Monday, August 31, 2026

Astronomers Catch Black Hole Spewing Matter After Feeding

Artist impression of the binary black hole, Swift J1727.8−1613, with eruptions of jets emanating from the black hole. (Credit: John A. Paice & Noel Castro Segura et al, ‘SwiftJ1727 - Final - No Overlay – DonorJetClouds’, (2026))

Black holes are some of the most awe-inspiring and mysterious celestial objects in the universe. This is primarily because astronomers still don’t understand the underlying mechanisms that drive black holes, including its formation, evolution, and end. As their name implies, black holes can’t be viewed directly since they blend into the background of the vastness of space. Therefore, astronomers are limited to “seeing” black holes when they consume other celestial objects, most notably stars. When this happens, the astronomers see the light from the star being violently consumed by a nearby black hole in a spectacular display. However, astronomers are still puzzled regarding what happens after the consumption.



Quantum Physicist Takes Aim at the Universe's Mysterious Arrow of Time

Physicist Jim Al-Khalili is the author of "On Time: The Physics That Makes the Universe Tick." (Credits: Clockwork photo adapted from Dietmar Rabich / Wikimedia Commons / Dülmen, Heilig-Kreuz-Kirche, Uhrwerk -- 2019 -- 3054. Al-Khalili image: Princeton University Press. Created under CC BY-SA 4.0 license)

Scientists and philosophers have argued over the nature of time since … well, since time immemorial. Is time real, or is it a convenient illusion? Why does time seem to flow in just one direction? In a new book called “On Time,” British physicist Jim Al-Khalili lays out what he thinks is the answer to such questions.



Martian Astronomy: Percy Sees a ‘Phobos Eclipse’ From Mars

Perseverance sees Phobos cross in front of the Sun. Credit: NASA/JPL-Caltech/ASU/MSSS/SSI

Sure. It’s just another image of Phobos crossing the disk of the Sun, as seen from the surface of Mars. Like so much of the modern space era, these images, once amazing, are now almost routine. But there’s some real science behind tasking the Mars rovers to conduct a little ‘Martian astronomy.’



Sunday, August 30, 2026

ESA JUICE probe targets dark Jovian moon Kallichore in 2031

Artist's impression of the ESA JUICE spacecraft. (Credit: ESA)

The planet Jupiter hosts more than 100 moons with the majority of attention going to the four Galilean moons, Io, Europa, Ganymede, and Callisto. This is primarily due to their active geology, including Io being the most volcanically active planetary body in the solar system and Europa having a vast subsurface liquid water ocean beneath its icy crust. However, Jupiter’s smaller and lesser-known moons could provide astronomers key insights into the history of the solar system since they’ve remained largely unchanged, unlike the Galilean moons.



Gardening the Moon's Cosmic Archives

Kepler's Supernova scattered debris across space as its giant star ended in an explosion. Credit: NASA/CXC/SAO/DSS/D. Patnaude

When a meteoroid hits the Moon's surface, it does more than just dig up a little dirt. It actually excavates a little bit of cosmic history that recorded a long-ago supernova explosion. Scientists at the University of Hawaii Institute of Geophysics and Planetology have come up with a way to decode that history and learn something about such energetic events in the Universe.



Roman Rises! Five Things to Know About NASA's New Space Telescope

A SpaceX Falcon Heavy rocket rises from NASA's Kennedy Space Center in Florida, sending the Nancy Grace Roman Space Telescope into space. (NASA Photo / Joel Kowsky)

NASA's newest eye on the sky, the Nancy Grace Roman Space Telescope, has begun its journey to unravel the secrets of dark matter, dark energy and Earthlike planets — months ahead of schedule.



Ancient Dust Grains Hold Magnetic Clues to the Sun's Birth

Our early Solar System likely had embedded magnetic fields at work even before the Sun was born, according to a new study. Credit: Hernán Cañellas

Those little dust grains that fall to Earth during meteor showers or end up as part of larger meteorites found on Earth may hold surprising clues to the formation of the Sun. That's because they record the state of the magnetic field in the protostellar nebula from which Earth (and ultimately the planets) formed.



