Apollo 9 astronaut and Lunar Module Pilot Rusty Schweickart paid a visit to the Lunar Orbiter Image Recovery (LOIRP) facility in Building 596 (aka “McMoon’s) at NASA Ames Research Park today. Pictured (L to R) Keith Cowing, LOIRP-co-lead, Rusty Schweikart, Austin Epps LOIRP, Neulyn Moss LOIRP, and Dennis Wingo, LOIRP co-lead.
Schweickart also signed our FR-900 tape drive as have other distinguished visitors before have done (image below)
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“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 17 and Lunokhod 1 was obtained during a low altitude (33 km) pass providing the highest resolution view yet of the landing site.”
Luna 24 landed on the northwestern rim of a 64 m diameter impact crater, on the volcanic plains of Mare Crisium. Enlargement of lander at lower left, NAC M174868307L [NASA/GSFC/Arizona State University].
Three Soviet missions (Luna 16, Luna 20, and Luna 24) successfully collected and returned pieces of the lunar surface. Before the successful Luna 24 sample return mission in August 1976, Luna 23 was sent two years earlier (November 1974) to nearly the same location in Mare Crisium, but was unsuccessful.
Luna 24 landed in Mare Crisium on 18 August 1976 to complete the unfinished mission of Luna 23. The landing sites of Luna 23 and 24 are only 2.3 km apart. The region of Mare Crisium where they landed is a typical smooth mare surface with little relief in the immediate vicinity. There are numerous secondary craters scattered across the region, and Luna 24 landed on the edge of one of these. The secondary craters are the result of an impact to the northeast of the landing site, perhaps from the crater Giordano Bruno.
More information and imagery.
Integrating LRO Data Products for Preliminary North Pole Rover Mission Planning
“The authors believe that the selection of future sites for unmanned exploration of the Lunar surface should be driven by several short and long term objectives to maximize not only the scientific value of the selected site, but also the applicability of ground- truth data obtained from the surface to the longer term goal of Lunar resource utilization. Sites selected for unmanned surface science missions, such as the one being proposed in this document, will be a natural location of future outposts both unmanned and manned. Those outposts, in turn, become the natural beginnings for the economic development of the Moon’s resources.”
Image: GRAIL’s MoonKAM Looks Homeward Toward Earth
“This image of the far side of the lunar surface, with Earth in the background, was taken by the MoonKAM system onboard the Ebb spacecraft as part of the first image set taken from lunar orbit from March 15 – 18, 2012. A little more than half-way up and on the left side of the image is the crater De Forest. Due to its proximity to the southern pole, DeForest receives sunlight at an oblique angle when it is on the illuminated half of the Moon.”
Unfortunately, Luna 23 experienced a malfunction and hit the surface at a very high velocity. Contact was maintained between Earth and the spacecraft after landing, but a sample could not be acquired. At the time, the cause of the failure was not known, but it seemed probable that the whole spacecraft tipped over upon landing at an unexpectedly high velocity. Indeed, the high resolution LROC NAC image (below) shows the spacecraft lying on its side!
More information and imagery.
The Apollo 12 landing site in Oceanus Procellarum imaged during the second LRO low-altitude campaign. Image width is 225 m, NAC Image M175428601R [NASA/GSFC/Arizona State University].
The LRO mission continues to collect observations that are enabling ground-breaking new scientific discoveries about the Moon. As geologists, whenever we look at remotely sensed data collected from another planet, in a sense we are staring back in time. But this is the “deep time” of geology, where we are trying to understand natural processes that (at least on the Moon, anyway) could have happened billions of years ago. But the LRO mission is unique because we can also see human history. Not just any history, either, but one of humanity’s greatest accomplishments, our first steps on another world. Twelve astronauts explored the lunar surface, directly seeing things with their own eyes, making observations, and collecting samples with their own hands. These samples and observations revolutionized our understanding of our solar system.
