<p><BR/>Replying to:<BR/><DIV CLASS='Discussion_PostQuote'><font color="#ff0000">Ah I didn't know the GRS and they MDIS were basically kept online, thanks! So this pass tomorrow will confirm or deny that Mercury has a dual core layering? Slammin! Yea I'm with ya'll in good excitement on MESSNGERs magnometric and spectrographic sciences, unfortunately I'm trying to balance reading with studying naval architecture and electrical machinery for my classes heh
Got another question, this pertaining to the GRNS. How does it gather data on wether Mercury has ice at its poles? The ice (if there) almost never receives direct sunlight? So do they figure there is some reflection of cosmic rays from the surface, against the atmosphere, to the poles, and back out again? Or do they figure theres a fair amount of radioactive material up their that will emit neutrons at a slower rate (based on be colder I figure) than somewhere else? <br /> Posted by neuvik</font></DIV></p><p><strong><font size="2">Hi again neuvik,</font></strong></p><p><strong><font size="2">Yes the existance of Mercury's double layered core will be settled once & for all with tomorrow's encounter. Certainly Mercury has a massive core, that is beyond any doubt, but what is open to question is, is it double layered like Earth & Ganymede or is is singular like Venus, Mars or the Moon? We'll know on Tuesday once all of the data is downloaded.</font></strong></p><p><font size="2"><strong>I am no expert on this, but the existence of ice in polar shadowed craters, is based on hydrogen concentrations above the cold traps. Despite Mercury being the closest major object to the Sun, the permanently shadowed craters could be as cold as -235 C, or about the same as Neptune's moon Triton. Mercury is a world of oxymorons, equatorial early afternoon temps reach approx +427 C (not far short of Venus), the same spot at dawn, -186 C (similar to Saturn's moons).</strong></font></p><p><font size="2"><strong>So my guess is that the GRNS will measure the concentration & motion of cold hydrogen over the poles. Cosmic Rays are indeed though to splutter the cryonic ice, the vapour rises into the sunlight where the Oxygen & Hydrogen are seperated. Oxygen being heavier & Mercury having quite a considerable surface gravity (37.7 % of Earth, more or less equal to Mars's 37.8% g) either travels more slowly or descends into the cold trap.</strong></font></p><p><font size="2"><strong>Yes I found two navigation images of Sirius & the Pleiades. Not easy but have all of MESSENGERs raw images directories bookmarked.</strong></font></p><p><font size="3">
Sirius / Alpha Canis Majoris & Pleiades imaged by MESSENGER. </font><br /> <img src="http://sitelife.space.com/ver1.0/Content/images/store/15/1/3fa7e9b9-28f6-421b-915b-87c0ea59b8c8.Medium.jpg" alt="" /><br /> </p><strong><font size="2">Countdown to 2nd closest approach: Monday 6th October 2008. <br /><br />0 Day. <br />14 Hours. <br />15 Minutes. <br />43 Seconds.</font></strong><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>
<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>