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Democratic Allies Must Join Forces in the Race for UAP Disclosure

Since February 2026, the United States Department of War (DOW), under the direction of President Donald Trump, has released an unprecedented number of documents, videos, and firsthand witness accounts detailing the United States’ extensive history of encounters with unidentified anomalous phenomena, or “UAP.”

Despite the questions that remain, this initiative under the Presidential Unsealing and Reporting System for UAP Encounters (PURSUE) has been nothing short of historic. For more than 75 years, Americans pleading for the truth on the issue have been routinely ridiculed and even misled by their own government. It’s difficult to imagine the nation’s posture being anything other than one of obfuscation, secrecy, and resistance to transparency.

Documents, particularly those detailing reports from senior intelligence officials encountering “orbs”, are a stark departure from the U.S. government’s nearly century-long position of secrecy.

Lawmakers, however, have been left with more questions than answers. Who or what flies with such impunity over our sensitive military installations? Who owns this technology? Are they a threat to national security?

Across the Pacific, members of Japan’s National Diet are confronting the same questions. The May 2026 file releases from the U.S. DOW disclosed two unresolved UAP incidents from the U.S. Indo-Pacific Command. Japanese legislators only learned the details of these cases near their own territory after the American file release—not through any internal channels.

Democratic allies, it seems, face a shared challenge. For too long, elected officials in our respective nations have been denied adequate information about the phenomena operating in our common security environment. And in the U.S., whenever we are informed, it’s only through the preferred methods and timing of unelected bureaucrats deeply entrenched in our national security apparatus. In Japan, by contrast, the Ministry of Defense has stated that information may be made public when something arises that it determines should be explained.

But this raises a fundamental question: should the government alone decide what should be explained to the public?

If a grave national security threat truly exists, then elected representatives have been left with little choice but to entrust the security of their nations to the very institutions that have obscured the truth from us and even each other.

It is therefore incumbent upon us—Representatives solely accountable to the citizens of our respective nations—to work together and to seek the truth wherever we may find it; both for the good of our people and to defend against whatever threats we face from strategic competitors.

As mentioned above, among the files released by the U.S. DOW were highly significant firsthand reports from high-ranking officials in the Office of the Director of National Intelligence. The documents detail a search operation at a classified missile testing site in the Western United States, explicitly for aerial phenomena:

En route, ground teams reported spotting a UAP on FLIR [Forward Looking Infrared], describing it as “super-hot,” low to the ground, and moving east then south at high speed. The object then split into two and changed direction. Upon arrival, we scanned the area using NVG [Night Vision Goggles], FLIR, and the naked eye. The ground team suddenly radioed that the object had risen from the ground, approached within ten feet of the helicopter, dropped below us, and then sped away.

The documents were accompanied by what the DOW labeled as “related photos.”

Accounts such as these are hardly “proof” of anything, but for elected officials, they do cement the reality of our national security concerns. Missing from this account—or any account we have been allowed to access—is an answer to a fundamental question: What do the various U.S. government agencies believe these objects are? Are they merely civilian drones? Do they represent technology belonging to a foreign actor? And if someone within the government does know, who decides that elected officials shouldn’t?

Members of Japan’s UAP Parliamentary League, led by former Japanese Defense Minister Yasukazu Hamada, share similar concerns.

DOW data, released through the Pentagon’s All-domain Anomaly Resolution Office (AARO) in August of 2023, identified specific regions of Japan, particularly in the western and southern parts of the country, as being among the world’s notable hotspots for UAP reports.

One such instance occurred as recently as July of last year. Security guards at the Genkai Nuclear Power Station in Saga Prefecture observed three luminous objects in the sky above the facility. The lights remained visible for nearly two hours; long enough for local police to arrive and observe them. The police stated that what they themselves observed was an airplane, leaving a discrepancy between the two accounts. The incident was also recorded by Kyushu Electric Power’s security cameras, but the footage has not been made available even to members of the National Diet. Police have likewise declined to disclose related information on the grounds that the matter remains under investigation. As a result, elected lawmakers still lack access to the information necessary to independently assess the incident, and to this day, members of Japan’s National Diet have no answers.

Like their American counterparts, Japanese lawmakers have been left without the tools or information for proper oversight despite reports of UAP operating near critical infrastructure within restricted airspace.

