Details

Autor(en) / Beteiligte

• Stuurman, C. M.
• Osinski, G. R.
• Holt, J. W.
• Levy, J. S.
• Brothers, T. C.
• Kerrigan, M.
• Campbell, B. A.

Titel

SHARAD detection and characterization of subsurface water ice deposits in Utopia Planitia, Mars

Ist Teil von

• Geophysical research letters, 2016-09, Vol.43 (18), p.9484-9491

Ort / Verlag

Washington: John Wiley & Sons, Inc

Erscheinungsjahr

2016

Quelle

Wiley

Beschreibungen/Notizen

• Morphological analyses of Utopia Planitia, Mars, have led to the hypothesis that the region contains a substantial amount of near‐surface ice. This paper tests this hypothesis using ground‐penetrating radar techniques. We have identified an expansive radar reflective region spanning approximately 375,000 km2 in SHAllow RADar (SHARAD) data over western Utopia Planitia. The SHARAD reflective regions coincides with high densities of scalloped depressions and polygonal terrain. The reflectors are associated with layered mesas ∼80–170 m thick. We find a value of 2.8 ± 0.8 for the dielectric constant of the material overlying the reflectors. This work finds that the dielectric constant is consistent with a mixture of ice, air, and dust, containing a water ice volume up to 14,300 km3 in this unit. Key Points Layered mesas up to 170 m high in western Utopia Planitia, Mars, exhibit periglacial morphologies SHARAD data were used to map a regional subsurface reflector associated with the layered mesas The dielectric constant is consistent with a 50‐85% water ice composition, with an ice volume of up to 14,300 km3