
NASA's Morpheus Project has developed and tested a prototype planetary lander capable of vertical takeoff and landing. This is an image of the lander being installed in the B-2 facility for testing at Plum Brook Station.

Engineers at NASA's Jet Propulsion Laboratory – from left, Matthew Cameron-Hooper, and Thomas Reynoso – prepare flight-like landing gear in the Europa Lander landing gear testbed in summer 2022. Europa Lander is a concept for a potential future mission that would look for signs of life in the icy surface material of Jupiter's moon Europa. The moon is thought to contain a global ocean of salty water beneath its frozen crust. If life exists in that ocean, signs of its existence called biosignatures could potentially find their way to the surface. In this mission concept, a spacecraft would land on Europa and collect and study samples from about 4 inches (10 centimeters) beneath the surface, looking for signs of life. The Europa Lander landing gear testbed was developed to test and inform the design of the landing gear for the spacecraft: It mimics the landing loads and ground interaction forces that a single flight landing gear would experience when touching down on the Europan surface. It does this by using gravity offloading to simulate the reduced gravity on Europa, and by replicating the mass and inertial properties of a flight lander as well as all the degrees of freedom that the landing gear would experience. https://photojournal.jpl.nasa.gov/catalog/PIA26198

The solar arrays on NASA's InSight Mars lander were deployed as part of testing conducted Jan. 23, 2018, at Lockheed Martin Space in Littleton, Colorado. Engineers and technicians evaluated the solar arrays and performed an illumination test to confirm that the solar cells were collecting power. The launch window for InSight opens May 5, 2018. A video is available at https://photojournal.jpl.nasa.gov/catalog/PIA22205

While in the landed configuration for the last time before arriving on Mars, NASA's InSight lander was commanded to deploy its solar arrays to test and verify the exact process that it will use on the surface of the Red Planet. During the test on Jan. 23, 2018 from the Lockheed Martin clean room in Littleton, Colorado, engineers and technicians evaluated that the solar arrays fully deployed and conducted an illumination test to confirm that the solar cells were collecting power. A video is available at https://photojournal.jpl.nasa.gov/catalog/PIA22203

While in the landed configuration for the last time before arriving on Mars, NASA's InSight lander was commanded to deploy its solar arrays to test and verify the exact process that it will use on the surface of the Red Planet. During the test on Jan. 23, 2018 from the Lockheed Martin clean room in Littleton, Colorado, engineers and technicians evaluated that the solar arrays fully deployed and conducted an illumination test to confirm that the solar cells were collecting power. A video is available at https://photojournal.jpl.nasa.gov/catalog/PIA22202

While in the landed configuration for the last time before arriving on Mars, NASA's InSight lander was commanded to deploy its solar arrays to test and verify the exact process that it will use on the surface of the Red Planet. During the test on Jan. 23, 2018 from the Lockheed Martin clean room in Littleton, Colorado, engineers and technicians evaluated that the solar arrays fully deployed and conducted an illumination test to confirm that the solar cells were collecting power. A video is available at https://photojournal.jpl.nasa.gov/catalog/PIA22201

While in the landed configuration for the last time before arriving on Mars, NASA's InSight lander was commanded to deploy its solar arrays to test and verify the exact process that it will use on the surface of the Red Planet. During the test on Jan. 23, 2018 from the Lockheed Martin clean room in Littleton, Colorado, engineers and technicians evaluated that the solar arrays fully deployed and conducted an illumination test to confirm that the solar cells were collecting power. A video is available at https://photojournal.jpl.nasa.gov/catalog/PIA22200

While in the landed configuration for the last time before arriving on Mars, NASA's InSight lander was commanded to deploy its solar arrays to test and verify the exact process that it will use on the surface of the Red Planet. During the test on Jan. 23, 2018 from the Lockheed Martin clean room in Littleton, Colorado, engineers and technicians evaluated that the solar arrays fully deployed and conducted an illumination test to confirm that the solar cells were collecting power. A video is available at https://photojournal.jpl.nasa.gov/catalog/PIA22204

Locating Landers on Mars
Phoenix Lander Work Area
Looking Westward at the Lander
Mars Polar Lander NOT Found

Pathfinder Landers - In Test and On Mars
Underneath the Phoenix Lander

NASA's Lunar Lander exhibit is located at the Mississippi I-10 Welcome Center in Hancock County, Miss., just west of Bay St. Louis and 45 miles east of New Orleans on I-10 at Exit 2. The exhibit features a 30-foot-tall replica of a Lunar Lander used as a trainer by the Apollo 13 astronauts. Apollo 13 astronaut and Mississippi native Fred Haise left space-boot prints and signature in concrete at the base of the exhibit.

