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By NASA
4 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater)
A major component of NASA’s Nancy Grace Roman Space Telescope just took a spin on the centrifuge at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. Called the Outer Barrel Assembly, this piece of the observatory is designed to keep the telescope at a stable temperature and shield it from stray light.
This structure, called the Outer Barrel Assembly, will surround and protect NASA’s Nancy Grace Roman Space Telescope from stray light that could interfere with its observations. In this photo, engineers prepare the assembly for testing.NASA/Chris Gunn The two-part spin test took place in a large, round test chamber. Stretching across the room, a 600,000-pound (272,000-kilogram) steel arm extends from a giant rotating bearing in the center of the floor.
The test itself is like a sophisticated version of a popular carnival attraction, designed to apply centrifugal force to the rider — in this case, the outer covering for Roman’s telescope. It spun up to 18.4 rotations per minute. That may not sound like much, but it generated force equivalent to just over seven times Earth’s gravity, or 7 g, and sent the assembly whipping around at 80 miles per hour.
“We couldn’t test the entire Outer Barrel Assembly in the centrifuge in one piece because it’s too large to fit in the room,” said Jay Parker, product design lead for the assembly at Goddard. The structure stands about 17 feet (5 meters) tall and is about 13.5 feet (4 meters) wide. “It’s designed a bit like a house on stilts, so we tested the ‘house’ and ‘stilts’ separately.”
The “stilts” went first. Technically referred to as the elephant stand because of its similarity to structures used in circuses, this part of the assembly is designed to surround Roman’s Wide Field Instrument and Coronagraph Instrument like scaffolding. It connects the upper portion of the Outer Barrel Assembly to the spacecraft bus, which will maneuver the observatory to its place in space and support it while there. The elephant stand was tested with weights attached to it to simulate the rest of the assembly’s mass.
This photo shows a view from inside the Outer Barrel Assembly for NASA’s Nancy Grace Roman Space Telescope. The inner rings, called baffles, will help protect the observatory’s primary mirror from stray light.NASA/Chris Gunn Next, the team tested the “house” — the shell and a connecting ring that surround the telescope. These parts of the assembly will ultimately be fitted with heaters to help ensure the telescope’s mirrors won’t experience wide temperature swings, which make materials expand and contract.
To further protect against temperature fluctuations, the Outer Barrel Assembly is mainly made of two types of carbon fibers mixed with reinforced plastic and connected with titanium end fittings. These materials are both stiff (so they won’t warp or flex during temperature swings) and lightweight (reducing launch demands).
If you could peel back the side of the upper portion –– the house’s “siding” –– you’d see another weight-reducing measure. Between inner and outer panels, the material is structured like honeycomb. This pattern is very strong and lowers weight by hollowing out portions of the interior.
Designed at Goddard and built by Applied Composites in Los Alamitos, California, Roman’s Outer Barrel Assembly was delivered in pieces and then put together in a series of crane lifts in Goddard’s largest clean room. It was partially disassembled for centrifuge testing, but will now be put back together and integrated with Roman’s solar panels and Deployable Aperture Cover at the end of the year.
In 2025, these freshly integrated components will go through thermal vacuum testing together to ensure they will withstand the temperature and pressure environment of space. Then they’ll move to a shake test to make sure they will hold up against the vibrations they’ll experience during launch. Toward the end of next year, they will be integrated with rest of the observatory.
To virtually tour an interactive version of the telescope, visit:
https://roman.gsfc.nasa.gov/interactive
The Nancy Grace Roman Space Telescope is managed at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, with participation by NASA’s Jet Propulsion Laboratory and Caltech/IPAC in Southern California, the Space Telescope Science Institute in Baltimore, and a science team comprising scientists from various research institutions. The primary industrial partners are BAE Systems, Inc in Boulder, Colorado; L3Harris Technologies in Rochester, New York; and Teledyne Scientific & Imaging in Thousand Oaks, California.
By Ashley Balzer
NASA’s Goddard Space Flight Center, Greenbelt, Md.
Media Contact:
Claire Andreoli
NASA’s Goddard Space Flight Center
301-286-1940
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Last Updated Oct 08, 2024 EditorJamie AdkinsContactClaire Andreoli Related Terms
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By NASA
1 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater)
Gateway’s Habitation and Logistics Outpost stands vertically inside a Thales Alenia Space facility in Turin, Italy, after completing static load testing. Thales Alenia Space Major Gateway hardware recently crossed an important testing milestone on its path to launch to the Moon, where it will support new science and house astronauts in lunar orbit.
Gateway’s HALO (Habitation and Logistics Outpost) successfully completed static load testing, a rigorous stress test of how well the structure responds to the forces encountered in deep space. Thales Alenia Space, subcontractor to Northrop Grumman, conducted the testing in Turin, Italy. Static load testing is one of the major environmental stress tests HALO will undergo, and once all phases of testing are complete, the module will be ready to move from Italy to Gilbert, Arizona, where Northrop Grumman will complete final outfitting.
