Friday, August 21, 2026

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.



Upgraded Sardinia Radio Telescope To Continue Probing Mysterious Fast Radio Bursts

Italy's Sardinia Radio Telescope. Credit: Bruce Dorminey

Largest Italian radio telescope located on an out of the way mountain plateau in southern Sardinia sheds light on the cosmos’ still misunderstood Fast Radio Bursts (FRBs).