Death Clock promises to predict when you’re going to die and help you extend your time on Earth. After a month, I felt like it was sucking the life out of me.
The first named storm of the 2026 North Indian Ocean cyclone season—Arnab (pronounced Or-nab)—emerged in the Bay of Bengal on October 25, a rather late start for a basin that typically produces named cyclones in April or May.
When the VIIRS (Visible Infrared Imaging Radiometer Suite) on NOAA-20 captured this nighttime image at 20:12 Universal Time on October 26 (1:42 a.m. India Standard Time on October 27), the storm had sustained winds of about 140 kilometers (85 miles) per hour, according to the India Meteorological Department (IMD).
When Arnab made landfall on the Andhra Pradesh and Yanam coast early on October 28, sustained winds were 130 kilometers per hour. IMD categorizes a storm that strength as a “very severe cyclonic storm,” which is similar to a Category 1 storm on the Saffir-Simpson hurricane wind scale. It made landfall between Bapatla and Visakhapatnam, a heavily settled area home to large cities, farmland, and fishing communities.
Arnab caused extensive damage, uprooting trees, inundating crops and homes, limiting fishing operations, and disrupting transportation and power networks, according to news reports. Prior to landfall, Indian authorities had evacuated tens of thousands of people from vulnerable coastal areas.
The storm comes in the midst of an El Niño, a climate pattern marked by warmer-than-normal water temperatures in parts of the equatorial Pacific that emerges roughly every two to seven years. The changed ocean conditions can influence the atmosphere in ways that alter global weather patterns and change the distribution of rainfall, winds, tropical cyclones, fires, floods, and other phenomena.
In the Bay of Bengal, for instance, some research indicates that altered environmental conditions during an El Niño are associated with a reduction in tropical cyclone activity. The ocean basin sees both less frequent and less intense tropical cyclones during El Niño years, researchers have found.
Preparations for Next Moonwalk Simulations Underway (and Underwater)
Former NASA astronaut and Artemis II Commander Reid Wiseman joins Caltech and NASA JPL as Caltech associate vice president and JPL deputy director on Nov. 30.
Photo Credit: NASA
Artemis II Commander Reid Wiseman has been named Caltech associate vice president and deputy director of NASA’s Jet Propulsion Laboratory in Southern California. The emeritus astronaut and retired U.S. Navy captain begins his new role at NASA’s center of excellence for robotics and deep space exploration and at Caltech, which manages JPL for NASA, on Nov. 30, 2026.
“Reid has spent his career at the edge of what is possible, and he has the technical judgment, operational experience, and leadership to help push that edge farther,” said NASA Administrator Jared Isaacman. “As commander of Artemis II, he helped carry America back around the Moon, and now, as an emeritus astronaut, he will continue giving back to NASA from a new vantage point at JPL. Reid is joining a storied laboratory that has made an enormous amount of history, and there is a lot more ahead. I am excited to see what he and the JPL team accomplish in the years to come.”
During the Artemis II test flight, Wiseman, Victor Glover, Christina Koch, and Jeremy Hansen journeyed 695,081 miles on a lunar flyby that took them farther than any humans have ever traveled before.
“It feels fitting for Reid, who with the Artemis II crew traveled farther from Earth than any human in history, to join Caltech and JPL — institutions that for nearly 90 years have sent spacecraft into the far reaches of our solar system and beyond,” said Dave Gallagher, JPL director and Caltech vice president. “Reid shares our drive for discovery, knows what it takes to lead teams through high-stakes missions, and has a remarkable ability to inspire people everywhere. He adds incredible bench strength to our leadership team as we build on the lab’s legacy and shape its future together.”
After joining NASA’s astronaut corps in 2009, Wiseman went on to serve as flight engineer aboard the International Space Station for the 165-day Expedition 41 mission in 2014 and was a commander of NASA’s 21st Extreme Environment Mission Operations expedition, during which he lived for eight days in a habitat on the ocean floor in 2016. As the agency’s chief astronaut from December 2020 to November 2022, Wiseman led NASA’s astronaut corps, overseeing crew flight readiness and crew safety for all NASA human spaceflight missions. During his years of service at the agency, he has conducted hundreds of scientific experiments.
“I’ve explored the furthest reaches of what a human can explore at NASA — and there were truly no words in the English vocabulary to describe seeing the Sun disappear behind the Moon from deep space. But that experience was really the jumping off point to go do the impossible things that Caltech and JPL dream, dare together, and do for NASA and the nation,” Wiseman said. “What an awesome time in my career to join this team and to try and push humanity and push our understanding of the solar system and the universe.”