HALO is one of four pressurized Gateway modules where astronauts will live, conduct science, and prepare for missions to the lunar South Pole region. It will launch with Gateway’s Power and Propulsion Element on a SpaceX Falcon Heavy rocket to lunar orbit.
Gateway is humanity’s first lunar space station supporting a new era of exploration and scientific discovery as part of NASA’s Artemis campaign that will establish a sustained presence on and around the Moon, paving the way for the first crewed mission to Mars.
Gateway’s Habitation and Logistics Outpost stands vertically inside a Thales Alenia Space facility in Turin, Italy, after completing static load testing. Thales Alenia Space Learn More About Gateway Share
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Last Updated Oct 03, 2024 ContactBriana R. Zamorabriana.r.zamora@nasa.govLocationJohnson Space Center Related Terms
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By NASA
Oct. 1, 2024
NASA astronaut Josh Cassada holds a roll-out solar array as he rides the Canadarm2 robotic arm during a spacewalk in support of the Expedition 68 mission aboard the International Space Station on Dec. 3, 2022. Credit: NASA Three-time Spacewalker Josh Cassada to Retire from NASA
NASA astronaut Josh Cassada retired Oct. 1, after 11 years of service to the agency across multiple programs, including 157 days in space and three spacewalks. Cassada also is a retired United States Navy captain and naval aviator with more than two decades of service.
Cassada served as pilot of NASA’s SpaceX Crew-5 mission and Expedition 68 flight engineer aboard the International Space Station, executing myriad maintenance, contingency, and upgrade activities inside the station while also contributing to hundreds of experiments and technology demonstrations. His three spacewalks outside of the orbiting laboratory totaled more than 21 hours, successfully installing a pair of International Space Station Roll-Out Solar Arrays (IROSAs) to boost the station’s electrical capacity. Cassada, alongside crewmate NASA astronaut Frank Rubio, also assembled the infrastructure for a future IROSA installation and fully restored a malfunctioning legacy solar array.
“I want to extend my sincere gratitude to Josh for his dedication and service to human space exploration,” said NASA Johnson Space Center Director Vanessa Wyche. “Josh’s contributions and achievements to the advancement of science and exploration will inspire the next generation of explorers, the Artemis generation, and benefit humanity for decades to come.”
NASA astronaut Josh Cassada poses for a portrait in his extravehicular mobility unit spacesuit on August 8, 2022. Credit: NASA/Robert Markowitz Throughout Expedition 68, Cassada and his crewmates completed extensive problem-solving with ground teams, including the modification of the SpaceX Dragon spacecraft to accommodate an additional crew member in the event of an emergency return, and leveraged the crew’s various skill sets and training to ensure continued safe and effective operations for current and future crews.
In Houston, Cassada served as a capsule communicator in NASA’s Mission Control Center and assistant to the chief of the Astronaut Office for space station operations. As a physicist and test pilot, Cassada also contributed to the development of NASA’s Commercial Crew Program and Orion spacecraft and represented the Astronaut Office in technical and operational reviews of scientific experiments such as the Alpha Magnetic Spectrometer and Cold Atom Lab.
“Josh has played a significant role in NASA’s deliverance of reliable and cost-effective human transportation to and from the space station,” said Norm Knight, director of flight operations at NASA Johnson. “Through his dedication and commitment to human spaceflight exploration, Josh’s work will continue to push us forward on our journey back to the Moon, and beyond. We will miss him and are excited to see what his next journey entails.”
As he transitions from government service, Cassada will return to the private sector, working on extremely low light detection technologies with broad and emerging applications in various areas, including quantum networks and computing, remote sensing, long-range communication, semiconductor manufacturing, and medical imaging.
“I am incredibly grateful for my many opportunities here at NASA,” Cassada said, “and especially to have served alongside some of the most amazing people both on and off our planet, accomplishing things that are only possible when we work and innovate together as a team. As humans, we explore . And each scientific adventure, whether in a lab on Earth or in space, requires courage to explore and advance society. I am incredibly fortunate to have been surrounded by explorers during my entire career so far and going forward. An expedition may seem daunting, but it’s a lot less so when you’re prepared and with the right crewmates.”
Before his selection by NASA in 2013 as a member of NASA’s 21st Class, Cassada earned his doctorate in High Energy Particle Physics from the University of Rochester, New York and was a U.S. Navy pilot, instructor pilot, test pilot, and instructor test pilot. Throughout his career, Cassada has accumulated more than 4,000 flight hours in over 50 different aircraft and has been awarded various military and civilian awards.
Cassada graduated from White Bear Lake Area High School in Minnesota in 1991 and received his bachelor’s in Physics in 1995 from Albion College in Michigan.
