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The road to the Moon landing cleared a major hurdle in March 1969 with the flight of Apollo 9 that tested all components of the spacecraft in low Earth orbit. Astronauts James A. McDivitt and Russell L. Schweickart flew the Lunar Module (LM) Spider while David R. Scott awaited their return in the Command Module (CM) Gumdrop. The success of Apollo 9 paved the way for Apollo 10, the next mission planned for May, to test the combined spacecraft in lunar orbit. Preparations for Apollo 10 continued with the rollout of the Saturn V to its launch pad. And if that dress rehearsal mission completed all its objectives, Apollo 11 could achieve the first Moon landing in July. The astronauts for that mission continued their training as engineers tested the spacecraft and assembled the rocket.

Apollo 9

Apollo 9 astronauts James A. McDivitt, left, David R. Scott, and Russell L. Schweickart pose in front of their Saturn V rocket at NASA’s Kennedy Space Center in Florida The Apollo 9 crew patch Liftoff of Apollo 9
Left: Apollo 9 astronauts James A. McDivitt, left, David R. Scott, and Russell L. Schweickart pose in front of their Saturn V rocket at NASA’s Kennedy Space Center in Florida. Middle: The Apollo 9 crew patch. Right: Liftoff of Apollo 9!

At 11 a.m. on March 3, 1969, Apollo 9 lifted off from Launch Pad 39A at NASA’s Kennedy Space Center (KSC) in Florida. For only the second time, the giant Saturn V lifted three astronauts into space. Although planned for Feb. 28, managers delayed the liftoff by three days to give the astronauts time to recover from upper respiratory infections. The incident prompted NASA to institute a preflight medical quarantine for astronauts on future missions to minimize their risk of contracting infectious diseases.

In the Launch Control Center (LCC) at NASA’s Kennedy Space Center (KSC) in Florida, KSC Director Kurt H. Debus, left, gives a tour to Vice President Spiro T. Agnew as they await the launch of Apollo 9 Controllers in the LCC’s Firing Room 2 monitor Apollo 9’s countdown In Mission Control at the Manned Spacecraft Center, now NASA’s Johnson Space Center in Houston, Apollo 9 Lead Flight Director Eugene F. Kranz, seated, monitors the flight’s progress
Left: In the Launch Control Center (LCC) at NASA’s Kennedy Space Center (KSC) in Florida, KSC Director Kurt H. Debus, left, gives a tour to Vice President Spiro T. Agnew as they await the launch of Apollo 9. Middle: Controllers in the LCC’s Firing Room 2 monitor Apollo 9’s countdown. Right: In Mission Control at the Manned Spacecraft Center, now NASA’s Johnson Space Center in Houston, Apollo 9 Lead Flight Director Eugene F. Kranz, seated, monitors the flight’s progress.

Controllers in Firing Room 2 of the Launch Control Center (LCC) monitored Apollo 9’s smooth countdown. Vice President Spiro T. Agnew, who chaired the National Aeronautics and Space Council, attended the launch, escorted by NASA Acting Administrator Thomas O. Paine and KSC Director Kurt H. Debus. As soon as the Saturn V cleared the launch tower, control of the flight switched from the LCC to Mission Control at the Manned Spacecraft Center (MSC), now NASA’s Johnson Space Center in Houston. Apollo 9 Lead Flight Director Eugene F. Kranz and his team of controllers monitored the launch. Eleven minutes after liftoff, the Saturn V’s three stages placed Apollo 9 in orbit around the Earth. During the 10-day mission, Flight Directors Gerald D. Griffin and M.P. “Pete” Frank took their turns along with Kranz leading their teams to monitor the flight.

The Lunar Module Spider still attached to the Saturn V rocket’s S-IVB third stage Apollo 9 astronaut Russell L. Schweickart on Spider’s front porch during the mission’s dual spacewalk – note fellow astronaut David R. Scott reflected in Schweickart’s visor Scott in the open hatch of the Command Module Gumdrop
Left: The Lunar Module Spider still attached to the Saturn V rocket’s S-IVB third stage. Middle: Apollo 9 astronaut Russell L. Schweickart on Spider’s front porch during the mission’s dual spacewalk – note fellow astronaut David R. Scott reflected in Schweickart’s visor. Right: Scott in the open hatch of the Command Module Gumdrop.

Two hours and 41 minutes after launch, the Command and Service Module (CSM) separated from the S-IVB third stage and pulled a safe distance away to begin the Transposition and Docking maneuver. Scott turned Gumdrop around to face Spider, still attached to the S-IVB, and slowly closed the gap between the two spacecraft, completing the first successful docking of the Apollo program. About an hour later, springs ejected the docked spacecraft from the S-IVB. Over the next few hours, ground controllers twice restarted the S-IVB’s engine to simulate a Trans Lunar Injection, eventually sending the spent rocket stage into solar orbit. Meanwhile, the astronauts pressurized the tunnel between Gumdrop and Spider and connected umbilicals to power the LM while the two spacecraft remained docked. The astronauts next performed the first of eight planned burns of the Service Module’s (SM) Service Propulsion System (SPS) engine, a five-second maneuver that raised the spacecraft’s orbit. The burn validated that the docking mechanism between the two vehicles and that the LM itself could withstand the firing of the large SPS engine. The crew settled down for their first night’s sleep in space – for the first time in the Apollo Program, all crew members slept at the same time and not in shifts as on previous missions. The next day, the crew conducted three SPS engine burns of varying durations to demonstrate the controllability of the docked vehicles using the spacecraft’s digital autopilot.

The third day saw the initial activation of the LM Spider. Schweickart first and then McDivitt floated through the tunnel from Gumdrop. They closed the hatch, brought the LM’s systems to life, and extended the vehicle’s four landing legs. McDivitt informed Mission Control that Schweickart had experienced symptoms of space motion sickness, including vomiting twice, but that he now felt better.  Mission Control, in consultation with flight surgeons and the crew, agreed that the mission could continue as planned, but out of an abundance of caution they curtailed the spacewalk scheduled for the next day. Instead of translating to Gumdrop and back as originally planned, Schweickart would remain on Spider’s front porch to evaluate the spacesuit and the Portable Life Support System (PLSS) backpack. Schweickart and McDivitt then began the first TV transmission of the mission, a seven-minute broadcast showing the duo in the confined space of the LM.

