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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...
If budget allows, the E-M10 Mark III is the superior choice, offering a significant leap in features while retaining the compact form factor. It boasts improved autofocus, better video capabilities, and modern connectivity. This camera is built for the modern hybrid shooter who needs reliability, ad...
Kepler-11c is an exoplanet orbiting the Sun-like star Kepler-11, located approximately 2,000 light-years from Earth in the constellation Cygnus. The Kepler-11 system, announced by NASA in 2011, is notable for having six confirmed transiting planets in a remarkably compact orbital configuration, with...
Third of six confirmed planets orbiting Kepler-11, part of the 2011 announcement that revealed how tightly packed planetary systems can be arranged within a single solar system.
Kepler-11e is a sub-Neptune exoplanet orbiting the Sun-like star Kepler-11, discovered by NASA's Kepler space telescope. As the fourth of six confirmed planets in this system, it completes an orbit around its host star approximately every 32 days. The planet is distinguished by its exceptionally low...
Kepler-11f is one of six known transiting planets orbiting the Sun-like star Kepler-11. Announced in 2011, it belongs to an unusually compact system in which five planets orbit closer to their star than Mercury does to the Sun. Transit timing variations allowed researchers to estimate planetary mass...
Kepler-11g is an extrasolar planet orbiting the sun-like star Kepler-11, located approximately 2,000 light-years from Earth. Announced by NASA in 2011, it is the largest and outermost of six confirmed planets within this densely packed planetary system. Unlike its five inner companions that orbit cl...
Innermost of five planets in the Kepler-62 system announced in 2013, a hot super-Earth orbiting its K-type host star every ~5.7 days, well inside the inner edge of the habitable zone.
Second planet in the Kepler-62 system announced in 2013, a small hot super-Earth orbiting its K-type star every ~12.4 days, too close to its host for conditions favorable to liquid water.
Super-Earth in the Kepler-62 system announced in 2013, roughly 1.95 times Earth's radius, orbiting its K-dwarf host every ~18.2 days just interior to the inner edge of the habitable zone.
