Roman Telescope’s “Exoskeleton” Passes NASA’s Extreme Centrifuge Trials

Roman Space Telescope Spacecraft Flat Illustration
The Outer Barrel Assembly of the Nancy Grace Roman Space Telescope was tested for endurance under high-speed and gravitational forces at NASA’s Goddard Space Flight Center, ensuring its readiness for the 2025 space mission. Credit: NASA’s Goddard Space Flight Center

The Nancy Grace Roman Space Telescope’s Outer Barrel Assembly underwent rigorous centrifuge testing at NASA’s Goddard Space Flight Center.

This crucial component, designed to stabilize temperature and protect against stray light, was tested in parts due to its large size. The tests subjected it to forces over seven times that of Earth’s gravity to ensure it can withstand the extreme conditions of space.

Nancy Grace Roman Space Telescope’s OBA Testing

A key component of NASA’s Nancy Grace Roman Space Telescope recently underwent a centrifuge test at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. Known as the Outer Barrel Assembly, this crucial part of the observatory helps maintain a stable temperature for the telescope and protects it from stray light.

The two-stage spin test was conducted inside a huge, circular test chamber. A massive 600,000-pound (272,000-kilogram) steel arm, anchored to a giant rotating bearing at the center of the floor, spans across the room.

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.

NASA Roman Space Telescope Outer Barrel Assembly
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. Credit: NASA/Chris Gunn

Stress Testing the Assembly Components

“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.

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.

Roman Space Telescope OBA
The Outer Barrel Assembly (OBA) will protect the telescope from stray light and help keep the mirrors cool. It also serves as structural support for the Solar Array Sun Shield and Deployable Aperture Cover. The OBA is connected directly to the upper deck of the spacecraft support system’s primary structure with a series of struts that extend past the Wide Field Instrument and the Coronagraph Instrument. Credit: NASA’s Goddard Space Flight Center

Advanced Materials and Assembly Design

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.

NASA Roman Space Telescope Inside Outer Barrel Assembly
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. Credit: NASA/Chris Gunn

Final Assembly and Future Testing

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

Roman Space Telescope Spacecraft Details
Three key points about the Roman Space Telescope mission. Credit: NASA’s Goddard Space Flight Center

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.