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6 Hebe : ウィキペディア英語版
6 Hebe

6 Hebe ( ) is a large main-belt asteroid, containing around half a percent of the mass of the belt. However, due to its apparently high bulk density (greater than that of the Moon or even Mars), Hebe does not rank among the top twenty asteroids by volume. This high bulk density suggests an extremely solid body that has not been impacted by collisions, which is not typical of asteroids of its size – they tend to be loosely bound rubble piles.
In brightness, Hebe is the fifth brightest object in the asteroid belt after Vesta, Ceres, Iris and Pallas. It has a mean opposition magnitude of +8.3, about equal to the mean brightness of Titan,〔(The Brightest Asteroids )〕 and can reach +7.5 at an opposition near perihelion.
Hebe is probably the parent body of the H chondrite meteorites, which account for about 40% of all meteorites striking Earth.
==History==
Hebe was discovered on 1 July 1847 by Karl Ludwig Hencke, the sixth asteroid discovered. It was the second and final asteroid discovery by Hencke, after 5 Astraea. The name ''Hebe'', goddess of youth, was proposed by Carl Friedrich Gauss.

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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