Learn more about International Space Station research and operations at:
https://www.nasa.gov/station
-end-
Courtney Beasley
Johnson Space Center, Houston
281-483-5111
courtney.m.beasley@nasa.gov
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By NASA
4 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater)
Water piping is installed near the Thad Cochran Test Stand (B-1/B-2) at NASA’s Stennis Space Center in December 2014. The project to replace and upgrade the center’s high pressure industrial water system was a key milestone in preparations to test the SLS (Space Launch System) core stage ahead of the successful Artemis I launch.NASA/Danny Nowlin Employees install a 96-inch valve near the Thad Cochran Test Stand (B-1/B-2) at NASA’s Stennis Space Center as part of a high-pressure industrial water upgrade project in March 2015.NASA/Danny Nowlin In this March 2022 photo, crews use a shoring system to hold back soil as they install new 75-inch piping leading from the NASA Stennis High Pressure Industrial Water Facility to the valve vault pit serving the Fred Haise Test Stand.NASA/Danny Nowlin Crews use a specially designed tool to place a new pipeline liner inside the existing carrier pipe near the Fred Haise Test Stand in 2024 in the last phase of updating the original test complex industrial water system at NASA’s Stennis Space Center.NASA/Danny Nowlin Crews prepare new pipeline liner sections for installation near the Fred Haise Test Stand in 2024 in the last phase of updating the original test complex industrial water system at NASA’s Stennis Space Center.NASA/Danny Nowlin For almost 60 years, NASA’s Stennis Space Center has tested rocket systems and engines to help power the nation’s human space exploration dreams. Completion of a critical water system infrastructure project helps ensure the site can continue that frontline work moving forward.
“The infrastructure at NASA Stennis is absolutely critical for rocket engine testing for the agency and commercial companies,” said NASA project manager Casey Wheeler. “Without our high pressure industrial water system, testing does not happen. Installing new underground piping renews the lifespan and gives the center a system that can be operated for the foreseeable future, so NASA Stennis can add to its nearly six decades of contributions to space exploration efforts.”
The high pressure industrial water system delivers hundreds of thousands of gallons of water per minute through underground pipes to cool rocket engine exhaust and provide fire suppression capabilities during testing. Without the water flow, the engine exhaust, reaching as hot as 6,000 degrees Fahrenheit, could melt the test stand’s steel flame deflector.
Each test stand also features a FIREX system that holds water in reserve for use in the event of a mishap or fire. During SLS (Space Launch System) core stage testing, water also was used to create a “curtain” around the test hardware, dampening the high levels of noise generated during hot fire and lessening the video-acoustic impact that can cause damage to infrastructure and the test hardware.
Prior to the system upgrade, the water flow was delivered by the site’s original piping infrastructure built in the 1960s. However, that infrastructure had well exceeded its expected 30-year lifespan.
Scope of the Project
The subsequent water system upgrade was planned across multiple phases over a 10-year span. Crews worked around ever-changing test schedules to complete three major projects representing more than $50 million in infrastructure investment.
“Many people working the construction jobs for these projects are from the Gulf Coast area, so it has created jobs and work for the people doing the construction,” Wheeler said. “Some of the specialty work has had people coming in from all over the country, as well as vendors and suppliers that are supplying the materials, so that has an economic impact here too.”
Crews started by replacing large sections of piping, including a 96-inch line, from the 66-million-gallon onsite reservoir to the Thad Cochran (B-1/B-2) Test Stand. This phase also included the installation of a new 25,000-gallon electric pump at the High Pressure Industrial Water Facility to increase water flow capacity. The upgrades were critical for NASA Stennis to conduct Green Run testing of the SLS core stage in 2020-21 ahead of the successful Artemis I launch.
Work in the A Test Complex followed with crews replacing sections of 75-inch piping from the water plant and installing several new 66-inch gate valves.
In the final phase, crews used an innovative approach to install new steel liners within existing pipes leading to the Fred Haise Test Stand (formerly A-1 Test Stand). The work followed NASA’s completion of a successful RS-25 engine test campaign last April for future Artemis missions to the Moon and beyond. The stand now is being prepared to begin testing of new RS-25 flight engines.
Overall, the piping project represents a significant upgrade in design and materials. The new piping is made from carbon steel, with protective linings to prevent corrosion and gate valves designed to be more durable.
Importance of Water
It is hard to overstate the importance of the work to ensure ongoing water flow. For a typical 500-second RS-25 engine test on the Fred Haise Test Stand, around 5 million gallons of water is delivered from the NASA Stennis reservoir through a quarter-of-a-mile of pipe before entering the stand to supply the deflector and cool engine exhaust.
“Without water to cool the deflector and the critical parts of the test stand that will get hot from the hot fire itself, the test stand would need frequent corrective maintenance,” Wheeler said. “This system ensures the test stands remain in a condition where continuous testing can happen.”
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Last Updated Sep 26, 2024 EditorNASA Stennis CommunicationsContactC. Lacy Thompsoncalvin.l.thompson@nasa.gov / (228) 688-3333LocationStennis Space Center Related Terms
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