S03E144: BepiColombo's Mercury Flyby, China's Sea-Based Launch, and Artemis 4G Revolution
In this episode
Astronomy Daily - The Podcast: 3rd September 2024Welcome to Astronomy Daily, your go-to Podcast for all the latest news in the world of space and Astronomy. I'm Anna, your host for today. We've got some exciting stories lined up for you, from NASA's Artemis III mission to the latest updates on the BepiColombo spacecraft and more. So stay tuned for some incredible space news and insights.
Highlights:
- BepiColombo's Fourth Mercury Flyby: The joint mission by the European Space Agency and Japan Aerospace Exploration Agency (JAXA) is gearing up for its fourth Mercury flyby. Scheduled for 23:48 CEST (21:48 UTC) on September 4, BepiColombo will pass just 165 km above Mercury's surface. This flyby is crucial for adjusting the spacecraft's speed and trajectory, and it offers scientists a valuable opportunity to gather preliminary data and fine-tune onboard instruments. Despite challenges with its electric thrusters, the mission remains on track, with 10 of the 16 scientific instruments operational during this flyby. Expect the first images to be released on September 5, with initial scientific results to follow on September 13.
- China's Sea-Based Satellite Launch: Galactic Energy, a private rocket manufacturer based in Beijing, has achieved its third sea-based launch of the Series One carrier rocket, marking China's 12th successful sea-based satellite launch. The rocket deployed six satellites into a sun-synchronous orbit approximately 535 km above Earth, showcasing the reliability and effectiveness of their technology. This successful launch highlights China's growing prowess in space exploration and satellite deployment.
- Artemis III Mission and 4G Connectivity: NASA's upcoming Artemis III mission will break new ground by equipping astronauts with cutting-edge 4G connectivity designed by Nokia. This technology will allow lunar explorers to broadcast high-definition video and transmit large volumes of scientific data back to Earth in real-time. The 4G network will be tested later this year with Intuitive Machines' IM-2 mission, and the technology could benefit future lunar missions and various lunar devices.
- The Mystery of Lunar Swirls: Visible through even basic telescopes, lunar swirls have long puzzled scientists. Recent studies suggest that these light-colored swirls are the result of magnetized rocks that create a magnetic field strong enough to deflect solar wind particles. Understanding the origin of these swirls could reveal more about the Moon's geological history and its ancient magnetic environment. NASA plans to send a rover to the famous Reiner Gamma swirl in 2025 as part of the Lunar Vertex mission to gather more data.
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Speaker 1: Welcome to Astronomy Daily, your go to podcast for all
Speaker 1: the latest news in the world of space and astronomy.
Speaker 2: Him Anna your host for today.
Speaker 1: We've got some exciting stories lined up for you, from
Speaker 1: NASA's Artemis three mission, to the latest updates on the
Speaker 1: BEPY Columbo spacecraft and more. First, we'll dive into the
Speaker 1: latest maneuver by the BEPI Columbo mission as it prepares
Speaker 1: for its fourth flyby of Mercury. We'll also explore China's
Speaker 1: impressive twelfth successful sea based satellite launch, a significant milestone
Speaker 1: in space exploration. Later, we'll talk about how the Artemis
Speaker 1: three mission will leverage cutting edge four G technology designed
Speaker 1: by Nokia to revolutionize lunar communication. Finally, we'll unravel the
Speaker 1: mystery behind the enigmatic lunar swirls, shedding light on new
Speaker 1: scientific findings about these fascinating features on the Moon's surface.
Speaker 2: So stay tuned for some incredible space news and insights.
Speaker 1: First up today, the BEPI Columbo mission, a joint effort
Speaker 1: by the European Space Agency ESA and the japan Aerospace
Speaker 1: Exploration Agency JACKSA, is gearing up for its fourth Mercury flyby.
