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SKY NIGHTLY
Charting the slow death of the Universe
by Staff Writers
Paris (SPX) Aug 12, 2015


This composite picture shows how a typical galaxy appears at different wavelengths in the GAMA survey. This huge project has measured the energy output of more than 200,000 galaxies and represents the most comprehensive assessment of the energy output of the nearby Universe. The results confirm that the energy produced in a section of the Universe today is only about half what it was two billion years ago and find that this fading is occurring across all wavelengths from the ultraviolet to the far infrared. Image courtesy ICRAR/GAMA and ESO. For a larger version of this image please go here.

The study, which is part of the Galaxy And Mass Assembly (GAMA) project, the largest multi-wavelength survey ever put together, involved many of the world's most powerful telescopes [1].

"We used as many space and ground-based telescopes as we could get our hands on to measure the energy output of over 200 000 galaxies across as broad a wavelength range as possible," says Simon Driver ICRAR, The University of Western Australia), who heads the large GAMA team.

The survey data, released to astronomers around the world today, includes measurements of the energy output of each galaxy at 21 wavelengths, from the ultraviolet to the far infrared. This dataset will help scientists to better understand how different types of galaxies form.

All the energy in the Universe was created in the Big Bang, with some portion locked up as mass. Stars shine by converting mass into energy, as described by Einstein's famous equation E=mc2 [2]. The GAMA study sets out to map and model all of the energy generated within a large volume of space today and at different times in the past.

"While most of the energy sloshing around in the Universe arose in the aftermath of the Big Bang, additional energy is constantly being generated by stars as they fuse elements like hydrogen and helium together," Simon Driver says. "This new energy is either absorbed by dust as it travels through the host galaxy, or escapes into intergalactic space and travels until it hits something, such as another star, a planet, or, very occasionally, a telescope mirror."

The fact that the Universe is slowly fading has been known since the late 1990s, but this work shows that it is happening across all wavelengths from the ultraviolet to the infrared, representing the most comprehensive assessment of the energy output of the nearby Universe.

"The Universe will decline from here on in, sliding gently into old age. The Universe has basically sat down on the sofa, pulled up a blanket and is about to nod off for an eternal doze," concludes Simon Driver.

The team of researchers hope to expand the work to map energy production over the entire history of the Universe, using a swathe of new facilities, including the world's largest radio telescope, the Square Kilometre Array, which is due to be built in Australia and South Africa over the next decade.

The team will present this work at the International Astronomical Union XXIX General Assembly in Honolulu, Hawai`i, on Monday 10 August 2015.


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SKY NIGHTLY
Stars in Our Galaxy Move Far From Home
Boston MA (SPX) Aug 01, 2015
When it comes to our galaxy, home is where the star is. Scientists with the Sloan Digital Sky Survey (SDSS) have created a new map of the Milky Way and determined that 30 percent of stars have dramatically changed their orbits. This discovery, published in yesterday's issue of The Astrophysical Journal, brings a new understanding of how stars are formed, and how they travel throughout our galaxy ... read more


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