Bright dunes on Mars View Full Text


Ontology type: schema:ScholarlyArticle     


Article Info

DATE

1999-02

AUTHORS

P. C. Thomas, M. C. Malin, M. H. Carr, G. E. Danielson, M. E. Davies, W. K. Hartmann, A. P. Ingersoll, P. B. James, A. S. McEwen, L. A. Soderblom, J. Veverka

ABSTRACT

Seasonal changes observed on the surface of Mars can in part be attributed to the transport of geological materials by wind1. Images obtained by orbiting spacecraft in the 1970s showed large wind-formed features such as dunes, and revealed regional time-varying albedos that could be attributed to the effects of dust erosion and deposition. But the resolution of these images was insufficient to identify different types and sources of aeolian materials, nor could they reveal aeolian deposits other than large dunes or extensive surface coverings that were redistributed by dust storms. Here we present images of Mars with up to 50 times better resolution. These images show that martian dunes include at least two distinct components, the brighter of which we interpret to be composed of relatively soft minerals, possibly sulphates. We also find large areas of the martian surface that have several metres or more of aeolian mantle lacking obvious bedforms. More... »

PAGES

592-594

References to SciGraph publications

Identifiers

URI

http://scigraph.springernature.com/pub.10.1038/17557

DOI

http://dx.doi.org/10.1038/17557

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1050217216


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