Theta Aurigae has a mean apparent magnitude of 2.65. The star's Galacto-Centric Distance is 7,472.00 Parsecs or 24,370.93 Light Years. The number of A.U. Eta Aurigae is a blue-white B-type main sequence dwarf located about 219 light years away. The Galacto-Centric Distance is the distance from the … [717] th eta Aurigae , sometimes also called Bogardus or Mahasim ("wrist"), is a binary star with an A-type main sequence dwarf for a primary component and a yellow G-type main sequence dwarf for its companion. The primary component is an Alpha-2 Canum Venaticorum type variable, a chemically peculiar star with a strong magnetic field and strong strontium, silicon, or chromium spectral lines. Using the 2007 distance, the star is roughly 15,393,435.23 Astronomical Units from the Earth/Sun give or take a few. The two components are designated Theta Aurigae A (also named Mahasim) and B. An Astronomical Unit is the distance between Earth and the Sun. The baby planet is forming relatively far from AB Aurigae — about 30 times the Earth-sun distance, or roughly equivalent to Neptune's distance from our sun, researchers said. Theta Aurigae is a double star about 173 light years from Earth. It has an apparent magnitude of 3.18. is the number of times that the star is from the Earth compared to the Sun. Theta Aurigae (θ Aurigae, abbreviated Theta Aur, θ Aur) is a binary star in the constellation of Auriga.Based upon parallax measurements, the distance to this system is about 166 light-years (51 parsecs)..