Jump to content

Lunar Autonomy Mobility Pathfinder Workshop: A NASA Chief Technologist Sponsored Workshop


NASA

Recommended Posts

  • Publishers
4 Min Read

Lunar Autonomy Mobility Pathfinder Workshop: A NASA Chief Technologist Sponsored Workshop

gsfc-20171208-archive-e000868large.jpg?w

OVERVIEW

The NASA chief technologist’s team, within the Office of Technology, Policy, and Strategy (OTPS), is hosting a Lunar Autonomy Mobility Pathfinder (LAMP) workshop on Tuesday, November 12, 2024, to provide a community forum to discuss modeling and simulation testbeds in this domain. The workshop is in coordination with NASA’s Space Technology Mission Directorate. 

With the Artemis campaign, NASA will land the first woman and first person of color on the Moon, using innovative technologies to explore more of the lunar surface than ever before. Technologies like trusted autonomy are necessary to support these types of sustained operations. Trusted autonomy is a more robust level of autonomy designed for long-term operational use. 

The LAMP workshop will be held on Tuesday, November 12, 2024, from 10 a.m. to 5 p.m. PST at the University of Nevada Las Vegas (UNLV) Black Fire Innovation Facility in Las Vegas, Nevada. The Black Fire Innovation Center Building is located at 8400 W. Sunset Blvd. Las Vegas, NV 89113, approximately 20 minutes from the UNLV main campus. 

This workshop has been designed to coincide with the 2024 Lunar Surface Innovation Consortium fall meeting (also taking place in Las Vegas, Nevada).  

The OTPS solver-in-residence is the main organizer and facilitator for this workshop.

PROGRAM 

The LAMP workshop will provide a forum for a discussion on topics that include: 

  • A modeling and simulation (M&S) pathfinder to explore an integrated sim environment for lunar stakeholders from commercial industry, other U.S. government agencies, international partners and academia, to simulate their systems that would eventually operate in the lunar environment and to test interoperability between systems.     
  • How to leverage the planned rover missions to 1) calibrate and improve this M&S environment over time, and 2) potentially use them as autonomy testbeds to safely mature algorithms in a relevant environment. 

Please RSVP for in-person or virtual attendance by registering at the following site:
 https://nasaevents.webex.com/weblink/register/rdf4dd38bc3bf176dc32d147513f7b77c

*Please note registration is on an individual basis. If attending with multiple guests, each guest must register for the event separately. 

LAMP Workshop Agenda

(All times listed are in PST and subject to change)

10:00 a.m. 12:00p.m.Modeling and Simulation (M&S) showcase(In-person only & optional)
This is an opportunity for interested participants to show their lunar simulation capabilities inside of UNLV’s Blackfire Innovation esports arena. Space is limited. Please indicate if you are interested in participating when you register, and we will reach out with additional information. 
1:00 –2:00p.m.Challenges to Developing Trusted Autonomy 
NASA will discuss the challenges of maturing autonomy that can be trusted to operate over long periods of time and how we can work together to overcome those challenges.
2:00 –3:00p.m.Pre-Formulation Discussion of a Lunar Autonomy Mobility Pathfinder Modeling and Simulation Environment
Subject matter experts (SMEs) from NASA will layout thoughts on what a digital transformation pathfinder would look like that benefits lunar autonomy efforts across the globe. 
3:00 – 3:15p.m.Break
3:15 – 4:15p.m.Lunar Testbeds Discussion
This will be a discussion focused on how assets on the moon could be used as testbeds to generate truth data for Earth-based simulations and to validate that autonomy can be trusted in the lunar environment.
4:15 – 5:00p.m.Polling and Discussions
Audience feedback will be solicited on various topics. This will include a pre-formulated series of questions and real time polls.

CONTACT 

For questions, please email:

Dr. Adam Yingling

Dr. Adam Yingling
2024 OTPS Solver-in-Residence
Office of Technology, Policy, and Strategy (OTPS) 
NASA Headquarters 
Email: adam.j.yingling@nasa.gov

The Solver-in-Residence (SiR) program is a one-year detail position with the chief technologist in NASA’s Office of Technology Policy and Strategy. The program enables a NASA civil servant to propose a one-year investigation on a specific technology challenge and then work to identify solutions to address those challenges.

