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This is Spacetime Series twenty eight, episode one hundred and sixteen,
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for broadcast on the twenty sixth of September twenty twenty five.
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Coming up on Spacetime, mysterious red dots in the early
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universe could there be black hole atmospheres? The discovery of
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mudible episodes of habitability on the red planet Mars, and
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the European Space Agency's newest Australian deep space dish about
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to begin operations. All that and more coming up on
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space Time.
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Welcome to space Time with Stuart Gary.
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Astronomers believe that a population of mysterious red dots spotted
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in the very early universe could be exotic stellar atmospheres
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around ancient black holes. The findings were a port order
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of the journal Astronomy. In astrophysics might represent a missing
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link the rapid growth of super massive black holes. Stellar
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mass black holes are created through the supernova deaths of
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massive stars, and those stellar massholes can get bigger and
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bigger through mergers. But the discovery of super massive black
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holes in the early universe has remained a problem. See
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there's no way enough stellar mass black holes could have
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merged back then in the amount of time available since
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the universe began, and that's where these tiny red objects
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come in. They were spotted by NASA's web Space telescope
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and there offering scientists new insights to the origins of
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galaxies in the universe, and they may represent an entirely
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new class of celestial object, a black hole swallowing massive
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amounts of matter spitting out light. Using the first data
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set released byweb back in twenty twenty two, astronomers who
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first discovered those mysterious little red dots suggested the objects
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might be galaxies. They were as mature as our current
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Milky Way is, but at a time when the universe
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itself was only five hundred to seven hundred million years old.
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That suggests that these so called universe breakers are far
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older than anyone expected in the infant universe, and that
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calls in the question what scientists had previously understood about
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galaxy formation. This new hypothesis suggested that dots may not
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be galaxies, but an entirely new class of object known
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as a black hole star. The authors say their analysis
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indicates these tiny pinpoints of light may be giant spheres
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of hard gas that are so dense they look like
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the atmospheres of a typical nuclear fusion powered star. However,
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instead of fusion, they're being powered by super massive black
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holes at their centers, which are rapidly pulling in matter
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and converting into energy in the process, giving off light.
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One of the studies authors, Joel Leega from Penn State University, says,
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as his team studied the red dots, they eventually found
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one that had so much atmosphere around it it couldn't
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simply be explained as a typical star. They originally thought
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it could be a tiny galaxy full of many spectrotype
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M red dwarf stars, but instead it's actually effectively just
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one giant, very cold star. Most stars are low mass
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spectral type M red dwarf stars. In fact, that population
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makes up about three quarters of all stars in our galaxy.
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They're typically hard to see because they're washed out by
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rare and more luminous massive stars. Still, astronomers can identify
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these stars by their glow, which is primarily in the
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red optical and their infrared end of the electromagnetic spectrum.
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While the gas around supermassive black holes is typically very
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hot millions of degrees celsius, the light from these red
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dot black holes was instead dominated by very cold gas,
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and that's similar to the atmospheres of low mass red
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dwarf stars based on the wavelength of the light they're
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giving off. The most powerful telescope in space, Web was
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designed to see the genesis of the cosmos using infrared
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sensing instruments, which are capable of detecting light that was
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emitted by the most ancient stars and galaxies. Essentially, webs
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allowing scientists to see back in time roughly thirteen point
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five billion years, pretty well near the beginning of the
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universe as we know it, and from the moment the
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telescope turned on, astronomers around the world began seeing these
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little red dance objects that appeared to be far more
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massive than what galaxy models predicted. At first, they thought
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these objects must have been mature galaxies, which tend to
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get redder as the stars inside the age, but the
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objects were too bright to be explained. Those stars would
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need to be packed in side galaxies at impossible densities.
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If this interpretation holds, it implies that stars form through
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extraordinary processes that have never been observed before. To better
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understand the mystery, the authors needed spectra, a type of
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data that could provide information about how much slight the
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objects emitted at different wavelengths. So between January and December
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twenty twenty four, astronomers used nearly sixty hours of WEB
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observation time to obtain spectra from a total of four thousand,
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five hundred distant galaxy is and that makes this one
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of the largest spectroscopic databases yet obtained from WEB. In
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July twenty twenty four, the authors spotted an object with
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a specter that indicated a huge amount of mass, making
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it the most extreme case of such an early large object.
