1042:
larger than approximately 1.6 Earth-radius (more massive than approximately 6 Earth-masses) contain significant fractions of volatiles or H/He gas (such planets appear to have a diversity of compositions that is not well-explained by a single mass-radius relation as that found in rocky planets). After measuring 65 super-Earths smaller than 4 Earth-radii, the empirical data points out that Gas
Dwarves would be the most usual composition: there is a trend where planets with radii up to 1.5 Earth-radii increase in density with increasing radius, but above 1.5 radii the average planet density rapidly decreases with increasing radius, indicating that these planets have a large fraction of volatiles by volume overlying a rocky core. Another discovery about exoplanets' composition is that about the
1022:
planets with a core mass of more than 1.5 Earth-mass (1.15 Earth-radius max.), most likely cannot get rid of their nebula captured hydrogen envelopes during their whole lifetime. Other calculations point out that the limit between envelope-free rocky super-Earths and sub-Neptunes is around 1.75 Earth-radii, as 2 Earth-radii would be the upper limit to be rocky (a planet with 2 Earth-radii and 5 Earth-masses with a mean Earth-like core composition would imply that 1/200 of its mass would be in a H/He envelope, with an atmospheric pressure near to 2.0 GPa or 20,000 bar). Whether or not the primitive nebula-captured H/He envelope of a super-Earth is entirely lost after formation also depends on the orbital distance. For example, formation and evolution calculations of the
94:
508:
272:
449:) orbiting within the Gliese 581 planetary system. The planet has a minimum mass 3.1 times that of Earth and a nearly circular orbit at 0.146 AU with a period of 36.6 days, placing it in the middle of the habitable zone where liquid water could exist and midway between the planets c and d. It was discovered using the radial velocity method by scientists at the University of California at Santa Cruz and the Carnegie Institution of Washington. However, the existence of Gliese 581 g has been questioned by another team of astronomers, and it is currently listed as unconfirmed at
146:
31:
163:
6128:
976:
6152:
4767:
6104:
1102:(after migrating towards the proximity of their parent star). The amount of the outermost layers that is lost depends on the size and the material of the planet and the distance from the star. In a typical system, a gas giant orbiting 0.02 AU around its parent star loses 5–7% of its mass during its lifetime, but orbiting closer than 0.015 AU can mean evaporation of the whole planet except for its core.
6140:
6116:
4888:
632:, one of three stars located a relatively close 22 light years from Earth in the constellation of Scorpio, it said. The planets orbit Gliese 667C in the so-called Goldilocks Zone — a distance from the star at which the temperature is just right for water to exist in liquid form rather than being stripped away by stellar radiation or locked permanently in ice.
407:, is 2.7 times as large as Earth and orbits a star much smaller and less luminous than the Sun. "This planet probably does have liquid water," said David Charbonneau, a Harvard professor of astronomy and lead author of an article on the discovery. However, interior models of this planet suggest that under most conditions it does not have liquid water.
372:, with a mass estimated at 4.8 Earth masses and an orbital period of only 0.853 days, was announced on 3 February 2009. The density estimate obtained for COROT-7b points to a composition including rocky silicate minerals similar to that of the Solar System's four inner planets, a new and significant discovery. COROT-7b, discovered right after
116:, which is the Solar System's giant planet with the least mass), the lower bound varies from 1 or 1.9 to 5, with various other definitions appearing in the popular media. The term "super-Earth" is also used by astronomers to refer to planets bigger than Earth-like planets (from 0.8 to 1.2 Earth-radius), but smaller than
1073:
due to thinner plates under more stress. In fact, their models suggested that Earth was itself a "borderline" case, just barely large enough to sustain plate tectonics. These findings were corroborated by van Heck et al., who determined that plate tectonics may be more likely on super-Earths than on
1138:
that keep the Earth warmer. Venus has a black-body temperature of only 184.2 K (−89 °C or −128 °F ) even though Venus has a true temperature of 737 K (464 °C or 867 °F ). Though the atmosphere of Venus traps more heat than Earth's, NASA lists the black-body temperature of Venus
1105:
The low densities inferred from observations imply that a fraction of the super-Earth population has substantial H/He envelopes, which may have been even more massive soon after formation. Therefore, contrary to the terrestrial planets of the solar system, these super-Earths must have formed during
1090:
New research suggests that the rocky centres of super-Earths are unlikely to evolve into terrestrial rocky planets like the inner planets of the Solar System because they appear to hold on to their large atmospheres. Rather than evolving into a planet composed mainly of rock with a thin atmosphere,
395:
of 1.9 Earth masses was announced on 21 April 2009. It was at the time the smallest extrasolar planet discovered around a normal star and the closest in mass to Earth. Being at an orbital distance of just 0.03 AU and orbiting its star in just 3.15 days, it is not in the habitable zone, and may have
124:
personnel. Some authors further suggest that the term Super-Earth might be limited to rocky planets without a significant atmosphere, or planets that have not just atmospheres but also solid surfaces or oceans with a sharp boundary between liquid and atmosphere, which the four giant planets in the
996:
or sub-Neptune). A super-Earth of high density is believed to be rocky and/or metallic, like Earth and the other terrestrial planets of the Solar System. A super-Earth's interior could be undifferentiated, partially differentiated, or completely differentiated into layers of different composition.
503:
On 5 December 2011, the Kepler team announced that they had discovered 2,326 planetary candidates, of which 207 are similar in size to Earth, 680 are super-Earth-size, 1,181 are
Neptune-size, 203 are Jupiter-size and 55 are larger than Jupiter. Compared to the February 2011 figures, the number of
1041:
If a super-Earth is detectable by both the radial-velocity and the transit methods, then both its mass and its radius can be determined; thus its average bulk density can be calculated. The actual empirical observations are giving similar results as theoretical models, as it's found that planets
1009:
of detecting planets and the mass of the relevant planet what the structural composition is. For Gliese 876 d, calculations range from 9,200 km (1.4 Earth radii) for a rocky planet and very large iron core to 12,500 km (2.0 Earth radii) for a watery and icy planet. Within this range of
1159:
Earth's magnetic field results from its flowing liquid metallic core, but in super-Earths the mass can produce high pressures with large viscosities and high melting temperatures, which could prevent the interiors from separating into different layers and so result in undifferentiated coreless
1021:
The limit between rocky planets and planets with a thick gaseous envelope is calculated with theoretical models. Calculating the effect of the active XUV saturation phase of G-type stars over the loss of the primitive nebula-captured hydrogen envelopes in extrasolar planets, it's obtained that
627:
On 25 June 2013, three "super Earth" planets have been found orbiting a nearby star at a distance where life in theory could exist, according to a record-breaking tally announced on
Tuesday by the European Southern Observatory. They are part of a cluster of as many as seven planets that circle
1037:
respectively (which are within measurement errors), are extremely vulnerable to envelope loss. In particular, the complete removal of the primordial H/He envelope by energetic stellar photons appears almost inevitable in the case of Kepler-11b, regardless of its formation hypothesis.
983:
Due to the larger mass of super-Earths, their physical characteristics may differ from Earth's; theoretical models for super-Earths provide four possible main compositions according to their density: low-density super-Earths are inferred to be composed mainly of hydrogen and helium
504:
Earth-size and super-Earth-size planets increased by 200% and 140% respectively. Moreover, 48 planet candidates were found in the habitable zones of surveyed stars, marking a decrease from the
February figure; this was due to the more stringent criteria in use in the December data.
438:, one of which, although not yet confirmed, has an estimated minimum mass of 1.35 ± 0.23 times that of Earth, which would be the lowest mass of any exoplanet found to date orbiting a main-sequence star. Although unconfirmed, there is a 98.6% probability that this planet does exist.
1160:
mantles. Magnesium oxide, which is rocky on Earth, can be a liquid metal at the pressures and temperatures found in super-Earths and could generate a magnetic field in the mantles of super-Earths. That said, super-Earth magnetic fields are yet to be detected observationally.
477:
estimates "within a thousand light-years of Earth" there are "at least 30,000 of these habitable worlds." Also based on the findings, the Kepler Team has estimated "at least 50 billion planets in the Milky Way" of which "at least 500 million" are in the habitable zone.
434:. The only confirmed radial velocity planet smaller than this planet is Gliese 581e at 1.9 Earth masses (see above). On 24 August, astronomers using ESO's HARPS instrument announced the discovery of a planetary system with up to seven planets orbiting a Sun-like star,
279:
O" for those made of water. Those between the two lines, and closer to the Fe line, are most likely solid rocky planets, while those near or above the water line are more likely gas and/or liquid. Planets in the Solar System are on the chart, labeled with their
1061:, show that the magnesium-silicate internal regions of the planet would undergo phase changes under the immense pressures and temperatures of a super-Earth planet, and that the different phases of this liquid magnesium silicate would separate into layers.
473:." Six candidates in this zone were less than twice the size of the Earth A more recent study found that one of these candidates (KOI 326.01) is in fact much larger and hotter than first reported. Based on the latest Kepler findings, astronomer
1182:. The higher surface gravity would lead to a thicker atmosphere, increased surface erosion and hence a flatter topography. The result could be an "archipelago planet" of shallow oceans dotted with island chains ideally suited for
216:(two Jupiter-sized gas giants had previously been discovered in that system). It has an estimated mass of 7.5 Earth masses and a very short orbital period of about 2 days. Due to the proximity of Gliese 876 d to its host star (a
651:, it is currently the largest known planet likely to have a predominantly rocky composition. At 17 Earth masses, it is well above the 10 Earth mass upper limit that is commonly used for the term 'super-Earth' so the term
2893:
256:(6.8 million mi, 11 million km), it is on the "warm" edge of the habitable zone around Gliese 581 with an estimated mean temperature (without considering effects from an atmosphere) of −3 degrees Celsius with an
2016:
Udry, Stéphane; Bonfils, Xavier; Delfosse, Xavier; Forveille, Thierry; Mayor, Michel; Perrier, Christian; Bouchy, François; Lovis, Christophe; Pepe, Francesco; Queloz, Didier; Bertaux, Jean-Loup (2007).
469:, including 68 candidates of approximately "Earth-size" (Rp < 1.25 Re) and 288 candidates of "super-Earth-size" (1.25 Re < Rp < 2 Re). In addition, 54 planet candidates were detected in the "
5881:
5876:
5871:
523:
was calculated which turned out to be similar to Earth's. At the size of about 2 Earth radii, it was the largest planet until 2014, which was determined to lack a significant hydrogen atmosphere.
655:
has been proposed. However, in July 2017, more careful analysis of HARPS-N and HIRES data showed that Kepler-10c was much less massive than originally thought, instead around 7.37 (6.18 to 8.69)
662:
with a mean density of 3.14 g/cm. Instead of a primarily rocky composition, the more accurately determined mass of Kepler-10c suggests a world made almost entirely of volatiles, mainly water.
5866:
931:
in the Solar System, and all larger planets have both at least 14 times the mass of Earth and thick gaseous envelopes without well-defined rocky or watery surfaces; that is, they are either
947:, but it is speculated to also be an ice giant like Uranus or Neptune. A refined model in 2019 constrains it to around five Earth masses; planets of this mass are probably mini-Neptunes.
3086:
Mayor, M.; et al. (2011). "The HARPS search for southern extra-solar planets XXXIV. Occurrence, mass distribution and orbital properties of super-Earths and
Neptune-mass planets".
489:. On HD 85512 b, it would be habitable if it exhibits more than 50% cloud cover. Then less than a month later, a flood of 41 new exoplanets, including 10 super-Earths, were announced.
