S03E116: An Invitation from NASA to You!
In this episode
Welcome to another thrilling episode of Astronomy Daily!Join Anna as she takes you on a journey through the latest astronomical discoveries.
In this episode, we explore the groundbreaking findings of NASA's Parker Solar Probe, the discovery of the Earth-sized exoplanet Gliese 12 b, and the rapid formation of organic macromolecules in star-forming regions. Plus, learn how you can virtually engage with Northrop Grumman's upcoming resupply mission to the International Space Station. Don't miss out on these fascinating topics and more!
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Speaker 1: Welcome to Astronomy Daily, your go to podcast for the
Speaker 1: latest updates in space and astronomy. I'm your host, Anna,
Speaker 1: and today's episode is packed with riveting news and discoveries.
Speaker 1: We'll delve into the latest findings from NASA's Parker Solar
Speaker 1: Probe as it unravels the mysteries of the Sun's extreme
Speaker 1: corona heat. Then we'll discuss the discovery of a new
Speaker 1: Earth sized exoplanet, Giza twelve B, that promises thrilling potential
Speaker 1: for future study. We'll also explore how organic macromolecules form
Speaker 1: rapidly in star forming regions, shedding light on the origins
Speaker 1: of life's building blocks. Finally, we'll look at virtual engagement
Speaker 1: opportunities for Northrop Grummans upcoming resupply mission to the International
Speaker 1: Space Station. Let's get started. NASA invites the public to
Speaker 1: engage virtually with Northrop Grummans upcoming twenty first commercial resupply
Speaker 1: mission to the International Space Station, scheduled for August tenth,
Speaker 1: twenty twenty four, at eight thirty one pm EDT. The
Speaker 1: launch will take place from NASA's Wallops Flight Facility on
Speaker 1: Wallops Island, Virginia. The event promises to be a spectacular
Speaker 1: showcase of innovation and collaboration. This mission is particularly special
Speaker 1: because it honors the late NASA astronaut Laurel Clerk, naming
Speaker 1: the signas spacecraft the SS Laurel Clerk in her memory.
Speaker 1: Clark was a mission specialist on the Tragic Space Shuttle
Speaker 1: Columbia's STS one hundred seven mission, and this tribute underscores
Speaker 1: the spirit of exploration and sacrifice that drives space missions.
Speaker 1: Northrop Grumman's Signus spacecraft, carried into orbit by an Antares rocket,
Speaker 1: will deliver over eight thousand, two hundred pounds of science experiments,
Speaker 1: research materials, supplies, and hardware to support the work of
Speaker 1: Expedition sixty nine astronauts aboard the space station. This critical
Speaker 1: mission will help sustain the continuous human presence in Low
Speaker 1: Earth orbit. The Virtual Engagement Program offers a unique opportunity
Speaker 1: for space enthusiasts to be part of this exciting event.
Speaker 1: By registering as a virtual guest, participants will receive curated
Speaker 1: launch resources and notifications about interactive opportunities. As a bonus,
Speaker 1: virtual attendees will receive a commemorative Virtual Guest passport stamp
Speaker 1: post launch, a small token of involvement in this significant milestone.
Speaker 1: Participation in the Virtual Guest Program is free and open
Speaker 1: to the public. This initiative aims to make space exploration
Speaker 1: accessible to everyone, fostering a sense of global community and
Speaker 1: shared curiosity about the universe. By bringing the excitement of
Speaker 1: a live launch into homes around the world, NASA continues
Speaker 1: to inspire the next generation of scientists, engineers, and dreamers.
