Thursday, 12 March 2026

Efficient Large Displacement/Large Rotation Dynamic Simulations Using Nonlinear Dynamic Substructures

Download PDF: Efficient Large Displacement/Large Rotation Dynamic Simulations Using Nonlinear Dynamic Substructures

Utilizing reduced-order dynamic math models (DMM) in linear system-level dynamic analyses is a well-known practice that enables extreme computational efficiencies. But what about nonlinear system dynamics? Reduced-order DMMs have found their way into contact dynamics. The engineer must look no further than the Henkel-Mar pad separation analysis methodology to verify this fact. More sophisticated applications of DMMs in contact dynamics are possible when certain repetitive geometry pattens are present. For example, Figure 1 shows a type of pipe known as a “flexible” pipe used by the subsea industry. This design features four layers of helically wound steel wires that provide the pipe with its stick/slip behavior during bending, thereby enabling a longer fatigue life in harsh ocean environments. With these helically wound armor layers presenting a repetitive contact topology, contact surfaces can be constructed and tracked enabling the friction logic to operate resulting in the friction hysteretic moment-curvature plot provided in Figure 1 (top). 

Flexible pipe used in subsea industry; moment-curvature of the flexible pipe using reduced-order dynamic math models for surface contact
Flexible pipe used in subsea industry; moment-curvature of the flexible pipe using reduced-order dynamic math models for surface contact 

As seen from Figure 1, the pipe was subjected to many bending cycles and executed in essentially a real-time computation. A single bending cycle of the same pipe in full finite element model (FEM) resolution (i.e., no use of DMMs) would require 48 hours of computation on 36 central processing units (CPUs) running in parallel given the very large order of the FEM.   

What about utilizing DMMs for computationally efficient nonlinear dynamics involving large displacements and rotations? Before addressing this question, the residual flexibility mixed boundary transformation (RFMB1) must be defined. The RFMB coordinate transformation is given as follows: 

The RFMB transformation connects physical and modal degrees of freedom (DoFs) to a reduced set of generalized coordinates

The transformation is a mix of the following submatrices: constraint modes (ψ) due to unit displacements on the b-set boundary degrees of freedom (DoFs) that remain fixed during the eigenvalue problem, residual flexibility (g) due to unit forces at the c-set boundary DoFs that remain free during the eigenvalue problem, and a truncated set of normal modes (φ) computed with the b-set DoFs constrained. It can be shown that the transformation retains full flexibility at the DMM physical DoFs and retains the full dynamics of the FEM up to the user-selected truncation frequency for the normal modes. The reduction of DoFs, and hence the computational efficiency, arises from the number of kept modes (k) being significantly less than the number of interior FEM DoFs. 

Cantilever beam model composed of 20 DMMs
Cantilever beam model composed of 20 DMMs
Cantilever beam rolled up using the 20 NDS DMMs
Cantilever beam rolled up using the 20 NDS DMMs
Same beam bent into “catenary-like” configuration by turning on gravity
Same beam bent into “catenary-like” configuration by turning on gravity

To enable DMM large displacements/rotations, four coordinates are added to the above RFMB to track large rotations. These quaternions replace the rigid-body modes that are only valid for infinitesimal rotations. With this process, the RFMB is transformed into a nonlinear dynamic substructure (NDS). Solution algorithms need to be modified accordingly as well to allow for equilibrium iterations since the problem now is highly nonlinear. As an example, consider the undeformed cantilever beam model (Figure 2) composed of 20 DMMs (single DMM of a beam composed of 5 CBAR elements repeated 20x).   

A moment is applied at the free end (right end) of Figure 2. While small displacement theory is limited and breaks down after a few degrees of rotation, the cantilever beam can be completely rolled up using NDS (see Figure 3) in a highly nonlinear dynamic simulation. Also note that the entire nonlinear dynamic simulation was executed in seconds on a laptop and included all dynamic effects. Similarly, the beam can be bent into a “catenary-like2” shape by turning on gravity and enforcing displacements at each end to the required coupling location (see Figure 4). 

