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A Well-Traveled 'Eagle Crate
PIA05631
Sol (our sun)
Navigation Camera
Title |
A Well-Traveled 'Eagle Crater' (right-eye) |
Original Caption Released with Image |
This is the right-eye version of the Mars Exploration Rover Opportunity's view on its 56th sol on Mars, before it left its landing-site crater. To the right, the rover tracks are visible at the original spot where the rover attempted unsuccessfully to exit the crater. After a one-sol delay, Opportunity took another route to the plains of Meridiani Planum. This image was taken by the rover's navigation camera. |
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A Well-Traveled 'Eagle Crate
PIA05632
Sol (our sun)
Navigation Camera
Title |
A Well-Traveled 'Eagle Crater' (left-eye) |
Original Caption Released with Image |
This is the left-eye version of the Mars Exploration Rover Opportunity's view on its 56th sol on Mars, before it left its landing-site crater. To the right, the rover tracks are visible at the original spot where the rover attempted unsuccessfully to exit the crater. After a one-sol delay, Opportunity took another route to the plains of Meridiani Planum. This image was taken by the rover's navigation camera. |
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Ring Around the Rover
PIA05150
Sol (our sun)
Navigation Camera
Title |
Ring Around the Rover |
Original Caption Released with Image |
This polar projection of an image from the navigation camera on the Mars Exploration Rover Opportunity shows an overhead perspective of the rover. Opportunity's view of the martian horizon can also be seen in this image, taken shortly after the rover touched down at Meridiani Planum, Mars at 9:05 p.m. PST on Saturday, Jan. 24. |
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Eagle-eye View of "Eagle Cra
PIA05636
Sol (our sun)
Navigation Camera
Title |
Eagle-eye View of "Eagle Crater |
Original Caption Released with Image |
This image shows the Mars Exploration Rover Opportunity's view on its 56th sol on Mars, before it left its landing-site crater. To the right, the rover tracks are visible at the original spot where the rover attempted unsuccessfully to exit the crater. After a one-sol delay, Opportunity took another route to the plains of Meridiani Planum. This image was taken by the rover's navigation camera. |
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Sojourner Rover View of Path
title |
Sojourner Rover View of Pathfinder Lander |
Description |
Image of Pathfinder Lander on Mars taken from Sojourner Rover left front camera on sol 33. The IMP (on the lattice mast) is looking at the rover. Airbags are prominent, and the meteorology mast is shown to the right. Lowermost rock is Ender, with Hassock behind it and Yogi on the other side of the lander. NOTE: original caption as published in Science Magazine Science Magazine, Volume 278, Number 5344, 5 December 1997, 'Overview of the Mars Pathfinder Mission and Assessment of Landing Site Predictions' (Fig. 2) |
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Spirit Tracks on Mars, Sol 1
PIA06052
Sol (our sun)
Navigation Camera
Title |
Spirit Tracks on Mars, Sol 151 |
Original Caption Released with Image |
"" Click on the image for Spirit Tracks on Mars, Sol 151 (QTVR) This cylindrical projection mosaic was created from navigation camera images acquired by NASA's Mars Exploration Rover Spirit during Spirit's 151st martian day, or sol, on June 5, 2004. The rover sits at site 63, still more than 100 meters (328 feet) from the base of the "Columbia Hills." As suggested by the rover tracks fading off in the distance, Spirit made great progress on this sol, roving 73 meters (240 feet) to get to this point. |
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Surveying the Scene Above Op
PIA09687
Sol (our sun)
HiRISE, Panoramic Camera
Title |
Surveying the Scene Above Opportunity (Simulation) |
Original Caption Released with Image |
"" Click on the image to view the animation""Lower resolution animation This animation shows a hypothetical flyover above Victoria Crater, where NASA's Mars Exploration Rover Opportunity is perched on a rim. The rover is expected to begin rolling down into the crater in early July 2007. The first part of the movie is based on data taken by the Mars Reconnaissance Orbiter's High Resolution Imaging Science Experiment camera. A simulated rover is shown at the site where Opportunity will enter the crater, an alcove nicknamed "Duck Bay." The movie then transitions to a panoramic view of Victoria Crater taken from the top of Duck Bay by Opportunity's panoramic camera. |
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Surveying the Scene Above Op
PIA09687
Sol (our sun)
HiRISE, Panoramic Camera
Title |
Surveying the Scene Above Opportunity (Simulation) |
Original Caption Released with Image |
"" Click on the image to view the animation""Lower resolution animation This animation shows a hypothetical flyover above Victoria Crater, where NASA's Mars Exploration Rover Opportunity is perched on a rim. The rover is expected to begin rolling down into the crater in early July 2007. The first part of the movie is based on data taken by the Mars Reconnaissance Orbiter's High Resolution Imaging Science Experiment camera. A simulated rover is shown at the site where Opportunity will enter the crater, an alcove nicknamed "Duck Bay." The movie then transitions to a panoramic view of Victoria Crater taken from the top of Duck Bay by Opportunity's panoramic camera. |
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What Time is it on Mars?
