Meteorites
to Interstellar Gas Clouds

Right)
A cut piece of the Parnallee meteorite, which is a carbonaceous
chondrite. It still has a slight sweet smell of organic
solvent. Courtesy of the Natural History Museum, UK.
© John Hodges, 2000
(Left)
A meteor fireball from the 1998 Leonids meteor shower. ©
John Hodges, 1998
There
are four main types of meteorite. Three are metallic or
rocky in nature, but the fourth is high in carbon compounds, some
of which are organic. These carbonaceous
chondrites, as they are known, are rich not only in carbon
but in organic hydrocarbons and amino acids. Though none
of these organics has yet been proven to be alive (or even dead
- implying it was once alive).
Comets
leave tails of dust and ice. If the Earth passes through
them we can usually see a meteor shower. The microscopic
particles burn up as they strike the upper atmosphere, leaving
a distinct trail in the sky. The colors vary and can give
an idea of the composition of the the meteor. Occasionally,
the color suggests the presence of organic compounds.
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(Above)
Asteroid meteorite.
Click on image to see more microscopic views
Certain
times of the year the Earth passes through the tails of comets
and this can sometimes result in a spectacular meteor
shower. Meteor trails can vary in color, and this
can sometimes give an indication of the probably chemical composition
of the meteor, which is a tiny ice or dust particle the size
of a sand grain. Attempts have also been made to record
the spectrum of meteor trails. This gives a much more
reliable result, and though many meteors are found to be water
or silica, some have proven to be made of carbon, and carbon
compounds. Some of these latter spectra indicate the presence
of organic matter. Could a meteor contain bacteria or
viral strands?
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(above)
The Eagle Nebula © NASA, 1995
©
1995-2000 by Michael W. Davidson and The Florida State University.
If so, this means that these organics originated in
deep space, perhaps within an interstellar cloud, such as this one
in the Eagle
Nebula. Such regions have not only been detected in our
own Milky Way, but have been seen in other galaxies too. There
is so much gas that, even across the vast distances of space, we
can detect from the nature of the spectrum emitted exactly what
the clouds are made of. Though many are just helium
and hydrogen - the simplest of elements - a good many others consist
of simple molecules such as water. In addition, more complex
molecules exist, such as methane and ammonia; and as we might expect
from the meteoritic evidence, some clouds contain compounds that
are clearly organic in nature. One such is ethanol - basic
alcohol.
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(Left)
A section through a fragment of the Murchison Meteorite, courtesy
of the Natural History Museum, UK. © John Hodges, 1999
In
September 1969 one of the most important meteorites ever discovered
fell near the town of Murchison
in Australia. It broke up in the atmosphere and fragments
rained down. Many of these were recovered. The rock
was black and had a strange texture. It also smelled of methylated
spirit. Samples were sent to the University
of Melbourne and the meteorite was identified as a carbonaceous
chondrites, rich in organic material. It is thought to
be the fragmentary remains of an extinct comet. Amino acids
were found in the meteorite, identical to those commonly used in
life processes. But some amino acids in the meteorite were
chirally right-handed, and not common to terrestrial life.
Left-handed molecules outnumbered right-handed molecules by a significant
number, though, so speculation mounted as to whether or not the
organic residues in the meteorite were of biological origin.
The question remains open, however, for it is possible to create
such molecules by purely physical processes as well as biological
ones.
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David
Deamer, a biologist at the University of California, Santa Cruz,
made an astounding discovery
in the early 1980's, while working on Murchison fragments.
He extracted tiny double-layered cell-like structures as he flushed
out the organic compounds with solvent - structures that resembled
primitive cells. These "vesicles" as David Deamer called them,
were unique to science and perplexed researchers as to their origin
and nature.
So
while the Murchison meteorite raised questions about there being
life in deep space, it did provide categorical evidence that complex
organic compounds do exist and probably form in deep space.
That
was until very recently.

(above)
A fragment of the Allende Meteorite, courtesy of the Natural
History Museum, UK. © John Hodges, 2000
In
late January 2000 the findings of research on several carbonaceous
chondrites was reported at a conference in Denver, Colorado.
The interiors of pieces of the Murchison,
the Efremovka and the Allende
meteorites have been examined by Dr
Stanislav Zhmur and Lyudmila M. Gerasimenkoof the Russian Academy
of Sciences. Their results are as spectacular as we saw with
the famous "life-bearing" Mars Meteorite,
ALH84001.
The
images they showed, reveal six different types of microstructure
in the meteorites which the claim are reminiscent of colonies of
different cyanobacteria,
in a fossilized state. They identify each structure with a
specific Earth organism and point out that on Earth, these organism
would live in water,"... probably in hydrothermal volcanic activity
zones."
Questions
about how well living bacteria in a meteorite might survive entry
into the Earth's atmosphere is being addressed by a group of European
scientists which includes Professor
Colin Pillinger. They are planning to create an
artificial
life-carrying meteorite.
Go to Life
on deep space
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David
Deamer - article
David
Deamer - personal
Create
space! - making vesicles
the
process - a vesicle
Teachers
Wormhole
©
1999 Satellite Events Enterprises Inc.
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