Sunday, May 31, 2026

A Brief-ish History of SETI. Part VIII: Paradox? What Paradox?

This illustration shows a hypothetical distant planet inhabited by a technological civilization, with “city lights” visible on the darkened surface. Credit: NASA/JPL-Caltech/Lizbeth B. De La Torre

In recent decades, the Search for Extraterrestrial Intelligence (SETI) has seen a revival, and future surveys will benefit from new technologies. Similarly, our perception of what technologies an advanced civilization might use has expanded.



The Galaxy That Forgot to Spin

Galaxies spin, that's a given, and M101 imaged here is no exception but astronomers have now discovered one that doesn't agree! (Credit : ESA/Hubble)

Every galaxy we know of spins. It's one of those rules of the universe so fundamental that astronomers barely think about it anymore. So when the James Webb Space Telescope pointed at one of the most massive galaxies in the early universe and found…well nothing. No spin, just stillness. They had to look twice.



Did We Invent Dark Energy for Nothing?

This map of the cosmic microwave background is what ultimately forced astronomers to invoke the concept of dark energy but a new study reveals that may not be the case (Credit : NASA/WMAP)

For nearly thirty years, dark energy has been cosmology's great get out of jail free card, the invisible, mysterious force we invented to explain why the universe is expanding faster than it should be. Now a team of mathematicians says we may never have needed it at all. And the implications are stranger than you might think.



It Took a Cosmic Village to Shape Early Galaxies

The Loktak protocluster region that lies some 12.6 billion light-years away. It shows how early cluster environments influence the evolution of young member galaxies. Credit: Laishram et al./NAOJ/NASA/ESA/CSA

An early galaxy cluster named after an Indian lake is teaching astronomers about influences on galaxy evolution in the infant Universe. Astronomer Ronaldo Laishram of the National Astronomical Observatory of Japan (NAOJ) used the Subaru Telescope’s wide-field camera, Hyper Suprime-Cam (HSC), to conduct a large sky survey to look for early galaxies with active star formation. The result was the discovery of a massive protocluster of galaxies that existed some 12.6 billion years ago, very early in cosmic time. Detailed study of this region could give new insight into how galaxies and their clusters form and evolve.



Saturday, May 30, 2026

Lasers at the Lunar Poles Could Help Astronauts Navigate

This view of the lunar south pole captured by the Artemis astronauts showes the heavily cratered terrain of the Aitken basin. Laser installations in shadowed craters could provide navigational aid to astronauts exploring the Moon. Courtesy NASA

A team of scientists is exploring ways to use dark craters at the lunar poles as sites for ultrastable lasers to aid in surface and near-lunar navigation. The group, led by Physicist Jun Ye, an expert on lasers and precision measurements, were discussing the types of instruments that Artemis astronauts could install and use during their time on the Moon.



Who You Send to the Moon Matters More Than You Think

Astronauts working together in close proximity and for extended duration causes stress levels to increase. A team of researchers have modelled what this might look like in a lunar base. Image shows Jessica Watkins and Bob Hines working on XROOTS, an experiment using the Veggie facility of the ISS (Credit : NASA)

Building a permanent base on the Moon sounds like an engineering problem. Design the habitat, sort the power supply, figure out life support, and you're most of the way there. But the engineers who've spent time thinking hard about this will tell you the real challenge isn't the hardware — it's the humans inside it. Now researchers have built a virtual Moon base and run tens of thousands of simulated missions inside it, studying not the rocket engines or the radiation shielding, but the astronauts themselves. What they found could reshape how we plan humanity's return to the lunar surface.



