Forum for Science, Industry and Business

Sponsored by:     3M 
Search our Site:

 

Stardust in the laboratory

21.02.2006


Space science discoveries are being made in earthly labs



Reaching for the stars isn’t so out of reach these days. With the development of increasingly sophisticated instruments, researchers not only are able to get more detailed information about circumstellar and interstellar dust from afar by using advanced telescopes, but they also are now able to study actual stardust right in their own labs.

Since the discovery two decades ago that primitive meteorites contain microscopic grains of preserved stardust, physicists, chemists, astrophysicists and astronomers have taken advantage of this interstellar material that falls to Earth.


With new and ever-improving instruments to analyze these grains in the laboratory, researchers around the world are gaining new insights into the formation of the elements and the evolution of stars.

And with the successful January 2006 completion of NASA’s seven-year 2.88 billion mile round-trip Stardust mission to collect cometary and interstellar dust particles, researchers worldwide will be busy analyzing these samples for years to come looking for answers to fundamental questions about comets and the origin of the solar system.

Ernst K. Zinner, Ph.D., research professor of physics and of earth and planetary sciences, both in Arts & Sciences, at Washington University in St. Louis, provided an overview of the study of "Stardust in the Laboratory" Monday, Feb. 20, 2006, at the annual meeting of the American Association for the Advancement of Science (AAAS), held in St. Louis. He also participated in the AAAS "Exploring a Dusty Cosmos" press briefing that morning.

Zinner, the recipient of both the National Academy of Sciences’ J. Lawrence Smith Medal and the Meteoritical Society’s Leonard Medal, is a pioneer in the analysis of stellar dust grains found in primitive meteorites.

In 1987, Zinner and colleagues at Washington University and a group of scientists at the University of Chicago found the first stardust in a meteorite. Those presolar grains were specks of diamond and silicon carbide.

Since then, Zinner and other members of WUSTL’s Laboratory for Space Sciences’ research group have played leading roles in analyzing these grains in the laboratory and interpreting the results. The Laboratory for Space Sciences is part of the departments of Physics and Earth and Planetary Sciences and the McDonnell Center for the Space Sciences, all in Arts & Sciences.

It is generally believed that these grains were formed billions of years ago in the atmospheres of dying stars. "As a star dies," Zinner explains, "its atmosphere begins to expand and cool. Then ions turn into atoms, atoms form molecules and, eventually, molecules condense into grains."

The dust then is ejected into outer space, where it collects with gas and dust from other stars to form cold, dark clouds.

More than 4.5 billion years ago, one such cloud collapsed to form our solar system, and the dust -- literally pieces of distant and long-dead stars -- was preserved in meteorites.

By studying the isotopic composition of these grains, researchers are gaining new information on nuclear and chemical processes in stars and on conditions during the formation of the solar system.

Advancements in instrumentation

Using a microanalytic instrument called an ion microprobe to measure the proportions of specific isotopes, Zinner and his colleagues in the late 1980s and ’90s identified three types of interstellar grains -- silicon carbide, graphite and aluminum oxide -- and two important stellar sources of the grains.

The researchers determined through signature isotopic compositions that the grains came from red giant stars of low to medium mass during late stages of their evolution and from supernovae, massive stars that exploded at the end of their evolution.

These grains, Zinner explains, condensed when the envelope of red giants cooled during expansion or when supernovae exploded, thus preserving the elemental and isotopic composition of their stellar sources.

Zinner adapted the microprobe to permit precise isotopic measurements in samples weighing as little as a millionth of a millionth of a gram.

Isotopes are versions of an element that have different numbers of neutrons and, consequently, different masses. In the same way that a zoologist studies a set of footprints to learn about the animal that made them, Zinner and his colleagues study the isotopes in a grain to learn about the parent star -- its mass, age, composition and other characteristics.

The latest ion microprobe on the scene is the NanoSIMS (SIMS is short for Secondary Ion Mass Spectrometer), which can resolve objects smaller than a micrometer -- one millionth of a meter -- or 1/100th smaller than the diameter of a human hair.

Zinner and Frank J. Stadermann, Ph.D., senior research scientist in the Department of Physics in Arts & Sciences, helped design and test the NanoSIMS, which is made by CAMECA in Paris. At a cost of $2 million, Washington University acquired the first NanoSIMS in the world in 2000. There are now some 16 worldwide.

Ion probes direct a beam of ions onto one spot on a sample. The beam dislodges some of the sample’s own atoms, some of which become ionized. This secondary beam of ions enters a mass spectrometer that is set to detect a particular isotope. Thus, ion probes can identify grains that have an unusually high or low proportion of that isotope.

Unlike most other ion probes, however, the NanoSIMS can detect five different isotopes simultaneously. The beam can also travel automatically from spot to spot so that many hundreds or thousands of grains can be analyzed in one experimental setup.

Using the NanoSIMS, Ann Nguyen, Ph.D., at the time a WUSTL graduate student under Zinner, persevered -- after a WUSTL team had already sifted through 100,000 grains looking for a particular type of stardust without success -- and found the first silicate stardust in a meteorite.

