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Comet Particles Tell New Story About Birth Of Solar System

Date:
December 17, 2006
Source:
Lawrence Livermore National Laboratory
Summary:
Particulate materials captured from the comet Wild two have revealed clues about the birth of our solar system that counter some of the basic theories that the solar nebular is gently collapsing inward to form the sun and the planets.

Stardust fire and ice: Livermore scientists were able to determine that this tiny mineral is osbornite using X-ray fluorescence maps and backscattered electron images (shown above). Osbornite forms much closer to the sun than where Comet Wild 2 formed on the outskirts of Neptune.
Credit: s: Hope Ishii, Stewart Fallon, Ian Hutcheon, John Bradley

Particulate materials captured from the comet Wild 2 have revealed clues about the birth of our solar system that counter some of the basic theories that the solar nebular is gently collapsing inward to form the sun and the planets.

The thousands of samples of dust, gathered from the Stardust mission, tell a story of a comet that formed in the Kuiper Belt, outside the orbit of Neptune, and only recently entered the inner regions of the solar system.

Wild 2 spent most of its life orbiting in the Kuiper Belt, far beyond Neptune, and in 1974 had a close encounter with Jupiter that placed it into its current orbit. The Stardust spacecraft's seven-year mission returned to earth earlier this year with particles that are the same material that accreted along with ice to shape the comet about 4.57 billion years ago, when the sun and planets formed.

But during its lifetime, Wild 2 gathered material that formed much closer to the sun.

"We're talking about a mineral that forms around 3,000 degrees Kelvin, which means it formed close to the hot infant star," said John Bradley, director of the Laboratory's Institute for Geophysics and Planetary Physics and the head of the Livermore Stardust team. "If we found it in the comet, then how the heck did it get out there""

The mineral in question is osbornite, which only has been found on earth in Russia.

More than 200 investigators worldwide including researchers from Lawrence Livermore will publish several papers in a series of analyses of the space dust in the Dec. 15 issue of the journal Science.

By using state-of-the-art technology, scientists from Lawrence Livermore National Laboratory have been able to determine the make-up of the tiny particles at the angstrom scale using the SuperSTEM (scanning transmission electron microscope).

The osbornite finding is an indication that during its infancy, the solar system was a very volatile locale in which objects in the inner area may have been ejected in bipolar outflows perpendicular to the solar accretion disc and rained down into the outer regions.

"It appears to have been a much more dynamic and perhaps even violent nebula environment than we expected," Bradley said.

And it is this mixing of the solar system that initially had scientists scratching their heads. In addition to outer solar system materials, the comet samples also contain pre-solar materials that in turn mean they must have been transported beyond the orbit of Neptune by a process that was capable of moving particles at least as large as 20 microns (a micron is 10 times smaller than a human hair).

The osbornite discovery supports the theory that large particles could be launched by a type of wind from a region within a few radii of the young sun and ballistically be transported above and below the midplane of the nebular disk. This wind model would transport these hot-formed particles from near the sun to the edge of the solar system where Wild 2 formed.

Most of the particles larger than a micron are made up of the silicate minerals olivine and pyroxene, also minerals that form at very high temperatures.

"It's shaking up our view of the solar system condensation process," said Hope Ishii, one of the Livermore Stardust researchers. "It's been pretty intense. It opens up a whole bunch of new questions."

In addition to the SuperSTEM, Livermore researchers used the Laboratory's secondary electron microscope, nanoSIMS and Focused Ion Beam (FIB) technology to analyze the dust particles. Using the FIB, Livermore researchers Giles Graham and Nick Teslich were the first scientists to detect the craters containing miniscule particles in the collector foil. The foils contained the only examples found thus far of presolar material.

In addition to silicates and sulfides, Stardust samples contain organic materials dispersed around the impacts.

"We didn't expect any organics to survive" from the impact and heat during the collection process, said Livermore researcher Sasa Bajt. "But we found a rich variety of organics that were both oxygen-rich and nitrogen rich compared to organics previously found in meteorites."

And those organics could point to the beginnings of life on Earth.

Stardust is a part of NASA's series of Discovery missions and is managed by the Jet Propulsion Laboratory. Stardust launched in February 1999 and set off on three giant loops around the sun. It began collecting interstellar dust in 2000 and met Wild 2 in January 2004, when the spacecraft was slammed by millions of comet particles, nearly halting the mission. It is the first spacecraft to safely make it back to Earth with cometary dust particles in tow.


Story Source:

The above story is based on materials provided by Lawrence Livermore National Laboratory. Note: Materials may be edited for content and length.


Cite This Page:

Lawrence Livermore National Laboratory. "Comet Particles Tell New Story About Birth Of Solar System." ScienceDaily. ScienceDaily, 17 December 2006. <www.sciencedaily.com/releases/2006/12/061215123117.htm>.
Lawrence Livermore National Laboratory. (2006, December 17). Comet Particles Tell New Story About Birth Of Solar System. ScienceDaily. Retrieved October 20, 2014 from www.sciencedaily.com/releases/2006/12/061215123117.htm
Lawrence Livermore National Laboratory. "Comet Particles Tell New Story About Birth Of Solar System." ScienceDaily. www.sciencedaily.com/releases/2006/12/061215123117.htm (accessed October 20, 2014).

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