Astronomy:HD 74272
Observation data Equinox J2000.0]] (ICRS) | |
---|---|
Constellation | Vela |
Right ascension | 08h 41m 13.12966s[1] |
Declination | −47° 19′ 01.6610″[1] |
Apparent magnitude (V) | 4.74[2] |
Characteristics | |
Spectral type | A5 II[3] |
B−V color index | 0.137±0.029[2] |
Astrometry | |
Radial velocity (Rv) | +17.4±2.8[2] km/s |
Proper motion (μ) | RA: −8.228[1] mas/yr Dec.: +10.051[1] mas/yr |
Parallax (π) | 1.7639 ± 0.1441[1] mas |
Distance | 1,800 ± 200 ly (570 ± 50 pc) |
Absolute magnitude (MV) | −4.67[2] |
Details | |
Mass | 8.8±0.1[4] M☉ |
Radius | 33.11+1.76 −0.82[1] R☉ |
Luminosity | 3,287±312[1] L☉ |
Temperature | 7,595+96 −194[1] K |
Rotational velocity (v sin i) | [5] km/s |
Age | 29.8±3.4[4] Myr |
Other designations | |
Database references | |
SIMBAD | data |
HD 74272 is a star in the constellation Vela. It has the Bayer designation n Velorum, while HD 74272 is the identifier from the Henry Draper catalogue. This is a white hued star that is faintly visible to the naked eye with an apparent visual magnitude of 4.74.[2] It is located at a distance of approximately 1,800 light years from the Sun based on parallax.[1] The star is drifting further away with a radial velocity of +17 km/s.[2]
This is an aging, massive bright giant star with a stellar classification of A5 II.[3] It is an estimated 30 million years old with 8.8 times the mass of the Sun.[4] Having exhausted the supply of hydrogen at its core, it has expanded to around 33[1] times the radius of the Sun. The star is radiating 3,287[1] times the Sun's luminosity from its enlarged photosphere at an effective temperature of 7,595 K.[1]
References
- ↑ 1.00 1.01 1.02 1.03 1.04 1.05 1.06 1.07 1.08 1.09 1.10 1.11 Brown, A. G. A. (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics 616: A1. doi:10.1051/0004-6361/201833051. Bibcode: 2018A&A...616A...1G. Gaia DR2 record for this source at VizieR.
- ↑ 2.0 2.1 2.2 2.3 2.4 2.5 Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters 38 (5): 331, doi:10.1134/S1063773712050015, Bibcode: 2012AstL...38..331A.
- ↑ 3.0 3.1 Houk, Nancy (1978), Michigan catalogue of two-dimensional spectral types for the HD stars, 2, Ann Arbor: Dept. of Astronomy, University of Michigan, Bibcode: 1978mcts.book.....H.
- ↑ 4.0 4.1 4.2 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
- ↑ Uesugi, Akira; Fukuda, Ichiro (1970), "Catalogue of rotational velocities of the stars", Contributions from the Institute of Astrophysics and Kwasan Observatory (University of Kyoto), Bibcode: 1970crvs.book.....U.
- ↑ "n Vel". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=n+Vel.
Original source: https://en.wikipedia.org/wiki/HD 74272.
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