Share

Details

Last Updated
Oct 10, 2024
Editor
Bill Keeter

View the full article

Link to comment
Share on other sites

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
      2 min read
      Preparations for Next Moonwalk Simulations Underway (and Underwater)
      The Ohio State University Marching Band pays tribute to NASA with a NASA worm logo formation. Credit: NASA/Brian Newbacher  The Ohio State University (OSU) teamed up with NASA’s Glenn Research Center in Cleveland for a multi-faceted tribute to NASA on Sept 21. During a home football game against Marshall University, OSU’s Marching Band recognized the agency with a NASA-themed halftime show, in-game salute, and tribute to Glenn and two alums who play significant roles in NASA’s spaceflight operations.  
      NASA Glenn Center Director Dr. Jimmy Kenyon and NASA employees and Ohio State alums Jeff and Molly Radigan are recognized by more than 100,000 fans in Ohio Stadium. Credit: NASA/Brian Newbacher  The event kicked off in the morning during the Skull Session (pep rally) at St. John Arena on OSU’s campus. Public Address Announcer Wes Clark talked with Center Director Dr. Jimmy Kenyon, who shared information about Glenn and thanked OSU for the honor. During a special spotlight, Kenyon and OSU alums who now work at NASA’s Kennedy Space Center – Jeff Radigan, a NASA flight director, and Molly Radigan, deputy chief of Space Flight Systems – came onto the field to be recognized. 
      The Ohio State University Marching Band pays tribute to NASA while in formation of an astronaut on the Moon. Credit: NASA/Brian Newbacher  At halftime, a special astronaut video from the International Space Station introduced the NASA-themed show. The band then blasted off with its space-themed performance that included several songs — from “Fly Me to the Moon” to “Starman.” The talented band members marched in formations that included an astronaut and spaceship blasting off, garnering excitement for NASA and cheers from the audience. 
      Back to Newsletter Explore More
      1 min read Dr. Rickey Shyne Named Crain’s Notable Black Leader 
      Article 14 mins ago 1 min read NASA Glenn Connects with Morehead State University  
      Article 15 mins ago 1 min read Visitors Explore NASA at Ingenuity Fest 
      Article 15 mins ago View the full article
    • By NASA
      1 min read
      Preparations for Next Moonwalk Simulations Underway (and Underwater)
      The Harvest Moon refers to the nearest full Moon to the autumnal equinox. The Moon appeared full for about three days last month from the evening of Monday, Sept. 16, through Thursday morning, Sept. 19. The brightest Moon was on Sept. 17. 
      NASA’s Glenn Research Center photographers captured images of this supermoon as it shone across Cleveland. Here’s how they described it: 
      “Complex.” Sara Lowthian-Hanna captured this composite image of the Moon above a Guardians of Traffic statue near downtown Cleveland. The Sept. 17 Harvest Moon had a lot going on: it was full, a supermoon, and experienced a partial lunar eclipse (when the Earth’s shadow falls upon the Moon’s surface). Credit: NASA/Sara Lowthian-Hanna  “Shy.” Quentin Schwinn patiently waited for the Moon to peek out from behind clouds above the hangar at NASA’s Glenn Research Center. He took this shot just as a plane whizzed in front of the face of the Moon. Credit: NASA/Quentin Schwinn  “Epic.” Jef Janis captured this shot of the Moon above the colorfully illuminated Rock & Roll Hall of Fame in downtown Cleveland. Credit: NASA/Jef Janis  “Dramatic.” Jordan Salkin took this up-close image of wispy aircraft contrails crossing the face of the Moon. Credit: NASA/Jordan Salkin  Return to Newsletter Explore More
      1 min read Dr. Rickey Shyne Named Crain’s Notable Black Leader 
      Article 14 mins ago 2 min read Ohio State Marching Band Performs Tribute to NASA 
      Article 14 mins ago 1 min read NASA Glenn Connects with Morehead State University  
