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64 Andromedae

From Wikipedia, the free encyclopedia
G-type giant star in the constellation Andromeda
64 Andromedae
Location of 64 Andromedae (circled)
Observation data
Epoch J2000      Equinox J2000
ConstellationAndromeda
Right ascension02h 24m 24.91594s[1]
Declination+50° 00′ 23.5619″[1]
Apparent magnitude (V)5.19[2]
Characteristics
Spectral typeG8III[2]
U−Bcolor index1.74[2]
B−Vcolor index0.976[3]
Astrometry
Radial velocity (Rv)–13.34[1] km/s
Proper motion (μ)RA: +24.618±0.272[1]mas/yr
Dec.: −36.335±0.262[1]mas/yr
Parallax (π)7.7770±0.1296 mas[1]
Distance419 ± 7 ly
(129 ± 2 pc)
Absolute magnitude (MV)−0.25[4]
Details
Mass3.12±0.19[5] M
Radius15.90±0.56[5] R
Luminosity135.6±8.8[5] L
Surface gravity (log g)2.55±0.05[5] cgs
Temperature4,944±33[5] K
Metallicity[Fe/H]−0.03±0.10[5] dex
Rotational velocity (v sin i)0.69[3] km/s
Age350±60[5] Myr
Other designations
64 And,BD+49°649,HD 14770,HIP 11220,HR 694,SAO 38005,PPM 27578[2]
Database references
SIMBADdata

64 Andromedae, abbreviated64 And, is a single[6]star in the northernconstellation ofAndromeda. With aspectral type G8III, it is a deep-yellow colouredG-typegiant approximately 419light years fromEarth with anapparent magnitude of 5.19.[1] The star is moving closer to the Earth with a heliocentricradial velocity of –13 km/s.[1]

This star is estimated to be 350[5] million years old with a negligible rotation rate, showing aprojected rotational velocity of 0.69 km/s.[3] It has a little more than 3[5] times themass of the Sun and has expanded to 16[5] times theSun's radius. 64 And is radiating 136[5] times theluminosity of the Sun from its enlargerphotosphere at aneffective temperature of 4,944 [5]

Position and chosen constellation

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As to the faint triangle and context in which the star figures see63 Andromedae.

References

[edit]
  1. ^abcdefghBrown, 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.
  2. ^abcd"64 And".SIMBAD.Centre de données astronomiques de Strasbourg. RetrievedOctober 5, 2018.
  3. ^abcHekker, S.; Meléndez, J. (December 2007), "Precise radial velocities of giant stars. III. Spectroscopic stellar parameters",Astronomy & Astrophysics,475 (3):1003–1009,arXiv:0709.1145,Bibcode:2007A&A...475.1003H,doi:10.1051/0004-6361:20078233,S2CID 10436552.
  4. ^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.
  5. ^abcdefghijklReffert, S.; Bergmann, C.; Quirrenbach, A.; Trifonov, T.; Künstler, A. (2016), "Precise radial velocities of giant stars. VII. Occurrence rate of giant extrasolar planets as a function of mass and metallicity",Astronomy & Astrophysics,574: 13,arXiv:1608.00963,Bibcode:2015A&A...574A.116R,doi:10.1051/0004-6361/201322360,hdl:10722/215277,S2CID 59334290, A116.
  6. ^Eggleton, P. P.; Tokovinin, A. A. (September 2008), "A catalogue of multiplicity among bright stellar systems",Monthly Notices of the Royal Astronomical Society,389 (2):869–879,arXiv:0806.2878,Bibcode:2008MNRAS.389..869E,doi:10.1111/j.1365-2966.2008.13596.x,S2CID 14878976.
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