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Study Suggests Component of Volcanic Gas May Have Played a SignificantRole in the Origins of Life on Earth (Forwarded)



 
 
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  #1  
Old October 8th 04, 03:36 PM
Andrew Yee
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Default Study Suggests Component of Volcanic Gas May Have Played a SignificantRole in the Origins of Life on Earth (Forwarded)

Scripps Research Institute

For more information contact:

Keith McKeown
10550 North Torrey Pines Road
La Jolla, California 92037
Tel: 858.784.8134
Fax: 858.784.8118


October 7, 2004

Study Suggests Component of Volcanic Gas May Have Played a Significant Role in
the Origins of Life on Earth

Carbonyl Sulfide Forms Peptide Bonds

La Jolla, CA -- Scientists at The Scripps Research Institute and the Salk
Institute for Biological Studies are reporting a possible answer to a
longstanding question in research on the origins of life on Earth -- how did the
first amino acids form the first peptides?

Peptides and proteins are strings of amino acid building blocks, and they are
one of the most important classes of biological molecules found in living things
today. Fifty years of chemical research on the origins of life has shown that
amino acids could have formed spontaneously on the early Earth environment or
could have been introduced onto the early Earth from meteorites.

"There are lots of ways to make amino acids," says Professor M. Reza Ghadiri,
Ph.D., who is a member of The Skaggs Institute for Chemical Biology at Scripps
Research. "But the question is, how do you couple them together?"

Ghadiri and Luke Leman, who is a member of the Kellogg School of Science and
Technology at Scripps Research, worked out one possible solution with Leslie
Orgel of the Salk Institute. In the latest issue of the journal Science, Leman,
Ghadiri, and Orgel suggest that the missing link is a chemical component of
volcanic gas known as carbonyl sulfide.

Carbonyl sulfide is present in volcanic gasses and deep sea vent emissions
today, and since these geological phenomena were prominent features on the early
Earth, it is reasonable to assume that the gas was present.

In their report, the scientists demonstrate that the gas can bring about a
vigorous chemical reaction that forms peptides under mild aqueous conditions.
Within a few minutes of introducing the gas to a reaction vessel containing
amino acids, they observed high yields of di-, tri-, and tetra-peptides. They
carried out the reaction in the presence of air, without air, and with and
without other ingredients like metal ions, and they found peptides formed
readily under all these conditions.

"It's really efficient, actually," says Ghadiri. "This addresses a very
important question that we did not have a real good answer for."

Life -- What We Know, and What We Don't

The question of how life originated is one of the most interesting gaps in our
knowledge -- interesting perhaps because we know approximately when it occurred,
but we do not know how it occurred.

The earliest fossils scientists have found are stromatolites -- large clumps of
cyanobacteria that grew in abundance in the ancient world over 3.5 billion years
ago in what is now western Australia. These most likely evolved from some
simpler life forms because, like all modern life, cyanobacteria are highly
sophisticated living organisms -- with cell walls, complex metabolism, and DNA
genes. The question of the origins of life is: what came before the stromatolites?

Research on the origins of life has suggested the notion of an ancient RNA world
-- one in which RNA genes stored genetic information (something done by DNA
today), carried out the chemistry necessary for life, and formed the essential
physical structures of life (something done primarily by proteins today).

But how did that RNA world come about?

"Anybody who thinks they know the solution to this problem [of the origin of
life] is deluded," says Orgel.

"But," he adds, "anybody who thinks this is an insoluble problem is also deluded."

One possible approach to the problem of life's origins is to ask the question
scientifically rather than historically -- how can life emerge rather than how
did life emerge. In order to address this, scientists try to determine
experimentally what is chemically feasible and what could have occurred on the
prebiotic earth.

One possibility, which was suggested in the 1920s by the Russian scientist A.I.
Oparin, is that life emerged in its most primitive forms from minerals, metals,
and the elements carbon, hydrogen, oxygen, and nitrogen, which were combined
into amino acids, nucleotides, and the other the building blocks of life under
the violent energy of lightning, solar radiation, comet impacts, and volcanic
events that were present.

In 1953, this theory was given a boost when a paper was published in Science by
Stanley L. Miller, who is Professor Emeritus at the University of California,
San Diego. In the paper, Miller described an experiment he devised with Harold
C. Urey -- now called the Miller and Urey experiment -- that gave experimental
underpinnings to Oparin's ideas.

In the experiment, Miller boiled H2O, CH4,H2, and NH3 gases in a glass apparatus
containing a pair of tungsten electrodes. He subjected the chemicals to an
electric discharge, intended to simulate conditions on the early Earth, and he
collected and analyzed the molecules that formed -- which included the amino
acids alanine, glycine, and a few others. In the years since, several other
investigators have expanded on the Miller–Urey experiment to demonstrate the
formation and chemistry of many of the common biological amino acids, sugars,
and nucleotides. Orgel, who is a long-time investigator in the field, has done
pioneering research on the prebiotic chemistry of nucleotides.

This latest study is an advance because previous attempts to demonstrate the
formation of peptides on early Earth depended on reaction schemes that were less
plausible or were not as efficient. Next, the team plans to examine carbonyl
sulfide's reactive properties further and see if the gas can bring about other
chemical reactions that are relevant to prebiotic chemistry.

The article, "Carbonyl Sulfide–Mediated Prebiotic Formation of Peptides" by Luke
Leman, Leslie Orgel, and M. Reza Ghadiri, appears in the October 8, 2004 issue
of the journal Science. See:
http://www.sciencemag.org .

