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20 news items
TESSI292 - "Dataset: updated structure"
Data & Statistics
1 min read

TESSI292 - "Dataset: updated structure"

Share of total population living in a dwelling with a leaking roof, damp walls, floors or foundation, or rot in window frames of floor - EU-SILC survey

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NASA, USGS Scientists Go Rock Hounding in California’s High Desert
Science & Space
6 min read

NASA, USGS Scientists Go Rock Hounding in California’s High Desert

Geologists recently converged on a site near Barstow, California, to ground-truth a mineral discovery made on public land by a NASA JPL sensor flying aboard a plane overhead. NASA/JPL-Caltech Equipped with rock picks and hand lenses, a team of geoscientists deployed to the Mojave Desert recently to investigate a tantalizing “fingerprint” detected by a NASA sensor. Their target: a cache of topaz hiding in plain sight. The geologists weren’t searching for gem-grade treasure. Rather, the presence of topaz could hint at a more valuable deposit below of something known as porphyry copper. One of the world’s primary sources of copper, these deposits are left behind when magma and hot water from deep underground course through Earth’s crust, chemically transforming the surrounding rock. This tends to occur where one tectonic plate dives below another, known as a subduction zone, such as the North American Cordillera, which stretches from the Canadian Rockies to western Mexico. California’s high desert stretches below a bright spring sky in April 2026. NASA and USGS scientists are using airborne remote sensing to home in on potential sources of critical minerals here and across the Western U.S. NASA/JPL-Caltech In addition to copper — the third most used metal in the world after steel and aluminum — the deposits can hold other critical minerals like molybdenum and tellurium, which are used in everything from steelmaking to solar panels. Finding the deposits isn’t easy. Geologists look for topaz because it forms under the same volcanic conditions. For the team in the Mojave, the goal was to collect more evidence. That would require boots on the ground and a heavy bag of samples. The scientists who converged on the site included three experts from the U.S. Geological Survey (USGS) and Robert Green of NASA’s Jet Propulsion Laboratory in Southern California. “What we’re doing out here is geologic CSI,” said Green, referring to the investigative TV show, as he split open a weathered red rock to expose a sparkling core. “We’re looking for clues to reconstruct what happened here.” Three-dimensional image cubes illustrate the volume of data captured by NASA imaging spectrometers. The front face shows an aerial view of the Mojave Desert. The colorful side panels reveal what no eye or camera can detect: the spectral fingerprints of minerals present in every pixel. NASA/JPL-Caltech Next-generation mineral mapping The sensor that detected the topaz deposit on public land near Barstow, California, was built at JPL. Called AVIRIS, short for Airborne Visible Infrared Imaging Spectrometer, it analyzes reflected sunlight and can be used to identify chemicals and minerals by their unique spectral fingerprint. The technology was pioneered in the early 1980s by a team that included Green, and space-hardened versions have explored the Moon, Mars, and other rocky bodies in the solar system in the decades since. While its cousins study distant worlds aboard spacecraft, the AVIRIS line of sensors is advancing Earth science from aircraft. The latest model, AVIRIS-5, recently took to the skies for the first time as part of the NASA-USGS Geologic Earth Mapping Experiment ( GEMx ). The goal of GEMx is to identify sources of