SLOPE Excavation Laboratory

This color image from NASA Curiosity rover shows an area excavated by the blast of the Mars Science Laboratory descent stage rocket engines. This is part of a larger, high-resolution color mosaic made from images obtained by Curiosity Mast Camera.

CAPE CANAVERAL, Fla. -- Inside a laboratory in the Engineering Development Laboratory, or EDL, at NASA’s Kennedy Space Center in Florida, research physicist Phil Metzger describes lunar excavators and soil processing technologies to a group of Society of Physics students. About 800 graduate and undergraduate physics students toured Kennedy facilities. A group of about 40 students toured laboratories in the Operations and Checkout Building and the EDL during their visit. The physics students were in Orlando for the 2012 Quadrennial Physics Congress. Photo credit: NASA/Cory Huston

CAPE CANAVERAL, Fla. -- Inside a laboratory in the Engineering Development Laboratory, or EDL, at NASA’s Kennedy Space Center in Florida, research physicist Phil Metzger describes lunar excavators and soil processing technologies to a group of Society of Physics students. About 800 graduate and undergraduate physics students toured Kennedy facilities. A group of about 40 students toured laboratories in the Operations and Checkout Building and the EDL during their visit. The physics students were in Orlando for the 2012 Quadrennial Physics Congress. Photo credit: NASA/Cory Huston

Groups from the Granular Mechanics and Regolith Operations (GMRO) laboratory and the Electrostatics and Surface Physics Laboratory (ESPL) gather for a photograph to celebrate the 10th anniversary of Swamp Works at NASA’s Kennedy Space Center in Florida on Feb. 13, 2023. Studies of the mechanics of materials in a launch pad environment are performed in the GMRO lab. The team also develops technologies for handling lunar and Martian regolith, including excavator technologies, pneumatic transport of soil, and magnetic handling of soil. The ESPL group performs scientific investigations to protect flight hardware and launch equipment from the phenomenon of electrostatic discharges, commonly known as sparks.

Groups from the Granular Mechanics and Regolith Operations (GMRO) laboratory and the Electrostatics and Surface Physics Laboratory (ESPL) gather for a photograph to celebrate the 10th anniversary of Swamp Works at NASA’s Kennedy Space Center in Florida on Feb. 13, 2023. Studies of the mechanics of materials in a launch pad environment are performed in the GMRO lab. The team also develops technologies for handling lunar and Martian regolith, including excavator technologies, pneumatic transport of soil, and magnetic handling of soil. The ESPL group performs scientific investigations to protect flight hardware and launch equipment from the phenomenon of electrostatic discharges, commonly known as sparks.

CAPE CANAVERAL, Fla. – At NASA’s Kennedy Space Center in Florida, Robert Lightfoot, NASA associate director, learns about the Regolith Advanced Surface Systems Operations Robot, or RASSOR, Excavator during a tour of the Swamp Works laboratories. Kennedy’s Swamp Works provides rapid, innovative and cost-effective exploration mission solutions, leveraging partnerships across NASA, industry and academia. Kennedy’s research and technology mission is to improve spaceports on Earth, as well as lay the groundwork for establishing spaceports at destinations in space. For more information, visit http:__www.nasa.gov_centers_kennedy_exploration_researchtech_index.html. Photo credit: NASA_Jim Grossmann

The 50-foot diameter primary cooler for the new Propulsion Systems Laboratory No. 3 and 4 facility constructed at the National Aeronautics and Space Administration (NASA) Lewis Research Center. In 1968, 20 years after planning began for the original Propulsion Systems Laboratory test chambers, No. 1 and 2, NASA Lewis began preparations to add two additional and more powerful chambers. The move coincided with the center’s renewed focus on aeronautics in 1966. The new 40-foot long and 24-foot diameter chambers were capable of testing engines twice as powerful any then in existence and significantly larger than those in the original two test chambers. After exiting the engine nozzle, the hot exhaust air passed through a 17-foot diameter water exhaust duct and the 50-foot diameter primary cooler. Twenty-seven hundred water-filled tubes inside the cooler reduced the temperature of the air flow as it passed between the tubes from 3000 to 600 °F. A spray cooler further reduced the temperature of the gases to 150 °F before they were sent to the Central Air Building. Excavations for the new facility were completed by October 1967, and the shell of the building was completed a year later. In September 1968, work began on the new test chambers and associated infrastructure. Construction was completed in late 1972, and the first test was scheduled for February 1973.

