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New isotopic evidence supporting moon formation via Earth collision with planet-sized body

Date:
June 5, 2014
Source:
European Association of Geochemistry
Summary:
A new series of measurements of oxygen isotopes provides increasing evidence that the moon formed from the collision of the Earth with another large, planet-sized astronomical body, around 4.5 billion years ago.

The moon. A new series of measurements of oxygen isotopes provides increasing evidence that the moon formed from the collision of the Earth with another large, planet-sized astronomical body, around 4.5 billion years ago.
Credit: NASA/JPL

A new series of measurements of oxygen isotopes provides increasing evidence that the Moon formed from the collision of Earth with another large, planet-sized astronomical body, around 4.5 billion years ago.

This work will be published in Science on 6th June, and will be presented to the Goldschmidt geochemistry conference in California on 11th June.

Most planetary scientists believe that the Moon formed from an impact between Earth and a planet-sized body, which has been given the name Theia. Efforts to confirm that the impact had taken place had centred on measuring the ratios between the isotopes of oxygen, titanium, silicon and others. These ratios are known to vary throughout the solar system, but their close similarity between Earth and Moon conflicted with theoretical models of the collision that indicated that the Moon would form mostly from Theia, and thus would be expected to be compositionally different from Earth.

Now a group of German researchers, led by Dr. Daniel Herwartz, have used more refined techniques to compare the ratios of 17O/16O in lunar samples, with those from Earth. The team initially used lunar samples which had arrived on Earth via meteorites, but as these samples had exchanged their isotopes with water from Earth, fresher samples were sought. These were provided by NASA from the Apollo 11, 12 and 16 missions; they were found to contain significantly higher levels of 17O/16O than their Earthly counterparts.

Dr Herwartz said "The differences are small and difficult to detect, but they are there. This means two things; firstly we can now be reasonably sure that the Giant collision took place. Secondly, it gives us an idea of the geochemistry of Theia. Theia seems to have been similar to what we call E-type chondrites.If this is true, we can now predict the geochemical and isotopic composition of the Moon, because the present Moon is a mixture of Theia and the early Earth. The next goal is to find out how much material of Theia is in the Moon."

Most models estimate that the Moon it is composed of around 70% to 90% material from Theia, with the remaining 10% to 30% coming from the early Earth. However, some models argue for as little as 8% Theia in the Moon. Dr Herwartz said that the new data indicate that a 50:50 mixture seems possible, but this needs to be confirmed.

The team used an advanced sample preparation technique before measuring the samples via stable isotope ratio mass spectrometry, which showed a 12 parts per million ( 3 ppm) difference in 17O/16O ratio between Earth and Moon.


Story Source:

The above story is based on materials provided by European Association of Geochemistry. Note: Materials may be edited for content and length.


Journal Reference:

  1. D. Herwartz, A. Pack, B. Friedrichs, A. Bischoff. Identification of the giant impactor Theia in lunar rocks. Science, 2014; 344 (6188): 1146 DOI: 10.1126/science.1251117

Cite This Page:

European Association of Geochemistry. "New isotopic evidence supporting moon formation via Earth collision with planet-sized body." ScienceDaily. ScienceDaily, 5 June 2014. <www.sciencedaily.com/releases/2014/06/140605141503.htm>.
European Association of Geochemistry. (2014, June 5). New isotopic evidence supporting moon formation via Earth collision with planet-sized body. ScienceDaily. Retrieved August 27, 2014 from www.sciencedaily.com/releases/2014/06/140605141503.htm
European Association of Geochemistry. "New isotopic evidence supporting moon formation via Earth collision with planet-sized body." ScienceDaily. www.sciencedaily.com/releases/2014/06/140605141503.htm (accessed August 27, 2014).

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