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How NASA Reinvented The Wheel

Veritasium·
6 min read

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TL;DR

Nitinol’s shape memory and superelastic behavior allow large reversible deformation (about 6–8%) without permanent plastic damage, which is crucial for long-duration rover mobility.

Briefing

A NASA-backed breakthrough in shape-memory metal is turning “wheels” into something closer to a self-healing suspension system—built to survive the vacuum and extreme temperatures of the Moon and Mars without relying on air pressure. The key material is nitinol, a nickel-titanium alloy that can be stretched or bent far beyond what ordinary metals can handle elastically, then snap back to its programmed shape after the stress is removed. That combination—large reversible deformation plus durability—lets engineers design tires that don’t go flat, don’t require confining pressure, and can keep rovers moving even when the terrain pounds the wheel repeatedly.

The need is stark. On Earth, pneumatic tires depend on internal air pressure to maintain shape. On the Moon and Mars, there’s no external pressure to balance the tire, and temperatures swing from blistering sun exposure to deep cold in shadow. Rubber becomes brittle at those lows, and without confining pressure a conventional rubber tire can effectively fail catastrophically. That’s why many planetary wheels have leaned toward hard metal designs—like aluminum mesh wheels for the Curiosity rover—despite the tradeoffs. Those wheels are lightweight and avoid welds or fasteners that could fail, but their thin skins can crack under higher-than-predicted peak loads, leaving holes and reducing efficiency even if the rover can still complete its mission.

NASA’s earlier attempts show the engineering problem in mechanical terms: materials can only tolerate limited elastic strain before they undergo plastic deformation—permanent change caused by defects moving through the crystal structure. Ordinary metals typically handle only about 0.3–0.8% elastic strain before yielding, a constraint that shapes how spacecraft components are designed. For the Apollo Lunar Roving Vehicle, engineers used a pantograph-like steel mesh with tread coverage and a “bump stop” concept to keep deformation below the proportional limit. It worked for short trips, but longer journeys allowed permanent deformation to accumulate.

Nitinol offered a different physics route. Discovered through experiments at the Naval Ordnance Laboratory, it undergoes a solid-state phase change between austenite (high-temperature structure) and martensite (lower-temperature structure). Stress can force austenite into detwinned martensite, allowing large deformation without breaking bonds or driving edge dislocations the way ordinary plasticity does. When the stress is released, the alloy returns toward austenite, restoring its original geometry. This is the “shape memory” effect, and it also enables “superelastic” behavior: nitinol can stretch roughly 6–8% and still spring back, even when the transformation happens without changing temperature.

Those properties translate directly into wheel design. Engineers weave nitinol springs into a mesh tire, a process described as tedious—hundreds of loops per tire—but one that produces a structure flexible enough to deform up to about 8% without permanent damage. Testing uses a rotating terrain carousel that can simulate sand, rocks, and slip conditions at rover-like speeds, while demonstrations on Earth include puncture and bullet resistance to show how the structure maintains performance when damaged. The payoff is a tire that can last for an entire rover mission lifetime on Mars, while also pointing to terrestrial benefits: airless operation eliminates flats and underinflation, and avoids the high-pressure risks that make conventional aircraft tires expensive and failure-prone.

Beyond wheels, nitinol’s phase-change behavior powers medical stents, high-force actuators, and temperature-tuned aircraft control surfaces—illustrating why NASA’s “reinvented wheel” is really part of a broader materials revolution built on controllable transformations inside the solid state.

Cornell Notes

Nitinol—a nickel-titanium shape memory alloy—lets engineers build wheels that survive conditions where conventional rubber tires fail. Without air pressure on the Moon and Mars, pneumatic tires can’t rely on internal confinement, and rubber can become brittle in extreme cold. Nitinol solves the strain problem: it can undergo a stress-induced phase change (austenite ↔ detwinned martensite) that allows roughly 6–8% deformation and then recovery, avoiding permanent plastic deformation that would crack or permanently deform metal wheels. NASA’s rover tires use woven nitinol spring meshes designed to deform within that limit and maintain mobility over long missions. The same material also drives stents, actuators, and aircraft mechanisms, showing how phase-change physics can replace brittle or pressure-dependent designs.

Why do pneumatic rubber tires struggle on the Moon and Mars?

They depend on internal air pressure to maintain structure, but those environments lack the external confining pressure that keeps a tire stable. Without that balance, a tire can effectively “explode” under extreme conditions. Temperature swings also matter: in sunlight the temperature facing the sun can be about 250°F above zero, while in shadow it can be about 250°F below zero. Rubber’s glass transition temperature is around 90°F, meaning it can shift from flexible to rigid and become brittle—demonstrated by dipping rubber in liquid nitrogen until it explodes.

