Saskatoon StarPhoenix

A SOUND IN THE ANCIENT STARS

‘VERY EXCITING’ CLUE

- Sarah kaplan

For the first time, scientists have detected a signal from “cosmic dawn” — the moment when the universe’s earliest stars emerged.

The signal, reported Wednesday in the journal Nature, is little more than a blip in the radio echo of that ancient era, as difficult to detect as the wingbeat of a hummingbir­d caught in a hurricane. But if confirmed, researcher­s say it can help explain the events that gave rise to the first stars, black holes, galaxies and, eventually, every other object in existence.

In a companion study, another scientist proposes that the unexpected size of the signal suggests it was influenced by dark matter—a potential new clue to one of the most persistent mysteries in the universe.

“It’s very, very exciting for the field,” said Anastasia Fialkov, a Harvard University astrophysi­cist who was not involved in either study. “We have never seen the light of the first stars, and this is its signature.”

For millions of years after it began, the universe was a chilly and lightless place. Its only contents were tenuous, invisible clouds of inert hydrogen gas. Its only energy was the radiation left over from the Big Bang — a persistent hum known as the cosmic microwave background.

Then, slowly, gravity began to gather up the densest regions of gas. Matter coalesced, collided, collapsed. Ultimately, this created the nurseries from which the first stars formed.

No telescope today can detect the glow of these primitive stars. But theoretica­l models had suggested that their ultraviole­t radiation would have pierced the hydrogen haze of the early universe, exciting the atoms within. This in turn would cause the atoms to absorb a small sliver of the cosmic microwave background radiation, imprinting it with a faint but indelible signature.

In a 1999 study, astrophysi­cists proposed that researcher­s could detect this signature by searching the entire sky for the muted wavelength­s, which would appear as a dip in the radio end of the electromag­netic spectrum. Such a project would require only a small antenna but incredibly careful analysis — the dip overlaps with the most popular frequencie­s on the FM radio dial, as well as many natural radio signals. Peter Kurczynski, a program director for the National Science Foundation, has compared the effort to turning on every radio station but one simultaneo­usly, then listening to figure out which station was missing.

A decade later, the NSF opted to fund the constructi­on of an antenna in the Australian desert to listen for this signal. The instrument was deceptivel­y simple, just two metal plates perched atop a dining roomtable-type structure and situated at the centre of a 30-metre-wide mesh carpet. But it sensed everything: the cacophony of human communicat­ion, the din of radio waves coming from the Milky Way and, beneath it all, the subtle buzz of the cosmic microwave background.

“The cosmologic­al signal is ... 0.1 to 0.01 per cent of the total amount of radio power we’re received,” said Judd Bowman, an astrophysi­cist at Arizona State University and the lead author of the first Nature study. But by subtractin­g out the louder, closer signals, Bowman and his colleagues could pin down the signature of emerging stars emanating from the moment 180 million years after the Big Bang.

For comparison, the most distant astronomic­al object ever observed is a galaxy that existed 400 million years after the universe began.

To ensure their signal was real, rather than a quirk of their instrument or a fluke in their data, Bowman and his colleagues spent two years considerin­g and discarding a range of alternativ­e explanatio­ns. They reposition­ed the antenna, tested it in the lab with simulated radio sky, even built a copy of the instrument to demonstrat­e that the experiment was reproducib­le. So far, they haven’t been able to prove themselves wrong.

The stars whose light led to the newly detected signal were very different from the ones that glitter in our night sky. Comprising just hydrogen and helium — the only elements that existed in the early universe—they burned blue, bright and fast. But when they died, they produced the explosions that gave rise to the heavier elements, including the carbon and oxygen atoms on which all life depends.

“These stars made the seeds for everything that came out of them ,” Bowman said.

THESE STARS MADE THE SEEDS FOR EVERYTHING THAT CAME OUT OF THEM.

 ?? N.R.FULLER / NATIONAL SCIENCE FOUNDATION VIA AP ?? A rendering of how the earliest stars in the universe might have looked.
N.R.FULLER / NATIONAL SCIENCE FOUNDATION VIA AP A rendering of how the earliest stars in the universe might have looked.

Newspapers in English

Newspapers from Canada