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Unfinished Earth

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Until Shoemaker-Levy 9! Berringer Crater, Arizona. Young impact structure ... Planetary Accretion Today: Shoemaker-Levy 9. Significance of Shoemaker-Levy 9 ... – PowerPoint PPT presentation

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Title: Unfinished Earth


1
Unfinished Earth
  • History and modern continuation of planetary
    accretion and
  • The Origin of Crust

2
(No Transcript)
3
Earths Early History
  • Hadean Eon Earths first 500 Ma
  • Intense bombardment by bolides (meteors, comets,
    etc.)
  • No permanent crust destroyed by impacts
  • Little direct evidence on Earth
  • Excellent evidence on Moon, Mars and other
    terrestrial planets

4
Craters on the Moon Hadean and later bombardment
5
Earth the water planet
6
Earth the water planet
  • Presently, Oceans cover 71 of Earths surface
  • Odds of impact on land are 29
  • Water and oxygen weather rocks and destroy
    evidence of impacts

7
Crater Preservation
  • Arid climate is more likely to preserve craters
    than humid climate
  • Less weathering
  • Less erosion

Australian Outback
Quebec, Canada
8
Location of Craters on Earth
9
Craters in North America
10
Gene and Carolyn Shoemaker
  • Gene Shoemaker, geologist
  • Pioneer in study of impact structures worldwide
  • Studied Berringer Crater, AZ
  • Well-respected in geology, but not in astronomy
  • Until Shoemaker-Levy 9!

11
Berringer Crater, Arizona
  • Young impact structure
  • Approximately 40,000 years old
  • Arid climate excellent preservation
  • Remnants of meteorite found in crater and in
    ejecta

12
Planetary Accretion Today Shoemaker-Levy 9
13
Significance of Shoemaker-Levy 9
  • Convinced astronomers that such events were still
    possible
  • Focused attention on near-Earth objects
  • Showed how little we know of such objects
  • Showed how completely unprepared we are

14
A Focus on Earth
15
Why the Gap 4.6 3.98 Ga?
  • Asteroids, meteorites, comets, planetesimals
    collide as Earth accretes to form homogeneous
    protoplanet
  • Intense bombardment during continued accretion
    destroyed primeval crust (if there was any)
  • Inertial heating from impacts and radioactive
    decay may have liquified the entire planet
  • This afforded mobility for the start of density
    differentiation

16
Earths Layered Structure
  • Gravity caused Earths interior to differentiate
    into layers
  • Layers are arranged according to density
  • Most dense material sank to the center core
  • Density decreases outward
  • Density layering includes the hydrosphere
    (oceans) and atmosphere

17
Evidence for Earths Internal Structure
  • Refraction of seismic waves
  • Density of the entire planet
  • Gravity (mass) of entire planet
  • Composition of meteorites
  • Existence of magnetic field

18
Earth The Unfinished Planet
  • Earth continues to lose heat
  • Volcanism brings material to Earths surface
  • Other processes (subduction) return more dense
    material to interior
  • Conclusion
    Earth is still under construction!

19
Theory of Plate Tectonics
  • Plates move as a result of heat inside the Earth
  • Plates interact to cause
  • Earthquakes
  • Volcanos
  • Mountain systems
  • Earths lithosphere (crust uppermost mantle) is
    divided into plates

20
What makes the plates move?
  • Uneven distribution of heat in the upper mantle
    (Asthenosphere) causes heat to rise in some
    places (e.g., Mid-ocean ridges)
  • Differences in density cause colder, more dense
    Lithosphere to sink back into the asthenosphere
    (subduction)
  • This Convection drives the motion of the plates

21
Plate Tectonics andthe Origin of Crust
  • Direct link with formation of oceanic crust (sea
    floor spreading)
  • Less obvious connections with continental crust
    (continental accretion)

22
Plate Tectonics andthe Origin of Crust
  • Archean convection may have caused earliest crust
    to float to surface as scum
  • Subduction returned more dense material to
    interior
  • Less dense components were scraped off or
    returned to surface via volcanism
  • Plate interactions added continental crust to
    margins of continents
  • Quantity of continental crust has increased
    through time
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