Aug. 24, 2026
Cosmic Collisions and Gluon Mysteries: NASA's Swift Mission Scrapped
SpaceTime Series 29 Episode 101 *NASA scraps its Swift rescue mission NASA has been forced to abandon its planned rescue mission to save the Swift Gamma Ray Space Telescope. *The Milky Way’s first big galactic collision Astronomers have discovered what was probably the first major galactic collision involving our home galaxy the Milky Way cannibalising a dwarf galaxy less than two billion years after the big bang. *Understanding the stuff atoms are made of New observations by the world’s largest atom smasher have revealed some of the basic fundamental physics of the universe, challenging long-standing theories of how gluons behave inside atomic nuclei. *The Science Report Australia records its first confirmed case of H5 N1 bird flu in a mammal on the nation’s main land. How bushfires are polluting water supplies with arsenic. Successful Phase 3 trials of a new Australian developed personalized mRNA cancer vaccine. The growing impact of plastic pollution on Lord Howe Island’s Sable Shearwaters rookery. Over 90% of Blue Mountains rainforests wrongly catalogued as eucalypt forests. The Skeptics guide to the ghost of the Crying Tree pub.
Our guests: Alex Zaharov-Reutt from techadvice.life Tim Mendham from Australian Skeptics And Senior science writer and Sky and Telescope magazine contributor Jonathan Nally 🌏 Get Our Exclusive NordVPN deal here ➼ www.bitesz.com/nordvpn . The discounts and bonuses are incredible! And it’s risk-free with Nord’s 30-day money-back guarantee! ✌ If you’d like to support the podcast and gain access to bonus content by becoming a SpaceTime crew member, you can do just that through The Big Bang editions on Patreon, Spotify and Apple Podcasts. Details on the Support page on our website https://www.bitesz.com/show/spacetime/support/ For more SpaceTime and show links: https://linktr.ee/biteszHQ If you love this podcast, please get someone else to listen too. Thank you…
Our guests: Alex Zaharov-Reutt from techadvice.life Tim Mendham from Australian Skeptics And Senior science writer and Sky and Telescope magazine contributor Jonathan Nally 🌏 Get Our Exclusive NordVPN deal here ➼ www.bitesz.com/nordvpn . The discounts and bonuses are incredible! And it’s risk-free with Nord’s 30-day money-back guarantee! ✌ If you’d like to support the podcast and gain access to bonus content by becoming a SpaceTime crew member, you can do just that through The Big Bang editions on Patreon, Spotify and Apple Podcasts. Details on the Support page on our website https://www.bitesz.com/show/spacetime/support/ For more SpaceTime and show links: https://linktr.ee/biteszHQ If you love this podcast, please get someone else to listen too. Thank you…
The Astronomy, Space, Technology & Science News Podcast.
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This is Spacetime Series twenty nine, episode one hundred and one,
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for broadcast on the twenty fourth of August twenty twenty six.
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Coming up on Space Time, NASA forced to scrap its
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Swift rescue mission, the Milky Way's first big galactic collision,
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and Understanding the stuff Adams Are made of. All that
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and more. Coming up on space Time.
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Welcome to Space Time with Stuart Gary.
