Loading the Lunar Reconnaissance Orbiter into the thermal vacuum chamber at Goddard Space Flight Center. Diviner is one of seven instruments aboard NASA LRO Mission.
Loading Lunar Reconnaissance Orbiter LRO in the Thermal Vacuum Chamber
Artist rendering of the Lunar Reconnaissance Orbiter LRO, above the moon.  LRO carries seven instruments that make comprehensive remote sensing observations of the moon and measurements of the lunar radiation environment. The LRO mission is managed by NASA Goddard for the Science Mission Directorate at NASA Headquarters in Washington.  http://photojournal.jpl.nasa.gov/catalog/PIA18163
Lunar Reconnaissance Orbiter Artist Concept
Scientists, using cameras aboard NASA Lunar Reconnaissance Orbiter LRO, have created the largest high resolution mosaic of our moon north polar region.
NASA Releases First Interactive Mosaic of Lunar North Pole
These graben - a kind of trench that is formed as a surface expands - were imaged near a region of the Moon called Mare Frigoris by NASA's Lunar Reconnaissance Orbiter (LRO).  https://photojournal.jpl.nasa.gov/catalog/PIA23237
Graben on the Moon
This image of lobate scarps - a kind of curved hill - was taken near a region of the Moon called Mare Frigoris by NASA's Lunar Reconnaissance Orbiter (LRO).  https://photojournal.jpl.nasa.gov/catalog/PIA23236
Lobate Scarps on the Moon
This NASA Lunar Reconnaissance Orbiter LRO image is of the summit crater of Hortensius Dome Phi. Summit craters of all the Hortensius Domes show no raised rims and are not circular, indicating they are analogous to volcanic calderas.
Hortensius Dome Phi
The Diviner instrument following integration to NASA Lunar Reconnaissance Orbiter. Diviner is one of seven instruments aboard the Lunar Reconnaissance Orbiter.
Diviner Following Integration to the Lunar Reconnaissance Orbiter LRO
NASA is scheduled to launch the Lunar Reconnaissance Orbiter, an unmanned mission to comprehensively map the entire moon, on June 18, 2009.
Lunar Reconnaissance Orbiter LRO Artist Concept
New surface features of the Moon have been discovered in a region called Mare Frigoris, outlined here in teal. This image is a mosaic composed of many images taken by NASA's Lunar Reconnaissance Orbiter (LRO).  https://photojournal.jpl.nasa.gov/catalog/PIA23209
The Moon's Mare Frigoris
Scientists have discovered these wrinkle ridges in a region of the Moon called Mare Frigoris. These ridges add to evidence that the Moon has an actively changing surface. This image was taken by NASA's Lunar Reconnaissance Orbiter (LRO).  https://photojournal.jpl.nasa.gov/catalog/PIA23210
Wrinkle Ridges on the Moon
Research using data from NASA's ARTEMIS mission suggests that lunar swirls, like the Reiner Gamma lunar swirl imaged here by NASA's Lunar Reconnaissance Orbiter, could be the result of solar wind interactions with the Moon's isolated pockets of magnetic field.  Credits: NASA LRO WAC science team
Lunar Swirl Reiner Gamma
Diviner undergoing post thermal vacuum range of motion testing. Diviner is one of seven instruments aboard NASA LRO Mission.
Diviner Undergoing Post Thermal Vacuum Range of Motion Testing
Close-up of the Diviner solar calibration target. Diviner is one of seven instruments aboard NASA LRO Mission.
Close-up of Diviner Solar Calibration Target
This image shows final preparations being made for thermal balance testing of the Diviner Lunar Radiometer Experiment at JPL. Diviner is one of seven instruments aboard NASA LRO Mission.
Final Preparations for Diviner Thermal Balance Testing at JPL
The Diviner Instrument prior to shipment. Diviner is one of seven instruments aboard NASA LRO Mission.