PIA05017
Sol (our sun)
Panoramic Camera
Title |
What Time is it on Mars? |
Original Caption Released with Image |
This image of the martian sundial onboard the Mars Exploration Rover Spirit was processed by students in the Red Rover Goes to Mars program to impose hour markings on the face of the dial. The position of the shadow of the sundial's post within the markings indicates the time of day and the season, which in this image is 12:17 p.m. local solar time, late summer. A team of 16 students from 12 countries were selected by the Planetary Society to participate in this program. This image was taken on Mars by the rover's panoramic camera. |
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Right on Target
Title |
Right on Target |
Description |
This map shows the estimated location of the Mars Exploration Rover Spirit within Gusev Crater, Mars. Engineers targeted Spirit for the center of the blue ellipse. Measurements taken during the rover's descent by the Deep Space Network predicted its landing site to be the spot marked with a black dot. Later measurements taken on the ground by both the Deep Space Network and the orbiter Mars Odyssey narrowed the predicted landing site to a spot marked with a white dot. When initially choosing a landing site for the rover, engineers avoided hazardous terrain outlined here in yellow and red. This map consists of data from Mars Odyssey and Mars Global Surveyor. |
Date |
01.13.2004 |
|
Right on Target-2
Title |
Right on Target-2 |
Description |
This map shows a close-up look at the estimated location of the Mars Exploration Rover Spirit within Gusev Crater, Mars. Measurements taken during the rover's descent by the Deep Space Network predicted its landing site to be the spot marked with a black dot. Later measurements taken on the ground by both the Deep Space Network and the orbiter Mars Odyssey narrowed the predicted landing site to a spot marked with a white dot. When initially choosing a landing site for the rover, engineers avoided hazardous craters outlined here in yellow and red. This map consists of data from Mars Odyssey and Mars Global Surveyor. |
Date |
01.13.2004 |
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Spirit's Neighborhood in 'Co
title |
Spirit's Neighborhood in 'Columbia Hills,' in Stereo |
Description |
Two Earth years ago, NASA's Mars Exploration Rover Spirit touched down in Gusev Crater. The rover marked its first Mars-year (687 Earth days) anniversary in November 2005. On Nov. 2, 2005, shortly before Spirit's Martian anniversary, the Mars Orbiter Camera on NASA's Mars Global Surveyor acquired an image covering approximately 3 kilometers by 3 kilometers (1.9 miles by 1.9 miles) centered on the rover's location in the "Columbia Hills." The tinted portion of this image gives a stereo, three-dimensional view when observed through 3-D glasses with a red left eye and blue right eye. The tallest peak is "Husband Hill," which was climbed by Spirit during much of 2005. The region south (toward the bottom) of these images shows the area where the rover is currently headed. The large dark patch and other similar dark patches in these images are accumulations of windblown sand and granules. North is up, illumination is from the left. The location is near 14.8 degrees south latitude, 184.6 degrees west longitude. Credit: NASA/JPL-Caltech/MSSS |
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Spirit's Course
PIA06691
Sol (our sun)
Mars Orbiter Camera
Title |
Spirit's Course |
Original Caption Released with Image |
This digital elevation map shows the topography of the "Columbia Hills," just in front of the Mars Exploration Rover Spirit's current position. Rover planners have plotted the safest route for Spirit to climb to the front hill, called "West Spur." The black line in the middle of the image represents the rover's traverse path, which starts at "Hank's Hollow" and ends at the top of "West Spur." Scientists are sending Spirit up the hill to investigate the interesting rock outcrops visible in images taken by the rover. Data from the Mars Orbital Camera on the orbiting Mars Global Surveyor were used to create this 3-D map. In figure 1, the digital map shows the slopes of the "Columbia Hills," just in front of the Mars Exploration Rover Spirit's current position. Colors indicate the slopes of the hills, with red areas being the gentlest and blue the