Gravity and Space Flashcards

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1
Q

gravity

A
  • An attractive force between 2 objects

- Acceleration due to gravity: 9.81 m/s^2

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2
Q

strength of gravity depends on

A
  • gravitational constant
  • size of masses involved (density and volume)
  • distance between masses (r)
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3
Q

Changes in gravity: imagine a satellite circling a planet that is a uniform sphere

A

some gravitational force at the same distance from center of mass

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4
Q

Changes in gravity: imagine a satellite circling a planet that is uniform material, but not perfect sphere

A

force of gravity is lower over large depressions and higher over high elevations

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5
Q

Changes in gravity: imagine a satellite circling a planet that is a spherical planet, but not uniform material

A
  • higher density materials = stronger force of gravity

- Ex. Mafic igneous rocks have higher density -> higher force of gravity

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6
Q

Changes in gravity: imagine a satellite circling a planet that is a non-uniform body

A

have to divide it into pieces, calculate gravity from each piece, then add them up

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7
Q

force of gravity at centre of earth

A

zero!

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8
Q

why are gravity and topography somewhat related?

A

Elevation that could cause higher gravity is offset by isostasy

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9
Q

isostasy

A
  • Balancing act that prevents huge gravity anomalies on Earth
  • Large masses won’t have huge positive gravity anomaly as the dense mantle below will be displaced on either side
    • Ex. Causes blocks of same mass but different densities to sink into mantle at same depth
    • Ex. Causes blocks of same density but different masses to sink at different depths
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10
Q

isostatic equilibrium

A
  • Mountains come into isostatic equilibrium through erosion -> roots of mountain rise as overlying rock is eroded
  • Not all areas are in isostatic equilibrium yet (ie. Himalayas)
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11
Q

isostatic equilibrium: oceanic vs. continental plate

A

Low density of continental lithosphere compensates for elevation -> same gravitational force on both blocks

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12
Q

isostatic equilibrium: within a continental plate

A

“root” compensates for elevated continental crust (ie. Mountains)

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13
Q

isostatic rebound

A

negative anomaly due to removal of ice sheet that once covered the area -> crust is still bouncing back (ie. Hudson’s Bay area)

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14
Q

isostatic compensation (oceanic vs. continental)

A

Continental crust tends to be more elevated and thicker than oceanic crust in order to account for its smaller density

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15
Q

measuring gravity

A
  • Pendulums
  • Weight vs. Spring
  • Satellite orbital patterns (Mars, Venus, Earth)
  • When reading gravity measurements, remember to check where the black line is -> our measurements can’t go any deeper than that line
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16
Q

measuring anomalies

A
  • GRACE (Gravity Recovery And Climate Experiment): 2 identical orbiting satellites, part of their job is to observe isostasy
  • Wordon gravimeter: used to measure smaller anomalies, like variations over UBC’s underground library -> applications: indicate buried dense material, groundwater, etc.
17
Q

evidence for gravity and solar system formation

A
  • Planets orbit in same direction (counter-clockwise)
  • Orbits of planets are approximately in same plane
  • Density of planets decreases away from the sun
  • Terrestrial/rocky planets close to sun, Jovian/gassy planets farther away
18
Q

solar nebula hypothesis

A
  • Cloud of dust and debris from supernova starts to contract and rotate
  • Temperature in centre of cloud starts to increase and glow
  • Gravity attracts particles together in surrounding disk (accretion)
  • Accreted matter starts to form larger bodies (protoplanets)
  • Pressures/temperatures increase, initating nuclear fusion -> our sun is born!
  • Radiation from sun pushed lighter elements away -> only denser material is close to sun
19
Q

planetary formation

A
  • Division between terrestrial and Jovian due to where they formed
  • Close to the sun, lighter gases blown away -> gases condense beyond “snow line” to form Jovians
20
Q

formation of earth

A
  • Following accretion – earth heats and differentiates
  • Heavier elements sink to centre -> iron core (gravity)
  • Initially a magma ocean
21
Q

All planets have ____ and all physical bodies _______

A
  • gravity

- attract each other