Jump to content

Recommended Posts

  • Publishers
Posted
gsfc-20230407-makenzie-lystrup-portrait-
Portrait of Dr. Makenzie Lystrup, director of NASA’s Goddard Space Flight Center in Greenbelt, Maryland.
Credit: NASA

On Monday, NASA announced Dr. Makenzie Lystrup, director of NASA’s Goddard Space Flight Center in Greenbelt, Maryland, is set to leave the agency on Friday, Aug. 1.

As center director of Goddard, a role she has held since April 2023, Lystrup also was responsible for guiding the direction and management of multiple other NASA field installations including Wallops Flight Facility in Virginia, Katherine Johnson Independent Verification & Validation Facility in West Virginia, the White Sands Complex in New Mexico, and the Columbia Scientific Balloon Facility in Texas.

“Having served in a variety of science and aerospace civilian and government roles in her career, Makenzie has led development of, and/or contributed to a variety of NASA’s priority science missions including successful operations of our James Webb Space Telescope and Imaging X-Ray Polarimetry Explorer, as well as development of the agency’s Roman Space Telescope, and more,” said Vanessa Wyche, acting NASA associate administrator. “We’re grateful to Makenzie for her leadership at NASA Goddard for more than two years, including her work to inspire a Golden Age of explorers, scientists, and engineers.”

Throughout her time at NASA, Lystrup led Goddard’s workforce, which consists of more than 8,000 civil servants and contractors. Before joining the agency, Lystrup served as senior director for Ball’s Civil Space Advanced Systems and Business Development, where she managed new business activities for NASA, National Oceanic and Atmospheric Administration (NOAA), and other civilian U.S. government agencies as well as for academia and other science organizations. In addition, she served in the company’s Strategic Operations organization, based in Washington where she led Ball’s space sciences portfolio.

Prior to joining Ball, Lystrup worked as an American Institute of Physics – Acoustical Society of American Congressional Fellow from 2011 to 2012 where she managed a portfolio including technology, national defense, nuclear energy, and nuclear nonproliferation.

Lystrup also has served on boards and committees for several organizations to include the University Corporation for Atmospheric Research, International Society for Optics and Photonic, the University of Colorado, and the American Astronomical Society. She was named an American Association for the Advancement of Science fellow in 2019 for her distinguished record in the fields of planetary science and infrared astronomy, science policy and advocacy, and aerospace leadership. Lystrup also served as an AmeriCorps volunteer focusing on STEM education.

Lystrup holds a bachelor’s in physics from Portland State University and attended graduate school at University College London earning her doctorate in astrophysics. She was a National Science Foundation Astronomy & Astrophysics Postdoctoral Research Fellow spending time at the Laboratory for Atmospheric & Space Physics in Boulder, Colorado, and University of Liege in Belgium. As a planetary scientist and astronomer, Lystrup’s scientific work has been in using ground- and space-based astronomical observatories to understand the interactions and dynamics of planetary atmospheres and magnetospheres – the relationships between planets and their surrounding space environments.

Following Lystrup’s departure, NASA’s Cynthia Simmons will serve as acting center director. Simmons is the current deputy center director.

For more information about NASA’s work, visit:

https://www.nasa.gov

-end-

Cheryl Warner / Kathryn Hambleton
Headquarters, Washington
202-358-1600
cheryl.m.warner@nasa.gov / kathryn.hambleton@nasa.gov

Katy Mersmann
Goddard Space Flight Center, Greenbelt, Md.
301-377-1724
katy.mersmann@nasa.gov

Share

Details

Last Updated
Jul 21, 2025
Editor
Jessica Taveau

View the full article

Join the conversation

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

Guest
Reply to this topic...

×   Pasted as rich text.   Paste as plain text instead

  Only 75 emoji are allowed.

