[meteorite-list] NASA, Planetary Scientists Find Meteoritic Evidence of Mars Water Reservoir

From: Galactic Stone & Ironworks <meteoritemike_at_meteoritecentral.com>
Date: Thu, 18 Dec 2014 18:50:32 -0500
Message-ID: <CAKBPJW_sm+cb_p7-rGwY33phEdiNTABZ+jS7euRJV3uY63asYA_at_mail.gmail.com>

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
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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
>
> ______________________________________________
>
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Received on Thu 18 Dec 2014 06:50:32 PM PST


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