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 Achernar (Alpha Eridani) Achernar is extremely flattened by its rapid spin. Image: ESO The ninth brightest star in the sky but one that is not well known to northern observers as it can only be seen at latitudes below 32° N. Its name, derived from the Arabic Al Ahir al Nahr, means "river's end" and refers to its location at the southernmost point of the constellation Eridanus. Achernar's high spin velocity of at least 250 km/s has led to it becoming a Be star. Observations by the Very Large Telescope, published in 2003, reveal that it is extraordinarily flattened, with an equatorial radius 50% larger than its polar radius. The high degree of flattening measured for Achernar – a first in observational astrophysics – now poses an unprecedented challenge for theoretical astrophysics. The effect can't be reproduced by common models of stellar interiors unless certain phenomena are incorporated, e.g. meridional circulation on the surface ("north-south streams") and non-uniform rotation at different depths inside the star. Achernar also shows small, regular light variations of a type that make it a Lambda Eridani star. Visual magnitude 0.45 Absolute magnitude -2.77 Spectral type B3Vpe Surface temperature 14,500-19,300 K Luminosity (Sun = 1) 2,900-5,400 Mass (Sun = 1) 6-8 Distance 144 light-years (44.1 pc) Position R.A. 01h 37m 42.9s, Dec. -57° 14' 12" Other designations HR 472, CD -57°334, HD 10144, SAO 232481, FK5 54, HIP 7588 Related entry    • brightest stars Related category    • NOTABLE STARS Also on this site: Encyclopedia of Alternative Energy & Sustainable Living Encyclopedia of History Transport Concepts & Designs (partner site) BACK TO TOP