A new look at more than two decades’ worth of archival data from NASA’s Spirit mission suggests that the Martian soil may hold iron-bearing minerals -- hematite and altered magnetite -- that were too faint for scientists to detect in real time during the mission.
New NASA imagery has revealed a growing Martian “crescent” and surface details on the Red Planet as the agency’s Psyche spacecraft recently completed a flyby of Earth’s nearby planetary neighbor.
Launched on October 13, 2023, Psyche is currently on its way toward a rendezvous with a metal-rich asteroid after which the space probe was named. Now, in a series of composite images captured as the spacecraft flew past Mars during a gravity assist in early May, the growing crescent shape of the Red Planet is shown in successive views of Earth’s nearby planetary neighbor.
“After these views were captured by the spacecraft’s multispectral imager instrument, Mars began to overfill the field of view as Psyche made close approach with the planet and captured a series of high-resolution images of the surface,” read a NASA statement accompanying the imagery.
Composite imagery of Mars recently obtained by NASA’s Psyche spacecraft (Image Credit: NASA)
In several of the images, Mars appears as a thin sliver due to the high phase angle of approach as Psyche made its way toward the planet. In the days that followed, the crescent is shown as it appears to “grow” as more sunlight illuminates its surface.
A Detailed Glimpse of the Martian Surface Captured by Psyche
The recent crescent features weren’t all that Psyche captured during its recent near approach to Mars. In additional images released by the American space agency, the Martian surface appeared in colorful views obtained by the spacecraft’s multispectral imager instrument.
The resulting “mosaic” was created from four separate images acquired near the end of Psyche’s recent visit, shown in enhanced color that highlights several details visible on the Martian surface.
Traveling along a southwesterly path with relation to the Martian poles, the mosaic imagery appears slightly blurry, as it represents close to six minutes of travel above the planet. According to NASA, pixel scale resolution in the imagery “varies from 381 meters per pixel on the right to 440 meters per pixel on the left.”
Imagery showing the Iapygia region of the rugged southern highlands of Mars, obtained by NASA’s Psyche spacecraft (Image Credit: NASA)
Color enhancements to the imagery, collected with the imager’s green, blue, and near-infrared filters, reveal additional details about the various features of the volcanic region of Mars that Psyche flew over on May 15, 2026, known as the Iapygia region.
This area comprises part of the Martian southern highlands, and in the recent imagery, Fournier crater—the largest shown in the new imagery—can be seen, alongside hills, cliffs, and other features, including the irregular Oenotria Scopuli cliff system, forming one side of the boundary of a massive ancient impact feature on the Red Planet.
Additional details about the new imagery, as well as information about Psyche’s mission, can be found on NASA’s official mission page.
Micah Hanks is the Editor-in-Chief and Co-Founder of The Debrief. A longtime reporter on science, defense, and technology with a focus on space and astronomy, he can be reached atmicah@thedebrief.org. Follow him on X @MicahHanks, and at micahhanks.com.
That visitor—a robotic rover named Perseverance—has been conducting investigations on Mars since February 18, 2021, and the new aerial images reveal its current location in an area that mission specialists have dubbed “Arbot.”
While Perseverance’s latest appearance reveals little more than a greenish spec on the planet’s rust-colored surface, also visible in the new images are the long path its formidable tires have left in the Martian soil as the robotic explorer has trekked west of its initial landing site.
The new images, captured on June 13, 2026, were taken just one day before Perseverance broke the previous distance record held by a robotic explorer on Mars: NASA’s Opportunity rover.
However, Perseverance completed this phase of its journey in record time compared to its predecessor, which took more than 11 years to traverse a similar distance. Perseverance, by contrast, covered the same distance in less than half that time, with just five years and four months of travel now behind it.
In the image above, NASA’s Perseverance Rover appears in the center of the image as a small, greyish-green reflective spot. Also visible are the impressions left by its all-terrain tires, revealing the robotic rover’s long path over the last several years of Martian exploration (Image Credit: Credits: NASA/JPL-Caltech/University of Arizona)
The images were made possible by the MROs’ High-Resolution Imaging Science Experiment (HiRISE) camera, which also captured surface features in the Arbot area that include ridges and windswept areas along Mars’ rugged exterior.
Built and operated by the University of Arizona, HiRISE captures images with resolutions as fine as about 25 centimeters (10 inches) per pixel, allowing researchers to distinguish features roughly the size of a kitchen table from orbit. The camera has returned hundreds of thousands of detailed images since the MRO arrived at Mars two decades ago, contributing to a growing data set that has transformed scientists’ understanding of the Red Planet.
Documenting everything from active dust avalanches and shifting dunes to fresh impact craters, the unprecedented resolution its imagery provides has made HiRISE one of the most powerful planetary imaging instruments ever deployed.
Last year, the MRO’s HiRISE camera also successfully captured images of the interstellar comet 3I/ATLAS as it made its way past Mars during its trip through our Solar System. Although the HiRISE images weren’t the clearest images of the interstellar visitor obtained during its visit, they did help demonstrate just how formidable NASA’s MRO and its suite of instruments are.
Micah Hanks is the Editor-in-Chief and Co-Founder of The Debrief. A longtime reporter on science, defense, and technology with a focus on space and astronomy, he can be reached atmicah@thedebrief.org. Follow him on X @MicahHanks, and at micahhanks.com.