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NASA has been forced to abandon its planned rescue mission
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to save the Swift Gamma ray space telescope. Ongoing attitude
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control problems with the Link rescue craft mean the mission
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has been scrapped and Swift will now be allowed to
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fall back to Earth in an uncontrolled disscent in the
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next couple of months, burning up in the atmosphere. Swift
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was designed to provide astronomers with an early warning system
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for the detection of the most powerful explosions in the universe,
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gamma ray bursts. These events only last a matter of
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seconds before quickly fading away, and Swift provided the necessary
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heads up needed to allow astronomers to swing more powerful
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telescopes towards the direction of the blasts. Swift was launched
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in November two thousand and four on a six hundred
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kilometer high orbit, which was thought to be high enough
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to allow it to remain operational for its primary two
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year mission, and so it wasn't equipped with any onboard
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proportion systems. However, the mission has been so successful, detecting
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around one hundred gamma ray bursts every year, that managers
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just kept the mission going for twenty one years. However,
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the current climax of the Sun's eleven year solar cycle
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has been more violent than anticipated, sending powerful solar flares
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and chronal mass ejections towards the Earth and causing the
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planet's atmosphere to wobble, expanding and contracting with each new
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space weather event, and that led to increased atmospheric drag
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on the spacecraft, accelerating its orbital decay. The Link rescue
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craft was meant to rendezvous with Swift. The maneuver around
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the orbital telescope, find a good attachment point, and then
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use its three robotic arms to capture and gradually boost
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Swift back up into a higher orbit. The Link spacecraft
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was floating into orbit on July the third, aboard a
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Northrop Grumm and Pegasus Excel rocket which was drop launched
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from the underbelly of especially modified Lockheed L ten eleven
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Trista airliner forty thousand feet above the South Pacific Ocean.
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Mission managers established communications with Link and conducted in orbit
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checkouts over the following weeks. However, the Link spacecraft suddenly
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experienced a major anomaly, sending the vehicle into an uncontrolled
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multi axis spin, tumbling widely in orbit, and sporadically losing
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communications with mission managers on the ground. While the rescue
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vehicles operators Catalyst Space were able to get some control
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over the spacecraft, it wasn't enough to save the mission,
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and so NASA have taken the decision not to proceed
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with a rescue attempt. This is space time still to come,
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the Milky Way's first big galactic collision and understanding the
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stuff that Adams are made of. All that and more
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still to come on space time, Astronomers have discovered what
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was probably the first major galactic collision involving our home galaxy,
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the Milky Way, cannibalizing a dwarf galaxy called the Low
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Energy Craken Heracles or LKH. Less than two billion years
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after the Big Bang, the Milky Way grew to its
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current size by consuming, merging with, or cannibalizing smaller galaxies.
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In fact, that's how all galaxies grow now. New data
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from NASA's Hubble Space telescope has shown definitive evidence of
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a dwarf galaxy merging with the young Milky Way in
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the earliest phases of its evolution. The findings, reported in
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the journal Nature Astronomy, extend sciences understanding of our galaxy's
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history by some one point eight billion years. The most
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recent massive merger in our galaxy's history took place with
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a sagittarist dwarf galaxy beginning more than six billion years
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ago and still happening today. Looking back into the even
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more distant past, astronomers learned that the Milky Way consumed
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another dwarf galaxy called the Guy Sausage and Soladus about
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ten billion years ago. This ancient merger greatly affected the
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structure of our galaxies disc of stars. Lots of other
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smaller mergers have occurred between these two major events, but
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of course our galaxy's history doesn't stop there. Both observations
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and computer simulations have suggested another much larger merger preceded
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these two, though the exact specific so this event have
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been heavily debated. Now Hubble's uncovered definitive evidence of the
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earlier merger, which occurred around eleven point eight billion years ago,
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that's just two billion years after the Big Bang. The Sturdies.
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Lead author David Massari from the Astrophysics and Space Science
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Observatory in Bologna, says, while the Milky Way's our home galaxy,
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we don't fully understand how our house was built. Using
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NASAs Hubble space Telescope, together with astronomical surveys and data
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from other spacecraft like the European Space Agency's Guy emission,
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Bazarian colleagues have been piecing together the early history of
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our galaxy. Of course, the further back in our galaxies
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history scientists attempt to look, the more difficult it becomes
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to fully understand what's going on. When the Milky Way
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was young, it was much smaller and much closer in
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size to the galaxies it was crashing into. It was
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also more chaotic, and it's possible that science of mergers
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have been erased over billions of years, and it was
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into this murky past that Hubble has been peering. The
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authors used Hubble to study the Milky Way's globular clusters,
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immense roughly spherical collections of tens of thousands to millions
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of stars. Globular clusters contain some of the oldest stars
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in our galaxy, and they get act as cosmic archaeological
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sites preserving stars from other galaxies the Milky Ways collected.
