J Alexis P Rodriguez1, Kenneth L Tanaka2, Ali M Bramson3
1Planetary Science Institute, 1700 East Fort Lowell Road, Suite 106, Tucson, AZ, 85719-2395, USA. alexis@psi.edu.
View abstract on PubMed
The Martian north polar spiral troughs formed from in-situ erosion and gradual growth, not just poleward migration. This erosion may have supplied significant ice to mid-latitude mantles, potentially usable for future human exploration.
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