

1053: 563: 445: 14631: 12619: 11018: 10708: 10643: 10589: 10534: 10379: 10323: 10268: 10165: 10053: 9820: 9709: 9653: 9485: 9429: 9373: 9318: 9263: 8890: 8835: 8776: 8643: 8535: 8425: 8370: 8231: 8172: 8113: 8054: 7999: 7940: 7881: 7828: 7683: 7597: 7544: 7363: 7304: 7155: 7100: 6990: 6888: 6833: 6778: 6680: 6108: 5932: 5777: 5722: 5667: 5493: 5131: 2164:

CoRot-1b, the first planet detected by CoRoT is a hot Jupiter. By further analysis,

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of the exoplanets found. Radial velocity follow-up is performed with high-precision

641:

The CoRoT optical design minimized stray light coming from the Earth and provided a

15210: 15069: 14794: 14134: 13347: 12121: 11979: 11522: 11145: 11051: 11006: 10950: 10894: 10812: 10753: 10688: 10631: 10577: 10522: 10473: 10423: 10367: 10311: 10256: 10209: 10153: 10097: 10041: 9985: 9929: 9885: 9863: 9855: 9808: 9764: 9752: 9697: 9641: 9585: 9541: 9529: 9473: 9417: 9361: 9306: 9251: 9160: 8962: 8878: 8821: 8764: 8688: 8631: 8576: 8523: 8468: 8413: 8358: 8309: 8268: 8217: 8158: 8148: 8099: 8042: 7985: 7926: 7869: 7816: 7753: 7720: 7669: 7585: 7532: 7491: 7471: 7463: 7406: 7349: 7292: 7249: 7237: 7143: 7088: 7033: 6978: 6931: 6876: 6821: 6766: 6711: 6668: 6611: 6558: 6507: 6450: 6428: 6420: 6376: 6333: 6296: 6284: 6238: 6218: 6210: 6162: 6142: 6088: 6004: 5969: 5920: 5873: 5824: 5814: 5765: 5710: 5655: 5481: 5427: 5307: 5223: 5045: 4366: 2312: 2224: 2011: 1837: 1774: 1613: 1505: 1234: 1119: 1086: 1009: 722: 714: 677: 650: 571: 328: 13083: 11055: 11010: 10955: 10817: 10782: 10758: 10723: 10692: 10635: 10581: 10526: 10478: 10451: 10427: 10371: 10315: 10260: 10213: 10157: 10101: 10045: 9989: 9933: 9812: 9756: 9701: 9645: 9589: 9533: 9477: 9421: 9365: 9310: 9255: 9164: 9069: 9048:

Papers describing the two exoplanets, with radial-velocity follow-up, appeared in

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respectively: the theory does not yet provide a consistent model for such objects;

15623: 15381: 15026: 14863: 14122: 13911: 13450: 13331: 12283: 11902: 11887: 11149: 10853: 10840: 9119: 7820: 7725: 7698: 7241: 6008: 5485: 5078: 4765:

about 6%, other cases being eclipsing binaries ( 46%) or unresolved cases (48%).

4438: 4347: 2383: 2293: 1409: 1362: 1297: 793: 559: 345: 64: 2252:

CoRoT-22b, notable for its small size, having less than half the mass of Saturn.

1378: 16017: 15523: 15059: 14260: 14016: 12768: 12748: 12319: 11393: 11366: 11321: 11238: 5793:"Planetary transit candidates in the CoRoT initial run: Resolving their nature" 4466: 4423: 4413: 2411: 2368: 2358: 1685: 1140: 1114:

normally. The loss of photo-detector chain number 1 results in the loss of one

1102: 1090: 1021: 681: 657: 601: 395: 237: 8988: 6715: 5227: 1728: 1645: 1605:

whose goal is to measure metallicities for 100 000 red giants in this galaxy,

1551:

3D map of this galaxy from seismic data of red giants observed by CoRoT. From

1441: 1195:

Interesting transiting planets could be further followed-up with the infrared

968:, from 10 January 2012 to 29 March 2012 – a run dedicated to reobservation of 16012: 16001: 15809: 15551: 15457: 14403: 14344: 14211: 14034: 12643: 12540: 12254: 11918: 11478: 11063: 10908: 10899: 10872: 10826: 10767: 10700: 6401:"Deviations from a uniform period spacing of gravity modes in a massive star" 5156: 5073: 4342: 2288: 1528:. The readjustment following the flash brings the red giant to the so-called 1384: 1179:. Once the planetary nature of the candidate is established, high-resolution 1127: 789: 726: 646: 642: 510: 484: 11196: 6214: 6092: 1665: 1547: 1155:

in Hawaii. The radial velocity follow-up allows to discard binaries or even

1057: 1039:

and 25% was contributed by Austria, Belgium, Germany, Spain, Brazil and the

15693: 15345: 14387: 14206: 12803: 12627: 11473: 11423: 10960: 9877: 8693: 8658: 8384:

Mahy, L (2011). "Plaskett's star: analysis of the CoRoT photometric data".

7483: 7433: 7354: 7319: 6511: 6442: 6400: 6230: 6154: 6100: 5605: 5351: 4975: 4397: 2342: 1525: 1334: 1164: 1098: 1002: 940:, from 1 July 2011 to 5 July 2011 – a run made to reobserve the transit of 425: 9835: 6180: 4730: 4333: 2279: 1681: 1599: 1325:

while the other CCDs were reserved for exoplanet hunting in the so-called

51:

The CoRoT satellite in the integration hall of Thales Alenia Space, Cannes

15967: 15963: 15959: 15756: 15601: 15556: 15425: 15418: 15144: 15064: 14737: 14733: 14723: 14719: 14715: 14705: 14701: 14418: 14255: 13107: 12246: 12145: 11987: 11488: 10450:

Ferraz-Mello, S; Fridlund, M; Gillon, M; Guillot, T; et al. (2012).

8086: 7856: 7803: 7224: 7185: 5468: 5218: 4923: 4460: 4354: 2405: 2300: 2176: 2083: 2000: 1833: 1677: 1480: 1393: 1342: 1306:

By revealing their microvariability, measuring their oscillations at the

1156: 1144: 1025: 809: 778: 661: 435: 338: 264: 13950: 9859: 7467: 7377:

Mosser, B (2011). "Mixed modes in red-giant stars observed with CoRoT".

6424: 6146: 5497: 5132:"COROT discovers its first exoplanet and catches scientists by surprise" 1585:

the figure where different colors relate to different CoRoT runs and to

15954: 15707: 15366: 15159: 14810: 14802: 14778: 14749: 14729: 14711: 14697: 14520: 13586: 12898: 12738: 12455: 8659:"Rotation in NGC 2264: a study based on CoRoT photometric observations" 7741: 7475: 6433: 5829: 4371: 2317: 2249:, the parameter that quantifies the energy dissipation by tidal forces; 2235:

CoRoT-11b and CoRoT-2b, two inflated planets, with radius 1.4 and 1.5 R

2229: 2103: 1804:

The CoRoT observations led to the discovery of about a dozen pulsating

1013: 813: 609: 9868: 9836:"A transiting giant planet with a temperature between 250 K and 430 K" 8163: 7758: 7114:

Mosser, B (2010). "Red-giant seismic properties analyzed with CoRoT".

6222: 4823: – 2007 European study concept of an array of space observatories 2216:

CoRoT-8b, a planet of the same class as Neptune, with a mass of 0.22 M

2200: 15677: 15596: 15507: 15452: 15200: 15174: 15099: 14922: 14764: 14685: 14496: 14351: 13993: 13251: 12659: 12367: 12182: 11631: 11448: 11418: 11243: 9222:

Alonso, R.; et al. (2009). "The secondary eclipse of CoRoT-1b".

4572: 4273: 4151: 4094: 4037: 3976: 3926: 3894: 3837: 3815: 3783: 3761: 3729: 3700: 3645: 3588: 3531: 3479: 3422: 3365: 3308: 3251: 3194: 3137: 3080: 3023: 2966: 2717: 2272:

The following transiting planets have been announced by the mission.

2146: 2142: 2138: 2134: 2130: 2126: 2122: 2118: 2114: 2110: 2087: 2079: 2075: 2071: 2067: 2063: 1857: 1576: 1529: 1501: 1423: 1422:

Such an additional mixing also affects the structure of more evolved

1338: 5550:. DLR Institute of Planetary Research. February 2011. Archived from 2036:

In February 2009, during the First CoRoT Symposium, the super-Earth

1714: 1673: 1001:

to allow planetary detections. CoRoT was sensitive enough to detect

691: 46: 15949: 15944: 15935: 15925: 15698: 15627: 15590: 15528: 15476: 15442: 15407: 15403: 14591: 14526: 14456: 14265: 14029: 14024: 13538: 13474: 13315: 13091: 13027: 12783: 12683: 12675: 12579: 12524: 12335: 12198: 12024: 12016: 11856: 11371: 11289: 11046: 10889: 10799: 10740: 10675: 7873: 6312:"HD 50844: a new look at δ Scuti stars from CoRoT space photometry" 5999: 4768: 4544: 4510: 3867: 3756: 3618: 3561: 3509: 3452: 3395: 3338: 3281: 3224: 3167: 3110: 3053: 2996: 2939: 2909: 2852: 2795: 2738: 2682: 2625: 2569: 2512: 2455: 2180: 2165: 2091: 2059: 2052: 2045: 2041: 2037: 2030: 2026: 2022: 2007: 2003: 1820: 1755: 1494: 1405: 1208: 1204: 969: 941: 805: 685: 654: 625: 590: 11122: 10993: 10780: 10618: 10564: 10509: 10410: 10354: 10298: 10243: 10196: 10140: 10084: 10028: 9972: 9916: 9795: 9739: 9684: 9628: 9572: 9554: 9516: 9460: 9404: 9348: 9293: 9238: 9147: 9095: 8949: 8865: 8808: 8751: 8736: 8722: 8675: 8618: 8563: 8510: 8455: 8400: 8345: 8204: 8029: 7972: 7913: 7656: 7572: 7519: 7450: 7393: 7336: 7279: 7130: 7075: 7020: 6965: 6949:

Samadi, R.; et al. (2010). "The CoRoT target HD 49933".

6918: 6902:

Samadi, R.; et al. (2010). "The CoRoT target HD 49933".

6863: 6808: 6753: 6655: 6598: 6545: 6271: 6197: 6075: 5907: 5860: 5752: 5697: 5642: 5517:(Press release) (in French). CNES. 5 February 2007. Archived from 5414: 5294: 4817: – Robotic optical telescope searching for extrasolar planets 874:, from 6 October 2008 to 12 November 2008 – 10,265 stars observed; 868:, from 8 September 2008 to 6 October 2008 – 11,408 stars observed; 15930: 15890: 15875: 15859: 15818: 15814: 15775: 15729: 15723: 15578: 15561: 15497: 15472: 15164: 15039: 15032: 15014: 15008: 14946: 14940: 14934: 14655: 14381: 14181: 14161: 14101: 14006: 13761: 13692: 13530: 13179: 13139: 13035: 12946: 12938: 12930: 12922: 12914: 12906: 12603: 12571: 11361: 11356: 11309: 9055: 4612: 4483: 3872: 3623: 3566: 3001: 2887: 2882: 2825: 2768: 2712: 2655: 2599: 2542: 2485: 2428: 2184: 2099: 2018: 1892: 1853: 1653:

is one of the main uncertainties affecting theoretical modeling.

1572: 880:, from 12 November 2008 to 30 March 2009 – 11,408 stars observed; 862:, from 31 March 2008 to 8 September 2008 – 11,408 stars observed; 782: 268: 10392: 9276: 4743: 1626:

Increasing even further the scrutiny in analyzing the CoRoT and

898:, from 30 September 2009 to 1 March 2010 – 5,289 stars observed; 15884: 15854: 15823: 15619: 15467: 15462: 15154: 14786: 14556: 14490: 14320: 13865: 13602: 13458: 13171: 13115: 13075: 12998: 12978: 12833: 12548: 12447: 12423: 12262: 12089: 12049: 11926: 11731: 11622: 11500: 11331: 11175: 11082: 10602: 10547: 4976:"Successful launch of the CoRoT satellite, on 27 December 2006" 4407: 2352: 2331: 2095: 1337:

from every observed field. Stellar activity, rotation periods,

998: 892:, from 2 July 2009 to 30 September 2009 – 5,716 stars observed; 850:, from 15 October 2007 to 3 March 2008 – 11,408 stars observed; 241: 11031: 10870: 10178: 8715: 7208:

Girardi, L.; et al. (2005). "Star Counts in the Galaxy".

4850: – Online astronomical exoplanet catalog and data service 1457: 832:, from 18 January 2007 to 3 April 2007 – 9,879 stars observed; 15804: 15607: 15546: 15542: 15538: 14996: 14667: 14583: 14478: 13835: 13830: 13633: 13570: 13490: 13427: 13422: 13417: 13412: 13407: 13402: 13392: 13323: 13187: 13147: 13099: 13059: 12651: 12032: 11669: 11552: 11336: 10010: 1790: 1535: 1471:

Amplitudes and line widths in solar-like oscillation spectra:

1379:

Extension of the chemically mixed zone in main sequence stars

1189: 1176: 1172: 844:, from 9 May 2007 to 15 October 2007 – 11,408 stars observed; 729:

for planetary detection is 3.5°. The satellite, built in the

375: 365: 10492: 10448: 9954: 9666: 9442: 7897:"The two hybrid B-type pulsators: ν Eridani and 12 Lacertae" 2213:

and a period of 3.79 days. A third planet is even suspected.

1862: 1606: 1361:

Discoveries were numerous, including the first detection of

856:, from 3 March 2008 to 31 March 2008 – 8,150 stars observed; 717:. The data output stream from the CCDs are connected in two 688:

designed to disperse more strongly in the blue wavelengths.

15129: 15104: 15084: 13875: 13825: 13783: 13756: 13676: 13267: 12667: 12359: 11754: 10976: 9898: 9834:

Deeg, HJ; Moutou, C; Erikson, A; et al. (March 2010).

9610: 5447:"Exoplanet detection capability of the CoRoT space mission" 5104: 4983: 4838: – NASA space telescope for exoplanetology (2009–2018) 4391: 4337: 2336: 2283: 1313: 1160: 1036: 886:, from 30 March 2009 to 2 July 2009 – 5,661 stars observed; 579: 10721: 9331: 9187:"CoRoT's new detections highlight diversity of exoplanets" 9130: 4881:"Events Archive: Last telecommand sent to Corot satellite" 4862: – NASA concept study of an array of space telescopes 189:

2 m × 4 m (6.6 ft × 13.1 ft)

27:

European space telescope that operated between 2006 - 2014

11186: 10924:"The CoRoT-7 planetary system: two orbiting super-Earths" 10066: 9777: 9096:"Rich exoplanet harvest for CoRoT – CNRS Web site – CNRS" 4781:) for short periods (less than 5 days) and bright stars. 4431: 2376: 1950:

should at least be observed for a time interval between 2

1603:(Apache Point Observatoty Galactic Evolution Environment) 1354:. The figure shows where most of them are located in the 1284: 1274: 838:, from 3 April 2007 to 9 May 2007 – 6,975 stars observed; 597: 227: 123: 15313: 10336: 10122: 9386: 5444: 1264: 1254: 1108: 566:

with short orbital periods, particularly those of large

9498: 5948:"Planetary transit candidates in the CoRoT-SRc01 field" 5541:"CoRoT: Mission Brochur – Hunting for Planets in Space" 4731:

Global properties of the exoplanets discovered by CoRoT

2058:

In June 2010 the CoRoT team announced six new planets,

1668:

while a much smaller one is favored for HD 129929, for

1227: 2090:. All the planets announced are Jupiter sized, except 705: 7894: 5242: 1199:, to give an independent confirmation at a different 1020:

The mission began on 27 December 2006 when a Russian

721:. Each chain has one planetary detection CCD and one 11107: 10656: 10452:"Transiting exoplanets from the CoRoT space mission" 7748:. Veröffentlichungen der Kommission für Astronomie. 6250: 6248: 6174: 6172: 4831:

Pages displaying wikidata descriptions as a fallback

4796: 1999:

CoRoT discovered its first two planets in 2007: the

1994: 1617:(Global Astrometric Interferometer for Astrophysics) 1500:

important expansion and cooling. The star becomes a

1358:

together with some others observed from the ground.

1064:, the Laboratoire d'Astrophysique de Marseille, the 684:

