1369:
1703:
1118:
1256:, but these events are rare. The last occultation of Antares by Venus took place on September 17, 525 BC; the next one will be November 17, 2400. Other planets have been calculated not to have occulted Antares over the last millennium, nor will they in the next millennium, as most planets stay near the ecliptic and pass north of Antares. Venus will be extremely near Antares on October 19, 2117, and every eight years thereafter through to October 29, 2157, it will pass
945:
39:
7070:
5122:
46:
5146:
5134:
4219:
Perryman, M. A. C.; Lindegren, L.; Kovalevsky, J.; Hoeg, E.; Bastian, U.; Bernacca, P. L.; Crézé, M.; Donati, F.; Grenon, M.; Grewing, M.; van
Leeuwen, F.; van der Marel, H.; Mignard, F.; Murray, C. A.; Le Poole, R. S.; Schrijver, H.; Turon, C.; Arenou, F.; Froeschlé, M.; Petersen, C. S. (July 1997).
1598:
were derived from older measurements of the diameter, but those measurements are likely to have been affected by asymmetry of the atmosphere and the narrow range of infrared wavelengths observed; Antares has an extended shell which radiates strongly at those particular wavelengths. Despite its large
1505:
Like most cool supergiants, Antares's size has much uncertainty due to the tenuous and translucent nature of the extended outer regions of the star. Defining an effective temperature is difficult due to spectral lines being generated at different depths in the atmosphere, and linear measurements
2404:
Ohnaka, K; Hofmann, K.-H; Schertl, D; Weigelt, G; Baffa, C; Chelli, A; Petrov, R; Robbe-Dubois, S (2013). "High spectral resolution imaging of the dynamical atmosphere of the red supergiant
Antares in the CO first overtone lines with VLTI/AMBER".
1781:, Antares may have been known by various names: Urbat, Bilu-sha-ziri ("the Lord of the Seed"), Kak-shisa ("the Creator of Prosperity"), Dar Lugal ("The King"), Masu Sar ("the Hero and the King"), and Kakkab Bir ("the Vermilion Star"). In ancient
1245:. The occultation of 31 July 2009 was visible in much of southern Asia and the Middle East. Every year around December 2 the Sun passes 5° north of Antares. Lunar occultations of Antares are fairly common, depending on the 18.6-year cycle of the
1353:(AU) (≈ 80 billion km) at the estimated distance of Antares, giving a minimum value for the distance between them. Spectroscopic examination of the energy states in the outflow of matter from the companion star suggests that the latter is over
1422:
is around 100,000 times that of the Sun. There is a large margin of error assigned to values for the bolometric luminosity, typically 30% or more. There is also considerable variation between values published by different authors, for example
1690:, or the result of the mixing of light from the two stars when they are seen together through a telescope and are too close to be completely resolved. Antares B can sometimes be observed with a small telescope for a few seconds during lunar
1132:
orbits. It became apparent that the small variations could not be due to orbital motion, and they were actually caused by pulsation of the star's atmosphere. Even in 1928, it was calculated that the size of the star must vary by about 20%.
1205:
1685:
Antares B is normally difficult to see in small telescopes due to glare from
Antares, but can sometimes be seen in apertures over 150 millimetres (5.9 inches). It is often described as green, but this is probably either a
1642:
of spectral type B2.5V; it also has numerous unusual spectral lines suggesting it has been polluted by matter ejected by
Antares. It is assumed to be a relatively normal early-B main sequence star with a mass around
1342:. The variations in the separation are often interpreted as evidence of orbital motion, but are more likely to be simply observational inaccuracies with very little true relative motion between the two components.
4986:
Bester, M.; et al. (May 1996). "Measurement at 11 Micron
Wavelengths of the Diameters of alpha Orionis and alpha Scorpii: Changes in Effective Temperature of alpha Orionis and Very Recent Dust Emission".
1545:
in 2010. The linear radius of the star can be calculated from its angular diameter and distance. However, the distance to
Antares is not known with the same accuracy as modern measurements of its diameter.
2525:
Mark J. Pecaut; Eric E. Mamajek & Eric J. Bubar (February 2012). "A Revised Age for Upper
Scorpius and the Star Formation History among the F-type Members of the Scorpius-Centaurus OB Association".
4200:. The Biggest, Baddest, Coolest Stars. Proceedings of the workshop held 16-18 July 2007, at the Millennium Centre, Johnson City, Tennessee, USA. ASP Conference Series. Vol. 412. p. 113.
1506:
produce different results depending on the wavelength observed. In addition, Antares appears to pulsate, varying its radius by 19%. It also varies in temperature by 150 K, lagging 70 days behind
1109:
Antares is easier to see from the southern hemisphere due to its southerly declination. In the whole of
Antarctica, the star is circumpolar as the whole continent is above 64° S latitude.
2590:
Kudritzki, R. P.; Reimers, D. (1978). "On the absolute scale of mass-loss in red giants. II. Circumstellar absorption lines in the spectrum of alpha Sco B and mass-loss of alpha Sco A".
1177:
slowly varies between extremes of +0.6 and +1.6, although usually near magnitude +1.0. There is no obvious periodicity, but statistical analyses have suggested periods of 1,733 days or
1079:(WGSN) to catalog and standardise proper names for stars. The WGSN's first bulletin of July 2016 included a table of the first two batches of names approved by the WGSN, which included
1185:
days. No separate long secondary period has been detected, although it has been suggested that primary periods longer than a thousand days are analogous to long secondary periods.
3377:
1276:
to the Sun. It is a member of the Upper
Scorpius subgroup of the association, which contains thousands of stars with a mean age of 11 million years. Antares is located about 170
1213:
Lunar
Occultation of Antares (reappearance) was observed on 2006 May 14 from The Blue Mountains, Australia. Antares B reappears first, followed by Antares A 7.53 seconds later.
1051:
which is considered an outdated speculation, because the name of this star in Mesopotamian astronomy has always been "heart of Scorpion" and it was associated with the goddess
1308:. The best calculated orbit for the stars is still considered to be unreliable. It describes an almost circular orbit seen nearly edge-on, with a period of 1,218 years and a
1209:
1206:
1140:
during an occultation on April 13, 1819, although this was not widely accepted and dismissed as a possible atmospheric effect. It was then observed by Scottish astronomer
1008:
697:
692:
2210:
1106:
with the Sun. In higher northern latitudes, Antares is only visible low in the south in summertime. Higher than 64° northern latitude, the star does not rise at all.
613:
465:
1490:. These correspond to ages from 11.8 to 17.3 MYr. These initial mass estimates mean that Antares may have once resembled massive blue stars like the members of the
1163:
4456:
1162:
In 1952, Antares was reported to vary in brightness. A photographic magnitude range from 3.00 to 3.16 was described. The brightness has been monitored by the
3473:
Melnik, A. M.; Dambis, A. K. (2020). "Distance scale for high-luminosity stars in OB associations and in field with Gaia DR2. Spurious systematic motions".
1249:. The last cycle ended in 2010 and the next begins in 2023. Shown at right is a video of a reappearance event, clearly showing events for both components.
1208:
3140:
A Handbook of Double Stars, with a Catalogue of Twelve Hundred Double Stars and Extensive Lists of Measures. with Additional Notes Bringing the Measur
2317:
Evans, D. S. (June 20–24, 1966). "The Revision of the General Catalogue of Radial Velocities". In Batten, Alan Henry; Heard, John Frederick (eds.).
1144:
1472:
and an age of 11 to 15 MYr. Comparison of observations from antiquity to theoretical evolutionary tracks suggests an initial mass of 15 to 16
7147:
4924:
Justtanont, K.; et al. (May 1999). "Atomic fine-structure lines in the ISO-SWS spectra of the supergiants alpha Orionis and alpha Scorpii".
7127:
892:
system, with its two components called α Scorpii A and α Scorpii B. The brighter of the pair is the red supergiant, while the fainter is a hot
4644:
O'Gorman, E.; et al. (June 2020). "ALMA and VLA reveal the lukewarm chromospheres of the nearby red supergiants Antares and Betelgeuse".
1102:
For two to three weeks on either side of November 30, Antares is not visible in the night sky from mid-northern latitudes, because it is near
4510:
4485:
4380:
3436:
3409:
3148:
2818:
2791:
2701:
2361:
2028:
1103:
4526:
2870:
1092:
3351:
2717:
Samus, N. N.; Durlevich, O. V.; et al. (2009). "VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013)".
2617:
Schröder, K.-P.; Cuntz, M. (April 2007). "A critical test of empirical mass loss formulas applied to individual giants and supergiants".
7097:
2944:
2940:
2936:
1012:
957:
3387:
1495:
1269:
835:
5178:
3793:
Dave, Gault; Brian, Loader (September 2006). "Determining the Separation and Position Angle of Antares A–B during Lunar Occultation".
2687:
2920:
2465:"Colour evolution of Betelgeuse and Antares over two millennia, derived from historical records, as a new constraint on mass and age"
1694:
while Antares is hidden by the Moon. Antares B appears a profound blue or bluish-green color, in contrast to the orange-red Antares.
7107:
3857:"ICCD Speckle Observations of Binary Stars. V. Measurements During 1988–1989 from the Kitt Peak and the Cerro Tololo 4 M Telescopes"
128:
1557:
gave Antares a diameter of 400 to 430 million mi (640 to 690 million km), equal to approximately 463-497
2207:
1141:
1072:
4746:
Ohnaka, K. (August 2014). "Imaging the outward motions of clumpy dust clouds around the red supergiant Antares with VLT/VISIR".
1207:
7137:
1076:
70:
1004:
704:
4503:
Aboriginal mythology : an A-Z spanning the history of aboriginal mythology from the earliest legends to the present day
2189:
Hoffleit, D.; Warren, W. H. (1995). "VizieR Online Data Catalog: Bright Star Catalogue, 5th Revised Ed. (Hoffleit+, 1991)".
3828:
Anton, Rainer (2015). "Double Star Measurements at the Southern Sky with a 50 cm Reflector and a Fast CCD Camera in 2014".
1368:
1117:
5203:
2743:
1857:
636:
495:
5112:
1568:. Antares is now known to be somewhat larger, but still recognized as one of the largest stars known. For instance, the
92:
7112:
7092:
1630:
million years. For a few months, the Antares supernova could be as bright as the full moon and be visible in daytime.
1565:
1319:. Other recent estimates of the period have ranged from 880 years for a calculated orbit, to 2,562 years for a simple
1196:
observed the variability of Antares and incorporated it into their oral traditions as Waiyungari (meaning 'red man').
680:
3699:
Reimers, D.; Hagen, H. -J.; Baade, R.; Braun, K. (2008). "The Antares emission nebula and mass loss of α Scorpii A".
1387:
of M1.5Iab-Ib, and is indicated to be a spectral standard for that class. Due to the nature of the star, the derived
4852:
Sanad, M. R.; Bobrowsky, M. (October 2010). "Spectral variability of the α Sco AB binary system observed with IUE".
4439:
1458:
and luminosity of Antares to theoretical evolutionary tracks for massive stars suggest a progenitor mass of 17
7152:
7142:
2755:
1711:
1285:
851:
6619:
1702:
1525:
has been published. Interferometry allows synthesis of a view of the stellar disc, which is then represented as a
5469:
5198:
5103:
Best Ever Image of a Star’s Surface and Atmosphere – First map of motion of material on a star other than the Sun
1639:
1016:
996:
823:
688:
4626:
1128:
variations were observed in the spectrum of Antares in the early 20th century, and attempts were made to derive
5187:
1949:
1554:
1522:
1415:
20:
7117:
2226:
Keenan, Philip C; McNeil, Raymond C (1989). "The Perkins catalog of revised MK types for the cooler stars".
1170:
827:
819:
235:
6624:
7132:
6360:
5171:
3752:
Mason, Brian D.; Wycoff, Gary L.; Hartkopf, William I.; Douglass, Geoffrey G.; Worley, Charles E. (2001).
