| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Lynx |
| Right ascension | 08h 53m 50.80524s[1] |
| Declination | +33° 03′ 24.5206″[1] |
| Apparent magnitude (V) | 8.03[2] |
| Characteristics | |
| Spectral type | F8V[2] |
| B−V color index | 0.626[2] |
| Astrometry | |
| Radial velocity (Rv) | 21.79±0.13[1] km/s |
| Proper motion (μ) | RA: −95.110(29) mas/yr[1] Dec.: −28.503(26) mas/yr[1] |
| Parallax (π) | 12.8110 ± 0.0329 mas[1] |
| Distance | 254.6 ± 0.7 ly (78.1 ± 0.2 pc) |
| Absolute magnitude (MV) | 3.49[2] |
| Details[3] | |
| Mass | 1.295±0.015 M☉ |
| Radius | 1.58±0.11[4] R☉ |
| Luminosity | 2.9±0.3[4] L☉ |
| Surface gravity (log g) | 4.34±0.13 cgs |
| Temperature | 6122±52 K |
| Metallicity [Fe/H] | +0.29±0.06 dex |
| Rotational velocity (v sin i) | 4.2±0.5 km/s |
| Age | 3.2±0.4 Gyr |
| Other designations | |
| Database references | |
| SIMBAD | data |
HD 75898 is an 8th magnitude star approximately 255 light-years away in the constellation Lynx. The star is 28% more massive, 60% larger, and 3 times as luminous as the Sun. It is a metal-rich star, with 186% the solar abundance of iron. In 2007 the California and Carnegie Planet Search team found one planet orbiting HD 75898.[2]
GaiaDR3 was invoked but never defined (see the help page).Robinson2007 was invoked but never defined (see the help page).Ruggieri2024 was invoked but never defined (see the help page).Ment2018 was invoked but never defined (see the help page).Simbad was invoked but never defined (see the help page).