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This asteroid belt is also called the main asteroid belt or main belt to distinguish it from other asteroid populations in the Solar System. [ 1 ] The asteroid belt is the smallest and innermost known circumstellar disc in the Solar System.
The asteroid and comet belts orbit the Sun from the inner rocky planets into outer parts of the Solar System, interstellar space. [ 16 ] [ 17 ] [ 18 ] An astronomical unit , or AU, is the distance from Earth to the Sun, which is approximately 150 billion meters (93 million miles). [ 19 ]
English: This chart is based on data published in Gradie and Tedesco (1982). Source references: Gradie, J.; Tedesco, E. (June 1982). "Compositional Structure of the Asteroid Belt".
Most highly inclined known main-belt asteroid from September 26, 2008, to March 8, 2010 [citation needed] MPC: 2010 EQ 169: 91.606° March 8, 2010 Most highly inclined known main-belt asteroid (orbit is not well-known) [citation needed] MPC: 2024 TF 3: 89.154° March 8, 2010 Extremely high-inclined trans-Neptunian object. [citation needed] MPC
Parts-per-million chart of the relative mass distribution of the Solar System, each cubelet denoting 2 × 10 24 kg. This article includes a list of the most massive known objects of the Solar System and partial lists of smaller objects by observed mean radius.
outer main-belt (a > 2.82 AU) A plot of inner solar system asteroids and planets as of 2006 May 9, in a manner that exposes the Kirkwood gaps. Similar to the position plot, planets (with trajectories) are orange, Jupiter being the outer most in this view. Various asteroid classes are colour coded: 'generic' main-belt asteroids are white.
Venus-crosser asteroid: 66391 Moshup: 0.642: Aten asteroid, Mercury-crosser asteroid, Venus-crosser asteroid: Objects in Venus's zone of influence (33342) 1998 WT 24: 0.718: Aten asteroid, Mercury-crosser asteroid, Venus-crosser asteroid. Venus: 0.723: Planet: 524522 Zoozve: 0.724: Aten asteroid, Mercury-crosser asteroid, Venus-crosser asteroid ...
The total mass of the asteroid belt is estimated to be 2.39 × 10 21 kg, which is just 3% of the mass of the Moon; the mass of the Kuiper Belt and Scattered Disk is over 100 times as large. [48] The four largest objects, Ceres, Vesta, Pallas, and Hygiea, account for maybe 62% of the belt's total mass, with 39% accounted for by Ceres alone.