October 9, 2001
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Contents of this News Tip:
Scientists have long debated whether the universe is
headed for a fiery finish or an icy end. Now one group
of researchers supported by the National Science Foundation
(NSF) believes that its analysis of the shapes of
nearby galaxies favors the theory of a cold demise.
A team led by Adrian Melott, a University of Kansas
cosmologist, studied the shapes of 180 galaxy clusters
containing galaxies numbering from the hundreds to
the thousands. The team found that while nearby galaxy
clusters were fairly spherical, the farthest clusters
were more squashed and irregular. The team reported
its findings in the October 1 Astrophysical Journal
Letters.
The light from the faraway galaxies began its journey
toward Earth early in the development of the universe,
and therefore presents a snapshot of the universe
as it was long ago. The shapes of those clusters led
the researchers to believe that galaxy clusters have
been evolving toward a more regular, spherical shape.
This is an indicator of a low-density universe, in
which the expansion is outrunning the clumping effect
of gravity. The clusters are becoming more spherical
because they are less often deformed by new matter
falling into them.
As the gases and other materials that make up the universe
spread out even further, the researchers say the universe
could become a cold, empty place. [Amber Jones]
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NSF-supported researchers have fabricated a minute
sensor for detecting hydrogen gas leaks that could
make storing the explosive substance a safer proposition,
thereby aiding in the development of the gas as an
alternative energy source.
Hydrogen combustion is a potentially attractive method
of producing energy because it produces only water
as a by-product. But hydrogen -- like gasoline --
is potentially explosive. This complicates storage,
particularly in confined areas such as a tank in a
hydrogen-powered vehicle. As greater use is made of
this clean-burning fuel for basic energy needs, the
development of reliable, inexpensive sensors will
be more important for detecting leaks.
Analytical chemist Reginald Penner and colleagues from
the University of California at Irvine and Montpellier
University in France report that their ultra-small
device, made from nanoscale arrays of palladium wires,
responds to leaks an order of magnitude faster than
conventional sensors. In the presence of hydrogen,
the resistance of the array decreases rapidly, apparently
due to the closing of nano-sized gaps in the wires
as the palladium absorbs the gas. In the absence of
hydrogen, the circuits reopen.
Besides being reliable, reusable, small and unobtrusive,
the device operates on only a few nanowatts of power.
Penner’s team reported its findings in the September
21 issue of Science. [Amber Jones]
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NSF has selected a consortium of universities to establish
the new organization that will manage an NSF-funded
network of earthquake engineering research facilities,
named the George E. Brown, Jr. Network for Earthquake
Engineering Simulation (NEES), slated to start operation
in 2004.
The Consortium of Universities for Research in Earthquake
Engineering (CUREE) of Richmond, Calif., will involve
the broad earthquake engineering community in establishing
the entity that will manage NEES during its first
decade.
NEES will allow researchers to share and remotely operate
experimental equipment at advanced earthquake engineering
facilities and to more easily share data and computations.
The equipment -- including shake tables, a tsunami
wave basin, geotechnical centrifuges and laboratory,
and mobile geotechnical and structural experimental
capabilities -- models and analyzes earthquake forces
and helps engineers design buildings, bridges and
other infrastructure to withstand those forces.
While the management project is under way, the information
technology network called NEESgrid is being designed
and implemented by a team led by the University of
Illinois at Urbana Champaign. [Amber Jones]
For more information, see: http://www.eng.nsf.gov/nees
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