in front of the planet detection CCDs gives a small

1035:, of which 75% was paid by the French space agency 616:, opening the way for more advanced probes such as 6120: 6118: 5399: 4752:All CoRoT planets were detected during long runs 2029:, as well as an unknown massive celestial object, 1711:of acoustic modes like those observed in the Sun. 10877:Monthly Notices of the Royal Astronomical Society 10866: 10864: 10862: 9833: 8796:Monthly Notices of the Royal Astronomical Society 8663:Monthly Notices of the Royal Astronomical Society 8192:Monthly Notices of the Royal Astronomical Society 8133:Monthly Notices of the Royal Astronomical Society 8074:Monthly Notices of the Royal Astronomical Society 7960:Monthly Notices of the Royal Astronomical Society 7901:Monthly Notices of the Royal Astronomical Society 7644:Monthly Notices of the Royal Astronomical Society 7324:Monthly Notices of the Royal Astronomical Society 6693: 6585:Monthly Notices of the Royal Astronomical Society 6245: 6169: 15999: 14076:Space Applications and Telecommunications Centre 9722: 5126: 5124: 5122: 2267: 1495:Red giants and chemical evolution of this galaxy 1490:although significant disagreements still remain. 1296:When applied to the Sun, this science is called 140:Final: 7 years, 5 months, 20 days 7168: 6115: 5988: 5574: 5572: 4924:"COROT Satellite details 2006-063A NORAD 29678" 4844: – A list of systems with multiple planets 14086:Space Telescope European Coordinating Facility 10859: 10854:https://exoplanet.eu/catalog/corot_31_b--1212/ 10852:CoRoT-31 b. Exoplanet Catalogue. Available at 10841:https://exoplanet.eu/catalog/corot_30_b--1211/ 10839:CoRoT-30 b. Exoplanet Catalogue. Available at 7895:Dziembowski, W. A.; Pamyatnykh, A. A. (2008). 7699:"Asteroseismology of the β Cep star HD 129929" 1852:: This semi-detached binary system contains a 1520:, this new combustion takes place in a highly 15299: 13966: 11872: 11226: 11212: 11088:Centre de données astronomiques de Strasbourg 6394: 6392: 6056: 6054: 5119: 4827:High Accuracy Radial Velocity Planet Searcher 956:, from 30 September 2011 to 28 November 2011; 922:, from 27 September 2010 to 16 December 2010; 10871:Sebastian, D; et al. (27 August 2022). 5569: 5060: 2242:CoRoT-15b, a bona fide brown dwarf in orbit; 1749: 1159:and, given enough observations, provide the 1024:rocket lifted the satellite into a circular 664:. Inside the focal box was an array of four 530: 7610: 6181:"Solar-Like Oscillations in a Massive Star" 5250:"Retirement for planet-hunting space probe" 5151: 5149: 4873: 4829: – high-precision echelle spectrograph 1458:Structure of the superficial stellar layers 1076:in the Centre spatial de Cannes Mandelieu. 624:. It detected its first extrasolar planet, 15306: 15292: 14235:European Launcher Development Organisation 13973: 13959: 11879: 11865: 11219: 11205: 8912:Gandolfi, D. et al. 2013, work in progress 8903:Maceroni, C. et al. 2013, work in progress 8067: 6389: 6051: 5507: 4968: 4684:−03° 49′ 03.46″ 4622:+05° 37′ 28.79″ 4560:+06° 11′ 10.47″ 4283:+07° 11′ 00.05″ 4226:−02° 46′ 28.82″ 4161:+09° 15′ 26.69″ 4104:−04° 25′ 20.16″ 4047:+06° 50′ 09.36″ 3986:+06° 28′ 46.68″ 3882:+05° 32′ 18.32″ 3825:+06° 58′ 12.00″ 3771:+06° 30′ 49.74″ 2727:+06° 39′ 47.95″ 2557:+00° 07′ 18.62″ 1247:A few examples of stellar vibration modes 962:, from 29 November 2011 to 9 January 2012; 704:detectors are model 4280 CCDs provided by 96: 14298: 13980: 11139: 11121: 11045: 10992: 10954: 10898: 10888: 10816: 10798: 10757: 10739: 10674: 10617: 10563: 10508: 10477: 10409: 10353: 10297: 10242: 10226: 10195: 10139: 10083: 10027: 9971: 9915: 9867: 9794: 9738: 9683: 9627: 9571: 9515: 9459: 9403: 9347: 9292: 9237: 9146: 9067: 8948: 8864: 8825: 8807: 8750: 8721: 8692: 8674: 8617: 8562: 8509: 8454: 8399: 8344: 8313: 8221: 8203: 8162: 8152: 8126: 8103: 8085: 8028: 7989: 7971: 7930: 7912: 7855: 7802: 7757: 7724: 7673: 7655: 7571: 7518: 7504: 7449: 7392: 7353: 7335: 7278: 7223: 7184: 7129: 7074: 7019: 6964: 6917: 6862: 6807: 6752: 6654: 6615: 6597: 6562: 6544: 6524: 6432: 6380: 6337: 6270: 6196: 6124: 6074: 5998: 5973: 5906: 5859: 5828: 5818: 5751: 5696: 5641: 5606:"CoRoT back on track, on April 7th, 2009" 5467: 5438: 5413: 5293: 5273: 5271: 5179: 5066: 5007:"Planet-hunting space telescope launched" 4946:"Europe goes searching for rocky planets" 4498:−01° 03′ 46.0″ 2783:−01° 03′ 46.0″ 1532:(RC) in the Hertzsprung-Russell diagram. 9093: 8989:"Two Planet-hunters Snapped at La Silla" 8848: 7786: 6736: 6465:"The CoRoT space mission: early results" 6398: 6254: 6178: 5735: 5625: 5598: 5515:"First scientific observations by Corot" 5277: 5146: 5101:"COROT all set to begin science mission" 4998: 4938: 4767: 4742: 4734: 3296:−06° 36′ 44 ″ 2954:+00° 44 ′ 46″ 2199: 2175:, it appears to be "something between a 2048:, were also announced at the Symposium. 1932: 1867:Carla Maceroni and the CoRoT binary team 1861: 1713: 1595:Age-metallicity relation in this galaxy: 1546: 1534: 1350:and more than 150 000 weak stars in the 1312: 1283: 1273: 1263: 1253: 950:, from 6 July 2011 to 30 September 2011; 928:, from 16 December 2010 to 5 April 2011; 916:, from 5 July 2010 to 27 September 2010; 690: 10281: 9056:Barge 2008, Alonso 2008 and Bouchy 2008 8934: 8601: 8185: 7637: 7431: 7207: 6846: 6487: 6309: 5945: 5843: 4918: 3936:+05° 34′ 26″ 3690:−03° 43′ 09″ 3633:+04° 21′ 28″ 3576:+06° 13′ 08″ 3467:+00° 13′ 37″ 3410:−00° 01′ 01″ 3353:−00° 01′ 54″ 3239:−06° 00′ 09″ 3182:−05° 32′ 10″ 3125:−05° 05′ 11″ 3068:−01° 17′ 47″ 3011:+05° 56′ 16″ 2897:+06° 12′ 15″ 2840:+01° 25′ 36″ 2670:+00° 48′ 55″ 2614:−00° 40′ 22″ 2500:+01° 23′ 02″ 2443:−03° 06′ 08″ 2094:, which appears to be somewhat between 1464:Transition layers in stellar envelopes: 1387:phase of evolution. The extent of this 796:, and during the winter it observed in 14: 16048:Spacecraft launched by Soyuz-2 rockets 16000: 10921: 9221: 9038:(Press release). ESA. 20 December 2007 8789: 8548: 8493: 8438: 8244: 8068:Pamyatnykh, A.A.; et al. (2004). 7953: 7776:from the original on 11 February 2023. 7696: 7557: 7376: 7317: 7262: 7113: 7058: 7003: 6948: 6901: 6791: 6638: 6577: 6060: 5890: 5790: 5368: 5268: 5035: 4916: 4914: 4912: 4910: 4908: 4906: 4904: 4902: 4900: 4898: 4856: – Cancelled NASA space telescope 15287: 14297: 14197:Space Situational Awareness Programme 13954: 11860: 11200: 9036:"COROT surprises a year after launch" 8656: 8012: 7841: 7739: 5445:P. Bordé; D. Rouan; A. Léger (2003). 5004: 1341:evolution, star–planet interactions, 1109:Failure of Data Processing Unit No. 1 578:in stars. The mission was led by the 15244: 14240:European Space Research Organisation 14056:Space Research and Technology Centre 11886: 11839: 8383: 8328: 8285: 6352: 5680: 5211: 4326: 1569:Red giant population in this galaxy: 1228:Asteroseismology and stellar physics 1133: 978:, from 10 April 2012 to 5 July 2012; 934:, from 5 April 2011 to 30 June 2011; 904:, from 1 March 2010 to 2 April 2010; 740: 636: 15268: 8288:"The B0.5IVe CoRoT target HD 49330" 8127:Ausseloos, M.; et al. (2004). 6525:Deheuvels, S.; et al. (2010). 6355:"The B0.5IVe CoRoT target HD 49330" 5187:"CoRoT Mission Extended Until 2013" 4895: 2017:In May 2008, two new exoplanets of 1126:dedicated to planet detection. The 910:, from 2 April 2010 to 5 July 2010; 24: 9070:"New exoplanet like 'one of ours'" 7746:Communications in Asteroseismology 7613:Communications in Asteroseismology 6399:Degroote, P.; et al. (2010). 6179:Belkacem, K.; et al. (2009). 1974:, using respectively as units for 1791:Canadian-French-Hawaiian Telescope 1764:, is located in the constellation 1610:(Galactic Archaeology with HERMES) 589:Among the notable discoveries was 586:and other international partners. 25: 16069: 13907:List of proposed space telescopes 12588:Nancy Grace Roman Space Telescope 11678:Nancy Grace Roman Space Telescope 11168: 9016:(Press release). CNRS. 3 May 2007 8286:Huat, A.-L.; et al. (2009). 8186:Briquet, M.; et al. (2012). 7638:Briquet, M.; et al. (2007). 7432:Bedding, T.; et al. (2011). 6353:Huat, A.-L.; et al. (2009). 6310:Poretti, E.; et al. (2009). 5946:Erikson, A.; et al. (2012). 5375:idoc-corotn2-public.ias.u-psud.fr 5067:Hellemans, A. (18 January 2007). 4952:. 26 October 2006. Archived from 2014:were published in the same year. 1995:Timeline of planetary discoveries 1827: 1066:Institut d'Astrophysique Spatiale 736: 16023:European Space Agency satellites 15267: 15255: 15243: 15232: 15231: 14061:ESA Centre for Earth Observation 13935: 13934: 11838: 11827: 11826: 11499: 11493: 11487: 11174: 11101: 11070: 11025: 10970: 10935:Extrasolar Planets Encyclopaedia 10915: 10846: 10833: 10774: 10715: 10650: 10596: 10541: 10486: 10442: 10386: 10330: 10275: 10220: 10172: 10116: 10060: 10004: 9948: 9892: 9827: 9771: 9716: 9660: 9604: 9548: 9492: 9436: 9380: 9325: 9270: 9215: 8827:10.1111/j.1365-2966.2009.15659.x 8790:Desmet, M.; et al. (2010). 8245:Neiner, C.; et al. (2012). 8223:10.1111/j.1365-2966.2012.21933.x 8154:10.1111/j.1365-2966.2004.08320.x 8105:10.1111/j.1365-2966.2004.07721.x 7991:10.1111/j.1365-2966.2009.14790.x 7954:Desmet, M.; et al. (2009). 7932:10.1111/j.1365-2966.2008.12964.x 7675:10.1111/j.1365-2966.2007.12142.x 7318:Miglio, A.; et al. (2013). 6617:10.1111/j.1365-2966.2008.13112.x 6578:Miglio, A.; et al. (2008). 5791:Moutou, C.; et al. (2009). 5214:"Exoplanet hunter nears its end" 5134:(Press release). ESA. 3 May 2007 5038:"Soyuz 2-1B launches with CoRoT" 4799: 2190:CoRot-7b, with a radius of 1.7 R 1639: 745: 649:telescope housed in a two-stage 45: 12809:Nautilus Deep Space Observatory 11802:Habitable zone for complex life 11717:Nautilus Deep Space Observatory 9205:"CoRoT's haul of 25 exoplanets" 9197: 9179: 9124: 9106: 9087: 9061: 9028: 9006: 8981: 8928: 8915: 8906: 8897: 8842: 8783: 8730: 8709: 8657:Affer, L.; et al. (2013). 8650: 8595: 8542: 8487: 8432: 8377: 8322: 8279: 8238: 8179: 8120: 8061: 8006: 7947: 7888: 7835: 7780: 7740:Thoul, A.; et al. (2004). 7733: 7690: 7631: 7604: 7551: 7498: 7425: 7370: 7311: 7256: 7201: 7162: 7107: 7052: 6997: 6942: 6895: 6840: 6785: 6730: 6687: 6632: 6571: 6518: 6481: 6457: 6346: 6303: 6033: 5982: 5939: 5884: 5837: 5784: 5729: 5674: 5619: 5533: 5393: 5362: 5344: 5326: 5205: 5036:Bergin, C. (27 December 2006). 4335: 2281: 2155: 1031:The mission's cost amounted to 596:CoRoT was launched at 14:28:00 450:8 March 2016, 11:58:39 UTC 15080:Columbus Man-Tended Free Flyer 8921:Loeb, A. and Gaudi, B.S. 2003 6696:Astrophysics and Space Science 5093: 5029: 5005:Clark, S. (27 December 2006). 4842:List of multiplanetary systems 1937:Two Planet-hunters Snapped at 1524:matter and proceeds through a 1222: 1211:have already been observed by 1151:in Germany and the 3,6 m 1046: 812:to be monitored, and to avoid 612:dedicated to the detection of 457: 108: 13: 1: 13917:List of heliophysics missions 7507:Astrophysical Journal Letters 5212:Hand, E. (16 November 2012). 5165:Cannes Mandelieu Space Center 4866: 2268:List of exoplanets discovered 2171:CoRoT-3b, with a mass of 22 M 1928: 731:Cannes Mandelieu Space Center 614:transiting extrasolar planets 380:898.1 km (558.1 mi) 370:607.8 km (377.7 mi) 350:7,123 km (4,426 mi) 11767:Space Interferometry Mission 11150:10.1016/j.icarus.2013.03.022 11034:Astronomy & Astrophysics 10856:; accessed 10 December 2017. 10843:, accessed 10 December 2017. 10606:Astronomy & Astrophysics 7537:10.1088/2041-8205/721/2/l182 6041:"Stellar Seismology results" 6009:10.1007/978-3-319-55333-7_79 4854:Space Interferometry Mission 2044:, and of a new Hot Jupiter, 1918:A beaming effect in a binary 1812:in pre-main sequence stars. 1591:observations (green points). 1079: 668:detectors protected against 600:on 27 December 2006, atop a 7: 16053:Spacecraft launched in 2006 13897:Great Observatories program 11056:10.1051/0004-6361/201526763 11011:10.1051/0004-6361/201015276 10956:10.1051/0004-6361/200913096 10818:10.1051/0004-6361/201424501 10759:10.1051/0004-6361/201629882 10693:10.1051/0004-6361/201527881 10636:10.1051/0004-6361/201323049 10582:10.1051/0004-6361/201323049 10527:10.1051/0004-6361/201117916 10479:10.1051/0004-6361/201118425 10428:10.1051/0004-6361/201117681 10372:10.1051/0004-6361/201117706 10316:10.1051/0004-6361/201117192 10261:10.1051/0004-6361/201117009 10214:10.1051/0004-6361/201117460 10158:10.1051/0004-6361/201015480 10102:10.1051/0004-6361/201015154 10046:10.1051/0004-6361/201014981 9990:10.1051/0004-6361/201015132 9934:10.1051/0004-6361/201014943 9813:10.1051/0004-6361/201014775 9757:10.1051/0004-6361/200911933 9702:10.1051/0004-6361/200913767 9646:10.1051/0004-6361/200911902 9590:10.1051/0004-6361:200810246 9534:10.1051/0004-6361:200810625 9478:10.1051/0004-6361:200809431 9422:10.1051/0004-6361:200809353 9366:10.1051/0004-6361/201015550 9311:10.1051/0004-6361/201116713 9256:10.1051/0004-6361/200912102 9165:10.1051/0004-6361/201014303 8967:10.1088/0004-637x/746/2/185 8883:10.1051/0004-6361/200913311 8769:10.1051/0004-6361/201220755 8636:10.1051/0004-6361/201014184 8528:10.1051/0004-6361/201220127 8473:10.1051/0004-6361/201220934 8418:10.1051/0004-6361/201014777 8363:10.1051/0004-6361/200911662 8315:10.1051/0004-6361/200911928 8273:10.1051/0004-6361/201118151 8047:10.1051/0004-6361/201117629 7590:10.1051/0004-6361/201220561 7411:10.1051/0004-6361/201116825 7297:10.1051/0004-6361/200912822 7148:10.1051/0004-6361/201014036 7093:10.1051/0004-6361/200911858 7038:10.1051/0004-6361/200911930 6983:10.1051/0004-6361/200911868 6936:10.1051/0004-6361/200911867 6881:10.1051/0004-6361/200913111 6826:10.1051/0004-6361/201015442 6771:10.1051/0004-6361/201118495 6673:10.1051/0004-6361/201218809 6564:10.1051/0004-6361/200913490 6382:10.1051/0004-6361/200911928 6339:10.1051/0004-6361/200912039 6289:10.1051/0004-6361/201014543 5975:10.1051/0004-6361/201116934 5925:10.1051/0004-6361/201116968 5878:10.1051/0004-6361/200912684 5820:10.1051/0004-6361/200911911 5770:10.1051/epjconf/20101102001 5715:10.1051/0004-6361/200912011 5660:10.1051/0004-6361/200911926 5548:DLR German Aerospace Center 5432:10.1051/epjconf/20101101001 5334:"Les exoplanètes – Accueil" 5312:10.1051/0004-6361/200810860 4792: 2106:, a non-transiting planet. 