2281:
2579:
1317:
1614:
it has a P Cygni profile; most of the rest of the time, the line has an inverse P Cygni profile, where the emission component is on the short wavelength side of the line. Rarely, there is a pure emission Hα line. The line profile changes are interpreted as variations in the quantity and velocity of material being expelled from the star. Occasional very high-velocity outflows have been inferred, and, more rarely, infalling material. The overall picture is one of large
1818:
52:
8052:
2190:(DR2) contains a somewhat unreliable parallax for Rigel B, placing it at about 1,100 light-years (340 parsecs), further away than the Hipparcos distance for Rigel, but similar to the Taurus-Orion R1 association. There is no parallax for Rigel in Gaia DR2. The Gaia DR2 proper motions for Rigel B and the Hipparcos proper motions for Rigel are both small, although not quite the same.
1631:
8076:
59:
8100:
1304:, each three to four times as massive as the Sun. Rigel and the triple system orbit a common center of gravity with a period estimated to be 24,000 years. The inner stars of the triple system orbit each other every 10 days, and the outer star orbits the inner pair every 63 years. A much fainter star, separated from Rigel and the others by nearly an
8088:
1452:
1613:
The unusual Hα line profile is observed to vary unpredictably. It is a normal absorption line around a third of the time. About a quarter of the time, it is a double-peaked line, that is, an absorption line with an emission core or an emission line with an absorption core. About a quarter of the time
2550:
in its core. Due to strong convection of helium produced in the core while Rigel was on the main sequence and in the hydrogen-burning shell since it became a supergiant, the fraction of helium at the surface has increased from 26.6% when the star formed to 32% now. The surface abundances of carbon,
2249:
days. The two spectroscopic components Rigel Ba and Rigel Bb cannot be resolved in optical telescopes but are known to both be hot stars of spectral type around B9. This spectroscopic binary, together with the close visual component Rigel C, is likely a physical triple-star system, although Rigel C
1399:
has speculated that Rigel was designated by Bayer during a rare period when it was outshone by the variable star
Betelgeuse, resulting in the latter star being designated "alpha" and Rigel designated "beta". Bayer did not strictly order the stars by brightness, instead grouping them by magnitude.
4970:
Van
Genderen, A. M.; Bovenschen, H.; Engelsman, E. C.; Goudfrooy, P.; Van Haarlem, M. P.; Hartmann, D.; Latour, H. J.; Ng, Y. K.; Prein, J. J.; Van Roermund, F. H. P. M.; Roogering, H. J. A.; Steeman, F. W. M.; Tijdhof, W. (1989). "Light variations of massive stars (alpha Cygni variables). IX".
5068:
Chesneau, O.; Dessart, L.; Mourard, D.; Bério, Ph.; Buil, Ch.; Bonneau, D.; Borges
Fernandes, M.; Clausse, J. M.; Delaa, O.; Marcotto, A.; Meilland, A.; Millour, F.; Nardetto, N.; Perraut, K.; Roussel, A.; Spang, A.; Stee, P.; Tallon-Bosc, I.; McAlister, H.; Ten Brummelaar, T.; Sturmann, J.;
1672:
class of variable stars, defined as "non-radially pulsating supergiants of the Bep–AepIa spectral types". In those spectral types, the 'e' indicates that it displays emission lines in its spectrum, while the 'p' means it has an unspecified spectral peculiarity. Alpha Cygni type variables are
1677:. Rigel was added to the General Catalogue of Variable Stars in the 74th name-list of variable stars on the basis of the Hipparcos photometry, which showed variations with a photographic amplitude of 0.039 magnitudes and a possible period of 2.075 days. Rigel was observed with the Canadian
2933:
Al-Sufi's book was translated into Latin and other
European languages. Al-Sufi himself planned the figures, two for each constellation: one shows how they appear to an observer looking up toward the heavens; the other how they appear to the observer looking down upon a celestial
2384:
Although Rigel is often considered the most luminous star within 1,000 light-years of the Sun, its energy output is poorly known. Using the
Hipparcos distance of 860 light-years (264 parsecs), the estimated relative luminosity for Rigel is about 120,000 times that of the Sun
1654:
to be reliably detected. This brightness variation has no obvious period. Observations over 18 nights in 1984 showed variations at red, blue, and yellow wavelengths of up to 0.13 magnitudes on timescales of a few hours to several days, but again no clear period. Rigel's
2155:
first measured the relative position of the companion in 1822, cataloguing the visual pair as Σ 668. The secondary star is often referred to as Rigel B or β Orionis B. The angular separation of Rigel B from Rigel A is 9.5 arc seconds to its south along
1730:
line profiles, and measurement of the regions producing the lines, show that Rigel's stellar wind varies greatly in structure and strength. Loop and arm structures were also detected within the wind. Calculations of mass loss from the Hγ line give
2329:
Estimation of many physical characteristics of blue supergiant stars, including Rigel, is challenging due to their rarity and uncertainty about how far they are from the Sun. As such, their characteristics are mainly estimated from theoretical
2271:
A spectroscopic companion to Rigel was reported on the basis of radial velocity variations, and its orbit was even calculated, but subsequent work suggests the star does not exist and that observed pulsations are intrinsic to Rigel itself.
1239:
is estimated to be ten million times that of the Sun. With an estimated age of seven to nine million years, Rigel has exhausted its core hydrogen fuel, expanded, and cooled to become a supergiant. It is expected to end its life as a
4510:
Moore's
Navigation Improved: Being the Theory and Practice of Finding the Latitude, the Longitude, and the Variation of the Compass, by the Fixed Stars and Planets. To which is Prefixed, the Description and Use of the New Celestial
1493:. In the Southern Hemisphere, Rigel is the first bright star of Orion visible as the constellation rises. Correspondingly, it is also the first star of Orion to set in most of the Northern Hemisphere. The star is a vertex of the "
1371:
3823. For simplicity, Rigel's companions are referred to as Rigel B, C, and D; the IAU describes such names as "useful nicknames" that are "unofficial". In modern comprehensive catalogs, the whole multiple star system is known as
2538:
models suggest the pulsations of Rigel are powered by nuclear reactions in a hydrogen-burning shell that is at least partially non-convective. These pulsations are stronger and more numerous in stars that have evolved through a
2197:
suspected Rigel B to be a binary system, and in 1878, he resolved it into two components. This visual companion is designated as component C (Rigel C), with a measured separation from component B that varies from less than
1568:
of its spectral lines, was seen to vary. This was confirmed and interpreted at the time as being due to a spectroscopic companion with a period of about 22 days. The radial velocity has since been measured to vary by about
4320:
Markova, N.; Prinja, R. K.; Markov, H.; Kolka, I.; Morrison, N.; Percy, J.; Adelman, S. (2008). "Wind structure of late B supergiants. I. Multi-line analyses of near-surface and wind structure in HD 199 478 (B8 Iae)".
1335:(IAU) included the name "Rigel" in the IAU Catalog of Star Names. According to the IAU, this proper name applies only to the primary component A of the Rigel system. The system is listed variously in historical
2522:
Due to their closeness to each other and ambiguity of the spectrum, little is known about the intrinsic properties of the members of the Rigel BC triple system. All three stars seem to be near equally hot
6698:
4872:
Waelkens, C.; Aerts, C.; Kestens, E.; Grenon, M.; Eyer, L. (1998). "Study of an unbiased sample of B stars observed with
Hipparcos: the discovery of a large amount of new slowly pulsating B star".
5069:
Sturmann, L.; Turner, N.; Farrington, C.; Goldfinger, P. J. (2010). "Time, spatial, and spectral resolution of the Hα line-formation region of Deneb and Rigel with the VEGA/CHARA interferometer".
4414:
4152:
Dommanget, J.; Nys, O. (1994). "Catalogue des composantes d'etoiles doubles et multiples (CCDM) premiere edition – Catalogue of the components of double and multiple stars (CCDM) first edition".
1836:
Rigel's distance from the Sun is somewhat uncertain, different estimates being obtained by different methods. Old estimates placed it 166 parsecs (or 541 light years) away from the Sun. The 2007
2551:
nitrogen, and oxygen seen in the spectrum are compatible with a post-red supergiant star only if its internal convection zones are modeled using non-homogeneous chemical conditions known as the
4065:
5125:
Chesneau, O.; Kaufer, A.; Stahl, O.; Colvinter, C.; Spang, A.; Dessart, L.; Prinja, R.; Chini, R. (2014). "The variable stellar wind of Rigel probed at high spatial and spectral resolution".
2164:
6.7, the overall difference in brightness from Rigel A (about 6.6 magnitudes or 440 times fainter) makes it a challenging target for telescope apertures smaller than 15 cm (6 in).
1400:
Rigel and
Betelgeuse were both considered to be of the first magnitude class, and in Orion the stars of each class are thought to have been ordered north to south. Rigel is included in the
3922:
2135:
discovered Rigel to be a visual double star on 1 October 1781, cataloguing it as star 33 in the "second class of double stars" in his
Catalogue of Double Stars, usually abbreviated to H
3600:
De
Almeida, E S G.; Hugbart, M.; Domiciano De Souza, A.; Rivet, J-P; Vakili, F.; Siciak, A.; Labeyrie, G.; Garde, O.; Matthews, N.; Lai, O.; Vernet, D.; Kaiser, R.; Guerin, W. (2022).
6676:
2543:
phase and then increased in temperature to again become a blue supergiant. This is due to the decreased mass and increased levels of fusion products at the surface of the star.
2326:. Further observations of radial velocity variations indicate that it simultaneously oscillates in at least 19 non-radial modes with periods ranging from about 1.2 to 74 days.
1678:
3422:
Moravveji, Ehsan; Moya, Andres; Guinan, Edward F. (2012). "Asteroseismology of the nearby SN-II Progenitor: Rigel. Part II. ε-mechanism Triggering Gravity-mode Pulsations?".
3128:
5451:
Catalogus novus stellarum duplicium et multiplicium maxima ex parte in Specula Universitatis Caesareae Dorpatensis per magnum telescopium achromaticum Fraunhoferi detectarum
4998:
Kazarovets, E. V.; Samus, N. N.; Durlevich, O. V.; Frolov, M. S.; Antipin, S. V.; Kireeva, N. N.; Pastukhova, E. N. (1999). "The 74th Special Name-list of Variable Stars".
1377:
1069:
1021:
4806:
3662:
2570:(about the same brightness as a quarter Moon or around 300 times brighter than Venus ever gets). The supernova would leave behind either a black hole or a neutron star.
1296:. It has an apparent magnitude of 6.7, making it 1/400th as bright as Rigel. Two stars in the system can be seen by large telescopes, and the brighter of the two is a
3995:
3794:
Moravveji, Ehsan; Guinan, Edward F.; Shultz, Matt; Williamson, Michael H.; Moya, Andres (2012). "Asteroseismology of the nearby SN-II Progenitor: Rigel. Part I. The
785:
6861:
3722:
Baines, Ellyn K.; Armstrong, J. Thomas; Schmitt, Henrique R.; Zavala, R. T.; Benson, James A.; Hutter, Donald J.; Tycner, Christopher; van Belle, Gerard T. (2017).
4641:
4548:
2504:
leads to a significantly larger size. Older distance estimates were mostly far lower than modern estimates, leading to lower radius estimates; a 1922 estimate by
1095:
1681:
satellite for nearly 28 days in 2009. Milli-magnitude variations were observed, and gradual changes in flux suggest the presence of long-period pulsation modes.
4406:
2394:), but another recently published distance of 1,170 ± 130 light-years (360 ± 40 parsecs) suggests an even higher luminosity of 219,000
6352:
5716:
Mason, Brian D.; Hartkopf, William I.; Gies, Douglas R.; Henry, Todd J.; Helsel, John W. (2009). "The High Angular Resolution Multiplicity of Massive Stars".
3388:
3088:
6827:
2264:, almost due north at a position angle of 1°. Gaia DR2 finds it to be a 12th magnitude sunlike star at approximately the same distance as Rigel. Likely a
1391:
in 1603. The "beta" designation is commonly given to the second-brightest star in each constellation, but Rigel is almost always brighter than α Orionis (
6515:
4052:
5689:
Burnham, S.W. (1900). "A General Catalogue of the Double Stars discovered by S. W. Burnham from 1871 to 1899, arranged in order of Right Ascension".
1610:
where there is simultaneously emission from a dense wind close to the star and absorption from circumstellar material expanding away from the star.
8173:
6781:
6759:
2764:, the river, marks a line of stars in the sky leading to it, and the other stars of Orion are his ceremonial tools and entourage. Betelgeuse is
5000:
4845:
1901:, somewhat closer at 1,200 light-years (360 parsecs). Rigel is thought to be considerably closer than most of the members of Orion OB1 and the
3295:
6731:
6615:
6583:
6488:
6445:
6414:
6334:
6305:
6146:
6109:
6025:
5855:
4491:
4454:
4390:
4269:
4242:
4209:
4136:
3004:
2976:
2434:
6183:
5527:
3124:"Times-Series Photometry & Spectroscopy of the Bright Blue Supergiant Rigel: Probing the Atmosphere and Interior of a SN II Progenitor"
2401:. Other calculations based on theoretical stellar evolutionary models of Rigel's atmosphere give luminosities anywhere between 83,000
4843:
Guinan, E. F.; McCook, G. P.; Harris, W. T.; Speranzini, D.; Wacker, S. W. (1985). "Light, Color, and H-alpha Line Variations of Rigel".
8128:
6854:
6132:
1401:
5935:
Demarque, P.; Guenther, D. B.; Li, L. H.; Mazumdar, A.; Straka, C. W. (August 2008). "YREC: the Yale rotating stellar evolution code".
2125:
of which Rigel is a part has at least four components. Rigel (sometimes called Rigel A to distinguish from the other components) has a
1557:
class Ia. Variations in the spectrum have resulted in the assignment of different classes to Rigel, such as B8 Ia, B8 Iab, and B8 Iae.
6000:
Aufdenberg, J. P.; et al. (2008). "Limb Darkening: Getting Warmer". In Richichi A.; Delplancke F.; Paresce F.; Chelli A. (eds.).
5976:
5521:
3170:
2152:
1340:
1010:
4020:
8153:
4948:
4899:
Samus, N. N.; Kazarovets, E. V.; Durlevich, O. V.; Kireeva, N. N.; Pastukhova, E. N. (2017). "General Catalogue of Variable Stars".
2626:
meaning "leg, foot"), which can be traced to the 10th century. "Jauzah" was a proper name for Orion; an alternative Arabic name was
1886:
of 2.5° from the star, or a projected distance of 39 light-years (12 parsecs) away. From measures of other nebula-embedded stars, IC
5476:
2129:, which is likely a close triple-star system. A fainter star at a wider separation might be a fifth component of the Rigel system.
