July 15, 2025
Astronauts Homeward Bound, Sun's Secrets Unveiled, and Uranus's Heat Revelation
- Axiom Space's AX4 Mission Returns: Join us as we check-in on the return of the AX4 crew from the International Space Station. Led by Commentaor Peggy Whitson, the crew conducted over 60 experiments during their extended stay, making history as the first astronauts from India, Poland, and Hungary to visit the ISS. We discuss their journey aboard the SpaceX Crew Dragon capsule, and the implications of their research for future missions.
- - Parker Solar Probe's Groundbreaking Discoveries: Delve into the latest stunning images from NASA's Parker Solar Probe, which recently flew closer to the Sun than any spacecraft before. Learn how these insights into solar weather and the Sun's atmosphere are reshaping our understanding of space weather threats and improving safety for astronauts and technology on Earth.
- - Global Launch Roundup: Catch up on a whirlwind week of space launches, including China's successful cargo resupply mission to the Tiangong Space Station, and Gilmour Space's maiden launch attempt of its Eris rocket from Australia. We also highlight SpaceX's busy schedule, featuring the launch of Starlink satellites and Amazon's Kuiper satellites.
- - Surprising Findings on Uranus: Discover new research suggesting that Uranus emits more internal heat than it receives from the Sun, challenging previous assumptions made by Voyager 2. This revelation could redefine our understanding of Uranus's internal structure and evolution, bolstering the case for future exploration missions.
- For more cosmic updates, visit our website at astronomydaily.io. Join our community on social media by searching for #AstroDailyPod on Facebook, X, YouTube Music Music, TikTok, and our new Instagram account! Don’t forget to subscribe to the podcast on Apple Podcasts, Spotify, iHeartRadio, or wherever you get your podcasts.
- Thank you for tuning in. This is Anna signing off. Until next time, keep looking up and stay curious about the wonders of our universe.
Axiom Space AX4 Mission
[Axiom Space](https://www.axiomspace.com/)
Parker Solar Probe
[NASA](https://www.nasa.gov/content/parker-solar-probe)
Global Launches
[SpaceX](https://www.spacex.com/)
Uranus Research
[University of Houston](https://www.uh.edu/)
Astronomy Daily
[Astronomy Daily](http://www.astronomydaily.io/)
Become a supporter of this podcast: https://www.spreaker.com/podcast/astronomy-daily-space-news-updates--5648921/support.
WEBVTT
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Anna: Welcome to Astronomy Daily, your daily dose of
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cosmic updates and celestial wonders. I'm your
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host, Anna, and I'm thrilled to dive into some truly
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captivating space news with you today. First,
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we'll be looking at the return trip of private astronauts from
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the International Space Station after an extended stay
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highlighting their incredible work and a new splashdown
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location. Then we'll zoom in on our very own star,
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the sun, as NASA's Parker Solar Probe sends
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back the closest ever images, revealing
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groundbreaking insights into solar weather. Our
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journey continues with a global launch roundup
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featuring a busy week for space agencies worldwide,
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including cargo resupply missions, maiden
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rocket flights and a flurry of Internet satellite
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deployments. And finally, we'll uncover
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a surprising new discovery about the distant ice
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giant Uranus that might just rewrite its
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planetary history and bolster the case for a
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future mission. So buckle up because there's a lot to
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explore.
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We kick things off today with news from above our heads
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as the four intrepid astronauts of Axiom
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Space's latest private mission, AX4,
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have successfully concluded their stay aboard the International
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Space Station and are, uh, currently headed home.
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Their SpaceX Crew Dragon capsule, aptly named
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Grace, undocked from the ISS this morning,
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July 14, marking the final leg of
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their journey back to Earth. The undocking
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happened precisely at 7:15am
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EDT. Grace then gracefully
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maneuvered away from the orbital laboratory which had been
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the AX4 crew's home for the past two and a half
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weeks. This was actually a bit longer than their
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originally planned two week stay, giving them even
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more time to complete their extensive research.
