Jump to content

30 Years Ago: STS-61, the First Hubble Servicing Mission


Recommended Posts

  • Publishers
Posted

“Trying to do stellar observations from Earth is like trying to do birdwatching from the bottom of a lake.”  James B. Odom, Hubble Program Manager 1983-1990.

The discovery after its launch that the Hubble Space Telescope’s primary mirror suffered from a flaw disappointed scientists who could not obtain the sharp images they had expected. But thanks to the Hubble’s built-in feature of on-orbit servicing, NASA devised a plan to correct the telescope’s optics during the first planned repair mission. The agency assigned one of its most experienced crews to undertake the complex tasks, naming Richard O. Covey, Kenneth D. Bowersox, Kathryn C. Thornton, Claude Nicollier of the European Space Agency, Jeffrey A. Hoffman, F. Story Musgrave, and Thomas D. Akers to the STS-61 first Hubble Servicing Mission. The first all veteran crew since the STS-26 return to flight mission in 1988 had a cumulative 16 previous missions among them and all had previous spacewalking experience. During their 11-day flight in December 1993, they repaired the telescope during an unprecedented five spacewalks in a single space shuttle mission, rendering it more capable than originally designed.

The STS-61 crew of Kenneth D. Bowersox, sitting left, Kathryn C. Thornton, F. Story Musgrave, and Claude Nicollier of the European Space Agency; Richard O. Covey, standing left, Jeffrey A. Hoffman, and Thomas D. Akers The STS-61 crew patch Endeavour rolls over from Launch Pad 39A to 39B at NASA’s Kennedy Space Center in Florida
Left: The STS-61 crew of Kenneth D. Bowersox, sitting left, Kathryn C. Thornton, F. Story Musgrave, and Claude Nicollier of the European Space Agency; Richard O. Covey, standing left, Jeffrey A. Hoffman, and Thomas D. Akers. Middle: The STS-61 crew patch. Right: Endeavour rolls over from Launch Pad 39A to 39B at NASA’s Kennedy Space Center in Florida.

The first Hubble servicing mission proved to be one of the most complex up to that time. With that in mind, on March 16, 1992, NASA named Musgrave, an astronaut since 1967 and a veteran of four previous missions including conducting the first spacewalk of the shuttle era, as the payload commander and one of the four spacewalkers for STS-61. On Aug. 28, NASA named Hoffman, Akers, and Thornton as the other three spacewalkers who in teams of two would carry out the five spacewalks on alternating days. Finally, on Dec. 3, NASA named Covey, Bowersox, and Nicollier as the commander, pilot, and flight engineer, respectively, for the mission. Nicollier also served as the prime operator of the Remote Manipulator System (RMS), or robotic arm, with Bowersox as his backup. The seven-person crew trained intensely for the next year preparing for the complex tasks ahead, including simulating the spacewalks at the Neutral Buoyancy Simulator at NASA’s Marshall Space Flight Center in Huntsville, Alabama, and the Weightless Environment Training Facility at NASA’s Johnson Space Center in Houston. Meanwhile, at NASA’s Kennedy Space Center in Florida, workers prepared space shuttle Endeavour for its fifth journey into space. They rolled the shuttle, assembled with its external tank and solid rocket booster, to Launch Pad 39A on Oct. 28. However, following a wind storm on Oct. 30 that contaminated the payload changeout room with sandy grit, managers decided to move Endeavour to neighboring Pad B on Nov. 15, in only the second roll around in shuttle history.

Schematic of the Hubble Space Telescope’s major components Workers inspect the Hubble Space Telescope’s 94-inch diameter primary mirror prior to assembly Astronauts release the Hubble Space Telescope in April 1990 during the STS-31 mission
Left: Schematic of the Hubble Space Telescope’s major components. Middle: Workers inspect the Hubble Space Telescope’s 94-inch diameter primary mirror prior to assembly. Right: Astronauts release the Hubble Space Telescope in April 1990 during the STS-31 mission.

The first concrete plan for placing an optical telescope in space, above the obscuring and distorting effects of the Earth’s atmosphere, originated with Princeton University astronomer Lyman S. Spitzer in 1946. In 1972, NASA first proposed a plan to launch a Large Space Telescope (LST) and five years later Congress approved the funding. As envisioned, the LST would contain a 94-inch diameter primary mirror and launch on the space shuttle, then still under development, in 1983. With an expected on-orbit lifetime of 15 years, the LST’s instruments would make observations primarily in the visible and ultraviolet parts of the electromagnetic spectrum. In 1983, managers abandoned the original plan to use the space shuttle to return the telescope to Earth for refurbishment and relaunch in favor of in-orbit maintenance and upgrades by astronauts during spacewalks in the shuttle’s payload bay. The same year, NASA renamed the LST after astronomer Edwin P. Hubble and set the launch for October 1986. The Challenger accident in January 1986 delayed the launch of the Hubble Space Telescope until April 24, 1990, during Discovery’s STS-31 mission. The shuttle flew to an unusually high 380-mile orbit to ensure that Hubble would operate above as much of the Earth’s atmosphere as possible. After initial on-orbit activation and checkout of the telescope’s systems, it was time for the much-anticipated “first light” images. The initial images, however, puzzled scientists as they showed stars not as single well-focused points of light but as blurred and fuzzy. Investigators learned that the telescope’s primary mirror suffered from a production error, its edges too flat by 0.003 mm, resulting in an optical problem called spherical aberration. While this significantly degraded the capability of several of Hubble’s instruments to return exceptionally detailed photographs, the telescope still produced some good images. NASA put in place a plan to fix the Hubble’s optical problems without resorting to repairing the mirror. With the spherical aberration well-defined, engineers designed a set of mirrors that astronauts could place aboard Hubble during the previously planned first servicing mission.

