Jump to content

Dedicating The Neil A. Armstrong Facility for an American Hero


Recommended Posts

Join the conversation

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

Guest
Reply to this topic...

×   Pasted as rich text.   Paste as plain text instead

  Only 75 emoji are allowed.

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

×   Your previous content has been restored.   Clear editor

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

  • Similar Topics

    • By NASA
      NASA’s Michoud Assembly Facility in New Orleans, includes 43 acres of manufacturing space under one roof — a space large enough to contain more than 31 professional football fields. Credit: NASA Media are invited to visit NASA’s Michoud Assembly Facility in New Orleans between Tuesday, Feb. 4, and Thursday, Feb. 6, ahead of Super Bowl LIX for an inside look America’s rocket factory, as well as interview agency experts.
      During this behind-the-scenes visit, media will tour NASA’s location for the manufacturing and production of large-scale space structures and see hardware that will carry astronauts back to the Moon as part of the Artemis campaign.
      Registered members of the media will have the opportunity to:
      Capture images and video of hardware NASA Michoud is building for the SLS (Space Launch System) rocket, Orion spacecraft, and SLS exploration upper stage for the agency’s Artemis campaign. Tour special locations around NASA Michoud, one of the largest facilities in the world, with 43 acres of manufacturing space under one roof — a space large enough to contain more than 31 professional football fields. Learn about NASA’s state-of-the-art manufacturing and welding equipment — including the world’s largest friction-stir welding tool. Media must RSVP no later than 6 p.m. EST, Thursday, Jan. 30, to Jonathan Deal at: jonathan.deal@nasa.gov and Craig Betbeze at: craig.c.betbeze@nasa.gov. Please indicate a preferred date to visit between Feb. 4 and Feb. 6. This event is open to U.S. media. NASA’s media accreditation policy is available online.
      Through Artemis, NASA will send astronauts to explore the Moon for scientific discovery, economic benefits, and to build the foundation for the first crewed missions to Mars.
      Learn more about NASA’s Artemis campaign:
      https://www.nasa.gov/artemis
      -end- 
      Rachel Kraft
      NASA Headquarters, Washington
      202-358-1100
      rachel.h.kraft@nasa.gov
      Jonathan Deal
      Marshall Space Flight Center, Huntsville, Ala. 
      256-544-0034 
      jonathan.e.deal@nasa.gov
      Share
      Details
      Last Updated Jan 27, 2025 LocationMarshall Space Flight Center View the full article
    • By NASA
      Learn Home First NASA Neurodiversity… Heliophysics Overview Learning Resources Science Activation Teams SME Map Opportunities More Science Activation Stories Citizen Science   2 min read
      First NASA Neurodiversity Network Intern to Present at the American Geophysical Union Annual Conference
      The NASA Science Activation Program’s NASA’s Neurodiversity Network (N3) project sponsors a summer internship program for high school students, in which learners on the autism spectrum are matched with NASA Subject Matter Experts. N3 intern Lillian Hall and mentor Dr. Juan Carlos Martinez Oliveros presented Lilly’s summer research project on December 9 at the 2024 American Geophysical Union conference in Washington, D.C. Their poster, entitled “Eclipse Megamovie: Image Processing”, represents the first time an N3 intern has co-authored a presentation at the prestigious AGU conference.
      The NASA Citizen Science project, Eclipse Megamovie, is leveraging the power of citizen science to construct a high-resolution time-lapse of the Sun’s corona during the April 8, 2024 total solar eclipse. By coordinating the work of hundreds of participants along the path of totality, a substantial dataset of images was obtained. The goal of the project is to unveil dynamic transformations in the Sun’s atmosphere that are only visible during a total solar eclipse.
      To process the vast quantity of imaging data collected, Lilly assisted Dr. Martinez Oliveros and other researchers in implementing a robust pipeline involving image calibration, registration, and co-location. Image registration techniques aligned the solar features across different frames, compensating for Earth’s rotation and camera movement. Finally, they used imaging techniques to enhance the signal-to-noise ratio, revealing subtle coronal structures and possible dynamics. This comprehensive data processing methodology has enabled the extraction of meaningful scientific information from the Eclipse Megamovie dataset.
      Here’s what Lilly had to say: “Working with N3 has given me a chance to use my neurodiverse perspective to make an impact on NASA research. Through the processes of my project and the opportunity to share it at the American Geophysical Union conference, I am so grateful to have found my spot in the planetary science field I dream to continue researching in the future.”
      Learn more about NASA Citizen Science and how you can participate (participation does not require citizenship in any particular country): https://science.nasa.gov/citizen-science/
      The N3 project is supported by NASA under cooperative agreement award number 80NSSC21M0004 and is part of NASA’s Science Activation Portfolio. Learn more about how Science Activation connects NASA science experts, real content, and experiences with community leaders to do science in ways that activate minds and promote deeper understanding of our world and beyond: https://science.nasa.gov/learn
      https://www.agu.org/annual-meeting/schedule
      Lilly Hall with her Eclipse Megamovie Image Processing poster. Kristen Hall Share








