Seth Aulton, a mechanical engineering and integration technician, installs part of the Propellant Transfer System onto the servicing payload of OSAM-1 inside a cleanroom at Goddard Space Flight Center, Greenbelt, Md., Feb 14, 2023. This photo has been reviewed by OSAM-1 project management and the Export Control Office and is released for public view. NASA/Mike Guinto

Engineering Technician Ryan Fischer torques the Force Gauge Ring on to the vibe table in preparation for vibration testing of the PACE spacecraft bus at NASA Goddard Space Flight Center in Greenbelt Maryland on June 16th, 2021. Photographer: Denny Henry – Goddard Space Flight Center

KENNEDY SPACE CENTER, FLA. - In NASA’s Orbiter Processing Facility Bay 3, United Space Alliance senior shuttle machinist Jake Jackson checks the torque on a newly installed flight tire on Discovery. Discovery processing is under way for the second return to flight test mission, STS-121.

KENNEDY SPACE CENTER, FLA. - In NASA’s Orbiter Processing Facility Bay 3, United Space Alliance senior shuttle machinist Jake Jackson (left) installs and torques flight tires on Discovery. Discovery processing is under way for the second return to flight test mission, STS-121.

KENNEDY SPACE CENTER, FLA. - In the Space Station Processing Facility, workers help maneuver the Control Moment Gyroscope (CMG) onto a stand prior to its being returned to the vendor for repair. The faulty CMG was removed from the International Space Station and replaced with a new one on mission STS-114 in August. A control moment gyroscope is an actuator used to apply very high attitude-control torques to agile spacecraft. The Space Station uses four massive control moment gyroscopes to maintain the Station’s orientation in space.

KENNEDY SPACE CENTER, FLA. - In the Space Station Processing Facility, the Control Moment Gyroscope (CMG) at left is being returned to the vendor for repair. The faulty CMG was removed from the International Space Station and replaced with a new one on mission STS-114 in August. A control moment gyroscope is an actuator used to apply very high attitude-control torques to agile spacecraft. The Space Station uses four massive control moment gyroscopes to maintain the Station’s orientation in space.

KENNEDY SPACE CENTER, FLA. - In the Space Station Processing Facility, workers oversee the packing of the Control Moment Gyroscope (CMG) in a shipping container. The faulty CMG was removed from the International Space Station and replaced with a new one on mission STS-114 in August. A control moment gyroscope is an actuator used to apply very high attitude-control torques to agile spacecraft. The Space Station uses four massive control moment gyroscopes to maintain the Station’s orientation in space.

KENNEDY SPACE CENTER, FLA. - The Control Moment Gyroscope (CMG) is moved across the floor of the Space Station Processing Facility. It is being transferred to a stand prior to its being returned to the vendor for repair. The faulty CMG was removed from the International Space Station and replaced with a new one on mission STS-114 in August. A control moment gyroscope is an actuator used to apply very high attitude-control torques to agile spacecraft. The Space Station uses four massive control moment gyroscopes to maintain the Station’s orientation in space.

KENNEDY SPACE CENTER, FLA. - In the Space Station Processing Facility, the Control Moment Gyroscope (CMG) is moved toward a stand prior to its being returned to the vendor for repair. The faulty CMG was removed from the International Space Station and replaced with a new one on mission STS-114 in August. A control moment gyroscope is an actuator used to apply very high attitude-control torques to agile spacecraft. The Space Station uses four massive control moment gyroscopes to maintain the Station’s orientation in space.

Bolts are torqued on a Compact Fiber Optic Sensing System unit, also known as a FOSS Rocket Box, which was developed at NASA's Armstrong Flight Research Center in California. NASA research engineer Jonathan Lopez works on the unit that is a new variant of aircraft technology that researchers have advanced to withstand the harsh environments of a rocket launch and space travel

As depicted in this illustration, Cassini will plunge into Saturn's atmosphere on Sept. 15, 2017. Using its attitude control thrusters, the spacecraft will work to keep its antenna pointed at Earth while it sends its final data, including the composition of Saturn's upper atmosphere. The atmospheric torque will quickly become stronger than what the thrusters can compensate for, and after that point, Cassini will begin to tumble. When this happens, its radio connection to Earth will be severed, ending the mission. Following loss of signal, the spacecraft will burn up like a meteor in Saturn's upper atmosphere. https://photojournal.jpl.nasa.gov/catalog/PIA21440

