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Billions of phones can detect and warn about nearby earthquakes
Billions of phones can detect and warn about nearby earthquakes
Genetically tailored microbes could tweak our microbiomes
Genetically tailored microbes could tweak our microbiomes
Three-Person Mitochondrial IVF Leads to Eight Healthy Births
Long-awaited results of a three-person IVF technique suggest that mitochondrial donation can prevent babies from inheriting diseases caused by mutant mitochondria
Europe working to launch 'Invictus' hypersonic space plane by 2031 (video)
NASA to Launch SNIFS, Sun’s Next Trailblazing Spectator
4 min read
NASA to Launch SNIFS, Sun’s Next Trailblazing SpectatorJuly will see the launch of the groundbreaking Solar EruptioN Integral Field Spectrograph mission, or SNIFS. Delivered to space via a Black Brant IX sounding rocket, SNIFS will explore the energy and dynamics of the chromosphere, one of the most complex regions of the Sun’s atmosphere. The SNIFS mission’s launch window at the White Sands Missile Range in New Mexico opens on Friday, July 18.
The chromosphere is located between the Sun’s visible surface, or photosphere, and its outer layer, the corona. The different layers of the Sun’s atmosphere have been researched at length, but many questions persist about the chromosphere. “There’s still a lot of unknowns,” said Phillip Chamberlin, a research scientist at the University of Colorado Boulder and principal investigator for the SNIFS mission.
The reddish chromosphere is visible on the Sun’s right edge in this view of the Aug. 21, 2017, total solar eclipse from Madras, Oregon.Credit: NASA/Nat Gopalswamy
The chromosphere lies just below the corona, where powerful solar flares and massive coronal mass ejections are observed. These solar eruptions are the main drivers of space weather, the hazardous conditions in near-Earth space that threaten satellites and endanger astronauts. The SNIFS mission aims to learn more about how energy is converted and moves through the chromosphere, where it can ultimately power these massive explosions.
“To make sure the Earth is safe from space weather, we really would like to be able to model things,” said Vicki Herde, a doctoral graduate of CU Boulder who worked with Chamberlin to develop SNIFS.
To view this video please enable JavaScript, and consider upgrading to a web browser that supports HTML5 video
This footage from NASA’s Solar Dynamics Observatory shows the Sun in the 304-angstrom band of extreme ultraviolet light, which primarily reveals light from the chromosphere. This video, captured on Feb. 22, 2024, shows a solar flare — as seen in the bright flash on the upper left.Credit: NASA/SDOThe SNIFS mission is the first ever solar ultraviolet integral field spectrograph, an advanced technology combining an imager and a spectrograph. Imagers capture photos and videos, which are good for seeing the combined light from a large field of view all at once. Spectrographs dissect light into its various wavelengths, revealing which elements are present in the light source, their temperature, and how they’re moving — but only from a single location at a time.
The SNIFS mission combines these two technologies into one instrument.
“It’s the best of both worlds,” said Chamberlin. “You’re pushing the limit of what technology allows us to do.”
By focusing on specific wavelengths, known as spectral lines, the SNIFS mission will help scientists to learn about the chromosphere. These wavelengths include a spectral line of hydrogen that is the brightest line in the Sun’s ultraviolet (UV) spectrum, and two spectral lines from the elements silicon and oxygen. Together, data from these spectral lines will help reveal how the chromosphere connects with upper atmosphere by tracing how solar material and energy move through it.
The SNIFS mission will be carried into space by a sounding rocket. These rockets are effective tools for launching and carrying space experiments and offer a valuable opportunity for hands-on experience, particularly for students and early-career researchers.
(From left to right) Vicki Herde, Joseph Wallace, and Gabi Gonzalez, who worked on the SNIFS mission, stand with the sounding rocket containing the rocket payload at the White Sands Missile Range in New Mexico.Credit: courtesy of Phillip Chamberlin
“You can really try some wild things,” Herde said. “It gives the opportunity to allow students to touch the hardware.”
Chamberlin emphasized how beneficial these types of missions can be for science and engineering students like Herde, or the next generation of space scientists, who “come with a lot of enthusiasm, a lot of new ideas, new techniques,” he said.
The entirety of the SNIFS mission will likely last up to 15 minutes. After launch, the sounding rocket is expected to take 90 seconds to make it to space and point toward the Sun, seven to eight minutes to perform the experiment on the chromosphere, and three to five minutes to return to Earth’s surface.
A previous sounding rocket launch from the White Sands Missile Range in New Mexico. This mission carried a copy of the Extreme Ultraviolet Variability Experiment (EVE).Credit: NASA/University of Colorado Boulder, Laboratory for Atmospheric and Space Physics/James Mason
The rocket will drift around 70 to 80 miles (112 to 128 kilometers) from the launchpad before its return, so mission contributors must ensure it will have a safe place to land. White Sands, a largely empty desert, is ideal.
