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Launched in 1977, the twin Voyager probes are NASA’s longest-operating mission and the only spacecraft ever to explore interstellar space. For two decades after launch, the spacecraft were planetary explorers, giving us up-close views of the gas giants Jupiter, Saturn, Uranus, and Neptune. Now, as they reach distances far beyond the hopes of their original designers, the aging spacecraft challenge their team in new ways, requiring creative solutions to keep them operating and sending back science data from the space between the stars. As we celebrate the 45th anniversary of these epic explorers, join Voyager deputy project scientist Linda Spilker and propulsion engineer Todd Barber for a live Q&A.

NASA’s Double Asteroid Redirection Test, also known as DART, is humanity’s first attempt to change the motion of a non-hazardous asteroid in space by intentionally crashing a spacecraft into it. After impact, ground-based observatories across the globe will turn their eyes to the skies to determine if this planetary defense test was successful. In this video, NASA visits Lowell Observatory to learn more about how astronomers have been tracking this double asteroid over the course of many years, and how they will document the orbital change post-impact. DART is a spacecraft designed to impact an asteroid as a test of technology. DART’s target asteroid is NOT a threat to Earth. This asteroid system is a perfect testing ground to see if intentionally crashing a spacecraft into an asteroid is an effective way to change its course, should a hazardous asteroid be discovered in the future. For more on DART, visit https://nasa.gov/dart. Credit: NASA

"Best day of my whole life. Ever." Watch the reactions of a group of students, joined by NASA Administrator Bill Nelson and NASA Associate Administrator Bob Cabana, who hopped on a tour bus at Kennedy Space Center for an opportunity of a lifetime to view the Artemis I Space Launch System rocket and Orion spacecraft in the Vehicle Assembly Building's High Bay 3. #Artemis I is scheduled to launch no earlier than Aug. 29 at 8:33 a.m. EDT from the center’s Launch Complex 39B on a flight test around the Moon and back to Earth. All about Artemis I: https://www.nasa.gov/specials/artemis-i Music Courtesy of Gothic Storm Music Editor: Christopher Chamberland Producers: Sami Aziz and John Sackman Song Credits: Existence from Gothic Storm The Artemis Generation: Exploration, Discovery and the Unknowns, written by Doug Wallace and performed by the Cooper Middle School Band Percussion Section Credit: NASA

NASA’s Perseverance Mars Rover has arrived at an ancient delta in Jezero Crater, one of the best places on the Red Planet to search for potential signs of ancient life. The delta is an area where scientists surmise that a river once flowed billions of years ago into a lake and deposited sediments in a fan shape. Rachel Kronyak, a member of the Perseverance science operations team, guides the viewer through this Martian panorama and its intriguing sedimentary rocks. It’s the most detailed view ever returned from the Martian surface, consisting of 2.5 billion pixels and generated from 1,118 individual Mastcam-Z images. Those images were acquired on June 12, 13, 16, 17, and 20, 2022 (the 466th, 467th, 470th, 471st, and 474th Martian day, or sol, of Perseverance’s mission). In this panorama, an area called Hogwallow Flats is visible, as is Skinner Ridge, where two rock core samples were taken. The color enhancement in this image improves the visual contrast and accentuates color differences. This makes it easier for the science team to use their everyday experience to interpret the landscape. For more information on the Perseverance rover, visit https://mars.nasa.gov/perseverance. Credit: NASA/JPL-Caltech/ASU/MSSS

