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1 min read Preparations for Next Moonwalk Simulations Underway (and Underwater) Why do we grow plants in space? Plants are such versatile organisms that they can fulfill many roles in our exploration of space. Plants provide us with food, with oxygen, they can recycle water and waste, and they can even provide us with psychological benefits. So all these functions will help NASA in fulfilling our goal of trying to create a sustainable environment for human presence in space. But there are also other benefits. We can investigate how plants adapt to the novel environment of space, something that’s completely outside their evolutionary history. We can develop new processes and technologies to cultivate plants in difficult and even extreme environments. All these lessons learned will help us in ultimately improving the lives of humans here on Earth by being able to better cultivate plants. So why do we grow plants in space? To be able to create a sustainable environment for us to thrive in space, as well as improve lives and agricultural techniques here on Earth. [END VIDEO TRANSCRIPT] Full Episode List Full YouTube Playlist Share Details Last Updated Apr 15, 2025 Related TermsGeneralAdvanced Plant Habitat (APH)Biological & Physical SciencesInternational Space Station (ISS)ISS ResearchPlant BiologyScience & ResearchScience Mission DirectorateSpace BiologySpace Biology Program Explore More 5 min read Can Solar Wind Make Water on Moon? NASA Experiment Shows Maybe Scientists have hypothesized since the 1960s that the Sun is a source of ingredients that… Article 2 hours ago 5 min read NASA’s Hubble Tracks a Roaming Magnetar of Unknown Origin Researchers using NASA’s Hubble Space Telescope have discovered the magnetar called SGR 0501+4516 is traversing… Article 3 hours ago 3 min read In the Starlight: Tina Preyan Fuels the Future at Johnson Article 5 hours ago Keep Exploring Discover Related Topics Missions Humans in Space Climate Change Solar System View the full article

NASA's SpaceX 32nd Commercial Resupply Services Launch

Why Do We Grow Plants in Space? We Asked a NASA Expert

When Michael Ciancone joined NASA in 1983, he could hardly imagine what his 40-plus-year career would entail. From honoring and preserving spaceflight history to advancing safety standards, he has undoubtedly woven his knowledge and experience into NASA’s history as well as its future. Ciancone currently serves as the Orion Program safety lead, overseeing the Office of Safety and Mission Assurance’s effort to ensure the safety of the Orion crew, vehicle, and associated hardware. In his role, he manages safety reviews of all flight hardware, with a current focus on Artemis II. His everyday success is backed by decades of learning and global collaboration within the areas of human spaceflight safety and history. Michael Ciancone with Space Shuttle Atlantis at the launch gantry at NASA’s Kennedy Space Center in Florida in 2009. Image courtesy of Michael Ciancone In 1997, Ciancone transferred from NASA’s Glenn Research Center in Cleveland to Johnson Space Center in Houston to serve as the executive officer for the Shuttle/International Space Station Payload Safety Review Panel, as well as group lead for Payload Safety. To better understand the scope and nature of his new role, Ciancone sought opportunities to engage with other safety professionals at conferences and symposia. At the suggestion of his manager, Ciancone instead organized a conference on spaceflight safety for payloads at Johnson, creating a forum for colleagues from the international spaceflight community. These efforts were the catalyst for the formation of the International Association for the Advancement of Spaceflight Safety (IAASS), an organization founded by Ciancone and Skip Larsen of Johnson along with Alex Soons and Tommaso Sgobba of the European Space Agency. The IAASS is committed to furthering international cooperation and scientific advancements in space system safety and is recognized as the pre-eminent international forum for spaceflight and safety professionals. The organization is responsible for hosting an annual conference, conducting specialized safety training, and publishing seminal books on the aspects of spaceflight safety. Throughout his tenure, Ciancone has worked closely with colleagues from around the world and he emphasizes that human spaceflight is a global endeavor made possible through respect and collaboration. “[In human spaceflight] there are different and equally valid approaches for achieving a common goal. Successful partnership requires an understanding and respect for the experiences and history of international partners,” he said. Michael Ciancone (far left) pictured with Spaceflight Safety team members from NASA, the European Space Agency (ESA), and Airbus during a joint NASA/ESA safety review of the European Service Module (ESM) of the Orion Program at the Airbus facility in Bremen, Germany. Image courtesy of Michael Ciancone In addition to his dedication to spaceflight safety, Ciancone is active in the field of spaceflight history. He serves as the chair of the History Committee of the American Astronautical Society and, as a member of the International Academy of Astronautics, he also serves on the History Committee. Working in this community has made Ciancone more keenly aware of dreams of spaceflight as viewed from a historical perspective and guides his daily work at NASA. Michael Ciancone (left) with Giovanni Caprara, science editor for the Corriere della Sera and co-author of “Early Italian Contributions to Astronautics: From the First Visionary to Construction of the first Italian Liquid Propellant Rocket” during the 75th International Astronautical Congress in Milan, Italy. Image courtesy of Michael Ciancone Beyond his technical achievements, Ciancone has also found creative ways to spice up the spaceflight community. While at Glenn Research Center, he co-founded the NASA Hot Pepper Club—a forum for employees who share a passion for cultivating and consuming hot peppers and pepper products. The club served as a unique space for camaraderie and connection, adding flavor to NASA life. Ciancone’s immersion in spaceflight history and spaceflight safety has shaped his unique and valuable perspective. In addition to encouraging others to embrace new challenges and opportunities, Ciancone paraphrases Albert Einstein to advise the Artemis Generation to “learn from the past, live in the moment, and dream of the future.” This mentality has enabled him to combine his interest in spaceflight history with his work on Orion over the past 15 years, laying the groundwork for what he refers to as “future history.” View the full article

Scientists have hypothesized since the 1960s that the Sun is a source of ingredients that form water on the Moon. When a stream of charged particles known as the solar wind smashes into the lunar surface, the idea goes, it triggers a chemical reaction that could make water molecules. Now, in the most realistic lab simulation of this process yet, NASA-led researchers have confirmed this prediction. The finding, researchers wrote in a March 17 paper in JGR Planets, has implications for NASA’s Artemis astronaut operations at the Moon’s South Pole. A critical resource for exploration, much of the water on the Moon is thought to be frozen in permanently shadowed regions at the poles. “The exciting thing here is that with only lunar soil and a basic ingredient from the Sun, which is always spitting out hydrogen, there’s a possibility of creating water,” Li Hsia Yeo, a research scientist at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. “That’s incredible to think about,” said Yeo, who led the study. Solar wind flows constantly from the Sun. It’s made largely of protons, which are nuclei of hydrogen atoms that have lost their electrons. Traveling at more than one million miles per hour, the solar wind bathes the entire solar system. We see evidence of it on Earth when it lights up our sky in auroral light shows. Computer-processed data of the solar wind from NASA’s STEREO spacecraft. Download here: https://svs.gsfc.nasa.gov/20278/ NASA/SwRI/Craig DeForest Most of the solar particles don’t reach the surface of Earth because our planet has a magnetic shield and an atmosphere to deflect them. But the Moon has no such protection. As computer models and lab experiments have shown, when protons smash into the Moon’s surface, which is made of a dusty and rocky material called regolith, they collide with electrons and recombine to form hydrogen atoms. Then, the hydrogen atoms can migrate through the lunar surface and bond with the abundant oxygen atoms already present in minerals like silica to form hydroxyl (OH) molecules, a component of water, and water (H2O) molecules themselves. Scientists have found evidence of both hydroxyl and water molecules in the Moon’s upper surface, just a few millimeters deep. These molecules leave behind a kind of chemical fingerprint — a noticeable dip in a wavy line on a graph that shows how light interacts with the regolith. With the current tools available, though, it is difficult to tell the difference between hydroxyl and water, so scientists use the term “water” to refer to either one or a mix of both molecules. Many researchers think the solar wind is the main reason the molecules are there, though other sources like micrometeorite impacts could also help by creating heat and triggering chemical reactions. In 2016, scientists discovered that water is released from the Moon during meteor showers. When a speck of comet debris strikes the moon, it vaporizes on impact, creating a shock wave in the lunar soil. With a sufficiently large impactor, this shock wave can breach the soil’s dry upper layer and release water molecules from a hydrated layer below. NASA’s LADEE spacecraft detected these water molecules as they entered the tenuous lunar atmosphere. NASA’s Goddard Space Flight Center Conceptual Image Lab Spacecraft measurements had already hinted that the solar wind is the primary driver of water, or its components, at the lunar surface. One key clue, confirmed by Yeo’s team’s experiment: the Moon’s water-related spectral signal changes over the course of the day. In some regions, it’s stronger in the cooler morning and fades as the surface heats up, likely because water and hydrogen molecules move around or escape to space. As the surface cools again at night, the signal peaks again. This daily cycle points to an active source — most likely the solar wind—replenishing tiny amounts of water on the Moon each day. To test whether this is true, Yeo and her colleague, Jason McLain, a research scientist at NASA Goddard, built a custom apparatus to examine Apollo lunar samples. In a first, the apparatus held all experiment components inside: a solar particle beam device, an airless chamber that simulated the Moon’s environment, and a molecule detector. Their invention allowed the researchers to avoid ever taking the sample out of the chamber — as other experiments did — and exposing it to contamination from the water in the air. “It took a long time and many iterations to design the apparatus components and get them all to fit inside,” said McLain, “but it was worth it, because once we eliminated all possible sources of contamination, we learned that this decades-old idea about the solar wind turns out to be true.” Using dust from two different samples picked up on the Moon by NASA’s Apollo 17 astronauts in 1972, Yeo and her colleagues first baked the samples to remove any possible water they could have picked up between air-tight storage in NASA’s space-sample curation facility at NASA’s Johnson Space Center in Houston and Goddard’s lab. Then, they used a tiny particle accelerator to bombard the dust with mock solar wind for several days — the equivalent of 80,000 years on the Moon, based on the high dose of the particles used. They used a detector called a spectrometer to measure how much light the dust molecules reflected, which showed how the samples’ chemical makeup changed over time. In the end, the team saw a drop in the light signal that bounced to their detector precisely at the point in the infrared region of the electromagnetic spectrum — near 3 microns — where water typically absorbs energy, leaving a telltale signature. While they can’t conclusively say if their experiment made water molecules, the researchers reported in their study that the shape and width of the dip in the wavy line on their graph suggests that both hydroxyl and water were produced in the lunar samples. By Lonnie Shekhtman NASA’s Goddard Space Flight Center, Greenbelt, Md. Explore More 5 min read NASA’s Hubble Tracks a Roaming Magnetar of Unknown Origin Article 2 hours ago 3 min read What Does NASA Science Do For Me? Article 4 hours ago 3 min read Exploring the Universe Through Sight, Touch, and Sound Article 20 hours ago View the full article

