Researchers from Northwestern University in the US, using supercomputer simulations, found a major and unexpected new mode for how galaxies, including our own Milky Way, acquired their matter: intergalactic transfer.
The simulations show that supernova explosions eject copious amounts of gas from galaxies, which causes atoms to be transported from one galaxy to another via powerful galactic winds, researchers said.
Intergalactic transfer is a newly identified phenomenon, which simulations indicate will be critical for understanding how galaxies evolve.
"It is likely that much of the Milky Way's matter was in other galaxies before it was kicked out by a powerful wind, travelled across intergalactic space and eventually found its new home in the Milky Way," Angles-Alcazar said.
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Galaxies are far apart from each other, so even though galactic winds propagate at several hundred kilometres per second, this process occurred over several billion years.
They then developed state-of-the-art algorithms to mine this wealth of data and quantify how galaxies acquire matter from the universe.
"This study transforms our understanding of how galaxies formed from the Big Bang," said Claude-Andre Faucher-Giguere, professor at Northwestern University.
"What this new mode implies is that up to one-half of the atoms around us - including in the solar system, on Earth and in each one of us - comes not from our own galaxy but from other galaxies, up to one million light years away," he said.
This transfer of mass through galactic winds can account for up to 50 per cent of matter in the larger galaxies.
"In our simulations, we were able to trace the origins of stars in Milky Way-like galaxies and determine if the star formed from matter endemic to the galaxy itself or if it formed instead from gas previously contained in another galaxy," said Angles-Alcazar.
"Our origins are much less local than we previously thought. This study gives us a sense of how things around us are connected to distant objects in the sky," Giguere said.