Saturday, March 21, 2026

How Will Martian Gravity Affect Skeletal Muscle?

Astronauts working outside a habitat on the surface of Mars. Credit: NASA

Marie Mortreux, an assistant professor in the University of Rhode Island’s College of Health Sciences, is part of an international team of researchers studying how the Mars’s gravity would affect astronauts’ skeletal muscle.



Friday, March 20, 2026

Saturn-mass world discovered orbiting two low-mass stars

Artist's illustration of an exoplanet orbiting two stars. (Credit: NASA/JPL-Caltech/T. Pyle)

You just established a settlement on an Earth-like planetary body far from our solar system. You did your evening chores after eating dinner, and you want to go out for the evening view, which consists of two setting stars, reminiscent of the infamous scene in Star Wars. However, there’s one major difference: a large planetary body is in the sky. As you were aware before arriving, you’re on an exomoon orbiting a Saturn-sized exoplanet, both of which orbits two stars.



This Pair Of Brown Dwarfs Can't Get Enough Of Each Other

Astronomers have found binary pair of brown dwarfs that are transferring mass from one to another. Though mass transfer between binary objects isn't rare, this is the first time it's been observed in brown dwarfs. The pair will either eventually merge and become a brighter star, or one will continue to become more massive and eventually ignite fusion. Image Credit: Caltech/R. Hurt (IPAC)

Astronomers have found the first case of a brown dwarf binary pair experiencing mass transfer. The pair are very close to one another, with an orbital period of only 57 minutes. The pair will eventually merge into one, brighter star, or the accretor will become massive enough to trigger fusion. At only 1,000 light-years away, the system is a strong candidate for more detailed, follow-up observations.



This Super-Puff Planet is Hiding its True Nature Behind Thick Haze

This artist's illustration shows Kepler-51d orbiting its Sun-like star about 2,600 light-years away. The exoplanet is a super-puff planet, an odd type of world with extremely low densities. It's unclear how these types of planets form, and new research uses JWST observations to try to understand them. Unfortunately, the exoplanet's thick haze poses a challenge. Image Credit: NASA, ESA, and L. Hustak, J. Olmsted, D. Player and F. Summers (STScI).

Super-puff planets have extremely low densities, and exoplanet scientists aren't sure why. They seem to defy our understanding of how planets form. Researchers used the JWST to observe the atmosphere of Kepler-51d, one of the puffiest of the super-puffs. Unfortunately, even the powerful space telescope found a featureless spectrum. What does it mean?



The Sun’s Long-Lived Active Regions Are Massive Flare Factories—But We Don’t Know Why

Image of multiple ARs on the Sun in May 2024. Credit - NASA Visualization Studio

Space weather is a fascinating subject, but one we still have a lot to learn about. One of the main components of it is the active regions (ARs) of the Sun. These huge concentrations of magnetic fields show up throughout the Sun’s photosphere and are the primary source of solar flares and coronal mass ejections (CMEs). They can be simple pairings of magnetic flux or huge, magnetically complex tangles that spend weeks creating massive solar storms before dissipating. But tracking the longest lived of these ARs has been a headache for solar physicists, and a recent paper by Emily Mason and Kara Kniezewski, published in The Astrophysical Journal, both dives into this tracking problem and uncovers some interesting features of the Sun’s most persistent ARs.



Thursday, March 19, 2026

Canada Allocates $200 Million Towards the Creation of Nation's First Spaceport

Minister of National Defence David McGuinty speaks at an announcement on Canada’s sovereign space program, with parliamentary secretary Jenna Sudds, left, and Space Canada CEO Brian Gallant, right. Credit: Justin Tang/The Canadian Press

Minister of National Defence David McGuinty announced on Monday, March 16th, that the Canadian government is committing $200 million to develop Canada's first commercial spaceport in Nova Scotia, which will be run by Maritime Launch Services.



The Crab Pulsar's Puzzling Emissions Finally Explained.

