[meteorite-list] Phoenix Analyzing Martian Soil Data

From: mexicodoug at aim.com <mexicodoug_at_meteoritecentral.com>
Date: Tue, 05 Aug 2008 01:54:09 -0400
Message-ID: <8CAC4D6D00A069B-7AC-2BF8_at_FWM-M42.sysops.aol.com>

NASA wrote:

"This is surprising since an earlier TEGA measurement of surface
materials was consistent with but not conclusive of the presence of
perchlorate," said Peter Smith"

Dear List ... this really sounds like wishful thinking, two holes in
one...though the flip side could be a poisoned planet...

Would be nice ...
(1) having enough the raw material to make perchlorate candles for the
generation of all the oxygen needed for colonization of the area, no
water or electroysis wasted to make breathable oxygen.
(2) burning the perchlorate and the principal result: Water. Iron
filings work (lots of iron on rusty Mars, and there are always
meteorites as a back-up.

Not to mention having most of the material needed to manufacture rocket
fuel in situ (just add the iron or better yet aluminum shavings) to get
the heck out when necessary. So all we need is confirmation of this at
a mineable level plus the upoming announcement (?) of clay to provide a
water reservior to complement this oxygen and H2O reservior and there'd
even be a back up source of water.

The challenge could be to detoxify the water of perchlorate and make it
safe - something that seems impossible on earth for regulators?

http://www.americanchemistry.com/s_chlorine/sec_content.asp?CID=1236&DID=4709&CTYPEID=113

http://en.wikipedia.org/wiki/Chemical_oxygen_generator#Oxygen_candle

Best wishes,
Doug




-----Original Message-----
From: Ron Baalke <baalke at zagami.jpl.nasa.gov>
To: Meteorite Mailing List <meteorite-list at meteoritecentral.com>
Sent: Mon, 4 Aug 2008 5:21 pm
Subject: [meteorite-list] Phoenix Analyzing Martian Soil Data




Aug. 4, 2008

Dwayne Brown
Headquarters, Washington
202-358-1726
dwayne.c.brown at nasa.gov

Guy Webster
Jet Propulsion Laboratory, Pasadena, Calif.
818-354-6278
guy.webster at jpl.nasa.gov

Sara Hammond
University of Arizona, Tucson
520-626-1974
shammond at lpl.arizona.edu

RELEASE: 08-199

NASA SPACECRAFT ANALYZING MARTIAN SOIL DATA

WASHINGTON -- Scientists are analyzing results from soil samples
delivered several weeks ago to science instruments on NASA's Phoenix
Mars Lander to understand the landing site's soil chemistry and
mineralogy.

Within the last month, two samples have been analyzed by the Wet
Chemistry Lab of the spacecraft's Microscopy, Electrochemistry, and
Conductivity Analyzer, or MECA, suggesting one of the soil
constituents may be perchlorate, a highly oxidizing substance. The
Phoenix team has been waiting for complementary results from the
Thermal and Evolved-Gas Analyzer, or TEGA, which also is capable of
detecting perchlorate. TEGA is a series of ovens and analyzers that
"sniff" vapors released from substances in a sample.

NASA will hold a media teleconference on Tuesday, Aug. 5, at 2 p.m.
EDT, to discuss these recent science activities. Participants will be
introduced at the start of the briefing. To participate in the
teleconference, reporters should contact Steve Cole on 202-358-0918
for dial-in and passcode information.

Confirmation of the presence of perchlorate and supporting data is
important prior to scientific peer review and subsequent public
announcements. The results from Sunday's TEGA experiment, which
analyzed a sample taken directly above the ice layer, found no
evidence of this compound.

"This is surprising since an earlier TEGA measurement of surface
materials was consistent with but not conclusive of the presence of
perchlorate," said Peter Smith, Phoenix's principal investigator at
the University of Arizona, Tucson.

Scientists at the Phoenix Science Operations Center at the University
of Arizona, Tucson, are specifically looking at the data from these
instruments to provide information on the composition of Martian
soil.

"We are committed to following a rigorous scientific process. While we
have not completed our process on these soil samples, we have very
interesting intermediate results," said Smith, "Initial MECA analyses
suggested Earth-like soil. Further analysis has revealed un-Earthlike
aspects of the soil chemistry."

The team also is working to totally exonerate any possibility of the
perchlorate readings being influenced by terrestrial sources which
may have migrated from the spacecraft, either into samples or into
the instrumentation.

"When surprising results are found, we want to review and assure our
extensive pre-launch contamination control processes covered this
potential," said Barry Goldstein, Phoenix project manager at NASA's
Jet Propulsion Laboratory in Pasadena, Calif.

Since landing on May 25, Phoenix has been studying Martian soil with
MECA's wet chemistry lab, two microscopes and a conductivity probe,
TEGA's ovens and two cameras.

MECA's robotic wet chemistry lab studies soluble chemicals in the soil
by mixing a soil sample with a water-based solution with several
reagents brought from Earth. The inner surface of each cell's beaker
has 26 sensors that give information about the acidity or alkalinity
and concentrations of elements such as chloride or perchlorate. The
beaker also can detect concentrations of magnesium, calcium and
potassium, which form salts that are soluble in water.

With continuing results and the spacecraft in good condition, the
mission has been extended through Sept. 30. The original prime
mission of three months ends in late August. The mission extension
adds five weeks to the 90 days of the prime mission.

The Phoenix mission is led by Smith at the University of Arizona with
project management at NASA's Jet Propulsion Laboratory in Pasadena,
Calif., and development partnership at Lockheed Martin in Denver.
International contributions come from the Canadian Space Agency; the
University of Neuchatel, Switzerland; the universities of Copenhagen
and Aarhus in Denmark; the Max Planck Institute in Germany; and the
Finnish Meteorological Institute. For information about Phoenix,
visit:

http://www.nasa.gov/phoenix


-end-

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Received on Tue 05 Aug 2008 01:54:09 AM PDT