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천문학이야기 End(Audience) Certificate
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천문학이야기
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Field Natural (Mathematics, Physics, Astronomy & Geography)
Operating Institute Operating Institute University of Science and Technology Go to the operating agency Opens new window
Week Week 15 Week
Course Registration Period Course Registration Period 24.10.13 ~ 25.01.10
Phone Number Phone Number 01097901012
Course Satisfaction 4.3
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Difficulty Difficulty intermediate
Certificate Certificate Unissued
Learning recognition time Learning recognition time 16Hour 46Minute (16Hour 46Minute)
Course Duration Course Duration 24.10.15 ~ 25.02.15
Subtitle language 한국어 Others 1ea Subtitle language
Course language 한국어(ko)
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List of participating institutions
Course Introduction
강좌 소개
홍보영상
강좌 수강 정보
이수/평가정보
과제명 | 퀴즈 | 토론 | 최종 TEST |
반영 비율 | 40% | 40% | 20% |
최종 70% 이상시 이수됩니다. (관련문의: 박상우 T.A swpark@kasi.re.kr)
강좌 수준 및 선수 요건
해당 강좌는 천문학 기초부터 심화 과정까지 다루고 있어 우주에 관심 있는 일반인 및 천문학 학부생, 항공 우주 관련 일반 산업체 종사자까지 누구나 수강 가능합니다.
교재 및 참고 문헌
교재는 별도로 필요 없으며 매 차시마다 강의자료를 별도 제공합니다.
자주 묻는 질문
강좌 교재가 따로 있나요?
매 차시마다 강의자료를 별도 제공합니다.
- 강좌 관련 문의
UST-KASI 박사과정 박상우 swpark@kasi.re.kr
강좌운영팀 소개

Syllabus
강좌 운영 계획
주차 | 주차명 (주제) | 주차별 학습 목표 | 차시 | 차시명 |
학습내용 | ||||
1 | Interstellar Medium (ISM) | The audience is to understand astronomical scales and the physical characteristics of the interstellar medium, such as 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 is to study molecular clouds where stars are born. They will also have the chance to study the mechanisms of heating, cooling, and maintaining the form of 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 is to study how molecular clouds become protostars. | 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 is to study the 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, measuring stellar distances and magnitudes, and classifying 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 stellar nuclei and understanding 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 stages of stellar evolution, supernova explosions, and understanding 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 | Understanding the shape and structure of our Galaxy, stellar populations, and connecting star clusters to 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 | Understanding the discovery and classification of external galaxies and 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 | Understanding galaxy clusters, which consist of many galaxies, and studying the physical properties of galaxy clusters. | 10-1 | Galaxy Clusters |
10-2 | Hubble’s Law | |||
10-3 | Distance Scale | |||
11 | Active Galaxies | Understanding active galactic nuclei (AGNs) with supermassive black holes that enable various AGN activities, as well as the sub-components of AGNs. | 11-1 | Radiation Mechanisms |
11-2 | Active Galactic Nuclei | |||
11-3 | Astrophysical Jets | |||
12 | Theory of Relativity and Universe Evolution | The audience is to study the theory of relativity and the expanding universe. | 12-1 | Theory of Relativity |
12-2 | Expanding Universe | |||
12-3 | Space Origin Controversy | |||
13 | Evolution of the Expanding Universe | The audience is to study theories that explain the history of the universe and the experiments that proved these theories. | 13-1 | Expanding Universe and Energy 1 |
13-2 | Expanding Universe and Energy 2 | |||
13-3 | Standard Candle | |||
14 | Start and Evolution of the Large-scale Structure of the Universe | The audience is to study the discovery of the accelerating expansion of the universe and the experiments on the 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 | 기말고사 |
Field Natural (Mathematics, Physics, Astronomy & Geography)
Difficulty Difficulty intermediate
Operating Institute University of Science and Technology Go to the operating agencyOpens new window
Certificate Certificate Unissued
Week Week 15 Week
Learning recognition time Learning recognition time 16Hour 46Minute (16Hour 46Minute)
Course Registration Period Course Registration Period 24.10.13 ~ 25.01.10
Course Duration Course Duration 24.10.15 ~ 25.02.15
Phone Number Phone Number 01097901012
Subtitle language 한국어 Others 1ea Subtitle language
Course language 한국어(ko)
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