steepest. Rover planners have plotted the safest route for Spirit to climb the front hill, called "West Spur." The path is indicated here with a curved black line. Stereo images from the Mars Orbital Camera on the orbiting Mars Global Surveyor were used to create this 3-D map. In figure 2, the map shows the north-facing slopes of the "Columbia Hills," just in front of the Mars Exploration Rover Spirit's current position. Bright areas indicate surfaces sloping more toward the north than dark areas. To reach the rock outcrop at the top of the hill, engineers will aim to drive the rover around the dark areas, which would yield less solar power. The curved black line in the middle represents the rover's planned traverse path. |
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Spirit's Course
PIA06691
Sol (our sun)
Mars Orbiter Camera
Title |
Spirit's Course |
Original Caption Released with Image |
This digital elevation map shows the topography of the "Columbia Hills," just in front of the Mars Exploration Rover Spirit's current position. Rover planners have plotted the safest route for Spirit to climb to the front hill, called "West Spur." The black line in the middle of the image represents the rover's traverse path, which starts at "Hank's Hollow" and ends at the top of "West Spur." Scientists are sending Spirit up the hill to investigate the interesting rock outcrops visible in images taken by the rover. Data from the Mars Orbital Camera on the orbiting Mars Global Surveyor were used to create this 3-D map. In figure 1, the digital map shows the slopes of the "Columbia Hills," just in front of the Mars Exploration Rover Spirit's current position. Colors indicate the slopes of the hills, with red areas being the gentlest and blue the steepest. Rover planners have plotted the safest route for Spirit to climb the front hill, called "West Spur." The path is indicated here with a curved black line. Stereo images from the Mars Orbital Camera on the orbiting Mars Global Surveyor were used to create this 3-D map. In figure 2, the map shows the north-facing slopes of the "Columbia Hills," just in front of the Mars Exploration Rover Spirit's current position. Bright areas indicate surfaces sloping more toward the north than dark areas. To reach the rock outcrop at the top of the hill, engineers will aim to drive the rover around the dark areas, which would yield less solar power. The curved black line in the middle represents the rover's planned traverse path. |
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Spirit's Course
PIA06691
Sol (our sun)
Mars Orbiter Camera
Title |
Spirit's Course |
Original Caption Released with Image |
This digital elevation map shows the topography of the "Columbia Hills," just in front of the Mars Exploration Rover Spirit's current position. Rover planners have plotted the safest route for Spirit to climb to the front hill, called "West Spur." The black line in the middle of the image represents the rover's traverse path, which starts at "Hank's Hollow" and ends at the top of "West Spur." Scientists are sending Spirit up the hill to investigate the interesting rock outcrops visible in images taken by the rover. Data from the Mars Orbital Camera on the orbiting Mars Global Surveyor were used to create this 3-D map. In figure 1, the digital map shows the slopes of the "Columbia Hills," just in front of the Mars Exploration Rover Spirit's current position. Colors indicate the slopes of the hills, with red areas being the gentlest and blue the steepest. Rover planners have plotted the safest route for Spirit to climb the front hill, called "West Spur." The path is indicated here with a curved black line. Stereo images from the Mars Orbital Camera on the orbiting Mars Global Surveyor were used to create this 3-D map. In figure 2, the map shows the north-facing slopes of the "Columbia Hills," just in front of the Mars Exploration Rover Spirit's current position. Bright areas indicate surfaces sloping more toward the north than dark areas. To reach the rock outcrop at the top of the hill, engineers will aim to drive the rover around the dark areas, which would yield less solar power. The curved black line in the middle represents the rover's planned traverse path. |
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Rover Does a Wheelie
PIA04317
Sol (our sun)
Imager for Mars Pathfinder
Title |
Rover Does a Wheelie |
