Established | 2012 |
---|---|
Research type | Unclassified |
Director | Robert Mueller |
Location | Kennedy Space Center, Florida |
Operating agency | NASA |
Website | Swamp Works website |
The Swamp Works is a lean-development, rapid innovation environment at NASA's Kennedy Space Center. [1] [2] [3] [4] It was founded in 2012, [5] when four laboratories in the Surface Systems Office were merged into an enlarged facility with a modified philosophy for rapid technology development. [6] Those laboratories are the Granular Mechanics and Regolith Operations Lab, [7] the Electrostatics and Surface Physics Lab, [8] the Applied Chemistry Lab, [9] and the Life Support and Habitation Systems (LSHS) team. [10] The first two of these are located inside the main Swamp Works building, while the other two use the facility although their primary work is located elsewhere. The team developed the Swamp Works operating philosophy from Kelly Johnson's Skunk Works, including the "14 Rules of Management", from the NASA development shops of Wernher von Braun, and from the innovation culture of Silicon Valley. [11] [12] [13] The team prototypes space technologies rapidly to learn early in the process how to write better requirements, enabling them to build better products, rapidly, and at reduced cost. It was named the Swamp Works for similarity with the Skunk Works and the Phantom Works, but branded by the widespread marshes (swamps) on the Cape Canaveral and Merritt Island property of the Kennedy Space Center. The Swamp Works was co-founded by NASA engineers and scientists Jack Fox, Rob Mueller, and Philip Metzger. The logo, a robotic alligator, was designed by Rosie Mueller, a professional designer and the spouse of Rob Mueller.[ citation needed ]
The Swamp Works' main facility is the high bay in KSC's Engineering Development Lab, which was formerly the Astronaut Training Building during the NASA Apollo program. The building is where Apollo astronauts practiced working with the Lunar Module for lunar landings and extravehicular activities. During the Space Shuttle era it was used as a destination for bus tours from the KSC Visitor Complex. After the visitor complex decided it no longer needed the facility, it was handed back to NASA and was renovated for Swamp Works. The high bay was furnished with a lunar soil testing facility, [14] [15] the "Big Bin", which is thought to be the world's largest indoor, climate controlled lunar regolith chamber [16] and contains 120 tons of BP-1 simulated lunar soil. [17] The simulated soil is a finely crushed basalt from Black Point, Arizona, that has mechanical properties matching lunar soil. [18] The facility has four 3D printers and an adjacent machine shop with lathes, drill presses, a CNC Router, and other equipment to enable rapid iterative prototyping. The facility also includes an Innovation Space where employees are encouraged to work informally in the upstairs loft.[ citation needed ]
The Granular Mechanics and Regolith Operations (GMRO) Lab combines theoretical and experimental granular mechanics with applied robotics to operate with the soil on other planetary bodies, known as regolith. GMRO develops technologies to mine, convey, extract resources from, manufacture with, and construct infrastructure, like buildings and rocket landing pads, from regolith. GMRO also develops self-cleaning connectors for the dusty lunar and martian environments, performs research into rocket blast effects for landing or launching on the surfaces of the Moon, Mars or asteroids, and has developed a miniature space mining robot called the Regolith Advanced Surface Systems Operations Robot (RASSOR). [19] RASSOR has fore-and-after counter-rotating bucket drums to dig in soil in almost zero gravity. The GMRO Lab is involved in organizing and judging the NASA Robotic Mining competition, [20] held annually at the Kennedy Space Center each May, and the Swarmathon University Challenge for swarming robots. [21] GMRO also built the KSC Hazard Field at the north end of the Space Shuttle's runway, which is a field of simulated craters and boulders in sandy regolith. [22] The hazard field was used by the Morpheus Lander project for flight tests in 2013-2014. The GMRO Lab has a large industrial robot arm used for printing buildings from lunar or martian (simulated) regolith mixed with recycled plastic. [23] [24]
