CoRoT-14b

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CoRoT-14b
Discovery
Discovered by CoRoT space telescope
Transit
Orbital characteristics
0.027 AU (4,000,000 km) [1]
Eccentricity 0
1.51214 d
Inclination 79.6
Star CoRoT-14  [ ru ]
Physical characteristics
Mean radius
1.09 RJ
Mass 7.6MJ
Temperature 1781 K [2]
    Exoplanet CoRoT-14 b size comparison to Jupiter Exoplanet Comparison CoRoT-14 b.png
    Exoplanet CoRoT-14 b size comparison to Jupiter

    CoRoT-14b is a transiting Hot Jupiter exoplanet found by the CoRoT space telescope in 2010.[ citation needed ]

    Contents

    Host star

    CoRoT-14b orbits CoRoT-14 in the constellation of Monoceros. It is a F9V star with Te = 6035K, M = 1.13M, R = 1.21R, and near-solar metallicity. It has an estimated age between 0.4 and 8.0 Gyr.[ citation needed ]

    Characteristics

    The planet is unusually dense (7.3 g/cm3) for its mass and distance from host star, making CoRoT-14b one of the most dense gas giants known. [3]

    Related Research Articles

    <span class="mw-page-title-main">CoRoT</span> European space telescope that operated between 2006 - 2014

    CoRoT was a space telescope mission which operated from 2006 to 2013. The mission's two objectives were to search for extrasolar planets with short orbital periods, particularly those of large terrestrial size, and to perform asteroseismology by measuring solar-like oscillations in stars. The mission was led by the French Space Agency (CNES) in conjunction with the European Space Agency (ESA) and other international partners.

    <span class="mw-page-title-main">Hot Jupiter</span> Class of high mass planets orbiting close to a star

    Hot Jupiters are a class of gas giant exoplanets that are inferred to be physically similar to Jupiter but that have very short orbital periods. The close proximity to their stars and high surface-atmosphere temperatures resulted in their informal name "hot Jupiters".

    The Hungarian Automated Telescope Network (HATNet) project is a network of six small fully automated "HAT" telescopes. The scientific goal of the project is to detect and characterize extrasolar planets using the transit method. This network is used also to find and follow bright variable stars. The network is maintained by the Center for Astrophysics | Harvard & Smithsonian.

    <span class="mw-page-title-main">CoRoT-2b</span> Extrasolar planet in the constellation Aquila

    CoRoT-2b is the second extrasolar planet to be detected by the French-led CoRoT mission, and orbits the star CoRoT-2 at a distance of 700 light years from Earth towards the constellation Aquila. Its discovery was announced on 20 December 2007. After its discovery via the transit method, its mass was confirmed via the radial velocity method.

    This page describes exoplanet orbital and physical parameters.

    <span class="mw-page-title-main">CoRoT-3b</span> Brown dwarf or exoplanet orbiting CoRoT-3

    CoRoT-3b is a brown dwarf or massive extrasolar planet with a mass 21.66 times that of Jupiter. The object orbits an F-type star in the constellation of Aquila. The orbit is circular and takes 4.2568 days to complete. It was discovered by the French-led CoRoT mission which detected the dimming of the parent star's light as CoRoT-3b passes in front of it.

    CoRoT-2 is a yellow dwarf main sequence star a little cooler than the Sun. This star is located approximately 700 light-years away in the constellation of Aquila. The apparent magnitude of this star is 12, which means it is not visible to the naked eye but can be seen with a medium-sized amateur telescope on a clear dark night.

    <span class="mw-page-title-main">HAT-P-14b</span> Exoplanet in the constellation of Hercules

    HAT-P-14b, officially named Sissi also known as WASP-27b, is an extrasolar planet located approximately 224.2 ± 0.6 parsecs (731.2 ± 2.0 ly) away in the constellation of Hercules, orbiting the 10th magnitude F-type main-sequence star HAT-P-14. This planet was discovered in 2010 by the HATNet Project using the transit method. It was independently detected by the SuperWASP project.

    <span class="mw-page-title-main">K2-33b</span> Young Super-Neptune orbiting K2-33

    K2-33b is a very young super-Neptune exoplanet, orbiting the pre-main-sequence star K2-33. It was discovered by NASA's Kepler spacecraft on its "Second Light" mission. It is located about 456 light-years away from Earth in the constellation of Scorpius. The exoplanet was found by using the transit method, in which the dimming effect that a planet causes as it crosses in front of its star is measured.

    CoRoT-21b is a transiting exoplanet reportedly found by the CoRoT space telescope in 2011. Planetary parameters were published in 2012.

    CoRoT-10b is a transiting Hot Jupiter exoplanet found by the CoRoT space telescope in 2010.

    CoRoT-11b is a transiting Hot Jupiter-sized exoplanet found by the CoRoT space telescope in 2010.

    CoRoT-12b is a transiting Hot Jupiter-sized exoplanet found by the CoRoT space telescope in 2010.

    CoRoT-18b is a transiting Hot Jupiter exoplanet found by the CoRoT space telescope in 2011.

    CoRoT-20b is a transiting exoplanet found by the CoRoT space telescope in 2011.

    CoRoT-23b is a transiting Hot Jupiter exoplanet found by the CoRoT space telescope in 2011.

    References

    1. "Notes on CoRoT-14 b". Extrasolar Planets Encyclopaedia . Retrieved February 25, 2019.
    2. "COROT-14 Planets in the system" . Retrieved February 25, 2019.
    3. Tingley, B.; Endl, M.; Gazzano, J. -C.; Alonso, R.; Mazeh, T.; Jorda, L.; Aigrain, S.; Almenara, J. -M.; Auvergne, M.; Baglin, A.; Barge, P.; Bonomo, A. S.; Bordé, P.; Bouchy, F.; Bruntt, H.; Cabrera, J.; Carpano, S.; Carone, L.; Cochran, W. D.; Csizmadia, Sz.; Deleuil, M.; Deeg, H. J.; Dvorak, R.; Erikson, A.; Ferraz-Mello, S.; Fridlund, M.; Gandolfi, D.; Gillon, M.; Guenther, E. W.; et al. (2011). "Transiting exoplanets from the CoRoT space mission⋆ XIII. CoRoT-14b: an unusually dense very hot Jupiter". arXiv: 1101.1899 . doi:10.1051/0004-6361/201015480. S2CID   56139010.{{cite journal}}: Cite journal requires |journal= (help)

    See also