Engineer Matthew Cameron-Hooper performs a checkout on some systems of the Europa Lander landing gear testbed at NASA's Jet Propulsion Laboratory in Southern California on May 27, 2022. Europa Lander is a concept for a potential future mission that would look for signs of life in the icy surface material of Jupiter's moon Europa. The moon is thought to contain a global ocean of salty water beneath its frozen crust. If life exists in that ocean, signs of its existence called biosignatures could potentially find their way to the surface. In this mission concept, a spacecraft would land on Europa and collect and study samples from about 4 inches (10 centimeters) beneath the surface, looking for signs of life. The Europa Lander landing gear testbed was developed to test and inform the design of the landing gear for the spacecraft: It mimics the landing loads and ground interaction forces that a single flight landing gear would experience when touching down on the Europan surface. It does this by using gravity offloading to simulate the reduced gravity on Europa, and by replicating the mass and inertial properties of a flight lander as well as all the degrees of freedom that the landing gear would experience. This system checkout confirmed two critical functionalities of the testbed: low friction of the horizontal degree of freedom that carries the test landing gear, and proper functioning of the gravity offloading system. Together these functionalities ensure that only ground interaction forces cause the test landing gear to come to a stop during a test, just as a flight landing gear would experience when landing on the Europan surface. Video available at https://photojournal.jpl.nasa.gov/catalog/PIA26200

Nathaniel Brown, a mechanical design engineer, works the structure design and interfaces for the Lunar Pallet Lander.

On December 3, 1999) Mars Polar Lander (MPL) was set to touchdown on the enigmatic layered terrain located near the South Pole. Unfortunately, communications with the spacecraft were lost and never regained. The Mars Program Independent Assessment Team concluded that this loss was most likely due to premature retrorocket shutdown resulting in the crash of the lander. The image primarily shows what appears to be a ridged surface with some small isolated hills. Historically, exploration has and will continue to be a very hard and risky endeavor and sometimes you lose. But the spirit of exploration and discovery has served mankind well throughout the ages and it has now driven us to the far reaches of space. Therefore, with this in mind the THEMIS Team today is releasing an image of the region where MPL was set to land in memory of this mission and the unquenchable spirit of exploration. It is hoped that in the near future we will once again attempt another landing in the Martian polar regions. http://photojournal.jpl.nasa.gov/catalog/PIA04016

Lisa Watson-Morgan, center left, program manager of NASA’s Human Landing System Program at NASA’s Marshall Space Flight Center in Huntsville, Alabama, shows NASA Administrator Jim Bridenstine equipment used to test seismic sensors on a lunar lander platform on a simulated lunar surface at the center Aug. 16, 2019. Bridenstine was joined by Representatives Mo Brooks and Robert Aderholt of Alabama and Representative Scott DesJarlais of Tennessee. Planetary scientists performed the experiment to learn how these waves travel through simulated regolith, which is material similar to the Moon’s surface. The experiment will help guide instrument deployment scenarios for NASA’s Commercial Lunar Payload Service (CLPS) Program, delivering small science and technology payloads for Artemis. That same day, Bridenstine announced Marshall will lead the agency’s Human Landing System Program. (NASA/Fred Deaton) For more information: https://www.nasa.gov/artemis-1
Sunset at the Viking Lander 1 Site

Big Crater as Viewed by Pathfinder Lander
Frost at the Viking Lander 2 Site
Martian Surface Beneath Phoenix Lander
Sojourner Rover View of Pathfinder Lander