Herde, who spent four years working on the rocket, expressed her immense excitement for the launch. “This has been my baby.”
By Harper Lawson
NASA’s Goddard Space Flight Center, Greenbelt, Md.
Doing NASA Science brings many rewards. But can taking part in NASA citizen science help…
Article 1 day ago Keep Exploring Discover More Topics From NASAMissions
Humans in Space
Climate Change
Solar System
NASA to Launch SNIFS, Sun’s Next Trailblazing Spectator
4 min read
NASA to Launch SNIFS, Sun’s Next Trailblazing SpectatorJuly will see the launch of the groundbreaking Solar EruptioN Integral Field Spectrograph mission, or SNIFS. Delivered to space via a Black Brant IX sounding rocket, SNIFS will explore the energy and dynamics of the chromosphere, one of the most complex regions of the Sun’s atmosphere. The SNIFS mission’s launch window at the White Sands Missile Range in New Mexico opens on Friday, July 18.
The chromosphere is located between the Sun’s visible surface, or photosphere, and its outer layer, the corona. The different layers of the Sun’s atmosphere have been researched at length, but many questions persist about the chromosphere. “There’s still a lot of unknowns,” said Phillip Chamberlin, a research scientist at the University of Colorado Boulder and principal investigator for the SNIFS mission.
The reddish chromosphere is visible on the Sun’s right edge in this view of the Aug. 21, 2017, total solar eclipse from Madras, Oregon.Credit: NASA/Nat GopalswamyThe chromosphere lies just below the corona, where powerful solar flares and massive coronal mass ejections are observed. These solar eruptions are the main drivers of space weather, the hazardous conditions in near-Earth space that threaten satellites and endanger astronauts. The SNIFS mission aims to learn more about how energy is converted and moves through the chromosphere, where it can ultimately power these massive explosions.
“To make sure the Earth is safe from space weather, we really would like to be able to model things,” said Vicki Herde, a doctoral graduate of CU Boulder who worked with Chamberlin to develop SNIFS.
To view this video please enable JavaScript, and consider upgrading to a web browser that supports HTML5 video
This footage from NASA’s Solar Dynamics Observatory shows the Sun in the 304-angstrom band of extreme ultraviolet light, which primarily reveals light from the chromosphere. This video, captured on Feb. 22, 2024, shows a solar flare — as seen in the bright flash on the upper left.Credit: NASA/SDOThe SNIFS mission is the first ever solar ultraviolet integral field spectrograph, an advanced technology combining an imager and a spectrograph. Imagers capture photos and videos, which are good for seeing the combined light from a large field of view all at once. Spectrographs dissect light into its various wavelengths, revealing which elements are present in the light source, their temperature, and how they’re moving — but only from a single location at a time.
The SNIFS mission combines these two technologies into one instrument.
“It’s the best of both worlds,” said Chamberlin. “You’re pushing the limit of what technology allows us to do.”
By focusing on specific wavelengths, known as spectral lines, the SNIFS mission will help scientists to learn about the chromosphere. These wavelengths include a spectral line of hydrogen that is the brightest line in the Sun’s ultraviolet (UV) spectrum, and two spectral lines from the elements silicon and oxygen. Together, data from these spectral lines will help reveal how the chromosphere connects with upper atmosphere by tracing how solar material and energy move through it.
The SNIFS mission will be carried into space by a sounding rocket. These rockets are effective tools for launching and carrying space experiments and offer a valuable opportunity for hands-on experience, particularly for students and early-career researchers.
(From left to right) Vicki Herde, Joseph Wallace, and Gabi Gonzalez, who worked on the SNIFS mission, stand with the sounding rocket containing the rocket payload at the White Sands Missile Range in New Mexico.Credit: courtesy of Phillip Chamberlin“You can really try some wild things,” Herde said. “It gives the opportunity to allow students to touch the hardware.”
Chamberlin emphasized how beneficial these types of missions can be for science and engineering students like Herde, or the next generation of space scientists, who “come with a lot of enthusiasm, a lot of new ideas, new techniques,” he said.
The entirety of the SNIFS mission will likely last up to 15 minutes. After launch, the sounding rocket is expected to take 90 seconds to make it to space and point toward the Sun, seven to eight minutes to perform the experiment on the chromosphere, and three to five minutes to return to Earth’s surface.
A previous sounding rocket launch from the White Sands Missile Range in New Mexico. This mission carried a copy of the Extreme Ultraviolet Variability Experiment (EVE).Credit: NASA/University of Colorado Boulder, Laboratory for Atmospheric and Space Physics/James Mason
The rocket will drift around 70 to 80 miles (112 to 128 kilometers) from the launchpad before its return, so mission contributors must ensure it will have a safe place to land. White Sands, a largely empty desert, is ideal.
Herde, who spent four years working on the rocket, expressed her immense excitement for the launch. “This has been my baby.”
