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- Zeta Canis Majoris, or ζ Canis Majoris, also named Furud /ˈfjʊərəd/, is a binary star system in the southern constellation of Canis Major. This system...14 KB (1,116 words) - 09:41, 6 January 2024
- 2013). "Eta Canis Majoris". AAVSO Website. American Association of Variable Star Observers. Retrieved 5 February 2014. "Zeta Canis Majoris – Cepheid Variable"...59 KB (6,873 words) - 16:08, 17 July 2024
- stars in the known universe Murzim (Beta Canis Majoris) Muliphen (Gamma CMa) Wezen (Delta CMa) Adhara (Epsilon CMa) Furud (Zeta CMa) Aludra (Eta CMa)....498 bytes (98 words) - 13:42, 24 November 2021
- the direction opposite of the solar apex, is located near the star Zeta Canis Majoris. Animations of star motions around apex and antapex The movement of...8 KB (908 words) - 02:52, 17 July 2024
- lion's mane) الضفيرة الْضَّفِيرَة Zeta Leonis Adhara al-ʽAdhārā the Virgin / Nymph العذارى الْعَذَارَى Epsilon Canis Majoris A Adhil adh-Dhayl the Tail / Annex...35 KB (572 words) - 04:47, 2 July 2024
- Psi Ursae Majoris Star 3.01 Gamma Gruis Star 3.01 Beta Capricorni Quintuple star system 3.02 2.97 Omicron2 Canis Majoris Star 3.03 2.88 Zeta Tauri Binary...37 KB (1,546 words) - 21:08, 17 March 2024
- supergiant Eta Canis Majoris, a blue supergiant of spectral type B5Ia UW Canis Majoris (UW CMa), two blue (O-type) supergiants in a binary system Zeta Puppis...20 KB (2,390 words) - 23:42, 16 July 2024
- known stars: Mu Cephei VV Cephei A NML Cygni RW Cephei S Persei VY Canis Majoris - potentially the largest star in the Milky Way KY Cygni PZ Cassiopeiae...39 KB (4,440 words) - 17:10, 1 June 2024
- sometimes used for the most extended and unstable red supergiants like VY Canis Majoris and NML Cygni. The "red" part of "red supergiant" refers to the cool...33 KB (4,223 words) - 01:57, 17 July 2024
- IAU-approved Star Names. (The historical form Furud was chosen for Zeta Canis Majoris.) In Chinese, 孫 (Sūn), meaning Grandson, refers to an asterism consisting...10 KB (807 words) - 05:49, 27 March 2022
- 20 ly. Spectral standards: F0IIIa – Zeta Leonis F0Ib – Alpha Leporis F1V - 37 Ursae Majoris F2V – 78 Ursae Majoris F7V - Iota Piscium F9V - Beta Virginis...104 KB (11,345 words) - 02:10, 20 July 2024
- 7s Crux 321 B0.5IV+B1V Zeta Ophiuchi 16h 37m 09.54s –10° 34′ 01.5″ Ophiuchus 366 O9.5V Adhara 06h 58m 37.6s –28° 58′ 19″ Canis Major 430±30 B2 II Betelgeuse...34 KB (2,399 words) - 23:04, 16 July 2024
- 4 visibly bright O-type stars are Gamma Velorum, Alnitak (Zeta Orionis), Mintaka (Delta Orionis), and Zeta Puppis. The corona present in other spectral types...30 KB (3,350 words) - 09:26, 22 April 2024
- disks and increase in brightness are known as shell events. 27 Canis Majoris Beta Canis Minoris Pleione Labadie-Bartz, Jonathan; Baade, Dietrich; Carciofi...10 KB (821 words) - 20:00, 16 July 2024
- VV Cephei (redirect from Zeta Aurigae star)accretion disc around the hot secondary. Stellar classification VY Canis Majoris List of largest known stars Van Leeuwen, F. (2007). "Validation of the...26 KB (2,675 words) - 22:59, 28 June 2024
- Current distance Current magnitude Epsilon Canis Majoris ... −4,460,000 −4,700,000 −3.99 34 430 1.50 Beta Canis Majoris −4,460,000 −3,700,000 −4,420,000 −3.65...6 KB (488 words) - 17:20, 14 July 2024
- Cygni — suddenly brightened in the 17th century WNC4 — Messier Object 40 Zeta Boötis — speckle binary test system Lists of astronomical objects Astronomical...5 KB (518 words) - 03:59, 28 June 2024
- was computed in 1827, when Félix Savary computed the orbit of Xi Ursae Majoris. Over the years, many more double stars have been catalogued and measured...67 KB (8,092 words) - 18:30, 16 July 2024
- Size comparison of some well-known supergiant and hypergiant stars, featuring Cygnus OB2-12, V382 Carinae, Betelgeuse, VV Cephei, and VY Canis Majoris...146 KB (16,331 words) - 03:00, 17 July 2024
- Silva, L.; Porto de Mello, G. F. (2000-06-01). "zeta 1 and zeta 2 Reticuli and the existence of the zeta Herculis group". Astronomy and Astrophysics. 358:...161 KB (13,298 words) - 22:28, 16 July 2024
- invicem alligantur.) Ex parte Joannis Mori patris Uxor Johannis Clements: (zetas hujus Domine videtur interiisse:) et Elz. Danceta Tho. Mori filia A®°. 21
- was based on the star Vega, or α Lyrae. The brightest star Sirius (α Canis Majoris) has a magnitude of −1.46. The limiting magnitude for a typical person's