Fences on the Moon?

Oblique image of impact melt flows exhibiting blocky margins
Mysterious farside impact melt deposits, image width 12 kilometers at center, looking west-to-east, north is to the left, M1451669615LR [NASA/GSFC/Arizona State University].

 

Early in the LRO mission, LROC images of the central farside revealed impact melt deposits with no prominent source crater. Very mysterious. Soon, scientists noticed that these enigmatic deposits were found at the Tycho crater antipode (opposite side of the Moon). Perhaps the Tycho forming event was so energetic that it ejected melt to the opposite side of the Moon, a distance of 5400 kilometers requiring a time-of-flight of 164 minutes. M1451669615, looking west-to-east, acquired 2023-10-11, incidence angle 60°, slew angle 47°, phase angle 110°, spacecraft altitude 112 kilometers, image width 12 kilometers.

Detail of opening image highlighting "fences"
Full-resolution view showing impact melt that ponded in the bottom of a 10-kilometer diameter crater. The dark lines (fences) formed as impact melt flow fronts solidified, not quite making it down to crater bottom. The flow fronts are so dark because they are very blocky and LROC was looking back towards the Sun enhancing topographic shadows. The flat ponded impact melt rock deposit is 600 meters by 800 meters wide, north is to the left NAC M1451669615 [NASA/GSFC/Arizona State University].

The complete NAC oblique shows a portion of the enigmatic highland pond area. Image width is approximately 72 kilometers in the center; north is to the left, NAC M1451669615LR [NASA/GSFC/Arizona State University].

Related Featured Images

LROC NAC Anaglyph: Highland Ponds

An Impact Melt Veneer in the Highlands

What Lies Beneath

Published by Mark Robinson on 25 April 2025