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

×   Your previous content has been restored.   Clear editor

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

  • Similar Topics

    • By NASA
      NASA's SpaceX Crew-11 Launch
    • By NASA
      Technicians have successfully installed two sunshields onto NASA’s Nancy Grace Roman Space Telescope’s inner segment. Along with the observatory’s Solar Array Sun Shield and Deployable Aperture Cover, the panels (together called the Lower Instrument Sun Shade), will play a critical role in keeping Roman’s instruments cool and stable as the mission explores the infrared universe.
      To view this video please enable JavaScript, and consider upgrading to a web browser that supports HTML5 video
      This video shows technicians installing two sunshields onto NASA's nearly complete Nancy Grace Roman Space Telescope on July 17. The large yet lightweight panels will block sunlight, keeping Roman’s instruments cool and stable as the mission explores the infrared universe.Credit: NASA/Sophia Roberts The team is on track to join Roman’s outer and inner assemblies this fall to complete the full observatory, which can then undergo further prelaunch testing.
      “This shield is like an extremely strong sunblock for Roman’s sensitive instruments, protecting them from heat and light from the Sun that would otherwise overwhelm our ability to detect faint signals from space,” said Matthew Stephens, an aerospace engineer at NASA’s Goddard Space Flight Center in Greenbelt, Maryland.
      The sunshade, which was designed and engineered at NASA Goddard, is essentially an extension of Roman’s solar panels, except without solar cells. Each sunshade flap is roughly the size of a garage door — about 7 by 7 feet (2.1 by 2.1 meters) — and 3 inches (7.6 centimeters) thick.
      “They’re basically giant aluminum sandwiches, with metal sheets as thin as a credit card on the top and bottom and the central portion made up of a honeycomb structure,” said Conrad Mason, an aerospace engineer at NASA Goddard.
      This design makes the panels lightweight yet stiff, and the material helps limit heat transfer from the side facing the Sun to the back—no small feat considering the front will be hot enough to boil water (up to 216 degrees Fahrenheit, or 102 degrees Celsius) while the back will be much colder than Antarctica’s harshest winter (minus 211 Fahrenheit, or minus 135 Celsius). A specialized polymer film blanket will wrap around each panel to temper the heat, with 17 layers on the Sun side and one on the shaded side.
      The sunshade will be stowed and gently deploy around an hour after launch.
      To view this video please enable JavaScript, and consider upgrading to a web browser that supports HTML5 video
      In this time-lapse video, technicians manually deploy the Lower Instrument Sun Shield for NASA's Nancy Grace Roman Space Telescope. The test helps verify the panels will operate as designed in space.NASA/Sophia Roberts “The deploying mechanisms have dampers that work like soft-close hinges for drawers or cabinets, so the panels won’t slam open and rattle the observatory,” Stephens said. “They each take about two minutes to move into their final positions. This is the very first system that Roman will deploy in space after the spacecraft separates from the launch vehicle.”
      Now completely assembled, Roman’s inner segment is slated to undergo a 70-day thermal vacuum test next. Engineers and scientists will test the full functionality of the spacecraft, telescope, and instruments under simulated space conditions. Following the test, the sunshade will be temporarily removed while the team joins Roman’s outer and inner assemblies, and then reattached to complete the observatory. The mission remains on track for launch no later than May 2027 with the team aiming for as early as fall 2026.
      Click here to virtually tour an interactive version of the telescope Download high-resolution video and images from NASA’s Scientific Visualization Studio
      The Nancy Grace Roman Space Telescope is managed at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, with participation by NASA’s Jet Propulsion Laboratory in Southern California; Caltech/IPAC in Pasadena, California; the Space Telescope Science Institute in Baltimore; and a science team comprising scientists from various research institutions. The primary industrial partners are BAE Systems Inc. in Boulder, Colorado; L3Harris Technologies in Rochester, New York; and Teledyne Scientific & Imaging in Thousand Oaks, California.
      By Ashley Balzer
      NASA’s Goddard Space Flight Center, Greenbelt, Md.
      Share
      Details
      Last Updated Jul 31, 2025 EditorAshley BalzerContactAshley Balzerashley.m.balzer@nasa.govLocationGoddard Space Flight Center Related Terms
      Nancy Grace Roman Space Telescope Dark Energy Dark Matter Exoplanets Galaxies Goddard Space Flight Center Nebulae Sensing the Universe & Multimessenger Astronomy Stars The Universe Explore More
      7 min read One Survey by NASA’s Roman Could Unveil 100,000 Cosmic Explosions
      Article 2 weeks ago 3 min read NASA’s Roman Space Telescope Team Installs Observatory’s Solar Panels
      Article 3 weeks ago 6 min read NASA’s Roman Mission Shares Detailed Plans to Scour Skies
      Article 3 months ago View the full article
    • By NASA
      View of the NASA Glenn Research Center hangar from the Cleveland Hopkins International Airport runway during a testing flight on Thursday, June 13, 2024. The Operations and Integration Building sits to the hangar’s right.Credit: NASA/Sara Lowthian Hanna NASA’s Glenn Research Center in Cleveland is seeking proposals for the use of its historic aircraft hangar, along with a parking lot, tarmac, and a small neighboring office building. Proposals are due by 1 p.m. EDT on Nov. 28.  