NASA’s InSight lander detected seismic waves from a meteoroid and was able to capture the sound of the space rock striking the surface of Mars for the first time. The meteoroid – the term used for incoming space rocks before they hit the ground – entered Mars’ atmosphere on Sept. 5, 2021, exploding into at least three shards that each left craters behind. Mars’ atmosphere is just 1% as dense as Earth’s, allowing far more meteoroids to pass through and impact the Red Planet’s surface. This event marks the first time seismic and acoustic waves from an impact were detected on the Red Planet. Why does this meteoroid impact sound like a “bloop” in the video? It has to do with a peculiar atmospheric effect that’s also observed in deserts on Earth. After sunset, the atmosphere retains some heat accumulated during the day. Sound waves travel through this heated atmosphere at different speeds, depending on their frequency. As a result, lower-pitched sounds arrive before high-pitched sounds. An observer close to the impact would hear a “bang,” while someone many miles away would hear the bass sounds first, creating a “bloop.” NASA’s Mars Reconnaissance Orbiter flew over the estimated impact site to confirm the location. The orbiter used its black-and-white Context Camera to reveal three darkened spots on the surface. After locating these spots, the orbiter’s team used the High-Resolution Imaging Science Experiment camera, or HiRISE, to get a color close-up of the craters. Because HiRISE sees wavelengths the human eye can’t detect, scientists change the camera’s filters to enhance the color of the image. The areas that appear blue around the craters are where dust has been removed or disturbed by the blast of the impact. Martian dust is bright and red, so removing it makes the surface appear relatively dark and blue. For more information on InSight, visit https://mars.nasa.gov/insight. Credit: NASA/JPL-Caltech/University of Maryland/University of Arizona/CNES/IPGP/Manchu/Bureau 21/ETH Zurich/Kirschner/van Driel

NASA’s Lucy mission is heading to the Jupiter Trojans – two swarms of primitive asteroids trapped in Jupiter’s orbit that may hold clues to the formation of the planets. Lucy launched on October 16, 2021. After a year in orbit around the Sun, it is returning home on its launch anniversary for the first of three Earth gravity assists. On October 16, 2022, Lucy will fly by the Earth like a partner in a swing dance, boosting its speed and elongating its orbit around the Sun. At 7:04 am, Eastern Time, Lucy will make its closest approach at just 219 miles above the planet: lower than the International Space Station. This exceptionally close shave will increase its velocity by four-and-a-half miles per second, setting Lucy on track to gain even more speed when it returns to Earth for its second gravity assist in December 2024. Read more: https://www.nasa.gov/feature/goddard/2022/lucy-ega Credit: NASA’s Goddard Space Flight Center Dan Gallagher (KBRwyle): Producer Kel Elkins (USRA): Lead Visualizer Walt Feimer (KBRwyle): Lead Animator Jenny McElligott (AIMM): Animator Krystofer Kim (KBRwyle): Animator Jonathan North (KBRwyle): Animator Katherine Kretke (SwRI): Support Ernie Wright (USRA): Support Aaron E. Lepsch (ADNET): Technical Support Universal Production Music: “Determined Arrival 5” by Joel Goodman; “Finding Solace” by Eric Chevalier; “Subtle Confidence 3” by Joel Goodman This video can be freely shared and downloaded at https://svs.gsfc.nasa.gov/14225. While the video in its entirety can be shared without permission, the music and some individual imagery may have been obtained through permission and may not be excised or remixed in other products. Specific details on such imagery may be found here: https://svs.gsfc.nasa.gov/14225. For more information on NASA’s media guidelines, visit https://nasa.gov/multimedia/guidelines. If you liked this video, subscribe to the NASA Goddard YouTube channel: https://www.youtube.com/NASAGoddard Follow NASA’s Goddard Space Flight Center · Instagram http://www.instagram.com/nasagoddard · Twitter http://twitter.com/NASAGoddard · Twitter http://twitter.com/NASAGoddardPix · Facebook: http://www.facebook.com/NASAGoddard · Flickr http://www.flickr.com/photos/gsfc

When Artemis astronauts land on the Moon, they’ll travel to sites never before visited by humans. Namely, they'll explore the South Pole region, home to the Moon’s largest crater, areas of near-constant light and deep shadows, and some of the coldest temperatures in the solar system. Exploring the South Pole will teach us more about the Moon’s history, as well as the history of our solar system. It's home to frozen water, which is crucial for living sustainably on the lunar surface and exploring deeper into the solar system. Artemis astronauts will explore the Moon on behalf of all of us and bring back lunar rocks and soil for analyses by generations of scientists who will help us gain unimaginable insights into our cosmic history. Series Executive Producers: Katy Mersmann/Lauren Ward Season Producers: Lonnie Shekhtman/Stephanie Sipila/James Tralie/Molly Wasser Explorers: Jose Aponte/Natalie Curran/Julie Mitchell/Adam Naids/Noah Petro/Kelsey Young/Jessica Watkins Music: a. “Daylight Falls” by Jay Price b. “Good Omens” by Count Zero and Rohan Stevenson c. “Lightspeed” by Gresby Race Nash d. “Wonders of Life” by Enrico Cacace and Lorzeno Castellarin e. “Hold Still” by Enrico Cacace f. “We Shall Overcome” by Laurent Couson Credit: NASA #NASAExplorers #Artemis #NASA-

