Planck's most detailed map ever reveals an almost perfect Universe - 0 views
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the most detailed map ever created of the cosmic microwave background
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revealing the existence of features that challenge the foundations of our current understanding of the Universe
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The image is based on the initial 15.5 months of data from Planck and is the mission's first all-sky picture of the oldest light in our Universe, imprinted on the sky when it was just 380 000 years old.
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At that time, the young Universe was filled with a hot dense soup of interacting protons, electrons and photons at about 2700ºC
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As the Universe has expanded, this light today has been stretched out to microwave wavelengths, equivalent to a temperature of just 2.7 degrees above absolute zero.
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that correspond to regions of slightly different densities at very early times, representing the seeds of all future structure: the stars and galaxies of today
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According to the standard model of cosmology, the fluctuations arose immediately after the Big Bang and were stretched to cosmologically large scales during a brief period of accelerated expansion known as inflation.
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Planck was designed to map these fluctuations across the whole sky with greater resolution and sensitivity than ever before
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By analysing the nature and distribution of the seeds in Planck's CMB image, we can determine the composition and evolution of the Universe from its birth to the present day
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because precision of Planck's map is so high, it also made it possible to reveal some peculiar unexplained features that may well require new physics to be understood
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Since the release of Planck's first all-sky image in 2010, we have been carefully extracting and analysing all of the foreground emissions that lie between us and the Universe's first light
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One of the most surprising findings is that the fluctuations in the CMB temperatures at large angular scales do not match those predicted by the standard model
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This runs counter to the prediction made by the standard model that the Universe should be broadly similar in any direction we look
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One way to explain the anomalies is to propose that the Universe is in fact not the same in all directions on a larger scale than we can observe
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In this scenario, the light rays from the CMB may have taken a more complicated route through the Universe than previously understood, resulting in some of the unusual patterns observed today.
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the Planck data conform spectacularly well to the expectations of a rather simple model of the Universe, allowing scientists to extract the most refined values yet for its ingredients
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dark energy, a mysterious force thought to be responsible for accelerating the expansion of the Universe, accounts for less than previously thought.
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Normal matter that makes up stars and galaxies contributes just 4.9% of the mass/energy density of the Universe
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Dark matter, which has thus far only been detected indirectly by its gravitational influence, makes up 26.8%, nearly a fifth more than the previous estimate.
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Planck data also set a new value for the rate at which the Universe is expanding today, known as the Hubble constant
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At 67.15 kilometres per second per megaparsec, this is significantly less than the current standard value in astronomy
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We see an almost perfect fit to the standard model of cosmology, but with intriguing features that force us to rethink some of our basic assumptions