Jump to content

Mycotecture off Planet: En route to the Moon and Mars


Recommended Posts

  • Publishers
Posted

4 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

Artist concept depicting a new novel aerospace concept for NIAC Phase 3 2024. Lab above Earth with LEO spacecraft above it. Moon, mars and in distance.
Artist concept depicting a new novel aerospace concept for NIAC Phase III 2024.
Credit: Lynn Rothschild

Lynn Rothschild
NASA Ames Research Center (ARC)

A turtle carries its habitat. While reliable, it costs energy in transporting mass. NASA makes the same trade-off when it transports habitats and other structures off planet “on the back” of its missions. While this approach is reliable, to save upmass and increase mission flexibility, NASA must be more like a bird, low mass, agile and building structures from local resources. We identified a novel biology-based solution to the in situ production of usable structures for space exploration: using fungal mycelial (myco) composites to grow structures off-planet, from habitats to furniture to tableware. As a living material it has the potential to self heal, self replicate, be bioengineered, and enhanced with materials such as metals and melanin. Prior performance: During Phase 1, we raised the TRL to 2 by assessing the growth of fungi on different food substrates and analyzing their use on Mars and Earth. In Phase II we completed TRL 3 for an integrated system of inflatables and myco-material production. We designed prototypes and subsystems. We performed proof-of-concepts analyzing myco-material function before and after exposure to relevant environments in a planetary simulator. Our Phase II report and publications documented analytical and experimental results on fungal and inflatable components of the system validating prediction of key parameters. Phase II developed the Phase I mission concept, with an Artemis-inspired focus towards lunar habitats with a “feed forward to Mars” concept.

We assessed fungal/algal/bacterial mixtures by testing different combinations at different temperatures with different food sources, and developed a high throughput, reproducible method for producing fungal materials. We tested sand and regolith simulant composites for in situ material construction. We developed prototypes in silicone scale models, and a 4X4 m model of inflatable architecture and grew a mycelium dome on top. We determined the effect of simulated extraterrestrial conditions on materials showing hyphal damage under UV. By tuning different steps of production, we can change the mechanical properties of the mycelium biocomposites as they undergo compression. We incorporated melanin-producing strains into experiments and models for radiation protection. We drafted designs for mycelium-based lunar habitats. We utilized the 500-Day DRM to the Apollo 15 Hadley-Apenine Region to define science objective and infrastructure requirements to support extended exploration missions to the Moon and Mars, identifying critical gaps that can be filled by mycotecture. Archetypes were drafted per this DRM. Terrestrial applications demonstrated the spin-off potential of the NIAC technology from habitats to tableware.

Innovation and Benefits: If we succeed in developing a fungal biocomposite that can grow itself, we will provide NASA with a radically new, cheaper, faster, more flexible, lighter and sustainable material for extended duration Lunar and Mars mission habitats, as well as for furniture and other structures in flight or at destination.

Milestones and Transition Strategy: The mission context of Phase I was Martian habitats. Mindful of the more immediate focus on Artemis, Phase II focused on a lunar implementation, with a DRM for a 500 day mission to the Apollo 15 Hadley-Max region and the south polar region. En route to realizing these visions, we have identified two intermediate opportunities, both of which require NIAC Phase III funding. They are to (1) test mycotecture suitability and growth in LEO by the integration into an orbiting space station, Starlab, and (2) test mycotecture habitat prototypes on the lunar surface through a CLPS mission. To participate in Starlab, we will develop prototypes for this application and then team with Starlab LLC to raise funding to produce flight-ready structures. To be competitive for a CLPS mission, we will use NIAC funding to raise the technology to TRL6 for this lunar demo mission.

Back to NIAC 2024

Share

Details

Last Updated
Jun 26, 2024
Editor
Loura Hall

View the full article

Join the conversation

You can post now and register later. If you have an account, sign in now to post with your account.
Note: Your post will require moderator approval before it will be visible.

Guest
Reply to this topic...

×   Pasted as rich text.   Paste as plain text instead

  Only 75 emoji are allowed.

×   Your link has been automatically embedded.   Display as a link instead

×   Your previous content has been restored.   Clear editor

×   You cannot paste images directly. Upload or insert images from URL.

