NASA
Sunrise on Crew-11 Launch Attempt
NASA Installs Key ‘Sunblock’ Shield on Roman Space Telescope
Technicians have successfully installed two sunshields onto NASA’s Nancy Grace Roman Space Telescope’s inner segment. Along with the observatory’s Solar Array Sun Shield and Deployable Aperture Cover, the panels (together called the Lower Instrument Sun Shade), will play a critical role in keeping Roman’s instruments cool and stable as the mission explores the infrared universe.
To view this video please enable JavaScript, and consider upgrading to a web browser that supports HTML5 video
This video shows technicians installing two sunshields onto NASA's nearly complete Nancy Grace Roman Space Telescope on July 17. The large yet lightweight panels will block sunlight, keeping Roman’s instruments cool and stable as the mission explores the infrared universe.Credit: NASA/Sophia RobertsThe team is on track to join Roman’s outer and inner assemblies this fall to complete the full observatory, which can then undergo further prelaunch testing.
“This shield is like an extremely strong sunblock for Roman’s sensitive instruments, protecting them from heat and light from the Sun that would otherwise overwhelm our ability to detect faint signals from space,” said Matthew Stephens, an aerospace engineer at NASA’s Goddard Space Flight Center in Greenbelt, Maryland.
The sunshade, which was designed and engineered at NASA Goddard, is essentially an extension of Roman’s solar panels, except without solar cells. Each sunshade flap is roughly the size of a garage door — about 7 by 7 feet (2.1 by 2.1 meters) — and 3 inches (7.6 centimeters) thick.
“They’re basically giant aluminum sandwiches, with metal sheets as thin as a credit card on the top and bottom and the central portion made up of a honeycomb structure,” said Conrad Mason, an aerospace engineer at NASA Goddard.
This design makes the panels lightweight yet stiff, and the material helps limit heat transfer from the side facing the Sun to the back—no small feat considering the front will be hot enough to boil water (up to 216 degrees Fahrenheit, or 102 degrees Celsius) while the back will be much colder than Antarctica’s harshest winter (minus 211 Fahrenheit, or minus 135 Celsius). A specialized polymer film blanket will wrap around each panel to temper the heat, with 17 layers on the Sun side and one on the shaded side.
The sunshade will be stowed and gently deploy around an hour after launch.
To view this video please enable JavaScript, and consider upgrading to a web browser that supports HTML5 video
In this time-lapse video, technicians manually deploy the Lower Instrument Sun Shield for NASA's Nancy Grace Roman Space Telescope. The test helps verify the panels will operate as designed in space.NASA/Sophia Roberts“The deploying mechanisms have dampers that work like soft-close hinges for drawers or cabinets, so the panels won’t slam open and rattle the observatory,” Stephens said. “They each take about two minutes to move into their final positions. This is the very first system that Roman will deploy in space after the spacecraft separates from the launch vehicle.”
Now completely assembled, Roman’s inner segment is slated to undergo a 70-day thermal vacuum test next. Engineers and scientists will test the full functionality of the spacecraft, telescope, and instruments under simulated space conditions. Following the test, the sunshade will be temporarily removed while the team joins Roman’s outer and inner assemblies, and then reattached to complete the observatory. The mission remains on track for launch no later than May 2027 with the team aiming for as early as fall 2026.
Click here to virtually tour an interactive version of the telescopeDownload high-resolution video and images from NASA’s Scientific Visualization Studio
The Nancy Grace Roman Space Telescope is managed at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, with participation by NASA’s Jet Propulsion Laboratory in Southern California; Caltech/IPAC in Pasadena, California; the Space Telescope Science Institute in Baltimore; and a science team comprising scientists from various research institutions. The primary industrial partners are BAE Systems Inc. in Boulder, Colorado; L3Harris Technologies in Rochester, New York; and Teledyne Scientific & Imaging in Thousand Oaks, California.
By Ashley Balzer
NASA’s Goddard Space Flight Center, Greenbelt, Md.
NASA Installs Key ‘Sunblock’ Shield on Roman Space Telescope
Technicians have successfully installed two sunshields onto NASA’s Nancy Grace Roman Space Telescope’s inner segment. Along with the observatory’s Solar Array Sun Shield and Deployable Aperture Cover, the panels (together called the Lower Instrument Sun Shade), will play a critical role in keeping Roman’s instruments cool and stable as the mission explores the infrared universe.
To view this video please enable JavaScript, and consider upgrading to a web browser that supports HTML5 video
This video shows technicians installing two sunshields onto NASA's nearly complete Nancy Grace Roman Space Telescope on July 17. The large yet lightweight panels will block sunlight, keeping Roman’s instruments cool and stable as the mission explores the infrared universe.Credit: NASA/Sophia RobertsThe team is on track to join Roman’s outer and inner assemblies this fall to complete the full observatory, which can then undergo further prelaunch testing.
“This shield is like an extremely strong sunblock for Roman’s sensitive instruments, protecting them from heat and light from the Sun that would otherwise overwhelm our ability to detect faint signals from space,” said Matthew Stephens, an aerospace engineer at NASA’s Goddard Space Flight Center in Greenbelt, Maryland.
The sunshade, which was designed and engineered at NASA Goddard, is essentially an extension of Roman’s solar panels, except without solar cells. Each sunshade flap is roughly the size of a garage door — about 7 by 7 feet (2.1 by 2.1 meters) — and 3 inches (7.6 centimeters) thick.
“They’re basically giant aluminum sandwiches, with metal sheets as thin as a credit card on the top and bottom and the central portion made up of a honeycomb structure,” said Conrad Mason, an aerospace engineer at NASA Goddard.
This design makes the panels lightweight yet stiff, and the material helps limit heat transfer from the side facing the Sun to the back—no small feat considering the front will be hot enough to boil water (up to 216 degrees Fahrenheit, or 102 degrees Celsius) while the back will be much colder than Antarctica’s harshest winter (minus 211 Fahrenheit, or minus 135 Celsius). A specialized polymer film blanket will wrap around each panel to temper the heat, with 17 layers on the Sun side and one on the shaded side.
The sunshade will be stowed and gently deploy around an hour after launch.
To view this video please enable JavaScript, and consider upgrading to a web browser that supports HTML5 video
In this time-lapse video, technicians manually deploy the Lower Instrument Sun Shield for NASA's Nancy Grace Roman Space Telescope. The test helps verify the panels will operate as designed in space.NASA/Sophia Roberts“The deploying mechanisms have dampers that work like soft-close hinges for drawers or cabinets, so the panels won’t slam open and rattle the observatory,” Stephens said. “They each take about two minutes to move into their final positions. This is the very first system that Roman will deploy in space after the spacecraft separates from the launch vehicle.”
Now completely assembled, Roman’s inner segment is slated to undergo a 70-day thermal vacuum test next. Engineers and scientists will test the full functionality of the spacecraft, telescope, and instruments under simulated space conditions. Following the test, the sunshade will be temporarily removed while the team joins Roman’s outer and inner assemblies, and then reattached to complete the observatory. The mission remains on track for launch no later than May 2027 with the team aiming for as early as fall 2026.
Click here to virtually tour an interactive version of the telescopeDownload high-resolution video and images from NASA’s Scientific Visualization Studio
The Nancy Grace Roman Space Telescope is managed at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, with participation by NASA’s Jet Propulsion Laboratory in Southern California; Caltech/IPAC in Pasadena, California; the Space Telescope Science Institute in Baltimore; and a science team comprising scientists from various research institutions. The primary industrial partners are BAE Systems Inc. in Boulder, Colorado; L3Harris Technologies in Rochester, New York; and Teledyne Scientific & Imaging in Thousand Oaks, California.
By Ashley Balzer
NASA’s Goddard Space Flight Center, Greenbelt, Md.
NASA Invites Proposals to Lease Aircraft Hangar in Cleveland
NASA’s Glenn Research Center in Cleveland is seeking proposals for the use of its historic aircraft hangar, along with a parking lot, tarmac, and a small neighboring office building. Proposals are due by 1 p.m. EDT on Nov. 28.
The hangar, formally known as the Flight Research Building, is available for lease by signing a National Historic Preservation Act agreement for a 10-year base period and two optional five-year extensions.
NASA first announced plans to lease the Flight Research Building and other facilities in May 2024 under the government’s Enhanced Use Lease authority. These lease agreements allow space, aeronautics, and other related industries to use agency land and facilities, reducing NASA’s maintenance costs while fostering strategic partnerships that spur innovation.
