This image shows InSight's domed Wind and Thermal Shield, which covers its seismometer. The image was taken on the 110th Martian day, or sol, of the mission. The seismometer is called Seismic Experiment for Interior Structure, or SEIS. https://photojournal.jpl.nasa.gov/catalog/PIA23177

NASA's InSight lander used the scoop on its robotic arm to begin trickling soil over the cable connecting its seismometer to the spacecraft on March 14, 2021, the 816th Martian day, or sol of the mission. Scientists hope this make it easier to detect marsquakes by helping to insulate the cable from the wind and from the extreme temperature shifts that cause the cable to expand and contract. Animation available at https://photojournal.jpl.nasa.gov/catalog/PIA24450

A fish-eye view of NASA's InSight lander deploying its first instrument onto the surface of Mars. InSight's robotic arm placed the seismometer on Dec. 19, 2018, around the time of dusk on Mars. These images were taken by the Instrument Context Camera (ICC), a fish-eye camera under the spacecraft's deck. Animation available at https://photojournal.jpl.nasa.gov/catalog/PIA22978

S69-39587 (20 July 1969) --- Dr. Garry Latham (left) with the Lamont Geological Observatory, studies seismometer tracings in the Mission Control Center's (MCC) ALSEP control room. The electronic data was coming from the Passive Seismic Experiments Package (PSEP) which the Apollo 11 astronauts had just deployed on the surface of the moon. Dr. Lamont is the principal investigator for the PSEP, a component of the Early Apollo Scientific Experiments Package (EASEP). PSEP uses three long-period seismometers and one short-period vertical seismometer for measuring meteoroid impacts and moonquakes. Such data will be useful in determining the interior structure of the moon; for example, does the moon have a core and mantle like Earth? Here, the flapping of the PSEP's solar panels is picked up and registered as a tracing. The PSEP was sensitive enough to pick up the footsteps of astronauts Neil A. Armstrong and Edwin E. Aldrin Jr., as they walked on the moon.

S69-39588 (20 July 1969) --- Dr. Garry Latham, with the Lamont Geological Observatory, studies seismometer tracings in the Mission Control Center?s ASEP control room. The electronic data was coming from the Passive Seismic Experiments Package which the Apollo 11 astronauts had just deployed on the surface of the moon. Dr. Lamont is the principal investigator for the PSEP, a component of the Early Apollo Scientific Experiments Package (EASEP). PSEP uses three long-period seismometers and one short-period vertical seismometer for measuring meteoroid impacts and moonquakes. Such data will be useful in determining the interior structure of the moon; for example, does the moon have a core and mantle like Earth? Here, the center trace shows evidence of activity on the moon. The PSEP was sensitive enough to pick up the footsteps of astronauts Neil A. Armstrong and Edwin E. Aldrin Jr. as they walked on the moon.

NASA's InSight lander placed its seismometer onto Mars on Dec. 19, 2018. This was the first time a seismometer had ever been placed onto the surface of another planet. The seismometer is the copper-colored object in this image, which was taken around Martian dusk. The seismometer, called Seismic Explorations for Interior Structure (SEIS), will measure seismic waves caused by marsquakes, meteorite strikes and other phenomena. Watching how these waves travel through Mars' interior will let scientists study how the planet's crust, mantle and core are layered. It will also reveal more about how all rocky bodies are formed, including Earth and its Moon. https://photojournal.jpl.nasa.gov/catalog/PIA22956

The seismometer reading from the impact made by the Apollo 15 Saturn S-IVB stage when it struck the lunar surface is studied by scientists in the Mission Control Center. Dr. Gary Latham (dark suit, wearing lapel button) of Columbia University is responsible for the design and experiment data analysis of the Passive Seismic Experiment of the Apollo Lunar Surface Experiment Package (ALSEP). The man on the left, writing, is Nafi Toksos of the Massachusetts Institute of Technology. Looking on at upper left is Dave Lamneline, also with Columbia.

A copy of one of the sensors on NASA InSight's seismometer, compared to a 2-euro coin (about 1 inch wide). The short-period seismometer has three of these sensors. https://photojournal.jpl.nasa.gov/catalog/PIA22926

From left, mechanical engineer Gabrielle Ludwig, technician Alex Schaeffer, and mechanical engineer Mitchell Hamann install the Lunar Environment Monitoring Station (LEMS) instrument onto a test plate in a thermal vacuum chamber at Goddard Space Flight Center, Greenbelt Md., March 30, 2026. LEMS is a compact, autonomous, and self-sustaining seismometer suite designed to carry out continuous, long-term, monitoring of the lunar seismic environment at the South Polar region. Photo Credit: NASA/Denny Henry

Engineering technician Jancilon Viegas installs thermocouples onto the The Lunar Environment Monitoring Station (LEMS) instrument in preparation for testing in a thermal vacuum chamber at Goddard Space Flight Center, Greenbelt Md., March 30, 2026. LEMS is a compact, autonomous, and self-sustaining seismometer suite designed to carry out continuous, long-term, monitoring of the lunar seismic environment at the South Polar region. Photo Credit: NASA/Denny Henry

Mitchell Hamann and John Pindell configure the Lunar Environment Monitoring Station (LEMS) instrument for testing in the Electromagnetic Interference/Electromagnetic Compatibility (EMI/EMC) Chamber at Goddard Space Flight Center, Greenbelt Md., Feb 17, 2026. LEMS is a compact, autonomous, and self-sustaining seismometer suite designed to carry out continuous, long-term, monitoring of the lunar seismic environment at the South Polar region. Photo Credit: NASA/Mike Guinto

Lunar Environment Monitoring Station (LEMS) team members install the instrument for testing in the Electromagnetic Interference/Electromagnetic Compatibility (EMI/EMC) Chamber at Goddard Space Flight Center, Greenbelt Md., Feb 13, 2026. LEMS is a compact, autonomous, and self-sustaining seismometer suite designed to carry out continuous, long-term, monitoring of the lunar seismic environment at the South Polar region. Photo Credit: NASA/Denny Henry

Chief Operating Officer of Quest Thermal Group Phillip Tyler installs Integrated Multilayer Insulation (IMLI) on the Lunar Environment Monitoring Station for Artemis (LEMS) bus inside a cleanroom at Goddard Space Flight Center, Greenbelt Md., Jan 13, 2026. LEMS is a compact, autonomous, and self-sustaining seismometer suite designed to carry out continuous, long-term, monitoring of the lunar seismic environment at the South Polar region. Photo Credit: NASA/Denny Henry

A detail view of the Lunar Environment Monitoring Station, (LEMS) bus prior to thermal blanket installation inside the cleanroom at Goddard Space Flight Center, Greenbelt Md., Jan 12, 2026. LEMS is a compact, autonomous, and self-sustaining seismometer suite designed to carry out continuous, long-term, monitoring of the lunar seismic environment at the South Polar region. Photo Credit: NASA/Denny Henry

Artemis Scientist, Trevor Graff, performs instrument deployment exercises with a medium fidelity mock up of the Lunar Environment Monitoring Station (LEMS) in the lunar simulant bin at the Florida Space Institute Exolith Lab, Orlando, Fl., Aug 6, 2025. LEMS is a compact, autonomous, and self-sustaining seismometer suite designed to carry out continuous, long-term, monitoring of the lunar seismic environment at the South Polar region. Photo Credit: NASA/Katie Mellos.

Artemis Scientist, Trevor Graff, performs instrument deployment exercises with a medium fidelity mock up of the Lunar Environment Monitoring Station (LEMS) in the lunar simulant bin at the Florida Space Institute Exolith Lab, Orlando, Fl., Aug 6, 2025. LEMS is a compact, autonomous, and self-sustaining seismometer suite designed to carry out continuous, long-term, monitoring of the lunar seismic environment at the South Polar region. Photo Credit: NASA/Katie Mellos.

