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Trump Wants Venezuela’s Oil. Why Does It Have So Much?
Trump has cited Venezuela’s oil resources as motivation for capturing the nation’s leader—here’s the geology behind the news
How New Public Health Changes Could Leave Vulnerable Children Behind
A look at how evolving national health policies could reshape the future of kids’ care, from vaccines to essential treatments.
‘Microbubbles’ Help Spread Dangerous Microplastics Through Our Water, Study Finds
Water plays a crucial role in how tiny pieces of plastic enter our environment—and us
AI chatbots miss urgent issues in queries about women's health
AI chatbots miss urgent issues in queries about women's health
Sentinel-1's decade of essential data over shifting ice sheets
The extent and speed of ice moving off the ice sheets of Greenland and Antarctica into the sea – an important dynamic for climate and sea-rise modelling – has been captured over a 10-year period by satellites from the Copernicus Sentinel-1 mission.
Sandblasting on Mars
Martian winds can have quite an impact. ESA’s Mars Express has spotted them whipping up sand grains and acting as a cosmic sandblaster, carving out intriguing grooves near Mars’s equator.
CAR T-cell therapy makes ageing guts heal themselves
CAR T-cell therapy makes ageing guts heal themselves
Algae Swirls Across a South African Reservoir
- Earth
- Earth Observatory
- Image of the Day
- EO Explorer
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Algae Swirls Across a South African Reservoir
- Earth
- Earth Observatory
- Image of the Day
- EO Explorer
- Topics
- More Content
- About
Does Free Will Exist? Part 1: The Clockwork Universe
Check this out. There are some experiments that just make you…stop. That make you reconsider everything you’ve ever known.
Astronomers Discover a Bright Supernova Using Gravitational Lensing for the First Time
An international team of astronomers using a combination of ground-based telescopes, including the W. M. Keck Observatory on Maunakea, Hawaiʻi Island, has discovered the first-ever spatially resolved, gravitationally lensed superluminous supernova. The object, dubbed SN 2025wny, offers a rare look at a stellar cataclysm from the early Universe and provides a striking confirmation of Einstein’s theory of general relativity.
As Puzzling As A Platypus: The JWST Finds Some Hard To Categorize Objects
Astronomers found a handful of unusual objects in JWST survey data. These 9 point sources are being called 'Astronomy's Platypus' because, like the animal, they seem to defy categorization. They're not like active galactic nuclei, and they're not like star-forming galaxies. What are they?
Supernova Remnant Video From NASA’s Chandra Is Decades in Making
To view this video please enable JavaScript, and consider upgrading to a web browser that supports HTML5 video
A new video shows changes in Kepler’s Supernova Remnant using data from NASA’s Chandra X-ray Observatory captured over more than two and a half decades with observations taken in 2000, 2004, 2006, 2014, and 2025. In this video, which is the longest-spanning one ever released by Chandra, X-rays (blue) from the telescope have been combined with an optical image (red, green, and blue) from Pan-STARRS. X-ray: NASA/CXC/SAO; Optical: Pan-STARRSA new video shows the evolution of Kepler’s Supernova Remnant using data from NASA’s Chandra X-ray Observatory captured over more than two and a half decades.
Kepler’s Supernova Remnant, named after the German astronomer Johannes Kepler, was first spotted in the night sky in 1604. Today, astronomers know that a white dwarf star exploded when it exceeded a critical mass, after pulling material from a companion star, or merging with another white dwarf. This kind of supernova is known as a Type Ia, and scientists use it to measure the expansion of the universe.
Supernova remnants, the debris fields left behind after a stellar explosion, often glow strongly in X-ray light because the material has been heated to millions of degrees from the blast. The remnant is located in our galaxy, about 17,000 light-years from Earth, allowing Chandra to make detailed images of the debris and how it changes with time. This latest video includes its X-ray data from 2000, 2004, 2006, 2014, and 2025. This makes it the longest-spanning video that Chandra has ever released, enabled by Chandra’s longevity.
“The plot of Kepler’s story is just now beginning to unfold,” said Jessye Gassel, a graduate student at George Mason University in Virginia, who led the work. “It’s remarkable that we can watch as these remains from this shattered star crash into material already thrown out into space.” Gassel presented the new Chandra video and the associated research at the 247th meeting of the American Astronomical Society in Phoenix.