One application for this large displacement/rotation NDS capability has been to include umbilical models in the coupled loads analysis (CLA) framework. Figure 5 shows the Interim Cryogenic Propulsion Stage (ICPS) umbilical that was integrated into the Space Launch System (SLS) CLA. The SLS CLA is an integrated assembly of various component DMMs (boosters, core stage, mobile launcher (ML), upper stage, etc.) to which the ICPS umbilical (ICPSU) and its hoses as NDS DMMs can now be added. For each hose, one end connects to the SLS vehicle and the other end to the ML structure. As an example, Figure 6 shows the evolution of the deformations of the forward vent hose (modeled with 20 NDS DMMs) as it goes from the undeformed geometry (straight line) into its prelaunch geometry during the initial condition setup in the CLA. 

As the timed command for umbilical separation is given, the vehicle-side ground plate separates (using the Henkel-Mar contact/separation algorithm) and the ML gantry rotates the separating umbilical away from the already lifting vehicle (the gantry was brought into the CLA as a NDS capable of large rotations). Figure 7 captures the post-separation forward vent hose dynamics (extracted from the CLA). From this, 100  ICPSU hose clearances to the lifting vehicle can be computed. 

The power of the reduced-order models does not end with linear dynamics. It is possible to introduce large displacements and rotations into reduced-order models to enable seamless integration into large substructured integrated system dynamic analyses such as a CLA. For the specific case of the SLS, this capability allowed us to integrate umbilicals into the CLA to more accurately capture the impact of system flexibilities, dynamic response to forcing functions, pad separation “twang” effects, ML dynamics, and gantry/umbilical timings on clearances.  

For information, contact Dr. Dexter Johnson.  dexter.johnson@nasa.gov 

ICPSU model integratedinto the SLS CLA
ICPSU model integratedinto the SLS CLA
ICPSU forward vent hose evolution of deformations from undeformed (straight line) to prelaunch configuration (locking in preloads) during the CLA initial conditions setup (extracted from the CLA)
ICPSU forward vent hose evolution of deformations from undeformed (straight line) to prelaunch configuration (locking in preloads) during the CLA initial conditions setup (extracted from the CLA)
Forward vent hose post-separation dynamics (extracted from the CLA)
Forward vent hose post-separation dynamics (extracted from the CLA)


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Dust Outbreak Reaches Europe

March 1–9, 2026

Winter winds lofted clouds of dust from the Sahara Desert, carrying it north toward the Mediterranean and dispersing it widely across Europe in March 2026. When the dust combined with moisture-laden weather systems, a dirty rain fell in parts of Spain, France, and the United Kingdom.

This animation highlights the concentration and movement of dust throughout the region from March 1 to March 9. It depicts dust column mass density—a measure of the amount of dust contained in a column of air—produced with a version of the GEOS (Goddard Earth Observing System) model. The model integrates satellite data with mathematical equations that represent physical processes in the atmosphere.

The animation shows dust plumes originating in northwestern Africa being blown both to the west across the Atlantic Ocean and north toward the Mediterranean. As plumes spread throughout Western Europe over several days, people observed hazy skies from southern England, where sunrises and sunsets took on an eerie glow, to the Alps in Switzerland and Italy, where a dust layer encroached on the Matterhorn.

Not all of the dust remained aloft. Storms encountered some of the dust, causing particles to fall to the ground with rain and coat surfaces with a brownish residue. A low-pressure system, named Storm Regina by Portugal’s weather service, moved across the Iberian Peninsula and brought so-called blood rain to southern and eastern Spain, along with parts of France and the southern UK in early March, according to news reports.

Over the Mediterranean, areas of “dusty cirrus” clouds developed higher in the atmosphere, where dust particles can act as condensation nuclei for ice crystals, according to MeteoSwiss, Switzerland’s Federal Office for Meteorology and Climatology. Scientists are studying these clouds to better understand their formation and how they affect weather, climate, and even solar power generation.

