File:Hr8799_orbit_hd.gif · Wikimedia Commons · See Wikimedia Commons
Also known as extrasolar planet, exosolar planet
alt=Timelapse of exoplanets orbit motion|thumb|upright=1.5|Four exoplanets of the HR 8799 system imaged by the [[W. M. Keck Observatory over the course of seven years. Motion is interpolated from annual observations.]] thumb|295x295px|Comparison of the size of exoplanets orbiting Kepler-37 to Mercury, Mars and Earth An exoplanet or extrasolar planet is a planet outside of the Solar System. The first confirmed detection of an exoplanet was in 1992 around a pulsar, and the first detection around a main-sequence star was in 1995. A different planet, first detected in 1988, was confirmed in 2003.
An exoplanet is a planet that orbits a star outside our Solar System. Scientists have been detecting exoplanets since the early 1990s, which has expanded our understanding of how common planets may be throughout the universe.
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Discovered by embedding cosine similarity (sentence-transformers MiniLM, 384-dim).