Aug. 3, 2026
Unleashing a Wandering Black Hole and Chasing the Solar Eclipse
SpaceTime Series 29 Episode 92 The monster that’s been let out of its cage Astronomers have for the first time discovered a monstrous supermassive black hole wandering unseen near the edge of a galaxy. Counting down to next week’s solar eclipse Spain, Portugal, Iceland, Greenland Russia and the arctic are about to experience a total solar eclipse as the Moon’s shadow sweeps across the surface of the Earth. The Swift Space Telescope rescue mission suffers a major setback NASA’s Link mission to save the Swift Space Telescope has suffered a few problems with a sudden loss of attitude control putting the spacecraft into an uncontrollable spin. The Science Report Former Biden administration chief health advisor Anthony Fauci pleads the fifth on everything. Antimicrobial resistance in children on the rise globally. The footprints of an ancient civilisation discovered in the Amazon. Discovery of fossils of a giant mosasaur eating an ichthyosaur that ate a pterosaur. Skeptics guide to the 2026 Bent Spoon Awards. This Week’s Guests NASA WB-57 pilot Tom Parent NASA WB-57 Sensor Equipment Operator Cary Klemm Nation Wide Eclipse Ballooning Project Principal Investigator Dr Angela Des Jardins from Montana State University. Juno Principal Investigator Scott Bolton Southwest Research Institute in San Antonio Texas Juno Launch Director Omar Baez NASA Juno Mission Manager John Calvert NASA Our regular guests: Alex Zaharov-Reutt from techadvice.life Tim Mendham from Australian Skeptics And Senior science writer and Sky and Telescope magazine contributor Jonathan Nally 🌏 Get Our Exclusive NordVPN deal here ➼ www.bitesz.com/nordvpn . The discounts and bonuses are incredible! And it’s risk-free with Nord’s 30-day money-back guarantee! ✌
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The Astronomy, Space, Technology & Science News Podcast.
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This is Spacetime Series twenty nine, Episode ninety two, for
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broadcast on the third of August twenty twenty six. Coming
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up on Spacetime, The Monster That's been let out of
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its cage, counting down to next week's solar eclipse, and
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a major setback for NASA Swift Space Telescope Rescue mission.
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All that and more coming up on space Time.
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Welcome to space Time with Stuart Gary.
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Astronomers have for the first time discovered a monster as
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super massive black hole wandering alone near the edge of
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a galaxy. These giants of the universe, which can be
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millions to billions of times the mass of our Sun,
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are usually found at the centers of galaxies, are reporting.
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The Astrophysical journal Letters claims the newly identified behemoth was
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only discovered as a released a flash of light while
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destroying and consuming a nearby star in a tidal disruption event.
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It's the first time scientists have detected a super massive
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black hole so far away from a galaxy center. The
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studies lead author, Robert david Stein from the Joint Space
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Science Institute, says the new discovery will have huge implications.
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Until now, the assumption was that super massive black holes
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always reside at the centers of their galaxies. The new
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discovery means astronomers will be able to better understand how
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galaxies and their black holes merge and how they build
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up over time. Theorists have predicted that wandering black holes
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would exist roaming along the outskirts of galaxies as a
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result of galaxy collisions and mergers. But the thing is,
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many of these black holes would be quiescent, meaning they're
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not swallowing material and consequently not emitting any light, literally
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tiptoeing around the universe undetected. This newly discovered black hole
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was detected by this Vicki transient facility, which searches the
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skies looking for transient objects. Vicki scans the entire northern
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sky every two days using a pair of telescopes at
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the Palomar Observatory in San Diego. Mind you, it's virtually
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impossible to check for black holes in each of the
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hundreds of thousands of celestial events at Ziki documents every evening.
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So astronomers developed an artificial intelligence program which identifies a
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characteristic light signature that occurs when the black hole shreds
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a star. These title disruption events are well documented at
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galaxy centers, but the AI looked for similar flares elsewhere
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in the sky. The authors launched the artificial intelligence program
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back in August twenty twenty five, and made their first
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black hole discovery using it just three months later. In
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this case, the super massive black hole was located some
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thirty thousand light years from the galactic center. It's around
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four million solar masses, about the same as set us
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a star. The super massive black hole at the center
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of our own galaxy, the Milky Way. It likely ended
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up at its current location following a collision between two galaxies.
