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The power of gravitational lensing!
The NASA/ESA Hubble Space Telescope has discovered the brightest quasar ever seen in the early Universe. After 20 years of searching, astronomers have identified the ancient quasar with the help of strong gravitational lensing. This unique object provides an insight into the birth of galaxies when the Universe was less than a billion years old.
Go to our @instagram Story to learn more about this discovery.
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@europeanspaceagency / @hubbleesa, @NASA, M. Kornmesser
Computer simulation of a Supernova ️
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Only three, Milky Way naked-eye supernova events have been observed during the last thousand years, though many have been seen in other galaxies using telescopes. The most recent directly observed supernova in the Milky Way was Kepler's Supernova in 1604, but two more recent supernova remnants have also been found. Statistical observations of supernovae in other galaxies suggest they occur on average about three times every century in the Milky Way, and that any galactic supernova would almost certainly be observable with modern astronomical telescopes.
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Planet ballons ❤️️ Via @space_love.rs
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Pictured above is an artists rendition of a Blazar. What is a Blazar? Well, at the center of most galaxies, there lies a supermassive black hole collecting gas, dust, and other debris all around. As material in the disk falls toward the black hole, its gravitational energy can be converted to light, making the centers of these galaxies very bright and giving them the name Active Galactic Nuclei (AGN). Some of these AGN’s also shoot out colossal jets of material that travel close to the speed of light! Scientists call this a quasar. However, when these jets of matter are pointed at Earth, we call them a Blazar. Definitely not something we’d wanna be close to!
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Black Hole What do you think guys? Tag someone
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There might be a new model for cosmic expansion
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According to the leading scenario, our Universe contains only a few percent of ordinary matter. One quarter of the cosmos is made of the elusive dark matter, which we can feel gravitationally but not observe, and the rest consists of the even more mysterious dark energy that is driving the current acceleration of the Universe’s expansion.
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This model is based on a multitude of data collected over the last couple of decades, from the cosmic microwave background – the first light in the history of the cosmos, released only 380 000 years after the big bang and observed in unprecedented detail by our Planck mission – to more ‘local’ observations. The latter include supernova explosions, galaxy clusters and the gravitational distortion imprinted by dark matter on distant galaxies, and can be used to trace cosmic expansion in recent epochs of cosmic history – across the past nine billion years. •
A new study, led by Guido Risaliti of Università di Firenze, Italy, and Elisabeta Lusso of @durhamuniversity, UK, points to another type of cosmic tracer – quasars – that would fill part of the gap between these observations, measuring the expansion of the Universe up to 12 billion years ago.
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Go to our @instagram Story to learn more.
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@europeanspaceagency–C. Carreau
Most of us have heard of Quasars, but what about Blazars? Well, let’s look at a quasar first. These extremely bright phenomena are known as AGN, or active galactic nuclei. Typically found in the center of dense galaxies, they are among the most powerful objects in the known universe. They have a jet stream of incredibly charged particles just flying th through the universe at high speeds. Now, what’s a Blazar? Where there’s only one different between and a Blazar and a Quasar, and that difference is what makes Blazars so scary. A Blazar is another word for a Quasar whose jet stream of dangerous particles is aimed at Earth... not so fun anymore
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