A delicate waxing crescent Moon creates an elongated triangle with bright planets Jupiter and Mercury in the evening sky.
Google DeepMind just dropped a massive paper called From AGI to ASI, and the message is bigger than another AI release. The paper argues that AGI may not be the finish line everyone is waiting for. It may be the moment the real race begins. Once human-level AI can be copied, sped up, connected into agent teams, and used to build better AI, the jump after AGI could matter even more than AGI itself.
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Google DeepMind’s new From AGI to ASI paper.
SOURCE: https://deepmind.google/research/publ… 2026 framework for tracking progress toward AGI SOURCE: https://blog.google/innovation-and-ai… DeepMind’s approach to AGI safety and security SOURCE: https://deepmind.google/blog/taking-a… Demis Hassabis on AI agents and the road to AGI SOURCE: https://www.axios.com/2026/05/26/deep… The Legg and Hutter paper behind formal machine intelligence SOURCE: https://arxiv.org/abs/cs/0605024 🚨 Why It Matters This is bigger than another AI paper. Google DeepMind is already talking about what happens after AGI. If human-level AI can be copied, sped up, connected, and used to build better AI, then intelligence itself could become an industrial process. #ai #agi #deepmind.
The full technical paper on arXiv.
SOURCE: https://arxiv.org/abs/2606.12683
DeepMind’s earlier framework for measuring AGI progress.
SOURCE: https://deepmind.google/research/publ…
Google’s 2026 framework for tracking progress toward AGI
SOURCE: https://blog.google/innovation-and-ai…
DeepMind’s approach to AGI safety and security.
SOURCE: https://deepmind.google/blog/taking-a…
Demis Hassabis on AI agents and the road to AGI
SOURCE: https://www.axios.com/2026/05/26/deep…
The Legg and Hutter paper behind formal machine intelligence.
SOURCE: https://arxiv.org/abs/cs/0605024
🚨 Why It Matters.
This is bigger than another AI paper. Google DeepMind is already talking about what happens after AGI. If human-level AI can be copied, sped up, connected, and used to build better AI, then intelligence itself could become an industrial process.
#ai #agi #deepmind
An international team led by astronomers at the University of Sydney has uncovered the clearest evidence yet for the origin of an unusual class of cosmic signals. In doing so, they have identified a rare stellar system that is providing scientists with a natural laboratory to study extreme physics.
Using CSIRO’s ASKAP radio telescope, the team discovered a small, dense star, called a white dwarf, shredding material from its larger, but less dense, companion star.
As this material spirals in, it produces powerful bursts of radio waves and X-rays in a cycle that repeats every 1.4 hours.
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Today’s video explores the most terrifying calculation I’ve ever done, one that comes with some deeply unsettling implications for the Universe in which we live…
Written & presented by David Kipping, edited by Jorge Casas.
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REFERENCES
Every galaxy you’ve ever seen in a photograph is hiding something. Beyond the glowing disc of stars and gas that the camera captures lies a vast, ghostly outer region called a halo, too faint to see easily but packed with clues about how that galaxy came to be. ESA has just formally committed to a mission designed to reveal those hidden haloes in unprecedented detail, and in doing so, finally answer one of the most fundamental questions in astronomy: how did galaxies like our own Milky Way form?
Explore the future of space habitats, from rotating cylinders and torus colonies to orbital cities, asteroid homes, and the megastructures humanity may one day live inside.
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/ discord Credits: Space Habitats: The Megastructures We’ll Call Home Written, Produced & Narrated by: Isaac Arthur Editors: Briana Brownell, Ludwig Luska Select imagery/video supplied by Getty Images, Anthrofuturism, Apogii.uk, Bryan Versteeg, Fishy Tree, Katie Byrne, Jarred Eagley, Jeremy Jozwik, Justin Dixon, Ken York YD Visual, Neil Blevins, Sergio Botero, Steve Bowers, and Udo Schroeter Music by Epidemic Sound: http://nebula.tv/epidemic and Markus Junnikkala, Phase Shift, Kai Engel, Chris Zabriskie, Taras Harkavyi, and Stellardrone 0:00 Intro 4:37 The Sunflower 14:07 The O’Neill Cylinder 49:00 Lewis One 57:40 Stanford Torus 1:22:19 Kalpana One 1:28:14 Nebula 1:29:27 Bernal Sphere 1:54:13 Bishop Ring 2:03:23 Topopolis 2:27:36 McKendree Cylinder 2:33:57 Hammer Habs 2:59:01 Rungworlds 3:04:35 Conglomerations 3:38:45 Epilogue.
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Credits:
Space Habitats: The Megastructures We’ll Call Home.
Written, Produced \& Narrated by: Isaac Arthur.
Editors: Briana Brownell, Ludwig Luska.
Select imagery/video supplied by Getty Images, Anthrofuturism, Apogii.uk, Bryan Versteeg, Fishy Tree, Katie Byrne, Jarred Eagley, Jeremy Jozwik, Justin Dixon, Ken York YD Visual, Neil Blevins, Sergio Botero, Steve Bowers, and Udo Schroeter.
Music by Epidemic Sound: http://nebula.tv/epidemic and Markus Junnikkala, Phase Shift, Kai Engel, Chris Zabriskie, Taras Harkavyi, and Stellardrone.
0:00 Intro.
4:37 The Sunflower.
14:07 The O’Neill Cylinder.
49:00 Lewis One.
57:40 Stanford Torus.
1:22:19 Kalpana One.
1:28:14 Nebula.
1:29:27 Bernal Sphere.
1:54:13 Bishop Ring.
2:03:23 Topopolis.
2:27:36 McKendree Cylinder.
2:33:57 Hammer Habs.
2:59:01 Rungworlds.
3:04:35 Conglomerations.
3:38:45 Epilogue
NASA’s Nancy Grace Roman Space Telescope is poised to make a major leap in the hunt for worlds outside our solar system, known as exoplanets. Scientists expect the mission to reveal around 100,000 worlds—a staggering leap compared to the nearly 6,300 found so far thanks to NASA missions working in tandem with other observatories. And Roman will primarily find them in underexplored regions of the Milky Way.
“Our galaxy is home to a variety of different environments, but when it comes to hunting for exoplanets, we’ve really only explored one: our own neighborhood,” said Elisa Quintana, an exoplanet researcher at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. Quintana leads a team focused on building software and simulations to help prepare for Roman’s exoplanet transit observations. “Roman will extend the search far enough to encompass other galactic habitats, which could help us learn how planet formation varies across different regions of the Milky Way.”
Most known exoplanets are located within a couple thousand light-years of Earth. But one of Roman’s core surveys will peer all the way through the Milky Way’s galactic bulge, the central hub where stars are packed more densely than anywhere else, to the fringes of the far side of the galaxy.
Astronomers have discovered a huge reservoir of cold molecular gas, the direct fuel for star formation, in REBELS-25, a massive, star-forming galaxy. The team, led from Leiden University, focused on REBELS-25, seen when the universe was only about 700 million years old, around 5% of its current age. The research is published in the journal Monthly Notices of the Royal Astronomical Society.
Astronomers use “redshift” to describe this distance, which measures how much the universe’s expansion has stretched a galaxy’s light to redder wavelengths. The higher the redshift, the farther back in time we look. REBELS-25 sits at redshift z = 7.3, deep in the Epoch of Reionization, a key era in which the first stars and galaxies transformed the dark, neutral universe into the universe we see around us today.
Galaxies grow by turning gas into stars, and cold molecular gas is the primary fuel. Until now, astronomers suspected early bright, massive galaxies had huge gas supplies, but no one had directly detected them at these distances.