Transiting exoplanets

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thumb | right | alt=Comparison of best-fit size of the exoplanet Kepler-9 b with the Solar System planet Jupiter, as reported in the Open Exoplanet Catalogue, 2015 | Comparison of best-fit size of the exoplanet Kepler-9 b with the Solar System planet Jupiter, as reported in the Open Exoplanet Catalogue, 2015 Kepler-15b is a planet discovered by the Kepler spacecraft. It is a hot Jupiter, with a mass of 0.66 MJ, a radius 0.96 RJ and a period of about 4.94 days.

Kepler-90e is an exoplanet orbiting the star Kepler-90, located in the constellation Draco. It was discovered by the Kepler telescope in October 2013. It orbits its parent star at only 0.42 astronomical units away, and at its distance it completes an orbit once every 91.94 days. thumb|center|600px|

thumb | right | Relative sizes of Earth, Kepler-24b and [[Jupiter]] Kepler-24b is an exoplanet orbiting the star Kepler-24, located in the constellation Lyra. It was discovered by the Kepler telescope in January 2012. It orbits its parent star at only 0.08 astronomical units away, and at its distance it completes an orbit once every 8.145 days.

candidate Exoplanet detected by Kepler space telescope

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Kepler-32c (alt. name KOI 952.02) is an extrasolar planet in orbit around its M-dwarf-type star in the Kepler-32 system, in the constellation of Cygnus. Discovered by planetary transit methods with the Kepler space telescope in January 2012, it presents a semi-major axis of 0.033 AU and temperature of 417.3 K. It has a radius of 2.2 Earth-radius and an orbital period of 8.7522 days.

Kepler-40b, formerly known as KOI-428b, is a hot Jupiter discovered in orbit around the star Kepler-40, which is about to become a red giant. The planet was first noted as a transit event by NASA's Kepler spacecraft. The Kepler team made data collected by its satellite publicly available, including data on Kepler-40; French and Swiss astronomers used the equivalent to one night of measurements on the SOPHIE échelle spectrograph to collect all the data needed to show that a planet was producing the periodic dimming of Kepler-40. The planet, Kepler-40b, is twice the mass of Jupiter and slightly

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thumb | right | alt=Comparative sizes of Earth, Kepler-23 c and Jupiter. | Comparative sizes of Earth, Kepler-23 c and Jupiter. Kepler-23c is a Neptune-sized exoplanet orbiting the star Kepler-23, located in the constellation Cygnus. The planet is 3.12 times wider than the Earth and is 0.189 Jupiter masses. The planet was discovered using data taken from the Kepler space telescope. It is likely a gas giant. The planets Kepler-23b and d both reside in the same planetary system.

thumb|right|alt=Comparison of best-fit size of the exoplanet CoRoT-11 b with the Solar System planet Jupiter|CoRoT-11 b beside Jupiter CoRoT-11b is a transiting Hot Jupiter-sized exoplanet found by the CoRoT space telescope in 2010. From obtained light curves and Bayesian inference on the data, it is highly likely that CoRoT-11b has been observed in a secondary eclipse around its host star (transiting behind it).

CoRoT-10b is a transiting Hot Jupiter exoplanet found by the CoRoT space telescope in 2010. ==Host star== CoRoT-10b orbits CoRoT-10 in the constellation of Aquila. It is a K1V star with Te = 5075K, M = 0.89M☉, R = 0.79R☉, above solar metallicity. It has an estimated age below 3.0 Gyr.

SWEEPS-10 is an extrasolar planet that, from June 2007 to August 2011, was the planet candidate with the shortest orbital period yet found, until PSR J1719-1438 b was discovered in 2011 with an even shorter orbit. The planet orbits the star SWEEPS J175902.00−291323.7 located in the Galactic bulge at a distance of approximately 22,000 light years from Earth (based on a distance modulus of 14.1).

exoplanet in the Neptunian Desert

Kepler-87c is a planet orbiting Kepler-87, a star slightly more massive than the Sun and nearing the end of its main-sequence period.

REDIRECT WASP-21 Category:Exoplanets discovered in 2010 Category:Exoplanets with proper names Category:Transiting exoplanets Category:Exoplanets discovered by WASP

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

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Kepler-447b is a confirmed exoplanet. The planet's mass and radius indicate that it is a gas giant with a bulk composition similar to that of Jupiter. Unlike Jupiter, but similar to many planets detected around other stars, Kepler-447b is located very close to its star, and belongs to the class of planets known as hot Jupiters. It has an extremely grazing transit, a property that could be used to detect further properties such as perturbations of the orbit due to other nearby objects or stellar pulsations.

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Kepler-432b (also known by its Kepler Object of Interest designation KOI-1299.01) is a hot super-Jupiter (or "warm" super-Jupiter) exoplanet orbiting the giant star Kepler-432 A, the innermost of two such planets discovered by NASA's Kepler spacecraft. It is located about 2,830 light-years (870 parsecs, or nearly km) from Earth in the constellation Cygnus. 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.

exoplanet

Kepler-453b is a transiting circumbinary exoplanet in the binary-star system Kepler-453. It orbits the binary system in the habitable zone every 240.5 days. The orbit of the planet is inclined relative to the binary orbit therefore precession of the orbit leads to it spending most of its time in a non-transiting configuration. By the time the TESS and PLATO spacecraft are available for follow up observations it will no longer be transiting.

Kepler-419b (also known by its Kepler Object of Interest designation KOI-1474.01) is a hot Jupiter exoplanet orbiting the star Kepler-419, the outermost of two such planets discovered by NASA's Kepler spacecraft. It is located about 3,400 light-years (1040 parsecs from Earth in the constellation Cygnus.

