Abstract
Formation of amino acids in interstellar space was experimentally examined. A mixture of CO (or CH3OH), NH3 and H2O was irradiated with high energy particles or g-rays. A wide variety of amino acids were detected in the products after acid-hydrolysis. It was suggested that complex precursors of amino acids can be formed in interstellar dusts. When the amino acid precursors were irradiated with circular polarized UV from a synchrotron, enantiomeric excess of alanine was observed in the hydrolysate of the product.