Discover the cosmos! Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer.
Total Solar Eclipse Over Spain
Explanation: On August 12th, 2026, the Moon totally eclipsed the Sun and cast its shadow across Siberia, Greenland, Iceland, Spain, and Portugal. Today’s image features two total solar eclipses viewed from Zaragoza, Spain, one over the Cathedral-Basilica of Our Lady of the Pillar and the other reflecting in the Ebro River. For a few moments, Spain saw its first major total solar eclipse since 1905. Those witnessing totality may experience a chill in the air, the quieting of birds, the confused chirps of insects, and the shared awe of many. It’s the corona’s time to shine as the Sun’s bright disk is blocked by the Moon. Among other reasons to study eclipses, they help scientists understand why the corona is millions of degrees hotter than the Sun’s surface. Enthusiastic citizens can contribute to these studies by recording how wildlife responds, imaging the corona, and monitoring air temperature and clouds.
A total solar eclipse is seen from San Millán de los Caballeros, Spain, Wednesday, Aug. 12, 2026. A total solar eclipse – the Moon passing between the Sun and Earth, completely blocking the face of the Sun – swept across parts of Greenland, Iceland, northern Russia, the Atlantic Ocean, Spain, and a small corner of Portugal. A partial eclipse was visible in parts of the U.S., most of Canada, much of Europe, and northwest Africa.
Preparations for Next Moonwalk Simulations Underway (and Underwater)
The Vertical Motion Simulator at NASA’s Ames Research Center in California’s Silicon Valley is capable of vertical and horizontal motion to simulate a range of flight experiences, such as lunar landers, helicopters, and commercial aircraft.
NASA/Jesse Carpenter
Imagine stepping into a machine that can make you feel like you’re flying a spacecraft, piloting a next generation air taxi, or landing on the Moon, all without leaving the ground. NASA’s Vertical Motion Simulator, the largest of its kind in the world, does exactly that. And now, with new upgrades, it’s more powerful and realistic than before.
The Vertical Motion Simulator, located at NASA’s Ames Research Center in California’s Silicon Valley, has shaped the future of aviation and spaceflight since 1979. It allows pilots and researchers to experience realistic aircraft motion due to its ability to travel 60 feet vertically and 40 feet horizontally, simulating vehicles ranging from helicopters to spacecraft with high accuracy.
New improvements are making the simulator even more powerful. One of the biggest changes is the switch from analog systems to modern digital technology. This upgrade includes a dome surrounding the simulator’s cockpit with advanced 4K projectors that create visuals with nearly 20/20 clarity, giving pilots clearer, sharper images and a larger field of view of the world outside the cockpit.
The upgraded cab of the Vertical Motion Simulator at NASA’s Ames Research Center in California’s Silicon Valley provides researchers with near-20/20 visual clarity, providing clearer, sharper images.
NASA/Brandon Torres-Navarrete
“The new dome configuration and improved systems can support far more aggressive mission tasks while giving pilots and crews a more realistic environment to work in,” said Diana Acosta, aerospace simulation research and development branch chief at NASA Ames. “It strengthens how teams coordinate, react, and manage challenging scenarios, exactly the kind of preparation we need for the missions coming next.”
The system also can automatically line up and color‑match images to integrate them into a simulated background, a process that used to take hours, or even days, to do by hand.
In the past, changing simulation configurations from lunar lander to air taxi required swapping out the cab, a large, heavy structure that was time‑consuming and complex to move. Instead of replacing an entire cab, teams can use lighter, removable inserts that include only the controls, seats, and panels needed to stand in for a specific vehicle. The inserts drastically reduce physical labor and cut the time needed to configure a simulation in half.
The upgrades to the Vertical Motion Simulator will enable tests of next-generation aircraft and spacecraft before they ever leave the ground, bringing us closer to safer skies, more efficient air travel, and successful human landings on the Moon and Mars.
A new quality assessment report from NASA’s Commercial Satellite Data Acquisition (CSDA) program evaluates data from the Polar Geospatial Center’s (PGC) EarthDEM product. The results of the evaluation help inform NASA program management and the user community about the quality of commercial Digital Elevation Models (DEMs) for use in NASA science.
At left, the cover of the Commercial Satellite Data Acquisition programs’s recently released Polar Geospatial Center EarthDEM Quality Assessment Report. At right, a shaded relief rendering of EarthDEM data showing the Virgin River in Nevada. DEM derived from Vantor imagery.
