Tuesday, May 19, 2026

A Brief-ish History of SETI. Part VI: The Great Silence and the Great Filter

The Allen Telescope Array in Northern California is dedicated to astronomical observations and a simultaneous search for extraterrestrial intelligence (SETI). Credit: Seth Shostak/SETI Institute

In the closing decades of the 20th century, several proposed explanations were put forward for why humanity has not yet found evidence of extraterrestrial intelligence in the cosmos.



An Explanation for the Massive Black Holes the JWST Found in the Early Universe

This artist's illustration shows a supermassive black hole (SMBH) in the early Universe. The JWST found galaxies in the very early Universe that were extremely massive compared to their host galaxies. New research has an explanation for those puzzling findings. Image Credit: NOIRLab/NSF/AURA/J. da Silva (Spaceengine)

Ever since the JWST found over-massive black holes in the early Universe, researchers have been trying to understand them. Theory showed that black holes and their galaxies grew in synchronization with each other. That can't explain the JWST's findings, but new research might.



Monday, May 18, 2026

Astronomers Find New Circumbinary "Tatooine-like" Planet Candidates

An artist's concept of a circumbinary world orbiting two suns. Courtesy UNSW.

There's a distinct category of exoworlds out there that orbit two stars. They're called "circumbinary" planets and up until recently, astronomers had only found about 18 of them among the 6000+ other known exoplanets and candidates. Now, a team at the University of New South Wales (UNSW) in Sydney, Australia, have found 27 more potential circumbinary worlds. They credit a new method, called apsidal precession, for their finding.



A Brief-ish History of SETI. Part V: The First Interstellar Messengers

The Voyager Golden Record, including the "Sounds of Earth" record (right) and the cover with instructions on how to play it (left). Credit: NASA/JPL-Caltech

During the 1970s, the first interstellar probes were launched, carrying messages specifically designed to be intelligible to extraterrestrial species. The messages were essentially a "message in a bottle" intended for an advanced civilization, should they find the probes someday.



Iron and Ice: Earth's Passage Through the Interstellar Cloud

This illustration shows the Solar System's passage through the Local Interstellar Cloud (LIC). The LIC could've been created by supernovae shockwaves, which also produced the isotope 60Fe. By examining that isotope in Antarctic ice, scientists are learning more about the LIC and Earth's passage through it. Image Credit: NASA / Adler / University of Chicago / Wesleyan.

Our Solar System is currently passing through the Local Interstellar Cloud, a region of highly diluted gas and dust between the stars. On its path, Earth continuously accumulates iron-60, a rare radioactive isotope of iron produced in stellar explosions. This has now been confirmed by an international research team led by the Helmholtz-Zentrum Dresden-Rossendorf (HZDR) through the analysis of Antarctic ice tens of thousands of years old. From the steady but time-varying influx, the researchers conclude that the radioactive isotope has been stored within the cloud since a long-past stellar explosion.



Asteroid 2022 OB5 Spins Too Fast For Current Prospectors Highlighting the Divide Between "Accessible" and "Exploitable"

Artist's concept of OSIRIS-Rex Mission to asteroid Bennu. Credit - NASA/Goddard/Chris Meaney

Asteroid mining seems simple in theory. A spacecraft flies up to a giant rock in space, scoops out some material, and either processes it on site or returns it back to a huge central processing facility. But in practice, it is certainly not that simple, and a new paper from some Spanish researchers, available in pre-print form on arXiv, showcases one of the reasons why - many small asteroids are spinning ridiculously fast.



Gazing Into the Past With TIME

This illustration shows the early Universe's progression into the Epoch of Reionization. This is when the first stars and galaxies ionized hydrogen and changed the Universe from opaque to translucent. The new TIME instrument is poised to study this time with a new technique. Image Credit: ESA / C. Carreau. LICENCE: ESA Standard Licence

How can astronomers observe ancient galaxies when they're so challenging to resolve? By looking at a whole bunch of them at once in a single spectral line and seeing how it changes over time. That's what a new instrument called the Tomographic Ionized-carbon Mapping Experiment (TIME) does.