Set far away from residents and surrounded by dunes, the Remote Hypervelocity Test Laboratory at NASA’s White Sands Test Facility in Las Cruces, New Mexico, has supported every human spaceflight program from the Space Shuttle to Artemis. A team designing shields to protect NASA's Mars Earth Entry System from micrometeorites and space debris traveled to this facility to safely recreate dangerous impacts, and to test the team’s shields and computer models. Video Credit: NASA’s Goddard Space Flight Center James Tralie (ADNET): Lead Producer Lead Editor Videographer Sam Molleur (NASA/JPL): Producer Videographer Dave Hendon (NASA/White Sands): White Sands Videographer Support Marcus Sandy (NASA/White Sands): Manager, White Sands Hypervelocity Testing Dennis Garcia (NASA/White Sands): .50-Caliber Test Conductor Russ Stein (NASA/Goddard): Micrometeoroid Protection System Product Design Lead Bruno Sarli (NASA/Goddard): System Engineer for CCRS Art Pardo (NASA/White Sands): White Sands Lead Electrical Technician Animations from NASA/CILabs, NASA/JPL, and ESA Music is "Tumbleweed" by Paul Osborne, "Old as the Hills" by Matthieu Ouaki, and "Texas Moon" by Anders Johan Greger Lewen of Universal Production Music. This video can be freely shared and downloaded at https://svs.gsfc.nasa.gov/14219. While the video in its entirety can be shared without permission, the music and some individual imagery may have been obtained through permission and may not be excised or remixed in other products. Specific details on such imagery may be found here: https://svs.gsfc.nasa.gov/14219. For more information on NASA’s media guidelines, visit https://nasa.gov/multimedia/guidelines. If you liked this video, subscribe to the NASA Goddard YouTube channel: https://www.youtube.com/NASAGoddard Follow NASA’s Goddard Space Flight Center · Instagram http://www.instagram.com/nasagoddard · Twitter http://twitter.com/NASAGoddard · Twitter http://twitter.com/NASAGoddardPix · Facebook: http://www.facebook.com/NASAGoddard · Flickr http://www.flickr.com/photos/gsfc

An image from NASA’s James Webb Space Telescope reveals a remarkable sight: at least 17 concentric dust rings emanating from a pair of stars located about 5,300 light-years from Earth. Each ring was created when the stars came close together and their colliding stellar winds (streams of gas they blow into space) caused some of the gas to compress into dust. Collectively known as Wolf-Rayet 140, the stars’ orbits bring them together about once every eight years, so just like the growth rings of a tree trunk, these dusty loops mark the passage of time: The 17 rings reveal more than a century of stellar interactions. And while other Wolf-Rayet stars produce dust, no other pair is known to produce rings quite like Wolf-Rayet 140. Because the stars’ orbits are elliptical rather than circular, the distance between the stars changes constantly, and dust forms only when they are close. The amount of dust produced by this interaction varies, so the system doesn’t form a perfect bullseye. One of the densest regions of dust production creates the bright feature repeating at 2 o’clock. Credit: NASA/JPL-Caltech For more information about the Webb telescope’s mission, visit: https://www.nasa.gov/webb

After months aboard the International Space Station, the astronauts of NASA’s SpaceX Crew-4 mission are returning home. Traveling back to Earth inside a SpaceX Dragon capsule are NASA astronauts Kjell Lindgren, Robert Hines, and Jessica Watkins, along with ESA (European Space Agency) astronaut Samantha Cristoforetti. During their time aboard the orbiting laboratory, these crew members contributed to ongoing and new scientific investigations and technology demonstrations, work that is helping to prepare humans for future space exploration missions and generating innovations and benefits for humanity on Earth. Learn more: https://go.nasa.gov/3Sv0vkE Credit: NASA #space #iss #spacex

