Sinister Security: Andromeda Galaxy

Check Out This 1.5 BILLION Pixel Image Of The Andromeda Galaxy

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This 1.5 Billion pixel image is the largest and sharpest photograph ever taken of the Andromeda Galaxy. In order to observe all of the 1.5 billion pixels, you’d need 600 HD TV screens to observe the image in full. (Image Caption: Each dot is a star.)

Using the Hubble Space Telescope, astronomers have taken what is considered one of the most fascinating images of our cosmic neighbor. The 1.5 BILLION pixel image of the Andromeda galaxy shows the beauty and mystery engulfing our cosmic neighbor. Oh and, each one of those little dots is a star, and most of them have at least one planet, and many of them have several alien worlds.

The Andromeda galaxy also referred to as Messier 31 or just M31 is the only member of the local group of galaxies that has more mass than our own galaxy, the Milky Way. It is located a staggering 2.5 million light years from Earth.

The galaxy is approaching our galaxy at about 300 kilometers per second. The first reference to the Andromeda galaxy dates back to 961, and was made by Persian astronomer Azophi, whom in his Book of Fixed Stars describes as a “small cloud in the constellation of Andromeda.” The first telescopic observation corresponds to Simon Marius in 1612.

This image is the largest and sharpest image of the Andromeda galaxy ever taken.

As noted by Cosmos, in order to observe all of the 1.5 billion pixels you’d need 600 HD TV screens to observe the image in full.

In this unprecedented, jaw-dropping image you can witness over 100 million—of its estimated TRILLION stars.

You can’t say that this view isn't magical!

In order to observe the image in all of its beauty, and to actually see all of those tiny little dots, head on over to the Hubble website where you’ll get a chance to zoom in and out into different parts of the galaxy, which will allow you to see—in unprecedented detail—a galaxy coming to life.

What for many may have seemed like one single star turns out to be a cluster of different stars surrounded by other countless Suns that are too faint to make it into the picture.

And as you drool over this image remember that even though you can’t even contemplate Andromeda’s true size, it is just a small, tiny part compared to the rest of the universe.

The most awesome image of the Andromeda galaxy:http://www.spacetelescope.org/images/heic1502a/zoom

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NASA Detects "Powerful Signals From The Center Of The Milky Way And Andromeda Galaxy" -- May Be Evidence Of The Mysterious Dark Side Of The Universe

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NASA's Fermi Gamma-ray Space Telescope has found a signal at the center of the neighboring Andromeda galaxy that could indicate the presence of the mysterious dark side of the universes known as dark matter. The signal is similar to one seen by Fermi at the center of our own Milky Way galaxy.

Surprisingly, the latest Fermi data shows the gamma rays in Andromeda -- also known as M31 -- are confined to the galaxy's center instead of spread throughout. To explain this unusual distribution, scientists are proposing that the emission may come from several undetermined sources. One of them could be dark matter, an unknown substance that makes up most of the universe.

The image of the Milky Way above, shown in visible light, superimposes a gamma-ray map of the galactic center from NASA's Fermi. Raw data transitions to a view with all known sources removed, revealing a gamma-ray excess hinting at the presence of dark matter.

The Milky Way's galactic center teems with gamma-ray sources, from interacting binary systems and isolated pulsars to supernova remnants and particles colliding with interstellar gas. It's also where astronomers expect to find the galaxy's highest density of dark matter, which only affects normal matter and radiation through its gravity. Large amounts of dark matter attract normal matter, forming a foundation upon which visible structures, like galaxies, are built.

No one knows the true nature of dark matter, but WIMPs, or Weakly Interacting Massive Particles, represent a leading class of candidates. Theorists have envisioned a wide range of WIMP types, some of which may either mutually annihilate or produce an intermediate, quickly decaying particle when they collide. Both of these pathways end with the production of gamma rays -- the most energetic form of light -- at energies within the detection range of Fermi's Large Area Telescope (LAT).

When astronomers carefully subtract all known gamma-ray sources from LAT observations of the galactic center, a patch of leftover emission remains. This excess appears most prominent at energies between 1 and 3 billion electron volts (GeV) -- roughly a billion times greater than that of visible light -- and extends outward at least 5,000 light-years from the galactic center.

Hooper and his colleagues conclude that annihilations of dark matter particles with a mass between 31 and 40 GeV provide a remarkable fit for the excess based on its gamma-ray spectrum, its symmetry around the galactic center, and its overall brightness. Writing in a paper submitted to the journal Physical Review D, the researchers say that these features are difficult to reconcile with other explanations proposed so far, although they note that plausible alternatives not requiring dark matter may yet materialize.

"Dark matter in this mass range can be probed by direct detection and by the Large Hadron Collider (LHC), so if this is dark matter, we're already learning about its interactions from the lack of detection so far," said co-author Tracy Slatyer, a theoretical physicist at MIT in Cambridge, Mass. "This is a very exciting signal, and while the case is not yet closed, in the future we might well look back and say this was where we saw dark matter annihilation for the first time."

The researchers caution that it will take multiple sightings – in other astronomical objects, the LHC or in some of the direct-detection experiments now being conducted around the world -- to validate their dark matter interpretation.

A Fermi 2015 study was an example of innovative techniques applied to Fermi data by the science community, said Peter Michelson, a professor of physics at Stanford University in California and the LAT principal investigator. "The Fermi LAT Collaboration continues to examine the extraordinarily complex central region of the galaxy, but until this study is complete we can neither confirm nor refute this interesting analysis."

While the great amount of dark matter expected at the galactic center should produce a strong signal, competition from many other gamma-ray sources complicates any case for a detection. But turning the problem on its head provides another way to attack it. Instead of looking at the largest nearby collection of dark matter, look where the signal has fewer challenges.

Dwarf galaxies orbiting the Milky Way lack other types of gamma-ray emitters and contain large amounts of dark matter for their size – in fact, they're the most dark-matter-dominated sources known. But there's a tradeoff. Because they lie much farther away and contain much less total dark matter than the center of the Milky Way, dwarf galaxies produce a much weaker signal and require many years of observations to establish a secure detection.

For the past few years, the LAT team has been searching dwarf galaxies for hints of dark matter. The published results of these studies have set stringent limits on the mass ranges and interaction rates for many proposed WIMPs, even eliminating some models.

There's about a one-in-12 chance that what they saw in 2015 in the dwarf galaxies is not even a signal at all, but a fluctuation in the gamma-ray background, explained Elliott Bloom, a member of the LAT Collaboration at the Kavli Institute for Particle Astrophysics and Cosmology, jointly located at the SLAC National Accelerator Laboratory and Stanford University. If it's real, the signal should grow stronger as Fermi acquires additional years of observations and as wide-field astronomical surveys discover new dwarfs. "If we ultimately see a significant signal," he added, "it could be a very strong confirmation of the dark matter signal claimed in the galactic center."

Via NASA Goddard; A. Mellinger, CMU; T. Linden, Univ. of Chicago

Sinister Security

Check Out This 1.5 BILLION Pixel Image Of The Andromeda Galaxy

A Supermassive Black Hole Is Heading Earth’s Way At 110 Km Per Second

NASA Detects "Powerful Signals From The Center Of The Milky Way And Andromeda Galaxy" -- May Be Evidence Of The Mysterious Dark Side Of The Universe

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