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Anna: Welcome to Astronomy Daily. Your cosmic

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connection to the stars and beyond. I'm

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Anna bringing you the latest developments in

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space exploration and astronomical

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discoveries right to your ears. Today's

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episode is packed with fascinating stories

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that showcase both the mysteries of our

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universe and humanity's incredible

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technological ingenuity in uncovering them.

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We'll be exploring several breaking stories

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that highlight just how dynamic our solar

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system truly is. We'll start by delving into

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a new gravity study that finally helps

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explain why the two sides of our moon look so

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dramatically different. A question that has

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puzzled scientists for decades. The research

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reveals fascinating asymmetries deep within

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the lunar interior that have shaped its

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distinctive appearance. Then

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we'll head down under to Australia, where an

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aerospace firm was preparing for a historic

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rocket launch that would have been the first

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Australian made rocket to reach orbit from

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Australian soil. We'll look at what happened

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with this milestone attempt and what it means

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for the growing global space industry.

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Next, we'll travel to the very edge of our

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solar system, where NASA engineers have

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achieved what many would consider impossible.

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Reviving thrusters on the Voyager 1

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spacecraft that had been deemed unusable

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since 2004. This remarkable feat

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of remote engineering shows just how

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resourceful our space teams can be,

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especially when working with a spacecraft

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that's now over 15 billion miles from Earth.

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We'll also examine fascinating new findings

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about Venus that suggest our nearest

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planetary neighbor may be more geologically

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active than previously thought. Data from

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NASA's Magellan mission has revealed evidence

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of ongoing tectonic processes that reshape

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our understanding of this enigmatic world.

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Finally, we'll look at a historic first on

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Mars, where the Perseverance rover has

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captured an image that no human has ever seen

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before. A visible aurora on the

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red planet. This subtle green glow

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gives us a preview of what future Martian

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explorers might witness in the night sky.

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These stories remind us that our solar system

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is not a static place, but an ever changing

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dynamic environment full of ongoing processes

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and unexpected discoveries. They also

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highlight the incredible technological

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achievements that allow us to explore these

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distant worlds from right here on Earth.

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So settle in as we journey across the cosmos,

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exploring the latest findings that continue

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to expand our understanding of the universe

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we call home. Let's get things underway.

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One of the most enduring mysteries about our

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closest celestial neighbor has been why the

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moon's near side. The face we see from Earth

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looks so dramatically different from its far

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side. Now, an exhaustive

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examination of lunar gravity. You using data

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from NASA's GRAIL mission is offering

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compelling new evidence to explain this lunar

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dichotomy the research team discovered that

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the Moon's near side flexes slightly more

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than the far side during its elliptical orbit

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around Earth. This difference in tidal

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deformation caused by Earth's gravitational

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pull indicates significant structural

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differences between the two sides of the

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lunar interior, particularly in the mantle

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layer. M. Our study shows that the Moon's

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interior is not uniform except, explains Ryan

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park, lead author of the study published in

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the journal Nature. The side facing Earth,

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the near side, is warmer and more

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geologically active deep down than the far

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side. This temperature difference is

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substantial. Researchers estimate that the

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near side Mantle averages between 180

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to 360 degrees Fahrenheit,

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hotter than the far side mantle. This thermal

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difference is likely sustained by the

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radioactive decay of elements like the

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thorium and titanium, which appear to have

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accumulated on the near side over billions of

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years. The findings help explain the stark

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visual contrast between the two lunar

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hemispheres. If you've ever looked up at the

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Moon, you've noticed that the near side is

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dominated by vast dark plains called mare,

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formed when molten rock cooled and solidified

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billions of years ago. In contrast, the

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far side has a much more rugged, mountainous

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terrain, with very few of these plains.

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Scientists have long hypothesized that

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intense volcanism on the near side caused

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radioactive heat generating elements to

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accumulate in the mantle beneath this

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hemisphere, driving these surface

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differences. The new GRAIL data provides

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the strongest evidence yet supporting this

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theory. The researchers devoted years to

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analyzing data from the twin GRAIL spacecraft

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Ebb and Flow, which orbited the Moon from

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December 2011 to to December

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2012. Their work has resulted in

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what park describes as the most detailed and

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accurate gravitational map of the Moon to

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date. Beyond solving this lunar mystery,

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the enhanced gravity map has practical

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applications. It will be crucial for

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developing lunar positioning, navigation, and

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timing systems, essential tools for future

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lunar exploration missions. By improving

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our understanding of the Moon's gravity

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field, the research contributes to

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establishing a precise lunar reference frame

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that will enable safer and more reliable

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navigation for spacecraft and surface

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operations. This asymmetry in the

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Moon's interior structure also deepens our

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appreciation of our celestial companions

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importance to Earth. The Moon stabilizes our

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planet's rotation and generates ocean tides

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that influence countless natural systems and

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daily rhythms on our world. What's

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particularly exciting is that the

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gravitational analysis techniques used in

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this study could potentially be applied to

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other bodies in our solar system, such as

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Saturn's moon Enceladus and Jupiter's moon

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Ganymede, both considered prime candidates in

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the search for potential life beyond Earth.

