65 Arietis
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Aries |
| Right ascension | 03h 24m 26.11530s[1] |
| Declination | +20° 48′ 12.5626″[1] |
| Apparent magnitude (V) | 6.07[2] |
| Characteristics | |
| Evolutionary stage | main sequence[3] |
| Spectral type | A1 V[4] |
| B−V color index | −0.028±0.006[2] |
| Astrometry | |
| Radial velocity (Rv) | −6.2±2.3[2] km/s |
| Proper motion (μ) | RA: +0.28[5] mas/yr Dec.: −10.35[5] mas/yr |
| Parallax (π) | 9.4511 ± 0.0940 mas[1] |
| Distance | 345 ± 3 ly (106 ± 1 pc) |
| Absolute magnitude (MV) | 1.17[2] |
| Details | |
| Mass | 2.45±0.03[3] M☉ |
| Radius | 2.7[6] R☉ |
| Luminosity | 36.75[2] L☉ |
| Temperature | 10,304+71 −142[3] K |
| Rotational velocity (v sin i) | 27[3] km/s |
| Other designations | |
| Database references | |
| SIMBAD | data |
65 Arietis is a star in the northern constellation of Aries, located near Tau Arietis. 65 Arietis, abbreviated '65 Ari', is the Flamsteed designation. It has an apparent visual magnitude of 6.07,[7] which, according to the Bortle Dark-Sky Scale, means it is faintly visible to the naked eye when viewed from dark suburban skies. Based upon an annual parallax shift of 9.45±0.09 mas,[5] it is approximately 345 light-years (106 parsecs) distant from the Sun. The star is moving closer to the Earth with a heliocentric radial velocity of around −6 km/s.[2]
This is an ordinary A-type main sequence star with a stellar classification of A1 V.[4] It has about 2.45 times the mass of the Sun and shines with 40 times the Sun's luminosity. This energy is being radiated into outer space at an effective temperature of 10.300 K,[3] giving it the white-hued glow of an A-type star. It is roughly 23% of the way through its lifetime on the main sequence of core hydrogen burning stars.[3]
References
[edit]- ^ a b c 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.
- ^ a b c d e f 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.
- ^ a b c d e f Zorec, J.; Royer, F. (2012), "Rotational velocities of A-type stars. IV. Evolution of rotational velocities", Astronomy & Astrophysics, 537: A120, arXiv:1201.2052, Bibcode:2012A&A...537A.120Z, doi:10.1051/0004-6361/201117691, S2CID 55586789, A120.
- ^ a b Cowley, A.; et al. (April 1969), "A study of the bright A stars. I. A catalogue of spectral classifications", Astronomical Journal, 74: 375–406, Bibcode:1969AJ.....74..375C, doi:10.1086/110819.
- ^ a b c van Leeuwen, F. (November 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.
- ^ Pasinetti Fracassini, L. E.; et al. (February 2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS)", Astronomy and Astrophysics, 367 (2) (Third ed.): 521–524, arXiv:astro-ph/0012289, Bibcode:2001A&A...367..521P, doi:10.1051/0004-6361:20000451, S2CID 425754.
- ^ a b "65 Ari". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2012-07-18.
