NASA Dawn asteroid lithograph of Eros and other asteroids. http://photojournal.jpl.nasa.gov/catalog/PIA19379

This animation shows the distance between the Apophis asteroid and Earth at the time of the asteroid's closest approach. The blue dots are the many man-made satellites that orbit our planet, and the pink represents the International Space Station. Movie available at https://photojournal.jpl.nasa.gov/catalog/PIA23195

This illustration shows asteroid 2020 QG's trajectory bending during its close approach to Earth. The asteroid is the closest known non-impacting asteroid ever detected. The asteroid passed by 1,830 miles (2,945 kilometers) above the southern Indian Ocean on Sunday, Aug. 16 at 12:08 a.m. EDT (Saturday, Aug. 15 at 9:08 p.m. PDT). Movie available at https://photojournal.jpl.nasa.gov/catalog/PIA24037

This diagram shows the orbit of binary asteroid Didymos around the Sun. Didymos consists of a large, nearly half-mile-wide (780-meter-wide) asteroid orbited by a smaller, 525-foot-wide (160-meter-wide) asteroid, or moonlet. Didymos' orbital path around the Sun is shown as the thin white ellipse and Earth's orbit is the thick white line. In the background are the orbits for 2,200 other known potentially hazardous asteroids. A potentially hazardous asteroid is classified as an asteroid wider than about 460 feet (140 meters) with an orbit that brings it within 5 million miles (8 million kilometers) of Earth's orbit. Didymos' smaller asteroid is the target of NASA's Double Asteroid Redirect Test (DART) mission. The DART spacecraft is a kinetic impactor designed to collide with the moonlet to see how its orbit around the larger asteroid will be changed by the impact. The outcome of this mission will help NASA determine whether the method could be used to modify the trajectory of an asteroid should one threaten Earth in the future. Didymos is not a danger to our planet. This orbital diagram was produced by the Center for Near Earth Object Studies (CNEOS), which is managed by NASA's Jet Propulsion Laboratory in Southern California. CNEOS characterizes every known near-Earth asteroid (NEA) orbit to improve long-term impact hazard assessments in support of NASA's Planetary Defense Coordination Office (PDCO). https://photojournal.jpl.nasa.gov/catalog/PIA24565

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

Artist graphic of the asteroid belt, part of Dawn Mission Art series. http://photojournal.jpl.nasa.gov/catalog/PIA19380

These two radar images of near-Earth asteroid 2003 SD220 were obtained on Dec. 18 and 19 by coordinating observations with the Arecibo Observatory's 1,000-foot (305-meter) antenna in Puerto Rico and the National Science Foundation's (NSF) 330-foot (100-meter) Green Bank Telescope in West Virginia. The radar images reveal the asteroid is at least one mile (1.6 kilometers) long. https://photojournal.jpl.nasa.gov/catalog/PIA22969

The streak circled in the center of this image is asteroid 2020 QG, which came closer to Earth than any other nonimpacting asteroid on record. It was detected by the Zwicky Transient Facility on Sunday, Aug. 16 at 12:08 a.m. EDT (Saturday, Aug. 15 at 9:08 p.m. PDT). The wide-field camera image of the Zwicky Transient Facility, a sky-scanning survey telescope funded by the National Science Foundation and NASA, and based at Caltech's Palomar Observatory in Southern California. The image was taken six hours after the close approach, as the asteroid was heading away from Earth. https://photojournal.jpl.nasa.gov/catalog/PIA24038

This illustration, created in March 2021, depicts the 140-mile-wide (226-kilometer-wide) asteroid Psyche, which lies in the main asteroid belt between Mars and Jupiter. Psyche is the focal point of NASA's mission of the same name. The Psyche spacecraft is set to launch in August 2022 and arrive at the asteroid in 2026, where it will orbit for 21 months and investigate its composition. Based on data obtained from Earth, scientists believe Psyche is a mixture of metal and rock. The rock and metal may be in large provinces, or areas, on the asteroid — as illustrated in this rendering. Another possibility is that rock and metal may be intimately mixed on a scale too small to detect from orbit — as depicted in an illustration here: PIA24472. Observing and measuring how the metal and rock are mixed will help scientists determine how Psyche formed. Exploring the asteroid could also give valuable insight into how our own planet and others formed. The Psyche team will use a magnetometer to measure the asteroid's magnetic field. A multispectral imager will capture images of the surface, as well as data about the Psyche's composition and topography. Spectrometers will analyze the neutrons and gamma rays coming from the surface to reveal the elements that make up the asteroid itself. The image was created by Peter Rubin. https://photojournal.jpl.nasa.gov/catalog/PIA24471

This illustration, created in March 2021, depicts the 140-mile-wide (226-kilometer-wide) asteroid Psyche, which lies in the main asteroid belt between Mars and Jupiter. Psyche is the focal point of NASA's mission of the same name. The Psyche spacecraft is set to launch in August 2022 and arrive at the asteroid in 2026, where it will orbit for 21 months and investigate its composition. Based on data obtained from Earth, scientists believe Psyche is a mixture of metal and rock. The rock and metal may be in large provinces, or areas, on the asteroid — as depicted in an illustration here: PIA24471. Another possibility is that rock and metal may be intimately mixed on a scale too small to detect from orbit — as depicted in the illustration above. Observing and measuring how the metal and rock are mixed will help scientists determine how Psyche formed. Exploring the asteroid could also give valuable insight into how our own planet and others formed. The Psyche team will use a magnetometer to measure the asteroid's magnetic field. A multispectral imager will capture images of the surface, as well as data about the Psyche's composition and topography. Spectrometers will analyze the neutrons and gamma rays coming from the surface to reveal the elements that make up the asteroid itself. The image was created by Peter Rubin. https://photojournal.jpl.nasa.gov/catalog/PIA24472

This illustration shows how NASA's Psyche spacecraft will explore the asteroid Psyche, beginning with Orbit A when it arrives at the asteroid in early 2026. The initial orbit is designed to be at a high altitude – about 435 miles (700 kilometers) above the asteroid's surface. Over the following 20 months, the spacecraft will use its electric propulsion system to dip into lower and lower orbits as it conducts its science investigation. Eventually, the spacecraft will establish a final orbit (Orbit D) about 53 miles (85 kilometers) above the surface. Set to launch in August 2022, Psyche will investigate a metal-rich asteroid of the same name, which lies in the main asteroid belt between Mars and Jupiter. Scientists believe the asteroid could be part or all of the iron-rich interior of an early planetary building block that was stripped of its outer rocky shell as it repeatedly collided with other large bodies during the early formation of the solar system. https://photojournal.jpl.nasa.gov/catalog/PIA24896

Artist's illustration of the trajectory of asteroid 2017 YE5 through the solar system. At its closest approach to Earth, the asteroid came to within 16 times the distance between Earth and the moon. A movie is available at https://photojournal.jpl.nasa.gov/catalog/PIA22560

Artists concept of NASA Asteroid Redirect Robotic ARM Mission capturing an asteroid boulder before redirecting it to a astronaut-accessible orbit around Earth moon. http://photojournal.jpl.nasa.gov/catalog/PIA19349

The asteroid Euphrosyne glides across a field of background stars in this time-lapse view from NASA's WISE spacecraft. WISE obtained the images used to create this view over a period of about a day around May 17, 2010, during which it observed the asteroid four times. Because WISE (renamed NEOWISE in 2013) is an infrared telescope, it senses heat from asteroids. Euphrosyne is quite dark in visible light, but glows brightly at infrared wavelengths. This view is a composite of images taken at four different infrared wavelengths: 3.4 microns (color-coded blue), 4.6 microns (cyan), 12 microns (green) and 22 microns (red). The moving asteroid appears as a string of red dots because it is much cooler than the distant background stars. Stars have temperatures in the thousands of degrees, but the asteroid is cooler than room temperature. Thus the stars are represented by shorter wavelength (hotter) blue colors in this view, while the asteroid is shown in longer wavelength (cooler) reddish colors. The WISE spacecraft was put into hibernation in 2011 upon completing its goal of surveying the entire sky in infrared light. WISE cataloged three quarters of a billion objects, including asteroids, stars and galaxies. In August 2013, NASA decided to reinstate the spacecraft on a mission to find and characterize more asteroids. http://photojournal.jpl.nasa.gov/catalog/PIA19645

This animation depicts the motion of small near-Earth asteroid 2024 PT5 as it orbits the Sun. Because it has a similar orbit as our planet, the asteroid will linger as a distant companion for a few months, but it will not be captured by Earth's gravity. Asteroid 2024 PT5 was first observed on Aug. 7, 2024, by the Sutherland, South Africa, telescope of the University of Hawaii's Asteroid Terrestrial-impact Last Alert System (ATLAS), which is funded by NASA. Estimated to be about 33 feet (10 meters) wide, the asteroid does not pose a hazard to Earth. The 53-second animation depicts the orbits of Earth and 2024 PT5 from Dec. 31, 2023, to Sept. 9, 2025, speeded up by about 1 million times. For more information about 2024 PT5 can be found at: https://blogs.nasa.gov/planetarydefense/2024/10/02/nasa-to-track-asteroid-2024-pt5-on-next-close-pass-january-2025/ Animation available at https://photojournal.jpl.nasa.gov/catalog/PIA26452

Illustrated in this artist concept are two possible structures for asteroid 2011 MD. NASA Spitzer infrared camera helped reveal that this asteroid consists of about two-thirds empty space.

