May 3, 2026
Milky Way's Black Hole Secrets, Solar Flare Spectacles, and Mars Rover Discoveries
SpaceTime Series 29 Episode 53 *Milky Way's mysterious black hole gas clouds finally explained Astronomers have discovered a massive binary star system near Sagittarius A* the supermassive black hole at the centre of our Milky Way Galaxy.. *Two massive solar flares explode out from the Sun The Sun has just emitted two strong solar flares blasting out into deep space within a day of each other. *NASA’s rovers show the two sides of Mars NASA’s Mars Curiosity and Perseverance Rovers have provided astronomers with two very different views helping to piece together the puzzle of the Red Planet’s past.. *The Science Report Warning a mega El Niño event is expected to develop within the next month or so. Some of the earliest octopus were enormous, powerful kraken like predators 20 metres long. Scientists have uncovered how Australia's iconic Twelve Apostles were formed. Skeptics guide to the British big foot sighting. 🌏 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! ✌ If you’d like to support the podcast and gain access to bonus content by becoming a SpaceTime crew member, you can do just that through premium versions on Patreon, Spotify and Apple Podcasts. Details on the Support page on our website https://www.bitesz.com/show/spacetime/support/
The Astronomy, Space, Technology & Science News Podcast.
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This is Spacetime Series twenty nine, Episode fifty three were
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broadcast on the fourth of May twenty twenty six. Coming
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up on Space Time, the Milky Ways, mysterious black hole
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gas clouds finally explained, two massive solar flares explode out
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of the Sun, and NASA's Mars rovers show the two
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sides of the Red planet. All that and more Coming
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up on space.
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Time Welcome to space Time with Stewart Gary.
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Astronomers have discovered a massive binary star system, the Sagittarius
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A star the super massive black hole at the center
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of our Milky Way galaxy. The findings, reported in the
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journal Astronomy in Astrophysics, suggested the star system may be
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responsible for a series of mysterious gas clouds which have
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been observed feeding in two Sagittarius A star, the center
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of our Milky Weight galaxy, is a remarkably dense and
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dynamic region. At its heart, some twenty seven thousand light
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years away, lies the super massive black hole Sagittarius A star,
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which has some four point three million times the mass
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of our Sun. Most, if not all, galaxies are thought
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to have supermassive black holes at their centers. These are
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the monsters which hold the galaxy together and provide the
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pivot point for their rotation. Sagittarius A Star is surrounded
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by stars, gas and dust moving under extreme gravitational forces,
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and these surroundings provide a natural laboratory for astronomers who
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are studying how matter behaves close to a black hole
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and how these central monsters are supplied with new material.
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Over the past twenty years, astronomers using infrared observations have
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discussed several compact gas clouds, and these Sagittarius A Star.
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These clumps for one of a better.
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Term are important clues to understanding how gas eventually reaches
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the black hole, yet their exact origin and the physical
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processes that shape them have remained uncertain. In twenty twelve,
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astronomers identified a first compact ionized gas cloud, which they
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named G two. It had several times the mass of
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the Earth and was emitting light from hydrogen and helium,
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which is fairly typical for hot, dusty gas. G two
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follows an elongated orbit around Sagittarius A Star and it
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shows a faint trailing structure, which astronomers then named G
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two t revisiting earlier observations, revealed a similar object, G one,
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also moving along a similar orbit around the black hole.
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So G one, G two, and G two t seemed
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to be denser clumps of gas, all moving within a
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common stream. Moderate density fluctuations can lead to a clump
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appearance because the cloud's brightness increases with a square of
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its density. More recently, astronomers found that gas from G
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two's tail is condensed into a third compact clump moving
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along a similar path, which the astronomers would have named
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G three, except that that name had already been taken
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by a different object. Together, these objects form coherent structure,
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the G one two three streamer, tracing material that flows
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through the galactic center. Calculations show that the infall of
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one such clump, roughly one Earth's mass every decade, would
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provide enough material to sustain Sagittari's a star's current activity level.
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So understanding how these clumps form is therefore key to
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explaining how the black hole is fuelled. Several origins have
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been proposed still a winds from massive nearby stars, explosive
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events such as supernovae, or tidal stripping of stars by
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Sagittaris a star itself to test these ideas, astronomers used
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adaptive optics assisted space, which enable sharp infrared spectroscopy. Focusing
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on the hydrogen bracket gamma emission line. The authors reconstructed
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the orbits of the three gas clouds based on their
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positions and velocities. Their analysis revealed that G one, G two,
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and G two T all travel on orbits with almost
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identical orientation and shape. The chance that three unrelated objects
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share such specific orbital parameters is extremely small, and so
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this indicates a common origin for all three clumps. By
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tracing the motions of the gas streamer backwards through space
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and radio velocity, the authors eventually identified a visible source,
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a massive contact binary star headlogged as IRS sixteen s W,
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which is located in a clockwise disc of young stars
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orbiting Sagittarius a star. The small differences between the G
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cloud orbits can be explained by the binary star system's
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own orbital motion. Follow up hydrodynamical computer simulations support this conclusion.
