Infrared spectroscopy of organics of planetological interest at low temperatures.
In the context of prebiotic chemistry in space, some of the outer planetary objects display H, C, N and O rich chemistry similar to the one in the biosphere of Earth. Of particular interest are Saturn's moon, Titan; Neptune's moon, Triton; and Pluto where extreme cold conditions prevail. Identifications of chemical species on these objects (surfaces and atmospheres) is essential to a better understanding of the radiation induced chemical reactions occurring thereon. There have been several ground based observations of these planetary objects in the infrared windows from 1 to 2.5 micrometers. Voyager also provided spectra in the thermal infrared (6 to 50 micrometers) region. Interpretation of these data require laboratory infrared spectra of relevant species under the temperature conditions appropriate to these objects. The results of some of these studies carried out in our laboratory and elsewhere and their impact on the analyses of the observed data will be summarized.
Khanna
R K
RK
Department of Chemistry and Biochemistry, University of Maryland, College Park 20742, USA.
D003080:Cold Temperature; D019418:Evolution, Chemical; D018559:Exobiology; D005118:Extraterrestrial Environment; D006838:Hydrocarbons / Q000032:analysis* / Q000737:chemistry; D007053:Ice / Q000032:analysis; D018541:Neptune; D009570:Nitriles / Q000032:analysis / Q000737:chemistry; D016083:Planets; D018542:Pluto; D018539:Saturn; D013055:Spectrophotometry, Infrared
D006838:Hydrocarbons; D007053:Ice; D009570:Nitriles