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Kepler-296f

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description Kepler-296f Overview

Kepler-296f is a transiting exoplanet categorized as a super-Earth, located approximately 1,000 light-years away. Confirmed by NASA's Kepler mission in 2014, it orbits within the habitable zone of a binary star system composed of two red dwarfs. This positioning makes it a subject of ongoing study for astronomers researching the potential for rocky planets to retain liquid water in multiple-star systems.

help Kepler-296f FAQ

Where is Kepler-296f located?

This exoplanet is located approximately 1,000 light-years away from Earth within the constellation Lyra. It resides in a binary M-dwarf system, meaning it circles a pair of cool, dim red dwarf stars.

When was Kepler-296f discovered?

NASA's Kepler mission confirmed the existence of Kepler-296f in 2014. It was identified alongside four other planets in the same system using transit photometry data gathered by the Kepler space telescope.

What makes Kepler-296f interesting to astrobiologists?

It is a super-Earth orbiting within the habitable zone of its host stars, meaning it sits at a distance where liquid water could potentially exist. Because it circles binary M-dwarfs, studying it helps astronomers understand planetary formation around cooler, long-lived stars.

Is Kepler-296f a rocky planet?

Astronomers classify it as a super-Earth, but its exact composition is still debated due to uncertainties in its radius and mass. While its size suggests it could be rocky, it may also hold a thick atmosphere or a deep ocean.

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