earth structure

    Cards (79)

    • planet
      sizeable object orbiting a star massive enough to have its own gravity
      elliptical and co-planar orbits in the same direction as the suns rotation
    • comets
      made of ice and dust
      outer layer melts to water vapor close to the sun
    • the sun
      a yellow dwarf star composed of hydrogen and helium 99.8% of total mass of solar system
    • meteorites
      rocky fragments falling to earth from space
    • asteroids
      rocky objects that failed to form a planet
    • moons
      natural satellites that orbit planets
    • mercury
      heavily cratered, signs of volcanism, iron rich core, thin atmosphere, no moons,
    • Venus
      no oceans, craters, shield volcanos and lava flows, huge greenhouse effect, dense atmosphere, sulfuric acid clouds
    • mars
      large shield volcanos, water in ice caps, sedimentary rocks and structures
    • Jupiter
      small rocky metallic core, powerful magnetic field, H+He cloud, great red spot- huge storm, 63+ moons and volcanically active
    • Saturn
      rings made of ice, rocky core, powerful storms, second largest moon in the solar system
    • Uranus
      icy rings, orbits on the side, windy, 27 major moons, methane atmosphere
    • neptune
      great dark spot, magnetic field, rocky core possible, 14 known moons.
    • solar system
      8 planets
      four inner terrestrial planets
      four outer Jovian gas giants
      172 moons and natural satellites
      asteroid belt
      Kuiper belt
    • asteroid belt
      the region of the solar system between the orbits of Mars and Jupiter, where many asteroids are found
    • Kuiper Belt
      A region of the solar system that is just beyond the orbit of Neptune and that contains small bodies made mostly of ice
    • terrestrial
      internal structure similar
      differentiated
      topographic features on surface
      silicate rocks composition
      secondary atmosphere
    • the moon
      lunar maria- dark and made of basalt- flat w few craters
      lunar highland- pale, anorthosite, steep topography, heavy craters
      collision- giant impact hypothesis
    • Jovian Planets
      large and low density
      composed of gas (hydrogen, helium ,methane and ammonia)
      all have a planetary ring system
      mobile surface features
      all rotate rapidly causing strong east-west wind direction- leads to formations of bands or stripes
    • Io- Jupiter moon
      massive volcanic plumes
      most volcanically active place in solar system
      gravity from other bodies causes it to change shape- friction
      heat and melting of rock caused
    • birth of the solar system
      -Material that did not become a star in the nebula forms protoplanetary disk
      -Contains all 92 elements as solitary atoms or clumps
      -Planetesimals form (>1km)
      -Protoplanets form
      -Inner planets (terrestrial) form from dust
      -Outer planets (gas) form from ice and other gases
    • Earth structure- compositional layers

      continental crust
      oceanic crust
      moho
      mantle
      Gutenberg discontinuity
      core
    • Earth structure- mechanical layers
      lithosphere
      asthenosphere
      inner mantle
      outer core
      Lehmann discontinuity
    • crust
      oceanic and continental
    • continental crust
      made from granite
      rich in silicone and aluminum
      all rock types
      av density 2.7 g/cm3
      all ages up to 4Go
      average thickness 35km
    • oceanic crust
      basalt, dolerite, gabbro
      mafic igneous rock
      rich in iron and magnesium
      av density 2.9 g/cm3
      up to 200ma
      average thickness 7km
    • Moho
      the boundary between the earth's mantle and crust
    • upper mantle
      solid silicate rocks
      main peridotite made of augite and olivine
      xenoliths may occur
      topmost upper mantle is cooler, rigid and responds in brittle manner
      together with crust is lithosphere
      rest of the upper mantle deforms in a ductile manner but is still solid
    • the lower mantle
      solid- less ductile due to great pressure
      composition similar to stony meteorites
      convection currents from core-mantle boundary
    • outer core
      boundary between the lower mantle and outer core is called the Gutenberg discontinuity
      liquid state
      Fe-Ni alloy similar in composition to iron meteorites
      extends from 2900-5150km
      convection currents also occur
      source of the earths magnetism
    • inner core
      solid state
      Fe-Ni similar to iron meteorites
      extends from 5150-6371km - Centre of the earth
    • mechanical layers
      crust and mantle are based on the compositions of the rocks
      lithosphere and asthenosphere are based on the properties of the rocks that mean they react in different ways due to temp and pressure
    • the lithosphere
      composed of part of the crust and topmost mantle
      includes the moho which marks the base of the crust
      the base of lithosphere is marked by a change in physical properties rather than a change in composition
      base of lithosphere lies at the 1300 isotherm
    • asthenosthere
      next layer underneath, forms next part of the upper mantle down to approx. 200km
      ultramafic
      sometimes referred to low velocity zone as seismic waves slow down
      temp is high enough to be close to melting temp of peridotite
      rheid
      ductile/plastic
      5% melt
      seismic waves reduce in velocity because rocks are less rigid and incompressible
    • mines and boreholes
      rock at the surface can be collected and sampled
      taken to labs to analyze their chemical comp and physical properties
      mines and boreholes allow geologist to directly examine and sample rocks
      only reach so far
      project Mohole reach to mantle, reached 183m
      KTB borehole in Russia- deepest
    • mines and geothermal gradient
      (-) temp and pressure increase w depth- geothermal gradient
      lord kelvin- estimate age of earth
    • magmas, xenoliths and kimberlites
      normal basalt magmas at MOR made from partial melting of upper mantle
      by analyzing the composition of these magmas and their volatiles we can estimate composition
      kimberlites are volcanic rocks that occur in the earths crust in vertical structures - kimberlite pipes
      sourced deep within lithospheric mantle at depths of 250km
      erupt rapidly and violently
      carrier of diamonds and other mantle xenoliths
      by examining minerals found in these kimberlites we can analyze the composition at these depths
    • ophiolites
      oceanic crust subducted and destroyed during plate collision but sometimes they are thrust up or obducted onto the continents
      sections of oceanic lithosphere can be obducted i=onto land called ophiolites
      show us what oceanic lithosphere looks like
      magma that erupts into water cools forming a basalt pillow lava
      the magma in the feeder pipe cools slower forming a dolerite and the magma left in the magma chamber cools slowly forming a gabbro
    • elastic rebound for a cause of earthquakes
      1. a body becomes under stress due to opposing tectonic forces
      2. rocks distort and deform, energy stored as elastic strain energy
      3. the strength of rocks is exceeded by increasing stress and rock fractures
      4.two parts of the rock suddenly move relative to each other and there is displacement along the fault
      5. energy is released in form of seismic waves that radiate out from the source
    • seismometer
      device that receives seismic vibrations, converts them into recordable signal