ASTR 202: Exploration of the Solar System
Fall 2001
Course Content
- Introduction: A Brief Tour of the Universe
- The Sun: Size, mean Earth-Sun distance (1 AU), radiated power
- The Planets: Relative sizes and distances
- Stars: Birth, evolution and death, the next-nearest star, the light-year
- Galaxies: Our galaxy, nearby galaxies, clusters,
superclusters, the large-scale structure of the Universe
- Powers of Ten video
- Scientific notation, conversion of units
- The small-angle formula. Degrees, arcminutes and arcseconds
- Text reference: Chapter 1
- Knowing the Heavens
- Constellations
- Diurnal motion
- Seasonal variations of the night sky
- The tilt of the Earth's axis and the seasons
- The celestial sphere
- The celestial poles and the celestial equator
- Zenith and circumpolar stars
- The ecliptic, equinoxes and solstices
- The daily motion of the Sun across the sky
- Celestial coordinates: declination and right ascension
- Precession of the equinoxes
- Text reference: Chapter 2
- Eclipses and the Motion of the Moon
- The phases of the Moon
- The synchronous rotation of the Moon
- Synodic months and sidereal months
- Eclipses and the line of nodes
- Three types of lunar eclipse (total, partial and penumbral)
- Three types of solar eclipse (total, partial and annular)
- Text reference: Chapter 3
- Gravitation and the Waltz of the Planets
- The direct and retrograde motion of the planets
- The Ptolemaic (geocentric) model
- Epicycles and deferents
- Explanation of retrograde motion
- Objections to the Ptolemaic model
- The Copernican (heliocentric) model
- Explanation of retrograde motion
- The planets at different times of the year
- Inferior and superior planets, conjunctions and oppositions
- Support for a heliocentric model from Galileo's telescope observations
- The phases of Venus
- The moons of Jupiter
- Kepler's Laws of Planetary Motion
- Kepler's First Law: Elliptical orbits, semimajor axis,
eccentricity, perihelion and aphelion
- Kepler's Second Law: Equal areas in equal times, perihelion, aphelion
- Kepler's Third Law: P2 = a3
- Newton's Laws of Motion (statement, examples, implications for
planetary motion)
- Newton's First Law: Inertia, zero net force
- Newton's Second Law: Acceleration, mass, F=ma
- Newton's Third Law: Equal and opposite forces, action and reaction
- Newton's Law of Gravitation
- Newton's law of gravitation in equations and pictures
- Centrifugal force Fc = mv2/R
- The derivation of Kepler's Laws from Newton's Laws, Newton's
form of Kepler's Third Law
- Calculating the mass of the Sun
- Exam 1
- Tidal forces and an explanation of the synchronous rotation of the
Moon
- Text reference: Chapter 4
- Our Solar System
- The New Solar System video
- Tom Hill's lectures on Jupiter (see below)
- Orbital properties of the planets
- Orbital planes, eccentricities, direction
- Formation of the solar system: Solar nebula, gravitational
collapse, protosun formation, disk formation
- Physical properties of inner (terrestrial) and outer (Jovian) planets
- Diameters and average densities
- Information from spectroscopy and from samples
- Initial composition of the solar nebula
- Formation of planetesimals and protoplanets
- Formation of the inner planets: accretion
- Formation of the outer planets: accretion at much lower temperatures
- Temperature and planetary atmospheres: Temperature scales, kinetic
energy and escape velocity
- Extrasolar planetary systems
- Proplyds
- Astrometric and radial velocity methods
- The Doppler effect
- Properties of extrasolar planetary systems and open questions
- Text reference: Chapter 7
- Jupiter: Lord of the Planets
- Basic Jupiter data (diameter, mass, composition)
- Jupiter's appearance: Belts, zones, the Great Red Spot and other
storms
- Fast differential rotation rate, large internal energy
and consequences for Jupiter's atmosphere
- The comet Shoemaker-Levy 9 impacts
- Results from the Galileo Probe
- Internal structure
- Oblateness and implications for a rocky core
- Liquid metallic hydrogen and helium
- A thin gaseous outer layer
- Strong magnetic field
- The Jovian magnetosphere
- Text reference: Chapter 13
- The Galilean Satellites of Jupiter
- Orbital properties
- Unique physical properties
- A mini solar system
- Io's volcanoes and the Io torus
- The Io-Jupiter current system and Jovian aurora
- Europa's ice rafts
- Text reference: Chapter 14
- Our Living Earth
- Unique features of planet Earth
- Dynamic features of Earth's oceans, atmosphere and land masses
- Energy sources of geophysical activity
- The solar energy flux incident on Earth (the solar constant)
- Earth's albedo
- The greenhouse effect and its effect on Earth's surface temperature
- The internal structure of the Earth
- Chemical differential and formation of a dense iron core
- Buoyancy force and Archimedes' Principle
- Layers: Inner core, outer core, mantle, crust
- Seismic waves: P waves, S waves, surface waves
- Propagation of seismic waves through the Earth, the shadow zone
- Plate tectonics
- The basic mechanism: convection, asthenosphere, lithosphere
- The Earth's major plates
- Plate tectonics and earthquakes, strike-slip fault
- Collisions of plates: subduction zones, mountain ranges, volcanoes
- Separation of plates: oceanic rifts, sea floor spreading
- Earth's magnetic field, electrodynamics and the magnetosphere
- Generation of Earth's magnetic field
- Charged particles, electric fields and magnetic fields
- Rutherford's nuclear model of the atom, the New Zealand $100 bill
- Motion of charged particles in electromagnetic fields
- Plasma!
