![]() |
THE UNIVERSITY of EDINBURGHDEGREE REGULATIONS & PROGRAMMES OF STUDY 2007/2008
|
|
Specialist Topics in Astrophysics (U01423)? Credit Points : 10 ? SCQF Level : 10 ? Acronym : PHY-4-SpeTopAst Formation and Evolution of Planetary Systems: One of the biggest questions in modern-day astronomy is whether other stars have planetary systems similar to our own and whether they harbour Earth-like planets, possibly containing life. This course will cover the enormous progress that has been made in recent years in the understanding of how planetary systems form and evolve. Describing the methods used it will discuss the level of success so far achieved in detecting extrasolar planets and will address fundamental questions such as to whether our Solar System is unique. A key part of the course will be to look towards the future and examine the likelihood of finding Earth-like planets around nearby stars in our lifetimes. The search for biomarkers leading to the possible discovery of life will also be addresseed. Entry Requirements? Pre-requisites : At least 40 credit points accrued in courses of SCQF Level 9 or 10 drawn from Schedule Q, including Galaxies, Quasars & the Universe (PHY-3-GalQuas) and Physics of Stars & Nebulae (PHY-3-StarNeb). Subject AreasHome subject areaUndergraduate (School of Physics), (School of Physics, Schedule Q) Delivery Information? Normal year taken : 4th year ? Delivery Period : Semester 2 (Blocks 3-4) ? Contact Teaching Time : 2 hour(s) per week for 11 weeks First Class Information
All of the following classes
? Additional Class Information : Lecture times will be 1220-1310 Summary of Intended Learning Outcomes
Formation and Evolution of Planetary Systems: to follow
Upon successful completion of (the X-ray part of) this course, it is intended that a student will be able to: * Demonstrate an understanding of the radiation processes giving rise to X-ray emission, and be able to describe the astrophysical situations in which these take place. * Demonstrate an understanding of the thermal emission of galaxy clusters,apply hydrostatic models to these, and discuss the interpretation of the results in a cosmological context. * Explain the different modes of gas accretion onto compact bodies, and summarise the differences in their observable properties. * Review the observational evidence for supermassive black holes, and describe the X-ray properties of active galactic nuclei. Assessment Information
Degree Examination, 100%
Exam times
Contact and Further InformationThe Course Secretary should be the first point of contact for all enquiries. Course Secretary Mrs Linda Grieve Course Organiser Dr Ross McLure School Website : http://www.ph.ed.ac.uk/ College Website : http://www.scieng.ed.ac.uk/ |
|