NASA’s Wideband Technology Demo Proves Space Missions are Free to Roam

NASA’s Wideband Technology Demo Proves Space Missions are Free to Roam

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NASA’s Wideband Technology Demo Proves Space Missions are Free to Roam

An artist’s concept of the Polylingual Experimental Terminal transmitting data in space.

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NASA/Morgan Johnson

Just like your cellphone stays connected by roaming between networks, NASA’s Polylingual Experimental Terminal, or PExT, technology demonstration is proving space missions can do the same by switching seamlessly between government and commercial communications networks.

NASA missions rely on critical data to navigate, monitor spacecraft health, and transmit scientific information back to Earth, and this game-changing technology could provide multiple benefits to government and commercial missions by enabling more reliable communications with fewer data interruptions.

“This mission has reshaped what’s possible for NASA and the U.S. satellite communications industry,” said Kevin Coggins, deputy associate administrator for the agency’s SCaN (Space Communications and Navigation) Program at NASA Headquarters in Washington. “PExT demonstrated that interoperability between government and commercial networks is possible near-Earth, and we’re not stopping there. The success of our commercial space partnerships is clear, and we’ll continue to carry that momentum forward as we expand these capabilities to the Moon and Mars.”

This mission has reshaped what’s possible for NASA and the U.S. satellite communications industry.

Kevin Coggins

Kevin Coggins

Deputy Associate Administrator for SCaN

Wideband technology enables data exchange across a broad range of frequencies, helping bridge government and commercial networks as NASA advances commercialization of space communications. By providing interoperability between government and commercial assets, this technology unlocks new advantages not currently available to agency missions.

As commercial providers continue to advance their technology and add new capabilities to their networks, missions equipped with wideband terminals can integrate these enhancements even after launch and during active operations. The technology also supports NASA’s network integrity by allowing missions to seamlessly switch back and forth between providers if one network faces critical disruptions that would otherwise interfere with timely communications.

An artist’s concept of the BARD mission in space.
NASA/Dave Ryan

“Today, we take seamless cellphone roaming for granted, but in the early days of mobile phones, our devices only worked on one network,” said Greg Heckler, SCaN’s capability development lead at NASA Headquarters. “Our spaceflight missions faced similar limitations—until now. These revolutionary tests prove wideband terminals can connect spacecraft to multiple networks, a huge benefit for early adopter missions transitioning to commercial services in the 2030s.”

On July 23, the communications demo launched into low Earth orbit aboard the York Space Systems’ BARD mission. Designed by Johns Hopkins Applied Physics Laboratory, the compact wideband terminal communicates over a broad range of the Ka-band frequency, which is commonly used by NASA missions and commercial providers. After completing a series of tests that proved the BARD spacecraft and the demonstration payload were functioning as expected, testing kicked off with NASA’s TDRS (Tracking and Data Relay Satellite) fleet and commercial satellite networks operated by SES Space & Defense and Viasat.

During each demonstration, the terminal completed critical space communications and navigation operations, ranging from real-time spacecraft tracking and mission commands to high-rate data delivery. By showcasing end-to-end services between the BARD spacecraft, multiple commercial satellites, and mission control on Earth, the wideband terminal showed future NASA missions could become interoperable with government and commercial infrastructure.

An artist’s concept of the Polylingual Experimental Terminal transmitting data in space.
NASA/Morgan Johnson

Due to the flexibility of wideband technology and the innovative nature of this mission, NASA recently extended the Polylingual Experiment Terminal demonstration for an additional 12 months of testing. Extended mission operations will include new direct-to-Earth tests with the Swedish Space Corporation, scheduled to begin in early 2026.

This technology demonstration will continue testing spaceflight communications capabilities through April 2027. By 2031, NASA plans to purchase satellite relay services for science missions in low Earth orbit from one or more U.S. companies.

To learn more about this wideband technology demonstration visit:

PExT – NASA

The Polylingual Experimental Terminal technology demonstration is funded and managed by NASA’s SCaN Program within the Space Operations Mission Directorate at NASA Headquarters in Washington. York Space Systems provided the host spacecraft. Johns Hopkins Applied Physics Laboratory developed the demonstration payload. Commercial satellite relay demonstrations were conducted in partnership with SES Space & Defense and Viasat.

An artist’s concept of the BARD mission in space.
NASA/Dave Ryan

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Molly Kearns

Water Droplet Science

Water Droplet Science

White streaks of motion swirl and swoop all over the image. At the middle of the image is a Teflon knitting needle.
NASA/Don Pettit

NASA astronaut Don Pettit demonstrates electrostatic forces using charged water droplets and a knitting needle made of Teflon. This series of overlapping frames from Feb. 19, 2025, displays the unique attraction-repulsion properties of Teflon and charged droplets, similar to how charged particles from the Sun behave when they come in contact with Earth’s magnetic field. Highly energetic particles from space that collide with atoms and molecules in the atmosphere create the aurora borealis.

