Rigel

**Rigel** (/ˈraɪdʒəl, -ɡəl/), also designated **Beta Orionis** (**β Orionis**, abbreviated **Beta Ori**, **β Ori**), is generally the seventh-brightest star in the night sky and the brightest star in the constellation of Orion—though periodically it is outshone within the constellation by the variable Betelgeuse. With a visual magnitude of 0.13, it is a luminous star some 863 light-years distant from Earth.

The star as seen from Earth is actually a multiple star system of three to five stars, the primary star (Rigel A) being a blue-white supergiant which is estimated to be anywhere from 120,000 to 279,000 times as luminous as the Sun, depending on the method used to calculate its properties. It has exhausted its core of hydrogen and swollen to between 79 and 115 times the Sun's radius. It pulsates quasi-periodically and is classified as an Alpha Cygni variable. A companion, Rigel B, is 500 times fainter than the supergiant Rigel A and visible only with a telescope. Rigel B is itself a spectroscopic binary system, consisting of two main sequence blue-white stars of spectral type B9V that are estimated to be respectively 3.9 and 2.9 times as massive as the Sun; Rigel Bb may itself be a binary. Rigel B also appears to have a very close visual companion Rigel C of almost identical appearance.

## Nomenclature

*Beta Orionis* is the star's Bayer designation. The traditional name *Rigel* is first recorded in the Alfonsine Tables of 1252. It is derived from the Arabic name **Rijl Jauzah al Yusrā**, "the left leg (foot) of Jauzah" (i.e. *rijl* meaning "leg, foot"), which can be traced to the 10th century. "Jauzah" was a proper name of the Orion figure, an alternative Arabic name was رجل الجبار **riǧl al-ǧabbār**, "the foot of the great one", which is the source of the rarely used variant names **Algebar** or *Elgebar*. The *Alphonsine Tables* saw its name split into "Rigel" and "Algebar", with the note, "et dicitur Algebar. Nominatur etiam Rigel."
Alternate spellings from the 17th century include *Regel* by Italian astronomer Giovanni Battista Riccioli, *Riglon* by German astronomer Wilhelm Schickard, and *Rigel Algeuze* or *Algibbar* by English scholar Edmund Chilmead.

In 2016, the International Astronomical Union organized a Working Group on Star Names (WGSN) to catalog and standardize 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 *Rigel* for this star. It is now so entered in the IAU Catalog of Star Names.

## Visibility

The apparent visual magnitude of Rigel is 0.13, making it on average the seventh-brightest star in the celestial sphere excluding the Sun—just fainter than Capella. It is an irregular pulsating variable with a visual range of magnitude 0.05–0.18. Although Rigel has the Bayer designation "beta", it is almost always brighter than Alpha Orionis (Betelgeuse). Since 1943, the spectrum of this star has served as one of the stable anchor points by which other stars are classified. Rigel is the third most inherently luminous first magnitude star after Deneb and Betelgeuse. Rigel has a color index (B–V) of −0.03, meaning it appears white or slightly blue-white.

Culminating at midnight on 12 December, and at 9 pm on 24 January, Rigel is most visible in winter evenings in the northern hemisphere and summer in the southern. In the southern hemisphere, Rigel is the first bright star of Orion visible as the constellation rises.
In stellar navigation, Rigel is one of the most important navigation stars, since it is bright, easily located and equatorial, which means it is visible all around the world's oceans (the exception, areas within 8° of the North Pole).

### Parallax

The revised 2007 Hipparcos reduction of Rigel's parallax gives a distance of 863 light-years (265 parsecs), with a margin of error of about 9%. Earlier spectroscopic estimates placed its distance between 360 and 500 parsecs (1,200 and 1,600 light-years).

## System

Rigel has been known as a visual double star since at least 1822, when it was measured by Friedrich Georg Wilhelm von Struve. The companion is not particularly faint at magnitude 6.7, and with a separation of 9.5 arcsec both components are resolvable in most amateur astronomers' telescopes. However, the large difference in brightness makes it a challenging target for telescope apertures smaller than 15.0 cm (5.9 in). At Rigel's estimated distance, Rigel B's projected separation from its primary is over 2200 AU. Since its discovery, there has been no sign of orbital movement, although both stars share similar common proper motion. The pair would have a minimum orbital period of around 18,000 years.

