Lecture 6: Solar System / Earth Flashcards

1
Q

Earth

A
  • Strong magnetic field
  • Differentiated interior
  • Active Surface
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2
Q

Planetary Interiors

A
  • Seismic Waves, Magnetic Fields, Surface Features, and Gravitational Deviations are the best way to determine the inside of a planet
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3
Q

Earthquake Waves

A
  • P waves are primary or pressure waves and are the fastest seismic waves
  • S waves are secondary or shear waves
  • Surface waves are slower than S and P waves
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4
Q

Earth Seismic Waves

A
  • Waves refract depending on different things
  • Temperature and density increase with depth
  • heat generate dis proportional to planet’s mass
  • Heat escapes through planet’s surface
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5
Q

Heating vs. Cooling of Planets

A
  • Heating mechanisms are proportional to mass, volume or radius cubed
  • Cooling mechanisms are proportional to surface area or radius squared
  • Larger bodies cool more slowly
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6
Q

Planetary magnetic fields

A
  • A rotating metallic core will act as a dynamo and produce a magnetic field
  • Earth’s magnetic field comes form charged particles in its outer liquid core
  • Solar wind distorts shape of magnetosphere
  • Aurora’s are caused by solar winds with magnetic field (northern lights)
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7
Q

Planetary Surfaces: Earth

A
  • The surface of a planet can give clues to what’s happening inside the planet
  • Continental drift causes constant changes to surface (mountains)
  • Erosion of surface, meteorite impacts
  • North America result of subduction, collisions, volcanism, erosion, and sedimentary deposits
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8
Q

Techtonic Plates

A
  • Can compress or stretch the crust
  • Can slide along each other and pull apart, causing earthquakes and rift valleys
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9
Q

Volcanism

A
  • An upwelling of molten rock (magma) from deep within the planet to the surface
  • Can cover up old surface features and make new ones, as well as produce additional gas
  • Caused by Techtonic plates and thermal plumes
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10
Q

Impact Cratering

A
  • Features depend on speed, angle, impactor, and surface material, and are different from volcanic craters
  • Small craters bowl shaped
  • Large craters have central peak and concentric rings, multiring basins
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11
Q

Erosion

A
  • Atmosphere and Surface Water act to level the surface
  • Acts on all scale
  • Chemical Reactions
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12
Q

Planetary Atmospheres: Earth

A
  • CO2 has increased in the last 50 years likely due to global warming
  • Surface Temperature is a combination of solar heating, infrared radiation trapped by cloud layer, and hot interior
  • Climate depends on heating and rotation
  • Atmosphere blocks some light, transmits others
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13
Q

Atmospheric Mass Change

A
  • Greenhouse effect heats surface
  • Atmospheres gain mass due to outgassing, evaporation, and impacts
  • Atmospheres lose mass by thermal escape, solar winds, impacts, condensation, and chemical reactions
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14
Q

Atmospheric Heating

A
  • Warm air rises near the equator and cools as it gets to the poles
  • Circulation cell in each hemisphere
  • Rotation affects atmospheric circulation
  • Coriolis Effect causes circulation cells to divide into three cells per hemisphere
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