Planets in the solar-system are considered to be formed in protosolar nebular around protosun. Recent optical and radio observations have revealed existence of proto-planertary disks and planets around other stars. How did our solar-system and these extra-solar planetary systems form and evolve? This course will first provide basic knowledge about observational astronomy. Next, basics of optical, infrared and radio astronomy will be introduced, together with those of stars, planets, mocluar clouds, and proto-planetary disks. Lastly theories of planetary formation, evolution, interior, and atmosphere will be overviewed.
By the end of this course, students will be able to:
1) Understand the basics of optical, infrared, and ratio astronomy, and planet formation theory
2) Apply these knowledge to interpret properties of the solar-system and extrasolar planetary systems
optical and infrared astronomy, radio astronomy, planet formation theory, solar system, extrasolar planets, proto-planetary disk
|✔ Specialist skills||Intercultural skills||Communication skills||Critical thinking skills||Practical and/or problem-solving skills|
At the beginning of the class, a summary of the previous lecture is given. Then the main points of the day's lecuture are given, and students are asked to provide solutions to some of the questiones as necessary.
|Course schedule||Required learning|
|Class 1||Basics of astronomy: basic knowledge||Understand the definition of coorinates, distance, brightness and color of celstial objects.|
|Class 2||Basics of astronomy: two-body problem||Understand orbital motion of a star and a planet.|
|Class 3||Basics of astronomy: radiation and spectrum||Understand black body radiation, and formation of emission and absorption lines.|
|Class 4||Introduction to optical and infrared astronomy: various types of stars||Understand HR diagram and stellar evolution.|
|Class 5||Introduction to optical and infrared astronomy: stellar interior and atmosphere||Understand internal structure and stellar atmosphere.|
|Class 6||Introduction to optical and infrared astronomy: telescope and instrument||Understand photometric and spectroscopic observations.|
|Class 7||Introduction to optical and infrared astronomy: extrasolar planet||Understand observational methods and properties of extrasolar planets.|
|Class 8||Introduction to radio astronomy: basic knowledge||observations of star and planet forming regions, thermal emission of radio wavelengths, radio telescopes|
|Class 9||Introduction to radio astronomy: gravitational collapse of molecular clouds||molecular cloud, molecular cloud core, self-gravity|
|Class 10||Introduction to radio astronomy: formation of protostars and protoplanetary disks||protostar, T Tauri star, outflow, protoplanetary disk|
|Class 11||Introduction to radio astronomy: chemical processes of star and planet forming regions||molecular line observations of star and planet forming regions, astrochemistry|
|Class 12||Introduction to planet formation theory: basic knowledge||temperature and density structure of protoplanetary disks|
|Class 13||Introduction to planet formation theory: gas evolution in protoplanetary disks I||turbulent viscosity, gravitational instability|
|Class 14||Introduction to planet formation theory: gas evolution in protoplanetary disks II||magnetorotational instability, ionization degree, photoevaporation|
|Class 15||Introduction to planet formation theory: dust evolution in protoplanetary disks||dust dynamics and coagulation|
Reference books and course materials are introduced during the course.
Student's knowledge of basics of observational astronomy and planet formaiton theory, and the applications will be assessed by exercise problems and reports.