Since the 19th century, Rigel B has been reported to be resolved into a close binary of two equal components, with the measured separation varying from less than 0.1" to nearly 0.2". Speckle interferometry showed in 2009 two almost identical components separated by 0.124". Both stars have apparent visual magnitudes of 7.6 with a likely orbital period of 63 years.

Rigel Bb may itself be a spectroscopic binary system, consisting of two main sequence stars that orbit each other every 9.86 days. The stars both belong to the spectral class B9. These two stars do not appear to make up the visual binary components of B or C, so the B sub-system might be a triple star, although the true arrangement of them is unclear.

A 15.4 magnitude star at 44.6 arcsec in north position angle of 1° is catalogued as component D in the system although it is unclear whether it is physically related or a coincidental alignment.

## Properties

 File:Hertzsprung-Russel StarData.png
Moravveji and colleagues calculate a luminosity for Rigel A of 120,000 times that of the Sun. Its surface temperature is around 12,100 K. The interferometer-measured angular diameter of this star, after correction for limb darkening, is 7000275000000000000♠2.75±0.01 mas. At its estimated distance, this yields a size of about 78.9 times the radius of the Sun. Norbert Przybilla and colleagues used atmospheric modelling in 2006 to come up with a distance of 360 ± 40 parsecs (1,170 ± 130 light-years). They calculated it to be around 218,000 times as luminous as the Sun, and have around 21±3 solar masses and 109±12 times its radius. The CMFGEN code is an atmosphere code used to determine the properties of massive stars from analysing their spectrum and atmosphere. Analysis of Rigel using this method yields a luminosity 279,000 times that of the Sun, a radius 115 times that of the Sun and stellar wind velocity of 671,080 miles per hour.

Rigel A is a blue supergiant that has exhausted burning the hydrogen fuel in its core and left the main sequence, expanding and brightening as it progresses across the Hertzsprung–Russell diagram. Przybilla estimated that it has lost around 3 solar masses since beginning life as a star of 24 ± 3 solar masses 7 to 9 million years ago. It will become a red supergiant and eventually end its stellar life by exploding as a type II supernova, in the process flinging out material that will serve to seed future generations of stars. It is one of the closest known potential supernova progenitors to Earth.

Rigel's variability is complex and is caused by stellar pulsations similar to those of Deneb, the prototype of the class of Alpha Cygni pulsating stars. The radial velocity variations of Rigel prove that it simultaneously oscillates in at least 19 non-radial modes with periods ranging from about 1.2 to 74 days. It is notable among blue supergiant stars in the sense that while its pulsations are powered by the nuclear reactions in a hydrogen-burning shell that is at least partially non-convective, the star also burns helium in its core. Rigel was identified as belonging to the Alpha Cygni variables in 1998 by Christoffel Waelkens and colleagues.

As it is both bright and moving through a region of nebulosity, Rigel lights up several dust clouds in its vicinity, most notably IC 2118 (the Witch Head Nebula). Rigel is also associated with the Orion Nebula, which–while more or less along the same line of sight as the star–is almost twice as far away from Earth. Despite the difference in distance, projecting Rigel's path through space for its expected age brings it close to the nebula. As a result, Rigel is sometimes classified as an outlying member of the Orion OB1 Association although it is considerably closer than most of the members. Betelgeuse and Saiph lie at a similar distance to Rigel, although Betelgeuse is a runaway star with a complex history and is likely to have originally formed in the main body of the association. It has been listed as a member of the poorly-defined Taurus-Orion R1 Association

The companions Rigel Ba, Bb, and C all appear to be similar B class main sequence stars of 3 - 4 M☉, but their properties are not accurately known.

### Space photometry

 File:Treasures3.jpg
Rigel was observed with the Canadian MOST satellite for nearly 28 days in 2009. The light variations in this supergiant star were at the milli magnitude level. The gradual changes in the flux highlights the presence of long-period pulsation modes in the star.

