Mars Pathfinder
NASA’s Mars Pathfinder successfully demonstrated a new way to safely land on the Red Planet and deliver the first-ever robotic rover, Sojourner, to the Martian surface.
mission Type
Lander, Rover
Launch
Dec. 4, 1996
objective
Land a rover on Mars
landing
July 4, 1997

This is the "gallery" or "presidential" panorama taken by the Pathfinder lander. Roughly 100 frames have been stitched manually to produce this seamless image. The color has been processed to retain as much of the dynamic range of the original color filters as possible while still keeping the hues in the color space of JPL's calibrated color images. The goal of the color balancing was to provide a view of the terrain that as clearly as possible showed differentiations in rock and soil types. The sky and a small area near the low-gain antenna have been retouched.
NASA/JPL-Caltech
Key Facts
| Launch | Dec. 4, 1996 UTC |
| Launch Location | Cape Canaveral Air Force Station, Florida |
| Rocket | Delta II 7925 |
| Mars Landing | July 4, 1997 |
| Landing Site: | Ares Vallis, Mars |
| End of Mission | Sept. 27, 1997 |
360-Degree view
NASA's Mars Pathfinder & Sojourner Rover
Explore the landing site of NASA's Pathfinder mission to Mars with your mouse or mobile device. This 360-degree panorama includes the lander's companion rover, Sojourner, and top science targets.
NOTE: Not all browsers support viewing 360 videos/images.
Mars Pathfinder Lander
Mars Pathfinder was originally designed as a technology demonstration to deliver an instrumented lander and a free-ranging robotic rover to the surface of the Red Planet.
Both the lander and the 23-pound (10.6 kilogram) rover, Sojourner, carried instruments for scientific observations and to provide engineering data on the new technologies being demonstrated. Included were scientific instruments to analyze the Martian atmosphere, climate, geology, and the composition of its rocks and soil. Mars Pathfinder used an innovative method of directly entering the Martian atmosphere and landing.
From landing until the final data transmission on Sept. 27, 1997, Mars Pathfinder returned 2.3 billion bits of information, including more than 16,500 images from the lander and 550 images from the rover, as well as more than 15 chemical analyses of rocks and soil and extensive data on winds and other weather factors. Findings from the investigations carried out by scientific instruments on both the lander and the rover suggest that Mars was at one time in its past warm and wet.
Airbag Landing
Pathfinder used an innovative method of directly entering the Martian atmosphere, assisted by a parachute to slow its descent through the thin Martian atmosphere and a giant system of airbags to cushion the impact. It was the first time this airbag technique had been used.
At a speed of 31 mph (14 meters per second) and measuring 19 feet (5.8 meters) in diameter, Pathfinder bounced like a giant beach ball about 15 times, as high as 50 feet (15 meters), before coming to rest 2-1/2 minutes later about six-tenths of a mile (1 kilometer) from the point of initial impact.

Engineers tested these huge, multi-lobed air bags, which enveloped and protected the Mars Pathfinder spacecraft before it impacted the surface of Mars. The air bags are composed of four large bags with six smaller, interconnected spheres within each bag. The bags measure 17 feet (5 meters) tall and about 17 feet (5 meters) in diameter. As Pathfinder descended to the Martian surface on a parachute, an onboard altimeter inside the lander monitored its distance from the ground. The computer inflated these large air bags about 330 feet (100 meters) above the surface of Mars. Upon landing, the airbag-encased Pathfinder bounced more than 15 times before rolling to a stop.
Sojourner Rover
The lander, named the Carl Sagan Memorial Station to honor the famed astronomer who had died the year before, deployed the rover, named Sojourner after American civil-rights crusader Sojourner Truth.
On the night of July 5, late in the second Martian day, or sol 2, Sojourner stood up to its full height of 1 foot (30 centimeters) and rolled down the lander’s rear ramp, which was tilted at 20 degrees from the surface, well within the limits of safe deployment.

This eight-image mosaic was acquired during the late afternoon on Sol 2 as part of the predeploy 'insurance panorama' and shows the newly deployed rover sitting on the Martian surface. The insurance panorama was designed as 'insurance' against camera failure upon deployment. Had the camera failed, the losslessly compressed, multispectral insurance panorama would have been the main source of image data from the Imager for Mars Pathfinder.
NASA/JPL-Caltech
Landing Site: Ares Vallis
The landing site, Ares Vallis (named for Ares, the Greek counterpart to the Roman god Mars, and the Latin word for valley), is an ancient flood plain in Mars’ northern hemisphere, and known as among the rockiest parts of the planet. It was chosen because scientists believed it to be a relatively safe surface to land on and one which contained a wide variety of rocks deposited during a catastrophic flood. In the event early in Mars’ history, scientists believe that the floodplain was cut by a volume of water the size of North America’s Great Lakes in about two weeks.

Large boulders are visible in this enlargement of pictures taken by the Imager for Mars Pathfinder (IMP) lander camera on July 4, 1997. The landing site is in the dry flood channel named Ares Valles. The boulders probably represent deposits from one of the catastrophic floods that carved the ancient channel. Between the rocks is brownish windblown soil. The gray-tan sky results from dust particles in the atmosphere.
NASA/JPL-Caltech
Mars Pathfinder Science Instruments
- Alpha Proton X-ray Spectrometer: Determined the elemental composition of rocks and soils
- Three Cameras: Provided images of the surrounding terrain for geological studies, and documented the performance and operating environment for Pathfinder mission technologies
- Atmospheric Structure Instrument/Meteorology Package: Measured the Martian atmosphere during Pathfinder's descent to the surface, and provided meteorological measurements at the lander
Mars Pathfinder Science Highlights
- Rounded pebbles and cobbles at the landing site, and other observations, suggested conglomerates that formed in running water during a warmer past in which liquid water was stable.
- Radio tracking of Mars Pathfinder provided a precise measure of the lander's location and Mars' pole of rotation. The measurements suggested that the radius of the planet's central metallic core is greater than 800 miles (1,300 kilometers) but less than roughly 1,250 miles (2,000 kilometers).
- Airborne dust is magnetic, and its characteristics suggest the magnetic mineral is maghemite, a very magnetic form of iron oxide, which may have been freeze-dried on the particles as a stain or cement. An active water cycle in the past may have leached out the iron from materials in the crust.
- Dust devils were seen and frequently measured by temperature, and sensors for wind and pressure. Observations suggested that these gusts are a mechanism for mixing dust into the atmosphere.
- Early morning water ice clouds were seen in the lower atmosphere.
- Abrupt temperature fluctuations were recorded in the morning, suggesting that the atmosphere is warmed by the planet's surface, with heat convected upward in small eddies.
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