The Lunar Environment Monitoring Station (LEMS) medium fidelity instrument mock up is configured for instrument deployment exercises in the lunar simulant bin at the Florida Space Institute Exolith Lab, Orlando, Fl., Aug 6, 2025. LEMS is a compact, autonomous, and self-sustaining seismometer suite designed to carry out continuous, long-term, monitoring of the lunar seismic environment at the South Polar region. Photo Credit: NASA/Katie Mellos.

Team members install the Lunar Environment Monitoring Station (LEMS) instrument for testing in a thermal vacuum chamber at Goddard Space Flight Center, Greenbelt Md., March 30, 2026. LEMS is a compact, autonomous, and self-sustaining seismometer suite designed to carry out continuous, long-term, monitoring of the lunar seismic environment at the South Polar region. Photo Credit: NASA/Denny Henry

The Lunar Environment Monitoring Station (LEMS) in Electromagnetic Interference/Electromagnetic Compatibility (EMI/EMC) Chamber at Goddard Space Flight Center, Greenbelt Md., Feb 11, 2026. LEMS is a compact, autonomous, and self-sustaining seismometer suite designed to carry out continuous, long-term, monitoring of the lunar seismic environment at the South Polar region. Photo Credit: NASA/Denny Henry

The Lunar Environment Monitoring Station (LEMS) instrument is installed for testing in a thermal vacuum chamber at Goddard Space Flight Center, Greenbelt Md., March 30, 2026. LEMS is a compact, autonomous, and self-sustaining seismometer suite designed to carry out continuous, long-term, monitoring of the lunar seismic environment at the South Polar region. Photo Credit: NASA/Denny Henry

The Lunar Environment Monitoring Station (LEMS) instrument is installed for testing in a thermal vacuum chamber at Goddard Space Flight Center, Greenbelt Md., March 30, 2026. LEMS is a compact, autonomous, and self-sustaining seismometer suite designed to carry out continuous, long-term, monitoring of the lunar seismic environment at the South Polar region. Photo Credit: NASA/Denny Henry

Electrical test engineer Thomas Schluszas configures the Lunar Environment Monitoring Station (LEMS) instrument for testing in the Electromagnetic Interference/Electromagnetic Compatibility (EMI/EMC) Chamber at Goddard Space Flight Center, Greenbelt Md., Feb 17, 2026. LEMS is a compact, autonomous, and self-sustaining seismometer suite designed to carry out continuous, long-term, monitoring of the lunar seismic environment at the South Polar region. Photo Credit: NASA/Denny Henry

S69-59547 (20 Nov. 1969) --- The seismometer reading from the impact made by the Lunar Module ascent stage when it struck the lunar surface. The impact was registered by the Passive Seismic Experiment Package which was deployed on the moon by the Apollo 12 astronauts. PSEP, which is a component of the Apollo Lunar Surface Experiments Package, will detect surface tilt produced by tidal deformations, moonquakes, and meteorite impacts. The LM's ascent stage was jettisoned and sent journeying toward impact on the moon after astronauts Charles Conrad Jr. and Alan L. Bean returned to lunar orbit and rejoined astronaut Richard F. Gordon Jr. in the Command and Service Modules. Information from the PSEP is transmitted to Earth through the ALSEP's central station and monitored by equipment at the Manned Spacecraft Center.

Engineer Marleen Sundgaard watches as a test version of NASA's Mars InSight lander grasps a model of the spacecraft's seismometer. This work was done at NASA's Jet Propulsion Laboratory in Pasadena, California. https://photojournal.jpl.nasa.gov/catalog/PIA22952

This is one of the last images ever taken by NASA's InSight Mars lander. Captured on Dec. 11, 2022, the 1,436th Martian day, or sol, of the mission, it shows InSight's seismometer on the Red Planet's surface. https://photojournal.jpl.nasa.gov/catalog/PIA25680

NASA's InSight spacecraft and its recently deployed Wind and Thermal Shield were imaged on Mars on Feb. 4, 2019, by the HiRISE camera aboard NASA's Mars Reconnaissance Orbiter. On Feb. 2, 2019, InSight's robotic arm placed the special shield over its seismometer on the Martian surface to protect the instrument from wind and extreme temperatures. The green object in this image is the InSight lander; the white dot just below it is the shield, which is especially bright and reflective. The shield is a little less than 6 feet (1.8 meters) away from the lander. The dark circles on either side of the lander are its solar panels. The total width of the lander with both panels open is 19 feet, 8 inches (6 meters). The image also shows the darkened ground where InSight's retrorockets blew away lighter-colored dust as the lander touched down on Nov. 26, 2018. Scientists are interested in imaging this location over time to watch how quickly the lighter-colored Martian dust covers that darkened surface. https://photojournal.jpl.nasa.gov/catalog/PIA23043

NASA's Farside Seismic Suite (FSS) is assembled in a clean room at the agency's Jet Propulsion Laboratory in Southern California in November 2023. Two sensitive seismometers packaged in the suite's cube-within-a-cube structure will gather NASA's first seismic data from the Moon in nearly 50 years and take the first-ever seismic measurements from the Moon's far side. FSS will operate continuously for at least 4½ months, working through the long, cold lunar nights. Seen here is the inner cube structure, with the suite's large battery at rear. The gold, puck-shaped device at left is the Short Period sensor, or SP, which measures motion in three directions using sensors etched into a trio of square silicon chips, each about 1 inch (25 millimeters) wide. At right, within the silver cylindrical enclosure, is the Very Broadband seismometer, or VBB, the most sensitive seismometer ever built for use in space exploration. It can detect ground motions smaller than the size of a single hydrogen atom, measuring up-and-down movement using a pendulum held in place by a spring. Constructed as a backup instrument (a "flight spare") for NASA's InSight Mars lander by the French space agency, CNES (Centre National d'Études Spatiales), the VBB was slightly modified and packaged in a new enclosure for lunar use. The suite's computer and electronics are packed alongside the battery and seismometers. After being encased in insulation, this inner cube was suspended within a protective outer cube, which was in turn covered with a shiny insulating blanket. https://photojournal.jpl.nasa.gov/catalog/PIA26300

NASA's InSight lander deployed its Wind and Thermal Shield on Feb. 2, 2019 (sol 66). The shield covers InSight's seismometer, which was set down onto the Martian surface on Dec. 19, 2018. This image was taken by the Instrument Deployment Camera on the lander's robotic arm. https://photojournal.jpl.nasa.gov/catalog/PIA22959

The spectrogram of vibrations (frequency spectrum over time) recorded by two of the three sensors of the short period seismometer on NASA's InSight lander on Mars. This spectrogram shows the first 1,000 seconds, roughly 20 minutes, of InSight's first seismic data from the Red Planet. The vibrations of the lander are due to the wind passing over the spacecraft, particularly the large solar arrays. https://photojournal.jpl.nasa.gov/catalog/PIA22925

NASA's InSight Mars lander uses a seismometer to study the inner layers of Mars. Seismic signals from quakes change as they pass through different kinds of materials; seismologists can "read" the squiggles of a seismogram to study the properties of the planet's crust, mantle, and core. This infographic shows those layers, and how InSight uses quakes to study them. It also shows a close-up of InSight and the major sources of marsquakes. Most quakes are created by heat and pressure inside the planet, which cause rock to fracture; another source is meteors striking the surface. https://photojournal.jpl.nasa.gov/catalog/PIA25282

