442:
29:
392:, a large collection of scattered stars that also share a similar trajectory with the Hyades Cluster. Recent results have found that at least 15% of stars in the Hyades Stream share the same chemical fingerprint as the Hyades cluster stars. However, about 85% of stars in the Hyades Stream have been shown to be completely unrelated to the original cluster on the grounds of dissimilar age and metallicity; their common motion is attributed to tidal effects of the massive rotating
430:
4335:
4355:
762:
4345:
4381:
4405:
4393:
744:. Although the exact ratio of single to multiple systems in the cluster remains uncertain, this ratio has considerable implications for our understanding of its population. For example, Perryman and colleagues list about 200 high-probability Hyades members. If the binary fraction is 50%, the total cluster population would be at least 300 individual stars.
714:. This tight concentration of heavy stars gives the Hyades its overall structure, with a core defined by bright, closely packed systems and a halo consisting of more widely separated stars in which later spectral types are common. The core radius is 2.7 parsecs (8.8 light-years, a little more than the distance between the Sun and
673:
of spectral types M0-M2. Additional M dwarfs have been proposed in the past. This deficiency at the bottom of the mass range contrasts strongly with the distribution of stars within 10 parsecs of the Solar System, where at least 239 M dwarfs are known, comprising about 76% of all neighborhood stars.
467:
Another DR2 study from 2019 focused on mapping the 3D Topology & Velocities of the Hyades main body out to 30 parsecs, and included Sub-Stellar members as well. They identified 1764 member candidates, including 10 Brown Dwarfs and 17 White Dwarfs. The White Dwarfs included 9 single stars, and 4
360:
for stars of their type, and use the resulting data to infer their intrinsic brightness. Comparing this data to the brightness of the stars as seen from Earth allows their distances to be estimated. Both methods have yielded a distance estimate of 153 light-years (47 parsecs) to the cluster center.
752:
Surveys indicate that 90% of open clusters dissolve less than 1 billion years after formation, while only a tiny fraction survive for the present age of the Solar System (about 4.6 billion years). Over the next few hundred million years, the Hyades will continue to lose both mass and membership as
721:
Stellar evaporation occurs in the cluster halo as smaller stars are scattered outward by more massive insiders. From the halo they may then be lost to tides exerted by the
Galactic core or to shocks generated by collisions with drifting hydrogen clouds. In this way the Hyades probably lost much of
576:
reported almost 25 years of observations to support this premise, arguing for the existence of a co-moving group of stars that he called the Taurus Stream (now generally known as the Hyades Stream or Hyades
Supercluster). Boss published a chart that traced the scattered stars' movements back to a
2467:
Schneider, Adam C.; Vrba, Frederick J.; Munn, Jeffrey A.; Dahm, Scott E.; Bruursema, Justice; Williams, Stephen J.; Dorland, Bryan N.; Faherty, Jacqueline K.; Rothermich, Austin; Calamari, Emily; Cushing, Michael C.; Caselden, Dan; Kabatnik, Martin; Pendrill, William; Sainio, Arttu (2022-05-01).
580:
By the 1920s, the notion that the Hyades shared a common origin with the
Praesepe Cluster was widespread, with Rudolf Klein-Wassink noting in 1927 that the two clusters are "probably cosmically related". For much of the twentieth century, scientific study of the Hyades focused on determining its
664:
The remaining population of confirmed cluster members includes numerous bright stars of spectral types A (at least 21), F (about 60), and G (about 50). All these star types are concentrated much more densely within the tidal radius of the Hyades than within an equivalent 10-parsec radius of the
718:), while the half-mass radius, within which half the cluster's mass is contained, is 5.7 parsecs (19 light-years). The tidal radius of ten parsecs (33 light-years) represents the Hyades' average outer limit, beyond which a star is unlikely to remain gravitationally bound to the cluster core.
753:
its brightest stars evolve off the main sequence and its dimmest stars evaporate out of the cluster halo. It may eventually be reduced to a remnant containing about a dozen star systems, most of them binary or multiple, which will remain vulnerable to ongoing dissipative forces.
2854:
Kuzuhara, Masayuki; Currie, Thayne; Takarada, Takuya; Brandt, Timothy D.; Sato, Bun'ei; Uyama, Taichi; Janson, Markus; Chilcote, Jeffrey; Tobin, Taylor; Lawson, Kellen; Hori, Yasunori; Guyon, Olivier; Groff, Tyler D.; Lozi, Julien; Vievard, Sebastien (2022-08-01).
335:
galaxy – is 33 light-years (10 parsecs). However, about one-third of confirmed member stars have been observed well outside the latter boundary, in the cluster's extended halo; these stars are probably in the process of escaping from its gravitational influence.
635:, while less massive stars continue fusing hydrogen on the main sequence. Extensive surveys have revealed a total of 8 white dwarfs in the cluster core, corresponding to the final evolutionary stage of its original population of B-type stars (each about 3
730:
Another result of mass segregation is the concentration of binary systems in the cluster core. More than half of the known F and G stars are binaries, and these are preferentially located within this central region. As in the immediate Solar neighborhood,
735:
increases with increasing stellar mass. The fraction of binary systems in the Hyades increases from 26% among K-type stars to 87% among A-type stars. Hyades binaries tend to have small separations, with most binary pairs in shared orbits whose
28:
1203:
Bouvier J, Kendall T, Meeus G, Testi L, Moraux E, Stauffer JR, James D, Cuillandre J-C, Irwin J, McCaughrean MJ, Baraffe I, Bertin E. (2008) Brown dwarfs and very low mass stars in the Hyades cluster: a dynamically evolved mass function.
2796:
Gaia
Collaboration; Smart, R. L.; Sarro, L. M.; Rybizki, J.; Reylé, C.; Robin, A. C.; Hambly, N. C.; Abbas, U.; Barstow, M. A.; de Bruijne, J. H. J.; Bucciarelli, B.; Carrasco, J. M.; Cooper, W. J.; Hodgkin, S. T.; Masana, E. (2021-05-01).
597:, can avoid evaporation over extended timescales. As one such survivor, the Hyades Cluster probably contained a much larger star population in its infancy. Estimates of its original mass range from 800 to 1,600 times the
668:
The Hyades' cohort of lower-mass stars – spectral types K and M – remains poorly understood, despite proximity and long observation. At least 48 K dwarfs are confirmed members, along with about a dozen
1469:
Vauclair, S.; Laymand, M.; Bouchy, F.; Vauclair, G.; Hui Bon Hoa, A.; Charpinet, S.; Bazot, M. (2008). "The exoplanet-host star iota
Horologii: an evaporated member of the primordial Hyades cluster".