McDivitt and Schweickart moved on to perform the first test of the Descent Propulsion System (DPS) engine, the rocket used to land the LM on the Moon. Although successfully tested during the uncrewed Apollo 5 mission in January 1968, this test included a CSM docked to the LM. The burn evaluated if the LM’s engine could serve as a backup in case of a problem with the SPS – in retrospect a very useful test given Apollo 13 relied on the method just over a year later. After the 372-second burn, capsule communicator (capcom) Stuart A. Roosa called up to the crew, “Spider, that was a beautiful burn, man, you were right down the tube,” generating this response from McDivitt, “Looked pretty neat from here, too.” McDivitt and Schweickart deactivated Spider for the night and transferred back to Gumdrop. The crew conducted the 43-second fifth burn of the SPS to circularize the spacecraft’s orbit.

The Apollo 9 astronauts began their fourth day in space by donning their spacesuits and Schweicakrt and McDivitt once again transferred to Spider. In the LM, Schweickart, fully recovered from his earlier illness, donned the PLSS that provided him with oxygen during his spacewalk. Scott received his life support via umbilicals connected to the CM and McDivitt similarly used the LM’s life support system.  McDivitt depressurized Spider, and minutes later Scott did the same with Gumdrop. Schweickart floated out through the LM’s side hatch onto the front porch, exclaiming “Hey, this is like spectacular.” He placed his feet into specialized gold-painted foot restraints dubbed the “golden slippers.” Scott then opened the CM side hatch and floated partway out of the spacecraft. Mission Control now communicated with three different parties, with Schweickart picking up the callsign Red Rover, a nod to his red hair. Scott retrieved thermal samples from the outside of Gumdrop. Schweickart did the same from the outside of Spider and tested out the handrails near the hatch and found them to be easy for maneuvering. Scott and Schweickart reentered their respective vehicles, having each spent about 37 minutes outside. Mission Control considered this first, and the only one before the Moon landing, test of the spacesuits and PLSS a complete success. After a 15-minute TV broadcast, McDivitt and Schweickart returned to Gumdrop to rejoin Scott for the night.

The Lunar Module (LM) Spider with James A. McDivitt and Russell L. Schweickart aboard, begins its departure from the Command Module (CM) Gumdrop, with David R. Scott aboard McDivitt and Schweickart aboard Spider’s ascent stage have returned to Gumdrop View of Gumdrop from Spider
Left: The Lunar Module (LM) Spider with James A. McDivitt and Russell L. Schweickart aboard, begins its departure from the Command Module (CM) Gumdrop, with David R. Scott aboard. Middle: McDivitt and Schweickart aboard Spider’s ascent stage have returned to Gumdrop. Right: View of Gumdrop from Spider.

For their fifth day in space, the Apollo 9 crew had a full plate – undocking of Spider from Gumdrop, testing the LM’s Descent and Ascent Stage engines by conducting separation maneuvers followed by a rendezvous and docking with the CM. This marked the first time astronauts flew in a spacecraft not designed to reenter the Earth’s atmosphere, making redocking with Gumdrop essential. Spider backed away from Gumdrop to about 50 feet and began a slow turn so Scott in the CM could inspect it. He commented about Spider, “That’s a nice looking machine.” A small 10-second burn by the SM’s Reaction Control System (RCS) thrusters increased the separation distance to about three miles. About 45 minutes after undocking, McDivitt fired Spider’s DPS engine for 19 seconds, first at 10% thrust then throttling it up to 40% thrust, to begin the separation maneuver that placed it about 50 miles from Gumdrop before orbital mechanics brought the two spacecraft closer again. The next maneuver in the separation sequence, a 22-second DPS burn, opened the distance to about 100 miles. 

To begin the rendezvous back to Gumdrop, McDivitt first fired Spider’s Ascent Stage RCS thrusters for 32 seconds, at the same time jettisoning the Descent Stage. It remained in orbit until March 22, burning up on reentry over the Indian Ocean. The next rendezvous maneuver, lasting three seconds, tested the Ascent Propulsion System (APS) engine for the first time, followed by a second APS burn lasting 38 seconds, putting Spider on an intercept course with Gumdrop. Two small course corrections refined the trajectory and Spider stopped about 100 feet from Gumdrop to begin a pitchover maneuver, allowing Scott to inspect the ascent stage including its engine, commenting, “You’re the biggest, friendliest, funniest looking Spider I’ve ever seen.” The two craft docked, having flown separately for six hours 23 minutes. Two hours after docking, McDivitt and Schweickart rejoined Scott in Gumdrop, and then they jettisoned Spider. Mission Control commanded Spider’s APS to fire for six minutes, placing it into a highly elliptical Earth orbit from which it did not decay until Oct. 23, 1981. The Apollo 9 astronauts had met their mission’s primary objectives, and they still had five more days in space.

Experiment S065 multispectral camera installed on the Command Module’s side hatch window Multispectral image of the San Diego area Color infrared image of the Salton Sea area in California
Left: Experiment S065 multispectral camera installed on the Command Module’s side hatch window. Middle: Multispectral image of the San Diego area. Right: Color infrared image of the Salton Sea area in California.

The first major task of flight day six involved the sixth SPS engine. This brief one and a half second burn lowered the low point of Gumdrop’s orbit, to enhance a backup capability to use the RCS thrusters for the deorbit burn at the end of the mission, should a problem arise with the SPS. Shortly after this burn, the crew set up the one formal scientific investigation of their mission – Experiment S065 Multispectral Terrain Photography, a cluster of four Hasselblad 70 mm cameras mounted in Gumdrop’s round hatch window. The experiment provided photographs taken simultaneously in four specific portions of the visible and near infrared spectrum. The experiment served as a precursor for the Earth Resources Technology Satellite (ERTS), later renamed Landsat, and for multispectral photography conducted aboard the Skylab space station in the early 1970s. Over the next four days, the astronauts continued observations with the S065 camera system, exposing 127 complete four-frame sets.

