New Volunteer Data from 143 Observatories Unveils the 2024 Total Solar Eclipse

New Volunteer Data from 143 Observatories Unveils the 2024 Total Solar Eclipse

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New Volunteer Data from 143 Observatories Unveils the 2024 Total Solar Eclipse

On April 8, 2024, volunteers participating in NASA’s Eclipse Megamovie citizen science project all around the United States hurried to photograph the solar eclipse with the latest, greatest equipment, capturing groundbreaking images of the Sun’s corona.

Now, the Eclipse Megamovie team has released the remarkable new dataset that resulted from this effort — the first-ever, white-light eclipse dataset with calibration frames, spanning more than a cumulative hour and a half of observations of the solar corona. This data, which includes 52,469 total photographs uploaded by project volunteers, is now live: https://eclipsemegamovie.org/database. The data include contributions from 143 unique, mobile, volunteer-led “observatories” – people with cameras charged with taking precise images of the eclipse, taking extra steps to allow the painstaking calibration required to reveal how the corona evolves from one person’s view to the next. Researchers around the world can now use these observations to identify solar jets leaving the Sun’s surface and study how solar plumes grow and develop. The public can also peruse and download all of this data, which is highly accessible and searchable by observatory name and location.

“Thank you for all you do and have done for us,” said Eclipse Megamovie volunteer Jessi McKenna. “Everyone in the group has been amazingly supportive of each other. And those who are running things are always so obviously appreciative of everyone who has contributed to the project.” 

The files include data at three different levels of processing, from raw (level 1) data to calibrated (level 3) data, in a format called FITS, or Flexible Image Transport System. It is the standard astronomical data format used by NASA and the International Astronomical Union. Of the 143 unique observatories involved, 28 observatories had clear skies, sufficient calibration frames, and enough unique exposure times to create calibrated level 3 images.

The Eclipse Megamovie team at Sonoma State University and the University of California, Berkeley and collaborators at NASA’s Goddard Space Flight Center began working together long before the eclipse to construct this database, together with EdEon STEM (Science, Technology, Engineering, & Mathematics) Learning programmer Troy Wilson. But crucially, Eclipse Megamovie 2024 was made possible because of hundreds of volunteers who journeyed into the path of the April 8, 2024 total solar eclipse with their cameras, patience, and curiosity.

Black and white photograph of 2024 total solar eclipse. Black circle in the middle surrounded by white sun beams
Photograph taken during the April 8th, 2024, total solar eclipse uploaded by EM2024 volunteer Franz Zabroky G. This picture has been aligned and processed and is available in the new database. https://eclipsemegamovie.org/database.
Franz Zabroky G.

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Last Updated
Feb 24, 2026

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Webb Maps Uranus’ Upper Atmosphere

Webb Maps Uranus’ Upper Atmosphere

This image shows the planet Uranus set against the blackness of space. The planet appears as a smooth, bright cyan disc at the center, its atmosphere reveals soft, hazy tones of blue. Surrounding the planet is a vivid reddish glow, forming a diffuse halo that contrasts strongly with the cool blue of the planetary disc. Encircling Uranus are several thin, concentric rings, visible as pale gray arcs. Subtle variations in brightness can be seen across the planet’s face, with slightly brighter patches near the limb, hinting at atmospheric structure.
ESA/Webb, NASA, CSA, STScI, P. Tiranti, H. Melin, M. Zamani (ESA/Webb)

NASA’s James Webb Space Telescope provided the first vertical view of Uranus’s ionosphere in this image released on Feb. 19, 2026, revealing auroras shaped by its tilted magnetic field.

Getting a look at the structure of the region where the atmosphere interacts strongly with the planet’s magnetic field is giving us the most detailed portrait yet of where its auroras form, how the magnetic field influences them, and also data on how Uranus’s atmosphere has continued to cool since the 1990s.

Uranus has the strangest magnetosphere in the Solar System. It is tilted and offset from the planet’s rotation axis (and this planet already rolls around the Sun nearly on its side), which means auroras move across the surface in complex ways. Better understanding Uranus will give us insight into ice-giant planets and help us better characterize giant planets outside our Solar System.

Read more about this image.

Image credit: ESA/Webb, NASA, CSA, STScI, P. Tiranti, H. Melin, M. Zamani (ESA/Webb)

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Monika Luabeya

Technology Originally Developed for Space Missions Now Integral to Everyday Life

Technology Originally Developed for Space Missions Now Integral to Everyday Life

Groundbreaking “camera-on-a-chip” technology that was originally developed at NASA’s Jet Propulsion Laboratory (JPL) for use in space missions is currently employed in billions of devices like cell phones that are used daily by people worldwide.

A group of people standing in a lab surrounded by technical equipment.
Eric Fossum (in the center of the front row) and the team that invented the CMOS image sensor on site at NASA’s Jet Propulsion Laboratory.
Courtesy NASA/JPL-Caltech

In the 1980s, sensors used to produce high-quality images for space science (including the amazing images from NASA’s Hubble Space Telescope) and other applications employed charge coupled device (CCD) technology. Dr. Eric Fossum was originally hired at JPL in 1990 to advance CCD technology for use in interplanetary space missions, but he ended up advancing another technology called complementary metal-oxide semiconductor (CMOS) technology for that purpose and much more. While at JPL, Fossum took advantage of a technique commonly used for CCDs and applied it to CMOS sensors to develop the first CMOS active pixel image sensor. This development began a chain of events that led to the present use of CMOS technology not only in space science missions, but also in billions of cameras in smartphones, webcams, automobiles, and medical devices used worldwide.