2201:
Johnson JA, Fischer D, Marcy GW, Wright JT, Driscoll P, Butler RP, Hekker S, Reffert S, Vogt SS. (2007a) Retired A stars and their companions: Exoplanets orbiting three intermediate-mass subgiants.
642:). The preceding evolutionary stage is currently represented by the cluster's four red clump giants. Their present spectral type is K0 III, but all are actually "retired A stars" of around 2.5
327:
The age of the Hyades is estimated to be about 625 million years. The core of the cluster, where stars are the most densely packed, has a radius of 8.8 light-years (2.7 parsecs), and the cluster's
461:
A 2018 Gaia DR1 study of the Hyades
Cluster determined a (U, V, W) group velocity of (−41.92 ± 0.16, −19.35 ± 0.13, −1.11 ± 0.11) km/sec, based on the space velocities of the 138 core stars.
267:, it consists of a roughly spherical group of hundreds of stars sharing the same age, place of origin, chemical characteristics, and motion through space. From the perspective of observers on
316:
that is traditionally identified as the head of Taurus the Bull. The fifth of these stars is Theta Tauri, a tight naked-eye companion to the brighter Theta Tauri. Epsilon Tauri, known as
2772:
Schneider, Adam C.; Cushing, Michael C.; Stiller, Robert A.; Munn, Jeffrey A.; Vrba, Frederick J.; Bruursema, Justice; Williams, Stephen J.; Liu, Michael C.; Bravo, Alexia (2024-08-19),
441:
622:. However, studies of the Hyades show that it is deficient in stars at both extremes of mass. At an age of 625 million years, the cluster's main sequence turn-off is about 2.3
471:
A 2022 Hyades study utilizing Gaia EDR3 derived a (U, V, W) group velocity of (-42.11±6.50, - 19.09±4.37, -1.32±0.44) km/sec, also with close agreement to DR1 and DR2 studies.
1722:
Elsanhoury, Waleed; Al-Johani, Amnah; Al-anzi, Aneefah; Al-jaber, Bashayr; Al-Bishi, Fatmah; Kanaan, Nourah; Al-atwi, Ragwa; Al-khubrani, Reem; Al-anzi, Sarah (2022-03-16).
2710:
Schneider, Adam C.; Munn, Jeffrey A.; Vrba, Frederick J.; Bruursema, Justice; Dahm, Scott E.; Williams, Stephen J.; Liu, Michael C.; Dorland, Bryan N. (2023-09-01).
2288:
Endl, M; Cochran, WD; Kurster, M; Paulson, DB; Wittenmyer, RA; MacQueen, PJ; Tull, RG (2006). "Exploring the frequency of close-in Jovian planets around M dwarfs".
557:
did not include the Hyades in his 1781 catalog of deep sky objects. It therefore lacks a
Messier number, unlike many other, more distant open clusters – e.g.,
2219:
Armstrong, JT; Mozurkewich, D; Hajian, AR; et al. (2006). "The Hyades binary Theta2 Tauri: Confronting evolutionary models with optical interferometry".
618:
Theory predicts that a young cluster of this size should give birth to stars and substellar objects of all spectral types, from huge, hot O stars down to dim
3029:
Patience J, Ghez AM, Reid IN, Weinberger AJ, Matthews K. (1998) The multiplicity of the Hyades and its implications for binary star formation and evolution.
589:
All stars form in clusters, but most clusters break up less than 50 million years after star formation concludes. The astronomical term for this process is "
1000:
has a system of three planets. Another star, HD 283869, may also host a planet, but this has not been confirmed as only one transit has been detected.
282:. However, Aldebaran is unrelated to the Hyades, as it is located much closer to Earth (65 ly) and merely happens to lie along the same line of sight.
1313:
572:
In 1869, the astronomer R.A. Proctor observed that numerous stars at large distances from the Hyades share a similar motion through space. In 1908,
3393:
3508:
502:. After the death of their brother, Hyas, the weeping sisters were transformed into a cluster of stars that was afterwards associated with rain.
464:
A 2019 Gaia DR2 study finds a (U, V, W) group velocity of (−42.24, −19.00, −1.48) km/sec, in very close agreement with the 2018 DR1 derivation.
3681:
3676:
3671:
3666:
3656:
3651:
3646:
3641:
1451:
Famaey B, Pont F, Luri X, Udry S, Mayor M, Jorissen A. (2007) The Hyades stream: an evaporated cluster or an intrusion from the inner disk?
388:, and the trajectories of both clusters can be traced back to the same region of space, indicating a common origin. Another associate is the
3714:
3356:
2015:
Weideman V, Jordan S, Iben I, Casertano S. (1992) White dwarfs in the halo of the Hyades
Cluster – The case of the missing white dwarfs.
707:. With the exception of its white dwarfs, the cluster's central two parsecs (6.5 light-years) contain only star systems of at least 1
2857:"Direct-imaging Discovery and Dynamical Mass of a Substellar Companion Orbiting an Accelerating Hyades Sun-like Star with SCExAO/CHARIS"
686:
DR2 allowed the identification of 710 cluster members within 30 parsec, including 23 candidates with estimated masses between 60 and 80
4300:
505:
As a naked-eye object, the Hyades cluster has been known since prehistoric times. It is mentioned by numerous
Classical authors from
3420:
997:
3118:
Quinn, Samuel N.; White, Russel J.; et al. (May 2014). "HD 285507b: An
Eccentric Hot Jupiter in the Hyades Open Cluster".
1516:
542:
In England the cluster was known as the "April Rainers" from an association with April showers, as recorded in the folk song "
4315:
380:
measured at +0.14. The Hyades Cluster is related to other stellar groups in the Sun's vicinity. Its age, metallicity, and
3501:
590:
4348:
3228:"Zodiacal Exoplanets in Time (ZEIT). VI. A Three-planet System in the Hyades Cluster Including an Earth-sized Planet"
3707:
348:
of the member stars as the Earth orbits the Sun. This measurement has been performed with great accuracy using the
344:
The cluster is sufficiently close to the Sun that its distance can be directly measured by observing the amount of
2916:"The Hawaii Infrared Parallax Program. V. New T-dwarf Members and Candidate Members of Nearby Young Moving Groups"
674:
In more recent studies more low-mass members were discovered. This is due targeted searches and an improvement in
581:
distance, modeling its evolution, confirming or rejecting candidate members, and characterizing individual stars.
