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Cyanide Abundance of Highly Aqueously Altered CM Chondrites
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Asteroids, and the meteorites that come from them, retained the composition of
the early Solar System and can give us insight to the processes that lead to the
origin of life. The current NASA mission, OSIRIS-REx, has returned asteroid
samples from the near-Earth asteroid Bennu. This asteroid is thought to be
similar in composition to highly aqueously altered meteorites including CM1 and
CM1/2 meteorites. Cyanide is thought to be an important molecule for prebiotic
chemistry. Simple cyanide salts would have been the most accessible form of
cyanide for reactions to occur; however, they may have recombined to form
different metal-cyanide complexes most likely during the aqueous alteration
stage(s). Understanding more about both the acid-releasable cyanide abundance
and simple salt cyanide abundance of meteorites and asteroids will give insight
to speciation of cyanide in these samples. This information will help in
understanding cyanide’s role in prebiotic chemistry.
Only one highly aqueously altered meteorite sample, and no asteroid samples, have
been analyzed for acid-releasable cyanide abundance previously. In this work, I
determined acid-releasable cyanide abundances for three highly aqueously altered
meteorites and simple salt cyanide abundances for four highly aqueously altered
meteorites using capillary-flow liquid chromatography high-resolution mass
spectrometry. The most altered meteorite analyzed, a CM1, had the lowest
abundance of acid-releasable cyanide present. The other two meteorites analyzed,
both CM1/2s, had very similar cyanide abundances compared to one another and
have a higher acid-releasable cyanide abundance than the CM1. However, there was
only one meteorite that had a simple salt cyanide concentration above my
detection limit. This concentration corresponded to less than 1% of the
acid-releasable cyanide abundance for that meteorite. If Bennu is truly similar
in composition to highly aqueously altered CM meteorites we expect to see
acid-releasable cyanide present with very little of it being due to simple
cyanide salts.
Title: Cyanide Abundance of Highly Aqueously Altered CM Chondrites
Description:
Asteroids, and the meteorites that come from them, retained the composition of
the early Solar System and can give us insight to the processes that lead to the
origin of life.
The current NASA mission, OSIRIS-REx, has returned asteroid
samples from the near-Earth asteroid Bennu.
This asteroid is thought to be
similar in composition to highly aqueously altered meteorites including CM1 and
CM1/2 meteorites.
Cyanide is thought to be an important molecule for prebiotic
chemistry.
Simple cyanide salts would have been the most accessible form of
cyanide for reactions to occur; however, they may have recombined to form
different metal-cyanide complexes most likely during the aqueous alteration
stage(s).
Understanding more about both the acid-releasable cyanide abundance
and simple salt cyanide abundance of meteorites and asteroids will give insight
to speciation of cyanide in these samples.
This information will help in
understanding cyanide’s role in prebiotic chemistry.
Only one highly aqueously altered meteorite sample, and no asteroid samples, have
been analyzed for acid-releasable cyanide abundance previously.
In this work, I
determined acid-releasable cyanide abundances for three highly aqueously altered
meteorites and simple salt cyanide abundances for four highly aqueously altered
meteorites using capillary-flow liquid chromatography high-resolution mass
spectrometry.
The most altered meteorite analyzed, a CM1, had the lowest
abundance of acid-releasable cyanide present.
The other two meteorites analyzed,
both CM1/2s, had very similar cyanide abundances compared to one another and
have a higher acid-releasable cyanide abundance than the CM1.
However, there was
only one meteorite that had a simple salt cyanide concentration above my
detection limit.
This concentration corresponded to less than 1% of the
acid-releasable cyanide abundance for that meteorite.
If Bennu is truly similar
in composition to highly aqueously altered CM meteorites we expect to see
acid-releasable cyanide present with very little of it being due to simple
cyanide salts.
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