Delta Leporis

Star in the constellation Lepus From Wikipedia, the free encyclopedia

Delta Leporis which is latinized from δ Leporis is a solitary,[10] orange-hued star in the southern constellation of Lepus. It is visible to the naked eye with an apparent visual magnitude of 3.85.[2] Based upon an annual parallax shift of 28.68 mas,[1] it is 114 light years distant from Earth.

Right ascension05h 51m 19.29613s[1]
Declination−20° 52 44.7232[1]
Quick facts Constellation, Right ascension ...
Delta Leporis
Location of δ Leporis (circled in red)
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Lepus
Right ascension 05h 51m 19.29613s[1]
Declination −20° 52 44.7232[1]
Apparent magnitude (V) 3.85[2]
Characteristics
Spectral type K1 IV Fe−0.5[3] or K0 IIIb Fe−1.5 CH0.5[4]
U−B color index +0.71[2]
B−V color index +0.98[2]
Astrometry
Radial velocity (Rv)+100.20[5] km/s
Proper motion (μ) RA: +229.49[1] mas/yr
Dec.: −648.41[1] mas/yr
Parallax (π)28.68±0.17 mas[1]
Distance113.7 ± 0.7 ly
(34.9 ± 0.2 pc)
Absolute magnitude (MV)+1.04[6]
Details
Mass0.94[6][7] M
Radius10.01±0.43[7] R
Luminosity45.7[6] L
Surface gravity (log g)2.41±0.10[7] cgs
Temperature4,684±80[7] K
Metallicity [Fe/H]−0.68±0.08[7] dex
Rotational velocity (v sin i)0[8] km/s
Age10.7[6] Gyr
Other designations
δ Lep, 15 Lep, BD−20°1211, FK5 222, GC 7362, HD 39364, HIP 27654, HR 2035, SAO 170926, LHS 1792[9]
Database references
SIMBADdata
Close

This is an old, evolved K-type star with an age of about 10.7 billion years.[6] Keenan and McNeil (1989) classified it as K0 IIIb Fe−1.5 CH0.5,[4] indicating it is a giant star showing a deficiency of iron and an excess of cyanogen in its atmosphere. However, Gray et al. (2006) listed it as K1 IV Fe−0.5,[3] which would suggest a less evolved subgiant star. It may be a red clump star, which indicates it is generating energy through helium fusion at its core.[11]

It has 94% of the Sun's mass, but a radius 10 times wider.[7] It is radiating 46 times the Sun's luminosity from its photosphere[6] at an effective temperature of 4,660 K.[12] It is a Population II star.[7]

References

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