File:Properties of Low-Mass Stars and Planets.jpg

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English: Illustration of the properties of low-mass stars and planets, expressed in solar units. The newly determined, precise values of the mass and radius of OGLE-TR-122b are indicated as the red dot. The blue symbols are values for low-mass stars, while the black symbols on the left represent exoplanets. Note that the "hot Jupiters" — exoplanets orbiting very close to their host star — are larger than OGLE-TR-122b. The various lines represent theoretical models from G. Chabrier, I. Baraffe and colleagues, showing a good agreement between theory and observations.
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Source http://www.eso.org/public/images/eso0507b/
Author ESO

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Date/TimeThumbnailDimensionsUserComment
current18:29, 26 August 2019Thumbnail for version as of 18:29, 26 August 2019800 × 771 (62 KB)BevinKacon (talk | contribs)Reverted to version as of 18:06, 25 May 2013 (UTC) actual size from source
15:27, 1 June 2013Thumbnail for version as of 15:27, 1 June 20131,280 × 1,234 (84 KB)Stas1995 (talk | contribs)1280 × 1234
18:06, 25 May 2013Thumbnail for version as of 18:06, 25 May 2013800 × 771 (62 KB)Stas1995 (talk | contribs)User created page with UploadWizard

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