Cosmos Week
Martian Space Suits Will Need To Be 40% Lighter
Earth scienceEnglish editionScience journalismJournalistic coverage

Martian Space Suits Will Need To Be 40% Lighter

Long before a human ever sets foot on the Red Planet, we already know how hard the environment is.

Original source cited and editorially framed by Cosmos Week. Universe Today
Editorial signatureCosmos Week Editorial Desk
Published28 Jul 2026 11: 53 UTC
Updated2026-07-28
Coverage typeScience journalism
Evidence levelJournalistic coverage
Read time4 min read

Key points

  • Focus: Long before a human ever sets foot on the Red Planet, we already know how hard the environment is
  • Detail: Science reporting: verify primary technical documentation
  • Editorial reading: science reporting; whenever possible, verify the cited primary source.
Full story

Long before a human ever sets foot on the Red Planet, we already know how hard the environment is. Once one finally does, the only things protecting them from that harsh environment will be the infrastructure we’ve built up there, and the. The science-journalism coverage adds useful context, while the strongest evidential footing still comes from the underlying data, papers or institutional documentation.

The significance lies in Earth science becomes stronger when local observations can be placed inside a broader physical pattern that spans time and geography. The planet operates as a coupled system in which atmospheric, oceanic, cryospheric and solid-Earth processes interact across timescales from days to millions of years. A measurement that captures one variable at one location and one moment has limited interpretive value until it is embedded in the longer series and wider spatial coverage that allow natural variability to be separated from forced change. Unfortunately, modern space suits aren’t built with Martian gravity, which is 3/8ths of Earth’s, in mind. To prove that point, a team of NASA and industry engineers made a presentation at the 55th International Conference on Environmental Systems (ICES) that showed that the newest.

That might be fine for the Moon, where the gravity is 1/6th that of Earth, and the suit consequently feels more like 28kg (61 lbs). But on Mars, it would still burden an astronaut with an additional 64 kg (141 lbs).

First, they took a conservative approach and set a baseline astronaut weight of 50 kg (108 lbs), representing the 5th percentile of female human astronauts, though admittedly none. With that weight in mind, the authors note that astronauts are expected to maintain a VO2 max (a measure of their aerobic capacity) of 36 ml/min/kg - which is above the average.

Unfortunately, the authors also note astronauts will also lose 15-25% of their aerobic capacity in the months of travel to Mars, meaning their VO2 max will be lower by the time. Which brings the total absolute maximum that a Mars Exploration Extravehicular Mobility Unit (MxEMU) to 104 kg (229 lbs) - a 40% reduction in mass from the current xEMU.

The broader interest lies in linking the observation to climatic, geophysical or environmental dynamics that extend well beyond the immediate event or location. Earth science is unusual in that its most important questions operate on timescales that no single research career can observe directly, making the archival record, whether in ice, sediment, rock or satellite data, as important as any new measurement. Results that can be embedded in that record, and that either confirm or challenge the patterns it reveals, carry disproportionate scientific weight.

Even with the weight reduction, to ensure the astronauts return safely, the authors suggest only a 30-minute walkback radius. Historically, spacesuits allocate about 60% of their weight to the life preserving backpack - the Portable Life Support System (PLSS) - and the other 40% of their weight to the.

Because this item comes through Universe Today as science journalism, it should be treated as contextual reporting rather than primary evidence. Good science reporting can identify why a result matters, connect it to the wider literature and make technical work readable, but the decisive evidence remains in the original paper, dataset, mission release or technical record. That distinction is especially important when a story is later repeated by aggregators, because repetition increases visibility, not evidential strength.

The next step is to place the result inside longer time series and to compare it with independent instruments and independent sites. Earth system observations gain most of their interpretive power from network density and temporal depth, not from any single measurement however precise. Model simulations that assimilate the new data will help clarify whether the observation fits comfortably within known natural variability or represents a shift that existing models do not reproduce.

Source