Saturday, August 29, 2026

NASA Announces Next Steps for Swift Rescue Mission

NASA’s Neil Gehrels Swift Observatory, shown in this artist’s concept, has orbited Earth for more than 20 years, studying the ever-changing universe. Credit: NASA’s GSFC Conceptual Image Lab

Due to an ongoing commercial spacecraft attitude control issue, NASA and Katalyst Space announced Wednesday the LINK spacecraft will attempt to conduct rendezvous and proximity operations with NASA’s Neil Gehrels Swift Observatory to demonstrate key capabilities for the future of space exploration.



Measuring the Mass of the Universe Isn't As Simple as Astronomers Thought

Milky Way galaxy as seen from the Earth's surface. Measurements of the Milky Way's star populations form part of an analytical tool called the Initial Mass Function. It helps astronomers estimate stellar masses in other galaxies. Source: Adobe Stock

How do scientists know the mass of the Universe? Measuring it has traditionally relied on knowing how many stars there are in galaxies, as well as clouds of gas and dust, and associated dark matter. Astronomers generally use the mass of the brightest stars to estimate the mass of an entire galaxy. That means the rest of a galaxy's stars and its dark matter are essentially invisible. For decades, astronomers estimated the number of small, unseen stars in clusters and galaxies using a mathematical rule that assumed stars formed in roughly the same mass proportions everywhere in the Universe. That tool is called the initial mass function (IMF). It describes how many stars of each size there are in a given cluster or galaxy. However, there are challenges with the way it's currently applied because of assumptions it contains.



Friday, August 28, 2026

Interstellar Travel V: Warp Drives, Wormholes, and Halo Drives

Artist's impression of a spacecraft equipped with an Alcubierre Warp Drive. Credit: Limitless Space

In our fifth installment, we explore the most exotic proposals for interstellar travel, including the Alcubierre Warp Metric, wormhole travel, the Halo Drive, and other truly advanced concepts.



Spaceflight Leaves Heart Muscle Cell Strength Intact

NASA Astronaut Sunita Williams seen exercising on an International Space Station treadmill. (Credit: NASA)

Since the dawn of human space exploration, astronauts, scientists, and engineers have examined the short- and long-term effects of microgravity (often mistakenly called zero-gravity) on the human body. This includes the distribution of fluids to the upper body (called “puffy face”), an increase in height from the spine slightly extending, how solar and cosmic radiation impacts humans at the genetic level, and skeletal and muscle loss. However, arguably all these aspects pale in comparison to how the microgravity from spaceflight impacts the heart, and specifically heart muscle cells.



Thursday, August 27, 2026

Astronaut Microbes Might Survive at Moon's Pole, NASA Warns

Image taken by the Artemis II crew during its historic mission around the Moon in April 2026. (Credit: NASA)

One of the primary objectives of space exploration that often gets overlooked is the intense effort that goes into ensuring Earth microbes don’t contaminate planetary objects, also called forward contamination. This is done to prevent contaminating any potential life that might be present could get killed off my Earth microbes and scientists don’t want to make false discoveries. While space radiation and extreme temperatures often kill off any pesky microbes that hitch a ride on spacecraft, there remains a longstanding knowledge gap regarding whether microbes could survive the lunar polar regions due to its deep craters and varying topography.



Some Comets are Naked, and One Just Got Caught Photo-Bombing

Researchers found this image of comet 28P/Neujmin in the archives of Japan's Subaru Telescope and its Subaru Prime Focus Camera (Suprime-Cam). It turned out to be from almost the perfect angle to study the comet from. It's a naked comet without a coma, and these lucky observations gave astronomers a great look at its surface. Image Credit: NAOJ

Japanese researchers got lucky when a comet they wanted to study was found photo-bombing archival images from Japan's Subaru Telescope. The Subaru, with its 8.2 meter mirror, happened to image comet 28P/Neujmin from just the right angle to accurately characterize its surface. Their work is part of the ongoing effort to understand comets and asteroids, why some of them share properties, and what that means for their formation and evolution as Solar System objects.



Why Astronauts' Lower Eyelids "Let Go" in Space

NASA astronaut Karen Nyberg images her eye with a fundoscope aboard the International Space Station during the Expedition 37 mission in 2013. Credit: NASA

A new study identifies possible mechanisms behind changes in astronauts' lower eyelids, a symptom associated with long periods in space that can affect their eyesight.



