Grant: Discovery Grants Program - Individual
University of Western Ontario
$61,000.00
Experimental Studies of Earth and Planetary Materials at Extreme Conditions of Pressure and Temperature
FY 2018-19
Summary
Large scale processes of heat and mass movement deep in the interior of planets control much of what happens on the surface. The focus of Dr. Secco's research program is to bring the inaccessible deep interior of planets into the lab by measuring physical properties of core and mantle materials under simultaneous extreme pressure (0-23GPa) and temperature (220-2300K) conditions in four large volume presses one of which is the largest capacity research press in North America. Novel techniques have been developed and will be employed at high pressures to measure electrical conductivity of terrestrial planetary core mimetic Fe-S-Si solids and liquids at high temperatures as well as NH3-H2O fluids at the low temperatures of subsurface oceans of outer planetary satellites. These studies will provide critical data to address the new controversies in models of thermal convection in fluid outer cores, inner core age, geodynamo, and magnetic induction in subsurface oceans of icy satellites. Using a technique recently developed in our lab, the enigmatic origin of deep focus earthquakes will be investigated by measuring acoustic emission in phase transforming mantle olivines (Mg1-xFex)2SiO4 (0.1<x<0.8) at high pressures and temperatures. These studies aim to provide an answer for the first time to the question of whether earthquakes at 350-660km depth are caused by release of seismic energy during high pressure-temperature mineral phase transformation in the olivine wedge of subducting slabs.*Answers to these questions will be woven into the fabric of the long term goals of Dr. Secco's research program. Those goals are to improve understanding of the macro-scale engines of planetary interior heat and mass flow processes by studying the micro-scale behaviour of planetary materials at interior pressure and temperature conditions. Thirteen HQP will receive extensive training in experimental high pressure-temperature mineral physics that will provide transferrable skills to 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
RGPIN-2018-05021
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
2018
Competition year année de concours
2018
Award amount
61000
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
1
Nb partie
5
Application title
Experimental Studies of Earth and Planetary Materials at Extreme Conditions of Pressure and Temperature
Keyword
NSERC
Application summary
Large scale processes of heat and mass movement deep in the interior of planets control much of what happens on the surface. The focus of Dr. Secco's research program is to bring the inaccessible deep interior of planets into the lab by measuring physical properties of core and mantle materials under simultaneous extreme pressure (0-23GPa) and temperature (220-2300K) conditions in four large volume presses one of which is the largest capacity research press in North America. Novel techniques have been developed and will be employed at high pressures to measure electrical conductivity of terrestrial planetary core mimetic Fe-S-Si solids and liquids at high temperatures as well as NH3-H2O fluids at the low temperatures of subsurface oceans of outer planetary satellites. These studies will provide critical data to address the new controversies in models of thermal convection in fluid outer cores, inner core age, geodynamo, and magnetic induction in subsurface oceans of icy satellites. Using a technique recently developed in our lab, the enigmatic origin of deep focus earthquakes will be investigated by measuring acoustic emission in phase transforming mantle olivines (Mg1-xFex)2SiO4 (0.1<x<0.8) at high pressures and temperatures. These studies aim to provide an answer for the first time to the question of whether earthquakes at 350-660km depth are caused by release of seismic energy during high pressure-temperature mineral phase transformation in the olivine wedge of subducting slabs.*Answers to these questions will be woven into the fabric of the long term goals of Dr. Secco's research program. Those goals are to improve understanding of the macro-scale engines of planetary interior heat and mass flow processes by studying the micro-scale behaviour of planetary materials at interior pressure and temperature conditions. Thirteen HQP will receive extensive training in experimental high pressure-temperature mineral physics that will provide transferrable skills to prepare them for employment in academic, government and private sectors.*