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Thanks to the high resolution and deep Hubble imaging, the
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authors rather to measure about the age and metallicity of
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these clusters with unprecedented precision. Astronomers refer to all elements
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on the periodic table other than hydrogen and helium, which
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were formed in the Big Bang as metals. And metals
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are created in stars either during their lifetime or when
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they die, and so the greater the metallicity of a star,
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the older it is. Thanks to the high resolution and
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deep Hubble imaging coupled with the measurements from GUY, this
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made it possible to distinguish a population of globular clusters
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that appear to be very different from the others. And
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these are the clusters that were born in the ancient
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dwarf galaxy LKH, and they tell both how big this
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galaxy was and when it was cannibalized by the Milky Way.
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The authors analyzed Hubble observations of thirty nine globular clusters
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from the inner twenty thousand light years of our galaxy,
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where evidence of the most ancient mergers should be preserved.
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They expected this sample to contain globular clusters that form
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within the young Milky Way, as well as those collected
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from the Gius Sausage and Solidus dwarf galaxy about ten
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billion years ago. Using Hubble's sensitive observations that determine each
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cluster's precise age and associated metallicity, Missourian colleagues determined there
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was a third population of globular clusters within the inner
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regions of our galaxy. They found these clusters are older
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than the group collected in the Gia, Sausage and Solidus merger,
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but younger than those born in the original Milky Way,
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regardless of their metallicity. These clusters therefore came from a separate,
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even earlier merger in which our Milky Way absorbed, cannibalized,
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if you will, a dwarf galaxy containing roughly five hundred
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million times the mass of our Sun, a significant fraction
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of our galaxy's total mass at the time. They named
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this dwarf galaxy Low Energy crackn Heracles or LKH in
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honor of three earlier research papers that championed the idea
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of a merger early in our galaxies history. Now, when
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you think about it, such a large merger so early
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in the Milky waste formation history would have had profound
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implications for the evolution of our galaxy. Zuri says that
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some past studies have argued that this earliest phase of
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our galaxies evolution was defined by stars born only in
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our own galaxy, but he says this shows that stars
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born in external galaxies also need to be considered. This
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is space time still to come understanding the stuff Adams
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are made of. Later in the science report, successful phase
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three trials of a new Australian developed personalized mRNA cancer vaccine.
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All that and more still to come on space time.
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New observations made at the Large Hadron Collider the Ward's
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Biggus atom smasher, are revealing some of the basic fundamental
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physics of our universe. The new measurements are challenging long
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standing hypotheses of how gluons behave inside atomic nuclei. Gluons
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are force particles that bind subatomic elemental particles called quakes
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together inside protons and neutrons making up the nucleus of atoms. Now,
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new research by the Alis experiment turns large hadron collider
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is showing how two rival explanations for how gluons behave
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inside atomic nuclei can now be experimentally distinguished. The researcher,
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reported in the journal Physical Review Letters, provides the first
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multi dimensional measurements of incoherent JSI photonuclear production as a
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function of both interaction energy and momentum transfer. Sagement gives
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scientists their clearest view yet of how gluons act at
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high energies. One of the studies authors, Daniel Tapia Takaki
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from the Allis Collaboration at CERN, the European Organization for
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Nuclear Research, says that although quarks are often described as
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the fundamental building blocks of matter, nearly all the mass
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of the visible universe, from the atoms in your body
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to the matter inside stars, actually comes from the energy
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carried by gluons, the strong nuclear force that binds quarks together.
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Understanding how gluons behave inside nuclei is therefore essential to
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understanding how matter itself acquires its mass and structure. The
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study of how gluons fluctuate within nuclei with more spatial
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resolution than ever previously possible. The authors used an experimental
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technique called incoherent JSI furt nuclear production. Tapia Dakaki says
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the measurements were performed using data collected during run two
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of the large Adrin Collider. We're fast moving lead nuclei
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pass close to one another without directly colliding. In these encounters,
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intense electron magnetic fields surrounding the nuclei behaved as beams
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of high energy photons. When one of these photons strikes
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another nucleus, it can briefly produce a particle called JSI,
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whose production provides a sensitive probe for the underlying gluon structure.