      Details
      Last Updated Jan 10, 2025 Editor NASA Science Editorial Team Related Terms
      Citizen Science Heliophysics Planetary Geosciences & Geophysics Science Activation Explore More
      2 min read NASA eClips Educator Receives 2024 VAST Science Educator Specialist Award


      Article


      3 days ago
      5 min read NASA’s LEXI Will Provide X-Ray Vision of Earth’s Magnetosphere


      Article


      1 week ago
      2 min read NASA Workshops Culturally Inclusive Planetary Engagement with Educators


      Article


      1 week ago
      Keep Exploring Discover More Topics From NASA
      James Webb Space Telescope


      Webb is the premier observatory of the next decade, serving thousands of astronomers worldwide. It studies every phase in the…


      Perseverance Rover


      This rover and its aerial sidekick were assigned to study the geology of Mars and seek signs of ancient microbial…


      Parker Solar Probe


      On a mission to “touch the Sun,” NASA’s Parker Solar Probe became the first spacecraft to fly through the corona…


      Juno


      NASA’s Juno spacecraft entered orbit around Jupiter in 2016, the first explorer to peer below the planet’s dense clouds to…

      View the full article
    • By NASA
      6 min read
      NASA Research To Be Featured at American Astronomical Society Meeting
      In this mosaic image stretching 340 light-years across, Webb’s Near-Infrared Camera (NIRCam) displays the Tarantula Nebula star-forming region in a new light, including tens of thousands of never-before-seen young stars that were previously shrouded in cosmic dust. The most active region appears to sparkle with massive young stars, appearing pale blue. NASA, ESA, CSA, STScI, Webb ERO Production Team From new perspectives on the early universe to illuminating the extreme environment near a black hole, discoveries from NASA missions will be highlighted at the 245th meeting of the American Astronomical Society (AAS). The meeting will take place Jan. 12-16 at the Gaylord National Resort & Convention Center in National Harbor, Maryland.
      Press conferences highlighting results enabled by NASA missions will stream live on the AAS Press Office YouTube channel. Additional agency highlights for registered attendees include:
      NASA Town Hall: Monday, Jan. 13, 12:45 p.m. EST Nancy Grace Roman Space Telescope Town Hall: Tuesday, Jan. 14, 6:30 p.m. EST James Webb Space Telescope Town Hall: Wednesday, Jan. 15, 6:30 p.m. EST Throughout the week, experts at the NASA Exhibit Booth will deliver science talks about missions including NASA’s James Webb Space Telescope (also called “Webb” or “JWST”), Hubble Space Telescope, Chandra X-ray Observatory, TESS (Transiting Exoplanet Survey Satellite), and NICER (Neutron star Interior Composition Explorer), an X-ray telescope on the International Space Station that will be repaired in a spacewalk Jan. 16. Talks will also highlight future missions such as Pandora, Roman, LISA (Laser Interferometer Space Antenna), the Habitable Worlds Observatory, and SPHEREx (Spectro-Photometer for the History of the Universe, Epoch of Reionization and Ices Explorer), which is targeted to launch in late February; as well as mission concepts for NASA’s new Probe Explorers mission class in astrophysics, open science, heliophysics, and NASA Science Activation.