critical minerals across the American West, including in the waste rock of active and legacy mines. It is led by the USGS as part of its larger, nationwide initiative . Carrying next-generation sensors, a high-altitude NASA ER-2 aircraft takes off from the agency’s Armstrong Flight Research Center in Edwards, California, on March 31, 2026, to support the GEMx mineral mapping campaign. NASA/Carla Thomas Since 2023, GEMx flights have covered more than 386,000 square miles (1 million square kilometers) of American soil, including most of California. Ground-truthing the sensor data can entail hot field work, scrambling over steep crags to uncover samples for lab analysis. While testing has confirmed the topaz discovery, determining if the Mojave site overlies a porphyry copper deposit will require intensive investigation using ground-penetrating equipment. But the AVIRIS finding shows how advanced NASA airborne sensing can help lead geologists to the metaphorical needle in a haystack, even in heavily explored Southern California. “People have been prospecting this area for generations,” said Erik Tharalson, a USGS geologist. “But there’s a lot more to discover.” High flyer From the beginning, the GEMx mineral mapping campaign has been enabled by one of the highest-flying aircraft in NASA’s fleet: the ER‑2 . It deployed on March 31 from NASA’s Armstrong Flight Research Center in Edwards, California, to Colorado Springs Airport in Colorado. “We deployed to Colorado Springs to maximize flight time for data collection needed in Colorado, Utah, New Mexico, Arizona, and Texas,” said John McGrath, ER‑2 project manager at NASA Armstrong. By the conclusion of this deployment on June 5, the aircraft had completed 26 flights totaling more than 125 hours. Soaring at about 65,000 feet, the ER-2 can fly at high altitudes that allow it to collect broad‑area, high‑resolution spectral measurements in a single pass, supporting researchers studying mineral composition and surface processes. In 2025, the aircraft flew 36 science missions, collecting more than 7 billion measurements over 200 flight hours. The data has contributed to the largest airborne surface mineralogy dataset gathered in a single NASA-USGS campaign. The GEMx survey is led and funded by the USGS Earth Mapping Resources Initiative . Earth MRI is modernizing mapping the nation’s surface and subsurface to find new, critical, and other minerals. It is a partnership effort with 45 state geological surveys, federal agencies, private industry, tribes, universities, and others. The initiative will capitalize on both the technology developed by NASA for spectroscopic imaging, as well as the USGS expertise in analyzing the datasets, conducting field work, and deriving critical mineral information from them. To learn more about GEMx visit: https://science.nasa.gov/mission/gemx/ Media Contacts Andrew Wang / Andrew Good Jet Propulsion Laboratory, Pasadena, Calif. 626-379-6874 / 818-393-2433 [email protected] / [email protected] Written by Sally Younger 2026-037 Explore More 6 min read Air Pollution’s Daily Pulse Over the Northeast The TEMPO mission helped scientists track morning nitrogen dioxide that contributed to afternoon ozone along… Article 17 hours ago 2 min read NASA, NOAA to Hold Joint Session at 23rd Symposium on Operational Environmental Satellite Systems Abstracts are now being accepted for the session, which will take place at the 2027… Article 1 day ago 9 min read Jim Irons, Former Landsat Project Scientist, Wins Pecora Award Landsat’s Jim Irons won the prestigious William T. Pecora Award. Irons, now an emeritus scientist at… Article 1 day ago Keep Exploring Discover More Topics From NASA GEMx Armstrong Flight Research Center Jet Propulsion Laboratory Earth Science – Technology

