Theta Ursae Minoris
| |
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Ursa Minor |
Right ascension | 15h 31m 24.9s[1] |
Declination | +77° 20′ 58″[1] |
Apparent magnitude (V) | 5.00[1] |
Characteristics | |
Spectral type | K5III |
Astrometry | |
Radial velocity (Rv) | -25.30 ± 0.5 km/s |
Proper motion (μ) | RA: -47.55 ± 0.37[2] mas/yr Dec.: 5.33 ± 0.43[2] mas/yr |
Parallax (π) | 3.81 ± 0.37[2] mas |
Distance | 860 ± 80 ly (260 ± 30 pc) |
Details | |
Radius | 4.8[3] R☉ |
Luminosity | 1618[4] L☉ |
Temperature | 4053 K[4] K |
Other designations | |
Theta Ursae Minoris (θ UMi, θ Ursae Minoris) is a star in the constellation Ursa Minor. It is an orange giant of spectral type K5III with an apparent magnitude of +5.00. It is approximately 860 light years from Earth. Its diameter has been estimated as around 4.8 times that of the Sun,[3] and its luminosity approximately 1618 times that of the Sun and has a surface temperature of 4053 K.[4]
References
- 1 2 3 SIMBAD, Theta Ursae Minoris (accessed 16 June 2014)
- 1 2 3 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 Pasinetti Fracassini, L. E.; Pastori, L.; Covino, S.; Pozzi, A. (February 2001). "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS) - Third edition - Comments and statistics". Astronomy and Astrophysics. 367: 521–24. arXiv:astro-ph/0012289. Bibcode:2001A&A...367..521P. doi:10.1051/0004-6361:20000451.
- 1 2 3 McDonald, I.; Zijlstra, A. A.; Boyer, M. L. (2012). "Fundamental Parameters and Infrared Excesses of Hipparcos Stars". Monthly Notices of the Royal Astronomical Society. 427 (1): 343–57. arXiv:1208.2037. Bibcode:2012MNRAS.427..343M. doi:10.1111/j.1365-2966.2012.21873.x.
This article is issued from Wikipedia - version of the 4/20/2016. The text is available under the Creative Commons Attribution/Share Alike but additional terms may apply for the media files.