On 18 June 2009, NASA launched the Lunar Reconnaissance Orbiter (LRO) to map the surface of the Moon and collect measurements of potential future landing sites as well as key science targets. After two and a half years in a near-circular polar orbit, LRO entered an elliptical polar orbit on 11 December 2011 with a periapsis (point where the LRO is closest to the surface) near the south pole, and t
Lunokhod 1 rover in its final parking place (38.315°N, 324.992°E) on the surface of Mare Imbrium. The inset in the lower left shows an expanded view of the rover. LROC NAC image M175502049RE. [NASA/GSFC/Arizona State University]. Luna 17, carrying Lunokhod 1, landed on the flood basalt surface of Mare Imbrium on 17 November 1970, after entering orbit on 15 November. Today's Featured Image of Luna
Lunokhod 2 rover parked facing southeast with the lid still open. Rover tracks extend north to the final parking place. The inset is a zoomed in view of the rover, the main rover body is labeled B, the open lid is labeled L and the instrument suite on the front of the rover is labeled I. LROC image M175070494 [NASA/GSFC/Arizona State University]. The Lunokhod 2 rover is still parked on the floor o
LROC's best look yet at the Apollo 11 Landing site. The remnants of Armstrong and Aldrin's historic first steps on the surface are seen as dark paths around the Lunar Module (LM), Lunar Ranging RetroReflector (LRRR) and Passive Seismic Experiment Package (PSEP), as well as leading to and from Little West crater. LROC M175124932R [NASA/GSFC/Arizona State University]. This image of the Apollo 11 lan
A large boulder stopped on its way down a sloping wall in the central peak complex of Schiller crater (51.8°S, 40.0°W). Illumination from the north, image is ~500 m across, NAC M109502471L [NASA/GSFC/Arizona State University]. The lonely journey of this large boulder is apparent from its track in a sloping regolith surface. A casual glance might suggest that it happened last week, or even that its
Low periapsis Narrow Angle Camera image of the Apollo 17 Landing Site. Image is 150 meters wide, Sun from the left, north towards top [NASA/GSFC/Arizona State University]. Normally the Lunar Reconnaissance Orbiter (LRO) orbits the Moon in a 50 km altitude, near-circular, polar orbit. The orbit is “near”-circular, as LRO’s altitude can vary between its lowest altitude (periapsis) of 35 km and its h
LROC WAC mosaic of the lunar nearside [NASA/GSFC/Arizona State University]. For two weeks in mid-December 2010, the LRO spacecraft remained nadir looking (straight down) so that the LROC Wide Angle Camera (WAC) could acquire ~1300 images, allowing the LROC team to construct this spectacular mosaic. As the Moon rotated under LRO's orbit, the ground track progressed from east to west (right to left
The LROC NAC acquired an oblique view of the Marius Hills pit with just the right angle to reveal an overhang! Pit is about 65 meters in diameter, M137929856R [NASA/GSFC/Arizona State University]. Since LRO completes a full cycle of lunar imaging each month, it is possible to follow up previous discoveries and re-image targets under different lighting conditions. The LROC team waited patiently unt
Another amazing bit of lunar geology revealed by LROC! NAC M113168034R, north is up [NASA/GSFC/Arizona State University]. Just when you think you have seen everything, LROC reveals a natural bridge on the Moon! Who would have thought? Natural bridges on the Earth are typically the result of wind and water erosion - not a likely scenario on the Moon. So how did this natural bridge form? The most li
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