      Members of the media can request interviews with NASA experts on any of these topics by contacting Alise Fisher at alise.m.fisher@nasa.gov.
      Schedule of Highlights (EST)
      Monday, Jan. 13
      10 a.m.: Special Session – “SPHEREx: The Upcoming All-Sky Infrared Spectroscopic Survey”
      Chesapeake 4-5
      10 a.m.: Special Session – “Early Science Results from XRISM [X-Ray Imaging and Spectroscopy Mission]”
      National Harbor 10
      10:15 a.m.: AAS News Conference – “A Feast of Feasting Black Holes”
      Maryland Ballroom 5/6
      News based on data from NASA’s Neil Gehrels Swift Observatory, NICER, NuSTAR (Nuclear Spectroscopic Telescope Array), and Hubble, as well as XMM-Newton, an ESA (European Space Agency) mission with NASA contributions, will be featured:
      “Witnessing the Birth of a New Plasma Jet from a Supermassive Black Hole” “Rapidly Evolving X-Ray Oscillations in the Active Galaxy 1ES 1927+654” “Uncovering the Dining Habits of Supermassive Black Holes in Our Cosmic Backyard with NuLANDS” “The Discovery of a Newborn Quasar Jet Triggered by a Cosmic Dance” 12:45 p.m.: NASA Town Hall
      Mark Clampin, acting deputy associate administrator, Science Mission Directorate at NASA Headquarters
      Potomac Ballroom AB
      2:15 p.m.: AAS News Conference – “Supernovae and Massive Stars”
      Maryland Ballroom 5/6
      News from NASA’s Webb and Hubble space telescopes will be highlighted:
      “JWST Discovery of a Distant Supernova Linked to a Massive Progenitor in the Early Universe” “Core-Collapse Supernovae as Key Dust Producers: New Insights from JWST” “JWST Tracks the Expanding Dusty Fingerprints of a Massive Binary” “Stellar Pyrotechnics on Display in Super Star Cluster” “A Blue Lurker Emerges from a Triple-System Merger” Tuesday, Jan. 14
      10:15 a.m.: AAS News Conference – “Black Holes & New Outcomes from the Sloan Digital Sky Survey”
      Maryland Ballroom 5/6
      News based on data from NASA’s NuSTAR, Chandra, and Webb missions will be highlighted:
      “A Variable X-Ray Monster at the Epoch of Reionization” “JWST’s Little Red Dots and the Rise of Obscured Active Galactic Nuclei in the Early Universe” “Revealing the Mid-Infrared Properties of the Milky Way’s Supermassive Black Hole” 2 p.m.: Special Session – “Open Science: NASA Astrophysics in the Roman Era”
      Chesapeake 4-5
      2:15 p.m.: AAS News Conference – “New Information from Milky Way Highlights”
      Maryland Ballroom 5/6
      News from NASA’s Webb and Chandra missions will be highlighted:
      “Infrared Echoes of Cassiopeia A Reveal the Dynamic Interstellar Medium” “A Path-Breaking Observation of the Cold Neutral Medium of the Milky Way Through Thermal Light Echoes” “X-Ray Echoes from Sgr A* Provide Insight on the 3D Structure of Molecular Clouds in the Galactic Center” 3:40 p.m.: Plenary – “A Detector Backstory: How Silicon Detectors Came to Enable Space Missions”
      Shouleh Nikzad, NASA’s Jet Propulsion Laboratory
      Potomac Ballroom AB
      6:30 p.m.: Nancy Grace Roman Space Telescope Town Hall
      National Harbor 11
      Wednesday, Jan. 15
      8 a.m.: Plenary – “HEAD Bruno Rossi Prize Lecture: The Imaging X-ray Polarimetry Explorer (IXPE)”
      Martin Weisskopf, NASA’s Marshall Space Flight Center (emeritus), and Paolo Soffitta, INAF-IAPS (National Institute for Astrophysics-Institute of Space Astrophysics and Planetology)
      Potomac Ballroom AB
      10 a.m.: Special Session – Habitable Worlds Observatory
      Potomac Ballroom C
      10:15 a.m.: AAS News Conference – “Discovering the Universe Beyond Our Galaxy”
      Maryland Ballroom 5/6
      News from NASA’s Hubble and Webb will be highlighted:
      “The Hubble Tension in Our Own Backyard” “JWST Reveals the Early Universe in Our Backyard” “Growing in the Wind: Watching a Galaxy Seed Its Environment” 11:40 a.m.: Plenary – “Are We Alone? The Search for Life on Habitable Worlds”
      Giada Arney, NASA’s Goddard Space Flight Center
      Potomac Ballroom AB
      2:15 p.m.: AAS News Conference – “New Findings About Stars”
      Maryland Ballroom 5/6
      News based on data from NASA’s Webb and Solar Dynamics Observatory will be highlighted:
      “A Super Star Cluster Is Born: JWST Reveals Dust and Ice in a Stellar Nursery” “The Discovery of Ancient Relics in a Distant Evolved Galaxy” “Exploring the Sun’s Active Regions in the Moments Before Flares” 6:30 p.m.: James Webb Space Telescope Town Hall
      Potomac Ballroom C
      Thursday, Jan. 16
      10:15 a.m.: AAS News Conference – “Exoplanets: From Formation to Disintegration”
      Maryland Ballroom 5/6
      News from NASA’s Pandora, Chandra, TESS, and Webb missions, as well as XMM-Newton, will be highlighted:
      “A New NASA Mission to Characterize Exoplanets and Their Host Stars” “X-Rays in the Prime of Life: Irradiating Vulnerable Planets” “Bright Star, Fading World: Dusty Debris of a Dying Planet” “JWST Exposes Hot Rock Entrails from a Planet’s Demise” 2:15 p.m.: AAS News Conference – “Galactic Histories and Policy Futures”
      Maryland Ballroom 5/6
      News from NASA’s Webb and Hubble will be highlighted:
      “The Boundary of Galaxy Formation: Constraints from the Ancient Star Formation of the Isolated, Extremely Low-Mass Galaxy Leo P” “Resolving 90 Million Stars in the Southern Half of Andromeda” For more information on the meeting, including press registration and the complete meeting schedule, visit:
      https://aas.org/meetings/aas245
      Media Contacts
      Alise Fisher / Liz Landau
      Headquarters, Washington
      202-358-2546 / 202-358-0845
      alise.m.fisher@nasa.gov / elizabeth.r.landau@nasa.gov
      Share








