exoplanet designated Omicron Ursae Majoris Ab was found to be orbiting the primary. ο Ursae Majoris (Latinised to Omicron Ursae Majoris) is the star's Bayer... 15 KB (1,418 words) - 15:02, 25 December 2023 |
Althiba V, σ2 as Althiba VI, and d as Althiba VII. 47 Ursae Majoris Omicron Ursae Majoris Pi Ursae Majoris van Leeuwen, F. (November 2007), "Validation of the... 11 KB (811 words) - 12:52, 9 May 2024 |
Suspected variable star 3.45 Lambda Ursae Majoris Star 3.45 Eta Ceti Star 3.466 Epsilon Gruis Star 3.47 3.41 Sigma Canis Majoris Star 3.47 Gamma Sagittae Star... 37 KB (1,546 words) - 21:08, 17 March 2024 |
 | asterism consisting of ω Ursae Majoris, 57 Ursae Majoris, 47 Ursae Majoris, 58 Ursae Majoris, 49 Ursae Majoris and 56 Ursae Majoris. Consequently, the Chinese... 10 KB (687 words) - 11:58, 14 May 2023 |
4.8 microlensing 13110 1.06 Omicron Coronae Borealis b 1.5 187.83 0.83 radial vel. 274.1 2.13 4749 Omicron Ursae Majoris b 4.1 1630 3.9 radial vel. 183... 69 KB (4,155 words) - 14:07, 28 April 2024 |
Zeta Ceti Beid Bayḍ Eggs بيض Omicron¹ Eridani Benetnash Banāt un-Naʿash Daughters of the bier بنات النعش Eta Ursae Majoris see also Alkaid Betelgeuse yad... 33 KB (565 words) - 08:42, 19 April 2024 |
MT Tauri G5 V 16.8 Photography ΔU = 0.7 mag ~ 10 min EU ~ 1035 Pi1 Ursae Majoris G1.5 Vb 5.64 X-ray LX = 1029 erg/s >~ 35 min EX = 2 × 1033 S Fornacis... 55 KB (7,591 words) - 11:59, 23 March 2024 |
 | Variable star (section W Ursae Majoris variables) standstills are seen, part way between maximum and minimum brightness. SU Ursae Majoris stars, which undergo both frequent small outbursts, and rarer but larger... 50 KB (6,468 words) - 06:01, 22 April 2024 |
 | orbit each other roughly every 8.5 to 10 hours. It belongs to the UX Ursae Majoris subgroup of cataclysmic variable star systems, where material from the... 38 KB (4,129 words) - 21:08, 30 April 2024 |
Double-Lined Spectroscopic Binaries. IX. HD 54371, HR 2692, and 16 Ursa Majoris", The Astronomical Journal, 149 (2): 13, Bibcode:2015AJ....149...63F, doi:10... 31 KB (1,429 words) - 22:25, 25 April 2024 |
 | into one of the traditional classes, with features of Beta Lyrae, W Ursae Majoris, and cataclysmic variables. It may be a representative of a very brief... 67 KB (7,533 words) - 05:18, 11 May 2024 |
 | 2007). "Long-Period Objects in the Extrasolar Planetary Systems 47 Ursae Majoris and 14 Herculis". The Astrophysical Journal. 654 (1): 625–632. arXiv:astro-ph/0609117... 37 KB (3,928 words) - 14:30, 8 May 2024 |
 | Located 3° northeast of Gamma is the VW Hydri, a dwarf nova of the SU Ursae Majoris type. It is a close binary system that consists of a white dwarf and... 29 KB (3,095 words) - 21:09, 30 April 2024 |
 | stable celestial clock. SX Leonis Minoris is a dwarf nova of the SU Ursae Majoris type that was identified in 1994. It consists of a white dwarf and a... 40 KB (3,840 words) - 03:26, 16 March 2024 |
 | Mskegwǒm, the den of the celestial bear (Alpha, Beta, Gamma and Delta Ursae Majoris). Polynesian peoples often recognized Corona Borealis; the people of... 55 KB (6,365 words) - 11:55, 6 May 2024 |
 | range of 0.6 magnitudes; its orbital period is 6.4 hours. It is a W Ursae Majoris variable that ranges in magnitude from a minimum of 7.1 to a maximum... 73 KB (8,385 words) - 12:58, 20 March 2024 |
Kappa Ursae Majoris Alkaphrah 上台二 Shàng Tái èr The Second Upper Step Lambda Ursae Majoris Tania Borealis 中台一 Zhōng Tái yī The First Middle Step Mu Ursae Majoris... 185 KB (2,182 words) - 08:18, 30 April 2024 |