Category:Non-circumbinary planetary systems
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- Planets that orbit a single star in a binary star system are called “non-circumbinary planets”. In general, a planet in a non-circumbinary system, though, must orbit relatively close to its host star in relation to the closest approach of the second star in order for the planet’s orbit to be stable - National Radio Astronomy Observatory
Subcategories
This category has the following 8 subcategories, out of 8 total.
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Media in category "Non-circumbinary planetary systems"
The following 8 files are in this category, out of 8 total.
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Eclipse in a system with ocean planet and gas giant orbiting in non-circumbinary system.jpg 3,000 × 1,688; 1.58 MB
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Eclipse in a system with ocean planet and gas giant orbiting in non-circumbinary system.tif 3,000 × 1,688; 28.98 MB
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Planets in binary star systems - P- and S-type.svg 220 × 220; 13 KB
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Planets in binary star systems - S-type.svg 220 × 220; 8 KB
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Sunset in a binary star system with a gas giant planet.jpg 2,000 × 1,125; 2.37 MB
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Sunset in a binary star system with a gas giant planet.tif 2,000 × 1,125; 12.87 MB
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Sunset in a binary system with a red dwarf and a white dwarf.jpg 2,500 × 1,406; 3.72 MB
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Sunset in a binary system with a red dwarf and a white dwarf.tif 2,500 × 1,406; 20.11 MB