Wiseman joins JPL, NASA’s only federally funded research and development center, as the lab approaches its 90th anniversary since being founded by Caltech. In his role as Caltech’s associate vice president and JPL deputy director, Wiseman will be responsible for the strategic leadership, stewardship and continuous improvement of laboratory operations, including close partnership with Caltech on institutional planning, management and compliance. Serving as Center Management Authority for JPL mission execution, Wiseman will ensure operational excellence across mission support functions in accordance with NASA requirements and applicable federal and state regulations. In addition, he will be JPL’s primary interface for national security programs.
“Reid brings to Caltech and JPL a truly unprecedented view of what humanity can achieve when ingenuity and determination are matched with the courage to pursue the furthest frontiers,” said Caltech president Ray Jayawardhana. “His pioneering spirit coupled with unbounded curiosity make him a natural fit for Caltech and JPL, a force-multiplier for a community whose daring continues to push the limits of humanity’s reach. I look forward to working closely with Dave and Reid as we chart our next era of exploration in partnership with NASA, elevating America’s space ambitions to breathtaking new heights.”
After receiving a bachelor’s degree in computer and systems engineering from Rensselaer Polytechnic Institute, Wiseman joined the Navy, going on to fly combat missions and serve as a test pilot. He also has a master’s degree in systems engineering from Johns Hopkins University in his hometown of Baltimore.
ICE’s Homeland Security Investigations is engaged in far-reaching spying against left-wing activists that rivals the FBI and CIA crackdowns on the Civil Rights and anti-war movements.
A visualization shows the orbital path of the dwarf planet candidate 2026 ED138 in relation to the orbits of the solar system’s larger planets. Click on the image for a larger version. (Credit: NSF-DOE Vera C. Rubin Observatory / NOIRLab / SLAC /AURA / R. Proctor)
Astronomers sorting through data from the Vera C. Rubin Observatory in Chile have found an icy world that has a good chance of joining Pluto in the solar system’s retinue of dwarf planets.
University of Washington astronomer Mario Jurić joined the astronomer who made the discovery, Matthew Holman of the Harvard & Smithsonian Center for Astrophysics, to announce the findings today at a meeting of the American Astronomical Society’s Division for Planetary Sciences in Spokane, Wash.
Jurić, the Rubin team’s solar system lead scientist, said the observatory’s capabilities made it possible to detect and characterize the new dwarf planet candidate, known as 2026 ED138.
“Rubin is giving us an unprecedented capacity to explore the sky through a combination of speed, depth, and precision,” Jurić said in a news release. “And the discovery is just the beginning: Once we identify a new object, we can search back months, and sometimes even decades, finding it in images where nobody knew to look. This ability to both discover and ‘precover’ objects is transforming how quickly and accurately we can determine their orbits and understand the distant solar system.”
2026 ED138 traces a tilted orbital path that takes it well beyond Pluto, the solar system’s best-known dwarf planet. It’s currently at a distance of 46 astronomical units, where 1 AU equals the average distance between Earth and the sun. Pluto, by comparison, is currently about 40 AU from the sun.
Astronomers suspect ED138 formed billions of years ago closer to the sun before being flung into a wider orbit by gravitational interactions with Neptune.
Based on an analysis of its distance, brightness and assumed composition, ED138 is thought to be somewhere between 600 and 1,500 kilometers (373 to 932 miles) in diameter. At that size, an icy object should possess enough gravity to pull itself into a round shape — satisfying the primary physical criterion for a dwarf planet.
Rubin’s researchers analyze the data from those scans to find objects of interest — ranging from asteroids to gamma-ray bursts — and track them over time. On Oct. 13, Holman was running data through a search code that he developed with Kevin Napier, a colleague at the Center for Astrophysics. ED138 stood out due to its exceptional size and brightness.
“My first reaction was one of excited disbelief,” Holman said. “Objects like this are very rare, so I immediately started checking whether I or the code had done something wrong.”
To confirm the discovery, Holman, Jurić and their colleagues found 30 archived observations of ED138 dating back to March 4. The Asteroid Institute’s ADAM Precovery service found still more images of the object, going back to 2016, in the archives of a different astronomical survey.
The precovery data confirmed that ED138 was a special case.
“Finding an object this big, roughly 1,000 kilometers across, is something that happens maybe once in a generation,” Jurić said. “It’s the largest trans-Neptunian object found in about 20 years, and Rubin turned it up while we were still commissioning the telescope.”
In 2006, the International Astronomical Union defined dwarf planets as planetary objects that are big enough to crush themselves into a roundish shape — technically speaking, into a state of hydrostatic equilibrium — but not big enough to clear their orbital neighborhood.
