[meteorite-list] Wanted: Meteorites from Mercury
From: Stuart McDaniel <actionshooting_at_meteoritecentral.com>
Date: Sun, 8 Jan 2012 15:51:12 -0500 Message-ID: <CF2286A067C140869B28C5B5309BC656_at_StuartMcDaniel> That is what was mentioned in the article. Stuart McDaniel Lawndale, NC Secr., Cleve. Co. Astronomical Society IMCA #9052 http://spacerocks.weebly.com -----Original Message----- From: Pete Pete Sent: Sunday, January 08, 2012 3:12 PM To: baalke at zagami.jpl.nasa.gov ; meteoritelist meteoritelist Subject: Re: [meteorite-list] Wanted: Meteorites from Mercury Hi, All, I know there's been only scattered remarks about the Messenger mission, but is the current consensus that angrites do not originate from Mercury? Best, Pete > From: baalke at zagami.jpl.nasa.gov > To: meteorite-list at meteoritecentral.com > Date: Fri, 6 Jan 2012 10:20:11 -0800 > Subject: [meteorite-list] Wanted: Meteorites from Mercury > > > http://www.skyandtelescope.com/news/Wanted-Meteorites-from-Mercury-136803313.html > > Wanted: Meteorites from Mercury > By Kelly Beatty > Sky & Telescope > January 6, 2012 > > During a recent science conference discussing Messenger's results from > Mercury, investigator Shoshana Weider (Carnegie Institution of > Washington) commented, "Short of landing on the surface, picking up a > rock, and bringing it home, the instruments on Messenger that > characterize chemistry are the best we're going to get." > > Well, Shoshana, you might still get to hold such a rock someday. > > According to a 2008 analysis > <http://arxiv.org/ftp/arxiv/papers/0801/0801.4038.pdf> by Brett Gladman > and Jaime Coffey (University of British Columbia), chunks of Mercury > should be lying somewhere on Earth right now. The dynamicists conclude > that 2% to 5% of the debris blasted by impacts off the surface of > Mercury at or above escape velocity (2.6 miles per second) should reach > Earth within 30 million years. > > Their numbers suggest that Mercurian meteorites should be roughly one > third as common as those from Mars, for which the count now stands at 60. > Gladman conservatively suggests that at least a half dozen stones should > be > lying around somewhere on terra firma. > > Meteorite collectors would value a Mercurian meteorite above all others, > likely fetching $5,000 or more per gram, so they've been on the lookout > for one. A few years ago, prior to Messenger's arrival, meteoriticists > had speculated that the best existing match to Mercury were a rare > handful of ancient, basalt-rich stones known as angrites > <http://research.jsc.nasa.gov/PDF/Ares-1.pdf>. > > But even before Messenger's arrival, ground-based astronomers had > concluded that Mercurian surface rocks contained very little iron - > strange indeed, given that the innermost planet has an iron core that > takes up 80% of its diameter and more than half of its volume! > > "At that time," comments geochemist David Blewett (Applied Physics > Laboratory), "people were expecting Mercury to have a composition more > like a lower-iron version of the lunar highlands. We now know that it's > much different than that." After nearly a yearly scrutinizing the planet > from orbit, Messenger has confirmed that iron is in short supply at the > surface. > > Instead, the compositional clues suggest that a Mercurian meteorite would > be an igneous rock - or perhaps a fused breccia of different rock types - > rich in magnesium and volatile elements (especially sulfur and potassium). > This closely matches the composition of another rare meteorite group, > the aubrites. Also known as enstatite achondrites, aubrites are igneous > rocks dominated by the iron-free mineral enstatite (Mg_2 Si_2 O_6 ). > > But aubrites aren't from the innermost planet. For one thing, they're > too reflective - anything coming from Mercury would be much darker, > tinted by some yet-to-be-identified compound that's seen widely > <http://photojournal.jpl.nasa.gov/catalog/PIA14492> in Messenger's > images. It might also smell faintly of sulfur, appear heavily shocked, > exhibit significant exposure to cosmic rays, and might even be slightly > magnetic. Such characteristics would certainly have come to the > attention of hunters and collectors, and it's safe to say that none of > the world's 40,000 well-documented meteorites are from Mercury. > > Yet dynamical probabilities argue otherwise, so why haven't such samples > been found? Gladman and Coffey didn't address how chunks of rock might > get blasted off the Mercurian surface, only that the high collision > velocities of asteroids and comets should make it easy to do so. > > Maybe the launch mechanics aren't understood well enough, suggests Jay > Melosh, an impact specialist at Purdue University. "Perhaps at the very > high speeds required for direct transfer, the fragments are simply too > small," he says. "These ejecta have to be launched from the surface > very close to the impact point - and perhaps our current models do not > give very good results here." However, Messenger finds that big impacts > on Mercury are accompanied by clusters of secondary pits, created by > tossed-out debris, that are generally much larger - not smaller - than > those around comparable lunar craters. "This fact is one of the current > big puzzles about the Mercurian cratering record," Melosh concedes. > > And so the search goes on for what will almost certainly be the most > celebrated meteorite discovery since the finding of stones blasted from > surfaces of the Moon and Mars a few decades ago. > > ______________________________________________ > HAPPY HOLIDAYS!! > Visit the Archives at > http://www.meteoritecentral.com/mailing-list-archives.html > Meteorite-list mailing list > Meteorite-list at meteoritecentral.com > http://six.pairlist.net/mailman/listinfo/meteorite-list ______________________________________________ HAPPY HOLIDAYS!! Visit the Archives at http://www.meteoritecentral.com/mailing-list-archives.html Meteorite-list mailing list Meteorite-list at meteoritecentral.com http://six.pairlist.net/mailman/listinfo/meteorite-list Received on Sun 08 Jan 2012 03:51:12 PM PST |
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