Liftoff of space shuttle Endeavour on the STS-61 mission to repair the Hubble Space Telescope The Hubble Space Telescope as seen from Endeavour during the rendezvous, with the end of the Remote Manipulator System (RMS), or robotic arm, visible at lower right On the shuttle’s flight deck, European Space Agency astronaut Claude Nicollier operates the RMS to grapple Hubble
Left: Liftoff of space shuttle Endeavour on the STS-61 mission to repair the Hubble Space Telescope. Middle: The Hubble Space Telescope as seen from Endeavour during the rendezvous, with the end of the Remote Manipulator System (RMS), or robotic arm, visible at lower right. Right: On the shuttle’s flight deck, European Space Agency astronaut Claude Nicollier operates the RMS to grapple Hubble.

Planning for the first servicing mission to Hubble began in 1988, two years before the launch of the telescope. With the post-launch discovery of spherical aberration, the scope of the first servicing mission changed dramatically. The primary goal now focused on correcting the telescope’s optics to ensure that its onboard instruments could function as planned. Engineers developed the Corrective Optics Space telescope Axial Replacement (COSTAR), a tool to correct Hubble’s blurry vision, consisting of five pairs of corrective mirrors placed in front of the Faint Object Camera, the Faint Object Spectrograph, and the Goddard High Resolution Spectrograph (GHRS) instruments. Installing COSTAR required the removal of the High-Speed Photometer, the sacrifice of one instrument outweighed by the saving of the other three. The astronauts also replaced the original Wide Field Planetary Camera (WFPC) with the more advanced WFPC2 to improve the telescope’s ultraviolet performance. The WFPC2 carried its own corrective optics. The astronauts also replaced fuses and the telescope’s two solar arrays, one of which imparted vibrations that prevented precise pointing. On Dec. 2, 1993, space shuttle Endeavour lifted off from Pad 39B at 4:27 a.m. EST, after a one-day weather delay. Following insertion into an unusually high 360-mile orbit to reach Hubble, the astronauts began their initial on-orbit operations by opening the payload bay doors. The next day, Covey and Bowersox performed several engine burns as part of the rendezvous maneuvers. The astronauts checked out the rendezvous radar, the Ku-band antenna, the Canadian-built Remote Manipulator System (RMS) or robotic arm, and the spacesuits, and reduced the pressure inside the shuttle from 14.7 pounds per square inch (psi) to 10.2 psi in preparation for the upcoming spacewalks to reduce the pre-breathe time required to prevent decompression sickness or the bends.

Endeavour approach to the Hubble Space Telescope Hubble secured onto its flight support structure in Endeavour’s payload bay The STS-61 crew poses on Endeavour’s flight deck, with Hubble visible through the windows
Left: Endeavour continues its approach to the Hubble Space Telescope. Middle: Hubble secured onto its flight support structure in Endeavour’s payload bay. Right: The STS-61 crew poses on Endeavour’s flight deck, with Hubble visible through the windows.

On the third day, Covey brought Endeavour to within 30 feet of Hubble so Nicollier could grapple it with the RMS. Covey radioed Houston, “Endeavour has a firm handshake with Mr. Hubble’s telescope.” Nicollier berthed the giant telescope onto its turntable-like Flight Support System (FSS) in the shuttle’s payload bay. Nicollier then used the RMS cameras to perform an inspection of Hubble.

European Space Agency astronaut Claude Nicollier operates the shuttle’s Remote Manipulator System (RMS) or robotic arm in support of the spacewalks Astronaut F. Story Musgrave works on the Hubble Musgrave releases bolts on the replacement solar arrays
First spacewalk. Left: European Space Agency astronaut Claude Nicollier operates the shuttle’s Remote Manipulator System (RMS) or robotic arm in support of the spacewalks. Middle: Astronaut F. Story Musgrave works on the Hubble. Right: Near the end of the first spacewalk, Musgrave releases bolts on the replacement solar arrays.

With Nicollier operating the RMS as he did for all five spacewalks, Hoffman and Musgrave conducted the mission’s first excursion on flight day four. They replaced two sets of Rate Sensing Units that contain gyroscopes to orient the telescope and replaced electrical control units and fuse plugs, providing the telescope with six healthy gyroscopes. Musgrave and Hoffman prepared for the next day’s spacewalk by loosening bolts on the replacement solar arrays, stored in the forward part of the payload bay. The pair spent 7 hours and 54 minutes outside on this first spacewalk. The ground commanded the two existing solar arrays on the telescope to retract, and while one did so the second one did not due to a bent support rod.

