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Orbiting Mars since October 2016, the European Space Agency's ExoMars spacecraft has made a startling discovery: Mars is lovely in spring. The orbiter's camera has captured images such as ice receding from the southern highlands, an impact crater encompassing black dune fields surrounded by red soil, and this one-taken on May 5, 2020, just as Mars passed its spring equinox-which shows a part of the floor of the Ius Chasma canyon. Ius Chasma is located in the western part of the Valles Marineris canyon system, which spans nearly a quarter of the circumference of Mars and is the largest known canyon in the solar system. But Ius Chasma itself is no slacker, measuring about 1,000 kilometers (621 miles) long and up to 8 kilometers (5 miles) deep, more than twice as long and four times as deep as Arizona's Grand Canyon. The varying colors on the canyon floor indicate different types of rock. Geologists believe that the lighter rocks are salts left behind after an ancient lake evaporated. By studying the role that water played in the formation of the canyon, researchers hope to develop a more precise timeline for climate change on ancient Mars.
机译:自2016年10月以来轨道火星,欧洲航天局的屈光宇宙飞船已经令人惊讶的发现:火星在春天很可爱。轨道器的摄像机已经捕获了诸如从南高区退回的冰块等图像,这是一个受到红土包围的黑沙丘场的冲击火山口,并且这是在2020年5月5日拍摄的,就像火星通过它的弹簧股份 - 这表明一部分ius chasma峡谷的地板。 IUS Chasma位于Valles Marineris Canyon系统的西部,该系统距离火星的四分之一距离,是太阳系中最大的已知峡谷。但IUS Chasma本身并没有懒散,衡量大约1000公里(621英里),长达8公里(5英里)深,两倍多,亚利桑那州的大峡谷深四次。峡谷地板上的不同颜色表示不同类型的岩石。地质学家认为,在古老的湖泊蒸发之后,较轻的岩石是盐留下的盐。研究人员希望在峡谷中扮演水中的作用,希望为古代火星的气候变化开发更精确的时间表。

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  • 来源
    《Air and Space》 |2020年第5期|8-1012|共4页
  • 作者

    MARK STRAUSS;

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