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NASA to Preview Katalyst Mission to Boost Swift Spacecraft’s Orbit
Science & Space
3 min read

NASA to Preview Katalyst Mission to Boost Swift Spacecraft’s Orbit

Katalyst Space’s LINK robotic servicing satellite awaits encapsulation inside a Northrop Grumman Pegasus XL on June 8, 2026, at NASA’s Wallops Flight Facility in Virginia. The rocket will carry LINK to space for an attempted orbital boost of NASA’s Neil Gehrels Swift Observatory. Credit: NASA/Ron Beard NASA will host an audio-only media teleconference at 11 a.m. EDT, Wednesday, June 17, to preview the Katalyst Space mission to boost the orbit of NASA’s Neil Gehrels Swift Observatory. Katalyst’s robotic servicing spacecraft, called LINK, will attempt to rendezvous with Swift and raise its altitude, extending its science mission lifespan and advancing a key capability for the future of space exploration. The LINK spacecraft will launch on Northrop Grumman’s Pegasus XL rocket later this month from Kwajalein Atoll in the Marshall Islands. Media interested in participating by phone must RSVP no later than two hours before the start of the call to Amy Barra at: [email protected] . NASA’s media accreditation policy is available online. Audio of the media teleconference will stream on the agency’s website at: https://www.nasa.gov/live Participants in the media teleconference include: Shawn Domagal-Goldman, division director, Astrophysics, NASA Headquarters in Washington Brad Cenko, principal investigator, Swift, NASA’s Goddard Space Flight Center in Greenbelt, Maryland Kieran Wilson, principal investigator, LINK, Katalyst Space Robert Lamontagne, vice president, strategic partnerships, Katalyst Space Wes Collier, vice president, launch systems, Northrop Grumman The Swift mission, which launched in 2004, leads NASA’s fleet of telescopes in studying changes in the high-energy universe, like gamma-ray bursts, which are the most powerful explosions in the cosmos. When a rapid, sudden event takes place in the sky, Swift serves as a “dispatcher,” providing critical information that allows other “first responder” missions to follow up to learn more about how the universe works. After 21 years, Swift’s low Earth orbit has begun to rapidly decay because of increased solar activity. Rather than allowing the observatory to re-enter Earth’s atmosphere, as many missions do at the end of their lifetimes, NASA is using this opportunity to advance U.S. spacecraft servicing technology. In September 2025, NASA awarded a contract to Katalyst to mount a robotic servicing mission for Swift in less than a year. The mission will use LINK to rendezvous with Swift and boost it to a higher altitude, demonstrating a key capability for the future of space exploration. The mission is targeted for launch in June from Kwajalein Atoll, Marshall Islands. Learn more about the mission to boost Swift’s orbit at: https://science.nasa.gov/mission/swift/swift-boost-mission/ -end- Karen Fox / Alise Fisher Headquarters, Washington 202-385-1287 / 202-358-2546 [email protected] / [email protected] Amy Barra Wallops Flight Facility, Wallops Island, Va. 757-824-1579 [email protected] Share Details Last Updated Jun 11, 2026 Editor Jessica Taveau Location NASA Headquarters Related Terms Swift Boost Mission Astrophysics Division Goddard Space Flight Center Neil Gehrels Swift Observatory Science Mission Directorate

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Air Pollution’s Daily Pulse Over the Northeast
Science & Space
10 min read