Friday, May 29, 2026

MAVEN Spacecraft Finds New Plasma Squeezing at Mars

Artist’s illustration of the Zwan-Wolf effect at Mars, which is an atmospheric effect involving the solar wind, and was observed by NASA’s MAVEN (Mars Atmosphere and Volatile Evolution) spacecraft in December 2023. (Credit: LASP/CU Boulder)

A cloaked alien invasion force is approaching Earth and coming up on Mars. The first officer looks through a viewfinder and says, “Captain, the fourth planet’s atmosphere is behaving strangely. As though it were trying to block incoming energy.” The captain takes a moment, then his (already big) eyes get wide and he exclaims, “It’s a defense shield! The Earthlings are hiding on the fourth planet and are prepared to attack us! Abort the invasion!” The first officer responds, “Aye aye, Captain!”



Thursday, May 28, 2026

Earthly Hors d'oeuvres For Hungry Red Dwarfs

This illustration shows the red dwarf star TRAPPIST-1 and two of its rocky planets. Researchers detected several red dwarfs just like it that have appeared to have eaten their planets, though TRAPPIST-1 isn't one of them. Planetary engulfment is a rare yet possible outcome of normal planetary system evolution. Image Credit: ESA/Hubble. Licence Type: Attribution (CC BY 4.0)

We know that stars can engulf planets because stars that swell up to become red giants overwhelm any close-in planets. The Sun will do this to Venus, Mercury, and possibly Earth in a few billion years. But research shows that it can happen when low-mass stars first enter the main sequence. Lithium gives it away.



An Orbiting Satellite Triad Reveals Motions Inside Earth

Earth’s magnetic field is thought to be generated largely by an ocean of superheated, swirling liquid iron that makes up Earth’s outer core. That activity generates electric currents and thus the continuously changing electromagnetic field. Courtesy SA/AOES Medialab

Our planet's liquid iron outer core is slowly giving up its secrets to a trio of satellites launched by ESA in 2013. Called Swarm, the three probes have been studying Earth's magnetic field at the source. In the process, they've revealed startling changes in a molten layer region 2,200 kilometers beneath the Pacific Ocean. In 2010, material in that area of Earth's outer core changed direction. Insteading of moving slowly westward, it's now headed east and picking up speed. Scientists are working to figure out why by using the European Space Agency's (ESA) Swarm data and additional information from ESA's CryoSat mission and ground-based instruments.



Just Like Stars, Open Clusters Can Form Binary Pairs

An extended gaseous finger points to the Pismis 24 open star cluster in this JWST NIRCam image. Stars in a cluster are siblings, having been birthed from the same massive cloud of gas. But clusters themselves can also be siblings arranged in binary pairs, and recent research illuminates their heirarchical nature. Image Credit: NASA, ESA, CSA, STScI; Image Processing: Alyssa Pagan (STScI)

Open star clusters are prevalent stellar structures in the Milky Way. Astronomers think their could be 100,000 of them. But they're not all the same: some are binary clusters, and within those, there's a hierarchy based on how they form. Recent research explores the different types and how many of each type is in the Milky Way.



Wednesday, May 27, 2026

When Spacetime Crystallises, a Black Hole is Born

The Event Horizon Telescope captured this image of the black hole at the centre of the galaxy M87. Other black holes are thought to form out of the crystallisation of space time (Credit : Event Horizon Telescope)

Physicists have thought for decades that microscopic black holes can theoretically emerge not from exploding stars but from delicate "critical states" in which space and time organise themselves into a crystal like structure. Now, for the first time, researchers from TU Wien and Goethe University Frankfurt have derived an exact mathematical formula describing this bizarre phenomenon using a surprising trick involving infinitely many dimensions!



The Weirdness of Early Universe SMBHs Gets Even Weirder

This JWST NIRCam image shows Abell2744-QSO1, a prototypical Little Red Dot (LRD) discovered by the JWST. QS01 is magnified and tripled by gravitational lensing from the galaxy cluster Abell 2744. When scientists studied it in detail, they found a 50 million solar mass supermassive black hole (SMBH). It contains twice as much mass as its galaxy, throwing a curveball at astrophysicists trying to understand the growth of SMBH. Image Credit: NASA, ESA, CSA, L. Furtak (Ben-Gurion University), R. Maiolino (Cambridge), F. D'Eugenio (Cambridge), I. Juodžbalis (Cambridge), H. Übler (MPE), C. Marconcini (University of Florence). Image processing: A. Pagan

The JWST has shown us some strange things about supermassive black holes (SMBH) in the early Universe. Many of them are far more massive than we think they should be. Now astronomers working with the JWST have found one that seems to have formed before its galaxy did.



