A new study reveals Mars’s missing water may have slowly seeped underground, becoming trapped in ancient aquifers beneath the surface.

The study proposes that fine dust particles from the Martian atmosphere settle on sloped terrain. Events like wind gusts, ...

Coupled with the complexity of subsurface flow routes, such as overflow behaviour from storage reservoirs, water movement to speleothems can be expected to display non-linear behaviour.

Images taken of Mars from orbit dating back as far as the 1970s have captured curious dark streaks running down the sides of ...

A new study by planetary scientists at Brown University and the University of Bern in Switzerland casts doubt on one of the ...

By studying seismic waves, researchers have found a layer deep beneath the surface of Mars that could contain enough liquid ...

Water movement in soil is closely linked with storage ... is fundamental to most land use decisions. B horizon: Subsurface soil horizons that are zones of accumulation of soil constituents ...

From the water’s surface, you can easily appreciate the beauty, vastness, and intrigue of the Great Lakes. Yet a subsurface dive truly begins ... by an operator who dictates the vehicle’s movements ...

The quick movement of water also adds additional pressure to ... water from seeping naturally into the ground, so it runs into subsurface cavities. Over time, this dissolves the limestone ...

Through subsurface imaging and lab experiments, Stanford scientists have shown how pressure buildup from water and vapor in the reservoir under Campi Flegrei can lead to earthquakes when the ...