This report presented to the 7th International Conference on Mars suggests they *might* have seen one of the more common south polar geysers actively venting:<br /><br />HiRISE Views of the Sublimation of Mars’ Southern Seasonal CO2 Cap. <br />C. J. Hansen1 , C. Okubo2, A. McEwen 2, Shane Byrne3, E. DeJong1, K. Herkenhoff3, M. Mellon4, P. Russell5, and N. Thomas5, 1Jet Propulsion Lab, Pasadena, CA 91101, 2University of Arizona, Department of Planetary Sciences, Tucson, AZ 85721, 3USGS, 2255 <br />N. Gemini Dr., Flagstaff, AZ 86001, 4University of Colorado, Boulder, CO, 5Physikalisches Institut, Universitaet Bern, Schweiz. <br />Seventh International Conference on Mars 3364.pdf <br />
http://www.lpi.usra.edu/meetings/7thmars2007/pdf/3364.pdf<br /><br />From the report:<br /><br />"Our approach was to attempt to detect dust <br />plumes by acquiring stereo images separated by a very <br />short time interval. Near the pole the orbit groundtracks <br />are closely spaced allowing us to image a given <br />location with just one orbit (~2 hour) separation. Any <br />geyser-like activity should be detectable in stereo images <br />as a plume rising above the surface. The hypothesis <br />that every spot is a site of gas jets [3,4] implies <br />that the probability of catching a geyser in action <br />is very high." <br />HiRISE Views of the Sublimation of Mars’ Southern Seasonal CO2 Cap, p. 1.<br /><br />"At one location in the Manhattan Island region, using <br />our stereo imaging technique, we may have captured <br />a geyser in the process of eruption. It is a tenuous <br />detection at best, very near the limits of the camera <br />capability. The putative plume is not high above the <br />surface (< 10m high) and is optically very thin. In <br />stereo small bumps on the surface can be observed that <br />may be the site of other gas jets. Figure 5 shows the <br />bumps and small fans that may be the in <div class="Discussion_UserSignature"> </div>