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Anna: Hello and welcome to Astronomy Daily. I'm

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your host, Anna, bringing you the latest and

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most fascinating developments from across the

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cosmos. Today we've got a great lineup of

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stories that showcase both human ingenuity

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and the wonders of our universe. We'll

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dive into SpaceX's ninth Starship test

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flight, a mission with impressive successes,

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but also some dramatic setbacks along the

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way. Then we'll explore a significant new

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discovery in our own solar system. A a dwarf

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planet that's been hiding in plain sight for

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years and represents the largest such find in

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over a decade. We'll also journey to

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Europa and examine its potential future

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habitability, peek at a bizarre star within a

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star system and investigate new research

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suggesting habitable moons might be more

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common than we thought. So get comfortable

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and join me for a journey through the latest

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astronomical discoveries that continue to

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expand our understanding of the universe we

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call home.

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First up today, SpaceX's Starship

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Super Rocket completed its ninth flight test

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recently and it was quite the rollercoaster

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of achievements and challenges. The launch

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began impressively at SpaceX's starbase in

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Texas, with the massive 400 foot tall

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rocket lifting off as planned. The first

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stage booster, known as Super Heavy,

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performed Beautifully with all 33 methane

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fueled engines firing perfectly, generating

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an astonishing 16.7 million pounds

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of thrust, more than twice the power of the

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Saturn 5 rockets from the Apollo era.

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What made this launch particularly notable

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was that this marked the first time SpaceX

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reused a Super heavy booster, as this

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same first stage had previously flown during

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January's seventh test flight. The successful

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reuse represents a significant milestone in

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SpaceX's quest for rapid reusability of its

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rocket components. However, the mission

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encountered several significant challenges.

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Once the second stage, known as ship,

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separated from the booster, the planned

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deployment of eight Starlink satellite

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simulators had to be scrubbed when SHIP

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couldn't open its payload doors. This would

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have been Starship's first ever payload

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deployment, making the failure particularly

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disappointing. Things went from bad to worse

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as SHIP continued its journey. As it headed

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toward a scheduled splashdown in the Indian

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Ocean, it began spinning uncontrollably.

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SpaceX commentators reported that the second

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stage had lost attitude control, apparently

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due to propellant leaks. The spacecraft

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ultimately broke up during its uncontrolled

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descent over a cleared area of ocean. Despite

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these setbacks, the test flight wasn't

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without its successes. The super heavy

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booster executed several challenging

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manoeuvres after stage separation, including

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a directional flip over and maintaining a

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heightened angle of attack. Both techniques

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aimed at improving fuel efficiency for future

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missions. The booster also demonstrated its

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ability to maintain controlled descent even

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when simulating a single engine failure.

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SpaceX CEO Elon Musk remained

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characteristically optimistic, noting on

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social media that Starship made it to the

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scheduled engine cutoff point, which

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represented a significant improvement over

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previous flights. He also highlighted that

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there was no significant loss of heat shield

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tiles during ascent, another important

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achievement. Looking ahead, Musk

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indicated that SpaceX plans to accelerate its

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launch cadence for the next three Starship

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flights, aiming for approximately one launch

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every three to four weeks. This aggressive

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schedule reflects SpaceX's determination to

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rapidly iterate and improve the Starship

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system. This persistence is crucial

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given Starship's central role in NASA's

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Artemis programme, where a version of the

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spacecraft is slated to serve as the landing

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system for the Artemis 3 mission, which would

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mark humanity's return to the lunar surface.

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Beyond moon missions, SpaceX has even

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more ambitious plans, with Musk suggesting

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that starship flights to Mars could begin as

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early as 2024. While that timeline

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seems extraordinarily ambitious, the

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company's approach of testing, failing,

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learning, and rapidly improving continues to

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push the boundaries of what's possible in

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space exploration.

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Now let's turn our attention to discovery. In

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exciting news for planetary scientists, a

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newly discovered object in the outer solar

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system has been confirmed as a dwarf planet,

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the largest such discovery in more than a

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decade. Currently bearing the

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preliminary designation 2017 of

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201, this celestial body measures

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approximately 700 kilometres, about 400

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miles across, and follows an extremely

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elliptical orbit around our sun.

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What makes this orbit particularly remarkable

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is its lengthy duration, taking an

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estimated 25,000 years to complete a single

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circuit around the sun. This places

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2017 of 201 in the

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exclusive category of dwarf planets,

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alongside more familiar objects like Pluto,

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the asteroid Ceres, and a handful of other

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similar bodies in the outer solar system.

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The discovery story is almost as fascinating

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as the object itself is. The dwarf planet was

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hiding in plain sight, buried within

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terabytes of publicly available astronomical

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data, some of which was collected more than a

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decade ago. Finding this celestial needle in

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a haystack required months of computational

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work to distinguish it from the countless

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background stars and noise. The

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detection came through painstaking analysis

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of data originally collected for the Dark

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Energy Survey, or ds. While

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that project primarily focuses on studying

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gravitational lensing in distant galaxies,

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the survey's ability to detect extremely

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faint objects made it inadvertently perfect

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for hunting distant solar system objects.