It is no longer acceptable for elected representatives to be agnostic on this issue. Events such as these, along with countless videos now made publicly available, are more than mere optical illusions and cannot be dismissed on account of prosaic explanations like parallax effect. For many members of Congress and members of Japan’s UAP Parliamentary League, the evidence presented before us indicates an unknown technology.

Our understanding of what is technologically feasible in propulsion, the manipulation of physical matter, and even space-time itself is being challenged. From what we know, our current defense capabilities appear insufficient. Furthermore, the origin of these phenomena remains unknown—not only to the U.S. and Japan, but seemingly to other nations as well. China, for instance, recently established its own military body dedicated to investigating UAP, even supplementing human resources with artificial intelligence dedicated to tracking what the People’s Liberation Army refers to as “Unidentified Air Conditions.”

We are, by all indications, in a global arms race for technological supremacy, one that is rapidly rendering today’s weapons obsolete through advances in quantum technology, artificial intelligence, and drone warfare. UAP and whatever technology allows them to operate with apparent impunity over sensitive military and nuclear installations could redefine the competition.

If harnessed by democratic allies, breakthroughs could bolster deterrence and stability in the South China Sea. Conversely, failure to establish a coordinated effort among democratic allies could give China an unforeseen technological advantage over a future invasion of Taiwan, making an already difficult fight impossible.

U.S. global leadership, along with the territorial integrity of the Pacific are at stake. For members of Japan’s National Diet, UAP investigations are of great national importance—an issue that demands cross-party attention.

As for their American counterparts, it’s clear representatives can’t reach the truth through traditional pathways that amount to asking the Central Intelligence Agency ‘nicely.’ It stands to reason that close alliances with democratic allies like Japan may be the most viable pathway for disclosure.

Indeed, if our tools are limited in scope, perhaps new revelations made by democratic allies provide a unique leverage point. After all, it was the Trump administration’s disclosure under the PURSUE program that significantly increased pressure on Japan’s Defense Ministry to acknowledge its own previously undisclosed UAP-related activities.

This is why we, as elected representatives of our nations, have engaged the Emerging Technologies Interparliamentary Caucus (ETIC) as a platform for international dialogue regarding emerging technologies and the security threats presented by UAP. Comprised of representatives from across the globe, the ETIC presents a rare opportunity to ensure elected representatives are equipped to assess potential threats, safeguard our nations, and prepare for the realities of emerging technologies in the 21st century.

Whether the phenomena we are encountering originate from an adversary or something else entirely, democratic nations cannot afford to be complacent.

The people of our nations deserve answers, and we intend to find them.

Rep. Eric Burlison (R-MO-07) is the Chairman of the Subcommittee on Economic Growth, Energy Policy, and Regulatory Affairs. 

Yasukazu Hamada is a Member of the House of Representatives, Japan, Former Minister of Defense, and Chairman of the UAP Parliamentary League.  

Yoshiharu Asakawa is a Former Member of the House of Representatives, Japan, and Assistant to the Chairman of the UAP Parliamentary League.

Android 17 QPR1 Stable Update Rolls Out to Pixel Phones With New UI and Pixel Features

16 September 2026 at 06:18

Google has started rolling out the Android 17 QPR1 stable update to compatible Pixel devices, building on the features introduced with Android 17 while adding new animations, Quick Settings changes, multitasking improvements and additional health features.

The update covers a wide range of Pixel phones and tablets, extending from the Pixel 6 generation through the newly released Pixel 11 family. For users coming from the Android 17 QPR1 beta program, the final release is also arriving as a relatively small update rather than requiring a complete system reset.

Android 17 QPR1 Gives the System UI a More Expressive Look

One of the most obvious changes in Android 17 QPR1 is the increased use of blur and transparency throughout the system interface.

The volume panel now uses a semi-transparent design with dynamic colors, while the expanded volume interface has received a visual update. Google has also added background blur to the power menu, giving system controls a more layered appearance.

These changes make the interface feel less static and put more emphasis on depth, transparency and animated transitions.

New Material 3 Multitasking Interface

These changes are part of Google’s broader Material 3 design direction, which emphasizes more expressive motion, adaptive colors and updated interface components.