So far, the IAU has classified five solar system objects as dwarf planets — including Ceres in the main asteroid belt, plus Pluto, Eris, Haumea and Makemake in the region beyond Neptune. 2026 ED138 joins a host of other celestial objects that are thought to be dwarf planets but haven’t yet been added to the IAU’s official list.
“The official list hasn’t moved since 2008,” Jurić told GeekWire in an email. “I’m not sure if there’s an active process that reviews candidates, and what are the timelines.”
Jurić and his colleagues hope additional observations will boost ED138’s chances of attaining true dwarf planethood.
“The next step in building the case would be to prove it’s round (in hydrostatic equilibrium),” he wrote. “The means to do that would be directly through occultations (and there’s a good chance of that, given it’s in a dense stellar field), and then thermal measurements plus modeling and light curves (or the absence of variability).”
Some 27 million years ago, a volcano in what’s now southeastern Arizona unleashed a spectacular series of eruptions, strewing more than 1,000 times as much volcanic material across the landscape as Mount St. Helens did in 1980.
The explosive eruptions blanketed the region, part of the Chiricahua Apache Nation’s traditional lands, with ash and pumice. Layered into this were massive pyroclastic flows that hardened into deposits of welded rhyolitic tuff that in some areas were nearly 1,600 feet (500 meters) thick, about three times the height of the Washington Monument. As the magma chamber emptied, the ground above it collapsed, leaving a gaping depression—the Turkey Creek caldera—that was roughly 12 miles (19 kilometers) wide and 4,900 feet (1,500 meters) deep.
An array of geologic processes, including erosion and weathering, gradually sculpted the welded layer of tuff into the collection of dramatic spires, hoodoos, and canyons that visitors to the caldera area encounter today.
The area was designated a national monument in 1924 to preserve its remarkable geology. In October 2026, it was redesignated as Chiricahua National Park (pronounced cheery-cow-ah). The OLI (Operational Land Imager) on Landsat 9 captured this cloud-free image of the new national park on July 2, 2026.
Individual rock spires are too small to distinguish, but the eroding rhyolitic tuff landscape appears gray. Stream valleys dense with trees and other vegetation, including Rhyolite Canyon and Bonita Canyon, snake across the landscape. With four biogeographic regions converging in the park—the Sonoran Desert, the Chihuahuan Desert, the Rocky Mountains, and the Sierra Madre—it is a haven of plant diversity.
Among the 1,000 species growing within the park’s varied desert, grassland, chaparral, deciduous forest, and coniferous forest ecosystems are agaves, prickly pear cacti, yuccas, manzanita, pine, fir, cypress, sycamore, juniper, and oak. The park’s location within the Chiricahua Mountains puts it among several “sky islands” in Arizona—isolated mountain ranges that emerge from the surrounding desert “sea.” According to the National Park Service, the range’s highest point (outside the park) rises 2,986 meters (9,795 feet) above sea level, more than 1,800 meters above the surrounding valley.
NASA Earth Observatory image by Lauren Dauphin, using Landsat data from the U.S. Geological Survey. Story by Adam Voiland.
Many readers will be familiar with Douglas Englebart’s 1968 so-called “Mother of All Demos”, in which he described many of the devices and technologies we would be using two or three decades later. Among these was a primitive computer mouse, but while famous it was by no means the earliest pointing device. At the recent Vintage Computer Festival Berlin, [Dmitriy Kostiuk] delivered a fascinating lecture of the history of the pointing device.
It’s a long video that we’ve placed below, and it’s an exhaustive examination of the topic from the earliest examples to the 1990s when mice became commoditized. It’s a surprise to find that the first pointing device was a trackball built for a 1950s Canadian warship, with a surprisingly modern-looking optical encoder. Englebart’s 1966 wooden block with its pair of wheels and potentiometers had a less-well-known and much more stylish competitor in the same year from Telefunken.
We visit the various design iterations as the form of what we’d call a mouse today took shape. It’s unexpected to find that those Sun mice with the spotty mouse pad weren’t from Sun at all, they were from Mouse Systems. The first mice from Microsoft and Apple make an appearance, as do some awful designs for 8-bit computrs. Remembering those in particular perhaps it’s as well we didn’t have the cash to buy such a disappointing product for ourselves.
The video is long, but interesting. Give it a watch.
Header image, Douglas Englebart’s prototype, Michael Hicks, CC BY 2.0.
Recently a new project was released by Praetorian. Praetorian is open-sourcing the offensive tools their red team actually uses on engagements. They call it 12 Caesars and their team is planning to release one tool a week for twelve weeks. Every tool is written in Go and ships as a single binary with zero external dependencies.