      The hangar, formally known as the Flight Research Building, is available for lease by signing a National Historic Preservation Act agreement for a 10-year base period and two optional five-year extensions.

      NASA first announced plans to lease the Flight Research Building and other facilities in May 2024 under the government’s Enhanced Use Lease authority. These lease agreements allow space, aeronautics, and other related industries to use agency land and facilities, reducing NASA’s maintenance costs while fostering strategic partnerships that spur innovation.

      “Glenn is making great progress as we modernize our Cleveland and Sandusky campuses to support NASA’s future missions,” said Dr. Jimmy Kenyon, Glenn’s center director. “Through Enhanced Use Leases, we’re ensuring full use of land and facilities while preserving an iconic, historic building and creating regional economic opportunities.”

      The property available for lease includes up to 6.7 acres of land, which contains the heated aircraft hangar, Operations and Integration Building, parking lot, and tarmac. The hangar is 160 feet by 280 feet, and the Operations and Integration Building is 5,947 square feet. Proceeds from this lease will be used to maintain Glenn facilities and infrastructure. 

      Visible from Brookpark Road and Cleveland Hopkins International Airport, Glenn’s hangar was the first building completed after the center was established in 1941. It has sheltered many unique aircraft used to perform vital research. From studying ice accumulation on aircraft wings to the first use of laser communications to stream 4K video from an aircraft to the International Space Station, Glenn flight research has contributed to aviation safety, atmospheric studies, and cutting-edge technology development.

      Interested parties should contact both Carlos Flores at carlos.a.flores-1@nasa.gov and Diana Munro at diana.c.munro@nasa.gov to sign up for a walk-through from Monday, Sept. 8, to Friday, Sept. 12, or the week of Oct. 6.  

      For a 360-degree virtual tour of the Flight Research Building, visit:
      https://www3.nasa.gov/specials/hangar360/
      -end-
      Jan Wittry
      Glenn Research Center, Cleveland
      216-433-5466
      jan.m.wittry-1@nasa.gov
      Share
      Details
      Last Updated Jul 31, 2025 Related Terms
      Doing Business with NASA Glenn Research Center Media Resources Explore More
      3 min read NASA Drop Test Supports Safer Air Taxi Design and Certification
      Article 3 days ago 3 min read NASA Rehearses How to Measure X-59’s Noise Levels
      Article 6 days ago 4 min read NASA Tests 5G-Based Aviation Network to Boost Air Taxi Connectivity
      Article 1 week ago Keep Exploring Discover Related Topics
      Missions
      Humans in Space
      Climate Change
      Solar System

