5973 Takimoto
Near-Earth Object, Small Solar System Body, Centaur (Minor Planet), Kuiper Belt
Herausgegeben: Valère Kresten, Proteus
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5973 Takimoto (1991 QC) is a main-belt asteroid discovered on August 17, 1991 by S. Otomo at Kiyosato. Asteroids (from Greek 'star' and 'like, in form') are a class of small Solar System bodies in orbit around the Sun. They have also been called planetoids, especially the larger ones. These terms have historically been applied to any astronomical object orbiting the Sun that did not show the disk of a planet and was not observed to have the characteristics of an active comet, but as small objects in the outer Solar System were discovered, their volatile-based surfaces were found to more closel...
5973 Takimoto (1991 QC) is a main-belt asteroid discovered on August 17, 1991 by S. Otomo at Kiyosato. Asteroids (from Greek 'star' and 'like, in form') are a class of small Solar System bodies in orbit around the Sun. They have also been called planetoids, especially the larger ones. These terms have historically been applied to any astronomical object orbiting the Sun that did not show the disk of a planet and was not observed to have the characteristics of an active comet, but as small objects in the outer Solar System were discovered, their volatile-based surfaces were found to more closely resemble comets, and so were often distinguished from traditional asteroids.
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