Astronomy 1 (Physics 1513)
Lecture Notes
Wednesday, Oct 28, 1997
The Earth
(Interior, Atmosphere, Energy Balance, Tectonics)
Read Text Chapters (Chaisson and McMillan) #7 - The Earth (include Interludes)
More Precisely 7-1 (Atmospheric Scattering)
More Precisely 7-2 (Radioactive Dating)
More Precisely 8-1 (Trapping Atmosphere on Planets)
Notes:
Homework Due Wednesday, Nov 4:
(See also Assignment #6 on Acme)
Chapter 6 Probs #2, 9, 10
Chapter 7 Probs #2, 3, 4, 10
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Where we are in the course:
Done Chap 1-6 (Weeks 1-8)
To do Chap 7-15 (Weeks 8 - 13)
approximately 1 chapter per class period (
(two per week)
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LECTURE
(Outline - read Chapter 7 for details)
Atmosphere
How Planets Keep their atmospheres (New Physics)
More Precisely 8-1 (Trapping Atmosphere on Planets)
Thermal distribution of molecular speeds
vaverage= (3kT/m)1/2
H2 --> 6.2 km/s
4He --> 4.4 km/s
N2 --> 1.6 km/s
Escape Velocity
vescape= 11.2 km/s
rule of thumb to escape
6 * vaverage > vescape
Earth's Atmosphere History
- 1st - Hydrogen, Helium (Remnant of Solar Nebula)
- 2nd Volcanic - Carbon Dioxide, Sulphur Dioxide, Water Vapor
- 3rd (3.5 billion ya) Oxygen/Nitrogen from life (algae)
Height Profile
Temperature (figure 7.2)
reversal defines
Troposphere (0-12 km)
Stratosphere (12 - 45 km)
Mesosphere (45 - 80 km)
Ionosphere 100 km
Pressure (Force/Area)
Sea level - 101,000 Pascals = 1 bar = 14.7 lb/in2
= 760 mm Hg = 30 inch water
Pascal = N/m2
Change in pressure with height = 1 inch/1000 feet
Fraction of Atmosphere
21% oxygen
78% nitrogen
0.03% Carbon Dioxide
0.1-3% Water Vapor
Radiation Balance (New Physics)
Concept of Albedo (depending on wavelength)
Concept of Greenhouse effect
(wavelength dependent transmission)
Short Wave (Solar Radiation)
Long Wave (Heat)
Atmospheric Optics (New Physics)
Blue Sky, Red Sunset
Rayleigh Scattering ~ 1/(wavelength)4
When particles < 0.1 of wavelength (molecules)
Ice Halos. sun Pillars and Rainbows
Scintillation (Due variations of index of refraction)
Circulation of the Atmosphere (Convection Cells) (New Physics)
Coriolis effect (New Physics)
Tropical, Temperate, and Arctic Cells
Wind Directions
Interior of the Earth
[concept of Pressure and Shear Waves - seismic waves] Figure 7.6
Crust (Ocean versus Continent) Thickness and Composition
Mantle Temperature and Convection
Core
Pressure and Temperature with Depth (Figure 7.7)
Tectonics
(Mountains, Troughs and Mid-ocean rifts, Volcanoes and Hot Spots)
Movement ~ cm/yr
Age of the Earth
Nuclear Physics and Radioactive Decay (New Physics)
(elements used) Half-life
40K --> 40Ar 1.3 billion years
238U --> 206Pb 4.5 billion
232Th --> 208Pb 14.0 billion
87Rb --> 87Sr 48.8 billion
Daughter Nucleii and aging
Magnetosphere
Magnetic Dipole Field of the Earth (New Physics)
Angle of magnetic dipole to Earth geometry
North Magnetic Pole 76N 100W
South Magnetic Pole 66S 139E
magnetic field ~ 0.5 Gauss (0.00005 Tesla)
Trapping of charged Particles in a magnetic field (New Physics)
Van Allen Belts:
Particles E=10-100 keV H+ (<10/cm3)
Aurora (green 558nm oxygen lines)
Solar Winds and magnetosphere (protons and electrons)
Plate Tectonics
Crust and Mantle circulation
Plate collisions (movement ~ cm/year = 1000km/108yr)
Mountains
Subduction zones and Volcanoes
Faults
Mid-Ocean Ridges
Magnetization variation and age
History of Crust Movement
Oceans
Circulation
Tides
Physics of Tidal Effects (New Physics)
Differential Tidal Force ~ M/r3
Timing of Tides
Daily (52 minute delay of high tides)
Phases of the Moon (neap and spring tides)
(Tides due to the Sun = 1/2 those due to the Moon)
Slowing of the Earth's Rotation (2 ms/century)
Determined by coral growth daily rings and annual rings
(Friction of water on the ocean bottoms)
Moon recedes from Earth (4 cm/year)
(Earth angular momentum decreases so to keep the
total momentum of the Earth-Moon system constant
the orbital momentum of the Moon must increase -
orbital momentum, L~r1/2 so the radius
of the orbit must increase)
[NOTE: L=mvr but Kepler's 3rd law says r3~P2
and P = 2(pi)r/v. So v ~ r-1/2 and when
all this is put together L~r1/2]
NEW PHYSICAL PRINCIPLES INTRODUCED IN THIS LECTURE
(We will see them again and again in talking about
other planets)
- Velocity Distribution of Gases versus Temperature
- Escape Velocity of Gases in an Atmosphere
- Convection in the Atmosphere and the Mantle
- Coriolis Force on a Rotating Earth
- Waves in Solids (seismic waves)
- Radioactive Decay and Half-life of Nuclei
- Infrared and Visible Optical Properties of the Atmosphere
- Scattering of Light and its function of Wavelength
- Magnetic Field of a Dipole Magnet
- Magnetic Forces on a Charged Particle
- Fluorescence of Atmosphere Gases Excited by High Energy Particles
- Tidal Force by Gravity of Large Bodies