Air Pollution’s Daily Pulse Over the Northeast

Earth Observatory Science Earth Observatory Air Pollution’s Daily Pulse… Earth Earth Observatory Image of the Day EO Explorer Topics All Topics Atmosphere Land Heat & Radiation Life on Earth Human Dimensions Natural Events Oceans Remote Sensing Technology Snow & Ice Water More Content Collections Global Maps World of Change Articles Earth Matters Blog Blue Marble: Next Generation EO Kids Mission: Biomes About About Us Subscribe 🛜 RSS Contact Us Search 7:05 am 3:05 pm TEMPO detected high concentrations of nitrogen dioxide during the morning commute at 7:05 a.m. local time on May 18, 2026 (left), along the New York-Washington corridor. The instrument detected lower levels of the gas at 3:05 p.m. (right), after chemical reactions involving nitrogen dioxide had contributed to elevated ozone concentrations in the afternoon. NASA Earth Observatory/Michala Garrison TEMPO detected high concentrations of nitrogen dioxide during the morning commute at 7:05 a.m. local time on May 18, 2026 (left), along the New York-Washington corridor. The instrument detected lower levels of the gas at 3:05 p.m. (right), after chemical reactions involving nitrogen dioxide had contributed to elevated ozone concentrations in the afternoon. NASA Earth Observatory/Michala Garrison 7:05 am 3:05 pm TEMPO detected high concentrations of nitrogen dioxide during the morning commute at 7:05 a.m. local time on May 18, 2026 (left), along the New York-Washington corridor. The instrument detected lower levels of the gas at 3:05 p.m. (right), after chemical reactions involving nitrogen dioxide had contributed to elevated ozone concentrations in the afternoon. NASA Earth Observatory/Michala Garrison TEMPO detected high concentrations of nitrogen dioxide during the morning commute at 7:05 a.m. local time on May 18, 2026 (left), along the New York-Washington corridor. The instrument detected lower levels of the gas at 3:05 p.m. (right), after chemical reactions involving nitrogen dioxide had contributed to elevated ozone concentrations in the afternoon. NASA Earth Observatory/Michala Garrison 7:05 am 3:05 pm Curtain Toggle 2-Up Image Details TEMPO detected high concentrations of nitrogen dioxide during the morning commute at 7:05 a.m. local time on May 18, 2026 (left) , along the New York-Washington corridor.The instrument detected lower levels of the gas at 3:05 p.m. EDT (right), after chemical reactions involving nitrogen dioxide had contributed to elevated ozone concentrations in the afternoon. NASA Earth Observatory images by Michala Garrison. More than 35 million people live along the New York–Washington corridor and breathe the region’s air. While air quality has improved significantly in recent decades, outbreaks of ground-level ozone remain common, particularly in the warm summer months, when the chemical reactions that produce the pollutant accelerate and stagnant air allows ozone to accumulate. A reminder of this seasonal phenomenon came earlier than usual in 2026, when a mid-May heat wave prompted the New York State Department of Health and the New York Department of Environmental Conservation to issue a health advisory on May 17 over concerns about ozone. The code orange advisory warned young people, older adults, and those working or exercising outdoors to limit activity due to ozone’s respiratory and cardiovascular health impacts. As expected, ground-based air-quality sensors operated by state and federal agencies showed ozone reaching unhealthy levels for sensitive groups on May 18, something that typically happens several times per year . Meanwhile, NASA’s TEMPO (Tropospheric Emissions: Monitoring of Pollution) instrument observed the event from geostationary orbit 22,000 miles (35,000 kilometers) above the equator, a unique vantage point that allows the sensor to collect frequent observations of air pollution. TEMPO detects nitrogen dioxide (NO 2 ), a gas emitted by burning fuels, particularly by motor vehicles, that contributes to ozone formation. “There’s often a clear and interesting pattern in TEMPO’s nitrogen dioxide data during ozone alert days,” said Hazem Mahmoud, an atmospheric scientist at NASA’s Atmospheric Science Data Center at Langley Research Center. “We see high concentrations of nitrogen dioxide during the early morning commute that drop off sharply in the late afternoon as ozone increases.” The decline occurs as sunlight fuels photochemical reactions involving nitrogen dioxide, volatile organic compounds , and oxygen that lead to ozone formation. By late afternoon, these reactions deplete much of the available nitrogen dioxide, slowing ozone production until the cycle begins again the next day. The pair of images above underscores the pattern. The image on the left was acquired at 7:05 a.m. local time when nitrogen dioxide concentrations were high during the morning commute. By 3:05 p.m. (right), most of the nitrogen dioxide had declined substantially, and surface ozone levels were elevated (below). Meanwhile, afternoon sea breezes appear to have transported the remaining nitrogen dioxide slightly to the west. Note that the data shown is provisional , and processing methods are still being refined. Sensors on earlier polar-orbiting satellites, such as OMI (Ozone Monitoring Instrument) and TROPOMI (Tropospheric Monitoring Instrument), sampled nitrogen dioxide over New York once per day. After its launch in 2023, TEMPO began providing data every hour, allowing