
25 Canum Venaticorum
Constellation, Canes Venatici, Binary star, Apparent magnitude, Light-year, Stellar classification
Herausgegeben: Christer, Emory
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Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. 25 Canum Venaticorum is a binary star in the constellation Canes Venatici. It has a combined apparent magnitude of +4.82 and is approximately 192 light years from Earth. The primary component, 25 Canum Venaticorum A, is a white A-type giant with an apparent magnitude of +5.01. The companion, 25 Canum Venaticorum B, is a yellow-white F-type main sequence dwarf with an apparent magnitude of +6.91. The two stars are separated by 1.8 arcseconds on the sky and have an orbi...
Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. 25 Canum Venaticorum is a binary star in the constellation Canes Venatici. It has a combined apparent magnitude of +4.82 and is approximately 192 light years from Earth. The primary component, 25 Canum Venaticorum A, is a white A-type giant with an apparent magnitude of +5.01. The companion, 25 Canum Venaticorum B, is a yellow-white F-type main sequence dwarf with an apparent magnitude of +6.91. The two stars are separated by 1.8 arcseconds on the sky and have an orbital period of 220 years.