This frame from a movie shows the progression of NASA's Near-Earth Object Wide-field Survey Explorer (NEOWISE) investigation for the mission's first three years following its restart in December 2013. Green circles represent near-Earth objects (asteroids and comets that come within 1.3 astronomical units of the sun; one astronomical unit is Earth's distance from the sun). Yellow squares represent comets. Gray dots represent all other asteroids, which are mostly in the main asteroid belt between Mars and Jupiter. The orbits of Mercury, Venus, Earth and Mars are shown. The spacecraft has characterized a total of 693 near-Earth objects since the mission was restarted in December 2013. Of these, 114 are new discoveries. A movie is avaiable at https://photojournal.jpl.nasa.gov/catalog/PIA21653

Near-Earth objects (NEOs) are asteroids and comets that orbit the Sun like the planets with orbits that come within 30 million miles of Earth’s orbit. NASA established the Planetary Defense Coordination Office (PDCO) to manage the agency’s ongoing efforts in Planetary Defense, which is the “applied planetary science” to address the NEO impact hazard. One key element of the PDCO is NASA’s NEO Observations program, which is composed of projects to find, track, and characterize NEOs. Here’s what we’ve found so far. This page is updated monthly with the most up-to-date numbers.

NASA NEOWISE, snapped this infrared picture of near-Earth object 1998 KN3 as it zips past a cloud of dense gas and dust near the Orion nebula.

The NEOCam sensor right is the lynchpin for the proposed Near Earth Object Camera, or NEOCam, space mission left.

This frame from a movie shows the progression of NASA Near-Earth Object Wide-field Survey Explorer NEOWISE investigation for the mission first two years following its restart in December 2013. Green circles represent near-Earth objects.

NASA Administrator Bill Nelson points to a model of the Near-Earth Object Surveyor space telescope (NEO Surveyor) as he testifies before the Senate Committee on Commerce, Science, and Transportation during a hearing titled “Examining NASA’s Budget and Priorities,” Tuesday, May 16, 2023, at the Russell Senate Office Building in Washington. Photo Credit: (NASA/Bill Ingalls)

The red dot at the center of this image is the first near-Earth asteroid discovered by NASA Wide-Field Infrared Survey Explorer, or WISE -- an all-sky mapping infrared mission designed to see all sorts of cosmic objects.

Asteroid 1997 QK1 is shown to be an elongated, peanut-shaped near-Earth object in this series of 28 radar images obtained by the Deep Space Network's Goldstone Solar System Radar on Aug. 21, 2025. The asteroid is about 660 feet (200 meters) long and completes one rotation every 4.8 hours. It passed closest to our planet on the day before these observations were made at a distance of about 1.9 million miles (3 million kilometers), or within eight times the distance between Earth and the Moon. The 2025 flyby is the closest that 1997 QK1 has approached to Earth in more than 350 years. Prior to the recent Goldstone observations, very little was known about the asteroid. These observations resolve surface features down to a resolution of about 25 feet (7.5 meters) and reveal that the object has two rounded lobes that are connected, with one lobe twice the size of the other. Both lobes appear to have concavities that are tens of meters deep. Asteroid 1997 QK1 is likely a "contact binary," one of dozens of such objects imaged by Goldstone. At least 15% of near-Earth asteroids larger than about 660 feet (200 meters) have a contact binary shape. The asteroid is classified as potentially hazardous, but it does not pose a hazard to Earth for the foreseeable future. These Goldstone measurements have greatly reduced the uncertainties in the asteroid's distance from Earth and in its future motion for many decades. The Goldstone Solar System Radar Group is supported by NASA's Near-Earth Object Observations Program within the Planetary Defense Coordination Office at the agency's headquarters in Washington. Managed by NASA's Jet Propulsion Laboratory, the Deep Space Network receives programmatic oversight from Space Communications and Navigation program office within the Space Operations Mission Directorate, also at NASA Headquarters. https://photojournal.jpl.nasa.gov/catalog/PIA26588

Data from NASA Wide-field Infrared Survey Explorer has led to revisions in the estimated population of near-Earth asteroids. The most accurate survey to date has allowed new estimates of the total numbers of objects in different size categories.

These first radar images of 2015 TB145 from the National Science Foundation 1,000-foot 305-meter Arecibo Observatory in Puerto Rico, indicate the near-Earth object is spherical in shape and approximately 2,000 feet 600 meters in diameter. The radar images were taken on Oct. 30, 2015, and the image resolution is 25 feet (7.5 meters) per pixel. The celestial object is more than likely a dead comet that has shed its volatiles after numerous passes around the sun. http://photojournal.jpl.nasa.gov/catalog/PIA20040

This mosaic shows NASA's radar observations in one-minute increments of asteroid 2024 MK, a 500-foot-wide (150-meter-wide) near-Earth object, made June 30, 2024, a day after it passed our planet from a distance of only 184,00 miles (295,000 kilometers). The Deep Space Network's 230-foot (70-meter) Goldstone Solar System Radar, called Deep Space Station 14 (or DSS-14), was used to transmit radio frequency signals to the asteroid, and the 114-foot (34-meter) DSS-13 received the reflected signals. The result of this "bistatic" radar observation is a detailed image of the asteroid's surface, revealing concavities, ridges, and boulders about 30 feet (10 meters) wide. The observations were made just before 5:55 a.m. UTC June 30 (10:55 p.m. PDT June 29). The asteroid's close approach occurred at 13:49 UTC June 29 (6:49 a.m. PDT June 29). Close approaches of near-Earth objects the size of 2024 MK are relatively rare, occurring about every couple of decades, on average, so scientists at NASA's Jet Propulsion Laboratory in Southern California sought to gather as much data about the object as possible. The Goldstone Solar System Radar Group is supported by NASA's Near-Earth Object Observations Program within the Planetary Defense Coordination Office at the agency's headquarters in Washington. Managed by NASA's Jet Propulsion Laboratory, the Deep Space Network receives programmatic oversight from Space Communications and Navigation program office within the Space Operations Mission Directorate, also at NASA Headquarters. Animation available at https://photojournal.jpl.nasa.gov/catalog/PIA26383

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/

This artist's concept depicts NASA's Near-Earth Object Surveyor (NEO Surveyor) in deep space. After launch, the spacecraft will travel a million miles to a region of gravitational stability – called the L1 Lagrange point – between Earth and the Sun. From there, its large sunshade will block the glare and heat of sunlight, allowing the mission to discover and track near-Earth objects as they approach Earth from the direction of the Sun, which is difficult for other observatories to do. The black-paneled angular structure in the belly of the spacecraft is the instrument enclosure that is being built at NASA's Jet Propulsion Laboratory in Southern California. The spacecraft's only instrument, its infrared telescope, will be installed inside the enclosure. Fabricated from dark composite material that allows heat to escape, the enclosure will help keep the telescope cool and prevent its own heat from obscuring observations. https://photojournal.jpl.nasa.gov/catalog/PIA26388

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/

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/

CAPE CANAVERAL, Fla. – At NASA’s Kennedy Space Center in Florida, workers are constructing 40-foot-diameter dish antenna arrays for the Ka-Band Objects Observation and Monitoring, or Ka-BOOM system. The antennas will be part of the operations command center facility. The construction site is near the former Vertical Processing Facility, which has been demolished. The Ka-BOOM project is one of the final steps in developing the techniques to build a high power, high resolution radar system capable of becoming a Near Earth Object Early Warning System. While also capable of space communication and radio science experiments, developing radar applications is the primary focus of the arrays. Photo credit: NASA/ Ben Smegelsky

