A celestial body about the size of the moon slams into a planetary body the size of Mercury in this artist's conception. Credit: NASA/JPL-Caltech

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FOR RELEASE ON Wednesday, October 17, 2012 10:00 AM PDT

Wednesday, October 17, 2012


Massive Planetary Collision May Have Zapped Key Elements from Moon

New study traces moon evaporation and leads to questions about why Earth has so much water

Scripps Institution of Oceanography / University of California, San Diego

Fresh examinations of lunar rocks gathered by Apollo mission astronauts have yielded new insights about the moon's chemical makeup as well as clues about the giant impacts that may have shaped the early beginnings of Earth and the moon.

Geochemist James Day of Scripps Institution of Oceanography at UC San Diego and colleagues Randal Paniello and Frédéric Moynier at Washington University in St. Louis used advanced technological instrumentation to probe the chemical signatures of moon rocks obtained during four lunar missions and meteorites collected from the Antarctic. The data revealed new findings about elements known as volatiles, which offer key information about how planets may have formed and evolved.

A cross-polarized transmitted-light image of a polished section of Apollo sample 12021.

The researchers discovered that the volatile element zinc, which they call "a powerful tracer of the volatile histories of planets," is severely depleted on the moon, along with most other similar elements. This led them to conclude that a "planetary-scale" evaporation event occurred in the moon's history, rather than regional evaporation events on smaller scales.

The results are published in the October 18 issue of the journal Nature.

"This is compelling evidence of extreme volatile depletion of the moon," said Day. "How do you remove all of the volatiles from a planet, or in this case a planetary body? You require some kind of wholesale melting event of the moon to provide the heat necessary to evaporate the zinc."

According to Day, a gigantic planetary collision resulting in global transformations might be responsible for eradicating such elements. Day recently led a study in the journal Nature Geoscience that showed how such a collision might have brought precious metals such as gold and platinum to Earth, likely just after the solar system formed (http://explorations.ucsd.edu/research-highlights/2012/not-of-this-world).

James Day

To derive the findings published in the new study, the researchers employed a mass spectrometer device, an advanced instrument that precisely measures the ratios of isotopes of a particular chemical element, which Day said revealed information not accessible even five years ago. Comparing the zinc composition of moon rocks with rocks from Earth and Mars revealed severe depletions in the lunar samples.

The researchers argue in the paper that such a disparity points to a large-scale evaporation of zinc, "most likely in the aftermath of the Moon-forming event, rather than small-scale processes during volcanic processes."

The next stage of this research, Day said, is to investigate why Earth is not similarly depleted of zinc and similar volatile elements, a line of exploration which could lead to answers about how and why the earth is mostly covered by water.

"Where did all the water on Earth come from?" asked Day. "This is a very important question because if we are looking for life on other planets we have to recognize that similar conditions are probably required. So understanding how planets obtain such conditions is critical for understanding how life ultimately occurs on a planet."

Although the Apollo mission rocks were collected more than 40 years ago, the new study proves they are still offering new insights.

Apollo 17 astronaut Jack Schmitt at the lunar rover near Shorty Crater, Taurus-Littrow valley of the moon. Image courtesy of J. Schmitt, the Apollo 17 crew and NASA

"They still have a lot of science to be done on them and that's exciting," said Day. "Hopefully these kinds of results will help push for future sample collection missions to try to more fully understand the moon."

The NASA Lunar Advanced Science and Exploration Research and Cosmochemistry programs supported the research, which is representative of the work of planetary scientists at Scripps.

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About Scripps Institution of Oceanography
Scripps Institution of Oceanography at University of California, San Diego, is one of the oldest, largest and most important centers for global science research and education in the world. Now in its second century of discovery, the scientific scope of the institution has grown to include biological, physical, chemical, geological, geophysical and atmospheric studies of the earth as a system. Hundreds of research programs covering a wide range of scientific areas are under way today in 65 countries. The institution has a staff of about 1,400, and annual expenditures of approximately $170 million from federal, state and private sources. Scripps operates robotic networks, and one of the largest U.S. academic fleets with four oceanographic research ships and one research platform for worldwide exploration. Birch Aquarium at Scripps serves as the interpretive center of the institution and showcases Scripps research and a diverse array of marine life through exhibits and programming for more than 415,000 visitors each year. Learn more at scripps.ucsd.edu.


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