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Leading the AX4 mission was Commander Peggy
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Whitson, a former NASA astronaut and now
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Axiom's Director of Human Spaceflight. As
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Grace cleared the isss safety keep out
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sphere, Whitson transmitted a heartfelt message
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saying Space Station grace, the AX4 crew wants
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to thank you very much for your support. You guys are
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amazing. This mission marks
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Whitson's fifth trip to orbit, pushing her
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impressive record for most cumulative days in space by
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an American to an incredible 695
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days. Her crewmates included pilot
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Shubanshu Shuks Shukla and mission
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specialists Slawas Suave, Uznansky
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Wisniewski and Tibor Kapu. What's
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particularly exciting is that this was the first space flight for
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Shucks, Suave and Kapu. And they also
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made history as the first citizens of India, Poland and
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Hungary respectively to launch on a mission to the
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International Space Station. Throughout their
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time in microgravity, the AX4 crew
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undertook more than 60 experiments and technology
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demonstrations with contributions from a
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remarkable 31 different nations. They
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also participated in numerous public outreach events,
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setting a new record for Axiom as the company continues to
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refine its orbital operations.
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Launched aboard a SpaceX Falcon 9 rocket from
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NASA's storied Launch Complex 39A in
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Florida on June 26, the crew spent just
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over a day catching up to the International Space Station
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after their extended mission. The departure procedures began
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early this morning with the crew entering Grace and closing
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the hatch. Now Grace and its crew are on a
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22.5 hour trajectory, set to splash
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down in the Pacific Ocean off the coast of California
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early on Tuesday, Eastern Daylight Time.
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This will be a notable event as it's only
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SpaceX's second West coast crew recovery.
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Following the Crew 9 ISS mission in March,
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SpaceX has made a permanent shift to Pacific Ocean
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recoveries instead of the Atlantic or Gulf, a uh
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change driven by instances of debris from Dragon's trunk
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surviving atmospheric reentry and crashing back to Earth.
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This new re entry path significantly minimizes the
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chances of such debris causing any damage or injury,
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prioritizing safety for everyone.
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Now let's turn our gaze to our closest star, the sun,
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where NASA's Parker Solar Probe continues to
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redefine our understanding. Understanding this
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incredible spacecraft is certainly no stranger to
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breaking records. On December 24,
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2024, Parker made history by flying
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closer to the sun than any spacecraft ever,
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reaching a mere 3.8 million miles from the
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solar surface. In doing so, it
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entered the outermost layer of the Sun's atmosphere, the
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corona. During this daring flyby, it
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also broke its own record as the fastest human made
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object, soaring at an astonishing
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430,000 miles per hour.
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Recently, NASA released some truly remarkable video
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footage captured during this historic flyby,
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offering us the closest views of the sun ever
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recorded. These groundbreaking images were
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captured by Parker's Wide Field Imager for Solar
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Probe or Wispiar, revealing a uh, never before
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seen perspective of the Sun's corona and the solar
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winds shortly after they're released from it.
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As Nikki Fox, Associate Administrator for the Science
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Mission Directorate at NASA Headquarters, noted,
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Parker Solar Probe has once again transported us into
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the dynamic atmosphere of our closest star.
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She emphasized the incredible advantage of
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witnessing where space weather threats to Earth begin
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with our eyes, not just with models.
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This new data is set to vastly improve
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our space weather predictions, enhancing
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the safety of our astronauts and the protection
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of our vital technology both on Earth and
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throughout the solar system. WISPR's
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images have unveiled an important boundary within the Sun's
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atmosphere known as the heliospheric current sheet,
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where the Sun's magnetic field Dramatically shifts direction
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from north to south. Even more impressively,
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it captured for the first time in high resolution
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collisions between multiple coronal mass ejections,
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or CMEs. These CMEs are major drivers
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of space weather and are crucial for understanding
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risks to astronauts and Earth based technology
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like power grids and communication satellites.