CAPE CANAVERAL, Fla. – At NASA’s Kennedy Space Center in Florida, workers are constructing 40-foot-diameter dish antenna arrays for the Ka-Band Objects Observation and Monitoring, or Ka-BOOM system. The antennas will be part of the operations command center facility. The construction site is near the former Vertical Processing Facility, which has been demolished. The Ka-BOOM project is one of the final steps in developing the techniques to build a high power, high resolution radar system capable of becoming a Near Earth Object Early Warning System. While also capable of space communication and radio science experiments, developing radar applications is the primary focus of the arrays. Photo credit: NASA/ Ben Smegelsky

CAPE CANAVERAL, Fla. – At NASA’s Kennedy Space Center in Florida, new towers are being constructed for the Antenna Test Bed Array for the Ka-Band Objects Observation and Monitoring, or Ka-BOOM system. The antennas will be part of the operations command center facility. The construction site is near the former Vertical Processing Facility, which has been demolished. The Ka-BOOM project is one of the final steps in developing the techniques to build a high power, high resolution radar system capable of becoming a Near Earth Object Early Warning System. While also capable of space communication and radio science experiments, developing radar applications is the primary focus of the arrays. Photo credit: NASA/ Ben Smegelsky

CAPE CANAVERAL, Fla. – At NASA’s Kennedy Space Center in Florida, workers are constructing 40-foot-diameter dish antenna arrays for the Ka-Band Objects Observation and Monitoring, or Ka-BOOM system. The antennas will be part of the operations command center facility. The construction site is near the former Vertical Processing Facility, which has been demolished. The Ka-BOOM project is one of the final steps in developing the techniques to build a high power, high resolution radar system capable of becoming a Near Earth Object Early Warning System. While also capable of space communication and radio science experiments, developing radar applications is the primary focus of the arrays. Photo credit: NASA/ Ben Smegelsky

CAPE CANAVERAL, Fla. – At NASA’s Kennedy Space Center in Florida, workers are constructing 40-foot-diameter dish antenna arrays for the Ka-Band Objects Observation and Monitoring, or Ka-BOOM system. The antennas will be part of the operations command center facility. The construction site is near the former Vertical Processing Facility, which has been demolished. The Ka-BOOM project is one of the final steps in developing the techniques to build a high power, high resolution radar system capable of becoming a Near Earth Object Early Warning System. While also capable of space communication and radio science experiments, developing radar applications is the primary focus of the arrays. Photo credit: NASA/ Ben Smegelsky

CAPE CANAVERAL, Fla. – At NASA’s Kennedy Space Center in Florida, construction is almost complete on the Antenna Test Bed Array for the Ka-Band Objects Observation and Monitoring, or Ka-BOOM, system. The Ka-BOOM project is one of the final steps in developing the techniques to build a high power, high resolution radar system capable of becoming a Near Earth Object Early Warning System. While also capable of space communication and radio science experiments, developing radar applications is the primary focus of the arrays. The 40-foot-diameter dish antenna arrays are near the former Vertical Processing Facility, which has been demolished. Photo credit: NASA_Charisse Nahser

CAPE CANAVERAL, Fla. – At NASA’s Kennedy Space Center in Florida, construction is almost complete on the Antenna Test Bed Array for the Ka-Band Objects Observation and Monitoring, or Ka-BOOM, system. The Ka-BOOM project is one of the final steps in developing the techniques to build a high power, high resolution radar system capable of becoming a Near Earth Object Early Warning System. While also capable of space communication and radio science experiments, developing radar applications is the primary focus of the arrays. The 40-foot-diameter dish antenna arrays are near the former Vertical Processing Facility, which has been demolished. Photo credit: NASA_Charisse Nahser

The Near Earth Asteroid Rendezvous (NEAR) spacecraft embarks on a journey that will culminate in a close encounter with an asteroid. The launch of NEAR inaugurates NASA's irnovative Discovery program of small-scale planetary missions with rapid, lower-cost development cycles and focused science objectives. NEAR will rendezvous in 1999 with the asteroid 433 Eros to begin the first long-term, close-up look at an asteroid's surface composition and physical properties. NEAR's science payload includes an x-ray/gamma ray spectrometer, an near-infrared spectrograph, a laser rangefinder, a magnetometer, a radio science experiment and a multi-spectral imager.

NASA's Galaxy Evolution Explorer took this image of the spiral galaxy Messier 51 on June 19 and 20, 2003. Messier 51 is located 27 million light-years from Earth. Due to a lack of star formation, the companion galaxy in the top of the picture is barely visible as a near ultraviolet object. http://photojournal.jpl.nasa.gov/catalog/PIA04628

CAPE CANAVERAL, Fla. – At NASA’s Kennedy Space Center in Florida, Marc Seibert, the manager for Tracking and Timing Integration in the Research and Technology Management Office, stands near one of the three antennas that comprise the KA-Band Objects Observation and Monitoring, or Ka-BOOM, System. The Ka-BOOM project is one of the final steps in developing the techniques to build a high power, high resolution radar system capable of becoming a Near Earth Object Early Warning System. While also capable of space communication and radio science experiments, developing radar applications is the primary focus of the arrays. The 40-foot-diameter dish antenna arrays are near the former Vertical Processing Facility, which has been demolished. Photo credit: NASA_Jim Grossmann

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

In this image, the NASA/ESA Hubble Space Telescope has captured the smoking gun of a newborn star, the Herbig–Haro objects numbered 7 to 11 (HH 7–11). These five objects, visible in blue in the top center of the image, lie within NGC 1333, a reflection nebula full of gas and dust found about a thousand light-years away from Earth. Bright patches of nebulosity near newborn stars, Herbig-Haro objects like HH 7–11 are transient phenomena. Traveling away from the star that created them at a speed of up to about 150,000 miles per hour, they disappear into nothingness within a few tens of thousands of years. The young star that is the source of HH 7–11 is called SVS 13, and all five objects are moving away from SVS 13 toward the upper left. The current distance between HH 7 and SVS 13 is about 20,000 times the distance between Earth and the Sun. Herbig–Haro objects are formed when jets of ionized gas ejected by a young star collide with nearby clouds of gas and dust at high speeds. The Herbig-Haro objects visible in this image are no exception to this and were formed when the jets from the newborn star SVS 13 collided with the surrounding clouds. These collisions created the five brilliant clumps of light within the reflection nebula.

In this illustration showing NEO Surveyor, NASA's next-generation near-Earth object hunter, the spacecraft floats in an infrared starfield containing stars, star clusters, gas, and dust. More than 100 asteroids can be seen as red dots, with some of them visible in a track that shows how they were captured at different times as they marched across the sky. This starfield was observed by NASA's Wide-field Infrared Survey Explorer, or WISE, during its primary all-sky survey in March 2010 before it was put into hibernation a year later. In December 2013, the space telescope was reactivated to search for more asteroids as the NEOWISE mission. NASA's NEO Surveyor will build upon the successes of NEOWISE as the first space mission built specifically to find large numbers of hazardous asteroids and comets. The space telescope will launch to a region of gravitational stability between the Earth and the Sun called the L1 Lagrange point, where the spacecraft will orbit during its five-year primary mission. From this location, the space telescope will view the solar system in infrared wavelengths &ndash light that is invisible to the human eye. Because those wavelengths are mostly blocked by Earth's atmosphere, larger ground-based observatories may miss near-Earth objects that NEO Surveyor will be able to spot from space by using its modest light-collecting aperture of nearly 20 inches (50 centimeters). NEO Surveyor's cutting-edge detectors are designed to observe two heat-sensitive infrared bands that were chosen specifically so the spacecraft can track the most challenging-to-find near-Earth objects, such as dark asteroids and comets that don't reflect much visible light. In the infrared wavelengths to which NEO Surveyor is sensitive, these objects glow as they are heated by sunlight. In addition, NEO Surveyor will be able to find asteroids that approach Earth from the direction of the Sun, as well as those that lead and trail our planet's orbit, where they are typically obscured by the glare of sunlight – objects known as Earth Trojans. The mission is tasked by NASA's Planetary Science Division within the Science Mission Directorate; program oversight is provided by the PDCO, which was established in 2016 to manage the agency's ongoing efforts in planetary defense. NASA's Planetary Missions Program Office at Marshall Space Flight Center provides program management for NEO Surveyor. The project is being developed by JPL and is led by survey director Amy Mainzer at the University of Arizona. Established aerospace and engineering companies have been contracted to build the spacecraft and its instrumentation, including Ball Aerospace , Space Dynamics Laboratory, and Teledyne. The Laboratory for Atmospheric and Space Physics at the University of Colorado, Boulder will support operations, and IPAC-Caltech in Pasadena, California, is responsible for processing survey data and producing the mission's data products. Caltech manages JPL for NASA. https://photojournal.jpl.nasa.gov/catalog/PIA25253

