Retired Marine Corps Gen. Anthony Zinni, Chairman of the Board at BAE Systems, speaks to those gathered at the 2009 NASA Executive Summit, Tuesday, Oct. 6, 2009, at the Ronald Reagan Building in Washington. (Photo Credit: (NASA/Paul E. Alers)
Retired Marine Corps Gen. Anthony Zinni, Chairman of the Board at BAE Systems, speaks to those gathered at the 2009 NASA Executive Summit, Tuesday, Oct. 6, 2009, at the Ronald Reagan Building in Washington. (Photo Credit: (NASA/Paul E. Alers)
Retired Marine Corps Gen. Anthony Zinni, Chairman of the Board at BAE Systems, speaks to those gathered at the 2009 NASA Executive Summit, Tuesday, Oct. 6, 2009, at the Ronald Reagan Building in Washington. (Photo Credit: (NASA/Paul E. Alers)
Retired Marine Corps Gen. Anthony Zinni, Chairman of the Board at BAE Systems, speaks to those gathered at the 2009 NASA Executive Summit, Tuesday, Oct. 6, 2009, at the Ronald Reagan Building in Washington. (Photo Credit: (NASA/Paul E. Alers)
Retired Marine Corps Gen. Anthony Zinni, Chairman of the Board at BAE Systems, speaks to those gathered at the 2009 NASA Executive Summit, Tuesday, Oct. 6, 2009, at the Ronald Reagan Building in Washington. (Photo Credit: (NASA/Paul E. Alers)
Retired Marine Corps Gen. Anthony Zinni, Chairman of the Board at BAE Systems, makes a point while speaking at the 2009 NASA Executive Summit, Tuesday, Oct. 6, 2009, at the Ronald Reagan Building in Washington. (Photo Credit: (NASA/Paul E. Alers)
Employees with BAE Systems pose for a photo following the arrival of NASA’s SPHEREx (Spectro-Photometer for the History of the Universe, Epoch of Reionization and Ices Explorer) observatory inside the Astrotech Space Operations Facility at Vandenberg Space Force Base in California on Tuesday, Jan. 14, 2025. BAE Systems (formerly Ball Aerospace) built the telescope and the spacecraft bus. SPHEREx will use its telescope to provide an all-sky spectral survey, creating a 3D map of the entire sky to help scientists investigate the origins of our universe. Riding along with SPHEREx, NASA’s PUNCH (Polarimeter to Unify the Corona and Heliosphere) mission will study origins of the Sun’s outflow of material, or the solar wind. Liftoff aboard a SpaceX Falcon 9 rocket is targeted for 10:09 p.m. EST (7:09 p.m. PST), Thursday, Feb. 27, 2025, from Space Launch Complex 4 East.
Employees with BAE Systems conduct spacecraft processing of NASA’s SPHEREx (Spectro-Photometer for the History of the Universe, Epoch of Reionization and Ices Explorer) observatory inside the Astrotech Space Operations Facility at Vandenberg Space Force Base in California on Thursday, Jan. 16, 2025. BAE Systems (formerly Ball Aerospace) built the telescope and the spacecraft bus. SPHEREx will use its telescope to provide an all-sky spectral survey, creating a 3D map of the entire sky to help scientists investigate the origins of our universe. Riding along with SPHEREx, NASA’s PUNCH (Polarimeter to Unify the Corona and Heliosphere) mission will study origins of the Sun’s outflow of material, or the solar wind. Liftoff aboard a SpaceX Falcon 9 rocket is targeted for 10:09 p.m. EST (7:09 p.m. PST), Thursday, Feb. 27, 2025, from Space Launch Complex 4 East.
Employees with BAE Systems conduct spacecraft processing of NASA’s SPHEREx (Spectro-Photometer for the History of the Universe, Epoch of Reionization and Ices Explorer) observatory inside the Astrotech Space Operations Facility at Vandenberg Space Force Base in California on Thursday, Jan. 16, 2025. BAE Systems (formerly Ball Aerospace) built the telescope and the spacecraft bus. SPHEREx will use its telescope to provide an all-sky spectral survey, creating a 3D map of the entire sky to help scientists investigate the origins of our universe. Riding along with SPHEREx, NASA’s PUNCH (Polarimeter to Unify the Corona and Heliosphere) mission will study origins of the Sun’s outflow of material, or the solar wind. Liftoff aboard a SpaceX Falcon 9 rocket is targeted for 10:09 p.m. EST (7:09 p.m. PST), Thursday, Feb. 27, 2025, from Space Launch Complex 4 East.
Employees with BAE Systems conduct spacecraft processing of NASA’s SPHEREx (Spectro-Photometer for the History of the Universe, Epoch of Reionization and Ices Explorer) observatory inside the Astrotech Space Operations Facility at Vandenberg Space Force Base in California on Thursday, Jan. 16, 2025. BAE Systems (formerly Ball Aerospace) built the telescope and the spacecraft bus. SPHEREx will use its telescope to provide an all-sky spectral survey, creating a 3D map of the entire sky to help scientists investigate the origins of our universe. Riding along with SPHEREx, NASA’s PUNCH (Polarimeter to Unify the Corona and Heliosphere) mission will study origins of the Sun’s outflow of material, or the solar wind. Liftoff aboard a SpaceX Falcon 9 rocket is targeted for 10:09 p.m. EST (7:09 p.m. PST), Thursday, Feb. 27, 2025, from Space Launch Complex 4 East.
The SPHEREx observatory sits in a clean room after environmental testing at BAE Systems in Boulder, Colorado, in late 2024. Short for Spectro-Photometer for the History of the Universe, Epoch of Reionization and Ices Explorer, SPHEREx will create a map of the cosmos like no other. Using a technique called spectroscopy to image the entire sky in 102 wavelengths of infrared light, SPHEREx will gather information about the composition of and distance to millions of galaxies and stars. With this map, scientists will study what happened in the first fraction of a second after the big bang, how galaxies formed and evolved, and the origins of water in planetary systems in our galaxy. https://photojournal.jpl.nasa.gov/catalog/PIA26537
Final assembly of NASA's SPHEREx spacecraft is shown at BAE Systems in Boulder, Colorado, in March 2024. Short for Spectro-Photometer for the History of the Universe, Epoch of Reionization and Ices Explorer, SPHEREx will create a map of the cosmos like no other. Using a technique called spectroscopy to image the entire sky in 102 wavelengths of infrared light, SPHEREx will gather information about the composition of and distance to millions of galaxies and stars. With this map, scientists will study what happened in the first fraction of a second after the big bang, how galaxies formed and evolved, and the origins of water in planetary systems in our galaxy. https://photojournal.jpl.nasa.gov/catalog/PIA26543
NASA's SPHEREx observatory undergoes integration and testing at BAE Systems in Boulder, Colorado, in April 2024. Short for Spectro-Photometer for the History of the Universe, Epoch of Reionization and Ices Explorer, SPHEREx will create a map of the cosmos like no other. Using a technique called spectroscopy to image the entire sky in 102 wavelengths of infrared light, SPHEREx will gather information about the composition of and distance to millions of galaxies and stars. With this map, scientists will study what happened in the first fraction of a second after the big bang, how galaxies formed and evolved, and the origins of water in planetary systems in our galaxy. https://photojournal.jpl.nasa.gov/catalog/PIA26538
NASA's SPHEREx observatory is installed in the Titan Thermal Vacuum (TVAC) test Chamber at BAE Systems in Boulder, Colorado, in June 2024. As part of the test setup, the spacecraft and photon shield are covered in multilayer insulation and blankets and surrounded by ground support equipment. Short for Spectro-Photometer for the History of the Universe, Epoch of Reionization and Ices Explorer, SPHEREx will create a map of the cosmos like no other. Using a technique called spectroscopy to image the entire sky in 102 wavelengths of infrared light, SPHEREx will gather information about the composition of and distance to millions of galaxies and stars. With this map, scientists will study what happened in the first fraction of a second after the big bang, how galaxies formed and evolved, and the origins of water in planetary systems in our galaxy. https://photojournal.jpl.nasa.gov/catalog/PIA26541
NASA's SPHEREx space observatory was photographed at BAE Systems in Boulder, Colorado, in November 2024 after completing environmental testing. The spacecraft's three concentric cones help direct heat and light away from the telescope and other components, keeping them cool. Short for Spectro-Photometer for the History of the Universe, Epoch of Reionization and Ices Explorer, SPHEREx will create a map of the cosmos like no other. Using a technique called spectroscopy to image the entire sky in 102 wavelengths of infrared light, SPHEREx will gather information about the composition of and distance to millions of galaxies and stars. With this map, scientists will study what happened in the first fraction of a second after the big bang, how galaxies formed and evolved, and the origins of water in planetary systems in our galaxy. https://photojournal.jpl.nasa.gov/catalog/PIA26536
