July 15, 2026
Cosmic Discoveries: Japan's Asteroid Encounter and the Life Potential of Europa
SpaceTime Series 29 Episode 84 Japan swoops past a cosmic snowman shaped asteroid Japan’s Hayabusa2 spacecraft has just swooped past a tiny asteroid in deep space that’s shaped like a snow man. Revealing the secrets of the ice moon Europa A new study has shown that the Jovian Ice Moon Europa is reflecting radio signals in a strange unexpected way. What happens to Earth when the Sun dies A new study has provided astronomers with a glimpse of the future we’re likely to face when our Sun dies in around seven billion years from now. The Science Report Study’s show early risers have more nutritious diets than people who prefer staying up late. Australia shown to be home to a large chunk of the world's seagrasses, but is losing them rapidly. A new study claims Meta’s AI smart glasses could help people with low or no vision. Data centres found to have a far bigger carbon footprint than previously thought. Alex on Tech: Samsung Galaxy Z fold 8.
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The Astronomy, Space, Technology & Science News Podcast.
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It's is Spacetime Series twenty nine, episode eighty four, for
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broadcast on the fifteenth of July twenty twenty six. Coming
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up on Spacetime, Japan swoops past a cosmic snowman shaped asteroid,
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revealing the secrets of the ice moon Europa and what
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will happen to the planet Earth when our Sun dies?
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All that and more coming up on Spacetime.
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Welcome to space Time with Stuart Gary.
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Japan's Hiblsit spacecraft has just swooped past a tiny asteroid
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in deep space that shed like a snowman. Traveling at
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more than eighteen thousand kilometers an hour, the probe flew
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within eight hundred meters of the tiny Earth asteroid. The asteroid,
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called Torri Foon, was known to have an elongated shape,
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but its exact details were unknown until this flyby. Ground
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based observations suggested that it was a stony or silicon
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S type asteroid around four inch and fifty meters wide.
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These are high density asteroids that make him about seventeen
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percent of the entire asteroid population of our Solar System,
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making them the second most common type after carbonaceous C
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type asteroids. Images of the space rock taken by the hybris.
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The two spacecraft revealed what appeared to be a contact binary,
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two round objects, one bigger than the other, joined together
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and strewn with surface rocks and boulders. Contact binaries are
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composed of two separate asteroids that previously orbited a common
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center of gravity, eventually spiraling in towards each other and
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then molding together to form a single body. The Hibers
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two mission by JACKSA the Japan Aerospace Exploration Agency was
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designed to demonstrate our mission managers could precisely control the
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dejectory of the spacecraft ever be needed to perform an
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asteroid deflection maneuver. It follows NASA's successful twenty twenty two
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dart Or double asteroid redirection test that changed the orbit
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of one hundred and sixty meters white asteroid Dimorphous by
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deliberately smashing into it with a spacecraft. Impact cameras Abord
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hier Bussa II studied Toifin's surface, including geographical features, its texture,
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and temperature, vital information for future planetary defense missions. See
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If astronomers need to deflect an asteroid at some time
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in the future by impact, the response won't be the
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same for every asteroid. It depends on whether the asteroid's
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a rubble pile or a solid rock, and this is
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in the end of Jack's punetary defense efforts. The agency,
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together with the European Space Agency, are teeming up on
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another planetary defense mission, this one to explore the asteroid
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of Offits, which will pass close to the Earth in
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April twenty twenty nine. Launched back in twenty fourteen, Hibusat
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is already scientists by landing on and gathering material from
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the asteroid Rayugu, which was some three hundred million kilometers
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from the Earth. Six years later, it brought those samples
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to Earth, providing scientists with clues about what the Solar
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System was like at its birth some four point six.
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Billion years ago.
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After the Tory food mission, Hybussitu's next milestone will be
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in December twenty twenty seven, when it swings past the
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Earth on a gravity assist maneuver. Then in June twenty
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twenty eight, they'll swing past the Earth again and that
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will set it up for its next rendezvous with the
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asteroid nineteen ninety eight k Y twenty six in July
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twenty thirty one. A little bit the asteroid for a
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while and eventually land on it. The exact nature of
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nineteen ninety eight k Y twenty six is still unclear.
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Optical and radar observations suggest it's a water rich world,
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and since it's known to be a fast rotator, it's
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likely there'd be a single chunk of rock rather than
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a rubble pile asteroid. Needless to say, we'll keep you
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in form owned this is space time still to calm.