researchers to track the evolution and dispersion of air pollution at much finer time scales. “TEMPO is helping fill data gaps between ground stations and allowing us to ask new questions,” Mahmoud said. The mission provides data that can improve not only air quality forecasts during crisis situations, such as wildfires, but also the atmospheric models used to forecast the daily rhythms of urban pollution. Such models help researchers understand how natural factors such as winds, humidity levels, and air temperatures influence pollution plumes over the course of a day. TEMPO detected elevated ozone concentrations in an area extending from New York City to Washington, D.C., at 5:05 p.m. on May 18, 2026. NASA Earth Observatory/Michala Garrison TEMPO also detects ozone directly, but determining how much of that ozone is near the surface versus higher in the atmosphere can be challenging. Most of Earth’s ozone resides in the stratosphere , well above the troposphere, where people live and breathe. At times, however, stratospheric ozone can be transported downward into the troposphere. During events known as stratospheric intrusions , it can even descend far enough to affect air quality at the surface and add to the ozone produced at ground level. By combining TEMPO observations with other sources of information , researchers are studying the processes that influence the distribution of ozone vertically in the atmosphere. On May 18, NASA’s ground-based tropospheric lidar network (TOLNet) in New York City recorded high concentrations of ozone near the surface, indicating that TEMPO was detecting mostly surface-level ozone associated with urban emissions and not ozone aloft, said Mahmoud. However, on May 19, the same sensor observed a layer of ozone descending from above 5 kilometers (3 miles), he added, a clue that some of the ozone TEMPO detected that day may have originated in the stratosphere. “This is the type of information that leads to better air quality forecast models and more accurate alerts,” Mahmoud said. “Alerts can affect tens of millions of people and lead to disruptions in school, sports, and other activities, so it’s essential that they be as accurate as possible.” On June 6, New York authorities issued another health advisory for ozone. People interested in following the event can access daily near-real-time TEMPO observations of ozone, nitrogen dioxide, and other gases on NASA’s Worldview browser , on an interactive Harvard & Smithsonian Center for Astrophysics browsing tool , and on NASA’s Earthdata portal . NASA Earth Observatory images by Michala Garrison, using TEMPO data from NASA Earthdata . Story by Adam Voiland. Downloads Nitrogen Dioxide – May 18, 2026 7:05 AM EDT JPEG (2.52 MB) Nitrogen Dioxide – May 18, 2026 3:05 PM EDT JPEG (2.25 MB) Ozone – May 18, 2026 5:05 PM EDT JPEG (2.10 MB) References & Resources Acker, S., et al. (2025) Satellite detection of NO 2 distributions using TROPOMI and TEMPO and comparison with ground-based concentration measurements . Atmospheric Chemistry and Physics, 25(14), 8271-8288. City of New York (2024) Community Air Survey Report: 2008-2024 . Accessed June 9, 2026. Energy Education, Ozone . Accessed June 10, 2026. Environmental Protection Agency (2026, May 13) What is Ozone ? Accessed June 9, 2026. Environmental Protection Agency (2025, July 10) Basic Information about NO 2 . Accessed June 9, 2026. Holloway, T., et al. (2025) Satellite data to support air quality assessment and management . Journal of the Air & Waste Management Association , 75(6), 429-463. Lee, J., et al. (2024) The Evolutions and Large-Scale Mechanisms of Summer Stratospheric Ozone Intrusion Across Global Hotspots . JGR Atmospheres, 129(4),e2023JD039877. NASA (2026) TOLNet . Accessed June 9, 2026. NASA Air Quality (AQ) Monitoring from Space by NASA using TEMPO . Accessed June 9, 2026 NASA Air Quality (2026) Nitrogen Dioxide . Accessed June 9, 2026. NASA Air Quality (2026) Nitrogen Dioxide Trends for US Cities . Accessed June 9, 2026. NASA Earthdata (2024, May 3) TEMPO Mission Releases Beta Level 1, 2, and 3 Version 03 Data Products . Accessed June 9, 2026. New York State Department of Environmental Conservation (2026, May 18) Air Quality Health Advisory Extended for New York City Metro Region . Accessed June 9, 2026. Zhang, J., et al. (2026) Revealing the Formation and Control of NYC Downwind Coastal High Ozone via New TEMPO Observations . Geophysical Research Letters, 53(2),e2025GL117523. You may also be interested in: Stay up-to-date with the latest content from NASA as we explore the universe and discover more about our home planet. Smoke Shrouds Northern Thailand 3 min read Seasonal fires have darkened skies over Southeast Asia. Article Winter’s End Is Written in the Clouds 3 min read As winter turned to spring, the skies over the Gulf of Alaska displayed textbook examples of numerous cloud formations. Article Extreme January Cold 3 min read Following a significant winter storm, frigid temperatures lingered in late January 2026 across a vast swath of the U.S. Article 1 2 3 4 Next Keep Exploring Discover More from NASA Earth Science Subscribe to Earth Observatory Newsletters Subscribe to the Earth Observatory and get the Earth in your inbox. Earth Observatory Image of the Day NASA’s Earth Observatory brings you the Earth, every day, with in-depth stories and stunning imagery. Explore Earth Science Earth Science Data Open access to NASA’s archive of Earth science data

