Lambda Ursae Majoris
From Wikipedia, the free encyclopedia
| Observation data Epoch J2000.0 Equinox J2000.0 |
|
|---|---|
| Constellation | Ursa Major |
| Right ascension | 10h 17m 05.8s |
| Declination | +42° 54' 52" |
| Apparent magnitude (V) | +3.45 |
| Distance | 134 ± 4 ly (41 ± 1 pc) |
| Spectral type | A2IV |
| Other designations | |
Lambda Ursae Majoris (λ UMa / λ Ursae Majoris) is a star in the constellation Ursa Major. It also has the proper names Tania Borealis (former Tania borealis[1]) meaning "the Northern (star) of Tania." The word Tania comes from the Arabic phrase (al-Qafzah) al-Thāniyah meaning "the Second (Leap)" (the distinctions "northern" (borealis) is added in Latin), and Alkafzah Borealis[citation needed]. With Mu Ursae Majoris, they were Chung Tae (中台), the Middle Dignitary, in Chinese astronomy.[2]
Lambda Ursae Majoris is a white A-type subgiant with an apparent magnitude of 3.5m. It is approximately 135 light years from the Earth.
[edit] References
- ^ Piazzi, G., The Palermo Catalogue, Palermo, 1814.
- ^ Allen, Richard Hinckley (1899). Star-Names and Their Meanings. New York: G. E. Stechert., p.443.
|
||||||||
| This subgiant star-related article is a stub. You can help Wikipedia by expanding it. |