S03E194: Black Holes' Dark Energy Dance, Neutron Star's Speed Record, and Mars' Green Mystery
In this episode
Astronomy Daily - The Podcast: S03E194Welcome to Astronomy Daily, your Daily source for the latest space and Astronomy news. I'm Anna, and today we have a stellar lineup of stories that will take you from the depths of black holes to the surface of Mars.
Highlights:
- Black Holes and Dark Energy: Discover groundbreaking research suggesting that black holes might hold the key to understanding dark energy, a force that constitutes 70% of our universe and drives its accelerating expansion.
- Fastest Spinning Neutron Star: Researchers at DTU Space have identified one of the fastest spinning neutron stars ever observed in our galaxy, spinning at an astonishing 716 times per second, offering insights into the life cycles of binary star systems.
- NASA's Solar Observatory Mission: NASA is set to launch Codex, an innovative solar coronagraph, to the International Space Station, aiming to unlock the mysteries of the solar wind and improve space weather predictions.
- Lunar Water Mapping Mission: NASA's Lunar Trailblazer mission is gearing up to map water on the Moon, potentially revolutionizing future lunar exploration by providing detailed insights into the Moon's water resources.
- Planet-Forming Disks Around Brown Dwarfs: The James Webb Space Telescope has confirmed the existence of planet-forming disks around brown dwarfs in the Orion Nebula, challenging previous planetary formation theories.
- Perseverance Rover's Martian Discovery: NASA's Perseverance rover has discovered intriguing green patches on the Martian surface, hinting at the Red Planet's potentially water-rich past.
For more cosmic news, visit our website at astronomydaily.io. Sign up for our free Daily newsletter and explore sponsor links for great deals. Catch up on all our previous episodes and join our celestial community on social media. Find us as #AstroDailyPod on Facebook, X, YouTubeMusic, Tumblr, and TikTok. Share your thoughts and connect with fellow space enthusiasts.
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.
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Speaker 1: Welcome to Astronomy Daily, your daily dose of space and
Speaker 1: astronomy news. I'm Anna, and we've got an absolutely packed
Speaker 1: show for you today, filled with groundbreaking discoveries from across
Speaker 1: the Cosmos. We'll be diving into fascinating new research that
Speaker 1: suggests black holes might hold the key to understanding dark energy,
Speaker 1: and we'll explore an incredible discovery of one of the
Speaker 1: fastest spinning neutron stars ever observed in our galaxy. We'll
Speaker 1: also look at NASA's innovative new Solar observatory headed to
Speaker 1: the International Space Station and discuss the upcoming mission to
Speaker 1: map water on the Moon. But that's not all. We've
Speaker 1: got some exciting findings from the James Web Space Telescope
Speaker 1: about planet forming disks around failed stars, and we'll wrap
Speaker 1: up with the latest intriguing discovery from the Perseverance Rover
Speaker 1: on Mars. So stick around as we journey through today's
Speaker 1: biggest space in astronomy stories. Our universe is a mysterious place,
Speaker 1: and one of its biggest puzzles has always been what
Speaker 1: exactly makes up most of it? Would you believe that
Speaker 1: everything we can see, see and touch, all the stars, planets, galaxies,
Speaker 1: and even US only accounts for about five percent of
Speaker 1: the universe. Scientists have long wondered about the other ninety
Speaker 1: five percent, and now they might be onto something big
Speaker 1: involving black holes. Of all things, A wopping seventy percent
Speaker 1: of our universe is made up of something called dark energy,
Speaker 1: a force that's driving the universe's accelerating expansion. It's been
Speaker 1: doing this since the Cosmos began its inflation thirteen point
Speaker 1: eight billion years ago. The remaining twenty five percent is
Speaker 1: dark matter, which we can only detect through its gravitational
Speaker 1: effects on galaxies. Now, researchers think black holes might help
Speaker 1: us understand how dark energy works. As Gregory Tarrel from
Speaker 1: the University of Michigan explains, black holes are the only
Speaker 1: places in today's universe where gravity is as strong as
Speaker 1: it was at the beginning of time. His team suggests
Speaker 1: that when massive stars collapse into black holes, they might
Speaker 1: actually be converting matter back into dark energy, like a
Speaker 1: cosmic recycling program running in reverse. This theory is getting
Speaker 1: support from observations made by the Dark Energy Spectroscopic Instrument,
Speaker 1: or DC, which uses five thousand robotic eyes to study
Speaker 1: the Cosmos. The team found that as new black holes
Speaker 1: form from dying stars, the amount of dark energy in
Speaker 1: the universe increases in a corresponding way. It's like watching
Speaker 1: two sides of the same cosmic equation balance out. What
Speaker 1: makes this discovery particularly exciting is that it's no longer
Speaker 1: just theoretical. Scientists can now actually test these ideas through
Speaker 1: observations watching how black holes might be coupling with and
Speaker 1: growing alongside our expanding universe. They're studying tens of millions
Speaker 1: of distant galaxies to track how fast the universe is
Speaker 1: expanding at different points in its history, giving us new
Speaker 1: insights into how dark energy changes over time. Whether or
Speaker 1: not black holes turn out to be the source of
Speaker 1: dark energy, this research is pushing us closer to understanding
Speaker 1: one of the universe's most fundamental mystery, and that's what
Speaker 1: makes astronomy so fascinating. Just when we think we've got
Speaker 1: things figured out, the cosmos throws us another curveball to unravel.
