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  2. Asteroid belt - Wikipedia

    en.wikipedia.org/wiki/Asteroid_belt

    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.

  3. Solar System belts - Wikipedia

    en.wikipedia.org/wiki/Solar_System_belts

    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 ]

  4. List of exceptional asteroids - Wikipedia

    en.wikipedia.org/wiki/List_of_exceptional_asteroids

    Most highly inclined known main-belt asteroid from August 17, 1998, to October 19, 1998 MPC (88043) 2000 UE 110: 51.998° October 29, 2000 First main-belt asteroid discovered and numbered to have an inclination greater than 50°. MPC (138925) 2001 AU 43: 72.132° January 4, 2001 A Mars-crosser and near-Earth object. MPC (127546) 2002 XU 93: 77 ...

  5. (458271) 2010 UM26 and 2010 RN221 - Wikipedia

    en.wikipedia.org/wiki/(458271)_2010_UM26_and...

    2010 UM 26 and 2010 RN 221 both orbit the Sun in the middle zone of the main asteroid belt. They share extremely similar elliptical orbits with semi-major axes of 2.58 astronomical units (386 million km, 240 million mi) and orbital periods of 4.14 years.

  6. Category:Main-belt asteroids - Wikipedia

    en.wikipedia.org/wiki/Category:Main-belt_asteroids

    42 of the largest objects in the asteroid belt. If possible, asteroids should always be placed into one of the numerous sub-categories, in line with the category information given in the minor-planet catalog. Used sources: Small Body Data Ferret (Nesvorný) and AstDys (Milani and Knežević).

  7. Geology of Ceres - Wikipedia

    en.wikipedia.org/wiki/Geology_of_Ceres

    At a diameter of 964 km, Ceres is the largest object in the main asteroid belt and comprises about one-third of the belt's total mass. Ceres possesses sufficient gravity to form a rounded, ellipsoid shape, suggesting that it is close to being in hydrostatic equilibrium [ 6 ] —one of the conditions for defining a dwarf planet according to the ...

  8. 12373 Lancearmstrong - Wikipedia

    en.wikipedia.org/wiki/12373_Lancearmstrong

    12373 Lancearmstrong, provisional designation 1994 JE 9, is a bright Vestian asteroid from the inner regions of the asteroid belt, approximately 5 kilometers (3.1 miles) in diameter. It was discovered on 15 May 1994, by American astronomer and software engineer Charles de Saint-Aignan after examining films taken at Palomar Observatory ...

  9. 426 Hippo - Wikipedia

    en.wikipedia.org/wiki/426_Hippo

    426 Hippo is a rather large main-belt asteroid. It was discovered by Auguste Charlois on August 25, 1897, in Nice. In the 22nd century, it will come closer than 6,000,000 km (0.04 AU) to the larger asteroids 65 Cybele and 511 Davida. [2] Orbital diagram of Hippo