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Curiosity Blog: Sols 4913-4919: Planetary explorers, freewheeling to the Yardang unit!
Science & Space
5 min read

Curiosity Blog: Sols 4913-4919: Planetary explorers, freewheeling to the Yardang unit!

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 Perseverance Rover Mars Curiosity Rover Mars Reconnaissance Orbiter Mars Odyssey More Mars Missions Mars Home 3 min read Curiosity Blog: Sols 4913-4919: Planetary explorers, freewheeling to the Yardang unit! Navcam image from sol 4916 showing the rough drive direction. The yardang unit can be seen as a series of pale coloured hills in the centre of the image, at the very back. NASA/JPL-Caltech Written by Catherine O’Connell-Cooper, APXS Strategic Planner and Payload Uplink/Downlink Lead, University of New Brunswick, Canada Earth planning day: Friday, June 5th, 2026 In a very broad sense, Curiosity has two modes of doing science – one centred around a defined science campaign (such as the recent boxwork campaign) and the other as we move between campaigns. During a science campaign, with a very defined start and end location, every image and every workspace is carefully choregraphed to make sure we hit all of our science goals for the campaign. This is a lot of pressure! But in between campaigns, the emphasis moves to driving towards the next major campaign. Our next major stop is the yardang unit, a series of intriguing wind sculpted, pale coloured hills which you can just see in the distance in the cover image for this blog . The rover planners (RPs) sometimes make our drives as long as they can and we drive as far as we can go, other times we stop a little short to look at interesting looking workspaces as we go. As part of the APXS team, I loved being part of the boxwork campaign and getting all the information we needed there … but as a geologist, there is something very special about this kind of exploring, the sense of being a planetary explorer, ambling along to see what the rocks will show us. So we continue southwards, trundling over laminated bedrock which varies from predominantly pale coloured laminated bedrock to bands with abundant thin flaky, darker coloured, layers and patches. Some of the rocks stick out at strange angles, which make planning drives more challenging. This past week there has been abundant dark layers interbedded with the more dominant pale coloured rock, both in place and in fragments around the workspace. APXS and MAHLI characterized some of this darker material, for example at “ Rio Bio Bio ” and “ Placilla de Caracoles ” and some of the paler material at the brushed targets “ La Primavera ” and “ Los Quemados .” ChemCam also analyzed both types of rocks along the way. We are busily acquiring Mastcam and ChemCam LD-RMI (“Long Distance Remote Micro Imager”) images of everything even remotely interesting – and there are lots and lots of cool features around here. The wide open landscape here allows us to image features from several different angles and distances, such as “Mira Flores,” a small erosional outlier seen from a distance in this image and closer up here . Another great example is the “Kimsa Chata” trough which shows some amazing sedimentary structures, which may help us to determine if this was a desert or a lake or maybe something in between, such as a desert with some water moving through. The Environmental Theme Group continues to populate each plan with environmental monitoring activities. Activities varied from dust devil monitoring in Gale crater to looking at levels of dust in the skies overhead. The weekend drive is planned to take us further into that drive distance shown in the cover image, to an area where the contrast between dark and light bedrock is more pronounced, and just beyond that, to an area which looks very smooth, with no jutting out blocks. From where we sit today, its impossible to say what it is but that is the fun of exploring – who knows what we will find? Stay tuned to find out over the coming weeks. Want to read more posts from the Curiosity team? Visit Mission Updates Want to learn more about Curiosity’s science instruments? Visit the Science Instruments page NASA’s Curiosity rover at the base of Mount Sharp NASA/JPL-Caltech/MSSS Share Details Last Updated Jun 10, 2026 Related Terms Blogs Explore More 5 min read Curiosity Blog, Sols 4908-4912: Goodbye Campo Marte, It’s Been Fun! Article 7 days ago 3 min read Curiosity Blog, Sols 4900-4907: Pasadena, We Have a Drill Sample! Article 2 weeks ago 3 min read Curiosity Blog, Sols 4893-4899: Drilling at Campo Marte and a Visit From the Psyche Spacecraft Article 3 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…

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NASA Awards Contract for Construction Services in California
Science & Space
2 min read

