Uusi opinto-opas (sisältäen myös opetusohjelmat) lukuvuodelle 2018-2019 sijaitsee osoitteessa https://opas.peppi.utu.fi . Tältä sivustolta löytyvät enää vanhat opinto-oppaat ja opetusohjelmat.

The new study guide (incl. teaching schedules) for academic year 2018-2019 can be found at https://studyguide.utu.fi. This site contains only previous years' guides.

x !
Archived teaching schedules 2016–2017
You are browsing archived teaching schedule. Current teaching schedules can be found here.
TÄHT7040 Stellar structure and evolution 8 ECTS
Period I Period II Period III Period IV
Language of instruction
Type or level of studies
Advanced studies
Course unit descriptions in the curriculum
MDP in Astronomy and Space Physics
Department of Physics and Astronomy

Learning outcomes

At the end of the course, students should be able to:
outline the main observed properties of stars as well as their masses;
use the equation of hydrostatic equilibrium to estimate the core properties of stars;
calculate the dynamical, thermal, and nuclear timescales of stars;
write down the four ordinary differential equations of stellar structure and their boundary conditions;
describe the main nuclear reactions that power high and low mass stars;
demonstrate a basic understanding of energy transport, sources of pressure;
outline the principles of evolution of high and low mass stars from the main sequence to the final stages;
explain how ages of stellar clusters can be measured from HR diagrams;
calculate the Jeans mass and describe the process of star formation;
explain the difference between degenerate and ideal gas;
describe the physics of compact stars and derive the mass-radius relationship for white dwarfs;
discuss the terminal stages of stellar evolution;
describe the main characteristics of different types of supernovae;
apply quantum and classical mechanics, and thermal physics to stellar systems;
describe the main difference between single and binary star evolution;
explain how to measure stellar masses in binary systems;
describe the main characteristics of different classes of white dwarf binary systems;
describe the relation between radio and X-ray pulsars;
develop self-study skills;
solve problems on topics in the syllabus.

Teacher responsible

Seppo Mattila


Anna Chashkina

Homepage URL


8-Sep-2016 –
Lectures 40 h
Thu 8-Sep-2016 - 24-Nov-2016 weekly at 10.00-12.00, Qh314
10-Nov-2016 , No lecture
Tue 13-Sep-2016 - 22-Nov-2016 weekly at 12.00-14.00, XVI
8-Nov-2016 , No lecture
Exercises 16 h
Mon 26-Sep-2016 - 3-Oct-2016 weekly at 14.00-16.00, Room 109, Quantum 1st floor, According to agreement
Mon 10-Oct-2016 - 24-Oct-2016 weekly at 10.00-12.00, Wihuri colloquium, Quantum 0-floor
17-Oct-2016 , No exercises
Mon 31-Oct-2016 at 10.00-12.00, Room 109, Quantum 1st floor, According to agreement
Mon 21-Nov-2016 at 10.00-12.00, Room 109, Quantum 1st floor, According to agreement