There may not be any humans aboard NASA's #Artemis I flight test, but there will be a special canine: Snoopy! Learn why Astronaut Snoopy is flying to space when Artemis launches on its historic mission around the Moon and back. Artemis I is the first integrated flight test of the Space Launch System rocket that will send the uncrewed Orion spacecraft around the Moon and back to Earth. The mission will check out all spacecraft systems for the first time before crew fly aboard Artemis II. It's one more step toward taking the next giant leap: sending the first astronauts to Mars. Get all the info on this historic mission: https://nasa.gov/specials/artemis-i The history of Snoopy and NASA: https://go.nasa.gov/3cNgB65 Producers: Scott Bednar, Jessica Wilde, Sami Aziz Videographer: Ben Smegelsky Credit: NASA

A new NASA and Durham University simulation puts forth a different theory of the Moon’s origin – the Moon may have formed in a matter of hours, when material from the Earth and a Mars sized-body were launched directly into orbit after the impact. The simulations used in this research are some of the most detailed of their kind, operating at the highest resolution of any simulation run to study the Moon’s origins or other giant impacts. Learn more: https://www.nasa.gov/feature/ames/lunar-origins-simulations Credit: NASA/Durham University/Jacob Kegerreis Music Provided by Universal Production Music: Genosequence by Alessandro Rizzo. This video can be downloaded from the NASA Image and Video Library at: https://images.nasa.gov/details-ARC-20221004-AAV3443-MoonOrigin-Social-NASAWeb-1080p NASA's Ames Research Center is located in California's Silicon Valley. Follow us on social media to hear about the latest developments in space, science, technology, and aeronautics. Facebook https://www.facebook.com/nasaames​Twitter https://twitter.com/nasaames​Instagram https://www.instagram.com/nasaames

The DART mission deployed a kinetic impactor to smack the small moon Dimorphos of the asteroid Didymos on the evening of Sept. 26. This was an on-orbit demonstration of asteroid deflection, a key test of NASA's kinetic impactor technology, designed to impact an asteroid to adjust its speed and path. This particular asteroid moon is NOT a threat to Earth, but is technology being explored to use for when we DO find a potentially hazardous asteroid. The Hubble Space Telescope captured these extraordinary views of the asteroid moon soon after the successful impact. For more information, visit https://nasa.gov/hubble. Credit: NASA's Goddard Space Flight Center Paul Morris: Lead Producer Music & Sound “The Beauty Beyond” by Jeremy Noel William Abbott [PRS] and Vasco [PRS] via Freshworx Music Limited [PRS] and Universal Production Music This video can be freely shared and downloaded at https://svs.gsfc.nasa.gov/14215. While the video in its entirety can be shared without permission, the music and some individual imagery may have been obtained through permission and may not be excised or remixed in other products. Specific details on such imagery may be found here: https://svs.gsfc.nasa.gov/14215. For more information on NASA’s media guidelines, visit https://www.nasa.gov/multimedia/guidelines/index.html. See more Hubble videos on YouTube: https://www.youtube.com/playlist?list=PLiuUQ9asub3Ta8mqP5LNiOhOygRzue8kN Follow NASA's Hubble Space Telescope: · Facebook: https://www.facebook.com/NASAHubble · Twitter: https://twitter.com/NASAHubble · Instagram: https://www.instagram.com/NASAHubble · Flickr: https://www.flickr.com/photos/nasahubble --- If you liked this video, subscribe to the NASA Goddard YouTube channel: https://www.youtube.com/NASAGoddard Follow NASA’s Goddard Space Flight Center · Instagram http://www.instagram.com/nasagoddard · Twitter http://twitter.com/NASAGoddard · Twitter http://twitter.com/NASAGoddardPix · Facebook: http://www.facebook.com/NASAGoddard · Flickr http://www.flickr.com/photos/gsfc

