Three Reasons Why Silverfield Has Arkansas Razorbacks Trending Up in Spring Ball  Sports Illustrated

OU mailbag: What position group is trending up during spring practice?  On3

iOS 26.5 adds new Apple Maps feature for trending places  9to5Mac

Trending tickers: Exxon Mobil, Eli Lilly, Rio Tinto and Boohoo  Yahoo Finance UK

Monday Musings: Oilers trending up, surprising playoff pushes and more  oilersnation.com

1. iOS 26.5 beta 1: Here are all the new features  9to5Mac
2. Everything New in iOS 26.5 Beta 1  MacRumors
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4. iOS 26.5’s Messages app has RCS end-to-end encryption in beta  9to5Mac
5. Apple watchOS 26.5 beta: What's new for Apple Watch and how to update  Sportskeeda Tech

1. Apple at 50: How a garage startup became a $3.5-trillion titan  Los Angeles Times
2. Apple at 50: eight technology leaps that changed our world  The Conversation
3. Think different — for 50 years  Harvard Gazette
4. 10 unsung Apple heroes you should know  Macworld
5. 50 years of Apple pushing tech forward, for better or worse  Engadget

1. Apple Leans Into Little Finder Guy With New TikTok Videos  MacRumors
2. Apple’s “Finder guy” is so dang cute.  The Verge
3. Apple’s new Finder Guy escapades chased away my Monday blues  Macworld
4. Steve Jobs Meets Brain Rot: Inside Apple’s Bold New Social Strategy  inc.com
5. Apple Unveils Lil Finder Guy Mascot To Promote New MacBook Neo  AugustMan Singapore

1. Older Galaxy phones are now getting AirDrop support, but don't celebrate yet  Android Authority
2. Samsung Brings AirDrop Support to Quick Share with Galaxy S26 Series  samsung.com
3. More phones, including Galaxy A models, will support Quick Share to AirDrop  SamMobile
4. AirDrop sharing for older Samsung Galaxy devices could be here very soon  Android Central
5. Samsung Galaxy S26: How To Finally AirDrop Photos To An iPhone  Forbes

1. Here’s When The ‘Arc Raiders’ Flashpoint Update Goes Live With New Guns, New Arc Enemies And More  Forbes
2. FLASHPOINT UPDATE - FIND THE TRUTH  ARC Raiders
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On the afternoon of March 12, 2026, a wildland fire ignited in Morrill County, Nebraska. Within 12 hours, high winds had propelled flames approximately 70 miles (110 kilometers) east-southeast across the prairie. The Morrill fire would burn over 640,000 acres (260,000 hectares) within a week, becoming the largest wildfire in the state’s history.

This image (right) shows the extent of recently burned areas near the North Platte River in western Nebraska on March 29. By this time, authorities reported the Morrill fire was 100 percent contained. However, crews were working to contain two smaller blazes immediately to the northeast, the Ashby and Minor fires, which ignited early on March 26. For comparison, the left image was acquired on February 28, before the fires. Both are false-color to better distinguish the burned areas.

The fires occurred amid an active start for wildfires in the U.S. in 2026. The National Interagency Fire Center (NIFC) reported that 15,436 fires had burned 1,510,973 acres nationwide as of March 27. That’s far higher than the 10-year average—9,195 fires burning 664,792 acres—for the same period.

The Great Plains have been particularly prone to fire in early 2026. Exceptionally dry fuels contributed to rapid fire growth and other unusual fire behavior for the time of year, according to the NIFC. Throughout the winter, much of the region saw warmer and windier-than-average conditions, as well as less than 50 percent of average precipitation over a 90-day period, leading to low soil moisture and grass fuels that were primed to burn.

The fires in western Nebraska affected large areas of ranch and pasture lands, destroyed homes, barns, and fences, and injured or killed livestock, according to news reports. The Morrill fire also burned much of the Crescent Lake National Wildlife Refuge in the Nebraska Sandhills, an area of grasslands, wetlands, and dunes used by migratory birds. Despite the fires, reports indicate that hundreds of thousands of sandhill cranes are still making their annual migration through the Platte River valley.