Speaker 1: This is not just another flyby, but a pivotal moment
Speaker 1: in the mission's journey. Scheduled for twenty three forty eight
Speaker 1: CESST twenty one forty eight UTC on September fourth, BEPI
Speaker 1: Colombo will pass just one hundred and sixty five kilometers
Speaker 1: above Mercury surface, getting closer than ever before. Why is
Speaker 1: this fly by so crucial, Well, it serves a dual purpose. First,
Speaker 1: it will help adjust the spacecraft's speed and trajectory, essential
Speaker 1: for eventually settling into orbit around Mercury. Second, it offers
Speaker 1: a valuable opportunity for scientists to gather preliminary data and
Speaker 1: fine tune the operations of the onboard instruments before the
Speaker 1: main mission begins. Initially launched in October twenty eighteen, BEPI
Speaker 1: Columbo utilizes a series of nine planetary flybys to aid
Speaker 1: its journey, one around Earth, two around Venus, and six
Speaker 1: around Mercury. The mission's complexity stems from Mercury's close proximity
Speaker 1: to the Sun, which demands intricate maneuvers to counter the
Speaker 1: Sun's powerful gravitational pull and the spacecraft's own high velocity. Interestingly,
Speaker 1: the upcoming flyby wasn't solely routine. Engineers had to overcome
Speaker 1: a challenge that emerged back in April twenty twenty four
Speaker 1: when BEPI Colombo's Mercury Transfer Module MTM encountered an issue
Speaker 1: with its electric thrusters. These thrusters, essential for the spacecraft's journey,
Speaker 1: have been operating below the required thrust due to unexpected
Speaker 1: electric currents affecting the power distribution from the solar arrays.
Speaker 1: After months of grueling investigations, a workaround was devised. ESA's
Speaker 1: flight dynamics team created a new trajectory, ensuring the spacecraft
Speaker 1: stays on mission despite reduced thrust. This shows the resilience
Speaker 1: and ingenuity of the mission team, emphasizing that space exploration
Speaker 1: is as much about overcoming unexpected roadblocks as it is
Speaker 1: about discovery. The fourth flyby, set to occur soon, is
Speaker 1: expected to bring the spacecraft within just one hundred and
Speaker 1: sixty five kilometers of Mercury's surface, about thirty five kilometers
Speaker 1: closer than originally planned. This closer approach will further reduce
Speaker 1: the propulsion needed for the next two Mercury flybys in
Speaker 1: December twenty twenty four and January twenty twenty five, which
Speaker 1: are crucial for aligning bepy Colombo's orbit with Mercury. What's
Speaker 1: exciting is that although the mtm's primary thrusters are underperforming,
Speaker 1: the mission scientific objectives remain unaffected. Ten of the sixteen
Speaker 1: scientific instruments on board will be operational during this flyby.
Speaker 1: These instruments will collect data on magnetic fields, plasma, and particles,
Speaker 1: offering a preview of the detailed science to come once
Speaker 1: BEPY Columbo settles into orbit around Mercury. Johannesbenkoff, BEPY Columbo's
Speaker 1: project scientist, couldn't contain his excitement. He pointed out that
Speaker 1: this fly by allows us to explore parts of Mercury's
Speaker 1: environment that wouldn't be accessible once the spacecraft is in orbit.
Speaker 1: This is a chance to gather unique data and ensure
Speaker 1: a smooth transition when the main mission begins. Moreover, BEPY
Speaker 1: Columbo's trio of monitoring cameras mcams will capture images of Mercury.
Speaker 1: While these cameras were designed to monitor the spacecraft's equipment,
Speaker 1: they also provide black and white snapshots of the planet
Speaker 1: as the spacecraft zooms past Mercury. MCAM two and MCAM
Speaker 1: three will start capturing well lit images two minutes after
Speaker 1: the closest approach, giving us unprecedented views of Mercury's terrain.
Speaker 1: There's an extra bit of excitement surrounding this fly by,
Speaker 1: as it marks the first time Bepy Colombo will pass
Speaker 1: over Mercury's poles. This maneuver is essential for adjusting the
Speaker 1: spacecraft's trajectory to match Mercury's inclined orbit relative to Earth.
Speaker 1: Scientists are particularly eager to get a glimpse of Mercury's
Speaker 1: south pole through the captured images. All of these thrilling
Speaker 1: developments make Bepy Columbo's fourth fly by a cornerstone in
Speaker 1: its journey. With new data, images and a fine tuned trajectory,
Speaker 1: the mission is not just on track, but poised to
Speaker 1: deepen our understanding of Mercury and its place in our
Speaker 1: Solar system. Expect the first images to be released on
Speaker 1: September fifth, and the initial scientific results to follow on
Speaker 1: September thirteenth. Stay tuned as we bring you more updates
Speaker 1: on this incredible mission, pushing the boundaries of what we
Speaker 1: know about our closes planetary neighbor. Next up in today's
Speaker 1: story list, Galactic Energy, a private rocket manufacturer based in
Speaker 1: Beijing has achieved its third sea based launch of the
Speaker 1: Series one carrier rocket, marking China's twelfth successful sea based
Speaker 1: satellite launch overall. This is a significant milestone for Galactic Energy,
Speaker 1: cementing its position as a leading private entity in the
Speaker 1: Chinese space industry. On Thursday afternoon, the Series one rocket
Speaker 1: blasted off from a mobile launch platform, which was essentially
Speaker 1: a modified deck barge positioned in the Yellow Sea off
Speaker 1: the eastern province of Shandong. The launch was a success,
Speaker 1: and the rocket deployed six satellites into a sun synchronous
Speaker 1: orbit approximately five hundred and thirty five kilometers above the Earth.