The Crab Nebula is one of the most well-studied objects in astronomy. A pulsar is in the center of the nebula, and pulsars emit radio waves. Most pulsar radio emissions are broad and noisy, but the Crab's are in a sort of zebra pattern. New research has figured out why. Image Credit: NASA/JWST

Pulsars are rapidly rotating neutron stars. The Crab Pulsar, an often studied supernova remnant, is known for its unusual radio emission patterns. New researchs says it's because of a "tug-of-war" between magnetism and gravity. Gravity acts as a focusing lens and plasma in the magnetosphere acts as a defocusing lens.



Sometimes You Get Lucky, Just Like the Hubble Did When It Caught This Comet Disintegrating

These three sequential images from the Hubble Space Telescope caught Comet K1 as it broke into pieces. This is the first time that the telescope has captured the early stages of a comet breaking apart. K1 had passed perihelion and was on its way out of the Solar System. Image Credit: NASA, ESA, D. Bodewits (Auburn). Image processing: J. DePasquale (STScI)

A team of astronomers were fortunate when their original comet target couldn't be observed with the Hubble. They quickly pivoted to a different target, and caught Comet K1 in the process of breaking apart. This gave them an excellent opportunity to learn more about the doomed object.



JUICE is Planning To Do Science On Jupiter's "Minor" Moons Too

Artist's impression of JUICE arriving at the Jupiter system. Credit - ESA (acknowledgement: ATG Medialab)

The European Space Agency’s (ESA’s) Jupiter Icy Moons Explorer (JUICE) probe is on its (very long) way to Jupiter, and will finally arrive at the King of Planets in 2031. Its primary mission is to focus on the “big three” icy moons - Ganymede, Europa, and Callisto. But while JUICE is busy mapping Ganymede’s magnetic field, it will also be keeping a sharp eye on the other 94 moons in the Jupiter system. A recent paper published in Space Science Reviews by Tilmann Denk of DLR, Germany’s space research association, and his co-authors showcases just how much “bonus science” JUICE is expected to squeeze out of these other targets.



Wednesday, March 18, 2026

Something is Changing the Small Magellanic Cloud

The Small Magellanic Cloud Imaged by the Herschel mission, Planck observatory, Infrared Astronomical Satellite, and Cosmic Background Explorer. Credits: ESA/NASA/JPL-Caltech/CSIRO/NANTEN2/C. Clark (STScI)

A strange lack of stellar orbits around the core of the Small Magellanic Cloud (SMC) mystified astronomers for decades. Not only that, but the SMC has a strange, irregular shape, and sports a tidal. Now, a team of observers led by graduate student Himansch Rathore at the University of Arizona, has tracked down the reason why the stars don't orbit. It's because the SMC crashed directly through its neighbor, the Large Magellanic Cloud (LMC), in the distant past. That huge collision disrupted stellar motions and [sent them on wildly different trajectories](https://ift.tt/7Obtc31). It also disturbed the clouds of gas within the SMC and created a tail of gas stretching out across space.



NASA Exoplanet-Hunting CubeSat Delivers "First Light" Images

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With the first images from the spacecraft now in hand, the team behind NASA’s Star-Planet Activity Research CubeSat (SPARCS) is ready to begin charting the energetic lives of the galaxy’s most common stars to help answer one of humanity’s most profound questions: Which distant worlds beyond our solar system might be habitable?



Tuesday, March 17, 2026

CERN Adds a New Particle to Large Hadron Collider's Subatomic Zoo

An artist’s impression shows the composition of the newly discovered subatomic particle, with two charm quarks and one down quark. (Credit: CERN)

Scientists at Europe's CERN research center say the Large Hadron Collider's LHCb experiment has discovered a "doubly charmed" particle that's like a proton, but four times as weighty.