“Glenn is making great progress as we modernize our Cleveland and Sandusky campuses to support NASA’s future missions,” said Dr. Jimmy Kenyon, Glenn’s center director. “Through Enhanced Use Leases, we’re ensuring full use of land and facilities while preserving an iconic, historic building and creating regional economic opportunities.”
The property available for lease includes up to 6.7 acres of land, which contains the heated aircraft hangar, Operations and Integration Building, parking lot, and tarmac. The hangar is 160 feet by 280 feet, and the Operations and Integration Building is 5,947 square feet. Proceeds from this lease will be used to maintain Glenn facilities and infrastructure.
Visible from Brookpark Road and Cleveland Hopkins International Airport, Glenn’s hangar was the first building completed after the center was established in 1941. It has sheltered many unique aircraft used to perform vital research. From studying ice accumulation on aircraft wings to the first use of laser communications to stream 4K video from an aircraft to the International Space Station, Glenn flight research has contributed to aviation safety, atmospheric studies, and cutting-edge technology development.
Interested parties should contact both Carlos Flores at carlos.a.flores-1@nasa.gov and Diana Munro at diana.c.munro@nasa.gov to sign up for a walk-through from Monday, Sept. 8, to Friday, Sept. 12, or the week of Oct. 6.
For a 360-degree virtual tour of the Flight Research Building, visit:
https://www3.nasa.gov/specials/hangar360/
-end-
Jan Wittry
Glenn Research Center, Cleveland
216-433-5466
jan.m.wittry-1@nasa.gov
Missions
Humans in Space
Climate Change
Solar System
NASA Invites Proposals to Lease Aircraft Hangar in Cleveland
NASA’s Glenn Research Center in Cleveland is seeking proposals for the use of its historic aircraft hangar, along with a parking lot, tarmac, and a small neighboring office building. Proposals are due by 1 p.m. EDT on Nov. 28.
The hangar, formally known as the Flight Research Building, is available for lease by signing a National Historic Preservation Act agreement for a 10-year base period and two optional five-year extensions.
NASA first announced plans to lease the Flight Research Building and other facilities in May 2024 under the government’s Enhanced Use Lease authority. These lease agreements allow space, aeronautics, and other related industries to use agency land and facilities, reducing NASA’s maintenance costs while fostering strategic partnerships that spur innovation.
“Glenn is making great progress as we modernize our Cleveland and Sandusky campuses to support NASA’s future missions,” said Dr. Jimmy Kenyon, Glenn’s center director. “Through Enhanced Use Leases, we’re ensuring full use of land and facilities while preserving an iconic, historic building and creating regional economic opportunities.”
The property available for lease includes up to 6.7 acres of land, which contains the heated aircraft hangar, Operations and Integration Building, parking lot, and tarmac. The hangar is 160 feet by 280 feet, and the Operations and Integration Building is 5,947 square feet. Proceeds from this lease will be used to maintain Glenn facilities and infrastructure.
Visible from Brookpark Road and Cleveland Hopkins International Airport, Glenn’s hangar was the first building completed after the center was established in 1941. It has sheltered many unique aircraft used to perform vital research. From studying ice accumulation on aircraft wings to the first use of laser communications to stream 4K video from an aircraft to the International Space Station, Glenn flight research has contributed to aviation safety, atmospheric studies, and cutting-edge technology development.
Interested parties should contact both Carlos Flores at carlos.a.flores-1@nasa.gov and Diana Munro at diana.c.munro@nasa.gov to sign up for a walk-through from Monday, Sept. 8, to Friday, Sept. 12, or the week of Oct. 6.
For a 360-degree virtual tour of the Flight Research Building, visit:
https://www3.nasa.gov/specials/hangar360/
-end-
Jan Wittry
Glenn Research Center, Cleveland
216-433-5466
jan.m.wittry-1@nasa.gov
Missions
Humans in Space
Climate Change
Solar System
NASA Releases Opportunity to Boost Commercial Space Tech Development
5 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater) Credit: NASANASA has released a new proposal opportunity for industry to tap into agency know-how, resources, and expertise. The Announcement of Collaboration Opportunity (ACO), managed by the Space Technology Mission Directorate, enables valuable collaboration without financial exchanges between NASA and industry partners. Instead, companies leverage NASA subject matter experts, facilities, software, and hardware to accelerate their technologies and prepare them for future commercial and government use.
On Wednesday, NASA issued a standing ACO announcement for partnership proposals which will be available for five years and will serve as the umbrella opportunity for topic-specific appendix releases. NASA intends to issue appendices every six to 12 months to address evolving space technology needs. The 2025 ACO appendix is open for proposals until Sept. 24.
NASA will host an informational webinar about the opportunity and appendix at 2 p.m. EDT on Wednesday, Aug. 6. Interested proposers are encouraged to submit questions which will be answered during the webinar and will be available online after the webinar.
NASA teaming with industry isn’t new – decades of partnerships have resulted in ambitious missions that benefit all of humanity. But in recent years, NASA has also played a key role as a technology enabler, providing one-of-a-kind tools, resources, and infrastructure to help commercial aerospace companies achieve their goals.
Since 2015, NASA has collaborated with industry on approximately 80 ACO projects. Here are some ways the collaborations have advanced space technology:
Lunar lander systemsBlue Origin and NASA worked together on several ACOs to mature the company’s lunar lander design. NASA provided technical reports and assessments and conducted tests at multiple centers to help Blue Origin advance a stacked fuel cell system for a lander’s primary power source. Other Blue Origin ACO projects evaluated high-temperature engine materials and advanced a landing navigation and guidance system.
Blue Origin’s Blue Moon Mark 1 (MK1) lander is delivering NASA science and technology to the Moon through the agency’s Commercial Lunar Payload Services initiative. In 2023, NASA selected Blue Origin as a Human Landing System provider to develop its Blue Moon MK2 lander for future crewed lunar exploration.
Artist concept of Blue Origin’s Blue Moon Mark 1 (MK1) lander.Credit: Blue Origin Cryogenic fluid transferThroughout a year-long ACO, NASA and SpaceX engineers worked together to perform in-depth computational fluid analysis of proposed propellant transfer methods between two SpaceX Starship spacecraft in low-Earth orbit. The SpaceX-specific analysis utilized Starship flight data and data from previous NASA research and development to identify potential risks and help mitigate them during the early stages of commercial development. NASA also provided inputs as SpaceX developed an initial concept of operations for its orbital propellant transfer missions.
SpaceX used the ACO analyses to inform the design of its Starship Human Landing System, which NASA selected in 2021 to put the first Artemis astronauts on the Moon.
This artist’s concept depicts a SpaceX Starship tanker (bottom) transferring propellant to a Starship depot (top) in low Earth orbit. Before astronauts launch in Orion atop the agency’s SLS (Space Launch System) rocket, SpaceX will launch a storage depot to Earth orbit. For the Artemis III and Artemis IV missions, SpaceX plans to complete propellant loading operations in Earth orbit to send a fully fueled Starship Human Landing System (HLS) to the Moon.Credit: SpaceX Autonomous spacecraft navigation solutionAdvanced Space and NASA partnered to advance the company’s Cislunar Autonomous Positioning System – software that allows lunar spacecraft to determine their location without relying exclusively on tracking from Earth.
Dylan Schmidt, CAPSTONE assembly integration and test lead, installs solar panels onto the CAPSTONE spacecraft at Tyvak Nano-Satellite Systems, Inc., in Irvine, California.NASA/Dominic HartThe CAPSTONE (Cislunar Autonomous Positioning System Technology Operations and Navigation Experiment) spacecraft launched to the Moon in 2022 and continues to operate and collect critical data to refine the software. Under the ACO, Advanced Space was able to use NASA’s Lunar Reconnaissance Orbiter to conduct crosslink experiments with CAPSTONE, helping mature the navigation solution for future missions. The mission’s Cislunar Autonomous Positioning System technology was initially supported through the NASA Small Business Innovation Research program.
Multi-purpose laser sensing systemSensuron and NASA matured a miniature, rugged fiber optic sensing system capable of taking thermal and shape measurements for multiple applications. Throughout the ACO, Sensuron benefitted from NASA’s expertise in fiber optics and electrical, mechanical, and system testing engineering to design, fabricate, and “shake and bake” its prototype laser.
