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40 Years Ago: STS-41B, the First Flight of the Manned Maneuvering Unit


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On Feb. 3, 1984, space shuttle Challenger took off on its fourth flight, STS-41B. Its five-person crew of Commander Vance D. Brand, Pilot Robert L. “Hoot” Gibson, and Mission Specialists Ronald E. McNair, Robert L. Stewart, and Bruce McCandless flew an eight-day mission ending with the first return to NASA’s Kennedy Space Center (KSC) in Florida. Many of the flight activities practiced tasks required for the upcoming Solar Maximum Mission satellite retrieval and repair mission. Among these, successful test flights of the Manned Maneuvering Unit (MMU) astronaut propulsion device during two untethered spacewalks proved the most critical, and visually spectacular. The two commercial communications satellites, Westar VI and Palapa-B2, successfully deployed during the mission ended up in non-operational orbits due to upper stage failures.

The STS-41B crew of Commander Vance D. Brand, Mission Specialists Robert L. Stewart, Ronald E. McNair, and Bruce McCandless, and Pilot Robert L. “Hoot” Gibson The STS-41B crew patch Challenger’s payload bay for STS-41B
Left: The STS-41B crew of (clockwise from bottom left) Commander Vance D. Brand, Mission Specialists Robert L. Stewart, Ronald E. McNair, and Bruce McCandless, and Pilot Robert L. “Hoot” Gibson. Middle: The STS-41B crew patch. Right: Challenger’s payload bay for STS-41B.

On Feb. 4, 1983, NASA announced Brand, Gibson, McNair, Stewart, and McCandless as the STS-11 crew. Brand, the flight’s only veteran, had flown on the Apollo-Soyuz Test Project in 1975 and commanded STS-5 in 1982. For the other four, STS-41B represented their first trip into space, although McCandless had served as an astronaut since his selection in 1966. He helped to develop the MMU and as a backup crew member for the Skylab 2 mission in 1973, he helped train astronauts to fly the Astronaut Maneuvering Unit, the MMU’s predecessor, inside Skylab. Gibson, McNair, and Stewart joined NASA as astronauts in 1978. At the time of the crew announcement, the seven-day mission’s objectives included the Large Format Camera for Earth photography, deploying the Palapa-B2 communications satellite for Indonesia, and the Payload Deployment and Retrieval System (PDRS) to test the Canadian-built Remote Manipulator System (RMS), or robotic arm. Over the course of the next year, both the mission’s designation and its payload complement changed due to a shuffling of payloads among shuttle flights. The PDRS moved up to STS-8, replaced by the Westar VI communications satellite for Western Union. In addition to the two spacewalks by McCandless and Stewart to test the MMU, the mission, re-designated STS-41B in September 1983, now included the Shuttle Pallet Satellite-01A (SPAS-01A), a reflight of the German-built deployable satellite flown on STS-7 in June 1983. The mission also included practicing rendezvous maneuvers with the Integrated Rendezvous Target (IRT), an inflatable 6-foot balloon deployed from the payload bay. During their spacewalks, McCandless and Stewart planned to perform the first tests of the Manipulator Foot Restraint (MFR), a work platform attached to the end of the RMS.

Aerial view at NASA’s Kennedy Space Center (KSC) in Florida of the Vehicle Assembly Building (VAB) and the Shuttle Landing Facility, where STS-41B made the first landing of the program Workers in the VAB prepare to lift space shuttle Challenger to mate it with its External Tank and twin Solid Rocket Boosters The STS-41B crew arrives at KSC three days before launch
Left: Aerial view at NASA’s Kennedy Space Center (KSC) in Florida of the Vehicle Assembly Building (VAB) and the Shuttle Landing Facility, where STS-41B made the first landing of the program. Middle: Workers in the VAB prepare to lift space shuttle Challenger to mate it with its External Tank and twin Solid Rocket Boosters. Right: The STS-41B crew arrives at KSC three days before launch.

After its previous mission, STS-8, Challenger arrived at KSC on Sept. 9, 1983, and workers towed it to the Orbiter Processing Facility to refurbish it for STS-41B. They replaced the orbiter’s three Auxiliary Power Units following a fire during Columbia’s landing on STS-9. They towed Challenger to the Vehicle Assembly Building on Jan. 6, 1984, for mating with its External Tank and twin Solid Rocket Boosters, and rolled the completed stack to Launch Pad 39A six days later. The astronauts participated in the Terminal Countdown Demonstration Test, a dress rehearsal for the actual countdown, on Jan. 16, and senior managers held the Flight Readiness Review on Jan. 25 to confirm the Feb. 3 launch date. Engineers began the countdown on Jan. 31, the same day the crew arrived at KSC.

Liftoff of space shuttle Challenger on the STS-41B mission Congressman C. William “Bill” Nelson, left, of Florida cheers on the STS-41B launch Challenger rises into the sky
Left: Liftoff of space shuttle Challenger on the STS-41B mission. Middle: Congressman C. William “Bill” Nelson, left, of Florida cheers on the STS-41B launch. Right: Challenger rises into the sky.