- The solar wind and its interaction with Earth's magnetic field
- The bow shock, magnetosphere and the Van Allen radiation belts
- The aurora
- Text reference: Chapter 8
- Our Barren Moon
- Basic Moon data (E.g., radius, mass, distance from Earth, eccentricity,
orbit plane, spin tilt, albedo)
- Absence of an atmosphere (and consequences of this)
- Surface features: Maria, terrae, craters
- The far side of the Moon
- Absence of plate tectonics
- General rule: An abundance of craters implies an old surface with little
or no geological activity
- Absence of a (present-day) lunar magnetic field
- Lunar seismology
- Seismic waves and moonquakes
- The interior structure of the Moon
- General rule: Smaller worlds retain less internal heat and display less
geological activity on their surface
- Formation of the Moon
- Competing theories
- The collisional ejection theory
- Text reference: Chapter 9
- Exam 2
- Sun-Scorched Mercury
- Observing Mercury from Earth (favorable and unfavorable elongations,
appearance)
- Basic Mercury data
- Solar transits
- Measuring rotation using radio waves; the Arecibo Observatory
- 3-2 spin-orbit coupling
- Day and night on Mercury
- Basic surface features (craters, smooth plains, scarps, the Caloris
basin)
- Interior and magnetic field
- Magnetosphere
- Text reference: Chapter 10
- Cloud-Covered Venus
- Observing Venus from Earth (elongations, appearance)
- Basic Venus data
- Solar transits
- Slow retrograde rotation
- Atmosphere: Composition, pressure, density, the runaway greenhouse effect
- The Stefan-Boltzmann law and planetary surface temperatures
- Sulfuric acid clouds and volcanoes
- Results from Magellan mapping of Venus's surface
- Text reference: Chapter 11
- Red Planet Mars
- Thunderbirds Martian Invasion!
- Observing Mars from Earth (favorable oppositions, appearance)
- Basic Mars data
- Martian canals
- Craters, volcanoes and canyons
- The Mars Orbiter laser altimeter map
- Northern lowlands and southern highlands
- Olympus Mons
- Valles Marineris
- Signs of water on Mars
- Atmosphere: Composition, pressure, the runaway icehouse effect
- Loss of water on Venus and Mars (the role of solar wind and magnetic
fields)
- Martian moons: Phobos and Deimos
- Text reference: Chapter 12
- The Spectacular Saturnian System
- Basic data and appearance from Earth
- Saturn's rings
- A, B and C rings, the Cassini division, ring thickness
- Composition and sizes of ring particles
- The Roche limit
- Fine structure: The Encke gap, ringlets, the F ring
- Influences of Saturn's moons: the Cassini division, the F ring and the
Encke gap
- Atmosphere and internal structure: Similarities to Jupiter, helium rain
- Saturn's moons: Titan and it's properties, mid-sized and small moons
- The Cassini mission
- Text reference: Chapter 15
- The Outer Planets
- Uranus and Neptune
- Discovery of Uranus
- Prediction and discovery of Neptune
- Appearance from Earth and basic data
- Voyager 2 fly-bys in 1986 and 1989
- Methane and the greenish-blue color of Uranus and Neptune
- Uranus's 98-degree (retrograde) tilt and extreme seasons
- The Great Dark Spot and methane crystal clouds
- Effects of Neptune's internal heat source: Storms, increase in
cloud-top temperature
- Internal structure and magnetic fields
- Dark, narrow planetary rings
- Pluto
- Basic data
- Discovery
- Pluto and Charon: a binary planet system in double synchronous
rotation
- Text reference: Chapter 16
- Vagabonds of the Solar System
- Asteroids
- The discovery of 1 Ceres
- The asteroid belt
- Jupiter's influence on the formation of the asteroid belt
- The Kirkwood gaps
- Impacts with Earth, extinction of the dinosaurs
- Meteoroids, meteors and meteorites
- Comets
- Structure: "dirty snowballs", coma, dust tail, ion tail
- Meteor showers
- Text reference: Chapter 17
Back to Home Page