In a new analysis, researchers used NASA’s MERRA-2 (Modern-Era Retrospective Analysis for Research and Applications, Version 2), observations from MODIS (Moderate Resolution Imaging Spectroradiometer), and other satellite products to parse the effect of airborne Saharan dust on solar power in Hungary. They found that photovoltaic performance dropped to 46 percent on high-dust days, compared with 75 percent or more on low-dust days. They determined the greatest losses occurred because dust enhanced the presence and reflectance of cirrus clouds and reduced the amount of radiation that reached solar panels.

Some research suggests more frequent and intense wintertime dust events have affected Europe in recent years. Researchers have proposed several factors contributing to these outbreaks, including drier-than-normal conditions in northwestern Africa and weather patterns more often driving winds north from the Sahara.

NASA Earth Observatory animation by Lauren Dauphin, using GEOS-FP data from the Global Modeling and Assimilation Office at NASA GSFC. Story by Lindsey Doermann.

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2026 William T. Pecora Award Nominations Now Being Accepted

Posed portrait of William T. Pecora writing at a desk while smiling
William T. Pecora was Director of the USGS from 1965 to 1971 and Under Secretary of the Interior from 1971 to 1972.

By USGS Landsat Missions 

The William T. Pecora Award is presented annually to individuals or teams using satellite or aerial remote sensing that make outstanding contributions toward understanding the Earth (land, oceans, and air), educating the next generation of scientists, informing decision-makers, or supporting natural or human-induced disaster response. Both national and international nominations are welcome.

The award is sponsored jointly by the U.S. Department of the Interior and the National Aeronautics and Space Administration and was established in 1974 to honor the memory of Dr. William T. Pecora, former Director of the U.S. Geological Survey and Under Secretary, Department of the Interior.  

Dr. Pecora was a motivating force behind the establishment of a program for civil remote sensing of the Earth from space.  His early vision and support helped establish what we know today as the Landsat satellite program. 

Nominations for the 2026 award will be accepted until May 29, 2026.

Visit the William T. Pecora Awards webpage for eligibility requirements and the nomination process.  

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About University Innovation Project (UI)

Books with eye glasses on top.

NASA’s University Innovation (UI) project funds university-led innovation to address the agency’s Aeronautics Research Mission Directorate’s system-level challenges via independent, NASA-alternate-path, multi-disciplinary awards.

Strategic Goals

The UI portfolio’s strategic goals in descending order of importance are:

1.    Assist in achieving aviation outcomes defined in the ARMD Strategic Implementation Plan through NASA-complementary research.
2.    Transition research results to an appropriate range of stakeholders that leads to a continuation of the research.
3.    Provide broad opportunities for students at different levels, including graduate and undergraduate, to participate in aeronautics research.

Portfolio Elements

The UI project’s strategic goals are achieved through two opportunities that are available through NASA Research Announcement awards.

University Leadership Initiative (ULI)
ULI provides the opportunity for university teams to exercise technical and organizational leadership in proposing unique technical challenges, defining interdisciplinary solutions, establishing peer review mechanisms, and applying innovative teaming strategies to strengthen the research impact. By addressing the most complex challenges associated with ARMD’s strategic thrusts, universities will accelerate progress toward achievement of high impact outcomes while leveraging their capability to bring together the best and brightest minds across many disciplines. To transition their research, principal investigators are expected to actively explore transition opportunities and pursue follow-on funding from stakeholders and industrial partners during the course of the award.

University Students Research Challenge (USRC)
USRC seeks to develop novel concepts with the potential to create new capabilities in aeronautics by stimulating aeronautics research in the U.S. student community. USRC provides students, from accredited U.S. colleges or universities, with grants for aeronautics projects that also raise cost sharing funds using crowdfunding platforms. By including the process of creating and preparing a crowdfunding campaign, USRC can act as a teaching accelerator to help students develop entrepreneurial skills.

