Stellar Measurements, Icy Moon Missions, and Meteorite Ownership Dilemmas: S04E23
In this episode
Astronomy Daily - The Podcast: S04E23In this episode of Astronomy Daily, host Anna delves into a series of remarkable advancements in space science, covering everything from the universe's expansion rate to innovative concepts for lunar habitats. Join us as we explore the latest findings that are reshaping our understanding of the cosmos.
Highlights:
- Hubble and James Webb Collaboration: Discover how combined observations from the Hubble and James Webb Space Telescopes have refined the measurement of the universe's expansion rate, known as the Hubble constant, to approximately 72.6 kilometers per second per megaparsec.
- Arctic Ocean as an Enceladus Testbed: Learn about scientists using Earth's Arctic Ocean to simulate conditions on Saturn's moon Enceladus, searching for chemical signatures that could indicate extraterrestrial life.
- Changes in M87 Black Hole: Get insights into the evolving dynamics of the M87 black hole, including the movement of its luminous ring, which reveals critical information about its orientation and surrounding environment.
- Meteorite Ownership Debate: Explore the fascinating and complex world of meteorite ownership, as recent discoveries spark discussions about the balance between private collectors and scientific research.
- NASA's PUNCH Mission: Follow the progress of NASA's PUNCH mission, which aims to study the sun's outer atmosphere using a fleet of four compact satellites, enhancing our understanding of solar wind dynamics.
- Visionary Concepts from NASA: Discover NASA's NIAC program's groundbreaking proposals for 2025, including innovative ideas for lunar habitats made from lunar glass and advanced propulsion systems for deep space exploration.
For more cosmic updates, visit our website at astronomydaily.io. Join our community on social media by searching for #AstroDailyPod on Facebook, X, YouTubeMusic, Tumblr, and TikTok. Share your thoughts and connect with fellow space enthusiasts. 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.
00:00 - Astronomy Daily brings you the latest in space and astronomy news
00:50 - Hubble and James Webb refine the Hubble constant
03:20 - Arctic Ocean used to simulate Enceladus conditions
06:15 - M87 black hole shows signs of change
09:30 - Meteorite ownership and the debate over scientific access
12:20 - NASA's PUNCH mission prepares for launch
15:00 - Innovative concepts from NASA's NIAC program for 2025
✍️ Episode References
NASA
[NASA](https://www.nasa.gov)
Hubble Space Telescope
[HST](https://hubblesite.org)
James Webb Space Telescope
[JWST](https://www.jwst.nasa.gov)
Event Horizon Telescope
[EHT](https://eventhorizontelescope.org)
Astronomy Daily
[Astronomy Daily](https://www.astronomydaily.io)
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Speaker 1: Welcome to Astronomy Daily, your daily dose of space and
Speaker 1: astronomy news. I'm your host, Anna, and today we'll explore
Speaker 1: some fascinating developments in space science. From black holes to meteorites,
Speaker 1: and from lunar glass homes to groundbreaking NASA missions. A
Speaker 1: lot to cover, so let's get started. In an exciting
Speaker 1: development for our understanding of the cosmos, scientists have made
Speaker 1: significant progress in measuring the universe's expansion rate thanks to
Speaker 1: combined observations from both the Hubble and James Webb Space telescopes.
Speaker 1: These latest findings are helping to fine tune one of
Speaker 1: astronomy's most crucial measurements, the Hubble constant. The Hubble constant
Speaker 1: tells us how fast galaxies are moving away from each
Speaker 1: other as the universe expans. Think of it as the
Speaker 1: cosmic speedometer of our universe. Recent analysis from the James
Speaker 1: Webb Space Telescope has validated earlier calculations made by Hubble,
Speaker 1: providing even more precise measurements. When the research team combined
Speaker 1: all measurements from both telescopes, they found the Hubble constant
Speaker 1: to be approximately seventy two point six kilometers per second
Speaker 1: per megaparsec. This means that for every megaparsec, roughly three
Speaker 1: point two six million light years, galaxies are moving away
Speaker 1: from each other at about seventy two point six kilometers
Speaker 1: per second. This conformation is particularly significant because it helps
Speaker 1: address what scientists call the Hubble tension, a long standing
Speaker 1: disagreement between different methods of measuring the universe's expansion rate.
