[meteorite-list] NASA, Planetary Scientists Find Meteoritic Evidence of Mars Water Reservoir
From: Karen Ziegler <kziegler_at_meteoritecentral.com>
Date: Thu, 18 Dec 2014 23:54:06 +0000 Message-ID: <D0B8B6DD.2D7B6%kziegler_at_unm.edu> The actual 9full) paper is online. The meteorites are: LAR06, EETA79, Y98. Karen On 12/18/14 4:50 PM, "Meteorite Mailing List" <meteorite-list at meteoritecentral.com> wrote: >Hi Ron and List, > >Are these new findings based on the study of NWA 7034/pairings or Tissint >or ? > >It makes mention of shergottites and Martian meteorites, but the >abstract does not say which meteorite(s) was studied. > >Meteoritic evidence for a previously unrecognized hydrogen reservoir on >Mars >Tomohiro Usuia, b, , , Conel M. O'D. Alexanderc, Jianhua Wangc, Justin >I. Simond, John H. Jones > >Abstract : > >Fluvial landforms on Mars suggest that it was once warm enough to >maintain persistent liquid water on its surface. The transition to the >present cold and dry Mars is closely linked to the history of surface >water, yet the evolution of surficial water is poorly constrained. >Based on in situ hydrogen isotope (D/H) analyses of quenched and >impact glasses in Martian meteorites, we provide evidence for the >existence of a distinct but ubiquitous water/ice reservoir (D/H=?2?3 >times Earth's ocean water) that lasted from at least the time when the >meteorites crystallized (173?472 million years ago) to the time they >were ejected by impacts (0.7?3.3 million years ago), but possibly much >longer. The origin of this reservoir appears to predate the current >Martian atmospheric water (D/H=?5?6 times Earth's ocean water) and is >unlikely to be a simple mixture of atmospheric and primordial water >retained in the Martian mantle (D/H ? Earth's ocean water). This >reservoir could represent hydrated crust and/or ground ice interbedded >within sediments. Our results corroborate the hypothesis that a buried >cryosphere accounts for a large part of the initial water budget of >Mars. > >Best regards, > >MikeG >-- >------------------------------------------------------------- >Web - http://www.galactic-stone.com >Facebook - http://www.facebook.com/galacticstone >Twitter - http://twitter.com/galacticstone >Pinterest - http://pinterest.com/galacticstone >------------------------------------------------------------- > > > >On 12/18/14, Ron Baalke via Meteorite-list ><meteorite-list at meteoritecentral.com> wrote: >> >> >> December 18, 2014 >> >> NASA, Planetary Scientists Find Meteoritic Evidence of Mars Water >>Reservoir >> >> >> NASA and an international team of planetary scientists have found >>evidence >> in >> meteorites on Earth that indicates Mars has a distinct and global >>reservoir >> >> of water or ice near its surface. >> >> Though controversy still surrounds the origin, abundance and history of >> water >> on Mars, this discovery helps resolve the question of where the "missing >> Martian water" may have gone. Scientists continue to study the planet's >> historical record, trying to understand the apparent shift from an >>early wet >> >> and warm climate to today's dry and cool surface conditions. >> >> The reservoir's existence also may be a key to understanding climate >> history and the potential for life on Mars. The team's findings are >> reported in the journal Earth and Planetary Science Letters. >> >> "There have been hints of a third planetary water reservoir in previous >> studies of Martian meteorites, but our new data require the existence >>of a >> water or ice reservoir that also appears to have exchanged with a >>diverse >> set >> of Martian samples," said Tomohiro Usui of Tokyo Institute of >>Technology in >> >> Japan, lead author of the paper and a former NASA/Lunar and Planetary >> Institute postdoctoral fellow. "Until this study there was no direct >> evidence for this surface reservoir or interaction of it with rocks that >> have >> landed on Earth from the surface of Mars." >> >> Researchers from the Tokyo Institute of Technology, the Lunar and >>Planetary >> >> Institute in Houston, the Carnegie Institution for Science