CoRoT-25b

Last updated
CoRoT-25b
Discovery
Discovered by CoRoT
Discovery date2013
Transit
Orbital characteristics
0.0578
Eccentricity 0
4.9 d
StarCoRoT-25
Physical characteristics
Mean radius
1.08 RJ
Mass 0.27 MJ

    CoRoT-25b is a gas giant exoplanet that orbits an F-type star. Its mass is 0.27 Jupiters, it takes 4.9 days to complete a single orbit of its star, and is 0.0578 AU from the star. Its discovery was announced in 2013. [1] [2]

    Related Research Articles

    <span class="mw-page-title-main">Super-Jupiter</span> Class of planets with more mass than Jupiter

    A super-Jupiter is a gas giant exoplanet that is more massive than the planet Jupiter. For example, companions at the planet–brown dwarf borderline have been called super-Jupiters, such as around the star Kappa Andromedae.

    <span class="mw-page-title-main">CoRoT-1b</span> Extrasolar planet orbiting CoRoT-1

    CoRoT-1b is a transiting extrasolar planet approximately 2,630 light-years away in the constellation of Monoceros. The planet was discovered orbiting the yellow dwarf star CoRoT-1 in May 2007. The planet was the first discovery by the French-led CoRoT Mission.

    <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.

    <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-4 is a yellow-white dwarf main-sequence star in the constellation Monoceros.

    <span class="mw-page-title-main">Extrasolar Planets Encyclopaedia</span> Astronomical database

    The Extrasolar Planets Encyclopaedia is an astronomy website, founded in Paris, France at the Meudon Observatory by Jean Schneider in February 1995, which maintains a database of all the currently known and candidate extrasolar planets, with individual pages for each planet and a full list interactive catalog spreadsheet. The main catalogue comprises databases of all of the currently confirmed extrasolar planets as well as a database of unconfirmed planet detections. The databases are frequently updated with new data from peer-reviewed publications and conferences.

    <span class="mw-page-title-main">CoRoT-1</span> Yellow dwarf star in the constellation Monoceros

    CoRoT-1 is a yellow dwarf main sequence star similar to the Sun. The star is located approximately 2,630 light-years away in the constellation of Monoceros. The apparent magnitude of this star is 13.6, which means it is not visible to the naked eye; however, it can be seen through a medium-sized amateur telescope on a clear, dark night. The first exoplanet discovered in the course of the CoRoT mission orbits this star; it is considered to be a "hot Jupiter", and is approximately as massive as the planet Jupiter itself.

    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">CoRoT-9b</span> Extrasolar planet in the constellation Serpens

    CoRoT-9b is an exoplanet orbiting the star CoRoT-9, approximately 1500 light years away in the constellation Serpens. CoRoT-9b's distance of nearest approach to its parent star of approximately 0.36 AU was the largest of all known transiting planets at the time of its discovery, with an orbital period of 95 days. The transit of this planet lasts 8 hours. The planet is at a distance from its star where there is a strong increase in albedo as the temperature decreases, because of the condensation of reflective water clouds in the atmosphere. This suggests its atmosphere may be locked into one of two states: a cloudless state with temperatures between 380 K and 430 K, or covered in water clouds with a temperature in the range 250 K to 290 K.

    CoRoT-13b is a transiting exoplanet found by the CoRoT space telescope on 12 July 2010.

    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.

    <span class="mw-page-title-main">CoRoT-14b</span>

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

    CoRoT-19b is a transiting exoplanet found by the CoRoT space telescope in 2011.

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

    K2-66b is a confirmed mega-Earth orbiting the subgiant K2-66, about 520 parsecs (1,700 ly) from Earth in the direction of Aquarius. It is an extremely hot and dense planet heavier than Neptune, but with only about half its radius.

    <span class="mw-page-title-main">YSES 2 b</span> Exoplanet orbiting YSES 2

    YSES 2 b is an exoplanet orbiting the star YSES 2 in the constellation of Musca. It was discovered through direct imaging by Bohn et al. in 2021. The planet is unusually far from its young host star.

    CoRoT-24c is a transiting exoplanet found by the CoRoT space telescope in 2011 and announced in 2014. Along with CoRoT-24b, it is one of two exoplanets orbiting CoRoT-24, making it the first multiple transiting system detected by the telescope. It is a hot Neptune orbiting at a distance of 0.098 AU from its host star.

    CoRoT-26b is a gas giant exoplanet that orbits a G-type star, CoRoT-26. It has a mass is 0.52 Jupiters, takes 4.2 days to complete one orbit of its star, and is 0.0526 AU from its star. Its discovery was announced in 2013.

    References

    1. Transiting exoplanets from the CoRoT space mission XXIV. CoRoT-25b and CoRoT-26b: two low-density giant planets
    2. "The Extrasolar Planet Encyclopaedia — CoRoT-25 b". Extrasolar Planets Encyclopaedia . Retrieved 4 September 2023.