275:
Mass and radius values for transiting super-Earths in context of other detected exoplanets and selected composition models. The "Fe" line defines planets made purely of iron, and "H
77:, which are 14.5 and 17 times Earth's, respectively. The term "super-Earth" refers only to the mass of the planet, and so does not imply anything about the surface conditions or
2834:
Borucki, W. J.; for the Kepler Team (2010). "Characteristics of Kepler
Planetary Candidates Based on the First Data Set: The Majority are Found to be Neptune-Size and Smaller".
2514:
496:
is 2.4 times the radius of the Earth and occupies an orbit 15% closer to its star than the Earth to the Sun. This is compensated for, however, as the star, with a spectral type
1489:
2908:
5861:
6023:
5888:
616:, 1,200 light years from Earth. These new super-Earths have radii of 1.3, 1.4, 1.6, and 1.9 times that of Earth. Theoretical modelling of two of these super-Earths,
4600:
D'Angelo, G.; Bodenheimer, P. (2013). "Three-dimensional
Radiation-hydrodynamics Calculations of the Envelopes of Young Planets Embedded in Protoplanetary Disks".
1078:
in the mantle acting on strong gravity would make the crust stronger and thus inhibit plate tectonics. The planet's surface would be too strong for the forces of
1094:
Theoretical models show that Hot
Jupiters and Hot Neptunes can evolve by hydrodynamic loss of their atmospheres to Mini-Neptunes (as it could be the Super-Earth
1359:
Fortney, J. J.; Marley, M. S.; Barnes, J. W. (2007). "Planetary Radii across Five Orders of
Magnitude in Mass and Stellar Insolation: Application to Transits".
2980:
Pepe, F.; et al. (2011). "The HARPS search for Earth-like planets in the habitable zone: I – Very low-mass planets around HD20794, HD85512 and HD192310".
108:. The term does not imply temperatures, compositions, orbital properties, habitability, or environments. While sources generally agree on an upper bound of 10
3237:
1961:
Zhou, J.-L.; et al. (2005). "Origin and
Ubiquity of Short-Period Earth-like Planets: Evidence for the Sequential Accretion Theory of Planet Formation".
1332:"Newly Discovered Exoplanet May be Best Candidate in Search for Signs of Life - Transiting rocky super-Earth found in habitable zone of quiet red dwarf star"
962:
led some astronomers believing that a super-Earth might have formed in proximity to the Sun, cleared its neighborhood and rapidly get disrupted by the Sun.
997:
Researchers at Harvard Astronomy Department have developed user-friendly online tools to characterize the bulk composition of the super-Earths. A study on
5915:
1046:, which is explained by a bimodal formation of planets (rocky Super-Earths below 1.75 and sub-Neptunes with thick gas envelopes being above such radii).
4127:
2571:"The HARPS search for southern extra-solar planets XXVII. Up to seven planets orbiting HD 10180: probing the architecture of low-mass planetary systems"
3468:
1677:
Borucki, William J.; et al. (2011). "Characteristics of planetary candidates observed by Kepler, II: Analysis of the first four months of data".
526:
On 20 December 2011, the Kepler team announced the discovery of the first Earth-size exoplanets, Kepler-20e and Kepler-20f, orbiting a Sun-like star,
5700:
5695:
4132:
5856:
5319:
1235:
205:
3211:
492:
On 5 December 2011, the Kepler space telescope discovered its first planet within the habitable zone or "Goldilocks region" of its Sun-like star.
2781:
Borucki, W. J.; et al. (2011). "Characteristics of planetary candidates observed by Kepler, II: Analysis of the first four months of data".
2329:
1870:
Mayor, M.; Pepe, F.; Lovis, C.; Oueloz, D.; Udry, S. (2008). "The quest for very low-mass planets". In Livio, M.; Sahu, K.; Valenti, J. (eds.).
5623:
3321:
1186:. A more massive planet of two Earth masses would also retain more heat within its interior from its initial formation much longer, sustaining
2203:
541:(GJ 667 Cc) was included in a paper published on 21 November 2011. More detailed data on Gliese 667 Cc were published in early February 2012.
4698:
4660:
4491:
2093:
1534:"A team of ICE/IEEC astronomers announces the discovery of a possible terrestrial-type exoplanet orbiting a star in the constellation of Leo"
1126:
of super-Earths are unknown, the surface temperatures are unknown and generally only an equilibrium temperature is given. For example, the
1069:
Further theoretical work by Valencia and others suggests that super-Earths would be more geologically active than Earth, with more vigorous
3386:
Rajpaul, V.; Buchhave, L. A.; Aigrain, S. (2017), "Pinning down the mass of Kepler-10c: the importance of sampling and model comparison",
5594:
5177:
4309:
939:, not terrestrial planets. In January 2016, the existence of a hypothetical super-Earth ninth planet in the Solar System, referred to as
2120:
Bennett, D. P.; et al. (2008). "A Low-Mass Planet with a Possible Sub-Stellar-Mass Host in Microlensing Event MOA-2007-BLG-192".
2091:
Bennett, D. P.; et al. (2008). "Discovery of a Low-mass Planet Orbiting a Low-mass Star in Microlensing Event MOA-2007-BLG-192".
5910:
5454:
4862:
4691:
4653:
1513:
1499:
323:
5630:
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840:
b was announced. At 16 light-years it is the closest super-Earth known, and its star is the second-brightest hosting a super-Earth.
5893:
5730:
5459:
3929:
3333:
Dumusque, Xavier (2014). "The Kepler-10 Planetary System Revisited by Harps-N: A Hot Rocky World and a Solid Neptune-Mass Planet".
4749:
2522:
5577:
829:(USP) Super-Earth, with a period of 0.28 days orbiting the host star K2-141 (EPIC 246393474) was reported. Another Super-Earth,
6063:
5606:
4737:
2018:
1050:
6038:
5990:
5985:
5980:
5975:
5970:
5965:
5960:
5955:
5950:
5945:
5940:
5935:
5930:
5925:
5920:
5611:
4576:
3802:
1537:
5720:
5710:
3241:
1533:
450:
264:
and 40 degrees Celsius with an albedo comparable to Earth. Subsequent research suggested Gliese 581c had likely suffered a
5444:
4128:
Origin and loss of nebula-captured hydrogen envelopes from `sub´- to `super-Earths´in the habitable zone of Sun-like stars
1127:
5756:
5690:
4804:
703:
said they found a planetary system with three super-Earths orbiting a bright, dwarf star. The four-planet system, dubbed
5123:
341:. Planets have at least the following minimum masses: 4.2, 6.7, and 9.4 times Earth's. The planets were detected by the
6048:
5898:
5705:
5582:
1883:
1276:
Valencia, V.; Sasselov, D. D.; O'Connell, R. J. (2007). "Radius and structure models of the first super-earth planet".
1198:) for longer. The thicker atmosphere and stronger magnetic field would also shield life on the surface against harmful
3054:
2678:
1730:
Seager, S.; Kuchner, M.; Hier-Majumder, C. A.; Militzer, B. (2007). "Mass–radius relationships for solid exoplanets".
6081:
5715:
4378:
2361:
93:
3245:
2746:
5776:
5766:
5254:
3901:
3059:
2751:
500:, is slightly dimmer than the Sun (G2V). Thus, surface temperatures would still allow liquid water on its surface.
2931:
2659:
81:. The alternative term "gas dwarfs" may be more accurate for those at the higher end of the mass scale, although "
5851:
5802:
5725:
5564:
4867:
4066:
Zeng, Li; Sasselov, Dimitar (2013). "A Detailed Model Grid for Solid Planets from 0.1 through 100 Earth Masses".
4030:
3271:
1054:
3584:
2570:
5807:
4261:
Geoffrey W. Marcy, Lauren M. Weiss, Erik A. Petigura, Howard Isaacson, Andrew W. Howard and Lars A. Buchhave. "
3696:"The first super-Earth Detection from the High Cadence and High Radial Velocity Precision Dharma Planet Survey"
3182:
612:, of the agency's Ames Research Center, found five planets orbiting in the habitable zone of a Sun-like star,
356:
In addition, the same European research team announced a planet 7.5 times the mass of Earth orbiting the star
6033:
5680:
5635:
5514:
5504:
5499:
5484:
5479:
4771:
4512:
3613:"An Ultra-short Period Rocky Super-Earth with a Secondary Eclipse and a Neptune-like Companion around K2-141"
2548:
2333:
1217:
674:
discovered by the Kepler space telescope. Three of the newly confirmed exoplanets were found to orbit within
6018:
5364:
410:
By November 2009, a total of 30 super-Earths had been discovered, 24 of which were first observed by HARPS.
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5449:
3828:
NASA found a super-Earth. It's in a tantalizing place. Scientists are investigating this curious new world.
712:
5324:
2492:
2415:
1562:
Fressin, François; et al. (2013). "The false positive rate of Kepler and the occurrence of planets".
6013:
5812:
4403:
4034:
2663:
2578:
2359:
Barnes, R.; Jackson, B.; Greenberg, R.; Raymond, S. N. (2009). "Tidal Limits to Planetary Habitability".
442:
237:
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4417:
Lammer, Helmut; Erkaev, N. V.; Odert, P.; Kislyakova, K. G.; Leitzinger, M.; Khodachenko, M. L. (2013).
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5846:
5841:
5831:
5589:
5249:
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Howard, A. W.; et al. (2009). "The NASA-UC Eta-Earth Program: I. A Super-Earth Orbiting HD 7924".
2239:
1875:
708:
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303:
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2122:
1963:
1908:
1732:
1278:
826:
497:
466:
381:
265:
4777:
2878:
2211:
1853:
1837:
1391:
6182:
5836:
5781:
5642:
5534:
5429:
5189:
4832:
4725:
4541:
D'Angelo, G.; Lissauer, J. J. (2018). "Formation of Giant Planets". In Deeg H., Belmonte J. (ed.).
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3617:
1026:
planetary system show that the two innermost planets Kepler-11b and c, whose calculated mass is ≈2
570:
5549:
3776:
988:); super-Earths of intermediate density are inferred to either have water as a major constituent (
6058:
5761:
5685:
5259:
4797:
3827:
1058:
1043:
644:
was determined to have the mass comparable to Neptune (17 Earth masses). With the radius of 2.35
333:
In June 2008, European researchers announced the discovery of three super-Earths around the star
3442:"NASA's Kepler Marks 1,000th Exoplanet Discovery, Uncovers More Small Worlds in Habitable Zones"
326:
collaboration on June 2, 2008. This planet has approximately 3.3 Earth masses and orbits a
5771:
5652:
5264:
5214:
4276:
Masses, Radii, and Orbits of Small Kepler Planets: The Transition from Gaseous to Rocky Planets
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2518:
1494:
1386:
1169:
944:
734:
462:
431:
167:
121:
78:
5239:
6172:
5740:
5509:
5384:
5284:
5118:
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2693:
814:
809:
602:
537:(GJ 667 Cb) was announced by HARPS on 19 October 2009, together with 29 other planets, while
507:
5309:
4347:
3003:
2601:
2252:
2054:
271:
6053:
6028:
6008:
5618:
5289:
5204:
4900:
4827:
4619:
4556:
4440:
4343:
4187:
4085:
3969:
3865:
3717:
3677:
3636:
3553:
3405:
3352:
3207:
3147:
2999:
2959:
2800:
2712:
2597:
2458:
2380:
2295:
2248:
2207:
2141:
2102:
2050:
1982:
1927:
1804:
1751:
1696:
1641:
1581:
1446:
1378:
1297:
1018:
and 3.3g (19 and 32 m/s). However, this planet is not known to transit its host star.
281:
126:
4702:
4664:
4147:
Understanding the Mass-Radius Relation for Sub-Neptunes: Radius as a Proxy for Composition
1074:
Earth itself, assuming similar composition. However, other studies determined that strong
8:
6156:
5821:
5369:
5349:
5304:
5274:
5083:
5078:
4877:
4528:
Are terrestrial exoplanets Earth-like, Venus-like, or the remnants of gas- or ice-giants?