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Sihao Cheng from the Institute for Advanced

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Study led the discovery team, noting that

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while in principle anyone could have made

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this discovery using the public data, the

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process was extraordinarily demanding.

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Developing the algorithm alone took several

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months, followed by additional months of

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computation. And as they scanned through

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roughly 200 terabytes of data using hundreds

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of processors, what made the search

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particularly challenging was the widely

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separated observation dates. Unlike

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targeted asteroid searches that typically

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take successive exposures separated by hours

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or days, these images were often separated

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by months or even years, containing numerous

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points of light from unrelated objects that

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needed to be filtered out. After identifying

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the object in DES data, the team confirmed

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its existence by locating it in another

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public data set from the Canada France

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Hawaii Telescope. In total, they

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found 19 observations of the object spanning

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from 2011 to 2017, all

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showing it exactly where their orbital

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calculations predicted. The extreme

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elongation of 2017 of

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201's orbit means it's only visible over a

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tiny fraction of its journey around the sun,

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too faint to detect for more than 99% of its

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orbit. This suggests there could be many

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more similar objects lurking undetected at

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the edges of our solar system. M

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Interestingly, this discovery has

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implications for the hypothesised Planet X

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or Planet nine. Some astronomers have

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suggested this unknown planet's gravitational

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influence explains the clustered orbits of

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certain trans neptunian objects. However,

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2017 of 201's

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orbit doesn't fit this pattern, potentially

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challenging the Planet X hypothesis, though

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debate continues among experts about what

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this new discovery actually tells us about

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our outer solar system.

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Next on the story list today. While Europa is

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currently an icy world with a subsurface

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ocean, its distant future might hold

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something remarkable. In about 12 billion

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years, when our sun exhausts its hydrogen

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fuel and enters the red giant phase of its

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evolution, the habitable zone of our solar

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system will dramatically shift outward from

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its current position. This cosmic

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relocation of real estate suitable for liquid

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water will eventually encompass Jupiter and

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its moons, potentially transforming Europa in

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fascinating ways. Researchers estimate that

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as the expanding sun grows more luminous,

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Europa could develop and maintain a tenuous

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water vapour atmosphere for several hundred

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thousand years. The process begins with the

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Sun's inevitable evolution. After spending

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billions of years as a stable main sequence

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star, our sun will eventually deplete its

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core hydrogen fuel. This triggers the fusion

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of heavier elements like helium, causing the

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Sun's outer envelope to expand dramatically.

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During this red giant phase, the sun will

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grow hundreds of times larger than its

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current size, engulfing Mercury and Venus

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entirely while rendering Earth unless

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uninhabitable. However, for the

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outer planets, this stellar evolution creates

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new possibilities. Computer models suggest

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that Jupiter's system will enter the red

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giant branch habitable zone in about 12

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billion years when it's approximately 2

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astronomical units from the expanding sun,

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less than half its current distance, Jupiter

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itself will likely develop bright water

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clouds in its upper atmosphere as it

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experiences the increased solar radiation.

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More intriguingly, Europa's surface ices will

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begin to sublimate under the influence of

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both the brighter Jupiter and the expanded

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Sun. Much like dry ice sizzling away

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in sunlight, Europa's frozen surface will

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transform directly from solid to vapour.

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While most of this sublimated ice will escape

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to space, simulations suggest some

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water vapour will remain bound to Europa for

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approximately 200,000 years before being

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completely lost. During this brief

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cosmic window, Europa might actually be

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considered habitable. Though whether this

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timespan is sufficient for life to emerge and

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thrive remains an open question.

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This scenario offers valuable insights for

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astronomers studying exoplanetary systems

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around sun like stars. As we identify more

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exoplanets and potentially exomoons,

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understanding how these worlds evolve

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alongside their ageing stars becomes

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increasingly important. The fate of Europa

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serves as a model for what might happen to

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similar icy worlds in distant star systems.

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Now for something pretty rare. In a

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remarkable discovery, Chinese astronomers

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have identified an extremely rare type of

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binary star system that gives us a glimpse

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into a fleeting phase of stellar evolution.

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Using the 500 metre aperture spherical radio

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Telescope, also known as the China Sky Eye,

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researchers led by Han Jin Lin from the

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National Astronomical Observatories of China

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detected a unique pulsar designated

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PSRJ 1928 1815.

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Located about 455 light years away,

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this system features something astronomers

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have long theorised but rarely observed a

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pulsar whose radiation pulses are

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occasionally blocked by its companion star

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every few hours. What makes this

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discovery particularly special is that the

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two stars are actually orbiting inside a

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common envelope of hydrogen gas. Pulsars

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themselves aren't uncommon. Scientists have

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identified nearly 3,500 in our galaxy

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alone. These dense stellar remnants form

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after massive stars explode as supernovae.