This collage of radar images of near-Earth asteroid 1999 JD6 was collected by NASA scientists on July 25, 2015. The images show the rotation of the asteroid, which made its closest approach on July 24 at 9:55 p.m. PDT (12:55 a.m. EDT on July 25) at a distance of about 4.5 million miles (7.2 million kilometers, or about 19 times the distance from Earth to the moon). The asteroid appears to be a contact binary -- an asteroid with two lobes that are stuck together. These views, which are radar echoes, were obtained by pairing NASA's 230-foot-wide (70-meter) Deep Space Network antenna at Goldstone, California, with the 330-foot (100-meter) National Science Foundation Green Bank Telescope in West Virginia. Using this approach, the Goldstone antenna beams a radar signal at an asteroid and Green Bank receives the reflections. The technique, referred to as a bistatic observation, dramatically improves the amount of detail that can be seen in radar images. The new views obtained with the technique show features as small as about 25 feet (7.5 meters) wide. The images show the asteroid is highly elongated, with a length of approximately 1.2 miles (2 kilometers) on its long axis. http://photojournal.jpl.nasa.gov/catalog/PIA19647

The six red dots in this composite picture indicate the location of the first new near-Earth asteroid, called 2013 YP139, as seen by NASA NEOWISE.

Observations of infrared light from NASA Spitzer Space Telescope coming from asteroids provide a better estimate of their true sizes than visible-light measurements.

On March 21, 2021, the large asteroid 2001 FO32 made a close approach with our planet, passing at a distance of about 1.25 million miles (2 million kilometers) — or 5 1/4 times the distance from Earth to the Moon. While there was no risk of the near-Earth asteroid colliding with Earth as its orbit is very well known, scientists at NASA's Jet Propulsion Laboratory in Southern California took the opportunity to capture these radar images of the asteroid as it tumbled past. Using NASA's 34-meter (111.5-feet) Deep Space Station 13 (DSS-13) radio antenna at the Deep Space Network's Goldstone Deep Space Communication Complex near Barstow, California, radio signals were transmitted to 2001 FO32. The signals then bounced off the surface of the asteroid and were received by the 100-meter (328-feet) Green Bank Telescope in West Virginia. Such radar observations can offer additional insight into the asteroid's orbit, provide a better estimate of its dimensions and rotation rate, and help glimpse surface features (like large boulders or craters). Other radar observations were carried out by scientists using the 34-meter DSS-43 antenna at the Deep Space Network's Canberra Deep Space Communication Complex in Australia. Along with the Commonwealth Scientific and Industrial Research Organisation's Australia Telescope Compact Array near Narrabri in New South Wales, both antennas worked together to track 2001 FO32. Asteroid 2001 FO32 was discovered in March 2001 by the Lincoln Near-Earth Asteroid Research (LINEAR) program in Socorro, New Mexico, and had been estimated, based on optical measurements, to be roughly 3,000 feet (1 kilometer) wide. In more recent follow-up observations by NEOWISE, 2001 FO32 appears to be faint when observed in infrared wavelengths, which suggests the object is likely less than 1 kilometer in diameter. Analysis by the NEOWISE team shows that it is between 1,300 to 2,230 feet (440 to 680 meters) wide. Further analysis of data from the radar campaign will better refine the size of the asteroid and increase the precision of its orbital calculations. For more information about 2001 FO32 and observing campaign, read: https://www.jpl.nasa.gov/news/asteroid-2001-fo32-will-safely-pass-by-earth-march-21 https://photojournal.jpl.nasa.gov/catalog/PIA24561

This radar image of asteroid 1999 RQ36 was obtained NASA Deep Space Network antenna in Goldstone, Calif. on Sept 23, 1999. NASA detects, tracks and characterizes asteroids and comets passing close to Earth using both ground- and space-based telescopes.

This image shows asteroids observed so far by NASA Wide-field Infrared Survey Explorer. An animation is available at the Photojournal.

These images and animation represent NASA radar observations of 4660 Nereus on Dec. 10, 2021, before the asteroid's close approach on Dec. 11, when it came within 2.5 million miles (4 million kilometers) of Earth. Using the 70-meter radio antenna at the Deep Space Network's Goldstone Deep Space Communications Complex near Barstow, California, scientists from NASA's Jet Propulsion Laboratory acquired the most detailed radar images of the nearly 1,100-foot-wide (330-meter-wide) near-Earth asteroid since its discovery almost four decades earlier. Nereus' orbit is very well known and the asteroid does not pose a threat to Earth. During the asteroid's close approach, an image resolution of about 12.3 feet (3.75 meters) per pixel was possible, revealing surface features such as potential boulders and craters, plus ridges and other topography. Asteroid Nereus' previous approach in 2002 was near enough to Earth to reveal the asteroid's size and overall shape, but too distant to show surface features. The new observations will also help scientists better understand the asteroid's shape and rotation while providing them new data to further refine its orbital path around the Sun. Nereus belongs to the relatively rare E-type asteroid family that exhibits very unusual radar scattering properties. It's thought that this may be caused by asteroids of this type having particularly rough terrain. Also, E-type asteroids are optically bright, sometimes reflecting as much as 50% of the sunlight that hits their surface. Typical S-type asteroids reflect about 15%, whereas dark C-type asteroids reflect only a few percent. It's thought that E-class asteroids may be the source of very rare Aubrite meteorites and are composed of comparatively bright material. The 2021 close approach was the best opportunity for radar imaging of Nereus until 2060, when the asteroid will approach within 750,000 miles (1.2 million kilometers) of Earth, only three times the Earth-Moon distance. At that time, Nereus will be an easy target for small telescopes and possibly even powerful binoculars. Nereus – named after a sea god from Greek mythology – was discovered in 1982 by Eleanor "Glo" Helin as part of the JPL Palomar Planet-Crossing Asteroid Survey. Movie available at https://photojournal.jpl.nasa.gov/catalog/PIA24566

The 230-foot 70-meter DSS-14 antenna at Goldstone, Ca. obtained these radar images of asteroid 2015 TB145 on Oct. 31, 2015. Asteroid 2015 TB145 is depicted in eight individual radar images collected on Oct. 31, 2015 between 5:55 a.m. PDT (8:55 a.m. EDT) and 6:08 a.m. PDT (9:08 a.m. EDT). At the time the radar images were taken, the asteroid was between 440,000 miles (710,000 kilometers) and about 430,000 miles (690,000 kilometers) distant. Asteroid 2015 TB145 safely flew past Earth on Oct. 31, at 10:00 a.m. PDT (1 p.m. EDT) at about 1.3 lunar distances (300,000 miles, 480,000 kilometers). To obtain the radar images, the scientists used the 230-foot (70-meter) DSS-14 antenna at Goldstone, California, to transmit high power microwaves toward the asteroid. The signal bounced of the asteroid, and their radar echoes were received by the National Radio Astronomy Observatory's 100-meter (330-foot) Green Bank Telescope in West Virginia. The images achieve a spatial resolution of about 13 feet (4 meters) per pixel. http://photojournal.jpl.nasa.gov/catalog/PIA20043

