NASA Uses New Technology to Understand California Wildfires

NASA Uses New Technology to Understand California Wildfires

3 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

A scientific instrument sits on top of a metal surface. The instrument is composed of several metal blocks, cables, tubes, and dials. The central block appears to have a microchip and is connected by cables and tubes to the adjacent blocks. Some electrical wiring protrudes from parts of the instrument.
The Compact Fire Infrared Radiance Spectral tracker, or C-FIRST, is managed an operated by NASA’s Jet Propulsion Laboratory, and supported by NASA’s Earth Science Technology Office. Combining state-of-the-art imaging technology with a compact design, C-FIRST enables scientists to gather data about fires and their impacts on ecosystems with greater accuracy and speed than other instruments. C-FIRST was developed as a spaceborne instrument, and flew onboard NASA’s B200 aircraft in January 2025 to conduct an airborne test.
NASA/JPL-Caltech

The January wildfires in California devastated local habitats and communities. In an effort to better understand wildfire behavior, NASA scientists and engineers tried to learn from the events by testing new technology.

The new instrument, the Compact Fire Infrared Radiance Spectral Tracker (c-FIRST), was tested when NASA’s B200 King Air aircraft flew over the wildfires in the Pacific Palisades and Altadena, California. Based at NASA’s Armstrong Flight Research Center in Edwards, California, the aircraft used the c-FIRST instrument to observe the impacts of the fires in near real-time. Due to its small size and ability to efficiently simulate a satellite-based mission, the B200 King Air is uniquely suited for testing c-FIRST.

Managed and operated by NASA’s Jet Propulsion Laboratory in Southern California, c-FIRST gathers thermal infrared images in high-resolution and other data about the terrain to study the impacts of wildfires on ecology. In a single observation, c-FIRST can capture the full temperature range across a wide area of wildland fires – as well as the cool, unburned background – potentially increasing both the quantity and quality of science data produced.

“Currently, no instrument is able to cover the entire range of attributes for fires present in the Earth system,” said Sarath Gunapala, principal investigator for c-FIRST at NASA JPL. “This leads to gaps in our understanding of how many fires occur, and of crucial characteristics like size and temperature.”

For decades, the quality of infrared images has struggled to convey the nuances of high-temperature surfaces above 1,000 degrees Fahrenheit (550 degrees Celsius). Blurry resolution and light saturation of infrared images has inhibited scientists’ understanding of an extremely hot terrain, and thereby also inhibited wildfire research. Historically, images of extremely hot targets often lacked the detail scientists need to understand the range of a fire’s impacts on an ecosystem.

NASA’s Armstrong Flight Research Center in Edwards, California, flew the B200 King Air in support of the Signals of Opportunity Synthetic Aperture Radar (SoOpSAR) campaign on Feb. 27, 2023.
NASA/Steve Freeman

To address this, NASA’s Earth Science Technology Office supported JPL’s development of the c-FIRST instrument, combining state-of-the-art imaging technology with a compact and efficient design. When c-FIRST was airborne, scientists could detect smoldering fires more accurately and quickly, while also gathering important information on active fires in near real-time.

“These smoldering fires can flame up if the wind picks up again,” said Gunapala. “Therefore, the c-FIRST data set could provide very important information for firefighting agencies to fight fires more effectively.”

For instance, c-FIRST data can help scientists estimate the likelihood of a fire spreading in a certain landscape, allowing officials to more effectively monitor smoldering fires and track how fires evolve. Furthermore, c-FIRST can collect detailed data that can enable scientists to understand how an ecosystem may recover from fire events.

“The requirements of the c-FIRST instrument meet the flight profile of the King Air,” said KC Sujan, operations engineer for the B200 King Air. “The c-FIRST team wanted a quick integration, the flight speed in the range 130 and 140 knots on a level flight, communication and navigation systems, and the instruments power requirement that are perfectly fit for King Air’s capability.”

By first testing the instrument onboard the B200 King Air, the c-FIRST team can evaluate its readiness for future satellite missions investigating wildfires. On a changing planet where wildfires are increasingly common, instruments like c-FIRST could provide data that can aid firefighting agencies to fight fires more effectively, and to understand the ecosystemic impacts of extreme weather events.

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Dede Dinius

What’s Up: March 2025 Skywatching Tips from NASA

What’s Up: March 2025 Skywatching Tips from NASA

A Fast-Moving Planet and a Crimson Moon!

Catch Mercury if you can, then stay up late for a total lunar eclipse, and learn the truth about the dark side of the Moon.

Skywatching Highlights

All Month – Planets Visibility:

  • Mercury: Speedy Mercury is visible beneath Venus for the first week and a half of March, for about 30 minutes each evening, as sunset fades. 
  • Venus: Venus hangs low in the west after sunset early in the month, but quickly drops lower as the days pass. After mid-March, it’s difficult to observe in the glow of fading sunlight.
  • Mars: Find Mars high in the east following sunset, then setting around 3 a.m.
  • Jupiter: Visible high in the west after dark, and setting about 1 a.m.