Astronaut Kathryn C. Thornton, on the end of the Remote Manipulator System, releases Hubble’s old solar array that failed to retract properly The solar array drifting away from space shuttle Endeavour Thornton disconnects Hubble’s retracted solar array
Second spacewalk. Left: Astronaut Kathryn C. Thornton, on the end of the Remote Manipulator System, releases Hubble’s old solar array that failed to retract properly. Middle: The solar array drifting away from space shuttle Endeavour. Right: Thornton disconnects Hubble’s retracted solar array.

On flight day five, Thornton and Akers stepped outside for the mission’s second spacewalk, lasting 6 hours 36 minutes. The primary tasks revolved around replacing the telescope’s two solar arrays. First, they disconnected the array that would not retract as planned, working only at night since the array generated electricity when exposed to sunlight. With Thornton on the end of the RMS, she released the partially open array as Nicollier pulled her away. Bowersox fired thrusters to separate from the array, the plumes impinging on it causing it to flap like a giant bird. Thornton and Akers then connected one of the new arrays, rotated the telescope on its FSS, disconnected the other array, stowing it in the payload bay for return to Earth, and replaced it with a new one.

Astronauts Jeffrey A. Hoffman, left, and F. Story Musgrave have removed the old Wide Field Planetary Camera (WFPC) from Hubble, the black rectangle at upper left shows its former location With European Space Agency astronaut Claude Nicollier operating the Remote Manipulator System from inside the shuttle, Hoffman guides the new WFPC2 into position, with Musgrave ready to assist Musgrave, left, and Hoffman have installed WFPC2, the white triangle in the middle of the telescope, with Hoffman about to pick up WFPC1 temporarily stowed on the side of the payload bay and place it in its permanent location for return to Earth
Third spacewalk. Left: Astronauts Jeffrey A. Hoffman, left, and F. Story Musgrave have removed the old Wide Field Planetary Camera (WFPC) from Hubble, the black rectangle at upper left shows its former location. Middle: With European Space Agency astronaut Claude Nicollier operating the Remote Manipulator System from inside the shuttle, Hoffman guides the new WFPC2 into position, with Musgrave ready to assist. Right: Musgrave, left, and Hoffman have installed WFPC2, the white triangle in the middle of the telescope, with Hoffman about to pick up WFPC1 temporarily stowed on the side of the payload bay and place it in its permanent location for return to Earth.

On the sixth day, Hoffman and Musgrave took their turn outside for the mission’s third spacewalk. Their primary task involved the replacement of the original WFPC with the more advance WFPC2 instrument. With Nicollier controlling the RMS, Hoffman removed the WFPC1 from the telescope and temporarily stowed it on the side of the payload bay. He then removed WFPC2 from its stowage location and he and Musgrave installed it into the telescope. After stowing WFPC1 in the payload bay for return to Earth, Hoffman replaced two magnetometers, essentially compasses the telescope uses to determine its orientation in space. This third spacewalk lasted 6 hours 47 minutes.

Astronaut Kathryn C. Thornton works in shuttle Endeavour’s payload bay European Space Agency astronaut Claude Nicollier controlling the Remote Manipulator System, Thornton, top, removes the Corrective Optics Space telescope Axial Replacement (COSTAR) from its storage location Astronaut Thomas D. Akers, inside the Hubble Space Telescope prepares to install the COSTAR
Fourth spacewalk. Left: Astronaut Kathryn C. Thornton works in shuttle Endeavour’s payload bay. Middle: With European Space Agency astronaut Claude Nicollier controlling the Remote Manipulator System, Thornton, top, removes the Corrective Optics Space telescope Axial Replacement (COSTAR) from its storage location. Right: Astronaut Thomas D. Akers, inside the Hubble Space Telescope prepares to install the COSTAR.

For Akers and Thornton, the primary tasks of the fourth spacewalk on the mission’s seventh day focused on the removal of the HSP instrument and replacing it with the COSTAR system to correct the telescope’s optics. Akers opened the telescope’s shroud doors and with Thornton removed the HSP, temporarily stowing it on the side of the payload bay. Nicollier then maneuvered the RMS with Thornton to pick up COSTAR from its storage location and translate them to Hubble where Akers awaited to help with the installation. After closing the door and stowing the HSP, and installing an electronics package with additional computer memory, Akers and Thornton finished the 6-hour 50-minut spacewalk.

Remote Manipulator System operator European Space Agency astronaut Claude Nicollier translates Jeffrey A. Hoffman and F. Story Musgrave to the top of the Hubble Space Telescope The second of two solar arrays unfurls as Hoffman and Musgrave continue working Hoffman celebrates the first Hannukah in space, with a spinning dreidel floating nearby
Fifth spacewalk. Left: Remote Manipulator System operator European Space Agency astronaut Claude Nicollier translates Jeffrey A. Hoffman and F. Story Musgrave to the top of the Hubble Space Telescope. Middle: The second of two solar arrays unfurls as Hoffman and Musgrave continue working. Right: Hoffman celebrates the first Hannukah in space, with a spinning dreidel floating nearby.

