Gamma Leporis

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Template:Short description

γ Leporis
Template:Location mark
Location of γ Leporis (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Lepus
Right ascension Template:RA[1]
Declination Template:DEC[1]
Apparent magnitude (V) 3.587[2]
Characteristics
Spectral type F6 V[3]
U−B Template:Engvar −0.007[2]
B−V Template:Engvar +0.494[2]
Astrometry
Radial velocity (Rv)Script error: No such module "val".[1] km/s
Proper motion (μ) RA: −291.757 mas/yr[1]
Dec.: −368.521 mas/yr[1]
Parallax (π)112.2960±0.1452 mas[1]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)3.84[4]
Details
MassScript error: No such module "val".[5] Template:Solar mass
RadiusScript error: No such module "val".[5] Template:Solar radius
Luminosity (bolometric)Script error: No such module "val".[5] Template:Solar luminosity
Surface gravity (log g)Script error: No such module "val".[5] cgs
TemperatureScript error: No such module "val".[5] K
Metallicity [Fe/H]−0.12[6] dex
RotationScript error: No such module "val".[7] days
Rotational velocity (v sin i)15[8] km/s
Age1.3[4] Gyr
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[9]
Database references
SIMBADdata

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Gamma Leporis, Latinized from γ Leporis, is a star in the southern half of the constellation Lepus, southeast of Beta Leporis and southwest of Delta Leporis. With an apparent visual magnitude of 3.587,[2] it is bright enough to be seen with the naked eye. Based upon an annual parallax shift of Script error: No such module "val". as seen from Earth, its distance can be calculated as 29.04 light-years. It has a common proper motion companion, AK Leporis (or Gamma Leporis B), which is a variable star of the BY Draconis type and has an average brightness of magnitude 6.28.[10] The two are Script error: No such module "val". apart can be well seen in binoculars.[9] Gamma Leporis is a member of the Ursa Major Moving Group.[11]

Gamma Leporis is an F-type main-sequence star with a stellar classification of F6 V.[3] It is larger than the Sun with 1.30 times the radius of the Sun and 1.17 times the Sun's mass.[5] The star is around 1.3 billion years old[4] and is spinning with a rotation period of about six days.[7] 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.[7]

Van Biesbroeck's star catalog of 1961 lists the red dwarf star VB 1 as a companion of Gamma Leporis,[12] but this is a background star that is not physically associated.[13] It should not be confused with AK Leporis (Gamma Leporis B), which is a true companion star.[14][15]

See also

References

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  4. a b c Script error: No such module "Citation/CS1". Note: see VizieR catalogue V/130.
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  15. Script error: No such module "Citation/CS1". Data available at https://gruze.org/10pc/ Template:Webarchive

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External links

Template:Stars of Lepus