<[Does] anyone know how deep these holes would need to be for the atmospheric pressure to be high enough for water to exist in it's liquid state.><br /><br />I've looked at the water question and it's a little complicated. (The information I've compiled is a purely amateur effort, so keep that in mind.) <br /><br />Liquid water depends on a combination of temperature and pressure. And temperature and pressure on Mars varies radically depending on season, altitude, and time of day. Then there is the variation of how saline the water is. Brines can have a significantly lower freezing temperature than pure water.<br /><br />The 'skylights' are located in a volcanic region of Mars which has higher than average elevation, so therefore lower pressure and lower temperature. Two strikes right off the bat.<br /><br />A better place to look for liquid water is at the greatest depths of Mars, such as the Hellas basin which is in the southern hemisphere. Pressure is 1/3 higher than average because of the great depth of Hellas which is lower than 6 km below the average altitude.<br /><br />But you also want to look during the right time of year too. Because of the eccentricity of the Martian orbit, the southern hemisphere has colder winters and hotter summers than the northern hemisphere. So much so that during the southern winter, a good chunk of the Martian atmosphere condenses out and adds to the size of the southern icecap. During the southern summer, the southern icecap partly evaporates and increases the pressure of the martian atmosphere by as much as 1/3!<br /><br />But the final problem of liquid water on Mars is the most vexing. Even if liquid water forms on the surface, the martian atmosphere is so dry that liquid water would evaporate fairly quickly. Some experiments show that evaporation in cold still air is much slower, but evaporation is still a problem.<br /><br />Unless continually fed, perhaps by some underground spring, any occurance of liquid water on th