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“卡西尼号”第100次掠过泰坦卫星

(2014-03-14 11:12:08)
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健康

分类: 科学与技术

http://photos.state.gov/libraries/amgov/3234/Week_1/03062014_cassini20140305-640_jpg_600.jpg

2014.03.11

美国国家航空航天局的卡西尼号航天器高度下降,第100次掠过土星的卫星泰坦。

10年前,人类所知的泰坦(Titan)卫星是一个与水星(Mercury)大小相仿的、模糊的橙色球体。科学家当时知道它有由氮气组成的大气层——是除地球(Earth)外唯一有厚厚的氮气大气层的星球。但在朦胧的大气之下可能存在什么物质在当时仍只是一种猜想。

美国国家航空航天局(NASA)的卡西尼号(Cassini)航天器于3月6日下降到距离泰坦卫星1500千米内,进行第100次掠过土星(Saturn)卫星的飞行。每一次飞掠都让人类获得更多有关泰坦卫星的信息,以及它与地球明显的相似之处的知识。泰坦卫星即使表面冰冷,温度为零下179摄氏度(94开氏度),仍与早期处于深冻状态的地球相似。

自2004年抵达土星以来,卡西尼号上的雷达仪器已识别出泰坦卫星不同寻常的表面特征。包括由液态甲烷和乙烷形成的、比北美的五大湖(Great Lakes)还大的湖泊和海洋,以及表面以下深处大规模的液态水层。泰坦卫星大气中充满有机分子,它们是太阳辐射所分解的甲烷构成的。

上图是泰坦卫星可能具有的内部结构模型的艺术构想图。

有关泰坦卫星和卡西尼的详情请见美国国家航空航天局新闻简报



Read more: http://iipdigital.usembassy.gov/st/chinese/inbrief/2014/03/20140311296134.html#ixzz2vu3RO1Mj

http://photos.state.gov/libraries/amgov/3234/Week_1/03062014_cassini20140305-640_jpg_600.jpg

07 March 2014

NASA’s Cassini spacecraft swoops down to make its 100th flyby of Saturn’s moon Titan.

Ten years ago, humanity knew Titan as a fuzzy orange ball about the size of Mercury. Scientists knew it had a nitrogen atmosphere — the only known world with a thick nitrogen atmosphere besides Earth. But what might lie beneath the hazy air was still just a guess.

On March 6, NASA’s Cassini spacecraft swooped down within 1,500 kilometers of Titan to conduct its 100th flyby of the Saturn moon. Each flyby gives humanity a little more knowledge of Titan and its striking similarities to Earth. Even with its cold surface temperatures of minus 179 degrees Celsius (94 kelvins), Titan is like early Earth in a deep freeze.

Since its 2004 arrival at Saturn, Cassini’s radar instrument has identified remarkable surface features on Titan. The features include lakes and seas made of liquid methane and ethane, which are larger than North America’s Great Lakes, and an extensive layer of liquid water deep beneath the surface. Organic molecules abound in Titan’s atmosphere, formed from the breakup of methane by solar radiation.

Shown above is an artist’s conception of a possible model of Titan’s internal structure.

For more on Titan and Cassini, see the NASA press release.



Read more: http://iipdigital.usembassy.gov/st/english/inbrief/2014/03/20140307295587.html#ixzz2vu3ShsDn

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