SpaceMan

From left, team members Annie Meier, Malay Shah, and Jamie Toro assemble the flight hardware for NASA’s Orbital Syngas Commodity Augmentation Reactor, or OSCAR, on Oct. 10, 2019, in the Space Station Processing Facility at the agency’s Kennedy Space Center in Florida. OSCAR began as an Early Career Initiative project at the spaceport that studies technology to convert trash and human waste into useful gasses such as methane, hydrogen, and carbon dioxide. NASA/Cory Huston There’s no “I” in team, and that holds true for NASA and its partners as the agency ramps up efforts to recruit tenured professors to research science for a semester at the agency’s Kennedy Space Center in Florida. The tenured teachers work for up to a year in an area where the agency needs specific expertise. NASA often finds tenured professors – someone who has been guaranteed a job with their university until they retire – through seminars or publications. Assignments must be mutually beneficial to the agency and organizations involved. “At NASA, we want researchers who are doing something that could help us, that could be synergistic, and to not reinvent the wheel,” said Dr. Jose Nuñez, University Partnerships and Small Sat Capabilities manager at NASA Kennedy. “The goal is to find professors who can benefit the agency in an area that needs more research.” The U.S. government’s Intergovernmental Personnel Act Mobility Program allows the temporary assignment of personnel between the federal, state, local governments, colleges and universities, Indian tribal governments, federally funded research and development centers, and other eligible organizations. Dr. Reza Toufiq, an associate professor of chemical engineering at Florida Institute of Technology in Melbourne, Florida, is the first professor to leverage school funds to spend a semester at NASA Kennedy and work on projects dealing with waste and resource recovery. Toufiq specializes in how to convert everyday trash into energy, including the ash or char left behind from thermally treated trash. He worked with Dr. Annie Meier, who leads a team that converts astronauts’ trash into gasses that can be used for fuel. Flight hardware for NASA’s Orbital Syngas Commodity Augmentation Reactor, or OSCAR, is inside the Applied Physics Lab inside the Neil Armstrong Operations and Checkout Facility at the agency’s Kennedy Space Center in Florida on July 21, 2022. By processing small pieces of trash in a high-temperature reactor, OSCAR is advancing new and innovative technology for managing waste in space. NASA/Kim Shiflett “I wanted to learn on the terrestrial side how we can infuse some of our technology, and he wanted to learn from us to grow into the space sector, so it was a really cool match,” said Meier, technical lead for situ resource utilization and waste management resource recovery systems at NASA Kennedy. Although Toufiq’s sabbatical with NASA is over, his work is not. Meier just received approval for a project through a Space Act Agreement, which allows a research sponsor to use NASA scientists and facilities to benefit both parties. Meier and other researchers at NASA will give Toufiq information on space waste products and lunar regolith stimulants; in turn, he will do the testing, and provide data to the agency because some of that information is currently unknown. “He’s learning a lot about the fundamentals of different things with waste that we aren’t really doing, so we lean on academia to get some of that information and offer a fresh perspective,” Meier said. An intergovernmental assignment is generally approved for up to two years, but it can extend for up to six years with authorization. The length of the appointment also depends on the agency’s needs and university’s sabbatical guidelines, which could pay for one or more semesters. The University Partnerships team now is working to bring on two professors to NASA Kennedy next semester. “There are many tenured professors and universities who would like to come here, but we are careful to use due diligence to make sure what they’re doing is something that aligns with our research and technology interests,” Nuñez said. To learn more about the wide range of research happening at the Florida spaceport, click here. View the full article

3 min read Preparations for Next Moonwalk Simulations Underway (and Underwater) This illustration of the large Quetzalpetlatl Corona located in Venus’ southern hemisphere depicts active volcanism and a subduction zone, where the foreground crust plunges into the planet’s interior. A new study suggests coronae reveal locations where active geology is shaping Venus’ surface. The stars above and on Earth aligned as an inspirational message and lyrics from the song “The Rain (Supa Dupa Fly)” by hip-hop artist Missy Elliott were beamed to Venus via NASA’s DSN (Deep Space Network). The agency’s Jet Propulsion Laboratory in Southern California sent the transmission at 10:05 a.m. PDT on Friday, July 12. As the largest and most sensitive telecommunication service of NASA’s Space Communications and Navigation (SCaN) program, DSN has an array of giant radio antennas that allow missions to track, send commands, and receive scientific data from spacecraft venturing to the Moon and beyond. To date, the system has transmitted only one other song into space, making the transmission of Elliott’s song a first for hip-hop and NASA. “Both space exploration and Missy Elliott’s art have been about pushing boundaries,” said Brittany Brown, director, Digital and Technology Division, Office of Communications at NASA Headquarters in Washington, who initially pitched ideas to Missy’s team to collaborate with the agency. “Missy has a track record of infusing space-centric storytelling and futuristic visuals in her music videos so the opportunity to collaborate on something out of this world is truly fitting.” The song traveled about 158 million miles (254 million kilometers) from Earth to Venus — the artist’s favorite planet. Transmitted at the speed of light, the radio frequency signal took nearly 14 minutes to reach the planet. The transmission was made by the 34-meter (112-foot) wide Deep Space Station 13 (DSS-13) radio dish antenna, located at the DSN’s Goldstone Deep Space Communications Complex, near Barstow in California. Coincidentally, the DSS-13 also is nicknamed Venus. Elliott’s music career started more than 30 years ago, and the DSN has been communicating with spacecraft for over 60 years. Now, thanks to the network, Elliott’s music has traveled far beyond her Earth-bound fans to a different world. “I still can’t believe I’m going out of this world on tour with NASA through the Deep Space Network when “The Rain” (Supa Dupa Fly) becomes the first ever hip-hop song to transmit to space!,” said Elliott. “I chose Venus because it symbolizes strength, beauty, and empowerment and I am so humbled to have the opportunity to share my art and my message with the universe!” Two NASA missions, selected in 2021, will explore Venus and send data back to Earth using the DSN. DAVINCI (Deep Atmosphere Venus Investigation of Noble gases, Chemistry, and Imaging), led out of NASA’s Goddard Space Flight Center in Greenbelt, Maryland, is slated to launch no earlier than 2029. The VERITAS (Venus Emissivity, Radio Science, InSAR, Topography, and Spectroscopy), launching no earlier than 2031, is lead out of NASA’s Jet Propulsion Laboratory in Southern California. NASA and the DSN are also partnering with the ********* Space Agency’s Venus mission, Envision. A team at JPL is developing the spacecraft’s Venus Synthetic Aperture Radar (VenSAR). In continuous operations since 1963, NASA SCaN’s DSN is composed of three complexes spaced equidistant from each other — approximately 120 degrees apart in longitude — around the planet. The ground stations are in Goldstone in California, Madrid, and Canberra in Australia. The Deep Space Network is managed by JPL for the SCaN program within the Space Operations Mission Directorate, based at NASA Headquarters. For more information about NASA’s Deep Space Network, visit: [Hidden Content] Share Details Last Updated Jul 15, 2024 Related TermsGeneral Explore More 1 min read Attention Civil ******** Retirees Article 4 days ago 5 min read Surfing NASA’s Internet of Animals: Satellites Study Ocean Wildlife Article 5 days ago 1 min read NASA Technology Soars at Selfridge Air Show Article 6 days ago Keep Exploring Discover Related Topics Missions Humans in Space Climate Change Solar System View the full article

Painters work on the official NASA insignia, nicknamed “the meatball,” on the Vehicle Assembly Building at NASA’s Kennedy Space Center in Florida on May 29, 2020.NASA/Kim Shiflett NASA’s official logo, nicknamed the “meatball,” turned 65 on July 15, 2024. The insignia dates back to 1959, when the National Advisory Committee on Aeronautics (NACA) metamorphosed into an agency that would advance both space and aeronautics: the National Aeronautics and Space Administration. After a NASA Lewis (now Glenn) Research Center illustrator’s design was chosen for the new agency’s official seal, the head of Lewis’ Research Reports Division, James Modarelli, was asked by the executive secretary of NACA to design a logo that could be used for less formal purposes. In the design, the sphere represents a planet, the stars represent space, the red chevron is a wing representing aeronautics (the latest design in hypersonic wings at the time the logo was developed), and then there is an orbiting spacecraft going around the wing. The red, white, and blue design, which includes elements representing NASA’s space and aeronautics missions, became the official logo of the ******* States’ new space agency in 1959. Image Credit: NASA/Kim Shiflett View the full article

6 Min Read NASA’s Webb Investigates Eternal Sunrises, Sunsets on Distant World Artists concept of WASP-39 b (full image below). Near-infrared spectral analysis of terminator confirms differences in morning and evening atmosphere Researchers using NASA’s James Webb Space Telescope have finally confirmed what models have previously predicted: An exoplanet has differences between its eternal morning and eternal evening atmosphere. WASP-39 b, a giant planet with a diameter 1.3 times greater than Jupiter, but similar mass to Saturn that orbits a star about 700 light-years away from Earth, is tidally locked to its parent star. This means it has a constant dayside and a constant nightside—one side of the planet is always exposed to its star, while the other is always shrouded in darkness. Using Webb’s NIRSpec (Near-Infrared Spectrograph), astronomers confirmed a temperature difference between the eternal morning and eternal evening on WASP-39 b, with the evening appearing hotter by roughly 300 Fahrenheit degrees (about 200 Celsius degrees). They also found evidence for different cloud cover, with the forever morning portion of the planet being likely cloudier than the evening. Image A: Artist Concept WASP-39 b This artist’s concept shows what the exoplanet WASP-39 b could look like based on indirect transit observations from NASA’s James Webb Space Telescope as well as other space- and ground-based telescopes. Data collected by Webb’s NIRSpec (Near-Infrared Spectrograph) show variations between the eternal morning and evening atmosphere of the planet. Astronomers analyzed the 2- to 5-micron transmission spectrum of WASP-39 b, a technique that studies the exoplanet’s terminator, the boundary that separates the planet’s dayside and nightside. A transmission spectrum is made by comparing starlight filtered through a planet’s atmosphere as it moves in front of the star, to the unfiltered starlight detected when the planet is beside the star. When making that comparison, researchers can get information about the temperature, composition, and other properties of the planet’s atmosphere. “WASP-39 b has become a sort of benchmark planet in studying the atmosphere of exoplanets with Webb,” said Néstor Espinoza, an exoplanet researcher at the Space Telescope Science Institute and lead author on the study. “It has an inflated, puffy atmosphere, so the signal coming from starlight filtered through the planet’s atmosphere is quite strong.” Previously published Webb spectra of WASP-39b’s atmosphere, which revealed the presence of carbon dioxide, sulfur dioxide, water vapor, and sodium, represent the entire day/night boundary – there was no detailed attempt to differentiate between one side and the other. Now, the new analysis builds two different spectra from the terminator region, essentially splitting the day/night boundary into two semicircles, one from the evening, and the other from the morning. Data reveals the evening as significantly hotter, a searing 1,450 degrees Fahrenheit (800 degrees Celsius), and the morning a relatively cooler 1,150 degrees Fahrenheit (600 degrees Celsius). Image B: Transmission Spectra “It’s really stunning that we are able to parse this small difference out, and it’s only possible due Webb’s sensitivity across near-infrared wavelengths and its extremely stable photometric sensors,” said Espinoza. “Any tiny movement in the instrument or with the observatory while collecting data would have severely limited our ability to make this detection. It must be extraordinarily precise, and Webb is just that.” Extensive modeling of the data obtained also allows researchers to investigate the structure of WASP-39 b’s atmosphere, the cloud cover, and why the evening is hotter. While future work by the team will study how the cloud cover may affect temperature, and vice versa, astronomers confirmed gas circulation around the planet as the main culprit of the temperature difference on WASP-39 b. On a highly irradiated exoplanet like WASP-39 b that orbits relatively close to its star, researchers generally expect the gas to be moving as the planet rotates around its star: Hotter gas from the dayside should move through the evening to the nightside via a powerful equatorial jet stream. Since the temperature difference is so extreme, the air pressure difference would also be significant, which in turn would cause high wind speeds. Image C: Transit Light Curve Using General Circulation Models, 3-dimensional models similar to the ones used to predict weather patterns on Earth, researchers found that on WASP-39 b the prevailing winds are likely moving from the night side across the morning terminator, around the dayside, across the evening terminator and then around the nightside. As a result, the morning side of the terminator is cooler than the evening side. In other words, the morning side gets slammed with winds of air that have been cooled on the nightside, while the evening is hit by winds of air heated on the dayside. Research suggests the wind speeds on WASP-39 b can reach thousands of miles an hour! “This analysis is also particularly interesting because you’re getting 3D information on the planet that you weren’t getting before,” added Espinoza. “Because we can tell that the evening edge is hotter, that means it’s a little puffier. So, theoretically, there is a small swell at the terminator approaching the nightside of the planet.” The team’s results have been published in Nature. The researchers will now look to use the same method of analysis to study atmospheric differences of other tidally locked hot Jupiters, as part of Webb Cycle 2 General Observers Program 3969. WASP-39 b was among the first targets analyzed by Webb as it began regular science operations in 2022. The data in this study was collected under Early Release Science program 1366, designed to help scientists quickly learn how to use the telescope’s instruments and realize its full science potential. The James Webb Space Telescope is the world’s premier space science observatory. Webb is solving mysteries in our solar system, looking beyond to distant worlds around other stars, and probing 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 (********* Space Agency) and CSA (********* Space Agency). Downloads Right click any image to save it or open a larger version in a new tab/window via the browser’s popup menu. View/Download all image products at all resolutions for this article from the Space Telescope Science Institute. The research results have been published in Nature. Media Contacts Rob Gutro – *****@*****.tld NASA’s Goddard Space Flight Center, Greenbelt, Md. Hannah Braun *****@*****.tld Christine Pulliam – *****@*****.tld Space Telescope Science Institute, Baltimore, Md. Related Information ARTICLE: What is an Exoplanet? VIDEO: How do we learn about a planet’s Atmosphere? VIDEO: Reading the Rainbow of Light from an Exoplanet’s Atmosphere VIDEO: Science Snippets – Exoplanets BLOG: Reconnaissance of Potentially Habitable Worlds with NASA’s Webb More Webb News – [Hidden Content] More Webb Images – [Hidden Content] Webb Mission Page – [Hidden Content] Related For Kids What is a exoplanet? What is the Webb Telescope? SpacePlace for Kids En Español Para Niños : Qué es una exoplaneta? 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… Exoplanets Exoplanet Stories Universe Share Details Last Updated Jul 15, 2024 Editor Stephen Sabia Related Terms Astrophysics Exoplanet Atmosphere Exoplanet Science Exoplanets Gas Giant Exoplanets Goddard Space Flight Center James Webb Space Telescope (JWST) Science & Research The Universe View the full article

