NASA

NASA White Sands Test Facility Las Cruces, New Mexico Soil Remediation at the 600 Area Off-Site Pile Origins of the 600 Area Off-Site Pile The NASA White Sands Test Facility (WSTF) is crucial for supporting space exploration and technology development. Located in New Mexico, it provides a controlled environment for testing and evaluating spacecraft, propulsion systems, and other aerospace technologies. The facility is instrumental in conducting critical tests such as engine firings, thermal and environmental testing, and materials research. Its role in ensuring the safety, reliability, and performance of spacecraft and systems makes it a key asset in NASA’s mission to explore space and advance scientific knowledge. Unfortunately, past practices associated with the execution of its mission adversely impacted soil and groundwater resources. From June 1974 to December 1979, sludge and soil removed from a domestic and industrial wastewater lagoon was stockpiled on Bureau of Land Management land west of the NASA White Sands Test Facility (WSTF) facility boundary, less than a mile from the lagoon. When accumulation of material ceased, the sludge/soil debris pile lay dormant with no boundary identification. In 1993, during a Resource Conservation and Recovery Act field investigation the debris pile was identified and reported to the New Mexico Environment Department (NMED) and designated as Solid Waste Management Unit (SWMU) 16. Investigation Summary Initial investigations were completed at SWMU 16 in 2015 and 2018 to characterize the stockpiled sludge/soil and native soils beneath the stockpile to a depth of 30 feet. Analysis of soil sample data indicated the contaminants in the pile posed a risk to human health and the environment due to identified concentrations of nitrates, metals, volatile and semi-volatile organics, pesticides, polychlorinated biphenyls, and dioxins and furans. The NMED agreed to the removal and off-site disposal of New Mexico Special Waste in 2021. Removal, Disposal, Confirmation Sampling Excavation of the stockpile and the upper 6 inches of native soil was completed in January 2024. Excavation of native soils extended approximately 10 ft beyond the extent of the pile. A total of 1,072.7 tons of sludge and soil were disposed at the Corralitos Landfill. In February 2024, confirmatory soil samples were collected from 38 locations on a 30-foot grid established across SWMU 16, encompassing the location of the removed stockpile and all areas potentially affected by site operations. These samples were submitted for laboratory chemical analyses to determine if NASA had met is remedial objectives and eliminated the exposure risk to human health and the environment. Risk Assessment The results showed that NASA had succeeded. The site was restored. Results of soil sample analyses did not identify site contaminants remain at the site, and a risk assessment did not identify elevated risk to receptors or to groundwater beneath the site. NASA concluded that site contaminants have been removed, the risk to human health and the environment are below regulatory targets. NASA recommended a change in site status from “Requiring Corrective Action” to “Corrective Action Complete without Controls”. The report of results is currently under review by the NMED. Visit nasa.gov/emd to learn more about NASA’s Environmental Management Division (EMD)! View the full article

1 Min Read Small Business Innovation Research (SBIR) and Small Business Technology Transfer (STTR) The SBIR/STTR programs provide an opportunity for small, high technology companies and research institutions (RI) to participate in Government sponsored research and development (R&D) efforts in key technology areas. NASA SBIR Phase I contracts have a period of performance for 6 months with a maximum funding of $125,000, and Phase II contracts have a period of performance up to 24 months with a maximum funding of $750,000. The STTR Phase I contracts last for 13 months with a maximum funding of $125,000, and Phase II contracts last for 24 months with the maximum contract value of $750,000. SBIR/STTR Status Search SBIR.NASA.GOV Home Page SBIR/STTR Extension Request Form SBIR/STTR Electronic Handbook SBA – SBIR/STTR Policy Directive View the full article

To put boots on the Moon—and keep them there—will require bold thinkers ready to tackle the challenges of tomorrow. That’s why NASA’s Office of STEM Engagement at Johnson Space Center in Houston is on a mission to empower the next generation of explorers in science, technology, engineering, and mathematics (STEM). Through the High School Aerospace Scholars (HAS) program, Texas juniors have the opportunity to immerse themselves in space exploration through interactive learning experiences. “HAS is such an important program because we introduce students to the multitude of careers and experiences that contribute to space exploration,” said NASA HAS Activity Manager Jakarda Varnado. “We go beyond asking students who they want to be when they grow up and ask what problems they want to solve.” Meet Former HAS Student Madeline King Madeline King always knew she wanted a career in STEM, with a dream of working at NASA influencing her decision to pursue a degree in Engineering. Before joining HAS, King thought scientists mainly worked in labs and engineers focused on design. But the HAS program revealed a different reality—scientists and engineers often collaborated on interdisciplinary projects, sometimes even sharing roles. Official portrait of Madeline King.NASA The program broadened King’s perspective on the diverse paths a STEM degree can lead to. It showed her that careers at NASA offer opportunities across various fields and disciplines. King said participating in HAS helped to strengthen her problem-solving skills and ability to think creatively. The program required students to tackle complex technical tasks independently, emphasizing self-directed learning. King describes HAS as fun, challenging, and engaging, which helped her excel in technical roles. “Learning to digest and internalize this information is a skill I continue to use when getting up to speed in new groups or taking on projects outside my current skill set,” said King. Though King joined HAS during COVID-19, which limited in-person interactions, the experience still made an impact. Her mentors also offered insights into graduate school options, helping her weigh the benefits of advanced degrees against gaining hands-on experience at NASA. The program opened doors to internships at Johnson in the Engineering Robotics and the Avionics Systems Integration Division. Now, she is studying mechanical engineering at the University of Houston, bringing passion and experience in electronics, robotics, education, project management, and aviation. “Early on in my internship journey, HAS shined on my resume,” she said. “It demonstrated that I already had experience with NASA’s culture, values, and mission.” Looking forward, King envisions herself as a flight controller, contributing to both the International Space Station Program and the Artemis campaign. Driven by her passion for NASA’s mission, King is just beginning her journey and is eager to be part of the future of space exploration. “My internships since HAS have allowed me to make small contributions to both of these missions, and I’m excited to specialize as a full-time engineer,” said King. Meet Caroline Vergara As a first-generation student, Caroline Vergara lacked the resources to fully explore her interests in aerospace engineering, let alone envision what that career might look like. That all changed when she was accepted into NASA’s HAS program. “The exposure to real-world innovation ignited my desire to be part of something bigger, something that pushes the boundaries of human knowledge and capability,” she said. Caroline Vergara announces the launch of the model rocket she built during her time in the HAS program. NASA/David DeHoyos Touring NASA facilities and watching engineers work on projects opened her eyes to the possibilities in STEM. Today, Vergara is a propulsion design engineering intern at United Launch Alliance, contributing to the Vulcan rocket as a Brooke Owens Fellow. Vergara initially thought working in STEM was mostly about writing equations or running simulations but HAS showed her it is so much more. “A STEM career is about curiosity, collaboration, and the power to change the world,” she said. During the program, Vergara joined a team of students to tackle a mission simulation project. They called themselves “Charlie and the Rocket Factory” and designed a prototype rocket together. Working with peers from all over the country showed her the power of diverse perspectives. She experienced firsthand what it was like to be part of a team with a shared vision, working toward something bigger than themselves. Vergara also discovered her love for 3D printing and computer-aided design through HAS. She spent hours fine-tuning designs, fascinated by the process of turning digital models into physical reality. Her experience with HAS also sparked a desire to give back. She returned to her hometown to share her story and encourage other students to pursue STEM. Partnering with Johnson Community Engagement Lead Jessica Cordero, she organized video conferences with NASA engineers on International Women in Engineering Day to inspire a new wave of students to be part of space exploration. “The aerospace industry is entering a new space age, and we have the unique opportunity to put humans back on the Moon and explore beyond,” she said. Her advice to the Artemis Generation is: “Go for it! You could be part of the generation that changes humanity’s destiny.” Caroline Vergara, University of Houston Class of 2025. As a mechanical engineering honors student at the University of Houston and chief engineer of Space City Rocketry, Vergara envisions contributing to the Artemis campaign and advancing NASA’s mission to explore the cosmos. “My dream is to contribute to space exploration efforts that put humans back on the Moon and beyond, and to one day work in Mission Control Center, where I can help guide those historic missions into the future.” Meet Iker Aguirre For Iker Aguirre, the spark that ignited his journey toward a career in aerospace was lit by a passing conversation during his freshman year of high school. A senior classmate described the HAS program as a once-in-a-lifetime experience that cemented his passion for aerospace. That moment stayed with Aguirre, and when the opportunity arose, he did not hesitate to apply. Iker Aguirre inside the Vehicle Assembly Building at NASA’s Kennedy Space Center in Florida. “HAS showed me that in order to accomplish something as complex as Artemis, you need a well-rounded set of teams and individuals,” he said. “You don’t need to study aerospace to be in the aerospace industry!” In 2020, Aguirre participated during the remote-only version of HAS, but he recalls that the program still gave him a much deeper understanding of the spaceflight industry. Despite already being interested in aerospace, Aguirre says HAS broadened his horizons, showing him the diverse pathways into the field. Through collaborative projects with peers across Texas, he discovered that solving the challenges of space exploration requires more than just aerospace engineers. The program’s emphasis on teamwork left a lasting impression. During his time with HAS, Aguirre found himself working alongside students from different backgrounds, each bringing unique perspectives to problem-solving. It introduced him to dedicated and passionate people with various personalities and cultures who all shared similar dreams and aspirations as him. Aguirre credits HAS with not only refining his technical skills but also shaping his approach to innovation and teamwork. That experience paid off as he moved through his academic and professional journey, including Pathways program internships with NASA’s Johnson Space Center in Houston and Marshall Space Flight Center in Huntsville, Alabama. “Getting connections at NASA through HAS helped me open many doors so far,” said Aguirre. “I met many good friends through HAS and my internship at Johnson, which I value to this day.” Now pursuing a degree in rocket propulsion, with a focus on turbomachinery design, Aguirre remains committed to advancing space exploration. He hopes to contribute to humanity’s mobility in space, tackling challenges in rocket engine feed systems. Iker Aguirre at NASA’s Johnson Space Center during his HAS internship. Through HAS, Aguirre found not just an educational program, but a community and a purpose. “My journey will forever be interlinked with NASA’s core values of benefiting humanity on and off the Earth,” he said. “I hope to inspire others just as much as the people who inspired me through my journey!” View the full article

3 min read Preparations for Next Moonwalk Simulations Underway (and Underwater) A Boeing 777-300ER aircraft is being inspected by one of Near Earth Autonomy’s drones Feb. 2, 2024, at an Emirates Airlines facility in Dubai, United Arab Emirates.Near Earth Autonomy A small business called Near Earth Autonomy developed a time-saving solution using drones for pre-flight checks of commercial airliners through a NASA Small Business Innovation Research (SBIR) program and a partnership with The Boeing Company. Before commercial airliners are deemed safe to fly before each trip, a pre-flight inspection must be completed. This process can take up to four hours, and can involve workers climbing around the plane to check for any issues, which can sometimes result in safety mishaps as well as diagnosis errors. With NASA and Boeing funding to bolster commercial readiness, Near Earth Autonomy developed a drone-enabled solution, under their business unit Proxim, that can fly around a commercial airliner and gather inspection data in less than 30 minutes. The drone can autonomously fly around an aircraft to complete the inspection by following a computer-programmed task card based on the Federal Aviation Administration’s rules for commercial aircraft inspection. The card shows the flight path the drone’s software needs to take, enabling aircraft workers with a new tool to increase safety and efficiency. “NASA has worked with Near Earth Autonomy on autonomous inspection challenges in multiple domains,” says Danette Allen, NASA senior leader for autonomous systems. “We are excited to see this technology spin out to industry to increase efficiencies, safety, and accuracy of the aircraft inspection process for overall public benefit.” The photos collected from the drone are shared and analyzed remotely, which allows experts in the airline maintenance field to support repair decisions faster from any location. New images can be compared to old images to look for cracks, popped rivets, leaks, and other common issues. The user can ask the system to create alerts if an area needs to be inspected again or fails an inspection. Near Earth Autonomy estimates that using drones for aircraft inspection can save the airline industry an average of $10,000 per hour of lost earnings during unplanned time on the ground. Over the last six years, Near Earth Autonomy completed several rounds of test flights with their drone system on Boeing aircraft used by American Airlines and Emirates Airlines. NASA’s Small Business Innovation Research / Small Business Technology Transfer program, managed by the agency’s Space Technology Mission Directorate, aims to bolster American ingenuity by supporting innovative ideas put forth by small businesses to fulfill NASA and industry needs. These research needs are described in annual SBIR solicitations and target technologies that have significant potential for successful commercialization. Small business concerns with 500 or fewer employees, or small businesses partnering with a non-profit research institution such as a university or a research laboratory can apply to participate in the NASA SBIR/STTR program. Share Details Last Updated Jan 03, 2025 EditorDede DiniusContactTeresa Whitingteresa.whiting@nasa.govLocationArmstrong Flight Research Center Related TermsArmstrong Flight Research CenterAdvanced Air MobilityAmes Research CenterDrones & YouFlight InnovationGlenn Research CenterLangley Research CenterSBIR STTR Explore More 3 min read How a NASA Senior Database Administrator Manifested her Dream Job Article 2 weeks ago 16 min read NASA Ames Astrogram – December 2024 Article 2 weeks ago 5 min read NASA’s Ames Research Center Celebrates 85 Years of Innovation Article 2 weeks ago Keep Exploring Discover More Topics From NASA Armstrong Flight Research Center Aeronautics Drones & You Sky for All View the full article

Credit: NASA NASA Administrator Bill Nelson and Nicky Fox, associate administrator, Science Mission Directorate, will host a media teleconference at 1 p.m. EST, Tuesday, Jan. 7, to provide an update on the status of the agency’s Mars Sample Return Program. The briefing will include NASA’s efforts to complete its goals of returning scientifically selected samples from Mars to Earth while lowering cost, risk, and mission complexity. Audio of the media call will stream live on the agency’s website. Media interested in participating by phone must RSVP no later than two hours prior to the start of the call to: dewayne.a.washington@nasa.gov. A copy of NASA’s media accreditation policy is online. The agency’s Mars Sample Return Program has been a major long-term goal of international planetary exploration for more than two decades. NASA’s Perseverance rover is collecting compelling science samples that will help scientists understand the geological history of Mars, the evolution of its climate, and prepare for future human explorers. The return of the samples also will help NASA’s search for signs of ancient life. For more information about NASA’s Mars exploration, visit: https://nasa.gov/mars -end- Meira Bernstein / Dewayne Washington Headquarters, Washington 202-358-1100 meira.b.bernstein@nasa.gov / dewayne.a.washington@nasa.gov Share Details Last Updated Jan 03, 2025 EditorJessica TaveauLocationNASA Headquarters Related TermsMars Sample Return (MSR)Science Mission Directorate View the full article

This letter from SARA is to issue a waiver for NASA grantees attending the 2025 Lunar and Planetary Science Conference (LPSC), allowing them to be reimbursed out of their grants for their actual lodging, although it’s expected to be above the approved GSA amount. This waiver does not supersede the travel policy of your institution if it is more restrictive. Note: I have specified grants (including cooperative agreements). This may also apply to those traveling on NASA contracts, but they should communicate with their contracting officers. The host hotel for the 56th Lunar and Planetary Science Conference on March 10–14, 2025, is The Woodlands Waterway Marriott Hotel and Convention Center. Hotel information for this conference may be found at https://www.hou.usra.edu/meetings/lpsc2025/plan/. The GSA-allowed daily lodging expense for March 2025 for zip code 77380 (for The Woodlands Waterway Marriott Hotel and Convention Center) is $128 per night. Many of the hotels may be significantly higher than the GSA allowed $128. Grantee travelers may need a waiver to cover lodging in excess of the GSA value, depending on the travel policy of your organization. This waiver does not supersede the travel policy of your institution if it is more restrictive. By the power vested in me by the NSSC to issue approval of the actual lodging costs for a conference in “bulk” instead of individual approvals, I hereby affirm that for the 56th Lunar and Planetary Science Conference NASA, SMD grants may be charged up to $266/night plus taxes and fees, consistent with the average actual cost of the conference hotel, even though this exceeds the $128 allotted for lodging by GSA for The Woodlands for March 2025. Share Details Last Updated Jan 03, 2025 Editor NASA Science Editorial Team Related Terms For Researchers Grants & Opportunities Lunar Science Planetary Science Science Mission Directorate Explore More 5 min read NASA’s LEXI Will Provide X-Ray Vision of Earth’s Magnetosphere Article 3 hours ago 2 min read NASA Workshops Culturally Inclusive Planetary Engagement with Educators Article 23 hours ago 3 min read Astronomy Activation Ambassadors: A New Era Article 3 days ago Keep Exploring Discover More Topics From NASA James Webb Space Telescope Webb is the premier observatory of the next decade, serving thousands of astronomers worldwide. It studies every phase in the… Perseverance Rover This rover and its aerial sidekick were assigned to study the geology of Mars and seek signs of ancient microbial… Parker Solar Probe On a mission to “touch the Sun,” NASA’s Parker Solar Probe became the first spacecraft to fly through the corona… Juno NASA’s Juno spacecraft entered orbit around Jupiter in 2016, the first explorer to peer below the planet’s dense clouds to… View the full article

Earth Observer Earth Home Earth Observer Home Editor’s Corner Feature Articles Meeting Summaries News Science in the News Calendars In Memoriam More Archives 27 min read Summary of the Third Annual AEOIP Workshop Introduction The Applied Earth Observations Innovation Partnership (AEOIP) was established in 2018 to facilitate knowledge coproduction and optimization of NASA Earth observations that can be used by natural resource managers for decision making. Through continued iteration and reflection, coproduction brings together stakeholders to share responsibilities and the completion of activities towards a common goal. AEOIP enables strong collaborations between NASA and the U.S. Forest Service (USFS), along with growing participation from U.S. Geological Survey (USGS), Bureau of Land Management (BLM), and other federal land management agencies. AEOIP has held several previous meetings: the first was a Joint Applications Workshop on Satellite Data for Natural Resource Management held April 29–May 2, 2019, reported in an Earth Observer article, “Summary of the USFS–NASA Joint Applications Workshop on Satellite Data for Natural Resource Management.” The group met again virtually in 2020 during PitchFest. In 2022, a virtual workshop on Integrating Remote Sensing Data for Land Management Decision-Making took place March 23–24, 2022. In 2023, the AEOIP workshop took place April 25–27, 2023, with a hybrid format – the in-person participants met at the USFS Geospatial Technology and Applications Center (GTAC) in Salt Lake City, UT. The 2023 workshop focused on Addressing Land & Water Monitoring Needs Using Remote Sensing Data. These workshops have been designed to build connections between participants across the research-to-applications spectrum with subject matter experts from a variety of federal agencies and other affiliations to continue to promote interagency collaboration within the Earth Observations (EO) applications field. This goal is accomplished using interactive panels and guided discussion sessions that highlight new tools and techniques, promote NASA EO data product uptake, and foster connections between data providers and data users. 2024 Workshop Overview The most recent AEOIP workshop took place April 23–25, 2024, with a hybrid format. The in-person participants met in Ann Arbor, MI. The three-day event had a similar structure to its predecessors but with a wildland fire management theme. Altogether, 135 people participated in the workshop, with 77 attending in person and 58 virtually – see Photo 1. Photo 1. Participants at the 2024 AEOIP workshop. Photo credit: AEOIP Meeting Objectives The workshop objectives were to: meet AEOIP’s mission by providing a forum for building new relationships among Earth observations data providers, users, and stakeholders; gather and/or codevelop “shovel-ready” ideas to better leverage Earth observations to meet science and management priorities of U.S. land and natural resource management agencies; gather needs for and/or develop educational materials to support the use of existing EO training resources for fire management; and gather ideas for the 2025 workshop and other AEOIP activities. Breakout Sessions A large segment of this workshop was dedicated to four concurrent topical breakout sessions – referred to in this report as Breakout Sessions A–D. The topics covered in each breakout session are listed below, along with the name(s) of those who facilitated discussion. Breakout Session A: Fuels, Wildland Fire Emissions, Carbon & Climate – Andy Hudak [USFS] and Edil Sepulveda Carlo [NASA’s Goddard Space Flight Center (GSFC)/Science Systems and Applications Inc. (SSAI)]; Breakout Session B: Prescribed Fire Planning & Management – Nancy French [Michigan Tech Research Institute (MTRI)], Birgit Peterson [USGS], and Jessica Meisel [University of Idaho]; Breakout Session C: Fractional Vegetation Cover Products & Decision Making – Tim Assal and Jake Slyder [both U.S. Department of Interior, BLM], and Liz Hoy and Amanda Armstrong [both at GSFC]; and Alexis O’Callahan [University of Arkansas]. Breakout Session D: Post-fire Effects & Recovery: Assess, Predict, Remediate, and Monitor – Mary Ellen Miller [MTRI]. All of the breakout groups met on each day of the meeting. On the morning of the first day, the facilitators of each group gave brief “elevator pitches” about each breakout topic, and participants selected a topic for focus. After that, a block of time each day was dedicated to breakout activities and discussions. Participants were asked to focus on different aspects of the topic each day. In the afternoon of the first day, each group focused on identifying needs and challenges in the area being discussed – with a brief report-out at the end of the day. On the afternoon of the second day, the focus was on data availability and solutions – i.e., finding ways to overcome obstacles to making data more readily available to users – again with a brief report- out at the end of the day. On the morning of the third day, there were topical presentations. Each group worked to synthesize their three days of discussions and chose a representative to give a summary report during the closing plenary later that morning. Workshop Summary The remainder of this article presents highlights from each day of the workshop. This includes the most important presentations given during the meeting and those given during the breakout sessions. The report also includes highlights from training breakouts given on the second day of the workshop and a summary of a prescribed fire field trip, which took place the day before the workshop and visited two locations – see Optional “Field Trip” for AEOIP Workshop Participants to learn more. Optional “Field Trip” for AEOIP Workshop Participants On April 22, 2024, an optional field trip was offered that featured two sites demonstrating prescribed fire in Michigan. For the first stop on the trip, Kevin Butler [Washtenaw County—Natural Areas Preservation Program Stewardship Supervisor] gave a tour of a prescribed fire site in Park Lyndon, a county park in the northwest part of Washtenaw County, MI. The park is being restored to maintain native species using prescribed fire as invasive species control. The intent of these efforts is to restore oak meadows and preserve over 500 species of plants across fens, marshes, ponds, forest, and prairie lands. On the second leg of the trip, Tina Stephens [City of Ann Arbor—Volunteer and Outreach Coordinator] led a tour of Furstenberg Nature Area, in the city of Ann Arbor, MI. She highlighted the importance of prescribed burning to achieve ecological benefits. The 0.15-km2 (38-acre) park contains wetlands, woodlands, prairie, and oak savanna. Since the mid-1990’s, Natural Area Preservation staff and volunteers have maintained those ecosystems through controlled burns and invasive shrub removal. The second tour stop included a small prescribed fire demonstration – see Photo 2. Photo 2. Ann Arbor park staff conduct a prescribed fire demonstration for workshop participants during the Furstenberg Nature Area tour portion of the AEOIP field trip. Photo credit: Joseph Paki DAY ONE On the first day, Kira Sullivan-Wiley [Pew Institute] gave a plenary presentation, in which she discussed the value of coproduction, which in the context of AEOIP can be described as honoring the generative capacity of others as a means of optimizing the use of Earth by natural resource managers for decision making – see Photo 3. The benefits of this approach include cost reduction, tracking new ideas, and empowering marginalized voices. The first block of breakout sessions also occurred during the afternoon of the first day, along with a short report-out. In light of the keynote discussion on coproduction, deliverables from this meeting’s breakout sessions can be seen as coproduced, new or improved conduits between NASA and land-managing entities. After the keynote, representatives of government agencies (NASA, USFS, and BLM) presented their respective agency’s perspectives. The manager of a nearby state park in Michigan followed with a local perspective. A series of short presentations in the late afternoon featured various program highlights from NASA’s Earth Science Division, which are not detailed in this report – see workshop agenda for list of programs and speakers. Notable Presentations In addition to Kira Sullivan–Wiley’s keynote (described above), Christina Moats-Xavier [NASA Headquarters, Earth Action Program—Program Manager for Mission Engagement] shared NASA’s perspective, focusing on NASA’s Earth Science-to-Action strategy, which aims to increase the impact of scientific data. NASA’s Applied Science Program is now included under the broader umbrella of the new Earth Action program element of NASA’s Earth Science Division. This strategy has three pillars: 1) scaling existing efforts; 2) building bridges; and 3) focusing on the user. By collaborating with NASA, AEOIP can address real-world challenges to develop solutions that benefit society. Overall, the presentations on the first day highlighted the importance of collaborative, user-centered approaches and community engagement in addressing environmental challenges. Everett Hinkley and Frenchy Morisette [both USFS] provided a practitioner’s perspective. They discussed USFS efforts to address climate adaptation, wildfire management, and incorporation of Indigenous traditional ecological knowledge. They also emphasized the application of artificial intelligence/machine learning (AI/ML) for mapping and remote sensing tools. Both Jake Slyder and Tim Assal described their respective government agency’s management of vast (mostly western) land areas and use of remote sensing for post-fire emergency stabilization and integration with the Assessment, Inventory, and Monitoring (AIM) program. Kevin Butler offered more of a local perspective as he discussed land stewardship in Michigan. He emphasized the importance of community involvement and respecting natural ecosystems, especially fire-dependent ones, at the local level. Photo 3. Kira Sullivan-Wiley [Pew Institute] presents on co-production of knowledge during the first day’s plenary session. Photo credit: AEOIP DAY TWO The presentations on the second day of the workshop highlighted the opportunities that Earth observing satellite data presents for natural resource management applications. Five presenters contributed to the panel discussion, titled “Communicating and Soliciting End User Needs: Past, Present and Future.” The second – longer – block of breakout sessions also occurred with a short report-out at the end of the day. A poster session ran concurrently with the report-outs. While this session is not described in this report, it afforded participants an opportunity to showcase their Earth observation related projects and/or interact with their peers. Highlights from the day follow below. Notable Presentations Pontus Olafsson [NASA’s Marshall Space Flight Center] and Natasha Sadoff [NASA HQ—Satellite Needs Program Manager] presented on the Satellite Needs Working Group (SNWG), which provides a coordinated approach to identify and communicate federal satellite Earth observation needs and develop solutions based on Earth observation data. The speakers explained that as part of this effort, SNWG facilitates a biannual survey to all civilian federal agencies. SNWG provides federal agencies a path to coordinate Earth observing needs and a mechanism to develop actionable solutions for decision makers. Solutions cover thematic areas, including air quality, land use/land cover, and water resources. They noted that NASA is also making a greater effort to engage with agency partners in the co-development of new solutions that are useful, accessible, and actionable. Alison York [University of Alaska Fairbanks] spoke about the Joint Fire Science Program (JFSP) and Fire Science Exchange Network (FSEN). JFSP’s main function is to maintain and grow a data repository and community based on fuels, fire behavior, fire ecology, and human dimensions. The goal is to help enable informed, actionable change by policy makers and land managers with the best available scientific support. York then discussed the FSEN, which acts as a mechanism to collate research needs from a collection of regional fire exchanges. The syntheses of data and data needs provides more effective understanding and management of fire. Training Breakout Session Takeaways On the second day, the four breakout sessions met, beginning with four short (25-minute) trainings. The speakers each gave half-hour presentations, which they repeated twice during the hour dedicated to the training breakouts, allowing participants to engage in two of the training breakouts if desired. Pete Robichaud [USFS] discussed training opportunities for modeling post-fire hydrological response using the Water Erosion Prediction Project (WEPP). Soil burn severity is first assessed with remote sensing and then field verified. A subsequent soil burn severity map can be created to give details on physical features, e.g., ash color, ash depth, fine roots, soil structure, water repellency, and ground cover. This resource can be used to create a risk assessment table of probability and consequence parameters. Following the risk assessment, the Forest Service Water WEPP suite of tools can be used to model the landscape. The WEPP suite includes both hillslope and watershed modeling tools. The final step in the Burned Area for Emergency Response (BAER) program is to implement and monitor solutions. Rupesh Shretha [Oak Ridge National Laboratory (ORNL), Distributed Active Archive Center (DAAC)] discussed the Earth Observing System Data and Information System (EOSDIS) DAACs, which are collocated with centers of science discipline expertise and archive and distribute NASA Earth Science data products. The ORNL DAAC archives and distributes terrestrial ecology data, particularly data from field and airborne campaigns. The Terrestrial Ecology Subsetting & Visualization Services (TESViS) – formerly MODIS–VIIRS subsets tool – provide subsets of satellite data in easy-to-use formats that are particularly valuable for site-based field research. The Ecological Spectral Information System (ECOSIS) integrates spectral data with measurements of vegetation functional traits (i.e., species, foliar chemistry). ECOSIS allows users to submit spectral data and return a citable DOIs. ECOSIS also provides users application programming interface (API)-based methods to retrieve thousands of field spectra. Jake Slyder discussed the use of remote sensing for efficient resource management over vast tracts of land with limited human and financial resources. He explained that while the vast collection of remotely sensed data makes it challenging to effectively exploit, Google Earth Engine (GEE) has become an important tool in leveraging remotely sensed information to address BLM management questions. The Change and Disturbance Event Detection Tool (CDEDT), a GEE-based application, allows users to detect and develop vector geospatial products to identify changes and disturbances to surface cover between two dates of observations [10 m (~33 ft) resolution] from the European Space Agency’s (ESA) Copernicus Sentinel-2 mission. Slyder said that the Version 2 (V2) beta product includes the National Agriculture Imagery Program (NAIP) and ESA Copernicus Sentinel-1 SAR Imagery. CDEDT supports a range of BLM monitoring applications, including disaster events, energy development, forest disturbances, and seasonal patterns and processes (e.g., vegetation, water cover). The CDEDT tool is publicly available and does not require any license or special software. DAY THREE The third day was dedicated to the final block of the breakout sessions and a final plenary, where a representative from each breakout group gave five to seven minute summaries of their discussions throughout the meeting. The overview was followed by a meeting wrap-up and adjournment. The sections below summarize the topical presentations given on day three and encapsulate the three days of discussions. Breakout Session A: Focus on Carbon The carbon breakout aimed to inform participants about carbon-related EO initiatives and spark discussion about user needs. Aaron Piña [USFS] spoke about the Forest Service’s broad base of applied research that spans wildfire weather and behavior to dynamics of the smoke produced – see Photo 2. Recent assessments have been made for wildland fire, controlled burn smoke, and remote air monitors. Piña spoke about Bluesky Playground, a community-driven tool aimed at providing the public with information on fuels and smoke modeling. These data have been used to identify important indicators for fires and fuels (e.g., vertical plume structure). Piña then discussed a fusion Fire Radiative Power (FRP) data product [MOD19A2] that combines data from four sources – the Visible and Infrared Scanner (VIRS) on the former Tropical Rainfall Measuring Mission (TRMM), the Visible Infrared Imaging Radiometer Suite (VIIRS) on the Suomi National Polar-orbiting Partnership (Suomi NPP), the Moderate Resolution Imaging Spectroradiometer (MODIS) on the Terra and Aqua platforms, and the Multi-Angle Implementation of Atmospheric Correction (MAIAC) aerosol product. A group discussion followed Piña’s presentation, during which several participants expressed concerns about the continuity of VIIRS and the other observations that are used in the fusion FRP product. Another topic of discussion was the potential of remotely sensed data to improve the characterization of duff (decaying vegetation) in satellite data products. NASA’s Tropospheric Emissions: Monitoring of Pollution (TEMPO) mission data have also been used to characterize the vertical structure of smoke plumes; however, these efforts have thus far been limited by personnel knowledge gaps as well as raw data formats. Chris Woodall [USFS] discussed the growing emphasis on carbon metrics for a variety of sectors and applications. The USFS wants to work in tandem with other entities, especially federal organizations, to maximize efforts and workstream. USFS is seen as the in-situ carbon observer, while NASA is the remote sensor, and USGS is the lateral flux assessor. The coproduction of knowledge and data regarding carbon among these agencies is an iterative process. The USFS investment in improved Measurement, Monitoring, Reporting, and Verification (MMRV) of greenhouse gas (GHG), for example, can expand soil and land-use inventories to improve alignment with remote-sensing platforms. Challenges to implementing this cooperative approach to collecting carbon metrics include creating a workflow that incorporates a wealth of existing resources and accruing data from multiple federal agencies concerned with ecosystem carbon management to create scalable GHG knowledge. The coproduction, iteration, and dissemination of knowledge should be a major focus with all interested parties – not just the aforementioned federal agencies. Sydney Neugebauer [NASA’s Langley Research Center] and Melanie Follette-Cook [GSFC] discussed NASA’s capacity building initiatives, which are aimed at developing and strengthening an organization or community’s skills, abilities, processes, and resources to enable them to survive, adapt, and thrive in a fast changing world. The DEVELOP, Indigenous Peoples Initiative, and SERVIR programs (all under the Earth Action program element) work towards capacity building through co-development projects, collaborative training, and data availability. The NASA Applied Remote Sensing Training (ARSET) program has offered over 100,000 training sessions since it was created in 2009 – primarily to international participants. The trainings are free and virtual for individuals interested in using remotely sensed data in a diverse suite of environmental applications. All content is archived. NASA’s Carnegie-Ames-Stanford Approach (CASA), which has contributed to global carbon dioxide (CO2) sequestration datasets for the past 30-years, will be upgraded to incorporate CO2 fluxes. The NASA cooperative interagency U.S. Greenhouse Gas Center is also looking for feedback on its beta portal. The group discussions that followed identified and addressed AEOIP needs and questions (e.g., obtaining carbon and smoke emission estimates from prescribed wildfires and ensuring global satellite fire record continuity). Participants also identified the need for near real-time active fire and burned area mapping at medium scale and for continuity of these measurements. The group is interested in engaging federal agency end users to obtain feedback on their capacity to facilitate and elucidate capacity needs. Prominent challenges going forward include preparing for the end of the Terra and Aqua missions, which will include the decommissioning of MODIS, and ensuring the continuity of VIIRS, which is being used to allow for continuity of MODIS data products. One of the greatest unknowns identified was being able to determine wildfire fuel conditions in near-real time, and the ability to constrain estimates of fuel attributes to a focused fire event. Andy Hudak discussed the diverse coalition of practitioners who manage more than just carbon (e.g., forest health, harvest, fires). Of the diverse group of stakeholders, Indigenous Tribes are at the cutting edge using lidar for carbon assessment. While Forest Inventory and Analysis plots are used for bias correction, they do not provide synoptic coverage for accurate carbon assessments. Lidar and other passive remote sensing satellite data provide a way to address this need. Tree lists are also highly valuable to carbon and forest managers for diverse applications. Application-specific metrics (e.g., timber volume, basal area, and density) can be weighted based on stakeholder priorities, as quantified from stakeholder surveys, to optimize data products. Sarah Lewis [USFS] explained the needs and applications of Earth observations in a post-fire environment. The information needs to be available quickly, integrated into effective decision-making tools, and delivered in a functional product. Information is needed on water, soils, vegetation recovery, and habitat – all major metrics of interest in a data product. Areas of concern during post-fire management for water quality and erosion control include ash and soil–water transport. In addition, major concerns exist for timely data acquisition and processing, along with the fate and transport mapping of post-fire ash. Data products would benefit from end-user input to optimize relevance and accessibility of decision ready maps, models, and trusted recommendations. The group identified the need for heavy carbon fuels and duff estimates for ecological modeling, which is critical to achieving a better understanding of smoke and carbon emissions. The heavy carbon fuel and duff estimates may be achieved through multiple means but may be most accessible currently through a new layer in the LANDFIRE database. They also identified the need for more post-fire data for model training and integration of active remote sensing data. Finally, the group identified the need for more regulation and research on prescribed fire emissions and disturbance. Breakout Session B: Prescribed Fire This breakout session focused on prescribed fires. Some of the major objectives and needs that emerged from this session were improved access to data, cultivating deeper public trust in the practice, creating networks of future coproduction, and assessing end-user needs, burn maps, and securing funding. The discussions emphasized knowledge and awareness gaps as a major impediment to prescribed fire implementation. Uniform capacity building is an ideal approach to engage stakeholders at a reference level appropriate to their background to optimize equity and efficacy. Another issue that came up during discussion is that land management professionals do not have the time or resources to stay current with data sources and analysis techniques. The participants suggested the creation of a “Fire Science Library” as an iterative data tool to organize and present fire knowledge in an actionable and streamlined manner for public land managers. The interface would allow practitioners to filter unique categories (e.g., role, scope, region, ecosystem type, weather, agency affiliation) to provide the ability to search, modify, and maintain fire science knowledge as it evolves. This interface would also provide provenance through references to papers, justification for methods, and case studies. The library would guide and streamline data collection, analyses, and interpretation workflows that are needed for holistic prescribed fire planning and monitoring based on tangible needs from fire professionals. The virtual library tool would provide a user with a fire-science knowledge graph, which is an organized representation of real-world entities and their relationships that could quickly connect fire-related management with current research questions concerning data products, processing methods, and data sources along with references and case studies. Information provided in the knowledge graph would need to be context specific but not overly prescriptive to avoid constraining users to a rigid workflow that is more common in basic data portals. Knowledge graphs are associated with semantic web technology that forms a modern version of a database. The tool establishes relationships between entities that promote new relationship discovery, search, and modification. It also provides a foundation on which other applications can be built, such as prescribed fires in the southeast and incorporating drone data. Focusing on prescribed fire may help to bound the initial product development but leave the door open for eventual expansion for wildfire. The group identified objectives moving forward, including the need to finalize the main set of prescribed fire management questions (e.g., planning, implementation, pre/post monitoring), establish user personas based on known representatives and gaps, engage the Earth Science Information Partners (ESIP), identify cluster members (e.g., subject matter experts from local and federal agencies, private industry, and academia/research), and investigate additional funding sources. (Clusters are agile working groups within ESIP formed to focus on specific topics.) Breakout Session C: Fractional Vegetation Cover This breakout session focused on fractional vegetation cover (FVC) – see Photo 4. The presenters introduced three large FVC assessment efforts, and the participants contributed to a Strengths, Weakness, Opportunities, and Threats (SWOT) analysis of FVC products intended to improve the use of this data by decision makers – see Table. Photo 4. [left to right] Amanda Armstrong, Elizabeth Hoy [both at Goddard Space Flight Center], and Timothy Assal [Bureau of Land Management] collaborating during the Fractional Vegetation Cover Breakout. Photo credit: AEOIP Tim Assal discussed the BLM’s Assessment Inventory and Monitoring (AIM) strategy. He explained that AIM has nearly 60,000 monitoring locations across the terrestrial uplands, aquatic systems, and riparian and wetland habitat of the U.S., and the data collected are being used for monitoring and restoration activities. Assai added that integration of remote sensing data with field plot data enables the generation of continuous datasets (e.g., FVC that can relate field plot-level indicators to those based on remote-sensing). He also reported that FVC data are currently being used to address numerous management decisions. Sarah McCord [USDA] discussed V3 of the Rangeland Analysis Platform (RAP). McCord explained that V3 uses vegetation cover and rangeland production data to monitor these parameters. The model also uses species composition data. She explained that there are approximately 85,000 training/validation locations across the U.S. that have been incorporated into the modeling process. She said that enhancements to future versions of RAP are expected as data from new satellite instruments, field plots, and deep learning (i.e., application of AI/ML techniques) are all incorporated into the model. McCord chairs a working group that is actively investigating sources of error and uncertainty within individual and across different FVC products. Matt Rigge [USGS Earth Resources Observation and Science (EROS) Center] discussed V3 of the Rangeland Condition Monitoring Assessment and Projection (RCMAP), which will provide current and future condition using Landsat time series. Data available includes cover maps and potential cover. The platform uses various training data in addition to AIM plot data. In the future RCMAP plans to incorporate data from synthetic NASA-Indian Space Research Organization Synthetic Aperture Radar (NISAR), from NASA’s Earth Surface Mineral Dust Source (EMIT) mission, and from convolution neural network-based (CNN) algorithms. Bo Zhou [University of California, Los Angeles (UCLA)] discussed V2 of the Landscape Cover Analysis and Reporting Tool (LandCART). V3 will be different and coming in the future. He explained that the BLM uses V3 to make legally defensible decisions. He then discussed the training data, which come mostly from AIM. The training dataset includes 71 Level-4 (L4) Ecoregions, as defined by the U.S. Environmental Protection Agency, with at least 100 observations. Zhou noted that these training data are used to define spatial extent, the temporal extent is defined by available satellite imagery, and uncertainty estimates are based on CNN and random forest (RF) machine-learning algorithms. Eric Jensen [Desert Research Institute] discussed how ClimateEngine.org uses cloud-based tools, such as GEE, to access, visualize, and share Earth observation datasets to overcome computational limitations of big data in a real-time environment. It encompasses over 85 datasets, including RAP and RCMAP, and the group is working to add LandCART. Two core functionalities of the ClimateEngine app are producing maps and making graphs. Jensen provided a brief demonstration of the app using a juniper removal project in sage grouse habitat in southern Idaho. Strengths • Tools available for accessing and processing data are user-friendly and widely accessible, making it easy to compile, use, and display data for users of all expertise levels across a range of management activities. • Tools provide a comprehensive view of an area, offering both current and retrospective insights that are highly regarded by the restoration community. • Tool format supports integration of new datasets, ensuring inclusivity and consistency over time and space. Weaknesses • Training data exhibits spatial and temporal biases. • Training data is biased towards federal data, lacking global representation. • Sensors have limitations for both temporal and spatial accuracy. Opportunities • Managers can use these tools to make informed decisions and evaluate the effectiveness of their treatments. • Additional training (e.g., training in how to process new data types, such as hyperspectral data) could institutionalize remote sensing and reach more end users. • Future expansion of AI/ML techniques and cloud-based services could reduce error, enhance data quality, and increase user reach. Threats • Stability of funding could threaten continuity of measurements. • Falling into a “one size fits all” mentality could stifle innovation. • Variation in land management organizations’ willingness to update data and lack of cohesion could prevent obtaining full potential of FVC. • Transition from research to operations could hinder collaboration and tool development and weaken the community of practice. • Poor performance, misuse of information, and data sovereignty could diminish the community’s trust in the tools. • Rapid technological advancements could displace smaller businesses. Table. Results of a Strengths, Weaknesses, Opportunities, and Threats (SWOT) analysis of the current state of Fractional Vegetation Cover (FVC) data analysis tools and techniques. Breakout Session D: Post-fire Effects and Recovery This session focused on assessing, predicting, remediating, and monitoring areas in the aftermath of fires. The focus was on “shovel-ready” ideas, such as improving operational soil burn severity maps to connect post-fire ground conditions and soil properties. The participants highlighted the need to leverage information (e.g., active fire thermal data) to better detect changes in post-fire cover and soil properties. Such information would be beneficial to USFS’s Burned Area for Emergency Response (BAER) program as well as to researchers, data providers, decision makers, and community leaders. The group discussed steps that would aid in this collaboration (e.g., incorporating thermal imagery into mapping soil burn severity, developing and validating products, getting first-look data to field teams, monitoring threats by conducting rapid burn severity assessment before official soil burn severity maps are made available, and sharing outputs quickly with decision makers). The breakout participants also noted the challenge of ash load mapping, which they suggested might be constrained by using information on pre-fire fuels (e.g., biomass, understory, and canopy vegetation) to constrain potential ash production. Derived information products [e.g., Normalized Difference Vegetation Index (NDVI), Leaf Area Index (LAI), LANDFIRE fuels layers, and RAP] may improve this process. The group noted the limitations of the VIIRS instrument for mapping fire duration and soil heating. The group proposed adding supplemental data through the use of National Infrared Operations (NIROPS) raw infrared imagery – see Figure 1. Fire tools currently available – and under consideration for improving maps – include VIIRS active fire data through NASA’s Fire Information for Resource Management System (FIRMS), fire event tracking through NASA’s Earth Information System Fire Event Data Suite (FEDS), the burn severity prediction model at MTRI, and Rapid Differenced Normalized Burn Ratio Mapping at the University of Wisconsin, Madison. The group identified VIIRS L1 image capture to detect smoldering fires as a potential improvement in wildfire characterization. The group also suggested more frequent observations of moderate resolution satellites, GOES Integration [0.5–2 km (0.3–1.2 mi) spatial resolution], and comprehensive field data. They identified possible ways to improve post-fire soil burn severity maps (e.g., information on pre-fire fuels, soil characteristics, and thermal properties, such as fire heating, residence time, spread rate), optical characteristic (e.g., vegetation mortality, ash production), and lidar canopy metrics. Presently, burn severity is assessed using a simple spectral index derived from remote sensing data, driven by necessity, data access, and computing power. The group presented the need to break this single number into ecologically meaningful components for better post-fire assessment and remediation. Improvements could involve incorporating additional information (e.g., peak soil temperature, heat residence time, and fuel moisture). Coupling atmospheric fire behavior models could address temporal gaps, necessitating high-spatial and temporal resolution thermal data sets. The participants agreed that future strategies should include monitoring warmer areas and smoldering zones instead of just flaming fronts, as well as exploring temperature differences across burn severities. Additionally, post-fire assessments would benefit from using other spectral bands and post-fire Ecosystem Spaceborne Thermal Radiometer Experiment on Space Station (ECOSTRESS) products. They also added that access to more field information is crucial for scientific post-fire observations. Efforts are underway to make the SBS S123 survey system a national standard, though surveys currently reside with local units that have good record-keeping practices. Figure 1. Optical [left and right] and thermal [right, overlay] images of participants at the 2024 AEOIP workshop obtained by an unpiloted aerial vehicle (UAV). Image credit: Colin Brooks Conclusion The 2024 AEOIP workshop addressed a wide range of geospatial data tool and training needs and forums. The meeting centered on coproduction of knowledge and community-of-practice building as key needs for the geospatial data topics. Participants identified capacity building – through awareness, accessibility, and utility of data and tools – as the top priority for processing and technological advancement initiatives. The breakout session topics selected (e.g., carbon concentrations, wildfires, prescribed fires, and landscape dynamics) were chosen to promote dialogue between data users and scientists, leading to plans for action and change in data and tool utility in four areas of interest for land managers. Following the meeting, the organizers submitted a spreadsheet detailing the data and tool needs identified during the breakouts to the Earth Action Program. The SNWG has also been made aware of the most compelling needs that participants identified. The AEOIP believes that by bridging two groups – data users and research and development – it will be possible to bolster user provenance and efficacy of NASA resources moving forward. Severin Scott Washington State University severin.scott@wsu.edu Alan B. Ward NASA’s Goddard Space Flight Center (GSFC)/Global Science and Technology (GST) alan.b.ward@nasa.gov Alexis O’Callahan University of Arkansas aocallah@uark.edu Share Details Last Updated Jan 03, 2025 Related Terms Earth Science View the full article