4289:
3957:
1332:
2366:
million years has been estimated by comparing evolutionary tracks, while atmospheric modeling from the spectrum gives a mass of
2300:
2285:
8163:
6789:
6755:
1080:
80:
8148:
8138:
8133:
8055:
6847:
5937:
2257:
555, although it is unclear whether it is physically related or a coincidental alignment. Its 2017 separation from Rigel was
1871:, suggesting a distance around 1,000 light-years (310 parsecs). However, the measurements for this object may be unreliable.
1646:
Rigel has been known to vary in brightness since at least 1930. The small amplitude of Rigel's brightness variation requires
1416:
1373:
1028:
7859:
7437:
6323:
Aboriginal mythology : an A-Z spanning the history of aboriginal mythology from the earliest legends to the present day
4098:
1897:, which is located at a distance of up to 1,600 light-years (500 parsecs) from Earth. It is a member of the loosely defined
6451:
6891:
2223:
1358:
1003:
837:
8066:
3602:"Combined spectroscopy and intensity interferometry to determine the distances of the blue supergiants P Cygni and Rigel"
2253:
In 1878, Burnham found another possibly associated star of approximately 13th magnitude. He listed it as component D of β
8035:
8027:
7574:
2416:
1553:
for B8 stars is estimated from the strength and narrowness of the hydrogen spectral lines, and Rigel is assigned to the
1518:
1365:
989:
7442:
4562:
Morgan, W. W.; Roman, Nancy G. (1950). "Revised Standards for Supergiants on the System of the Yerkes Spectral Atlas".
4293:
3330:
Przybilla, N.; Butler, K.; Becker, S. R.; Kudritzki, R. P. (2006). "Quantitative spectroscopy of BA-type supergiants".
102:
8143:
8123:
4048:
1898:
5782:
5624:
4418:
2811:, as well as some Maori groups in New Zealand, mark the start of their New Year with Rigel rather than the Pleiades.
2740:). The distance between them signified the taboo preventing a man from approaching his mother-in-law. The indigenous
3545:
Gontcharov, G. A. (2006). "Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system".
2280:
8178:
8168:
6886:
6639:
6350:
Hamacher, Duane W.; Frew, David J. (2010). "An Aboriginal Australian Record of the Great Eruption of Eta Carinae".
4479:
4128:
4061:
3086:
Ducati, J. R. (2002). "VizieR On-line Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system".
3033:
2968:
2914:
2660:
1351:
1221:
996:
1874:
Indirect distance estimation methods have also been employed. For example, Rigel is believed to be in a region of
7354:
6297:
5769:
5611:
5271:
3800:
3210:
2524:
2265:
1409:
1301:
1055:
5249:
2706:, himself represented by the three stars of Orion's Belt. The leg had been severed with a cutlass by the maiden
1859:
of about 9%. Rigel B, usually considered to be physically associated with Rigel and at the same distance, has a
1471:, excluding the Sun, although occasionally fainter than Betelgeuse. Rigel appears slightly blue-white and has a
5823:
5665:
5411:
2761:
2315:
2194:
1829:
1689:
From observations of the variable Hα spectral line, Rigel's mass-loss rate due to stellar wind is estimated be
6505:
2897:, renamed after originally being called Utskjera. They were given their current name as Rigel was used as an
1521:, being easily located and readily visible in all the world's oceans (the exception is the area north of the
6253:
2207:
1837:
1275:
6823:
NASA Astronomy Picture of the Day: A Blazing Fireball between the Orion Nebula and Rigel (16 November 2015)
2578:
8158:
7759:
7515:
6881:
6128:
3264:
Mason, Brian D.; Wycoff, Gary L.; Hartkopf, William I.; Douglass, Geoffrey G.; Worley, Charles E. (2001).
1537:
is a defining point of the classification sequence for supergiants. The overall spectrum is typical for a
1534:
1436:
1205:
1048:
342:
281:
31:
3386:
Nicolet, B. (1978). "Photoelectric photometric Catalogue of homogeneous measurements in the UBV System".
2863:
was originally a Norwegian ship, built in Copenhagen in 1924. It was requisitioned by the Germans during
2178:(AU). Since its discovery, there has been no sign of orbital motion, although both stars share a similar
1549:
as well as neutral helium lines and some of heavier elements such as oxygen, calcium, and magnesium. The
1443:
34085. These designations frequently appear in the scientific literature, but rarely in popular writing.
7705:
7452:
7151:
6870:
2583:
2505:
2304:
1894:
1428:
1420:
1384:
1336:
1320:
1158:
1147:
1076:
1044:
793:
95:
6793:
6747:
2867:
and sunk in 1944 while being used to transport prisoners of war. Two US Navy ships have borne the name
6371:
6192:
6054:
6005:
5956:
5899:
5801:
5735:
5698:
5643:
5577:
5509:
5420:
5369:
5290:
5221:
5144:
5088:
5040:
5009:
4980:
4910:
4881:
4854:
4815:
4774:
4744:
4708:
4677:
4623:
4571:
4530:
4382:
Burnham's Celestial Handbook, Volume Two: An Observer's Guide to the Universe Beyond the Solar System
4340:
4197:
4161:
3931:
3879:
3819:
3745:
3681:
3623:
3566:
3509:
3441:
3397:
3349:
3277:
3219:
3179:
3137:
3097:
3052:
2547:
2268:, this star would have an orbital period of around 250,000 years, if it is part of the Rigel system.
2234:
2168:
2122:
1669:
1647:
1498:
1297:
1267:
579:
439:
318:
274:
7634:
3656:
Shultz, M.; Wade, G. A.; Petit, V.; Grunhut, J.; Neiner, C.; Hanes, D.; MiMeS Collaboration (2014).
1270:
due to the amplitude and periodicity of its brightness variation, as well as its spectral type. Its
6480:
5505:
3265:
2588:
2245:. Periodic changes observed in relative positions of these lines indicate an orbital period of 9.86
1860:
1522:
1490:
1486:
1062:
5472:
8104:
6387:
6361:
6272:
6208:
6138:
6078:
5982:
5946:
5917:
5889:
5791:
5751:
5725:
5633:
5593:
5567:
5387:
5359:
5306:
5280:
5239:
5211:
5160:
5134:
5104:
5078:
4926:
4667:
4635:
4542:
4356:
4330:
3949:
3895:
3869:
3835:
3809:
3763:
3735:
3699:
3671:
3613:
3582:
3556:
3527:
3457:
3431:
3365:
3339:
3068:
3042:
2844:; the stars were seen as facing off against each other and kept apart only by the three stars of
2319:
2126:
1883:
1464:
1263:
475:
244:
191:
7909:
2295:
that has exhausted the hydrogen fuel in its core, expanded and cooled as it moved away from the
4380:
7764:
6966:
6920:
6727:
6611:
6607:
6579:
6484:
6474:
6441:
6437:
6410:
6330:
6301:
6167:
6142:
6105:
6070:
6021:
5972:
5851:
5841:
5517:
5499:
4901:
4604:
4508:
4487:
4483:
4450:
4440:
4386:
4265:
4238:
4205:
4193:
4132:
3547:
3168:
Epchtein, N.; et al. (March 1997). "The deep near-infrared southern sky survey (DENIS)".
3000:
2972:
2816:
2687:
2668:
2559:
2535:
2331:
2175:
1890:
2118's distance is estimated to be 949 ± 7 light-years (291 ± 2 parsecs).
1822:
1715:
1554:
1405:
1241:
1236:
1151:
1127:
985:
865:
330:
269:
76:
6291:
6097:
3122:
Guinan, E. F.; Eaton, J. A.; Wasatonic, R.; Stewart, H.; Engle, S. G.; McCook, G. P. (2010).
1913:
with a complex history and might have originally formed in the main body of the association.
8080:
7889:
7639:
7053:
7048:
7006:
7001:
6996:
6991:
6986:
6981:
6976:
6971:
6901:
6379:
6262:
6200:
6062:
6013:
5964:
5960:
5907:
5847:
5811:
5806:
5743:
5653:
5648:
5585:
5581:
5428:
5377:
5298:
5229:
5225:
5152:
5148:
5096:
5092:
5048:
5044:
4984:
4918:
4885:
4823:
4782:
4716:
4579:
4471:
4348:
4344:
3985:
3939:
3887:
3883:
3827:
3753:
3689:
3631:
3574:
3517:
3513:
3449:
3401:
3357:
3353:
3285:
3227:
3145:
3060:
3056:
2610:
2438:
2386:
2242:
2161:
2132:
1841:
1572:
1550:
1468:
1209:
829:
753:
423:
135:
109:
2566:
progenitors to Earth, and would be expected to have a maximum apparent magnitude of around
2334:. Its effective temperature can be estimated from the spectral type and color to be around
2214:, with visual magnitudes of 7.5 and 7.6, respectively. Their estimated orbital period is 63
7103:
6511:
6233:
4944:
4016:
2808:
2790:
2749:
2711:
2699:
2680:
2292:
1856:
1659:
varies slightly, but this is not significantly correlated with its brightness variations.
1603:
1561:
1542:
1139:
1118:
766:
364:
215:
162:
6896:
3266:"The 2001 US Naval Observatory Double Star CD-ROM. I. The Washington Double Star Catalog"
2845:
2772:
1878:, its radiation illuminating several nearby clouds. Most notable of these is the 5°-long
6375:
6196:
6058:
6009:
5903:
5878:"The puzzle of the CNO abundances of α Cygni variables resolved by the Ledoux criterion"
5739:
5702:
5513:
5466:
5424:
5373:
5294:
5013:
4914:
4858:
4819:
4778:
4748:
4712:
4681:
4627:
4575:
4534:
4201:
4165:
3935:
3823:
3749:
3685:
3627:
3570:
3445:
3281:
3223:
3183:
3141:
3101:
2965:
A Dictionary of Modern star Names: A Short Guide to 254 Star Names and Their Derivations
2250:
cannot be detected in the spectrum, which is inconsistent with its observed brightness.
51:
7013:
6599:
5747:
5332:
4446:
2890:
2879:
2804:
2540:
2446:
2419:
from historical photometry with the Hipparcos distance suggests a luminosity as low as
2157:
1851:
1651:
1538:
1494:
1396:
1324:
977:
655:
592:
566:
523:
431:
411:
399:
6383:
6181:
Kunitzsch, P. (1986). "The Star Catalogue Commonly Appended to the Alfonsine Tables".
5348:"The APOGEE-2 Survey of the Orion Star-forming Complex. II. Six-dimensional Structure"
3918:"Catalogue of Double Stars. By Mr. Herschel, F. R. S. Communicated by Dr. Watson, Jun"
3831:
1216:, depending on the method and assumptions used. Its radius is more than seventy times
8117:
8009:
7422:
7141:
7093:
6391:
6326:
6212:
5921:
5755:
5597:
5391:
5310:
5302:
5243:
5164:
4930:
4598:
4472:
3953:
3767:
3703:
3586:
3461:
3453:
3369:
2875:
2296:
2260:
2238:
2179:
1606:
after a star that shows this feature strongly in its spectrum. It is associated with
1595:
1565:
1546:
1506:
1460:
1271:
1143:
388:
335:
313:
89:
6818:
NASA Astronomy Picture of the Day: Rigel and the Witch Head Nebula (15 January 2018)
5986:
5108:
4360:
4189:
The Brightest Stars: Discovering the Universe through the Sky's Most Brilliant Stars
3899:
3658:"An observational evaluation of magnetic confinement in the winds of BA supergiants"
3531:
3072:
8092:
8004:
7924:
7864:
7694:
7564:
7417:
7412:
7136:
7126:
7121:
7116:
7111:
7018:
5178:
3724:"Fundamental parameters of 87 stars from the Navy Precision Optical Interferometer"
2864:
2691:
2469:
2114:
1910:
1902:
1674:
1615:
1388:
1252:
1232:
1217:
1174:
954:
925:
900:
725:
681:
6409:(Revised ed.). Merimbula, New South Wales: Hugh C. Cairns. pp. 139–140.
6267:
6248:
6227:
5816:
5773:
5658:
5615:
5234:
5195:
5156:
5100:
5053:
5028:
4352:
3891:
3839:
6721:
6565:
6431:
5589:
5449:
4259:
4226:
4187:
4090:
3361:
3064:
7680:
7098:
7088:
7083:
7078:
7073:
7068:
7063:
7058:
6958:
6833:
6575:
6017:
5029:"A systematic study of variability among OB-stars based on HIPPARCOS photometry"
2992:
2902:
2552:
1656:
1635:
1619:
1602:
to the long wavelength side of the main absorption line. This is now known as a
1478:
1316:
1292:
1182:
815:
303:
292:
231:
178:
17:
6204:
5382:
5347:
3758:
3723:
2760:
and chief conductor of ceremonies in a songline when Orion is high in the sky.
7999:
7994:
7989:
7919:
7914:
7854:
7675:
7670:
7665:
7599:
7594:
7589:
7584:
7407:
7402:
7397:
7392:
7387:
7382:
7377:
7344:
7339:
7334:
7329:
7324:
7319:
7314:
7309:
7304:
7299:
7294:
7289:
7284:
7279:
7274:
7269:
7264:
7259:
7254:
7249:
7244:
7239:
7234:
7229:
7224:
7219:
7214:
7209:
7204:
7199:
7194:
7189:
7184:
7179:
7174:
7169:
7131:
7043:
7038:
7033:
6928:
6538:
5968:
4922:
4828:
4801:
4659:
3578:
3150:
3123:
2894:
2841:
2837:
2823:
2726:
2702:. In the Caribbean, Rigel represented the severed leg of the folkloric figure
2639:, "the foot of the great one", from which stems the rarely used variant names
1875:
1702:
1630:
1392:
1305:
1283:
1256:
1213:
1194:
961:
932:
907:
695:
453:
352:
6074:
3636:
3601:
2803:) in the dawn sky, marking the Māori New Year in late May or early June. The
1467:
ranging from 0.05 to 0.18. It is typically the seventh-brightest star in the
7657:
7548:
7372:
7367:
7362:
7164:
7159:
6938:
6004:. Eso Astrophysics Symposia. Vol. 1. Berlin: Springer. pp. 71–82.
5912:
5877:
4765:
Struve, O. (1933). "An Emission Line of Hydrogen in the Spectrum of Rigel".