JET PROPULSION LABORATORY, CALIF. - The impactor of the Deep Impact spacecraft, suspended by an overhead crane, undergoes inspection in the Fischer Assembly building at Ball Aerospace in Boulder, Colo. Deep Impact will probe beneath the surface of Comet Tempel 1 on July 4, 2005, when the comet is 83 million miles from Earth, and reveal the secrets of its interior. After releasing a 3- by 3-foot projectile (impactor) to crash onto the surface, Deep Impact’s flyby spacecraft will collect pictures and data of how the crater forms, measuring the crater’s depth and diameter, as well as the composition of the interior of the crater and any material thrown out, and determining the changes in natural outgassing produced by the impact. The impactor will separate from the flyby spacecraft 24 hours before it impacts the surface of Tempel 1's nucleus. The impactor delivers 19 Gigajoules (that's 4.8 tons of TNT) of kinetic energy to excavate the crater. This kinetic energy is generated by the combination of the mass of the impactor and its velocity when it impacts. To accomplish this feat, the impactor uses a high-precision star tracker, the Impactor Target Sensor (ITS), and Auto-Navigation algorithms developed by Jet Propulsion Laboratory to guide it to the target. Deep Impact is a NASA Discovery mission. Launch of Deep Impact is scheduled for Jan. 12 from Launch Pad 17-B, Cape Canaveral Air Force Station, Fla.

A caravan of large steel castings arrived at the National Advisory Committee for Aeronautics (NACA) Lewis Flight Propulsion Laboratory in January 1951. These pieces would serve as the two 14-foot diameter test chambers in the new Propulsion Systems Laboratory (PSL). NACA Lewis specialized in aircraft engines and offered many engine test facilities. In the late 1940s, however, the NACA realized a larger facility was required to test the newest jet engines. When completed in October 1952, PSL became the nation’s most powerful facility for testing full-scale engines at simulated flight altitudes. NACA engineers began designing the PSL in 1947, and excavations commenced in September 1949. In the spring of 1950, the facility’s supports were erected, and the two large exhaust gas coolers were installed. Work on the Access Building began in early 1951 with the arrival of the large test section pieces, seen in this photograph. The massive pieces were delivered to the area from the Henry Pratt Company by rail and then loaded on a series of flatbed trucks that transported them to Lewis. The nearest vehicle has one of the clamshell access hatches. PSL was initially used to study the jet engines of the early 1950s and ramjets for missile programs such as Navaho and Bomarc. With the advent of the space program in the late 1950s, the facility was used to investigate complex rocket engines, including the Pratt and Whitney RL-10.

CAPE CANAVERAL, Fla. -- Dr. Phil Metzger, at right, a principal investigator in the Surface Systems Office, discusses some of NASA's cutting-edge projects with media representatives touring the Granular Mechanics and Regolith Operations, or GMRO, Lab in the Swamp Works at NASA's Kennedy Space Center in Florida. The GMRO team develops robotics to excavate regolith and ice as resources and to prepare berms, roads and landing pads. The laboratory also studies the physics of blowing rego¬lith and other materials in a rocket exhaust plume to predict and mitigate the blast effects of launches and landings. The team performed a demonstration of the Regolith Advanced Surface Systems Operations Robot, or RASSOR, for the media. Kennedy's Swamp Works provides rapid, innovative and cost-effective exploration mission solutions, leveraging partnerships across NASA, industry and academia. Kennedy's research and technology mission is to improve spaceports on Earth, as well as lay the groundwork for establishing spaceports at destinations in space. For more information, visit http:__www.nasa.gov_centers_kennedy_exploration_researchtech_index.html. Photo credit: NASA_Frankie Martin

KENNEDY SPACE CENTER, FLA. - At Ball Aerospace in Boulder, Colo., the impactor on the Deep Impact spacecraft is tested. Deep Impact will probe beneath the surface of Comet Tempel 1 on July 4, 2005, when the comet is 83 million miles from Earth, and reveal the secrets of its interior. After releasing a 3- by 3-foot projectile (impactor) to crash onto the surface, Deep Impact’s flyby spacecraft will collect pictures and data of how the crater forms, measuring the crater’s depth and diameter, as well as the composition of the interior of the crater and any material thrown out, and determining the changes in natural outgassing produced by the impact. The impactor will separate from the flyby spacecraft 24 hours before it impacts the surface of Tempel 1's nucleus. The impactor delivers 19 Gigajoules (that's 4.8 tons of TNT) of kinetic energy to excavate the crater. This kinetic energy is generated by the combination of the mass of the impactor and its velocity when it impacts. To accomplish this feat, the impactor uses a high-precision star tracker, the Impactor Target Sensor (ITS), and Auto-Navigation algorithms developed by Jet Propulsion Laboratory to guide it to the target. Deep Impact is a NASA Discovery mission. Launch of Deep Impact is scheduled for Jan. 12 from Launch Pad 17-B, Cape Canaveral Air Force Station, Fla.

