Gamma Leporis
  | |
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Lepus |
| Right ascension | 05h 44m 27.79089s[1] |
| Declination | −22° 26′ 54.1808″[2] |
| Apparent magnitude (V) | 3.587[3] |
| Characteristics | |
| Spectral type | F6 V[4] |
| U−B color index | −0.007[3] |
| B−V color index | +0.494[3] |
| Absolute magnitude (MV) | 3.84[6] |
| Details | |
Gyr | |
| Database references | |
| SIMBAD | data |
Gamma Leporis,
Ursa Major Moving Group.[7]
Gamma Leporis is an
rotation period of about six days.[8] Based upon its stellar characteristics and distance from Earth, Gamma Leporis was considered a high-priority target for NASA's Terrestrial Planet Finder mission. It has been examined for an infrared excess, but none has been observed.[8]
See also
References
- S2CID 18759600.
- ^ Bibcode:1997A&A...323L..49P.
- ^ Bibcode:1966PDAUC...1....1G.
- ^ S2CID 55727428.
- Bibcode:1967IAUS...30...57E.
- ^ .
- ^ S2CID 119260429.
- ^ S2CID 55251562, A51.
- ^ Bibcode:1996A&A...314..191G.
- Bibcode:1970CoAsi.239....1B.
- ^ Centre de Données astronomiques de Strasbourg. Retrieved 2011-01-16.
- ^ STERNBILD HASE (PDF), archived from the original (PDF) on 2021-06-02, retrieved 2022-01-19