      Details
      Last Updated Jan 10, 2025 Related Terms
      Astrophysics Astrophysics Division Chandra X-Ray Observatory Hubble Space Telescope IXPE (Imaging X-ray Polarimetry Explorer) James Webb Space Telescope (JWST) Nancy Grace Roman Space Telescope TESS (Transiting Exoplanet Survey Satellite) The Universe Explore More
      2 min read Hubble Rings In the New Year


      Article


      11 hours ago
      4 min read Astronaut Set to Patch NASA’s X-ray Telescope Aboard Space Station


      Article


      2 days ago
      3 min read Astronomy Activation Ambassadors: A New Era


      Article


      1 week ago
      Keep Exploring Discover Related Topics
      Missions



      Humans in Space



      Climate Change



      Solar System


      View the full article
    • By NASA
      On Jan. 9, 1990, space shuttle Columbia took off on its ninth flight, STS-32, from NASA’s Kennedy Space Center (KSC) in Florida. Its five-person crew of Commander Daniel Brandenstein, Pilot James Wetherbee, and Mission Specialists Bonnie Dunbar, Marsha Ivins, and David Low flew a then record-breaking 11-day mission to deploy the Syncom IV-F5 communications satellite for the U.S. Navy and retrieve the Long-Duration Exposure Facility (LDEF). Astronauts aboard a shuttle mission in 1984 deployed the LDEF and scientists eagerly awaited the return of their 57 experiments to study the effects of nearly six years exposure to the low Earth orbit environment. The crew also conducted several middeck experiments in biotechnology and materials processing and used an echocardiograph to study changes in their hearts. 
      The STS-32 crew of Mission Specialist Bonnie Dunbar, left, Commander Daniel Brandenstein, Pilot James Wetherbee, and Mission Specialists Marsha Ivins and David Low. The STS-32 crew patch. The Long Duration Exposure Facility during its deployment on the STS-41C mission in 1984.  In November 1988, NASA announced Brandenstein, Wetherbee, Dunbar, Ivins, and Low as the STS-32 crew for the flight then planned for November 1989. Brandenstein, from the Class of 1978, had flown twice before, as pilot on STS-8 in August-September 1983 and commander of STS-51G in June 1985. Dunbar, selected in 1980, had flown once before on STS-61A in October-November 1985. For Wetherbee, Ivins, and Low, all selected in 1984, STS-32 marked their first spaceflight. During the second day of their planned 10-day mission, the astronauts would deploy the Syncom IV-F5, also known as Leasat-5, communications satellite for the U.S. Navy. The main focus of the flight involved the retrieval of LDEF, deployed by the STS-41C crew in April 1984. The original plan had LDEF, containing 57 science and technology experiments, retrieved by the STS-51D crew in February 1985. Delays in the shuttle program first pushed the retrieval to STS-61I in September 1986, and then the Challenger accident delayed it to STS-32. The facility ended up staying in orbit nearly six years instead of the originally intended 10 months. The crew rounded out the mission by conducting a series of middeck science and medical experiments. 
      Space shuttle Columbia rolls out to its launch pad on a foggy morning. NASA scientist John Charles, at rear, trains astronauts David Low, left, and Bonnie Dunbar, supine, in the operation of a cardiovascular experiment. The STS-32 crew exits crew quarters for the ride to Launch Pad 39A. Columbia returned to KSC on Aug. 21, 1989, following STS-28’s landing at Edwards Air Force Base (AFB) in California, and workers towed it to the Orbiter Processing Facility (OPF) the next day. They made 26 modifications to the orbiter, including the installation of the Remote Manipulator System (RMS), or robotic arm, and a fifth set of liquid hydrogen and liquid oxygen tanks to extend the vehicle’s duration in space. Rollover to the nearby Vehicle Assembly Building took place on Nov. 16, where Columbia joined its External Tank and twin Solid Rocket Boosters (SRB) on refurbished Mobile Launch Platform 3, last used in 1975. Rollout took place on Nov. 28 to Launch Pad 39A, newly refurbished since its previous launch in 1986.  
      On Dec. 1, engineers and the astronaut crew completed the Terminal Countdown Demonstration Test, a dress rehearsal for the planned Dec. 18 launch. Based on that date and the mission’s planned 10-day duration, the STS-32 crew would have spent Christmas in space, only the third American crew and the first space shuttle crew to do so. However, unfinished work on Pad 39A delayed the launch into January 1990. Trajectory specialists had estimated that due to orbital decay, LDEF would reenter the Earth’s atmosphere by March 1990, so a timely launch remained crucial for mission success. The countdown began on Jan. 4 for an expected Jan. 8 launch, with the crew arriving at KSC on Jan. 5. 

