Bilingual edition: English is preserved and Chinese follows each unit. Terminology uses the confirmed v20260916 glossary; automated semantic review remains traceable.
中英双语版:英文原文完整保留,中文紧随对应单元;术语采用 v20260916 确认表,自动语义审校结果可追溯。

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。

All solid bodies in our Solar Systen show craters where they have collided with asteroids and comets.

太阳系中的所有固体天体都显示出陨石和彗星碰撞形成的陨坑。

A few asteroids cross the Earth's orbit. The most notable of these are Apollo, Icarus, Adonis, and Eros. Hector has an orbit similar to that of Jupiter, and Hidalgo has a large elliptical orbit which extends from about the orbit of Mars out well beyond the orbit of Jupiter.

一些小行星穿越地球的轨道。其中最著名的是阿波罗、伊卡洛斯、阿多尼斯和 eros。赫克托的轨道类似于木星的轨道,而希达戈的轨道是一个很大的椭圆轨道,从火星的轨道延伸到木星轨道之外。

Asteroid Gaspra was used in slingshot maneuver with Galileo in 1991 on the way toward ultimate rendevouz with Jupiter. Galileo also provided a close view of asteroid Ida.

小行星Gaspra曾被用于伽利略探测器的引力弹弓 maneuver,于1991年在前往木星最终会合的途中。伽利略还提供了小行星Ida的近距离观测。

Another class of asteroids travel in a synchronous orbit with Jupiter and are called Trojan asteroids.

另一类小行星以同步轨道绕木星运行,被称为特洛伊小行星。

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:
NASA/Asteroids

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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