The Electrostatics and Surface Physics Lab (ESPL) develops technologies related to the unique physics that occur at material surfaces, leveraging it for applications in space. It developed an Electrodynamic Dust Shield that uses electrostatic forces that shift locations to sweep lunar or Martian dust from spacecraft surfaces. [25] It created sensors that can be mounted into the wheels of planetary rovers to measure the spectrometry of tribocharging as an identification tool for the minerals it is driving over. [26] It is also working on graphene as an energy storage medium. [27] The ESPL and GMRO Lab worked together to develop a Mars Entry Heat Shield made out of regolith bonded by high temperature polymer. [28] It could be made on the Martian moon Phobos then attached to a spacecraft from Earth to land on Mars, resulting in a cost savings for Mars missions. [29]
The Applied Chemistry Lab develops technologies to support launch activities on the Kennedy Space Center and for use on the surfaces of the Moon, Mars or asteroids. [30] Technologies for terrestrial ground operations include toxic vapor detection and environmental remediation. Technologies for use in space include chemical extraction of resources from lunar or Martian soil, recycling packing materials from space launch to create methane and other needed gases, and development of payload instruments for prospecting lunar ice. [31]
The Life Support and Habitation Systems team develops technologies in four main areas. [32] The first is recovery and recycling of water onboard spacecraft. The second is controlling the trace amounts of chemicals such as ammonia that could build up in a spacecraft's enclosed atmosphere. The third is characterizing the microbial content of solid waste during space missions. The fourth is producing food through plant growth. The lab developed and operates the payload VEGGIE on board the International Space Station, which uses LED lighting at specific frequencies to cause plant growth with minimum energy. [33] [34]
The John F. Kennedy Space Center, located on Merritt Island, Florida, is one of the National Aeronautics and Space Administration's (NASA) ten field centers. Since 1968, KSC has been NASA's primary launch center of American spaceflight, research, and technology. Launch operations for the Apollo, Skylab and Space Shuttle programs were carried out from Kennedy Space Center Launch Complex 39 and managed by KSC. Located on the east coast of Florida, KSC is adjacent to Cape Canaveral Space Force Station (CCSFS). The management of the two entities work very closely together, share resources, and operate facilities on each other's property.
Regolith is a blanket of unconsolidated, loose, heterogeneous superficial deposits covering solid rock. It includes dust, broken rocks, and other related materials and is present on Earth, the Moon, Mars, some asteroids, and other terrestrial planets and moons.
Phoenix was an uncrewed space probe that landed on the surface of Mars on May 25, 2008, and operated until November 2, 2008. Phoenix was operational on Mars for 157 sols. Its instruments were used to assess the local habitability and to research the history of water on Mars. The mission was part of the Mars Scout Program; its total cost was $420 million, including the cost of launch.
In space exploration, in situ resource utilization (ISRU) is the practice of collection, processing, storing and use of materials found or manufactured on other astronomical objects that replace materials that would otherwise be brought from Earth.
Lunar regolith is the unconsolidated material found on the surface of the Moon and in the Moon's tenuous atmosphere. Sometimes referred to as Lunar soil, Lunar soil specifically refers to the component of regolith smaller than 1 cm. It differs substantially in properties from terrestrial soil.
David Stewart McKay was chief scientist for astrobiology at the Johnson Space Center. During the Apollo program, McKay provided geology training to the first men to walk on the Moon in the late 1960s. McKay was the first author of a scientific paper postulating past life on Mars on the basis of evidence in Martian meteorite ALH 84001, which had been found in Antarctica. This paper has become one of the most heavily cited papers in planetary science. The NASA Astrobiology Institute was founded partially as a result of community interest in this paper and related topics. He was a native of Titusville, Pennsylvania.
The Solar System Exploration Research Virtual Institute (SSERVI), originally the NASA Lunar Science Institute, is an organization, established by NASA in 2008, that supplemented and extended existing NASA lunar science programs. Supported by the NASA Science Mission Directorate (SMD) and the Exploration Systems Mission Directorate (ESMD), SSERVI is a NASA program office located at the NASA Ames Research Center and was modeled on the NASA Astrobiology Institute (NAI) with dispersed teams across the nation working together to help lead the agency's research activities related to NASA's human exploration goals. Competitively selected team investigations focused on one or more aspects of lunar science investigations of the Moon, from the Moon, and on the Moon.
