Fabrizio Nestola

Fabrizio Nestola

orcid

Research Focus & Metrics

Academic Career Length

26Years (2001-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

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12 March 2014 in Nature
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Journal Article
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DPD. G. Pearson
D. G. Pearson
FBF. E. Brenker
F. E. Brenker
FNFabrizio Nestola
Fabrizio Nestola
JMJ. McNeill
J. McNeill
LNL. Nasdala
L. Nasdala
LVL. Vincze
L. Vincze

20 June 2016 in Journal of Applied Crystallography
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Journal Article
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JGJavier Gonzalez-Platas
Javier Gonzalez-Platas
Matteo AlvaroMatteo Alvaro
Matteo Alvaro
FNFabrizio Nestola
Fabrizio Nestola
RARoss Angel
Ross Angel

1 January 2013 in Reviews in Mineralogy and Geochemistry
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Journal Article
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SSSteven B. Shirey
Steven B. Shirey
PCPierre Cartigny
Pierre Cartigny
DFDaniel J. Frost
Daniel J. Frost
SKShantanu Keshav
Shantanu Keshav
FNFabrizio Nestola
Fabrizio Nestola
MWMichael J. Walter
Michael J. Walter
Earth’s carbon, derived from planetesimals in the 1 AU region during accretion of the Solar System, still retains similarities to carbon found in meteorites (Marty et al. 2013) even after 4.57 billion years of geological processing. The range in isotopic composition of carbon on Earth versus meteorites is nearly identical and, for both, diamond is a common, if volumetrically minor, carbon mineral (Haggerty 1999). Diamond is one of the three native carbon minerals on Earth (the other two being graphite and lonsdaleite). It can crystallize throughout the mantle below about 150 km and can occur metastably...

16 December 2016 in Science
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ESEvan M. Smith
Evan M. Smith
SSSteven B. Shirey
Steven B. Shirey
FNFabrizio Nestola
Fabrizio Nestola
EBEmma S. Bullock
Emma S. Bullock
JWJianhua Wang
Jianhua Wang
WWWuyi Wang
Wuyi Wang
Diamonds rock their metal roots: Massive diamonds are rare, expensive, and captivating. These diamonds now appear to be distinctive not only in their size but also in their origin. Smith et al. probed mineral inclusions from these very large diamonds and found abundant slivers of iron metal surrounded by reducing gases. This suggests that the large diamonds grew from liquid metal in Earth's mantle. The inclusions also provide direct evidence of a long-suspected metal precipitation reaction that requires a more reducing mantle. Science , this issue p. 1403

1 August 2006 in Geophysical Research Letters
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JSJ. R. Smyth
J. R. Smyth
DFD. J. Frost
D. J. Frost
FNFabrizio Nestola
Fabrizio Nestola
CHC. M. Holl
C. M. Holl
GBG. Bromiley
G. Bromiley
Although water controls the biology and geology of the surface, hydrogen is perhaps the most poorly constrained compositional variable in the bulk Earth. Its concentration in the upper mantle appears to be controlled by its solubility as hydroxyl in the nominally anhydrous silicate phases, olivine, pyroxene, garnet, wadsleyite, and ringwoodite. Here we describe a series of experiments showing that the solubility of H2O in olivine at 12 GPa increases with temperature to 8900 ppm by weight at 1250°C and decreases at higher temperature with the onset of melting. Sample characterization by infrared spectroscopy indicates that the primary hydration mechanism is the substitution of 2H+ for Mg2+. Similar results obtained from samples coexisting with clinohumite (low‐silica) and with clinoenstatite (high‐silica) indicate that silica activity has minimal effect on hydration under these conditions. Single‐crystal X‐ray diffraction measurements constrain the volume of hydration and indicate significant M‐site vacancies. Hydrogen thus appears to become a geochemically compatible element as depths approach 400 km.

1 August 2010 in Physics of the Earth and Planetary Interiors
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BPBrent T. Poe
Brent T. Poe
CRClaudia Romano
Claudia Romano
FNFabrizio Nestola
Fabrizio Nestola
JSJoseph R. Smyth
Joseph R. Smyth