Giant planets

HAT-P-14b, officially named Sissi and also known as WASP-27b, is an extrasolar planet located approximately 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.

extrasolar planet

extrasolar planet

Kepler-419c (also known by its Kepler Object of Interest designation KOI-1474.02) is a super-Jupiter exoplanet orbiting within the habitable zone of 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. The exoplanet was found by using the transit timing variation method, in which the variations of transit data from an exoplanet are studied to reveal a more distant companion.

extrasolar planet

extrasolar planet

OGLE-2003-BLG-235Lb/MOA-2003-BLG-53Lb is an extrasolar planet discovered in April 2004 by the OGLE and MOA collaborations. Its high mass indicates that it is most probably a gas giant planet similar to Jupiter. It is located around 4.3 AU away from its parent star.

extrasolar planet in the constellation Carina

extrasolar planet orbiting BD-17°63

extrasolar planet

extrasolar planet

extrasolar planet

extrasolar planet

extrasolar planet

extrasolar planet

extrasolar planet

extrasolar planet orbiting the star Kappa Coronae Borealis

OGLE-TR-113b is an extrasolar planet orbiting the star OGLE-TR-113.

extrasolar planet

thumb | right OGLE-2007-BLG-368Lb is an extrasolar planet located approximately 19,230 light-years away in the constellation of Scorpius, orbiting the star OGLE-2007-BLG-368L. This planet was detected on December 8, 2009 by the gravitational microlensing by Sumi. It has mass 6.94% of Jupiter (i.e. 22 times that of Earth) and is located 3.3 AU from the star when observed. Based on those properties it would classify as a Cold Neptune. It is the second Cold Neptune to be observed, the first being OGLE-2005-BLG-169Lb. This planet is most likely be similar to Uranus and Neptune in the Solar System

extrasolar planet

extrasolar planet

Exoplanets orbiting main sequence star HD 147018 of spectral type G

extrasolar planet

Kepler-12b is a hot Jupiter that orbits G-type star Kepler-12 some away. The planet has an anomalously large radius that could not be explained by standard models at the time of its discovery, almost 1.7 times Jupiter's size while being 0.4 times Jupiter's mass. The planet was detected by the Kepler spacecraft, a NASA project searching for planets that transit (cross in front of) their host stars. The discovery paper was published on September 5, 2011.

extrasolar planet

extrasolar planet

Kepler-39b (formerly known as KOI-423b), is a confirmed extrasolar object (either a Jovian planet or brown dwarf because of its mass) discovered orbiting the F-type star Kepler-39. It is eighteen times more massive than Jupiter, and is about five fourths its size. The planet orbits its host star at about 15% of the average distance between the Earth and Sun. Kepler-39b's host star was investigated by European astronomers along with three other stars, including the host star of Kepler-40b, using equipment at the Haute-Provence Observatory in France. Collection and analysis of data in late 2010

extrasolar planet

extrasolar planet

extrasolar planet

extrasolar planet

extrasolar planet

gas giant exoplanet orbiting Bosona star in constellation Aquarius

extrasolar planet orbiting HD 11964

extrasolar planet

extrasolar planet

extrasolar planet

extrasolar planet

extrasolar planet

extrasolar planet

extrasolar planet

extrasolar planet

extrasolar planet in the constellation Ursa Major

extrasolar planet

extrasolar planet

extrasolar planet

extrasolar planet

Kepler-90g (also known by its Kepler Object of Interest designation KOI-351.02) is a super-puff exoplanet orbiting the early G-type main sequence star Kepler-90, one of eight planets around this star discovered using NASA's Kepler space telescope. It is located about from Earth, in the constellation Draco. 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. It orbits its parent star about every 210.5 days at a distance of 0.71 astronomical units.

extrasolar planet

extrasolar planet orbiting HD 11506

extrasolar planet orbiting HIP 14810

extrasolar planet

extrasolar planet in the constellation Centaurus

extrasolar planet

extrasolar planet

extrasolar planet in the constellation Centaurus

extrasolar planet orbiting HD 132406

extrasolar planet

extrasolar planet orbiting the star HD 101930