This “snapshot in time” effect is especially evident at the Apollo 12 landing site in Oceanus Procellarum, now known as Statio Cognitum. Here, you can see the remnants of not one, but two missions to the Moon. Astronauts Pete Conrad and Alan Bean demonstrated that a precision lunar landing with the Apollo system was possible, enabling all of the targeted landings that followed. Bean and Conrad collected rock samples and made field observations, which resulted in key discoveries about lunar geology. They also collected and returned components from the nearby US Surveyor 3 spacecraft, which landed at this site almost two and half years previously, providing important information to engineers about the how materials survive in the lunar environment.
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 landing site captured from just 24 km (15 miles) above the surface provides LRO’s best look yet at humanity’s first venture to another world. When Neil Armstrong took his famous first steps onto the lunar surface, he kicked around the soil. “Yes, the surface is fine and powdery.” Gazing at the flat horizon, he took in the view. “Isn’t that something! Magnificent sight out here.” After collecting a contingency sample Neil looked around and observed, “it has a stark beauty all its own. It’s like much of the high desert of the United States. It’s different, but it’s very pretty out here.” A few minutes later Buzz Aldrin descended the ladder and joined Neil on the surface of the Moon!
You can see the remnants of their first steps as dark regions around the Lunar Module (LM) and in dark tracks that lead to the scientific experiments the astronauts set up on the surface. The Passive Seismic Experiment Package (PSEP) provided the first lunar seismic data, returning data for three weeks after the astronauts left, and the Laser Ranging RetroReflector (LRRR) allows precise measurements to be collected to this day. You can even spot the discarded cover of the LRRR.
Another trail leads toward Little West crater around 50 meters (164 feet) to the east of the LM. This was an unplanned excursion near the end of the two and a half hours spent on the surface. Armstrong ran over to get a look inside the crater, and this was the farthest either astronaut ventured from the landing site. Compared to Apollo 12 and 14, which allowed for more time on the surface, and Apollo 15, 16, and 17, which had the benefit of a Lunar Roving Vehicle, Armstrong and Aldrin’s surface activities were quite restricted. Their tracks cover less area than a typical city block!
The Apollo 15 Lunar Module (LM) Falcon set down on the Hadley plains (26.132*N, 3.634*E) a mere 2 kilometers from Hadley Rille. The goals: sample the basalts that compose the mare deposit, explore a lunar rille for the first time, and search for ancient crustal rocks. Additionally, Dave Scott and Jim Irwin deployed the third Apollo Lunar Surface Experiments Package (ALSEP) and unveiled the first Lunar Roving Vehicle (LRV). The ALSEP consisted of several experiments that were powered by a Radioisotope Thermoelectric Generator (RTG) and sent back valuable scientific data to the Earth for over six years after the astronauts left. This new LROC NAC image taken from low altitude shows the hardware and tracks in even more detail.
The LRV, a lunar “dune buggy”, allowed the astronauts to traverse far from the LM and explore much more local geology than the astronauts on previous missions (Apollo 11, 12, 14). Not only did the LRV allow the astronauts to move from place-to-place at a lively rate of eight to sixteen kilometers per hour (five to ten miles per hour), but the LRV also allowed brief periods of rest that in turn helped to conserve oxygen.
The LRV wheels were 82 centimeters (32 inches) in diameter, and 23 centimeters (9 inches) wide. Typically LROC NAC pixels are about 50 centimeters square, so it is not always easy to pick out the LRV tracks. In previous LROC images, the LRV tracks are usually only visible near the LM where the descent engine exhaust plume disturbed the surface. The LRV wheels broke through the changed surface and thus the tracks have more contrast near the LM.
For two one-month periods last year (2011), the LRO orbit was lowered such that overflights of the Apollo sites were only 25 to 30 kilometers, rather than the usual 50 kilometers. These low passes resulted in NAC pixel scales near 25 centimeters! LRO has a ground speed of a bit over 1600 meters (5249 feet) per second, and the shortest NAC exposure time is 0.34 millseconds, so images taken from this low altitude are smeared down track a bit. However, the smear is hardly noticeable and features at the Apollo sites definitely come into sharper focus. In this new low-altitude NAC image of the LRV, tracks are visible about half of the time, usually when the tracks are at an angle to the Sun direction, rather than parallel.