Lead author of the study, PhD student Yuanming Wang. Photo: Louise Cooper
Astronomers have for the first time used distant galaxies as scintillating pins to locate and identify a piece of the Milky Ways missing matter.
For decades, scientists have been puzzled as to why they couldnt account for all the matter in the universe as predicted by theory. While most of the universes mass is thought to be mysterious dark matter and dark energy, 5 percent is normal matter that makes up stars, planets, asteroids, peanut butter and butterflies. This is known as baryonic matter.
However, direct measurement has only accounted for about half the expected baryonic matter.
Yuanming Wang, a doctoral candidate in the School of Physics at the University of Sydney, has developed an ingenious method to help track down the missing matter. She has applied her technique to pinpoint a hitherto undetected stream of cold gas in the Milky Way about 10 light years from Earth. The cloud is about a trillion kilometres long and 10 billion kilometres wide but only weighing about the mass of our Moon.
The results, published in the Monthly Notices of the Royal Astronomical Society, offer a promising way for scientists to track down the Milky Ways missing matter.
We suspect that much of the missing baryonic matter is in the form of cold gas clouds either in galaxies or between galaxies, said Ms Wang, who is pursuing her PhD at the Sydney Institute for Astronomy.
This gas is undetectable using conventional methods, as it emits no visible light of its own and is just too cold for detection via radio astronomy, she said.
What the astronomers did is look for radio sources in the distant background to see how they shimmered.
We found five twinkling radio sources on a giant line in the sky. Our analysis shows their light must have passed through the same cold clump of gas, Ms Wang said.
Just as visible light is distorted as it passes through our atmosphere to give stars their twinkle, when radio waves pass through matter, it also affects their brightness. It was this scintillation that Ms Wang and her colleagues detected.
Dr Artem Tuntsov, a co-author from Manly Astrophysics, said: We arent quite sure what the strange cloud is, but one possibility is that it could be a hydrogen snow cloud disrupted by a nearby star to form a long, thin clump of gas.
Hydrogen freezes at about minus 260 degrees and theorists have proposed that some of the universes missing baryonic matter could be locked up in these hydrogen snow clouds. They are almost impossible to detect directly.
However, we have now developed a method to identify such clumps of invisible cold gas using background galaxies as pins, Ms Wang said.
Ms Wangs supervisor, Professor Tara Murphy, said: This is a brilliant result for a young astronomer. We hope the methods trailblazed by Yuanming will allow us to detect more missing matter.
Continued here:
Student astronomer finds galactic missing matter - News - The University of Sydney
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