Skip to Main Content
Skip Nav Destination

Sinuous rilles on the lunar surface may have been formed by the movement of volatiles (H2O + CO2) in a channel between the basement surface and a surficial permafrost layer. Later sublimation of the ice formed in the vicinity of this channel would produce the features observed today.

You do not currently have access to this chapter.

Figures & Tables





Citing Books via

Close Modal

or Create an Account

Close Modal
Close Modal