HD 74272
Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Vela[1] |
Right ascension | 08h 41m 13.12966s[2] |
Declination | −47° 19′ 01.6610″[2] |
Apparent magnitude (V) | 4.74[1] |
Characteristics | |
Spectral type | A5 II[3] |
B−V color index | 0.137±0.029[1] |
Astrometry | |
Radial velocity (Rv) | +17.4±2.8[1] km/s |
Proper motion (μ) | RA: −8.228[2] mas/yr Dec.: +10.051[2] mas/yr |
Parallax (π) | 1.7639±0.1441 mas[2] |
Distance | 1,800 ± 200 ly (570 ± 50 pc) |
Absolute magnitude (MV) | −4.67[1] |
Details | |
Mass | 8.8±0.1[4] M☉ |
Radius | 33.11+1.76 −0.82[2] R☉ |
Luminosity | 3,287±312[2] L☉ |
Temperature | 7,595+96 −194[2] K |
Rotational velocity (v sin i) | [5] km/s |
Age | 29.8±3.4[4] Myr |
Other designations | |
n Vel, CD−46°4448, FK5 2570, HD 74272, HIP 42624, HR 3452, SAO 220284[6] | |
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.[1] It is located at a distance of approximately 1,800 light years from the Sun based on parallax.[2] The star is drifting further away with a radial velocity of +17 km/s.[1]
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[2] times the radius of the Sun. The star is radiating 3,287[2] times the Sun's luminosity from its enlarged photosphere at an effective temperature of 7,595 K.[2]
References
[edit]- ^ a b c d e f g Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters. 38 (5): 331. arXiv:1108.4971. Bibcode:2012AstL...38..331A. doi:10.1134/S1063773712050015. XHIP record for this object at VizieR.
- ^ a b c d e f g h i j k l Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
- ^ a b Houk, Nancy (1978), Michigan catalogue of two-dimensional spectral types for the HD stars, vol. 2, Ann Arbor: Dept. of Astronomy, University of Michigan, Bibcode:1978mcts.book.....H.
- ^ a b c 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, arXiv:1007.4883, Bibcode:2011MNRAS.410..190T, doi:10.1111/j.1365-2966.2010.17434.x, S2CID 118629873
- ^ 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. Retrieved 2020-01-19.