Timing/Location: Tu/Thurs from 10:00 to 11:45 in E&MS D236 (and occasionally Friday 2-3:30 in D250)

Course Goals: To provide a quantitative, graduate-level investigation of the physical processes controlling the formation of planets and satellites in this (and other) solar systems.

Texts:  Most of the course will consist of close reading of journal articles, but Lissauer and DePater Planetary Sciences (2nd ed.) will be used heavily, and some use may be made of Murray and Dermott Solar System Dynamics.

(Approximate) Course Outline

Week 1 (4 Jan): Overview, gravity & orbits. Notes.

Week 2 (11 Jan): Disks and migration. Notes.

  • Lecture on Fri, 2-3:30 in D250 instead of Tuesday
  • Order-of-magnitude scalings, in D.J. Stevenson, Formation and early evolution of the Earth, in Mantle convection, ed. W.R. Peltier, Gordon & Breach, pp. 817-873, 1989.
  • An excellent one-page summary by A.P. Boss, Temperatures in protoplanetary disks, Ann. Rev. Earth Planet. Sci. 26, 53-80, 1998.
  • Section 4 of Hartmann et al., Ap. J. 495, 385-400, 1998 is useful.
  • Problem Set #2

Week 3 (18 Jan): Condensation and chemistry. Notes

  • Lecture on Fri, 2-3:30 in D250 instead of Tuesday
  • P. Cassen, Models for the fractionation of moderately volatile elements in the solar nebula, Meteorit. Planet. Sci. 31, 793-806, 1996.
  • Alexander et al. (2001) provide a good overview, and Drake & Righter (2002) are good on silicate bodies.
  • Problem Set #3

Week 4 (25 Jan): Solid body accretion. Notes

Week 5 (1 Feb): Obliquity and precession. Notes

Week 6 (8 Feb): Effects of impactsNotes.

Week 7 (15 Feb): Clocks. Notes.

Week 8 (22 Feb): Gas giant accretion. Notes.

  • Another Stevenson article provides an excellent discussion.

Week 9 (1 Mar): Satellite accretion

Week 10 (8 Mar): No lectures – LPSC