Scientists Find Evidence of Worlds Colliding ... 11,000 Light-Years Away

An artist's conception shows a planetary collision around a distant star. (Credit: Andy Tzanidakis / Univ. of Washington)

Astronomers say unusual readings from a star system 11,000 light-years away suggest that two of the planets circling the star crashed into each other, creating a huge, light-obscuring cloud of rocks and dust.



Is the Universe Defective? Part 4: Hiding in Plain Darkness

Credit: X-ray: NASA/CXC/CfA/M. Markevitch; Optical/Lensing: NASA/STScI, Magellan/U. Arizona/D. Clowe; Lensing map: ESO WFI

The WHAT? Yeah, the vortons. It’s not an anime monster-hunting show. It’s not some AI startup company. It’s a…it’s a thing. I think.



New Study Complicates the Search for Alien Oxygen

Artist's depiction of TRAPPIST-1 b. Credit - NASA, ESA, CSA, J. Olmsted (STScI), T. P. Greene (NASA Ames), T. Bell (BAERI), E. Ducrot (CEA), P. Lagage (CEA)

Oxygen has been the most important gas in our search for life among the cosmos thus far. On Earth, we have it in abundance because it is produced by biological synthesis. But that might not be the case on other planets, so even if we do find a very clear high oxygen signal in the atmosphere of an exoplanet, it might not be a clear indication that life exists there. A new paper, available in pre-print on arXiv, from Margaret Turcotte Seavey and a team of researchers from institutions like the NASA Goddard Space Flight Center and Johns Hopkins University, adds some additional context to what else might be going on in those atmospheres. In particular, they note that if there’s even a little bit of water vapor, it can make a big difference in whether a lifeless rock looks like a living, thriving world.



Monday, March 16, 2026

The Coming Age of Space Stations

International Space Station in 2011, as seen during the last spaceflight of the Space Shuttle Endeavor (STS-134). Credit: NASA

With the ISS set to retire in 2030, several plans are in place to replace it. These include existing space stations, proposals by rising national space agencies, and commercial space stations. With multiple outposts in orbit, the potential for research, development, and even conflict is considerable!



Are Rogue Exomoons the Newest Frontier in the Search for Habitability?

This AI-generated illustration shows an exomoon orbiting a free-floating planet. New research shows that there are some evolutionary pathways where exomoons orbiting rogue planets could be warm enough for liquid water. It also says that these habitable conditions could last for billions of years. There's at least a chance that complex life could arise in the right circumstances on rogue planet exomoons. Image Credit: D.Dahlbüdding / ChatGPT / DALL·E

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.



Microscopic "Ski-Jumps" Could Shrink Spacecraft LiDAR to the Size of a Microchip

Image of the "ski jumps" on the photonic chip. Credit - MIT / M. Saha et al.

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.



Sunday, March 15, 2026

The Sun's Great Escape

The Sun is now thought to have left its original location in the Milky Way as part of a mass migration (Credit : Matúš Motlo)

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.



Is the Universe Defective? Part 2: The Persistence of Memory

Credit: Frank Summers (STScI), Martin White & Lars Hernquist (Harvard)

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



Saturday, March 14, 2026

The Seven Hour Explosion Nobody Could Explain

Positions on the sky of all gamma-ray bursts detected during the BATSE mission (Credit : NASA)

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!



NASA's DART Mission Also Changed Didymos' Orbit Around Sun

This image of asteroids Didymos, left, and Dimorphos was captured by NASA’s DART mission a few seconds before the spacecraft smashed into Dimorphos on Sept. 26th, 2022. Credit: NASA/Johns Hopkins APL

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.



Is the Universe Defective? Part 1: The Good Old Days

Credit: ESA and the Planck Collaboration

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.



The Universe's Most Powerful Particle Accelerators Were Here All Along

Cutaway drawing of two radiation belts around Earth; the inner belt (red) dominated by protons and the outer one (blue) by electrons. (Credit : JHUAPL, NASA)

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.