NASA/Kim Shiflett From left, CSA (Canadian Space Agency) astronaut Jenni Gibbons, NASA astronaut Andre Douglas, CSA astronaut Jeremy Hansen, and NASA astronauts Christina Koch, Victor Glover, and Reid Wiseman participate in a media day event on Monday, Dec. 16, 2024, inside the Vehicle Assembly Building at the agency’s Kennedy Space Center in Florida. Gibbons and Douglas are Artemis II backup crew members. The Artemis II test flight will be NASA’s first mission with crew under the Artemis campaign, sending astronauts on a 10-day journey around the Moon and back. Image Credit: NASA/Kim Shiflett View the full article

NASA astronaut and Expedition 72 Flight Engineer Don Pettit points a camera outside a window on the International Space Station’s Poisk module for a sun photography session. (Credit: NASA) Students from Hawthorne Elementary School in Boise, Idaho, will have the chance to hear NASA astronaut Don Pettit answer their prerecorded science, technology, engineering, and math (STEM) related questions from aboard the International Space Station. Watch the 20-minute space-to-Earth call at 12:30 p.m. EST Friday, Jan. 10, on NASA+ and learn how to watch NASA content on various platforms, including social media. Media interested in covering the event must RSVP by 5 p.m., Tuesday, Jan. 7, to Dan Hollar at dan.hollar@boiseschools.org or 208-854-4064. For more than 24 years, astronauts have continuously lived and worked aboard the space station, testing technologies, performing science, and developing skills needed to explore farther from Earth. Astronauts aboard the orbiting laboratory communicate with NASA’s Mission Control Center in Houston 24 hours a day through SCaN’s (Space Communications and Navigation) Near Space Network. Important research and technology investigations taking place aboard the space station benefit people on Earth and lays the groundwork for other agency missions. As part of NASA’s Artemis campaign, the agency will send astronauts to the Moon to prepare for future human exploration of Mars; inspiring Artemis Generation explorers and ensuring the United States continues to lead in space exploration and discovery. See videos and lesson plans highlighting space station research at: https://www.nasa.gov/stemonstation -end- Abbey Donaldson Headquarters, Washington 202-358-1600 Abbey.a.donaldson@nasa.gov Sandra Jones Johnson Space Center, Houston 281-483-5111 sandra.p.jones@nasa.gov View the full article

