Gamma-rays from an Asteroid
Gamma-Rays from an Asteroid Perched on the surface of asteroid 433 Eros, NASA's
NEAR spacecraft is beaming back measurements of gamma-rays leaking
from the space rock's dusty soil.
Listen to this story (requires RealPlayer)
February 27, 2001 -- When NASA's Near Earth Asteroid Rendezvous (NEAR) spacecraft left for asteroid 433 Eros five years ago, scientists weren't certain what they would find when the probe arrived. Was Eros a 30-km fragment from a planet that broke apart billions of years ago? Or perhaps a jumble of space boulders barely held together by gravity? Was Eros young or old, tough or fragile ... no one knew for sure.
But now, after a year in orbit and a daring landing on the asteroid itself, NEAR Shoemaker is beaming back data that could confirm what many scientists have lately come to believe: Asteroid Eros is not a piece of some long-dead planet or a loose collection of space debris. Instead, it's a relic from the dawn of our solar system, one of the original building blocks of planets that astronomers call "planetesimals."
As NEAR Shoemaker was heading for its historic landing on Feb. 12, 2001, team members hoped the spacecraft --which was designed to orbit, not land-- would simply survive. When it did survive, they set their sights a little higher. From its perch on the surface of the asteroid, NEAR's gamma-ray spectrometer (GRS) can detect key chemical signatures of a planetesimal -- data that scientists are anxious to retrieve.
"The gamma-ray instrument is more sensitive on the ground than it was in orbit," says Goddard's Jack Trombka, team leader for the GRS. "And the longer we can accumulate data the better." NASA recently gave the go-ahead for NEAR's mission to continue through Feb. 28th, tacking four days onto an extension granted just after the spacecraft landed.
"Cosmic rays shatter atomic nuclei in the asteroid's soil," explains Trombka. Neutrons that fly away from the cosmic ray impact sites hit other atoms in turn. "These secondary neutrons can excite atomic nuclei (by inelastic scattering) without breaking them apart." Such excited atoms emit gamma-rays that the GRS can decipher to reveal which elements are present.
"We can detect cosmic-ray excited oxygen, iron and silicon, along with the naturally radioactive elements potassium, thorium and uranium," says Trombka. Measuring the abundances of these substances is an important test of the planetesimal hypothesis.
Planetesimals came to be when the solar system was just a swirling interstellar cloud, slowly collapsing to form the Sun and planets. Dust grains condensed within that primeval gas. The grains were small, but by hitting and sticking together they formed pebble-sized objects that fell into the plane of the rotating nebula. The pebbles accumulated into boulders, which in turn became larger bodies, 1 to 100 km wide. These were planetesimals -- the fundamental building blocks of the planets.
Left: Scientist and artist William K. Hartmann (copyright 2001, all rights reserved) created this painting of the inner solar system as it may have been less than 1 million years after the Sun formed. Dust grains are accumulating into asteroid-sized planetesimals, the building blocks of planets.
Fully-developed planets like Earth are chemically segregated -- that is, they have heavier elements near their cores and lighter ones at the surface. Planetary scientists call this "differentiation." If Eros were a chip from a planet that broke apart, perhaps in the asteroid belt, it would exhibit chemical signatures corresponding to some layer from a differentiated world.
For example, Eros might be iron-rich if it came from the core of such a planet or silicon-rich if it came from the crust.
Instead, "orbital data from the x-ray spectrometer (a low-energy cousin of the GRS) showed Eros is very much like a type of undifferentiated meteorite we find on Earth called ordinary chondrites," says Andrew Cheng, the NEAR project scientist at Johns Hopkins University Applied Physics Laboratory (APL), which manages the mission for NASA.
Eros seems to harbor a mixture of elements that you would
only find in a solar system body unaltered by melting (an unavoidable
step in the process of forming rocky planets). But, says Cheng,
there is a possible discrepancy.
"The abundance of the element sulfur on Eros is less than we would expect from an ordinary chondrite. However, the x-ray spectra tell us only about the uppermost hundred microns of the surface, and we do not know if the sulfur depletion occurs only in a thin surface layer or throughout the bulk of the asteroid."
The GRS can go deeper, as much as 10 cm below the surface. Although the instrument can't detect sulfur, it is sensitive to gamma-ray emissions from other elements such as radioactive potassium that are indicators of melting. Like sulfur, potassium is a volatile element -- it easily evaporates when a rock is heated. Finding plenty of potassium would strengthen the conclusion that Eros is an unmelted and primitive body.
On the other hand, a widespread dearth of "volatiles" would hint that Eros isn't so primitive after all.
Above: NEAR Shoemaker's X-ray/Gamma-ray Spectrometer [more]
It might sound like an ivory-tower question, but knowing the makeup of this asteroid -- both its internal structure and its chemical composition-- has a practical application. The solar system is littered with space rocks more or less like Eros, and many come uncomfortably close to Earth. One day we may need to blow one apart (or deflect one without blowing it apart) to avoid an unpleasant collision. Near-Earth asteroids are also potential mining resources as humans expand into space. In either case, knowing more about them is a good idea!
"Our first four data sets are here and they look great," says Jack Trombka. "John Goldsten, the lead engineer for the gamma-ray spectrometer at the Johns Hopkins Applied Physics Laboratory, has done a fabulous job making the instrument work on the surface, which is a different environment than orbit.
"We're just hoping to get as much data as we can before the mission ends."
NEAR Shoemaker launched on Feb. 17, 1996 - the first in NASA's Discovery Program of low-cost, scientifically focused planetary missions -- and became the first spacecraft to orbit an asteroid on Feb. 14, 2000. The car-sized spacecraft gathered 10 times more data during its orbit than originally planned, and completed all the mission's science goals before its controlled descent on February 12, 2001. Funding for the mission extension comes from the NEAR project.Web Links
Near Earth Asteroid Rendezvous mission - NEAR home page from Johns Hopkins University Applied Physics Laboratory
A Close Encounter with Asteroid Eros - Oct. 26, 2000 Science@NASA story: NASA's NEAR Shoemaker spacecraft swooped 3 miles above the surface of 433 Eros on Oct 26th, marking its closest-ever approach to the tumbling space rock.
Square Craters -- September 26, 2000 Science@NASA story: NASA's NEAR Shoemaker spacecraft has spotted square-shaped craters on asteroid Eros, a telltale sign of mysterious goings-on in the asteroid belt long ago.
Asteroids Have Seasons, Too - June 21, 2000 Science@NASA story: Later this week, the Sun will rise over the south pole of asteroid Eros, revealing unexplored terrain to the instruments on NASA's NEAR-Shoemaker spacecraft.
circles the Sun once every 1.76 Earth years. It spins on its
axis once every 5.27 hours.[more]
Join our growing list of subscribers - sign up for our express news delivery and you will receive a mail message every time we post a new story!!!
|The Science and Technology Directorate at NASA's Marshall Space Flight Center sponsors the Science@NASA web sites. The mission of Science@NASA is to help the public understand how exciting NASA research is and to help NASA scientists fulfill their outreach responsibilities.|
|For lesson plans and educational activities related to breaking science news, please visit Thursday's Classroom||
Production Editor: Dr. Tony Phillips
Curator: Bryan Walls
Media Relations: Steve Roy
Responsible NASA official: Ron Koczor