Gateways To Blue Skies
Gateways to Blue Skies expands engagement between universities and NASA’s University Innovation Project, industry, and government partners by providing an opportunity for multi-disciplinary teams of students from all academic levels (i.e., freshman, sophomore, junior, senior, and graduate) to tackle significant challenges and opportunities for the aviation industry through a new project theme each year. The competition is guided by a push toward new technologies as well as environmentally and socially conscious aviation.

UI Project Page, University Innovation (UI) Tech Talks

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Last Updated
Mar 11, 2026
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Wednesday, 11 March 2026

Computational Modeling of Failure at the Fabric Weave Level in Reentry Parachute Energy Modulators  

Download PDF: Computational Modeling of Failure at the Fabric Weave Level in Reentry Parachute Energy Modulators

Energy modulators (EM) are textile mechanical devices designed to dissipate snatch loads that occur when parachutes are deployed. Although critical for mitigating shock loads, recent flight testing has shown increasing variability in EM behavior, raising concerns about their performance predictability and potential failure under dynamic loading conditions. In response, a novel approach was implemented to create a computational model of an EM at the fabric weave level using the simulation software, LS-DYNA. This work was organized into two primary objectives: (1) development of a per-unit stitch model capturing the geometry and material behavior of the EM stitching pattern, and (2) implementation of a Python script to duplicate the unit model along the full length of an EM ear, simplifying the process of generating complex, patterned geometries in LS-DYNA. 

Depiction of EM extension during stroking from a tensile force applied at the blue arrows with (a) an unextended EM, (b) a partially extended EM, and (c) a fully extended EM
Depiction of EM extension during stroking from a tensile force applied at the blue arrows with (a) an unextended EM, (b) a partially extended EM, and (c) a fully extended EM.

EMs typically consist of a long strip of structural Kevlar webbing that is folded and stitched together with a nylon zigzag stitching pattern to form an EM “ear.” As an EM is pulled above a threshold load during deployment, the nylon stitching rips, unfolding the EM and dissipating shock forces. This process is illustrated in Figure 1, exemplifying stages of EM extension during stroking. In nominal cases, the EM cleanly tears with little damage to the Kevlar webbing. However, anomalous cases have been observed where the nylon stitches along the ear are skipped during loading, i.e., when a row of stitches do not tear in sequence. This results in failure of the surrounding Kevlar webbing, referred to as EM shredding. The inherent unpredictability of the fabric behavior and the high variability of flight loading conditions make a root cause challenging to identify through mechanical testing. 

In this study, development of a computational model of an EM in LS-DYNA was used to gain deeper insight into the cause of EM shredding. While similar studies of fabric webbing have modeled fabrics at a global level, this approach represents each thread of the Kevlar weave and nylon stitching as individually modeled 3D solid elements. Modeling each thread individually within the weave is essential not only for analyzing the failure mechanisms of the nylon stitching as it rips, but also for understanding the Kevlar weave failure during the EM shredding events. 

The first phase of this work focused on modeling individual Kevlar and nylon threads within a representative stitch geometry. A 3D model of the Kevlar weave was first generated using TexGen, an open-source software developed at the University of Nottingham. Using computer-aided design (CAD) software, nylon stitching passing through two layers of the Kevlar fabric weave was added. The nylon stitching pattern consisted of a bobbin thread and a needle thread that looped through the top and bottom layers, respectively, of the Kevlar weave pattern and twisted together at the end of every stitch between the two layers. The unit model was meshed in Hypermesh with 3D tetrahedral solid elements. 

