-------- Original Message --------
Subject:        RE:Could Adenine From Interstellar Dust Have Triggered Life On 
Earth? Elsewhere?
Date:   Sun, 7 Oct 2007 10:29:19 -0700
From:   Chris de Morsella <[EMAIL PROTECTED]>
http://www.sciencedaily.com/releases/2007/10/071002113036.htm   *Could 
Adenine From Interstellar Dust Have Triggered Life On Earth?
   Elsewhere?*

**/Science Daily/** <http://www.sciencedaily.com/>**/ —/**** Some of the
elements necessary to support life on Earth are widely known - oxygen,
carbon and water, to name a few. Just as important in the existence of
life as any other component is the presence of adenine, an essential
organic molecule. Without it, the basic building blocks of life would
not come together. Scientists have been trying to find the origin of
Earth's adenine and where else it might exist in the solar system.
University of Missouri-Columbia researcher Rainer Glaser may have the
answer.**

Life exists on Earth because of a delicate combination of chemical
ingredients. Using a theoretical model, Glaser is hypothesizing the
existence of adenine in interstellar dust clouds. Those same clouds may
have showered young Earth with adenine as it began cooling billions of
years ago, and could potentially hold the key for initiating a similar
process on another planet.

"The idea that certain molecules came from space is not outrageous,"
said Glaser, professor of chemistry in MU's College of Arts and Science.
"You can find large molecules in meteorites, including adenine. We know
that adenine can be made elsewhere in the solar system, so why should
one consider it impossible to make the building blocks somewhere in
interstellar dust?"

Glaser believes astronomers should look for interstellar dust clouds
that have highly-concentrated hydrogen cyanide (HCN), which can indicate
the presence of adenine. Finding such pockets would narrow the spectrum
of where life could exist within the Milky Way galaxy.

"There is a lot of sky with a few areas that have dust clouds. In those
dust clouds, a few of them have HCN. A few of those have enough HCN to
support the synthesis of the molecules of life. Now, we have to look for
the HCN concentrations, and that's where you want to look for adenine,"
Glaser said. "Chemistry in space and 'normal chemistry' can be very
different because the concentrations and energy-exchange processes are
different. These features make the study of chemistry in space very
exciting and academically challenging; one really must think without
prejudice."

This theory describing the fusion of early life-forming chemicals is
presented in the latest issue of the peer-reviewed journal
"Astrobiology" and is co-authored by Brian Hodgen (Creighton
University), Dean Farrelly (University of Manchester) and Elliot McKee
(St. Louis University). The paper, "Adenine Synthesis in Interstellar
Space: Mechanisms of Prebiotic Pyrimidine-Ring Formation of Monocyclic
HCN-Pentamers," describes the absence of a sizeable barrier that would
prevent formation of the skeleton needed for adenine synthesis. The
article is also featured in the Aug. 6 issue of "Chemical & Engineering
News."

/Note: This story has been adapted from material provided by University
of Missouri-Columbia./








 
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