Liftoff occurred on schedule at 8:00 a.m. EST, with Challenger taking its five-member crew into the skies. Among the guests on hand to view the launch, Florida Congressman C. William “Bill” Nelson, who two years later flew on Columbia’s STS-61C mission, and in 2021 became NASA’s 14th administrator. Nine minutes after liftoff, Challenger’s three main engines cut off. The astronauts had reached space and experienced weightlessness for the first time, although they had not yet achieved orbit. The shuttle’s two Orbital Maneuvering System engines fired twice to complete the insertion into a circular 190-mile-high orbit.

Astronauts Ronald E. McNair, left, and Robert L. Stewart minutes after Challenger reached orbit Deploy of the Westar VI communications satellite for Western Union Deploy of the Palapa-B2 communications satellite for Indonesia
Left: Astronauts Ronald E. McNair, left, and Robert L. Stewart minutes after Challenger reached orbit. Middle: Deploy of the Westar VI communications satellite for Western Union. Right: Deploy of the Palapa-B2 communications satellite for Indonesia.

Once in orbit, the astronauts opened Challenger’s payload bay doors, deployed the Ku-band high-gain antenna to communicate with the Tracking and Data Relay Satellite, and closed the protective sunshields around the two satellites at the back of the payload bay. They tested the cameras in the payload bay and found that the one on the forward bulkhead’s starboard side did not tilt and panned only slowly, and only provided black and white imagery. Approximately eight hours into their first day, after opening its sunshield, the astronauts deployed the Westar VI communications satellite. Although the deployment went perfectly, 45 minutes later when the satellite’s Payload Assist Module-D (PAM-D) upper stage ignited to send it to geosynchronous transfer orbit, it fired for only a few seconds, stranding the satellite in a low, elliptical, and operationally useless orbit. Mission managers decided to delay the deployment of the Palapa satellite from the mission’s second day to the fourth day since it used an identical PAM-D upper stage. This provided engineers time to determine the cause of the first PAM-D failure. In place of the delayed deployment, the astronauts began several of the mission’s experiments, including activating the SPAS, and performed an initial checkout of the spacesuits. The third flight day included two retrograde OMS burns to lower Challenger’s orbit to a circular 173-mile-high orbit, and had planned to include the rendezvous operations with the IRT. However, shortly after its deployment from the payload bay, the balloon initially failed to inflate and then exploded, leaving no suitable target for a rendezvous. Using the shuttle’s radar and star trackers, the astronauts tracked the remains of the balloon to a distance of about 63 miles before abandoning the activity. In place of the IRT rendezvous, the crew checked out the RMS, with McNair at the controls.

The Shuttle Pallet Satellite-01A (SPAS-01A) in Challenger’s payload bay Robert L. Stewart wears the launch entry helmet during a prebreathe activity prior to a spacewalk
Left: The Shuttle Pallet Satellite-01A (SPAS-01A) in Challenger’s payload bay. Right: Robert L. Stewart wears the launch entry helmet during a prebreathe activity prior to a spacewalk.

The morning of flight day four, the astronauts decreased the shuttle’s cabin pressure from 14.7 pounds per square inch (psi) to 10.2 psi. This reduced the time the two spacewalkers needed to prebreathe pure oxygen to rid their blood of excess nitrogen that could result in the bends when working in their spacesuits at 4.3 psi. The astronauts deployed the Palapa satellite, and oriented the orbiter so that cameras on the RMS could observe the firing of the PAM-D engine. The burn initially appeared to go as planned, but engineers later determined that this engine suffered the same failure as the Westar PAM-D, similarly stranding Palapa in a low, elliptical, and operationally useless orbit. As a footnote, spacewalking astronauts flying MMUs retrieved both satellites during the STS-51A mission in November 1984 and returned them to Earth for reflight.

View of Bruce McCandless during the first test flight of the Manned Maneuvering Unit View of Bruce McCandless during the first test flight of the Manned Maneuvering Unit View of Bruce McCandless during the first test flight of the Manned Maneuvering Unit View of Challenger from McCandless’ vantage point
Views of Bruce McCandless during the first test flight of the Manned Maneuvering Unit, and a view, right, of Challenger from McCandless’ vantage point.

