Images, instrument studies, and rock samples brought back from Apollo missions have provided information about the composition, age, and origin of the Moon.
Images, instrument studies, and rock samples brought back from Apollo missions have provided information about the composition, age, and origin of the Moon.

Our Geological Wonderland: The Moon

The Moon is our closest celestial neighbor. Recognized in antiquity, often saddled with mysterious traits, and considered to sometimes have negative effects on humans and other animals, it remained mostly a mystery until the late 1950s when the first Russian unmanned spacecraft landed on its surface. And so began the “space race.”

The United States was not the first in space or to land on the Moon, beaten by Russia with their Sputnik in 1958, and by Luna 2 with landed in 1959. In response, the U.S. formed the National Aeronautics and Space Administration in 1958 and 11 years later became the first country to land humans on the Moon. This momentous event happened 50 years ago, on July 20, 1969 (Figure 1; Table 1). I think that landing event is perhaps the most spectacular accomplishment of Homo sapiens.

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Figure 1. President JFK at Rice Stadium in Houston, Texas Sept. 12, 1962. Of note, at that time a poll indicated that 58 percent of the U.S. population was not in favor of this program!

Launched from the Kennedy Space Center at Cape Canaveral, Florida July 16, NASA’S Apollo 11 spacecraft carried three Astronauts, Neil Armstrong, Edwin (Buzz) Aldrin and Michael Collins and landed safely on the Moon’s surface (Figure 1). Armstrong was first to descend the ladder and walk on the surface followed shortly thereafter by Aldrin. Collins stayed aboard in case of trouble (Figure 2). All three were brought back safely, landing in the Pacific Ocean July 24. In all, NASA sent six manned Apollo missions to the Moon between 1969 and 1972, and a total of 12 astronauts walked on its surface.

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Figure 2. Saturn V rocket blasts off from the John F. Kennedy Space Center at Cape Canaveral July 16, 1969.
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Table 1. Brief history of space explorations to the Moon.

Apollo 11 carried three astronauts in a trip that extended from liftoff from Florida July 16 to splash down July 24 in the Pacific Ocean (Figure 3). Two of the three astronauts spent July 20 exploring the surface, performing experiments and collecting rock and soil samples from the landing site.

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Figure 3. Three astronauts aboard Apollo 11 (left to right), Neil Armstrong, Michael Collins and Edwin Aldrin.

Armstrong was first to descend the ladder and walk on the surface followed shortly thereafter by Aldrin. Collins stayed aboard in case of trouble (Figure 4). All three were brought back safely, landing in the Pacific Ocean July 24. In all, NASA sent six manned Apollo missions to the Moon between 1969 and 1972, and a total of 12 astronauts walked on its surface.

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Figure 4. Neil Armstrong (left) and Edwin Aldrin (right) descending onto the surface of the Moon July 20, 1969.

To note here is the recent passing of Christopher Columbus Kraft July 22, 2019. He was the first director of NASA’S Mission Control and guided most of America’s space explorations, including the first crewed spaceflight, first crewed orbital flight, first spacewalk, and first manned mission to the Moon. The current NASA mission control building is named in his honor.

What did we learn?

Surface images, instrument studies, and lunar rock samples brought back from Apollo missions have provided considerable information about the composition, age, and origin of the Moon (Table 2).

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Table 2. Characteristics and features of the Moon.

Most of the lunar crust and surface consists of igneous rocks such as basalt and anorthosite, both of which occur on Earth. Chemical isotopic composition of these rocks is very similar to that of Earth (Figure 5). Other materials include impact breccias and lunar “soil” (Figure 6).

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Figure 5. Fist-sized samples of vesicular basalt. Holes result from release in pressure and escaping gasses during cooling at the surface. Left. Sample from the Moon, dated at almost 4 billion years old. Right. Sample from Earth. Similar basalt can be found in St. George and other volcanic areas such as Hawaii and Iceland.
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Figure 6. Other samples from the Moon. A. Igneous rock called anorthosite, which also occurs on Earth. B. Breccia consisting of various rock fragments formed from impacts. C. Volcanic ash and cinders which make up the lunar “soil.”

Various samples of moon rocks returned to earth have been radiometrically dated, with the oldest samples nearly 4.5 billion years in age. These samples, and other information gathered by NASA explorations indicate that the composition of the moon is very similar to that of the outer crust and mantle of Earth (Figure 7). Combining information about the composition and age of lunar rocks has provided support for the hypothesis that the Moon formed as a result of an impact with another planet very early in its history (Figure 8).

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Figure 7. Internal structure of the Moon.
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Figure 8. Hypothesis that a Mars sized planet called Theia glanced off Earth early in its history (between 5-4.5 billion years ago) when Earth was still mostly molten. The collision blew a portion of the Earth out into orbit to become the Moon. The ejected material was mostly from the mantle as indicated by its composition.

Proximity of the Moon to Earth and its gravitational pull over the past 4.5 billion years has affected the Earth. We recognize the daily diurnal and monthly changes in ocean tides. There was another unproven prediction by astronomers that this gravitational pull should have affected the Earth’s rotational rate over time. Proof for this hypothesis was first discovered accidentally in the early 1960s by, surprisingly, a paleontologist named John W. Wells who was studying fossilized corals from the rock record. His discovery was the changes in number of daily growth lines, which could be recognized in the calcium carbonate skeletons of fossilized and modern invertebrates (Figure 9).

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Figure 9. A result of the tidal pull of the Moon, Earth has been spinning slower on its axis through geologic time. This was discovered by counting the number of microscopic daily growth lines in marine-dwelling invertebrates from the fossil record and from modern specimens. Wells, J.W. (1963a). “Coral growth and geochronometry”. Nature. 197: 948–950.

Human interest

Over and above moon related things such as Moon Pies, moonshine and lunatics are a couple of thought-provoking observations (Figures 10 and 11).

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Figure 10. A recognition by Neil Armstrong of just how incredibly insignificant and fragile our “blue planet” really is in the overall pattern of the universe.
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Figure 11. Almost 4 million years of “progress.” Bipedal hominid footprints/boot prints in the sands of time. In these examples, the sands are volcanic ash.

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Rick Miller
Rick Miller is a semi-retired professor of geological sciences (San Diego State University) with primary interests in microscopic fossils and the history of our planet Earth. He moved to St. George in 2001 because of the beauty and geological setting. He has maintained a strong interest in teaching (and was at DSU as an adjunct in 2010-2015) and volunteer lecturing on topics within the geological sciences for the Institute for Continued Learning (2004-present) and the Community Education Program (starting this spring). He also enjoy vigorous exercise, bowling, old Corvettes and Chevy trucks, and caring for animals of all types. Writing is also a very satisfying hobby.

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