HD 72922

HD 72922
Location of HD 72922 on the map (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Chamaeleon
Right ascension 08h 24m 19.8867s[1]
Declination −80° 54′ 51.2175″[1]
Apparent magnitude (V) 5.67[2]
Characteristics
Evolutionary stage horizontal branch[3]
Spectral type G8 III[4]
U−B color index +0.74[5]
B−V color index +1.02[5]
Astrometry
Radial velocity (Rv)27.5±0.6[6] km/s
Proper motion (μ) RA: −149.123[1] mas/yr
Dec.: +226.547[1] mas/yr
Parallax (π)11.8882 ± 0.111 mas[1]
Distance274 ± 3 ly
(84.1 ± 0.8 pc)
Absolute magnitude (MV)+1.27[2]
Details[7]
Mass0.96±0.04 M☉
Radius9.65±0.17 R☉
Luminosity41.2±0.9 L☉
Surface gravity (log g)2.56±0.12 cgs
Temperature4,708±34 K
Metallicity [Fe/H]−0.43±0.03 dex
Rotational velocity (v sin i)<1[8] km/s
Other designations
6 G. Chamaeleontis[9], CD−80°290, CPD−80°258, FK5 2664, GC 11625, HD 72922, HIP 41191, HR 3393, SAO 258496[10]
Database references
SIMBADdata

HD 72922, also known as HR 3393, is a suspected astrometric binary[11] located in the southern circumpolar constellation Chamaeleon. A 1993 paper by Olin J. Eggen lists it as a member of the Milky Way's old disk population.[12]

It has an apparent magnitude of 5.67,[2] making it faintly visible to the naked eye under ideal conditions. Based on parallax measurements from the Gaia satellite, the system is estimated to be 274 light years away from the Solar System.[1] However, it is receding with a heliocentric radial velocity of 27.5 km/s.[6] At its current distance, HD 72922's brightness is diminished by magnitudes due to interstellar dust. It has an absolute magnitude of +1.27.[2]

The visible component is an evolved red giant with a stellar classification of G8 III. It is currently on the horizontal branch,[3] fusing helium at its core. It has 96% the mass of the Sun and an enlarged radius of 9.65 R☉.[7] It radiates 41.2 times the luminosity of the Sun from its photosphere at an effective temperature of 4,708 K, giving it a yellowish hue.[7] HD 72922 is metal poor with a metallicity only 37% that of the Sun;[7] it spins too slowly to be measured.[8]

  1. ^ a b c d e f Cite error: The named reference EDR3 was invoked but never defined (see the help page).
  2. ^ a b c d Cite error: The named reference Anderson2012 was invoked but never defined (see the help page).
  3. ^ a b Cite error: The named reference Laney2011 was invoked but never defined (see the help page).
  4. ^ Cite error: The named reference Houk1975 was invoked but never defined (see the help page).
  5. ^ a b Cite error: The named reference Johnson1966 was invoked but never defined (see the help page).
  6. ^ a b Cite error: The named reference Gontcharov2006 was invoked but never defined (see the help page).
  7. ^ a b c d Cite error: The named reference Ottoni2022 was invoked but never defined (see the help page).
  8. ^ a b Cite error: The named reference DeMed2014 was invoked but never defined (see the help page).
  9. ^ Cite error: The named reference Gould1879 was invoked but never defined (see the help page).
  10. ^ Cite error: The named reference SIMBAD was invoked but never defined (see the help page).
  11. ^ Cite error: The named reference Eggleton2008 was invoked but never defined (see the help page).
  12. ^ Cite error: The named reference Eggen1993 was invoked but never defined (see the help page).