The Diviner Instrument Prior to Shipment
CAPE CANAVERAL, Fla. – One of three solar panels is seen during closeout of the Lunar Reconnaissance Orbiter, or LRO, at Astrotech Space Operations in Titusville, Fla. The satellite's primary mission is to search for water ice on the moon in a permanently shadowed crater near one of the lunar poles. LCROSS is a low-cost, accelerated-development, companion mission to NASA's Lunar Reconnaissance Orbiter, or LRO. LCROSS and LRO are the first missions in NASA's plan to return humans to the moon and begin establishing a lunar outpost by 2020. Launch is targeted for no earlier than June 2 from Cape Canaveral Air Force Station in Florida. Photo credit: NASA/Jack Pfaller
KSC-2009-2987
CAPE CANAVERAL, Fla. – At Astrotech Space Operations in Titusville, Fla.,  technicians remove red-tag items from the Lunar Reconnaissance Orbiter, or LRO, before flight.  The LRO will be mated with NASA's Lunar CRater Observation and Sensing Satellite, known as LCROSS, spacecraft.  Instruments on the LRO seen here are the LEND (bottom) that will measure the flux of neutrons from the moon and the LROC (above it), a narrow angle camera that will provide panchromatic images. The satellite's primary mission is to search for water ice on the moon in a permanently shadowed crater near one of the lunar poles. LCROSS is a low-cost, accelerated-development, companion mission to NASA's Lunar Reconnaissance Orbiter, or LRO. LCROSS and LRO are the first missions in NASA's plan to return humans to the moon and begin establishing a lunar outpost by 2020. Launch is targeted for no earlier than June 2 from Cape Canaveral Air Force Station in Florida. Photo credit: NASA/Jack Pfaller
KSC-2009-2990
NASA Lunar Reconnaissance Orbiter sees hummocks and blocks on the ejecta blanket of Tsiolkovskiy crater.
Hummocks and Blocks and Craters
Full resolution detail from one of the first LROC NAC images. At this scale and lighting, impact craters dominate the landscape.
First LROC Images
This image taken by NASA Lunar Reconnaissance Orbiter shows a wide variety of geologic features on northwest of Plato crater.
Plato Crater
Farside Northern Highlands
Farside Northern Highlands
This image from NASA Lunar Reconnaissance Orbiter shows a view of boulders, on the floor of Rutherfurd crater, about to disappear into the shadows of dusk.
Central Peak of Rutherfurd
The Apollo 17 Lunar Module Challenger descent stage comes into focus in this image taken by NASA Lunar Reconnaissance Orbiter.
Exploring the Apollo 17 Site
Orientale Basin
Orientale Basin
 NASA Lunar Reconnaissance Orbiter catches the edge of Mare Moscoviense.
Where Moscoviense meets the Highlands
NASA Lunar Reconnaissance Orbiter captures a northeast-trending wrinkle ridge cuts across the plains of Mare Imbrium.
Wrinkle Ridges of Northwest Mare Imbrium
Approaching Aitken Crater - Vertregt J
Approaching Aitken Crater - Vertregt J
Boulder in Recht Crater
Boulder in Recht Crater
The same crater, as seen by NASA Lunar Reconnaissance Orbiter, under very different lighting. On the left the Sun was midway to the horizon and on the right the Sun was high, approaching noon.
Illumination Comparison of a Mare Crater
How did I form?
How did I form?
New View of Apollo 14
New View of Apollo 14
Boulders perched atop a wrinkle ridge in Mare Imbrium west of the Montes Teneriffe can be seen in this image taken by NASA Lunar Reconnaissance Orbiter.
Wrinkle Ridge Near Montes Teneriffe
Dark Halo Crater in Orientale
Dark Halo Crater in Orientale
Diverse textures on the floor of Saha E which could be the result of impact melt coating boulders and other deposits on the floor of the crater on the lunar farside in this image taken by NASA Lunar Reconnaissance Orbiter.