CAPE CANAVERAL, Fla. – At NASA’s Kennedy Space Center in Florida, 40-foot-diameter dish antenna arrays are being constructed as part of the Antenna Test Bed Array for the Ka-Band Objects Observation and Monitoring, or Ka-BOOM system. The antennas will be part of the operations command center facility. The construction site is near the former Vertical Processing Facility, which has been demolished. The Ka-BOOM project is one of the final steps in developing the techniques to build a high power, high resolution radar system capable of becoming a Near Earth Object Early Warning System. While also capable of space communication and radio science experiments, developing radar applications is the primary focus of the arrays. Photo credit: NASA_Jim Grossmann

CAPE CANAVERAL, Fla. – At NASA’s Kennedy Space Center in Florida, 40-foot-diameter dish antenna arrays are being constructed as part of the Antenna Test Bed Array for the Ka-Band Objects Observation and Monitoring, or Ka-BOOM system. The antennas will be part of the operations command center facility. The construction site is near the former Vertical Processing Facility, which has been demolished. The Ka-BOOM project is one of the final steps in developing the techniques to build a high power, high resolution radar system capable of becoming a Near Earth Object Early Warning System. While also capable of space communication and radio science experiments, developing radar applications is the primary focus of the arrays. Photo credit: NASA/Jim Grossmann

CAPE CANAVERAL, Fla. – At NASA’s Kennedy Space Center in Florida, new towers are being constructed for the Antenna Test Bed Array for the Ka-Band Objects Observation and Monitoring, or Ka-BOOM system. The construction site is near the former Vertical Processing Facility, which has been demolished. Workers soon will begin construction on the 40-foot-diameter dish antenna arrays and their associated utilities, and prepare the site for the operations command center facility. The Ka-BOOM project is one of the final steps in developing the techniques to build a high power, high resolution radar system capable of becoming a Near Earth Object Early Warning System. While also capable of space communication and radio science experiments, developing radar applications is the primary focus of the arrays. Photo credit: NASA/ Ben Smegelsky

CAPE CANAVERAL, Fla. – At NASA’s Kennedy Space Center in Florida, 40-foot-diameter dish antenna arrays are being constructed as part of the Antenna Test Bed Array for the Ka-Band Objects Observation and Monitoring, or Ka-BOOM system. The antennas will be part of the operations command center facility. The construction site is near the former Vertical Processing Facility, which has been demolished. The Ka-BOOM project is one of the final steps in developing the techniques to build a high power, high resolution radar system capable of becoming a Near Earth Object Early Warning System. While also capable of space communication and radio science experiments, developing radar applications is the primary focus of the arrays. Photo credit: NASA/ Ben Smegelsky

CAPE CANAVERAL, Fla. – At NASA’s Kennedy Space Center in Florida, 40-foot-diameter dish antenna arrays are being constructed as part of the Antenna Test Bed Array for the Ka-Band Objects Observation and Monitoring, or Ka-BOOM system. The antennas will be part of the operations command center facility. The construction site is near the former Vertical Processing Facility, which has been demolished. The Ka-BOOM project is one of the final steps in developing the techniques to build a high power, high resolution radar system capable of becoming a Near Earth Object Early Warning System. While also capable of space communication and radio science experiments, developing radar applications is the primary focus of the arrays. Photo credit: NASA_Jim Grossmann

CAPE CANAVERAL, Fla. – At NASA’s Kennedy Space Center in Florida, new towers are being constructed for the Antenna Test Bed Array for the Ka-Band Objects Observation and Monitoring, or Ka-BOOM system. The construction site is near the former Vertical Processing Facility, which has been demolished. Workers soon will begin construction on the 40-foot-diameter dish antenna arrays and their associated utilities, and prepare the site for the operations command center facility. The Ka-BOOM project is one of the final steps in developing the techniques to build a high power, high resolution radar system capable of becoming a Near Earth Object Early Warning System. While also capable of space communication and radio science experiments, developing radar applications is the primary focus of the arrays. Photo credit: NASA/ Ben Smegelsky

CAPE CANAVERAL, Fla. – At NASA’s Kennedy Space Center in Florida, new towers are being constructed for the Antenna Test Bed Array for the Ka-Band Objects Observation and Monitoring, or Ka-BOOM system. The construction site is near the former Vertical Processing Facility, which has been demolished. Workers soon will begin construction on the 40-foot-diameter dish antenna arrays and their associated utilities, and prepare the site for the operations command center facility. The Ka-BOOM project is one of the final steps in developing the techniques to build a high power, high resolution radar system capable of becoming a Near Earth Object Early Warning System. While also capable of space communication and radio science experiments, developing radar applications is the primary focus of the arrays. Photo credit: NASA/ Ben Smegelsky

CAPE CANAVERAL, Fla. – At NASA’s Kennedy Space Center in Florida, 40-foot-diameter dish antenna arrays are being constructed as part of the Antenna Test Bed Array for the Ka-Band Objects Observation and Monitoring, or Ka-BOOM system. The antennas will be part of the operations command center facility. The construction site is near the former Vertical Processing Facility, which has been demolished. The Ka-BOOM project is one of the final steps in developing the techniques to build a high power, high resolution radar system capable of becoming a Near Earth Object Early Warning System. While also capable of space communication and radio science experiments, developing radar applications is the primary focus of the arrays. Photo credit: NASA_Jim Grossmann

CAPE CANAVERAL, Fla. – At NASA’s Kennedy Space Center in Florida, 40-foot-diameter dish antenna arrays are being constructed as part of the Antenna Test Bed Array for the Ka-Band Objects Observation and Monitoring, or Ka-BOOM system. The antennas will be part of the operations command center facility. The construction site is near the former Vertical Processing Facility, which has been demolished. The Ka-BOOM project is one of the final steps in developing the techniques to build a high power, high resolution radar system capable of becoming a Near Earth Object Early Warning System. While also capable of space communication and radio science experiments, developing radar applications is the primary focus of the arrays. Photo credit: NASA_Jim Grossmann

CAPE CANAVERAL, Fla. – At NASA’s Kennedy Space Center in Florida, 40-foot-diameter dish antenna arrays are being constructed as part of the Antenna Test Bed Array for the Ka-Band Objects Observation and Monitoring, or Ka-BOOM system. The antennas will be part of the operations command center facility. The construction site is near the former Vertical Processing Facility, which has been demolished. The Ka-BOOM project is one of the final steps in developing the techniques to build a high power, high resolution radar system capable of becoming a Near Earth Object Early Warning System. While also capable of space communication and radio science experiments, developing radar applications is the primary focus of the arrays. Photo credit: NASA_Jim Grossmann

