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Achernar

 
Dictionary: A·cher·nar   (ā'kər-när') pronunciation
Achernar
Source
n.
A star in the constellation Eridanus that is one of the brightest stars in the sky and is 114 light-years from Earth.

[From Arabic 'aḫīr an-nahr, the end of the river (referring to the star's position in the constellation Eridanus) : 'aḫīr, last, end + al-, the + nahr, river.]


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Columbia Encyclopedia: Achernar
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Achernar (ā'kərnär'), brightest star in the constellation Eridanus; Bayer designation α Eridani; 1992 position R.A. 1h37.4m, Dec. −57°16′. A bluish-white white star with apparent magnitude 0.51, it is one of the 10 brightest stars in the entire sky. Its distance is about 120 light-years, and its luminosity about 600 times that of the sun. Achernar is of spectral class B5 V. Its name is from the Arabic meaning "end of the river [Eridanus]."


Wikipedia: Achernar
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Achernar
Position Alpha Eri.png
The position of Achernar.
Observation data
Epoch J2000      Equinox J2000
Constellation Eridanus
Right ascension 01h 37m 42.8s
Declination −57° 14' 12"
Apparent magnitude (V) 0.50
Characteristics
Spectral type B3 Vpe
U-B color index −0.66
B-V color index −0.20
Variable type Lambda Eridani
Astrometry
Radial velocity (Rv) 16 km/s
Proper motion (μ) RA: 88.02 mas/yr
Dec.: −40.08 mas/yr
Parallax (π) 022.68 ± 0.57 mas
Distance 144 ± 4 ly
(44 ± 1 pc)
Absolute magnitude (MV) −2.77
Details
Mass 6–8 M
Radius ~10 R
Luminosity 3,311(bolometric) L
Temperature 14,510 K
Rotation 225–300 km/s
Age 1–5 × 108 years
Other designations
α Eri, HR 472, CD -57°334, HD 10144, SAO 232481, FK5 54, HIP 7588.

Achernar (α Eri / α Eridani / Alpha Eridani), sometimes spelled Achenar, is the brightest star in the constellation Eridanus and the ninth-brightest star in the nighttime sky. Of the top ten apparent brightest stars (excluding our Sun): Sirius, Canopus, Alpha Centauri, Arcturus, Vega, Capella, Rigel, Procyon, Achernar & Betelguese, Achernar is the hottest and bluest. It lies at the southern tip of the constellation.

The extreme rotation speed has flattened Achernar.

Achernar is a bright, blue, B3-type star of six to eight solar masses lying approximately 144 light-years (44 pc) away. Although classified as a main-sequence (dwarf) star, it is about 3,000 times more luminous than the Sun. Achernar is in the deep southern sky and never rises above 33°N. Achernar is best seen from the southern hemisphere in November; it is circumpolar below 33°S.

Until about March 2000, Achernar and Fomalhaut were the two first-magnitude stars furthest in angular distance from any other first-magnitude star in the celestial sphere. Antares, in the constellation of Scorpius, is now the most isolated first-magnitude star although Antares is located in a constellation with many bright second magnitude stars whereas the stars surrounding Achernar and Fomalhaut are considerably fainter.

It is the least spherical star in the Milky Way studied to date. (See “Achernar the Flattest star” in ‘Sky &Telescope’ P. 20 ‘Newsnotes’, September 2003.) Achernar spins so rapidly that its equatorial diameter is more than 50% greater than its polar diameter.

The name comes from the Arabic آخر النهر ākhir an-nahr "river's end".

It is known as 水委一 (Shuǐwěiyī, the First Star of the Crooked Running Water) in Chinese.

Fiction

External links

Coordinates: Sky map 01h 37m 42.8s, −57° 14′ 12″


 
 

 

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Dictionary. The American Heritage® Dictionary of the English Language, Fourth Edition Copyright © 2007, 2000 by Houghton Mifflin Company. Updated in 2009. Published by Houghton Mifflin Company. All rights reserved.  Read more
Columbia Encyclopedia. The Columbia Electronic Encyclopedia, Sixth Edition Copyright © 2003, Columbia University Press. Licensed from Columbia University Press. All rights reserved. www.cc.columbia.edu/cu/cup/ Read more
Wikipedia. This article is licensed under the Creative Commons Attribution/Share-Alike License. It uses material from the Wikipedia article "Achernar" Read more