The Apollo 9 Command Module Gumdrop descends on its three main parachutes just moments before touchdown Minutes after splashdown, the rescue helicopter from the U.S.S. Guadalcanal prepares to drop swimmers into the water to safe the capsule and retrieve the astronauts Apollo 9 astronauts Russell L. Schweickart, left, David R. Scott, and James A. McDivitt safely aboard the Guadalcanal
Left: The Apollo 9 Command Module Gumdrop descends on its three main parachutes just moments before touchdown. Middle: Minutes after splashdown, the rescue helicopter from the U.S.S. Guadalcanal prepares to drop swimmers into the water to safe the capsule and retrieve the astronauts. Right: Apollo 9 astronauts Russell L. Schweickart, left, David R. Scott, and James A. McDivitt safely aboard the Guadalcanal.

On flight day eight, the crew completed the seventh SPS burn, a 25-second firing to establish the proper trajectory for the deorbit burn. On Mar. 13, 1969, after 151 revolutions around the Earth and while passing over Hawaii, the crew fired the SPS engine for the eighth and final time. Lasting just under 12 seconds, the burn brought Apollo 9 out of orbit. Gumdrop separated from its SM and pointed its heat shield in the direction of flight. During reentry, a sheath of ionized gas formed around the capsule by the rapid deceleration led to a 4-minute radio blackout, after which the drogue parachutes deployed. The three main parachutes opened at 10,000 feet altitude, slowing the spacecraft to about 22 miles per hour at splashdown.

The Apollo 9 astronauts, in white overalls, on the elevator deck of the U.S.S. Guadalcanal, with the Mobile Quarantine Facility (MQF) visible in the background The Apollo 9 astronauts, wearing blue baseball caps, peer into the window of the MQF and greet the occupants Apollo 9 astronauts Russell L. Schweickart, left, David R. Scott, and James A. McDivitt prepare to cut the cake in their honor aboard the Guadalcanal
Left: The Apollo 9 astronauts, in white overalls, on the elevator deck of the U.S.S. Guadalcanal, with the Mobile Quarantine Facility (MQF) visible in the background. Middle: The Apollo 9 astronauts, wearing blue baseball caps, peer into the window of the MQF and greet the occupants. Right: Apollo 9 astronauts Russell L. Schweickart, left, David R. Scott, and James A. McDivitt prepare to cut the cake in their honor aboard the Guadalcanal.

Apollo 9 astronauts’ return trip from the U.S.S. Guadalcanal to Houston. Carrying flowers after a stopover on Eleuthera in The Bahamas. Apollo 9 astronauts’ return trip from the U.S.S. Guadalcanal to Houston. A brief layover at NASA’s Kennedy Space Center in Florida Apollo 9 astronauts’ return trip from the U.S.S. Guadalcanal to Houston. Arriving at Ellington Air Force Base in Houston
The Apollo 9 astronauts’ return trip from the U.S.S. Guadalcanal to Houston. Left: Carrying flowers after a stopover on Eleuthera in The Bahamas. Middle: A brief layover at NASA’s Kennedy Space Center in Florida. Right: Arriving at Ellington Air Force Base in Houston.

The splashdown occurred in the Atlantic Ocean about 670 miles south-southwest of Bermuda, and about 3 miles from the prime recovery ship the U.S.S. Guadalcanal (LPH-7). McDivitt, Scott, and Schweickart had spent 241 hours and 54 seconds in space. Forty-nine minutes after splashdown, recovery teams had the crew aboard the recovery ship. The next day, a helicopter flew them to Eleuthera in the Bahamas, where they boarded a plane to KSC for a brief ceremony, and then back to Houston for a large welcome home reception and a reunion with their families at Ellington Air Force Base. The successful Apollo 9 mission, the most complex crewed space mission flown to that time, brought the Moon landing one step closer.

In Washington, D.C., Vice President Spiro T. Agnew, second from left, accepts a framed American flag flown in space by Apollo 9 astronauts Russell L. Schweickart, left, David R. Scott, and James A. McDivitt In front of the Apollo 8 Command Module at the 1969 Paris Air Show, astronauts meet cosmonauts – Scott, Vladimir A. Shatalov, McDivitt, Aleksei S. Yeliseyev, and Schweickart
Left: In Washington, D.C., Vice President Spiro T. Agnew, second from left, accepts a framed American flag flown in space by Apollo 9 astronauts Russell L. Schweickart, left, David R. Scott, and James A. McDivitt. Right: In front of the Apollo 8 Command Module at the 1969 Paris Air Show, astronauts meet cosmonauts – Scott, Vladimir A. Shatalov, McDivitt, Aleksei S. Yeliseyev, and Schweickart.

Following postflight debriefs, McDivitt, Scott, and Schweickart traveled to Washington, D.C., where on March 26, Vice President Agnew presented them with Distinguished Service Medals for their execution of the historic Apollo 9 mission. They in turn presented the Vice President with a framed American flag they had taken to space. Among other postflight events and celebrations, the trio attended the Paris Air Show and on May 29 met Soviet cosmonauts Vladimir A. Shatalov and Aleksei S. Yeliseyev who had flown as part of the Soyuz 4 and 5 docking and spacewalk crew exchange mission in January 1969.

Workers at Norfolk Naval Air Station in Virginia offload the Apollo 9 Command Module Gumdrop from the U.S.S. Guadalcanal for its cross country trip to California Gumdrop on display at the Michigan Space and Science Center in Jackson Gumdrop on display at the San Diego Air & Space Museum
Left: Workers at Norfolk Naval Air Station in Virginia offload the Apollo 9 Command Module Gumdrop from the U.S.S. Guadalcanal for its cross country trip to California. Middle: Gumdrop on display at the Michigan Space and Science Center in Jackson. Image credit: courtesy Atlas Obscura. Right: Gumdrop on display at the San Diego Air & Space Museum.

