Meter-Scale Morphology of the North Polar Region of Mars

Author:

Herkenhoff K. E.1234,Byrne S.1234,Russell P. S.1234,Fishbaugh K. E.1234,McEwen A. S.1234

Affiliation:

1. Astrogeology Team, United States Geological Survey (USGS), Flagstaff, AZ 86001, USA.

2. Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ 85721, USA.

3. Physikalisches Institut, Universität Bern, CH-3012 Bern, Switzerland.

4. International Space Science Institute, CH-3012 Bern, Switzerland.

Abstract

Mars' north pole is covered by a dome of layered ice deposits. Detailed (∼30 centimeters per pixel) images of this region were obtained with the High-Resolution Imaging Science Experiment on board the Mars Reconnaissance Orbiter (MRO). Planum Boreum basal unit scarps reveal cross-bedding and show evidence for recent mass wasting, flow, and debris accumulation. The north polar layers themselves are as thin as 10 centimeters but appear to be covered by a dusty veneer in places, which may obscure thinner layers. Repetition of particular layer types implies that quasi-periodic climate changes influenced the stratigraphic sequence in the polar layered deposits, informing models for recent climate variations on Mars.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

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