ge 11a, 2014, lecture 5 spherical structure of the earth

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GE 11a, 2014, Lecture 5 Spherical structure of the earth

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Page 1: GE 11a, 2014, Lecture 5 Spherical structure of the earth

GE 11a, 2014, Lecture 5Spherical structure of the earth

Page 2: GE 11a, 2014, Lecture 5 Spherical structure of the earth
Page 3: GE 11a, 2014, Lecture 5 Spherical structure of the earth

The earth, ca. 1800

Page 4: GE 11a, 2014, Lecture 5 Spherical structure of the earth

Nevil Maskelyne and the Schiehallion experiment (1774)

Schiehallion (‘Sidh Chailleann’) ScotlandNevil Maskelyne doing his impression of Ben Franklin

Ms

F = m.g.tan() = G.m.Ms/d2

F

m.g

d

m.g = G.m.ME/RE2

ME = (RE2/d2).(Ms/tan()) ~ 6.1024 kg

RE = 6.37.106 m; VE = 1.1.1021 m3

~ 5.5 g/cm2 (initially found ~ 4.5)

Page 5: GE 11a, 2014, Lecture 5 Spherical structure of the earth

Densities of common substances (all in g/cc)

Ice 0.917Water 1.000Seawater 1.025Graphite 2.200Granite ~2.70Titanium 4.507Iron 7.870Copper 8.960Mercury 13.58Gas: proportional to P/RT

Two options: sub-equal mix of metal and rock or…an ideal gas, w/ high density at high P (B. Franklin)

Page 6: GE 11a, 2014, Lecture 5 Spherical structure of the earth

Period of precession

Period of spin

Torque (sun and moon trying to pull earth’s tidal bulge into plane of ecliptic)

Moment of inertia

I = i mi.ri

2 miri Higher

Lower

Earth has I much less thanexpected for homogeneous sphere

Mass distribution in earth’s interior

Page 7: GE 11a, 2014, Lecture 5 Spherical structure of the earth

Kraemer, 1902

View combining known density, moment of inertia,oblateness, rigidity of surface rocks, and topography

Note bad for a bunch of turn-of-the-century quacks!

Page 8: GE 11a, 2014, Lecture 5 Spherical structure of the earth

Focus

Mantle

SeismographCoreS P

“sample” outer ca. 200 km,but most energy in upper 10 km

Page 9: GE 11a, 2014, Lecture 5 Spherical structure of the earth

A mechanical seismograph

Page 10: GE 11a, 2014, Lecture 5 Spherical structure of the earth

Minutes

Surface waves

0

P S

10 20 30 40 50

‘Primary’ (first to arrive)

‘Secondary’ (second to arrive)

Anatomy of a seismic signal

Page 11: GE 11a, 2014, Lecture 5 Spherical structure of the earth

Amplitude=23 mm

Richtermagnitude

Amplitude(mm)

Inte

rval b

etw

een

S a

nd

P w

aves (

s)

Dis

tan

ce (

km

)

P S

S-wave interval = 24 secondsP-wave

measure the amplitude of the largest seismic wave…

…and the timeinterval between the P- and S-waves (I.e., the distance from the epicenter.

Connect the points to determine theRichter magnitude.

Page 12: GE 11a, 2014, Lecture 5 Spherical structure of the earth

Real data is more complicated…

Page 13: GE 11a, 2014, Lecture 5 Spherical structure of the earth
Page 14: GE 11a, 2014, Lecture 5 Spherical structure of the earth

Look at your notes, John!

Page 15: GE 11a, 2014, Lecture 5 Spherical structure of the earth
Page 16: GE 11a, 2014, Lecture 5 Spherical structure of the earth

Look at your notes, John!

Page 17: GE 11a, 2014, Lecture 5 Spherical structure of the earth

Look at your notes, John!

Page 18: GE 11a, 2014, Lecture 5 Spherical structure of the earth
Page 19: GE 11a, 2014, Lecture 5 Spherical structure of the earth
Page 20: GE 11a, 2014, Lecture 5 Spherical structure of the earth

Mg2SiO4 in upper mantle

Mg2SiO4 in lower mantle

Page 21: GE 11a, 2014, Lecture 5 Spherical structure of the earth

The core’s density is less than that of pure Fe. Requires a low-massAlloying agent. S? O? H? ???

Page 22: GE 11a, 2014, Lecture 5 Spherical structure of the earth

The events in early earth history that controlled core/mantle segregation

Page 23: GE 11a, 2014, Lecture 5 Spherical structure of the earth
Page 24: GE 11a, 2014, Lecture 5 Spherical structure of the earth

Robin Canup’s movie

Animation of Theia forming in Earth's L5 point and then drifting into impact. The animation progresses in one-year steps making Earth appear not to move. The view is of the south pole.

Page 25: GE 11a, 2014, Lecture 5 Spherical structure of the earth
Page 26: GE 11a, 2014, Lecture 5 Spherical structure of the earth
Page 27: GE 11a, 2014, Lecture 5 Spherical structure of the earth

Evidence for the ‘magma ocean’ stage of the earth is essentially erased by laterconvection, plate formation, subduction, etc. But the moon’s crust preserves

evidence planets are largely liquid early in their history.

Page 28: GE 11a, 2014, Lecture 5 Spherical structure of the earth

And today Io, a moon of Jupiter, seems to possess a partially crystallized magma ocean, supported by tidal heating

Page 29: GE 11a, 2014, Lecture 5 Spherical structure of the earth
Page 30: GE 11a, 2014, Lecture 5 Spherical structure of the earth