3441:
2904:
1107:
1075:
557:, about 6.9 times the mass of Earth and somewhat hotter, was considered to be within the
299:
4623:
4560:
4444:
4191:
4089:
3973:
3926:
3869:
3721:
3640:
3409:
3356:
3151:
2804:
2716:
2462:
2384:
2299:
2175:
2145:
2106:
1986:
1931:
1808:
1755:
1700:
1645:
1585:
1450:
1425:
Charbonneau, D.; et al. (2009). "A super-Earth transiting a nearby low-mass star".
1382:
1301:
852:
was announced. Thirty-one light-years from the Solar System, the planet is at least 6.1
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5417:
5334:
5294:
5209:
4909:
4790:
4635:
4609:
4582:
4546:
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Occurrence and core-envelope structure of 1-4x Earth-size planets around Sun-like stars
4205:
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4101:
4075:
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3959:
3883:
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3735:
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3423:
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3368:
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3137:
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3034:
3015:
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2728:
2702:
2637:
2613:
2587:
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2470:
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2437:
Rogers, L.; Seager, S. (2010). "Three Possible Origins for the Gas Layer on GJ 1214b".
2396:
2370:
2311:
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2040:
1998:
1972:
1943:
1917:
1820:
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1767:
1741:
1712:
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1631:
1597:
1571:
1470:
1436:
1404:
1368:
1313:
1287:
928:
775:
319:
197:) of the system have masses approximately four times Earth—too small to be gas giants.
4305:
3364:
3159:
2849:
2724:
2392:
1620:"The California-Kepler Survey. III. A Gap in the Radius Distribution of Small Planets"
5665:
5299:
5047:
5042:
4991:
4841:
4639:
4631:
4586:
4572:
4545:. Springer International Publishing AG, part of Springer Nature. pp. 2319–2343.
4506:
4383:
4359:
4209:
4200:
4165:
3991:
3982:
3947:
3878:
3841:
3525:
3427:
2898:
2812:
2307:
2070:
1879:
1708:
1663:
1593:
1462:
1123:
253:
4526:
4462:
4113:
3739:
3658:
3496:
3372:
3167:
3019:
2820:
2617:
2478:
2400:
2161:
2074:
2002:
1947:
1854:"Exoplanets: From Exhilarating to Exasperating, 22:59, Kepler-10c: The 'Mega-Earth'"
1716:
1601:
1317:
322:. The planet was announced by astrophysicist David P. Bennett for the international
6108:
6043:
5791:
5554:
5544:
5404:
5354:
5244:
5234:
5158:
5088:
5073:
4872:
4627:
4564:
4448:
4351:
4195:
4093:
3977:
3887:
3873:
3725:
3644:
3413:
3360:
3155:
3033:
Kaltenegger, L.; Udry, S.; Pepe, F. (2011). "A Habitable Planet around HD 85512?".
3007:
2845:
2808:
2732:
2720:
2605:
2466:
2388:
2315:
2303:
2256:
2149:
2058:
1990:
1935:
1824:
1812:
1771:
1759:
1704:
1649:
1589:
1474:
1454:
1427:
1408:
1396:
1305:
1144:
1099:
1015:
959:
886:
792:
746:
162:
145:
4568:
3011:
2609:
2261:
2234:
2019:"The HARPS search for southern extra-solar planets XI. Super-Earths (5 and 8
1226: – Planet with a mass similar to Uranus or Neptune orbiting close to its star
707:, had been found 21 light years from Earth in the M-shaped northern hemisphere of
233:
5489:
5329:
5229:
5153:
5143:
4922:
3933:
2936:
2857:
2062:
1187:
1070:
609:
342:
194:
190:
30:
1541:
236:
based in Switzerland announced the discovery of two new super-Earths within the
5394:
5389:
5194:
5103:
4355:
3649:
3612:
3589:
3107:
2894:"Exclusive: "Most Earth-Like" Exoplanet Gets Major Demotion—It Isn't Habitable"
1654:
1619:
1147:
0.67), giving it a lower black body temperature than the more absorbent (lower
1135:
1006:
1002:
906:
890:
782:
675:
598:
558:
470:
241:
217:
4105:
1858:
6166:
5529:
5524:
5519:
5199:
5138:
5093:
5032:
5027:
5002:
4937:
4927:
4917:
4363:
4331:
3461:
3128:
Winn, J.N.; et al. (2008). "A Super Earth Transiting a Naked-Eye Star".
1518:
1229:
955:
538:
534:
486:
377:
360:. This star also has a Jupiter-like planet that orbits it every three years.
201:
186:
24:
4289:
3730:
3695:
3418:
6120:
5675:
5660:
5539:
5436:
5359:
5128:
5108:
5098:
4996:
4932:
4453:
4418:
3064:
1466:
1331:
1211:
1191:
1183:
1178:
According to one hypothesis, super-Earths of about two Earth masses may be
1173:
1091:
the small rocky core remains engulfed by its large hydrogen-rich envelope.
998:
989:
985:
924:
554:
474:
423:
392:
213:
117:
82:
4388:
2544:
1005:
revealed that it would be possible to infer from a radius measured by the
5601:
5379:
5374:
5344:
5314:
5269:
5224:
5219:
5148:
5133:
5068:
5012:
5007:
4958:
4953:
4947:
2756:
1977:
1922:
1373:
1292:
1223:
1199:
1179:
1140:
940:
918:
758:
750:
716:
691:
687:
683:
629:
624:, suggests both could be solid, either rocky or rocky with frozen water.
520:
512:
446:
419:
388:
327:
245:
170:– based on 2,740 candidates orbiting 2,036 stars as of November 4, 2013 (
1458:
905:
reported the discovery of a super-Earth called TOI-715 b located in the
244:
around the star where liquid water may be possible on the surface. With
5572:
5339:
5113:
5037:
4963:
4942:
4332:"Plate tectonics on super-Earths: Equally or more likely than on Earth"
1246:
1027:
992:), or have a denser core enshrouded with an extended gaseous envelope (
936:
932:
853:
754:
652:
641:
621:
617:
608:
In April 2013, using observations by NASA's Kepler mission team led by
574:
550:
493:
482:
427:
307:
249:
209:
179:
150:
130:
109:
20:
5022:
5017:
4983:
4968:
4857:
4250:
The mass-radius relation for 65 exoplanets smaller than 4 Earth radii
3301:
3275:
3186:
1785:
Seager, S. (2007). "Mass-Radius Relationships for Solid Exoplanets".
1240:
1095:
1023:
993:
786:
778:
770:
762:
671:
613:
586:
527:
404:
397:
373:
357:
134:
125:
Solar System do not have. Planets above 10 Earth masses are termed
98:
66:
58:
19:
This article is about the planet type. For the fictional polity, see
5412:
4551:
4182:
4097:
3964:
3948:"Probabilistic Forecasting of the Masses and Radii of Other Worlds"
3860:
3712:
3631:
3558:
3440:
Clavin, Whitney; Chou, Felicia; Johnson, Michele (6 January 2015).
3400:
2180:
2153:
1994:
1939:
1816:
1763:
1636:
1400:
1309:
951:
882:
870:
849:
837:
738:
435:
369:
334:
178:
The first super-Earths were discovered by Aleksander Wolszczan and
137:, depending on whether they are mostly rock and ice or mostly gas.
35:
4778:
Why is the Earth called a unique planet in our solar system ?
4614:
4476:
4435:
4275:
4262:
4249:
4236:
4223:
4146:
4080:
3347:
3142:
3092:
3039:
2994:
2840:
2795:
2707:
2592:
2453:
2375:
2290:
2136:
2045:
1799:
1746:
1729:
1691:
1576:
1441:
1044:
gap or rarity observed for planets between 1.5 and 2.0 Earth-radii
881:
In 2022, the discovery of a super-Earth around the red dwarf star
5424:
4224:
The Mass of Kepler-93b and The Composition of Terrestrial Planets
3674:"Potentially habitable super-Earth found during exoplanet search"
1195:
1011:
943:, was proposed as an explanation for the orbital behavior of six
830:
719:, and is Earth's closest known rocky, and transiting, exoplanet.
704:
445:
announced on 29 September the discovery of a fourth super-Earth (
74:
43:
4291:
Laser-Driven Shock Compression Studies of Planetary Compositions
2660:"Newly Discovered Planet May Be First Truly Habitable Exoplanet"
485:
was found using the HARPS as well as a three super-Earth system
5735:
5063:
4887:
4822:
4766:
4419:"Probing the blow-off criteria of hydrogen-rich 'super-Earths'"
2686:
Planet in the Habitable Zone of the Nearby M3V Star Gliese 581"
1148:
1131:
1119:
975:
742:
396:
100 times more tidal heating than Jupiter's volcanic satellite
257:
221:
183:
113:
70:
4782:
2358:
1275:
1079:
927:
contains no known super-Earths, because Earth is the largest
800:
582:
350:
346:
261:
248:
having a mass of at least 5 Earth masses and a distance from
120:(from 2 to 4 Earth-radii). This definition was made by the
62:
39:
2015:
1617:
4728:, Charles Q. Choi, SPACE.com, November 22, 2012 02:01pm ET,
4599:
4540:
4416:
4166:"In Situ and Ex Situ Formation Models of Kepler 11 Planets"
4163:
4159:
4157:
4155:
4054:
3530:
3501:
3446:
1139:
based on the fact that Venus has an extremely high albedo (
902:
789:
728:
679:
590:
298:
Two further possible super-Earths were discovered in 2006:
171:
105:
6115:
3840:
Batygin, Konstantin; Brown, Michael E. (20 January 2016).
3388:
Monthly Notices of the Royal Astronomical Society: Letters
2833:
1490:"Canada's orbiting telescope tracks mystery 'super Earth'"
1232: – Planet larger than Neptune but smaller than Saturn
979:
Comparison of sizes of planets with different compositions
6024:
Exoplanetary Circumstellar Environments and Disk Explorer
3842:"Evidence for a distant giant planet in the Solar System"
3473:
2235:"The CoRoT-7 planetary system: two orbiting Super-Earths"
796:
594:
549:
In September 2012, the discovery of two planets orbiting
338:
4593:
4152:
3803:"Discovery Alert: A 'Super-Earth' in the Habitable Zone"
3183:"Oozing Super-Earth: Images of Alien Planet 55 Cancri e"
1010:
radii the super-Earth Gliese 876 d would have a surface
65:'s, but substantially below those of the Solar System's
4068:
Publications of the Astronomical Society of the Pacific
3238:"A Hot Potential Habitable Exoplanet around Gliese 163"
2780:
1838:
Astronomers find a new type of planet: The 'mega-Earth'
807:
may be a flyby destination for a fleet of interstellar
768:
In August 2016, astronomers announced the detection of
670:
On 6 January 2015, NASA announced the 1000th confirmed
4494:. 2009-04-25. Archived from the original on 2011-05-27
4031:"Scientists Model a Cornucopia of Earth-sized Planets"
3385:
1220: – Liquid water naturally occurring outside Earth
6092:
4752:, René Heller, Scientific American 312, January, 2015
4740:, René Heller, Scientific American 312, January, 2015
3755:"Super-Earth Discovered in (Fictional) Vulcan System"
3693:
3585:"One Star Over, a Planet That Might Be Another Earth"
3497:"PIA19832: Location of Nearest Rocky Exoplanet Known"
1420:
1418:
589:
candidate (1.5 times the radius of Earth) orbiting a
337:, a star that is only slightly less massive than the
149:
Illustration of the inferred size of the super-Earth
34:
Illustration of the inferred size of the super-Earth
4726:
Super-Earths Get Magnetic 'Shield' from Liquid Metal
4525:
Sotin, Christophe; Grasset, O.; Mocquet, A. (2013),
4007:"Our sun may have eaten a super-Earth for breakfast"
3272:"Newfound Alien Planet a Top Contender to Host Life"
2960:"Cosmic census finds crowd of planets in our galaxy"
2204:"AFP: Astronomers discover clutch of 'super-Earths'"
1869:
376:, is the first super-Earth discovered that orbits a
302:
with a mass of 5.5 Earth masses, which was found by
4686:
4684:
3244:(Planetary Habitability Laboratory). Archived from
3032:
1358:
715:of its star. The planet with the shortest orbit is
690:, are near-Earth-size and likely rocky; the third,
349:(High Accuracy Radial Velocity Planet Searcher) in
3777:"Super-Earth Skimming Habitable Zone of Red Dwarf"
1872:A Decade of Extrasolar Planets around Normal Stars
1415:
1214: – Planet with environment similar to Earth's
481:On 17 August, a potentially habitable super-Earth
5701:Habitability of K-type main-sequence star systems
5696:Habitability of F-type main-sequence star systems
4423:Monthly Notices of the Royal Astronomical Society
4330:van Heck, H.J.; Tackley, P.J. (15 October 2011).
