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An asteroid family is a population of asteroids that share similar proper orbital elements, such as semimajor axis, eccentricity, and orbital inclination. The members of the families are thought to be fragments of past asteroid collisions.
An asteroid is a minor planet—an object that is neither a true planet nor a comet—that orbits within the inner Solar System. They are rocky, metallic, or icy bodies with no atmosphere. The size and shape of asteroids vary significantly, ranging from small rubble piles under a kilometer across to Ceres, a dwarf planet almost 1000 ...
Pages in category "Background asteroids" The following 200 pages are in this category, out of approximately 15,388 total. This list may not reflect recent changes .
284996 Rosaparks, provisional designation 2010 LD58, is a dark background asteroid from the outer regions of the asteroid belt, approximately 3.5 kilometers (2.2 miles) in diameter. It was discovered on 9 June 2010 by scientists working with data from the Wide-field Infrared Survey Explorer spacecraft. [1]
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The asteroid belt is a torus-shaped region in the Solar System, centered on the Sun and roughly spanning the space between the orbits of the planets Jupiter and Mars. It contains a great many solid, irregularly shaped bodies called asteroids or minor planets.
Asteroids, sometimes called minor planets, are rocky remnants left over from the early formation of our solar system about 4.6 billion years ago. The current known asteroid count is: . Most of this ancient space rubble can be found orbiting our Sun between Mars and Jupiter within the main asteroid belt.
