HD 100825

Star in the constellation Centaurus From Wikipedia, the free encyclopedia

HD 100825 is a single[7] star in the southern constellation of Centaurus. It has the Bayer designation C2 Centauri, while HD 100825 is the identifier from the Henry Draper catalogue. The star has a yellow-white hue and is dimly visible to the naked eye with an apparent visual magnitude of +5.26.[1] It is located at a distance of 187 light years from the Sun based on parallax, with an absolute magnitude of +1.31.[1] The radial velocity is poorly constrained, but the star appears to be drifting further away from the Sun at the rate of around 5 km/s.[1] It is a member of the Sirius supercluster of co-moving stars.[8]

Quick facts Observation data Epoch J2000.0 Equinox J2000.0, Constellation ...
C2 Centauri
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Centaurus[1]
Right ascension 11h 35m 55.58491s[2]
Declination −47° 38 29.9038[2]
Apparent magnitude (V) +5.26[1]
Characteristics
Evolutionary stage main sequence[2]
Spectral type F0V[3] or A7m[4]
B−V color index +0.257±0.003[1]
Astrometry
Radial velocity (Rv)+5.2±2.8[1] km/s
Proper motion (μ) RA: +33.654[2] mas/yr
Dec.: −49.433[2] mas/yr
Parallax (π)17.1828±0.0741 mas[2]
Distance189.8 ± 0.8 ly
(58.2 ± 0.3 pc)
Absolute magnitude (MV)+1.31[1]
Details
Mass1.62[5] M
Radius2.83[2] R
Luminosity21[2] L
Surface gravity (log g)3.97±0.14[5] cgs
Temperature7,737±263[5] K
Age467[5] Myr
Other designations
C2 Cen, CD−46°7205, FK5 435, GC 15901, HD 100825, HIP 56573, HR 4466, SAO 222895[6]
Database references
SIMBADdata
Close

This is an Am star[4] or metallic-line star with a stellar classification of F0V,[3] indicating it is a F-type main-sequence star that is generating energy by core hydrogen fusion. It is an estimated 467[5] million years old and has 1.62[5] times the mass of the Sun. The star is radiating 21 times the luminosity of the Sun[2] from its photosphere at an effective temperature of 7,737 K.[5]

References

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