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This is Spacetime Series twenty eight, episode one hundred and
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forty nine, for broadcast on the nineteenth of December twenty
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twenty five. Coming up on Space Time, the earliest super
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and over ever seen. New clues suggest that liquid water
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and consequently the potential for life could still exist on
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the red planet Mars today and the Great Geminid's meteor
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shower of twenty twenty five. All that and more coming
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up on space Time.
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Welcome to space Time with Stuart Gary.
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Astronomers have detected the earliest supernova ever seen, dating back
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to a time when the universe was just seven hundred
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and thirty million years old. The observations, reported in the
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journal Astronomy in Astrophysics, were made using the web Space Telescope.
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The exploding star, catalogged as GiB twenty five zero three
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fourteen A, emitted a super bright flash of light known
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as a gamma ray burst. The detection broke the previous
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super and ova distance record, an event dating back some
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twelve billion years. The studies lead author, Andrew Levin from
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Redbound University in the Netherlands, says this new detection shows
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that astronomers using web can find individual stars when the
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universe was just five percent of its current age. While
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a gamma ray burst typically lasts for just seconds or minutes,
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a supernerva rapidly brightens over several weeks before it slowly
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begins to dim. In contrast, this supernova brightened over months.
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Since it exploded so early in the history of the universe,
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its light was stretched as the cosmos expanded over billions
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of years. As light is stretched, so is the time
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it takes for events to unfold. Web's observations were intentionally
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taken three and a half months after the gamma ray
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burst ended, since the underlying supernova was expected to be
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brightest at that time. Gamma ray bursts are incredibly rare.
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Short period gamma ray bursts can last for just a
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few seconds and are thought to be caused by the
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merger of two neutron stars creating a black hole, or alternatively,
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by the merger of a neutron star into a black hole.
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On the other hand, long period gamma ray bursts can
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last around ten seconds and are thought to be caused
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through the explosive supernova deaths of massive stars resulting in
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the formation of a black hole. As for this event,
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the first alert was sent out back on March the fourteenth,
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news of a gamma ray burst from a very distant
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source came from so FOAM, the space based Multiband Astronomical
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Variable Object's Monitor mission, which is designed to detect brief
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transient events like gamma ray bursts. Within ninety minutes, NASA
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Swift Space Telescope pin pointed the X ray source's location
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in the sky, and that enabled subsequent observations to pin
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down the distance for where ZEB. Eleven hours later, the
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Nordic Optical Telescope on the Canary Islands was skewed up
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and revealed an infrared light gamma ray burst afterglow, an
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indication that gamma rays might be associated with a very
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distant object. Four hours later, the European Southern observatori's Very
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Large Telescope, the VLT in Chile estimated the object existed
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just seven hundred and thirty million years after the Big Bang.
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Eleven points out there have only been a handful of
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gamma ray bursts in the last fifty years that have
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been detected during the first billion years of the universe's existence,
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and he says that makes this event both very rare
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and very exciting. Since this is the earliest and most
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distant superinova ever seen. Astronomers compared it to modern day,
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more nearby supernovae. Amazingly, the two turned out to be
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very similar. That's surprise scientists because very little is known
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about the first billion years of the universe's existence. It's
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thought that early stars likely contained far fewer heavy elements,
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they were more mad, and they led far shorter lives.
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They also existed during the epoch of realization, that's when
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the gases between galaxies was largely opaque. The high energy
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light but WEB showed that this supernova looked exactly like
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modern supernovae. Before researchers can determine why such an early
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supernova is so similar to nearby events, more data will
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need to be gathered in order to pinpoint tiny differences.
