You can edit almost every page by Creating an account. Otherwise, see the FAQ.

6 Orionis

From EverybodyWiki Bios & Wiki

Script error: No such module "AfC submission catcheck".

6 Orionis
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Orion
Right ascension  04h 54m 46.895s
Declination +11° 25′ 33.825″
Apparent magnitude (V) +5.149
Characteristics
Evolutionary stage Red supergiant
Spectral type M1–M2 Ia–ab
Apparent magnitude (J) −3.00
Apparent magnitude (K) −4.05
U−B color index +2.06
B−V color index +1.85
Variable type SRc
Astrometry
Radial velocity (Rv)+21.91 km/s
Proper motion (μ) RA: 26.42±0.25 mas/yr
Dec.: 9.60±0.12[1] mas/yr
Parallax (π)14.128[2] mas
Distance548+90
−49
 ly
(168.1+27.5
−14.9
[2] pc)
Absolute magnitude (MV)−5.85[3]
Details
Mass16.5-19[2] M
Radius764+116
−62
[2]–1,021[4] R
Luminosity126,000+83,000
−50,000
[5] (90,000150,000)[6] L
Surface gravity (log g)−0.5[7] cgs
Temperature3,600±200[2] K
Metallicity [Fe/H]+0.05[8] dex
Rotation36±8[9] years
Rotational velocity (v sin i)5.47±0.25[9] km/s
Age8.0–8.5[5] Myr
Other designations
Betelgeuse, α Ori, 58 Ori, HR 2061, BD+7°1055, HD 39801, FK5 224, HIP 27989, SAO 113271, GC 7451, CCDM J05552+0724, AAVSO 0549+07
Database references
SIMBADdata

6 Orionis (also known by its Flamsteed designation g Orionis is a double star in the constellation of Orion.




References[edit]

  1. Cite error: Invalid <ref> tag; no text was provided for refs named harper2017
  2. 2.0 2.1 2.2 2.3 2.4 Cite error: Invalid <ref> tag; no text was provided for refs named joyce2020
  3. Lambert, D.L.; Brown, J.A.; Hinkle, K.H.; Johnson, H.R. (September 1984). "Carbon, nitrogen and oxygem abundances in Betelgeuse". Astrophysical Journal. 284: 223–237. Bibcode:1984ApJ...284..223L. doi:10.1086/162401. ISSN 0004-637X.
  4. Kravchenko, K.; Jorissen, A.; Van Eck, S.; Merle, T.; Chiavassa, A.; Paladini, C.; Freytag, B.; Plez, B.; Montargès, M.; Van Winckel, H. (2021-04-01). "Atmosphere of Betelgeuse before and during the Great Dimming event revealed by tomography". Astronomy & Astrophysics. 2104: arXiv:2104.08105. arXiv:2104.08105. Bibcode:2021A&A...650L..17K. doi:10.1051/0004-6361/202039801. Unknown parameter |s2cid= ignored (help)
  5. 5.0 5.1 Dolan, Michelle M.; Mathews, Grant J.; Lam, Doan Duc; Lan, Nguyen Quynh; Herczeg, Gregory J.; Dearborn, David S.P. (2017). "Evolutionary Tracks for Betelgeuse". The Astrophysical Journal. 819 (1): 7. arXiv:1406.3143v2. Bibcode:2016ApJ...819....7D. doi:10.3847/0004-637X/819/1/7. Unknown parameter |s2cid= ignored (help)
  6. Cite error: Invalid <ref> tag; no text was provided for refs named SMITH2009
  7. Lobel, Alex; Dupree, Andrea K. (2000). "Modeling the variable chromosphere of α Orionis". The Astrophysical Journal. 545 (1): 454–74. Bibcode:2000ApJ...545..454L. doi:10.1086/317784.
  8. Ramírez, Solange V.; Sellgren, K.; Carr, John S.; Balachandran, Suchitra C.; Blum, Robert; Terndrup, Donald M.; Steed, Adam (July 2000). "Stellar Iron Abundances at the Galactic Center". The Astrophysical Journal. 537 (1): 205–20. arXiv:astro-ph/0002062. Bibcode:2000ApJ...537..205R. doi:10.1086/309022. Unknown parameter |s2cid= ignored (help)
  9. 9.0 9.1 Kervella, Pierre; Decin, Leen; Richards, Anita M.S.; Harper, Graham M.; McDonald, Iain; O'Gorman, Eamon; Montargès, Miguel; Homan, Ward; Ohnaka, Keiichi (2018). "The close circumstellar environment of Betelgeuse. V. Rotation velocity and molecular envelope properties from ALMA". Astronomy and Astrophysics. 609: A67. arXiv:1711.07983. Bibcode:2018A&A...609A..67K. doi:10.1051/0004-6361/201731761. Unknown parameter |s2cid= ignored (help)


This article "6 Orionis" is from Wikipedia. The list of its authors can be seen in its historical and/or the page Edithistory:6 Orionis. Articles copied from Draft Namespace on Wikipedia could be seen on the Draft Namespace of Wikipedia and not main one.