CAPE CANAVERAL, Fla. – At NASA’s Kennedy Space Center in Florida, workers continue construction of the Antenna Test Bed Array for the Ka-Band Objects Observation and Monitoring, or Ka-BOOM, system. The construction site is near the former Vertical Processing Facility, which has been demolished. Workers soon will begin construction on the 40-foot-diameter dish antenna arrays and their associated utilities, and prepare the site for the operations command center facility. The Ka-BOOM project is one of the final steps in developing the techniques to build a high power, high resolution radar system capable of becoming a Near Earth Object Early Warning System. While also capable of space communication and radio science experiments, developing radar applications is the primary focus of the arrays. Photo credit: NASA/ Ben Smegelsky

CAPE CANAVERAL, Fla. – At NASA’s Kennedy Space Center in Florida, 40-foot-diameter dish antenna arrays are being constructed as part of the Antenna Test Bed Array for the Ka-Band Objects Observation and Monitoring, or Ka-BOOM system. The antennas will be part of the operations command center facility. The construction site is near the former Vertical Processing Facility, which has been demolished. The Ka-BOOM project is one of the final steps in developing the techniques to build a high power, high resolution radar system capable of becoming a Near Earth Object Early Warning System. While also capable of space communication and radio science experiments, developing radar applications is the primary focus of the arrays. Photo credit: NASA/ Ben Smegelsky

CAPE CANAVERAL, Fla. – At NASA’s Kennedy Space Center in Florida, 40-foot-diameter dish antenna arrays are being constructed as part of the Antenna Test Bed Array for the Ka-Band Objects Observation and Monitoring, or Ka-BOOM system. The antennas will be part of the operations command center facility. The construction site is near the former Vertical Processing Facility, which has been demolished. The Ka-BOOM project is one of the final steps in developing the techniques to build a high power, high resolution radar system capable of becoming a Near Earth Object Early Warning System. While also capable of space communication and radio science experiments, developing radar applications is the primary focus of the arrays. Photo credit: NASA_Jim Grossmann

CAPE CANAVERAL, Fla. – At NASA’s Kennedy Space Center in Florida, 40-foot-diameter dish antenna arrays are being constructed as part of the Antenna Test Bed Array for the Ka-Band Objects Observation and Monitoring, or Ka-BOOM system. The antennas will be part of the operations command center facility. The construction site is near the former Vertical Processing Facility, which has been demolished. The Ka-BOOM project is one of the final steps in developing the techniques to build a high power, high resolution radar system capable of becoming a Near Earth Object Early Warning System. While also capable of space communication and radio science experiments, developing radar applications is the primary focus of the arrays. Photo credit: NASA/ Ben Smegelsky

CAPE CANAVERAL, Fla. – At NASA’s Kennedy Space Center in Florida, new towers are being constructed for the Antenna Test Bed Array for the Ka-Band Objects Observation and Monitoring, or Ka-BOOM system. The construction site is near the former Vertical Processing Facility, which has been demolished. Workers soon will begin construction on the 40-foot-diameter dish antenna arrays and their associated utilities, and prepare the site for the operations command center facility. The Ka-BOOM project is one of the final steps in developing the techniques to build a high power, high resolution radar system capable of becoming a Near Earth Object Early Warning System. While also capable of space communication and radio science experiments, developing radar applications is the primary focus of the arrays. Photo credit: NASA/ Ben Smegelsky

CAPE CANAVERAL, Fla. – At NASA’s Kennedy Space Center in Florida, 40-foot-diameter dish antenna arrays are being constructed as part of the Antenna Test Bed Array for the Ka-Band Objects Observation and Monitoring, or Ka-BOOM system. The antennas will be part of the operations command center facility. The construction site is near the former Vertical Processing Facility, which has been demolished. The Ka-BOOM project is one of the final steps in developing the techniques to build a high power, high resolution radar system capable of becoming a Near Earth Object Early Warning System. While also capable of space communication and radio science experiments, developing radar applications is the primary focus of the arrays. Photo credit: NASA_Jim Grossmann

CAPE CANAVERAL, Fla. – At NASA’s Kennedy Space Center in Florida, new towers are being constructed for the Antenna Test Bed Array for the Ka-Band Objects Observation and Monitoring, or Ka-BOOM system. The construction site is near the former Vertical Processing Facility, which has been demolished. Workers soon will begin construction on the 40-foot-diameter dish antenna arrays and their associated utilities, and prepare the site for the operations command center facility. The Ka-BOOM project is one of the final steps in developing the techniques to build a high power, high resolution radar system capable of becoming a Near Earth Object Early Warning System. While also capable of space communication and radio science experiments, developing radar applications is the primary focus of the arrays. Photo credit: NASA/ Ben Smegelsky

CAPE CANAVERAL, Fla. – At NASA’s Kennedy Space Center in Florida, workers continue construction of the Antenna Test Bed Array for the Ka-Band Objects Observation and Monitoring, or Ka-BOOM, system. The construction site is near the former Vertical Processing Facility, which has been demolished. Workers soon will begin construction on the 40-foot-diameter dish antenna arrays and their associated utilities, and prepare the site for the operations command center facility. The Ka-BOOM project is one of the final steps in developing the techniques to build a high power, high resolution radar system capable of becoming a Near Earth Object Early Warning System. While also capable of space communication and radio science experiments, developing radar applications is the primary focus of the arrays. Photo credit: NASA/ Ben Smegelsky

CAPE CANAVERAL, Fla. – At NASA’s Kennedy Space Center in Florida, 40-foot-diameter dish antenna arrays are being constructed as part of the Antenna Test Bed Array for the Ka-Band Objects Observation and Monitoring, or Ka-BOOM system. The antennas will be part of the operations command center facility. The construction site is near the former Vertical Processing Facility, which has been demolished. The Ka-BOOM project is one of the final steps in developing the techniques to build a high power, high resolution radar system capable of becoming a Near Earth Object Early Warning System. While also capable of space communication and radio science experiments, developing radar applications is the primary focus of the arrays. Photo credit: NASA/ Ben Smegelsky

CAPE CANAVERAL, Fla. – At NASA’s Kennedy Space Center in Florida, a worker makes adjustments on a new tower being constructed for the Antenna Test Bed Array for the Ka-Band Objects Observation and Monitoring, or Ka-BOOM system. The antennas will be part of the operations command center facility. The construction site is near the former Vertical Processing Facility, which has been demolished. The Ka-BOOM project is one of the final steps in developing the techniques to build a high power, high resolution radar system capable of becoming a Near Earth Object Early Warning System. While also capable of space communication and radio science experiments, developing radar applications is the primary focus of the arrays. Photo credit: NASA/ Ben Smegelsky

CAPE CANAVERAL, Fla. – At NASA’s Kennedy Space Center in Florida, 40-foot-diameter dish antenna arrays are being constructed as part of the Antenna Test Bed Array for the Ka-Band Objects Observation and Monitoring, or Ka-BOOM system. The antennas will be part of the operations command center facility. The construction site is near the former Vertical Processing Facility, which has been demolished. The Ka-BOOM project is one of the final steps in developing the techniques to build a high power, high resolution radar system capable of becoming a Near Earth Object Early Warning System. While also capable of space communication and radio science experiments, developing radar applications is the primary focus of the arrays. Photo credit: NASA_Jim Grossmann

CAPE CANAVERAL, Fla. – At NASA’s Kennedy Space Center in Florida, 40-foot-diameter dish antenna arrays are being constructed as part of the Antenna Test Bed Array for the Ka-Band Objects Observation and Monitoring, or Ka-BOOM system. The antennas will be part of the operations command center facility. The construction site is near the former Vertical Processing Facility, which has been demolished. The Ka-BOOM project is one of the final steps in developing the techniques to build a high power, high resolution radar system capable of becoming a Near Earth Object Early Warning System. While also capable of space communication and radio science experiments, developing radar applications is the primary focus of the arrays. Photo credit: NASA/ Ben Smegelsky

