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HR 7955

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(Redirected from Upsilon1 Cephei) Star in the constellation Cepheus
HR 7955
Observation data
Epoch J2000      Equinox J2000
Constellation Cepheus
Right ascension 20 45 21.12879
Declination +57° 34′ 47.0080″
Apparent magnitude (V) 4.51
Characteristics
Spectral type F8IV-V + F9IV-V
Astrometry
Radial velocity (Rv)−32.82±0.04 km/s
Proper motion (μ) RA: −62.32 mas/yr
Dec.: −236.00 mas/yr
Parallax (π)36.64 ± 0.48 mas
Distance89 ± 1 ly
(27.3 ± 0.4 pc)
Absolute magnitude (MV)2.35
Orbit
Period (P)494.16±0.58 d
Semi-major axis (a)0.065±0.001"
(≥50.2±0.5 Gm)
Eccentricity (e)0.551±0.004
Inclination (i)24.53±3.13°
Longitude of the node (Ω)325.21±1.05°
Periastron epoch (T)B 1996.335 ± 0.0017
Argument of periastron (ω)
(secondary)
68.86±0.76°
Details
HR 7955 A
Mass1.071±0.037 M
Age2.25 Gyr
HR 7955 B
Mass1.047±0.037 M
Other designations
BD+57°2240, FK5 782, GJ 9706, HD 198084, HIP 102431, HR 7955, SAO 32862
Database references
SIMBADdata

HR 7955 is a binary star system in the northern circumpolar constellation of Cepheus, near the constellation border with Cygnus. It has a yellow-white hue and is faintly visible to the naked eye with a combined apparent visual magnitude of 4.51. The system is located at a distance of 89 light-years (27.3 parsecs) from the Sun, based on parallax. It has a relatively high proper motion, traversing the celestial sphere at the rate of 0.243 arc seconds per annum, and is drifting closer to the Sun with a radial velocity of -33 km/s.

The double-lined nature of this spectroscopic binary system was not announced until 1972. It has an orbital period of 1.35 years and an eccentricity of 0.551. Both components appear to be slightly evolved stars that are leaving the main sequence and becoming subgiant stars, with stellar classifications of F8IV-V and F9IV-V. They each have slightly greater mass than the Sun: 107% and 105%, respectively. The system is about 2.25 billion years old.

References

  1. ^ 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. ^ Farrington, C. D.; et al. (2010). "Separated Fringe Packet Observations with the CHARA Array. I. Methods and New Orbits for χ Draconis, HD 184467, and HD 198084". The Astronomical Journal. 139 (6): 2308. Bibcode:2010AJ....139.2308F. doi:10.1088/0004-6256/139/6/2308. S2CID 122357261.
  3. ^ Pourbaix, D.; et al. (2004). "SB: The ninth catalogue of spectroscopic binary orbits". Astronomy and Astrophysics. 424 (2): 727–732. arXiv:astro-ph/0406573. Bibcode:2004A&A...424..727P. doi:10.1051/0004-6361:20041213. S2CID 119387088.
  4. Griffin, R. F.; Suchkov, A. A. (July 2003). "The Nature of Overluminous F Stars Observed in a Radial-Velocity Survey". The Astrophysical Journal Supplement Series. 147 (1): 103–144. Bibcode:2003ApJS..147..103G. doi:10.1086/367855.
  5. ^ Griffin, R. F. (October 1999), "Spectroscopic binary orbits from photoelectric radial velocities. Paper 148: HR 7955", The Observatory, 119: 272–283, Bibcode:1999Obs...119..272G
  6. ^ Luck, R. Earle (January 2017), "Abundances in the Local Region II: F, G, and K Dwarfs and Subgiants", The Astronomical Journal, 153 (1): 19, arXiv:1611.02897, Bibcode:2017AJ....153...21L, doi:10.3847/1538-3881/153/1/21, S2CID 119511744, 21.
  7. "HD 198084". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 6 September 2012.
  8. Lépine, Sébastien; Shara, Michael M. (March 2005). "A Catalog of Northern Stars with Annual Proper Motions Larger than 0.15" (LSPM-NORTH Catalog)". The Astronomical Journal. 129 (3): 1483–1522. arXiv:astro-ph/0412070. Bibcode:2005AJ....129.1483L. doi:10.1086/427854. S2CID 2603568.
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