Extract from ABC News
A 7-billion-year-old grain of stardust — older than our solar system —
has been discovered inside a meteorite by an international team of
scientists.
This makes it the oldest solid material found on Earth the researchers said. It's even older than our Earth and the Sun, which are 4.5 and 4.6 billion years old, respectively.
And this stardust has an Australian connection.
It was extracted from the Murchison meteorite, which fell to Earth in the Victorian country town of Murchison in 1969.
"This meteorite is really a treasure trove for science," said cosmochemist Philipp Heck, of the Field Museum in Chicago, who was the lead author of the paper published today in the Proceedings of the National Academy of Sciences.
The stardust is made of grains of presolar silicon carbide, a mineral formed before our solar system was born.
"The presolar grains are a tiny fraction of meteorites like Murchison, only parts per million," Dr Heck said.
"We use a chemical recipe of different chemical reagents, mainly acids, to dissolve away everything else, and then we extract those minerals.
"We image them, we analyse their isotopic composition to find out what type of star they came from, and then we can start our study … to find out how old they are."
The ratios of carbon-12 to carbon-13 isotopes in these grains were a perfect match to what astronomers have observed in the clouds of dust and gas around ageing stars like the Egg Nebula and the Ring Nebula.
But unfortunately, traditional dating methods geochemists use on Earth don't work when you're dating stardust, Dr Heck said.
Instead the researchers measured how long the grains have been exposed to the cosmic rays shooting through the universe.
When a cosmic ray —a stream of high energy particles, mainly protons and alpha particles — penetrates a presolar grain it occasionally splits one of its carbon atoms into fragments.
By counting all the fragments produced by the cosmic rays, and knowing how often they are produced, scientists can work out how old the stardust is.
"Each grain probably came from a different star," Dr Heck said.
"We have some grains which are a billion years older than the Sun, making them 5.5 billion years old … a few grains that are 2 billion years older and we have one grain that is 3 billion years older [than the Sun].
The cosmic ray method doesn't give us an absolute age of the stardust, said planetary scientist and meteorite hunter Phil Bland of Curtin University, who wasn't involved in the research.
But it's our best approximation so far.
While some astronomical models assume stars form at a constant rate, Dr Heck and his colleagues' work shows that isn't the case.
"In order to explain our age distribution, where we have many more younger grains that we would otherwise expect, we have to explain this by this dust forming from more stars than normal," he said.
"We came to the conclusion that about 7 billion years ago there must have been an episode of enhanced star formation, probably about 50 per cent more stars formed than normal."
Or in other words, a star-making baby boom.
And that's a fascinating result, Professor Bland said.
"That peak in star formation about 7 billion years ago … is really interesting because there's a target that other people can chase," Professor Bland said.
Now he said, we need more statistics from a different meteorite.
"What I would do now is pick another sample and go through the same process and say 'Okay, do we find that same distribution of stuff or is there something weird about this one?'."
For Dr Heck, this latest research is one of the most exciting studies he's worked on, but he's sure it won't be the last.
"Murchison is so important, and so rich and full of surprises," he said.
This makes it the oldest solid material found on Earth the researchers said. It's even older than our Earth and the Sun, which are 4.5 and 4.6 billion years old, respectively.
And this stardust has an Australian connection.
It was extracted from the Murchison meteorite, which fell to Earth in the Victorian country town of Murchison in 1969.
"This meteorite is really a treasure trove for science," said cosmochemist Philipp Heck, of the Field Museum in Chicago, who was the lead author of the paper published today in the Proceedings of the National Academy of Sciences.
How do you date stardust?
First of all, you have to get the stardust out of the meteorite.The stardust is made of grains of presolar silicon carbide, a mineral formed before our solar system was born.
"We use a chemical recipe of different chemical reagents, mainly acids, to dissolve away everything else, and then we extract those minerals.
"We image them, we analyse their isotopic composition to find out what type of star they came from, and then we can start our study … to find out how old they are."
The ratios of carbon-12 to carbon-13 isotopes in these grains were a perfect match to what astronomers have observed in the clouds of dust and gas around ageing stars like the Egg Nebula and the Ring Nebula.
But unfortunately, traditional dating methods geochemists use on Earth don't work when you're dating stardust, Dr Heck said.
Instead the researchers measured how long the grains have been exposed to the cosmic rays shooting through the universe.
When a cosmic ray —a stream of high energy particles, mainly protons and alpha particles — penetrates a presolar grain it occasionally splits one of its carbon atoms into fragments.
By counting all the fragments produced by the cosmic rays, and knowing how often they are produced, scientists can work out how old the stardust is.
"Each grain probably came from a different star," Dr Heck said.
"We have some grains which are a billion years older than the Sun, making them 5.5 billion years old … a few grains that are 2 billion years older and we have one grain that is 3 billion years older [than the Sun].
The cosmic ray method doesn't give us an absolute age of the stardust, said planetary scientist and meteorite hunter Phil Bland of Curtin University, who wasn't involved in the research.
But it's our best approximation so far.
An astronomical baby boom
The ages of these grains of stardust isn't only important in themselves, but also because of what they tell us about the evolution of our galaxy.While some astronomical models assume stars form at a constant rate, Dr Heck and his colleagues' work shows that isn't the case.
"In order to explain our age distribution, where we have many more younger grains that we would otherwise expect, we have to explain this by this dust forming from more stars than normal," he said.
"We came to the conclusion that about 7 billion years ago there must have been an episode of enhanced star formation, probably about 50 per cent more stars formed than normal."
Or in other words, a star-making baby boom.
"That peak in star formation about 7 billion years ago … is really interesting because there's a target that other people can chase," Professor Bland said.
Now he said, we need more statistics from a different meteorite.
"What I would do now is pick another sample and go through the same process and say 'Okay, do we find that same distribution of stuff or is there something weird about this one?'."
For Dr Heck, this latest research is one of the most exciting studies he's worked on, but he's sure it won't be the last.
"Murchison is so important, and so rich and full of surprises," he said.
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