<p><BR/>Replying to:<BR/><DIV CLASS='Discussion_PostQuote'><font color="#ff0000">It indeed looks relatively fresh... strange in fact as there is no wind or water erotion..Must have been a big rock, but older theories of moons that might have slammed into this planet now seem less likely as we see more and more of Mercury. <br /> Posted by efron_24<font color="#000000">[</font></font>/QUOTE]</p><p><strong><font size="2">Hi Chris,</font></strong></p><p><strong><font size="2">Yes indeed. That creater IS young on the hermeological time scale. Ejecta & the craters themselves over time darken as radiation & the surface regolith is slowly 'gardened ' by micrometeoroid impacts. </font></strong></p><p><strong><font size="2">With Mercury as Wayne said earlier, the actual cratering rate & I would also expect in conjunction with that, the micrometeoroid impact rate is poorly known, due to Mercury being on average only 0.34 AU from the gravity well of the the Solar System, namely the Sun. </font></strong></p><p><strong><font size="2">Also does solar energy this close in (currently on Mercury just over 11 KW per square metre or approx nine times that on Earth or the Moon), affect the micrometeoroid impact rate? Is it less on Mercury than the Moon, or Phobos, or 1 Ceres, etc? or could it be more due to the Sun's gravity, more than enough to counteract the radiation pressure?</font></strong></p><p><font size="2"><strong><font color="#000000">Wayne I would expect will know very much more than I do on this. We do know that particles can survive this close & even closer to the Sun than this due to the Geminid meteor stream left behind the now extinct comet that is now asteroid 3200 Pheathon. Once again, Wayne will know much more than I do on this.</font></strong></font></p><p><font size="2"><strong>Also I agree with you that there appears to be no evidence of impacted former moons of Mercury. We cannot discount that Mercury may have had small moons like Phobos, Deimos or Dactyl (the 1.5 KM wide moon of main belt Asteroid 243 Ida) at some time that could have impacted, but certainly no large ones. We have now seen enough of Mercury in sufficient detail now to rule that out. It was something I was looking for myself, as well as more volcanoes, though as yet, there have not been enough NAC frames released for me to study, but I think we can discount impacted former moons unless they were very small, certainly less than a few KM across. </strong></font></p><p>Replying to:<BR/><DIV CLASS='Discussion_PostQuote'><font color="#ff0000">If one would walk on Mercury with a good space suit ... what would one see of these white rays ?It will not be meters thick I think.. so no height differences in the terrain i suspectbut would it be powerly material that you can kick up with your shoes ?Can anyone take a quess what this would be like <br /> Posted by efron_24</font></DIV></p><p><font size="2"><strong>Yes I think you are spot on with this Chris. </strong></font></p><p><font size="2"><strong>The ejecta blanket close to the crater will be deep, certainly many metres in depth, maybe even a few hundred metres in depth. But further away, that depth will decrease as obviously less material will travel further. </strong></font></p><p><font size="2"><strong>Although those rays look impressive further away & dominating that side of Mercury, really they are very superficial, maybe for the most part, millimetres or even shallower than that. </strong></font></p><p><font size="2"><strong>An astronaut would certainly be able to kick it clear with space boots. I suspect at surface level, it may look like frost, looking not too unlike the frost that Phoenix has seen on Mars, except in this case, it will be rock dust (the daytime surface temperature of approx +420 C here & lack of atmosphere will not allow for frost, though at dawn even on the equator, the temperature is approx -186 C, similar to the moons of Saturn, but lack of atmosphere would IMO still rule out frost). For the most part except near the actual crater, there will be no elevation difference from the actual surface.</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>
<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>