Daily Highlights:

March 7-9 – Catch Mercury: Look for Mercury beginning about 30 minutes after sunset in the west, about 10 degrees above the horizon. 

March 13-14 – Total Lunar Eclipse: The Moon becomes a crimson orb over a couple of hours on March 13th and into the 14th, depending on your time zone.

March 14 – Full moon

March 29 – New moon: This is when the dark side of the Moon faces toward Earth. The new moon appears close to the Sun in the sky, so it’s essentially invisible from the surface (except during solar eclipses).

Transcript

What’s Up for March? A good time to catch Mercury, an eclipse approaches, and the dark side of the Moon.

March Planet Viewing

March begins with Venus still hanging out low in the west after sunset, but it quickly drops out of the sky – by mid-month it’s getting lost in the glare of sunset. Once it gets dark, you’ll find Jupiter and Mars high overhead, keeping you company through the evening. Mars sets a couple of hours after midnight this month, leaving the morning sky “planet free” for the first time in a year. 

An illustrated sky chart shows the evening sky on March 8th, facing west, 30 minutes after sunset. Venus is marked as a bright white dot near the horizon, with Mercury as a smaller (and thus less bright) white dot below Venus. Jupiter is a bright white dot high in the sky near top center. The scene features a dark twilight background with faint stars and labeled compass directions:
Sky chart showing Venus and Mercury after sunset in early March.
NASA/JPL-Caltech

March also has the best opportunity this year for trying to spot fast-moving Mercury if you’re in the Northern Hemisphere. It’s only visible for a few weeks at a time every 3 to 4 months. This is because the speedy planet orbits the Sun in just 88 days, so it quickly shifts its position in the sky from day to day. It’s always visible either just after sunset or just before sunrise. On March 7th through 9th, look for Mercury beginning about 30 minutes after sunset in the west, about 10 degrees above the horizon. 

You’ll want to ensure your view isn’t blocked by trees, buildings, or other obstructions. Observing from a large, open field, or the shore of a lake or the seaside can be helpful. Spying Mercury isn’t always easy, but catching the fleet-footed planet is a worthy goal for any skywatcher.

Total Lunar Eclipse

A map of the world centered on the Western Hemisphere shows a darkened area at center covering the Americas with the label
This map shows where the Moon will be above the horizon during the March 13-14 total lunar eclipse.

There’s a total lunar eclipse on the way this month, visible across the Americas. Lunar eclipses can be viewed from anywhere the Moon is above the horizon at the time. The show unfolds overnight on March 13th and into the 14th, depending on your time zone. Check the schedule for your area for precise timing.

Now, during a total lunar eclipse, we watch as the Moon passes through Earth’s shadow. It first appears to have a bite taken out of one side, but as maximum eclipse nears, the Moon transforms into a deep crimson orb. That red color comes from the ring of all the sunsets and sunrises you’d see encircling our planet if you were an astronaut on the lunar surface right then. Afterward, the eclipse plays out in reverse, with the red color fading, and the dark bite shrinking, until the Moon looks like its usual self again. 

And here’s an interesting pattern: eclipses always arrive in pairs. A couple weeks before or after a total lunar eclipse, there’s always a solar eclipse. This time, it’s a partial solar eclipse that will be visible across Eastern Canada, Greenland, and Northern Europe.

The Dark Side of the Moon

The Moon has a dark side, but it may not be what you think. As it orbits around Earth each month, the Moon is also rotating (or spinning). So, while we always see the same face of the Moon, sunlight sweeps across the lunar surface every month as it rotates. 

This means there’s no permanently “dark” side. The Moon’s dark side faces Earth when the Moon passes between our planet and the Sun each month. This is the moment when the Moon is said to be “new,” as in a fresh start for its changing phases.

The new moon is also located quite close the Sun in the sky, making it more or less invisible, unless there’s a solar eclipse.

Nights around the new moon phase provide excellent opportunities for observing the sky – especially if you’re using a telescope or doing astrophotography. Without moonlight washing out the sky, you can better see faint stars, nebulas, the Milky Way, and distant galaxies. So next time someone mentions the “dark side of the Moon,” you’ll know there’s more to the story – and you might even discover some deep-sky treasures while the Moon takes its monthly break.

The main phases of the Moon are illustrated in a horizontal row, with the first quarter on March 6, full moon on March 14, the third quarter moon on March 22, and the new moon on March 29.
The phases of the Moon for March 2025.
NASA/JPL-Caltech

Above are the phases of the Moon for March. Stay up to date on all of NASA’s missions exploring the solar system and beyond at NASA Science. I’m Preston Dyches from NASA’s Jet Propulsion Laboratory, and that’s What’s Up for this month.

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Crew Studies Space Exercise While Waiting for Saturday Delivery

Crew Studies Space Exercise While Waiting for Saturday Delivery

The Roscosmos Progress 89 cargo craft departs the vicinity of the International Space Station after undocking from the orbital outpost's Zvezda service module.
The Roscosmos Progress 89 cargo craft completes a cargo delivery mission to the International Space Station after undocking from the orbital outpost’s Zvezda service module on Feb. 25, 2025.
NASA

Exercise research and muscle stimulation were the main research topics aboard the International Space Station on Friday to keep crews fit in weightlessness and in the confinement of a spacecraft. The Expedition 72 crew also prepared for Saturday’s arrival of a cargo mission while working on spacesuit maintenance and housekeeping duties.

