Castor (Alpha Geminorum)
A modest telescope shows two similar A stars, of mid-second and mid-third magnitude, a couple of arcseconds apart, which orbit each other every 380 years. About 1 arc-minute to the south lies a ninth magnitude third companion that orbits the bright pair at a distance of about 1,000 AU. A spectrograph shows that each of the two bright components, A and B, is itself a double. Castor A consists of almost identical stars, each of about 2 solar masses, orbiting each other every 9.22 days and about one-tenth the distance of Mercury from the Sun. Castor B's twin stars orbit even faster, making their circuit in a mere 2.9 days. The faint, distant star, Castor C, is also double, consisting of nearly identical, low-mass M stars – red dwarfs – with temperatures of about 4,000K, some two solar diameters apart with an orbital period of 20 hours. One or both are flare stars. Castor is part of a group of widely dispersed stars known as the Castor Moving Group.
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