HD 95808

Star in the constellation Crater From Wikipedia, the free encyclopedia

HD 95808 is a double star in the constellation of Crater. Its apparent magnitude is 5.50,[3] but interstellar dust makes it appear 0.11 magnitudes dimmer than it should be.[5] It is located some 315 light-years (96.5 parsecs) away, based on parallax.[2]

Right ascension11h 03m 14.87928s[2]
Declination−11° 18 12.4984[2]
Quick facts Constellation, Right ascension ...
HD 95808
Observation data
Epoch J2000      Equinox J2000
Constellation Crater[1]
Right ascension 11h 03m 14.87928s[2]
Declination −11° 18 12.4984[2]
Apparent magnitude (V) 5.50[3]
Characteristics
Evolutionary stage red giant branch[2]
Spectral type G7-IIIb[4]
B−V color index +0.94[3]
Astrometry
Radial velocity (Rv)−8.90±0.10[5] km/s
Proper motion (μ) RA: −82.299[2] mas/yr
Dec.: −106.645[2] mas/yr
Parallax (π)10.3622±0.0926 mas[2]
Distance315 ± 3 ly
(96.5 ± 0.9 pc)
Absolute magnitude (MV)+0.44[1]
Details[5]
Mass2.43±0.15 M
Radius10.10±0.76 R
Luminosity64.6 L
Surface gravity (log g)3.05±0.07 cgs
Temperature5,029±34 K
Metallicity [Fe/H]−0.04±0.03 dex
Rotational velocity (v sin i)2.27±0.45 km/s
Age680±130 Myr
Other designations
BD−10°3184, HD 95808, HIP 54029, HR 4305, SAO 156421
Database references
SIMBADdata
Close

HD 95808 is a G-type giant star. At an age of 680 million years old, it has swelled up to a radius of 10.1 times that of the Sun, and it is 2.43 times as massive. It emits 64.6 times as much energy as the Sun at a surface temperature of 5,029 K.[5]

References

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