Speaker 1: Next on the agenda today, in an exciting breakthrough from
Speaker 1: the world of astronomy, researchers at DTU Space have discovered
Speaker 1: one of the fastest spinning objects ever observed in our
Speaker 1: Milky Way using an X ray telescope mounted on the
Speaker 1: International Space Station. They've identified a neutron star that's spinning
Speaker 1: at the mind boggling speed of seven hundred and sixteen
Speaker 1: times per second. This remarkable celestial object is part of
Speaker 1: what we call an X ray binary star system, located
Speaker 1: in the Sagittarius constellation near our galaxies center known as
Speaker 1: four U eighteen twenty to thirty. This system is giving
Speaker 1: us an unprecedented look at one of the universe's most
Speaker 1: extreme phenomena. To put this discovery in perspective, let's talk
Speaker 1: about what we're actually looking at. This neutron star is
Speaker 1: incredibly small, only about twelve kilometers in diameter, but don't
Speaker 1: let its size fool you. It packs up mass one
Speaker 1: point four times that of our Sun into that tiny space.
Speaker 1: Sitting about twenty six thousand light years from Earth. The
Speaker 1: light we're seeing from it has been traveling toward us
Speaker 1: for twenty six thousand years. What makes this system even
Speaker 1: more fascinating is its companion star, a white dwarf about
Speaker 1: the size of Earth. This pair performs an incredibly fast
Speaker 1: orbital dance, with the white dwarf completing its orbit around
Speaker 1: the neutron star every eleven minutes. That's the shortest orbital
Speaker 1: period we've ever seen in systems like this. The gravitational
Speaker 1: forces at play here are intense. The neutron Star's powerful
Speaker 1: gravity pulls material from its companion, building up on its
Speaker 1: surface until it triggers violent thermonuclear bursts. These explosions release
Speaker 1: energy comparable to an atomic bomb and can make the
Speaker 1: neutron stars shine up to one hundred thousand times brighter
Speaker 1: than our Sun. This discovery isn't just about breaking speed records.
Speaker 1: It's providing us with valuable insights into the life cycles
Speaker 1: of binary star systems and how elements form in our universe.
Speaker 1: It's another piece in the puzzle of understanding these fascinating
Speaker 1: cosmic objects that push the boundaries of physics as we
Speaker 1: know it. Next up in groundbreaking news for solar research,
Speaker 1: NASA is preparing to launch an innovative new instrument called
Speaker 1: Codex to the International Space Station next November. This cutting
Speaker 1: edge solar coronagraph will give us unprecedented views of our
Speaker 1: Sun's outer atmosphere and help unlock the mysteries of the
Speaker 1: solar wind. What makes CODEX special is its unique ability
Speaker 1: to not just observe the Sun's corona, but to measure
Speaker 1: both the temperature and speed of the solar wind as
Speaker 1: it forms. Previous coronagraphs could only capture images of plasma density,
Speaker 1: but Codex's special filters will provide a much more complete
Speaker 1: picture of how the solar wind evolves from its berth
Speaker 1: at the Sun's surface. The timing couldn't be better for
Speaker 1: this mission, as the Sun is currently at its solar maximum,
Speaker 1: a period of peak activity in its eleven year cycle.