Working out every day in space is necessary to counteract the effects of weightlessness including muscle and bone loss. The crew spends two hours seven days a week jogging on a treadmill, pedaling on an exercise cycle, and working out on the advanced resistive exercise device that mimics free weights on Earth.

NASA Flight Engineer Nick Hague spent his day on a pair of experiments investigating how the lack of gravity impacts an exercising astronaut. For his first experiment he wore a sensor-packed vest and headband that recorded his health data as he pedaled on an exercise cycle. Afterward, he downlinked the medical data so doctors on the ground could analyze his heart and breath rate, blood pressure, and more. Hague’s next experiment required him to wear electrodes that stimulated his leg muscles with small electrical signals. Results may improve muscle function, shorten workout sessions, and lead to lighter exercise equipment offsetting space-caused muscle atrophy.

Spacesuit work and lab cleanup filled the last day of the work week for NASA astronauts Butch Wilmore, Don Pettit, and Suni Williams. Wilmore was in the Quest airlock powering up a high-definition camera and swapping life support components on a spacesuit. Pettit switched out an optical cartridge inside the Mochii miniature scanning electron microscope then monitored its ground-controlled operations. Williams began her day collecting body samples for stowage and later analysis. Next, she inspected materials research hardware from the European Space Agency.

Roscosmos’ new Progress 91 cargo craft is orbiting Earth today carrying three tons of food, fuel, and supplies for the Expedition 72 crew following its launch on Thursday. The Progress 91 is scheduled to dock to the Zvezda service module’s aft port at 6:03 p.m. EST on Saturday where it will stay for a six-month cargo mission. NASA+ will begin its live rendezvous and docking coverage at 5:15 p.m.

Cosmonauts Alexey Ovchinin and Ivan Vagner will be on duty monitoring Progress 91 and at the controls of the TORU, or telerobotically operated rendezvous unit, ready to remotely control the approaching spacecraft, if necessary, though unlikely. The duo called down to mission controllers on Friday and discussed preparations for Saturday’s automated arrival of the Progress 91. Flight Engineer Aleksandr Gorbunov spent his day in the Nauka science module primarily working on the orbital plumbing system.

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

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Mark A. Garcia

Langley Laboratory Apprentice at Work

Langley Laboratory Apprentice at Work

A woman looks through a metal tube that she is holding up. Her elbows rest on the table in front of her. The photo is in black and white. There is text at the bottom that reads "LMAL 33037."
NASA

An apprentice at Langley Laboratory (now NASA’s Langley Research Center in Hampton, Virginia) inspects wind tunnel components in this image from May 15, 1943. During World War II, the National Advisory Committee for Aeronautics (NACA), the precursor to NASA, employed apprentices (which NASA has since transitioned into internships) to support meaningful jobs in data computing, testing, and mechanical work.

Make your own mark on NASA history. Apply to the agency’s summer internships by 11:59 p.m. EST Feb. 28.

Image credit: NASA

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Monika Luabeya

Hubble Captures New View of Colorful Veil

Hubble Captures New View of Colorful Veil

1 min read

Hubble Captures New View of Colorful Veil

A colorful, glowing nebula that reaches beyond the top and bottom of the image. This translucent cloud of gas holds wispy and thin filaments with hard edges in some places, and puffy and opaque in others. Blue, red, and yellow colors mix together, showing light emitted by different types of atoms in the hot gas. Scattered across the colorful nebula are bright and point-like foreground and background stars. The background is black.
This NASA/ESA Hubble Space Telescope image a supernova remnant called the Veil Nebula.
ESA/Hubble & NASA, R. Sankrit

In this NASA/ESA Hubble Space Telescope image, Hubble once again lifts the veil on a famous — and frequently photographed — supernova remnant: the Veil Nebula. The remnant of a star roughly 20 times as massive as the Sun that exploded about 10,000 years ago, the Veil Nebula is situated about 2,400 light-years away in the constellation Cygnus. Hubble images of this photogenic nebula were first taken in 1994 and 1997, and again in 2015.

This view combines images taken in three different filters by Hubble’s Wide Field Camera 3, highlighting emission from hydrogen, sulfur, and oxygen atoms. The image shows just a small fraction of the Veil Nebula; if you could see the entire nebula without the aid of a telescope, it would be as wide as six full Moons placed side-by-side.

Although this image captures the Veil Nebula at a single point in time, it helps researchers understand how the supernova remnant evolves over decades. Combining this snapshot with Hubble observations from 1994 will reveal the motion of individual knots and filaments of gas over that span of time, enhancing our understanding of this stunning nebula.

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Media Contact:

Claire Andreoli (claire.andreoli@nasa.gov)
NASA’s Goddard Space Flight CenterGreenbelt, MD

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