NASA's SPHEREx observatory is oriented in a horizontal position, revealing all three layers of photon shields as well as the telescope. This photo was taken at BAE Systems in Boulder, Colorado, in April 2024. Short for Spectro-Photometer for the History of the Universe, Epoch of Reionization and Ices Explorer, SPHEREx will create a map of the cosmos like no other. Using a technique called spectroscopy to image the entire sky in 102 wavelengths of infrared light, SPHEREx will gather information about the composition of and distance to millions of galaxies and stars. With this map, scientists will study what happened in the first fraction of a second after the big bang, how galaxies formed and evolved, and the origins of water in planetary systems in our galaxy. https://photojournal.jpl.nasa.gov/catalog/PIA26542
NASA's SPHEREx observatory is lifted and installed onto a vibration table in the Z-axis configuration at BAE Systems in Boulder, Colorado, in August 2024. In this test, the spacecraft is subjected to vibrations in all three axes separately. The test was successfully completed Aug. 16, 2024. Short for Spectro-Photometer for the History of the Universe, Epoch of Reionization and Ices Explorer, SPHEREx will create a map of the cosmos like no other. Using a technique called spectroscopy to image the entire sky in 102 wavelengths of infrared light, SPHEREx will gather information about the composition of and distance to millions of galaxies and stars. With this map, scientists will study what happened in the first fraction of a second after the big bang, how galaxies formed and evolved, and the origins of water in planetary systems in our galaxy. https://photojournal.jpl.nasa.gov/catalog/PIA26539
NASA's SPHEREx observatory is installed in the Fiesta Area at BAE Systems in Boulder, Colorado, in July 2024. The observatory is surrounded by speaker stacks used to perform acoustics testing, which subjects the spacecraft to the acoustics loads that it will experience during launch. Short for Spectro-Photometer for the History of the Universe, Epoch of Reionization and Ices Explorer, SPHEREx will create a map of the cosmos like no other. Using a technique called spectroscopy to image the entire sky in 102 wavelengths of infrared light, SPHEREx will gather information about the composition of and distance to millions of galaxies and stars. With this map, scientists will study what happened in the first fraction of a second after the big bang, how galaxies formed and evolved, and the origins of water in planetary systems in our galaxy. https://photojournal.jpl.nasa.gov/catalog/PIA26540
The National Oceanic and Atmospheric Administration’s (NOAA) Space Weather Follow On–Lagrange 1 (SWFO-L1) Observatory, set to provide quicker and more accurate space weather forecasts, arrived Sunday, July 20, 2025, at the Astrotech Space Operations Facility near NASA’s Kennedy Space Center in Florida. The SWFO-L1 mission will monitor the Sun and near-Earth environment using a suite of instruments that provide real-time measurements of solar activity. The observatory will launch as a rideshare with NASA’s IMAP (Interstellar Mapping and Acceleration Probe) no earlier than September 2025.
A photographer captures the National Oceanic and Atmospheric Administration’s (NOAA) Space Weather Follow On–Lagrange 1 (SWFO-L1) Observatory laying horizontal on Tuesday, July 22, 2025, following the arrival and unboxing of the observatory at the Astrotech Space Operations Facility near NASA’s Kennedy Space Center in Florida. The SWFO-L1 mission will monitor the Sun and near-Earth environment using a suite of instruments that provide real-time measurements of solar activity. The observatory will launch as a rideshare with NASA’s IMAP (Interstellar Mapping and Acceleration Probe) no earlier than September 2025.
Technicians inspect a motorized light band for NASA’s Carruthers Geocorona Observatory on Tuesday, July 22, 2025, at the Astrotech Space Operations Facility near the agency’s Kennedy Space Center in Florida. The Carruthers Geocorona Observatory is a small satellite set to operate at Lagrange Point 1 (L1), an orbit point between the Earth and Sun about one million miles away. Carruthers will use its ultraviolet cameras to monitor how space weather from the Sun impacts the exosphere, the outermost part of Earth’s atmosphere. The observatory will launch as a rideshare with NASA’s IMAP (Interstellar Mapping and Acceleration Probe) no earlier than September 2025.
Technicians remove the transport container covering NASA’s Carruthers Geocorona Observatory on Monday, July 21, 2025, at the Astrotech Space Operations Facility near the agency’s Kennedy Space Center in Florida. The Carruthers Geocorona Observatory is a small satellite set to operate at Lagrange Point 1 (L1), an orbit point between the Earth and Sun about one million miles away. Carruthers will use its ultraviolet cameras to monitor how space weather from the Sun impacts the exosphere, the outermost part of Earth’s atmosphere. The observatory will launch as a rideshare with NASA’s IMAP (Interstellar Mapping and Acceleration Probe) no earlier than September 2025.
The National Oceanic and Atmospheric Administration’s (NOAA) Space Weather Follow On–Lagrange 1 (SWFO-L1) Observatory, set to provide quicker and more accurate space weather forecasts, arrived Sunday, July 20, 2025, at the Astrotech Space Operations Facility near NASA’s Kennedy Space Center in Florida. The SWFO-L1 mission will monitor the Sun and near-Earth environment using a suite of instruments that provide real-time measurements of solar activity. The observatory will launch as a rideshare with NASA’s IMAP (Interstellar Mapping and Acceleration Probe) no earlier than September 2025.
Technicians inspect the National Oceanic and Atmospheric Administration’s (NOAA) Space Weather Follow On–Lagrange 1 (SWFO-L1) Observatory on Thursday, July 24, 2025, following the arrival and unboxing of the observatory at the Astrotech Space Operations Facility near NASA’s Kennedy Space Center in Florida. The SWFO-L1 mission will monitor the Sun and near-Earth environment using a suite of instruments that provide real-time measurements of solar activity. The observatory will launch as a rideshare with NASA’s IMAP (Interstellar Mapping and Acceleration Probe) no earlier than September 2025.
Technicians inspect the National Oceanic and Atmospheric Administration’s (NOAA) Space Weather Follow On–Lagrange 1 (SWFO-L1) Observatory on Thursday, July 24, 2025, following the arrival and unboxing of the observatory at the Astrotech Space Operations Facility near NASA’s Kennedy Space Center in Florida. The SWFO-L1 mission will monitor the Sun and near-Earth environment using a suite of instruments that provide real-time measurements of solar activity. The observatory will launch as a rideshare with NASA’s IMAP (Interstellar Mapping and Acceleration Probe) no earlier than September 2025.
Technicians inspect the National Oceanic and Atmospheric Administration’s (NOAA) Space Weather Follow On–Lagrange 1 (SWFO-L1) Observatory on Thursday, July 24, 2025, following the arrival and unboxing of the observatory at the Astrotech Space Operations Facility near NASA’s Kennedy Space Center in Florida. The SWFO-L1 mission will monitor the Sun and near-Earth environment using a suite of instruments that provide real-time measurements of solar activity. The observatory will launch as a rideshare with NASA’s IMAP (Interstellar Mapping and Acceleration Probe) no earlier than September 2025.
Technicians inspect the National Oceanic and Atmospheric Administration’s (NOAA) Space Weather Follow On–Lagrange 1 (SWFO-L1) Observatory on Thursday, July 24, 2025, following the arrival and unboxing of the observatory at the Astrotech Space Operations Facility near NASA’s Kennedy Space Center in Florida. The SWFO-L1 mission will monitor the Sun and near-Earth environment using a suite of instruments that provide real-time measurements of solar activity. The observatory will launch as a rideshare with NASA’s IMAP (Interstellar Mapping and Acceleration Probe) no earlier than September 2025.
Technicians inspect the National Oceanic and Atmospheric Administration’s (NOAA) Space Weather Follow On–Lagrange 1 (SWFO-L1) Observatory on Thursday, July 24, 2025, following the arrival and unboxing of the observatory at the Astrotech Space Operations Facility near NASA’s Kennedy Space Center in Florida. The SWFO-L1 mission will monitor the Sun and near-Earth environment using a suite of instruments that provide real-time measurements of solar activity. The observatory will launch as a rideshare with NASA’s IMAP (Interstellar Mapping and Acceleration Probe) no earlier than September 2025.