Speaker 1: The newly deployed satellites come from multiple operators and serve
Speaker 1: various functions. They are set to collect crucial meteorological data,
Speaker 1: demonstrate advanced optical remote sensing technologies, and gather hyper spectral
Speaker 1: remote sensing data. These capabilities are expected to provide valuable
Speaker 1: information for both scientific research and practical applications such as
Speaker 1: weather forecasting and environmental monitoring. So far, Galactic Energy has
Speaker 1: conducted fifteen orbital launches with the Series one model, outpacing
Speaker 1: other private competitors in China. These missions have successfully placed
Speaker 1: a total of fifty four commercial satellites into orbit, showcasing
Speaker 1: the reliability and effectiveness of their technology. The Series one
Speaker 1: rocket itself stands about twenty meters tall with a diameter
Speaker 1: of one point four meters, and it primarily uses solid propellant.
Speaker 1: With a lift off weight of thirty three metric tons,
Speaker 1: the rocket is capable of sending a three hundred kilogram
Speaker 1: satellite or several satellites with a combined weight of three
Speaker 1: hundred kilograms into a five hundred kilometer Sun synchronous orbit. Alternatively,
Speaker 1: it can deliver payloads of up to three hundred and
Speaker 1: fifty kilograms into a low Earth orbit at an altitude
Speaker 1: of two hundred kilometers. This successful launch not only highlights
Speaker 1: the capabilities of galactic energy, but also underscores China's growing
Speaker 1: prowess in space exploration and satellite deployment. The use of
Speaker 1: sea based launches offers unique advantages, including increased launch flexibility
Speaker 1: and reduced risk to populated areas. Now let's get an
Speaker 1: Artemis update. NASA's upcoming Artemis three mission is set to
Speaker 1: break new ground not just by landing astronauts on the
Speaker 1: Moon again, but by equipping them with cutting edge communications technology.
Speaker 1: The space suits these astronauts will wear won't just be
Speaker 1: your regular space attire. They'll come with four G connectivity
Speaker 1: designed by none other than Nokia. Imagine this lunar explorer
Speaker 1: is broadcasting high definition video or transmitting large volumes of
Speaker 1: scientific data back to Earth in real time. It's a
Speaker 1: huge leap forward from the traditional UHF radio communications that
Speaker 1: passed missions relied on. Nokia's innovation essentially miniaturizes a mobile
Speaker 1: network tower into a box that can fit onto a
Speaker 1: lunar lander. This compressed base station will allow the astronauts
Speaker 1: to stay connected up to two kilometers away from the lander,
Speaker 1: a considerable range when you think about it. On Earth,
Speaker 1: a network of based towers dotted landscapes to keep us connected,
Speaker 1: but on the Moon we only need this compact system,
Speaker 1: demonstrating how scalable and adaptable our technology has become now.
Speaker 1: The Aximu space suits, crafted by Axiom Space won't have
Speaker 1: a touchscreen interface like the smartphones we're all accustomed to. Instead,
Speaker 1: the suits will integrate components of a smartphone customized for
Speaker 1: the space environment. What they'll gain from this integration is remarkable,
Speaker 1: including the ability to stream high definition video or send
Speaker 1: substantial scientific data back to the base station, which will
Speaker 1: then relay it to Earth.
Speaker 2: Traditionally, UHF radio.
Speaker 1: Has been the go to technology for astronauts during their
Speaker 1: lunar missions. While UHF has served well, it pales in
Speaker 1: comparison to the higher bandwidth and faster speeds offered by
Speaker 1: four G. Nokia has been working on this technology for
Speaker 1: space application since receiving a fourteen point one million dollars
Speaker 1: NASA grant back in twenty twenty. The company envisions of
Speaker 1: future where four G connectivity will benefit not just Artemis
Speaker 1: three astronauts, but potentially all future lunar missions. In fact,
Speaker 1: the first test of this lunar four G network will
Speaker 1: occur later this year with Intuitive Machines IM two mission.
