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<p>features suggest the presence of ground ice (<a href="page.php?w=permafrost">permafrost</a>) and the movement of ice in <a href="page.php?w=glacier">glacier</a>s, both in the recent past and present. <a href="page.php?w=Gully_%28Mars%29">Gullies</a> and <a href="page.php?w=Seasonal_flows_on_warm_Martian_slopes">slope lineae</a> along cliffs and crater walls suggest that flowing water may continue to shape the surface of Mars, although what was thought to be low-volume liquid <a href="page.php?w=brine">brine</a>s in shallow <a href="page.php?w=Martian_soil">Martian soil</a>,</p><p>
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