4285:
3694:
3657:
2868:
2695:
2563:
2516:
1664:
1607:
1590:
1502:
1472:
1279:
1248:
1190:
6822:
6817:
3944:
2840:
adopted Betelgeuse and its red color. The two powerful families fought the
1274:
is caused by pulsations in its unstable atmosphere. Rigel is generally the
3522:
3497:
7973:
7968:
7963:
7958:
7953:
7904:
7874:
7849:
7844:
7828:
7823:
7818:
7813:
7808:
7803:
7798:
7793:
7743:
7738:
7733:
7728:
7723:
7718:
7713:
7629:
7624:
7614:
7609:
7543:
7538:
7533:
7528:
7523:
7505:
7500:
7490:
7485:
7480:
7475:
7470:
7465:
7460:
6839:
5572:
3344:
2898:
2857:
2800:
2795:
2753:
2690:, Rigel is his knee or (as its name suggests) foot; with the nearby star
879:
58:
6631:
6082:
6042:
1178:
7899:
7619:
7604:
7579:
7569:
7495:
7432:
7427:
6953:
6948:
6943:
4620:
An atlas of stellar spectra, with an outline of spectral classification
2883:
2786:
2741:
1879:
1825:
1817:
1510:
1451:
1282:
and the brightest star in Orion, though it is occasionally outshone by
6276:
4618:
Morgan, William Wilson; Keenan, Philip Childs; Kellman, Edith (1943).
3860:
Przybilla, N. (2010). "Mixing of CNO-cycled matter in massive stars".
2508:
gave Rigel a diameter of 25 million miles, or approximately 28.9
1769:
in 2009–10. Calculations using the Hα line give lower results, around
1208:
B8Ia, Rigel is calculated to be anywhere from 61,500 to 363,000 times
7938:
7894:
7884:
7869:
7778:
7028:
6104:. Princeton, New Jersey: Princeton University Press. pp. 92–93.
6100:. In Casagrande-Kim, Roberta; Thrope, Samuel; Ukeles, Raquel (eds.).
5827:
5669:
5253:
4741:
Hα line profile variability in the B8Ia-type supergiant Rigel (β Ori)
3990:
3031:
van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction".
2777:
2737:
2337:
2310:
1726:
interferometry, were taken from 2006 to 2010. Analysis of the Hα and
1514:
1227:
1198:
1112:
807:
708:
466:
3917:
2686:
With the constellation representing the mythological Greek huntsman
8087:
6476:
Exploring Ancient Skies: A Survey of Ancient and Cultural Astronomy
6066:
5796:
5638:
5433:
5406:
5364:
5216:
5027:
Lefèvre, L.; Marchenko, S. V.; Moffat, A. F. J.; Acker, A. (2009).
4786:
4721:
4696:
4583:
3740:
3618:
3561:
3290:
3232:
3205:
1710:/yr)—about ten million times more than the mass-loss rate from the
1587:
line in Rigel's spectrum was seen to be unusually weak and shifted
7879:
7023:
6366:
5951:
5894:
5730:
5285:
5269:
Guieu, S.; et al. (2010). "Spitzer Observations of IC 2118".
5139:
5083:
4672:
4335:
3874:
3814:
3676:
3436:
3047:
2729:
2694:
marking Orion's footstool. Rigel is presumably the star known as "
2577:
2323:
2279:
1906:
1816:
1727:
1629:
1584:
1450:
1323:, with Rigel at bottom right, at optical wavelengths plus the Hα (
1315:
627:
538:
495:
6102:
Romance and Reason: Islamic Transformations of the Classical Past
4802:"The inhomogeneous circumstellar envelope of Rigel (β Orionis A)"
6911:
6293:
Star Gods of the Maya: Astronomy in Art, Folklore, and Calendars
2905:, elevation 1,910 m (6,270 ft), is also in Antarctica.
2826:
chose Rigel and its white color as its symbol, calling the star
2496:. These radii are calculated assuming the Hipparcos distance of
1788:. It is estimated that Rigel has lost about three solar masses (
1723:
1186:
663:
531:
415:
403:
6843:
6828:
December double star of the month – beta Orionis
2732:
of southeastern Australia, and held to be the mother-in-law of
1475:
index of −0.06. It contrasts strongly with reddish Betelgeuse.
1259:
as a final remnant, depending on the initial mass of the star.
6665:. Garden City, New York: Doubleday & Company. p. 283.
5778:
Data Release 2: Summary of the contents and survey properties"
5620:
Data Release 2: Summary of the contents and survey properties"
2651:
saw its name split into "Rigel" and "Algebar", with the note,
1711:
1668:
satellite photometry, Rigel is identified as belonging to the
141:
124:
5200:
Data Release 3. Summary of the content and survey properties"
2997:
The Routledge Dictionary of Pronunciation for Current English
1909:
lie at a similar distance to Rigel, although Betelgeuse is a
1485:
pm on 24 January, Rigel is visible on winter evenings in the
4415:
Commonwealth Scientific and Industrial Research Organisation
4054:
Transactions IAU:Volume XXXA: Reports on Astronomy 2015–2018
1855:, giving a distance of 863 light-years (265 parsecs) with a
1289:
A triple-star system is separated from Rigel by an angle of
1193:. This system is located at a distance of approximately 860
3798:
High-precision Photometry and Radial Velocity Monitoring".
2943:
lit."... and it is called Algebar. It is also named Rigel."
2182:. The pair would have an estimated orbital period of 24,000
118:
6507:
Astronomical Knowledge of the Maori: Genuine and Empirical
5882:
Monthly Notices of the Royal Astronomical Society: Letters
2558:
Rigel is expected to eventually end its stellar life as a
121:
3923:
Philosophical Transactions of the Royal Society of London
1189:
that appear as a single blue-white point of light to the
138:
5194:
Vallenari, A.; et al. (Gaia collaboration) (2023).
4527:
Revised MK Spectral Atlas for stars earlier than the sun
2210:
showed the two almost identical components separated by
6726:. Forest Lake, Minnesota: Specialty Press. p. 69.
6047:
Publications of the Astronomical Society of the Pacific
5876:
Georgy, Cyril; Saio, Hideyuki; Meynet, Georges (2014).
5558:: The ninth catalogue of spectroscopic binary orbits".
4525:
Morgan, W. W.; Abt, Helmut A.; Tapscott, J. W. (1978).
2886:
that was cancelled in 1953 before reaching deployment.
1832:. Rigel B is not visible in the glare of the main star.
1455:
Rigel A and Rigel B as they appear in a small telescope
5327:
Jedicke, Peter; Levy, David H. (1992). "Regal Rigel".
1594:
towards shorter wavelengths, while there was a narrow
8064:
2477:. An older measurement of the angular diameter gives
6430:
Parker, Janet; Mills, Alice; Stanton, Julie (2007).
4385:. New York: Dover Publications. pp. 1299–1301.
3206:"The Spectrographic Orbit of the Companion to Rigel"
2633:
2616:
2527:
that are three to four times as massive as the Sun.
2218:
years. Burnham listed the Rigel multiple system as β
115:
8026:
7982:
7946:
7937:
7837:
7786:
7777:
7752:
7704:
7693:
7656:
7557:
7514:
7451:
7353:
7150:
6919:
6910:
4047:Mamajek, Eric E.; et al. (2018). "Division C:
3129:
Proceedings of the International Astronomical Union
1722:infrared spectroscopic observations, together with
112:
5772:; et al. (Gaia collaboration) (August 2018).
5614:; et al. (Gaia collaboration) (August 2018).
4739:Morrison, N. D.; Rother, R.; Kurschat, N. (2008).
4154:Communications de l'Observatoire Royal de Belgique
3789:
3787:
3785:
3783:
3781:
3779:
3777:
2655:Alternate spellings from the 17th century include
1481:every year at midnight on 12 December, and at 9:00
1266:ranging from 0.05 to 0.18. It is classified as an
6405:Harney, Bill Yidumduma; Cairns, Hugh C. (2004) .
4807:Monthly Notices of the Royal Astronomical Society
3663:Monthly Notices of the Royal Astronomical Society
3606:Monthly Notices of the Royal Astronomical Society
3417:
3415:
3413:
3411:
4800:Israelian, G.; Chentsov, E.; Musaev, F. (1997).
4237:. Cambridge, United Kingdom: Lutterworth Press.
4118:
4116:
6539:"Yowatashi Boshi; Stars that Pass in the Night"
5120:
5118:
4125:Star-hopping: your Visa to Viewing the Universe
3911:
3909:
3325:
3323:
3321:
3319:
3317:
3315:
3313:
2967:(2nd rev. ed.). Cambridge, Massachusetts:
2744:people of northwestern Victoria named Rigel as
6353:Journal of Astronomical History & Heritage
6226:Cleasby, Richard; Vigfusson, Gudbrand (1874).
5684:
5682:
5680:
5678:
5322:
5320:
3502:Astronomy & Astrophysics Supplement Series
3498:"MSC – a catalogue of physical multiple stars"
3026:
3024:
3022:
3020:
3018:
3016:
2831:
2768:"Owl Eyes Flicking", watching the ceremonies.
6855:
6537:Renshaw, Steve; Ihara, Saori (October 1999).
5501:1,001 Celestial Wonders to See Before You Die
4529:. Yerkes Observatory, University of Chicago.
4084:
4082:
4080:
4078:
3996:Centre de données astronomiques de Strasbourg
3916:Herschel, Mr.; Watson, Dr. (1 January 1782).
1673:generally considered to be irregular or have
185:−08° 12′ 05.8981″
8:
6723:The Complete History of U.S. Cruise Missiles
6473:Kelley, David H.; Milone, Eugene F. (2011).
5264:
5262:
4973:Astronomy and Astrophysics Supplement Series
3855:
3853:
3851:
3849:
3389:Astronomy and Astrophysics Supplement Series
2752:of northern Australia know Rigel as the Red
2627:
2614:of 1521. It is derived from the Arabic name
2151:33 in the Washington Double Star Catalogue.
4743:. Clumping in Hot-Star Winds. p. 155.
4734:
4732:
4514:. London: Baldwin and Cradock. p. 132.
4411:Australia Telescope, Outreach and Education
4042:
4040:
4038:
3381:
3379:
3089:CDS/ADC Collection of Electronic Catalogues
2562:. It is one of the closest known potential
1419:taken from various catalogs, including the
238:−08° 12′ 14.78″
79:J2000.0
8023:
7943:
7783:
7701:
7653:
6916:
6862:
6848:
6840:
5471:. London: Longmans, Green and Co. p.
4640:: CS1 maint: location missing publisher (
4547:: CS1 maint: location missing publisher (
4478:(3rd ed.). Port Melbourne, Victoria:
4374:
4372:
4370:
4315:
4313:
4311:
4019:. International Astronomical Union (IAU).
3651:
3649:
3647:
2653:et dicitur Algebar. Nominatur etiam Rigel.
6365:
6266:
6249:"Notes on the Star Lore of the Caribbees"
5950:
5911:
5893:
5840:Seeds, Michael A.; Backman, Dana (2015).
5815:
5805:
5795:
5729:
5657:
5647:
5637:
5571:
5432:
5381:
5363:
5284:
5233:
5215:
5138:
5082:
5052:
4827:
4760:
4758:
4720:
4671:
4334:
4181:
4179:
4177:
4175:
3943:
3873:
3813:
3757:
3739:
3717:
3715:
3713:
3693:
3675:
3635:
3617:
3560:
3521:
3435:
3343:
3289:
3231:
3199:
3197:
3195:
3193:
3149:
3046:
2999:(2nd ed.). Routledge. p. 1150.
2604:The earliest known recording of the name
2167:At Rigel's estimated distance, Rigel B's
2160:204°. Although not particularly faint at
1262:Rigel varies slightly in brightness, its
27:Brightest star in the constellation Orion
6123:
6121:
5448:Struve, Friedrich Georg Wilhelm (1827).
4945:"Variable Star Type Designations in VSX"
4653:
4651:
3117:
3115:
3113:
3111:
2622:, "the left leg (foot) of Jauzah" (i.e.
2303:. When it was on the main sequence, its
8071:
6830:Astronomical Society of Southern Africa
6433:Mythology: Myths, Legends and Fantasies
6098:"Mathematics, Astronomy, and Astrology"
5871:
5869:
5867:
5468:Celestial Objects for Common Telescopes
4697:"The spectroscopic binary beta Orionis"
3491:
3163:
3161:
2955:
2926:
1383:The designation of Rigel as β Orionis (
1327:) spectral line to emphasize gas clouds
1308:, may be part of the same star system.
395:
6002:The Power of Optical/IR Interferometry
5691:Publications of the Yerkes Observatory
5549:
5547:
5545:
5001:Information Bulletin on Variable Stars
4846:Information Bulletin on Variable Stars
4633:
4540:
4296:from the original on 30 September 2016
3489:
3487:
3485:
3483:
3481:
3479:
3477:
3475:
3473:
3471:
2995:; Kretzschmar, William A. Jr. (2017).
2485:, equivalent to a radius of 78.9
2449:, the angular diameter is found to be
38:
5454:. Dorpati Livonorum: J.C. Schuenmann.
5346:Kounkel, Marina; et al. (2018).
4470:Ellyard, David; Tirion, Wil (2008) .
4442:Universe: The Definitive Visual Guide
4089:Kaler, James B. (26 September 2009).
3259:
3257:
3255:
3253:
3251:
3249:
3247:
3245:
3243:
2435:Navy Precision Optical Interferometer
2104:
2099:
2093:
2091:
2071:
2061:
2048:
2032:
2011:
1997:
1978:
1970:
1951:
1945:
1935:
1930:
1924:
7:
6762:from the original on 2 February 2019
6701:. Naval History and Heritage Command
6679:. Naval History and Heritage Command
6677:"NH 1874 USS RIGEL (AD-13), 1922-46"
6642:from the original on 4 February 2019
6518:from the original on 4 November 2012
6184:Journal for the History of Astronomy
5554:Pourbaix, D.; et al. (2004). "S
5530:from the original on 1 February 2019
4071:from the original on 23 August 2019.
2963:Kunitzsch, Paul; Smart, Tim (2006).
2592:. The foot on the left is annotated
1795:) since beginning life as a star of
1286:, which varies over a larger range.
6454:from the original on 2 January 2014
4951:from the original on 5 October 2017
2628:
2574:Etymology and cultural significance
2284:Rigel's place at top-center on the
1893:Rigel is an outlying member of the
1882:(Witch Head Nebula), located at an
1560:As early as 1888, the heliocentric
1402:General Catalogue of Variable Stars
1177:component – and the
407:
6134:Star Names: Their Lore and Meaning
4417:. 21 December 2004. Archived from
4101:from the original on 22 April 2019
3298:from the original on 14 March 2016
2153:Friedrich Georg Wilhelm von Struve
1638:for Rigel, adapted from Moravveji
1173:. Rigel is the brightest and most
25:
6384:10.3724/SP.J.1440-2807.2010.03.06
5479:from the original on 4 April 2016
2314:. Rigel's complex variability at
1809:seven to nine million years ago.
