Kappa Draconis, Latinized from κ Draconis, is a blue giant star located in the northern circumpolar constellation of Draco. At an apparent magnitude of 3.88, it is barely visible to the naked eye when artificial lighting from cities is present. Nevertheless, it is a powerful star, approximately five time as massive as the Sun. It is about 460 light-years away, and is 1,400 times brighter than the Sun. The star is currently located at declination (right ascension ), but due to the effects of precession, Kappa Draconis was the nearest star to the north celestial pole visible to the naked eye from 1793 BC to approximately 1000 BC, though it was 6° removed from perfect alignment, making it only an approximate pole star, similar to the roughly 7° variance from perfect alignment of the much brighter (magnitude 2.08) star Kochab, at the same time during Earth's precession. Properties Kappa Draconis is a classical Be star, displaying Balmer emission lines in its spectrum. It is spinning rapidly with a projected rotational velocity of 170 km/s. The star is thought to be just entering its red giant phase, having exhausted the supply of hydrogen in its core. Over the next several thousand years, the star will expand, becoming more powerful but with a much cooler surface temperature. Tens of thousands of years from now, Kappa Draconis will appear much brighter, probably shining with a reddish hue. Kappa Draconis is a single-lined spectroscopic binary. The main Be star is orbited by another stellar companion, on a circular orbit with a period of 61.555 days. The General Catalogue of Variable Stars lists Kappa Draconis as a Gamma Cassiopeiae type star, a type of eruptive irregular variable star, whose visual magnitude varies from 3.82 to 4.01. However Balona and Dziembowsk classify it as a Zeta Ophiuchi star, a type of pulsating variable star, with a primary period of 10.4 hours. Chinese name In Chinese, (), meaning Right Wall of Purple Forbidden Enclosure, refers to an asterism consisting of κ Draconis, α Draconis, λ Draconis, 24 Ursae Majoris, 43 Camelopardalis, α Camelopardalis and BK Camelopardalis. Consequently, the Chinese name for κ Draconis itself is (, .), representing (), meaning Second Chief Judge References External links Kappa Draconis by Jim Kaler B-type giants Be stars Spectroscopic binaries Draco (constellation) Draconis, Kappa Durchmusterung objects Draconis, 05 109387 061281 4787 Northern pole stars