Friday, March 13, 2026

A Glorious Spiral of Star Formation

This is the spiral galaxy NGC 5134, captured by the JWST in both near-infrared and mid-infrared. Images of nearby spiral galaxies like this one are important for studying star formation. The image is the ESA's Picture of the Month. Image Credit: ESA/Webb, NASA & CSA, A. Leroy

Stars peek through the dusty, winding arms of NGC 5134, a spiral galaxy located 65 million light-years away, in this Feb. 20, 2026, image from NASA’s James Webb Space Telescope. Webb’s Mid-Infrared Instrument collects the mid-infrared light emitted by the warm dust speckled through the galaxy’s clouds, tracing the clumps and strands of dusty gas. The telescope’s Near Infrared Camera records shorter-wavelength near-infrared light, mostly from the stars and star clusters that dot the galaxy’s spiral arms. The image helps researchers understand star formation in spiral galaxies. Image Credit: ESA/Webb, NASA & CSA, A. Leroy



Why Are Interstellar Comets So Weird? Part 4: We Finally Turned On the Porch Lights

Credit: NSF–DOE Vera C. Rubin Observatory/NOIRLab/AURA/H. Stockebrand

So that's all nice. But why now? That's the question everyone asks. We went decades — centuries, millennia really — without seeing a single rock that didn't have a "Made in the Solar System" sticker on it. Then, in the span of less than ten years, we get the Big Three: 'Oumuamua, Borisov, and now 3I/ATLAS.



Thursday, March 12, 2026

ESA's Mars orbiters watch solar superstorm hit the Red Planet

Images of the 2024 solar storm captured by NASA's Solar Dynamics Observatory's instruments, developed by the ESA/NASA. The bright spots to the right of the Sun are Jupiter and Venus. Credit: NASA/ESA

What happens when a solar superstorm hits Mars? Thanks to the European Space Agency’s Mars orbiters, we now know: glitching spacecraft and a supercharged upper atmosphere.



This Isn't Just Another Rocky World Orbiting a Red Dwarf. This One's Special

This artist's illustration shows an exoplanet orbiting a dim red dwarf star. There are many unanswered questions about the survival of atmospheres on rocky world around M-dwarfs like this. Astronomers have found a red dwarf with an orbiting rocky exoplanet that is so well-understood it can serve as a benchmark for studies of exoplanet atmospheres. NASA/ ESA/ CSA/ Joseph Olmsted (STScI)/ Webb Space Telescope.

Rocky planets are found in abundance around M-type stars (red dwarfs), so finding another one doesn't always generate headlines. But an international team of astronomers say that one recent M-dwarf rocky planet found by TESS is especially noteworthy. This one can serve as a benchmark for comparative studies of this type of exoplanet and their at-risk atmospheres.



Why Are Interstellar Comets So Weird? Part 3: They SHOULD Be Weird

Credit: NASA, ESA, David Jewitt (UCLA)

So why should we expect interstellar comets like 3I/ATLAS and 'Oumuamua and even to some extent Borisov to be different-different?



"Ionic Liquids" Could Redefine the Habitable Zone

Artist's impression of exoplanet Kepler 1649c. Credit - NASA/Ames Research Center/Daniel Rutter

“Follow the water” has been a guiding mantra of astrobiology, and even space exploration more generally for decades. If you want to find life, it makes sense to look for the universal solvent that almost all types of life on Earth use. But what if life doesn’t actually need water to live or even evolve? A recent paper, available in pre-print on arXiv by researchers at MIT, including Dr. Sara Seager, and the University of Cardiff, proposes an alternative to water as the basis for life - ionic liquids (ILs) and deep eutectic solvents (DES). These liquids could allow life to exist in environments we had once thought were far too hot, too cold, or too barren to support life, and could dramatically change our search for it throughout the cosmos.



