page_title: HD 17156 b
hierarchical_section_title: HD 17156 b
caption_attribution_description: English: Comparison of best-fit size of the exoplanet HD 17156 b with the Solar System planet Jupiter, as reported in the Open Exoplanet Catalogue[1] as of 2010-09-30. ↑ Open Exoplanet Catalogue (2010-09-30). Retrieved on 2010-09-30.
context_page_description: HD 17156 b, named Mulchatna by the IAU, is an extrasolar planet approximately 255 light-years away in the constellation of Cassiopeia. The planet was discovered orbiting the yellow subgiant star HD 17156 in April 2007. The planet is classified as a relatively cool hot Jupiter planet slightly smaller than Jupiter but slightly larger than Saturn. This highly-eccentric three-week orbit takes it approximately 0.0523 AU of the star at periastron before swinging out to approximately 0.2665 AU at apastron. Its eccentricity is about the same as 16 Cygni Bb, a so-called "eccentric Jupiter". Until 2009, HD 17156 b was the transiting planet with the longest orbital period.
context_section_description: HD 17156 b, named Mulchatna by the IAU, is an extrasolar planet approximately 255 light-years away in the constellation of Cassiopeia.  The planet was discovered orbiting the yellow subgiant star HD 17156 in April 2007.  The planet is classified as a relatively cool hot Jupiter planet slightly smaller than Jupiter but slightly larger than Saturn. This highly-eccentric three-week orbit takes it approximately 0.0523 AU of the star at periastron before swinging out to approximately 0.2665 AU at apastron. Its eccentricity is about the same as 16 Cygni Bb, a so-called "eccentric Jupiter". Until 2009, HD 17156 b was the transiting planet with the longest orbital period.
caption: Size comparison of HD 17156 b with Jupiter.
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