4435:
3175:"Zodiacal Exoplanets in Time (ZEIT). I. A Neptune-sized Planet Orbiting an M4.5 Dwarf in the Hyades Star Cluster"
2163:"The Hyades binaries Theta1 Tauri and Theta2 Tauri: The distance to the cluster and the mass-luminosity relation"
357:
4425:
3494:
3104:
4310:
429:
1593:
704:
356:. An alternative method of computing the distance is to fit the cluster members to a standardized infrared
3466:
4445:
3700:
3458:
484:
285:
The five brightest member stars of the Hyades have consumed the hydrogen fuel at their cores and are now
3450:
2914:
Zhang, Zhoujian; Liu, Michael C.; Best, William M. J.; Dupuy, Trent J.; Siverd, Robert J. (2021-04-01).
657:
system that includes a less massive companion of spectral type A; this pair is visually associated with
4371:
3462:
3454:
3446:
3442:
550:
499:
448:
3430:
4440:
4338:
3179:
3120:
2974:
2798:
2649:
2406:
2241:
1262:
1036:
665:
Earth. By comparison, our local 10-parsec sphere contains only 4 A stars, 6 F stars, and 21 G stars.
162:
3411:
553:
in 1654, and it subsequently appeared in many star atlases of the 17th and 18th centuries. However,
4204:
3285:
3232:
2341:
Stauffer, JR; Balachandran, SC; Krishnamurthi, A; Pinsonneault, M; Terndrup, DM; Stern, RA (1997).
543:
3383:
3281:"Zodiacal Exoplanets in Time (ZEIT). VII. A Temperate Candidate Super-Earth in the Hyades Cluster"
3089:, A92. In the Vizier catalogue, sort on Vmag using '<4.51'. See also the linked entries in the
1541:
Reino, Stella; de Bruijne, Jos; Zari, Eleonora; d'Antona, Francesca; Ventura, Paolo (2018-03-28).
416:
4430:
4320:
2236:
797:
785:
362:
353:
328:
275:
180:
1180:
1158:
4305:
1723:
1048:
528:
361:
The fact that these independent measurements agree makes the Hyades an important rung on the
192:
3070:
3000:
2824:
2675:
2432:
2384:
Hogan E, Jameson R F, Casewell SL, Osbourne, SL, Hambly NC. (2008) L dwarfs in the Hyades.
1979:
1919:
1684:
1619:
1492:
1137:"Parallaxes and proper motions for 20 open clusters as based on the new Hipparcos catalogue"
1117:
1094:
Perryman, M.A.C.; et al. (1998). "The Hyades: distance, structure, dynamics, and age".
3834:
3517:
3474:
3304:
3251:
3198:
3139:
3066:
2996:
2937:
2878:
2820:
2733:
2671:
2612:
2553:
2491:
2428:
2354:
2307:
2228:
2174:
2113:
2055:
1975:
1927:
1915:
1680:
1615:
1488:
1416:
1332:
1271:
1113:
703:
The observed distribution of stellar types in the Hyades Cluster demonstrates a history of
393:
313:
70:
8:
3764:
3633:
2712:"Astrometry and Photometry for ≈1000 L, T, and Y Dwarfs from the UKIRT Hemisphere Survey"
1775:
158:
3431:
Warburg Institute Iconographic Database (medieval and early modern images of the Hyades)
3417:
3308:
3255:
3202:
3143:
2941:
2882:
2737:
2616:
2557:
2495:
2358:
2311:
2232:
2178:
2117:
2059:
1420:
1336:
1275:
1181:"Astrometry with the Hubble Space Telescope: Trigonometric Parallaxes of Selected Hyads"
4409:
3731:
3723:
3525:
3294:
3241:
3188:
3155:
3129:
3082:
3056:
2986:
2927:
2868:
2810:
2777:
2723:
2661:
2602:
2543:
2481:
2418:
2323:
2297:
2254:
2073:
2045:
1991:
1965:
1931:
1905:
1753:
1704:
1670:
1639:
1605:
1554:
1504:
1478:
1434:
1406:
1350:
1322:
1289:
1103:
1039:
questioned these findings, pointing out minor errors in the paper's astronomical data.
1009:
790:
722:
its original population of M dwarfs, along with substantial numbers of brighter stars.
491:
373:
154:
84:
1879:
Klein-Wassink WJ. (1927) The proper motion and the distance of the Praesepe cluster.
1833:
1456:
1209:
1136:
4354:
4039:
4034:
3333:
3211:
3174:
3159:
3151:
3098:
3086:
3012:
2955:
2896:
2836:
2751:
2687:
2630:
2571:
2509:
2444:
2068:
2033:
1757:
1745:
1708:
1696:
1643:
1631:
1574:
1429:
1394:
1345:
1308:
1293:
769:
This is a list of Hyades cluster member stars that are fourth magnitude or brighter.
741:
683:
495:
294:
286:
40:
3034:
2389:
2327:
2275:
2206:
2145:
2077:
1995:
1935:
1884:
1867:
1850:
1508:
1438:
1354:
331:– where the stars become more strongly influenced by the gravity of the surrounding
4385:
4358:
4249:
3470:
3312:
3259:
3206:
3147:
3074:
3004:
2945:
2886:
2828:
2741:
2679:
2620:
2561:
2499:
2436:
2362:
2315:
2258:
2246:
2182:
2121:
2063:
1983:
1923:
1735:
1688:
1623:
1564:
1520:
1496:
1424:
1340:
1279:
1226:
1179:
McArthur, Barbara E.; Benedict, G. Fritz; Harrison, Thomas E.; van Altena, William
1024:
780:
345:
207:
3078:
3008:
2832:
2683:
2532:"BANYAN. XIII. A First Look at Nearby Young Associations with Gaia Data Release 2"
2440:
1692:
1627:
408:
has recently been proposed as an escaped member of the primordial Hyades Cluster.