On the morning of the eighth day, Bowersox used Endeavour’s thrusters to slightly raise and circularize Hubble’s orbit. Hoffman and Musgrave stepped outside for the mission’s fifth and final spacewalk. When the two newly installed solar arrays failed to deploy after ground commanding, they manually deployed them, and the arrays unfurled without incident. They next replaced the solar array drive electronics and fitted an electronic connection box on the GHRS instrument. Hoffman and Musgrave’s final task involved installing covers, manufactured by Bowersox and Nicollier on board the shuttle, on the telescope’s magnetometers. The final spacewalk lasted 7 hours 21 minutes, bringing the mission’s total spacewalk time to 35 hours 28 minutes. Once back inside Endeavour, Hoffman celebrated the first Hanukkah in space during a televised broadcast, displaying a traveling menorah, unlit of course, and a spinning dreidel.

European Space Agency astronaut Claude Nicollier grapples the Hubble Space Telescope, with its high-gain antenna deployed, just prior to release Hubble slowly drifts away from Endeavour A distant view of Hubble, right, with a crescent Moon
Left: European Space Agency astronaut Claude Nicollier grapples the Hubble Space Telescope, with its high-gain antenna deployed, just prior to release. Middle: After its release, Hubble slowly drifts away from Endeavour. Right: A distant view of Hubble, right, with a crescent Moon.

On flight day nine, Nicollier grappled Hubble with the RMS for the final time and lifted it above the payload bay. Ground controllers commanded its aperture door to open, and Nicollier released the telescope. Bowersox fired Endeavour’s thrusters to slowly back away from the telescope. The next day, the astronauts enjoyed a well-deserved day of rest. They returned the shuttle’s cabin pressure to 14.7 psi and tidied up the spacecraft. On the mission’s 11th day, Covey and Bowersox tested Endeavour’s flight control surfaces and practiced touchdowns using a laptop computer, all in preparation for deorbit, entry, and landing the following day.

Astronaut Richard O. Covey guides Endeavour to a landing at NASA’s Kennedy Space Center (KSC) in Florida Workers at KSC continue to safe Endeavour following its landing Images of M100 galactic nucleus before, left, and after the first servicing mission showing the improved optical qualities
Left: Astronaut Richard O. Covey guides Endeavour to a landing at NASA’s Kennedy Space Center (KSC) in Florida. Middle: Workers at KSC continue to safe Endeavour following its landing. Right: Images of M100 galactic nucleus before, left, and after the first servicing mission showing the improved optical qualities.

On Dec. 13, 1993, their 12th and final day in space, the astronauts donned their pressure suits and prepared for the return to Earth. Due to predicted worsening weather conditions at KSC, Mission Control elected to bring them home one orbit earlier than planned. Covey guided Endeavour to a smooth landing at night at KSC, concluding a flight of 10 days, 19 hours, 59 minutes. They circled the Earth 163 times. Within a month, new images from Hubble indicated the repairs returned the telescope to its expected capabilities, providing astronomers with a unique observation platform. The lessons learned from planning and executing the complex series of spacewalks, with extensive coordination with teams on the ground, proved highly useful not only for future Hubble servicing mission but also for the difficult spacewalks required to assemble and maintain the International Space Station.

Timeline of the Hubble Space Telescope’s instruments and their replacements during servicing missions Hubble as it appeared after its release during the final servicing mission in 2009
Left: Timeline of the Hubble Space Telescope’s instruments and their replacements during servicing missions. Right: Hubble as it appeared after its release during the final servicing mission in 2009.

Although the STS-61 crew’s work left the Hubble Space Telescope in better condition than originally designed, over the years it required additional servicing to ensure it met its expected 15-year on-orbit life. Four additional shuttle crews serviced the telescope between 1997 and 2009, and today it carries a suite of instruments far more advanced than its original complement. During the five servicing missions, 16 space walking astronauts conducted 23 spacewalks totaling more than 165 hours, or just under 7 days, to make repairs or improvements to the telescope’s capabilities. To summarize the discoveries made by scientists using data from the Hubble Space Telescope is well beyond the scope of this article. Suffice it to say that during its more than 30 years of operation, information and images returned by Hubble continue to revolutionize astronomy, literally causing scientists to rewrite textbooks, and have dramatically altered how the public views the wonders of the universe. On the technical side, the launch of Hubble and the servicing missions to maintain and upgrade its capabilities have proven conclusively the value of maintainability of space-based scientific platforms. 

Watch the STS-61 crew narrate a video of their Hubble servicing mission.

Share

Details

Last Updated
Dec 04, 2023

Related Terms

View the full article

Join the conversation

You can post now and register later. If you have an account, sign in now to post with your account.
Note: Your post will require moderator approval before it will be visible.

Guest
Reply to this topic...

×   Pasted as rich text.   Paste as plain text instead

  Only 75 emoji are allowed.

×   Your link has been automatically embedded.   Display as a link instead

×   Your previous content has been restored.   Clear editor

×   You cannot paste images directly. Upload or insert images from URL.

