Creative Commons License Copyright © Michael Richmond. This work is licensed under a Creative Commons License.

Physics 440, "Astrophysics I", Winter 2003

This material can be found online at URL

http://spiff.rit.edu/classes/phys440/phys440.html

Outline for the course

Syllabus

Lectures

  1. A review of coordinates
  2. The distance to asteroid 2002 NY40 via parallax
  3. Heliocentric parallax
  4. Bias in parallax measurements

  5. The magnitude scale
  6. Blackbody radiation

  7. Astronomical spectra, filters and magnitudes
  8. Astronomical "color"
  9. Measuring stellar sizes

  10. Elliptical orbits
  11. Kepler's Third Law
  12. The "Reduced Mass" approach

  13. The equivalence of real and reduced-mass systems
  14. Integrals of motion and Kepler's Third Law (again)
  15. The effect of a tilted orbital plane

  16. Removing the tilt from a visual binary's orbit
  17. Using the virial theorem: mass of a globular cluster
  18. Using the virial theorem: mass of a cluster of galaxies
  19. Digression: the Lagrange points in the 3-body problem

  20. Introduction to Stellar Spectra
  21. Spectral Classification
  22. The Boltzmann Equation
  23. The Saha Equation

  24. Digression: The Expanding Photosphere Method
  25. Luminosity class and the HR diagram
  26. Properties of the Radiation Field
  27. (Local) Thermodynamic Equilibrium

  28. Optical Depth
  29. The causes of opacity
  30. Breaking News: A star is born!

  31. Vermin of the sky
  32. Random walks
  33. Limb darkening
  34. The shape of spectral lines
  35. The curve of growth

Homework sets

  1. HW 1: Coordinates and parallax.
  2. HW 2: Magnitudes, fluxes, and spectra: oh, my! (due in class Friday, Dec 19)
  3. HW 3: Orbits (due in class Monday, Jan 12)
  4. HW 4: The orbit of 70 Oph (due in class Wednesday, Jan 28)
  5. HW 5: Stellar atmospheres (due in class Friday, Feb 13)
  6. HW 6: Final homework set (due Thursday, Feb 26, at 9:00 AM)

For more information


This page maintained by Michael Richmond. Last modified Jul 19, 2007.

Creative Commons License Copyright © Michael Richmond. This work is licensed under a Creative Commons License.