HD 10307

HD 10307
Location of HD 10307 (circled)
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Andromeda
Right ascension 01h 41m 47.1431s[1]
Declination +42° 36′ 48.4435″[1]
Apparent magnitude (V) 4.95 / 11[2]
Characteristics
Spectral type G1.5 V + M V[3]
U−B color index 0.11[4]
B−V color index 0.62[4]
Astrometry
Radial velocity (Rv)3.1±0.12[5] km/s
Proper motion (μ) RA: 813.337±0.380[1] mas/yr
Dec.: −171.027±0.464[1] mas/yr
Parallax (π)79.08 ± 0.63 mas[6]
Distance41.2 ± 0.3 ly
(12.6 ± 0.1 pc)
Absolute magnitude (MV)4.43[7]
Absolute bolometric
magnitude (Mbol)		4.32±0.06[8]
Orbit[6]
Period (P)19.542±0.014 yr
Semi-major axis (a)0.6104±0.0097″
Eccentricity (e)0.4367±0.0020
Inclination (i)100.36±0.89°
Longitude of the node (Ω)32.25±0.35°
Periastron epoch (T)2016.702±0.012
Argument of periastron (ω)
(secondary)		27.15±0.35°
Semi-amplitude (K1)
(primary)		2.7160±0.0072 km/s
Details[8]
HD 10307 A
Mass0.95±0.11[6] M☉
Radius1.14±0.04 R☉
Luminosity1.44 L☉
Surface gravity (log g)4.3±0.1 cgs
Temperature5,878±60 K
Metallicity [Fe/H]+0.00±0.06 dex
Rotational velocity (v sin i)1.5±1.0 km/s
Age7.0[9] Gyr
HD 10307 B
Mass0.254±0.019[6] M☉
Luminosity0.0013[10] L☉
Other designations
BD+41°328, GJ 67, HD 10307, HIP 7918, HR 483, SAO 37434, LHS 1284, YPC 350
Database references
SIMBADHD 10307
ARICNSHD 10307 A
HD 10307 B

HD 10307 (HR 483) is a spectroscopic binary star in the constellation Andromeda. The primary is similar to the Sun in mass, temperature and metal content. It is situated about 42 light-years from Earth. Its companion, HR 483 B, is a little-studied red dwarf.

HD 10307 was identified in September 2003 by astrobiologist Margaret Turnbull from the University of Arizona in Tucson as one of the most promising nearby candidates for hosting life based on her analysis of the HabCat list of stars.[11]

  1. ^ a b c d Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
  2. ^ "Sixth Catalog of Orbits of Visual Binary Stars". United States Naval Observatory. Archived from the original on 2017-08-01. Retrieved 2017-05-21.
  3. ^ Belikov, A. N. (1995). "Stellar Mass Catalogue (SMAC). Preliminary version". Bulletin d'Information du Centre de Données Stellaires. 47: 9. Bibcode:1995BICDS..47....9B.
  4. ^ a b Cite error: The named reference 11colors was invoked but never defined (see the help page).
  5. ^ Cite error: The named reference ncsbo was invoked but never defined (see the help page).
  6. ^ a b c d Torres, Guillermo (2022). "Orbital solution and dynamical masses for the nearby binary system GJ 67 AB". Monthly Notices of the Royal Astronomical Society. 514 (4): 5183–5191. arXiv:2206.10627. Bibcode:2022MNRAS.514.5183T. doi:10.1093/mnras/stac1710.
  7. ^ Cite error: The named reference Holmberg2009 was invoked but never defined (see the help page).
  8. ^ a b Fuhrmann, Klaus (2011). "Nearby stars of the Galactic disc and halo - V". Monthly Notices of the Royal Astronomical Society. 414 (4): 2893–2922. Bibcode:2011MNRAS.414.2893F. doi:10.1111/j.1365-2966.2011.18476.x.
  9. ^ Cite error: The named reference apj687 was invoked but never defined (see the help page).
  10. ^ Cite error: The named reference SolStation was invoked but never defined (see the help page).
  11. ^ Cite error: The named reference Bagnall was invoked but never defined (see the help page).