Exoplanetary Scratchpad

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Zeta Tuc is also known as HR 77, Gl 17, and HD 1581. Nearby star system. It is a nearby yellowish star with a late F or early G spectrum. It may have an unseen spectroscopic binary partner. It is slightly less massive, slightly larger, and slightly brighter than the Sun and only 44 to 79% its metalicity. It is one of the least variable stars observed during the Hipparcos mission. Its similarity to the Sun make it an interesting target. It is about 3 Billion Years old. It is thought to have a debris disk. Its rotational velocity appears to be almost zero, indicating it presents its pole towards us, which would make finding planets through radial velocity nearly impossible.

Zeta Tucanae System Web PagesEdit

Zeta Tucanae System In the NewsEdit

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