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Next in today's story lineup An Australian

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aerospace firm has been forced to delay what

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would have been a historic rocket launch from

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Australian soil. Gilmour Space

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Technologies had planned to conduct the first

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test launch of their three stage ERIS rocket

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yesterday, but had to postpone after

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encountering a ground system glitch during

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pre launch operations. The company's

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communications chief, Michelle Gilmour,

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explained that the issue was with an external

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power system we used during system checks.

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The technical team identified the fix but ran

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out of time to implement it and fuel the

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rocket within the day's launch window. The

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they're now targeting today for the

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rescheduled launch attempt. The 23

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meter 75 foot ARIS rocket is

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poised to take off from a spaceport near

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Bowen, a coastal township approximately

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1000km north of Brisbane. If

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successful, it would mark a significant

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milestone as the first Australian made rocket

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to achieve an orbital launch from Australian

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soil. While the maiden flight is primarily

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a test, the rocket isn't traveling empty. In

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a quintessentially Australian touch, it will

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be carrying a jar of Vegemite, the iconic

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Australian toast spread, as its payload.

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CEO Adam Gilmour has been candid about

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managing expectations for this first flight.

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If it orbits Earth. I would probably have a

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heart attack actually because I'll be so

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surprised but deliriously happy, he told

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reporters. We're going to be happy if it gets

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off the pad. 10, 20,

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30 seconds of flight time. Fantastic. So

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orbit is just not in the realm of my belief

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right now, even though it's theoretically

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possible. The Aris rocket is designed

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to eventually carry small satellites weighing

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between 100 and 200 kg into low

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Earth orbit. Weighing 30 tons when

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fully fueled, it uses a hybrid propulsion

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system combining solid inert fuel with a

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liquid oxidizer. Gilmour Space

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Technologies has backing from private

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investors, including venture capital group

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Blackbird and pension fund Hesta. The

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company, which employs 230 people, has

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ambitious plans to commence commercial

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launches by late 2026 or early

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2027. Here's wishing them all the best with

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the next attempt.

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Now here's a story that truly showcases the

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incredible ingenuity of NASA's engineering

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team in what can only be described

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as a remarkable feat of remote problem

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solving, engineers at NASA's Jet Propulsion

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Laboratory have successfully revived a set of

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thrusters aboard Voyager 1 that had been

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considered completely inoperable since 2004.

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This achievement is particularly impressive

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when you consider that Voyager 1 is currently

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hurtling through interstellar space at

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approximately 35,000 miles per hour,

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over 15 billion miles from Earth.

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That's so far away that radio Signals take

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more than 23 hours to travel between the

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spacecraft and our planet. The thruster

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revival was critically timed. Engineers

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needed to fix these systems before May 4th,

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when the Deep Space Network's 230 foot wide

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antenna in Canberra, Australia, the only

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dish powerful enough to send commands to the

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distant Voyagers, went offline for extensive

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upgrades that will last until February

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2026. With only brief operational

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windows in August and December, why was this

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fix so urgent? The Voyager spacecraft

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rely on small thrusters to maintain their

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orientation, keeping their antennas pointed

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at Earth so they can continue sending back

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data and receiving commands. The

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primary set of thrusters currently in use on

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Voyager 1 have been experiencing fuel tube

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clogging due to residue buildup, which could

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cause them to fail completely as early as

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this northern fall. The situation was

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complicated by the fact that the backup

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thrusters had stopped working back in 2004,

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when two small internal heaters lost power.

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At that time, engineers determined the

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heaters were likely unfixable and switched to

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other backup systems. After all, who could

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have predicted Voyager would still be

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operational two decades later? After

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revisiting the 2004 thruster failure,

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the team suspected that an unexpected circuit

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disturbance had essentially flipped a switch

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to the wrong position. If they could turn the

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switch back, the heaters might work again.

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This M solution required precision timing and

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careful planning. If the spacecraft's star

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tracker drifted too far from its guide star

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during the fix, the dormant thrusters would

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automatically fire without their heaters,

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potentially causing a small explosion.

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On March 20th, after sending their commands

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and waiting anxiously through the 23 hour

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signal delay, the team witnessed the

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temperature of the thruster heaters rise

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dramatically, confirming their success.

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As mission propulsion lead Todd Barber

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described it, it was such a glorious moment.

