ABSTRACT
Since the discovery of the first exoplanet orbiting a main sequence star in 1995, nearly 500 planets have been detected, with this number expected to increase dramatically as new ground-based planetary searches begin to report their results. Emerging techniques offer the tantalizing possibility of detecting an Earth-mass planet in the habitable zon
TABLE OF CONTENTS
part |2 pages
I Detection of Extra-Solar Planets: Methods and Observations
part |2 pages
II Formation and Evolution of Planetary Systems
part |2 pages
III Dynamics of Planetary Systems