Observation data Epoch J2000 Equinox J2000 | |
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Constellation | Aries |
Right ascension | 02 48 32.08864 |
Declination | +18° 17′ 01.6491″ |
Apparent magnitude (V) | 5.82 |
Characteristics | |
Spectral type | K1 III |
U−B color index | 1.13 |
B−V color index | +1.20 |
R−I color index | 0.44 |
Variable type | suspected |
Astrometry | |
Radial velocity (Rv) | +47.1 km/s |
Proper motion (μ) | RA: +41.250 mas/yr Dec.: −32.585 mas/yr |
Parallax (π) | 7.3266 ± 0.1215 mas |
Distance | 445 ± 7 ly (136 ± 2 pc) |
Absolute magnitude (MV) | 0.09 |
Details | |
Mass | 1.60±0.48 M☉ |
Radius | 19.74+0.29 −0.96 R☉ |
Luminosity | 127.98±2.52 L☉ |
Surface gravity (log g) | 2.09±0.11 cgs |
Temperature | 4,473±92 K |
Metallicity | −0.21±0.05 dex |
Age | 2.63+1.00 −0.72 Gyr |
Other designations | |
40 Ari, NSV 937, BD+17°442, GC 3369, HD 17459, HIP 13108, HR 828, SAO 93118 | |
Database references | |
SIMBAD | data |
40 Arietis is a probable binary star system in the northern constellation of Aries. 40 Arietis is the Flamsteed designation. Their combined apparent magnitude is 5.82, putting the system near the limit of naked eye visibility. Based upon an annual parallax shift of just 7.33 mas, it is 445 light-years (136 parsecs) away from the Sun. At that distance, its brightness is diminished by 0.21 in magnitude from extinction caused by interstellar gas and dust.
This is a suspected spectroscopic binary with an angular separation of 0.2″ between the two components. The visible component is an evolved giant star with a stellar classification of K1 III. It is a suspected variable star of unknown type, and is around 2.6 billion years old with 1.6 times the mass of the Sun. With the supply of hydrogen at its core exhausted, the star has expanded to 20 times the Sun's radius. It is radiating 128 times the luminosity of the Sun from its swollen photosphere at an effective temperature of 4,473 K.
References
- ^ 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.
- ^ Nicolet, B. (1978), "Photoelectric photometric Catalogue of homogeneous measurements in the UBV System", Astronomy and Astrophysics Supplement Series, 34: 1–49, Bibcode:1978A&AS...34....1N.
- ^ 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.
- ^ Samus, N. N.; et al. (2017), "General Catalogue of Variable Stars", Astronomy Reports, 5.1, 61 (1): 80–88, Bibcode:2017ARep...61...80S, doi:10.1134/S1063772917010085, S2CID 125853869.
- Wilson, Ralph Elmer (1953), "General Catalogue of Stellar Radial Velocities", Carnegie Institute Washington D.C. Publication, Washington: Carnegie Institution of Washington, Bibcode:1953GCRV..C......0W.
- 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.
- ^ Feuillet, Diane K.; et al. (2016), "Determining Ages of APOGEE Giants with Known Distances", The Astrophysical Journal, 817 (1): 40, arXiv:1511.04088, Bibcode:2016ApJ...817...40F, doi:10.3847/0004-637X/817/1/40, S2CID 118675933.
- "40 Ari". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2012-07-18.
- Famaey, B.; et al. (January 2005), "Local kinematics of K and M giants from CORAVEL/Hipparcos/Tycho-2 data. Revisiting the concept of superclusters", Astronomy and Astrophysics, 430 (1): 165–186, arXiv:astro-ph/0409579, Bibcode:2005A&A...430..165F, doi:10.1051/0004-6361:20041272, S2CID 17804304.
External links
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