### Spectroscopy

The general spectral type of Rigel as B8 is well-established and it has been used as a defining point of the spectral classification sequence for supergiants. However the details of the spectrum vary considerably owing to periodic atmospheric eruptions. The spectral lines show emission, absorption, line doubling, P Cygni profiles, and inverse P Cygni profiles, with no obvious periodicity. This has resulted in classification as B8 Iab, B8 Iae, or blendings by different authors.

## Etymology and cultural significance

Rigel is presumably the star known as "Aurvandil's toe" in Norse mythology.

In Chinese, 參宿 (*Shēn Sù*), meaning *Three Stars (asterism)*, refers to an asterism consisting of Rigel, Alnitak, Alnilam, Mintaka, Betelgeuse, Bellatrix and Saiph. Consequently, Rigel are known as 參宿七 (*Shēn Sù qī*, English: the Seventh Star of Three Stars).

In Japan, the Minamoto or Genji clan chose Rigel and its white color as its symbol, calling the star *Genji-boshi* (源氏星), while the Taira or Heike clan adopted Betelgeuse and its red color. The two powerful families fought a legendary war in Japanese history, the stars seen as facing each other off and only kept apart by the Belt. Rigel was also known as *Gin-waki*, (銀脇), "the Silver (Star) beside (*Mitsu-boshi*)".

Rigel was known as *Yerrerdet-kurrk* to the Wotjobaluk koori of southeastern Australia, and held to be the mother-in-law of *Totyerguil* (Altair). The distance between them signified the taboo preventing a man from approaching his mother-in-law.
The indigenous Boorong people of northwestern Victoria named Rigel as *Collowgullouric Warepil*.
The Wardaman people of northern Australia know Rigel as the Red Kangaroo Leader *Unumburrgu* and chief conductor of ceremonies in a songline when Orion is high in the sky. The river Eridanus 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 *Ya-jungin* "Owl Eyes Flicking", watching the ceremonies.

The Māori people named Rigel as *Puanga*, which was said to be a daughter of *Rehua* (Antares), the chief of all stars. Its heliacal rising also presaged the appearance of *Matariki* (the Pleiades) in the dawn sky which marked the Māori New Year in late May or early June. The Moriori people of the Chatham Islands, as well as some Maori groups in New Zealand, marked the start of their New Year with Rigel rather than the Pleiades. *Puaka* was a local variant used in the South Island.

The Lacandon people of southern Mexico knew it as *tunsel* ("little woodpecker").

