其他受潮汐影响的卫星还有土星卫星以及海王星卫星。
Other moons affected by tidal forces are Enceladus (Saturn) and Triton (Neptune).
这些水分至今还以冰冻的形式存在于土星环，木星的卫星欧罗巴，海王星、天王星以及数以十亿计的彗星之中。
Most of it is still there, frozen solid in, among other things, the rings of Saturn, Jupiter's moon Europa, the bodies of Neptune and Uranus and billions upon billions of comets.
泰坦是最大的卫星…出来呀海王星。
这里可以看见它的已知3个卫星：冥卫1，冥卫2，和冥卫3。 包括冥王星在内的一群物体，在海王星的凯伯带（数十亿颗在海王星轨道之外绕行的小型冰体构成的碟形带）之上，围绕着太阳的作盘形轨道运行。
Seen here with its three known moons, Charon, Nix, and Hydra, Pluto is a member of a group of objects that orbit in a disklike zone beyond the orbit of Neptune called the Kuiper belt.
在木星、天王星、海王星的系统中，卫星的位置也和行星环的特性密切相关。
Correlations of satellite positions and ring features occur in the jovian uranian and neptunian systems as well.
海王星的命名来源于罗马神话中的海神（注：海神在罗马神话作''Neptune''，希腊神话中为波塞冬''Poseidon''）；而海王星的卫星被命名为崔顿（即海卫一），这个名字在罗马神话中意为海神最强大的武器。
Named after the Roman god of the sea; possessing a giant moon called Triton, named after Neptune's mighty weapon in Roman myth.
谷神星，小卫星带上的一颗矮卫星，以及比海王星更加远的矮卫星——冥王星，也可能拥有海洋。
Indeed so could Ceres, a dwarf planet in the asteroid belt, and Pluto, a dwarf planet even farther off than Neptune.
此时海王星、冥王星都是规则的，且适用于大多数卫星。
In this case Neptune and Pluto are regular, and so are mostly satellites.
海王星有两个卫星。
这里有一个寻找海王星的小提示，若你有个拥有精准长筒望远镜的朋友，你或许能看到海神——海王星最大的卫星。
There's a detailed article about how to find Neptune here. If you have a friend with a fair-sized telescope you may be able to see Triton, the biggest moon of Neptune.
这里有一个寻找海王星的小提示，若你有个拥有精准长筒望远镜的朋友，你或许能看到海神——海王星最大的卫星。
There's a detailed article about how to find Neptune here. If you have a friend with a fair-sized telescope you may be able to see Triton, the biggest moon of Neptune.
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