On Earth, water is so intertwined with life that our search for life on other worlds is essentially a search for water. When scientists find exoplanets around distant stars, a primary consideration is if they're in the stars' habitable zones where liquid water could persist on the planet's surface. The search for atmospheric biosignatures takes a backseat to the search for water.
If humanity intends to live and work beyond Earth, we need solutions for living sustainably in inhospitable environments. Even Mars, the most hospitable planet in the Solar System beyond Earth, is hostile to life as we know it. These include extreme temperature variations, a thin, unbreathable atmosphere, toxic soil, and higher-than-normal levels of solar and cosmic radiation. Given the distance between Earth and Mars and the time it takes to send missions there (6 to 9 months using conventional propulsion), these habitats must be closed-loop, self-sustaining environments that provide crews with food, water, and breathable air.
Dark matter is one of Nature's most confounding mysteries. It keeps particle physicists up at night and cosmologists glued to their supercomputer simulations. We know it's real because its mass prevents galaxies from falling apart. But we don't know what it is.
The Hubble Space Telescope is one of the most successful scientific endeavours in history, maybe the most successful. It's been observing the heavens for more than 35 years since its launch in 1990. The JWST is the most powerful and complex space telescope ever built, and has been expanding our horizons since its launch in December, 2021. When working together, they create synergy that not only benefits science, but provides stunning images of the cosmos.
We all know what it's like when Earth is on the receiving end of a solar flare. Things get spicy in the upper atmosphere, and the outbursts have the potential to disrupt technology here at home. Catastrophic flares of radiation devastate planets around other stars, too. Now it looks like scientists have found that planets orbiting close to their stars can trigger the flares that threaten to harm them.
The James Webb Space Telescope (JWST) can tell us a lot about the subjects of its observations if it spends enough time with them. That includes lonely rocks on the edges of our solar system, such as the Trans-Neptunian Object (TNO) Quaoar. Recent observations using the NIRCam on JWST and pre-published on arXiv by researchers at the University of Central Florida, the Space Telescope Science Institute, and Kyoto University add a plethora of new data to our understanding of this enigmatic object, including insights into what might be causing its ring system and its hydrocarbon atmosphere.
Sometimes there are profound questions in life that must be answered, like “What is the meaning of existence?”, “Are we alone in the universe?” or “What happens if you throw a paper airplane from the International Space Station?” Luckily, that third one has finally been answered, because of course someone would eventually. A new paper from Maximilien Berthet and Kojiro Suzuki from the University of Tokyo looks at “the dynamics of an origami space plane during Earth atmospheric reentry” - in other words, what happens when you throw a paper plane out of the ISS.
Earth is the only habitable world we know of and it remains habitable because of natural cycles that maintain a balanced climate. Earth's carbon cycle plays a critical role in maintaining its temperate climate, and carbonate rocks are a big part of it. Carbonate rocks like limestone and dolomite are huge carbon sinks, and if their carbon was released into the atmosphere, Earth's temperature would spike catastrophically, rendering our planet uninhabitable. Conversely, if all of Earth's carbon were locked away in rock, Earth would likely become glaciated, photosynthesis would cease, and a mass extinction would leave extremophiles as the sole survivors of life's rich, living heritage.
Gravitational waves come in all shapes and sizes - and frequencies. But, so far, we haven’t been able to capture any of the higher frequency ones. That’s unfortunate, as they might hold the key to unlocking our understanding of some really interesting physical phenomena, such as Boson clouds and tiny block hole mergers. A new paper from researchers at Notre Dame and Caltech, led by PhD student Christopher Jungkind, explores how we might use one of the world’s most prolific gravitational wave observatories, GEO600, to capture signals from those phenomena for the first time.
Research shows that modern disk galaxies have two overall components: a thin disk containing higher-metallicity young stars, and a thick disk containing lower-metallicity older stars. The thin disk sits inside the thick disk. Astronomers are trying to understand how these parts form and how disk galaxies evolve. To make progress, astronomers need to observe edge-on rather than face-on galaxies. They also need to observe them in the past, something that the JWST is built to do.