      Article 15 mins ago View the full article
    • By NASA
      1 min read
      Preparations for Next Moonwalk Simulations Underway (and Underwater)
      Artemis II crew members (left to right) Reid Wiseman, Christina Koch, and Jeremy Hansen share information about themselves and their mission during a town hall at NASA’s Glenn Research Center in Cleveland. Credit: NASA/Sara Lowthian-Hanna  Three of the four astronauts who will venture around the Moon on Artemis II, the first crewed flight paving the way for future lunar surface missions, visited NASA’s Glenn Research Center in Cleveland, Sept. 10-11. NASA Glenn is an integral part of the development of the Orion spacecraft and a leader in propulsion, power, and communications research. 
      Commander Reid Wiseman  and Mission Specialists  Christina Koch and Jeremy Hansen (Canadian Space Agency) discussed their upcoming mission and hosted a question-and-answer session during town hall events at Lewis Field in Cleveland and NASA’s Neil Armstrong Test Facility in Sandusky, Ohio. Victor Glover, who was unable to attend, is the pilot and fourth crew member. Both events included tours and recognition of employees who have contributed to the success of Artemis missions.  
      Artemis II crew members Reid Wiseman, Christina Koch, and Jeremy Hansen (left to right, wearing blue flight suits) and other NASA personnel look down into the stainless-steel vacuum chamber in the In-Space Propulsion Facility at NASA’s Neil Armstrong Test Facility in Sandusky, Ohio. This is the world’s only facility capable of testing full-scale upper stage launch vehicles and rocket engines under simulated high-altitude conditions.Credit: NASA/Sara Lowthian-Hanna  The Artemis II crew will lift off on an approximately 10-day mission from Launch Complex 39B at NASA’s Kennedy Space Center in Florida, blazing beyond Earth’s grasp atop the agency’s mega Moon rocket. The crew will check out Orion’s systems and perform a targeting demonstration test relatively close to Earth before venturing around the Moon.  
      Back to Newsletter Explore More
      1 min read Dr. Rickey Shyne Named Crain’s Notable Black Leader 
      Article 14 mins ago 2 min read Ohio State Marching Band Performs Tribute to NASA 
      Article 14 mins ago 1 min read NASA Glenn Connects with Morehead State University  
      Article 15 mins ago View the full article
    • By NASA
      6 min read
      NASA, NOAA: Sun Reaches Maximum Phase in 11-Year Solar Cycle
      In a teleconference with reporters on Tuesday, representatives from NASA, the National Oceanic and Atmospheric Administration (NOAA), and the international Solar Cycle Prediction Panel announced that the Sun has reached its solar maximum period, which could continue for the next year.
      The solar cycle is a natural cycle the Sun goes through as it transitions between low and high magnetic activity. Roughly every 11 years, at the height of the solar cycle, the Sun’s magnetic poles flip — on Earth, that’d be like the North and South poles swapping places every decade — and the Sun transitions from being calm to an active and stormy state.
      Visible light images from NASA’s Solar Dynamics Observatory highlight the appearance of the Sun at solar minimum (left, Dec. 2019) versus solar maximum (right, May 2024). During solar minimum, the Sun is often spotless. Sunspots are associated with solar activity and are used to track solar cycle progress. For these images and more relating to solar maximum, visit https://svs.gsfc.nasa.gov/14683.
      NASA/SDO Images from NASA’s Solar Dynamics Observatory highlight the appearance of the Sun at solar minimum (left, December 2019) versus solar maximum (right, May 2024). These images are in the 171-angstrom wavelength of extreme ultraviolet light, which reveals the active regions on the Sun that are more common during solar maximum. For these images and more relating to solar maximum, visit https://svs.gsfc.nasa.gov/14683.
      NASA/SDO




