Universe Today

Even the universe’s emptiest regions, the vast voids that make up most of the volume of space, are not entirely empty. A new study using the CAVITY survey hunts for galaxy groups hiding within these voids, applying a friends of friends technique to chart how nearby galaxies cluster together despite the surrounding emptiness. The results paint a striking picture that most void galaxies actually live entirely solitary lives, yet where groups do form, they are small, loose and curiously indifferent to just how empty their void actually is. It raises a deceptively simple question that turns out to be anything but: in the universe’s quietest neighbourhoods, what makes some galaxies choose company while most remain alone?

Saturn’s moon, Enceladus, has become a prime solar system target for astrobiologists. This is because the small moon, which is just over 10 percent the diameter of Earth’s Moon, harbors a vast subsurface ocean beneath its icy crust. This subsurface ocean combined with the geysers at Enceladus’ south pole that discharges bits of this ocean into the void provides scientists with a treasure trove of opportunities for scientific research into whether Enceladus could harbor ingredients for life as we know it, or even direct evidence for life.

Searching for habitable worlds beyond our solar system consists of more than just having it orbit within its star’s habitable zone, which is the region where temperatures could be just right for liquid water to exist on the surface. On Earth, where water comprises approximately 75 percent of the planet’s surface, life is absurdly abundant. But what about the exoplanet’s star, specifically its activity and rotation? How could this influence how exoplanets are identified for current and future missions?

Astronomers using W. M. Keck Observatory on Maunakea, Hawaiʻi Island, have discovered the third known galaxy apparently lacking dark matter, part of a strange linear structure that may have formed during a violent collision between galaxies.

Exoplanet atmospheres have become prima targets for astrobiologists in the search for life beyond Earth. This is because exoplanet surfaces can’t be directly imaged yet, so astronomers must get creative with how to search for signs of life, also called biosignatures. Presently, powerful ground- and space-based telescopes like the Atacama Large Millimeter Array (ALMA) and NASA’s James Webb Space Telescope (JWST) are improving in their ability to observe and analyze exoplanet atmospheres. But did these atmospheres form and evolve, and what could this mean for the search for life beyond Earth?

The Vera Rubin Observatory's long-awaited Legacy Survey of Space and Time has begun. This decade-long movie of the cosmos will capture anything that changes brightness, position, or both in the southern night sky. It will study grand subjects like dark energy and dark matter, and important things closer to home like near-Earth objects.

The way that dark matter is distributed may need a rethink. New research shows that dark matter could gather near supermassive black holes. The evidence is based on a new detection method, and is only moderately convincing so far. But if true, it also turns SMBH into 'dark matter labs' and could change how we understand SMBH growth.

Hopefully, we’re about to travel back to the Moon relatively soon. And while the original “giant leap for mankind” was taken by a human, Neil Armstrong brought a plethora of other forms of life along with him. Humans themselves are essentially walking ecosystems, and understanding how our microbial companions survive in the harsh environments of space will be critical to ensure the health and safety of future astronauts, no matter where their giant leaps might be. A new PhD thesis from Tommaso Zaccaria at Radboud University showcases just how well-suited to some of these harsh environments terrestrial pathogens actually are.

The famous opening scene of the Martian has Mark Watney stabbed in the torso with a communications antenna. While this accident sets up the plot for what is widely regarded as a modern classic of sci-fi storytelling, what if he was wearing a space suit that would have stopped the impact altogether? That’s the idea behind a recent NASA Small Business Innovation Research (SBIR) Phase I program run by researchers from Materials Research & Design, Fiber Materials, Inc, and NASA’s Johnson Space Center. Their work, which was recently presented at the National Space & Missile Materials Symposium, showcased a type of advanced 3D-reinforced fabric that could have saved Watney and his compatriots a whole lot of trouble.

