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Gacrux

Coordinates:Sky map12h 31m 09.95961s, −57° 06′ 47.5684″
From Wikipedia, the free encyclopedia
Star in the constellation Crux
γ Crucis

Gacrux, γ Crucis
Observation data
EpochJ2000.0      EquinoxJ2000.0
ConstellationCrux
Right ascension12h 31m 09.960s[1]
Declination−57° 06′ 47.57″[1]
Apparent magnitude (V)+1.64[2]
Characteristics
Evolutionary stageRed giant branch
Spectral typeM3.5 III[3]
Apparent magnitude (J)−1.99
U−Bcolor index+1.78[2]
B−Vcolor index+1.59[2]
Variable typeSRV[3]
Astrometry
Radial velocity (Rv)+20.6[4] km/s
Proper motion (μ)RA: +28.23mas/yr[1]
Dec.: −265.08mas/yr[1]
Parallax (π)36.83±0.18 mas[1]
Distance88.6 ± 0.4 ly
(27.2 ± 0.1 pc)
Absolute magnitude (MV)−0.68±0.01[5]
Details
Mass1.5±0.2[6] M
Radius73[7] R
Luminosity830[6] L
Surface gravity (log g)0.75±0.02[6] cgs
Temperature3689±125[6] K
Other designations
Gacrux,γ Crucis,CD−56 4504,GJ 470,HD 108903,HIP 61084,HR 4763,SAO 240019,LTT 4752
Database references
SIMBADdata

Gacrux is the third-brightest star in the southern constellation ofCrux, the Southern Cross. It has theBayer designationGamma Crucis, which isLatinised fromγ Crucis and abbreviatedGamma Cru orγ Cru. With anapparent visual magnitude of +1.63,[8] it is the26th brightest star in thenight sky. A line from the two "Pointers",Alpha Centauri throughBeta Centauri, leads to within 1° north of this star. Usingparallax measurements made during theHipparcos mission, it is 88.6light-years (27.2parsecs) distant.[1] It is the nearest M-typered giant star.[9]

Nomenclature

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The constellationCrux, with the reddish star Gacrux at the top of the constellation (north) in this image

γ Crucis (Latinised toGamma Crucis) is the star'sBayer designation. Gacrux is currently at roughly 60° southdeclination. It was known and visible to theancient Greeks andRomans as it was visible north of 40°latitude because of theprecession of equinoxes. Oddly, it lacked a traditional name. The astronomerPtolemy counted it as part of the constellation ofCentaurus.[10] The nameGacrux was coined by astronomer Elijah Hinsdale Burritt (1794-1838) as a contraction of the Bayer designation.[11][12] In 2016, theInternational Astronomical Union organized aWorking Group on Star Names (WGSN)[13] to catalog and standardize proper names for stars. The WGSN's first bulletin of July 2016[14] included a table of the first two batches of names approved by the WGSN, which includedGacrux for this star.

InChinese astronomy, Gamma Crucis was known as十字架一 (Shí Zì Jià yī, English:the First Star of Cross).[15]

The people ofAranda andLuritja tribe aroundHermannsburg,Central Australia namedIritjinga, "The Eagle-hawk", a quadrangular arrangement comprising Gacrux,Delta Crucis (Imai),Gamma Centauri (Muhilfain) andDelta Centauri (Ma Wei).[16] To the Boorong clan of theWergaia, this star is known as Bunya.[17][18]

Among Portuguese-speaking peoples, especially in Brazil, it is also namedRubídea (or Ruby-like), in reference to its colour.[19]

Physical properties

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Pulsation Periods[3]
Period
(days)
Amplitude
(magnitude)
12.10.016
15.10.027
16.50.016
54.80.026
82.70.015
104.90.016
Alight curve for Gamma Crucis, plotted from data published by Taburet al.[3]

Gacrux has the MK systemstellar classification of M3.5 III.[3] It hasevolved off of themain sequence to become ared giant star, but is most likely on thered giant branch rather than theasymptotic giant branch.[9] Although only 50% more massive than the Sun,[6] at this stage the star has expanded to 73[7] times theSun's radius. It is radiating roughly 830 times theluminosity of the Sun from its expandedouter envelope.[6] With aneffective temperature of 3,689 K,[6] the colour of Gacrux is a prominent reddish-orange, well in keeping with its spectral classification. It is asemi-regular variable with multiple periods.[3] (See table at left.)

The atmosphere of this star is enriched withbarium, which is usually explained by the transfer of material from a more evolved companion. Typically this companion will subsequently become awhite dwarf.[20] However, no such companion has yet been detected. A +6.4 magnitude companion star named HD 108925 (A3IVn) lies about 2 arcminutes away at aposition angle of 128° from the main star, and can be observed withbinoculars. But it is only an optical companion,[21] which is about 400 light years distant from Earth.

In culture

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Gacrux is represented in the flags ofAustralia,New Zealand,Samoa, andPapua New Guinea as one of five stars (four in the case of New Zealand) that compose theSouthern Cross.