NASA Awards Contract for Construction Services in California

Credit: NASA NASA has selected multiple small businesses for the Western Regional Multiple Award Construction Contract, which supports a broad range of facility enhancement, modernization, and sustainment work at NASA’s Armstrong Flight Research Center in Edwards, California, NASA’s Ames Research Center in California’s Silicon Valley, and other federal agencies in the region. The contract provides general construction, modification, maintenance and repair, and demolition services, as well as new construction of buildings and facilities that incorporate Leadership in Energy and Environmental Design practices and building information modeling to support efficient and sustainable project execution. The indefinite-delivery/indefinite-quantity, firm-fixed-price contract is a follow-on to the agency’s previous regional construction contract and has a potential value of $450 million over a five‑year period. Contract awardees are: Abide International Inc. Able Heating and Air Conditioning Anderson Burton Construction Inc. Anna Lisa Luna Construction Barkley Andross Corporation Bibro Construction Company Inc. CM Construction Services CMS Construction Inc. FASONE G‑1 Lead Builders JV LLC Gideon USA Good‑men Roofing & Construction Inc. Groundlevel Construction Inc. IPI Construction Inc. Innovative Project Solutions Inc. Ironwood Commercial Builders Inc. J.I. Garcia Construction Inc. JG Contracting Lead Builders Inc. Martinez Construction Services MX Construction Inc. OCS Construction Services Inc. Patricia I. Romero Inc., doing business as Pacific West Builders Gustav Keoni, doing business as Precision Construction Prime MIK JV LLC Spectrum Builders and Renovations Inc. Sea Pac Engineering Inc. Sergent Construction Souza Construction Inc. TLI Construction Inc. For more information about NASA and agency programs, visit: https://www.nasa.gov -end- Jennifer Dooren / Jessica Taveau Headquarters, Washington 202-358-1600 [email protected] / [email protected] Dede Dinius Armstrong Flight Research Center, Edwards, Calif. 661-276-5701 [email protected] Share Details Last Updated Jun 10, 2026 Editor Jessica Taveau Location NASA Headquarters Related Terms Armstrong Flight Research Center Ames Research Center NASA Centers & Facilities

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NASA, NOAA to Hold Joint Session at 23rd Symposium on Operational Environmental Satellite Systems
Science & Space
2 min read

NASA, NOAA to Hold Joint Session at 23rd Symposium on Operational Environmental Satellite Systems

CSDA Menu CSDA Commercial Data Available Datasets End User License Agreements Commercial Satellite Data Explorer Satellite Data Evaluation CSDA Vendors Airbus BlackSky Capella GeoOptics GHGSat ICEYE MDA Space Pixxel Planet PlanetiQ Polar Geospatial Center Satellogic Spire Teledyne Brown Engineering Tomorrow.io Umbra Vantor Program Activities Learning Resources FAQs News News and Events Subscribe to CSDA Orbit Credit: AMS Submit your abstract for “Advancing Weather and Environmental Science Through NASA and NOAA Commercial Satellite Data Programs,” a joint session hosted by NASA’s Commercial Satellite Data Acquisition (CSDA) program, in partnership with the NOAA National Environmental Satellite, Data, and Information Service (NESDIS) Commercial Data Program (CDP). The session is part of the 23rd Symposium on Operational Environmental Satellite Systems, which will take place at the 2027 American Meteorological Society (AMS) Annual Meeting January 10-14 in Denver, Colorado. It will examine the growing capabilities of commercial Earth observation providers that are creating new opportunities to advance weather research, operational forecasting, and environmental science applications. NASA’s CSDA program and NESDIS’s CDP collaborate to expand federal access to commercial satellite data and accelerate its use in both research and operational applications. The CSDA program supports the scientific community by evaluating and acquiring diverse commercial datasets, including optical, Synthetic Aperture Radar, Global Navigation Satellite System Radio Occultation and Reflectometry, methane, precipitation, and Digital Elevation/Terrain Models for modeling, hazard monitoring, climate studies, and applied research. Similarly, the CDP operationalizes commercial space-based environmental data, with demonstrated impacts from assimilated observations in weather forecasting and space weather applications. It also conducts pilot projects and transitions the piloted data to operations. Together, the CSDA and CDP strengthen the nation’s weather enterprise by enabling innovative research, closing observational gaps, and integrating commercial data into real-world forecasting and decision support applications. To submit an abstract or for additional information about the abstract submission process, visit the symposium’s website.