Theory-Defying Exoplanet Atmospheres Force a Rethink of Theories

This artist's illustration shows the exoplanet 55 Cancri e. It's a super-Earth that is so close to its star that its a lava world, or magma ocean. But recent JWST observations show it has a thick atmosphere. That's challenging our theories of how atmospheres escape and forcing a rethink of the 'cosmic shoreline.' Image Credit: ESA/Hubble, M. Kornmesser

The discovery of lava worlds with atmospheres is challenging our theories of how atmospheres escape, and calling into question the idea of the cosmic shoreline. Stanford researchers have developed a model that explains how lava-covered worlds close to their stars can retain their atmospheres. The new theory could inform the search for life beyond our Solar System.



Wednesday, August 26, 2026

NASA’s Webb Telescope Rules Out Two New Dyson Sphere Candidates

*A hypothetical Dyson Sphere Swarm.  Credit: Wikipedia*

Recent searches for the technosignatures of hypothetical Dyson Spheres again turn up empty.



AI Spots Hidden Solar Storm Signs 9 Hours Early

An AI tool created by New Jersey Institute of Technology researchers can spot the hidden warning signs of solar storms almost nine hours before they become visible on the Sun. (Credit: NASA's Goddard Space Flight Center/SDO)

When we think of weather forecasts, we instinctively think of weather on Earth like rain or shine. However, we rarely consider weather forecasts from outside of the Earth, also called space weather. While space weather often results in the awe-inspiring aurora located at the northern and southern latitudes, we often forget the negative impacts of space weather on our everyday lives. This includes potential disruption of communication satellites or ground stations. The primary conundrum that has eluded researchers is being able to forecast incoming space weather so we can better prepare for its impact.



Scientists Melted A Diamond and Cracked a Secret of Ice Giants

Artist's concept of the diamond target melting. Credit - James Wickboldt/LLNL

Some of the strangest weather in the solar system doesn’t happen on Earth, or even Jupiter’s Great Red Spot - it happens in the interior of the Ice Giants like Neptune and Uranus. Specifically, scientists have long believed that, at certain pressure and temperatures, it literally rains diamonds inside of these planets. And for the first time, scientists have mimicked the process they believe creates that. A new paper by physicists at the Lawrence Livermore National Laboratory (LLNL), published in Nature Physics, resolves a 20 year old scientific mystery, and shows how the same physics that makes it rain diamonds inside Neptune could also help us triple our fusion energy output.



A Greenland Glacier Loses Another Chunk of Ice

This satellite image shows a 76 sq. km., 150 meter thick piece of glacier that broke off of the Petermann Glacier in Greenland. It's the largest loss of floating ice since 2012, and the most significant Arctic calving since 2020. It shows how quickly the Arctic is changing in the face of climate change, and will lead to even more ice loss. Image Credit: contains modified Copernicus Sentinel data (2026), processed by ESA. Licence: CC BY-SA 3.0 IGO or ESA Standard Licence

The ESA's Sentinel satellites captured a 76 sq. km. chunk of ice breaking off from Greenland's Petermann Glacier. They watched the cracks and deformations happen in real time leading up to the calving. While calving is normal, it's happening more often, and this is another clear sign that the Arctic is rapidly changing due to the warming climate.



Tuesday, August 25, 2026

New Simulations Show How Galactic Centers Grow Together

NGC 1365 imaged by the Cerro Tololo Inter-American Observatory. Credit:DES/DOE/FNAL/DECam/CTIO/NOIRLab/NSF/AURA

Using a state-of-the-art galaxy simulation, a team led by scientists from the Leibniz Institute for Astrophysics Potsdam (AIP) gained new insights into the processes shaping galactic centres across the Universe and the formation history of the Milky Way.



Surface Chemistry Shows Which Massive Stars Have Gained Mass from Binary Companions

This artist's illustration shows a blue star gaining mass from its red giant companion. Mass transfer is common in massive stars, most of which are in binary relationships. A pair of researchers have developed a way to identify stars that have gained mass, even if the transfer happened a long time ago. Image Credit: NASA/ESA, A. Feild (STScI))

Most stars, including massive ones, are in binary pairs. Astronomers think that about 70% of them have gained mass from their companions, but there's been no way to determine which ones have done so. Now, researchers have found a way.



