PHYS1005 Introduction to Astronomy and Space Science

Module Overview

The module shows how simple physical principles can be used to learn about the Universe. The focus is upon how one can measure physical quantities such as size, distance, temperature, age and mass for the variety of objects in the Universe. By its end students should be able to appreciate topics of current interest in astronomy and cosmology. Students should be aware that this module requires A-level physics (with a C grade or above) and A-level maths (grade C or above).

Aims and Objectives

Learning Outcomes

Knowledge and Understanding

Having successfully completed this module, you will be able to demonstrate knowledge and understanding of:

Know the essentials of astronomical measurements of brightness and velocities
Understand how the distances, sizes and masses of astrophysical objects can be measured
Understand how the elements are formed inside stars
Know about the expansion of the Universe and how observations can lead to the determination of its age, mass and future evolution

Subject Specific Intellectual and Research Skills

Having successfully completed this module you will be able to:

Have an appreciation of the relative distances, sizes and masses of the various objects in the Universe

Syllabus

Solar system: - the properties of the planets and moons - solar system physics including formation - comets and asteroids Exoplanets: - classification - detection methods - state-of-the-art Stars: - The Hertzsprung-Russell (H-R) diagram; H-R diagrams of star clusters; classification of stars from their position in the H-R diagram - The dependence of stellar properties and timescales on mass - The determination of the ages of clusters - Physical conditions within stars - Nuclear fusion - Stellar evolution - Core-collapse supernovae - White dwarfs, neutron stars and black-holes Galaxies: - Classification of galaxies by their appearance - Galaxy interactions - The Milky Way - Active galaxies - Radio jets Cosmology: - The expansion of the Universe - The Cosmic Microwave Background - The Big Bang model - Measurement of the age and mass and the future evolution of the Universe

Learning and Teaching

Teaching and learning methods

Teaching will be primarily by delivered lectures, and learning is enhanced by problem sheets.

Type	Hours
Follow-up work	15
Completion of assessment task	56
Preparation for scheduled sessions	15
Wider reading or practice	36
Lecture	28
Total study time	150

Resources & Reading list

Chaisson & McMillan. Astronomy Today - Global Edition.

Assessment

Summative

Method	Percentage contribution
Continuous Assessment	100%

Repeat

Method	Percentage contribution
Set Task	100%

Referral

Method	Percentage contribution
Set Task	100%

Repeat Information

Repeat type: Internal & External