[meteorite-list] Supernova Shrapnel Found in Meteorite

From: MEM <mstreman53_at_meteoritecentral.com>
Date: Thu, 16 Sep 2010 01:01:15 -0700 (PDT)
Message-ID: <936675.99434.qm_at_web55205.mail.re4.yahoo.com>

Yet another meteorite related news item. Check your specimens for chromium 54
grains and see if you've hit the lottery for pre-pre-solar grains! They will be
magnetic but at 100 nm not somehting you'll see with the eye alone.
Elton

Supernova Shrapnel Found in Meteorite
ScienceDaily (Sep. 14, 2010) ? Scientists have identified the microscopic
shrapnel of a nearby star that exploded just before or during the birth of the
solar system 4.5 billion years ago.

Faint traces of the supernova, found in a meteorite, account for the mysterious

variations in the chemical fingerprint of chromium found from one planet and
meteorite to another. University of Chicago cosmochemist Nicolas Dauphas and
eight co-authors report their finding in the late Sept. 10, 2010 issue of the
Astrophysical Journal.
Scientists formerly believed that chromium 54 and other elements and their
isotopic variations became evenly spread throughout the cloud of gas and dust
that collapsed to form the solar system. "It was a very well-mixed soup," said
Bradley Meyer, a professor of astronomy and astrophysics at Clemson University
who was not a co-author of the study. "But it looks like some of the
ingredients got in there and didn't get completely homogenized, and that's a
pretty interesting result."
Scientists have known for four decades that a supernova probably occurred
approximately 4.5 billion years ago, possibly triggering the birth of the sun.
Their evidence: traces of aluminum 26 and iron 60, two short-lived isotopes
found in meteorites but not on Earth.
These isotopes could have come from a type II supernova, caused by the
core-collapse of a massive star. "It seems likely that at least one massive
star contributed material to the solar system or what was going to become the
solar system shortly before its birth," Meyer said.
Researchers have already extracted many type II supernova grains from
meteorites, but never from a type IA supernova. The latter type involves the
explosion of a small but extremely dense white-dwarf star in a binary system,
one in which two stars orbit each other. It should now be possible to determine

which type of supernova contributed the chromium 54 to the Orgueil meteorite.
"The test will be to measure calcium 48," Dauphas said. "You can make it in
very large quantities in type Ia, but it's very difficult to produce in type
II." So if the grains are highly enriched in calcium 48, they no doubt came
from a type Ia supernova.
Cosmochemists have sought the carrier of chromium 54 for the last 20 years but
only recently have instrumentation advances made it possible to find it.
Dauphas's own quest began in 2002, when he began the painstaking meteorite
sample-preparation process for the analysis he was finally able to complete
only last year.
Dauphas and his associates spent three weeks searching for chromium 54-enriched
nanoparticles with an ion probe at the California Institute of Technology. "Time

is very precious on those instruments and getting three weeks of instrument time

is not that easy," he said.
The researchers found a hint of an excess of the chromium-54 isotope in their
first session, but as luck would have it, they had to search 1,500 microscopic
grains of the Orgueil and Murchison meteorites before finding just one with
definitely high levels.
The grain measured less than 100 nanometers in diameter -- 1,000 times smaller
than the diameter of a human hair. "This is smaller than all the other kinds of

presolar grains that have been documented before, except for nanodiamonds that
have been found here at the University of Chicago," Dauphas said.
The findings suggest that a supernova sprayed a mass of finely grained
particles into the cloud of gas and dust that gave birth to the solar system
4.5 billion years ago. Dynamical processes in the early solar system then
sorted these grains by size. These size-sorting processes led the grains to
become disproportionally incorporated into the meteorites and planets newly
forming around the sun.
"It's remarkable that you can look at an isotope like chromium 54 and
potentially find out a whole lot about what happened in the very first period
of the solar system's formation," Meyer said.
Received on Thu 16 Sep 2010 04:01:15 AM PDT