Each tool is assigned a Caesar name and a blog post, where you can learn more about these tools.
We’ll look at four of these tools, including the basic ones, to make this article suitable for everyone. Before we proceed, it’s important to remind you that you can only test systems you own or have explicit written authorization to test. We will use our lab for it.
Titus
Our first tool is Titus. Titus finds credentials, API keys, and tokens in source code, files, git history, container images, and more. The tool has 487 detection rules covering AWS, GCP, Azure, GitHub, Slack, databases and hundreds of other services. Similar to TruffleHog, it can validate credentials as it finds them by calling the provider APIs.
It’s also available as a Burp Suite extension and a Chrome extension.
kali > curl -sL -o titus https://github.com/praetorian-inc/titus/releases/latest/download/titus-linux-amd64
kali > chmod 777 titus
kali > ./titus --help
Let’s start by pointing it at test keys released by Truffle Security.
It found all the keys in the repo. Companies often publish their secrets by accident. Some live in the repositories for years, so it’s good to do regular checks to prevent unnecessary leakage.
Nerva
Nerva is a fingerprinter supporting 170 protocols across TCP, UDP, and SCTP, plus dozens of HTTP technology fingerprinters. You can feed it with open ports from naabu, nmap or other tools and it’ll tell you what’s actually running with its version.
kali > curl -sL -o nerva.tar.gz https://github.com/praetorian-inc/nerva/releases/download/v1.70.3/nerva_1.70.3_linux_amd64.tar.gz
kali > tar --no-same-owner -xzf nerva.tar.gz
kali > chmod 777 nerva
kali > ./nerva --help
Now let’s use our Ubuntu to show a basic test.
kali > ./nerva -t 192.168.131.9:22,11434
It will be way more useful when you work with big lists of corporate assets during a pentest.
Brutus
Brutus is a modern Hydra alternative. It supports more than 40 protocols including SSH, RDP, MySQL, PostgreSQL and a lot more. Brutus was built to work with Nerva or naabu output.
kali > curl -sL -o brutus.tar.gz https://github.com/praetorian-inc/brutus/releases/latest/download/brutus-linux-amd64.tar.gz
kali > tar --no-same-owner -xzf brutus.tar.gz
kali > chmod 777 brutus
kali > ./brutus --help
Each command has its own help menu to make it easy to work with.
kali > ./brutus creds --help
Now once again lets use our Ubuntu to spay passwords.
kali > ./brutus creds --target 127.0.0.1:22 --protocol ssh “admin:admin”
It was easy. As mentioned before, this tool chains with Nerva, and that’s how it becomes useful to test the entire infrastructure against common password and detection.
Julius
With AI services proliferating inside corporate environments, we want to know what LLM infrastructure is running on our hosts. Julius will fingerprint more than 60 AI services including Ollama, vLLM, LiteLLM, LocalAI, Hugging Face TGI, AWS Bedrock and AnythingLLM. It can also list available models from endpoints.
kali > curl -sL -o julius.tar.gz https://github.com/praetorian-inc/julius/releases/download/v1.5.1/julius_1.5.1_linux_amd64.tar.gz
kali > tar --no-same-owner -xzf julius.tar.gz
kali > ./julius --help
You can list all the AI services Julious can fingerprint:
kali > ./julius list
We will take a look at our machine.
kali > ./julius probe http://192.168.131.7:11434
Ollama sits on port 11434, and it’s important not to leave it exposed publicly, because everyone can use your models without authentication.
Summary
There are more tools available in this project. Most of them are meant to be chained together and work well this way. The company says its team is actively using these same tools during their engagements. While you won’t need everything at once, experiment with those tools and see what fits you best.
If you like red teaming, we have our Red Team Operator training, where we cover more tools and techniques to help you emulate real APT work, so you can give a company a realistic stress test and help make it secure.
Jess Asato’s public campaigning for victims of online abuse put her in the crosshairs of Grok’s deepfake scandal. Then the UK member of parliament became a victim of the abuse herself.
“Sovereign citizens” think they can live beyond the reach of the state. Now the movement has influencers—and they’re selling all sorts of anarchist courses to expectant families.
Iceberg A-81 slows its drift near the edge of South Georgia’s shallow underwater shelf in this image, acquired on October 20, 2026, by the MODIS (Moderate Resolution Imaging Spectroradiometer) on NASA’s Terra satellite.