2683:
1384:
1027:
988:
916:
861:
858:
734:
718:
674:
196:
4691:
Ohnaka, K.; et al. (August 2017). "Vigorous atmospheric motion in the red supergiant star Antares".
1706:
Antares seen from the ground. The very bright star towards the upper left corner of the frame is Antares.
7102:
6850:
5877:
5396:
5018:"Direct Measurement of the Inner Radius of the Dust Shell around the Cool Supergiant Star alpha Scorpii"
4552:
4396:
Rogers, J. H. (February 1998). "Origins of the ancient constellations: I. The Mesopotamian traditions".
1619:
1455:
1419:
984:
980:
869:
803:
669:
621:
473:
1137:
818:
near the center of the constellation. Distinctly reddish when viewed with the naked eye, Antares is a
7157:
6659:
6654:
6524:
6489:
5029:
4996:
4958:
4933:
4894:
4861:
4822:
4765:
4710:
4663:
4603:
4448:
4405:
4333:
4260:
4229:
4201:
4154:
4085:
4048:
3996:
3955:
3909:
3868:
3837:
3802:
3765:
3718:
3681:
3644:
3600:
3545:
3492:
3317:
3280:
3233:
3196:
3091:
3000:
2965:
2726:
2636:
2599:
2545:
2486:
2424:
2326:
2289:
2235:
2198:
2138:
2074:
1832:
1346:
1222:
1156:
1129:
1048:
897:
322:
6649:
6644:
6529:
6484:
3897:
3271:
Percy, John R.; Sato, Hiromitsu (2009). "Long Secondary Periods in Pulsating Red Supergiant Stars".
2842:
6810:
6805:
6800:
6734:
6729:
6724:
6609:
5847:
5842:
5827:
5822:
5817:
5807:
5802:
5797:
5792:
5782:
5767:
5762:
5757:
1980:
1273:
1056:
839:
684:
6815:
6604:
6599:
6594:
6469:
6464:
5752:
5747:
5717:
5712:
5702:
5697:
5662:
5657:
5652:
5642:
5637:
5627:
5622:
5612:
5607:
5597:
5592:
5587:
5577:
5572:
5567:
5562:
5557:
3116:
1529:
disk surrounded by an extended atmosphere. The diameter of the limb-darkened disk was measured as
6689:
6679:
6574:
6569:
6564:
6554:
5150:
4912:
4840:
4781:
4755:
4734:
4700:
4679:
4653:
4593:
4178:
4123:
4014:
3986:
3734:
3708:
3569:
3535:
3508:
3482:
3382:
3333:
3307:
2863:
2763:
2652:
2626:
2561:
2535:
2476:
2440:
2414:
2251:
2164:
2128:
2090:
2064:
1970:
1714:
dating from at least 1100 BCE, Antares was called GABA GIR.TAB, "the Breast of the Scorpion". In
1403:
1174:
343:
167:
6684:
6674:
6669:
6449:
5552:
5547:
5542:
5537:
5517:
5507:
5502:
5497:
5492:
5487:
5089:
4530:
4196:
Wing, R. F. (2009-09-01). Luttermoser, Donald G.; Smith, Beverly J.; Stencel, Robert E. (eds.).
2991:
Lunt, J. (1916). "On the orbits of the spectroscopic binaries alpha Orionis and alpha Scorpii".
2319:
Determination of Radial Velocities and their Applications, Proceedings from IAU Symposium no. 30
944:
763:
6509:
6423:
6418:
6403:
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6393:
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6373:
6368:
6350:
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6330:
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6320:
6315:
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6305:
6300:
6295:
6290:
6280:
6275:
6270:
6265:
6260:
6255:
6250:
6245:
6240:
6235:
6230:
6225:
6220:
6215:
6210:
6205:
6200:
6195:
6190:
6185:
6180:
6175:
6170:
6165:
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6155:
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6145:
6140:
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6100:
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6015:
6010:
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5990:
5985:
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5970:
5965:
5960:
5955:
5950:
5945:
5935:
5930:
5925:
5920:
5915:
5910:
5900:
5895:
5885:
5862:
5857:
5772:
5737:
5732:
5722:
5707:
5692:
5414:
5081:
3355:
7122:
7073:
6579:
6549:
6499:
6494:
5222:
5164:
5073:
4974:
4726:
4506:
4481:
4376:
4370:
4351:
4170:
4115:
3925:
3810:
3561:
3432:
3405:
3144:
2824:
2814:
2787:
2697:
2693:
2367:
2357:
2156:
2117:"Variability in red supergiant stars: pulsations, long secondary periods and convection noise"
2024:
1356:
1350:
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1152:
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905:
796:
772:
665:
516:
184:
63:
6589:
5777:
5617:
5085:
5077:
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5065:
4076:
A. Richichi (April 1990). "A new accurate determination of the angular diameter of Antares".
3298:
Hamacher, D.W. (2018). "Observations of red–giant variable stars by Aboriginal Australians".
5126:
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4966:
4937:
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4004:
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3685:
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3604:
3553:
3500:
3496:
3325:
3204:
3039:
3008:
2973:
2644:
2640:
2603:
2553:
2494:
2432:
2428:
2349:
2297:
2293:
2243:
2146:
2082:
2078:
1959:
1866:
1600:
1550:
754:
588:
440:
306:
99:
38:
6634:
6504:
4582:"The inner circumstellar dust of the red supergiant Antares as seen with VLT/SPHERE/ZIMPOL"
1494:
system, which have similar initial masses (both Antares and Acrux are members of the wider
6519:
5338:
5313:
5245:
4249:"Observation of 23 Supernovae That Exploded <300 pc from Earth during the past 300 kyr"
2924:
2895:
2767:
2004:
1687:
1507:
1391:
measurements have large errors, so that the true distance of Antares is approximately 550
1380:
1309:
1193:
1125:
601:
453:
254:
143:
3754:"The 2001 US Naval Observatory Double Star CD-ROM. I. The Washington Double Star Catalog"
3452:
1893:
1320:
5033:
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4898:
4865:
4826:
4714:
4607:
4452:
4409:
4337:
4264:
4205:
4158:
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4000:
3959:
3872:
3841:
3806:
3769:
3648:
3549:
3321:
3284:
3237:
3224:
Cousins, A. W. J. (1952). "Bright variable stars in southern hemisphere (second list)".
3200:
3110:
3095:
3004:
2969:
2730:
2549:
2490:
2330:
2239:
2202:
2142:
2021:
A Dictionary of Modern star Names: A Short Guide to 254 Star Names and Their Derivations
1067:. However, the name "Antares" is already proven in the Greek culture, e.g. in Ptolemy's
888:. Antares appears as a single star when viewed with the naked eye, but it is actually a
6825:
6479:
6474:
5358:
5353:
5288:
4291:
1955:
1526:
1514:
865:
656:
314:
294:
282:
189:
2557:
1723:
1292:
is sometimes referred to as the Antares Nebula or is otherwise identified as VdB 107.
7086:
6639:
5867:
5852:
5832:
5812:
5328:
5280:
5275:
5270:
5265:
5255:
5250:
5240:
4916:
4844:
4835:
4810:
4683:
4473:
4346:
4321:
4273:
4248:
4061:
4036:
4009:
3974:
3512:
3337:
2751:
2565:
2325:. Vol. 30. University of Toronto: International Astronomical Union. p. 57.
2255:
2151:
2116:
1999:
1862:
1845:
1824:
1743:
1599:
size compared to the Sun, Antares is dwarfed by even larger red supergiants, such as
1315:
1305:
1064:
953:
893:
811:
788:
271:
230:
80:
4785:
4372:
The Brightest Stars: Discovering the Universe Through the Sky's Most Brilliant Stars
4018:
3738:
3573:
2656:
2444:
2094:
7053:
6839:
6694:
6629:
6559:
5727:
5687:
5672:
5602:
5582:
5235:
5138:
4738:
4295:
2168:
1189:
873:
570:
543:
401:
374:
4777:
4675:
3730:
3672:
Baize, P.; Petit, M. (1989). "Etoiles doubles orbitales a composantes variables".
3613:
3588:
2436:
5097:
4970:
4873:
3426:
3164:
3138:
2921:"LASCO Star Maps (identify objects in the field of view for any day of the year)"
2781:
2719:
VizieR On-line Data Catalog: B/GCVS. Originally Published in: 2009yCat....102025S
2648:
2302:
2277:
2086:
1083:
for the star α Scorpii A. It is now so entered in the IAU Catalog of Star Names.
6954:
6780:
6775:
6770:
6765:
6760:
6584:
5348:
5343:
5333:
5323:
5298:
5293:
5260:
2353:
1973:
1828:
1816:
1778:
1691:
1675:
1604:
1518:
1301:
1284:) from Earth at the rim of the Upper Scorpius subgroup, and is illuminating the
1238:
949:
889:
850:) from Earth at the rim of the Upper Scorpius subgroup, and is illuminating the
815:
220:
209:
156:
3504:
2191:
VizieR On-line Data Catalog: V/50. Originally Published in: 1964BS....C......0H
1928:); the stars on each side represented his wives. The Kulin Kooris saw Antares (
6949:
6719:
6699:
6664:
6459:
6454:
5632:
5532:
5527:
5522:
5512:
5459:
5454:
5449:
5444:
5439:
5434:
5429:
5424:
5318:
5308:
5303:
3526:
Mamajek, E.E. (2008). "On the distance to the Ophiuchus star-forming region".
2923:. Large Angle and Spectrometric Coronagraph Experiment (LASCO). Archived from
2828:
2055:
van Leeuwen, F. (November 2007). "Validation of the new Hipparcos reduction".
1912:), an important star in the calculation of the Māori calendar. The Wotjobaluk
1644:
1615:
1392:
1281:
1246:
885:
847:
550:
414:
381:
329:
242:
4355:
4174:
4119:
3929:
3814:
3565:
3209:
3184:
3044:
3027:
2766:, with the assistance of McKenzie, Roderick. Oxford: Clarendon Press. In the
2499:
2464:
2371:
2160:
1855:, "second star of the Heart"), because it was the second star of the mansion
1334:
apart in 1848. More modern observations consistently give separations around
1091:
Antares is visible all night around May 31 of each year, when the star is at
6944:
6939:
6752:
6514:
6433:
6428:
6413:
6408:
6388:
6378:
6345:
6335:
6285:
6115:
6020:
5995:
5940:
5905:
5890:
5837:
5787:
5742:
5682:
5677:
5667:
5647:
5482:
5477:
5419:
5409:
5404:
5386:
5377:
5368:
5363:
5156:
4616:
4581:
3946:
Hockey, T.; Trimble, V. (2010). "Public reaction to a V = −12.5 supernova".
1837:
1671:
1667:
1623:
1608:
1569:
1499:
1480:
1234:
901:
831:
4730:
3557:
5102:
4978:
3921:
1584:
with modern angular diameter estimates lead to a radius of about 680
810:. Often referred to as "the heart of the scorpion", Antares is flanked by
7037:
7008:
7003:
6998:
6993:
6988:
6983:
6923:
6918:
6913:
6908:
6903:
6898:
6893:
6888:
6883:
6878:
6873:
6868:
6863:
6858:
6820:
6544:
5093:
3991:
2631:
2133:
1963:
1925:
1901:
1715:
1573:
1411:
1410:, but because the star radiates a considerable part of its energy in the
1388:
1218:
1068:
992:
961:
792:
530:
85:
45:
4722:
4182:
4142:
3657:
3632:
1835:(the eldest or biggest, probably attributing its huge size), one of the
1055:. Some scholars have speculated that the star may have been named after
6704:
6614:
5061:
4794:
4127:
4103:
3329:
3251:
1230:
881:
3587:
Malkov, O. Yu; Tamazian, V. S.; Docobo, J. A.; Chulkov, D. A. (2012).
2808:
1666:. As it falls short of the mass limit required for stars to undergo a
1099:. Antares then rises at dusk and sets at dawn as seen at the equator.
