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2. Basic Scientific Goals
Pages 18-20

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From page 18...
... The primely initial goals are to confirm the presence and frequency of, or limit the existence of, extrasolar planets in the Jupiter- to Uranus-mass range, and to study the dynamics of discovered systems. 1b achieve these goals requires the following: · Development of instrumentation to enable sensitive search techniques, and application of these techniques to a stellar population sufficient)
From page 19...
... This general goal requires both new theoretical comparisons among such systems and related laboratory experiments, including considerations of the following: · Companion of low-mass stars, substellar objects, and planets and the differences and similarities of their formation conditions; Various types of binary systems and plan eddy systems and the relations among them; · Fragmentation of a collapsing and rotating assemblage into multiple objects and their subsequent evolution; · Physical and chemical characterization of stellar nebulae through time, silicate-carbon dust grains and icy-organic Gain mantles, the precipitation of solid matter from cooling nebular gas, He conditions under which dust paroles and planetesimals accrete or erode, and the evolution of accretion
From page 20...
... 20 disks from initiation of dust agglomeranon into subplanetary objects through subsequent plarzet-buildingsta~s; and · Defininon of propernes of planetary systems in the process of formation that could be subject to astronomical observanow


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