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First crystal-structure determination of olivine in diamond: Composition and implications for provenance in the Earth's mantle. (Articolo in rivista)
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- First crystal-structure determination of olivine in diamond: Composition and implications for provenance in the Earth's mantle. (Articolo in rivista) (literal)
- Anno
- 2011-01-01T00:00:00+01:00 (literal)
- Alternative label
Nestola, F. (1),(2), Nimis, P.(1),(2), Ziberna, L.(1), Longo, M., Marzoli(1), A., Harris, J.W. (3), Manghnani, M.H.(4), Fedortchouk, Y. (5) (2011)
First crystal-structure determination of olivine in diamond: Composition and implications for provenance in the Earth's mantle.
in Earth and planetary science letters; Elsevier, Amsterdam (Paesi Bassi)
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- Nestola, F. (1),(2), Nimis, P.(1),(2), Ziberna, L.(1), Longo, M., Marzoli(1), A., Harris, J.W. (3), Manghnani, M.H.(4), Fedortchouk, Y. (5) (literal)
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- ID_PUMA:/cnr.igg/2011-A0-047Area di valutazione 04 - Scienze della Terra (literal)
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- (1) Department of Geoscience, University of Padua, Padova, Italy;
(2) IGG-CNR, UO Padova, Italy;
(3) Department of Geographical and Earth Sciences, University of Glasgow, United Kingdom;
(4) Hawaii Institute of Geophysics and Planetology, University of Hawaii, Honolulu, United States;
(5) Department of Earth Sciences, Dalhousie University, Canada. (literal)
- Titolo
- First crystal-structure determination of olivine in diamond: Composition and implications for provenance in the Earth's mantle. (literal)
- Abstract
- We report for the first time a complete X-ray diffraction in-situ crystal-structure refinement of a single crystal
of olivine still trapped in a diamond (Udachnaya kimberlite, Siberia). A two-step experimental procedure,
consisting of accurate crystal centering using a four-circle diffractometer equipped with a point detector and
subsequent collection of complete intensity data using a second diffractometer equipped with a CCD detector,
allowed us to overcome previously reported experimental problems and to refine the crystal structure
without extracting the inclusion from the diamond host. The data allowed us to obtain the cation distribution
over the two crystallographic M2 and M1 sites, which provided composition of olivine inclusion as Fo92.7(4). A
novel experimental calibration of the pressure-volume equation of state for such composition was obtained
using new in situ high-pressure X-ray data on a Fo92 olivine single-crystal and new established compositional
effects on olivine unit-cell volume. Such equation of state allowed us to determine the internal pressure at the
olivine inclusion, Pi=0.40(1)GPa. The value for the internal pressure compares well with but has lower
uncertainty than estimates obtained using micro-Raman spectrometry for similar olivine inclusions in
diamonds from the same kimberlite. Taking into account elastic relaxation of the diamond-olivine pair to
ambient P-T, we determined formation pressures of 3.5 GPa to 4.9 GPa, depending on the assumed
temperature (800 °C to 1300 °C). These values suggest formation near the graphite-diamond boundary and
are comparable to estimates from conventional and Raman thermobarometry for other peridotitic inclusions
in Siberian diamonds. (literal)
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