Mars Polar Lander: The Search Continues

Mars Polar Lander: The Search Begins

Rock Moved by Mars Lander Arm
Rover Camera Mosaic of Lander & Wedge

Panoramic View of Lander During Turn

Plains West of Viking Lander 2

Fish Eye View of Horizon and Lander

On Aug. 16, 2019, NASA Administrator Jim Bridenstine announced the agency’s Marshall Space Flight Center in Huntsville, Alabama, will lead the Human Landing System Program. Bridenstine was joined by Representatives Mo Brooks and Robert Aderholt of Alabama and Representative Scott DesJarlais of Tennessee. NASA will rapidly develop the lander for safely carrying the first woman and the next man to the Moon’s surface in 2024. The Artemis missions will start with launch by the world’s most powerful rocket, NASA’s Space Launch System, also managed by Marshall. Bridenstine made the announcement in front of the 149-foot-tall SLS liquid hydrogen structural test article, currently being tested to help ensure the structure can safely launch astronauts on the Artemis lunar missions. (NASA/Fred Deaton) For more information: https://www.nasa.gov/artemis-1

IM-1, the first NASA Commercial Launch Program Services launch for Intuitive Machines’ Nova-C lunar lander, will carry multiple payloads to the Moon, including Lunar Node-1, demonstrating autonomous navigation via radio beacon to support precise geolocation and navigation among lunar orbiters, landers, and surface personnel. NASA’s CLPS initiative oversees industry development of small robotic landers and rovers to support NASA’s Artemis campaign.
The Meteorology Instrument on Viking Lander 1 http://photojournal.jpl.nasa.gov/catalog/PIA00392
Viking Lander Buried Footpad #3 http://photojournal.jpl.nasa.gov/catalog/PIA00390

A Martian mechanic checks beneath the completely deployed NASA Rover 1 lander. Atop the lander is Rover 1 with its wheels and solar arrays in the stowed position.

The Philae lander of the European Space Agency Rosetta mission is safely on the surface of Comet 67P/Churyumov-Gerasimenko, as these first two images from the lander CIVA camera confirm. One of the lander three feet can be seen in the foreground.

Environmental portrait of Renee Weber, commemorating her recent transition to the MSFC Chief Scientist position. Pictured with lunar lander models in the lander lab building 4747.

Environmental portrait of Renee Weber, commemorating her recent transition to the MSFC Chief Scientist position. Pictured with lunar lander models in the lander lab building 4747.

This is one of two images taken nearly a decade apart of NASA's Mars Phoenix Lander and related hardware around the mission's May 25, 2008, landing site on far-northern Mars. By late 2017, dust had obscured much of what was visible two months after the landing. Both images were taken by the High Resolution Imaging Science Experiment (HiRISE) camera on NASA's Mars Reconnaissance Orbiter. The one with three patches of darker ground -- where landing events removed dust -- was taken on July 20, 2008. It is Fig. 1, an excerpt of HiRISE observation PSP_009290_2485. The one with a more even coating of pale dust throughout the area was taken on Dec. 21, 2017. It is Fig. 2, an excerpt of HiRISE observation ESP_053451_2485. Both cover an area roughly 300 meters wide at 68 degrees north latitude, 234 degrees east longitude, and the two are closely matched in viewing and illumination geometry, from about five Martian years apart in northern hemisphere summers. An animation comparing the two images shows a number of changes between mid-2008 and late 2017. The lander (top) appears darker, and is now covered by dust. The dark spot created by the heat shield impact (right) is brighter, again due to dust deposition. The back shell and parachute (bottom) shows a darker parachute and brighter area of impact disturbance, thanks again to deposits of dust. We also see that the parachute has shifted in the wind, moving to the east. In August 2008, Phoenix completed its three-month mission studying Martian ice, soil and atmosphere. The lander worked for two additional months before reduced sunlight caused energy to become insufficient to keep the lander functioning. The solar-powered robot was not designed to survive through the dark and cold conditions of a Martian arctic winter. An animation and both images are available at https://photojournal.jpl.nasa.gov/catalog/PIA22223
This graphic shows a possible robotic lander for a future mission to Jupiter moon Europa.
The Phoenix lander, housed in a 100,000-class clean room at Lockheed Martin Space Systems facilities near Denver, Colo. Shown here, the lander is contained inside the backshell portion of the aeroshell with the heat shield removed.
Vivid Colors of the Viking Lander 1 Scene

La Mancha Trench Dug by Phoenix Mars Lander

Phoenix Lander Self Portrait on Mars, Vertical Projection
First Color Image of the Viking Lander 2 Site
Viking Lander 1 U.S. Flag on Mars Surface
Mars Polar Lander Site Compared With Washington, D.C.

