Entering a planet’s atmosphere is a dangerous maneuver for any spacecraft, as it must withstand the intense frictional heat generated by high-speed contact with atoms and molecules.

That’s why landers and rovers have heat shields. And new research from the Grainger College of Engineering at the University of Illinois Urbana-Champaign suggests that an atmosphere’s composition has a big impact on how heat shields work.

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two side-by-side images showing conical bursts of nitrogen in a test chamber

High-speed image frames illustrate extreme particle burst events in supersonic nitrogen. In rare instances, particles are observed traveling upstream, indicating a pressure driven ejection mechanism. (Image credit: Francesco Panerai/University of Illinois)

“What was very surprising about the study is that, when we changed the gas, the ablation phenomenon behaved in different ways,” Panerai said in a March 12 statement. “In a classical air environment where you have oxygen present, the ablation happens in a steady way. The flow around the spacecraft erodes the surface, and particles get ejected as a constant stream.”

ready for a 2028 launch toward the huge Saturn moon Titan. Titan has a thick atmosphere that’s quite different from that of Earth: It’s composed of about 95% nitrogen and 5% methane, whereas ours is 78% nitrogen and 21% oxygen.

Dragonfly will study Titan’s surface, which could give scientists clues on whether or not the moon’s hydrocarbon lakes and rivers hold molecules that are a precursor for life.

“Although this work doesn’t directly influence heat shield design, it does have very profound implications on the physics of the material — on the way the material behaves at extreme temperatures,” Panerai says. “Understanding at what conditions this phenomenon becomes prominent in flight can help us design better heat shields.”

The study was published Feb. 5 in the science journal Carbon.