Speaker 1: This means CODEX will be able to study different types
Speaker 1: of solar wind that are only present during this active phase,
Speaker 1: including fascinating blobs of hot plasma that form when magnetic
Speaker 1: field loops open up and release their contents into space.
Speaker 1: One of the key mysteries CODEX aims to solve is
Speaker 1: why the solar wind reaches such extreme temperatures about one
Speaker 1: point eight million degrees fahrenheit, which is remarkably one hundred
Speaker 1: and seventy five times hotter than the Sun's surface. It
Speaker 1: will also study how this superheated plasma accelerates to speeds
Speaker 1: of nearly a million miles per hour as it streams
Speaker 1: outward from the Sun. This mission builds on years of research,
Speaker 1: including ground based experiments during solar eclipses and high altitude
Speaker 1: balloon tests. Now, by placing Codex on the space station,
Speaker 1: scientists can finally observe the Sun's corona without interference from
Speaker 1: Earth's atmosphere, giving us our clearest view yet of these
Speaker 1: fundamental solar processes. Understanding how the solar wind forms and
Speaker 1: evolves is crucial for predicting space weather conditions that can
Speaker 1: affect everything from satellites to power grids here on Earth.
Speaker 1: Just as meteorologists need to understand atmospheric conditions to forecast hurricanes,
Speaker 1: space weather forecasters need to understand the environment through which
Speaker 1: solar storms travel. Codex will provide vital data to help
Speaker 1: improve these predictions and protect our technology dependent society. Now
Speaker 1: moving on to another mystery that's about to become one
Speaker 1: step closer to being answered. NASA's ambitious Lunar Trailblazer mission
Speaker 1: is gearing up to solve one of the Moon's most
Speaker 1: intriguing mysteries, the presence and behavior of water on our
Speaker 1: celestial neighbor. While scientists have long suspected water exists on
Speaker 1: the Moon, we still have many questions about where exactly
Speaker 1: it is, what form it takes, and how it moves
Speaker 1: across the lunar surface. Set to launch next year, this
Speaker 1: compact but powerful satellite will orbit just sixty miles above
Speaker 1: the lunar surface, creating the most detailed maps ever of
Speaker 1: lunar water distribution. Using two sophisticated instruments, the High resolution
Speaker 1: Volatile Aisles and Minerals Moon Mapper and the Lunar Thermal Mapper,
Speaker 1: it will track not just where water exists, but also
Speaker 1: its abundance, chemical composition, and how it changes over time.
Speaker 1: This mission could be revolutionary for future lunar exploration. Understanding
Speaker 1: the Moon's water resources could help establish sustainable human presence
Speaker 1: on the lunar surface, as water can be processed into
Speaker 1: breathable oxygen and even rocket fuel. But beyond practical applications,
Speaker 1: the data could also reveal fascinating details about the Moon's history,
Speaker 1: much like how ice cores on Earth tell us about
Speaker 1: our planets past. The mission will investigate whether lunar water
Speaker 1: stays locked in minerals or migrates across the surface in
Speaker 1: daily cycles, potentially forming frost in extremely cold regions before
Speaker 1: evaporating and redepositing elsewhere. This could help us understand similar
Speaker 1: processes on other airless bodies throughout our Solar system. For
Speaker 1: scientists like Bethany Alman, the mission's principal investigator, these findings
Speaker 1: could even provide clues about Earth's own water origin story.
Speaker 1: By analyzing the chemical composition of lunar ice, particularly in
Speaker 1: permanently shadowed craters, researchers might finally determine whether the Moon's
Speaker 1: water arrived via comet impacts or emerge during its volcanic past.
