From CSIROscope: “Dying, not waving: nearby dwarf galaxy running out of gas”

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From CSIROscope

30 October 2018
Nicholas Kachel

A radio image of hydrogen gas in the Small Magellanic Cloud as observed by CSIRO’s ASKAP telescope. Image credit: Naomi McClure-Griffiths et al, CSIRO’s ASKAP telescope.

Even though it’s on an astronomical timeline, a close intergalactic neighbour of ours known as the Small Magellanic Cloud (SMC) is slowly dying.

The SMC (named after famous Portuguese explorer Ferdinand Magellan) is about 200,000 light years away, and is one of the furthest objects viewable in our skies with the naked eye. Astronomers from the Australian National University (ANU) and our own team have used our powerful Australian SKA Pathfinder (ASKAP) radio telescope array to capture images of the dwarf galaxy, observing a powerful outflowing of hydrogen gas from it.

Hydrogen is the most abundant element in the Universe, and is the main ingredient of stars. But for every Sun sized star that the SMC makes, it loses up to 10 times that amount of this star-forming gas due to its (comparatively) weaker gravitational fields. If the SMC loses all its hydrogen it will eventually lose its ability to create new stars, slowly but surely fading into oblivion.

Thankfully, we’re not talking a Macauley Caulkin post-Richie Rich timeline here: astronomers say the process will take billions of years.

And it’s not all doom and gloom. This observation has helped confirm simulations developed by theorists on how small galaxies like the SMC might evolve.

Lead researcher Professor Naomi McClure-Griffiths from ANU said the discovery, which is part of a project that investigates the evolution of galaxies, provided the first clear observational measurement of the amount of mass lost from a dwarf galaxy.

“The result is also important because it provides a possible source of gas for the enormous Magellanic Stream that encircles the Milky Way,” she said.

CSIRO co-researcher Dr David McConnell said ASKAP was unrivalled in the world for this kind of research due to its unique radio receivers that give it a panoramic view of the sky.

“The telescope covered the entire SMC galaxy in a single shot and photographed its hydrogen gas with unprecedented detail,” he said.

Astronomers expect the SMC will ultimately be gobbled up by our own Milky Way.

See the full article here .


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SKA/ASKAP radio telescope at the Murchison Radio-astronomy Observatory (MRO) in Mid West region of Western Australia

So what can we expect these new radio projects to discover? We have no idea, but history tells us that they are almost certain to deliver some major surprises.

Making these new discoveries may not be so simple. Gone are the days when astronomers could just notice something odd as they browse their tables and graphs.

Nowadays, astronomers are more likely to be distilling their answers from carefully-posed queries to databases containing petabytes of data. Human brains are just not up to the job of making unexpected discoveries in these circumstances, and instead we will need to develop “learning machines” to help us discover the unexpected.

With the right tools and careful insight, who knows what we might find.

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CSIRO, the Commonwealth Scientific and Industrial Research Organisation, is Australia’s national science agency and one of the largest and most diverse research agencies in the world.