5 min read NASA’s LEXI Will Provide X-Ray Vision of Earth’s Magnetosphere A NASA X-ray imager is heading to the Moon as part of NASA’s Artemis campaign, where it will capture the first global images of the magnetic field that shields Earth from solar radiation. The Lunar Environment Heliospheric X-ray Imager, or LEXI, instrument is one of 10 payloads aboard the next lunar delivery through NASA’s CLPS (Commercial Lunar Payload Services) initiative, set to launch from the agency’s Kennedy Space Center in Florida no earlier than mid-January, with Firefly Aerospace’s Blue Ghost Lander. The instrument will support NASA’s goal to understand how our home planet responds to space weather, the conditions in space driven by the Sun. NASA’s next mission to the Moon will carry an instrument called LEXI (the Lunar Environment Heliospheric X-ray Imager), which will provide the first-ever global view of the magnetic environment that shields Earth from solar radiation. This video can be freely shared and downloaded at https://svs.gsfc.nasa.gov/14739. Credits: NASA’s Goddard Space Flight Center Once the dust clears from its lunar landing, LEXI will power on, warm up, and direct its focus back toward Earth. For six days, it will collect images of the X-rays emanating from the edges of our planet’s vast magnetosphere. This comprehensive view could illustrate how this protective boundary responds to space weather and other cosmic forces, as well as how it can open to allow streams of charged solar particles in, creating aurora and potentially damaging infrastructure. “We’re trying to get this big picture of Earth’s space environment,” said Brian Walsh, a space physicist at Boston University and LEXI’s principal investigator. “A lot of physics can be esoteric or difficult to follow without years of specific training, but this will be science that you can see.” What LEXI will see is the low-energy X-rays that form when a stream of particles from the Sun, called the solar wind, slams into Earth’s magnetic field. This happens at the edge of the magnetosphere, called the magnetopause. Researchers have recently been able to detect these X-rays in a patchwork of observations from other satellites and instruments. From the vantage point of the Moon, however, the whole magnetopause will be in LEXI’s field of view. In this visualization, the LEXI instrument is shown onboard Firefly Aerospace’s Blue Ghost Mission 1, which will deliver 10 Commercial Lunar Payload Services (CLPS) payloads to the Moon. Firefly Aerospace The team back on Earth will be working around the clock to track how the magnetosphere expands, contracts, and changes shape in response to the strength of the solar wind. “We expect to see the magnetosphere breathing out and breathing in, for the first time,” said Hyunju Connor, an astrophysicist at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, and the NASA lead for LEXI. “When the solar wind is very strong, the magnetosphere will shrink and push backward toward Earth, and then expand when the solar wind weakens.” The LEXI instrument will also be poised to capture magnetic reconnection, which is when the magnetosphere’s field lines merge with those in the solar wind and release energetic particles that rain down on Earth’s poles. This could help researchers answer lingering questions about these events, including whether they happen at multiple sites simultaneously, whether they occur steadily or in bursts, and more. These solar particles streaming into Earth’s atmosphere can cause brilliant auroras, but they can also damage satellites orbiting the planet or interfere with power grids on the ground. “We want to understand how nature behaves,” Connor said, “and by understanding this we can help protect our infrastructure in space.” The LEXI team packs the instrument at Boston University. Michael Spencer/Boston University The CLPS delivery won’t be LEXI’s first trip to space. A team at Goddard, including Walsh, built the instrument (then called STORM) to test technology to detect low-energy X-rays over a wide field of view. In 2012, STORM launched into space on a sounding rocket, collected X-ray images, and then fell back to Earth. It ended up in a display case at Goddard, where it sat for a decade. When NASA put out a call for CLPS projects that could be done quickly and with a limited budget, Walsh thought of the instrument and the potential for what it could see from the lunar surface. “We’d break the glass — not literally — but remove it, restore it, and refurbish it, and that would allow us to look back and get this global picture that we’ve never had before,” he said. Some old optics and other components were replaced, but the instrument was overall in good shape and is now ready to fly again. “There’s a lot of really rich science we can get from this.” Under the CLPS model, NASA is investing in commercial delivery services to the Moon to enable industry growth and support long-term lunar exploration. As a primary customer for CLPS deliveries, NASA aims to be one of many customers on future flights. NASA Goddard is a lead science collaborator on LEXI. NASA’s Marshall Space Flight Center in Huntsville, Alabama, manages the development of seven of the 10 CLPS payloads carried on Firefly’s Blue Ghost lunar lander, including LEXI. Learn more about CLPS and Artemis at: https://www.nasa.gov/clps By Kate Ramsayer NASA’s Goddard Space Flight Center, Greenbelt, Md. Share Details Last Updated Jan 03, 2025 Editor Abbey Interrante Related Terms Artemis Commercial Lunar Payload Services (CLPS) Earth’s Magnetic Field Earth’s Moon Goddard Space Flight Center Heliophysics Heliophysics Division Magnetosphere Science & Research The Sun Explore More 2 min read NASA Workshops Culturally Inclusive Planetary Engagement with Educators Article 20 hours ago 3 min read Astronomy Activation Ambassadors: A New Era Article 3 days ago 5 min read NASA’s Parker Solar Probe Makes History With Closest Pass to Sun Article 7 days ago Keep Exploring Discover Related Topics Missions Humans in Space Climate Change Solar System View the full article

This map depicts global temperature anomalies for meteorological summer in 2024 (June, July, and August). It shows how much warmer or cooler different regions of Earth were compared to the baseline average from 1951 to 1980. (Credit: NASA/NOAA) Climate researchers from NASA and NOAA (National Oceanic and Atmospheric Administration) will release their annual assessments of global temperatures and discuss the major climate trends of 2024 during a media briefing at 12 p.m. EST Friday, Jan. 10. NASA will share the briefing on the agency’s website at: https://www.nasa.gov/live. Participants will include: Gavin Schmidt, director, NASA’s Goddard Institute for Space Studies Russ Vose, chief, Monitoring and Assessment Branch, NOAA National Centers for Environmental Information Media interested in participating must RSVP to NOAA by the time of the event. NASA and NOAA are stewards of global temperature data and independently produce a record of Earth’s surface temperatures and changes based on historical observations over land and ocean. For more information about NASA’s Earth science programs, visit: https://www.nasa.gov/earth -end- Liz Vlock Headquarters, Washington 202-358-1600 elizabeth.a.vlock@nasa.gov Peter Jacobs Goddard Space Flight Center, Greenbelt, Maryland 301-286-0535 peter.jacobs@nasa.gov View the full article

4 Min Read Lagniappe for January 2025 Explore the January 2025 issue, highlighting the year in review at NASA Stennis, and how to become a NASA test conductor at the official visitor center and more! Explore Lagniappe for January 2025 featuring: NASA Stennis Celebrates Key Testing, Operations Milestones in 2024 NASA Exhibit Puts Visitors in Test Conductor Seat NASA Stennis Hosts Mississippi Kween Gator Speaks Gator SpeaksNASA/Stennis This time of year is one Gator enjoys. The ending of one year and beginning of another provides the opportunity to reflect, reset, and refocus. This is true at NASA Stennis, a place that powers space dreams, or for someone who enjoys staying up to date with all the happenings around NASA Stennis – you! In 2024, Gator witnessed the legacy of excellence continue at the south Mississippi NASA center. There were milestones reached with RS-25 engine testing and preparations for testing NASA’s new exploration upper stage for future Artemis missions, the center continued to fuel the space market with its support of commercial companies at the E Test Complex, and it was announced the historic in-space payload mission for the NASA Stennis Autonomous Systems Laboratory team would continue. Another bright spot at NASA Stennis is range operations. The partnership between NASA Stennis and Skydweller Aero represents the first big step in this area. In 2024, NASA Stennis entered into an agreement with Skydweller Aero for the company to operate its solar-powered autonomous aircraft in the site’s restricted airspace. It marks the first agreement between NASA Stennis and a commercial company to use the center’s unique capabilities to support testing and operation of uncrewed systems. The future is indeed bright. The new year is like the NASA Stennis buffer zone. The 125,000-plus acre buffer zone enables many opportunities for site achievement and advancement, much like a new year does. We all can make 2025 the best year to date by building on what we have accomplished and setting bold, new goals. Here is to 2025 – a year of focus, ambition, and collaboration. Together, we can turn our goals into achievements and make this year one of our best yet. Happy New Year! > Back to Top NASA Stennis Top News NASA Stennis Celebrates Key Testing, Operations Milestones in 2024 NASA’s Stennis Space Center near Bay St. Louis, Mississippi, celebrated propulsion testing and site operations milestones in 2024, all while inspiring the Artemis Generation and welcoming new leadership that will help NASA Stennis innovate and grow into the future. Read more about key milestones from 2024 NASA Exhibit Puts Visitors in Test Conductor Seat NASA’s Stennis Space Center near Bay St. Louis, Mississippi, is helping the Artemis Generation learn how to power space dreams with an interactive exhibit at INFINITY Science Center. Read more about the engine test simulator exhibit > Back to Top Center Activities NASA Stennis Hosts Mississippi Kween Cookbook author and culinary content creator Caroline Davis, popularly known as Mississippi Kween, and her family enjoy touring facilities and learning about NASA Stennis and its frontline work during a site visit Dec. 18. Davis, husband Joe, and children Zeke and Zoey, met with NASA Stennis leadership before touring the L3Harris (formerly Aerojet Rocketdyne) Engine Assembly Facility, Thad Cochran Test Stand, Autonomous Systems Laboratory, and the NASA Stennis rocket engine garden. The tour highlighted the NASA Stennis story and how the south Mississippi NASA center has the ingredients for a recipe that accelerates the exploration and commercialization of space, innovates to benefit NASA and industry, and leverages assets to stimulate the economy.NASA/Danny Nowlin Cookbook author and culinary content creator Caroline Davis, popularly known as Mississippi Kween, and her family enjoy touring facilities and learning about NASA Stennis and its frontline work during a site visit Dec. 18. Davis, husband Joe, and children Zeke and Zoey, met with NASA Stennis leadership before touring the L3Harris (formerly Aerojet Rocketdyne) Engine Assembly Facility, Thad Cochran Test Stand, Autonomous Systems Laboratory, and the NASA Stennis rocket engine garden. The tour highlighted the NASA Stennis story and how the south Mississippi NASA center has the ingredients for a recipe that accelerates the exploration and commercialization of space, innovates to benefit NASA and industry, and leverages assets to stimulate the economy.NASA/Danny Nowlin Cookbook author and culinary content creator Caroline Davis, popularly known as Mississippi Kween, and her family enjoy touring facilities and learning about NASA Stennis and its frontline work during a site visit Dec. 18. Davis, husband Joe, and children Zeke and Zoey, met with NASA Stennis leadership before touring the L3Harris (formerly Aerojet Rocketdyne) Engine Assembly Facility, Thad Cochran Test Stand, Autonomous Systems Laboratory, and the NASA Stennis rocket engine garden. The tour highlighted the NASA Stennis story and how the south Mississippi NASA center has the ingredients for a recipe that accelerates the exploration and commercialization of space, innovates to benefit NASA and industry, and leverages assets to stimulate the economy.NASA/Danny Nowlin Cookbook author and culinary content creator Caroline Davis, popularly known as Mississippi Kween, and her family enjoy touring facilities and learning about NASA Stennis and its frontline work during a site visit Dec. 18. Davis, husband Joe, and children Zeke and Zoey, met with NASA Stennis leadership before touring the L3Harris (formerly Aerojet Rocketdyne) Engine Assembly Facility, Thad Cochran Test Stand, Autonomous Systems Laboratory, and the NASA Stennis rocket engine garden. The tour highlighted the NASA Stennis story and how the south Mississippi NASA center has the ingredients for a recipe that accelerates the exploration and commercialization of space, innovates to benefit NASA and industry, and leverages assets to stimulate the economy.NASA/Danny Nowlin Cookbook author and culinary content creator Caroline Davis, popularly known as Mississippi Kween, and her family enjoy touring facilities and learning about NASA Stennis and its frontline work during a site visit Dec. 18. Davis, husband Joe, and children Zeke and Zoey, met with NASA Stennis leadership before touring the L3Harris (formerly Aerojet Rocketdyne) Engine Assembly Facility, Thad Cochran Test Stand, Autonomous Systems Laboratory, and the NASA Stennis rocket engine garden. The tour highlighted the NASA Stennis story and how the south Mississippi NASA center has the ingredients for a recipe that accelerates the exploration and commercialization of space, innovates to benefit NASA and industry, and leverages assets to stimulate the economy.NASA/Danny Nowlin SLS Rocket on Display at Governor’s Mansion A model of NASA’s SLS (Space Launch System) rocket is part of the holiday display in the Mississippi Governor’s Mansion in Jackson, the official residence of state Gov. Tate Reeves. The model symbolizes the longtime relationship and shared history between the state of Mississippi and NASA’s Stennis Space Center near Bay St. Louis, Mississippi, the nation’s largest rocket propulsion test site. Built in the 1960s, NASA Stennis tested Apollo rocket stages that carried humans to the Moon and every main engine that helped launch 135 space shuttle missions. It now is testing engines and systems for NASA’s Artemis missions and operates as a powerful aerospace and technology hub for the region and state. “We are grateful for our ongoing relationship with the state of Mississippi,” NASA Stennis Director John Bailey said. “We appreciate every opportunity to highlight the role NASA Stennis and the state play in helping to power the nation’s human space exploration program. We look forward to 2025 and continuing our work to test engines and systems that will help launch Artemis missions back to the Moon and beyond.” NASA Stennis/Troy Frisbie NASA Stennis Director Hosts Java with John NASA Stennis Director John Bailey hosts a Java with John session on Dec. 10 with employees representing the Office of the Chief Financial Officer, Office of STEM Engagement, Office of Diversity and Equal Opportunity, Office of the Chief Human Capital Officer, and the center’s Autonomous Systems Laboratory team. Java with John is an employee-led discussion in a casual environment aimed at fostering a culture in which employees are welcome to share what matters most to them at work. NASA/Danny Nowlin NASA Assistant Administrator for Procurement Visits NASA Stennis The NASA assistant administrator for procurement stands with leaders of NASA’s Stennis Space Center and the NASA Shared Services Center during a visit to the south Mississippi site Dec. 11 to deliver an agency update, highlighting key initiatives and priorities across NASA’s procurement activities. The visit focused on fostering open communications and collaboration, and included an opportunity for Jackson to engage with procurement staff, provide updates, and respond to questions. The assistant administrator met with NASA leadership to align on strategic goals, discuss procurement-related challenges and opportunities, and reinforce support for the NASA Stennis mission. The visit highlighted NASA’s continued commitment to innovation, efficiency, and mission success through effective procurement strategies. Pictured (left to right) are James Bailey, NASA Shared Services Center/NASA Stennis deputy procurement officer; NASA Stennis Deputy Director Christine Powell; NASA Stennis Director John Bailey; Karla Smith, NASA assistant administrator for procurement; Eli Ouder, NASA Shared Services Center/NASA Stennis procurement officer; and Jamiel Charlton, NASA executive officer. Photo Credit: NASA/Danny Nowlin > Back to Top NASA in the News Artemis II Core Stage Vertical Integration Begins at NASA Kennedy – NASA New Commercial Artemis Moon Rovers Undergo Testing at NASA – NASA NASA Accelerates Space Exploration, Earth Science for All in 2024 – NASA Space Meets Sound: NASA Lands in 2024 Spotify Wrapped – NASA Artemis Accords Reach 50 Signatories as NASA Welcomes Panama, Austria – NASA > Back to Top Employee Profile: Heather Seagren Heather Seagren grew up near NASA’s Stennis Space Center and visited for field trips as a child. Now, as a financial management specialist, Seagren coordinates work trips for NASA employees at the south Mississippi NASA center. NASA/Danny Nowlin A leap of faith for Heather Seagren eight years ago brought the Gulf Coast native to something new, yet also returned her to a familiar place at NASA’s Stennis Space Center near Bay St. Louis, Mississippi. Read More About Heather Seagren > Back to Top Additional Resources Good Things with Rebecca Turner – SuperTalk Mississippi (interview with NASA Stennis Director John Bailey) Subscription Info Lagniappe is published monthly by the Office of Communications at NASA’s Stennis Space Center. The NASA Stennis office may be contacted by at 228-688-3333 (phone); ssc-office-of-communications@mail.nasa.gov (email); or NASA OFFICE OF COMMUNICATIONS, Attn: LAGNIAPPE, Mail code IA00, Building 1111 Room 173, Stennis Space Center, MS 39529 (mail). The Lagniappe staff includes: Managing Editor Lacy Thompson, Editor Bo Black, and photographer Danny Nowlin. To subscribe to the monthly publication, please email the following to ssc-office-of-communications@mail.nasa.gov – name, location (city/state), email address. Explore More 4 min read Lagniappe for October 2024 Article 3 months ago 6 min read Lagniappe for November 2024 Article 2 months ago 4 min read Lagniappe for December 2024 Article 1 month ago View the full article

