Featured Images
Slipher Crater: Fractured Moon in 3-D
Over time, the surface of the Moon fractures and buckles as it cools and shrinks, resulting in spectacular landforms. Stereo images provided by the LROC NAC allow a detailed look at these amazing features; view is to the east,...
Published on 12 Oct 2010
Photogrammetric Processing of LROC NAC Stereo Images
High-resolution 3D Digital Terrain Model (DTM) of a lunar crater created from a LROC NAC stereo pair. The scale bar on the left is the elevation in meters [NASA/GSFC/Arizona State University/Ohio State University].
Published on 12 Aug 2010
Linné Crater
Linné crater (2.2 km diameter) is a beautifully preserved young mare crater. Small white arrows indicate layering preserved just below the rim; these rock outcrops probably represent discrete lava flow deposits [NASA/GSFC/Arizona State...
Published on 06 Jul 2010
Hunting for Ancient Lunar Impact Basins
Fig. 1: A lesser-known impact basin, Freundlich-Sharonov, is visible in this Digital Terrain Model (DTM) made from LROC WAC stereo images, and darker shades represent lower elevations than brighter shades. The diameter of the...
Published on 09 Jun 2010
Hortensius Domes - Constellation Region of Interest
Summit crater of Hortensius Dome Phi. Summit craters of all the Hortensius Domes show no raised rims and are not circular, indicating they are not impact craters, rather that they are analogous to volcanic calderas. Image width 1.22 km,...
Published on 01 Apr 2010
Apollo Basin: Mare in a Sea of Highlands
High resolution LROC image of floor of the Apollo Basin, a large (538 km diameter) double-ringed impact crater in the southern hemisphere of the far side. This image shows part of the boundary between two flow units within the...
Published on 30 Mar 2010
A Digital Terrain Model of the Orientale Basin
A Digital Terrain Model (DTM) of the large Orientale Basin (1100 km diameter), located on the western hemisphere of the Moon, produced from stereo LROC WAC images. The image shows the hill-shaded, color-coded DTM with heights varying...
Published on 20 Jan 2010