“…Among these are FTT reactions; ion-molecule and radical-radical reactions; γ-, proton-and UV-irradiation; Strecker's type reactions involving aqueous processing of simple molecules such as H 2 O, HCN, H 2 CO and NH 3 ; internal heating of the parent body produced by the radioactive decay of short-lived nuclides. Although quite significant amounts of glycine are detected in the Murchison meteorite, no ascertained interstellar glycine has yet been identified since its first observational report in 1979 [47] suggesting that molecules formed in the interstellar medium, ISM, underwent further processing. It has been suggested that the primary products from proton irradiation of a mixture of CO, N 2 /NH 3 , H 2 O are amino acid precursors, molecules that provide amino acids after acid hydrolysis [36,38].…”