Geophysics, Lecture Notes- Physics - 3, Study notes of Physics

Geological Time, Radiometric Dating

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2010/2011

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PX266 Geophysics (2010/11)
Lecture 2 Handout Earth’s Internal Structure
Dr. Gavin Bell
Radii and average densities
av given in figure; equatorial (Req) and polar (Rpol) radii
given for Earth, approximate average radii for inner (Ri) and outer (Ro) core.
Crust: cool, low density outer layer of the Earth, mainly silicates (~50% is SiO2);
oceanic and continental crust very distinct in composition and thickness.
Mantle: hotter, higher density shell between crust and core; infer composition from
indirect evidence mostly magnesium and iron silicate minerals, whose crystal
structures change with pressure or temperature (and hence depth). Upper mantle has
layers of olivine (Mg,Fe)2SiO4,spinel then perovskite (Mg,Fe)SiO3.
Core: mostly iron outer core is liquid, inner core is solid with a transition region
some 500 km thick. Average density of whole core = 1.2104kg m-3.
Lithosphere: cooler upper layer around 60 km thick includes crust and some upper
mantle. Heat transferred mostly by conduction. Undergoes elastic deformation and
brittle fracture over geological time mechanically rigid compared to asthenosphere.
Asthenosphere: below lithosphere. Undergoes viscous flow over geological time, but
behaves as an elastic solid (transmitting shear and compressional elastic waves) over
timescales of seconds or minutes. Heat transferred mainly by convection.
(Mesosphere): more rigid, less ductile than asthenosphere, reaching down to the
outer core. Chemically similar to asthenosphere; properties differ due to pand T.
(Core): very distinct both chemically and mechanically; inner / outer core state
difference (solid / liquid) is due to “pressure-freezing” of iron.
Crust
av = 2.9103kg m-3
average thickness:
35 km (continental)
7 km (oceanic)
Outer Core
Inner Core
Ri
Ro
Req = 6378 km (equator)
Rpol = 6357 km (polar)
Ri= 1220 km (inner core)
Ro= 3480 km (outer core)
Mantle
av = 4.5103kg m-3
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PX266 Geophysics (2010/11)

Lecture 2 Handout – Earth’s Internal Structure

Dr. Gavin Bell Radii and average densities  av given in figure; equatorial ( R eq) and polar ( R pol) radii given for Earth, approximate average radii for inner ( R i) and outer ( R o) core. Crust: cool, low density outer layer of the Earth, mainly silicates (~50% is SiO 2 ); oceanic and continental crust very distinct in composition and thickness. Mantle : hotter, higher density shell between crust and core; infer composition from indirect evidence – mostly magnesium and iron silicate minerals, whose crystal structures change with pressure or temperature (and hence depth). Upper mantle has layers of olivine (Mg,Fe) 2 SiO 4 , spinel then perovskite (Mg,Fe)SiO 3. Core : mostly iron – outer core is liquid, inner core is solid with a transition region some 500 km thick. Average density of whole core = 1.2 10 4 kg m

  • . Lithosphere : cooler upper layer around 60 km thick – includes crust and some upper mantle. Heat transferred mostly by conduction. Undergoes elastic deformation and brittle fracture over geological time – mechanically rigid compared to asthenosphere. Asthenosphere : below lithosphere. Undergoes viscous flow over geological time, but behaves as an elastic solid (transmitting shear and compressional elastic waves) over timescales of seconds or minutes. Heat transferred mainly by convection. (Mesosphere): more rigid, less ductile than asthenosphere, reaching down to the outer core. Chemically similar to asthenosphere; properties differ due to p and T. (Core): very distinct both chemically and mechanically; inner / outer core state difference (solid / liquid) is due to “pressure-freezing” of iron. Crust av = 2.9 103 kg m- average thickness: 35 km (continental) 7 km (oceanic) Outer Core Inner Core R i R o R eq = 6378 km (equator) R pol = 6357 km (polar) R i = 1220 km (inner core) R o = 3480 km (outer core) Mantle av = 4.5 103 kg m-

Two more views of Earth’s internal structure: (from W. Sullivan, Continents in Motion – The New Earth Debate ): As depth increases:  Density increases (2 or 3 tonne m

  • for crustal rocks, perhaps 12 or 13 tonne m

for the iron & impurities of the inner core).  Elastic constants increase (detailed in Seismology topic).  Pressure increases (136 GPa at base of mantle).  Temperature generally increases (around 4000°C at core/mantle boundary).  Mantle viscosity generally increases (perhaps 10^19 – 10^24 Pa s) Further Study

  1. Problems 3 and 4 – review Earth’s structure and find out about the “Moho”. Question 3 involves our favourite movie, The Core. Question 4 will involve finding out a little bit about seismology in advance of our treating the topic properly later on.
  2. You will need to know the overall structure of the Earth and be able to distinguish the important mechanical properties and BASIC chemical / mineral composition of the various layers. You should also have a good idea of a few basic rock types. However, I would not expect you to memorise lots of complex mineralogy for the exam – this is geophysics, not geology! For example, understanding the principle that different pressures and temperatures can cause materials of similar chemical composition to adopt different crystal structures (with different densities and elastic moduli) is much more important than learning a long list of rock or mineral types. Past exams and model answers are a good guide to how much detail you should learn. The USGS site has a basic intro to Earth structure: http://pubs.usgs.gov/gip/interior/