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      Mars Orbiter Laser Altimeter: Experiment summary after the first year of global mapping of Mars

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          Gridding with continuous curvature splines in tension

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            Evidence for recent groundwater seepage and surface runoff on Mars.

            Relatively young landforms on Mars, seen in high-resolution images acquired by the Mars Global Surveyor Mars Orbiter Camera since March 1999, suggest the presence of sources of liquid water at shallow depths beneath the martian surface. Found at middle and high martian latitudes (particularly in the southern hemisphere), gullies within the walls of a very small number of impact craters, south polar pits, and two of the larger martian valleys display geomorphic features that can be explained by processes associated with groundwater seepage and surface runoff. The relative youth of the landforms is indicated by the superposition of the gullies on otherwise geologically young surfaces and by the absence of superimposed landforms or cross-cutting features, including impact craters, small polygons, and eolian dunes. The limited size and geographic distribution of the features argue for constrained source reservoirs.
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              Mars Global Surveyor Thermal Emission Spectrometer experiment: Investigation description and surface science results

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                Author and article information

                Journal
                Journal of Geophysical Research: Planets
                J. Geophys. Res.
                American Geophysical Union (AGU)
                01480227
                October 25 2001
                October 25 2001
                : 106
                : E10
                : 23689-23722
                Article
                10.1029/2000JE001364
                bcced148-4cbc-413d-91fd-068792dcd280
                © 2001

                http://doi.wiley.com/10.1002/tdm_license_1

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