• So to talk about where meteorites come from, we need to talk about comets and asteroids.

    那么讲到流星体从何而来,我们就需要讨论下彗星和小行星。

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  • Rubin suggests that asteroids' heat could have derived from collisions between asteroids.

    鲁宾认为,小行星的热量可能来自小行星之间的碰撞。

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  • Earth's crust contains very little of this element, but most asteroids contain a lot more.

    地壳中含有的这种元素很少,但大多数小行星上的要多得多。

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  • A recent discovery that asteroids are highly porous makes Rubin's hypothesis more plausible.

    最近的一项发现表明小行星非常多孔,这使得鲁宾的假设更加可信。

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  • I'm not going to go into any depth on comets and asteroids now, but we'll come back later and do that.

    我现在不打算深入讨论彗星和小行星了,但是我们稍后会再回到这个点上,讨论这方面的内容。

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  • The solar system also has two analogous classes of objects, smaller than planets—namely, asteroids and comets.

    太阳系也有两类类似的物体,比行星还小——即小行星和彗星。

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  • These asteroids are like the terrestrial planets, in that they're composed mostly of rocky material and metals.

    这些小行星像类地行星一样,主要由岩石物质和金属构成。

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  • The Sun is the hub of a huge rotating system consisting of nine planets, their satellites, and numerous small bodies, including asteroids, comets, and meteoroids.

    太阳是一个巨大的旋转系统的中心,这个旋转系统由九大行星、它们的卫星和无数的小天体组成,包括小行星、彗星和流星体。

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  • Skeptics have argued that a single impact would raise an asteroid's overall temperature very little and that asteroids would cool too quickly between impacts to accumulate much heat.

    怀疑派认为,一次撞击只会使小行星的整体温度上升很小,而且小行星在两次撞击之间会迅速冷却,从而无法积聚大量热量。

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  • Dr Bottke has been tracking the orbits of asteroids.

    伯克(Bottke)博士一直在追踪小行星的运行轨迹。

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  • If there were no asteroids would there be no extinctions?

    如果没有小行星,就不会有灭绝了吗?

    youdao

  • Astronomers know these condense into planets and asteroids.

    而天文学家知道这些云状物最终将凝结成大小行星。

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  • It's most likely the result of a recent collision between two asteroids.

    这很可能是两个小行星之间相撞产生的结果。

    youdao

  • Just as most orbiting planets spin on their axes, so asteroids also rotate.

    正如其它沿轨道运行的行星自转一样,这些小行星也有自转。

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  • Stars would stay fixed, but objects like comets, asteroids, and planets moved.

    通过这种方法可以观察到,恒星是固定不动的,而像彗星、小行星和行星这样的物体都在移动。

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  • Scale models of asteroids fill the windowsill of his office at JPL in Pasadena.

    在帕萨迪纳喷气推进实验室,他办公室的窗台上摆满了小行星按比例制作的模型。

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  • This goes on until the particles get to the size of boulders or small asteroids.

    这现象一直持续,直到微粒达到巨石或者是微型小行星的大小。

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  • Apollo asteroids pose a threat to our planet as they routinely cross Earth's orbit.

    阿波罗型小行星因定期地穿越地球轨道而构对地球的威胁。

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  • They have also looked for interesting asteroids, and kept an eye out for solar storms.

    业余天文学家们也已参与寻找有趣的小行星和观测太阳风暴。

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  • And a new study shows that asteroids weren't just passive couriers of organic material.

    并且新的研究显示,小行星并不只是被动地携带着有机物。

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  • It turns out that NASA is taking on that challenge, but not necessarily to chase asteroids.

    结果是美国国家航空航天管理局接受了那项挑战,但目的并不是一定要去追赶什么小行星。

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  • Astronomers group asteroids into different classes based on how the rocks reflect light in space.

    天文学家通过在太空中反射光的方式将小行星分门别类。

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  • Rock Farm: Most asteroids lie in the main belt [white] between Mars and Jupiter and pose no threat.

    太空岩石场:大部分小行星位于火星和木星之间的小行星带(图中白色部分),对地球没有威胁。

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  • The researchers observed 95 asteroids in the vicinity of our planet, called near-Earth asteroids (NEAs).

    研究人员们观测了95颗地球附近的小行星,它们被称为近地小行星(NEAs)。

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  • Many asteroids are weakly bound piles of rubble, held together by their own minute gravitational attraction.

    大多数的小行星都是由碎石组成,而这些碎石靠着自身之间微弱的万有引力结合在一起。

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  • A fragment from the same family of asteroids is thought to have wiped out the dinosaurs 65 million years ago.

    据认为,同一小行星家族的一个碎片曾经在六千五百万年前灭绝了恐龙。

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  • Hill and his fellow NEO hunters hope to detect large asteroids sooner, preferably years or decades in advance.

    希尔和他的同事希望能够更早地发现较大的小行星,最好提前几年或几十年。

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  • That's according to a survey of the sky that NASA is calling the most accurate census yet of near-Earth asteroids.

    这是根据美国宇航局(NASA)称之为“最准确的”一次近地小行星普查的结论。

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  • That's according to a survey of the sky that NASA is calling the most accurate census yet of near-Earth asteroids.

    这是根据美国宇航局(NASA)称之为“最准确的”一次近地小行星普查的结论。

    youdao

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