A crane lifts NASA’s Carruthers Geocorona Observatory on Thursday, July 24, 2025, at the Astrotech Space Operations Facility near the agency’s Kennedy Space Center in Florida. The Carruthers Geocorona Observatory is a small satellite set to operate at Lagrange Point 1 (L1), an orbit point between the Earth and Sun about one million miles away. Carruthers will use its ultraviolet cameras to monitor how space weather from the Sun impacts the exosphere, the outermost part of Earth’s atmosphere. The observatory will launch as a rideshare with NASA’s IMAP (Interstellar Mapping and Acceleration Probe) no earlier than September 2025.
A crane lifts NASA’s Carruthers Geocorona Observatory on Thursday, July 24, 2025, at the Astrotech Space Operations Facility near the agency’s Kennedy Space Center in Florida. The Carruthers Geocorona Observatory is a small satellite set to operate at Lagrange Point 1 (L1), an orbit point between the Earth and Sun about one million miles away. Carruthers will use its ultraviolet cameras to monitor how space weather from the Sun impacts the exosphere, the outermost part of Earth’s atmosphere. The observatory will launch as a rideshare with NASA’s IMAP (Interstellar Mapping and Acceleration Probe) no earlier than September 2025.
A crane lifts NASA’s Carruthers Geocorona Observatory on Thursday, July 24, 2025, at the Astrotech Space Operations Facility near the agency’s Kennedy Space Center in Florida. The Carruthers Geocorona Observatory is a small satellite set to operate at Lagrange Point 1 (L1), an orbit point between the Earth and Sun about one million miles away. Carruthers will use its ultraviolet cameras to monitor how space weather from the Sun impacts the exosphere, the outermost part of Earth’s atmosphere. The observatory will launch as a rideshare with NASA’s IMAP (Interstellar Mapping and Acceleration Probe) no earlier than September 2025.
A crane lifts NASA’s Carruthers Geocorona Observatory on Thursday, July 24, 2025, at the Astrotech Space Operations Facility near the agency’s Kennedy Space Center in Florida. The Carruthers Geocorona Observatory is a small satellite set to operate at Lagrange Point 1 (L1), an orbit point between the Earth and Sun about one million miles away. Carruthers will use its ultraviolet cameras to monitor how space weather from the Sun impacts the exosphere, the outermost part of Earth’s atmosphere. The observatory will launch as a rideshare with NASA’s IMAP (Interstellar Mapping and Acceleration Probe) no earlier than September 2025.
Technicians rotate the National Oceanic and Atmospheric Administration’s (NOAA) Space Weather Follow On–Lagrange 1 (SWFO-L1) Observatory vertically and use a crane to lift it from its transport container on Wednesday, July 23, 2025, following the arrival and unboxing of the observatory at the Astrotech Space Operations Facility near NASA’s Kennedy Space Center in Florida. The SWFO-L1 mission will monitor the Sun and near-Earth environment using a suite of instruments that provide real-time measurements of solar activity. The observatory will launch as a rideshare with NASA’s IMAP (Interstellar Mapping and Acceleration Probe) no earlier than September 2025.
Technicians rotate the National Oceanic and Atmospheric Administration’s (NOAA) Space Weather Follow On–Lagrange 1 (SWFO-L1) Observatory vertically and use a crane to lift it from its transport container on Wednesday, July 23, 2025, following the arrival and unboxing of the observatory at the Astrotech Space Operations Facility near NASA’s Kennedy Space Center in Florida. The SWFO-L1 mission will monitor the Sun and near-Earth environment using a suite of instruments that provide real-time measurements of solar activity. The observatory will launch as a rideshare with NASA’s IMAP (Interstellar Mapping and Acceleration Probe) no earlier than September 2025.
Technicians rotate the National Oceanic and Atmospheric Administration’s (NOAA) Space Weather Follow On–Lagrange 1 (SWFO-L1) Observatory vertically and use a crane to lift it from its transport container on Wednesday, July 23, 2025, following the arrival and unboxing of the observatory at the Astrotech Space Operations Facility near NASA’s Kennedy Space Center in Florida. The SWFO-L1 mission will monitor the Sun and near-Earth environment using a suite of instruments that provide real-time measurements of solar activity. The observatory will launch as a rideshare with NASA’s IMAP (Interstellar Mapping and Acceleration Probe) no earlier than September 2025.
Technicians inspect the solar array panel attached to NASA’s Carruthers Geocorona Observatory on Wednesday, July 23, 2025, at the Astrotech Space Operations Facility near the agency’s Kennedy Space Center in Florida. The solar array will use the Sun to help power Carruthers Geocorona Observatory as it operates at Lagrange Point 1 (L1), an orbit point between the Earth and Sun about one million miles away. Carruthers will use its ultraviolet cameras to monitor how space weather from the Sun impacts the exosphere, the outermost part of Earth’s atmosphere. The observatory will launch as a rideshare with NASA’s IMAP (Interstellar Mapping and Acceleration Probe) no earlier than September 2025.
A photographer captures a photo of NASA’s Carruthers Geocorona Observatory on Wednesday, July 23, 2025, following arrival and unboxing of the observatory at the Astrotech Space Operations Facility near the agency’s Kennedy Space Center in Florida. The Carruthers Geocorona Observatory is a small satellite set to operate at Lagrange Point 1 (L1), an orbit point between the Earth and Sun about one million miles away. Carruthers will use its ultraviolet cameras to monitor how space weather from the Sun impacts the exosphere, the outermost part of Earth’s atmosphere. The observatory will launch as a rideshare with NASA’s (Interstellar Mapping and Acceleration Probe) no earlier than September 2025.
Technicians inspect NASA’s Carruthers Geocorona Observatory on Wednesday, July 23, 2025, following arrival and unboxing of the observatory at the Astrotech Space Operations Facility near the agency’s Kennedy Space Center in Florida. The Carruthers Geocorona Observatory is a small satellite set to operate at Lagrange Point 1 (L1), an orbit point between the Earth and Sun about one million miles away. Carruthers will use its ultraviolet cameras to monitor how space weather from the Sun impacts the exosphere, the outermost part of Earth’s atmosphere. The observatory will launch as a rideshare with NASA’s IMAP (Interstellar Mapping and Acceleration Probe) no earlier than September 2025.
Technicians inspect NASA’s Carruthers Geocorona Observatory on Wednesday, July 23, 2025, following arrival and unboxing of the observatory at the Astrotech Space Operations Facility near the agency’s Kennedy Space Center in Florida. The Carruthers Geocorona Observatory is a small satellite set to operate at Lagrange Point 1 (L1), an orbit point between the Earth and Sun about one million miles away. Carruthers will use its ultraviolet cameras to monitor how space weather from the Sun impacts the exosphere, the outermost part of Earth’s atmosphere. The observatory will launch as a rideshare with NASA’s IMAP (Interstellar Mapping and Acceleration Probe) no earlier than September 2025.
Technicians use a crane to lift the National Oceanic and Atmospheric Administration’s (NOAA) Space Weather Follow On–Lagrange 1 (SWFO-L1) Observatory onto a work stand on Friday, July 25, 2025, during prelaunch processing at the Astrotech Space Operations Facility near NASA’s Kennedy Space Center in Florida. The SWFO-L1 mission will observe solar eruptions, and monitor incoming space weather 24/7, providing early warnings and validating forecasts that protect vital communication and navigation infrastructure, economic interests, and national security, both on Earth and in space. The observatory will launch as a rideshare with NASA’s IMAP (Interstellar Mapping and Acceleration Probe) no earlier than September 2025.
Technicians use a crane to lift the National Oceanic and Atmospheric Administration’s (NOAA) Space Weather Follow On–Lagrange 1 (SWFO-L1) Observatory onto a work stand on Friday, July 25, 2025, during prelaunch processing at the Astrotech Space Operations Facility near NASA’s Kennedy Space Center in Florida. The SWFO-L1 mission will observe solar eruptions, and monitor incoming space weather 24/7, providing early warnings and validating forecasts that protect vital communication and navigation infrastructure, economic interests, and national security, both on Earth and in space. The observatory will launch as a rideshare with NASA’s IMAP (Interstellar Mapping and Acceleration Probe) no earlier than September 2025.
With hardware in the foreground, technicians use a crane to lift the National Oceanic and Atmospheric Administration’s (NOAA) Space Weather Follow On–Lagrange 1 (SWFO-L1) Observatory onto a work stand on Friday, July 25, 2025, during prelaunch processing at the Astrotech Space Operations Facility near NASA’s Kennedy Space Center in Florida. The SWFO-L1 mission will observe solar eruptions, and monitor incoming space weather 24/7, providing early warnings and validating forecasts that protect vital communication and navigation infrastructure, economic interests, and national security, both on Earth and in space. The observatory will launch as a rideshare with NASA’s IMAP (Interstellar Mapping and Acceleration Probe) no earlier than September 2025.
