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Chap 2-4: Earth Shape of the planet Size of the planet Orientation to the Sun Distribution of land & sea Reference frames Map Projections Shape of Ocean Basins Plate Tectonics (shaper of ocean basins) OC3230-Paduan images Copyright © McGraw Hill Chap 2-4: Earth Earth is an “oblate spheriod:” equatorial radius is 21 km greater than polar R ~ 6400 km Rotation axis runs north-south through the poles points “up” from north pole and has magnitude of 1/day OC3230-Paduan images Copyright © McGraw Hill Chap 2-4: Earth On the surface, we use latitude and longitude coordinate reference system There are 111 Latitude “Parallels” km per degree of latitude but the spacing between degrees of longitude varies with latitude OC3230-Paduan Longitude images Copyright © McGraw Hill Chap 2-4: Earth Longitude reference is arbitrary but convention defines a specific longitude through Greenwich Longitude Time is also referenced to Prime “Meridian” in Greenwich, England “Greenwich Mean Time” or GMT OC3230-Paduan images Copyright © McGraw Hill Chap 2-4: Earth Earth rotates on its axis 15˚ each hour-to determine longitude requires knowing the time of local noon relative to GMT (latitude could be determined by measuring the angle between the horizon and the north star) OC3230-Paduan images Copyright © McGraw Hill Chap 2-4: Earth Today the Global Positions System (GPS) satellite network makes location determination easy worldwide OC3230-Paduan images Copyright © McGraw Hill Chap 2-4: Earth Today the Global Positions System (GPS) satellite network makes location determination easy worldwide OC3230-Paduan But make sure you have the correct datum! images Copyright © McGraw Hill Chap 2-4: Earth equatorial cylindrical (includes Mercator) Map Projections Related topics: contour lines or isopleths topography & bathymetry physiographic (3-D) views simple polar conic Upcoming topics: plan/map views (vertical) sections profiles OC3230-Paduan polar tangent plane images Copyright © McGraw Hill Chap 2-4: Earth Bathymetric Chart: Contour lines connect areas of constant depth Contours could also be called “isobaths” OC3230-Paduan images Copyright © McGraw Hill Chap 2-4: Earth 3-D, Shaded-Relief Map OC3230-Paduan images Copyright © McGraw Hill Chap 2-4: Earth Water Planet: 71% of Earth’s surface Northern Hemisphere: 60% “Continental” OC3230-Paduan Southern Hemisphere: 80% “Maritime” images Copyright © McGraw Hill Chap 2-4: Earth Surface area per 5˚ of latitude Note: 1) no area at poles 2) ocean area is dominant, particularly in s. hemisphere OC3230-Paduan images Copyright © McGraw Hill Chap 2-4: Earth OC3230-Paduan The Hydrological Cycle: where is the water? images Copyright © McGraw Hill Chap 2-4: Earth The Hydrological Cycle: where is the water? Related topics: Budgets (water budget here; heat budget later) Residence Time = Volume Reservoir/Rate of Filling m 3 units: 3 1 sec m sec OC3230-Paduan images Copyright © McGraw Hill Chap 2-4: Earth Pacific Atlantic Indian Arctic Major Ocean Basins -we also refer to the “Southern Ocean,” which circles the globe around Antarctica OC3230-Paduan images Copyright © McGraw Hill Chap 2-4: Earth Major Ocean Basins mean depth = 3729m (~4000m) OC3230-Paduan images Copyright © McGraw Hill Chap 2-4: Earth Major Ocean Basins mean depth = 3729m (~4000m) much of Earth’s surface is covered by ocean with depth of about 4000m-6000m OC3230-Paduan Hypsographic Curve images Copyright © McGraw Hill Chap 2-4: Earth Looking ahead: we want to memorize the components of the continental margin; First: we’ll look at the geological factors that have created them OC3230-Paduan images Copyright © McGraw Hill Chap 2-4: Earth The Earth a.k.a. “pac man” OC3230-Paduan images Copyright © McGraw Hill Chap 2-4: Earth There is