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Phi2 Orionis

From Wikipedia, the free encyclopedia
Star in the constellation Orion
For other stars with thisBayer designation, seePhi Orionis.
φ2 Orionis
φ2 (circled) in the constellation Orion
Observation data
EpochJ2000.0      EquinoxJ2000.0 (ICRS)
ConstellationOrion
Right ascension05h 36m 54.389s[1]
Declination+09° 17′ 26.42″[1]
Apparent magnitude (V)4.081[2]
Characteristics
Evolutionary stageYellow giant
Spectral typeG8 III-IV[3]
U−Bcolor index+0.618[2]
B−Vcolor index+0.966[2]
Astrometry
Radial velocity (Rv)99.03±0.18[1] km/s
Proper motion (μ)RA: +98.301mas/yr[1]
Dec.: −305.022mas/yr[1]
Parallax (π)28.6722±0.1859 mas[1]
Distance113.8 ± 0.7 ly
(34.9 ± 0.2 pc)[1]
Absolute magnitude (MV)+1.33±0.07[4]
Details[5]
Mass1.07±0.04 M
Radius8.22±0.07[6] R
Luminosity29.8±0.4[6] L
Surface gravity (log g)3.00±0.02 cgs
Temperature4,703±11[6] K
Metallicity[Fe/H]−0.56±0.02 dex
Rotational velocity (v sin i)1.91±0.53 km/s
Age6.91±1.04 Gyr
Other designations
φ2 Ori,40 Orionis,BD+09°898,HD 37160,HIP 26366,HR 1907,SAO 112958[7]
Database references
SIMBADdata
Yellow φ2 Orionis with nebulosity east ofφ1 Orionis and south-east ofλ Orionis

Phi2 Orionis is astar in theconstellationOrion, where it forms a small triangle on thecelestial sphere with the nearbyMeissa andPhi1 Orionis.[8] This star is visible to the naked eye with anapparent visual magnitude of 4.081.[2] Based upon an annualparallax shift of 28.67 mas,[6] it is located around 114 light-years from theSun.

This is an evolvedG-type star ofstellar classification G8 III-IV,[3] which means that it is in anevolutionary stage between asubgiant (IV) and agiant star (III). It is estimated to be 6.9 billion years old, has 1.07 times themass of the Sun,[5] but has expanded to 8 times theSun's radius. The star shines with 30 times thesolar luminosity from itsouter atmosphere at aneffective temperature of4,700 K.[6]

References

[edit]
  1. ^abcdefVallenari, A.; et al. (Gaia collaboration) (2023)."Gaia Data Release 3. Summary of the content and survey properties".Astronomy and Astrophysics.674: A1.arXiv:2208.00211.Bibcode:2023A&A...674A...1G.doi:10.1051/0004-6361/202243940.S2CID 244398875. Gaia DR3 record for this source atVizieR.
  2. ^abcdCousins, A. W. J. (1984), "Standardization of Broadband Photometry of Equatorial Standards",South African Astronomical Observatory Circulars,8: 59,Bibcode:1984SAAOC...8...59C.
  3. ^abFrasca, A.; et al. (December 2009), "REM near-IR and optical photometric monitoring of pre-main sequence stars in Orion. Rotation periods and starspot parameters",Astronomy and Astrophysics,508 (3):1313–1330,arXiv:0911.0760,Bibcode:2009A&A...508.1313F,doi:10.1051/0004-6361/200913327,S2CID 118361131.
  4. ^Charbonnel, Corinne; et al. (April 1998), "Mixing processes during the evolution of red giants with moderate metal deficiencies: the role of molecular-weight barriers",Astronomy and Astrophysics,332:204–214,arXiv:astro-ph/9712207,Bibcode:1998A&A...332..204C.
  5. ^abJofré, E.; et al. (2015), "Stellar parameters and chemical abundances of 223 evolved stars with and without planets",Astronomy & Astrophysics,574: A50,arXiv:1410.6422,Bibcode:2015A&A...574A..50J,doi:10.1051/0004-6361/201424474,S2CID 53666931, A50.
  6. ^abcdeBaines, Ellyn K.; Clark, James H., III; Schmitt, Henrique R.; Stone, Jordan M.; von Braun, Kaspar (2023-12-01)."33 New Stellar Angular Diameters from the NPOI, and Nearly 180 NPOI Diameters as an Ensemble".The Astronomical Journal.166 (6): 268.arXiv:2505.23514.Bibcode:2023AJ....166..268B.doi:10.3847/1538-3881/ad08be.ISSN 0004-6256.{{cite journal}}: CS1 maint: multiple names: authors list (link)
  7. ^"phi02 Ori".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2016-11-30.{{cite web}}: CS1 maint: postscript (link)
  8. ^Kaler, James B. (February 10, 2012),"Phi-1 Orionis",Stars, University of Illinois, retrieved2016-11-30.
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