Technicians use a crane to lift the National Oceanic and Atmospheric Administration’s (NOAA) Space Weather Follow On–Lagrange 1 (SWFO-L1) Observatory onto a work stand on Friday, July 25, 2025, during prelaunch processing at the Astrotech Space Operations Facility near NASA’s Kennedy Space Center in Florida. The SWFO-L1 mission will observe solar eruptions, and monitor incoming space weather 24/7, providing early warnings and validating forecasts that protect vital communication and navigation infrastructure, economic interests, and national security, both on Earth and in space. The observatory will launch as a rideshare with NASA’s IMAP (Interstellar Mapping and Acceleration Probe) no earlier than September 2025.
Technicians use a crane to lift the National Oceanic and Atmospheric Administration’s (NOAA) Space Weather Follow On–Lagrange 1 (SWFO-L1) Observatory onto a work stand on Friday, July 25, 2025, during prelaunch processing at the Astrotech Space Operations Facility near NASA’s Kennedy Space Center in Florida. The SWFO-L1 mission will observe solar eruptions, and monitor incoming space weather 24/7, providing early warnings and validating forecasts that protect vital communication and navigation infrastructure, economic interests, and national security, both on Earth and in space. The observatory will launch as a rideshare with NASA’s IMAP (Interstellar Mapping and Acceleration Probe) no earlier than September 2025.
Technicians use a crane to lift the National Oceanic and Atmospheric Administration’s (NOAA) Space Weather Follow On–Lagrange 1 (SWFO-L1) Observatory onto a work stand on Friday, July 25, 2025, during prelaunch processing at the Astrotech Space Operations Facility near NASA’s Kennedy Space Center in Florida. The SWFO-L1 mission will observe solar eruptions, and monitor incoming space weather 24/7, providing early warnings and validating forecasts that protect vital communication and navigation infrastructure, economic interests, and national security, both on Earth and in space. The observatory will launch as a rideshare with NASA’s IMAP (Interstellar Mapping and Acceleration Probe) no earlier than September 2025.
Technicians use a crane to lift the National Oceanic and Atmospheric Administration’s (NOAA) Space Weather Follow On–Lagrange 1 (SWFO-L1) Observatory onto a work stand on Friday, July 25, 2025, during prelaunch processing at the Astrotech Space Operations Facility near NASA’s Kennedy Space Center in Florida. The SWFO-L1 mission will observe solar eruptions, and monitor incoming space weather 24/7, providing early warnings and validating forecasts that protect vital communication and navigation infrastructure, economic interests, and national security, both on Earth and in space. The observatory will launch as a rideshare with NASA’s IMAP (Interstellar Mapping and Acceleration Probe) no earlier than September 2025.
Technicians use a crane to lift the National Oceanic and Atmospheric Administration’s (NOAA) Space Weather Follow On–Lagrange 1 (SWFO-L1) Observatory onto a work stand on Friday, July 25, 2025, during prelaunch processing at the Astrotech Space Operations Facility near NASA’s Kennedy Space Center in Florida. The SWFO-L1 mission will observe solar eruptions, and monitor incoming space weather 24/7, providing early warnings and validating forecasts that protect vital communication and navigation infrastructure, economic interests, and national security, both on Earth and in space. The observatory will launch as a rideshare with NASA’s IMAP (Interstellar Mapping and Acceleration Probe) no earlier than September 2025.
Technicians use a crane to lift the National Oceanic and Atmospheric Administration’s (NOAA) Space Weather Follow On–Lagrange 1 (SWFO-L1) Observatory onto a work stand on Friday, July 25, 2025, during prelaunch processing at the Astrotech Space Operations Facility near NASA’s Kennedy Space Center in Florida. The SWFO-L1 mission will observe solar eruptions, and monitor incoming space weather 24/7, providing early warnings and validating forecasts that protect vital communication and navigation infrastructure, economic interests, and national security, both on Earth and in space. The observatory will launch as a rideshare with NASA’s IMAP (Interstellar Mapping and Acceleration Probe) no earlier than September 2025.
Technicians use a crane to lift the National Oceanic and Atmospheric Administration’s (NOAA) Space Weather Follow On–Lagrange 1 (SWFO-L1) Observatory onto a work stand on Friday, July 25, 2025, during prelaunch processing at the Astrotech Space Operations Facility near NASA’s Kennedy Space Center in Florida. The SWFO-L1 mission will observe solar eruptions, and monitor incoming space weather 24/7, providing early warnings and validating forecasts that protect vital communication and navigation infrastructure, economic interests, and national security, both on Earth and in space. The observatory will launch as a rideshare with NASA’s IMAP (Interstellar Mapping and Acceleration Probe) no earlier than September 2025.
Silicon Valley FIRST Regional Robotics competition: The Apes of Wrath - Team 668 - BAE Systems/Capitol Honda/D&M Model & Machine shop/Mchale Creative & Pioneer High School ASB, San Jose California (CA) do battle with Quixilver - Team 604 - Exatron/Google Leland High School, San Jose, California (CA)
NASA’s SPHEREx (Spectro-Photometer for the History of the Universe, Epoch of Reionization and Ices Explorer), a space telescope, is situated on a work stand ahead of prelaunch operations at the Astrotech Processing Facility at Vandenberg Space Force Base in California on Thursday, Jan. 16, 2025. SPHEREx will enter a polar orbit around Earth and create a 3D map of the entire sky, gathering information about millions of galaxies for scientists to study what happened after the big bang, the history of galaxy evolution, and the origins of water in planetary systems in our galaxy. SPHEREx will launch aboard a SpaceX Falcon 9 rocket in late February 2025.
NASA’s SPHEREx (Spectro-Photometer for the History of the Universe, Epoch of Reionization and Ices Explorer), a space telescope, is situated on a work stand ahead of prelaunch operations at the Astrotech Processing Facility at Vandenberg Space Force Base in California on Thursday, Jan. 16, 2025. SPHEREx will enter a polar orbit around Earth and create a 3D map of the entire sky, gathering information about millions of galaxies for scientists to study what happened after the big bang, the history of galaxy evolution, and the origins of water in planetary systems in our galaxy. SPHEREx will launch aboard a SpaceX Falcon 9 rocket in late February 2025.
Technicians and engineers encapsulate NASA’s SPHEREx (Spectro-Photometer for the History of the Universe, Epoch of Reionization and Ices Explorer) observatory and PUNCH (Polarimeter to Unify the Corona and Heliosphere) satellites within a protective payload fairing inside the Astrotech Space Operations facility at Vandenberg Space Force Base in California, on Thursday, Feb. 27, 2025. SPHEREx will use its telescope to provide an all-sky spectral survey, creating a 3D map of the entire sky to help scientists investigate the origins of our universe. PUNCH will study origins of the Sun’s outflow of material, or the solar wind, capturing continuous 3D images of the Sun’s corona and the solar wind’s journey into the solar system. Liftoff aboard a SpaceX Falcon 9 rocket is targeted for NET 10:09 EST (7:09 p.m. PST), Tuesday, March 4, 2025, at Space Launch Complex 4 East from Vandenberg Space Force Base in California.
Technicians and engineers encapsulate NASA’s SPHEREx (Spectro-Photometer for the History of the Universe, Epoch of Reionization and Ices Explorer) observatory and PUNCH (Polarimeter to Unify the Corona and Heliosphere) satellites within a protective payload fairing inside the Astrotech Space Operations facility at Vandenberg Space Force Base in California, on Thursday, Feb. 27, 2025. SPHEREx will use its telescope to provide an all-sky spectral survey, creating a 3D map of the entire sky to help scientists investigate the origins of our universe. PUNCH will study origins of the Sun’s outflow of material, or the solar wind, capturing continuous 3D images of the Sun’s corona and the solar wind’s journey into the solar system. Liftoff aboard a SpaceX Falcon 9 rocket is targeted for NET 10:09 EST (7:09 p.m. PST), Tuesday, March 4, 2025, at Space Launch Complex 4 East from Vandenberg Space Force Base in California.
Technicians and engineers encapsulate NASA’s SPHEREx (Spectro-Photometer for the History of the Universe, Epoch of Reionization and Ices Explorer) observatory and PUNCH (Polarimeter to Unify the Corona and Heliosphere) satellites within a protective payload fairing inside the Astrotech Space Operations facility at Vandenberg Space Force Base in California, on Thursday, Feb. 27, 2025. SPHEREx will use its telescope to provide an all-sky spectral survey, creating a 3D map of the entire sky to help scientists investigate the origins of our universe. PUNCH will study origins of the Sun’s outflow of material, or the solar wind, capturing continuous 3D images of the Sun’s corona and the solar wind’s journey into the solar system. Liftoff aboard a SpaceX Falcon 9 rocket is targeted for NET 10:09 EST (7:09 p.m. PST), Tuesday, March 4, 2025, at Space Launch Complex 4 East from Vandenberg Space Force Base in California.
