Grant: Discovery Grants Program - Individual
University of New Brunswick
$50,000.00
Supersonic impact, shock and frictional processes in planetary materials
EF 2014-15
Résumé
This proposal seeks funding to investigate high strain-rate phenomena in planetary materials. Many geological processes take hundreds, thousands or millions of years to complete. In contrast, dynamic events associated with asteroid impact typically occur in less than a second (shock wave passage), with a total event lasting minutes (dominated by gravity-driven readjustments). Coseismic slip is typically several seconds duration for a large earthquake. Our collective knowledge of ""fast"" deformation is limited, especially in terms of the response of natural ceramics (i.e., most planetary materials). I will investigate two main areas of dynamic behaviour: (1) hypervelocity impact, and associated shock wave-materials interactions, and (2) seismogenic faulting via laboratory-based simulations and field studies. The impact research will embrace shock wave generation and the transformation of materials in the solid state (e.g., the creation of new high-pressure and high-temperature mineral states), as well as their conversion into melt and vapour. Associated graduate student training at the Master's and PhD levels will focus on terrestrial impact craters (e.g., Manicouagan), lunar, martian and asteroid materials, and shock and frictional processes. Emphasis will be placed on understanding shock and associated shock focussing mechanisms, the latter resulting in shock energies greater than the bulk shock. Seismogenic faulting research will relate the mechanics of the sliding interface to seismic hazard in terms of fault lubrication and earthquake magnitude. Along with a state-of-the-art laboratory-based friction apparatus used to simulate earthquakes, my recently established high-speed impact laboratory provides the research foundation for directly investigating shock wave-materials interactions. The proposed activities will further our understanding of materials behaviour under extreme conditions. This is relevant to (a) understanding impact and shock as fundamental planet-building and planet-modifying processes, and (b) developing protective materials for our society (e.g., impact shielding for space-based infrastructure). An enhanced knowledge of earthquake mechanics will help characterize hazardous fault systems, with the goal of developing new predictive tools.
Programme
Discovery Grants Program - Individual
Bénéficiaire
Emplacement
New Brunswick, Canada
Type de bénéficiaire
Academia
Type
Grant
Source
NSERC's Awards Data
Tel que publié
Application id
1455-2011
Name nom
Spray, John
Department département
Earth Sciences
Organization id
75
Institution établissement
University of New Brunswick
Province en
New Brunswick
Province fr
Nouveau-Brunswick
Country en
CANADA
Country fr
CANADA
Fiscal year exercice financier
2014
Competition year année de concours
2011
Award amount
50000
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
4014
Research subject group en
Earth science
Research subject group fr
Sciences de la terre
Research subject en
Planetary geology
Research subject fr
Géologie planétaire
Partie
4
Nb partie
5
Application title
Supersonic impact, shock and frictional processes in planetary materials
Keyword
NSERC
Application summary
This proposal seeks funding to investigate high strain-rate phenomena in planetary materials. Many geological processes take hundreds, thousands or millions of years to complete. In contrast, dynamic events associated with asteroid impact typically occur in less than a second (shock wave passage), with a total event lasting minutes (dominated by gravity-driven readjustments). Coseismic slip is typically several seconds duration for a large earthquake. Our collective knowledge of ""fast"" deformation is limited, especially in terms of the response of natural ceramics (i.e., most planetary materials). I will investigate two main areas of dynamic behaviour: (1) hypervelocity impact, and associated shock wave-materials interactions, and (2) seismogenic faulting via laboratory-based simulations and field studies. The impact research will embrace shock wave generation and the transformation of materials in the solid state (e.g., the creation of new high-pressure and high-temperature mineral states), as well as their conversion into melt and vapour. Associated graduate student training at the Master's and PhD levels will focus on terrestrial impact craters (e.g., Manicouagan), lunar, martian and asteroid materials, and shock and frictional processes. Emphasis will be placed on understanding shock and associated shock focussing mechanisms, the latter resulting in shock energies greater than the bulk shock. Seismogenic faulting research will relate the mechanics of the sliding interface to seismic hazard in terms of fault lubrication and earthquake magnitude. Along with a state-of-the-art laboratory-based friction apparatus used to simulate earthquakes, my recently established high-speed impact laboratory provides the research foundation for directly investigating shock wave-materials interactions. The proposed activities will further our understanding of materials behaviour under extreme conditions. This is relevant to (a) understanding impact and shock as fundamental planet-building and planet-modifying processes, and (b) developing protective materials for our society (e.g., impact shielding for space-based infrastructure). An enhanced knowledge of earthquake mechanics will help characterize hazardous fault systems, with the goal of developing new predictive tools.