7022:
6968:
6795:
6790:
6785:
6714:
3975:"Multiwavelength diameters of nearby Miras and semiregular variables"
1937:
1874:
1812:
1786:
1767:
1679:
1655:
1396:
1277:
1047:. The comparison of Antares with Mars may have originated with early
1003:
catalogue as IRAS 16262–2619. It is also catalogued as a double star
983:
21 Scorpii, as well as catalogue designations such as HR 6134 in the
843:
748:
628:
563:
487:
394:
334:
4946:
2278:"Multi-component absorption lines in the HST spectra of α Scorpii B"
1465:
and an age of 12 million years (MYr), or an initial mass of 15
5133:
5042:
5017:
5008:
4907:
4882:
4705:
4658:
4598:
4166:
3881:
3856:
3778:
3753:
3487:
3312:
3012:
2977:
2692:(Reprint ed.). New York, NY: Dover Publications Inc. pp.
2481:
2247:
1722:
in the southern sky and denotes the breast of the Scorpion goddess
1406:
of Antares at visual wavelengths is about 10,000 times that of the
6709:
6539:
6534:
4760:
3713:
3540:
3354:. The International Occultation Timing Association. Archived from
3137:
Edward Crossley; Joseph Gledhill; J. M. Wilson (6 February 2018).
2540:
2419:
2069:
1913:
1909:
1842:
1820:
1782:
1771:
1701:
1491:
1367:
1253:
1226:
1203:
1148:
1116:
1060:
1052:
943:
834:. Antares is the brightest and most evolved stellar member of the
722:
73:
66:
2956:
Wright, W. H. (1907). "The variable radial velocity of Antares".
1718:, which dates between 1100 and 700 BC, it is one of the stars of
5213:
4883:"Mid-Infrared Images of the Circumstellar Dust around α Scorpii"
3855:
McAlister, Harold; Hartkopf, William I.; Franz, Otto G. (1990).
1790:
1726:. Later names that translate as "the Heart of Scorpion" include
1719:
1372:
1268:
Antares is the brightest and most evolved stellar member of the
1242:
1044:
1036:
1000:
933:
925:
877:
784:
298:
286:
5160:
2348:. Patrick Moore's Practical Astronomy Series. pp. 43–71.
1795:
1513:
The diameter of Antares can be measured most accurately using
1407:
1096:
1040:
929:
117:
114:
2744:
1900:, and regard it as the chief of all the stars especially the
1752:
1746:
1440:
The mass of the star has been calculated to be about 12
1030:
1015:, but as a Bayer-designated star it does not have a separate
1011:
J16294-2626. Antares is a variable star and is listed in the
919:
4143:"The Diameter of Alpha Scorpii by the Interferometer Method"
4037:"On the Six-year Period in the Radial Velocity of Antares A"
4811:"Short Timescale Variations in the Atmosphere of Antares A"
3589:"Dynamical masses of a selected sample of orbital binaries"
3028:"The Radial Velocity Variations of a Orionis and a Scorpii"
664:
Cor Scorpii, Kalb al Akrab, Scorpion's Heart, Vespertilio,
3402:
Journal of the British Astronomical Association – Volume 2
1521:
events. An apparent diameter from occultations 41.3 ± 0.1
2323:
Determination of Radial Velocities and Their Applications
1889:'fiery star') because of its reddish appearance.
1510:
changes which are likely to be caused by the pulsations.
1498:). Massive stars like Antares are expected to explode as
876:, it would extend out to somewhere between the orbits of
872:
visible to the naked eye. If placed at the center of the
102:
2864:"Bulletin of the IAU Working Group on Star Names, No. 1"
2023:(2nd rev. ed.). Cambridge, Massachusetts: Sky Pub.
4322:"A physical interpretation of the 'red Sirius' anomaly"
4147:
Publications of the Astronomical Society of the Pacific
2458:
2456:
2454:
1136:
Antares was first reported to have a companion star by
1001:
Infrared Astronomical Satellite (IRAS) Sky Survey Atlas
1326:
Early measurements of the pair found them to be about
5110:
4945:
Jennings, Donald E.; Sada, Pedro V. (February 1998).
3428:
NightWatch: A Practical Guide to Viewing the Universe
884:. Its mass is calculated to be around 12 to 16 times
129:
120:
105:
3378:"Sky watchers report occultation of Antares by moon"
1736:
111:
19:
This article is about the star. For other uses, see
7046:
7030:
7021:
6976:
6967:
6932:
6849:
6838:
6751:
6442:
6359:
5876:
5468:
5395:
5221:
5212:
3273:
Journal of the Royal Astronomical Society of Canada
2344:Buick, Tony (2010). "Classification of the Stars".
108:
2115:Kiss, L. L.; Szabo, G. M.; Bedding, T. R. (2006).
1549:An estimate obtained by interferometry in 1925 by
1252:Antares can also be occulted by the planets, e.g.
4586:Monthly Notices of the Royal Astronomical Society
4326:Monthly Notices of the Royal Astronomical Society
3979:Monthly Notices of the Royal Astronomical Society
3189:Monthly Notices of the Royal Astronomical Society
3082:Johnson, S. J. (1879). "Occultation of Antares".
3032:Monthly Notices of the Royal Astronomical Society
2469:Monthly Notices of the Royal Astronomical Society
2121:Monthly Notices of the Royal Astronomical Society
1614:Antares, like the similarly sized red supergiant
1063:warrior-hero celebrated in the pre-Islamic poems
16:Red supergiant star in the constellation Scorpius
2810:The Babylonian astronomical compendium MUL. APIN
5016:Bloemhof, E. E.; Danen, R. M. (February 1995).
4398:Journal of the British Astronomical Association
1958:, which displays 27 stars, each representing a
1916:people of Victoria, Australia, knew Antares as
1164:American Association of Variable Star Observers
4480:. Wellington: Huia Publishers. pp. 22–4.
3898:"MSC - a catalogue of physical multiple stars"
3404:. BiblioBazaar. 29 October 2015. p. 155.
3169:. H. M. Stationery Office. 1899. p. 161A.
3077:
3075:
2271:
2269:
2267:
2265:
2050:
2048:
2046:
2044:
2042:
2040:
1375:reconstructed view of the surface of Antares A
868:, a large evolved massive star and one of the
5172:
3941:
3939:
3633:"Orbits of Seven Edge-On Visual Double Stars"
3143:. Creative Media Partners, LLC. p. 329.
3068:. New York: Dover Publications. p. 1666.
2399:
2397:
2395:
2393:
2391:
2389:
2387:
2385:
2383:
2381:
1742:. This had been directly translated from the
1188:Research published in 2018 demonstrated that
1166:since 1945, and it has been classified as an
999:catalogue as 2MASS J16292443-2625549 and the
161:−26° 25′ 55.2094″
8:
3902:Astronomy and Astrophysics Supplement Series
3674:Astronomy and Astrophysics Supplement Series
3166:Reference Catalogue of Southern Double Stars
1793:in the pyramidal ceremonies). It was called
4881:Marsh, K. A.; et al. (February 2001).
4438:Lull, José; Belmonte, Juan Antonio (2009).
4427:. Wiesbaden: Otto Harrasowitz. p. 169.
4030:
4028:
3626:
3624:
3132:
3130:
3128:
3126:
2585:
2583:
2581:
2579:
2577:
2575:
1884:
1785:, Antares represented the scorpion goddess
1760:
1728:
1591:. Older radii estimates exceeding 850
7027:
6973:
6846:
6748:
5218:
5179:
5165:
5157:
4809:Pugh, T.; Gray, David F. (November 2013).
4527:"Science in Portugal - The Star of Cabral"
3185:"On an Occultation of Antares by the Moon"
3059:
3057:
3055:
1479:, or the possibility that Antares is on a
1360:beyond the primary (about 33 billion km).
1264:Illumination of Rho Ophiuchi cloud complex
1225:within 6° of the ecliptic (the others are
5041:
4906:
4834:
4759:
4704:
4657:
4627:"Meet Antares: the star that is not Mars"
4615:
4597:
4345:
4272:
4060:
4008:
3990:
3880:
3777:
3712:
3656:
3612:
3539:
3486:
3311:
3208:
3043:
2630:
2539:
2520:
2518:
2516:
2514:
2512:
2510:
2498:
2480:
2418:
2301:
2221:
2219:
2150:
2132:
2068:
4286:
4284:
3973:Ireland, M. J.; et al. (May 2004).
3178:
3176:
2914:
2912:
2843:"IAU Working Group on Star Names (WGSN)"
2678:
2676:
2674:
2672:
2670:
2668:
2666:
2463:Neuhäuser, R.; et al. (July 2022).
1851:The ancient Chinese called Antares 心宿二 (
1815:, Antares was known as one of the four "
1151:on 23 July 1844. It was rediscovered by
1121:Antares near the Sun on 30 November 2012
5117:
2919:Star Maps created using XEphem (2008).
2276:Baade, R.; Reimers, D. (October 2007).
2228:Astrophysical Journal Supplement Series
1991:
1865:, and it was sometimes referred to as (
826:of +0.6 down to +1.6. It is on average
822:star that ranges in brightness from an
278:
4795:"Antares: Betelgeuse's Neglected Twin"
4580:Cannon, E.; et al. (March 2021).
3352:"Occultation of Antares on 31 July 09"
3300:The Australian Journal of Anthropology
3252:"Antares: Betelgeuse's Neglected Twin"
2762:, revised and augmented throughout by
2110:
2108:
2106:
2104:
25:
4625:Johnson, Daniel (September 3, 2020).
2213:. Accessed on line September 07, 2012
1861:(心). It was the national star of the
1622:, will almost certainly explode as a
1217:Antares is 4.57 degrees south of the
7:
4505:. London: HarperCollins. p. 5.
4375:. John Wiley and Sons. p. 218.
3631:Pavlovic, R.; Todorovic, N. (2005).
2184:
2182:
2180:
2178:
2019:Kunitzsch, Paul; Smart, Tim (2006).
1043:hue to the appearance of the planet
932:hue to the appearance of the planet
842:to the Sun. It is located about 170
69:
4441:The constellations of ancient Egypt
3830:Journal of Double Star Observations
1734:from the Arabic قَلْبُ ٱلْعَقْرَبِ
1013:General Catalogue of Variable Stars
896:star of magnitude 5.5. They have a
290:
4529:. Instituto Camões. Archived from
2783:The Arkana Dictionary of Astrology
2689:Star Names: Their Lore and Meaning
1962:. Antares represents the state of
14:
4947:"Water in Betelgeuse and Antares"
7069:
7068:
5144:
5132:
5120:
4462:from the original on 2022-10-09.
4347:10.1046/j.1365-8711.1999.02975.x
4320:Whittet, D. C. B. (1999-12-01).
4010:10.1111/j.1365-2966.2004.07651.x
2152:10.1111/j.1365-2966.2006.10973.x
1483:with an initial mass of 13
1073:International Astronomical Union
1039:", due to the similarity of its
956:; Antares appears white in this
928:", due to the similarity of its
98:
44:
37:
3896:Tokovinin, A. A. (1997-07-01).
3431:. A & C Black. p. 46.
3386:. 2 August 2009. Archived from
2876:from the original on 2022-10-09
1979:Antares is one of the medieval
1670:, it will likely expand into a
1659:, and a radius of about 5
7148:Henry Draper Catalogue objects
4425:Arabische Sternnamen in Europa
4247:Firestone, R. B. (July 2014).
3475:Astrophysics and Space Science
2005:Merriam-Webster.com Dictionary
1879:
1770:of the Greek name rendered in
1496:Scorpius–Centaurus association
1270:Scorpius–Centaurus association
1071:and Tetrabiblos. In 2016, the
1059:, or Antarah ibn Shaddad, the
836:Scorpius–Centaurus association
1:
7128:Bright Star Catalogue objects
5204:Scorpius in Chinese astronomy
5022:Astrophysical Journal Letters
4035:Pugh, T.; Gray, D.F. (2013).
3109:William Arthur Darby (1864).