      View the full article
    • By NASA
      2 min read
      Preparations for Next Moonwalk Simulations Underway (and Underwater)
      NASA/Lori Losey
      The best way to solve a mystery is by gathering evidence and building a case. That’s exactly what NASA researchers are doing with a series of research flights aimed at advancing a sensor for supersonic parachutes. The clues they find could help make these parachutes more reliable and safer for delivering scientific instruments and payloads to Mars.
      These investigative research flights are led by the EPIC (Enhancing Parachutes by Instrumenting the Canopy) team at NASA’s Armstrong Fight Research Center in Edwards, California. During a June flight test, a quadrotor aircraft, or drone, air-launched a capsule that deployed a parachute equipped with a sensor. The flexible, strain-measuring sensor attached to the parachute did not interfere with the canopy material, just as the EPIC team had predicted. The sensors also provided data, a bonus for planning upcoming tests.
      “Reviewing the research flights will help inform our next steps,” said Matt Kearns, project manager for EPIC at NASA Armstrong. “We are speaking with potential partners to come up with a framework to obtain the data that they are interested in pursuing. Our team members are developing methods for temperature testing the flexible sensors, data analysis, and looking into instrumentation for future tests.”
      The flight tests were a first step toward filling gaps in computer models to improve supersonic parachutes. This work could also open the door to future partnerships, including with the aerospace and auto racing industries.
      NASA’s Space Technology Mission Directorate (STMD) funds the EPIC work through its Entry Systems Modeling project at NASA’s Ames Research Center in California’s Silicon Valley. The capsule and parachute system were developed by NASA’s Langley Research Center in Hampton, Virginia. NASA Armstrong interns worked with Langley to build and integrate a similar system for testing at NASA Armstrong. An earlier phase of the work focused on finding commercially available flexible strain sensors and developing a bonding method as part of an STMD Early Career Initiative project.
      NASA researchers Paul Bean, center, and Mark Hagiwara, right, attach the capsule with parachute system to the Enhancing Parachutes by Instrumenting the Canopy test experiment on June 4, 2025, at NASA’s Armstong Flight Research Center in Edwards, California. NASA researchers are developing technology to make supersonic parachutes safer and more reliable for delivering science instruments and payloads to Mars.NASA/Christopher LC Clark Derek Abramson, left, and Justin Link, right, attach an Alta X drone to the Enhancing Parachutes by Instrumenting the Canopy test experiment on June 4, 2025, at NASA’s Armstong Flight Research Center in Edwards, California. Abramson is NASA chief engineer at the center’s Dale Reed Subscale Flight Research Laboratory, where Link also works as a pilot for small uncrewed aircraft systems. NASA researchers are developing technology to make supersonic parachutes safer and more reliable for delivering science instruments and payloads to Mars.NASA/Christopher LC Clark An Alta X drone is positioned at altitude for an air launch of the Enhancing Parachutes by Instrumenting the Canopy test experiment on June 4, 2025, at NASA’s Armstong Flight Research Center in Edwards, California. NASA researchers are developing technology to make supersonic parachutes safer and more reliable for delivering science instruments and payloads to Mars.NASA/Christopher LC Clark The parachute of the Enhancing Parachutes by Instrumenting the Canopy test experiment deploys following an air launch from an Alta X drone on June 4, 2025, at NASA’s Armstong Flight Research Center in Edwards, California. NASA researchers are developing technology to make supersonic parachutes safer and more reliable for delivering science instruments and payloads to Mars.NASA/Christopher LC Clark The Enhancing Parachutes by Instrumenting the Canopy project team examines a capsule and parachute following an air launch from an Alta X drone on June 4, 2025, at NASA’s Armstong Flight Research Center in Edwards, California. NASA researchers are developing technology to make supersonic parachutes safer and more reliable for delivering science instruments and payloads to Mars.NASA/Christopher LC Clark Share