8098:
8086:
8074:
8051:
8050:
6699:"80-G-1017252 USS Rigel (AF-58)"
4664:Handbook of Star Forming Regions
4290:British Astronomical Association
4286:"Nomenclature of Variable Stars"
4023:from the original on 7 July 2018
2893:are a chain of small islands in
2237:system, which shows two sets of
1784:. The terminal wind velocity is
1564:of Rigel, as estimated from the
1333:International Astronomical Union
134:
108:
57:
50:
6790:U.S. Department of the Interior
6756:U.S. Department of the Interior
6636:Minnehallen (The Memorial Hall)
6229:An Icelandic-English Dictionary
5824:Gaia DR2 record for this source
5666:Gaia DR2 record for this source
5250:Gaia DR3 record for this source
4660:"Overview of the Orion Complex"
4603:. New York: Macmillan. p.
4449:. 1 October 2012. p. 233.
3963:from the original on 3 May 2019
2789:), the chief of all-stars. Its
2582:Orion illustrated in a copy of
1622:and driven by magnetic fields.
1212:as the Sun, and 18 to 24 times
8174:Henry Draper Catalogue objects
6164:Arabische Sternnamen in Europa
6137:(Reprint ed.). New York:
5938:Astrophysics and Space Science
4051:". In Benvenuti, Piero (ed.).
2775:of New Zealand named Rigel as
2714:of southern Mexico knew it as
2233:Component B is a double-lined
1489:and on summer evenings in the
1302:blue-white main-sequence stars
1:
6892:Orion molecular cloud complex
6782:"Antarctica Detail: ID 12639"
6748:"Antarctica Detail: ID 12640"
6663:U.S. Warships of World War II
6661:Silverstone, Paul H. (1968).
6268:10.1525/aa.1946.48.2.02a00030
6043:"The Dimensions of the Stars"
5407:"Stars in reflection nebulae"
4127:. Cambridge, United Kingdom:
4123:Garfinkle, Robert A. (1997).
2596:, the Arabic name from which
2299:across the upper part of the
1404:, but since it already has a
1387:to Beta Orionis) was made by
6574:] (in Japanese). Tokyo:
6096:Langermann, Y. Tzvi (2018).
5783:Astronomy & Astrophysics
5748:10.1088/0004-6256/137/2/3358
5625:Astronomy & Astrophysics
5033:Astronomy & Astrophysics
2515:, smaller than its neighbor
2417:spectral energy distribution
1714:. More detailed optical and
1300:. These three stars are all
6510:. Wellington, New Zealand:
6018:10.1007/978-3-540-74256-2_8
5817:10.1051/0004-6361/201833051
5659:10.1051/0004-6361/201833051
5498:Bakich, Michael E. (2010).
5235:10.1051/0004-6361/202243940
5157:10.1051/0004-6361/201322894
5101:10.1051/0004-6361/201014509
5054:10.1051/0004-6361/200912304
4353:10.1051/0004-6361:200809376
4049:Working Group on Star Names
4017:"IAU Catalog of Star Names"
3892:10.1051/0004-6361/201014164
3832:10.1088/0004-637X/747/2/108
3204:Sanford, Roscoe F. (1942).
2793:presages the appearance of
2781:, said to be a daughter of
2634:
2617:
2301:Hertzsprung–Russell diagram
2286:Hertzsprung–Russell diagram
2241:combined within its single
1899:Taurus-Orion R1 Association
1043:: Rigel, Algebar, Elgebar,
430:3.78 ± 0.34
68:Location of Rigel (circled)
8195:
8129:B-type main-sequence stars
6887:Orion in Chinese astronomy
6232:. Oxford, United Kingdom:
6205:10.1177/002182868601700202
5590:10.1051/0004-6361:20041213
5560:Astronomy and Astrophysics
5303:10.1088/0004-637X/720/1/46
5204:Astronomy and Astrophysics
5127:Astronomy and Astrophysics
5071:Astronomy and Astrophysics
4874:Astronomy and Astrophysics
4480:Cambridge University Press
4447:Dorling Kindersley Limited
4323:Astronomy and Astrophysics
4129:Cambridge University Press
4062:Cambridge University Press
3862:Astronomy and Astrophysics
3454:10.1088/0004-637X/749/1/74
3362:10.1051/0004-6361:20053832
3332:Astronomy and Astrophysics
3065:10.1051/0004-6361:20078357
3034:Astronomy and Astrophysics
2915:Orion in Chinese astronomy
2822:In Japan, the Minamoto or
2819:used in the South Island.
2661:Giovanni Battista Riccioli
2525:B-type main-sequence stars
2186:years. Gaia Data Release 2
2171:from Rigel A is over 2,200
1541:B class star, with strong
1519:equatorial navigation star
29:
8048:
8022:
7860:Becklin–Neugebauer Object
7652:
6877:
6298:University of Texas Press
5969:10.1007/s10509-007-9698-y
5846:. Boston, Massachusetts:
5272:The Astrophysical Journal
4923:10.1134/S1063772917010085
4767:The Astrophysical Journal
4701:The Astrophysical Journal
4564:The Astrophysical Journal
4379:Burnham, Robert (1978) .
4196:. pp. 159–162, 257.
3801:The Astrophysical Journal
3579:10.1134/S1063773706110065
3496:Tokovinin, A. A. (1997).
3424:The Astrophysical Journal
3211:The Astrophysical Journal
3151:10.1017/S1743921310009798
2832:
2500:; adopting a distance of
2433:. A 2018 study using the
2266:K-type main-sequence star
2108:
2085:
2069:
2057:
2055:
2046:
2040:
2038:
2036:
2034:
2009:
2001:
1999:
1993:
1985:
1976:
1968:
1964:
1949:
1947:
1410:variable star designation
1105:
1090:
1039:
983:
976:
972:
947:
943:
918:
893:
889:
885:
674:
669:
626:
537:
494:
490:
358:
351:
324:
263:
258:
205:
152:
73:
44:
8154:Arabic words and phrases
6564:Akira Matsumura (1988).
6290:Milbrath, Susan (1999).
6247:Taylor, Douglas (1946).
6166:(in German). Wiesbaden:
6162:Kunitzsch, Paul (1959).
6041:Plaskett, J. S. (1922).
5843:Foundations of Astronomy
5718:The Astronomical Journal
5412:The Astronomical Journal
5383:10.3847/1538-3881/aad1f1
5352:The Astronomical Journal
4695:Plaskett, J. S. (1909).
4597:Abetti, Giorgio (1963).
4507:Kerigan, Thomas (1835).
3759:10.3847/1538-3881/aa9d8b
3728:The Astronomical Journal
3270:The Astronomical Journal
2332:stellar evolution models
2276:Physical characteristics
2195:Sherburne Wesley Burnham
6834:My Favorite Double Star
6254:American Anthropologist
6141:Inc. pp. 312–313.
6129:Allen, Richard Hinckley
5961:2008Ap&SS.316...31D
5807:2018A&A...616A...1G
5649:2018A&A...616A...1G
5582:2004A&A...424..727P
5331:. Waukesha, Wisconsin:
5226:2023A&A...674A...1G
5180:Galaxy v23n06 (1965 08)
5149:2014A&A...566A.125C
5093:2010A&A...521A...5C
5045:2009A&A...507.1141L
4985:1989A&AS...79..263V
4886:1998A&A...330..215W
4829:10.1093/mnras/290.3.521
4345:2008A&A...487..211M
4258:Moore, Patrick (1996).
4192:. Hoboken, New Jersey:
3884:2010A&A...517A..38P
3514:1997A&AS..124...75T
3402:1978A&AS...34....1N
3354:2006A&A...445.1099P
3057:2007A&A...474..653V
2746:Collowgullouric Warepil
2718:("little woodpecker").
2457:, yielding a radius of
2445:. After correcting for
2307:would have been around
2117:for Rigel's components
1838:Hipparcos new reduction
1701:solar masses per year (
1517:. Rigel is a prominent
1181: – of a
738:Luminosity (bolometric)
476:Absolute magnitude
331:Evolutionary stage
270:Evolutionary stage
245:Apparent magnitude
192:Apparent magnitude
8164:Durchmusterung objects
7760:Lambda Orionis Cluster
6882:List of stars in Orion
6871:Constellation of Orion
6786:U.S. Geological Survey
6752:U.S. Geological Survey
4474:The Southern Sky Guide
3945:10.1098/rstl.1782.0014
3637:10.1093/mnras/stac1617
2836:), while the Taira or
2659:by Italian astronomer
2601:
2594:rijl al-jauza al-yusra
2546:Rigel is likely to be
2288:
2208:speckle interferometry
1833:
1643:
1456:
1437:Henry Draper Catalogue
1427:Orionis (19 Ori), the
1328:
1276:seventh-brightest star
32:Rigel (disambiguation)
8149:Orion (constellation)
8139:Multiple star systems
8134:Alpha Cygni variables
7765:Trapezium Cluster (θ)
6504:Best, Elsdon (1922).
5913:10.1093/mnrasl/slt165
4622:. Chicago, Illinois.
4407:"The Colour of Stars"
4225:Ridpath, Ian (1989).
4186:Schaaf, Fred (2008).
3973:Read January 10, 1782
3695:10.1093/mnras/stt2260
2817:southern name variant
2667:by German astronomer
2584:Abd al-Rahman al-Sufi
2581:
2506:John Stanley Plaskett
2305:effective temperature
2283:
1895:Orion OB1 association
1820:
1633:
1454:
1429:Bright Star Catalogue
1421:Flamsteed designation
1415:Rigel has many other
1337:astronomical catalogs
1319:
1272:intrinsic variability
6720:Yenne, Bill (2018).
5465:Webb, T. W. (1917).
2618:Rijl Jauzah al Yusrā
2415:, while summing the
2322:similar to those of
2235:spectroscopic binary
2180:common proper motion
2169:projected separation
1417:stellar designations
1298:spectroscopic binary
1268:Alpha Cygni variable
30:For other uses, see
8028:Astronomical events
6376:2010JAHH...13..220H
6197:1986JHA....17...89K
6059:1922PASP...34...79P
6010:2008poii.conf...71A
5904:2014MNRAS.439L...6G
5740:2009AJ....137.3358M
5703:1900PYerO...1....1B
5514:2010ocws.book.....B
5425:1968AJ.....73..233R
5405:Racine, R. (1968).
5374:2018AJ....156...84K
5295:2010ApJ...720...46G
5014:1999IBVS.4659....1K
4915:2017ARep...61...80S
4859:1985IBVS.2762....1G
4820:1997MNRAS.290..521I
4779:1933ApJ....77...67S
4749:2008cihw.conf..155M
4713:1909ApJ....30...26P
4682:2008hsf1.book..459B
4628:1943assw.book.....M
4576:1950ApJ...112..362M
4535:1978rmsa.book.....M
4264:. London: Cassell.
4202:2008bsdu.book.....S
4166:1994CoORB.115....1D
3936:1782RSPT...72..112H
3824:2012ApJ...747..108M
3750:2018AJ....155...30B
3686:2014MNRAS.438.1114S
3628:2022MNRAS.515....1D
3571:2006AstL...32..759G
3523:10.1051/aas:1997181
3446:2012ApJ...749...74M
3282:2001AJ....122.3466M
3224:1942ApJ....95..421S
3184:1997Msngr..87...27E
3142:2010HiA....15..359G
3102:2002yCat.2237....0D
2721:Rigel was known as
2679:by English scholar
2589:Book of Fixed Stars
2230:555 in modern use.
2224:double star catalog
2115:Hierarchical scheme
1861:Gaia Data Release 3
1523:82nd parallel north
1491:Southern Hemisphere
1487:Northern Hemisphere
1408:it has no separate
1222:surface temperature
1106:Database references
838:Rotational velocity
41:
8144:Population I stars
8124:B-type supergiants
6796:on 5 November 2020
6604:Shin seiza jyunrei
6514:. pp. 39–40.
6321:Mudrooroo (1994).
6139:Dover Publications
4658:Bally, J. (2008).
4231:and Bayer letters"
4131:. pp. 70–71.
2602:
2320:stellar pulsations
2316:visual wavelengths
2289:
2176:astronomical units
1884:angular separation
1834:
1644:
1616:looping structures
1465:apparent magnitude
1461:intrinsic variable
1457:
1329:
1264:apparent magnitude
978:Other designations
343:Spectral type
314:Variable type
282:Spectral type
39:
8179:Hipparcos objects
8169:Flamsteed objects
8062:
8061:
8044:
8043:
8018:
8017:
7933:
7932:
7773:
7772:
7689:
7688:
7648:
7647:
6733:978-1-58007-256-4
6617:978-4-12-204128-8
6608:Chuokoron-Shinsha
6585:978-4-385-14001-8
6490:978-1-4419-7623-9
6447:978-1-77007-453-8
6438:Struik Publishers
6416:978-0-9750908-0-0
6336:978-1-85538-306-7
6307:978-0-292-75226-9
6296:. Austin, Texas:
6168:Otto Harrassowitz
6148:978-0-486-21079-7
6111:978-0-691-18184-4
6027:978-3-540-74253-1
5857:978-1-305-56239-4
5335:. pp. 48–53.
4902:Astronomy Reports
4493:978-0-521-71405-1
4456:978-1-4093-2825-4
4392:978-0-486-23568-4
4271:978-0-304-34903-6
4244:978-0-7188-2695-6
4211:978-0-470-24917-8
4138:978-0-521-59889-7
4060:. Cambridge, UK:
3548:Astronomy Letters
3006:978-1-138-12566-7
2978:978-1-931559-44-7
2852:In modern culture
2669:Wilhelm Schickard
2649:Alphonsine tables
2560:type II supernova
2536:Stellar evolution
2408:and 363,000
2112:
2111:
1952:Separation = 9.5″
1905:. Betelgeuse and
1823:reflection nebula
1662:From analysis of
1618:arising from the
1576:around a mean of
1555:bright supergiant
1406:Bayer designation
1185:of at least four
1152:Bayer designation
1133:
1132:
410: +0.50
398: +1.31
16:(Redirected from
8186:
8103:
8102:
8101:
8091:
8090:
8079:
8078:
8077:
8070:
8054:
8053:
8024:
7944:
7890:Horsehead Nebula
7784:
7702:
7654:
6917:
6864:
6857:
6850:
6841:
6806:
6805:
6803:
6801:
6792:. Archived from
6778:
6772:
6771:
6769:
6767:
6744:
6738:
6737:
6717:
6711:
6710:
6708:
6706:
6695:
6689:
6688:
6686:
6684:
6673:
6667:
6666:
6658:
6652:
6651:
6649:
6647:
6638:(in Norwegian).