## See also

* File:Crab Nebula.jpgAstronomy portal
* File:He1523a.jpgStar portal

* Rigel in fiction

## References

1. ↑ 1.0 1.1 1.2 1.3 1.4 1.5 **Lua error in Module:Citation/CS1/Identifiers at line 47: attempt to index field 'wikibase' (a nil value).**
2. ↑ **Lua error in Module:Citation/CS1/Identifiers at line 47: attempt to index field 'wikibase' (a nil value).**
3. ↑ **Lua error in Module:Citation/CS1/Identifiers at line 47: attempt to index field 'wikibase' (a nil value).**
4. ↑ 4.0 4.1 **Lua error in Module:Citation/CS1/Identifiers at line 47: attempt to index field 'wikibase' (a nil value).**
5. ↑ 5.0 5.1 **Lua error in Module:Citation/CS1/Identifiers at line 47: attempt to index field 'wikibase' (a nil value).**
6. ↑ 6.0 6.1 6.2 6.3 6.4 **Lua error in Module:Citation/CS1/Identifiers at line 47: attempt to index field 'wikibase' (a nil value).**
7. ↑ 7.0 7.1 7.2 7.3 **Lua error in Module:Citation/CS1/Identifiers at line 47: attempt to index field 'wikibase' (a nil value).**
8. ↑ 8.0 8.1 8.2 8.3 **Lua error in Module:Citation/CS1/Identifiers at line 47: attempt to index field 'wikibase' (a nil value).**
9. ↑ 9.0 9.1 9.2 9.3 9.4 9.5 **Lua error in Module:Citation/CS1/Identifiers at line 47: attempt to index field 'wikibase' (a nil value).**
10. ↑ **Lua error in Module:Citation/CS1/Identifiers at line 47: attempt to index field 'wikibase' (a nil value).**
11. ↑ 11.0 11.1 **Lua error in Module:Citation/CS1/Identifiers at line 47: attempt to index field 'wikibase' (a nil value).**
12. ↑ 12.0 12.1 12.2 12.3 **Lua error in Module:Citation/CS1/Identifiers at line 47: attempt to index field 'wikibase' (a nil value).**
13. ↑ 13.0 13.1 13.2 13.3 13.4 13.5 13.6 **Lua error in Module:Citation/CS1/Identifiers at line 47: attempt to index field 'wikibase' (a nil value).**
14. ↑ 14.0 14.1 **Lua error in Module:Citation/CS1/Identifiers at line 47: attempt to index field 'wikibase' (a nil value).**
15. ↑ "SIMBAD Astronomical Database". *Results for Rigel*. Retrieved 2008-04-10.<templatestyles src="Module:Citation/CS1/styles.css"></templatestyles>
16. ↑ 16.0 16.1 Allen, Richard Hinckley (1963) [1899]. *Star Names: Their Lore and Meaning* (Reprint ed.). New York, NY: Dover Publications Inc. pp. 312–13. ISBN 0-486-21079-0.<templatestyles src="Module:Citation/CS1/styles.css"></templatestyles>
17. ↑ Kunitzsch, Paul (1959). *Arabische Sternnamen in Europa*. Wiesbaden: Otto Harrassowitz. p. 46.<templatestyles src="Module:Citation/CS1/styles.css"></templatestyles>
18. ↑ **Lua error in Module:Citation/CS1/Identifiers at line 47: attempt to index field 'wikibase' (a nil value).**
19. ↑ "IAU Working Group on Star Names (WGSN)". Retrieved 22 May 2016.<templatestyles src="Module:Citation/CS1/styles.css"></templatestyles>
20. ↑ "Bulletin of the IAU Working Group on Star Names, No. 1" (PDF). Retrieved 28 July 2016.<templatestyles src="Module:Citation/CS1/styles.css"></templatestyles>
21. ↑ "IAU Catalog of Star Names". Retrieved 28 July 2016.<templatestyles src="Module:Citation/CS1/styles.css"></templatestyles>
22. ↑ **Lua error in Module:Citation/CS1/Identifiers at line 47: attempt to index field 'wikibase' (a nil value).**
23. ↑ "The Colour of Stars", *Australia Telescope, Outreach and Education*, Commonwealth Scientific and Industrial Research Organisation, 21 December 2004, retrieved 28 June 2014<templatestyles src="Module:Citation/CS1/styles.css"></templatestyles>
24. ↑ Schaaf, Fred (2008). "Appendix C". *The Brightest Stars*. Hoboken, New Jersey: Wiley. p. 257. ISBN 0-471-70410-5.<templatestyles src="Module:Citation/CS1/styles.css"></templatestyles>
25. ↑ Ellyard, David; Tirion, Wil (2008) [1993]. *The Southern Sky Guide* (3rd ed.). Port Melbourne, Victoria: Cambridge University Press. pp. 58–59. ISBN 978-0-521-71405-1.<templatestyles src="Module:Citation/CS1/styles.css"></templatestyles>
26. ↑ **Lua error in Module:Citation/CS1/Identifiers at line 47: attempt to index field 'wikibase' (a nil value).**