in >>Washington and >> >> NASA's Astromaterials Research and Exploration Science Division, >>located at >> >> the agency's Johnson Space Center in Houston, studied three Martian >> meteorites. >> >> The samples revealed water comprised of hydrogen atoms that have a >>ratio of >> >> isotopes distinct from that found in water in the Red Planet's mantle >>and >> current atmosphere. Isotopes are atoms of the same element with >>differing >> numbers of neutrons. >> >> While recent orbiter missions have confirmed the presence of subsurface >>ice, >> >> and melting ground-ice is believed to have formed some geomorphologic >> features on Mars, this study used meteorites of different ages to show >>that >> >> significant ground water-ice may have existed relatively intact over >>time. >> >> Researchers emphasize that the distinct hydrogen isotopic signature of >>the >> water reservoir must be of sufficient size that it has not reached >>isotopic >> >> equilibrium with the atmosphere. >> >> "The hydrogen isotopic composition of the current atmosphere could be >>fixed >> >> by a quasi-steady-state process that involves rapid loss of hydrogen to >> space >> and the sublimation from a widespread ice layer," said coauthor John >>Jones, >> >> a JSC experimental petrologist and member of NASA's Mars Curiosity rover >> team. >> >> Curiosity's observations in a lakebed, in an area called Mount Sharp, >> indicate Mars lost its water in a gradual process over a significant >>period >> >> of time. >> >> "In the absence of returned samples from Mars, this study emphasizes the >> importance of finding more Martian meteorites and continuing to study >>the >> ones we have with the ever-improving analytical techniques at our >> disposal," said co-author Conel Alexander, a cosmochemist at the >>Carnegie >> Institution for Science. >> >> In this investigation, scientists compared water, other volatile element >> concentrations and hydrogen isotopic compositions of glasses within the >> meteorites, which may have formed as the rocks erupted to the surface of >> Mars >> in ancient volcanic activity or by impact events that hit the Martian >> surface, knocking them off the planet. >> >> "We examined two possibilities, that the signature for the newly >>identified >> >> hydrogen reservoir either reflects near surface ice interbedded with >> sediment >> or that it reflects hydrated rock near the top of the Martian crust," >>said >> coauthor and JSC cosmochemist Justin Simon. "Both are possible, but the >> fact that the measurements with higher water concentrations appear >> uncorrelated with the concentrations of some of the other measured >>volatile >> >> elements, in particular chlorine, suggests the hydrogen reservoir likely >> existed as ice." >> >> The information being gathered about Mars from studies on Earth, and >>data >> being returned from a fleet of robotic spacecraft and rovers on and >>around >> the Red Planet, are paving the way for future human missions on a >>journey to >> >> Mars in the 2030s. >> >> These findings can be viewed online in their entirety at: >> >> http://go.nasa.gov/1zwSjTa >> >> For more about the ARES Division at JSC, visit: >> >> http://ares.jsc.nasa.gov >> >> Learn about NASA's Journey to Mars at: >> >> http://www.nasa.gov/content/nasas-journey-to-mars/ >> >> >> -end- >> >> Dwayne Brown >> Headquarters, Washington >> 202-358-1726 >> dwayne.c.brown at nasa.gov >> >> William Jeffs >> Johnson Space Center, Houston >> 281-483-5111 >> william.p.jeffs at nasa.gov >> >> ______________________________________________ >> >> Visit the Archives at http://www.meteorite-list-archives.com >> Meteorite-list mailing list >> Meteorite-list at meteoritecentral.com >> https://pairlist3.pair.net/mailman/listinfo/meteorite-list >> >______________________________________________ > >Visit the Archives at http://www.meteorite-list-archives.com >Meteorite-list mailing list >Meteorite-list at meteoritecentral.com >https://pairlist3.pair.net/mailman/listinfo/meteorite-list Received on Thu 18 Dec 2014 06:54:06 PM PST |
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