Best Kepler
Kepler-186f is an exoplanet approximately Earth-sized orbiting the red dwarf star Kepler-186. It resides within its star’s habitable zone, meaning liquid water could potentially exist on its surface. This makes it notable as one of the first discovered planets similar in size to Earth and residing i...
William Borucki is a prominent astronomer recognized for his leadership of NASA’s Kepler space telescope. The Kepler mission, launched in 2009, utilized the transit method to discover thousands of exoplanets orbiting distant stars. This work significantly advanced our understanding of planetary syst...
Kepler-452b is an exoplanet orbiting a G-type star approximately 1,400 light-years from Earth. It’s notable as a super-Earth within its star's habitable zone, suggesting potential for liquid water on its surface. Scientists study this planet to understand the characteristics of potentially habitable...
Kepler-16b is a giant exoplanet orbiting two stars. Its notable feature is its circumbinary orbit, meaning it circles both stars simultaneously—a configuration similar to the fictional planet Tatooine. This discovery, made by NASA’s Kepler mission, offers scientists an opportunity to study planetary...
Kepler-1649c is an exoplanet roughly Earth-sized orbiting a red dwarf star named Kepler-1649. Its location within its star’s habitable zone—the region where liquid water could exist on the surface—makes it notable. Scientists study this super-Earth to assess the potential for habitability around M-d...
Kepler-442b is an exoplanet orbiting a cooler star approximately 1,200 light-years from Earth. Its size and position within its star’s habitable zone make it notable for potential liquid water on its surface. Scientists study this super-Earth to understand the diversity of planets capable of support...
Kepler-62f is an exoplanet located in the Kepler-62 system. It’s notable as a super-Earth orbiting a red dwarf star within its habitable zone. This means it receives approximately the same amount of energy from its star as Earth does, raising possibilities for liquid water on its surface. The planet...
Kepler-22b is an exoplanet orbiting a G-type star similar to our Sun. Discovered by NASA’s Kepler mission in 2011, it resides within its star's habitable zone, the region where liquid water could potentially exist on a planet’s surface. This “super-Earth,” roughly 2.4 times Earth’s size, is notable...
Natalie Batalha is an astronomer specializing in the study of exoplanets. Her leadership of the Kepler mission’s science team resulted in the discovery of numerous potential planets orbiting distant stars. This work significantly advanced our understanding of planetary systems beyond our own and is...
Kepler-90i is an Earth-sized exoplanet orbiting within the habitable zone of its star, Kepler-90. Its discovery in 2017 was notable as it represented the first confirmed system containing eight planets. The planet’s detection utilized machine learning analysis of data from NASA's Kepler mission. Thi...
Kepler-62e is an exoplanet orbiting the star Kepler-62. It’s notable as a super-Earth residing within its star's habitable zone, the region where liquid water could potentially exist on the planet’s surface. This makes it of interest to astronomers studying the possibility of other Earth-like worlds...
Kepler-78b is an Earth-sized rocky exoplanet announced in 2013, notable for being the first exoplanet confirmed to possess an Earth-like density and an iron-rock composition. It was discovered using data from NASA's Kepler space telescope and orbits a K-type star. The planet completes an orbit aroun...
Kepler-438b is a near-Earth-sized exoplanet confirmed by NASA in 2015, orbiting within the habitable zone of a red dwarf star located approximately 472 light-years away. It has a radius only 12 percent larger than Earth's, making it one of the most Earth-like planets discovered in terms of physical...
Kepler-69c is a super-Earth exoplanet announced in 2013, discovered using data from NASA's now-retired Kepler space telescope. It orbits a sun-like G-type star within the Kepler-69 system, positioned near the inner edge of the conservative habitable zone. Although its location initially suggested it...
David Latham is an American astronomer associated with the Harvard-Smithsonian Center for Astrophysics. He helped develop precise radial velocity techniques used to detect exoplanets by measuring small shifts in starlight, and he authored or co-authored hundreds of studies on planet detection and ch...