This frame from a movie made from radar images of asteroid 1999 JD6 was collected by NASA scientists on July 25, 2015. The images show the rotation of the asteroid, which made its closest approach on July 24 at 9:55 p.m. PDT (12:55 a.m. EDT on July 25) at a distance of about 4.5 million miles (7.2 million kilometers, or about 19 times the distance from Earth to the moon). The asteroid appears to be a contact binary -- an asteroid with two lobes that are stuck together. The radar images show the asteroid is highly elongated, with a length of approximately 1.2 miles (2 kilometers) on its long axis. These images are radar echoes, which are more like a sonogram than a photograph. The views were obtained by pairing NASA's 230-foot-wide (70-meter) Deep Space Network antenna at Goldstone, California, with the 330-foot (100-meter) National Science Foundation Green Bank Telescope in West Virginia. Using this approach, the Goldstone antenna beams a radar signal at an asteroid and Green Bank receives the reflections. The technique, referred to as a bistatic observation, dramatically improves the amount of detail that can be seen in radar images. The new views obtained with the technique show features as small as about 25 feet (7.5 meters) wide. http://photojournal.jpl.nasa.gov/catalog/PIA19646

This frame from a sequence of four images taken during one night of observation by NASA's Catalina Sky Survey near Tucson, Arizona, shows the speck of light that moves relative to the background stars is a small asteroid that was, at the time, about as far away as the moon. This asteroid, named 2014 AA, was the second one ever detected on course to impact Earth. It was estimated to be about 6 to 10 feet (2 to 3 meters) in diameter, and it harmlessly hit Earth's atmosphere over the Atlantic Ocean about 20 hours after its discovery in these images. The images were taken Jan. 1, 2014. They provide an example of how asteroids are typically discovered by detection of their motion relative to background stars. An animation is available at https://photojournal.jpl.nasa.gov/catalog/PIA21712

Observations from NASA Spitzer Space Telescope, taken in infrared light, have helped to reveal that a small asteroid called 2011 MD is made-up of two-thirds empty space.

This image of asteroid 2011 MD was taken by NASA Spitzer Space Telescope in Feb. 2014, over a period of 20 hours.

Artist's concept of what binary asteroid 2017 YE5 might look like. The two objects showed striking differences in radar reflectivity, which could indicate that they have different surface properties. A movie is available at https://photojournal.jpl.nasa.gov/catalog/PIA22556

Scientists using two giant, Earth-based radio telescopes bounced radar signals off passing asteroid 2011 UW158 to create images for this animation showing the rocky body's fast rotation. The passing asteroid made its closest approach to Earth on July 19, 2015 at 7:37 a.m. PST (4:37 a.m. EST) at a distance of about 1.5 million miles (2.4 million kilometers, or 6 times the distance from Earth to the moon). The close proximity during the pass made 2011 UW158 one of the best asteroid flybys of 2015 for imaging from Earth using radar. The radar images reveal that the shape of the asteroid is extremely irregular and quite elongated. Prominent parallel, linear features run along the length of the object that cause a large increase in brightness of the radar images as they rotate into view. Scientists note that the asteroid appears to be fairly unusual. Its fast rotation suggests the object has greater mechanical strength than other asteroids its size. A fast-rotating asteroid with lower mechanical strength would tend to split apart. To obtain the views, researchers paired the 230-foot- (70-meter-) wide Deep Space Network antenna at Goldstone, California, in concert with the National Radio Astronomy Observatory's 330-foot (100-meter) Green Bank Telescope. Using this technique, the Goldstone antenna beams a radar signal at an asteroid and Green Bank receives the reflections. The technique, referred to as a bi-static observation, dramatically improves the amount of detail that can be seen in radar images. The new views obtained with the technique show features as small as about 24 feet (7.5 meters) wide. The 171 individual images used in the movie were generated from data collected on July 18. They show the asteroid is approximately 2000 by 1000 feet (600 by 300 meters) across. The observations also confirm earlier estimates by astronomers that the asteroid rotates quickly, completing one spin in just over half an hour. The movie spans a period of about an hour and 45 minutes. The trajectory of asteroid 2011 UW158 is well understood. This flyby was the closest approach the asteroid will make to Earth for at least the next 93 years. Asteroid 2011 UW158 was discovered on October 25, 2011, by the PanSTARRS 1 telescope, located on the summit of Haleakala on Maui, Hawaii. Managed by the University of Hawaii, the PanSTARRS survey receives NASA funding. Radar is a powerful technique for studying an asteroid's size, shape, rotation state, surface features and surface roughness, and for improving the calculation of asteroid orbits. Radar measurements of asteroid distances and velocities often enable computation of asteroid orbits much further into the future than if radar observations weren't available. http://photojournal.jpl.nasa.gov/catalog/PIA19644

This animation shows asteroid 2022 EB5's predicted orbit around the Sun before impacting into the Earth's atmosphere on March 11, 2022. The asteroid – estimated to be about 6 ½ feet (2 meters) wide – was discovered two hours before impact. Using NASA's Scout impact hazard assessment system, members of the Center for Near Earth Object Studies (CNEOS) – which is managed by NASA's Jet Propulsion Laboratory in Southern California – accurately predicted where and when the asteroid would harmlessly break up in Earth's atmosphere. Infrasound sensors, which can detect low frequency sound waves as they travel through the atmosphere, confirmed the impact occurred over the Norwegian Sea, southwest of Norway's Jan Mayen island. Animation available at https://photojournal.jpl.nasa.gov/catalog/PIA24568

These are the discovery observations of asteroid 2018 LA from the Catalina Sky Survey, taken June 2, 2018. About eight hours after these images were taken, the asteroid entered Earth's atmosphere (about 9:44 a.m. PDT, 12:44 p.m. EDT, 16:44 UTC, 6:44 p.m. local Botswana time), and disintegrated in the upper atmosphere near Botswana, Africa. https://photojournal.jpl.nasa.gov/catalog/PIA22468

Bi-static radar images of the binary asteroid 2017 YE5 from the Arecibo Observatory and the Green Bank Observatory on June 25. The observations show that the asteroid consists of two separate objects in orbit around each other. A movie is available at https://photojournal.jpl.nasa.gov/catalog/PIA22559

SCI2017_0004: Artist's illustration of the Epsilon Eridani system showing Epsilon Eridani b, right foreground, a Jupiter-mass planet orbiting its parent star at the outside edge of an asteroid belt. In the background can be seen another narrow asteroid or comet belt plus an outermost belt similar in size to our solar system's Kuiper Belt. The similarity of the structure of the Epsilon Eridani system to our solar system is remarkable, although Epsilon Eridani is much younger than our sun. SOFIA observations confirmed the existence of the asteroid belt adjacent to the orbit of the Jovian planet. Credit: NASA/SOFIA/Lynette Cook

Using data collected by NASA's OSIRIS-REx mission, this animation shows the trajectories of rocky particles after being ejected from asteroid (101955) Bennu's surface. The animation emphasizes the four largest particle-ejection events detected at Bennu between December 2018 and September 2019. Additional particles not related to the ejections are also visible. Most of these pebble-size pieces of rock, typically measuring around a quarter inch (7 millimeters), were pulled back to Bennu under the asteroid's weak gravity after a short hop, sometimes even ricocheting back into space after colliding with the surface. Others remained in orbit for a few days and up to 16 revolutions. And some were ejected with enough force to completely escape from the Bennu environs. OSIRIS-REx — which stands for Origins, Spectral Interpretation, Resource Identification, and Security-Regolith Explorer — arrived at Bennu in December 2018. On Oct. 20, 2020, the mission will attempt to briefly touch down on the asteroid to scoop up material likely to include particles that were ejected before dropping back to the surface. If all goes as planned, the spacecraft will return to Earth in September 2023 with a cache of Bennu's particles for further study, including of which may even hold the physical clues as to what ejection mechanisms are at play. Movie available at https://photojournal.jpl.nasa.gov/catalog/PIA24101

An asteroid discovered by NASA NEOWISE spacecraft has been given the formal designation 316201 Malala, in honor of Malala Yousafzai of Pakistan, who received the Nobel Peace Prize in 2014. The asteroid previous appellation was 2010 ML48. The International Astronomical Union (IAU) renamed the asteroid as the request of Amy Mainzer of NASA's Jet Propulsion Laboratory, Pasadena, California. Mainzer is the principal investigator of NASA's NEOWISE space telescope. The IAU is the sole worldwide organization recognized by astronomers everywhere to designate names for astronomical bodies. So far, Mainzer and the NEOWISE team have focused on pioneers in civil rights, science and the arts for the astronomical honor. Among the strong women of history who have already had NEOWISE-discovered asteroids named for them are civil rights activist Rosa Parks, conservationist Wangari Maathai, abolitionists Sojourner Truth and Harriet Tubman, and singer Aretha Franklin. Asteroid Malala is in the main belt between Mars and Jupiter and orbits the sun every five-and-a-half years. It is about two-and-a-half miles (four kilometers) in diameter, and its surface is very dark, the color of printer toner. http://photojournal.jpl.nasa.gov/catalog/PIA19362

