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Fwd = Sedimentary Rocks On Mars May Suggest An Ancient Land Of Lakes

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  • Frits Westra
    Forwarded by: fwestra@hetnet.nl Originally from: baalke@jpl.nasa.gov Original Subject: Sedimentary Rocks On Mars May Suggest An Ancient Land Of Lakes
    Message 1 of 1 , Dec 4, 2000
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      Forwarded by: fwestra@...
      Originally from: baalke@...
      Original Subject: Sedimentary Rocks On Mars May Suggest An Ancient Land Of Lakes
      Original Date: Mon, 4 Dec 2000 09:56:04 -0800 (PST)

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      American Association for the Advancement of Science

      Contact:
      Ginger Pinholster, gpinhols@..., 202-326-6421

      FOR IMMEDIATE RELEASE: 4 DECEMBER 2000

      NOTE: THE EMBARGO TIME FOR THIS RELEASE HAS BEEN CHANGED SINCE IT WAS
      ORGINALLY POSTED. ALL OTHER EMBARGOES FOR THE 8 DECEMBER 2000 ISSUE
      OF SCIENCE REMAIN IN EFFECT.

      * For a version of this release with graphics, please click here,
      http://www.eurekalert.org/E-lert/current/public_releases/scipak/malin.html

      * Images for this release can be found here,
      http://www.eurekalert.org/E-lert/current/public_releases/scipak/malinimages.
      html

      * This news release is also available in French
      [http://www.eurekalert.org/releases/aaas-french-srs120100.html%5d
      and German [http://www.eurekalert.org/releases/aaas-german-srs120100.html%5d.

      Science report: sedimentary rocks on Mars may suggest an ancient land of
      lakes

      8 December 2000 -- Layered geologic outcrops on Mars, described in today's
      issue of the journal Science -- may be composed of sedimentary rock that
      dates from the earliest span of martian history, between 4.3. and 3.5 billion
      years ago.

      Images of these sedimentary rock exposures, captured by the Mars Orbiter
      Camera (MOC), suggest that parts of ancient Mars may have resembled a
      land of lakes, and that the geology of early Mars was much more dynamic
      than previously suspected.

      If life existed on Mars during this time period, researchers believe that the
      fossil remnants of that past life may be sandwiched within the sedimentary
      rock layers, just as they are on Earth.

      The martian outcrops, in some cases a few kilometers thick, appear to be
      made of fine-grained materials deposited in horizontal layers, the hallmark
      of sedimentary rock. These outcrops are found inside craters, between
      craters, and within chasms, said Michael C. Malin and Kenneth S. Edgett of
      Malin Space Science Systems in San Diego, California.

      The Science researchers identified three main outcrop types from the MOC
      images: layered units, massive units, and thin mesa units.

      Layered units, as their name suggests, consist of relatively thin rock beds --
      some only a few meters thick -- stacked on top of one another in distinct
      groups. Massive units appear as one bulky rock layer with no clearly defined
      horizontal bedding. In a few cases, these types appear together, with the
      massive unit always perched on top of the bedded unit like a thick, indistinct
      coat of frosting on a layer cake.

      Thin mesa units, with surfaces ranging from smooth to pitted to ridged and
      grooved, are almost always found on top of eroded massive or layered
      sedimentary rock.

      While sediments can be deposited in a variety of ways -- including wind,
      water, volcanic activity, and even cosmic impact -- the prevalence of the
      martian sedimentary outcrops within basin-like features suggests that they
      were deposited by water, perhaps in lakes that formed within the craters
      and chasms, said Malin and Edgett.

      Under this scenario, sediments may have been transported into the lakes in
      regular, swift pulses, building up thin layer units. Massive units may have
      been deposited when the lake became stagnant or deep enough to cause
      sediments to sift down through the water over longer intervals.

      "Some of the MOC images of these outcrops show hundreds and hundreds
      of identically thick layers, which is almost impossible to have without
      water," said Malin.

      The sedimentary units show no telltale signs of wind deposition, and the
      researchers concluded that explosive volcanic eruptions and impact
      cratering probably could not have produced enough sediment to create
      the large-scale and geographically widespread outcrops seen on the
      martian surface.

      Although Malin and Edgett favor water as the sedimentary suspect, they
      also offer an alternative model that involves changes in atmospheric
      pressure on early Mars. They suggest that periods of relatively high
      atmospheric pressure -- caused by fluctuations in the amount of solid
      carbon dioxide on the planet's surface -- could have increased the
      atmosphere's ability to carry dust produced by heavy cratering.

      To confuse matters, the Science researchers don't know where the original
      sediments came from, or how they were transported to their final resting
      places, since there are no traces of gullies or streams or other channels
      associated with the outcrops. They think that erosion may have wiped out
      both the source of the sediments and their travel routes.

      In some cases, sedimentary rock has eroded out of the crater in which it
      formed, also vanishing without a geologic clue.

      To Malin, the history of martian geology looks like a jigsaw puzzle.

      "In the center of the puzzle, we have these layered rocks, which are good
      evidence of an extremely dynamic environment. On either side of this
      well-developed puzzle piece, we have mysteries."

      In any case, Mars' sedimentary rocks suggest a very active early history
      for the planet.

      "This makes Mars more complicated and more exciting. This record is going
      to tell us a lot about what early Mars was like, and maybe the early Earth
      as well, since we don't have a lot of rocks on our own planet from this time
      period," said Edgett.

      ###

      This research was supported by the National Aeronautics and Space
      Administration through Contract No. 959060 from the Jet Propulsion
      Laboratory.



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