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This is Spacetime Series twenty eight, Episode one hundred and
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thirty five for broadcasts on the seventeenth of November twenty
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twenty five. Coming up on Space Time, spectacular auroral activity
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cover the planet skies, Earth's largest modern impact crater discovered
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in southern China, and a key NASA communications disc damaged
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and out of action. All that and more coming up
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on space Time.
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Welcome to space Time with Stuart Gary.
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Planet Earth's been treated to a spectacular series of auroral displays,
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the Aurora Australas and Aurora Borealis. The Southern and Northern
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lights were triggered by three massive X class solar flares,
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including a next five point one event on November eleven,
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Remember and Stay, which was the most powerful blast this
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year and the most intense since October twenty twenty four.
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These explosions triggered a series of chronal mass ejections or CMEs,
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including a fast so called Cannibal CME, traveling at fifteen
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hundred kilomets per second, which caught up with and consumed
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to earlier CMEs as all three headed directly towards the Earth.
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The events were monitored by so ASLASCOW and the GOES
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nineteen core one chronographs. The X five point one event
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was caused by an eruption from a highly active sunspot
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region known as AAR forty two to seventy four, which
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had been erupting violently for days. AAR forty two seventy
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four is enormous, with primary duck umbracres as wide or
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even wider than the Earth and an overall active region
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more than a dozen earths in diameter. The number of
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sun spots on the solar surface increases as the Sun
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moves towards solar maximum solar MAX, the climax of its
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eleven year solar cycle. The current solar cycle twenty five
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began back in November twenty nineteen, and he's now at
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its peak, so this sort of activity really isn't all
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that unusual. Sunspots are cooler and hence darker looking regions
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on the Sun's surface caused by magnetic field lines from
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deep inside the Sun extending out into space. As different
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latitudes of the Sun rotate at different rates, these magnetic
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field lines become twisted and can snap, causing magnetic reconnection
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and triggering powerful blasts of energy called solar flares. Solar
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flares are categorized in five main groups, A, B, C, M,
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and X based on their X ray intensity, with X
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being the most powerful. Each class represents a logarithmic tenfold
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increase in energy, and each grouping is further divided into
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subclasses from one to nine, except for X class events
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which can exceed nine and so are considered open ended.
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Solar flares can trigger coronal mass ejections or CMEs. These
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are blasts of magnetic energy in charged particle or plasma
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from the Sun which can be flung deep into space
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as geomagnetic storms. When these solar storms reach the Earth,
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the flux of ionized particles can slam into the planet's
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magnetosphere and are guided by the planet's magnetic field lines
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through the ionosphere, a region already filled with charged particles,
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and down towards the north and South magnetic poles. This
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triggers the excitation of atoms and molecules in the atmosphere,
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causing auroral displays, just like those we've just witnessed. Different
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atoms and molecules light up in different colors at different altitudes.
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The colours being emitted depends on the particles being ionized
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reddish brown glows are caused by the collision of particles
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with single oxygen atoms in the Earth's upper atmosphere, usually
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above three hundred kilometers. Lower down, a green hue is
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created by single oxygen atoms. Down to an altitude of
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around one hundred kilometers, the kaleidoscope turns to a whitish,
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yellowish beige, and nitrogens mixed in with the oxygen. Aurora
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also exhibit blue, red, and evil purple blows in the
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lower atmosphere. These are caused by the excitation of molecular
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nitrogen Below one hundred kilometers. Auroral displays are common at
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high latitudes, but these latest events were seen globally at
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far lower latitudes than usual, including reports from Sydney and
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even as far north as Cairns in tropical Queensland north
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of the equator. Auroral activity was seen as far south
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as Florida. Space weather forecaster Gene Young from the Australian
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Bureau of Meteorology says auroral events are spectacular and well
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worth a look if you get the chance.
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You do have to be pretty lucky to see an aurora,
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but if you do see one, you won't be disappointed.
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The brightest auroras are concentrated in rings called the aurora
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ovals around the North or South poles. The auroras in
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the northern hemisphere are called Aurora borealis. Southern lights are
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called Aurora australis. Astrallus comes from the Latin word for
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southern Their best feud from Antarctica tasmi and the southern
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mainland coastlines. The colors displayed by an aurora are generally
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visible to the naked eye if you're near the pooles.