When the Hunga Tonga-Hunga Ha’apai volcano erupted on Jan. 15, it sent a tsunami racing around the world and set off a sonic boom that circled the globe twice. The underwater eruption in the South Pacific Ocean also blasted an enormous plume of water vapor into Earth’s stratosphere – enough to fill more than 58,000 Olympic-size swimming pools. The sheer amount of water vapor could be enough to temporarily affect Earth’s global average temperature. So outside of its sheer magnitude, what makes this eruption so unique? Well, it’s really a matter of our ability to see it through NASA and ESA satellites. Music credit: “Color Chart” and “Bright Horizons” from Universal Production Music Credit: NASA's Goddard Space Flight Center Emily Watkins (GSFC Interns): Lead Producer Kathleen Gaeta(GSFC AIMMS): Producer Dr. James Garvin (NASA Chief Scientist Goddard): Lead Scientist This video can be freely shared and downloaded at https://svs.gsfc.nasa.gov/14214. While the video in its entirety can be shared without permission, the music and some individual imagery may have been obtained through permission and may not be excised or remixed in other products. Specific details on such imagery may be found here: https://svs.gsfc.nasa.gov/14214. For more information on NASA’s media guidelines, visit https://www.nasa.gov/multimedia/guidelines/index.html. If you liked this video, subscribe to the NASA Goddard YouTube channel: https://www.youtube.com/NASAGoddard Follow NASA’s Goddard Space Flight Center · Instagram http://www.instagram.com/nasagoddard · Twitter http://twitter.com/NASAGoddard · Twitter http://twitter.com/NASAGoddardPix · Facebook: http://www.facebook.com/NASAGoddard · Flickr http://www.flickr.com/photos/gsfc

Paul Smith is a night-sky fanatic and photographer. His obsession is sprites: immense jolts of light that flicker high above thunderstorms. Last October, he guided NASA scientist Dr. Burcu Kosar through the backroads of Oklahoma to catch one herself. Although she’d studied sprites for more than 15 years, she hadn’t yet chased one. Read more about chasing sprites with Paul and Burcu: https://blogs.nasa.gov/sunspot/2022/10/27/the-great-sprites-chase Learn about NASA’s citizen science project Spritacular: https://www.nasa.gov/feature/goddard/2022/sun/spritacular-nasa-s-new-citizen-science-project-to-capture-elusive-upper-atmospheric Learn about the Heliophysics Big Year: https://solarsystem.nasa.gov/solar-system/sun/helio-big-year Image credits: Paul Smith, Frankie Lucena, Panagiotis Tsouras, Thomas Ashcraft. All imagery of sprites is copyrighted and used with permission. Music credits: “The Beauty Beyond” by Jeremy Noel William Abbott [PRS], Vasco [PRS]; “Outer Orbit” by Alexander Ryder Mcnair [ASCAP], Harry Gregson Williams [BMI], Ho Ling Tang [BMI]; “Wonderful Orbit” by Tom Furse Fairfax Cowan [PRS]; “Starlights” by Marc Teitler [PRS], Vasco [PRS]; “A Tranquil End” by Luke Gordon [PRS]; “Virtual Tidings” by Andrew Michael Britton [PRS], David Stephen Goldsmith [PRS]; “Winter Aurora” by Samuel Karl Bohn [PRS]; “Lava Flow” and “Water Dance” by Ben Niblett [PRS], Jon Cotton [PRS]. Credit: NASA's Goddard Space Flight Center Producer: Joy Ng (KBRwyle) Scientist: Burcu Kosar (Catholic University of America) Photographer: Paul Smith Photographer: Frankie Lucena Photographer: Panagiotis Tsouras Photographer: Thomas Ashcraft Videographer: Joy Ng, Thomas Smith Writer: Lina Tran This video can be freely shared and downloaded at https://svs.gsfc.nasa.gov/14206. While the video in its entirety can be shared without permission, the music and some individual imagery may have been obtained through permission and may not be excised or remixed in other products. Specific details on such imagery may be found here: https://svs.gsfc.nasa.gov/14206. For more information on NASA’s media guidelines, visit https://nasa.gov/multimedia/guidelines. If you liked this video, subscribe to the NASA Goddard YouTube channel: https://www.youtube.com/NASAGoddard Follow NASA’s Goddard Space Flight Center · Instagram http://www.instagram.com/nasagoddard · Twitter http://twitter.com/NASAGoddard · Twitter http://twitter.com/NASAGoddardPix · Facebook: http://www.facebook.com/NASAGoddard · Flickr http://www.flickr.com/photos/gsfc

