AK Leporis

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AK Leporis
Observation data
Epoch J2000      Equinox J2000
Constellation Lepus
Right ascension 05h 44m 26.543s[1]
Declination −22° 25′ 18.77″[1]
Apparent magnitude (V) 6.141[2]
Characteristics
Spectral type K2V[3]
U−B color index +0.74[4]
B−V color index +0.96[4]
Variable type BY Draconis[3]
Astrometry
Radial velocity (Rv) −9.57 ± 0.13[5] km/s
Proper motion (μ) RA: −304.4[6] mas/yr
Dec.: −352.2[6] mas/yr
Parallax (π) 112.0[7] mas
Distance 28 ly
(9.0[8] pc)
Absolute magnitude (MV) 6.31[2]
Details
Surface gravity (log g) 4.66 ± 0.01[9] cgs
Temperature 4,869 ± 61[9] K
Metallicity [Fe/H] 0.01 ± 0.06[9] dex
Rotational velocity (v sin i) 2.8 ± 1.8[5] km/s
Age 0.9[8] Gyr
Other designations
BD−22 1210, GJ 216 B, HD 38392, HR 1982, LTT 2363, SAO 170757.[10]
Database references
SIMBAD data

AK Leporis is a star in the southern constellation of Lepus the hare. It has an apparent visual magnitude of 6.141,[2] so, according to the Bortle scale, it is faintly visible from rural skies at night. This star forms a visual double with Gamma Leporis—the two have an angular separation of 97, making them difficult to separate with the naked eye even under the best conditions.[11] Both Gamma Leporis and AK Leporis are members of the Ursa Major Moving Group of stars that share a common motion through space.[5]

This is a BY Draconis variable star that undergoes brightness variations due to stellar activity. Differential rotation causes changes to the periodicity of the variation depending on the latitude of the activity.[3] X-ray emission has been detected from AK Leporis, and it is located at or near a radio source.[7]

Infrared observation of this star shows a large excess at a wavelength of 24 µm. This may be explained by the proximity of Gamma Leporis to the line of sight, or there may be a red dwarf companion. There is no excess observed at 70 µm.[8]

References

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