Kepler-138c is a super-Earth exoplanet located in the Kepler-138 system, confirmed by NASA's Kepler space telescope in 2015. It orbits its M-dwarf host star every 13.8 days and is believed to be a water world, with a significant portion of its mass consisting of water. The planet orbits in near reso...
Kepler-47c is a giant exoplanet orbiting in the Kepler-47 circumbinary system, which was announced in 2012. It holds the distinction of being the first circumbinary planet discovered orbiting within the habitable zone of its two host stars. Despite its placement in the habitable zone, the planet its...
Kepler-296f is a transiting exoplanet categorized as a super-Earth, located approximately 1,000 light-years away. Confirmed by NASA's Kepler mission in 2014, it orbits within the habitable zone of a binary star system composed of two red dwarfs. This positioning makes it a subject of ongoing study f...
Kepler-138d is a transiting exoplanet orbiting the M-dwarf star Kepler-138 approximately 200 light-years from Earth. It is the outermost of three known planets in the system, completing an orbit every 23.1 days. Categorized as a super-Earth, its mass and radius suggest a low bulk density. Researcher...
Kepler-47b is a transiting circumbinary exoplanet located in the Kepler-47 system, which was announced in 2012. It was part of the first system discovered to host multiple planets orbiting a binary star pair. The planet completes an orbit around the two host stars approximately every 49 days. It is...
Announced in 2011, Kepler-10b was the first confirmed rocky exoplanet discovered by NASA's Kepler space telescope. It is an ultrashort-period planet, completing a full orbit around its host star in less than a single Earth day. With a density comparable to solid iron, it is categorized as a super-Ea...
Super-Earth confirmed in 2014 orbiting within the habitable zone of Kepler-296, a red dwarf binary system ~1,200 light-years away, making it one of few potentially habitable planets known around a binary star.
Rocky super-Earth discovered in 2012 sharing an unusually close orbit with the larger Kepler-36c, with the two planets passing within 0.013 AU of each other — one of the tightest adjacent pairs known.
Kepler-36c is a transiting exoplanet orbiting the star Kepler-36 and was reported in 2012 from observations by NASA's Kepler mission. It is larger and less dense than neighboring Kepler-36b, indicating a substantial volatile envelope rather than a predominantly rocky composition. The two planets hav...
Kepler-10c is a transiting exoplanet orbiting Kepler-10, a Sun-like star also known to host the rocky planet Kepler-10b. With a radius of about 2.35 times Earth's, it was initially described as a massive, potentially rocky "mega-Earth" after an early mass estimate near 17 Earth masses. Later measure...
Kepler-138b is a Mars-sized exoplanet orbiting the red dwarf star Kepler-138, located roughly 217 light-years away in the constellation Lyra. Confirmed in 2015 using data from the Kepler space telescope, it was one of the smallest exoplanets to have both its mass and radius directly measured. This m...
Kepler-20f is a near-Earth-sized exoplanet orbiting the sun-like star Kepler-20, located approximately 929 light-years from Earth in the constellation Lyra. Confirmed alongside Kepler-20e in December 2011 by NASA's Kepler space telescope, the planet has a radius roughly 1.03 times that of Earth, mak...
Kepler-20e is an extrasolar planet orbiting the sun-like star Kepler-20, located approximately 950 light-years away from Earth. Detected by NASA's Kepler space telescope, its discovery was officially confirmed in December 2011, marking it as one of the first identified Earth-sized exoplanets. The pl...
Kepler-444 b is a rocky sub-Earth exoplanet orbiting the ancient K-type star Kepler-444, a system estimated to be approximately 11 billion years old. Discovered through transit photometry by NASA's Kepler space telescope and announced in 2015, it is the innermost of five known planets in the system....
Kepler-11b is a sub-Neptune exoplanet orbiting the Sun-like star Kepler-11, approximately 2,000 light-years from Earth. Announced in 2011, it is one of six confirmed planets in the Kepler-11 system, which was notable for having one of the most compact multi-planet configurations discovered. Kepler-1...