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Angelus Vorlidas, the Whisper instrument
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scientist, explained that in these images, we're
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seeing the CMEs basically piling up on top of
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one another. We're using this to figure out how the
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CMEs merge together. Before the
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Parker Solar Probe, NASA and its international
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partners could only study solar wind from a distance.
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That's why Parker has been instrumental in bridging key knowledge
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gaps. It identified the widespread presence
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of switchbacks, which are zigzagging magnetic
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field patterns Even at distances of around
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14.7 million miles from the sun,
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linking them directly to the origins of one of the two main
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types of solar wind. Closer in, at just
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8 million miles, Parker revealed that the boundary of the
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Sun's corona Is far more uneven and complex
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Than previously imagined. But the
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probe's discoveries didn't stop there. The big
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unknown has always been how solar wind is generated
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and how it manages to escape the Sun's immense
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gravitational pull. Noor
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Rawafi, the project scientist for Parker Solar
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Probe, Described understanding this continuous flow
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of particles, especially the slow solar wind,
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as a major challenge, Particularly given the
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diversity in the properties of these streams.
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However, thanks to Parker Solar Probe,
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scientists are closer than ever to uncovering their
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origins and how they evolve. Prior to
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Parker Solar Probe, distant observations suggested there
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were two varieties of slow solar wind differentiated
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by the orientation or variability of their magnetic
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fields. One type, called alphenic,
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Exhibits small scale switchbacks, While the second,
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non alphenic, does not. As it spiraled
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closer to the Sun, Parker confirmed the existence of
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both types. Its close up views are also
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helping scientists distinguish the origins of these two
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unique types. It's believed that the non
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alvenic wind May emerge From features called
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helmet streamers, Large loops connecting
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active regions where some particles can heat up enough to
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escape. While the alphenic wind might originate near
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coronal holes, which are dark, cooler regions in
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the corona. As Adam Sabo, Parker Solar
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Probe mission scientist, put it in we don't have a final
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consensus yet, but we have a whole lot of new intriguing data.
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So how does the Parker Solar Probe Manage to endure
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such extreme conditions? From the freezing
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cold of deep space to the intense heat near the Sun?
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A, uh, key factor in its survival lies in the fundamental
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difference between temperature and heat. While the
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space near the sun can reach temperatures of several million
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degrees, this doesn't necessarily mean there's a lot of heat
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transferred. This is because the Sun's corona is
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incredibly thin, meaning there are far fewer
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particles. Even though individual particles in the
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corona are exceptionally hot, their scarcity
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means the probe doesn't receive much actual heat.
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NASA scientists explain that while the probe travels
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through space with temperatures of several million degrees,
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the surface of its heat shield facing the sun will only be
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heated to about 2500°F,
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or roughly 1400°C.
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These temperatures are, of course, still incredibly hot,
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which makes its robust heat shield, the Thermal
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Protection System, or tps, absolutely essential.
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This shield is crafted from a carbon composite foam
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sandwiched between two carbon plates. Carbon
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is an ideal material for this purpose because it is both
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remarkably lightweight and capable of
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withstanding extremely high temperatures without melting.
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Tested to withstand up to 3,000 degrees Fahrenheit,
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or 1,650 degrees Celsius,
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the TPS can handle any heat the sun sends
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its way, keeping almost all the probe's
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instrumentation safe. Its unique structure
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enables it to endure intense heat while minimizing
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weight, a crucial factor for a spacecraft designed to
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travel at such extreme speeds.
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Furthermore, the outer surface of the TPS is coated with a
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white ceramic paint designed to reflect as much solar
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energy as possible and further reduce the amount of heat
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absorbed.
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Next, let's look at this week's launch schedule. And
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this week has certainly been a whirlwind in the world of space
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launches, with multiple missions lifting off from
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sites across the globe. First, from
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China, their latest cargo supply mission to the
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Tiangong Space Station successfully lifted off
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The Chang Geng 7 rocket. Launched the Tianzhou 9
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cargo vehicle from the Wencheng space launch site on
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Monday, July 14. This mission brings
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essential supplies for the Shenzhou 20 crew,
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including food, life support, scientific experiments,
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and propellants. Notably, it also
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delivered two upgraded Fei Shen extravehicular
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activity suits designed for extensive use.
