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Star in the constellation Vela From Wikipedia, the free encyclopedia
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]
Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
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 mas[1] |
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 |
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]
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