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Team morale was very high that day. These

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thrusters were considered dead. It was yet

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another miracle, save for Voyager. Launched

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in 1977, both Voyager 1 and its twin

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Voyager 2 continue to push the boundaries of

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space exploration. As the only spacecraft to

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have ever sent back data from interstellar

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space, the region beyond our solar system's

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protective bubble, this latest engineering

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triumph ensures that this incredible

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scientific journey can continue even longer.

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Let's move on now to some news from one of

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our celestial neighbors. Our, understanding

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of Venus, Earth's so called twin planet,

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continues to evolve as scientists uncover

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evidence that it may be more geologically

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active than previously thought. New research

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based on Data gathered over 30 years ago by

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NASA's Magellan mission has revealed

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fascinating insights about vast

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quasicircular features on Venus called

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coronae, which suggest ongoing

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tectonic activity beneath the planet's

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surface. Unlike Earth, with its shifting

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tectonic plates, Venus doesn't have plate

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tectonics as we know it. However, this

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doesn't mean Venus is geologically dead. The

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new study, published in Science Advances

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indicates that its surface is still being

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deformed by molten material rising from

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below. Coronae are enormous structures

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ranging from dozens to hundreds of miles

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across, where plumes of hot buoyant material

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from Venus's mantle are thought to push

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against the lithosphere, the planet's crust

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and uppermost mantle layer. These features

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typically appear as oval structures

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surrounded by concentric fracture systems,

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and hundreds of them have been identified

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across Venus. What makes this

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research particularly exciting is that it

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suggests multiple ongoing processes are are

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actively shaping these coronae. By combining

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gravity and topography data from Magellan and

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developing sophisticated three dimensional

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geodynamic models, researchers were able to

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identify 52 carony out of the 75

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studied that appear to have buoyant mantle

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material beneath them, likely driving

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tectonic processes. The team

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identified several different mechanisms

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potentially at work in some carony. A,

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venous specific type of subduction may be

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occurring. As hot rock pushes upward

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from the mantle surface, material rises and

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spreads outward, eventually colliding with

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surrounding material and pushing it downward

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into the mantle. Another process called

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lithospheric dripping, might also be present

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where dense accumulations of cooler material

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sink from the lithosphere into the hot mantle

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below. Lead researcher Gail

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Cascioli, who is part of NASA's forthcoming

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Veritas mission to Venus, noted that these

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features might provide a unique window into

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Earth's past. Coronae are not found

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on Earth today. However, they may have

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existed when our planet was young and before

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plate tectonics had been established, he

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explained. This work is especially

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significant as it represents yet another

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instance where scientists are finding Venus

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exhibits more Earth like geologic processes

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than originally thought. Just recently,

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researchers were able to identify erupting

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volcanoes and vast lava flows in radar images

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from Magellan, providing direct evidence of

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volcanic activity. While these discoveries

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are groundbreaking, scientists will need even

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higher resolution data to fully understand

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the tectonic processes driving corona

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formation. That's where NASA's upcoming

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Veritas mission comes in. Scheduled to launch

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no earlier than 2031, Veridus will

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create detailed three dimensional global maps

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00:14:07.530 --> 00:14:10.290
of Venus and measure its gravitational field

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00:14:10.370 --> 00:14:12.500
to determine the structure of the planet's

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interior at unprecedented resolution,

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potentially revolutionizing our understanding

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of Venus and what it might tell us about

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Earth's early history.

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Next, let's head off to our other near

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neighbor and One of our favorite planets. In

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a groundbreaking astronomical first, NASA's

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Perseverance rover has captured an image of a

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visible aurora on Mars. On March

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18, 2024, the rover

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observed what scientists describe as a subtle

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green glow hanging low in the Martian sky,

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Wreathing the horizon in every direction.

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This marks not only the first sighting of a

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visible Martian aurora, but also the first

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observation of any aurora from the surface of

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a planet other than Earth. Until now,

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auroras had been spotted on Mercury, Jupiter,

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00:14:58.870 --> 00:15:01.270
and every other non Earth planet in our solar

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system, but only from orbit. On Mars

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specifically, scientists had only detected

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auroral wavelengths of light that are

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invisible to the naked eye. Using specialized

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instruments. This new observation answers a

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long standing question. About what future

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human explorers might witness in the Martian

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night sky. According to Roger Wiens,

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a planetary scientist at Purdue University,

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00:15:23.510 --> 00:15:26.150
future astronauts would see a dull or dim

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00:15:26.150 --> 00:15:29.150
green glow with their own eyes. The image

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00:15:29.150 --> 00:15:31.030
from Perseverance appears somewhat fuzzy

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Compared to the spectacular aurora displays

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00:15:33.230 --> 00:15:34.950
we're accustomed to seeing from Earth. And

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for good reason. The rover's cameras aren't

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00:15:37.470 --> 00:15:40.030
optimized for night photography, Performing

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00:15:40.030 --> 00:15:42.350
with sensitivity roughly comparable to human

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00:15:42.350 --> 00:15:44.750
eyes. Another factor contributing to the

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00:15:44.750 --> 00:15:46.870
aurora's different appearance Is Mars's

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00:15:46.870 --> 00:15:49.750
unique magnetic environment. Unlike Earth,

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00:15:49.750 --> 00:15:51.430
with its global magnetic field that

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00:15:51.430 --> 00:15:53.770
concentrates auroras near the poles. Mars

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Mars has a patchy magnetized crust. This

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means auroras can appear all over the planet

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00:15:58.720 --> 00:16:00.840
Rather than being confined to polar regions.