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They show the gas clumps can form where the stellar
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winds from the binary collide with the surrounding medium, producing
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a shock front between the two stars. There, gas accumulates
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and becomes compressed eventually detaching as individual clumps that travel inwards,
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exactly like what's observed in the G one two three streamer.
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These findings suggest that stellar winds from massive stars at
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the galactic center can continually supply material to feed the
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black hole. This result connects stellar revolution, gas dynamics, and
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black hole feeding into one consistent picture, showing astronomers how
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star formation and black hole growth can be linked even
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in our own galaxy. This is space time still to come.
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Two massive solar flares explode out of the Sun, and
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NASA's Mars rovers show the two sides of the red planet.
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All that and more still to come on space time.
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The Sun has just emitted two strong solar flares, lasting
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out into deep space within the day of each other.
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NASA's Solar Dynamics Observatory captured both explosions, classifying them as
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X two point four and X two point five class events.
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Solar flares are powerful bursts of energy caused by magnetic
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field lines from deep inside the Sun bursting through the
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solar surface, creating dark regions called sun spots, and then twisting, snapping,
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and finally reconnecting. The twisting happens because different parts of
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the sun rotated different speeds. Studying these intense streams of
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radiation is important because they can damage or even destroy satellites,
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They disrupt communications and navigation signals, they can overload power
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grids on the ground, triggering electrical blackouts, and they expose
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astronauts and even people in high flying aircraft increased radiation exposure.
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Solar flares are classified on a logarithmic scale according to
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their strength. The smallest ones are B class, followed by C,
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then M, and finally X being the largest and most powerful.
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It's similar to a Richter scale for earthquakes, each litter
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representing a ten fold increase in energy output, and so
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an X class flare has ten times the power of
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an M class flare and one hundred times are strong
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as a C class flare. Within each letter classification, there's
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a finer scale from one to nine. B and C
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class flares are far too weak to noticeably affect the Earth,
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so astronomers really only start paying attention when an M
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class flare occurs, because these can cause brief radio blackouts
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at the polls and minor radiation storms that could endanger astronauts,
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and of course they pay even more attention when it's
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at X class flare.
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Now, unlike the BC and M class flares, X class flares.
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Go beyond the once in night scale. That's because they
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can reach far higher levels of power. There have been
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flares more than ten times the power of an X one.
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In fact, the most powerful solar flare ever recorded was
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back in two thousand and three. That was during the
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last solar maximum cycle twenty four. It was so powerful
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it overloaded the sensors measuring it. They cut out at
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X seventeen and the flare was later estimated to be
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about at X forty five. The Sun goes through a
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regular eleven year solar cycle. This starts at solar minimum,
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where there are often no sun spots on the solar
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surface and the Sun is comparatively quiet. This is also
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where the Sun's poles switch polarity. The magnetic north pole
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becomes south and the magnetic south pole becomes north. The
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last solar minimum was in November twenty nineteen. Then gradually,
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over the next five and a half years, the rate
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of activity on the Sun increases. It becomes more violent
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until it reaches solar maximum, which occurred late last year.
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Then gradually the Sun starts to quieten down again, which
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is what it's doing now, but interestingly, it's during this
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quietening down period where some of the biggest solar storms
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can occur. The next solar minimum won't occur until around
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twenty thirty, and needless to say, we'll keep you informed.
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This is space time still to come. NASAs Mars rovers
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show the two sides of the Red planet, and later
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in the science report warnings that Omega Almino events expected
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to develop within the next month or so.
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All that and more still to come on space time.
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NASA is Mars Curiosity and Perseverance rovers have provided astronomers
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with two very different views of the Red planet, which
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are hoping to piece together puzzles on how this near
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neighbor of Earth has changed and evolved. The two three
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hundred and sixty degree landscapes highlight how the missions are
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revealing details of the Red planet's formation, it's watery past,
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and its potential for life. Located three thousand, seven hundred
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and seventy five kilometas apart on almost opposite sides of
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the Red planet, the two Cassis six World Mobile Laboratories
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are both exploring areas that are billions of years old,
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but as the nearly fifteen year old Curiosity rover reaches
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ever younger terrain in the foothills of gal Crater's central
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peak five and a half kilometator mount Sharp, the five
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year old Perseverance rover is venturing into some of the
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oldest landscapes in the entire Solar System, the outer ring
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of Czro Crater. By time traveling in opposite directions, the
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two rovers are filling in missing details about Martian history.