NASA Earth Observatory/Michala Garrison
Some Antarctic icebergs linger close to home for decades, running aground near the ice shelves that spawned them or circling partway around the continent on coastal currents. Others, like Iceberg A-81, make a faster exit, heading north out of the Weddell Sea along a route well-traveled by the region’s bergs.
Fast is relative, though. After breaking from the Brunt Ice Shelf in January 2023, the roughly 1,550-square-kilometer (600-square-mile) berg spent more than three years in the Weddell Sea, carried along the coast by the clockwise-flowing Weddell Gyre. By May 2026, it reached the tip of the Antarctic Peninsula. It then moved north into the Scotia Sea, and by late October 2026, it approached the remote island of South Georgia in the South Atlantic Ocean, 2,300 kilometers (1,400 miles) north-northwest of the Brunt Ice Shelf.
This image, acquired by the MODIS (Moderate Resolution Imaging Spectroradiometer) on NASA’s Terra satellite, shows the berg on October 20. In the days before, its progress slowed noticeably, and it appeared to be bumping along the edge of the island’s underwater shelf, according to Jan Lieser of Australia’s Bureau of Meteorology and Christopher Shuman of the University of Maryland (retired). South Georgia has slowed and even stopped icebergs before. In 2025, for instance, Iceberg A-23A ran aground on the shelf and later broke apart.
Though Iceberg A-81 was a steadfast traveler once it broke free, it took its time in becoming an iceberg in the first place. For about 35 years, one of the Brunt Ice Shelf’s rifts known as Chasm 1 was relatively stable. Then, around 2012, it began growing again, and by 2019, it was advancing quickly enough that a break seemed imminent. But the floating glacial ice held on for several more years until finally, in January 2023, the berg let go.
Calving is a normal part of the life cycle of ice shelves, but scientists keep a close eye on Brunt, which has recently shed several large icebergs in quick succession and is home to the British Antarctic Survey’s Halley Research Station, a major base for Earth, atmospheric, and space science research since the 1950s. Besides A-81, the ice shelf calved Iceberg A-74 from the North Rift in 2021 and Iceberg A-83 from the Halloween Crack in 2024. A-74 has since broken up, while A-83 remains intact and is trailing A-81 northward, along with a handful of other icebergs that appear to be clearing out of the Weddell Sea.
NASA Earth Observatory image by Michala Garrison, using MODIS data from NASA EOSDIS LANCE and GIBS/Worldview. Story by Kathryn Hansen.
Sir Arthur Conan Doyle created one of the most beloved fictional detectives of all time in Sherlock Holmes, spawning countless novels, films, TV series, and so forth featuring the sleuth. Far fewer people know about the real-life inspiration for Holmes: a renowned surgeon at Scotland's University of Edinburgh named Joseph Bell, who taught Doyle when the author was still a young medical student. Bell is the subject of a new, eminently readable biography, Sleuth-Hound: The Case of the Real Sherlock Holmes, by medical historian Lindsey Fitzharris.
In 2020, Fitzharris hosted a documentary for the Smithsonian Channel, The Curious Life and Death Of…, exploring famous deaths, ranging from drug lord Pablo Escobar to magician Harry Houdini. Fitzharris performed virtual autopsies, experimented with blood samples, interviewed witnesses, and conducted real-time demonstrations in hopes of gleaning fresh insights. And last year she and her husband, caricaturist Adrian Teal, collaborated on an illustrated children's book, Dead Ends! Flukes, Flops, and Failuresthat Sparked Medical Marvels.
Preparations for Next Moonwalk Simulations Underway (and Underwater)
This 360-degree panorama from NASA’s Perseverance Mars rover shows Neretva Vallis, the dusty, long-dried river channel that cuts through the western rim of Mars’ Jezero Crater.
NASA/JPL-Caltech/ASU/MSSS
Over 1,645 Martian days, NASA’s Perseverance Mars rover measured the fine and ultrafine Martian dust particles found clinging to samples of spacesuit materials that are carried aboard the rover, including some that are small enough to penetrate the lungs and enter the bloodstream. The findings will be published Tuesday, Oct. 27, in the Proceedings of the National Academy of Sciences and could inform spacesuit and habitat design, dust-removal procedures, and crew health standards for future NASA missions to Mars.
“NASA has a long history of turning challenges into workable solutions and of finding creative ways to use the data that we have to answer questions beyond what it was originally collected for,” said Lindsay Hays, acting director, Planetary Science Division, NASA Headquarters in Washington. “Dust has been a surface-exploration challenge since the Apollo program. Perseverance is giving our engineers and flight surgeons measurements they can use to improve our existing designs well before the first American astronauts arrive on Mars.”