      Liftoff of space shuttle Columbia on STS-32. The deployment of the Syncom IV-F5 satellite. Syncom following deployment. Cloudy skies scrubbed the first launch attempt on Jan. 8. Liftoff took place the next day at 7:35 a.m. EST from Launch Pad 39A, with LDEF 1,500 miles ahead of Columbia. The powered ride to space took 8.5 minutes, placing Columbia into a 215-by-38-mile orbit. A burn of the two Orbiter Maneuvering System (OMS) engines 40 minutes later changed the orbit to the desired 222-by-180-mile altitude. The crew opened the shuttle’s payload bay doors and deployed its radiators. The major activities for the first day in space involved the checkout of the RMS and the first rendezvous maneuver in preparation for the LDEF grapple three days later. The astronauts also activated four of the middeck experiments. On the mission’s second day, Low deployed the 15,000-pound Syncom satellite, releasing it in a frisbee motion out of the payload bay. The satellite extended its antenna, stabilized itself, and 40 minutes after deployment, fired its engine for the first burn to send it to its geostationary orbit. 

      The Long Duration Exposure Facility (LDEF) during the rendezvous. STS-32 astronaut Bonnie Dunbar has grappled LDEF with the Remote Manipulator System. Dunbar lowers LDEF into the payload bay. Following the Syncom deploy, the crew turned its attention to the rendezvous with LDEF while also continuing the middeck experiments. On Flight Day 3, they completed three rendezvous burns as they steadily continued their approach to LDEF. Soon after awakening on Flight Day 4, the astronauts spotted LDEF appearing as a bright star. After the first of four rendezvous burns, Columbia’s radar locked onto the satellite. As they continued the approach, with three more burns carried out successfully, Dunbar activated the RMS in preparation for the upcoming grapple. Brandenstein took over manual control of Columbia for the final approach and parked the shuttle close enough to LDEF for Dunbar to reach out with the 50-foot arm and grapple the satellite. Brandenstein reported, “We have LDEF.”  
      For the next four hours, with Wetherbee flying the orbiter and Dunbar operating the arm, Ivins performed a comprehensive photo survey of LDEF, documenting the effects of nearly six years of space exposure on the various experiments. The survey completed, Dunbar slowly and carefully lowered LDEF into the payload bay, and five latches secured it in place for the ride back to Earth. With the two major goals of their mission completed, the astronauts settled down for the remainder of their 10-day mission conducting science experiments. 

      With astronaut David Low acting as an operator, astronaut Bonnie Dunbar serves as a subject for a cardiovascular experiment. Astronaut Marsha Ivins with several cameras testing the effects of spaceflight on different types of film. During the mission, the STS-32 crew conducted several middeck experiments. The Protein Crystal Growth experiment used vapor diffusion to grow 120 crystals of 24 different proteins, for study by scientists following their return to Earth. The Characterization of Neurospora Circadian Rhythm experiment studied whether spaceflight affected the daily cycles of pink bread mold. The Fluid Experiment Apparatus performed materials processing research in the microgravity environment. The astronauts used the American Flight Echocardiograph (AFE) to study changes in their hearts as a result of weightlessness. The crew used the large format IMAX camera to film scenes inside the cabin as well as through the windows, such as the capture of LDEF. 

      Astronaut Daniel Brandenstein holds an inflatable plastic cake given to him by his crew mates in honor of his birthday. The STS-32 crew poses in Columbia’s middeck. On Jan. 17, Brandenstein celebrated his 47th birthday, the fifth American astronaut to do so in space. His crew presented him with an inflatable plastic cake including candles while controllers in Mission Control passed on their birthday wishes as did his wife and teenage daughter. On the same day, NASA announced the selection of its 13th group of astronauts. Among them, engineer Ronald Sega, Dunbar’s husband, as well as the first female shuttle pilot, Eileen Collins, and the first Hispanic woman astronaut, Ellen Ochoa. 