It is also featured on theflag of Brazil, along with 26 other stars, each of which represents a state. Gacrux represents the State ofBahia.[22] The position of the line passing through Gacrux andAcrux marks thelocal meridian of the sky observed fromRio de Janeiro, at 8:30 am on 15 November 1889, the time when the republic was formally ratified.[23]

See also

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References

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  1. ^abcdevan Leeuwen, F. (November 2007). "Validation of the new Hipparcos reduction".Astronomy and Astrophysics.474 (2):653–664.arXiv:0708.1752.Bibcode:2007A&A...474..653V.doi:10.1051/0004-6361:20078357.S2CID 18759600.
  2. ^abcDucati, J. R. (2002). "VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system".CDS/ADC Collection of Electronic Catalogues.2237: 0.Bibcode:2002yCat.2237....0D.
  3. ^abcdefTabur, V.; et al. (December 2009)."Long-term photometry and periods for 261 nearby pulsating M giants".Monthly Notices of the Royal Astronomical Society.400 (4):1945–1961.arXiv:0908.3228.Bibcode:2009MNRAS.400.1945T.doi:10.1111/j.1365-2966.2009.15588.x.S2CID 15358380.
  4. ^Wielen, R.; et al. (1999). "Sixth Catalogue of Fundamental Stars (FK6). Part I. Basic fundamental stars with direct solutions".Veröff. Astron. Rechen-Inst. Heidelb.35 (35). Astronomisches Rechen-Institut Heidelberg: 1.Bibcode:1999VeARI..35....1W.
  5. ^R., Neuhäuser; G., Torres; M., Mugrauer; D. L., Neuhäuser; J., Chapman; D., Luge; Matteo, Cosci (2022)."Colour evolution of Betelgeuse and Antares over two millennia, derived from historical records, as a new constraint on mass and age".Monthly Notices of the Royal Astronomical Society (in Italian).516 (1).arXiv:2207.04702.doi:10.1093/mnras/stac1969.hdl:10278/5003332.ISSN 0035-8711.
  6. ^abcdefgKallinger, T.; Beck, P. G.; Hekker, S.; Huber, D.; Kuschnig, R.; Rockenbauer, M.; Winter, P. M.; Weiss, W. W.; Handler, G.; Moffat, A. F. J.; Pigulski, A.; Popowicz, A.; Wade, G. A.; Zwintz, K. (2019-04-01)."Stellar masses from granulation and oscillations of 23 bright red giants observed by BRITE-Constellation".Astronomy & Astrophysics.624: A35.arXiv:1902.07531.Bibcode:2019A&A...624A..35K.doi:10.1051/0004-6361/201834514.ISSN 0004-6361.
  7. ^abNielsen, Krister E.; Airapetian, Vladimir S.; Carpenter, Kenneth G.; Rau, Gioia (2023-08-01)."The Advanced Spectral Library: The Evolution of Chromospheric Wind Characteristics from Noncoronal to Hybrid Giant Stars".The Astrophysical Journal.953 (1): 16.Bibcode:2023ApJ...953...16N.doi:10.3847/1538-4357/acdcf1.ISSN 0004-637X.
  8. ^Johnson, H. L.; et al. (1966). "UBVRIJKL photometry of the bright stars".Communications of the Lunar and Planetary Laboratory.4 (99): 99.Bibcode:1966CoLPL...4...99J.
  9. ^abIreland, M. J.; et al. (May 2004)."Multiwavelength diameters of nearby Miras and semiregular variables".Monthly Notices of the Royal Astronomical Society.350 (1):365–374.arXiv:astro-ph/0402326.Bibcode:2004MNRAS.350..365I.doi:10.1111/j.1365-2966.2004.07651.x.S2CID 15830460.
  10. ^Richard Hinckley Allen, "Star Names: Their Lore and Meaning", Dover Press, 1963.
  11. ^"Gacrux/Gamma Crucis 2?". SolStation.com. Archived fromthe original on 7 April 2023. Retrieved2011-11-03.
  12. ^Lesikar, Arnold V."Gacrux". Dome Of The Sky. Archived fromthe original on 2011-09-28. Retrieved2011-11-03.
  13. ^"IAU Working Group on Star Names (WGSN)". Archived fromthe original on 10 June 2016. Retrieved22 May 2016.
  14. ^"Bulletin of the IAU Working Group on Star Names, No. 1"(PDF). Retrieved28 July 2016.
  15. ^(in Chinese)香港太空館 - 研究資源 - 亮星中英對照表Archived January 30, 2011, at theWayback Machine, Hong Kong Space Museum. Accessed on line November 23, 2010.
  16. ^Raymond Haynes; Roslynn D. Haynes; David Malin; Richard McGee (1996),Explorers of the Southern Sky: A History of Australian Astronomy, Cambridge: Cambridge University Press, p. 8,ISBN 978-0-521-36575-8
  17. ^Hamacher, Duane W.; Frew, David J. (2010). "An aboriginal Australian record of the great eruption of Eta Carinae".Journal of Astronomical History and Heritage.13 (3):220–234.arXiv:1010.4610.Bibcode:2010JAHH...13..220H.doi:10.3724/SP.J.1440-2807.2010.03.06.S2CID 118454721.
  18. ^"NameExoWorlds 2022 Naming Rules".IAU. Retrieved26 April 2025.
  19. ^da Silva Oliveira, R.,"Crux Australis: o Cruzeiro do Sul", Artigos: Planetario Movel Inflavel AsterDomus.
  20. ^Gomez, A. E.; Luri, X.; Grenier, S.; et al. (March 1997). "Absolute magnitudes and kinematics of barium stars".Astronomy and Astrophysics.319:881–885.Bibcode:1997A&A...319..881G.
  21. ^Kaler, James B."GACRUX (Gamma Crucis)".Stars.University of Illinois. Retrieved2012-03-03.
  22. ^"Astronomy of the Brazilian Flag". FOTW Flags Of The World website.
  23. ^"Flag of Brazil". World Afropedia.

Further reading

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