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Tianzhou 9 is expected to spend six to seven months
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at the station carrying a substantial
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7,400kg of cargo,
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showcasing China's robust orbital resupply
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capabilities. Meanwhile, a significant
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milestone is on the horizon for Australia.
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Gilmour Space is gearing up to try again for its second attempt
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at the maiden launch of its Eris small satellite rocket this
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Wednesday, July 16, from the Bowen Orbital
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Spaceport. This pivotal launch follows a
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previous stand down in May due to an unexpected
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power surge. Now mitigated, this three
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stage Eris launcher, proudly Australian made,
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is poised to become the very first orbital launch from
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from Australian soil performed by a sovereign built
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vehicle. Standing at 25 meters tall,
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Eris can carry payloads of up to 215
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kilograms to a 500 kilometer Sun Synchronous
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Orbit. Its first stage uses unique
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hybrid Sirius engines and a successful
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orbital launch would also mark a historic first
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for a hybrid rocket design globally.
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Gilmour Space recently partnered with Tokyo based
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Space bd, opening up opportunities for
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Japanese and global satellite customers.
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And Speaking of busy, SpaceX continues its
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relentless pace with a packed schedule of
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launches, predominantly expanding Internet
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satellite constellations earlier this week,
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a Falcon 9 rocket launched 26 Starlink
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VTU mini Internet satellites into low Earth
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orbit from Vandenberg, California. This particular
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launch was significant as it marked the
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150th consecutive successful mission for a Falcon
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rocket since an anomaly back in July
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2024. A truly remarkable streak.
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Looking ahead, SpaceX is also set to launch its very
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first contracted batch of Amazon's Kuiper satellites
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this Wednesday, July 16th from Cape Canaveral in
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Florida. Project Kuiper is Amazon's direct
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competitor to Starlink, aiming to build its own
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massive Internet constellation. This mission will
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carry at least 20 of these crucial
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satellites. Amazon faces ambitious
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deadlines, needing to launch its full constellation of
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over 3200 satellites by
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July 2029, with half required by
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July 2026. This requires numerous
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launches across various providers. To
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round out SpaceX's week. Two more Starlink launches
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are scheduled from Vandenberg. On Wednesday, July
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16, another Falcon 9 will launch satellites
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into Starlink's Group 17 shell, flying into
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a highly inclined sun synchronous orbit.
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And finally, on Sunday, July 20, a third
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batch of Starlink satellites will launch from the same
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California pad, completing a remarkably busy
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period for SpaceX and further expanding global
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Internet access.
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Now let's turn our attention to one of our solar system's distant
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ice giants, Uranus, which is proving to be
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far more fascinating than we once thought.
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New scientific findings have revealed something quite surprising
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about this enigmatic planet. It's emitting its
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own internal heat, even more than it receives from the
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sun. This discovery actually
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contradicts observations made by NASA's Voyager 2
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probe nearly four decades ago. Back in
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1986, Voyager 2 flew by Uranus, and
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its readings suggested the planet didn't have significant
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internal heat. However, new research
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led by Xinyue Yang of the University of Houston
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analyzed decades of spacecraft readings and computer
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models. Their findings indicate that Uranus
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emits 12.5% more internal heat
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than it absorbs from solar radiation. While
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this is less than other outer planets like Jupiter, Saturn,
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and Neptune, which radiate 100% more heat
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than they receive, it's still a significant amount that
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challenges our previous understanding. It
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turns out we might have caught Uranus at a peculiar time during the
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Voyager 2 flyby, with some readings potentially
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skewed by a surge in solar weather. By combining
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archival data with advanced computer models,
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scientists now believe this internal heat suggests a
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completely different internal structure or evolutionary
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history for the planet. For a long time,
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it was thought that Uranus formed closer to the sun
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before migrating outwards. These
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new findings are now calling that story into question.