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Revealing the secrets of the ice moon Europa and what
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will happen to the Earth when our sun dies. Scientists
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may have gotten a bit of a glimpse from a
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distant star system. All that and more still to calm
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on space time. A new study has shown that the
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Jervian ice moon Europa is reflecting radio signals in a
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strange and unexpected way. The findings are providing intriguing new
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clues about this frozen world, which contains a global subsurface
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liquid water ocean hidden below an estimated twenty five kilometer
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thick ice sheet. The ocean is kept liquid by tidal
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heating caused by constant gravitational pulling and pushing on Europa
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as it orbits its giant host plot Jupiter and similar
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smaller gravitational perturbations caused by its many sister moons. These
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tidal interactions cause internal friction inside Europa, which is generating
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enough heat to melt the ice into water, producing more
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water than all the Earth's oceans combined, and it doesn't
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end there. Sighters speculate that that tidal heating could also
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be generating geological features similar to the mid ocean ridges
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common in seas on Earth. On Earth, these mid ocean
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ridges are but unique life forms feeding on the chemicals
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being pumped out through formations such as hot springs and
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black smokers. Many sighters speculate that this hot chemical soup
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might be where life on Earth first began, and that
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raises the interesting possibility of whether the same thing is
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happening in the oceans of Europa. You see, if we
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do find life on Mars past or present, that could
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have been the result of meteorite contamination from the Earth.
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Or on the other hand, life on Earth may well
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have originated on Mars. That's because Mars and the Earth
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have been squat rocks for billions of years, so the
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possibility of cross contamination is always there. But the Jervian
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system is much too far away, so any life found
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there would likely have started independently, and if it starts
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independently on Europa, that means life could start anywhere in
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the universe.
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The preponderance of.
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Life we see in Star Trek might well be real.
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To discover more about Europa, astronomers use NASA's Goldstone radar
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and the US National Science Foundation's Greenbank radio telescope to
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carry out the most extensive radar study yet of the
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ice moon. By repeatedly pinging Europa with three point five
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centimeter radio waves, the authors measure how the moon reflects
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radar signals and confirm that its icy surface scatters radio
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energy in an unusually strong and complex way not seen
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on rocky worlds. Jupiter has four big Galilean moons i
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Owe Europa Ganny meaning Callisto, and those last three, Europa
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Gany meaning Colie, are especially intriguing to scientists because they
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all have icy outer shells and are thought to hide
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oceans of liquid water underneath. Of the three, Europa is
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a prime target in the search for habitable environments beyond Earth.
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Geologic features provide clues to how the ice shall underlying
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oceans interact, but these features only reveal what's happening at
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or near the surface. One of the studies authors, Tng
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from the University of California, Los Angeles, says radio waves
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can penetrate deep into the ice and determined features about
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its internal structure and purity. These new observations show that
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Europa's radar albedo, that is a measure of how bright
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it appears in radar, is much higher than that of
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typical planets and asteroids. The returning radar signal is dominated
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by the same circular polarization as the transmitted beam, and
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that's a hallmark of modible scattering inside clean.
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Porous ice.
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These properties strongly support an explanation known as the coherent
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backscatter opposition affair, in which radio waves bounce around inside
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the ice before returning to the telescope, dramatically boosting the echo.
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Because Gene colleagues observed Europa as a bistatic configuration with
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Goldstone transmitting in both goldstone and greenback receiving, it could
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also test how the coherent backscatter effect changes with the
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angle between transmitter Europa and receiver, and the authors found
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Europa's radar brightness stayed roughly consistent even when the angle increased.
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That implies that the bright back scattered peak must be
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broader than the range of the angles it's sampled, placing
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a limit on the depth that the radio waves diffused
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before being absorbed, and that depth limit offers a new
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constraint on how transparent Europa's ice is and that will
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help scientists interpret upcoming ice penetration radar data from mass
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is europa Clipper mission and the European Space Agency's Due spacecraft,
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which are both now on their way to the Jovian System.
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The new results also fill a three decades long gap
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is the last major radar study of your Back in
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the nineteen eighties and early nineties, and the authors found
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strong agreement between their measurements and those of the earlier
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results That reinforces the picture of Europa as an object
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with a very high radar reflectivity and strongly diffuse scattering,
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rather than the mirror like reflections seen on many rocky surfaces.
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This consistency increases the confidence that Europa's radar properties are
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stable over time and that both earth based and spacecraft
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radar measurements can be interpreted within a unified physical framework.
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Because the observing campaigns spanned many years. In viewing geometries,
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the authors asked whether Europe's radar brightness changed from one
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hemisphere to the other or with longitude, and they found
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that Europea's disc integrated radar properties are statistically consistent with
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remaining nearly constant as the moon rotates, which also agreed
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with the earlier observations. However, when the authors divided the
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data into leading and trailing hemispheres and performed statistical analysis,
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they saw a hint and not statistically conclusive, that the
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trailing hemisphere could be slightly brighter in one polarizing state. Now,
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if confirmed by future observations, that subtle difference could be
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related to how charged particles from Jupiter's magnetosphy a modifying
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the ice or affecting the formation of small scale surface
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structures that absorb le scatter radio waves. Whether that provides
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a catalyst for the formation of life is another question.