4133:Monthly Notices of the Royal Astronomical Society
3700:Monthly Notices of the Royal Astronomical Society
3526:"NASA's Spitzer Confirms Closest Rocky Exoplanet"
3439:
3265:
3263:
2515:"Second Smallest Exoplanet Found To Date At Keck"
1049:Additional studies, conducted with lasers at the
761:, the first time the atmosphere of a super-Earth
330:. It was detected by gravitational microlensing.
97:Artist's impression of the super-Earth exoplanet
6164:
5320:List of interstellar and circumstellar molecules
4681:
4646:
3611:Malavolta, Luca; et al. (9 February 2018).
3517:
1851:
1778:
1236:List of nearest terrestrial exoplanet candidates
909:of a red dwarf star about 137 light-years away.
220:), it may have a surface temperature of 430–650
4478:A super-Earth transiting a nearby low-mass star
4329:
3610:
3578:
3576:
3524:Chou, Felicia; Clavin, Whitney (30 July 2015).
3469:"Astronomers find star with three super-Earths"
3231:
3229:
3199:
970:
3289:
3260:
1847:
1845:
1670:
430:, is the least massive planet detected by the
318:The smallest super-Earth found as of 2008 was
104:In general, super-Earths are defined by their
4798:
3545:
3489:
3433:
3298:"Most Earth-Like Alien Planet Possibly Found"
3212:Centre de données astronomiques de Strasbourg
2633:"New Planet May Be Able to Nurture Organisms"
2094:Bulletin of the American Astronomical Society
1555:
4065:
3839:
3573:
3226:
2493:"32 planets discovered outside solar system"
2436:
1723:
1514:"Life could survive longer on a super-Earth"
813:spacecraft currently being developed by the
4310:Harvard-Smithsonian Center for Astrophysics
4237:Most 1.6 Earth-Radius Planets are not Rocky
3945:
3939:
3604:
3554:"First detection of super-earth atmosphere"
3174:
3108:"First Detection of Super-Earth Atmosphere"
3026:
2951:
2679:"The Lick-Carnegie Exoplanet Survey: A 3.1
1842:
1424:
4805:
4791:
4404:"Super-Earths are more like mini-Neptunes"
3781:National Astronomical Observatory of Japan
3523:
3127:
2957:
2776:
2774:
2430:
2352:
2269:
2226:
1906:Planet Orbiting the Nearby Star, GJ 876".
1271:
1269:
1267:
1265:
1263:
227:
140:
4863:Exoplanet orbital and physical parameters
4750:Box 1 Super-Earths' Big Benefits for Life
4613:
4550:
4452:
4434:
4287:
4248:Lauren M. Weiss, and Geoffrey W. Marcy. "
4199:
4181:
4079:
3981:
3963:
3877:
3859:
3830:Mashable, Mark Kaufman, February 7, 2024
3729:
3711:
3689:
3687:
3671:
3648:
3630:
3417:
3399:
3346:
3295:
3141:
3091:
3038:
2993:
2839:
2794:
2706:
2591:
2452:
2374:
2289:
2260:
2135:
2044:
1976:
1921:
1798:
1745:
1690:
1653:
1635:
1618:Fulton, Benjamin J.; et al. (2017).
1613:
1611:
1575:
1440:
1390:
1372:
1354:
1352:
1291:
467:list of 1235 extrasolar planet candidates
5731:List of potentially habitable exoplanets
3332:
3326:
2537:
1954:
1899:Rivera, E.; et al. (2005). "A ~7.5
1134:(−18 °C or 0 °F ). It is the
974:
727:In February 2016, it was announced that
601:and possibly a "prime candidate to host
569:On 7 January 2013, astronomers from the
506:
270:
224:and be too hot to support liquid water.
161:
144:
92:
29:
3946:Chen, Jingjing; Kipping, David (2016).
2929:
2923:
2771:
2630:
2322:
2119:
2090:
1676:
1561:
1260:
418:Discovered on 5 January 2010, a planet
6165:
4534:
4306:"Earth: A Borderline Planet for Life?"
4164:D'Angelo, G.; Bodenheimer, P. (2016).
4004:
3684:
3235:
3121:
2416:"Scientists spot nearby 'super-Earth'"
2413:
2275:
2232:
1898:
1784:
1608:
1487:
1349:
1051:Lawrence Livermore National Laboratory
6039:Geodynamics of terrestrial exoplanets
4786:
4379:"The plate tectonics of alien worlds"
4376:
3752:
3582:
3551:
3214:(Strasbourg astronomical Data Center)
3205:
3180:
3085:
2891:
2885:
2568:
2545:"Richest Planetary System Discovered"
1249: – Super-Earth orbiting TOI-1452
1098:), or even to rocky planets known as
463:Kepler Space Observatory mission team
5721:Habitability of yellow dwarf systems
5711:Habitability of neutron star systems
4145:Eric D. Lopez, Jonathan J. Fortney "
3936:findplanetnine.com February 26, 2019
3753:Young, Monica (September 17, 2018).
3296:Moskowitz, Clara (January 9, 2013).
3269:
3242:University of Puerto Rico at Arecibo
2979:
2973:
2676:
2009:
1960:
1064:
553:was announced. One of the planets,
451:The Extrasolar Planets Encyclopaedia
204:star was discovered by a team under
6064:Sudarsky's gas giant classification
5691:Habitability of binary star systems
4336:Earth and Planetary Science Letters
3672:Jorgenson, Amber (March 14, 2018).
3208:"LHS 188 – High proper-motion Star"
2958:Borenstein, S. (19 February 2011).
2330:"Lightest exoplanet yet discovered"
2176:"Trio of 'super-Earths' discovered"
1190:(which is vital for regulating the
950:The fact that there are barely any
885:was reported. Part of the planet's
825:In February 2018, K2-141b, a rocky
640:In May 2014, previously discovered
13:
6049:Nexus for Exoplanet System Science
5706:Habitability of natural satellites
4475:Charbonneau, David et al. (2009),
3902:"New planet lurks in Solar System"
2414:Sutter, J. D. (16 December 2009).
1106:the gas-phase of their progenitor
965:
912:
14:
6194:
5716:Habitability of red dwarf systems
4759:
4692:"Emission Temperature of Planets"
4654:"Emission Temperature of Planets"
4401:
4288:Spaulding, Dylan Kenneth (2010).
3583:Chang, Kenneth (24 August 2016).
2677:Vogt, S. S.; et al. (2010).
2631:Overbye, D. (29 September 2010).
2362:The Astrophysical Journal Letters
1243: – Planet smaller than Earth
1154:
403:A planet found in December 2009,
288:
6150:
6138:
6126:
6114:
6102:
5813:Stars with proto-planetary discs
5777:NASA Star and Exoplanet Database
5767:Extrasolar Planets Encyclopaedia
5255:Extraterrestrial sample curation
4886:
4765:
4743:
4531:, American Astronomical Society.
4492:"Exoplanets Exposed to the Core"
3270:Redd, Nola (20 September 2012).
3060:Extrasolar Planets Encyclopaedia
2752:Extrasolar Planets Encyclopaedia
2521:. 7 January 2010. Archived from
2233:Queloz, D.; et al. (2009).
1852:Dimitar Sasselov (2 June 2014).
1082:to break the crust into plates.
310:with a mass of 10 Earth masses.
232:In April 2007, a team headed by
189:in 1992. The two outer planets (
153:(right) in comparison with Earth
5726:Habitable zone for complex life
5164:Ultra-short period planet (USP)
4868:Methods of detecting exoplanets
4731:
4719:
4519:
4484:
4469:
4410:
4395:
4370:
4323:
4298:
4281:
4268:
4255:
4242:
4229:
4216:
4139:
4120:
4059:
4048:
4023:
3998:
3920:
3894:
3833:
3821:
3795:
3769:
3746:
3665:
3379:
3315:
3236:Méndez, Abel (29 August 2012).
3100:
3079:
3047:
2930:Shostak, S. (3 February 2011).
2827:
2739:
2670:
2652:
2624:
2569:Lovis, C.; et al. (2015).
2562:
2507:
2485:
2407:
2336:. 21 April 2009. Archived from
2196:
2168:
2113:
2084:
1892:
1863:
1831:
1540:. 10 April 2008. Archived from
1538:Institut de Ciències de l'Espai
1488:Spotts, P. N. (28 April 2007).
1163:
1113:
848:In July 2019, the discovery of
836:In July 2018, the discovery of
200:The first super-Earth around a
5907:Discovered exoplanets by year
4812:
4005:Gough, Evan; Today, Universe.
2210:. 16 June 2008. Archived from
1526:
1506:
1481:
1324:
1:
6034:Extrasolar planets in fiction
5681:Extraterrestrial liquid water
4569:10.1007/978-3-319-55333-7_140
4377:Barry, C. (17 October 2007).
4222:Courtney D. Dressing et al. "
2549:European Southern Observatory
2334:European Southern Observatory
1253:
1218:Extraterrestrial liquid water
212:and received the designation
88:
6054:Planets in globular clusters
5671:Circumstellar habitable zone
3694:Ma, Bo; et al. (2018).
2982:Astronomy & Astrophysics
2579:Astronomy & Astrophysics
2471:10.1088/0004-637X/716/2/1208
2033:Astronomy & Astrophysics
1085:
971:Density and bulk composition
700:Astronomy & Astrophysics
38:(center) in comparison with
7:
6014:Exoplanet naming convention
5124:Planet/Brown dwarf boundary
4035:Goddard Space Flight Center
3365:10.1088/0004-637X/789/2/154
3206:Staff (20 September 2012).
3160:10.1088/2041-8205/737/1/L18
3012:10.1051/0004-6361/201117055
2850:10.1088/0004-637X/728/2/117
2725:10.1088/0004-637X/723/1/954
2664:National Science Foundation
2610:10.1051/0004-6361/201015577
2393:10.1088/0004-637X/700/1/L30
2262:10.1051/0004-6361/200913096
1205:
765:was analyzed successfully.
573:announced the discovery of
515:in front of its parent star
443:National Science Foundation
238:Gliese 581 planetary system
10:
6199:
5250:Extraterrestrial materials
4884:
4632:10.1088/0004-637X/778/1/77
4356:10.1016/j.epsl.2011.07.029
4274:Geoffrey W. Marcy et al. "
4201:10.3847/0004-637X/828/1/33
4136:, Oxford University Press.
3983:10.3847/1538-4357/834/1/17
3927:The Search for Planet Nine
3879:10.3847/0004-6256/151/2/22
3552:Staff (16 February 2016).
2892:Grant, A. (8 March 2011).