      NASA and NOAA track sunspots to determine and predict the progress of the solar cycle — and ultimately, solar activity. Sunspots are cooler regions on the Sun caused by a concentration of magnetic field lines. Sunspots are the visible component of active regions, areas of intense and complex magnetic fields on the Sun that are the source of solar eruptions.
      “During solar maximum, the number of sunspots, and therefore, the amount of solar activity, increases,” said Jamie Favors, director, Space Weather Program at NASA Headquarters in Washington. “This increase in activity provides an exciting opportunity to learn about our closest star — but also causes real effects at Earth and throughout our solar system.”
      The solar cycle is the natural cycle of the Sun as it transitions between low and high activity. During the most active part of the cycle, known as solar maximum, the Sun can unleash immense explosions of light, energy, and solar radiation — all of which create conditions known as space weather. Space weather can affect satellites and astronauts in space, as well as communications systems — such as radio and GPS — and power grids on Earth.
      Credits: Beth Anthony/NASA Solar activity strongly influences conditions in space known as space weather. This can affect satellites and astronauts in space, as well as communications and navigation systems — such as radio and GPS — and power grids on Earth. When the Sun is most active, space weather events become more frequent. Solar activity has led to increased aurora visibility and impacts on satellites and infrastructure in recent months.
      During May 2024, a barrage of large solar flares and coronal mass ejections (CMEs) launched clouds of charged particles and magnetic fields toward Earth, creating the strongest geomagnetic storm at Earth in two decades — and possibly among the strongest displays of auroras on record in the past 500 years.
      May 3–May 9, 2024, NASA’s Solar Dynamics Observatory observed 82 notable solar flares. The flares came mainly from two active regions on the Sun called AR 13663 and AR 13664. This video highlights all flares classified at M5 or higher with nine categorized as X-class solar flares.
      Credit: NASA “This announcement doesn’t mean that this is the peak of solar activity we’ll see this solar cycle,” said Elsayed Talaat, director of space weather operations at NOAA. “While the Sun has reached the solar maximum period, the month that solar activity peaks on the Sun will not be identified for months or years.”
      Scientists will not be able to determine the exact peak of this solar maximum period for many months because it’s only identifiable after they’ve tracked a consistent decline in solar activity after that peak. However, scientists have identified that the last two years on the Sun have been part of this active phase of the solar cycle, due to the consistently high number of sunspots during this period. Scientists anticipate that the maximum phase will last another year or so before the Sun enters the declining phase, which leads back to solar minimum. Since 1989, the Solar Cycle Prediction Panel — an international panel of experts sponsored by NASA and NOAA — has worked together to make their prediction for the next solar cycle.
      Solar cycles have been tracked by astronomers since Galileo first observed sunspots in the 1600s. Each solar cycle is different — some cycles peak for larger and shorter amounts of time, and others have smaller peaks that last longer.
      Sunspot number over the previous 24 solar cycles. Scientists use sunspots to track solar cycle progress; the dark spots are associated with solar activity, often as the origins for giant explosions — such as solar flares or coronal mass ejections — which can spew light, energy, and solar material out into space. For these images and more relating to solar maximum, visit https://svs.gsfc.nasa.gov/14683.
      NOAA’s Space Weather Prediction Center “Solar Cycle 25 sunspot activity has slightly exceeded expectations,” said Lisa Upton, co-chair of the Solar Cycle Prediction Panel and lead scientist at Southwest Research Institute in San Antonio, Texas. “However, despite seeing a few large storms, they aren’t larger than what we might expect during the maximum phase of the cycle.”
      The most powerful flare of the solar cycle so far was an X9.0 on Oct. 3 (X-class denotes the most intense flares, while the number provides more information about its strength).
      NOAA anticipates additional solar and geomagnetic storms during the current solar maximum period, leading to opportunities to spot auroras over the next several months, as well as potential technology impacts. Additionally, though less frequent, scientists often see fairly significant storms during the declining phase of the solar cycle.
      The Solar Cycle 25 forecast, as produced by the Solar Cycle 25 Prediction Panel. Sunspot number is an indicator of solar cycle strength — the higher the sunspot number, the stronger the cycle. For these images and more relating to solar maximum, visit https://svs.gsfc.nasa.gov/14683.
      NOAA’s Space Weather Prediction Center NASA and NOAA are preparing for the future of space weather research and prediction. In December 2024, NASA’s Parker Solar Probe mission will make its closest-ever approach to the Sun, beating its own record of closest human-made object to the Sun. This will be the first of three planned approaches for Parker at this distance, helping researchers to understand space weather right at the source.
      NASA is launching several missions over the next year that will help us better understand space weather and its impacts across the solar system.
      Space weather predictions are critical for supporting the spacecraft and astronauts of NASA’s Artemis campaign. Surveying this space environment is a vital part of understanding and mitigating astronaut exposure to space radiation. 
      NASA works as a research arm of the nation’s space weather effort. To see how space weather can affect Earth, please visit NOAA’s Space Weather Prediction Center, the U.S. government’s official source for space weather forecasts, watches, warnings, and alerts.
      By Abbey Interrante
      NASA’s Goddard Space Flight Center, Greenbelt, Md.
      Media Contact:
      Sarah Frazier, NASA’s Goddard Space Flight Center, Greenbelt, Md.
      sarah.frazier@nasa.gov
      About the Author
      Abbey Interrante