A new technology emerges…

In 1990, CCDs were the primary technology used to generate high-quality images. CCD sensors consist of arrays of pixels that convert light into electric charges. The charge from each pixel is transferred step-by-step to an output amplifier at the corner of the sensor and converted to a voltage that represents the brightness of the light received at the corresponding pixel. The data from all the pixels is then aggregated to generate an image. While CCD cameras can produce very high-quality images that are suitable for scientific use, they require a lot of power and an efficient charge transfer process to be effective.

CMOS sensors, on the other hand, have signal amplifiers within each pixel and signals can be read directly from each pixel instead of being transferred long distances to an amplifier for conversion. CMOS sensors therefore require less voltage to operate than CCDs and issues with the charge transfer process such as radiation susceptibility are greatly reduced. Although CMOS sensors existed in the 1990s, they produced too much noise to produce high-quality images required for science applications.

To reduce the signal noise typical of CMOS sensors at that time, Fossum applied a technique that was often used in CCD devices. This technique—called “intra-pixel charge transfer with correlated double sampling”—enables a double measurement of a pixel’s voltage without and with the light-generated charge. Subtracting the values of these two samples enables noise to be suppressed, improving the signal-to-noise ratio.

The next steps

Soon several companies signed Technology Cooperation Agreements with JPL and partnered with Fossum and his colleagues to develop the promising new technology. In 1995, Fossum and co-worker Dr. Sabrina Kemeny licensed the technology from CalTech and founded a company called Photobit to develop CMOS sensors. In 1996, Fossum left JPL to work at Photobit full time. The Photobit, team further refined the CMOS technology to get it closer to CCD capabilities, reduce power requirements, and make manufacturing cheaper.

Shortly thereafter, CMOS cameras started to be used in webcams, “pill cams” (small, swallowable devices that incorporate a tiny camera to take thousands of high-resolution images of the digestive tract), and other applications. In 2001 Photobit was acquired by Micron Technology, a larger company that devoted even more resources to development of CMOS technology. With the subsequent explosion of the cell phone industry, by 2013 more than a billion CMOS sensors were manufactured each year, and today that number has grown to about seven billion per year.

Where are these sensors now?

The CMOS technology Dr. Fossum originally developed has not only enabled space science, it has been infused into devices we depend on every day, dramatically and positively transforming many aspects of our lives. Virtually all digital still and video cameras, including those on cell phones, employ them. In addition, CMOS technology is used in automotive electronics, webcams, sports cameras, industrial equipment, security cameras including doorbells, and cinematography cameras, and for medical and dental imaging, among many other applications.

Image of solar wind racing out from the Sun’s outer atmosphere, looking like smoke on a black background.
A frame from a video made from images taken by the Wide-Field Imager for Solar Probe (WISPR) instrument (which employs CMOS technology) onboard NASA’s Parker Solar Probe. This image was captured during the mission’s record-breaking flyby of the Sun on Dec. 25, 2024, and shows the solar wind racing out from the Sun’s outer atmosphere, the corona.
Credit: NASA/Johns Hopkins APL/Naval Research Lab

In addition to dominating the commercial and consumer market, CMOS imagers have been used as engineering cameras to enable the entry, descent, and landing of NASA’s Perseverance Mars rover, in the camera onboard the OCO-3 (Orbiting Carbon Observatory-3) mission that monitors the distribution of carbon dioxide on Earth, and as scientific imagers on NASA’s Parker Solar Probe mission that is revolutionizing our understanding of the Sun. CMOS imagers are on their way to Jupiter’s moon, Europa, on the agency’s Europa Clipper mission, and a delta-doped ultraviolet version with tailored response is under development for use on the upcoming UVEX (UltraViolet EXplorer) mission that will provide insight into how galaxies and stars evolve.

CMOS imagers are routinely used in monitoring the launch and deployment of CubeSats and SmallSats. They were recently used to monitor the deployment of Pandora, a small satellite that will characterize exoplanet atmospheres and their host stars; BLACKCAT (the Black Hole Coded Aperture Telescope), a small X-ray telescope; and the SPARCS (Star-Planet Activity Research CubeSat) mission designed to monitor and characterize the stellar flares of low-mass stars in ultraviolet to provide context for the habitability of exoplanets in their system. NASA is also developing descendants of this technology for use in missions that will search for life beyond Earth like its Habitable Worlds Observatory.

In recognition of the impact this CMOS technology has had, the National Academy of Engineering (NAE) has named Dr. Fossum the recipient of the 2026 Charles Stark Draper Prize for Engineering “for innovation, development, and commercialization of the complementary metal-oxide semiconductor (CMOS) active pixel image sensor ‘camera-on-a-chip.’” The NAE bestows this award biennially to honor an engineer “whose accomplishment has significantly impacted society by improving the quality of life, providing the ability to live freely and comfortably, and/or permitting the access to information.”