NASA's Mars Reconnaissance Orbiter captured this image of a meteoroid impact that was first detected by the agency's InSight lander using its seismometer. This crater was formed on Feb. 18, 2021. MRO's High Resolution Imaging Science Experiment (HiRISE) camera captured this scene in color. The ground is not actually blue; this enhanced-color image highlights certain hues in the scene to make details more visible to the human eye – in this case, dust and soil disturbed by the impact. https://photojournal.jpl.nasa.gov/catalog/PIA25409

NASA's Mars Reconnaissance Orbiter captured this image of a meteoroid impact that was first detected by the agency's InSight lander using its seismometer. This crater was formed on Aug. 30, 2021. MRO's High Resolution Imaging Science Experiment (HiRISE) camera captured this scene in color. The ground is not actually blue; this enhanced-color image highlights certain hues in the scene to make details more visible to the human eye – in this case, dust and soil disturbed by the impact. https://photojournal.jpl.nasa.gov/catalog/PIA25411

This artist's rendering shows a cutaway of the Seismic Experiment for Interior Structure instrument, or SEIS, which will fly as part of NASA's Mars InSight lander. SEIS is a highly sensitive seismometer that will be used to detect marsquakes from the Red Planet's surface for the first time. There are two layers in this cutaway. The outer layer is the Wind and Thermal Shield -- a covering that protects the seismometer from the Martian environment. The wind on Mars, as well as extreme temperature changes, could affect the highly sensitive instrument. The inside layer is SEIS itself, a brass-colored dome that houses the instrument's three pendulums. These insides are inside a titanium vacuum chamber to further isolate them from temperature changes on the Martian surface. https://photojournal.jpl.nasa.gov/catalog/PIA22320

The Seismic Experiment for Interior Structure (SEIS) instrument for NASA's InSight mission to Mars undergoes a checkout for the spacecraft's assembly, test and launch operations (ATLO) in this photo taken July 20, 2017, in a Lockheed Martin clean room facility in Littleton, Colorado. The SEIS was provided by France's national space agency (CNES) with collaboration from the United States, the United Kingdom, Switzerland and Germany. The InSight mission (for Interior Exploration using Seismic Investigations, Geodesy and Heat Transport) is scheduled to launch in May 2018 and land on Mars Nov. 26, 2018. It will investigate processes that formed and shaped Mars and will help scientists better understand the evolution of our inner solar system's rocky planets, including Earth. https://photojournal.jpl.nasa.gov/catalog/PIA21846

In a clean room at NASA's Jet Propulsion Laboratory in Southern California in March 2024, engineers and technicians prepare the agency's Farside Seismic Suite (FSS) for testing. The cube-shaped payload contains two instruments that will gather NASA's first seismic data from the Moon in nearly 50 years and take the first-ever seismic measurements from the Moon's far side. FSS will operate continuously for at least 4½ months, working through the long, cold lunar nights. Here, engineers move FSS onto a fixture that will allow them to tilt the payload, simulating the pull of lunar gravity in the direction at which one of the instrument's two seismometers is sensitive to motion. (The Moon's gravity is about one-sixth of Earth's.) Called an ambient tilt test, this activity allows engineers to check the seismometers' performance. The two seismometers are packaged together with a large battery, a computer, and electronics inside a cube structure that's surrounded by several layers of insulation and suspended within an outer protective cube, which is in turn covered with a shiny insulating blanket. The suite's single solar panel can be seen right of center. Surrounding the instrument are (from left): Nik Schwarz, Vik Singh, Joanna Farias, and Bert Turney. https://photojournal.jpl.nasa.gov/catalog/PIA26298

NASA's InSight Mars lander detected a giant meteoroid strike on Dec. 24, 2021, the 1,094th Martian day, or sol, of the mission. InSight's seismometer recorded seismic signals that are not in the range of human hearing. In order to make the signals audible, the data was sped up 100 times. Animation available at https://photojournal.jpl.nasa.gov/catalog/PIA25582

NASA's Mars Reconnaissance Orbiter captured this image of a meteoroid impact that was later associated with a seismic event detected by the agency's InSight lander using its seismometer. This crater was formed on May 27, 2020. MRO's Context Camera originally located the impact. Then, the spacecraft's High Resolution Imaging Science Experiment (HiRISE) camera captured this scene in color. The ground is not actually blue; this enhanced-color image highlights certain hues in the scene to make details more visible to the human eye – in this case, dust and soil disturbed by the impact. https://photojournal.jpl.nasa.gov/catalog/PIA25410

An artist's rendition of Mars, highlighting one of InSight's goals -- to figure out just how tectonically active Mars is today and how often meteorites impact it. Interior Exploration using Seismic Investigations, Geodesy and Heat Transport, or InSight, is scheduled to launch from Vandenberg Air Force Base on the California coast between May 5 through June 8, 2018, and land on Mars six months later. InSight will give the Red Planet its first thorough check up since it formed, 4.5 billion years ago. The InSight lander carries a seismometer, SEIS, that listens to the pulse of Mars. The seismometer records the waves traveling through the interior structure of a planet. Studying seismic waves tells us what might be creating the waves. On Mars, scientists suspect that the waves may be caused by marsquakes, meteorites striking the surface, or hot, molten magma moving at great depths underneath the surface. https://photojournal.jpl.nasa.gov/catalog/PIA22230

This is NASA InSight's second full selfie on Mars. Since taking its first selfie, the lander has removed its heat probe and seismometer from its deck, placing them on the Martian surface; a thin coating of dust now covers the spacecraft as well. This selfie is a mosaic made up of 14 images taken on March 15 and April 11 - the 106th and 133rd Martian days, or sols, of the mission - by InSight's Instrument Deployment Camera, located on its robotic arm. InSight's first selfie showed its instruments still on the deck. Now that they're removed, the viewer can see the spacecraft's air pressure sensor (white object in center), the tether box for its seismometer and the tether for its heat probe running across the deck. Also visible is its robotic arm and grapple. https://photojournal.jpl.nasa.gov/catalog/PIA23203

The science deck of NASA's InSight lander is being turned over in this April 29, 2015, photo from InSight assembly and testing operations inside a clean room at Lockheed Martin Space Systems, Denver. The large circular component on the deck is the protective covering to be placed over InSight's seismometer after the seismometer is placed directly onto the Martian ground. InSight, for Interior Exploration Using Seismic Investigations, Geodesy and Heat Transport, is scheduled for launch in March 2016 and landing in September 2016. It will study the deep interior of Mars to advance understanding of the early history of all rocky planets, including Earth. Note: After thorough examination, NASA managers have decided to suspend the planned March 2016 launch of the Interior Exploration using Seismic Investigations Geodesy and Heat Transport (InSight) mission. The decision follows unsuccessful attempts to repair a leak in a section of the prime instrument in the science payload. http://photojournal.jpl.nasa.gov/catalog/PIA19670

NASA's InSight mission tests an engineering version of the spacecraft's robotic arm in a Mars-like environment at NASA's Jet Propulsion Laboratory. The five-fingered grapple on the end of the robotic arm is lifting up the Wind and Thermal Shield, a protective covering for InSight's seismometer. The test is being conducted under reddish "Mars lighting" to simulate activities on the Red Planet. https://photojournal.jpl.nasa.gov/catalog/PIA22806

ForeSight, a fully functional, full-size model of NASA's InSight lander, practices deploying a model of the lander's Wind and Thermal Shield while engineers Phil Bailey (left) and Jaime Singer (center) look on. The Wind and Thermal Shield protects InSight's seismometer. This testing was done at NASA's Jet Propulsion Laboratory in Pasadena, California. Bailey is wearing sunglasses to block the bright yellow lights in the test space, which mimic sunlight as it appears on Mars. https://photojournal.jpl.nasa.gov/catalog/PIA22955

