The table below shows the sequence of topics we will cover in this course. The dates are slightly tentative -- we may occasionally move ahead or fall behind. As you can see, we are not always following the textbook's arrangement of material. We may skip some sections within chapters.
Sep 6 | Introduction | |
Sep 8 | Tools: geometry and clocks | 9.1 |
Sep 10 | Tools: optical telescopes | 6.1 - 6.2 |
Sep 13 | Tools: telescopes beyond the optical | 6.4-6.5 |
Sep 15 | Tools: spectrographs | 6.3, 7.3 |
Sep 17 | Tools: interpretation of spectra | 7.1-7.4 |
Sep 20 | The Sun: overview | 8.1-8.2 |
Sep 22 | The Sun: energy source, neutrinos | 8.3 |
Sep 24 | Test 1 | |
Sep 27 | Special Guest Lecture | |
Sep 29 | Nearby stars: distances, absolute magnitudes | 2.1, 9.1-9.2 |
Oct 1 | Nearby stars: colors, the HR diagram | 9.3 |
Oct 4 | Nearby stars: masses, eclipsing binary stars | 9.4-9.5 | Oct 6 | The ISM and dust | 10.1-10.2 |
Oct 8 | Gas in the ISM | 10.3 |
Oct 11 | Star formation in the ISM | 11.1 | Oct 13 | Stellar Evolution: structure and energy sources | 11.2-11.3 |
Oct 15 | Stellar Evolution: timescales and the HR diagram | 12.1-12.2 |
Oct 18 | Stellar Evolution: clusters and ages | 12.3 | Oct 20 | Death of low-mass stars | 13.1-13.2 |
Oct 22 | Death of high-mass stars | 13.3 |
Oct 25 | Neutron stars | 14.1-14.2 |
Oct 27 | Black Holes | 14.1-14.2 |
Oct 29 | Test 2 | |
Nov 1 | The Milky Way Galaxy: overview | 15.1, 15.3-15.4 |
Nov 3 | The Milky Way Galaxy: pulsing stars determine its size | 15.1, 12.4 |
Nov 5 | The Milky Way Galaxy: its neighborhood | 16.1, 16.3 |
Nov 8 | Planets around other stars I: how to find them | 9.4 (for background) |
Nov 10 | Planets around other stars II: what are they like? | |
Nov 12 | Life on Earth -- and elsewhere? | 19.1-19.3 |
Nov 15 | Final Exam. 2:45 PM - 4:45 PM | 08-3305 |
Nov 16 | Alternate final. 2:45 PM - 4:45 PM | 76-1274 |
This page maintained by Michael Richmond. Last modified Oct 22, 2004.
Copyright © Michael Richmond. This work is licensed under a Creative Commons License.