Friday, October 23, 2026

The Largest Canyon in the Solar System is Still Tectonically Active

Artist's impression of the Valles Marineris canyon system on Mars. Credit: Mark Garlick/Science Photo Library

Scientists at Imperial College London and Columbia University have found that the largest canyon system in the solar system is still active and shaping Mars today, billions of years after it first formed.



Saudi Arabia Joins the Search for Alien Civilizations

Saudi Arabia has installed a pair of LaserSETI detectors in a region in a region named AlUla Manara, a site being established as the kingdom's first major astronomical observatory. They're part of a network of optical detectors will scan the heavens for laser signals from alien technological civilizations. Image Credit: LaserSETI.

Saudi Arabia is joining the search for alien signals coming from the cosmos. They're collaborating with SETI in the endeavour. SETI has announced that two LaserSETI instruments will be positioned in Saudi Arabia, adding to a growing network of optical sensors designed to detect laser pulses that could come from alien technological civilizations.



Thursday, October 22, 2026

Advancing Astronomy at MIT with X-ray Reverberation Mapping

Artist's concept of a supermassive black hole with an accretion disk and a relativistic jet. Credit: NASA

Professor Erin Kara of MIT's Kavli Institute for Astrophysics and Space Research is helping advance our understanding of the most extreme objects in the Universe by analyzing X-ray reverberations and other astrophysical data.



Even the Rubin's Test Camera Produces Stunning Images

IC 2177, or the Seagull Nebula, as captured by the Vera Rubin Observatory's Commissioning Camera in 2024. This image features the Seagull's head, a cloud of gas named Sharpless 2-292. Image Credit: NSF–DOE Vera C. Rubin Observatory/NOIRLab/SLAC/AURA. Image Processing: T.A. Rector (University of Alaska Anchorage/NSF NOIRLab), D. de Martin & M. Zamani (NSF NOIRLab)

The Vera Rubin Observatory's Commissioning Camera operated for about 7 weeks in 2024, before the observatory released its well-known first look images. It's an engineering camera, and its job was to test the VRO's equipment and procedures. Now, the VRO has released the ComCam's image of the Seagull nebula. It's a pretty stunning image for an engineering camera.



Two Disks in One: How Accretion Disks Drive Black Hole Jets

This artist's illustration shows a rapidly-feeding supermassive black hole launching jets from its poles. For this to happen, the accretion disk has to have large-scale magnetic fields. But not all do, generating a contradiction. New research has an answer. Image Credit: Tohoku University.

SMBH jets are driven by thick, hot accretion disks with powerful magnetic fields. But there's a bit of a paradox. Some SMBH produce jets, even though they appear to have thin, cold accretion disks. New research has solved this paradox, showing that disks can be truncated into an outer cold disk and an inner hot disk.



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.