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The NASA Exoplanet Archive is an online astronomical exoplanet catalog and data service that collects and serves public data that support the search for and characterization of extra-solar planets (exoplanets) and their host stars.
To search for new exoplanets; rotating so by the end of its two-year mission it will have observed stars from all over the sky. It is expected to find at least 3,000 new exoplanets. CHEOPS: 2019 [45] Ongoing 2+ 0 To learn more about how exoplanets form, probe atmospheres, and characterize super-Earths. 20% of time will be open to community use ...
HD 38801 b is an extrasolar gas giant planet located in the constellation of Orion [3] whose discovery was announced in 2009 and was made using the radial velocity method. [4]
The Extrasolar Planets Encyclopaedia [9] is an astronomy website, founded in Paris, France at the Meudon Observatory by Jean Schneider in February 1995, [10] [11] which maintains a database of all the currently known and candidate extrasolar planets, with individual "note" pages for each planet and a full list interactive catalog spreadsheet ...
TOI-1601 b is an exoplanet that was discovered by TESS in January 2021. It has an orbital period of 5.3 days and is located 1098 light years away from Earth . It also has a mass similar to that of Jupiter .
OGLE-2005-BLG-390Lb (known sometimes as Hoth by NASA [1]) is a super-Earth ice exoplanet orbiting OGLE-2005-BLG-390L, a star 21,500 ± 3,300 light-years (6,600 ± 1,000 parsecs) from Earth near the center of the Milky Way, making it one of the most distant planets known.
G 9-40 b is a sub-Neptune exoplanet that has an orbital period of 5.7 days. The host star is a red dwarf located 91 light-years (28 parsecs ) away from Earth in the constellation Cancer . [ 4 ] The planet was discovered in 2019.
OGLE-2014-BLG-0124Lb is known as an exoplanet. These planets are located outside of our solar system. The Kepler telescope has allowed astronomers to discover thousands of these types of planets. Exoplanets obviously range in size, types, and orbits, but using this technique will help us search for planets that are of similar size to Earth.