Abundances of light hydrocarbons (methane to pentane) adsorbed and occluded in sandstones within the Salt Wash Member, Late Jurassic Morrison Formation were determined and evaluated. Total concentrations of these hydrocarbons range from 10 to 1000 H-l/g. Chlorite-bearing sandstones contain significantly more methane, ethane, and propane than sandstones containing kaolinite. The lower hydrocarbon abundances of kaolinite-bearing rocks are probably related to alteration of chlorite and dissolution of carbonate minerals. Among chlorite-containing samples, gray sandstones have twice the abundance of hydrocarbons as red sandstones. No systematic variations in hydrocarbon content were detected near uranium-vanadium deposits, or near faults, which were conduits for solutions from depth. The proportions of hydrocarbon gases 83 percent methane, 11 percent ethane, 4 percent propane and 2 percent other, are uniform among samples and indicate a homogeneous gas source. Ethane and propane suggest a thermogenic origin of the gas, which probably originated in the Pennsylvanian Hermosa Formation. Interpretation of the results was limited by the lack of understanding on where and how hydrocarbons are retained in sandstones. Abundances of hydrocarbons in Salt Wash sandstones are apparently independent of the abundances of aluminum (clays) and carbonate minerals. To properly interpret results of this and similar studies, the mechanisms of occlusion, adsorption, and preservation must be better known.