Crossed molecular beams experiments were utilized to explore the chemical reaction dynamics of groundstate cyano radicals, CN(X 2 Σ + ), with propylene (CH 3 CHCH 2 ) together with two d 3 -isotopologues (CD 3 CHCH 2 , CH 3 CDCD 2 ) as potential pathways to form organic nitriles under single collision conditions in the atmosphere of Saturn's moon Titan and in the interstellar medium. On the basis of the center-of-mass translational and angular distributions, the reaction dynamics were deduced to be indirect and commenced via an addition of the electrophilic cyano radical with its radical center to the R-carbon atom of the propylene molecule yielding a doublet radical intermediate: CH 3 CHCH 2 CN. Crossed beam experiments with propylene-1,1,2-d 3 (CH 3 CDCD 2 ) and propylene-3,3,3-d 3 (CD 3 CHCH 2 ) indicated that the reaction intermediates CH 3 CDCD 2 CN (from propylene-1,1,2-d 3 ) and CD 3 CHCH 2 CN (from propylene-3,3,3-d 3 ) eject both atomic hydrogen through tight exit transition states located about 40-50 kJmol -1 above the separated products: 3-butenenitrile [H 2 CCDCD 2 CN] (25%), and cis/trans-2-butenenitrile [CD 3 CHCHCN] (75%), respectively, plus atomic hydrogen. Applications of our results to the chemical processing of cold molecular clouds like TMC-1 and OMC-1 are also presented.