Explore Hubble Hubble Home Overview About Hubble The History of Hubble Hubble Timeline Why Have a Telescope in Space? Hubble by the Numbers At the Museum FAQs Impact & Benefits Hubble’s Impact & Benefits Science Impacts Cultural Impact Technology Benefits Impact on Human Spaceflight Astro Community Impacts Science Hubble Science Science Themes Science Highlights Science Behind Discoveries Hubble’s Partners in Science Universe Uncovered Explore the Night Sky Observatory Hubble Observatory Hubble Design Mission Operations Missions to Hubble Hubble vs Webb Team Hubble Team Career Aspirations Hubble Astronauts News Hubble News Social Media Media Resources Multimedia Multimedia Images Videos Sonifications Podcasts e-Books Online Activities Lithographs Fact Sheets Posters Hubble on the NASA App Glossary More 35th Anniversary Online Activities 5 Min Read NASA’s Hubble Tracks a Roaming Magnetar of Unknown Origin This is an artist’s impression of a magnetar, a special type of neutron star with an incredibly strong magnetic field. Credits: ESA Researchers using NASA’s Hubble Space Telescope have discovered the magnetar called SGR 0501+4516 is traversing our galaxy from an unknown place of origin. Researchers say that this runaway magnetar is the likeliest candidate in our Milky Way galaxy for a magnetar that was not born in a supernova explosion as initially predicted. It is so strange it might even offer clues to the mechanism behind events known as fast radio bursts. “Magnetars are neutron stars — the dead remnants of stars — composed entirely of neutrons. What makes magnetars unique is their extreme magnetic fields,” said Ashley Chrimes, lead author of the discovery paper published in the April 15 journal Astronomy & Astrophysics. Chrimes is a European Space Agency Research Fellow at the European Space Research and Technology Center in the Netherlands. Magnetars have comic-book-hero superpowers. A magnetar has a magnetic field about a trillion times more powerful than Earth’s magnetosphere. If a magnetar flew by Earth at half the Moon’s distance, its intense field would wipe out every credit card on our planet. If a human got within 600 miles, the magnetar would become a proverbial sci-fi death-ray, ripping apart every atom inside the body. The magnetar’s strangeness was identified with the help of Hubble’s sensitive instruments as well as precise benchmarks from ESA’s (European Space Agency) Gaia spacecraft. Initially, the mysterious magnetar was discovered in 2008 when NASA’s Swift Observatory spotted brief, intense flashes of gamma rays from the outskirts of the Milky Way. The source, which turned out to be one of only about 30 known magnetars in the Milky Way, was dubbed SGR 0501+4516. This is an artist’s impression of a magnetar, which is a special type of neutron star with an incredibly strong magnetic field. Neutron stars are some of the most compact and extreme objects in the universe. These stars typically pack more than the mass of the Sun into a sphere of neutrons about 12 miles across. The neutron star is depicted as a white-blueish sphere. The magnetic field is shown as filaments streaming out from its polar regions. Illustration: ESA Because magnetars are neutron stars, the natural explanation for their formation is that they are born in supernovae, when a star explodes and can collapse down to an ultra-dense neutron star. This appeared to be the case for SGR 0501+4516, which is located close to a supernova remnant called HB9. The separation between the magnetar and the center of the supernova remnant on the sky is just 80 arcminutes, or slightly wider than your pinky finger when viewed at the end of your outstretched arm. But a decade-long study with Hubble cast doubt on the magnetar’s birthplace. After initial observations with ground-based telescopes shortly after SGR 0501+4516’s discovery, researchers used Hubble’s exquisite sensitivity and steady pointing to spot the magnetar’s faint infrared glow in 2010, 2012, and 2020. Each of these images was aligned to a reference frame defined by observations from the Gaia spacecraft, which has crafted an extraordinarily precise three-dimensional map of nearly two billion stars in the Milky Way. This method revealed the subtle motion of the magnetar as it traversed the sky. “All of this movement we measure is smaller than a single pixel of a Hubble image,” said co-investigator Joe Lyman of the University of Warwick, United Kingdom. “Being able to robustly perform such measurements really is a testament to the long-term stability of Hubble.” By tracking the magnetar’s position, the team was able to measure the object’s apparent motion across the sky. Both the speed and direction of SGR 0501+4516’s movement showed that the magnetar could not be associated with the nearby supernova remnant. Tracing the magnetar’s trajectory thousands of years into the past showed that there were no other supernova remnants or massive star clusters with which it could be associated. If SGR 0501+4516 was not born in a supernova, the magnetar must either be older than its estimated 20,000-year age, or it may have formed in another way. Magnetars may also be able to form through the merger of two lower-mass neutron stars or through a process called accretion-induced collapse. Accretion-induced collapse requires a binary star system containing a white dwarf: the core of a dead Sun-like star. If the white dwarf pulls in gas from its companion, it can grow too massive to support itself, leading to an explosion — or possibly the creation of a magnetar. “Normally, this scenario leads to the ignition of nuclear reactions, and the white dwarf exploding, leaving nothing behind. But it has been theorized that under certain conditions, the white dwarf can instead collapse into a neutron star. We think this might be how SGR 0501 was born,” added Andrew Levan of Radboud University in the Netherlands and the University of Warwick in the United Kingdom. Understanding Fast Radio Bursts SGR 0501+4516 is currently the best candidate for a magnetar in our galaxy that may have formed through a merger or accretion-induced collapse. Magnetars that form through accretion-induced collapse could provide an explanation for some of the mysterious fast radio bursts, which are brief but powerful flashes of radio waves. In particular, this scenario may explain the origin of fast radio bursts that emerge from stellar populations too ancient to have recently birthed stars massive enough to explode as supernovae. “Magnetar birth rates and formation scenarios are among the most pressing questions in high-energy astrophysics, with implications for many of the universe’s most powerful transient events, such as gamma-ray bursts, super-luminous supernovae, and fast radio bursts,” said Nanda Rea of the Institute of Space Sciences in Barcelona, Spain. The research team has further Hubble observations planned to study the origins of other magnetars in the Milky Way, helping to understand how these extreme magnetic objects form. The Hubble Space Telescope has been operating for over three decades and continues to make ground-breaking discoveries that shape our fundamental understanding of the universe. Hubble is a project of international cooperation between NASA and ESA (European Space Agency). NASA’s Goddard Space Flight Center in Greenbelt, Maryland, manages the telescope and mission operations. Lockheed Martin Space, based in Denver, also supports mission operations at Goddard. The Space Telescope Science Institute in Baltimore, which is operated by the Association of Universities for Research in Astronomy, conducts Hubble science operations for NASA. Related Images & Videos Illustration of Magnetar This is an artist’s impression of a magnetar, which is a special type of neutron star with an incredibly strong magnetic field. Share Details Last Updated Apr 15, 2025 Editor Andrea Gianopoulos Location NASA Goddard Space Flight Center Contact Media Claire Andreoli NASA’s Goddard Space Flight Center Greenbelt, Maryland claire.andreoli@nasa.gov Bethany Downer ESA/Hubble bethany.downer@esahubble.org Garching, Germany Ray Villard Space Telescope Science Institute Baltimore, Maryland Science Ashley Chrimes ESA-ESTEC/Radboud University Related Terms Hubble Space Telescope Astrophysics Astrophysics Division Goddard Space Flight Center Magnetars Neutron Stars Stars The Universe Related Links and Documents ESA/Hubble’s Release The science paper by A.A. Chrimes et al. Keep Exploring Discover More Topics From Hubble Hubble Space Telescope Since its 1990 launch, the Hubble Space Telescope has changed our fundamental understanding of the universe. Hubble Science Highlights Hubble Images Hubble News View the full article

Exploring the unknown and preparing for humanity’s next giant leap really works up an appetite. Thankfully, employees at NASA’s Johnson Space Center in Houston can count on Tina Preyan to help them fuel up and stay focused. Preyan is a food service specialist at Starport, a quality-of-life program that contributes to Johnson’s mission by providing employee services and activities that enhance work life and promote mental well-being and physical fitness. Part of the agency’s network of 12 NASA Exchanges — each located at a NASA center or facility — Starport offers everything from group fitness classes to retail shopping, with programs designed to engage, energize, and support the workforce. Tina Preyan supports a NASA Exchange display at a Johnson Space Center event. Image courtesy of Tina Preyan Preyan oversees the on-site dining options at Johnson, from its cafés and food trucks to vending machines and mini markets. She helps set the budget for food services, creates monthly calendars of food offerings, schedules vendors and pop-up events, and ensures annual food safety inspections are conducted. She also works with teams across Johnson to order food and related supplies for NASA events. “The best part of my job is working in customer service, meeting new NASA workers every day, and making everyone feel welcome and at home when coming to Johnson’s cafés,” she said. Preyan has been a fixture at Johnson for the last 19 years. She previously worked at NASA’s Michoud Assembly Facility in New Orleans but transferred to Houston shortly after Hurricane Katrina hit the city in 2005. At Starport, she worked her way up from prep cook to lead cashier and then to lead assistant. She also served as the office’s administrative assistant before transitioning to her current role. Tina Preyan poses for a photo with NASA astronauts Jessica Watkins and Victor Glover. Image courtesy of Tina Preyan Preyan has enjoyed meeting many NASA astronauts and Johnson team members and learning more about the work they do. The occasional celebrity sighting is another job perk. Preyan is something of a celebrity herself. “So many employees know my name. I am proud of meeting so many people, and the love they give me every day just being here,” she said. She was also proud to receive Starport’s Jackie Kingery Award in fall 2024. The award recognizes extraordinary customer service and exemplary dedication to the NASA Exchange mission at Johnson. “It felt amazing to receive this award and know that I am doing a great job in everyone’s eyes,” she said. “I value high integrity and am always willing to help others in the organization.” Tina Preyan receives Starport’s Jackie Kingery Award from Starport Deputy Operations Manager Sam Miller in October 2024. Image courtesy of Tina Preyan Another source of pride for Preyan? Her son, Cameron, who is set to graduate from the University of Texas at San Antonio in May with a degree in Finance and Marketing. In addition to her son’s graduation, Preyan looks forward to continuing her work in a positive environment and pursuing more growth opportunities. “I’m going to stay busy and stay focused on ensuring proper procedures are being used by vendors,” she said. “And making sure all customers are happy and will continue to return to cafés.” View the full article