  • Similar Topics

    • By NASA
      Download Press Kit (PDF) Return to CLPS Homepage
      View the full article
    • By NASA
      6 Min Read NASA Marshall Reflects on 65 Years of Ingenuity, Teamwork 
      NASA’s Marshall Space Flight Center in Huntsville, Alabama, is celebrating its 65-year legacy of ingenuity and service to the U.S. space program – and the expansion of its science, engineering, propulsion, and human spaceflight portfolio with each new decade since the NASA field center opened its doors on July 1, 1960.
      What many Americans likely call to mind are the “days of smoke and fire,” said Marshall Director Joseph Pelfrey, referring to the work conducted at Marshall to enable NASA’s launch of the first Mercury-Redstone rocket and the Saturn V which lifted Americans to the Moon, the inaugural space shuttle mission, and the shuttle flights that carried the Hubble Space Telescope, Chandra X-ray Observatory, and elements of the International Space Station to orbit. Most recently, he said they’re likely to recall the thunder of NASA’s SLS (Space Launch System), rising into the sky during Artemis I.
      NASA’s Space Launch System, carrying the Orion spacecraft, launches on the Artemis I flight test on Nov. 16, 2022. NASA’s Marshall Space Flight Center in Huntsville, Alabama, led development and oversees all work on the new flagship rocket, building on its storied history of propulsion and launch vehicle design dating back to the Redstone and Saturn rockets. The most powerful rocket ever built, SLS is the backbone of NASA’s Artemis program, set to carry explorers back to the Moon in 2026, help establish a permanent outpost there, and make possible new, crewed journeys to Mars in the years to come.NASA/Bill Ingalls Yet all the other days are equally meaningful, Pelfrey said, highlighting a steady stream of milestones reflecting the work of Marshall civil service employees, contractors, and industry partners through the years – as celebrated in a new “65 Years of Marshall” timeline.
      “The total sum of hours, contributed by tens of thousands of men and women across Marshall’s history, is incalculable,” Pelfrey said. “Together they’ve blended legacy with innovation – advancing space exploration and scientific discovery through collaboration, engineering excellence, and technical solutions. They’ve invented and refined technologies that make it possible to safely live and work in space, to explore other worlds, and to help safeguard our own.
      The total sum of hours, contributed by tens of thousands of men and women across Marshall’s history, is incalculable.
      Joseph Pelfrey
      Marshall Space Flight Center Director
      “Days of smoke and fire may be the most visible signs, but it’s the months and years of preparation and the weeks of post-launch scientific discovery that mark the true dedication, sacrifice, and monumental achievements of this team.”
      Reflecting on Marshall history
      Marshall’s primary task in the 1960s was the development and testing of the rockets that carried the first American astronaut to space, and the much larger and more technically complex Saturn rocket series, culminating in the mighty Saturn V, which carried the first human explorers to the Moon’s surface in 1969.
      “Test, retest, and then fly – that’s what we did here at the start,” said retired engineer Harry Craft, who was part of the original U.S. Army rocket development team that moved from Fort Bliss, Texas, to Huntsville to begin NASA’s work at Marshall. “And we did it all without benefit of computers, working out the math with slide rules and pads of paper.”
      The 138-foot-long first stage of the Saturn V rocket is lowered to the ground following a successful static test firing in fall 1966 at the S-1C test stand at NASA’s Marshall Space Flight Center in Huntsville, Alabama. The Saturn V, developed and managed at Marshall, was a multi-stage, multi-engine launch vehicle that stood taller than the Statue of Liberty and lofted the first Americans to the Moon. Its success helped position Marshall as an aerospace leader in propulsion, space systems, and launch vehicle development.NASA “Those were exciting times,” retired test engineer Parker Counts agreed. He joined Marshall in 1963 to conduct testing of the fully assembled and integrated Saturn first stages. It wasn’t uncommon for work weeks to last 10 hours a day, plus weekend shifts when deadlines were looming. 
      Counts said Dr. Wernher von Braun, Marshall’s first director, insisted staff in the design and testing organizations be matched with an equal number of engineers in Marshall’s Quality and Reliability Assurance Laboratory. 
      “That checks-and-balances engineering approach led to mission success for all 32 of the Saturn family of rockets,” said Counts, who went on to support numerous other propulsion programs before retiring from NASA in 2003.
      “We worked with the best minds and best equipment available, pushing the technology every day to deliver the greatest engineering achievement of the 20th century,” said instrumentation and electronics test engineer Willie Weaver, who worked at Marshall from 1960 to 1988 – and remains a tour guide at its visitor center, the U.S. Space & Rocket Center. 
      We worked with the best minds and best equipment available, pushing the technology every day to deliver the greatest engineering achievement of the 20th century.
      Willie Weaver
      Former Marshall Space Flight Center Employee
      The 1970s at Marshall were a period of transition and expanded scientific study, as NASA ended the Apollo Program and launched the next phase of space exploration. Marshall provided critical work on the first U.S. space station, Skylab, and led propulsion element development and testing for NASA’s Space Shuttle Program.
      Marshall retiree Jim Odom, a founding engineer who got his start launching NASA satellites in the run-up to Apollo, managed the Space Shuttle External Tank project. The role called for weekly trips to NASA’s Michoud Assembly Facility in New Orleans, which has been managed by Marshall since NASA acquired the government facility in 1961. The shuttle external tanks were manufactured in the same bays there where NASA and its contractors built the Saturn rockets. 
      This photograph shows the liquid hydrogen tank and liquid oxygen tank for the Space Shuttle external tank (ET) being assembled in the weld assembly area of the Michoud Assembly Facility (MAF). The ET provides liquid hydrogen and liquid oxygen to the Shuttle’s three main engines during the first eight 8.5 minutes of flight. At 154-feet long and more than 27-feet in diameter, the ET is the largest component of the Space Shuttle, the structural backbone of the entire Shuttle system, and the only part of the vehicle that is not reusable. The ET is manufactured at the Michoud Assembly Facility near New Orleans, Louisiana, by the Martin Marietta Corporation under management of the Marshall Space Flight Center.NASA “We didn’t have cellphones or telecon capabilities yet,” Odom recalled. “I probably spent more time with the pilot of the twin-engine plane in those days than I did with my wife.”