We’re testing a new way of landing on Mars… by crashing into its surface. The Simplified High Impact Energy Landing Device (SHIELD) is a lander concept being tested at NASA’s Jet Propulsion Laboratory (JPL). It could one day provide a new way for low-cost missions to land on Mars. Rather than rely on parachutes or retrorockets, SHIELD would include a collapsible, accordion-like base to absorb the energy of a landing. A full-size prototype of the base was tested on Aug. 12, 2022. The prototype was hurled at the ground from the top of a nearly 90-foot-tall (27-meter-tall) drop tower at JPL. A steel plate ensured the impact was even harder than what would be experienced on Mars. The design worked: After crushing against the steel plate at 110 mph (177 kph), several electronic components inside the SHIELD prototype, including a smartphone, survived the impact. Credit: NASA/JPL-Caltech/California Academy of Science

NASA’s Perseverance Mars rover is filling sample tubes with rocky material on the Red Planet as the agency works on the next steps to get them safely back to Earth. The Mars Sample Return campaign would bring samples collected by the Perseverance rover to Earth for detailed study. The campaign involves an international interplanetary relay team, including the European Space Agency (ESA). These samples could answer a key question: did life ever exist on Mars? Aaron Yazzie, who works on the Mars Sample Return campaign, explains the work being done at NASA’s Jet Propulsion Laboratory to ensure the safe return of the sample tubes. For more information on Mars Sample Return, visit mars.nasa.gov/msr Credit: NASA/JPL-Caltech

Are Hurricanes Getting Stronger? We Asked a NASA Scientist Are hurricanes getting stronger? Although we’ll never see a Category 6 hurricane, data does show that more hurricanes are becoming more severe. Hurricane and climate expert Mara Cordero-Fuentes of NASA's Goddard Space Flight Center tells us more about the connection between climate change and tropical cyclones. Learn more: https://go.nasa.gov/3yQ168I Producers: Scott Bednar, Jessica Wilde Editor: Daniel Salazar Credit: NASA

In this video, measurements collected by the Waves instrument aboard NASA’s Juno spacecraft during its close flyby of Jupiter’s moon Europa on Sept. 29, 2022 have been converted to an audible frequency. As the white line moves across the spectrogram, which is a visual way of representing signal strength over time, the variation of frequency of the plasma waves observed near Europa can be heard as the plasma density varies. The video shows data collected over approximately 1.5 hours during the Europa flyby. For more information about NASA’s Juno mission, visit: http://nasa.gov/juno and https://missionjuno.com Details about the Europa flyby can be found at: https://www.nasa.gov/feature/jpl/nasa-s-juno-will-perform-close-flyby-of-jupiter-s-icy-moon-europa Credit: NASA/JPL-Caltech/SwRI/Univ of Iowa

New time-lapse movies from NASA’s NEOWISE mission give astronomers the opportunity to see objects, like stars and black holes, as they move and change over time. The videos include previously hidden brown dwarfs, a feeding black hole, a dying star, a star-forming region, and a brightening star. They combine more than 10 years of NEOWISE observations and 18 all-sky images, enabling a long-term analysis and a deeper understanding of the universe. 0:44 – NEOWISE all-sky scan animation 1:03 – Feeding black hole 1:14 – Pulsing star reaches the end of its life 1:21 – Protostars in star-forming region 1:34 – Brown dwarf moves across the sky 2:00 – Unexplained stellar brightening The NEOWISE mission uses a space telescope to hunt for asteroids and comets, including those that could pose a threat to Earth. Launched in December 2009 as the Wide-Field Infrared Survey Explorer, or WISE, the space telescope was originally designed to survey the sky in infrared, detecting asteroids, stars and some of the faintest galaxies in space. WISE did so successfully until completing its primary mission in February 2011. Observations resumed in December 2013, when the telescope was taken out of hibernation and re-purposed for the NEOWISE project as an instrument to study near-Earth objects, or NEOs, as well as more distant asteroids and comets. For more information on the NEOWISE mission go to: https://www.jpl.nasa.gov/missions/neowise For more NEOWISE data go to: https://neowise.ipac.caltech.edu Credit: NASA/JPL-Caltech WISE-NEOWISE movies compiled by Dan Caselden

