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== References ==
[[Category:Exoplanets]]
[[Category:Exoplanets]]

Revision as of 16:29, 28 June 2025

Kepler-296d
Discovery
Discovered byKepler spacecraft
Discovery date2014
Transit
Orbital characteristics
0.118 AU
Eccentricity<0.33
19.9 d
StarKepler-296
Physical characteristics
2.09 Earth radii
Mass5.02 Earth masses

Kepler-296d is an exoplanet orbiting the M-dwarf star Kepler-296[1].[2][3], located in the constellation Draco[4]. It was discovered in 2014 by the Kepler space telescope using the transit method[1][5]

Characteristics

Kepler-296d has a radius approximately 2.09 times[1] that of Earth and a mass estimated at 5.02[1] [4]Earth masses, placing it in the category of Neptune-like exoplanets. The planet orbits its host star every 19.9 days at a distance of approximately 0.118 AU[1][5]. Its orbit has an eccentricity of less than 0.33[5].

Host Star

The host star, Kepler-296, is an M-type dwarf.[2]. These stars are cooler and smaller than the Sun, and often host multiple exoplanets. Kepler-296 is known to host at least five planets[1][3]

Discovery

Kepler-296d was identified in 2014[1] as part of the data collected by NASA's Kepler space telescope, which monitored the brightness of over 150,000 stars[6] to detect periodic dips in light indicative of planetary transits. The detection of Kepler-296d was achieved through the transit method[1][5], wherein a planet passes between its host star and the observer, causing a measurable decrease in the star’s apparent brightness.

See also

Kepler-296

List of exoplanets discovered in 2014

Exoplanet

References

  1. ^ a b c d e f g h "Kepler-296 | NASA Exoplanet Archive". exoplanetarchive.ipac.caltech.edu. Retrieved 2025-06-28.
  2. ^ a b "Kepler-296 - NASA Science". 2023-11-28. Retrieved 2025-06-28.
  3. ^ a b https://iopscience.iop.org/article/10.1088/0004-637X/809/1/7/pdf
  4. ^ a b "Kepler-296". www.exoplanetkyoto.org. Retrieved 2025-06-28.
  5. ^ a b c d "Kepler-296 d - NASA Science". 2017-10-02. Retrieved 2025-06-28.
  6. ^ "Kepler / K2 - NASA Science". 2023-05-23. Retrieved 2025-06-28.