Speaker 1: The new data from James Web provides independent verification of
Speaker 1: Hubble's observations, giving astronomers more confidence in their understanding of
Speaker 1: this fundamental cosmic property. The team used several techniques to
Speaker 1: reach these conclusions, including studying special types of stars called
Speaker 1: Cepheid variables and explosive events known as type one A supernovae.
Speaker 1: These cosmic phenomena act like standard candles, allowing astronomers to
Speaker 1: measure vast distances across space with remarkable precision. Next up today,
Speaker 1: in one of the most intriguing quests for extraterrestrial life,
Speaker 1: scientists are turning to Earth's Arctic Ocean as a testing
Speaker 1: ground for future missions to Saturn's moon, Enceladus. This icy
Speaker 1: moon has captured the imagination of astrobiologists worldwide since the
Speaker 1: Cassini mission discovered its subsurface ocean and active geysers erupting
Speaker 1: from its south pole. The Arctic ocean serves as an
Speaker 1: excellent analog for Ensilatus's conditions, with its ice covered surface
Speaker 1: and underwater hydrothermal vents. Scientists are collecting water and ice
Speaker 1: samples searching for telltale chemical signatures like methane and hydrogen
Speaker 1: that could indicate biological activity. These same chemical markers could
Speaker 1: potentially reveal life on Enceladus. When Cassini sampled Enceladus's plumes
Speaker 1: back in two thousand and four, it detected water, ice, methane,
Speaker 1: and various carbon based molecules. The spacecraft also found molecular
Speaker 1: hydrogen and nitrogen, all the basic ingredients needed for life
Speaker 1: as we know it. The Moon's ice crust, estimated to
Speaker 1: be anywhere from a few to forty kilometers thick, conceals
Speaker 1: a global ocean that could potentially harbor life. What makes
Speaker 1: Enceladus particularly promising are its hydrothermal vents, similar to those
Speaker 1: found in Earth's oceans. These vents could provide the energy
Speaker 1: necessary to support entire ecosystems, just as they do in
Speaker 1: our planet's deepest waters. The research team has successfully demonstrated
Speaker 1: that they can detect and measure various chemical compounds in
Speaker 1: Arctic waters using the same technology planned for future Enceladus missions.
Speaker 1: These Arctic trials are crucial for perfecting the techniques and
Speaker 1: instruments that will one day explore Enceladus's mysterious ocean. By
Speaker 1: practicing here on Earth, scientists can refine their methods and
Speaker 1: ensure they're ready to detect any potential biosignatures when we
Speaker 1: finally send a dedicated mission to this fascinating Saturnian moon.
Speaker 1: And In other news, in a groundbreaking development, the Event
Speaker 1: Horizon telescope team has revealed that M eighty seven in Star,
Speaker 1: the first black hole ever photographed, is showing remarkable signs
Speaker 1: of change. The latest analysis, combining data from twenty seventeen
Speaker 1: and twenty eighteen observations, gives us an unprecedented look at
Speaker 1: how these cosmic giants evolve over time. The most striking
Speaker 1: change is in the black hole's luminous ring. While the
Speaker 1: ring's diameter remains consistent at about forty three micro arc seconds,
Speaker 1: exactly what we'd expect from a black hole weighing six
Speaker 1: point five billion solar masses, its brightest region has shifted
Speaker 1: by thirty degrees counterclockwise. This movement isn't random, It's exactly
Speaker 1: what theoretical models predicted, caused by turbulence in the hot
Speaker 1: gas swirling around the black hole. Perhaps even more fascinating
Speaker 1: is what these observations tell us about M eighty seven
Speaker 1: stars orientation. The fact that the ring consistently appears brightest
Speaker 1: on its bottom side confirms that the black hole's rotational
Speaker 1: axis is tilted away from Earth. This persistent feature helps
Speaker 1: scientists better understand the three dimensional structure of the environment
Speaker 1: around this massive cosmic object. Think of it like watching
Speaker 1: clouds move around a mountain peak while the mountain itself
Speaker 1: stays the same. The changing patterns of clouds can tell
Speaker 1: us about wind directions and atmospheric conditions. Similarly, these subtle
Speaker 1: changes in M eighty seven stars appearance reveal crucial information
Speaker 1: about how matter behaves in the most extreme environments in
Speaker 1: our universe. The EHT team isn't stopping here. They're already
Speaker 1: analyzing data from twenty twenty one and twenty twenty two,
Speaker 1: working toward their ultimate goal creating the first ever time
Speaker 1: lapse video of a black hole. This ongoing monitoring of
Speaker 1: m eighty seven Star promises to revolutionize our understanding of
Speaker 1: these cosmic giants and the fundamental physics that governs our universe. Okay,
Speaker 1: here are some statistics that may stagger you. Every day,
Speaker 1: Earth receives about forty eight point five tons of visitors
Speaker 1: from space in the form of meteorites. While most of
Speaker 1: these as cosmic rocks disappear into our oceans never to
Speaker 1: be found, the ones that land on solid ground often
Speaker 1: spark fascinating debates about who has the right to keep them.
