Achernar (star)

From Traveller Wiki - Science-Fiction Adventure in the Far future
Revision as of 17:46, 7 March 2019 by WHULorigan (talk | contribs)
Jump to navigation Jump to search
Achernar A
Imperiumgrey-2.jpg
Spectral B6 Vep
Type Main Sequence
Multiple Binary
Luminosity 3150 LSol
Absolute magnitude -2.77
Mag Terra 0.46
Temperature 10,000 - 20,000° K
Mass 6.7 MSol
Radius 7.3 x 11.4 RSol
Achernar B
Imperiumgrey-2.jpg
Spectral A1-A3 V
Type Main Sequence
Luminosity LSol
Absolute magnitude
Mag Terra 0.46
Temperature ° K

The star Achernar (also spelled Achenar and otherwise known as Alpha Eridani) is a binary system composed of a hot blue main sequence star of spectral classification B6 orbited by a smaller blue-white main sequence star of spectral type A.

Description (Specifications)

  • Achernar A has an unusually rapid rotational velocity, causing it to become oblate in shape. It is one of the least spherical stars in Galaxias.
  • Achernar B orbits Achernar A at a distance of 12.3AU with an orbital period of about 14.5 years.

The Achernar star system lies approximately 42.8pc from Terra, and is located in a Rimtrailing/Trailing direction from Terra at bearing 290.8o Galactic Longitude and -58.8o South Galactic Latitude.

History & Background (Dossier)

Despite the similarity in name, Achernar is NOT the primary star of the world Archernar/Orichalc (Alpha Crucis 0719), which orbits a yellow-white giant star of classification G4 III.

  • Achernar may or may not have lent its name to the slightly differently spelled world of Archernar which lies in the same sector.

Image Repository

TravellerMap (T5SS):
[1]

References & Contributors (Sources)

This article has metadata.
Smallwikipedialogo.png This page uses content from Wikipedia. The original article was at Achernar. The list of authors can be seen in the page history. The text of Wikipedia is available under the Commons Attribution-ShareAlike 3.0 Unported License.
This list of sources was used by the Traveller Wiki Editorial Team and individual contributors to compose this article. Copyrighted material is used under license from Mongoose Publishing or by permission of the author. The page history lists all of the contributions.