Quantifying noble gas contamination during terrestrial alteration in Martian meteorites from Antarctica
Version of Record online: 10 APR 2013
© The Meteoritical Society, 2013.
Meteoritics & Planetary Science
Volume 48, Issue 6, pages 929–954, June 2013
How to Cite
Schwenzer, S. P., Greenwood, R. C., Kelley, S. P., Ott, U., Tindle, A. G., Haubold, R., Herrmann, S., Gibson, J. M., Anand, M., Hammond, S. and Franchi, I. A. (2013), Quantifying noble gas contamination during terrestrial alteration in Martian meteorites from Antarctica. Meteoritics & Planetary Science, 48: 929–954. doi: 10.1111/maps.12110
- Issue online: 13 JUN 2013
- Version of Record online: 10 APR 2013
- Manuscript Accepted: 21 FEB 2013
- Manuscript Received: 26 JUN 2012
- STFC. Grant Number: ST/I001964/1ST/I001964/1
We investigated exterior and interior subsamples from the Martian shergottite meteorites Allan Hills (ALH) A77005 and Roberts Massif (RBT) 04261 for secondary minerals, oxygen isotopes, Ar-Ar, and noble gas signatures. Electron microprobe investigations revealed that RBT 04261 does not contain any visible alteration even in its most exterior fractures, whereas fracture fillings in ALHA77005 penetrate into the meteorite up to 300 μm, beyond which the fractures are devoid of secondary minerals. Light noble gases seem to be almost unaffected by terrestrially induced alteration in both meteorites. Thus, a shock metamorphic overprint of 30–35 GPa can be deduced from the helium measurements in RBT 04261. Oxygen isotopes also seem unaffected by terrestrially weathering and variations can easily be reconciled with the differences in modal mineralogy of the exterior and interior subsamples. The measurements on irradiated samples (Ar-Ar) showed a clear Martian atmospheric contribution in ALHA77005, but this is less apparent in our sample of RBT 04261. Exterior and interior subsamples show slight differences in apparent ages, but the overall results are very similar between the two. In contrast, krypton and xenon are severely affected by terrestrial contamination, demonstrating the ubiquitous presence of elementally fractionated air in RBT 04261. Although seemingly contradictory, our results indicate that RBT 04261 was more affected by contamination than ALHA77005. We conclude that irrespective of on which planet the alteration occurred, exposure of Martian rocks to atmosphere (or brine) introduces noble gases with signatures elementally fractionated relative to the respective atmospheric composition into the rock, and relationships of that process with oxygen isotopes or mineralogical observations are not straightforward.