This series of radar images obtained by the Goldstone Solar System Radar near Barstow, California, on Aug. 18, 2024, shows the asteroid 2024 JV33 shortly before its close approach with Earth. The images were captured when the asteroid was at a distance of 2.8 million miles (4.6 million kilometers), about 12 times the distance between the Moon and Earth. Discovered by the NASA-funded Catalina Sky Survey in Tucson, Arizona, on May 4, the near-Earth asteroid's shape resembles that of a peanut – with two rounded lobes, one lobe larger than the other. Scientists used the radar images to determine that it is about 980 feet (300 meters) long and that its length is about double its width. Asteroid 2024 JV33 rotates once every seven hours. Radar is the principal technique for discovering such asteroids, which are called contact binaries. Dozens of them have been imaged by Goldstone, which is part of NASA's Deep Space Network. At least 14% of near-Earth asteroids larger than about 660 feet (200 meters) have a contact binary shape. Asteroid 2024 JV33 has an elongated orbit similar to that of many comets that are strongly influenced by the gravity of Jupiter. While no comet-like activity has been observed, the possibility remains that the asteroid may be an inactive cometary nucleus. 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. https://photojournal.jpl.nasa.gov/catalog/PIA26389

Between Aug. 20 and 24, near-Earth asteroid (NEA) 2016 AJ193 drifted past Earth at a distance of 2.1 million miles (about 3.4 million kilometers), creating an opportunity for planetary radar to image its surface for the first time since its discovery in 2016. Using the 70-meter (230-foot) Deep Space Station 14 antenna at the Deep Space Network's Goldstone Deep Space Complex near Barstow, California, considerable detail in the asteroid's surface was revealed, including ridges, small hills, flat areas, concavities, and possible boulders. In addition, the radar observations of 2016 AJ193 confirmed that it is about three-quarters-of-a-mile (1.3-kilometers) wide. This series of images show the asteroid rotate (with a period of 3.5 hours) as each radar observation was made. 2016 AJ193 is the 1,001st asteroid to be observed by planetary radar, making its close approach with Earth only seven days after the 1,000th NEA to be observed by radar – asteroid 2021 PJ1, which measures between 65 and 100 feet (20 and 30 meters) wide – approached Earth at a distance of 1 million miles (about 1.7 million kilometers). https://photojournal.jpl.nasa.gov/catalog/PIA24564

NASA Deep Space Network, Goldstone radar images show triple asteroid 1994 CC, which consists of a central object approximately 700 meters 2,300 feet in diameter and two smaller moons that orbit the central body. Animation available at the Photojournal

NASA scientists used Earth-based radar to produce these sharp views -- an image montage and a movie sequence -- of the asteroid designated 2014 HQ124 on June 8, 2014.

This image of asteroid Toutatis was generated with data collected using NASA Deep Space Network antenna at Goldstone, Calif., on Dec. 12 and 13, 2012 and indicates that it is an elongated, irregularly shaped object with ridges and perhaps craters.

Asteroid 1998 WT24 left in December 2001, right on December 11, 2015 taken by NASA the 230-foot 70-meter DSS-14 antenna at Goldstone, California.

This collage of radar images of near-Earth asteroid 2005 WK4 was collected by NASA scientists using the 230-foot 70-meter Deep Space Network antenna at Goldstone, Calif., on Aug. 8, 2013.

Dr. Holdren (left), Administrator Bolden (center) and Dr. Michele Gates (right) discuss the ARM mission during a live NASA TV briefing. Behind them is a mockup of robotic capture module for the Asteroid Redirect Mission. More info: Asteroid Redirect Mission Update – On Sept. 14, 2016, NASA provided an update on the Asteroid Redirect Mission (ARM) and how it contributes to the agency’s journey to Mars and protection of Earth. The presentation took place in the Robotic Operations Center at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. Assistant to the President for Science and Technology Dr. John P. Holdren, NASA Administrator Charles Bolden and NASA’s ARM Program Director, Dr. Michele Gates discussed the latest update regarding the mission. They explained the mission’s scientific and technological benefits and how ARM will demonstrate technology for defending Earth from potentially hazardous asteroids. The briefing aired live on NASA TV and the agency’s website. For more information about ARM go to <a href="https://www.nasa.gov/arm" rel="nofollow">www.nasa.gov/arm</a>. Credit: NASA/Goddard/Peter Sooy <b><a href="http://www.nasa.gov/audience/formedia/features/MP_Photo_Guidelines.html" rel="nofollow">NASA image use policy.</a></b> <b><a href="http://www.nasa.gov/centers/goddard/home/index.html" rel="nofollow">NASA Goddard Space Flight Center</a></b> enables NASA’s mission through four scientific endeavors: Earth Science, Heliophysics, Solar System Exploration, and Astrophysics. Goddard plays a leading role in NASA’s accomplishments by contributing compelling scientific knowledge to advance the Agency’s mission. <b>Follow us on <a href="http://twitter.com/NASAGoddardPix" rel="nofollow">Twitter</a></b> <b>Like us on <a href="http://www.facebook.com/pages/Greenbelt-MD/NASA-Goddard/395013845897?ref=tsd" rel="nofollow">Facebook</a></b> <b>Find us on <a href="http://instagrid.me/nasagoddard/?vm=grid" rel="nofollow">Instagram</a></b>

Dr. Holdren (left), Administrator Bolden (center) and Dr. Michele Gates (right) discuss the ARM mission during a live NASA TV briefing. Behind them is a mockup of robotic capture module for the Asteroid Redirect Mission. More info: Asteroid Redirect Mission Update – On Sept. 14, 2016, NASA provided an update on the Asteroid Redirect Mission (ARM) and how it contributes to the agency’s journey to Mars and protection of Earth. The presentation took place in the Robotic Operations Center at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. Assistant to the President for Science and Technology Dr. John P. Holdren, NASA Administrator Charles Bolden and NASA’s ARM Program Director, Dr. Michele Gates discussed the latest update regarding the mission. They explained the mission’s scientific and technological benefits and how ARM will demonstrate technology for defending Earth from potentially hazardous asteroids. The briefing aired live on NASA TV and the agency’s website. For more information about ARM go to <a href="https://www.nasa.gov/arm" rel="nofollow">www.nasa.gov/arm</a>. Credit: NASA/Goddard/Debbie Mccallum <b><a href="http://www.nasa.gov/audience/formedia/features/MP_Photo_Guidelines.html" rel="nofollow">NASA image use policy.</a></b> <b><a href="http://www.nasa.gov/centers/goddard/home/index.html" rel="nofollow">NASA Goddard Space Flight Center</a></b> enables NASA’s mission through four scientific endeavors: Earth Science, Heliophysics, Solar System Exploration, and Astrophysics. Goddard plays a leading role in NASA’s accomplishments by contributing compelling scientific knowledge to advance the Agency’s mission. <b>Follow us on <a href="http://twitter.com/NASAGoddardPix" rel="nofollow">Twitter</a></b> <b>Like us on <a href="http://www.facebook.com/pages/Greenbelt-MD/NASA-Goddard/395013845897?ref=tsd" rel="nofollow">Facebook</a></b> <b>Find us on <a href="http://instagrid.me/nasagoddard/?vm=grid" rel="nofollow">Instagram</a></b>

This sequence of radar images of asteroid 2013 ET was obtained on Mar. 10, 2013, by NASA scientists using the 230-foot 70-meter DSN antenna at Goldstone, CA, when the asteroid was about 693,000 mi 1.1 million km from Earth.

Photographed inside a laboratory at NASA's Goddard Space Flight Center in Greenbetl, Maryland, this vial contains a portion of the asteroid Bennu sample delivered to Earth by the agency's OSIRIS-REx (Origins, Spectral Interpretation, Resource Identification, and Security – Regolith Explorer) mission.

