Toggle light / dark theme

Why it matters

The new study explains a longstanding puzzle in medicine: why do some people who’ve inherited a disease-causing mutation experience fewer symptoms than others with the same mutation? “In many diseases, we’ll see that 90% of people who carry a mutation are sick, but 10% who carry the mutation don’t get sick at all,” says Bogunovic, a scientist who studies children with rare immunological disorders at Columbia University Irving Medical Center.

Enlisting an international team of collaborators, the researchers looked at several families with different genetic disorders affecting their immune systems. In each case, the disease-causing copy was more likely to be active in sick patients and suppressed in healthy relatives who had inherited the same genes.

What if the secret to slowing down aging was hiding in our brains? A groundbreaking study by researchers at the Allen Institute for Brain Science in Seattle, published in Nature in January 2025, may have uncovered some exciting clues. Using cutting-edge technology, the team analyzed over 1.2 million brain cells from young and aged mice to understand how they change with time. They found that certain cells become inflamed, while others lose critical functions, and all eyes are now on the hypothalamus as a key player in the aging process. These findings deepen our understanding of aging and could pave the way for treatments that keep our brains younger for longer.

Early Formation of Life’s Building Blocks

A groundbreaking study published in Nature Astronomy has revealed that amino acids, essential for life, can form in dark interstellar clouds long before stars and planets emerge. Glycine, the simplest amino acid, was shown to form on the surface of icy dust grains in cold, energy-deprived environments through a process called “dark chemistry.” These findings challenge the long-standing belief that UV radiation was required to create glycine, significantly expanding our understanding of how life’s precursors emerge in space.

Astronomers using the James Webb Space Telescope have used a distortion in space to reveal over 40 individual stars in a galaxy 6.5 billion light-years from the Milky Way—halfway back to the beginning of the universe. It’s the largest number of individual stars ever detected in the distant universe.

The unique image, which takes advantage of JWST’s high-resolution optics, was only possible because the light from 44 stars in a distant galaxy was magnified by a massive cluster of galaxies in front of it called Abell 370.

This technique, called gravitational lensing—also known as an “Einstein ring” because it was predicted by the famous scientist Albert Einstein—works when the gravitational field of a foreground object distorts the space around it. Light is bent from an object behind it into circular rings or arcs, both revealing the existence of something in the background and, crucially, magnifying it by factors of hundreds or even thousands. In this case, an arc was visible, dubbed the “Dragon Arc.”

The latest AI News. Learn about LLMs, Gen AI and get ready for the rollout of AGI. Wes Roth covers the latest happenings in the world of OpenAI, Google, Anthropic, NVIDIA and Open Source AI.

My Links 🔗
➡️ Subscribe: / @wesroth.
➡️ Twitter: https://twitter.com/WesRothMoney.
➡️ AI Newsletter: https://natural20.beehiiv.com/subscribe.

00:00 singularity is near.
01:37 Sam Altman’s Blog Post \

Get ready to be inspired by Camp Peavy, a well-known figure in the robotics industry and a passionate member of the HomeBrew Robotics Club in Silicon Valley! 🤖✨

In this engaging Q\&A, Camp dives into his incredible robotics journey, offering unique insights into the world of innovation and technology. He also shares invaluable tips for those who are new to robotics, feeling unsure, or looking for a spark of motivation to dive into this exciting field.

Learn about the amazing work happening at the HomeBrew Robotics Club and discover how you, too, can become part of this thriving community. Whether you’re a seasoned techie or just starting out, this video has something for everyone.

Sign Up for Page Launch: https://forms.gle/ijzxGKNJUj5dCLnL7

Currently, 5,788 exoplanets have been confirmed in 4,326 star systems, while thousands more candidates await confirmation. So far, the vast majority of these planets have been gas giants (3,826) or Super-Earths (1,735), while only 210 have been “Earth-like”—meaning rocky planets similar in size and mass to Earth.

What’s more, the majority of these planets have been discovered orbiting within M-type (red dwarf) star systems, while only a few have been found orbiting sun-like stars. Nevertheless, no Earth-like planets orbiting within a sun-like star’s habitable zone (HZ) have been discovered so far.

This is largely due to the limitations of existing observatories, which have been unable to resolve Earth-sized planets with longer orbital periods (200 to 500 days). This is where next-generation instruments like the ESA’s PLAnetary Transits and Oscillations of stars (PLATO) mission come into play.