NASA Earth Observatory images by Lauren Dauphin, using VIIRS data from NASA EOSDIS LANCE, GIBS/Worldview, and the Joint Polar Satellite System (JPSS). Story by Lindsey Doermann.

References & Resources

• InciWeb (2026) Morrill Fire. Accessed March 30, 2026.
• National Interagency Fire Center (2026, March 27) National Fire News. Accessed March 30, 2026.
• National Interagency Fire Center (2026, March 20) Fuels and Fire Behavior Advisory: Northern and Central Great Plains. Accessed March 30, 2026.
• Nebraska Public Media (2026, March 30) ‘It’s like a death’: Grief, hope and resilience after fire ravages Nebraska Sandhills. Accessed March 30, 2026.
• The Washington Post (2026, March 24) Wildfires rip through unusual parts of U.S., raising fears of a brutal season. Accessed March 30, 2026.

From left to right, NASA astronauts Andre Douglas, Victor Glover, and Christina Koch, CSA (Canadian Space Agency) astronauts Jenni Gibbons, NASA astronaut Reid Wiseman, and CSA astronaut Jeremy Hansen pose for a photo before the Artemis II crew proceed to a media event on March 27, 2026. Douglas and Gibbons are the backup crew members for the mission; they would join the crew if a NASA or CSA astronaut, respectively, is unable to take part in the flight.

Artemis II is NASA’s first crewed mission under the Artemis program and will launch from the agency’s Kennedy Space Center in Florida. It will send Wiseman, Glover, Koch, and Hansen on an approximately 10-day journey around the Moon. Among other objectives, the agency will test the Orion spacecraft’s life support systems for the first time with people and lay the groundwork for future crewed Artemis missions.

Image credit: NASA/Josh Valcarcel

Summer is a busy season at Schirmacher Oasis, a rocky, ice-free plateau in Queen Maud Land, East Antarctica. Located near the grounding line of Nivlisen Ice Shelf and about 100 kilometers (60 miles) from the open waters of the Lazarev Sea, the “oasis” of land amid an otherwise continuous expanse of ice is home to dozens of small ice-covered freshwater lakes and two research stations.

It’s the season when all-white snow petrels are sometimes spotted soaring over the oasis, and fuzzy south polar skua and Wilson’s storm petrel chicks grow up in sheltered crevices on its cliffs and ridges. Under constant sunlight, the plateau’s freshwater lakes come to life, supporting cyanobacterial growth and teeming with microscopic tardigrades, rotifers, and nematodes. At times, groups of Adélie penguins toddle through the oasis and attempt to breed.

The summer months are also when temperatures creep just above freezing long enough for expansive networks of seasonal melt ponds and drainage channels on and within the surrounding ice to fill with bright blue meltwater that flows north onto and across the Nivlisen Ice Shelf. The satellite image above shows seasonal melt on January 6, 2026, during the peak of the 2026 melt season.  

The Nivlisen Ice Shelf is a floating tongue that forms as glacial ice flows off Antarctica and into the waters of the Lazarev Sea. The many blue ice areas found around the oasis are snow-free areas where old, compressed glacial ice with few air bubbles has been exposed by powerful katabatic winds and sublimation. This dense ice absorbs red wavelengths of light and reflects blue wavelengths, making it appear blue. Blue ice areas are rare in Antarctica, covering about 1 percent of the continent’s surface. 

“The image captures the Nivlisen Ice Shelf during a phase of strong, system-wide hydrological connectivity,” said Geetha Priya Murugesan, a remote sensing scientist with the Jyothy Institute of Technology in Bengaluru, India. Such features aren’t always visible in optical satellite imagery, she added, noting that they are often frozen, buried under snow, or drained. “This image is notable because the ‘cerulean veins’ we see on the surface align with a deeper, persistent plumbing system that we monitor with radar.”

Murugesan and colleagues have analyzed decades of satellite data and conducted several years of field research in the area, including in 2026. Their work shows that since 2000, the surface melting caused by seasonal melt ponds and channels on the ice shelf has grown in depth, area, and volume. The depth and volume of melt features grew by a factor of 1.5, while their surface area increased by a factor of 1.2.

Murugesan thinks that the visibility of the drainage network in images like these hints at a deeper vulnerability of the ice shelf. The drainage channels trace preexisting structural weaknesses, including crevasses, that act as “hydraulic pathways” that concentrate meltwater in vulnerable zones near the grounding line, where it can weaken the ice shelf, Murugesan said.

The researchers have also linked peak melting periods like this one to atmospheric rivers and foehn winds that enhance surface melting and help route meltwater through the drainage networks. The dark color—low albedo—of the many blue ice areas surrounding the oasis contributes to drainage events by making ice surfaces less reflective, warmer, and thus more prone to summer melting, Murugesan added.                        

While Murugesan and colleagues are currently conducting a detailed analysis of the 2026 melt season to determine how it compares to past years, she said it appears to be a “strong melt event consistent with elevated melt conditions.”

NASA Earth Observatory images by Michala Garrison, using Landsat data from the U.S. Geological Survey. Story by Adam Voiland.

References & Resources

• Chen, J., et al. (2026) Interannual and Seasonal Evolution of Supraglacial Channel Networks on Nivlisen Ice Shelf, East Antarctica. Egusphere, preprint.  
• Chouksey, A., et al. (2021) Mapping and identification of ice-sheet and glacier features using optical and SAR data in parts of central Dronning Maud Land (cDML), East Antarctica. Polar Science, 30, 100740.
• EGU Blogs (2024, June 21) Blue ice in Antarctica: small extent, big science. Accessed March 26, 2026.
• Murugesan, G.P., et al. (2026) Decadal Evolution of Supraglacial Hydrology on the Nivlisen Ice Shelf: From Localized Ponding to Spatially Synchronized Hydrofracture Forcing (2015-2026). Earth ArXiv, preprint.
• Murugesan, G.P., et al. (2025) Surface Melt Assessment of Nivlisen Ice Shelf, East Antarctica via SAR Satellite Data Analysis During Austral Summer 2022-2023. In: Shukla, P.K., et al. Computer Vision and Robotics. CVR 2024. Algorithms for Intelligent Systems. (Springer, Singapore.) 
• Murugesan, G.P., et al. (2024) Monitoring of Melt Ponds and Supra-Glacial Lakes over Nivlisen Ice Shelf, East Antarctica, Using Satellite-Based Multispectral Data. Civil Engineering Innovations for Sustainable Communities with Net Zero Targets.                                                              
• Murugesan, G.P., et al. (2023) Decoding the Dynamics of Climate Change Impact: Temporal Patterns of Surface Warming and Melting on the Nivlisen Ice Shelf, Dronning Maud Land, East Antarctica. Remote Sensing, 15(24), 5676. 
• Pande, A., et al. (2020) Past records and current distribution of seabirds at Larsemann Hills and Schirmacher Oasis, east Antarctica. Polar Record, 56, e40
• Ryan, P.G. (2024) Notes on the birds of Schirmacher Oasis. Marine Ornithology, 52(2).
• Tollenaar, V., et al. (2024) Where the White Continent Is Blue: Deep Learning Locates Bare Ice in Antarctica. Geophysical Research Letters, 51(3), e2023GL106285.

Listen to this audio excerpt from Erik Richards, Near Space Network Mission Manager:

For Erik Richards, supporting NASA’s first crewed Artemis mission to the Moon and back is the culmination of a career spent helping spacecraft communicate with Earth. 

Like many kids who grew up at the height of the Space Shuttle Program, Richards dreamed of spaceflight — a dream that eventually took him from the remote McMurdo Station in Antarctica to NASA’s Goddard Space Flight Center in Greenbelt, Maryland. 

