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Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Cassiopeia |
Right ascension | 01 43 40.72450 |
Declination | +63° 49′ 24.2390″ |
Apparent magnitude (V) | 8.40 |
Characteristics | |
Spectral type | K5 Vbe |
U−B color index | +1.12 |
B−V color index | +1.22 |
Astrometry | |
Radial velocity (Rv) | −50.827 ± 0.0075 km/s |
Proper motion (μ) | RA: −394.73 mas/yr Dec.: −582.26 mas/yr |
Parallax (π) | 73.65 ± 0.98 mas |
Distance | 44.3 ± 0.6 ly (13.6 ± 0.2 pc) |
Details | |
Mass | 0.624 M☉ |
Radius | 0.59 R☉ |
Surface gravity (log g) | 4.70 cgs |
Temperature | 4312 K |
Metallicity | −0.39 dex |
Age | 6.89 ± 4.70 Gyr |
Other designations | |
BD+63° 229, GJ 69, HD 10436, HIP 8070, SAO 11943, LHS 1291. | |
Database references | |
SIMBAD | data |
ARICNS | data |
Gliese 69 is a star located in the constellation of Cassiopeia. It has an apparent magnitude of 8.40. Parallax measurements by Hipparcos put it at a distance of 44.3 light-years (13.6 parsecs) away.
Gliese 69 is a K-type main-sequence star that is smaller and less massive than the Sun. It glows with an effective temperature of 4,312 K. It is around 6.9 billion years old, significantly older than the Sun. Gliese 69 is also known by its designations HD 10436 and LHS 1291.
Planetary System
In 2019 one candidate planet been detected by the radial velocity method.
Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
b | 8.3+3.7 −3.2 M🜨 |
0.043±0.004 | 3.84237+0.00085 −0.00054 |
0.03+0.20 −0.03 |
— | — |
References
- ^ van Leeuwen, F.; et al. (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.
- ^ Keenan, Philip C.; McNeil, Raymond C. (1989). "The Perkins catalog of revised MK types for the cooler stars". Astrophysical Journal Supplement Series. 71: 245. Bibcode:1989ApJS...71..245K. doi:10.1086/191373.
- ^ Mermilliod, J.-C. (1986). "Compilation of Eggen's UBV data, transformed to UBV (unpublished)". Catalogue of Eggen's UBV Data. Bibcode:1986EgUBV........0M.
- Soubiran, C.; Jasniewicz, G.; Chemin, L.; Crifo, F.; Udry, S.; Hestroffer, D.; Katz, D. (2013). "The catalogue of radial velocity standard stars for Gaia. I. Pre-launch release". Astronomy & Astrophysics. 552: A64. arXiv:1302.1905. Bibcode:2013A&A...552A..64S. doi:10.1051/0004-6361/201220927. S2CID 56094559.
- ^ Takeda, Genya; Ford, Eric B.; Sills, Alison; Rasio, Frederic A.; Fischer, Debra A.; Valenti, Jeff A. (February 2007). "Structure and Evolution of Nearby Stars with Planets. II. Physical Properties of ~1000 Cool Stars from the SPOCS Catalog". The Astrophysical Journal Supplement Series. 168 (2): 297–318. arXiv:astro-ph/0607235. Bibcode:2007ApJS..168..297T. doi:10.1086/509763. S2CID 18775378.
- ^ Pace, G. (March 2013). "Chromospheric activity as age indicator. An L-shaped chromospheric-activity versus age diagram". Astronomy & Astrophysics. 551: 4. arXiv:1301.5651. Bibcode:2013A&A...551L...8P. doi:10.1051/0004-6361/201220364. S2CID 56420519. L8.
- ^ "HD 10436". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 22 September 2017.
- Barnes, J. R.; et al. (2019-06-11). "Frequency of planets orbiting M dwarfs in the Solar neighbourhood". arXiv:1906.04644v1. Bibcode:2019arXiv190604644T.
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