Buzzing with bees, baby birds, and wildflowers, the rooftop garden atop building 12 at Johnson Space Center in Houston reflects NASA’s commitment to environmental stewardship. Originally constructed in 1963, the facility was transformed in 2012, incorporating energy-efficient features that earned it LEED Gold certification. The certification is a globally recognized symbol of sustainability achievement and leadership. Today, the building serves as a testament to NASA’s commitment to ecological innovation. Nestled between the Mission Control Center and building 16, this hidden gem is part of a series of pioneering efforts at Johnson to demonstrate how even the most unexpected locations can become vibrant ecosystems. Aerial views of Johnson Space Center’s rooftop garden. NASA/Bill Stafford Initiated by Joel Walker, director of Center Operations, and designed alongside NASA engineers, the rooftop garden exemplifies green architecture with integrated solar panels, an underfloor air distribution system, and wind turbines. “It was something of an experiment to see what worked well and what we might use in future projects,” said Walker. Native Texas Bluebonnet atop building 12 at NASA’s Johnson Space Center in Houston. The Center Operations team leads sustainability efforts at Johnson, working across multiple directorates and teams. Together, they manage Johnson’s 1,600 acres, which host a diverse array of plants and wildlife. Building 12’s green roof provides benefits such as reduced potable water and energy usage, better stormwater management, protection from UV rays, and increased stability in high winds. This unique space provides an ideal environment for nesting birds and visiting pollinators and boasts a projected lifespan of 50 years, significantly longer than the 20 to 25 years typical of a conventional roof. “I was genuinely surprised by the variety of native species thriving in our rooftop garden,” said Johnson’s wildlife biologist Strausser. “We’ve observed far more species than we ever anticipated, which is both fascinating and encouraging for our conservation efforts.” Johnson team members meet on the building 12 rooftop to assess and monitor the plants. Initially, the project started with non-native ornamental plants that ******* in the harsh Houston climate. Replanting the garden yielded mixed results until the team hand-scattered a blend of native grass seed and wildflowers. This method proved to be a successful, at a fraction of the cost estimated for professional planting. “Sometimes the easiest way is the best!” said Walker. “It looks great now and is much more durable too.” View the full article

4 min read Preparations for Next Moonwalk Simulations Underway (and Underwater) This image shows an aviation version of a smartphone navigation app that makes suggestions for an aircraft to fly an alternate, more efficient route. The new trajectories are based on information available from NASA’s Digital Information Platform and processed by the Collaborative Departure Digital Rerouting tool.NASA Just like your smartphone navigation app can instantly analyze information from many sources to suggest the best route to follow, a NASA-developed resource is now making data available to help the aviation industry do the same thing. To assist air traffic managers in keeping airplanes moving efficiently through the skies, information about weather, potential delays, and more is being gathered and processed to support decision making tools for a variety of aviation applications. Appropriately named the Digital Information Platform (DIP), this living database hosts key data gathered by flight participants such as airlines or drone operators. It will help power additional tools that, among other benefits, can save you travel time. Ultimately, the aviation industry… and even the flying public, will benefit from what we develop. Swati Saxena NASA Aerospace Engineer “Through DIP we’re also demonstrating how to deliver digital services for aviation users via a modern cloud-based, service-oriented architecture,” said Swati Saxena, DIP project manager at NASA’s Ames Research Center in California. The intent is not to compete with others. Instead, the hope is that industry will see DIP as a reference they can use in developing and implementing their own platforms and digital services. “Ultimately, the aviation industry – the Federal Aviation Administration, commercial airlines, flight operators, and even the flying public – will benefit from what we develop,” Saxena said. The platform and digital services have even more benefits than just saving some time on a journey. For example, NASA recently collaborated with airlines to demonstrate a traffic management tool that improved traffic flow at select airports, saving thousands of pounds of jet fuel and significantly reducing carbon emissions. Now, much of the data gathered in collaboration with airlines and integrated on the platform is publicly available. Users who qualify can create a guest account and access DIP data at a new website created by the project. It’s all part of NASA’s vision for 21st century aviation involving revolutionary next-generation future airspace and safety tools. Managing Future Air Traffic During the 2030s and beyond, the skies above the ******* States are expected to become much busier. Facing this rising demand, the current National Airspace System – the network of U.S. aviation infrastructure including airports, air navigation facilities, and communications – will be challenged to keep up. DIP represents a key piece of solving that challenge. NASA’s vision for future airspace and safety involves new technology to create a highly automated, safe, and scalable environment. What this vision looks like is a flight environment where many types of vehicles and their pilots, as well as air traffic managers, use state-of-the-art automated tools and systems that provide highly detailed and curated information. These tools leverage new capabilities like machine learning and artificial intelligence to streamline efficiency and handle the increase in traffic expected in the coming decades. Digital Services Ecosystem in Action To begin implementing this new vision, our aeronautical innovators are evaluating their platform, DIP, and services at several airports in Texas. This initial stage is a building block for larger such demonstrations in the future. “These digital services are being used in the live operational environment by our airline partners to improve efficiency of the current airspace operations,” Saxena said. “The tools are currently in use in the Dallas/Fort Worth area and will be deployed in the Houston airspace in 2025.” The results from these digital tools are already making a difference. Proven Air Traffic Results During 2022, a NASA machine learning-based tool named Collaborative Digital Departure Rerouting, designed to improve the flow of air traffic and prevent flight delays, saved more than 24,000 lbs. (10,886 kg.) of fuel by streamlining air traffic in the Dallas area. If such tools were used across the entire country, the improvements made in efficiency, safety, and sustainability would make a notable difference to the flying public and industry. “Continued agreements with airlines and the aviation industry led to the creation and expansion of this partnership ecosystem,” Saxena said. “There have been benefits across the board.” DIP was developed under NASA’s Airspace Operations and Safety Program. Learn about NASA’s Collaborative Digital Departure Rerouting tool and how it uses information from the Digital Information Platform to provide airlines with routing options similar to how drivers navigate using cellphone apps. About the AuthorJohn GouldAeronautics Research Mission DirectorateJohn Gould is a member of NASA Aeronautics' Strategic Communications team at NASA Headquarters in Washington, DC. He is dedicated to public service and NASA’s leading role in scientific exploration. Prior to working for NASA Aeronautics, he was a spaceflight historian and writer, having a lifelong passion for space and aviation. Facebook logo @NASA@NASAaero@NASA_es @NASA@NASAaero@NASA_es Instagram logo @NASA@NASAaero@NASA_es Linkedin logo @NASA Explore More 2 min read NASA Prepares for Air Taxi Passenger Comfort Studies Article 2 weeks ago 2 min read Hypersonic Technology Project Overview Article 3 weeks ago 2 min read Hypersonics Technical Challenges Article 3 weeks ago Keep Exploring Discover More Topics From NASA Missions Artemis Aeronautics STEM Explore NASA’s History Share Details Last Updated Jul 12, 2024 EditorJim BankeContactJim Banke*****@*****.tld Related TermsAeronauticsAeronautics Research Mission DirectorateAir Traffic Management – ExplorationAir Traffic SolutionsAirspace Operations and Safety Program View the full article

Curiosity Navigation Curiosity Mission Overview Where is Curiosity? Mission Updates Science Overview Instruments Highlights Exploration Goals News and Features Multimedia Curiosity Raw Images Mars Resources Mars Missions Mars Sample Return Mars Perseverance Rover Mars Curiosity Rover MAVEN Mars Reconnaissance Orbiter Mars Odyssey More Mars Missions All Planets Mercury Venus Earth Mars Jupiter Saturn Uranus Neptune Pluto & Dwarf Planets 2 min read Sols 4241–4242: We Can’t Go Around It…We’ve Got To Go Through It! This image was taken by the Front Hazard Avoidance Camera (Front Hazcam) aboard NASA’s Mars rover Curiosity on Sol 4237 – Martian day 4,237 of the Mars Science Laboratory mission – on July 7, 2024 at 14:46:38 UTC. Earth planning date: Wednesday, July 10, 2024 Curiosity is currently trekking across Gediz Vallis channel because, as my nephew’s favorite book says, if we can’t go around it… we’ve got to go through it! Recently we’ve been parked for a while on the channel to drill “Mammoth Lakes,” ([Hidden Content]) and are now on the move once again exploring the rubbly rocks. Today the science team planned two sols of activity for Curiosity as we venture on through and across Gediz Vallis channel. On the first sol we undertake nearly two hours of planned science. This includes Navcam deck monitoring and a Mastcam tau, to measure dust in the atmosphere as part of our atmospheric and environmental activities, alongside some geology-focused observations. MAHLI is taking a close up image of “Donohue Pass” that we targeted with ChemCam LIBS and Mastcam imagery in the previous plan ([Hidden Content]). ChemCam will take a LIBS on a rock named “Negit Island” that caught the team’s eye with a lighter base and a darker upper section. ChemCam will also take two RMIs of Gediz Vallis, one to document the wall of Gediz Vallis channel that we can see up ahead of us, and one looking at the rocks that sit within the channel. Mastcam is also taking a look at the wall of Gediz Vallis, as well as continuing a mega-mosaic started in the last plan that took 54 images of “Stubblefield Canyon.” Today we planned another 48 images to document the rest of this area named “Echo Ridge.” ChemCam will take a passive observation of an interesting rubbly target in this region called “Wishbone Lake,” prior to a five-meter drive (about 16 feet) over to this feature. Once we have arrived, Curiosity will take some post-drive Navcam imaging and a MARDI image of our left-front wheel. After a well-deserved sleep, on the second sol of this plan Curiosity will automatically choose a LIBS target in our new workspace, before taking a dust-****** and suprahorizon movie to round off this plan. Written by Emma Harris, Graduate Student at Natural History Museum, London Share Details Last Updated Jul 12, 2024 Related Terms Blogs Explore More 2 min read Sols 4239-4240: ‘Vuggin’ Out’ Article 2 days ago 2 min read Sols 4236-4238: One More Time… for Contact Science at Mammoth Lakes Article 6 days ago 2 min read Sols 4234-4235: And That’s (Nearly) a Wrap on Mammoth Lakes! Article 1 week ago Keep Exploring Discover More Topics From NASA Mars Mars is the fourth planet from the Sun, and the seventh largest. It’s the only planet we know of inhabited… All Mars Resources Explore this collection of Mars images, videos, resources, PDFs, and toolkits. Discover valuable content designed to inform, educate, and inspire,… Rover Basics Each robotic explorer sent to the Red Planet has its own unique capabilities driven by science. Many attributes of a… 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… View the full article

Apollo astronaut Buzz Aldrin poses for a photograph beside the deployed ******* States flag during an Apollo 11 moonwalk on July 20, 1969. The Lunar Module is on the left, and the footprints of the astronauts are clearly visible in the soil of the moon.Credit: NASA As the agency explores more of the Moon than ever before under the Artemis campaign, NASA will celebrate the 55th anniversary of the first astronauts landing on the Moon through a variety of in-person, virtual, and engagement activities nationwide between Monday, July 15, and Thursday, July 25. Events will honor America’s vision and technology that enabled the Apollo 11 crewed lunar landing on July 20, 1969, as well as Apollo-era inventions and techniques that spread into public life, many of which are still in use today. Activities also will highlight NASA’s Artemis campaign, which includes landing the first woman, first person of ******, and first international astronaut on the Moon, inspiring great achievements, exploration, and scientific discovery for the benefit of all. NASA’s subject matter experts are available for a limited number of interviews about the anniversary. To request an interview virtually or in person, contact Jessica Taveau in the newsroom: *****@*****.tld. During the week of July 15, the agency also will share the iconic bootprint image and the significance of Apollo 11 to NASA’s mission, as well as use the #Apollo11 hashtag, across its digital platforms online. Additional activities from NASA include: Monday, July 15 and Tuesday, July 16, NASA’s Michoud Assembly Facility in New Orleans, Louisiana: NASA will host the rollout of the agency’s Artemis II SLS (Space Launch System) core stage. Friday, July 19, NASA’s Johnson Space Center in Houston: In a dedication and ribbon cutting, the center will name its building 12 the ‘Dorothy Vaughan Center in Honor of the Women of Apollo.’ Vaughan was a mathematician, computer programmer, and NASA’s first ****** manager. Sunday, July 21, NASA’s Goddard Space Flight Center in Greenbelt, Maryland: NASA Goddard will host a model rocket contest conducted by the National Association of Rocketry Headquarters Astro Modeling Section. This free contest is open to all model rocketeers and the public. Other activities include: Tuesday, July 16 through Wednesday, July 24, Space Center Houston: The center will host pop-up science labs, mission briefings, special tram tours that feature the Mission Control Center at NASA Johnson, and more. Friday, July 19 through Saturday, July 20, National Cathedral in Washington: The cathedral will host a festival marking the 50th anniversary of its Space Window, which contains a piece of lunar rock that was donated by NASA and the crew of Apollo 11. Thursday, July 25, San Diego Comic-****: NASA representatives will participate in a panel entitled ‘Exploring the Moon: the Artemis Generation.’ Panelists are:Stan Love, NASA astronaut A.C. Charania, NASA chief technologist Dionne Hernandez-Lugo, NASA’s Gateway Program Jackelynne Silva-Martinez, NASA Human Health and Performance For more details about NASA’s Apollo Program, please visit: [Hidden Content] -end- Cheryl Warner / Jessica Taveau Headquarters, Washington 202-356-1600 *****@*****.tld / *****@*****.tld Share Details Last Updated Jul 12, 2024 LocationNASA Headquarters Related TermsApollo 11Artemis View the full article