On flight day five, McCandless and Stewart began the second spacewalk of the shuttle program. After opening the airlock hatch, McCandless checked out the MMUs, donning the port side unit, designated with a number “3,” while Stewart prepared the Trunnion Pin Attachment Device (TPAD) and the MFR for use later in the spacewalk. As he began his first test flight in the MMU, McCandless said, “that may have been one small step for Neil, but it’s a heck of a big leap for me,” humorously echoing Apollo 11 astronaut Neil A. Armstrong’s first words after stepping onto the lunar surface. As an historical footnote, McCandless has served as capsule communicator during Armstrong’s historic Moonwalk. Floating just outside the flight deck aft windows, McCandless checked out the MMU’s flying in all three axes. He next translated down the length of the payload bay before beginning his long-distance travel. He flew 150 feet away from the orbiter, with a helmet mounted camera showing the receding shuttle, returned to the spacecraft, then backed out again to 320 feet before returning to the payload bay and stowing the MMU. With McNair operating the RMS, Stewart attached the MFR to the arm’s end effector. With the astronauts running slightly behind schedule, Mission Control decided to skip Stewart’s checkout of the MFR so he could proceed to his checkout of the MMU, the same unit McCandless just finished flying. McNair maneuvered McCandless in the MFR to the the SPAS to practice activities required for the Solar Max repair mission. Meanwhile Stewart began his test of the MMU, flying out to 150 feet, stopping, flying out to 300 feet, and returning to the payload bay. Once there, he attached the TPAD to the front of the MMU and practiced docking to the trunnion pin attached to the SPAS. He then returned the MMU to its stowage location. The two astronauts ended the spacewalk after 5 hours 55 minutes.

View in Mission Control at NASA’s Johnson Space Center in Houston during the first STS-41B spacewalk
View in Mission Control at NASA’s Johnson Space Center in Houston during the first STS-41B spacewalk as Bruce McCandless makes the first flight of the Manned Maneuvering Unit.

View of Bruce McCandless testing the Manipulator Foot Restraint at the end of the Remote Manipulator System, operated by Ronald E. McNair View of Bruce McCandless testing the Manipulator Foot Restraint at the end of the Remote Manipulator System, operated by Ronald E. McNair View of Bruce McCandless testing the Manipulator Foot Restraint at the end of the Remote Manipulator System, operated by Ronald E. McNair
Three views of Bruce McCandless testing the Manipulator Foot Restraint at the end of the Remote Manipulator System, operated by Ronald E. McNair.

Robert L. Stewart begins his first test flight of the Manned Maneuvering Unit (MMU) Stewart during his flight away from the payload bay Bruce McCandless prepares to dock his MMU with the attached Trunnion Pin Attachment Device to the SPAS-01A in Challenger’s payload bay
Left: Robert L. Stewart begins his first test flight of the Manned Maneuvering Unit (MMU). Middle: Stewart during his flight away from the payload bay. Right: Bruce McCandless prepares to dock his MMU with the attached Trunnion Pin Attachment Device to the SPAS-01A in Challenger’s payload bay.

Astronaut Ronald E. McNair poses with the camera for the Cinema 360 project, wearing a humorous “Cecil B. McNair” name tag, sunglasses, and beret McNair plays the soprano saxophone while floating in the middeck
Left: Astronaut Ronald E. McNair poses with the camera for the Cinema 360 project, wearing a humorous “Cecil B. McNair” name tag, sunglasses, and beret. Right: McNair plays the soprano saxophone while floating in the middeck.

On flight day six, McCandless and Stewart busied themselves with cleaning and recharging their spacesuits for the next day’s second spacewalk. McNair, an accomplished saxophonist, took some free time to play an instrument he brought along, the first musical instrument played on the shuttle. Space limitations in the shuttle precluded McNair flying his favorite tenor sax, so he learned to play the smaller soprano version of the instrument. McNair encountered unexpected effects of weightlessness on his playing. The water that normally accumulates inside wind instruments on Earth resulted instead in unwanted “bubbly” effects. The shuttle cabin’s dry air had unplanned effects on the instrument’s felt and leather pads, requiring several minutes of “rehydration” before proper playing. The reduced cabin atmospheric pressure for the spacewalks also required special reeds and mode of playing. Another historic event on this day, the Soviet Union launched a trio of cosmonauts to their Salyut-7 space station, bringing the total number of people in space to a then record-setting eight. This prompted one of the astronauts to comment, “It’s really getting to be populated up here.”

Bruce McCandless flies the Manned Maneuvering Unit (MMU) above Challenger’s payload bay during the second spacewalk McCandless grabs the Manipulator Foot Restraint that had floated away Robert L. Stewart flies the MMU above Challenger’s payload bay
Left: Bruce McCandless flies the Manned Maneuvering Unit (MMU) above Challenger’s payload bay during the second spacewalk. Middle: McCandless grabs the Manipulator Foot Restraint that had floated away. Right: Robert L. Stewart flies the MMU above Challenger’s payload bay.