  • Similar Topics

    • By Amazing Space
      Backyard Astronomy: LIVE Streaming the Moon 1st July
    • By European Space Agency
      Asteroid 2024 YR4 made headlines earlier this year when its probability of impacting Earth in 2032 rose as high as 3%. While an Earth impact has now been ruled out, the asteroid’s story continues.
      The final glimpse of the asteroid as it faded out of view of humankind’s most powerful telescopes left it with a 4% chance of colliding with the Moon on 22 December 2032.
      The likelihood of a lunar impact will now remain stable until the asteroid returns to view in mid-2028. In this FAQ, find out why we are left with this lingering uncertainty and how ESA's planned NEOMIR space telescope will help us avoid similar situations in the future.
      View the full article
    • By European Space Agency
      The European Space Agency’s Mars Express has captured a swirl of colour on the Red Planet, with yellows and rust-oranges meeting deep reds and browns. Lurking within this martian palette are not one but four dust devils, each snaking their way across the surface.
      View the full article
    • By NASA
      NASA/Bob Hines NASA astronaut Bob Hines took this picture of the waning crescent moon on May 8, 2022, as the International Space Station flew into an orbital sunrise 260 miles above the Atlantic Ocean off the northwest coast of the United States. Since the station became operational in November 2000, crew members have produced hundreds of thousands of images of our Moon and Earth through Crew Earth Observations.
      Image credit: NASA/Bob Hines
      View the full article
    • By NASA
      6 min read
      Preparations for Next Moonwalk Simulations Underway (and Underwater)
      In addition to drilling rock core samples, the science team has been grinding its way into rocks to make sense of the scientific evidence hiding just below the surface.
      NASA’s Perseverance rover uses an abrading bit to get below the surface of a rocky out-crop nicknamed “Kenmore” on June 10. The eight images that make up this video were taken approximately one minute apart by one of the rover’s front hazard-avoidance cameras. NASA/JPL-Caltech On June 3, NASA’s Perseverance Mars rover ground down a portion of a rock surface, blew away the resulting debris, and then went to work studying its pristine interior with a suite of instruments designed to determine its mineralogic makeup and geologic origin. “Kenmore,” as nicknamed by the rover science team, is the 30th Martian rock that Perseverance has subjected to such in-depth scrutiny, beginning with drilling a two-inch-wide (5-centimeter-wide) abrasion patch.  
      “Kenmore was a weird, uncooperative rock,” said Perseverance’s deputy project scientist, Ken Farley from Caltech in Pasadena, California. “Visually, it looked fine — the sort of rock we could get a good abrasion on and perhaps, if the science was right, perform a sample collection. But during abrasion, it vibrated all over the place and small chunks broke off. Fortunately, we managed to get just far enough below the surface to move forward with an analysis.”
      The science team wants to get below the weathered, dusty surface of Mars rocks to see important details about a rock’s composition and history. Grinding away an abrasion patch also creates a flat surface that enables Perseverance’s science instruments to get up close and personal with the rock.
      This close-up view of an abrasion showing distinctive “tool marks” created by the Perseverance’s abrading bit was acquired on June 5. The image was taken from approximately 2.76 inches (7 centimeters) away by the rover’s WATSON imager. NASA/JPL-Caltech/MSSS Perseverance’s gold-colored abrading bit takes center stage in this image of the rover’s drill taken by the Mastcam-Z instrument on Aug. 2, 2021, the 160th day of the mission to Mars.NASA/JPL-Caltech/ASU/MSSS Time to Grind
      NASA’s Mars Exploration Rovers, Spirit and Opportunity, each carried a diamond-dust-tipped grinder called the Rock Abrasion Tool (RAT) that spun at 3,000 revolutions per minute as the rover’s robotic arm pushed it deeper into the rock. Two wire brushes then swept the resulting debris, or tailings, out of the way. The agency’s Curiosity rover carries a Dust Removal Tool, whose wire bristles sweep dust from the rock’s surface before the rover drills into the rock. Perseverance, meanwhile, relies on a purpose-built abrading bit, and it clears the tailings with a device that surpasses wire brushes: the gaseous Dust Removal Tool, or gDRT.
      “We use Perseverance’s gDRT to fire a 12-pounds-per-square-inch (about 83 kilopascals) puff of nitrogen at the tailings and dust that cover a freshly abraded rock,” said Kyle Kaplan, a robotic engineer at NASA’s Jet Propulsion Laboratory in Southern California. “Five puffs per abrasion — one to vent the tanks and four to clear the abrasion. And gDRT has a long way to go. Since landing at Jezero Crater over four years ago, we’ve puffed 169 times. There are roughly 800 puffs remaining in the tank.” The gDRT offers a key advantage over a brushing approach: It avoids any terrestrial contaminants that might be on a brush from getting on the Martian rock being studied.
