WEBVTT

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

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Anna, your host and I'm thrilled to have you

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join us for another journey through the

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latest and most captivating stories from the

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cosmos. Today we're delving

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into some truly fascinating developments that

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span from the challenges faced by astronauts

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in space to humanity's ambitious future on

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the Moon and beyond. We'll start by

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exploring an unexpected side effect of space

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travel. How it can permanently change an

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astronaut's eyesight. Then we're heading to

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the Moon to look at South Korea's bold plans

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for a lunar base by 2045,

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showcasing the growing global race to return

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to our celestial neighbour. Next up,

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we'll dive into the incredible potential of

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NASA's upcoming Nancy Grace Roman Telescope,

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which is poised to uncover tens of thousands

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of cosmic explosions and shed light on

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mysteries like dark energy. Finally,

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we'll take a trip back in time to the Apollo

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11 mission, revealing the little known

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stories of where the Eagle could have landed

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if circumstances had been different. Stick

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around. It's going to be an exciting episode.

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You've spent months aboard the International

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Space Station, witnessing Earth from an

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unparalleled vantage point, performing

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groundbreaking science and pushing the

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boundaries of human exploration. You return

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home a hero, but with an unexpected side

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effect. Your eyesight has changed. This

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isn't a rare occurrence. It affects about 70%

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of astronauts on long duration missions. And

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it's got NASA scientists intensely focused on

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understanding why weightlessness impacts our

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vision so profoundly. One astronaut, Dr.

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Sarah Johnson, reported that text perfectly

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clear before her six month ISS stay

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became blurry. She's far from alone.

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Astronauts frequently report difficulty

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reading blurred distance vision and other

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visual changes that can persist for years

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after returning to Earth. This condition has

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been given a spaceflight associated

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neuro ocular syndrome, or

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sans. It has rapidly become one of the most

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pressing health concerns for extended space

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missions. Unlike other temporary issues like

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motion sickness or or muscle weakness, which

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quickly resolve, on Earth, sans related

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vision changes can unfortunately be

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permanent. The primary culprit appears to be

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microgravity itself. Here on Earth, gravity

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consistently pulls fluids downwards through

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our bodies. In the microgravity environment

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of space, these fluids redistribute. This

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leads to facial puffiness and more

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critically, increased pressure inside the

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skull. This elevated intracranial pressure

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can flatten the back of the eyeball and cause

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swelling of the optic nerve, directly

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impacting vision. These findings carry

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significant implications for future missions

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to Mars, which could realistically last two

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to three years. As Dr. Michael Roberts,

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NASA's Vision Research Lead, put it, we need

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to understand whether these changes stabilise

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or continue worsening over time. An astronaut

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with severely compromised vision could

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jeopardise an entire Mars mission. To

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combat SANS, Dr. Roberts and his team at

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NASA are actively developing various

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countermeasures. These include specialised

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contact lenses, medications designed to

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reduce fluid pressure, and specific exercise

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protocols that might help maintain normal

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circulation. They are also testing an

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innovative device called the Visual

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Impairment Intracranial pressure, or

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viip chamber, which could simulate

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Earth like pressure conditions for the eyes

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while in space. While SANS presents a

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serious challenge for space exploration, this

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research offers a broader benefit for

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everyone on Earth. Scientists are gaining

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invaluable new insights into how pressure

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affects vision, which could potentially lead

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to improved treatments for conditions like

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glaucoma and intracranial hypertension. Here

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on our home planet, understanding how our

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bodies adapt to and are affected by space

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remains crucial as we continue to test the

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limits of human endurance and explore further

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into the cosmos. The research into

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solutions will continue at NASA and onboard

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the iss, with the hope that when humanity

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finally embarks on a trip to Mars, our vision

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will be clear enough to fully appreciate what

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we have accomplished.

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Shifting our gaze from astronaut health to

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ambitious national goals let's talk about

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South Korea's burgeoning space ambitions the

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nation is making headlines with its bold plan

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to establish a moon base by 2045.

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This significant goal was revealed in a long

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term exploration roadmap laid out by the

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Korea aerospace administration, or

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CASA, which was established just last year.

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CASA's roadmap outlines five core missions

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encompassing everything from low Earth orbit

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and microgravity exploration to lunar

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exploration and even solar and space science

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missions. A key focus for CASA is

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developing homegrown lunar landing and roving

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technology alongside the crucial ability to

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extract and utilise moon resources like water

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ice. Some of this preparatory work is

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already well underway. For instance, the

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Korea Institute of Geoscience and Mineral

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Resources has been testing prototype lunar

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rovers in an abandoned coal mine, practising

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techniques that could be vital for future

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space mining operations. South Korea isn't

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new to lunar endeavours. In August

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2022, the nation successfully launched its

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first moon probe, known as the Korea

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Pathfinder lunar orbiter, or Dnuri, atop a

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SpaceX Falcon 9 rocket. Dannuri reached

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lunar orbit four months later and is still

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actively studying the moon with its array of

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instruments, proving South Korea's growing

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capabilities in space. While South Korea

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had already aimed to place a robotic lander

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on the moon by 2032, this newly

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revealed roadmap significantly ups the

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ante. The plan now includes developing a

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more capable moon lander by 2040,

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all with the ultimate goal of building a

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robust lunar economic base by

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2045. It's important to note that

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South Korea isn't alone in this race to the

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moon. The United States, through NASA's

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Artemis programme, also plans to build lunar

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outposts in the coming decade. China is

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pursuing similar goals, often in partnership

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with Russia and other nations. And India has

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set its sights on a moon base by 2047.