Phoenix Lander on Mars with Surrounding Terrain, Vertical Projection

MGS MOC Coverage of Mars Polar Lander Region

Mars Polar Lander and Mars Pathfinder Sites Compared
First Color Image From Viking Lander 1
Potential Ice Table Under Lander Imaged

Mars Polar Lander Landing Zone Compared With JPL
Underneath Phoenix Lander 97 Sols After Touchdown
Mars Surface near Viking Lander 1 Footpad
Mars Polar Lander Site Surface Details

Connecting the Dots: Lander, Heat Shield, Parachute

Mars Polar Lander Landing Zone Compared With JPL

Engineers test the mechanical landing system for the proposed Europa Lander project at NASA's Jet Propulsion Laboratory on Sept. 15, 2022. This test, using the Europa Lander landing gear testbed, fully exercises the Europa Lander landing gear mechanism through a simulated dynamic landing. Europa Lander is a concept for a potential future mission that would look for signs of life in the icy surface material of Jupiter's moon Europa. The moon is thought to contain a global ocean of salty water beneath its frozen crust. If life exists in that ocean, signs of its existence called biosignatures could potentially find their way to the surface. In this mission concept, a spacecraft would land on Europa and collect and study samples from about 4 inches (10 centimeters) beneath the surface, looking for signs of life. The Europa Lander landing gear testbed was developed to test and inform the design of the landing gear for the spacecraft: It mimics the landing loads and ground interaction forces that a single flight landing gear would experience when touching down on the Europan surface. It does this by using gravity offloading to simulate the reduced gravity on Europa, and by replicating the mass and inertial properties of a flight lander as well as all the degrees of freedom that the landing gear would experience. Video available at https://photojournal.jpl.nasa.gov/catalog/PIA26199

The descent of its comet lander Philae was captured by ESA Rosetta spacecraft main camera as the lander approached -- and then rebounded off -- the comet surface.

The Philae lander of the European Space Agency Rosetta mission took this parting shot of its mother ship, Rosetta, shortly after separation on Nov. 12, 2014. The image was taken with the lander CIVA-P imaging system.

Near the lower left corner of this view is the three-petal lander platform that NASA Mars Exploration Rover Spirit drove off in January 2004. The lander is still bright, but with a reddish color, probably due to accumulation of Martian dust.

In the Payload Hazardous Servicing Facility, technicians lower a crane over the Phoenix Mars Lander spacecraft. The crane will be used to remove the heat shield from around the Phoenix. The Phoenix mission is the first project in NASA's first openly competed program of Mars Scout missions. Phoenix will land in icy soils near the north polar permanent ice cap of Mars and explore the history of the water in these soils and any associated rocks, while monitoring polar climate. Landing is planned in May 2008 on arctic ground where a mission currently in orbit, Mars Odyssey, has detected high concentrations of ice just beneath the top layer of soil. It will serve as NASA's first exploration of a potential modern habitat on Mars and open the door to a renewed search for carbon-bearing compounds, last attempted with NASA’s Viking missions in the 1970s. A stereo color camera and a weather station will study the surrounding environment while the other instruments check excavated soil samples for water, organic chemicals and conditions that could indicate whether the site was ever hospitable to life. Microscopes can reveal features as small as one one-thousandth the width of a human hair. Launch of Phoenix aboard a Delta II rocket is targeted for Aug. 3 from Cape Canaveral Air Force Station in Florida.

In the Payload Hazardous Servicing Facility, technicians attach a crane to the Phoenix Mars Lander spacecraft. The crane will be used to remove the heat shield from around the Phoenix. The Phoenix mission is the first project in NASA's first openly competed program of Mars Scout missions. Phoenix will land in icy soils near the north polar permanent ice cap of Mars and explore the history of the water in these soils and any associated rocks, while monitoring polar climate. Landing is planned in May 2008 on arctic ground where a mission currently in orbit, Mars Odyssey, has detected high concentrations of ice just beneath the top layer of soil. It will serve as NASA's first exploration of a potential modern habitat on Mars and open the door to a renewed search for carbon-bearing compounds, last attempted with NASA’s Viking missions in the 1970s. A stereo color camera and a weather station will study the surrounding environment while the other instruments check excavated soil samples for water, organic chemicals and conditions that could indicate whether the site was ever hospitable to life. Microscopes can reveal features as small as one one-thousandth the width of a human hair. Launch of Phoenix aboard a Delta II rocket is targeted for Aug. 3 from Cape Canaveral Air Force Station in Florida.
The Collector Head Of Viking Lander 1 Surface Sampler http://photojournal.jpl.nasa.gov/catalog/PIA00395
Viking Lander 2 First Picture On The Surface Of Mars http://photojournal.jpl.nasa.gov/catalog/PIA00396

