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Course Syllabus - AST 307

Chapter 1
-scales and sizes in the Universe
-angles, parallax and the parsec (pp 438-439)
-seeing (pp 118-119)
-celestial coordinates
-the earth's size and motions: rotation, revolution, precession
-the moon: phases, rotation (p 202), eclipses, tides (pp 187-190)

Chapter 2
-planetary motions and configurations (Fig. 9.2)
-sidereal vs synodic periods
-Kepler's laws and the size of the solar system
-Newton's laws, gravity, falling objects, orbits

Chapter 3
-waves, the EM spectrum, atmospheric windows, photons (pp 92-94)
-blackbody radiation laws, the Doppler effect

Chapter 4
-spectral lines, the Bohr model and energy levels
-molecular spectra, line widths

Chapter 5
-telescopes: refracting, reflecting, main properties
-detectors. Telescopes for radio and other wavelengths

Chapter 6
-brief summary of the solar system

Chapter 15
-other planetary systems?

Chapter 17
-properties and motions of stars: luminosities, the magnitude system,
 temperature and spectral classes, radii
-the H-R diagram, spectroscopic parallax
-masses of stars (binaries), the mass-luminosity relation

Chapter 16
-the sun: nuclear fusion and solar neutrinos

Chapter 18
-interstellar gas and dust, 21 cm radiation

Chapter 19
-star formation

Chapter 20
-evolution of low- and high-mass stars, white dwarfs
-evolution of binary systems

Chapter 21
-death of high-mass stars: supernovae, the Crab Nebula

Chapter 22
-neutron stars (pulsars) and black holes

Chapter 23
-the Milky Way galaxy: size, shape, stellar populations, spiral arms
-mass of our galaxy, dark matter

Chapter 24
-normal galaxies - types, masses
-Hubble's law, large-scale distribution of galaxies

Chapter 26
-cosmology, age of the Universe and its fate, the cosmic
 microwave background

Chapter 27
-the early Universe, inflation

Chapter 25
-active galaxies and quasars





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17 January 2003
Astronomy Program · The University of Texas at Austin · Austin, Texas 78712
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