Scientists from the Southwest Research Institute’s Center for Lunar Origin and Evolution (CLOE) have revealed new models of the Moon’s oldest and largest impact crater, the South Pole-Aitken (SPA) basin, providing fresh insights into the event and resulting material deposition on the lunar surface.
The SwRI team behind the new models, which is part of NASA’s Solar System Exploration Research Virtual Institute, said such details will help prepare future Artemis astronauts for what they could encounter during their upcoming missions.
Impact Study Reveals Details About Moon’s Oldest and Largest Crater
In a statement announcing the new models, Dr. William Bottke, director of CLOE and executive director of SwRI’s Science Directorate in Boulder, Colorado, said that the basin is an attractive potential target for future Artemis missions since it offers a “rare opportunity” to study an earlier era in the Moon’s history.
“The collision struck the lunar surface with such force that it may have excavated material from deep inside the Moon, including portions of the lunar mantle,” explained the co-author of the impact study detailing the new research.
Although previous studies have modeled impacts that may have caused the Moon’s oldest and largest crater, the team’s new effort has revealed new evidence about the composition of the impacting object and its likely direction and angle.
“Our simulation produces the right shape and nature of the impact basin,” explained the impact study’s lead author, Dr. Shigeru Wakita of Purdue University. “It also tells us about the projectile that created it and the direction of the impact.”
Image shows materials excavated (blue) from the SPA by its forming impact, including mantle-derived rocks (orange and black). Models suggest the proposed landing sites for upcoming Artemis missions to the lunar south pole (white blocks) lie within the region. Image Credit: NASA/JPL-Caltech/Goddard/Gabe Gowman-U. Arizona. Data from NASA’s GRAIL mission and NASA’s Lunar Reconnaissance Orbiter Laser Altimeter.
For example, the new model suggests that the object was not a single, uniform object. Instead, the team found that the impactor was likely a “differentiated” object, such as a protoplanet or asteroid, composed of rock and surrounded by an iron core. The models also found that the object approached from the north “at a low angle” before impacting the Moon’s surface on a southward trajectory.
According to the impact study authors, the impact excavated a deep, “asymmetric” cavity and generated enough energy to melt the rock within the crater’s central basin, resulting in the SPA basin’s elongated, tapered shape. Their models also indicated that the object’s lunar collision “lofted” large amounts of material into the air. Critically, their models also revealed that material from both the lunar crust and mantle was likely ejected before ultimately settling back onto the basin floor.
Exploring Gravity’s Role and the Possibility of ‘Valuable’ Mantle in the Impact Ejecta
To help potential future lunar astronauts, including members of NASA’s Artemis mission, target the most scientifically valuable lunar samples, a second companion study explored the effects of gravity on ejecta distribution beneath and around the impact basin. According to the team behind that effort, their effort involved direct comparisons of high-resolution gravity data with models. Specifically, they wanted to determine if pieces of the Moon’s crust and mantle were included in the ejection.
After comparing the two, the authors of the second study determined that the SPA basin “likely contains substantial amounts of mantle-derived rocks” both within its interior and mixed into the wider ejecta blanket surrounding the basin. Also critical for future missions, the analysis revealed that this material was not all scattered during the initial impact.
Instead, the new models showed that subsequent, smaller impacts appear to have “excavated” these underlying mantle deposits. As a result, the team suggests that there is likely enough material on the surface of the Moon’s oldest and largest crater “where it could be readily sampled by robotic rovers or astronauts during future missions.”
The Studies Provide Future Lunar Missions with a “Powerful Roadmap”
When discussing the significance of the gravity study’s findings, lead author Dr. Gabriel Gowman of the University of Arizona said that before now, the “precise distribution” of lunar mantle material on the Moon’s surface “has been a big unknown.” For example, some previous theories suggested that the deepest ejecta might be found only in parts of the basin that are not currently included in planned Artemis missions.
Now, the team’s new models suggest that the impact that formed the SPA basin “ejected enough deep material to form a significant deposit that should still be accessible today.” More importantly, Dr. Gowman added, some of that scientifically valuable mantle material “at a trace level” may exist in regions currently under consideration for upcoming Artemis landings. Taken together, Bottke said, the two studies can provide a “powerful roadmap” for future lunar scientific missions to the Moon’s oldest and largest crater.
“It tells us not just how SPA formed, but where to look for the rocks that can answer some of our biggest questions about the Moon’s origin and evolution,” the researcher explained.
Christopher Plain is a Science Fiction and Fantasy novelist and Head Science Writer at The Debrief. Follow and connect with him on X, learn about his books at plainfiction.com, or email him directly at christopher@thedebrief.org.
Planetary scientists analyzing a lunar meteorite known as Northwest Africa (NWA) 12593 have uncovered evidence of an asteroid impact that occurred 3.5 billion years ago on the Moon, helping to reconstruct a period of intense bombardment that left lasting marks across the inner Solar System.
The Earth's atmosphere, though thin, protects against meteors and asteroids, causing most to burn up upon entry. Significant impacts, like the Vredefort and Chicxulub craters, demonstrate catastrophic events, which occurred during or just after the Genesis Flood, highlighting a biblical perspective on geological history.
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