1510:Hertzsprung–Russell diagram 1356:Hertzsprung–Russell diagram 631: 584:European Space Agency (ESA) 173:630 kg (1,390 lb) 10: 16074: 15150:Mars sample return mission 14970:European Data Relay System 14650:Meteosat Second Generation 14563:James Webb Space Telescope 14425:Jupiter Icy Moons Explorer 14107:European Data Relay System 14081:Concurrent Design Facility 13388:Orbiting Solar Observatory 11641:James Webb Space Telescope 10980:Astronomy and Astrophysics 10931:Astronomy and Astrophysics 10787:Astronomy and Astrophysics 10728:Astronomy and Astrophysics 10663:Astronomy and Astrophysics 10551:Astronomy and Astrophysics 10496:Astronomy and Astrophysics 10457:Astronomy and Astrophysics 10397:Astronomy and Astrophysics 10341:Astronomy and Astrophysics 10285:Astronomy and Astrophysics 10230:Astronomy and Astrophysics 10183:Astronomy and Astrophysics 10127:Astronomy and Astrophysics 10071:Astronomy and Astrophysics 10015:Astronomy and Astrophysics 9959:Astronomy and Astrophysics 9903:Astronomy and Astrophysics 9782:Astronomy and Astrophysics 9726:Astronomy and Astrophysics 9671:Astronomy and Astrophysics 9615:Astronomy and Astrophysics 9559:Astronomy and Astrophysics 9503:Astronomy and Astrophysics 9447:Astronomy and Astrophysics 9391:Astronomy and Astrophysics 9335:Astronomy and Astrophysics 9280:Astronomy and Astrophysics 9225:Astronomy and Astrophysics 9134:Astronomy and Astrophysics 9113:Six new planets discovered 9051:Astronomy and Astrophysics 8852:Astronomy and Astrophysics 8739:Astronomy and Astrophysics 8605:Astronomy and Astrophysics 8581:10.1088/0004-637x/729/1/20 8497:Astronomy and Astrophysics 8442:Astronomy and Astrophysics 8387:Astronomy and Astrophysics 8332:Astronomy and Astrophysics 8293:Astronomy and Astrophysics 8252:Astronomy and Astrophysics 8016:Astronomy and Astrophysics 7821:10.1051/0004-6361:20064980 7790:Astronomy and Astrophysics 7726:10.1051/0004-6361:20034143 7704:Astronomy and Astrophysics 7560:Astronomy and Astrophysics 7380:Astronomy and Astrophysics 7266:Astronomy and Astrophysics 7242:10.1051/0004-6361:20042352 7211:Astronomy and Astrophysics 7172:Astronomy and Astrophysics 7117:Astronomy and Astrophysics 7062:Astronomy and Astrophysics 7007:Astronomy and Astrophysics 6952:Astronomy and Astrophysics 6905:Astronomy and Astrophysics 6850:Astronomy and Astrophysics 6795:Astronomy and Astrophysics 6740:Astronomy and Astrophysics 6642:Astronomy and Astrophysics 6532:Astronomy and Astrophysics 6470:Astronomy and Astrophysics 6360:Astronomy and Astrophysics 6317:Astronomy and Astrophysics 6258:Astronomy and Astrophysics 5953:Astronomy and Astrophysics 5894:Astronomy and Astrophysics 5847:Astronomy and Astrophysics 5798:Astronomy and Astrophysics 5684:Astronomy and Astrophysics 5629:Astronomy and Astrophysics 5486:10.1051/0004-6361:20030675 5455:Astronomy and Astrophysics 5281:Astronomy and Astrophysics 1745:properties of its members. 1724:V1449 Aquilae (HD 180642): 1512:; they are commonly named 1372:Astronomy and Astrophysics 580:French Space Agency (CNES) 29: 16028:Exoplanet search projects 16008:Satellites orbiting Earth 15981: 15868: 15842: 15784: 15716: 15686: 15570: 15516: 15485: 15435: 15396: 15359: 15338: 15223: 15188: 15050: 14979: 14909: 14841: 14773:Meteosat Third Generation 14632:Meteosat First Generation 14618: 14467: 14362: 14313: 14306: 14293: 14281:Planetary Science Archive 14248: 14227: 14115: 14094: 14066:European Astronaut Centre 14043: 14015: 13992: 13988: 13940:Category:Space telescopes 13930: 13889: 13744: 13645: 13614: 12867: 12719: 12564: 12467: 12282: 12173: 12007: 11962: 11901: 11894: 11822: 11797:Discoveries of exoplanets 11784: 11772:Terrestrial Planet Finder 11740: 11689: 11652: 11597: 11515: 11508: 11485: 11252: 11234: 11228:Exoplanet search projects 9094:ARTIFICA (28 July 2023). 6491:Astronomische Nachrichten 5371:"CoRoT N2 Public Archive" 5228:10.1038/nature.2012.11845 4860:Terrestrial Planet Finder 4756:of at least 70 days. The 3694: 3692: 3689: 3684: 3679: 3674: 2263:system detected by CoRoT. 2033:, were announced by ESA. 1750:The open cluster NGC 2264 754:This section needs to be 520: 516: 506: 498: 490: 480: 475: 471: 467: 454: 444: 434: 424: 414: 404: 394: 384: 374: 364: 354: 344: 334: 324: 319: 315: 311: 295: 287: 282: 278: 274: 260: 247: 233: 214: 209: 205: 201: 193: 185: 181:300 kg (660 lb) 177: 169: 157: 152: 148: 144: 134: 118: 105: 84: 70: 60: 56: 44: 13902:List of space telescopes 5069:"COROT sees first light" 582:in conjunction with the 14192:Living Planet Programme 14051:Space Operations Centre 11192:CoRoT N2 Public archive 11003:2011A&A...525A..68B 10947:2009A&A...506..303Q 10809:2015A&A...579A..36C 10750:2017A&A...602A.107B 10685:2016A&A...589A..62P 10628:2014A&A...562A.140P 10574:2014A&A...562A.140P 10519:2012A&A...537A..54R 10470:2012A&A...545A...6P 10420:2012A&A...538A.145D 10364:2012A&A...537A.136G 10308:2011A&A...533A.130H 10253:2011A&A...531A..41C 10206:2012A&A...541A.149O 10150:2011A&A...528A..97T 10094:2010A&A...522A.110C 10038:2010A&A...520A..97G 9982:2010A&A...524A..55G 9926:2010A&A...520A..65B 9805:2010A&A...520A..66B 9749:2009A&A...506..287L 9694:2010A&A...512A..14F 9638:2009A&A...506..281R 9582:2008A&A...488L..43A 9526:2008A&A...491..889D 9470:2008A&A...482L..21A 9414:2008A&A...482L..17B 9358:2010A&A...521L..59M 9303:2011A&A...532A..79S 9248:2009A&A...506..353A 9157:2010A&A...518L.153G 8993:ESO Picture of the Week 8875:2009A&A...508.1375M 8761:2013A&A...552A..60M 8628:2010A&A...519A..88A 8520:2013A&A...550A.121Z 8465:2013A&A...552A..68Z 8410:2011A&A...525A.101M 8355:2009A&A...502..937M 8306:2009A&A...506...95H 8265:2012A&A...539A..90N 8039:2011A&A...534A..98A 7813:2006A&A...459..589M 7717:2004A&A...415..251D 7582:2013A&A...552A..82G 7403:2011A&A...532A..86M 7289:2009A&A...503L..21M 7234:2005A&A...436..895G 7195:1995A&A...293...87K 7140:2010A&A...517A..22M 7085:2009A&A...506..465H 7030:2009A&A...506..167L 6975:2010A&A...509A..16S 6928:2010A&A...509A..15S 6873:2009A&A...507L..13B 6818:2010A&A...520L...6M 6763:2012A&A...540A..31M 6716:10.1023/a:1002016703076 6708:1998Ap&SS.261...21R 6665:2012A&A...542A..55P 6555:2010A&A...515A..87D 6373:2009A&A...506...95H 6330:2009A&A...506...85P 6281:2010A&A...519A..38D 6215:10.1126/science.1171913 6093:10.1126/science.1163004 5966:2012A&A...539A..14E 5917:2012A&A...538A.112C 5870:2009A&A...506..501C 5811:2009A&A...506..321M 5707:2009A&A...506..343D 5652:2009A&A...506..337A 5478:2003A&A...405.1137B 5304:2009A&A...506..411A 4815:Automated Planet Finder 1410:solar-like oscillations 1363:solar-like oscillations 1197:Spitzer Space Telescope 1070:Centre spatial de Liège 576:solar-like oscillations 502:1.1 m (43 in) 494:27 cm (11 in) 218:27 December 2006, 14:24 138:Planned: 2.5 + 4 years 14503:Hubble Space Telescope 14071:Space Astronomy Centre 13228:HEAO-2 (Einstein Obs.) 11187:CoRoT on the CNES site 10900:10.1093/mnras/stac2131 7697:Dupret, M.-A. (2004). 6512:10.1002/asna.201011435 5993:. pp. 1135–1158. 5991:Handbook of Exoplanets 5739:EPJ Web of Conferences 5402:EPJ Web of Conferences 4848:NASA Exoplanet Archive 4836:Kepler space telescope 4773: 4749: 4740: 2206: 1942: 1868: 1799:Calar Alto Observatory 1761:Christmas tree cluster 1719: 1556: 1544: 1476:stochastic excitations 1329:. Albeit with a lower 1318: 1289: 1279: 1269: 1259: 1068:(IAS) from Orsay, the 816:, for which planetary 697: 531: 32:Corot (disambiguation) 16058:Derelict space probes 14300:Projects and missions 13982:European Space Agency 12849:Space Solar Telescope 8937:Astrophysical Journal 8923:Astrophysical Journal 8551:Astrophysical Journal 7844:Astrophysical Journal 4771: 4746: 4738: 4306:5.616531 (± 0.000023) 4076:0.007 (+0.031 -0.007) 2203: 1936: 1865: 1815:The investigation of 1717: 1550: 1538: 1343:multiple star systems 1331:signal to noise ratio 1316: 1287: 1277: 1267: 1257: 1062:Observatoire de Paris 1041:European Space Agency 694: 554:tation and planetary 325:Reference system 153:Spacecraft properties 16038:Satellites of France 15322:Orbital launches in 14900:European Robotic Arm 14744:Sentinel-5 Precursor 13922:List of planetariums 12819:NRO donation to NASA 11183:at Wikimedia Commons 9118:17 June 2010 at the 8694:10.1093/mnras/stt003 7355:10.1093/mnras/sts345 5369:department, IAS IT. 4926:. N2YO. 8 March 2016 4883:. CNES. 17 June 2014 1939:La Silla Observatory 1891:: The binary system 1795:McDonald Observatory 1787:Very Large Telescope 1660:Seismic analyses of 1404:The solar-like star 1157:multiple star system 1149:Tautenburg telescope 1074:Alcatel Alenia Space 390:90.0336 degrees 30:For other uses, see 15225:Future missions in 14271:European Space Camp 14002:Guiana Space Centre 13618:(Mission completed) 11903:Radio and Microwave 11807:Lists of exoplanets 11578:detected exoplanets 11132:2013Icar..226.1625M 10966:on 11 January 2012. 10922:Queloz, D. (2009). 9860:10.1038/nature08856 9852:2010Natur.464..384D 8959:2012ApJ...746..185F 8818:2010MNRAS.401..418D 8685:2013MNRAS.430.1433A 8573:2011ApJ...729...20Z 8214:2012MNRAS.427..483B 8145:2004MNRAS.355..352A 8096:2004MNRAS.350.1022P 7982:2009MNRAS.396.1460D 7923:2008MNRAS.385.2061D 7866:2006ApJ...642L.165A 7666:2007MNRAS.381.1482B 7625:2009CoAst.158..220G 7529:2010ApJ...721L.182M 7468:10.1038/nature09935 7460:2011Natur.471..608B 7346:2013MNRAS.429..423M 6608:2008MNRAS.386.1487M 6504:2010AN....331..956B 6425:10.1038/nature08864 6417:2010Natur.464..259D 6207:2009Sci...324.1540B 6191:(5934): 1540–1542. 6147:10.1038/nature08022 6139:2009Natur.459..398D 6085:2008Sci...322..558M 5762:2011EPJWC..1102001S 5503:on 25 October 2007. 5424:2011EPJWC..1101001D 5167:. 18 September 2006 5042:NASASpaceFlight.com 4252:0.04290 (± 0.00092) 4249:3.22748 (± 0.00008) 4127:4.62941 (± 0.00075) 4070:9.06005 (± 0.00024) 2194:and a mass of 7.3 M 1249: 1008:CoRoT also studied 802:Galactic anticenter 543:ransits planétaires 430:213.16 degrees 420:148.21 degrees 416:Argument of perigee 299:17 June 2014, 10:27 164:Thales Alenia Space 41: 16033:Optical telescopes 15636:KUTESat Pathfinder 15075:Ceres Polar Lander 14910:Telecommunications 13555:Suzaku (Astro-EII) 13380:OAO-3 (Copernicus) 13364:Mikhailo Lomonosov 13212:Hinotori (Astro-A) 12814:New Worlds Mission 11722:New Worlds Mission 6477:(1). October 2009. 5557:on 24 October 2013 5011:SpaceflightNow.com 4956:on 9 December 2012 4807:Spaceflight portal 4774: 4750: 4741: 4300:0.68 (+0.47 -0.43) 4133:0.02 (+0.16 -0.02) 2207: 1943: 1869: 1838:eclipsing binaries 1832:A large number of 1732:star and named it 1720: 1651:(extra-mixed zone) 1635:totally unrelated. 1560:at maximum power ν 1557: 1545: 1319: 1303:frequency spectrum 1290: 1280: 1270: 1260: 1245: 1239:spherical harmonic 698: 604:rocket, reporting 564:extrasolar planets 440:14.44 rev/day 410:13.64 degrees 320:Orbital parameters 303:2014-06-17UTC10:28 222:2006-12-27UTC14:24 39: 15993: 15992: 15281: 15280: 15219: 15218: 14837: 14836: 14619:Earth observation 14449:Comet Interceptor 14440:Rosalind Franklin 14412:Trace Gas Orbiter 14363:Planetary science 14289: 14288: 14202:Science Programme 13948: 13947: 13846:SIM & SIMlite 13220:Hisaki (SPRINT-A) 13180:Hakucho (CORSA-b) 12734:Astro-1 Telescope 12560: 12559: 11854: 11853: 11792:Detection methods 11780: 11779: 11179:Media related to 9846:(7287): 384–387. 7769:978-3-7001-3974-4 7759:10.1553/cia144s35 7444:(7340): 608–611. 6498:(9–10): 956–960. 6411:(7286): 259–261. 6133:(7245): 398–400. 6069:(5901): 558–560. 6018:978-3-319-55332-0 5381:on 18 August 2011 5193:. 29 October 2009 5157:"COROT Satellite" 5107:. 2 February 2007 4980:COROT 2006 Events 4948:(Press release). 4761:be true planets, 4728: 4727: 4470: 4450: 4435: 4420: 4404: 4375: 4327:Other discoveries 4324: 4323: 2415: 2395: 2380: 2365: 2349: 2321: 1900:A low mass binary 1806:pre-main sequence 1797:in Texas, or the 1555:and collaborators 1543:and collaborators 1402:Solar-like stars: 1294: 1293: 1186:UVES spectrograph 1134:Follow-up program 1087:habitable planets 1054:Paris Observatory 775: 774: 710:13.5 μm × 13.5 μm 637:Spacecraft design 570:, and to perform 524: 523: 400:99.7 minutes 16:(Redirected from 16065: 16043:Space telescopes 15384: 15327: 15326: 15325: 15308: 15301: 15294: 15285: 15284: 15271: 15270: 15259: 15247: 15246: 15235: 15234: 15211:Schiaparelli EDM 15070:Calathus Mission 14894:Georges Lemaître 14852:ISS contribution 14311: 14310: 14295: 14294: 13990: 13989: 13975: 13968: 13961: 13952: 13951: 13938: 13937: 13737: 13733:Hitomi (Astro-H) 13729: 13721: 13713: 13705: 13697: 13689: 13681: 13673: 13665: 13657: 13638: 13630: 13619: 13607: 13599: 13591: 13583: 13575: 13567: 13559: 13551: 13543: 13535: 13527: 13519: 13511: 13503: 13495: 13487: 13479: 13471: 13463: 13455: 13447: 13439: 13384: 13376: 13368: 13360: 13352: 13344: 13336: 13328: 13320: 13312: 13304: 13296: 13288: 13280: 13272: 13264: 13256: 13248: 13240: 13232: 13224: 13216: 13208: 13200: 13192: 13184: 13176: 13168: 13160: 13152: 13144: 13136: 13128: 13120: 13112: 13104: 13096: 13088: 13080: 13072: 13064: 13056: 13048: 13040: 13032: 13024: 13016: 13008: 12983: 12975: 12967: 12959: 12951: 12943: 12935: 12927: 12919: 12911: 12903: 12895: 12887: 12879: 12712: 12704: 12696: 12688: 12680: 12672: 12664: 12656: 12648: 12640: 12632: 12624: 12616: 12608: 12600: 12592: 12584: 12576: 12553: 12545: 12537: 12529: 12521: 12513: 12505: 12497: 12489: 12481: 12470:or unclassified) 12460: 12452: 12444: 12436: 12428: 12420: 12412: 12404: 12396: 12388: 12380: 12372: 12364: 12356: 12348: 12340: 12332: 12324: 12316: 12308: 12300: 12275: 12267: 12259: 12251: 12243: 12235: 12227: 12219: 12215:Hinode (Solar-B) 12211: 12203: 12195: 12187: 12166: 12158: 12150: 12142: 12134: 12126: 12118: 12110: 12106:Hinode (Solar-B) 12102: 12094: 12086: 12078: 12070: 12062: 12054: 12046: 12038: 12029: 12021: 12000: 11992: 11984: 11976: 11955: 11947: 11939: 11931: 11923: 11915: 11899: 11898: 11888:Space telescopes 11881: 11874: 11867: 11858: 11857: 11842: 11841: 11830: 11829: 11682: 11674: 11666: 11645: 11637: 11627: 11619: 11611: 11590: 11580: 11573: 11565: 11562: 11549: 11541: 11538: 11527: 11513: 11512: 11503: 11497: 11491: 11295:FINDS Exo-Earths 11221: 11214: 11207: 11198: 11197: 11178: 11162: 11161: 11143: 11125: 11116:(2): 1625–1634. 11105: 11099: 11098: 11096: 11094: 11074: 11068: 11067: 11049: 11029: 11023: 11022: 10996: 10974: 10968: 10967: 10965: 10959:. Archived from 10958: 10928: 10919: 10913: 10912: 10902: 10892: 10868: 10857: 10850: 10844: 10837: 10831: 10830: 10820: 10802: 10778: 10772: 10771: 10761: 10743: 10719: 10713: 10712: 10678: 10654: 10648: 10647: 10621: 10600: 10594: 10593: 10567: 10545: 10539: 10538: 10512: 10490: 10484: 10483: 10481: 10446: 10440: 10439: 10413: 10390: 10384: 10383: 10357: 10334: 10328: 10327: 10301: 10279: 10273: 10272: 10246: 10224: 10218: 10217: 10199: 10176: 10170: 10169: 10143: 10120: 10114: 10113: 10087: 10064: 10058: 10057: 10031: 10008: 10002: 10001: 9975: 9952: 9946: 9945: 9919: 9896: 9890: 9889: 9871: 9831: 9825: 9824: 9798: 9775: 9769: 9768: 9742: 9720: 9714: 9713: 9687: 9664: 9658: 9657: 9631: 9608: 9602: 9601: 9575: 9552: 9546: 9545: 9519: 9496: 9490: 9489: 9463: 9440: 9434: 9433: 9407: 9384: 9378: 9377: 9351: 9329: 9323: 9322: 9296: 9274: 9268: 9267: 9241: 9219: 9213: 9212: 9211:. 