When several apps are open, the system media and multitasking interface now uses a Material 3-style carousel. Instead of displaying a row of simple dots at the bottom, the interface provides previews of other open applications.

The active app card can also shrink to make room for additional previews, making it easier to recognize and switch between recently used apps.

Quick Settings Get New Animations and Controls

The Quick Settings panel receives several practical changes in this release.

Google has introduced new elastic-style animations when opening Quick Settings, while an edit button is now displayed in the lower-right area for easier customization.

The mobile data tile also gains a “Don’t ask me again” option. Another new addition is a dedicated Keyboard Quick Settings tile, which provides faster access to the system keyboard switcher.

Screen recording has also been adjusted. The tool now defaults to the application that was used for the previous screen recording session, potentially reducing the number of steps needed to start another recording.

Home Screen Menus Are More Clearly Organized

Android 17 QPR1 changes several interactions on the Pixel home screen.

Long-pressing an app icon now separates app-specific shortcuts from system-level actions such as widgets and bubbles. This creates a clearer distinction between functions provided by the app and Android’s own controls.

Long-pressing an empty area of the home screen also opens an updated wallpaper switching interface. The new design uses more noticeable rounded corners and a cleaner arrangement of menu options.

Settings Gets New Material 3 Expressive Icons

The Settings application is another area receiving a visual update.

Android 17 QPR1 introduces new Material 3 Expressive icons in Settings. The design language was previously seen on Pixel Watch devices and is now being brought more prominently to the phone experience.

Google has also added a new animation when users double-click the power button from the lock screen to launch the camera.

Health Connect Tracks More Activity Data

Health-related tracking also gets an expansion in Android 17 QPR1.

Health Connect can now track additional activity measurements, including distance traveled and calories burned, alongside existing step information.

This gives Pixel users more data points for monitoring everyday movement without requiring every activity metric to be handled by a separate application.

Android 17 QPR1 Compatible Pixel Devices

The stable update is available across a broad range of Google Pixel phones and tablets, covering several generations from the Pixel 6 series onward:

  • Pixel 6 and Pixel 6 Pro
  • Pixel 6a
  • Pixel 7, Pixel 7 Pro and Pixel 7a
  • Pixel Tablet
  • Pixel Fold
  • Pixel 8, Pixel 8 Pro and Pixel 8a
  • Pixel 9, Pixel 9 Pro, Pixel 9 Pro XL, Pixel 9 Pro Fold and Pixel 9a
  • Pixel 10, Pixel 10 Pro, Pixel 10 Pro XL, Pixel 10 Pro Fold and Pixel 10a
  • Pixel 11, Pixel 11 Pro, Pixel 11 Pro XL and Pixel 11 Pro Fold

The inclusion of the latest Pixel 11 series means the QPR1 release covers Google’s recent Pixel generations as well as several older devices.

What Beta Users Need to Know

Users who are currently running Android 17 QPR1 Beta 9 should receive a relatively small update to move to the stable release.

However, users participating in the Android Beta Program may need to exit the beta program before receiving the stable OTA update, depending on their current enrollment status.

The stable update is being distributed over the air and does not require users to erase their device data as part of the normal upgrade process.

Android 17 QPR1 Is More Than a Visual Update

While the new blur effects and Material 3 styling are among the most visible changes, Android 17 QPR1 also improves everyday interactions through redesigned multitasking, Quick Settings controls, home screen menus and additional Health Connect measurements.

For Pixel owners, the update therefore represents a combination of visual refinement and practical interface changes, rather than simply another maintenance release. The continued Android Beta Program will also allow Google to test future QPR releases and feature updates on supported devices.

The post Android 17 QPR1 Stable Update Rolls Out to Pixel Phones With New UI and Pixel Features appeared first on IGeeKphone China Phone, Tablet PC, VR, RC Drone News, Reviews.

Breaking the Ice: Origins of Carbon Oxides on Uranian Moons

11 September 2026 at 22:06

Uranus close-up

For decades, astronomers have tried to decipher the source of carbon oxides on Uranus’s largest moons from ground-based telescopes. A recent study has leveraged JWST spectroscopy and laboratory experiments to identify carbon oxides and their origins for Ariel, Umbriel, Titania, and Oberon.

