... Temperatures at the Martiansurface vary from as low as about -195 degrees F (-125 degrees C) near the poles during the winter to as much as 70 degrees F (20 degrees C) at midday near the equator. ...
... The primary mission objectives were to obtain high resolution images of the Martiansurface, characterize the structure and composition of the atmosphere and surface, and search for evidence of life. ...
... can be identified with the formation of our Solar System and the development of life on this planet with its liquid surface ... Mars has become the center of intense interest since the Martian Meteorite results were announced. ...
... Цитировать None of the martian meteorites are weathered surface samples, but are all igneous rocks crystallized from molten lava near Mars' surface. ...
... and the techniques of map creation are the same with the Martian and Lunar maps ... 10 000 sq. km at the Venus surface, which corresponded with areas approximately more ...
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Ссылки http://selena.sai.msu.ru/Laz/Publications/6_Automatic%20creation%20of%20the%20hypsometric%20map%20of%20Venus.pdf -- 116.8 Кб -- 26.02.2009 Похожие документы
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