Technicians and engineers encapsulate NASA’s SPHEREx (Spectro-Photometer for the History of the Universe, Epoch of Reionization and Ices Explorer) observatory and PUNCH (Polarimeter to Unify the Corona and Heliosphere) satellites within a protective payload fairing inside the Astrotech Space Operations facility at Vandenberg Space Force Base in California, on Thursday, Feb. 27, 2025. SPHEREx will use its telescope to provide an all-sky spectral survey, creating a 3D map of the entire sky to help scientists investigate the origins of our universe. PUNCH will study origins of the Sun’s outflow of material, or the solar wind, capturing continuous 3D images of the Sun’s corona and the solar wind’s journey into the solar system. Liftoff aboard a SpaceX Falcon 9 rocket is targeted for NET 10:09 EST (7:09 p.m. PST), Tuesday, March 4, 2025, at Space Launch Complex 4 East from Vandenberg Space Force Base in California.
Technicians and engineers encapsulate NASA’s SPHEREx (Spectro-Photometer for the History of the Universe, Epoch of Reionization and Ices Explorer) observatory and PUNCH (Polarimeter to Unify the Corona and Heliosphere) satellites within a protective payload fairing inside the Astrotech Space Operations facility at Vandenberg Space Force Base in California, on Saturday, March 1, 2025. SPHEREx will use its telescope to provide an all-sky spectral survey, creating a 3D map of the entire sky to help scientists investigate the origins of our universe. PUNCH will study origins of the Sun’s outflow of material, or the solar wind, capturing continuous 3D images of the Sun’s corona and the solar wind’s journey into the solar system. Liftoff aboard a SpaceX Falcon 9 rocket is targeted for NET 10:09 EST (7:09 p.m. PST), Tuesday, March 4, 2025, at Space Launch Complex 4 East from Vandenberg Space Force Base in California.
Technicians and engineers encapsulate NASA’s SPHEREx (Spectro-Photometer for the History of the Universe, Epoch of Reionization and Ices Explorer) observatory and PUNCH (Polarimeter to Unify the Corona and Heliosphere) satellites within a protective payload fairing inside the Astrotech Space Operations facility at Vandenberg Space Force Base in California, on Thursday, Feb. 27, 2025. SPHEREx will use its telescope to provide an all-sky spectral survey, creating a 3D map of the entire sky to help scientists investigate the origins of our universe. PUNCH will study origins of the Sun’s outflow of material, or the solar wind, capturing continuous 3D images of the Sun’s corona and the solar wind’s journey into the solar system. Liftoff aboard a SpaceX Falcon 9 rocket is targeted for NET 10:09 EST (7:09 p.m. PST), Tuesday, March 4, 2025, at Space Launch Complex 4 East from Vandenberg Space Force Base in California.
Technicians and engineers encapsulate NASA’s SPHEREx (Spectro-Photometer for the History of the Universe, Epoch of Reionization and Ices Explorer) observatory and PUNCH (Polarimeter to Unify the Corona and Heliosphere) satellites within a protective payload fairing inside the Astrotech Space Operations facility at Vandenberg Space Force Base in California, on Thursday, Feb. 27, 2025. SPHEREx will use its telescope to provide an all-sky spectral survey, creating a 3D map of the entire sky to help scientists investigate the origins of our universe. PUNCH will study origins of the Sun’s outflow of material, or the solar wind, capturing continuous 3D images of the Sun’s corona and the solar wind’s journey into the solar system. Liftoff aboard a SpaceX Falcon 9 rocket is targeted for NET 10:09 EST (7:09 p.m. PST), Tuesday, March 4, 2025, at Space Launch Complex 4 East from Vandenberg Space Force Base in California.
Flags for NASA’s IMAP (Interstellar Mapping and Acceleration Probe) mission and its two rideshares, NASA’s exosphere-studying Carruthers Geocorona Observatory and National Oceanic and Atmospheric Administration’s (NOAA) Space Weather Follow On–Lagrange 1 (SWFO-L1) spacecraft fly outside Astrotech Space Operations Facility near NASA’s Kennedy Space Center in Florida. Launch of the three missions on a SpaceX Falcon 9 rocket is targeted for no earlier than Tuesday, Sept. 23, 2025, from Launch Complex 39A at NASA Kennedy.
Technicians at Astrotech Space Operations Facility near NASA’s Kennedy Space Center in Florida encapsulate NASA’s IMAP (Interstellar Mapping and Acceleration Probe), along with the agency’s Carruthers Geocorona Observatory and National Oceanic and Atmospheric Administration’s (NOAA) Space Weather Follow On–Lagrange 1 (SWFO-L1) spacecraft on Tuesday, Sept. 16, 2025, inside a SpaceX Falcon 9 payload fairing. The missions will each focus on different effects of the solar wind — the continuous stream of particles emitted by the Sun — and space weather — the changing conditions in space driven by the Sun — from their origins at the Sun to their farthest reaches billions of miles away at the edge of our solar system.
A SpaceX Falcon 9 rocket with NASA’s IMAP (Interstellar Mapping and Acceleration Probe), the agency’s Carruthers Geocorona Observatory, and National Oceanic and Atmospheric Administration’s (NOAA) Space Weather Follow On–Lagrange 1 (SWFO-L1) spacecraft atop stands vertical at Launch Complex 39A as the sun sets on Monday, Sept. 22, 2025, at the agency’s Kennedy Space Center in Florida. The missions will each focus on different effects of the solar wind — the continuous stream of particles emitted by the Sun — and space weather — the changing conditions in space driven by the Sun — from their origins at the Sun to their farthest reaches billions of miles away at the edge of our solar system.
A SpaceX Falcon 9 rocket with NASA’s IMAP (Interstellar Mapping and Acceleration Probe), the agency’s Carruthers Geocorona Observatory, and National Oceanic and Atmospheric Administration’s (NOAA) Space Weather Follow On–Lagrange 1 (SWFO-L1) spacecraft atop stands vertical at Launch Complex 39A as the sun sets on Monday, Sept. 22, 2025, at the agency’s Kennedy Space Center in Florida. The missions will each focus on different effects of the solar wind — the continuous stream of particles emitted by the Sun — and space weather — the changing conditions in space driven by the Sun — from their origins at the Sun to their farthest reaches billions of miles away at the edge of our solar system.
A SpaceX Falcon 9 rocket with NASA’s IMAP (Interstellar Mapping and Acceleration Probe), the agency’s Carruthers Geocorona Observatory, and National Oceanic and Atmospheric Administration’s (NOAA) Space Weather Follow On–Lagrange 1 (SWFO-L1) spacecraft atop stands vertical at Launch Complex 39A as the sun sets on Monday, Sept. 22, 2025, at the agency’s Kennedy Space Center in Florida. The missions will each focus on different effects of the solar wind — the continuous stream of particles emitted by the Sun — and space weather — the changing conditions in space driven by the Sun — from their origins at the Sun to their farthest reaches billions of miles away at the edge of our solar system.
A SpaceX Falcon 9 rocket carrying NASA’s IMAP (Interstellar Mapping and Acceleration Probe), the agency’s Carruthers Geocorona Observatory, and National Oceanic and Atmospheric Administration’s (NOAA) Space Weather Follow On–Lagrange 1 (SWFO-L1) spacecraft lifts off from Launch Complex 39A at NASA’s Kennedy Space Center in Florida at 7:30 a.m. EDT Wednesday, Sept. 24, 2025. The missions will each focus on different effects of the solar wind — the continuous stream of particles emitted by the Sun — and space weather — the changing conditions in space driven by the Sun — from their origins at the Sun to their farthest reaches billions of miles away at the edge of our solar system.
A SpaceX Falcon 9 rocket carrying NASA’s IMAP (Interstellar Mapping and Acceleration Probe), the agency’s Carruthers Geocorona Observatory, and National Oceanic and Atmospheric Administration’s (NOAA) Space Weather Follow On–Lagrange 1 (SWFO-L1) spacecraft lifts off from Launch Complex 39A at NASA’s Kennedy Space Center in Florida at 7:30 a.m. EDT Wednesday, Sept. 24, 2025. The missions will each focus on different effects of the solar wind — the continuous stream of particles emitted by the Sun — and space weather — the changing conditions in space driven by the Sun — from their origins at the Sun to their farthest reaches billions of miles away at the edge of our solar system.