23 April 2015. 9201: 9195: 9194: 9183: 9177: 9176: 9150: 9128: 9122: 9110: 9104: 9103: 9091: 9085: 9084: 9082: 9080: 9065: 9059: 9047: 9045: 9043: 9032: 9026: 9025: 9023: 9021: 9010: 9004: 9003: 9001: 8999: 8985: 8979: 8978: 8952: 8932: 8926: 8919: 8913: 8910: 8904: 8901: 8895: 8894: 8868: 8859:(3): 1375–1389. 8846: 8840: 8839: 8829: 8811: 8787: 8781: 8780: 8754: 8734: 8728: 8727: 8725: 8713: 8707: 8706: 8696: 8678: 8669:(2): 1433–1446. 8654: 8648: 8647: 8621: 8599: 8593: 8592: 8566: 8546: 8540: 8539: 8513: 8491: 8485: 8484: 8458: 8436: 8430: 8429: 8403: 8381: 8375: 8374: 8348: 8326: 8320: 8319: 8317: 8283: 8277: 8276: 8242: 8236: 8235: 8225: 8207: 8183: 8177: 8176: 8166: 8156: 8124: 8118: 8117: 8107: 8089: 8087:astro-ph/0402354 8080:(3): 1022–1028. 8065: 8059: 8058: 8032: 8010: 8004: 8003: 7993: 7975: 7966:(3): 1460–1472. 7951: 7945: 7944: 7934: 7916: 7907:(4): 2061–2068. 7892: 7886: 7885: 7859: 7857:astro-ph/0604037 7839: 7833: 7832: 7806: 7804:astro-ph/0607261 7784: 7778: 7777: 7761: 7737: 7731: 7730: 7728: 7694: 7688: 7687: 7677: 7659: 7650:(4): 1482–1488. 7635: 7629: 7628: 7608: 7602: 7601: 7575: 7555: 7549: 7548: 7522: 7502: 7496: 7495: 7453: 7429: 7423: 7422: 7396: 7374: 7368: 7367: 7357: 7339: 7315: 7309: 7308: 7282: 7260: 7254: 7253: 7227: 7225:astro-ph/0504047 7205: 7199: 7198: 7188: 7186:astro-ph/9403015 7166: 7160: 7159: 7133: 7111: 7105: 7104: 7078: 7056: 7050: 7049: 7023: 7001: 6995: 6994: 6968: 6946: 6940: 6939: 6921: 6899: 6893: 6892: 6866: 6844: 6838: 6837: 6811: 6789: 6783: 6782: 6756: 6734: 6728: 6727: 6691: 6685: 6684: 6658: 6636: 6630: 6629: 6619: 6601: 6592:(3): 1487–1502. 6575: 6569: 6568: 6566: 6548: 6522: 6516: 6515: 6485: 6479: 6478: 6461: 6455: 6454: 6436: 6396: 6387: 6386: 6384: 6350: 6344: 6343: 6341: 6307: 6301: 6300: 6274: 6252: 6243: 6242: 6200: 6176: 6167: 6166: 6122: 6113: 6112: 6078: 6058: 6049: 6048: 6037: 6031: 6030: 6002: 5986: 5980: 5979: 5977: 5943: 5937: 5936: 5910: 5888: 5882: 5881: 5863: 5841: 5835: 5834: 5832: 5822: 5788: 5782: 5781: 5755: 5733: 5727: 5726: 5700: 5678: 5672: 5671: 5645: 5623: 5617: 5616: 5614: 5612: 5602: 5596: 5595: 5593: 5591: 5576: 5567: 5566: 5564: 5562: 5556: 5545: 5537: 5531: 5530: 5528: 5526: 5511: 5505: 5504: 5502: 5496:. Archived from 5471: 5469:astro-ph/0305159 5462:(3): 1137–1144. 5451: 5442: 5436: 5435: 5417: 5397: 5391: 5390: 5388: 5386: 5377:. Archived from 5366: 5360: 5359: 5348: 5342: 5341: 5330: 5324: 5323: 5297: 5275: 5266: 5265: 5263: 5261: 5246: 5240: 5239: 5209: 5203: 5202: 5200: 5198: 5183: 5177: 5176: 5174: 5172: 5153: 5144: 5143: 5141: 5139: 5128: 5117: 5116: 5114: 5112: 5097: 5091: 5090: 5088: 5086: 5077:. Archived from 5064: 5058: 5057: 5055: 5053: 5044:. Archived from 5033: 5027: 5026: 5024: 5022: 5013:. Archived from 5002: 4996: 4995: 4993: 4991: 4972: 4966: 4965: 4963: 4961: 4942: 4936: 4935: 4933: 4931: 4920: 4893: 4892: 4890: 4888: 4877: 4832: 4809: 4804: 4803: 4802: 4681: 4671: 4619: 4609: 4557: 4547: 4495: 4464: 4444: 4429: 4411: 4395: 4369: 4334: 4280: 4223: 4193: 4191: 4184: 4182: 4158: 4101: 4044: 3983: 3933: 3879: 3822: 3768: 3687: 3630: 3573: 3464: 3407: 3350: 3293: 3236: 3179: 3122: 3065: 3008: 2951: 2894: 2837: 2780: 2724: 2667: 2611: 2554: 2497: 2440: 2409: 2389: 2374: 2356: 2340: 2315: 2280: 2012:asteroseismology 1840:with members of 1758:. The so-called 1506:red giant branch 1420:Sub-giant stars: 1389:extra mixed zone 1250: 1244: 1235:Asteroseismology 1145:stellar binaries 1120:asteroseismology 1034: 1012:. It can detect 1010:asteroseismology 770: 767: 761: 749: 748: 741: 723:asteroseismology 715:asteroseismology 711: 706:E2V Technologies 678:asteroseismology 676:10mm thick. The 572:asteroseismology 568:terrestrial size 545: 460: 459: 366:Perigee altitude 306: 304: 225: 223: 210:Start of mission 135:Mission duration 130: 127: 125: 110: 101: 100: 94: 49: 42: 38: 21: 16073: 16072: 16068: 16067: 16066: 16064: 16063: 16062: 15998: 15997: 15994: 15989: 15984: 15977: 15864: 15838: 15780: 15712: 15682: 15566: 15512: 15481: 15431: 15392: 15380: 15355: 15334: 15333: 15323: 15321: 15320: 15318: 15312: 15282: 15277: 15215: 15184: 15052: 15046: 15027:LISA Pathfinder 14984: 14982: 14975: 14905: 14888:Albert Einstein 14876:Johannes Kepler 14833: 14614: 14472: 14470: 14463: 14358: 14302: 14285: 14244: 14223: 14111: 14090: 14039: 14017:Launch vehicles 14011: 13984: 13979: 13949: 13944: 13926: 13912:X-ray telescope 13885: 13767:Constellation-X 13740: 13735: 13727: 13719: 13711: 13703: 13695: 13687: 13679: 13671: 13663: 13655: 13641: 13636: 13628: 13617: 13616: 13610: 13605: 13603:Yokoh (Solar-A) 13597: 13589: 13581: 13573: 13571:Tenma (Astro-B) 13565: 13557: 13549: 13541: 13533: 13525: 13517: 13509: 13501: 13493: 13485: 13477: 13469: 13461: 13453: 13445: 13437: 13382: 13374: 13366: 13358: 13350: 13342: 13334: 13332:LISA Pathfinder 13326: 13318: 13310: 13302: 13294: 13286: 13278: 13270: 13262: 13254: 13246: 13238: 13230: 13222: 13214: 13206: 13198: 13190: 13188:HALCA (MUSES-B) 13182: 13174: 13166: 13164:Ginga (Astro-C) 13158: 13150: 13142: 13134: 13126: 13118: 13110: 13102: 13094: 13086: 13078: 13070: 13062: 13054: 13046: 13038: 13030: 13022: 13014: 13006: 12981: 12973: 12965: 12957: 12949: 12941: 12933: 12925: 12917: 12909: 12901: 12893: 12885: 12883:Akari (Astro-F) 12877: 12863: 12715: 12710: 12702: 12694: 12686: 12678: 12670: 12662: 12654: 12646: 12638: 12630: 12622: 12614: 12606: 12598: 12590: 12582: 12574: 12556: 12551: 12543: 12535: 12527: 12519: 12511: 12503: 12495: 12487: 12479: 12469: 12468:Other (particle 12463: 12458: 12450: 12442: 12434: 12426: 12418: 12410: 12402: 12394: 12386: 12378: 12370: 12362: 12354: 12346: 12338: 12330: 12322: 12314: 12306: 12298: 12278: 12273: 12265: 12257: 12249: 12241: 12233: 12225: 12217: 12209: 12201: 12193: 12185: 12169: 12164: 12156: 12148: 12140: 12132: 12124: 12116: 12108: 12100: 12092: 12084: 12076: 12068: 12060: 12052: 12044: 12036: 12027: 12019: 12003: 11998: 11990: 11982: 11974: 11958: 11953: 11945: 11937: 11929: 11921: 11913: 11890: 11885: 11855: 11850: 11818: 11776: 11736: 11685: 11680: 11672: 11664: 11648: 11643: 11635: 11625: 11617: 11609: 11593: 11588: 11576: 11571: 11563: 11555: 11547: 11539: 11533: 11525: 11504: 11498: 11492: 11483: 11248: 11230: 11225: 11171: 11166: 11165: 11141:10.1.1.767.8062 11106: 11102: 11092: 11090: 11076: 11075: 11071: 11030: 11026: 10975: 10971: 10963: 10926: 10920: 10916: 10869: 10860: 10851: 10847: 10838: 10834: 10779: 10775: 10720: 10716: 10655: 10651: 10601: 10597: 10546: 10542: 10491: 10487: 10447: 10443: 10391: 10387: 10335: 10331: 10280: 10276: 10225: 10221: 10177: 10173: 10121: 10117: 10065: 10061: 10009: 10005: 9953: 9949: 9897: 9893: 9832: 9828: 9776: 9772: 9721: 9717: 9665: 9661: 9609: 9605: 9553: 9549: 9497: 9493: 9441: 9437: 9385: 9381: 9330: 9326: 9275: 9271: 9220: 9216: 9203: 9202: 9198: 9185: 9184: 9180: 9129: 9125: 9120:Wayback Machine 9111: 9107: 9092: 9088: 9078: 9076: 9068:Doreen Walton. 9066: 9062: 9041: 9039: 9034: 9033: 9029: 9019: 9017: 9012: 9011: 9007: 8997: 8995: 8987: 8986: 8982: 8933: 8929: 8920: 8916: 8911: 8907: 8902: 8898: 8847: 8843: 8788: 8784: 8735: 8731: 8714: 8710: 8655: 8651: 8600: 8596: 8547: 8543: 8492: 8488: 8437: 8433: 8382: 8378: 8327: 8323: 8284: 8280: 8243: 8239: 8184: 8180: 8125: 8121: 8066: 8062: 8011: 8007: 7952: 7948: 7893: 7889: 7840: 7836: 7785: 7781: 7770: 7738: 7734: 7695: 7691: 7636: 7632: 7609: 7605: 7556: 7552: 7503: 7499: 7430: 7426: 7375: 7371: 7316: 7312: 7261: 7257: 7206: 7202: 7167: 7163: 7112: 7108: 7057: 7053: 7002: 6998: 6947: 6943: 6900: 6896: 6845: 6841: 6790: 6786: 6735: 6731: 6692: 6688: 6637: 6633: 6576: 6572: 6523: 6519: 6486: 6482: 6463: 6462: 6458: 6397: 6390: 6351: 6347: 6308: 6304: 6253: 6246: 6177: 6170: 6123: 6116: 6059: 6052: 6039: 6038: 6034: 6019: 5987: 5983: 5944: 5940: 5889: 5885: 5842: 5838: 5789: 5785: 5734: 5730: 5679: 5675: 5624: 5620: 5610: 5608: 5604: 5603: 5599: 5589: 5587: 5586:on 29 June 2008 5578: 5577: 5570: 5560: 5558: 5554: 5543: 5539: 5538: 5534: 5524: 5522: 5521:on 15 June 2008 5513: 5512: 5508: 5500: 5449: 5443: 5439: 5398: 5394: 5384: 5382: 5367: 5363: 5352:"CoRoTsky Tool" 5350: 5349: 5345: 5338:media4.obspm.fr 5332: 5331: 5327: 5276: 5269: 5259: 5257: 5248: 5247: 5243: 5210: 5206: 5196: 5194: 5185: 5184: 5180: 5170: 5168: 5155: 5154: 5147: 5137: 5135: 5130: 5129: 5120: 5110: 5108: 5099: 5098: 5094: 5084: 5082: 5065: 5061: 5051: 5049: 5048:on 29 June 2008 5034: 5030: 5020: 5018: 5003: 4999: 4989: 4987: 4974: 4973: 4969: 4959: 4957: 4944: 4943: 4939: 4929: 4927: 4922: 4921: 4896: 4886: 4884: 4879: 4878: 4874: 4869: 4830: 4805: 4800: 4798: 4795: 4780: 4758:detection team 4733: 4679: 4667: 4617: 4605: 4555: 4543: 4493: 4474: 4463: 4455: 4443: 4440: 4428: 4425: 4417: 4410: 4401: 4394: 4380: 4361: 4349: 4329: 4309:0.066 (± 0.007) 4278: 4221: 4189: 4187: 4180: 4178: 4156: 4099: 4073:0.084 (± 0.001) 4042: 3981: 3931: 3877: 3820: 3766: 3685: 3628: 3571: 3462: 3405: 3348: 3291: 3234: 3177: 3120: 3063: 3006: 2949: 2892: 2835: 2778: 2722: 2665: 2609: 2552: 2495: 2438: 2419: 2408: 2400: 2388: 2385: 2373: 2370: 2362: 2355: 2346: 2339: 2326: 2307: 2295: 2270: 2258: 2248: 2238: 2219: 2212: 2197: 2193: 2174: 2158: 1997: 1973: 1931: 1913: 1909: 1879:CoRoT 102918586 1830: 1793:in Hawaii, the 1752: 1704:Plaskett's star 1670:β Canis Majoris 1658:β Cephei stars: 1642: 1563: 1519: 1497: 1460: 1433: 1415: 1381: 1298:helioseismology 1230: 1225: 1136: 1111: 1082: 1049: 1032: 794:Galactic Center 771: 765: 762: 759: 750: 746: 739: 709: 639: 634: 560:space telescope 558:ransits) was a 455: 376:Apogee altitude 346:Semi-major axis 302: 300: 267: 221: 219: 162: 139: 122: 95: 90: 65:Space telescope 52: 35: 28: 23: 22: 15: 12: 11: 5: 16071: 16061: 16060: 16055: 16050: 16045: 16040: 16035: 16030: 16025: 16020: 16015: 16010: 15991: 15990: 15986:Crewed flights 15982: 15979: 15978: 15976: 15975: 15970: 15957: 15952: 15947: 15942: 15933: 15928: 15923: 15887: 15878: 15872: 15870: 15866: 15865: 15863: 15862: 15857: 15852: 15846: 15844: 15840: 15839: 15837: 15836: 15831: 15826: 15821: 15812: 15807: 15802: 15788: 15786: 15782: 15781: 15779: 15778: 15773: 15760: 15753: 15748: 15743: 15738: 15726: 15720: 15718: 15714: 15713: 15711: 15710: 15705: 15696: 15690: 15688: 15684: 15683: 15681: 15680: 15675: 15604: 15599: 15594: 15587: 15574: 15572: 15568: 15567: 15565: 15564: 15559: 15554: 15549: 15536: 15531: 15526: 15524:Resurs-DK No.1 15520: 15518: 15514: 15513: 15511: 15510: 15501: 15495: 15489: 15487: 15483: 15482: 15480: 15479: 15470: 15465: 15460: 15455: 15450: 15445: 15439: 15437: 15433: 15432: 15430: 15429: 15422: 15415: 15410: 15400: 15398: 15394: 15393: 15391: 15390: 15385: 15382:CUTE-1.7 + APD 15374: 15369: 15363: 15361: 15357: 15356: 15354: 15353: 15348: 15342: 15340: 15336: 15335: 15329: 15314: 15311: 15310: 15303: 15296: 15288: 15279: 15278: 15276: 15275: 15265: 15253: 15241: 15224: 15221: 15220: 15217: 15216: 15214: 15213: 15208: 15203: 15198: 15192: 15190: 15186: 15185: 15183: 15182: 15177: 15172: 15167: 15162: 15157: 15152: 15147: 15142: 15137: 15132: 15127: 15122: 15117: 15112: 15107: 15102: 15097: 15092: 15090:Darwin Mission 15087: 15082: 15077: 15072: 15067: 15062: 15056: 15054: 15048: 15047: 15045: 15044: 15036: 15035:(2019–present) 15030: 15024: 15018: 15017:(2013–present) 15012: 15011:(2009–present) 15006: 15000: 14999:(2001–present) 14994: 14987: 14985: 14980: 14977: 14976: 14974: 14973: 14972:(2016–present) 14967: 14962: 14961:(2014–present) 14956: 14955:(2011–present) 14950: 14949:(2010–present) 14944: 14943:(2008–present) 14938: 14937:(2005–present) 14932: 14931:(2001–present) 14926: 14920: 14913: 14911: 14907: 14906: 14904: 14903: 14897: 14891: 14885: 14882:Edoardo Amaldi 14879: 14873: 14872:(2010–present) 14867: 14861: 14860:(2008–present) 14855: 14854:(1998–present) 14848: 14846: 14839: 14838: 14835: 14834: 14832: 14831: 14823: 14815: 14807: 14799: 14791: 14783: 14769: 14761: 14753: 14752:(2018–present) 14747: 14746:(2017–present) 14741: 14740:(2016–present) 14727: 14726:(2015–present) 14709: 14708:(2014–present) 14695: 14694:(2013–present) 14689: 14688:(2010–present) 14683: 14682:(2009–present) 14677: 14671: 14670:(2006–present) 14665: 14659: 14653: 14652:(2002–present) 14647: 14641: 14635: 14629: 14628:(1988–present) 14622: 14620: 14616: 14615: 14613: 14612: 14604: 14596: 14588: 14580: 14572: 14571:(2023–present) 14566: 14565:(2021–present) 14560: 14559:(2019–present) 14554: 14553:(2013–present) 14548: 14542: 14536: 14530: 14529:(2002–present) 14524: 14523:(1999–present) 14518: 14512: 14506: 14505:(1990–present) 14500: 14494: 14488: 14482: 14475: 14473: 14468: 14465: 14464: 14462: 14461: 14453: 14445: 14436: 14428: 14422: 14421:(2018–present) 14416: 14415:(2016–present) 14407: 14401: 14391: 14390:(2003–present) 14385: 14379: 14373: 14366: 14364: 14360: 14359: 14357: 14356: 14348: 14347:(2020–present) 14342: 14336: 14335:(1995–present) 14330: 14324: 14317: 14315: 14308: 14304: 14303: 14291: 14290: 14287: 14286: 14284: 14283: 14278: 14273: 14268: 14263: 14261:ESA Television 14258: 14252: 14250: 14249:Related topics 14246: 14245: 14243: 14242: 14237: 14231: 14229: 14225: 14224: 14222: 14221: 14216: 14215: 14214: 14209: 14199: 14194: 14189: 14184: 14179: 14174: 14169: 14164: 14159: 14154: 14153: 14152: 14142: 14137: 14132: 14131: 14130: 14119: 14117: 14113: 14112: 14110: 14109: 14104: 14098: 14096: 14095:Communications 14092: 14091: 14089: 14088: 14083: 14078: 14073: 14068: 14063: 14058: 14053: 14047: 14045: 14041: 14040: 14038: 14037: 14032: 14027: 14021: 14019: 14013: 14012: 14010: 14009: 14004: 13998: 13996: 13986: 13985: 13978: 13977: 13970: 13963: 13955: 13946: 13945: 13943: 13942: 13931: 13928: 13927: 13925: 13924: 13919: 13914: 13909: 13904: 13899: 13893: 13891: 13887: 13886: 13884: 13883: 13878: 13873: 13868: 13863: 13858: 13853: 13848: 13843: 13838: 13833: 13828: 13823: 13818: 13813: 13808: 13803: 13798: 13793: 13786: 13781: 13776: 13769: 13764: 13759: 13754: 13748: 13746: 13742: 13741: 13739: 13738: 13730: 13722: 13714: 13706: 13698: 13690: 13682: 13674: 13666: 13658: 13649: 13647: 13643: 13642: 13640: 13639: 13631: 13622: 13620: 13612: 13611: 13609: 13608: 13600: 13592: 13584: 13576: 13568: 13560: 13552: 13544: 13536: 13528: 13520: 13512: 13504: 13496: 13488: 13480: 13472: 13464: 13456: 13448: 13440: 13432: 13431: 13430: 13425: 13420: 13415: 13410: 13405: 13400: 13395: 13385: 13377: 13369: 13361: 13353: 13345: 13337: 13329: 13321: 13313: 13305: 13297: 13289: 13281: 13273: 13265: 13257: 13249: 