6628:
6622:
6621:
6596:
6590:
6589:
6560:
6554:
6553:
6551:
6549:
6534:
6528:
6527:
6525:
6523:
6501:
6495:
6494:
6470:
6464:
6463:
6461:
6459:
6427:
6421:
6420:
6402:
6396:
6395:
6369:
6347:
6341:
6340:
6318:
6312:
6311:
6287:
6281:
6280:
6270:
6244:
6238:
6237:
6223:
6217:
6216:
6178:
6172:
6171:
6159:
6153:
6152:
6125:
6116:
6115:
6093:
6087:
6086:
6038:
6032:
6031:
5997:
5991:
5990:
5954:
5932:
5926:
5925:
5915:
5897:
5873:
5862:
5861:
5848:Cengage Learning
5837:
5831:
5821:
5819:
5809:
5799:
5766:
5760:
5759:
5733:
5713:
5707:
5706:
5686:
5673:
5663:
5661:
5651:
5641:
5608:
5602:
5601:
5575:
5573:astro-ph/0406573
5551:
5540:
5539:
5537:
5535:
5495:
5489:
5488:
5486:
5484:
5462:
5456:
5455:
5445:
5439:
5438:
5436:
5402:
5396:
5395:
5385:
5367:
5343:
5337:
5336:
5324:
5315:
5314:
5288:
5266:
5257:
5247:
5237:
5219:
5191:
5185:
5184:
5175:
5169:
5168:
5142:
5122:
5113:
5112:
5086:
5065:
5059:
5058:
5056:
5039:(2): 1141–1201.
5024:
5018:
5017:
4995:
4989:
4988:
4967:
4961:
4960:
4958:
4956:
4941:
4935:
4934:
4896:
4890:
4889:
4869:
4863:
4862:
4840:
4834:
4833:
4831:
4797:
4791:
4790:
4762:
4753:
4752:
4736:
4727:
4726:
4724:
4692:
4686:
4685:
4675:
4655:
4646:
4645:
4639:
4631:
4615:
4609:
4608:
4594:
4588:
4587:
4559:
4553:
4552:
4546:
4538:
4522:
4516:
4515:
4504:
4498:
4497:
4477:
4467:
4461:
4460:
4437:
4431:
4430:
4428:
4426:
4421:on 18 March 2012
4403:
4397:
4396:
4376:
4365:
4364:
4338:
4317:
4306:
4305:
4303:
4301:
4282:
4276:
4275:
4255:
4249:
4248:
4222:
4216:
4215:
4183:
4170:
4169:
4149:
4143:
4142:
4120:
4111:
4110:
4108:
4106:
4086:
4073:
4072:
4070:
4059:
4044:
4033:
4032:
4030:
4028:
4013:
4007:
4006:
4004:
4002:
3982:
3976:
3975:
3970:
3968:
3962:
3947:
3913:
3904:
3903:
3877:
3857:
3844:
3843:
3817:
3791:
3772:
3771:
3761:
3743:
3719:
3708:
3707:
3697:
3679:
3653:
3642:
3641:
3639:
3621:
3597:
3591:
3590:
3564:
3542:
3536:
3535:
3525:
3493:
3466:
3465:
3439:
3419:
3406:
3405:
3383:
3374:
3373:
3347:
3345:astro-ph/0509669
3338:(3): 1099–1126.
3327:
3308:
3307:
3305:
3303:
3293:
3276:(6): 3466–3471.
3261:
3238:
3237:
3235:
3201:
3188:
3187:
3165:
3156:
3155:
3153:
3119:
3106:
3105:
3083:
3077:
3076:
3050:
3028:
3011:
3010:
2989:
2983:
2982:
2960:
2944:
2941:
2935:
2931:
2882:program for the
2835:
2834:
2637:
2631:
2630:
2620:
2611:Alfonsine tables
2569:
2503:
2499:
2495:
2484:
2482:
2467:
2466:
2465:
2456:
2454:
2444:
2439:angular diameter
2432:
2424:
2373:
2371:
2365:
2362:
2360:
2354:
2346:
2340:
2313:
2263:
2256:
2248:
2243:stellar spectrum
2229:
2221:
2217:
2213:
2205:
2201:
2189:
2185:
2174:
2162:visual magnitude
2150:
2146:
2142:
2138:
2133:William Herschel
2127:visual companion
2080:
2075:
2020:
2015:
1957:
1922:
1921:
1889:
1870:
1868:
1854:
1849:
1808:
1800:
1787:
1783:
1774:
1768:
1759:
1755:
1749:
1740:
1736:
1719:
1700:
1698:
1694:
1601:
1593:
1579:
1575:
1551:luminosity class
1545:of the hydrogen
1543:absorption lines
1484:
1469:celestial sphere
1442:
1434:
1426:
1370:
1363:
1356:
1349:
1344:
1295:
1245:
1230:
1201:) from the Sun.
1165:and abbreviated
1100:
1085:
1074:
1067:
1060:
1053:
1033:
1026:
1019:
1014:
1008:
1001:
994:
877:
875:
858:
856:
827:
825:
805:
803:
783:
781:
751:
750:
749:
723:
722:
721:
693:
691:
464:
462:
451:
449:
409:
397:
381:
379:
259:Characteristics
254:
248:
235:
224:
219:
201:
195:
182:
171:
166:
148:
147:
144:
143:
140:
131:
130:
127:
126:
123:
120:
117:
114:
74:Observation data
61:
54:
42:
21:
18:Rigel in fiction
8194:
8193:
8189:
8188:
8187:
8185:
8184:
8183:
8114:
8113:
8111:
8109:
8099:
8097:
8085:
8075:
8073:
8065:
8063:
8058:
8040:
8014:
7978:
7929:
7910:McNeil's Nebula
7833:
7769:
7748:
7696:
7685:
7644:
7640:WISE J0521+1025
7635:WISE J0457−0207
7553:
7510:
7447:
7349:
7146:
6906:
6873:
6868:
6814:
6809:
6799:
6797:
6780:
6779:
6775:
6765:
6763:
6746:
6745:
6741:
6734:
6719:
6718:
6714:
6704:
6702:
6697:
6696:
6692:
6682:
6680:
6675:
6674:
6670:
6660:
6659:
6655:
6645:
6643:
6630:
6629:
6625:
6618:
6598:
6597:
6593:
6586:
6563:
6561:
6557:
6547:
6545:
6536:
6535:
6531:
6521:
6519:
6512:Dominion Museum
6503:
6502:
6498:
6491:
6483:. p. 341.
6472:
6471:
6467:
6457:
6455:
6448:
6440:. p. 419.
6429:
6428:
6424:
6417:
6404:
6403:
6399:
6349:
6348:
6344:
6337:
6329:. p. 142.
6320:
6319:
6315:
6308:
6289:
6288:
6284:
6246:
6245:
6241:
6234:Clarendon Press
6225:
6224:
6220:
6180:
6179:
6175:
6161:
6160:
6156:
6149:
6127:
6126:
6119:
6112:
6095:
6094:
6090:
6040:
6039:
6035:
6028:
5999:
5998:
5994:
5979:
5934:
5933:
5929:
5875:
5874:
5865:
5858:
5850:. p. 274.
5839:
5838:
5834:
5770:Brown, A. G. A.
5768:
5767:
5763:
5715:
5714:
5710:
5688:
5687:
5676:
5612:Brown, A. G. A.
5610:
5609:
5605:
5557:
5553:
5552:
5543:
5533:
5531:
5524:
5508:. p. 434.
5497:
5496:
5492:
5482:
5480:
5464:
5463:
5459:
5447:
5446:
5442:
5404:
5403:
5399:
5345:
5344:
5340:
5326:
5325:
5318:
5268:
5267:
5260:
5193:
5192:
5188:
5177:
5176:
5172:
5124:
5123:
5116:
5067:
5066:
5062:
5026:
5025:
5021:
4997:
4996:
4992:
4969:
4968:
4964:
4954:
4952:
4943:
4942:
4938:
4898:
4897:
4893:
4871:
4870:
4866:
4842:
4841:
4837:
4799:
4798:
4794:
4764:
4763:
4756:
4738:
4737:
4730:
4694:
4693:
4689:
4657:
4656:
4649:
4632:
4617:
4616:
4612:
4596:
4595:
4591:
4561:
4560:
4556:
4539:
4524:
4523:
4519:
4506:
4505:
4501:
4494:
4469:
4468:
4464:
4457:
4439:
4438:
4434:
4424:
4422:
4405:
4404:
4400:
4393:
4378:
4377:
4368:
4319:
4318:
4309:
4299:
4297:
4284:
4283:
4279:
4272:
4261:Brilliant Stars
4257:
4256:
4252:
4245:
4224:
4223:
4219:
4212:
4185:
4184:
4173:
4151:
4150:
4146:
4139:
4122:
4121:
4114:
4104:
4102:
4088:
4087:
4076:
4068:
4057:
4046:
4045:
4036:
4026:
4024:
4015:
4014:
4010:
4000:
3998:
3984:
3983:
3979:
3966:
3964:
3960:
3915:
3914:
3907:
3859:
3858:
3847:
3793:
3792:
3775:
3721:
3720:
3711:
3655:
3654:
3645:
3599:
3598:
3594:
3555:(11): 759–771.
3544:
3543:
3539:
3495:
3494:
3469:
3421:
3420:
3409:
3385:
3384:
3377:
3329:
3328:
3311:
3301:
3299:
3263:
3262:
3241:
3203:
3202:
3191:
3167:
3166:
3159:
3121:
3120:
3109:
3085:
3084:
3080:
3030:
3029:
3014:
3007:
2991:
2990:
2986:
2979:
2962:
2961:
2957:
2953:
2948:
2947:
2942:
2938:
2932:
2928:
2923:
2911:
2854:
2809:Chatham Islands
2791:heliacal rising
2750:Wardaman people
2723:Yerrerdet-kurrk
2712:Lacandon people
2700:Norse mythology
2681:Edmund Chilmead
2576:
2567:
2553:Ledoux Criteria
2533:
2514:
2511:
2501:
2497:
2493:
2491:
2488:
2480:
2478:
2475:
2472:
2463:
2461:
2460:
2458:
2452:
2450:
2442:
2431:
2428:
2422:
2420:
2414:
2411:
2407:
2404:
2400:
2397:
2392:
2389:
2380:
2377:
2369:
2367:
2363:
2358:
2356:
2353:
2344:
2342:
2335:
2308:
2293:blue supergiant
2278:
2258:
2254:
2246:
2227:
2219:
2215:
2211:
2203:
2199:
2187:
2183:
2172:
2148:
2144:
2140:
2136:
2119:
2078:
2076:
2073:
2018:
2016:
2013:
1955:
1954:Period = 24,000
1953:
1919:
1887:
1869:0.0553 mas
1866:
1864:
1857:margin of error
1847:
1845:
1815:
1807:
1804:
1798:
1796:
1794:
1791:
1785:
1781:
1778:
1772:
1770:
1766:
1763:
1757:
1753:
1751:
1747:
1744:
1738:
1734:
1732:
1717:
1708:
1705:
1696:
1692:
1690:
1687:
1628:
1604:P Cygni profile
1599:
1588:
1577:
1570:
1562:radial velocity
1531:
1482:
1449:
1440:
1432:
1424:
1368:
1361:
1354:
1347:
1342:
1314:
1290:
1243:
1225:
1218:that of the Sun
1140:blue supergiant
1098:
1083:
1072:
1065:
1058:
1051:
1035:
1031:
1024:
1017:
1012:
1006:
999:
992:
967:
964:
938:
935:
913:
910:
873:
871:
854:
852:
844: sin
823:
821:
801:
799:
779:
777:
767:Surface gravity
759:
756:
747:
745:
744:
742:
731:
728:
719:
717:
716:
714:
701:
698:
689:
687:
618:
616:
601:
599:
481:
460:
458:
456:
447:
445:
406:
377:
375:
370:
365:Radial velocity
275:Blue supergiant
252:
243:
229:
222:
216:Right ascension
213:
199:
190:
176:
169:
163:Right ascension
160:
137:
133:
111:
107:
75:
69:
67:
66:
65:
64:
63:
62:
35:
28:
23:
22:
15:
12:
11:
5:
8192:
8190:
8182:
8181:
8176:
8171:
8166:
8161:
8156:
8151:
8146:
8141:
8136:
8131:
8126:
8116:
8115:
8108:
8107:
8095:
8083:
8060:
8059:
8049:
8046:
8045:
8042:
8041:
8039:
8038:
8032:
8030:
8020:
8019:
8016:
8015:
8013:
8012:
8007:
8002:
7997:
7992:
7986:
7984:
7980:
7979:
7977:
7976:
7971:
7966:
7961:
7956:
7950:
7948:
7941:
7935:
7934:
7931:
7930:
7928:
7927:
7922:
7917:
7912:
7907:
7902:
7897:
7892:
7887:
7882:
7877:
7872:
7867:
7862:
7857:
7852:
7847:
7841:
7839:
7835:
7834:
7832:
7831:
7826:
7821:
7816:
7811:
7806:
7801:
7796:
7790:
7788:
7781:
7775:
7774:
7771:
7770:
7768:
7767:
7762:
7756:
7754:
7750:
7749:
7747:
7746:
7741:
7736:
7731:
7726:
7721:
7716:
7710:
7708:
7699:
7691:
7690:
7687:
7686:
7684:
7683:
7678:
7673:
7668:
7662:
7660:
7650:
7649:
7646:
7645:
7643:
7642:
7637:
7632:
7627:
7622:
7617:
7612:
7607:
7602:
7597:
7592:
7587:
7582:
7577:
7572:
7567:
7561:
7559:
7555:
7554:
7552:
7551:
7546:
7541:
7536:
7531:
7526:
7520:
7518:
7512:
7511:
7509:
7508:
7503:
7498:
7493:
7488:
7483:
7478:
7473:
7468:
7463:
7457:
7455:
7449:
7448:
7446:
7445:
7440:
7435:
7430:
7425:
7420:
7415:
7410:
7405:
7400:
7395:
7390:
7385:
7380:
7375:
7370:
7365:
7359:
7357:
7351:
7350:
7348:
7347:
7342:
7337:
7332:
7327:
7322:
7317:
7312:
7307:
7302:
7297:
7292:
7287:
7282:
7277:
7272:
7267:
7262:
7257:
7252:
7247:
7242:
7237:
7232:
7227:
7222:
7217:
7212:
7207:
7202:
7197:
7192:
7187:
7182:
7177:
7172:
7167:
7162:
7156:
7154:
7148:
7147:
7145:
7144:
7139:
7134:
7129:
7124:
7119:
7114:
7109:
7101:
7096:
7091:
7086:
7081:
7076:
7071:
7066:
7061:
7056:
7051:
7046:
7041:
7036:
7031:
7026:
7021:
7016:
7011:
7010:
7009:
7004:
6999:
6994:
6989:
6984:
6979:
6974:
6964:
6956:
6951:
6946:
6941:
6936:
6931:
6929:α (Betelgeuse)
6925:
6923:
6914:
6908:
6907:
6905:
6904:
6899:
6894:
6889:
6884:
6878:
6875:
6874:
6869:
6867:
6866:
6859:
6852:
6844:
6838:
6837:
6831:
6825:
6820:
6813:
6812:External links
6810:
6808:
6807:
6773:
6739:
6732:
6712:
6690:
6668:
6653:
6623:
6616:
6610:. p. 19.