In this video frame, Jason Dworkin holds up a vial that contains part of the sample from asteroid Bennu delivered to Earth by NASA's OSIRIS-REx (Origins, Spectral Interpretation, Resource Identification, and Security – Regolith Explorer) mission in 2023. Dworkin is the mission's project scientist at NASA's Goddard Space Flight Center in Greenbelt, Maryland.

This image of an asteroid that is at least 3,600 feet (1,100 meters) long was taken on Dec. 17, 2015, by scientists using NASA's 230-foot (70-meter) DSS-14 antenna at Goldstone, California. This asteroid, named 2003 SD2020, will safely fly past Earth on Thursday, Dec. 24, at a distance of 6.8 million miles (11 million kilometers). At the time this image was taken, the asteroid was about 7.3 million miles (12 million kilometers) from Earth. In 2018, this asteroid will fly past Earth at a distance of 1.8 million miles (2.8 million kilometers). http://photojournal.jpl.nasa.gov/catalog/PIA20279

This figure represents the 1,000th near-Earth asteroid (NEA) to be detected by planetary radar since 1968. Being only 65 to 100 feet (20 to 30 meters) wide, asteroid 2021 PJ1 was too small to be imaged in any detail, but the powerful 70-meter (230-foot) Deep Space Station 14 (DSS-14) antenna at the Deep Space Network's Goldstone Deep Space Complex near Barstow, California, was able to measure the Doppler frequency of the radio waves that reflected off the object's surface. The data was recorded for 16 minutes between 2:26 p.m. and 2:42 p.m. PDT on Aug. 14, 2021. The figure shows radar echo signal strength on the vertical axis versus Doppler frequency (in units of hertz, or Hz) on the horizontal axis. The strong spike at a value of minus 70 Hz is the reflected signal (or "echo") from 2021 PJ1; the other, smaller spikes are receiver noise, which is like the static on an AM radio if there aren't any nearby stations. Using this information, scientists at NASA's Jet Propulsion Laboratory in Southern California could more accurately calculate the asteroid's velocity, its distance from Earth and its future motion around the Sun. These observations used a prediction – known as an "ephemeris" – that had relatively large uncertainties because the asteroid had been discovered only a few days earlier. If the original prediction had been perfect, the radar echo would appear at zero Hz. The fact that the radar echo is at minus 70 Hz indicates a correction could be made to the predicted velocity of minus 2.7 miles per hour (minus 1.2 meters per second). This measurement also reduced the uncertainty in the asteroid's distance from Earth from 1,300 miles (2,100 kilometers) to 5.2 miles (8.3 kilometers) – a reduction of a factor of about 250. https://photojournal.jpl.nasa.gov/catalog/PIA24563

This composite of 30 images of asteroid 2014 JO25 was generated with radar data collected using NASA Goldstone Solar System Radar in California Mojave Desert. https://photojournal.jpl.nasa.gov/catalog/PIA21594

Stardust Image of Asteroid Annefrank

Two Very Different Asteroids

This set of images from the La Sagra Sky Survey, operated by the Astronomical Observatory of Mallorca in Spain, shows the passage of asteroid 2012 DA14 shortly after its closest, and safe, approach to Earth.

This collage represents a selection of NASA radar observations of near-Earth asteroid 2006 HV5 on April 25, 2023, less than one day before its close approach with our planet at a distance of about 1.5 million miles (2.4 million kilometers, or about 6.3 times the distance between the Moon and Earth). Asteroid 2006 HV5 was discovered by the Lincoln Near-Earth Asteroid Research (LINEAR) program in New Mexico in April 2006. The radar images show that 2006 HV5 is about 1,000 feet (300 meters) across, roughly the height of the Eiffel Tower, confirming size estimates derived from infrared observations made previously by NASA's NEOWISE mission. 2006 HV5 is classified as a potentially hazardous asteroid as its orbit brings it close to Earth, but its path around the Sun is very well known and the asteroid is not an impact risk to our planet. Asteroids of this size come this close to Earth roughly once a year, on average. The new observations were made by scientists at NASA's Jet Propulsion Laboratory using the powerful 230-foot (70-meter) Goldstone Solar System Radar antenna at the Deep Space Network's facility near Barstow, California. The images confirm the asteroid's size, while also providing a detailed look at its meatball-like shape. The asteroid has a rounded appearance, is "squished" at the poles (i.e., it is oblate), and has a rotation period of about 3.6 hours. The sequence of radar images spans slightly more than one rotation. The images, which have a resolution of about 12 feet (3.75 meters) per pixel, reveal surface features such as ridges, flat regions, concavities, and small-scale topography that might indicate boulders. https://photojournal.jpl.nasa.gov/catalog/PIA25834

This composite of 25 images of asteroid 2017 BQ6 was generated with radar data collected using NASA's Goldstone Solar System Radar in California's Mojave Desert. The images were gathered on Feb. 7, 2017, between 8:39 and 9:50 p.m. PST (11:39 p.m. EST and 12:50 a.m., Feb. 7), revealing an irregular, angular-appearing asteroid about 660 feet (200 meters) in size that rotates about once every three hours. The images have resolutions as fine as 12 feet (3.75 meters) per pixel. http://photojournal.jpl.nasa.gov/catalog/PIA21452

Benjamin Reed (right), deputy program manager of NASA’s Satellite Servicing Capabilities Office, shows Dr. Holdren the technologies that NASA is developing for the Restore-L satellite servicing mission. NASA will launch the Restore-L servicer in 2020 to refuel a live satellite and demonstrate that a suite of satellite-servicing technologies are operational. More info: Asteroid Redirect Mission Update – On Sept. 14, 2016, NASA provided an update on the Asteroid Redirect Mission (ARM) and how it contributes to the agency’s journey to Mars and protection of Earth. The presentation took place in the Robotic Operations Center at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. Assistant to the President for Science and Technology Dr. John P. Holdren, NASA Administrator Charles Bolden and NASA’s ARM Program Director, Dr. Michele Gates discussed the latest update regarding the mission. They explained the mission’s scientific and technological benefits and how ARM will demonstrate technology for defending Earth from potentially hazardous asteroids. The briefing aired live on NASA TV and the agency’s website. For more information about ARM go to <a href="https://www.nasa.gov/arm" rel="nofollow">www.nasa.gov/arm</a>. Credit: NASA/Goddard/Debbie Mccallum <b><a href="http://www.nasa.gov/audience/formedia/features/MP_Photo_Guidelines.html" rel="nofollow">NASA image use policy.</a></b> <b><a href="http://www.nasa.gov/centers/goddard/home/index.html" rel="nofollow">NASA Goddard Space Flight Center</a></b> enables NASA’s mission through four scientific endeavors: Earth Science, Heliophysics, Solar System Exploration, and Astrophysics. Goddard plays a leading role in NASA’s accomplishments by contributing compelling scientific knowledge to advance the Agency’s mission. <b>Follow us on <a href="http://twitter.com/NASAGoddardPix" rel="nofollow">Twitter</a></b> <b>Like us on <a href="http://www.facebook.com/pages/Greenbelt-MD/NASA-Goddard/395013845897?ref=tsd" rel="nofollow">Facebook</a></b> <b>Find us on <a href="http://instagrid.me/nasagoddard/?vm=grid" rel="nofollow">Instagram</a></b>

Benjamin Reed, deputy program manager of NASA’s Satellite Servicing Capabilities Office, shows Dr. Holdren the technologies that NASA is developing for the Restore-L satellite servicing mission. NASA will launch the Restore-L servicer in 2020 to refuel a live satellite and demonstrate that a suite of satellite-servicing technologies are operational. More info: Asteroid Redirect Mission Update – On Sept. 14, 2016, NASA provided an update on the Asteroid Redirect Mission (ARM) and how it contributes to the agency’s journey to Mars and protection of Earth. The presentation took place in the Robotic Operations Center at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. Assistant to the President for Science and Technology Dr. John P. Holdren, NASA Administrator Charles Bolden and NASA’s ARM Program Director, Dr. Michele Gates discussed the latest update regarding the mission. They explained the mission’s scientific and technological benefits and how ARM will demonstrate technology for defending Earth from potentially hazardous asteroids. The briefing aired live on NASA TV and the agency’s website. For more information about ARM go to <a href="https://www.nasa.gov/arm" rel="nofollow">www.nasa.gov/arm</a>. Credit: NASA/Goddard/Debbie Mccallum <b><a href="http://www.nasa.gov/audience/formedia/features/MP_Photo_Guidelines.html" rel="nofollow">NASA image use policy.</a></b> <b><a href="http://www.nasa.gov/centers/goddard/home/index.html" rel="nofollow">NASA Goddard Space Flight Center</a></b> enables NASA’s mission through four scientific endeavors: Earth Science, Heliophysics, Solar System Exploration, and Astrophysics. Goddard plays a leading role in NASA’s accomplishments by contributing compelling scientific knowledge to advance the Agency’s mission. <b>Follow us on <a href="http://twitter.com/NASAGoddardPix" rel="nofollow">Twitter</a></b> <b>Like us on <a href="http://www.facebook.com/pages/Greenbelt-MD/NASA-Goddard/395013845897?ref=tsd" rel="nofollow">Facebook</a></b> <b>Find us on <a href="http://instagrid.me/nasagoddard/?vm=grid" rel="nofollow">Instagram</a></b>

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

Images of asteroid 2007 PA8 have been generated with data collected by NASA Goldstone Solar System Radar. The images of 2007 PA8 reveal possible craters, boulders, an irregular, asymmetric shape, and very slow rotation.