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In fact, the entire question of whether life does exist
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in the depths of the global seas beneath the Europe's
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icy surface is still open for debate. This report from MESSERTV.
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That's a great question, and it's a question that NASA
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will seek to answer with the Europa Clipper spacecraft. Europa
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is a moon of Jupiter. It's about the same size
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as Earth's moon, but its surface looks very different. The
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surface of Europa is covered with a layer of ice,
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and below that ice, we think there's a layer of
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liquid water, with more water than all of Earth's oceans combined.
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So because of this giant ocean, we think that Europa
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is actually one of the best places in the Solar
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System to look for life beyond the Earth. Life as
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we know it has three main requirements. Liquid water. All
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life here on Earth uses liquid water as a basis.
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The second is the right chemical elements. These are elements
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like carbon, hydrogen, nitrogen, oxygen, phosphorus, sulfur. They're elements that
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create the building blocks for life as we know it
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on Earth. We think that those elements exist on Europa.
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The third component is an energy source. As Europa orbits
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around Jupiter, Jupiter's strong gravity tugs and pulls on it.
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It actually stretches out the surface and it produces a
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heat source called tidal heating. So it's possible that hydrothermal
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systems could exist at the bottom of Europa's ocean and
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it's possible that those could be locations for abundant life.
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So could there be life on Europa? It's possible, and
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Europa Clipper is going to explore Europa to help try
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to answer that question.
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That report from that's a TV we heard from the
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agency's punetary geologist, Cynthia Phillips. This is space time still
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to come what happens to the Earth when the Sun dies?
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And later in the science report, a new study found
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that data centers far more massive carbon footprints than previously thought.
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Seems they may be great for technology's advancement, but they're
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not good for the environment. All that and more still
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to come on space time. A new study that's provided
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astronomers with a glimpse of the future we're likely to
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face when our Sun dies in around seven billion years
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from now. The Sun will eventually run out of the
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core hydrogen it uses the fuse into helium, the process
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that makes the sun shine. When that happens, the core
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will contract, increasing in temperature and pressure until it gets
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hot enough to begin fusing helium in the core into
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carbon and oxygen. At the same time, a shell of
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hydrogen outside the core will begin burning. Now, all this
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increased temperature will cause the Sun's auter atmosphere to expand,
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becoming one hundred times bigger than it is now. As
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it expands outwards, the Sun's now bloated surface, being further
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away from the core, will start to cool down, turning
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our star into a red giant. Finally, then our bloated
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Sun will puff off its outer gaseous layers, which will
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float away as a planetary nebula, leaving behind its searingly
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hot stellar core about the size of the Earth called
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a white dwarf. Now, as the Sun transforms into a
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red giant, it will consume the inner planets of our
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Solar system, Mercury and Venus, and most likely the Earth
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as well. Even if the Earth does survive, it'll be
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roasted to a crisp. However, the fate of the more
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distant planets, especially the gas giants, is still unclear. Finding
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and studying planets that orbit around the remnants of Sun
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like stars after their death is a means astronomers have
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for learning what might happen to our Solar System in
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the far distant future. So astronomers using NASA's web Space
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Telescope now studied a distant star system made up of
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a white dwarf star about ten million years old, which
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is being orbited by a gas giant planet named w
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D eighteen fifty six B, which is somewhere between four
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point three and ten point nine times the mass of Jupiter.
234
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Their five dings are reported in the journal Nature. So
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this gas giant has a thick methane aerosol atmosphere and
236
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a Balmi temperature of between one hundred and seventeen and
237
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one hundred and thirty nine degrees celsius, which the authors
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00:14:39.960 --> 00:14:42.080
say is quite a lot hotter than expected for a
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planet of the size. WD eighteen fifty six B was
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discovered in twenty twenty by scientists using NASA's tests Transitting
241
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Exoplanet Survey satellite and the Spitzer Space Telescope.
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It's orbiting its host white dwarf.
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Star WD eighteen fifty six plus five point thirty four,
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24
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26
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27
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35
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36
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39
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63
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64
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65
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66
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67
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68
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69
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70
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71
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72
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73
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82
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85
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90
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91
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92
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95
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96
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99
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102
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103
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104
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105
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106
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108
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109
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111
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112
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115
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117
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118
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119
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120
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121
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122
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123
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126
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127
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128
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129
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130
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131
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132
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133
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134
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135
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136
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137
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138
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139
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140
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141
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142
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143
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144
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145
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146
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147
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148
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149
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150
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151
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152
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153
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154
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155
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156
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157
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158
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159
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160
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161
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162
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163
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