October 25, 1996
For more information on these science news
and feature story tips, please contact the public information officer at the end of each item at
(703) 292-8070. Editor: Beth Gaston
Contents of this Tipsheet:
The most sensitive fully robotic telescope anywhere, the Katzman
Automatic Imaging Telescope (KAIT), will allow astronomers to search
for and monitor supernovas or exploding stars without spending endless
hours looking through a telescope. The KAIT, located at Lick
Observatory at the University of California, can track an area of the
sky for hours, better than any other robotic telescope now in
operation, and can detect objects 10,000 times fainter than other such
telescopes can recognize.
The KAIT, funded largely through an NSF Presidential Young
Investigator Award, obtains astronomical images using a separate
charge-coupled device (CCD) imaging system for a guide star that
allows it to remain precisely fixed on a given area of the sky. Other
robotic telescopes use simpler tracking that allows a star to drift
significantly in a couple of minutes.
"There have been other robotic telescopes, but this implementation
is the most complex, and addresses a complicated astrophysical
problem," said Eileen Friel, program director for NSF's Division of
Stellar Astronomy and Astrophysics.
The KAIT will be used to check the night sky for flaring
supernovas, to follow the brightness of variable stars and to observe
changing objects. Since it is under computer control, it can also use
complex software to analyze the data. The computer can automatically
change the priority of a given target, depending on whether
observations were successful in preceding nights. More broadly, the
techniques of remote CCD imaging and software analysis have wide
applications in other scientific fields and in medicine.
[Cary Lee Hanes]
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More than two millennia ago, the Roman natural philosopher Pliny
the Elder wrote of a "slime" that could be obtained from marine
creatures and used to make objects glow green. Today, molecular and
cellular biologists have turned this marvel into a powerful research
tool used to illuminate the workings of genes and follow the wanderings of protein molecules inside a
living cell. The source of the green glow is a unique protein, called
green fluorescent protein (GFP), found in a Pacific Northwest
jellyfish.
NSF-supported biologists James Remington of the University of
Oregon and Roger Tsien of the University of California at San Diego
have determined the structure of an altered form of the protein and
revealed the source of the green glow. "The unusual molecule
responsible for the glow resembles a Chinese finger puzzle: a
barrel-shaped structure with a coil of amino acids corked in the
center," explained Kamal Shukla, program director in NSF's division of
molecular and cellular biosciences, which funded the research. "The
green color results from the collapse of one turn of the coil to form
a ring of three amino acids." The researchers chose to study the
modified GFP because it is more useful for cell biologists, glowing
much more brightly than the natural variant. Modifications have also
changed the color of the glow.
The uses for GFP are almost unlimited, they say. In gene therapy,
doctors could inject GFP along with the therapy substance, and by
checking for fluorescence, determine whether the therapy had been
properly delivered. By "tuning" the green dye to different colors,
scientists studying vision may be able to gain insight into how the
human eye is able to respond to so many different colors. Said Kamal
Shukla, "Pliny the Elder probably never would have guessed where his
original observations would lead." [Cheryl Dybas]
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An international team of scientists representing nine countries is
about to board the drill ship JOIDES Resolution--currently docked in
San Diego, California--for an Ocean Drilling Program expedition to the
continental margin off Costa Rica. The researchers hope to determine
the ages and compositions of the area's rocks and sediments and their
chemical and physical properties. They will also use a newly
developed tool called "LWD," or Logging While Drilling. The LWD
technique samples chemical and physical properties within the drill
hole while drilling is occurring, giving scientists "pristine" results
unaffected by the vertical movements of the drill.
The NSF-supported team is led by geologists Eli Silver of the
University of California at Santa Cruz, and Gaku Kimura of the
University of Osaka in Japan. "The Costa Rica margin is an important
location where tectonic plates collide," explained Silver, "forcing
one plate to slide under the other, creating a subduction zone."
Subduction zones are the most active features on Earth, added Bruce
Malfait, director of NSF's Ocean Drilling Program. "They control the
movement of plates, produce most of the world's volcanic and seismic
activity, and play a key role in recycling surface material to great
depths within the Earth." With this expedition, scientists hope to
make major inroads into understanding this recycling process.
[Cheryl Dybas]
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