Martian regolith is the fine blanket of unconsolidated, loose, heterogeneous superficial deposits covering the surface of Mars. The term Martian soil typically refers to the finer fraction of regolith. So far, no samples have been returned to Earth, the goal of a Mars sample-return mission, but the soil has been studied remotely with the use of Mars rovers and Mars orbiters. Its properties can differ significantly from those of terrestrial soil, including its toxicity due to the presence of perchlorates.
Lunarcrete, also known as "mooncrete", an idea first proposed by Larry A. Beyer of the University of Pittsburgh in 1985, is a hypothetical construction aggregate, similar to concrete, formed from lunar regolith, that would reduce the construction costs of building on the Moon. AstroCrete is a more general concept also applicable for Mars.
A lunar regolith simulant is a terrestrial material synthesized in order to approximate the chemical, mechanical, engineering, mineralogical, or particle-size distribution properties of lunar regolith. Lunar regolith simulants are used by researchers who wish to research the materials handling, excavation, transportation, and uses of lunar regolith. Samples of actual lunar regolith are too scarce, and too small, for such research, and have been contaminated by exposure to Earth's atmosphere.
Honeybee Robotics, LLC is a subsidiary of Blue Origin that builds advanced spacecraft, robotic rovers, and other technologies for the exploration of Mars and other planetary bodies in deep space. The company, headquartered in Brooklyn, New York, has additional production facilities in Altadena, California and Longmont, Colorado. The company has 284 employees and creates exploration systems, infrastructure systems, and motion control software for the National Aeronautics and Space Administration (NASA), the Japanese Aerospace Exploration Agency (JAXA), Blue Origin, and other customers. On May 19th, 2023, Honeybee Robotics' parent company, Blue Origin, won a $3.4 Billion contract to build a moon lander and additional spacecraft for NASA's Artemis program. The team, led by Blue Origin, is a partnership between Lockheed Martin, Draper, Boeing, Astrobotic, and Honeybee Robotics.
Interplanetary contamination refers to biological contamination of a planetary body by a space probe or spacecraft, either deliberate or unintentional.
A Mars habitat is a hypothetical place where humans could live on Mars. Mars habitats would have to contend with surface conditions that include almost no oxygen in the air, extreme cold, low pressure, and high radiation. Alternatively, the habitat might be placed underground, which helps solve some problems but creates new difficulties.
Martian regolith simulant is a terrestrial material that is used to simulate the chemical and mechanical properties of Martian regolith for research, experiments and prototype testing of activities related to Martian regolith such as dust mitigation of transportation equipment, advanced life support systems and in-situ resource utilization.
NASA's Lunabotics Challenge
Martian Moons eXploration (MMX) is a robotic space probe set for launch in 2026 to bring back the first samples from Mars' largest moon Phobos. Developed by the Japan Aerospace Exploration Agency (JAXA) and announced on 9 June 2015, MMX will land and collect samples from Phobos once or twice, along with conducting Deimos flyby observations and monitoring Mars's climate.
The Heat Flow and Physical Properties Package (HP3) is a science payload on board the InSight lander that features instruments to study the heat flow and other thermal properties of Mars. One of the instruments, a burrowing probe nicknamed "the mole", was designed to penetrate 5 m (16 ft) below Mars' surface. In March 2019, the mole burrowed a few centimeters, but then became unable to make progress due to various factors. In the following year further attempts were made to resolve the issues, with little net progress. On January 14, 2021, it was announced that efforts to drill into the martian surface using the device had been terminated.
The World Is Not Enough (WINE) is a US project developing a refuelable steam engine system for spacecraft propulsion. WINE developed a method of extracting volatiles from ice, ice-rich regolith, and hydrated soils and uses it as steam propulsion which allows the spacecraft to refuel multiple times and have an extraordinary long service lifetime. This would allow a single spacecraft to visit multiple asteroids, comets or several landing locations at an icy world such as the Moon, Mars, Pluto, Enceladus, Ganymede, Europa, etc.
The Moon bears substantial natural resources which could be exploited in the future. Potential lunar resources may encompass processable materials such as volatiles and minerals, along with geologic structures such as lava tubes that, together, might enable lunar habitation. The use of resources on the Moon may provide a means of reducing the cost and risk of lunar exploration and beyond.
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