From Wikipedia, the free encyclopedia
49 Persei
Observation data
Epoch J2000       Equinox J2000
Constellation Perseus
Right ascension 04h 08m 15.38813s [1]
Declination +37° 43′ 38.9875″ [1]
Apparent magnitude (V) 6.07 [2]
Characteristics
Spectral type K1 III [3]
B−V color index 0.943±0.003 [2]
Astrometry
Radial velocity (Rv)−44.35±0.20 [2] km/s
Proper motion (μ) RA: −98.909 [1]  mas/ yr
Dec.: −195.772 [1]  mas/ yr
Parallax (π)22.0897 ± 0.0483  mas [1]
Distance147.7 ± 0.3  ly
(45.27 ± 0.10  pc)
Absolute magnitude (MV)2.85 [2]
Details
Mass1.38 [4]  M
Radius3.72+0.10
−0.09
[1]  R
Luminosity7.95±0.03 [1]  L
Surface gravity (log g)3.45 [4]  cgs
Temperature5,028+61
−70
[1]  K
Metallicity [Fe/H]0.02±0.04 [2]  dex
Age3.93 [4]  Gyr
Other designations
40 Per, BD+37°881, HD 25975, HIP 19302, HR 1277, SAO 57000 [5]
Database references
SIMBAD data

49 Persei is a star in the northern constellation of Perseus. It is just visible to the naked eye as a dim, orange-hued star with an apparent visual magnitude of 6.09. [2] Based upon parallax measurements, this star is located around 147.7 light-years (45.27 parsecs) away from the Sun, but is drifting closer with a radial velocity of −44 km/s. [2] It has a relatively large proper motion, traversing the celestial sphere at a rate of 0.220 ·yr−1. [6]

This is an aging red giant star with a stellar classification of K1III, a star that has used up its core hydrogen and is expanding. It is a candidate horizontal branch star, which would indicate it is past the red giant branch stage and is fusing helium at its core. [7] The star is nearly four [4] billion years old with 1.4 [4] times the mass of the Sun and 3.7 [1] times the Sun's radius. It is radiating eight [1] times the luminosity of the Sun from its photosphere at an effective temperature of 5,028 K. [1]

References

  1. ^ a b c d e f g h i j k 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. ^ a b c d e f g 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. ^ Roman, Nancy G. (December 1955), "A Catalogue of High-Velocity Stars", The Astrophysical Journal Supplement Series, 2: 195, Bibcode: 1955ApJS....2..195R, doi: 10.1086/190021, ISSN  0067-0049.
  4. ^ a b c d e 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.
  5. ^ "49 Per". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-07-18.
  6. ^ 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.
  7. ^ Afșar, Melike; et al. (June 2018), "A Spectroscopic Survey of Field Red Horizontal-branch Stars", The Astronomical Journal, 155 (6): 25, arXiv: 1804.04477, Bibcode: 2018AJ....155..240A, doi: 10.3847/1538-3881/aabe86, S2CID  119336618, 240.