Lunar dust scratched visors, degraded outer spacesuit layers, and damaged their seals during NASA’s Apollo missions, and some crew members reported symptoms similar to hay fever.
Rounded by wind-driven collisions with other particles, dust grains on Mars are less abrasive than those on the Moon. They also are enriched in sulfur, chlorine, and iron and contain more silica than lunar dust. Regional and global dust storms on Mars can keep the grains recirculating throughout the atmosphere as well.
The rover carries a set of five samples of spacesuit material. The swatches, each three-quarters of an inch (20 millimeters) square, are part of a calibration target used to test the settings of SHERLOC (Scanning Habitable Environments with Raman and Luminescence for Organics and Chemicals), an instrument on Perseverance’s robotic arm. The calibration target for another instrument that provided the dust measurements, called PIXL (Planetary Instrument for X-ray Lithochemistry), carries a sample of Teflon and of basaltic glass.
Because Teflon contains no elements that PIXL can directly detect, whatever elemental signals the X-ray spectrometer picks up from that sample comes from dust resting on it.
The team also analyzed swatches of Teflon and Vectran, two materials used in spacesuits, on SHERLOC’s calibration target. NASA sent the swatches to Mars to study how spacesuit materials hold up on the planet’s surface.
“Perseverance’s main job is to search for signs of ancient microbial life, but the mission was also designed to help prepare for human explorers. That effort includes technology demonstrations like MOXIE (Mars Oxygen In-Situ Resource Utilization Experiment) and Ingenuity, as well as the spacesuit samples,” said Katie Stack Morgan, Perseverance’s project scientist at NASA’s Jet Propulsion Laboratory in Southern California.
Fine, ultrafine
While earlier measurements on Mars resolved dust particles down to about 3 micrometers across, PIXL detected two categories of even smaller particles: fine particles measuring less than 2.5 micrometers (a human hair is about 70 micrometers wide) and ultrafine particles around 100 nanometers (about 700 times thinner than a human hair). Particles on PIXL’s Teflon target and SHERLOC’s Vectran swatch averaged about 2 micrometers. On PIXL’s basaltic glass and SHERLOC’s Teflon swatch, dust particle sizes ranged down to about 100 to 300 nanometers.
This annotated composite image shows the location on NASA’s Perseverance of the calibration target for rover’s SHERLOC (Scanning Habitable Environments with Raman & Luminescence for Organics and Chemicals) instrument. At right is a close-up of the calibration target.
NASA/JPL-Caltech
Static electricity appears to determine which size dust particles stick to which surface. Dust grains become charged as they collide in the air, and different materials on the calibration target attract grains of different sizes. The finest particles stayed attached through years of driving and drilling. Organic polymers like SHERLOC’s Teflon spacesuit sample are common in the outer layers of spacesuits, and the results show they readily collect fine dust.
The study also found that some materials hold less dust than others, which could guide future choices of materials and protective coatings for spacesuits and habitats. Designs such as suitports, which let astronauts enter a suit attached to the outside of a habitat, and dual-chamber airlocks could reduce how much dust gets inside astronauts’ living quarters.
“The existence of Mars dust at these ultrafine sizes has been predicted for a long time, and PIXL gave us the chance to measure it directly on Mars,” said Scott VanBommel, a Perseverance scientist at Washington University in St. Louis and the paper’s lead author. “The larger clumps, the Martian dust bunnies, get shaken off over time. But the smallest particles stay behind, and those are the ones that pose the greatest challenge for human support systems.”
Chemically, the dust matches the iron- and sulfur-rich composition that earlier missions measured. The PIXL instrument also found the dust to be enriched in phosphorus and detected signs of calcium sulfate.
Protecting crews
On Earth, airborne particles, or particulate matter, below 2.5 micrometers (that is, fine particles) are tied to a range of negative health effects because they can penetrate deep into the lungs and enter the bloodstream. Studies have shown that ultrafine particles (those no larger than 100 nanometers) can travel from the nasal cavity to the brain along the olfactory nerve.
Martian dust is composed predominantly of silicate minerals and carries chemically reactive compounds, including perchlorates that can disrupt thyroid function and reactive iron that induces cellular damage. Scientists believe that the health risks of Mars dust depend on the quantity of dust and length of exposure.
The PIXL results are the first on-site measurements of fine and ultrafine particles on Mars, and this research can inform broader efforts to refine indoor dust-exposure limits for astronauts, develop safe habits, and establish ways to remove dust while exploring Mars.
