<p><BR/>Replying to:<BR/><DIV CLASS='Discussion_PostQuote'><font color="#ff0000">Wasn't there recently an article posted on space.com which claimed evidence had been found that there may still have been rainy/mist on Mars as recent as a few hundred million years ago? I could be wrong, but I'm SURE I read that.Not that a little rain/mist would make the planet earthlike, since I believe the article stated the water was still not stable on the surface, just that the atmosphere was enough denser for rains. <br />Posted by baulten</font></DIV></p><p><font size="2"><strong>Hi baulten,</strong></font> </p><p><font size="2"><strong>I remeber something about that also. Not sure if it was rain, or subsurface water erupting in flash flooding events, subsurface ice being melted during impact events. </strong></font></p><p><font size="2"><strong>I think Jon is correct though, the Mars we see today is not a lot different to the one of 1 GYA or even 2 GYA, but there appear to have been shortlived water revivals in the meantime.</strong></font> </p><p><font size="2"><strong>This brings me to something I was trying to figure a while back, with Mars Pathfinder & the evidence that Mars Pathfinder provided about flash flooding through Ares Vallis. Was it a one off, or did it occur over several episodes?</strong></font></p><p><font size="2"><strong>The fact that many boulders, some quite large were leaning in the same direction, seemed to suggest a major one off event would have been enough. However MarsPathfinder also found evidence of stacked rocks, rocks pitted & with corners rounded, also ponding, one of which the little Soj</strong></font> <font size="2"><strong>ourner Rover examined, seemed to suggust that there were also less energetic flooding events & that the area at times may have been inundated for long enough to allow ponding & conglomerates to form.</strong></font></p><p><strong><font size="2">Below, Half Dome as seen by Sojourner. Did a flash flood once push against this flat face on the boulder?</font></strong> <br />#<img src="http://sitelife.space.com/ver1.0/Content/images/store/2/10/22d59978-1ce6-4c91-aa73-d2ab22e8a153.Medium.jpg" alt="" /><br /> </p><p><font size="2"><strong>View from Mars Pathfinder in Ares Vallis clearly showing many rocks & boulders aligned in the same direction. Evidence of massive flash flooding. </strong></font></p><p>#<img src="http://sitelife.space.com/ver1.0/Content/images/store/12/13/2c60c9e9-69fa-4f9f-8d56-7f9ca8d757a9.Medium.jpg" alt="" /></p><p><font size="2"><strong>Certainly Viking 1 in Chryse Planitia some 800 KM to the NW also imaged ponding & some stacked but much smaller rocks, but the Viking 1 site lacked the leaning boulders, the boulders there appear to be more random, less rock sorting & also generally lacked the rounded corners, suggesting to me at least, that the Viking 1 site experienced inundation but not the energe</strong></font> <font size="2"><strong>tic flooding events that Mars Pathfinder found evidence for.</strong></font></p><p><font size="2"><strong>Viking 1 view towards Big</strong></font> <font size="2"><strong> Joe boulder in Chryse Planitia. Note how the rocks appear to be sharper & </strong></font>#<font size="2"><strong>more haphazard than those in Ares Vallis.</strong></font><br /><img src="http://sitelife.space.com/ver1.0/Content/images/store/8/3/a8defe78-f98e-4712-b3ec-eacb52ddae1f.Medium.jpg" alt="" /> </p><p><font size="2"><strong>Below Viking 1 looking towards an impact crater in Chryse Planitia. A few rocks appear stacked, but are not aligned as at the Mars Pathfinder site some 800 KM to the S E. </strong></font></p><p><img src="http://sitelife.space.com/ver1.0/Content/images/store/15/15/1f3febc7-ee7d-4dc1-afd8-2faac7aca067.Medium.jpg" alt="" /> </p><p><font size="2"><strong>However both point to a much wetter & warmer Mars in the very remote past.