Kepler-395c is a potentially habitable exoplanet 616 light-years away in the constellation of Cygnus.

thumb|right|alt=Exoplanet CoRoT-14 b size comparison to Jupiter. Jupiter is on the left and is around 7.6 times less massive than CoRoT-14 b, which is white in colour|Exoplanet CoRoT-14 b size comparison to Jupiter CoRoT-14b is a transiting Hot Jupiter exoplanet found by the CoRoT space telescope in 2010.

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Kepler-68c is an Earth-sized planet orbiting the star Kepler-68 in the constellation of Cygnus. It was discovered by planetary-transit methods by the Kepler space telescope in February 2013. It has a mass of 4.8 times that of Earth (0.015 MJ) and a radius of 0.953 Earth radii. It has an orbital period of 9.605085 days at a distance of about 0.09059 AU from its star. Relatively wide constraints on Kepler-68c's mass are the result lack of detection of the planet through radial-velocity and transit-timing-variation methods.

Kepler-1708b (previously known as KIC 7906827.01) is a Jupiter-sized exoplanet orbiting the Sun-like star Kepler-1708, located in the constellation of Cygnus approximately 5,600 light years away from Earth. It was first detected in 2011 by NASA's Kepler mission using the transit method, but was not identified as a candidate planet until 2019. In 2021, a candidate Neptune-sized exomoon in orbit around Kepler-1708b was found by astronomer David Kipping and colleagues in an analysis using Kepler transit data. Some subsequent research has raised discrepancies about the possible existence of an exo

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exoplanet in the constellation Volans

exoplanet in the constellation Fornax

K2-24c also known as EPIC 203771098 c is an exoplanet orbiting the Sun-like star K2-24 every 42 days. It has a density far lower than that of Saturn, which indicates that the planet is clearly a gas giant.

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Kepler-91b is a giant planet orbiting Kepler-91, a star slightly more massive than the Sun. Kepler-91 has left the main sequence and is now a red giant branch star.

Kepler-28b is an extrasolar planet orbiting the star Kepler-28. It is a transiting planet that is smaller than Jupiter that orbits very closely to Kepler-28.

WASP-28b or K2-1b is an extrasolar planet discovered in 2010 by the Wide Angle Search for Planets (WASP) project orbiting WASP-28, a magnitude 12 star also known as 1SWASP J233427.87-013448.1, 2MASS J23342787-0134482 and K2-1. Since it orbits its star very closely, the planet is a strongly irradiated hot Jupiter. As seen from the Earth, WASP-28b transits its host star every 3.41 days taking about 3 hours to do so.

exoplanet in the constellation Boötes

K2-138b is a potentially rocky Super-Earth exoplanet orbiting every 2 days around a K1V star. The planet, along with the four others in the system, was found by citizen scientists of the Exoplanet Explorers project on Zooniverse. It was the final planet found in the system and was officially announced on January 8, 2018.

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HAT-P-24b is an extrasolar planet discovered by the HATNet Project in 2010 orbiting the F8 dwarf star HAT-P-24. It is a hot Jupiter, with a mass three quarters that of Jupiter and a radius 20% larger.

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CoRoT-22b is a transiting exoplanet smaller than Uranus found by the CoRoT space telescope in 2011 and confirmed in 2014.

HAT-P-33b is a planet in the orbit of HAT-P-33, which lies 1,310 light years away from Earth. Its discovery was reported in June 2011, although it was suspected to be a planet as early as 2004. The planet is about three-fourths the mass of Jupiter, but is almost eighty percent larger than Jupiter is; this inflation has, as with the discovery of similar planets WASP-17b and HAT-P-32b, raised the question of what (other than temperature) causes these planets to become so large.

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Kepler-296d is an exoplanet orbiting the M-dwarf star Kepler-296, located in the constellation Draco. It was discovered in 2014 by the Kepler space telescope using the transit method.

extrasolar planet in the constellation Ursa Major

Kepler-93b (KOI-69b) is a hot, dense transiting Super-Earth exoplanet located approximately away in the constellation of Lyra, orbiting the G-type star Kepler-93. Its discovery was announced in February 2014 by American astronomer Geoffrey Marcy and his team. In July 2014, its radius was determined with a mere 1.3% margin of error, the most precise measurement ever made for an exoplanet's radius at the time.

REDIRECT Kepler-51#Planetary system

database of stars and planets that is associated with the K2 "Second Light" plan of the Kepler space telescope mission

K2-3b, also known as EPIC 201367065 b, is an exoplanet orbiting the red dwarf K2-3 every 10 days. It is the largest and most massive planet of the K2-3 system, with about 2.1 times the radius of Earth and about 5 times the mass. Its density of about 3.1 g/cm3 may indicate a composition of almost entirely water, or a hydrogen envelope comprising about 0.7% of the planet's mass.

extrasolar planet

CoRoT-16b is a transiting exoplanet orbiting the G or K type main sequence star CoRoT-16 2,433 light years away in the southern constellation Scutum. The planet was discovered in June 2011 by the French-led CoRoT mission. CoRoT-16b was detected using the transit method, which measures the brightness changes during an eclipse. However, this planet has an eccentric orbit, which is unusual due to CoRoT-16b's proximity to its parent star and the age.

Kepler-1652b (also known by its Kepler Objects of Interest designation KOI-2626.01) is a super-Earth exoplanet, orbiting within the habitable zone of the red dwarf Kepler-1652 about 822 light-years away in the Cygnus constellation. Discovered by NASA's Kepler spacecraft, Kepler-1652b was first announced as a candidate in 2013, but wasn't validated until four years later in 2017. It is a potential super-Earth with 160% Earth's radius. The planet orbits well within the habitable zone of its system, the region where liquid water can exist on a planet's surface. The planet is an eyeball planet can