Asteroids小行星
![]() NASA Image from Ceres site Asteroids are small rocky bodies, most of which orbit the Sun between Mars and Jupiter. Their orbits are typically more eccentric than those of the planets. The largest asteroid, Ceres, is 940 kilometers in diameter and has about 1/10000 the mass of the Earth. With over 7000 asteroids catalogued, the total number may exceed 100,000. However, their combined mass is less than 1/10 that of the Earth's Moon. Ceres and the second-largest asteroid, Vesta, were visited by the Dawn spacecraft. 小行星是 rocky 的小天体,大多数绕太阳运行在火星和木星之间。它们的轨道通常比行星更偏心。最大的小行星,谷神星(Ceres),直径为940公里,其质量约为地球的1/10000。已 catalogued 的小行星超过7000个,总数可能超过100,000个。然而,它们的总质量不到地球月球质量的1/10。谷神星和第二大的小行星,灶神星(Vesta),已被 Dawn 探测器访问。
The vast majority of the meteorites that hit the Earth are thought to come from the asteroid belt. 绝大多数撞击地球的陨石被认为来自小行星带。
Asteroids are classified from their observed reflectivity, with C-type asteroids making up about 75% of them. C-type or carbonaceous asteroids are dark from the high content of carbon in them. S-type asteroids contain silicate and are more reflective - they make up about 15% of the asteroids. Most of the remaining asteroids are called M-type and contain large fractions of iron and nickel. The C-type asteroids are supposed to be very primitive material that has not been significantly heated or changed chemically since they were formed some 4.6 billion years ago. 小行星根据观测到的反照率进行分类,其中C型小行星约占75%。C型或碳质小行星因其中高含量的碳而显得暗淡。S型小行星含有硅酸盐,且更具有反射性,约占小行星的15%。其余大部分小行星被称为M型,其中含有大量铁和镍。C型小行星被认为是非常原始的物质,自约46亿年前形成以来,几乎没有受到显著的加热或化学变化。
References: 参考文献:NASA/小行星 Chapter 9 of Planetary Sciences by de Pater and Lissauer is a detailed treatment of asteroids. 《行星科学》(德帕特与利萨尔著)第九章对小行星进行了详细论述。
NASA 从Ceres网站图片 |
Index Solar System Illustration Solar System Concepts Reference Chaisson and McMillan Ch 14 索引 太阳系图示 太阳系概念 参考 Chaisson 和 McMillan 第14章 | ||
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