A Tangle of Talus

Multiple dry debris flows along the wall of Schubert A crater; NAC M141743432; image width 420 meters [NASA/GSFC/Arizona State University].

A 2.2-km diameter crater, Schubert A (79.341°E, 2.132°N), has steep walls, up to ~30° in slope. These steep walls are susceptible to gravity-driven mass wasting events. Mass wasting is a geologic process that acts on all planetary surfaces to erode or degrade landforms over time, and results from the downslope movement of rocks and soil under the influence of gravity. On the Moon, the slope of a surface is a key influencing factor: the steeper the slope, the faster mass wasting occurs. Mass wasting is typically triggered by nearby moonquakes, some caused by impact events.

Subsampled NAC showing Schubert A crater in its entirety; NAC M141743432; crater is 2.2 km in diameter [NASA/GSFC/Arizona State University].

Mass wasting on the Moon can take many forms from rockfalls, the plummeting of a few boulders, to rock avalanches and landslides. Material moving downslope in a fluid-like manner is often called a debris flow. And even though water is not required to cause debris flows, the resulting landforms resemble rivers of rock particles. At the base of the slope where mass wasting occurs, a mound of material piles up, called a talus deposit. The portion of Schubert A crater shown in the opening image exhibits the scars of many dry debris flows terminating in a mounded talus deposit, near the base of the crater floor.

Northeast wall of Schubert A crater displays the traces of numerous dry debris flows terminating in a talus deposit near the base of the wall; NAC M141743432 [NASA/GSFC/Arizona State University].

This talus deposit appears to be size or density sorted, with coarse material in the lower unit and a patina of finer materials on top. Perhaps a coarser mix of material was dislodged from the crater wall initially, as the result of a triggering event, while finer material continued to slide downslope after the main failure.

Talus deposit is size or density sorted, with coarser materials on the bottom (black arrow) and finer materials on top (white arrow); NAC M141743432 [NASA/GSFC/Arizona State University].

Explore these debris flows in the full resolution NAC and see if you can figure out why they are so dark (hint: look for materials eroding from near the crater rim).

Check out some more examples of rockfalls:

Bounce, Roll and Stop

Bouncing, Bounding Boulders!

A Recent Journey

Related Posts:

Recent Debris Flow

Lobate Debris Aprons on the Moon

It's All Downhill From Here

Tendrils in Reiner Crater

Published by J. Stopar on 14 January 2014