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Welcome to Astronomy Daily, your latest source of space and
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astronomy news. With your host Anna, Today, we're diving into
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some fascinating topics, ranging from the latest findings about Mars's
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escaping water to the exciting flyby of Mercury by the
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BEPI Columbo mission. We'll also discuss China's ambitious plans with
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g Space's new low Earth orbit satellites, SpaceX's launch of
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next gen spy satellites, and how amateur astronomers are aiding
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the study of Jupiter's weather. Stick around for an engaging
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episode packed with the latest updates and discoveries from the Cosmos.
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Let's start today with a Mars update. NASA's Hubble Space
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Telescope and Maven mission are making significant strides in unlocking
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one of Mars's biggest secrets, what happened to all its water.
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Mars was once a very wet planet, evidenced by its
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surface geological features. Over the past three billion years. Scientists
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suggest that some of this water went underground, but where
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did the rest go? The Hubble and Maven missions have
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combined data to offer answers. There are only two places
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water can go, explains John Clark, Boston University. It can
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freeze into the ground, or the water molecule can break
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into atoms, and the atoms can escape from the top
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of the atmosphere into space. Essentially, Clark's team needs to
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understand how these atoms escape to gauge how much water
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Mars once held. Water molecules in the Martian atmosphere are
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broken apart by sunlight into hydrogen and oxygen atoms. Clark's
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team focused on hydrogen and its heavier cousin, deuterium, which
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has a neutron in its nucleus. Because deuterium is heavier,
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it escapes Mars's atmosphere more slowly than regular hydrogen. By
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measuring the current ratio of deuterium to hydrogen, scientists can
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work backwards to estimate the amount of water Mars used
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to have. What makes this study groundbreaking is the combination
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of data collected over different Martian years. Maven, not sensitive
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enough to detect uterium throughout the Martian year, relied on
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Hubble's data to fill in the gaps, offering a complete picture.
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This holistic approach over years allowed a more dynamic understanding
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of Mars's atmosphere, showing that it is much more turbulent
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and changes more quickly than previously thought. One significant discovery
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is that hydrogen and deuterium escape rates spike dramatically when
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Mars is closest to the Sun. Traditional models had shown
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these atoms slowly diffusing upward, but the new data indicate
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a more rapid and energy intensive process. Collisions with solar
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wind protons and sunlight driven chemical reactions help give these
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atoms the extra kick needed to escape Mars's gravity. Beyond
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understanding Mars, the study offers insights into the evolution of
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planets around other stars, especially Earth like planets and habitable
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zones where liquid water might exist. Mars, Earth, and Venus
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all occupy or very near our Solar System's habitable zone,
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but have vastly different environments today. By studying Mars, we
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gain a better understanding of these distinctions and their implications
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for distant worlds. The Hubble Space Telescope and Maven missions
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have been crucial in this research. Hubble, a joint project
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between NASA and ISA, has been studying the universe for
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over three decades. Meanwhile, Maven, managed by NASA's gold Dottered
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Space Flight Center, is preparing to celebrate its tenth year
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at Mars. Both of these missions underscore the importance of
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international cooperation and long term investments in space exploration. Thanks
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to the efforts of these powerful telescopes and the dedicated
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scientists interpreting their data, we are one step closer to
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understanding not only the history of Mars, but settings more
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applicable universally. Now, let's turn our attention to some groundbreaking
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news from China. Chinese automaker Guile's g space has announced
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an impressive milestone with the launch of ten low Earth
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orbit satellites. This launch is part of their ambitious plan
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to form a global communications mega constellation. Essentially, it's China's
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answer to SpaceX's Starlink, which has already revolutionized the satellite
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communications industry. These ten new satellites were launched from the
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Taiyuan Satellite Launch Center in Shanshi Province, significantly extending the
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capabilities of g Space's constellation. With this batch, the constellation
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now boasts thirty satellites covering ninety percent of the globe
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with twenty four hour communication services. That's a massive achievement
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for g space and marks the first time a Chinese
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commercial aerospace company has offered low Earth orbit satellite communication
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on a global scale. G space was established by Gely
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Technology Group in twenty eighteen. Their mission to research, launch,
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and operate low orbit satellites that can provide global broadband services,
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and they're well on their way. Their initial plan includes
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placing seventy two satellites in orbit by the end of
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twenty twenty five, aiming to serve over two hundred million
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users worldwide. But that's just the beginning. The company plans
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to expand its constellation to nearly six thousand satellites. This
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robust network will be designed to offer global broadband services,
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positioning g space as a strong competitor to starlink. LEO
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satellites typically orbit at altitudes of three hundred to two
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thousand kilometers above the Earth surface. One of their main
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advantages is that they're cheaper and provide more efficient transmission
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compared to those in higher orbits. G Space's deployment strategy
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leverages these benefits, making it a cost effective and scalable
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solution for global communications. G Space's endeavor is part of
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a broader wave of Chinese companies entering the satellite communications space.