The Floor of Saha E
The Moon Largest Impact Basin
The Moon Largest Impact Basin
NASA Lunar Reconnaissance Orbiter captured this anaglyph image is a close up view of Copernicus crater. 3D glasses are necessary to view this image.
Central Peak of Copernicus Crater Anaglyph
A Path not Taken
A Path not Taken
Slipher Crater: Fractured Moon in 3-D
Slipher Crater: Fractured Moon in 3-D
NASA Lunar Reconnaissance Orbiter looks at the Moon in 3D. 3D glasses are necessary to view this image.
The Moon in 3-D
Slope Failure near Aratus Crater
Slope Failure near Aratus Crater
This image taken by NASA Lunar Reconnaissance Orbiter shows the spectacularly preserved viscous flow on the NE rim of Byrgius A crater.
Out of the Shadows: Impact Melt Flow at Byrgius A Crater
Necho Terraces
Necho Terraces
Seeing small areas of the Moon at 50 cm per pixel often presents unexpected views, and sometimes it is hard to interpret the geology at first glance, much less what is up and what is down, as evidenced by NASA Lunar Reconnaissance Orbiter.
Moon or Abstract Expressionism?
One month after its first image of the Apollo 11 landing site was acquired, NASA Lunar Reconnaissance Orbiter passed over the site again providing a new view of the historic site.
Apollo 11: Second Look
Moon seen from the East
Moon seen from the East
The Apollo 15 Lunar Laser Ranging Retroreflector - A Fundamental Point on the Moon
The Apollo 15 Lunar Laser Ranging Retroreflector - A Fundamental Point on the Moon
Lava Flows Exposed in Bessel Crater
Lava Flows Exposed in Bessel Crater
Close-up view of the lunar highlands, northeast of Clavius crater, taken by NASA Lunar Reconnaissance Orbiter.
Swooping over the Lunar Highlands
This image from NASA Lunar Reconnaissance Orbiter shows a view of boulders, on the floor of Rutherfurd crater, about to disappear into the shadows of dusk.
Cluster of Farside Secondary Craters
A bottleneck at the start of the lunar sinuous rille within Vallis Alpes formed several morphologic features including a lava pond, a breached dam, and an island in the rille in this image captured by NASA Lunar Reconnaissance Orbiter.
Vallis Alpes
Eratosthenes Crater and the Lunar Timescale
Eratosthenes Crater and the Lunar Timescale
Wrinkle Ridge in Oceanus Procellarum
Wrinkle Ridge in Oceanus Procellarum
NASA Lunar Reconnaissance Orbiter spied a very subtle mare-highlands boundary in Mare Moscoviense on the lunar farside, near the center of the Constellation Program region of interest.
Mare Moscoviense Constellation Site
A sinuous rille created by a lava flow snakes around the base of a massif in the Prinz-Harbinger region on the Moon in this image taken by NASA Lunar Reconnaissance Orbiter.
Rimae Prinz Region - Constellation Region of Interest
NASA Lunar Reconnaissance Orbiter shows a lobate scarp in the mare basalts of Aitken crater on the lunar farside arrows.
Aitken Crater
Fresh Crater on Oceanus Procellarum
Fresh Crater on Oceanus Procellarum
Diviner Global Composition
Diviner Global Composition
Barnstorming Linné Crater
Barnstorming Linné Crater
This is a synthetic perspective view looking south from the Apollo 16 landing area, topography is rendered naturally as seen by NASA Lunar Reconnaissance Orbiter.
First LROC Stereo Results
Terraces in Eratosthenes Crater
Terraces in Eratosthenes Crater
Small Crater in Oceanus Procellarum
Small Crater in Oceanus Procellarum
NASA Lunar Reconnaissance Orbiter shows boulders and impact melt line the floor of the 85-km crater Tycho, a potential site for future human exploration.
The Floor of Tycho
NASA Lunar Reconnaissance Orbiter shows a sinuous rille winding its way across a much larger rille in the heart of the Aristarchus Plateau.