CAPE CANAVERAL, Fla. -- In the Space Shuttle Main Engine Processing Facility at NASA's Kennedy Space Center in Florida, space shuttle main engine No. 1 is outfitted with a new turbopump. A suspect turbopump experienced an issue during torque testing and had to be removed and replaced for Discovery's STS-133 mission to the International Space Station. Next, all three main engines will be transported back to Orbiter Processing Facility-3 and reinstalled. The shuttle and its STS-133 crew are targeted to deliver the Express Logistics Carrier-4 filled with external payloads and experiments, as well as critical spare components to the station later this year. Photo credit: NASA_Jack Pfaller

KENNEDY SPACE CENTER, FLA. - In the Space Station Processing Facility, the Control Moment Gyroscope (CMG) is separated from its base and workers help guide it toward a shipping container for its return to the vendor for repair. The faulty CMG was removed from the International Space Station and replaced with a new one on mission STS-114 in August. A control moment gyroscope is an actuator used to apply very high attitude-control torques to agile spacecraft. The Space Station uses four massive control moment gyroscopes to maintain the Station’s orientation in space.

STS078-430-009 (20 June-7 July 1996) --- Astronaut Richard M. Linnehan, mission specialist, performs a test on his leg using the Torque Velocity Dynamometer (TVD). Dr. Thirsk was measuring changes in muscle forces of the leg in this particular view. The TVD hardware is also used to measure arm muscle forces and velocity at the bicep and tricep areas. Crewmembers for the mission performed all experiment protocols prior to flight to develop a baseline and will also perform post-flight tests to complete the analysis. Additionally, muscle biopsies were taken before the flight and will be conducted after the flight.

CAPE CANAVERAL, Fla. -- In Orbiter Processing Facility-3 at NASA's Kennedy Space Center in Florida, space shuttle main engine No. 3 is installed in shuttle Discovery. The engine was removed to give technicians time to replace a suspect turbopump in main engine No. 1, which encountered an issue during torque testing. Discovery and its STS-133 crew are targeted to deliver the Express Logistics Carrier-4 filled with external payloads and experiments, as well as critical spare components to the International Space Station later this year. Photo credit: NASA_Jack Pfaller

STS078-304-018 (20 June - 7 July 1996) --- Payload specialist Robert B. Thirsk, representing the Canadian Space Agency (CSA), performs a test on his arm using the Torque Velocity Dynamometer (TVD). Dr. Thirsk was measuring changes in muscle forces of the bicep and tricep in this particular view. The TVD hardware is also used to measure leg muscle forces and velocity at the ankle and elbow joints. Crew members for the mission performed all experiment protocols prior to flight to develop a baseline and will also perform post-flight tests to complete the analysis. Additionally, muscle biopsies were taken before the flight and will be conducted after the flight.

STS078-398-032 (20 June - 7 July 1996) --- Astronaut Susan J. Helms, payload commander, measures the distance between Jean-Jacques Favier’s head and the luminous torque, used for the Canal and Otolith Interaction Study (COIS) on the Life and Microgravity Spacelab (LMS-1) mission. Favier, representing the French Space Agency (CNES), is one of two international payload specialists on the almost-17-day flight. This view shows the Voluntary Head Movement (VHM) segment of the experiment. The VHM is meant to characterize how the coordination of head and eye movement changes as a result of spaceflight. Since most vestibular functions are influenced by gravity, the COIS experiment is meant to measure response differences in microgravity.

These Vapor Diffusion Apparatus (VDA) trays were first flown in the Thermal Enclosure System (TES) during the USMP-2 (STS-62) mission. Each tray can hold 20 protein crystal growth chambers. Each chamber contains a double-barrel syringe; one barrel holds protein crystal solution and the other holds precipitant agent solution. During the microgravity mission, a torque device is used to simultaneously retract the plugs in all 20 syringes. The two solutions in each chamber are then mixed. After mixing, droplets of the combined solutions are moved onto the syringe tips so vapor diffusion can begin. During the length of the mission, protein crystals are grown in the droplets. Shortly before the Shuttle's return to Earth, the experiment is deactivated by retracting the droplets containing protein crystals, back into the syringes.