Observations of a distant cluster of stars in our galaxy have resulted in a new class of objects that turn out to be galactic building blocks. Researchers used Hubble Space Telescope (HST) and the James Webb Space Telescope (JWST) to study the stars that make up Terzan 5, long though to be a globular cluster. What they found puts that cluster into a very rare class of objects called "bulge fossil fragments."

The wreckage of an exploded star is meant to fade quietly, cooling over thousands of years like the embers of a fire. So astronomers were stunned when NASA's Chandra X-ray Observatory caught dozens of these supernova remnants in a nearby galaxy doing the opposite, flaring and flickering in X-rays as though refusing to die. In each case a star appears to have survived its partner's explosion, only to be slowly devoured by the black hole or neutron star its companion left behind. It’s a discovery that turns the calm graveyards of dead stars into something far stranger and more alive.

Jezero Crater on Mars is a 45-kilometer-wide (28-mile) crater that once hosted a lake billions of years ago fed by two distinct river valleys with Jezero eventually forming an exit channel over time. One of Jezero’s most prominent features is the massive river delta that consists of sediments that were deposited as the inflow slowed down. Researchers hypothesize that the delta and lake were formed under freshwater conditions, indicating the potential for life as we know it, also called biosignatures.

Europe's CERN physics research center bids 'Farewell' to the Large Hadron Collider, but it's actually more like 'See You Later, Accelerator!' The new, improved High-Luminosity LHC is due to make its debut in 2030.

After more than eight years of searching and with instruments designed to detect it, the European Space Agency’s (ESA) Mars Trace Gas Orbiter has yet to find methane in the red planet’s atmosphere.

On September 22, 2021, the IceCube Neutrino Detector in Antarctica caught a blast of neutrinos as it passed through the solar system. These neutrinos were remarkably high-energy and came from a galaxy 11 billion light-years away. That's a period of the Universe's history known as "Cosmic Noon". It's when star formation in galaxies was at its most active and that provided an interesting clue to their origin. The source of the neutrinos was nicknamed "Shadow Blaster" because the event that created the neutrinos was hidden by a dense cloud of dust, which made it invisible to optical observations.

Stellar mass black holes may not be black holes at all. Instead, they could be a type of extremely compact star called a gravastar, which mimics a black hole. This is according to theoretical phsyicists who have discovered a solution to Einstein's Theory of General Relativity that doesn't automatically result in a black hole when a star collapses at the end of its life.

Researchers from the University of Oxford have uncovered evidence that Mars once hosted widespread, Earth-like magmatic systems deep beneath its surface – despite the planet lacking the plate tectonics long thought necessary for this kind of geological complexity. The findings, published June 26th in Nature Astronomy, reveal fascinating new possibilities for how rocky planets become habitable.

Giant mirrors in space have been a staple of science fiction for decades. But so far there’s been very little work looking at the actual physics behind the concept - possibly because we’re still so far from making them ourselves. Still, they could potentially serve as a passive technosignature, if we manage to find one. In order to do that, though, we have to understand what we’re looking for. That is the purpose of a new paper, available in pre-print on arXiv, by Shauna Sallmen of the University of Wisconsin - LaCrosse, and Eric Korpela of UC Berkeley.

Artificial Intelligence (AI) is continuing to have a disruptive impact on ever more parts of humanity. But what does it mean in the long run? A new paper, available in pre-print on arXiv from Austrian researcher Sergey Ivliev, extrapolates what the wide scale adoption of AI means for the future of humanity in space - and in particular what it means for the ultimate question of whether we’re truly alone in the galaxy or not.

When a star strays too close to a supermassive black hole, it is torn apart in a brief, brilliant flare, and astronomers long assumed that was the end of the story. It isn't. Using the Very Large Array to follow dozens of these stellar killings, a team has discovered that many black holes "burp" months or even years later, belching out streams of radio light as they fling part of their meal back into space. These delayed flares let astronomers watch a black hole's appetite change in real time, and reveal that even our Galaxy's quietest looking giants are messier, and far more active, than anyone realised.