Sensuron Ruggedized Fiber Optics Sensing System.SensuronSpace missions could use the technology to monitor cryogenic propellant levels and determine a fuel tank’s structural integrity throughout an extended mission. The laser technology also has medical applications on Earth, which ultimately resulted in the Sensuron spinoff company, The Shape Sensing Company.
Flexible lunar tiresIn 2023, Venturi Astrolab began work with NASA under an ACO to test its flexible lunar tire design. The company tapped into testing capabilities unique to NASA, including heat transfer to cold lunar soil, traction, and life testing. The data validated the performance of tire prototypes, helping ready the design to support future NASA missions.
In 2024, NASA selected three companies, including Venturi Astrolab, to advance capabilities for a lunar terrain vehicle that astronauts could use to travel around the lunar surface, conducting scientific research on the Moon and preparing for human missions to Mars.
Venturi Lab designed and developed a durable, robust, and hyper-deformable lunar wheel.Venturi LabThe Announcement of Collaboration Opportunity (ACO) is one of many ways NASA enables commercial industry to develop, build, own, and eventually operate space systems. To learn more about these technology projects and more, visit: https://techport.nasa.gov/.
Facebook logo @NASATechnology @NASA_Technology Explore More 2 min read NASA Seeks Industry Concepts on Moon, Mars Communications Article 1 week ago 1 min read USBR Seal Team Fix Challenge Article 1 week ago 4 min read NASA Tests New Heat Source Fuel for Deep Space Exploration Article 1 week ago Share Details Last Updated Jul 31, 2025 EditorJennifer M. Dooren Related TermsNASA Releases Opportunity to Boost Commercial Space Tech Development
5 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater) Credit: NASANASA has released a new proposal opportunity for industry to tap into agency know-how, resources, and expertise. The Announcement of Collaboration Opportunity (ACO), managed by the Space Technology Mission Directorate, enables valuable collaboration without financial exchanges between NASA and industry partners. Instead, companies leverage NASA subject matter experts, facilities, software, and hardware to accelerate their technologies and prepare them for future commercial and government use.
On Wednesday, NASA issued a standing ACO announcement for partnership proposals which will be available for five years and will serve as the umbrella opportunity for topic-specific appendix releases. NASA intends to issue appendices every six to 12 months to address evolving space technology needs. The 2025 ACO appendix is open for proposals until Sept. 24.
NASA will host an informational webinar about the opportunity and appendix at 2 p.m. EDT on Wednesday, Aug. 6. Interested proposers are encouraged to submit questions which will be answered during the webinar and will be available online after the webinar.
NASA teaming with industry isn’t new – decades of partnerships have resulted in ambitious missions that benefit all of humanity. But in recent years, NASA has also played a key role as a technology enabler, providing one-of-a-kind tools, resources, and infrastructure to help commercial aerospace companies achieve their goals.
Since 2015, NASA has collaborated with industry on approximately 80 ACO projects. Here are some ways the collaborations have advanced space technology:
Lunar lander systemsBlue Origin and NASA worked together on several ACOs to mature the company’s lunar lander design. NASA provided technical reports and assessments and conducted tests at multiple centers to help Blue Origin advance a stacked fuel cell system for a lander’s primary power source. Other Blue Origin ACO projects evaluated high-temperature engine materials and advanced a landing navigation and guidance system.
Blue Origin’s Blue Moon Mark 1 (MK1) lander is delivering NASA science and technology to the Moon through the agency’s Commercial Lunar Payload Services initiative. In 2023, NASA selected Blue Origin as a Human Landing System provider to develop its Blue Moon MK2 lander for future crewed lunar exploration.
Artist concept of Blue Origin’s Blue Moon Mark 1 (MK1) lander.Credit: Blue Origin Cryogenic fluid transferThroughout a year-long ACO, NASA and SpaceX engineers worked together to perform in-depth computational fluid analysis of proposed propellant transfer methods between two SpaceX Starship spacecraft in low-Earth orbit. The SpaceX-specific analysis utilized Starship flight data and data from previous NASA research and development to identify potential risks and help mitigate them during the early stages of commercial development. NASA also provided inputs as SpaceX developed an initial concept of operations for its orbital propellant transfer missions.
SpaceX used the ACO analyses to inform the design of its Starship Human Landing System, which NASA selected in 2021 to put the first Artemis astronauts on the Moon.
This artist’s concept depicts a SpaceX Starship tanker (bottom) transferring propellant to a Starship depot (top) in low Earth orbit. Before astronauts launch in Orion atop the agency’s SLS (Space Launch System) rocket, SpaceX will launch a storage depot to Earth orbit. For the Artemis III and Artemis IV missions, SpaceX plans to complete propellant loading operations in Earth orbit to send a fully fueled Starship Human Landing System (HLS) to the Moon.Credit: SpaceX Autonomous spacecraft navigation solutionAdvanced Space and NASA partnered to advance the company’s Cislunar Autonomous Positioning System – software that allows lunar spacecraft to determine their location without relying exclusively on tracking from Earth.
Dylan Schmidt, CAPSTONE assembly integration and test lead, installs solar panels onto the CAPSTONE spacecraft at Tyvak Nano-Satellite Systems, Inc., in Irvine, California.NASA/Dominic HartThe CAPSTONE (Cislunar Autonomous Positioning System Technology Operations and Navigation Experiment) spacecraft launched to the Moon in 2022 and continues to operate and collect critical data to refine the software. Under the ACO, Advanced Space was able to use NASA’s Lunar Reconnaissance Orbiter to conduct crosslink experiments with CAPSTONE, helping mature the navigation solution for future missions. The mission’s Cislunar Autonomous Positioning System technology was initially supported through the NASA Small Business Innovation Research program.
Multi-purpose laser sensing systemSensuron and NASA matured a miniature, rugged fiber optic sensing system capable of taking thermal and shape measurements for multiple applications. Throughout the ACO, Sensuron benefitted from NASA’s expertise in fiber optics and electrical, mechanical, and system testing engineering to design, fabricate, and “shake and bake” its prototype laser.
Sensuron Ruggedized Fiber Optics Sensing System.SensuronSpace missions could use the technology to monitor cryogenic propellant levels and determine a fuel tank’s structural integrity throughout an extended mission. The laser technology also has medical applications on Earth, which ultimately resulted in the Sensuron spinoff company, The Shape Sensing Company.
Flexible lunar tiresIn 2023, Venturi Astrolab began work with NASA under an ACO to test its flexible lunar tire design. The company tapped into testing capabilities unique to NASA, including heat transfer to cold lunar soil, traction, and life testing. The data validated the performance of tire prototypes, helping ready the design to support future NASA missions.
In 2024, NASA selected three companies, including Venturi Astrolab, to advance capabilities for a lunar terrain vehicle that astronauts could use to travel around the lunar surface, conducting scientific research on the Moon and preparing for human missions to Mars.
Venturi Lab designed and developed a durable, robust, and hyper-deformable lunar wheel.Venturi LabThe Announcement of Collaboration Opportunity (ACO) is one of many ways NASA enables commercial industry to develop, build, own, and eventually operate space systems. To learn more about these technology projects and more, visit: https://techport.nasa.gov/.
Facebook logo @NASATechnology @NASA_Technology Explore More 2 min read NASA Seeks Industry Concepts on Moon, Mars Communications Article 1 week ago 1 min read USBR Seal Team Fix Challenge Article 1 week ago 4 min read NASA Tests New Heat Source Fuel for Deep Space Exploration Article 1 week ago Share Details Last Updated Jul 31, 2025 EditorJennifer M. Dooren Related TermsNASA Tests Epic Solution for Supersonic Parachute Deliveries
2 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater)NASA/Lori Losey
The best way to solve a mystery is by gathering evidence and building a case. That’s exactly what NASA researchers are doing with a series of research flights aimed at advancing a sensor for supersonic parachutes. The clues they find could help make these parachutes more reliable and safer for delivering scientific instruments and payloads to Mars.
These investigative research flights are led by the EPIC (Enhancing Parachutes by Instrumenting the Canopy) team at NASA’s Armstrong Fight Research Center in Edwards, California. During a June flight test, a quadrotor aircraft, or drone, air-launched a capsule that deployed a parachute equipped with a sensor. The flexible, strain-measuring sensor attached to the parachute did not interfere with the canopy material, just as the EPIC team had predicted. The sensors also provided data, a bonus for planning upcoming tests.