Workers offloaded Gumdrop from the Guadalcanal in Norfolk, Virginia, for transport aboard a U.S. Air Force cargo jet to Long Beach, California, from where they trucked it to the North American Rockwell plant in Downey for postflight inspection. NASA transferred Gumdrop to the Smithsonian Institution in 1973. In 1977, it went on display at the Michigan Space and Science Center in Jackson, Michigan, McDivitt’s hometown. When that facility closed in 2004, Gumdrop transferred to the San Diego Air & Space Museum, where visitors can view it today.

Apollo 10

The Apollo 10 Saturn V leaves the Vehicle Assembly Building at NASA’s Kennedy Space Center in Florida The Apollo 10 Saturn V has reached Launch Pad 39B Apollo 10 astronauts John W. Young, left, Eugene A. Cernan, and Thomas P. Stafford pose before their Saturn V rocket
Left: The Apollo 10 Saturn V leaves the Vehicle Assembly Building at NASA’s Kennedy Space Center in Florida. Middle: The Apollo 10 Saturn V has reached Launch Pad 39B. Right: Apollo 10 astronauts John W. Young, left, Eugene A. Cernan, and Thomas P. Stafford pose before their Saturn V rocket.

On March 11, as the Apollo 9 astronauts neared the end of their mission, workers at KSC rolled the Apollo 10 Saturn V vehicle from the Vehicle Assembly Building (VAB) to its launch pad. Apollo 10’s assembly marked the first use of the VAB’s High Bay 2, requiring the stack to exit the VAB’s rear and make a sweeping loop around the building to reach the crawlerway to the launch pads. Apollo 10 also marked the first use of Pad 39B. On March 17, NASA managers formally set Apollo 10’s launch date as May 18. Apollo 10 astronauts Thomas P. Stafford, John W. Young, and Eugene A. Cernan and their backups L. Gordon Cooper, Donn F. Eisele, and Edgar D. Mitchell continued training in spacecraft simulators and testing their spacesuits in vacuum chambers. On March 27, the prime crew conducted a walk-through of Pad 39B and trained on emergency escape procedures. The next day, the backup crew practiced water egress training in the Water Immersion Facility in MSC’s Building 260, and repeated the training in the Gulf of Mexico the following week.

Apollo 11

Apollo 11 astronauts Neil A. Armstrong, left, Edwin E. “Buzz” Aldrin, and Michael Collins, not visible, prepare for an altitude chamber test of their Command Module at NASA’s Kennedy Space Center (KSC) in Florida Apollo 11 backup crew members James A. Lovell and Frew W. Haise have entered the chamber for a Lunar Module altitude test In KSC’s Vehicle Assembly Building, workers lower the S-IVB third stage onto the Apollo 11 Saturn V rocket
Left: Apollo 11 astronauts Neil A. Armstrong, left, Edwin E. “Buzz” Aldrin, and Michael Collins, not visible, prepare for an altitude chamber test of their Command Module at NASA’s Kennedy Space Center (KSC) in Florida. Middle: Apollo 11 backup crew members James A. Lovell and Frew W. Haise have entered the chamber for a Lunar Module altitude test. Right: In KSC’s Vehicle Assembly Building, workers lower the S-IVB third stage onto the Apollo 11 Saturn V rocket.

Workers in the VAB’s High Bay 3 stacked the Apollo 11 Saturn V’s S-IC first stage on Feb. 21. They added the S-II second stage and S-IVB third stage on March 4 and 5, respectively. The spacecraft for Apollo 11 continued testing in KSC’s Manned Spacecraft Operations Building (MSOB). With their historic mission only five months away, the Apollo 11 prime crew of Neil A. Armstrong, Michael Collins, and Edwin E. “Buzz” Aldrin and their backups James A. Lovell, William A. Anders, and Fred W. Haise busied themselves training for the Moon landing, spending time in spacecraft simulators. The prime and backup crews participated in altitude chamber tests of both their CM and LM.

Mobile Quarantine Facility, Lunar Receiving Laboratory, and Lunar Module Drop Tests

Flight surgeon Dr. William R. Carpentier, left, and the three astronaut surrogates wearing Biological Isolation Garments, prepare to enter the Mobile Quarantine Facility (MQF) aboard the U.S.S. Guadalcanal Dr. Carpentier, left, astronaut surrogates Paul H. Kruppenbacher, Arthur E. Lizza, and Michael T. “Tex” Ward, and engineer John K. Hirasake inside the MQF aboard the Guadalcanal Workers at Norfolk Naval Air Station in Virginia lift the MQF off the Guadalcanal onto a truck for its return to Houston
Left: Flight surgeon Dr. William R. Carpentier, left, and the three astronaut surrogates wearing Biological Isolation Garments, prepare to enter the Mobile Quarantine Facility (MQF) aboard the U.S.S. Guadalcanal. Middle: Dr. Carpentier, left, astronaut surrogates Paul H. Kruppenbacher, Arthur E. Lizza, and Michael T. “Tex” Ward, and engineer John K. Hirasake inside the MQF aboard the Guadalcanal. Right: Workers at Norfolk Naval Air Station in Virginia lift the MQF off the Guadalcanal onto a truck for its return to Houston.