Original Caption Released with Image |
During a soil mechanics experiment, the rover does a wheelie, lifting its front left wheel into the air. |
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Opportunity Digs
PIA05309
Sol (our sun)
Title |
Opportunity Digs |
Original Caption Released with Image |
This image is a screenshot from a computer-generated animation showing the Mars Exploration Rover Opportunity trenching a hole in the sandy soil at Meridiani Planum, Mars. Data taken during trenching by the rover's onboard sensors were used to create the movie. |
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As Far as Opportunity's Eye
PIA05199
Sol (our sun)
Panoramic Camera
Title |
As Far as Opportunity's Eye Can See |
Original Caption Released with Image |
"" Click on the image for As Far as Opportunity's Eye Can See (QTVR) This expansive view of the martian real estate surrounding the Mars Exploration Rover Opportunity is the first 360 degree, high-resolution color image taken by the rover's panoramic camera. The airbag marks, or footprints, seen in the soil trace the route by which Opportunity rolled to its final resting spot inside a small crater at Meridiani Planum, Mars. The exposed rock outcropping is a future target for further examination. This image mosaic consists of 225 individual frames. |
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Airbag Deflates on Mars
PIA05002
Sol (our sun)
Navigation Camera
Title |
Airbag Deflates on Mars |
Original Caption Released with Image |
This image, taken by the navigation camera onboard the Mars Exploration Rover Spirit, shows the airbags used to protect the rover during landing. One bright, dust-covered bag is slightly puffed up against the lander. |
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MRPS #80911 (Sol 2) Rover to
This picture taken by the IM
7/5/97
Date |
7/5/97 |
Description |
This picture taken by the IMP (Imager for Mars Pathfinder) aboard the Mars Pathfinder spacecraft depicts the rover Sojourner's position after driving onto the Martian surface. Sojourner has become the first autonomous robot ever to traverse the surface of Mars. This image reflects the success of Pathfinder's principle objective -- to place a payload on Mars in a safe, operational configuration. The primary mission of Sojourner, scheduled to last seven days, will be to use its Alpha Proton X-ray Spectrometer (APXS) instrument to determine the elements that make up the rocks and soil on Mars. A full study using the APXS takes approximately ten hours, and can measure all elements except hydrogen at any time of the Martian day or night. The APXS will conduct its studies by bombarding rocks and soil samples with alpha particle radiation -- charged particles equivalent to the nucleus of a helium atom, consisting of two protons and two neutrons. Mars Pathfinder is the second in NASA's Discovery program of low- cost spacecraft with highly focused science goals. The Jet Propulsion Laboratory, Pasadena, CA, developed and manages the Mars Pathfinder mission for NASA's Office of Space Science, Washington, D.C. ##### |
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Opportunity Egress Practice
MER Egress test in JPL's In-
1/31/04
Spirit's Landing Site
title |
Spirit's Landing Site |
description |
This image, taken previously by the thermal emission spectrometer onboard Mars Global Surveyor, highlights the same cluster of craters captured by the Mars Exploration Rover Spirit as it descends to Mars. *Image Credit*: NASA |
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Windows to Meridiani's Water
PIA05504
Sol (our sun)
Hazard Identification Camera
Title |
Windows to Meridiani's Water-Soaked Past |
Original Caption Released with Image |
This image taken by the Mars Exploration Rover Opportunity shows the two holes that allowed scientists to peer into Meridiani Planum's wet past. The rover drilled the holes into rocks in the region dubbed "El Capitan" with its rock abrasion tool. By analyzing the freshly exposed rock with the rover's suite of scientific instruments, scientists gathered evidence that this part of Mars may have once been drenched in water. The lower hole, located on a target called "McKittrick," was made on the 30th martian day, or sol, of Opportunity's journey. The upper hole, located on a target called "Guadalupe" was made on the 34th sol of the rover's mission. This image was taken on the 35th martian day, or sol, by the rover's hazard-avoidance camera. The rock abrasion tool and scientific instruments are located on the rover's robotic arm. |
