Astronomy:Xi1 Sagittarii
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Short description: Star in the constellation Sagittarius
Observation data Equinox J2000.0]] (ICRS) | |
---|---|
Constellation | Sagittarius |
Right ascension | 18h 57m 20.47670s[1] |
Declination | −20° 39′ 22.8539″[1] |
Apparent magnitude (V) | +5.06[2] |
Characteristics | |
Spectral type | B9/A0 Ib[3] |
U−B color index | −0.14[2] |
B−V color index | +0.12[2] |
Astrometry | |
Proper motion (μ) | RA: −1.46[1] mas/yr Dec.: −5.75[1] mas/yr |
Parallax (π) | 1.58 ± 0.26[1] mas |
Distance | approx. 2,100 ly (approx. 600 pc) |
Absolute magnitude (MV) | −3.92[4] |
Details | |
Mass | 7.8±0.1[5] M☉ |
Radius | 15[6] R☉ |
Luminosity | 2,753[7] L☉ |
Surface gravity (log g) | 2.3[8] cgs |
Temperature | 9,400[8] K |
Metallicity [Fe/H] | −0.20[8] dex |
Rotational velocity (v sin i) | 10[9] km/s |
Age | 39.8±4.9[5] Myr |
Other designations | |
Database references | |
SIMBAD | data |
Xi1 Sagittarii (ξ1 Sagittarii) is a solitary,[11] blue-white hued star in the zodiac constellation of Sagittarius. It is visible to the naked eye with an apparent visual magnitude of +5.06.[2] Based upon a small annual parallax shift of 1.58 mas as seen from Earth,[1] this system is located roughly 2,100 light years from the Sun.
This is a massive supergiant star[6] with a stellar classification of B9/A0 Ib.[3] With an estimated 7.8[5] times the mass of the Sun and an age of about 40[5] million years it has depleted the hydrogen at its core, causing it to expand to about 15 times the Sun's radius.[6] It is radiating 2,753[7] times the Sun's luminosity from its photosphere at an effective temperature of about 9,400 K.[8]
References
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 van Leeuwen, F. (2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics 474 (2): 653–664, doi:10.1051/0004-6361:20078357, Bibcode: 2007A&A...474..653V.
- ↑ 2.0 2.1 2.2 2.3 Fernie, J. D. (1983), "New UBVRI photometry for 900 supergiants", Astrophysical Journal Supplement Series 52: 7, doi:10.1086/190856, Bibcode: 1983ApJS...52....7F.
- ↑ 3.0 3.1 Houk, Nancy; Smith-Moore, M. (1978), Michigan catalogue of two-dimensional spectral types for the HD stars, 4, Ann Arbor: Dept. of Astronomy, University of Michigan, Bibcode: 1988mcts.book.....H.
- ↑ Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters 38 (5): 331, doi:10.1134/S1063773712050015, Bibcode: 2012AstL...38..331A.
- ↑ 5.0 5.1 5.2 5.3 Tetzlaff, N. et al. (January 2011), "A catalogue of young runaway Hipparcos stars within 3 kpc from the Sun", Monthly Notices of the Royal Astronomical Society 410 (1): 190–200, doi:10.1111/j.1365-2966.2010.17434.x, Bibcode: 2011MNRAS.410..190T.
- ↑ 6.0 6.1 6.2 Venn, Kim A. (August 1995), "Atmospheric Parameters and LTE Abundances for 22 Galactic, A-Type Supergiants", Astrophysical Journal Supplement 99: 659, doi:10.1086/192201, Bibcode: 1995ApJS...99..659V.
- ↑ 7.0 7.1 McDonald, I. et al. (2012), "Fundamental Parameters and Infrared Excesses of Hipparcos Stars", Monthly Notices of the Royal Astronomical Society 427 (1): 343–57, doi:10.1111/j.1365-2966.2012.21873.x, Bibcode: 2012MNRAS.427..343M.
- ↑ 8.0 8.1 8.2 8.3 Soubiran, C.; Le Campion, J.-F.; Cayrel de Strobel, G.; Caillo, A. (June 2010), "The PASTEL catalogue of stellar parameters", Astronomy and Astrophysics 515: A111, doi:10.1051/0004-6361/201014247, Bibcode: 2010A&A...515A.111S.
- ↑ Royer, F. et al. (January 2012), "Rotational velocities of A-type stars. I. Measurement of v sin i in the southern hemisphere", Astronomy and Astrophysics 381: 105–121, doi:10.1051/0004-6361:20011422, Bibcode: 2002A&A...381..105R.
- ↑ "ksi01 Sgr". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=ksi01+Sgr.
- ↑ Eggleton, P. P.; Tokovinin, A. A. (September 2008), "A catalogue of multiplicity among bright stellar systems", Monthly Notices of the Royal Astronomical Society 389 (2): 869–879, doi:10.1111/j.1365-2966.2008.13596.x, Bibcode: 2008MNRAS.389..869E.
Original source: https://en.wikipedia.org/wiki/Xi1 Sagittarii.
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