Picture of the Week—Apollo 11 Solar Wind Composition Experiment | Science | Smithsonian

Picture of the Week—Apollo 11 Solar Wind Composition Experiment

NASA didn’t send people to the moon just to bounce around and hit golf balls; Neil Armstrong and Buzz Aldrin of Apollo 11 were performing science experiments during their brief time on the lunar surface. What looks like a white towel next to Aldrin in the photo above was the Solar Wind Composition ...

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Photo courtesy of NASA




NASA didn’t send people to the moon just to bounce around and hit golf balls; Neil Armstrong and Buzz Aldrin of Apollo 11 were performing science experiments during their brief time on the lunar surface. What looks like a white towel next to Aldrin in the photo above was the Solar Wind Composition Experiment:

The Sun continually emits a flux of electrically charged particles into space. This is termed the solar wind. The Earth's magnetic field prevents these charged particles from reaching the Earth's surface, although in the Earth's polar regions, these particles can reach the upper part of the atmosphere, causing auroras. The Moon is outside the Earth's magnetic field for most of each month and has a negligible atmosphere, allowing solar-wind particles to reach the Moon's surface….



The Solar Wind Composition Experiment was performed on Apollo 11, 12, 14, 15, and 16. It consisted of an aluminum foil sheet, 1.4 meters by 0.3 meters, that was deployed on a pole facing the sun. On Apollo 16, a platinum sheet was also used. This foil was exposed to the sun for periods ranging from 77 minutes on Apollo 11 to 45 hours on Apollo 16, allowing solar-wind particles to embed themselves into the foil. The foil was then returned to Earth for laboratory analysis. This allowed the chemical composition of the embedded solar wind to be determined more accurately than would be possible if the measurement were made using remotely controlled instruments on the Moon, but limited the periods at which observations could be made. The isotopes of the light noble gases were measured, including helium-3, helium-4, neon-20, neon-21, neon-22, and argon-36. Some variation in the composition of the solar wind was observed in the measurements from the different mission. These variations were correlated with variations in the intensity of the solar wind as determined from magnetic field measurements.


Behind Aldrin in the photo is the Lunar Module “ Eagle.” A second lunar module, designed for an unmanned test that was deemed unnecessary, now sits in the National Air and Space Museum. Read more about LM-2 in One Great Leap, from the July issue.
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Sarah Zielinski

Sarah Zielinski is an award-winning science writer and editor. She is a contributing writer in science for Smithsonian.com and blogs at Wild Things, which appears on Science News.

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