Rare, but not impossible...
Last month, astronomers were studying pictures of asteroid 433 Eros when they noticed some unusual craters. Most impact craters are circular, but these were square!
Right: NASA's NEAR-Shoemaker spacecraft spotted these square-shaped craters on asteroid 433 Eros. [more information]
An overzealous fan of Star Trek might mistake the impact scars for places where cube-shaped Borg vessels touched down and lifted off again, but scientists say they are natural -- albeit unusual -- features.
Square craters add to accumulating evidence that Eros is riddled with cracks and ridges that extend the entire 33 km length of the peanut-shaped space rock. "We first saw long grooves in global pictures of the asteroid when NEAR was entering orbit around Eros in February 2000," continued Cheng. "Now, if we look carefully, most of the closeup pictures seem to show signs of grooves and ridges."
"We have to ask ourselves how these cracks could have formed. Presumably they are the result of large impacts. The question is: did these impacts take place after Eros was its present size and shape or while Eros was part of a larger parent body?"
It's a question that goes to the heart of the asteroid's origin.
Scientists believe that billions of years ago, when the solar system was young and planets were newly-forming, Eros circled the Sun in an orbit between Mars and Jupiter. It was a denizen of the asteroid belt. Since then, collisions with other asteroids and gravitational perturbations by Mars and Jupiter have altered Eros's orbit, so that now it comes close enough to Earth to study with spacecraft like NEAR.
Above: The Barringer "Meteor Crater" on Earth has a square-shaped rim, indicative of fractured terrain around the impact site. [more information].
"If continued mapping confirms that faults and ridges extend from one end of Eros to the other, I would consider it to be strong evidence that Eros is a piece of something that was once much larger," says Cheng. If all of the rocks in the modern-day asteroid belt were assembled, they would form a small planet about 1500 km in diameter -- roughly half the size of Earth's moon. Such a body might have existed in an orbit between Mars and Jupiter billions of years ago, before it shattered as a result of collisions with other planetoids.
But if Eros is a "chip off the old block," there's a new mystery to consider. When rocky planets like the Earth and its moon (and maybe the parent body of Eros) are formed, heavier elements sink to the core while lighter ones remain near the crust. This leads to a core-mantle structure with distinctive chemical signatures in each layer.
The looming conundrum is that Eros does not exhibit the chemical signatures of differentiation. NEAR X-ray spectrometer data show that aluminum, magnesium, and silicon on Eros have the same relative abundances that they do in the Sun and in the early solar nebula. Evidently, Eros was not part of a body that experienced the Earth-like process of heating and segregation of metals from silicates to form an iron core and rocky mantle.
"Eros is an example of a very primitive body ... nothing much has happened to it other than formation and cratering. If you want the most pristine material in the solar system [where very little has happened] Eros is a good example," says Joe Veverka, professor of astronomy at Cornell University, and the principal investigator for two of NEAR's cameras.
"Even before we visited Eros we knew that asteroids were a mixed group -- some appear to be differentiated and some not," says Cheng. "The largest asteroid of all, 933 km-wide Ceres, is not differentiated. Yet, we believe it's possible for objects even smaller than Ceres to melt and chemically segregate. We simply don't know why some asteroids appear to be more primitive than others. We have to reserve a little skepticism here and pursue this mystery."
Above: This global mosaic of asteroid Eros shows some of the grooves that hint at fractures and faults that may permeate the rocky asteroid. [more information]
Cheng says that a global map of Eros's grooves and ridges -- and possibly more square craters -- will likely shed new light on the asteroid's history. For now researchers and asteroid enthusiasts wait with anticipation as NEAR Shoemaker continues its first-ever and often surprising survey 433 Eros, knowing that the best answers and most perplexing mysteries may be yet to come.
For more information about asteroid Eros and the NEAR mission, please visit the Near-Earth Asteroid Rendezvous mission home page at http://near.jhuapl.edu. The Johns Hopkins University Applied Physics Laboratory in Laurel, MD, designed and built the NEAR spacecraft and manages the mission for NASA.Web Links
Near Earth Asteroid Rendezvous mission - NEAR home page from Johns Hopkins University Applied Physics Laboratory
Eros or Bust - February 8, 2000. SpaceScience.com. NASA's Near-Earth Asteroid Rendezvous Mission is nearing 433 Eros. It is scheduled to go into orbit around the space rock on Valentines Day, 2000. University
Guess Who's Coming to Breakfast? - February 13, 2000. SpaceScience.com. Critical science observations of Eros are scheduled to begin 11 hours before NEAR's orbit insertion on Valentines Day, 2000.
First Orbit Around an Asteroid - February 14, 2000. SpaceScience.com. NEAR successfully entered orbit around 433 Eros on Valentines Day, 2000
Highlights from Asteroid Eros - February 19, 2000. SpaceScience.com. Scientists review exciting results from the first few days in orbit.
NEARer to Eros - February 25, 2000. SpaceScience.com. NEAR moves closer to Eros.
Wanted: a few good solar flares - March 3, 2000. SpaceScience.com. Solar radiation could reveal new details about Eros
NEAR Shoemaker -- Mar. 14, 2000. SpaceScience.com. NASA has renamed the Near Earth Asteroid Rendezvous (NEAR) spacecraft for planetary science pioneer Gene Shoemaker.
Earth's Seasons -- A table of solstices and equinoxes from the US Naval Observatory
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|For lesson plans and educational activities related to breaking science news, please visit Thursday's Classroom||Author: Dr. Tony Phillips
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