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Astronomer's nickname the object the Cliff, flagging it as the
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most promising test case yet to investigate exactly what these
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little red dots were. The extreme properties of the cliff
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forced astronomers to go back to the drawing boards and
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come up with entirely new models. This object was so
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distant that it took light almost eleven point nine billion
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years to reach the Earth. The spectral analysis of that
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light indicates it was actually a super massive black hole,
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pulling in surrounding material at such a rate that it
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cocooned itself in a fiery ball of hydrogen gas, so
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the light wasn't coming from a thick cluster of stars,
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but from just one single giant object. Super Massive black
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holes are found at the cet as of most, if
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not all galaxies. In some cases, those black holes are
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millions to beans, at times more massive than our Sun,
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pulling in nearby matter with such strength that it converts
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to energy it shines. No one's ever really known why
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or where these gigantic black holes are the centers of
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galaxies come from, and these black hole stars maybe will
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be the first face of formation for these super massive
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black holes. Webs already found evidence of high mass black
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holes in the early universe, and these new black hole
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star objects, which are essentially turbo charged mass builders, could
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help explain the early evolution of the universe and may
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therefore be a welcome addition to current models this space time.
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Still to come discovery of multiple episodes of habitability on
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the red planet Mars, and the European Space agencies newest
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Australian deep space antenna about to begin operations. All that
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and more still to come on space time NASAs Mars
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perseverance rovers discovered strong evidence the red planet's Jezro crater
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experienced modible episodes of liquid water flooding, each with conditions
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that could have supported life as we know it. By
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analyzing high resolution geochemical data from the six wild casseised
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mobile laboratory, scientists have identified two dozen types of minerals
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that help reveal a dynamic histuy of volcanic rocks which
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were altered during interactions with liquid water on the red planet.
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The new findings, reported in the Journal of Geophysical Research Planets,
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provides important clues about the ongoing search for ancient life
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on Mars. The studies lead author Elinor Moreland from Rice
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University says the minerals in Jezro support modible, temporarily distinct
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episodes of fluid alteration. She says it indicates there were
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several times in history when these volcanic rocks interacted with
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liquid water, and therefore more than one time when this
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location hosted environments which would have potentially been suitable for life.
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Minerals form in the very specific environmental conditions of temperature,
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pH and chemical makeup of fluids, and that makes them
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reliable storytellers of a planet's geologic history. In Jezro, the
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twenty four mineral species they're found reveal the volcanic nature
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of the Martian surface and its interactions with water over time.
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The water chemically weathers the rocks and creates salts or
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clay minerals, and the specific minerals that form depend on
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the environmental conditions. The identified minerals in Jezro reveal three
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types of fluid interactions, each with different applications for habitability.
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The first squid of minerals, including greenolite, is ingerlite, and
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ferro aluminous cellar dunite, indicate localized high temperature acidic fluids
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that are only found on rocks on the crater floor.
