| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Vela |
| Right ascension | 09h00m 05.4104s[1] |
| Declination | −41° 15′ 12.9734″[1] |
| Apparent magnitude (V) | 4.45[2] |
| Characteristics | |
| Spectral type | G8-K1III[3] + A7[4] |
| B−V color index | 0.75±0.02[2] |
| Variable type | Constant[3] |
| Astrometry | |
| Radial velocity (Rv) | −7.4±4.1[2] km/s |
| Proper motion (μ) | RA: −42.227[1] mas/yr Dec.: 50.599[1] mas/yr |
| Parallax (π) | 14.9687 ± 0.2155 mas[1] |
| Distance | 218 ± 3 ly (66.8 ± 1.0 pc) |
| Absolute magnitude (MV) | 0.40[2] |
| Orbit[3] | |
| Period (P) | 74.13715±0.00073 d |
| Semi-major axis (a) | ≥ (2.0057±0.0004)×107 km |
| Eccentricity (e) | 0.00085±0.00019 |
| Periastron epoch (T) | 2453625.5112±0.0017 HJD |
| Argument of periastron (ω) (secondary) | 106±13° |
| Semi-amplitude (K1) (primary) | 19.6744±0.0041 km/s |
| Details | |
| A | |
| Radius | 7.97+0.66 −1.42[1] R☉ |
| Luminosity | 68.769±1.152[1] L☉ |
| Temperature | 5889+607 −232[1] K |
| Metallicity [Fe/H] | 0.72±0.15[5] dex |
| Other designations | |
w Vel, CD−40° 4810, FK5 1234, HD 77258, HIP 44191, HR 3591, SAO 220730[6] | |
| Database references | |
| SIMBAD | data |
HD 77258 is a binary star system in the southern constellationofVela. It has the Bayer designation w Velorum, while HD 77258 is the identifier from the Henry Draper Catalogue. The system is visible to the naked eye as a faint point of light with a combined apparent visual magnitude of 4.45.[2] It is located at a distance of approximately 218 light years from the Sun based on parallax.[1] The radial velocity of the system barycenter is poorly constrained, but it appears to be drifting away at a rate of ~7 km/s.[2]
The radial velocity variation of this system was first reported by H. K. Palmer in 1904. It is a single-lined spectroscopic binary with an orbital period of 74.14 days and an eccentricity (ovalness) of 0.00085, indicating the orbit is essentially circular.[3] The visible component has a stellar classification of G8-K1III,[3] matching a late G-type giant star. This is an evolved star that has exhausted the supply of hydrogen at its core, then cooled and expanded away from the main sequence. In 1975, S. Maladora flagged the spectrumaspeculiar.[7]
The level of ultraviolet flux coming from this system suggests the companion is a hot A-type star of class A6.5 or A7.[4] The system is a source of X-ray emission.[8]
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