Preparations for ground support facilities for the first lunar landing mission continued. In conjunction with the Apollo 9 splashdown and recovery operations aboard the Guadalcanal, NASA conducted a simulation of recovery operations of astronauts returning from a lunar mission. NASA Flight Surgeon Dr. William R. Carpentier, project engineer John K. Hirasaki, and three astronaut stand-ins, Paul H. Kruppenbacher, Michael T. “Tex” Ward, and Arthur E. Lizza, spent 10 days inside a Mobile Quarantine Facility (MQF), a modified Airstream trailer designed to temporarily house astronauts returning from the Moon. The three astronaut surrogates began the simulation by entering a mockup CM that sailors placed in the ocean and recovered as if returning from a space mission. The trio donned Biological Isolation Garments (BIG), meant to prevent contamination of Earth by any possible lunar organisms. Once on board the Guadalcanal, the three accompanied by Carpentier and Hirasaki entered the MQF for four days, where the just-recovered Apollo 9 crew visited them through the window of the trailer. The five stayed inside the MQF except for the short time it was transferred from the Guadalcanal to a waiting transport aircraft at Norfolk Naval Air Station and flown back to Houston. After offloading, the MQF and its five inhabitants transferred to the Lunar Receiving Laboratory (LRL) in MSC’s Building 37 to begin a simulated quarantine. Overall, the exercise tested the procedures for the activities after the first lunar landing mission, with many lessons learned.

During a simulation, workers line up in the kitchen of the Crew Reception Area of the Lunar Receiving Laboratory at the Manned Spacecraft Center (MSC), now NASA’s Johnson Space Center in Houston The Vibration and Acoustics Test Facility (VATF) at MSC The Lunar Module during drop testing in the VATF
Left: During a simulation, workers line up in the kitchen of the Crew Reception Area of the Lunar Receiving Laboratory at the Manned Spacecraft Center (MSC), now NASA’s Johnson Space Center in Houston. Middle: The Vibration and Acoustics Test Facility (VATF) at MSC. Right: The Lunar Module during drop testing in the VATF.

Managers, scientists, technicians, and engineers conducted a 30-day simulation in the LRL, the most complex test of the facility to verify that all its components would be ready to support crewmembers and their samples returning from the Moon, possibly by July 1969. A separate seven-day simulation of the astronaut quarantine capabilities in the LRL’s Crew Reception Area began on March 25. Fifteen NASA and contractor employees, most of whom would participate in the activities following the actual lunar landing mission, demonstrated the logistics of maintaining astronauts and support staff in isolation. All biological barriers operated during the simulation, and the only contact test personnel had with the outside world was via telephone or through glass walls.  The first part of the test included the simulated arrival of lunar materials and film, followed the next day by the arrival of the stand-in crew. The last part of the test included the process for releasing the crew and personnel from quarantine.

The Structures and Mechanics Division at MSC conducted a series of drop tests in the Vibration and Acoustic Test Facility (VATF) to verify that the LM’s systems would operate following a lunar landing. The LM’s manufacturer, the Grumman Aircraft Engineering Corporation, located in Bethpage, New York, provided technical support for the tests using LM-2, a flight qualified  vehicle with all subsystems installed. To simulate the LM’s configuration at landing, workers filled the tanks in the ascent stage with inert fluid to mimic a full load of fuel, while keeping the descent stage tanks mostly empty as they would be following the powered descent from orbit. The series of five tests began on March 21, 1969, and finished on May 7. Engineers dropped LM-2 from heights ranging from eight to 24 inches onto artificial slopes and obstructions to simulate landings on rough lunar terrain. Successful completion of the drop tests removed a constraint from carrying out the first lunar landing. Visitors can view LM-2 on display at the Smithsonian Institution’s National Air and Space Museum in Washington, D.C.

Apollo 12

The S-IVB third stage for the Apollo 12 Saturn V arrives at NASA’s Kennedy Space Center (KSC) in Florida The Apollo 12 Lunar Module arrives at KSC In KSC’s Manned Spacecraft Operations Building, workers uncrate the Apollo 12 Command and Service Modules, foreground, as they continue work on the Apollo 11 spacecraft
Left: The S-IVB third stage for the Apollo 12 Saturn V arrives at NASA’s Kennedy Space Center (KSC) in Florida. Middle: The Apollo 12 Lunar Module arrives at KSC. Right: In KSC’s Manned Spacecraft Operations Building, workers uncrate the Apollo 12 Command and Service Modules, foreground, as they continue work on the Apollo 11 spacecraft.

In case Apollo 11 could not achieve the Moon landing in July, NASA planned to try again with Apollo 12 in September. To protect for that launch date, components of the rocket and spacecraft began arriving at KSC. The Saturn V’s S-IVB third stage arrived on March 10 and workers placed it in storage in the VAB until the other two stages arrived in April and May. The Apollo 12 LM’s two stages arrived on March 24, and workers transported them to the MSOB. The CM and SM arrived four days later, and they shared space in the MSOB with the Apollo 11 spacecraft undergoing testing.

To be continued …

News from around the world in March 1969:

March 2 – First test flight of the Anglo-French Concorde supersonic jet transport in Toulouse.

March 3 – The U.S. Navy established the Navy Fighter Weapons School, better known as Top Gun, at Naval Air Station Miramar in California.

March 16 – Historical musical “1776” opens, runs for 1,217 performances, and wins three Tony Awards

March 17 – Golda Meir becomes Israel’s fourth and first, and so far only, woman prime minister.

March 26 – “Marcus Welby, M.D.” debuts as a TV movie on ABC, then becomes a series.

March 27 – Mariner 7 joins Mariner 6 on a journey to fly by Mars.

March 28 – Dwight D. Eisenhower, 34th president of the U.S., died at age 78.

March 31 – Kurt Vonnegut’s novel “Slaughterhouse-Five” was published.