The distorted spiral galaxy at center, the Penguin, and the compact elliptical at left, the Egg, are locked in an active embrace. This near- and mid-infrared image combines data from NASA’s James Webb Space Telescope’s NIRCam (Near-Infrared Camera) and MIRI (Mid-Infrared Instrument), and marks the telescope’s second year of science. Webb’s view shows that their interaction is marked by a glow of scattered stars represented in blue. Known jointly as Arp 142, the galaxies made their first pass by one another between 25 and 75 million years ago, causing “fireworks,” or new star formation, in the Penguin. The galaxies are approximately the same mass, which is why one hasn’t consumed the other.NASA, ESA, CSA, STScI To celebrate the second science anniversary of NASA’s James Webb Space Telescope, the team has released a near- and mid-infrared image on July 12, 2024, of two interacting galaxies: The Penguin and the Egg. Webb specializes in capturing infrared light – which is beyond what our own eyes can see – allowing us to view and study these two galaxies, collectively known as Arp 142. Their ongoing interaction was set in motion between 25 and 75 million years ago, when the Penguin (individually cataloged as NGC 2936) and the Egg (NGC 2937) completed their first pass. They will go on to shimmy and sway, completing several additional loops before merging into a single galaxy hundreds of millions of years from now. Learn more about the Penguin and the Egg. Image Credit: NASA, ESA, CSA, STScI Text Credit: NASA Webb Mission Team View the full article

4 min read Preparations for Next Moonwalk Simulations Underway (and Underwater) Paul Dumbacher, right, lead test engineer for the Propulsion Test Branch at NASA’s Marshall Space Flight Center in Huntsville, Alabama, confers with Meredith Patterson, solid propulsion systems engineer, as they install the 11-inch hybrid rocket motor testbed into its cradle in Marshall’s East Test Stand. The new testbed, offering versatile, low-cost test opportunities to NASA propulsion engineers and their government, academic, and industry partners, reflects the collaboration of dozens of team members across multiple departments at Marshall. NASA/Charles Beason In June, engineers at NASA’s Marshall Space Flight Center in Huntsville, Alabama, unveiled an innovative, 11-inch hybrid rocket motor testbed. The new hybrid testbed, which features variable flow capability and a 20-second continuous ***** duration, is designed to provide a low-cost, quick-turnaround solution for conducting hot-***** tests of advanced nozzles and other rocket engine hardware, composite materials, and propellants. Solid rocket propulsion ******** a competitive, reliable technology for various compact and heavy-lift rockets as well as in-space missions, offering low propulsion element mass, high energy density, resilience in extreme environments, and reliable performance. “It’s time consuming and costly to put a new solid rocket motor through its paces – identifying how materials perform in extreme temperatures and under severe structural and dynamic loads,” said Benjamin Davis, branch chief of the Solid Propulsion and Pyrotechnic Devices Branch of Marshall’s Engineering Directorate. “In today’s fast-paced, competitive environment, we wanted to find a way to condense that schedule. The hybrid testbed offers an exciting, low-cost solution.” Initiated in 2020, the project stemmed from NASA’s work to develop new composite materials, additively manufactured – or 3D-printed – nozzles, and other components with proven benefits across the spacefaring spectrum, from rockets to planetary landers. After analyzing future industry requirements, and with feedback from NASA’s aerospace partners, the Marshall team recognized that their existing 24-inch rocket motor testbed – a subscale version of the Space Launch System booster – could prove too costly for small startups. Additionally, conventional, six-inch test motors limited flexible configuration and required multiple tests to achieve all customer goals. The team realized what industry needed most was an efficient, versatile third option. “The 11-inch hybrid motor testbed offers the instrumentation, configurability, and cost-efficiency our government, industry, and academic partners need,” said Chloe Bower, subscale solid rocket motor manufacturing lead at Marshall. “It can accomplish multiple test objectives simultaneously – including different nozzle configurations, new instrumentation or internal insulation, and various propellants or flight environments.” “That quicker pace can reduce test time from months to weeks or days,” said Precious Mitchell, solid propulsion design lead for the project. Engineers at NASA’s Marshall Space Flight Center in Huntsville, Alabama, assess components of the 11-inch hybrid rocket motor testbed in the wake of successful testing in June. Among Marshall personnel leading in-house development of the new testbed are, from left, Chloe Bower, subscale solid rocket motor manufacturing lead; Jacobs manufacturing engineer Shelby Westrich; and Precious Mitchell, solid propulsion design lead. NASA/Benjamin Davis Another feature of great interest is the on/off switch. “That’s one of the big advantages to a hybrid testbed,” Mitchell continued. “With a solid propulsion system, once it’s ignited, it will ***** until the fuel is spent. But because there’s no oxidizer in hybrid fuel, we can simply turn it off at any point if we see anomalies or need to fine-tune a test element, yielding more accurate test results that precisely meet customer needs.” The team expects to deliver to NASA leadership final test data later this summer. For now, Davis congratulates the Marshall propulsion designers, analysts, chemists, materials engineers, safety personnel, and test engineers who collaborated on the new testbed. “We’re not just supporting the aerospace industry in broad terms,” he said. “We’re also giving young NASA engineers a chance to get their hands ****** in a practical test environment solving problems. This work helps educate new generations who will carry on NASA’s mission in the decades to come.” For nearly 65 years, Marshall teams have led development of the U.S. space program’s most powerful rocket engines and spacecraft, from the Apollo-era Saturn V rocket and the space shuttle to today’s cutting-edge propulsion systems, including NASA’s newest rocket, the Space Launch System. NASA technology testbeds designed and built by Marshall engineers and their partners have shaped the reliable technologies of spaceflight and continue to enable discovery, testing, and certification of advanced rocket engine materials and manufacturing techniques. Learn more about NASA Marshall capabilities at: [Hidden Content] Ramon J. Osorio Marshall Space Flight Center, Huntsville, Alabama 256-544-0034 *****@*****.tld Share Details Last Updated Jul 12, 2024 EditorBeth RidgewayLocationMarshall Space Flight Center Related TermsMarshall Space Flight Center Explore More 15 min read The Marshall Star for July 10, 2024 Article 2 days ago 4 min read NASA Marshall Researchers Battle Biofilm in Space Article 2 days ago 30 min read The Marshall Star for July 3, 2024 Article 1 week ago View the full article

6 Min Read Vivid Portrait of Interacting Galaxies Marks Webb’s Second Anniversary Webb’s view of the interacting galaxies of Arp 142 that combines Webb’s NIRCam and MIRI instrument images. Full image below. Two for two! A duo of interacting galaxies commemorates the second science anniversary of NASA’s James Webb Space Telescope, which takes constant observations, including images and highly detailed data known as spectra. Its operations have led to a “parade” of discoveries by astronomers around the world. “Since President Biden and Vice President Harris unveiled the first image from the James Webb Space Telescope two years ago, Webb has continued to unlock the mysteries of the universe,” said NASA Administrator Bill Nelson. “With remarkable images from the corners of the cosmos, going back nearly to the beginning of time, Webb’s capabilities are shedding new light on our celestial surroundings and inspiring future generations of scientists, astronomers, and explorers.” “In just two years, Webb has transformed our view of the universe, enabling the kind of world-class science that drove NASA to make this mission a reality,” said Mark Clampin, director of the Astrophysics Division at NASA Headquarters in Washington. “Webb is providing insights into longstanding mysteries about the early universe and ushering in a new era of studying distant worlds, while returning images that inspire people around the world and posing exciting new questions to answer. It has never been more possible to explore every facet of the universe.” The telescope’s specialization in capturing infrared light — which is beyond what our own eyes can detect — shows these galaxies, collectively known as Arp 142, locked in a slow cosmic dance. Webb’s observations, which combine near- and mid-infrared light from Webb’s NIRCam (Near-Infrared Camera) and MIRI (Mid-Infrared Instrument), respectively, clearly show that they are joined by a haze represented in blue that is a mix of stars and gas, a result of their mingling. Their ongoing interaction was set in motion between 25 and 75 million years ago, when the Penguin (individually cataloged as NGC 2936) and the Egg (NGC 2937) completed their first pass. They will go on to shimmy and sway, completing several additional loops before merging into a single galaxy hundreds of millions of years from now. Image A: Interacting Galaxies Arp 142 (NIRCam and MIRI) The distorted spiral galaxy at center, the Penguin, and the compact elliptical at left, the Egg, are locked in an active embrace. This near- and mid-infrared image combines data from NASA’s James Webb Space Telescope’s NIRCam (Near-Infrared Camera) and MIRI (Mid-Infrared Instrument), and marks the telescope’s second year of science. Webb’s view shows that their interaction is marked by a glow of scattered stars represented in blue. Known jointly as Arp 142, the galaxies made their first pass by one another between 25 and 75 million years ago, causing “fireworks,” or new star formation, in the Penguin. The galaxies are approximately the same mass, which is why one hasn’t consumed the other. Let’s Dance! Before their first approach, the Penguin held the shape of a spiral. Today, its galactic center gleams like an eye, its unwound arms now shaping a beak, head, backbone, and fanned-out tail. Like all spiral galaxies, the Penguin is still very rich in gas and dust. The galaxies’ “dance” gravitationally pulled on the Penguin’s thinner areas of gas and dust, causing them to ****** in waves and form stars. Look for those areas in two places: what looks like a fish in its “beak” and the “feathers” in its “tail.” Surrounding these newer stars is smoke-like material that includes carbon-containing molecules, known as polycyclic aromatic hydrocarbons, which Webb is exceptional at detecting. Dust, seen as fainter, deeper orange arcs also swoops from its beak to tail feathers. In contrast, the Egg’s compact shape ******** largely unchanged. As an elliptical galaxy, it is filled with aging stars, and has a lot less gas and dust that can be pulled away to form new stars. If both were spiral galaxies, each would end the first “twist” with new star formation and twirling curls, known as tidal tails. Another reason for the Egg’s undisturbed appearance: These galaxies have approximately the same mass or heft, which is why the smaller-looking elliptical wasn’t consumed or distorted by the Penguin. It is estimated that the Penguin and the Egg are about 100,000 light-years apart — quite close in astronomical terms. For context, the Milky Way galaxy and our nearest neighbor, the Andromeda Galaxy, are about 2.5 million light-years apart. They too will interact, but not for about 4 billion years. Now, look to the top right to spot a galaxy that is not at this party. This edge-on galaxy, cataloged PGC 1237172, is 100 million light-years closer to Earth. It’s also quite young, teeming with new, blue stars. Want one more party trick? Switch to Webb’s mid-infrared-only image to see PGC 1237172 practically disappear. Mid-infrared light largely captures cooler, older stars and an incredible amount of dust. Since the galaxy’s stellar population is so young, it “vanishes” in mid-infrared light. Image B: Interacting Galaxies Arp 142 (MIRI Only) NASA’s James Webb Space Telescope’s mid-infrared view of interacting galaxies Arp 142 seems to sing in primary colors. The Egg shows up as a tiny, teal-******** oval, because it is made up of old stars and has lost or used up most of its gas and dust. At right, the Penguin’s star-forming regions are represented in pink and purple, and contain smoke-like material known as polycyclic aromatic hydrocarbons. Also take a moment to scan the background. Webb’s image is overflowing with distant galaxies. Some take spiral and oval shapes, like those threaded throughout the Penguin’s “tail feathers,” while others scattered throughout are shapeless dots. This is a testament to the sensitivity and resolution of the telescope’s infrared instruments. (Compare Webb’s view to the 2018 observation that combines infrared light from NASA’s retired Spitzer Space Telescope and near-infrared and visible light from NASA’s Hubble Space Telescope.) Even though these observations only took a few hours, Webb revealed far more distant, redder, and dustier galaxies than previous telescopes – one more reason to expect Webb to continue to expand our understanding of everything in the universe. Want more? Take a tour to the image, “fly through” it in a visualization, and compare Webb’s image to the Hubble Space Telescope’s. Arp 142 ***** 326 million light-years from Earth in the constellation Hydra. Video: Tour the Arp 142 Image Video tour transcript Credit: NASA, ESA, CSA, STScI, Danielle Kirshenblat (STScI) Video: Arp 142 Visualization Credit: NASA, ESA, CSA, Ralf Crawford (STScI), Joseph DePasquale (STScI), ********** Nieves (STScI), Joseph Olmsted (STScI), Alyssa Pagan (STScI), Frank Summers (STScI), Greg Bacon (STScI) Image C: Compare Hubble/Webb Image Before/After The James Webb Space Telescope is the world’s premier space science observatory. Webb is solving mysteries in our solar system, looking beyond to distant worlds around other stars, and probing 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 (********* Space Agency) and CSA (********* Space Agency). Downloads Right click any image to save it or open a larger version in a new tab/window via the browser’s popup menu. View/Download all image products at all resolutions for this article from the Space Telescope Science Institute. Media Contacts Laura Betz – laura.e*****@*****.tld, Rob Gutro – *****@*****.tld NASA’s Goddard Space Flight Center, Greenbelt, Md. Claire Blome – *****@*****.tld Christine Pulliam – *****@*****.tld Space Telescope Science Institute, Baltimore, Md. Related Information Video: Learn more about Arp 142 and galaxy collisions Video: Learn more about galactic collisions Video: What happens when galaxies collide? Interactive: Explore “Interacting Galaxies: Future of the Milky Way” – Video: Galaxy Collisions: Simulations vs. Observations Article: More about Galaxy Evolution More Webb News More Webb Images Webb Mission Page Related For Kids What is a galaxy? What is the Webb Telescope? SpacePlace for Kids En Español ¿Qué es una galaxia? 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… Hubble Space Telescope Since its 1990 launch, the Hubble Space Telescope has changed our fundamental understanding of the universe. Hubble vs. Webb Galaxies View the full article

