Tau CetiTau Ceti is a star commonly used by science fiction authors since it is similar to the Sun, being of similar mass and similar spectral type as well as being relatively close to us. However, Tau Ceti is a "metal-deficient" star and therefore extremely unlikely to have rocky planets around it. It is also known as HD 10700, HR 509, BD-16°295, GCTP 365.00 and LHS 146. In 2004 a team of UK astronomers led by Jane Greaves discovered that Tau Ceti has more than ten times the amount of cometary and asteroidal material orbiting it than the Sun does. This was determined by measuring the disc of cold dust orbiting the star produced by collisions between such small bodies. This result puts a damper on the possibility of complex life in this system, as planets there would suffer from large impact events roughly ten times more frequently than Earth. Tau Ceti can be seen with the unaided eye as a faint star in the constellation of Cetus. Some facts about Tau Ceti
Tau Ceti in fictionSeveral science fiction novels are set on or around a habitable planet orbiting Tau Ceti, of which the following is a sample.
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Categories: Stars | Cetus constellation |
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