20 Canum Venaticorum

20 Canum Venaticorum is a single variable star in the northern constellation of Canes Venatici, located 238 light years from the Sun. This object has the variable star designation AO Canum Venaticorum; "20 Canum Venaticorum "is the Flamsteed designation. It is visible to the naked eye as a faint, white-hued star with a baseline apparent visual magnitude of +4.72. The star is moving further from the Earth with a heliocentric radial velocity of +9 km/s. Eggen (1971) listed this star as a member of the Hyades Stream.
This star has a stellar classification of , which indicates the hydrogen line matches an A-type bright giant but the metal lines are closer to an F-type star. However, it does not appear to be an Am star as the Calcium K line is normal. Earlier, Morgan and Abt (1972) assigned it a giant star class of F3 III. It is classified as a Delta Scuti type variable star with a single radial pulsation mode providing the best fit to the observed variation. Its brightness varies from magnitude +4.70 to +4.75 with a period of 2.92 hours.
20 Canum Venaticorum is 750 million years old with 2.43 times the mass of the Sun and 4 time the Sun's radius. It is radiating 63 times the Sun's luminosity from its photosphere at an effective temperature of 7,314 K.