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Kepler-90f

From Wikipedia, the free encyclopedia

Kepler-90f
Illustration of the Kepler-90 system compared to the inner solar system. Kepler-90f orbits between Kepler-90e and Kepler-90g.
Discovery[1]
Discovered byJ. Cabrera et al.
Discovery siteKepler space telescope
Discovery date23 October 2013
Transit method
Orbital characteristics
0.48 ± 0.09 AU (72,000,000 ± 13,000,000 km)[1]
Eccentricity0[2]
124.9144 ± 0.0019 d[1]
Inclination89.77 ± 0.31[1]
StarKepler-90
Physical characteristics
Mean radius
2.88 ± 0.52 R🜨[1]
Temperature407 K (134 °C)

Kepler-90f is an exoplanet orbiting the star Kepler-90, located in the constellation Draco. It was discovered by the Kepler telescope in October 2013. It orbits its parent star at only 0.48 astronomical units away, and at its distance it completes an orbit once every 124.91 days.[1]

Artist's impression of the planets of the Kepler-90 exoplanetary system compared to the eight planets of the Solar System.

Host star

Main article: Kepler-90

The planet orbits a G-type star named Kepler-90, its host star. The star is 1.2 times as massive as the Sun and is 1.2 times as large as the Sun. It is estimated to be 2 billion years old, with a surface temperature of 6080 K. In comparison, the Sun is about 4.6 billion years old[3] and has a surface temperature of 5778 K.[4]

References

  1. ^ a b c d e f Cabrera, J; Csizmadia, Sz; Lehmann, H; Dvorak, R; Gandolfi, D; Rauer, H; Erikson, A; Dreyer, C; Eigmüller, Ph; Hatzes, A (2013). "The Planetary System to KIC 11442793: A Compact Analogue to the Solar System". The Astrophysical Journal. 781 (1): 18. arXiv:1310.6248. Bibcode:2014ApJ...781...18C. doi:10.1088/0004-637X/781/1/18. S2CID 118875825.
  2. ^ Thompson; et al. (31 August 2017). "Kepler Objects of Interest". NASA Exoplanet Archive. NASA Exoplanet Science Institute. Retrieved 8 August 2020.
  3. ^ Fraser Cain (16 September 2008). "How Old is the Sun?". Universe Today. Retrieved 19 February 2011.
  4. ^ Fraser Cain (15 September 2008). "Temperature of the Sun". Universe Today. Retrieved 19 February 2011.


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This page was last edited on 28 September 2023, at 07:36
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