This panorama of the region to the northeast of the lander was constructed to support the Sojourner Rover Team's plans to conduct an "autonomous traverse" to explore the terrain away from the lander after science objectives in the lander vicinity had been met. The large, relatively bright surface in the foreground, about 10 meters (33 feet) from the spacecraft, in this scene is "Baker's Bench." The large, elongated rock left of center in the middle distance is "Zaphod." This view was produced by combining 8 individual "Superpan" scenes from the left and right eyes of the IMP camera. Each frame consists of 8 individual frames (left eye) and 7 frames (right eye) taken with different color filters that were enlarged by 500% and then co-added using Adobe Photoshop to produce, in effect, a super-resolution panchromatic frame that is sharper than an individual frame would be. http://photojournal.jpl.nasa.gov/catalog/PIA01000

NASA Rover 1 sits atop the deployed lander with its solar arrays and wheels stowed.
Lander and Mini

An overhead crane lifts the backshell with the Phoenix Mars Lander inside off its work stand in the Payload Hazardous Servicing Facility. The spacecraft is being moved to a spin table (back left) for spin testing. The Phoenix mission is the first project in NASA's first openly competed program of Mars Scout missions. Phoenix will land in icy soils near the north polar permanent ice cap of Mars and explore the history of the water in these soils and any associated rocks, while monitoring polar climate. Landing is planned in May 2008 on arctic ground where a mission currently in orbit, Mars Odyssey, has detected high concentrations of ice just beneath the top layer of soil. It will serve as NASA's first exploration of a potential modern habitat on Mars and open the door to a renewed search for carbon-bearing compounds, last attempted with NASA’s Viking missions in the 1970s. A stereo color camera and a weather station will study the surrounding environment while the other instruments check excavated soil samples for water, organic chemicals and conditions that could indicate whether the site was ever hospitable to life. Microscopes can reveal features as small as one one-thousandth the width of a human hair. Launch of Phoenix aboard a Delta II rocket is targeted for Aug. 3 from Cape Canaveral Air Force Station in Florida.

In the Payload Hazardous Servicing Facility, an overhead crane lifts the heat shield from the Phoenix Mars Lander spacecraft. The Phoenix mission is the first project in NASA's first openly competed program of Mars Scout missions. Phoenix will land in icy soils near the north polar permanent ice cap of Mars and explore the history of the water in these soils and any associated rocks, while monitoring polar climate. Landing is planned in May 2008 on arctic ground where a mission currently in orbit, Mars Odyssey, has detected high concentrations of ice just beneath the top layer of soil. It will serve as NASA's first exploration of a potential modern habitat on Mars and open the door to a renewed search for carbon-bearing compounds, last attempted with NASA’s Viking missions in the 1970s. A stereo color camera and a weather station will study the surrounding environment while the other instruments check excavated soil samples for water, organic chemicals and conditions that could indicate whether the site was ever hospitable to life. Microscopes can reveal features as small as one one-thousandth the width of a human hair. Launch of Phoenix aboard a Delta II rocket is targeted for Aug. 3 from Cape Canaveral Air Force Station in Florida.

In the Payload Hazardous Servicing Facility, the Phoenix Mars Lander (foreground) can be seen inside the backshell. In the background, workers are helping place the heat shield, just removed from the Phoenix, onto a platform. The Phoenix mission is the first project in NASA's first openly competed program of Mars Scout missions. Phoenix will land in icy soils near the north polar permanent ice cap of Mars and explore the history of the water in these soils and any associated rocks, while monitoring polar climate. Landing is planned in May 2008 on arctic ground where a mission currently in orbit, Mars Odyssey, has detected high concentrations of ice just beneath the top layer of soil. It will serve as NASA's first exploration of a potential modern habitat on Mars and open the door to a renewed search for carbon-bearing compounds, last attempted with NASA’s Viking missions in the 1970s. A stereo color camera and a weather station will study the surrounding environment while the other instruments check excavated soil samples for water, organic chemicals and conditions that could indicate whether the site was ever hospitable to life. Microscopes can reveal features as small as one one-thousandth the width of a human hair. Launch of Phoenix aboard a Delta II rocket is targeted for Aug. 3 from Cape Canaveral Air Force Station in Florida.

