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 

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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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Mar 09, 2026


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About Flight Demonstrations and Capabilities (FDC) Project

Image of a sleek, white airplane with a sharp, pointed nose flies above arid mountains. The plane's wheels are down. NASA is painted in blue lettering on its tail. The X-59 has a role in NASA's Flight Demonstrations and Capabilities (FDC) project.
NASA’s X-59 quiet supersonic research aircraft lifts off for its first flight Tuesday, Oct. 28, 2025, from U.S. Air Force Plant 42 in Palmdale, California. The aircraft’s first flight marks the start of flight testing for NASA’s Quesst mission, the result of years of design, integration, and ground testing and begins a new chapter in NASA’s aeronautics research legacy.
NASA/Lori Losey

The FDC project conducts complex integrated small-scale flight research to validate the benefits of new technologies.

By modifying aircraft from FDC’s support fleet, the project enables aggressive, success-oriented flight campaign schedules. While many technologies are at mid-levels of technology readiness, the FDC project supports all phases of technology maturation.  

FDC’s support aircraft fleet enables safety chase and in-flight experimental measurements for a variety of NASA missions.

The project collaborates with academia, industry, and government organizations to leverage flight opportunities, and engages with NASA researchers and university students to bring innovative concepts to flight.  

The FDC project operates, sustains, and enhances other national flight research capabilities that enable complex high-risk flight research for both NASA and the aviation industry.

These capabilities are located at NASA’s Armstrong Flight Research Center at Edwards, California, and includes the Aeronautics Test Data Portal, Flight Loads Laboratory, the Dryden Aeronautical Test Range, and a suite of flight simulators.

The project leverages collaborative opportunities for flight testing from across the aeronautical industry. 

Flight Research Facilities

The FDC project validates benefits associated with critical technologies through focused flight experiments. Through the integration of appropriate flight test capabilities and assets — whether from NASA. other government agencies, or industry — FDC campaigns focus on aggressive, success-oriented schedules using the best collection of assets.

The FDC project supports tests of technology at all phases of maturation.

Flight Loads Laboratory

Simulation Lab

Research Aircraft Integration Facility

Dryden Aeronautical Test Range

Support Aircraft and Maintenance Operations

FDC

IASP  

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Mar 09, 2026
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NASA Armstrong Director Brad Flick to Retire After 40 Years of Service

Brad Flick, NASA Armstrong Flight Research Center Director, December 2022 - Current
Portrait of Brad Flick
Credit: NASA

On Monday, NASA announced Bradley Flick, director of NASA’s Armstrong Flight Research Center in Edwards, California, will retire Thursday, March 19, after a nearly 40-year career advancing aeronautics and flight research.

Flick began his NASA journey in 1986 as a flight systems engineer and rose through the ranks to lead the center. His career spanned historic achievements by NASA, bookended by the groundbreaking X‑29 forward-swept wing aircraft and the first flight of the X‑59 quiet supersonic technology aircraft and including many other experimental flight research and airborne science projects in support of NASA and the nation.

“Brad’s career reflects the kind of disciplined engineering and steady leadership NASA relies on to tackle difficult problems,” said NASA Administrator Jared Isaacman. “For nearly four decades, he contributed to some of the agency’s most challenging flight research efforts—from the X-29 through the first flight of the X-59—and helped strengthen the team and capabilities at Armstrong along the way. NASA is grateful for his service and the example he’s set for the next generation of engineers and flight test professionals.”

After earning a bachelor’s degree in electrical and computer engineering from Clarkson University, Flick joined NASA, working on the F/A-18 High Alpha Research Vehicle project. In 1988, he moved to the Operations Engineering branch, where he played a lead role in developing experimental systems including thrust vectoring control, emergency electrical and hydraulic systems, and the spin recovery parachute system. He also served as mission controller for about 100 HARV research flights.

