Laboratory experiments in the study of the chemistry of the outer planets.
The investigation of chemical evolution of bodies in our solar system has, in the past, included observations, theoretical modeling, and laboratory simulations.  Of these programs, the last one has been the most criticized due to the inherent difficulties in accurately recreating alien environments in the laboratory.  Processes such as wall reactions and changes in chemistry due to difficulties in achieving realistic conditions of temperature, pressure, composition, and energy flux may yield results which are not truly representative of the systems being modeled.  However, many laboratory studies have been done which have yielded data useful in planetary science.  Gross simulations of atmospheric chemistry have placed constraints on the nature of complex molecules expected in planetary atmospheres.  More precise studies of specific chemical processes have provided information about the sources and properties of product gases and aerosols.  Determinations of basic properties such as spectral features and reaction rate constants yield data useful in the interpretation of observations and in computational modeling.  Alone, and in conjunction with modeling, laboratory experiments will continue to be used to further our understanding of the outer solar system, and some experiments that need to be done are listed.
Scattergood
T W
TW
Department of Earth and Space Sciences, SUNY at Stony Brook 11794, USA.
D000336:Aerosols; D001256:Astronomy / Q000379:methods* / Q000639:trends; D001272:Atmosphere; D055598:Chemical Phenomena; D002621:Chemistry; D002845:Chromatography; D005118:Extraterrestrial Environment; D005544:Forecasting; D006838:Hydrocarbons; D016083:Planets; D012107:Research Design; D018539:Saturn; D016082:Solar System
D000336:Aerosols; D006838:Hydrocarbons