Eros the dwarf planet








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Surface gravity depends on the distance from a spot on the surface to the center of a body's mass. An analysis of crater densities over the surface indicates that the areas with lower crater density are within 9 kilometers of the impact point. This article's use of external links may not follow Wikipedia's policies or guidelines. On January 31, , Eros passed Earth at 0. It rotates once every 5. Here is one of the final images. The NEAR Shoemaker probe visited Eros twice, first with a flyby , and then by orbiting it in when it extensively photographed its surface. Namespaces Article Talk. This page was last edited on 6 January , at Eros was one of the first asteroids visited by a spacecraft, the first one orbited, and the first one soft-landed on. Retrieved 13 December Views Read Edit View history. Wikimedia Commons has media related to Eros.

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Description: From Wikipedia, the free encyclopedia. NEAR scientists have found that most of the larger rocks strewn across Eros were ejected from a single crater in an impact approximately 1 billion years ago. Surface gravity depends on the distance from a spot on the surface to the center of a body's mass. Eros was the first asteroid detected by the Arecibo Observatory 's radar system. Eros has a giant gouge which was of interest. Here's a close-up image. By using this site, you agree to the Terms of Use and Privacy Policy. Dictionary of Minor Planet Names — Eros. Eros was one of the first asteroids visited by a spacecraft, the first one orbited, and the first one soft-landed on. During the opposition of —, a worldwide program was launched to make parallax measurements of Eros to determine the solar parallax or distance to the Sun , with the results published in by Arthur Hinks of Cambridge. Inside the gouge, however, only smaller craters are present, indicating that the area within the gouge is younger than the surface along the terminator.
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