1640:blue-white main-sequence star
1638:Antares B is a magnitude 5.5
1200:Occultations and conjunctions
55:Location of Antares (circled)
4971:10.1126/science.279.5352.844
4874:10.1016/j.newast.2010.04.002
4748:Astronomy & Astrophysics
4646:Astronomy & Astrophysics
3637:Serbian Astronomical Journal
3066:Burnham's Celestial Handbook
3064:Burnham, Robert Jr. (1978).
2786:. Penguin Publishing Group.
2407:Astronomy & Astrophysics
1896:of New Zealand call Antares
1808:"the red one of the prow".
1796:
1753:
1437:published in 2012 and 2013.
828:the fifteenth-brightest star
6816:PSR B1620−26 b (Methuselah)
4778:10.1051/0004-6361/201423893
4676:10.1051/0004-6361/202037756
4220:"The HIPPARCOS Catalogue".
3731:10.1051/0004-6361:200809983
3614:10.1051/0004-6361/201219774
2896:"IAU Catalog of Star Names"
2558:10.1088/0004-637X/746/2/154
2437:10.1051/0004-6361/201321063
2354:10.1007/978-1-4419-1053-0_4
1737:
1077:Working Group on Star Names
313:5.89 ± 1.00
7174:
7098:B-type main-sequence stars
4926:Astronomy and Astrophysics
4836:10.1088/0004-637X/777/1/10
4274:10.1088/0004-637X/789/1/29
4222:Astronomy and Astrophysics
4078:Astronomy and Astrophysics
4062:10.1088/0004-6256/145/2/38
3701:Astronomy and Astrophysics
3593:Astronomy and Astrophysics
3505:10.1007/s10509-020-03827-0
3425:Terence Dickinson (2006).
3026:Spencer Jones, H. (1928).
2745:
2649:10.1051/0004-6361:20066633
2619:Astronomy and Astrophysics
2592:Astronomy and Astrophysics
2303:10.1051/0004-6361:20077308
2282:Astronomy and Astrophysics
2087:10.1051/0004-6361:20078357
2057:Astronomy and Astrophysics
1947:
1747:
1712:Babylonian star catalogues
1674:before dying as a massive
1304:that is thought to form a
1286:Rho Ophiuchi cloud complex
1031:
995:source, it appears in the
920:
852:Rho Ophiuchi cloud complex
18:
7066:
6747:
5199:List of stars in Scorpius
5194:
5188:Constellation of Scorpius
4887:The Astrophysical Journal
4815:The Astrophysical Journal
4253:The Astrophysical Journal
3528:Astronomische Nachrichten
3112:The astronomical observer
2993:The Astrophysical Journal
2958:The Astrophysical Journal
1976:is named after the star.
1870:
1543:0.09 milliarcseconds
1535:0.06 milliarcseconds
1017:variable star designation
997:Two Micron All-Sky Survey
824:apparent visual magnitude
741:
729:
713:
662:
655:
536:
400:680 (varies by 19%)
367:
362:
358:
248:
241:
178:
60:
31:
7108:Slow irregular variables
4198:The Biggest Stars of All
4041:The Astronomical Journal
3861:The Astronomical Journal
3758:The Astronomical Journal
2807:Hunger, Hermann (2019).
1960:federated unit of Brazil
1950:Antares (disambiguation)
1555:Mount Wilson Observatory
1155:in 1846 and measured by
1049:Mesopotamian astronomers
21:Antares (disambiguation)
4938:1999A&A...345..605J
4770:2014A&A...568A..17O
4668:2020A&A...638A..65O
4234:1997A&A...323L..49P
4090:1990A&A...230..355R
3914:1997A&AS..124...75T
3723:2008A&A...491..229R
3686:1989A&AS...77..497B
3605:2012A&A...546A..69M
3497:2020Ap&SS.365..112M
3453:"Interactive sky chart"
3115:. Hardwicker. pp.
2768:Perseus Digital Library
2764:Jones, Sir Henry Stuart
2760:A Greek–English Lexicon
2641:2007A&A...465..593S
2604:1978A&A....70..227K
2429:2013A&A...555A..24O
2294:2007A&A...474..229B
2079:2007A&A...474..653V
1954:Antares appears in the
1789:(and was the symbol of
1698:Etymology and mythology
1652:, a temperature around
1288:in its foreground. The
1192:Aboriginal people from
1171:slow irregular variable
820:slow irregular variable
344:Absolute magnitude
185:Evolutionary stage
168:Apparent magnitude
7138:Durchmusterung objects
4423:Kunitzsch, P. (1959).
3558:10.1002/asna.200710827
3210:10.1093/mnras/16.6.143
3045:10.1093/mnras/88.8.660
2780:Fred Gettings (1990).
2500:10.1093/mnras/stac1969
1761:
1729:
1707:
1574:trigonometric parallax
1385:stellar classification
1376:
1214:
1122:
989:Henry Draper Catalogue
965:
6625:1RXS J170849.0−400910
6620:1RXS J160929.1−210524
4989:Astrophysical Journal
4617:10.1093/mnras/stab018
4369:Schaaf, Fred (2008).
4141:Pease, F. G. (1921).
4114:(1576): x–xiv. 1925.
3455:. Sky & Telescope
3183:Dawes, W. R. (1856).
2752:Liddell, Henry George
2528:Astrophysical Journal
2208:Vizier database entry
1904:. Rēhua is father of
1705:
1618:in the constellation
1564:, making it the then
1456:effective temperature
1447:, or 11 to 14.3
1420:bolometric luminosity
1371:
1330:apart in 1847–49, or
1223:first magnitude stars
1212:
1120:
1022:Its traditional name
987:and HD 148478 in the
985:Bright Star Catalogue
981:Flamsteed designation
947:
911:Its traditional name
666:Alpha Sco, α Sco
4793:Percy, John (2014).
4553:"Oldsmobile Antares"
1981:Behenian fixed stars
1932:) as the brother of
1454:. Comparison of the
1347:projected separation
1157:William Rutter Dawes
1035:, meaning "rival to
924:, meaning "rival to
898:projected separation
6811:OGLE-2007-BLG-368Lb
6806:OGLE-2005-BLG-390Lb
6801:OGLE-2005-BLG-071Lb
6515:HIP 79431 (Sharjah)
5098:Articles and images
5034:1995ApJ...440L..93B
5001:1996ApJ...463..336B
4963:1998Sci...279..844J
4899:2001ApJ...548..861M
4866:2010NewA...15..646S
4827:2013ApJ...777...10P
4723:10.1038/nature23445
4715:2017Natur.548..310O
4631:Sky & Telescope
4608:2021MNRAS.502..369C
4453:2009iscc.book..155L
4410:1998JBAA..108....9R
4338:1999MNRAS.310..355W
4265:2014ApJ...789...29F
4206:2009ASPC..412..113W
4159:1921PASP...33..204P
4053:2013AJ....145...38P
4001:2004MNRAS.350..365I
3960:2010Obs...130..167H
3922:10.1051/aas:1997181
3873:1990AJ.....99..965M
3842:2015JDSO...11...81A
3807:2006SouSt..45c..14G
3770:2001AJ....122.3466M
3658:10.2298/SAJ0570073P
3649:2005SerAJ.170...73P
3550:2008AN....329...10M
3534:(1). Wiley: 10–14.
3390:on 4 November 2012.
3322:2018AuJAn..29...89H
3285:2009JRASC.103...11P
3238:1952Obs....72...86C
3201:1856MNRAS..16..143D
3096:1879Obs.....3...84J
3005:1916ApJ....44..250L
2970:1907ApJ....25...58W
2770:, Tufts University.
2731:2009yCat....102025S
2550:2012ApJ...746..154P
2491:2022MNRAS.516..693N
2331:1967IAUS...30...57E
2240:1989ApJS...71..245K
2203:1995yCat.5050....0H
2143:2006MNRAS.372.1721K
1142:James William Grant
900:of about 79.1
854:in its foreground.
742:Database references
637:Rotational velocity
496:Rotational velocity
28:
7113:Population I stars
7093:M-type supergiants
6575:OGLE-2006-BLG-109L
6570:OGLE-2005-BLG-390L
6565:OGLE-2005-BLG-071L
4501:Mudrooroo (1994).
3383:The Times of India
3330:10.1111/taja.12257
2008:. Merriam-Webster.
1971:Oldsmobile Antares
1708:
1566:largest star known
1519:lunar occultations
1377:
1351:astronomical units
1338: –
1215:
1175:apparent magnitude
1138:Johann Tobias Bürg
1123:
979:. Antares has the
966:
657:Other designations
464:−0.1 to −0.2
333:(approx. 170
293: −23.30
281: −12.11
231:Variable type
202:M1.5Iab-Ib + B2.5V
197:Spectral type
26:
7153:Hipparcos objects
7143:Flamsteed objects
7080:
7079:
7062:
7061:
7017:
7016:
6963:
6962:
6834:
6833:
6743:
6742:
6580:Oph 162225-240515
6550:MOA-2008-BLG-310L
4957:(5352): 844–847.
4699:(7667): 310–312.
4512:978-1-85538-306-7
4487:978-1-77550-325-5
4382:978-0-471-70410-2
4294:(June 26, 2009).
3438:978-0-7136-7939-7
3411:978-1-345-66291-7
3150:978-1-376-84608-9
2820:978-1-138-05047-1
2793:978-0-14-019287-2
2703:978-0-486-21079-7
2363:978-1-4419-1052-3
2030:978-1-931559-44-7
1887:
1379:Antares is a red
1290:illuminated cloud
1210:
1153:Ormsby M. Mitchel
1026:derives from the
991:. As a prominent
977:Bayer designation
952:(lower left) and
915:derives from the
797:Bayer designation
783:is the brightest
778:
777:
328:approx. 550
7165:
7072:
7071:
7028:
6974:
6847:
6749:
5219:
5181:
5174:
5167:
5158:
5149:
5148:
5147:
5137:
5136:
5125:
5124:
5123:
5116:
5047:
5045:
5012:
4982:
4941:
4920:
4910:
4877:
4848:
4838:
4805:
4803:
4802:
4789:
4763:
4742:
4708:
4687:
4661:
4640:
4638:
4637:
4621:
4619:
4601:
4567:
4566:
4564:
4563:
4549:
4543:
4542:
4540:
4538:
4533:on July 16, 2011
4523:
4517:
4516:
4498:
4492:
4491:
4470:
4464:
4463:
4461:
4446:
4435:
4429:
4428:
4420:
4414:
4413:
4393:
4387:
4386:
4366:
4360:
4359:
4349:
4317:
4311:
4310:
4308:
4306:
4288:
4279:
4278:
4276:
4244:
4238:
4237:
4216:
4210:
4209:
4193:
4187:
4186:
4153:(194): 204–205.
4138:
4132:
4131:
4100:
4094:
4093:
4073:
4067:
4066:
4064:
4032:
4023:
4022:
4012:
3994:
3992:astro-ph/0402326
3970:
3964:
3963:
3943:
3934:
3933:
3893:
3887:
3886:
3884:
3852:
3846:
3845:
3825:
3819:
3818:
3790:
3784:
3783:
3781:
3764:(6): 3466–3471.