4229:
4059:
3869:
3424:
3405:
1987:
1658:
1500:
1013:
737:
594:
558:
554:
48:
4295:
4134:
3979:
3804:
3400:
3317:
3280:
3264:
3227:
2950:
2915:
2891:
2856:
2746:
2711:
2566:
2531:
2504:
2469:
2407:"A new L5 brown dwarf member of the Hyades cluster with chromospheric activity"
1804:
1740:
405:
240:
1159:"Deep Infrared ZAMS Fits to Benchmark Open Clusters Hosting delta Scuti Stars"
4419:
4194:
4009:
3929:
3481:
3016:
2959:
2900:
2840:
2755:
2691:
2634:
2575:
2513:
2448:
2340:
1749:
1700:
1635:
1578:
977:
918:
822:
675:
389:
381:
305:
272:
175:
2625:
2590:
2343:"Rotational velocities and chromospheric activity of M dwarfs in the Hyades"
4397:
4049:
3047:
Röser, S.; et al. (July 2011), "A deep all-sky census of the Hyades",
1569:
1542:
934:
854:
687:
278:, where its brightest stars form a "V" shape along with the still-brighter
260:
256:
188:
144:
4119:
3904:
3899:
3754:
3623:
3618:
3613:
3608:
3603:
3598:
3593:
3588:
3583:
3573:
3568:
3563:
3558:
3553:
3548:
3543:
3538:
3533:
2302:
2050:
1956:
Pavani, DB; Bica, E (2007). "Characterization of open cluster remnants".
1910:
1771:
1395:"High-resolution elemental abundance analysis of the Hyades supercluster"
1327:
1108:
989:
984:
planet, which was the first planet to be discovered in any open cluster.
981:
886:
870:
838:
806:
732:
682:
are currently reported as Hyades members or candidate members. Meanwhile
679:
661:, one of the four red giants, which also has an A-type binary companion.
658:
654:
650:
632:
631:, meaning that all heavier stars have evolved into subgiants, giants, or
619:
377:
309:
301:
297:
60:
3486:
2973:
Lodieu, N.; Smart, R. L.; Pérez-Garrido, A.; Silvotti, R. (2019-03-01).
2648:
Pérez-Garrido, A.; Lodieu, N.; Rebolo, R.; Chinchilla, P. (2018-12-01).
1657:
Lodieu, N.; Smart, R. L.; Pérez-Garrido, A.; Silvotti, R. (2019-02-27).
1032:
678:
searches. About 35 L-type (7+1+8+6+3+4+3+3) and 15 T-type (2+1+3+1+4+4)
4264:
2774:
Eight New Substellar Hyades Candidates from the UKIRT Hemisphere Survey
1256:
Sato, Bun'ei; Izumiura, Hideyuki; Toyota, Eri; et al. (May 2007).
1028:
623:
602:
598:
573:
566:
532:
524:
385:
368:
The stars of the Hyades are more enriched in heavier elements than the
324:
exoplanet candidate, the first planet to be found in any open cluster.
290:
115:
76:
1368:
3692:
1819:
Translated by Richmond Lattimore. University of Chicago Press, 1951.
985:
973:
420:
401:
397:
349:
332:
321:
279:
3357:""Wolf's jaw" star cluster may have inspired parts of Ragnarök myth"
2140:
Böhm-Vitense E. (1995) White dwarf companions to Hyades F stars.
1896:
Lada, CJ; Lada, EA (2003). "Embedded clusters in molecular clouds".
1862:
Hertzsprung E. (1922) On the motions of Praesepe and of the Hyades.
1592:
Röser, Siegfried; Schilbach, Elena; Goldman, Bertrand (2019-01-01).
1309:"New Praesepe white dwarfs and the initial mass-final mass relation"
4279:
4274:
4269:
4259:
4239:
4224:
4219:
4214:
4209:
4199:
4189:
4184:
4179:
4174:
4169:
4164:
4154:
4149:
4144:
4139:
4129:
4124:
4114:
4109:
4104:
4099:
4089:
4079:
4074:
4069:
4064:
4054:
4029:
4024:
4019:
4004:
3999:
3994:
3984:
3974:
3969:
3964:
3959:
3954:
3949:
3944:
3934:
3924:
3919:
3914:
3909:
3894:
3884:
3879:
3864:
3859:
3854:
3844:
3839:
3814:
3809:
3794:
3789:
3769:
3749:
3299:
3246:
3193:
2991:
2932:
2873:
2815:
2795:
2782:
2728:
2666:
2647:
2548:
2486:
2423:
2367:
2342:
2319:
2274:
Research Consortium on Nearby Stars (RECONS). Ten-parsec census at
2250:
2187:
2162:
2126:
2101:
1675:
1610:
1559:
1284:
1257:
950:
902:
562:
536:
520:
480:
412:
3134:
3061:
2607:
1970:
1721:
1483:
1411:
447:
Map of stars within 100 parsecs of the Sun, the Hyades is at 180°
4254:
4244:
4234:
4159:
4084:
4044:
4014:
3989:
3874:
3849:
3829:
3824:
3819:
3799:
3784:
3774:
3739:
3438:
3226:
Mann, Andrew W.; Vanderburg, Andrew; et al. (January 2018).
1017:
670:
411:
The Hyades are unrelated to two other nearby stellar groups, the
3279:
Vanderburg, Andrew; Mann, Andrew W.; et al. (August 2018).
3046:
2972:
2650:"Exploring the substellar population in the Hyades open cluster"
1656:
761:
4094:
3889:
3759:
3744:
3388:
2799:"Gaia Early Data Release 3. The Gaia Catalogue of Nearby Stars"
2470:"Substellar Hyades Candidates from the UKIRT Hemisphere Survey"
1540:
715:
649:. An additional "white giant" of type A7 III is the primary of
1163:
Journal of the American Association of Variable Star Observers
479:
Together with the other eye-catching open star cluster of the
400:
galaxy. Among the remaining members of the Hyades Stream, the
365:
method for estimating the distances of extragalactic objects.
228:
3779:
1881:
Publications of the Kapteyn Astronomical Laboratory Groningen
1468:
1307:
Dobbie, PD; Napiwotzki, R; Burleigh, MR; et al. (2006).
993:
515:
506:
268:
3334:"The Wolf's Jaw: an Astronomical Interpretation of Ragnarök"
3173:
Mann, Andrew W.; Gaidos, Eric; et al. (February 2016).
2975:"A 3D view of the Hyades stellar and sub-stellar population"
2853:
1659:"A 3D view of the Hyades stellar and sub-stellar population"
2771:
510:
263:. Located about 153 light-years (47 parsecs) away from the
222:
216:
4392:
2709:
2589:
Lodieu, N.; Boudreault, S.; Béjar, V. J. S. (2014-12-01).
2218:
1864:
Bulletin of the Astronomical Institutes of the Netherlands
1845:
Boss L. (1908) Convergent of a moving cluster in Taurus.
593:." Only extremely massive clusters, orbiting far from the
2404:
2287:
369:
264:
2405:
Pérez-Garrido, A.; Lodieu, N.; Rebolo, R. (2017-03-01).
