Modeling studies of Martian dust storms have generally focused on simulating storms in the solstice season due to the expectation that dust is most efficiently lifted and distributed by the Hadley circulation which is most intense in this time. However, the observational record indicates that most years are characterized by pre-and post-solstice regional dust lifting. Moreover, in some years (1977, 1982, and, most notably, 2001) major dust storms occurred well before the solstice, suggesting that the Hadley circulation may not necessarily play the dominant role in dust storm development. It is suggested here that the thermal tides may play a more prominent role in the dust cycle than is often assumed. Results from a simulation of a representative Mars year are used to illustrate and explore aspects of the thermal tides of relevance to the dust cycle.