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Cross sections for photoabsorption of HCl and DCl are determined in the spectral region of 135-232 nm using radiation from a synchrotron light source. At wavelengths near the onset of absorption ( nm), cross l 1 200 sections of HCl are approximately 5-10 times larger than those of DCl. These data are used to calculate rates of photodissociation of HCl and DCl in the Venusian atmosphere. For the entire wavelength region measured, the rate of photodissociation of DCl is only 16% that of HCl. The difference in rates of photodissociation contributes to the exceptionally large (D)/(H) ratio of the Venusian atmosphere. Subject headings: planets and satellites: individual (Venus) — ultraviolet: solar system

Absorption Cross Sections of HC[CLC]l[/CLC] and DC[CLC]l[/CLC] at 135–232 Nanometers: Implications for Photodissociation on Venus