A SpaceX Falcon 9 rocket carrying NASA’s IMAP (Interstellar Mapping and Acceleration Probe), the agency’s Carruthers Geocorona Observatory, and National Oceanic and Atmospheric Administration’s (NOAA) Space Weather Follow On–Lagrange 1 (SWFO-L1) spacecraft lifts off from Launch Complex 39A at NASA’s Kennedy Space Center in Florida at 7:30 a.m. EDT Wednesday, Sept. 24, 2025. The missions will each focus on different effects of the solar wind — the continuous stream of particles emitted by the Sun — and space weather — the changing conditions in space driven by the Sun — from their origins at the Sun to their farthest reaches billions of miles away at the edge of our solar system.
The sunshade for NASA’s Near-Earth Object (NEO) Surveyor mission towers above a fixture at supplier Applied Aerospace in Stockton, California, in September 2025. Standing at over 20 feet (6 meters) high, the sunshade is the largest component of spacecraft. The structure was next shipped to BAE Systems in Boulder, Colorado, for a “fit check” with the spacecraft bus. For scale, technicians and engineers from the project in front of the sunshade. The sunshade’s Sun-facing surface (visible here) will next be fitted with solar panels that will generate power for the spacecraft after launch. The spacecraft’s instrument enclosure, which houses the telescope and sensitive infrared cameras, will be located behind the sunshade, allowing the spacecraft to detect and track near-Earth objects that would otherwise be hidden by the Sun’s glare. Targeting launch in late 2027, the NEO Surveyor mission is led by Professor Amy Mainzer at the University of California, Los Angeles for NASA’s Planetary Defense Coordination Office and is being managed by the agency’s Jet Propulsion Laboratory in Southern California for the Planetary Missions Program Office at NASA’s Marshall Space Flight Center in Huntsville, Alabama. BAE Systems and the Space Dynamics Laboratory in Logan, Utah, and Teledyne are among the companies that were contracted to build the spacecraft and its instrumentation. The Laboratory for Atmospheric and Space Physics at the University of Colorado Boulder will support operations, and IPAC at Caltech in Pasadena, California, is responsible for producing some of the mission’s data products. Caltech manages JPL for NASA. More information about NEO Surveyor is available at: https://science.nasa.gov/mission/neo-surveyor/
The sunshade for NASA’s Near-Earth Object (NEO) Surveyor mission towers above a fixture at supplier Applied Aerospace in Stockton, California, in September 2025. Standing at over 20 feet (6 meters) high, the sunshade is the largest component of spacecraft. The structure was next shipped to BAE Systems in Boulder, Colorado, for a “fit check” with the spacecraft bus. The sunshade’s Sun-facing surface (visible here) will next be fitted with solar panels that will generate power for the spacecraft after launch. The spacecraft’s instrument enclosure, which houses the telescope and sensitive infrared cameras, will be located behind the sunshade, allowing the spacecraft to detect and track near-Earth objects that would otherwise be hidden by the Sun’s glare. Targeting launch in late 2027, the NEO Surveyor mission is led by Professor Amy Mainzer at the University of California, Los Angeles for NASA’s Planetary Defense Coordination Office and is being managed by the agency’s Jet Propulsion Laboratory in Southern California for the Planetary Missions Program Office at NASA’s Marshall Space Flight Center in Huntsville, Alabama. BAE Systems and the Space Dynamics Laboratory in Logan, Utah, and Teledyne are among the companies that were contracted to build the spacecraft and its instrumentation. The Laboratory for Atmospheric and Space Physics at the University of Colorado Boulder will support operations, and IPAC at Caltech in Pasadena, California, is responsible for producing some of the mission’s data products. Caltech manages JPL for NASA. More information about NEO Surveyor is available at: https://science.nasa.gov/mission/neo-surveyor/
Superimposed on an image taken by the HiRISE camera aboard NASA's Mars Reconnaissance Orbiter, this map shows the path taken by the agency's Perseverance Mars rover between Jan. 31, 2024, and June 11, shortly after it arrived at a geologic area of interest the science team calls "Bright Angel." The route where the rover paralleled the Neretva Vallis river channel is depicted in white. The portion of the route where the rover was inside the river channel is depicted in pale blue. The dots along the white line signify locations where the rover stopped after completing a traverse. The University of Arizona, in Tucson, operates HiRISE, which was built by BAE Systems, in Boulder, Colorado. JPL manages the Mars Reconnaissance Orbiter Project for NASA's Science Mission Directorate, Washington. A key objective for Perseverance's mission on Mars is astrobiology, including the search for signs of ancient microbial life. The rover will characterize the planet's geology and past climate, pave the way for human exploration of the Red Planet, and be the first mission to collect and cache Martian rock and regolith (broken rock and dust). Subsequent NASA missions, in cooperation with ESA (European Space Agency), would send spacecraft to Mars to collect these sealed samples from the surface and return them to Earth for in-depth analysis. https://photojournal.jpl.nasa.gov/catalog/PIA26334
A truck arrives at NASA's Jet Propulsion Laboratory in Southern California on June 3, 2024, to deliver the Medium Articulating Transportation System (MATS), which will be used during the construction and transportation of components for NASA's Near-Earth Object Surveyor mission. Originating at the aerospace company Beyond Gravity in Vienna, Austria, the MATS traveled via ship through the Panama Canal to Port Hueneme, California, before arriving by road at JPL. Construction has begun on NEO Surveyor's instrument enclosure in the High Bay 1 clean room at JPL's Spacecraft Assembly Facility. When the enclosure is complete later this year, it will be moved inside the MATS to NASA's Johnson Space Center in Houston for environmental testing. The MATS is a transportable clean room with its own filtration and climate control systems that keep the spacecraft and components clean, stable, and safe while being moved between facilities. NEO Surveyor's instrument enclosure contains the spacecraft's telescope, mirrors, and infrared sensors that will be used to detect, track, and characterize the most hazardous near-Earth objects. BAE Systems, Space Dynamics Laboratory, and Teledyne are among the aerospace and engineering companies contracted to build the spacecraft and its instrumentation. The Laboratory for Atmospheric and Space Physics at the University of Colorado, Boulder will support operations, and IPAC at Caltech in Pasadena, California, is responsible for processing survey data and producing the mission's data products. JPL manages the project; Caltech manages JPL for NASA. Launching no earlier than 2027, NEO Surveyor supports the objectives of NASA's Planetary Defense Coordination Office (PDCO) at NASA Headquarters in Washington. The NASA Authorization Act of 2005 directed NASA to discover and characterize at least 90% of the near-Earth objects more than 140 meters (460 feet) across that come within 30 million miles (48 million kilometers) of our planet's orbit. Objects of this size can cause significant regional damage, or worse, should they impact the Earth. https://photojournal.jpl.nasa.gov/catalog/PIA26381
At NASA's Jet Propulsion Laboratory in Southern California, on June 7, 2024, clean room technicians use a crane to lift the lid of the Medium Articulating Transportation System (MATS) that will be used during the construction and transportation of components for NASA's Near-Earth Object Surveyor mission. Inside the MATS is the Medium Articulating Assembly Dolly (MAAD), a platform that will support the spacecraft's instrument enclosure, which is being constructed inside the High Bay 1 clean room at JPL's Spacecraft Assembly Facility. The MAAD is an articulating platform on which a spacecraft (or spacecraft components) can be mounted securely and positioned as required during assembly. It can tilt a spacecraft vertically and horizontally, rotating it 360 degrees. JPL plans to use the MAAD for future missions to reduce the number of crane lifts during assembly, test, and launch operations, known as ATLO. NEO Surveyor is the first mission to use the platform. NEO Surveyor's instrument enclosure contains the spacecraft's telescope, mirrors, and infrared sensors that will be used to detect, track, and characterize the most hazardous near-Earth objects. BAE Systems, Space Dynamics Laboratory, and Teledyne are among the aerospace and engineering companies contracted to build the spacecraft and its instrumentation. The Laboratory for Atmospheric and Space Physics at the University of Colorado, Boulder will support operations, and IPAC at Caltech in Pasadena, California, is responsible for processing survey data and producing the mission's data products. JPL manages the project; Caltech manages JPL for NASA. Launching no earlier than 2027, NEO Surveyor supports the objectives of NASA's Planetary Defense Coordination Office (PDCO) at NASA Headquarters in Washington. The NASA Authorization Act of 2005 directed NASA to discover and characterize at least 90% of the near-Earth objects more than 140 meters (460 feet) across that come within 30 million miles (48 million kilometers) of our planet's orbit. Objects of this size can cause significant regional damage, or worse, should they impact the Earth. https://photojournal.jpl.nasa.gov/catalog/PIA26382
