Planetary Society Protests Stop to Near-Earth Object Observations
by Susan Lendroth
The Planetary Society strongly condemns NASA's decision, announced today, December 19, 2001, to terminate radar observations of Near Earth Objects (NEOs) from the Arecibo Observatory in Puerto Rico. Arecibo is the most powerful radio observatory on Earth and is the most accurate instrument we have for studying NEOs.
NASA made its decision because of being inadequately funded to meet a congressionally mandated goal of detecting all objects larger than one kilometer in near-Earth orbits by 2008.
"Arecibo radar observations are crucial for determining the exact location, speed and direction of objects that approach Earth," said Louis Friedman, Executive Director of The Planetary Society. "We need this information to know how significant the probability is of any one asteroid hitting the Earth. It is irresponsible for Congress to mandate that NASA undertake asteroid and comet detection, and then to not provide sufficient funds for that program."
The Arecibo Observatory in Puerto Rico and the Goldstone Tracking Station in Barstow California, which is part of the Deep Space Network, are the only two radar sites capable of asteroid observations. Goldstone is not as powerful as Arecibo and is very busy supporting spacecraft missions.
The funding problem arose when funds to provide facility support at Arecibo had to be taken out of the asteroid observation program in NASA. That program includes the high-priority optical telescope searches for Near-Earth Objects, a class of bodies that includes asteroids and comets whose orbits carry them close by our planet.
Radar observations provide the very accurate position and velocity information necessary to determining the orbits and predicting the future paths for the objects that come very close to Earth.
"The decision to eliminate these Arecibo observations, and not obtain precision data, is very short-sighted," commented Friedman. "If an object is discovered headed to Earth, we are certainly going to wish we had the ability to track it accurately."
In addition to providing detailed position and velocity information, the Arecibo observations also are often the only way to characterize the NEO's shape and rotation. This information is critical to the science of NEOs, and to understanding their origin and evolution, and the important role they have played in the evolution of terrestrial planets.
A NEO that struck the Earth 65 million years ago triggered the extinction of the dinosaurs and most species then flourishing. Another such object could come our way at any time.
THE PLANETARY SOCIETY:
Carl Sagan, Bruce Murray and Louis Friedman founded The Planetary Society in 1980 to advance the exploration of the solar system and to continue the search for extraterrestrial life. With members in over 140 countries, the Society is the largest space interest group in the world.
Item of Interest
For more information about The Planetary Society, contact Susan Lendroth at (626) 793-5100 ext 237 or by e-mail at email@example.com.
2002 Presidential Award for Excellence in Mathematics and Science Teaching
Do you know a great mathematics or science teacher?
Encourage them to apply for the 2002 Presidential Award for Excellence in Mathematics and Science Teaching (PAEMST), the nation's highest honor for mathematics and science teachers in grades K through 12. The application deadline is April 1, 2002.
Each year, after an initial selection process at the state or territorial level, a national panel of distinguished scientists, mathematicians and educators recommends teachers to receive a presidential award - one elementary and one secondary math teacher and one elementary and one secondary science teacher from each jurisdiction. Awardees each receive a $7,500 educational grant for his or her school, a presidential citation and a trip to Washington, D.C. for a series of recognition events.
A new video component in the application process will be used this year in many states. The video component will be used in all jurisdictions next year. Applications are available on the following web site: