Binance.US plans to apply for a CFTC designated contract market license next month as it expands into prediction markets and derivatives.
The post Binance.US plans CFTC application in prediction market expansion appeared first on Crypto Briefing.
On Wednesday, Aug. 12, a total solar eclipse will be visible in parts of Greenland, Iceland, northern Russia, the Atlantic Ocean, Spain, and a small corner of Portugal. NASA will stream the eclipse live with views across the path and interviews with subject matter experts through a variety of platforms.
Learn where to watch online:
Viewers in other places in the Northern Hemisphere also will have the chance to experience a partial solar eclipse, including parts of the U.S. (from Alaska to North Carolina), most of Canada, much of Europe, and northwestern Africa.
During the eclipse, NASA will conduct experiments in the path of totality. To investigate the dynamics of the Sun’s corona, a NASA-funded science team will chase the Moon’s shadow with a WB-57 high-altitude research aircraft. The NASA-supported Nationwide Eclipse Ballooning Project is sending students from several U.S. universities to Iceland and Spain to launch scientific balloons before, during, and after the eclipse to research how the temporary darkening of our skies during the eclipse affects Earth’s atmosphere.
NASA’s eclipse coverage is as follows (all times Eastern):
Wednesday, Aug. 12
NASA photography coverage
Photos of the eclipse, dependent on visibility, will be available shortly after the eclipse. View images on the agency’s Flickr account.
Watch, engage on social media
During the broadcast, NASA experts will answer questions submitted on social media. Send in your questions and let people know you’re watching the eclipse on X, Facebook, and Instagram by following and tagging these accounts:
X: @NASA, @NASASolarSystem, @NASAScience_
Facebook: NASA, NASASolarSystem, @NASAScience
Instagram: @NASA, @NASASolarSystem, @NASAScience_
Learn more about the eclipse at:
https://science.nasa.gov/eclipses
-end-
Abbey Interrante / Karen Fox
Headquarters, Washington
301-201-0124 / 202-358-1600
abbey.a.interrante@nasa.gov / karen.c.fox@nasa.gov
Solflare's integration simplifies cross-chain asset transfers, potentially boosting Solana's adoption by reducing onboarding friction and enhancing user trust.
The post Solflare launches simpler cross-chain deposits powered by Aurora Intents appeared first on Crypto Briefing.
Zcash's swift infrastructure overhaul highlights the critical need for robust cryptographic audits to maintain trust in privacy protocols.
The post Zcash Ironwood pool receives $80M on first day following security upgrade appeared first on Crypto Briefing.
A team of Bellevue, Wash., high schoolers soared above teams from France, Japan, the UK, and Ukraine to win the International Rocketry Challenge in England over the weekend.
Washington Youth Aerospace, a team made up of six ninth graders from Bellevue’s Interlake High School, represented the United States in the competition at the Farnborough International Airshow. Team members include Daniel Tadesse, Bao-Ky Tran, Mikhail Antipin, Antoine Vigneron, Nikhil Sirivara, and Anay Mediwala.
With a target altitude of 750 feet, the team launched its rocket, carrying a raw egg payload, to an altitude of 765 feet with a flight time of 38.16 seconds.
The rocket launch counts for 60% of a team’s score and a presentation for judges counts for 40%. The team ranked first in both categories.
“Our success in the competition is extremely special given the work we have been putting in from middle school,” team member Nikhil Sirivara told GeekWire. “We could not have done this without the mentors and friends who helped us along the way and this win has inspired us to aim even higher going forward.”
Washington Youth Aerospace finished second in May at the 2026 National Finals of the American Rocketry Challenge, overcoming a last-minute scramble to replace a rocket motor that was lost in the mail. The team stepped in to represent the U.S. in the international event when the national finals winner from California had a scheduling conflict.
Sudheer Sirivara, a parent advisor and chaperone, said the students got a chance to interact with the teams from other countries and also had a cultural exchange program where each group presented something unique about their hometown.
They also explored interesting aircraft, including Black Hawk and Chinook helicopters, and C-130 and F-35 airplanes. The team had a chance to see London before returning to the Pacific Northwest on Sunday.
“This remarkable achievement reflects months of dedication, innovation, teamwork, and perseverance,” the American Rocketry Challenge said in a LinkedIn post. “From designing and testing their rocket to competing on the global stage, these students demonstrated the technical skill and determination that define the next generation of aerospace leaders.”
The American Rocketry Challenge is the flagship STEM initiative from the Aerospace Industries Association (AIA) trade group, and is supported by industry partners as a way of strengthening the workforce pipeline of engineers and scientists.
Washington Youth Aerospace is looking forward to participating in the NASA Student Launch Initiative (SLI) next, as well as next year’s rocket challenge.
Welcome to Edition 9.04 of the Rocket Report! We've had to wait an extra week for SpaceX to get its 13th Starship test flight off the ground. A last-second abort on July 16 led engineers to roll the booster back to its hangar in South Texas to swap out engines. Starship is now back on the launch pad. Liftoff is set for Friday evening. A flawless launch and reentry will put SpaceX on the cusp of an orbital flight later this year. Ars will have a comprehensive recap story after the completion of the test flight.
As always, we welcome reader submissions. If you don't want to miss an issue, please subscribe using the box below (the form will not appear on AMP-enabled versions of the site). Each report will include information on small-, medium-, and heavy-lift rockets, as well as a quick look ahead at the next three launches on the calendar.
India's first private rocket reaches orbit. Indian space officials celebrated the debut flight of Skyroot Aerospace’s Vikram-1 rocket, India’s first fully commercial satellite launcher, as a “grand success” Saturday after an on-target climb into a 280-mile-high orbit following liftoff from an island spaceport in the Bay of Bengal, Ars reports. The Vikram-1 lifted off from India’s primary spaceport on Sriharikota Island around midday local time. The launch was delayed more than a half-hour to resolve a last-minute technical problem. The countdown resumed, culminating in the command to ignite Vikram-1’s solid-fueled first stage booster to propel the rocket off the launch pad.
© Zhou Quan/VCG via Getty Images
NASA MAVEN (Mars Atmosphere and Volatile Evolution) mission scientists have uncovered a key puzzle piece in understanding certain types of auroras on Mars, finding that they form in a similar way to Earth-based auroras.
Results published Thursday in Nature Communications show the same mechanism that circulates and catapults charged particles into Earth’s atmosphere is happening at Mars on much smaller scales because of differences in the two planets’ magnetic fields.
The MAVEN spacecraft, in orbit around Mars, experienced a loss of signal with ground stations on Earth on Dec. 6, 2025. On June 3, NASA declared the mission had concluded after finding the spacecraft to be unrecoverable. However, data from the mission is still being used to inform NASA science and future missions to Mars.
When the Sun’s magnetic field lines get close to Earth’s magnetosphere, the large magnetic bubble protecting the planet, they can reconnect and inject energy and mass throughout Earth’s magnetosphere and magnetotail, ultimately firing electrons back into the atmosphere to generate Earth’s auroras. This process, called the Dungey cycle, drives electrical currents, accelerates charged particles that create auroras, and controls the circulation of plasma in Earth’s magnetosphere and ionosphere.
This new study shows that a miniature version of the Dungey cycle is happening over Mars’ strong crustal magnetic fields, which gives scientists a better look into the physics of Martian auroras.
“We knew that magnetic reconnection was happening at Mars but did not expect it to be like the Dungey cycle,” said Shaosui Xu, lead author of the study and associate research physicist at the Space Sciences Laboratory at the University of California, Berkeley.
Mars does not have a global magnetic field like Earth. Earth’s magnetic field is created by our planet’s churning core, while Mars has numerous miniature magnetospheres that arise from intensely magnetized crust scattered around the planet. These regions were formed around 4 billion years ago when lava cooled in the presence of Mars’ ancient global magnetic field, which has since disappeared due to intense solar wind stripping the planet’s atmosphere.
The MAVEN mission has observed highly localized auroras over these crustal fields, similar to Earth’s auroras at the poles, but it wasn’t until now that scientists could fully understand the physics of how they form. The study used several instruments aboard the MAVEN spacecraft to build up a picture of the Dungey-like behavior: the Magnetometer and Solar Wind Electron Analyzer instruments, which were used to determine the magnetic configuration and derive electrical currents, and the STATIC (Suprathermal and Thermal Ion Composition) instrument, which was used to measure plasma flows in the ionosphere.
“We really pushed the limit of STATIC to get the data we needed,” said Xu. “It was the final piece to the puzzle in understanding these localized auroras.”
The realization that a Dungey-like cycle was happening within these crustal magnetic fields answered the question of how the electrons were being energized to create the auroras. It also shows that a Dungey-like mechanism can happen on both large and small scales, giving more insight into where in the solar system this process could be taking place.
“This is a remarkable result that changes how we think of Martian auroras and is another important step toward understanding why Mars and Earth have evolved so differently despite being governed by the same underlying physics.” said Shannon Curry, MAVEN’s principal investigator and a research scientist at the Laboratory for Atmospheric and Space Physics at the University of Colorado Boulder. “I am incredibly proud of our team’s work on this discovery and excited to uncover new insights into the Red Planet and its evolution.”
By finding out more about this process, scientists also are gaining a better understanding of how the solar environment interacts with the Red Planet as a whole, which is essential for future robotic and crewed missions.
“I remember in graduate school discussing with my advisor how the cycling of crustal magnetic fields could work at Mars,” said Xu. “It’s incredible to be part of the team that found the answer to that question.”
The MAVEN mission is part of NASA’s Mars Exploration Program portfolio. The mission’s principal investigator is based at the Laboratory for Atmospheric and Space Physics at the University of Colorado Boulder, which also is responsible for managing science operations and public outreach and communications. NASA’s Goddard Space Flight Center in Greenbelt, Maryland, manages the MAVEN mission. Lockheed Martin Space built the spacecraft and is responsible for mission operations. NASA’s Jet Propulsion Laboratory in Southern California provides navigation and Deep Space Network support.
For more information on NASA’s MAVEN mission, visit:
https://science.nasa.gov/mission/maven/
Karen Fox / Alana Johnson
Headquarters, Washington
240-285-5155 / 202-672-4780
karen.c.fox@nasa.gov / alana.r.johnson@nasa.gov
Lonnie Shekhtman
NASA’s Goddard Space Flight Center, Greenbelt, Md.
lonnie.shekhtman@nasa.gov
Microsoft is redesigning Windows Search with improved local results, fewer promotional elements, better file previews, and more control over web-based search.
The post Windows Search Gets a Major Revamp Focused on Usability appeared first on TechRepublic.
Microsoft is redesigning Windows Search with improved local results, fewer promotional elements, better file previews, and more control over web-based search.
The post Windows Search Gets a Major Revamp Focused on Usability appeared first on TechRepublic.
Jurassic Park, while beloved as a film, has been the subject of snarky memes for the infamous line in which one of the characters declares, "This is a Unix system, I know this!" while using a computer with an unusual 3D file manager interface.
Despite the memes, the film's production team was meticulous in accurately sourcing the right PCs (and adjacent details) for the sets—not too much of a surprise, given writer Michael Crichton's background with computing and his obsessive attention to detail in the book the film is based on.
© Universal Pictures
Before replacing Windows 10 with ChromeOS Flex, check device support, hardware, apps, security requirements, and backup options.
The post 5 Things to Check Before Installing ChromeOS Flex on a Windows 10 PC appeared first on TechRepublic.
Before replacing Windows 10 with ChromeOS Flex, check device support, hardware, apps, security requirements, and backup options.
The post 5 Things to Check Before Installing ChromeOS Flex on a Windows 10 PC appeared first on TechRepublic.
Solana’s user-growth story is one of the strongest narratives around the network, but it needs careful handling. Wallet counts can be encouraging, yet they do not tell the whole story. What matters is whether users keep coming back and whether applications are generating durable activity.
That makes the current address-growth discussion useful but incomplete. It points to momentum, not final proof.
For more details, visit the official GitHub platform.
A new wallet is not always a new long-term user. It can come from incentives, farming, bots, migrations, or temporary campaigns. That is why serious analysis has to look at transactions, fees, app activity, and retention as well.
Solana’s advantage is that its low-cost environment makes repeat activity easier. The challenge is proving that low friction turns into real loyalty.
The strongest case would include rising DeFi usage, steady stablecoin flows, app-level retention, and validator economics that show demand is meaningful. Those signals would make address growth much more convincing.
Until then, the market should treat wallet growth as a positive early indicator rather than a complete adoption story.
The practical takeaway is that Solana stories now have to be read through both market structure and product execution. A headline can create attention, but the more durable signal is whether the underlying source points to real activity, a real filing, a real integration, or a measurable change in how users and institutions behave.
That is why this development is worth separating from ordinary market noise. It gives readers a specific point to track over the next few sessions rather than a vague reason to be bullish or bearish. If follow-up data confirms the direction, the story can build. If not, it still gives the market a clearer snapshot of where attention is concentrating today.
The cleaner way to read this story is not to force it into a simple bullish or bearish box. For Solana readers, the useful part is the change in context. A new filing, integration, market signal, or regulatory step can alter how traders think about the next few sessions even when it does not instantly change price.
That is especially true after the last few volatile weeks, when crypto has been dealing with a mix of ETF flows, legal updates, exchange listings, protocol upgrades, and shifting liquidity. The market is no longer reacting to one dominant theme. It is weighing several smaller signals at once, and that makes source-backed developments more important than ordinary chatter.
For Bitcoinist readers, the important question is what this changes from here. If follow-up data, filings, governance updates, or wallet movement confirm the direction, the story can develop into a larger market theme. If the next update is weak, delayed, or contradicted by new data, the market may quickly move on.
That is why the scope matters. This article is not treating the development as a guaranteed price trigger. It is treating it as a fresh signal inside a market that is trying to sort durable activity from short-term noise. The distinction is important because crypto narratives can move faster than the facts behind them.
The next thing to watch is whether this becomes part of a wider pattern. In some cases that means more institutional flows. In others it means stronger developer adoption, cleaner regulatory access, deeper exchange liquidity, or a clearer technical roadmap. Either way, the story is strongest if it is followed by measurable execution rather than another round of speculative headlines.
This report is based on Solana ecosystem materials and the source pack’s network-growth lead.
This article was written by the News Desk and edited by Samuel Rae.
Source: GitHub
Solana’s growth story is often told through speed, fees, and developer momentum. Address growth adds another layer, but it needs to be read carefully. A higher wallet count can be encouraging, yet it does not automatically prove that a network has deeper economic activity.
That is the right way to look at the current Solana signal. The market wants to know whether user growth is sticky, whether dApps are retaining activity, and whether validators and applications are seeing enough demand to make the network’s momentum durable.
For more details, visit the official GitHub platform.
New wallets can reflect real adoption, speculative farming, airdrop behaviour, or short-term campaign activity. That is why address counts are useful, but not complete. They need to be paired with fees, transactions, DEX activity, app usage, and retention.
For Solana, the positive case is that low fees and fast execution make it easier for users to keep coming back. The challenge is proving that those users are not just passing through.
The strongest confirmation would come from broader app-level data: more users on DeFi protocols, stronger NFT or gaming activity, sustained stablecoin transfers, and fee demand that does not disappear after incentives fade.
Until then, address growth is a constructive sign, not a finished thesis. Solana has the attention. The question is how much of that attention becomes durable network value.
The practical takeaway is that Solana stories now have to be read through both market structure and product execution. A headline can create attention, but the more durable signal is whether the underlying source points to real activity, a real filing, a real integration, or a measurable change in how users and institutions behave.
That is why this development is worth separating from ordinary market noise. It gives readers a specific point to track over the next few sessions rather than a vague reason to be bullish or bearish. If follow-up data confirms the direction, the story can build. If not, it still gives the market a clearer snapshot of where attention is concentrating today.
The cleaner way to read this story is not to force it into a simple bullish or bearish box. For Solana readers, the useful part is the change in context. A new filing, integration, market signal, or regulatory step can alter how traders think about the next few sessions even when it does not instantly change price.
That is especially true after the last few volatile weeks, when crypto has been dealing with a mix of ETF flows, legal updates, exchange listings, protocol upgrades, and shifting liquidity. The market is no longer reacting to one dominant theme. It is weighing several smaller signals at once, and that makes source-backed developments more important than ordinary chatter.
For NewsBTC readers, the important question is what this changes from here. If follow-up data, filings, governance updates, or wallet movement confirm the direction, the story can develop into a larger market theme. If the next update is weak, delayed, or contradicted by new data, the market may quickly move on.
That is why the scope matters. This article is not treating the development as a guaranteed price trigger. It is treating it as a fresh signal inside a market that is trying to sort durable activity from short-term noise. The distinction is important because crypto narratives can move faster than the facts behind them.
The next thing to watch is whether this becomes part of a wider pattern. In some cases that means more institutional flows. In others it means stronger developer adoption, cleaner regulatory access, deeper exchange liquidity, or a clearer technical roadmap. Either way, the story is strongest if it is followed by measurable execution rather than another round of speculative headlines.