27. ↑ **Lua error in Module:Citation/CS1/Identifiers at line 47: attempt to index field 'wikibase' (a nil value).**<
28. ↑ 28.0 28.1 28.2 28.3 "Washington Double Star Catalogue". *US Naval Observatory*. Retrieved 13 March 2016.<templatestyles src="Module:Citation/CS1/styles.css"></templatestyles>
29. ↑ Burnham, Robert, Jr. (1978). *Burnham's Celestial Handbook*. New York: Dover Publications. p. 1300.<templatestyles src="Module:Citation/CS1/styles.css"></templatestyles>
30. ↑ 30.0 30.1 Jedicke, Peter; Levy, David H. (1992). "Regal Rigel". *The New Cosmos*. Waukesha: Kalmbach Books. pp. 48–53.<templatestyles src="Module:Citation/CS1/styles.css"></templatestyles>
31. ↑ **Lua error in Module:Citation/CS1/Identifiers at line 47: attempt to index field 'wikibase' (a nil value).**
32. ↑ "Spectroscopic Binary Catalogue (SB9)". *D.Pourbaix*. Retrieved 13 March 2016.<templatestyles src="Module:Citation/CS1/styles.css"></templatestyles>
33. ↑ **Lua error in Module:Citation/CS1/Identifiers at line 47: attempt to index field 'wikibase' (a nil value).**
34. ↑ **Lua error in Module:Citation/CS1/Identifiers at line 47: attempt to index field 'wikibase' (a nil value).**
35. ↑ 35.0 35.1 **Lua error in Module:Citation/CS1/Identifiers at line 47: attempt to index field 'wikibase' (a nil value).**
36. ↑ **Lua error in Module:Citation/CS1/Identifiers at line 47: attempt to index field 'wikibase' (a nil value).**
37. ↑ Rother, Sara (2009). "A time series study of Rigel, a B8Ia supergiant".<templatestyles src="Module:Citation/CS1/styles.css"></templatestyles>
38. ↑ Richard Cleasby, *An Icelandic-English Dictionary, Clarendon Press, 1874, s.v.* auvandils-tá*.*
39. ↑ (in Chinese) *中國星座神話*, written by 陳久金. Published by 台灣書房出版有限公司, 2005, <templatestyles src="Module:Citation/CS1/styles.css" />ISBN 978-986-7332-25-7.
40. ↑ (in Chinese) AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 5 月 25 日
41. ↑ Steve Renshaw & Saori Ihara (October 1999). "Yowatashi Boshi; Stars that Pass in the Night". Griffith Observer. Archived from the original on 2 January 2013. Retrieved 25 June 2012.<templatestyles src="Module:Citation/CS1/styles.css"></templatestyles>
42. ↑ "Daijirin" p. 815 <templatestyles src="Module:Citation/CS1/styles.css" />ISBN 978-4-385-13902-9
43. ↑ Hōei Nojiri "Shin seiza jyunrei" p. 19 <templatestyles src="Module:Citation/CS1/styles.css" />ISBN 978-4-12-204128-8
44. ↑ Mudrooroo (1994). *Aboriginal mythology : an A-Z spanning the history of aboriginal mythology from the earliest legends to the present day*. London: HarperCollins. p. 142. ISBN 978-1-85538-306-7.<templatestyles src="Module:Citation/CS1/styles.css"></templatestyles>
45. ↑ **Lua error in Module:Citation/CS1/Identifiers at line 47: attempt to index field 'wikibase' (a nil value).**
46. ↑ Harney, Bill Yidumduma; Cairns, Hugh C. (2004) [2003]. *Dark Sparklers* (Revised ed.). Merimbula, New South Wales: Hugh C. Cairns. pp. 139–40. ISBN 0-9750908-0-1.<templatestyles src="Module:Citation/CS1/styles.css"></templatestyles>
47. ↑ p. 419, *Mythology: Myths, Legends and Fantasies*, Janet Parker, Alice Mills, Julie Stanton, Durban, Struik Publishers, 2007.
48. ↑ Kelley, David H.; Milone, Eugene F. (2011). *Exploring Ancient Skies: A Survey of Ancient and Cultural Astronomy*. Springer. p. 341. ISBN 144197623X.<templatestyles src="Module:Citation/CS1/styles.css"></templatestyles>
49. ↑ Best, Elsdon (1922). *Astronomical Knowledge of the Maori: Genuine and Empirical*. Wellington, New Zealand: Dominion Museum. pp. 39–40.<templatestyles src="Module:Citation/CS1/styles.css"></templatestyles>
50. ↑ Milbrath, Susan (1999). *Star Gods of the Maya: Astronomy in Art, Folklore, and Calendars*. Austin, Texas: University of Texas Press. p. 39. ISBN 0292752261.<templatestyles src="Module:Citation/CS1/styles.css"></templatestyles>

## External links

File:Commons-logo.svg Media related to Rigel at Wikimedia Commons

* NASA Astronomy Picture of the Day: Image of Rigel (29 December 2009)

Coordinates: Sky map 05h 14m 32.272s, −08° 12′ 05.91″