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As they rotate, they emit beams of

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electromagnetic radiation from their magnetic

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poles that sweep across space like lighthouse

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beams. When one of these beams crosses Earth,

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we detect it as a regular pulse of radio

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waves. But the PSR

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J1928 1815 system

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captures a critical moment in binary star

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evolution. In these systems, the heavier star

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ages faster and eventually collapses into a

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neutron star, or pulsar. Meanwhile, the

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smaller companion star loses material to its

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dense partner, causing them to share a common

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envelope of hydrogen gas for a relatively

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short period. Astronomically speaking, the

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two stars orbit within this shared envelope.

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Over approximately 1,000 years, the neutron

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star gradually clears away this envelope,

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eventually leaving behind a hot helium

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burning star orbiting the neutron star. This

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observation provides compelling evidence

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supporting long standing theories about how

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stars in binary systems exchange mass,

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shrink their orbits and eject shared gas

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envelopes. Understanding these processes

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helps astronomers piece together the complex

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puzzle of stellar evolution, neutron star

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behaviour, and how such pairs eventually

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merge to produce gravitational waves. The

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discovery is particularly significant because

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binary systems are extremely common in our

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galaxy. More than half of all stars

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exist as part of binary or multiple star

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systems, their gravitational dance shaping

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their evolution in dramatic ways. In some

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cases, one star's gravity can drag material

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from its companion, leading to explosive

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events like novae or even supernovae.

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With increasingly powerful telescopes like

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fast, astronomers hope to find more of these

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rare cosmic pairs, further illuminating the

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processes that shape stars throughout their

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lifetimes and after their deaths.

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Finally today, while we've focused much

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of our search for extraterrestrial life on

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Earth like exoplanets, a fascinating new

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study suggests we should broaden our horizons

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to include moons orbiting giant planets.

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Researchers from Hungary and the Netherlands

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have published compelling findings about the

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potential habitability of exomoons in the

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journal Astronomy and Astrophysics.

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Their study, titled Grand Theft

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Formation of Habitable Moons Around Giant

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Planets, used complex simulations to

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investigate how moons form around giant

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exoplanets and whether these moons could

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support life. The team, led by

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Zoltan Denks from the Hun Ren Research Centre

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for Astronomy and Earth Sciences, focused

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specifically on the formation of large moons

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in circumplanetary discs, the rotating

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collections of material that remain after a

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planet forms. The researchers

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examined 461 known giant

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exoplanets, modelling how lunar embryos might

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grow through collisions within these discs.

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Their simulations revealed that moons with

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masses between Mars and Earth could form

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around planets roughly 10 times the size of

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Jupiter, with many potentially habitable.

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Perhaps most interestingly, the study found

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that the optimal distance for habitable

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exomoons is between 1 and 2

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astronomical units from their stars.

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Beyond this range, tidal heating rather than

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stellar radiation becomes the primary heat

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source for these moons. This is similar to

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what we see in our own solar system, where

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moons like Europa and Enceladus likely

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harbour subsurface oceans warmed by tidal

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flexing rather than direct sunlight. The

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simulations also showed that as distance from

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the star increases, more moons tend to form,

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but their masses become too small to maintain

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habitability. Meanwhile, closer to the star,

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fewer but more massive moons form, with more

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being lost to stellar theft, where the star's

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gravity pulls them away from their host

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planet. While astronomers haven't

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definitively confirmed the existence of any

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exomoons yet several candidates have been

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identified. The James Webb Space Telescope is

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currently examining potential exomoon

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candidates. And the European Space Agency's

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upcoming PLATO mission may also be capable

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of detecting these distant moons.

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This research effectively expands our

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definition of the habitable zone to include

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moons orbiting giant planets. As one

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researcher put it, the circumstellar

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habitable zone can be extended to moons

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around giant planets, potentially multiplying

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the number of worlds where we might someday

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find evidence of life.

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Well, that's all for today's episode of

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Astronomy Daily. What an incredible journey

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through space we've taken from watching

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SpaceX push the boundaries of rocket

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technology despite setbacks to discovering

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a massive new dwarf planet that was

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hiding in plain sight within existing data.

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We've peered into the distant future where

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Europa might briefly become habitable as our

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sun expands, and witnessed the bizarre

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spectacle of a pulsar orbiting inside another

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star. Perhaps most tantalising is the

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possibility that habitable moons may be far

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more common than we once thought, potentially

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expanding our search for life beyond

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traditional Earth like planets. Each

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of these stories reminds us that the universe

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remains full of surprises, constantly

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challenging our assumptions about what's

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possible as our tools and techniques for

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observation continue to improve. From

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powerful radio telescopes like FAST to the

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upcoming PLATO mission, we stand on the

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threshold of even more remarkable

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discoveries. The cosmos is vast and

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ancient, yet we're learning new things about

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it every day. Thank you for joining me on

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Astronomy Daily. I'm Anna, and I'll see

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you again tomorrow as we continue to explore

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the wonders of our universe together. In the

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meantime, keep looking up in wonder.