 

Most recently, his work has taken him to the agency’s White Sands Complex in New Mexico — and into a key role in America’s return to the Moon. As mission manager for NASA’s Near Space Network, Richards ensures the Artemis II crew and Orion spacecraft can communicate with Earth during liftoff and early orbit, through re-entry and splashdown. 

The Near Space Network consists of an interconnected web of relay satellites and more than 40 government and commercial ground stations stretching from Bermuda to South Africa. Together with NASA’s Deep Space Network, this global infrastructure is critical to keeping the Orion spacecraft and its four astronauts connected to mission control throughout their roughly 10-day mission. 

It’s Richards’ job to keep the many pieces of the Near Space Network operating in sync across multiple missions. He compares the system to a telephone network on Earth: invisible when everything works, critical when it doesn’t. Without communications, there’s no contact with home.  

Working with the Deep Space Network, Artemis II will rely on the Near Space Network for navigation, real-time voice communications, data transfer, and situational awareness. For Richards and the teams supporting NASA’s networks, having crew aboard makes their work more essential than ever.  

Richards’ professional journey across the Near Space Network has been key to coordinating communications across the Artemis’ three flight segments, dozens of ground stations, and hundreds of people supporting humanity’s return to the Moon. 

In the months leading up to launch, Richards has supported extensive testing, requirements development, and readiness operations to prepare the network. During the mission, he will be on console, monitoring data flow and coordinating support across NASA and its partner sites worldwide. 

The support Richards and his team provide Artemis II will carry forward to Artemis III and NASA’s goal of a sustained human presence on the lunar surface. For Richards, being part of that progression — from shuttle to the Moon and eventually Mars — connects him to his childhood love of spaceflight. 

“The most exciting part about the Artemis campaign is being part of something greater,” said Richards. “You don’t have to be an astronaut to contribute to the future of human exploration.”  

NASA has awarded Intuitive Machines of Houston, $180.4 million to deliver NASA-funded science and technology to the lunar surface as part of the agency’s CLPS (Commercial Lunar Payload Services) initiative and Artemis program. This lunar delivery, which includes seven payloads — five of them NASA’s — is expected to increase understanding of the chemical composition and structure of regolith, as well as the radiation environment in and around the South Pole region. This science will continue to build a sustainable human presence by future Artemis missions.

“NASA continues to progress lunar science and exploration by enabling commercial lunar landings,” said Joel Kearns, deputy associate administrator for exploration, Science Mission Directorate, at NASA Headquarters in Washington. “These science and technology investigations aim to support long-term sustainability and contribute to a deeper understanding of the lunar surface, test technologies, and prepare for future human missions at the South Pole.”

Intuitive Machines is responsible for delivering end-to-end payload services to the lunar surface, targeted to land at the Moon’s South Pole region in 2030. This is the fifth CLPS contract for the company, which has delivered payloads to the Moon twice with their IM-1 and IM-2 missions.

“As NASA prepares to send humans and more robotic missions to the Moon, regular CLPS deliveries will provide a better understanding of the exploration environment, accelerating progress toward establishing a long-term human presence on the Moon, setting the stage for eventual human missions to Mars,” said Adam Schlesinger, manager of the CLPS initiative at NASA’s Johnson Space Center in Houston.

The rovers and instruments, totaling 165 pounds (75 kilograms) in collective mass include:

• Stereo Cameras for Lunar Plume Surface Studies (SCALPSS) will use enhanced stereo imaging photogrammetry, active illumination, and ejecta impact detection sensors to capture the impact of the engine exhaust plume on lunar regolith as the lander descends on the Moon’s surface. This payload flew on both Intuitive Machines’ IM-1 and Firefly Aerospace’s Blue Ghost Mission 1 and captured first of its kind imagery. The high-resolution stereo images will aid in creating models to predict lunar regolith erosion and ejecta characteristics, which is important as bigger, heavier spacecraft and hardware are delivered to the Moon near each other.
  Lead organization: NASA’s Langley Research Center in Hampton, Virginia
• Near-Infrared Volatiles Spectrometer System (NIRVSS) will observe light emitted or reflected by the lunar soil to help identify its composition. NIRVSS is designed to detect minerals and various types of ices that may be present. NIRVSS will also take high resolution images of the lunar soil and composition variability, which could help inform how ices interact with the lunar soil. The instrument successfully powered on and collected data while in flight on Astrobotic’s Peregrine Mission One in 2024. NIRVSS aims to measure the surface temperature at fine scales, which may help determine where ice can exist or remain stable.
  Lead organization: NASA’s Ames Research Center in California’s Silicon Valley
• Mass Spectrometer for Observing Lunar Operations (MSolo) will characterize the makeup of volatiles (things that easily evaporate) in the environment around the lander following touchdown. The mass spectrometer demonstrated its gas analysis capabilities in lunar conditions during Intuitive Machines’ IM-2 mission in 2025. MSolo measures low molecular weight volatiles, which can be used as resources on the lunar surface.
  Lead organization: NASA’s Kennedy Space Center in Florida
• Lunar Vehicle Radiation Dosimeter system (LVRaD), a suite of four radiation detectors, is designed to quantify the radiation environment on the lunar surface and assess its potential impacts of radiation on biology and the human body in preparation for future human-related activities on the Moon. Additional sensors will investigate volatiles and geological resources that will help us plan for long-term exploration, as well as gain insights into the Moon’s formation and solar system evolution.
  Lead organization: Korea Astronomy and Space Science Institute
• Multifunctional Nanosensor Platform (MNP) is a highly compact and sensitive chemical analysis instrument designed to advance understanding of the lunar environment. It will investigate how exhaust plumes from a lander’s engines interact with the lunar regolith by measuring volatile compounds over time and at varying distances from the landing site. These measurements will provide critical data to better understand plume-surface interactions and their effects, informing the design of safer, more sustainable landing systems and surface operations, directly supporting NASA’s broader lunar exploration objectives. To enable these measurements, the MNP instrument will be integrated into the Australian Space Agency’s rover (“Roo-ver”), a foundation services technology demonstration. The rover will showcase Australia’s robotics capabilities, with the ability to traverse complex terrain and operate with limited human intervention. In doing so, Roo-ver will validate key mobility and autonomy technologies in the lunar environment while serving as the enabling platform for MNP’s scientific objectives.
  Lead organization for MNP: NASA’ Goddard Space Flight Center in Greenbelt, Maryland
  Lead organization for Roover: Australian Space Agency

• NASA’s Laser Retroreflector Array (LRA) is a small device that reflects laser beams transmitted by Moon orbiters or landing spacecraft to help them determine their orbit position or navigate to the surface. Made of eight quartz corner-cube prisms set into a dome-shaped aluminum frame, the array is passive, meaning it requires no power or maintenance. One LRA payload has already been delivered through CLPS to the surface of the Moon. These arrays will continue to be used to build a network of permanent location markers on the Moon for future exploration.
  Lead development organization: NASA’s Goddard Space Flight Center
• “Sanctuary on the Moon” is a lunar time capsule of 24 synthetic sapphire discs containing a curated archive of human civilization. The discs highlight over 100 billion micropixels of data including the history of science, technology, mathematics, architecture, culture, paleontology, art, literature, music, and the human genome. Sanctuary was developed in France.
  Lead organization: Grapevine Productions

Through NASA’s CLPS initiative, lunar landing and surface operations services are purchased from American companies. By sending science and technology to the Moon, we continue to learn how to prepare for human exploration that could eventually take us to Mars.

For more information about CLPS and Artemis:

https://www.nasa.gov/clps

-end-

Tiffany Blake
Headquarters, Washington
202-358-2546
tiffany.n.blake@nasa.gov

Kenna Pell / Ivry Artis
Johnson Space Center, Houston
281-483-5111
kenna.m.pell@nasa.gov / ivry.w.artis@nasa.gov

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