Contact: James V. Scotti, 520-621-2717, email@example.com
TUCSON, Ariz. -- A unique near-Earth asteroid discovered last year by Spacewatch at the Univerity of Arizona in Tucson is the fastest-spinning solar system object yet found, scientists report in today's issue (July 23) of Science.
Only 30 meters (100 feet) across, asteroid 1998 KY26 spins once every 10.7 minutes. That’s 10 times faster than the spin rate of any other object and almost 60 times faster than the average of all known asteroid rotation periods, the scientists say.
Whirling at that speed and given its size, 1998 KY26 has to be a strong, single chunk of rock that was sent reeling from its parent asteroid in some space collision, said James V. Scotti , a senior research specialist at the UA Lunar and Planetary Laboratory (LPL) and a co-author of the Science paper.
LPL Professor Tom Gehrels, Spacewatch co-founder, discovered asteroid 1998 KY26 on May 28, 1998, using the 0.9 meter (36-inch) Spacewatch telescope at Kitt Peak, Ariz. Six nights later Scotti, joined at the Spacewatch telescope by Dan Durda, took 111 images of the asteroid, measuring its minimum to maximum changes in brightness. Durda of the Southwest Research Institute in Boulder, Co., was formerly with LPL.
Astronomers at telescopes in the Czech Republic, Hawaii and California also made the same kind of photometric measurements from June 2 to 8. This was when the asteroid made its closest swing by Earth at a half million miles, or twice the distance between the Earth and the moon. Between June 6 and 8, Steven J. Ostro headed a team from the NASA Jet Propulsion Laboratory in Pasadena, Calif., that used the Goldstone X- band radar of NASA’s Deep Space Network to track the asteroid. Radar echoes revealed the asteroid’s rapid spin rate. Petr Pravec of Ondrejov Astronomy Institute in the Czech Republic combined data gathered by the different optical observing groups and constructed a light curve to determine the precise rotation rate.
The astronomers discovered the size and shape of 1998 KY26 from the radar echoes. This asteroid is unusual in that it is almost spherical, with a bare-rock surface pocked at least in part by meteoroid bombardment, they report. Their optical and radar observations show this asteroid is similar to carbonaceous chondritic meteorites, objects that formed early in solar system history. These meteorites are rich in primordial complex organic compounds and water.
Asteroids in the 30-meter-diameter range survive between 10 million and 100 million years before being destroyed in space collisions. Carbonaceous chondrites are weaker meteorites, so this asteroid will be smashed sooner than later, they add.
Information from recent asteroid flybys suggest that large asteroids are less dense than the meteorites recovered and measured on Earth. Scientists theorize that most larger asteroids are porous "rubble piles" rather than monolithic bodies, Scotti said. Current theory says that "these rubble piles are conglomerates of debris broken apart by multiple collisions and held together by their mutual gravity, spinning slowly enough so that they don’t fall apart," he added.
Studying the detailed structure of these asteroids involves more than just scientific curiosity, Scotti said. There are two practical reasons for learning more about them: Asteroid minerals can provide raw materials for future space construction, and knowing how asteroids are put together provides critical knowledge for deflecting large ones headed for Earth.
Each month, Spacewatch – the world’s first telescope dedicated to searching for near-Earth asteroids – finds an average of two-to-three asteroids in our vicinity, and another 2,000 new ones in the asteroid belt. Spacewatch is funded by NASA, the University of Arizona and private donors.
The above post is reprinted from materials provided by University Of Arizona. Note: Materials may be edited for content and length.
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