What Is Extravehicular Activity? How Spacewalks Work

Extravehicular activity, universally abbreviated as EVA, is any work an astronaut performs outside the pressurized shell of a spacecraft or habitat. What looks from Earth like a serene float alongside the International Space Station is actually one of the most physiologically demanding and technically complex tasks in human spaceflight, requiring hours of preparation before the hatch even opens and carrying risks that range from decompression sickness to fingernail loss. The engineering behind a single spacewalk touches on pressure physics, thermal insulation, radiation shielding, carbon dioxide scrubbing, and human biomechanics, all packed into a suit that must function as a one-person spacecraft.

The Pressure Trade-Off That Defines Every Spacesuit

The single most consequential design decision in any spacesuit is its internal gas pressure, because that number dictates almost everything else. A higher-pressure suit protects astronauts from decompression sickness but becomes stiff and hard to move in, like trying to bend an over-inflated balloon. A lower-pressure suit restores dexterity but pushes the body closer to the threshold where dissolved nitrogen can bubble out of tissues, causing joint pain, neurological symptoms, or worse.

NASA’s current Extravehicular Mobility Unit operates at about 4.3 psi of pure oxygen. The ISS cabin, meanwhile, sits at roughly 14.7 psi with a normal nitrogen-oxygen mix. Stepping from one environment into the other is analogous to a scuba diver ascending too quickly. To manage this, astronauts on the ISS breathe pure oxygen for up to four hours before an EVA, flushing nitrogen from their tissues until the ratio of tissue nitrogen pressure to suit pressure falls to around 1.7, a level considered acceptably safe.1PubMed Central. Revisiting decompression sickness risk and mobility in the context of the SmartSuit, a hybrid planetary spacesuit That four-hour prebreathe is a significant operational penalty. It eats into a crew’s limited schedule and delays urgent repairs.

Engineers have explored several ways around this bottleneck. The Space Shuttle used a reduced cabin atmosphere of about 10.2 psi before EVA days, which shortened the prebreathe to roughly 40 minutes. Another approach is mechanical counterpressure, where tight fabric presses directly against the skin instead of relying entirely on gas pressure. A hybrid design called the SmartSuit proposes combining 4.3 psi of gas pressure with an additional 1 psi of mechanical counterpressure, which could cut prebreathe time while preserving the mobility of a lower-pressure suit.2PubMed Central. Revisiting decompression sickness risk and mobility in the context of the SmartSuit, a hybrid planetary spacesuit – Section: Trade-off analysis The fundamental tension, though, remains unchanged: every psi you add for safety is a psi that fights back against every hand squeeze and arm bend.3SAE International. Essential Aspects of Space Suit Operating Pressure Trade-Off

Breathing, Cooling, and Staying Alive in a Personal Spacecraft

A spacesuit is not just a pressure vessel with limbs. It carries a portable life support system that handles oxygen supply, carbon dioxide removal, temperature regulation, and humidity control for six or more hours at a stretch. Each of those jobs presents its own engineering puzzle.

Carbon dioxide removal is a particularly interesting challenge for future missions to Mars. Current life support systems use either consumable lithium hydroxide canisters, which absorb CO₂ but cannot be reused, or regenerable amine-based beds that adsorb CO₂ during one cycle and vent it to the vacuum of space during the next. The amine approach works beautifully in orbit because the vacuum outside the suit provides an enormous pressure difference that pulls CO₂ off the adsorbent. On Mars, the ambient atmosphere is almost entirely carbon dioxide at a pressure between about 750 and 1,000 pascals, which is higher than the safe partial pressure inside the suit. That means a simple pressure-swing system cannot vent CO₂ effectively, because it would be trying to push carbon dioxide into an environment already rich in it. Engineers have proposed three workarounds: boosting pressure during the uptake phase, pulling a harder vacuum during the regeneration phase, or combining temperature swings with pressure swings.4PubMed Central. Revisiting decompression sickness risk and mobility in the context of the SmartSuit, a hybrid planetary spacesuit None of these is trivial to miniaturize onto someone’s back, which is why Martian suit design remains an active research problem.

Temperature control is equally demanding. In direct sunlight in low Earth orbit, exterior surfaces can exceed 120 °C, while shadowed surfaces plummet well below −100 °C. The suit’s outermost layer, the Thermal Micrometeoroid Garment, is a multi-layer stack, typically around eight distinct layers, each with a specific job: reflecting solar radiation, insulating against conducted heat, and stopping tiny hypervelocity particles.5PubMed Central. Numerical Modeling of the Thermal Insulating Properties of Space Suits Multi-layer insulation remains the standard for the vacuum of low Earth orbit and the lunar surface, though researchers acknowledge that improving these materials is necessary to give astronauts better freedom of movement.6ES Energy and Environment. Research Progress of Thermal Insulation Materials Used in Spacesuits

Underneath all those layers, the astronaut wears a liquid cooling garment threaded with narrow tubes of circulating water. The suit’s control system adjusts the coolant inlet temperature based on real-time physiological signals like skin temperature, core temperature, and estimated metabolic rate, which can swing dramatically as the astronaut shifts between heavy tasks and rest periods during a single EVA.7PubMed. Model of human/liquid cooling garment interaction for space suit automatic thermal control Getting this wrong means either a dangerously overheated astronaut or one burning through cooling resources too fast to finish the job.