NASA image acquired September 3, 2011 Dominici crater, the very bright crater to the top of this image, exhibits bright rays and contains hollows. This crater lies upon the peak ring of Homer Basin, a very degraded peak ring basin that has been filled by volcanism. This image contains several examples of craters that have excavated materials from depth that are spectrally distinct from the surface volcanic layers, providing windows into the subsurface. MESSENGER scientists are estimating the approximate depths of these spectrally distinct materials by applying knowledge of how impacts excavate material during the cratering process. The 1000, 750, and 430 nm bands of the Wide Angle Camera are displayed in red, green, and blue, respectively. This image was acquired as a high-resolution targeted observation. Targeted observations are images of a small area on Mercury's surface at resolutions much higher than the 250-meter/pixel (820 feet/pixel) morphology base map or the 1-kilometer/pixel (0.6 miles/pixel) color base map. It is not possible to cover all of Mercury's surface at this high resolution during MESSENGER's one-year mission, but several areas of high scientific interest are generally imaged in this mode each week. The MESSENGER spacecraft is the first ever to orbit the planet Mercury, and the spacecraft's seven scientific instruments and radio science investigation are unraveling the history and evolution of the Solar System's innermost planet. Visit the Why Mercury? section of this website to learn more about the key science questions that the MESSENGER mission is addressing. During the one-year primary mission, MDIS is scheduled to acquire more than 75,000 images in support of MESSENGER's science goals. Credit: NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington <b><a href="http://www.nasa.gov/audience/formedia/features/MP_Photo_Guidelines.html" rel="nofollow">NASA image use policy.</a></b> <b><a href="http://www.nasa.gov/centers/goddard/home/index.html" rel="nofollow">NASA Goddard Space Flight Center</a></b> enables NASA’s mission through four scientific endeavors: Earth Science, Heliophysics, Solar System Exploration, and Astrophysics. Goddard plays a leading role in NASA’s accomplishments by contributing compelling scientific knowledge to advance the Agency’s mission. <b>Follow us on <a href="http://twitter.com/NASA_GoddardPix" rel="nofollow">Twitter</a></b> <b>Like us on <a href="http://www.facebook.com/pages/Greenbelt-MD/NASA-Goddard/395013845897?ref=tsd" rel="nofollow">Facebook</a></b> <b>Find us on <a href="http://instagrid.me/nasagoddard/?vm=grid" rel="nofollow">Instagram</a></b>

Spacesuit engineer Shane McFarland, left, of the Advanced Suit Team at NASA's Johnson Space Center prepares an astronaut glove for thermal vacuum testing inside a chamber at the agency's Jet Propulsion Laboratory in Southern California on Nov. 1, 2023. Tim Brady of the NASA Engineering and Safety Center (NESC), which spearheaded the glove testing campaign, looks on as McFarland positions the glove in a load lock – one of four small drawer-like chambers through which test materials are inserted into the larger main chamber of a facility called CITADEL (Cryogenic Ice Testing, Acquisition Development, and Excavation Laboratory). The glove was tested at vacuum and temperatures as low as minus 352 degrees Fahrenheit (minus 213 degrees Celsius) – temperatures as frigid as those Artemis III astronauts could experience on the Moon's South Pole. Built to prepare potential future robotic spacecraft for the frosty, low-pressure conditions on ocean worlds like Jupiter's frozen moon Europa, CITADEL has also proven key to evaluating how astronaut gloves and boots hold up in extraordinary cold. The NASA Engineering and Safety Center spearheaded a glove testing campaign in CITADEL from October 2023 to March 2024. Part of a spacesuit design called the Extravehicular Mobility Unit, the gloves tested in the chamber are the sixth version of a glove NASA began using in the 1980s. The testing in CITADEL showed that the legacy glove would not meet thermal requirements in the more challenging lunar South Pole environment. In addition to spotting vulnerabilities with existing suits, the CITADEL experiments will help NASA develop this unique test capability and prepare criteria for standardized, repeatable, and inexpensive test methods for the next-generation lunar suit being built by Axiom Space. https://photojournal.jpl.nasa.gov/catalog/PIA26591