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This is because the aurora is overhead and more intense. However,
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at lower latitudes, the auroras are on the horizon, less
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color is seen by the naked eye. The lights tend
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to be shades of gray. However, if there is a
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high intense solar storm, there will be more color. Auroras
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can occur at any time in the year, but they're
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most likely to occur during the months of March and September.
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That's when the Earth's magnetic field is best oriented to
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interact with the solar wind. Of course, you ideally need
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a dark night with little cloud cover. You don't want
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a bright moon or any light pollution, so good location
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is a dark beach or a hill where you have
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an unobstructed view to the south. Bright auroras usually last
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for one to three hours, and the best viewing time
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is around midnight between ten pm and two am. When
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we forecast solar wind conditions that look favorable for auras
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occurring in the next one to three days, the forecasters
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from the Bureau Space Weather Center issue what's called an
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aurora watch notice when there's a high chance that there
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will be an aurora visible. Now, we issue an aurora alert.
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To be truthful, nothing beat seeing an aurora with the naked.
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Eye that space with the forecast Genine Young from the
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Bureau of Meteorology. But as well as spectacular auroral displays,
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these space wheather events can damage or even destroy spacecraft.
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They can disrupt communications and navigation systems, force aircraft to
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change their flight paths, trigger widespread power blackouts, and increase
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radiation exposure for astronauts and people in high altitude aircraft.
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All three of the coronal mass ejections last week slammed
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into the Earth, with the most severe X five point
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one class event, powerful enough to cause radio blackouts across
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Africa and Europe and disrupt high frequency communications on Earth.
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Sunlit side. Forecasters from the National Oceanographic and Atmospheric Administration
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NOAH are evaluating the Sun's activity and they could increase
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the threat level. According to the Space Weather Scales, there
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is currently a G three watching effect, which means there's
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a strong chance a geomagnetic storm could disrupt its magnetic
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field and effect communications. If NOAH raises the watch level
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to a G four, that means there's a higher chance
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of widespread problems with electrical communications and spacecraft operations. The
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highest watch level is a G five. This report from NOAH.
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What is space weather? When you think of weather, you
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probably think of Earth's weather snow, rain, and of course sunshine.
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Thank goodness, we only have Earth's weather to worry about, right.
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Actually that's not quite true. Did you know the Sun
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has weather?
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Two.
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We call this space weather. The Sun is a bubbling,
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boiling ball of gas and energy. It constantly belches out
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great clouds of hot gas that is charged up with electricity.
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This stuff travels through space really fast, some of it
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right toward Earth. This means that Earth's weather happens inside
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the Sun's weather. Thank goodness, we're mostly protected from this
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blast by Earth's magnetic field and atmosphere. Solar wind flows
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outward from the Sun charged particles, and that solar wind
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interact with Earth's magnetic field. That interaction can cause energy
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and particles to stream down to Earth's poles. When these
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charged particles hit oxygen and nitrogen atoms in Earth's atmosphere,
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the energy from the collision can create beautiful shades of
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green and red. We call these glowing colors the Northern
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lights and Southern lights, or the Aurora Borealis and Aurora Australia.
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They are beautiful curtains of light that move and sway
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in the night sky. But sometimes the Sun releases more
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energy than usual. These sudden and intense hiccups and burbs
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are called solar flares and coronal mass ejections. These are
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huge explosions of high energy X rays, charged particles, and
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magnetic field. When the Sun's burps of X rays and
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charged particles and magnetic field reach Earth, they can cause trouble.
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Bad space weather can interrupt radio signals. It can also
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damage satellites. Electrical systems that bring power to our homes
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and businesses can be knocked out by this bad space
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weather too. That is why the goes short for Geostationary
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Operational Environmental Satellite has instruments like the Solar X Ray
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Imager to monitor the space around Earth for an increase
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in high energy particles from the Sun. We can't see
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the Sun's harmful X rays with our eyes, but these
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special telescopes can. Forecasters at the Space Weather Prediction Center
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analyze these observations and issue alerts and warnings about space
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weather that could harm satellites and the power grid. With
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early detection from satellites like the goes Are series, power
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companies and satellite operators alike will have enough time to
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adapt to any troubling space weather headed our way.