a difference in composition and density between continental and oceanic crust Thicker, lighter continental crust “floats” like an iceberg on the mantle Isostacy=vertical equilibrium OC3230-Paduan images Copyright © McGraw Hill Chap 2-4: Earth Isostacy: Columns of crustal material are unequal in height and density but generate the same pressure at the same depth within the mantle OC3230-Paduan images Copyright © McGraw Hill Chap 2-4: Earth Part 1: Continental Drift Alfred Wegner proposed in 1912 that the shape of the continents appear to fit together (others before him had also noted this) OC3230-Paduan images Copyright © McGraw Hill Chap 2-4: Earth Part 2: Sea Floor Spreading; Proposed by Harry Hess (1962) OC3230-Paduan images Copyright © McGraw Hill Chap 2-4: Earth SPECIAL DATES: MPA meeting…6 Jul R/V Pt Sur Cruise…14 Jul R/V Pt Sur Cruise…25 Jul Exam-1 (definite)...2 Aug Exam-2 (Tentative)…1 Sep Labor Day Holiday...5 Sep Final Exam...19 Sep (Sp-226, 1300-1450) OC3230-Paduan OC3230 Calendar, Summer 2005 version 13 July 2005 EX 1 images Copyright © McGraw Hill Chap 2-4: Earth Evidence for sea floor spreading Distribution of Seismic Activity Magnetic Reversal Patterns Age Patterns of Oceanic Crust (related to magnetic reversals) Sediment Thickness Distribution Heat Flow Distribution Direct (GPS) Measurements of Crustal Movement OC3230-Paduan images Copyright © McGraw Hill Chap 2-4: Earth Evidence for sea floor spreading Earthquake epicenters for 1961-1967 Observed to occur on “plate boundaries” depth <100 km Note: difference between plate boundary and coastline depth >100 km OC3230-Paduan images Copyright © McGraw Hill Chap 2-4: Earth OC3230-Paduan Evidence for sea floor spreading images Copyright © McGraw Hill Chap 2-4: Earth Evidence for sea floor spreading The magnetic time scale: Pattern of reversals is tied to dates when molten rock cooled OC3230-Paduan images Copyright © McGraw Hill Chap 2-4: Earth Evidence for sea floor spreading Age of oceanic crust OC3230-Paduan images Copyright © McGraw Hill Chap 2-4: Earth Evidence for sea floor spreading Sediment thickness increases away from the mid-ocean ridge OC3230-Paduan images Copyright © McGraw Hill Chap 2-4: Earth Evidence for sea floor spreading Heat decreases away from the mid-ocean ridge OC3230-Paduan images Copyright © McGraw Hill Chap 2-4: Earth Global topography from gravity anomalies OC3230-Paduan images Copyright © McGraw Hill Chap 2-4: Earth OC3230-Paduan images Copyright © McGraw Hill Chap 2-4: Earth Million km2 OC3230-Paduan images Copyright © McGraw Hill Chap 2-4: Earth OC3230-Paduan images Copyright © McGraw Hill Chap 2-4: Earth OC3230-Paduan images Copyright © McGraw Hill Chap 2-4: Earth Most plate boundaries are at sea or at a land-sea boundary OC3230-Paduan images Copyright © McGraw Hill Chap 2-4: Earth Most plate boundaries are at sea or at a land-sea boundary But not all! OC3230-Paduan images Copyright © McGraw Hill Chap 2-4: Earth OC3230-Paduan images Copyright © McGraw Hill Chap 2-4: Earth Convergent Plate Boundaries Horizontal distance to volcanic activity (melting of crust) depends on angle of subducting plate If the boundary is between continental and oceanic crust, can have parallel mountain chains formed inland (e.g., Cascade Mountains, Andes Mountains) or as an Island Arc offshore (e.g., Japan) OC3230-Paduan images Copyright © McGraw Hill Chap 2-4: Earth Active margins are found at plate boundaries Passive margins, such as the north American east coast, are landsea margins that occur within a tectonic plate OC3230-Paduan images Copyright © McGraw Hill Chap 2-4: Earth Transform Margins have fault zones as a results of sideways motions OC3230-Paduan images Copyright © McGraw Hill Chap 2-4: Earth Its our fault! OC3230-Paduan images Copyright © McGraw Hill Chap 2-4: