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Phobos 火卫一(英)

Phobos 火卫一(英)

Phobos (FOH bus) is the larger and innermost of Mars' two moons. Phobos is closer to its primary than any other moon in the solar system, less than 6000 km above the surface of Mars. It is also one of the smallest moons in the solar system.
  orbit: 9378 km from the center of Mars
  diameter: 22.2 km (27 x 21.6 x 18.8)
  mass: 1.08e16 kg
  In Greek mythology, Phobos is one of the sons of Ares (Mars) and Aphrodite (Venus). phobos is Greek for fear (the root of phobia).
  Discovered 1877 August 18 by Hall; photographed by Mariner 9 in 1971, Viking 1 in 1977, and Phobos in 1988.
  Phobos orbits Mars below the synchronous orbit radius. Thus it rises in the west, moves very rapidly across the sky and sets in the east, usually twice a day. It is so close to the surface that it cannot be seen above the horizon from all points on the surface of Mars.
  And Phobos is doomed: because its orbit is below synchronous altitude tidal forces are lowering its orbit (current rate: about 1.8 meters per century). In about 50 million years it will either crash onto the surface of Mars or (more likely) break up into a ring. (This is the opposite effect to that operating to raise the orbit of the Moon.)
  Phobos and Deimos may be composed of carbon-rich rock like C-type asteroids. But their densities are so low that they cannot be pure rock. They are more likely composed of a mixture of rock and ice. Both are heavily cratered. New images from Mars Global Surveyor indicate that Phobos is covered with a layer of fine dust about a meter thick, similar to the regolith on the Earth's Moon.
  The Soviet spacecraft Phobos 2 detected a faint but steady outgassing from Phobos. Unfortunately, Phobos 2 died before it could determine the nature of the material; water is the best bet. Phobos 2 also returned a few images (right).
  The most prominent feature on Phobos is the large crater named Stickney, the maiden name of Hall's wife (above). Like Mimas' crater Herschel (on a smaller scale) the impact that created Stickney must have almost shattered Phobos. The grooves and streaks on the surface were probably also caused by the Stickney impact.
  Phobos and Deimos are widely believed to be captured asteroids. There is some speculation that they originated in the outer solar system rather than in the main asteroid belt.
  Phobos and Deimos may someday be useful as space stations from which to study Mars or as intermediate stops to and from the Martian surface; especially if the presence of ice is confirmed.
[Chinese Version]

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回复:Phobos 火卫一(英)

Phobos 是火星的两颗卫星中较大,也是离火星较近的一颗。火卫一与火星之间的距离也是太阳系中所有的卫星与其主星的距离中最短的,从火星表面算起,只有6000千米。它也是太阳系中最小的卫星之一。

    公转轨道:距火星中心9378 千米

    卫星直径:22.2 千米 (27 x 21.6 x 18.8)

    质量:1.08e16 千克

    在希腊神话中,火卫一是阿瑞斯(火星)和阿芙罗狄蒂(金星)的一个儿子。“phobos”在希腊语中意味着“恐惧”(是“phobia”-恐惧的构词成分)。

    火卫一在1877年由Hall发现,1971年由“水手9号”首次拍得照片,并由1977年的“海盗1号”、1988年的“火卫一号”进行观测。

    火卫一的环绕运动半径小于同步运行轨道半径,因此它的运行速度快,通常每天有两次西升东落的过程。由于它离火星表面过近,以至于从火星表面的任何角度都无法在地平线上看到它。

    据推断,由于它的运行轨道小于同步运行的轨道,所以潮汐力正不断地使它的轨道越变越小(最近的统计数字表明,它正以每世纪1.8米的速度在减小)。所以,据估计大约5000万年后,火卫一不是撞向火星,便是分解而成为光环。(这同月亮的升力的反作用力的作用效果相似。)

    火卫一和火卫二可能像C型小行星一样是由富含碳的岩石组成的。但它们不可能是由纯岩石组成的,因为它们的密度太低了。它们很可能是由岩石与冰的混合物组成的,并且它们都有很深的地壳坑。

    前苏联的探测器火卫一2号探测到一种从Phobos上逸出的微弱但又持久的气体。可惜的是,Phobos 2号在探测出这气体的组成成份之前便无法工作了。水或许是最有可能的组成部分。

    Phobos上最显著的地形特色是一个名为Stickney的大坑,这是前面所提到的Hall的妻子的名字。就像土卫一的环形山赫歇耳(Herschel)一样(尺寸较小)。Stickney必然曾经具有过破坏火卫一的作用,现在火卫一表面上的一些大沟和条纹层脉极有可能是由于Stickney的影响而造成的。

    火卫一和火卫二大多被认为是捕捉到的小行星,也有一些人认为它们是起源于太阳系外的,而不是来自于小行星带。

    火卫一和火卫二或许某天会成为了解火星的、非常重要的“空间站”。特别是随着冰的存在的事实,它便是成为了研究火星的中转站。

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Thebe 木卫十四(中英对照)