1306:
3412:
WEBDA open cluster database website for Hyades cluster
2530:
Gagné, Jonathan; Faherty, Jacqueline K. (2018-08-01).
1828:
Zuckerman B, Song I. (2004) Young stars near the Sun.
1027:
paper suggested that the Hyades may have inspired the
610:), implying still larger numbers of individual stars.
4369:
2588:
2466:
1591:
231:
2160:
225:
2095:
2093:
2091:
2089:
2087:
1834:
http://adsabs.harvard.edu/abs/2004ARA%26A..42..685Z
1457:
http://adsabs.harvard.edu/abs/2007A%26A...461..957F
1258:"A Planetary Companion to the Hyades Giant ɛ Tauri"
1210:
http://adsabs.harvard.edu/abs/2008A%26A...481..661B
487:, which has been known for several thousand years.
384:coincide with those of the larger and more distant
213:
210:
2386:Monthly Notices of the Royal Astronomical Society,
1951:
1949:
1947:
1945:
1255:
3035:http://adsabs.harvard.edu/abs/1998AJ....115.1972P
2913:
2595:Monthly Notices of the Royal Astronomical Society
2390:http://adsabs.harvard.edu/abs/2008MNRAS.388..495H
2276:http://joy.chara.gsu.edu/RECONS/census.posted.htm
2207:http://adsabs.harvard.edu/abs/2007ApJ...665..785J
2146:http://adsabs.harvard.edu/abs/1995AJ....110..228B
2038:Monthly Notices of the Royal Astronomical Society
1885:http://adsabs.harvard.edu/abs/1927PGro...41....1K
1868:http://adsabs.harvard.edu/abs/1922BAN.....1..150H
1851:http://adsabs.harvard.edu/abs/1908AJ.....26...31B
1547:Monthly Notices of the Royal Astronomical Society
1314:Monthly Notices of the Royal Astronomical Society
972:Four stars in the Hyades have been found to host
4417:
2134:
2084:
2011:
2009:
2007:
2005:
1724:"The Hyades Kinematical Structure with Gaia Era"
1093:
3091:All-sky Compiled Catalogue of 2.5 million stars
1942:
3278:
3272:
3225:
1830:Annual Review of Astronomy & Astrophysics.
1157:Majaess, D.; Turner, D.; Lane, D.; Krajci, T.
1131:
1129:
1127:
765:Bright stars in the core of the Hyades Cluster
519:the stars of the Hyades appear along with the
3708:
3502:
3394:Centre de données astronomiques de Strasbourg
2212:
2156:
2154:
2002:
1898:Annual Review of Astronomy & Astrophysics
1873:
549:The cluster was probably first catalogued by
3023:
2591:"Spectroscopy of Hyades L dwarf candidates★"
2529:
2161:Torres, G; Stefanik, RP; Latham, DW (1997).
2099:
1728:Indian Journal of Pure & Applied Physics
1175:
1173:
1171:
2031:
1153:
1151:
1149:
1124:
1089:
1087:
1085:
1083:
584:
219:
4301:Catalogue of Nebulae and Clusters of Stars
3715:
3701:
3509:
3495:
3172:
3117:
2151:
1955:
1856:
1081:
1079:
1077:
1075:
1073:
1071:
1069:
1067:
1065:
1063:
3516:
3354:
3338:Archaeoastronomy and Ancient Technologies
3316:
3298:
3263:
3245:
3210:
3192:
3133:
3111:
3060:
2990:
2949:
2931:
2890:
2872:
2814:
2781:
2745:
2727:
2665:
2624:
2606:
2565:
2547:
2503:
2485:
2422:
2366:
2301:
2270:
2268:
2240:
2186:
2125:
2067:
2049:
2027:
2025:
1969:
1909:
1822:
1809:
1739:
1674:
1609:
1594:"Hyades tidal tails revealed by Gaia DR2"
1568:
1558:
1543:"A Gaia study of the Hyades open cluster"
1514:
1482:
1428:
1410:
1344:
1326:
1283:
1220:
1218:
1199:
1197:
1195:
1193:
1168:
1107:
3418:Distance to the Hyades undergraduate lab
3219:
3166:
2380:
2378:
2334:
1895:
1889:
1462:
1392:
1146:
760:
16:Open cluster in the constellation Taurus
2195:
2034:"On the mass function of star clusters"
1800:
1798:
1796:
1770:
1764:
1060:
725:
4418:
3722:
3331:
2265:
2102:"Hyades morphology and star formation"
2022:
1928:10.1146/annurev.astro.41.011802.094844
1445:
1251:
1249:
1247:
1215:
1190:
1020:is located on a planet in the Hyades.
339:
3696:
3490:
2767:
2765:
2705:
2703:
2701:
2525:
2523:
2462:
2460:
2458:
2400:
2398:
2375:
2019:104: 1876-1891. 1992AJ....104.1876W.
1300:
1224:
4344:
2281:
1866:, Vol. 1, p.150. Full text link at
1839:
1793:
1016:, and others, the fictional city of
271:, the Hyades Cluster appears in the
3401:Information on the Hyades from SEDS
1805:Information on the Hyades from SEDS
1776:"The Hyades – the face of the bull"
1244:
747:
698:
613:
13:
3355:Ouellette, Jennifer (2018-11-16).
2762:
2698:
2520:
2455:
2395:
756:
419:, which are easily visible to the
14:
4457:
3427:– J. Lucey (University of Durham)
3376:
1832:Volume 42, 685-721. Abstract at
1393:De Silva, G; et al. (2011).
4403:
4391:
4379:
4353:
4343:
4334:
4333:
2069:10.1046/j.1365-8711.2002.05848.x
1849:, 26: 31-36. Full text link at
1430:10.1111/j.1365-2966.2011.18728.x
1346:10.1111/j.1365-2966.2006.10311.x
996:has a Neptune-sized planet, and
440:
435:Star chart of the Hyades cluster
428:
372:and other ordinary stars in the
206:
33:Photograph of the Hyades Cluster
27:
3348:
3325:
3040:
2966:
2907:
2847:
2789:
2641:
2582:
1883:, 41: 1-48. Full text link at
1715:
1650:
1585:
1534:
1386:
2388:388 (2) 495-499. Abstract at
1361:
1:
4316:Revised New General Catalogue
3482:Hyades at Constellation Guide
3344:(1) – via ResearchGate.
3033:115: 1972-1988. Abstract at
2032:Kroupa, P; Boily, CM (2002).