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FIDO Rover
Title |
FIDO Rover |
Full Description |
The Field Integrated Design and Operations (FIDO) rover is being used in ongoing NASA field tests to simulate driving conditions on Mars. FIDO is at a geologically interesting site in central Nevada while it is controlled from the mission control room at JPL's Planetary Robotics Laboratory in Pasadena. FIDO uses a robot arm to manipulate science instruments and it has a new mini-corer or drill to extract and cache rock samples. Several camera systems onboard allow the rover to collect science and navigation images by remote-control. The rover is about the size of a coffee table and weighs as much as a St. Bernard, about 70 kilograms (150 pounds). It is approximately 85 centimeters (about 33 inches) wide, 105 centimeters (41 inches) long, and 55 centimeters (22 inches) high. The rover moves up to 300 meters an hour (less than a mile per hour) over smooth terrain, using its onboard stereo vision systems to detect and avoid obstacles as it travels "on-the-fly." During these tests, FIDO is powered by both solar panels that cover the top of the rover and by replaceable, rechargeable batteries. |
Date |
04/01/1999 |
NASA Center |
Jet Propulsion Laboratory |
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FIDO Rover Retracted Arm and
Title |
FIDO Rover Retracted Arm and Camera |
Full Description |
The Field Integrated Design and Operations (FIDO) rover extends the large mast that carries its panoramic camera. The FIDO is being used in ongoing NASA field tests to simulate driving conditions on Mars. FIDO is controlled from the mission control room at JPL's Planetary Robotics Laboratory in Pasadena. FIDO uses a robot arm to manipulate science instruments and it has a new mini-corer or drill to extract and cache rock samples. Several camera systems onboard allow the rover to collect science and navigation images by remote-control. The rover is about the size of a coffee table and weighs as much as a St. Bernard, about 70 kilograms (150 pounds). It is approximately 85 centimeters (about 33 inches) wide, 105 centimeters (41 inches) long, and 55 centimeters (22 inches) high. The rover moves up to 300 meters an hour (less than a mile per hour) over smooth terrain, using its onboard stereo vision systems to detect and avoid obstacles as it travels "on-the-fly." During these tests, FIDO is powered by both solar panels that cover the top of the rover and by replaceable, rechargeable batteries. |
Date |
04/01/1999 |
NASA Center |
Jet Propulsion Laboratory |
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Pathfinder Landing
This photo shows Mars Pathfi
6/14/95
Date |
6/14/95 |
Description |
This photo shows Mars Pathfinder's configuration shortly after landing on the Martian surface on July 4, 1997. The spacecraft will land four hours before sunrise and spend most of that time standing itself upright, retracting its air bags, as seen here, and opening its petals to expose the 22-pound rover. As the sun comes up on Mars, the rover will power up its solar panels and prepare to roll off onto the Martian surface for a week of exploration. Mars Pathfinder, managed by NASA's Jet Propulsion Laboratory, is scheduled for launch on Dec. 2, 1996. |
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Turning in the Testbed
PIA05053
Hazard Identification Camera
Title |
Turning in the Testbed |
Original Caption Released with Image |
This image, taken in the JPL In-Situ Instruments Laboratory or "Testbed," shows the view from the front hazard avoidance cameras on the Mars Exploration Rover Spirit after the rover has backed up and turned 45 degrees counterclockwise. Engineers rehearsed this maneuver at JPL before performing it on Mars. This maneuver is the first step in a 3-point turn that will rotate the rover 115 degrees to face the rear direction and drive off a rear side lander petal. |
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Panoramic View of Lander Dur
PIA05083
Sol (our sun)
Hazard Identification Camera
Title |
Panoramic View of Lander During Turn |
Original Caption Released with Image |
