A-type star in the constellation Eridanus
For other star systems with this Bayer designation , see Tau Eridani .
Tau Eridani , Latinized from τ Eridani , is a star in the constellation Eridanus . It is visible to the naked eye with an apparent visual magnitude of 4.10. Using the parallax method , the distance to this star can be estimated as 88.6 light years . In 2001 it was reported as a candidate Vega -like star, meaning it appears to radiate an infrared excess from an orbiting circumstellar disk . However, this has not been confirmed.
This is an A-type star with a stellar classification of A3 IV-V. The luminosity class of IV-V indicates the spectrum displays traits intermediate between a main sequence and subgiant star . It is around 476 million years old and is spinning rapidly with a projected rotational velocity of 133 km/s. This is creating an equatorial bulge that might be 7% wider than the polar radius. Tau Eridani has 178% of the Sun's mass and nearly double the radius of the Sun . The star shines with 13.7 times the solar luminosity from an outer atmosphere at an effective temperature of 8,251 K.
References
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: CS1 maint: postscript (link )
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