NASA is already working on solutions to extraterrestrial dust hazards, using ground test facilities and lunar missions as proving grounds for future Mars explorers. In March 2025, the agency tested an Electrodynamic Dust Shield, which used electric fields to clear lunar regolith from glass and thermal radiator surfaces on the Moon. Developed at NASA’s Kennedy Space Center in Florida, it landed on the Moon aboard Firefly Aerospace’s Blue Ghost Mission 1. At NASA’s Johnson Space Center in Houston, engineers at the Lunar Development and Test Facility use vacuum chambers and lunar regolith simulant to test spacesuit components, mechanisms, and a Handheld Lunar Electrostatic Dust Mitigation tool ahead of Artemis missions to the lunar surface.
More about Perseverance
Managed for NASA by Caltech, JPL built and manages operations of the Perseverance rover on behalf of the agency’s Science Mission Directorate as part of NASA’s Mars Exploration Program portfolio. NASA JPL also built PIXL and SHERLOC.
Every day, Wikipedia biographies of living people are flagged for deletion because the subjects are not “notable” enough. How do these poor souls take the news?
A map depicts vegetated parts of Earth’s land surfaces from September 29 to October 4. Vegetation color is depicted on a spectrum ranging from dark green to light yellow to dark red. The largest patches of red vegetation appear in Alaska, northern Canada, Mongolia, and Russia. Smaller patches of red are visible in Australia.
NASA Earth Observatory / Lauren Dauphin
A similar global map depicts the redness of vegetation from October 5 to 11. The reddest areas have shifted equatorward, with more color visible in the Mid-Atlantic, the U.S. Southeast, southern Russia, China, and Mongolia.
NASA Earth Observatory / Lauren Dauphin
A map depicts vegetated parts of Earth’s land surfaces from September 29 to October 4. Vegetation color is depicted on a spectrum ranging from dark green to light yellow to dark red. The largest patches of red vegetation appear in Alaska, northern Canada, Mongolia, and Russia. Smaller patches of red are visible in Australia.
NASA Earth Observatory / Lauren Dauphin
A similar global map depicts the redness of vegetation from October 5 to 11. The reddest areas have shifted equatorward, with more color visible in the Mid-Atlantic, the U.S. Southeast, southern Russia, China, and Mongolia.
NASA Earth Observatory / Lauren Dauphin
September 29 to October 4
October 5 to 11
These maps show the redness of vegetation as measured by the OCI (Ocean Color Instrument) on the PACE (Plankton, Aerosol, Cloud, ocean Ecosystem) satellite in September and October 2026. Red foliage appears to peak in New England, northern Canada, and northern Russia from September 29 to October 4, then spreads southward into the Mid-Atlantic, Mongolia, and northern China from October 5 to 11 (right).
The Japanese tradition of momijigari, or “red leaf hunting,” stretches back more than a millennium, as evidenced by ancient poems describing journeys to admire fall foliage. In America, mentions of foliage trips began appearing in the historical record in the 19th century, around the time artists and poets such as Frederic Church and Emily Dickinson celebrated autumn color in depictions of the Northeast.
Modern-day leaf peepers have a new way to track and savor the seasonal phenomenon. The hyperspectral OCI (Ocean Color Instrument) on NASA’s PACE (Plankton, Aerosol, Cloud, ocean Ecosystem) satellite observes the planet’s oceans and vegetation daily at 286 spectral bands. Among this array are a few groups of wavelengths that allow scientists to track subtle changes in leaf pigments key to fall foliage displays, including anthocyanins (reds), carotenoids (yellows and oranges), and chlorophylls (greens).
NASA scientists can track fall color by measuring how much red, orange, and yellow forests show compared with green. Tracking the ratio over time reveals where leaves are changing and when color peaks. The maps above show vegetation “redness” from September 29 to October 4 (left) and October 5 to 11 (right). Areas shown in green have values near 1, meaning the satellite detects about as much red as green, and most leaves have not yet turned. Areas shown in light yellow and red have higher values, indicating progressively more red pigment relative to green.
The satellite detected particularly high levels of redness in parts of northern and eastern Russia, northern Alaska, and northern Canada from September 29 to October 4. In New England and upstate New York, redness began to fade during the week of October 5 to 11, even as it spread across much of the Midwest and the Mid-Atlantic. (Not all the yellows and reds on the maps represent fall colors. Crops in some agricultural areas, for instance, show high anthocyanin levels as they age and after they are harvested. Also, in some regions, clouds produce what appear to be gaps in the vegetation.)
Seeing Red in Vermont
Many of the reddest areas—such as the Adirondacks in New York, the Green Mountains in Vermont, and the White Mountains in New Hampshire—have large numbers of sugar maples (Acer saccharum) and red maples (Acer rubrum), deciduous trees that turn a brilliant shade of crimson in the fall. Blueberries, bilberries, sedges, mosses, and grasses likely contribute to the intense reds detected in marshy tundra areas in northern Alaska, Canada, and Russia.