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      Intuitive Machines of Houston will receive two task order awards on its contract for Subcategory 1.2 GEO to Cislunar Direct to Earth (DTE) Services and Subcategory 1.3 xCislunar DTE Services to support NASA’s Lunar Exploration Ground Segment, providing additional capacity to alleviate demand on the Deep Space Network and to meet the mission requirements for unique, highly elliptical orbits. The company also previously received a task order award for Subcategory 2.2 GEO to Cislunar Relay Services. Kongsberg Satellite Services of Tromsø, Norway, will receive two task order awards on its contract for Subcategory 1.1 Earth Proximity DTE and Subcategory 1.2 to support science missions in low Earth orbit and NASA’s Lunar Exploration Ground Segment, providing additional capacity to alleviate demand on the Deep Space Network. SSC Space U.S. Inc. of Horsham, Pennsylvania, will receive two task order awards on its contract for Subcategories 1.1 and 1.3 to support science missions in low Earth orbit and to meet the mission requirements for unique, highly elliptical orbits. Viasat, Inc. of Duluth, Georgia, will be awarded a task order on its contract for Subcategory 1.1 to support science missions in low Earth orbit. The Near Space Network’s direct-to-Earth capability supports many of NASA’s missions ranging from climate studies on Earth to research on celestial objects. It also will play a role in NASA’s Artemis campaign, which calls for long-term exploration of the Moon.
      NASA’s goal is to provide users with communication and navigation services that are secure, reliable, and affordable, so that all NASA users receive the services required by their mission within their latency, accuracy, and availability requirements.
      These awards demonstrate NASA’s ongoing commitment to fostering strong partnerships with the commercial space sector, which plays an essential role in delivering the communications infrastructure critical to the agency’s science and exploration missions.
      As part of the agency’s SCaN (Space Communications and Navigation) Program, teams at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, will carry out the work of the Near Space Network. The Near Space Network provides missions out to 1.2 million miles (2 million kilometers) with communications and navigation services, enabling spacecraft to exchange critical data with mission operators on Earth. Using space relays in geosynchronous orbit and a global system of government and commercial direct-to-Earth antennas on Earth, the network brings down terabytes of data each day.
      Learn more about NASA’s Near Space Network:
      https://www.nasa.gov/near-space-network
      -end-
      Joshua Finch
      Headquarters, Washington
      202-358-1100
      joshua.a.finch@nasa.gov
      Jeremy Eggers
      Goddard Space Flight Center, Greenbelt, Maryland
      757-824-2958
      jeremy.l.eggers@nasa.gov
      View the full article
    • By NASA
      5 Min Read NASA’s Ames Research Center Celebrates 85 Years of Innovation
      The NACA Ames laboratory in 1944 Credits: NASA Ames Research Center in California’s Silicon Valley pre-dates a lot of things. The center existed before NASA – the very space and aeronautics agency it’s a critical part of today. And of all the marvelous advancements in science and technology that have fundamentally changed our lives over the last 85 years since its founding, one aspect has remained steadfast; an enduring commitment to what’s known by some on-center simply as, “an atmosphere of freedom.” 
      Years before breaking ground at the site that would one day become home to the world’s preeminent wind tunnels, supercomputers, simulators, and brightest minds solving some of the world’s toughest challenges, Joseph Sweetman Ames, the center’s namesake, described a sentiment that would guide decades of innovation and research: 
      My hope is that you have learned or are learning a love of freedom of thought and are convinced that life is worthwhile only in such an atmosphere
      Joseph sweetman ames
      Founding member of the N.A.C.A.
      “My hope is that you have learned or are learning a love of freedom of thought and are convinced that life is worthwhile only in such an atmosphere,” he said in an address to the graduates of Johns Hopkins University in June 1935.
      That spirit and the people it attracted and retained are a crucial part of how Ames, along with other N.A.C.A. research centers, ultimately made technological breakthroughs that enabled humanity’s first steps on the Moon, the safe return of spacecraft through Earth’s atmosphere, and many other discoveries that benefit our day-to-day lives.
      Russell Robinson momentarily looks to the camera while supervising the first excavation at what would become Ames Research Center.NACA “In the context of my work, an atmosphere of freedom means the freedom to pursue high-risk, high-reward, innovative ideas that may take time to fully develop and — most importantly — the opportunity to put them into practice for the benefit of all,” said Edward Balaban, a researcher at Ames specializing in artificial intelligence, robotics, and advanced mission concepts.
      Balaban’s career at Ames has involved a variety of projects at different stages of development – from early concept to flight-ready – including experimenting with different ways to create super-sized space telescopes in space and using artificial intelligence to help guide the path a rover might take to maximize off-world science results. Like many Ames researchers over the years, Balaban shared that his experience has involved deep collaborations across science and engineering disciplines with colleagues all over the center, as well as commercial and academic partners in Silicon Valley where Ames is nestled and beyond. This is a tradition that runs deep at Ames and has helped lead to entirely new fields of study and seeded many companies and spinoffs.
      Before NASA, Before Silicon Valley: The 1939 Founding of Ames Aeronautical Laboratory “In the fields of aeronautics and space exploration the cost of entry can be quite high. For commercial enterprises and universities pursuing longer term ideas and putting them into practice often means partnering up with an organization such as NASA that has the scale and multi-disciplinary expertise to mature these ideas for real-world applications,” added Balaban.
      “Certainly, the topics of inquiry, the academic freedom, and the benefit to the public good are what has kept me at Ames,” reflected Ross Beyer, a planetary scientist with the SETI Institute at Ames. “There’s not a lot of commercial incentive to study other planets, for example, but maybe there will be soon. In the meantime, only with government funding and agencies like NASA can we develop missions to explore the unknown in order to make important fundamental science discoveries and broadly share them.”
      For Beyer, his boundary-breaking moment came when he searched – and found – software engineers at Ames capable and passionate about open-source software to generate accurate, high-resolution, texture-mapped, 3D terrain models from stereo image pairs. He and other teams of NASA scientists have since applied that software to study and better understand everything from changes in snow and ice characteristics on Earth, as well as features like craters, mountains, and caves on Mars or the Moon. This capability is part of the Artemis campaign, through which NASA will establish a long-term presence at the Moon for scientific exploration with commercial and international partners. The mission is to learn how to live and work away from home, promote the peaceful use of space, and prepare for future human exploration of Mars. 
      “As NASA and private companies send missions to the Moon, they need to plan landing sites and understand the local environment, and our software is freely available for anyone to use,” Beyer said. “Years ago, our management could easily have said ‘No, let’s keep this software to ourselves; it gives us a competitive advantage.’ They didn’t, and I believe that NASA writ large allows you to work on things and share those things and not hold them back.” 
      When looking forward to what the next 85 years might bring, researchers shared a belief that advancements in technology and opportunities to innovate are as expansive as space itself, but like all living things, they need a healthy atmosphere to thrive. Balaban offered, “This freedom to innovate is precious and cannot be taken for granted. It can easily fall victim if left unprotected. It is absolutely critical to retain it going forward, to ensure our nation’s continuing vitality and the strength of the other freedoms we enjoy.”
      Ames Aeronautical Laboratory.NACAView the full article
    • By NASA
      “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 third servicing mission to the Hubble Space Telescope, placed in orbit in 1990, occurred during the STS-103 mission in December 1999. During the mission, originally planned for June 2000 but accelerated by six months following unexpected failures of the telescope’s attitude control gyroscopes, the astronauts restored the facility to full functionality. During their eight-day mission that featured the first space shuttle crew to spend Christmas in space, the seven-member U.S. and European crew rendezvoused with and captured Hubble, and four astronauts in rotating teams of two conducted three lengthy and complex spacewalks to service and upgrade the telescope. They redeployed the telescope with greater capabilities than ever before to continue its mission to help scientists unlock the secrets of the universe.
      Schematic showing 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. The discovery after the Hubble Space Telescope’s launch in 1990 that its primary mirror suffered from a flaw called spherical aberration 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 in 1993. A second servicing mission in 1997 upgraded the telescope’s capabilities until the next mission planned for three years later. But after three of the telescope’s six gyroscopes failed in 1997, 1998, and 1999, mission rules dictated a call up mission in case additional gyroscope failures sent Hubble into a safe mode. NASA elected to move up some of the servicing tasks from the third mission, splitting it into missions 3A and 3B, planning to fly 3A in October 1999 on Discovery’s STS-103 mission primarily to replace the failed gyroscopes. Delays to the shuttle fleet resulting from anomalies during the launch of STS-93 in July 1993 slipped STS-103 first into November and ultimately into December. Technical issues with Discovery itself pushed the launch date to mid-December, and raised concerns about having a shuttle in orbit during the Y2K transition. Once the launch had slipped to Dec. 19, mission planners cut the mission from 10 to eight days, deleting one of the four spacewalks, to ensure a return before the end of the calendar year. The servicing mission couldn’t come soon enough, as a fourth gyroscope failed aboard Hubble in mid-November, with Discovery already poised on the launch pad to prepare for STS-103. Controllers placed Hubble in a safe mode until the astronauts arrived.
      The STS-103 crew of C. Michael Foale, left, Claude Nicollier, Scott J. Kelly, Curtis L. Brown, Jean-François A. Clervoy, John M. Grunsfeld, and Steven L. Smith. The STS-103 crew patch. The mission patch for the Hubble Servicing Mission-3A. To execute the third Hubble Servicing Mission, in July 1998 NASA selected an experienced four-person team to carry out a record-breaking six spacewalks on the flight then planned for June 2000. The spacewalkers included Mission Specialists Steven L. Smith serving as payload commander, John M. Grunsfeld, C. Michael Foale, and European Space Agency (ESA) astronaut Claude Nicollier from Switzerland. The addition in March 1999 of Commander Curtis L. Brown, Pilot Scott J. Kelly, and Mission Specialist ESA astronaut Jean-François A. Clervoy of France rounded out the highly experienced crew with 18 previous spaceflights among them. Brown earned the distinction as only the fifth person to fly in space six times. For Kelly, STS-103 marked his first spaceflight. Smith, Clervoy, and Grunsfeld each had flown two previous missions, Foale four including a long-duration mission aboard Mir, and Nicollier three. Smith participated in three spacewalks during the second Hubble Servicing Mission and Nicollier served as the Remote Manipulator System (RMS) or robotic arm operator during the first.
      The STS-103 crew at the traditional prelaunch breakfast at NASA’s Kennedy Space Center in Florida. Suited up, the STS-103 astronauts leave crew quarters for the trip to Launch Pad 39B. Space shuttle Discovery on Launch Pad 39B, awaiting launch. Discovery arrived back to KSC at the end of the STS-96 mission on June 6, 1999, and workers towed it to the Orbiter Processing Facility the same day to begin readying it for STS-103. The vehicle rolled over to the Vehicle Assembly Building on Nov. 4, where workers mated it with its external tank and twin solid rocket boosters, before rolling the stack out to Launch Pad 39B on Nov. 13.
      Liftoff of space shuttle Discovery on the STS-103 Hubble Space Telescope servicing mission 3A. The Hubble Space Telescope as Discovery approaches. The STS-103 crew berthing the Hubble into the payload bay. Beginning its 27th trip into space, Discovery lifted off from Launch Pad 39B at 7:50 p.m. EST on Dec. 19 to fix the ailing space telescope. Two days later, Brown and Kelly maneuvered Discovery to within range of Hubble so Clervoy operating the 50-foot-long RMS could grapple the telescope and berth it into the payload bay.
      During the first spacewalk, astronauts John M. Grunsfeld, left, and Steven L. Smith replacing one of the Rate Sensor Units containing two gyroscopes. Smith gives a thumbs up with his image reflected in the Hubble Space Telescope. Smith and Grunsfeld conducted the mission’s first spacewalk on Dec. 22, the flight’s fourth day in space. The duo, aided by Clervoy operating the RMS from inside Discovery, completed two of mission’s highest priority objectives. They replaced the failed gyroscopes, installing three new Rate Sensor Units, each containing two gyroscopes, to return control to the ailing telescope. They also installed six Voltage/Temperature Improvement Kits to prevent the telescope’s batteries from overheating as they aged. The excursion lasted eight hours 15 minutes, at the time the second longest spacewalk.
      During the second spacewalk, astronauts C. Michael Foale, left, and Claude Nicollier during the changeout of the fine guidance sensor. Foale at the end of the Remote Manipulator System services the Hubble Space Telescope. The next day, Nicollier and Foale conducted the mission’s second spacewalk. The main task for this excursion involved installing a new computer aboard Hubble, replacing the original 1970s vintage unit. The new radiation-hardened system ran 20 times faster and carried six times more memory while using one-third the electrical power. They also installed a fine guidance sensor before concluding the eight-hour 10-minute spacewalk.
      Astronauts Steven L. Smith, left, and John M. Grunsfeld begin their servicing activities during the third spacewalk. At the end of the third and final spacewalk, Grunsfeld, left, and Smith provide closing comments about the work the mission accomplished to service the Hubble Space Telescope. Smith and Grunsfeld ventured outside for a second time to complete the flight’s third and final spacewalk on Dec. 24, the first spacewalk conducted on Christmas Eve day. First, they replaced an old reel-to-reel tape recorder with a solid state unit providing a 10-fold increase in recording capability and replaced a failed data transmitter. They installed seven new covers on Hubble’s electronics bay doors for added protection of the telescope’s insulation. This third spacewalk lasted eight hours eight minutes.
      The first space shuttle crew to celebrate Christmas in space, the STS-103 astronauts pose wearing Santa hats. The Hubble Space Telescope shortly after the STS-103 crew released it. The next day, the STS-103 astronauts earned the distinction as the first space shuttle crew to spend Christmas Day in space. Clervoy grappled Hubble, lifted it out of the payload bay and released it to continue its mission. Hubble Space Telescope Program Manager John H. Campbell said after the release, “The spacecraft is being guided by its new gyros under the control of its brand new computer. [It] is now orbiting freely and is in fantastic shape.” After deploying Hubble, the astronauts enjoyed a well-deserved Christmas dinner, with Clervoy providing French delicacies. The crew spent Dec. 26 readying Discovery for its return to Earth, including testing its reaction control system thrusters and aerodynamic surfaces and stowing unneeded gear.
      Astronauts Steven L. Smith, left, Claude Nicollier, and John M. Grunsfeld complete their fluid loading protocol and put on their launch and entry suits prior to reentry. Space shuttle Discovery makes a perfect night landing at NASA’s Kennedy Space Center in Florida. The crew welcome home ceremony at Ellington Field in Houston. On Dec. 27, the astronauts donned their launch and entry suits and prepared for the return to Earth. They closed the payload bay doors and fired Discovery’s engines to bring them out of orbit. Just before landing, Kelly lowered the craft’s landing gear and Brown guided Discovery to a smooth night landing at KSC, concluding a flight of seven days, 23 hours, 11 minutes. They circled the Earth 119 times. The flight marked Discovery’s last solo flight as all its subsequent missions docked with the International Space Station. Workers at KSC began readying it for its next mission, STS-92 in October 2000.

