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Astronomy 171
Solar System Astronomy
Prof. Paul Martini
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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
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