Thebe is the fourth of Jupiter's known satellites:
    orbit: 222,000 km from Jupiter
    diameter: 100 km (100 x 90)
    mass: 7.77e17 kg
    Thebe was a nymph, daughter of the river god Asopus.
    Discovered by Synnott in 1979 (Voyager 1).
    Thebe 是离木星第四近的一颗卫星:
    公转轨道:距木星 222,000 千米
    卫星直径:100 千米(100×90)
    质量:7.77e17 千克
    Thebe是位仙女,河神Asopus的女儿。
    它由Synnott于1979年发现 (旅行者1号)。

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Amalthea 木卫五(中英对照)

Amalthea is the third of Jupiter's known satellites:
    orbit: 181,300 km from Jupiter
    diameter: 189 km (270 x 166 x 150)
    mass: 3.5e18 kg ?
    Amalthea was the nymph who nursed the infant Jupiter with goat's milk.
    Discovered by Barnard 1892 September 9 using the 36 inch (91 cm) refractor at Lick Observatory. Amalthea was the last moon to be discovered by direct visual observation (as opposed to photography).
    Amalthea and Himalia are Jupiter's fifth and sixth largest moons; they are about the same size but only 1/15 the size of next larger one, Europa.
    Like most of Jupiter's moons, Amalthea rotates synchronously; its long axis is pointed toward Jupiter.
    Amalthea is the reddest object in the solar system. The reddish color is apparently due to sulfur originating from Io.
    Earlier, it was thought that its size and irregular shape should imply that Amalthea is a fairly strong, rigid body. But measurements of its mass made during Galileo's last orbit indicate otherwise. It now appears that Amalthea's density is only about the same as water and since it is unlikely to be composed of ice it is most likely a loose rubble pile with a lot of empty spaces.
    Like Io, Amalthea radiates more heat than it receives from the Sun (probably due to the electrical currents induced by Jupiter's magnetic field).
    Amalthea 是已知卫星中离木星第三近的一颗:
    公转轨道:距木星 181,300 千米
    卫星直径:189 千米(270×166×150)
    质量:7.17e18 千克
    Amalthea是一位用山羊奶照顾朱比特成人的仙女。
    它于1892年9月9日由Barnard于Lick天文台用36英尺(91厘米)折射望远镜发现。木卫五是最后一颗直接用视觉观察发现的卫星(相对于摄相而言)。
    木卫五与木卫六是木星第五与第六大卫星,它们的大小是第四大卫星木卫二的15分之一。
    像大多数的木星卫星,木卫五同步自转,它的长轴直指木星。
    木卫五是太阳系中最红的物体。红色可能是由木卫一发出的含硫物质造成的。
    它的大小及不规则外形意味着它是一个相当坚硬的物体。它的组成更像是一颗小行星而不是伽利略类的卫星。
    与木卫一类似,木卫五辐射出的热量比从太阳处收到的多(可能是因为木星磁场感应出的电流的关系)。

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Adrastea 木卫十五(中英对照)

Adrastea is the second of Jupiter's known satellites:
    orbit: 129,000 km from Jupiter
    diameter: 20 km (23 x 20 x 15)
    mass: 1.91e16 kg
    Adrastea, the distributor of rewards and punishments, was the daughter of Jupiter and Ananke.
    Discovered by graduate student David Jewitt (working under Danielson) in 1979 (Voyager 1).
    Metis and Adrastea orbit inside the synchronous orbit radius and inside the Roche limit. They may be small enough to avoid tidal disruption but their orbits will eventually decay.
    Adrastea is one of the smallest moons in the solar system.
    Adrastea 是已知卫星中离木星第二近的一颗:
    公转轨道:距木星 129,000 千米
    卫星直径:20 千米(23×20×15)
    质量:1.91e16 千克
    Adrastea是奖赏和惩罚的分配者,是朱比特(木星)与Ananke(木卫十二)的女儿。
    它是研究生David Jewitt(在丹尼尔森手下工作)于1979年发现(旅行者1号)。
    木卫十六与木卫十五的公转轨道处在同步公转轨道半径之内,并在Roche极限之内。它们太小以致于能避免引潮力把它们拉碎,但它们的轨道将逐渐变小,最终坠入木星。
    木卫十五是太阳系中最小的卫星之一。

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Metis 木卫十六(中英对照)

Metis is the innermost of Jupiter's known satellites:
    orbit: 128,000 km from Jupiter
    diameter: 40 km
    mass: 9.56e16 kg
    Metis was a Titaness who was the first wife of Zeus (Jupiter).
    Discovered by Synnott in 1979 (Voyager 1).
    Metis and Adrastea lie within Jupiter's main ring. They may be the source of the material comprising the ring.
    Small satellites within a planet's rings are sometimes called moons.
    Metis 是已知木星卫星中离木星最近的一颗:
    公转轨道:  距木星 128,000 千米
    卫星直径:  40 千米
    质量:  9.56e16 千克
    Metis是位女巨人,也是宙斯(木星)的第一任妻子。
    它是Synnott于1979年发现的(由旅行者1号拍摄)。
    木卫十六与木卫十五存在于木星主光环之内。它们可能是光环物质的主要来源。
    在行星光环内的小卫星有时被称为“moons”。

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