KENNEDY SPACE CENTER, FLA. - In the Astrotech payload processing facility, General Dynamics technicians use a socket wrench equipped with a torque meter to tighten the bolts holding one of twin solar arrays to NASA's Gamma-Ray Large Area Space Telescope, or GLAST. The telescope will launch aboard a Delta II rocket May 16 from Launch Pad 17-B on Cape Canaveral Air Force Station. A powerful space observatory, the GLAST will explore the most extreme environments in the universe, and answer questions about supermassive black hole systems, pulsars and the origin of cosmic rays. It also will study the mystery of powerful explosions known as gamma-ray bursts. Photo credit: NASA/Chris Rhodes

CAPE CANAVERAL, Fla. - In Orbiter Processing Facility-1 at NASA's Kennedy Space Center in Florida, United Space Alliance mid-body mechanic Saul Ngy performs torque checks on a wrist camera before it is installed on the orbiter boom sensor system, or OBSS, in space shuttle Atlantis' payload bay. Atlantis is being prepared for its upcoming STS-132 mission. The 50-foot-long OBSS attaches to the end of the shuttle’s robotic arm and supports the cameras and laser systems used to inspect the shuttle’s thermal protection system while in space. Atlantis will deliver an Integrated Cargo Carrier and Russian-built Mini Research Module to the International Space Station on STS-132. Launch is targeted for May 14. Photo credit: NASA_Jim Grossmann

CAPE CANAVERAL, Fla. – The tools that will be used to service NASA's Hubble Space Telescope on the STS-125 mission are displayed in the NASA News Center at NASA's Kennedy Space Center in Florida. This is a closeup of the pistol grip tool that can install and remove instruments, drive latches and open doors. A self-contained, high-torque drive, the tool features an on-board computer that permits users to tailor its performance to the mission demands. On space shuttle Atlantis’ STS-125 mission, Hubble will be serviced for the fifth and final time. The flight will include five spacewalks during which astronauts will refurbish and upgrade the telescope with these state-of-the-art science instruments. As a result, Hubble's capabilities will be expanded and its operational lifespan extended through at least 2014. The payload includes a Wide Field Camera 3, fine guidance sensor and the Cosmic Origins Spectrograph. Launch is scheduled for 2:01 p.m. EDT May 11. Photo credit: NASA/Jack Pfaller

51A-41-058 (12 November 1984) --- Astronaut Joseph P. Allen IV appears to be lifting weights. Astronaut Dale A. Gardner holding on. Actually, Dr. Allen is the sole anchor for the top portion (and most of) the captured Palapa B-2 communications satellite during the Nov. 12 retrieval extravehicular activity (EVA) of the two mission specialists. This scene came near the end of the long-duration task. Gardner used a torque wrench to tighten clamps on an adapter used to secure the Palapa to its "parking place" in Discovery's cargo bay. Note the difference between the two stinger devices stowed on Challenger's port side (right side of frame). The one nearer the spacecraft's vertical stabilizer is spent, having been inserted by Allen earlier in the day to stabilize the communications satellite. The one nearer the camera awaited duty in two days when it would aid in the capture of the Westar VI satellite.

CAPE CANAVERAL, Fla. – The tools that will be used to service NASA's Hubble Space Telescope on the STS-125 mission are displayed in the NASA News Center at NASA's Kennedy Space Center in Florida. At far right is the pistol grip tool. It can install and remove instruments, drive latches and open doors. A self-contained, high-torque drive, the tool features an on-board computer that permits users to tailor its performance to the mission demands. In the foreground are the card extraction and insertion tools to enable removal of electronic cards. At top center is the plastic version of the pistol grip tool used by astronauts during practice in the water tank at NASA' Johnson Space Center. At center left is the bit caddy. On space shuttle Atlantis’ STS-125 mission, Hubble will be serviced for the fifth and final time. The flight will include five spacewalks during which astronauts will refurbish and upgrade the telescope with these state-of-the-art science instruments. As a result, Hubble's capabilities will be expanded and its operational lifespan extended through at least 2014. The payload includes a Wide Field Camera 3, fine guidance sensor and the Cosmic Origins Spectrograph. Launch is scheduled for 2:01 p.m. EDT May 11. Photo credit: NASA/Jack Pfaller

