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Kepler-296f

Kepler-296f^[1][2][3] (also known by its Kepler Object of Interest designation KOI-1422.04) is a confirmed super-Earth exoplanet orbiting within the habitable zoneofKepler-296. The planet was discovered by NASA's Kepler spacecraft using the transit method, in which the dimming effect that a planet causes as it crosses in front of its star is measured. NASA announced the discovery of the exoplanet on 26 February 2014.^[1]

Confirmed exoplanet[edit]

Kepler 296f is a super-Earth with a radius 1.79 times that of Earth. The planet orbits Kepler-296 once every 63.3 days.

Habitability[edit]

The planet is located within the habitable zone of Kepler-296, a region where liquid water could exist on the surface of the planet.

Notable Exoplanets – Kepler Space Telescope
Confirmed small exoplanets in habitable zones. (Kepler-62e, Kepler-62f, Kepler-186f, Kepler-296e, Kepler-296f, Kepler-438b, Kepler-440b, Kepler-442b) (Kepler Space Telescope; 6 January 2015).[4]

See also[edit]

• Habitability of red dwarf systems
• List of potentially habitable exoplanets

References[edit]

External links[edit]

• NASA – Kepler Mission.
• NASA – Kepler Discoveries – Summary Table.
• NASA – Kepler-296fatThe NASA Exoplanet Archive.
• NASA – Kepler-296fatThe Exoplanet Data Explorer.
• NASA – Kepler-296fatThe Extrasolar Planets Encyclopaedia.
• Habitable Exolanets CatalogatUPR-Arecibo.

Biology