Three‑panel graphic showing the workflow for modeling a woven composite: a 3D woven fabric CAD model in SOLIDWORKS, a meshed version of the weave in HyperMesh, and a color‑coded finite‑element simulation model in LS‑DYNA
A three‑step digital workflow showing how a woven composite structure moves from CAD modeling in SOLIDWORKS, to meshing in HyperMesh, to a color‑coded simulation‑ready model in LS‑DYNA

In LS-DYNA, the material properties, contact, failure conditions, and boundary conditions were defined to assess the dynamic response of a stitch during tensile loading. Material behavior for both fabric types was defined using *MAT_ELASTIC (*MAT_001), and two-way, surface-to-surface contact with erosion was implemented to capture progressive failure of the Kevlar weave and nylon threads. Boundary conditions were applied to replicate in-flight tensile loading scenarios. Additionally, several case studies were conducted to reduce computation time, including manual mass scaling, characteristic length analysis, and mesh quality optimization. 

Preliminary results from the EM per-unit model validated the use of solid elements to capture EM behavior, particularly the interaction between Kevlar and nylon threads. To streamline the construction of full-length EM models, the second phase of this work focused on developing a Python script to replicate the per-unit LS-DYNA model along the length of an EM ear. This eliminated the need for large CAD assemblies by generating the full model directly from duplicating the unit model. This model is applicable to both solid and shell 2D and 3D elements. Overall, these results will not only aid in identifying the root cause of EM shredding but also support the evaluation of new EM design variations. This modeling approach has broader implications for other work involving fabrics, enabling more accurate simulations and efficient design workflows in aerospace textile applications.  

For information, contact Annika M. Vaidyanathan, Alexander Chin, John Bell, and Rumaasha Maasha. 



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Developing Robust Electronics That Can Withstand Harsh Conditions on Cold Planetary Bodies 

A NASA-sponsored team has developed electronics that can operate reliably in the harsh radiation and temperature conditions found on distant planetary bodies like Europa, an ocean world orbiting Jupiter. Not only could this new technology enable autonomous sensors and robotic exploration of distant ocean worlds, it could also support NASA’s goal to establish human outposts on the Moon and Mars by enabling electronic systems to function in those cold regions with reduced heating requirements.   

Figure Overview: Artist’s conceptions of Europa, an ocean world (left), and its liquid water ocean and ice cap where life may exist (right).
Figure Overview: Artist’s conceptions of Europa, an ocean world (left), and its liquid water ocean and ice cap where life may exist (right).
Image credit: NASA

Numerous bodies in our solar system are believed to contain water in the form of ice, vapor, or liquid on or below the surface. These ocean worlds include planetary moons like Jupiter’s Europa and Ganymede, and Satern’s Enceladus and Titan; the dwarf planet Pluto; and even comets and Uranus. The liquid water beneath ice crusts on ocean worlds can offer insights about the origins of our solar system and provide clues that could enable us to discover life elsewhere in the universe.  

Unfortunately, exploring these locations is challenging. Ocean world environments are very harsh, with high radiation levels (5 Mrad of ionizing radiation, which is 50 times more than is lethal to humans) and extremely low temperatures (-180°C). Missions to explore these destinations require electronics for sensing, control, and communications that can function under such unforgiving conditions. It would be particularly advantageous if these electronic systems could operate not only on the surfaces of these worlds, but also underwater or in bores drilled through ice caps. In addition, such systems will need to meet very low size, weight, power, and cost (SWaP-C) requirements to enable their accommodation in missions traveling to such distant locations. NASA is sponsoring a promising effort to develop the electronics infrastructure needed to explore distant ocean worlds.  

A team at Georgia Tech in Atlanta led by Professor John D. Cressler and assisted by personnel at NASA’s Jet Propulsion Laboratory in Southern California and the University of Tennessee-Knoxville is working to develop and demonstrate robust silicon-germanium (SiGe) electronics that can survive both the intense radiation and low temperatures found on ocean worlds. Previous missions to the Moon and Mars have necessarily enclosed their electronic systems in protective “warm boxes” to shield them from radiation exposure and maintain Earth-like temperatures to ensure robust operation, but this approach for ocean worlds is not viable due to the severe SWaP-C constraints imposed.  