3749:
3743:
3742:
3716:
3696:
3690:
3689:
3669:
3663:
3662:
3660:
3628:
3619:
3618:
3616:
3584:
3578:
3577:
3543:
3523:
3517:
3516:
3490:
3470:
3464:
3463:
3461:
3460:
3449:
3443:
3442:
3422:
3416:
3415:
3398:
3392:
3391:
3374:
3368:
3367:
3365:
3363:
3348:
3342:
3341:
3315:
3295:
3289:
3288:
3268:
3262:
3261:
3259:
3258:
3248:
3242:
3241:
3221:
3215:
3214:
3212:
3180:
3171:
3170:
3161:
3155:
3154:
3134:
3121:
3120:
3106:
3100:
3099:
3079:
3070:
3069:
3061:
3050:
3049:
3047:
3023:
3017:
3016:
2988:
2982:
2981:
2953:
2947:
2935:
2933:
2932:
2916:
2907:
2906:
2904:
2902:
2892:
2886:
2885:
2883:
2881:
2875:
2868:
2860:
2854:
2853:
2851:
2849:
2839:
2833:
2832:
2804:
2798:
2797:
2777:
2771:
2748:
2747:
2741:
2735:
2734:
2714:
2708:
2707:
2680:
2661:
2660:
2634:
2632:astro-ph/0702172
2614:
2608:
2607:
2587:
2570:
2569:
2543:
2522:
2505:
2504:
2502:
2484:
2460:
2449:
2448:
2422:
2401:
2376:
2375:
2341:
2335:
2334:
2314:
2308:
2307:
2305:
2273:
2260:
2259:
2223:
2214:
2206:
2186:
2173:
2172:
2154:
2136:
2134:astro-ph/0608438
2127:(4): 1721–1734.
2112:
2099:
2098:
2072:
2052:
2035:
2034:
2016:
2010:
2009:
1996:
1888:
1885:
1881:
1872:
1806:
1764:
1756:
1750:
1749:
1740:
1732:
1658:
1629:
1601:VY Canis Majoris
1583:
1581:
1551:Francis G. Pease
1544:
1542:
1536:
1534:
1430:and 97,700
1399:) from the Sun.
1359:
1345:The pair have a
1341:
1337:
1333:
1329:
1318:
1237:), so it can be
1211:
1184:
1182:
1034:
1033:
1007:J16294-2626 and
975:) is the star's
948:Antares between
923:
922:
708:
701:
678:
528:
526:
485:
483:
438:
437:
436:
435:
430:
424:
354:−5.28 (variable)
292:
280:
203:
179:Characteristics
171:
151:
146:
133:
127:
126:
123:
122:
119:
116:
113:
110:
107:
104:
61:Observation data
48:
41:
29:
7173:
7172:
7168:
7167:
7166:
7164:
7163:
7162:
7083:
7082:
7081:
7076:
7058:
7042:
7013:
6959:
6928:
6841:
6830:
6739:
6660:Trumpler 27-105
6655:Trumpler 27-102
6530:IRAS 17163−3907
6525:IGR J17252−3616
6520:IGR J17091-3624
6490:GSC 06214-00210
6485:GCRT J1745−3009
6438:
6409:153950 (Rapeto)
6355:
5872:
5464:
5391:
5208:
5190:
5185:
5155:
5145:
5143:
5131:
5121:
5119:
5111:
5108:
5055:
5050:
5015:
4985:
4944:
4923:
4880:
4851:
4808:
4800:
4798:
4792:
4745:
4690:
4643:
4635:
4633:
4624:
4579:
4575:
4573:Further reading
4570:
4561:
4559:
4551:
4550:
4546:
4536:
4534:
4525:
4524:
4520:
4513:
4500:
4499:
4495:
4488:
4472:
4471:
4467:
4459:
4447:. p. 162.
4444:
4437:
4436:
4432:
4422:
4421:
4417:
4395:
4394:
4390:
4383:
4368:
4367:
4363:
4319:
4318:
4314:
4304:
4302:
4290:
4289:
4282:
4246:
4245:
4241:
4218:
4217:
4213:
4195:
4194:
4190:
4140:
4139:
4135:
4102:
4101:
4097:
4075:
4074:
4070:
4034:
4033:
4026:
3972:
3971:
3967:
3948:The Observatory
3945:
3944:
3937:
3895:
3894:
3890:
3854:
3853:
3849:
3827:
3826:
3822:
3792:
3791:
3787:
3751:
3750:
3746:
3698:
3697:
3693:
3671:
3670:
3666:
3630:
3629:
3622:
3586:
3585:
3581:
3525:
3524:
3520:
3472:
3471:
3467:
3458:
3456:
3451:
3450:
3446:
3439:
3424:
3423:
3419:
3412:
3400:
3399:
3395:
3376:
3375:
3371:
3361:
3359:
3350:
3349:
3345:
3297:
3296:
3292:
3270:
3269:
3265:
3256:
3254:
3250:
3249:
3245:
3226:The Observatory
3223:
3222:
3218:
3182:
3181:
3174:
3163:
3162:
3158:
3151:
3136:
3135:
3124:
3108:
3107:
3103:
3084:The Observatory
3081:
3080:
3073:
3063:
3062:
3053:
3025:
3024:
3020:
2990:
2989:
2985:
2955:
2954:
2950:
2930:
2928:
2918:
2917:
2910:
2900:
2898:
2894:
2893:
2889:
2879:
2877:
2873:
2866:
2862:
2861:
2857:
2847:
2845:
2841:
2840:
2836:
2821:
2806:
2805:
2801:
2794:
2779:
2778:
2774:
2742:
2738:
2716:
2715:
2711:
2704:
2682:
2681:
2664:
2616:
2615:
2611:
2589:
2588:
2573:
2524:
2523:
2508:
2462:
2461:
2452:
2403:
2402:
2379:
2364:
2346:The Rainbow Sky
2343:
2342:
2338:
2316:
2315:
2311:
2275:
2274:
2263:
2225:
2224:
2217:
2188:
2187:
2176:
2114:
2113:
2102:
2054:
2053:
2038:
2031:
2018:
2017:
2013:
1998:
1997:
1993:
1989:
1952:
1946:
1748:Καρδία Σκορπίου
1700:
1688:contrast effect
1665:
1662:
1653:
1650:
1647:
1636:
1627:
1597:
1594:
1590:
1587:
1579:
1577:
1563:
1560:
1540:
1538:
1532:
1530:
1523:milliarcseconds
1508:radial velocity
1489:
1486:
1478:
1475:
1471:
1468:
1464:
1461:
1453:
1450:
1446:
1443:
1436:
1433:
1429:
1426:
1381:supergiant star
1366:
1354:
1339:
1335:
1331:
1327:
1313:
1310:semi-major axis
1300:α Scorpii is a
1298:
1266:
1204:
1202:
1194:South Australia
1180:
1178:
1159:in April 1847.
1126:Radial velocity
1115:
1089:
942:
886:that of the Sun
864:, Antares is a
709:
703:
696:
673:
643: sin
602:Surface gravity
594:
591:
576:
573:
556:
553:
524:
522:
502: sin
481:
479:
454:Surface gravity
446:
443:
433:
431:
428:
426:
425:
422:
420:
407:
404:
387:
384:
349:
332:
289:
260:
255:Radial velocity
201:
166:
149:
144:Right ascension
142:
131:
101:
97:
62:
56:
54:
53:
52:
51:
50:
49:
24:
17:
12:
11:
5:
7171:
7169:
7161:
7160:
7155:
7150:
7145:
7140:
7135:
7130:
7125:
7120:
7118:Upper Scorpius
7115:
7110:
7105:
7100:
7095:
7085:
7084:
7078:
7077:
7067:
7064:
7063:
7060:
7059:
7057:
7056:
7050:
7048:
7044:
7043:
7041:
7040:
7034:
7032:
7025:
7019:
7018:
7015:
7014:
7012:
7011:
7006:
7001:
6996:
6991:
6986:
6980:
6978:
6971:
6965:
6964:
6961:
6960:
6958:
6957:
6952:
6947:
6942:
6936:
6934:
6930:
6929:
6927:
6926:
6921:
6916:
6911:
6906:
6901:
6896:
6891:
6886:
6881:
6876:
6871:
6866:
6861:
6855:
6853:
6844:
6836:
6835:
6832:
6831:
6829:
6828:
6826:V921 Scorpii b
6823:
6818:
6813:
6808:
6803:
6798:
6793:
6788:
6783:
6778:
6773:
6768:
6763:
6757:
6755:
6745:
6744:
6741:
6740:
6738:
6737:
6732:
6727:
6722:
6717:
6712:
6707:
6705:WASP-17 (Dìwö)
6702:
6697:
6692:
6687:
6682:
6677:
6672:
6667:
6662:
6657:
6652:
6650:Trumpler 27-28
6647:
6645:Trumpler 27-27
6642:
6637:
6632:
6627:
6622:
6617:
6612:
6607:
6605:PSR J1614−2230
6602:
6597:
6592:
6587:
6582:
6577:
6572:
6567:
6562:
6557:
6552:
6547:
6542:
6537:
6532:
6527:
6522:
6517:
6512:
6507:
6502:
6497:
6492:
6487:
6482:
6480:EPIC 204376071
6477:
6475:EPIC 204278916
6472:
6467:
6462:
6457:
6452:
6446:
6444:
6440:
6439:
6437:
6436:
6431:
6426:
6421:
6416:
6411:
6406:
6401:
6396:
6391:
6386:
6381:
6376:
6371:
6365:
6363:
6357:
6356:
6354:
6353:
6348:
6343:
6338:
6333:
6328:
6323:
6318:
6313:
6308:
6303:
6298:
6293:
6288:
6283:
6278:
6273:
6268:
6263:
6258:
6253:
6248:
6243:
6238:
6233:
6228:
6223:
6218:
6213:
6208:
6203:
6198:
6193:
6188:
6183:
6178:
6173:
6168:
6163:
6158:
6153:
6148:
6143:
6138:
6133:
6128:
6123:
6118:
6113:
6108:
6103:
6098:
6093:
6088:
6083:
6078:
6073:
6068:
6063:
6058:
6053:
6048:
6043:
6038:
6033:
6028:
6023:
6018:
6013:
6008:
6003:
5998:
5993:
5988:
5983:
5978:
5973:
5968:
5963:
5958:
5953:
5948:
5943:
5938:
5933:
5928:
5923:
5918:
5913:
5908:
5903:
5898:
5893:
5888:
5882:
5880:
5874:
5873:
5871:
5870:
5865:
5860:
5855:
5850:
5845:
5840:
5835:
5830:
5825:
5820:
5815:
5810:
5805:
5800:
5795:
5790:
5785:
5780:
5775:
5770:
5765:
5760:
5755:
5750:
5745:
5740:
5735:
5730:
5725:
5720:
5715:
5710:
5705:
5700:
5695:
5690:
5685:
5680:
5675:
5670:
5665:
5660:
5655:
5650:
5645:
5640:
5635:
5630:
5625:
5620:
5615:
5610:
5605:
5600:
5595:
5590:
5585:
5580:
5575:
5570:
5565:
5560:
5555:
5550:
5545:
5540:
5535:
5530:
5525:
5520:
5515:
5510:
5505:
5500:
5495:
5490:
5485:
5480:
5474:
5472:
5466:
5465:
5463:
5462:
5457:
5452:
5447:
5442:
5437:
5432:
5427:
5422:
5417:
5412:
5407:
5401:
5399:
5393:
5392:
5390:
5389:
5384:
5375:
5366:
5361:
5356:
5351:
5346:
5341:
5336:
5334:τ (Paikauhale)
5331:
5326:
5321:
5316:
5311:
5306:
5301:
5296:
5294:μ (Xamidimura)
5291:
5286:
5278:
5273:
5268:
5263:
5258:
5253:
5248:
5243:
5238:
5233:
5227:
5225:
5216:
5210:
5209:
5207:
5206:
5201:
5195:
5192:
5191:
5186:
5184:
5183:
5176:
5169:
5161:
5154:
5153:
5141:
5129:
5106:
5105:
5100:
5058:
5054:
5053:External links
5051:
5049:
5048:
5043:10.1086/187769
5013:
5009:10.1086/177246
4983:
4942:
4921:
4908:10.1086/319035
4893:(2): 861–867.
4878:
4860:(7): 646–651.
4849:
4806:
4790:
4743:
4688:
4641:
4622:
4592:(1): 369–382.
4576:
4574:
4571:
4569:
4568:
4544:
4518:
4511:
4493:
4486:
4474:Matamua, Rangi
4465:
4430:
4415:
4388:
4381:
4361:
4332:(2): 355–359.
4312:
4280:
4239:
4211:
4188:
4167:10.1086/123081
4133:
4104:"Science News"
4095:
4084:(2): 355–362.