The researchers used the video to show that the fastest parts of the remnant are traveling at about 13.8 million miles per hour (2% of the speed of light), moving toward the bottom of the image. Meanwhile, the slowest parts are traveling toward the top at about 4 million miles per hour (0.5% of the speed of light). This large difference in speed is because the gas that the remnant is plowing into toward the top of the image is denser than the gas toward the bottom. This gives scientists information about the environments into which this star exploded.
“Supernova explosions and the elements they hurl into space are the lifeblood of new stars and planets,” said Brian Williams of NASA’s Goddard Space Flight Center in Greenbelt, Maryland, and principal investigator of the new Chandra observations of Kepler. “Understanding exactly how they behave is crucial to knowing our cosmic history.”
The team also examined the widths of the rims forming the blast wave of the explosion. The blast wave is the leading edge of the explosion and the first to encounter material outside of the star. By measuring how wide it is and how fast it is traveling, astronomers glean more information about both the explosion of the star and its surroundings.
NASA’s Marshall Space Flight Center in Huntsville, Alabama, manages the Chandra program. The Smithsonian Astrophysical Observatory’s Chandra X-ray Center controls science operations from Cambridge, Massachusetts, and flight operations from Burlington, Massachusetts.
To learn more about Chandra, visit:
https://science.nasa.gov/chandra
Read more from NASA’s Chandra X-ray Observatory
Learn more about the Chandra X-ray Observatory and its mission here:
Visual DescriptionThis release features a ten second silent video of Kepler’s expanding Supernova Remnant, located in our own galaxy, about 17,000 light-years from Earth. The video was created using X-ray data gathered in 2000, 2004, 2006, 2014, and 2025. Those distinct datasets were turned into highly-detailed visuals, creating a 25-year timelapse-style video of the growing remnant.
Kepler’s Supernova Remnant was once a white dwarf star that exploded when it exceeded its critical mass. Here, in X-ray light, the remnant resembles a cloudy neon blue ring with a diagonal cross line stretching from our upper right down to our lower left. The ring appears thinner and wispier at the bottom, with a band of white arching across the top.
As the video plays, cycling through the 5 datasets, the ring subtly, but clearly, expands, like a slowly inflating balloon. In the video, this sequence is replayed several times with dates included at our lower right, to give sighted learners time to absorb the visual information. Upon close inspection, researchers have determined that the bottom of the remnant is expanding fastest; about 13.8 million miles per hour, or 2% of the speed of light. The top of the ring appears to be expanding the slowest; about 4 million miles per hour, or 0.5% of the speed of light. The large difference in speed is because the gas that the remnant is plowing into towards the top of the image is denser than the gas towards the bottom.
Collecting and interpreting this data over decades has provided information about the environment into which the white dwarf star exploded, and has helped scientists understand how remnants change with time.
Share Details Last Updated Jan 06, 2026 EditorLee MohonContactJoel WallaceLocationMarshall Space Flight Center Related Terms Explore More 4 min read 25 Years in Orbit: Science, Innovation, and the Future of Exploration Article 24 hours ago 6 min read NASA Marshall Prepares for Demolition of Historic Test, Simulation Facilities Article 2 days ago 5 min read Scientists Identify ‘Astronomy’s Platypus’ with NASA’s Webb TelescopeAfter combing through NASA’s James Webb Space Telescope’s archive of sweeping extragalactic cosmic fields, a…
Article 2 days ago Keep Exploring Discover More Topics From NASA ChandraSpace Telescope
Hubble Space TelescopeHubble, the observatory, is the first major optical telescope to be placed in space, the ultimate mountaintop. Above the distortion…
James Webb Space TelescopeWebb is the premier observatory of the next decade, serving thousands of astronomers worldwide. It studies every phase in the…
Spitzer Space TelescopeSpitzer uses an ultra-sensitive infrared telescope to study asteroids, comets, planets and distant galaxies.