2813:10.1088/0004-637X/736/1/19
2308:10.1088/0004-637X/696/1/75
2240:Astronomy and Astrophysics
2063:10.1051/0004-6361:20077612
1876:Cambridge University Press
1709:10.1088/0004-637X/736/1/19
1594:10.1088/0004-637X/766/2/81
1167:
916:
799:. Due to its closeness to
795:, the closest star to the
304:gravitational microlensing
240:, both on the edge of the
18:
6077:Discoveries of exoplanets
6072:
6001:
5790:
5749:
5651:
5563:
5470:
5403:
5280:Interplanetary dust cloud
5176:
5056:
4982:
4908:
4895:
4850:
4818:
4602:The Astrophysical Journal
4511:: CS1 maint: unfit URL (
4170:The Astrophysical Journal
3952:The Astrophysical Journal
3335:The Astrophysical Journal
3181:Staff (20 January 2012).
3130:The Astrophysical Journal
2783:The Astrophysical Journal
2440:The Astrophysical Journal
2278:The Astrophysical Journal
2123:The Astrophysical Journal
1964:The Astrophysical Journal
1909:The Astrophysical Journal
1787:The Astrophysical Journal
1733:The Astrophysical Journal
1679:The Astrophysical Journal
1522:(2629). 11 November 2007.
1361:The Astrophysical Journal
1279:The Astrophysical Journal
827:ultra-short period planet
266:runaway greenhouse effect
85:" is a more common term.
5782:Open Exoplanet Catalogue
5757:Nearby Habitable Systems
5643:Transit-timing variation
3847:The Astronomical Journal
3650:10.3847/1538-3881/aaa5b5
3618:The Astronomical Journal
1655:10.3847/1538-3881/aa80eb
1624:The Astronomical Journal
709:constellation Cassiopeia
571:Kepler space observatory
168:Kepler Planet Candidates
157:
61:with a mass higher than
6059:Small planet radius gap
5762:Exoplanet Data Explorer
5686:Galactic habitable zone
5260:Giant-impact hypothesis
4481:, Nature 462, p.891–894
4348:2011E&PSL.310..252V
3004:2011A&A...534A..58P
2932:"A Bucketful of Worlds"
2602:2011A&A...528A.112L
2253:2009A&A...506..303Q
2055:2007A&A...469L..43U
2026:) in a 3-planet system"
1145:Visual geometric albedo
1118:Since the atmospheres,
1059:University of Rochester
945:trans-Neptunian objects
896:
876:
869:In 2021, the exoplanet
864:
843:
820:
722:
711:, but it is not in the
665:
635:
564:
544:
511:Artist's impression of
456:
413:
363:
313:
293:
228:First in habitable zone
141:History and discoveries
6019:Exoplanet phase curves
5857:Terrestrial candidates
5808:Multiplanetary systems
5772:NASA Exoplanet Archive
5455:Mean-motion resonances
5265:Gravitational collapse
5215:Circumstellar envelope
4543:Handbook of Exoplanets
4294:(Thesis). UC Berkeley.
2873:Cite journal requires
2519:W. M. Keck Observatory
2495:. CNN. 19 October 2009
1495:The Hamilton Spectator
1170:Planetary habitability
1130:of the Earth is 255.3
1128:black-body temperature
1033:and between ≈5 and 6 M
980:
735:Hubble Space Telescope
519:In 2011, a density of
516:
432:radial velocity method
285:
175:
154:
122:Kepler space telescope
101:
46:
5894:Potentially habitable
5799:Exoplanetary systems
5741:Superhabitable planet
5500:F/Yellow-white dwarfs
5385:Sample-return mission
5285:Interplanetary medium
3731:10.1093/mnras/sty1933
3419:10.1093/mnrasl/slx116
2694:Astrophysical Journal
1564:Astrophysical Journal
1168:Further information:
978:
815:Breakthrough Starshot
510:
274:
165:
148:
127:massive solid planets
112:(~69% of the mass of
96:
33:
6029:Extragalactic planet
6009:Carl Sagan Institute
5290:Interplanetary space
5205:Circumplanetary disk
4878:Planet-hosting stars
4774:at Wikimedia Commons
4454:10.1093/mnras/sts705
2666:. 29 September 2010.
2208:Agence France-Presse
958:inside the orbit of
889:takes it within the
745:(and suggestions of
694:, is a super-Earth.
682:: two of the three,
282:astronomical symbols
6178:Terrestrial planets
5370:Protoplanetary disk
5350:Planetary migration
5305:Interstellar medium
5084:Circumtriple planet
5079:Circumbinary planet
4624:2013ApJ...778...77D
4561:2018haex.bookE.140D
4445:2013MNRAS.430.1247L
4192:2016ApJ...828...33D
4090:2013PASP..125..227Z
4037:. 24 September 2007
3974:2017ApJ...834...17C
3870:2016AJ....151...22B
3757:. Sky and Telescope
3722:2018MNRAS.480.2411M
3641:2018AJ....155..107M
3410:2017MNRAS.471L.125R
3357:2014ApJ...789..154D
3152:2011ApJ...737L..18W
2905:Kalmbach Publishing
2805:2011ApJ...736...19B
2717:2010ApJ...723..954V
2525:on 25 December 2014
2463:2010ApJ...716.1208R
2385:2009ApJ...700L..30B
2300:2009ApJ...696...75H
2146:2008ApJ...684..663B
2107:2008AAS...212.1012B
2080:on October 8, 2010.
1987:2005ApJ...631L..85Z
1932:2005ApJ...634..625R
1809:2007ApJ...669.1279S
1756:2007ApJ...669.1279S
1701:2011ApJ...736...19B
1646:2017AJ....154..109F
1586:2013ApJ...766...81F
1459:10.1038/nature08679
1451:2009Natur.462..891C
1383:2007ApJ...659.1661F
1302:2007ApJ...656..545V
1108:protoplanetary disk
1076:convection currents
901:On 31 January 2024
461:On 2 February, the
300:OGLE-2005-BLG-390Lb
208:in 2005. It orbits
5335:Nebular hypothesis
5310:Interstellar space
5295:Interstellar cloud
5275:Internal structure
5210:Circumstellar disc
4235:Leslie A. Rogers "
4126:H. Lammer et al. "
3932:2020-11-30 at the
3678:Astronomy Magazine
3248:on 21 October 2019
3067:on October 5, 2011
2962:. Associated Press
2638:The New York Times
1124:greenhouse effects
1057:laboratory at the
981:
929:terrestrial planet
517:
320:MOA-2007-BLG-192Lb
286:
254:astronomical units
176:
155:
102:
47:
6090:
6089:
5666:Astrooceanography
5300:Interstellar dust
5172:
5171:
5048:Ultra-hot Neptune
5043:Ultra-hot Jupiter
4992:Eccentric Jupiter
4842:Planetary science
4770:Media related to
4738:Better Than Earth
4578:978-3-319-55332-0
4308:(Press release).
4055:www.astrozeng.com
3908:. 22 January 2016
3906:The Straits Times
3809:. 31 January 2024
2901:– Blogs / 80beats
2899:Discover Magazine
2662:(Press release).
1435:(7275): 891–894.
1180:conducive to life
1100:chthonian planets
1065:Geologic activity
1001:by a team around
833:, is discovered.
697:On 30 July 2015,
678:of their related
387:The discovery of
135:gas giant planets
16:Type of exoplanet
6190:
6155:
6154:
6153:
6143:
6142:
6141:
6131:
6130:
6129:
6119:
6118:
6107:
6106:
6105:
6098:
6044:Neptunian desert
5430:Tidally detached
5365:Planet formation
5355:Planetary system
5245:Exozodiacal dust
5235:Disrupted planet
5159:Ultra-cool dwarf
5089:Disrupted planet
5074:Chthonian planet
4906:
4905:
4890:
4873:Planetary system
4807:
4800:
4793:
4784:
4783:
4769:
4753:
4747:
4741:
4735:
4729:
4723:
4717:
4716:
4714:
4713:
4707:
4701:. Archived from
4696:
4688:
4679:
4678:
4676:
4675:
4669:
4663:. Archived from
4658:
4650:
4644:
4643:
4617:
4597:
4591:
4590:
4554:
4538:
4532:
4523:
4517:
4516:
4510:
4502:
4500:
4499:
4488:
4482:
4473:
4467:
4466:
4456:
4438:
4429:(2): 1247–1256.
4414:
4408:
4407:
4402:Black, Charles.
4399:
4393:
4392:
4387:. Archived from
4374:
4368:
4367:
4342:(3–4): 252–261.
4327:
4321:
4320:
4318:
4317:
4312:. 9 January 2008
4302:
4296:
4295:
4285:
4279:
4272:
4266:
4259:
4253:
4246:
4240:
4233:
4227:
4220:
4214:
4213:
4203:
4185:
4161:
4150:
4143:
4137:
4124:
4118:
4117:
4083:
4074:(925): 227–239.
4063:
4057:
4052:
4046:
4045:
4043:
4042:
4027:
4021:
4020:
4018:
4017:
4002:
3996:
3995:
3985:
3967:
3943:
3937:
3924:
3918:
3917:
3915:
3913:
3898:
3892:
3891:
3881:
3863:
3837:
3831:
3825:
3819:
3818:
3816:
3814:
3799:
3793:
3792:
3790:
3788:
3773:
3767:
3766:
3764:
3762:
3750:
3744:
3743:
3733:
3715:
3691:
3682:
3681:
3669:
3663:
3662:
3652:
3634:
3608:
3602:
3601:
3599:
3597:
3580:
3571:
3570:
3568:
3566:
3549:
3543:
3542:
3540:
3538:
3521:
3515:
3514:
3512:
3510:
3493:
3487:
3486:
3484:
3482:
3465:
3459:
3458:
3456:
3454:
3437:
3431:
3430:
3421:
3403:
3394:(1): L125–L130,
3383:
3377:
3376:
3350:
3330:
3324:
3319:
3313:
3312:
3310:
3308:
3293:
3287:
3286:
3284:
3282:
3267:
3258:
3257:
3255:
3253:
3233:
3224:
3223:
3221:
3219:
3203:
3197:
3196:
3194:
3193:
3178:
3172:
3171:
3145:
3125:
3119:
3118:
3116:
3114:
3104:
3098:
3097:
3095:
3083:
3077:
3076:
3074:
3072:
3063:. Archived from
3055:"Star: HD 20781"
3051:
3045:
3044:
3042:
3030:
3024:
3023:
2997:
2977:
2971:
2970:
2968:
2967:
2955:
2949:
2948:
2946:
2944:
2927:
2921:
2920:
2918:
2916:
2907:. Archived from
2889:
2883:
2882:
2876:
2871:
2869:
2861:
2843:
2831:
2825:
2824:
2798:
2778:
2769:
2768:
2766:
2764:
2755:. Archived from
2743:
2737:
2736:
2710:
2690:
2674:
2668:
2667:
2656:
2650:
2649:
2647:
2645:
2628:
2622:
2621:
2595:
2575:
2566:
2560:
2559:
2557:
2556:
2551:. 24 August 2010
2541:
2535:
2534:
2532:
2530:
2511:
2505:
2504:
2502:
2500:
2489:
2483:
2482:
2456:
2447:(2): 1208–1216.
2434:
2428:
2427:
2425:
2423:
2411:
2405:
2404:
2378:
2356:
2350:
2349:
2347:
2345:
2340:on 6 August 2009
2326:
2320:
2319:
2293:
2273:
2267:
2266:
2264:
2230:
2224:
2223:
2221:
2219:
2200:
2194:
2193:
2191:
2189:
2172:
2166:
2165:
2139:
2117:
2111:
2110:
2088:
2082:
2081:
2079:
2073:. Archived from
2048:
2030:
2013:
2007:
2006:
1980:
1978:astro-ph/0508305
1958:
1952:
1951:
1925:
1923:astro-ph/0510508
1896:
1890:
1889:
1867:
1861:
1857:
1849:
1840:
1835:
1829:
1828:
1802:
1793:(2): 1279–1297.
