NFYK16008U Exoplanets and Astrobiology
MSc Programme in Physics
The purpose of the course is to present an understanding of how
the complexity of matter has evolved from its simplest forms during
Big Bang to the rise of intelligent life that is capable of
understanding its own place in this fabulous development.
Formation of the elements during Big Bang, supernovae and red
giants. Dust formation, stellar winds, and the re-circulation of
cosmic material. Formation of the solar system. Planets around
other stars. The physical-chemical basis for life. The arise and
development of life on the Earth. Conditions for finding life
beyond Earth. The search for extraterrestrial
intelligence.
Knowledge:
- Understanding of how the simplest elements were formed during Big Bang and how stars have processed them into larger atoms, molecules and solid material during the lifetime of the universe.
- Understanding how we today can measure the conditions and processes that formed our solar system 4.6 Gyr ago, and how we can compare that with the formation of other planetary systems.
- Understand the existing search methods for finding planets around other stars, and being able to compare the results of these methods to the knowledge we have about our own solar system.
- Understand the basic conditions that played a role for the rise of life on Earth, and some theories for how the development to advanced life forms can have taken place.
Skills:
When the course is finished, the student is expected to be able
to:
- Explain how the simplest material arose and developed into the complex matter of modern day universe.
- Put our own solar system in context of planetary systems in the Galaxy in general.
- Explain the difference between dead and living material, and explain what is meant by intelligence and by alien life.
- Explain how we at least in principle can identify and communicate with extraterrestrial life forms.
Competences:
Being able to argue for and against whether similar processes can
have taken place on other planets. Understand how we can search for
traces of life elsewhere in the universe and what our limitations
in searching for it are.
This course will provide the students with a competent background
for further studies within this research field, e.g. an MSc
project
Lecture notes
Most importantly, the student should have a curiosity about the synergy between the broad range of sciences that are involved in obtaining an understanding of why the universe exist and ended up with including intelligent life -- from Big Bang to Biology.
- Category
- Hours
- Lectures
- 48
- Preparation
- 129,5
- Exercises
- 28
- Exam
- 0,5
- Total
- 206,0
- Credit
- 7,5 ECTS
- Type of assessment
- Oral examination, 30 minutes (no preparation time)
- Type of assessment details
- The student will draw one of the approximately 8 known exam questions.
- Examination prerequisites
Participation in one of the large group presentations during the course.
- Aid
- No aids allowed
- Marking scale
- 7-point grading scale
- Censorship form
- No external censorship
Several internal examiners
- Re-exam
Same as ordinary exam.
If the student has not fulfilled the examination prerequisites, a presentation must be given in front of the teacher no later than 2 weeks before the re-exam.
Criteria for exam assesment
See Learning Outcome
Course information
- Language
- English
- Course code
- NFYK16008U
- Credit
- 7,5 ECTS
- Level
- Full Degree Master
- Duration
- 1 block
- Placement
- Block 3
- Schedule
- A
- Course capacity
- No limitation – unless you register in the late-registration period (BSc and MSc) or as a credit or single subject student.
Study board
- Study Board of Physics, Chemistry and Nanoscience
Contracting department
- The Niels Bohr Institute
Contracting faculty
- Faculty of Science
Course Coordinators
- Uffe Gråe Jørgensen (6-77686867696c4270646b306d7730666d)
Lecturers
Uffe Gråe Jørgensen