13241: 13233: 13225: 13217: 13209: 13201: 13193: 13185: 13177: 13169: 13161: 13153: 13145: 13137: 13129: 13121: 13113: 13105: 13097: 13089: 13081: 13073: 13065: 13057: 13049: 13044:Compton (CGRO) 13041: 13033: 13025: 13017: 13009: 12996: 12995: 12994: 12989: 12976: 12971:ASCA (Astro-D) 12968: 12960: 12952: 12944: 12936: 12928: 12920: 12912: 12904: 12896: 12888: 12880: 12871: 12869: 12865: 12864: 12862: 12861: 12856: 12851: 12846: 12841: 12836: 12831: 12826: 12821: 12816: 12811: 12806: 12801: 12796: 12791: 12786: 12781: 12776: 12771: 12769:Hypertelescope 12766: 12761: 12756: 12751: 12749:Fresnel Imager 12746: 12741: 12736: 12731: 12725: 12723: 12717: 12716: 12714: 12713: 12705: 12697: 12689: 12681: 12673: 12665: 12657: 12649: 12641: 12633: 12625: 12617: 12609: 12601: 12593: 12585: 12577: 12568: 12566: 12562: 12561: 12558: 12557: 12555: 12554: 12546: 12538: 12530: 12522: 12514: 12506: 12498: 12490: 12482: 12473: 12471: 12465: 12464: 12462: 12461: 12453: 12445: 12437: 12429: 12421: 12413: 12405: 12397: 12392:Max Valier Sat 12389: 12381: 12373: 12365: 12357: 12349: 12341: 12333: 12328:HXMT (Insight) 12325: 12320:Einstein Probe 12317: 12309: 12304:Chandra (AXAF) 12301: 12292: 12290: 12280: 12279: 12277: 12276: 12268: 12260: 12252: 12244: 12236: 12228: 12220: 12212: 12204: 12196: 12188: 12179: 12177: 12171: 12170: 12168: 12167: 12159: 12151: 12143: 12135: 12127: 12119: 12111: 12103: 12095: 12087: 12079: 12071: 12063: 12055: 12047: 12039: 12035:constellation 12030: 12022: 12013: 12011: 12005: 12004: 12002: 12001: 11993: 11985: 11977: 11968: 11966: 11960: 11959: 11957: 11956: 11948: 11940: 11932: 11924: 11916: 11907: 11905: 11896: 11892: 11891: 11884: 11883: 11876: 11869: 11861: 11852: 11851: 11849: 11848: 11836: 11823: 11820: 11819: 11817: 11816: 11815: 11814: 11804: 11799: 11794: 11788: 11786: 11782: 11781: 11778: 11777: 11775: 11774: 11769: 11764: 11757: 11752: 11744: 11742: 11738: 11737: 11735: 11734: 11729: 11724: 11719: 11714: 11709: 11704: 11699: 11693: 11691: 11687: 11686: 11684: 11683: 11675: 11667: 11656: 11654: 11650: 11649: 11647: 11646: 11644:(2021–present) 11638: 11636:(2021–present) 11628: 11626:(2019–present) 11620: 11618:(2018–present) 11612: 11610:(2013–present) 11601: 11599: 11595: 11594: 11592: 11591: 11583: 11582: 11581: 11566: 11550: 11542: 11528: 11519: 11517: 11510: 11509:Space missions 11506: 11505: 11486: 11484: 11482: 11481: 11476: 11471: 11466: 11461: 11456: 11451: 11446: 11441: 11436: 11431: 11426: 11421: 11416: 11411: 11406: 11401: 11396: 11391: 11386: 11385: 11384: 11374: 11369: 11364: 11359: 11354: 11349: 11344: 11339: 11334: 11329: 11324: 11319: 11314: 11313: 11312: 11307: 11297: 11292: 11287: 11282: 11277: 11272: 11267: 11262: 11256: 11254: 11250: 11249: 11247: 11246: 11241: 11239:Exoplanetology 11235: 11232: 11231: 11224: 11223: 11216: 11209: 11201: 11195: 11194: 11189: 11184: 11170: 11169:External links 11167: 11164: 11163: 11100: 11069: 11024: 10969: 10941:(1): 303–319. 10914: 10883:(1): 636–655. 10858: 10845: 10832: 10773: 10714: 10649: 10595: 10540: 10485: 10441: 10385: 10329: 10274: 10219: 10171: 10115: 10059: 10003: 9947: 9891: 9826: 9770: 9733:(1): 287–302. 9715: 9659: 9622:(1): 281–286. 9603: 9566:(2): L43–L46. 9547: 9510:(3): 889–897. 9491: 9454:(3): L21–L24. 9435: 9398:(3): L17–L20. 9379: 9324: 9269: 9232:(1): 353–358. 9214: 9196: 9178: 9123: 9105: 9086: 9060: 9027: 9005: 8980: 8927: 8914: 8905: 8896: 8841: 8802:(1): 418–432. 8782: 8729: 8708: 8649: 8594: 8541: 8486: 8431: 8376: 8339:(3): 937–950. 8321: 8278: 8237: 8198:(1): 483–493. 8178: 8139:(2): 352–358. 8119: 8060: 8005: 7946: 7887: 7874:10.1086/504634 7834: 7797:(2): 589–596. 7779: 7768: 7732: 7689: 7630: 7603: 7550: 7497: 7424: 7369: 7330:(1): 423–428. 7310: 7255: 7218:(3): 895–915. 7200: 7161: 7106: 7069:(1): 465–469. 7051: 7014:(1): 167–173. 6996: 6941: 6894: 6839: 6784: 6729: 6686: 6631: 6570: 6517: 6480: 6456: 6388: 6345: 6302: 6244: 6168: 6114: 6050: 6032: 6017: 5981: 5938: 5883: 5854:(1): 501–517. 5836: 5805:(1): 321–336. 5783: 5728: 5691:(1): 343–352. 5673: 5636:(1): 337–341. 5618: 5597: 5568: 5532: 5506: 5437: 5392: 5361: 5343: 5325: 5288:(1): 411–424. 5267: 5256:. 24 June 2013 5254:SpaceDaily.com 5241: 5204: 5191:SpaceDaily.com 5178: 5145: 5118: 5092: 5081:on 17 May 2008 5059: 5028: 5017:on 17 May 2008 4997: 4967: 4937: 4894: 4871: 4870: 4868: 4865: 4864: 4863: 4857: 4851: 4845: 4839: 4833: 4824: 4818: 4811: 4810: 4794: 4791: 4778: 4732: 4729: 4726: 4725: 4723: 4720: 4717: 4714: 4711: 4708: 4705: 4702: 4699: 4694: 4691: 4688: 4685: 4682: 4677: 4672: 4664: 4663: 4661: 4658: 4655: 4652: 4649: 4646: 4643: 4640: 4637: 4632: 4629: 4626: 4623: 4620: 4615: 4610: 4602: 4601: 4599: 4596: 4593: 4590: 4587: 4584: 4581: 4578: 4575: 4570: 4567: 4564: 4561: 4558: 4553: 4548: 4540: 4539: 4537: 4534: 4531: 4528: 4525: 4522: 4519: 4516: 4513: 4508: 4505: 4502: 4499: 4496: 4491: 4486: 4480: 4479: 4476: 4471: 4458: 4451: 4436: 4421: 4415: 4405: 4399: 4389: 4386: 4383: 4376: 4364: 4357: 4352: 4345: 4340: 4328: 4325: 4322: 4321: 4319: 4316: 4315:85.83 (± 0.26) 4313: 4310: 4307: 4304: 4301: 4298: 4293: 4290: 4287: 4284: 4281: 4276: 4271: 4265: 4264: 4262: 4259: 4256: 4253: 4250: 4247: 4244: 4241: 4236: 4233: 4230: 4227: 4224: 4219: 4214: 4208: 4207: 4205: 4203: 4201: 4199: 4197: 4194: 4185: 4176: 4171: 4168: 4165: 4162: 4159: 4154: 4149: 4143: 4142: 4140: 4137: 4134: 4131: 4128: 4125: 4122: 4119: 4114: 4111: 4108: 4105: 4102: 4097: 4092: 4086: 4085: 4083: 4080: 4077: 4074: 4071: 4068: 4065: 4062: 4057: 4054: 4051: 4048: 4045: 4040: 4035: 4029: 4028: 4022: 4019: 4016: 4013: 4010: 4007: 4004: 4001: 3996: 3993: 3990: 3987: 3984: 3979: 3974: 3970: 3969: 3967: 3965: 3963: 3961: 3959: 3957: 3954: 3951: 3946: 3943: 3940: 3937: 3934: 3929: 3924: 3920: 3919: 3917: 3914: 3912: 3909: 3906: 3903: 3900: 3897: 3892: 3889: 3886: 3883: 3880: 3875: 3870: 3864: 3863: 3861: 3858: 3855: 3852: 3849: 3846: 3843: 3840: 3835: 3832: 3829: 3826: 3823: 3818: 3813: 3809: 3808: 3806: 3803: 3800: 3798: 3795: 3792: 3789: 3786: 3781: 3778: 3775: 3772: 3769: 3764: 3759: 3753: 3752: 3750: 3747: 3745: 3743: 3741: 3738: 3735: 3732: 3727: 3724: 3723: 3721: 3718: 3716: 3714: 3712: 3709: 3706: 3703: 3698: 3696: 3693: 3691: 3688: 3683: 3678: 3672: 3671: 3669: 3666: 3663: 3660: 3657: 3654: 3651: 3648: 3643: 3640: 3637: 3634: 3631: 3626: 3621: 3615: 3614: 3612: 3609: 3606: 3603: 3600: 3597: 3594: 3591: 3586: 3583: 3580: 3577: 3574: 3569: 3564: 3558: 3557: 3555: 3552: 3549: 3546: 3543: 3540: 3537: 3534: 3529: 3526: 3524: 3521: 3519: 3517: 3512: 3506: 3505: 3503: 3500: 3497: 3494: 3491: 3488: 3485: 3482: 3477: 3474: 3471: 3468: 3465: 3460: 3455: 3449: 3448: 3446: 3443: 3440: 3437: 3434: 3431: 3428: 3425: 3420: 3417: 3414: 3411: 3408: 3403: 3398: 3392: 3391: 3389: 3386: 3383: 3380: 3377: 3374: 3371: 3368: 3363: 3360: 3357: 3354: 3351: 3346: 3341: 3335: 3334: 3332: 3329: 3326: 3323: 3320: 3317: 3314: 3311: 3306: 3303: 3300: 3297: 3294: 3289: 3284: 3278: 3277: 3275: 3272: 3269: 3266: 3263: 3260: 3257: 3254: 3249: 3246: 3243: 3240: 3237: 3232: 3227: 3221: 3220: 3218: 3215: 3212: 3209: 3206: 3203: 3200: 3197: 3192: 3189: 3186: 3183: 3180: 3175: 3170: 3164: 3163: 3161: 3158: 3155: 3152: 3149: 3146: 3143: 3140: 3135: 3132: 3129: 3126: 3123: 3118: 3113: 3107: 3106: 3104: 3101: 3098: 3095: 3092: 3089: 3086: 3083: 3078: 3075: 3072: 3069: 3066: 3061: 3056: 3050: 3049: 3047: 3044: 3041: 3038: 3035: 3032: 3029: 3026: 3021: 3018: 3015: 3012: 3009: 3004: 2999: 2993: 2992: 2990: 2987: 2984: 2981: 2978: 2975: 2972: 2969: 2964: 2961: 2958: 2955: 2952: 2947: 2942: 2936: 2935: 2933: 2930: 2927: 2924: 2921: 2918: 2915: 2912: 2907: 2904: 2901: 2898: 2895: 2890: 2885: 2879: 2878: 2876: 2873: 2870: 2867: 2864: 2861: 2858: 2855: 2850: 2847: 2844: 2841: 2838: 2833: 2828: 2822: 2821: 2819: 2816: 2813: 2810: 2807: 2804: 2801: 2798: 2793: 2790: 2787: 2784: 2781: 2776: 2771: 2765: 2764: 2762: 2759: 2756: 2753: 2750: 2747: 2744: 2741: 2736: 2733: 2731: 2728: 2725: 2720: 2715: 2709: 2708: 2706: 2703: 2700: 2697: 2694: 2691: 2688: 2685: 2680: 2677: 2674: 2671: 2668: 2663: 2658: 2652: 2651: 2649: 2646: 2643: 2640: 2637: 2634: 2631: 2628: 2623: 2620: 2618: 2615: 2612: 2607: 2602: 2596: 2595: 2593: 2590: 2587: 2584: 2581: 2578: 2575: 2572: 2567: 2564: 2561: 2558: 2555: 2550: 2545: 2539: 2538: 2536: 2533: 2530: 2527: 2524: 2521: 2518: 2515: 2510: 2507: 2504: 2501: 2498: 2493: 2488: 2482: 2481: 2479: 2476: 2473: 2470: 2467: 2464: 2461: 2458: 2453: 2450: 2447: 2444: 2441: 2436: 2431: 2425: 2424: 2421: 2416: 2403: 2396: 2381: 2366: 2360: 2350: 2344: 2334: 2329: 2322: 2310: 2303: 2298: 2291: 2286: 2269: 2266: 2265: 2264: 2256: 2253: 2250: 2246: 2243: 2240: 2236: 2233: 2221: 2217: 2214: 2210: 2195: 2191: 2188: 2172: 2169: 2157: 2154: 2051:In March 2010 1996: 1993: 1971: 1930: 1927: 1926: 1925: 1922:beaming effect 1915: 1911: 1907: 1906:star of 0.23 M 1897: 1886: 1876: 1870: 1850:AU Monocerotis 1834:binary systems 1829: 1828:Binary systems 1826: 1789:in Chile, the 1751: 1748: 1747: 1746: 1739: 1708: 1707: 1696: 1689: 1686:V2052 Ophiuchi 1641: 1638: 1637: 1636: 1621: 1592: 1561: 1517: 1496: 1493: 1492: 1491: 1484: 1468: 1459: 1456: 1455: 1454: 1435: 1431: 1417: 1413: 1392:their life as 1380: 1377: 1292: 1291: 1281: 1271: 1261: 1229: 1226: 1224: 1221: 1135: 1132: 1110: 1107: 1103:transit method 1091:transit method 1081: 1078: 1048: 1045: 986: 985: 979: 973: 963: 957: 951: 945: 935: 929: 923: 917: 911: 905: 899: 893: 887: 881: 875: 869: 863: 857: 851: 845: 839: 833: 822:types of stars 773: 772: 753: 751: 744: 738: 737:Mission design 735: 638: 635: 633: 630: 522: 521: 518: 517: 514: 513: 508: 504: 503: 500: 496: 495: 492: 488: 487: 482: 478: 477: 476:Main telescope 473: 472: 469: 468: 465: 464: 461: 452: 451: 448: 442: 441: 438: 432: 431: 428: 422: 421: 418: 412: 411: 408: 402: 401: 398: 392: 391: 388: 382: 381: 378: 372: 371: 368: 362: 361: 358: 352: 351: 348: 342: 341: 336: 332: 331: 326: 322: 321: 317: 316: 313: 312: 309: 308: 297: 293: 292: 291:Decommissioned 289: 285: 284: 283:End of mission 280: 279: 276: 275: 272: 271: 262: 258: 257: 249: 245: 244: 235: 231: 230: 216: 212: 211: 207: 206: 203: 202: 199: 198: 195: 191: 190: 187: 183: 182: 179: 175: 174: 171: 167: 166: 159: 155: 154: 150: 149: 146: 145: 142: 141: 136: 132: 131: 120: 116: 115: 112: 103: 102: 88: 82: 81: 72: 68: 67: 62: 58: 57: 54: 53: 50: 26: 9: 6: 4: 3: 2: 16070: 16059: 16056: 16054: 16051: 16049: 16046: 16044: 16041: 16039: 16036: 16034: 16031: 16029: 16026: 16024: 16021: 16019: 16016: 16014: 16011: 16009: 16006: 16005: 16003: 15996: 15987: 15980: 15974: 15971: 15969: 15965: 15961: 15958: 15956: 15953: 15951: 15948: 15946: 15943: 15941: 15937: 15934: 15932: 15929: 15927: 15924: 15921: 15917: 15913: 15909: 15905: 15901: 15897: 15893: 15892: 15888: 15886: 15882: 15879: 15877: 15874: 15873: 15871: 15867: 15861: 15858: 15856: 15853: 15851: 15848: 15847: 15845: 15841: 15835: 15832: 15830: 15827: 15825: 15822: 15820: 15816: 15813: 15811: 15810:Progress M-58 15808: 15806: 15803: 15801: 15797: 15793: 15790: 15789: 15787: 15783: 15777: 15774: 15772: 15768: 15764: 15761: 15759: 15758: 15754: 15752: 15749: 15747: 15744: 15742: 15739: 15736: 15732: 15731: 15727: 15725: 15722: 15721: 15719: 15715: 15709: 15706: 15704: 15700: 15697: 15695: 15692: 15691: 15689: 15685: 15679: 15676: 15674: 15673: 15669: 15665: 15661: 15657: 15653: 15649: 15645: 15641: 15637: 15633: 15629: 15625: 15621: 15617: 15613: 15609: 15605: 15603: 15600: 15598: 15595: 15593: 15592: 15588: 15585: 15581: 15580: 15576: 15575: 15573: 15569: 15563: 15560: 15558: 15555: 15553: 15552:Progress M-57 15550: 15548: 15544: 15540: 15537: 15535: 15532: 15530: 15527: 15525: 15522: 15521: 15519: 15515: 15509: 15505: 15502: 15499: 15496: 15494: 15491: 15490: 15488: 15484: 15478: 15474: 15471: 15469: 15466: 15464: 15461: 15459: 15458:Progress M-56 15456: 15454: 15451: 15449: 15446: 15444: 15441: 15440: 15438: 15434: 15428: 15427: 15423: 15421: 15420: 15416: 15414: 15411: 15409: 15405: 15402: 15401: 15399: 15395: 15389: 15386: 15383: 15378: 15375: 15373: 15370: 15368: 15365: 15364: 15362: 15358: 15352: 15349: 15347: 15344: 15343: 15341: 15337: 15332: 15328: 15317: 15309: 15304: 15302: 15297: 15295: 15290: 15289: 15286: 15274: 15266: 15264: 15263: 15258: 15254: 15252: 15251: 15242: 15240: 15239: 15230: 15229: 15228: 15222: 15212: 15209: 15207: 15204: 15202: 15199: 15197: 15194: 15193: 15191: 15187: 15181: 15178: 15176: 15173: 15171: 15168: 15166: 15163: 15161: 15158: 15156: 15153: 15151: 15148: 15146: 15143: 15141: 15138: 15136: 15133: 15131: 15128: 15126: 15123: 15121: 15118: 15116: 15113: 15111: 15108: 15106: 15103: 15101: 15098: 15096: 15093: 15091: 15088: 15086: 15083: 15081: 15078: 15076: 15073: 15071: 15068: 15066: 15063: 15061: 15058: 15057: 15055: 15049: 15042: 15041: 15037: 15034: 15031: 15028: 15025: 15022: 15019: 15016: 15013: 15010: 15007: 15004: 15001: 14998: 14995: 14992: 14989: 14988: 14986: 14983:demonstrators 14978: 14971: 14968: 14966: 14963: 14960: 14957: 14954: 14951: 14948: 14945: 14942: 14939: 14936: 14933: 14930: 14927: 14924: 14921: 14918: 14915: 14914: 14912: 14908: 14901: 14898: 14895: 14892: 14889: 14886: 14883: 14880: 14877: 14874: 14871: 14868: 14865: 14862: 14859: 14856: 14853: 14850: 14849: 14847: 14844: 14840: 14829: 14828: 14824: 14821: 14820: 14816: 14813: 14812: 14808: 14805: 14804: 14800: 14797: 14796: 14792: 14789: 14788: 14784: 14781: 14780: 14775: 14774: 14770: 14767: 14766: 14762: 14759: 14758: 14754: 14751: 14748: 14745: 14742: 14739: 14735: 14731: 14728: 14725: 14721: 14717: 14713: 14710: 14707: 14703: 14699: 14696: 14693: 14690: 14687: 14684: 14681: 14678: 14675: 14672: 14669: 14666: 14663: 14660: 14657: 14654: 14651: 14648: 14645: 14642: 14639: 14636: 14633: 14630: 14627: 14624: 14623: 14621: 14617: 14610: 14609: 14605: 14602: 14601: 14597: 14594: 14593: 14589: 14586: 14585: 14581: 14578: 14577: 14573: 14570: 14567: 14564: 14561: 14558: 14555: 14552: 14549: 14546: 14543: 14540: 14537: 14534: 14531: 14528: 14525: 14522: 14519: 14516: 14513: 14510: 14507: 14504: 14501: 14498: 14495: 14492: 14489: 14486: 14483: 14480: 14477: 14476: 14474: 14469:Astronomy and 14466: 14459: 14458: 14454: 14451: 14450: 14446: 14443: 14441: 14437: 14434: 14433: 14429: 14426: 14423: 14420: 14417: 14414: 14413: 14408: 14405: 14404:Venus Express 14402: 14399: 14395: 14392: 14389: 14386: 14383: 14380: 14377: 14374: 14371: 14368: 14367: 14365: 14361: 14354: 14353: 14349: 14346: 14345:Solar Orbiter 14343: 14340: 14337: 14334: 14331: 14328: 14325: 14322: 14319: 14318: 14316: 14314:Solar physics 14312: 14309: 14305: 14301: 14296: 14292: 14282: 14279: 14277: 