3 min read What Does NASA Science Do For Me? It is easy to forget that all of the hard work, technology, and money that NASA pours into space research actually comes back down to Earth. In fact, many of NASA’s missions and research focus on our planet! NASA also has many other projects with partners that use their research to enrich everyone’s lives here on Earth- and this is not including such notable achievements as satellite weather maps! The NASA Spinoff program was created over fifty years ago to facilitate the licensing and development of NASA’s technologies for commercial use by other companies and agencies. This program helps “spin off” NASA’s technology for use by others here on Earth and, in some cases, in space. To date, over 2,000 spinoff technologies have been documented by the NASA Spinoff program. Some notable examples of NASA spinoffs include: Solar Cells Water Purification Memory foam for your cozy bed and chairs Firefighting equipment, especially lightweight fireproof clothing and masks with much-improved air filters Highway safety grooves, which help your car go around curves without slipping off by giving your tire better traction Many safety features in modern aircraft, such as de-icing technologies for wings, chemical detectors and imaging for plane maintenance, improved flight controls, and many more Image stabilization for your binoculars and video cameras The Dustbuster Healthier baby food …and many more! Check out this Wikipedia page for a more extensive list of the technologies that NASA has had a direct role in developing, many of which we now take for granted. It is worth noting that there are a few technologies commonly thought to have been created by NASA that were actually independently developed. Tang is a great example; it was developed by General Foods in 1957 and attained fame when used during food testing by NASA in the 60s (even though some astronauts were not fans of the powdery, not-quite-orange juice). The microwave oven is another famous technology often falsely thought of as a NASA development. It was, in fact, created shortly after World War 2, when radar technicians discovered that it wasn’t such a good idea to stand in front of active equipment! Thankfully, they found out via a melted candy bar and not from severe burns! Every year, NASA releases a report on its program, and the 2025 edition of the NASA Spinoff magazine is now available! You can view the entire NASA Spinoff archive, dating back to 1976, here. Originally posted by Dave Prosper: May 2013 Last Updated by Kat Troche: March 2025 View the full article

To view this video please enable JavaScript, and consider upgrading to a web browser that supports HTML5 video NASA has announced the winners of it’s 31st Human Exploration Rover Challenge . The annual engineering competition – one of the agency’s longest standing student challenges – wrapped up on April 11 and April 12, at the U.S. Space & Rocket Center in Huntsville, Alabama, near NASA’s Marshall Space Flight Center. NASA NASA has announced the winning student teams in the 2025 Human Exploration Rover Challenge. This year’s competition challenged teams to design, build, and test a lunar rover powered by either human pilots or remote control. In the human-powered division, Parish Episcopal School in Dallas, Texas, earned first place in the high school division, and the Campbell University in Buies Creek, North Carolina, captured the college and university title. In the remote-control division, Bright Foundation in Surrey, British Columbia, Canada, earned first place in the middle and high school division, and the Instituto Tecnologico de Santa Domingo in the Dominican Republic, captured the college and university title. The annual engineering competition – one of NASA’s longest standing student challenges – wrapped up on April 11 and April 12, at the U.S. Space & Rocket Center in Huntsville, Alabama, near NASA’s Marshall Space Flight Center. The complete list of 2025 award winners is provided below: Human-Powered High School Division First Place: Parish Episcopal School, Dallas, Texas Second Place: Ecambia High School, Pensacola, Florida Third Place: Centro Boliviano Americano – Santa Cruz, Bolivia Human-Powered College/University Division First Place: Campbell University, Buies Creek, North Carolina Second Place: Instituto Tecnologico de Santo Domingo, Dominican Republic Third Place: University of Alabama in Huntsville Remote-Control Middle School/High School Division First Place: Bright Foundation, Surrey, British Columbia, Canada Second Place: Assumption College, Brangrak, Bangkok, Thailand Third Place: Erie High School, Erie, Colorado Remote-Control College/University Division First Place: Instituto Tecnologico de Santo Domingo, Dominican Republic Second Place: Campbell University, Buies Creek, North Carolina Third Place: Tecnologico de Monterey – Campus Cuernvaca, Xochitepec, Morelos, Mexico Ingenuity Award Queen’s University, Kingston, Ontario, Canada Phoenix Award Human-Powered High School Division: International Hope School of Bangladesh, Uttara, Dhaka, Bangladesh College/University Division: Auburn University, Auburn, Alabama Remote-Control Middle School/High School Division: Bright Foundation, Surrey, British Columbia, Canada College/University Division: Southwest Oklahoma State University, Weatherford, Oklahoma Task Challenge Award Remote-Control Middle School/High School Division: Assumption College, Bangrak, Bangkok, Thailand College/University Division: Instituto Tecnologico de Santo Domingo, Dominican Republic Project Review Award Human-Powered High School Division: Parish Episcopal School, Dallas, Texas College/University Division: Campbell University, Buies Creek, North Carolina Remote-Control Middle School/High School Division: Bright Foundation, Surrey, British Columbia, Canada College/University Division: Instituto Tecnologico de Santo Domingo, Dominican Republic Featherweight Award Campbell University, Buies Creek, North Carolina Safety Award Human-Powered High School Division: Parish Episcopal School, Dallas, Texas College/University Division: University of Alabama in Huntsville Crash and Burn Award Universidad de Monterrey, Nuevo Leon, Mexico (Human-Powered Division) Team Spirit Award Instituto Tecnologico de Santo Domingo, Dominican Republic (Human-Powered Division) STEM Engagement Award Human-Powered High School Division: Albertville Innovation School, Albertville, Alabama College/University Division: Instituto Tecnologico de Santo Domingo, Dominican Republic Remote-Control Middle School/High School Division: Instituto Salesiano Don Bosco, Santo Domingo, Dominican Republic College/University Division: Tecnologico de Monterrey, Nuevo Leon, Mexico Social Media Award Human-Powered High School Division: International Hope School of Bagladesh, Uttara, Dhaka, Bangladesh College/University Division: Universidad Catolica Boliviana “San Pablo” La Paz, Bolivia Remote-Control Middle School/High School Division: ATLAS SkillTech University, Mumbai, Maharashtra, India College/University Division: Instituto Salesiano Don Bosco, Santo Domingo, Dominican Republic Most Improved Performance Award Human-Powered High School Division: Space Education Institute, Leipzig, Germany College/University Division: Purdue University Northwest, Hammond, Indiana Remote-Control Middle School/High School Division: Erie High School, Erie, Colorado College/University Division: Campbell University, Buies Creek, North Carolina Pit Crew Award Human-Powered High School Division: Academy of Arts, Career, and Technology, Reno, Nevada College/University Division: Queen’s University, Kingston, Ontario, Canada Artemis Educator Award Fabion Diaz Palacious from Universidad Catolica Boliviana “San Pablo” La Paz, Bolivia Rookie of the Year Deira International School, Dubai, United Arab Emirates More than 500 students with 75 teams from around the world participated in the 31st year of the competition. Participating teams represented 35 colleges and universities, 38 high schools, and two middle schools from 20 states, Puerto Rico, and 16 other nations. Teams were awarded points based on navigating a half-mile obstacle course, conducting mission-specific task challenges, and completing multiple safety and design reviews with NASA engineers. NASA expanded the 2025 challenge to include a remote-control division, Remote-Operated Vehicular Research, and invited middle school students to participate. “This student design challenge encourages the next generation of scientists and engineers to engage in the design process by providing innovative concepts and unique perspectives,” said Vemitra Alexander, who leads the challenge for NASA’s Office of STEM Engagement at Marshall. “This challenge also continues NASA’s legacy of providing valuable experiences to students who may be responsible for planning future space missions, including crewed missions to other worlds.” The rover challenge is one of NASA’s eight Artemis Student Challenges reflecting the goals of the Artemis campaign, which will land Americans on the Moon while establishing a long-term presence for science and exploration, preparing for future human missions to Mars. NASA uses such challenges to encourage students to pursue degrees and careers in the fields of science, technology, engineering, and mathematics. The competition is managed by NASA’s Southeast Regional Office of STEM Engagement at Marshall. Since its inception in 1994, more than 15,000 students have participated – with many former students now working at NASA, or within the aerospace industry. To learn more about the Human Exploration Rover Challenge, please visit: https://www.nasa.gov/roverchallenge/home/index.html News Media Contact Taylor Goodwin Marshall Space Flight Center, Huntsville, Ala. 256.544.0034 taylor.goodwin@nasa.gov View the full article

2 min read Preparations for Next Moonwalk Simulations Underway (and Underwater) NASA’s Wallops Flight Facility commemorated the start of construction of its new Wallops Island causeway bridge during a groundbreaking ceremony at 10 a.m., Monday, April 14, 2025, on the island. NASA’s Wallops Flight Facility commemorated the start of construction of its new Wallops Island causeway bridge during a groundbreaking ceremony at 10 a.m., Monday, April 14, 2025, on the island. NASA’s Wallops Flight Facility Facility Director David Pierce, NASA’s Goddard Space Flight Center Associate Center Director Ray Rubilotta, and Virgnia Sen. Bill DeSteph attended the ceremony.NASA/Danielle Johnson The ceremony was held at the base of the old Wallops Island causeway bridge. Virgina state Sen. Bill DeSteph attended the groundbreaking, along with staffers from the offices of Sen. Mark Warner, Sen. Tim Kaine, Congresswomen Jen Kiggans, Sen. Chris Van Hollen, and Sen. Angela Alsobrooks. NASA Wallops Facility Director David Pierce and NASA’s Goddard Space Flight Center Associate Center Director Ray Rubilotta attended on behalf of the agency. “Much has changed over the decades, but one thing that has remained the same is our reliance on the causeway bridge as the only means for vehicular access to and from the island,” said Pierce. “Our bridge supports a growing portfolio of commercial launch and government partners. The work we do advances science, technology, and national security missions. This vital work for our nation is enabled by our bridge.” In 2023, NASA Wallops was awarded $103 million in federal funds to fully construct and replace the current 65-year-old causeway bridge that serves as the only vehicular access from NASA Wallops Mainland facilities to its Wallops Island facilities and launch range. After years of exposure to coastal weather and repeated repairs to extend its viability, the existing causeway bridge is reaching the end of its service life. The new causeway bridge, slated for completion in early 2028, will feature a flatter structure, capable of accommodating the increase in heavier loads transported to and from the island in support of an increased cadence of launch operations by NASA, its tenants, and commercial partners. This vital investment in NASA’s infrastructure supports the launch range’s continued growth, strengthening its role as a key asset in Virginia and the nation. An architectural rendering showing the new Wallops Island causeway bridge next to the old causeway bridge.Courtesy of Kokosing NASA is partnering with the Federal Highway Administration to lead the delivery of the design-build project. The project has been awarded to Kokosing Construction Company. For more information on NASA’s Wallops Flight Facility, visit www.nasa.gov/wallops. Share Details Last Updated Apr 14, 2025 Related TermsWallops Flight Facility View the full article

