Seasonal Slumps in Juventae Chasma, Mars

Seasonal Slumps in Juventae Chasma, Mars

Dark topographic slumps several meters wide, tens of meters in length, and up to a meter in depth are observed on the slopes of Juventae Chasma (JC), Valles Marineris (VM), Mars. These slumps usually originate near the terminal points of recurring slope lineae (RSL). Near their initiation points, th...

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Bibliographic Details
Main Authors: Ojha, Lujendra, Chojnacki, Matt, McDonald, George D., Shumway, Andrew, Wolff, Michael J., Smith, Michael D., McEwen, Alfred S., Ferrier, Ken, Huber, Christian, Wray, James J., Toigo, Anthony
Other Authors: Univ Arizona, Lunar & Planetary Lab
Language:en
Published: AMER GEOPHYSICAL UNION 2017
Online Access:http://hdl.handle.net/10150/626275
http://arizona.openrepository.com/arizona/handle/10150/626275

Internet

http://hdl.handle.net/10150/626275
http://arizona.openrepository.com/arizona/handle/10150/626275

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