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Another notable player is Shanghai spacecom Satellite Technology, which has
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also launched LEO satellites under its thousand sales constellation or
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the G sixty Starlink plan. They have equally ambitious plans,
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aiming to deploy fifteen thousand satellites by twenty thirty. It's
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clear that China is heavily investing in satellite technology to
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ensure they're not left behind in this new space race.
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G Space's latest launch is a significant step forward, not
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just for Giele and g Space, but for the overall
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landscape of global satellite communications. This competitive spirit and rapid
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technological advancement could lead to more affordable and accessible communication
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services worldwide. Speaking of that other satellite communications company, SpaceX,
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is showing no signs of slowan down. On September fifth,
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one of SpaceX's Falcon nine rockets launched from California's Vandenberg
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Space Force Space. This wasn't just any mission. This launch
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sent a new batch of next gen spy satellites into
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orbit for the US National Reconnaissance Office, or NRO. It
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was their eighty sixth orbital mission of the year, underscoring
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just how prolific SpaceX has become in the realm of
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space launches. What's intriguing about this particular operation, known as
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NROL one hundred and thirteen, is that it's part of
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the NRO's new strategy called Proliferated Architecture. This concept involves
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deploying numerous smaller satellites to create a network designed to
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be more capable and resilient than traditional single satellite systems.
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In simple terms, having more satellites in orbit can ensure
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the network remains operational and less vulnerable to threats. SpaceX's
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efforts didn't just end with launching the satellites. The Falcon
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nine booster used in this mission also executed a flawless
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landing About eight point five minutes after liftoff. The booster
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settled back down onto the deck of the SpaceX Drone ship.
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Of course, I still love you, floating in the Pacific Ocean.
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This marks the twentieth time this particular booster has been
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launched and landed, highlighting the reusability goals SpaceX founder Elon
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Musk has championed. Interestingly, this wasn't the only mission SpaceX
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managed that day. Earlier, on September fifth, another Falcon nine
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rocket launched from Florida's Space coast, delivering twenty one starlink
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Internet satellites into orbit. This shows how SpaceX has become
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adept at handling multiple missions almost simultaneously. While the exact
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details of these spy satellites remain classified, as is typical
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with NRO missions, it's clear that they play a critical
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role in national security. The NRO has described prior launches
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in this series as essential to their proliferated architecture strategy,
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and this third launch in the series continues to build
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on that foundation. It's a testament to the growing relationship
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and trust between SpaceX and government agencies for crucial and
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classified missions. Now, let's turn our gaze to Jupiter, with
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its iconic great red spot and swirling, turbulent atmosphere, has
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long fascinated astronomers and space enthusiasts alike. While professional observatories
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and high cost missions like the very large telescope in
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Chile and NASA's Juno orbiter have offered invaluable insights into
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Jupiter's meteorology, they can't monitor the gas giant continuously. This
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is where amateur astronomers armed with relatively affordable telescopes are
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stepping up to the plate. A recent study published in
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Earth and Space Science highlights how amateur astronomers can significantly
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aid in this endeavor. Using equipment costing as little as
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four thousand dollars, These officionados are making sizable contributions to
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our understanding of Jupiter's atmospheric phenomena, especially its cloud formations
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and ammonia distribution. You see, Jupiter's topmost clouds aren't water
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based like Earth's, but are primarily composed of ammonia ice.
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By analyzing the absorption of specific wavelengths of light six
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hundred and forty seven nanometers absorbed by ammonia and six
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hundred and nineteen nanometers absorbed by methane, amateur astronomers can
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determine the abundance of ammonia in different regions of Jupiter's atmosphere.
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Methane levels remain relatively constant and well studied, allowing for
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this comparative technique. Higher absorption at six hundred and forty
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seven nanometers compared to six hundred and nineteen indicates increased
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ammonia content, providing critical clues about Jupiter's intricate weather patterns.