He later earned a master’s degree in engineering management from Rochester Institute of Technology, which supported his progression through increasingly responsible leadership roles. Before his appointment as center director on Dec. 5, 2022, following a period as acting director, Flick held leadership positions spanning engineering and operations, including Flight Systems branch chief, acting associate director for Flight Operations, center chief engineer (where he chaired the Airworthiness and Flight Safety Review Board), deputy director and director for Research and Engineering, and deputy center director.

Flick’s leadership and technical expertise shaped flight research at NASA. His work advanced aeronautics and pushed the boundaries of aviation technology. As NASA continues to lead innovations in sustainable aviation and supersonic flight, his contributions will remain an integral part of that legacy.

Troy Asher will serve as acting center director, effective Friday, March 20. Asher previously served as director, Flight Operations, at NASA Armstrong.

For more about NASA’s missions, visit:

https://www.nasa.gov

-end-

Bethany Stevens / Cheryl Warner
Headquarters, Washington
202-358-1600
bethany.c.stevens@nasa.gov / cheryl.m.warner@nasa.gov

Dede Dinius
Armstrong Flight Research Center, California
661-276-5701
darin.l.dinius@nasa.gov

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Mar 09, 2026
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Monday, 9 March 2026

Webb Studies Cranium Nebula

A shell of ghostly gas encapsulates a cloud of amber-colored gases that blow out in both directions from a central point. This makes the nebula look like a top-down view of two brain hemispheres inside a transparent skull. The scene is decorated with multicolor dots of light, representing distant galaxies and stars. The stars shown here have six points, characteristic of Webb images.
NASA, ESA, CSA, STScI; Image Processing: Joseph DePasquale (STScI)

Nebula PMR 1 is a cloud of gas and dust that bears an uncanny resemblance to a brain in a transparent skull, inspiring its nickname, the “Exposed Cranium” nebula. Webb captured its unusual features in both near- and mid-infrared light. The nebula was first revealed in infrared light by a predecessor to Webb, NASA’s now-retired Spitzer Space Telescope, more than a decade ago. Webb’s advanced instruments show detail that enhances the nebula’s brain-like appearance. This image, released on Feb. 25, 2026, is in near-infrared light.

The nebula appears to have distinct regions that capture different phases of its evolution — an outer shell of gas that was blown off first and consists mostly of hydrogen, and an inner cloud with more structure that contains a mix of different gases. Both Webb’s NIRCam (Near-Infrared Camera) and MIRI (Mid-Infrared Instrument) show a distinctive dark lane running vertically through the middle of the nebula that defines its brain-like look of left and right hemispheres. Webb’s resolution shows that this lane could be related to an outburst or outflow from the central star, which typically occurs as twin jets burst out in opposite directions. 

Read more about the Exposed Cranium nebula and see another view of it from Webb’s MIRI (Mid-Infrared Range Instrument).

Image credit: NASA, ESA, CSA, STScI; Image Processing: Joseph DePasquale (STScI)



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NASA Astronauts to Answer Questions from Students in New York

NASA astronaut Chris Williams is seated inside the Destiny laboratory module aboard the International Space Station. He is wearing a red shirt and black shorts with three white stripes underneath the right pocket. Chris is holding a device with a cord in his left hand and there are blank computer screens in front of him. He is smiling brightly and looking directly at the camera.
NASA astronaut Chris Williams calls mission controllers during Crew Medical Officer training while inside the International Space Station’s Destiny laboratory module.
NASA/Jessica Meir

Students in New York will hear from NASA astronauts Jack Hathaway and Chris Williams as they answer prerecorded science, technology, engineering, and mathematics (STEM) questions while aboard the International Space Station.

The Earth-to-space call will begin at 12:05 p.m. EDT Wednesday, March 11, and will stream live on the agency’s Learn With NASA YouTube channel.

This event is hosted by the Queens Borough Public Library in Jamaica, New York, for students in grades K-12 and members of the community. This unique opportunity aims to deepen understanding of space exploration and inspire young people to pursue a future career in STEM.