How Spacewalks Wear Down the Body

EVA is physically exhausting. Russian researchers developed three independent methods for tracking astronaut metabolic rates during spacewalks: measuring oxygen consumption from pressure drops in the suit’s high-pressure bottle, calculating carbon dioxide production from concentrations in the life support loop, and computing heat removal from coolant temperature differences.8Acta Astronautica. Metabolic assessments during extra-vehicular activity All three approaches pointed to the same reality: spacewalks impose significant cardiovascular and muscular workloads, with metabolic demand spiking unpredictably as tasks change.

But the most widely discussed injury from EVA is surprisingly mundane: losing a fingernail. Onycholysis, where the nail separates from the nail bed, has been a persistent complaint among astronauts who perform multiple EVAs. The culprit is the pressurized glove. When the glove is inflated, the area around the large knuckle joints at the base of the fingers can constrict blood flow. Over the course of a six-hour EVA, that repeated vascular compression can damage the nail bed enough for the nail to detach days or weeks later. Research found that the probability of this injury correlates with hand circumference; astronauts with larger hands are more likely to experience constriction at those critical knuckle joints in NASA’s Phase VI glove. Older glove designs and the Russian Orlan glove, which provide more volume around the knuckles, showed lower injury rates, suggesting that a relatively straightforward design change could reduce the problem.9PubMed. Probability of spacesuit-induced fingernail trauma is associated with hand circumference

The glove issue illustrates a broader theme in EVA design: seemingly small ergonomic compromises accumulate into real medical problems when someone repeats the activity dozens of times over a career. Shoulder injuries, hand fatigue, and pressure sores are all documented consequences, and they are one reason NASA has invested heavily in improving suit fit and joint design for the next generation of spacesuits.

Radiation Exposure During EVA

Inside a spacecraft, astronauts are shielded by layers of aluminum, equipment racks, and water stores. Step outside in a spacesuit, and that protection drops dramatically. The suit provides excellent thermal insulation but relatively little radiation shielding, which makes EVA one of the higher-exposure activities in spaceflight.

Two radiation sources dominate EVA planning. Galactic cosmic rays deliver a slow, steady background dose that is difficult to shield against without impractically thick materials. The more acute concern is solar particle events, when the sun ejects bursts of energetic protons that can deliver dangerous doses in minutes to hours. For lunar and deep-space EVAs, where Earth’s magnetic field offers no protection, the timing and duration of spacewalks must account for solar activity forecasts. Research modeling solar proton event occurrence across solar cycles suggests that EVAs could account for a significant fraction of total crew time on lunar missions, making the cumulative probability of encountering a solar event non-trivial.10Acta Astronautica. Probabilistic assessment of radiation risk for astronauts in space missions

Hard X-ray flares from the sun pose a distinct threat because they arrive at the speed of light, giving essentially zero warning. One analysis calculated that hazardous doses, defined as at least 0.1 gray, should occur with a probability of roughly 10% per 100 hours of accumulated EVA time inside a current spacesuit during lunar or deep-space operations.11Space Weather. Risks due to X‐ray flares during astronaut extravehicular activity Unlike solar proton events, which typically build over hours and can sometimes be anticipated by observing earlier flares, X-ray flares demand strategies based on quick retreat to shelter rather than advance warning. Planning EVA schedules in low Earth orbit can partly mitigate solar proton exposure by routing orbital tracks to avoid the high-latitude regions where protons funnel toward Earth.12Advances in Space Research. Minimizing space radiation exposure during extra-vehicular activity

Taking EVA to the Surface

Orbital EVA and surface EVA are different animals. In orbit, the astronaut floats, tethered to the station, with no dust, no terrain, and no gravity pulling on the suit. On the Moon or Mars, the astronaut walks, climbs, kneels, and digs in an environment that introduces entirely new problems.

Lunar dust is the one that keeps engineers up at night. The fine particles that blanket the Moon’s surface are jagged and electrostatically charged, nothing like the wind-rounded sand grains on Earth. They cling tenaciously to suit fabric, scratch visors, jam seals, and can infiltrate joints. Lunar dust is also biologically toxic if inhaled, which makes keeping it out of the habitat after an EVA just as important as protecting against it outside.13Journal of Space Safety Engineering. Advances in active dust mitigation technologies for spacesuits Active mitigation approaches under development include electrostatic cleaning systems, vibration-based removal, and coatings that reduce particle adhesion, but none has yet proven fully effective under realistic conditions.

