The widespread presence of perchlorate (ClO 4 − ) on Mars has significant implications for the alteration or destruction of indigenous organic compounds that may have been or still be present on Mars. The intermediary products of the UV-driven production of ClO 4 − include oxychlorines (ClO x ) such as chlorite (ClO 2 − ), chlorate (ClO 3 − ), and chlorine-dioxide (ClO 2 ) gas. The objective of this study was to start with ClO 2 − or ClO 3 − under Mars ambient and vary temperature, humidity, and UV wavelengths in order to isolate the reaction pathways leading to ClO 4 − . We also investigated the role of titanium dioxide (TiO 2 ) as a catalyst for these reactions. We show here that the production of ClO 4 − from ClO 2 − and ClO 3 − proceeds through different pathways. The ClO 2 − is rapidly converted to stable levels of ClO 3 − and Cl − , suggesting that the amount present on Mars will likely be very low compared to other ClO x . We also observed that temperature does not affect ClO 4 − production when starting with NaClO 2 but causes a decrease in ClO 4− production when starting with NaClO 3 , and production of ClO 4 − using UV > 300 nm with O 2 present does not involve an ozone (O 3 ) pathway. We have also shown that adding TiO 2 to the SiO 2 /ClO x mixture has a catalytic effect in the production of ClO 4 − under terrestrial conditions but shows primarily a shielding effect under Mars ambient; ClO 3 − is stable under Mars ambient even in the presence of TiO 2 and is not affected by temperature or humidity. Finally, it was shown that water is necessary for generation of ClO 2 (g) during perchlorate production from either NaClO 2 or NaClO 3 . This suggests that production of ClO 2 might be occurring on Mars in areas where ice can provide increased humidity levels.