Speaker 1: As the countdown begins. Don't miss out on being part
Speaker 1: of this momentous occasion. Register now to engage in this
Speaker 1: spectacular virtual experience and witness firsthand the brilliance and dedication
Speaker 1: that propels our journey into space. The Parker Solar Probe
Speaker 1: has made groundbreaking town discoveries about the Sun's corona, challenging
Speaker 1: long held beliefs and opening new avenues for understanding solar dynamics. Traditionally,
Speaker 1: scientists suggested that s shaped magnetic field bends or switchbacks,
Speaker 1: contributed to the extreme heat of the corona. These switchbacks,
Speaker 1: observed in the solar wind, were thought to be the
Speaker 1: source of the Sun's outer atmospheres immense temperatures, which can
Speaker 1: be up to two hundred times hotter than its surface. However,
Speaker 1: the Parker Solar Probe's recent findings have turned this theory
Speaker 1: on its head. As it ventured closer to the Sun,
Speaker 1: the probe observed that while these magnetic switchbacks are common
Speaker 1: in the solar wind near the Sun, they are notably
Speaker 1: absent in the corona itself. This suggests that these bends
Speaker 1: are not the culprits behind the corona's scorching heat. So
Speaker 1: if switchbacks aren't responsible, what is the Absence of these
Speaker 1: magnetic bends in the corona hints at the existence of other,
Speaker 1: yet to be discovered mechanisms that could be driving the
Speaker 1: heating process. This discovery has set the state for further
Speaker 1: research to unveil what exactly causes the Sun's outer atmosphere
Speaker 1: to defy the laws of physics. As the Parker Solar
Speaker 1: Probe continues its mission, it aims to collect more data,
Speaker 1: especially during its upcoming trips closer to the Sun. These
Speaker 1: future observations will help scientists test new hypotheses and potentially
Speaker 1: identify other phenomena that could explain the corona's extreme temperatures.
Speaker 1: This ongoing research is crucial because understanding the corona is
Speaker 1: essential for comprehending solar wind space weather and their impacts
Speaker 1: on our solar system. This revelation from the Parker Solar
Speaker 1: Probe underscores the importance of continual exploration and data collection
Speaker 1: in unraveling the mysteries of our solar system. Each new
Speaker 1: discovery not only demystifies the Sun's behavior, but also brings
Speaker 1: us a step closer to predicting and mitigating the effects
Speaker 1: of solar activities on Earth. In an exciting breakthrough for
Speaker 1: astronomy and the search for extraterrestrials life, scientists have announced
Speaker 1: the discovery of Gliza twelve B, a temperate Earth sized
Speaker 1: exoplanet situated just forty light years away. This might sound
Speaker 1: like a great distance, but in terms of the cosmos,
Speaker 1: it's a mere stones throwaway. A relatively neighborly three hundred
Speaker 1: and seventy eight trillion kilometers Gleasi twelve B was discovered
Speaker 1: by an international team of researchers, including key players from
Speaker 1: McGill University and Western University. This effort was part of
Speaker 1: the Infrared Doppler Subaru Strategic Program, which focuses on finding
Speaker 1: planets within the habitable zones of red dwarf stars. Red
Speaker 1: dwarfs are smaller cooler and more abundant compared to stars
Speaker 1: like our Sun, making them prime candidates in the ongoing
Speaker 1: quest to find life beyond Earth. The planet orbits its
Speaker 1: host star, Gliza twelve, which is a red dwarf. Unlike
Speaker 1: more active red dwarfs that exhibit frequent and intense stellar
Speaker 1: flares potentially harmful to any orbiting planets, Gliza twelve is
Speaker 1: unusually inactive. This translates to less harmful radiation, creating a
Speaker 1: more stable environment for Gleisa twelve B, thereby increasing the
Speaker 1: planet's chances of being habitable. What makes Glesa twelve bee
Speaker 1: particularly intriguing is its location within the star's habitable zone,
Speaker 1: often referred to as the Goldilocks zone. This is the
Speaker 1: region around a star where conditions are just right for
Speaker 1: liquid water to exist on a planet's surface, neither too
Speaker 1: hot nor too cold. Given that water is essential for
Speaker 1: life as we know it, this discovery is a significant
Speaker 1: step forward in the search for potentially habitable worlds, although
Speaker 1: more observations and modeling are needed to confirm the presence
Speaker 1: of liquid water or any biosignatures. The planet's earth like
Speaker 1: size and location within this habitable zone make it a
Speaker 1: tantalizing subject for further study. Indeed, Gleisa twelve bee's proximity
Speaker 1: allows for detailed analysis of its atmosphere and other characteristics.
Speaker 1: One particularly useful method for studying such planets is atmospheric
Speaker 1: transmission spectroscopy. This technique involves examining the starlight that passes
Speaker 1: through a planet's atmosphere during transit. By analyzing the changes
Speaker 1: in the lights spectra, scientists can infer the atmospheric composition,
Speaker 1: looking for gases like oxygen, water, vapor, methane, and carbon dioxide.
