Thursday, October 22, 2026

New Evidence for an Old Prediction: Recoiling Supermassive Black Holes

This artist's impression shows a distant quasar, an extremely luminuos active galactic nuclei hosted by a supermassive black hole. We know that SMBH can merge, but theory says that in some mergers, the merger remnant recieves a powerful kick that drives it into a pendulum-like motion across the center of the galaxy. New research has uncovered statistical proof of these merger remnant SMBH. Image Credit: ESO/M. Kornmesser.

Theory says that during some SMBH mergers, the merger remnant receives a recoil kick from gravitational waves. Instead of sitting placidly in the galactic center, these recoiled SMBH are sent on a pendulum-like motion, back and forth through the galactic center. New research has found statistical evidence supporting their existence.



Wednesday, October 21, 2026

How Flare Ribbons Reveal Hidden Solar Explosions on the Sun

NASA’s Solar Dynamics Observatory captured this image of a solar flare – as seen in the bright flash on the right side – on Sept. 10, 2017. The image shows a combination of wavelengths of extreme ultraviolet light that highlights the extremely hot material in flares, which has been colorized. There's a lot to learn about flaring, and the ever-changing Sun itself, and new research made progress in understanding its flaring behaviour. Image Credit: NASA/SDO

Solar flaring is complex behaviour triggered by reconnection, when magnetic field lines break and then snap back to the Sun's surface. The flaring is complex behaviour, and its details are difficult to observe. Researchers found a new way to study flaring behaviour.



There Should Be Black Holes in our Neighbourhood. Can We Find Them?

This artist's illustration shows a stellar-mass black hole (left) accreting material from a much larger Wolf-Rayet star. In this case, the black hole is emitting bright energy and is hard to miss. But other stellar-mass black holes are more isolated, with little to feed on and emitting little radiation, and finding them is difficult. Image Credit: By ESO, CC BY 4.0, https://commons.wikimedia.org/w/index.php?curid=9551709

Stellar-mass black holes should be in our neighbourhood within about 50 light years of the Solar System. But they're likely isolated, without much to feed on, making them difficult to find. Gaia found some candidates, but confirming them is tough.



There Must Be Stellar-Mass Black Holes in our Stellar Neighbourhood. Can We Find Them?

This artist's illustration shows a stellar-mass black hole (left) accreting material from a much larger Wolf-Rayet star. In this case, the black hole is emitting bright energy and is hard to miss. But other stellar-mass black holes are more isolated, with little to feed on and emitting little radiation, and finding them is difficult. Image Credit: By ESO, CC BY 4.0, https://commons.wikimedia.org/w/index.php?curid=9551709

Stellar-mass black holes should be in our neighbourhood within about 50 light years of the Solar System. But they're likely isolated, without much to feed on, making them difficult to find. Gaia found some candidates, but confirming them is tough.



Mars’s Most Mysterious Cloud Might Be Defying Textbook Cloud Physics

The Arsia Mons Elongated Cloud as seen from Mars Express. Credit - ESA/DLR/FU Berlin

It may not be as obvious, but just like Earth, Mars has seasons. And every day of every summer, an 1,800 kilometer long thin white cloud appears to the west of Arsia Mons, a 20 kilometer high extinct shield volcano. At least for a few hours, before it dissipates until it reappears the next morning. Scientists have known about this feature, which they call the Arsia Mons Elongated Cloud (AMEC), for decades, but planetary scientists have been unable to explain it using traditional atmospheric models. But a new paper, published in Nature Geoscience by a research team led by Dr. Jorge Hernández-Bernal of the Sorbonne, suggests that the cloud could be the first documented real-world example of a cloud flash-freezing out of thin air.



Tuesday, October 20, 2026

Scientists Use Ancient Rains to Map the Possible Origin Life on Mars

This artist's concept depicts the early Martian environment (right) – believed to contain liquid water and a thicker atmosphere – versus the cold, dry environment seen on Mars today (left). Credit: NASA's Goddard Space Flight Center.

Billions of years ago, rain may have helped shape where the chemistry of life could begin on Mars. A new study maps how formaldehyde, an important prebiotic molecule, may have reached the surface. This map could help guide future missions searching for signs of past life on Mars.



JAXA's Martian Moons eXploration Mission is on its Way to Mars and Phobos

JAXA launched its MMX sample return mission to Phobos on October 20th. It was sent on its way in an H3 launch vehicle, Japan's next-generation heavy-lift launch vehicle. It will reach Mars in August 2027, and after several years will return a sample from Phobos to Earth. Image Credit: JAXA.

JAXA successfully launched its Martian Moon eXplorer on its way to Mars and Phobos. It'll reach Mars in about six months, and will orbit the planet for about a month before transferring to an orbit around Phobos. It will deploy a small lander, which will help select a sample-gathering location for the main part of the mission. By 2031, the regolith sample from Phobos should be back on Earth.