4068:
4024:
3985:(1): 365–374.
3965:
3935:
3888:
3882:10.1086/115387
3847:
3820:
3795:Southern Stars
3785:
3779:10.1086/323920
3744:
3707:(1): 229–238.
3691:
3664:
3643:(170): 73–78.
3620:
3579:
3518:
3465:
3444:
3437:
3417:
3410:
3393:
3369:
3358:on 5 July 2009
3343:
3290:
3263:
3243:
3216:
3172:
3156:
3149:
3122:
3101:
3071:
3051:
3038:(8): 660–679.
3018:
3013:10.1086/142291
2983:
2978:10.1086/141419
2948:
2908:
2887:
2855:
2834:
2819:
2799:
2792:
2772:
2736:
2709:
2702:
2662:
2625:(2): 593–601.
2609:
2571:
2506:
2475:(1): 693–719.
2450:
2377:
2362:
2336:
2309:
2288:(1): 229–237.
2261:
2248:10.1086/191373
2215:
2174:
2100:
2063:(2): 653–664.
2036:
2029:
2011:
1990:
1988:
1985:
1956:flag of Brazil
1945:
1942:
1846:lunar mansions
1754:Kardia Skorpiū
1699:
1696:
1663:
1660:
1648:
1645:
1635:
1632:
1626:, probably in
1595:
1592:
1588:
1585:
1561:
1558:
1515:interferometry
1487:
1484:
1476:
1473:
1469:
1466:
1462:
1459:
1451:
1448:
1444:
1441:
1434:
1431:
1427:
1424:
1365:
1362:
1297:
1296:Stellar system
1294:
1274:OB association
1272:, the nearest
1265:
1262:
1221:, one of four
1201:
1198:
1114:
1111:
1088:
1085:
971:(Latinised to
941:
938:
866:red supergiant
857:Classified as
840:OB association
838:, the nearest
776:
775:
770:
767:
766:
761:
758:
757:
752:
744:
743:
739:
738:
727:
726:
721: 148478,
711:
710:
695: 184415,
663:
660:
659:
653:
652:
649:
632:
631:
625:
617:
616:
610:
597:
596:
592:
589:
585:
579:
578:
574:
571:
567:
559:
558:
554:
551:
547:
539:
538:
534:
533:
520:
512:
511:
508:
491:
490:
477:
469:
468:
462:
449:
448:
444:
441:
418:
410:
409:
405:
402:
398:
390:
389:
385:
382:
378:
370:
369:
365:
364:
360:
359:
356:
355:
352:
347:
339:
338:
326:
318:
317:
311:
302:
301:
276:
267:
266:
265:−3.4 km/s
263:
258:
250:
249:
246:
245:
239:
238:
233:
227:
226:
223:
216:
215:
212:
205:
204:
199:
193:
192:
190:Red supergiant
187:
181:
180:
176:
175:
174:0.6–1.6 + 5.5
172:
163:
162:
159:
153:
152:
150:16 29 24.45970
147:
139:
138:
95:
89:
88:
83:
77:
76:
58:
57:
43:
42:
36:
35:
34:
33:
32:
15:
13:
10:
9:
6:
4:
3:
2:
7170:
7159:
7156:
7154:
7151:
7149:
7146:
7144:
7141:
7139:
7136:
7134:
7133:Bayer objects
7131:
7129:
7126:
7124:
7121:
7119:
7116:
7114:
7111:
7109:
7106:
7104:
7101:
7099:
7096:
7094:
7091:
7090:
7088:
7075:
7065:
7055:
7052:
7051:
7049:
7045:
7039:
7036:
7035:
7033:
7029:
7026:
7024:
7020:
7010:
7007:
7005:
7002:
7000:
6997:
6995:
6992:
6990:
6987:
6985:
6982:
6981:
6979:
6975:
6972:
6970:
6966:
6956:
6953:
6951:
6948:
6946:
6943:
6941:
6938:
6937:
6935:
6931:
6925:
6922:
6920:
6917:
6915:
6912:
6910:
6907:
6905:
6902:
6900:
6897:
6895:
6892:
6890:
6887:
6885:
6882:
6880:
6877:
6875:
6872:
6870:
6867:
6865:
6862:
6860:
6857:
6856:
6854:
6852:
6848:
6845:
6843:
6837:
6827:
6824:
6822:
6819:
6817:
6814:
6812:
6809:
6807:
6804:
6802:
6799:
6797:
6794:
6792:
6789:
6787:
6784:
6782:
6779:
6777:
6774:
6772:
6769:
6767:
6764:
6762:
6759:
6758:
6756:
6754:
6750:
6746:
6736:
6735:XTE J1751−305
6733:
6731:
6730:XTE J1739−302
6728:
6726:
6725:XTE J1720−318
6723:
6721:
6718:
6716:
6713:
6711:
6708:
6706:
6703:
6701:
6698:
6696:
6693:
6691:
6688:
6686:
6683:
6681:
6678:
6676:
6673:
6671:
6668:
6666:
6663:
6661:
6658:
6656:
6653:
6651:
6648:
6646:
6643:
6641:
6640:Trumpler 27-1
6638:
6636:
6633:
6631:
6628:
6626:
6623:
6621:
6618:
6616:
6613:
6611:
6610:Rapid Burster
6608:
6606:
6603:
6601:
6598:
6596:
6593:
6591:
6588:
6586:
6583:
6581:
6578:
6576:
6573:
6571:
6568:
6566:
6563:
6561:
6558:
6556:
6553:
6551:
6548:
6546:
6543:
6541:
6538:
6536:
6533:
6531:
6528:
6526:
6523:
6521:
6518:
6516:
6513:
6511:
6508:
6506:
6503:
6501:
6498:
6496:
6493:
6491:
6488:
6486:
6483:
6481:
6478:
6476:
6473:
6471:
6468:
6466:
6463:
6461:
6458:
6456:
6453:
6451:
6448:
6447:
6445:
6441:
6435:
6432:
6430:
6427:
6425:
6422:
6420:
6417:
6415:
6412:
6410:
6407:
6405:
6402:
6400:
6397:
6395:
6392:
6390:
6387:
6385:
6382:
6380:
6377:
6375:
6372:
6370:
6367:
6366:
6364:
6362:
6358:
6352:
6349:
6347:
6344:
6342:
6339:
6337:
6334:
6332:
6329:
6327:
6324:
6322:
6319:
6317:
6314:
6312:
6309:
6307:
6304:
6302:
6299:
6297:
6294:
6292:
6289:
6287:
6284:
6282:
6279:
6277:
6274:
6272:
6269:
6267:
6264:
6262:
6259:
6257:
6254:
6252:
6249:
6247:
6244:
6242:
6239:
6237:
6234:
6232:
6229:
6227:
6224:
6222:
6219:
6217:
6214:
6212:
6209:
6207:
6204:
6202:
6199:
6197:
6194:
6192:
6189:
6187:
6184:
6182:
6179:
6177:
6174:
6172:
6169:
6167:
6164:
6162:
6159:
6157:
6154:
6152:
6149:
6147:
6144:
6142:
6139:
6137:
6134:
6132:
6129:
6127:
6124:
6122:
6119:
6117:
6114:
6112:
6109:
6107:
6104:
6102:
6099:
6097:
6094:
6092:
6089:
6087:
6084:
6082:
6079:
6077:
6074:
6072:
6069:
6067:
6064:
6062:
6059:
6057:
6054:
6052:
6049:
6047:
6044:
6042:
6039:
6037:
6034:
6032:
6029:
6027:
6024:
6022:
6019:
6017:
6014:
6012:
6009:
6007:
6004:
6002:
5999:
5997:
5994:
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:
5907:
5904:
5902:
5899:
5897:
5894:
5892:
5889:
5887:
5884:
5883:
5881:
5879:
5875:
5869:
5866:
5864:
5861:
5859:
5856:
5854:
5851:
5849:
5846:
5844:
5841:
5839:
5836:
5834:
5831:
5829:
5826:
5824:
5821:
5819:
5816:
5814:
5811:
5809:
5806:
5804:
5801:
5799:
5796:
5794:
5791:
5789:
5786:
5784:
5781:
5779:
5776:
5774:
5771:
5769:
5766:
5764:
5761:
5759:
5756:
5754:
5751:
5749:
5746:
5744:
5741:
5739:
5736:
5734:
5731:
5729:
5726:
5724:
5721:
5719:
5716:
5714:
5711:
5709:
5706:
5704:
5701:
5699:
5696:
5694:
5691:
5689:
5686:
5684:
5681:
5679:
5676:
5674:
5671:
5669:
5666:
5664:
5661:
5659:
5656:
5654:
5651:
5649:
5646:
5644:
5641:
5639:
5636:
5634:
5631:
5629:
5626:
5624:
5621:
5619:
5616:
5614:
5611:
5609:
5606:
5604:
5601:
5599:
5596:
5594:
5591:
5589:
5586:
5584:
5581:
5579:
5576:
5574:
5571:
5569:
5566:
5564:
5561:
5559:
5556:
5554:
5551:
5549:
5546:
5544:
5541:
5539:
5536:
5534:
5531:
5529:
5526:
5524:
5521:
5519:
5516:
5514:
5511:
5509:
5506:
5504:
5501:
5499:
5496:
5494:
5491:
5489:
5486:
5484:
5481:
5479:
5476:
5475:
5473:
5471:
5467:
5461:
5458:
5456:
5453:
5451:
5448:
5446:
5443:
5441:
5438:
5436:
5433:
5431:
5428:
5426:
5423:
5421:
5418:
5416:
5413:
5411:
5408:
5406:
5403:
5402:
5400:
5398:
5394:
5388:
5385:
5383:
5381:
5376:
5374:
5372:
5367:
5365:
5362:
5360:
5357:
5355:
5352:
5350:
5347:
5345:
5342:
5340:
5337:
5335:
5332:
5330:
5327:
5325:
5322:
5320:
5317:
5315:
5312:
5310:
5307:
5305:
5302:
5300:
5297:
5295:
5292:
5290:
5287:
5285:
5284:
5279:
5277:
5274:
5272:
5269:
5267:
5264:
5262:
5259:
5257:
5254:
5252:
5249:
5247:
5244:
5242:
5239:
5237:
5234:
5232:
5229:
5228:
5226:
5224:
5220:
5217:
5215:
5211:
5205:
5202:
5200:
5197:
5196:
5193:
5189:
5182:
5177:
5175:
5170:
5168:
5163:
5162:
5159:
5152:
5142:
5140:
5135:
5130:
5128:
5118:
5114:
5109:
5104:
5101:
5099:
5095:
5091:
5087:
5083:
5079:
5075:
5071:
5067:
5063:
5059:
5057:
5056:
5052:
5044:
5039:
5035:
5031:
5027:
5023:
5019:
5014:
5010:
5006:
5002:
4998:
4994:
4990:
4984:
4980:
4976:
4972:
4968:
4964:
4960:
4956:
4952:
4948:
4943:
4939:
4935:
4931:
4927:
4922:
4918:
4914:
4909:
4904:
4900:
4896:
4892:
4888:
4884:
4879:
4875:
4871:
4867:
4863:
4859:
4855:
4854:New Astronomy
4850:
4846:
4842:
4837:
4832:
4828:
4824:
4820:
4816:
4812:
4807:
4796:
4791:
4787:
4783:
4779:
4775:
4771:
4767:
4762:
4757:
4753:
4749:
4744:
4740:
4736:
4732:
4728:
4724:
4720:
4716:
4712:
4707:
4702:
4698:
4694:
4689:
4685:
4681:
4677:
4673:
4669:
4665:
4660:
4655:
4651:
4647:
4642:
4632:
4628:
4623:
4618:
4613:
4609:
4605:
4600:
4595:
4591:
4587:
