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(NASA AS11-40-5877) This photo was used again in Figure 3-12 in the Apollo 11 Preliminary Science Report, which has the following caption: Hasselblad photograph AS11-40-5877 showing an astronaut's bootprint in the lunar surface. This photo was used again in Figure 4-24 in the Apollo 11 Preliminary Science Report, which has the following caption:
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The Passive Seismic Experiment Package (PSEP) was a scientific experiment deployed on the lunar surface by the astronauts of Apollo 11 as part of the Early Apollo Surface Experiments Package (EASEP). The experiment's goal was to determine the structure, tectonic activity, physical nature, and composition of the Moon. [1]
Unlike Apollo 11 though, a higher proportion of these were taken whilst on the surface rather than inside the LM before or after the EVAs. The post-mission Preliminary Science Report [2] indicates that the crew took 23 [3] panoramas whereas the ALSJ records 29 examples. In some cases, the complete, 360° panoramas were impacted by the low Sun ...
NASA's Apollo Site Selection Board announced five potential landing sites on February 8, 1968. These were the result of two years' worth of studies based on high-resolution photography of the lunar surface by the five uncrewed probes of the Lunar Orbiter program and information about surface conditions provided by the Surveyor program. [83]
The Apollo Lunar Surface Experiments Package (ALSEP) comprised a set of scientific instruments placed by the astronauts at the landing site of each of the five Apollo missions to land on the Moon following Apollo 11 (Apollos 12, 14, 15, 16, and 17). Apollo 11 left a smaller package called the Early Apollo Scientific Experiments Package, or EASEP.
The Lunar Sample Laboratory Facility (LSLF) is a repository and laboratory facility at NASA's Lyndon B. Johnson Space Center in Houston, Texas, opened in 1979 to house geologic samples returned from the Moon by the Apollo program missions to the lunar surface between 1969 and 1972. The facility preserves most of the 382 kilograms (842 lb) of ...
The preliminary scientific report of Apollo era [3] indicate that two processes, not mutually excluding, can be responsible for the development of fillets: 1) Deposition of material eroded from the boulder itself by the abrasive action of micrometeoroids, and 2) deposition of ejecta material from distant impact craters against the side of the boulder.