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Stitch together from one thousand and thirty one images taken
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late last year, Curiosity's latest three hundred and sixty degree
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panorama offers a detailed look at a region filled with
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a vast network of box work formations resembling giant spiderwebs
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in orbital images. These strange surface structures of low ridges
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created by groundwater that once flowed through large cracks and
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fishes in the bedrock. The minerals left behind hardened the
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rock along the fractures, resulting in erosion resistant ridges. Meanwhile,
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Perseverances panorama focused on a place named Lac de Chameais,
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which sits just outside the rim of Jesro Crater. Its
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nine hundred and eighty images stitched together over the Christmas
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New Holiday period provides a three hundred and sixty degree
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view capturing the jesiro Rim and the ancient rocks around
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the crater. Today, both these landscapes are frigid deserts that
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evidence of a more dynamic past hides within. When Curiosity
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landed on the floor of gal Crater back in twenty twelve,
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it's set out to determine whether Mars once had an
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environment capable of supporting life as we know it. Within
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a year, a sample drawled from an ancient lake bed
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confirmed those conditions work present once, and that included the
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right chemistry and potential nutrients for microbes to survive and
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even possibly thrive. Since twenty fourteen, Curiosity has been ascending
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the lower ridges of Mount Shark, which first began forming
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when layers of sediment were deposited in a series of lakes.
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These lakes, ponds, and streams dried up, refilled, and dried
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up again over repeated cycles, leaving a record of the
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mountains layers that formed in drier eras a sort of
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geological history book which scientists can read. And because the
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lowest layers of the oldest and higher and higher layers
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are younger curiosities, essentially progressing through geological time as it
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slowly climbs the mountain. Last year, Curiosity science team documented
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how they found that the mineral ciderite might be storing
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carbon dioxide that once was part of the thicker early
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Martian atmosphere. A thicker atmosphere would have retained heat also
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allowed water to pul on the surface, thereby suggesting Mars
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was once a warmer, wetter play one capable of supporting life.
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Scientists are long suspected that cabinet minerals such as ciderite
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formed when carbon diox are dissolved into ancient lakes, but
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supporting evidence in the guise of these deposits have only
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rarely been found. The mission also announced the detection of
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three of the largest organic molecules ever discovered on Mars,
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that was in a sample drilled back in twenty thirteen.
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These long chain hydrocarbons, possibly the remains of fatty acids,
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are a milestone in the search for more complex prebioder
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chemistry on the red planet, and just this year, scientists
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announced that a rock Curiosity drilled and analyzed back in
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twenty twenty includes the most diverse collection of organic molecules
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ever found on the Red planet. Of the twenty one
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carbon containing molecules identified in the sample, seven of them
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were detect it here for the first time. Meanwhile, on
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the other side of the planet, the Perseverance were over
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which landed on Mars in twenty twenty one, has been
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studying the origin of ancient rocks within Jezro cre and
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the hunt for evidence that microbial life may once have
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existed there. Billions of years ago, molten rock cooled and
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formed the crater's floor. Then a river fed a lake
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in the crater, leaving behind sediments where traces of microbes
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might have been preserved.
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In twenty twenty.
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Four, Perseverance discovered a rock named she Ava Falls. It
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was dotted with what scientists called leopard spots, a pattern
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formed by chemical reactions that microbes are known to create
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in rocks here on Earth. It's not proof that life
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existed on Mars, but it is tantalizing evidence. While Curiosity
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pulverizes its rock samples for analysis, Perseverance collects samples as
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intact rock cares, each about the size of a piece
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of blackboard chalk, and then stores them in metal tubes.
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Aside from a backup of ten tubes Perseverance deposited into
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sample reserve. The rover keeps all its samples twenty three
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so far in an onboard cage. Scientists are hoping that
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if they ever get enough funds, there'll be out of
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center mission Mars to collect these samples and return them
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to labs on Earth where they can investigate them more
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fully with instruments far bigger and more complicated than those
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that can be sent to Mars. While the sample return
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mission funding debate continues, Perseverance continues to investigate other aspects
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of the red planet. For instance, late last year, mission
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scient has shared the first recordings of electrical sparks in
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a passing dust devil lightning on Mars. That's a phenomenon
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that had only been theorized before Perseverance's microphone actually caught them. Meanwhile,
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a separate study detailed how one of Perseverance's cameras was
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able to capture the first visible light auroras from the
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