VANDENBERG AIR FORCE BASE, Calif. – In a clean room inside the Astrotech Payload Processing Facility at Vandenberg Air Force Base in California, a technician performs a torque bolt stress test on NASA’s National Polar-orbiting Operational Environmental Satellite System Preparatory Project (NPP). Technicians will perform many tests and checkouts on the satellite system to prepare it for launch. NPP represents a critical first step in building the next-generation of Earth-observing satellites. NPP will carry the first of the new sensors developed for this satellite fleet, now known as the Joint Polar Satellite System (JPSS), to be launched in 2016. NPP is the bridge between NASA’s Earth Observing System (EOS) satellites and the forthcoming series of JPSS satellites. The mission will test key technologies and instruments for the JPSS missions. NPP is targeted to launch Oct. 25 from Space Launch Complex-2 aboard a United Launch Alliance Delta II rocket. For more information, visit http://www.nasa.gov/NPP. Photo credit: NASA/30th Communications Squadron, VAFB

VANDENBERG AIR FORCE BASE, Calif. – In a clean room inside the Astrotech Payload Processing Facility at Vandenberg Air Force Base in California, technicians perform a torque bolt stress test on NASA’s National Polar-orbiting Operational Environmental Satellite System Preparatory Project (NPP). Technicians will perform many tests and checkouts on the satellite system to prepare it for launch. NPP represents a critical first step in building the next-generation of Earth-observing satellites. NPP will carry the first of the new sensors developed for this satellite fleet, now known as the Joint Polar Satellite System (JPSS), to be launched in 2016. NPP is the bridge between NASA’s Earth Observing System (EOS) satellites and the forthcoming series of JPSS satellites. The mission will test key technologies and instruments for the JPSS missions. NPP is targeted to launch Oct. 25 from Space Launch Complex-2 aboard a United Launch Alliance Delta II rocket. For more information, visit http://www.nasa.gov/NPP. Photo credit: NASA/30th Communications Squadron, VAFB

Engineers and technicians prepare NASA's Cold Operable Lunar Deployable Arm (COLDArm) robotic arm system for testing in a thermal vacuum chamber at the agency's Jet Propulsion Laboratory in Southern California in November 2023. Successful testing in this chamber, which was reduced to minus 292 F (minus 180 C), demonstrates the arm can withstand the conditions it would face on the surface of the Moon. To operate in the cold, COLDArm combines several key new technologies: gears made of bulk metallic glass, which require no wet lubrication or heating; cold motor controllers that don't need to be kept warm in an electronics box near the core of the spacecraft, and a cryogenic six-axis force torque sensor that lets the arm "feel" what it's doing and make adjustments. A variety of attachments and small instruments could go on the end of the arm, including a 3D-printed titanium scoop that could be used for collecting samples from a celestial body's surface. Like the arm on NASA's InSight Mars lander, COLDArm could deploy science instruments to the surface. https://photojournal.jpl.nasa.gov/catalog/PIA26162

The 3D-printed titanium scoop of the Cold Operable Lunar Deployable Arm (COLDArm) robotic arm system is poised above a test bed filled with material to simulate lunar regolith (broken rocks and dust) at NASA's Jet Propulsion Laboratory in Southern California. COLDArm can function in temperatures as cold as minus 280 degrees Fahrenheit (minus 173 degrees Celsius). COLDArm is designed to go on a Moon lander and operate during lunar night, a period that lasts about 14 Earth days. Frigid temperatures during lunar night would stymie current spacecraft, which must rely on energy-consuming heaters to stay warm. To operate in the cold, the 6-foot-6-inch (2-meter) arm combines several key new technologies: gears made of bulk metallic glass that require no lubrication or heating, cold motor controllers that don't need to be kept warm in an electronics box near the core of the spacecraft, and a cryogenic six-axis force torque sensor that lets the arm "feel" what it's doing and make adjustments. A variety of attachments and small instruments could go on the end of the arm, including the scoop, which could be used for collecting samples from a planet's surface. Like the arm on NASA's InSight Mars lander, COLDArm could deploy science instruments to the surface. https://photojournal.jpl.nasa.gov/catalog/PIA25317