The instrument enclosure for NASA's Near-Earth Object (NEO) Surveyor on May 22, 2025, is seen in a clean room at the Space Dynamics Laboratory (SDL) in Logan, Utah, shortly after arriving from the agency's Jet Propulsion Laboratory in Southern California, where it was assembled. The instrument enclosure is attached to an articulating assembly dolly and wrapped in silver-colored material (composed of a metalized polyester film and a low charging polyethylene laminate) to protect the flight hardware from static electricity and dust particles during transport. The instrument enclosure will house the observatory's scientific instrument, which includes a three-reflection aluminum telescope, state-of-the-art infrared detectors, and an innovative passive cooling system to keep the instrument at cryogenic temperatures. The telescope, which has an aperture of nearly 20 inches (50 centimeters), features detectors sensitive to two infrared wavelengths in which near-Earth objects re-radiate solar heat. The instrument enclosure is designed to ensure heat produced by the spacecraft and instrument during operations doesn't interfere with its infrared observations. As NASA's first space-based detection mission specifically designed for planetary defense, NEO Surveyor will seek out, measure, and characterize the hardest-to-find asteroids and comets that might pose a hazard to Earth. While many near-Earth objects don't reflect much visible light, they glow brightly in infrared light due to heating by the Sun. Targeting launch in late 2027, the NEO Surveyor mission is led by Professor Amy Mainzer at UCLA for NASA's Planetary Defense Coordination Office and is being managed by JPL for the Planetary Missions Program Office at NASA's Marshall Space Flight Center in Huntsville, Alabama. BAE Systems, SDL, and are among the companies that were contracted to build the spacecraft and its instrumentation. The Laboratory for Atmospheric and Space Physics at the University of Colorado Boulder will support operations, and IPAC at Caltech in Pasadena, California, is responsible for producing some of the mission's data products. Caltech manages JPL for NASA. https://photojournal.jpl.nasa.gov/catalog/PIA26589
Technicians and engineers inspect NASA's Near-Earth Object (NEO) Surveyor's instrument enclosure at the Space Dynamics Laboratory (SDL) in Logan, Utah, after it arrived from the agency's Jet Propulsion Laboratory in Southern California in May 2025. The instrument enclosure will house the spacecraft's telescope, which is fitted with state-of-the-art detectors and a novel cryogenic system to keep the instrument cool. The telescope, which has an aperture of nearly 20 inches (50 centimeters), features detectors sensitive to two infrared wavelengths in which near-Earth objects re-radiate solar heat. The instrument enclosure is designed to ensure heat produced by the telescope during operations doesn't interfere with its observations. As NASA's first space-based detection mission specifically designed for planetary defense, NEO Surveyor will seek out, measure, and characterize the hardest-to-find asteroids and comets that might pose a hazard to Earth. While many near-Earth objects don't reflect much visible light, they glow brightly in infrared light due to heating by the Sun. Targeting launch in late 2027, the NEO Surveyor mission is led by Professor Amy Mainzer at UCLA for NASA's Planetary Defense Coordination Office and is being managed by JPL for the Planetary Missions Program Office at NASA's Marshall Space Flight Center in Huntsville, Alabama. BAE Systems, SDL, and are among the companies that were contracted to build the spacecraft and its instrumentation. The Laboratory for Atmospheric and Space Physics at the University of Colorado Boulder will support operations, and IPAC at Caltech in Pasadena, California, is responsible for producing some of the mission's data products. Caltech manages JPL for NASA. https://photojournal.jpl.nasa.gov/catalog/PIA26590
The aluminum telescope of NASA’s Near-Earth Object (NEO) Surveyor mission is shown here attached its flight base frame at a Space Dynamics Laboratory (SDL) clean room in Logan, Utah, in early September 2025. The telescope is connected via a system of struts that prevent heat from passing from the spacecraft to the instrument, keeping it secure, isolated, and cool. The spacecraft’s instrument enclosure will later be fitted over the instrumentation and then the pair will be attached to the spacecraft bus and sunshade. With an aperture of nearly 20 inches (50 centimeters), the telescope features detectors sensitive to two infrared wavelengths in which near-Earth objects re-radiate solar heat. The instrument enclosure is designed to ensure heat produced by the spacecraft and instrument during operations doesn’t interfere with its infrared observations. Targeting launch in late 2027, the NEO Surveyor mission is led by Professor Amy Mainzer at the University of California, Los Angeles for NASA’s Planetary Defense Coordination Office and is being managed by the agency’s Jet Propulsion Laboratory in Southern California for the Planetary Missions Program Office at NASA’s Marshall Space Flight Center in Huntsville, Alabama. BAE Systems and the Space Dynamics Laboratory in Logan, Utah, and Teledyne are among the companies that were contracted to build the spacecraft and its instrumentation. The Laboratory for Atmospheric and Space Physics at the University of Colorado Boulder will support operations, and IPAC at Caltech in Pasadena, California, is responsible for producing some of the mission’s data products. Caltech manages JPL for NASA. More information about NEO Surveyor is available at: https://science.nasa.gov/mission/neo-surveyor/
Engineers with NASA’s Near-Earth Object (NEO) Surveyor mission work in a Space Dynamics Laboratory (SDL) clean room in Logan, Utah, to attach the spacecraft’s aluminum telescope to the flight base frame in early September 2025. The telescope is connected via a system of struts that prevent heat from passing from the spacecraft to the instrument, keeping it secure, isolated, and cool. With an aperture of nearly 20 inches (50 centimeters), the telescope features detectors sensitive to two infrared wavelengths in which near-Earth objects re-radiate solar heat. The instrument enclosure is designed to ensure heat produced by the spacecraft and instrument during operations doesn’t interfere with its infrared observations. Targeting launch in late 2027, the NEO Surveyor mission is led by Professor Amy Mainzer at the University of California, Los Angeles for NASA’s Planetary Defense Coordination Office and is being managed by the agency’s Jet Propulsion Laboratory in Southern California for the Planetary Missions Program Office at NASA’s Marshall Space Flight Center in Huntsville, Alabama. BAE Systems and the Space Dynamics Laboratory in Logan, Utah, and Teledyne are among the companies that were contracted to build the spacecraft and its instrumentation. The Laboratory for Atmospheric and Space Physics at the University of Colorado Boulder will support operations, and IPAC at Caltech in Pasadena, California, is responsible for producing some of the mission’s data products. Caltech manages JPL for NASA. More information about NEO Surveyor is available at: https://science.nasa.gov/mission/neo-surveyor/
The instrument enclosure for NASA's Near-Earth Object Surveyor is prepared for environmental testing inside the historic Chamber A in the Space Environment Simulation Laboratory at the agency's Johnson Space Center in Houston in December 2024. Mounted to its articulating platform, on which it was securely positioned during assembly, the 12-foot-long (3.7-meter-long) angular structure was inspected by technicians before being placed inside the testing chamber. Figure A shows the reflective side of the instrument enclosure as it was rotated on the assembly dolly before being transferred to a testing platform. The cavernous opening to Chamber A is in the background. The instrument enclosure is designed to protect the spacecraft's infrared telescope while also removing heat from it during operations. After environmental testing was completed, the enclosure returned to NASA's Jet Propulsion Laboratory in Southern California for further work, after which it will ship to the Space Dynamics Laboratory (SDL) in Logan, Utah, and be joined to the telescope. Both the instrument enclosure and telescope were assembled at JPL. As NASA's first space-based detection mission specifically designed for planetary defense, NEO Surveyor will seek out, measure, and characterize the hardest-to-find asteroids and comets that might pose a hazard to Earth. While many near-Earth objects don't reflect much visible light, they glow brightly in infrared light due to heating by the Sun. The spacecraft's telescope, which has an aperture of nearly 20 inches (50 centimeters), features detectors sensitive to two infrared wavelengths in which near-Earth objects re-radiate solar heat. Targeting launch in late 2027, the NEO Surveyor mission is led by Prof. Amy Mainzer at UCLA for NASA's Planetary Defense Coordination Office and is being managed by JPL for the Planetary Missions Program Office at NASA's Marshall Space Flight Center in Huntsville, Alabama. BAE Systems, SDL, and Teledyne are among the companies that were contracted to build the spacecraft and its instrumentation. The Laboratory for Atmospheric and Space Physics at the University of Colorado Boulder will support operations, and Caltech/IPAC in Pasadena, California, is responsible for producing some of the mission's data products. Caltech manages JPL for NASA. https://photojournal.jpl.nasa.gov/catalog/PIA26582