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One possibility is that a larger galaxy cannibalized a smaller
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one and then slowly stripped away all its stars until
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only the core remained. But a more intriguing second possibility
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is that one galaxy already had two black holes orbiting
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close to the center in a binary system, having already
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merged with another galaxy. Then if a third black hole
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from yet another galaxy merger enters the mixed complex, three
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body interactions could kick the smallest one out. Continued observations
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of this title disruption event but eventually favor one of
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these two hypotheses. Characterizing how quiesce and black holes behave
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is important because most black holes, including the one at
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the center of the Milky Way, are dormant for most
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of the time. In other words, you only know they're
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there when they start feeding. The authors in asking the
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Skies for more wandering black holes so they can determine
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just how common they really are. This is space time
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still to come, counting down to next week's solar eclipse
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and a major setback for NASA Swift Space Telescope Rescue mission.
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All that and more still to come on space Time. Spain, Portugal, Greenland, Iceland, Russia,
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and the Arctic are about to experience a total solar
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eclipse as the Moon's shadow sweeps across the surface of
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the Earth. Other parts of Europe, from the British Isles
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and France across to Greece, Italy and Lithuania, as well
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as northern Africa, will experience a partial eclipse during the event.
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Depending on where you are, the celestial spectacular will begin
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around three point thirty four in the afternoon of August
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the twurth, with totality occurring at five four and the
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show ending just before eight o'clock in the evening Solar
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eclipses happen when the Moon passes directly between the Earth
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and the Sun. You see, the Moon's orbit around the
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Earth is inclined by five degrees compared to the Earth's
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orbit around the Sun, so normally the Moon appears to
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cross the sky slightly above or below the path of
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the Sun. But about every eighteen months or so, the
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lunar orbit places the Moon directly between the Sun and Earth,
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resulting in a solar eclipse. Eclipses happen because the Moon
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is four hundred times smaller than the Sun, but it's
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also four hundred times closer to the Earth, and so
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the two appear to be about the same size in
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the sky as seen from Earth, and when the Sun, Moon,
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and Earth line up exactly, the Earth experiences a total
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solar eclipse. As this occurs, the Moon begins to slowly
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pass in front of the Sun and the partial lunar
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shadow or penumber, crosses the surface of the Earth. This
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can last for more than an hour as more and
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more of the Sun is hidden by the face of
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the Moon. Then, just before totality occurs, the crescent Sun
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converges into a single, bright white diamond of sunlight as
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the last bit of the Sun's bright disk shines along
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the edge of the Moon, and the first glimpses of
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the fake corona create a ring around the Moon, an
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effect known as the diamond ring. In the last fleeting
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moments before totality, the diamond ring breaks up into a
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string of beads created by the Sun's rays shining through
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the low lying valleys between the mountains along the limb
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or edge of the Moon. Once this effect, known as
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Bailey's beads, comes to an end, the Moon has completely
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covered the entire disk of the Sun and ear in totality.
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During totality, the largest part of the Moon's shadow, the umbra,
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crosses the Earth's surface. People along the path of totality
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view a total eclipse, which can last up to seven
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minutes and thirty one seconds, but is usually far shorter.
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During this period, the sky goes down, stars will appear,
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and it will suddenly get noticeably cooler. Birds will start roosting,
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shadows will take on an unusual crescent shape, and you'll
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be able to see the Sun's tenuous outer atmosphere, The corona,
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glowing milky white. Often explosions on the Sun's surface, called prominences,
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will appear as spectacular bright pink or red clouds stretching
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above the lunar limb. The path of totality can be
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up to two hundred and seventy two kilometers wide, although
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it's usually a lot less, and the further away you
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are from the center of the path, the shorter the
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eclipse duration will be. Now, if you're outside the line
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of totality, either to the north or south of it,
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you'll only see a partial eclipse, in which only part
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of the Sun's disk will be covered by the Moon.
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The reason each eclipse is only visible over a small
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part of the Earth is because the Moon's shadow is
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relatively small when it falls on the Earth's surface. Now,
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another important factor is that, on average, the Moon orbits
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about three hundred and eighty four thy four hundred kilometers
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away from the Earth. But the Moon's orbit around the
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Earth is in a perfect circle, it's slightly elliptical. That
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means one part of the orbit may be a bit
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closer to the Earth, maybe three hundred and fifty seven
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thousand kilometers that's known as perigy. Well, another part of
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the orbit will be a bit further away, around four
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hundred and six thousand kilometers, known as apergy, and when
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the Moon's orbit takes it a bit further away, the
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Moon looks a bit smaller in the sky, and if
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that coincides with the solar eclipse, it doesn't cover the
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entire face of the Sun, so instead of a solar eclipse,
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the Moon's passage across the Sun creates an annulus, a
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ring of fire, as light from the Sun surrounds the
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dark Moon, resulting in an annular eclipse. Solar eclipses are
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accompanied by a lunar eclipse, occurring either two weeks before
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or after the main event. That's due to the same
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alignment which caused the solar eclipse, so lunar and solar
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eclipses occur with equal frequency, but lunar eclipses are seen
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over a far broader area because the Earth's shadow is
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far larger and therefore covers more of the lunar surface.