6591:
6584:
6555:
6529:
6496:
6489:
6465:
6446:
6422:
6415:
6407:Dark Sparklers
6397:
6360:(3): 220–234.
6342:
6335:
6313:
6306:
6300:. p. 39.
6282:
6261:(2): 215–222.
6239:
6218:
6173:
6154:
6147:
6117:
6110:
6088:
6067:10.1086/123157
6053:(198): 79–93.
6033:
6026:
5992:
5978:978-1402094408
5977:
5945:(1–4): 31–41.
5927:
5863:
5856:
5832:
5761:
5708:
5674:
5603:
5566:(2): 727–732.
5555:
5541:
5523:978-1441917775
5522:
5490:
5457:
5440:
5434:10.1086/110624
5397:
5338:
5333:Kalmbach Books
5329:The New Cosmos
5316:
5258:
5186:
5170:
5114:
5060:
5019:
4990:
4962:
4936:
4891:
4864:
4835:
4814:(3): 521–532.
4792:
4787:10.1086/143448
4754:
4728:
4722:10.1086/141674
4687:
4647:
4610:
4600:Solar research
4589:
4584:10.1086/145351
4554:
4517:
4499:
4492:
4462:
4455:
4432:
4398:
4391:
4366:
4307:
4277:
4270:
4250:
4243:
4217:
4210:
4171:
4144:
4137:
4112:
4074:
4034:
4008:
3977:
3905:
3845:
3808:(1): 108–115.
3773:
3709:
3643:
3592:
3537:
3467:
3407:
3375:
3309:
3291:10.1086/323920
3239:
3233:10.1086/144412
3189:
3157:
3107:
3078:
3041:(2): 653–664.
3012:
3005:
2984:
2977:
2954:
2952:
2949:
2946:
2945:
2936:
2925:
2924:
2922:
2919:
2918:
2917:
2910:
2907:
2891:Rigel Skerries
2880:cruise missile
2853:
2850:
2805:Moriori people
2710:(Sirius). The
2635:rijl al-jabbār
2575:
2572:
2541:red supergiant
2532:
2529:
2512:
2509:
2489:
2486:
2473:
2470:
2455:0.009 mas
2447:limb darkening
2443:2.526 mas
2429:
2426:
2412:
2409:
2405:
2402:
2398:
2395:
2390:
2387:
2378:
2375:
2351:
2277:
2274:
2239:spectral lines
2158:position angle
2110:
2109:
2106:
2105:
2103:
2098:
2096:
2094:
2092:
2089:
2088:
2086:
2083:
2082:
2070:
2068:
2066:
2064:
2062:
2059:
2058:
2056:
2053:
2052:
2047:
2045:
2043:
2041:
2039:
2037:
2035:
2033:
2030:
2029:
2027:
2025:
2022:
2021:
2010:
2008:
2006:
2004:
2002:
2000:
1998:
1995:
1994:
1992:
1990:
1988:
1986:
1983:
1982:
1977:
1975:
1973:
1971:
1969:
1967:
1965:
1962:
1960:
1959:
1950:
1948:
1946:
1943:
1942:
1940:
1937:
1936:
1934:
1929:
1927:
1925:
1920:
1918:
1917:Stellar system
1915:
1814:
1811:
1805:
1802:
1792:
1789:
1779:
1776:
1764:
1761:
1750:in 2006-7 and
1745:
1742:
1706:
1703:
1686:
1683:
1652:CCD photometry
1627:
1624:
1596:emission spike
1578:21.5 km/s
1566:Doppler shifts
1530:
1527:
1501:that includes
1495:Winter Hexagon
1448:
1445:
1435:1713, and the
1397:James B. Kaler
1395:). Astronomer
1376:05145-0812 or
1325:hydrogen-alpha
1313:
1310:
1131:
1130:
1125:
1122:
1121:
1116:
1108:
1107:
1103:
1102:
1088:
1087:
1037:
1036:
984:
981:
980:
974:
973:
970:
969:
965:
962:
958:
950:
949:
945:
944:
941:
940:
936:
933:
929:
921:
920:
916:
915:
911:
908:
904:
896:
895:
891:
890:
887:
886:
883:
882:
869:
861:
860:
850:
833:
832:
819:
811:
810:
797:
789:
788:
775:
762:
761:
757:
754:
740:
734:
733:
729:
726:
712:
704:
703:
699:
696:
685:
677:
676:
672:
671:
667:
666:
660:
651:
650:
647:
641:
640:
637:
631:
630:
624:
623:
620:
614:
611:Semi-amplitude
607:
606:
603:
597:
593:Semi-amplitude
588:
587:
584:
575:
574:
571:
562:
561:
558:
552:
551:
548:
542:
541:
535:
534:
528:
519:
518:
515:
509:
508:
505:
499:
498:
492:
491:
488:
487:
484:
479:
471:
470:
443:
435:
434:
428:
419:
418:
393:
384:
383:
373:
368:
360:
359:
356:
355:
349:
348:
345:
339:
338:
333:
327:
326:
322:
321:
316:
310:
309:
306:
299:
298:
295:
288:
287:
284:
278:
277:
272:
266:
265:
261:
260:
256:
255:
249:
240:
239:
236:
226:
225:
220:
210:
209:
203:
202:
196:
187:
186:
183:
173:
172:
170:05 14 32.27210
167:
157:
156:
150:
149:
105:
99:
98:
93:
85:
84:
71:
70:
56:
55:
49:
48:
47:
46:
45:
26:
24:
14:
13:
10:
9:
6:
4:
3:
2:
8191:
8180:
8177:
8175:
8172:
8170:
8167:
8165:
8162:
8160:
8159:Bayer objects
8157:
8155:
8152:
8150:
8147:
8145:
8142:
8140:
8137:
8135:
8132:
8130:
8127:
8125:
8122:
8121:
8119:
8112:
8106:
8096:
8094:
8089:
8084:
8082:
8072:
8068:
8057:
8047:
8037:
8034:
8033:
8031:
8029:
8025:
8021:
8011:
8008:
8006:
8003:
8001:
7998:
7996:
7993:
7991:
7988:
7987:
7985:
7981:
7975:
7972:
7970:
7967:
7965:
7962:
7960:
7957:
7955:
7952:
7951:
7949:
7945:
7942:
7940:
7936:
7926:
7923:
7921:
7918:
7916:
7913:
7911:
7908:
7906:
7903:
7901:
7898:
7896:
7893:
7891:
7888:
7886:
7883:
7881:
7878:
7876:
7873:
7871:
7868:
7866:
7863:
7861:
7858:
7856:
7853:
7851:
7848:
7846:
7843:
7842:
7840:
7836:
7830:
7827:
7825:
7822:
7820:
7817:
7815:
7812:
7810:
7807:
7805:
7802:
7800:
7797:
7795:
7792:
7791:
7789:
7785:
7782:
7780:
7776:
7766:
7763:
7761:
7758:
7757:
7755:
7751:
7745:
7742:
7740:
7737:
7735:
7732:
7730:
7727:
7725:
7722:
7720:
7717:
7715:
7712:
7711:
7709:
7707:
7703:
7700:
7698:
7692:
7682:
7679:
7677:
7674:
7672:
7669:
7667:
7664:
7663:
7661:
7659:
7655:
7651:
7641:
7638:
7636:
7633:
7631:
7628:
7626:
7623:
7621:
7618:
7616:
7613:
7611:
7608:
7606:
7603:
7601:
7598:
7596:
7593:
7591:
7588:
7586:
7583:
7581:
7578:
7576:
7573:
7571:
7568:
7566:
7563:
7562:
7560:
7556:
7550:
7547:
7545:
7542:
7540:
7537:
7535:
7532:
7530:
7527:
7525:
7522:
7521:
7519:
7517:
7513:
7507:
7504:
7502:
7499:
7497:
7494:
7492:
7489:
7487:
7484:
7482:
7479:
7477:
7474:
7472:
7469:
7467:
7464:
7462:
7459:
7458:
7456:
7454:
7450:
7444:
7441:
7439:
7436:
7434:
7431:
7429:
7426:
7424:
7421:
7419:
7416:
7414:
7411:
7409:
7406:
7404:
7401:
7399:
7396:
7394:
7391:
7389:
7386:
7384:
7381:
7379:
7376:
7374:
7371:
7369:
7366:
7364:
7361:
7360:
7358:
7356:
7352:
7346:
7343:
7341:
7338:
7336:
7333:
7331:
7328:
7326:
7323:
7321:
7318:
7316:
7313:
7311:
7308:
7306:
7303:
7301:
7298:
7296:
7293:
7291:
7288:
7286:
7283:
7281:
7278:
7276:
7273:
7271:
7268:
7266:
7263:
7261:
7258:
7256:
7253:
7251:
7248:
7246:
7243:
7241:
7238:
7236:
7233:
7231:
7228:
7226:
7223:
7221:
7218:
7216:
7213:
7211:
7208:
7206:
7203:
7201:
7198:
7196:
7193:
7191:
7188:
7186:
7183:
7181:
7178:
7176:
7173:
7171:
7168:
7166:
7163:
7161:
7158:
7157:
7155:
7153:
7149:
7143:
7140:
7138:
7135:
7133:
7130:
7128:
7125:
7123:
7120:
7118:
7115:
7113:
7110:
7108:
7107:
7102:
7100:
7097:
7095:
7092:
7090:
7087:
7085:
7082:
7080:
7077:
7075:
7072:
7070:
7067:
7065:
7062:
7060:
7057:
7055:
7052:
7050:
7047:
7045:
7042:
7040:
7037:
7035:
7032:
7030:
7027:
7025:
7022:
7020:
7017:
7015:
7012:
7008:
7005:
7003:
7000:
6998:
6995:
6993:
6990:
6988:
6985:
6983:
6980:
6978:
6975:
6973:
6970:
6969:
6968:
6965:
6963:
6962:
6957:
6955:
6952:
6950:
6947:
6945:
6942:
6940:
6939:γ (Bellatrix)
6937:
6935:
6932:
6930:
6927:
6926:
6924:
6922:
6918:
6915:
6913:
6909:
6903:
6902:Orion's Sword
6900:
6898:
6895:
6893:
6890:
6888:
6885:
6883:
6880:
6879:
6876:
6872:
6865:
6860:
6858:
6853:
6851:
6846:
6845:
6842:
6835:
6832:
6829:
6826:
6824:
6821:
6819:
6816:
6815:
6811:
6795:
6791:
6787:
6783:
6777:
6774:
6761:
6757:
6753:
6749:
6743:
6740:
6735:
6729:
6725:
6724:
6716:
6713:
6700:
6694:
6691:
6678:
6672:
6669:
6664:
6657:
6654:
6641:
6637:
6633:
6627:
6624:
6619:
6613:
6609:
6605:
6601:
6595:
6592:
6587:
6581:
6577:
6573:
6569:
6568:
6559:
6556:
6544:
6543:Renshaw Works
6540:
6533:
6530:
6517:
6513:
6509:
6508:
6500:
6497:
6492:
6486:
6482:
6478:
6477:
6469:
6466:
6453:
6449:
6443:
6439:
6435:
6434:
6426:
6423:
6418:
6412:
6408:
6401:
6398:
6393:
6389:
6385:
6381:
6377:
6373:
6368:
6363:
6359:
6355:
6354:
6346:
6343:
6338:
6332:
6328:
6327:HarperCollins
6324:
6317:
6314:
6309:
6303:
6299:
6295:
6294:
6286:
6283:
6278:
6274:
6269:
6264:
6260:
6256:
6255:
6250:
6243:
6240:
6235:
6231:
6230:
6222:
6219:
6214:
6210:
6206:
6202:
6198:
6194:
6190:
6186:
6185:
6177:
6174:
6170:. p. 46.