14274: 14272: 14269: 14267: 14264: 14262: 14259: 14257: 14254: 14253: 14251: 14247: 14241: 14238: 14236: 14233: 14232: 14230: 14226: 14220: 14217: 14213: 14212:Cosmic Vision 14210: 14208: 14205: 14204: 14203: 14200: 14198: 14195: 14193: 14190: 14188: 14185: 14183: 14180: 14178: 14175: 14173: 14170: 14168: 14165: 14163: 14160: 14158: 14155: 14151: 14148: 14147: 14146: 14143: 14141: 14138: 14136: 14133: 14129: 14126: 14125: 14124: 14121: 14120: 14118: 14114: 14108: 14105: 14103: 14100: 14099: 14097: 14093: 14087: 14084: 14082: 14079: 14077: 14074: 14072: 14069: 14067: 14064: 14062: 14059: 14057: 14054: 14052: 14049: 14048: 14046: 14042: 14036: 14033: 14031: 14028: 14026: 14023: 14022: 14020: 14018: 14014: 14008: 14005: 14003: 14000: 13999: 13997: 13995: 13991: 13987: 13983: 13976: 13971: 13969: 13964: 13962: 13957: 13956: 13953: 13941: 13933: 13932: 13929: 13923: 13920: 13918: 13915: 13913: 13910: 13908: 13905: 13903: 13900: 13898: 13895: 13894: 13892: 13888: 13882: 13879: 13877: 13874: 13872: 13869: 13867: 13864: 13862: 13859: 13857: 13854: 13852: 13849: 13847: 13844: 13842: 13839: 13837: 13834: 13832: 13829: 13827: 13824: 13822: 13819: 13817: 13814: 13812: 13809: 13807: 13804: 13802: 13799: 13797: 13794: 13792: 13791: 13787: 13785: 13782: 13780: 13777: 13775: 13774: 13770: 13768: 13765: 13763: 13760: 13758: 13755: 13753: 13750: 13749: 13747: 13743: 13734: 13731: 13726: 13723: 13718: 13715: 13710: 13707: 13702: 13699: 13694: 13691: 13686: 13683: 13678: 13675: 13670: 13667: 13662: 13659: 13654: 13651: 13650: 13648: 13644: 13635: 13632: 13627: 13624: 13623: 13621: 13613: 13604: 13601: 13596: 13593: 13588: 13585: 13580: 13577: 13572: 13569: 13564: 13563:Taiyo (SRATS) 13561: 13556: 13553: 13548: 13545: 13540: 13537: 13532: 13529: 13524: 13521: 13516: 13513: 13508: 13505: 13500: 13497: 13492: 13489: 13484: 13481: 13476: 13473: 13468: 13465: 13460: 13457: 13452: 13449: 13444: 13441: 13436: 13433: 13429: 13426: 13424: 13421: 13419: 13416: 13414: 13411: 13409: 13406: 13404: 13401: 13399: 13396: 13394: 13391: 13390: 13389: 13386: 13381: 13378: 13373: 13370: 13365: 13362: 13357: 13354: 13349: 13346: 13341: 13338: 13333: 13330: 13325: 13322: 13317: 13314: 13309: 13306: 13301: 13298: 13293: 13290: 13285: 13282: 13277: 13274: 13269: 13266: 13261: 13258: 13253: 13250: 13245: 13242: 13237: 13234: 13229: 13226: 13221: 13218: 13213: 13210: 13205: 13202: 13197: 13194: 13189: 13186: 13181: 13178: 13173: 13170: 13165: 13162: 13157: 13154: 13149: 13146: 13141: 13138: 13133: 13130: 13125: 13122: 13117: 13114: 13109: 13106: 13101: 13098: 13093: 13090: 13085: 13082: 13077: 13074: 13069: 13066: 13061: 13058: 13053: 13050: 13045: 13042: 13037: 13034: 13029: 13026: 13021: 13018: 13013: 13010: 13004: 13000: 12997: 12993: 12990: 12988: 12985: 12984: 12980: 12977: 12972: 12969: 12964: 12961: 12956: 12953: 12948: 12945: 12940: 12937: 12932: 12929: 12924: 12921: 12916: 12913: 12908: 12905: 12900: 12897: 12892: 12889: 12884: 12881: 12876: 12873: 12872: 12870: 12866: 12860: 12857: 12855: 12852: 12850: 12847: 12845: 12842: 12840: 12837: 12835: 12832: 12830: 12827: 12825: 12822: 12820: 12817: 12815: 12812: 12810: 12807: 12805: 12802: 12800: 12797: 12795: 12792: 12790: 12787: 12785: 12782: 12780: 12777: 12775: 12772: 12770: 12767: 12765: 12762: 12760: 12757: 12755: 12752: 12750: 12747: 12745: 12742: 12740: 12737: 12735: 12732: 12730: 12727: 12726: 12724: 12722: 12718: 12709: 12706: 12701: 12698: 12693: 12690: 12685: 12682: 12677: 12674: 12669: 12666: 12661: 12658: 12653: 12650: 12645: 12644:Solar-C EUVST 12642: 12637: 12634: 12629: 12626: 12621: 12618: 12613: 12610: 12605: 12602: 12597: 12594: 12589: 12586: 12581: 12578: 12573: 12570: 12569: 12567: 12563: 12550: 12547: 12542: 12541:Solar Orbiter 12539: 12534: 12531: 12526: 12523: 12518: 12515: 12510: 12507: 12502: 12499: 12494: 12491: 12486: 12483: 12478: 12475: 12474: 12472: 12466: 12457: 12454: 12449: 12446: 12441: 12438: 12433: 12430: 12425: 12422: 12417: 12414: 12409: 12406: 12401: 12398: 12393: 12390: 12385: 12382: 12377: 12374: 12369: 12366: 12361: 12358: 12353: 12350: 12345: 12342: 12337: 12334: 12329: 12326: 12321: 12318: 12313: 12310: 12305: 12302: 12297: 12294: 12293: 12291: 12289: 12285: 12281: 12272: 12269: 12264: 12261: 12256: 12255:Solar Orbiter 12253: 12248: 12245: 12240: 12237: 12232: 12229: 12224: 12221: 12216: 12213: 12208: 12205: 12200: 12197: 12192: 12189: 12184: 12181: 12180: 12178: 12176: 12172: 12163: 12160: 12155: 12152: 12147: 12144: 12139: 12136: 12131: 12128: 12123: 12120: 12115: 12112: 12107: 12104: 12099: 12096: 12091: 12088: 12083: 12080: 12075: 12072: 12067: 12064: 12059: 12056: 12051: 12048: 12043: 12040: 12034: 12031: 12026: 12023: 12018: 12015: 12014: 12012: 12010: 12006: 11997: 11994: 11989: 11986: 11981: 11978: 11973: 11970: 11969: 11967: 11965: 11961: 11952: 11949: 11944: 11941: 11936: 11933: 11928: 11925: 11920: 11919:Solar Orbiter 11917: 11912: 11909: 11908: 11906: 11904: 11900: 11897: 11893: 11889: 11882: 11877: 11875: 11870: 11868: 11863: 11862: 11859: 11847: 11846: 11837: 11835: 11834: 11825: 11824: 11821: 11813: 11810: 11809: 11808: 11805: 11803: 11800: 11798: 11795: 11793: 11790: 11789: 11787: 11783: 11773: 11770: 11768: 11765: 11763: 11762: 11758: 11756: 11753: 11751: 11750: 11746: 11745: 11743: 11739: 11733: 11730: 11728: 11725: 11723: 11720: 11718: 11715: 11713: 11710: 11708: 11705: 11703: 11700: 11698: 11695: 11694: 11692: 11688: 11679: 11676: 11671: 11668: 11663: 11662: 11658: 11657: 11655: 11651: 11642: 11639: 11634: 11633: 11629: 11624: 11621: 11616: 11613: 11608: 11607: 11603: 11602: 11600: 11596: 11587: 11584: 11579: 11575: 11574: 11570: 11567: 11561: 11560: 11554: 11551: 11546: 11543: 11537: 11532: 11529: 11524: 11521: 11520: 11518: 11514: 11511: 11507: 11502: 11496: 11490: 11480: 11479:ZIMPOL/CHEOPS 11477: 11475: 11472: 11470: 11467: 11465: 11462: 11460: 11457: 11455: 11452: 11450: 11447: 11445: 11442: 11440: 11437: 11435: 11432: 11430: 11427: 11425: 11422: 11420: 11417: 11415: 11412: 11410: 11407: 11405: 11402: 11400: 11397: 11395: 11392: 11390: 11387: 11383: 11380: 11379: 11378: 11375: 11373: 11370: 11368: 11365: 11363: 11360: 11358: 11355: 11353: 11350: 11348: 11345: 11343: 11340: 11338: 11335: 11333: 11330: 11328: 11325: 11323: 11320: 11318: 11315: 11311: 11308: 11306: 11303: 11302: 11301: 11298: 11296: 11293: 11291: 11288: 11286: 11283: 11281: 11278: 11276: 11273: 11271: 11268: 11266: 11263: 11261: 11258: 11257: 11255: 11251: 11245: 11242: 11240: 11237: 11236: 11233: 11229: 11222: 11217: 11215: 11210: 11208: 11203: 11202: 11199: 11193: 11190: 11188: 11185: 11182: 11177: 11173: 11172: 11159: 11155: 11151: 11147: 11142: 11137: 11133: 11129: 11124: 11119: 11115: 11111: 11104: 11089: 11085: 11084: 11079: 11073: 11065: 11061: 11057: 11053: 11048: 11043: 11039: 11035: 11028: 11020: 11016: 11012: 11008: 11004: 11000: 10995: 10990: 10986: 10982: 10981: 10973: 10962: 10957: 10952: 10948: 10944: 10940: 10936: 10932: 10925: 10918: 10910: 10906: 10901: 10896: 10891: 10886: 10882: 10878: 10874: 10867: 10865: 10863: 10855: 10849: 10842: 10836: 10828: 10824: 10819: 10814: 10810: 10806: 10801: 10796: 10792: 10788: 10784: 10777: 10769: 10765: 10760: 10755: 10751: 10747: 10742: 10737: 10733: 10729: 10725: 10718: 10710: 10706: 10702: 10698: 10694: 10690: 10686: 10682: 10677: 10672: 10668: 10664: 10660: 10653: 10645: 10641: 10637: 10633: 10629: 10625: 10620: 10615: 10611: 10607: 10599: 10591: 10587: 10583: 10579: 10575: 10571: 10566: 10561: 10557: 10553: 10552: 10544: 10536: 10532: 10528: 10524: 10520: 10516: 10511: 10506: 10502: 10498: 10497: 10489: 10480: 10475: 10471: 10467: 10463: 10459: 10458: 10453: 10445: 10437: 10433: 10429: 10425: 10421: 10417: 10412: 10407: 10403: 10399: 10398: 10389: 10381: 10377: 10373: 10369: 10365: 10361: 10356: 10351: 10347: 10343: 10342: 10333: 10325: 10321: 10317: 10313: 10309: 10305: 10300: 10295: 10291: 10287: 10286: 10278: 10270: 10266: 10262: 10258: 10254: 10250: 10245: 10240: 10236: 10232: 10231: 10223: 10215: 10211: 10207: 10203: 10198: 10193: 10189: 10185: 10184: 10175: 10167: 10163: 10159: 10155: 10151: 10147: 10142: 10137: 10133: 10129: 10128: 10119: 10111: 10107: 10103: 10099: 10095: 10091: 10086: 10081: 10077: 10073: 10072: 10063: 10055: 10051: 10047: 10043: 10039: 10035: 10030: 10025: 10021: 10017: 10016: 10007: 9999: 9995: 9991: 9987: 9983: 9979: 9974: 9969: 9965: 9961: 9960: 9951: 9943: 9939: 9935: 9931: 9927: 9923: 9918: 9913: 9909: 9905: 9904: 9895: 9887: 9883: 9879: 9875: 9870: 9865: 9861: 9857: 9853: 9849: 9845: 9841: 9837: 9830: 9822: 9818: 9814: 9810: 9806: 9802: 9797: 9792: 9788: 9784: 9783: 9774: 9766: 9762: 9758: 9754: 9750: 9746: 9741: 9736: 9732: 9728: 9727: 9719: 9711: 9707: 9703: 9699: 9695: 9691: 9686: 9681: 9677: 9673: 9672: 9663: 9655: 9651: 9647: 9643: 9639: 9635: 9630: 9625: 9621: 9617: 9616: 9607: 9599: 9595: 9591: 9587: 9583: 9579: 9574: 9569: 9565: 9561: 9560: 9551: 9543: 9539: 9535: 9531: 9527: 9523: 9518: 9513: 9509: 9505: 9504: 9495: 9487: 9483: 9479: 9475: 9471: 9467: 9462: 9457: 9453: 9449: 9448: 9439: 9431: 9427: 9423: 9419: 9415: 9411: 9406: 9401: 9397: 9393: 9392: 9383: 9375: 9371: 9367: 9363: 9359: 9355: 9350: 9345: 9341: 9337: 9336: 9328: 9320: 9316: 9312: 9308: 9304: 9300: 9295: 9290: 9286: 9282: 9281: 9273: 9265: 9261: 9257: 9253: 9249: 9245: 9240: 9235: 9231: 9227: 9226: 9218: 9210: 9206: 9200: 9192: 9188: 9182: 9174: 9170: 9166: 9162: 9158: 9154: 9149: 9144: 9140: 9136: 9135: 9127: 9121: 9117: 9114: 9109: 9101: 9097: 9090: 9075: 9071: 9064: 9057: 9054:in May 2008 ( 9053: 9052: 9037: 9031: 9015: 9009: 8994: 8990: 8984: 8976: 8972: 8968: 8964: 8960: 8956: 8951: 8946: 8942: 8938: 8931: 8924: 8918: 8909: 8900: 8892: 8888: 8884: 8880: 8876: 8872: 8867: 8862: 8858: 8854: 8853: 8845: 8837: 8833: 8828: 8823: 8819: 8815: 8810: 8805: 8801: 8797: 8793: 8786: 8778: 8774: 8770: 8766: 8762: 8758: 8753: 8748: 8744: 8740: 8733: 8724: 8719: 8712: 8704: 8700: 8695: 8690: 8686: 8682: 8677: 8672: 8668: 8664: 8660: 8653: 8645: 8641: 8637: 8633: 8629: 8625: 8620: 8615: 8611: 8607: 8606: 8598: 8590: 8586: 8582: 8578: 8574: 8570: 8565: 8560: 8556: 8552: 8545: 8537: 8533: 8529: 8525: 8521: 8517: 8512: 8507: 8503: 8499: 8498: 8490: 8482: 8478: 8474: 8470: 8466: 8462: 8457: 8452: 8448: 8444: 8443: 8435: 8427: 8423: 8419: 8415: 8411: 8407: 8402: 8397: 8393: 8389: 8388: 8380: 8372: 8368: 8364: 8360: 8356: 8352: 8347: 8342: 8338: 8334: 8333: 8325: 8316: 8311: 8307: 8303: 8300:(1): 95–101. 8299: 8295: 8294: 8289: 8282: 8274: 8270: 8266: 8262: 8258: 8254: 8253: 8248: 8241: 8233: 8229: 8224: 8219: 8215: 8211: 8206: 8201: 8197: 8193: 8189: 8182: 8174: 8170: 8165: 8160: 8155: 8150: 8146: 8142: 8138: 8134: 8130: 8123: 8115: 8111: 8106: 8101: 8097: 8093: 8088: 8083: 8079: 8075: 8071: 8064: 8056: 8052: 8048: 8044: 8040: 8036: 8031: 8026: 8022: 8018: 8017: 8009: 8001: 7997: 7992: 7987: 7983: 7979: 7974: 7969: 7965: 7961: 7957: 7950: 7942: 7938: 7933: 7928: 7924: 7920: 7915: 7910: 7906: 7902: 7898: 7891: 7883: 7879: 7875: 7871: 7867: 7863: 7858: 7853: 7849: 7845: 7838: 7830: 7826: 7822: 7818: 7814: 7810: 7805: 7800: 7796: 7792: 7791: 7783: 7775: 7771: 7765: 7760: 7755: 7751: 7747: 7743: 7736: 7727: 7722: 7718: 7714: 7710: 7706: 7705: 7700: 7693: 7685: 7681: 7676: 7671: 7667: 7663: 7658: 7653: 7649: 7645: 7641: 7634: 7626: 7622: 7618: 7614: 7607: 7599: 7595: 7591: 7587: 7583: 7579: 7574: 7569: 7565: 7561: 7554: 7546: 7542: 7538: 7534: 7530: 7526: 7521: 7516: 7512: 7508: 7501: 7493: 7489: 7485: 7481: 7477: 7473: 7469: 7465: 7461: 7457: 7452: 7447: 7443: 7439: 7435: 7428: 7420: 7416: 7412: 7408: 7404: 7400: 7395: 7390: 7386: 7382: 7381: 7373: 7365: 7361: 7356: 7351: 7347: 7343: 7338: 7333: 7329: 7325: 7321: 7314: 7306: 7302: 7298: 7294: 7290: 7286: 7281: 7276: 7272: 7268: 7267: 7259: 7251: 7247: 7243: 7239: 7235: 7231: 7226: 7221: 7217: 7213: 7212: 7204: 7196: 7192: 7187: 7182: 7178: 7174: 7173: 7165: 7157: 7153: 7149: 7145: 7141: 7137: 7132: 7127: 7123: 7119: 7118: 7110: 7102: 7098: 7094: 7090: 7086: 7082: 7077: 7072: 7068: 7064: 7063: 7055: 7047: 7043: 7039: 7035: 7031: 7027: 7022: 7017: 7013: 7009: 7008: 7000: 6992: 6988: 6984: 6980: 6976: 6972: 6967: 6962: 6958: 6954: 6953: 6945: 6937: 6933: 6929: 6925: 6920: 6915: 6911: 6907: 6906: 6898: 6890: 6886: 6882: 6878: 6874: 6870: 6865: 6860: 6856: 6852: 6851: 6843: 6835: 6831: 6827: 6823: 6819: 6815: 6810: 6805: 6801: 6797: 6796: 6788: 6780: 6776: 6772: 6768: 6764: 6760: 6755: 6750: 6746: 6742: 6741: 6733: 6725: 6721: 6717: 6713: 6709: 6705: 6701: 6697: 6690: 6682: 6678: 6674: 6670: 6666: 6662: 6657: 6652: 6648: 6644: 6643: 6635: 6627: 6623: 6618: 6613: 6609: 6605: 6600: 6595: 6591: 6587: 6586: 6581: 6574: 6565: 6560: 6556: 6552: 6547: 6542: 6538: 6534: 6533: 6528: 6521: 6513: 6509: 6505: 6501: 6497: 6493: 6492: 6484: 6476: 6472: 6471: 6466: 6460: 6452: 6448: 6444: 6440: 6435: 6430: 6426: 6422: 6418: 6414: 6410: 6406: 6402: 6395: 6393: 6383: 6378: 6374: 6370: 6367:(1): 95–101. 6366: 6362: 6361: 6356: 6349: 6340: 6335: 6331: 6327: 6323: 6319: 6318: 6313: 6306: 6298: 6294: 6290: 6286: 6282: 6278: 6273: 6268: 6264: 6260: 6259: 6251: 6249: 6240: 6236: 6232: 6228: 6224: 6220: 6216: 6212: 6208: 6204: 6199: 6194: 6190: 6186: 6182: 6175: 6173: 6164: 6160: 6156: 6152: 6148: 6144: 6140: 6136: 6132: 6128: 6121: 6119: 6110: 6106: 6102: 6098: 6094: 6090: 6086: 6082: 6077: 6072: 6068: 6064: 6057: 6055: 6046: 6042: 6036: 6028: 6024: 6020: 6014: 6010: 6006: 6001: 5996: 5992: 5985: 5976: 5971: 5967: 5963: 5959: 5955: 5954: 5949: 5942: 5934: 5930: 5926: 5922: 5918: 5914: 5909: 5904: 5900: 5896: 5895: 5887: 5879: 5875: 5871: 5867: 5862: 5857: 5853: 5849: 5848: 5840: 5831: 5826: 5821: 5816: 5812: 5808: 5804: 5800: 5799: 5794: 5787: 5779: 5775: 5771: 5767: 5763: 5759: 5754: 5749: 5745: 5741: 5740: 5732: 5724: 5720: 5716: 5712: 5708: 5704: 5699: 5694: 5690: 5686: 5685: 5677: 5669: 5665: 5661: 5657: 5653: 5649: 5644: 5639: 5635: 5631: 5630: 5622: 5607: 5601: 5585: 5581: 5575: 5573: 5553: 5549: 5542: 5536: 5520: 5516: 5510: 5499: 5495: 5491: 5487: 5483: 5479: 5475: 5470: 5465: 5461: 5457: 5456: 5448: 5441: 5433: 5429: 5425: 5421: 5416: 5411: 5407: 5403: 5396: 5380: 5376: 5372: 5365: 5357: 5353: 5347: 5339: 5335: 5329: 5321: 5317: 5313: 5309: 5305: 5301: 5296: 5291: 5287: 5283: 5282: 5274: 5272: 5255: 5251: 5245: 5237: 5233: 5229: 5225: 5221: 5220: 5215: 5208: 5192: 5188: 5182: 5166: 5162: 5158: 5152: 5150: 5133: 5127: 5125: 5123: 5106: 5102: 5096: 5080: 5076: 5075: 5074:Physics World 5070: 5063: 5047: 5043: 5039: 5032: 5016: 5012: 5008: 5001: 4986:. 