A Natural Chemistry Laboratory in Protostar Shock Waves

Astronomers have studied the outflow from a Class 0 protostar and found complex molecules like methanol. They form in the shockwave environment where the outflows slam into the interstellar medium. Image Credit: NASA, ESA, CSA, STScI

Complex organic molecules (COMS) are at the heart of life. They're created where jets from protostars slam into the interstellar medium, environments that scientists call natural laboratories. In these intense environments, important carbon-bearing molecules are created. Recent research took a close look at one of these jets and found some COMS in them for the first time.



Tuesday, May 26, 2026

When the Sun Tries to Explode and Fails

When observed in white light coronagraph imagery, CMEs sometimes resemble a light bulb, possessing a bright bulb like outer shell surrounding a dark void and compact inner structure. A new discovery reveals why some solar eruptions fail before reaching CME status (Credit : NASA/SOHO)

Scientists have captured one of the most detailed observations ever of a failed solar eruption, a powerful blast from the Sun that built into what should have been a billion tonne plasma ejection, then stalled and collapsed back to the surface. Using data from five spacecraft simultaneously, the team identified a double magnetic process that strangled the eruption from both above and below.



The Definitive Census of Multiple Star Systems Within 10 Parsecs

Artist's concept of a planet orbiting a binary star system. Credit - NASA's Goddard Space Flight Center/Chris Smith (USRA)

Our Sun is a loner. It lacks a stellar companion hurtling through interstellar space with it. But we’ve known for a long time that’s actually relatively rare - most stars have at least one gravitationally bound partner. Understanding how exactly those stars are related to each other is critical for observational campaigns - especially for those of exoplanets. So a new paper from researchers at the University of Madrid that categorizes almost every star within ten light years into companion categories is a welcome addition to the literature on the subject, and could be used to inform the next round of planet habitable planet hunting satellites.



Monday, May 25, 2026

NASA's Next-Generation AI Processor Passes Early Testing

Small enough to fit in the palm of a hand, NASA’s High Performance Spaceflight Computing processor packs the power of a full system-on-a-chip. Credit: NASA/JPL-Caltech

As part of a commercial partnership, NASA is developing a sophisticated chip that will give spacecraft the processing capabilities to think for themselves.



Ultrahigh-energy Cosmic Rays May Be Ultraheavy in Origin

Artist’s impression of an ultra-high energy cosmic ray reaching Earth. Credit: Osaka Metropolitan University/Kyoto University L-INSIGHT/Ryuunosuke Takeshige

New research led by Penn State scientists suggests that some of the highest-energy cosmic rays may consist of atomic nuclei heavier than iron and could help narrow down the cosmic sources capable of accelerating these particles.



Early Life on Earth May Have Thrived in Impact Craters

This artist's illustration shows a pair of asteroids passing by the modern-day Earth. New research shows that impact craters on the ancient Earth could have created "oxygen oases," where hydrothermal activity supercharged the growth of cyanobacteria and their stromatolite structures. It suggests that the Late Heavy Bombardment could have played a role in the oxygenation of Earth's atmosphere, paving the way for complex life. Image Credit: ESA/P.Carril

A team of South Korean scientists has uncovered new evidence that could help explain how Earth’s atmosphere became rich in oxygen, one of the most transformative events in the planet’s history. Researchers from the Korea Institute of Geoscience and Mineral Resources (KIGAM) report the finding of stromatolites, layered structures formed by microbial communities, within the Hapcheon impact crater on the Korean Peninsula. While the Hapcheon crater is only about 40,000 years old, it shows how stromatolites got a boost from the heat in impact crater hydrothermal systems.