Speaker 1: The meteorite hunting business has evolved into a lucrative global enterprise,
Speaker 1: with space rocks being traded online and shipped between countries
Speaker 1: like precious commodities. While these celestial souvenirs captivate collectors, they're
Speaker 1: also invaluable to scientists studying the mysteries of our universe. Unfortunately,
Speaker 1: many significant specimens are being lost to private collections, potentially
Speaker 1: depriving researchers of crucial data. Take New Zealand's recent Tacopo
Speaker 1: meteorite discovery, for example. This apple sized space rock, weighing
Speaker 1: eight hundred and ten grams, sparked an interesting legal discussion
Speaker 1: about ownership rights. While it was found on public land,
Speaker 1: the citizen science group that discovered it became its legal
Speaker 1: owner under the finders keeper's principle. Fortunately, they chose to
Speaker 1: donate it for scientific study. Not all cases are so straightforward.
Speaker 1: Entries handle meteorite ownership in vastly different ways. Some nations
Speaker 1: allow private ownership, while others mandate state ownership without compensation.
Speaker 1: When meteorites land on private property, they typically belong to
Speaker 1: the landowner, but public land findings can get complicated, leading
Speaker 1: to various legal interpretations and disputes. The commercial value of
Speaker 1: meteorites has skyrocketed, with some specimens fetching millions of dollars.
Speaker 1: High profile collectors, including celebrities and tech entrepreneurs, have helped
Speaker 1: turn meteorite collecting into a glamorous hobby. This has led
Speaker 1: some countries to implement strict regulations on meteorite exports, recognizing
Speaker 1: these space rocks as protected objects of scientific and cultural significance.
Speaker 1: These regulations aim to balance private collection rights with scientific needs.
Speaker 1: But as the market value of meteorites continues to rise,
Speaker 1: the tension between collectors and researchers grows. It raises an
Speaker 1: important question, should we prioritize scientific study over private ownership
Speaker 1: when it comes to these ancient messengers from space. NASA's
Speaker 1: latest mission to study our Sun is making exciting progress
Speaker 1: as four compact satellites part of the PUNCH mission have
Speaker 1: arrived at their launch site in California. These specialized satellites
Speaker 1: will work together like pieces of a puzzle to study
Speaker 1: something we've never fully understood, how the Sun's outer atmosphere
Speaker 1: transforms into the solar wind that flows through our solar system.
Speaker 1: The mission, whose full name is the Polarimeter to Unify
Speaker 1: the Corona and Heliosphere, isn't traveling alone. It's hitching a
Speaker 1: ride on a SpaceX Falcon nine rocket alongside another fascinating
Speaker 1: piece of technology, the SPHEREx space telescope. The launch is
Speaker 1: scheduled for the end of February from Vandenberg Space Force Space.
