Plate Nº 13 · recorded October 10, 2026

Space & AstronomyReported finding

X-rays and AI Reveal Spacecraft Heat Shields Burning in Real Time

Researchers combined X-ray micro-CT and AI super-resolution to watch heat shield materials decompose at 1,652°F, yielding 3D time-lapse data for NASA-grade ablators.

By Priya Raman5 min read946 words

In brief

  1. Researchers imaged heat shield ablation in real time at 1,652°F (900°C), published in npj Materials Degradation in 2025.
  2. The technique, in situ X-ray micro-CT at Berkeley Lab's Advanced Light Source, produced time-lapse 3D images at the micrometer scale.
  3. SLA-561V's cork filler burns away leaving empty pockets, while SLA-220's silicone matrix forms interconnected branching channels.
  4. Nearly every major NASA ablative heat shield material, including Artemis and Mars entry materials, has been studied with this ALS technique.
  5. AI super-resolution based on generative adversarial networks turned low-resolution live scans into a high-resolution record.

For the first time, researchers have watched spacecraft heat shield materials decompose in real time at 1,652 degrees Fahrenheit (900 degrees Celsius), producing time-lapse 3D images sharp enough to guide the design of NASA's next thermal protection systems. The study, led by Collin W. Foster and colleagues, appeared in 2025 in the journal npj Materials Degradation.

Until now, engineers could only inspect heat shield materials before and after heating tests. They had to infer what happened in between and build computational models around that guesswork. The new work, carried out in part at the Advanced Light Source (ALS) at the Department of Energy's Lawrence Berkeley National Laboratory, closes that gap.

Why heat shields must burn to survive

When a spacecraft reenters Earth's atmosphere at hypersonic speeds, its shield faces temperatures beyond 3,000 degrees Fahrenheit (1,650 degrees Celsius). The shield survives through a process called ablation: specialized materials absorb heat as they degrade in a controlled way, sacrificing their outer layers to protect the vehicle and crew inside.

Designing better ablators requires understanding exactly how they degrade at the microscopic level. That has been hard to observe live, which is why the ALS result matters.

"Directly observing how heat shield materials degrade during heating with this technique has been transformative for atmospheric entry research since it gives us unique insights and helps us visualize the internal structural changes that drive ablation as it occurs," said Vishnu Oruganti, a postdoctoral fellow at the University of Illinois Urbana-Champaign at the time of the study and now a researcher at NASA's Johnson Space Center in Houston.

"Nearly every major NASA ablative heat shield material has been studied with this technique at the Advanced Light Source, including those relevant to the Artemis and Mars entry missions," Oruganti added.

How did the team watch materials burn?

A team from the University of Illinois Urbana-Champaign and NASA, in a long-term collaboration with the ALS, used in situ X-ray micro-computed tomography — micro-CT for short — a technique that builds 3D images of a material's interior without cutting it open. They examined a class of materials called superlight ablators, the same kind used on the backshells of NASA spacecraft.

The samples sat in a specially controlled environment that independently adjusts temperature, pressure and gas mixture, recreating realistic, evolving reentry conditions. The team heated samples to 1,652 degrees Fahrenheit — the upper end of the range where these materials begin to decompose — and imaged them at the micrometer scale at multiple time points.

They focused on two commercial ablators used in different parts of spacecraft backshells and with different chemical compositions:

  • SLA-561V, which contains cork — the same natural material used in wine bottle stoppers — as a structural filler
  • SLA-220, which has no organic filler and relies on a rubber-like silicone matrix

The scans tracked how reentry-like heating drives real-time, multiphase chemical decomposition and changing porosity inside both materials. These direct measurements feed predictive models, reduce uncertainty about heat shield performance, and improve mission planning and crew safety.

Where does AI come in?

The researchers faced a trade-off. Fast scans of large, representative sample areas came at low resolution; high-resolution images captured fine structural detail but only of static samples before and after heating. The team resolved this with an AI-based super-resolution method built on generative adversarial networks — machine learning systems that generate realistic images from training data.

The bright, broad-spectrum X-ray beam from the light source let the team quickly capture large-volume, lower-resolution scans at short intervals, tracking fast structural changes during heating. A single-wavelength beam then produced crisp, high-resolution snapshots of the samples before and after heating. By training the AI on those before-and-after images, the researchers enhanced the entire real-time image sequence into a complete high-resolution record of each material's transformation.

"We can perform 3D imaging of samples under different extreme conditions such as heat, cold, pressure, and tension, and we can watch the internal structure of materials evolve and give a deep look into internal structure in high detail as their properties change under these conditions," said ALS scientist Liz Clark.

What did the images show?

The AI-enhanced imaging revealed a striking difference between the two materials. When heated, the cork in SLA-561V chemically breaks down and disappears, leaving open, empty pockets distributed throughout the material. SLA-220 responds differently: its silicone matrix forms a dense, branching network of interconnected channels.

These are not just visual quirks. Open, isolated pockets behave differently from an interconnected channel network when heat and gas move through a material under reentry conditions — and those differences affect how each material performs as a heat shield.

"This is a great example of how years of working together to customize the imaging technique and integrate AI are helping us generate high-quality data and facilitate analysis, leading to more detailed scientific insights in a fraction of the time," Clark said.

What changes for future missions?

After the first Artemis mission, when heat shields did not perform as NASA's computational methods predicted, the agency used the ALS to examine shield materials and better understand how their internal structure evolves over time, Clark noted.

The new findings give engineers something they have not had before: direct microscopic measurements of heat shield materials changing under thermal conditions similar to atmospheric reentry. The results remain tied to laboratory simulations of reentry rather than flight tests, so real-world validation will continue. Still, the measurements bolster past observational studies, sharpen model development, and help missions return safely home.

via Phys.org Space & Astronomy (Source)

Filed under

  • heat-shields
  • spacecraft
  • ai
  • x-ray-imaging
  • materials-science
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Priya Raman

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Senior reporter covering industry trends and analytics at SciBeat.

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