On the seventh flight day, when Gibson began to operate the RMS, it did not respond as expected due to a failure in its wrist joint, and Mission Control requested that he stow it. Without the RMS, McCandless and Stewart could not practice docking with a slowly rotating SPAS, a critical test for the Solar Max mission. Instead, they practiced docking with the satellite berthed in the payload bay. McCandless placed himself in the starboard MMU, designated with a “2,” attached the TPAD, and practiced dockings before returning the MMU to its stowage location. Meanwhile, Stewart recharged the port MMU’s nitrogen tanks and took flight to practice dockings with the TPAD to the SPAS. He then returned the MMU to its portside location. At one point during the spacewalk, the MFR got loose and began drifting away. In an impromptu demonstration of rescuing an untethered astronaut, Brand maneuvered the orbiter so McCandless could retrieve it. McCandless donned the portside MMU to conduct evaluations of its automatic attitude hold and translation and rotational acceleration capabilities. In the meantime, Stewart practiced a hydrazine transfer operation using red-dyed freon as a substitute for the hazardous fuel. President Ronald W. Reagan called the astronauts during the spacewalk to congratulate them. McCandless returned the MMU to the port station while Stewart put away the fuel transfer equipment and tools. They climbed back into the airlock to close out the 6-hour 17-minute spacewalk, the longest of the shuttle program up to that time. Shortly after, the astronauts removed their spacesuits, exited the airlock, and repressurized Challenger’s cabin to 14.7 psi.

The STS-41B crew members pose near the end of their successful mission, in the middeck The STS-41B crew members pose near the end of their successful mission on the flight deck
The STS-41B crew members pose near the end of their successful mission, in the middeck, left, and on the flight deck, right.

On flight day eight, the day before entry, the astronauts busied themselves with stowing equipment. Brand and Gibson tested Challenger’s reaction control system thrusters and flight control surfaces in preparation for the next day’s landing. They held a 30-minute press conference with reporters on the ground asking them questions about their mission, with special emphasis on the historic spacewalks.

The astronauts close the payload bay doors at the end of the STS-41B mission Orange glow outside the windows during Challenger’s reentry A chase plane photographs Challenger during its descent to NASA’s Kennedy Space Center in Florida
Left: The astronauts close the payload bay doors at the end of the STS-41B mission. Middle: Orange glow outside the windows during Challenger’s reentry. Right: A chase plane photographs Challenger during its descent to NASA’s Kennedy Space Center in Florida.

Space shuttle Challenger touches down on the Shuttle Landing Facility at NASA’s Kennedy Space Center in Florida
Space shuttle Challenger touches down on the Shuttle Landing Facility at NASA’s Kennedy Space Center in Florida.

Space shuttle Challenger rolls down the Shuttle Landing Facility (SLF) at NASA’s Kennedy Space Center (KSC) in Florida STS-41B astronauts depart space shuttle Challenger at the SLF A welcome home ceremony for the STS-41B crew at the KSC Visitor Center
Left: Space shuttle Challenger rolls down the Shuttle Landing Facility (SLF) at NASA’s Kennedy Space Center (KSC) in Florida. Middle: STS-41B astronauts depart space shuttle Challenger at the SLF. Right: A welcome home ceremony for the STS-41B crew at the KSC Visitor Center.

On entry day, Feb. 11, the astronauts opened the two sunshields that protected the two satellites before their deployments, retracted and stowed the Ku antenna, and closed the payload bay doors. Brand and Gibson oriented Challenger with its tail in the direction of flight and fired its two OMS engines to slow the spacecraft enough to drop it out of orbit. They reoriented the orbiter to fly with its heat shield exposed to the direction of flight as it entered Earth’s atmosphere. The buildup of ionized gases caused by the heat of reentry prevented communications for about 15 minutes. The shuttle’s reentry path took it over the U.S. Gulf coast as it traveled toward the Shuttle Landing Facility at KSC. At an altitude of 110,000 feet and traveling at Mach 4.3, Challenger crossed Florida’s west coast, carrying out roll reversal maneuvers to reduce its speed. As the shuttle went subsonic, it made its final turn onto the KSC runway. Gibson lowered Challenger’s landing gear and Brand brought the shuttle down for its first landing at KSC, just a few miles from where it launched 7 days 23 hours 16 minutes earlier.

Enjoy the crew narrated video of the STS-41B mission. Read Brand’s and Gibson’s recollections of the STS-41B mission in their oral histories with the JSC History Office.

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      The 13th flight of the space shuttle program and the sixth of Challenger, STS-41G holds many distinctions. As the first mission focused almost entirely on studying the Earth, it deployed a satellite, employed multiple instruments, cameras, and crew observations to accomplish those goals. The STS-41G crew set several firsts, most notably as the first seven-member space crew. Other milestones included the first astronaut to make a fourth shuttle flight, the first and only astronaut to fly on Challenger three times and on back-to-back missions on any orbiter, the first crew to include two women, the first American woman to make two spaceflights, the first American woman to conduct a spacewalk, and the first Canadian and the first Australian-born American to make spaceflights.