For ocean world missions, the envisioned electronics should be commercially available; flexible, supporting various application needs like communications, instrumentation, and control; highly integrated, supporting digital, analog, and radio frequency (RF) functions in a small form factor; and low-cost. These electronic systems should also provide order-of-magnitude improved SWaP-C advantages without requiring a power-hungry, heavy, and bulky protective warm box. The Georgia Tech-led team has demonstrated that silicon-germanium (SiGe) technology can satisfy these needs, achieving robust operation down to -180ºC, with simultaneous radiation exposure as high as 5 Mrad. However, this SiGe technology requires additional development before it becomes commercially available. 

Transistors are the fundamental building blocks of electronics, enabling useful functionalities such as on/off switching and amplification. The ability of SiGe transistors to operate reliably and with higher speeds at extremely cold temperatures is a direct consequence of the internal physics of the device. SiGe transistors incorporate a nanoscale SiGe alloy, which acts to accelerate electrons moving through the transistor as it switches on and off, and this effect is amplified as the temperature drops, yielding faster operation when cold. Furthermore, since the transistor’s physical structure incorporates the SiGe alloy, the portions of the transistor that are typically made from radiation-soft oxides (materials that experience significant degradation when exposed to radiation) are dramatically minimized, improving overall radiation tolerance of the device. The result is a win-win for operating SiGe transistors at cold temperatures in a high-radiation environment, as is found on ocean worlds and in other extremely cold environments in the solar system. 

A Scanning Electron Microscope (SEM) micrograph of a SiGe transistor for use on ocean worlds (left), and an example of a SiGe integrated circuit (IC) prototype for ocean worlds (right). This SiGe IC is built from large numbers of micron-sized (10-6 m) SiGe transistors to enable electronic functionalities such as communications, sensing, and control. The entire SiGe IC is 5x5 mm2 and the X-band (8-12 GHz) SiGe RF communications link is shown in the lower right.
A Scanning Electron Microscope (SEM) micrograph of a SiGe transistor for use on ocean worlds (left), and an example of a SiGe integrated circuit (IC) prototype for ocean worlds (right). This SiGe IC is built from large numbers of micron-sized (10^-6 m) SiGe transistors to enable electronic functionalities such as communications, sensing, and control. The entire SiGe IC is 5×5 mm^2 and the X-band (8-12 GHz) SiGe RF communications link is shown in the lower right.
Image credit: John D. Cressler, Georgia Tech

Cressler’s team developed ocean-worlds-ready transistor models for electronic circuit design and used them to create and test analog and RF electronic SiGe building blocks that would not require containment in a warm-box to operate on ocean worlds, thus reducing the system’s size, weight and power requirements. They used a component library (analog, digital, and RF circuit building blocks) to create an integrated circuit (IC) prototype as proof-of-concept, validating it to a Technology Readiness Level (TRL) of 5/6 (i.e., validation and demonstration on Earth in an environment that simulates the conditions on an ocean world as closely as possible).  

A major milestone for the project was the conception, design, and demonstration of a power-efficient X-band (8-12 GHz) SiGe RF communications link that is less than 10 mm2 in size (see the above image on the lower right) and operates flawlessly, while pumping modulated RF data at -180ºC and being simultaneously exposed to 5 Mrad of radiation. Design and test of a system with these unique capabilities had never been accomplished before. This type of SiGe RF communications link could enable ocean worlds missions by serving as an electronic data interface to distributed sensor networks, a lander, an orbiter, or ice cap boring machinery and submersibles. 

Outputs of this project include design files for the SiGe component library and an associated electronic design ecosystem (transistor models, test results, documentation, best practices for design and testing, etc.). These products are available for NASA reuse and can be directly infused into future NASA missions. These new SiGe elements could support a wide variety of electronic needs for ocean world missions and other missions that need to function in cold temperatures, including communications systems, sensors, instruments, control systems, etc., each of which could operate without protection in an autonomous fashion. 

