Featured Images

'Shaping' Lunar Science with Vector Data

Twenty new shapefiles created by the LROC Team are now available! A few of the shapefiles shown here include mare age units, footprints of digital terrain models (DTMs), and the locations of small geologic features such as...

Published on 18 Jul 2017

NAC Anaglyph: Mare Shoreline in Apollo Basin

A portion of the southwestern mare "shoreline" in the Apollo basin on the farside. This contact between ancient lava plains and a remnant crater rim shows the lunar surface as a land of contrasts -- of expansive plains and jutting...

Published on 30 Jun 2017

NAC Anaglyph: van den Bos Crater

van den Bos is a small (22 km) floor-fractured crater on the lunar farside.  The shallow floor of the crater is crossed with fractures rougly concentric to the crater walls. [NASA/GSFC/Arizona State University].

Published on 23 Jun 2017

NAC Anaglyph: Dorsa Whiston

A distinctive wrinkle ridge in Oceanus Procellarum named Dorsa Whiston. Ridges like this one result from substantial compression within portions of the lunar maria  [NASA/GSFC/Arizona State University].

Published on 12 May 2017

Tycho Limb Shot!

Magnificent oblique view of the eastern side of Tycho's central peak acquired when the Sun was relatively high above the horizon. From the viewpoint of LROC the Sun was behind and a bit to the north, so shadows are mostly hidden, thus...

Published on 27 Apr 2017

NAC Anaglyph: Maunder Central Peak

Maunder Central Peak - created when Maunder crater (55 km in diameter) was formed.  The central portion of the crater was initially compressed, then subsequently rebounded to form these large peaks which rise over a kilometer above...

Published on 07 Apr 2017

NAC Anaglyph: Manners Crater

Fresh material (bright streaks) is exposed along the wall of the relatively young Manners crater  [NASA/GSFC/Arizona State University].

Published on 31 Mar 2017

NAC Anaglyph: Mature 4 km crater in southern Mare Fecunditatis

Mature 4 km crater in southern Mare Fecunditatis. The irregular formation to the southwest is probably a secondary crater from crater Langrenus, 200+ km to the north-northeast [NASA/GSFC/Arizona State University].

Published on 24 Mar 2017

NAC Anaglyph: "Bathtub Ring" of Lava

The pit-like Bawa crater (off-center left) is located on the edge of Lacus Solitudinus. The pit is congested with old lava and spiny, razerback ridges. The ridges are composed of debris that slumped from the upslope (western) wall above...

Published on 17 Mar 2017

NAC Anaglyph: Dorsum Cloos

Dorsum Cloos -- a wrinkle ridge signifying that substantial forces within the rocks have led to folding and faulting in eastern Mare Smythii [NASA/GSFC/Arizona State University].

Published on 10 Mar 2017

NAC Anaglyph: Mare Frigoris Wrinkle Ridges

Wrinkle Ridges in Mare Frigoris -  Wrinkle ridges are a response to a local mass concentration, while others, as in this case, may be due to global contractional stress [NASA/GSFC/Arizona State University].

Published on 03 Mar 2017

NAC Anaglyph: Fissures in Bowditch Crater

A complex grouping of fissures in the mare-flooded Bowditch crater that were once likely sites of volcanic eruptions in this area. Bowditch crater is part of the lava-flooded region named Lacus Solitudinus [NASA/GSFC/Arizona State...

Published on 24 Feb 2017

NAC Anaglyph: Atlas Crater Wall

The rough-and-tumble morphology of this crater wall results, at least in part, from large-scale wall instability and failures [NASA/GSFC/Arizona State University].

Published on 17 Feb 2017

NAC Anaglyph: Briggs Fractures

Fractures in the floor of Briggs crater suggest intrusive volcanic activity , i.e. magma rising from below to push up the crater floor, causing it to crack [NASA/GSFC/Arizona State University].

Published on 10 Feb 2017

NAC Anaglyph: Cobra Head

Deposits on the east rim of the head of the Vallis Schröteri, or "Cobra Head" [NASA/GSFC/Arizona State University].

Published on 03 Feb 2017

NAC Anaglyph: Tsiolkovskiy Slumping

The wall of Tsiolkovskiy crater has slumped downward due to gravity since its formation, giving it a lumpy appearance [NASA/GSFC/Arizona State University].

Published on 27 Jan 2017

NAC Anaglyph: Rima Sharp

The floor of Rima Sharp, a sinuous rille, is broad and relatively flat [NASA/GSFC/Arizona State University].

Published on 13 Jan 2017

NAC Anaglyph: Buffon Flow Front

This lobate flow, found to the south of Buffon crater, likely formed as fluidized basin ejecta moved across the surface [NASA/GSFC/Arizona State University].

Published on 06 Jan 2017

NAC Anaglyph: Langmuir Central Peak

The bouldery and blocky uppermost slopes of the central peak of Langmuir crater [NASA/GSFC/Arizona State University].

Published on 30 Dec 2016

NAC Anaglyph: Orientale Mare and Melt

Fractured impact melt from the Orientale basin-forming impact stands out from the mare lavas that later embayed it [NASA/GSFC/Arizona State University].

Published on 23 Dec 2016