Robotics technologist Brendan Chamberlain-Simon, left, of NASA's Jet Propulsion Laboratory and spacesuit engineer Zach Fester of the agency's Johnson Space Center adjust a thermal vacuum chamber called CITADEL at JPL on Nov. 12, 2024, before testing an astronaut boot inside the chamber. Built to prepare potential robotic explorers for the frosty, low-pressure conditions on ocean worlds like Jupiter's frozen moon Europa, CITADEL (Cryogenic Ice Testing, Acquisition Development, and Excavation Laboratory) has also proven key to evaluating how astronaut gloves and boots hold up in extraordinary cold. It can reach temperatures as low as low as minus 370 degrees Fahrenheit (minus 223 degrees Celsius), approximating extreme conditions Artemis III astronauts will confront in permanently shadowed regions of the lunar South Pole. The boot testing was initiated by the Extravehicular Activity and Human Surface Mobility Program at NASA Johnson and took place from October 2024 to January 2025. The boot is part of a NASA spacesuit called the Exploration Extravehicular Mobility Unit, or xEMU. Test results haven't yet been fully analyzed. In addition to spotting vulnerabilities with existing suits, the experiments are intended to help NASA develop this unique test capability and prepare criteria for standardized, repeatable, and inexpensive test methods for the next-generation lunar suit being built by Axiom Space. https://photojournal.jpl.nasa.gov/catalog/PIA26593

An astronaut glove designed for use during spacewalks on the International Space Station is prepared for thermal vacuum testing inside a chamber at NASA's Jet Propulsion Laboratory in Southern California on Nov. 1, 2023. The glove lies in a load lock, one of four small drawer-like chambers through which test materials are inserted into the larger main chamber of a facility called CITADEL (Cryogenic Ice Testing, Acquisition Development, and Excavation Laboratory). The glove was tested at vacuum and temperatures as low as minus 352 degrees Fahrenheit (minus 213 degrees Celsius) – temperatures as frigid as those Artemis III astronauts could experience on the Moon's South Pole. Built to prepare potential future robotic spacecraft for the frosty, low-pressure conditions on ocean worlds like Jupiter's frozen moon Europa, CITADEL has also proven key to evaluating how astronaut gloves and boots hold up in extraordinary cold. The NASA Engineering and Safety Center spearheaded a glove testing campaign in CITADEL from October 2023 to March 2024. Part of a spacesuit design called the Extravehicular Mobility Unit, the gloves tested in the chamber are the sixth version of a glove NASA began using in the 1980s. The testing in CITADEL showed that the legacy glove would not meet thermal requirements in the more challenging lunar South Pole environment. In addition to spotting vulnerabilities with existing suits, the CITADEL experiments will help NASA develop this unique test capability and prepare criteria for standardized, repeatable, and inexpensive test methods for the next-generation lunar suit being built by Axiom Space. https://photojournal.jpl.nasa.gov/catalog/PIA26430

A boot that's part of a NASA lunar surface spacesuit prototype is readied for testing inside a thermal vacuum chamber called CITADEL at the agency's Jet Propulsion Laboratory in Southern California on Nov. 8, 2024. The thick aluminum plate at right stands in for the frigid surface of the lunar South Pole, where Artemis III astronauts will confront conditions more extreme than any previously experienced by humans. Built to prepare potential future robotic spacecraft for the frosty, low-pressure conditions on ocean worlds like Jupiter's frozen moon Europa, CITADEL (Cryogenic Ice Testing, Acquisition Development, and Excavation Laboratory) has also proven key to evaluating how astronaut gloves and boots hold up in extraordinary cold. It can reach temperatures as low as low as minus 370 degrees Fahrenheit (minus 223 degrees Celsius), approximating conditions in permanently shadowed regions that astronauts will explore. Figure A, showing the outer boot sole, was taken from inside CITADEL on Nov. 13, 2024. The boot is positioned in a load lock, one of four small drawer-like chambers through which test materials are inserted into the larger chamber. Initiated by the Extravehicular Activity and Human Surface Mobility Program at NASA's Johnson Space Center, the boot testing took place from October 2024 to January 2025. The boot is part of a NASA spacesuit called the Exploration Extravehicular Mobility Unit, or xEMU. Results haven't yet been fully analyzed. In addition to spotting vulnerabilities with existing suits, the experiments are intended to help NASA develop this unique test capability and prepare criteria for standardized, repeatable, and inexpensive test methods for the next-generation lunar suit being built by Axiom Space. https://photojournal.jpl.nasa.gov/catalog/PIA26592

