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54 Cancri

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Star in the constellation Cancer
54 Cancri
Observation data
Epoch J2000      Equinox J2000
Constellation Cancer
Right ascension 08 51 01.4644
Declination +15° 21′ 02.364″
Apparent magnitude (V) 6.38
Characteristics
Spectral type G5 V-IV or G1V
B−V color index 0.629±0.020
Astrometry
Radial velocity (Rv)+45.098±0.032 km/s
Proper motion (μ) RA: −112.475 mas/yr
Dec.: +75.099 mas/yr
Parallax (π)24.79 ± 0.33 mas
Distance132 ± 2 ly
(40.3 ± 0.5 pc)
Absolute magnitude (MV)3.39
Details
Mass1.23±0.05 M
Radius1.81±0.20 R
Luminosity3.72+0.55
−0.48 L
Surface gravity (log g)4.04±0.04 cgs
Temperature5,862±15 K
Rotational velocity (v sin i)3.10±0.56 km/s
Age5.0+0.7
−0.4 Gyr
Other designations
54 Cnc, BD+15° 1917, FK5 2699, HD 75528, HIP 43454, HR 3510, SAO 98168
Database references
SIMBADdata

54 Cancri is a star in the zodiac constellation of Cancer. It has an apparent visual magnitude of 6.38, which places it just below the normal brightness limit of stars visible to the naked eye. The annual parallax shift is 24.79 mas as measured from Earth's orbit, which yields a distance estimate of about 132 light years. It is moving away from the Sun with a radial velocity of +45 km/s.

Measurement of the stars proper motion over time suggest changes due to an acceleration component, which may indicate it is a close binary system. The visible component has a stellar classification of G5 V, indicating it is an ordinary G-type main-sequence star that is generating energy through hydrogen fusion in its core region. Hall et al. (2007) classify it as a low-activity variable star. The star is about five billion years old with a projected rotational velocity of 3.1 km/s. It has 1.23 times the mass of the Sun and 1.81 times the Sun's radius.

References

  1. ^ Gaia Collaboration; et al. (November 2016), "Gaia Data Release 1. Summary of the astrometric, photometric, and survey properties", Astronomy & Astrophysics, 595: 23, arXiv:1609.04172, Bibcode:2016A&A...595A...2G, doi:10.1051/0004-6361/201629512, S2CID 1828208, A2.
  2. ^ Niedzielski, A.; et al. (January 2016), "The Penn State - Toruń Centre for Astronomy Planet Search stars", Astronomy & Astrophysics, 585: 14, arXiv:1407.4956, Bibcode:2016A&A...585A..73N, doi:10.1051/0004-6361/201527362, A73.
  3. ^ Hall, Jeffrey C.; et al. (March 2007), "The Activity and Variability of the Sun and Sun-like Stars. I. Synoptic Ca II H and K Observations", The Astronomical Journal, 133 (3): 862–881, Bibcode:2007AJ....133..862H, doi:10.1086/510356.
  4. ^ "54 Cnc". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2018-02-09.
  5. Mason, Brian D.; et al. (1999), "Speckle Interferometry of New and Problem HIPPARCOS Binaries", The Astronomical Journal, 117 (4): 1890−1904, Bibcode:1999AJ....117.1890M, doi:10.1086/300823.
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