“Reviewing the research flights will help inform our next steps,” said Matt Kearns, project manager for EPIC at NASA Armstrong. “We are speaking with potential partners to come up with a framework to obtain the data that they are interested in pursuing. Our team members are developing methods for temperature testing the flexible sensors, data analysis, and looking into instrumentation for future tests.”
The flight tests were a first step toward filling gaps in computer models to improve supersonic parachutes. This work could also open the door to future partnerships, including with the aerospace and auto racing industries.
NASA’s Space Technology Mission Directorate (STMD) funds the EPIC work through its Entry Systems Modeling project at NASA’s Ames Research Center in California’s Silicon Valley. The capsule and parachute system were developed by NASA’s Langley Research Center in Hampton, Virginia. NASA Armstrong interns worked with Langley to build and integrate a similar system for testing at NASA Armstrong. An earlier phase of the work focused on finding commercially available flexible strain sensors and developing a bonding method as part of an STMD Early Career Initiative project.
NASA researchers Paul Bean, center, and Mark Hagiwara, right, attach the capsule with parachute system to the Enhancing Parachutes by Instrumenting the Canopy test experiment on June 4, 2025, at NASA’s Armstong Flight Research Center in Edwards, California. NASA researchers are developing technology to make supersonic parachutes safer and more reliable for delivering science instruments and payloads to Mars.NASA/Christopher LC Clark Derek Abramson, left, and Justin Link, right, attach an Alta X drone to the Enhancing Parachutes by Instrumenting the Canopy test experiment on June 4, 2025, at NASA’s Armstong Flight Research Center in Edwards, California. Abramson is NASA chief engineer at the center’s Dale Reed Subscale Flight Research Laboratory, where Link also works as a pilot for small uncrewed aircraft systems. NASA researchers are developing technology to make supersonic parachutes safer and more reliable for delivering science instruments and payloads to Mars.NASA/Christopher LC Clark An Alta X drone is positioned at altitude for an air launch of the Enhancing Parachutes by Instrumenting the Canopy test experiment on June 4, 2025, at NASA’s Armstong Flight Research Center in Edwards, California. NASA researchers are developing technology to make supersonic parachutes safer and more reliable for delivering science instruments and payloads to Mars.NASA/Christopher LC Clark The parachute of the Enhancing Parachutes by Instrumenting the Canopy test experiment deploys following an air launch from an Alta X drone on June 4, 2025, at NASA’s Armstong Flight Research Center in Edwards, California. NASA researchers are developing technology to make supersonic parachutes safer and more reliable for delivering science instruments and payloads to Mars.NASA/Christopher LC Clark The Enhancing Parachutes by Instrumenting the Canopy project team examines a capsule and parachute following an air launch from an Alta X drone on June 4, 2025, at NASA’s Armstong Flight Research Center in Edwards, California. NASA researchers are developing technology to make supersonic parachutes safer and more reliable for delivering science instruments and payloads to Mars.NASA/Christopher LC Clark Share Details Last Updated Jul 29, 2025 EditorDede DiniusContactJay Levinejay.levine-1@nasa.gov Related Terms Explore More 5 min read NASA Releases Opportunity to Boost Commercial Space Tech Development Article 1 day ago 3 min read NASA Drop Test Supports Safer Air Taxi Design and Certification Article 3 days ago 3 min read NASA Rehearses How to Measure X-59’s Noise Levels Article 6 days ago Keep Exploring Discover More Topics From NASAArmstrong Flight Research Center
Humans in Space
Climate Change
Solar System
NASA Tests Epic Solution for Supersonic Parachute Deliveries
2 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater)NASA/Lori Losey
The best way to solve a mystery is by gathering evidence and building a case. That’s exactly what NASA researchers are doing with a series of research flights aimed at advancing a sensor for supersonic parachutes. The clues they find could help make these parachutes more reliable and safer for delivering scientific instruments and payloads to Mars.
These investigative research flights are led by the EPIC (Enhancing Parachutes by Instrumenting the Canopy) team at NASA’s Armstrong Fight Research Center in Edwards, California. During a June flight test, a quadrotor aircraft, or drone, air-launched a capsule that deployed a parachute equipped with a sensor. The flexible, strain-measuring sensor attached to the parachute did not interfere with the canopy material, just as the EPIC team had predicted. The sensors also provided data, a bonus for planning upcoming tests.
“Reviewing the research flights will help inform our next steps,” said Matt Kearns, project manager for EPIC at NASA Armstrong. “We are speaking with potential partners to come up with a framework to obtain the data that they are interested in pursuing. Our team members are developing methods for temperature testing the flexible sensors, data analysis, and looking into instrumentation for future tests.”
The flight tests were a first step toward filling gaps in computer models to improve supersonic parachutes. This work could also open the door to future partnerships, including with the aerospace and auto racing industries.
NASA’s Space Technology Mission Directorate (STMD) funds the EPIC work through its Entry Systems Modeling project at NASA’s Ames Research Center in California’s Silicon Valley. The capsule and parachute system were developed by NASA’s Langley Research Center in Hampton, Virginia. NASA Armstrong interns worked with Langley to build and integrate a similar system for testing at NASA Armstrong. An earlier phase of the work focused on finding commercially available flexible strain sensors and developing a bonding method as part of an STMD Early Career Initiative project.
NASA researchers Paul Bean, center, and Mark Hagiwara, right, attach the capsule with parachute system to the Enhancing Parachutes by Instrumenting the Canopy test experiment on June 4, 2025, at NASA’s Armstong Flight Research Center in Edwards, California. NASA researchers are developing technology to make supersonic parachutes safer and more reliable for delivering science instruments and payloads to Mars.NASA/Christopher LC Clark Derek Abramson, left, and Justin Link, right, attach an Alta X drone to the Enhancing Parachutes by Instrumenting the Canopy test experiment on June 4, 2025, at NASA’s Armstong Flight Research Center in Edwards, California. Abramson is NASA chief engineer at the center’s Dale Reed Subscale Flight Research Laboratory, where Link also works as a pilot for small uncrewed aircraft systems. NASA researchers are developing technology to make supersonic parachutes safer and more reliable for delivering science instruments and payloads to Mars.NASA/Christopher LC Clark An Alta X drone is positioned at altitude for an air launch of the Enhancing Parachutes by Instrumenting the Canopy test experiment on June 4, 2025, at NASA’s Armstong Flight Research Center in Edwards, California. NASA researchers are developing technology to make supersonic parachutes safer and more reliable for delivering science instruments and payloads to Mars.NASA/Christopher LC Clark The parachute of the Enhancing Parachutes by Instrumenting the Canopy test experiment deploys following an air launch from an Alta X drone on June 4, 2025, at NASA’s Armstong Flight Research Center in Edwards, California. NASA researchers are developing technology to make supersonic parachutes safer and more reliable for delivering science instruments and payloads to Mars.NASA/Christopher LC Clark The Enhancing Parachutes by Instrumenting the Canopy project team examines a capsule and parachute following an air launch from an Alta X drone on June 4, 2025, at NASA’s Armstong Flight Research Center in Edwards, California. NASA researchers are developing technology to make supersonic parachutes safer and more reliable for delivering science instruments and payloads to Mars.NASA/Christopher LC Clark Share Details Last Updated Jul 29, 2025 EditorDede DiniusContactJay Levinejay.levine-1@nasa.gov Related Terms Explore More 5 min read NASA Releases Opportunity to Boost Commercial Space Tech Development Article 1 day ago 3 min read NASA Drop Test Supports Safer Air Taxi Design and Certification Article 3 days ago 3 min read NASA Rehearses How to Measure X-59’s Noise Levels Article 6 days ago Keep Exploring Discover More Topics From NASAArmstrong Flight Research Center
Humans in Space
Climate Change
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NASA-ISRO Satellite Lifts Off to Track Earth’s Changing Surfaces
Editor’s Note: This release was edited on July 30, 2025, to correct the mission launch time in the IST time zone.
Carrying an advanced radar system that will produce a dynamic, three-dimensional view of Earth in unprecedented detail, the NISAR (NASA-ISRO Synthetic Aperture Radar) satellite has launched from Satish Dhawan Space Centre in Sriharikota, Andhra Pradesh, India.
Jointly developed by NASA and the Indian Space Research Organisation (ISRO), and a critical part of the United States – India civil-space cooperation highlighted by President Trump and Prime Minister Modi earlier this year, the satellite can detect the movement of land and ice surfaces down to the centimeter. The mission will help protect communities by providing unique, actionable information to decision-makers in a diverse range of areas, including disaster response, infrastructure monitoring, and agricultural management.