This collage and animation represent NASA radar observations of near-Earth asteroid 7335 1989 JA on May 26, 2022, one day before it made its closest approach with Earth. The potentially hazardous asteroid came within 2.5 million miles (4 million kilometers) of our planet, or 10.5 times the distance between the Earth and the Moon. Astronomers at NASA's Jet Propulsion Laboratory used the 230-foot (70-meter) radio antenna at the Deep Space Network's Goldstone Deep Space Communications Complex near Barstow, California, to precisely track the asteroid's motion and obtain detailed radar images. 1989 JA is a binary system, consisting of a large asteroid and a significantly smaller satellite asteroid that revolve around each other without touching. The larger asteroid is about 0.4 miles (700 meters) across and shows several topographic features as it rotates. The secondary asteroid, which was discovered this year, is between 100 and 200 meters in diameter and has an orbital period of about 17 hours. 1989 JA was discovered by Eleanor F. Helin at Palomar Observatory in Southern California on May 1, 1989. Follow-up radar observations that year did not reveal a satellite. In 2010, NASA's Wide-field Infrared Survey Explorer (WISE) was used to help determine the primary asteroid's size. This year, a few weeks before the asteroid's most recent close approach, astronomers at Ondrejov Observatory in the Czech Republic measured the asteroid's light curve (the change in reflected light intensity over time) and found hints of the satellite in orbit. The new Goldstone observations refined the size of 1989 JA and established that it is a binary system. 1989 JA does not currently pose an impact risk to Earth, but observations by planetary radar can help astronomers better understand its orbit around the Sun so that any future risk can be continually assessed. https://photojournal.jpl.nasa.gov/catalog/PIA25251

This series of 41 radar images obtained by the Deep Space Network's Goldstone Solar System Radar on July 28, 2025, shows the near-Earth asteroid 2025 OW as it made its close approach with our planet. The asteroid safely passed at about 400,000 miles (640,000 kilometers), or 1.6 times the distance from Earth to the Moon. The asteroid was discovered on July 4, 2025, by the NASA-funded Pan-STARRS2 survey telescope on Haleakala in Maui, Hawaii. These Goldstone observations suggest that 2025 OW is about 200 feet (60 meters) wide and has an irregular shape. The observations also indicate that it is rapidly spinning, completing one rotation every 1½ to 3 minutes, making it one of the fastest-spinning near-Earth asteroids that the powerful radar system has observed. The observations resolve surface features down to 12 feet (3.75 meters) wide. Asteroids can be "spun up" by sunlight being unevenly absorbed and re-emitted across their irregular surfaces. As photons (quantum particles of light) carry a tiny amount of momentum away from the asteroid, a tiny amount of torque is applied and, over time, the asteroid's spin can increase – a phenomenon known as the YORP effect. For 2025 OW to maintain such a fast rotation without breaking apart, it may be a solid object rather than a loosely bound rubble pile like many asteroids. The Goldstone measurements have allowed scientists to greatly reduce uncertainties in the asteroid's distance from Earth and in its future motion for many decades. This July 28 close approach is the closest asteroid 2025 OW will come to Earth for the foreseeable future. Animation available at https://photojournal.jpl.nasa.gov/catalog/PIA26587

The elongated asteroid in this radar image, named 2003 SD220, will safely fly past Earth on Thursday, Dec. 24, 2015, at a distance of 6.8 million miles (11 million kilometers). The image was taken on Dec. 22 by scientists using NASA's 230-foot (70-meter) Deep Space Network antenna at Goldstone, California, when the asteroid was approaching its flyby distance. This asteroid is at least 3,600 feet (1,100 meters) long. In 2018, it will safely pass Earth at a distance of 1.8 million miles (2.8 million kilometers). http://photojournal.jpl.nasa.gov/catalog/PIA20280

Radar images of the binary asteroid 2017 YE5 from NASA's Goldstone Solar System Radar (GSSR). The observations, conducted on June 23, 2018, show two lobes, but do not yet show two separate objects. A movie is available at https://photojournal.jpl.nasa.gov/catalog/PIA22557

This optical composite image shows asteroid 2017 YE5, taken on June 30, 2018, by the Cadi Ayyad University Morocco Oukaimeden Sky Survey, one of the first surveys to identify 2017 YE5 in December 2017. https://photojournal.jpl.nasa.gov/catalog/PIA22558

Though fragile comet nuclei have been seen falling apart as they near the Sun, nothing like the slow breakup of an asteroid has ever before been observed in the asteroid belt. A series of Hubble Space Telescope images shows that the fragments are drifting away from each other at a leisurely one mile per hour. This makes it unlikely that the asteroid is disintegrating because of a collision with another asteroid. A plausible explanation is that the asteroid is crumbling due to a subtle effect of sunlight. This causes the rotation rate to slowly increase until centrifugal force pulls the asteroid apart. The asteroid's remnant debris, weighing in at 200,000 tons, will in the future provide a rich source of meteoroids. Hubble Observation of P/2013 R3 - November 15, 2013 Credit: NASA, ESA, and D. Jewitt (University of California, Los Angeles) Read more: <a href="http://1.usa.gov/1ig2E0x" rel="nofollow">1.usa.gov/1ig2E0x</a> <b><a href="http://www.nasa.gov/audience/formedia/features/MP_Photo_Guidelines.html" rel="nofollow">NASA image use policy.</a></b> <b><a href="http://www.nasa.gov/centers/goddard/home/index.html" rel="nofollow">NASA Goddard Space Flight Center</a></b> enables NASA’s mission through four scientific endeavors: Earth Science, Heliophysics, Solar System Exploration, and Astrophysics. Goddard plays a leading role in NASA’s accomplishments by contributing compelling scientific knowledge to advance the Agency’s mission. <b>Follow us on <a href="http://twitter.com/NASAGoddardPix" rel="nofollow">Twitter</a></b> <b>Like us on <a href="http://www.facebook.com/pages/Greenbelt-MD/NASA-Goddard/395013845897?ref=tsd" rel="nofollow">Facebook</a></b> <b>Find us on <a href="http://instagram.com/nasagoddard?vm=grid" rel="nofollow">Instagram</a></b>

Though fragile comet nuclei have been seen falling apart as they near the Sun, nothing like the slow breakup of an asteroid has ever before been observed in the asteroid belt. A series of Hubble Space Telescope images shows that the fragments are drifting away from each other at a leisurely one mile per hour. This makes it unlikely that the asteroid is disintegrating because of a collision with another asteroid. A plausible explanation is that the asteroid is crumbling due to a subtle effect of sunlight. This causes the rotation rate to slowly increase until centrifugal force pulls the asteroid apart. The asteroid's remnant debris, weighing in at 200,000 tons, will in the future provide a rich source of meteoroids. Hubble Observation of P/2013 R3 - November 15, 2013 Credit: NASA, ESA, and D. Jewitt (University of California, Los Angeles) Read more: <a href="http://1.usa.gov/1ig2E0x" rel="nofollow">1.usa.gov/1ig2E0x</a> <b><a href="http://www.nasa.gov/audience/formedia/features/MP_Photo_Guidelines.html" rel="nofollow">NASA image use policy.</a></b> <b><a href="http://www.nasa.gov/centers/goddard/home/index.html" rel="nofollow">NASA Goddard Space Flight Center</a></b> enables NASA’s mission through four scientific endeavors: Earth Science, Heliophysics, Solar System Exploration, and Astrophysics. Goddard plays a leading role in NASA’s accomplishments by contributing compelling scientific knowledge to advance the Agency’s mission. <b>Follow us on <a href="http://twitter.com/NASAGoddardPix" rel="nofollow">Twitter</a></b> <b>Like us on <a href="http://www.facebook.com/pages/Greenbelt-MD/NASA-Goddard/395013845897?ref=tsd" rel="nofollow">Facebook</a></b> <b>Find us on <a href="http://instagram.com/nasagoddard?vm=grid" rel="nofollow">Instagram</a></b>