1782:
1776:
1775:
1749:
1740:(2): 1279–1297.
1727:
1721:
1720:
1694:
1674:
1668:
1667:
1657:
1639:
1615:
1606:
1605:
1579:
1559:
1553:
1552:
1550:
1549:
1530:
1524:
1523:
1510:
1504:
1503:
1498:. Archived from
1485:
1479:
1478:
1444:
1422:
1413:
1412:
1394:
1376:
1374:astro-ph/0612671
1367:(2): 1661–1672.
1356:
1347:
1346:
1344:
1342:
1328:
1322:
1321:
1295:
1293:astro-ph/0610122
1273:
1136:greenhouse gases
887:elliptical orbit
873:was discovered.
793:Proxima Centauri
747:hydrogen cyanide
733:
420:HD 156668 b
6198:
6197:
6193:
6192:
6191:
6189:
6188:
6187:
6183:Types of planet
6163:
6162:
6161:
6151:
6149:
6139:
6137:
6127:
6125:
6113:
6103:
6101:
6093:
6091:
6086:
6082:Search projects
6068:
5997:
5786:
5745:
5647:
5619:Radial velocity
5559:
5515:K/Orange dwarfs
5505:G/Yellow dwarfs
5466:
5460:Titius–Bode law
5399:
5330:Molecular cloud
5230:Detached object
5181:
5179:
5168:
5154:Toroidal planet
5144:Sub-brown dwarf
5052:
4978:
4950:(Super-Mercury)
4923:Coreless planet
4899:
4897:
4891:
4882:
4846:
4814:
4811:
4762:
4757:
4756:
4748:
4744:
4736:
4732:
4724:
4720:
4711:
4709:
4705:
4694:
4690:
4689:
4682:
4673:
4671:
4667:
4656:
4652:
4651:
4647:
4598:
4594:
4579:
4539:
4535:
4524:
4520:
4504:
4503:
4497:
4495:
4490:
4489:
4485:
4474:
4470:
4415:
4411:
4400:
4396:
4375:
4371:
4328:
4324:
4315:
4313:
4304:
4303:
4299:
4286:
4282:
4273:
4269:
4260:
4256:
4247:
4243:
4234:
4230:
4221:
4217:
4176:(1): in press.
4162:
4153:
4144:
4140:
4125:
4121:
4064:
4060:
4053:
4049:
4040:
4038:
4029:
4028:
4024:
4015:
4013:
4003:
3999:
3944:
3940:
3934:Wayback Machine
3925:
3921:
3911:
3909:
3900:
3899:
3895:
3838:
3834:
3826:
3822:
3812:
3810:
3801:
3800:
3796:
3786:
3784:
3783:. 1 August 2022
3775:
3774:
3770:
3760:
3758:
3751:
3747:
3692:
3685:
3670:
3666:
3609:
3605:
3595:
3593:
3581:
3574:
3564:
3562:
3550:
3546:
3536:
3534:
3522:
3518:
3508:
3506:
3495:
3494:
3490:
3480:
3478:
3467:
3466:
3462:
3452:
3450:
3438:
3434:
3384:
3380:
3331:
3327:
3320:
3316:
3306:
3304:
3294:
3290:
3280:
3278:
3268:
3261:
3251:
3249:
3234:
3227:
3217:
3215:
3204:
3200:
3191:
3189:
3179:
3175:
3126:
3122:
3112:
3110:
3106:
3105:
3101:
3084:
3080:
3070:
3068:
3053:
3052:
3048:
3031:
3027:
2978:
2974:
2965:
2963:
2956:
2952:
2942:
2940:
2937:Huffington Post
2928:
2924:
2914:
2912:
2911:on 9 March 2011
2890:
2886:
2874:
2872:
2863:
2862:
2832:
2828:
2779:
2772:
2762:
2760:
2745:
2744:
2740:
2688:
2685:
2682:
2675:
2671:
2658:
2657:
2653:
2643:
2641:
2629:
2625:
2573:
2567:
2563:
2554:
2552:
2543:
2542:
2538:
2528:
2526:
2513:
2512:
2508:
2498:
2496:
2491:
2490:
2486:
2435:
2431:
2421:
2419:
2412:
2408:
2357:
2353:
2343:
2341:
2328:
2327:
2323:
2274:
2270:
2231:
2227:
2217:
2215:
2214:on 19 June 2008
2202:
2201:
2197:
2187:
2185:
2174:
2173:
2169:
2118:
2114:
2089:
2085:
2077:
2028:
2025:
2022:
2014:
2010:
1959:
1955:
1905:
1902:
1897:
1893:
1886:
1868:
1864:
1850:
1843:
1836:
1832:
1783:
1779:
1728:
1724:
1675:
1671:
1616:
1609:
1560:
1556:
1547:
1545:
1544:on 1 March 2012
1532:
1531:
1527:
1512:
1511:
1507:
1486:
1482:
1423:
1416:
1392:10.1.1.337.1073
1357:
1350:
1340:
1338:
1330:
1329:
1325:
1274:
1261:
1256:
1208:
1188:plate tectonics
1176:
1166:
1157:
1116:
1088:
1071:plate tectonics
1067:
1036:
1031:
973:
968:
966:Characteristics
921:
915:
913:In Solar system
899:
879:
867:
859:
856:
846:
823:
781:that is in the
731:
725:
676:habitable zones
668:
661:
658:
650:
647:
638:
610:William Borucki
593:similar to the
567:
547:
459:
416:
366:
343:radial velocity
316:
296:
291:
278:
230:
160:
143:
91:
28:
17:
12:
11:
5:
6196:
6186:
6185:
6180:
6175:
6160:
6159:
6147:
6135:
6123:
6111:
6088:
6087:
6085:
6084:
6079:
6073:
6070:
6069:
6067:
6066:
6061:
6056:
6051:
6046:
6041:
6036:
6031:
6026:
6021:
6016:
6011:
6005:
6003:
5999:
5998:
5996:
5995:
5994:
5993:
5988:
5983:
5978:
5973:
5968:
5963:
5958:
5953:
5948:
5943:
5938:
5933:
5928:
5923:
5918:
5913:
5904:
5903:
5902:
5901:
5896:
5891:
5886:
5885:
5884:
5879:
5874:
5869:
5859:
5854:
5849:
5844:
5839:
5834:
5829:
5818:
5817:
5816:
5815:
5810:
5805:
5796:
5794:
5788:
5787:
5785:
5784:
5779:
5774:
5769:
5764:
5759:
5753:
5751:
5747:
5746:
5744:
5743:
5738:
5733:
5728:
5723:
5718:
5713:
5708:
5703:
5698:
5693:
5688:
5683:
5678:
5673:
5668:
5663:
5657:
5655:
5649:
5648:
5646:
5645:
5640:
5639:
5638:
5631:Transit method
5628:
5627:
5626:
5616:
5615:
5614:
5604:
5599:
5598:
5597:
5587:
5586:
5585:
5578:Direct imaging
5575:
5569:
5567:
5561:
5560:
5558:
5557:
5552:
5547:
5542:
5537:
5532:
5527:
5522:
5517:
5512:
5507:
5502:
5497:
5492:
5487:
5482:
5476:
5474:
5468:
5467:
5465:
5464:
5463:
5462:
5457:
5452:
5447:
5439:
5434:
5433:
5432:
5422:
5421:
5420:
5409:
5407:
5401:
5400:
5398:
5397:
5395:Star formation
5392:
5390:Scattered disc
5387:
5382:
5377:
5372:
5367:
5362:
5357:
5352:
5347:
5342:
5337:
5332:
5327:
5322:
5317:
5312:
5307:
5302:
5297:
5292:
5287:
5282:
5277:
5272:
5267:
5262:
5257:
5252:
5247:
5242:
5240:Excretion disk
5237:
5232:
5227:
5222:
5217:
5212:
5207:
5202:
5197:
5195:Accretion disk
5192:
5186:
5184:
5174:
5173:
5170:
5169:
5167:
5166:
5161:
5156:
5151:
5146:
5141:
5136:
5131:
5126:
5121:
5116:
5111:
5106:
5104:Eyeball planet
5101:
5096:
5091:
5086:
5081:
5076:
5071:
5066:
5060:
5058:
5054:
5053:
5051:
5050:
5045:
5040:
5035:
5030:
5025:
5020:
5015:
5010:
5005:
5000:
4994:
4988:
4986:
4980:
4979:
4977:
4976:
4971:
4966:
4961:
4956:
4951:
4945:
4940:
4935:
4930:
4925:
4920:
4914:
4912:
4903:
4893:
4892:
4885:
4883:
4881:
4880:
4875:
4870:
4865:
4860:
4854:
4852:
4848:
4847:
4845:
4844:
4839:
4838:
4837:
4836:
4835:
4819:
4816:
4815:
4810:
4809:
4802:
4795:
4787:
4781:
4780:
4775:
4761:
4760:External links
4758:
4755:
4754:
4742:
4730:
4718:
4680:
4645:
4592:
4577:
4533:
4518:
4483:
4468:
4409:
4394:
4391:on 4 May 2012.
4369:
4322:
4297:
4280:
4267:
4254:
4241:
4228:
4215:
4151:
4138:
4119:
4106:10.1086/669163
4098:10.1086/669163
4058:
4047:
4022:
3997:
3938:
3919:
3893:
3832:
3820:
3794:
3768:
3745:
3683:
3664:
3603:
3590:New York Times
3572:
3544:
3516:
3505:. 30 July 2015
3488:
3477:. 30 July 2015
3460:
3432:
3378:
3325:
3322:Indian Express
3314:
3288:
3259:
3225:
3198:
3173:
3120:
3099:
3078:
3046:
3025:
2972:
2950:
2922:
2884:
2875:|journal=
2826:
2770:
2759:on 10 May 2012
2747:"Star: Gl 581"
2738:
2701:(1): 954–965.
2683:
2680:
2669:
2651:
2623:
2561:
2536:
2506:
2484:
2429:
2406:
2369:(1): L30–L33.
2351:
2321:
2268:
2247:(1): 303–319.
2225:
2195:
2184:. 16 June 2008
2167:
2154:10.1086/589940
2130:(1): 663–683.
2112:
2083:
2039:(3): L43–L47.
2023:
2020:
2008:
1995:10.1086/497094
1971:(1): L85–L88.
1953:
1940:10.1086/491669
1916:(1): 625–640.
1903:
1900:
1891:
1885:978-0521897846
1884:
1862:
1841:
1830:
1817:10.1086/521346
1777:
1764:10.1086/521346
1722:
1669:
1607:
1554:
1525:
1505:
1502:on 2015-11-06.
1480:
1414:
1401:10.1086/512120
1348:
1323:
1310:10.1086/509800
1286:(1): 545–551.