      Left: The STS-41G crew patch. Right: The STS-41G crew of Jon A. McBride, front row left, Sally K. Ride, Kathryn D. Sullivan, and David C. Leestma; Paul D. Scully-Power, back row left, Robert L. Crippen, and Marc Garneau of Canada.
      In November 1983, NASA named the five-person crew for STS-41G, formerly known as STS-17, then planned as a 10-day mission aboard Columbia in August 1984. When assigned to STS-41G, Commander Robert L. Crippen had already completed two missions, STS-1 and STS-7, and planned to command STS-41C in April 1984. On STS-41G, he made a record-setting fourth flight on a space shuttle, and as it turned out the first and only person to fly aboard Challenger three times, including back-to-back missions. Pilot Jon A. McBride, and mission specialists Kathryn D. Sullivan from the Class of 1978 and, David C. Leestma from the Class of 1980, made their first flights into space. Mission specialist Sally K. Ride made her second flight, and holds the distinction as the first American woman to return to space, having flown with Crippen on STS-7. The flight marked the first time that two women, Ride and Sullivan, flew in space at the same time. In addition, Sullivan holds the honor as the first American woman to conduct a spacewalk and made her second flight and holds the distinction as the first American woman to return to space, having flown with Crippen on STS-7. The flight marked the first time that two women, Ride and Sullivan, flew in space at the same time. In addition, Sullivan holds the honor as the first American woman to conduct a spacewalk, and Leestma as the first of the astronaut Class of 1980 to make a spaceflight.
      Columbia’s refurbishment following STS-9 ran behind schedule and could not meet the August launch date, so NASA switched STS-41G to the roomier and lighter weight Challenger. This enabled adding crew members to the flight. In February 1984, NASA and the Canadian government agreed to fly a Canadian on an upcoming mission in recognition for that country’s major contribution to the shuttle program, the Remote Manipulator System (RMS), or robotic arm. In March, Canada named Marc Garneau as the prime crewmember with Robert B. Thirsk as his backup. NASA first assigned Garneau to STS-51A, but with the switch to Challenger transferred him to the STS-41G crew. On June 1, NASA added Australian-born and naturalized U.S. citizen Paul D. Scully-Power, an oceanographer with the Naval Research Laboratory who had trained shuttle crews in recognizing ocean phenomena from space, to the mission rounding out the seven-person crew, the largest flown to that time. Scully-Power has the distinction as the first person to launch into space sporting a beard.

      Left: Space shuttle Challenger returns to NASA’s Kennedy Space Center (KSC) in Florida atop a Shuttle Carrier Aircraft following the STS-41C mission. Middle: The Earth Resources Budget Satellite during processing at KSC for STS-41G. Right: Technicians at KSC process the Shuttle Imaging Radar-B for the STS-41G mission.
      The STS 41G mission carried a suite of instruments to study the Earth. The Earth Radiation Budget Satellite (ERBS), managed by NASA’s Goddard Space Flight Center in Greenbelt, Maryland, contained three instruments, including the Stratospheric Aerosol and Gas Experiment-2 (SAGE-2), to measure solar and thermal radiation of the Earth to better understand global climate changes. NASA’s Office of Space and Terrestrial Applications sponsored a cargo bay-mounted payload (OSTA-3) consisting of four instruments. The Shuttle Imaging Radar-B (SIR-B), managed by NASA’s Jet Propulsion Laboratory in Pasadena, California, and an updated version of SIR-A flown on STS-2, used synthetic aperture radar to support investigations in diverse disciplines such as archaeology, geology, cartography, oceanography, and vegetation studies. Making its first flight into space, the 900-pound Large Format Camera (LFC) took images of selected Earth targets on 9-by-18-inch film with 70-foot resolution. The Measurement of Air Pollution from Satellites (MAPS) experiment provided information about industrial pollutants in the atmosphere. The Feature Identification and Location Experiment (FILE) contained two television cameras to improve the efficiency of future remote sensing equipment. In an orbit inclined 57 degrees to the Equator, the instruments aboard Challenger could observe more than 75% of the Earth’s surface. 
      The Orbital Refueling System (ORS), managed by NASA’s Johnson Space Center in Houston, while not directly an Earth observation payload, assessed the feasibility of on-orbit refueling of the Landsat-4 remote sensing satellite, then under consideration as a mission in 1987, as well as Department of Defense satellites not designed for on-orbit refueling. In the demonstration, the astronauts remotely controlled the transfer of hydrazine, a highly toxic fuel, between two tanks mounted in the payload bay. During a spacewalk, two crew members simulated connecting the refueling system to a satellite and later tested the connection with another remotely controlled fuel transfer. Rounding out the payload activities, the large format IMAX camera made its third trip into space, with footage used to produce the film “The Dream is Alive.”

      Four views of the rollout of space shuttle Challenger for STS-41G. Left: From inside the Vehicle Assembly Building (VAB). Middle left: From Firing Room 2 of the Launch Control Center (LCC). Middle right: From the crawlerway, with the LCC and the VAB in the background. Right: From atop the VAB.

