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)