2 min read Preparations for Next Moonwalk Simulations Underway (and Underwater) Heather Seagren grew up near NASA’s Stennis Space Center and visited for field trips as a child. Now, as a financial management specialist, Seagren coordinates work trips for NASA employees at the south Mississippi NASA center. NASA/Danny Nowlin A leap of faith for Heather Seagren eight years ago brought the Gulf Coast native to something new, yet also returned her to a familiar place at NASA’s Stennis Space Center near Bay St. Louis, Mississippi. Following graduation from Pearl River Community College, Seagren worked as an office manager at a pediatric office. Seagren anticipated a full career in the medical field until an opportunity at the south Mississippi NASA center “kind of fell in my lap,” she said. The NASA Shared Services Center, located at NASA Stennis, was hiring for its travel department, so Seagren applied. “There are many different roles here, and my biggest thing was, do not second guess your decisions,” she said. “It was a big change for me, and I made the leap and ended up where I am today, even though it was a completely different career field.” A new career field, yes, but not a new place. Seagren grew up in Pearlington, Mississippi, less than 10 miles from the nation’s largest propulsion test site. Her grandfather, Grover “Shu-Shu” Bennett, retired from NASA Stennis as a tugboat captain, helping to deliver rocket propellants along the site canal system to the test stands at NASA Stennis. Just as her grandfather ensured the rocket engine fuel made it to its destination on time, Seagren does the same for NASA employees by coordinating travel plans. She now is in a similar role as a NASA Stennis financial management specialist. Working with astronauts, engineers, and many other NASA employees, no two trips are alike, which is a part of the job Seagren enjoys. What is similar is the trips coordinated by Seagren align with NASA’s mission to explore the secrets of the universe for the benefit of all. The Kiln, Mississippi, resident plays a vital role in the NASA mission by bringing together the details of booking flights, arranging accommodations, and managing schedules. “The best thing about working at NASA Stennis is getting to experience everything,” she said. “It is always interesting to see what other projects and duties everybody is doing. The process kind of starts with the travel department. … It is a small step, but we are involved, making sure everybody is where they need to be, when they need to be there, so, I think that is pretty cool.” Learn more about the people who work at NASA Stennis View the full article

Learn Home Science Activation NASA Workshops Culturally… Overview Learning Resources Science Activation Teams SME Map Opportunities More Science Activation Stories Citizen Science 2 min read NASA Workshops Culturally Inclusive Planetary Engagement with Educators From November 6-8, 2024, the NASA Science Activation Program’s Planetary Resources and Content Heroes (ReaCH) project held a Culturally Inclusive Planetary Engagement workshop at the Bradley Observatory at Agnes Scott College in Atlanta, Georgia for the space sciences community, including planetary science, astrobiology, astronomy, and heliophysics professionals, as well as invited education specialists. To practice the skills learned in the workshop, participants facilitated a variety of space-themed, culturally-inclusive, hands-on activities for 79 students, family, and staff at the Center for a New Generation at the Tuskegee Airmen Global Academy Boys and Girls Club. Workshop participants provided anonymous feedback as a part of their workshop evaluations: “[This experience] helped me learn a lot about how to make different cultures and ethnicities feel involved and included and also engage with them to inspire in them a love for science” “. . .I feel like the discussions were so important to me, considering we all come from so many different backgrounds, and our exposure has been different, so we all have a different point of view to bring to the discussion that others, that I, might not think of right away. So I think it was really nice to hear so many different perspectives in all of these discussions.” “[The facilitator] connected cultural diversity to an activity. That is not easy to do. I loved it and it is what I expected coming into this workshop.” This workshop was conducted in partnership with Agnes Scott College, Georgia Tech, the Boys & Girls Clubs of Metro Atlanta, and members of the Center for Lunar Environment and Volatile Exploration Research (CLEVER) NASA Solar System Exploration Research Institute (SSERVI) Center. ReaCH workshops are designed to enhance the ability of scientists to engage their local communities in science. The Planetary ReaCH project is building a replicable model that will be used to support similar workshops for other science fields. NASA-funded researchers, including early-career scientists, are invited to apply for the 2025 workshops! The Planetary ReaCH project is supported by NASA under cooperative agreement award number 80NSSC21M0003 and is part of NASA’s Science Activation Portfolio. Learn more about how Science Activation connects NASA science experts, real content, and experiences with community leaders to do science in ways that activate minds and promote deeper understanding of our world and beyond: https://science.nasa.gov/learn The workshop was attended by researchers including early career scientists, planetary scientists, astrobiologists, astronomers, heliophysicists, and education specialists. Share Details Last Updated Jan 02, 2025 Editor NASA Science Editorial Team Related Terms Grades 5 – 8 for Educators Grades 9-12 for Educators Grades K – 4 for Educators Opportunities For Educators to Get Involved Planetary Science Science Activation Explore More 3 min read Astronomy Activation Ambassadors: A New Era Article 2 days ago 5 min read NASA Study Shows Ferns Facilitate Recovery from Environmental Disaster NASA-supported scientists have shown how ferns might help ecosystems recover from disasters. Article 2 weeks ago 5 min read NASA DAVINCI Mission’s Many ‘Firsts’ to Unlock Venus’ Hidden Secrets NASA’s DAVINCI probe will be first in the 21st century to brave Venus’ atmosphere as… Article 2 weeks ago Keep Exploring Discover More Topics From NASA James Webb Space Telescope Webb is the premier observatory of the next decade, serving thousands of astronomers worldwide. It studies every phase in the… Perseverance Rover This rover and its aerial sidekick were assigned to study the geology of Mars and seek signs of ancient microbial… Parker Solar Probe On a mission to “touch the Sun,” NASA’s Parker Solar Probe became the first spacecraft to fly through the corona… Juno NASA’s Juno spacecraft entered orbit around Jupiter in 2016, the first explorer to peer below the planet’s dense clouds to… View the full article

3 min read Preparations for Next Moonwalk Simulations Underway (and Underwater) Next Generation Lunar Retroreflector, or NGLR-1, is one of 10 payloads set to fly aboard the next delivery for NASA’s CLPS (Commercial Lunar Payload Services) initiative in 2025. NGLR-1, outfitted with a retroreflector, will be delivered to the lunar surface to reflect very short laser pulses from Earth-based lunar laser ranging observatories. Photo courtesy Firefly Aerospace Apollo astronauts set up mirror arrays, or “retroreflectors,” on the Moon to accurately reflect laser light beamed at them from Earth with minimal scattering or diffusion. Retroreflectors are mirrors that reflect the incoming light back in the same incoming direction. Calculating the time required for the beams to bounce back allowed scientists to precisely measure the Moon’s shape and distance from Earth, both of which are directly affected by Earth’s gravitational pull. More than 50 years later, on the cusp of NASA’s crewed Artemis missions to the Moon, lunar research still leverages data from those Apollo-era retroreflectors. As NASA prepares for the science and discoveries of the agency’s Artemis campaign, state-of-the-art retroreflector technology is expected to significantly expand our knowledge about Earth’s sole natural satellite, its geological processes, the properties of the lunar crust and the structure of lunar interior, and how the Earth-Moon system is changing over time. This technology will also allow high-precision tests of Einstein’s theory of gravity, or general relativity. That’s the anticipated objective of an innovative science instrument called NGLR (Next Generation Lunar Retroreflector), one of 10 NASA payloads set to fly aboard the next lunar delivery for the agency’s CLPS (Commercial Lunar Payload Services) initiative. NGLR-1 will be carried to the surface by Firefly Aerospace’s Blue Ghost 1 lunar lander. Developed by researchers at the University of Maryland in College Park, NGLR-1 will be delivered to the lunar surface, located on the Blue Ghost lander, to reflect very short laser pulses from Earth-based lunar laser ranging observatories, which could greatly improve on Apollo-era results with sub-millimeter-precision range measurements. If successful, its findings will expand humanity’s understanding of the Moon’s inner structure and support new investigations of astrophysics, cosmology, and lunar physics – including shifts in the Moon’s liquid core as it orbits Earth, which may cause seismic activity on the lunar surface. “NASA has more than half a century of experience with retroreflectors, but NGLR-1 promises to deliver findings an order of magnitude more accurate than Apollo-era reflectors,” said Dennis Harris, who manages the NGLR payload for the CLPS initiative at NASA’s Marshall Space Flight Center in Huntsville, Alabama. Deployment of the NGLR payload is just the first step, Harris noted. A second NGLR retroreflector, called the Artemis Lunar Laser Retroreflector (ALLR), is currently a candidate payload for flight on NASA’s Artemis III mission to the Moon and could be set up near the lunar south pole. A third is expected to be manifested on a future CLPS delivery to a non-polar location. “Once all three retroreflectors are operating, they are expected to deliver unprecedented opportunities to learn more about the Moon and its relationship with Earth,” Harris said. Under the CLPS model, NASA is investing in commercial delivery services to the Moon to enable industry growth and support long-term lunar exploration. As a primary customer for CLPS deliveries, NASA aims to be one of many customers on future flights. NASA’s Marshall Space Flight Center in Huntsville, Alabama, manages the development of seven of the 10 CLPS payloads carried on Firefly’s Blue Ghost lunar lander. Learn more about. CLPS and Artemis at: https://www.nasa.gov/clps Alise Fisher Headquarters, Washington 202-358-2546 Alise.m.fisher@nasa.gov Headquarters, Washington 202-358-2546 Alise.m.fisher@nasa.gov Corinne Beckinger Marshall Space Flight Center, Huntsville, Ala. 256-544-0034 corinne.m.beckinger@nasa.gov Share Details Last Updated Jan 02, 2025 EditorBeth RidgewayContactCorinne M. Beckingercorinne.m.beckinger@nasa.govLocationMarshall Space Flight Center Related TermsCommercial Lunar Payload Services (CLPS)ArtemisMarshall Space Flight Center Explore More 3 min read NASA Science Payload to Study Sticky Lunar Dust Challenge Article 2 weeks ago 4 min read Artemis II Core Stage Vertical Integration Begins at NASA Kennedy Article 2 weeks ago 2 min read NASA Names Carlos Garcia-Galan as Gateway Program Deputy Manager Article 2 weeks ago Keep Exploring Discover Related Topics Missions Humans in Space Climate Change Solar System View the full article

