Gravity, Isostasy & Heat flow · Figure 4.16 Non-uniform body: divide it into pieces, calculate...
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Transcript of Gravity, Isostasy & Heat flow · Figure 4.16 Non-uniform body: divide it into pieces, calculate...
m
M
Gravity: force which is caused by mass.
g =GMm
r2
r
g is much bigger for smaller r
g is bigger for bigger M and m
G is a universal constantIt never changes. We can ignore it.
uniform sphere
g
gg
Uniform sphere: same gravity at the same distance from center of mass
but no planets or moons are uniform spheres...
Figure 4.16
Non-uniform body: divide it into pieces, calculate gravity from each piece, and add them up
mars.jpl.nasa.gov
Mars: big gravity anomalies that correlate with large-scale topography, as we’d expect...
Philippine Plate
Pacific PlateEurasian Plate
Australian-Indian Plate
Arabian Plate
Average Surface Elevation Oceanic: - 4.5 km Continental: + 0.5 km
Earth topography
Density of ice = 0.9 g/cmDensity of water = 1.0 g/cmDensity of air = 0.0 g/cm
“Just the tip of the iceberg”
Ice heavier than air -- sinks Ice lighter than water -- floats
Reaches a balance determined by the densities
3
3
3
Isostasy (a.k.a. “Isostatic Compensation”
Isostatic CompensationBimodal Topography & Crustal Thickness
Average Crustal Thickness Oceanic: 5 km Continental: 35 km
Average Surface Elevation Oceanic: - 4.5 km Continental: + 0.5 km
Surface elevations: coloursCrustal thickness: contour lines
Mooney et al., 1998
Average Crustal Density Oceanic: 3.0 g/cm Continental: 2.7 g/cm
3
3
Fig. 4.15
How isostasy is maintained (though imperfectly) - 3
adding bouyant plutons / thickening the continent
Local (small area) anomalies• local variations in rock density (mass = density times volume)• can be used to find metal ores• never isostatically compensated because they are small: crust is strong enough to prevent sinking or rising
Regional (large area) anomalies• none would exist if isostasy were perfect• tectonic forces cause anomalies surface pulled down at subduction zone trenches (-) rapidly building mountains lack buoyant roots (+)
Gravity anomalies are still present...
Heat flow
The inside of the Earth is HOT
High temperatures make asthenosphere gooey, allowing plate motion
Heat is needed for convection of the • core (which makes the magnetic field) • mantle (which starts plate tectonics)
Biggest sources of heat: • stored heat from when the Earth formed • heat from decay of radioactive elements
Geothermal gradient• Temperature increases with depth• Geothermal gradient is (change in T) /
(change in depth)– Deep mines are very hot (need AC)– On average 25 degrees per km– Heat can be used for geothermal energy– Temp at drill bit can be > 200 degrees
• Steep gradients do not persist– temperatures in convecting layers increase
just slightly with depth (pressure): 0.4 degrees/km in mantle