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<jats:title>Abstract</jats:title> <jats:p>The absence of abundant organics on the Martian surface is a much discussed observation. So far, no explanation is completely satisfactory. In this study we aim for a deeper understanding of the degradation processes of organics in the presence of perchlorates that can take place on the Martian surface. Our primary goal is to study the radiation-induced decomposition process of glycine (H<jats:sub>2</jats:sub>NCH<jats:sub>2</jats:sub>COOH) in the absence and presence of an oxidizer relevant to the Martian surface—perchlorate anions <jats:inline-formula> <jats:tex-math> <?CDATA $({{\mathrm{ClO}}_{4}}^{-})$?> </jats:tex-math> <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:mo stretchy="false">(</mml:mo> <mml:msup> <mml:mrow> <mml:msub> <mml:mrow> <mml:mi>ClO</mml:mi> </mml:mrow> <mml:mrow> <mml:mn>4</mml:mn> </mml:mrow> </mml:msub> </mml:mrow> <mml:mrow> <mml:mo>−</mml:mo> </mml:mrow> </mml:msup> <mml:mo stretchy="false">)</mml:mo> </mml:math> <jats:inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="apjaa554aieqn1.gif" xlink:type="simple" /> </jats:inline-formula>. Glycine and various samples of glycine-1-<jats:sup>13</jats:sup>C (<jats:sup>+</jats:sup>H<jats:sub>3</jats:sub>NC<jats:inline-formula> <jats:tex-math> <?CDATA ${{{\rm{H}}}_{2}}^{13}$?> </jats:tex-math> <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:msup> <mml:mrow> <mml:msub> <mml:mrow> <mml:mi mathvariant="normal">H</mml:mi> </mml:mrow> <mml:mrow> <mml:mn>2</mml:mn> </mml:mrow> </mml:msub> </mml:mrow> <mml:mrow> <mml:mn>13</mml:mn> </mml:mrow> </mml:msup> </mml:math> <jats:inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="apjaa554aieqn2.gif" xlink:type="simple" /> </jats:inline-formula>COO<jats:sup>−</jats:sup>)–magnesium perchlorate hexahydrate (Mg(ClO<jats:sub>4</jats:sub>)<jats:sub>2</jats:sub> · 6H<jats:sub>2</jats:sub>O) were exposed to energetic electrons mimicking secondary electrons originating from the interaction of galactic cosmic rays (GCRs) with the Martian regolith. Using isotope-labeled and deuterated pure glycine samples such as glycine-1-<jats:sup>13</jats:sup>C, glycine-d<jats:sub>5</jats:sub> (<jats:sup>+</jats:sup>D<jats:sub>3</jats:sub>NCD<jats:sub>2</jats:sub>COO<jats:sup>−</jats:sup>), glycine-N,N,N-d<jats:sub>3</jats:sub> (<jats:sup>+</jats:sup>D<jats:sub>3</jats:sub>NCH<jats:sub>2</jats:sub>COO<jats:sup>−</jats:sup>), and glycine-2,2-d<jats:sub>2</jats:sub> (<jats:sup>+</jats:sup>H<jats:sub>3</jats:sub>NCD<jats:sub>2</jats:sub>COO<jats:sup>−</jats:sup>), we can conclude that decarboxylation (carbon dioxide loss) of the glycine molecule is exclusively the first decay step during irradiation regardless of whether perchlorate anions are present or not. In pure glycine samples, the decarboxylation co-product methylamine (CH<jats:sub>3</jats:sub>NH<jats:sub>2</jats:sub>) and its radiolytic decay product ammonia could both be detected explicitly for the first time. In the presence of perchlorates, (partial) oxidation of the glycine decarboxylation product CH<jats:sub>3</jats:sub>NH<jats:sub>2</jats:sub> may occur. Because the decarboxylation is an equilibrium reaction and the CH<jats:sub>3</jats:sub>NH<jats:sub>2</jats:sub> is effectively removed from the system by this oxidation, glycine cannot be recycled. Therefore the depletion of the CH<jats:sub>3</jats:sub>NH<jats:sub>2</jats:sub> facilitates the process, resulting in an overall 10-fold increase in the formation rate of carbon dioxide and its elevated concentrations in the perchlorate-containing irradiated samples.</jats:p>