Stardust that formed to up to seven billion years ago and fell to Earth in a meteorite during the 20th century is now believed to the oldest solid material ever found.
Stars are born when dust and gas floating through space find each other, collapse in on each other and heat up.
After burning for millions of years they die and throw particles that formed in their winds out into space.
Those bits of stardust eventually form new stars, along with new planets and moons and meteorites.
Lead author Philipp Heck, a curator at the Field Museum, and associate professor at the University of Chicago, said: ‘This is one of the most exciting studies I’ve worked on.
A view of the stellar substance (Source: PA)
‘These are the oldest solid materials ever found, and they tell us about how stars formed in our galaxy.’
The materials examined in the study published in Proceedings of the National Academy of Sciences are called presolar grains-minerals formed before the Sun was born.
‘They’re solid samples of stars, real stardust,’ said Professor Heck.
The material formed more than seven billion years ago (Source: PA)
However, presolar grains are tiny and rare, only found in about 5% of meteorites that have fallen to Earth.
But the Field Museum has the largest portion of the Murchison meteorite, a treasure trove of presolar grains that fell in Victoria, Australia, in 1969.
Presolar grains for this study were isolated from the Murchison meteorite about 30 years ago at the University of Chicago.
The process involves crushing fragments of the meteorite into a powder.
Co-author Jennika Greer, a graduate student at the Field Museum and the University of Chicago, said: ‘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.
Researchers compared the process to burning down a haystack to find the needle.
Once the presolar grains were isolated, the researchers figured out from what types of stars they came and how old they were.
Exposure age data allowed the researchers to measure their exposure to cosmic ray.
By measuring how many of the new cosmic-ray produced elements are present in a pre-solar grain, scientists can tell how long it was exposed to cosmic rays, telling them how old it is.
The researchers learned that some of the presolar grains in their sample were the oldest ever discovered on Earth.
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