1258:
1257:
1255:
1252:
1251:
1250:
1244:
1238:
1233:
1227:
1221:
1215:
1207:
1204:
1194:and hence the
1165:
1162:
1156:
1155:Magnetic field
1153:
1115:
1112:
1087:
1084:
1066:
1063:
1034:
1029:
1007:transit method
1003:Diana Valencia
972:
969:
967:
964:
917:Main article:
914:
911:
907:habitable zone
898:
895:
891:habitable zone
878:
875:
866:
863:
857:
854:
845:
842:
822:
819:
783:habitable zone
724:
721:
713:habitable zone
667:
664:
659:
656:
648:
645:
637:
634:
599:habitable zone
566:
563:
559:habitable zone
546:
543:
471:habitable zone
458:
455:
415:
412:
405:GJ 1214 b
365:
362:
345:method by the
315:
312:
295:
292:
290:
289:Others by year
287:
276:
260:comparable to
242:habitable zone
229:
226:
206:Eugenio Rivera
159:
156:
142:
139:
90:
87:
15:
9:
6:
4:
3:
2:
6195:
6184:
6181:
6179:
6176:
6174:
6171:
6170:
6168:
6158:
6148:
6146:
6136:
6134:
6124:
6122:
6117:
6112:
6110:
6100:
6099:
6096:
6083:
6080:
6078:
6075:
6074:
6071:
6065:
6062:
6060:
6057:
6055:
6052:
6050:
6047:
6045:
6042:
6040:
6037:
6035:
6032:
6030:
6027:
6025:
6022:
6020:
6017:
6015:
6012:
6010:
6007:
6006:
6004:
6000:
5992:
5989:
5987:
5984:
5982:
5979:
5977:
5974:
5972:
5969:
5967:
5964:
5962:
5959:
5957:
5954:
5952:
5949:
5947:
5944:
5942:
5939:
5937:
5934:
5932:
5929:
5927:
5924:
5922:
5919:
5917:
5914:
5912:
5909:
5908:
5906:
5905:
5900:
5897:
5895:
5892:
5890:
5887:
5883:
5880:
5878:
5875:
5873:
5870:
5868:
5865:
5864:
5863:
5860:
5858:
5855:
5853:
5850:
5848:
5845:
5843:
5840:
5838:
5835:
5833:
5830:
5828:
5825:
5824:
5823:
5820:
5819:
5814:
5811:
5809:
5806:
5804:
5801:
5800:
5798:
5797:
5795:
5793:
5789:
5783:
5780:
5778:
5775:
5773:
5770:
5768:
5765:
5763:
5760:
5758:
5755:
5754:
5752:
5748:
5742:
5739:
5737:
5734:
5732:
5729:
5727:
5724:
5722:
5719:
5717:
5714:
5712:
5709:
5707:
5704:
5702:
5699:
5697:
5694:
5692:
5689:
5687:
5684:
5682:
5679:
5677:
5674:
5672:
5669:
5667:
5664:
5662:
5659:
5658:
5656:
5654:
5650:
5644:
5641:
5637:
5634:
5633:
5632:
5629:
5625:
5622:
5621:
5620:
5617:
5613:
5610:
5609:
5608:
5605:
5603:
5600:
5596:
5593:
5592:
5591:
5588:
5584:
5581:
5580:
5579:
5576:
5574:
5571:
5570:
5568:
5566:
5562:
5556:
5555:Yellow giants
5553:
5551:
5548:
5546:
5543:
5541:
5538:
5536:
5533:
5531:
5528:
5526:
5523:
5521:
5518:
5516:
5513:
5511:
5508:
5506:
5503:
5501:
5498:
5496:
5493:
5491:
5488:
5486:
5483:
5481:
5478:
5477:
5475:
5473:
5469:
5461:
5458:
5456:
5453:
5451:
5448:
5446:
5443:
5442:
5440:
5438:
5435:
5431:
5428:
5427:
5426:
5423:
5419:
5416:
5415:
5414:
5411:
5410:
5408:
5406:
5402:
5396:
5393:
5391:
5388:
5386:
5383:
5381:
5378:
5376:
5373:
5371:
5368:
5366:
5363:
5361:
5358:
5356:
5353:
5351:
5348:
5346:
5343:
5341:
5338:
5336:
5333:
5331:
5328:
5326:
5325:Merging stars
5323:
5321:
5318:
5316:
5313:
5311:
5308:
5306:
5303:
5301:
5298:
5296:
5293:
5291:
5288:
5286:
5283:
5281:
5278:
5276:
5273:
5271:
5268:
5266:
5263:
5261:
5258:
5256:
5253:
5251:
5248:
5246:
5243:
5241:
5238:
5236:
5233:
5231:
5228:
5226:
5223:
5221:
5218:
5216:
5213:
5211:
5208:
5206:
5203:
5201:
5200:Asteroid belt
5198:
5196:
5193:
5191:
5188:
5187:
5185:
5183:
5175:
5165:
5162:
5160:
5157:
5155:
5152:
5150:
5147:
5145:
5142:
5140:
5139:Pulsar planet
5137:
5135:
5132:
5130:
5127:
5125:
5122:
5120:
5117:
5115:
5112:
5110:
5107:
5105:
5102:
5100:
5097:
5095:
5094:Double planet
5092:
5090:
5087:
5085:
5082:
5080:
5077:
5075:
5072:
5070:
5067:
5065:
5062:
5061:
5059:
5055:
5049:
5046:
5044:
5041:
5039:
5036:
5034:
5033:Super-Neptune
5031:
5029:
5028:Super-Jupiter
5026:
5024:
5021:
5019:
5016:
5014:
5011:
5009:
5006:
5004:
5003:Helium planet
5001:
4998:
4995:
4993:
4990:
4989:
4987:
4985:
4981:
4975:
4972:
4970:
4967:
4965:
4962:
4960:
4957:
4955:
4952:
4949:
4946:
4944:
4941:
4939:
4938:Hycean planet
4936:
4934:
4931:
4929:
4928:Desert planet
4926:
4924:
4921:
4919:
4918:Carbon planet
4916:
4915:
4913:
4911:
4907:
4904:
4902:
4894:
4889:
4879:
4876:
4874:
4871:
4869:
4866:
4864:
4861:
4859:
4856:
4855:
4853:
4849:
4843:
4840:
4834:
4831:
4830:
4829:
4826:
4825:
4824:
4821:
4820:
4817:
4808:
4803:
4801:
4796:
4794:
4789:
4788:
4785:
4779:
4776:
4773:
4768:
4764:
4763:
4751:
4746:
4739:
4734:
4727:
4722:
4708:on 2018-08-26
4704:
4700:
4693:
4687:
4685:
4670:on 2018-08-26
4666:
4662:
4655:
4649:
4641:
4637:
4633:
4629:
4625:
4621:
4616:
4611:
4607:
4603:
4596:
4588:
4584:
4580:
4574:
4570:
4566:
4562:
4558:
4553:
4548:
4544:
4537:
4530:
4529:
4522:
4514:
4508:
4493:
4487:
4480:
4479:
4472:
4464:
4460:
4455:
4450:
4446:
4442:
4437:
4432:
4428:
4424:
4420:
4413:
4405:
4398:
4390:
4386:
4385:
4380:
4373:
4365:
4361:
4357:
4353:
4349:
4345:
4341:
4337:
4333:
4326:
4311:
4307:
4301:
4293:
4292:
4284:
4277:
4271:
4264:
4258:
4251:
4245:
4238:
4232:
4225:
4219:
4211:
4207:
4202:
4197:
4193:
4189:
4184:
4179:
4175:
4171:
4167:
4160:
4158:
4156:
4148:
4142:
4135:
4134:
4129:
4123:
4115:
4111:
4107:
4103:
4099:
4095:
4091:
4087:
4082:
4077:
4073:
4069:
4062:
4056:
4051:
4036:
4032:
4026:
4012:
4008:
4001:
3993:
3989:
3984:
3979:
3975:
3971:
3966:
3961:
3957:
3953:
3949:
3942:
3935:
3931:
3928:
3923:
3907:
3903:
3897:
3889:
3885:
3880:
3875:
3871:
3867:
3862:
3857:
3853:
3849:
3848:
3843:
3836:
3829:
3824:
3808:
3804:
3798:
3782:
3778:
3772:
3756:
3749:
3741:
3737:
3732:
3727:
3723:
3719:
3714:
3709:
3705:
3701:
3697:
3690:
3688:
3679:
3675:
3668:
3660:
3656:
3651:
3646:
3642:
3638:
3633:
3628:
3624:
3620:
3619:
3614:
3607:
3592:
3591:
3586:
3579:
3577:
3561:
3560:
3555:
3548:
3533:
3532:
3527:
3520:
3504:
3503:
3498:
3492:
3476:
3475:
3470:
3464:
3449:
3448:
3443:
3436:
3429:
3425:
3420:
3415:
3411:
3407:
3402:
3397:
3393:
3389:
3382:
3374:
3370:
3366:
3362:
3358:
3354:
3349:
3344:
3340:
3336:
3329:
3323:
3318:
3303:
3299:
3292:
3277:
3273:
3266:
3264:
3247:
3243:
3239:
3232:
3230:
3213:
3209:
3202:
3188:
3184:
3177:
3169:
3165:
3161:
3157:
3153:
3149:
3144:
3139:
3135:
3131:
3124:
3109:
3103:
3094:
3089:
3082:
3066:
3062:
3061:
3056:
3050:
3041:
3036:
3029:
3021:
3017:
3013:
3009:
3005:
3001:
2996:
2991:
2987:
2983:
2976:
2961:
2954:
2939:
2938:
2933:
2926:
2910:
2906:
2902:
2900:
2895:
2888:
2880:
2867:
2859:
2855:
2851:
2847:
2842:
2837:
2830:
2822:
2818:
2814:
2810:
2806:
2802:
2797:
2792:
2788:
2784:
2777:
2775:
2758:
2754:
2753:
2748:
2742:
2734:
2730:
2726:
2722:
2718:
2714:
2709:
2704:
2700:
2696:
2695:
2687:
2673:
2665:
2661:
2655:
2640:
2639:
2634:
2627:
2619:
2615:
2611:
2607:
2603:
2599:
2594:
2589:
2585:
2581:
2580:
2572:
2565:
2550:
2546:
2540:
2524:
2520:
2516:
2510:
2494:
2488:
2480:
2476:
2472:
2468:
2464:
2460:
2455:
2450:
2446:
2442:
2441:
2433:
2417:
2410:
2402:
2398:
2394:
2390:
2386:
2382:
2377:
2372:
2368:
2364:
2363:
2355:
2339:
2335:
2331:
2325:
2317:
2313:
2309:
2305:
2301:
2297:
2292:
2287:
2283:
2279:
2272:
2263:
2258:
2254:
2250:
2246:
2242:
2241:
2236:
2229:
2213:
2209:
2205:
2199:
2183:
2182:
2177:
2171:
2163:
2159:
2155:
2151:
2147:
2143:
2138:
2133:
2129:
2125:
2124:
2116:
2108:
2104:
2100:
2096:
2095:
2087:
2076:
2072:
2068:
2064:
2060:
2056:
2052:
2047:
2042:
2038:
2034:
2027:
2012:
2004:
2000:
1996:
1992:
1988:
1984:
1979:
1974:
1970:
1966:
1965:
1957:
1949:
1945:
1941:
1937:
1933:
1929:
1924:
1919:
1915:
1911:
1910:
1895:
1887:
1881:
1877:
1873:
1866:
1860:
1855:
1848:
1846:
1839:
1834:
1826:
1822:
1818:
1814:
1810:
1806:
1801:
1796:
1792:
1788:
1781:
1773:
1769:
1765:
1761:
1757:
1753:
1748:
1743:
1739:
1735:
1734:
1726:
1718:
1714:
1710:
1706:
1702:
1698:
1693:
1688:
1684:
1680:
1673:
1665:
1661:
1656:
1651:
1647:
1643:
1638:
1633:
1629:
1625:
1621:
1614:
1612:
1603:
1599:
1595:
1591:
1587:
1583:
1578:
1573:
1569:
1565:
1558:
1543:
1539:
1535:
1529:
1521:
1520:
1519:New Scientist
1515:
1509:
1501:
1497:
1496:
1491:
1484:
1476:
1472:
1468:
1464:
1460:
1456:
1452:
1448:
1443:
1438:
1434:
1430:
1429:
1421:
1419:
1410:
1406:
1402:
1398:
1393:
1388:
1384:
1380:
1375:
1370:
1366:
1362:
1355:
1353:
1337:
1333:
1327:
1319:
1315:
1311:
1307:
1303:
1299:
1294:
1289:
1285:
1281:
1280:
1272:
1270:
1268:
1266:
1264:
1259:
1248:
1245:
1242:
1239:
1237:
1234:
1231:
1230:Super-Neptune
1228:
1225:
1222:
1219:
1216:
1213:
1210:
1209:
1203:
1201:
1197:
1193:
1189:
1185:
1181:
1175:
1171:
1161:
1152:
1150:
1146:
1142:
1137:
1133:
1129:
1125:
1121:
1111:
1109:
1103:
1101:
1097:
1092:
1083:
1081:
1077:
1072:
1062:
1060:
1056:
1052:
1047:
1045:
1039:
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956:planetesimals
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57:is a type of
56:
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26:
25:Helldivers II
22:
6173:Super-Earths
6157:Solar System
5899:Proper names
5676:Earth analog
5661:Astrobiology
5653:Habitability
5590:Microlensing
5550:White dwarfs
5520:M/Red dwarfs
5510:Herbig Ae/Be
5495:Brown dwarfs
5437:Rogue planet
5418:Interstellar
5360:Planetesimal
5129:Planetesimal
5109:Giant planet
5099:Ecumenopolis
4997:Mini-Neptune
4973:
4933:Dwarf planet
4772:Super-Earths
4745:
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4721:
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4703:the original
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4665:the original
4648:
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1493:
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1432:
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1360:
1339:. Retrieved
1335:
1326:
1283:
1277:
1212:Earth analog
1192:carbon cycle
1184:biodiversity
1177:
1174:astrobiology
1164:Habitability
1158:
1117:
1114:Temperatures
1104:
1093:
1089:
1068:
1048:
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999:Gliese 876 d
982:
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925:Solar System
922:
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555:Gliese 163 c
548:
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480:
475:Seth Shostak
460:
440:
428:Earth masses
424:minimum mass
417:
409:
402:
393:minimum mass
386:
367:
355:
332:
317:
297:
268:like Venus.