24 May 2007 4985: 4981: 4977: 4971: 4955: 4951: 4947: 4941: 4925: 4919: 4917: 4915: 4913: 4911: 4909: 4907: 4905: 4903: 4901: 4899: 4882: 4876: 4872: 4861: 4858: 4855: 4852: 4849: 4846: 4843: 4840: 4837: 4834: 4828: 4825: 4822: 4819: 4816: 4813: 4812: 4808: 4797: 4790: 4786: 4782: 4770: 4766: 4764: 4759: 4755: 4745: 4737: 4724: 4721: 4718: 4715: 4712: 4709: 4706: 4703: 4700: 4698: 4695: 4692: 4689: 4686: 4683: 4678: 4676: 4673: 4670: 4666: 4665: 4662: 4659: 4656: 4653: 4650: 4647: 4644: 4641: 4638: 4636: 4633: 4630: 4627: 4624: 4621: 4616: 4614: 4611: 4608: 4604: 4603: 4600: 4597: 4594: 4591: 4588: 4585: 4582: 4579: 4576: 4574: 4571: 4568: 4565: 4562: 4559: 4554: 4552: 4549: 4546: 4542: 4541: 4538: 4535: 4532: 4529: 4526: 4523: 4520: 4517: 4514: 4512: 4509: 4506: 4503: 4500: 4497: 4492: 4490: 4487: 4485: 4482: 4481: 4477: 4472: 4468: 4462: 4459: 4457: 4452: 4448: 4442: 4437: 4433: 4427: 4422: 4418: 4409: 4406: 4402: 4393: 4390: 4387: 4384: 4382: 4377: 4373: 4368: 4365: 4363: 4358: 4356: 4353: 4351: 4346: 4344: 4343:Constellation 4341: 4339: 4336: 4332: 4320: 4317: 4314: 4311: 4308: 4305: 4303:1.41 (± 0.14) 4302: 4299: 4297: 4294: 4291: 4288: 4285: 4282: 4277: 4275: 4272: 4270: 4267: 4266: 4263: 4260: 4257: 4254: 4251: 4248: 4246:1.68 (± 0.11) 4245: 4243:1.10 (± 0.37) 4242: 4240: 4237: 4234: 4231: 4228: 4225: 4220: 4218: 4215: 4213: 4210: 4209: 4206: 4204: 4202: 4200: 4198: 4195: 4186: 4177: 4175: 4172: 4169: 4166: 4163: 4160: 4155: 4153: 4150: 4148: 4145: 4144: 4141: 4138: 4135: 4132: 4129: 4126: 4123: 4121:2.84 (± 0.22) 4120: 4118: 4115: 4112: 4109: 4106: 4103: 4098: 4096: 4093: 4091: 4088: 4087: 4084: 4081: 4079:90.0 (± 0.56) 4078: 4075: 4072: 4069: 4067:1.02 (± 0.08) 4066: 4064:0.84 (± 0.34) 4063: 4061: 4058: 4055: 4052: 4049: 4046: 4041: 4039: 4036: 4034: 4031: 4030: 4027: 4025: 4023: 4020: 4017: 4014: 4011: 4008: 4005: 4002: 4000: 3997: 3994: 3991: 3988: 3985: 3980: 3978: 3975: 3972: 3971: 3968: 3966: 3964: 3962: 3960: 3958: 3956:0.9550±0.0660 3955: 3952: 3950: 3947: 3944: 3941: 3938: 3935: 3930: 3928: 3925: 3922: 3921: 3918: 3915: 3913: 3910: 3907: 3904: 3901: 3898: 3896: 3893: 3890: 3887: 3884: 3881: 3876: 3874: 3871: 3869: 3866: 3865: 3862: 3859: 3856: 3853: 3850: 3847: 3844: 3841: 3839: 3836: 3833: 3830: 3827: 3824: 3819: 3817: 3814: 3811: 3810: 3807: 3804: 3801: 3799: 3796: 3793: 3790: 3787: 3785: 3782: 3779: 3776: 3773: 3770: 3765: 3763: 3760: 3758: 3755: 3754: 3751: 3748: 3746: 3744: 3742: 3739: 3736: 3733: 3731: 3728: 3726: 3725: 3722: 3719: 3717: 3715: 3713: 3710: 3707: 3704: 3702: 3699: 3697: 3682: 3677: 3673: 3670: 3667: 3664: 3661: 3658: 3655: 3652: 3649: 3647: 3644: 3641: 3638: 3635: 3632: 3627: 3625: 3622: 3620: 3617: 3616: 3613: 3610: 3607: 3604: 3601: 3598: 3595: 3592: 3590: 3587: 3584: 3581: 3578: 3575: 3570: 3568: 3565: 3563: 3560: 3559: 3556: 3553: 3550: 3547: 3544: 3541: 3538: 3535: 3533: 3530: 3527: 3525: 3522: 3520: 3518: 3516: 3513: 3511: 3508: 3507: 3504: 3501: 3498: 3495: 3492: 3489: 3486: 3483: 3481: 3478: 3475: 3472: 3469: 3466: 3461: 3459: 3456: 3454: 3451: 3450: 3447: 3444: 3441: 3438: 3435: 3432: 3429: 3426: 3424: 3421: 3418: 3415: 3412: 3409: 3404: 3402: 3399: 3397: 3394: 3393: 3390: 3387: 3384: 3381: 3378: 3375: 3372: 3369: 3367: 3364: 3361: 3358: 3355: 3352: 3347: 3345: 3342: 3340: 3337: 3336: 3333: 3330: 3327: 3324: 3321: 3318: 3315: 3312: 3310: 3307: 3304: 3301: 3298: 3295: 3290: 3288: 3285: 3283: 3280: 3279: 3276: 3273: 3270: 3267: 3264: 3261: 3258: 3255: 3253: 3250: 3247: 3244: 3241: 3238: 3233: 3231: 3228: 3226: 3223: 3222: 3219: 3216: 3213: 3210: 3207: 3204: 3201: 3198: 3196: 3193: 3190: 3187: 3184: 3181: 3176: 3174: 3171: 3169: 3166: 3165: 3162: 3159: 3156: 3153: 3150: 3147: 3144: 3141: 3139: 3136: 3133: 3130: 3127: 3124: 3119: 3117: 3114: 3112: 3109: 3108: 3105: 3102: 3099: 3096: 3093: 3090: 3087: 3084: 3082: 3079: 3076: 3073: 3070: 3067: 3062: 3060: 3057: 3055: 3052: 3051: 3048: 3045: 3042: 3039: 3036: 3033: 3030: 3027: 3025: 3022: 3019: 3016: 3013: 3010: 3005: 3003: 3000: 2998: 2995: 2994: 2991: 2988: 2985: 2982: 2979: 2976: 2973: 2970: 2968: 2965: 2962: 2959: 2956: 2953: 2948: 2946: 2943: 2941: 2938: 2937: 2934: 2931: 2928: 2925: 2922: 2919: 2916: 2913: 2911: 2908: 2905: 2902: 2899: 2896: 2891: 2889: 2886: 2884: 2881: 2880: 2877: 2874: 2871: 2868: 2865: 2862: 2859: 2856: 2854: 2851: 2848: 2845: 2842: 2839: 2834: 2832: 2829: 2827: 2824: 2823: 2820: 2817: 2814: 2811: 2808: 2805: 2802: 2799: 2797: 2794: 2791: 2788: 2785: 2782: 2777: 2775: 2772: 2770: 2767: 2766: 2763: 2760: 2757: 2754: 2751: 2748: 2745: 2742: 2740: 2737: 2734: 2732: 2729: 2726: 2721: 2719: 2716: 2714: 2711: 2710: 2707: 2704: 2701: 2698: 2695: 2692: 2689: 2686: 2684: 2681: 2678: 2675: 2672: 2669: 2664: 2662: 2659: 2657: 2654: 2653: 2650: 2647: 2644: 2641: 2638: 2635: 2632: 2629: 2627: 2624: 2621: 2619: 2616: 2613: 2608: 2606: 2603: 2601: 2598: 2597: 2594: 2591: 2588: 2585: 2582: 2579: 2576: 2573: 2571: 2568: 2565: 2562: 2559: 2556: 2551: 2549: 2546: 2544: 2541: 2540: 2537: 2534: 2531: 2528: 2525: 2522: 2519: 2516: 2514: 2511: 2508: 2505: 2502: 2499: 2494: 2492: 2489: 2487: 2484: 2483: 2480: 2477: 2474: 2471: 2468: 2465: 2462: 2459: 2457: 2454: 2451: 2448: 2445: 2442: 2437: 2435: 2432: 2430: 2427: 2426: 2422: 2417: 2413: 2407: 2404: 2402: 2397: 2393: 2387: 2382: 2378: 2372: 2367: 2363: 2354: 2351: 2347: 2338: 2335: 2333: 2330: 2328: 2323: 2319: 2314: 2311: 2309: 2304: 2302: 2299: 2297: 2292: 2290: 2289:Constellation 2287: 2285: 2282: 2278: 2277: 2273: 2262: 2254: 2251: 2244: 2241: 2234: 2231: 2226: 2222: 2215: 2202: 2189: 2186: 2182: 2178: 2170: 2167: 2163: 2162: 2161: 2153: 2150: 2148: 2144: 2140: 2136: 2132: 2128: 2124: 2120: 2116: 2112: 2107: 2105: 2101: 2097: 2093: 2089: 2085: 2081: 2077: 2073: 2069: 2065: 2061: 2056: 2054: 2049: 2047: 2043: 2039: 2034: 2032: 2028: 2024: 2020: 2015: 2013: 2010:. Results on 2009: 2005: 2002: 1992: 1989: 1983: 1981: 1977: 1969: 1965: 1961: 1957: 1953: 1949: 1940: 1935: 1923: 1919: 1916: 1914:star MS star. 1905: 1901: 1898: 1894: 1890: 1887: 1884: 1880: 1877: 1874: 1871: 1864: 1859: 1855: 1851: 1848: 1847: 1846: 1843: 1839: 1835: 1825: 1822: 1818: 1813: 1811: 1807: 1802: 1800: 1796: 1792: 1788: 1784: 1780: 1776: 1770: 1767: 1763: 1762: 1757: 1743: 1740: 1737: 1736: 1730: 1725: 1722: 1721: 1716: 1712: 1705: 1700: 1697: 1693: 1690: 1687: 1683: 1679: 1675: 1671: 1667: 1663: 1659: 1656: 1655: 1654: 1652: 1647: 1640:Massive stars 1634: 1629: 1625: 1622: 1618: 1615: 1611: 1608: 1604: 1601: 1596: 1593: 1590: 1589: 1583: 1582:Andrea Miglio 1578: 1574: 1570: 1567: 1566: 1565: 1554: 1553:Andrea Miglio 1549: 1542: 1541:Andrea Miglio 1537: 1533: 1531: 1527: 1523: 1515: 1511: 1507: 1503: 1488: 1485: 1482: 1477: 1472: 1469: 1465: 1462: 1461: 1452: 1448: 1443: 1439: 1436: 1429: 1425: 1421: 1418: 1411: 1407: 1403: 1400: 1399: 1398: 1395: 1390: 1386: 1385:main sequence 1376: 1374: 1373: 1368: 1367:δ Scuti stars 1364: 1359: 1357: 1353: 1349: 1344: 1340: 1336: 1332: 1328: 1324: 1315: 1311: 1309: 1304: 1299: 1286: 1282: 1276: 1272: 1266: 1262: 1256: 1252: 1251: 1248: 1243: 1240: 1236: 1220: 1216: 1214: 1210: 1206: 1202: 1198: 1193: 1191: 1187: 1182: 1178: 1174: 1170: 1166: 1165:spectrographs 1162: 1158: 1154: 1150: 1146: 1142: 1131: 1129: 1128:field of view 1125: 1121: 1118:dedicated to 1117: 1106: 1104: 1100: 1095: 1092: 1088: 1077: 1075: 1071: 1067: 1063: 1059: 1055: 1044: 1042: 1038: 1029: 1027: 1023: 1018: 1015: 1011: 1006: 1004: 1003:rocky planets 1000: 995: 991: 983: 980: 977: 974: 971: 967: 964: 961: 958: 955: 952: 949: 946: 943: 939: 936: 933: 930: 927: 924: 921: 918: 915: 912: 909: 906: 903: 900: 897: 894: 891: 888: 885: 882: 879: 876: 873: 870: 867: 864: 861: 858: 855: 852: 849: 846: 843: 840: 837: 834: 831: 828: 827: 826: 823: 819: 815: 811: 807: 803: 799: 795: 792:, toward the 791: 790:Serpens Cauda 786: 784: 780: 769: 757: 752: 743: 742: 734: 732: 728: 727:field of view 724: 720: 716: 707: 703: 693: 689: 687: 683: 679: 675: 671: 667: 663: 659: 656: 652: 651:opaque baffle 648: 644: 643:field of view 629: 627: 623: 619: 615: 611: 607: 603: 599: 594: 592: 587: 585: 581: 577: 574:by measuring 573: 569: 565: 561: 557: 553: 549: 544: 542: 538: 534: 528: 519: 515: 512: 511:Visible light 509: 505: 501: 497: 493: 489: 486: 483: 479: 474: 470: 466: 462: 453: 449: 447: 443: 439: 437: 433: 429: 427: 423: 419: 417: 413: 409: 407: 403: 399: 397: 393: 389: 387: 383: 379: 377: 373: 369: 367: 363: 359: 357: 353: 349: 347: 343: 340: 337: 333: 330: 327: 323: 318: 314: 310: 298: 294: 290: 286: 281: 277: 273: 270: 266: 263: 259: 256: 253: 250: 246: 243: 239: 236: 232: 229: 217: 213: 208: 204: 200: 196: 192: 188: 184: 180: 176: 172: 168: 165: 160: 156: 151: 147: 143: 137: 133: 129: 121: 117: 113: 111: 104: 99: 93: 89: 87: 83: 80: 76: 73: 69: 66: 63: 59: 55: 48: 43: 37: 33: 19: 15995: 15985: 15972: 15900:SpaceHab LSM 15889: 15876:Fengyun 2-05 15755: 15746:Chinasat-22A 15728: 15606: 15589: 15577: 15424: 15417: 15346:New Horizons 15260: 15249: 15236: 15226: 15135:Lunar Lander 15053:and proposed 15038: 14825: 14817: 14809: 14801: 14793: 14785: 14777: 14771: 14763: 14755: 14606: 14598: 14590: 14582: 14574: 14532: 14455: 14447: 14439: 14430: 14411: 14388:Mars Express 14350: 14228:Predecessors 14207:Horizon 2000 13788: 13771: 13615:Hibernating 13367:(2016–2019?) 13051: 12910:(1962, 1964) 12804:Nano-JASMINE 12628:NEO Surveyor 12552:(since 2006) 12544:(since 2020) 12536:(since 1995) 12528:(since 2019) 12520:(since 2017) 12512:(since 2008) 12504:(since 2015) 12496:(since 2015) 12488:(since 2011) 12480:(since 1997) 12459:(since 1999) 12451:(since 2024) 12443:(since 2023) 12435:(since 2022) 12427:(since 2012) 12419:(since 2017) 12411:(since 2018) 12403:(since 2009) 12395:(since 2017) 12387:(since 2004) 12379:(since 2024) 12371:(since 2019) 12363:(since 2021) 12355:(since 2020) 12347:(since 2008) 12339:(since 2002) 12331:(since 2017) 12323:(since 2024) 12315:(since 2015) 12307:(since 1999) 12299:(since 2015) 12274:(since 2004) 12266:(since 2006) 12258:(since 2020) 12250:(since 2008) 12242:(since 1995) 12234:(since 2010) 12226:(since 2013) 12218:(since 2006) 12210:(since 2021) 12202:(since 2015) 12194:(since 2022) 12186:(since 2023) 12165:(since 2018) 12157:(since 2004) 12149:(since 2008) 12141:(since 1995) 12133:(since 2010) 12125:(since 2001) 12117:(since 2013) 12109:(since 2006) 12101:(since 1990) 12093:(since 2005) 12085:(since 2013) 12077:(since 2021) 12069:(since 2023) 12061:(since 2015) 12053:(since 2019) 12045:(since 2021) 12037:(since 2013) 12028:(since 2015) 12020:(since 2018) 11999:(since 2009) 11991:(since 2008) 11983:(since 2001) 11975:(since 2022) 11954:(since 2024) 11946:(since 1994) 11938:(since 2018) 11930:(since 2006) 11922:(since 2020) 11914:(since 2018) 11844: 11831: 11759: 11747: 11659: 11630: 11604: 11557: 11544: 11474:XO Telescope 11424:Project 1640 11253:Ground-based 11113: 11109: 11103: 11093:10 September 11091:. 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Retrieved 4875: 4787: 4783: 4775: 4762: 4757: 4753: 4751: 4456:eccentricity 4330: 4258:84.1 (± 0.1) 4136:83.2 (± 2.3) 4130:1.46 (± 0.3) 4124:1.46 (± 0.3) 4026: 4024: 3767:18 42 31.120 2553:19 28 13.265 2401:eccentricity 2275: 2274: 2271: 2260: 2159: 2156:Main results 2151: 2108: 2057: 2050: 2035: 2016: 2001:hot Jupiters 1998: 1984: 1979: 1975: 1967: 1963: 1959: 1955: 1951: 1947: 1944: 1917: 1899: 1888: 1882: 1878: 1872: 1849: 1831: 1814: 1803: 1771: 1759: 1753: 1741: 1734: 1723: 1709: 1698: 1691: 1657: 1650: 1643: 1632: 1627: 1623: 1616: 1609: 1602: 1594: 1587: 1568: 1558: 1526:helium flash 1513: 1498: 1487:Granulation: 1486: 1474:modeling of 1470: 1463: 1437: 1419: 1401: 1394:white dwarfs 1388: 1382: 1370: 1360: 1351: 1348:seismo field 1347: 1335:light curves 1326: 1323:seismo field 1322: 1320: 1295: 1246: 1231: 1217: 1194: 1181:spectroscopy 1153:CFHT/Megacam 1137: 1112: 1099:Solar System 1096: 1083: 1058:person-years 1056:and took 60 1050: 1033:€170 million 1030: 1019: 1007: 987: 981: 975: 965: 959: 953: 947: 937: 931: 925: 919: 913: 907: 901: 895: 889: 883: 877: 871: 865: 859: 853: 847: 841: 835: 829: 787: 779:occultations 776: 763: 755: 718: 699: 672:by aluminum 640: 595: 588: 555: 551: 547: 540: 536: 532: 526: 525: 499:Focal length 426:Mean anomaly 356:Eccentricity 178:Payload mass 158:Manufacturer 77: / 61:Mission type 36: 15968:Kosmos 2426 15964:Kosmos 2425 15960:Kosmos 2424 15757:Soyuz TMA-9 15751:Kosmos 2423 15703:Syracuse 3B 15668:Mea Huaka'i 15602:Kosmos 2422 15557:Kosmos 2421 15493:Kosmos 2420 15426:Soyuz TMA-8 15419:FalconSAT-2 15408:Hot Bird 7A 15273:WikiProject 15145:MarcoPolo-R 15095:Don Quijote 15065:Ariane 5 ME 15029:(2015–2017) 14959:Galileo FOC 14953:Galileo IOV 14925:(1989–1993) 14864:Jules Verne 14845:spaceflight 14676:(2009–2013) 14664:(2003–2007) 14662:Double Star 14658:(2002–2012) 14646:(1995–2011) 14640:(1991–2000) 14634:(1977–1997) 14547:(2009–2013) 14541:(2009–2013) 14517:(1995–1998) 14499:(1989–1993) 14493:(1983–1986) 14487:(1978–1996) 14481:(1975–1982) 14419:BepiColombo 14406:(2005–2014) 14400:(2004–2016) 14384:(2003–2006) 14378:(1997–2005) 14372:(1985–1992) 14341:(2000–2024) 14329:(1990–2009) 14323:(1977–1987) 14256:Arianespace 13728:(2014–2015) 13680:(2012–2013) 13646:Lost/Failed 13637:(1998–2010) 13629:(1998–2005) 13606:(1991–2001) 13598:(2001–2010) 13582:(1970–1973) 13574:(1983–1985) 13566:(1975–1980) 13558:(2005–2015) 13550:(2003–2020) 13542:(2011–2019) 13534:(1979–1985) 13526:(1975–1979) 13518:(1972–1973) 13510:(1992–2004) 13502:(1995–2012) 13494:(1990–1999) 13486:(2002–2018) 13478:(1983–1984) 13470:(2009–2013) 13454:(2006–2016) 13383:(1972–1981) 13375:(1968–1973) 13359:(1996–1997) 13351:(2003–2019) 13343:(2015–2017) 13335:(2015–2017) 13327:(1997–2002) 13319:(1990–2001) 13311:(2009–2018) 13303:(1996–2004) 13295:(1978–1996) 13287:(1996–1998) 13279:(1995–1996) 13255:(1989–1993) 13247:(2000–2008) 13239:(1979–1981) 13231:(1978–1982) 13223:(2013–2023) 13215:(1981–1991) 13207:(2009–2013) 13199:(1977–1979) 13191:(1997–2005) 13183:(1979–1985) 13175:(1989–1998) 13167:(1987–1991) 13159:(1990–1992) 13151:(2003–2013) 13143:(1987–2001) 13135:(1999–2007) 13127:(1992–2001) 13119:(1983–1986) 13108:Explorer 11 13079:(2017–2019) 13071:(1989–1993) 13063:(1975–1982) 13055:(2006–2013) 13047:(1991–2000) 13039:(2003–2008) 13031:(1996–2003) 13023:(1974–1976) 13015:(1983–1991) 12974:(1993–2000) 12966:(1973–1974) 12958:(2017–2019) 12950:(1979–1982) 12942:(1974–1980) 12934:(1971–1972) 12926:(1967–1969) 12902:(1962–1972) 12894:(1993–2005) 12886:(2006–2011) 12878:(2007–2024) 12175:Ultraviolet 11681:(mid-2020s) 11589:(2017–2020) 11572:(2009–2018) 11564:(2008–2013) 11559:Deep Impact 11548:(2006–2013) 11526:(2003–2019) 10237:(41): A41. 9209:www.cnes.fr 9191:sci.esa.int 8998:26 November 7850:(2): L165. 