      Left: The STS-41G astronauts answer reporters’ questions at Launch Pad 39A during the Terminal Countdown Demonstration Test. Right: The STS-41G crew leaves crew quarters and prepares to board the Astrovan for the ride to Launch Pad 39A for liftoff.
      Following the STS-41C mission, Challenger returned to KSC from Edwards Air Force Base in California on April 18. Workers in KSC’s Orbiter Processing Facility refurbished the orbiter and changed out its payloads. Rollover to the Vehicle Assembly Building (VAB) took place on Sept. 8 and after workers stacked Challenger with its External Tank and Solid Rocket Boosters, they rolled it out of the VAB to Launch Pad 39A on Sept. 13. Just two days later, engineers completed the Terminal Countdown Demonstration Test, a final dress rehearsal before the actual countdown and launch, with the astronaut crew participating as on launch day. They returned to KSC on Oct. 2 to prepare for the launch three days later.

      Left: Liftoff of space shuttle Challenger on the STS-41G mission. Middle: Distant view of Challenger as it rises through the predawn skies. Right: The Earth Resources Budget Satellite just before the Remote Manipulator System released it.
      Space shuttle Challenger roared off Launch Pad 39A at 7:03 a.m. EDT, 15 minutes before sunrise, on Oct. 5, 1984, to begin the STS-41G mission. The launch took place just 30 days after the landing of the previous mission, STS-41D. That record-breaking turnaround time between shuttle flights did not last long, as the launch of Discovery on STS-51A just 26 days after Challenger’s landing set a new record on Nov. 8.
      Eight and a half minutes after liftoff, Challenger and its seven-member crew reached space and shortly thereafter settled into a 218-mile-high orbit, ideal for the deployment of the 5,087-pound ERBS. The crew noted that a 40-inch strip of Flexible Reusable Surface Insulation (FRSI) had come loose from Challenger’s right-hand Orbiter Maneuvering System (OMS) pod, presumably lost during launch. Mission Control determined that this would not have any impact during reentry. Ride grappled the ERBS with the shuttle’s RMS but when she commanded the satellite to deploy its solar arrays, nothing happened. Mission Control surmised that the hinges on the arrays had frozen, and after Ride oriented the satellite into direct sunlight and shook it slightly on the end of the arm, the panels deployed. She released ERBS about two and a half hours late and McBride fired Challenger’s steering jets to pull away from the satellite. Its onboard thrusters boosted ERBS into its operational 380-mile-high orbit. With an expected two-year lifetime, it actually operated until October 14, 2005, returning data about how the Earth’s atmosphere absorbs and re-radiates the Sun’s energy, contributing significant information about global climate change.

      Left: The SIR-B panel opens in Challenger’s payload bay. Right: Jon A. McBride with the IMAX large format camera in the middeck. 
      Near the end of their first day in space, the astronauts opened the panels of the SIR-B antenna and activated it, also deploying the Ku-band antenna that Challenger used to communicate with the Tracking and Data Relay System (TDRS) satellite. The SIR-B required a working Ku-band antenna to downlink the large volume of data it collected, although it could store a limited amount on onboard tape recorders. But after about two minutes, the data stream to the ground stopped. One of the two motors that steered the Ku antenna failed and it could no longer point to the TDRS satellite. Mission Control devised a workaround to fix the Ku antenna in one position and steer the orbiter to point it to the TDRS satellite and downlink the stored data to the ground. Challenger carried sufficient fuel for all the maneuvering, but the extra time for the attitude changes resulted in achieving only about 40% of the planned data takes. The discovery of the 3,000-year-old lost city of Udar in the desert of Oman resulted from SIR-B data, one of many interesting findings from the mission.

      Left: The shuttle’s Canadian-built Remote Manipulator System or robotic arm closes the SIR-B panel. Middle: The patch for Canadian astronaut Marc Garneau’s mission. Right: Spiral eddies in the eastern Mediterranean Sea.
      During the second mission day, the astronauts lowered Challenger’s orbit to an intermediate altitude of 151 miles. Flight rules required that the SIR-B antenna be stowed for such maneuvers but the latches to clamp the antenna closed failed to activate. Ride used the RMS to nudge the antenna panel closed. From the orbiter’s flight deck, Leestma successfully completed the first ORS remote-controlled hydrazine fuel transfer. Garneau began working on his ten CANEX investigations related to medical, atmospheric, climatic, materials and robotic sciences while Scully-Power initiated his oceanographic observations. Despite greater than expected global cloud cover, he successfully photographed spiral eddies in the world’s oceans, particularly notable in the eastern Mediterranean Sea.

      Left: Mission Specialists Kathryn D. Sullivan, left, and Sally K. Ride on Challenger’s flight deck. Right: Payload Specialists Marc Garneau and Paul D. Scully-Power working on a Canadian experiment in Challenger’s middeck.
      The third day saw the crew lower Challenger’s orbit to 140 miles, the optimal altitude for SIR-B and the other Earth observing instruments. For the next few days, all the experiments continued recording their data, including Garneau’s CANEX and Scully-Power’s oceanography studies. Leestma completed several scheduled ORS fuel transfers prior to the spacewalk. Preparations for that activity began on flight day 6 with the crew lowering the cabin pressure inside Challenger from the normal sea level 14.7 pounds per square inch (psi) to 10.2 psi. The lower pressure prevented the buildup of nitrogen bubbles in the bloodstreams of the two spacewalkers, Leestma and Sullivan, that could result in the development of the bends. The two verified the readiness of their spacesuits.

