Universe Today Feed

How long did it take to establish the water content within Jupiter’s Galilean moons, Io and Europa? This is what a recent study published in The Astrophysical Journal hopes to address as a team of scientists from the United States and France investigated the intricate processes responsible for the formation and evolution of Io and Europa. This study has the potential to help scientists better understand the formation and evolution of two of the most unique moons in the solar system, as Io and Europa are known as the most volcanically active body in the solar system and an ocean world estimated to contain twice the volume of Earth’s oceans, respectively.

Icy comets contain common crystals that can only be formed in extreme heat. But comets reside in the frigid outer reaches of the Solar System. How did these materials form, and how did they find their way into the Solar System's cold fringes?

Water exists across Mars in underground ice, soil moisture, and atmospheric vapour, yet most of it remains frustratingly beyond practical reach for future explorers. A new comparative study from the University of Strathclyde evaluates the technologies that could extract this vital resource from various Martian sources, assessing each method's energy demands, scalability, and suitability for the Red Planet's harsh conditions.

Stars change in brightness for all kinds of reasons, but all of them are interesting to astronomers at some level. So imagine their excitement when a star known as J0705+0612 (or, perhaps more politically incorrectly, ASASSN-24fw) dropped to around 2.5% of its original brightness for 8.5 months. Two new papers - one from Nadia Zakamska and her team at the Gemini Telescope South and one from Raquel Forés-Toribio at Ohio State and her co-authors - examine this star and have come to the same conclusion - it’s likely being caused by a circumsecondary disk.

Thousands of pieces of abandoned spacecraft orbit Earth, and when gravity finally pulls them down, authorities rarely know exactly where they'll land. Now researchers at Johns Hopkins University have demonstrated a clever solution. Surprisingly they have found using earthquake detecting seismometers they can track falling space debris in real time by listening for the sonic booms it produces. The technique successfully traced a Chinese spacecraft module as it streaked across California at Mach 25-30, revealing its actual trajectory lay 25 miles north of predictions, a significant improvement that could help authorities quickly locate potentially toxic debris and protect people from contamination.

New research from the International Space Station reveals that in near weightless conditions, both bacteriophages and their *E. coli* hosts mutate in ways not seen on Earth. This unexpected finding not only deepens our understanding of how microbial life adapts to extreme environments but has already yielded practical benefits. Some of the mutations discovered in space dwelling viruses led researchers to create superior viruses that specifically infect and kill bacteria, capable of fighting drug resistant bacterial infections back on Earth.

The Circinus Galaxy, a galaxy about 13 million light-years away, contains an active supermassive black hole that continues to influence its evolution. The largest source of infrared light from the region closest to the black hole itself was thought to be outflows, or streams of superheated matter that fire outward.

We live near a fusion reactor in space that provides all our heat and light. That reactor is also responsible for the creation of various elements heavier than hydrogen, and that's true of all stars. So, how do we know that stars are element generators?

The earliest galaxies in the universe earned the nickname "monster galaxies" for good reason, they formed stars at rates hundreds of times faster than the Milky Way, growing rapidly after the dawn of time. Astronomers using ALMA and the James Webb Space Telescope have now revealed that three such monsters each achieved their extraordinary growth through completely different mechanisms. By comparing where stars are forming today with where they formed in the past, researchers discovered that galaxy collisions, internal instability, and minor mergers can all trigger these growth spurts, fundamentally changing our understanding of how the universe's most massive galaxies came to be.

Gravitational lensing is a powerful tool that brings impossibly distant galaxies into reach. The JWST uses galaxy clusters and their overpowering to magnify background galaxies that are otherwise beyond our observational capabilities. One cluster, named MACS J1149.5+2223, is 5 billion light-years away and holds at least 300 galaxies, probably many more. It's been chosen as the JWST's Picture Of The Month.

As they roll across shadowed regions of the moon's surface, future lunar rovers could develop hazardous buildups of electric charge on their wheels. Through new analysis published in Advances in Space Research, Bill Farrell at the Space Science Institute in Colorado, together with Mike Zimmerman at Johns Hopkins University, outline realistic precautions for mitigating this risk—offering valuable guidance for engineers designing future lunar missions.

How do blue stragglers defy the aging that turns their mates red? Blue stragglers are found in ancient star clusters, where they outshine stars the same age, looking far bluer and younger than their true age. Astrophysicists have tried to understand blue stragglers for decades. New research using the NASA/ESA Hubble Space Telescope is finally revealing how these ageless stars come to be and why they thrive in quieter cosmic neighbourhoods.

The Helix Nebula is one of the closest and brightest planetary nebula. It's what's left of a dying star and has nothing to do with planets. Our Sun will end up as one of these sumptuous displays, and a new JWST image reveals even more detail in the stunning nebula.

Some really unique science can be done during a total solar eclipse. Totality is the one time we can see the elusive corona of the Sun, the pearly white segment of our host star’s lower atmosphere where space weather activity originates. The trouble is, totality is fleeting. What researchers really need are eclipses on demand. ESA’s innovative Proba-3 mission does just that, by making use of a free-flying occulting disk. Launched in late 2024, we’re now seeing some unique science and images from the space observatory.

If humans are ever going to expand into space itself, it will have to be for a reason. Optimists think that reason is simply due to our love of exploration itself. But in history, it is more often a profit motive that has led humans to seek out new lands. So, it stands to reason that, in order for us to truly begin space colonization, we will have to have a business-related reason to do so. A new paper from the lab of Srivatsan Raman at the University of Wisconsin-Madison and recently published in PLOS Biology, describes one potential such business case - genetically modifying bacteriophages to attack antibiotic resistant bacteria.

High-precision oxygen isotopes in Apollo lunar soils reveal a persistent impactor fingerprint, showing that impacts contributed only a tiny fraction of Earth’s water.

The Hubble Mission Team has released another image of the space telescope's study of star formation. This image shows the dark cloud Lupus 3, a star-forming region about 500 light-years away. Lupus 3 contains bright young T-Tauri stars, and 2 hot young stars that are creating a beautiful nebula.

The resolution of the Event Horizon Telescope is limited by the diameter of Earth, and our observations of the black hole in M87 and in our own galaxy are at the edge of that limit. To observe other, more distant black holes we will need radio telescopes on the Moon.

Back in 2014, the Atacama Large Millimeter/submillimeter Array (ALMA) captured an image of a young protoplanetary disk around a young star named HL Tauri. The image showed gaps and rings in the disk, substructures indicating that young planets forming there. This meant that planet formation began around young stars a lot sooner than thought. ALMA is continuing its investigation of protoplanetary disks in its ARKS survey (ALMA survey to Resolve exoKuiper belt Substructures).

Material science plays an absolutely critical role in space exploration. So when a new type of self-healing composite is announced, it’s worth a look–especially when the press release specifically calls out its ability to repair microtears associated with micrometeoroid impacts on satellites. It sounds like just such a composite material was recently invented at North Carolina State University - and it’s even already been spun out into a start-up company.