The satellite lifted off aboard an ISRO Geosynchronous Satellite Launch Vehicle (GSLV) rocket at 5:40 p.m. IST (8:10 a.m. EDT), Wednesday. The ISRO ground controllers began communicating with NISAR about 20 minutes after launch, at just after 8:29 a.m. EDT, and confirmed it is operating as expected.
“Congratulations to the entire NISAR mission team on a successful launch that spanned across multiple time zones and continents in the first-ever partnership between NASA and ISRO on a mission of this sheer magnitude,” said Nicky Fox, associate administrator, Science Mission Directorate at NASA Headquarters in Washington. “Where moments are most critical, NISAR’s data will help ensure the health and safety of those impacted on Earth, as well as the infrastructure that supports them, for the benefit of all.”
From 464 miles (747 kilometers) above Earth, NISAR will use two advanced radar instruments to track changes in Earth’s forests and wetland ecosystems, monitor deformation and motion of the planet’s frozen surfaces, and detect the movement of Earth’s crust down to fractions of an inch — a key measurement in understanding how the land surface moves before, during, and after earthquakes, volcanic eruptions, and landslides.
“ISRO’s GSLV has precisely injected NISAR satellite into the intended orbit, 747 kilometers. I am happy to inform that this is GSLV’s first mission to Sun-synchronous polar orbit. With this successful launch, we are at the threshold of fulfilling the immense scientific potential NASA and ISRO envisioned for the NISAR mission more than 10 years ago,” said ISRO Chairman V Narayanan. “The powerful capability of this radar mission will help us study Earth’s dynamic land and ice surfaces in greater detail than ever before.”
The mission’s two radars will monitor nearly all the planet’s land- and ice-covered surfaces twice every 12 days, including areas of the polar Southern Hemisphere rarely covered by other Earth-observing radar satellites. The data NISAR collects also can help researchers assess how forests, wetlands, agricultural areas, and permafrost change over time.
“Observations from NISAR will provide new knowledge and tangible benefits for communities both in the U.S. and around the world,” said Karen St. Germain, director, Earth Science division at NASA Headquarters. “This launch marks the beginning of a new way of seeing the surface of our planet so that we can understand and foresee natural disasters and other changes in our Earth system that affect lives and property.”
The NISAR satellite is the first free-flying space mission to feature two radar instruments — an L-band system and an S-band system. Each system is sensitive to features of different sizes and specializes in detecting certain attributes. The L-band radar excels at measuring soil moisture, forest biomass, and motion of land and ice surfaces, while S-band radar excels at monitoring agriculture, grassland ecosystems, and infrastructure movement.
Together, the radar instruments will enhance all of the satellite’s observations, making NISAR more capable than previous synthetic aperture radar missions. Unlike optical sensors, NISAR will be able to “see” through clouds, making it possible to monitor the surface during storms, as well as in darkness and light.
NASA’s Jet Propulsion Laboratory in Southern California provided the L-band radar, and ISRO’s Space Applications Centre in Ahmedabad developed the S-band radar. The NISAR mission marks the first time the two agencies have co-developed hardware for an Earth-observing mission.
“We’re proud of the international team behind this remarkable satellite. The mission’s measurements will be global but its applications deeply local, as people everywhere will use its data to plan for a resilient future,” said Dave Gallagher, director, NASA JPL, which manages the U.S. portion of the mission for NASA. “At its core is synthetic aperture radar, a technology pioneered at NASA JPL that enables us to study Earth night and day, through all kinds of weather.”
Including L-band and S-band radars on one satellite is an evolution in SAR airborne and space-based missions that, for NASA, started in 1978 with the launch of Seasat. In 2012, ISRO began launching SAR missions starting with Radar Imaging Satellite (RISAT-1), followed by RISAT-1A in 2022, to support a wide range of applications in India.
In the coming weeks, the spacecraft will begin a roughly 90-day commissioning phase during which it will deploy its 39-foot (12-meter) radar antenna reflector. This reflector will direct and receive microwave signals from the two radars. By interpreting the differences between the two, researchers can discern characteristics about the surface below. As NISAR passes over the same locations twice every 12 days, scientists can evaluate how those characteristics have changed over time to reveal new insights about Earth’s dynamic surfaces.
The NISAR mission is an equal collaboration between NASA and ISRO. Managed for the agency by Caltech, NASA JPL leads the U.S. component of the project and is providing the mission’s L-band SAR. NASA also is providing the radar reflector antenna, the deployable boom, a high-rate communication subsystem for science data, GPS receivers, a solid-state recorder, and payload data subsystem.
Space Applications Centre Ahmedabad, ISRO’s lead center for payload development, is providing the mission’s S-band SAR instrument and is responsible for its calibration, data processing, and development of science algorithms to address the scientific goals of the mission. U R Rao Satellite Centre in Bengaluru, which leads the ISRO components of the mission, is providing the spacecraft bus. The launch vehicle is from ISRO’s Vikram Sarabhai Space Centre, launch services are through ISRO’s Satish Dhawan Space Centre, and satellite operations are by ISRO Telemetry Tracking and Command Network. National Remote Sensing Centre in Hyderabad is responsible for S-band data reception, operational products generation, and dissemination.
To learn more about NISAR, visit:
-end-
Karen Fox / Elizabeth Vlock
Headquarters, Washington
202-358-1600
karen.c.fox@nasa.gov / elizabeth.a.vlock@nasa.gov
Andrew Wang / Jane J. Lee
Jet Propulsion Laboratory, Pasadena, Calif.
626-379-6874 / 818-354-0307
andrew.wang@jpl.nasa.gov / jane.j.lee@jpl.nasa.gov
NASA-ISRO Satellite Lifts Off to Track Earth’s Changing Surfaces
Editor’s Note: This release was edited on July 30, 2025, to correct the mission launch time in the IST time zone.
Carrying an advanced radar system that will produce a dynamic, three-dimensional view of Earth in unprecedented detail, the NISAR (NASA-ISRO Synthetic Aperture Radar) satellite has launched from Satish Dhawan Space Centre in Sriharikota, Andhra Pradesh, India.
Jointly developed by NASA and the Indian Space Research Organisation (ISRO), and a critical part of the United States – India civil-space cooperation highlighted by President Trump and Prime Minister Modi earlier this year, the satellite can detect the movement of land and ice surfaces down to the centimeter. The mission will help protect communities by providing unique, actionable information to decision-makers in a diverse range of areas, including disaster response, infrastructure monitoring, and agricultural management.
The satellite lifted off aboard an ISRO Geosynchronous Satellite Launch Vehicle (GSLV) rocket at 5:40 p.m. IST (8:10 a.m. EDT), Wednesday. The ISRO ground controllers began communicating with NISAR about 20 minutes after launch, at just after 8:29 a.m. EDT, and confirmed it is operating as expected.
“Congratulations to the entire NISAR mission team on a successful launch that spanned across multiple time zones and continents in the first-ever partnership between NASA and ISRO on a mission of this sheer magnitude,” said Nicky Fox, associate administrator, Science Mission Directorate at NASA Headquarters in Washington. “Where moments are most critical, NISAR’s data will help ensure the health and safety of those impacted on Earth, as well as the infrastructure that supports them, for the benefit of all.”
From 464 miles (747 kilometers) above Earth, NISAR will use two advanced radar instruments to track changes in Earth’s forests and wetland ecosystems, monitor deformation and motion of the planet’s frozen surfaces, and detect the movement of Earth’s crust down to fractions of an inch — a key measurement in understanding how the land surface moves before, during, and after earthquakes, volcanic eruptions, and landslides.
“ISRO’s GSLV has precisely injected NISAR satellite into the intended orbit, 747 kilometers. I am happy to inform that this is GSLV’s first mission to Sun-synchronous polar orbit. With this successful launch, we are at the threshold of fulfilling the immense scientific potential NASA and ISRO envisioned for the NISAR mission more than 10 years ago,” said ISRO Chairman V Narayanan. “The powerful capability of this radar mission will help us study Earth’s dynamic land and ice surfaces in greater detail than ever before.”
The mission’s two radars will monitor nearly all the planet’s land- and ice-covered surfaces twice every 12 days, including areas of the polar Southern Hemisphere rarely covered by other Earth-observing radar satellites. The data NISAR collects also can help researchers assess how forests, wetlands, agricultural areas, and permafrost change over time.