A Distant Stream of Stars May Offer New Clues to Dark Matter

A Hubble Space Telescope view of the ultra-diffuse galaxy UGC9050-Dw1 and a stream of stars from an associated globular cluster. The stream is shaped by the influence of dark matter. Credit: STScI, Holm, et al.

Dark matter continues to challenge astronomers as they work to solve the mystery of this so-far-unseen material that permeates the Universe. It's not that the stuff doesn't exist. It does, but we just can't see it. The only way it can be detected is by its gravitational effects on ordinary matter. A team of researchers led by University of Copenhagen PhD student Julie Kiel Holm has found a stream of stars stretching out more than 3,000 light-years from a globular cluster that appears to have been shaped by dark matter in a distant galaxy.



Comet 220P McNaught Puts On An Encore Performance

Comet 220P McNaught from August 22nd. Credit: Frank Astro.

It has been a busy month for astronomy. In the midst of an eclipse season bookended by the total solar eclipse on August 12th and the deep partial lunar eclipse coming right up this week on August 28th, an outbound comet hanging high in the dawn sky just refuses to die: 220P/McNaught.



Monday, August 24, 2026

Can We Steal Energy from Black Holes? Part 1: Leveling Up Spacetime

An illustration of spacetime as a warped grid around the Earth, the picture at the heart of general relativity and frame dragging. Credit: NASA (public domain).

Roger Penrose found a way to extract energy from a spinning black hole without breaking any laws of physics. To understand it, we first have to level up our picture of spacetime, from Newton's empty stage to a swirling, draggable fabric.



NASA Starshade Would Enable Astronomers To Directly Image Rocky Exoworlds

An artist's concept of a generic starshade.  Credit:  Public Domain

Innovative NASA-funded orbital starshade could help capture first direct images from extrasolar earths.



Sunday, August 23, 2026

Astronomers Use Rare Ultra-Magnetic Star to Crack a Quantum Mystery

A Swinburne astronomer may have just confirmed one of the quirkiest aspects of quantum mechanics: that seemingly empty space can alter the behavior of light. Credit: NASA.

An international team observed a magnetar known as 1E 1547.0–5408 using NASA’s Imaging X-ray Polarimetry Explorer (IXPE), leading to what could be the first detection of vacuum birefringence taking place in the magnetar’s ultra-strong magnetic field. These findings could potentially resolve a long-standing mystery quantum mechanics.



NASA Highlights Next-Gen Cargo Landers Paving the Way for a Moon Base

Artist's depiction of a NASA moon based, along with it's update imagery. Credit - NASA

NASA and its commercial partners are making progress on their way to a permanent human presence on the Moon. As part of that, a recent press release and accompanying YouTube video hints they may be looking to provide regular updates to the progress of those efforts - and, at least for this first one, that progress looks pretty good.



Saturday, August 22, 2026

White Dwarf-Red Dwarf Binaries Power Cosmic Lasers

Artwork of a white dwarf–M dwarf binary stars. The white dwarf's magnetic field lines, which are stronger than those from the M dwarf, play a key role in creating long-period bursts of radio emission observed from binary stars like these. Credit: Elias Most (AI-generated)

Researchers have helped unravel the mystery of why certain pairs of stars pulse with regular, long-period bursts of radio waves. The particular class of objects they observed come in pairs that always include a compact dead star, called a white dwarf, locked in orbit with an M dwarf, a red star smaller than our Sun.



Friday, August 21, 2026

Dry Martian Meteorite Reveals Early Water in Mars's Crust

Meteorite Northwest Africa 7034 (NWA 7034) aka Black beauty. (Credit: NASA)

Billions of years ago, Mars was hypothesized to have been a habitable world with flowing liquid water and the potential for life. But directly studying its ancient past is currently limited to orbiters and rovers, as scientists have yet to obtain direct samples from Mars. However, meteorites have been found on Earth to have potentially originated from Mars during large impacts that flung chunks of the Red Planet into space, eventually being grabbed by Earth’s gravity and crashing into the Earth’s surface.