A group of National Advisory Committee for Aeronautics (NACA) officials and local dignitaries were on hand on May 8, 1942, to witness the Initiation of Research at the NACA's new Aircraft Engine Research Laboratory in Cleveland, Ohio. The group in this photograph was in the control room of the laboratory's first test facility, the Engine Propeller Research Building. The NACA press release that day noted, "First actual research activities in what is to be the largest aircraft engine research laboratory in the world was begun today at the National Advisory Committee for Aeronautics laboratory at the Cleveland Municipal Airport.” The ceremony, however, was largely symbolic since most of the laboratory was still under construction. Dr. George W. Lewis, the NACA's Director of Aeronautical Research, and John F. Victory, NACA Secretary, are at the controls in this photograph. Airport Manager John Berry, former City Manager William Hopkins, NACA Assistant Secretary Ed Chamberlain, Langley Engineer-in-Charge Henry Reid, Executive Engineer Carlton Kemper, and Construction Manager Raymond Sharp are also present. The propeller building contained two torque stands to test complete engines at ambient conditions. The facility was primarily used at the time to study engine lubrication and cooling systems for World War II aircraft, which were required to perform at higher altitudes and longer ranges than previous generations.

CAPE CANAVERAL, Fla. – The tools that will be used to service NASA's Hubble Space Telescope on the STS-125 mission are displayed in the NASA News Center at NASA's Kennedy Space Center in Florida. In the foreground is the pistol grip tool. It can install and remove instruments, drive latches and open doors. A self-contained, high-torque drive, the tool features an on-board computer that permits users to tailor its performance to the mission demands. Behind it is the plastic version used by astronauts during practice in the water tank at NASA' Johnson Space Center. At center left are the card extraction and insertion tools to enable removal of electronic cards. And behind those is the bit caddy. On space shuttle Atlantis’ STS-125 mission, Hubble will be serviced for the fifth and final time. The flight will include five spacewalks during which astronauts will refurbish and upgrade the telescope with these state-of-the-art science instruments. As a result, Hubble's capabilities will be expanded and its operational lifespan extended through at least 2014. The payload includes a Wide Field Camera 3, fine guidance sensor and the Cosmic Origins Spectrograph. Launch is scheduled for 2:01 p.m. EDT May 11. Photo credit: NASA/Jack Pfaller

The 3D-printed titanium scoop of the Cold Operable Lunar Deployable Arm (COLDArm) robotic arm system is poised above a test bed filled with material to simulate lunar regolith (broken rocks and dust) at NASA's Jet Propulsion Laboratory in Southern California. COLDArm can function in temperatures as cold as minus 280 degrees Fahrenheit (minus 173 degrees Celsius). COLDArm is designed to go on a Moon lander and operate during lunar night, a period that lasts about 14 Earth days. Frigid temperatures during lunar night would stymie current spacecraft, which must rely on energy-consuming heaters to stay warm. To operate in the cold, the 6-foot-6-inch (2-meter) arm combines several key new technologies: gears made of bulk metallic glass that require no lubrication or heating, cold motor controllers that don't need to be kept warm in an electronics box near the core of the spacecraft, and a cryogenic six-axis force torque sensor that lets the arm "feel" what it's doing and make adjustments. A variety of attachments and small instruments could go on the end of the arm, including the scoop, which could be used for collecting samples from a planet's surface. Like the arm on NASA's InSight Mars lander, COLDArm could deploy science instruments to the surface. https://photojournal.jpl.nasa.gov/catalog/PIA25318