Credit: NASA CSDA program/EarthDEM Project
Issued August 8, 2026, the CSDA Polar Geospatial Center EarthDEM Quality Assessment Reportwas conducted by NASA Digital Elevation Model (DEM) subject matter experts (SMEs) enlisted to evaluate the horizontal and vertical accuracy of two PGC EarthDEM1 (i.e., Digital Elevation Model) products: the center’s “Mosaic Tile” and “Strip” Digital Surface Models (DSMs).
To assess the vertical and horizontal accuracy of the EarthDEM Strip DSM and Mosaic Tile products over a variety of surface characteristics, the SMEs compared them to airborne lidar data samples from across the United States and Senegal. They found the horizontal accuracy of the EarthDEM products (Strip DSM: 0.5-meter (m) Root Mean Square Error Horizontal (RMSEH); Mosaic Tile: 0.3 m RMSEH) agreed with the specifications provided by the PGC and graded them “Excellent.” The vertical accuracy results of the EarthDEM Strip DSM (5.6 m Root Mean Square Error Vertical (RMSEV)) and the Mosaic Tile (4.9 m RMSEV) products varied by land cover type, with all land cover types exceeding the specification provided by the PGC (0.5 m RMSEV). Strip DSM vertical accuracy was found to vary from 4.6-6.8 m RMSEV depending on the cloud cover metadata field generated by the PGC. Given this variation, the vertical accuracy compliance for the EarthDEM products was graded as “Basic.”
Overall, the assessment report supports the use of EarthDEM data for NASA Earth science research and applications, as long as the data characteristics (e.g., vertical accuracy, poor cloud masking, missing surface features, data voids, etc.) are compatible with the specific science objectives and use cases.
The report also provides a Data Provider Documentation Review for the EarthDEM product that evaluated information from the PGC website, as well as a series of peer-reviewed publications by researchers at The Ohio State University’s Byrd Polar and Climate Research Center. (Only documents listed in this report were considered in the evaluation.) The report’s authors found that, overall, the EarthDEM product is “well documented,” with most information present within the product User Guide, a series of peer reviewed papers, or the PGC GitHub repository.
About the CSDA Program
The CSDA program was established to identify, evaluate, and acquire data from commercial sources that support the NASA Earth science research and application goals. NASA’s Earth Science Division recognizes the potential impact commercial satellite constellations may have in encouraging/enabling efficient approaches to advancing Earth System Science and applications development for societal benefit. Commercially acquired data may also provide a cost-effective means to augment and/or complement the suite of Earth observations acquired by NASA, other U.S. government agencies, and international partners.
1. According the authors of the report, “it should be noted that the PGC EarthDEM product is not technically a commercial product…. EarthDEM is a digital elevation dataset derived from imagery collected from the Vantor (formerly Maxar) fleet of optical satellites.”
The glacier-capped Snæfellsjökull volcano is the defining feature of Iceland’s Snæfellsnes peninsula, shown in this image acquired with the OLI (Operational Land Imager) on Landsat 9 on July 25, 2026.
NASA Earth Observatory/Michala Garrison
The Sun, Moon, and Earth align on August 12, 2026, to produce a total solar eclipse. When this celestial event last occurred, on April 8, 2024, the path of totality stretched across North America, giving millions the chance to glimpse the Sun’s corona. In 2026, the viewing locales are more limited; only a handful of land areas in the Northern Hemisphere, including parts of Iceland and Spain, fall within the path of totality.
On August 12, the Moon’s shadow will first cross over the Arctic Circle from northern Russia and then track along the eastern side of Greenland. At about 5:45 p.m. local time in Iceland (17:45 Universal Time), the country’s western fringes—including the Snæfellsnes peninsula, shown in the Landsat image above—will begin to experience totality. The greatest eclipse will occur near this sparsely populated peninsula when the Moon appears the largest and covers more of the Sun.
The path of totality of the solar eclipse on August 12, 2026, spans Greenland, Iceland, and Spain. The base imagery for the map comes from Blue Marble: Next Generation, with data from Black Marble shown in the path of totality. Blue Marble is built from scenes captured by MODIS (Moderate Resolution Imaging Spectroradiometer), while Black Marble is based on observations by the VIIRS (Visible Infrared Imaging Radiometer Suite) day-night band.