      Details
      Last Updated Jul 29, 2025 EditorDede DiniusContactJay Levinejay.levine-1@nasa.gov Related Terms
      Ames Research Center Armstrong Flight Research Center Flight Innovation Langley Research Center Space Technology Mission Directorate Technology Explore More
      3 min read NASA Drop Test Supports Safer Air Taxi Design and Certification
      Article 2 days ago 3 min read NASA Rehearses How to Measure X-59’s Noise Levels
      Article 5 days ago 4 min read NASA Scientist Finds Predicted Companion Star to Betelgeuse
      Article 7 days ago Keep Exploring Discover More Topics From NASA
      Armstrong Flight Research Center
      Humans in Space
      Climate Change
      Solar System
      View the full article
    • By NASA
      The Indian Space Research Organisation’s Geosynchronous Satellite Launch Vehicle lifts off from Satish Dhawan Space Centre on India’s southeastern coast at 8:10 a.m. EDT (5:40 a.m. IST), July 30, 2025.Credit: ISRO Carrying an advanced radar system that will produce a dynamic, three-dimensional view of Earth in unprecedented detail, the NISAR (NASA-ISRO Synthetic Aperture Radar) satellite has launched from Satish Dhawan Space Centre in Sriharikota, Andhra Pradesh, India.
      Jointly developed by NASA and the Indian Space Research Organisation (ISRO), and a critical part of the United States – India civil-space cooperation highlighted by President Trump and Prime Minister Modi earlier this year, the satellite can detect the movement of land and ice surfaces down to the centimeter. The mission will help protect communities by providing unique, actionable information to decision-makers in a diverse range of areas, including disaster response, infrastructure monitoring, and agricultural management. 
      The satellite lifted off aboard an ISRO Geosynchronous Satellite Launch Vehicle (GSLV) rocket at 8:10 a.m. EDT (5:10 p.m. IST), Wednesday, July 30. The ISRO ground controllers began communicating with NISAR about 20 minutes after launch, at just after 8:29 a.m. EDT, and confirmed it is operating as expected.
      “Congratulations to the entire NISAR mission team on a successful launch that spanned across multiple time zones and continents in the first-ever partnership between NASA and ISRO on a mission of this sheer magnitude,” said Nicky Fox, associate administrator, Science Mission Directorate at NASA Headquarters in Washington. “Where moments are most critical, NISAR’s data will help ensure the health and safety of those impacted on Earth, as well as the infrastructure that supports them, for the benefit of all.”
      From 464 miles (747 kilometers) above Earth, NISAR will use two advanced radar instruments to track changes in Earth’s forests and wetland ecosystems, monitor deformation and motion of the planet’s frozen surfaces, and detect the movement of Earth’s crust down to fractions of an inch — a key measurement in understanding how the land surface moves before, during, and after earthquakes, volcanic eruptions, and landslides.
      “ISRO’s GSLV has precisely injected NISAR satellite into the intended orbit, 747 kilometers. I am happy to inform that this is GSLV’s first mission to Sun-synchronous polar orbit. With this successful launch, we are at the threshold of fulfilling the immense scientific potential NASA and ISRO envisioned for the NISAR mission more than 10 years ago,” said ISRO Chairman V Narayanan. “The powerful capability of this radar mission will help us study Earth’s dynamic land and ice surfaces in greater detail than ever before.”
      The mission’s two radars will monitor nearly all the planet’s land- and ice-covered surfaces twice every 12 days, including areas of the polar Southern Hemisphere rarely covered by other Earth-observing radar satellites. The data NISAR collects also can help researchers assess how forests, wetlands, agricultural areas, and permafrost change over time.
      “Observations from NISAR will provide new knowledge and tangible benefits for communities both in the U.S. and around the world,” said Karen St. Germain, director, Earth Science division at NASA Headquarters. “This launch marks the beginning of a new way of seeing the surface of our planet so that we can understand and foresee natural disasters and other changes in our Earth system that affect lives and property.”