Sunday, May 24, 2026

Alien life may be missed by current space missions, but AI might help

Illustration depicting how alien life could be incorrectly identified on some worlds while being correctly identified on other worlds. (Credit: NASA)

It’s 2035 and NASA’s Dragonfly quadcopter has been “hopping” around the surface of Saturn’s largest moon Titan for just over a year taking images, scanning pebbles, drilling holes, and analyzing surface material for potential signs of life. You’re at NASA JPL and just moved to Blue Team (12am-8am) from Red Team (4pm-12am), so you’re hyped up on coffee, Red Bull, and will power. It’s 3:30am, you’ve been analyzing data since you clocked in, and you keep discarding what you’ve been told looks like positive signs of life but is more commonly known as false positives. In the meantime, some microbes on Titan that got scanned by Dragonfly keep posing in front of its main camera with signs saying, “We’re here!”



Friday, May 22, 2026

Is Dust the Best Thing in the Universe? Part 4: We Owe Dust Our Lives

The protoplanetary disk around the young star HL Tau, imaged by ALMA. The dark gaps are where dust has accumulated into proto-planets, with the bright rings showing the dust grains that haven't yet combined into anything larger. (CC BY 4.0, ALMA / ESO / NAOJ / NRAO)

No dust, no way to cool a collapsing gas cloud. No way to cool it, no stars. No dust, no first rung on the ladder from grain to pebble to planet. The substance I spent two articles complaining about turns out to be the substance that makes me possible.



NASA’S Juno Makes Closest Ever Approach To Jupiter’s Moon Of Thebe

New NASA Juno image of Jupiter's tiny moon of Thebe presented at the EGU26 general assembly early this month. Credit: NASA via Bruce Dorminey

NASA’S Juno spacecraft images Jupiter’s tiny moon of Thebe in a recent close approach.



A Beautiful Death: How a Dying Star Created the Crystal Ball Nebula

The 8.1-meter Gemini North telescope on the summit of Maunakea in Hawai‘i captured this image of the Crystal Ball Nebula. It's about 1500 light-years away, and was discovered in 1790. It's a double-shell nebula and a binary pair of stars sits inside the delicate, gaseous shell. Image Credit: International Gemini Observatory/NOIRLab/NSF/AURA

Image Processing: J. Miller & M. Rodriguez (International Gemini Observatory/NSF NOIRLab), T.A. Rector (University of Alaska Anchorage/NSF NOIRLab), D. de Martin & M. Zamani (NSF NOIRLab)

Planetary nebula are created when a dying star sheds it outer layers. The gas is lit up by the star and all the gorgeous, changing detail is exposed. NGC 1514, the Crystal Ball Nebula, is about 1500 light years away and contains a binary pair in its center. The orbits and winds from the stars create the Crystal Ball's beautiful form.



Supermassive Black Holes Can Render Exoplanets Uninhabitable at Great Distances

This artist's illustration shows a spinning SMBH at the center of its AGN. New research shows how AGN affect exoplanet habitability. The powerful energy can strip away atmospheres and ozone at great distances, shaping habitability in large portions of a galaxy. Image Credit: National Aeronautics and Space Administration / Jet Propulsion Laboratory-Caltech.

Life on Earth relies on energy from astrophysical sources. But what if the astrophysical source isn't a star, but a supermassive black hole and its active galactic nuclei? Life needs shelter from their powerful energy, and the only shelter is distance. New research shows that SMBH and their AGN could strip away exoplanet atmospheres and destroy their ozone at vast distances.



Is Dust the Best Thing in the Universe? Part 3: Tiny Chemistry Labs

Barnard 68, a dark molecular cloud where dust grains shield the densest interior from UV radiation and catalyze the formation of complex molecules. (CC BY 4.0, ESO)

Two hydrogen atoms can't form an H2 molecule on their own in empty space. They need a surface. The universe has only one surface available, and it's something I have just spent two articles complaining about.