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This fresh understanding of Uranus's internal
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processes could also significantly boost the case
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for future missions to the distant planet.
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The National Academy of Sciences had already
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flagged a mission concept called the Uranus Orbiter
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and Probe, or uop, as a high priority
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for the next decade. These new results showing
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how Uranus stores and loses heat not only
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deepen our understanding of this icy world, but
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also offer valuable insights into
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fundamental processes that shape planetary
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atmospheres, weather systems, and even
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climate systems. It's groundbreaking science that
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could inform our studies of Earth's own changing climate.
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And that brings us to the end of another fascinating
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episode of Astronomy Daily. Thank you so much
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for tuning in and joining me on this cosmic
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exploration. I'm Anna, and it's been a
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pleasure sharing the latest in space and astronomy news with you.
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Remember, you can catch up on all the latest space and astronomy
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news and listen to all our back episodes by visiting our
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website@astronomydaily.IO. and don't
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forget to subscribe to the podcast on Apple podcasts,
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Spotify and YouTube Music or wherever you get your
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podcasts so you never miss an episode. Until next time, keep
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looking up
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Anna: Welcome to Astronomy Daily, your daily dose of
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cosmic updates and celestial wonders. I'm your
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host, Anna, and I'm thrilled to dive into some truly
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captivating space news with you today. First,
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we'll be looking at the return trip of private astronauts from
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the International Space Station after an extended stay
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highlighting their incredible work and a new splashdown
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location. Then we'll zoom in on our very own star,
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the sun, as NASA's Parker Solar Probe sends
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back the closest ever images, revealing
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groundbreaking insights into solar weather. Our
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journey continues with a global launch roundup
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featuring a busy week for space agencies worldwide,
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including cargo resupply missions, maiden
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rocket flights and a flurry of Internet satellite
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deployments. And finally, we'll uncover
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a surprising new discovery about the distant ice
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giant Uranus that might just rewrite its
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planetary history and bolster the case for a
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future mission. So buckle up because there's a lot to
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explore.
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We kick things off today with news from above our heads
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as the four intrepid astronauts of Axiom
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Space's latest private mission, AX4,
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have successfully concluded their stay aboard the International
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Space Station and are, uh, currently headed home.
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Their SpaceX Crew Dragon capsule, aptly named
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Grace, undocked from the ISS this morning,
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July 14, marking the final leg of
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their journey back to Earth. The undocking
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happened precisely at 7:15am
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EDT. Grace then gracefully
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maneuvered away from the orbital laboratory which had been
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the AX4 crew's home for the past two and a half
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weeks. This was actually a bit longer than their
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originally planned two week stay, giving them even
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more time to complete their extensive research.
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Leading the AX4 mission was Commander Peggy
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Whitson, a former NASA astronaut and now
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Axiom's Director of Human Spaceflight. As
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Grace cleared the isss safety keep out
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sphere, Whitson transmitted a heartfelt message
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saying Space Station grace, the AX4 crew wants
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to thank you very much for your support. You guys are
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amazing. This mission marks
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Whitson's fifth trip to orbit, pushing her
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impressive record for most cumulative days in space by
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an American to an incredible 695
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days. Her crewmates included pilot
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Shubanshu Shuks Shukla and mission
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specialists Slawas Suave, Uznansky
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Wisniewski and Tibor Kapu. What's
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particularly exciting is that this was the first space flight for
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Shucks, Suave and Kapu. And they also
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made history as the first citizens of India, Poland and
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Hungary respectively to launch on a mission to the
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International Space Station. Throughout their
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time in microgravity, the AX4 crew
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undertook more than 60 experiments and technology
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demonstrations with contributions from a
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remarkable 31 different nations. They
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also participated in numerous public outreach events,
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setting a new record for Axiom as the company continues to
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refine its orbital operations.