      Share








      Details
      Last Updated Oct 15, 2024 Related Terms
      Goddard Space Flight Center Heliophysics Heliophysics Division Parker Solar Probe (PSP) Solar Science Sunspots The Sun The Sun & Solar Physics Explore More
      3 min read Eclipse Megamovie Coding Competition


      Article


      5 hours ago
      2 min read ESA/NASA’s SOHO Spies Bright Comet Making Debut in Evening Sky
      The Solar and Heliospheric Observatory (SOHO) has captured images of the second-brightest comet to ever pass…


      Article


      4 days ago
      2 min read Hubble Spots a Grand Spiral of Starbursts


      Article


      4 days ago
      Keep Exploring Discover More Topics From NASA
      Sunspots



      Solar Storms and Flares


      Solar storms and flares are eruptions from the Sun that can affect us here on Earth.


      Sun



      Parker Solar Probe


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

      View the full article
    • By NASA
      6 min read
      Preparations for Next Moonwalk Simulations Underway (and Underwater)
      A natural color view from Cassini of Saturn with its Titan moon in the foreground in August 2012. Titan’s diameter is 50% larger than Earth’s moon.Credit: NASA NASA’s ambitious Cassini mission to Saturn in the late 1990s was one of the agency’s greatest accomplishments, providing unprecedented revelations about the esoteric outer planet and its moons. The complex undertaking was also a tremendous, yet bittersweet, achievement for the Lewis Research Center (today, NASA’s Glenn Research Center in Cleveland), which oversaw the rockets that propelled Cassini to Saturn. Cassini brought a close to over 35 years of Lewis’ management of NASA’s launch vehicles.
      Cassini Mission: 5 Things to Know About NASA Lewis’ Last Launch
      1. NASA Lewis Launched the Largest and Most Complex Deep-Space Mission to Date
      In the early 1980s, NASA began planning the first-ever in-depth study of the planet Saturn. The mission would use the Cassini orbiter designed by NASA’s Jet Propulsion Laboratory in Southern California and the European Space Agency’s Huygens lander. It was one of the heaviest and most complex interplanetary spacecraft ever assembled. Cassini’s plutonium power system and intricate flight path further complicated the mission.
      NASA Lewis was responsible for managing the launches of government missions involving the Centaur upper stage and the Atlas and Titan boosters. Cassini’s 6-ton payload forced Lewis to use the U.S. Air Force’s three-stage Titan IV, the most powerful vehicle available, and pair it with the most advanced version of the Centaur, referred to as G-prime.
      The Titan IV shroud in the Space Power Facility in October 1990. It was only the second test since the world-class facility had been brought back online after over a decade in standby conditions.Credit: NASA/Quentin Schwinn 2. Lewis Performed Hardware Testing for the Cassini Launch
      One of NASA Lewis’ primary launch responsibilities was integrating the payload and upper stages with the booster. This involved balancing weight requirements, providing adequate insulation for Centaur’s cryogenic propellants, determining correct firing times for the stages, and ensuring that that the large shroud, which encapsulated both the upper stage and payload, jettisoned cleanly after launch.
      By the time of Cassini, the center had been testing shrouds (including the Titan III fairing) in simulated space conditions for over 25 years. NASA’s Space Power Facility possesses the world’s largest vacuum chamber and was large enough to accommodate the Titan IV’s 86-foot-tall, 16-foot-diameter fairing. In the fall of 1990, the shroud was installed in the chamber, loaded with weights that simulated the payload, and subjected to atmospheric pressures found at an altitude of 72 miles.
      The system was successfully separated in less than half a second. Using simulated Cassini and Centaur vehicles, NASA engineers also redesigned a thicker thermal blanket that would protect Cassini’s power system from acoustic vibrations during liftoff.


