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<b> Buried craters and underground ice</b><br /><br /><i>30 November 2005<br />For the first time in the history of planetary exploration, the MARSIS radar on board ESA's Mars Express has provided direct information about the deep subsurface of Mars. <br /><br />First data include buried impact craters, probing of layered deposits at the north pole and hints of the presence of deep underground water-ice. <br /><br />The subsurface of Mars has been so far unexplored territory. Only glimpses of the Martian depths could be deduced through analysis of impact crater and valley walls, and by drawing cross-sections of the crust deduced from geological mapping of the surface. <br /><br />With measurements taken only for a few weeks during night-time observations last summer, MARSIS - the Mars Advanced Radar for Subsurface and Ionospheric Sounding - is already changing our perception of the Red Planet, adding to our knowledge the missing 'third' dimension: the Martian interior. </i><br /><br />Full Story Here: http://www.esa.int/SPECIALS/Results_from_Mars_Express_and_Huygens/SEM7ZTULWFE_0.html<br /><br /><b>Photo caption</b>:<br /><br /><i>These MARSIS 'radargram' images show echoes obtained from an approximately 250 km diameter circular structure in the subsurface of Mars, interpreted to be a buried impact basin. In both orbits, which are spaced about 50 km apart, MARSIS detected a series of arc-shaped reflectors that have no apparent source in the surface topography or geology. <br />In the lower image, a linear reflector nearly parallel to the surface is seen embedded in the arcs. This reflection may be coming from the floor of the basin. The time delay to the linear reflector suggests a depth of 1.5-2.5 km. </i><br /><br />From: http://www.esa.int/SPECIALS/Results_from_M <div class="Discussion_UserSignature"> <strong><font color="#3366ff">Made weak by time and fate, but strong in will to strive, to seek, to find and not to yeild.</font> - <font color="#3366ff"><em>Tennyson</em></font></strong> </div>