Alpha Ursae Majoris
| Observation data Epoch J2000 Equinox J2000 |
|
|---|---|
| Constellation | Ursa Major |
| Right ascension | 11h 03m 43.67152s[1] |
| Declination | +61° 45′ 03.7249″[1] |
| Apparent magnitude (V) | 1.79[2] |
| Characteristics | |
| Spectral type | K1 II-III[3] / F0 V[3] |
| U−B color index | +0.93[2] |
| B−V color index | +1.07[2] |
| Variable type | Pulsating |
| Astrometry | |
| Radial velocity (Rv) | –9[4] km/s |
| Proper motion (μ) | RA: –134.11[1] mas/yr Dec.: –34.70[1] mas/yr |
| Parallax (π) | 26.54 ± 0.48[1] mas |
| Distance | 123 ± 2 ly (37.7 ± 0.7 pc) |
| Absolute magnitude (MV) | –1.10 ± 0.04 |
| Orbit[citation needed] | |
| Companion | α UMa B |
| Period (P) | 44.4 yr |
| Semimajor axis (a) | 0.603" |
| Eccentricity (e) | 0.4 |
| Inclination (i) | 152° |
| Longitude of the node (Ω) | 2000° |
| Periastron epoch (T) | 1956.8 |
| Details | |
| Surface gravity (log g) | 2.46[5]/— |
| Temperature | 4,660[5]/— K |
| Metallicity [Fe/H] | –0.20 ± 0.07[5] dex |
| Rotational velocity (v sin i) | 2.6 ± 1.0[6]/— km/s |
| Other designations | |
| Database references | |
| SIMBAD | data |
Alpha Ursae Majoris (α UMa, α Ursae Majoris) is the second-brightest star in the constellation of Ursa Major (despite its Bayer designation of "alpha"). It has the traditional name Dubhe, and a rarer name Ak. The traditional name comes from the Arabic for "bear", dubb, from the phrase ظهر الدب الاكبر żahr ad-dubb al-akbar "the back of the Greater Bear". In Chinese it is known as 北斗一 (the First Star of the Northern Dipper) or 天樞 (the Celestial Pivot).
This star forms part of the Big Dipper (also known as the Plough or the Great Bear), and is the northern of the 'pointers' (or 'guards'), the two stars of Ursa Major which point towards Polaris, the North Star. Dubhe is about 123 light years away and is a giant star that has evolved away from the main sequence after consuming the hydrogen at its core. It is a spectroscopic binary with a main sequence companion α UMa B that has a stellar classification of F0V. This star orbiting at a mean separation of about 23 astronomical units (AU) and completes an orbit every 44.4 years. More than 90,000 AU distant from this pair is a second binary system that includes an F-type star, making this a four star system.[8]
Although it is part of the constellation of Ursa Major, it does not form part of the Ursa Major Moving Group of stars that have a common motion through space.[citation needed]
[edit] In culture
Dubhe is the official star of the State of Utah. USS Dubhe (ID-2562) was a ship in the United States navy.
[edit] References
- ^ a b c d e van Leeuwen, F. (November 2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics 474 (2): 653–664. Bibcode 2007A&A...474..653V. doi:10.1051/0004-6361:20078357.
- ^ a b c Johnson, H. L. et al. (1966), "UBVRIJKL photometry of the bright stars", Communications of the Lunar and Planetary Laboratory 4 (99), Bibcode 1966CoLPL...4...99J
- ^ a b Edwards, T. W. (April 1976), "MK classification for visual binary components", Astronomical Journal 81: 245–249, Bibcode 1976AJ.....81..245E, doi:10.1086/111879
- ^ Wilson, Ralph Elmer (1953), General catalogue of stellar radial velocities, Carnegie Institution of Washington, Bibcode 1953QB901.W495.....
- ^ a b c McWilliam, Andrew (December 1990), "High-resolution spectroscopic survey of 671 GK giants. I - Stellar atmosphere parameters and abundances", Astrophysical Journal Supplement Series 74: 1075–1128, Bibcode 1990ApJS...74.1075M, doi:10.1086/191527
- ^ Carney, Bruce W. et al. (March 2008), "Rotation and Macroturbulence in Metal-Poor Field Red Giant and Red Horizontal Branch Stars", The Astronomical Journal 135 (3): 892–906, Bibcode 2008AJ....135..892C, doi:10.1088/0004-6256/135/3/892
- ^ "DUBHE -- Spectroscopic binary", SIMBAD (Centre de Données astronomiques de Strasbourg), http://simbad.u-strasbg.fr/simbad/sim-id?Ident=Alpha+Ursae+Majoris, retrieved 2011-12-23
- ^ Kaler, James B., "DUBHE (Alpha Ursae Majoris)", Stars (University of Illinois), http://stars.astro.illinois.edu/sow/dubhe.html, retrieved 2011-12-23