Grant: Discovery Grants Program - Individual
University of Western Ontario
$33,000.00
Experimental Studies of Earth Materials at Extreme Pressure and Temperature Conditions of Planetary Interiors
FY 2014-15
Summary
How do planets work? Large scale processes deep in the interior of planets control much of what happens on the surface. For example, heat and mass flow within and from Earth's core through the mantle causes plate motions, earthquakes, and generates our life-protecting magnetic field. The cores of terrestrial-like planetary bodies, Earth, Mercury, Venus, Mars, and Jupiter's moons Io and Ganymede, are composed mainly of iron (Fe) with ~10-20wt% of other lighter elements such as sulfur (S) and/or silicon (Si). Our knowledge of the physical and chemical properties of core mimetic materials is central to improving our understanding of the integrated global processes of heat and mass flow inside these planetary bodies. My research focuses on high pressure (P), temperature (T) experimental studies of the physico-chemical properties of the materials deep in planetary interiors. We bring the inaccessible deep interior of planets into the lab by measuring properties of core and mantle materials under simultaneous extreme P (23GPa) and T (2300K) conditions in four large volume presses. My team will employ novel techniques developed in our lab to measure viscosity, electrical and thermal conductivity, density, and acoustic properties of core (Fe-S-Si) and mantle (serpentinite, olivine) materials. Our short term goals are to answer questions such as: Are Fe-S and Fe-Si in the core? What are the electrical and thermal conductivities of these binary systems? Does the solute affect these properties which are so important for core processes such as the geodynamo and conductive heat flow in terrestrial-like bodies? Can uranium dissolve in Fe and be a possible energy source in the core that helps drive Earth's heat engine? Are deep earthquakes triggered by mineral phase transitions? Answers to these questions on the micro-scale behaviour of planetary materials lead to a better understanding of the macro-scale processes that they control and help explain how planets work. The proposed work will involve 1 PDF, 8 PhD, 2 MSc and 2 BSc students, 1 research assistant and 7 technical personnel. My HQP will receive extensive training in experimental high P,T mineral physics which will prepare them for employment in academic, government and private sectors.
Program
Discovery Grants Program - Individual
Recipient
Location
Ontario, Canada
Recipient Type
Academia
Type
Grant
Source
NSERC's Awards Data
As published
Application id
105604-2013
Name nom
Secco, Richard
Department département
Earth Sciences
Organization id
36
Institution établissement
University of Western Ontario
Province en
Ontario
Province fr
Ontario
Country en
CANADA
Country fr
CANADA
Fiscal year exercice financier
2014
Competition year année de concours
2013
Award amount
33000
Program id
RGPIN
Program name en
Discovery Grants Program - Individual
Program name fr
Programme de subventions à la découverte - individuelles
Group en
Discovery grants programs
Group fr
Programmes de subventions à la découverte
Committee code
1506
Committee name en
Geosciences
Committee name fr
Géosciences
Area of application code
1203
Area of application group en
Advancement of knowledge
Area of application group fr
Avancement des connaissances
Area of application en
Earth sciences
Area of application fr
Sciences de la terre
Research subject code
4306
Research subject group en
Geophysics
Research subject group fr
Géophysique
Research subject en
Mineral physics
Research subject fr
Physique des minéraux
Partie
2
Nb partie
5
Application title
Experimental Studies of Earth Materials at Extreme Pressure and Temperature Conditions of Planetary Interiors
Keyword
NSERC
Application summary
How do planets work? Large scale processes deep in the interior of planets control much of what happens on the surface. For example, heat and mass flow within and from Earth's core through the mantle causes plate motions, earthquakes, and generates our life-protecting magnetic field. The cores of terrestrial-like planetary bodies, Earth, Mercury, Venus, Mars, and Jupiter's moons Io and Ganymede, are composed mainly of iron (Fe) with ~10-20wt% of other lighter elements such as sulfur (S) and/or silicon (Si). Our knowledge of the physical and chemical properties of core mimetic materials is central to improving our understanding of the integrated global processes of heat and mass flow inside these planetary bodies. My research focuses on high pressure (P), temperature (T) experimental studies of the physico-chemical properties of the materials deep in planetary interiors. We bring the inaccessible deep interior of planets into the lab by measuring properties of core and mantle materials under simultaneous extreme P (23GPa) and T (2300K) conditions in four large volume presses. My team will employ novel techniques developed in our lab to measure viscosity, electrical and thermal conductivity, density, and acoustic properties of core (Fe-S-Si) and mantle (serpentinite, olivine) materials. Our short term goals are to answer questions such as: Are Fe-S and Fe-Si in the core? What are the electrical and thermal conductivities of these binary systems? Does the solute affect these properties which are so important for core processes such as the geodynamo and conductive heat flow in terrestrial-like bodies? Can uranium dissolve in Fe and be a possible energy source in the core that helps drive Earth's heat engine? Are deep earthquakes triggered by mineral phase transitions? Answers to these questions on the micro-scale behaviour of planetary materials lead to a better understanding of the macro-scale processes that they control and help explain how planets work. The proposed work will involve 1 PDF, 8 PhD, 2 MSc and 2 BSc students, 1 research assistant and 7 technical personnel. My HQP will receive extensive training in experimental high P,T mineral physics which will prepare them for employment in academic, government and private sectors.