A SpaceX Falcon 9 rocket, with the company’s Dragon spacecraft atop, stands at Launch Complex 39A at NASA’s Kennedy Space Center in Florida on Nov. 4, 2024, in preparation for the agency’s SpaceX 31st Commercial Resupply Services mission to the International Space Station.Credit: SpaceX NASA and SpaceX are targeting 4:15 a.m. EDT, Monday, April 21, for the next launch to deliver science investigations, supplies, and equipment to the International Space Station. This is the 32nd SpaceX commercial resupply services mission to the orbiting laboratory for the agency. Filled with more than 6,400 pounds of supplies, a SpaceX Dragon spacecraft on a Falcon 9 rocket will lift off from Launch Complex 39A at NASA’s Kennedy Space Center in Florida. Live launch coverage will begin at 3:55 a.m. on NASA+. Learn how to watch NASA content through a variety of platforms. NASA’s coverage of Dragon’s arrival to the orbital outpost will begin at 6:45 a.m. Tuesday, April 22, on NASA+. The spacecraft will dock autonomously to the zenith port of the space station’s Harmony module. Along with food and essential equipment for the crew, Dragon is delivering a variety of science experiments, including a demonstration of refined maneuvers for free-floating robots. Dragon also carries an enhanced air quality monitoring system that could protect crew members on exploration missions to the Moon and Mars, and two atomic clocks to examine fundamental physics concepts such as relativity and test worldwide synchronization of precision timepieces. The Dragon spacecraft is scheduled to remain at the space station until May, when it will depart and return to Earth with research and cargo, splashing down off the coast of California. NASA’s mission coverage is as follows (all times Eastern and subject to change based on real-time operations): Wednesday, April 16 1 p.m. – International Space Station National Lab Science Webinar with the following participants: Jennifer Buchli, chief scientist, NASA’s International Space Station Program Michael Roberts, chief scientific officer, International Space Station National Lab Claire Fortenberry, research aerospace engineer, NASA’s Glenn Research Center in Cleveland Yupeng Chen, co-founder, Eascra Biotech Mari Anne Snow, CEO, Eascra Biotech Maj. Travis Tubbs, U.S. Air Force Academy Heath Mills, co-founder, Rhodium Scientific Sarah Wyatt, researcher, Ohio University Media who wish to participate must register for Zoom access no later than one hour before the start of the webinar. Audio of the teleconference will stream live on the International Space Station National Lab website. Friday, April 18 3 p.m. – Prelaunch media teleconference (no earlier than one hour after completion of the Launch Readiness Review) with the following participants: Zebulon Scoville, deputy manager, Transportation Integration Office, NASA’s International Space Station Program Jennifer Buchli, chief scientist, NASA’s International Space Station Program Sarah Walker, director, Dragon Mission Management, SpaceX Jimmy Taeger, launch weather officer, 45th Weather Squadron, Cape Canaveral Space Force Station Media who wish to participate by phone must request dial-in information by 5 p.m. Thursday, April 17, by emailing Kennedy’s newsroom at: ksc-media-accreditat@mail.nasa.gov. Audio of the teleconference will stream live on the agency’s website. Monday, April 21: 3:55 a.m. – Launch coverage begins on NASA+. 4:15 a.m. – Launch Tuesday, April 22: 6:45 a.m. – Arrival coverage begins on NASA+. 8:20 a.m. – Docking NASA website launch coverage Launch day coverage of the mission will be available on the NASA website. Coverage will include live streaming and blog updates beginning no earlier than 3:55 a.m., April 21, as the countdown milestones occur. On-demand streaming video on NASA+ and photos of the launch will be available shortly after liftoff. For questions about countdown coverage, contact the NASA Kennedy newsroom at 321-867-2468. Follow countdown coverage on our International Space Station blog for updates. Attend Launch Virtually Members of the public can register to attend this launch virtually. NASA’s virtual guest program for this mission also includes curated launch resources, notifications about related opportunities or changes, and a stamp for the NASA virtual guest passport following launch. Watch, Engage on Social Media Let people know you’re watching the mission on X, Facebook, and Instagram by following and tagging these accounts: X: @NASA, @NASAKennedy, @NASASocial, @Space_Station, @ISS_Research, @ISS National Lab Facebook: NASA, NASAKennedy, ISS, ISS National Lab Instagram: @NASA, @NASAKennedy, @ISS, @ISSNationalLab Coverage en Espanol Did you know NASA has a Spanish section called NASA en Espanol? Check out NASA en Espanol on X, Instagram, Facebook, and YouTube for additional mission coverage. Para obtener información sobre cobertura en español en el Centro Espacial Kennedy o si desea solicitar entrevistas en español, comuníquese con Antonia Jaramillo o Messod Bendayan a: antonia.jaramillobotero@nasa.gov o messod.c.bendayan@nasa.gov. Learn more about the commercial resupply mission at: https://www.nasa.gov/mission/nasas-spacex-crs-32/ -end- Julian Coltre / Josh Finch Headquarters, Washington 202-358-1100 julian.n.coltre@nasa.gov / joshua.a.finch@nasa.gov Stephanie Plucinsky / Steven Siceloff Kennedy Space Center, Florida 321-876-2468 stephanie.n.plucinsky@nasa.gov / steven.p.siceloff@nasa.gov Sandra Jones Johnson Space Center, Houston 281-483-5111 sandra.p.jones@nasa.gov Share Details Last Updated Apr 14, 2025 EditorJessica TaveauLocationNASA Headquarters Related TermsCommercial ResupplyHumans in SpaceInternational Space Station (ISS)ISS ResearchSpaceX Commercial Resupply View the full article

Credit: NASA NASA’s Office of Small Business Programs will host the U.S. Small Business Administration (SBA) for the first time at its monthly webinar for small businesses at 1 p.m. EDT Wednesday, April 16. The webinar, currently open for registration, will focus on a new SBA manufacturing initiative and provide information about SBA’s flagship 7(a) loan program in addition to small business program updates from NASA. Participants in the webinar include: Casey Swails, deputy associate administrator, NASA Dwight Deneal, assistant administrator, Office of Small Business Programs (OSBP), NASA Headquarters in Washington Charles Williams, program manager, NASA OSBP SBA Administrator Kelly Loeffler Dianna Seaborn, deputy associate administrator, Office of Capital Access, SBA The NASA OSBP Learning Series is a collection of webinars that provide small businesses with an opportunity to receive training and ask questions to experts at the agency. Upcoming webinars are listed on OSBP website. Previous webinars the office has hosted can be found on the OSBP Learning Series Archives. For more information about NASA OSBP’s learning series and other outreach events, visit: https://www.nasa.gov/osbp -end- Share Details Last Updated Apr 14, 2025 LocationNASA Headquarters Related TermsGeneralNASA HeadquartersOffice of Small Business Programs (OSBP) View the full article

Explore This Section Science Science Activation Exploring the Universe Through… Overview Learning Resources Science Activation Teams SME Map Opportunities More Science Activation Stories Citizen Science 3 min read Exploring the Universe Through Sight, Touch, and Sound For the first time in history, we can explore the universe through a rich blend of senses—seeing, touching, and hearing astronomical data—in ways that deepen our understanding of space. While three-dimensional (3D) models are essential tools for scientific discovery and analysis, their potential extends far beyond the lab. Space can often feel distant and abstract, like watching a cosmic show unfold on a screen light-years away. But thanks to remarkable advances in technology, software, and science, we can now transform telescope data into detailed 3D models of objects millions or even billions of miles away. These models aren’t based on imagination—they are built from real data, using measurements of motion, light, and structure to recreate celestial phenomena in three dimensions. What’s more, we can bring these digital models into the physical world through 3D printing. Using innovations in additive manufacturing, data becomes something you can hold in your hands. This is particularly powerful for children, individuals who are blind or have low vision, and anyone with a passion for lifelong learning. Now, anyone can quite literally grasp a piece of the universe. These models also provide a compelling way to explore concepts like scale. While a 3D print might be just four inches wide, the object it represents could be tens of millions of billions of times larger—some are so vast that a million Earths could fit inside them. Holding a scaled version of something so massive creates a bridge between human experience and cosmic reality. In addition to visualizing and physically interacting with the data, we can also listen to it. Through a process called sonification, telescope data is translated into sound, making information accessible and engaging in a whole new way. Just like translating a language, sonification conveys the essence of astronomical data through audio, allowing people to “hear” the universe. To bring these powerful experiences to communities across the country, NASA’s Universe of Learning, in collaboration with the Library of Congress, NASA’s Chandra X-ray Observatory, and the Space Telescope Science Institute, has created Mini Stars 3D Kits that explore key stages of stellar evolution. These kits have been distributed to Library of Congress state hubs across the United States to engage local learners through hands-on and multisensory discovery. Each Mini Stars Kit includes: Three 3D-printed models of objects within our own Milky Way galaxy: Pillars of Creation (M16/Eagle Nebula) – a stellar nursery where new stars are born Eta Carinae – a massive, unstable star system approaching the end of its life Crab Nebula – the aftermath of a supernova, featuring a dense neutron star at its core Audio files with data sonifications for each object—mathematical translations of telescope data into sound Descriptive text to guide users through each model’s scientific significance and sensory interpretation These kits empower people of all ages and abilities to explore the cosmos through touch and sound—turning scientific data into a deeply human experience. Experience your universe through touch and sound at: https://chandra.si.edu/tactile/ministar.html Credits: 3D Prints Credit: NASA/CXC/ K. Arcand, A. Jubett, using software by Tactile Universe/N. Bonne & C. Krawczyk & Blender Sonifications: Dr. Kimberly Arcand (CXC), astrophysicist Dr. Matt Russo, and musician Andrew Santaguida (both of the SYSTEM Sounds project) 3D Model: K. Arcand, R. Crawford, L. Hustak (STScI) Photo of NASA’s Universe of Learning (UoL) 3D printed mini star kits sent to the Library of Congress state library hubs. The kits include 3D printed models of stars, sonifications, data converted into sound, and descriptive handouts available in both text and braille. Share Details Last Updated Apr 14, 2025 Editor NASA Science Editorial Team Related Terms Science Activation 3D Resources Astrophysics Manufacturing, Materials, 3-D Printing The Universe Explore More 5 min read With NASA’s Webb, Dying Star’s Energetic Display Comes Into Full Focus Article 5 hours ago 4 min read GLOBE Mission Earth Supports Career Technical Education Article 3 days ago 2 min read Hubble Captures a Star’s Swan Song Article 3 days 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