      Left: David C. Leestma, left with red stripes on his suit, and Kathryn D. Sullivan during their spacewalk. Middle: Leestma, left, and Sullivan working on the Orbital Refueling System during the spacewalk. Right: Sullivan, left, and Leestma peer into Challenger’s flight deck during the spacewalk.
      On flight day 7, Leestma and Sullivan, assisted by McBride, donned their spacesuits and began their spacewalk. After gathering their tools, the two translated down to the rear of the cargo bay to the ORS station. With Sullivan documenting and assisting with the activity, Leestma installed the valve assembly into the simulated Landsat propulsion plumbing. After completing the ORS objectives, Leestma and Sullivan proceeded back toward the airlock, stopping first at the Ku antenna where Sullivan secured it in place. They returned inside after a spacewalk that lasted 3 hours and 29 minutes, and the crew brought Challenger’s cabin pressure back up to 14.7 psi.

      STS-41G crew Earth observation photographs. Left: Hurricane Josephine in the Atlantic Ocean. Middle: The Strait of Gibraltar. Right: Karachi, Pakistan, and the mouth of the Indus River.

      False color image of Montreal generated from SIR-B data.

      Left: Traditional inflight photo of the STS-41G crew on Challenger’s flight deck. Right: Robert L. Crippen with the orange glow generated outside Challenger during reentry.

      Left: Kathryn D. Sullivan photograph of NASA’s Kennedy Space Center (KSC) in Florida during Challenger’s approach, minutes before touchdown. Middle: Space shuttle Challenger moments before touchdown at N KSC at the end of the STS-41G mission. Right: The crew of STS-41G descends from Challenger after completing a highly successful mission.
      During their final full day in space, Challenger’s crew tidied the cabin for reentry and completed the final SIR-B and other Earth observations. On Oct. 13, the astronauts closed the payload bay doors and fired the OMS engines over Australia to begin the descent back to Earth. Because of the mission’s 57-degree inclination, the reentry path took Challenger and its crew over the eastern United States, another Shuttle first. Crippen guided the orbiter to a smooth landing at KSC, completing a flight of 8 days, 5 hours, and 24 minutes, the longest mission of Challenger’s short career. The crew had traveled nearly 3.3 million miles and completed 133 orbits around the Earth.