</strong></font></p><p><font size="2"><strong>MER B Opportunity also with the confirmation of the Grey Hematite in large quantities & cross bedding of the layering, als</strong></font> <font size="2"><strong>o suggests long term inundation. MER A Spirit in the Columbia Hills withi</strong></font> <font size="2"><strong>n Gusev Crater, in the southern 'tropics' has found evidence of hydration through volcanism such as geysers, fumeroles. The basalt on the Gusev Crater floor though disappointed many scientists, hoping for lake beds, in fact for many others like myself was a huge boost in gathering data for the volcanic timescale & chemistry on the red planet (mind you I am a volcano head, so I would say that). </strong></font></p><p><font size="2"><strong>Below, MER B Opportunity, the bleak smoo</strong></font> <font size="2"><strong>th plains of Meridiani Planum. Was this a sea bed?</strong></font></p><p><img src="http://sitelife.space.com/ver1.0/Content/images/store/15/6/efb280b8-a0ed-4add-96f3-d0402f2261f2.Medium.jpg" alt="" /> <br /><font size="2"><strong><br />#Below. MER B Opportunity, layering in the Eagle Crater. Crossbedding & Hematite Rich 'blueberries abound.</strong></font><br /> <br /><img src="http://sitelife.space.com/ver1.0/Content/images/store/2/6/f2ea3b35-7f7b-4522-864c-d18b77022cf8.Medium.jpg" alt="" /> <img src="http://sitelife.space.com/ver1.0/Content/images/store/12/2/6cd6f3ce-ecd9-4890-b2ef-998061127c8d.Medium.jpg" alt="" /></p><p><font size="2"><strong>More recently Mars Phoenix Lander has shown ample evidence of long term hydration through the rock hard icy regolith beneath the first few CM of 'dry' regolith, not to men</strong></font><font size="2"><strong>tion the many polygons, sorted stones & the general smooth terrain clearly visible on the images. In some ways show some similarities with the Viking 2 site in Utopia Planitia, though Utopia is not as far north or gets as cold during the Winter, but the Phoenix site is not nearly as rocky as the landscape Viking 2 showed.</strong></font></p><p><font size="2"><strong>Below MER A Spirit, some of the volcanic rocks on the floor of Gusev Crater. </strong></font></p><p><img src="http://sitelife.space.com/ver1.0/Content/images/store/8/1/e8736b2d-282a-4516-81b1-8a2af667ff29.Medium.jpg" alt="" /></p><p><font size="2"><strong>MER A Spirit wheels uncovered hydrated sulphurous salts, perhaps even Epson Salts???</strong></font></p><p><img src="http://sitelife.space.com/ver1.0/Content/images/store/12/15/ac243d3d-37b5-44ba-afcb-e53ef18c3565.Medium.jpg" alt="" /></p><p><font size="2"><strong>Phoenix Mars Lander, views of Scandia Colles, Vastitas Borealis. Was this once a sea bed, before Mars lost most of its atmosphere?</strong></font><br /><img src="http://sitelife.space.com/ver1.0/Content/images/store/11/6/9bb137e7-c87e-4bda-86b2-cfd85f7dba3f.Medium.jpg" alt="" /> <img src="http://sitelife.space.com/ver1.0/Content/images/store/2/7/a285013a-5be6-404f-b714-7e3422e3bae1.Medium.jpg" alt="" /><br />#</p><p><font size="2"><strong>None though appear to show evidence of recent rain.</strong></font></p><p><font size="2"><strong>My strong point is with volcanic processes rather than hydration processes, but I think the gist of what I have said is correct. I am sure Jon Clark will correct anything I have gotten wrong. <br /></strong></font></p><p><font size="2"><strong>Andrew Brown. </strong></font></p> <div class="Discussion_UserSignature"> <p><font color="#000080">"I suddenly noticed an anomaly to the left of Io, just off the rim of that world. It was extremely large with respect to the overall size of Io and crescent shaped. It seemed unbelievable that something that big had not been visible before".</font> <em><strong><font color="#000000">Linda Morabito </font></strong><font color="#800000">on discovering that the Jupiter moon Io was volcanically active. Friday 9th March 1979.</font></em></p><p>
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