3 min read Hubble Measures the Distance to a Supernova This NASA/ESA Hubble Space Telescope image features the galaxy NGC 3810. ESA/Hubble & NASA, D. Sand, R. J. Foley Measuring the distance to truly remote objects like galaxies, quasars, and galaxy clusters is a crucial task in astrophysics, particularly when it comes to studying the early universe, but it’s a difficult one to complete. We can only measure the distances to a few nearby objects like the Sun, planets, and some nearby stars directly. Beyond that, astronomers need to use various indirect methods; one of the most important examines Type Ia supernovae, and this is where the NASA/ESA Hubble Space Telescope excels. NGC 3810, the galaxy featured in this image, was the host of a Type Ia supernova in 2022. In early 2023, Hubble focused on this and a number of other galaxies to closely examine recent Type Ia supernovae. Type Ia supernovae are the result of a white dwarf exploding, and their peak brightness is very consistent. This attribute allows astronomers to use Type Ia supernovae to measure distances: we know how bright a Type Ia supernova should be, so we can tell how far away it must be by how dim it appears. One snag with this method is intergalactic dust. Because intergalactic dust blocks some of the supernova’s light, astronomers need to determine how much light the dust reduces to accurately measure the supernova’s brightness and calculate its distance. Hubble’s unique capabilities offer them a clever way of doing this. Astronomers use Hubble to take images of the same Type Ia supernovae in ultraviolet light, which the dust almost completely blocks out, and in infrared light, which passes through dust nearly unaffected. By carefully noting how much light comes through at each wavelength, astronomers can determine how much dust ***** between Hubble and the supernova, letting them confidently calibrate the relationship between a supernova’s brightness and its distance. Hubble’s unique capability to observe in ultraviolet and infrared wavelengths of light in great detail with the same instrument makes it the perfect tool for these types of observations. Indeed, some of the data used to make this beautiful image of NGC 3810 focused on its 2022 supernova. You can see it as a point of light just below the galactic nucleus in the annotated image below. This annotated Hubble image of NGC 3810 denotes the location of the Type Ia supernovae SN 2022zut, It was the eighteen thousand, one hundred and forty-second supernova found in 2022! ESA/Hubble & NASA, D. Sand, R. J. Foley There are many ways to measure cosmic distances, but Type Ia supernovae are one of the most useful and accurate tools because they are so bright. Astronomers must use other methods as well, either as an independent check against other distance measurements, or to measure at much closer or farther distances. One such method, that also works for galaxies, is comparing their rotation speed to their brightness; based on that method, NGC 3810 is about 50 million light-years from Earth. Download the featured image Download the annotated image Explore More Hubble Space Telescope Hubble’s Galaxies The ****** Throes of Stars Exploring the Birth of Stars Facebook logo @NASAHubble @NASAHubble Instagram logo @NASAHubble Media Contact: Claire Andreoli NASA’s Goddard Space Flight Center, Greenbelt, MD *****@*****.tld Share Details Last Updated Jul 12, 2024 Editor Andrea Gianopoulos Location NASA Goddard Space Flight Center Related Terms Astrophysics Astrophysics Division Galaxies Goddard Space Flight Center Hubble Space Telescope Missions Spiral Galaxies Stars Supernovae 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. Discovering a Runaway Universe Our cosmos is growing, and that expansion rate is accelerating. Hubble E-books Hubble Images View the full article

Portrait of retired NASA astronaut Joe Engle wearing flight suit in front of an X-15 fighter circa 1963. Retired NASA astronaut and U.S. Air Force Maj. Gen. Joe Engle ***** July 10, surrounded by his family at home in Houston. Among his many honors, he is the only astronaut to pilot both the X-15 and space shuttle. He was 91. Engle became an astronaut at age 32 while flying the X-15 for the U.S. Air Force, becoming the youngest pilot ever to qualify as an astronaut. When selected as a NASA astronaut candidate in 1966, he was the only person selected that was already engaged in spaceflight operations. He was the last surviving X-15 pilot. “A natural pilot, Gen. Joe Engle helped humanity’s dreams take flight – in the X-15 program, the Apollo Program, and as one of the first commanders in the Space Shuttle Program,” said NASA Administrator Bill Nelson. “He was one of the first astronauts I met at NASA’s Johnson Space Center in Houston. I’ll never forget his big smile, his warmth, and his courage. We all will miss him.” Engle was born in Dickinson County, Kansas, and attended the University of Kansas, Lawrence, where he graduated with a degree in Aeronautical Engineering in 1955. He received his commission through the Air Force Reserve Officers Training Course, earning his pilot wings in 1958. As a NASA astronaut, he supported the Apollo Program, and was backup lunar module pilot for Apollo 14. In 1977, he served as commander of the space shuttle Enterprise, which used a modified Boeing 747 shuttle carrier aircraft to release Enterprise for approach and landing tests. In November 1981, he commanded the second flight of the space shuttle Columbia. He was the first and only pilot to manually fly an aerospace vehicle from Mach 25 to landing. He accumulated the last of his 224 hours in space when he commanded the space shuttle Discovery in August 1985, one of the most challenging shuttle missions ever. On that mission the crew deployed three commercial satellites and retrieved, repaired, and redeployed another malfunctioning satellite that had been launched on a previous shuttle mission. “As we mourn the immense loss of Joe, we’re thankful for his notable contributions to the advancement of human spaceflight,” said Vanessa Wyche, center director, NASA Johnson. “Joe’s accomplishments and legacy of perseverance will continue to inspire and impact generations of explorers for years to come.” Engle flew more than 180 different aircraft types and logged more than 14,000 flight hours. His military decorations include the Department of Defense Distinguished Service Medal, U.S. Air Force Distinguished Service Medal, and the Air Force Distinguished Flying Cross with Oak Leaf Cluster. He has received the NASA Distinguished Service Medal and Space Flight Medal, as well as the Harmon International Aviation Trophy, the Collier Trophy, the Goddard Space Trophy, the Gen. Thomas D. White Space Trophy, and the Kinchelow Experimental Test Pilot’s Trophy. In 1992, he was inducted into the Aerospace Walk of Honor. “Joe Henry was a loving husband, father, and grandfather. Blessed with natural piloting skills, General Joe, as he was known to many, was at his happiest in any cockpit. Always with a smile, he lived a fulfilled life as a proud *********, U.S. Air Force pilot, astronaut, and Kansas Jayhawk,” said his wife, Jeanie Engle. “His passing leaves a tremendous loss in our hearts. We take comfort that he has joined Tom Stafford and George Abbey, two of the best friends anyone could ask for.” Learn more about Engle’s life as an astronaut and pilot: [Hidden Content] -end- ****** McKie / Cheryl Warner Headquarters, Washington 202-358-1600 ***********@*****.tld / *****@*****.tld Chelsey Ballarte / Courtney Beasley Johnson Space Center, Houston 281-483-5111 c*****@*****.tld / *****@*****.tld View the full article

A few days before they left Skylab on Feb. 8, 1974, the final crew to occupy the station raised its altitude, hoping to keep it in orbit until a future space shuttle could revisit it. But higher than predicted solar activity caused the Earth’s atmosphere to expand, increasing drag on the large vehicle, causing its orbit to decay faster than expected. In 1978, controllers reactivated the station and changed its attitude, hoping to keep it in orbit as long as possible by reducing atmospheric drag. In the meantime, delays in the space shuttle’s development eventually made it impossible for a shuttle to revisit Skylab before it reentered the Earth’s atmosphere. On July 11, 1979, Skylab reentered, with debris landing over the Indian Ocean and Australia. Lessons learned from deorbiting large spacecraft like Skylab and others will inform the eventual deorbiting of the International Space Station. Left: Skylab as it appeared to the final crew upon its departure. Middle: Illustration of a proposed Skylab boost mission by the space shuttle. Right: A more whimsical depiction of the Skylab reboost by the space shuttle, as drawn by a cartoonist at NASA’s Johnson Space Center in Houston. When the Skylab 4 astronauts departed the station on Feb. 8, 1974, they left it in a 269-by-283-mile orbit. Just one day after the crew left the station, operators in the Mission Control Center at NASA’s Johnson Space Center in Houston ran a few final systems checks, oriented Skylab in a gravity-gradient attitude – meaning the heavier workshop faced the Earth – vented its atmosphere, and turned off its power. In this attitude, and based on predictions of the Sun’s activity in the upcoming solar cycle that would increase atmospheric drag and reduce Skylab’s altitude, scientists estimated that the station would remain in orbit until March 1983. However, the solar cycle intensified into the second most active one in a century and atmospheric perturbations shifted Skylab out of the gravity-gradient attitude, increasing its drag. By 1977, revised estimates projected Skylab’s reentry occurring as early as mid-1979. Although the space shuttle had yet to fly, NASA devised a plan for astronauts on one of its early missions to attach a rocket stage to Skylab and use it to either boost the station into a higher storage orbit or deorbit it in a controlled fashion into the Pacific Ocean. At 169,000 pounds, Skylab represented the heaviest spacecraft to reenter up to that time, and engineers believed that some of its components would survive the entry. Keeping the debris away from populated areas remained a priority. Left: Plot of Skylab’s altitude from launch until reentry. Right: Illustration of the five ground stations used during the reactivation and tracking of Skylab. To ensure that Skylab stayed aloft long enough for this shuttle mission to reach it, NASA needed to reactivate it. Because Skylab had no ability to reboost itself, its rate of decay could only be slightly controlled by changing the station’s attitude. Between March and June 1978, using the limited communications afforded by five ground stations, a small team of controllers methodically reactivated Skylab after a more than four-year passive *******. Remarkably, the station’s systems, including its all-important batteries, had survived the intervening ******* in good condition. When controllers fully reactivated Skylab on June 11, 1978, its altitude had decreased to 250 miles, and to prolong its life NASA decided to keep the station activated to control its attitude. Using its Thruster Attitude Control System, operators commanded Skylab into an End On Velocity Vector (EOVV) minimum drag attitude, with its forward end pointing in the direction of flight. Skylab remained in the EOVV attitude until Jan. 25, 1979, and engineers estimated that this extended the station’s orbital life by 3.5 months. By late 1978, with slips in the shuttle schedule, saving Skylab seemed no longer feasible. In a Dec. 19, 1978, press conference, NASA’s Associate Administrator for Space Transportation Systems John F. Yardley announced the cancellation of the shuttle reboost mission and the end of efforts to control Skylab’s attitude. Yardley emphasized the low likelihood of an uncontrolled Skylab reentry resulting in debris hitting populated areas, citing the example of the spent second stage of the Saturn V rocket that launched Skylab. That empty stage, larger in size although at 83,000 pounds less massive than Skylab, reentered out of control on Jan. 11, 1975, falling harmlessly into the Atlantic Ocean, about 1,000 miles west of Gibraltar. Left: Illustration of Skylab in the End On Velocity Vector minimum drag attitude. Middle: Cartoon of “Skylab is falling” fever. Image credit: courtesy Chicago Tribune. Right: Ground track of Skylab’s final orbit and the debris footprint in the Indian Ocean and Australia. On Jan. 25, 1979, controllers maneuvered Skylab from EOVV to solar inertial attitude, the orientation it maintained during its operational life, to ensure its solar arrays remained pointed at the Sun to keep the station’s batteries charged. Studies indicated that as Skylab descended below 161 miles, aerodynamic torques would make it difficult to maintain the solar inertial attitude. On June 20, with Skylab at 163 miles, controllers commanded it into a high-drag Torque Equilibrium Attitude (TEA). This gave controllers the ability to select the best orbit to ******** the final reentry, one that overflew mostly water to minimize any potential harm to people and property. Orbit 34,981 on July 11 met those criteria. On that orbit, after Skylab passed over North America, it flew southeast over the Atlantic Ocean, round the southern tip of *******, then northeast across the Indian Ocean before passing over the next major landmass, mainly sparsely populated areas of Australia. On the planned day of reentry, controllers commanded Skylab into a slow tumble at an altitude of 93 miles to better aim the entry point to the east of the southern tip of *******, causing the breakup over the Indian Ocean. After this point, the ground no longer controlled the station. With a debris footprint possibly 3,500 miles long, some debris landing in Australia remained a possibility. Left: Skylab’s entry path over Western Australia, showing sites that recovered debris from the station. Middle and right: The museum in Esperance, Western Australia, displays an oxygen tank and a titanium tank from Skylab. Image credits: courtesy Ben Cooper. Left: Operators in Mission Control at NASA’s Johnson Space Center in Houston during the Skylab reentry. Right: Managers and flight controllers monitor Skylab’s reentry. Tracking at the Bermuda station indicated Skylab’s large solar array still attached to the workshop. Controllers at Ascension Island in the South Atlantic made contact with Skylab as it flew 66 miles overhead, its large solar array beginning to detach from the workshop, itself already heating from the reentry. Once the disintegrating station passed out of range of Ascension, it continued its reentry unmonitored. Skylab finally broke apart at an altitude of 10 miles, slightly lower than expected, moving the impact footprint further east than planned. Pieces of Skylab falling on Western Australia created sonic booms heard by the inhabitants of the few towns in the Outback. The actual documented debris footprint stretched 2,450 miles. A museum in Esperance houses some of the recovered debris. Skylab Flight Director Charles S. Harlan said in a news conference after the event, “The surprise is over. No more suspense. Skylab is on the planet Earth.” Left: The Salyut 7-Kosmos 1686 complex photographed by the last departing crew. Middle: Reentry trajectory of the Salyut 7-Kosmos 1686 complex. Image credit: courtesy H. Klinkrad. Right: A piece of Salyut 7 recovered in Argentina. Image credit: courtesy Carlos Zelayeta. In contrast to the partially controlled Skylab entry, the Salyut 7-Kosmos 1686 complex made an uncontrolled reentry over Argentina on Feb. 7, 1991. At 88,491 pounds, the complex had about half the mass of Skylab. Although controllers had sent all previous Salyut stations on controlled reentries into the Pacific Ocean, they lost communications with Salyut 7 more than two years before its reentry. A crew last occupied the Salyut 7-Kosmos 1686 complex in June 1986. In August 1986, engines on the Kosmos 1686 module raised the complex’s orbit by 84 miles to 295 miles, with an anticipated reentry in 1994. Like Skylab, controllers considered a possible retrieval of Salyut 7 by a Buran space shuttle before that program’s cancellation. The last communications with Salyut 7 occurred in December 1989. Again, like Skylab, higher than anticipated solar activity in the late 1980s accelerated its descent. The station initially entered a gravity gradient attitude with the heavier Kosmos 1686 facing the Earth, but that attitude degraded significantly as the station encountered denser atmosphere in January 1991. And although said to be uncontrollable, apparently on Feb. 5, ground teams commanded it into a head on attitude to reduce drag and direct entry to an orbit that overflew less populated areas. Fuel depletion did not allow completion of the maneuver and atmospheric drag torqued the vehicle away from this attitude. Although planned for reentry over the south Pacific Ocean, Salyut 7 overshot the target and came down over Argentina, with a few fragments recovered. Left: The Mir complex in 1998. Middle: The March 2001 reentry of Mir photographed from Fiji. Right: The reentry trajectory of Mir in March 2001. Lessons learned from the earlier reentries of large space stations led controllers to devise a three-stage process to deorbit the Mir space station in a controlled fashion into the Pacific Ocean in March 2001. In the first stage, controllers allowed orbital drag to bring the 285,940-pound station, at the time the heaviest object to reenter, down to an average altitude of 140 miles. For the second stage, on March 23, the docked Progress M1-5 fired its engines twice to lower Mir’s orbit to 103 by 137 miles. Two orbits later, the Progress fired its engines for 22 minutes to bring Mir out of orbit. It burned up on reentry over the South Pacific Ocean, with observers in Nadi, Fiji, watching its final moments. The International Space Station, the largest spacecraft in orbit. In anticipation of the eventual controlled disposal of the International Space Station, on June 26, 2024, NASA selected SpaceX to develop and deliver the U.S. Deorbit Vehicle. The vehicle will safely deorbit the space station, the largest and, at over 900,000 pounds, by far the heaviest spacecraft in orbit, after the end of its operational life, currently expected in 2030. Past experiences can provide useful lessons learned. Explore More 8 min read 30 Years Ago: STS-65, the Second International Microgravity Lab Mission Article 1 day ago 11 min read Fourth of July Holidays in Space Article 1 week ago 9 min read 40 Years Ago: STS-41D – First Space Shuttle Launch Pad Abort Article 2 weeks ago View the full article

