Astronomy 225 - GALAXIES & DARK MATTER

Fall
2013
01
4.00
Suzan Edwards

MW 03:20-05:10

Smith College
19905-F13
WRIGHT 237
sedwards@science.smith.edu
Discover the compelling evidence that most of the mass of a galaxy is dark matter based on analysis of orbital data, stellar populations, and basic laws of physics in a simulated research experience. Interactive format includes computer simulations, data analysis, and confronting observations with theory. Final projects explore the viability of dark matter candidates. Offered in alternate years with 224. Prerequisites: PHY 115, MTH 111, plus one astronomy class.
Permission is required for interchange registration during the add/drop period only.
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