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KOI 81 System

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Exoplanetary Scratchpad

[SysBP Img]

Contains one of two of a new class of objects discovered in early Kepler data that is too hot to be a planet (13,500K), but too small to be a star (0.9 RJ), and is actually hotter than its host star (10,000K). Possibly a white dwarf star that lost much of its mass to be Jupiter sized, rather than Earth sized. Mass measurements are needed.

KOI 81 System Web Pages

KOI 81 System In the News

First batch of five planets discovered by Kepler (2010)

Year in Review (2010)

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