In the March 5, 2004, issue of Science, Nguyen and Zinner describe nine specks of silicate stardust -- presolar silicate grains -- from one of the most primitive meteorites known. Silicate is a compound of silicon, oxygen and other elements such as magnesium and iron. Nguyen is now a postdoctoral research associate in the Department of Terrestrial Magnetism at the Carnegie Institution in Washington, D.C.

"Finding presolar silicates in a meteorite tells us that the solar system formed from gas and dust, some of which never got very hot, rather than from a hot solar nebula," Zinner says. "Analyzing such grains provides information about their stellar sources, nuclear processes in stars and the physical and chemical compositions of stellar atmospheres.

"The NanoSIMS was essential for this discovery," Zinner says. "These presolar silicate grains are very small -- only a fraction of a micrometer. The instrument’s high spatial resolution and high sensitivity made these measurements possible."

This detailed information about stardust proves that space science can be done in the laboratory, Zinner says. "Analyzing these small specks can give us information, such as detailed isotopic ratios, that cannot be obtained by the traditional techniques of astronomy," he adds.

Other instrumentation being used for studying very small particles include various kinds of mass spectrometers for chemical and isotopic analysis and radioactive dating, electron microscopes for chemical and structural analysis, and chemical and physical apparatus geared to the processing of microscopic material.

Zinner and Stadermann’s current project will be analyzing the three slices of a cometary dust particle they recently received from the Stardust mission -- the first U.S. mission since Apollo 17 in 1972 to bring back extraterrestrial material.

Susan Killenberg McGinn | EurekAlert!
Further information:
http://www.wustl.edu

More articles from Physics and Astronomy:

nachricht Further Improvement of Qubit Lifetime for Quantum Computers
09.12.2016 | Forschungszentrum Jülich

nachricht Electron highway inside crystal
09.12.2016 | Julius-Maximilians-Universität Würzburg

All articles from Physics and Astronomy >>>

The most recent press releases about innovation >>>

Die letzten 5 Focus-News des innovations-reports im Überblick:

Im Focus: Electron highway inside crystal

Physicists of the University of Würzburg have made an astonishing discovery in a specific type of topological insulators. The effect is due to the structure of the materials used. The researchers have now published their work in the journal Science.

Topological insulators are currently the hot topic in physics according to the newspaper Neue Zürcher Zeitung. Only a few weeks ago, their importance was...

Im Focus: Significantly more productivity in USP lasers

In recent years, lasers with ultrashort pulses (USP) down to the femtosecond range have become established on an industrial scale. They could advance some applications with the much-lauded “cold ablation” – if that meant they would then achieve more throughput. A new generation of process engineering that will address this issue in particular will be discussed at the “4th UKP Workshop – Ultrafast Laser Technology” in April 2017.

Even back in the 1990s, scientists were comparing materials processing with nanosecond, picosecond and femtosesecond pulses. The result was surprising:...

Im Focus: Shape matters when light meets atom

Mapping the interaction of a single atom with a single photon may inform design of quantum devices

Have you ever wondered how you see the world? Vision is about photons of light, which are packets of energy, interacting with the atoms or molecules in what...

Im Focus: Novel silicon etching technique crafts 3-D gradient refractive index micro-optics

A multi-institutional research collaboration has created a novel approach for fabricating three-dimensional micro-optics through the shape-defined formation of porous silicon (PSi), with broad impacts in integrated optoelectronics, imaging, and photovoltaics.

Working with colleagues at Stanford and The Dow Chemical Company, researchers at the University of Illinois at Urbana-Champaign fabricated 3-D birefringent...

Im Focus: Quantum Particles Form Droplets

In experiments with magnetic atoms conducted at extremely low temperatures, scientists have demonstrated a unique phase of matter: The atoms form a new type of quantum liquid or quantum droplet state. These so called quantum droplets may preserve their form in absence of external confinement because of quantum effects. The joint team of experimental physicists from Innsbruck and theoretical physicists from Hannover report on their findings in the journal Physical Review X.

“Our Quantum droplets are in the gas phase but they still drop like a rock,” explains experimental physicist Francesca Ferlaino when talking about the...

All Focus news of the innovation-report >>>

Anzeige

Anzeige

Event News

ICTM Conference 2017: Production technology for turbomachine manufacturing of the future

16.11.2016 | Event News

Innovation Day Laser Technology – Laser Additive Manufacturing

01.11.2016 | Event News

#IC2S2: When Social Science meets Computer Science - GESIS will host the IC2S2 conference 2017

14.10.2016 | Event News

 
Latest News

Researchers identify potentially druggable mutant p53 proteins that promote cancer growth

09.12.2016 | Life Sciences

Scientists produce a new roadmap for guiding development & conservation in the Amazon

09.12.2016 | Ecology, The Environment and Conservation

Satellites, airport visibility readings shed light on troops' exposure to air pollution

09.12.2016 | Health and Medicine

VideoLinks
B2B-VideoLinks
More VideoLinks >>>