Thursday, May 21, 2026

Crypto Investor Works on a Plan to Ride SpaceX's Starship Around Mars

Mission commander Chun Wang works on his laptop with Earth looming outside the window of SpaceX's Dragon capsule during the Fram2 mission in 2025. (Chun Wang / SpaceX via X)

Chinese-born cryptocurrency investor Chun Wang has become the latest deep-pocketed space enthusiast to set his sights on a trip around Mars. But first, he wants to take a ride around the moon on SpaceX's Starship. And SpaceX is willing to work with him.



Both Hemispheres of 3I/ATLAS Observed Simultaneously by JUICE and Europa Clipper

Image of 3I/ATLAS captured by the Subaru Telescope on December 13th, 2025. Credit: NAOJ

The Southwest Research Institute-led Ultraviolet Spectrograph (UVS) instruments aboard ESA’s Jupiter Icy Moons Explorer (Juice) spacecraft and NASA’s Europa Clipper made unique observations of interstellar comet 3I/ATLAS in late 2025. SwRI leads the UVS instruments on both spacecraft, simultaneously imaging both hemispheres of the comet and detecting the comet’s ultraviolet emissions.



The Magnetar at the Heart of a Superluminous Supernova

This artist's illustrations shows a superluminous supernova, which can be 100 times brighter than a "regular" supernova. Their cause is debated, and figuring it out comes down to detecting gamma rays from superluminous supernova. That's been very difficult to do, but one group of researchers may have figured it all out. Image Credit: NASA/Dana Berry/Skyworks Digital

Superluminous supernovae are the royalty in the supernova world. They're up to 100 times brighter than a standard supernova, and astrophysicists want to know why. New research shows that magnetars are responsible.



Wednesday, May 20, 2026

Hellish Venus-Like Planets May Be More Prevalent Than True ExoEarths

Processed using ultraviolet (365nm & 283nm) filtered images of Venus taken by Akatsuki on December 23 2016. JAXA/ISAS/DARTS/Kevin M. Gill via Wikipedia

Exoplanet hunters are keen to find the next extrasolar earthlike planet, one that may harbor life as we know it. But preliminary results from a new study indicate that our galaxy may be filled with a plethora of exo-Venuses. Yet as one exoplanetary researcher notes: the template for such exo-worlds --- our own Venus --- has been ‘criminally underexplored.’



NASA's Psyche Mission Says Goodbye to Mars and Heads for its Metal-Rich Target

NASA's Psyche captured this false colour image of Mars during its recent flyby of the planet on May 15th. The spacecraft captured this image with its multispectral imager. The flyby was a trial run for its encounter with the asteroid Psyche, and was also a gravity-assist maneuver that helped send the spacecraft on its way. Image Credit: NASA/JPL-Caltech/ASU

Spacecraft often use planets for gravity-assist or "slingshot" maneuvers. NASA's Psyche mission used Mars for that purpose during a May 15th flyby. The flyby accelerated the spacecraft and aimed it at its eventual destination, the asteroid 16 Psyche. The flyby was also an opportunity to take some pictures of Mars, and to test and calibrate the spacecraft's science instruments.



It Looks Like Europa Doesn't Have Plumes of Water Vapour After All

This artist's illustration shows what the water vapour plumes tentatively detected on Jupiter's icy moon Europa would look like. A 2014 paper based on Hubble observations showed that these intermittent plumes reach 200 km above Europa's surface. In the following couple of years, subsequent research also found them. But new research from the original discoverers is reconsidering the original findings. Image Credit: University of Cologne.

In 2014, researchers presented the discovery of water vapour plumes being emitted from Jupiter's moon Europa. This caused quite a stir; it meant that the moon's buried ocean was accessible without contending with the thick ice shell that concealed it. But new research by the same researchers questions those detections.



