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Dark Streaks (Mars)

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Dark streaks is a general term for temporarily darkened surface patches occurring on various slopes on Mars (e.g., crater walls or dune faces) that display a range of morphologies (e.g., conical, linear, or braided). The darkening of the surface is believed to be caused by the removal of the surficial dust cover due to dry grain flow, wetting of the soil, or fluvial activity. Over the course of months and years, the dark coloration fades away, which is presumably the result of the surficial accumulation of bright dust particles and/or drying of the soil.

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Correspondence to Alessandro Airo .

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© 2014 Springer-Verlag Berlin Heidelberg

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Airo, A. (2014). Dark Streaks (Mars). In: Amils, R., et al. Encyclopedia of Astrobiology. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-27833-4_5092-1

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  • DOI: https://doi.org/10.1007/978-3-642-27833-4_5092-1

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  • Online ISBN: 978-3-642-27833-4

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