Kepler-7b

Kepler-7b
Size comparison of Kepler-7b with Jupiter, showing a rudimentary map of its atmosphere[1] derived from telescope observations.
Discovery[2]
Discovery dateJanuary 4, 2010[3]
Transit (Kepler Mission)[2]
Orbital characteristics
0.06224 AU
Eccentricity0[2]
4.885525±0.000040[2] d
Inclination86.5[4]
StarKepler-7
Physical characteristics
1.478+0.050
−0.051[2] RJ
Mass0.433+0.040
−0.041[2] MJ
Mean density
0.166+0.019
−0.020 g/cm3[citation needed]
Albedo0.32±0.03[5][6]
Temperature1,540 K (1,270 °C; 2,310 °F)[2]

Kepler-7b is one of the first five exoplanets to be confirmed by NASA's Kepler spacecraft, and was confirmed in the first 33.5 days of Kepler's science operations.[2] It orbits a star slightly hotter and significantly larger than the Sun that is expected to soon reach the end of the main sequence.[2] Kepler-7b is a hot Jupiter that is about half the mass of Jupiter, but is nearly 1.5 times its size; at the time of its discovery, Kepler-7b was the second most diffuse planet known, surpassed only by WASP-17b.[2] It orbits its host star every five days at a distance of approximately 0,06 AU (9.000.000 km or 5.592.340 mi). Kepler-7b was announced at a meeting of the American Astronomical Society on January 4, 2010. It is the first extrasolar planet to have a crude map of cloud coverage.[7][8][9]

  1. ^ Cite error: The named reference cloudUCSC was invoked but never defined (see the help page).
  2. ^ a b c d e f g h i j Cite error: The named reference Latham2010 was invoked but never defined (see the help page).
  3. ^ Cite error: The named reference sciencenews was invoked but never defined (see the help page).
  4. ^ Cite error: The named reference datatable was invoked but never defined (see the help page).
  5. ^ Angerhausen, Daniel; DeLarme, Em; Morse, Jon A. (2015). "A Comprehensive Study of Kepler Phase Curves and Secondary Eclipses: Temperatures and Albedos of Confirmed Kepler Giant Planets". Publications of the Astronomical Society of the Pacific. 127 (957): 1113–1130. arXiv:1404.4348. Bibcode:2015PASP..127.1113A. doi:10.1086/683797. S2CID 118462488.
  6. ^ Heng, Kevin; Demory, Brice-Oliver (2013). "Understanding Trends Associated With Clouds In Irradiated Exoplanets". The Astrophysical Journal. 777 (2): 100. arXiv:1309.5956. Bibcode:2013ApJ...777..100H. doi:10.1088/0004-637X/777/2/100. S2CID 119298230.
    And errata in Heng, Kevin; Demory, Brice-Olivier (2014). "ERRATUM: "UNDERSTANDING TRENDS ASSOCIATED WITH CLOUDS IN IRRADIATED EXOPLANETS" (2013, ApJ, 777, 100)". The Astrophysical Journal. 785: 80. doi:10.1088/0004-637X/785/1/80.
  7. ^ Clavin, Whitney; Johnson, Michele; Cole, Steve (30 September 2013). "NASA Space Telescopes Find Patchy Clouds on Exotic World". NASA. Archived from the original on 17 October 2013. Retrieved 30 September 2013.
  8. ^ Chu, Jennifer (2 October 2013). "Scientists generate first map of clouds on an exoplanet". MIT. Retrieved 2 January 2014.
  9. ^ Demory, Brice-Olivier; et al. (2013). "Inference of Inhomogeneous Clouds in an Exoplanet Atmosphere". The Astrophysical Journal Letters. 776 (2): L25. arXiv:1309.7894. Bibcode:2013ApJ...776L..25D. doi:10.1088/2041-8205/776/2/L25. S2CID 701011.