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Physical Science Lecture: Earth’s Seismic Interior Professor Kenny L. Tapp Rock Type: Rock Name: The$Earth’s$Interior • How$do$we$know$what$the$Earth$comprises? • How$deep$have$we$drilled? The$Earth’s$Interior • Most$of$what$we$know$is$from$geophysics. • Geophysics$is$basically$“remote$sensing”$of$ Earth’s$interior – Seismic$waves – MagneCc$field – Gravity – Heat Earth's(layered(structure( Possible(seismic(paths( through(the(Earth Most$of$our$knowledge$of$Earth’s$interior$ comes$from$the$study$of$P$and$S$earthquake$ waves$ • Travel$Cmes$of$P$and$S$waves$through$Earth$vary$ depending$on$the$properCes$of$the$materials$ • S$waves$travel$only$through$solids$ Figure 7.24 Earth's(layered(structure( (((Seismic(shadow(zones Discovering$Earth’s$major$layers$ • Shadow$zone$$ • Absence$of$P$waves$from$about$105$degrees$to$140$ degrees$around$the$globe$from$an$earthquake • Explained$if$Earth$contained$a$core$composed$of$ materials$unlike$the$overlying$mantle$$$$ Figure 7.26 Earth's(layered(structure( Layers$defined$by$composiCon$ • Crust$ • Thin,$rocky$outer$layer$ • Varies$in$thickness$ • Roughly$7$km$(5$miles)$in$oceanic$regions$ • ConCnental$crust$averages$35[40$km$(25$miles)$ • Exceeds$70$km$(40$miles)$in$some$mountainous$ regions$$ Earth's(layered(structure( Layers$defined$by$composiCon$ • Crust$ • ConCnental$crust$$ • Upper$crust$composed$of$graniCc$rocks$ • Lower$crust$is$more$akin$to$basalt • Average$density$is$about$2.7$g/cm3$$ • Up$to$4$billion$years$old$$ Earth's(layered(structure( Layers$defined$by$composiCon$ • Crust$ • Oceanic$Crust$$ • BasalCc$composiCon$$ • Density$about$3.0$g/cm3$ • Younger$(180$million$years$or$less)$than$the$ conCnental$crust$$$$ Earth's(layered(structure( Earth's(layered(structure( Layers$defined$by$composiCon$ • Mantle • Below$crust$to$a$depth$of$2900$kilometers$(1800$miles) • ComposiCon$of$the$uppermost$mantle$is$the$igneous$ rock$peridoCte$(changes$at$greater$depths)$ Views(of(Earth’s( layered(structure Layers$defined$by$composiCon$ • Outer$Core • • • • Below$mantle$ A$sphere$having$a$radius$of$3486$km$(2161$miles)$ Composed$of$an$iron[nickel$alloy$ Average$density$of$nearly$11$g/cm3$ Figure 7.25 Earth's(layered(structure( Layers$defined$by$physical$properCes$ • Lithosphere • Crust$and$uppermost$mantle$(about$100$km$thick)$ • Cool,$rigid,$solid$ • Asthenosphere • • • • Beneath$the$lithosphere$ Upper$mantle To$a$depth$of$about$660$kilometers Soe,$weak$layer$that$is$easily$deformed$ Earth's(layered(structure( Layers$defined$by$physical$properCes$ • Mesosphere$(or$lower$mantle)$ • 660[2900$km$ • More$rigid$layer$ • Rocks$are$very$hot$and$capable$of$gradual$flow • Outer$core$ • Liquid$layer$ • 2270$km$(1410$miles)$thick • ConvecCve$flow$of$metallic$iron$within$generates$Earth’s$ magneCc$field$ • Inner$Core$ • Sphere$with$a$radius$of$1216$km$(754$miles)$ • Behaves$like$a$solid$ Views(of(Earth’s( layered(structure Continental drift: an idea before its time Alfred Wegener • First proposed hypothesis, 1915 • Published The Origin of Continents and Oceans Continental drift hypothesis • Supercontinent called Pangaea began breaking apart about 200 million years ago • Continents "drifted" to present positions • Continents "broke" through the ocean crust Figure 7.25 Pangaea approximately 200 million years ago Continental drift: an idea before its time Wegener's continental drift hypothesis • Evidence used by Wegener • • • • Fit of South America and Africa Fossils match across the seas Rock types and structures match Ancient climates • Main objection to Wegener's proposal was its inability to provide a mechanism Figure 8.2 Wegener’s matching of mountain ranges on different continents Figure 8.6 Paleoclimatic evidence for Continental Drift Figure 8.7 Plate tectonics: the new paradigm More encompassing than continental drift Associated with Earth's rigid outer shell • Called the lithosphere • Consists of several plates • Plates are moving slowly • Largest plate is the Pacific plate • Plates are mostly beneath the ocean Divergent boundaries are located mainly along oceanic ridges Plate tectonics: the new paradigm Plate boundaries • Types of plate boundaries • Divergent plate boundaries (constructive margins) • Two plates move apart • Mantle material upwells to create new seafloor • Ocean ridges and seafloor spreading • Oceanic ridges develop along well-developed boundaries • Along ridges, seafloor spreading creates new seafloor Plate tectonics: the new paradigm Plate boundaries • Types of plate boundaries • Convergent plate boundaries (destructive margins) • Plates collide, an ocean trench forms and lithosphere is subducted into the mantle • Oceanic-continental convergence • Denser oceanic slab sinks into the asthenosphere • Pockets of magma develop and rise • Continental volcanic arcs form • Examples include the Andes, Cascades, and the Sierra Nevadan system Figure 8.10 An oceanic-continental convergent plate boundary Plate tectonics: the new paradigm Plate boundaries • Types of plate boundaries • Convergent plate boundaries (destructive margins) • Continental-continental convergence • When subducting plates contain continental material, two continents collide • Can produce new mountain ranges such as the Himalayas Figure 8.14 A A continental-continental convergent plate boundary Figure 8.14 C The collision of India and Asia produced the Himalayas (after) The collision of India and Asia produced the Himalayas (before) Figure 8.15 A Testing the plate tectonics model Hot spots and mantle plumes • Caused by rising plumes of mantle material • Volcanoes can form over them (Hawaiian Island chain) • Mantle plumes • Long-lived structures • Some originate at great depth, perhaps at the mantle-core boundary Figure 8.15 C The Hawaiian Islands have formed over a stationary hot spot Measuring plate motion Measuring plate motion • By using hot spot “tracks” like those of the Hawaiian Island - Emperor Seamount chain • Using space-age technology to directly measure the relative motion of plates • Very Long Baseline Interferometry (VLBI) • Global Positioning System (GPS) Figure 8.19 Directions and rates of plate motions Plate tectonics into the future Present-day motions have been extrapolated into the future some 50 million years • Areas west of the San Andreas Fault slide northward past the North American plate • Africa collides with Eurasia, closing the Mediterranean and initiating mountain building • Australia and new Guinea are on a collision course with Asia Figure 8.26 A possible view of the world 50 million years from now Figure 8.29