Wednesday, March 11, 2026

New Study Says There's a Way to Make Dyson Bubbles and Stellar Engines Stable

Megastructures like Dyson Bubbles, Swarms, and Stellar Engines could be designed to be passively stable. Credit: Kevin Gill

While megastructures are clearly speculative, new research shows that they can (in theory) be built in a way that ensures long-term stability. These findings can provide insight into the properties of potential technosignatures in search for extraterrestrial intelligence studies.



Finding Gold In A Stellar Explosion

This artist's illustration shows a group of merging galaxies about 8.5 billion years away. A pair of merging neutron stars in one of these galaxies caused a kilonova explosion that generated what could be the most distant gamma-ray burst ever detected. Image Credit: Maria Cristina Fortuna/NASA/Chandra X-ray Center.

NASA telescopes have detected what could be the most distant gamma-ray burst ever detected. A merging pair of neutron stars generated when they merged and exploded as a kilonova. It happened in an unusual location: a tidal stream of debris created by a group of merging galaxies.



Why Are Interstellar Comets So Weird? Part 2: Why Comets Are Like Cats

Credit: Halley Multicolor Camera Team, Giotto Project, ESA.

Once you start listing the properties of 3I/ATLAS, it becomes clear pretty quickly that this thing is distinctly different from any other comet we've ever seen. Here's just a small taste.



Tuesday, March 10, 2026

New Study Addresses Clotting Risks for Female Astronauts

A new study shed new light on how blood clots could threaten female astronauts. Credit: NASA

Just a few days in simulated microgravity can subtly change the way women’s blood clots, sparking bigger questions about health monitoring protocols for astronauts who can spend six months or more in orbit, say Simon Fraser University researchers.



Sunday Morning's European Fireball Was Probably Only a Few Meters in Diameter

The fireball above Germany on Sunday March 8th, 2026. It glowed for about 6 seconds, and some observers even heard it from the ground. Image Credit: ALLSKY7 / Bernd Klemt – AMS76 Herkenrath/DE

Multiple mobile phones, dashcams, and dedicated meteor cameras capture a fireball over part of Europe on Sunday night. Thousands of people witnessed it, and the ESA's Planetary Defence Team is analyzing it. So far, it looks like it was a few meters in diameter. It lit up the sky, and some debris even struck some buildings in Koblenz, Germany.



The Rubin Observatory's LSST Will Detect Imminent Impactors Before They Crash Into Earth

This artist's illustration shows asteroids moving in Earth's vicinity. The Vera Rubin Observatory's Legacy Survey of Space and Time will detect many more small rocks that are about to strike Earth, giving ample time for follow-up observations with other telescopes. Not only does this mean we'll learn more about the Near Earth Object population, but we will be able to recover more of them. Image Credit: ESA/P.Carril

One of the Vera Rubin Observatory's objectives is to detect incoming objects. It's decade-long Legacy Survey of Space and Time will detect one-meter class objects about to impact Earth and allow more detailed observations of them. That will help determine their impact sites with greater accuracy, allowing for more recovery.



The Answer is Written in the Stars

The stars of the Milky Way captured above Paranal, Chile on 21 July 2007, taken by ESO astronomer Yuri Beletsky (Credit : ESO/Y. Beletsky)

Astronomers have turned to some of the oldest stars in our Galaxy to tackle one of cosmology's most stubborn puzzles and their answer might surprise you. By analysing precise age data for more than 200,000 Milky Way stars, researchers have placed the age of the universe at around 13.6 billion years. It's a deceptively simple idea that the universe cannot be younger than the stars it contains. What they found doesn't just give us a number, it adds a compelling new dimension to a decades long argument that has divided the scientific world.