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This simple yet effective method has allowed researchers to observe
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changes in ammonia distribution over various time scales from weeks
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to years. However, more comprehensive data is needed to better
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understand what these fluctuations signify and how they influence Jupiter's
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overall weather system. Amateur astronomers are perfectly positioned to fill
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this gap, and the researchers hope these celestial hobbyists will
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rally around the cause making regular observations. With a larger
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global network of observers, we can capture a much more
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detailed and can continuous picture of Jupiter's atmospheric conditions. This
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would enable weekly or even daily monitoring, a feat that's
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unmanageable with sporadic professional observations alone. By joining forces, citizens,
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scientists and professional astronomers can unlock new levels of understanding,
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helping us unravel the complexities of not just Jupiter, but
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planetary weather systems in general. Whether you're an experienced stargazer
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or a curious newcomer, your contributions could make a meaningful
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difference in space research. So if you've ever pointed a
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telescope at Jupiter and marveled at its grandeur, consider becoming
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part of this significant scientific effort. Whether you capture an
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image of a swirling storm or a fleeting atmospheric anomaly.
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Your work might just change our understanding of the largest
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planet in our Solar System. Now onto Mercury, the BEPY
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Columbo mission completed its fourth and closest fly by yet
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of Mercury, a fascinating event that has offered us brand new,
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unprecedented views of the planet Southpole region. This close encounter
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took place on September fourth, marking a significant milestone in
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the mission's journey toward a comprehensive study of Mercury. A
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joint effort by the European Space Agency ESA and the
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japan Aerospace Exploration Agency jacksa BEPI Colombo whizzed just one
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hundred sixty five kilometers about one hundred three miles from
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the surface of Mercury. Not only did this flyby produce
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stunning photos, but it also played a crucial role in
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adjusting the spacecraft's trajectory to match Mercury's more inclined orbit
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relative to Earth. The primary objective of these flybys is
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to slow down the spacecraft, effectively using Mercury's gravity as
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a break to ease it deeper into the Sun's gravitational
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poll Unlike missions that slingshot pass planets to gain speed,
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BEPI Colombo needs to decelerate to ensure it gets captured
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by Mercury's minuscule gravity. Launched in twenty eighteen and named
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after Italian scientists to set a BEPI Colombo, this mission
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is unique. It consists of two orbiters ISAs Mercury Planetary
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Orbiter and Jackson's Mercury Magnetospheric Orbiter, stacked together aboard the
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Mercury Transfer Module MTM. These orbiters will separate once they're
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inserted into Mercury's orbit in late twenty twenty six to
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commence their primary science mission. The recent flyby was a
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pivotal event for the mission, providing a unique opportunity for
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the scientists involved. Johannes Bankoff Essay's BEPY Columbo project scientists
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emphasized how crucial these flybys are for both navigating the
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spacecraft and preparing for its scientific mission. He noted, we
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get to fly our world class science laboratory through diverse
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and unexplored parts of Mercury's environment that we don't have
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access to once in orbit. Even though the main science
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camera aboard ESA's orbiter remains shielded until final orbit insertion.
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Ten of the spacecraft's sixteen instruments were active during the flyby.
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These instruments collected valuable data on Mercury's particles, plasma, and
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magnetic fields. Additionally, the Japanese orbiters monitoring cameras captured striking
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black and white images of the planet's terrain, including unusual
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double peak ring crater basins. Interestingly, the close encounter was
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made possible due to an issue discovered earlier this year.
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The spacecraft's electric propulsion system wasn't operating at full power
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due to unanticipated current levels between the solar arrays and
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the electrical distribution system. This glitch led the mission controllers
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to plan a closer flyby, thereby also extending the mission
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timeline to late twenty twenty six. Once BEPI Columbo enters
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Mercury's orbit, it aims to transform our understanding of this
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enigmatic planet. The mission will investigate everything from Mercury's internal
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structure and surface geology to its magnetic field and exosphere,
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promising to enrich our knowledge of the smallest and innermost
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planet in our Solar System. BEPI Colombo's journey has been extensive,
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involving one flyby of Earth in twenty twenty, to a
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venus in twenty twenty and twenty twenty one, and now
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four of Mercury, with two more scheduled before final orbital insertion.
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After nearly eight years in space. The mission is poised
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to deliver for groundbreaking science starting in November twenty twenty six.
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Thank you for tuning in to Astronomy Daily with Anna.
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For more space updates, visit our website at Astronomy Daily
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dot io to sign up for our free daily newsletter.
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Sunday Stars starz
237
00:14:52.200 --> 00:14:52.240
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