4583:
4578:
4577:
4572:
4558:
4554:
4548:
4545:
4532:
4528:
4522:
4519:
4514:
4508:
4504:
4497:
4494:
4489:
4483:
4479:
4475:
4469:
4466:
4458:
4454:
4450:
4443:
4442:
4434:
4431:
4426:
4419:
4416:
4411:
4407:
4403:
4399:
4392:
4389:
4384:
4378:
4374:
4373:
4365:
4362:
4357:
4353:
4348:
4343:
4339:
4335:
4331:
4327:
4323:
4316:
4313:
4301:
4297:
4293:
4287:
4285:
4281:
4275:
4270:
4266:
4262:
4258:
4254:
4250:
4243:
4240:
4235:
4231:
4227:
4223:
4215:
4212:
4207:
4203:
4199:
4192:
4189:
4184:
4180:
4176:
4172:
4168:
4164:
4160:
4156:
4152:
4148:
4144:
4137:
4134:
4129:
4125:
4121:
4117:
4113:
4109:
4105:
4099:
4096:
4091:
4087:
4083:
4079:
4072:
4069:
4063:
4058:
4054:
4050:
4046:
4042:
4038:
4031:
4029:
4025:
4020:
4016:
4011:
4006:
4002:
3998:
3993:
3988:
3984:
3980:
3976:
3969:
3966:
3961:
3957:
3953:
3949:
3942:
3940:
3936:
3931:
3927:
3923:
3919:
3915:
3911:
3907:
3903:
3899:
3892:
3889:
3883:
3878:
3874:
3870:
3866:
3862:
3858:
3851:
3848:
3843:
3839:
3835:
3831:
3824:
3821:
3816:
3812:
3808:
3804:
3800:
3796:
3789:
3786:
3780:
3775:
3771:
3767:
3763:
3759:
3755:
3748:
3745:
3740:
3736:
3732:
3728:
3724:
3720:
3715:
3710:
3706:
3702:
3695:
3692:
3687:
3683:
3679:
3675:
3668:
3665:
3659:
3654:
3650:
3646:
3642:
3638:
3634:
3627:
3625:
3621:
3615:
3610:
3606:
3602:
3598:
3594:
3590:
3583:
3580:
3575:
3571:
3567:
3563:
3559:
3555:
3551:
3547:
3542:
3537:
3533:
3529:
3522:
3519:
3514:
3510:
3506:
3502:
3498:
3494:
3489:
3484:
3480:
3476:
3469:
3466:
3454:
3448:
3445:
3440:
3434:
3430:
3429:
3421:
3418:
3413:
3407:
3403:
3397:
3394:
3389:
3385:
3384:
3379:
3373:
3370:
3357:
3353:
3347:
3344:
3339:
3335:
3331:
3327:
3323:
3319:
3314:
3309:
3305:
3301:
3294:
3291:
3286:
3282:
3278:
3274:
3267:
3264:
3253:
3247:
3244:
3239:
3235:
3231:
3227:
3220:
3217:
3211:
3206:
3202:
3198:
3194:
3190:
3186:
3179:
3177:
3173:
3168:
3167:
3160:
3157:
3152:
3146:
3142:
3141:
3133:
3131:
3129:
3127:
3123:
3118:
3114:
3113:
3105:
3102:
3097:
3093:
3089:
3085:
3078:
3076:
3072:
3067:
3060:
3058:
3056:
3052:
3046:
3041:
3037:
3033:
3029:
3022:
3019:
3014:
3010:
3006:
3002:
2998:
2994:
2987:
2984:
2979:
2975:
2971:
2967:
2963:
2959:
2952:
2949:
2946:
2942:
2938:
2927:on 2015-02-24
2926:
2922:
2915:
2913:
2909:
2897:
2891:
2888:
2872:
2865:
2859:
2856:
2844:
2838:
2835:
2830:
2826:
2822:
2816:
2813:. Routledge.
2812:
2811:
2803:
2800:
2795:
2789:
2785:
2784:
2776:
2773:
2769:
2765:
2761:
2757:
2756:Scott, Robert
2753:
2749:
2740:
2737:
2732:
2728:
2724:
2720:
2713:
2710:
2705:
2699:
2695:
2691:
2690:
2685:
2679:
2677:
2675:
2673:
2671:
2669:
2667:
2663:
2658:
2654:
2650:
2646:
2642:
2638:
2633:
2628:
2624:
2620:
2613:
2610:
2605:
2601:
2597:
2593:
2586:
2584:
2582:
2580:
2578:
2576:
2572:
2567:
2563:
2559:
2555:
2551:
2547:
2542:
2537:
2533:
2529:
2521:
2519:
2517:
2515:
2513:
2511:
2507:
2501:
2496:
2492:
2488:
2483:
2478:
2474:
2470:
2466:
2459:
2457:
2455:
2451:
2446:
2442:
2438:
2434:
2430:
2426:
2421:
2416:
2412:
2408:
2400:
2398:
2396:
2394:
2392:
2390:
2388:
2386:
2384:
2382:
2378:
2373:
2369:
2365:
2359:
2355:
2351:
2347:
2340:
2337:
2332:
2328:
2324:
2320:
2313:
2310:
2304:
2299:
2295:
2291:
2287:
2283:
2279:
2272:
2270:
2268:
2266:
2262:
2257:
2253:
2249:
2245:
2241:
2237:
2233:
2229:
2222:
2220:
2216:
2212:
2209:
2204:
2200:
2196:
2192:
2185:
2183:
2181:
2179:
2175:
2170:
2166:
2162:
2158:
2153:
2148:
2144:
2140:
2135:
2130:
2126:
2122:
2118:
2111:
2109:
2107:
2105:
2101:
2096:
2092:
2088:
2084:
2080:
2076:
2071:
2066:
2062:
2058:
2051:
2049:
2047:
2045:
2043:
2041:
2037:
2032:
2026:
2022:
2015:
2012:
2007:
2006:
2001:
1995:
1992:
1986:
1984:
1982:
1977:
1975:
1972:
1967:
1965:
1961:
1957:
1951:
1943:
1941:
1939:
1935:
1931:
1927:
1923:
1922:Marpean-kurrk
1919:
1915:
1911:
1907:
1903:
1899:
1895:
1890:
1882:
1876:
1868:
1864:
1863:Shang dynasty
1860:
1859:
1854:
1849:
1847:
1844:
1840:
1839:
1834:
1830:
1826:
1822:
1818:
1814:
1809:
1807:
1805:
1803:
1799:
1792:
1788:
1784:
1780:
1775:
1773:
1769:
1765:
1763:
1757:
1755:
1745:
1744:Ancient Greek
1741:
1739:
1738:Qalb al-Άqrab
1733:
1731:
1725:
1721:
1717:
1713:
1704:
1697:
1695:
1693:
1689:
1683:
1681:
1677:
1673:
1669:
1657:
1651:
1641:
1633:
1631:
1625:
1621:
1617:
1612:
1610:
1606:
1602:
1582:1.00 mas
1575:
1571:
1567:
1556:
1552:
1547:
1528:
1527:limb-darkened
1524:
1520:
1517:or observing
1516:
1511:
1509:
1503:
1501:
1497:
1493:
1482:
1457:
1438:
1421:
1417:
1413:
1409:
1405:
1400:
1398:
1394:
1390:
1386:
1382:
1374:
1370:
1363:
1361:
1358:
1352:
1349:of about 529
1348:
1343:
1324:
1322:
1317:
1311:
1307:
1306:binary system
1303:
1295:
1293:
1291:
1287:
1283:
1279:
1275:
1271:
1263:
1261:
1260:of the star.
1259:
1255:
1250:
1248:
1244:
1240:
1236:
1232:
1228:
1224:
1220:
1199:
1197:
1195:
1191:
1186:
1176:
1172:
1169:
1165:
1160:
1158:
1154:
1150:
1146:
1143:
1139:
1134:
1131:
1130:spectroscopic
1127:
1119:
1112:
1110:
1107:
1105:
1100:
1098:
1094:
1086:
1084:
1082:
1078:
1074:
1070:
1066:
1062:
1058:
1054:
1050:
1046:
1042:
1038:
1029:
1028:Ancient Greek
1025:
1020:
1018:
1014:
1010:
1006:
1002:
998:
994:
990:
986:
982:
978:
974:
973:Alpha Scorpii
970:
963:
960:false-colour
959:
955:
951:
946:
939:
937:
935:
931:
927:
918:
917:Ancient Greek
914:
909:
907:
903:
899:
895:
894:main sequence
891:
887:
883:
879:
875:
871:
870:largest stars
867:
863:
860:
859:spectral type
855:
853:
849:
845:
841:
837:
833:
829:
825:
821:
817:
813:
809:
808:Alpha Scorpii
805:
801:
798:
795:. It has the
794:
790:
789:constellation
786:
782:
774:
771:
769:
768:
765:
762:
760:
759:
756:
753:
751:
750:
746:
745:
740:
736:
732:
728:
725: 1623-26
724:
720:
716:
712:
706:
699:
694:
690:
687: 80763,
686:
682:
676:
671:
667:
661:
658:
654:
651:250 km/s
650:
648:
646:
642:
638:
634:
633:
630:
626:
624:
623:
619:
618:
615:
611:
609:
607:
603:
599:
598:
595:
586:
584:
581:
580:
577:
568:
566:
565:
561:
560:
557:
548:
546:
545:
541:
540:
535:
532:
521:
519:
518:
514:
513:
509:
507:
505:
501:
497:
493:
492:
489:
478:
476:
475:
471:
470:
467:
463:
461:
459:
455:
451:
450:
447:
419:
417:
416:
412:
411:
408:
399:
397:
396:
392:
391:
388:
379:
377:
376:
372:
371:
366:
361:
357:
353:
351:
345:
341:
340:
336:
331:
327:
325:
324:
320:
319:
316:
312:
310:
308:
304:
303:
300:
296:
288:
284:
277:
275:
273:
272:Proper motion
269:
268:
264:
262:
256:
252:
251:
247:
244:
240:
237:
234:
232:
229:
228:
224:
222:
218:
217:
213:
211:
207:
206:
200:
198:
195:
194:
191:
188:
186:
183:
182:
177:
173:
169:
165:
164:
160:
158:
155:
154:
148:
145:
141:
140:
136:
135:
125:
96:
94:
93:Pronunciation
91:
90:
87:
84:
82:
81:Constellation
79:
78:
75:
72:
68:
65:
59:
47:
40:
30:
22:
7103:Binary stars
7054:TXS 1545-234
6695:UScoCTIO 108
6630:Scorpius X-1
6600:PSR B1737−30
6595:PSR B1706−44
6590:PSR B1620−26
6560:OAO 1657-415
6470:CD -38 10980
6465:CD -35 11760
5379:
5370:
5299:μ (Pipirima)
5282:
5241:δ (Dschubba)
5230:
5107:
5025:
5021:
4992:
4988:
4954:
4950:
4929:
4925:
4890:
4886:
4857:
4853:
4818:
4814:
4799:. Retrieved
4751:
4747:
4696:
4692:
4649:
4645:
4634:. Retrieved
4630:
4589:
4585:
4560:. Retrieved
4556:
4547:
4537:November 14,
4535:. Retrieved
4531:the original
4521:
4502:
4496:
4477:
4468:
4440:
4433:
4424:
4418:
4401:
4397:
4391:
4371:
4364:
4329:
4325:
4315:
4303:. Retrieved
4299:
4292:Kaler, James
4256:
4252:
4242:
4225:
4221:
4214:
4197:
4191:
4150:
4146:
4136:
4111:
4107:
4098:
4081:
4077:
4071:
4044:
4040:
3982:
3978:
3968:
3951:
3947:
3908:(1): 75–84.
