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First super-earths. [1] First planet discovered via radial velocity: 51 Pegasi b: 51 Pegasi: 1995 First convincing exoplanet discovered around a Sun-like star. [2] While the minimum mass of HD 114762 b was high enough (11 Jupiter-masses) that it could be a brown dwarf, 51 Peg b's minimum mass meant that it almost certainly was near the mass of ...
The IAU's names for exoplanets – and on most occasions their host stars – are chosen by the Executive Committee Working Group (ECWG) on Public Naming of Planets and Planetary Satellites, a group working parallel with the Working Group on Star Names (WGSN). [1] Proper names of stars chosen by the ECWG are explicitly recognised by the WGSN ...
List of proper names of exoplanets * Exoplanet naming convention; 0–9. 14 Andromedae b; 41 Lyncis b; 42 Draconis b; 47 Ursae Majoris b; 47 Ursae Majoris c; 51 Pegasi b;
0–9. List of exoplanets discovered before 2000; List of exoplanets discovered between 2000–2009; List of exoplanets discovered in 2010; List of exoplanets discovered in 2011
These are lists of planets.A planet is a large, rounded astronomical body that is neither a star nor its remnant. The best available theory of planet formation is the nebular hypothesis, which posits that an interstellar cloud collapses out of a nebula to create a young protostar orbited by a protoplanetary disk.
The exoplanet naming convention is an extension of the system used for naming multiple-star systems as adopted by the International Astronomical Union (IAU). For exoplanets orbiting a single star, the name is normally formed by taking the name of its parent star and adding a lowercase letter.
Exoplanets have been discovered using several different methods for collecting or combining direct images to isolate planets from the background light of their star. Non-Redundant Aperture Masking Interferometry is a method of combining the views of multiple telescopes into a single image, while the other methods are algorithms for combining ...
(g/cm 3) Orbital period Semimajor axis Orbital eccentricity Year of confirmation Ref. Earth (for reference) 0.003 15: 0.0892: 5.515: 365.2563: 1: 0.0167 — [1] TrES-2b (Kepler-1b) Transit: 1.197: 1.247: 0.8: 2.47061317: 0.0367 — 2006 [2] HAT-P-7b (Kepler-2b) Transit: 1.781: 1.419: 0.8: 2.2047354: 0.0355: 0: 2008 [3] HAT-P-11b (Kepler-3b ...