This research was supported by The Skaggs Institute for Research, by the NASA
Astrobiology Institute, by NASA Exobiology, and through a National Science
Foundation Predoctoral Fellowship. About The Scripps Research Institute

The Scripps Research Institute in La Jolla, California and Palm Beach County,
Florida, is one of the world's largest, private, non-profit biomedical research
organizations. It stands at the forefront of basic biomedical science that seeks
to comprehend the most fundamental processes of life. Scripps Research is
internationally recognized for its research into immunology, molecular and
cellular biology, chemistry, neurosciences, autoimmune diseases, cardiovascular
diseases and synthetic vaccine development.
  #2  
Old October 8th 04, 06:39 PM
Jonathan Silverlight
external usenet poster
 
Posts: n/a
Default

In message , Andrew Yee
writes
Scripps Research Institute

For more information contact:

Keith McKeown
10550 North Torrey Pines Road
La Jolla, California 92037
Tel: 858.784.8134
Fax: 858.784.8118


October 7, 2004

Study Suggests Component of Volcanic Gas May Have Played a Significant
Role in the Origins of Life on Earth

Carbonyl Sulfide Forms Peptide Bonds

La Jolla, CA -- Scientists at The Scripps Research Institute and the
Salk Institute for Biological Studies are reporting a possible answer
to a longstanding question in research on the origins of life on Earth
-- how did the first amino acids form the first peptides?

Peptides and proteins are strings of amino acid building blocks, and
they are one of the most important classes of biological molecules
found in living things today. Fifty years of chemical research on the
origins of life has shown that amino acids could have formed
spontaneously on the early Earth environment or could have been
introduced onto the early Earth from meteorites.

"There are lots of ways to make amino acids," says Professor M. Reza
Ghadiri, Ph.D., who is a member of The Skaggs Institute for Chemical
Biology at Scripps Research. "But the question is, how do you couple
them together?"

Ghadiri and Luke Leman, who is a member of the Kellogg School of
Science and Technology at Scripps Research, worked out one possible
solution with Leslie Orgel of the Salk Institute. In the latest issue
of the journal Science, Leman, Ghadiri, and Orgel suggest that the
missing link is a chemical component of volcanic gas known as carbonyl
sulfide.

Carbonyl sulfide is present in volcanic gasses and deep sea vent
emissions today, and since these geological phenomena were prominent
features on the early Earth, it is reasonable to assume that the gas
was present.

In their report, the scientists demonstrate that the gas can bring
about a vigorous chemical reaction that forms peptides under mild
aqueous conditions. Within a few minutes of introducing the gas to a
reaction vessel containing amino acids, they observed high yields of
di-, tri-, and tetra-peptides. They carried out the reaction in the
presence of air, without air, and with and without other ingredients
like metal ions, and they found peptides formed readily under all these
conditions.

"It's really efficient, actually," says Ghadiri. "This addresses a very
important question that we did not have a real good answer for."


snip


One possible approach to the problem of life's origins is to ask the
question scientifically rather than historically -- how can life
emerge rather than how did life emerge. In order to address this,
scientists try to determine experimentally what is chemically feasible
and what could have occurred on the prebiotic earth.

One possibility, which was suggested in the 1920s by the Russian
scientist A.I. Oparin, is that life emerged in its most primitive forms
from minerals, metals, and the elements carbon, hydrogen, oxygen, and
nitrogen, which were combined into amino acids, nucleotides, and the
other the building blocks of life under the violent energy of
lightning, solar radiation, comet impacts, and volcanic events that
were present.

In 1953, this theory was given a boost when a paper was published in
Science by Stanley L. Miller, who is Professor Emeritus at the
University of California, San Diego. In the paper, Miller described an
experiment he devised with Harold C. Urey -- now called the Miller and
Urey experiment -- that gave experimental underpinnings to Oparin's ideas.

In the experiment, Miller boiled H2O, CH4,H2, and NH3 gases in a glass
apparatus containing a pair of tungsten electrodes. He subjected the
chemicals to an electric discharge, intended to simulate conditions on
the early Earth, and he collected and analyzed the molecules that
formed -- which included the amino acids alanine, glycine, and a few
others. In the years since, several other investigators have expanded
on the Miller–Urey experiment to demonstrate the formation and
chemistry of many of the common biological amino acids, sugars, and
nucleotides. Orgel, who is a long-time investigator in the field, has
done pioneering research on the prebiotic chemistry of nucleotides.


Getting peptide bonds to form in those conditions is neat, but isn't the
CH4/H2/NH3 model of the early atmosphere as dead as yesterday's news?
OTOH, what are the chances of a volcano on Titan? Huygens may find
something interesting!
--
What have they got to hide? Release the ESA Beagle 2 report.
Remove spam and invalid from address to reply.
  #3  
Old October 15th 04, 08:46 PM
Steve Willner
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Posts: n/a
Default

In article ,
Jonathan Silverlight writes:
Getting peptide bonds to form in those conditions is neat, but isn't the
CH4/H2/NH3 model of the early atmosphere as dead as yesterday's news?


I thought it was methane, ammonia, and carbon dioxide, not that I'm
any expert on the subject. I'd expect the hydrogen to escape during
the early, hot phase of planet formation. Anybody know what current
thinking really is?

--
Steve Willner Phone 617-495-7123
Cambridge, MA 02138 USA
(Please email your reply if you want to be sure I see it; include a
valid Reply-To address to receive an acknowledgement. Commercial
email may be sent to your ISP.)
 




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