NASA Earth Observatory/Michala Garrison
The Snæfellsjökull volcano on the western end of the peninsula is covered in ice and last erupted about 1,800 years ago. It is the highlight of a national park of the same name, where people are expected to visit to view the eclipse. The stratovolcano even has a literary claim to fame: in Jules Verne’s A Journey to the Center of the Earth, characters venture underground through its crater, later emerging in an eruption of Stromboli, in Italy. In 2025, a broader area of the peninsula was designated a UNESCO biosphere reserve, containing over 70 percent of Iceland’s flora and an agglomeration of volcanic landscapes, wetlands, and grasslands.
From Iceland, the eclipse shadow, or umbra, progresses across the North Atlantic and reaches northern Spain shortly before sunset. It runs east-southeast across the country, much like the Ebro River (Río Ebro), seen in the Landsat image below.
The Ebro River, meandering across northern Spain in this image acquired with the OLI (Operational Land Imager) on Landsat 8 on July 21, 2026, is in the path of totality of the August 2026 solar eclipse.
NASA Earth Observatory/Michala Garrison
The upper Ebro emerges from rugged terrain in Parque Natural de Montes Obarenes-San Zadornil, where it carves canyons and gorges through the eastern foothills of the Cantabrian Mountains. It then meanders through La Rioja, a region known for its vineyards. About 400 kilometers (250 miles) away, the river reaches a delta on the Mediterranean coast between Barcelona and Valencia.
Based on satellite measurements of cloud cover in August over several decades, viewers in Spain have a higher likelihood than those in Iceland of getting a clear look at the eclipse. And despite limited viewing opportunities in the path of totality, the rest of Europe, parts of Africa, Canada, and the northern and northeastern U.S. will experience a partial eclipse.
Preparations for Next Moonwalk Simulations Underway (and Underwater)
This article is for students grades 5-8.
The Nancy Grace Roman Space Telescope is NASA’s newest astrophysics observatory. The telescope will scan large sections of space. Roman will help astronomers answer questions about dark energy, dark matter, exoplanets, and more.
The Nancy Grace Roman Space Telescope is NASA’s newest space telescope that will study dark energy, exoplanets, and astrophysics.
Astrophysics: a branch of space science that applies physics and mathematics to study the universe.
Lagrange point: a position in space where the gravitational forces of a two-body system, such as the Sun and Earth, are balanced. This point creates an “orbital parking spot” where minimal fuel is needed to maintain a spacecraft’s position.
Infrared light: light that is completely invisible to the human eye but can be felt as heat. It’s the area on the electromagnetic spectrum where wavelengths are longer than visible red light, but shorter than microwaves.
Dark energy: the mysterious force that is causing the universe to expand at an accelerated rate.
Exoplanet: a planet outside of our solar system.
Dark matter: the mysterious gravitational “glue” that holds cosmic structures together.
When and Where Will the Nancy Grace Roman Space Telescope Launch?
The Nancy Grace Roman Space Telescope is scheduled to launch Aug. 30, 2026. It will launch aboard a SpaceX Falcon Heavy rocket. Liftoff will take place from Launch Complex 39A at NASA’s Kennedy Space Center in Florida.
Where Will the Nancy Grace Roman Space Telescope Go in Space?
The Nancy Grace Roman Space Telescope will orbit about 930,000 miles (1.5 million kilometers) away from Earth. It will orbit around a special place in space called the second Sun-Earth Lagrange point, or L2. This gravitational sweet spot is perfect for unobstructed views of the universe.
What Instruments Does the Nancy Grace Roman Space Telescope Have?
The Nancy Grace Roman Space Telescope will peer through dust and across vast stretches of space using infrared light. Roman’s primary mirror is 7.9 feet (2.4 meters) across. The large surface of the telescope mirror gathers lots of light. More light equals finer details.
The primary mirror will send light to Roman’s two science instruments: the Wide Field Instrument and the Coronagraph Instrument.
The Wide Field Instrument is a 300-megapixel infrared camera. It allows scientists to look very far back in time because the light captured by the camera has been traveling for billions of years before reaching the instrument. Seeing the universe in its early stages will help unravel how it has expanded throughout its history. This will give scientists hints about how the universe may continue to evolve.
The Coronagraph Instrument uses technology that blocks the glare from a star. This lets astronomers see planets in orbit around it. This instrument is the most powerful coronagraph ever flown in space. It will allow astronomers to see planets that are almost a billion times fainter than their host star.