An overhead crane lowers the backshell with the Phoenix Mars Lander inside toward a spin table for spin testing in the Payload Hazardous Servicing Facility. The Phoenix mission is the first project in NASA's first openly competed program of Mars Scout missions. Phoenix will land in icy soils near the north polar permanent ice cap of Mars and explore the history of the water in these soils and any associated rocks, while monitoring polar climate. Landing is planned in May 2008 on arctic ground where a mission currently in orbit, Mars Odyssey, has detected high concentrations of ice just beneath the top layer of soil. It will serve as NASA's first exploration of a potential modern habitat on Mars and open the door to a renewed search for carbon-bearing compounds, last attempted with NASA’s Viking missions in the 1970s. A stereo color camera and a weather station will study the surrounding environment while the other instruments check excavated soil samples for water, organic chemicals and conditions that could indicate whether the site was ever hospitable to life. Microscopes can reveal features as small as one one-thousandth the width of a human hair. Launch of Phoenix aboard a Delta II rocket is targeted for Aug. 3 from Cape Canaveral Air Force Station in Florida.

In the Payload Hazardous Servicing Facility, workers help guide the heat shield onto a platform. The heat shield was removed from the Phoenix Mars Lander spacecraft.. The Phoenix mission is the first project in NASA's first openly competed program of Mars Scout missions. Phoenix will land in icy soils near the north polar permanent ice cap of Mars and explore the history of the water in these soils and any associated rocks, while monitoring polar climate. Landing is planned in May 2008 on arctic ground where a mission currently in orbit, Mars Odyssey, has detected high concentrations of ice just beneath the top layer of soil. It will serve as NASA's first exploration of a potential modern habitat on Mars and open the door to a renewed search for carbon-bearing compounds, last attempted with NASA’s Viking missions in the 1970s. A stereo color camera and a weather station will study the surrounding environment while the other instruments check excavated soil samples for water, organic chemicals and conditions that could indicate whether the site was ever hospitable to life. Microscopes can reveal features as small as one one-thousandth the width of a human hair. Launch of Phoenix aboard a Delta II rocket is targeted for Aug. 3 from Cape Canaveral Air Force Station in Florida.

This closeup shows the spin test of the Phoenix Mars Lander in the Payload Hazardous Servicing Facility. The Phoenix mission is the first project in NASA's first openly competed program of Mars Scout missions. Phoenix will land in icy soils near the north polar permanent ice cap of Mars and explore the history of the water in these soils and any associated rocks, while monitoring polar climate. Landing is planned in May 2008 on arctic ground where a mission currently in orbit, Mars Odyssey, has detected high concentrations of ice just beneath the top layer of soil. It will serve as NASA's first exploration of a potential modern habitat on Mars and open the door to a renewed search for carbon-bearing compounds, last attempted with NASA’s Viking missions in the 1970s. A stereo color camera and a weather station will study the surrounding environment while the other instruments check excavated soil samples for water, organic chemicals and conditions that could indicate whether the site was ever hospitable to life. Microscopes can reveal features as small as one one-thousandth the width of a human hair. Launch of Phoenix aboard a Delta II rocket is targeted for Aug. 3 from Cape Canaveral Air Force Station in Florida.

This closeup shows the Phoenix Mars Lander spacecraft nestled inside the backshell. The spacecraft is ready for spin testing on the spin table to which it is attached in the Payload Hazardous Servicing Facility. The Phoenix mission is the first project in NASA's first openly competed program of Mars Scout missions. Phoenix will land in icy soils near the north polar permanent ice cap of Mars and explore the history of the water in these soils and any associated rocks, while monitoring polar climate. Landing is planned in May 2008 on arctic ground where a mission currently in orbit, Mars Odyssey, has detected high concentrations of ice just beneath the top layer of soil. It will serve as NASA's first exploration of a potential modern habitat on Mars and open the door to a renewed search for carbon-bearing compounds, last attempted with NASA’s Viking missions in the 1970s. A stereo color camera and a weather station will study the surrounding environment while the other instruments check excavated soil samples for water, organic chemicals and conditions that could indicate whether the site was ever hospitable to life. Microscopes can reveal features as small as one one-thousandth the width of a human hair. Launch of Phoenix aboard a Delta II rocket is targeted for Aug. 3 from Cape Canaveral Air Force Station in Florida.

