NASA Releases Powerful LAVA Software to US Aerospace Industry

NASA Releases Powerful LAVA Software to US Aerospace Industry

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Preparations for Next Moonwalk Simulations Underway (and Underwater)

This simulation of the Artemis I launch generated by NASA’s Launch, Ascent, and Vehicle Aerodynamics (LAVA) framework shows how the Space Launch System rocket’s exhaust plumes interact with the air, water, and the launchpad. Colors on surfaces indicate pressure levels — red for high pressure and blue for low pressure. Teal contours illustrate where water is present.
NASA/Chris DeGrendele, Nguyen Ly, François Cadieux, Michael Barad, Emre Sozer, Jared Duensing, Timothy Sandstrom

For years, NASA engineers have turned to a tool called the Launch, Ascent, and Vehicle Aerodynamics (LAVA) framework to solve airflow challenges that could mean the difference between mission success or failure. When engineers need to know how a spacecraft will navigate re-entry or whether a new aircraft wing design will create enough lift, they turn to LAVA.

NASA recently released this tool to the aerospace community. 

LAVA is a computational fluid dynamics software package NASA developed to advance critical aerospace missions, harnessing the agency’s collective expertise. It helps predict how air moves around rockets, aircraft, and spacecraft with stunning accuracy.

The same computational tools simulating Mars landers, predicting launch environments, and optimizing aircraft for efficiency is now available to U.S. researchers, companies, and innovators.

“This isn’t only about releasing software; it’s about accelerating innovation,” said Jared Duensing, LAVA team lead at NASA’s Ames Research Center in California’s Silicon Valley. “When university researchers can run more complex simulations and when small companies can optimize designs with NASA-grade precision, we’re not only sharing tools, we’re unleashing potential.”

This video shows a simulation of the SLS (Space Launch System) rocket using NASA’s Launch Ascent and Vehicle Aerodynamics solver. For the Artemis II test flight, a pair of six-foot-long strakes were added to the core stage of SLS that will smooth vibrations induced by airflow during ascent. The green and yellow colors on the rocket’s surface show how the airflow scrapes against the rocket’s skin. The white and gray areas show changes in air density between the boosters and core stage, with the brightest regions marking shock waves. The strakes reduce vibrations and improve the safety of the integrated vehicle.
NASA/Gerrit-Daniel Stich, François Cadieux, Michael Barad, Jared Duensing, Timothy Sandstrom, Derek Dalle

Big questions, fast answers

NASA has been using computational tools for years to predict how air will move around new aircraft or simulate the thunderous acoustic environment of a rocket launch.

Imagine watching your favorite show on a slow flip-phone versus loading it on a lightning-fast network in crystal-clear 4K high definition. That’s the kind of transformation LAVA brings to aerospace simulations. Complex problems that once took days or weeks now run in hours.

The LAVA software also is compatible with computer hardware employing specialized microprocessors known as graphics processing units (GPUs), which can run many tasks at the same time and reduce power consumption when compared to systems using traditional, more general-purpose central processing units. For traditionally costly simulation methods needed for NASA’s most complex aerospace applications, LAVA has yielded stand-out efficiency on NASA’s flagship GPU-based supercomputer, Cabeus.

But the real breakthrough is how LAVA makes the seemingly impossible routine. Aerospace engineers rely on “scale-resolving simulations” to capture high-fidelity renderings of phenomena that can have profound effects on missions, including pressure waves, turbulent swirls, and acoustic signatures. Those were once resource- and time-consuming. Now, LAVA runs them on modest computing resources, making them readily available and easy to produce, even for novice users.

This video shows a simulation of the flow over a scaled Common Research Model wing using NASA’s Launch Ascent and Vehicle Aerodynamics solver. This video highlights the large region of separated flow on the upper surface of the wing that forms due to the leading-edge ice. Particle tracers are injected near the leading-edge ice and advected downstream. Particles are colored by streamwise velocity, where red indicates lower velocity, and the increasingly lighter blue indicates higher velocity (with white indicating very high velocity).
NASA/David Craig Penner, Jeffrey Housman, Timothy A. Sandstrom

At NASA, engineers have put those capabilities into action to help launch and land spacecraft on the Moon and Mars while driving innovation for the next-generation aircraft. When NASA needed to understand supersonic parachute deployment for Mars missions – something you can’t easily test in Earth’s atmosphere  – LAVA provided critical insights.

When engineers had to predict how ice formations would affect aircraft performance, LAVA delivered answers on conditions that are critical for flight safety.

To help astronauts launch safely on Artemis missions, LAVA simulated the launch of Artemis I, enabling engineers to understand the Space Launch System flight environment in detail. Releasing the software means that industry will be able to harness those same capabilities, potentially applying them toward everything from large supersonic airliners to smaller delivery drones and air taxis.

The Launch, Ascent, and Vehicle Aerodynamics (LAVA) team at NASA Ames  is developing the capability to simulate supersonic parachute inflation by coupling several physics modules together. It couples computational fluid dynamics for the motion of the air as well as structural dynamics and contact mechanics for the deformation of the parachute. The capability could help reduce risk for upcoming interplanetary missions with atmospheric entry like Dragonfly (Titan) and DaVinci (Venus). The video shows snapshots from the fluid-structure interaction simulation of the third Advanced Supersonic Parachute Inflation Research Experiment (ASPIRE) flight test (SR03) used to validate the approach and develop best practices.
NASA/Francois Cadieux, Michael Barad, Timothy Sandstrom

Three approaches, one framework

Most computational fluid dynamics software forces engineers to pick one approach, like being handed a hammer when you need an entire toolbox. The LAVA framework offers three options for generating meshes, or grids of connected dots used to predict the behavior of fluids (including air) in a simulation.

This allows users to switch between the meshes depending on a specific problem or use multiple mesh types to compare predictions. They also can use LAVA alongside other tools for analysis and optimization to improve designs.

Among many other NASA programs and projects, the work on LAVA was supported through NASA’s Transformational Tools and Technologies project, which works to develop new computational tools to help predict aircraft performance. The project is part of NASA’s Transformative Aeronautics Concepts Program under its Aeronautics Research Mission Directorate.

Ready to dive deeper into LAVA? Visit the NASA software catalog for access information and learn more about the tool’s computational capabilities through this seminar about LAVA.

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Tara Friesen

NASA’s Chandra Finds Young Stars Dim Quickly

NASA’s Chandra Finds Young Stars Dim Quickly

The images of Trumpler 3 and NGC 2353 are open clusters that contains hundreds of young stars that are gravitationally bound together because they formed from the same gas cloud. In this composite image of the clusters, X-rays from Chandra (purple) have been combined with an optical image from the PanSTARRS telescope in Hawaii (red, green, and blue). The stars look like fuzzy dots of different sizes dotting the darkness of space.
Scientists have found that young stellar cousins of our Sun are calming down and dimming more quickly in their X-ray output than previously thought, according to a study using NASA’s Chandra X-ray Observatory.
X-ray: NASA/CXC/Penn State Univ/K. Getman; Optical/IR: PanSTARRS; Image Processing: NASA/CXC/SAO/N. Wolk

These images, released on April 14, 2026, show two open star clusters, Trumpler 3 (left) and NGC 2353 (right). They represent a recent study from NASA’s Chandra X-ray Observatory that shows how young Sun-like stars are dimmer in X-rays than previously thought.

This latest study looked at eight clusters of stars between the ages of 45 million and 750 million years old. The researchers found that Sun-like stars in these clusters unleashed only about a quarter to a third of the X-rays they expected. This quieting of young stars is a benefit for the prospects for life on orbiting planets around these stars — not a threat.

Learn more about what this finding means.

Image credit: X-ray: NASA/CXC/Penn State Univ/K. Getman; Optical/IR: PanSTARRS; Image Processing: NASA/CXC/SAO/N. Wolk

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Monika Luabeya

Smoke Shrouds Northern Thailand

Smoke Shrouds Northern Thailand

A satellite image shows gray smoke obscuring most of the landscape around Chiang Mai except for small areas where mountain ridges are visible.
The MODIS (Moderate Resolution Imaging Spectroradiometer) on NASA’s Terra satellite captured this hazy view of the city and the surrounding region on April 22, 2026.
NASA Earth Observatory/Lauren Dauphin

Chiang Mai, Thailand’s second-largest city, lies within a network of narrow valleys in the country’s northern highlands. Though the historic city is known for panoramic views of the surrounding mountains, clear skies have become less common. In recent decades, smoke has increasingly darkened the skies during the dry season, particularly in March and April.

A NASA satellite captured this smoky view of the city and the surrounding region on April 22, 2026, when haze partially obscured valleys and ridges typically visible under clearer conditions. Most of the smoke likely comes from small agricultural and forest fires lit to burn off crop debris or maintain forest ecosystems. In 2026, satellite sensors detected small numbers of fires throughout January, but fire detections became more numerous and widespread in February, March, and April. Fire activity typically peaks in March and fades by May as seasonal rains increase. 

Research indicates that smoke from biomass burning is one of the largest contributors to poor air quality in northern Thailand during the dry season. By one estimate, about 70 percent of fine particulate matter (PM2.5) in Chiang Mai in April comes from biomass burning. Smaller contributors to the region’s hazy skies include vehicles, power plants and industry, and charcoal burning for cooking and heating. Geography also plays a key role; the surrounding mountains block air flow and encourage temperature inversions that trap both local pollution and haze from the broader region in the valleys.

On the same day the satellite image was captured, air quality sensors on the ground recorded “unhealthy” and “very unhealthy” levels of PM2.5 air pollution throughout Chiang Mai and the region, according to data from the World Air Quality Index project. Prolonged exposure to high levels of air pollution can contribute to respiratory and cardiovascular diseases and other health problems.

News reports suggest that the haze is affecting the tourism industry and has contributed to a decrease in the number of international travelers coming to Chiang Mai. After more than a month of persistent haze, the number of tourists arriving in the town of Pai, a popular destination for backpackers northwest of Chiang Mai, was down 90 percent, according to one local newspaper.

Unusually warm and dry conditions have gripped the region in recent weeks, according to meteorologists with the ASEAN Specialised Meteorological Centre (ASMC). On March 27, the group advised that there was a “high risk” of severe transboundary haze in the region and elevated its alert level to three, the highest on the scale. 

In late March, the group noted that dry conditions were forecast to persist over most parts of the Mekong sub-region, with prevailing winds expected to blow mostly from the south or southwest. “Under these conditions,” ASMC noted, “the hotspot and smoke haze situation could escalate further.”

NASA Earth Observatory image by Lauren Dauphin, using MODIS data from NASA EOSDIS LANCE and GIBS/Worldview. Story by Adam Voiland.

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DNA Research on Station Promoting Cancer Therapies, Radiation Repair

DNA Research on Station Promoting Cancer Therapies, Radiation Repair

NASA astronaut and Expedition 74 flight engineer Chris Williams configures research hardware inside a portable glovebag for a biotechnology investigation exploring how bacteria affect heart tissue in the microgravity environment. Results from the MVP (Multi-use Variable-g Platform) Cell-09 experiment could lead to advanced methods for preventing or treating heart damage in humans living on and off the Earth.
NASA astronaut Chris Williams configures research hardware inside a portable glovebag for a biotechnology investigation exploring how bacteria affect heart tissue in the microgravity environment.
NASA/Jessica Meir

More biotechnology research was underway aboard the International Space Station on Wednesday taking advantage of the microgravity environment to boost knowledge about the properties of DNA and DNA-like nanomaterials. The Expedition 74 crew also completed the installation of an advanced exercise device and tested a set of new virtual reality goggles while continuing to unpack a U.S. cargo spacecraft.

Flight engineers Chris Williams of NASA and Sophie Adenot of ESA (European Space Agency) joined each other in the Kibo laboratory module processing samples of genetic materials for the DNA Nano Therapeutics-3 experiment. The investigation is exploring DNA-inspired assembly techniques as a way to manufacture treatments, or nano-therapies such as chemotherapy and immunotherapy, to kill cancer cells and activate the immune system. The manufactured samples will be analyzed first on the orbital outpost with a spectrophotometer then returned to Earth for more analysis.

NASA flight engineer Jessica Meir began her shift swapping scientific hardware inside the Columbus laboratory module’s BioLab, an incubator supporting research into the effects of microgravity on small organisms. The science maintenance work is supporting the Lux in Space investigation that observes how DNA damaged by space radiation repairs itself. While still working inside Columbus, Meir checked and secured power connections for the new European Enhanced Exploration Exercise Device, or E4D. The E4D is being tested for its ability to support crew workouts on missions to the Moon, Mars, and beyond. Finally, Meir reviewed the Nevada Vision Screening System, a head-mounted virtual reality display that measures as astronaut’s visual function to protect eyesight in space.

NASA flight engineer Jack Hathaway worked throughout Wednesday supporting his crewmates with the scientific work then continued with cargo transfers and medical inventory management. He first activated Kibo’s Life Science Glovebox enabling Williams and Adenot to work on the DNA therapy study then photographed Meir as she swapped hardware on the BioLab. Next, Hathway unpacked more cargo from Northrop Grumman’s Cygnus XL resupply ship then refilled the Columbus lab’s Human Research Facility with medical gear including blood tube kits, needles, electrodes, and gloves.

Working together in the Roscosmos segment of the orbital outpost, flight engineers Sergei Mikaev and Andrey Fedyaev participated in a fitness evaluation. Mikaev pedaled on an exercise cycle while attached to sensors measuring his cardiac activity while Fedyaev assisted him. Next, Fedyaev tested the operation of the Zvezda service module’s treadmill then worked on the Nauka science module’s orbital plumbing system.

Later, Mikaev joined station commander Sergey Kud-Sverchkov and began configuring simulation hardware that will help the duo prepare for the automated rendezvous and docking of the Progress 95 cargo mission planned for 8 p.m. EDT on Monday, April 27. Kud-Sverchkov also worked inside the Zarya module replacing battery units inside its power supply system.

Learn more about station activities by following the space station blog, @space_station on X, as well as the ISS Facebook and ISS Instagram accounts.

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Mark A. Garcia