This mosaic, made of 52 individual images from NASA's InSight lander, shows the workspace where the spacecraft will eventually set its science instruments. The workspace is roughly 14 by 7 feet (4 by 2 meters). The lavender annotation shows where InSight's seismometer (called the Seismic Experiment for Interior Structure, or SEIS) and heat flow probe (called the Heat Flow and Physical Properties Package, or HP3) can be placed. https://photojournal.jpl.nasa.gov/catalog/PIA22874

This set of images shows NASA's InSight lander deploying its first instrument onto the surface of Mars, completing a major mission milestone. InSight's robotic arm is white, with a black, handlike grapple at the end. The grapple is holding onto the copper-colored seismometer. The color-calibrated image was taken on Dec. 19, 2018, around dusk on Mars, with InSight's Instrument Deployment Camera (IDC), which is on the lander's robotic arm. Animation available at https://photojournal.jpl.nasa.gov/catalog/PIA22977

NASA's InSight spacecraft flipped open the lens cover on its Instrument Context Camera (ICC) on Nov. 30, 2018, and captured this view of Mars. Located below the deck of the InSight lander, the ICC has a fisheye view, creating a curved horizon. Some clumps of dust are still visible on the camera's lens. One of the spacecraft's footpads can be seen in the lower right corner. The seismometer's tether box is in the upper left corner. https://photojournal.jpl.nasa.gov/catalog/PIA22893

A detail view of the Lunar Environment Monitoring Station, (LEMS) inside the cleanroom at Goddard Space Flight Center, Greenbelt Md., Jan 30, 2026. The Lunar Environment Monitoring Station for Artemis (LEMS) is a compact, autonomous, and self-sustaining seismometer suite designed to carry out continuous, long-term, monitoring of the lunar seismic environment at the South Polar region. Photo Credit: NASA/Mike Guinto

Engineers practice deploying InSight's instruments in a lab at NASA's Jet Propulsion Laboratory in Pasadena, California. Several of them are wearing sunglasses to block the bright yellow lights in the test space, which mimic sunlight as it appears on Mars. The yellow lights are used to test cameras which are the same as those used by InSight on Mars. The entire lab space in the center of the image has been sculpted to mimic the terrain in front of the lander on Mars, creating more reliable test conditions. The area in the center of the image is the "workspace" where the lander's instruments can be set down; wood blocks have been laid down to mark the perimeter of these areas. Rocks have been chosen to match the size, shape and location of those in front of InSight on Mars. In the center of the image is a model of the lander's copper-colored seismometer; at the bottom-right is a second model of the seismometer used for a different kind of testing. In the lower left corner of the image is a bag of crushed granite, which is used in this lab to simulate Martian sand. https://photojournal.jpl.nasa.gov/catalog/PIA22744

NASA's Jet Propulsion Laboratory InSight principal investigator Bruce Banerdt gives remarks during the NASA InSight Mars Lander (Interior Exploration using Seismic Investigations, Geodesy and Heat Transport) media briefing, Wednesday, Oct. 31, 2018 at NASA Headquarters in Washington. InSIght will land on the Red Planet at approximately 3 p.m. EST (noon PST) Monday, Nov. 26. InSight will study the deep interior of Mars to learn how all celestial bodies with rocky surfaces, including Earth and the Moon, formed. The lander’s instruments include a seismometer to detect marsquakes and a probe to monitor the flow of heat in the planet's subsurface. Photo Credit: (NASA/Bill Ingalls)

NASA's Jet Propulsion Laboratory InSight project manager Tom Hoffman gives remarks during a media briefing regarding the NASA InSight Mars Lander (Interior Exploration using Seismic Investigations, Geodesy and Heat Transport), Wednesday, Oct. 31, 2018 at NASA Headquarters in Washington. InSIght will land on the Red Planet at approximately 3 p.m. EST (noon PST) Monday, Nov. 26. InSight will study the deep interior of Mars to learn how all celestial bodies with rocky surfaces, including Earth and the Moon, formed. The lander’s instruments include a seismometer to detect marsquakes and a probe to monitor the flow of heat in the planet's subsurface. Photo Credit: (NASA/Bill Ingalls)

NASA Headquarters acting director of the Planetary Science Division Lori Glaze gives remarks during the NASA InSight Mars Lander (Interior Exploration using Seismic Investigations, Geodesy and Heat Transport) media briefing, Wednesday, Oct. 31, 2018 at NASA Headquarters in Washington. InSIght will land on the Red Planet at approximately 3 p.m. EST (noon PST) Monday, Nov. 26. InSight will study the deep interior of Mars to learn how all celestial bodies with rocky surfaces, including Earth and the Moon, formed. The lander’s instruments include a seismometer to detect marsquakes and a probe to monitor the flow of heat in the planet's subsurface. Photo Credit: (NASA/Bill Ingalls)

NASA's Jet Propulsion Laboratory InSight principal investigator Bruce Banerdt gives remarks during the NASA InSight Mars Lander (Interior Exploration using Seismic Investigations, Geodesy and Heat Transport) media briefing, Wednesday, Oct. 31, 2018 at NASA Headquarters in Washington. InSIght will land on the Red Planet at approximately 3 p.m. EST (noon PST) Monday, Nov. 26. InSight will study the deep interior of Mars to learn how all celestial bodies with rocky surfaces, including Earth and the Moon, formed. The lander’s instruments include a seismometer to detect marsquakes and a probe to monitor the flow of heat in the planet's subsurface. Photo Credit: (NASA/Bill Ingalls)

NASA Administrator Bill Nelson and President of the Centre National d’Etudes Spatiales (CNES) Dr. Philippe Baptiste sign an agreement for the Farside Seismic Suite (FSS), Wednesday, Nov. 30, 2022 at the Mary W. Jackson NASA Headquarters building in Washington. The FSS will return the first lunar seismic data from the far side of the Moon. CNES is contributing one of the seismometers to this payload, which will be delivered via NASA’s Commercial Lunar Payloads Services (CLPS) initiative, based on heritage capabilities from the Mars InSight mission. Photo Credit: (NASA/Keegan Barber)

NASA Administrator Bill Nelson and President of the Centre National d’Etudes Spatiales (CNES) Dr. Philippe Baptiste sign an agreement for the Farside Seismic Suite (FSS), Wednesday, Nov. 30, 2022 at the Mary W. Jackson NASA Headquarters building in Washington. The FSS will return the first lunar seismic data from the far side of the Moon. CNES is contributing one of the seismometers to this payload, which will be delivered via NASA’s Commercial Lunar Payloads Services (CLPS) initiative, based on heritage capabilities from the Mars InSight mission. Photo Credit: (NASA/Keegan Barber)

NASA Administrator Bill Nelson and President of the Centre National d’Etudes Spatiales (CNES) Dr. Philippe Baptiste sign an agreement for the Farside Seismic Suite (FSS), Wednesday, Nov. 30, 2022 at the Mary W. Jackson NASA Headquarters building in Washington. The FSS will return the first lunar seismic data from the far side of the Moon. CNES is contributing one of the seismometers to this payload, which will be delivered via NASA’s Commercial Lunar Payloads Services (CLPS) initiative, based on heritage capabilities from the Mars InSight mission. Photo Credit: (NASA/Keegan Barber)

NASA's Jet Propulsion Laboratory InSight deputy principal investigator Sue Smrekar gives remarks during a NASA InSight Mars Lander (Interior Exploration using Seismic Investigations, Geodesy and Heat Transport) media briefing, Wednesday, Oct. 31, 2018 at NASA Headquarters in Washington. InSIght will land on the Red Planet at approximately 3 p.m. EST (noon PST) Monday, Nov. 26. InSight will study the deep interior of Mars to learn how all celestial bodies with rocky surfaces, including Earth and the Moon, formed. The lander’s instruments include a seismometer to detect marsquakes and a probe to monitor the flow of heat in the planet's subsurface. Photo Credit: (NASA/Bill Ingalls)

During a prelaunch briefing at Vandenberg Air Force Base in California, Annick Sylvestre-Baron, Deputy Project Manager for InSight Seismometer Investigation at CNES, speaks to members of the media. The presentation focused on NASA's Interior Exploration using Seismic Investigations, Geodesy and Heat Transport, or InSight, Mars lander. InSight is scheduled for liftoff May 5, 2018, atop a United Launch Alliance (ULA) Atlas V rocket from Space Launch Complex 3 at Vandenberg. The spacecraft will be the first mission to look deep beneath the Martian surface studying the planet's interior by measuring its heat output and listen for marsquakes.

