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Asteroid classification

机译:小行星分类

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Near-Earth asteroids and comets range in size between a few metres to tens of kilometres. They are essentially primordial material left over from the solar system's creation 4.6mn years ago. Ceres, now classified as a dwarf planet, was the largest asteroid with a diameter of 1,000 km. Comets consist of dust, water ice and frozen gases such as carbon dioxide and methane, that were formed in the outer solar system while rocky asteroids, also containing water ice and possibly other frozen gases, formed in the warmer space between the orbits of Jupiter and Mars. Planetary gravitational forces nudged them close to the Earth and Jupiter's gravity prevented them from accreting into planets.
机译:近地小行星和彗星的大小范围在几米到几十公里之间。它们本质上是460万年前太阳系产生后遗留下来的原始物质。谷神星现在被归类为矮行星,是最大的小行星,直径为1000公里。彗星由尘埃,水冰和冷冻气体(如二氧化碳和甲烷)形成,这些气体是在太阳系外部形成的,而岩石状的小行星也含有水冰和可能的其他冷冻气体,是在木星和木星轨道之间的较暖空间中形成的。火星。行星引力将它们推向靠近地球的位置,而木星的引力阻止它们吸积到行星中。

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