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Extraterrestrial gases in buckyballs found on Earth
EXTRATERRESTRIAL GASES, including helium, are trapped in
"buckyball" molecules in a layer of sedimentary clay found in
many places on Earth, according to a paper published in the
Proceedings of the National Academy of Sciences. The discovery
provides a new tool for tracing asteroid and comet impacts in
Earth's geological and biological records.
A University of Hawaii geochemist and her colleagues, including a
NASA scientist, found gases that did not originate on Earth
inside buckyballs, or fullerene carbon molecules.
The fullerene molecule is a hollow, cage-like structure typically
made of 60 or more carbon atoms; it is also referred to as a
"buckyball,". Ted Bunch, a scientist at NASA's Ames Research
Center in California's Silicon Valley, said.
"The buckyballs containing the gases arrived on Earth about 65
million years ago during an asteroid impact that scientists
theorize ended the age of the dinosaurs. The clay layer that
formed from fallout of the impact debris was globally
distributed," Bunch explained.
Luann Becker, of the University of Hawaii, Honolulu, HI; Robert
Poreda, of the University of Rochester, Rochester, NY; and Ted
Bunch of NASA Ames, discovered the extraterrestrial gases in the
fullerenes.
"Helium from different sources on Earth, like our atmosphere or
the emissions from volcanoes, have a very different isotopic
signature from the helium in a meteorite," Becker said.
An isotopic signature is the ratio of the isotopes of an element;
for example, terrestrial helium consists of a small amount of
helium 3 (whose nucleus has two protons and one neutron), and
mostly helium 4 that has 2 protons and 2 neutrons. Cosmic helium
is mostly helium 3.
"The helium we found within the fullerene cages of Australia's
Murchison meteorite, for example, is similar to the helium that
existed when our Solar System first formed," Becker stated. That
finding points to a cosmic source for the fullerenes, the
researchers say.
In contrast, molecules formed in the high pressure and
temperature of an earthly impact or the heat of wildfires that
followed would have encapsulated terrestrial helium, according to
the researchers.
They say the finding also supports the theory that atmospheric
gases and organic compounds arrived on the Earth's surface during
asteroid and comet strikes early in the planet's history when
impacts were very numerous.
The discovery relates to previous work by Becker and Bunch,
published in Nature in July 1999 that first identified naturally
occurring fullerenes in a meteorite. The scientists found
significant quantities of very large fullerene molecules, some
containing as many as 400 carbon atoms, in samples from the 4.6-
billion-year-old Allende meteorite that landed in Mexico three
decades ago.
The subsequent work examined several Cretaceous/Tertiary boundary
clay sediments distributed worldwide, including deposits in
Denmark, New Zealand and North America.
In each case, the researchers found fullerenes that encapsulated
noble gases with unmistakable extraterrestrial and possibly
extra-solar isotopic signatures.The scientists examined the one-
inch clay layer because it is a well-studied sediment that
contains extraterrestrial iridium and highly shocked minerals
resulting from an asteroid impact 65 million years ago.
A highly shocked mineral is one that has experienced temperatures
of more than 2,000 C and pressures of about 400,000 atmospheres
from impact shock.
The clay layer documents a period of abrupt change in biological
evolution, including mass extinction of the dinosaurs, now
generally attributed to the impact of a carbonaceous asteroid
with the Earth.
Becker said she hopes to expand the research to examine other
periods of mass extinction such as the even more devastating
event that formed the 250-million-year-old Permian/Triassic layer
of sediment.
She added that she hopes to determine if impacts with Earth
trigger global change, including whether fullerenes of
extraterrestrial origin delivered gases and carbon necessary to
establish life on Earth.
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