24 Ursae Majoris

24 Ursae Majoris is a variable star in the northern circumpolar constellation of Ursa Major, located 101.5 light-years from the Sun. It has the variable star designation DK Ursae Majoris and the Bayer designation d Ursae Majoris; "24 Ursae Majoris" is the Flamsteed designation. This object is visible to the naked eye as a faint, yellow-hued star with an apparent visual magnitude of 4.54. It is moving closer to the Earth with a heliocentric radial velocity of −27 km/s, and is expected to come as close as in around 879,000 years.
Description.
24 Ursae Majoris has a stellar classification of G4 III-IV, which, at the estimated age of about one billion years, matches the spectrum of an aging giant star blended with features of a subgiant luminosity class. Based upon its position on the H–R diagram, this star has just passed through the Hertzsprung gap and is ready to begin its first ascent along the red-giant branch. It is a suspected RS Canum Venaticorum variable that changes in brightness by up to 0.058 in magnitude with a period of 0.9202 days, and is an X-ray source with a luminosity of .
This star has 1.9 times the mass of the Sun and has expanded to 4.6 times the Sun's radius. It is spinning with a rotation period of 10 days. The star is radiating 14.9 times the Sun's luminosity from its enlarged photosphere at an effective temperature of 5,335 K.
Nomenclature.
With π1, π2, σ1, σ2, ρ and 2 Ursae Majoris, it composed the Arabic asterism Al Ṭhibā᾽, the Gazelle. According to the catalogue of stars in the "Technical Memorandum 33-507 - A Reduced Star Catalog Containing 537 Named Stars", "Al Ṭhibā" were the title for seven stars : 2 Ursae Majoris as "Althiba I", π1 as "Althiba II", π2 as "Althiba III", ρ as "Althiba IV", σ1 as "Althiba V", σ2 as "Althiba VI", and this star (d) as "Althiba VII".