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The moon isn't Khasa's only distant

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destination either. The agency also has its

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sights set on South Korea's first ever Mars

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landing, also by 2045.

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Now let's shift our focus to a truly exciting

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development on the horizon. NASA's next

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big space telescope project, the Nancy Grace

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Roman Telescope. Astronomers are absolutely

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buzzing with anticipation for its launch,

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currently set for no later than May

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2027. And for good reason.

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Recent research suggests that Roman, during

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its High Latitude Time Domain Survey

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observation programme, could discover an, uh,

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astounding 100,000 powerful cosmic

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explosions. We're talking about a dazzling

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array of violent events, including

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supernovas, marking the dramatic deaths of

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massive stars, which occur

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when two of the universe's most extreme dead

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stars or neutron stars, Viking violently

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collide and even burps from actively feeding

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supermassive black holes. Roman might even

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detect the explosive destruction of the very

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first generation of stars in our universe.

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These cosmic fireworks are more than just

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spectacular sights. They're crucial clues

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that could help scientists finally crack the

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mystery of dark energy. That's the

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placeholder name for the strange unseen force

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that's causing the expansion of the universe

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to accelerate. According to Benjamin Rose,

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an assistant professor at Baylor University

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and the research leader, this survey will be

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a goldmine. Whether you're exploring dark

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energy, dying stars, galactic

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powerhouses, or even entirely new phenomena

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we've never encountered before, Roman will

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achieve these explosive results by

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systematically scanning the same vast region

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of space every five days for a period of two

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years. These observations will then be

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meticulously stitched together to create

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incredible cosmic movies, revealing a wealth

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of these dynamic events. Many of the

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explosions Roman detects will be type 1A

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supernovas. These particular cosmic

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blasts happen when a dead star known as a

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white dwarf greedily syphons material from a

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companion star until it becomes unstable and

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erupts. Type 1a supernovas

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are incredibly valuable to astronomers

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because their light output is and peak

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brightness are so consistent from one event

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to the next. This makes them what astronomers

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affectionately call standard candles,

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allowing them to accurately measure cosmic

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distances. The new research, which

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simulated Roman's entire High Latitude Time

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Domain Survey indicates the telescope could

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uncover up to 27,000 new Type 1A

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supernovas. That's about 10 times the

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combined total from all previous surveys. By

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observing these standard candles across

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immense and varying distances,

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astronomers are essentially looking back in

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time, enabling them to pinpoint how fast the

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universe was expanding at different points in

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cosmic history. This unprecedented

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wealth of type 1A supernovas should offer

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significant hints about the secrets of dark

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energy. It could even help confirm recent

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findings from the Dark Energy Spectroscopic

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Instrument, or dece, which suggests that this

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mysterious force might actually be weakening

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over time. As Rose explained, filling

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these data gaps could also fill in gaps in

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our understanding of dark energy. Evidence is

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mounting that dark energy has changed over

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time, and Roman will help us understand that

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change by exploring cosmic history in ways

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other telescopes can't. Beyond dark

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energy, Roman will also shed light on the

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life cycles of stars. The team estimates that

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as many as 60,000 of the 100,000

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cosmic explosions detected could be core

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collapse supernovas. These occur when massive

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stars at least eight times heavier than our

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sun exhaust their nuclear fuel and can

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no longer support themselves against

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gravitational collapse. As their cores

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rapidly implode, their outer layers are

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violently blasted away. This process

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disperses elements forged within these stars

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throughout the cosmos, providing the building

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blocks for the next generations of stars,

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their planets, and perhaps even life itself.

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While not directly linked to dark energy,

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these events are crucial for understanding

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stellar evolution and the chemical enrichment

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of the universe. Rebecca Hounsell, a

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member of the research team from NASA's

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Goddard Space Flight Centre, highlighted how

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Roman's data will allow scientists to

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distinguish between different types of cosmic

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flashes. She noted that while searching for

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type 1A supernovas, Roman will collect a

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lot of cosmic bycatch, other phenomena that

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may not be useful for some scientists, but

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will be invaluable to others. Among these

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rarer cosmic gems, Roman could detect tidal

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disruption events, or TDEs, where black

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holes ruthlessly devour stars that wander too

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close. As the star is torn apart by immense

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tidal forces, much of its material is spewed

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out at near light speed, creating powerful

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emissions that Roman will hunt for. The team

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predicts around 40 such star destroying

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events could be found. Even more elusive are

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kilonovas, those explosive bursts of light

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that happen when two neutron stars smash

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together and merge. The team estimates Roman

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could uncover around five new kilonovas.

