Dunes are known to form on Earth, Mars, Venus, Titan and Comet 67P – and now on the dwarf planet Pluto, according to a new study, the latest discovery from New Horizons. These dunes are unlike the dunes made of sand seen on Earth though; instead, Pluto’s dunes are likely made of tiny grains of solid methane, the study’s authors say.
“What makes this discovery surprising,” writes Alexander Hayes in a related Perspective, “is that the sediment can be mobilized despite Pluto’s tenuous atmosphere, whose surface pressure (1 Pa) is 100,000 times lower than Earth’s.”
When the New Horizons spacecraft flew by Pluto on 14 July 2015, it obtained the most detailed images yet of the dwarf planet. When analyzing the data, Matt Telfer and colleagues spotted a collection of 357 pale ridges, as well as six darker wind streaks, located on one of Pluto’s largest features, a vast plain called Sputnik Planitia. Along the western area of the plain, the ridges run parallel with a mountain range, but farther east, they shift their orientation and become more spread out, a pattern also seen in the wind streaks.
Several clues revealed that these landforms were created by wind; namely, the locations of the ridges and their distribution patterns demonstrate this. Modeling by the authors shows that wind can create these dunes once the grains are airborne; however, a process called sublimation is required first, to lift the grains from the planet’s surface.
In this process, the Sun heats surface ice enough that gas is released into the atmosphere, lofting particles into the air as a result. The likely source of the dune grains is methane ice blown from nearby mountains, say the authors, although nitrogen ice cannot be ruled out, as a source. “If an extremely tenuous atmosphere like that of Pluto can support the generation of bedforms from wind-driven sediment,” poses Hayes in his Perspective, “what kind of aeolian activity might we see on places like Io or Triton?”
Publication: Matt W. Telfer, et al., “Dunes on Pluto,” Science 01 Jun 2018: Vol. 360, Issue 6392, pp. 992-997; DOI: 10.1126/science.aao2975