... L ike Mercury and the Moon, Mars appears to lack active plate tectonics at present; there is no evidence of recent horizontal motion of the surface such as the folded mountains so common on Earth . ...
... Distribution of coronae on surface of Venus in compliance with morphological parameters of inside depression of these ... and slide session 3 October 9:00-13:00 Session "The Moon, Titan, Mercury and Radiation Issues" Co-Chairs: M.A. Kreslavsky and A ...
... Mercury has an extra large core (relative to its diameter); the mantles of Mars and ... Earth's surface and thereby eliminate almost all traces of earlier geologic surface ...
... things being equal formation of a wave bunch is determined by velocity of seismic waves in besides surface structures of a planet crust, therefore for more densities of Mercury medium the minimal diameter of craters with the central hill exceeds 5 km ...
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Ссылки http://www.iki.rssi.ru/conf/2009elw/presentations/presentations_pdf/session4/khavroshkin_ELW.pdf -- 302.0 Кб -- 02.03.2009 Похожие документы
... The planet Mercury, only slightly larger, also lacks any atmosphere, while Mars, with 1/3 the Earth's surface gravity, only retains a very thin atmosphere. ...
... SOHO), show (top) magnetic fields on the sun's surface near the south solar pole; (middle) an ultraviolet image of the 1 million degree plumes from the same region; and (bottom) an ultraviolet image of the "quiet" solar atmosphere closer to the surface ...
... by composition: . terrestrial or rocky planets : Mercury, Venus, Earth, and Mars: . ... and metal and have relatively high densities, slow rotation, solid surfaces, no rings and few satellites. jovian or gas planets ...
... can see a little more than half the surface of the Moon, thanks to processes known ... the entire Moon follows that motion, librations reveal a little more of its surface ...