      Marshall’s shuttle propulsion leadership led to the successful STS-1 mission in 1981, launching an era of orbital science exemplified by NASA’s Spacelab program. 
      “Spacelab demonstrated that NASA could continue to achieve things no one had ever done before,” said Craft, who served as mission manager for Spacelab 1 in 1983 – a highlight of his 40-year NASA career. “That combination of science, engineering, and global partnership helped shape our goals in space ever since.” 
      Engineers in the X-ray Calibration Facility at NASA’s Marshall Space Flight Center in Huntsville, Alabama, work to integrate elements of the Chandra X-ray Observatory in this March 1997 photo. Chandra was lifted to orbit by space shuttle Columbia on July 23, 1999, the culmination of two decades of telescope optics, mirror, and spacecraft development and testing at Marshall. In the quarter century since, Chandra has delivered nearly 25,000 detailed observations of neutron stars, supernova remnants, black holes, and other high-energy objects, some as far as 13 billion light-years distant. Marshall continues to manage the program for NASA. NASA Bookended by the successful Hubble and Chandra launches, the 1990s also saw Marshall deliver the first U.S. module for the International Space Station, signaling a transformative new era of human spaceflight.
      Odom, who retired in 1989 as associate administrator for the space station at NASA Headquarters, reflects on his three-decade agency career with pride. 
      “It was a great experience, start to finish, working with the teams in Huntsville and New Orleans and our partners nationwide and around the globe, meeting each new challenge, solving the practical, day-to-day engineering and technology problems we only studied about in college,” he said. 
      Shrouded for transport, a 45-foot segment of the International Space Station’s “backbone” truss rolls out of test facilities at NASA’s Marshall Space Flight Center in Huntsville, Alabama, in July 2000, ready to be flown to the Kennedy Space Center in Florida for launch. Marshall played a key role in the development, testing, and delivery of the truss and other critical space station modules and structural elements, as well as the station’s air and water recycling systems and science payload hardware. Marshall’s Payload Operations Integration Center also continues to lead round-the-clock space station science. NASA That focus on human spaceflight solutions continued into the 21st century. Marshall delivered additional space station elements and science hardware, refined its air and water recycling systems, and led round-the-clock science from the Payload Operations Integration Center. Marshall scientists also managed the Gravity Probe Band Hinode missions and launched NASA’s SERVIR geospatial observation system. Once primary space stationconstruction – and the 40-year shuttle program – concluded in the 2010s, Marshall took on oversight of NASA’s Space Launch System, led James Webb Space Telescope mirror testing, and delivered the orbiting Imaging X-ray Polarimetry Explorer.
      As the 2020s continue, Marshall meets each new challenge with enthusiasm and expertise, preparing for the highly anticipated Artemis II crewed launch and a host of new science and discovery missions – and buoyed by strong industry partners and by the Huntsville community, which takes pride in being home to “Rocket City USA.”
      “Humanity is on an upward, outward trajectory,” Pelfrey said. “And day after day, year after year, Marshall is setting the course to explore beyond tomorrow’s horizon.”
      Read more about Marshall and its 65-year history:
      https://www.nasa.gov/marshall
      Hannah Maginot
      Marshall Space Flight Center, Huntsville, Ala.
      256-544-0034
      hannah.l.maginot@nasa.gov  
      Share
      Details
      Last Updated Feb 24, 2025 EditorBeth RidgewayLocationMarshall Space Flight Center Related Terms
      Marshall Space Flight Center Explore More
      6 min read How NASA’s Lunar Trailblazer Will Make a Looping Voyage to the Moon
      Article 2 weeks ago 5 min read NASA Readies Moon Rocket for the Future with Manufacturing Innovation
      Article 2 weeks ago 5 min read Exoplanets Need to Be Prepared for Extreme Space Weather, Chandra Finds
      Article 1 month ago Keep Exploring Discover More Topics From NASA
      Legacy to Horizon: Marshall 65
      Marshall Space Flight Center Missions
      Marshall Space Flight Center
      Marshall Space Flight Center History
      View the full article
    • By NASA
      4 min read
      Preparations for Next Moonwalk Simulations Underway (and Underwater)
      The Project F.I.R.E. team, part of Falcon Research Labs and current students at Cerritos Community College in California, is researching the use of drones to extinguish fires as part of a NASA research award called the University Student Research Challenge. From left, Logan Stahl, Juan Villa, Angel Ortega, Larisa Mayoral, Jenny Escobar, and Paola Mayoral-Jimenez.Falcon Research Labs Great ideas, and the talent and passion that bring them to life, can be found anywhere.
      In that spirit, NASA’s University Student Research Challenge (USRC) in 2024 selected its first group of community college students to contribute original research to the agency’s transformative vision for 21st century aviation.
      The student-led group, from Cerritos Community College in California, is researching a new method of safely extinguishing wildfires using eco-friendly pellets dropped from uncrewed drones they call Project F.I.R.E. (Fire Intervention Retardant Expeller).
      “Wildfires are a major problem we’re facing today,” said Angel Ortega, project technical director and lead research engineer for Project F.I.R.E. at Cerritos Community College. “The goal of our research is to demonstrate that our prototype drone with biodegradable fire retardant can successfully put out a controlled fire.”
      A Community College First
      Until now, USRC has only selected participants from traditional four-year institutions, compared to a two-year community college. This award exemplifies the activity’s goal of giving all of tomorrow’s aeronautical innovators a shot at NASA support for their research ideas.
      “The University Innovation (UI) project provides a number of different avenues for students to contribute to aeronautics,” said Steven Holz, who manages the USRC award process. “All of the opportunities are different and help build knowledge and skills that would be advantageous to those wanting to continue working on UI opportunities or within NASA.”
      This award is one of two from NASA’s USRC selected in 2024. The team received the USRC award prior to the devastating Los Angeles fires of January 2025.
      “Our thoughts are with everyone affected by this tragedy,” members of the team said in a statement. “As a team, we are deeply committed to advancing innovative solutions to enhance safety and resilience, working toward a future where communities are better protected against such disasters.”
      Innovating a Solution
      The six team members of Project F.I.R.E. are driven by an ethic of public service. As fires continue to affect communities in their native southern California, they are applying their skills to finding a way to help.