NASA's Cold Operable Lunar Deployable Arm (COLDArm) robotic arm system reaches out from a lander on the Moon and scoops up regolith (broken rock and dust). Managed by NASA's Jet Propulsion Laboratory in Southern California, COLDArm is designed to operate during lunar night, a period that lasts about 14 Earth days. It can function in temperatures as cold as minus 280 degrees Fahrenheit (minus 173 degrees Celsius). Frigid temperatures during lunar night would stymie the arms on current spacecraft, which must rely on energy-consuming heaters to stay warm. To operate in the cold, the 6-foot-6-inch (2-meter) arm combines several key new technologies: gears made of bulk metallic glass that require no wet lubrication or heating, cold motor controllers that don't need to be kept warm in an electronics box near the core of the spacecraft, and a cryogenic six-axis force torque sensor that lets the arm "feel" what it's doing and make adjustments. A variety of attachments and small instruments could go on the end of the arm, such as a 3D-printed titanium scoop that could collect samples from a planet's surface, similar to what's depicted here. Like the arm on NASA's now-retired InSight Mars lander, COLDArm is also capable of deploying science instruments to the surface. The arm system could be attached to a stationary lander or to a rover. Motiv Space Systems, a partner on COLDArm, developed the cold motor controllers, and also built sections of the arm and assembled it from JPL-supplied parts at the company's Pasadena, California, facility. The COLDArm project is funded through the Lunar Surface Innovation Initiative and managed by the Game Changing Development program in NASA's Space Technology Mission Directorate. Animation available at https://photojournal.jpl.nasa.gov/catalog/PIA26347

In early 2022, the Cold Operable Lunar Deployable Arm (COLDArm) project – led by NASA's Jet Propulsion Laboratory in Southern California – successfully integrated special gears into pieces of a robotic arm that is planned to perform a robot-controlled lunar surface experiment with imagery in the coming years. These bulk metallic glass (BMG) gears, integrated into COLDArm's joints and actuators, were developed through the Game Changing Development bulk metallic glass gears project to operate at extreme temperatures below minus 280 degrees Fahrenheit (minus 173 degrees Celsius). The gear alloys have a disordered atomic-scale structure, making them both strong and elastic enough to withstand these exceptionally low temperatures. Typical gearboxes require heating to operate at such cryogenic temperatures. The BMG gear motors have been tested and successfully operated at roughly minus 279 degrees Fahrenheit (minus 173 degrees Celsius) without heating assistance. This gear motor is one of the key technologies to enable the robotic arm to operate in extremely cold environments, such as during lunar night. Each of the four joints containing BMG gears will be tested once the arm is fully assembled, which is scheduled for spring of 2022. Robotic joint testing will include dynamometer testing to measure torque/rotational speed, as well as cryogenic thermal vacuum testing to understand how the equipment would perform in an environment similar to space. Once proven, the BMG gears and COLDArm capabilities will enable future missions to work in extreme environments on the Moon, Mars, and ocean worlds. https://photojournal.jpl.nasa.gov/catalog/PIA24567

This series of 41 radar images obtained by the Deep Space Network's Goldstone Solar System Radar on July 28, 2025, shows the near-Earth asteroid 2025 OW as it made its close approach with our planet. The asteroid safely passed at about 400,000 miles (640,000 kilometers), or 1.6 times the distance from Earth to the Moon. The asteroid was discovered on July 4, 2025, by the NASA-funded Pan-STARRS2 survey telescope on Haleakala in Maui, Hawaii. These Goldstone observations suggest that 2025 OW is about 200 feet (60 meters) wide and has an irregular shape. The observations also indicate that it is rapidly spinning, completing one rotation every 1½ to 3 minutes, making it one of the fastest-spinning near-Earth asteroids that the powerful radar system has observed. The observations resolve surface features down to 12 feet (3.75 meters) wide. Asteroids can be "spun up" by sunlight being unevenly absorbed and re-emitted across their irregular surfaces. As photons (quantum particles of light) carry a tiny amount of momentum away from the asteroid, a tiny amount of torque is applied and, over time, the asteroid's spin can increase – a phenomenon known as the YORP effect. For 2025 OW to maintain such a fast rotation without breaking apart, it may be a solid object rather than a loosely bound rubble pile like many asteroids. The Goldstone measurements have allowed scientists to greatly reduce uncertainties in the asteroid's distance from Earth and in its future motion for many decades. This July 28 close approach is the closest asteroid 2025 OW will come to Earth for the foreseeable future. Animation available at https://photojournal.jpl.nasa.gov/catalog/PIA26587