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This is space time still to come. Earth's largest modern
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impact credit discovered in southern China, and a key NASA
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communications dishes damaged and out of action. All that and
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most still to colm on space time, scientists have discovered
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what appears to be the largest modern impact crater on Earth.
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The nine hundred meters wide Ginlling Crater was founding Guandong
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Province in southern China, nestled on a hillside and preserved
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within thick granite weathering crust. A report in the journal
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Matter and Radiation at Extremes claims the impact structure dates
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to Earth's current geological epoch and is remarkably well preserved now.
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Based on measurements of nearby soil erosion. The studies authors
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claim the impact likely hit during the early to mid Holocene,
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that's the current geological epoch, which began at the end
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of the Last Ice Age around eleven thousand, seven hundred
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years ago. The steadiesly author Mingcheng says it's one of
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only around two hundred identified craters worldwide and could provide
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new insights on how extraterrestrial bodies collide with the Earth.
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It's also the largest known impact crater from the Holocene,
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far exceeding Russia's three hundred made a Malca crater, previously
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the largest known impact structure from this eparch. Ming says
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the discovery shows that the scale of impacts from small
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extraterrestrial objects on the Earth in the Holocene is far
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greater than previously recorded. In this case, the impact would
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have been a metia or rather than a comet, which
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would have left a crater at least ten kilometers wide. However,
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Ming and colleagues have not yet determined whether the impacting
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meteorite was made of iron or stone. The authors say
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one of the most surprising traits of the crater is
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how well preserved it is, especially given the regions monsoons,
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heavy rainfall, and high humidity, all conditions that accelerate erosion
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within the granite layers that helped to protect and preserve
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of the impact structure. The authors found many pieces of
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quartz with unique micro features called planar defamation features. Geologists
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can use this as evidence for some specific types of impacts.
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Ming says on Earth, the formation of planar deformation features
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in quartz only happens in really intense shock waves generated
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by telets to your body impacts, and its formation pressure
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ranges from ten to thirty five gigapascals, which is a
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shock effect that cannot be produced by any geological processes
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of the Earth itself. Now, it's generally accepted that throughout
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Earth's history, virtually every point on the planet's surface faces
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a roughly equal chance of being hit by an extraterrestrial object. However,
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geological differences mean the historical footprints of these impacts have
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been eroded at different rates, and many have now fully disappeared,
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and that makes the Ginlin Crater's discovery especially significant, Ming,
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says the impact crater is a true record of Earth's
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impact history, and the discovery can provide scientists with a
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more objective basis for understanding the distribution, geological evolution, and
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impact history of small terrestrial bodies. This is space time
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still to come. NASAs confirmed that its key seventy meter
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Goldstone deep space communications dish is out of service following
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a major accident, and later when the science report a
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new study says twenty twenty five won't be the hottest
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yur on record, but it will come in second or third.
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All that and more still to come on spacetime. NASA
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has now confirmed that its key seventy meter Goldstone deep
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space communications dish is out of service following a major
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accident back in September. A re book by NASA's Jet
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Propulsion Laboratory in Passing to California, which operates the facility,
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says the antenna, located near Barstow, was over rotated, damaging
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cabling and piping in the center of the structure. JPL
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says hoses from the antenna's fire suppression system were also
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damaged in the incident, resulting in flooding. There is no
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timetable yet for its return to service. The antenna, designated
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DSS fourteen is the largest at the Goldstone complex and
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is essential for communication with multiple missions.
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Now.
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The facility does have four other antennas, but they're all
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small at thirty four meta dishes. NASAs Deep Space Network
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does have two other seventy meta dishes, one at its
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camera facility at Tidbinbilla and the other near Madrid in Spain,
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but the loss of DSS fourteen is putting extra strain
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on the rest of the network, which is already at capacity,
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especially with the upcoming Artemis two man mission to the Moon,
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which is slated for launch in April next year, although
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an earlier launch date of February is being considered. Other
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missions being affected include the web Space Telescope, with scientists
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00:15:40.639 --> 00:15:43.720
having to adjust its operations because of the reduced access