On Nov. 25, 2025, technicians joined the inner and outer segments together and the observatory was complete.
NASA / Sydney Rohde
What Will Scientists Study With the Nancy Grace Roman Space Telescope?
Scientists using the Nancy Grace Roman Space Telescope will focus on three main topic areas: dark energy, exoplanets, and dark matter.
Dark energy is a mysterious part of the universe. Scientists aren’t sure what it is, but it makes up about 68% of the universe’s total contents. It is believed to be responsible for the accelerating rate at which our universe is expanding. But recent observations seem to show that the pressure from dark energy is shifting over time. Scientists hope to use the Roman Space Telescope to help solve the mystery of dark energy’s true nature.
Exoplanets are planets outside of our solar system. Scientists have discovered more than 6,000 exoplanets. But they believe that billions could exist. Most of the exoplanets detected so far are wildly different than the planets in our solar system. Scientists expect Roman to find more unusual exoplanets. It will also allow astronomers to find planets in the habitable zone of their stars. This will be key to finding planets similar to Earth.
Dark matter is the invisible glue that holds the universe together. Scientists aren’t sure what dark matter is made of. Roman will allow scientists to peer back in time to trace how galaxies and galaxy clusters formed. If dark matter consists of heavy, sluggish particles, it would clump together readily and Roman should see galaxy formation early in cosmic history. If dark matter is made up of lighter, faster-moving particles, it should take longer to settle into clumps and for large-scale structures to develop. If astronomers can narrow down the candidates for dark matter particles, we’ll be one step closer to finally detecting them directly in experiments on Earth.
Who Was Nancy Grace Roman?
Nancy Grace Roman was NASA’s first chief astronomer and the first female executive at the agency. Roman championed the making of the first space-based telescope — the Hubble Space Telescope. She was involved in every crucial decision about the telescope from its funding to where it was built to the details of its instruments. Her vital role in making the project a reality led her to be known as “the mother of the Hubble Space Telescope.”
Roman was born May 16, 1925, in Nashville, Tennessee. She died Dec. 25, 2018.
Nancy Grace Roman was NASA’s first chief astronomer. She is knows as “the mother of the Hubble Space Telescope.”
NASA
Career Corner
More than a thousand technicians and engineers assembled Roman from millions of individual components. Here are a few examples of the careers that shaped NASA’s newest space telescope:
Instrument technician: These experts install, calibrate, and maintain sensors and control systems. They troubleshoot issues that might come up with delicate systems and equipment. This career path often starts with an apprenticeship or hands-on training alongside experienced technicians. An associate’s degree is often required.
Mechanical engineer: This branch of engineering focuses on complex machines and engines. Mechanical engineers design, build, test, and improve mechanical systems. They play an essential role in making a complex observatory like the Roman Space Telescope a reality. A career in engineering demands a strong understanding of math and complex problem-solving and usually requires an advanced college degree.
Astrophysicist: These scientists study the physics of the universe. They are interested in learning how the universe began, how it is evolving, and how it works. Becoming an astrophysicist requires advanced college degrees.
NASA also needs people who work in photography, management, social media, videography, and much more. Learn about some of the people who have made the Roman mission possible here!
The fully-integrated LEMS (Lunar Environment Monitoring Station) ready for environmental testing. A small suitcase-size instrument suite built at NASA Goddard, LEMS is designed to carry out continuous, long-term monitoring of the seismic environment at the Moon, including surface motion caused by moonquakes and meteorite impacts in the lunar south polar region.
NASA Goddard
NASA has declared “wrenches down” on the first completed payload designed for Artemis astronauts to deploy on the Moon’s surface. Engineers working on NASA’s Lunar Environment Monitoring Station, or LEMS, have completed hardware development and testing and the payload is ready for its permanent home near the lunar South Pole. With the hardware complete, LEMS is ready to support one of the Artemis program’s core goals: enabling sustained lunar science and exploration.
The LEMS instrument package contains two highly sensitive seismometers that will monitor ground vibrations from moonquakes and meteorite impacts, providing scientists with insights into the Moon’s interior and the seismic hazards astronauts might encounter at the surface. Its modular design allows the system to be adapted or expanded to host new instruments in the future, creating a reusable platform that can evolve as scientific priorities grow.