ESA/Hubble and NASA, A. Nota, P. Massey, E. Sabbi, C. Murray, M. Zamani (ESA/Hubble) This new image, released on April 4, 2025, showcases the dazzling young star cluster NGC 346. Although both the James Webb Space Telescope and the Hubble Space Telescope have released images of NGC 346 previously, this image includes new data and is the first to combine Hubble observations made at infrared, optical, and ultraviolet wavelengths into an intricately detailed view of this vibrant star-forming factory. Hubble’s exquisite sensitivity and resolution were instrumental in uncovering the secrets of NGC 346’s star formation. Using two sets of observations taken 11 years apart, researchers traced the motions of NGC 346’s stars, revealing them to be spiraling in toward the center of the cluster. This spiraling motion arises from a stream of gas from outside of the cluster that fuels star formation in the center of the turbulent cloud. Learn more about NGC 346 and the nebula it has shaped. Image credit: ESA/Hubble and NASA, A. Nota, P. Massey, E. Sabbi, C. Murray, M. Zamani (ESA/Hubble) View the full article

NASA’s Lucy spacecraft is 6 days and less than 50 million miles (80 million km) away from its second close encounter with an asteroid; this time, the small main belt asteroid Donaldjohanson. Download high-resolution video and images from NASA’s Scientific Visualization Studio. NASA/Dan Gallagher This upcoming event represents a comprehensive “dress rehearsal” for Lucy’s main mission over the next decade: the exploration of multiple Trojan asteroids that share Jupiter’s orbit around the Sun. Lucy’s first asteroid encounter – a flyby of the tiny main belt asteroid Dinkinesh and its satellite, Selam, on Nov. 1, 2023 – provided the team with an opportunity for a systems test that they will be building on during the upcoming flyby. Lucy’s closest approach to Donaldjohanson will occur at 1:51pm EDT on April 20, at a distance of 596 miles (960 km). About 30 minutes before closest approach, Lucy will orient itself to track the asteroid, during which its high-gain antenna will turn away from Earth, suspending communication. Guided by its terminal tracking system, Lucy will autonomously rotate to keep Donaldjohanson in view. As it does this, Lucy will carry out a more complicated observing sequence than was used at Dinkinesh. All three science instruments – the high-resolution greyscale imager called L’LORRI, the color imager and infrared spectrometer called L’Ralph, and the far infrared spectrometer called L’TES – will carry out observation sequences very similar to the ones that will occur at the Trojan asteroids. However, unlike with Dinkinesh, Lucy will stop tracking Donaldjohanson 40 seconds before the closest approach to protect its sensitive instruments from intense sunlight. “If you were sitting on the asteroid watching the Lucy spacecraft approaching, you would have to shield your eyes staring at the Sun while waiting for Lucy to emerge from the glare. After Lucy passes the asteroid, the positions will be reversed, so we have to shield the instruments in the same way,” said encounter phase lead Michael Vincent of Southwest Research Institute (SwRI) in Boulder, Colorado. “These instruments are designed to photograph objects illuminated by sunlight 25 times dimmer than at Earth, so looking toward the Sun could damage our cameras.” Fortunately, this is the only one of Lucy’s seven asteroid encounters with this challenging geometry. During the Trojan encounters, as with Dinkinesh, the spacecraft will be able to collect data throughout the entire encounter. After closest approach, the spacecraft will “pitch back,” reorienting its solar arrays back toward the Sun. Approximately an hour later, the spacecraft will re-establish communication with Earth. “One of the weird things to wrap your brain around with these deep space missions is how slow the speed of light is,” continued Vincent. “Lucy is 12.5 light minutes away from Earth, meaning it takes that long for any signal we send to reach the spacecraft. Then it takes another 12.5 minutes before we get Lucy’s response telling us we were heard. So, when we command the data playback after closest approach, it takes 25 minutes from when we ask to see the pictures before we get any of them to the ground.” Once the spacecraft’s health is confirmed, engineers will command Lucy to transmit the science data from the encounter back to Earth, which is a process that will take several days. Donaldjohanson is a fragment from a collision 150 million years ago, making it one of the youngest main belt asteroids ever visited by a spacecraft. “Every asteroid has a different story to tell, and these stories weave together to paint the history of our solar system,” said Tom Statler, Lucy mission program scientist at NASA Headquarters in Washington. “The fact that each new asteroid we visit knocks our socks off means we’re only beginning to understand the depth and richness of that history. Telescopic observations are hinting that Donaldjohanson is going to have an interesting story, and I’m fully expecting to be surprised – again.” NASA’s Goddard Space Flight Center in Greenbelt, Maryland, designed and built the L’Ralph instrument and provides overall mission management, systems engineering and safety and mission assurance for Lucy. Hal Levison of SwRI’s office in Boulder, Colorado, is the principal investigator. SwRI, headquartered in San Antonio, also leads the science team and the mission’s science observation planning and data processing. Lockheed Martin Space in Littleton, Colorado, built the spacecraft, designed the original orbital trajectory and provides flight operations. Goddard and KinetX Aerospace are responsible for navigating the Lucy spacecraft. The Johns Hopkins Applied Physics Laboratory in Laurel, Maryland, designed and built the L’LORRI (Lucy Long Range Reconnaissance Imager) instrument. Arizona State University in Tempe, Arizona, designed and build the L’TES (Lucy Thermal Emission Spectrometer) instrument. Lucy is the thirteenth mission in NASA’s Discovery Program, which is managed by NASA’s Marshall Space Flight Center in Huntsville, Alabama. By Katherine Kretke, Southwest Research Institute Media Contact: Karen Fox / Molly Wasser Headquarters, Washington 202-358-1600 karen.c.fox@nasa.gov / molly.l.wasser@nasa.gov Nancy N. Jones NASA’s Goddard Space Flight Center, Greenbelt, Md. Share Details Last Updated Apr 14, 2025 EditorMadison OlsonContactNancy N. Jonesnancy.n.jones@nasa.govLocationGoddard Space Flight Center Related TermsLucyGoddard Space Flight CenterPlanetary Science Explore More 4 min read New Modeling Assesses Age of Next Target Asteroid for NASA’s Lucy Article 4 weeks ago 3 min read NASA’s Lucy Spacecraft Takes Its 1st Images of Asteroid Donaldjohanson Article 2 months ago 3 min read NASA’s Lucy Asteroid Target Gets a Name Article 2 years ago View the full article

This long-duration photograph highlights the Roscosmos segment of the International Space Station with the Soyuz MS-26 spacecraft docked to the Rassvet module. Star trails and Earth’s atmospheric glow also are pictured from the orbital outpost as it soared 258 miles above the Pacific Ocean.Credit: NASA NASA astronaut Don Pettit, along with Roscosmos cosmonauts Alexey Ovchinin and Ivan Vagner, will depart the International Space Station aboard the Soyuz MS-26 spacecraft and return to Earth on Saturday, April 19. Pettit, Ovchinin, and Vagner will undock from the orbiting laboratory’s Rassvet module at 5:57 p.m. EDT, heading for a parachute-assisted landing at 9:20 p.m. (6:20 a.m. Kazakhstan time, Sunday, April 20) on the steppe of Kazakhstan, southeast of the town of Dzhezkazgan. Landing will occur on Pettit’s 70th birthday. NASA’s live coverage of return and related activities will stream on NASA+. Learn how to stream NASA content through a variety of platforms. A change of command ceremony also will stream on NASA platforms at 2:40 p.m. Friday, April 18. Ovchinin will handover station command to JAXA (Japan Aerospace Exploration Agency) astronaut Takuya Onishi for Expedition 73, which begins at the time of undocking. Spanning 220 days in space, Pettit and his crewmates will have orbited the Earth 3,520 times and completed a journey of 93.3 million miles over the course of their mission. The Soyuz MS-26 spacecraft launched and docked to the station on Sept. 11, 2024. This was Pettit’s fourth spaceflight, where he served as flight engineer for Expedition 71 and 72. He has a career total of 590 days in orbit. Ovchinin completed his fourth flight in space, totaling 595 days, and Vagner has earned an overall total of 416 days in space during two trips to the orbiting laboratory. After returning to Earth, the three crew members will fly on a helicopter from the landing site to the recovery staging city of Karaganda, Kazakhstan. Pettit will board a NASA plane and return to Houston, while Ovchinin and Vagner will depart for a training base in Star City, Russia. NASA’s coverage is as follows (all times Eastern and subject to changed based on real-time operations): Friday, April 18: 2:40 p.m. – Expedition 72/73 change of command ceremony begins on NASA+. Saturday, April 19: 2 p.m. – Farewells and hatch closing coverage begins on NASA+. 2:25 p.m. – Hatch closing 5:30 p.m. – Undocking coverage begins on NASA+. 5:57 p.m. – Undocking 8 p.m. – Coverage begins for deorbit burn, entry, and landing on NASA+. 8:26 p.m. – Deorbit burn 9:20 p.m. – Landing For more than two decades, people have lived and worked continuously aboard the International Space Station, advancing scientific knowledge, and making research breakthroughs that are not possible on Earth. The station is a critical testbed for NASA to understand and overcome the challenges of long-duration spaceflight and to expand commercial opportunities in low Earth orbit. As commercial companies focus on providing human space transportation services and destinations as part of a robust low Earth orbit economy, NASA is focusing more resources on deep space missions to the Moon as part of Artemis in preparation for future human missions to Mars. Learn more about International Space Station research and operations at: https://www.nasa.gov/station -end- Claire O’Shea / Josh Finch Headquarters, Washington 202-358-1100 claire.a.o’shea@nasa.gov / joshua.a.finch@nasa.gov Sandra Jones Johnson Space Center, Houston 281-483-5111 sandra.p.jones@nasa.gov Share Details Last Updated Apr 14, 2025 LocationNASA Headquarters Related TermsHumans in SpaceInternational Space Station (ISS) View the full article