      The Hubble Space Telescope continues to operate today, far exceeding the five-year life extension expected from the last of the servicing missions in 2009. Joined in space by the James Webb Space Telescope in 2021, the two instruments together continue to image the skies across a broad range of the electromagnetic spectrum to provide scientists with the tools to gain unprecedented insights into the universe and its formation.

      Watch the STS-103 crew narrate a video of their Hubble servicing mission.
      View the full article
    • By European Space Agency
      Video: 00:10:27 In 1975, 10 European countries came together with a vision to collaborate on key space activities: science and astronomy, launch capabilities and space applications: the European Space Agency, ESA, was born.
      In 2025, we mark half a century of joint European achievement – filled with firsts and breakthroughs in science, exploration and technology, and the space infrastructure and economy that power Europe today.
       
      During the past five decades ESA has grown, developing ever bolder and bigger projects and adding more Member States, with Slovenia joining as the latest full Member State in January.
       
      We’ll also celebrate the 50th anniversary of ESA’s Estrack network, 30 years of satellite navigation in Europe and 20 years since ESA launched the first demonstration satellite Giove-A which laid the foundation for the EU’s own satnav constellation Galileo. Other notable celebrations are the 20th anniversary of ESA’s Business Incubation Centres, or BICs, and the 30th year in space for SOHO, the joint ESA and NASA Solar and Heliospheric Observatory.
       
      Sadly though, 2025 will mean end of science operations for Integral and Gaia. Integral, ESA's gamma-ray observatory has exotic objects in space since 2002 and Gaia concludes a decade of mapping the stars. But as some space telescopes retire, another one provides its first full data release. Launched in 2023, we expect Euclid’s data release early in the new year.
       
      Launch-wise, we’re looking forward to Copernicus Sentinel-4 and -5 (Sentinel-4 will fly on an MTG-sounder satellite and Sentinel-5 on the MetOp-SG-A1 satellite), Copernicus Sentinel-1D, Sentinel-6B and Biomass. We’ll also launch the SMILE mission, or Solar wind Magnetosphere Ionosphere Link Explorer, a joint mission with the Chinese academy of science.
       
      The most powerful version of Europe’s new heavy-lift rocket, Ariane 6, is set to fly operationally for the first time in 2025. With several European commercial launcher companies planning to conduct their first orbital launches in 2025 too, ESA is kicking off the European Launcher Challenge to support the further development of European space transportation industry.
       
      In human spaceflight, Polish ESA project astronaut Sławosz Uznański will fly to the ISS on the commercial Axiom-4 mission. Artemis II will be launched with the second European Service Module, on the first crewed mission around the Moon since 1972.
      The year that ESA looks back on a half century of European achievement will also be one of key decisions on our future. At the Ministerial Council towards the end of 2025, our Member States will convene to ensure that Europe's crucial needs, ambitions and the dreams that unite us in space become reality.
      So, in 2025, we’ll celebrate the legacy of those who came before but also help establish a foundation for the next 50 years. Join us as we look forward to a year that honours ESA’s legacy and promises new milestones in space.
      View the full article
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