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  2. Transiting Exoplanet Survey Satellite - Wikipedia

    en.wikipedia.org/wiki/Transiting_Exoplanet...

    ICON (Explorer 96) →. Wikinews has related news: NASA launches exoplanet-hunting satellite TESS. Transiting Exoplanet Survey Satellite ( TESS) is a space telescope for NASA 's Explorer program, designed to search for exoplanets using the transit method in an area 400 times larger than that covered by the Kepler mission. [ 6]

  3. Exoplanet - Wikipedia

    en.wikipedia.org/wiki/Exoplanet

    An exoplanet was defined by the following criteria: Objects with true masses below the limiting mass for thermonuclear fusion of deuterium (currently calculated to be 13 Jupiter masses for objects of solar metallicity) that orbit stars or stellar remnants are "planets" (no matter how they formed).

  4. Exoplanet orbital and physical parameters - Wikipedia

    en.wikipedia.org/wiki/Exoplanet_orbital_and...

    The eccentricity of an orbit is a measure of how elliptical (elongated) it is. All the planets of the Solar System except for Mercury have near-circular orbits (e<0.1). [ 8] Most exoplanets with orbital periods of 20 days or less have near-circular orbits, i.e. very low eccentricity.

  5. CHEOPS - Wikipedia

    en.wikipedia.org/wiki/CHEOPS

    CHEOPS (CHaracterising ExOPlanets Satellite) is a European space telescope.Its objective is to determine the size of known extrasolar planets, which will allow the estimation of their mass, density, composition and their formation.

  6. Massive exoplanet orbiting small star upends planet ... - AOL

    www.aol.com/massive-exoplanet-orbiting-small...

    A few massive planets have been found orbiting low-mass stars, such as the planet GJ 3512 b discovered in 2019, but their orbital periods are much longer, and the planets don’t orbit their stars ...

  7. Discoveries of exoplanets - Wikipedia

    en.wikipedia.org/wiki/Discoveries_of_exoplanets

    51 Pegasi b: In 1995 this became the first exoplanet orbiting a main-sequence star to have its existence confirmed.It is a hot Jupiter with a 4.2-day orbit. [12]47 Ursae Majoris b: In 1996 this Jupiter-like planet was the first long-period planet discovered, orbiting at 2.11 AU from the star with the eccentricity of 0.049.

  8. Proxima Centauri b - Wikipedia

    en.wikipedia.org/wiki/Proxima_Centauri_b

    Proxima Centauri b is the closest exoplanet to Earth, [20] at a distance of about 4.2 ly (1.3 parsecs). [5] It orbits Proxima Centauri every 11.186 Earth days at a distance of about 0.049 AU, [1] over 20 times closer to Proxima Centauri than Earth is to the Sun. [21] As of 2021, it is unclear whether it has an eccentricity [e] [24] but Proxima Centauri b is unlikely to have any obliquity. [25]

  9. Exomoon - Wikipedia

    en.wikipedia.org/wiki/Exomoon

    An exomoon or extrasolar moon is a natural satellite that orbits an exoplanet or other non-stellar extrasolar body. [ 2] Exomoons are difficult to detect and confirm using current techniques, [ 3] and to date there have been no confirmed exomoon detections. [ 4]