Astronomers have studied the globular cluster 47 Tucanae extensively, but still have many questions. It may have an intermediate mass black hole in its center like Omega Centauri is expected to have. There are reasons to believe it may be the remnant of a dwarf galaxy that was gobbled up by the Milky Way, like other GCs. Also like other GCs, its center is extraordinarily dense with stars, and astronomers aren't certain how far the cluster spreads. Individual stars in 47 Tuc are difficult to observe because they're so tightly packed in the center and because they're difficult to differentiate from field stars on its outer edges. Can the Vera Rubin Observatory help?
The search for dark matter requires all of the best models, theories, and ideas we can throw at it. A new paper from Julia Monika Koulen, Stefano Profumo, and Nolan Smyth from the University of California at Santa Cruz (UCSC) tackles the sizes and abundance of one of the more interesting dark matter candidates - primordial black holes (PBHs).
How did Earth, alone among the Solar System's rocky planets, become the home for life? How, among all this frigid lifelessness, did our planet become warm, hospitable, and life-sustaining? The answer to these questions is complex and multi-faceted, and part of the answer comes from cosmochemistry, an interdisciplinary field that examines how chemical elements are distributed.
Proxima Centauri b is the closest known exoplanet that could be in the habitable zone of its star. Therefore, it has garnered a lot of attention, including several missions designed to visit it and send back information. Unfortunately, due to technological constraints and the gigantic distances involved, most of those missions only weigh a few grams and require massive solar scales or pushing lasers to get anywhere near their target. But why let modern technological levels limit your imagination when there are so many other options, if still theoretical, options to send a larger mission to our nearest potentially habitable neighbor? That was the thought behind the Master’s Thesis of Amelie Lutz at Virginia Tech - she looked at the possibility of using fusion propulsion systems to send a few hundred kilogram probe to the system, and potentially even orbit it.
One of the most iconic cosmic scenes in the Universe lies nearly 3.8 billion light-years away from us in the direction of the constellation Carina. This is where two massive clusters of galaxies have collided. The resulting combined galaxies and other material are now called the Bullet Cluster, after one of the two members that interacted over several billion years. It's one of the hottest-known galaxy clusters, thanks to clouds of gas that were heated by shockwaves during the event. Astronomers have observed this scene with several different telescopes in multiple wavelengths of light, including X-ray and infrared. Those observations and others show that the dark matter makes up the majority of the cluster's mass. Its gravitational effect distorts light from more distant objects and makes it an ideal gravitational lens.
What new methods can be developed in the search for extraterrestrial intelligence (SETI)? This is what a recent white paper submitted to the 2025 NASA Decadal Astrobiology Research and Exploration Strategy (DARES) Request for Information (RFI) hopes to address as a pair of researchers from the Breakthrough Listen project and Michigan State University discussed how high-energy astronomy could be used for identifying radio signals from an extraterrestrial technological civilization, also called technosignatures. This study has the potential to help SETI and other organizations develop novel techniques for finding intelligent life beyond Earth.
In the past fifteen years, five missions have returned samples of extraterrestrial material to Earth for analysis. These included missions that rendezvoused with Near Earth Asteroids (NEAs), like the Hayabusa 1 and 2 and the OSIRIS-REx missions, and the Chang'e-5 and -6 missions, which brought back samples from the far side of the Moon. In the coming years, China plans to return samples from 469219 Kamoʻoalewa with its Tianwen-2 mission. With all the extraterrestrial materials being returned to Earth for analysis, one could argue that we are entering a "golden age of sample-return missions."
Astronomers have achieved a first in exoplanet hunting by using the Hubble Space Telescope images to investigate a mysterious event that could reveal the existence of a "rogue planet" drifting through space without a host star.
For generations, humans have gazed at the stars and wondered about the ultimate fate of the Universe. Will it expand forever into the cold emptiness, or meet a more dramatic end? A new study published by physicists from Cornell University, Shanghai Jiao Tong University, and other institutions suggests we may finally have an answer, and it's surprisingly specific.
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