NOTABLE STARS A  B  C  D  E  F  G  H  I  J  K  L  M  N  O  P  Q  R  S  T  U  V  W  X  Y  Z                    HOME ABOUT CATEGORIES SITE MAP COPYRIGHT ADVERTISE CONTACT entire Web this site Zeta Aurigae Zeta Aurigae as portrayed by the artist Chesley Bonestell. © Bonestell Space Art, used with permission A famous eclipsing binary in the constellation Auriga and one of the Kids (in Latin "Haedus"). It is also known as Haedus I and by an astonishing coincidence, its constellation mate, Epsilon Aurigae, which is the second Kid ("Haedus II"), is also a well-known (and even more remarkable) eclipsing binary. Zeta consists an orange supergiant (spectral type K4) in orbit around a blue B star (type B5) with a period of 972.2 days (2.66 years). Because the orientation of the orbit lies within 3° of our line of sight, every 2.66 years the smaller B star hides completely behind the larger K star (which is about as wide as Venus's orbit), and the combined visual light drops by 0.15 magnitude (about 15%). Averaging 4.2 AU apart, the two go around each other in an elliptical orbit that takes them from 5.9 AU to 2.5 AU apart. visual magnitude 3.69 absolute magnitude -3.23 spectral type K4II surface temperature 3,950 K (K star), 15,300 K (B star) luminosity 4,800 Lsun (K star), 1,000 Lsun (B star) radius 148 Rsun (K star), 4.5 Rsun (B star) mass 5.8 Msun (K star), 4.8 Msun (B star) distance 790 ± 150 light-years (242 ± 47 pc) position R.A. 05h 02m 28.7s; Dec. +41° 04' 33" other designations Haedi Haedus, Sadatoni, Saclateni, 8 Aurigae, HR 1612, HD 32068, BD+40°1142A, FK5 1137, HIP 23453, SAO 39966, GC 6137, CCDM 05025+4105 Related categories    • NOTABLE STARS    • VARIABLE STARS Also on this site: Encyclopedia of Alternative Energy & Sustainable Living Encyclopedia of History Transport Concepts & Designs (partner site) BACK TO TOP