      The NISAR satellite is the first free-flying space mission to feature two radar instruments — an L-band system and an S-band system. Each system is sensitive to features of different sizes and specializes in detecting certain attributes. The L-band radar excels at measuring soil moisture, forest biomass, and motion of land and ice surfaces, while S-band radar excels at monitoring agriculture, grassland ecosystems, and infrastructure movement.
      Together, the radar instruments will enhance all of the satellite’s observations, making NISAR more capable than previous synthetic aperture radar missions. Unlike optical sensors, NISAR will be able to “see” through clouds, making it possible to monitor the surface during storms, as well as in darkness and light.
      NASA’s Jet Propulsion Laboratory in Southern California provided the L-band radar, and ISRO’s Space Applications Centre in Ahmedabad developed the S-band radar. The NISAR mission marks the first time the two agencies have co-developed hardware for an Earth-observing mission.
      “We’re proud of the international team behind this remarkable satellite. The mission’s measurements will be global but its applications deeply local, as people everywhere will use its data to plan for a resilient future,” said Dave Gallagher, director, NASA JPL, which manages the U.S. portion of the mission for NASA. “At its core is synthetic aperture radar, a technology pioneered at NASA JPL that enables us to study Earth night and day, through all kinds of weather.”
      Including L-band and S-band radars on one satellite is an evolution in SAR airborne and space-based missions that, for NASA, started in 1978 with the launch of Seasat. In 2012, ISRO began launching SAR missions starting with Radar Imaging Satellite (RISAT-1), followed by RISAT-1A in 2022, to support a wide range of applications in India.
      In the coming weeks, the spacecraft will begin a roughly 90-day commissioning phase during which it will deploy its 39-foot (12-meter) radar antenna reflector. This reflector will direct and receive microwave signals from the two radars. By interpreting the differences between the two, researchers can discern characteristics about the surface below. As NISAR passes over the same locations twice every 12 days, scientists can evaluate how those characteristics have changed over time to reveal new insights about Earth’s dynamic surfaces.
      The NISAR mission is an equal collaboration between NASA and ISRO. Managed for the agency by Caltech, NASA JPL leads the U.S. component of the project and is providing the mission’s L-band SAR. NASA also is providing the radar reflector antenna, the deployable boom, a high-rate communication subsystem for science data, GPS receivers, a solid-state recorder, and payload data subsystem.
      Space Applications Centre Ahmedabad, ISRO’s lead center for payload development, is providing the mission’s S-band SAR instrument and is responsible for its calibration, data processing, and development of science algorithms to address the scientific goals of the mission. U R Rao Satellite Centre in Bengaluru, which leads the ISRO components of the mission, is providing the spacecraft bus. The launch vehicle is from ISRO’s Vikram Sarabhai Space Centre, launch services are through ISRO’s Satish Dhawan Space Centre, and satellite operations are by ISRO Telemetry Tracking and Command Network. National Remote Sensing Centre in Hyderabad is responsible for S-band data reception, operational products generation, and dissemination.
      To learn more about NISAR, visit:
      https://nisar.jpl.nasa.gov
      -end-
      Karen Fox / Elizabeth Vlock
      Headquarters, Washington
      202-358-1600
      karen.c.fox@nasa.gov / elizabeth.a.vlock@nasa.gov
      Andrew Wang / Jane J. Lee
      Jet Propulsion Laboratory, Pasadena, Calif.
      626-379-6874 / 818-354-0307
      andrew.wang@jpl.nasa.gov / jane.j.lee@jpl.nasa.gov
      Share
      Details
      Last Updated Jul 30, 2025 EditorJessica TaveauLocationNASA Headquarters Related Terms
      NISAR (NASA-ISRO Synthetic Aperture Radar) Earth Science Earth Science Division Jet Propulsion Laboratory NASA Headquarters Science Mission Directorate View the full article
  • Check out these Videos

×
×
  • Create New...