Rille within a Rille
Wrinkle Ridges in Aitken Crater
Wrinkle Ridges in Aitken Crater
Boulder Trails in Menelaus Crater
Boulder Trails in Menelaus Crater
Two small black arrows on today image taken by NASA Lunar Reconnaissance Orbiter show the location of a small graben 28 meters in width in a pyroclastic mantling deposit in the SW portion of Mare Humorum.
Graben and Pyroclastics in SW Mare Humorum
Color of the Moon
Color of the Moon
NASA Lunar Reconnaissance Orbiter captured this image close up view of Copernicus crater showing light-toned fractured bedrock exposed on the higher slopes on the central structural uplift.
Central Peak of Copernicus Crater
Slice of Mare
Slice of Mare
Rilles as far as the eye can see in Prinz
Rilles as far as the eye can see in Prinz
Exposed Boulders in the Aitken Mare
Exposed Boulders in the Aitken Mare
Cracks form in the impact melt sheet on the floor of Necho Crater in this image taken by NASA Lunar Reconnaissance Orbiter.
Necho Crater
Retracing the Steps of Apollo 15
Retracing the Steps of Apollo 15
Crater rim of Flamsteed P
Crater rim of Flamsteed P
Rima Bradley
Rima Bradley
Action Shot
Action Shot
Ejecta from Copernicus
Ejecta from Copernicus
Impact Melt at Necho Crater
Impact Melt at Necho Crater
Sublunarean Void
Sublunarean Void
Farside! And All the Way Around
Farside! And All the Way Around
Scouring Secondary Ejecta
Scouring Secondary Ejecta
The unusual shapes of craters at the Flamsteed Constellation region of interest provide information about the thickness of the lunar regolith in this region in this image taken by NASA Lunar Reconnaissance Orbiter.
Each Crater Tells a Story
NASA Lunar Reconnaissance Orbiter shows a small portion of the rim of Erlanger crater. Much of its floor remains in permanent shadow due to its location near the north pole.
Eternal Darkness Near the North Pole
Delicate Patterns in Giordano Bruno Ejecta
Delicate Patterns in Giordano Bruno Ejecta
High-albedo marks on the lunar surface left by a boulder bouncing down the northeast wall of farside highlands crater Moore F in this image captured by NASA Lunar Reconnaissance Orbiter.
Bright Boulder Trail
Mare Ingenii may be best known for its prominent lunar swirls, which are high albedo surface features associated with magnetic anomalies.
Depths of Mare Ingenii
NASA Lunar Reconnaissance Orbiter looks at a mare-highlands boundary in northern Mare Frigoris.
Relative Timing of Geologic Events in Mare Frigoris
Reiner Gamma
Reiner Gamma
NASA Lunar Reconnaissance Orbiter sees bright crater rays and boulders.
Bright Crater Rays and Boulders
The Marius Hills pit is a possible skylight in a lava tube in an ancient volcanic region of the Moon called the Marius Hills. This image was taken by NASA Lunar Reconnaissance Orbiter.
Marius Hills Pit -- Lava Tube Skylight?
Sinus Iridum
Sinus Iridum
This image acquired by NASA Lunar Reconnaissance Orbiter shows a crater center of image formed by impact of the Apollo 14 Saturn IVB booster.
Ejecta Sweeps the Surface
Hole in One
Hole in One
Up from the Depths
Up from the Depths
This image taken NASA Lunar Reconnaissance Orbiter is a high-resolution view of part of the floor of Riccioli Crater. The view is centered on the boundary between a spur of the crater central peak materials and volcanic lava flow deposits.
Riccioli Crater: Cracked, Melted, and Draped
Buckland Boulders
Buckland Boulders
Southern Rim of Menelaus Crater
Southern Rim of Menelaus Crater
Highest Point on the Moon
Highest Point on the Moon
Splendors of Mare Smythii
Splendors of Mare Smythii
Ejecta in Tycho Crater
Ejecta in Tycho Crater