      Columbia touches down at Edwards Air Force Base in California. At the welcome home ceremony at Ellington Field in Houston, director of NASA’s Johnson Space Center Aaron Cohen addresses the crowd as the STS-32 astronauts and their families listen. On Jan. 19, the astronauts awakened for their planned final day in space. However, due to fog at their landing site, Edwards AFB in California, Mission Control first informed them that they would have to spend an extra orbit in space, and finally decided to delay the landing by an entire day. With their experiments already packed, the crew spent a quiet day, looking at the Earth and using up what film still remained. As they slept that night, they passed the record for the longest space shuttle mission, set by STS-9 in 1983.  
      In preparation for reentry, the astronauts donned their orange spacesuits and closed the payload bay doors. A last-minute computer problem delayed reentry by one orbit, then Brandenstein and Wetherbee oriented Columbia into the deorbit attitude, with the OMS engines facing in the direction of travel. Over the Indian Ocean, they fired the two engines for 2 minutes 48 seconds to bring the spacecraft out of orbit. They reoriented the orbiter to fly with its heat shield exposed to the direction of flight as it encountered Earth’s atmosphere at 419,000 feet. The buildup of ionized gases caused by the heat of reentry prevented communications for about 15 minutes but provided the astronauts a great light show. After completing the Heading Alignment Circle turn, Brandenstein aligned Columbia with the runway, and Wetherbee lowered the landing gear. Columbia touched down and rolled to a stop, making the third night landing of the shuttle program and ending a 10-day 21-hour 1-minute flight, the longest shuttle flight up to that time, having completed 172 orbits of the Earth.  
      Other records set by the astronauts on this mission included Brandenstein as the new record holder for most time spent in space by a shuttle crew member – 24 days – and Dunbar accumulating the most time in space by a woman – 18 days – up to that time. Following eight hours of postflight medical testing, the astronauts boarded a jet bound for Houston’s Ellington Field, where they reunited with their families and took part in a welcome home ceremony led by Aaron Cohen, director of NASA’s Johnson Space Center. 

      Columbia returns to NASA’s Kennedy Space Center in Florida atop the Shuttle Carrier Aircraft. Workers lift the Long Duration Exposure Facility from Columbia’s payload bay. Following postlanding inspections, workers placed Columbia, with LDEF still cradled in its payload bay, atop a Shuttle Carrier Aircraft, a modified Boeing-747, and the combination left Edwards on Jan. 25. Following a refueling stop at Monthan Davis AFB in Tucson, an overnight stay at Kelly AFB in San Antonio, and another refueling stop at Eglin AFB in Fort Walton Beach, Florida, Columbia and LDEF arrived back at KSC on Jan. 26. The next day, workers towed Columbia to the OPF and on Jan. 30 lifted LDEF out of its payload bay, in preparation for the detailed study of the effects of nearly six years in space on the 57 experiments it carried. Meanwhile, workers began to prepare Columbia for its next flight, STS-35 in December 1990. 
      Enjoy the crew narrate a video of the STS-32 mission. Read Brandenstein‘s and Dunbar‘s recollections of the STS-32 mission in their oral histories with the JSC History Office. For an overview of the LDEF project, enjoy this video. For detailed information on the results of the LDEF experiments, follow this link. 