Aliens Might Have Their Radio Signals Blurred By Their Star's Solar Wind

Depiction of an active red dwarf and its nearby planet. Credit - NASA

Back in the early 2000s, my computer screen, like that of many other space enthusiasts, was typically covered in a series of rainbow-colored spectral signals. As my computer crunched through thousands of data points of radio signals collected by the SETI@Home initiative, I was hoping I was in some small way contributing to one of humanity’s greatest scientific endeavours - the search for extraterrestrial life. But, according to a new paper published in The Astrophysical Journal by Vishal Gajjar and Grayce Brown of the SETI Institute, it seems unlikely that the signals SETI@Home was tailored to look for actually exist. That doesn’t mean there weren’t aliens yelling into the void at the top of their electronic lungs, but simply that the space weather from their local star might have changed the signal to make it unrecognizable by the time it reached us.



Scientists Find the First Direct Evidence of Binary Asteroids Sharing Material

One of the final images of Dimorphos' surface, taken about 2 seconds (6 miles) before impact of the DART mission. Credit - NASA/Johns Hopkins APL

Scientists occasionally have a hard time figuring out whether data they are seeing is an actual physical phenomenon or just a trick of their instrumentation. A new paper in The Planetary Science Journal from Jessica Sunshine and their colleagues at the University of Maryland describes one such confusing scenario. In this case, the researchers noted some fan-like patterns across the surface of Dimorphos, the asteroid hit by NASA’s DART mission, and thought it might be a trick of their camera. But after some image correction, computation, and physical experimentation, they determined the patterns were caused by the first-ever documented cases of material transfer between two asteroids.



Monday, March 9, 2026

The JWST Reveals Some Puzzling Surprises in Jupiter's Northern Aurora

This image shows the two auroral footprints in Jupiter's aurora borealis created by the moons Io and Europa. The JWST observed these footprints and provided the first spectral measurements. These showed extreme temperature and densities in Io's footprint, a big surprise to the researchers behind the work. Image Credits: Webb/NIRCam Credit: NASA, ESA, CSA, Jupiter ERS Team; image processing by Judy Schmidt. Webb/NIRSpec Credit: Katie L. Knowles (Northumbria University).

Jupiter's powerful, continuous aurorae dwarf those of Earth. Scientists know that Jupiter's Galilean moons created bright spots on Jupiter's northern aurora. The JWST observed these bright spots and generated infrared spectra of them for the first time. Those observations showed that Io's bright spot is extremely variable in both temperature and density, and researchers want to know why.



How Jagged Moon Dust Could Support Future Astronauts

Chang'e 6 lander on the lunar far side - taken by a small rover accompanying it. Credit - Chinese National Space Agency/Chinese Academy of Sciences

Lunar dust can be a pain - but it’s also literally the ground we will have to traverse if we are ever to have a permanent human settlement on the Moon. In that specific use case, it’s clingy, jagged, staticky properties can actually be an advantage, according to a new paper, recently published in Research from researchers at Beihang University, who analyzed the mechanical properties of samples returned by Chang’e 6 mission to the far side of the Moon.



Terraforming Mars Isn't a Climate Problem—It's an Industrial Nightmare

Realistic image of a completely terraformed Mars. Credit - Daein Ballard

Even when the idea of terraforming Mars was originally put forward, the idea was daunting. Changing the environment of an entire planet is not something to do easily. Over the following decades, plenty of scientists and engineers have looked at the problem, and most have come to the same conclusion - we’re not going to be able to make Mars anything like Earth anytime soon. A new paper available in pre-print on arXiv from Slava Turyshev of NASA’s Jet Propulsion Laboratory, is a good explainer as to why.



Starshade concept could reveal Earth-like exoplanets

Artist's rendition depicting a proposed concept using a space-based starshade and ground-based telescopes to find Earth-like exoplanets. (Credit: Dr. Ahmed Soliman)

Finding Earth-like exoplanets with the composition and ingredients for life as we know it is the Holy Grail of exoplanet hunting. Since the first exoplanets were identified in the 1990s, scientists have pushed the boundaries of finding exoplanets through new and exciting methods. One of these methods is the direct imaging method, which involves carefully blocking out the host star within the observing telescope, thus revealing the orbiting exoplanets that were initially hiding within the star’s immense glare.