In the Payload Hazardous Servicing Facility, workers watch as an overhead crane lowers the heat shield toward a platform. The heat shield was removed from the Phoenix Mars Lander spacecraft. The Phoenix mission is the first project in NASA's first openly competed program of Mars Scout missions. Phoenix will land in icy soils near the north polar permanent ice cap of Mars and explore the history of the water in these soils and any associated rocks, while monitoring polar climate. Landing is planned in May 2008 on arctic ground where a mission currently in orbit, Mars Odyssey, has detected high concentrations of ice just beneath the top layer of soil. It will serve as NASA's first exploration of a potential modern habitat on Mars and open the door to a renewed search for carbon-bearing compounds, last attempted with NASA’s Viking missions in the 1970s. A stereo color camera and a weather station will study the surrounding environment while the other instruments check excavated soil samples for water, organic chemicals and conditions that could indicate whether the site was ever hospitable to life. Microscopes can reveal features as small as one one-thousandth the width of a human hair. Launch of Phoenix aboard a Delta II rocket is targeted for Aug. 3 from Cape Canaveral Air Force Station in Florida.

In the Payload Hazardous Servicing Facility, an overhead crane moves the heat shield toward a platform at left. The heat shield was removed from the Phoenix Mars Lander spacecraft at right. The Phoenix mission is the first project in NASA's first openly competed program of Mars Scout missions. Phoenix will land in icy soils near the north polar permanent ice cap of Mars and explore the history of the water in these soils and any associated rocks, while monitoring polar climate. Landing is planned in May 2008 on arctic ground where a mission currently in orbit, Mars Odyssey, has detected high concentrations of ice just beneath the top layer of soil. It will serve as NASA's first exploration of a potential modern habitat on Mars and open the door to a renewed search for carbon-bearing compounds, last attempted with NASA’s Viking missions in the 1970s. A stereo color camera and a weather station will study the surrounding environment while the other instruments check excavated soil samples for water, organic chemicals and conditions that could indicate whether the site was ever hospitable to life. Microscopes can reveal features as small as one one-thousandth the width of a human hair. Launch of Phoenix aboard a Delta II rocket is targeted for Aug. 3 from Cape Canaveral Air Force Station in Florida.

In the Payload Hazardous Servicing Facility, technicians secure the backshell with the Phoenix Mars Lander inside onto a spin table for spin testing. The Phoenix mission is the first project in NASA's first openly competed program of Mars Scout missions. Phoenix will land in icy soils near the north polar permanent ice cap of Mars and explore the history of the water in these soils and any associated rocks, while monitoring polar climate. Landing is planned in May 2008 on arctic ground where a mission currently in orbit, Mars Odyssey, has detected high concentrations of ice just beneath the top layer of soil. It will serve as NASA's first exploration of a potential modern habitat on Mars and open the door to a renewed search for carbon-bearing compounds, last attempted with NASA’s Viking missions in the 1970s. A stereo color camera and a weather station will study the surrounding environment while the other instruments check excavated soil samples for water, organic chemicals and conditions that could indicate whether the site was ever hospitable to life. Microscopes can reveal features as small as one one-thousandth the width of a human hair. Launch of Phoenix aboard a Delta II rocket is targeted for Aug. 3 from Cape Canaveral Air Force Station in Florida.

This closeup shows the Phoenix Mars Lander spacecraft nestled inside the backshell. The spacecraft will undergo spin testing on the spin table to which it is attached in the Payload Hazardous Servicing Facility. The Phoenix mission is the first project in NASA's first openly competed program of Mars Scout missions. Phoenix will land in icy soils near the north polar permanent ice cap of Mars and explore the history of the water in these soils and any associated rocks, while monitoring polar climate. Landing is planned in May 2008 on arctic ground where a mission currently in orbit, Mars Odyssey, has detected high concentrations of ice just beneath the top layer of soil. It will serve as NASA's first exploration of a potential modern habitat on Mars and open the door to a renewed search for carbon-bearing compounds, last attempted with NASA’s Viking missions in the 1970s. A stereo color camera and a weather station will study the surrounding environment while the other instruments check excavated soil samples for water, organic chemicals and conditions that could indicate whether the site was ever hospitable to life. Microscopes can reveal features as small as one one-thousandth the width of a human hair. Launch of Phoenix aboard a Delta II rocket is targeted for Aug. 3 from Cape Canaveral Air Force Station in Florida.