The dust problem also influenced a clever architectural concept called the suit port. Instead of cycling through a traditional airlock, which brings a contaminated suit into the habitat and then requires cleaning, a suit port docks the rear of the spacesuit directly onto the outside of a rover or habitat wall. The astronaut climbs in through a hatch in the suit’s back, seals it, and walks away, leaving the dusty exterior permanently outside. This eliminates the airlock cycle entirely, saving time and consumables while keeping fine particles out of the living space.14International Conference On Environmental Systems. Preliminary Development of a Suit Port for Planetary Surface EVA — Design Studies

How Astronauts Train for Spacewalks

You cannot practice a spacewalk in space. The closest analog is underwater, where neutral buoyancy simulates the feeling of weightlessness well enough for astronauts to rehearse hand-over-hand translation along structures, tool handling, and task sequencing. NASA’s Neutral Buoyancy Laboratory in Houston holds about 23 million liters of water and contains full-scale mockups of ISS modules submerged in the pool.15Dagstuhl Publishing. Underwater VR for Astronaut Training Astronauts typically rehearse each planned EVA multiple times in the pool, often spending six or more hours underwater for every hour they will spend in space.

New training approaches are pushing the boundaries of what the pool can teach. One concept being developed for the Blue Abyss facility, a deep-water complex under construction in Cornwall, combines neutral buoyancy with virtual and augmented reality. The idea is to overlay a digital representation of the actual space environment onto the diver’s view while they experience the physical resistance of working in a pressurized suit underwater, creating a more immersive rehearsal than either medium alone.16New Space. Commercial Spaceflight Preparation and Extravehicular Activities Training: The Next Generation Researchers have also built waterproof VR headsets integrated into full-face diving masks, paired with external camera tracking systems, that allow a diver to perform basic EVA tasks on a physical handrail while seeing a virtual space station around them. The tracking system uses four underwater cameras covering a small experimental area, with the physical handrail mirrored precisely in the virtual scene so the astronaut’s hand meets a real object exactly where the digital one appears.17Dagstuhl Publishing. Underwater VR for Astronaut Training The hope is that this kind of system could eventually reduce the need for enormous pools, making EVA training more accessible and more realistic at the same time.

Heads-Up Displays and the Future of EVA Information

Apollo-era astronauts relied on checklists printed on cards strapped to their wrists. The next generation of surface explorers will likely have data projected directly onto their helmet visors. Researchers have designed and tested hybrid heads-up displays for Martian surface EVA that overlay navigation cues, suit health monitors, and emergency alerts onto the astronaut’s field of view without blocking their line of sight. Four prototype displays were built to address different operational needs: surface navigation, suit status monitoring, emergency response, and task-specific guidance. Usability testing found that the surface navigation and task support displays scored well, with mean ratings above 5.3 out of 7, suggesting that helmet-mounted information systems are practical for real missions rather than just a nice idea.18engrXiv. Design of a Hybrid Spacesuit Display for Martian Surface Exploration

The shift toward richer in-helmet displays reflects a broader trend in EVA design: making the astronaut more autonomous. On the Moon or Mars, communication delays with Earth range from barely noticeable to over 20 minutes each way, which means the ground team cannot provide the moment-by-moment guidance that ISS crews have relied on for decades. Astronauts will need to make more decisions on their own, and putting the right information in front of their eyes at the right time is one way to make that feasible.

Robotic Alternatives and the Crewed EVA Question

Given the expense, risk, and physical toll of sending a human outside, a reasonable question is whether robots can do the job instead. In practice, the answer has been “sometimes.” Robotic arms handle a large share of station maintenance, and free-flying inspection drones have been tested both inside and outside the ISS. But complex tasks that require judgment, improvisation, and fine motor control in unpredictable conditions remain stubbornly difficult for robots. The Hubble Space Telescope servicing missions are a classic example: astronauts replaced instruments and repaired systems that were never designed to be serviced in orbit, adapting on the fly when bolts would not cooperate or cable routes did not match the diagrams.

One concept that blurs the line between EVA and robotics is SCOUT, a one-person pod with an integrated robotic arm. Because SCOUT’s cabin pressure can be set at 8.3 psi, close to normal atmospheric pressure, there is no prebreathe requirement before operations. A single operator in a SCOUT pod can theoretically perform tasks that normally require two suited astronauts and a third crew member operating the station’s robotic arm from inside. The system includes cold-gas thrusters for mobility and a self-rescue capability. A probabilistic risk assessment of the concept estimated a 99.9% chance of completing a 600-EVA mission model without crew loss.19SAE International. SCOUT: EVA Capabilities of the Space Construction and Orbital Utility Transport Designs like this suggest that the future of extravehicular work may not always look like a person in a suit drifting against a backdrop of Earth. It might look more like a small pressurized vehicle with arms, piloted by someone in a shirt-sleeve environment, eliminating many of the physiological hazards that have defined EVA since the first spacewalk in 1965.