Explore more of what Pettit has coined “science of opportunity.”

Image credit: NASA/Don Pettit

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Monika Luabeya

Space Station Research Supports New FDA-Approved Cancer Therapy

Space Station Research Supports New FDA-Approved Cancer Therapy

European Space Agency astronaut Thomas Pesquet works inside the International Space Station, . He is holding two cylindrical black experiment containers to deactivate and stow the Protein Crystal Growth-5 hardware. The background is filled withIn the background, cables, silver knobs, instruments, and research equipment are visible.
European Space Agency (ESA) astronaut Thomas Pesquet removes the Protein Crystallization Facility hardware from an incubator aboard the International Space Station for the CASIS PCG-5 investigation, which crystallized a monoclonal antibody developed by Merck Research Labs.
NASA

NASA opens the International Space Station for scientists and researchers, inviting them to use the benefits of microgravity for private industry research, technology demonstrations, and more. Today, half of the crew’s time aboard station is devoted to these aims, including medical research that addresses complex health challenges on Earth and prepares astronauts for future deep space missions.

Supported by knowledge gained from space station experiments, researchers at Merck Research Labs received approval in September from the U.S. Food and Drug Administration for a new injectable version of a medication used to treat several types of early-stage cancers called pembrolizumab, also known by its brand name KEYTRUDA. The development of the injectable formula has been supported by research efforts aboard the space station through the ISS National Laboratory, resulting in reduced treatment times while maintaining its efficacy. 

Originally, the treatment was delivered during an in-office visit via infusion therapy into the patient’s veins, a process that could take up to two hours. Initial delivery improvements reduced infusion times to less than 30 minutes every three weeks. The newly approved subcutaneous injectable form takes about one minute every three weeks, promising to reduce cost and significantly reduce treatment time for patients and healthcare providers.

Black-and-white UV images show white crystals against a black background, comparing crystal growth on Earth and in space. The ground sample on the left features large, coarse clusters with varying sizes and shapes, while the spaceflight sample on the right exhibits more uniform size distribution, characterized by fine, evenly spaced bright dots.
UV imaging of a ground control sample (left) and spaceflight sample (right) from Merck’s research shows the much more uniform size and distribution of crystals grown in microgravity. These results helped researchers to refine ground-based production of uniform crystalline suspensions required for an injectable version of KEYTRUDA.
Merck

Since 2014, Merck has flown crystal growth experiments to the space station to better understand how crystals form, including the monoclonal antibody used in this cancer treatment. Monoclonal antibodies are lab-made proteins that help the body fight diseases. This research focused on producing crystalline suspensions that dissolve easily in liquid, making it possible to deliver the medication by injection. In microgravity, the absence of gravity’s physical forces allows scientists to grow larger, more uniform, and higher-quality crystals than those grown in ground-based labs, advancing medication development and structural modeling.

Research aboard the space station has provided valuable insights into how gravity influences crystallization, helping to improve drug formulations. The work of NASA and its partners aboard the space station improves lives on Earth, grows a commercial economy in low Earth orbit, and prepares for human exploration of the Moon and Mars.

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Christian M. Getteau

Curiosity Blog, Sols 4743-4749:  Polygons in the Hollow

Curiosity Blog, Sols 4743-4749:  Polygons in the Hollow

3 min read

Curiosity Blog, Sols 4743-4749:  Polygons in the Hollow

A close-up view of tan-orange rocks on the Martian surface that are in a vaguely honeycomb array, with grooves separating the edges of polygonal chunks of surface material.
NASA’s Mars rover Curiosity acquired this close-up image of polygon-shaped features in the “Monte Grande” boxwork hollow. Similar polygonal patterns in various strata were seen previously, elsewhere in Gale Crater. Curiosity captured the image using its Mars Hand Lens Imager (MAHLI), located on the turret at the end of the rover’s robotic arm, on Dec. 11, 2025 — Sol 4745, or Martian day 4,745 of the Mars Science Laboratory mission — at 16:55:37 UTC.
NASA/JPL-Caltech/MSSS

Written by Lucy Lim, Planetary Scientist at NASA’s Goddard Space Flight Center

Earth Planning Date: Friday, Dec. 12, 2025

The weekend drive starting from the “Nevado Sajama” drill site brought Curiosity back into the “Monte Grande” boxwork hollow. We’ve been in this hollow before for the “Valle de la Luna” drill campaign, but now that the team has seen the results from both the “Valle de la Luna” and “Nevado Sajama” drilled samples, we’ve decided that there’s more work to do here. 

Overall science goals here included analysis of the other well-exposed bedrock block in Monte Grande to improve our statistics on the composition of the bedrock in the hollows, and also high-resolution imaging and compositional analysis of portions of the walls of the hollow, other than those that had been covered during the Valle de la Luna campaign. These are part of a systematic mini-campaign to map a transect over the hollow-to-ridge structure from top to bottom at this site.

The post-drive imaging revealed a surprise — Valle de la Luna’s neighboring block was covered with polygons! As it turned out, the rover’s position during our previous visit for the Valle de la Luna drill campaign happened to have stood in the way of imaging of the polygonal features on this block so this was our first good look at them. We have seen broadly similar polygonal patterns in various strata in Gale Crater before — recently in the layered sulfate units (for instance, during Sols 4532-4533 and Sols 4370-4371) but we hadn’t seen them in the bottom of a boxwork hollow. Interestingly, this block looks more rubbly in texture than many of the previously observed polygon-covered blocks.

We’re interested in the relationship of the visibly protruding fracture-filling material here to fracture-filling materials seen in previous polygons, and also in the relationship of the polygonal surface on top to the more chaotic-appearing exposures lower on the block, and to the equivalent strata in the nearby wall of the hollow. We therefore planned a super-sized MAHLI mosaic that will support three-dimensional modeling of the upper and lower exposed surfaces of the polygon-bearing block. Several APXS and ChemCam LIBS observations targeted on the polygon centers and polygon ridges were also planned, to measure composition. Meanwhile, Mastcam has been busy planning stereo images of the nearby hollow wall in addition to the various blocks on the hollow floor.

The hollow also included freshly exposed light-toned material from where the rover had driven over and scuffed some bedrock, so another APXS measurement and a ChemCam LIBS went to the scuffed patch to measure the fresh surface.

We’ll be driving on Sol 4748. As we drive we’ll be taking a MARDI “sidewalk” observation, to image the ground beneath the rover as we approach the wall for a closer view, and hopefully some contact science in next week’s plans.

A rover sits on the hilly, orange Martian surface beneath a flat grey sky, surrounded by chunks of rock.
NASA’s Mars rover Curiosity at the base of Mount Sharp
NASA/JPL-Caltech/MSSS

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Dec 18, 2025

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Hi ya! Hyha

Hi ya! Hyha

A color photograph from the Martian surface shows mostly smooth, pale orange colored terrain beneath a sky of flat, warm beige; the ground extends into the distance where an undulating line of gentle peaks forms a horizon about two-thirds of the way above the bottom of the frame. Closer to the foreground the terrain slopes from the upper left of the image toward lower right, with scattered rocks and streaks of gray along the ground.
This image from NASA’s Mars Perseverance rover shows a potential megablock on the Jezero crater rim, taken by the Mastcam-Z instrument’s “right eye.” Mastcam-Z is a pair of cameras located high on the rover’s mast. Perseverance acquired this image looking east across the rim heading towards “Lac de Charmes” on Dec. 7, 2025 — Sol 1706, or Martian day 1,706 of the Mars 2020 mission — at the local mean solar time of 13:38:46.
NASA/JPL-Caltech/ASU

Written by Margaret Deahn, Ph.D. student at Purdue University 

NASA’s Mars 2020 rover is currently trekking towards exciting new terrain. After roughly four months of climbing up and over the rim of Jezero crater, the rover is taking a charming tour of the plains just beyond the western crater rim, fittingly named “Lac de Charmes.” This area just beyond Jezero’s rim will be the prime place to search for pre-Jezero ancient bedrock and Jezero impactites — rocks produced or affected by the impact event that created Jezero crater.  

The formation of a complex crater like Jezero is, well… complex. Scientists who study impact craters like to split the formation process into three stages: contact & compression (when the impactor hits), excavation (when materials are thrown out of the crater), and modification (when gravity causes everything to collapse). This process happens incredibly fast, fracturing the impacted rock and even melting some of the target material. Sometimes on Earth, the classic “bowl” shaped crater has been completely weathered and unrecognizable, so geologists are able to identify craters by the remnants of their impactites. Just when you thought it couldn’t get any more complicated — Jezero crater’s rim is located on the rim of another, even bigger basin called Isidis. That means there is an opportunity to have impactites from both cratering events exposed in and just around the rim — some of which could be several billions of years old! We may have already encountered one of these blocks on our trek towards Lac de Charmes. In the foreground of this image taken by the Mastcam-Z instrument on the rover, there is a potential impactite called a “megablock” that the team has named “Hyha.” We can actually see this block from orbit, it is that large! The team is excited to continue exploring these ancient rocks as we take our next steps off Jezero’s rim.

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