Castor — Double Star in Gemini
HIP 36850; Alpha Geminorum; 66 Geminorum
About Castor
Description
Castor is one of the most remarkable multiple star systems in the sky, appearing as a single star of magnitude 1.98 in Gemini. A telescope reveals two bright components (A and B) orbiting each other, and each of those is itself a spectroscopic binary. A third, fainter eclipsing binary (C) orbits the inner pair, making Castor a sextuple star system — six stars gravitationally bound together. Located about 51 light-years from Earth.
Observing Tips
Castor is the more northerly of the twin heads in Gemini, slightly fainter and whiter than the orange Pollux below it. A small telescope at 100x easily splits the A and B components (currently about 5 arcseconds apart), revealing a lovely pair of white stars. The faint C component is visible nearby in larger telescopes. Best observed January through May.
History
Named after one of the Dioscuri twins of Greek mythology — Castor was the mortal twin, a skilled horseman, while Pollux was the immortal boxer. Despite being the fainter twin, Castor received the Alpha designation, likely because Bayer considered it the 'first' twin positionally. William Herschel studied the orbital motion of Castor A and B, helping establish that binary stars are gravitationally bound.
Fun Facts
Castor is one of the finest visual double stars in the northern sky and one of the few sextuple star systems known. All six stars are gravitationally bound, making it a remarkable celestial clockwork. The A-B pair has an orbital period of about 445 years.
Observe
1Physical Properties
2Position & Identifiers
3How easy to split?
| Telescope | Bortle 3 | Bortle 4 | Bortle 5 |
|---|---|---|---|
| 80 mm refractor 80mm refr. | Easy | Easy | Easy |
| 150 mm Newton 150mm Newt. | Easy | Easy | Easy |
| Celestron C8 (203 mm SCT) C8 203mm | Easy | Easy | Easy |
Bortle 3 = rural · 4 = outer suburbs · 5 = suburbs
4Visibility
Set a location in User Settings to see visibility data.
5Multiple Star System Sextuple D: optical
Separation over time
Apparent separation over time, computed from ORB6 orbital elements. Steep curves indicate fast-changing pairs — catch them while they're splittable.
Eyepiece View
A: 2.0 · B: 3.0 · Sep: 5.7″ · PA: 51° · N up, E right
Resolved · Rayleigh: 2.3″ · Dawes: 1.9″ · Eff: 2.3″
Explore
7
Size Comparison
8
Compare Stars
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Spectral Classification
10
Hertzsprung-Russell Diagram
11
Stellar Lifecycle
12
Blackbody Spectrum
13
Stellar Absorption Spectrum
Simulated absorption spectrum based on spectral type. Hover over lines to identify elements.
14
Stellar Fusion
Discover
15Stellar Notes
16
Light Travel Time Machine
17
Relativistic Travel
Nearby in the Sky
Other targets within a few degrees — pan your scope a little and keep exploring.
Visibility scores assume a 150 mm Newton at Bortle 4.
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