      View the full article
    • By NASA
      3 min read
      Preparations for Next Moonwalk Simulations Underway (and Underwater)
      NASA/Lori Losey What do the X-15 and the space shuttles have in common? Information from the rocket plane and the spacecraft, as well as many experimental aircraft, were tracked from a pedestal and telemetry dish during key eras in flight history at or near NASA’s Armstrong Flight Research Center in Edwards, California.
      When the NASA facility’s administration Building 4800 was built in the 1950s, the infrastructure was included to anchor the rooftop pedestal and dish as the primary way to gather data from aircraft during flights. It was retired in 2015, but a recent roofing project enabled relocation of the artifact to a new place of honor for its support of many experimental aircraft such as the lifting body aircraft, the reverse swept wing X-29, and the highly maneuverable X-31.
      “Gathering telemetry data from aircraft on missions is at the core of what we do. Close proximity to the back ramp was one of the big advantages of having the telemetry antenna on the roof in the early days,” said Bob Guere, NASA Armstrong Range Operations chief, referring to the area where aircraft taxi from the hangar to the flightline. “You were able to support ground tests and check airplanes before they taxied without having to use telemetry antennas positioned further away.”
      A cable is secured on a rooftop pedestal located on Building 4800 at NASA’s Armstrong Flight Research Center in Edwards, California, on Oct. 4, 2024. The pedestal, which was prepared for a helicopter lift to remove it from the roof, was used since the 1950s until 2015 to enable different telemetry dishes to collect data from research aircraft.NASA/Carla Thomas The rooftop pedestal was key in the early days of the center and its refurbishment in 2003 restored its value. The transformation also included certification to meet Space Shuttle Program landing requirements.
      “When a space shuttle deorbited from space it was coming over the top of Edwards,” Guere said. “Telemetry antennas on the hill near NASA Armstrong looked down and with dirt and concrete in the background there were reflections. The rooftop antenna was closer to ground level and looked up as the orbiter was coming in for a landing. It provided an excellent link for shuttle landings.”
      The pedestal and dish were not removed when it was decommissioned because of the cost. Now, it’s economical to use a helicopter to remove the pedestal from the roof compared to other options as part of a major project focusing primarily on re-roofing Building 4800. The helicopter lift of the pedestal took a month to plan, plus time to obtain airspace operation and landing permits from the Air Force for the removal project, said Bryan Watters, NASA Armstrong roof project manager.
      A helicopter is positioned to remove a rooftop pedestal from Building 4800 at NASA’s Armstrong Flight Research Center in Edwards, California, on Oct. 4, 2024. The pedestal was used since the 1950s to 2015 to house different telemetry dishes to collect data from research aircraft.NASA/Carla Thomas The pedestal and riser measured 16 feet tall above the rooftop and housed an assembly for the 12-foot dish to rotate. The pedestal and dish together weight about 2,500 pounds and were removed separately. Crews checked the eight bolts anchoring the pedestal and dish to infrastructure on the roof prior to the arrival of a helicopter Oct. 3 before the helicopter arrived.
      The following day, after additional briefings, the helicopter was positioned over Building 4800 and a cable was lowered and attached to the pedestal. Once secured, the helicopter slowly gained altitude and took its passenger to the south side of the building. There it was released from the cable and taken to a nearby warehouse for storage. Roofers demolished the steel platform on which the pedestal was located to prepare the area for new roofing materials.
      Officials have not determined where the pedestal will be displayed. There are several options to place the pedestal and dish by the famous retired research aircraft on display near the entrance of NASA Armstrong.
      A pedestal carried by a helicopter is positioned for a gentle placement on the ground. The helicopter removed the pedestal from the rooftop of Building 4800 at NASA’s Armstrong Flight Research Center in Edwards, California, on Oct. 4, 2024. The pedestal was used since the 1950s to 2015 to house different telemetry dishes to collect data from research aircraft.NASA/Carla Thomas A rooftop pedestal and telemetry dish gathered information from research aircraft at Building 4800 at NASA’s Armstrong Flight Research Center in Edwards, California. The pedestal was used since the 1950s to 2015 to house different dishes to collect data from research aircraft. On Oct. 4, 2024, a helicopter was used to remove the pedestal from the roof.NASA/Jim Ross Share
      Details
      Last Updated Jan 08, 2025 EditorDede DiniusContactJay Levinejay.levine-1@nasa.govLocationArmstrong Flight Research Center Related Terms
      Armstrong Flight Research Center Explore More
      4 min read 2024: NASA Armstrong Prepares for Future Innovative Research Efforts
      Article 3 weeks ago 3 min read Atmospheric Probe Shows Promise in Test Flight
      Article 4 weeks ago 3 min read NASA Moves Drone Package Delivery Industry Closer to Reality
      Article 4 weeks ago Keep Exploring Discover More Topics From NASA
      Armstrong Flight Research Center
      Aeronautics
      Flight Innovation
      Armstrong Flight Research Center History
      View the full article
  • Check out these Videos

×
×
  • Create New...