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Rho Geminorum (ρ Gem) is a star system that lies 59 light-years away in the constellation of Gemini, about 5 degrees west of Castor.The system consists of a primary bright enough to be seen with the naked eye, a faint secondary which has rarely been observed even professionally, and a distant, somewhat bright tertiary which requires telescopic equipment for observation.
The two red dwarfs of Castor C are almost identical, with masses around a half M ☉ and luminosities less than 10% of the Sun. [11] Since 2018 it is suspected a brown dwarf with a mass at least 49 ± 7 times the mass of Jupiter might be orbiting Castor C with a period of 50 years. If it is confirmed, Castor would turn out to be a seven-star ...
Eumnamusun_(Kalopanax_septemlobus)_blanched_prickly_castor_oil_tree_shoots.jpg (698 × 523 pixels, file size: 124 KB, MIME type: image/jpeg) This is a file from the Wikimedia Commons . Information from its description page there is shown below.
A visual band light curve for the 1979-1980 eclipse of Eta Geminorum [22] In 1865, Julius Schmidt first reported that η Geminorum was a variable star. The light variations were described by Schmidt and other observers as having long maxima of constant brightness, minima of greatly varying size and shape, and a period around 231 days. [23]
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The full size is ~2200x2300. Are you sure you are looking at that, rather than the image page? It might also be autoscaling in your browser. Debivort 17:23, 6 January 2006 (UTC) Support Scaling issues aside, I am very pleased with the direction that recent Featured Picture candidates have been going in. This image is very informative, and very ...
Gamma Geminorum (γ Geminorum, abbreviated Gamma Gem, γ Gem), formally named Alhena / æ l ˈ h iː n ə /, [13] is the third-brightest object in the constellation of Gemini. It has an apparent visual magnitude of 1.9, [ 2 ] making it easily visible to the naked eye even in urban regions .
TV Geminorum (TV Gem / HD 42475 / HR 2190) is a variable red supergiant in the constellation Gemini. Its visual magnitude varies from 6.3 to 7.5, making it very faintly visible to the naked eye of an observer with excellent observing conditions, when the star is near its peak brightness.