3905:
3901:
3891:
3864:
3860:
3850:
3833:
3829:
3823:
3798:
3794:
3788:
3761:
3757:
3747:
3704:
3700:
3694:
3677:
3673:
3667:
3640:
3636:
3596:
3592:
3582:
3531:
3527:
3521:
3478:
3474:
3468:
3457:. Retrieved
3447:
3427:
3420:
3401:
3396:
3388:the original
3381:
3372:
3360:. Retrieved
3356:the original
3346:
3303:
3299:
3293:
3276:
3272:
3266:
3255:. Retrieved
3246:
3229:
3225:
3219:
3192:
3188:
3165:
3159:
3139:
3111:
3104:
3087:
3083:
3065:
3035:
3031:
3021:
2996:
2992:
2986:
2961:
2957:
2951:
2929:. Retrieved
2925:the original
2899:. Retrieved
2890:
2878:. Retrieved
2858:
2846:. Retrieved
2837:
2809:
2802:
2782:
2775:
2759:
2739:
2722:
2718:
2712:
2688:
2622:
2618:
2612:
2595:
2591:
2531:
2527:
2472:
2468:
2410:
2406:
2345:
2339:
2322:
2318:
2312:
2285:
2281:
2231:
2227:
2194:
2190:
2124:
2120:
2060:
2056:
2020:
2014:
2003:
1994:
1978:
1968:
1953:
1933:
1929:
1921:
1917:
1906:Puanga/Puaka
1905:
1897:
1894:Māori people
1891:
1878:
1856:
1852:
1850:
1836:
1810:
1801:
1797:
1794:
1776:
1759:
1751:
1735:
1727:
1709:
1692:occultations
1684:
1654:18,500
1637:
1613:
1572:satellite's
1548:
1537:in 2009 and
1512:
1504:
1439:
1423:75,900
1414:part of the
1401:
1378:
1344:
1325:
1321:Kepler's Law
1299:
1267:
1257:
1251:
1216:
1190:Ngarrindjeri
1187:
1173:star, whose
1167:
1161:
1135:
1124:
1108:
1101:
1090:
1080:
1075:organised a
1023:
1021:
972:
968:
967:
940:Nomenclature
912:
910:
874:Solar System
856:
807:
799:
780:
779:
747:
737: 148479
730:
714:
691: 6134,
644:
640:
635:
627:18,500
620:
605:
600:
582:
562:
542:
515:
510:20 km/s
503:
499:
494:
472:
457:
452:
413:
393:
373:
342:
321:
305:
270:
253:
7158:TIC objects
6955:Trumpler 27
6781:HIP 79431 b
6776:HIP 78530 b
6771:HD 159868 b
6766:HD 153950 b
6761:HD 145377 b
6690:4U 1746-371
6680:4U 1724-307
6585:Pismis 24-1
6555:MXB 1735-44
5329:σ (Alniyat)
5246:ε (Larawag)
5231:α (Antares)
5151:Outer space
5060:Antares on
4932:: 605–610.
4404:(1): 9–28.
4228:: L49–L52.
2684:Allen, R.H.
1974:concept car
1817:royal stars
1779:Mesopotamia
1777:In ancient
1762:Cor Scorpii
1730:Calbalakrab
1678:similar to
1676:white dwarf
1605:VV Cephei A
1418:, the true
1393:light-years
1302:double star
1247:lunar nodes
1104:conjunction
1087:Observation
890:binary star
802:, which is
773:α Scorpii B
764:α Scorpii A
700:J16294-2626
683: 616,
670:21 Sco
622:Temperature
587:2,754
474:Temperature
380:11–16
221:color index
210:color index
157:Declination
7087:Categories
6950:Messier 80
6753:Exoplanets
6720:Wray 17-96
6700:VVV-WIT-07
6685:4U 1728-34
6675:4U 1705-44
6670:4U 1702-42
6665:4U 1700-37
6460:Gliese 682
6455:Gliese 667
6450:Gliese 618
5339:υ (Lesath)
5304:ν (Jabbah)
5289:λ (Shaula)
5266:θ (Sargas)
5090:Astrophoto
5082:Hydrogen α
4801:2019-06-01
4706:1708.06372
4659:2006.08023
4636:2022-08-27
4599:2101.02785
4562:2024-07-26
3954:(3): 167.
3488:2006.14649
3481:(7): 112.
3459:2022-08-27
3313:1709.04634
3306:: 89–107.
3257:2019-06-08
2931:2011-12-01
2829:1054505486
2534:(2): 154.
2482:2207.04702
1987:References
1948:See also:
1944:In culture
1823:, it with
1628:1.0 to 1.4
1616:Betelgeuse
1500:supernovae
1404:brightness
1323:estimate.
1280:(550
1093:opposition
1065:Mu'allaqat
904:(529
862:M1.5Iab-Ib
846:(550
707:16294-2626
604:(log
583:Luminosity
456:(log
415:Luminosity
243:Astrometry
6945:Messier 7
6940:Messier 4
6510:H1743-322
5813:V1073 (k)
5397:Flamsteed
5364:G (Fuyue)
5324:ρ (Iklil)
5236:β (Acrab)
5127:Astronomy
4917:120293812
4845:120406829
4821:(1): 10.
4761:1407.0715
4684:219484950
4356:0035-8711
4305:13 August
4296:"Antares"
4259:(1): 11.
4175:0004-6280
4120:0036-8075
3930:0365-0138
3836:(2): 81.
3815:0049-1640
3801:(3): 14.
3714:0809.4605
3566:0004-6337
3541:0709.0505
3513:220128144
3338:119453488
3279:(1): 11.
2750: in
2566:118461108
2541:1112.1695
2420:1304.4800
2372:1431-9756
2256:123149047
2161:0035-8711
2070:0708.1752
2000:"Antares"
1969:The 1995
1920:, son of
1853:Xīnxiù'èr
1838:nakshatra
1829:τ Scorpii
1825:σ Scorpii
1672:red giant
1668:supernova
1634:Antares B
1624:supernova
1609:Mu Cephei
1570:Hipparcos
1481:blue loop
1355:220
1312:of about
1235:Aldebaran
1147:while in
969:α Scorpii
954:σ Scorpii
832:night sky
816:τ Scorpii
812:σ Scorpii
804:Latinised
800:α Scorpii
677:−26°11359
612:3.9
569:5.2
549:7.2
170: (V)
7123:Scorpius
7074:Category
7023:Galaxies
6842:clusters
6821:WASP-17b
6545:LSS 4067
6500:GX 349+2
6495:GX 340+0
5996:6070 (d)
5470:Variable
5319:π (Fang)
5283:(Girtab)
4786:62795432
4731:28816248
4478:Matariki
4476:(2018).
4457:Archived
4183:40671460
4047:(2): 4.
4019:15830460
3739:18620644
3574:14027548
3362:2 August
2871:Archived
2686:(1963).
2657:55901104
2445:56396587
2095:18759600
1930:Balayang
1926:Arcturus
1902:Matariki
1833:Jyeshthā
1716:MUL.APIN
1680:Sirius B
1664:☉
1649:☉
1596:☉
1589:☉
1562:☉
1488:☉
1477:☉
1470:☉
1463:☉
1452:☉
1445:☉
1435:☉
1428:☉
1416:spectrum
1412:infrared
1389:parallax
1239:occulted
1219:ecliptic
1069:Almagest
993:infrared
962:infrared
793:Scorpius
593:☉
575:☉
555:☉
445:☉
406:☉
386:☉
346: (M
323:Distance
307:Parallax
86:Scorpius
27:Antares
6969:Nebulae
6615:ROXs 12
5113:Portals
5094:Sky Map
5062:WikiSky
5030:Bibcode
5028:: L93.
4997:Bibcode
4995:: 336.
4979:9452380
4959:Bibcode
4951:Science
4934:Bibcode
4895:Bibcode
4862:Bibcode
4823:Bibcode
4797:. AAVSO
4766:Bibcode
4754:: A17.
4739:4458627
4711:Bibcode
4664:Bibcode
4652:: A65.
4604:Bibcode
4449:Bibcode
4406:Bibcode
4334:Bibcode
4261:Bibcode
4230:Bibcode
4202:Bibcode
4155:Bibcode
4128:1650052
4108:Science
4086:Bibcode
4049:Bibcode
3997:Bibcode
3956:Bibcode
3910:Bibcode
3869:Bibcode
3867:: 965.
3838:Bibcode
3803:Bibcode
3766:Bibcode
3719:Bibcode
3682:Bibcode
3680:: 497.
3645:Bibcode
3601:Bibcode
3599:: A69.
3546:Bibcode
3493:Bibcode
3318:Bibcode
3281:Bibcode
3234:Bibcode
3197:Bibcode
3195:: 143.
3092:Bibcode
3001:Bibcode
2999:: 250.
2966:Bibcode
2901:28 July
2880:28 July
2758:(1940)
2746:ἀντάρης
2727:Bibcode
2694:364–366
2637:Bibcode
2600:Bibcode
2598:: 227.
2546:Bibcode
2487:Bibcode
2425:Bibcode
2413:: A24.
2327:Bibcode
2290:Bibcode
2236:Bibcode
2234:: 245.
2199:Bibcode
2169:5203133
2139:Bibcode
2075:Bibcode
1880:Huǒxīng
1867:Chinese
1724:Ishhara
1710:In the
1643:7
1553:at the
1397:parsecs
1383:with a
1364:Antares
1278:parsecs
1241:by the
1231:Regulus
1113:History
1095:to the
1081:Antares
1041:reddish
1032:Ἀντάρης
1024:Antares
930:reddish
921:Ἀντάρης
913:Antares
882:Jupiter
844:parsecs
830:in the
787:in the
781:Antares
755:Antares
363:Details
71:Equinox
6796:K2-33b
6786:K2-24b
6715:WR 93b
6434:162020
6429:159868
6424:158042
6419:155985
6414:155448
6404:153234
6399:152424
6394:150420
6389:150248
6384:146436
6379:145377
6374:144432
6369:143567
5450:22 (i)
5435:13 (c)
5430:12 (c)
4977:
4915:
4843:
4788:. A17.
4784:
4737:
4729:
4693:Nature
4686:. A65.
4682:
4509:
4484:
4379:
4354:
4181:
4173:
4126:
4118:
4017:
3928:
3813:
3737:
3572:
3564:
3511:
3435:
3408:
3336:
3232:: 86.
3147:
3090:: 84.
2964:: 58.
2848:22 May
2827:
2817:
2790:
2700:
2655:
2564:
2443:
2370:
2360:
2254:
2167:
2159:
2093:
2027:
1938:Altair
1934:Bunjil
1877::
1875:pinyin
1869::
1819:". In
1813:Persia
1787:Serket
1768:calque
1766:was a
964:image.
749:SIMBAD
564:Radius
529:
486:
439:
395:Radius
225:+1.83
214:+1.34
7047:Other
6933:Other
6710:WR 86
6635:Th 28
6540:K2-33
6535:K2-24
6505:H1-36
6443:Other
5868:V1309
5863:V1294
5858:V1292
5853:V1280
5848:V1187
5843:V1186
5838:V1104
5833:V1094
5828:V1077
5823:V1075
5818:V1074
5808:V1068
5803:V1058
5798:V1051
5793:V1040
5788:V1036
5783:V1034
5778:V1033
5773:V1026
5768:V1018
5763:V1007
5758:V1003
5410:2 (A)
5405:1 (b)
5380:α Nor
5371:β Nor
5223:Bayer
5214:Stars
5139:Stars
5086:X-Ray
5074:GALEX
4913:S2CID
4847:. 10.
4841:S2CID
4782:S2CID
4756:arXiv
4735:S2CID
4701:arXiv
4680:S2CID
4654:arXiv
4594:arXiv
4460:(PDF)
4445:(PDF)
4300:STARS
4277:. 29.
4179:JSTOR
4124:JSTOR
4065:. 38.
4015:S2CID
3987:arXiv
3735:S2CID
3709:arXiv
3570:S2CID
3536:arXiv
3509:S2CID
3483:arXiv
3334:S2CID
3308:arXiv
2945:2011)
2937:(2009
2874:(PDF)
2867:(PDF)
2653:S2CID
2627:arXiv
2562:S2CID
2536:arXiv
2477:arXiv
2441:S2CID
2415:arXiv
2252:S2CID
2165:S2CID
2129:arXiv
2091:S2CID
2065:arXiv
1964:Piauí
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