CAPE CANAVERAL, Fla. – At NASA’s Kennedy Space Center in Florida, 40-foot-diameter dish antenna arrays are being constructed as part of the Antenna Test Bed Array for the Ka-Band Objects Observation and Monitoring, or Ka-BOOM system. The antennas will be part of the operations command center facility. The construction site is near the former Vertical Processing Facility, which has been demolished. The Ka-BOOM project is one of the final steps in developing the techniques to build a high power, high resolution radar system capable of becoming a Near Earth Object Early Warning System. While also capable of space communication and radio science experiments, developing radar applications is the primary focus of the arrays. Photo credit: NASA_Jim Grossmann

CAPE CANAVERAL, Fla. – At NASA’s Kennedy Space Center in Florida, 40-foot-diameter dish antenna arrays are being constructed as part of the Antenna Test Bed Array for the Ka-Band Objects Observation and Monitoring, or Ka-BOOM system. The antennas will be part of the operations command center facility. The construction site is near the former Vertical Processing Facility, which has been demolished. The Ka-BOOM project is one of the final steps in developing the techniques to build a high power, high resolution radar system capable of becoming a Near Earth Object Early Warning System. While also capable of space communication and radio science experiments, developing radar applications is the primary focus of the arrays. Photo credit: NASA/ Ben Smegelsky

CAPE CANAVERAL, Fla. -- At NASA’s Kennedy Space Center in Florida, the three Ka-Band Objects Observation and Monitoring, or Ka-BOOM, testbed antennas are used to track the pattern of the sun during initial testing of the new system. The goal of Ka-BOOM is to prove technologies that will allow future systems to characterize near-Earth objects in terms of size, shape, rotation_tumble rate and to determine the trajectory of those objects. Radar studies can determine the trajectory 100,000 times more precisely than can optical methods. While also capable of space communication and radio science experiments, developing radar applications is the primary focus of the arrays. The 40-foot-diameter dish antenna arrays are at the site of the former Vertical Processing Facility, which has been demolished. Photo credit: NASA_Jim Grossmann

CAPE CANAVERAL, Fla. – At NASA’s Kennedy Space Center in Florida, Robert Lightfoot, NASA associate director, talks to members of the media at the Ka Band Objects Observation and Monitoring, or KaBOOM, testbed antenna array site during a tour of Kennedy facilities. At right, in the foreground is Kennedy Director Bob Cabana. The goal of KaBOOM is to prove technologies that will allow future systems to characterize near-Earth objects in terms of size, shape, rotation_tumble rate and to determine the trajectory of those objects. Radar studies can determine the trajectory 100,000 times more precisely than can optical methods. While also capable of space communication and radio science experiments, developing radar applications is the primary focus of the arrays. The 40-foot-diameter dish antenna arrays are at the site of the former Vertical Processing Facility, which has been demolished. Photo credit: NASA_Jim Grossmann

CAPE CANAVERAL, Fla. -- At NASA’s Kennedy Space Center in Florida, one of the three Ka-Band Objects Observation and Monitoring, or Ka-BOOM, testbed antennas is used to track the sun during initial testing of the new system. The goal of Ka-BOOM is to prove technologies that will allow future systems to characterize near-Earth objects in terms of size, shape, rotation_tumble rate and to determine the trajectory of those objects. Radar studies can determine the trajectory 100,000 times more precisely than can optical methods. While also capable of space communication and radio science experiments, developing radar applications is the primary focus of the arrays. The 40-foot-diameter dish antenna arrays are at the site of the former Vertical Processing Facility, which has been demolished. Photo credit: NASA_Jim Grossmann

CAPE CANAVERAL, Fla. -- At NASA’s Kennedy Space Center in Florida, the three Ka-Band Objects Observation and Monitoring, or Ka-BOOM, testbed antennas are used to track the pattern of the sun during initial testing of the new system. The goal of Ka-BOOM is to prove technologies that will allow future systems to characterize near-Earth objects in terms of size, shape, rotation_tumble rate and to determine the trajectory of those objects. Radar studies can determine the trajectory 100,000 times more precisely than can optical methods. While also capable of space communication and radio science experiments, developing radar applications is the primary focus of the arrays. The 40-foot-diameter dish antenna arrays are at the site of the former Vertical Processing Facility, which has been demolished. Photo credit: NASA_Jim Grossmann

CAPE CANAVERAL, Fla. -- At NASA’s Kennedy Space Center in Florida, the three Ka-Band Objects Observation and Monitoring, or Ka-BOOM, testbed antennas are used to track the pattern of the sun during initial testing of the new system. The goal of Ka-BOOM is to prove technologies that will allow future systems to characterize near-Earth objects in terms of size, shape, rotation_tumble rate and to determine the trajectory of those objects. Radar studies can determine the trajectory 100,000 times more precisely than can optical methods. While also capable of space communication and radio science experiments, developing radar applications is the primary focus of the arrays. The 40-foot-diameter dish antenna arrays are at the site of the former Vertical Processing Facility, which has been demolished. Photo credit: NASA_Jim Grossmann

CAPE CANAVERAL, Fla. -- At NASA’s Kennedy Space Center in Florida, the three Ka-Band Objects Observation and Monitoring, or Ka-BOOM, testbed antennas are used to track the pattern of the sun during initial testing of the new system. The goal of Ka-BOOM is to prove technologies that will allow future systems to characterize near-Earth objects in terms of size, shape, rotation_tumble rate and to determine the trajectory of those objects. Radar studies can determine the trajectory 100,000 times more precisely than can optical methods. While also capable of space communication and radio science experiments, developing radar applications is the primary focus of the arrays. The 40-foot-diameter dish antenna arrays are at the site of the former Vertical Processing Facility, which has been demolished. Photo credit: NASA_Jim Grossmann

CAPE CANAVERAL, Fla. – At NASA’s Kennedy Space Center in Florida, Robert Lightfoot, NASA associate director, talks to members of the media at the Ka Band Objects Observation and Monitoring, or KaBOOM, testbed antenna array site during a tour of Kennedy facilities. At right is Kennedy Director Bob Cabana. The goal of KaBOOM is to prove technologies that will allow future systems to characterize near-Earth objects in terms of size, shape, rotation_tumble rate and to determine the trajectory of those objects. Radar studies can determine the trajectory 100,000 times more precisely than can optical methods. While also capable of space communication and radio science experiments, developing radar applications is the primary focus of the arrays. The 40-foot-diameter dish antenna arrays are at the site of the former Vertical Processing Facility, which has been demolished. Photo credit: NASA_Jim Grossmann

CAPE CANAVERAL, Fla. -- At NASA’s Kennedy Space Center in Florida, the three Ka-Band Objects Observation and Monitoring, or Ka-BOOM, testbed antennas are used to track the pattern of the sun during initial testing of the new system. The goal of Ka-BOOM is to prove technologies that will allow future systems to characterize near-Earth objects in terms of size, shape, rotation_tumble rate and to determine the trajectory of those objects. Radar studies can determine the trajectory 100,000 times more precisely than can optical methods. While also capable of space communication and radio science experiments, developing radar applications is the primary focus of the arrays. The 40-foot-diameter dish antenna arrays are at the site of the former Vertical Processing Facility, which has been demolished. Photo credit: NASA_Jim Grossmann

CAPE CANAVERAL, Fla. -- At NASA’s Kennedy Space Center in Florida, one of the three Ka-Band Objects Observation and Monitoring, or Ka-BOOM, testbed antennas is used to track the pattern of the sun during initial testing of the new system. The goal of Ka-BOOM is to prove technologies that will allow future systems to characterize near-Earth objects in terms of size, shape, rotation_tumble rate and to determine the trajectory of those objects. Radar studies can determine the trajectory 100,000 times more precisely than can optical methods. While also capable of space communication and radio science experiments, developing radar applications is the primary focus of the arrays. The 40-foot-diameter dish antenna arrays are at the site of the former Vertical Processing Facility, which has been demolished. Photo credit: NASA_Jim Grossmann

