Kakkab (Alpha Lupi)
Image credit: ESO Online Digitized Sky Survey.
Kakkab (Alpha Lupi) is the brightest star in the constellation Lupus; its (rarely used) ancient name comes from the phrase Kakkab Su-gub Gud-Elim meaning "the Star Left of the Horned Bull."
Kakkab is a hot giant B star belonging to the Upper Centaurus-Lupus Association (UCL), which in turn is part of a huge collection of O and B stars called the Scorpius-Centaurus Association. From analysis of all its members, UCL lies at an average distance of 450 light-years, which fits well with Kakkab's individually measured distance.
Like many of its spectral type, Kakkab is a Beta Cephei star, a variable that pulsates subtly with multiple periods. With a major oscillation cycle of 0.259847 days (the period really is known to such accuracy), in which it varies by only 0.03 magnitudes (about 3%), Kakkab has one of the longest periods of its class. A secondary pulsation takes 0.236798 days. A thirteenth magnitude star, just 28" away, may be a genuine companion of Kakkab or may be simply an optical double.
|mass||10 to 11 Msun|
|distance||548 light-years (168 pc)|
|position||R.A. 14h 41m 55.8s,
Dec. -47° 23' 18"