231:
214:Gliese 876 d
199:
187:PSR B1257+12
177:
110:Earth masses
103:
79:habitability
55:super-terran
54:
50:
48:
6145:Outer space
6133:Spaceflight
5911:before 2000
5827:Discoveries
5602:Polarimetry
5490:Binary star
5380:Rubble pile
5375:Ring system
5345:Outer space
5315:Kuiper belt
5270:Hills cloud
5225:Debris disk
5220:Cosmic dust
5149:Sub-Neptune
5134:Protoplanet
5069:Brown dwarf
5057:Other types
5013:Hot Neptune
5008:Hot Jupiter
4999:(Gas dwarf)
4974:Super-Earth
4959:Ocean world
4954:Lava planet
4948:Iron planet
4910:Terrestrial
4851:Main topics
4699:Caltech Edu
4661:Caltech Edu
3706:(2): 2411.
3565:17 February
3113:18 February
1336:www.eso.org
1224:Hot Neptune
1200:cosmic rays
1141:Bond albedo
1014:between 1.9
941:Planet Nine
919:Planet Nine
776:Earth-sized
759:55 Cancri e
751:water vapor
717:HD 219134 b
692:Kepler-440b
688:Kepler-442b
684:Kepler-438b
630:Gliese 667C
521:55 Cancri e
513:55 Cancri e
465:released a
447:Gliese 581g
389:Gliese 581e
384:or larger.
328:brown dwarf
246:Gliese 581c
191:Poltergeist
182:around the
131:mega-Earths
51:Super-Earth
6167:Categories
5822:Exoplanets
5803:Host stars
5750:Catalogues
5573:Astrometry
5535:Subdwarf B
5472:Host stars
5445:Retrograde
5340:Oort cloud
5178:Formation
5114:Mesoplanet
5038:Super-puff
4964:Mega-Earth
4943:Ice planet
4828:Definition
4813:Exoplanets
4712:2018-01-13
4674:2018-01-13
4552:1806.05649
4498:2009-04-25
4316:2012-04-28
4183:1606.08088
4041:2012-04-28
4016:2024-09-04
3965:1603.08614
3912:8 February
3861:1601.05438
3813:6 February
3713:1807.07098
3632:1801.03502
3625:(3): 107.
3401:1707.06192
3341:(2): 154.
3192:2012-01-21
3136:(1): L18.
2966:2011-02-19
2943:3 February
2555:2010-08-24
1637:1703.10375
1630:(3): 109.
1548:2012-04-28
1254:References
1247:TOI-1452 b
937:ice giants
933:gas giants
838:40 Eridani
755:atmosphere
749:), but no
653:mega-Earth
642:Kepler-10c
622:Kepler-62f
618:Kepler-62e
603:alien life
579:KOI-172.02
577:(formerly
575:Kepler-69c
551:Gliese 163
494:Kepler-22b
483:HD 85512 b
308:HD 69830 b
250:Gliese 581
210:Gliese 876
180:Dale Frail
151:Kepler-10b
89:Definition
67:ice giants
21:Helldivers
6109:Astronomy
5916:2000–2009
5882:1501–2000
5877:1001–1500
5565:Detection
5530:Red giant
5190:Accretion
5182:evolution
5023:Ice giant
5018:Gas giant
4969:Sub-Earth
4858:Exoplanet
4640:118522228
4615:1310.2211
4608:(1): 77.
4587:116913980
4436:1210.0793
4364:0012-821X
4210:119203398
4081:1301.0818
3992:119114880
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3854:(2): 22.
3787:10 August
3596:24 August
3453:6 January
3428:119243418
3348:1405.7881
3307:9 January
3302:Space.com
3276:Space.com
3187:Space.com
3143:1104.5230
3093:1109.2497
3040:1108.3561
2995:1108.3447
2841:1006.2799
2796:1102.0541
2789:(1): 19.
2708:1009.5733
2644:2 October
2593:1411.7048
2529:7 January
2454:0912.3243
2376:0906.1785
2291:0901.4394
2137:0806.0025
2071:119144195
2046:0704.3841
1800:0707.2895
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1664:119339237
1577:1301.0842
1570:(2): 81.
1442:0912.3229
1387:CiteSeerX
1241:Sub-Earth
1151:) Earth.
1096:GJ 1214 b
1086:Evolution
1024:Kepler-11
994:gas dwarf
952:asteroids
817:project.
805:Proxima b
787:red dwarf
779:exoplanet
771:Proxima b
763:exoplanet
753:, in the
705:HD 219134
672:exoplanet
614:Kepler-62
587:exoplanet
528:Kepler-20
374:HD 7924 b
358:HD 181433
252:of 0.073
218:red dwarf
166:Sizes of
99:LHS 1140b
59:exoplanet
5872:501–1000
5852:Heaviest
5832:Extremes
5540:Subgiant
5413:Exocomet
4507:cite web
4463:55890198
4114:51914911
4011:phys.org
3930:Archived
3740:54871108
3659:54869937
3559:Phys.org
3373:53475787
3168:16768578
3020:15088852
2821:15233153
2763:28 April
2618:73558341
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2479:15288792
2401:16695095
2218:28 April
2181:BBC News
2162:14467194
2003:16632198
1948:14122053
1717:15233153
1602:28106368
1467:20016595
1341:19 April
1318:17656317
1206:See also
1053:and the
883:Ross 508
871:G 9-40 b
850:GJ 357 d
810:StarChip
739:hydrogen
436:HD 10180
426:of 4.15
370:COROT-7b
335:HD 40307
195:Phobetor
36:CoRoT-7b
6095:Portals
5847:Largest
5842:Nearest
5545:T Tauri
5441:Orbits
5425:Exomoon
5405:Systems
5119:Planemo
4984:Gaseous
4620:Bibcode
4557:Bibcode
4441:Bibcode
4344:Bibcode
4188:Bibcode
4086:Bibcode
3970:Bibcode
3888:2701020
3866:Bibcode
3761:Sep 20,
3718:Bibcode
3637:Bibcode
3537:31 July
3509:30 July
3481:30 July
3406:Bibcode
3353:Bibcode
3148:Bibcode
3000:Bibcode
2988:: A58.
2915:9 March
2801:Bibcode
2733:3163906
2713:Bibcode
2598:Bibcode
2459:Bibcode
2381:Bibcode
2344:15 July
2316:1415310
2296:Bibcode
2249:Bibcode
2142:Bibcode
2103:Bibcode
2101:: 529.
2051:Bibcode
1983:Bibcode
1928:Bibcode
1859:YouTube
1825:8369390
1805:Bibcode
1772:8369390
1752:Bibcode
1697:Bibcode
1642:Bibcode
1582:Bibcode
1475:4360404
1447:Bibcode
1409:3039909
1379:Bibcode
1298:Bibcode
1196:climate
1143:0.90,
1012:gravity
960:Mercury
831:K2-155d
785:of the
597:in the
533:Planet
422:with a
391:with a
382:G class
368:Planet
75:Neptune
44:Neptune
5862:Kepler
5837:Firsts
5736:Tholin
5607:Timing
5525:Pulsar
5450:Trojan
5064:Blanet
4823:Planet
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1120:albedo
743:helium
732:'s
585:-like
581:), an
306:, and
258:albedo
222:kelvin
184:pulsar
114:Uranus
106:masses
71:Uranus
6121:Stars
6002:Other
5867:1–500
5792:Lists
4901:types
4896:Sizes
4706:(PDF)
4695:(PDF)
4668:(PDF)
4657:(PDF)
4636:S2CID
4610:arXiv
4583:S2CID
4547:arXiv
4459:S2CID
4431:arXiv
4206:S2CID
4178:arXiv
4110:S2CID
4102:JSTOR
4076:arXiv
3988:S2CID
3960:arXiv
3884:S2CID
3856:arXiv
3736:S2CID
3708:arXiv
3655:S2CID
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3424:S2CID
3396:arXiv
3369:S2CID
3343:arXiv
3164:S2CID
3138:arXiv
3088:arXiv
3035:arXiv
3016:S2CID
2990:arXiv
2858:93116
2854:S2CID
2836:arXiv
2817:S2CID
2791:arXiv
2729:S2CID
2703:arXiv
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2475:S2CID
2449:arXiv
2418:. CNN
2397:S2CID
2371:arXiv
2312:S2CID
2286:arXiv
2158:S2CID
2132:arXiv
2078:(PDF)
2067:S2CID
2041:arXiv
2029:(PDF)
1999:S2CID
1973:arXiv
1944:S2CID
1918:arXiv
1821:S2CID
1795:arXiv
1768:S2CID
1742:arXiv
1713:S2CID
1687:arXiv
1660:S2CID
1632:arXiv
1598:S2CID
1572:arXiv
1471:S2CID
1437:arXiv
1405:S2CID
1369:arXiv
1314:S2CID
1288:arXiv
1080:magma
1055:OMEGA
801:Earth
774:, an
680:stars
583:Earth
351:Chile
347:HARPS
262:Venus
158:First
133:, or
63:Earth
40:Earth
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5986:2023
5981:2022
5976:2021
5971:2020
5966:2019
5961:2018
5956:2017
5951:2016
5946:2015
5941:2014
5936:2013
5931:2012
5926:2011
5921:2010
5636:list
5624:list
5612:list
5595:list
5583:list
5180:and
4898:and
4573:ISBN
4513:link
4360:ISSN
3914:2016
3815:2024
3807:NASA
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3539:2015
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3511:2015
3502:NASA
3483:2015
3455:2015
3447:NASA
3309:2013
3283:2012
3254:2012
3220:2012
3115:2016
3073:2011
2945:2011
2917:2011
2879:help
2765:2012
2646:2010
2531:2010
2501:2010
2424:2010
2346:2009
2220:2012
2190:2010
1880:ISBN
1463:PMID
1343:2017
1172:and
1122:and
923:The
903:NASA
897:2024
877:2022
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844:2019
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790:star
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686:and
666:2015
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620:and
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545:2012
457:2011
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