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ILC_LVHO05A - "Dataset: updated structure and data"
Data & Statistics
1 min read

ILC_LVHO05A - "Dataset: updated structure and data"

Overcrowding rate by age, sex and poverty status - total population

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SDG_06_10 - "Dataset: updated structure"
Technology
1 min read

SDG_06_10 - "Dataset: updated structure"

Population having neither a bath, nor a shower, nor indoor flushing toilet in their household by poverty status

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ILC_LVHO02 - "Dataset: updated structure and data"
Data & Statistics
1 min read

ILC_LVHO02 - "Dataset: updated structure and data"

Distribution of population by tenure status, type of household and income group

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ILC_DI15 - "Dataset: updated structure and data"
Data & Statistics
1 min read

ILC_DI15 - "Dataset: updated structure and data"

Mean and median income by group of citizenship (population aged 18 and over)

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ILC_MDHO01 - "Dataset: updated structure"
Data & Statistics
1 min read

ILC_MDHO01 - "Dataset: updated structure"

Total population living in a dwelling with a leaking roof, damp walls, floors or foundation, or rot in window frames or floor

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NASA Equips Astronauts, Industry with Robotic Intelligence 
Science & Space
3 min read

NASA Equips Astronauts, Industry with Robotic Intelligence 

2 min read Preparations for Next Moonwalk Simulations Underway (and Underwater) In the Integrated Mobile Evaluation Testbed for Robotics Operations facility at Johnson Space Center, PickNik robotic control software proved its prowess in tasks like passing cargo transfer bags through a hatch and placing them in storage bins, in anticipation of work NASA would like robots to carry out during the later Artemis missions. Credit: NASA As NASA plans long-term missions on the Moon, the agency could use robots to perform routine tasks, allowing crew members to dedicate more time to science and exploration. However, robotic motion control requires complex technology and advances in features like robotic decision-making and object recognition. These are the challenges a Boulder, Colorado-based robotics company is teaming up with NASA to overcome.  PickNik Inc. recently worked with Shaun Azimi, who leads the Dexterous Robotics team at NASA’s Johnson Space Center in Houston, and other agency roboticists. The team tested software that enabled a robotic arm to recognize a spacecraft hatch, then turn the latch, grasp the handle, and open the door. The arm then was able to transfer cargo bags between the hatch and a bin.  The work was carried out in NASA Johnson’s new Integrated Mobile Evaluation Testbed for Robotics Operations with funding from NASA’s Small Business Innovation Research program.  PickNik designed and refined the robotic software, called MoveIt Pro, with support from early government investments. Commercially released in 2023, MoveIt Pro has found a significant customer base.  Automotive company BMW is using the software on its robotic assembly lines. A company called Lightspeed is using MoveIt Pro to program huge robotic arms that build modular “panels” for constructing affordable housing. Another company, known as Hivebotics, used MoveIt Pro to automate its flagship product, a cleaning robot. Ezra Brooks, principal software engineer at PickNik, said the 35-person company might not have a product without NASA’s early support. Robotic software requires years of research and development to refine algorithms and create a commercial product. NASA enabled much of that foundational work.  NASA’s technological advancements unlock key capabilities for missions at the Moon and beyond while benefiting commercial industries on Earth. For 50 years, NASA has documented the everyday benefits of space technology through the agency’s Spinoff publication. To learn more about the project, visit:  https://go.nasa.gov/49CNSi7 Read More Share Details Last Updated Jun 10, 2026 Related Terms Technology Transfer & Spinoffs Spinoffs Technology Transfer Explore More 3 min read NASA-Supported Space Tech Advances Earthly Construction Article 4 weeks ago 4 min read Hello Universe: NASA’s Next-Gen Space Processor Undergoes Testing Article 4 weeks ago 3 min read NASA Heat Shield Technology Enables Space Industry Growth Article 4 months ago Keep Exploring Discover Related Topics Technology Transfer & Spinoffs Artemis Robotics Johnson Space Center

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