Zeta Ursae Minoris
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Ursa Minor |
Right ascension | 15h 44m 03.51892s[1] |
Declination | +77° 47′ 40.1788″[1] |
Apparent magnitude (V) | +4.29[2] |
Characteristics | |
Spectral type | A3Vn[3] |
U−B color index | +0.05[4] |
B−V color index | 0.038±0.005[2] |
Variable type | Suspected δ Sct[5] |
Absolute magnitude (MV) | −0.98[2] |
Details | |
Myr | |
Database references | |
SIMBAD | data |
Zeta Ursae Minoris, which is
apparent visual magnitude of +4.28. It is located at a distance of approximately 369 light-years from the Sun based on parallax,[1] but is drifting further closer with a radial velocity of about –13 km/s.[6]
The
projected rotational velocity of 210 km/s, which is creating an equatorial bulge that is estimated to be 10% larger than the polar radius.[9]
Zeta Ursae Minoris is about 180circumstellar disk.[10] A black body fit to the data yields a mean dust temperature of 160 K and an orbital radius of 42.5 AU.[8]
In some Arabic star charts it is listed as أخفى الفرقدين ʼakhfā al-farqadayn, meaning "the dimmer of the two calves", and paired with
β UMi, respectively, the brighter two stars in the rectangle of Ursa Minor.[15]
References
- ^ S2CID 18759600.
- ^ S2CID 119257644.
- ^ doi:10.1086/110819.
- Bibcode:1966CoLPL...4...99J.
- ^ Bibcode:1970IBVS..427....1F.
- ^ S2CID 119231169.
- ^ a b Kaler, James B. "Alifa al Farkadain". Stars. University of Illinois. Retrieved 21 June 2014.
- ^ S2CID 118438871. 15.
- ^ S2CID 119273474.
- ^ S2CID 14116473.
- ^ "zet UMi". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2021-01-08.
- S2CID 14878976.
- ISBN 9781139493680.
- ^ a b "zet UMi". The International Variable Star Index. AAVSO. Retrieved 16 October 2022.
- ^ Allen, Richard Hinckley (1899). Star-names and Their Meanings. G. E. Stechert. pp. 447–460.