Kappa Persei
| Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
|---|---|
| Constellation | Perseus |
| Right ascension | 03h 09m 29.77156s[1] |
| Declination | +44° 51′ 27.1463″[1] |
| Apparent magnitude (V) | 3.80[2] |
| Characteristics | |
| Spectral type | G9.5 IIIb[3] |
| U−B color index | +0.83[2] |
| B−V color index | +0.98[2] |
| Astrometry | |
| Radial velocity (Rv) | 27.43±0.42[4] km/s |
| Proper motion (μ) | RA: +172.99[1] mas/yr Dec.: −143.40[1] mas/yr |
| Parallax (π) | 28.93 ± 0.21[1] mas |
| Distance | 112.7 ± 0.8 ly (34.6 ± 0.3 pc) |
| Absolute magnitude (MV) | 1.20[5] |
| Details | |
| Mass | 1.50[6] M☉ |
| Radius | 9[4] R☉ |
| Luminosity | 39.8[6] L☉ |
| Surface gravity (log g) | 2.9[4] cgs |
| Temperature | 4,857±69[6] K |
| Metallicity [Fe/H] | 0.04[4] dex |
| Rotational velocity (v sin i) | 3.0[4] km/s |
| Age | 4.58[6] Gyr |
| Database references | |
| SIMBAD | data |
Kappa Persei is a triple star system in the constellation Perseus. It is 113 light-years away from the Sun.
See also
References
- ↑ 1.0 1.1 1.2 1.3 1.4 van Leeuwen, F. (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.
- ↑ 2.0 2.1 2.2 Mermilliod, J.-C. (1986), "Compilation of Eggen's UBV data, transformed to UBV (unpublished)", Catalogue of Eggen's UBV Data, SIMBAD, Bibcode:1986EgUBV........0M.
- ↑ 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.
- ↑ 4.0 4.1 4.2 4.3 4.4 Massarotti, Alessandro; et al. (January 2008), "Rotational and Radial Velocities for a Sample of 761 HIPPARCOS Giants and the Role of Binarity", The Astronomical Journal, 135 (1): 209–231, Bibcode:2008AJ....135..209M, doi:10.1088/0004-6256/135/1/209.
- ↑ 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.
- ↑ 6.0 6.1 6.2 6.3 Luck, R. Earle (2015), "Abundances in the Local Region. I. G and K Giants", Astronomical Journal, 150 (3), 88, arXiv:1507.01466, Bibcode:2015AJ....150...88L, doi:10.1088/0004-6256/150/3/88, S2CID 118505114.
Content Disclaimer
Informasi ini disarikan dari Wikipedia dan disajikan kembali untuk tujuan edukasi. Konten tersedia di bawah lisensi CC BY-SA 3.0. Kami tidak bertanggung jawab atas ketidakakuratan data yang bersumber dari kontribusi publik tersebut.
- The information displayed on this website is sourced in part or in whole from Wikipedia and has been adapted for the purpose of restating it. We strive to provide accurate and relevant information, however:
- There is no guarantee of absolute accuracy. Wikipedia is an open, collaborative project that can be edited by anyone, so information is subject to change.
- It is not intended to constitute professional advice. The content displayed is for informational and educational purposes only. For important decisions (e.g., medical, legal, or financial), please consult a professional.
- Content copyright. Wikipedia is licensed under the Creative Commons Attribution-ShareAlike License (CC BY-SA). This means that content may be reused with appropriate attribution and shared under a similar license.
- Responsible use. Any risk arising from the use of information from this website is entirely the responsibility of the user.