Theta Capricorni
Theta Capricorni is a binary star system in the southern constellation of Capricornus, positioned 0.58° south of the ecliptic. Sometimes, this star is called by the name Dorsum, meaning the back in Latin; Theta Capricorni is its Bayer designation, which is Latinized from θ Capricorni and abbreviated Theta Cap or θ Cap. It can be seen with the naked eye, having an apparent visual magnitude of +4.07. Based upon an annual parallax shift of as seen from the Earth, the star is about from the Sun. It is drifting closer with a radial velocity of −11 km/s.
The star or star system is almost eclipsed by the Sun on about 3 February, when it will figure behind the Sun's corona if there is a full solar eclipse. Thus the star can be viewed the whole night, crossing the sky, in early August. It can be occulted by the Moon.
Characteristics
Radial velocity variations indicated it may be a binary star system, but when the system was examined in the infrared, no companion was detected. However, a companion was subsequently confirmed in 2023 by direct observations by an interferometer.The main component of this system is an A-type main sequence star with a stellar classification of A1 V. Theta Capricorni has an estimated 2.54 times the mass of the Sun and around 2.35 times the Sun's radius. It is 280 million years old and is spinning fairly rapidly with a projected rotational velocity of 104 km/s. The star is radiating 65 times the solar luminosity from its photosphere at an effective temperature of around 10,000 K.
The secondary component does not have a known stellar classification, but is much smaller and cooler than its primary, with about 50% the mass and radius of the Sun, and a temperature of 3,900 K. It takes to complete an orbit around the barycenter, and is separated from its primary by 0.78 astronomical units.