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Launched aboard a SpaceX Falcon 9 rocket from
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NASA's storied Launch Complex 39A in
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Florida on June 26, the crew spent just
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over a day catching up to the International Space Station
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after their extended mission. The departure procedures began
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early this morning with the crew entering Grace and closing
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the hatch. Now Grace and its crew are on a
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22.5 hour trajectory, set to splash
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down in the Pacific Ocean off the coast of California
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early on Tuesday, Eastern Daylight Time.
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This will be a notable event as it's only
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SpaceX's second West coast crew recovery.
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Following the Crew 9 ISS mission in March,
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SpaceX has made a permanent shift to Pacific Ocean
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recoveries instead of the Atlantic or Gulf, a uh
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change driven by instances of debris from Dragon's trunk
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surviving atmospheric reentry and crashing back to Earth.
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This new re entry path significantly minimizes the
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chances of such debris causing any damage or injury,
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prioritizing safety for everyone.
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Now let's turn our gaze to our closest star, the sun,
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where NASA's Parker Solar Probe continues to
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redefine our understanding. Understanding this
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incredible spacecraft is certainly no stranger to
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breaking records. On December 24,
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2024, Parker made history by flying
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closer to the sun than any spacecraft ever,
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reaching a mere 3.8 million miles from the
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solar surface. In doing so, it
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entered the outermost layer of the Sun's atmosphere, the
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corona. During this daring flyby, it
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also broke its own record as the fastest human made
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object, soaring at an astonishing
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430,000 miles per hour.
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Recently, NASA released some truly remarkable video
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footage captured during this historic flyby,
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offering us the closest views of the sun ever
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recorded. These groundbreaking images were
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captured by Parker's Wide Field Imager for Solar
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Probe or Wispiar, revealing a uh, never before
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seen perspective of the Sun's corona and the solar
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winds shortly after they're released from it.
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As Nikki Fox, Associate Administrator for the Science
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Mission Directorate at NASA Headquarters, noted,
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Parker Solar Probe has once again transported us into
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the dynamic atmosphere of our closest star.
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She emphasized the incredible advantage of
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witnessing where space weather threats to Earth begin
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with our eyes, not just with models.
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This new data is set to vastly improve
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our space weather predictions, enhancing
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the safety of our astronauts and the protection
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of our vital technology both on Earth and
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throughout the solar system. WISPR's
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images have unveiled an important boundary within the Sun's
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atmosphere known as the heliospheric current sheet,
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where the Sun's magnetic field Dramatically shifts direction
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from north to south. Even more impressively,
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it captured for the first time in high resolution
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collisions between multiple coronal mass ejections,
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or CMEs. These CMEs are major drivers
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of space weather and are crucial for understanding
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risks to astronauts and Earth based technology
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like power grids and communication satellites.
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Angelus Vorlidas, the Whisper instrument
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scientist, explained that in these images, we're
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seeing the CMEs basically piling up on top of
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one another. We're using this to figure out how the
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CMEs merge together. Before the
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Parker Solar Probe, NASA and its international
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partners could only study solar wind from a distance.
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That's why Parker has been instrumental in bridging key knowledge
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gaps. It identified the widespread presence
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of switchbacks, which are zigzagging magnetic
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field patterns Even at distances of around
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14.7 million miles from the sun,
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linking them directly to the origins of one of the two main
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types of solar wind. Closer in, at just
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8 million miles, Parker revealed that the boundary of the
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Sun's corona Is far more uneven and complex
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Than previously imagined. But the
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probe's discoveries didn't stop there. The big
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unknown has always been how solar wind is generated
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and how it manages to escape the Sun's immense
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gravitational pull. Noor
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Rawafi, the project scientist for Parker Solar
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Probe, Described understanding this continuous flow
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of particles, especially the slow solar wind,
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as a major challenge, Particularly given the
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diversity in the properties of these streams.