The payload will remain in a clean room at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, where it was built, until it is assigned to an Artemis mission for deployment to the lunar surface.
“The completion of the LEMS scientific instrument is a major step in a new era of lunar surface science. Innovative science experiments will uncover, measure, and reveal the Moon’s secrets while astronauts open new frontiers for discovery,” said Joel Kearns, deputy associate administrator for exploration, Science Mission Directorate, NASA Headquarters in Washington. “And, behind the scenes, countless teams across NASA and our partners are pushing the boundaries of what surface instruments can do, building the tools that will make future exploration possible and safer.”
A scientist wearing NASA’s xEMU prototype space suit is testing the handling of a mockup version of NASA’s Lunar Environment Monitoring Station, or LEMS. The testing took place at the Active Response Gravity Offload System, a simulated reduced gravity environment at NASA’s Johnson Space Center in Houston.
NASA Johnson
The LEMS payload builds on a legacy of lunar seismic tracking. Apollo astronauts deployed a network of seismometers on the Moon’s nearside equatorial region between 1969 and 1972. Those instruments operated until 1977, recording about 13,000 moonquakes and other ground vibrations that helped scientists begin to understand the composition of the Moon’s interior. For decades, researchers have hoped to spread more seismometers, updated with new technologies, across the lunar surface.
Now, LEMS will carry the first seismometers to be deployed by future astronauts to listen for faint ground vibrations, collecting new clues to the Moon’s internal structure and ongoing seismic activity. The sensors will be the most compact, sensitive, and energy-efficient seismometers ever built for planetary exploration.
LEMS itself is about the size of a small suitcase, weighing 11 pounds in the Moon’s low-gravity environment. It will carry not just these seismic sensors, but everything it needs to function independently of humans after deployment. LEMS is built to manage its own power production via a lightweight, flexible solar array that conforms to the shape of the LEMS unit. It also will manage its operational activities to ensure continuous data collection based on a preset plan, and monthly data transmission to Earth. The payload will do all this while maintaining a stable internal temperature throughout the massive day-to-night temperature swings of the South Pole region.
Mechanical Engineer Brie Ludwig inspects the Lunar Environment Monitoring Station (LEMS) in preparation for testing in a thermal vacuum chamber at Goddard Space Flight Center in Greenbelt, Maryland, on March 31, 2026. LEMS is a compact, autonomous, and self-sustaining seismometer suite designed to carry out continuous, long-term monitoring of the lunar seismic environment at the South Polar region.
NASA/Denny Henry
“When we conceived of LEMS, we weren’t just thinking about the next mission, we were thinking about the next generation of lunar exploration,” said Mehdi Benna, a University of Maryland Baltimore County scientist who leads LEMS from NASA Goddard. “Our vision was to create a scientific buoy for the Moon. Like an ocean buoy on Earth, LEMS is designed to be easy to build, adaptable to different scientific objectives, and capable of operating independently for years.”
Before any surface science could happen, Benna and his team had to ensure that LEMS could survive the trip to the Moon and the harsh environment of its surface. Over the past five months, LEMS and its components have been subjected to a demanding series of environmental and operational tests. Engineers verified LEMS can endure the violent shaking of launch, the journey to the lunar surface, and the Moon’s temperature and radiation environment. The team also showed that the instrument package’s mechanical and electrical design is safe for astronaut handling.
The LEMS payload was built to operate through the lunar night, which lasts two Earth weeks, without external power assistance or a heat source. Past lunar surface instruments relied on radioisotope heaters for warmth and power. But LEMS instead will withstand temperatures that dip to minus 400 degrees Fahrenheit in some areas by using advanced insulation materials, low-thermal-conductivity cables that minimize heat loss, and a thermal regulator that conducts heat away during the day to prevent overheating and helps retain heat at night.
These innovations reduce mass and power needs, setting the stage for lighter, energy-efficient instruments that can operate continuously at future Artemis landing sites and the NASA-led Moon Base.
The LEMS payload is led by University of Maryland Baltimore County and University of Maryland College Park. Technical implementation is led by NASA Goddard. The University of Arizona, in partnership with Silicon Audio, Inc., supplied LEMS’ two state-of-the-art seismometers. Morehead State University in Kentucky provided LEMS’ telecommunication system and will operate the instrument on the surface. Washington University in St. Louis will manage the instrument’s data processing and dissemination to the larger scientific community.