Supernova Remnant Video From NASA’s Chandra Is Decades in Making
To view this video please enable JavaScript, and consider upgrading to a web browser that supports HTML5 video
A new video shows changes in Kepler’s Supernova Remnant using data from NASA’s Chandra X-ray Observatory captured over more than two and a half decades with observations taken in 2000, 2004, 2006, 2014, and 2025. In this video, which is the longest-spanning one ever released by Chandra, X-rays (blue) from the telescope have been combined with an optical image (red, green, and blue) from Pan-STARRS. X-ray: NASA/CXC/SAO; Optical: Pan-STARRSA new video shows the evolution of Kepler’s Supernova Remnant using data from NASA’s Chandra X-ray Observatory captured over more than two and a half decades.
Kepler’s Supernova Remnant, named after the German astronomer Johannes Kepler, was first spotted in the night sky in 1604. Today, astronomers know that a white dwarf star exploded when it exceeded a critical mass, after pulling material from a companion star, or merging with another white dwarf. This kind of supernova is known as a Type Ia, and scientists use it to measure the expansion of the universe.
Supernova remnants, the debris fields left behind after a stellar explosion, often glow strongly in X-ray light because the material has been heated to millions of degrees from the blast. The remnant is located in our galaxy, about 17,000 light-years from Earth, allowing Chandra to make detailed images of the debris and how it changes with time. This latest video includes its X-ray data from 2000, 2004, 2006, 2014, and 2025. This makes it the longest-spanning video that Chandra has ever released, enabled by Chandra’s longevity.
“The plot of Kepler’s story is just now beginning to unfold,” said Jessye Gassel, a graduate student at George Mason University in Virginia, who led the work. “It’s remarkable that we can watch as these remains from this shattered star crash into material already thrown out into space.” Gassel presented the new Chandra video and the associated research at the 247th meeting of the American Astronomical Society in Phoenix.
The researchers used the video to show that the fastest parts of the remnant are traveling at about 13.8 million miles per hour (2% of the speed of light), moving toward the bottom of the image. Meanwhile, the slowest parts are traveling toward the top at about 4 million miles per hour (0.5% of the speed of light). This large difference in speed is because the gas that the remnant is plowing into toward the top of the image is denser than the gas toward the bottom. This gives scientists information about the environments into which this star exploded.
“Supernova explosions and the elements they hurl into space are the lifeblood of new stars and planets,” said Brian Williams of NASA’s Goddard Space Flight Center in Greenbelt, Maryland, and principal investigator of the new Chandra observations of Kepler. “Understanding exactly how they behave is crucial to knowing our cosmic history.”
The team also examined the widths of the rims forming the blast wave of the explosion. The blast wave is the leading edge of the explosion and the first to encounter material outside of the star. By measuring how wide it is and how fast it is traveling, astronomers glean more information about both the explosion of the star and its surroundings.
NASA’s Marshall Space Flight Center in Huntsville, Alabama, manages the Chandra program. The Smithsonian Astrophysical Observatory’s Chandra X-ray Center controls science operations from Cambridge, Massachusetts, and flight operations from Burlington, Massachusetts.
To learn more about Chandra, visit:
https://science.nasa.gov/chandra
Read more from NASA’s Chandra X-ray Observatory
Learn more about the Chandra X-ray Observatory and its mission here:
Visual DescriptionThis release features a ten second silent video of Kepler’s expanding Supernova Remnant, located in our own galaxy, about 17,000 light-years from Earth. The video was created using X-ray data gathered in 2000, 2004, 2006, 2014, and 2025. Those distinct datasets were turned into highly-detailed visuals, creating a 25-year timelapse-style video of the growing remnant.
Kepler’s Supernova Remnant was once a white dwarf star that exploded when it exceeded its critical mass. Here, in X-ray light, the remnant resembles a cloudy neon blue ring with a diagonal cross line stretching from our upper right down to our lower left. The ring appears thinner and wispier at the bottom, with a band of white arching across the top.
As the video plays, cycling through the 5 datasets, the ring subtly, but clearly, expands, like a slowly inflating balloon. In the video, this sequence is replayed several times with dates included at our lower right, to give sighted learners time to absorb the visual information. Upon close inspection, researchers have determined that the bottom of the remnant is expanding fastest; about 13.8 million miles per hour, or 2% of the speed of light. The top of the ring appears to be expanding the slowest; about 4 million miles per hour, or 0.5% of the speed of light. The large difference in speed is because the gas that the remnant is plowing into towards the top of the image is denser than the gas towards the bottom.