“We have a group photo of my first project here, ASTRO-H, and that one means a lot to me because I came [to that NASA project] fresh off the street. I was super scared and intimidated. It was me and three other [technicians], who were also all new, and a handful of very seasoned scientists and engineers. And we came together. “And we actually came in — I believe — under budget, ahead of schedule, and exceeded all expectations for our test results. That’s kind of unheard of, you know what I mean? We had such a good environment in the lab. Everybody got along so well. It was all teamwork. And everything just gelled. “So when I look back on that photo from 14 years ago, first of all, I look really young in it. And secondly, it makes me realize how blessed and lucky I’ve been to be here for so long. It reminds me of that guy who was really nervous and still did alright. [It reminds me] to have a little confidence in myself, just be me, and do the work. It’ll all work out. “I love looking back at that first team photo and just remembering how raw everything was at the time and how well it still came out.” —Clifton Brown, Engineering Technician, OMES III, NASA’s Goddard Space Flight Center Image Credit: NASA/Thalia Patrinos Interviewer: NASA/Thalia Patrinos Check out some of our other Faces of NASA. View the full article

NASA/Eric Bordelon Team members are installing pedestals aboard NASA’s Pegasus barge to hold and secure the massive core stage of NASA’s SLS (Space Launch System) rocket, indicating NASA barge crews are nearly ready for its first delivery to support the Artemis II test flight around the Moon. The barge will ferry the core stage on a 900-mile journey from the agency’s Michoud Assembly Facility in New Orleans to its Kennedy Space Center in Florida. The Pegasus crew began installing the pedestals July 10.The barge, which previously was used to ferry space shuttle external tanks, was modified and refurbished to compensate for the much larger and heavier core stage for the SLS rocket. Measuring 212 feet in length and 27.6 feet in diameter, the core stage is the largest rocket stage NASA has ever built and the longest item ever shipped by a NASA barge. Pegasus now measures 310 feet in length and 50 feet in width, with three 200-kilowatt generators on board for power. Tugboats and towing vessels will move the barge and core stage from Michoud to Kennedy, where the core stage will be integrated with other elements of the rocket and prepared for launch. Pegasus is maintained at NASA Michoud. NASA is working to land the first woman, first person of ******, and its first international partner astronaut on the Moon under Artemis. SLS is part of NASA’s backbone for deep space exploration, along with the Orion spacecraft, supporting ground systems, advanced spacesuits and rovers, the Gateway in orbit around the Moon, and commercial human landing systems. SLS is the only rocket that can send Orion, astronauts, and supplies to the Moon in a single launch. View the full article

Cosmic Road Trip: four distinct composite images from NASA’s Chandra X-ray Observatory and the James Webb Space Telescope, presented in a two-by-two grid, Rho Ophiuchi at lower right, the heart of the Orion Nebula at upper right, the galaxy NGC 3627 at lower left and the galaxy cluster MACS J0416.X-ray: NASA/CXC/SAO; Optical/Infrared: (Hubble) NASA/ESA/STScI; IR: (JWST) NASA/ESA/CSA/STScI It’s time to take a cosmic road trip using light as the highway and visit four stunning destinations across space. The vehicles for this space get-away are NASA’s Chandra X-ray Observatory and James Webb Space Telescope. The first stop on this tour is the closest, Rho Ophiuchi, at a distance of about 390 light-years from Earth. Rho Ophiuchi is a cloud complex filled with gas and stars of different sizes and ages. Being one of the closest star-forming regions, Rho Ophiuchi is a great place for astronomers to study stars. In this image, X-rays from Chandra are purple revealing infant stars that violently flare and produce X-rays. Infrared data from Webb are red, yellow, cyan, light blue and darker blue and provide views of the spectacular regions of gas and dust. X-ray: NASA/CXC/MIT/C. Canizares; IR: NASA/ESA/CSA/STScI/K. Pontoppidan; Image Processing: NASA/ESA/STScI/Alyssa Pagan, NASA/CXC/SAO/L. Frattare and J. Major The next destination is the Orion Nebula. Still located in the Milky Way galaxy, this region is a little bit farther from our home planet at about 1,500 light-years away. If you look just below the middle of the three stars that make up the “belt” in the constellation of Orion, you may be able to see this nebula through a small telescope. With Chandra and Webb, however, we get to see so much more. Chandra reveals young stars that glow brightly in X-rays, ******** in red, green, and blue, while Webb shows the gas and dust in darker red that will help build the next generation of stars here. X-ray: NASA/CXC/Penn State/E.Fei It’s time to leave our galaxy and visit another. Like the Milky Way, NGC 3627 is a spiral galaxy that we see at a slight angle. NGC 3627 is known as a “barred” spiral galaxy because of the rectangular shape of its central region. From our vantage point, we can also see two distinct spiral arms that appear as arcs. X-rays from Chandra in purple show evidence for a supermassive ****** ***** in its center while Webb finds the dust, gas, and stars throughout the galaxy in red, green, and blue. This image also contains optical data from the Hubble Space Telescope in red, green, and blue. Spiral galaxy NGC 3627.X-ray: NASA/CXC/SAO; Optical: NASA/ESO/STScI, ESO/WFI; Infrared: NASA/ESA/CSA/STScI/JWST; Image Processing:/NASA/CXC/SAO/J. Major Our final landing place on this trip is the farthest and the biggest. MACS J0416 is a galaxy cluster, which are among the largest objects in the Universe held together by gravity. Galaxy clusters like this can contain hundreds or even thousands of individual galaxies all immersed in massive amounts of superheated gas that Chandra can detect. In this view, Chandra’s X-rays in purple show this reservoir of hot gas while Hubble and Webb pick up the individual galaxies in red, green, and blue. ACS J0416 galaxy cluster.X-ray: NASA/CXC/SAO/G. Ogrean et al.; Optical/Infrared: (Hubble) NASA/ESA/STScI; IR: (JWST) NASA/ESA/CSA/STScI/Jose M. Diego (IFCA), Jordan C. J. D’Silva (UWA), Anton M. Koekemoer (STScI), Jake Summers (****), Rogier Windhorst (****), Haojing Yan (University of Missouri) NASA’s Marshall Space Flight Center manages the Chandra program. The Smithsonian Astrophysical Observatory’s Chandra X-ray Center controls science from Cambridge Massachusetts and flight operations from Burlington, Massachusetts. Read more from NASA’s Chandra X-ray Observatory. For more Chandra images, multimedia and related materials, visit: [Hidden Content] Visual Description: This release features four distinct composite images from NASA’s Chandra X-ray Observatory and the James Webb Space Telescope, presented in a two-by-two grid. At our lower right is Rho Ophiuchi, a cloud complex filled with gas, and dotted with stars. The murky green and gold cloud resembles a ghostly head in profile, swooping down from the upper left, trailing tendrils of hair. Cutting across the bottom edge and lower righthand corner of the image is a long, narrow, brick red cloud which resembles the ember of a stick pulled from a *****. Several large white stars dot the image. Many are surrounded by glowing neon purple rings, and gleam with diffraction spikes. At our upper right of the grid is a peek into the heart of the Orion Nebula, which blankets the entire image. Here, the young star nursery resembles a dense, stringy, dusty rose cloud, peppered with thousands of glowing golden, white, and blue stars. Layers of cloud around the edges of the image, and a concentration of bright stars at its distant core, help convey the depth of the nebula. In the lower left of the two-by-two grid is a hazy image of a spiral galaxy known as NGC 3627. Here, the galaxy appears pitched at an oblique angle, tilted from our upper left down to our lower right. Much of its face is angled toward us, making its spiral arms, composed of red and purple dots, easily identifiable. Several bright white dots ringed with neon purple speckle the galaxy. At the galaxy’s core, where the spiral arms converge, a large white and purple glow identified by Chandra provides evidence of a supermassive ****** *****. At the upper left of the grid is an image of the distant galaxy cluster known as MACS J0416. Here, the blackness of space is packed with glowing dots and tiny shapes, in *******, purples, oranges, golds, and reds, each a distinct galaxy. Upon close inspection (and with a great deal of zooming in!) the spiraling arms of some of the seemingly tiny galaxies are revealed in this highly detailed image. Gently arched across the middle of the frame is a soft band of purple; a reservoir of superheated gas detected by Chandra. News Media Contact Megan Watzke Chandra X-ray Center Cambridge, Mass. 617-496-7998 Lane Figueroa Marshall Space Flight Center Huntsville, Ala. 256-544-0034 View the full article

“I did not know that NASA Langley was right here in my own backyard. I was born and raised in Portsmouth, Virginia, and NASA Langley is in Hampton, about 45 minutes away. All throughout elementary school, I didn’t know that NASA was here. I always thought NASA was in Florida or Texas or somewhere. “I was in this summer program [in eighth grade], learning physics at the university. I vividly remember we had a guest speaker. He was an ******** ********* mechanical engineer and he had on the blue flight suit. And he said he worked at NASA, and it just blew my mind. “And at that point, I saw myself in him. I didn’t even know that NASA was here, so close to me, and I hadn’t seen anybody who had ever worked there. So that left a mark in my mind: ‘Wow, NASA is here.’ “… When I was in college, I came back to my high school to talk to a class about majoring in physics. And there was a student, maybe two years under me. I remember meeting her. I remember interacting. I remember talking with her just briefly at this career fair event. “I found out years later that seeing me in high school and hearing my experience in college inspired her to major in physics, and so she became the first robotics director at her school. And now she’s a principal. And it just rocked me because I was just being me and trying to share. It seemed like I paid it forward the same way that NASA mechanical engineer made a mark on me.” — Dr. Phillip Williams, Acting Center Chief Technologist, NASA’s Langley Research Center Image Credit: NASA/Mark Knopp Interviewer: NASA/Thalia Patrinos Check out some of our other Faces of NASA. View the full article