This series of radar images obtained by the Deep Space Network's Goldstone Solar System Radar near Barstow, California, on Sept. 16, 2024, shows the near-Earth asteroid 2024 ON a day before its close approach with our planet. The asteroid passed Earth at a distance of 620,000 miles (1 million kilometers) – about 2.6 times the distance between the Moon and Earth. Discovered by the NASA-funded Asteroid Terrestrial-impact Last Alert System (ATLAS) on Mauna Loa in Hawaii on July 27, the near-Earth asteroid's shape resembles that of a peanut. Like the asteroid 2024 JV33 that made close approach with Earth a month earlier, 2024 ON is likely a contact binary, with two rounded lobes separated by a pronounced neck, one lobe about 50% larger than the other. The radar images determined that it is about 1150 feet (350 meters) long. Features larger than 12.3 feet (3.75 meters) across can be seen on the surface. Bright radar spots on the asteroid's surface likely indicate large boulders. The images show about 90% of one rotation over the course of about six hours. Radar is the principal technique for discovering contact binaries, dozens of which have been imaged by planetary radar. At least 14% of near-Earth asteroids larger than about 200 meters (660 feet) have a contact binary shape. This asteroid is classified as potentially hazardous, but it does not pose a hazard to Earth for the foreseeable future. These Goldstone measurements have allowed scientists to greatly reduce the uncertainties in the asteroid's distance from Earth and in its future motion for many decades. Animation available at https://photojournal.jpl.nasa.gov/catalog/PIA26451

This illustration depicts NASA's Double Asteroid Redirection Test (DART) spacecraft prior to impact at the Didymos binary asteroid system. DART's target asteroid is the moonlet Dimorphos, which orbits the larger asteroid Didymos; the pair are not a threat to Earth. This asteroid system will be a testing ground to see if intentionally crashing a spacecraft into an asteroid is an effective way to change its course, should an Earth-threatening asteroid be discovered in the future. The Johns Hopkins Applied Physics Laboratory in Laurel, Maryland, manages the DART mission for NASA's Planetary Defense Coordination Office as a project of the agency's Planetary Missions Program Office. DART is the world's first planetary defense test mission, intentionally executing a kinetic impact into Dimorphos to slightly change its motion in space. While the asteroid does not pose any threat to Earth, the DART mission will demonstrate that a spacecraft can autonomously navigate to a kinetic impact on a relatively small asteroid and prove this is a viable technique to deflect an asteroid on a collision course with Earth if one is ever discovered. DART will reach its target on Sept. 26, 2022. https://photojournal.jpl.nasa.gov/catalog/PIA25329

NEOWISE, the asteroid-hunting portion of NASA WISE mission, illustrates the differences between orbits of a typical near-Earth asteroid blue and a potentially hazardous asteroid, or PHA orange. PHAs are a subset of the near-Earth asteroids NEAs.

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

An animated set of images, from the telescope known as the iTelescope.net Siding Spring Observatory, shows asteroid 2012 DA14 as the streak moving from top to bottom in the field of view. The animation is available in the Planetary Photojournal.

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

Researchers at NASA's Goddard Space Flight Center in Greenbelt, Maryland, who had a hand in studying the asteroid Bennu sample delivered to Earth by the agency's OSIRIS-REx (Origins, Spectral Interpretation, Resource Identification, and Security – Regolith Explorer) mission.

This collage represents a selection of planetary radar observations of asteroid 2008 OS7 that were made the day before its close approach with our planet on Feb. 2, 2024. The stadium-size near-Earth object passed at a distance of about 1.8 million miles (2.9 million kilometers, or 7 ½ times the distance between Earth and the Moon). Scientists at NASA's Jet Propulsion Laboratory used the powerful 230-foot (70-meter) Goldstone Solar System Radar antenna at the Deep Space Network's facility near Barstow, California, to capture these images. The observations will help scientists better understand the asteroid's size, rotation, shape, and surface details. Until this close approach, very little was known about 2008 OS7 as it has been too distant for planetary radar to image it. The asteroid was discovered on July 30, 2008, during routine search operations for NEOs by the NASA-funded Catalina Sky Survey, which is headquartered at the University of Arizona in Tucson. Observations revealed that the asteroid is comparatively slow rotating, completing one rotation every 29 ½ hours. The rotational period of 2008 OS7 was determined Petr Pravec, at the Astronomical Institute of the Czech Academy of Sciences in Ondřejov, Czech Republic, who observed the asteroid's light curve – or how the brightness of the object changes over time. As the asteroid spins, variations on its shape can change the brightness of reflected light astronomers can see, and those changes can be recorded to understand the period of the asteroid's rotation. The Goldstone observations confirm the asteroid's uncommonly slow rotation. https://photojournal.jpl.nasa.gov/catalog/PIA26149

This composite image of asteroid 2007 PA8 was obtained using data taken by NASA 230-foot-wide 70-meter Deep Space Network antenna at Goldstone, Calif.

This frame from a video demonstrates how NASA Wide-field Infrared Survey Explorer surveys asteroids and comets in the solar system. Perspective shown here is looking down from high above Earth North Pole, a kind of bird eye view of the solar system.

This series of seven radar observations by the Deep Space Network's Goldstone Solar System Radar shows the asteroid 2011 UL21 during its close approach with Earth from 4.1 million miles (6.6 million kilometers) away – about 17 times the distance between the Moon and Earth. White circles highlight the main asteroid and its small moon (a bright dot at the bottom of the image). Passing Earth on June 27, 2024, the asteroid was discovered in 2011 by the NASA-funded Catalina Sky Survey, in Tucson, Arizona. This marked the first time it came close enough to Earth to be imaged by radar. While the nearly mile-wide (1.5-kilometer-wide) object is classified as being potentially hazardous, calculations of its future orbits show that it won't pose a threat to our planet for the foreseeable future. In addition to determining the asteroid is roughly spherical, scientists at NASA's Jet Propulsion Laboratory discovered that it's a binary system: A smaller asteroid, or moonlet, orbits it from a distance of about 1.9 miles (3 kilometers). https://photojournal.jpl.nasa.gov/catalog/PIA26384

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

Jason Dworkin, project scientist for NASA's OSIRIS-REx (Origins, Spectral Interpretation, Resource Identification, and Security – Regolith Explorer) mission, examines a portion of the asteroid Bennu sample delivered to Earth in a laboratory at the agency's Goddard Space Flight Center in Greenbelt, Maryland.

This frame from a movie of asteroid 2014 JO25 was generated using radar data collected by NASA 230-foot-wide 70-meter Deep Space Network antenna at Goldstone, California on April 19, 2017. When the observations began 2014 JO25 was 1.53 million miles (2.47 million kilometers) from Earth. By the time the observations concluded, the asteroid was 1.61 million miles (2.59 million kilometers) away. The asteroid has a contact binary structure -- two lobes connected by a neck-like region. The largest of the asteroid's two lobes is estimated to be 2,000 feet (610 meters) across. Asteroid 2014 JO25 approached to within 1.1 million miles (1.8 million kilometers) of Earth on April 19. There are no future flybys by 2014 JO25 as close as this one for more than 400 years. The resolution of the radar images is about 25 feet (7.5 meters) per pixel. 154 images were used to create a movie. The movie can be seen at. https://photojournal.jpl.nasa.gov/catalog/PIA21597

Radar Model of Asteroid 216 Kleopatra

NASA’s Double Asteroid Redirection Test (DART) command team at Johns Hopkins University, Applied Physics Laboratory monitoring the DART spacecraft’s impact into the asteroid Dimorphos. The operation is the first of its kind test to redirect deadly asteroids from hitting Earth.