CAPE CANAVERAL, Fla. -- At NASA’s Kennedy Space Center in Florida, the three Ka-Band Objects Observation and Monitoring, or Ka-BOOM, testbed antennas are used to track the pattern of the sun during initial testing of the new system. The goal of Ka-BOOM is to prove technologies that will allow future systems to characterize near-Earth objects in terms of size, shape, rotation_tumble rate and to determine the trajectory of those objects. Radar studies can determine the trajectory 100,000 times more precisely than can optical methods. While also capable of space communication and radio science experiments, developing radar applications is the primary focus of the arrays. The 40-foot-diameter dish antenna arrays are at the site of the former Vertical Processing Facility, which has been demolished. Photo credit: NASA_Jim Grossmann

CAPE CANAVERAL, Fla. -- At NASA’s Kennedy Space Center in Florida, the three Ka-Band Objects Observation and Monitoring, or Ka-BOOM, testbed antennas are used to track the pattern of the sun during initial testing of the new system. The goal of Ka-BOOM is to prove technologies that will allow future systems to characterize near-Earth objects in terms of size, shape, rotation_tumble rate and to determine the trajectory of those objects. Radar studies can determine the trajectory 100,000 times more precisely than can optical methods. While also capable of space communication and radio science experiments, developing radar applications is the primary focus of the arrays. The 40-foot-diameter dish antenna arrays are at the site of the former Vertical Processing Facility, which has been demolished. Photo credit: NASA_Jim Grossmann

CAPE CANAVERAL, Fla. -- At NASA’s Kennedy Space Center in Florida, the three Ka-Band Objects Observation and Monitoring, or Ka-BOOM, testbed antennas are used to track the pattern of the sun during initial testing of the new system. The goal of Ka-BOOM is to prove technologies that will allow future systems to characterize near-Earth objects in terms of size, shape, rotation_tumble rate and to determine the trajectory of those objects. Radar studies can determine the trajectory 100,000 times more precisely than can optical methods. While also capable of space communication and radio science experiments, developing radar applications is the primary focus of the arrays. The 40-foot-diameter dish antenna arrays are at the site of the former Vertical Processing Facility, which has been demolished. Photo credit: NASA_Jim Grossmann

CAPE CANAVERAL, Fla. -- At NASA’s Kennedy Space Center in Florida, the three Ka-Band Objects Observation and Monitoring, or Ka-BOOM, testbed antennas are used to track the pattern of the sun during initial testing of the new system. The goal of Ka-BOOM is to prove technologies that will allow future systems to characterize near-Earth objects in terms of size, shape, rotation_tumble rate and to determine the trajectory of those objects. Radar studies can determine the trajectory 100,000 times more precisely than can optical methods. While also capable of space communication and radio science experiments, developing radar applications is the primary focus of the arrays. The 40-foot-diameter dish antenna arrays are at the site of the former Vertical Processing Facility, which has been demolished. Photo credit: NASA_Jim Grossmann

CAPE CANAVERAL, Fla. -- At NASA’s Kennedy Space Center in Florida, one of the three Ka-Band Objects Observation and Monitoring, or Ka-BOOM, testbed antennas is used to track the pattern of the sun during initial testing of the new system. The goal of Ka-BOOM is to prove technologies that will allow future systems to characterize near-Earth objects in terms of size, shape, rotation_tumble rate and to determine the trajectory of those objects. Radar studies can determine the trajectory 100,000 times more precisely than can optical methods. While also capable of space communication and radio science experiments, developing radar applications is the primary focus of the arrays. The 40-foot-diameter dish antenna arrays are at the site of the former Vertical Processing Facility, which has been demolished. Photo credit: NASA_Jim Grossmann

CAPE CANAVERAL, Fla. -- At NASA’s Kennedy Space Center in Florida, one of the three Ka-Band Objects Observation and Monitoring, or Ka-BOOM, testbed antennas is used to track the sun during initial testing of the new system. The goal of Ka-BOOM is to prove technologies that will allow future systems to characterize near-Earth objects in terms of size, shape, rotation_tumble rate and to determine the trajectory of those objects. Radar studies can determine the trajectory 100,000 times more precisely than can optical methods. While also capable of space communication and radio science experiments, developing radar applications is the primary focus of the arrays. The 40-foot-diameter dish antenna arrays are at the site of the former Vertical Processing Facility, which has been demolished. Photo credit: NASA_Jim Grossmann

CAPE CANAVERAL, Fla. – At NASA’s Kennedy Space Center in Florida, Robert Lightfoot, NASA associate director, talks to members of the media at the Ka Band Objects Observation and Monitoring, or KaBOOM, testbed antenna array site during a tour of Kennedy facilities. The goal of KaBOOM is to prove technologies that will allow future systems to characterize near-Earth objects in terms of size, shape, rotation_tumble rate and to determine the trajectory of those objects. Radar studies can determine the trajectory 100,000 times more precisely than can optical methods. While also capable of space communication and radio science experiments, developing radar applications is the primary focus of the arrays. The 40-foot-diameter dish antenna arrays are at the site of the former Vertical Processing Facility, which has been demolished. Photo credit: NASA_Jim Grossmann

CAPE CANAVERAL, Fla. – At NASA’s Kennedy Space Center in Florida, Robert Lightfoot, NASA associate director, talks to members of the media at the Ka Band Objects Observation and Monitoring, or KaBOOM, testbed antenna array site during a tour of Kennedy facilities. The goal of KaBOOM is to prove technologies that will allow future systems to characterize near-Earth objects in terms of size, shape, rotation_tumble rate and to determine the trajectory of those objects. Radar studies can determine the trajectory 100,000 times more precisely than can optical methods. While also capable of space communication and radio science experiments, developing radar applications is the primary focus of the arrays. The 40-foot-diameter dish antenna arrays are at the site of the former Vertical Processing Facility, which has been demolished. Photo credit: NASA_Jim Grossmann

CAPE CANAVERAL, Fla. -- At NASA’s Kennedy Space Center in Florida, the three Ka-Band Objects Observation and Monitoring, or Ka-BOOM, testbed antennas are used to track the pattern of the sun during initial testing of the new system. The goal of Ka-BOOM is to prove technologies that will allow future systems to characterize near-Earth objects in terms of size, shape, rotation_tumble rate and to determine the trajectory of those objects. Radar studies can determine the trajectory 100,000 times more precisely than can optical methods. While also capable of space communication and radio science experiments, developing radar applications is the primary focus of the arrays. The 40-foot-diameter dish antenna arrays are at the site of the former Vertical Processing Facility, which has been demolished. Photo credit: NASA_Jim Grossmann

CAPE CANAVERAL, Fla. -- At NASA’s Kennedy Space Center in Florida, the three Ka-Band Objects Observation and Monitoring, or Ka-BOOM, testbed antennas are used to track the pattern of the sun during initial testing of the new system. The goal of Ka-BOOM is to prove technologies that will allow future systems to characterize near-Earth objects in terms of size, shape, rotation_tumble rate and to determine the trajectory of those objects. Radar studies can determine the trajectory 100,000 times more precisely than can optical methods. While also capable of space communication and radio science experiments, developing radar applications is the primary focus of the arrays. The 40-foot-diameter dish antenna arrays are at the site of the former Vertical Processing Facility, which has been demolished. Photo credit: NASA_Jim Grossmann