      “We want to get the public inspired that there are possible solutions at hand,” Ortega said. “And the work we’re doing now can hopefully build towards that bigger goal of a widespread solution.”
      The research they are pursuing involves dropping biodegradable pellets into fires from uncrewed, autonomous drones. The pellets, upon reaching the ground, combine chemical ingredients which create a foamlike solution of fire retardant that will not contaminate the environment after the fire is extinguished.
      Project F.I.R.E.’s innovative idea for fire suppression involves releasing eco-friendly foam pellets from uncrewed drones.Falcon Research Labs The team is keen to support firefighters and wildland fire managers and keep them safe while managing these natural disasters. The group has met with firefighters, discussed the idea with them, and received useful feedback on how to make the technology work best in the field.
      Though the group is only at the outset of the research, their idea has existed for longer.
      Blue Skies Forever
      Prior to applying for a USRC, Project F.I.R.E. also presented at NASA’s 2024 Gateway to Blue Skies competition, in which they won the “Future Game-Changer” award.
      Through Gateway to Blue Skies, NASA challenges college students to research climate-friendly technologies and applications related to the future of aviation and present them at an annual forum.
      Following Project F.I.R.E.’s participation in the forum, they applied for a USRC grant to begin turning their vision into reality.
      “Our experience with NASA has been incredibly supportive and inspiring,” said Logan Stahl, the project’s operations director. “We thought competing against some of the other schools would be intimidating, but the experience we’ve had is the complete opposite. Everyone was very welcoming, and the NASA representatives communicated with us and asked questions.”
      The USRC support will allow the team to build on their earlier foundations, they said.
      “Because Gateway to Blue Skies is more conceptual, it let us bring our idea to the table. Now through USRC, we can start building hands-on and make our idea come to life,” said Larisa Mayoral, chemical engineer and laboratory operations manager.
      The Project F.I.R.E. team receives their “Future Game-Changer” award during the 2024 Gateway to Blue Skies forum held at NASA’s Ames Research Center in California.NASA / Brandon Torres The team expressed gratitude, speaking as community college students, for their ability to participate in and contribute research at a level that competes with top-brass universities.
      “We’re very appreciative of our college and NASA providing us this opportunity,” said Paola Mayoral Jimenez, laboratory coordinator and safety manager. “By doing this project, we hope to shine a light on community colleges, their students, and what they have to offer.”
      Complete details on USRC awardees and solicitations, such as what to include in a proposal and how to submit it, are available on the NASA Aeronautics Research Mission Directorate solicitation page.
      About the Author
      John Gould
      Aeronautics Research Mission DirectorateJohn Gould is a member of NASA Aeronautics' Strategic Communications team at NASA Headquarters in Washington, DC. He is dedicated to public service and NASA’s leading role in scientific exploration. Prior to working for NASA Aeronautics, he was a spaceflight historian and writer, having a lifelong passion for space and aviation.
      Facebook logo @NASA@NASAaero@NASA_es @NASA@NASAaero@NASA_es Instagram logo @NASA@NASAaero@NASA_es Linkedin logo @NASA Explore More
      3 min read NASA Selects New Round of Student-Led Aviation Research Awards
      Article 5 days ago 3 min read NASA’s X-59 Turns Up Power, Throttles Through Engine Tests
      Article 2 weeks ago 3 min read NASA Supports GoAERO University Awardees for Emergency Aircraft Prototyping
      Article 2 weeks ago Keep Exploring Discover More Topics From NASA
      Missions
      Artemis
      Aeronautics STEM
      Explore NASA’s History
      Share
      Details
      Last Updated Feb 23, 2025 EditorJim BankeContactAngela Surgenorangela.d.surgenor@nasa.gov Related Terms
      Aeronautics Aeronautics Research Mission Directorate Flight Innovation Transformative Aeronautics Concepts Program University Innovation University Student Research Challenge View the full article
    • By NASA
      This NASA/ESA Hubble Space Telescope reveals clouds of gas and dust near the Tarantula Nebula, located in the Large Magellanic Cloud about 160,000 light-years away.ESA/Hubble & NASA, C. Murray The universe is a dusty place, as this NASA/ESA Hubble Space Telescope image featuring swirling clouds of gas and dust near the Tarantula Nebula reveals. Located in the Large Magellanic Cloud about 160,000 light-years away in the constellations Dorado and Mensa, the Tarantula Nebula is the most productive star-forming region in the nearby universe, home to the most massive stars known.
      The nebula’s colorful gas clouds hold wispy tendrils and dark clumps of dust. This dust is different from ordinary household dust, which may include bits of soil, skin cells, hair, and even plastic. Cosmic dust is often comprised of carbon or of molecules called silicates, which contain silicon and oxygen. The data in this image was part of an observing program that aims to characterize the properties of cosmic dust in the Large Magellanic Cloud and other nearby galaxies.
      Dust plays several important roles in the universe. Even though individual dust grains are incredibly tiny, far smaller than the width of a single human hair, dust grains in disks around young stars clump together to form larger grains and eventually planets. Dust also helps cool clouds of gas so that they can condense into new stars. Dust even plays a role in making new molecules in interstellar space, providing a venue for individual atoms to find each other and bond together in the vastness of space.
      View the full article
    • By NASA
      Explore Hubble Hubble Home Overview About Hubble The History of Hubble Hubble Timeline Why Have a Telescope in Space? Hubble by the Numbers At the Museum FAQs Impact & Benefits Hubble’s Impact & Benefits Science Impacts Cultural Impact Technology Benefits Impact on Human Spaceflight Astro Community Impacts Science Hubble Science Science Themes Science Highlights Science Behind Discoveries Hubble’s Partners in Science Universe Uncovered Explore the Night Sky Observatory Hubble Observatory Hubble Design Mission Operations Missions to Hubble Hubble vs Webb Team Hubble Team Career Aspirations Hubble Astronauts News Hubble News Hubble News Archive Social Media Media Resources Multimedia Multimedia Images Videos Sonifications Podcasts e-Books Online Activities Lithographs Fact Sheets Posters Hubble on the NASA App Glossary More 35th Anniversary Online Activities 2 min read
      Hubble Spies a Spiral That May Be Hiding an Imposter
      The spiral galaxy UGC 5460 shines in this NASA/ESA Hubble Space Telescope image. UGC 5460 sits about 60 million light-years away in the constellation Ursa Major. ESA/Hubble & NASA, W. Jacobson-Galán, A. Filippenko, J. Mauerhan
      Download this image

