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When the mighty Saturn V left the launch pad on July 16th, 1969, a new chapter was opened in the scientific understanding of the Moon. Already before the mission had scientists from the US initially Daniel Barringer and later Eugene Shoemaker postulated the theory that the craters on the Moon have not formed through volcanic activity, but by meteorite impact. Those colleagues had the opportunity to put together the evidence on Earth, where they could establish the different geologic contexts of volcano and meteorite craters: close to meteorite craters they found heavily shocked quartz rocks that could have formed under the extreme temperatures and pressures of a meteorite impact. This was widely accepted. The theory that also the lunar craters are the product of meteorites was rejected by the science community. Shoemaker cold not convince his colleagues at the time. Now it was the Apollo astronaut’s turn to explore the geology of the fractured lunar surface. All together they brought back 382 kilogrammes of lunar rocks and dust in the time frame between 1969 and 1972. This precious set of samples is still analysed in terrestrial labs to the present date, and it has a lot to tell about the story of the Moon as we will see in a moment. Immediately after the first lunar rocks were split in the lab the diagnosis was clear: shocked quartz no matter where people looked with the microscope. Like many times before natural science went through a shift of paradigm. Meteorites were the main actors of planetary surface gardening not volcanoes.
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