NASA/Joel Kowsky NASA photographer Joel Kowsky captured this image of the Monday, April 8, 2024, total solar eclipse from the Indianapolis Motor Speedway in Indianapolis, Indiana. The total solar eclipse swept across a narrow portion of the North American continent from Mexico’s Pacific coast to the Atlantic coast of Newfoundland, Canada. A partial solar eclipse was visible across the entire North American continent along with parts of Central America and Europe. The NASA Headquarters photo team chose this image as one of the best from 2024. See more of the top 100 from last year on Flickr. Image Credit: NASA/Joel Kowsky View the full article

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3 min read January’s Night Sky Notes: The Red Planet by Kat Troche of the Astronomical Society of the Pacific Have you looked up at the night sky this season and noticed a bright object sporting a reddish hue to the left of Orion? This is none other than the planet Mars! January will be an excellent opportunity to spot this planet and some of its details with a medium-sized telescope. Be sure to catch these three events this month. Martian Retrograde Mars entered retrograde (or backward movement relative to its usual direction) on December 7, 2024, and will continue throughout January into February 23, 2025. You can track the planet’s progress by sketching or photographing Mars’ position relative to nearby stars. Be consistent with your observations, taking them every few nights or so as the weather permits. You can use free software like Stellarium or Stellarium Web (the browser version) to help you navigate the night as Mars treks around the sky. You can find Mars above the eastern horizon after 8:00 PM local time. This mid-January chart shows the path of Mars from September 2024 to June 2025 as it enters and then exits in retrograde motion. Mars appears to change its direction of motion in the sky because Earth is passing the slower-moving Mars in its orbit. Stellarium Hide and Seek On the night of January 13th, you can watch Mars ‘disappear’ behind the Moon during an occultation. An occultation is when one celestial object passes directly in front of another, hiding the background object from view. This can happen with planets and stars in our night sky, depending on the orbit of an object and where you are on Earth, similar to eclipses. A simulated view of the Moon as Mars begins its occultation on January 13, 2025. Stellarium Depending on where you are within the contiguous United States, you can watch this event with the naked eye, binoculars, or a small telescope. The occultation will happen for over an hour in some parts of the US. You can use websites like Stellarium Web or the Astronomical League’s ‘Moon Occults Mars’ chart to calculate the best time to see this event. Closer and Closer As you observe Mars this month to track its retrograde movement, you will notice that it will increase in brightness. This is because Mars will reach opposition by the evening of January 16th. Opposition happens when a planet is directly opposite the Sun, as seen from Earth. You don’t need to be in any specific city to observe this event; you only need clear skies to observe that it gets brighter. It’s also when Mars is closest to Earth, so you’ll see more details in a telescope. Want a quick and easy way to illustrate what opposition is for Jupiter, Saturn, Mars, or other outer worlds? Follow the instructions on our Toolkit Hack: Illustrating Opposition with Exploring the Solar System page using our Exploring Our Solar System activity! A mosaic of the Valles Marineris hemisphere of Mars projected into point perspective, a view similar to that which one would see from a spacecraft. The mosaic is composed of 102 Viking Orbiter images of Mars. NASA/JPL-Caltech Mars has fascinated humanity for centuries, with its earliest recorded observations dating back to the Bronze Age. By the 17th century, astronomers were able to identify features of the Martian surface, such as its ice caps and darker regions. Since the 1960s, exploration of the Red Planet has intensified with robotic missions from various space organizations. Currently, NASA has five active missions, including rovers and orbiters, with the future focused on human exploration and habitation. Mars will always fill us with a sense of wonder and adventure as we reach for its soil through initiatives such as the Moon to Mars Architecture and the Mars Sample Return campaign. View the full article

Learn Home Astronomy Activation… STEM Engagement at NASA Overview Learning Resources Science Activation Teams SME Map Opportunities More Science Activation Stories Citizen Science 3 min read Astronomy Activation Ambassadors: A New Era The NASA Science Activation Program’s Astronomy Activation Ambassadors (AAA) project aims to measurably enhance student Science, Technology, Engineering, and Mathematics (STEM) engagement via middle school, high school, and community college science teacher professional development. In 2024, AAA transitioned its focus to the development of an Astronomy Academy with varying levels of extent and intensity available to more than 300 teachers per year. Participants draw on NASA resources and Subject Matter Experts (SME) to enhance their teaching and help share their excitement about astronomy with their students. The three strands that comprise the Astronomy Academy are: webinars regarding NASA astrophysics and planetary science content and facilities, curriculum workshops enabling classroom use of an electromagnetic spectrum and multi-wavelength astronomy (EMS/MWA) curriculum, and STEM immersion experiences including guided visits to working observatories. The first two of the AAA program’s new type of STEM immersion experiences took place in June and September, 2024. During the weekend of June 22-23, 19 teachers gathered in San Jose, California for a full agenda, including: NASA SME presentations regarding planetary protection and exoplanet detection, a journey to the University of California’s Lick Observatory on nearby Mt. Hamilton for an in-depth guided tour of the observatory’s astronomy research facilities, which included engagement with the astronomers using the 3-meter Shane telescope, and a 4-hour hands-on EMS/MWA curriculum teaching workshop. A similar STEM immersion sequence was offered September 14-15 to 23 AAA teachers who attended a curriculum teaching workshop, learned about current infrared astronomy research from NASA Jet Propulsion Laboratory scientists, and received guided visits to the Keck Observatory’s remote observing facility on the Caltech campus and the Mt. Wilson Observatory, including a half-night’s reserved use of the historic Mt. Wilson 60-inch telescope. The teachers were invited to submit a list of objects to be observed with the Mt. Wilson telescope and viewed a wonderful array of star clusters, colorful double stars, and galaxies, with a grand finale view of Saturn and its rings. Teacher participant, Domina Stamas (Westlake Charter School, Sacramento, California), had this to say: “My students and I are already benefiting greatly from the combination of NASA resources, science content, and curricular materials we have received from the AAA project. The evening at Lick Observatory talking with the astronomers who were using the research telescopes watching the laser guide star setup in action was a rich experience. I can convey to my students how scientists actually practice their craft.” The Astronomy Activation Ambassador project’s efforts to improve student STEM learning and engagement via science teacher professional development are detailed at: https://www.seti.org/aaa Educator enrollment is still open via the participant registration form: https://forms.gle/G34vCzz63ko5RRrM8 The AAA project, led by the SETI Institute, is supported by NASA under cooperative agreement award number NNX16AC51A and is part of NASA’s Science Activation Portfolio. Learn more about how Science Activation connects NASA science experts, real content, and experiences with community leaders to do science in ways that activate minds and promote deeper understanding of our world and beyond: https://science.nasa.gov/learn June 2024 teacher participants in front of the Lick Observatory’s historic 36-inch refracting telescope. SETI Institute/C. Clark Share Details Last Updated Dec 31, 2024 Editor NASA Science Editorial Team Location Jet Propulsion Laboratory Related Terms Astronomy Astrophysics Grades 9-12 for Educators Opportunities For Educators to Get Involved Opportunities For Students to Get Involved Planetary Science Science Activation STEM Engagement at NASA Explore More 5 min read NASA Study Shows Ferns Facilitate Recovery from Environmental Disaster NASA-supported scientists have shown how ferns might help ecosystems recover from disasters. Article 2 weeks ago 2 min read Hubble Spies a Cosmic Eye Article 2 weeks ago 7 min read Very Cold Detectors Reveal the Very Hot Universe and Kick Off a New Era in X-ray Astronomy Article 2 weeks ago Keep Exploring Discover More Topics From NASA James Webb Space Telescope Webb is the premier observatory of the next decade, serving thousands of astronomers worldwide. It studies every phase in the… Perseverance Rover This rover and its aerial sidekick were assigned to study the geology of Mars and seek signs of ancient microbial… Parker Solar Probe On a mission to “touch the Sun,” NASA’s Parker Solar Probe became the first spacecraft to fly through the corona… Juno NASA’s Juno spacecraft entered orbit around Jupiter in 2016, the first explorer to peer below the planet’s dense clouds to… View the full article

Peering through the window of the SpaceX Dragon Endeavour spacecraft, NASA astronaut Matthew Dominick captured this image on Oct. 7, 2024 of the SpaceX Dragon Freedom spacecraft as vivid green and pink aurora swirled through Earth’s atmosphere while the International Space Station soared 273 miles above the Indian Ocean. Visit Dominick’s photography on station to experience the wonders of space through his eyes, enriched by his remarkable journey of orbiting the Earth 3,760 times. To see a short-term forecast of the location and intensity of the next aurora check this link: Aurora – 30 Minute Forecast and also NASA’s Guide to Finding and Photographing Auroras. Image Credit: NASA/Matthew Dominick View the full article

6 min read Preparations for Next Moonwalk Simulations Underway (and Underwater) In-person participants L-R standing: Dave Francisco, Joanne Kaouk, Dr. Richard Moon, Dr. Tony Alleman, Dr. Sean Hardy, Sarah Childress, Kristin Coffey, Dr. Ed Powers, Dr. Doug Ebersole, Dr. Steven Laurie, Dr. Doug Ebert; L-R seated: Dr. Alejandro Garbino, Dr. Robert Sanders, Dr. Kristi Ray, Dr. Mike Gernhardt, Dr. Joseph Dervay, Dr. Matt Makowski). Not pictured: Dr. Caroline Fife In June 2024, the NASA Office of the Chief Health and Medical Officer (OCHMO) Standards Team hosted an independent assessment working group to review the status and progress of research and clinical activities intended to mitigate the risk of decompression sickness (DCS) related to patent foramen ovale (PFO) during spaceflight and associated ground testing and human subject studies. Decompression sickness (DCS) is a condition which results from dissolved gases (primarily nitrogen) forming bubbles in the bloodstream and tissues. It is usually experienced in conditions where there are rapid decreases in ambient pressure, such as in scuba divers, high-altitude aviation, or other pressurized environments. The evolved gas bubbles have various physiological effects and can obstruct the blood vessels, trigger inflammation, and damage tissue, resulting in symptoms of DCS. NASA presently classifies DCS into two categories: Type I DCS, which is less severe, typically leads to musculoskeletal symptoms including pain in the joints or muscles, or skin rash. Type II DCS is more severe and commonly results in neurological, inner ear, and cardiopulmonary symptoms. The risk of DCS in spaceflight presents during extravehicular activities (EVAs) in which astronauts perform mission tasks outside the spaceflight vehicle while wearing a pressurized suit at a lower pressure than the cabin pressure. DCS mitigation protocols based on strategies to reduce systemic nitrogen load are implemented through the combination of habitat environmental parameters, EVA suit pressure, and breathing gas procedures (prebreathe protocols) to achieve safe and effective mission operations. The pathophysiology of DCS has still not been fully elucidated since cases occur despite the absence of detected gas bubbles but includes right to left shunting of venous gas emboli (VGE) via several potential mechanisms, one of which is a Patent Foramen Ovale (PFO). From: Dr. Schochet & Dr. Lie, Pediatric Pulmonologists Reference OCHMO-TB-037 Decompression Sickness (DCS) Risk Mitigation technical brief for additional information. A PFO is a shunt between the right atrium and the left atrium of the heart, which is a persisting remnant of a physiological communication present in the fetal heart. Post-natal increases in left atrial pressure usually force the inter-septal valve against the septum secundum and within the first 2 years of life, the septae permanently fuse due to the development of fibrous adhesions. Thus, all humans are born with a PFO and approximately 75% of PFOs fuse following childbirth. For the 25% of the population’s whose PFOs do not fuse, ~6% have what is considered by some to be a large PFO (> 2 mm). PFO diameter can increase with age. The concern with PFOs is that with a right to left shunt between the atria, venous emboli gas may pass from the right atrium (venous) to the left atrium (arterial) (“shunt”), thus by-passing the normal lung filtration of venous emboli which prevent passage to the arterial system. Without filtration, bubbles in the arterial system may lead to a neurological event such as a stroke. Any activity that increases the right atrium/venous pressure over the left atrium/arterial pressure (such as a Valsalva maneuver, abdominal compression) may further enable blood and/or emboli across a PFO/shunt. From: Nuffield Department of Clinical Neurosciences The purpose of this working group was to review and provide analysis on the status and progress of research and clinical activities intended to mitigate the risk of PFO and DCS issues during spaceflight. Identified cases of DCS during NASA exploration atmosphere ground testing conducted in pressurized chambers led to the prioritization of the given topic for external review. The main goals of the working group included: Quantification of any increased risk associated with the presence of a PFO during decompression protocols utilized in ground testing and spaceflight EVAs, as well as unplanned decompressions (e.g., cabin depressurization, EVA suit leak). Describe risks and benefits of PFO screening in astronaut candidates, current crewmembers, and chamber test subjects. What are potential risk reduction measures that could be considered if a person was believed to be at increased risk of DCS due to a PFO? What research and/or technology development is recommended that could help inform and/or mitigate PFO-related DCS risk? The working group took place over two days at NASA’s Johnson Space Center and included NASA subject matter experts and stakeholders, as well as invited external reviewers from areas including cardiology, hypobaric medicine, spaceflight medicine, and military occupational health. During the working group, participants were asked to review past reports and evidence related to PFOs and risk of DCS, materials and information regarding NASA’s current experience and practices, and case studies and subsequent decision-making processes. The working group culminated in an open-forum discussion where recommendations for current and future practices were conferred and subsequently summarized in a final summary report, available on the public NASA OCHMO Standards Team website. The following key findings are the main take-aways from the OCHMO independent assessment: In an extreme exposure/high-risk scenario, excluding individuals with a PFO and treating PFOs does not necessarily decrease the risk of DCS or create a ‘safe’ environment. It may create incremental differences and slightly reduce overall risk but does not make the risk zero. There are other physiological factors that also contribute to the risk of DCS that may have a larger impact (see 7.0 Other Physiological Factors in the findings section). Based on the available evidence and the risk of current decompression exposures (based on current NASA protocols and NASA-STD-3001 requirements to limit the risk of DCS), it is not recommended to screen for PFOs in any spaceflight or ground testing participants. The best strategy to reduce the risk of DCS is to create as safe an environment as possible in every scenario, through effective prebreathe protocols, safety, and the capability to rapidly treat DCS should symptoms occur. Based on opinion, no specific research is required at this time to further characterize PFOs with DCS and altitude exposure, due to the low risk and preference to institute adequate safe protocols and ensuring treatment availability both on the ground and in spaceflight. For engineering protocols conducted on the ground, it should be ensured that the same level of treatment capability (treatment chamber in the immediate vicinity of the testing) is provided as during research protocols. The ability to immediately treat a DCS case is critical in ensuring the safety of the test subjects. The full summary report includes detailed background information, discussion points from the working group, and conclusions and recommendations. The findings from the working group and resulting summary report will help to inform key stakeholders in decision-making processes for future ground testing and spaceflight operations with the main goal of protecting crew health and safety to ensure overall mission success. Summary Report About the AuthorSarah D. Childress Share Details Last Updated Dec 31, 2024 Related TermsOffice of the Chief Health and Medical Officer (OCHMO)Human Health and PerformanceHumans in SpaceInternational Space Station (ISS) Explore More 2 min read Station Science Top News: Dec. 20, 2024 Article 2 weeks ago 4 min read Artemis II Core Stage Vertical Integration Begins at NASA Kennedy Article 2 weeks ago 3 min read NASA, Axiom Space Change Assembly Order of Commercial Space Station Article 2 weeks ago Keep Exploring Discover More Topics From NASA Missions Humans in Space Climate Change Solar System View the full article

