Angular Momentum
The Physics Hypertextbook™
© 1998-2008 by Glenn Elert -- A Work in Progress
All Rights Reserved -- Fair Use Encouraged
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Discussion
the idea
| Translational and Rotational Quantities Compared |
| |
translational |
connections |
rotational |
| momentum |
p =
|
m v
|
L =
|
r × p = m r × v
|
L =
|
I ω
|
| impulse-momentum |
∫ F · dt
F =
|
= Δp
dp / dt
|
|
|
∫ τ · dt
τ
|
= ΔL
dL / dt
|
text
| L = |
r × p = r × m v |
| L = |
m r × (ω × r) = m ω(r·r) − mr(r · ω) = mr2 ω − 0 = mr2 ω |
| L = |
I ω |
Moment of inertia again
| I = ∑ r2m = |
⌠ ⌡ |
r2 dm = ρ |
⌠ ⌡ |
r2 dV |
Conservation of angular momentum
Thus
L = constant
the earth
The earth is not the world's best clock.

[magnify]
[magnify]
types of LOD change … horrible mess …
- a linear increase owing to tidal dissipation
The tidal friction between the oceans and the Earth's surface causes the
Earth's rotation to slow by approximately 0.002 seconds every century.
However, ignoring energy lost to heat generated by the tides, the
angular momentum of the Earth-Moon system must remain constant. The
Earth's angular momentum is decreasing, so the Moon's must increase.
The only way it can do this is by moving into a higher orbit around
the Earth. Thus, the distance to the farthest point of the lunar
orbit is increasing by about 3.8 centimeters per year.
- Larger, irregular variations, on the scale of decades, owing to core-mantle
interactions
- Solar flares are known to abruptly alter the Earth's rotation. For example,
the great flares of 1959 and 1972 brought abrupt changes in the LOD.
Both long-term and short-term changes in solar activity alter the Earth's
rotation. The 11-year, 22-year and 56-year solar cycles are conspicuous
in the LOD data. Long-term (secular) changes were noted at times of fluctuations
in solar activity in the past, and the evidence indicates that these
changes were very likely abrupt. Observations of the LOD, like so many
other geophysical phenomena, reveal the solar-FEM linkage.
- Seasonal changes from the angular momentum exchange between crust and atmosphere.
The rate of rotation of the earth is high in summer and low in winter (northern hemisphere).
- exchange of angular momentum between the solid Earth and the atmosphere
- yearly melting of snow and ice in northern Spring
- and distribution of groundwater?
At time scales of hours to days, tidally driven? ocean currents and variations in the ocean height dominate
Summary
Problems
practice
- Write something.
- Write something different.
- Write something different.
- Write something completely different.
numerical
- Sun to a white dwarf. 27 days to … ?
Resources
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- earth's rotation
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