The Physics of Stars
Uppsala University
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End date:
Pace of study: 67 %
Published education catalogue
The Physics of Stars
Education information from the published source. The education record and its time-bound offerings are kept separate.
Education facts
Code: 1FA223
Elementary physics of gas and radiation in stellar interiors and stellar atmospheres. Interaction between electromagnetic radiation and matter. The state of matter in the Sun and stars, nuclear reactions, and opacity. Energy transport in the Sun and stars. Equations of stellar structure. Comparison between observations and predictions from theory. Formation of stars. Production of elements during different phases of stellar evolution. Red giants as advanced stages of stellar evolution. Solar and stellar variability and pulsation. Supernovae as engines of galactic evolution. Exotic stars: white dwarfs, neutron stars, and black holes. Self-studies in case of few participants.
Entry requirements
120 credits in science/engineering including Astrophysics 1. Astrophysics 1 may be taken in parallel. Proficiency in English equivalent to the Swedish upper secondary course English 6.
Education offerings
Each offering has its own dates and conditions. Closed offerings are retained as history and do not mean that a new application is open.
Source and updates
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Publication version: 8e217193-f5fa-4778-b085-a4521fd03e8d
Checksum: 1b0dc54c0fc8a359f83ba9dc8f9d468479ce432de4c03bce3b8b33dd67fe3f6c
Last changed according to the source: 2026-02-12T18:37:23