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Dark Energy Camera begins galaxies survey

Dark Energy Camera, the highest-resolution camera ever built, has begun its quest to pin down the mysterious stuff that makes up nearly three-quarters of our Universe.

The Dark Energy Survey’s 570-million-pixel camera will scan some 300 million galaxies in the coming five years.

The goal is to discover the nature of dark energy, which is theorized to be responsible for the ever-faster expansion of the Universe.

Its first image, taken 12 September, focused on the Fornax galaxy cluster.

In time, along with its massive haul of individual galaxies, it will study 100,000 galaxy clusters – the largest stable structures we know of – and 4,000 supernovae, the bright dying throes of stars.

This enormous survey is a collaboration between US, UK, Brazilian, Spanish and German astronomers.

The phone box-sized Dark Energy Camera or DECam is mounted on the 4 m Victor M Blanco telescope at the Cerro Tololo Inter-American Observatory in Chile’s Atacama desert.

The Dark Energy Survey's 570-million-pixel camera will scan some 300 million galaxies in the coming five years

The Dark Energy Survey's 570-million-pixel camera will scan some 300 million galaxies in the coming five years

DECam is particularly sensitive to red and infrared light, to better study cosmic objects as distant as eight billion light-years away.

More distant objects are moving away from us – and each other – faster than nearer objects, which causes a shift of their apparent color toward the red end of the spectrum – a “redshift”.

Careful studies of the shifted light from distant supernovae were what first demonstrated this expansion, leading to the 2011 Nobel Prize in physics.

What is believed to be causing this increase in the speed of expansion is called dark energy, making up more than 70% of the “stuff” of the Universe and the focus of the DECam’s mission.

Other efforts hope to get to the bottom of the mystery, including the Boss survey and a future space telescope dediated to the effort called Euclid.

But for now, Will Percival from the University of Portsmouth, a Dark Energy Survey collaborator, said DECam is an exciting prospect.

“This will be the largest galaxy survey of its kind, and the galaxy shapes and positions will tell us a great deal about the nature of the physical process that we call dark energy, but do not currently understand,” he said.

The survey will tackle the problem in four ways.

It will study the same kind of supernovae that led to the Nobel Prize, in a bid to unravel the “expansion history” of the Universe – when its expansion increased and decreased over billions of years.

It will also map out in 3D the distribution of galaxy clusters, measuring what are known as baryon acoustic oscillations – literally relics of the sound echoes of the Big Bang.

By counting the clusters and plotting out when they evidently formed, the survey can feed back to computer models that map out how we think the Universe organized itself in its earliest years.

And studies of the way galaxies and galaxy clusters bend passing light – in a process called weak gravitational lensing – will help to pin down the equally mysterious “dark matter” that is believed to make up more than 80% of the Universe’s mass.

DECam will now be run through a series of tests and will begin the official survey in December.

With each snapshot it acquires, it will see an apparent area of the sky 20 times larger than the full moon.

In its full five-year run, it should capture an eighth of the full sky.

“The achievement of first light through the Dark Energy Camera begins a significant new era in our exploration of the cosmic frontier,” said James Siegrist, associate director of science for high-energy physics at the US Department of Energy, which oversaw the instrument’s construction.

“The results of this survey will bring us closer to understanding the mystery of dark energy and what it means for the Universe.”

What is redshift?

• The term “redshift” arises from the fact that light from more distant objects shows up on Earth more red than when it left its source

• The color shift comes about because of the Doppler effect, which acts to “stretch” or “compress” waves from moving objects

• It is at work in the sound of a moving siren: an approaching siren sounds higher-pitched and a receding one sounds lower-pitched

• In the case of light, approaching objects appear more blue and receding objects appear more red

• The expansion of the Universe is accelerating, so in general, more distant objects are moving away from us (and each other, and everything else) more quickly than nearer ones

• At cosmic distances, the shift can profoundly affect the color – the factor by which the wavelength is “stretched” is called the redshift

Dark energy and dark matter mysteries

• Gravity acting across vast distances does not seem to explain what astronomers see

• Galaxies, for example, should fly apart; some other mass must be there holding them together

• Astrophysicists have thus postulated “dark matter” – invisible to us but clearly acting on galactic scales

• At the greatest distances, the Universe’s expansion is accelerating

• Thus we have also “dark energy” which acts to drive the expansion, in opposition to gravity

• The current theory holds that 73% of the Universe is dark energy, 23% is dark matter, and just 4% the kind of matter we know well