On Mars, meteorites can cause miles-long dust slides

On Mars, meteorites can cause miles-long dust slides

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Dark lines of discolored dust on slopes of Martian mountain

The slope slides seen above stretch across over 2 miles of the Martian surface. Credit: ESA/TGO/CaSSIS

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Mars receives its fair share of cosmic collisions. With less than one percent the atmosphere as Earth, some meteoroids fail to burn up entirely before reaching the Red Planet’s surface. When they do, they can usher dramatic changes to the barren Martian landscape that stretch for miles. In the future, they may even cause problems for human explorers.

The results of these events are detailed in a study published on November 6 in the journal Nature Communications by researchers at the European Space Agency (ESA) and Switzerland’s University of Bern. Planetary scientist Valentin Bickel used deep learning algorithms to identify and analyze images of over two million slope streaks–areas where Mars’ top layers of fine dust have been displaced. Given the planet’s lack of water, Bickel and colleagues theorize that wind is responsible for the vast majority of these feathery streaks.

However, around one in 1,000 slope streaks is caused by visitors from outer space. One such example was documented on Christmas Eve 2023 by the ESA’s ExoMars Trace Gas Orbiter. In a photo taken by the orbiter’s onboard Color and Stereo Surface Imaging System, a fading cluster of impact craters are visible near the base of Apollinaris Mons, an ancient shield volcano near Mars’equator. The results from the meteoroid’s powerful impacts sit above the crate–a roughly 2.3 square mile patch of discolored slope streaks. It’s a

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