Explore This Section Webb News Latest News Latest Images Blog (offsite) Awards X (offsite – login reqd) Instagram (offsite – login reqd) Facebook (offsite- login reqd) Youtube (offsite) Overview About Who is James Webb? Fact Sheet Impacts+Benefits FAQ Science Overview and Goals Early Universe Galaxies Over Time Star Lifecycle Other Worlds Observatory Overview Launch Deployment Orbit Mirrors Sunshield Instrument: NIRCam Instrument: MIRI Instrument: NIRSpec Instrument: FGS/NIRISS Optical Telescope Element Backplane Spacecraft Bus Instrument Module Multimedia About Webb Images Images Videos What is Webb Observing? 3d Webb in 3d Solar System Podcasts Webb Image Sonifications Team International Team People Of Webb More For the Media For Scientists For Educators For Fun/Learning 5 Min Read With NASA’s Webb, Dying Star’s Energetic Display Comes Into Full Focus NASA’s James Webb Space Telescope has taken the most detailed image of planetary nebula NGC 1514 to date thanks to its unique mid-infrared observations. Webb shows its rings as intricate clumps of dust. It’s also easier to see holes punched through the bright pink central region. Credits: NASA, ESA, CSA, STScI, Michael Ressler (NASA-JPL), Dave Jones (IAC) Gas and dust ejected by a dying star at the heart of NGC 1514 came into complete focus thanks to mid-infrared data from NASA’s James Webb Space Telescope. Its rings, which are only detected in infrared light, now look like “fuzzy” clumps arranged in tangled patterns, and a network of clearer holes close to the central stars shows where faster material punched through. “Before Webb, we weren’t able to detect most of this material, let alone observe it so clearly,” said Mike Ressler, a researcher and project scientist for Webb’s MIRI (Mid-Infrared Instrument) at NASA’s Jet Propulsion Laboratory in southern California. He discovered the rings around NGC 1514 in 2010 when he examined the image from NASA’s Wide-field Infrared Survey Explorer (WISE). “With MIRI’s data, we can now comprehensively examine the turbulent nature of this nebula,” he said. This scene has been forming for at least 4,000 years — and will continue to change over many more millennia. At the center are two stars that appear as one in Webb’s observation, and are set off with brilliant diffraction spikes. The stars follow a tight, elongated nine-year orbit and are draped in an arc of dust represented in orange. One of these stars, which used to be several times more massive than our Sun, took the lead role in producing this scene. “As it evolved, it puffed up, throwing off layers of gas and dust in in a very slow, dense stellar wind,” said David Jones, a senior scientist at the Institute of Astrophysics on the Canary Islands, who proved there is a binary star system at the center in 2017. Once the star’s outer layers were expelled, only its hot, compact core remained. As a white dwarf star, its winds both sped up and weakened, which might have swept up material into thin shells. Image A: Planetary Nebula NGC 1514 (MIRI Image) NASA’s James Webb Space Telescope has taken the most detailed image of planetary nebula NGC 1514 to date thanks to its unique mid-infrared observations. Webb shows its rings as intricate clumps of dust. It’s also easier to see holes punched through the bright pink central region. NASA, ESA, CSA, STScI, Michael Ressler (NASA-JPL), Dave Jones (IAC) Image B: Planetary Nebula NGC 1514 (WISE and Webb Images Side by Side) Two infrared views of NGC 1514. At left is an observation from NASA’s Wide-field Infrared Survey Explorer (WISE). At right is a more refined image from NASA’s James Webb Space Telescope. NASA, ESA, CSA, STScI, NASA-JPL, Caltech, UCLA, Michael Ressler (NASA-JPL), Dave Jones (IAC) Its Hourglass Shape Webb’s observations show the nebula is tilted at a 60-degree angle, which makes it look like a can is being poured, but it’s far more likely that NGC 1514 takes the shape of an hourglass with the ends lopped off. Look for hints of its pinched waist near top left and bottom right, where the dust is orange and drifts into shallow V-shapes. What might explain these contours? “When this star was at its peak of losing material, the companion could have gotten very, very close,” Jones said. “That interaction can lead to shapes that you wouldn’t expect. Instead of producing a sphere, this interaction might have formed these rings.” Though the outline of NGC 1514 is clearest, the hourglass also has “sides” that are part of its three-dimensional shape. Look for the dim, semi-transparent orange clouds between its rings that give the nebula body. A Network of Dappled Structures The nebula’s two rings are unevenly illuminated in Webb’s observations, appearing more diffuse at bottom left and top right. They also look fuzzy, or textured. “We think the rings are primarily made up of very small dust grains,” Ressler said. “When those grains are hit by ultraviolet light from the white dwarf star, they heat up ever so slightly, which we think makes them just warm enough to be detected by Webb in mid-infrared light.” In addition to dust, the telescope also revealed oxygen in its clumpy pink center, particularly at the edges of the bubbles or holes. NGC 1514 is also notable for what is absent. Carbon and more complex versions of it, smoke-like material known as polycyclic aromatic hydrocarbons, are common in planetary nebulae (expanding shells of glowing gas expelled by stars late in their lives). Neither were detected in NGC 1514. More complex molecules might not have had time to form due to the orbit of the two central stars, which mixed up the ejected material. A simpler composition also means that the light from both stars reaches much farther, which is why we see the faint, cloud-like rings. What about the bright blue star to the lower left with slightly smaller diffraction spikes than the central stars? It’s not part of this nebula. In fact, this star lies closer to us. This planetary nebula has been studied by astronomers since the late 1700s. Astronomer William Herschel noted in 1790 that NGC 1514 was the first deep sky object to appear genuinely cloudy — he could not resolve what he saw into individual stars within a cluster, like other objects he cataloged. With Webb, our view is considerably clearer. NGC 1514 lies in the Taurus constellation approximately 1,500 light-years from Earth. The James Webb Space Telescope is the world’s premier space science observatory. Webb will solve mysteries in our solar system, look beyond to distant worlds around other stars, and probe the mysterious structures and origins of our universe and our place in it. Webb is an international program led by NASA with its partners, ESA (European Space Agency) and the Canadian Space Agency. To learn more about Webb, visit: https://science.nasa.gov/webb Downloads Click any image to open a larger version. View/Download all image products at all resolutions for this article from the Space Telescope Science Institute. Media Contacts Laura Betz – laura.e.betz@nasa.gov NASA’s Goddard Space Flight Center, Greenbelt, Md. Claire Blome – cblome@stsci.edu Space Telescope Science Institute, Baltimore, Md. Christine Pulliam – cpulliam@stsci.edu Space Telescope Science Institute, Baltimore, Md. Science Advisor Michael Ressler (NASA-JPL) Related Information Read more about other planetary nebulae Watch: ViewSpace video about planetary nebulae View images of other planetary nebulae on AstroPix More Webb News More Webb Images Webb Science Themes Webb Mission Page Related For Kids What is the Webb Telescope? SpacePlace for Kids En Español Ciencia de la NASA NASA en español Space Place para niños Keep Exploring Related Topics James Webb Space Telescope Webb is the premier observatory of the next decade, serving thousands of astronomers worldwide. It studies every phase in the… Stars Stars Stories Universe Share Details Last Updated Apr 14, 2025 Editor Marty McCoy Contact Laura Betz laura.e.betz@nasa.gov Related Terms James Webb Space Telescope (JWST) Astrophysics Binary Stars Goddard Space Flight Center Nebulae Planetary Nebulae Science & Research Stars The Universe White Dwarfs View the full article

In an open challenge, NASA is seeking innovative business models that propose new approaches to solving complex Earth science problems using unconventional computing methods and is holding an informational webinar on Monday, April 28. The agency’s Beyond the Algorithm Challenge, sponsored by NASA’s Earth Science Technology Office, asks for proposals to more rapidly and accurately understand our home planet using transformative computing methods such as quantum computing, quantum machine learning, neuromorphic computing, in-memory computing, or other approaches. The Beyond the Algorithm Challenge kicked off in March and consists of three phases. Participant submissions, which are due on July 25, will be evaluated based on creativity, technical feasibility, impact, business model evaluation, and presentation. Up to 10 finalists will be invited to present their ideas to a panel of judges at a live pitch event, and winners will a monetary prize. For details about the challenge, interested participants can sign up for the informational webinar on Monday, April 28, here. Using the vantage point of space, NASA’s observations of Earth increase our understanding of our home planet, improve lives, and safeguard our future. The capabilities of NASA’s Earth Science Division include developing new technology, delivering actionable science, and providing environmental information to meet the increased demand for more sophisticated, more accurate, more trustworthy, and more actionable environmental information for decision-makers and policymakers. For example, rapid flood analysis is one area that may benefit from computing advancements. Flood hazards affect personal safety and land use, directly affecting individual livelihoods, community property, and infrastructure development and resilience. Advanced flood analysis capability enables contributions to protect and serve impacted communities, making a tangible difference in areas such as disaster preparedness, recovery, and resilience. Advancements in computing capabilities show promise in overcoming processing power, efficiency, and performance limitations of conventional computing methods in addressing Earth science challenges like rapid flood analysis. Quantum computers offer a fundamentally different paradigm of computation and can solve certain classes of problems exponentially faster than their classical counterparts. Likewise, quantum machine learning offers the potential to reduce required training data or produce more accurate models. The emerging field of neuromorphic, or brain-inspired, computing holds significant promise for algorithm development optimized for high-speed, low power. And in-memory computing saves time and energy for data-heavy processes like artificial intelligence training. Blue Clarity is hosting the Beyond the Algorithm Challenge on behalf of NASA. The NASA Tournament Lab, part of the Prizes, Challenges, and Crowdsourcing program in the Space Technology Mission Directorate, manages the challenge. The program supports global public competitions and crowdsourcing as tools to advance NASA research and development and other mission needs. For more information about the contest and a full list of rules and eligibility requirements, visit: https://www.nasa-beyond-challenge.org View the full article

