CoRoT-8b

COROT-8b
	CoRoT-8b compared to Jupiter and Neptune.
Discovery[1]
Discovered by	Borde et al.
Discovery site	CoRoT space telescope
Discovery date	12 April 2010
Detection method	Transit
Orbital characteristics
Semi-major axis	0.0636 ± 0.0014 AU (9,510,000 ± 210,000 km)[2]
Eccentricity	<0.19[3]
Orbital period	6.212445±0.000007 d[2]
Inclination	88.18°±0.08°[2]
Time of periastron	2,454,239.03317±0.00049 JD[2]
Semi-amplitude	27.6+5.8; −4.7 m/s[3]
Star	COROT-8
Physical characteristics
Mean radius	0.619+0.016; −0.017 RJ[2]
Mass	0.218±0.034 MJ[2]
Mean density	1.1±0.2 g/cm3[2]
Temperature	870 ± 14 K (1,106.3 ± 25.2 °F; 596.9 ± 14.0 °C)[2]

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

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. doi:10.1051/0004-6361/201014775. ISSN 0004-6361.
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: 824–839. doi:10.1093/mnras/sty3085. ISSN 0035-8711.
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. doi:10.1051/0004-6361/201629882. ISSN 0004-6361.

This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.

[Borde2010-1] 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. doi:10.1051/0004-6361/201014775. ISSN 0004-6361.

[Raetz2019-2] 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: 824–839. doi:10.1093/mnras/sty3085. ISSN 0035-8711.

[Bonomo2017-3] 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. doi:10.1051/0004-6361/201629882. ISSN 0004-6361.