<![CDATA[io9: dark energy]]> http://tags.lifehacker.com/assets/base/img/thumbs140x140/io9.com.png <![CDATA[io9: dark energy]]> http://io9.com/tag/darkenergy http://io9.com/tag/darkenergy <![CDATA[More Evidence that Dark Energy Is Ripping the Universe Apart]]> At a press conference today, NASA announced new measurements from the Chandra X-Ray Observatory confirm the existence of "dark energy" that is causing the universe to expand - and disintegrate - at a rapid clip.

Dark energy is a theory among astrophysicists that there is a force pulling galaxies apart - a force that that is accelerating, and will eventually lead to the destruction of every molecule in the universe. The theory first came about roughly a decade ago to explain why distant galaxies are moving away from our own more rapidly than ones that are close by. According to Live Science's Jeanna Bryner:

New measurements of this accelerating expansion . . . provide details about the nature of the unseen and unknown dark energy that is at work.

The results, announced today at a news conference organized by NASA, reveal a decrease in the mass of galaxy clusters in more recent times, which would be a consequence of this hastening and ripping force that some think could eventually tear apart even star systems, planets and eventually the very molecules we're made of.

"If there were any doubts 10 years after the initial discovery that the universe was speeding up, this should really dispel them," said Michael Turner of the University of Chicago's Department of Astronomy and Astrophysics, who was not involved in the current study.

What does this mean? In a few billion years, we won't be able to see any galaxies in the space around us. And, perhaps, it means the death of the universe will be a lonely business indeed.

More images and a complete report at LiveScience.

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<![CDATA[Earth: A Very Special Place In the Void]]> You know that "I'm an insignificant dot in the middle of this enormous universe" feeling you get when you stare up into the night sky a little too long? Well, some Oxford scientists think you might be a little more special than that - or at least, the planet you live on is. Their radical new theory would not only obviate the need for dark energy to explain observed patterns of galactic motion, it would overturn the centuries-old Copernican Principle. Not bad for a day's work.

In the 16th century, Copernicus hypothesized that the Earth is not the center of the solar system, but rather the sun is. Later, cosmologists expanded this idea into the Copernican Principle: Earth is not in a special place in the universe, therefore our observations of local space can be used to infer data about the rest of the universe. When astronomers observed that the universe appears to be expanding at an accelerating rate, they needed to add something to their equations to make it all make sense. That something is dark energy, which would have to exist in massive quantities (as yet, pretty much undetectable) to explain this expansion.

Here's the thing - the universe is really, really, really huge. Just the part we can see is almost incomprehensibly big, and there's a whole lot of universe we can't see. No one knows how big the whole universe is, but it's entirely possible that our part of the universe is just a tiny fraction of the whole. Physicists from Oxford University are considering the idea that the universe we can observe is actually anomalous, a giant void with a low density of matter. The rest of the universe may look substantially different. Doing some number crunching revealed that their model of the universe works without dark energy, but isn't quite as accurate as the current dark energy model. However, they need more observations of certain types of supernovae to refine their numbers - in a few months, their equations may look better with more data.

What's particularly cool is that this maverick theory that tosses a very accepted tenet of astronomy right out the window is being published in Physical Review Letters, one of the most respected physics journals. It sure beats excommunication. Image by: NASA.

Overturning Copernicus, eliminating dark energy. [Nobel Intent]

Tsunami invisibility cloak, dark energy v. the void, sorting nanotubes with light, and more. [EurekAlert!]

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<![CDATA[Heaviest, Farthest Cluster Points Toward Dark Energy]]> The XMM-Newton space telescope has been really into dark and heavy stuff lately. No, the x-ray observatory didn't find its parents' old Black Sabbath albums — it found the most massive galactic cluster on record, a conglomerate of galaxies weighing more than 1,000 times as much as the Milky Way. The cluster's extreme distance is a puzzling paradox, or it might help prove that the universe is full of mysterious dark energy.

Last week, we told you about two galactic clusters colliding, providing visual (and x-ray) evidence of the existence of dark matter. Dark energy is even more elusive, but astronomers who were looking at an entirely different cosmic object may have stumbled across a major clue.

The large blue glow in the image (taken with the Large Binocular Telescope at the Mt. Graham International Observatory to confirm XMM-Newton's discovery) is a galactic cluster with the catchy name 2XMM J083026+524133. It's heavier than any other cluster, and it's farther from Earth than any other as well. In fact, it's twice as far as the next farthest. Here's the mystery — really distant clusters should be very young, because it takes their light so long to reach us. Young clusters shouldn't be big, because it takes time for all those galaxies to pull together. A huge, distant cluster is seemingly impossible. That's where dark energy comes in.