The CosmoQuest Satellite Will Listen to the Early Universe From the Far Side of the Moon

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A tiny UK-developed satellite, roughly the size of a small carry-on suitcase, could help answer one of the biggest questions in cosmology: what happened in the roughly 150 million years of cosmic dark ages, before the universe’s first stars appeared?



Strange Signals Called Long-period Radio Transits Come From Cataclysmic Variables

This iullustration shows a white dwarf star accreting material from its companion. New research says that this can explain at least one of the puzzling Long Period Radio Transients, mysterious radio signals that repeat with periods ranging from a few minutes to a few hours. Image Credit: Carl Knox (OzGrav, Swinburne University of Technology) and Joshua Preston Pritchard (CSIRO).

Long-period Radio Transients are sources that emit repeating radio and x-ray signals. The signals are polarized and coherent, and are similar to pulsars in some respects. But the type of astrophysical object responsible for them has been vigorously debated. New research says that at least one of them comes from a cataclysmic variable, a binary star where a white dwarf and a red dwarf orbit closely.



New Solar System Models Show Earth Is No Fluke

The Blue Marble Credit: Harrison Schmitt / Apollo 17

Astrobiologists use new starting points to produce ‘organic’ models of our solar system’s formation.



Thursday, August 20, 2026

NASA's Lunar Reconnaissance Orbiter Images Falcon 9 Crater on Moon, With Some Help From a Korean Spacecraft

These images from NASA's Lunar Reconnaissance Orbiter show the Falcon upper-stage's crash site on the Moon. The left image is before the crash, the right image is after, showing the impact crater. Image Credit: NASA Goddard/Intuitive Machines

A SpaceX Falcon upper stage crashed into the Moon on August 5th. NASA's Lunar Reconnaissance Orbiter captured images of the crash site from different viewing angles and with different sunlight angles. The images showed that the crater is about 18 meters wide and about 3 meters deep. SpaceX says the crash was an accident.



Mars's Funky Moon Deimos was Shaped by an Impact

This illustration shows Mars' moon Deimos and its distinctive south pole depression. Thought the moon's surface appears smoother than its sibling Phobos, it's still been battered by impacts. One major impact created the south pole crater, and also spread a layer of regolith on the moon's surface. Image Credit: NASA Eyes on the Solar System.

Mars' moon Deimos has a large crater on its southern pole. It's also covered by a layer of regolith so deep it buries many other, smaller craters. New research shows that an impact is responsible for both, and that the moon is rather fragile and porous, like a rubble pile asteroid.



What Can We Actually Find on an Exoplanet? Part 4: Looking For Us

Earth at night, its city lights tracing the footprint of human civilization. Industry leaves atmospheric technosignatures an alien astronomer might detect. Credit: NASA (public domain).

Some signs of an alien civilization are easier to spot than signs of life itself. On technosignatures, from CFCs and industrial gases to the pandemic dip in pollution, and why Earth's most detectable moment might be right now.



Wednesday, August 19, 2026

Webb Captures the Treasure Chest at the Heart of the Carina Nebula

Hubble image of the Carina Nebula (NGC 3372), which lies just 7500 light-years away in the constellation Carina (the Keel). Credit: NASA/ESA/UC Berkeley/STScI/NOAO/AURA/NSF

This NASA/ESA/CSA James Webb Space Telescope Picture of the Month takes us to a fantastical realm within our home galaxy, where piercing starlight and billowing winds sculpt dust clouds into inventive shapes. This scene is from the Carina Nebula, which lies just 7500 light-years away in the constellation Carina (the Keel).



Pluto Planetary Science is the Gift that Keeps on Giving

Pluto as seen by New Horizons during its 2015 flyby. Sputnik Planitia is a heart-shaped region that appears to be resurfaced by upwelling liquid nitrogen from below. That action creates what look like convection cells outlined by darker lines that could be flow channels. Credit: NASA/JHU/APL/New Horizons mission

Something's wetting the surface of dwarf planet Pluto along the northern edge of Sputnik Planitia, and planetary scientists have found a good explanation for it. A recent study of new Horizons images taken during the 2015 flyby revealed evidence that liquid nitrogen is rising up through cracks in Sputnik Planitia. That's the giant heart-shaped glacial basin we see in all the Pluto images taken by the spacecraft.