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However, thanks to Parker Solar Probe,
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scientists are closer than ever to uncovering their
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origins and how they evolve. Prior to
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Parker Solar Probe, distant observations suggested there
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were two varieties of slow solar wind differentiated
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by the orientation or variability of their magnetic
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fields. One type, called alphenic,
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Exhibits small scale switchbacks, While the second,
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non alphenic, does not. As it spiraled
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closer to the Sun, Parker confirmed the existence of
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both types. Its close up views are also
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helping scientists distinguish the origins of these two
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unique types. It's believed that the non
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alvenic wind May emerge From features called
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helmet streamers, Large loops connecting
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active regions where some particles can heat up enough to
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escape. While the alphenic wind might originate near
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coronal holes, which are dark, cooler regions in
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the corona. As Adam Sabo, Parker Solar
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Probe mission scientist, put it in we don't have a final
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consensus yet, but we have a whole lot of new intriguing data.
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So how does the Parker Solar Probe Manage to endure
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such extreme conditions? From the freezing
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cold of deep space to the intense heat near the Sun?
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A, uh, key factor in its survival lies in the fundamental
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difference between temperature and heat. While the
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space near the sun can reach temperatures of several million
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degrees, this doesn't necessarily mean there's a lot of heat
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transferred. This is because the Sun's corona is
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incredibly thin, meaning there are far fewer
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particles. Even though individual particles in the
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corona are exceptionally hot, their scarcity
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means the probe doesn't receive much actual heat.
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NASA scientists explain that while the probe travels
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through space with temperatures of several million degrees,
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the surface of its heat shield facing the sun will only be
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heated to about 2500°F,
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or roughly 1400°C.
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These temperatures are, of course, still incredibly hot,
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which makes its robust heat shield, the Thermal
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Protection System, or tps, absolutely essential.
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This shield is crafted from a carbon composite foam
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sandwiched between two carbon plates. Carbon
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is an ideal material for this purpose because it is both
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remarkably lightweight and capable of
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withstanding extremely high temperatures without melting.
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Tested to withstand up to 3,000 degrees Fahrenheit,
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or 1,650 degrees Celsius,
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the TPS can handle any heat the sun sends
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its way, keeping almost all the probe's
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instrumentation safe. Its unique structure
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enables it to endure intense heat while minimizing
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weight, a crucial factor for a spacecraft designed to
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travel at such extreme speeds.
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Furthermore, the outer surface of the TPS is coated with a
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white ceramic paint designed to reflect as much solar
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energy as possible and further reduce the amount of heat
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absorbed.
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Next, let's look at this week's launch schedule. And
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this week has certainly been a whirlwind in the world of space
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launches, with multiple missions lifting off from
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sites across the globe. First, from
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China, their latest cargo supply mission to the
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Tiangong Space Station successfully lifted off
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The Chang Geng 7 rocket. Launched the Tianzhou 9
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cargo vehicle from the Wencheng space launch site on
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Monday, July 14. This mission brings
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essential supplies for the Shenzhou 20 crew,
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including food, life support, scientific experiments,
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and propellants. Notably, it also
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delivered two upgraded Fei Shen extravehicular
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activity suits designed for extensive use.
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Tianzhou 9 is expected to spend six to seven months
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at the station carrying a substantial
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7,400kg of cargo,
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showcasing China's robust orbital resupply
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capabilities. Meanwhile, a significant
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milestone is on the horizon for Australia.
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Gilmour Space is gearing up to try again for its second attempt
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at the maiden launch of its Eris small satellite rocket this
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Wednesday, July 16, from the Bowen Orbital
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Spaceport. This pivotal launch follows a
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previous stand down in May due to an unexpected
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power surge. Now mitigated, this three
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stage Eris launcher, proudly Australian made,
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is poised to become the very first orbital launch from
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from Australian soil performed by a sovereign built
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vehicle. Standing at 25 meters tall,
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Eris can carry payloads of up to 215
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kilograms to a 500 kilometer Sun Synchronous
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Orbit. Its first stage uses unique
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hybrid Sirius engines and a successful
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orbital launch would also mark a historic first
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for a hybrid rocket design globally.
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Gilmour Space recently partnered with Tokyo based
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Space bd, opening up opportunities for
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Japanese and global satellite customers.