      To view this video please enable JavaScript, and consider upgrading to a web browser that supports HTML5 video
      This video captures a test of Perseverance’s Gaseous Dust Removal Tool (gDRT) in a vacuum chamber at NASA’s Jet Propulsion Laboratory in August 2020. The tool fires puffs of nitrogen gas at the tailings and dust that cover a rock after it has been abraded by the rover.NASA/JPL-Caltech Having collected data on abraded surfaces more than 30 times, the rover team has in-situ science (studying something in its original place or position) collection pretty much down. After gDRT blows the tailings away, the rover’s WATSON (Wide Angle Topographic Sensor for Operations and eNgineering) imager (which, like gDRT, is at the end of the rover’s arm) swoops in for close-up photos. Then, from its vantage point high on the rover’s mast, SuperCam fires thousands of individual pulses from its laser, each time using a spectrometer to determine the makeup of the plume of microscopic material liberated after every zap. SuperCam also employs a different spectrometer to analyze the visible and infrared light that bounces off the materials in the abraded area.
      “SuperCam made observations in the abrasion patch and of the powdered tailings next to the patch,” said SuperCam team member and “Crater Rim” campaign science lead, Cathy Quantin-Nataf of the University of Lyon in France. “The tailings showed us that this rock contains clay minerals, which contain water as hydroxide molecules bound with iron and magnesium — relatively typical of ancient Mars clay minerals. The abrasion spectra gave us the chemical composition of the rock, showing enhancements in iron and magnesium.”
      Later, the SHERLOC (Scanning Habitable Environments with Raman & Luminescence for Organics & Chemicals) and PIXL (Planetary Instrument for X-ray Lithochemistry) instruments took a crack at Kenmore, too. Along with supporting SuperCam’s discoveries that the rock contained clay, they detected feldspar (the mineral that makes much of the Moon brilliantly bright in sunlight). The PIXL instrument also detected a manganese hydroxide mineral in the abrasion — the first time this type of material has been identified during the mission.  
      With Kenmore data collection complete, the rover headed off to new territories to explore rocks — both cooperative and uncooperative — along the rim of Jezero Crater.
      “One thing you learn early working on Mars rover missions is that not all Mars rocks are created equal,” said Farley. “The data we obtain now from rocks like Kenmore will help future missions so they don’t have to think about weird, uncooperative rocks. Instead, they’ll have a much better idea whether you can easily drive over it, sample it, separate the hydrogen and oxygen contained inside for fuel, or if it would be suitable to use as construction material for a habitat.”
      Long-Haul Roving
      On June 19 (the 1,540th Martian day, or sol, of the mission), Perseverance bested its previous record for distance traveled in a single autonomous drive, trekking 1,348 feet (411 meters). That’s about 210 feet (64 meters) more than its previous record, set on April 3, 2023 (Sol 753). While planners map out the rover’s general routes, Perseverance can cut down driving time between areas of scientific interest by using its self-driving system, AutoNav.
      “Perseverance drove 4½ football fields and could have gone even farther, but that was where the science team wanted us to stop,” said Camden Miller, a rover driver for Perseverance at JPL. “And we absolutely nailed our stop target location. Every day operating on Mars, we learn more on how to get the most out of our rover. And what we learn today future Mars missions won’t have to learn tomorrow.”
      News Media Contact
      DC Agle
      Jet Propulsion Laboratory, Pasadena, Calif.
      818-393-9011
      agle@jpl.nasa.gov
      Karen Fox / Molly Wasser
      NASA Headquarters, Washington
      202-358-1600
      karen.c.fox@nasa.gov / molly.l.wasser@nasa.gov    
      2025-082
      Share
      Details
      Last Updated Jun 25, 2025 Related Terms
      Perseverance (Rover) Jet Propulsion Laboratory Mars Explore More
      5 min read NASA’s Curiosity Mars Rover Starts Unpacking Boxwork Formations
      Article 2 days ago 4 min read NASA Mars Orbiter Captures Volcano Peeking Above Morning Cloud Tops
      Article 3 weeks ago 6 min read NASA’s Ready-to-Use Dataset Details Land Motion Across North America
      Article 3 weeks ago Keep Exploring Discover Related Topics
      Missions
      Humans in Space
      Climate Change
      Solar System
      View the full article
  • Check out these Videos

×
×
  • Create New...