7711:: 251–257. 7513:(2): L182. 7476:2268/107456 6434:2268/117827 5830:10036/87276 5611:27 February 5219:Nature News 4789:formation. 4701:brown dwarf 4680:06 51 29.01 4639:brown dwarf 4618:18 38 33.91 4577:brown dwarf 4556:06 28 27.82 4461:Inclination 4355:Declination 4279:18 31 00.24 4222:19 17 15.43 4157:06 40 46.84 4100:06 19 16.97 4043:18 30 24.28 3982:18 35 36.50 3953:0.484±0.087 3878:18 33 59.00 2723:18 44 17.42 2406:Inclination 2301:Declination 2187:lightcurve. 2177:brown dwarf 2084:brown dwarf 1896:particular. 1883:CoRoT Sol 1 1810:granulation 1729:κ mechanism 1678:12 Lacertae 1646:κ mechanism 1481:metallicity 1442:κ mechanism 1223:Discoveries 1047:Development 1026:polar orbit 994:V-magnitude 814:giant stars 810:dwarf stars 606:first light 546:; English: 507:Wavelengths 456:Revolution 436:Mean motion 386:Inclination 296:Deactivated 265:Arianespace 248:Launch site 215:Launch date 197:≈380 W 170:Launch mass 16002:Categories 15955:Meridian 1 15950:SAR-Lupe 1 15881:WildBlue 1 15819:Shijian 6D 15815:Shijian 6C 15792:DirecTV-9S 15708:Koreasat 5 15694:Hot Bird 8 15660:AeroCube-1 15388:Arabsat-4A 15367:EchoStar X 15160:Phootprint 15140:Marco Polo 14981:Technology 14811:MetOp-SG-B 14803:MetOp-SG-A 14779:Sentinel-4 14750:ADM-Aeolus 14730:Sentinel-3 14712:Sentinel-2 14698:Sentinel-1 14626:Copernicus 14521:XMM-Newton 14339:Cluster II 14145:Copernicus 14116:Programmes 14044:Facilities 13994:Spaceports 13587:Vanguard 3 12899:Alouette 1 12739:AstroSat-2 12456:XMM-Newton 11972:James Webb 11078:"CoRoT-33" 11047:1508.05763 10890:2207.08742 10800:1504.01532 10741:1704.00373 10676:1602.00506 9869:2268/76653 8943:(2): 185. 8164:2066/60145 7273:(3): L21. 6857:(1): L13. 6223:2268/76337 6000:1904.10793 5561:16 October 5260:6 February 5197:30 October 5111:6 February 4867:References 4494:06 43 49.0 4439:Semi-major 3932:18 34 45.0 3899:10.39±0.55 3821:18 39 00.0 2779:06 43 49.0 2666:06 45m 07s 2384:Semi-major 2261:transiting 1929:Exoplanets 1801:in Spain. 1676:, and for 1666:θ Ophiuchi 1577:Histograms 1522:degenerate 1438:SPB stars: 1201:wavelength 1022:Soyuz 2-1b 1014:luminosity 696:programme. 610:spacecraft 602:Soyuz 2.1b 550:nvection, 539:tation et 535:nvection, 329:Geocentric 261:Contractor 238:Soyuz 2.1b 186:Dimensions 15908:ANDE-FACL 15829:Sinosat-2 15724:Shijian 8 15717:September 15678:Arirang-2 15672:ICECube-2 15632:ICECube-1 15612:Baumanets 15597:Genesis I 15534:Galaxy 16 15508:Thaicom 5 15453:Astra 1KR 15201:CryoSat-1 15175:STE-QUEST 15110:Eddington 15100:e.Deorbit 15051:Cancelled 14923:Olympus-1 14765:EarthCARE 14686:CryoSat-2 14535:(2006–13) 14511:(1992–93) 14497:Hipparcos 14471:cosmology 13790:Eddington 13745:Cancelled 13252:Hipparcos 12660:Spektr-UV 12525:Mini-EUSO 12517:ISS-CREAM 12368:Spektr-RG 12288:Gamma-ray 12183:Aditya-L1 12074:Hayabusa2 11951:Queqiao 2 11895:Operating 11761:Eddington 11741:Cancelled 11632:Hayabusa2 11459:SuperWASP 11449:SPECULOOS 11419:PlanetPol 11382:Australis 11244:Exoplanet 11158:119188767 11136:CiteSeerX 11123:1306.0578 11064:0004-6361 10994:1010.0179 10909:0035-8711 10827:0004-6361 10768:0004-6361 10701:0004-6361 10619:1401.1122 10565:1401.1122 10510:1112.0584 10436:118339296 10411:1109.3203 10355:1112.1035 10299:1107.2032 10244:1106.4393 10197:0909.3397 10141:1101.1899 10110:119188073 10085:1007.5481 10029:1007.2497 9998:119184639 9973:1009.2597 9942:119223546 9917:1006.2949 9796:1008.0325 9740:0908.0241 9685:1001.1426 9629:0909.3397 9598:115916135 9573:0807.3767 9517:0810.0919 9461:0803.3207 9405:0803.3202 9349:1008.3028 9294:1106.0586 9239:0907.1653 9173:118522323 9148:1011.2690 8975:119266738 8950:1110.2133 8866:0910.3513 8809:0909.1546 8752:1302.0167 8723:1004.1525 8703:119183535 8676:1301.1856 8619:1005.4384 8589:119260690 8564:1101.2372 8557:(1): 20. 8511:1301.0991 8481:119212957 8456:1302.3369 8401:1010.4959 8346:0905.1592 8205:1208.4250 8030:1109.0705 7973:0903.5477 7914:0801.2451 7752:: 35–40. 7657:0706.3274 7573:1210.4257 7520:1009.1754 7451:1103.5805 7419:119248533 7394:1105.6113 7337:1211.0146 7280:0908.0210 7131:1004.0449 7076:0906.5002 7021:0905.2695 6966:0910.4037 6919:0910.4027 6864:0910.3060 6809:1009.1024 6754:1202.2692 6724:189820974 6702:: 21–22. 6656:1203.5231 6599:0802.2057 6546:1003.4368 6272:1006.3139 6198:0906.3788 6076:0812.1267 6027:129946089 5908:1110.2384 5861:1110.2384 5753:1101.0463 5746:: 02001. 5698:0907.2653 5643:0908.1172 5415:1105.1887 5408:: 01001. 5320:118466787 5295:0901.2206 5236:124190084 4675:Monoceros 4551:Monoceros 4489:Monoceros 4473:Discovery 4350:ascension 4274:Ophiuchus 4152:Monoceros 4095:Monoceros 4038:Ophiuchus 3977:Ophiuchus 3927:Ophiuchus 3911:<0.065 3902:1.01±0.04 3816:Ophiuchus 3762:Ophiuchus 3681:Monoceros 3593:< 0.15 3515:Monoceros 3458:Monoceros 3401:Monoceros 3376:1.9000693 3344:Monoceros 3173:Monoceros 3116:Monoceros 3059:Monoceros 2774:Monoceros 2718:Ophiuchus 2661:Monoceros 2605:Monoceros 2523:1.7429964 2466:1.5089557 2434:Monoceros 2418:Discovery 2296:ascension 2230:HD80606 b 2147:CoRoT-24c 2143:CoRoT-24b 2139:CoRoT-23b 2135:CoRoT-22b 2131:CoRoT-21b 2127:CoRoT-20b 2123:CoRoT-19b 2119:CoRoT-18b 2115:CoRoT-17b 2111:CoRoT-16b 2104:HD46375 b 2088:CoRoT-15b 2080:CoRoT-14b 2076:CoRoT-13b 2072:CoRoT-12b 2068:CoRoT-11b 2064:CoRoT-10b 1873:HD 174884 1858:ephemeris 1842:γ Doradus 1766:Monoceros 1742:HD 46149: 1692:Be stars: 1682:ν Eridani 1573:gravities 1530:red clump 1514:RGB stars 1502:red giant 1424:sub-giant 1352:exo field 1339:star spot 1327:exo field 1167:, namely 1080:Potential 800:, in the 798:Monoceros 725:CCD. The 700:The four 674:shielding 670:radiation 662:focal box 658:objective 529:(French: 360:0.0203702 307: UTC 92:2006-063A 86:COSPAR ID 15936:TacSat-2 15926:MEASAT-3 15904:ANDE-MAA 15869:December 15843:November 15796:Optus D1 15735:ITS P3/4 15699:JCSAT-3A 15648:HAUSAT-1 15628:Rincon 1 15591:INSAT-4C 15529:KazSat-1 15504:Satmex 6 15500:/ EWS-G1 15477:CloudSat 15468:Yaogan 1 15443:JCSAT-5A 15404:Spainsat 15360:February 15262:Wikinews 15238:Category 14858:Columbus 14782:) (2024) 14592:ARRAKIHS 14545:Herschel 14527:INTEGRAL 14457:EnVision 14410:ExoMars 14266:EUMETSAT 14157:Columbus 14150:Sentinel 14030:Ariane 6 14025:Ariane 5 13841:Sentinel 13539:Spektr-R 13475:RELIKT-1 13316:Kristall 13204:Herschel 13028:BeppoSAX 12784:JEM-EUSO 12779:iWF-MAXI 12721:Proposed 12684:LiteBIRD 12676:Spektr-M 12408:MinXSS-2 12336:INTEGRAL 12199:Astrosat 12025:Astrosat 11964:Infrared 11833:Category 11690:Proposed 11464:Systemic 11372:MicroFUN 11352:Magellan 11290:ESPRESSO 11019:54794954 10734:: A107. 10709:55412970 10644:46747735 10612:: A140. 10590:46747735 10558:: A140. 10535:55219945 10404:: A145. 10380:42622538 10348:: A136. 10324:59380182 10292:: A130. 10269:54618864 10190:: A149. 10166:56139010 10078:: A110. 10054:67815327 9878:20237564 9821:56357511 9710:54014374 9654:13117298 9486:14288300 9430:16507802 9374:59064890 9319:55994657 9264:18678539 9141:: L153. 9116:Archived 9074:BBC News 9042:2 August 9020:2 August 8925:588, 117 8891:55225546 8836:53314768 8777:53386835 8644:55225320 8536:56223156 8504:: A121. 8426:30687338 8394:: A101. 8371:17572695 8232:49485253 8173:54967603 8114:18221601 8055:53550571 8000:53526744 7941:16027828 7882:27867445 7829:11807580 7774:Archived 7684:18255593 7598:53687206 7545:56134436 7484:21455175 7364:55522551 7305:16706004 7156:27138238 7101:16920418 6991:54511502 6889:56458774 6834:54850954 6779:55844243 6681:55834143 6443:20220844 6231:19541991 6155:19458716 6109:14181048 6101:18948534 5933:23202373 5901:: A112. 5778:54062564 5723:14949658 5668:44068547 5590:3 August 5525:2 August 5494:15577360 5385:10 April 5171:2 August 5138:2 August 5085:2 August 5052:3 August 5021:2 August 4990:2 August 4960:3 August 4793:See also 4669:CoRoT-34 4648:5.819143 4607:CoRoT-33 4545:CoRoT-15 4379:Spectral 4367:Distance 4269:CoRoT-36 4212:CoRoT-35 4147:CoRoT-32 4090:CoRoT-31 4033:CoRoT-30 4015:<0.12 3973:CoRoT-29 3923:CoRoT-28 3868:CoRoT-27 3812:CoRoT-26 3757:CoRoT-25 3705:< 0.1 3686:06 47 41 3676:CoRoT-24 3629:18 39 08 3619:CoRoT-23 3605:< 0.6 3572:18 42 40 3562:CoRoT-22 3510:CoRoT-21 3463:06 30 53 3453:CoRoT-20 3406:06 28 08 3396:CoRoT-19 3382:<0.08 3349:06 32 41 3339:CoRoT-18 3319:3.768125 3292:18 34 47 3282:CoRoT-17 3235:18 34 06 3225:CoRoT-16 3178:06 53 42 3168:CoRoT-14 3121:06 50 53 3111:CoRoT-13 3091:2.828042 3064:06 43 04 3054:CoRoT-12 3007:18 42 45 2997:CoRoT-11 2950:19 24 15 2940:CoRoT-10 2929:>89.9 2893:18 43 09 2836:19 26 21 2806:0.853585 2755:< 0.1 2610:06 48 47 2496:19 27 07 2439:06 48 19 2325:Spectral 2313:Distance 2205:Catalano 2181:CoRoT-3b 2166:CoRoT-1b 2092:CoRoT-8b 2082:, and a 2060:CoRoT-8b 2053:CoRoT-9b 2046:CoRoT-6b 2042:CoRoT-7c 2038:CoRoT-7b 2031:CoRoT-3b 2027:CoRoT-5b 2023:CoRoT-4b 2008:CoRoT-2b 2004:CoRoT-1b 1978:, M and 1821:AA Tauri 1756:NGC 2264 1699:O stars: 1662:β Cephei 1633:a priori 1451:HD 43317 1447:HD 50230 1430:of 1.3 M 1428:HD 49385 1406:HD 49933 1288:l=4, m=2 1278:l=2, m=1 1268:l=2, m=0 1258:l=1, m=0 1209:CoRoT-9b 1205:CoRoT-7b 1141:periodic 1122:and one 970:CoRoT-7b 942:CoRoT-9b 818:transits 806:database 766:May 2016 686:spectrum 655:dioptric 632:Overview 626:CoRoT-1b 591:CoRoT-7b 491:Diameter 288:Disposal 252:Baikonur 71:Operator 15940:GeneSat 15931:USA-193 15920:MEPSI-2 15916:MARScom 15891:STS-116 15860:USA-192 15850:USA-191 15805:MetOp-A 15785:October 15776:USA-190 15767:HIT-SAT 15730:STS-115 15579:STS-121 15562:USA-184 15547:USA-189 15543:USA-188 15539:USA-187 15498:GOES 13 15473:CALIPSO 15372:MTSAT-2 15339:January 15250:Commons 15227:italics 15196:Cluster 15180:THESEUS 15165:SOLARIS 15040:PROBA-3 15033:OPS-SAT 15015:PROBA-V 15009:PROBA-2 14997:PROBA-1 14947:HYLAS-1 14941:GIOVE-B 14935:GIOVE-A 14929:Artemis 14757:Biomass 14656:Envisat 14595:(2030s) 14394:Rosetta 14382:SMART-1 14376:Huygens 14327:Ulysses 14307:Science 14182:ExoMars 14172:GALILEO 14162:CryoSat 14123:Artemis 14102:ESTRACK 14007:Esrange 13890:Related 13801:FINESSE 13779:Destiny 13762:Astro-G 13725:Tsubame 13717:Astro-E 13693:ABRIXAS 13547:Spitzer 13531:Solwind 13483:R/HESSI 13443:Orion 2 13435:Orion 1 13140:Kvant-1 13036:CHIPSat 12999:Astro-2 12979:Astro-1 12955:ASTERIA 12947:Ariel 6 12939:Ariel 5 12931:Ariel 4 12923:Ariel 3 12915:Ariel 2 12907:Ariel 1 12868:Retired 12859:THESEUS 12844:Solar-D 12839:PhoENiX 12679:(2030+) 12636:JASMINE 12604:Xuntian 12572:SPHEREx 12565:Planned 12114:NEOSSat 12009:Optical 11935:Queqiao 11845:Commons 11812:nearest 11785:Related 11653:Planned 11598:Current 11586:ASTERIA 11377:MINERVA 11362:MASCARA 11357:MARVELS 11310:HARPS-N 11275:EAPSNet 11270:CORALIE 11128:Bibcode 11040:: A13. 10999:Bibcode 10987:: A68. 10943:Bibcode 10805:Bibcode 10793:: A36. 10746:Bibcode 10681:Bibcode 10669:: A62. 10624:Bibcode 10570:Bibcode 10515:Bibcode 10503:: A54. 10466:Bibcode 10416:Bibcode 10360:Bibcode 10304:Bibcode 10249:Bibcode 10202:Bibcode 10146:Bibcode 10134:: A97. 10090:Bibcode 10034:Bibcode 10022:: A97. 9978:Bibcode 9966:: A55. 9922:Bibcode 9910:: A65. 9886:4307611 9848:Bibcode 9801:Bibcode 9789:: A66. 9765:5682749 9745:Bibcode 9690:Bibcode 9678:: A14. 9634:Bibcode 9578:Bibcode 9542:8944836 9522:Bibcode 9466:Bibcode 9410:Bibcode 9354:Bibcode 9342:: L59. 9299:Bibcode 9287:: A79. 9244:Bibcode 9153:Bibcode 9079:15 June 8955:Bibcode 8871:Bibcode 8814:Bibcode 8757:Bibcode 8745:: A60. 8681:Bibcode 8624:Bibcode 8569:Bibcode 8516:Bibcode 8461:Bibcode 8449:: A68. 8406:Bibcode 8351:Bibcode 8302:Bibcode 8261:Bibcode 8259:: A90. 8210:Bibcode 8141:Bibcode 8092:Bibcode 8035:Bibcode 8023:: A98. 7978:Bibcode 7919:Bibcode 7862:Bibcode 7809:Bibcode 7713:Bibcode 7662:Bibcode 7621:Bibcode 7619:: 220. 7578:Bibcode 7566:: A82. 7525:Bibcode 7492:4338871 7456:Bibcode 7399:Bibcode 7387:: A86. 7342:Bibcode 7285:Bibcode 7250:5310696 7230:Bibcode 7191:Bibcode 7136:Bibcode 7124:: A22. 7081:Bibcode 7026:Bibcode 6971:Bibcode 6959:: A16. 6924:Bibcode 6912:: A15. 6869:Bibcode 6814:Bibcode 6759:Bibcode 6704:Bibcode 6661:Bibcode 6649:: A55. 6604:Bibcode 6551:Bibcode 6539:: A87. 6500:Bibcode 6451:9172411 6413:Bibcode 6369:Bibcode 6326:Bibcode 6297:2827129 6277:Bibcode 6265:: A38. 6239:6950829 6203:Bibcode 6185:Science 6163:4394571 6135:Bibcode 6081:Bibcode 6063:Science 5962:Bibcode 5960:: A14. 5913:Bibcode 5866:Bibcode 5807:Bibcode 5758:Bibcode 5703:Bibcode 5648:Bibcode 5474:Bibcode 5420:Bibcode 5300:Bibcode 4930:16 June 4887:10 July 4713:0.03874 4710:2.11853 4613:Serpens 4484:CoRoT-7 4454:Orbital 4424:Orbital 4385:Object 3945:G8/9IV 3873:Serpens 3624:Serpens 3567:Serpens 3542:2.72474 3433:3.89713 3205:1.51215 3148:4.03519 3094:0.04016 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3077:G2V 3046:2010 3031:1.43 3028:2.33 3020:F6V 2989:2010 2983:0.53 2974:0.97 2971:2.75 2963:K1V 2932:2010 2926:0.11 2917:1.05 2914:0.84 2906:G3V 2900:13.7 2875:2010 2872:88.4 2860:0.57 2857:0.22 2849:K1V 2843:14.8 2818:2009 2815:80.1 2792:G9V 2761:2009 2749:8.89 2746:1.16 2735:F5V 2730:13.9 2705:2008 2699:0.09 2690:1.28 2679:F9V 2648:2008 2633:1.19 2630:0.72 2622:F0V 2617:13.7 2592:2008 2589:85.9 2577:1.01 2566:F3V 2560:13.3 2535:2007 2517:3.31 2509:G7V 2478:2007 2475:85.1 2463:1.49 2460:1.03 2452:G0V 2446:13.6 2423:Ref 2386:axis 2337:Mass 2327:type 2308:mag. 2306:App. 2284:Star 2098:and 2025:and 2006:and 1972:star 1781:and 1775:MOST 1614:GAIA 1612:and 1207:and 1175:and 1161:mass 1037:CNES 622:TESS 620:and 481:Type 406:RAAN 161:CNES 75:CNES 15624:ION 15486:May 15021:IXV 14991:ARD 14843:ISS 14515:ISO 14485:IUE 14140:ATV 14128:ESM 13871:TPF 13816:IXO 13811:HOP 13356:MSX 13292:IUE 13284:ISO 13084:DXS 13020:ANS 13003:HUT 12992:HUT 12963:ATM 12829:OST 12764:HWO 12477:ACE 12231:SDO 12130:SDO 12017:Aoi 11727:OST 11536:HST 11394:N2K 11389:MOA 11327:HEK 11317:GPI 11265:APF 11146:doi 11114:226 11052:doi 11038:584 11007:doi 10985:525 10951:doi 10939:506 10895:doi 10881:516 10813:doi 10791:579 10754:doi 10732:602 10689:doi 10667:589 10632:doi 10610:562 10578:doi 10556:562 10523:doi 10501:537 10474:doi 10462:545 10424:doi 10402:538 10368:doi 10346:537 10312:doi 10290:533 10257:doi 10235:531 10210:doi 10188:541 10154:doi 10132:528 10098:doi 10076:522 10042:doi 10020:520 9986:doi 9964:524 9930:doi 9908:520 9864:hdl 9856:doi 9844:464 9809:doi 9787:520 9753:doi 9731:506 9698:doi 9676:512 9642:doi 9620:506 9586:doi 9564:488 9530:doi 9508:491 9474:doi 9452:482 9418:doi 9396:482 9362:doi 9340:521 9307:doi 9285:532 9252:doi 9230:506 9161:doi 9139:518 8963:doi 8941:746 8879:doi 8857:508 8822:doi 8800:401 8765:doi 8743:552 8689:doi 8667:430 8632:doi 8610:519 8577:doi 8555:729 8524:doi 8502:550 8469:doi 8447:552 8414:doi 8392:525 8359:doi 8337:502 8310:doi 8298:506 8269:doi 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