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While that number seems small, it's a huge

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deal, as only one kilonova has been

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definitively confirmed to date. These

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observations are vital for understanding the

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origins of precious metals like gold and

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silver. While most elements are forged in the

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hearts of stars, the extreme conditions of

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neutron star collisions are thought to be the

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only cosmic furnaces powerful enough to

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create elements heavier than iron, like gold

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and plutonium. Studying the light from these

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kilonovas helps us understand this

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fundamental process. Kilonova studies could

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also reveal what types of celestial bodies

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are formed when neutron stars merge. Perhaps

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an even larger neutron star, an immediate

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black hole, or something entirely new.

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Perhaps the most thrilling, uh, potential

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discovery Roman could make is the observation

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of the strange explosive deaths of the

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universe's very first stars. Current

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theories suggest these early massive stars

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may have died differently than modern stars

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undergoing what's called a pair instability

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supernova. In these colossal

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blasts, gamma rays within the star could have

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generated matter antimatter pairs, leading

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to a self detonation so powerful it theorised

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to leave nothing behind but the elemental

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fingerprint of its lifetime. While

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astronomers have dozens of candidates for

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these events, none have been confirmed.

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The simulation suggests Roman could turn up

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as many as 10 confirmed pair instability

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supernovas. As Rose put it, they're

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incredibly far away and very rare. So you

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need a telescope that can survey a lot of the

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sky at a deep exposure level and in near

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infrared light, and that's Roman.

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The team plans further simulations to explore

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Roman's full capabilities, which might even

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include detecting phenomena not yet

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theorised. As Rebecca Hounsel aptly

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summarised, Roman's going to find a whole

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bunch of weird and wonderful things out in

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space, including some we haven't even thought

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of yet. We're definitely expecting the

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unexpected. This groundbreaking research,

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by the way, was published on July 15 in the

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Astrophysical Journal.

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From the cutting edge of cosmic discovery,

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let's take a quick look back at, ah, one of

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the most iconic moments in space. The

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Apollo 11 moon landing on July

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20, 1969. Neil Armstrong's famous

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words Houston Tranquilly Base here,

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the Eagle has landed, marked humanity's first

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steps on another world. But what if those

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words had been uttered from a different

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location on the lunar surface? It's a

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fascinating thought, isn't it? The truth is

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that historic phrase could very easily have

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come from a completely different part of the

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moon. In February 1968,

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NASA's Apollo Site Selection board had

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narrowed down a list of 30 potential landing

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sites for Apollo 11 to just five. Among these

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were two sites on the opposite side of the

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lunar disc from Tranquilly Base, specifically

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in Oceanus Procellarum, also known as the

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Ocean of Storms. Each of these prospective

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landing zones, which were roughly 3 by 5

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miles in size, underwent intensive orbital

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imaging and a rigorous selection process. The

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criteria were incredibly strict. Each site

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needed to be within 5 degrees of the lunar

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equator to minimise fuel consumption. There

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could be no large hills or deep craters along

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the lander's approach path, as these could

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confuse its landing radar. Furthermore, each

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site had to have a slope of less than 2

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degrees, with relatively few craters and

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excellent lighting conditions during the

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chosen landing windows. Ultimately,

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Site two in the Sea of Tranquilly was

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selected as the prime landing location.

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However, two of the other shortlisted zones

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were designated as contingency landing sites,

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ready to be targeted if the launch of Apollo

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11's mighty Saturn V rocket had been delayed.

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Imagine if the mission's launch had slipped

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by just two days from July 16

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to July 18, 1969.

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In that scenario, humanity's first steps on

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the moon would have taken place in the Sinus

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Medii region, right in the centre of the

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Earth facing lunar surface. And if the launch

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had been pushed back even further to July

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21, 1969,

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then the footprints would have been left in

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the regolith of Oceanus Procellarum.

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While Tranquilly Base has certainly become a

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legendary name, Procellarum Base just doesn't

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quite have the same ring to it, does it? It's

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a compelling reminder of the meticulous

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planning and the precise conditions that led

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to one of history's most defining moments.

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And that brings us to the end of another

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fascinating journey through the cosmos on

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Astronomy Daily. I hope you've enjoyed

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exploring these stories as much as I have

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enjoyed sharing them with you. Thank you for

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tuning in and being a part of our cosmic

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conversation. This has been Anna, your host,

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and I invite you to keep exploring the

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wonders of the universe with us. You can

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00:16:14.830 --> 00:16:16.910
become a completionist and listen to all our

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00:16:16.910 --> 00:16:19.470
back episodes and even get a shout out on the

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show by visiting our website at

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astronomydaily IO. That's

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astronomydaily IO. And don't forget

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get your podcasts so you never miss an

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update. Until tomorrow when I'll be back to

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do it all again. Keep looking up.
