卡西尼

The terrain seen here is located on the equator of Iapetus, in the transition region between the moon's bright and dark hemispheres.

我们现在看到的地域是Iapetus的赤道，在月球的黑白两面中间的过渡地区。2007年9月10日，卡西尼航天器的窄角相机拍摄了这张图片，当时相机距离Iapetus有大约9，240 千米（5，740里）。

This paper discusses the Western sources of the methods employed in the Lixiang Kaocheng Houbian (Later Edition of the Established System of Calendrical Astronomy) to resolve the Kepler Equation in calculating the solar and lunar equations of center.

研究《历象考成后编》中求解刻卜勒方程以计算日月中心差的方法的来源及其精度，同时对书中日月理论的总体精度进行分析，发现：书中用于太阳和月亮中心差计算的方法分别是薄利奥和卡西尼方法的简化版本。

The outer edge of the B ring which forms the inner boundary of the Cassini division is maintained by a gravitational resonance with Mimas. Near the outer edge of the A ring are the Encke Gap (325 kilometers, or 202 miles wide) and the barely visible Keeler Gap (35 kilometers, or 22 miles wide).

形成卡西尼环缝内缘的B环外侧的形状由其与土卫一的引力共振保持。A环外侧是恩克缝（宽325公里，202英里）和勉强能看到的科勒缝（宽35公里，22英里）。

A high-resolution closeup of Saturn's moon Mimas shows mysterious color differences around the huge Herschel crater. The combined picture, released March 29, 2010, is based on several shots taken by NASA's Cassini orbiter during its closest ever flyby of the tiny moon in February.

这是土卫一的一张高清特写照片，清晰的显示了巨大赫歇尔陨石坑周围不同颜色的神秘性。2010年3月29日美国宇航局公布了这张照片，它是由卡西尼号探测器于今年2月份飞过这颗卫星时，所拍摄到的几张照片拼合而成。

A high-resolution closeup of Saturn's moon Mimas shows mysterious color differences around the huge Herschel crater. The combined picture, released March 29, 2010, is based on several shots taken by NASA's Cassini orbiterduring its closest ever flyby of the tiny moon in February.

这是土卫一的一张高清特写照片，清晰的显示了巨大赫歇尔陨石坑周围不同颜色的神秘性。2010年3月29日美国宇航局公布了这张照片，它是由卡西尼号探测器于今年2月份飞过这颗卫星时，所拍摄到的几张照片拼合而成。

During the flyby, Cassini also captured the highest-resolution temperature map of Mimas, revealing an unexpected pattern of warm regions reminiscent of the arcade icon Pac-Man .Published March 30, 2010

在卡西尼号此次掠过土卫一飞行期间，它还捕获了土卫一高清晰的温度图谱，可以揭示其温暖地区令人意想不到的模式，而这张图能令人回忆起幼时常玩的"吃豆小精灵"。

The moonlet is too small to be resolved by Cassini's cameras, so its size cannot be measured directly.

因为它实在太小，以至于卡西尼携带的相机无法清晰分辨，因此其直径也无法直接测量。

Cassini , the robotic spacecraft orbiting Saturn that took this image , is not expected to survive to the next Saturnian equinox in 15 years.

卡西尼，围绕土星运行的机器人飞船，拍摄了这一张图片，当然，它是不可能支撑到土星的秋分的——那是15年之后的事了。

Cassini and curious Earthling s await the coming Saturnian equinox this summer when the ring plane will point directly at the Sun.

卡西尼和好奇的地球人正在等待土星夏季的春分来临，在那时环平面将直接指向太阳。

Cassini gathered information showing that Saturn's day is ten hours, forty-five minutes and forty-five seconds long. But that is about six minutes longer than information recorded by the spacecrafts Voyager One and Voyager two in nineteen eighty and nineteen eighty-one.

卡西尼收集的信息表明，土星的一天为十小时四十五分四十五钞，但这比航行者一号和航行者二号分别是于1980年和1981年所测定的时间要长六分钟。

I didn't watch TV last night, because it .

昨晚我没有看电视，因为电视机坏了。

Since this year, in a lot of villages of Beijing, TV of elevator liquid crystal was removed.

今年以来，在北京的很多小区里，电梯液晶电视被撤了下来。