From Wikipedia, the free encyclopedia
57 Cancri
Observation data
Epoch J2000.0       Equinox J2000.0
Constellation Cancer
Right ascension 08h 54m 14.73274s [1]
Declination +30° 34′ 44.8283″ [1]
Apparent magnitude (V) +5.40 [2] (6.09 + 6.37) [3]
Characteristics
Spectral type G7 III + K0 III [4]
B−V color index 1.05 [2]
Astrometry
Radial velocity (Rv)−59.2±0.4 [2] km/s
Proper motion (μ) RA: +41.60 [1]  mas/ yr
Dec.: −24.02 [1]  mas/ yr
Parallax (π)7.07 ± 0.68  mas [1]
Distance460 ± 40  ly
(140 ± 10  pc)
Absolute magnitude (MV)–0.33 [2]
Details [5]
57 Cnc A
Mass6.49±2.16  M
Luminosity173.13 [2]  L
Surface gravity (log g)2.74±0.11  cgs
Temperature4,810±92  K
Metallicity [Fe/H]0.08±0.05  dex
Age645+154
−120
  Myr
Other designations
57 Cnc, BD+31°1907, GC 12289, HD 75959, HIP 43721, HR 3532, SAO 61125, ADS 7071, WDS J08542+3035 [6]
Database references
SIMBAD data

57 Cancri is a double star in the zodiac constellation of Cancer, located around 460  light years away from the Sun. [1] They are visible to the naked eye as a faint star with a combined apparent visual magnitude of +5.40. [2] The brighter member, designated component A. is a yellow-hued giant star with a stellar classification of G7 III [4] and an apparent magnitude of +6.09. [3] Its companion, component B, is an orange-hued giant with a class of K0 III [4] and an apparent magnitude of +6.37. [3] As of 2017, the pair had an angular separation of 1.50 along a position angle of 310°. [3]

References

  1. ^ a b c d e f van Leeuwen, F. (2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics, 474 (2): 653–664, arXiv: 0708.1752, Bibcode: 2007A&A...474..653V, doi: 10.1051/0004-6361:20078357, S2CID  18759600.
  2. ^ a b c d e f Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters, 38 (5): 331, arXiv: 1108.4971, Bibcode: 2012AstL...38..331A, doi: 10.1134/S1063773712050015, S2CID  119257644.
  3. ^ a b c d Mason, B. D.; et al. (2014), "The Washington Visual Double Star Catalog", The Astronomical Journal, 122 (6): 3466, Bibcode: 2001AJ....122.3466M, doi: 10.1086/323920
  4. ^ a b c Abt, Helmut A. (2008), "Visual Multiples. IX. MK Spectral Types", The Astrophysical Journal Supplement Series, 176 (1): 216–217, Bibcode: 2008ApJS..176..216A, doi: 10.1086/525529.
  5. ^ Feuillet, Diane K.; et al. (2016), "Determining Ages of APOGEE Giants with Known Distances", The Astrophysical Journal, 817 (1): 40, arXiv: 1511.04088, Bibcode: 2016ApJ...817...40F, doi: 10.3847/0004-637X/817/1/40, S2CID  118675933.
  6. ^ "57 Cnc". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-03-06.