“Observations from NISAR will provide new knowledge and tangible benefits for communities both in the U.S. and around the world,” said Karen St. Germain, director, Earth Science division at NASA Headquarters. “This launch marks the beginning of a new way of seeing the surface of our planet so that we can understand and foresee natural disasters and other changes in our Earth system that affect lives and property.”
The NISAR satellite is the first free-flying space mission to feature two radar instruments — an L-band system and an S-band system. Each system is sensitive to features of different sizes and specializes in detecting certain attributes. The L-band radar excels at measuring soil moisture, forest biomass, and motion of land and ice surfaces, while S-band radar excels at monitoring agriculture, grassland ecosystems, and infrastructure movement.
Together, the radar instruments will enhance all of the satellite’s observations, making NISAR more capable than previous synthetic aperture radar missions. Unlike optical sensors, NISAR will be able to “see” through clouds, making it possible to monitor the surface during storms, as well as in darkness and light.
NASA’s Jet Propulsion Laboratory in Southern California provided the L-band radar, and ISRO’s Space Applications Centre in Ahmedabad developed the S-band radar. The NISAR mission marks the first time the two agencies have co-developed hardware for an Earth-observing mission.
“We’re proud of the international team behind this remarkable satellite. The mission’s measurements will be global but its applications deeply local, as people everywhere will use its data to plan for a resilient future,” said Dave Gallagher, director, NASA JPL, which manages the U.S. portion of the mission for NASA. “At its core is synthetic aperture radar, a technology pioneered at NASA JPL that enables us to study Earth night and day, through all kinds of weather.”
Including L-band and S-band radars on one satellite is an evolution in SAR airborne and space-based missions that, for NASA, started in 1978 with the launch of Seasat. In 2012, ISRO began launching SAR missions starting with Radar Imaging Satellite (RISAT-1), followed by RISAT-1A in 2022, to support a wide range of applications in India.
In the coming weeks, the spacecraft will begin a roughly 90-day commissioning phase during which it will deploy its 39-foot (12-meter) radar antenna reflector. This reflector will direct and receive microwave signals from the two radars. By interpreting the differences between the two, researchers can discern characteristics about the surface below. As NISAR passes over the same locations twice every 12 days, scientists can evaluate how those characteristics have changed over time to reveal new insights about Earth’s dynamic surfaces.
The NISAR mission is an equal collaboration between NASA and ISRO. Managed for the agency by Caltech, NASA JPL leads the U.S. component of the project and is providing the mission’s L-band SAR. NASA also is providing the radar reflector antenna, the deployable boom, a high-rate communication subsystem for science data, GPS receivers, a solid-state recorder, and payload data subsystem.
Space Applications Centre Ahmedabad, ISRO’s lead center for payload development, is providing the mission’s S-band SAR instrument and is responsible for its calibration, data processing, and development of science algorithms to address the scientific goals of the mission. U R Rao Satellite Centre in Bengaluru, which leads the ISRO components of the mission, is providing the spacecraft bus. The launch vehicle is from ISRO’s Vikram Sarabhai Space Centre, launch services are through ISRO’s Satish Dhawan Space Centre, and satellite operations are by ISRO Telemetry Tracking and Command Network. National Remote Sensing Centre in Hyderabad is responsible for S-band data reception, operational products generation, and dissemination.
To learn more about NISAR, visit:
-end-
Karen Fox / Elizabeth Vlock
Headquarters, Washington
202-358-1600
karen.c.fox@nasa.gov / elizabeth.a.vlock@nasa.gov
Andrew Wang / Jane J. Lee
Jet Propulsion Laboratory, Pasadena, Calif.
626-379-6874 / 818-354-0307
andrew.wang@jpl.nasa.gov / jane.j.lee@jpl.nasa.gov
NASA’s Webb Traces Details of Complex Planetary Nebula
- Webb
- News
- Overview
- Science
- Observatory
- Multimedia
- Team
- More
NASA, ESA, CSA, STScI
Since their discovery in the late 1700s, astronomers have learned that planetary nebulae, or the expanding shell of glowing gas expelled by a low-intermediate mass star late in its life, can come in all shapes and sizes. Most planetary nebula present as circular, elliptical, or bi-polar, but some stray from the norm, as seen in new high-resolution images of planetary nebulae by NASA’s James Webb Space Telescope.
Webb’s newest look at planetary nebula NGC 6072 in the near- and mid-infrared shows what may appear as a very messy scene resembling splattered paint. However, the unusual, asymmetrical appearance hints at more complicated mechanisms underway, as the star central to the scene approaches the very final stages of its life and expels shells of material, losing up to 80 percent of its mass. Astronomers are using Webb to study planetary nebulae to learn more about the full life cycle of stars and how they impact their surrounding environments.
Image A: NGC 6072 (NIRCam Image) NASA’s James Webb Space Telescope’s view of planetary nebula NGC 6072 in the near-infrared shows a complex scene of multiple outflows expanding out at different angles from a dying star at the center of the scene. In this image, the red areas represent cool molecular gas, for example, molecular hydrogen. NASA, ESA, CSA, STScIFirst, taking a look at the image from Webb’s NIRCam (Near-Infrared Camera), it’s readily apparent that this nebula is multi-polar. This means there are several different elliptical outflows jetting out either way from the center, one from 11 o’clock to 5 o’clock, another from 1 o’clock to 7 o’clock, and possibly a third from 12 o’clock to 6 o’clock. The outflows may compress material as they go, resulting in a disk seen perpendicular to it.
Astronomers say this is evidence that there are likely at least two stars at the center of this scene. Specifically, a companion star is interacting with an aging star that had already begun to shed some of its outer layers of gas and dust.
The central region of the planetary nebula glows from the hot stellar core, seen as a light blue hue in near-infrared light. The dark orange material, which is made up of gas and dust, follows pockets or open areas that appear dark blue. This clumpiness could be created when dense molecular clouds formed while being shielded from hot radiation from the central star. There could also be a time element at play. Over thousands of years, inner fast winds could be ploughing through the halo cast off from the main star when it first started to lose mass.
Image B: NGC 6072 (MIRI Image) The mid-infrared view of planetary nebula NGC 6072 from NASA’s James Webb Space Telescope show expanding circular shells around the outflows from the dying central star. In this image, the blue represents cool molecular gas seen in red in the image from Webb’s NIRCam (Near-Infrared Camera) due to color mapping. NASA, ESA, CSA, STScIThe longer wavelengths captured by Webb’s MIRI (Mid-Infrared Instrument) are highlighting dust, revealing the star researchers suspect could be central to this scene. It appears as a small pinkish-whitish dot in this image.
Webb’s look in the mid-infrared wavelengths also reveals concentric rings expanding from the central region, the most obvious circling just past the edges of the lobes.
This may be additional evidence of a secondary star at the center of the scene hidden from our view. The secondary star, as it circles repeatedly around the original star, could have carved out rings of material in a bullseye pattern as the main star was expelling mass during an earlier stage of its life.
The rings may also hint at some kind of pulsation that resulted in gas or dust being expelled uniformly in all directions separated by say, thousands of years.
The red areas in NIRCam and blue areas in MIRI both trace cool molecular gas (likely molecular hydrogen) while central regions trace hot ionized gas.
As the star at the center of a planetary nebula cools and fades, the nebula will gradually dissipate into the interstellar medium — contributing enriched material that helps form new stars and planetary systems, now containing those heavier elements.
Webb’s imaging of NGC 6072 opens the door to studying how the planetary nebulae with more complex shapes contribute to this process.
The James Webb Space Telescope is the world’s premier space science observatory. Webb is solving mysteries in our solar system, looking beyond to distant worlds around other stars, and probing the mysterious structures and origins of our universe and our place in it. Webb is an international program led by NASA with its partners, ESA (European Space Agency) and CSA (Canadian Space Agency).
To learn more about Webb, visit:
DownloadsView/Download all image products at all resolutions for this article from the Space Telescope Science Institute.
Media ContactsLaura Betz – laura.e.betz@nasa.gov
NASA’s Goddard Space Flight Center, Greenbelt, Md.
Hannah Braun – hbraun@stsci.edu
Space Telescope Science Institute, Baltimore, Md.