The Fastest Star in the Milky Way Will Test Relativity

These panels are Very Large Telescope images of the star S301 orbiting the Milky Way's SMBH, SgrA*. S301 is the fastest moving S star ever found, and also the closest to the black hole. The star can be used to measure the black hole's spin. S301's orbit is shown with an elliptical curve. In each frame, the solid curve shows the path that the star has already completed up to that point, whereas the dashed one marks the path it will follow afterwards. Image Credit: ESO/GRAVITY collaboration

Astronomers have discovered another S star, the population of stars that orbits the Milky Way's SMBH. This one is the fastest of them all, and also comes closest to the SMBH. It will let astronomers test relativity, especially the Lense-Thirring effect.



What Can We Actually Find on an Exoplanet? Part 3: Reading the Face of a Planet

Earth's full disk, the "Blue Marble." Oceans, continents, clouds, and vegetation, all of which can in principle be read off a single distant pixel of light. Credit: NASA (public domain).

A single pixel of light holds astonishing detail. How ocean glint, rotational mapping, and the vegetation red edge let us read a distant planet's oceans, continents, and even forests, all without ever resolving it as more than a point.



Tuesday, August 18, 2026

Life On Earth May Have Had A Cold Start

Earth as seen from the International Space Station.  Credit: NASA Johnson

Nitrous oxide (otherwise known as laughing gas) is likely a key atmospheric component of life in the cosmos.



Even Near a Supermassive Black Hole, Stars Enrich the Interstellar Medium

The JWST used NIRCam and MIRI to capture this region near the Milky Way's SMBH. The star IRS 3 is in this field. It's an AGB star, and researchers are studying it to investigate the connection between material cast off from these types of stars and the interstellar medium. The researchers were surprised to find water and dust here, even though powerful radiation from the SMBH inhibit them. Image Credit: ESA/Webb, NASA & CSA, F. Peißker, J. Lu, F. Yusef-Zadeh, N. B. Sabha, C. Chan. Licence: CC BY 4.0 INT or ESA Standard Licence

Astronomers know that evolved AGB stars shed their outer layers, contributing to the makeup of the interstellar medium. But new JWST observations show this can happen even near a supermassive black hole, where powerful radiation could obliterate molecules.



Astronomers Finally See the Twisted Magnetic Fields That Drive Protostar Jets

This artist's illustration shows the twisted magnetic fields from a young protostar, which shape and propel the jets of gas emitted by the star. Decades ago, astrophysicists predicted that these twisted magnetic fields were responsible for launching and shaping these jets, now thanks to ALMA, they've detected them. Image Credit: NSF/AUI/NSF NRAO/M. Weiss

For decades, scientists have theorized that young protostar jets are shaped and driven by complex, twisted magnetic fields. But they couldn't detect them. Now, thanks to ALMA, they've found them around a young binary protostar.



Monday, August 17, 2026

Massive Exoplanets Could Form Around Supermassive Black Holes

This artist's illustration shows an active galactic nuclei with accretion disk and jets. New research says that under specific disk conditions, giant planets could form in the outer regions of the disk. So could black holes, including the elusive intermediate mass black holes. Image Credit: JAXA.

Black holes aren't just engines of inexorable destruction. They're complex regions of space and time, and under the right conditions, giant planets can form in their AGN disks.



NASA's SkyFall Mars Helicopters Will Feature a Revolutionary Antenna Design

An artist’s concept depicts the three SkyFall Mars helicopters collecting data while flying over the surface of the Red Planet. Credit: NASA/JPL-Caltech

Engineers developed a unique fabric-based design for a ground-penetrating radar that will be a key instrument on NASA’s SkyFall Mars helicopters. The hardware will enable the SkyFall mission’s trio of planetary rotorcraft to use ground-penetrating radar to study the Martian subsurface.