Media interested in covering the event must RSVP by 5 p.m. EDT, Tuesday, March 10, to Ewa Kern-Jedrychowska at: 917-702-0016 or Ewa.KernJedrychowska@queenslibrary.org; or to Elisabeth deBourbon at: 917-650-3815 or Elisabeth.deBourbon@queenslibrary.org.

For more than 25 years, astronauts have continuously lived and worked aboard the space station, testing technologies, performing science, and developing skills needed to explore farther from Earth. Astronauts communicate with NASA’s Mission Control Center in Houston 24 hours a day through SCaN’s (Space Communications and Navigation) Near Space Network.

Research and technology investigations taking place aboard the space station benefit people on Earth and lay the groundwork for other agency deep space missions. As part of NASA’s Artemis program, the agency will send astronauts to the Moon to prepare for future human exploration of Mars, inspiring the world through discovery in a new Golden Age of innovation and exploration.

See more information on NASA in-flight calls at:

https://www.nasa.gov/stemonstation

-end-

Gerelle Dodson
Headquarters, Washington
202-358-1600
gerelle.q.dodson@nasa.gov

Sandra Jones
Johnson Space Center, Houston
281-483-5111
sandra.p.jones@nasa.gov



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Lake Coatepeque

A blue lake rests within a caldera with steep walls. Several volcanoes near the caldera are capped by clouds. The terrain is mostly lush and green, with patches of gray urban areas.
February 10, 2026

Just inland from the Pacific coast of El Salvador, the striking blue waters of Lake Coatepeque fill part of a caldera of the same name. An astronaut aboard the International Space Station took this photo of the lake and surrounding terrain on February 10, 2026, as the station passed over Central America.

The caldera formed during a series of explosive eruptions between 72,000 and 51,000 years ago. After the caldera’s formation, additional eruptions produced several lava domes along its western side, including one that became Isla del Cerro (Isla Teopán). According to the Smithsonian Institution’s Global Volcanism Program, there have been no reported eruptions from the caldera during the Holocene (the past 11,700 years). 

Today, homes, restaurants, boathouses, and other structures line the lakeshore. This human footprint extends westward toward the caldera’s steep rim, which abuts the eastern flank of Santa Ana—El Salvador’s tallest volcano. Unlike Coatepeque, Santa Ana remains active, with small to moderate explosive eruptions recorded since the 16th century. Its most recent severe eruption occurred in 2005.

Although the lake appears its usual blue in this photo, it can occasionally take on a strikingly different hue. At times, the water temporarily shifts to bright turquoise, prompting questions about its cause. In 2024, scientists reported that while pigments from microalgae and cyanobacteria can affect the lake’s color, the turquoise episodes are likely the result of natural mineralization.

The broader landscape around the lake and Santa Ana Volcano is a mosaic of urban areas, agricultural fields, and even more volcanic terrain. The city of Santa Ana lies about 15 kilometers (9 miles) to the north, while San Salvador, also nestled amid volcanoes, lies 40 kilometers (25 miles) to the east. The volcanic landscape stretches more than 1,000 kilometers (600 miles) along Central America’s Pacific coast, from Guatemala to Panama, composing the Central American Volcanic Arc

Astronaut photograph ISS074-E-312810 was acquired on February 10, 2026, with a Nikon Z9 digital camera using a focal length of 400 millimeters. It was provided by the ISS Crew Earth Observations Facility and the Earth Science and Remote Sensing Unit at NASA Johnson Space Center. The images were taken by a member of the Expedition 74 crew. The images have been cropped and enhanced to improve contrast, and lens artifacts have been removed. The International Space Station Program supports the laboratory as part of the ISS National Lab to help astronauts take pictures of Earth that will be of the greatest value to scientists and the public, and to make those images freely available on the Internet. Additional images taken by astronauts and cosmonauts can be viewed at the NASA/JSC Gateway to Astronaut Photography of Earth. Story by Kathryn Hansen.

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A blue lake rests within a caldera with steep walls. Several volcanoes near the caldera are capped by clouds. The terrain is mostly lush and green, with patches of gray urban areas.

