
HD 219134 b (HR 8832 b) is a super-Earth located just 21.25 light years from Earth in the direction of the Cassiopeia constellation. This planet is one of the closest known transiting exoplanets. It orbits a K-type star named HD 219134.The high-precision measurement of both its mass and radius has made HD 219134 b an important reference point for scientific studies on the densities and internal structures of rocky exoplanets. Based on the obtained data, its dense structure suggests that it likel
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Erhan Şencan

CoRoT-7b is one of the first terrestrial exoplanets discovered by the CoRoT (Convection, Rotation and planetary Transits) space telescope, led by the French space agency CNES (Centre National d'Études Spatiales) in collaboration with the European Space Agency (ESA). Announced in 2009, CoRoT-7b has become one of the key examples studied among super-Earth-class exoplanets with short orbital periods, due to its physical and dynamical characteristics.Discovery and Observational MethodCoRoT-7b was di
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Osman Özbay

Kepler-22b is an exoplanet orbiting the G-type main-sequence star Kepler-22 and located within the star’s habitable zone. Planet was detected by NASA’s Kepler Space Telescope using the transit method and confirmed in 2011. Kepler-22b holds a special place in exoplanet research because it was the first transiting exoplanet confirmed to reside within the habitable zone of its host star. habitable zoneDiscovery ProcessKepler-22b was discovered as part of NASA’s Kepler Mission. The Kepler Space Tele
ENMeltem Özmen

K2-155d is a super-Earth-type exoplanet orbiting the red dwarf star K2-155, located approximately 203 light years (62.2 parsecs) from Earth in the direction of the Taurus constellation. Discovered during NASA’s Kepler space telescope’s K2 mission, this planet has attracted scientific interest due to its orbital position near the inner edge of its host star’s habitable zone and climate modeling suggesting the potential presence of liquid water.DiscoveryThe exoplanet K2-155d was discovered using d
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Erhan Şencan

GJ 273 b, also known as Luyten b, is an exoplanet orbiting the red dwarf star GJ 273 (Luyten’s Star), located in the constellation Canis Minor at a distance of approximately 12.3 light years from Earth. Discovered in 2017, this planet belongs to the class of planets with masses greater than Earth’s and is classified as a “super-Earth”.It has been determined that GJ 273 b resides within the habitable zone of its host star and is relatively close to Earth. Due to these characteristics, the planet
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Erhan Şencan