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4 min read

By Susanne P. Schwenzer, Professor of Planetary Mineralogy at The Open University, UK
Earth planning date: Thursday, June 18, 2026
In the area Curiosity is currently exploring, the science team has mapped several areas with different-looking surface texture on the orbital images. If you wanted to have a look yourself at what there is to see, check the “Where is Curiosity?” map. You’ll discover different shades of orange and beige as well as more rough and more smooth-looking textures. This is what the geomorphologists in our team use to map the areas for exploration by the rover. Of course, we then supplement this all with ground-based images, including bespoke “drive direction imaging,” which is taken after each drive by the Mast Camera. Drive planning is done using a combination of all this information. So there shouldn’t be any surprises, right?
On Monday the team planned three sols in preparation for a Thursday planning to account for the U.S. federal holiday weekend. The workspace turned out to be a little spiky, so we could not find an area we could DRT. APXS still found one good bedrock target, “Rio Baker,” which also had MAHLI documentation. In addition, ChemCam investigated “Rica Aventura,” a textured bedrock, and “Tabebuia,” a darker-looking individual block, using its LIBS and conducted a passive spectral observation on a second dark float block called “Lago Ranco.” Of course, the team also wanted to look into the distance with ChemCam remote imaging, extending our investigation of the Cordillera base outcrop.
Imaging is always high on the list. In Monday’s plan Mastcam is looking into the modern dunes with the “Tacaza” mosaic, and with more mosaics looking forward to the future parking areas, some of which looked really smooth from that vantage point. We also continue our environmental and atmospheric observations looking for dust devils, the opacity of the atmosphere, and monitoring pressure and temperature. After all this, the rover drove about 35 meters (about 115 feet) to an area that looked really smooth in all images we had available at that point. So we were hoping for a good spot to deploy the DRT, but didn’t think we could be in for a surprise.
The drive ended exactly as planned, spot-on in the middle of that — from a distance — smooth-looking area. But when we opened the post-drive images on Thursday morning, we were all reacting with a lot of surprise. From up close, the parking spot looks anything but smooth. You can see the surprise in the title image of this blog. There are polygons, veins, lamination, and probably more, once we inspect the higher-resolution images taken today. “Higher-resolution” is the key for why we were in for such a surprise! The features are quite small, a few centimeters across, and therefore we could not see them in the orbital images or from a distance in our navigation and mast camera images. The camera resolution from a distance just isn’t enough to see them. But up close, the terrain revealed all its beauty! And I am sure there will be more in the even higher resolution of today’s MAHLI and ChemCam RMI imager images!
So, what did we plan after we caught our breath on Thursday? First, you guessed it, images, images, and more images. Mastcam takes a full panorama with its “left eye” and adds a range of closer-up mosaics with its higher-resolution “right eye.” In addition there is a ChemCam Remote Micro Imager image to document structures further afield at high resolution. ChemCam is investigating three targets using LIBS: “Rio Chimore” is a lighter-toned band; you can see some of those in the cover image of this blog, too. The other two LIBS targets are “Rio de Lava,” a vein target, and “Rio de Salta,” one of the polygons. APXS is also looking at the bedrock and the ridges, at the targets “Pampa Grande” and “Iquique Ridge.” MAHLI is having the above-mentioned close “hand lens” look. Let’s see what we will discover when we get those images.
Finally, Curiosity drove up the hill along very smooth-looking terrain that is just littered with tiny polygons. Let’s see if we are in for another surprise reverberating around all our offices — and across two continents, as I had the good fortune to be among the first ones, here in England (Or maybe it was our French ChemCam colleagues, who are in a time zone one hour ahead of me?). Whichever it is, this terrain has a lot to say about the geologic history of Mars!

2026-06-24 04:01
In preparing to visit the Moon’s surface, soon-to-be lunar explorers in NASA’s Apollo program first ventured into a variety of unfamiliar landscapes on Earth. A couple of these trips, in the summers of 1965 and 1966, took astronauts to Alaska’s remote Katmai National Park for simulations of field geology in Moon-like environments.
In one exercise, which they called “playing the Moon game,” pairs of astronauts were placed at unfamiliar field sites and asked to pretend as if they were on the Moon. By the account of William Phinney, Apollo’s science training coordinator, they were tasked with collecting representative geologic samples and practicing how to communicate their observations to scientists.
The Alaskan setting for the Moon game was an unusual volcanic landscape called the Valley of Ten Thousand Smokes. The valley is full of debris deposited by the 1912 eruption of Novarupta—the largest volcanic event on Earth in the 20th century.
The images above, acquired on September 29, 2025, with the OLI (Operational Land Imager) on Landsat 9, show the massive ash flow deposited by Novarupta. The layer measures up to 660 feet (200 meters) thick and was emplaced at a searing 1,380 degrees Fahrenheit (750 degrees Celsius).