Sunday, March 8, 2026

Astronomers Produce the Largest Image Ever Taken of the Heart of the Milky Way

The largest image of the Milky Way's center, captured by the ESO's ALMA array. Credit: ALMA (ESO/NAOJ/NRAO)/S. Longmore et al./ESO/D. Minniti et al.(background)

Astronomers have captured the central region of our Milky Way in a striking new image, unveiling a complex network of filaments of cosmic gas in unprecedented detail. Obtained with the Atacama Large Millimeter/submillimeter Array (ALMA), this rich dataset—the largest ALMA image to date—will allow astronomers to probe the lives of stars in the most extreme region of our galaxy, next to the supermassive black hole at its center.



Saturday, March 7, 2026

Astronauts Use Bacteria and Fungi to Harvest Metals in Space

Michael Scott Hopkins performs a microgravity experiment on the International Space Station. Credit: NASA/ESA

If humankind is to explore deep space, one small passenger should not be left behind: microbes. In fact, it would be impossible to leave them behind, since they live on and in our bodies, surfaces and food. Learning how they react to space conditions is critical, but they could also be invaluable fellows in our endeavor to explore space.



Friday, March 6, 2026

VLT Image Captures a "Cosmic Hawk" Spanning its Wings.

ESO's picture of the week shows a "cosmic hawk" and countless young stars in the RCW 36 nebula. Credit: ESO/A. R. G. do Brito do Vale et al. (2026).

Today’s Picture of the Week, taken with ESO’s Very Large Telescope (VLT), seems to have captured a cosmic hawk as it spans its wings.



The 4.6-Billion-Year-Old Tape Recorder Hidden Inside Asteroid Dust

Images of the surface of Ryugu taken by the navigation camera on Hayabusa-2. Credit - JAXA, Chiba Institute of Technology, University of Tokyo, Kochi University, Rikkyo University, Nagoya University, Meiji University, University of Aizu, AIST

Asteroids are critical to unlock our understanding of the early solar system. These chunks of rock and dust were around at the very beginning, and they haven’t been as modified by planetary formation processes as, say, Earth has been. So scientists were really excited to get ahold of samples from Ryugu when they were returned by Hayabusa-2 a few years ago. However, when they started analyzing the magnetic properties of those samples, different research groups came up with different answers. Theorizing those conflicting results came from small sample sizes, a new paper recently published in JGR Planets from Masahiko Sato and their colleagues at the University of Tokyo used many more samples to finally dig into the magnetic history of these first ever returned asteroid samples.



Thursday, March 5, 2026

Mars Express Images Reveal Mars' Pockmarked Surface

A slice of Arabia Terra, a large plain in Mars’s ancient highlands, imaged by the Mars Express' High Resolution Stereo Camera (HRSC). Credit: ESA/DLR/FU Berlin

Craters, craters, and yet more craters: this snapshot from ESA’s Mars Express is packed full of them, each as fascinating as the last.



Astronomers Using MeerKAT Spot a Cosmic Laser Halfway Across the Universe

A megamaser acts as an astronomical laser that beams out microwave emission rather than visible light. Credit: ESA/Hubble

Astronomers using the MeerKAT radio telescope in South Africa have discovered the most distant hydroxyl megamaser ever detected. It is located in a violently merging galaxy more than 8 billion light-years away, opening a new radio astronomy frontier.



Phew! NASA Rules Out Asteroid Smashup on the Moon in 2032

An animated image shows how NASA has refined the probability of a 2032 lunar impact by asteroid 2024 YR4. The first image shows the range of the asteroid's potential locations based on observations made in the spring of 2025 (4.3% impact probability), and the second image shows the potential locations based on observations made in February 2026 (zero percent impact probability). Credit: NASA / JPL Center for Near-Earth Object Studies.

Here’s one less thing to worry about — or to look forward to: NASA has ruled out any chance that an asteroid called 2024 YR4 will hit the moon in 2032.