On Nov. 1, 2016, the High Resolution Imaging Science Experiment (HiRISE) camera on NASA's Mars Reconnaissance Orbiter observed the impact site of Europe's Schiaparelli test lander, gaining the first color view of the site since the lander's Oct. 19, 2016, arrival. These cutouts from the observation cover three locations where parts of the spacecraft reached the ground: the lander module itself in the upper portion, the parachute and back shell at lower left, and the heat shield at lower right. The heat shield location was outside of the area covered in color. The scale bar of 10 meters (32.8 feet) applies to all three cutouts. Schiaparelli was one component of the European Space Agency's ExoMars 2016 project, which placed the Trace Gas Orbiter into orbit around Mars on the same arrival date. The ExoMars project received data from Schiaparelli during its descent through the atmosphere. ESA reports that the heat shield separated as planned, the parachute deployed as planned but was released (with back shell) prematurely, and the lander hit the ground at a velocity of more than 180 miles per hour (more than 300 kilometers per hour). Information gained from the Nov. 1 observation supplements what was learned from an Oct. 25 HiRISE observation, at PIA21131, which also shows the locations of these three cutouts relative to each other. Where the lander module struck the ground, dark radial patterns that extend from a dark spot are interpreted as "ejecta," or material thrown outward from the impact, which may have excavated a shallow crater. From the earlier image, it was not clear whether the relatively bright pixels and clusters of pixels scattered around the lander module's impact site are fragments of the module or image noise. Now it is clear that at least the four brightest spots near the impact are not noise. These bright spots are in the same location in the two images and have a white color, unusual for this region of Mars. The module may have broken up at impact, and some fragments might have been thrown outward like impact ejecta. The parachute has a different shape in the Nov. 1 image than in the Oct. 25 one, apparently from shifting in the wind. Similar shifting was observed in the parachute of NASA's Mars Science Laboratory mission during the first six months after the Mars arrival of that mission's Curiosity rover in 2012 [PIA16813]. At lower right are several bright features surrounded by dark radial impact patterns, located where the heat shield was expected to impact. The bright spots appear identical in the Nov. 1 and Oct. 25 images, which were taken from different angles, so these spots are now interpreted as bright material, such as insulation layers, not glinting reflections. http://photojournal.jpl.nasa.gov/catalog/PIA21132

This mosaic of Caloris basin is an enhanced-color composite overlain on a monochrome mosaic featured in a previous post. The color mosaic is made up of WAC images obtained when both the spacecraft and the Sun were overhead, conditions best for discerning variations in albedo, or brightness. The monochrome mosaic is made up of WAC and NAC images obtained at off-vertical Sun angles (i.e., high incidence angles) and with visible shadows so as to reveal clearly the topographic form of geologic features. The combination of the two datasets allows the correlation of geologic features with their color properties. In portions of the scene, color differences from image to image are apparent. Ongoing calibration efforts by the MESSENGER team strive to minimize these differences. Caloris basin has been flooded by lavas that appear orange in this mosaic. Post-flooding craters have excavated material from beneath the surface. The larger of these craters have exposed low-reflectance material (blue in this mosaic) from beneath the surface lavas, likely giving a glimpse of the original basin floor material. Analysis of these craters yields an estimate of the thickness of the volcanic layer: 2.5–3.5 km (1.6–2.2 mi.). The MESSENGER spacecraft is the first ever to orbit the planet Mercury, and the spacecraft's seven scientific instruments and radio science investigation are unraveling the history and evolution of the Solar System's innermost planet. In the mission's more than three years of orbital operations, MESSENGER has acquired over 250,000 images and extensive other data sets. MESSENGER is capable of continuing orbital operations until early 2015. Credit: NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington <b><a href="http://www.nasa.gov/audience/formedia/features/MP_Photo_Guidelines.html" rel="nofollow">NASA image use policy.</a></b> <b><a href="http://www.nasa.gov/centers/goddard/home/index.html" rel="nofollow">NASA Goddard Space Flight Center</a></b> enables NASA’s mission through four scientific endeavors: Earth Science, Heliophysics, Solar System Exploration, and Astrophysics. Goddard plays a leading role in NASA’s accomplishments by contributing compelling scientific knowledge to advance the Agency’s mission. <b>Follow us on <a href="http://twitter.com/NASAGoddardPix" rel="nofollow">Twitter</a></b> <b>Like us on <a href="http://www.facebook.com/pages/Greenbelt-MD/NASA-Goddard/395013845897?ref=tsd" rel="nofollow">Facebook</a></b> <b>Find us on <a href="http://instagrid.me/nasagoddard/?vm=grid" rel="nofollow">Instagram</a></b>