Epsilon Eridanistar

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Aspects of this topic are discussed in the following places at Britannica.

Assorted References

  • main-sequence stars ( in star: Hertzsprung-Russell diagram )

    ...the main sequence. These stars range from hot, O- and B-type, blue objects at least 10,000 times brighter than the Sun down through white A-type stars such as Sirius to orange K-type stars such as Epsilon Eridani and finally to M-type red dwarfs thousands of times fainter than the Sun. The sequence is continuous; the luminosities fall off smoothly with decreasing surface temperature; the...

  • Project Ozma ( in Ozma, Project )

    ...hydrogen; it was thought that this would be familiar, as a kind of universal standard, to anyone attempting interstellar radio communication. The telescope was aimed at two nearby stars (Epsilon Eridani and Tau Ceti, both about 11 light-years from the Earth) that resemble the Sun and seem reasonably likely to have inhabited planets.

Citations

MLA Style:

"Epsilon Eridani." Encyclopædia Britannica. 2008. Encyclopædia Britannica Online. 05 Dec. 2008 <http://www.britannica.com/EBchecked/topic/190517/Epsilon-Eridani>.

APA Style:

Epsilon Eridani. (2008). In Encyclopædia Britannica. Retrieved December 05, 2008, from Encyclopædia Britannica Online: http://www.britannica.com/EBchecked/topic/190517/Epsilon-Eridani

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