Hearing the Heavens - Book Review of The Echoing Universe

Cover image of The Echoing Universe. Credit - Dr. Emma Chapman / Basic Books

Typically when we think of astronomy, we think of pictures of M87 captured on a backyard telescope or the soaring colorful peaks of the Eagle Nebula seen by Hubble. But perhaps the most influential type of astronomy of the last 100+ years doesn’t directly result in the stunning pictures we’re so accustomed to today. It captures radio waves from some of the most interesting objects in the universe. And in her new book, The Echoing Universe: How Radio Astronomy Helps Us See the Invisible, Dr. Emma Chapman, a radio astronomer at the University of Nottingham, tracks how these longest wavelengths of the electromagnetic spectrum have influenced the practice of astronomy and our understanding of our place in the universe.



Is Dust the Best Thing in the Universe? Part 1: The Apology Begins

Apollo 17 commander Gene Cernan on the lunar surface, his spacesuit caked in moondust that proved to be one of the most persistent engineering problems of the mission. (Public domain, NASA)

Years of grievance against dust. It ruins lungs, suits, rovers, and Mars missions. The first installment of an apology, sort of, to the most annoying substance in the cosmos.



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.



New Algorithm Cracks the Asteroid Routing Problem

An example of an exact orbital trajectory between 10 different asteroids. Credit - Isaac Rudich

The Traveling Salesman is a classic problem in mathematics that requires a solution to the most efficient path to take to visit a given number of cities in the least amount of time. But scale this relatively simple concept up to space travel and the calculation becomes much more complex. Instead of visiting a stationary spot on Earth, when calculating the most efficient path to visit asteroids you must account for the fact they are traveling tens of thousands of miles an hour, and their exact position will change based on when a spacecraft leaves. This is known as the Asteroid Routing Problem, and a new paper from a group of Canadian and European researchers lays out a framework that can find the exact solution to any particular combination of asteroids to be visited.



Sunday, May 17, 2026

What If the Universe Had No Beginning? Part 2: No Boundary, No Problem

Stephen Hawking, whose no-boundary proposal argued that asking what came before the big bang is like asking what is south of the south pole. (Public domain, NASA StarChild)

Hawking faced a question with no answer hiding behind it. The best boundary condition for the universe, he decided, was that there was no boundary at all. To make that statement into physics, he had to do something deeply strange to time.



Friday, May 15, 2026

Bizarre Venus Surface Formations Puzzle Planetary Scientists

Venus image made with data made available by NASA shows the planet  from the Magellan spacecraft and Pioneer Venus Orbiter. Credit: NASA/JPL-Caltech

Enigmatic crownlike surface formations on Venus hold keys to understanding our twin planet’s deep interior. Or so says a new paper presented at the recent European Geosciences Union 2026 general assembly in Vienna.



Turbulence in the Milky Way's ISM Distorts Light from Distant Quasars

The left-hand side of this artist's illustration shows the distant quasar TXS 2005+403 as it really appears, with its bright accretion disk and its powerful astrophysical jets blasting radiation into the cosmos. The right-hand side shows how intervening turbulent gas blurs and distorts the light. New research has figured out exactly how that turbulence affects images of the Milky Way's supermassive black hole. Image Credit: Melissa Weiss/CfA

We may be getting better images of the Milky Way's supermassive black hole in the future. Astronomers used 10 years of observations of a distant blazar to detect turbulence in the Milky Way's interstellar medium. This turbulence makes images of Sagittarius A-star blurry.



NASA Captures Volatile Changes in Earth's Artificial Light

Some parts of the planet are shown to brighten (gold) and some dim (purple) in an analysis of nearly a decade of nighttime lights data from NASA's Black Marble product. NASA Earth Observatory/Michala Garrison

A study of NASA's Black Marble data reveals a pattern of regional volatility in nighttime illumination across the planet.



