[meteorite-list] Murchison and S & T (Part 1 of 2)
From: Bernd Pauli HD <bernd.pauli_at_meteoritecentral.com>
Date: Thu Apr 22 10:06:56 2004 Message-ID: <3DA00598.F4B5612B_at_lehrer.uni-karlsruhe.de> Organic Clues in Carbonaceous Meteorites (April, 1979, Sky & Telescope, pp. 330-332) C.R. Pellegrino and J.A. Stoff, Rockville Centre, New York On September 28, 1969, an ancient rock mass slammed into the upper atmosphere somewhere above Australia. It slid, danced, and leaped through the air, then exploded over the town of Murchison. For several days thereafter residents and scientists recovered curious shards of grayish matter from fields, roadsides, and rooftops. The pieces resembled dried carbon-rich clay and crumbled with similar ease. Upon closer examination, their matrix appeared to be studded with tiny glasslike spheres. When these were sectioned and viewed under a microscope, concentric layers of material, not unlike those distinctive patterns recognized in pearls, became visible. Further analysis revealed unexpected traces of water (as high as 10 percent by weight) locked inside the stony fragments. The 20th specimen then known of that most puzzling and sought after of all meteorite types, the carbonaceous chondrite, had arrived. Nearly three years later, scientists at NASA's Ames Research Center in California confirmed the presence of 17 different fatty acids and 18 amino acids in fragments of the Murchison meteorite. These highly complex substances are composed of organic elements and, when woven properly together, comprise the foundations of cellular life. But one very important question soon arose: were these substances truly indigenous to the meteorite, or did the meteorite, upon its penetration into our atmosphere, begin to "breathe in" earthly contaminants? After all, a mere fingerprint on its surface would have contributed most of the common amino acids known here on Earth. During the three-year investigation that followed its arrival, the Murchison meteorite was examined and compared closely with another carbonaceous chondrite that had fallen near Murray, Kentucky, 19 years earlier. The results were impressively similar. Of the 18 amino acids detected in the two meteorites, the 12 most abundant are seldom if ever associated with the living tissues of terrestrial plants and animals. The remaining six (valine, alanine, glycine, proline, aspartic acid, and glutamic acid) are prominent in earthly proteins, but relatively scarce in carbonecous chondrites. The first of a long series of paradoxes had begun to emerge. The meteorites may have originated in an age when the "dust" of the solar nebula was falling together into little bodies that became celestial vacuum cleaners, ever increasing in girth as they continued to sweep up debris in their path. Some, like our own earth, accumulated great mass. Their interiors began to heat up. Gases, steam, and vaporized rock held fast to their shifting skin: the primordial atmospheres were born. Whether the result of a cataclysm involving the collision of ancient worlds or simply a collection of discarded planetary scraps left hanging about the sun, a thin belt of solar driftwood - the asteroids -spreads wide between Mars and Jupiter. It is from this belt that most meteorites seem to originate. The presence of organized elements and hydrocarbons in some of these meteorites leaves several unanswered questions. These substances seem to have no business being out there in the first place. If they are native to the meteorites, then we are faced with a perplexing fact: these carbon compounds were somehow lifted, against entropy, to a highly ordered state from vast numbers of random dissociated, inanimate atoms, and gathered up and arranged in their present condition of seemingly improbable symmetry. Given only the extreme temperatures, damaging radiation, and near emptiness of outer space, it is not likely that this kind of clustering could have proceeded in objects so small as stones, boulders, or even asteroids (nor that it should be reproduced so agreeably among individual samples). Detailed comparisons with earthly tissues seem only to sharpen the contrasts between terrestrial proteins and the kinds of molecular ornamentation typically recovered from carbonaceous chondrites. That the history of these compounds differs from our own is underscored by important eccentricities in their molecular structure. It is generally believed by organic chemists that when the earth was still in its infancy, when its vapors had condensed into newly formed seas and its shroud of air lacked destructive oxidizing agents, the first organic acids were probably assembled in two very distinct varieties. Valine, for example, possibly occurred as mirror images of itself, much in the same way as your right and left hands are mirror images, or isomers, of each other. In those days before the dawn of living self-replicating matter, both "right-handed" and "left-handed" molecules might have drifted about the Precambrian seas in equal or near-equal quantities. Received on Sun 06 Oct 2002 05:42:48 AM PDT |
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