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<p><strong><font size="2">We often hear of the Roof of the World with Mount Everest @ 8,848 metres / 29,035 feet.<br /><br />What about the Roof of Mars at 27,000 metres / 88,580 feet.<br /><br />Recently the MRO HiRISE imaged the tallest point of the mountain, the South to South West portion of the summit caldera rim. This was one of the pool of ideas I submitted with the Phobos & Deimos observations in the HiRISE pointing suggestions.<br /><br /></font></strong><strong><font size="2" color="#000080">Link here to HiRISE release</font></strong><strong><font size="2">.<br /><br />The reasons being:<br /><br />1). There is a lot less dust at this altitude, as the atmospheric density is only 0.5 of 1 Millibar (approx 1 / 2,000 of the Earth's atmosphere at Sea Level) & winds here will have very little force.<br /><br />2). As above, but very, very little erosion.<br /><br />3). The cratering record will be better preserved, helping to date the age of this part of the gigantic volcano.<br /><br />4), The CRISM instrument should be able to determine the nature of the volcanic rock more accurately due to very little dust here.<br /><br />5). There may be clues as to the changing environment at this altitude above Mars (i.e was the atmosphere once denser even this high up)?<br /><br />What is obvious, is the layering exposed here, that makes up the huge volcano, just like the shields on Earth, thin layers, one on top of the other, on top of another, etc. The lava would have been similar to that in Hawaii.<br /><br />South west caldera wall including the very highest point on Mars.</font></strong><br /><img src="http://sitelife.space.com/ver1.0/Content/images/store/5/4/f5a272ae-e00c-430f-940d-03b89e6dcb54.Medium.jpg" alt="" /></p><p><font size="2" color="#000000"><strong>Close up of Lava Flows on the Roof of Mars.</strong></font><br /><img src="http://sitelife.space.com/ver1.0/Content/images/store/10/4/3a93e2b5-b7da-42a4-943d-c99f0a2f72a6.Medium.jpg" alt="" /></p><p><strong><font size="2" color="#000000">The large images are on the MRO HiRISE release.</font></strong><br /><br /><strong><font size="2">Andrew Brown.</font></strong></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><font size="1" color="#000080">http://www.launchphotography.com/</font><br /><br /><font size="1" color="#000080">http://anthmartian.googlepages.com/thisislandearth</font></p><p><font size="1" color="#000080">http://web.me.com/meridianijournal</font></p> </div>