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 |
Spectral Characteristics | |
Spectral type | F6-7 V/K2 V |
U-B color index | -0.01/0.75 |
B-V color index | 0.47/0.95 |
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 |
Physical Characteristics | |
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.