Achernar
Achernar, or Alpha Eridani, is located around 144 light-years (ly)
from Sun. The
star constitutes the southern end of Constellation
Eridanus,
the River, of which it is the brightest. The stars name derives from
"Al Ahir al Nahr" which is the Arabic phrase for "The End of the River,"
as it now marks the southern end of this great celestial river
that once ended at
Theta
Eridani. Achernar is the ninth brightest star in
Earth's night sky, beating out Betelgeuse
because of its variability. However, the star lies only 32
degrees from the South Pole and so is not well known to those
living in the northern hemisphere. The star has a mass that is six
to eight times greater than Sol's, 1,070 times its visual luminosity, and at least 2,900
to 5,400 times its bolometric luminosity. A fast-spinning hot
star, it is also very young with no more than a few
hundred million years, like
Regulus A.
Ejecting mass at a rate thousands of times greater than Sol,
Achernar's high spin velocity of 225 to 300 kilometers per
second (information taken from SolStation)http://en.es-static.us/upl/2009/06/achernar.jpeg |
Chemical Make Up: hydrogen, helium
Location: RA: 01h 37m 42.8s, Dec: -57° 14′ 12″
Spectrum Analysis:
http://www.umop.net/spctelem.htm |
Stellar Classification: Spectral class: B3p
Luminosity Class: V
Binary Star
Resources:
Achernar. (n.d.). Retrieved September 27, 2015, from http://www.solstation.com/x-objects/achernar.htm
Achernar. (n.d.). Retrieved October 1, 2015, from http://www.stellar-database.com/Scripts/search_star.exe?Name=Achernar
Stars. (n.d.). Retrieved October 1, 2015, from http://www.astronoo.com/en/stars.html
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