Given that ocean worlds represent the worst-case environmental conditions found in the solar system in terms of the combination of radiation and cold temperatures, SiGe components developed during this project also have direct and immediate applicability for use on the Moon, on Mars, and even in Earth orbit. For instance, to enable lunar exploration and eventual human settlement, SiGe electronics could operate autonomously on the lunar surface (which features modest radiation exposure, but very cold temperatures), boosting infrastructure and exploration capabilities. For example, SiGe radar sensors and communications links could operate unprotected on the boom of a lunar rover during nighttime traverses near the equator and with reduced heating requirements when operating in the permanently shadowed craters of the Moon, thereby enhancing mission capabilities. 

For additional details, see the entry for this project on NASA TechPort.  

Project Lead(s): John D. Cressler (Georgia Tech)  

Sponsoring Organization(s): NASA Planetary Science Division’s COLDTech program. 

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Mar 10, 2026


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Tuesday, 10 March 2026

NASA’s Van Allen Probe A to Re-Enter Atmosphere 

3 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

NASA’s Van Allen Probe A is expected to re-enter Earth’s atmosphere almost 14 years after launch. From 2012 to 2019, the spacecraft and its twin, Van Allen Probe B, flew through the Van Allen belts, rings of charged particles trapped by Earth’s magnetic field, to understand how particles were gained and lost. The belts shield Earth from cosmic radiation, solar storms, and the constantly streaming solar wind that are harmful to humans and can damage technology, so understanding them is important. 

As of March 9, 2026, the U.S. Space Force predicted that the roughly 1,323-pound spacecraft will re-enter the atmosphere at approximately 7:45 p.m. EDT on March 10, 2026, with an uncertainty of +/- 24 hours. NASA expects most of the spacecraft to burn up as it travels through the atmosphere, but some components are expected to survive re-entry. The risk of harm coming to anyone on Earth is low — approximately 1 in 4,200. NASA and Space Force will continue to monitor the re-entry and update predictions

Originally designed for a two-year mission, the Van Allen Probes A and B launched on Aug. 30, 2012, and gathered unprecedented data on Earth’s two permanent radiation belts — named for scientist James Van Allen — for almost seven years. NASA ended the mission after the two spacecraft ran out of fuel and were no longer able to orient themselves toward the Sun.  

The Van Allen Probes were the first spacecraft designed to operate and gather scientific data for many years within the belts, a region around our planet where most spacecraft and astronaut missions minimize time in order to avoid damaging radiation.  

The NASA mission, managed and operated by Johns Hopkins University Applied Physics Lab, made several major discoveries about how the radiation belts operate during its lifetime, including the first data showing the existence of a transient third radiation belt, which can form during times of intense solar activity.  

When the mission ended in 2019, analysis found that the spacecraft would re-enter Earth’s atmosphere in 2034. However, those calculations were made before the current solar cycle, which has proven far more active than expected. In 2024, scientists confirmed the Sun had reached its solar maximum, triggering intense space weather events. These conditions increased atmospheric drag on the spacecraft beyond initial estimates, resulting in an earlier-than-expected re-entry. 

Data from NASA’s Van Allen Probes mission still plays an important role in understanding space weather and its effects. By reviewing archived data from the mission, scientists study the radiation belts surrounding Earth, which are key to predicting how solar activity impacts satellites, astronauts, and even systems on Earth such as communications, navigation, and power grids. By observing these dynamic regions, the Van Allen Probes contributed to improving forecasts of space weather events and their potential consequences. 

Van Allen Probe B, the twin of the re-entering spacecraft, is not expected to re-enter before 2030. 

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Last Updated
Mar 09, 2026


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Efficient Large Displacement/Large Rotation Dynamic Simulations Using Nonlinear Dynamic Substructures

Download PDF: Efficient Large Displacement/Large Rotation Dynamic Simulations Using Nonlinear Dynamic Substructures Utilizing reduced-order...