CAPE CANAVERAL, Fla. -- At NASA’s Kennedy Space Center in Florida, the three Ka-Band Objects Observation and Monitoring, or Ka-BOOM, testbed antennas are used to track the pattern of the sun during initial testing of the new system. The goal of Ka-BOOM is to prove technologies that will allow future systems to characterize near-Earth objects in terms of size, shape, rotation_tumble rate and to determine the trajectory of those objects. Radar studies can determine the trajectory 100,000 times more precisely than can optical methods. While also capable of space communication and radio science experiments, developing radar applications is the primary focus of the arrays. The 40-foot-diameter dish antenna arrays are at the site of the former Vertical Processing Facility, which has been demolished. Photo credit: NASA_Jim Grossmann

These radar images of near-Earth asteroid 3200 Phaethon were generated by astronomers at the National Science Foundation's Arecibo Observatory on Dec. 17, 2017. Observations of Phaethon were conducted at Arecibo from Dec.15 through 19, 2017. At time of closest approach on Dec. 16 at 3 p.m. PST (6 p.m. EST, 11 p.m. UTC) the asteroid was about 6.4 million miles (10.3 million kilometers) away, or about 27 times the distance from Earth to the moon. The encounter is the closest the object will come to Earth until 2093. An animation is available at https://photojournal.jpl.nasa.gov/catalog/PIA22185

These images represent radar observations of asteroid 99942 Apophis on March 8, 9, and 10, 2021, as it made its last close approach before its 2029 Earth encounter that will see the object pass our planet by less than 20,000 miles (32,000 kilometers). The 70-meter radio antenna at the Deep Space Network's Goldstone Deep Space Communications Complex near Barstow, California, and the 100-meter Green Bank Telescope in West Virginia used radar to precisely track Apophis' motion. At the time of these observations, Apophis was about 10.6 million miles (17 million kilometers) from Earth, and each pixel has a resolution of 127 feet (38.75 meters). These observations helped scientists of the Center for Near Earth Object Studies (CNEOS), managed by NASA's Jet Propulsion Laboratory, precisely determine the 1,100-feet-wide (340-meter-wide) asteroid's orbit around the Sun, ruling out any Earth impact threat for the next hundred years or more. As a result of these observations, Apophis was removed from the Sentry Impact Risk Table. The radar team will continue to analyze these observations to determine more information about Apophis' size, shape, and rate of spin. Relying on optical telescopes and ground-based radar to help characterize every near-Earth object's orbit to improve long-term hazard assessments, CNEOS computes high-precision orbits in support of NASA's Planetary Defense Coordination Office. https://photojournal.jpl.nasa.gov/catalog/PIA24168

NASA Administrator Jim Bridenstine delivers a keynote speech at the sixth International Academy of Astronautics Planetary Defense Conference, Monday, April 29, 2019 at The Hotel at the University of Maryland in College Park Maryland. The conference brings together experts from around the world to present the latest research on Near-Earth Objects and will highlight the development of the first-ever mission to demonstrate an asteroid defection technique for planetary defense, NASA’s Double Asteroid Redirection Test (DART). Photo Credit: (NASA/Joel Kowsky)

ISS006-E-05070 (4 December 2002) --- The new crewmembers aboard the International Space Station (ISS) were able to document a rare occurrence early into their tour on the outpost. The dark area near Earth's horizon at center frame is actually a shadow cast by the Moon during the total solar eclipse of Dec. 4, 2002. The shadow obscures an area of cloud cover. The station, with three Expedition Six crewmembers aboard, was over the Indian Ocean at the time of the eclipse. The out-of-focus object in the foreground is part of the frame for the viewing port.

NASA Administrator Jim Bridenstine delivers a keynote speech at the sixth International Academy of Astronautics Planetary Defense Conference, Monday, April 29, 2019 at The Hotel at the University of Maryland in College Park Maryland. The conference brings together experts from around the world to present the latest research on Near-Earth Objects and will highlight the development of the first-ever mission to demonstrate an asteroid defection technique for planetary defense, NASA’s Double Asteroid Redirection Test (DART). Photo Credit: (NASA/Joel Kowsky)

ISS006-E-05064 (4 December 2002) --- The new crewmembers aboard the International Space Station (ISS) were able to document a rare occurrence early into their tour on the outpost. The dark area near Earth's horizon at center frame is actually a shadow cast by the Moon during the total solar eclipse of Dec. 4, 2002. The shadow obscures an area of cloud cover. The station, with three Expedition Six crewmembers aboard, was over the Indian Ocean at the time of the eclipse. The out-of-focus object in the foreground is part of the frame for the viewing port.

NASA Administrator Jim Bridenstine delivers a keynote speech at the sixth International Academy of Astronautics Planetary Defense Conference, Monday, April 29, 2019 at The Hotel at the University of Maryland in College Park Maryland. The conference brings together experts from around the world to present the latest research on Near-Earth Objects and will highlight the development of the first-ever mission to demonstrate an asteroid defection technique for planetary defense, NASA’s Double Asteroid Redirection Test (DART). Photo Credit: (NASA/Joel Kowsky)

NASA Administrator Jim Bridenstine delivers a keynote speech at the sixth International Academy of Astronautics Planetary Defense Conference, Monday, April 29, 2019 at The Hotel at the University of Maryland in College Park Maryland. The conference brings together experts from around the world to present the latest research on Near-Earth Objects and will highlight the development of the first-ever mission to demonstrate an asteroid defection technique for planetary defense, NASA’s Double Asteroid Redirection Test (DART). Photo Credit: (NASA/Joel Kowsky)

NASA Administrator Jim Bridenstine watches a short video as part of his keynote speech at the sixth International Academy of Astronautics Planetary Defense Conference, Monday, April 29, 2019 at The Hotel at the University of Maryland in College Park Maryland. The conference brings together experts from around the world to present the latest research on Near-Earth Objects and will highlight the development of the first-ever mission to demonstrate an asteroid defection technique for planetary defense, NASA’s Double Asteroid Redirection Test (DART). Photo Credit: (NASA/Joel Kowsky)

NASA Administrator Jim Bridenstine delivers a keynote speech at the sixth International Academy of Astronautics Planetary Defense Conference, Monday, April 29, 2019 at The Hotel at the University of Maryland in College Park Maryland. The conference brings together experts from around the world to present the latest research on Near-Earth Objects and will highlight the development of the first-ever mission to demonstrate an asteroid defection technique for planetary defense, NASA’s Double Asteroid Redirection Test (DART). Photo Credit: (NASA/Joel Kowsky)

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 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

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

This starfield was imaged by NASA's Near-Earth Object Wide-field Infrared Survey Explorer (NEOWISE) moments before the mission's science survey ended at midnight on July 31, 2024. The observation shows part of Fornax, a constellation that is visible in Southern Hemisphere skies. The spacecraft's final image, which was processed by IPAC at Caltech, takes in a view about three times the width of Earth's full Moon. This infrared exposure is the space telescope's 26,886,704th, a number that includes observations captured during its WISE (Wide-field Infrared Survey Explorer) mission. In addition to the stars and galaxies that appear as points of light, the spiral galaxy NGC 1339 can be seen as a fuzzy oval in the bottom right of the observation. NGC 1339 is about 64 million light-years from Earth. On Aug. 8, a week after the image was captured, project engineers commanded the spacecraft to turn its transmitter off for the last time. This concluded more than 10 years of the planetary defense mission's search for asteroids and comets, including those that could pose a threat to Earth. By repeatedly observing the sky from low Earth orbit, NEOWISE created all-sky maps featuring 1.45 million infrared measurements of more than 44,000 solar system objects. Of the 3,000-plus near-Earth objects it detected, 215 were first spotted by NEOWISE. The mission also discovered 25 new comets, including the famed comet C/2020 F3 NEOWISE. https://photojournal.jpl.nasa.gov/catalog/PIA26385

