Kursussøgning, efter- og videreuddannelse – Københavns Universitet

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Kursussøgning, efter- og videreuddannelse

CANCELED Origin and Evolution of the Solar System

Practical information
Study year 2016/2017
Time
Block 3
Programme level Bachelor
Full Degree Master
ECTS 7,5 ECTS
Course responsibles
  • Henning Haack (2-6c6c44777271326f7932686f)
  • Uffe Gråe Jørgensen (6-786969686a6d4371656c316e7831676e)
  • The Natural History Museum of Denmark
  • The Niels Bohr Institute
Course number: NNMA13002U

Course content

The formation and evolution of the solar system based on cosmo-chemical chronology using short- and long-lived isotopes (such as 26Al-26Mg and 207Pb-206Pb), and on astronomical observations and models of stars and planets.  Meteorites and the thermal and chronological evolution of their parent bodies.  Differentiated meteorites from core, mantle and crust of fully or partially molten asteroids.  Primitive meteorites: their origin and formation of their components. Origin and evolution of the Earth-Moon system. The terrestrial planets. The exploration of Mars with space probes. Origin of planetary atmospheres. The outer planets and their moons. Comets and ices. Comparison of our Solar System with other planetary systems (exoplanets).

Learning outcome

Knowledge

  • Star formation
  • Element synthesis in stars
  • The sequence of events leading to the formation of our Solar System
  • Origin and early evolution of the Solar System
  • Origin and early evolution of Planets and their atmospheres
  • Origin of the Moon
  • Asteroids and their connection to meteorites
  • Main types of meteorites and their relevance for understanding the origin of the Solar System
  • Origin and evolution of comets

  • Short and long-lived chronometers such as 26Al-26Mg and U-Pb
  • Understanding major differences and similarities between our Planetary system and other known planetary systems (exoplanets)

Skills

Ability to read and understand Planetary Science papers

Competences

An understanding of the theories and observations supporting our current understanding of how the Solar System formed. In particular, the students should be able to relate the bulk properties of our own planet to the processes that controlled them, when the Earth formed. Being able to understand the significance of new data for our understanding of the origin and evolution of the Solar System.

Recommended prerequisites

Knowledge of basic concepts of geology is recommended.

Remarks

The course may be taken as an optional course on both the bachelor and the master part. However, for geology students it is recommended that you take it in the 2nd or 3rd year of the bachelor part.

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Education

Master programme in Physics

Studyboard

Study Board of Physics, Chemistry and Nanoscience

Course type

Part time Master and Diploma courses

Teacher

Martin Bizzarro, SNM
James Connelly, SNM
Morten Bo Madsen, NBI
Jes Jørgensen, NBI

Duration

1 block

Schedulegroup

A
---- SKEMA LINK ----

Teaching and learning methods

Lectures, practical exercises and a written assignment.

Capacity

Max 40 participants

Language

English

Workload

Category Hours
Exam 30
Preparation 78
Lectures 42
Practical exercises 6
Project work 50
English 206

Exam

Type of assessment

Written assignment
Oral examination, 30 minutes
The written assignment weighs 20% of the final grade.
The oral exam is without preparation time and weighs 80% of the final grade.

Aid

Without aids

Marking scale

7-point grading scale

Criteria for exam assessment

See learning outcome

Censorship form

No external censorship
Mere information om kurset
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