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Unlike other measurements that average over the entire nucleus, incoherent
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JSI production is sensitive to local fluctuations in gluon density,
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allowing scientists to probe structures smaller than a proton. And
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these intense glu on fields, present inside every nucleus, make
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up nearly all of the visible matter in the universe,
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yet their collective behavior remains one of the greatest challenges
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in modern physics. Tapi Takaki says these experiments using incoherent
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production is sort of like switching from a blurry image
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to a high resolution microscope. It allows scientists to see
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how gluons fluctuate and organize themselves inside atomic nuclei. By
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varying the momentum transfer, the experiment effectively changes the focus
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of the microscope. At resolutions of zero six, zero three,
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and zero two femptometers, allus progressively probe smaller and smaller
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origins inside the nucleus. The finest resolution corresponds to structures
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only a quarter the size of a proton. At these
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extraordinary scales, physicists have observed evidence that the gluons begin
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to behave collectively, a phenomenon known as gluon saturation. The
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authors measured incoherent jside production across a wide range of
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photon nucleus energies from twenty right up to six hundred
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and thirty three billion electron vaults. At the same time,
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they also examined how the interaction changes with momentum transfer,
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which corresponds to how finely the nucleus is being probed.
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The results revealed a striking pattern at the smaller special
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scales explored, the production rate of J side particles was
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significantly suppressed, with a statistical significance of about three standard deviations.
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This suppression challenges a long standing explanation known as nuclear shadowing,
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which is successful describe previous measurements. Now in that framework,
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glawns inside the nucleus partially overlap and obscure each other,
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similar to layers of clouds blocking out sunlight, reducing the
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probability of certain particle production processes. The new measurements indicate
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that conventional nuclear shadowing alone can't fully explain the observed data. Instead,
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the observations are consistent with a different phenomenon known as
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gluon saturation, which is predicted by the theory of quantum chromodynamics,
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which describes the strong nuclear force the peer. Takaki says
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that in this regime, lawns become so densely packed that
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they begin interacting strongly with one another, limiting how many
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can exist in a given region. The project is just
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one of hundreds of experiments being undertaken by CERN, the
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European Center for Nuclear Research CERN.
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Is the world's largest particle physics research laboratory. It covers
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six square kilometers scattered over twelve sites either side of
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the Franco Swiss border near Geneva, in thirty four kilometers
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of tunnels and caverns the size of cathedral at over
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one hundred metres underground. CERN hosts facilities for experimental physics.
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Scientists from all over the world work here in international
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collaborations to study and understand the mysteries of the universe, stars, planets, sees, air, humans.
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Everything around us is made of matter. Matter is made
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of atoms. Atoms are made of electrons orbiting around a nucleus,
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which in turn is made of protons and neutrons. Inside
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these we find quarks. In CERN's newest accelerator, the Large
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Hadron Collider, particles collide at nearly the speed of light
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to study the quarks and other particles. Many of these
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particles only existed in the early universe for a fraction
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of a second after the Big Bar, when all the
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energy transformed into matter. In CERN's accelerators, we can recreate
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conditions that existed just after the Big Bang and shed
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light on such questions as why do particles have mass,
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what is the nature of dark matter in the universe,
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why did matter triumph over antimatter in the first moments
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of the universe, making our existence possible. What was the
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state of matter just after the Big Bang? For gigantic
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instruments called particle detectors study the data from the LHC
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collisions in search of the answers to these fundamental questions.
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The experimental and theoretical study of these conditions allows us
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to understand the fundamental laws of nature and to unveil
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the ultimate mysteries that govern our universe. In the course
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of their research, certain scientists have often come across discoveries
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that have affected our everyday life. The technology used for
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particle detectors is at the origin of security scanning equipment
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and several medical applications, and the World Wide Web was
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