The 3D-printed titanium scoop of the Cold Operable Lunar Deployable Arm (COLDArm) robotic arm system is poised above a test bed filled with material to simulate lunar regolith (broken rocks and dust) at NASA's Jet Propulsion Laboratory in Southern California. COLDArm can function in temperatures as cold as minus 280 degrees Fahrenheit (minus 173 degrees Celsius). Robotics engineer David E. Newill-Smith looks on during testing in September 2022. COLDArm is designed to go on a Moon lander and operate during lunar night, a period that lasts about 14 Earth days. Frigid temperatures during lunar night would stymie current spacecraft, which must rely on energy-consuming heaters to stay warm. To operate in the cold, the 6-foot-6-inch (2-meter) arm combines several key new technologies: gears made of bulk metallic glass that require no lubrication or heating, cold motor controllers that don't need to be kept warm in an electronics box near the core of the spacecraft, and a cryogenic six-axis force torque sensor that lets the arm "feel" what it's doing and make adjustments. A variety of attachments and small instruments could go on the end of the arm, including the scoop, which could be used for collecting samples from a planet's surface. Like the arm on NASA's InSight Mars lander, COLDArm could deploy science instruments to the surface. https://photojournal.jpl.nasa.gov/catalog/PIA25316

The Mast Camera, or Mastcam, aboard NASA's Curiosity Mars rover is built with two cameras – the left has a 34 mm focal length; the right, a 100 mm focal length. Behind each lens is a rotating wheel (circled in pink) arranged with filters. In addition to providing color images of the rover's surroundings, the cameras and their filters help scientists determine from afar the composition of rocks by the wavelengths of light, or spectra, they reflect in different colors. On Sept. 19, 2023, the left camera's filter wheel became stuck between the green and clear filter positions, the effects of which can be seen on the mission's raw, or unprocessed, images. The filter wheel is part of a spur-and-pinion mechanism, with the spur teeth around the filter wheel. The actuation uses a small motor that drives the pinion gear both forward and backward. Despite having been commanded at more than twice its normal torque, this motor has been unable to move in the counterclockwise direction. If unable to nudge the wheel back to the clear filter, the mission would rely on the higher resolution 100 mm right camera as the primary color-imaging system. The camera needs to take nine times more images than the left to cover the same area, which could affect how the team scouts for science targets and rover routes. The ability to observe detailed color spectra of rocks from afar would also be degraded. https://photojournal.jpl.nasa.gov/catalog/PIA26043

NASA's Curiosity Mars rover conducted a test on Oct. 17, 2017, as part of the rover team's development of a new way to use the rover's drill. This image from Curiosity's front Hazard Avoidance Camera (Hazcam) shows the drill's bit touching the ground during an assessment of measurements by a sensor on the rover's robotic arm. Curiosity used its drill to acquire sample material from Martian rocks 15 times from 2013 to 2016. In December 2016, the drill's feed mechanism stopped working reliably. During the test shown in this image, the rover touched the drill bit to the ground for the first time in 10 months. The image has been adjusted to brighten shaded areas so that the bit is more evident. The date was the 1,848th Martian day, or sol, of Curiosity's work on Mars In drill use prior to December 2016, two contact posts -- the stabilizers on either side of the bit -- were placed on the target rock while the bit was in a withdrawn position. Then the motorized feed mechanism within the drill extended the bit forward, and the bit's rotation and percussion actions penetrated the rock. A promising alternative now under development and testing -- called feed-extended drilling -- uses motion of the robotic arm to directly advance the extended bit into a rock. In this image, the bit is touching the ground but the stabilizers are not. In the Sol 1848 activity, Curiosity pressed the drill bit downward, and then applied smaller sideways forces while taking measurements with a force/torque sensor on the arm. The objective was to gain understanding about how readings from the sensor can be used during drilling to adjust for any sideways pressure that might risk the bit becoming stuck in a rock. While rover-team engineers are working on an alternative drilling method, the mission continues to examine sites on Mount Sharp, Mars, with other tools. https://photojournal.jpl.nasa.gov/catalog/PIA22063