When the first humans travel to the Red Planet, they will need to know how to repair and maintain equipment, grow their own food, and stay healthy, all while contending with Earth-to-Mars communication delays. They must also find ways to build comradery and have fun. The first all-volunteer CHAPEA (Crew Health and Performance Exploration Analog) crew accomplished all of that and more during their 378-day analog mission on the surface of Mars. Living in the isolated Mars Dune Alpha, a 3D-printed, 1,700-square-foot habitat, crew members Kelly Haston, Ross Brockwell, Nathan Jones, and Anca Selariu faced the rigors of a simulated Mars expedition, enduring stressors akin to those of a real mission to the Red Planet. They also celebrated holidays and birthdays, gave each other haircuts, and found moments of levity in isolation. Their journey will help scientists understand the challenges of deep space missions and offer invaluable insights into the resilience of the human spirit. NASA’s CHAPEA (Crew Health and Performance Exploration Analog) crew member Kelly Haston greets Deputy Director of Flight Operations Kjell Lindgren and Johnson Space Center Deputy Director Stephen Koerner at the habitat’s door. NASA/Josh Valcarcel As the crew concluded their journey on July 6, NASA astronaut and Deputy Director of Flight Operations Kjell Lindgren opened the habitat door and welcomed them home. “The crew and their families have committed a year of their lives in service to NASA, the country, and humanity’s exploration of space. Thank you to for committing yourselves to research that will enable our future exploration of space,” he said. “Your fingerprints are going to be an indelible part of those first footprints on Mars.” The CHAPEA crew brought their diverse backgrounds and experiences to the mission, collaborating with NASA’s scientists and engineers to collect data that will provide insight into maintaining crew health and performance for future missions to Mars. PHOTO DATE: July 06, 2024 LOCATION: Bldg. 220 – CHAPEA Habitat SUBJECT: ASA Crew Health and Performance Exploration Analog (CHAPEA) Mars Analog Mission 1 Egress Event with crew Anca Selariu, Nathan Jones, Kelly Haston, Ross Brockwell. PHOTOGRAPHER: NASA/Josh ValcarcelNASA/Josh Valcarcel Kelly Haston: Mission Commander and Pioneering Scientist Haston, the mission commander, is a research scientist who builds human ******** models. She has spearheaded innovative stem cell-based projects, deriving multiple cell types for work in infertility, liver ********, and neurodegeneration. Her role was pivotal in maintaining crew morale and ensuring the success of daily operations. She highlighted the importance of teamwork and adaptability in a mission with such high stakes. “We had to rely on each other and our training to navigate the challenges we faced,” she said. “Every day brought new obstacles, but also new opportunities for growth and learning.” Nathan Jones: Medical Officer and Expert Communicator Jones, the crew medical officer, used his emergency and international medicine experience to tackle the unique challenges of the Mars mission. His expertise in problem-solving and effective communication in a time-sensitive and resource-limited environment was essential due to the approximately one-hour transmission delay. “Even something as simple as when to communicate is important,” said Jones. The crew had to consider what observations were essential to report to each other or Mission Control to avoid overburdening the team or unnecessarily using the limited bandwidth to Earth. “Everything we do in CHAPEA is touched by the heroes working on the ground at NASA,” he said. “We couldn’t ask for a better experience or better people to work with.” The experience evolved into a journey of personal growth for Jones. “I am constantly looking forward, planning for the future,” he said. “I learned to take time to enjoy the current season and be patient for the coming ones.” He also discovered a new hobby: art. “I have even surprised myself with how well some of my sketches have turned out,” he said. Anca Selariu: Microbiologist and Innovative Thinker Anca Selariu brought expertise as a microbiologist in the U.S. Navy, with a background in viral vaccine discovery, prion transmission, gene therapy development, and infectious ******** research management. Selariu expressed that she owes much to the Navy, including her involvement in CHAPEA, as it helped shape her both personally and professionally. “I hope to bring back a fresh perspective, along with a strong inclination to think differently about a problem, and test which questions are worth asking before we set out answering them,” she said. Reflecting on the mission, Selariu said, “Every day seemed to be a new revelation about something; about Earth, about art, about humans, about cultures, about the history of life in the universe – what little we know of it.” She added, “As much as I appreciate having information at my fingertips, I will miss the luxury of being unplugged in a world that now validates humans by their digital presence.” Ross Brockwell: Structural Engineer and Problem Solver Brockwell, the mission’s flight engineer, focused on infrastructure, building design, and organizational leadership. His structural engineering background influenced his approach to problem solving in the CHAPEA habitat. “An engineering perspective leads you to build an understanding of how things will react and interact, anticipate possible ******** points, and ensure redundancy and contingency planning,” he said. That mindset helped the crew develop creative solutions to mission challenges, such as using a 3D printer to design part adapters and tools and find ways to connect as a team. “Several things we wanted to do for fun required innovation, one being developing a bracket so we could safely and securely mount our mini-basketball hoop,” he said. He advises Artemis Generation members interested in contributing to future analog missions to think about systems engineering theory and learn to develop and integrate whole systems while solving individual challenges. Brockwell believes the most important attributes for a CHAPEA crew member are imagination and a strong sense of wonder. “Of course, one needs to have patience, self-control, emotional regulation, and a sense of humor,” he said. “I would also add perspective, which means understanding the importance of exploration missions on behalf of humankind and appreciating being part of something greater than oneself.” The CHAPEA crew is “back on Earth” after their 378-day mission inside the simulated Martian habitat. NASA /Josh Valcarcel A Vision for the Future As the first CHAPEA mission concludes, the data collected and experiences shared by the crew will pave the way for future explorations, bringing humanity one step closer to setting foot on Mars. “One of the biggest things I have learned on this long-duration mission is that we should never underestimate the effects of small gains over time,” said Jones. “Be willing to do the hard things now and it may make all the difference for the future.” Selariu emphasized the importance of interdisciplinary collaboration in upcoming space missions. “What everyone at CHAPEA seems to have in common is passion for space and drive to pursue it no matter the challenges, inconvenience, and personal sacrifices.” Brockwell looks forward to missions to the Red Planet becoming a reality. “It still fills me with awe and excitement to think that one day there will be people on the surface of other worlds, overcoming immense challenges and expanding the existence and awareness of life from Earth.” View the full article

5 Min Read NASA’s Hubble Traces Dark Matter in Dwarf Galaxy Using Stellar Motions This NASA Hubble Space Telescope image reveals a section of the Draco dwarf galaxy. Credits: NASA, ESA, Eduardo Vitral, Roeland van der Marel, and Sangmo Tony Sohn (STScI); Image processing: Joseph DePasquale (STScI) The qualities and behavior of dark matter, the invisible “glue” of the universe, continue to be shrouded in mystery. Though galaxies are mostly made of dark matter, understanding how it is distributed within a galaxy offers clues to what this substance is, and how it’s relevant to a galaxy’s evolution. While computer simulations suggest dark matter should pile up in a galaxy’s center, called a density cusp, many previous telescopic observations have indicated that it is instead more evenly dispersed throughout a galaxy. The reason for this tension between model and observation continues to puzzle astronomers, reinforcing the mystery of dark matter. A team of astronomers has turned toward NASA’s Hubble Space Telescope to try and clarify this debate by measuring the dynamic motions of stars within the Draco dwarf galaxy, a system located roughly 250,000 light-years from Earth. Using observations that spanned 18 years, they succeeded in building the most accurate three-dimensional understanding of stars’ movements within the diminutive galaxy. This required scouring nearly two decades of Hubble archival observations of the Draco galaxy. A team of astronomers analyzed observations by NASA’s Hubble Space Telescope taken over a span of 18 years to measure the dynamic motions of stars within the Draco dwarf galaxy. The telescope’s extensive baseline and data archive enabled the team to build the most accurate three-dimensional map of the stars’ movements within the system. These improved measurements are helping to shed “light” on the mysterious qualities and behavior of dark matter, the universe’s invisible “glue.” The left image is from the Digitized Sky Survey (DSS). It presents a wider view of the region. The two right-side images are Hubble views. NASA, ESA, Eduardo Vitral, Roeland van der Marel, and Sangmo Tony Sohn (STScI), DSS; Image processing: Joseph DePasquale (STScI) Download this image “Our models tend to agree more with a cusp-like structure, which aligns with cosmological models,” said Eduardo Vitral of the Space Telescope Science Institute (STScI) in Baltimore and lead author of the study. “While we cannot definitively say all galaxies contain a cusp-like dark matter distribution, it’s exciting to have such well measured data that surpasses anything we’ve had before.” Charting the Movements of Stars To learn about dark matter within a galaxy, scientists can look to its stars and their movements that are dominated by the pull of dark matter. A common approach to measure the speed of objects moving in space is by the Doppler Effect – an observed change of the wavelength of light if a star is approaching or receding from Earth. Although this line-of-sight velocity can provide valuable insight, only so much can be gleaned from this one-dimensional source of information. Besides moving closer or further away from us, stars also move across the sky, measured as their proper motion. By combining line-of-sight velocity with proper motions, the team created an unprecedented analysis of the stars’ 3D movements. “Improvements in data and improvements in modeling usually go hand in hand,” explained Roeland van der Marel of STScI, a co-author of the paper who initiated the study more than 10 years ago. “If you don’t have very sophisticated data or only one-dimensional data, then relatively straightforward models can often fit. The more dimensions and complexity of data you gather, the more complex your models need to be to truly capture all the subtleties of the data.” A Scientific Marathon (Not a Sprint) Since dwarf galaxies are known to have a higher proportion of dark matter content than other types of galaxies, the team honed in on the Draco dwarf galaxy, which is a relatively small and spheroidal nearby satellite of the Milky Way galaxy. “When measuring proper motions, you note the position of a star at one epoch and then many years later measure the position of that same star. You measure the displacement to determine how much it moved,” explained Sangmo Tony Sohn of STScI, another co-author of the paper and the principal investigator of the latest observational program. “For this kind of observation, the longer you wait, the better you can measure the stars shifting.” The team analyzed a series of epochs spanning from 2004 to 2022, an extensive baseline that only Hubble could offer, due to the combination of its sharp stable vision and record time in operation. The telescope’s rich data archive helped decrease the level of uncertainty in the measurement of the stars’ proper motions. The precision is equivalent to measuring an annual shift a little less than the width of a golf ball as seen on the Moon from Earth. With three dimensions of data, the team reduced the amount of assumptions applied in previous studies and considered characteristics specific to the galaxy – such as its rotation, and distribution of its stars and dark matter – in their own modeling efforts. An Exciting Future The methodologies and models developed for the Draco dwarf galaxy can be applied to other galaxies in the future. The team is already analyzing Hubble observations of the Sculptor dwarf galaxy and the Ursa Minor dwarf galaxy. Studying dark matter requires observing different galactic environments, and also entails collaboration across different space telescope missions. For example, NASA’s upcoming Nancy Grace Roman Space Telescope will help reveal new details of dark matter’s properties among different galaxies thanks to its ability to survey large swaths of the sky. “This kind of study is a long-term investment and requires a lot of patience,” reflected Vitral. “We’re able to do this science because of all the planning that was done throughout the years to actually gather these data. The insights we’ve collected are the result of a larger group of researchers that has been working on these things for many years.” These results are accepted for publication in The Astrophysical Journal. 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 (********* Space Agency). NASA’s Goddard Space Flight Center in Greenbelt, Maryland, manages the telescope and mission operations. Lockheed Martin Space, based in Denver, Colorado, also supports mission operations at Goddard. The Space Telescope Science Institute (STScI) in Baltimore, Maryland, which is operated by the Association of Universities for Research in Astronomy, conducts Hubble science operations for NASA. Explore More Hubble Space Telescope Shining a Light on Dark Matter Mystery of Galaxy’s Missing Dark Matter Deepens Hubble Detects Smallest Known Dark Matter Clumps Detailed Dark Matter Map Yields Clues to Galaxy Cluster Growth Hubble Focus E-Book: Dark Universe NASA’s Curious Universe Podcast: Welcome to the Dark Side Dark Matter 101: Looking for the Missing Mass All image products for this article Facebook logo @NASAHubble @NASAHubble Instagram logo @NASAHubble Media Contacts: Claire Andreoli NASA’s Goddard Space Flight Center, Greenbelt, MD *****@*****.tld Abigail Major and Ray Villard Space Telescope Science Institute, Baltimore, MD Science Contacts: Eduardo Vitral, Roeland van der Marel, and Sangmo Tony Sohn Space Telescope Science Institute, Baltimore, MD Share Details Last Updated Jul 11, 2024 Editor Andrea Gianopoulos Location NASA Goddard Space Flight Center Related Terms Astrophysics Astrophysics Division Dark Matter Dark Matter & Dark Energy Goddard Space Flight Center Hubble Space Telescope Missions The Universe Keep Exploring Discover More Topics From NASA Hubble Space Telescope Since its 1990 launch, the Hubble Space Telescope has changed our fundamental understanding of the universe. Shining a Light on Dark Matter Dark Matter & Dark Energy Roman View the full article

1 min read Preparations for Next Moonwalk Simulations Underway (and Underwater) NASA’s Glenn Research Center civil ******** retirees are invited to attend the 2024 Summerfest! Wednesday, Aug. 7, 11 a.m. to 2:30 p.m. Along Taylor Road at Lewis Field For more information or to RSVP, contact Kathy Clark at 216–433–8354 or *****@*****.tld Registration closes: July 26 Credit: NASA Return to Newsletter View the full article

