Ross 695
| Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
|---|---|
| Constellation | Corvus |
| Right ascension | 12h 24m 52.50278 s[1] |
| Declination | −18° 14′ 32.2435″[1] |
| Apparent magnitude (V) | 11.272 |
| Characteristics | |
| Spectral type | M2.5 |
| Astrometry | |
| Proper motion (μ) | RA: 1095.66 ± 2.14[1] mas/yr Dec.: -2308.56 ± 1.38[1] mas/yr |
| Parallax (π) | 112.98 ± 2.51[1] mas |
| Distance | 28.9 ± 0.6 ly (8.9 ± 0.2 pc) |
| Details | |
| Mass | 0.23[2] M☉ |
| Radius | 0.24[2] R☉ |
| Luminosity | 0.007[2] L☉ |
| Temperature | 3403 ± 69[2] K |
| Metallicity [Fe/H] | −0.33 ± 0.09[2] dex |
| Other designations | |
LHS 45, Ross 695, Gliese 465, HIP 60559 | |
Ross 695, also known as Gliese 465, is a red dwarf star in the constellation Corvus. At apparent magnitude 11.27, it is much too faint to be seen with the unaided eye. A small star, it has around 23% the mass and radius of the Sun, but only 0.7% its luminosity.[2]
References
- 1 2 3 4 5 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. - 1 2 3 4 5 6 Maldonado, J.; Affer, L.; Micela, G.; Scandariato, G.; Damasso, M.; Stelzer, B.; Barbieri, M.; Bedin, L. R.; Biazzo, K.; Bignamini, A.; Borsa, F.; Claudi, R. U.; Covino, E.; Desidera, S.; Esposito, M.; Gratton, R.; González Hernández, J. I.; Lanza, A. F.; Maggio, A.; Molinari, E.; Pagano, I.; Perger, M.; Pillitteri, I.; Piotto, G.; Poretti, E.; Prisinzano, L.; Rebolo, R.; Ribas, I.; Shkolnik, E.; Southworth, J.; Sozzetti, A.; Suárez Mascareño, A. (2015). "Stellar parameters of early-M dwarfs from ratios of spectral features at optical wavelengths". Astronomy & Astrophysics. 577: 13. arXiv:1503.03010. Bibcode:2015A&A...577A.132M. doi:10.1051/0004-6361/201525797. A132.
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