The Philae lander of Europe Rosetta mission has returned the first panoramic image from the surface of a comet. The unprocessed panorama from the lander CIVA-P camera shows a 360-degree view around the point of final touchdown.

This graphic depicts the position of the Philae lander of the European Space Agency Rosetta mission, and a nearby cliff photographed by the lander, in the context of topographic modeling of the surface of comet 67P/Churyumov-Gerasimenko nucleus.

In this photograph of NASA Phoenix Mars Lander, the spacecraft specialists worked on the lander after its fan-like circular solar arrays had been spread open for testing.

Ahead of launch as part of NASA’s Commercial Lunar Payload Services (CLPS) initiative, Astrobotic’s Peregrine lunar lander is encapsulated in the payload fairing, or nose cone, of United Launch Alliance’s Vulcan rocket on Nov. 21, 2023, at Astrotech Space Operations Facility near the agency’s Kennedy Space Center in Florida. Launch of Astrobotic’s Peregrine Mission One will carry NASA and commercial payloads to the Moon in early 2024 to study the lunar exosphere, thermal properties, and hydrogen abundance of the lunar regolith, magnetic fields, and the radiation environment of the lunar surface.

Ahead of launch as part of NASA’s Commercial Lunar Payload Services (CLPS) initiative, Astrobotic’s Peregrine lunar lander is encapsulated in the payload fairing, or nose cone, of United Launch Alliance’s Vulcan rocket on Nov. 21, 2023, at Astrotech Space Operations Facility near the agency’s Kennedy Space Center in Florida. Launch of Astrobotic’s Peregrine Mission One will carry NASA and commercial payloads to the Moon in early 2024 to study the lunar exosphere, thermal properties, and hydrogen abundance of the lunar regolith, magnetic fields, and the radiation environment of the lunar surface.

Thrusters under NASA's InSight lander churned up soil during landing on Mars. This image shows two pits excavated by the thrusters. https://photojournal.jpl.nasa.gov/catalog/PIA23301

The targeted landing site for NASA Phoenix Mars Lander is at about 68 degrees north latitude, 233 degrees east longitude in the Martian arctic. The Phoenix lander, which landed May 25, 2008 ceased its operations about six months later.
NASA next Mars-bound spacecraft, the Phoenix Mars Lander, partway through assembly and testing at Lockheed Martin Space Systems, Denver, in September 2006.

In the Payload Hazardous Servicing Facility, technicians reopen the lander petals of the Mars Exploration Rover 2 MER-2 to allow access to one of the spacecraft circuit boards.

This artist's illustration shows NASA's InSight lander on the surface of Mars, with its solar arrays deployed. https://photojournal.jpl.nasa.gov/catalog/PIA22571

The science payload of NASA Phoenix Mars Lander includes a multi-tool instrument named the Microscopy, Electrochemistry, and Conductivity Analyzer MECA.

This annotated image depicts the backup landing site Site C chosen for ESA Rosetta spacecraft Philae lander.

Ahead of launch as part of NASA’s Commercial Lunar Payload Services (CLPS) initiative, Astrobotic’s Peregrine lunar lander is preparing to be encapsulated in the payload fairing, or nose cone, of United Launch Alliance’s Vulcan rocket on Nov. 21, 2023, at Astrotech Space Operations Facility near the agency’s Kennedy Space Center in Florida. Launch of Astrobotic’s Peregrine Mission One will carry NASA and commercial payloads to the Moon in early 2024 to study the lunar exosphere, thermal properties, and hydrogen abundance of the lunar regolith, magnetic fields, and the radiation environment of the lunar surface.

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

One of InSight's 7-foot (2.2 meter) wide solar panels was imaged by the lander's Instrument Deployment Camera, which is fixed to the elbow of its robotic arm. https://photojournal.jpl.nasa.gov/catalog/PIA22736
Mars Polar Lander Landing Site Noon-time Temperatures

Proposed Mars Polar Lander Landing Site Global Perspective
Hard Substrate, Possibly Ice, Uncovered Under the Mars Lander

Morning on Chryse Planitia - Viking Lander 1 Camera 2 Mosaic