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Astronomy: Stellar Structure and Evolution

Course • Master's level • 7.5 credits

What powers a star for billions of years? What causes it to collapse, explode, or fade away? How can we connect observations of the outer layers of a star with what happens deep inside it? This course gives you a solid understanding of stars and how they change over time.
Application dates

Start

Autumn 2026

Level

Master's

Language

English

Place of study

Lund

Course code

ASTM25

Application dates

In this course, you will bring together concepts and tools from many areas of physics to understand the interiors of stars, and show that physical processes taking place on the smallest scales determine their structures and ultimate fates. You will study the physical processes that govern their behaviour – including nuclear reactions, energy transport – and how the equation of state of stellar matter affects a star’s stability.

You will derive how a star’s mass determines its entire life cycle, from birth to supernova or white dwarf. You will also derive the differential equations that describe stellar interiors, develop insight into their behaviour from analytical approaches, and explore the details of stellar lifecycles using numerical solutions of the equations. Additionally, you will see how the interior structures are connected to observable properties via simple models of stellar atmospheres.

Teaching is based on lectures, group work, and problem-based learning where you work together with other students to solve astrophysical problems. You will also study independently to deepen your understanding.

Examination includes a final written exam and written reports from problem-based learning sessions. You will be expected to analyse complex problems, apply theoretical models, and collaborate with others to find solutions.

Autumn Semester 2026

Closed for applications.

Start

2 November 2026

2 Nov 2026

End

17 January 2027

17 Jan 2027

Form

Normal learning

Pace

Part time

Language

English

City

Lund

Prerequisites

75 credits in Physics and 45 credits in Mathematics, or a Bachelor of Science in Physics, in both cases including knowledge corresponding to FYSC11 Atomic and Molecular Physics, 7.5 credits, and FYSC12 Nuclear Physics and Reactors, 7.5 credits. English 6/English course B.

Selection criteria

Seats are allocated according to: ECTS (HPAV): 100 %.

Tuition fees for non-EU/EEA citizens

Citizens of countries outside:

  • The European Union (EU)
  • The European Economic Area (EEA) and
  • Switzerland

are required to pay tuition fees. You pay an instalment of the tuition fee in advance of each
semester.

Tuition fees, payments and exemptions

Full programme/course tuition fee: SEK 23,125
First payment: SEK 23,125

Convert currency – xe.com

Note that you may also need to pay an application fee, or provide proof of exemption.

Application fee

No tuition fees for citizens of the EU, EEA and Switzerland

There are no tuition fees for citizens of the European Union (EU), the European Economic Area (EEA) and Switzerland.

Contact us

Senior lecturer

Ross Church

Email: ross.church@fysik.lu.se

Study counsellor

Johanna Nilsson Onsberg

Email: studievagledning@fysik.lu.se