By Harper Lawson
NASA’s Goddard Space Flight Center, Greenbelt, Md.
Doing NASA Science brings many rewards. But can taking part in NASA citizen science help…
Article 1 day ago Keep Exploring Discover More Topics From NASAMissions
Humans in Space
Climate Change
Solar System
What has Webb Taught Us About Rocky Exoplanets So Far?
The JWST has pushed the boundaries of exoplanet characterization. But one thing it hasn't done yet is to determine if rocky exoplanets close to our Solar System can retain their atmospheres. The authors of a new study propose a new "five-scale height challenge" that will help astronomers obtain more precise atmospheric information on rocky exoplanets using Webb.
Satellite Constellations Are Too Bright, Threatening Astronomy and Our Night Sky
Our quest for universal internet is stealing the stars. Thousands of satellites now travelling across the night sky are far brighter than international safety limits, turning what was once humanity's window to the cosmos into a highway of artificial lights. New research reveals that major constellations like Starlink and OneWeb are breaking the brightness rules designed to protect both cutting edge astronomy and the simple joy of stargazing potentially robbing future generations of the dark skies that have inspired wonder for centuries.
Scientists Solve 400 Year Old Solar Mystery
For over four centuries, the dark blemishes on our Sun's surface have puzzled astronomers. Now, German scientists have cracked the code behind sunspot stability, revealing how these Earth sized magnetic monsters, each powerful enough to rival an MRI machine yet spanning areas larger than our entire planet, maintain their grip on the solar surface for weeks or months at a time. This breakthrough not only solves one of astronomy's oldest mysteries but could revolutionize our ability to predict the explosive solar storms that threaten our satellite dependent world.
Earth Was Born With Water; No Delivery Needed
The source of Earth's water is one of the most compelling questions facing scientists. Earth's habitability depends on multiple factors, but water is the basis for life, and it had to come from somewhere. Did comets and meteorites deliver it after Earth formed? Or did water become part of our planet as it formed?
A Lunar Base Could Start with a Dome over a Crater Made of Regolith
When astronauts live on the Moon permanently, they're going to need a safe habitat, ideally made out of local construction material. A new paper suggests that lunar astronauts could cover a 17-meter crater with a dome made from a lunar regolith-based geopolymer. A 3D printer would extrude a paste made of lunar regolith that would be sintered together into the shape of the dome. This would provide protection from radiation and could even maintain a pressurized habitat.
This Earth-sized Exoplanet is On a Death Spiral
An international team of astronomers have discovered an Earth-size exoplanet on a very tight orbit around its star. It completes an orbit in only 5 hours and 22 minutes. Unfortunately, the planet will either be torn to pieces or crash into its star in about 31 million years.
2 billion-year-old moon rock found in Africa reveals secret lunar history
Brain Activity Patterns Reveal Why Waking Up from Sleep Can Be So Difficult
Neuroscientists have found that the brain can wake up in different ways, explaining why some mornings feel like a dream and some feel like a disaster
Space Station Crew Celebrates Milestone
Space Station Crew Celebrates Milestone
In this June 13, 2025, photo, NASA astronaut Anne McClain shows off a hamburger-shaped cake to celebrate 200 cumulative days in space for JAXA (Japan Aerospace Exploration Agency) astronaut Takuya Onishi since his first spaceflight as an Expedition 48-49 Flight Engineer in 2016.
Onishi and McClain launched to the International Space Station along with NASA astronaut Nichole Ayers and Roscosmos cosmonaut Kirill Peskov on March 14, 2025, as part of the Crew-10 mission. Aboard the orbital laboratory, the Crew-10 members conduct scientific research to prepare for human exploration beyond low Earth orbit and benefit humanity on Earth. McClain and Ayers also performed a spacewalk on May 1, 2025 – McClain’s third and Ayers’ first.
Check out the International Space Station blog to follow the crew’s research and other activities.
Image credit: NASA/Jonny Kim
Space Station Crew Celebrates Milestone
In this June 13, 2025, photo, NASA astronaut Anne McClain shows off a hamburger-shaped cake to celebrate 200 cumulative days in space for JAXA (Japan Aerospace Exploration Agency) astronaut Takuya Onishi since his first spaceflight as an Expedition 48-49 Flight Engineer in 2016.
Onishi and McClain launched to the International Space Station along with NASA astronaut Nichole Ayers and Roscosmos cosmonaut Kirill Peskov on March 14, 2025, as part of the Crew-10 mission. Aboard the orbital laboratory, the Crew-10 members conduct scientific research to prepare for human exploration beyond low Earth orbit and benefit humanity on Earth. McClain and Ayers also performed a spacewalk on May 1, 2025 – McClain’s third and Ayers’ first.
Check out the International Space Station blog to follow the crew’s research and other activities.
Image credit: NASA/Jonny Kim