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Moon formed after collision of planets

06.06.2014

Göttingen scientists confirm “Giant impact“ theory – Lunar samples analyzed at Göttingen University

Scientists from the Universities of Göttingen, Cologne, and Münster in Germany have resolved an isotopic difference between the Earth and the Moon.

The slight variation in oxygen isotopes confirms the “Giant impact“ hypothesis of Moon formation, according to which the Moon formed from the debris of a giant collision between the Earth and another proto-Planet about 4.5 billion years ago. The results were published in the journal Science.

In the Stable Isotope Laboratory at Göttingen University’s Geoscience Centre, the scientists analyzed samples from the Moon that were provided by NASA. The lunar basalts were brought back to Earth between 1969 and 1972 with Apollo Missions 11, 12, and 16.

They released the oxygen from the rocks, purified it and measured the pure oxygen gas in the mass spectrometer. “For the first time, we were able to show a subtle difference between the rare 17O isotope and the abundant 16O isotope,” explains Dr. Daniel Herwartz, who lead the study at Göttingen University and is now employed at the University of Cologne.

“The similar isotopic composition of Earth and Moon appeared to be at odds with the giant impact hypothesis, because numerical models of the collision predicted a difference. The difference we found is smaller than initially predicted, but that might be due to the fact that both planets originated from the same region of the solar system.”

Only a few laboratories worldwide are able to measure the rare 17O isotope at all. “For the last three years, staff and students in Göttingen have persistently worked on improving the analytical procedure,” says Prof. Dr. Andreas Pack, head of the Stable Isotope Laboratory at Göttingen University’s Geoscience Centre.

“The results of this study show that this effort has paid off.” Some of the data were measured by student Bjarne Friedrichs for his Bachelor’s thesis.

Original publication: Daniel Herwartz, Andreas Pack, Bjarne Friedrichs, Addi Bischoff. Identification of the giant impactor Theia in lunar rocks. Science 2014. Doi: 10.1126/science.1251117.

Contact:
Dr. Daniel Herwartz
University of Cologne – Environmental Isotope Geochemistry
Greinstraße 4-6, 50939 Köln, Germany
Phone +49 221 470-3240 or +49 177 319 4278
Email: d.herwartz@uni-koeln.de

Prof. Dr. Andreas Pack
University of Göttingen
Geoscience Centre – Department of Isotope Geology
Goldschmidtstraße 3, 37077 Göttingen, Germany
Phone +49 551 39-12254 or +49 175 298 1638
Email: apack@uni-goettingen.de

Prof. Dr. Addi Bischoff
University of Münster
Institute for Planetology
Wilhelm-Klemm-Str. 10, 48149 Münster, Germany
Phone +49 251 83-33465
E-Mail: bischoa@uni-muenster.de

Weitere Informationen:

http://www.geologie.uni-koeln.de/1720.html
http://www.uni-goettingen.de/en/77365.html
http://www.uni-muenster.de/Planetology/ifp/personen/bischoff_addi/addihome.html

Thomas Richter | Georg-August-Universität Göttingen

Further reports about: Earth Environmental Geoscience Identification Moon Planetology collision difference isotope lunar

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