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Titlebook: Highlights of Astronomy; As Presented at the Richard M. West (General Secretary of the Union) Book 1983 International Astronomical Union 1

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The Origin and Early History of the Sun and the Planetary System in the Context of Stellar Evolutionologies. The meteorites apparently contain material exposed to two nucleo-synthetic events, one about 10. yr and another a few 10. yr before solidification. Following 11. Reeves, these are asso­ciated with supernovae occurring in star clusters in mole­cular clouds that formed during passage through
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Solar Luminosity Variationsprecision radiometers on teh the NIMBUS-7 and SMM spacecraft. A substantial fraction of the observed variation can be attributed to sunspot blocking. Thermanl storage models indicate that the blocked flux can be stored in a slight increase of the thermal and potential energy of the cinvective zone.
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Origin and Evolution of Interplanetary Objectsts may contain less than average volatile material, wheter in formation or by radiative heating, raises the question of why at least two very faint short-period comets suddenly experienced violent outbursts (~4000 times in brightness). A preliminary study of close double comet nuclei as affected by
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