91亚色 U research identifies icy ridges聽on Pluto
TORONTO, January 4, 2017聽- Using a model similar to what meteorologists use to forecast weather on Earth and a computer simulation of the physics of evaporating ices, a new study, published in the journal by , Department of Earth and Space Science and Engineering at 91亚色鈥檚 Lassonde School of Engineering, has found evidence that snow and ice features previously only seen on Earth, have been spotted on Pluto.
鈥淧enitentes鈥 which are formed by erosion, are bowl-shaped depressions with spires around the edge, and are several metres high.
The groundbreaking research, done in collaboration with researchers at NASA and Johns Hopkins University, indicates that these icy features may exist on other planets where environmental conditions are similar.
鈥淭he identification of the ridges of Tartarus Dorsa as Penitentes suggests that the presence of an atmosphere is necessary for the formation of penitentes, which would explain why they have not previously been seen on other airless icy satellites or dwarf planets,鈥 says Moores. 鈥淏ut exotic differences in the environment give rise to features with very different scales. This test of our terrestrial models for penitentes suggests that we may find these features elsewhere in the solar system, and in other solar systems, where the conditions are right."
Moores, along with his 91亚色 postgraduate fellow, Dr. Christina Smith, Dr. Anthony Toigo, at the Applied Physics Laboratory, Johns Hopkins University and NASA Research Astrophysicist, Dr. Scott D. Guzewich, at the in Maryland, USA compared their model to ridges on Pluto imaged by the New Horizons spacecraft in 2015. Pluto鈥檚 ridges are much larger - 500 metres tall and separated by three to five kilometres - as compared to their meter-sized earthly counterparts.
Photo Credit: NASA/Johns Hopkins University Applied Physics Laboratory/Southwest Research Institute
鈥淭his gargantuan size is predicted by the same theory that explains the formation of these features on Earth,鈥 says Moores. 鈥淚n fact, we were able to match the size and separation, the direction of the ridges, as well as their age: three pieces of evidence that support our identification of these ridges as penitentes.鈥
Moores says though Pluto's environment is very different from the Earth - it is much colder, the air much thinner, the sun much dimmer and the snow and ice on the surface are made from methane and nitrogen instead of water - the same laws of nature apply. Both NASA and Johns Hopkins University were instrumental in the collaboration that led to this new finding. Both provided background information on Pluto's atmosphere using a model similar to what meteorologists use to forecast weather on Earth. This was one of the key ingredients in Moores鈥 own models of the penitentes, without which this discovery would not have been made.
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Media contact:
Anjum Nayyar, Media Relations, 416 736 2100 ext. 44543,聽anayyar@yorku.ca.
