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نویسنده

  • M. J. Burchell
چکیده

Copyright and Moral Rights for the articles on this site are retained by the individual authors and/or other copyright owners. For more information on Open Research Online's data policy on reuse of materials please consult the policies page. Introduction: Several recent announcements of: i) the discovery of glycine on the comet 81P/Wild-2/P [1, 2]; ii) the successful shock synthesis of prebiotic compounds from liquid targets [3] and, iii) the results of molecular dynamics simulations demonstrating that amino acids could be created via shock synthesis of ices [4], have prompted a sequence of impact experiments using a light gas gun (LGG) at the Univ. of Kent [5]. The purpose of these experiments is to attempt to synthesise organic compounds from a mixture of simple ices (CO 2 , NH 3 and H 2 O). NH 3 compounds, CO 2 and H 2 O ices in the Sat-urnian system: According to observations made by Cassini's Visual and Infrared Mapping Spectrometer (VIMS) instrument, Enceladus' surface is composed mostly of nearly pure water ice except near its south pole, where there are light organics, CO 2 , and amorphous and crystalline water ice. The absorptions near 3.44 and 3.53 µm could be due to short-chain organics, but other features in the spectrum are still unidentified [5]. Remote IR acquired new high-resolution spectra of Iapetus, Tethys, Enceladus and Rhea that show the absorption feature of ammonia hydrate [6]. It thus seems probable that there are conditions on the surfaces of bodies in the Saturnian system where ammo-nium compounds, CO 2 and water ice co-exist in a solid form. Impact of a bolide traveling with sufficiently high velocity onto such a surface, should impart enough energy to promote shock synthesis of more complex organic compounds, including amino acids, from these ices. Laboratory experiments: Targets were prepared as follows: CO 2 ice (commercially purchased from BOC Ltd., stored in a freezer at a temperature of-130 °C) was repeatedly passed through a clean domestic ice crusher until the fragments' largest dimension was no bigger than ~3 mm. The crushed CO 2 ice was then placed in a lidded (135 mm x 95 mm x 110 mm) polystyrene box. 150 ml of previously chilled (-40° C) aqueous ammonia solution (Sigma-Aldrich, Cat. # 32, 014-5) was added, and the mix was shaken until the ammonia started to freeze, creating a well-mixed solid target in the box. The box was then …

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تاریخ انتشار 2016