The Office of the General Counsel provides functional leadership regarding legal services and issues related to all aspects of NASA activities for Center Chief and Patent Counsel and, for Agency-wide issues, the Administrator. These services and issues include establishing and disseminating legal policy and interpreting new statutes and cases. The Office of the General Counsel is also responsible for developing the ethics and patent program requirements, establishing metrics, and developing quality standards. As a functional office Associate Administrator, the General Counsel serves in an advisory capacity to the Administrator, and works with Enterprise Associate Administrators and Center Directors to ensure that Agency activities are conducted in accordance with all statutory and regulatory requirements. The Office of the General Counsel also serves as Washington, DC, litigation counsel, provides litigation expertise to the Agency, and acts as the Agency representative before the U.S. Patent and Trademark Office. The Office also provides expert advice, oversight and overflow support to Centers, and provides legal services to all the offices at Headquarters. The Office of the General Counsel at Headquarters is organized into a front office, one legal program and four legal practice groups: Acquisition Integrity Program — The Acquisition Integrity Program (AIP) has primary responsibility for legal issues regarding procurement ****** and other related irregularities, remedies coordination, and suspension and debarment. The Program is responsible for preventing, detecting, and deterring procurement ****** through education and training of the NASA workforce as well as for supporting the investigation and prosecution of ****** and *********** related to the acquisition process. Commercial & Intellectual Property — This Practice Group has primary responsibility for intellectual property issues in domestic and international agreements, technical data issues, patent and copyright licensing, and the distribution of computer software, as well as non-procurement (Space Act) agreements with commercial and international entities. Contracts & Procurement — This Practice Group has primary responsibility for contracts, grants, and cooperative agreements. General Law — This Practice Group has primary responsibility for areas such as ethics, personnel, fiscal, environmental, and safety and security law, as well as legislation and other areas not specifically assigned to one of the other divisions. International and Space Law — This Practice Group has primary responsibility over legal issues regarding export control, Freedom of Information Act appeals, and general matters of international law. General Counsel: Iris Lan Deputy General Counsel: Christine Pham (Acting) Lead, Paralegal Specialist: Carolyn L. Johnson Tel: 202-358-2450 Administrative Specialist: Jeanette Covington Tel: 202-358-2015 OGC Legal Operations Team: Bryan Diederich, (Acting) Director of Legal Operations Tanya Jefferson, Management and Program Analyst Justyna Ragiel-Smith, Management and Program Analyst OGC Leadership Directory — Contact Information for the Headquarters Leadership and Center Chief Counsels OGC Disclaimer: The materials within this website do not constitute legal advice. For details read our disclaimer. View the full article

ESA’s (********* Space Agency) Ariane 6 rocket launches NASA’s CURIE CubeSat from Europe’s Spacesport, the Guiana Space Center in Kourou, French Guiana on Tuesday, July 9, 2024. Photo credit: ESA/S. Corvaja NASA launched CURIE (CubeSat Radio Interferometry Experiment) as a rideshare payload on the inaugural flight of ESA’s (********* Space Agency) Ariane 6 rocket, which launched at 4 p.m. GFT on July 9 from Europe’s Spaceport, the Guiana Space Center in Kourou, in French Guiana. Designed by a team from the University of California, Berkeley, CURIE will use radio interferometry to study the primary drivers of space weather. CubeSats are built using standardized units, with one unit, or 1U, measuring about 10 centimeters in length, width, and height. The two-satellite CURIE mission launched as a 6U before separating into two separate spacecraft, each a 3U. The spacecraft will provide two separate vantage points to measure the same radio waves coming from the Sun and other sources in the sky. NASA’s CubeSat Launch Initiative selected CURIE in 2020 during the initiative’s 11th round of applications. NASA’s Launch Services Program, in collaboration with ESA, designated CURIE as one of eleven payloads supplied by space agencies, commercial companies, and universities for the first flight of ESA’s Ariane 6 rocket. Image Credit: ESA/M. Pédoussaut View the full article

15 Min Read The Marshall Star for July 10, 2024 NASA Moon Rocket Stage for Artemis II Moved, Prepped for Shipment NASA is preparing the SLS (Space Launch System) rocket core stage that will help power the first crewed mission of NASA’s Artemis campaign for shipment. On July 6, NASA and Boeing, the core stage lead contractor, moved the Artemis II rocket stage to another part of the agency’s Michoud Assembly Facility. The move comes as teams prepare to roll the massive rocket stage to the agency’s Pegasus barge for delivery to NASA’s Kennedy Space Center in mid-July. On July 6, NASA and Boeing, the core stage lead contractor, move the Artemis II rocket stage at the agency’s Michoud Assembly Facility. The move comes as teams prepare to roll the massive rocket stage to the agency’s Pegasus barge for delivery to NASA’s Kennedy Space Center in mid-July.NASA/Michael DeMocker Prior to the move, technicians began removing external access stands, or scaffolding, surrounding the rocket stage in early June. NASA and Boeing teams used the scaffolding surrounding the core stage to assess the interior elements, including its complex avionics and propulsion systems. The 212-foot core stage has two huge propellant tanks, avionics and flight computer systems, and four RS-25 engines, which together enable the stage to operate during launch and flight. The stage is fully manufactured and assembled at Michoud. Building, assembling, and transporting is a ****** process for NASA, Boeing, and lead RS-25 engines contractor Aerojet Rocketdyne, an L3Harris Technologies company. Teams at NASA’s Michoud Assembly Facility are preparing the core stage of the agency’s SLS (Space Launch System) for shipment to the agency’s Kennedy Space Center. The 212-foot-tall core stage and its four RS-25 engines will help power Artemis II, the first crewed mission of NASA’s Artemis campaign. In this video, watch as crew remove the external access stands, or scaffolding, before moving the rocket hardware to another area of the facility. (NASA) NASA is working to land the first woman, first person of ******, and its first international partner astronaut on the Moon under Artemis. SLS is part of NASA’s backbone for deep space exploration, along with the Orion spacecraft, supporting ground systems, advanced spacesuits and rovers, the Gateway in orbit around the Moon, and commercial human landing systems. SLS is the only rocket that can send Orion, astronauts, and supplies to the Moon in a single launch. NASA’s Marshall Space Flight Center manages the SLS Program and Michoud. › Back to Top Marshall Researchers Battle Biofilm in Space By Rick Smith A small group of scientists on the biofilm mitigation team at NASA’s Marshall Space Center study solutions to combat fast-growing colonies of bacteria or fungi, known as biofilm, for future space missions. Biofilm occurs when a cluster of bacteria or fungi generates a slimy matrix of “extracellular polymeric substances” to protect itself from adverse environmental factors. Biofilm can be found nearly anywhere, from the gray-green ***** floating on stagnant pond water to the pinkish ring of residue in a ****** bathtub. The biofilm mitigation research team at NASA’s Marshall Space Flight Center assembled its own test stand to undertake a multi-month assessment of a variety of natural and chemical compounds and strategies for eradicating biofilm accretion caused by bacteria and fungi in the wastewater tank assembly on the International Space Station. Testing will help NASA extend the lifecycle of water reclamation and recycling hardware and ensure astronauts can sustain clean, healthy water supplies on long-duration missions in space and on other worlds.NASA/Eric Beitle For medical, food production, and wastewater processing industries, biofilm is often a costly issue. But offworld, biofilm proves to be even more resilient. “Bacteria shrug off many of the challenges humans deal with in space, including microgravity, pressure changes, ultraviolet light, nutrient levels, even radiation,” said Yo-Ann Velez-Justiniano, a Marshall microbiologist and environmental control systems engineer. “Biofilm is icky, sticky – and hard to *****,” said Liezel Koellner, a chemical engineer and NASA Pathways intern from North Carolina State University in Raleigh. Koellner used sophisticated epifluorescence microscopy, 3D visualizations of 2D images captured at different focal planes, to fine-tune the team’s studies. Keenly aware of the potential hurdles biofilm could pose in future Artemis-era spacecraft and lunar habitats, NASA tasked engineers and chemists at Marshall to study mitigation techniques. Marshall built and maintains the International Space Station’s ECLSS (Environment Control and Life Support System) and is developing next-generation air and water reclamation and recycling technologies, including the system’s wastewater tank assembly. “The wastewater tank is ‘upstream’ from most of our built-in water purification methods. Because it’s a wastewater feed tank, bacteria and ******* grow well there, generating enough biofilm to clog flow paths and pipes along the route,” said Eric Beitle, ECLSS test engineer at Marshall. To date, the solution has been to pull and replace old hardware once parts become choked with biofilm. But engineers want to avoid the need for such tactics. “Even with the ability to 3D-print spare parts on the Moon or Mars, it makes sense to find strategies that prevent biofilm buildup in the first place,” said Velez-Justiniano. The team took the first step in June 2023 by publishing the complete genome sequence of several strains of bacteria isolated from the space station’s water reclamation system, all of which cultivate biofilm formation. Yo-Ann Velez-Justiniano, left, and Connor Murphy, right, both Environmental Control and Life Support Systems engineers at Marshall, prepare slides for study of cultured bacterial biofilm in the center’s test facility.NASA/Eric Beitle They next designed a test stand simulating conditions in the wastewater tank about 250 miles overhead, which permits simultaneous study of multiple mitigation options. The rig housed eight Centers for ******** Control and Prevention biofilm reactors – cylindrical devices roughly the size of a runner’s water bottle – each 1/60th the size of the actual tank. Each bioreactor holds up to 21 unique test samples on slides, bathed continuously in a flow of real or ersatz wastewater, timed and measured by the automated system, and closely monitored by the team. Because of the compact bioreactor size, the test stand required 2.1 gallons of ersatz flow per week, continuously trickling 0.1 milliliters per minute into each of the eight bioreactors. “Essentially, we built a collection of tiny systems that all had to permit minute changes to temperature and pressure, maintain a sterile environment, provide autoclave functionality, and run in harmony for weeks at a time with minimal human intervention,” Beitle said. “One phase of the test series ran nonstop for 65 days, and another lasted 77 days. It was a unique challenge from an engineering perspective.” Different surface mitigation strategies, upstream counteragents, antimicrobial coatings, and temperature levels were introduced in each bioreactor. One promising test involved duckweed, a plant already recognized as a natural water purification system and for its ability to capture toxins and control wastewater odor. By devouring nutrients upstream of the bioreactor, the duckweed denied the bacteria what it needs to thrive, reducing biofilm growth by up to 99.9%. Over the course of the three-month testing *******, teams removed samples from each bioreactor at regular intervals and prepared for study under a microscope to make a detailed count of the biofilm colony-forming units on each plate. “Bacteria and fungi are smart,” Velez-Justiniano said. “They adapt. We recognize that it’s going to take a mix of effective biofilm mitigation methods to overcome this challenge.” Biofilm poses as an obstacle to long-duration spaceflight and extended missions on other worlds where replacement parts may be costly or difficult to obtain. The biofilm mitigation team continues to assess and publish findings, alongside academic and industry partners, and will further their research with a full-scale tank experiment at Marshall. They hope to progress to flight tests, experimenting with various mitigation methods in real microgravity conditions in orbit to find solutions to keep surfaces clean, water potable, and future explorers healthy. Smith, an Aeyon/MTS employee, supports the Marshall Office of Communications. › Back to Top Pathways Intern Liezel Koellner Aids NASA Biofilm Mitigation By Rick Smith Liezel Koellner is a NASA Pathways intern pursuing her master’s degree in chemical engineering from North Carolina State University in Raleigh. Like most ambitious young engineers, she sought a variety of different internships to augment her classwork. But once she got word she’d been chosen to spend the spring 2024 term conducting biochemistry experiments at NASA’s Marshall Space Flight Center, her choice was made. NASA Pathways intern Liezel Koellner, right, and her mentor Yo-Ann Velez-Justiniano, a microbiologist at NASA’s Marshall Space Flight Center, prepare compact bioreactors to be installed in the Marshall biofilm mitigation test stand, which is helping researchers study ways to curtail bacterial and fungal biofilm growth in water reclamation systems such as the one on the International Space Station. NASA/Eric Beitle “As a ****, I never imagined I could work at NASA,” she said. “It was a mind-blowing idea!” That’s how she wound up spending the semester up to her safety gloves in bacterial goo – helping NASA’s biofilm mitigation team study strategies for vanquishing a pervasive, slimy invader playing havoc with space-based hardware. And Koellner couldn’t be happier. Biofilm is the sticky goo generated by bacteria or fungi to armor itself against radiation, airlessness, and other conditions in space. Astronauts keep their environment fairly ship-shape – but inside closed water reclamation systems, like the one on the International Space Station, biofilm can thrive, wreaking havoc on critical life support systems. Joining a team of Marshall microbiologists, chemists, and hardware engineers, Koellner spent weeks cultivating sample bacteria – either simulated stuff chemically created onsite or samples shipped frozen from NASA and Boeing archives. She closely monitored ongoing tests, regularly pulling samples to count biofilm colonies. Most importantly, she oversaw the use of precision epifluorescence microscopy, which employs 3D visualizations to identify layered growth in 2D sample images. That contribution most impressed Marshall microbiologist Yo-Ann Velez-Justiniano, Koellner’s supervisor and project mentor, who said it dramatically improved data accuracy. “Liezel was able to more accurately analyze patterns of sample growth and deliver precise quantitative data identifying biofilm progression,” Velez-Justiniano said. A formula for success Koellner said she’s always been driven to soak up as much practical experience as possible. She was born in Guam to ********* parents who later emigrated to San Diego, California, to raise their family. From a young age, she took school very seriously. Velez-Justiniano, left, who heads the biofilm mitigation science team at Marshall, looks on as Koellner, right, shows off her latest sample findings.NASA/Eric Beitle “I always enjoyed chemistry, observing scientific processes and documenting the effects,” Koellner said, but she was daunted by the challenges of calculus-based physics, used to model systems where change occurs and an integral part of scientific fields serving space exploration, engineering, pharmacology, and more. That changed when she got to the University of North Carolina in Wilmington. “Suddenly, everything clicked,” she said. “With physics, it was amazing to see how math could be applied to real-life applications.” That practical blend of disciplines led her to consider a career in chemical engineering – using chemical processes to develop products and resources for commercial uses. After completing her bachelor’s degree in chemistry at the University of North Carolina in 2022 and spending a year as a chemist for a private lab in Wilmington, she enrolled at North Carolina State, where she expects to graduate in 2026 with a master’s in chemical engineering. From water reclamation to air recycling With the biofilm mitigation tests completed – but her internship continuing until August – Koellner has shifted tracks, moving from the challenges of water reclamation to oxygen recovery solutions for future space habitats and on other worlds. She’s part of a different team of Marshall ECLSS (Environment Control and Life Support System) specialists, studying ways to recover oxygen from methane gas. That capability could support a variety of oxygen recovery and recycling systems, saving and storing breathable air instead of just jettisoning it into space along with waste gas products. Koellner will write documentation and help monitor and operate the active test stand, once again working alongside Marshall specialists from various disciplines. She said their commitment has left a lasting impression. “Everyone is so willing to lend their expertise to pursue work that could impact NASA missions years or even decades in the future,” she said. “The diligence and enthusiasm here are tangible things. That’s the kind of engineer – the kind of person – I want to be.” Smith, an Aeyon/MTS employee, supports the Marshall Office of Communications. › Back to Top Lisa Bates Named Director of Marshall’s Engineering Directorate Lisa Bates has been named director of the Engineering Directorate at NASA’s Marshall Space Flight Center, effective July 14. In her new role, Bates will be responsible for the center’s largest organization, comprised of more than 2,500 civil service and contractor personnel, who design, test, evaluate, and operate flight hardware and software associated with Marshall-developed space transportation and spacecraft systems, science instruments, and payloads. Lisa Bates has been named director of the Engineering Directorate at NASA’s Marshall Space Flight Center.NASA Since November 2023, Bates has served as deputy director of the Engineering Directorate. She was also previously director of Marshall’s Test Laboratory. Appointed to the position in 2021, Bates provided executive leadership for all aspects of the Laboratory, including workforce, budget, infrastructure, and operations for testing. She joined Marshall in 2008 as the Ares I Upper Stage Thrust Vector Control lead in the Propulsion Department. Since then, she has served in positions of increasing responsibility and authority. From 2009 to 2017, she served as the first chief of the new TVC Branch, which was responsible for defining operational requirements, performing analysis, and evaluating Launch Vehicle TVC systems and TVC components. As the Space Launch System (SLS) Program Executive from 2017 to 2018, Bates supported the NASA Deputy Associate Administrator for Exploration Systems Development as the liaison and advocate of the SLS. Upon returning to MSFC in 2018, she was selected as deputy manager of the SLS Booster Element Office. Bates also served as deputy manager of the SLS Stages Office from 2018 to 2021 where she shared the responsibilities, accountability, and authorities for all activities associated with the requirements definition, design, development, manufacturing, assembly, green run test, and delivery of the SLS Program’s Stages Element. Prior to her NASA career, Bates worked 18 years in private industry for numerous aerospace and defense contractors, including Jacobs Engineering, Marotta Scientific Controls, ******* Technologies (USBI), ******* Defense, and Sverdrup Technologies. Bates holds a bachelor’s degree in mechanical engineering from the University of Alabama in Huntsville. She was awarded a NASA Outstanding Leadership Medal in 2013 and 2022 and has received numerous group and individual achievement awards. › Back to Top Orion on the Rise Technicians lift NASA’s Orion spacecraft out of the Final Assembly and System Testing cell at NASA’s Kennedy Space Center on June 28. The integrated spacecraft, which will be used for the Artemis II mission to orbit the Moon, has been undergoing final rounds of testing and assembly, including end-to-end performance verification of its subsystems and checking for leaks in its propulsion systems. A 30-ton crane returned Orion into the recently renovated altitude chamber where it underwent electromagnetic testing. The spacecraft now will undergo a series of tests that will subject it to a near-vacuum environment by removing air, thus creating a space where the pressure is extremely low. This results in no atmosphere, similar to the one the spacecraft will experience during future lunar missions. The data recorded during these tests will be used to qualify the spacecraft to safely fly the Artemis II astronauts through the harsh environment of space. (NASA/Radislav Sinyak) › Back to Top NASA to Cover Northrop Grumman’s 20th Cargo Space Station Departure Northrop Grumman’s uncrewed Cygnus spacecraft is scheduled to depart the International Space Station on July 12, five and a half months after delivering more than 8,200 pounds of supplies, scientific investigations, commercial products, hardware, and other cargo to the orbiting laboratory for NASA and its international partners. Northrop Grumman’s Cygnus spacecraft and the International Space Station above western Mongolia.NASA This mission was the company’s 20th commercial resupply mission to the space station for NASA. Live coverage of the spacecraft’s departure will begin at 5:30 a.m. CDT on the NASA+, NASA Television, the NASA app, YouTube, and the agency’s website. Learn how to stream NASA TV through a variety of platforms including social media. Flight controllers on the ground will send commands for the space station’s Canadarm2 robotic arm to detach Cygnus from the Unity module’s Earth-facing port, then maneuver the spacecraft into position for its release at 6 a.m. NASA astronaut Mike Barratt will monitor Cygnus’ systems upon its departure from the space station. Following unberthing, the Kentucky Re-entry Probe Experiment-2 (KREPE-2), stowed inside Cygnus, will take measurements to demonstrate a thermal protection system for the spacecraft and its contents during re-entry in Earth’s atmosphere. Cygnus – filled with trash packed by the station crew – will be commanded to deorbit July 13, setting up a destructive re-entry in which the spacecraft will safely ***** up in Earth’s atmosphere. The Northrop Grumman spacecraft arrived at the space station Feb. 1, following a launch on a SpaceX Falcon 9 rocket from Space Launch Complex 40 at Cape Canaveral Space Force Station. The HOSC (Huntsville Operations Support Center) at NASA’s Marshall Space Flight Center provides engineering and mission operations support for 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 HOSC operates, plans, and coordinates the science experiments onboard the space station 365 days a year, 24 hours a day. Get breaking news, images, and features from the space station on the station blog. › Back to Top Happy Birthday, Meatball! NASA’s Iconic Logo Turns 65 On July 15, NASA’s logo is turning 65. The iconic symbol, known affectionately as “the meatball,” was developed at NASA’s Lewis Research Center (now called NASA Glenn). Employee James Modarelli, who started his career at the center as an artist and technical illustrator, was its chief designer. A painter applies a fresh coat of paint to the NASA “meatball” logo on the north façade of Glenn Research Center’s Flight Research Building, or hangar, in 2006.NASA/Marvin Smith The red, white, and blue design, which includes elements representing NASA’s space and aeronautics missions, became the official logo of the ******* States’ new space agency in 1959. A simplified version of NASA’s formal seal, the symbol has launched on rockets, flown to the Moon and beyond, and even adorns the International Space Station. Workers install the NASA “meatball” logo on the front of the Flight Research Building, or hangar, at Lewis Research Center (now NASA Glenn) in 1962.NASA Along with its importance as a timeless symbol of exploration and discovery, the logo is also one of the world’s most recognized brand symbols. It gained its nickname in 1975 to differentiate it from NASA’s “worm” logotype. The “meatball” and these other NASA designs have made waves in pop culture. “NASA’s brand elements are wildly popular,” said Aimee Crane, merchandising and branding clearance manager for the agency. “Every year, the agency receives requests to merchandise more than 10,000 NASA-inspired items.” › Back to Top View the full article