The flag of the United States stands on the surface of Mars. It is mounted on the housing of NASA's Viking 1's nuclear power system. Also seen are the U.S. Bicentennial symbol and a student designed Viking emblem. The bright flat surface near the center is the seismometer container. This picture was taken on July 23 at about 2:30 p.m. Mars time. The view is west of the spacecraft and includes a series of low hills. The blocky hill in the center appears to be part of a crater rim. The dark, rocky stripes may be material ejected from the crater. The light areas are dune-like and may be accumulations of windblown sand or dust. http://photojournal.jpl.nasa.gov/catalog/PIA00388

NASA Headquarters senior communications official Dwayne Brown moderates a media briefing regarding the NASA InSight Mars Lander (Interior Exploration using Seismic Investigations, Geodesy and Heat Transport), Wednesday, Oct. 31, 2018 at NASA Headquarters in Washington. InSIght will land on the Red Planet at approximately 3 p.m. EST (noon PST) Monday, Nov. 26. InSight will study the deep interior of Mars to learn how all celestial bodies with rocky surfaces, including Earth and the Moon, formed. The lander’s instruments include a seismometer to detect marsquakes and a probe to monitor the flow of heat in the planet's subsurface. Photo Credit: (NASA/Bill Ingalls)

JoAnna Wendel of NASA Headquarters ask questions from the social media during the NASA InSight Mars Lander (Interior Exploration using Seismic Investigations, Geodesy and Heat Transport) media briefing, Wednesday, Oct. 31, 2018 at NASA Headquarters in Washington. InSIght will land on the Red Planet at approximately 3 p.m. EST (noon PST) Monday, Nov. 26. InSight will study the deep interior of Mars to learn how all celestial bodies with rocky surfaces, including Earth and the Moon, formed. The lander’s instruments include a seismometer to detect marsquakes and a probe to monitor the flow of heat in the planet's subsurface. Photo Credit: (NASA/Bill Ingalls)

NASA's Jet Propulsion Laboratory InSight principal investigator Bruce Banerdt gives remarks during the NASA InSight Mars Lander (Interior Exploration using Seismic Investigations, Geodesy and Heat Transport) media briefing, Wednesday, Oct. 31, 2018 at NASA Headquarters in Washington. InSIght will land on the Red Planet at approximately 3 p.m. EST (noon PST) Monday, Nov. 26. InSight will study the deep interior of Mars to learn how all celestial bodies with rocky surfaces, including Earth and the Moon, formed. The lander’s instruments include a seismometer to detect marsquakes and a probe to monitor the flow of heat in the planet's subsurface. Photo Credit: (NASA/Bill Ingalls)

NASA Headquarters senior communications official Dwayne Brown moderates a media briefing regarding the NASA InSight Mars Lander (Interior Exploration using Seismic Investigations, Geodesy and Heat Transport), Wednesday, Oct. 31, 2018 at NASA Headquarters in Washington. InSIght will land on the Red Planet at approximately 3 p.m. EST (noon PST) Monday, Nov. 26. InSight will study the deep interior of Mars to learn how all celestial bodies with rocky surfaces, including Earth and the Moon, formed. The lander’s instruments include a seismometer to detect marsquakes and a probe to monitor the flow of heat in the planet's subsurface. Photo Credit: (NASA/Bill Ingalls)

NASA's Jet Propulsion Laboratory InSight project manager Tom Hoffman gives remarks during a NASA InSight Mars Lander (Interior Exploration using Seismic Investigations, Geodesy and Heat Transport) media briefing, Wednesday, Oct. 31, 2018 at NASA Headquarters in Washington. InSIght will land on the Red Planet at approximately 3 p.m. EST (noon PST) Monday, Nov. 26. InSight will study the deep interior of Mars to learn how all celestial bodies with rocky surfaces, including Earth and the Moon, formed. The lander’s instruments include a seismometer to detect marsquakes and a probe to monitor the flow of heat in the planet's subsurface. Photo Credit: (NASA/Bill Ingalls)

NASA's Jet Propulsion Laboratory InSight deputy principal investigator Sue Smrekar gives remarks during a NASA InSight Mars Lander (Interior Exploration using Seismic Investigations, Geodesy and Heat Transport) media briefing, Wednesday, Oct. 31, 2018 at NASA Headquarters in Washington. InSIght will land on the Red Planet at approximately 3 p.m. EST (noon PST) Monday, Nov. 26. InSight will study the deep interior of Mars to learn how all celestial bodies with rocky surfaces, including Earth and the Moon, formed. The lander’s instruments include a seismometer to detect marsquakes and a probe to monitor the flow of heat in the planet's subsurface. Photo Credit: (NASA/Bill Ingalls)

NASA's Jet Propulsion Laboratory InSight project manager Tom Hoffman gives remarks during a NASA InSight Mars Lander (Interior Exploration using Seismic Investigations, Geodesy and Heat Transport) media briefing, Wednesday, Oct. 31, 2018 at NASA Headquarters in Washington. InSIght will land on the Red Planet at approximately 3 p.m. EST (noon PST) Monday, Nov. 26. InSight will study the deep interior of Mars to learn how all celestial bodies with rocky surfaces, including Earth and the Moon, formed. The lander’s instruments include a seismometer to detect marsquakes and a probe to monitor the flow of heat in the planet's subsurface. Photo Credit: (NASA/Bill Ingalls)

NASA InSight Mars Lander (Interior Exploration using Seismic Investigations, Geodesy and Heat Transport) media briefing, Wednesday, Oct. 31, 2018 at NASA Headquarters in Washington. InSIght will land on the Red Planet at approximately 3 p.m. EST (noon PST) Monday, Nov. 26. InSight will study the deep interior of Mars to learn how all celestial bodies with rocky surfaces, including Earth and the Moon, formed. The lander’s instruments include a seismometer to detect marsquakes and a probe to monitor the flow of heat in the planet's subsurface. Photo Credit: (NASA/Bill Ingalls)

In a clean room at NASA's Jet Propulsion Laboratory in Southern California in March 2024, engineers and technicians work to prepare the agency's Farside Seismic Suite (FSS) for environmental testing to simulate conditions it will encounter in space. Along with being placed in a vacuum chamber and subjected to extreme temperatures, the instrument suite will undergo severe shaking that mimics the rocket's motion during launch. The cube-shaped payload contains two instruments that will gather NASA's first seismic data from the Moon in nearly 50 years and take the first-ever seismic measurements from the Moon's far side. FSS will operate continuously for at least 4½ months, working through the long, cold lunar nights. The two seismometers are packaged together with a large battery, a computer, and electronics inside a cube structure that's surrounded by several layers of insulation and suspended within an outer protective cube, which is in turn covered with a shiny insulating blanket. The suite's single solar panel can be seen at center. On top is a white radiator that will allow the suite to shed heat generated by its electronics during the hot lunar daytime hours. The puck-like object atop the radiator is the suite's antenna, for communicating with two small relay satellites that will orbit the Moon and send data to Earth. Pictured (from left): Joanna Farias, and Bert Turney, and Hsin-Yi Hao. https://photojournal.jpl.nasa.gov/catalog/PIA26299