Speaker 1: Speaking of space mysteries, in an exciting new discovery, the
Speaker 1: James Webb Space Telescope has confirmed for the first time
Speaker 1: that planet forming disks exist around brown dwarfs in the
Speaker 1: Orion Nebula. These fascinating objects, often called failed stars, appear
Speaker 1: to have the same potential for planetary formation as their
Speaker 1: larger stellar cousins. Located just one thousand, five hundred light
Speaker 1: years from Earth, the orion Nebula has proven to be
Speaker 1: the perfect laboratory for this groundbreaking research. Using web's superior
Speaker 1: infrared capabilities, astronomers have identified at least twenty brown dwarfs
Speaker 1: surrounded by protoplanetary disks, the same kind of structures that
Speaker 1: give birth to planets around normal stars. The smallest of
Speaker 1: these newly discovered objects is truly remarkable, measuring at just
Speaker 1: five times the mass of Jupiter. That's a mere fraction
Speaker 1: of our Sun's mass, yet it still maintains its own
Speaker 1: disc of gas and dust. Two other objects were found
Speaker 1: right at the boundary between brown dwarfs and proper stars,
Speaker 1: with masses about three quarters that of our Sun, making
Speaker 1: their exact classification a fascinating puzzle for astronomers. This discovery
Speaker 1: challenges our previous understanding of how planetary systems might form.
Speaker 1: These flattened clouds of gas and dust surrounding brown dwarfs
Speaker 1: suggest that even these cosmic underdogs might have the potential
Speaker 1: to form their own family of planets, despite never achieving
Speaker 1: true stardom through nuclear fusion. The findings open up exciting
Speaker 1: new possibilities for planetary formation theories and suggests that planetary
Speaker 1: systems might be even more common in our galaxy than
Speaker 1: previously thought. With hundreds more potential Brown dwarfs in the
Speaker 1: Orion nebula weigh to be studied, Webb's continued observations could
Speaker 1: reveal even more surprises about these mysterious objects and their
Speaker 1: potential role as planet hosts. Now Let's head over to
Speaker 1: Mars for an update and yet another intriguing discovery. As
Speaker 1: NASA's Perseverance rover approaches its fourth year exploring the Martian surface,
Speaker 1: it continues to make fascinating fines. The latest comes from
Speaker 1: a nighttime image taken at a location called Serpentine Rapids,
Speaker 1: where the rover has spotted something unexpected, patches of green
Speaker 1: coloring within the red Martian rocks. Using its Sherlock Watson camera,
Speaker 1: Perseverance captured these intriguing features while examining an abrasian patch
Speaker 1: in a rock formation known as Wallace Butte. The green spot,
Speaker 1: measuring about two millimeters across, stands out dramatically against the
Speaker 1: rust colored Martian landscape. What makes this discovery particularly interesting
Speaker 1: is that similar features on Earth typically form when liquid
Speaker 1: water seeps through sediment before it hardens into rock. The
Speaker 1: process triggers a chemical reaction that transforms oxidized iron, the
Speaker 1: same compound that gives Mars its distinctive red color, into
Speaker 1: its reduced form, creating these greenish hues. While microbes can
Speaker 1: play a role in this process, on Earth, the green
Speaker 1: coloring could also result from decaying organic matter or chemical
Speaker 1: interactions between sulfur and iron. Unfortunately, due to the challenging
Speaker 1: positioning of the spot, Perseverance wasn't able to conduct a
Speaker 1: detailed analysis with its sophisticated instruments. As the rover prepares
Speaker 1: for its next adventure, ascending the steep terrain of Jesuro
Speaker 1: Crater's rim before leaving the area it is called home
Speaker 1: for two years, this discovery adds another piece to the
Speaker 1: puzzle of Mars's potentially water rich past. These green spots
Speaker 1: might be telling us an important story about the red
Speaker 1: planet's ancient environmental conditions and its potential for having once
Speaker 1: harbored life. And that wraps up today fascinating journey through space.
Speaker 1: I'm Anna, and we've covered some incredible stories today, from
Speaker 1: the mysterious connection between black holes and dark energy, to
Speaker 1: a record breaking neutron star, exciting developments and solar studies,
Speaker 1: lunar exploration, and those intriguing green spots on Mars discovered
Speaker 1: by Perseverance. If you'd like to dive deeper into any
Speaker 1: of these stories or stay up to date with the
Speaker 1: latest developments in space and astronomy, head over to Astronomy
Speaker 1: Daily dot io. There you can sign up for our
Speaker 1: free daily newsletter. And access our constantly updating news feed.
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