6169:
6165:
6158:
6155:
6150:
6144:
6140:
6136:
6135:
6130:
6124:
6122:
6118:
6113:
6107:
6103:
6099:
6092:
6089:
6084:
6080:
6076:
6072:
6068:
6064:
6060:
6056:
6052:
6048:
6044:
6037:
6034:
6029:
6023:
6019:
6015:
6011:
6007:
6003:
5996:
5993:
5988:
5984:
5980:
5974:
5970:
5966:
5962:
5958:
5953:
5948:
5944:
5940:
5939:
5931:
5928:
5923:
5919:
5914:
5909:
5905:
5901:
5896:
5891:
5887:
5883:
5879:
5872:
5870:
5868:
5864:
5859:
5853:
5849:
5845:
5844:
5836:
5833:
5829:
5825:
5818:
5813:
5808:
5803:
5798:
5793:
5789:
5785:
5784:
5779:
5777:
5771:
5765:
5762:
5757:
5753:
5749:
5745:
5741:
5737:
5732:
5727:
5723:
5719:
5712:
5709:
5704:
5700:
5696:
5692:
5685:
5683:
5681:
5679:
5675:
5671:
5667:
5660:
5655:
5650:
5645:
5640:
5635:
5631:
5627:
5626:
5621:
5619:
5613:
5607:
5604:
5599:
5595:
5591:
5587:
5583:
5579:
5574:
5569:
5565:
5561:
5550:
5548:
5546:
5542:
5529:
5525:
5519:
5515:
5511:
5507:
5503:
5502:
5494:
5491:
5478:
5474:
5470:
5469:
5461:
5458:
5453:
5452:
5444:
5441:
5435:
5430:
5426:
5422:
5418:
5414:
5413:
5408:
5401:
5398:
5393:
5389:
5384:
5379:
5375:
5371:
5366:
5361:
5357:
5353:
5349:
5342:
5339:
5334:
5330:
5323:
5321:
5317:
5312:
5308:
5304:
5300:
5296:
5292:
5287:
5282:
5278:
5274:
5273:
5265:
5263:
5259:
5255:
5251:
5245:
5241:
5236:
5231:
5227:
5223:
5218:
5213:
5209:
5205:
5201:
5199:
5190:
5187:
5182:
5181:
5174:
5171:
5166:
5162:
5158:
5154:
5150:
5146:
5141:
5136:
5132:
5128:
5121:
5119:
5115:
5110:
5106:
5102:
5098:
5094:
5090:
5085:
5080:
5076:
5072:
5064:
5061:
5055:
5050:
5046:
5042:
5038:
5034:
5030:
5023:
5020:
5015:
5011:
5007:
5003:
5002:
4994:
4991:
4986:
4982:
4978:
4974:
4966:
4963:
4950:
4946:
4940:
4937:
4932:
4928:
4924:
4920:
4916:
4912:
4908:
4904:
4903:
4895:
4892:
4887:
4883:
4879:
4875:
4868:
4865:
4860:
4856:
4852:
4848:
4847:
4839:
4836:
4830:
4825:
4821:
4817:
4813:
4809:
4808:
4803:
4796:
4793:
4788:
4784:
4780:
4776:
4772:
4768:
4761:
4759:
4755:
4750:
4746:
4742:
4735:
4733:
4729:
4723:
4718:
4714:
4710:
4706:
4702:
4698:
4691:
4688:
4683:
4679:
4674:
4669:
4665:
4661:
4654:
4652:
4648:
4643:
4637:
4629:
4625:
4621:
4614:
4611:
4606:
4602:
4601:
4593:
4590:
4585:
4581:
4577:
4573:
4569:
4565:
4558:
4555:
4550:
4544:
4536:
4532:
4528:
4521:
4518:
4513:
4512:
4503:
4500:
4495:
4489:
4485:
4481:
4476:
4475:
4466:
4463:
4458:
4452:
4448:
4444:
4443:
4436:
4433:
4420:
4416:
4412:
4408:
4402:
4399:
4394:
4388:
4384:
4383:
4375:
4373:
4371:
4367:
4362:
4358:
4354:
4350:
4346:
4342:
4337:
4332:
4328:
4324:
4316:
4314:
4312:
4308:
4295:
4291:
4287:
4281:
4278:
4273:
4267:
4263:
4262:
4254:
4251:
4246:
4240:
4236:
4232:
4230:
4221:
4218:
4213:
4207:
4203:
4199:
4195:
4191:
4190:
4182:
4180:
4178:
4176:
4172:
4167:
4163:
4159:
4155:
4148:
4145:
4140:
4134:
4130:
4126:
4119:
4117:
4113:
4100:
4096:
4092:
4085:
4083:
4081:
4079:
4075:
4067:
4063:
4056:
4055:
4050:
4043:
4041:
4039:
4035:
4022:
4018:
4012:
4009:
3997:
3993:
3992:
3987:
3981:
3978:
3974:
3959:
3955:
3951:
3946:
3941:
3937:
3933:
3929:
3925:
3924:
3919:
3912:
3910:
3906:
3901:
3897:
3893:
3889:
3885:
3881:
3876:
3871:
3867:
3863:
3856:
3854:
3852:
3850:
3846:
3841:
3837:
3833:
3829:
3825:
3821:
3816:
3811:
3807:
3803:
3802:
3797:
3790:
3788:
3786:
3784:
3782:
3780:
3778:
3774:
3769:
3765:
3760:
3755:
3751:
3747:
3742:
3737:
3733:
3729:
3725:
3718:
3716:
3714:
3710:
3705:
3701:
3696:
3691:
3687:
3683:
3678:
3673:
3669:
3665:
3664:
3659:
3652:
3650:
3648:
3644:
3638:
3633:
3629:
3625:
3620:
3615:
3611:
3607:
3603:
3596:
3593:
3588:
3584:
3580:
3576:
3572:
3568:
3563:
3558:
3554:
3550:
3549:
3541:
3538:
3533:
3529:
3524:
3519:
3515:
3511:
3507:
3503:
3499:
3492:
3490:
3488:
3486:
3484:
3482:
3480:
3478:
3476:
3474:
3472:
3468:
3463:
3459:
3455:
3451:
3447:
3443:
3438:
3433:
3429:
3425:
3418:
3416:
3414:
3412:
3408:
3403:
3399:
3395:
3391:
3390:
3382:
3380:
3376:
3371:
3367:
3363:
3359:
3355:
3351:
3346:
3341:
3337:
3333:
3326:
3324:
3322:
3320:
3318:
3316:
3314:
3310:
3297:
3292:
3287:
3283:
3279:
3275:
3271:
3267:
3260:
3258:
3256:
3254:
3252:
3250:
3248:
3246:
3244:
3240:
3234:
3229:
3225:
3221:
3217:
3213:
3212:
3207:
3200:
3198:
3196:
3194:
3190:
3185:
3181:
3177:
3173:
3172:
3171:The Messenger
3164:
3162:
3158:
3152:
3147:
3143:
3139:
3135:
3131:
3130:
3125:
3118:
3116:
3114:
3112:
3108:
3103:
3099:
3095:
3091:
3090:
3082:
3079:
3074:
3070:
3066:
3062:
3058:
3054:
3049:
3044:
3040:
3036:
3035:
3027:
3025:
3023:
3021:
3019:
3017:
3013:
3008:
3002:
2998:
2994:
2988:
2985:
2980:
2974:
2970:
2966:
2959:
2956:
2950:
2940:
2937:
2930:
2927:
2920:
2916:
2913:
2912:
2908:
2906:
2904:
2900:
2896:
2892:
2887:
2885:
2881:
2877:
2876:SSM-N-6 Rigel
2873:
2872:
2866:
2862:
2861:
2851:
2849:
2847:
2843:
2839:
2829:
2825:
2820:
2818:
2814:
2810:
2806:
2802:
2798:
2797:
2792:
2788:
2784:
2780:
2779:
2774:
2769:
2767:
2763:
2759:
2755:
2751:
2747:
2743:
2739:
2735:
2731:
2728:
2724:
2719:
2717:
2713:
2709:
2705:
2701:
2697:
2693:
2689:
2684:
2682:
2678:
2674:
2673:Rigel Algeuze
2670:
2666:
2662:
2658:
2654:
2650:
2646:
2642:
2638:
2636:
2625:
2621:
2619:
2613:
2612:
2607:
2599:
2595:
2591:
2590:
2585:
2580:
2573:
2571:
2565:
2561:
2556:
2554:
2549:
2548:fusing helium
2544:
2542:
2537:
2530:
2528:
2526:
2520:
2518:
2507:
2483:0.01 mas
2476:
2448:
2440:
2437:measured the
2436:
2418:
2393:
2382:
2355:at an age of
2350:
2339:
2333:
2327:
2325:
2321:
2318:is caused by
2317:
2312:
2306:
2302:
2298:
2297:main sequence
2294:
2287:
2282:
2275:
2273:
2269:
2267:
2262:
2251:
2244:
2240:
2236:
2231:
2225:
2209:
2196:
2191:
2181:
2177:
2170:
2165:
2163:
2159:
2154:
2134:
2130:
2128:
2124:
2118:
2116:
2107:
2102:
2097:
2095:
2090:
2087:
2084:
2072:Separation =
2067:
2065:
2063:
2060:
2054:
2051:
2044:
2042:
2031:
2028:
2026:
2024:
2023:
2014:0.58 mas
2012:Separation =
2007:
2005:
2003:
1996:
1991:
1989:
1987:
1984:
1981:
1974:
1972:
1966:
1963:
1961:
1944:
1941:
1939:
1938:
1933:
1928:
1926:
1923:
1916:
1914:
1912:
1908:
1904:
1900:
1896:
1891:
1885:
1881:
1877:
1872:
1862:
1858:
1853:
1843:
1839:
1831:
1827:
1824:
1819:
1812:
1810:
1786:300 km/s
1729:
1725:
1721:
1713:
1709:
1684:
1682:
1680:
1676:
1675:quasi-periods
1671:
1667:
1666:
1660:
1658:
1653:
1649:
1648:photoelectric
1641:
1637:
1632:
1625:
1623:
1621:
1617:
1611:
1609:
1605:
1597:
1592:
1586:
1583:In 1933, the
1581:
1574:
1567:
1563:
1558:
1556:
1552:
1548:
1547:Balmer series
1544:
1540:
1536:
1535:spectral type
1528:
1526:
1524:
1520:
1516:
1512:
1508:
1504:
1500:
1496:
1492:
1488:
1480:
1476:
1474:
1470:
1466:
1463:star with an
1462:
1453:
1446:
1444:
1438:
1430:
1422:
1418:
1413:
1411:
1407:
1403:
1398:
1394:
1390:
1386:
1381:
1379:
1375:
1367:
1360:
1353:
1346:
1338:
1334:
1331:In 2016, the
1326:
1322:
1318:
1311:
1309:
1307:
1303:
1299:
1294:
1287:
1285:
1281:
1277:
1273:
1269:
1265:
1260:
1258:
1254:
1250:
1247:
1238:
1234:
1231:. Due to its
1229:
1223:
1219:
1215:
1211:
1207:
1206:spectral type
1202:
1200:
1196:
1192:
1188:
1184:
1180:
1176:
1172:
1168:
1164:
1160:
1156:
1153:
1150:. It has the
1149:
1145:
1144:constellation
1141:
1137:
1129:
1126:
1124:
1123:
1120:
1117:
1115:
1114:
1110:
1109:
1104:
1097:
1093:
1089:
1082:
1078:
1071:
1064:
1057:
1050:
1046:
1042:
1038:
1030:
1027:J05145-0812,
1023:
1016:
1005:
998:
991:
987:
982:
979:
975:
971:
968:
959:
957:
956:
952:
951:
946:
942:
939:
930:
928:
927:
923:
922:
917:
914:
905:
903:
902:
898:
897:
892:
888:
884:
881:
870:
868:
867:
863:
862:
851:
849:
847:
843:
839:
835:
834:
831:
820:
818:
817:
813:
812:
809:
798:
796:
795:
791:
790:
787:
776:
774:
772:
768:
764:
763:
760:
741:
739:
736:
735:
732:
713:
711:
710:
706:
705:
702:
686:
684:
683:
679:
678:
673:
668:
665:
661:
659:
657:
653:
652:
648:
646:
643:
642:
638:
636:
633:
632:
629:
625:
621:
612:
609:
608:
604:
595:
594:
590:
589:
585:
583:
581:
577:
576:
572:
570:
568:
564:
563:
559:
557:
554:
553:
549:
547:
544:
543:
540:
536:
533:
529:
527:
525:
521:
520:
516:
514:
511:
510:
506:
504:
501:
500:
497:
493:
489:
485:
483:
477:
473:
472:
468:
455:
444:
442:
441:
437:
436:
433:
429:
427:
425:
421:
420:
417:
413:
405:
401:
394:
392:
390:
389:Proper motion
386:
385:
374:
372:
366:
362:
361:
357:
354:
350:
346:
344:
341:
340:
337:
336:Main sequence
334:
332:
329:
328:
323:
320:
317:
315:
312:
311:
307:
305:
301:
300:
296:
294:
290:
289:
285:
283:
280:
279:
276:
273:
271:
268:
267:
262:
257:
250:
246:
242:
241:
237:
234:
233:
228:
227:
221:
218:
217:
212:
211:
208:
204:
197:
193:
189:
188:
184:
181:
180:
175:
174:
168:
165:
164:
159:
158:
155:
151:
146:
129:
106:
104:
103:Pronunciation
101:
100:
97:
94:
92:
91:
90:Constellation
87:
86:
82:
78:
72:
60:
53:
43:
37:
33:
19:
8110:
8010:TXS 0506+056
8005:II Zwicky 28
7925:Orion Nebula
7865:Flame Nebula
7105:
6960:
6933:
6897:Orion's Belt
6798:. Retrieved
6794:the original
6785:
6776:
6764:. Retrieved
6751:
6742:
6722:
6715:
6703:. Retrieved
6693:
6681:. Retrieved
6671:
6662:
6656:
6644:. Retrieved
6635:
6626:
6603:
6600:Nojiri, Hōei
6594:
6571:
6566:
6558:
6546:. Retrieved
6542:
6532:
6520:. Retrieved
6506:
6499:
6479:. New York:
6475:
6468:
6456:. Retrieved
6436:. New York:
6432:
6425:
6406:
6400:
6357:
6351:
6345:
6322:
6316:
6292:
6285:
6258:
6252:
6242:
6228:
6221:
6191:(2): 89–98.
6188:
6182:
6176:
6163:
6157:
6133:
6101:
6091:
6050:
6046:
6036:
6001:
5995:
5942:
5936:
5930:
5885:
5881:
5842:
5835:
5787:
5781:
5775:
5764:
5721:
5717:
5711:
5694:
5690:
5629:
5623:
5617:
5606:
5563:
5559:
5532:. Retrieved
5504:. New York:
5500:
5493:
5481:. Retrieved
5467:
5460:
5450:
5443:
5416:
5410:
5400:
5355:
5351:
5341:
5328:
5279:(1): 46–63.
5276:
5270:
5207:
5203:
5197:
5189:
5179:
5173:
5130:
5126:
5074:
5070:
5063:
5036:
5032:
5022:
5005:
4999:
4993:
4976:
4972:
4965:
4953:. Retrieved
4939:
4909:(1): 80–88.
4906:
4900:
4894:
4877:
4873:
4867:
4850:
4844:
4838:
4811:
4805:
4795:
4770:
4766:
4740:
4704:
4700:
4690:
4663:
4619:
4613:
4599:
4592:
4567:
4563:
4557:
4526:
4520:
4509:
4502:
4473:
4465:
4441:
4435:
4423:. Retrieved
4419:the original
4410:
4401:
4381:
4326:
4322:
4298:. Retrieved
4280:
4260:
4253:
4234:
4228:
4220:
4188:
4157:
4153:
4147:
4124:
4103:. Retrieved
4094:
4053:
4025:. Retrieved
4011:
3999:. Retrieved
3989:
3980:
3972:
3965:. Retrieved
3930:: 112–162 .
3927:
3921:
3865:
3861:
3805:
3799:
3795:
3731:
3727:
3667:
3661:
3609:
3605:
3595:
3552:
3546:
3540:
3505:
3501:
3430:(1): 74–84.
3427:
3423:
3393:
3387:
3335:
3331:
3300:. Retrieved
3273:
3269:
3215:
3209:
3175:
3169:
3133:
3127:
3093:
3087:
3081:
3038:
3032:
2996:
2993:Upton, Clive
2987:
2964:
2958:
2939:
2929:
2888:
2870:
2865:World War II
2859:
2855:
2846:Orion's Belt
2827:
2821:
2812:
2794:
2782:
2776:
2773:Māori people
2770:
2765:
2757:
2745:
2733:
2722:
2720:
2715:
2707:
2703:
2692:Beta Eridani
2685:
2676:
2672:
2664:
2656:
2652:
2648:
2644:
2640:
2632:
2623:
2615:
2609:
2605:
2603:
2600:is derived.
2597:
2593:
2587:
2557:
2545:
2534:
2521:
2425:11,486
2383:
2348:
2341:. A mass of
2336:12,100
2328:
2309:30,000
2290:
2270:
2252:
2232:
2192:
2166:
2131:
2120:
2113:
2100:
2049:
2019:9.860 d
1979:
1931:
1911:runaway star
1903:Orion Nebula
1892:
1873:
1863:parallax of
1835:
1688:
1663:
1661:
1645:
1639:
1612:
1582:
1559:
1532:
1529:Spectroscopy
1477:
1459:Rigel is an
1458:
1414:
1389:Johann Bayer
1382:
1380:05145–0812.
