E
exoscientist
Guest
The news release from the AGU conference argues that the Mars "spider"<br />features at the south pole are due to gas release:<br /><br />HiRISE | Isolated Araneiform Topography (PSP_003087_0930).<br />http://hirise.lpl.arizona.edu/PSP_003087_0930<br /><br />Spring at the South Pole of Mars.<br />AGU Press Conference<br />C. J. Hansen, A. McEwen and the HiRISE Team.<br />December 2007<br />http://hirise.lpl.arizona.edu/pdf/agu_press_conf_dec07.pdf<br /><br />However, this report shows temperatures above 250K can be reached<br />seasonally even as far south as the Mars spiders:<br /><br />Astrobiology<br />Spiders: Water-Driven Erosive Structures in the Southern Hemisphere of<br />Mars.<br />Aug 2006, Vol. 6, No. 4: 651-667<br />http://www.liebertonline.com/doi/abs/10.1089/ast.2006.6.651 [abstract]<br /><br />This is within the temperature range of calcium chloride liquid water<br />brines.<br />Evidence for a liquid water origin is the dendritic pattern shown by<br />the spider "legs". On Earth this is taken for evidence of channels cut<br />by liquid water.<br />The news release argues that the channels are cut by gas because some<br />channels travel uphill. But of course water can also travel uphill for<br />short distances under pressure or simply because it is traveling<br />quickly as in a flood.<br /><br />A related possibility is that the origin of the spiders is due to the<br />transition of CO2-water clathrates to liquid water brines. This report<br />shows this could occur on heating and would result in explosive gas<br />release:<br /><br />PTX PHASE EQUILIBRIA IN THE H2O-CO2-SALT SYSTEM AT MARS NEAR-SURFACE<br />CONDITIONS.<br />R.J. Bodnar1, 1Fluids Research Laboratory, Department of Geological<br />Sciences, Virginia Tech, Blacksburg, VA 24061 e <div class="Discussion_UserSignature"> </div>