This seismogram shows the largest quake ever detected on another planet. Estimated at magnitude 5, this quake was discovered by NASA's InSight lander on May 4, 2022, the 1,222nd Martian day, or sol, of the mission. InSight was sent to Mars with a highly sensitive seismometer, provided by France's Centre National d'Études Spatiales (CNES), to study the deep interior of the planet. As seismic waves pass through or reflect off material in Mars' crust, mantle, and core, they change in ways that seismologists can study to determine the depth and composition of these layers. What scientists learn about the structure of Mars can help them better understand the formation of all rocky worlds, including Earth and its Moon. https://photojournal.jpl.nasa.gov/catalog/PIA25180

S71-17610 (4 Feb. 1971) --- Partial view of activity in the Mission Operations Control Room in the Mission Control Center at the time the Apollo 14 S-IVB stage impacted on the lunar surface. The flight director's console is in the foreground. Eugene F. Kranz, chief of the MSC Flight Control Division, is in the right foreground. Seated at the console is Glynn S. Lunney, head of the Flight Director Office, Flight Control Division. Facing the camera is Gerald D. Griffin, flight director of the Third (Gold) Team. A seismic reading from the impact can be seen in the center background. The S-IVB impacted on the lunar surface at 1:40:54 a.m. (CST), Feb. 4, 1971, about 90 nautical miles south-southwest of the Apollo 12 passive seismometer. The energy release was comparable to 11 tons of TNT.

In a clean room at NASA's Jet Propulsion Laboratory in Southern California in March 2024, technician Nik Schwarz prepares the agency's Farside Seismic Suite (FSS) for testing. The cube-shaped payload contains two instruments that will gather NASA's first seismic data from the Moon in nearly 50 years and take the first-ever seismic measurements from the Moon's far side. FSS will operate continuously for at least 4½ months, working through the long, cold lunar nights. The two seismometers are packaged together with a large battery, a computer, and electronics inside a cube structure that's surrounded by several layers of insulation (the shiny, reflective material seen here) and suspended within an outer protective cube, which is in turn covered with a shiny insulating blanket. A technician is here attaching a stiffening brace to the bottom of the FSS outer cube structure. https://photojournal.jpl.nasa.gov/catalog/PIA26341

The craters seen here in blue were formed by a meteoroid impact on Mars on Sept. 5, 2021. The impact was the first to be detected by NASA's InSight mission; the image was taken later by NASA's Mars Reconnaissance Orbiter using its High Resolution Imaging Science Experiment (HiRISE) camera. The initial impact itself created a small marsquake that was detected by InSight's seismometer. The instrument recorded seismological data that showed the moment the meteoroid entered Mars' atmosphere, its explosion into pieces in the atmosphere, and finally, the impact that created a series of at least three craters in the surface. MRO then flew over the approximate site where the impact was "felt" to look for darkened patches of ground using its Context Camera. After finding this location, HiRISE captured the scene in color. The ground is not actually blue; this enhanced-color image highlights certain hues in the scene to make details more visible to the human eye – in this case, dust and soil disturbed by the impact. https://photojournal.jpl.nasa.gov/catalog/PIA25408

S71-17609 (4 Feb. 1971) --- These two individuals are examining a seismic reading in the Mission Control Center's ALSEP Room during the Apollo 14 S-IVB impact on the moon. Dr. Maurice Ewing (left) is the director of the Lamont-Doherty Geological Observatory at Columbia University. David Lammlein, a Columbia graduate student, is on the right. The Apollo 14 Saturn IVB stage impacted on the lunar surface at 1:40:54 a.m. (CST), Feb. 4, 1971, about 90 nautical miles south-southwest of the Apollo 12 passive seismometer. The energy release was comparable to 11 tons of TNT. Dr. Gary Latham of the Lamont-Doherty Geological Observatory is the principal investigator for the Passive Seismic Experiment, a component of the Apollo Lunar Surface Experiments Package.

NASA's Jet Propulsion Laboratory InSight deputy principal investigator Sue Smrekar introduces NASA's Jet Propulsion Laboratory InSight instrument deployment lead Jaime Singer during a media briefing regarding the NASA InSight Mars Lander (Interior Exploration using Seismic Investigations, Geodesy and Heat Transport), Wednesday, Oct. 31, 2018 at NASA Headquarters in Washington. InSIght will land on the Red Planet at approximately 3 p.m. EST (noon PST) Monday, Nov. 26. InSight will study the deep interior of Mars to learn how all celestial bodies with rocky surfaces, including Earth and the Moon, formed. The lander’s instruments include a seismometer to detect marsquakes and a probe to monitor the flow of heat in the planet's subsurface. Photo Credit: (NASA/Bill Ingalls)

This artist's concept shows the InSight lander, its sensors, cameras and instruments. InSight is will take the first-ever-in-depth look at Mars' "inner space." InSight stands for Interior Exploration using Seismic Investigations, Geodesy and Heat Transport. Its three instruments are a seismometer, a heat flow probe, and a radio science experiment. These instruments will shed light on how warm and geologically active Mars still is, study its reflexes as it whips about in its orbit around the sun, and provide essential clues on the evolution of the rocky planets of our solar system. So while InSight is a Mars mission, it's also more than a Mars mission. InSight will launch between May 5 through June 8, 2018 from Vandenberg Air Force Base in California. https://photojournal.jpl.nasa.gov/catalog/PIA22227

This image from InSight's robotic-arm mounted Instrument Deployment Camera shows the instruments on the spacecraft's deck, with the Martian surface of Elysium Planitia in the background. The color-calibrated picture was acquired on Dec. 4, 2018 (Sol 8). In the foreground, a copper-colored hexagonal cover protects the Seismic Experiment for Interior Structure instrument (SEIS), a seismometer that will measure marsquakes. The gray dome behind SEIS is the wind and thermal shield, which will be placed over SEIS. To the left is a black cylindrical instrument, the Heat Flow and Physical Properties Probe (HP3). HP3 will drill up to 16 feet (5 meters) below the Martian surface, measuring heat released from the interior of the planet. Above the deck is InSight's robotic arm, with the stowed grapple directly facing the camera. To the right can be seen a small portion of one of the two solar panels that help power InSight and part of the UHF communication antenna. https://photojournal.jpl.nasa.gov/catalog/PIA22871

This artist's concept shows a cutaway of Mars along with the paths of seismic waves from two separate quakes in 2021. These seismic waves, detected by NASA's InSight mission, were the first ever identified to enter another planet's core. InSight's seismometer allowed scientists to study these waves and gain an unprecedented look at the Martian core. The quakes were detailed in a paper published April 24, 2023, in the Proceedings of the National Academies of Sciences. Occurring on Aug. 25 and Sept. 18, 2021, the two temblors were the first identified by the InSight team to have originated on the opposite side of the planet from the lander – so-called farside quakes. The distance proved crucial: The farther a quake happens from InSight, the deeper into the planet its seismic waves can travel before being detected. https://photojournal.jpl.nasa.gov/catalog/PIA25827