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The web observations also indicate that the distant galaxy from
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which the supernova originated was also similar to other galaxies
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that existed around that same time. Since the galaxy's lights
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blended into a few pixels, making the galaxy look like
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a red and sponge, astronomers are still limited and exactly
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what they can learn about it. Still seeing it at
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all is a major breakthrough this is space time still
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to come. New clues suggest that liquid water and consequently
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the potential for life could still exist on the red
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planet Mars today, and how to observe the Great Geminids
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Metea or Shower of twenty twenty five. All that and
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more still to come on space time. A new study
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based on seismic data suggests that liquid water and the
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potential for life could still exist beneath the surface of
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the red planet Mars today. The findings are based on
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a new evaluation of mass quakes recorded by NASA's Mars
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Inside lander, which touched down on the red planet in
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twenty eighteen. This lander used its robotic arm to place
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a seismometer on the Martian surface, designed to measure seismic
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waves generated by meteor impacts or Martian geologic activity, and
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thereby providing a picture of the planet's interior. One of
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the studies authors, Ikukatama from Hiroshima University, says the new
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interpretation of this seismic data does suggest the presence of
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liquid water below the surface, and if liquid water does
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exist on Mars, that would present a habitable location for
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microbial activity. That is, if life does exist on the
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red planet. When a Mars quake, if that matter, a
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meteorite impact occurs, Insight was able to read that energy
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emitted as pea waves, S waves, and surface waves, allowing
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it to create an image of the planet's interior. Scientists
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can use the pea waves and S waves to determine
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a lot about the rocks that make up Mars, including
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the density of the material or potential compositional changes within rocks.
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For example, S waves can't travel through water, and they
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move at a much slower speed than pea waves. Therefore,
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the presence, absence and arrival time of S waves can
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determine what the subsurface looks like. Pea waves travel faster
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through high density material and slower through less dense stuff,
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so their velocity can help determine the density of the
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material they're traveling through, as well as if there are
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any changes in the density along the way. Searsmic data
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collected by Insight shows boundaries at a depth of round
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ten kilometers and at twenty kilometers based on discrepancies in
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the searsmic velocity. Now, these boundaries had previously been interpreted
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as sharp transitions in the porosity of rocks or the
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chemical composition of the Mustian interior. However, Caddiamor and colleagues
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have interpreted these cracks as potential evidence of water within
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the Russian subsurface. They say the searsmic data indicates a
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boundary between dry cracks and water filled cracks in the
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Russian subsurface. In order to test the hypothesis, the authors
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measure the searsmic velocity passing through rocks with the same
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structures and composition of typical Marshan crustal rock under wet, dry,
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and pros and conditions. Typical Martian rocks are similar to
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the diabase rocks found in Sweden due to their evenly
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sized plagia eclays and orthopyroxine grains. In the lab, Catiamor
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and colleagues measured P wave and S wave velocities using
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a piezoelectric transducer, which uses electrical energy as a wave
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source that monitors seized mcwave energy on dry, wet and
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frozen diabet samples. Their work showed that the searsmic velocities
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of the dry, wet and frozen samples were significantly different.
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That supports the idea that the boundary at ten kilometers
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and twenty kilometers could be caused by a change from
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a dry rock to a wet rock. These laboratory experiments
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back up the hypothesis that the boundary measured by seismic
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data indicates a transition from dry to wet rocks rather
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than a change in porosity or chemical composition. Katiyama says
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the findings therefore provide compelling evidence for the existence of
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liquid water beneath the Martian surface this space time still
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to come the Great Geminid Shower of twenty twenty five,
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and later in the Science report, a new study shows
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that the family housecat will mew more frequently for male
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caregivers and female ones, and the studies authors think they
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know why. All that and more still to come on
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space time, one of the most spectacular meteor showers of
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the year is now at its peak, giving sky watch
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is a chance to see up to one hundred meteors
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an hour under perfect conditions. The Geminids are visible between
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now and December the twentieth. They're considered to be one
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of the best and most reliable annual meteor shower events.
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They were first observed in eighteen sixty two and are
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thought to be intensifying every year. Most meteor showers are
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caused by comets, but the Geminids are unusual because they
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originate from a debris trail left by an object known
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as thirty two hundred feeton, which is more likely an asteroid.