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A lunar eclipseccurs during full moon, when the Sun, Earth,
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and Moon a line. During this event, the Moon passes
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completely through the Earth's dark shadow or umbra. Even though
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the Earth completely blocks out sunlight from directly reaching the
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surface of the Moon.
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The Moon is still visible.
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During a total lunar eclipse, you'll see the Moon gradually
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get darker than take on a rusty or blood red
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color as the light from the Sun refracts through Earth's
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atmosphere and undergoes rarely scattering, leaving only the longer red
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wavelengths as all the Earth's sunsets and sunrises happen at
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once to indirectly reflect on the lunar surface. A total
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lunar eclipse and also look yellow, orange, or even browning
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color depending on how different types of dust, particles, and
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clouds in Earth's atmosphere allow different wavelengths of light to
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reach the lunar surface. During next week's event, science teams
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will be chasing the Moon's shadow with one of NASA's
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high altitude WB fifty seven research jets and with scientific balloons.
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They'll investigate the Sun's dynamics the temporary darkening of our
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skies affects the atmosphere. A squeed of four cameras mounted
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in the nosecone will take high resolution images of the
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Sun's corona in different wavelengths of visible and infrared light.
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The cameras will capture at least twenty images per second.
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Recording structures, outflows, and rapid changes in the corona during
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the total eclipse. These images will allow scientists to learn
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more about the formation of prominences, better understand the corona
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and how it gets heated to nearly a million degrees,
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and the relationship between material and the corona and in
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the Solar wind, a continuous stream of charged particles flowing
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out from the Sun and bathing the Earth and rest
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of the Solar System. By chasing the Moon's shadow, the
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jet will extend how long cameras can observe the corona.
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See On the ground, the longest anyone will be able
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to see the corona is two minutes in eighteen seconds,
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but by flying along the eclipse path of totality, the
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WB fifty seven's view of the corona can last nearly
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three minutes. NASS WB fifty seven will flight fifty thousand
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feet that's above any clouds that might obscure the view
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of the Krona from the ground. The altitude will also
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allow cameras to observe some of the infrared wavelengths that
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get absorbed by the lower atmosphere before reaching the ground.
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The crone has only been observed at those wavelengths a
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few times before. The key instrument is called a multi
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spectral able in imager. It was developed by the Southwest
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Research Institooting Boulder, Colorado, and was also used during the
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April twenty twenty four solar eclipse, where it provided valuable
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observations this report from MESSATV.
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For most people, a total solar eclipse lasts just a
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few minutes, but NASA's pilots find a way to make
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it last longer by trying to outrun the Moon's shadow
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with an airplane.
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The truth is it's actually chasing us. We get out
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in front of it and let it overtake us. Once
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we're in totality, then we'll advance to artles to max
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and try and stay in totality for as long as
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we can.
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Making that happen takes extreme precision. Scientists calculate exactly where
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the airplane needs to be at each moment.
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We do a lot of missions where being in the
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right point and time and space are critical, and this
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is one of them.
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On eclipse Day, the WB fifty seven aircraft climbs more
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than fifty thousand feet into the stratosphere that's above most
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of Earth's atmosphere where clouds, dust, and water vapor could
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obscure the view.
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Viewing an eclipse from fifty thousand feet provides a really
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clear shot of the Sun, and that allows the scientists
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to have confidence of the data that they're seeing is
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on the Sun rather than distortions from the atmosphere.
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When the Moon's shadow arrives, it engulfs the aircraft.
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It's weird. Right where you're at is dark, but everywhere
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you see is twilight, and the temperature of the cockpit drops,
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so it's very noticeable.
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As the eclipse unfolds. The pilot keeps the aircraft on
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course while the sensor operator fine tunes the cameras, capturing
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every second of data.
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You're very, very, very busy, and it's very high pressure
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because of course there's no du overse. You only get
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one opportunity to get all these instruments trained on the
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rate spot.
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For the aircraft crew, it's a chance to witness one
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of nature's most spectacular events while helping scientists better understand
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our son.
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I'm sitting in the best seat in the house. It's
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pretty excited.
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And in that report from Massa TV, we heard from
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WB fifty seven Parlot, Tom Parnett, and WB fifty seven
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censor equipment operator carry CLAM. Meanwhile, a NASA funded nationwide
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eclipse ballooning project by Angelo de Jardines from Montana State
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University will be sending students from several American universities to
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Iceland and Spain to launch scientific balloons before, during, and
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after the eclipse in order to better understand how an
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eclipse affects the atmosphere. In Iceland, two teams will launch
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eighty balloons starting eighteen hours before the eclipse until eight
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