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But they tend to be comparatively dim.

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Scientists believe this particular aurora was

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00:16:05.960 --> 00:16:08.880
triggered by a coronal mass ejection, A large

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00:16:08.880 --> 00:16:11.280
cloud of plasma and magnetic fields blasted

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00:16:11.280 --> 00:16:14.240
from the sun into space. The Perseverance

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00:16:14.240 --> 00:16:16.360
team was alerted to this solar event days in

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00:16:16.360 --> 00:16:18.760
advance, allowing them to prepare the rover

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00:16:18.760 --> 00:16:20.780
to capture this historic image.

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00:16:21.180 --> 00:16:23.700
Interestingly, while Perseverance is located

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00:16:23.700 --> 00:16:26.500
near Mars's equator, Researchers suggest that

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observing auroras from Mars's southern

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00:16:28.500 --> 00:16:31.060
hemisphere Might yield even more spectacular

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00:16:31.060 --> 00:16:33.660
results. That region contains the most

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00:16:33.660 --> 00:16:36.260
magnetized part of the planet, Potentially

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00:16:36.260 --> 00:16:38.300
producing stronger auroral displays.

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00:16:39.100 --> 00:16:41.460
This discovery adds another fascinating

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00:16:41.460 --> 00:16:43.820
chapter to our understanding of Mars. And

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00:16:43.820 --> 00:16:45.860
provides a glimpse of the ethereal

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00:16:45.860 --> 00:16:48.130
experiences awaiting future human

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00:16:48.130 --> 00:16:51.090
explorers who might one day stand on the

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00:16:51.090 --> 00:16:54.050
red planet's surface, Gazing up at

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00:16:54.050 --> 00:16:56.090
a glowing green Martian sky.

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And that brings us to the end of today's

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00:16:59.930 --> 00:17:02.090
cosmic journey through the latest space news.

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00:17:02.410 --> 00:17:04.890
From the mysterious asymmetry of our Moon to

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00:17:04.890 --> 00:17:07.650
engineering marvels on Voyager 1, tectonic

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00:17:07.650 --> 00:17:10.290
activity on Venus, Delayed rocket launches in

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00:17:10.290 --> 00:17:12.850
Australia, and the first ever image of a

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00:17:12.850 --> 00:17:15.619
Martian aurora. The universe continues to

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00:17:15.619 --> 00:17:17.899
surprise and inspire us with each new

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00:17:17.899 --> 00:17:20.739
discovery. I'm Anna, your host here

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on Astronomy Daily, bringing you the stories

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that connect us to the vast cosmos beyond our

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00:17:25.699 --> 00:17:28.339
atmosphere. Whether you're a seasoned

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00:17:28.339 --> 00:17:31.339
astronomer or simply curious about what lies

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00:17:31.339 --> 00:17:34.019
beyond our blue marble, I hope today's

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00:17:34.019 --> 00:17:36.379
episode has sparked your imagination and

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00:17:36.379 --> 00:17:38.819
deepened your appreciation for the wonders of

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00:17:38.819 --> 00:17:41.730
space exploration. If you've enjoyed

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00:17:41.730 --> 00:17:43.410
today's show, please visit our

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00:17:43.410 --> 00:17:46.410
website@astronomydaily.IO where you can

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00:17:46.410 --> 00:17:48.570
sign up for our free daily newsletter and

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00:17:48.570 --> 00:17:50.690
stay informed about breaking astronomy news

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00:17:51.090 --> 00:17:52.850
while you're there. You can also browse

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00:17:52.850 --> 00:17:55.170
through all our back episodes to catch up on

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00:17:55.170 --> 00:17:57.570
any cosmic stories you might have missed.

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00:17:58.050 --> 00:18:00.330
Don't forget to subscribe to Astronomy Daily

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on Apple Podcasts, Spotify, YouTubeMusic,

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00:18:03.090 --> 00:18:05.450
or wherever you get your podcasts to ensure

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00:18:05.450 --> 00:18:08.110
you never miss an episode. Until next time,

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00:18:08.270 --> 00:18:10.470
keep looking up. The universe is putting on

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00:18:10.470 --> 00:18:11.070
quite a show.