Thursday, May 14, 2026

We've Been Listening for Ten Years. Here's What We Heard

A study has listened to 70,000 stars and planetary systems for signs of life! (Credit : ESO/Y. Beletsky)

For ten years, astronomers at UCLA have been pointing one of the world's most powerful radio telescopes at the stars and listening. Not for pulsars or gas clouds, or the hiss of the cosmic microwave background, but for something far more extraordinary. A signal from another civilisation. The result of a decade's work, 70,000 stars, and 100 million candidate signals is now in and every single one of them was us! But far from being a disappointment, the findings are among the most rigorous and revealing in the history of the search for extraterrestrial intelligence.



UC Student Gets a Closer Look at Lonely Gas Giant

Artist's rendering of the exoplanet TOI-2031A b, a "Hot Jupiter" 901 light-years from Earth. Credit: NASA

University of Cincinnati astrophysicist Paul Smith is part of an international team studying TOI-2031Ab, a gas giant orbiting a star 901 light years from Earth. Smith and his colleagues used the James Webb Space Telescope to study its atmosphere.



The Roman Space Telescope is Ahead of Schedule, and the Hubble is Giving it a Jump Start

This is a near-infrared image from the ground-based VISTA VVV Survey.  It shows the Milky Way's galactic bulge, with the location of the Nancy Grace Roman Space Telescope's Galactic Bulge Time Domain Survey superimposed over the regions the Hubble surveyed with its instruments. The Hubble's survey was completed in order to give astronomers a leg up in understanding and interpreting the Roman's results. Image Credit: NASA, Alyssa Pagan (STScI); Acknowledgment: VISTA, Dante Minniti (UNAB), Ignacio Toledo (ALMA), Martin Kornmesser (ESO)

One of the core community surveys of NASA’s Nancy Grace Roman Space Telescope, the Galactic Bulge Time-Domain Survey, is expected to locate over a thousand exoplanets that orbit far away from their stars, beyond the orbital distance of Earth from the Sun. Although Roman hasn’t launched yet, astronomers already are gathering useful supporting data by utilizing NASA's Hubble Space Telescope, which could assist astronomers in analyzing Roman data.



We've Been Wasting 99% of Our Supernova Data

SN 1994D (bright spot on the lower left), a Type Ia supernova within its host galaxy, NGC 4526 (Credit : NASA/ESA)

Every time an astronomer points a telescope at a distant supernova, they're trying to measure how far away it is. But the light from these stellar explosions arrives tangled up with interference from dust, the age of the host galaxy and the chemical make up of the original star . Unpicking it all has always been a painstaking business. Now a team of researchers has used artificial intelligence to cut through the noise in a single step, potentially making cosmological measurements four times more precise. In a universe full of unanswered questions, that's a very significant leap forward.



Wednesday, May 13, 2026

A Brief-ish History of SETI. Part IV: Arecibo and the WOW! Signal

Artist's impression of the Arecibo Message (left), aerial view of the Arecibo Radio Telescope (right). Credit: Arne Nordmann/Wikimedia/NIAC

During the 1970s, pioneering experiments were conducted that are known today as Messaging Extraterrestrial Intelligence (METI). At the same time, NASA launched four spacecraft bound for interstellar space, each carrying "messages in a bottle" intended for extraterrestrial beings.



Forget Searching for Individual Biosignatures. Instead, Find Their Patterns

This artist's illustration symbolizes the search for individual chemicals that are biosignatures. But new research shows how fruitless this search might be, and how searching for statistical patterns in amino acids and lipids could be the way forward in the search for life elsewhere in the Solar System. Image Credit: NASA

The search for life elsewhere focuses on biosignatures. These are chemicals in atmospheres that can only be attributed to life. But despite the prowess of the JWST, finding slam-dunk proof of life on other worlds is a confounding exercise. New research suggests that rather than focus on individual chemicals, we should look for statistical patterns.