The 18th Northrop Grumman commercial resupply services mission to the International Space Station carries scientific investigations of topics such as 3D printing of knee cartilage, plant mutations, and mudflow structure—along with a demonstration of camera technology and small satellites from Japan, Uganda, and Zimbabwe. The Cygnus spacecraft carrying these investigations to the orbiting laboratory is scheduled for liftoff no earlier than Nov. 6, 2022 from the Mid-Atlantic Regional Spaceport at NASA's Wallops Flight Facility on Wallops Island, Virginia. Learn more about some of the scientific research traveling to the station on this mission: https://go.nasa.gov/3rYCjvA CREDIT: NASA #NASA #SpaceStation #Science

In order to slow down spacecraft quickly and safely as they land, we get some help from an unexpected source: the planet’s atmosphere! To use the air around a planet to our advantage, we use heat shields, which have an air-resistant design. Learn more about heat shields, like LOFTID, and how they may help us land on Mars! For more information about the LOFTID technology demonstration, click here: https://go.nasa.gov/3aRdADV

Prepration For Lunar Exploration In 2009

How Do Spacecraft Slow Down? We Asked a NASA Technologist How do spacecraft slow down? Rigid heat shields and retropropulsion have been the favorites of engineers for years. Now NASA is testing a new inflatable heat shield technology that could allow us to carry even larger payloads to worlds with atmospheres: https://www.nasa.gov/loftid Launching on Nov. 1 aboard a United Launch Alliance Atlas V rocket along with NOAA’s JPSS-2 mission, the Low-Earth Orbit Flight Test of an Inflatable Decelerator, or LOFTID, will demonstrate the heat shield’s ability to slow down and survive atmospheric entry: https://go.nasa.gov/3N7yzBG Producers: Scott Bednar, Jessica Wilde Editor: Daniel Salazar Credit: NASA #NASA #Technology #Spacecraft

A new Earth science mission, led by NASA and the French space agency Centre National d’Études Spatiales (CNES), will help communities plan for a better future by surveying the planet’s salt and freshwater bodies. The Surface Water and Ocean Topography (SWOT) mission will measure the height of water in lakes, rivers, reservoirs, and the oceans. As climate change accelerates the water cycle, more communities around the world will be inundated with water while others won’t have enough. SWOT data will be used to improve flood forecasts and monitor drought conditions, providing essential information to water management agencies, civil engineers, universities, the U.S. Department of Defense, disaster preparedness agencies, and others who need to track water in their local areas. In this video, examples of how SWOT data will be used in these communities are shared by a National Weather Service representative in Oregon, an Alaska Department of Transportation engineer, researchers from the University of Oregon and University of North Carolina, a NASA Jet Propulsion Laboratory scientist working with the Department of Defense, and a JPL scientist working with the Louisiana Coastal Protection and Restoration Agency. :30 - Flood Watches & Warnings - Portland, Oregon 1:08 - Water Management - Fern Ridge Lake, Oregon 2:05 - Protecting Infrastructure - Alaska 2:54 - National Security - Department of Defense 3:24 - Coastal Protection - Mississippi River Delta SWOT is expected to launch from Vandenberg Space Force Base in California in December 2022. The mission is a collaboration between NASA and CNES, with contributions from the Canadian Space Agency and UK Space Agency. JPL, which is managed for NASA by Caltech in Pasadena, California, leads the U.S. component of the project. To learn more about the mission, visit: https://swot.jpl.nasa.gov Credit: NASA/JPL-Caltech/CNES/Thales Alenia Space