Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

HR 7955

From Wikipedia, the free encyclopedia
Star in the constellation Cepheus
HR 7955
Observation data
EpochJ2000      EquinoxJ2000
ConstellationCepheus
Right ascension20h 45m 21.12879s[1]
Declination+57° 34′ 47.0080″[1]
Apparent magnitude (V)4.51[2]
Characteristics
Spectral typeF8IV-V + F9IV-V[2]
Astrometry
Radial velocity (Rv)−32.82±0.04[3] km/s
Proper motion (μ)RA: −62.32[1]mas/yr
Dec.: −236.00[1]mas/yr
Parallax (π)36.64±0.48 mas[1]
Distance89 ± 1 ly
(27.3 ± 0.4 pc)
Absolute magnitude (MV)2.35[4]
Orbit[2]
Period (P)494.16±0.58 d
Semi-major axis (a)0.065±0.001"
(≥50.2±0.5 Gm[5])
Eccentricity (e)0.551±0.004
Inclination (i)24.53±3.13°
Longitude of the node (Ω)325.21±1.05°
Periastronepoch (T)B 1996.335 ± 0.0017
Argument of periastron (ω)
(secondary)
68.86±0.76°
Details[2]
HR 7955 A
Mass1.071±0.037 M
Age2.25[6] 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[7]
Database references
SIMBADdata

HR 7955 is abinary star[2] system in the northerncircumpolar constellation ofCepheus, near the constellation border withCygnus. It has a yellow-white hue and is faintly visible to the naked eye with a combinedapparent visual magnitude of 4.51.[2] The system is located at a distance of 89 light-years (27.3 parsecs) from theSun, based onparallax.[1] It has a relatively highproper motion, traversing thecelestial sphere at the rate of 0.243 arc seconds per annum,[8] and is drifting closer to the Sun with aradial velocity of -33 km/s.[3]

The double-lined nature of thisspectroscopic binary system was not announced until 1972.[5] It has anorbital period of 1.35 years and aneccentricity of 0.551.[2] Both components appear to be slightlyevolved stars that are leaving themain sequence and becomingsubgiant stars, withstellar classifications of F8IV-V and F9IV-V. They each have slightly greater mass than the Sun: 107% and 105%, respectively.[2] The system is about 2.25 billion years old.[6]

References

[edit]
  1. ^abcdefvan 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. ^abcdefghFarrington, 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. ^abPourbaix, D.; et al. (2004). "SB9: 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. ^abGriffin, 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. ^abLuck, 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. Retrieved6 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.
Stars
Bayer
Flamsteed
Variable
HR
HD
Other
Exoplanets
Star
clusters
NGC
Other
Nebulae
NGC
Other
Galaxies
NGC
Other
Retrieved from "https://en.wikipedia.org/w/index.php?title=HR_7955&oldid=1187421054"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2025 Movatter.jp