View more Webb planetary nebula images
Learn more about planetary nebula
Interactive: Explore the Helix Nebula planetary nebula
Watch ViewSpace videos about planetary nebulas
Related For Kids En Español Keep Exploring Related Topics James Webb Space TelescopeWebb is the premier observatory of the next decade, serving thousands of astronomers worldwide. It studies every phase in the…
Stars
Stars Stories
Universe
Share Details Last Updated Jul 30, 2025 Editor Marty McCoy Contact Laura Betz laura.e.betz@nasa.gov Related Terms
NASA’s Webb Traces Details of Complex Planetary Nebula
- Webb
- News
- Overview
- Science
- Observatory
- Multimedia
- Team
- More
NASA, ESA, CSA, STScI
Since their discovery in the late 1700s, astronomers have learned that planetary nebulae, or the expanding shell of glowing gas expelled by a low-intermediate mass star late in its life, can come in all shapes and sizes. Most planetary nebula present as circular, elliptical, or bi-polar, but some stray from the norm, as seen in new high-resolution images of planetary nebulae by NASA’s James Webb Space Telescope.
Webb’s newest look at planetary nebula NGC 6072 in the near- and mid-infrared shows what may appear as a very messy scene resembling splattered paint. However, the unusual, asymmetrical appearance hints at more complicated mechanisms underway, as the star central to the scene approaches the very final stages of its life and expels shells of material, losing up to 80 percent of its mass. Astronomers are using Webb to study planetary nebulae to learn more about the full life cycle of stars and how they impact their surrounding environments.
Image A: NGC 6072 (NIRCam Image) NASA’s James Webb Space Telescope’s view of planetary nebula NGC 6072 in the near-infrared shows a complex scene of multiple outflows expanding out at different angles from a dying star at the center of the scene. In this image, the red areas represent cool molecular gas, for example, molecular hydrogen. NASA, ESA, CSA, STScIFirst, taking a look at the image from Webb’s NIRCam (Near-Infrared Camera), it’s readily apparent that this nebula is multi-polar. This means there are several different elliptical outflows jetting out either way from the center, one from 11 o’clock to 5 o’clock, another from 1 o’clock to 7 o’clock, and possibly a third from 12 o’clock to 6 o’clock. The outflows may compress material as they go, resulting in a disk seen perpendicular to it.
Astronomers say this is evidence that there are likely at least two stars at the center of this scene. Specifically, a companion star is interacting with an aging star that had already begun to shed some of its outer layers of gas and dust.
The central region of the planetary nebula glows from the hot stellar core, seen as a light blue hue in near-infrared light. The dark orange material, which is made up of gas and dust, follows pockets or open areas that appear dark blue. This clumpiness could be created when dense molecular clouds formed while being shielded from hot radiation from the central star. There could also be a time element at play. Over thousands of years, inner fast winds could be ploughing through the halo cast off from the main star when it first started to lose mass.
Image B: NGC 6072 (MIRI Image) The mid-infrared view of planetary nebula NGC 6072 from NASA’s James Webb Space Telescope show expanding circular shells around the outflows from the dying central star. In this image, the blue represents cool molecular gas seen in red in the image from Webb’s NIRCam (Near-Infrared Camera) due to color mapping. NASA, ESA, CSA, STScIThe longer wavelengths captured by Webb’s MIRI (Mid-Infrared Instrument) are highlighting dust, revealing the star researchers suspect could be central to this scene. It appears as a small pinkish-whitish dot in this image.
Webb’s look in the mid-infrared wavelengths also reveals concentric rings expanding from the central region, the most obvious circling just past the edges of the lobes.
This may be additional evidence of a secondary star at the center of the scene hidden from our view. The secondary star, as it circles repeatedly around the original star, could have carved out rings of material in a bullseye pattern as the main star was expelling mass during an earlier stage of its life.
The rings may also hint at some kind of pulsation that resulted in gas or dust being expelled uniformly in all directions separated by say, thousands of years.
The red areas in NIRCam and blue areas in MIRI both trace cool molecular gas (likely molecular hydrogen) while central regions trace hot ionized gas.
As the star at the center of a planetary nebula cools and fades, the nebula will gradually dissipate into the interstellar medium — contributing enriched material that helps form new stars and planetary systems, now containing those heavier elements.
Webb’s imaging of NGC 6072 opens the door to studying how the planetary nebulae with more complex shapes contribute to this process.
The James Webb Space Telescope is the world’s premier space science observatory. Webb is solving mysteries in our solar system, looking beyond to distant worlds around other stars, and probing the mysterious structures and origins of our universe and our place in it. Webb is an international program led by NASA with its partners, ESA (European Space Agency) and CSA (Canadian Space Agency).
To learn more about Webb, visit:
DownloadsView/Download all image products at all resolutions for this article from the Space Telescope Science Institute.
Media ContactsLaura Betz – laura.e.betz@nasa.gov
NASA’s Goddard Space Flight Center, Greenbelt, Md.
Hannah Braun – hbraun@stsci.edu
Space Telescope Science Institute, Baltimore, Md.
View more Webb planetary nebula images
Learn more about planetary nebula
Interactive: Explore the Helix Nebula planetary nebula
Watch ViewSpace videos about planetary nebulas
Related For Kids En Español Keep Exploring Related Topics James Webb Space TelescopeWebb is the premier observatory of the next decade, serving thousands of astronomers worldwide. It studies every phase in the…
Stars
Stars Stories
Universe
Share Details Last Updated Jul 30, 2025 Editor Marty McCoy Contact Laura Betz laura.e.betz@nasa.gov Related Terms
Looking Forward to the Moon
Looking Forward to the Moon
On May 8, 2022, NASA’s Exploration Ground Systems’ Program Manager Shawn Quinn captured this crop of a full frame image of the Hadley–Apennine region of Earth’s Moon including the Apollo 15 landing site (very near the edge of the shadow of one of the lunar mountains in the area). Building upon the pioneers from the Apollo Program, Artemis crews will plan to verify capabilities for humans to explore deep space and pave the way for long-term exploration and science on the lunar surface.
Read the Artemis blog for the latest mission updates.
Image credit: NASA/Shawn Quinn
Looking Forward to the Moon
On May 8, 2022, NASA’s Exploration Ground Systems’ Program Manager Shawn Quinn captured this crop of a full frame image of the Hadley–Apennine region of Earth’s Moon including the Apollo 15 landing site (very near the edge of the shadow of one of the lunar mountains in the area). Building upon the pioneers from the Apollo Program, Artemis crews will plan to verify capabilities for humans to explore deep space and pave the way for long-term exploration and science on the lunar surface.
Read the Artemis blog for the latest mission updates.
Image credit: NASA/Shawn Quinn
Laine Havens: Melding Science and Storytelling
Laine Havens — now a senior at Cornell University and three-time NASA intern — grew up with a deep curiosity about how the universe works and a family that encouraged her to explore it. Throughout her childhood, Laine was immersed in science and exposed to wonderful science communicators by her mother and grandfather.
Her grandfather, a retired Kodak engineer, encouraged inquisition into all matters — whether it be the inner workings of a telescope or an abandoned hornet’s nest. Laine spent summer evenings watching Mythbusters or Cosmos, and her mother’s favorite science podcast soundtracked car trips. Inspired by the likes of Carl Sagan, Laine originally intended to become a scientist.
“I fell in love with physics in high school,” she says. “I figured I would study it in college all the way through to a Ph.D.”
As a three-time NASA communications intern, Laine Havens has translated science for an audience of millions of people around the globe through science writing, social media, and video production.Credit: Kristin Rutkowski PhotographyLaine enrolled at Cornell and originally majored in physics as planned. But then she discovered an even more exciting option serendipitously while browsing an academic catalog: science and technology studies.
“I was scrolling through looking for a different class, but then I saw science and technology studies and began reading more about what it involved,” Laine says. “It was all about studying science — the philosophy of what it is, and how it interacts with social, political, ethical, and historical dimensions.”
Seeing the new program made Laine realize she could connect her love for critical analysis with her interest in science. She changed her program to a double-major in science and technology studies and astronomy, resolving to not only study and communicate science but to better understand the factors that influence it.
Laine (left) is a senior at Cornell University, where she double-majors in astronomy and science and technology studies. She served as the student newspaper’s science editor and president of the Pants Improv Comedy group. Laine channeled her comedic skills for some of her NASA projects, including a reel that used puns to discuss the agency’s upcoming Nancy Grace Roman Space Telescope.Credit: Courtesy of Laine HavensLaine began by working as a science writer at her university’s student-run newspaper, The Cornell Daily Sun, where she later became the science editor. Meanwhile, she volunteered with The Physics Bus — basically a mini science museum on wheels with experiments for kids — and the Free Science Workshop, an after school program offering kids an opportunity to build things or craft using all sorts of materials and gadgets.