The instrument enclosure of NASA's Near-Earth Object Surveyor is prepared for critical environmental tests inside the historic Chamber A at the Space Environment Simulation Laboratory at the agency's Johnson Space Center in Houston in December 2024. Wrapped in silver thermal blanketing, the 12-foot-long (3.7-meter-long) angular structure was subjected to the frigid, airless conditions that the spacecraft will experience when in deep space. The cavernous thermal-vacuum test facility is famous for testing the Apollo spacecraft that traveled to the Moon in the 1960s and '70s. The instrument enclosure is designed to protect the spacecraft's infrared telescope while also removing heat from it during operations. After environmental testing was completed, the enclosure returned to NASA's Jet Propulsion Laboratory in Southern California for further work, after which it will ship to the Space Dynamics Laboratory (SDL) in Logan, Utah, and be joined to the telescope. Both the instrument enclosure and telescope were assembled at JPL. As NASA's first space-based detection mission specifically designed for planetary defense, NEO Surveyor will seek out, measure, and characterize the hardest-to-find asteroids and comets that might pose a hazard to Earth. While many near-Earth objects don't reflect much visible light, they glow brightly in infrared light due to heating by the Sun. The spacecraft's telescope, which has an aperture of nearly 20 inches (50 centimeters), features detectors sensitive to two infrared wavelengths in which near-Earth objects re-radiate solar heat. Targeting launch in late 2027, the NEO Surveyor mission is led by Prof. Amy Mainzer at UCLA for NASA's Planetary Defense Coordination Office and is being managed by JPL for the Planetary Missions Program Office at NASA's Marshall Space Flight Center in Huntsville, Alabama. BAE Systems, SDL, and Teledyne are among the companies that were contracted to build the spacecraft and its instrumentation. The Laboratory for Atmospheric and Space Physics at the University of Colorado Boulder will support operations, and Caltech/IPAC in Pasadena, California, is responsible for producing some of the mission's data products. Caltech manages JPL for NASA. https://photojournal.jpl.nasa.gov/catalog/PIA26583
The route (shown in blue) that the agency's Perseverance Mars rover is expected to take as it climbs up the western rim of Jezero Crater is superimposed on this image taken by the HiRISE camera aboard NASA's Mars Reconnaissance Orbiter. At upper right is "Serpentine Rapids," the final geologic location of interest for the Perseverance science team before the rover begins its ascent. "Dox Castle" is a region the science team would like to explore during the rover's ascent. Two of the first regions the science team wants study at the top of the crater are "Pico Turquino" and "Witch Hazel Hill." Imagery from NASA's Mars orbiters indicates that Pico Turquino contains ancient fractures that may have been caused by hydrothermal activity in the distant past. Orbital views of Witch Hazel show layered materials that likely date from a time when Mars had a very different climate than today. Those views have revealed light-toned bedrock similar to what was found at "Bright Angel," the area where Perseverance recently discovered and sampled the "Cheyava Falls" rock, which exhibits chemical signatures and structures that could possibly have been formed by life billions of years ago when the area contained running water. The distance the rover will drive to get from Serpentine Rapids to the Aurora Park/Pico Turquino area is about 1.1 miles (1.8 kilometers); the change in elevation between the two locations is about 980 feet (300 meters). The distance covered to go from Aurora Park/Pico Turquino to Witch Hazel Hill is about 1.2 miles (2,000 meters) and the change in elevation is about 820 feet (250 meters). The University of Arizona, in Tucson, operates HiRISE, which was built by BAE Systems, in Boulder, Colorado. JPL manages the Mars Reconnaissance Orbiter Project for NASA's Science Mission Directorate, Washington. A key objective for Perseverance's mission on Mars is astrobiology, including the search for signs of ancient microbial life. The rover will characterize the planet's geology and past climate, pave the way for human exploration of the Red Planet, and be the first mission to collect and cache Martian rock and regolith (broken rock and dust). https://photojournal.jpl.nasa.gov/catalog/PIA26374
After arriving at the Space Dynamics Laboratory (SDL) in Logan, Utah, from NASA's Jet Propulsion Laboratory in Southern California in May 2025, the instrument enclosure for the agency's Near-Earth Object (NEO) Surveyor mission was inspected prior to thermal vacuum testing. Shown here, the enclosure stands vertically atop an articulating assembly dolly. The shiny and black surfaces of the enclosure optimize the reflection and radiation properties of the structure. The telescope, which has an aperture of nearly 20 inches (50 centimeters), features detectors sensitive to two infrared wavelengths in which near-Earth objects re-radiate solar heat. The instrument enclosure is designed to ensure heat produced by the telescope during operations doesn't interfere with its observations. As NASA's first space-based detection mission specifically designed for planetary defense, NEO Surveyor will seek out, measure, and characterize the hardest-to-find asteroids and comets that might pose a hazard to Earth. While many near-Earth objects don't reflect much visible light, they glow brightly in infrared light due to heating by the Sun. Targeting launch in late 2027, the NEO Surveyor mission is led by Professor Amy Mainzer at UCLA for NASA's Planetary Defense Coordination Office and is being managed by JPL for the Planetary Missions Program Office at NASA's Marshall Space Flight Center in Huntsville, Alabama. BAE Systems, SDL, and are among the companies that were contracted to build the spacecraft and its instrumentation. The Laboratory for Atmospheric and Space Physics at the University of Colorado Boulder will support operations, and IPAC at Caltech in Pasadena, California, is responsible for producing some of the mission's data products. Caltech manages JPL for NASA. https://photojournal.jpl.nasa.gov/catalog/PIA26597
An engineer inspects the surface of four mid-wavelength infrared science detectors for NASA’s Near-Earth Object (NEO) Surveyor mission atop a clean room bench at the Space Dynamics Laboratory (SDL) in Logan, Utah. Mounted to a sensor chip assembly, the four blue-green-colored detectors are made with mercury cadmium telluride (HgCdTe), a versatile semiconducting alloy that is sensitive to infrared wavelengths. There are two such assemblies that form the heart of NEO Surveyor’s two science cameras. These state-of-the-art cameras sense solar heat re-radiated by near-Earth objects. The mission’s cameras and telescope, which has an aperture of nearly 20 inches (50 centimeters), will be housed inside the spacecraft’s instrument enclosure, a structure that is designed to ensure heat produced by the spacecraft and instrument during operations doesn’t interfere with its infrared observations. Targeting launch in late 2027, the NEO Surveyor mission is led by Professor Amy Mainzer at the University of California, Los Angeles for NASA’s Planetary Defense Coordination Office and is being managed by the agency’s Jet Propulsion Laboratory in Southern California for the Planetary Missions Program Office at NASA’s Marshall Space Flight Center in Huntsville, Alabama. BAE Systems and the Space Dynamics Laboratory in Logan, Utah, and Teledyne are among the companies that were contracted to build the spacecraft and its instrumentation. The Laboratory for Atmospheric and Space Physics at the University of Colorado Boulder will support operations, and IPAC at Caltech in Pasadena, California, is responsible for producing some of the mission’s data products. Caltech manages JPL for NASA. More information about NEO Surveyor is available at: https://science.nasa.gov/mission/neo-surveyor/
Four mid-wavelength infrared science detectors for NASA’s Near-Earth Object (NEO) Surveyor mission are shown here on a clean room bench at the Space Dynamics Laboratory (SDL) in Logan, Utah. Mounted to a sensor chip assembly, the four blue-green-colored detectors are made with mercury cadmium telluride (HgCdTe), a versatile semiconducting alloy that is sensitive to infrared wavelengths. There are two such assemblies that form the heart of NEO Surveyor’s two science cameras. These state-of-the-art cameras sense solar heat re-radiated by near-Earth objects. The mission’s cameras and telescope, which has an aperture of nearly 20 inches (50 centimeters), will be housed inside the spacecraft’s instrument enclosure, a structure that is designed to ensure heat produced by the spacecraft and instrument during operations doesn’t interfere with its infrared observations. Targeting launch in late 2027, the NEO Surveyor mission is led by Professor Amy Mainzer at the University of California, Los Angeles for NASA’s Planetary Defense Coordination Office and is being managed by the agency’s Jet Propulsion Laboratory in Southern California for the Planetary Missions Program Office at NASA’s Marshall Space Flight Center in Huntsville, Alabama. BAE Systems and the Space Dynamics Laboratory in Logan, Utah, and Teledyne are among the companies that were contracted to build the spacecraft and its instrumentation. The Laboratory for Atmospheric and Space Physics at the University of Colorado Boulder will support operations, and IPAC at Caltech in Pasadena, California, is responsible for producing some of the mission’s data products. Caltech manages JPL for NASA. More information about NEO Surveyor is available at: https://science.nasa.gov/mission/neo-surveyor/