1330:
1312:Nomenclature
1288:
1261:
1253:neutron star
1251:, leaving a
1233:stellar wind
1226:12,100
1203:
1170:
1166:
1163:Beta Orionis
1162:
1154:
1142:star in the
1135:
1134:
1111:
1091:
1040:
1034:J05145-0812
953:
924:
899:
864:
845:
841:
836:
814:
792:
770:
765:
737:
707:
680:
654:
644:
634:
610:
591:
580:Eccentricity
578:
565:
555:
545:
522:
512:
502:
474:
438:
422:
387:
363:
230:
223:05 14 32.049
214:
206:
177:
161:
153:
88:
36:
8105:Outer space
7681:HD 290327 b
7565:4U 0614+091
6954:ζ (Alnitak)
6949:ε (Alnilam)
6944:δ (Mintaka)
6632:"MS. Rigel"
6522:16 November
5724:(2): 3358.
4880:: 215–221.
4511:Planisphere
4482:. pp.
4300:11 February
4229:Uranometria
4001:13 February
3670:(2): 1114.
3612:(1): 1–12.
2903:Mount Rigel
2828:Genji-boshi
2698:'s toe" in
2502:360 pc
2498:264 pc
2494:264 pc
2291:Rigel is a
2222:555 in his
2206:. In 2009,
2143:33, or as H
2123:star system
2077:Period = 63
1840:of Rigel's
1670:Alpha Cygni
1657:color index
1636:light curve
1626:Variability
1620:photosphere
1600:1.5 nm
1505:, Capella,
1479:Culminating
1447:Observation
1293:arc seconds
1210:as luminous
1195:light-years
1183:star system
1157:, which is
1094:: Rigel B,
816:Metallicity
794:Temperature
619:(secondary)
319:Alpha Cygni
304:color index
293:color index
232:Declination
200:(0.05–0.18)
179:Declination
8118:Categories
8036:GRB 991216
8000:CGCG 396-2
7920:Messier 78
7915:Messier 43
7855:Barnard 30
7676:HD 38529 b
7671:HD 37605 b
7666:HD 34445 b
7658:Exoplanets
7600:Gliese 221
7595:Gliese 208
7590:Gliese 205
7585:Gliese 179
7575:GRB 991216
7029:λ (Meissa)
7019:ι (Hatysa)
6961:(Algjebba)
6800:2 February
6766:2 February
6458:3 November
6325:. London:
5888:: L6–L10.
5797:1804.09365
5639:1804.09365
5534:1 February
5365:1805.04649
5217:2208.00211
4445:. London:
4329:(1): 211.
4235:Star Tales
4105:1 February
3967:23 January
3741:1712.08109
3619:2204.00372
3562:1606.08053
2951:References
2895:Antarctica
2842:Genpei War
2838:Heike clan
2824:Genji clan
2758:Unumburrgu
2734:Totyerguil
2727:Wotjobaluk
2704:Trois Rois
2629:رجل الجبار
2608:is in the
2202:to around
1876:nebulosity
1850:0.34
1821:Rigel and
1393:Betelgeuse
1306:arc minute
1284:Betelgeuse
1257:black hole
1235:, Rigel's
1220:, and its
1214:as massive
1204:A star of
1197:(260
1079:−08°1063,
1045:19 Orionis
960:3.84
931:2.94
906:3.84
859: km/s
769:(log
573:9.860 days
382: km/s
353:Astrometry
347:B9V + B9V
8081:Astronomy
7995:4C +09.17
7990:4C +03.10
7152:Flamsteed
7069:π (Tabit)
7024:κ (Saiph)
6934:β (Rigel)
6646:5 January
6606:. Tokyo:
6392:118454721
6367:1010.4610
6213:118597258
6131:(1963) .
6075:0004-6280
5952:0710.4003
5922:118557550
5895:1311.4744
5756:119268845
5731:0811.0492
5697:: 59–60.
5598:119387088
5392:119509277
5358:(3): 22.
5311:119262311
5286:1007.0241
5244:244398875
5165:118404460
5140:1405.0907
5084:1007.2095
4947:. AAVSO.
4931:125853869
4673:0812.0046
4636:cite book
4543:cite book
4336:0806.0929
4227:"Bayer's
3986:"bet Ori"
3954:186209247
3875:1005.2278
3815:1201.0843
3768:119427037
3734:(1): 16.
3704:118557626
3677:1311.5116
3587:119231169
3508:: 75–84.
3462:119072203
3437:1202.1836
3370:118953817
3178:: 27–34.
3048:0708.1752
2766:Ya-jungin
2696:Aurvandil
2564:supernova
2531:Evolution
2517:Aldebaran
2193:In 1871,
2017:Period =
1685:Mass loss
1665:Hipparcos
1608:mass loss
1589:0.1
1503:Aldebaran
1473:B-V color
1439:number HD
1385:Latinized
1291:9.5
1280:night sky
1249:supernova
1237:mass-loss
1191:naked eye
1159:Latinized
1155:β Orionis
986:β Orionis
645:Companion
622:32.6 km/s
605:25.0 km/s
602:(primary)
556:Companion
513:Companion
253:(7.5/7.6)
247: (V)
194: (V)
8056:Category
7939:Galaxies
7905:LDN 1641
7875:HH 24-26
7850:Abell 13
7845:Abell 12
7697:clusters
7630:S Ori 70
7625:S Ori 52
7615:LP 658-2
7610:HOPS 383
7355:Variable
7106:(Thabit)
6760:Archived
6640:Archived
6602:(2002).
6576:Sanseidō
6572:Daijirin
6516:Archived
6481:Springer
6452:Archived
6083:40668597
5987:14254892
5528:Archived
5506:Springer
5477:Archived
5133:: A125.
5109:10340205
4955:26 April
4949:Archived
4361:18067739
4294:Archived
4099:Archived
4066:Archived
4021:Archived
3958:Archived
3900:55532189
3532:30387824
3396:: 1–49.
3302:13 March
3296:Archived
3073:18759600
2909:See also
2899:astrofix
2801:Pleiades
2796:Matariki
2762:Eridanus
2754:Kangaroo
2677:Algibbar
2513:☉
2490:☉
2474:☉
2430:☉
2413:☉
2406:☉
2399:☉
2391:☉
2379:☉
2352:☉
1842:parallax
1830:Eridanus
1813:Distance
1806:☉
1793:☉
1780:☉
1775:10
1765:☉
1760:10
1746:☉
1741:10
1707:☉
1571:10
1533:Rigel's
1499:asterism
1431:entry HR
1364:555, or
1167:Beta Ori
1075:131907,
966:☉
937:☉
912:☉
758:☉
730:☉
700:☉
478: (M
440:Distance
424:Parallax
83:J2000.0
8067:Portals
7900:IC 2118
7779:Nebulae
7620:PDS 110
7605:GJ 3379
7580:G 99-47
7570:CVSO 30
6705:14 June
6683:14 June
6548:16 June
6372:Bibcode
6193:Bibcode
6055:Bibcode
6006:Bibcode
5957:Bibcode
5900:Bibcode
5802:Bibcode
5736:Bibcode
5699:Bibcode
5644:Bibcode
5578:Bibcode
5510:Bibcode
5483:7 March
5421:Bibcode
5419:: 233.
5370:Bibcode
5291:Bibcode
5222:Bibcode
5145:Bibcode
5089:Bibcode
5041:Bibcode
5010:Bibcode
4981:Bibcode
4979:: 263.
4911:Bibcode
4905:. 5.1.
4882:Bibcode
4855:Bibcode
4816:Bibcode
4775:Bibcode
4745:Bibcode
4709:Bibcode
4678:Bibcode
4666:: 459.
4624:Bibcode
4572:Bibcode
4570:: 362.
4531:Bibcode
4425:28 June
4341:Bibcode
4198:Bibcode
4162:Bibcode
4091:"Rigel"
4027:28 July
3932:Bibcode
3880:Bibcode
3868:: A38.
3820:Bibcode
3746:Bibcode
3682:Bibcode
3624:Bibcode
3567:Bibcode
3510:Bibcode
3442:Bibcode
3398:Bibcode
3350:Bibcode
3278:Bibcode
3220:Bibcode
3218:: 421.
3180:Bibcode
3138:Bibcode
3136:: 359.
3098:Bibcode
3053:Bibcode
2969:Sky Pub
2884:US Navy
2807:of the
2787:Antares
2756:Leader
2742:Boorong
2725:to the
2645:Elgebar
2641:Algebar
2347:3
1880:IC 2118
1826:IC 2118
1801:3
1511:Procyon
1278:in the
1175:massive
1128:Rigel B
1068:24436,
1054:34085,
748:−21,000
746:+25,000
743:120,000
670:Details
635:Primary
546:Primary
530:24,000
503:Primary
81:Equinox
7895:IC 434
7885:HH 111
7870:HH 1/2
7549:290327
7345:75 (l)
7340:74 (k)
7330:72 (f)
7320:69 (f)
7265:51 (b)
7260:49 (d)
7250:42 (c)
7230:32 (A)
7220:29 (e)
7215:27 (p)
7210:23 (m)
7205:22 (o)
7190:16 (h)
7180:14 (i)
6730:
6614:
6582:
6487:
6444:
6413:
6390:
6333:
6304:
6277:663691
6275:
6211:
6145:
6108:
6081:
6073:
6024:
5985:
5975:
5920:
5854:
5828:VizieR
5790:. A1.
5754:
5670:VizieR
5632:. A1.
5596:
5520:
5390:
5309:
5254:VizieR
5242:
5210:: A1.
5163:
5107:
5077:: A5.
4929:
4773:: 67.
4707:: 26.
4490:
4453:
4389:
4359:
4268:
4241:
4208:
4135:
3991:SIMBAD
3952:
3898:
3840:425831
3838:
3766:
3702:
3585:
3530:
3460:
3368:
3071:
3003:
2975:
2934:globe.
2878:was a
2874:. The
2778:Puanga
2748:. The
2738:Altair
2716:tunsel
2671:, and
2665:Riglon
2647:. The
2468:
2421:61,515
2374:
2364:
2255:
2247:
2228:
2220:
2216:
2212:0.124″
2188:
2184:
2173:
2149:
2145:
2141:
2137:
2079:
1956:
1888:
1865:3.2352
1718:
1642:(2012)
1640:et al.
1598:about
1515:Sirius
1513:, and
1507:Pollux
1497:", an
1483:
1441:
1433:
1425:
1369:
1362:
1355:
1348:
1343:
1244:
1179:eponym
1113:SIMBAD
1099:
1084:
1073:
1066:
1061:1713,
1059:
1052:
1032:
1025:
1018:
1013:
1007:
1000:
995:3823,
993:
878:
828:
806:
800:12,100
784:
752:
724:
709:Radius
694:
656:Period
567:Period
524:Period
465:
452:
308:−0.03
297:−0.66
286:B8 Ia
40:Rigel
8093:Stars
7983:Other
7880:HH 34
7838:Other
7753:Other
7558:Other
7544:42618
7539:37605
7534:37320
7529:34445
7524:33636
7443:V2384
7438:V2254
7433:V1352
7428:V1201
7423:V1005
7165:6 (g)
6921:Bayer
6912:Stars
6836:AAVSO
6570:[
6388:S2CID
6362:arXiv
6273:JSTOR
6209:S2CID
6079:JSTOR
5983:S2CID
5947:arXiv
5918:S2CID
5890:arXiv
5822:
5792:arXiv
5752:S2CID
5726:arXiv
5664:
5634:arXiv
5594:S2CID
5568:arXiv
5394:. 84.
5388:S2CID
5360:arXiv
5307:S2CID
5281:arXiv
5248:
5240:S2CID
5212:arXiv
5161:S2CID
5135:arXiv
5105:S2CID
5079:arXiv
5008:: 1.
4927:S2CID
4853:: 1.
4668:arXiv
4486:–59.
4357:S2CID
4331:arXiv
4194:Wiley
4160:: 1.
4095:Stars
4069:(PDF)
4058:(PDF)
3961:(PDF)
3950:S2CID
3896:S2CID
3870:arXiv
3836:S2CID
3810:arXiv
3764:S2CID
3736:arXiv
3700:S2CID
3672:arXiv
3614:arXiv
3583:S2CID
3557:arXiv
3528:S2CID
3458:S2CID
3432:arXiv
3366:S2CID
3340:arXiv
3069:S2CID
3043:arXiv
2921:Notes
2871:Rigel
2860:Rigel
2815:is a
2813:Puaka
2799:(the
2783:Rehua
2730:koori
2688:Orion
2657:Regel
2606:Rigel
2598:Rigel
2451:2.606
2324:Deneb
2226:or BU
1932:Rigel
1907:Saiph
1357:668,
1321:Orion
1255:or a
1187:stars
1171:β Ori
1148:Orion
1138:is a
1136:Rigel
1119:Rigel
1009:555,
1002:668,
822:−0.06
628:Orbit
539:Orbit
496:Orbit
486:−7.84
408:Dec.:
251:6.67
198:0.13
96:Orion
77:Epoch
7974:2119
7969:2110
7964:1924
7959:1819
7954:1683
7829:2174
7824:2071
7819:2067
7814:2064
7809:2023
7804:2022
7799:1999
7794:1788
7744:2202
7739:2194
7734:2175
7729:2169
7724:1981
7719:1980
7714:1662
7695:Star
7506:2275
7501:2251
7496:2024
7491:2007
7486:1988
7481:1952
7476:1887
7471:1874
7466:1763
7461:1759
7418:V883
7413:V380
6802:2019
6768:2019
6728:ISBN
6707:2020
6685:2020
6648:2019
6612:ISBN
6580:ISBN
6550:2020
6524:2012
6485:ISBN
6460:2016
6442:ISBN
6411:ISBN
6331:ISBN
6302:ISBN
6143:ISBN
6106:ISBN
6071:ISSN
6022:ISBN
5973:ISBN
5852:ISBN
5776:Gaia
5618:Gaia
5536:2019
5518:ISBN
5485:2019
5198:Gaia
5006:4659
4957:2019
4851:2762
4642:link
4549:link
4488:ISBN
4451:ISBN
4427:2014
4387:ISBN
4302:2019
4266:ISBN
4239:ISBN
4206:ISBN
4133:ISBN
4107:2019
4029:2016
4003:2019
3969:2020
3796:MOST
3304:2016
3094:2237
3001:ISBN
2973:ISBN
2889:The
2869:USS
2856:The
2771:The
2708:Bįhi
2624:rijl
2479:2.75
2464:−7.3
2462:+6.1
2459:74.1
2259:44.5
2204:0.3″
2200:0.1″
2121:The
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