Curiosity Navigation Curiosity Home Mission Overview Where is Curiosity? Mission Updates Science Overview Instruments Highlights Exploration Goals News and Features Multimedia Curiosity Raw Images Images Videos Audio Mosaics More Resources Mars Missions Mars Sample Return Mars Perseverance Rover Mars Curiosity Rover MAVEN Mars Reconnaissance Orbiter Mars Odyssey More Mars Missions The Solar System The Sun Mercury Venus Earth The Moon Mars Jupiter Saturn Uranus Neptune Pluto & Dwarf Planets Asteroids, Comets & Meteors The Kuiper Belt The Oort Cloud 2 min read Sols 4402-4415: Rover Decks and Sequence Calls for the Holidays An image under the left-front wheel of NASA’s Mars rover Curiosity shows a block that Curiosity drove over and possibly broke in half. The rover acquired this image using its Mars Descent Imager (MARDI) on sol 4396 — Martian day 4,396 of the Mars Science Laboratory mission — on Dec. 18, 2024 at 06:03:35 UTC. NASA/JPL-Caltech/MSSS Earth planning date: Friday, Dec. 20, 2024 Welcome to the 2024 holiday plan for Curiosity! This year we’re spanning 14 sols to last us through the Earth new year. And this is my fourth year operating Mastcam during the holidays (throwback to 2023 Marsmas!). I already knew to expect a long day, so I got my lunch prepared — blew Mars a kiss in the pre-dawn sky — and headed to work at 0600 Pacific time to start planning prep. Luckily my team got a head start on Mastcam images by including a full 360-degree panorama, post-drive, last plan, so I just had to fill in some gaps and cover some buttes with our higher-resolution camera. In total we’re only planning about 438 images this holiday, which is a pretty light haul if you can believe it! We also didn’t pass SRAP to unstow the arm (again) today, which is a bummer for science but usually makes my job easier since Mastcam doesn’t have to worry about where the arm might be during our imaging. One instrument’s coal is another instrument’s present! So we’re doing things a little funky this holiday. We’re planning science on the first, seventh, 13th, and 14th sols — with a drive and a soliday! The hardest part of this plan was keeping it all straight in our heads. Without any contact science planned, MAHLI went on holiday early (actually, she’s been out all week!) and APXS only had to babysit an atmospheric integration, which doesn’t require any arm motion. ChemCam has three LIBS and four RMI mosaics planned, which is definitely more than usual. But actually, the highest sequence count for today goes to Mastcam! Our usual limit is around 20 sequences for complexity reasons, but today I delivered 34 total sequences. Of those 34 sequences, 10 are for tracking surface changes from wind, seven are for measuring the atmospheric opacity, three are ChemCam LIBS documentations, three are for documenting our location post-drive, two are large mosaics of Texoli and Wilkerson buttes, and two are for noctilucent cloud searching (our first attempts to find clouds this Martian winter!). With any luck, we’ll start passing SRAP again in 2025 after another approximately 58-meter drive (about 190 feet). Until then, Earthlings — Merry Marsmas and Happy Earth New Year! Written by Natalie Moore, Mission Operations Specialist at Malin Space Science Systems Share Details Last Updated Dec 30, 2024 Related Terms Blogs Explore More 4 min read Sols 4398-4401: Holidays Ahead, Rocks Under the Wheels Article 2 weeks ago 3 min read Perseverance Blasts Past the Top of Jezero Crater Rim Article 2 weeks ago 3 min read Sols 4396-4397: Roving in a Martian Wonderland Article 2 weeks 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

Skywatching Skywatching Home What’s Up Eclipses Explore the Night Sky Night Sky Network More Tips and Guides FAQ Four Planets in One View! Each evening this month, enjoy a sweeping view of four bright planets at once. Also look for a close approach of Venus and Saturn, Mars occulted by the Moon, and meteors! Skywatching Highlights January 3 – Quadrantid meteor shower peaks: This is a moderate shower, usually delivering 20 to 30 meteors per hour under clear, dark skies at its peak. No interference from the Moon makes this year’s peak a better bet for meteor watching. January 13 – Moon Occults Mars: For skywatchers in the continental U.S. and Eastern Canada, the Moon will appear to pass in front of Mars this evening. Times vary by location, so check your favorite skywatching app for details. January 17-18 – Venus and Saturn conjunction: Over a couple of weeks, the two planets come within just a couple of finger widths’ distance apart in the sky (about 2 degrees). They’re at their closest on the 17th and 18th. All month – Four planets Visible: In the first couple of hours after dark, you’ll find Venus and Saturn in the southwest, Jupiter high overhead, and Mars in the east. (Uranus and Neptune are there too, but a telescope is needed to see them.) Planets always appear a long a line on the sky to the “alignment” isn’t special. What’s less common is seeing four or five bright planets at once, which doesn’t happen every year. Is it a “planet parade”? This isn’t a technical term in astronomy, so call it what you wish! All month – Mars at Opposition: The Red Planet is directly opposite the Sun from Earth and shines brightly all night. It’s in the east as night falls and in the southwest at dawn. Transcript What’s Up for January? Cue the planet parade, Saturn and Venus cross paths, Mars expresses its opposition, and the outlook for the Quadrantid meteors. In January, you’ll have the opportunity to take in four bright planets in a single, sweeping view. Sky chart showing the planetary lineup visible after dark in January 2025. NASA/JPL-Caltech All month after dark, you’ll find Venus and Saturn in the southwest for the first couple of hours, while Jupiter shines brightly high overhead, and Mars rises in the east. Uranus and Neptune are there too, technically, but they don’t appear as “bright planets.” These multi-planet viewing opportunities aren’t super rare, but they don’t happen every year, so it’s worth checking it out. Now, these events are sometimes called “alignments” of the planets, and while it’s true that they will appear more or less along a line across the sky, that’s what planets always do. That line is called the ecliptic, and it represents the plane of the solar system in which the planets orbit around the Sun. This is, incidentally, why we sometimes observe planets appearing to approach closely to each other on the sky, as we view them along a line while they careen around the cosmic racetrack. Sky chart showing Venus and Saturn appearing quite close together on Jan. 17 and 18, 2025. NASA/JPL-Caltech This is exactly what we’ll be seeing from Venus and Saturn as they head for a super close approach in mid-January. After the beginning of the month, they quickly get closer and closer each evening, appearing at their most cozy on the 17th and 18th before going their separate ways. Remember, they’re really hundreds of millions of miles apart in space, so when you observe them, you’re staring clear across the solar system! Mars reaches “opposition” this month, which is when the planet lies directly on the opposite side of Earth from the Sun, forming a straight line. This is around the time when the planet is at its closest to Earth, making it appear at its biggest and brightest. For Mars, oppositions happen about every two years. This one won’t be the most spectacular ever, but it’s still closer than average, and provides a great opportunity to observe the nearby planet where NASA has five missions currently operating. And on the 13th, the full Moon cozies up to Mars, appearing super close to the Red Planet that evening. Across the U.S. and Eastern Canada, the Moon will appear to pass in front of Mars over a couple of hours, as the pair rise into the eastern sky. Mars also will be the lone planet in the sky on January mornings. You’ll find it hanging out in the west in morning twilight. The Quadrantid meteors peak in the early morning hours on January 3rd. Interference from moonlight won’t be a problem, as the Moon is a mere crescent and sets early in the night. The way to see the most meteors is to observe after midnight from clear, dark skies away from bright city lights, and let your eyes adapt to the dark. The meteor rate will be highest as dawn approaches, and you’ll see more meteors from rural locations than in the suburbs. Now, this is a shower best seen from the Northern Hemisphere, and observers in the Northwest and Pacific region will likely have the best viewing this year. Here are the phases of the Moon for January: The phases of the Moon for January 2025. NASA/JPL-Caltech Stay up to date on all of NASA’s missions exploring the solar system and beyond at science.nasa.gov. I’m Preston Dyches from NASA’s Jet Propulsion Laboratory, and that’s What’s Up for this month. Keep Exploring Discover More Topics From NASA Solar System Exploration Planets Moons Asteroids, Comets & Meteors View the full article

NASA President Jimmy Carter, wife Rosalynn, and daughter Amy, along with Kennedy Space Center Director Lee Scherer, look at a scale model of the crawler that transported the total shuttle launch configuration from the Vehicle Assembly Building to Pad 39. Despite the setbacks faced through technical and schedule problems during the development of the Space Shuttle Program, President Carter provided NASA with its first budget extension to complete funding for the program. His decision to support the creation of a peaceful scientific spacecraft enabled the creation of the International Space Station, the longest continuously maintained laboratory in space–dedicated to the peaceful advance of scientific discovery. President Carter passed away Sunday, Dec. 29, 2024. Read a statement from NASA Administrator Bill Nelson paying tribute. Image Credit: NASA View the full article

NASA Administrator Bill Nelson, and NASA Deputy Administrator Pam Melroy, react as they are recognized by employees during a NASA agencywide all hands on Dec. 6, 2024, at the NASA Headquarters Mary W. Jackson Building in Washington.Credit: NASA/Bill Ingalls NASA Administrator Bill Nelson and Deputy Administrator Pam Melroy will speak with NASA astronauts Nick Hague, Butch Wilmore, Suni Williams, and Don Pettit on Monday, Jan. 6, to discuss their mission aboard the International Space Station. The Earth to space call coverage begins at 1:30 p.m. EST on NASA+. Learn how to watch NASA content through a variety of platforms, including social media. NASA’s Commercial Crew Program has delivered on its goal of safe, reliable, and cost-effective transportation to and from the International Space Station from the United States through a partnership with American private industry. This partnership is opening access to low Earth orbit and the space station to more people, science, and commercial opportunities. The space station remains the springboard to NASA’s next great leap in space exploration, including future missions to the Moon and eventually, to Mars. For NASA’s launch blog and more information about the mission, visit: https://www.nasa.gov/commercialcrew -end- Meira Bernstein / Josh Finch Headquarters, Washington 202-358-1100 meira.b.bernstein@nasa.gov / joshua.a.finch@nasa.gov Share Details Last Updated Dec 30, 2024 LocationNASA Headquarters Related TermsInternational Space Station (ISS)Commercial CrewHumans in SpaceISS ResearchJohnson Space Center View the full article