This article is based on Solana ecosystem materials and the source pack’s network-growth lead.
This article was written by the News Desk and edited by Samuel Rae.
This report is based on information from GitHub. at GitHub
Australia has fired a live missile from a prototype ground-based air defense system for the first time, hitting a cruise missile target at the remote Woomera Test Range in South Australia and marking the debut pairing of an Australian-made radar with the U.S. Navy’s Aegis Combat System. The Department of Defence in Canberra announced the […]3 min read
Following its longest hibernation period ever of nearly a year, NASA’s New Horizons spacecraft has emerged in good health and is ready to begin transmitting science data gathered in the distant Kuiper Belt far beyond Pluto.
On June 23, flight controllers at the Johns Hopkins Applied Physics Laboratory (APL) in Laurel, Maryland, confirmed New Horizons, acting on stored commands uplinked to its main computer last July, had safely awakened from a 321‑day hibernation period that began Aug. 7. With the spacecraft now approximately 5.9 billion miles (9.5 billion kilometers) from Earth, the radio signals carrying that confirmation took about 8 hours and 52 minutes to reach the APL Mission Operations Center via NASA’s Deep Space Network station near Madrid, Spain.
The mission team typically places New Horizons in resource‑saving hibernation mode during long cruise periods. While the spacecraft is hibernating, operators do not send commands or retrieve data, but the spacecraft continues gathering and storing data around the clock from its heliospheric plasma sensors, Solar Wind at Pluto and the Pluto Energetic Particle Spectrometer Science Investigation, as well as its space dust detector, the Venetia Burney Student Dust Counter.
Alice Bowman, the New Horizons mission operations manager at APL, said the spacecraft reported back to Earth, via the Deep Space Network, with a weekly status beacon. “Every status report through this hibernation period was ‘green,’ meaning all was well aboard New Horizons each and every week,” she said.
As New Horizons resumes active operations, Bowman noted, the team will begin downlinking spacecraft health and safety data, followed by data from the three scientific instruments. In about three weeks, the spacecraft’s onboard Alice ultraviolet spectrograph will look at the hydrogen gas distribution in the outer heliosphere, while the Solar Wind at Pluto, the Pluto Energetic Particle Spectrometer Science Investigation, and the Venetia Burney Student Dust Counter instruments continue their measurements, and the ground team conducts a series of spacecraft and instrument checkouts.
The team also is completing upgrades to the ground‑system software that will make it easier to maintain operations of the spacecraft. Tests are already underway and are expected to continue through the year.
New Horizons is operating on updated autonomy logic designed for operations farther from the Sun and to accommodate the expected reduction in power and the naturally occurring increase in radio‑signal travel time.
The NASA spacecraft’s exploration of this distant region of the solar system marks the latest step in a journey that began in January 2006 with the fastest launch on record; a flyby of Jupiter in February 2007 that included stunning views of the gas giant and its moons; the first exploration through the Pluto system in July 2015; the first exploration of a Kuiper Belt object, Arrokoth, in January 2019, and unique studies of the Sun’s outer heliosphere and dozens of additional Kuiper Belt objects since then.
For more information on NASA’s New Horizons mission, visit:
https://science.nasa.gov/mission/new-horizons/
The NTSC television standard is a masterpiece of mid-century engineering, to pack a color image into the transmission bandwidth of a monochrome one, and to do so while maintaining backward compatibility with earlier monochrome TV sets. In terms of its timings and choice of sync and carrier frequencies it’s elegantly thought out for maximum quality on a 1950s round-CRT color TV set.
The trouble is, that while the standards are exacting, the receivers are quite forgiving, and will display adequately even with substantially off-spec video. [Nicole Express] is here with an in-depth examination of a time when that was pushed just a little bit too far, explaining why the Nintendo Entertainment System (NES) displayed wobbly color images.
We’re treated to a run-through of the NTSC standard itself, and a look at how some of the other consoles and home computers of that era either had similar problems, or managed to avoid them. The key lies in the exacting timing required to achieve perfect interlacing, and the NES’s use of a single crystal to provide all the clocks. The dot clock on adjacent frames was almost right, but not quite, leading to a side-to-side wobble that while barely perceptible, was exacerbated by some graphics. It’s a fascinating read.
We’ve looked at composite video in detail in the past.
NES image: JCD1981NL, CC BY 3.0.
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