Featured Images

Lobate Scarps: The Movie

Lobate scarps - like those shown here on the floor of the farside crater d'Alembert - are not large, but they tell us much about how hot the Moon was when it was born and its ongoing thermal evolution. Image width is about four...

Published on 31 Oct 2018

The South Side of Tycho Crater

Get out your red/blue anaglyph glasses for a three-dimensional treat! This extreme closeup of the south side of 86-kilometer-diameter Tycho Crater shows melt flows and pools, small craters, sagging slopes that look like ripples,...

Published on 08 Oct 2018

Another Layered Target

Copernicus crater central peak reveals the complexity of the lunar crust through distinct layering and patchy surface brightness. Image 3 km wide,  M1261372886LR [NASA/GSFC/Arizona State University].

Published on 04 Oct 2018

Layered Target

Spectacular view across the rim of Wallach crater (5700 meter diameter), acquired when LRO was 93 kilometers above the surface, M1236317761LR [NASA/GSFC/Arizona State University].

Published on 11 Sep 2018

Deflector Shields Up!

Part of the westernmost swirl feature in Mare Marginis. This closeup of the center of the anaglyph strip below highlights an area little more than five kilometers wide. Bright swirl areas appeared "painted on" the landscape. Part of NAC...

Published on 06 Sep 2018

Cool Cold Spots

Oblique (very!) view of Einthoven cold spot crater, located at 109.91° E, 6.74° S. White rays and the crater's rocky rim and rugged interior wall are visible signs of youth. The cold spot anomaly surrounding the crater is another sign...

Published on 21 Aug 2018

NAC Anaglyph: Moore F Crater

Moore F is an impact crater in transition. Image width is about eight kilometers. NAC images M125720601L/R and M125713813L/R. [NASA/GSFC/Arizona State University]

Published on 09 Aug 2018

Aristarchus Crater

The Aristarchus crater (40 kilometer diameter, 23.73°N, 312.51°E) and plateau is one of the most geologically complex areas on the Moon. In this amazing picture, the LRO spacecraft slewed 62° (west-to-east) looking across the crater....

Published on 04 Aug 2018

NAC Anaglyph: Eimmart A Crater

Eimmart A, partially visible at lower right, has a split personality. Image numbers M1098422839L/R, M1098408548L/R [NASA/GSFC/Arizona State University].

Published on 21 Jul 2018

John Young at South Ray Crater

Overhead view of South Ray crater, the most prominent feature at the Apollo 16 Descartes landing site in the central lunar highlands. Astronaut John Young landed Lunar Module Orion north of the crater on  21 April 1972 (UTC)....

Published on 05 Jul 2018

Self-Inflicted Secondaries?

This portion of an impact melt flow at Aristarchus Crater, centered at 24.6°N, 321.1°E, includes modified small craters and overlapping melt flows. What do the shapes of craters on impact melt and the statistics derived through careful...

Published on 30 Jun 2018

Another Lunar Enigma

Ina (18.66°N, 5.30°E) is one of the most enigmatic landforms on the Moon. First discovered in Apollo-era photographs, then intensely studied with modern observations, its nature is still unknown. The Sun is shining right-to-left, 40...

Published on 20 Jun 2018

Towering Peak

The summit of the unnamed peak in the foreground (50.2° S, 236.6° E) has an elevation of 6710 meters, about 7000 meters of relief relative to the low point at the bottom of the image. The two peaks on the horizon, 200 kilometers in the...

Published on 15 Jun 2018

South Massif Landslide

By lunar standards South Massif is a relatively modest mountain, but with a rich history (geologic and exploration). The massif is about 7000 meters across at the base and 2300 meters tall; M1266925685LR, incidence angle 33°, slew angle...

Published on 09 Jun 2018

Hell Q Crater

Recent impact craters are some of the most spectacular landforms on the Moon! For example, Hell Q (3.4 kilometers in diameter, 33.0° S, 355.5° E) shows off pristine impact melt that lined the crater walls and pooled in the bottom, now...

Published on 27 May 2018

Hawke Crater

Hawke crater, 13.2 km wide, is noticeably tilted because the impactor - an asteroid or a comet - that excavated it struck the sloping inner wall of Grotrian crater. Visible are light-colored rays that attest to the crater's youth, as...

Published on 03 May 2018

Curiously Fast Degradation of Small Lunar Craters

Taurus-Littrow valley, geologic exploration target for Apollo 17 and the Lunar Reconnaissance Orbiter Camera study team led by Dr. Prasun Mahanti.  Center latitude 20.15°N, center longitude 30.98°E, image 18 km wide, image...

Published on 24 Apr 2018

Lunar Light Plains: The Movie

The Orientale Basin, about 950 kilometers wide, is the striking multi-ringed impact feature at  lower right. New research suggests that the impact event that formed Orientale may have emplaced light plains deposits - visible here...

Published on 20 Apr 2018

NAC Anaglyph: Humboldt Crater Floor

A floor fracture and central peak structure on the floor of Humboldt Crater (207 km diameter) that  formed directly after impact. Intrusive volcanic activity likely caused the floor of the crater to lift up and then fracture ...

Published on 06 Apr 2018

Montes Carpatus

The Montes Carpatus region (16.67°N, 332.93°E) contains numerous examples of volcanic materials. The low albedo (dark) patterns may indicate pyroclastic (explosive) material that erupted over 3 billion years ago. Tobias Mayer G crater...

Published on 08 Mar 2018