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Titlebook: Exoplanets; Detection, Formation John W. Mason Book 2008 Springer-Verlag Berlin Heidelberg 2008 Brown Dwarfs.Evolution.Exoplanets.Extrasola

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Detection of Extrasolar Planets by Gravitational Microlensing,w-mass planets at separations of a few AU. The early evidence from microlensing indicates that the most common types of exoplanet yet detected are the so-called super-Earth planets of 10 Earth-masses at a separation of a few AU from their host stars. The detection of two such planets indicates that
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,The Brown Dwarf — Exoplanet Connection,nergy source, they cool and fade on timescales that are rapid by astronomical standards. Consequently, the observed characteristics of old, cold brown dwarfs provide insight into the expected properties of gas-giant exoplanets. This review focuses on brown dwarfs as companions to main-sequence and e
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Dynamics of Multiple Planet Systems,(long-term) effects. Basic analytical and numerical techniques can describe these interactions. Multiple planet systems may also evolve chaotically, and some principles of chaos theory are described. Finally, this chapter discusses the current distributions of dynamical properties of exoplanetary sy
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