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
- A review of coordinates
-
The distance to asteroid 2002 NY40 via parallax
-
Heliocentric parallax
-
Bias in parallax measurements
- The magnitude scale
- Blackbody radiation
-
Astronomical spectra, filters and magnitudes
-
Astronomical "color"
-
Measuring stellar sizes
- Elliptical orbits
- Kepler's Third Law
- The "Reduced Mass" approach
- The equivalence of
real and reduced-mass systems
- Integrals of motion
and Kepler's Third Law (again)
- The effect of a
tilted orbital plane
- Removing the tilt
from a visual binary's orbit
- Using the virial
theorem: mass of a globular cluster
- Using the virial
theorem: mass of a cluster of galaxies
- Digression:
the Lagrange points in the 3-body problem
- Introduction
to Stellar Spectra
- Spectral
Classification
- The Boltzmann Equation
- The Saha Equation
- Digression: The
Expanding Photosphere Method
- Luminosity
class and the HR diagram
- Properties of the
Radiation Field
- (Local)
Thermodynamic Equilibrium
- Optical Depth
- The causes of opacity
- Breaking News:
A star is born!
-
Vermin of the sky
- Random walks
- Limb darkening
- The shape of spectral lines
- The curve of growth
Homework sets
- HW 1: Coordinates and parallax.
- HW 2: Magnitudes, fluxes,
and spectra: oh, my!
(due in class Friday, Dec 19)
- HW 3: Orbits
(due in class Monday, Jan 12)
- HW 4: The orbit of 70 Oph
(due in class Wednesday, Jan 28)
- HW 5: Stellar atmospheres
(due in class Friday, Feb 13)
- 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.
Copyright © Michael Richmond.
This work is licensed under a Creative Commons License.