Red and orange hues cover the forested ridges of central Vermont, while river valleys and lower-elevation areas are still green. The OLI (Operational Land Imager) on Landsat 9 captured this image on October 3, 2026.
NASA Earth Observatory / Lauren Dauphin
The OLI (Operational Land Imager) on Landsat 9 captured an image (above) of intensely red foliage around Ripton, Vermont, on October 3, 2026, around the peak of redness in the region. Poet Robert Frost, author of “October,” “The Road Not Taken,” “Nothing Gold Can Stay,” and several other poems that evoke fall foliage, kept a summer home and farm in Ripton and taught at Middlebury’s Bread Loaf School of English.
Some other satellites with hyperspectral sensors can measure fall foliage pigments in a way that is similar to PACE, but only in more localized areas and less frequently. PACE is the first satellite capable of measuring all three key leaf pigments—anthocyanins, carotenoids, and chlorophylls—across the entire planet every day or two.
“It’s the ability to collect time-series data of anthocyanins and carotenoids everywhere on Earth repeatedly that is game-changing,” said Karl Huemmrich, a vegetation scientist with the Goddard Earth Sciences Technology and Research II center at the University of Maryland, Baltimore County. Huemmrich, who is also a member of the PACE science team, was eager to work with the satellite because of OCI’s broad swath and short revisit time. “The time-series data allow us to determine peak redness and yellowness anywhere on Earth,” he said.
In the fall, leaves change colors as they lose chlorophyll, a green molecule that plants use to synthesize food. Since chlorophyll is not a stable compound, plants must continuously synthesize it, a process that requires ample sunlight and warm temperatures. As temperatures decrease and days shorten in autumn, levels of chlorophyll drop, causing greens to fade and presenting an opportunity for carotenoids and anthocyanins to show their colors.
Observing Leaves in a Canopy Near You
As part of the ongoing North American Phenology Campaign run by the Global Learning and Observations to Benefit the Environment (GLOBE) program, NASA data scientist Skye Caplan has been posting weekly foliage maps of vegetation redness. The maps show waves of red emerging in the high latitudes in August and shifting equatorward in September and October. The PACE team is asking the public to submit photos of fall foliage to help scientists “ground truth” the satellite observations and better understand how various factors influence vegetation color.
Fall foliage sprinkles a forested New England landscape in a photo taken in Meredith, New Hampshire, on October 11, 2026, by a participant in GLOBE’s North America Phenology Campaign.
GLOBE
“Changes in pigments can also occur when vegetation is stressed due to drought or insect damage,” said Caplan. She noted that changes like these likely help explain why PACE measures high levels of redness in agricultural regions of Brazil, Australia, and Canada that don’t track closely with broader seasonal changes.
“The more photos we can get from the ground, the better,” Caplan said. Ground photos help scientists refine PACE’s observations of vegetation color, which the team hopes will eventually support several lines of research. These include how the timing of spring greening and fall senescence is changing, how vegetation changes affect the global carbon cycle, and how leaf color influences wildfire risk. Scientists also want to know whether PACE can detect early warning signs of drought, insect infestations, and plant disease.
People can participate in the GLOBE campaign even if they live in an area without dense forests or picturesque fall foliage displays. Scientists also want ground observations of shrubs, grasses, wildflowers, evergreens, crops, and other vegetation. But when it comes to “red leaf hunting,” don’t delay, Caplan said. “Color changes happen kind of slowly, then all at once, and then they’re gone.”
NASA Earth Observatory images by Lauren Dauphin, using PACE data courtesy of Skye Caplan/NASA’s Goddard Space Flight Center and Landsat data from the U.S. Geological Survey.Photo courtesy of the GLOBE Program. Story by Adam Voiland.
File systems are something we rarely think about anymore, but in the early days of Windows, they could make a surprisingly big difference in how much of your pricey hard drive you actually got to use. FAT16 had one incredibly frustrating quirk with how it handled cluster sizes. Its inefficiency effectively punished you for buying a bigger hard drive, as it could leave you wasting much of the storage you paid for.
The U.S. Navy has added $2.4 billion to Fluor Marine Propulsion’s contract to run naval nuclear propulsion work at the Naval Nuclear Laboratory, the network of government labs that designs and supports the reactors powering every U.S. Navy submarine and aircraft carrier. Naval Sea Systems Command awarded the $2,409,077,590 cost-plus-fixed-fee modification on Sept. 24, 2026, […]
Login