What mechanical limitation forces spacecraft materials to avoid large stretching?

When stress exceeds a material’s yield strength, deformation becomes plastic rather than elastic. Plastic deformation comes from defects like edge dislocations moving through the material, rearranging atoms so the shape doesn’t return when the load is removed. Ordinary metals can elastically handle only about 0.3–0.8% strain; beyond that, they yield and may fracture. That’s why spacecraft components are designed so they never stretch more than that elastic range.

How does nitinol achieve large reversible deformation?

Nitinol undergoes a solid-state phase change. In the austenite phase (higher symmetry), cooling leads to twinned martensite. Under applied stress in the martensite phase, the crystal structure can shift to detwinned martensite, enabling extensive deformation without the bond-breaking and dislocation motion typical of ordinary plasticity. When stress is released and the alloy returns to austenite, atoms return to their original locations, restoring the original shape—this is the shape memory effect. In “superelastic” use, the transformation can be stress-induced even without temperature change, enabling about 6–8% stretch and snap-back.

How do NASA rover wheels use nitinol’s properties in practice?

Instead of a rigid metal wheel that cracks under peak loads, engineers weave nitinol springs into a mesh tire. The mesh is designed to flex and absorb shocks while staying within the alloy’s reversible deformation window (about 8%) so it doesn’t permanently deform over long traverses. Testing uses a rotating carousel that can drive the wheel assembly under controlled force-slip conditions (including zero slip) across terrain types from sand to rocks, at rover-like speeds (around 6.7 cm/s).

What broader applications show nitinol’s value beyond tires?

Nitinol’s phase-change behavior powers medical stents: the alloy is cooled below martensite, deformed into a thin shape, inserted via catheter, then warms and “bounces” back to expand an artery. It also acts as an actuator because heating can generate significant force (demonstrations show tens of pounds of force). In aviation, temperature-tuned nitinol mechanisms can stow or deploy control surfaces; demonstrations include a 737 wing box where heating/cooling nitinol tubes can drive flap angles without hydraulic actuators.

Review Questions

  1. What specific environmental factors (pressure and temperature) make conventional rubber pneumatic tires unreliable on the Moon and Mars?
  2. Explain the difference between elastic and plastic deformation, and why the 0.3–0.8% elastic strain limit matters for spacecraft design.
  3. Describe, step by step, how stress-induced phase changes in nitinol enable both shape memory and superelastic recovery.

Key Points

  1. 1

    Nitinol’s shape memory and superelastic behavior allow large reversible deformation (about 6–8%) without permanent plastic damage, which is crucial for long-duration rover mobility.

  2. 2

    Moon and Mars conditions undermine pneumatic rubber tires because there’s little or no external confining pressure and temperatures can swing far enough to make rubber brittle.

  3. 3

    Ordinary metals yield when stress exceeds yield strength, producing plastic deformation via defect motion; typical elastic strain tolerance is about 0.3–0.8%.

  4. 4

    NASA’s planetary wheel designs evolved from hard metal and mesh approaches (e.g., aluminum and steel mesh concepts) toward nitinol mesh tires that can flex repeatedly without cracking.

  5. 5

    Nitinol’s phase transformation between austenite and martensite (including detwinned martensite under stress) restores the original crystal arrangement when stress is removed.

  6. 6

    Rover tire testing uses controlled terrain endurance rigs with a rotating carousel and force-slip conditions to simulate real surface challenges.

  7. 7

    Nitinol’s same phase-change physics also supports stents, high-force actuators, and temperature-driven aircraft mechanisms, not just wheels.

Highlights

Nitinol can stretch roughly 6–8% and still snap back because stress triggers a solid-state phase change rather than ordinary plastic deformation.
The lack of external confining pressure on the Moon and Mars makes pneumatic rubber tires fundamentally risky, and extreme cold can push rubber past its glass transition behavior.
Mars rover wheel failures often trace to thin skins cracking under peak loads, even when the wheel is made from lightweight aluminum.
NASA’s nitinol tires are built as woven spring meshes designed to keep deformation within the alloy’s reversible limit over mission lifetimes.
Phase-change enthalpy can be felt as heat release and absorption during the forward and reverse transformations, enabling concepts like elastocaloric heat pumping.

Topics

  • Nitinol
  • Shape Memory Alloys
  • Planetary Rover Tires
  • Elastic vs Plastic Deformation
  • Phase Transitions