Gamma Leporis
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| Observation data Epoch J2000 |
|
|---|---|
| Constellation | Lepus |
| Right ascension | 05h 44m 27.8s |
| Declination | -22° 26′ 54″ |
| Apparent magnitude (V) | 3.59/6.18 |
| Characteristics | |
| Spectral type | F6-7 V/K2 V |
| B-V color index | 0.47/0.95 |
| U-B color index | -0.01/0.75 |
| Variable type | None |
| Astrometry | |
| Radial velocity (Rv) | -9.7 km/s |
| Proper motion (μ) | RA: -292.42 mas/yr Dec.: -368.45 mas/yr |
| Parallax (π) | 111.69 ± 0.60 mas |
| Distance | 29.2 ± 0.2 ly (8.95 ± 0.05 pc) |
| Absolute magnitude (MV) | 3.83/6.42 |
| Details | |
| Mass | 1.2/0.63 M☉ |
| Radius | 1.3/0.63 R☉ |
| Luminosity | 2.6/0.25 L☉ |
| Temperature | 6439/5151 K |
| Metallicity | 82% |
| Rotation | 11 km/s. |
| Age | ? years |
| Other designations | |
Gamma Leporis (γ Lep / γ Leporis) is a multiple star system which is located at a distance of about 29 light-years from Earth and consists of 2 or 3 stars: Gamma Leporis A, Gamma Leporis B and possibly Gamma Leporis C.
Gamma Leporis lies in the south central part of the constellation Lepus, southeast of Beta Leporis and southwest of Delta Leporis. The system is a member of the Sirius group. Based upon its stellar characteristics and distance from Earth, Gamma Leporis is considered a high-priority target for NASA's Terrestrial Planet Finder mission.
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