Speaker 1: This mission will carry the base station, while two other payloads,
Speaker 1: the map rover and the Micronovadrone, will have four G receivers.
Speaker 1: Beyond the Artemis three mission, Nokia s's potential applications for
Speaker 1: this technology in various lunar devices. Think of a lunar
Speaker 1: terrain vehicle equipped with four G connectivity, or even smaller
Speaker 1: science experiments and sensors linking through this network. Throughout twenty
Speaker 1: twenty four and into twenty twenty five, the four G
Speaker 1: equipped suits will go through rigorous testing, everything from vacuum
Speaker 1: chambers to simulations in the indoor pool at NASA's Johnson
Speaker 1: Space Center. These tests aim to ensure that both the
Speaker 1: suits and their components can withstand the extreme conditions they'll
Speaker 1: face during life on the Moon. This technological leap doesn't
Speaker 1: just make communication easier, it opens the door for more
Speaker 1: advanced scientific exploration and data collection. It's an exciting time
Speaker 1: for SpaceX exploration as we blend the advancements made in
Speaker 1: consumer technology with the rigors of space travel. The Artemis
Speaker 1: three mission, with its four G connectivity, is certainly one
Speaker 1: to watch as we prepare for humanity's next giant leap
Speaker 1: on the lunar surface. Let's explore a truly fascinating topic,
Speaker 1: the mysterious light colored swirls on the Moon's surface.
Speaker 2: Visible through even the.
Speaker 1: Most basic backyard telescopes, These lunar swirls have long puzzled scientists.
Speaker 1: Some say these swirls resemble the brushstrokes in an abstract painting,
Speaker 1: but they are far from mere artistic flourishes. NASA's images
Speaker 1: show that These intricate patterns can extend for hundreds of miles.
Speaker 1: So what's behind these captivating formations. Recent studies suggest that
Speaker 1: lunar swirls are the result of magnetized rocks. These rocks
Speaker 1: create a magnetic field strong enough to deflect solar wind
Speaker 1: particles which bombard the Moon continuously. While nearby areas darken
Speaker 1: over time due to chemical reactions caused by these solar winds,
Speaker 1: the swirls maintain their lighter appearance because they are protected
Speaker 1: by their magnetic fields. This brings us to a crucial question,
Speaker 1: how did the rocks in these swirls become magnetized? After all,
Speaker 1: the Moon no longer has a global magnetic field. Recent
Speaker 1: modeling and spacecraft data have started to unravel this mystery.
Speaker 1: One popular theory is that these magnetic anomalies were caused
Speaker 1: by impacts, or possibly by subterranean lava with high titanium
Speaker 1: content cooling down in the presence of an ancient magnetic field.
Speaker 1: Assistant Professor Michael J. Krutchinsky from Washington University believes that
Speaker 1: localized magma could be the real culprit. His recent experiments,
Speaker 1: co designed with pH d graduate Yuan Yuan Liang, tested
Speaker 1: whether lunar light conditions could magnetize materials like ilmanite, a
Speaker 1: mineral abundant on the Moon. They concluded that high surface
Speaker 1: area to volume ratio in ilmanite grains could indeed create
Speaker 1: the necessary magnetic fields.
Speaker 2: These theories have significant implications.
Speaker 1: Understanding the origin of lunar swirls could help scientists piece
Speaker 1: together the historical magnetic environment of the Moon, revealing more
Speaker 1: about its geological history and even the broader surface effects
Speaker 1: experienced by other planets and moons.
Speaker 2: Looking ahead, NASA.
Speaker 1: Intends to send a rover to one of the most
Speaker 1: famous lunar swirls, Reiner Gamma, in twenty twenty five, as
Speaker 1: part of the Lunar Vertex mission. This mission aims to
Speaker 1: gather more data and possibly provide direct evidence of the
Speaker 1: processes behind these enigmatic patterns. Thus, while the mystery of
Speaker 1: lunar swirls has yet to be completely solved, ongoing research
Speaker 1: and upcoming missions are set to offer invaluable insights. For now,
Speaker 1: the study of these swirls continues to excite the scientific community,
Speaker 1: bridging the gap between remote observations and hands on lunar exploration.
Speaker 1: And that's all for today's episode of Astronomy Daily. Thanks
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