The JWST Little Red Dots Could Be 'Black Hole Stars'

New research proposes that the JWST's Little Red Dots, those puzzling objects from the early Universe, are objects the researchers have dubbed "Black Hole Stars." They're black holes, but instead of just an accretion ring, they're surrounded by a dense cocoon of gas that colours their light red. These could explain the SMBH found so early in the Universe by the JWST. Image Credit: Rohan Naidu (University of Hawai’i)

Little red dots have puzzled astronomers since their discovery in JWST data from the Universe’s deep past. Their ‘powering engines’ might resemble a newly discovered phenomenon dubbed a “black hole star”—an early, rapidly growing black hole wrapped in dense gas. This object, described in a study published today in Nature by researchers at the Institute of Science and Technology Austria (ISTA) and international collaborators, may help explain how billion-solar-mass black holes formed so soon after the Big Bang.



Nuking An Asteroid on Short Notice Could Save Us

Artist's concept of the DART satellite. Credit - NASA / JHU APL

Readers of a certain age will remember a golden area of asteroid films, capstoned by two with very different endings. Deep Impact engrained the devastating consequences of letting a large piece of rock hit our planet, whereas Armageddon, though arguably the more kitschy of the two films, was an uplifting story about technical ingenuity and sacrifice. And now, the central crux of that movie’s storyline - essentially blasting an asteroid with a nuclear detonation - is taking center stage as our last line of defense against a potential Deep Impact scenario. A new paper from researchers at the China Academy of Launch Vehicle Technology, and published in Space: Science & Technology, describes two potential scenarios examining how we might actually be able to nuke a space rock - and whether it would actually save us.



What Can We Actually Find on an Exoplanet? Part 1: The Atmospheric Fingerprint

The Pale Blue Dot: Earth photographed by Voyager 1 from six billion kilometers away in 1990. Everything we are is in that single point of light. Credit: NASA/JPL-Caltech (public domain).

If an alien civilization could see Earth only as a single pale blue dot, what could they learn? We start with transit spectroscopy, the biosignature cocktail of oxygen, methane, ozone, and water, and why even the James Webb will struggle to find life.



Saturday, August 15, 2026

The Planet That Lied About Its Own Spin

A radar mapped view of Venus's surface from NASA's Magellan mission since thick cloud hides the surface entirely, radar is one of the only ways to see the solid planet the paper argues astronomers have been mismeasuring by watching its clouds instead (Credit : NASA/JPL-Caltech)

A new study warns that astronomers measuring the rotation of distant exoplanets may often be measuring atmospheric winds instead, since the clouds of Venus circle the planet roughly 60 times faster than Venus itself actually spins. Kane proposes using multi-wavelength observations to correct for this, work that will matter enormously once the European Space Agency's PLATO mission launches in 2027 and, researchers predict, discovers several hundred Venus like exoplanets.



The Sun Doesn't Care About Your Flight Schedule

Earth's Van Allen radiation belts, the inner and outer bands of trapped high energy particles that swell dramatically during solar storms, the very radiation environment aircraft at cruising altitude briefly share in during an extreme space weather event ( Credit : NASA's Goddard Space Flight Center/Johns Hopkins University Applied Physics Laboratory)

New research shows that extreme space weather can significantly raise radiation exposure on commercial flights and increase electronic faults in aircraft systems. A severe 1956 scale solar storm could expose passengers to a year's worth of radiation in a single flight, and the researchers point to last year's Airbus A320 grounding, triggered by a solar radiation linked flight computer fault, as proof this isn't theoretical. To address the gap, the team has proposed a new aviation specific radiation scale designed to give airlines clearer, more reliable guidance on when to monitor, reroute, or ground flights during severe events.



Friday, August 14, 2026

The Tarantula That Lost Its Fire

The new composite image of the Tarantula Nebula (30 Doradus), layering X-ray data from Chandra (blue), infrared from Webb (red), and optical data from Hubble (green) — the combination that let astronomers trace where the nebula's missing energy has been escaping to (Credit : X-ray: NASA/CXC/Ohio State Univ./J. Rodriguez et al; Infrared: NASA/ESA/CSA/STScI; Optical: NASA/ESA/STScI; Image Processing: NASA/CXC/SAO/P. Edmonds)

A new composite image combining data from Chandra, Hubble, Webb and the retired Spitzer telescope has helped astronomers solve a long standing puzzle in the Tarantula Nebula, a star forming region 160,000 light years away. Young, massive stars there should be heating enough gas to emit X-rays, but observations showed far less X-ray emission than predicted.