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  2. File:VLT asteroid images aa41781-21 (Figure 1a).pdf - Wikipedia

    en.wikipedia.org/wiki/File:VLT_asteroid_images...

    You are free: to share – to copy, distribute and transmit the work; to remix – to adapt the work; Under the following conditions: attribution – You must give appropriate credit, provide a link to the license, and indicate if changes were made. You may do so in any reasonable manner, but not in any way that suggests the licensor endorses ...

  3. Asteroid belt - Wikipedia

    en.wikipedia.org/wiki/Asteroid_belt

    However, Centaurs and TNOs are unlikely to have significantly dispersed young asteroid families in the main belt, although they can have perturbed some old asteroid families. Current main belt asteroids that originated as Centaurs or trans-Neptunian objects may lie in the outer belt with short lifetime of less than 4 million years, most likely ...

  4. 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 ]

  5. 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).

  6. Nasa’s James Webb telescope looks at asteroid belt outside ...

    www.aol.com/nasa-james-webb-telescope-looks...

    Fomalhaut asteroid belt is far more complex than researchers had realised Nasa’s James Webb telescope looks at asteroid belt outside our solar system – and finds surprise Skip to main content

  7. (458271) 2010 UM26 and 2010 RN221 - Wikipedia

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

    (458271) 2010 UM 26 and 2010 RN 221 are a pair of sub-kilometer-sized asteroids that have extremely similar orbits in the main asteroid belt.These two asteroids are thought to have dissociated from a binary system sometime in the 2000s, which would make them one of the youngest asteroid pairs known.

  8. Small Solar System body - Wikipedia

    en.wikipedia.org/wiki/Small_Solar_System_body

    The orbits of the vast majority of small Solar System bodies are located in two distinct areas, namely the asteroid belt and the Kuiper belt. These two belts possess some internal structure related to perturbations by the major planets (particularly Jupiter and Neptune, respectively), and have fairly loosely defined boundaries. Other areas of ...

  9. 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 ...