%0 Journal Article %1 FEGLEY1994a %A FEGLEY, B. %A LODDERS, K. %D 1994 %J Icarus %K ABUNDANCE; COMBUSTION EVIDENCE; FLAMES; HELIUM INFRARED INHIBITION; KINETIC LUMINESCENT MATRIX MOLECULES; NEBULA; REACTIONS REACTIONS; SILANE-AIR SILICIC-ACID SOLAR SPECTROSCOPIC VERTICAL-DISTRIBUTION; %N 1 %P 117--154 %T Chemical-MODELS OF THE DEEP ATMOSPHERES OF JUPITER AND SATURN %V 110 %X New and updated chemical kinetic data, elemental abundances, and thermodynamic data are used for thermochemical equilibrium and, where relevant, thermochemical kinetic calculations of gas abundances and condensate stability in the hot, deep atmospheres of Jupiter and Saturn, Over 2000 compounds of all naturally occurring elements in the periodic table are considered. The calculations range from 298 to 2000 K and are done for adiabatic models of the two planetary atmospheres. The results predict the abundances of many gases which are potentially observable by the Galileo probe to Jupiter, by the Cassini mission to Saturn, and by Earth-based and Earth-orbital telescopes. In addition, the results also predict many new species which are potentially observable by a new generation of entry probes capable of penetrating deeper into the atmospheres of Jupiter and Saturn. (C) 1994 Academic Press, Inc.

@article{FEGLEY1994a, abstract = {New and updated chemical kinetic data, elemental abundances, and thermodynamic data are used for thermochemical equilibrium and, where relevant, thermochemical kinetic calculations of gas abundances and condensate stability in the hot, deep atmospheres of Jupiter and Saturn, Over 2000 compounds of all naturally occurring elements in the periodic table are considered. The calculations range from 298 to 2000 K and are done for adiabatic models of the two planetary atmospheres. The results predict the abundances of many gases which are potentially observable by the Galileo probe to Jupiter, by the Cassini mission to Saturn, and by Earth-based and Earth-orbital telescopes. In addition, the results also predict many new species which are potentially observable by a new generation of entry probes capable of penetrating deeper into the atmospheres of Jupiter and Saturn. (C) 1994 Academic Press, Inc.}, added-at = {2009-11-03T20:21:25.000+0100}, author = {FEGLEY, B. and LODDERS, K.}, biburl = {https://www.bibsonomy.org/bibtex/285b736bc11236659a54c702aff5bf1e1/svance}, interhash = {ef844bba46651926572ae4b5d62f6660}, intrahash = {85b736bc11236659a54c702aff5bf1e1}, journal = {Icarus}, keywords = {ABUNDANCE; COMBUSTION EVIDENCE; FLAMES; HELIUM INFRARED INHIBITION; KINETIC LUMINESCENT MATRIX MOLECULES; NEBULA; REACTIONS REACTIONS; SILANE-AIR SILICIC-ACID SOLAR SPECTROSCOPIC VERTICAL-DISTRIBUTION;}, number = 1, owner = {svance}, pages = {117--154}, timestamp = {2009-11-03T20:21:46.000+0100}, title = {Chemical-MODELS OF THE DEEP ATMOSPHERES OF JUPITER AND SATURN}, volume = 110, year = 1994 }