Dark energy, to put it into very simple terms, is a sort of anti-gravity force that actually pushes space apart and speeds the expansion of the universe. If it exists, that is. It is one possible explanation for 2XMM J083026+524133's distance. It might be an old cluster that appears more distant than it should be due to dark energy fueled expansion of space. What is the source of all the dark energy in the universe? Tony Iommi. Image by: ESA.

Cosmic Heavyweight. [Science News]

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<![CDATA[Ultracold Polar Telescope Searches for Dark Energy]]> Is an invisible, undetectable force tearing the universe apart? The South Pole Telescope is scanning the skies for signs of dark energy to help pinpoint the cause of cosmic expansion. The answers it provides could allow us to better explain the origin of the universe and its ultimate fate.

Earlier this week I pondered whether dark energy is just a new version of an outdated theory, but a team of astronomers in Antarctica is doing the hard work of trying to find out. The South Pole Telescope (SPT) uses 1,000 advanced optical sensors to peer at distant galaxy clusters looking for subtle variations in the cosmic background radiation. Those variations will give scientists a better idea of the structure of the universe, and whether or not dark energy is part of it.

The SPT is the largest Antarctic telescope. Despite the frigid cold of the region, the optics are further shielded from background heat by being chilled to a temperature not far from absolute zero. Photo by: The University of Chicago.

Cosmologists Probe Mystery Of Dark Energy With South Pole Telescope. [Science Daily]

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<![CDATA[Is Dark Energy the New Aether?]]> You may think physics has changed over the past 200 years, but it hasn't. Today, theoretical physicists can't understand why the universe is expanding at an observed rate that doesn't quite mesh with general relativity. Back in the 19th century, theoretical physicists couldn't understand how electromagnetic energy and gravity could propagate through empty space. The proposed solution in both cases was the same: there must some stuff out there that we can't see, yet affects the entire universe. In the past, that substance was aether. Is today's dark energy the modern equivalent?

Aether (also called ether) was a theoretical substance that supposedly permeated the entire universe, including solid matter, more or less evenly. While aether theories evolved over time, it was generally believed to be made of particles so tiny we couldn't detect them. The inherent properties of the aether determined many of the physical properties of the universe, such as the speed of light and the strength of gravity. These forces propagated as waves through the aether. Aether theory survived into the 20th century - Einstein even adapted it to fit his theory of special relativity, although it was so drastically changed that it was hardly aether theory at all. In his 1920 address "Ether and the Theory of Relativity," Einstein said:

The ether of the general theory of relativity is a medium which is itself devoid of all mechanical and kinematical qualities.
Dark energy is the theoretical source of the force that is causing the universe to expand at an accelerated rate. Physicists measure cosmic expansion by observing the redshift in the light from exploding stars. The rate of expansion they see doesn't fit into the equations of general relativity unless they add in what is basically an imaginary number, a force of some kind that causes the expansion. A form of energy that we are unable to observe directly and fills the universe more or less evenly (another flavor of the theory posits a scalar field of dark energy that would not be so homogeneous) creates this force. The energy may be an inherent property of space itself, sometimes known as vacuum energy, and it exerts a negative pressure. This negative pressure stretches space, causing a gravitational repulsion that makes the universe expand.

To be certain, neither theory is "bad science" in any way. They are the types of theories that physicists come up with when they are working out beyond the current observational abilities of humans. Eventually, physicists identified the dual wave/particle properties of electromagnetic energy. This, along with experiments that confirmed general relativity, negated the need for aether theory. Likewise, new experiments conducted with the Large Hadron Collider later this year could detect new particles like the Higgs boson that will give us additional clues to the physical makeup of the universe. Will they invalidate dark energy? Photo by: NASA.

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<![CDATA[Galaxies' Swan Dive May Give New Clues To Dark Energy]]> One day, we'll use images like this waterfall of galaxies to figure out where to refuel our ships with dark energy. That's because this computer simulation of millions of galaxies flowing towards the red zone, the area with the highest mass, gives some clues to the location and nature of dark energy and dark matter. The image shows a "snapshot" of galaxies in the process of forming large-scale structures, 10 billion years ago. Click through for details.

The whole picture occupies a space of 100 million light years and this computer simulation "paints" the densest areas red. The yellow lines show the intensity of the galaxies' velocities as they fall into the highest-density area. The speed of the galaxies' rush towards the center of the structure depends on the the balance between dark matter, dark energy and the overall expansion of the universe. Astronomers are learning how to measure this "infall pattern" by using a large survey of galaxies at different epochs. [European Southern Observatory]

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