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Planetary Society Awards Three New Gene Shoemaker NEO Grants
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- Date: Fri, 2 Apr 1999 1:30:41 GMT
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http://planetary.org/news/articlearchive/headlines/1999/headln-020599.html
Planetary Society Awards Three New Gene Shoemaker NEO Grants
February 5, 1999
Three researchers have been selected to receive Planetary
Society Gene Shoemaker Near Earth Object Grants. Named for one of
the pioneers in the field, the grants fund programs in the
discovery and tracking of near-Earth objects -- asteroids and
comets with Earth-crossing orbits that could impact our planet
with devastating results. Special emphasis is given to
international and amateur observers.
Only about 5% to 10% of the estimated total number of
one-kilometer or larger objects that cross Earth's orbit have
been discovered.
"Although the rate of NEO discovery has accelerated recently as
new professional survey programs have come on line, we are
still shy of the widely recommended rate needed to find 90% of
the near-Earth asteroids larger than one kilometer within a
decade," said Dan Durda, an asteroid researcher at the the
Southwest Research Institute's Boulder, Colorado office, and
coordinator of the Planetary Society's Gene Shoemaker NEO Grant
program.
Even though various astronomical groups and NASA advisory
committees have recommended that discovery of NEOs be
accelerated, government support for searches and follow-up
programs remains modest.
The 1999 Gene Shoemaker NEO Grants, totaling $27,000 (US), have
been awarded to an international collection of researchers:
Stefan Gajdos of the Slovak Republic, Paulo Holvorcem of
Brazil, and Frank Zoltowski of Australia.
Gajdos is a professional astronomer with the Institute of
Astronomy in Bratislava in the Slovak Republic. His grant
monies will be used to upgrade his program's equipment and
software, to fund needed computer services, and to create a
public outreach program.
Holvorcem, a teacher at the Universidade Estadual de Campinas
in Brazil, will use his Gene Shoemaker NEO Grant to upgrade
automation of equipment at his observatory, freeing a number of
volunteer observers to spend more time conducting data analysis
and taking more exposures during each observation session.
Zoltowski is an amateur astronomer who conducts NEO searches in
the small town of Woomera in the South Australian outback.
Grant money will enable Zoltowski to upgrade his charge-coupled
device (CCD) camera, improving his ability to detect NEOs in
sky images and confirm their orbits in a series of exposures.
A Swarm of Near-Earth Objects
Earth travels through a swarm of near-Earth objects of various
sizes and orbits. Scientists have only recently begun to
understand the significant contribution NEOs have made to the
evolution of Earth -- and life on our planet. It is now
believed that impacts from comets and asteroids have shaped the
evolution of all planets in our solar system.
So far, more than 600 NEOs have been discovered; more than 280
of these are larger than one kilometer across. Scientists
estimate, however, that about 2,000 NEOs larger than one
kilometer and 150,000 to 100 million objects larger than 100
meters in size exist.
NEOs have collided with Earth in the past with devastating
results. The Chicxulub crater off the north coast of Mexico's
Yucatan Peninsula was created by an Earth-colliding meteor 65
million years ago, a globally devastating event that is
believed to have wiped out the dinosaurs. Even relatively small
objects impacting our planet or exploded in Earth's atmosphere
can wreak considerable havoc.
The Gene Shoemaker NEO Grants
Gene Shoemaker was a leader in the study of impact structures
and an advocate for NEO discovery and tracking programs before
his death in 1997. Shoemaker was the first scientist to
demonstrate that the mile-wide crater in Arizona -- now known
as Meteor Crater -- was the result of a catastrophic impact by
an asteroid 50,000 years ago. Prior to Shoemaker's work, Meteor
Crater was believed to be the remnant of an extinct volcano.
The Gene Shoemaker NEO Grants are awarded to amateur observers,
observers in developing countries, and professional astronomers
who, with seed funding, could greatly increase their programs'
contributions to this critical research.
Funding for the Gene Shoemaker NEO Grant program comes from the
Planetary Society's 100,000 members, whose voluntary dues and
donations permit targeted support of research and development
programs in a number of areas.
An international advisory group recommends candidates to
receive the grant awards. The advisory group includes grant
coordinator Daniel D. Durda, as well as noted near-Earth object
scientists Dr. Richard Binzel of the Massachusetts Institute of
Technology, Dr. Clark Chapman, also of the Southwest Research
Institute, Dr. Andrea Carusi of the Spaceguard Foundation, and
Dr. Brian Marsden of the Smithsonian Astrophysical Observatory.
Society-Funded ROTSE Camera Images Gamma Ray Burst The
Planetary Society has funded many NEO efforts in the past,
including start-up money for the Robotic Optical Transient
Search Experiment (ROTSE) in Los Alamos, New Mexico. Operated
by a team led by Dr. Carl Akerlof of the University of Michigan
and including astrophysicists from Los Alamos and Lawrence
Livermore National Laboratories, ROTSE recently made
astronomical history on January 23, 1999, when it discovered an
unusual transient optical signal in images of the sky where a
gamma ray burst had been reported just 22 seconds earlier.
ROTSE is a multipurpose instrument, designed to continuously
map the entire visible evening sky, collecting data that can be
examined for near-Earth objects, as well as variable stars and
supernovas as they occur. When a gamma ray burst occurs, such
as the one detected by orbiting satellites on the morning of
January 23, ROTSE interrupts its regular sky-mapping activity
and automatically swings to the sky coordinates provided by the
satellites. In only a few seconds, ROTSE began taking a new
series of many images, capturing the first gamma ray burst ever
recorded in images.
Astronomers are not certain what produces gamma ray bursts, but
possible causes include the mergers of two neutron stars, two
black holes, a neutron star and a black hole, or the explosion
of a so-called hypernova, which is theorized to be a type of
supernova or exploding star.
For more information, contact Bill McGovern or Susan
Lendroth or call The Planetary Society at (626) 793-5100
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