1455:, 461: 957-962. Abstract at
1208:, 481: 661-672. Abstract at
1054:
1003:
577:common point of convergence.
456:
3406:Astronomy Picture of the Day
3049:Astronomy & Astrophysics
1958:Astronomy & Astrophysics
1663:Astronomy & Astrophysics
1598:Astronomy & Astrophysics
1453:Astronomy & Astrophysics
1206:Astronomy & Astrophysics
1096:Astronomy & Astrophysics
293:. Four of these stars, with
259:and one of the best-studied
130:10 light-years (core radius)
95:Apparent dimensions (V)
7:
3414:– E. Paunzen (Univ. Vienna)
3079:10.1051/0004-6361/201116948
3009:10.1051/0004-6361/201834045
2833:10.1051/0004-6361/202039498
2684:10.1051/0004-6361/201833672
2441:10.1051/0004-6361/201628778
2144:110: 228-231. Abstract at
1693:10.1051/0004-6361/201834045
1628:10.1051/0004-6361/201834608
1042:
531:on the shield that the god
494:were the five daughters of
485:Golden Gate of the Ecliptic
376:, with the overall cluster
10:
4462:
3212:10.3847/0004-637X/818/1/46
3152:10.1088/0004-637X/787/1/27
3103:: CS1 maint: postscript (
2979:Astronomy and Astrophysics
2803:Astronomy and Astrophysics
2654:Astronomy and Astrophysics
2411:Astronomy and Astrophysics
2205:665: 785-793. Abstract at
1988:10.1051/0004-6361:20066240
1741:10.56042/ijpap.v60i3.58781
1501:10.1051/0004-6361:20079342
1471:Astronomy and Astrophysics
967:
551:Giovanni Battista Hodierna
474:
320:(the "Bull's Eye"), has a
39:Observation data (J2000.0
4329:
4288:
3730:
3632:
3524:
3437:Hyades (star cluster) on
3180:The Astrophysical Journal
3121:The Astrophysical Journal
2920:The Astrophysical Journal
2861:The Astrophysical Journal
2536:The Astrophysical Journal
1263:The Astrophysical Journal
186:
174:
169:
150:
142:
134:
126:
110:
105:
94:
83:
69:
59:
47:
38:
26:
21:
3318:10.3847/1538-3881/aac894
3286:The Astronomical Journal
3265:10.3847/1538-3881/aa9791
3233:The Astronomical Journal
2951:10.3847/1538-4357/abe3fa
2892:10.3847/2041-8213/ac772f
2747:10.3847/1538-3881/ace9bf
2716:The Astronomical Journal
2567:10.3847/1538-4357/aaca2e
2505:10.3847/1538-3881/ac5f50
2474:The Astronomical Journal
2100:Böhm-Vitense, E (2007).
1780:Ian Ridpath’s Star Tales
585:Morphology and evolution
544:Green Grow the Rushes, O
498:and half-sisters to the
490:In Greek mythology, the
106:Physical characteristics
65:+15° 52′
3332:Langer, Johnni (2018).
3071:2011A&A...531A..92R
3001:2019A&A...623A..35L
2825:2021A&A...649A...6G
2676:2018A&A...620A.130P
2433:2017A&A...599A..78P
1980:2007A&A...468..139P
1920:2003ARA&A..41...57L
1685:2019A&A...623A..35L
1620:2019A&A...621L...2R
1493:2008A&A...482L...5V
1118:1998A&A...331...81P
423:under clear dark skies.
358:color–magnitude diagram
4436:Taurus (constellation)
4321:Herschel 400 Catalogue
2203:Astrophysical Journal,
774:Hyades brightest stars
766:
483:, the Hyades form the
363:cosmic distance ladder
354:Hubble Space Telescope
4426:Hyades (star cluster)
4306:New General Catalogue
3518:Astronomical catalogs
3031:Astronomical Journal,
2626:10.1093/mnras/stu2059
2347:Astrophysical Journal
2290:Astrophysical Journal
2167:Astrophysical Journal
2142:Astronomical Journal,
2017:Astronomical Journal,
1049:List of open clusters
764:
396:at the center of the
243:Ὑάδες, also known as
193:List of open clusters
2221:Astronomical Journal
2106:Astronomical Journal
1847:Astronomical Journal
1570:10.1093/mnras/sty793
740:are smaller than 50
726:Stellar multiplicity
513:. In Book 18 of the
49:Right ascension
3475:Articles and images
3309:2018AJ....156...46V
3256:2018AJ....155....4M
3203:2016ApJ...818...46M
3144:2014ApJ...787...27Q
3093:(Kharchenko+ 2009).
2942:2021ApJ...911....7Z
2883:2022ApJ...934L..18K
2738:2023AJ....166..103S
2617:2014MNRAS.445.3908L
2558:2018ApJ...862..138G
2496:2022AJ....163..242S
2359:1997ApJ...475..604S
2312:2006ApJ...649..436E
2233:2006AJ....131.2643A
2179:1997ApJ...485..167T
2118:2007AJ....133.1903B
2060:2002MNRAS.336.1188K
1517:"The Drifting Star"
1421:2011MNRAS.415..563D
1369:"Messier Object 44"
1337:2006MNRAS.369..383D
1276:2007ApJ...661..527S
1025:archaeoastronomical
776:
340:Location and motion
4446:Hyades (mythology)
3724:Caldwell catalogue
3423:2016-03-03 at the
1010:Robert W. Chambers
772:
767:
742:astronomical units
449:galactic longitude
374:solar neighborhood
352:satellite and the
295:Bayer designations
151:Other designations
135:Estimated age
85:Apparent magnitude
4367:
4366:
4296:Messier Catalogue
3690:
3689:
1231:Jim Kaler's Stars
965:
964:
561:(Praesepe), M45 (
468:binary systems.
417:Ursa Major Stream
255:) is the nearest
198:
197:
138:625 million years
4453:
4441:Caldwell objects
4408:
4407:
4406:
4396:
4395:
4384:
4383:
4382:
4375:
4357:
4347:
4346:
4337:
4336:
3717:
3710:
3703:
3694:
3693:
3511:
3504:
3497:
3488:
3487:
3397:
3371:
3370:
3368:
3367:
3352:
3346:
3345:
3329:
3323:
3322:
3320:
3302:
3276:
3270:
3269:
3267:
3249:
3223:
3217:
3216:
3214:
3196:
3170:
3164:
3163:
3137:
3115:
3109:
3108:
3102:
3094:
3064:
3044:
3038:
3027:
3021:
3020:
2994:
2970:
2964:
2963:
2953:
2935:
2911:
2905:
2904:
2894:
2876:
2851:
2845:
2844:
2818:
2793:
2787:
2786:
2785:
2769:
2760:
2759:
2749:
2731:
2707:
2696:
2695:
2669:
2645:
2639:
2638:
2628:
2610:
2601:(4): 3908–3918.
