Using helium, astronomers blow certainty into early Big Bang conditions
New data fortifies modern physics insights, researchers say
New observations regarding the composition of distant galaxies reveal insights into the earliest phases of the universe that confirm decades of scientific understanding of the elements and particles produced by the Big Bang, according to a new study.
Researchers used data from The Large Binocular Telescope (LBT) to measure the amount of helium — the second-most common element in the cosmos and a vital ingredient for the formation of life — in metal-poor nebulas, clouds of gas and dust in space where stars are sometimes born. Their findings strengthen long-held theories about how ancient elements, such as carbon and nitrogen, may have been dispersed in the period following the Big Bang.
Astronomers did this by analyzing helium signals in optical and infrared light to determine the temperature and density of the gases within faraway systems. After collecting 48 high-quality galactic samples, the team created a dataset aimed at significantly expanding researchers’ ability to infer the universe’s primordial helium abundance.
“Everything that we need to live here on Earth was once fused inside of a star,” said Miqaela Weller, lead author of the study and a PhD student in astronomy at The Ohio State University. “Understanding precisely where those elements come from helps inform us of how our universe evolved and how it will evolve in the future.”
Written by: Tatyana Woodall, Woodall.5@osu.edu
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