Collecting and interpreting this data over decades has provided information about the environment into which the white dwarf star exploded, and has helped scientists understand how remnants change with time.
Share Details Last Updated Jan 06, 2026 EditorLee MohonContactJoel WallaceLocationMarshall Space Flight Center Related Terms Explore More 4 min read 25 Years in Orbit: Science, Innovation, and the Future of Exploration Article 1 day ago 6 min read NASA Marshall Prepares for Demolition of Historic Test, Simulation Facilities Article 2 days ago 5 min read Scientists Identify ‘Astronomy’s Platypus’ with NASA’s Webb TelescopeAfter combing through NASA’s James Webb Space Telescope’s archive of sweeping extragalactic cosmic fields, a…
Article 2 days ago Keep Exploring Discover More Topics From NASA ChandraSpace Telescope
Hubble Space TelescopeHubble, the observatory, is the first major optical telescope to be placed in space, the ultimate mountaintop. Above the distortion…
James Webb Space TelescopeWebb is the premier observatory of the next decade, serving thousands of astronomers worldwide. It studies every phase in the…
Spitzer Space TelescopeSpitzer uses an ultra-sensitive infrared telescope to study asteroids, comets, planets and distant galaxies.
NASA Awards Launch Range Contract for Wallops Flight Facility
NASA has selected ARES Technical Services Corporation of McLean, Virginia, to provide launch range operations support at the agency’s Wallops Flight Facility in Virginia.
The Wallops Range Contract has a total potential value of $339.8 million with a one-year base period expected to begin Tuesday, Feb. 10, and four one-year option periods that if exercised would extend it to 2031. The contract includes a cost-plus-fixed-fee core with an indefinite-delivery/indefinite-quantity component and the ability to issue cost-plus-fixed-fee or firm-fixed-price task orders.
The scope of the work includes launch range operations support such as radar, telemetry, logistics, tracking, and communications services for flight vehicles including orbital and suborbital rockets, aircraft, satellites, balloons, and unmanned aerial systems. Additional responsibilities include information and computer systems services; testing, modifying, and installing communications and electronic systems at launch facilities, launch control centers, and test facilities; and range technology sustainment engineering services.
Work will primarily occur at NASA Wallops with additional support at sites such as the agency’s Bermuda Tracking Station, Poker Flat Research Range in Alaska, and other temporary duty locations.
For information about NASA and agency programs, visit:
-end-
Tiernan Doyle
Headquarters, Washington
202-358-1600
tiernan.doyle@nasa.gov
Robert Garner
Goddard Space Flight Center, Greenbelt, Md.
301-286-5687
rob.garner@nasa.gov
NASA Awards Launch Range Contract for Wallops Flight Facility
NASA has selected ARES Technical Services Corporation of McLean, Virginia, to provide launch range operations support at the agency’s Wallops Flight Facility in Virginia.
The Wallops Range Contract has a total potential value of $339.8 million with a one-year base period expected to begin Tuesday, Feb. 10, and four one-year option periods that if exercised would extend it to 2031. The contract includes a cost-plus-fixed-fee core with an indefinite-delivery/indefinite-quantity component and the ability to issue cost-plus-fixed-fee or firm-fixed-price task orders.
The scope of the work includes launch range operations support such as radar, telemetry, logistics, tracking, and communications services for flight vehicles including orbital and suborbital rockets, aircraft, satellites, balloons, and unmanned aerial systems. Additional responsibilities include information and computer systems services; testing, modifying, and installing communications and electronic systems at launch facilities, launch control centers, and test facilities; and range technology sustainment engineering services.
Work will primarily occur at NASA Wallops with additional support at sites such as the agency’s Bermuda Tracking Station, Poker Flat Research Range in Alaska, and other temporary duty locations.
For information about NASA and agency programs, visit:
-end-
Tiernan Doyle
Headquarters, Washington
202-358-1600
tiernan.doyle@nasa.gov
Robert Garner
Goddard Space Flight Center, Greenbelt, Md.
301-286-5687
rob.garner@nasa.gov
Starless ‘Cloud-9’ Is an Entirely New Astrophysical Object
Scientists have found the best evidence yet for long-predicted “failed galaxies”