@rosborne979,
Most of the following is speculation, and by scientists, not just by me. It is thought that there is a great deal of water in or under the regolith beneath the surface. It is believed (and not yet probed) that many of the channels that Schiaparelli first mapped may have been glacial in origin. It is believed that large aquifers may exist in many places on Mars (this latter is a part of the effort to explain where the Oceanus Borealis went).
Now, for my own part: Might not there be a dynamic cycle in which different forms of bacteria, or some kinds of symbiotes are active on the surface in austral summer? On both Earth and Mars, the southern hemispheres are the homes of extremes. When it is winter in the southern hemispheres, the planets are at aphelion (farthest from the sun) and therefore far colder than winters in the northern hemispheres. When it is summer in the southern hemispheres, the planets are at perihelion (nearest the sun) and far warmer than summers in the northern hemispheres. This could be crucial on Mars. The mean temperature seems to be about 230 K. (On Earth, that would be about minus 45 centigrade, but with Mars' near lack of an atmosphere, it's about -80 or -90 centigrade) However, in summer on Mars temperatures might reach 20 centigrade (about 70 F). The Martian year is about 22 terrestrial months, so summer lasts longer there than it does here. Right now, it's early spring on Mars. Curiosity may soon be able to tell us what kind of temperatures we will see in Gale Crater in summer time.
So-o . . . perhaps there might be a complex life cycle which takes advantage of a long "hot" summer (by Martian standards) and which lies dormant during the long, severe winter.
That's my story and i'm sticking to it.