|This article relies largely or entirely upon a single source. (January 2009)|
Epoch J2000.0 Equinox J2000.0
|Apparent magnitude (V)||+6.1/+6.74|
|Distance||137 ± 45 ly
(42 ± 14 pc)
Both components are white A-type main sequence dwarfs The primary, ο Capricorni A, sometimes called ο¹ Capricorni, has an apparent magnitude of +5.94, while the companion, ο Capricorni B or ο² Capricorni, has an apparent magnitude of +6.74. The two stars are currently separated by 21.9 arcseconds.
- Harvard College Observatory (1941). Sky and Telescope. Stanford University.
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