      Left: Missing insulation from Challenger’s right hand Orbiter Maneuvering System pod as seen after landing. Middle: Missing tile from the underside of Challenger’s left wing. Right: Damage to tiles on Challenger’s left wing.
      As noted above, on the mission’s first day in space the crew described a missing strip of FRSI from the right-hand OMS pod. Engineers noted additional damage to Challenger’s Thermal Protection System (TPS) after the landing, including several tiles on the underside the vehicle’s left wing damaged and one tile missing entirely, presumably lost during reentry. Engineers determined that the water proofing used throughout the TPS that allowed debonding of the tiles as the culprit for the missing tile. To correct the problem, workers removed and replaced over 4,000 tiles, adding a new water proofing agent to preclude the recurrence of the problem on future missions.
      Read recollections of the STS-41G mission by Crippen, McBride, Sullivan, Ride, and Leestma in their oral histories with the JSC History Office. Enjoy the crew’s narration of a video about the STS-41G mission.
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      NASA’s Psyche spacecraft is depicted receiving a laser signal from the Deep Space Optical Communications uplink ground station at JPL’s Table Mountain Facility in this artist’s concept. The DSOC experiment consists of an uplink and downlink station, plus a flight laser transceiver flying with Psyche.NASA/JPL-Caltech The Deep Space Optical Communications tech demo has completed several key milestones, culminating in sending a signal to Mars’ farthest distance from Earth.
      NASA’s Deep Space Optical Communications technology demonstration broke yet another record for laser communications this summer by sending a laser signal from Earth to NASA’s Psyche spacecraft about 290 million miles (460 million kilometers) away. That’s the same distance between our planet and Mars when the two planets are farthest apart.
      Soon after reaching that milestone on July 29, the technology demonstration concluded the first phase of its operations since launching aboard Psyche on Oct. 13, 2023.
      “The milestone is significant. Laser communication requires a very high level of precision, and before we launched with Psyche, we didn’t know how much performance degradation we would see at our farthest distances,” said Meera Srinivasan, the project’s operations lead at NASA’s Jet Propulsion Laboratory in Southern California. “Now the techniques we use to track and point have been verified, confirming that optical communications can be a robust and transformative way to explore the solar system.”
      Managed by JPL, the Deep Space Optical Communications experiment consists of a flight laser transceiver and two ground stations. Caltech’s historic 200-inch (5-meter) aperture Hale Telescope at Caltech’s Palomar Observatory in San Diego County, California, acts as the downlink station to which the laser transceiver sends its data from deep space. The Optical Communications Telescope Laboratory at JPL’s Table Mountain facility near Wrightwood, California, acts as the uplink station, capable of transmitting 7 kilowatts of laser power to send data to the transceiver.
      This visualization shows Psyche’s position on July 29 when the uplink station for NASA’s Deep Space Optical Communications sent a laser signal about 290 million miles to the spacecraft. See an interactive version of the Psyche spacecraft in NASA’s Eyes on the Solar System.NASA/JPL-Caltech By transporting data at rates up to 100 times higher than radio frequencies, lasers can enable the transmission of complex scientific information as well as high-definition imagery and video, which are needed to support humanity’s next giant leap when astronauts travel to Mars and beyond.
      As for the spacecraft, Psyche remains healthy and stable, using ion propulsion to accelerate toward a metal-rich asteroid in the main asteroid belt between Mars and Jupiter.
      Exceeding Goals
      The technology demonstration’s data is sent to and from Psyche as bits encoded in near-infrared light, which has a higher frequency than radio waves. That higher frequency enables more data to be packed into a transmission, allowing far higher rates of data transfer.
      Even when Psyche was about 33 million miles (53 million kilometers) away — comparable to Mars’ closest approach to Earth — the technology demonstration could transmit data at the system’s maximum rate of 267 megabits per second. That bit rate is similar to broadband internet download speeds. As the spacecraft travels farther away, the rate at which it can send and receive data is reduced, as expected.
      On June 24, when Psyche was about 240 million miles (390 million kilometers) from Earth — more than 2½ times the distance between our planet and the Sun — the project achieved a sustained downlink data rate of 6.25 megabits per second, with a maximum rate of 8.3 megabits per second. While this rate is significantly lower than the experiment’s maximum, it is far higher than what a radio frequency communications system using comparable power can achieve over that distance.
      This Is a Test
      The goal of Deep Space Optical Communications is to demonstrate technology that can reliably transmit data at higher speeds than other space communication technologies like radio frequency systems. In seeking to achieve this goal, the project had an opportunity to test unique data sets like art and high-definition video along with engineering data from the Psyche spacecraft. For example, one downlink included digital versions of Arizona State University’s “Psyche Inspired” artwork, images of the team’s pets, and a 45-second ultra-high-definition video that spoofs television test patterns from the previous century and depicts scenes from Earth and space.
      This 45-second ultra-high-definition video was streamed via laser from deep space by NASA’s Deep Space Optical Communications technology demonstration on June 24, when the Psyche spacecraft was 240 million miles from Earth. NASA/JPL-Caltech The technology demonstration beamed the first ultra-high-definition video from space, featuring a cat named Taters, from the Psyche spacecraft to Earth on Dec. 11, 2023, from 19 million miles away. (Artwork, images, and videos were uploaded to Psyche and stored in its memory before launch.)
      “A key goal for the system was to prove that the data-rate reduction was proportional to the inverse square of distance,” said Abi Biswas, the technology demonstration’s project technologist at JPL. “We met that goal and transferred huge quantities of test data to and from the Psyche spacecraft via laser.” Almost 11 terabits of data have been downlinked during the first phase of the demo.
      The flight transceiver is powered down and will be powered back up on Nov. 4. That activity will prove that the flight hardware can operate for at least a year.
      “We’ll power on the flight laser transceiver and do a short checkout of its functionality,” said Ken Andrews, project flight operations lead at JPL. “Once that’s achieved, we can look forward to operating the transceiver at its full design capabilities during our post-conjunction phase that starts later in the year.”
      More About Deep Space Optical Communications
      This demonstration is the latest in a series of optical communication experiments funded by the Space Technology Mission Directorate’s Technology Demonstration Missions Program managed at NASA’s Marshall Space Flight Center in Huntsville, Alabama, and the agency’s SCaN (Space Communications and Navigation) program within the Space Operations Mission Directorate. Development of the flight laser transceiver is supported by MIT Lincoln Laboratory, L3 Harris, CACI, First Mode, and Controlled Dynamics Inc. Fibertek, Coherent, Caltech Optical Observatories, and Dotfast support the ground systems. Some of the technology was developed through NASA’s Small Business Innovation Research program.
      For more information about the laser communications demo, visit:
      https://www.jpl.nasa.gov/missions/dsoc
      NASA’s Optical Comms Demo Transmits Data Over 140 Million Miles The NASA Cat Video Explained 5 Things to Know About NASA’s Deep Space Optical Communications News Media Contacts
      Ian J. O’Neill
      Jet Propulsion Laboratory, Pasadena, Calif.
      818-354-2649
      ian.j.oneill@jpl.nasa.gov
      2024-130
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      Last Updated Oct 03, 2024 Related Terms
      Deep Space Optical Communications (DSOC) Jet Propulsion Laboratory Psyche Mission Space Communications & Navigation Program Space Operations Mission Directorate Space Technology Mission Directorate Tech Demo Missions Explore More
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