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CoRoT-8b

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(Redirected from COROT-8b) Extrasolar planet in the constellation Aquila
CoRoT-8b
CoRoT-8b compared to Jupiter and Neptune.CoRoT-8b compared to Jupiter and Neptune.
Discovery
Discovered byBorde et al.
Discovery siteCoRoT space telescope
Discovery date12 April 2010
Detection methodTransit
Orbital characteristics
Semi-major axis0.0636 ± 0.0014 AU (9,510,000 ± 210,000 km)
Eccentricity<0.19
Orbital period (sidereal)6.212445±0.000007 d
Inclination88.18°±0.08°
Time of periastron2,454,239.03317±0.00049 JD
Semi-amplitude27.6+5.8
−4.7 m/s
StarCoRoT-8
Physical characteristics
Mean radius0.619+0.016
−0.017 RJ
Mass0.218±0.034 MJ
Mean density1.1±0.2 g/cm
Temperature870 ± 14 K (1,106.3 ± 25.2 °F; 596.9 ± 14.0 °C)

CoRoT-8b is a transiting exoplanet orbiting the K-type main sequence star CoRoT-8 1,050 light years away in the equatorial constellation Aquila. The planet was discovered in April 2010 by the CoRoT telescope.

Discovery

This planet was discovered using the transit method, which detects planet via eclipses. The discovery paper's abstract states that CoRoT-8b is extremely dense compared to Saturn.

Properties

CoRoT-8b has 21.8% Jupiter's mass, and due to its close orbit, a radius 61.9% that of Jupiter. This classifies the planet as a hot Saturn. Despite the bloated radius, the planet is extremely dense, with it being 1.1 times greater than water's; CoRoT-8b has a temperature of 870 K from its 6-day orbit.

References

  1. Bordé, P.; et al. (September 2010). "Transiting exoplanets from the CoRoT space mission. XI. CoRoT-8b: a hot and dense sub-Saturn around a K1 dwarf". Astronomy and Astrophysics. 520: A66. arXiv:1008.0325. Bibcode:2010A&A...520A..66B. doi:10.1051/0004-6361/201014775. ISSN 0004-6361. S2CID 56357511.
  2. ^ Raetz, St; Heras, A. M.; Fernández, M.; Casanova, V.; Marka, C. (February 2019). "Transit analysis of the CoRoT-5, CoRoT-8, CoRoT-12, CoRoT-18, CoRoT-20, and CoRoT-27 systems with combined ground- and space-based photometry". Monthly Notices of the Royal Astronomical Society. 483 (1): 824–839. arXiv:1812.01536. Bibcode:2019MNRAS.483..824R. doi:10.1093/mnras/sty3085. ISSN 0035-8711.
  3. ^ Bonomo, A. S.; et al. (June 2017). "The GAPS Programme with HARPS-N at TNG . XIV. Investigating giant planet migration history via improved eccentricity and mass determination for 231 transiting planets". Astronomy and Astrophysics. 602: A107. arXiv:1704.00373. Bibcode:2017A&A...602A.107B. doi:10.1051/0004-6361/201629882. ISSN 0004-6361. S2CID 118923163.
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