Curiosity Navigation Curiosity Home Mission Overview Where is Curiosity? Mission Updates Science Overview Instruments Highlights Exploration Goals News and Features Multimedia Curiosity Raw Images Images Videos Audio Mosaics More Resources Mars Missions Mars Sample Return Mars Perseverance Rover Mars Curiosity Rover MAVEN Mars Reconnaissance Orbiter Mars Odyssey More Mars Missions Mars Home 2 min read Sols 4507-4508: “Just Keep Driving” NASA’s Mars rover Curiosity acquired this image using its Mars Hand Lens Imager (MAHLI), located on the turret at the end of the rover’s robotic arm, on April 9, 2025, Sol 4505 of the Mars Science Laboratory Mission, at 00:56:30 UTC. NASA/JPL-Caltech/MSSS Written by Natalie Moore, Mission Operations Specialist at Malin Space Science Systems Earth planning date: Wednesday, April 9, 2025 Our drive from Monday’s plan was mostly successful, putting us ~22 meters down the “road” out of an expected 30 meters. A steering command halted the drive a little short when we tried to turn-in-place but instead turned into a rock, which also had the effect of making our position too unstable for arm activities. Oh well! APXS data has been showing the recent terrain as being pretty similar in composition, so the team isn’t complaining about trying again after another drive. Plus, keeping the arm stowed should give us a little more power to play with in the coming sols (an ongoing struggle this Martian winter). Recently, my job on Mastcam has been to make sure our science imaging is as concurrent as possible with required rover activities. This strategy helps save rover awake time, AKA power consumption. Today we did a pretty good job with this, only increasing the total awake time by ~2 minutes even though we planned 52 images! Our imaging today included a mosaic of the “Devil’s Gate” ridge including some nodular bedrock and distant “Torote Bowl,” a mosaic of a close-by vein network named “Moonstone Beach,” and several sandy troughs surrounding the bedrock blocks we see here. ChemCam is planning a LIBS raster on a vertical vein in our workspace named “Jackrabbit Flat,” and a distant RMI mosaic of “Condor Peak” (a butte to the north we’re losing view of). Our drive will happen in the 1400 hour on the first sol, hopefully landing us successfully 53 meters further into this new valley on our way to the boxwork structures to the west! Post-drive, we’re including a test of a “Post Traverse Autonav Terrain Observation” AKA PoTATO – an easy drop-in activity for ground analysis of a rover-built navigation map of our new terrain. Plus we get to say PoTATO a lot. Explore More 3 min read Sols 4505-4506: Up, up and onto the Devil’s Gate Article 3 days ago 3 min read Sols 4502-4504: Sneaking Past Devil’s Gate Article 4 days ago 3 min read Sols 4500-4501: Bedrock With a Side of Sand Article 4 days ago Keep Exploring Discover More Topics From NASA Mars Resources Explore this page for a curated collection of Mars resources. Mars Exploration: Science Goals The key to understanding the past, present or future potential for life on Mars can be found in NASA’s four… Rover Basics Each robotic explorer sent to the Red Planet has its own unique capabilities driven by science. Many attributes of a… Curiosity Rover (MSL) View the full article

3 min read Preparations for Next Moonwalk Simulations Underway (and Underwater) From left, Ramon Pedoto, Nathan Walkenhorst, and Tyrell Jemison review information at NASA’s Marshall Space Flight Center in Huntsville, Alabama. The three team members developed new automation tools at Marshall for flight controllers working with the International Space Station (Credit: NASA/Tyrell Jemison Two new automation tools developed at NASA’s Marshall Space Flight Center in Huntsville, Alabama, are geared toward improving operations for flight controllers working with the International Space Station from the Huntsville Operations Support Center. The tools, called AutoDump and Permanently Missing Intervals Checker, will free the flight control team to focus on situational awareness, anomaly response, and real-time coordination. The space station experiences routine loss-of-signal periods based on communication coverage as the space station orbits the Earth. When signal is lost, an onboard buffer records data that could not be downlinked during that period. Following acquisition of signal, flight controllers previously had to send a command to downlink, or “dump,” the stored data. The AutoDump tool streamlines a repetitive data downlinking command from flight controllers by detecting a routine loss-of-signal, and then autonomously sending the command to downlink data stored in the onboard buffer when the signal is acquired again. Once the data has been downlinked, the tool will automatically make an entry in the console log to confirm the downlink took place. “Reliably and quickly sending these dump commands is important to ensure that space station payload developers can operate from the most current data,” said Michael Zekoff, manager of Space Systems Operations at Marshall. As a direct result of this tool, we have eliminated the need to manually perform routine data dump commands by as much as 40% for normal operations. Michael Zekoff Space Systems Operations Manager AutoDump was successfully deployed on Feb. 4 in support of the orbiting laboratory. The other tool, known as the Permanently Missing Intervals Checker, is another automated process coming online that will improve team efficiency. Permanently missing intervals are gaps in the data stream where data can be lost due to a variety of reasons, including network fluctuations. The missing intervals are generally short but are documented so the scientific community and other users have confirmation that the missing data is unable to be recovered. “The process of checking for and documenting permanently missing intervals is challenging and incredibly time-consuming to make sure we capture all the payload impacts,” said Nathan Walkenhorst, a NASA contractor with Bailey Collaborative Solutions who serves as a flight controller specialist. The checker will allow NASA to quickly gather and assess payload impacts, reduce disruptions to operations, and allow researchers to get better returns on their science investigations. It is expected to be deployed later this year. In addition to Walkenhorst, Zekoff also credited Ramon Pedoto, a software architect, and Tyrell Jemison, a NASA contractor and data management coordinator with Teledyne Brown Engineering Inc, for their work in developing the automation tools. The development of the tools also requires coordination between flight control and software teams at Marshall, followed by extensive testing in both simulated and flight environments, including spacecraft operations, communications coverage, onboard anomalies, and other unexpected conditions. “The team solicited broad review to ensure that the tool would integrate correctly with other station systems,” Zekoff said. “Automated tools are evaluated carefully to prevent unintended commanding or other consequences. Analysis of the tools included thorough characterization of the impacts, risk mitigation strategies, and approval by stakeholders across the International Space Station program.” The Huntsville Operations Support Center provides payload, engineering, and mission operations support to the space station, the Commercial Crew Program, and Artemis missions, as well as science and technology demonstration missions. The Payload Operations Integration Center within the Huntsville Operations Support Center operates, plans, and coordinates the science experiments onboard the space station 365 days a year, 24 hours a day. For more information on the International Space Station, visit: www.nasa.gov/international-space-station/ Share Details Last Updated Apr 11, 2025 EditorBeth RidgewayLocationMarshall Space Flight Center Related TermsMarshall Space Flight Center Explore More 3 min read NASA’s IMAP Arrives at NASA Marshall For Testing in XRCF Article 4 hours ago 7 min read NASA’s First Flight With Crew Important Step on Long-term Return to the Moon, Missions to Mars Article 3 days ago 3 min read NASA Selects Finalist Teams for Student Human Lander Challenge Article 1 week ago Keep Exploring Discover Related Topics Missions Humans in Space Climate Change Solar System View the full article

Explore This Section Science Science Activation GLOBE Mission Earth Supports… Overview Learning Resources Science Activation Teams SME Map Opportunities More Science Activation Stories Citizen Science 4 min read GLOBE Mission Earth Supports Career Technical Education The NASA Science Activation program’s GLOBE Mission EARTH (GME) project is forging powerful connections between career technical education (CTE) programs and real-world science, inspiring students across the United States to pursue careers in Science, Technology, Engineering, and Mathematics (STEM). GME is a collaborative effort between NASA scientists, educators, and schools that brings NASA Earth science and the GLOBE Program into classrooms to support hands-on, inquiry-based learning. GLOBE (Global Learning and Observations to Benefit the Environment) is an international science and education program that provides students and the public with the opportunity to participate in data collection and the scientific process, contributing meaningfully to our understanding of the Earth system. By connecting students directly to environmental research and NASA data, GME helps make science more relevant, engaging, and applicable to students’ futures. In CTE programs—where project-based and work-based learning are key instructional strategies—GME’s integration of GLOBE protocols offers students the chance to develop not only technical skills, but also essential data literacy and professional competencies like collaboration, critical thinking, and communication. These cross-cutting skills are valuable across a wide range of industries, from agriculture and advanced manufacturing to natural resources and public safety. The real-world, hands-on approach of CTE makes it an ideal setting for implementing GLOBE to support STEM learning across industries. At Skyline High School in Oakland, California, for example, GLOBE has been embedded in multiple courses within the school’s Green Energy Pathway, originally launched by GLOBE partner Tracy Ostrom. Over the past decade, nearly 1,000 students have participated in GLOBE activities at Skyline. Many of these students describe their experiences with environmental data collection and interactions with NASA scientists as inspiring and transformative. Similarly, at Toledo Technology Academy, GME is connecting students with NASA science and renewable energy projects—allowing them to study how solar panels impact their local environment and how weather conditions affect wind energy generation. To expand awareness of how GLOBE can enhance CTE learning and career preparation, WestEd staff Svetlana Darche and Nico Janik presented at the Educating for Careers Conference on March 3, 2025, in Sacramento, California. This event, sponsored by the California chapter of the Association for Career and Technical Education (ACTE), brought together over 2,600 educators dedicated to equipping students with the tools they need to succeed in an evolving job market. Darche and Janik’s session, titled “Developing STEM Skills While Contributing to Science,” showcased GLOBE’s role in work-based learning and introduced new federal definitions from the Carl D. Perkins Act (Perkins V) that emphasize: Interactions with industry professionals A direct link to curriculum and instruction First-hand engagement with real-world tasks in a given career field GLOBE’s approach to scientific data collection aligns perfectly with these criteria. Janik led 40 educators through a hands-on experience using the GLOBE Surface Temperature Protocol, demonstrating how students investigate the Urban Heat Island Effect while learning critical technical and analytical skills. By collecting and analyzing real-world data, students gain firsthand experience with the tools and methods used by scientists, bridging the gap between classroom learning and future career opportunities. Through GME’s work with CTE programs, students are not only learning science—they are doing science. These authentic experiences inspire, empower, and prepare students for careers where data literacy, scientific inquiry, and problem-solving are essential. With ongoing collaborations between GLOBE, NASA, and educators nationwide, the next generation of STEM professionals is already taking shape—one real-world investigation at a time. GME is supported by NASA under cooperative agreement award number NNX16AC54A 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 GreenEnergyPathway presenting the Green Energy Pathway CTE program. Share Details Last Updated Apr 11, 2025 Editor NASA Science Editorial Team Related Terms Science Activation Earth Science For Kids and Students Opportunities For Educators to Get Involved Explore More 1 min read Kudos Test Article Article 3 hours ago 4 min read New York Math Teacher Measures Trees & Grows Scientists with GLOBE Article 24 hours ago 3 min read NASA Science Supports Data Literacy for K-12 Students Article 2 days 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

