To understand the basics of planetary sciences: structure and properties of our Solar System, stars, and planets, as well as the formation and evolution of planetary systems. Also, some relations with other classes provided in the Department of Earth and Planetary Sciences are introduced.
To understand basics of planetary sciences.
Planetary Science, Astronomy, Astrophysics
✔ Specialist skills | Intercultural skills | Communication skills | Critical thinking skills | Practical and/or problem-solving skills |
Lectures.
Contents and the order of contents listed in the plan may change due to the progress of the class.
Course schedule | Required learning | |
---|---|---|
Class 1 | Introduction: What are planets? | To understand planets. |
Class 2 | Motion of Planets 1: Two-Body Problem | To understand two-body problem. |
Class 3 | Motion of Planets 2: Kepler Motion | To understand Kepler motion. |
Class 4 | Motion of Planets 3: Multi-Body System | To understand multi-body system. |
Class 5 | Internal Structure of Objects 1: Sun 1 --- Basic Equations --- | Think of the internal structure of the Sun. |
Class 6 | Internal Structure of Objects 2: Sun 2 --- Thermodynamical Properties --- | To understand thermodynamical properties of the Sun. |
Class 7 | Internal Structure of Objects 3: Solid Planets | Think of the internal structure of solid planets. |
Class 8 | Generation of Elements by Stars | To understand the origin of elements generated by nucleosynthesis. |
Class 9 | Age of Solar System | To understand the radiometric dating and the age of our solar system. |
Class 10 | Solar System Small Bodies 1 | To understand basic properties of asteroids and comets. |
Class 11 | Solar System Small Bodies 2 | To think of the internal melting of meteorite parent bodies. |
Class 12 | Extrasolar Planets | To understand basics of exoplanets. |
Class 13 | Formation of Planetary Systems 1: Star and Protoplanetary Disk Formation | To understand the formation of star and protoplanetary disk. |
Class 14 | Formation of Planetary Systems 2: Evolution of Dust Particles in Disk and Formation of Planets | To understand the evolution of dust particles in the disk. |
To enhance effective learning, students are encouraged to spend approximately 100 minutes preparing for class and another 100 minutes reviewing class content afterwards (including assignments) for each class.
They should do so by referring to textbooks and other course material.
None
All materials used in the class can be found in OCW-i.
Homework assignments: 100%
None