Observational techniques, Radiative transfer, Star formation and stellar
evolution and large-scale structure of the Universe, Astrostatistics.
SH2402 Astrophysics 6.0 credits
Information per course offering
Choose semester and course offering to see current information and more about the course, such as course syllabus, study period, and application information.
Information for Spring 2025 Start 17 Mar 2025 programme students
- Course location
AlbaNova
- Duration
- 17 Mar 2025 - 2 Jun 2025
- Periods
- P4 (6.0 hp)
- Pace of study
33%
- Application code
60327
- Form of study
Normal Daytime
- Language of instruction
English
- Course memo
- Course memo is not published
- Number of places
Places are not limited
- Target group
CL/MAFY, CTFYS3, TELFM
- Planned modular schedule
- [object Object]
- Schedule
- Schedule is not published
- Part of programme
Degree Programme in Engineering Physics, åk 3, Optional
Master of Science in Engineering and in Education, åk 4, MAFY, Conditionally Elective
Master of Science in Engineering and in Education, åk 5, MAFY, Conditionally Elective
Master's Programme, Electromagnetics, Fusion and Space Engineering, åk 1, SPA, Mandatory
Contact
Felix Ryde (fryde@kth.se)
Course syllabus as PDF
Please note: all information from the Course syllabus is available on this page in an accessible format.
Course syllabus SH2402 (Spring 2022–)Content and learning outcomes
Course contents
Intended learning outcomes
After the course the student should be able to:
- Describe how fundamental astrophysical observations and measurements are performed: localisation, signal strength, distance scales. Plan and perform simpler astronomical observations and assess the outcome and give suggestions for improvements.
- By using physical reasoning, explain how radiation is transported within plasmas and in the universe. Explain how emission and absorption line features are formed and their diagnostics
- By using physical reasoning, explain the main evolutionary states for different types of stars.
- Describe the observations of the large-scale structure of the universe and assess the theories for structure formation in the universe on both small and large scales.
- Describe the various techniques for detection of extrasolar planets and discuss the conditions for life on other planets.
- Summarise the basis of astrophysics statistical analysis and solve basic problems.
Literature and preparations
Specific prerequisites
English B / English 6
Recommended prerequisites
Previous knowledge of mathematical methods in physics and quantum physics.
Equipment
Literature
Examination and completion
If the course is discontinued, students may request to be examined during the following two academic years.
Grading scale
Examination
- ANN1 - Notice, 1.0 credits, grading scale: P, F
- SEM1 - Seminar, 1.0 credits, grading scale: P, F
- TEN1 - Examination, 4.0 credits, grading scale: A, B, C, D, E, FX, F
Based on recommendation from KTH’s coordinator for disabilities, the examiner will decide how to adapt an examination for students with documented disability.
The examiner may apply another examination format when re-examining individual students.
Other requirements for final grade
Written exam (TEN1; 4 university credits)
Observation (ANN1; 1 university credit)
Seminarium (SEM1; 1 university credit)
Opportunity to complete the requirements via supplementary examination
Opportunity to raise an approved grade via renewed examination
Yes
Examiner
Ethical approach
- All members of a group are responsible for the group's work.
- In any assessment, every student shall honestly disclose any help received and sources used.
- In an oral assessment, every student shall be able to present and answer questions about the entire assignment and solution.