NASA NASA astronauts Jim Lovell, Fred Haise, and Jack Swigert launch aboard the Apollo 13 spacecraft from NASA’s Kennedy Space Center in Florida on April 11, 1970. The mission seemed to be going smoothly until 55 hours and 55 minutes in when an oxygen tank ruptured. The new mission plan involved abandoning the Moon landing, looping around the Moon and getting the crew home safely as quickly as possible. The crew needed to go into “lifeboat mode,” using the lunar module Aquarius to save the spacecraft and crew. On April 17, the crew returned to Earth, splashing down in the Pacific Ocean near Samoa. Image credit: NASA View the full article

Explore This Section Earth Earth Observer Editor’s Corner Feature Articles Meeting Summaries News Science in the News Calendars In Memoriam More Archives Conference Schedules Style Guide 1 min read Kudos Test Article The Global Learning and Observations to Benefit the Environment (GLOBE) Program is calling on volunteers of all ages to help students and citizen scientists document seasonal change through leaf color and land cover. The data collection event will support students across North America, Latin America, Central America, and Europe, who are working together to document the seasonal changes taking place from September through December – see Figure. The observations will also provide vital data for GLOBE students creating student research projects for the GLOBE 2025 International Virtual Science Symposium (IVSS). The project is part of GLOBE’s Intensive Observation Period (IOP), which collects data during a focused period to assess how climate change is unfolding in different regions of the world. Share Details Last Updated Apr 11, 2025 Related Terms Earth Science View the full article

3 Min Read NASA’s IMAP Arrives at NASA Marshall For Testing in XRCF On March 18, NASA’s IMAP (Interstellar Mapping and Acceleration Probe) arrived at NASA’s Marshall Space Flight Center in Huntsville, Alabama, for thermal vacuum testing at the X-ray and Cryogenic Facility, which simulates the harsh conditions of space. The IMAP mission is a modern-day celestial cartographer that will map the solar system by studying the heliosphere, a giant bubble created by the Sun’s solar wind that surrounds our solar system and protects it from harmful interstellar radiation. To view this video please enable JavaScript, and consider upgrading to a web browser that supports HTML5 video NASA’s IMAP mission being loaded into the thermal vacuum chamber of NASA Marshall Space Flight Center’s X-Ray and Cryogenic Facility (XRCF) in Huntsville, Alabama. IMAP arrived at Marshall March 18 and was loaded into the chamber March 19.Credit: NASA/Johns Hopkins APL/Princeton/Ed Whitman Testing performed in the X-ray and Cryogenic Facility will help to assess the spacecraft before its journey toward the Sun. The IMAP mission will orbit the Sun at a location called Lagrange Point 1 (L1), which is about one million miles from Earth towards the Sun. From this location, IMAP can measure the local solar wind and scan the distant heliosphere without background from planets and their magnetic fields. The mission will use its suite of ten instruments to map the boundary of the heliosphere, analyze the composition of interstellar particles that make it through, and investigate how particles change as they move through the solar system. Furthermore, IMAP will maintain a continuous broadcast of near real-time space weather data from five instruments aboard IMAP that will be used to test new space weather prediction models and improve our understanding of effects impacting our human exploration of space. Team members from Marshall Space Flight Center in Huntsville, Alabama, install IMAP into the XRCF’s chamber dome before the start of the thermal vacuum test. NASA/Johns Hopkins APL/Princeton/Ed Whitman While inside the Marshall facility, the spacecraft will undergo dramatic temperature changes to simulate the environment during launch, on the journey toward the Sun, and at its final orbiting point. The testing facility has multiple capabilities including a large thermal vacuum chamber which simulates the harsh conditions of space such as extreme temperatures and the near-total absence of an atmosphere. Simulating these conditions before launch allow scientists and engineers to identify successes and potential failures in the design of the spacecraft. Team members from Marshall Space Flight Center in Huntsville, Alabama work to close the chamber door of the XRCF for IMAP testing. The chamber is 20 feet in diameter and 60 feet long making it one of the largest across NASA. NASA/Johns Hopkins APL/Princeton/Ed Whitman “The X-ray and Cryogenic Facility was an ideal testing location for IMAP given the chamber’s size, availability, and ability to meet or exceed the required test parameters including strict contamination control, shroud temperature, and vacuum level,” said Jeff Kegley, chief of Marshall’s Science Test Branch. The facility’s main chamber is 20 feet in diameter and 60 feet long, making it the 5th largest thermal vacuum chamber at NASA. It’s the only chamber that is adjoined to an ISO 6 cleanroom — a controlled environment that limits the number and size of airborne particles to minimize contamination. The IMAP mission will launch on a SpaceX Falcon 9 rocket from NASA’s Kennedy Space Center in Florida, no earlier than September. NASA’s IMAP mission was loaded into NASA Marshall’s XRCF thermal vacuum chamber where the spacecraft will undergo testing such as dramatic temperature changes to simulate the harsh environment of space. NASA/Johns Hopkins APL/Princeton/Ed Whitman Learn More about IMAP Media Contact: Lane Figueroa Marshall Space Flight Center Huntsville, Alabama 256.544.0034 lane.e.figueroa@nasa.gov Share Details Last Updated Apr 11, 2025 Related TermsMarshall Space Flight CenterGoddard Space Flight CenterHeliophysicsMarshall Heliophysics & Planetary ScienceMarshall Science Research & ProjectsMarshall X-Ray & Cryogenic FacilityThe SunThe Sun & Solar Physics Explore More 2 min read Hubble Captures a Star’s Swan Song The swirling, paint-like clouds in the darkness of space in this stunning image seem surreal,… Article 4 hours ago 6 min read NASA Webb’s Autopsy of Planet Swallowed by Star Yields Surprise Observations from NASA’s James Webb Space Telescope have provided a surprising twist in the narrative… Article 1 day ago 3 min read Hubble Helps Determine Uranus’ Rotation Rate with Unprecedented Precision An international team of astronomers using the NASA/ESA Hubble Space Telescope has made new measurements… Article 2 days ago Keep Exploring Discover More Topics From NASA Missions Humans in Space Climate Change Solar System View the full article

Explore Hubble Hubble Home Overview About Hubble The History of Hubble Hubble Timeline Why Have a Telescope in Space? Hubble by the Numbers At the Museum FAQs Impact & Benefits Hubble’s Impact & Benefits Science Impacts Cultural Impact Technology Benefits Impact on Human Spaceflight Astro Community Impacts Science Hubble Science Science Themes Science Highlights Science Behind Discoveries Hubble’s Partners in Science Universe Uncovered Explore the Night Sky Observatory Hubble Observatory Hubble Design Mission Operations Missions to Hubble Hubble vs Webb Team Hubble Team Career Aspirations Hubble Astronauts News Hubble News Social Media Media Resources Multimedia Multimedia Images Videos Sonifications Podcasts e-Books Online Activities Lithographs Fact Sheets Posters Hubble on the NASA App Glossary More 35th Anniversary Online Activities 2 min read Hubble Captures a Star’s Swan Song This NASA/ESA Hubble Space Telescope image features the planetary nebula Kohoutek 4-55. ESA/Hubble & NASA, K. Noll The swirling, paint-like clouds in the darkness of space in this stunning image seem surreal, like a portal to another world opening up before us. In fact, the subject of this NASA/ESA Hubble Space Telescope image is very real. We are seeing vast clouds of ionized atoms and molecules, thrown into space by a dying star. This is a planetary nebula named Kohoutek 4-55, a member of the Milky Way galaxy situated just 4,600 light-years away in the constellation Cygnus (the Swan). Planetary nebulae are the spectacular final display at the end of a giant star’s life. Once a red giant star has exhausted its available fuel and shed its last layers of gas, its compact core will contract further, enabling a final burst of nuclear fusion. The exposed core reaches extremely hot temperatures, radiating ultraviolet light that energizes the enormous clouds of gas cast off by the star. The ultraviolet light ionizes atoms in the gas, making the clouds glow brightly. In this image, red and orange indicate nitrogen, green is hydrogen, and blue shows oxygen. Kohoutek 4-55 has an uncommon, multi-layered form: a faint layer of gas surrounds a bright inner ring, all wrapped in a broad halo of ionized nitrogen. The spectacle is bittersweet, as the brief phase of fusion in the core will end after only tens of thousands of years, leaving a white dwarf that will never illuminate the clouds around it again. This image itself was also the final work of one of Hubble’s instruments: the Wide Field and Planetary Camera 2 (WFPC2). Installed in 1993 to replace the original Wide Field and Planetary Camera, WFPC2 was responsible for some of Hubble’s most enduring images and fascinating discoveries. Hubble’s Wide Field Camera 3 replaced WFPC2 in 2009, during Hubble’s final servicing mission. A mere ten days before astronauts removed Hubble’s WFPC2 from the telescope, the instrument collected the data used in this image: a fitting send-off after 16 years of discoveries. Image processors used the latest and most advanced processing techniques to bring the data to life one more time, producing this breathtaking new view of Kohoutek 4-55. Facebook logo @NASAHubble @NASAHubble Instagram logo @NASAHubble Share Details Last Updated Apr 10, 2025 Editor Andrea Gianopoulos Location NASA Goddard Space Flight Center Related Terms Hubble Space Telescope Astrophysics Astrophysics Division Emission Nebulae Goddard Space Flight Center Nebulae Planetary Nebulae Stars The Universe Keep Exploring Discover More Topics From Hubble Hubble Space Telescope Since its 1990 launch, the Hubble Space Telescope has changed our fundamental understanding of the universe. The Death Throes of Stars From colliding neutron stars to exploding supernovae, Hubble reveals new details of some of the mysteries surrounding the deaths of… Exploring the Birth of Stars Seeing ultraviolet, visible, and near-infrared light helps Hubble uncover the mysteries of star formation. Hubble’s Nebulae View the full article