Magnitude 4.82 | Constellation Canes Venatici | |
Similar NGC 4534, I Zw 36, NGC 4145, NGC 5112 | ||
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.
References
25 Canum Venaticorum Wikipedia(Text) CC BY-SA