Speaker 1: What makes PUNCH particularly interesting is its innovative approach. Instead
Speaker 1: of using one large satellite, it employs four smaller ones,
Speaker 1: each about the size of a suitcase. These satellites will
Speaker 1: work in perfect harmony, combining their views to create a
Speaker 1: comprehensive map of the region where the Sun's corona transitions
Speaker 1: into solar wind. Think of it like having four cameras
Speaker 1: positioned around a sports field, each capturing a different angle
Speaker 1: to give viewers the complete picture. The satellites are currently
Speaker 1: undergoing their final preparations at Astrotech Space Operations teams are
Speaker 1: meticulously testing every component, particularly the solar arrays that will
Speaker 1: power each satellite. These tests are crucial to ensure everything
Speaker 1: functions perfectly once they're in space, as there won't be
Speaker 1: any opportunity for repairs after launch. This mission represents a
Speaker 1: significant step forward in our understanding of solar physics. By
Speaker 1: studying how the Sun's atmosphere becomes solar wind, scientists hope
Speaker 1: to better predict space weather events that can affect our satellites,
Speaker 1: power grids, and communication systems here on Earth. It's another
Speaker 1: example of how studying the Cosmos isn't just about satisfying
Speaker 1: our curiosity. It's about protecting our technological infrastructure and better
Speaker 1: understand our place in the Solar System. Finally, today, let's
Speaker 1: take a look into NASA's Crystal Ball. NASA's NIAC program
Speaker 1: has just unveiled its visionary concepts for twenty twenty five,
Speaker 1: and they're pushing the boundaries of what we thought possible
Speaker 1: in space exploration with a substantial investment of two point
Speaker 1: six two five million dollars in grants, NASA is backing
Speaker 1: fifteen groundbreaking ideas that could revolutionize how we explore and
Speaker 1: inhabit space. One of the most intriguing concepts comes from
Speaker 1: Holicity Space in Pasadena, where they're developing what they call
Speaker 1: the Holicity Drive, a compact fusion propulsion system. Imagine spacecraft
Speaker 1: powered by the same process that fuels our Sun, enabling
Speaker 1: faster and more efficient exploration of our Solar system and beyond.
Speaker 1: This technology could be a game changer for future Mars
Speaker 1: missions and deep space exploration. Another fascinating proposal focuses on
Speaker 1: building homes on the Moon, but not the way you
Speaker 1: might expect. Scientists at Skyports have pose creating large scale
Speaker 1: habitats made entirely from lunar glass. This innovative approach, nicknamed lungs,
Speaker 1: involves melting lunar materials to create massive spherical structures. It's
Speaker 1: a perfect example of in situ resource utilization, using what's
Speaker 1: already available on the Moon rather than shipping building materials
Speaker 1: from Earth. For those interested in the search for extraterrestrial life,
Speaker 1: there's an exciting robot concept called leap designed specifically for
Speaker 1: exploring Saturn's moon Enceladus. These jumping robots would hop between
Speaker 1: the moon's famous geysers, collecting samples of ocean derived materials
Speaker 1: shot into space through these icy jets. Other selected projects
Speaker 1: include everything from new ways to explore Venus using electrolysis
Speaker 1: to advanced propulsion systems for sustainable aviation. There's even a
Speaker 1: proposal for using fungi to grow space habitats and developing
Speaker 1: inflatable star shades for studying distant exoplanets. These concepts might
Speaker 1: sound like science fiction, but they represent serious scientific endeavors
Speaker 1: that could shape the future of space exploration. While they're
Speaker 1: all still in early development stages and aren't official NASA
Speaker 1: missions yet, they demonstrate the incredible creativity and innovation driving
Speaker 1: our journey to the stars. Just remember where you heard
Speaker 1: about them first. Thank you for joining me today on
Speaker 1: Astronomy Daily. I'm Anna, and I hope you've enjoyed exploring
Speaker 1: these fascinating developments in space science with me. For more
Speaker 1: astronomical discoveries in space exploration news, visit us at Astronomy
Speaker 1: Daily dot io, where you can sign up for our
Speaker 1: free daily newsletter and catch up on all the latest
Speaker 1: developments with our constantly updating news feed. You'll also find
Speaker 1: all our previous episodes there. Connect with us on social
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