Earth Locations of major hot spots OC3230-Paduan images Copyright © McGraw Hill Chap 2-4: Earth Locations of major hot spots OC3230-Paduan images Copyright © McGraw Hill Chap 2-4: Earth Island/Seamount chains produced by hot spots is one of the most important indicators of historical plate motions OC3230-Paduan images Copyright © McGraw Hill Chap 2-4: Earth Spreading rates: 1-20 cm/yr Max rates along East Pacific Rise Average rate about 5 cm/yr (similar to fingernail growth) OC3230-Paduan images Copyright © McGraw Hill Chap 2-4: Earth MARS NEPTUNE Ocean sciences are investing $$ in cabled observatories OC3230-Paduan images Copyright © McGraw Hill Chap 2-4: Earth Global topography from gravity anomalies (measured by altimeter) OC3230-Paduan images Copyright © McGraw Hill Chap 2-4: Earth Acoustic methods replaced old weighted lead line techniques with the 1925 Meteor Expedition; Today, we have satellite and airborne laser (LIDAR) Side-Scan Sonar (provides depth and Single depth trace from echo reflectivity data) sounder, such as 12kHz unit Previous: Multi-Beam on R/V Pt Sur-first used on Sonar Meteor Expedition OC3230-Paduan images Copyright © McGraw Hill Chap 2-4: Earth CA shelf and slope has been mapped with variable resolution OC3230-Paduan images Copyright © McGraw Hill Chap 2-4: Earth Elkhorn Slough (LIDAR Survey) Tidal creek, salt marsh, and mudflat habitats OC3230-Paduan NOAA/USGS Coast ©Survey Data images Copyright McGraw Hill Chap 2-4: Earth OC3230-Paduan NOAA/USGS Coast ©Survey Data images Copyright McGraw Hill Chap 2-4: Earth Side-scan sonar data Multi-beam sonar data OC3230-Paduan CSUMB images Seafloor Copyright Mapping © McGrawLab Hill Chap 2-4: Earth Topography profiles at various latitudes: reflect major mountain ranges and mid-oceans ridges What about “typical” ocean margin? OC3230-Paduan images Copyright © McGraw Hill Chap 2-4: Earth Shelf Break (~130m) is critical point at the junction between continental and oceanic crust OC3230-Paduan images Copyright © McGraw Hill Chap 2-4: Earth OC3230-Paduan Continental Shelves of the World (sort of) images Copyright © McGraw Hill Chap 2-4: Earth Shelf width varies in our region from about 50 km in the Gulf of the Farallones (San Francisco area) to, essentially, 0 km off Big Sur OC3230-Paduan images Copyright © McGraw Hill Chap 2-4: Earth Scale of topography in Monterey Submarine Canyon is comparable to the Grand Canyon OC3230-Paduan images Copyright © McGraw Hill Chap 2-4: Earth Deep-Ocean Features (seamount) Deepest areas are the trenches that are associated with convergent margins (11,020 m max in Mariana Trench) OC3230-Paduan images Copyright © McGraw Hill Chap 2-4: Earth Abyssal plain areas (4000 - 6000 m) (everywhere that mid ocean ridges are not) OC3230-Paduan images Copyright © McGraw Hill Chap 2-4: Earth Sediment Cover Coastal Origin Also: Lithogenous vs Biogenous sediments OC3230-Paduan Ocean Origin images Copyright © McGraw Hill Chap 2-4: Earth (low productivity region) (high productivity region) OC3230-Paduan images Copyright © McGraw Hill Chap 2-4: Earth foraminifera (calcareous) radiolarians (siliceous) (high productivity region) OC3230-Paduan images Copyright © McGraw Hill Chap 2-4: Earth Box Corer Grab Samplers OC3230-Paduan images Copyright © McGraw Hill Chap 2-4: Earth Gravity Corer OC3230-Paduan Piston Corer images Copyright © McGraw Hill Chap 2-4: Earth Paleoceanography studies the history of the oceans and climate looking at the sediment record OC3230-Paduan images Copyright © McGraw Hill Chap 2-4: Earth At finer scales, ocean bottom type is important to marine habitat characterization and to shallow water acoustics Seafloor Habitats Rocky Reefs Intertidal Zones Sandy or soft bottoms Underwater Pinnacles Submarine Canyons OC3230-Paduan images Copyright © McGraw Hill