      Members of NASA Lewis’ Launch Vehicle Directorate pose with a Centaur model in May 1979 to mark the 50th successful launch of the Atlas/Centaur.Credit: NASA/Martin Brown 3. Lewis Personnel Assisted with the Launch
      In late August 1997, a group of NASA Lewis engineers traveled to NASA’s Kennedy Space Center in Florida to make final preparations for the Cassini launch, working with Air Force range safety personnel at Patrick Air Force Base to ensure a safe launch under all circumstances.
      After an aborted launch two days earlier, the vehicle was readied for another attempt in the evening of October 14. Lewis personnel took stations in the Launch Vehicle Data Center inside Hangar AE to monitor the launch vehicle’s temperature, pressure, speed, trajectory, and vibration during the launch. The weather was mild, and the countdown proceeded into the morning hours of October 15 without any major issues.
      At 4:43 a.m. EDT, Titan’s first stage and the two massive solid rocket motors roared to life, and the vehicle rose into the dark skies over Florida. The Lewis launch team monitored the flight as the vehicle exited Earth’s atmosphere, Titan burned through its stages, and Centaur sent Cassini out of Earth orbit and on its 2-billion-mile journey to Saturn. After a successful spacecraft separation, Lewis’ responsibilities were complete. The launch had gone exceedingly well. 

      This illustration depicts the Cassini orbiter with the Huygens lander descending to the Titan moon (left) and Saturn in the background.Credit: NASA 4. Cassini-Huygens Brought a Close to Decades of Lewis Launch Operations
      Cassini-Huygens was NASA Lewis’ 119th and final launch, and it brought to a close the center’s decades of launch operations. The center had been responsible for NASA’s upper-stage vehicles since the fall of 1962. The primary stages were the Agena, which had 28 successful launches, and Centaur, which has an even more impressive track record and remains in service today.
      While Lewis continued to handle vehicle integration and other technical issues for launches of NASA payloads, in the 1980s, NASA began transferring launch responsibilities to commercial entities. In the mid-1990s, NASA underwent a major realignment that consolidated all launch vehicle responsibilities at NASA Kennedy.
      So it was with mixed emotions that around 20 Lewis employees and retirees gathered at the Cleveland center in the early morning hours of Oct. 15, 1997, to watch the Cassini launch. The group held its cheers for 40 minutes after liftoff until Lewis’ responsibilities concluded for the last time with the safe separation of Cassini from Centaur. “In many ways, this is the end of an era, across the agency and, in particular, here at Lewis,” noted one engineer from the Launch Vehicle and Transportation Office.

      The Titan IV/Centaur lifts off from Launch Complex 40 at Cape Canaveral on Oct. 15, 1997. NASA Lewis engineers were monitoring the launch from Hangar AE, roughly 3.5 miles to the south. Credit: NASA 5. Cassini Made Groundbreaking Discoveries That Inform Today’s NASA Missions
      Cassini’s seven-year voyage to Saturn included flybys of Venus (twice), Earth, and Jupiter so that the planets’ gravitational forces could accelerate the spacecraft. Cassini entered Saturn’s orbit in June 2004 and began relaying data and nearly half a million images back to Earth. Huygens separated from the spacecraft and descended to the surface of the Saturn’s largest moon, Titan, in January 2005. It was the first time a vehicle ever landed on a celestial body in the outer solar system.
      Cassini went on to make plunges into the planet’s upper atmosphere and through Saturn’s rings.  Scientific information on the mysterious planet, its moons, and rings led to the publication of nearly 4,000 technical papers. After over 13 years and nearly 300 orbits, on Sept. 15, 2017, NASA intentionally sent Cassini plummeting into the atmosphere where it burned up, ending its remarkable mission.
      NASA engineers used their experiences from the Cassini mission to help design the Europa Clipper, which is intended to perform flybys of Jupiter’s moon Europa. Europa Clipper launched on Oct. 14.

      Keep Exploring
      Read the “Sending Cassini to Saturn” Series from NASA Glenn Visit NASA’s Cassini-Huygens Website Visit the European Space Agency’s Cassini-Huygens Website Watch NASA Coverage of the Cassini Launch See NASA Glenn’s Historic Centaur Rocket Display
      Explore More
      24 min read NASA Celebrates Hispanic Heritage Month 2024
      Article 4 days ago 3 min read Pioneering NASA Astronaut Health Tech Thwarts Heart Failure
      Article 4 days ago 8 min read Kathryn Sullivan: The First American Woman to Walk in Space
      Article 5 days ago View the full article
  • Check out these Videos

×
×
  • Create New...