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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:
The combined TV/DAC camera/Photography/audio video hosted on YouTube as "Apollo 11 Moonwalk Part 1 of 4" [9] includes the Flight Director's audio loop as well as the CapCom-Crew audio. At 8 minutes 53 seconds into the video (109:30:53 MET) Armstrong states "I'll step out and take some of my first pictures here.", at 9:03 video/109:31:05 MET ...
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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 original slow-scan television signal from the Apollo TV camera, photographed at Honeysuckle Creek on July 21, 1969. The Apollo 11 missing tapes were those that were recorded from Apollo 11's slow-scan television (SSTV) telecast in its raw format on telemetry data tape at the time of the first Moon landing in 1969 and subsequently lost.
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]
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 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.