Universe Today

There may be as many rogue planets or free-floating planets in the Milky Way as there are stars. If there are billions of these worlds, some of them have likely held onto their moons. New research reveals a pathway to habitability for these rogue exomoons.

Every ounce counts when launching a rocket, which is why considerations for the Size, Weight, and Power (SWaP) of every component matters so much. For decades, one of the heaviest and most power-hungry components on a spacecraft has been its optical and communications hardware - specifically the bulky mechanical mirror used for LiDAR and free-space laser communications. But a new paper, published in Nature by researchers at MIT, MITRE, and Sandia National Laboratories, might have just fundamentally changed the SWaP considerations of LiDAR systems. Their technology, which they’re called a “photonic ski-jump” could one day revolutionize how spacecraft communicate.

And yeah, we have a problem.

One particularly well known fact about the Moon is that it doesn’t have much of a magnetosphere to speak of. There’s no blanket to protect it from the solar wind ravaging its surface, blowing away its atmosphere and charging the notoriously dangerous dust particles that make up its regolith. However, scientists have also known for around 60 years that some parts of the moon do experience sudden spikes in a magnetic field - some of which are up to 10 times stronger than the background magnetization. Since their discovery, these “lunar external magnetic enhancements” (LEMEs) have puzzled researchers - what was causing them, and why did they reach so high above the lunar surface that spacecraft could see them? A new paper published in The Astrophysical Journal Letters by Shu-Hua Lai and her colleagues at the National Central University in Taiwan explains for the first time what is likely causing these LEMEs - a novel type of the Kelvin-Helmholtz instability.

Beneath Europa's cracked and frozen shell lies a vast ocean of liquid water and what's seeping up through that ice may be one of the most compelling clues we have ever found about the moon's potential for life. A new analysis of James Webb Space Telescope observations has revealed that carbon dioxide on Europa's surface is far more widespread than previously thought, spreading across multiple regions of geological terrain in a distinctive lens like pattern. The findings are rewriting what we thought we knew about how material moves between Europa's hidden ocean and its surface.

For sixty years, the search for life beyond Earth has been built on the single assumption that alien life will look enough like us to recognise. A radical new idea called Assembly Theory is challenging that assumption. A team from the Arizona State University has proposed applying it to the atmospheres of distant exoplanets, not to look for specific gases, but to measure how much complexity a planetary atmosphere contains, and whether blind chemistry alone could plausibly have produced it. If it works, it could transform the way humanity searches for life among the stars, and redefine what we are even searching for.

Our Sun didn't always call this quiet corner of the Milky Way home. New research using data from the European Space Agency's Gaia satellite has uncovered evidence that the Sun fled the chaotic heart of our Galaxy four to six billion years ago and it didn't go alone. A vast migration of stars almost identical to our own swept outward together, a great exodus that may have made life on Earth possible. The story of how astronomers pieced this together is as remarkable as the discovery itself.

But here’s the thing about these defects. They can’t just go away. They’re stuck.

On 2 July 2025, NASA's Fermi Gamma-ray Space Telescope detected a gamma-ray burst lasting over seven hours, nearly twice the duration of anything previously recorded. Not only was it the longest ever seen, it repeated, firing off multiple distinct bursts across an entire day. GRB 250702B, as it became known, doesn't fit any known category of astronomical explosion. But a new paper in Monthly Notices of the Royal Astronomical Society offers the explanation that a star torn apart by an intermediate mass black hole may well be the culprit! On 2 July 2025, NASA's Fermi Gamma-ray Space Telescope detected a gamma-ray burst lasting over seven hours, nearly twice the duration of anything previously recorded. Not only was it the longest ever seen, it repeated, firing off multiple distinct bursts across an entire day. GRB 250702B, as it became known, doesn't fit any known category of astronomical explosion. But a new paper in Monthly Notices of the Royal Astronomical Society offers the explanation that a star torn apart by an intermediate mass black hole may well be the culprit!

The spacecraft changed the binary system’s orbit, confirming that a kinetic impactor can be an effective planetary defense technique for deflecting a near-Earth object.

Every time you flip a light switch, or check the time, or feel the sodium ions wiggling in your brain — don’t think about that one too much—you’re assuming something fundamental. You’re assuming the universe is a finished product. A completed work. You think the Big Bang happened, the forces of nature settled into their seats, and we’ve been cruising on a smooth, predictable ride ever since.

Every planet with a magnetic field has a radiation belt, a region of space where charged particles get trapped and flung around at extraordinary speeds. Earth has two of them, and they've been puzzling scientists for decades. Now, a physicist at the University of Helsinki has built a model that defines a universal upper limit to just how energetic those belts can ever get. The answer applies not just to Earth, but to every planet in the Solar System, every gas giant, and even the strange objects sitting halfway between planets and stars.