5 min read Preparations for Next Moonwalk Simulations Underway (and Underwater) An aerial view of Palmyra Atoll, where animal tracking data now being studied by NASA’s Internet of Animals project was collected using wildlife tags by partners at The Nature Conservancy, the U.S. Geological Survey, the National Oceanic and Atmospheric Administration, and several universities.The Nature Conservancy/Kydd Pollock Anchoring the boat in a sandbar, research scientist Morgan Gilmour steps into the shallows and is immediately surrounded by sharks. The warm waters around the tropical island act as a reef shark nursery, and these baby biters are curious about the newcomer. They zoom close and veer away at the last minute, as Gilmour slowly makes her way toward the kaleidoscope of green sprouting from the island ahead. Gilmour, a scientist at NASA’s Ames Research Center in California’s Silicon Valley, conducts marine ecology and conservation studies using data collected by the U.S. Geological Survey (USGS) from animals equipped with wildlife tags. Palmyra Atoll, a ******* States marine protected area, provides the perfect venue for this work. A juvenile blacktip reef shark swims toward researchers in the shallow waters around Palmyra Atoll.The Nature Conservancy/Kydd Pollock A collection of roughly 50 small islands in the tropical heart of the Pacific Ocean, the atoll is bursting with life of all kinds, from the reef sharks and manta rays circling the shoreline to the coconut ****** climbing palm branches and the thousands of seabirds swooping overhead. By analyzing the movements of dolphins, tuna, and other creatures, Gilmour and her collaborators can help assess whether the boundaries of the marine protected area surrounding the atoll actually protect the species they intend to, or if its limits need to shift. Launched in 2020 by The Nature Conservancy and its partners – USGS, NOAA (National Oceanic and Atmospheric Administration), and several universities – the project team deployed wildlife tags at Palmyra in 2022, when Gilmour was a scientist with USGS. Now with NASA, she is leveraging the data for a study under the agency’s Internet of Animals project. By combining information transmitted from wildlife tags with information about the planet collected by satellites – such as NASA’s Aqua, NOAA’s GOES (Geostationary Operational Environmental Satellite) satellites, and the U.S.-********* Jason-3 – scientists can work with partners to draw conclusions that inform ecological management. The Palmyra Atoll is a haven for biodiversity, boasting thriving coral reef systems, shallow waters that act as a shark nursery, and rich vegetation for various land animals and seabirds. In the Landsat image above, a small white square marks the research station, where scientists from all over the world come to study the many species that call the atoll home.NASA/Earth Observatory Team “Internet of Animals is more than just an individual collection of movements or individual studies; it’s a way to understand the Earth at large,” said Ryan Pavlick, then Internet of Animals project scientist at NASA’s Jet Propulsion Laboratory in Southern California, during the project’s kickoff event. The Internet of Animals at Palmyra “Our work at Palmyra was remarkably comprehensive,” said Gilmour. “We tracked the movements of eight species at once, plus their environmental conditions, and we integrated climate projections to understand how their habitat may change. Where studies may typically track two or three types of birds, we added fish and marine mammals, plus air and water column data, for a 3D picture of the marine protected area.” Tagged Yellowfin Tuna, Grey Reef Sharks, and Great Frigatebirds move in and out of a marine protected area (blue square), which surrounds the Palmyra Atoll (blue circle) in the tropical heart of the Pacific. These species are three of many that rely on the atoll and its surrounding reefs for food and for nesting.NASA/Lauren Dauphin Now, the NASA team has put that data into a species distribution model, which combines the wildlife tracking information with environmental data from satellites, including sea surface temperature, chlorophyll concentration, and ocean current speed. The model can help researchers understand how animal populations use their habitats and how that might shift as the climate changes. Preliminary results from Internet of Animals team show that the animals tracked are moving beyond the confines of the Palmyra marine protected area. The model identified suitable habitats both in and around the protected zone – now and under predicted climate change scenarios – other researchers and decisionmakers can utilize that knowledge to inform marine policy and conservation. Research scientist Morgan Gilmour checks on a young great frigatebird in its nest. The marine protected area around Palmyra Atoll protects these birds’ breeding grounds.UC Santa Barbara/Devyn Orr Following a 2023 presidential memorandum, NOAA began studying and gathering input on whether to expand the protected areas around Palmyra and other parts of the Pacific Remote Islands Marine National Monument. Analysis from NASA’s Internet of Animals could inform that and similar decisions, such as whether to create protected “corridors” in the ocean to allow for seasonal migrations of wildlife. The findings and models from the team’s habitat analysis at Palmyra also could help inform conservation at similar latitudes across the planet. Beyond the Sea: Other Internet of Animals Studies Research at Palmyra Atoll is just one example of work by Internet of Animals scientists. Claire Teitelbaum, a researcher with the Bay Area Environmental Research Institute based at NASA Ames, studies avian flu in wild waterfowl, investigating how their movement may contribute to transmission of the virus to poultry and other domestic livestock. Teams at Ames and JPL are also working with USGS to create next-generation wildlife tags and sensors. Low-power radar tags in development at JPL would be lightweight enough to track small birds. Ames researchers plan to develop long-range radio tags capable of maximizing coverage and transmission of data from high-flying birds. This could help researchers take measurements in hard-to-reach layers of the atmosphere. With the technology brought together by the Internet of Animals, even wildlife can take an active role in the study of Earth’s interacting systems, helping human experts learn more about our planet and how best to confront the challenges facing the natural world. To learn more about the Internet of Animals visit: [Hidden Content] The Internet of Animals project is funded by NASA and managed at NASA’s Jet Propulsion Laboratory in Southern California. The team at NASA’s Ames Research Center in California’s Silicon Valley is part of the NASA Earth Exchange, a Big Data initiative providing unique insights into Earth’s systems using the agency’s supercomputers at the center. Partners on the project include the U.S. Geological Survey, The Nature Conservancy, the National Oceanic and Atmospheric Administration, the Yale Center for Biodiversity and Global Change, Stanford University, University of Hawaii, University of California Santa Barbara, San Jose State University, University of Washington, and the Max Planck Institute for Animal Behavior. For Researchers The research collaboration’s dataset from Palmyra is available in open access: Palmyra Bluewater Research Marine Animal Telemetry Dataset, 2022-2023 Related research from Morgan Gilmour’s team was published in the journal Global Ecology and Conservation in June 2022: “Evaluation of MPA designs that protect highly mobile megafauna now and under climate change scenarios.” Media Contacts Members of the news media interested in covering this topic should reach out to the NASA Ames newsroom. About the AuthorMilan LoiaconoScience Communication SpecialistMilan Loiacono is a science communication specialist for the Earth Science Division at NASA Ames Research Center. Share Details Last Updated Jul 10, 2024 Related TermsGeneralAmes Research CenterAmes Research Center's Science DirectorateOceans Explore More 1 min read NASA Technology Soars at Selfridge Air Show Article 1 day ago 1 min read NASA Glenn Welcomes Summer Student Interns Article 1 day ago 7 min read Spectral Energies developed a NASA SBIR/STTR-Funded Tech that Could Change the Way We Fly Article 1 day ago Keep Exploring Discover More Topics From NASA Missions Humans in Space Climate Change Solar System View the full article