The Valley of Ten Thousand Smokes, shown in the 1917 photo below, is so named because of the abundance of fumaroles—gas and steam-emitting vents—that filled the valley for a decade after the eruption. A few hundred persisted more than 10 years, with some lasting until the 1990s.
Scientists initially suspected that the monster eruption occurred at Mount Katmai, a neighboring volcano with a large caldera located 6 miles (10 kilometers) east of Novarupta’s dome. However, they later determined that the eruption actually occurred at Novarupta—whose name means “new eruption”—after stealing magma from beneath Katmai. As the magma chamber emptied, Katmai collapsed, forming the 2.5-mile-wide (4-kilometer-wide) caldera present today.
The volcanic landscape in the Valley of Ten Thousand Smokes is far fresher than the ancient lava flows that formed the Moon’s volcanic features. But for the Apollo astronauts, it offered an “excellent opportunity to view volcanic materials and landforms in nearly pristine condition,” Phinney wrote. They studied evidence of fumaroles and examined vertical sections of the deposits where streams had eroded deep gorges.
Researchers continue to visit this Alaskan wilderness in search of clues that could help decipher the geology of the Moon and Mars. In 2024, the Goddard Instrument Field Team (GIFT) trekked to the Valley of Ten Thousand Smokes to study its icy volcanic landscape. Like the valley, Mars contains glaciers and ice sheets layered with dust and ash, a dynamic and difficult-to-interpret environment.
Advancing lunar science, the GIFT team also collected samples from rock formations comparable to the Moon’s Gruithuisen Domes. These mysterious features are made of hardened lava with a different composition than the surrounding rock. With more to learn about our nearest celestial neighbor, the spirit of the Moon game lives on in the 21st century.
NASA Earth Observatory images by Lauren Dauphin, using Landsat data from the U.S. Geological Survey. Photos from National Geographic Society Katmai expeditions photographs, Archives and Special Collections, Consortium Library, University of Alaska Anchorage, and from the U.S. Geological Survey Volcano Hazards Program. Story by Lindsey Doermann.
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2026-06-23 21:32
NASA has selected Sean Gallagher as the agency’s chief information officer (CIO). In this role, he is responsible for the agency’s entire portfolio of Information Technology products and services. Gallagher has been serving in an acting capacity since January and his permanent role is effective immediately.
“Sean Gallagher’s leadership has been instrumental in strengthening NASA’s IT foundation and ensuring our workforce has the secure, modern tools needed to enable groundbreaking missions every day,” said NASA Deputy Administrator Matt Anderson. “As CIO, Sean will continue advancing the agency’s technology capabilities to support discovery, innovation, and mission success across NASA.”
Most recently, Gallagher also has served as the deputy chief information officer for Operations in the Office of the Chief Information Officer at NASA Headquarters in Washington, as well as a senior advisor for Transformation. This team provides services to tens of thousands of end users located in the U.S. and abroad in support of NASA missions, enabling discoveries, faster data sharing, increased workforce productivity, and more. Gallagher has worked with all NASA centers to implement efficient and effective IT operating models.
Previously, Gallagher was the CIO of NASA’s Glenn Research Center in Cleveland, leading IT initiatives for aeronautics, space, research and engineering, and test missions. He joined NASA in 2012 as Glenn’s deputy CIO and previously worked at Booz Allen Hamilton as a senior associate supporting a variety of federal, defense, and commercial customers.
Gallagher developed his leadership and management experience as a Signal Corps officer in the United States Army. He also served as a platoon leader managing the combat service support readiness of a tactical communications unit, a human resource manager for the 40th Signal Battalion, and as a network engineer for the 11th Signal Brigade. He has a bachelor’s degree in physics from John Carroll University and a master’s degree in computer information systems from the University of Phoenix.
For more information about NASA’s missions, visit:
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Camille Gallo / Cheryl Warner
Headquarters, Washington
202-358-1600
camille.m.gallo@nasa.gov / cheryl.m.warner@nasa.gov
2026-06-23 18:57
NASA’s Commercial Satellite Data Acquisition program (CSDA) announced contract awards with eight commercial satellite data providers offering a range of data types to support the agency’s Earth science research and application goals.
The CSDA program On-Ramp 2 Multiple Award contract is a firm-fixed-price indefinite-delivery/indefinite-quantity (IDIQ) multiple-award contract with a maximum cumulative value of $476 million and a performance period through November 2028.
The CSDA IDIQ contract includes an on‑ramp provision that allows NASA to periodically reopen the solicitation, giving new vendors the opportunity to submit proposals. This mechanism also enables existing CSDA vendors to propose new data products, whether newly developed or derived from new instruments, that were not available during the original proposal period.
