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NASA and SpaceX are targeting a mid-May launch to deliver scientific investigations, supplies, and equipment to the International Space Station. 

Loaded with about 6,500 pounds of supplies, the SpaceX Dragon spacecraft will lift off aboard the company’s Falcon 9 rocket from Launch Complex 40 at Cape Canaveral Space Force Station in Florida. Following its arrival to the orbital complex, Dragon will dock autonomously to the forward port of the space station’s Harmony module. 

Watch agency launch and arrival coverage on NASA+, Amazon Prime, and NASA’s YouTube channel. Learn how to watch NASA content through a variety of online platforms, including social media. 

For more than 25 years, the International Space Station has provided research capabilities used by scientists from more than 110 countries to conduct more than 4,000 experiments in microgravity. Research conducted aboard the station helps advance long-duration missions to the Moon as part of the Artemis program and to Mars, while providing multiple benefits to humanity. 

Science highlights: 

In addition to cargo for the crew aboard the space station, Dragon will deliver several new science experiments, including: 

ODYSSEY will evaluate how well Earth-based microgravity simulators recreate space conditions. Researchers will examine bacterial behavior in space and compares the results to experiments conducted in microgravity simulators on Earth. 

STORIE will monitor charged particles in orbit around the Earth, which respond to space weather and can affect assets like power grids and satellites. The instrument could help researchers gain knowledge to better predict and respond to these changes. 

Laplace will study the movement and collision of dust particles in microgravity to understand particle motion in space. Researchers hope to learn more about Earth’s origins and provide fundamental understanding of how planets in our solar system and beyond came into existence. 

Green Bone will observe how bone cells grow and develop in space on a bone scaffold made from wood. Microgravity results could help researchers improve products that treat fragile bone conditions such as osteoporosis. 

SPARK will evaluate how red blood cells and the spleen change in space for future astronauts. Researchers will observe human samples and imagery taken before, during, and after spaceflight to identify ways to protect astronaut health during long-duration space missions.  

Arrival and return: 

NASA astronaut Jack Hathaway and ESA (European Space Agency) astronaut Sophie Adenot will monitor the spacecraft’s arrival. Dragon will remain docked to the orbiting laboratory for about a month before splashing down in the Pacific Ocean, returning critical science and hardware to teams on Earth. 

Cargo highlights: 

Launch  

European Enhanced Exploration Exercise Device Power Cable – A replacement power cable is launching for installation on the European Enhanced Exploration Exercise Device.  

Catalytic Reactor – A vital component of the Water Recovery and Management System, the catalytic reactor oxidizes volatile organics from wastewater that are removed by the Gas Separator and Ion Exchange Bed orbital replacement units. This part is launching to maintain on orbit sparing.  

Universal Pretreat Concentrate Tank – This is a passive tank to provide alternate pretreat concentrate to the Universal Waste Management System (UWMS) and Waste Hygiene Compartment (WHC). Two units are launching to maintain this hardware, in tandem with Russian pretreat tanks currently used. A universal pretreat concentrate tank adapter will accompany the tanks to connect with the Russian hose.  

Additional equipment launching includes an Ultraprobe to replace a worn ultrasonic inspection tool, a Remote Sensor Unit to restore spares for the station’s vibration monitoring system, and flexible repair patches for sealing the pressure hull if needed. The mission also will deliver an updated ARMADILLO (AOGA ReMediation, Advanced DeIonization and Limited Life Optimization) cartridge and hose assemblies to improve water processing for oxygen generation, along with a nitrogen recharge tank assembly to help maintain the station’s gas reserves. 

Return  

When Dragon returns in mid‑June, it will bring back an ocular imaging device used to monitor crew eye health, a sorbent bed that filters trace contaminants from cabin air, and a separator pump from the Waste and Hygiene Compartment. The Advanced Plant Habitat, which supported long-duration plant biology studies, also will return for eventual museum display. A pressure management device that recovers vestibule air during depressurization will come back for repair and storage as a ground spare.  

Description

This colorized image of Mars was captured by NASA’s Psyche mission on May 3, 2026, about 3 million miles (4.8 million kilometers) from the planet. The spacecraft is approaching the planet for a gravity assist on May 15 that will give it a boost in speed and adjust its trajectory toward asteroid Psyche for eventual arrival in 2029.

The spacecraft is approaching Mars from a high-phase angle, meaning that the planet appears only as a thin crescent, like our own crescent Moon seen around its new Moon phase. From this viewing geometry, the Sun is out of frame and “above” both Mars and Psyche.

Figure A is a zoomed-out view from the imager. No stars are visible in the background since they are much dimmer than the sunlight being reflected by Mars.

The observation was acquired by the multispectral imager instrument’s panchromatic or broadband filter, with an exposure time of just 2 milliseconds. Even with this very short exposure time, the crescent is extremely bright and parts of the image are oversaturated. The light seen here is sunlight reflected off the surface of Mars and also scattered by dust particles in its atmosphere. Because the quantity of dust in the atmosphere can vary rapidly over time, the anticipated brightness of the crescent was hard to predict before this early image was acquired.

The dustiness of Mars leads to sunlight being scattered by its atmosphere, making the crescent appear to extend farther around the planet than if it had no atmosphere (as with our Moon).Of note, on the right side of the extended crescent, there appears to be a gap, which coincides with the planet’s icy north polar cap. The cap is currently in winter and mission specialists hypothesize that seasonal clouds and hazes may be forming in that region, possibly blocking the atmospheric dust’s ability to scatter sunlight  like it does elsewhere around the planet.

The Psyche mission’s imager team will be acquiring, processing, and interpreting similar images in the lead-up to the close approach on May 15. The images are primarily designed to calibrate the cameras and to characterize their performance in flight as a practice run for the approach to asteroid Psyche in 2029.

For more information about the Psyche mission, read: https://science.nasa.gov/mission/psyche/

Listen to this audio excerpt from Anton Kiriwas, senior technical integration manager for NASA’s Exploration Ground Systems Program:

When Anton Kiriwas first spotted an image of the Moon and Mars hanging over a job fair booth while in college, it captured his imagination, yet felt like a dream too distant to chase. He had no way of knowing that years later he would play a critical role in NASA’s Artemis missions, helping launch humans back to the Moon for the first time in more than half a century.

Kiriwas’ journey to NASA began during the Space Shuttle Program, while he was working for United Launch Alliance, the same organization behind the memorable Moon and Mars booth that he passed by in college. Not long after, he joined NASA as a civil servant, designing electrical systems that set him on a path toward his current role with Exploration Ground Systems as senior technical integration manager. In simpler terms, Kiriwas is a problem solver.

A core part of Kiriwas’s role is to serve as a launch project engineer. Strategically positioned at the integration console in the center of Firing Room 1 of the Launch Control Center at the agency’s Kennedy Space Center in Florida, he acts as a bridge for the test management and engineering teams. Kiriwas, along with the other launch project engineers, reports directly to the launch director, making the final technical recommendation on any issues that may arise during launch countdown. From this seat, he works across all engineering disciplines, united under one mission: launch the spacecraft and crew safely.

Despite the intensity of launch day, Kiriwas describes it can often feel easier than the hundreds of rehearsals and simulations leading up to it. The team trains rigorously, preparing for every scenario imaginable. The ideal day is smooth and uneventful, but when it’s not, he and the team are ready.

When an issue arises, Kiriwas and his team begin asking the basic questions: ‘What are the requirements? Which systems are affected? Who needs to be involved?’ He pulls the technical community together to work through the situation, come up with any troubleshooting, and ultimately give the recommendation for a “go” or “no-go” for launch. It takes clarity, experience, and discipline, especially in moments when excitement is running high.

“There is adrenaline to get to launch, but you want to be careful to never let that turn into ‘launch fever,’” said Kiriwas. “We need to launch exactly when we’re ready and not a moment before.”

With Artemis II complete, Kiriwas continues applying his problem‑solving expertise, analyzing lessons learned, and shaping future mission requirements. Artemis III hardware is currently being processed at NASA Kennedy, and the teams are carefully preparing the next steps of NASA’s return to the lunar surface.

“There’s a million little pieces that go into this, and I get to be a part of it,” said Kiriwas.

For decades, NASA has advanced on-board spacecraft computer processors that coordinate and execute the functions needed to support mission success.

Space computing originated in the 1960s with the Apollo Guidance Computers, which were pivotal for guidance, navigation, and control computations during NASA’s first Moon missions. For decades, radiation-hardened processors have been the backbone of the agency’s space exploration missions.

NASA has landed computers on other planets and operated them for years in extreme conditions, as demonstrated by the Mars rovers. These computer processors have also powered several NASA orbiters, capsules, and space telescopes.

While legacy processors have enabled some of NASA’s greatest achievements, the next generation of space missions will increase in complexity and length, which will benefit from greater computing power, autonomy, and resilience. To meet the needs of this challenge, NASA and industry leader Microchip Technology Inc. entered a public, private partnership combining agency and commercial investments to develop a new solution: High-Performance Spaceflight Computing.

Advanced Computing

The High-Performance Spaceflight Computing project is a next-generation system-on-chip that delivers over 100 times the computing capability of current space processors. By integrating computing and networking into a single device, this technology significantly reduces system cost and power consumption. Its scalable architecture allows unused functions to power down, optimizing energy efficiency for critical operations.

The High-Performance Spaceflight Computing family of processors includes multiple distinct but compatible technologies for scalable mission needs. The radiation-hardened version of the processor is built for geosynchronous, deep-space, and long-duration missions to the Moon, Mars, and beyond, capable of operating in harsh environments while supporting real-time autonomous tasks. Tailored for the commercial space sector, the radiation-tolerant version of the processor provides fault tolerance and cybersecurity for low Earth orbit satellites.

Using advanced Ethernet to connect multiple sensors or cluster several chips, High-Performance Spaceflight Computing technology allows spacecraft to process massive amounts of data onboard and autonomously make real-time decisions, such as driving rovers at high speeds or filtering scientific images. Continuous system health monitoring and an integrated security controller ensure these complex operations remain safe and reliable.

Computing power for Golden Age of Exploration

The High-Performance Spaceflight Computing technology is a nationwide, public-private development effort anchored by NASA, Microchip, and a broad ecosystem of academic and industry partners. This collaboration reinforces U.S. leadership in spaceflight computing, strengthens supply chain resilience and security, stimulates regional economies, and drives innovation and high-tech workforce development across the nation.

This new technology has the potential for use on all future space missions, but unlike traditional space-specific chips, High-Performance Spaceflight Computing has a design platform for other Earth-based uses.

Adopting the same high-performance computing, network switching, high-reliability and cybersecurity technologies, the company’s processors enable mission-critical edge computing for Earth-based industries such as automotive, aviation, consumer electronics, industrial systems, and aerospace. These potential applications include drones, energy grids, medical equipment, communication services, artificial intelligence, and data transmission.

By leveraging a common technology base across space and terrestrial markets, High-Performance Spaceflight Computing helps strengthen domestic industrial capabilities and reduce risk and cost for both government and commercial users.

The Space Technology Mission Directorate’s Game Changing Development program based at NASA’s Langley Research Center in Hampton, Virginia, and NASA’s Jet Propulsion Laboratory led the end-to-end maturation of NASA’s High-Performance Spaceflight Computing by developing mission requirements, funding competitive industry studies, selecting and contracting with Microchip, and guiding the project through design reviews and the project life cycle to delivery.

To learn more about these chips, visit:  

https://go.nasa.gov/4cIGUKu

By: Jessica Jelke

NASA astronaut Chris Williams captured the Milky Way rising above Earth’s atmospheric glow on April 13, 2026, while aboard a SpaceX Dragon docked to the International Space Station.

This atmospheric glow is also called airglow. It occurs when atoms and molecules in the upper atmosphere, excited by sunlight, emit light to shed their excess energy. Alternatively, it can happen when atoms and molecules that have been ionized by sunlight collide with and capture a free electron. In both cases, they eject a particle of light — called a photon — in order to relax again. The phenomenon is similar to auroras, but where auroras are driven by high-energy particles originating from the solar wind, airglow is energized by ordinary, day-to-day solar radiation.

Image credit: NASA/Chris Williams

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