Astronomers using the Hubble Space Telescope (HST) have identified what may be the most luminous star known; a celestial mammoth that releases up to 10-million times the power of the Sun and is big enough to fill the diameter of Earth's orbit. The star unleashes as much energy in six seconds as our Sun does in one year. The image, taken by a UCLA-led team with the recently installed Near-Infrared Camera and Multi-Object Spectrometer (NICMOS) aboard the HST, also reveals a bright nebula, created by extremely massive stellar eruptions. The UCLA astronomers estimate that the star, called the Pistol Star, (for the pistol shaped nebula surrounding it), is approximately 25,000 light-years from Earth, near the center of our Milky Way galaxy. The Pistol Star is not visible to the eye, but is located in the direction of the constellation Sagittarius, hidden behind the great dust clouds along the Milky Way

These three radar images of near-Earth asteroid 2003 SD220 were obtained on Dec. 15-17, by coordinating observations with NASA's 230-foot (70-meter) antenna at the Goldstone Deep Space Communications Complex in California and the National Science Foundation's (NSF) 330-foot (100-meter) Green Bank Telescope in West Virginia. The radar image on the left was obtained on Dec. 15 when asteroid 2003 SD220 was 2.8 million miles (4.5 million kilometers) from Earth. The radar image in the middle was generated from data collected on Dec. 16 when the asteroid was 2.5 million miles (4.0 million kilometers) from Earth. The image on the right was obtained on Dec. 17 when 2003 SD220 was 2.2 million miles (3.6 million kilometers) from Earth. The spatial resolution on the images is as fine as 12 feet (3.7 meters) per pixel. The radar images reveal the asteroid is at least one mile (1.6 kilometers) long. Asteroid 2003 SD220 was discovered on Sept. 29, 2003, by astronomers at the Lowell Observatory Near-Earth-Object Search (LONEOS) in Flagstaff, Arizona -- an early Near-Earth Object (NEO) survey project supported by NASA that is no longer in operation. The asteroid will fly safely past Earth on Saturday, Dec. 22, 2018, at a distance of about 1.8 million miles (2.9 million kilometers). This will be the asteroid's closest approach in more than 400 years and the closest until 2070, when the asteroid will safely fly by slightly closer. https://photojournal.jpl.nasa.gov/catalog/PIA22970

A mirror set to be installed inside the telescope for NASA's Near-Earth Object Surveyor (NEO Surveyor) is seen during an inspection of the mirror's surface at NASA's Jet Propulsion Laboratory in Southern California on July 17, 2024. Being built in a JPL clean room, the infrared telescope is the spacecraft's only instrument and it will be used to seek out some of the hardest-to-find near-Earth objects that may pose a hazard to our planet. The reflection of principal optical engineer Brian Monacelli can be seen in the mirror. Known as a "three-mirror anastigmat telescope," the instrument will rely on a set of curved mirrors to focus light onto its infrared detectors in such a way that minimizes optical aberrations. Before being installed, the mirrors were examined for any debris or damage. Then, JPL's team of optomechanical technicians and engineers attached the mirrors to the telescope's "optical bench" in August. Next, they will measure the telescope's performance and align the telescope's mirrors. When complete, the telescope will be housed inside an instrument enclosure – being built at JPL in a different clean room – that is fabricated from dark composite material that allows heat to escape, helping to keep the telescope cool and prevent its own heat from obscuring observations. https://photojournal.jpl.nasa.gov/catalog/PIA26386

This image illustrates the Hubble Space Telescope's (HST's) Optical Telescope Assembly (OTA). One of the three major elements of the HST, the OTA consists of two mirrors (a primary mirror and a secondary mirror), support trusses, and the focal plane structure. The mirrors collect and focus light from selected celestial objects and are housed near the center of the telescope. The primary mirror captures light from objects in space and focuses it toward the secondary mirror. The secondary mirror redirects the light to a focal plane where the Scientific Instruments are located. The primary mirror is 94.5 inches (2.4 meters) in diameter and the secondary mirror is 12.2 inches (0.3 meters) in diameter. The purpose of the HST, the most complex and sensitive optical telescope ever made, is to study the cosmos from a low-Earth Orbit. By placing the telescope in space, astronomers are able to collect data that is free of the Earth's atmosphere. The HST detects objects 25 times fainter than the dimmest objects seen from the Earth and provides astronomers with an observable universe 250 times larger than visible from ground-based telescopes, perhaps as far away as 14 billion light-years. The HST views galaxies, stars, planets, comets, possibly other solar systems, and even unusual phenomena such as quasars, with 10 times the clarity of ground-based telescopes. The spacecraft is 42.5 feet (13 meters) long and weighs 25,000 pounds (11,600 kilograms). The HST was deployed from the Space Shuttle Discovery (STS-31 mission) into Earth orbit in April 1990. The Marshall Space Flight Center had responsibility for design, development, and construction of the HST. The Perkin-Elmer Corporation, in Danbury, Cornecticut, developed the optical system and guidance sensors. The Lockheed Missile and Space Company of Sunnyvale, California produced the protective outer shroud and spacecraft systems, and assembled and tested the finished telescope.

Comet NEOWISE is seen before sunrise over Washington, Sunday, July 12, 2020. The comet was discovered by NASA’s Near-Earth Object Wide-field Infrared Survey Explorer, or NEOWISE, on March 27. Since then, the comet — called comet C/2020 F3 NEOWISE and nicknamed comet NEOWISE — has been spotted by several NASA spacecraft, including Parker Solar Probe, NASA’s Solar and Terrestrial Relations Observatory, the ESA/NASA Solar and Heliospheric Observatory, and astronauts aboard the International Space Station. Photo Credit: (NASA/Bill Ingalls)

KENNEDY SPACE CENTER, FLA. -- Workers in the Payload Hazardous Servicing Facility prepare Deep Space 1 for launch aboard a Boeing Delta 7326 rocket in October. The first flight in NASA's New Millennium Program, Deep Space 1 is designed to validate 12 new technologies for scientific space missions of the next century. Onboard experiments include an ion propulsion engine and software that tracks celestial bodies so the spacecraft can make its own navigation decisions without the intervention of ground controllers. Most of its mission objectives will be completed within the first two months. A near-Earth asteroid, 1992 KD, has also been selected for a possible flyby

Comet NEOWISE is seen, upper left, before sunrise over Washington, Sunday, July 12, 2020. The comet was discovered by NASA’s Near-Earth Object Wide-field Infrared Survey Explorer, or NEOWISE, on March 27. Since then, the comet — called comet C/2020 F3 NEOWISE and nicknamed comet NEOWISE — has been spotted by several NASA spacecraft, including Parker Solar Probe, NASA’s Solar and Terrestrial Relations Observatory, the ESA/NASA Solar and Heliospheric Observatory, and astronauts aboard the International Space Station. Photo Credit: (NASA/Bill Ingalls)

A recent Hubble Space Telescope (HST) view reveals Uranus surrounded by its 4 major rings and 10 of its 17 known satellites. This false color image was generated by Erich Karoschka using data taken with Hubble's Near Infrared Camera and Multi-Object Spectrometer. The HST recently found about 20 clouds. The colors in the image indicate altitude. The green and blue regions show where the atmosphere is clear and can be penetrated by sunlight. In yellow and grey regions, the sunlight reflects from a higher haze or cloud layer. The orange and red colors indicate very high clouds, such as cirrus clouds on Earth.

KENNEDY SPACE CENTER, FLA. -- Workers in the Payload Hazardous Servicing Facility check equipment on Deep Space 1 to prepare it for launch aboard a Boeing Delta 7326 rocket in October. The first flight in NASA's New Millennium Program, Deep Space 1 is designed to validate 12 new technologies for scientific space missions of the next century. Onboard experiments include an ion propulsion engine and software that tracks celestial bodies so the spacecraft can make its own navigation decisions without the intervention of ground controllers. Most of its mission objectives will be completed within the first two months. A near-Earth asteroid, 1992 KD, has also been selected for a possible flyby