Newly Added Contract Holders
| Vendor | Sensor |
| HydroSat | Thermal Infrared Visible and Near-Infrared (VNIR) |
| Ororatech | Thermal Infrared – Medium Wavelength Infrared (MWIR) and Long Wavelength Infrared (LWIR) |
| ImageSat | Optical Multispectral Instrument (MSI) |
| Satlantis | Optical MSI / Greenhouse Gas (GHG) Emissions |
| Kuva Space | Hyperspectral – VNIR and Short Wavelength Infrared (SWIR) |
| Wyvern | Hyperspectral – VNIR |
| Orbital Sidekick | Hyperspectral – VNIR and SWIR |
| Muon Space | Global Navigation Satellite System – Radar (GNSS-R) |
Current CSDA Contract Holders with New Products
| Vendor | Sensor |
| Airbus | Optical MSI / Synthetic Aperture Radar (SAR) |
| ICEYE | SAR |
| GHGSat | GHG Emissions |
| Planet Labs | Optical MSI / Hyperspectral |
| PlanetiQ | Global Navigation Satellite System – Radio Occultation (GNSS-RO) |
| Tomorrow.io | Microwave Sounder |
“NASA’s Earth science community relies on a diverse suite of observations from spaceborne, airborne, and in situ assets to better understand our changing planet,” said CSDA Project Manager Dana Ostrenga. “The commercial providers added through this latest CSDA contract on-ramp complement NASA’s existing Earth observation capabilities and our current portfolio of commercial partners, expanding the range of data available for evaluation and use. Together, these observations provide researchers with a more comprehensive view of Earth’s atmosphere, land, oceans, cryosphere, and solid Earth, helping advance scientific discovery and applications that benefit our communities.”
Following issuance of the contract awards, the selected vendors’ data products will be made available to authorized CSDA data users via the Satellite Data Explorer (SDX), CSDA’s web-based data discovery and data access tool that allows approved users to search, discover, access, task, and download the data the program has acquired from its commercial partners.
The award process begins with the CSDA issuing a request for proposals that is posted on Sam.gov, the U.S. government’s official system for managing federal contract proposals. Interested companies then submit proposals to enter into an IDIQ contract with CSDA. A Solicitation Evaluation Board is formed to determine whether the proposals are competitive and meet the CSDA’s technical requirements for continuous observations, orbit platforms, and data that aligns with NASA Earth Science Division (ESD) goals. The CSDA makes its selections from the proposals that meet the requirements and then submits them to NASA leadership for approval. Once approved, the contracts are then awarded and the companies are able to get their data evaluated by CSDA. Once the evaluations are complete, the commercial data providers can then compete for competitive task orders through CSDA.
NASA’s Earth Science Division (ESD) established the CSDA Program as the agency’s central mechanism for identifying, acquiring, and evaluating commercial Earth observation (EO) data. The program augments NASA’s and partner agencies’ Earth-observing capabilities by acquiring commercial satellite data that offer higher spatial resolution, increased revisit frequency, complementary measurement capabilities, and taskable observations. To learn more about the program, its commercial partners, data evaluation process, and more, visit the CSDA website.
Commercial data discoverable through the SDX is made available to CSDA authorized data users. To become an authorized user, fill out the CSDA Program Data Authorization Form. Note: Use of SDX also requires an Earthdata Login.
2026-06-23 18:51
58th Girl Scouts Unite Event, July 23-25, 2026
Join NASA in the Exhibit Hall (Booth #206) for Hyperwall Storytelling by NASA experts. Full Hyperwall Agenda below.
Thursday, July 23
11:00AM – 11:15 AM
From Daisy to NASA Engineer
Barbara Hilton
11:15AM – 11:30 AM
Exploring Mars, The Planet Next Door
Lindsay Hays
11:30AM – 11:45 AM
Get Ready With Me: Going to the Moon
Naoma McCall
11:45Am – 12:00 PM
NASA Is for Everyone! (talk about careers at NASA beyond science and engineering)
Amy Kaminski
12:00PM – 12:15 PM
Finding Asteroids Before They Find Us: Planetary Defense at NASA
Kelly Fast
2:15 PM – 2:30 PM
How to Nerd Your Way Into Science Communications
Karen Romano Young
2:30 PM – 2:45 PM
Earth: Exploring our home planet is a team effort
Lesley Ott
2:45 PM – 3:00 PM
TBD
Jenny Mottar
3:00 PM – 3:15 PM
The Journey Starts HERE: One CREW, Your HOME, Our MISSION
Kaitlin Harbeck
3:15 PM – 3:30PM
TBD – Artemis Overview
Dominique Brewer
3:45 PM – 4:00 PM
Social Media… For Science!
Sofie Bates
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