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Rather than being white like other meteors, the geminids have
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a distinct greenish hue when they burn up in its atmosphere.
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That's because their chemical composition oxygen, magnesium, and nickel usually
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produce a green color. Meteors are small pieces of interplanetary
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debris which spurn up in its atmosphere after coming in
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at high speeds, typically around one hundred and thirty thousand
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kilometers an hour. In the case of the geminids, friction
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in the upper atmosphere quickly heats up the incoming debris.
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The air around them glows brightly, and the particles are
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rapidly destroyed. The resulting streak of light is what we
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see on the ground as a meteor, often incorrectly referred
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to as a shooting star. Robert Messi from the Royal
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Astronomical Society says the best way to see the geminids
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is in dark skies, well away from any light source.
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He says you can expect to see perhaps one hundred
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meteors an hour, and that means around one or two
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every minute.
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The Geminids are in meteor shower, and in this particular case,
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they all appear if you trace the meteors palms backwards
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to originate from a point in the sky in the
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constellation of Geminy near the bright Star Castle. And like
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other meteor showers, they're connected with a particular celestial object. Now,
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most meteor showers we connect to commets. In this particular case,
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they appear to originate from the asteroid thirty two hundred
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feeth On, which could be a weird example of something
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called a rock comet, which is putting debris into the
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Solar System, and once a year the Earth runs into
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that debris. It burns up in the Earth's atmosphere, and
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that's when we see a meteor shower with meteors. What
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you're going to expect to see is something that you
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might regard as a shooting star, in other words, a
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short streak of light that generally lasts maybe half a
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second or so, usually so quick it's impossible to point
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out someone you're with, so you need to keep your
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eyes up the advice on looking for them is to
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get yourself something comfortable to actually lie down on or
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sit down on, So take out a sun lounger and
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then simply look up at the sky. Now, the best
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view is if you're away from sources of light pollution,
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so try and get away from at least direct lights
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in towns and cities, ideally out in the countryside. Obviously
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you also need a clear sky if it's cloud and
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you're not going to see anything, and then really you're
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looking up at the sky and you expect to see
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perhaps if we're lucky, up to one hundred meteors an hour,
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so that might be one or two a minute, which
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would be a brilliant view. It is one of the
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strongest showers of the year. The great thing about a
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meteor shower, including the geminids, is that actually the naked
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eye is the best way to see them. If you
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get a telescope or a pair of bronocutas, you're automatically
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restricting your view of the sky. And with a meteor shower,
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what you want is the widest possible view. You want
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to be lying down looking up at the broad panoply
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of stars. I can use that expression and watching for meteors.
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That by far the best way to do that is
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with the naked eye. Now, some people are really really
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good at taking pictures of these things too, either with
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all sky cameras or or they get lucky they've got
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camera set up on tribuds and they snap them over
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a period of time. If you do manage to get
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some photos, please share them.
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That's doctor Robert Massey, Deputy Executive Director of the Royal
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Astronomic or Society, and this space time and time out
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take another brief look at some of the other stories
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making us in science this week with a science report.
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A new study has shown that drinking three to four
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cups of coffee a day might slow down the biological
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aging of people with severe mental illnesses. The findings, reported
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in the British Medical Journal, show that coffee can produce
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an additional five extra biological years by lengthening telomerase, a
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compound structure at the end of chromosomes which acts as
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an indicator of cellular aging. While tilomere shortening is a
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natural part of the aging process, seems to be accelerated
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in those with major psychiatric disorders like psychosis, schizophrenia, and
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bipolar disorder. A recently excavated site in POMPEII may have
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solved one of the great mysteries of Roman cement. The
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site appears to have been under active construction when it
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was suddenly a badge and in the year seventy nine
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due to volcanic activity. Now archaeologists say the rare find
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of construction tools and raw materials at the site has
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allowed them to better investigate how the Romans were making
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cement at the time. They found materials including limestone and
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volcanic ash, which supports the theory that they used the
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technique called hot mixing. Mixing dry heated limestone with water