7-Billion-Year-Old Stardust Found in Meteorite

Presolar Grain with Nebula

Dust-rich outflows of evolved stars similar to the pictured Egg Nebula are plausible sources of the large presolar silicon carbide grains found in meteorites like Murchison. Credit: Image courtesy NASA, W. Sparks (STScI) and R. Sahai (JPL). Inset: SiC grain with ~8 micrometers in its longest dimension. Inset image courtesy of Janaína N. Ávila.

The ancient stardust reveals a “baby boom” in star formation.

Stars have life cycles. They’re born when bits of dust and gas floating through space find
 each other and collapse in on each other and heat up. They burn for millions to billions of years,
 and then they die. When they die, they pitch the particles that formed in their winds out into 
space, and those bits of stardust eventually form new stars, along with new planets and moons 
and meteorites. And in a meteorite that fell fifty years ago in Australia, scientists have now
 discovered stardust that formed 5 to 7 billion years ago—the oldest solid material ever found on 
Earth.

“This is one of the most exciting studies I’ve worked on,” says Philipp Heck, 
a curator at 
the Field Museum, associate professor at the University of Chicago, and lead author of a paper
 describing the findings that was published today (January 1, 2020) in
 PNAS
. “These are the oldest solid materials ever found, and they tell us
 about how stars formed in our galaxy.”

The materials Heck and his colleagues examined are called presolar grains—
minerals
 formed before the Sun was born. “They’re solid samples of stars, real stardust,” says Heck.



 
These bits of stardust became trapped in meteorites where they remained unchanged for billions 
of years, making
 them time capsules of the time before the solar system.

But presolar grains are hard to come by. They’re rare, found only in about five percent of
 meteorites that have fallen to Earth, and they’re tiny
—a hundred of the biggest ones would fit on 
the period at the end of this sentence. But the Field Museum has the largest portion of the 
Murchison meteorite, a treasure trove of presolar grains that fell in Australia in 1969 and that the
 people of Murchison, Victoria, made available to science. Presolar g
rains for this study were 
isolated from the Murchison meteorite for this study about 30 years ago at the University of
 Chicago.

Presolar Grain

Scanning electron micrograph of a dated presolar silicon carbide grain. The grain is ~8 micrometers in its longest dimension. Credit: Image courtesy of Janaína N. Ávila.

“It starts with crushing fragments of the meteorite down into a powder,” explains
 Jennika Greer, a graduate student at the Fi
eld Museum and the University of Chicago and co
-
author of the study. “Once all the pieces are segregated, it’s a kind of paste, and it has a pungent
 characteristic—it smells like rotten peanut butter.”

This “rotten
-
peanut
-
butter
-
meteorite paste” was then dissolved with acid, until only the 
presolar grains remained. “It’s like burning down the haystack to find the needle,” says Heck.

Once the presolar grains were isolated, the researchers figured out from what types of
 stars they came and how old they w
ere. “We used exposure age data, which basically measures 
their exposure to cosmic rays, which are high
-
energy particles that fly through our galaxy and
 penetrate solid matter,” explains Heck. “Some of these cosmic rays interact with the matter and 
form new elements. And the longer they get exposed, the more those elements form.

“I compare this with putting out a bucket in a rainstorm. Assuming the rainfall is
 constant, the amount of water that accumulates in the bucket tells you how long it was exposed,”
he adds. By measuring how many of these new cosmic
-
ray produced elements are present in a
 presolar grain, we can tell how long it was exposed to cosmic rays, which tells us how old it is.

The researchers learned that some of the presolar grains in their s
ample were the oldest 
ever discovered—based on how many cosmic rays they’d soaked up, most of the grains had to be
 4.6 to 4.9 billion years old, and some grains were even older than 5.5 billion years. For context,
 our Sun is 4.6 billion years old, and the Earth is 4.5 billion.

But the age of the presolar grains wasn’t the end of the discovery. Since presolar grains
 are formed when a star dies, they can tell us about the history of stars. And 7 billion years ago, 
there was apparently a bumper crop of new
 stars forming
—
a sort of astral baby boom.

“We have more young grains that we expected,” says Heck. “Our hypothesis is that the majority of those grains, which are 4.9 to 4.6 billion years old, formed in an episode of enhanced star formation. There was a time before the start of the Solar System when more stars formed than normal.”

This finding is ammo in a debate between scientists about whether or not new stars form at a steady rate, or if there are highs and lows in the number of new stars over time. “Some people think that the star formation rate of the galaxy is constant,” says Heck. “But thanks to these grains, we now have direct evidence for a period of enhanced star formation in our galaxy 7 billion years ago with samples from meteorites. This is one of the key findings of our study.”

Heck notes that this isn’t the only unexpected thing his team found. As almost a side note to the main research questions, in examining the way that the minerals in the grains interacted with cosmic rays, the researchers also learned that presolar grains often float through space stuck together in large clusters, “like granola,” says Heck. “No one thought this was possible at that scale.”

Heck and his colleagues look forward to all of these discoveries furthering our knowledge of our galaxy. “With this study, we have directly determined the lifetimes of stardust. We hope this will be picked up and studied so that people can use this as input for models of the whole galactic life cycle,” he says.

Heck notes that there are lifetimes’ worth of questions left to answer about presolar grains and the early Solar System. “I wish we had more people working on it to learn more about our home galaxy, the Milky Way,” he says.

“Once learning about this, how do you want to study anything else?” says Greer. “It’s awesome, it’s the most interesting thing in the world.”

“I always wanted to do astronomy with geological samples I can hold in my hand,” says Heck. “It’s so exciting to look at the history of our galaxy. Stardust is the oldest material to reach Earth, and from it, we can learn about our parent stars, the origin of the carbon in our bodies, the origin of the oxygen we breathe. With stardust, we can trace that material back to the time before the Sun.”

“It’s the next best thing to being able to take a sample directly from a star,” says Greer.

Reference: “Lifetimes of interstellar dust from cosmic ray exposure ages of presolar silicon carbide” by Philipp R. Heck, Jennika Greer, Levke Kööp, Reto Trappitsch, Frank Gyngard, Henner Busemann, Colin Maden, Janaína N. Ávila, Andrew M. Davis and Rainer Wieler, 13 January 2020, Proceedings of the National Academy of Sciences.
DOI: 10.1073/pnas.1904573117

This study was contributed to by researchers from the Field Museum, University of Chicago, Lawrence Livermore National Laboratory, Washington University, Harvard Medical School, ETH Zurich, and the Australian National University. Funding was provided by NASA, the TAWANI Foundation, the National Science Foundation, the Department of Energy, the Swiss National Science Foundation, the Brazilian National Council for Scientific and Technological Development and the Field Museum’s Science and Scholarship Funding Committee.

Share With Your Friends !

Products You May Like