Titan Tholins: Simulating Titan Organic Chemistry in the Cassini-Huygens Era
Authors: M.L. Cable, S.M. Hörst, R. Hodyss, P.M. Beauchamp, M.A. Smith, P.A. Willis http://dx.doi.org/10.1021/cr200221x
Authors: M.L. Cable, S.M. Hörst, R. Hodyss, P.M. Beauchamp, M.A. Smith, P.A. Willis http://dx.doi.org/10.1021/cr200221x
https://doi.org/10.1016/s0273-1177(01)00049-7 Various types of organic compounds have been detected in Jupiter, Titan, and cometary coma. It is probable that organic compounds were formed in primitive Earth and Mars atmospheres. Cosmic rays and solar UV are believed to be two major energy sources for organic formation in space. We examined energetics of organic formation in simulated planetary atmospheres. Gas mixtures including…
Authors: S. Civiš, L. Juha, D. Babánková, J. Cvačka, O. Frank, J. Jehlička, B. Králiková, J. Krása, P. Kubát, A. Muck, M. Pfeifer, J. Skála, J. Ullschmied In a mixture of molecular gases with compositions (CO2–N2–H2O and CO–N2–H2O) and total pressure close to that of the EarthÕs early atmospheres, a centimeter-sized plasma was created by focusing a single 85-J, 450-ps…
Authors: H.J. Cleaves II, C. Neish, M.P. Callahan, E. Parker, F.M. Fernández, J.P. Dworkin Various analogues of Titan haze particles (termed ‘tholins’) have been made in the laboratory. In certain geologic environments on Titan, these haze particles may come into contact with aqueous ammonia (NH3) solutions, hydrolyzing them into molecules of astrobiological interest. A Titan tholin analogue hydrolyzed in aqueous…
Authors: G.C. Stevens, R.M. Clarke, E.J. Hart The gamma-ray and electron pulse irradiation of aqueous methane and some ethane solutions is reported. The ab- sorption spectra of the CH3 and C2H5 free radicals have been measured in the wavelength range 210-270 nm. At 210 nm e(CH3) = 850 M-1 cm-1 and e(C2Hs) = 520 M-1 cm-1. The bimolecular recombination rate…
Authors: L. Zhou, S. Maity, M. Abplanalp, A. Turner, R.I. Kaiser The chemical processing of ethylene ices (C2H4) by energetic electrons was investigated at 11 K to simulate the energy transfer processes and synthesis of new molecules induced by secondary electrons generated in the track of galactic cosmic ray particles. A combination of Fourier transform infrared spectrometry (solid state) and…
Authors: P. Jiang, Y. Katsumura, M. Domae, K. Ishikawa, R. Nagaishi, K. Ishigure In the pulse radiolysis of concentrated phosphoric acid solutions, the direct action of radiation on phosphoric acid gives rise to the phosphate radical. The yields of the phosphate radical and the hydroxyl radical are proportional, respectively, to the electron fractions of phosphoric acid and water, and can…
Authors: G.R. Dey Generation of NO-3 and NO-2 in aqueous phase within high ionizing radiation zone is normal phenomena. Their formation mechanisms, and controls still remain a challenge with reference to creation of corrosive environment. Nitrogen in such system relates mainly to air ingress, and from added nitrogen compounds, which are used to control pH and dissolved oxygen. Under radiation…
Authors: G.P. Home, T.A. Donoclift, H.E. Sims, R.M. Orr, S.M. Pimblott A multiscale modeling approach has been developed for the extended time scale long- term radiolysis of aqueous systems. The approach uses a combination of stochastic track structure and track chemistry as well as deterministic homogeneous chemistry techniques and involves four key stages: radiation track structure simulation, the subsequent physicochemical…
Authors: I. Kayano, I. Tanaka, I. Omura https://doi.org/10.1063/1.1725591