This spectrogram shows the largest quake ever detected on another planet. Estimated at magnitude 5, this quake was discovered by NASA's InSight lander on May 4, 2022, the 1,222nd Martian day, or sol, of the mission. InSight was sent to Mars with a highly sensitive seismometer, provided by France's Centre National d'Études Spatiales (CNES), to study the deep interior of the planet. As seismic waves pass through or reflect off material in Mars' crust, mantle, and core, they change in ways that seismologists can study to determine the depth and composition of these layers. What scientists learn about the structure of Mars can help them better understand the formation of all rocky worlds, including Earth and its Moon. https://photojournal.jpl.nasa.gov/catalog/PIA25044

The HiRISE camera on NASA's Mars Reconnaissance Orbiter got its best view yet of the agency's InSight lander on Sept. 23, 2019. HiRISE has been monitoring InSight's landing site on the Red Planet for changes such as dust-devil tracks (the slightly dark diagonals streaks crisscrossing the surface). This new image clearly shows the two circular solar panels on either side of the lander body. From end to end, the panels span 20 feet (6 meters); the image was taken from an elevation of 169 miles (272 kilometers) above the surface. The bright spot on the lower side of the spacecraft is the dome-shaped protective cover over InSight's seismometer. Surrounding the spacecraft is a dark halo created by retrorocket thrusters scouring the surface during landing. Dark streaks seen crossing diagonally across the surface are dust-devil tracks. Several factors make this image crisper than past images. For one thing, there's less dust in the air this time of year compared to before. And shadows are offset from the lander because this is an oblique view looking west. Moreover, the lighting was better for avoiding the bright reflections from the lander or its solar panels that have obscured surrounding pixels in other images. The seismometer cover to the south of the lander is still bright because its dome shape always produces a mirror-like reflection over some small area. https://photojournal.jpl.nasa.gov/catalog/PIA23376

This map shows the single area under continuing evaluation as the InSight mission's Mars landing site, as of a year before the mission's May 2016 launch. The finalist ellipse marked within the northern portion of flat-lying Elysium Planitia is centered at about 4.5 degrees north latitude and 136 degrees east longitude. InSight -- an acronym for Interior Exploration using Seismic Investigations, Geodesy and Heat Transport -- will study the interior of Mars to improve understanding of the processes that formed and shaped rocky planets, including Earth. The mission's launch period begins March 4, 2016, and lasts until late March. Whichever day during that period the launch occurs, landing is scheduled for Sept. 28, 2016. The landing ellipse on this map covers an area within which the spacecraft has about 99 percent chance of landing when targeted for the center of the ellipse. It is about 81 miles (130 kilometers) long, generally west to east, and about 17 miles (27 kilometers) wide. This ellipse covers the case of a launch at the start of the launch period. If the launch occurs later in the period, orientation of the landing ellipse would shift slightly clockwise. Four semifinalist sites in Elysium Planitia were evaluated as safe for InSight landing. This one was selected as having the largest proportion of its area classified as smooth terrain. If continuing analysis identifies unexpected problems with this site, another of the semifinalists could be reconsidered before final selection later this year. The InSight lander will deploy two instruments directly onto the ground using a robotic arm. One is a seismometer contributed by France's space agency (CNES) with components from Germany, Switzerland, the United Kingdom and the United States. The seismometer will measure microscopic ground motions, providing detailed information about the interior structure of Mars. The other instrument to be deployed by the arm is a heat-flow probe contributed by the German Aerospace Center (DLR), designed to hammer itself three to five meters (about 10 to 16 feet) deep. It will monitor heat coming from the planet's interior. The mission will also track the lander's radio to measure wobbles in the planet's rotation that relate to the size of its core. A suite of environmental sensors will monitor the weather and variations in the magnetic field. The base map is a mosaic of daytime thermal images from the Thermal Emission Imaging System (THEMIS) on NASA's Mars Odyssey orbiter. THEMIS was developed and is operated by Arizona State University, Tempe. Note: After thorough examination, NASA managers have decided to suspend the planned March 2016 launch of the Interior Exploration using Seismic Investigations Geodesy and Heat Transport (InSight) mission. The decision follows unsuccessful attempts to repair a leak in a section of the prime instrument in the science payload. http://photojournal.jpl.nasa.gov/catalog/PIA19143

This video and audio illustrates a seismic event detected by NASA's InSight on April 6, 2019, the 128th Martian day, or sol, of the mission. Three distinct kinds of sounds can be heard, all of them detected as ground vibrations by the spacecraft's seismometer, called the Seismic Experiment for Interior Structure (SEIS): There's noise from Martian wind; the seismic event itself; and the spacecraft's robotic arm as it moves to take pictures. This event is the first likely marsquake recorded by the InSight team. Several other seismic events have been recorded but are much more ambiguous than this signal. The audio underscores just how seismically noisy the Martian surface can be and was produced from two sets of sensors included with SEIS. You can hear sounds from the Very Broad Band sensors from your left speakers and sounds from the Short Period sensors from your right speakers. Audio from both sets of sensors have been sped up by a factor of 60; the actual vibrations on Mars would not have been audible to the human ear. https://photojournal.jpl.nasa.gov/catalog/PIA23176

A camera calibration target sits on the deck of the NASA's InSight lander, adorned with the flags of the countries participating in the mission. The target, which will be viewed by InSight's cameras, provides a variety of colors and shapes to help calibrate the lander's cameras. It also shows off international flags representing the agencies, institutions and participating scientists of the mission as of late 2014 (since that time, Italy has contributed an experiment). In the second row are the United States flag and the logos of NASA, the French space agency CNES, which provided InSight's seismometer; and the German Aerospace Center DLR, which provided InSight's heat flow probe. Below the target in the photo is an Italian experiment called the Laser Retroreflector for InSight (LaRRI). LaRRI is the small, copper-colored dome covered with circles just below the calibration target; it won't actually play a role in InSight's mission. The national space agency of Italy (ASI, for Agenzia Spaziale Italiana) provided LaRRI to be used by a possible future Mars orbiter mission with a laser altimeter making extremely precise measurements of the lander's location for fundamental physics studies and precision cartography. A microchip bearing the names of nearly a million members of the public is visible in this image to the right of the calibration target. A second microchip with more than a million additional names was added after this photo was taken. https://photojournal.jpl.nasa.gov/catalog/PIA22540

In the weeks after NASA's InSight mission reaches Mars in September 2016, the lander's arm will lift two key science instruments off the deck and place them onto the ground. This image shows testing of InSight's robotic arm inside a clean room at NASA's Jet Propulsion Laboratory, Pasadena, California, about two years before it will perform these tasks on Mars. InSight -- an acronym for Interior Exploration using Seismic Investigations, Geodesy and Heat Transport -- will launch in March 2016. It will study the interior of Mars to improve understanding of the processes that formed and shaped rocky planets, including Earth. One key instrument that the arm will deploy is the Seismic Experiment for Interior Structure, or SEIS. It is from France's national space agency (CNES), with components from Germany, Switzerland, the United Kingdom and the United States. In this scene, the arm has just deployed a test model of a protective covering for SEIS, the instrument's wind and thermal shield. The shield's purpose is to lessen disturbances that weather would cause to readings from the sensitive seismometer. Note: After thorough examination, NASA managers have decided to suspend the planned March 2016 launch of the Interior Exploration using Seismic Investigations Geodesy and Heat Transport (InSight) mission. The decision follows unsuccessful attempts to repair a leak in a section of the prime instrument in the science payload. http://photojournal.jpl.nasa.gov/catalog/PIA19144