Sponsoring Organizations: The original efforts at JPL to develop this CMOS technology were funded by JPL and NASA.

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Feb 24, 2026

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Showy Swirls Around Jeju Island

Showy Swirls Around Jeju Island

A series of spiraling clouds extends southeast from an oval-shaped island in the Korea Strait. To the west, a large sediment plume fans out from the coast of China and forms tan, teal, and blue swirls in the water.
February 19, 2026

The tallest point in South Korea is not located in the Taebaek Mountains that run along the country’s eastern coast. Rather, it is found atop a volcanic peak on Jeju Island, about 100 kilometers (60 miles) south of the Korean Peninsula. In winter 2026, winds blew past the island in just the right way to send clouds spinning in its wake.

The MODIS (Moderate Resolution Imaging Spectroradiometer) on NASA’s Terra satellite captured this image of swirling clouds—and colorful, turbulent water—near Jeju Island on February 19, 2026. The island rises about 1,950 meters (6,400 feet) above the sea surface. At its center is Hallasan, a shield volcano that last erupted in the 11th century and contains a notable network of lava tubes.

The trailing, staggered spirals, called von Kármán vortex streets, form when a fluid passes a tall, isolated, stationary object. If winds are too weak, clouds simply flow smoothly past, and if winds are too strong, vortices cannot maintain their shape. In the sweet spot, with winds between 18 and 54 kilometers (11 and 34 miles) per hour, clouds trace the airflow in patterns of counterrotating vortices. Though the underlying physics is the same, the appearance of the vortices can vary: sometimes they look wispy, as they do here, and other times they form more sharply defined, parallel rows, as they did at the same location the previous day.

The seas, as well as the atmosphere, were turbulent near Jeju Island in mid-February. To the west, a large plume of sediment coming off the coast of China’s Jiangsu province turned waters murky. While brown, sediment-laden water is present in the shallow nearshore area year-round, expansive plumes like this one are common during winter. Research suggests that seasonal changes in currents and vertical mixing of the water column may account for the large winter plumes.

NASA Earth Observatory image by Michala Garrison, using MODIS data from NASA EOSDIS LANCE and GIBS/Worldview. Story by Lindsey Doermann.

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Expedition 74 Relaxes on Monday Following Busy Weekend

Expedition 74 Relaxes on Monday Following Busy Weekend

The city lights of Türkiye sparkle 261 miles below the International Space Station in this photograph from a window aboard a SpaceX Dragon crew spacecraft taken at approximately 9:24 p.m. local time. In the foreground, is a set of the orbital outpost's main solar arrays (left) and another SpaceX Dragon spacecraft (lower right).
iss074e0225549 (Jan. 6, 2026) — The city lights of Türkiye sparkle 261 miles below the International Space Station in this photograph from a window aboard a SpaceX Dragon spacecraft taken at approximately 9:24 p.m. local time. In the foreground, is a set of the orbital outpost’s main solar arrays (left) and another SpaceX Dragon spacecraft (lower right).
JAXA/Kimiya Yui

Expedition 74 was off duty on Monday following a weekend of crew handover activities, cargo packing, and microbiology research. A SpaceX Dragon spacecraft will also depart the International Space Station for return to Earth later this week.

The orbital outpost’s newest residents spent Saturday and Sunday familiarizing themselves with space station systems and procedures following a busy first week of scientific operations. Standard housekeeping duties such as trash collecting, vacuuming modules and vents for dust, and wiping down surfaces with a disinfectant rounded out the weekend activities.

NASA Flight Engineer Chris Williams, who has been orbiting Earth since November, assisted the station’s newest crewmates Jessica Meir and Jack Hathaway, both from NASA, and Sophie Adenot of ESA (European Space Agency) helping them get up to speed with living and working in weightlessness. Williams showed the trio the location of food, drinks, and emergency gear, demonstrated the operation of medical equipment, communications gear, and computer networking hardware, and gave a tour of the modules while describing the operations and systems that take place in each. Williams also joined Meir and Adenot on Saturday and explored using ultraviolet light as a method to disinfect spacecraft inhibiting microbial growth to protect crew health and space equipment.

The quartet will also step up the pace of cargo transfers inside the Dragon cargo spacecraft as it nears its departure later this week. Dragon will return to Earth loaded with completed science experiments and station hardware for analysis. The astronauts also continued unloading crew supplies from the Dragon crew spacecraft delivered on Feb. 14.

Roscosmos Flight Engineer Andrey Fedyaev, who is beginning his second spaceflight, joined his cosmonaut crewmates over the weekend, Commander Sergey Kud-Sverchkov and Sergei Mikaev, cleaning ventilation systems and inspecting laptop computers and power supply systems. Fedyaev also continued his respiratory research on Saturday attaching an acoustic sensor to his neck that recorded his rapid exhalation to understand how microgravity affects his breathing.

Learn more about station activities by following the space station blog, @space_station on X, as well as the ISS Facebook and ISS Instagram accounts.

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Mark A. Garcia