Course title
CD0060003
Space Science

 ASAI Kazumi

YUMOTO Atsushi
Course description
This course introduces the origin of the universe, the structure of the solar system, our galaxy, a cluster of galaxies, and the large-scale structure of the cosmos.
In this course students will get a deep understanding of them by using the fundamental rules of nature such as the blackbody-radiation law in Thermodynamics, Kepler’s law in Dynamics, Doppler effect in Wave Mechanics, and so on.
Purpose of class
The aim of this course is for students to get an eye of looking at things on a global scale, and to put up his sense of question about environmental issues, peace issues, and so on.
Goals and objectives
  1. Explain the origin of the universe.
  2. Explain the hierarchical structure of the universe.
  3. Take a complicated phenomenon into some elementary phenomena and explain the essence of it by virtue of fundamental laws of Physics.
Relationship between 'Goals and Objectives' and 'Course Outcomes'

 short report final exam Total.
1. 5% 10% 15%
2. 5% 20% 25%
3. 20% 40% 60%
Total. 30% 70% -
Evaluation method and criteria
Your overall grade in the class will be decided based on the following:
- task of lessons each time:30%
- Term-end examination: 70%
Language
Japanese
Class schedule

 Class schedule HW assignments (Including preparation and review of the class.) Amount of Time Required
1. Introduction of this course

The origin of the univserse
1. Big-bang cosmology
2. Inflationary cosmology
3. Histroy of the universe 		Review this chapter in PDF files. 60minutes
2. The size of universe
1. The observation
2. The observation by electromagnetic waves
3. The hierarchical structure of the universe.
4. The measurements of distance
5. The end of universe 		Review this chapter in PDF files. 60minutes
3. The Sun
1. Color and temperature
2. The energy source of the Sun
3. The temperature of the Sun
4. The pehomina of the SUn
5. Magnetic reconnection
6. aurora 		Review this chapter in PDF files. 60minutes
4. The planets
1. The definition of planet
2. The definition of dwarf planet
3. Kepler's laws
4. The character of the planets 		Review this chapter in PDF files. 60minutes
5. Small objects in our solar system
1. Small objects
2. Asteroids
3. Comets
4. extrasolar planet 		Review this chapter in PDF files. 60minutes
6. The birth of star
1. The evolution of a star
2. Dark nebula
3. The birth of a protostar
4. From a protstar to main-sequence star
5. The structure of a protostar 		Review this chapter in PDF files. 60minutes
7. Star
1. Why does a star shine?
2. The brigthness of star
3. The size of star
4. The age of star
5. The end of star 		Review this chapter in PDF files. 60minutes
8. Super Nova
1. Super Nova (SN)
2. The observation of SN
3. The detection of neutrino
4. The classification and evolution of supernova remnant 		Review this chapter in PDF files. 60minutes
9. Compact object
1. White dwarf
2. Nutron star
3. Black hole
4. Observational compact objects 		Review this chapter in PDF files. 60minutes
10. Our galaxy
1. The structure of our galaxy
2. the rotation of galaxy and dark matter
3. the local galactic group 		Review this chapter in PDF files. 60minutes
11. Galaxy
1. The lassifiation of galaxy
2. Hubble's law
3. Gravitational lens effect 		Review this chapter in PDF files. 60minutes
12. Active galaxy
1. AGN and the classifications
2. Jets
3. Radio observations
4. Doppler effet 		Review this chapter in PDF files. 60minutes
13. Clusters of galaxies and Future of the Universe
1. Clusters of galaxies
2. Classification of clusters of galaxies
3. Large‐scale structure of the cosmos
4. Future of the Universe 		Review this chapter in PDF files. 60minutes
14. Final exam.
You can check the understanding of this course by the final exam. 		Review all chapters in PDF files. 60minutes
Total. - - 840minutes
Feedback on exams, assignments, etc.
ways of feedback specific contents about "Other"
Feedback in outside of the class (ScombZ, mail, etc.)
Textbooks and reference materials
Nothing in particular.
Prerequisites
Being able to use the differential calculus and integration is necessary.
Office hours and How to contact professors for questions
  • i029683@shibaura-it.ac.jp
Regionally-oriented
Non-regionally-oriented course
Development of social and professional independence
  • Course that cultivates an ability for utilizing knowledge
Active-learning course
N/A
Course by professor with work experience
Work experience Work experience and relevance to the course content if applicable
N/A N/A
Education related SDGs:the Sustainable Development Goals
  • 4.QUALITY EDUCATION
  • 9.INDUSTRY, INNOVATION AND INFRASTRUCTURE
Last modified : Fri Mar 07 11:49:24 JST 2025