NASA's Jet Propulsion Laboratory InSight instrument deployment lead Jaime Singer, on screen, NASA's Jet Propulsion Laboratory InSight deputy principal investigator Sue Smrekar, left, NASA's Jet Propulsion Laboratory InSight principal investigator Bruce Banerdt, NASA's Jet Propulsion Laboratory InSight project manager Tom Hoffman, and NASA Headquarters acting director of the Planetary Science Division Lori Glaze, right, discuss the NASA InSight Mars Lander (Interior Exploration using Seismic Investigations, Geodesy and Heat Transport) during media briefing, Wednesday, Oct. 31, 2018 at NASA Headquarters in Washington. InSIght will land on the Red Planet at approximately 3 p.m. EST (noon PST) Monday, Nov. 26. InSight will study the deep interior of Mars to learn how all celestial bodies with rocky surfaces, including Earth and the Moon, formed. The lander’s instruments include a seismometer to detect marsquakes and a probe to monitor the flow of heat in the planet's subsurface. Photo Credit: (NASA/Bill Ingalls)

In a clean room at NASA's Jet Propulsion Laboratory in Southern California in March 2024, engineers and technicians pose with the agency's Farside Seismic Suite while the payload is readied for testing. The suite contains two instruments that will gather NASA's first seismic data from the Moon in nearly 50 years and take the first-ever seismic measurements from the Moon's far side. FSS will operate continuously for at least 4½ months, working through the long, cold lunar nights. The two seismometers are packaged together with a large battery, a computer, and electronics inside a cube structure that's surrounded by several layers of insulation (the shiny material at center) and suspended within a protective outer cube, which is, in turn, covered with an insulating blanket. In this photo, the blanket has not yet been attached. Members of the FSS integration team pictured are (from left) Salvador Ramirez, Asad Aboobaker, Nik Schwarz, Joanna Farias, Clara MacFarland, Frank Barone, Hsin-Yi Hao, Nicholas Roy-Steier, and Vik Singh. https://photojournal.jpl.nasa.gov/catalog/PIA26342

This not-to-scale artist's concept depicts a cutaway view of Mars' interior, revealing the crust, mantle, and core. Debris from ancient impacts lies scattered in the mantle in the form of lumps that are as large as 2.5 miles (4 kilometers) across, data from NASA's InSight Mars lander shows. On the Martian surface at left, a meteoroid impact sends seismic signals (shown as curving concentric lines) through the planet; InSight is depicted at right. InSight placed the first seismometer on Mars' surface in 2018. The extremely sensitive instrument recorded 1,319 marsquakes before the lander ran out of power in 2022, the result of dust caked on its solar panels. Quakes produce seismic waves that change as they pass through different kinds of material, providing scientists with a way to study the interior of a planetary body. To date, the InSight team has measured the size, depth, and composition of Mars' crust, mantle, and core. The impact debris in the Martian mantle offers a geologic record that could be preserved only on worlds like Mars, whose lack of tectonic plates has kept its interior from being churned up the way Earth's is through a process known as convection. https://photojournal.jpl.nasa.gov/catalog/PIA26636

This artist's concept from August 2015 depicts NASA's InSight Mars lander fully deployed for studying the deep interior of Mars. This illustration updates the correct placement and look of Insight's main instruments. For an earlier artist rendition, see PIA17358. InSight, short for Interior Exploration using Seismic Investigations, Geodesy and Heat Transport, will investigate processes that formed and shaped Mars. Its findings will improve understanding about the evolution of our inner solar system's rocky planets, including Earth. The lander will be the first mission to permanently deploy instruments directly onto Martian ground using a robotic arm. The two instruments to be placed into a work area in front of the lander are a seismometer (contributed by the French space agency Centre National d'Études Spatiales, or CNES) to measure the microscopic ground motions from distant marsquakes providing information about the interior structure of Mars, and a heat-flow probe (contributed by the German Aerospace Center, or DLR) designed to hammer itself 3 to 5 meters (about 16 feet) deep and monitor heat coming from the planet's interior. The mission will also track the lander's radio to measure wobbles in the planet's rotation that relate to the size of its core and a suite of environmental sensors to monitor the weather and variations in the magnetic field. Two cameras will aid in instrument deployment and monitoring the local environment. Note: After thorough examination, NASA managers have decided to suspend the planned March 2016 launch of the Interior Exploration using Seismic Investigations Geodesy and Heat Transport (InSight) mission. The decision follows unsuccessful attempts to repair a leak in a section of the prime instrument in the science payload. http://photojournal.jpl.nasa.gov/catalog/PIA19811

This artist's concept depicts the stationary NASA Mars lander known by the acronym InSight at work studying the interior of Mars. The InSight mission (for Interior Exploration using Seismic Investigations, Geodesy and Heat Transport) is scheduled to launch in March 2016 and land on Mars six months later. It will investigate processes that formed and shaped Mars and will help scientists better understand the evolution of our inner solar system's rocky planets, including Earth. InSight will deploy two instruments to the ground using a robotic arm: a seismometer (contributed by the French space agency Centre National d'Etudes Spatiales, or CNES) to measure the microscopic ground motions from distant marsquakes, providing detailed information about the interior structure of Mars; and a heat-flow probe (contributed by the German Aerospace Center, or DLR) designed to hammer itself 3 to 5 meters (about 16 feet) deep and monitor heat coming from the planet's interior. The mission will also track the lander's radio to measure wobbles in the planet's rotation that relate to the size of its core and will include a camera and a suite of environmental sensors to monitor the weather and variations in the magnetic field. Lockheed Martin Space Systems, Denver, is building the spacecraft. Note: After thorough examination, NASA managers have decided to suspend the planned March 2016 launch of the Interior Exploration using Seismic Investigations Geodesy and Heat Transport (InSight) mission. The decision follows unsuccessful attempts to repair a leak in a section of the prime instrument in the science payload. http://photojournal.jpl.nasa.gov/catalog/PIA17358

After decades of uncertainty, the Apollo 16 S-IVB impact site on the lunar surface has been identified. S-IVBs were portions of the Saturn V rockets that brought astronauts to the moon. The site was identified in imagery from the high-resolution LROC Narrow Angle Camera aboard NASA's Lunar Reconnaissance Orbiter. Beginning with Apollo 13, the S-IVB rocket stages were deliberately impacted on the lunar surface after they were used. Seismometers placed on the moon by earlier Apollo astronauts measured the energy of these impacts to shed light on the internal lunar structure. Locations of the craters that the boosters left behind were estimated from tracking data collected just prior to the impacts. Earlier in the LRO mission, the Apollo 13, 14, 15 and 17 impact sites were successfully identified, but Apollo 16's remained elusive. In the case of Apollo 16, radio contact with the booster was lost before the impact, so the location was only poorly known. Positive identification of the Apollo 16 S-IVB site took more time than the other four impact craters because the location ended up differing by about 30 km (about 19 miles) from the Apollo-era tracking estimate. (For comparison, the other four S-IVB craters were all within 7 km -- about four miles -- of their estimated locations.) Apollo 16's S-IVB stage is on Mare Insularum, about 160 miles southwest of Copernicus Crater (more precisely: 1.921 degrees north, 335.377 degrees east, minus 1,104 meters elevation). Credit: NASA/Goddard/Arizona State University <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 view looks upward toward the InSight Mars lander suspended upside down. It shows the top of the lander's science deck with the mission's two main science instruments -- the Seismic Experiment for Interior Structure (SEIS) and the Heat Flow and Physical Properties Probe (HP3) -- plus the robotic arm and other subsystems installed. The photo was taken Aug. 9, 2017, in a Lockheed Martin clean room facility in Littleton, Colorado. The InSight mission (for Interior Exploration using Seismic Investigations, Geodesy and Heat Transport) is scheduled to launch in May 2018 and land on Mars Nov. 26, 2018. It will investigate processes that formed and shaped Mars and will help scientists better understand the evolution of our inner solar system's rocky planets, including Earth. https://photojournal.jpl.nasa.gov/catalog/PIA21847