Speaker 1: The presence of these gases could indicate biological processes. The
Speaker 1: discovery of GLESA twelve B is thrilling not just for
Speaker 1: its immediate scientific implications, but also for its potential to
Speaker 1: deepen our understanding of what makes a planet habitable. Future telescopes,
Speaker 1: including the James Web Space Telescope and ground based extremely
Speaker 1: large telescopes, will be instrumental in studying the planet's atmosphere
Speaker 1: and surface conditions more thoroughly. As we continue to explore
Speaker 1: the cosmos, each new discovery like Glisa twelve B brings
Speaker 1: us one step closer to answering the age old question
Speaker 1: are we alone in the universe. For now, Gleisa twelve
Speaker 1: B stands as a beacon of hope and curiosity, inviting
Speaker 1: us to learn more more about the possibilities that lie
Speaker 1: beyond our own solar system. In a fascinating discovery, an
Speaker 1: international team of researchers led by scientists from the Netherlands
Speaker 1: has shed light on how organic macromolecules form in the
Speaker 1: disks of gas and dust enveloping young stars. By employing
Speaker 1: observation based computer models, the team uncovered that dust traps,
Speaker 1: which are regions where dust and ice accumulate, can play
Speaker 1: a pivotal role in this process. These dust traps are
Speaker 1: not stationary. Instead, they exhibit vertical movement, constantly cycling material
Speaker 1: within the young stars disc When these dust particles, laden
Speaker 1: with simple ices are exposed to intense starlight, they undergo
Speaker 1: significant chemical transformations. The researchers found that this irradiation triggers
Speaker 1: the formation of complex organic molecules up to hundreds of
Speaker 1: atoms in size, akin to substances like soot and graphene.
Speaker 1: What's truly remarkable is the speed at which this process occurs.
Speaker 1: Under optimal conditions, macromolecules can form within just a few decades.
Speaker 1: This rapid formation provides a new perspective on how the
Speaker 1: building blocks of life could develop in star forming regions,
Speaker 1: suggesting that the ingredients for life might be much more
Speaker 1: common in the universe than previously thought. The studies model,
Speaker 1: grounded in a combination of laboratory research and observational data,
Speaker 1: demonstrates that the heavy irradiation from stellar light in these
Speaker 1: dust traps can effectively kickstart the creation of large, complex molecules.
Speaker 1: This new understanding enriches our knowledge of the chemical processes
Speaker 1: at work in protoplanetary disks and offers insights into the
Speaker 1: early stages of planetary system formation. One of the leading
Speaker 1: voices in this research, Neil's Legterink, highlighted the importance of
Speaker 1: considering the effects of intense radiation on complex chemical processes. Traditionally,
Speaker 1: scientists have focused on smaller organic molecules, but this study
Speaker 1: underscores the significance of larger macromolecules in the composition of chondrites,
Speaker 1: the primitive meteorites rich in organic compounds. Ninke Van der Morel,
Speaker 1: another co author, voiced her enthusiasm for the study, drawing
Speaker 1: attention to the unique intersection of astrochemistry observational astronomy, laboratory work,
Speaker 1: and the study of meteorites. This interdisciplinary approach has allowed
Speaker 1: researchers to develop a comprehensive model explaining how large organic
Speaker 1: molecules can form under certain conditions in young star systems.
Speaker 1: Going forward, the research team aims to explore how different
Speaker 1: types of dust traps respond to varying levels of radiation
Speaker 1: and dust motion. This line of investigation will help scientists
Speaker 1: better understand the potential for life around different types of
Speaker 1: stars and exoplanets, broadening our grasp of where and how
Speaker 1: life could arise in the universe. This discovery not only
Speaker 1: enhances our comprehension of the origin of macromolecules crucial for life,
Speaker 1: but also opens up new avenues for studying the early
Speaker 1: chemical environs of emerging planetary systems. It adds another piece
Speaker 1: to the intricate puzzle of how life's building blocks are
Speaker 1: assembled in the cosmos. Thank you for tuning in to
Speaker 1: this episode of Astronomy Daily. I'm anna and it was
Speaker 1: a pleasure to bring you the latest in astronomical discoveries.
Speaker 1: Don't forget to visit our website at Astronomy Daily dot io,
Speaker 1: where you can sign up for our free daily newsletter.
Speaker 1: Catch up on all the latest space and astronomy news
Speaker 1: with our constantly updating news feed, and listen to all
Speaker 1: our back episodes. You can also find us on social media.
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