2586:
2580:
2579:
2569:
2551:
2527:
2518:
2517:
2507:
2489:
2464:
2453:
2452:
2426:
2402:
2393:
2382:
2373:
2372:
2370:
2338:
2332:
2331:
2305:
2303:astro-ph/0606121
2285:
2279:
2272:
2263:
2262:
2244:
2242:10.1.1.1000.4076
2227:(5): 2643–2651.
2216:
2210:
2199:
2193:
2192:
2190:
2158:
2149:
2138:
2132:
2131:
2129:
2112:(5): 1903–1910.
2097:
2082:
2081:
2071:
2053:
2051:astro-ph/0207514
2044:(4): 1188–1194.
2029:
2020:
2013:
2000:
1999:
1973:
1953:
1940:
1939:
1913:
1911:astro-ph/0301540
1893:
1887:
1877:
1871:
1860:
1854:
1843:
1837:
1826:
1820:
1813:
1807:
1802:
1791:
1790:
1788:
1786:
1768:
1762:
1761:
1743:
1719:
1713:
1712:
1678:
1654:
1648:
1647:
1613:
1589:
1583:
1582:
1572:
1562:
1553:(3): 3197–3216.
1538:
1532:
1531:
1529:
1528:
1519:. Archived from
1512:
1486:
1466:
1460:
1449:
1443:
1442:
1432:
1414:
1390:
1384:
1383:
1381:
1380:
1365:
1359:
1358:
1348:
1330:
1328:astro-ph/0603314
1304:
1298:
1297:
1287:
1253:
1242:
1241:
1239:
1237:
1222:
1213:
1201:
1188:
1177:
1166:
1155:
1144:
1135:van Leeuwen, F.
1133:
1122:
1121:
1111:
1109:astro-ph/9707253
1091:
1008:In the works of
777:
771:
748:Future evolution
705:mass segregation
699:Mass segregation
614:Star populations
444:
432:
386:Praesepe Cluster
238:
237:
234:
233:
230:
227:
224:
221:
218:
215:
212:
101:
55:
31:
19:
18:
4461:
4460:
4456:
4455:
4454:
4452:
4451:
4450:
4416:
4415:
4414:
4404:
4402:
4390:
4380:
4378:
4370:
4368:
4363:
4325:
4311:Index Catalogue
4284:
3726:
3721:
3691:
3686:
3628:
3520:
3515:
3425:Wayback Machine
3384:"Cl Melotte 25"
3382:
3379:
3374:
3365:
3363:
3353:
3349:
3330:
3326:
3277:
3273:
3224:
3220:
3171:
3167:
3116:
3112:
3096:
3095:
3045:
3041:
3028:
3024:
2971:
2967:
2912:
2908:
2852:
2848:
2794:
2790:
2770:
2763:
2708:
2699:
2646:
2642:
2587:
2583:
2528:
2521:
2465:
2456:
2403:
2396:
2383:
2376:
2339:
2335:
2286:
2282:
2273:
2266:
2217:
2213:
2200:
2196:
2159:
2152:
2139:
2135:
2098:
2085:
2030:
2023:
2014:
2003:
1954:
1943:
1894:
1890:
1878:
1874:
1861:
1857:
1844:
1840:
1827:
1823:
1814:
1810:
1803:
1794:
1784:
1782:
1769:
1765:
1720:
1716:
1655:
1651:
1590:
1586:
1539:
1535:
1526:
1524:
1515:Emily Baldwin.
1513:, announced in
1467:
1463:
1450:
1446:
1391:
1387:
1378:
1376:
1367:
1366:
1362:
1305:
1301:
1254:
1245:
1235:
1233:
1223:
1216:
1202:
1191:
1178:
1169:
1156:
1147:
1134:
1125:
1092:
1061:
1057:
1045:
1014:H. P. Lovecraft
1006:
970:
799:
792:
759:
757:Brightest stars
750:
728:
713:
710:
701:
693:
690:
648:
645:
641:
638:
629:
626:
616:
608:
605:
599:mass of the Sun
595:Galactic Center
587:
555:Charles Messier
477:
459:
452:
445:
436:
433:
342:
209:
205:
121:
118:
99:
53:
34:
17:
12:
11:
5:
4459:
4449:
4448:
4443:
4438:
4433:
4428:
4413:
4412:
4400:
4388:
4365:
4364:
4362:
4361:
4351:
4341:
4330:
4327:
4326:
4324:
4323:
4318:
4313:
4308:
4303:
4298:
4292:
4290:
4286:
4285:
4283:
4282:
4277:
4272:
4267:
4262:
4257:
4252:
4247:
4242:
4237:
4232:
4227:
4222:
4217:
4212:
4207:
4202:
4197:
4192:
4187:
4182:
4177:
4172:
4167:
4162:
4157:
4152:
4147:
4142:
4137:
4132:
4127:
4122:
4117:
4112:
4107:
4102:
4097:
4092:
4087:
4082:
4077:
4072:
4067:
4062:
4057:
4052:
4047:
4042:
4037:
4032:
4027:
4022:
4017:
4012:
4007:
4002:
3997:
3992:
3987:
3982:
3977:
3972:
3967:
3962:
3957:
3952:
3947:
3942:
3937:
3932:
3927:
3922:
3917:
3912:
3907:
3902:
3897:
3892:
3887:
3882:
3877:
3872:
3867:
3862:
3857:
3852:
3847:
3842:
3837:
3832:
3827:
3822:
3817:
3812:
3807:
3802:
3797:
3792:
3787:
3782:
3777:
3772:
3767:
3762:
3757:
3752:
3747:
3742:
3736:
3734:
3728:
3727:
3720:
3719:
3712:
3705:
3697:
3688:
3687:
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1904:(1): 57–115.
