nt”We needed to leverage the very best the
ntscience community had to offer,” said Michael Wargo, chief lunar
ntscientist of ESMD. “And by doing that, we’ve fundamentally changed
ntour scientific understanding of the moon.”

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ntThis image shows a flow of impact melt moving away from its crater.

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ntCredit: NASA/GSFC/Arizona State University

ntThe Lunar Reconnaissance Orbiter Camera revealed  nearly 5.7 million square kilometers of the moon’s surface.

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ntIn the photo above, this crater which is located in Mare Humorum contains relatively few boulders. This means that the impact area is probably made of regolith and fragmented the underlying mare basalt into large boulders.

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ntCredit: NASA/GSFC/Arizona State University

ntFor a six month period (or six lunar days) the LRO collected 1,700 images of the same area at the south pole. The binary images were then stacked to form the map above which shows the areas that never see sunlight.

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ntThe LRO found the coldest spot in the
ntsolar system, with a temperature of minus 415 degrees Fahrenheit.

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ntCredit: NASA/GSFC/Arizona State University

ntIs this a volcano?

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ntCredit: NASA/GSFC/Arizona State University

ntBoulders clustered on a positive relief bulge in an impact melt deposit on the floor of Anaxagoras crater.

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ntCredit: NASA/GSFC/Arizona State University

ntA dry flow of boulders down the slope of Riccioli crater’s inner wall. The area slopes from the bottom right hand corner to the upper left hand corner.

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ntCredit: NASA/GSFC/Arizona State University

ntThis shows where the previous image was taken.

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ntCredit: NASA/GSFC/Arizona State University

ntIs it dry debris or liquid flow? Granular debris on the wall of Stevinus A flows downhill to the right. A 7 meter boulder impedes the progress of the flow, which bifurcates and reconnects about 10 m downhill.

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ntCredit: NASA/GSFC/Arizona State University

ntThe far side of the moon. Astronauts are the only humans to ever see it in person.

ntThe LRO detailed new maps of lunar surface characteristics.

ntThis is a south polar map of enhanced hydrogen which could potentially be used as fuel.

ntLRO also created a radar map of the north polar region.

ntThe lunar poles are shown in ultraviolet light.

ntThe LRO captured this landslide on the wall of a small crater which slopes from the top right to the bottom left. The landslide has exposed many boulder within the crater wall.

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ntCredit: NASA/GSFC/Arizona State University

ntNASA doesn’t know how pancake-like mounds like this one in thte Stevinus crater formed on a relatively flat surface. Perhaps they were formed by magma under the crust or maybe they were formed by slumping caused by small impacts over time.

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ntCredit: NASA/GSFC/Arizona State University

ntHere’s a farther view around the Stevinus crater.

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ntCredit: NASA/GSFC/Arizona State University

ntThis large hole is thought to be created by a collapsed lava tube.

ntThe upper slopes of Diophantus crater, located on the western edge of Mare Imbrium, shows dark materials that flowed downward from the crater walls. These dark features originate from several layers exposed in the crater walls. But what are they made of and how did they get there? Volcanos?

ntMore mounds on the floor of the King crater.

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ntCredit: NASA/GSFC/Arizona State University

ntHere’s an example of layering exposed in the wall of the Bessel crater.

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ntCredit: NASA/GSFC/Arizona State University

ntLRO finds evidence of humans on the moon. Here’s the landing site of Apollo 14.

ntHere’s what the surface of the moon looked like from Apollo 14.

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ntNASA has many, many more images and videos received from the LRO.