      The sparkling spiral galaxy gracing this NASA/ESA Hubble Space Telescope image is UGC 5460, which sits about 60 million light-years away in the constellation Ursa Major. This image combines four different wavelengths of light to reveal UGC 5460’s central bar of stars, winding spiral arms, and bright blue star clusters. Also captured in the upper left-hand corner is a far closer object: a star just 577 light-years away in our own galaxy.
      UGC 5460 has hosted two recent supernovae: SN 2011ht and SN 2015as. It’s because of these two stellar explosions that Hubble targeted this galaxy, collecting data for three observing programs that aim to study various kinds of supernovae.
      SN 2015as was as a core-collapse supernova: a cataclysmic explosion that happens when the core of a star far more massive than the Sun runs out of fuel and collapses under its own gravity, initiating a rebound of material outside the core. Hubble observations of SN 2015as will help researchers understand what happens when the expanding shockwave of a supernova collides with the gas that surrounds the exploded star.
      SN 2011ht might have been a core-collapse supernova as well, but it could also be an impostor called a luminous blue variable. Luminous blue variables are rare stars that experience eruptions so large that they can mimic supernovae. Crucially, luminous blue variables emerge from these eruptions unscathed, while stars that go supernova do not. Hubble will search for a stellar survivor at SN 2011ht’s location with the goal of revealing the explosion’s origin.
      Facebook logo @NASAHubble @NASAHubble Instagram logo @NASAHubble Explore More

      The Death Throes of Stars


      Homing in on Cosmic Explosions

      Media Contact:
      Claire Andreoli (claire.andreoli@nasa.gov)
      NASA’s Goddard Space Flight Center, Greenbelt, MD
      Share








      Details
      Last Updated Feb 21, 2025 Editor Andrea Gianopoulos Location NASA Goddard Space Flight Center Related Terms
      Hubble Space Telescope Astrophysics Astrophysics Division Galaxies Goddard Space Flight Center Spiral Galaxies Stars Supernovae Keep Exploring Discover More Topics From NASA
      Hubble Space Telescope


      Since its 1990 launch, the Hubble Space Telescope has changed our fundamental understanding of the universe.


      Hubble’s Night Sky Challenge



      Hubble’s Galaxies



      Reshaping Our Cosmic View: Hubble Science Highlights


      View the full article
  • Check out these Videos

×
×
  • Create New...