“When you first hear about physics there’s a huge stigma, so we aimed to expose kids to it at a young age so they would associate it with fun,” Laine says.
Laine volunteered with The Physics Bus to introduce kids to the subject in a fun environment, helping them see the magic of how the world works before they learn to associate physics with boredom or intimidation.Credit: Courtesy of Laine HavensDuring her junior year, Laine started searching for science communication internships and found one at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. She applied and was accepted to one focusing on NASA’s upcoming Nancy Grace Roman Space Telescope. Following her first internship, Laine came back for two more with the same team.
“Every day here at NASA is inspiring,” Laine says. “I’ve learned so much about both hard and soft skills involved in science communication.”
During her first internship, Laine leaned into her background as a science writer to cover engineering milestones and craft a Tumblr post that walks readers through the universe’s different stages. She also produced videos, including one about Goddard’s biggest clean room.
“Everybody let me take that and run,” Laine says. “I got to write the script, host the video, and edit it.” The video, which garnered millions of views on social media, was the first of several Laine created to engage NASA’s traditional audience while drawing in others who don’t typically follow NASA or science very closely.
In addition to her usual assigned tasks, Laine took opportunities to be involved in many different aspects of science storytelling. This photo was taken while Laine worked as a drone spotter, helping to ensure a camera-equipped drone wouldn’t damage sensitive space hardware.Credit: NASA/Sophia RobertsThroughout her internships, Laine also led tours to teach people more about Roman, helped manage a celebrity visit with John Rhys-Davies, wrote Roman team member profiles, helped gather drone footage, contributed to the release of the NASA documentary Cosmic Dawn, emceed an intern day event, and supported Live Shots — short, live TV interviews with NASA experts.
“It’s been cool to see a different side of things,” Laine says. “I ultimately want to keep doing what I’ve been doing, but also become engaged in how to make it better — the science of science communication.”
To others who are interested in interning at NASA, Laine recommends speaking up.
“Just ask people things, whether it’s for help or an opportunity,” she says. “Sometimes you don’t want to impose or risk looking dumb, but for the most part everyone wants to help you and see you succeed. I’m very grateful to the Roman team for making it feel like a safe space where I could speak up.”
In preparation for a clean room “Get Ready With Me” video, Laine shadowed NASA videographer Sophia Roberts in the clean room at the agency’s Goddard Space Flight Center, where she supported documentation of integration milestones for NASA’s Nancy Grace Roman Space Telescope. Credit: NASA/Sophia RobertsSometimes that meant pitching ideas that were ultimately rejected, but that still provided an opportunity for discussion. “Not everything works, but in talking about it you might think of something else that does work,” she says. “There’s no consequence to it, because either way you’re learning something from it — either from the process of seeing it through or figuring out why you can’t do it.”
The same advice applies to securing an internship in the first place.
“Don’t be afraid to advocate for yourself,” Laine says. “If you find something you love, you can’t wait for it to happen on its own — you have to decide to go for it and find a way to make it happen.”
By Ashley Balzer
NASA’s Goddard Space Flight Center, Greenbelt, Md.
Laine Havens: Melding Science and Storytelling
Laine Havens — now a senior at Cornell University and three-time NASA intern — grew up with a deep curiosity about how the universe works and a family that encouraged her to explore it. Throughout her childhood, Laine was immersed in science and exposed to wonderful science communicators by her mother and grandfather.
Her grandfather, a retired Kodak engineer, encouraged inquisition into all matters — whether it be the inner workings of a telescope or an abandoned hornet’s nest. Laine spent summer evenings watching Mythbusters or Cosmos, and her mother’s favorite science podcast soundtracked car trips. Inspired by the likes of Carl Sagan, Laine originally intended to become a scientist.
“I fell in love with physics in high school,” she says. “I figured I would study it in college all the way through to a Ph.D.”
As a three-time NASA communications intern, Laine Havens has translated science for an audience of millions of people around the globe through science writing, social media, and video production.Credit: Kristin Rutkowski PhotographyLaine enrolled at Cornell and originally majored in physics as planned. But then she discovered an even more exciting option serendipitously while browsing an academic catalog: science and technology studies.
“I was scrolling through looking for a different class, but then I saw science and technology studies and began reading more about what it involved,” Laine says. “It was all about studying science — the philosophy of what it is, and how it interacts with social, political, ethical, and historical dimensions.”
Seeing the new program made Laine realize she could connect her love for critical analysis with her interest in science. She changed her program to a double-major in science and technology studies and astronomy, resolving to not only study and communicate science but to better understand the factors that influence it.
Laine (left) is a senior at Cornell University, where she double-majors in astronomy and science and technology studies. She served as the student newspaper’s science editor and president of the Pants Improv Comedy group. Laine channeled her comedic skills for some of her NASA projects, including a reel that used puns to discuss the agency’s upcoming Nancy Grace Roman Space Telescope.Credit: Courtesy of Laine HavensLaine began by working as a science writer at her university’s student-run newspaper, The Cornell Daily Sun, where she later became the science editor. Meanwhile, she volunteered with The Physics Bus — basically a mini science museum on wheels with experiments for kids — and the Free Science Workshop, an after school program offering kids an opportunity to build things or craft using all sorts of materials and gadgets.
“When you first hear about physics there’s a huge stigma, so we aimed to expose kids to it at a young age so they would associate it with fun,” Laine says.
Laine volunteered with The Physics Bus to introduce kids to the subject in a fun environment, helping them see the magic of how the world works before they learn to associate physics with boredom or intimidation.Credit: Courtesy of Laine HavensDuring her junior year, Laine started searching for science communication internships and found one at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. She applied and was accepted to one focusing on NASA’s upcoming Nancy Grace Roman Space Telescope. Following her first internship, Laine came back for two more with the same team.
“Every day here at NASA is inspiring,” Laine says. “I’ve learned so much about both hard and soft skills involved in science communication.”
During her first internship, Laine leaned into her background as a science writer to cover engineering milestones and craft a Tumblr post that walks readers through the universe’s different stages. She also produced videos, including one about Goddard’s biggest clean room.
“Everybody let me take that and run,” Laine says. “I got to write the script, host the video, and edit it.” The video, which garnered millions of views on social media, was the first of several Laine created to engage NASA’s traditional audience while drawing in others who don’t typically follow NASA or science very closely.
In addition to her usual assigned tasks, Laine took opportunities to be involved in many different aspects of science storytelling. This photo was taken while Laine worked as a drone spotter, helping to ensure a camera-equipped drone wouldn’t damage sensitive space hardware.Credit: NASA/Sophia RobertsThroughout her internships, Laine also led tours to teach people more about Roman, helped manage a celebrity visit with John Rhys-Davies, wrote Roman team member profiles, helped gather drone footage, contributed to the release of the NASA documentary Cosmic Dawn, emceed an intern day event, and supported Live Shots — short, live TV interviews with NASA experts.
“It’s been cool to see a different side of things,” Laine says. “I ultimately want to keep doing what I’ve been doing, but also become engaged in how to make it better — the science of science communication.”
To others who are interested in interning at NASA, Laine recommends speaking up.
“Just ask people things, whether it’s for help or an opportunity,” she says. “Sometimes you don’t want to impose or risk looking dumb, but for the most part everyone wants to help you and see you succeed. I’m very grateful to the Roman team for making it feel like a safe space where I could speak up.”
In preparation for a clean room “Get Ready With Me” video, Laine shadowed NASA videographer Sophia Roberts in the clean room at the agency’s Goddard Space Flight Center, where she supported documentation of integration milestones for NASA’s Nancy Grace Roman Space Telescope. Credit: NASA/Sophia RobertsSometimes that meant pitching ideas that were ultimately rejected, but that still provided an opportunity for discussion. “Not everything works, but in talking about it you might think of something else that does work,” she says. “There’s no consequence to it, because either way you’re learning something from it — either from the process of seeing it through or figuring out why you can’t do it.”
The same advice applies to securing an internship in the first place.
“Don’t be afraid to advocate for yourself,” Laine says. “If you find something you love, you can’t wait for it to happen on its own — you have to decide to go for it and find a way to make it happen.”
By Ashley Balzer
NASA’s Goddard Space Flight Center, Greenbelt, Md.
