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Physics of the Earth and planetary interiors. EPS 122 – Spring 2014 M –W 11.00-12.30 McCone 325. Instructor: Barbara Romanowicz Office hours: Mon-Wed 2-3 pm or appointment Office: 291 McCone Hall. Earth has an atmosphere and water. Earth has plate tectonics.
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Physics of the Earth and planetary interiors EPS 122 – Spring 2014 M –W 11.00-12.30 McCone 325 Instructor: Barbara Romanowicz Office hours: Mon-Wed 2-3 pm or appointment Office: 291 McCone Hall
Earth has an atmosphere and water Earth has plate tectonics
….which protects us from cosmic radiations Earth has an internally generated magnetic field sil Silicate mantle (solid) Liquid outer core Solid inner core
Haiti, 12 Janvier 2010 M 7.0 Japan 12 Marchs 2011 M 9 Chili, 27 Février 2010, M 8.8
Japan, 2011 Haiti, 2010 Sumatra, 2004 Chile, 2010 New. Zealand 2010,2011
Elastic rebound theory After the earthquake Time scale: seconds -> minutes Before the earthquake Time scale ~100 years Initially North American Plate San Andreas Fault Pacific Plate San Francisco 1906
Time scale Seconds-> minutes San Andreas Fault - Carrizo Plain Time scale: Millions, tens of millions of years San Francisco 1906
Hotspots and plumes Morgan, 1971
Depth (km) Courtesy of CinziaFarnetani Temperature (oC)
Kola 1970-1989 -12,262 m Photographed in 2007
Understanding the Earth’s Interior structure, dynamics and evolution Anchored in observations at the Earth’s surface and remote sensing using satellites Geomagnetism Geochemistry/cosmochemistry
Silicates Alliage de Fer
Colder hotter Slices through the Earth’s mantle at different depths
05 11 Honshu 06 12 410 410 660 660 ±1.5 % 1000 07 ±1.5 % 13 13 northern Bonin 08 14 09 15 15
Colder hotter Colder hotter Slices through the Earth’s mantle at different depths
One layer convection “Abyssal Layer” Convection à “2 couches” after Albarède et Van der Hilst, 1999
Surface and remote sensing observations • Geodesy: • Gravity field-> density and viscosity • Surface deformation -> tectonics • Seismology: • Elastic and anelastic internal structure • Heat flow: • Thermal structure • Geochemistry/cosmochemistry: • Thermal evolution/differentiation/composition • Magnetic field: • Processes in the earth’s core
Laboratory experiments and theoretical computations • Mineral physics • behavior of rocks as a function of temperature (T) and pressure (P) (crystal structure and deformation properties) • Composition of earth’s interior • Geodynamics • Integrate knowledge from other disciplines (min. phys, seismology, geochemistry) • Experimental and theoretical simulations of convection
Current trends in geosciences • Integration effort between the different disciplines which contribute to the knowledge of the internal structure and dynamics: • Cooperative Institute for Dynamic Earth Research (CIDER): “Blind men and the elephant”