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Astronomy 171
Solar System Astronomy
Prof. Paul Martini

Lecture 19: Tides


Key Ideas:

Tides are caused by the difference between the Moon's gravitational pull on the near and far sides of the Earth
Tidal Effects:
Tidal Locking of the Moon's Rotation
Tidal Braking slowing the Earth's Rotation
Lunar Recession (increasing size of the Moon's orbit)


Seashore Astronomy

Tides are familiar to those living near the sea:
Sea level is highest twice a day at "high tide"
Sea level is lowest twice a day at "low tide"
Timing of Tides is governed by the Moon
Time between successive high tides: 12 hours, 25 minutes
Time between successive moonrises: 24 hours, 50 minutes, exactly twice the high-tide interval.
Tides are caused by the gravitational pull of the Moon.


Differential Gravity

The Moon is 12,740 km closer to the near side of the Earth than to the far side
Result is a 7% stronger pull on the near side of the Earth
The net front-to-back differential force
Stretches Earth along the Moon-Earth line
Squeezes Earth at right angles to this line
Results in 2 tidal bulges, so 2 tides per day


Land and Sea Tides

How big is the Tidal Bulge of the Earth?
Rock is stiff and resists tidal deformation
"Body Tides" on Earth are only 30 cm high
Water is fluid and flows more easily with gravity:
Ocean tides are 1 meter high on the open sea
Near the shore, tidal flows and seafloor shape can result in much larger local tides.
Canada's Bay of Fundy has 12 meter tides


Sun Tides

The Sun also raises tides on earth
The differential gravity force between the day and night sides is about half that due to the Moon
Highest High Tides are Spring Tides:
When the Sun and Moon are lined up
Occur at New Moon and Full Moon
Lowest High Tides are Neap Tides:
When the Sun and Moon are at right angles
Occur at First and Last Quarter Moon


Tidal Locking of the Moon

The Earth raises body tides on the Moon
Earth is more massive, so the tides are stronger
Constant squeezing and stretching in a rapidly rotating Moon would generate heat:
Energy gets taken from the Moon's rotation
The Moon slows down until its rotation and orbit periods are the same, stopping the squeezing.
Result: Moon is Tidally Locked to the Earth
Always keeps the same face toward the Earth


Tidal Braking of the Earth

The Earth rotates faster than the Moon orbits
Friction between the oceans and seafloor drag the ocean tidal bulges in the direction of rotation (eastware)
Ocean Tides lead the Moon by about 10 degrees
Friction also robs energy from Earth's rotation
Slows the Earth down a tiny bit
Day is getting longer by 0.0023 sec/century
This effect is called Tidal Braking


Lunar Recession

The Moon feels a slight forward gravitational tug from the ocean tidal bulge
Results in a net acceleration of the Moon
Moves it outward into a slightly larger orbit
Lunar Recession
Increase in average Moon-Earth distance by about 3.8 cm per year
Measured by Doppler Laser Ranging


The Once and Future Moon

Tidal Braking and Lunar Recession are coupled:
Rotational energy from the Earth is transferred to the Moon as orbital energy
The Earth rotates slower and the Moon moves further away
After a few Billion years
The Moon will be ~50% farther away
Lunar Sidereal Month will be ~47 days long
Earth's rotation period will be 47 days
Earth and Moon get locked in a Tidal Resonance


Dynamical Evolution

Tidal phenomena are extremely important throughout the Solar System
We see examples of:
Tidal Resonances determining rotation periods (Moon and Mercury)
Tidal Locking (Pluto and Charon)
Tidally-induced Heating (Io around Jupiter and Triton around Neptune)
Tides are essential to understanding the dynamical evolution of the Solar System


See A Note about Graphics to learn why some of the graphics shown in the lectures are not reproduced with these notes.

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Updated: 2007 January 27
Copyright © Paul Martini All Rights Reserved.