Unknown Origins of Carbon Oxide Enrichment

Forty years ago, the Voyager 2 spacecraft flew past Uranus and its twenty-seven moons, sending back prized portraits of the planet’s large and tidally locked satellites Miranda, Ariel, Umbriel, Titania, and Oberon. These images revealed extensive valleys, smooth plains, deep canyons, and possible icy volcanic (cryovolcanic) activity across the surfaces of the icy moons — the telltale signs of intense geologic activity. While Voyager 2 could take spectacular pictures, the spacecraft was not capable of identifying the molecules and materials making up these active surfaces.

Six largest moons of Uranus

Voyager 2 images of Uranus’s six largest moons. Click to enlarge. [NASA / JPL-Caltech / Ted Stryk; CC BY-NC-ND 4.0]

In the decades that followed, astronomers have used ground-based near-infrared spectroscopy of these moons to investigate their chemical compositions. These observations have detected weak carbon dioxide and hints of carbon monoxide ice features on the moons with clear spatial trends across the moons’ surfaces, but the origins of these carbon oxides remain unknown. There are two potential explanations for the presence of these molecules: 1) carbon oxides are native to the Uranus system, present from formation, or 2) they formed via radiolysis, in which charged particles trapped in Uranus’s magnetic field interact with water ice and carbon-bearing molecules on the moons’ surfaces.

Ground-based detections are limited due to contamination from Earth’s atmosphere as well as the overall weakness of the carbon dioxide spectral features, thus space-based near-infrared observations of the Uranian moons are necessary to better constrain the carbon oxides on the satellites. Luckily, JWST’s Near-Infrared Spectrograph (NIRSpec) now offers astronomers unimpeded access the moons’ carbon oxide spectral features.

Chemical Clues from Space and in the Lab

In 2024, a study acquired NIRSpec observations of Uranus’s moon Ariel, revealing prominent carbon dioxide features and confirming the presence of carbon monoxide ice hinted at by ground-based studies. Expanding on these observations to include Umbriel, Titania, and Oberon alongside Ariel, Richard J. Cartwright (Johns Hopkins University) and collaborators obtained JWST NIRSpec spectroscopy of Uranus’s four largest moons in hopes of disentangling the origin story of their carbon oxides.

Leading and trailing diagram

Diagram illustrating the leading and trailing sides of a moon orbiting Uranus. Click to enlarge. [AAS Nova/Kerry Hensley]

In addition to the JWST spectra, Cartwright and team performed laboratory experiments measuring the spectral properties of carbon dioxide ice over a range of very low temperatures (tens of kelvin). These experiments provided a better understanding of the spectral properties and nature of carbon dioxide on the surfaces of the Uranian moons. Comparing the JWST spectra with the laboratory spectra, the authors found that Ariel, Umbriel, Titania, and Oberon exhibit a variety of spectral features resulting from carbon dioxide ice, carbon monoxide ice, and other carbon-bearing molecules. The presence of these molecules varies between the leading and trailing hemispheres of the moons, these variations appearing strongest in Ariel and Umbriel. The carbon dioxide and carbon monoxide spectral features are stronger on the trailing hemispheres, decreasing with increasing distance from Uranus for all four moons.
spectral ratios

Spectral ratios of the trailing and leading hemispheres for each moon, labeling spectral features of multiple carbon-bearing molecules. Click to enlarge. [Cartwright et al 2026]

Carbon Oxide Origins

What does this mean for the origins of the carbon oxides on the Uranian moons? Spectral features of carbonate minerals and the widespread presence of carbon dioxide throughout the Uranus system suggest that these compounds exist natively. On the other hand, the concentration of carbon oxide features on the trailing hemispheres supports radiolytic production as these hemispheres are bombarded with more ionizing particles from Uranus’s magnetosphere.

Based on these results, the authors have postulated that both origin scenarios, native presence and radiolysis, are required to fully explain the presence of carbon oxides. Future laboratory studies and JWST observations will continue to reveal the nature and composition of bodies in the Uranus system, furthering our understanding of our solar system siblings.

Citation

“Tracing the Source of Carbon Oxides on the Large Moons of Uranus,” Richard J. Cartwright et al 2026 Planet. Sci. J. 7 199. doi:10.3847/PSJ/ae8818

The post Breaking the Ice: Origins of Carbon Oxides on Uranian Moons appeared first on AAS Nova.

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