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When these are interpreted as being some of the oldest
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rocks included in the study, the water involved in these
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episodes is considered the least habitable for life since research
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on Earth that's shown that high temperatures and low pH
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can damage biological structures. Now all these would be most
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challenging for life on Earth. Life can still persist even
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under these hot ascidic conditions. We're talking about the geothermal
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geyser pills of water at Yellowstone, so it doesn't rule
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out habitability. The second squad of minerals reflects moderate neutral
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fluids that support more favorable conditions for life, and which
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were present over a larger area. Minerals like minnesotaatee and
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Klinopdylo light formed at lower temperatures and neutral pH with
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minnesotype detected on both the crater floor and in the
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upper fan region of Gezo, while clinopdilo light was also
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detected on the crater floor. Finally, the third category represents
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low temperature alkaline fluids and is considered quite habitable from
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an Earth type perspective. Sepio light, a common auto mineral
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on Earth, formed under moderate temperatures and alkaline conditions and
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was widely found distributed right across Jezo. The presence of
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sepiolite in all these areas reveals a widespread episode of
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liquid water creating habitable conditions in Jezro crater and in
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filling sediments. Moreland says these minerals are telling scientists that
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Jezro experienced a shift from harsher hot acidic fluids to
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more neutral and alkaline ones over time, conditions increasingly supportive
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of life. Because Mars samples can't be prepared or scanned
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as precisely as Earth samples, the authors developed an uncertainly
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propagation model to strengthen their results. Using a statistical approach,
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Moreland colleagues repeatedly tested mirror identifications, considering the potential errors,
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similar to how meteorologists forecast hurricane tracks by running many models,
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and the results confirm that Jezro, once home of an
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ancient lake, experienced a complex and dynamic aqueous history. The
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new mineral discoveries not only brings scientists closer to answering
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whether Mars ever could have supported life, but it also
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sharpens perseverance of strategy for WIT samples to collect for
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a possible future return to Worth mission this space time
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still to come. The European Space Agency about the commission
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its newest Australian deep space dish, and later in the
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science report, researchers finally confirm that people really do see
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colors the same way. All that and more still to
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come on space time. The European Space Agency is about
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to inaugurate its fourth Australian deep space antenna at its
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new Nausea tracking station in Western Australia. The new thirty
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five meter parabolic dish will reinforce eas's deep space communications capabilities,
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supporting upcoming deep space missions and meeting a growing demand
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for the deep space network. The new Nouseier complex offers
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a strategic geographical position, complimenting aces deep space antennas in Sweden, Belgium, Spain, Portugal, French,
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Guiana and Argentina. They're all linked to ASA's European Space
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Operations Center in Damstadt, Germany. This report from ACTV LISA.
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The European Space Agency operates several missions in deep space
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and ensures that they meet their science objectives. Teams of
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specialized engineers design and deploy the technology needed to communicate
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with spacecraft that are exploring our Solar system.
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When designing space communications system we are confronted with strong
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constraints on board in terms of mass and power. Therefore,
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we try to move the complexity into the ground station
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where we can build much larger ground stations with much
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more performance.
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ISSA has deep space stations around the world organized in
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a network called s Track.
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We obviously need to receive data from the spacecraft. This
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is in particular scientific data coming from the instruments. It
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is navigation measurements and it is status information from the
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space cruft. On top of this, we need to command
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the spacecraft in order to navigate it and to operate it.
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When receiving data from deep space, we want to collect
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as much signal energy as possible, he says. Antennas are
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thirty five meters wide, with the same surface as an
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Olympic swimming pool. The dish alone weighs one hundred and
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thirty tons and we can point it with the accuracy
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of six milli degrees to any position in the sky.
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The mechanical design makes it possible to compensate for the
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rotation motion of the Earth or The received energy is
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captured by the large dish. It's focused on the so
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called sub reflector and the signal is then guided to
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the base of the antenna, where special dichroic mirrors separate
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the incoming frequency.
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Bands amplifies undertate the critical task of amplifying this week
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signal coming from the space using the high texts and
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conductor technology developed by European industry to woost this signal
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around one million times or sixty dep The use of
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Indian phosphi technology and pulling down to menus two hundred
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and sixty degrees celsius allows to genervate only five degree
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scalving of thermal noise that is only twice the cosmic
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background noise, the lowest nose you can find in the universe.
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The demodulated and decoded signal eventually goes through the Spacelink
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protocol processing, which outputs the data in a format we
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can easily handle. This is the telemetry data that includes
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the low rate data from the spacecraft platform and the
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high rate data from the scientific instruments. Communication also needs
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to be in the opposite direction. We need to transmit
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the so called telecommands to the spacecraft in order to
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activate thrusters or control our scientific payloads.
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Typically, we need to transmit around twenty kilo wards of
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radio frequency power. This is using clystone, is a high
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density energy debase that transforms around one hundred kilowatts of
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electrical power into twenty kilowatts of radio frequency power, amplifying