K-MOOC

주차

주차명

(주제)

주차별 학습 목표

차시

차시명

학습 내용

1

Interstellar Medium (ISM)

The audience are to understand astronomical scales and physical characteristics of interstellar medium, such as of dust and gas.

1-1

Astronomical scales, ISM introduction

1-2

Introduction to Interstellar Medium

1-3

Dust and radiative transfer

2

Molecular Clouds

The audience are to study Molecular Clouds where the stars are born. They will also have chance to study mechanisms for heating,cooling and form-maintaining of the Molecular Clouds.

2-1

Line Radiation

2-2

Interstellar Medium: gas and observations

2-3

Molecular Clouds: overview and molecule formation

3

Molecular Clouds

to Protostars

The audience are to study how Molecular clouds becomes Proto-stars.

3-1

Molecular Clouds to Protostars: Physical parameters

3-2

Turbulence and Magnetic fields of ISM

3-3

Molecular Clouds to Protostars

4

Protostars and Planets

The audience are to study evolutionary stages of Young Stellar objects and the structures around them.

4-1

(Low Mass) Young Stellar ObjectsⅠ:evolutionary stages

4-2

(Low Mass) Young Stellar ObjectsⅡ:discussion of physical properties

4-3

Multiple star formation and Massive star formation

5

Stars: The Hertzsprung-Russel Diagram

Plotting the HR Diagram, Measurement of the stellar distances and magnitudes, How to classify the stellar spectra

5-1

Two-dimensional distribution of stellar parameters

5-2

Distances and Magnitudes

5-3

Magnitudes

5-4

The Classfication of Stellar Spectra

6

The Evolution of Stars

Nucleosynthesis in the stellar nuclei, Understanding the stellar evolution, especially after the main sequence

6-1

Energy Generation

6-2

Stellar Evolution

6-3

Post-Main-Sequence Evolution

7

Star Deaths

Understanding the final stage of the stellar evolution and supernova explosion, understanding the white dwarfs, neutron stars and black holes

7-1

Final Stage of Stellar Evolution

7-2

Supernova Explosion

7-3

White Dwarfs, Neutron Stars, and Black Holes

8

The Milky Way Galaxy

The shape and structure of our own Galaxy, understanding the stellar populations, Connecting the star clusters and the HR diagram

8-1

The Morphology of the Galaxy

8-2

Stellar Populations

8-3

Star Clusters and the HR Diagram

9

Galaxies beyond the Milky Way

To understand the discovery and classification of external galaxies as well as their physical properties.

9-1

External Galaxies

9-2

Irregular Galaxies

9-3

Multiwavelength Observations

9-4

Normal Galaxies

10

Hubble’s Law and Distance Scale

To understand the galaxy clusters which consist of many galaxies and further study the physical properties of the galaxy clusters.

10-1

Galaxy Clusters

10-2

Hubble’s Law

10-3

Distance Scale

11

Active Galaxies

To understand active galactic nuclei (AGNs) with supermassive blackholes which enables various activities of the AGNs, as well as the sub-components of the AGNs.

11-1

Radiation Mechanisms

11-2

Active Galactic Nuclei

11-3

Astrophysical Jets

12

Theory of relativity and universe evolution

The audience are to study Theory of Relativity and expanding universe.

12-1

Theory of Relativity

12-2

Expanding Universe

12-3

Space Origin Controversy

13

Evolution of the expanding universe

The audience are to study theories that explain the history of universe and experiments that proved those theories.

13-1

Expanding Universe and Energy 1

13-2

Expanding Universe and Energy 2

13-3

Standard candle

14

Start and evolution of large scale structure of the universe

The audience are to study the discovery of the Accelerating expansion of the universe and the experiment of large scale structure of the universe to understand its principles.

14-1

Copy space background

14-2

The big bang theory

14-3

Space initial inflation

15

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