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And Speaking of busy, SpaceX continues its
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relentless pace with a packed schedule of
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launches, predominantly expanding Internet
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satellite constellations earlier this week,
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a Falcon 9 rocket launched 26 Starlink
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VTU mini Internet satellites into low Earth
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orbit from Vandenberg, California. This particular
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launch was significant as it marked the
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150th consecutive successful mission for a Falcon
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rocket since an anomaly back in July
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2024. A truly remarkable streak.
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Looking ahead, SpaceX is also set to launch its very
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first contracted batch of Amazon's Kuiper satellites
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this Wednesday, July 16th from Cape Canaveral in
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Florida. Project Kuiper is Amazon's direct
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competitor to Starlink, aiming to build its own
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massive Internet constellation. This mission will
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carry at least 20 of these crucial
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satellites. Amazon faces ambitious
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deadlines, needing to launch its full constellation of
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over 3200 satellites by
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July 2029, with half required by
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July 2026. This requires numerous
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launches across various providers. To
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round out SpaceX's week. Two more Starlink launches
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are scheduled from Vandenberg. On Wednesday, July
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16, another Falcon 9 will launch satellites
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into Starlink's Group 17 shell, flying into
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a highly inclined sun synchronous orbit.
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And finally, on Sunday, July 20, a third
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batch of Starlink satellites will launch from the same
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California pad, completing a remarkably busy
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period for SpaceX and further expanding global
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Internet access.
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Now let's turn our attention to one of our solar system's distant
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ice giants, Uranus, which is proving to be
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far more fascinating than we once thought.
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New scientific findings have revealed something quite surprising
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about this enigmatic planet. It's emitting its
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own internal heat, even more than it receives from the
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sun. This discovery actually
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contradicts observations made by NASA's Voyager 2
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probe nearly four decades ago. Back in
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1986, Voyager 2 flew by Uranus, and
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its readings suggested the planet didn't have significant
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internal heat. However, new research
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led by Xinyue Yang of the University of Houston
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analyzed decades of spacecraft readings and computer
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models. Their findings indicate that Uranus
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emits 12.5% more internal heat
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than it absorbs from solar radiation. While
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this is less than other outer planets like Jupiter, Saturn,
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and Neptune, which radiate 100% more heat
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than they receive, it's still a significant amount that
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challenges our previous understanding. It
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turns out we might have caught Uranus at a peculiar time during the
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Voyager 2 flyby, with some readings potentially
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skewed by a surge in solar weather. By combining
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archival data with advanced computer models,
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scientists now believe this internal heat suggests a
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completely different internal structure or evolutionary
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history for the planet. For a long time,
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it was thought that Uranus formed closer to the sun
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before migrating outwards. These
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new findings are now calling that story into question.
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This fresh understanding of Uranus's internal
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processes could also significantly boost the case
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for future missions to the distant planet.
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The National Academy of Sciences had already
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flagged a mission concept called the Uranus Orbiter
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and Probe, or uop, as a high priority
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for the next decade. These new results showing
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how Uranus stores and loses heat not only
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deepen our understanding of this icy world, but
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also offer valuable insights into
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fundamental processes that shape planetary
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atmospheres, weather systems, and even
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climate systems. It's groundbreaking science that
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could inform our studies of Earth's own changing climate.
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And that brings us to the end of another fascinating
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episode of Astronomy Daily. Thank you so much
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for tuning in and joining me on this cosmic
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exploration. I'm Anna, and it's been a
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pleasure sharing the latest in space and astronomy news with you.
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Remember, you can catch up on all the latest space and astronomy
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news and listen to all our back episodes by visiting our
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00:16:06.430 --> 00:16:09.390
website@astronomydaily.IO. and don't
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00:16:09.390 --> 00:16:12.190
forget to subscribe to the podcast on Apple podcasts,
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00:16:12.350 --> 00:16:15.270
Spotify and YouTube Music or wherever you get your
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podcasts so you never miss an episode. Until next time, keep
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looking up