February 10, 2026

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From Cabbages to Countdowns: NASA Marks 100 Years of Modern Rocketry

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From Cabbages to Countdowns: NASA Marks 100 Years of Modern Rocketry

black-and-white photograph of a man in an overcoat and hat standing next to a slender, 11-foot-tall rocket supported by a metal frame
Photograph of Robert Goddard and his liquid-fueled rocket, prior to its first flight on March 16, 1926, from a farm at Auburn, Mass.
Credits: Esther Goddard, Courtesy of Clark University

Snow covered the ground that Tuesday morning 100 years ago, when a college professor and his wife took a morning drive to the family farm a few miles south in Auburn, Massachusetts. Along for the ride, the couple brought two work colleagues — and “Nell.”

They may not have known it at the time, but thanks to Nell, the four New Englanders were about to attend an auspicious birth.

Some eleven feet tall and weighing a mere 10 pounds, Nell was a contraption of the professor’s invention. He had devised, constructed, and tested Nell methodically, incrementally, over the course of many, many years.

That snowy morning at Aunt Effie’s farm, the professor’s assistant took a blowtorch to Nell.

Moments later Nell ascended. The gangly apparatus climbed 41 feet high and landed in a cabbage patch 60 yards away. The entire journey took less than three seconds, but March 16, 1926, had just become the date of the world’s first liquid-fueled rocket flight, and Dr. Robert Goddard had just become a father of modern rocketry.

“It looked almost magical as it rose, without any appreciably greater noise or flame, as if it said, ‘I’ve been here long enough; I think I’ll be going somewhere else, if you don’t mind,’” Goddard wrote in his journal the next day.

black-and-white photograph of a trio of people standing outdoors with wooden crates at their feet
Robert Goddard’s assistant Henry Sachs (left), former student and fellow Clark University Physics professor Percy Roope (middle), and wife Esther Goddard who photographed and filmed much of her husband’s work. They stand with parts from the rocket — later named “Nell” — following the flight of March 16, 1926, at Aunt Effie’s (a distant relative of Robert Goddard’s) Ward Farm in Auburn, Mass. This test marked the world’s first successful launch of a liquid-propelled rocket.
Courtesy of Clark University

The idea of a liquid-fueled rocket was not new. Others around the world had been pondering theory and sketching designs for years: Liquid propellant would offer greater thrust control than solid fuel, but the benefit accompanies tricky challenges, like how to pressurize and control the rate of fuel mixture. Goddard, who filled Nell up with a blend of gasoline and liquid oxygen, became the first in the world to build and successfully launch such a rocket.

Recognition was slow to arrive — ridicule came faster. In 1920, The New York Times opined that Goddard’s work in rocketry and his suggestion that such a device could reach the Moon was “a severe strain on credulity”: How could a rocket function in a vacuum with no air to push against, the newspaper accused. “Of course [Goddard] only seems to lack the knowledge ladled out daily in high schools.”

It is difficult to say what is impossible, for the dream of yesterday is the hope of today, and the reality of tomorrow.

DR. ROBERT H. Goddard

DR. ROBERT H. Goddard

Rocketry Pioneer

But Goddard pressed on, refining and retooling his rockets over the years. At the dawn of the Space Age and with Esther Goddard championing her late husband’s work (Robert Goddard died in 1945), the true significance of the Clark University professor’s work became clearer. NASA named its first new complex the Goddard Space Flight Center in his honor in 1959. Liquid-propelled rocketry has been the backbone of spaceflight ever since.

A century after Goddard’s first launch, NASA’s Artemis II mission is poised to bring astronauts around the Moon for the first time since 1972. The SLS (Space Launch System) rocket that will take them there is 30 times taller and half a million times heavier than Nell — but still liquid-fueled, just as Goddard predicted and pioneered, 100 years ago in a snowy field next to a cabbage patch.

By Rob Garner
NASA’s Goddard Space Flight Center, Greenbelt, Md.

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Last Updated
Mar 06, 2026
Editor
Rob Garner
Contact
Rob Garner
Location
Goddard Space Flight Center


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