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1523:on 2008-04-21
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1038:
1035:. Astronomer
1034:
1030:
1026:
1021:
1019:
1015:
1011:
1001:
999:
995:
991:
987:
983:
979:
978:Epsilon Tauri
975:
960:
957:
954:
952:
949:
948:
944:
941:
938:
936:
933:
932:
928:
925:
922:
920:
919:Upsilon Tauri
917:
916:
912:
909:
906:
904:
901:
900:
896:
893:
890:
888:
885:
884:
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869:
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864:
861:
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856:
853:
852:
848:
845:
842:
840:
837:
836:
832:
829:
826:
824:
823:Epsilon Tauri
821:
820:
816:
813:
810:
808:
805:
804:
801:
796:
794:
789:
787:
784:
782:
779:
778:
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770:
763:
754:
745:
743:
739:
734:
723:
719:
717:
706:
696:
694:
685:
681:
677:
676:proper motion
672:
666:
662:
660:
656:
652:
634:
630:
621:
611:
609:
600:
596:
592:
582:
578:
575:
570:
568:
564:
560:
556:
552:
547:
545:
540:
538:
534:
530:
526:
522:
518:
517:
512:
508:
503:
501:
497:
493:
488:
486:
482:
472:
469:
465:
462:
450:
443:
438:
431:
426:
425:
424:
422:
418:
414:
409:
407:
403:
399:
395:
391:
390:Hyades Stream
387:
383:
382:proper motion
379:
375:
371:
366:
364:
359:
355:
351:
347:
337:
334:
330:
325:
323:
319:
315:
311:
307:
303:
299:
296:
292:
288:
283:
281:
277:
274:
273:constellation
270:
266:
262:
261:star clusters
258:
254:
250:
246:
242:
236:
203:
194:
190:
185:
182:
179:
177:
176:Constellation
173:
168:
164:
160:
156:
153:
149:
146:
141:
137:
133:
129:
125:
122:
113:
109:
104:
97:
93:
89:
86:
82:
78:
74:
72:
68:
64:
62:
58:
52:
50:
46:
42:
37:
30:
25:
20:
3939:
3682:Collinder 54
3677:Collinder 53
3672:Collinder 52
3667:Collinder 51
3662:Collinder 50
3661:
3657:Collinder 49
3652:Collinder 48
3647:Collinder 47
3642:Collinder 46
3578:
3408:(2000-09-29)
3387:
3364:. Retrieved
3361:Ars Technica
3360:
3350:
3341:
3337:
3327:
3290:
3284:
3274:
3237:
3231:
3221:
3184:
3178:
3168:
3125:
3119:
3113:
3090:
3052:
3048:
3042:
3030:
3025:
2982:
2978:
2968:
2923:
2919:
2909:
2864:
2860:
2849:
2806:
2802:
2791:
2773:
2719:
2715:
2657:
2653:
2643:
2598:
2594:
2584:
2539:
2535:
2477:
2473:
2414:
2410:
2385:
2350:
2346:
2336:
2293:
2289:
2283:
2224:
2220:
2214:
2202:
2197:
2170:
2166:
2141:
2136:
2109:
2105:
2041:
2037:
2016:
1961:
1957:
1901:
1897:
1891:
1880:
1875:
1863:
1858:
1846:
1841:
1829:
1824:
1816:
1811:
1783:. Retrieved
1779:
1766:
1731:
1727:
1717:
1666:
1662:
1652:
1601:
1597:
1587:
1550:
1546:
1536:
1525:. Retrieved
1521:the original
1477:(2): L5–L8.
1474:
1470:
1464:
1452:
1447:
1402:
1398:
1388:
1377:. Retrieved
1375:. 2007-08-25
1372:
1363:
1318:
1312:
1302:
1267:
1261:
1234:. Retrieved
1230:
1205:
1184:
1162:
1140:
1099:
1095:
1037:Donald Olson
1022:
1007:
971:
773:
768:
751:
729:
720:
702:
680:brown dwarfs
667:
663:
633:white dwarfs
620:brown dwarfs
617:
588:
579:
571:
548:
541:
514:
504:
489:
478:
470:
466:
463:
460:
410:
367:
343:
329:tidal radius
326:
317:
284:
257:open cluster
252:
249:Collinder 50
248:
244:
201:
199:
189:Open cluster
170:Associations
145:open cluster
4410:Outer space
1785:20 November
1772:Ian Ridpath
1225:Jim Kaler.
990:hot Jupiter
982:superjovian
935:Delta Tauri
887:Kappa Tauri
871:Theta Tauri
855:Delta Tauri
839:Gamma Tauri
807:Theta Tauri
781:Designation
591:evaporation
378:metallicity
310:Theta Tauri
291:giant stars
245:Caldwell 41
61:Declination
4420:Categories
3467:Astrophoto
3459:Hydrogen α
3366:2022-06-09
3300:1805.11117
3247:1709.10328
3194:1512.00483
2992:1901.07534
2933:2102.05045
2874:2205.02729
2867:(2): L18.
2816:2012.02061
2783:2408.10112
2729:2307.11882
2722:(3): 103.
2667:1810.12867
2549:1805.11715
2542:(2): 138.
2487:2203.11090
2480:(5): 242.
2424:1701.03398
1817:The Iliad.
1676:1901.07534
1611:1811.03845
1560:1804.00759
1527:2008-04-18
1379:2012-12-24
1236:29 October
1227:"Hyadum I"
1102:: 81–120.
1055:References
1029:Norse myth
1004:In culture
974:exoplanets
574:Lewis Boss
533:Hephaistos
525:Ursa Major
457:Astrometry
404:host star
312:, form an
253:Melotte 25
187:See also:
4386:Astronomy
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3062:1105.6093
3017:0004-6361
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2841:0004-6361
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2692:0004-6361
2635:0035-8711
2608:1410.0192
2576:0004-637X
2514:0004-6256
2449:0004-6361
2237:CiteSeerX
1971:0704.1159
1758:251335023
1750:0975-1041
1709:119385406
1701:0004-6361
1644:118909033
1636:0004-6361
1579:0035-8711
1484:0803.2029
1412:1103.2588
1294:122683844
986:HD 285507
793:magnitude
535:made for
421:naked eye
402:exoplanet
398:Milky Way
350:Hipparcos
333:Milky Way
322:gas giant
280:Aldebaran
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1043:See also
1033:Ragnarök
951:71 Tauri
903:90 Tauri
791:Apparent
733:binarity
712:☉
671:M dwarfs
647:☉
640:☉
628:☉
607:☉
563:Pleiades
537:Achilles
521:Pleiades
500:Pleiades
481:Pleiades
415:and the
413:Pleiades
314:asterism
287:evolving
155:Caldwell
143:Closest
120:☉
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4372:Portals
4349:Commons
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3439:WikiSky
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3242:arXiv
3189:arXiv
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