This computer generated image depicts a view of Earth as seen from the surface of the asteroid Toutatis on Nov 29th 1996. A 2.5 degree field-of-view synthetic computer camera was used for this simulation. Toutatis is visible on this date as a twelfth magnitude object in the night sky in the constellation of Virgo and could be viewed with a medium sized telescope. Toutatis currently approaches Earth once every four years and, on Nov. 29th, 1996 will be 5.2 million kilometers away (approx. 3.3 million miles). In approximately 8 years, on Sept. 29th, 2004, it will be less than 1.6 million kilometers from Earth. This is only 4 times the distance to the moon, and is the closest approach predicted for any known asteroid or comet during the next 60 years. http://photojournal.jpl.nasa.gov/catalog/PIA00515

This collage represents NASA radar observations of near-Earth asteroid 2011 AG5 on Feb. 4, 2023, one day after its close approach to Earth brought it about 1.1 million miles (1.8 million kilometers, or a little under five times the distance between the Moon and Earth) from our planet. While there was no risk of 2011 AG5 impacting Earth, scientists at NASA's Jet Propulsion Laboratory in Southern California closely tracked the asteroid, making invaluable observations to help determine its size, rotation, surface details, and shape. More than three times as long as it is wide, 2011 AG5 is one of the most elongated asteroids to be observed by planetary radar to date. This close approach provided the first opportunity to take a detailed look at the asteroid since it was discovered in 2011, showing an object about 1,600 feet (500 meters) long and about 500 feet (150 meters) wide – dimensions comparable to the Empire State Building. The powerful 230-foot (70-meter) Goldstone Solar System Radar antenna dish at the Deep Space Network's facility near Barstow, California, revealed the asteroid's noteworthy dimensions. The Goldstone observations show that 2011 AG5 has a large concavity in one of its hemispheres and some subtle dark and lighter regions that may indicate small-scale surface features a few dozen meters across. If viewed by the human eye, 2011 AG5 would appear as dark as charcoal. The observations also confirmed the asteroid has a slow rotation rate, taking nine hours to fully rotate. https://photojournal.jpl.nasa.gov/catalog/PIA25259

NASA Deputy Administrator Lori Garver discusses the progress being made on NASA's mission to capture, redirect, and explore an asteroid during the Asteroid Initiative Industry and Partner Day at NASA Headquarters on Tuesday, June 18, 2013 in Washington. NASA also announced an Asteroid Grand Challenge focused on finding all asteroid threats to human populations and knowing what to do about them. Photo Credit: (NASA/Bill Ingalls)

NASA Deputy Administrator Lori Garver discusses the progress being made on NASA's mission to capture, redirect, and explore an asteroid during the Asteroid Initiative Industry and Partner Day at NASA Headquarters on Tuesday, June 18, 2013 in Washington. NASA also announced an Asteroid Grand Challenge focused on finding all asteroid threats to human populations and knowing what to do about them. Photo Credit: (NASA/Bill Ingalls)

NASA Associate Administrator Robert Lightfoot, talks during the Asteroid Initiative Industry and Partner Day at NASA Headquarters on Tuesday, June 18, 2013 in Washington. During the event NASA Deputy Administrator Lori Garver and other senior NASA officials discussed the progress being made on NASA's mission to capture, redirect, and explore an asteroid. NASA also announced an Asteroid Grand Challenge focused on finding all asteroid threats to human populations and knowing what to do about them. Photo Credit: (NASA/Bill Ingalls)

NASA Deputy Administrator Lori Garver discusses the progress being made on NASA's mission to capture, redirect, and explore an asteroid during the Asteroid Initiative Industry and Partner Day at NASA Headquarters on Tuesday, June 18, 2013 in Washington. NASA also announced an Asteroid Grand Challenge focused on finding all asteroid threats to human populations and knowing what to do about them. Photo Credit: (NASA/Bill Ingalls)

This frame from a movie shows the asteroid 2012 DA14 flying safely by Earth, as seen by the Gingin Observatory in Australia around the time of its closest approach, 11:24:42 a.m. PST 2:24:42 p. The animation is available in the Planetary Photojournal.

This frame from a movie from the Samford Valley Observatory in Brisbane, Australia, shows the progress of asteroid 2012 DA14 across the night sky as it nears its closest approach. It was taken at 12:59 UTC on Feb. 15 7:59 a.m. EST, or 4:59 a.m. PST.

This radar image of asteroid 2005 YU55 was obtained NASA Deep Space Network antenna in Goldstone, Calif. on Nov. 7, 2011, when the space rock was at 3.6 lunar distances, which is about 860,000 miles, or 1.38 million kilometers, from Earth.

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

Jenn Gustetic, Prizes Program Executive, NASA Office of the Chief Technologist moderates the Asteroid Initiative Industry and Partner Day at NASA Headquarters on Tuesday, June 18, 2013 in Washington. During the event NASA Deputy Administrator Lori Garver and other senior NASA officials discussed the progress being made on NASA's mission to capture, redirect, and explore an asteroid. NASA also announced an Asteroid Grand Challenge focused on finding all asteroid threats to human populations and knowing what to do about them. Photo Credit: (NASA/Bill Ingalls)

NASA Associate Administrator Robert Lightfoot, listens as other NASA senior leadership talk during the Asteroid Initiative Industry and Partner Day at NASA Headquarters on Tuesday, June 18, 2013 in Washington. During the event NASA Deputy Administrator Lori Garver and other senior NASA officials discussed the progress being made on NASA's mission to capture, redirect, and explore an asteroid. NASA also announced an Asteroid Grand Challenge focused on finding all asteroid threats to human populations and knowing what to do about them. Photo Credit: (NASA/Bill Ingalls)

Jason Kessler, Special Projects Program Executive, NASA Office of the Chief Technologist, talks during the Asteroid Initiative Industry and Partner Day at NASA Headquarters on Tuesday, June 18, 2013 in Washington. During the event NASA Deputy Administrator Lori Garver and other senior NASA officials discussed the progress being made on NASA's mission to capture, redirect, and explore an asteroid. NASA also announced an Asteroid Grand Challenge focused on finding all asteroid threats to human populations and knowing what to do about them. Photo Credit: (NASA/Bill Ingalls)

NASA Associate Administrator for Human Exploration and Operations, William Gerstenmaier, talks during the Asteroid Initiative Industry and Partner Day at NASA Headquarters on Tuesday, June 18, 2013 in Washington. During the event NASA Deputy Administrator Lori Garver and other senior NASA officials discussed the progress being made on NASA's mission to capture, redirect, and explore an asteroid. NASA also announced an Asteroid Grand Challenge focused on finding all asteroid threats to human populations and knowing what to do about them. Photo Credit: (NASA/Bill Ingalls)

NASA Associate Administrator Science John Grunsfeld, Ph.D, displays a fragment of the Pallasite meteorite from Chubut, Argentina found in 1951 and given to him by his daughter on Father's Day during the Asteroid Initiative Industry and Partner Day at NASA Headquarters on Tuesday, June 18, 2013 in Washington. During the event NASA Deputy Administrator Lori Garver and other senior NASA officials discussed the progress being made on NASA's mission to capture, redirect, and explore an asteroid. NASA also announced an Asteroid Grand Challenge focused on finding all asteroid threats to human populations and knowing what to do about them. Photo Credit: (NASA/Bill Ingalls)

Jason Kessler, Special Projects Program Executive, NASA Office of the Chief Technologist, talks during the Asteroid Initiative Industry and Partner Day at NASA Headquarters on Tuesday, June 18, 2013 in Washington. During the event NASA Deputy Administrator Lori Garver and other senior NASA officials discussed the progress being made on NASA's mission to capture, redirect, and explore an asteroid. NASA also announced an Asteroid Grand Challenge focused on finding all asteroid threats to human populations and knowing what to do about them. Photo Credit: (NASA/Bill Ingalls)

NASA Associate Administrator Robert Lightfoot, left, talks as NASA Associate Administrator Science John Grunsfeld, Ph.D, listens during the Asteroid Initiative Industry and Partner Day at NASA Headquarters on Tuesday, June 18, 2013 in Washington. During the event NASA Deputy Administrator Lori Garver and other senior NASA officials discussed the progress being made on NASA's mission to capture, redirect, and explore an asteroid. NASA also announced an Asteroid Grand Challenge focused on finding all asteroid threats to human populations and knowing what to do about them. Photo Credit: (NASA/Bill Ingalls)