This 360-degree panoramic mosaic image composed of data from the hazard avoidance camera on the Mars Exploration Rover Spirit shows a view of the lander from under the rover deck. The images were taken as the rover turned from its landing position 95 degrees toward the northwest side of the lander. |
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Farewell Glance at 'Enduranc
PIA07112
Sol (our sun)
Hazard Avoidance Camera
Title |
Farewell Glance at 'Endurance' |
Original Caption Released with Image |
NASA's Mars Exploration Rover Opportunity climbed out of "Endurance Crater" during the rover's 315th sol (Dec. 12, 2004), and used its front hazard-avoidance camera to look back across the crater from the rim. The rover spent just over six months inside the stadium-sized crater, examining in detail the tallest stack of bedrock layers ever seen up close on a foreign planet. |
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Roll-Off Dress Rehearsal at
PIA05065
Title |
Roll-Off Dress Rehearsal at JPL |
Original Caption Released with Image |
This image shows a test rover as it attempts a complete 115-degree turn on the lander in the JPL In-Situ Instruments Laboratory, or "testbed." This is where engineers tested the rover's three-point turn before completing the manuever with the Mars Exploration Rover Spirit at Gusev Crater on Mars. At this point, the test rover has turned 95 degrees, with 115 degrees being its goal position. |
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Rover 1 in Cruise Stage
PIA04414
Title |
Rover 1 in Cruise Stage |
Original Caption Released with Image |
Rover 1 sits atop the deployed lander with its solar arrays and wheels stowed. |
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Rover Family Photo
PIA04421
Title |
Rover Family Photo |
Original Caption Released with Image |
Members of the Mars Exploration Rovers Assembly, Test and Launch Operations team gather around Rover 2 and its predecessor, a flight spare of the Pathfinder mission's Sojourner rover, named Marie Curie. |
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Rover 1 and Lander
PIA04417
Title |
Rover 1 and Lander |
Original Caption Released with Image |
Rover 1 sits atop the deployed lander with its solar arrays and wheels stowed. |
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2 Stages of Deployment
PIA04424
Title |
2 Stages of Deployment |
Original Caption Released with Image |
The twin rovers sit side-by-side in different stages of deployment. Rover 2's (left) front wheels are stowed, while Rover 1's front wheels are deployed. |
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Meridiani Planum in View
PIA05139
Sol (our sun)
Navigation Camera
Title |
Meridiani Planum in View |
Original Caption Released with Image |
This image shows one of the Mars Exploration Rover Opportunity's first breathtaking views of the martian landscape after its successful landing at Meridiani Planum on Mars. On the left, the rover's mast can be seen in a stowed position. Opportunity landed Saturday night at approximately 9:05 PST. The image was taken by the rover's navigation camera. |
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A Flyby Tour of Spirit's Des
PIA05129
Sol (our sun)
Title |
A Flyby Tour of Spirit's Descent |
Original Caption Released with Image |
Telemetry sent down to Earth from the Mars Exploration Rover Spirit has been reconstructed to create a reenactment of the rover's final 30 seconds before landing at Gusev Crater, Mars. This image is a still from that movie. Just seconds before the rover touched down and its airbags were inflated, a gust of wind threatened to significantly increase the rover's horizontal speed. But the firing of a lateral rocket, called the Tranverse Impulse Rocket System (blue), kept the rover on course, orienting the main retrorockets (white) to the their correct upright position. Subsequent igniting of these rockets reduced the rover's speed to near zero, 23 feet (7 meters) above the martian surface. The colored bars to the right indicate Spirit's north, east and downward velocities. The telemetry was acquired through the Mars Global Surveyor. |
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A Flyby Tour of Spirit's Des
PIA05130
Sol (our sun)
Title |
A Flyby Tour of Spirit's Descent-2 |
Original Caption Released with Image |
Telemetry sent down to Earth from the Mars Exploration Rover Spirit has been reconstructed to create this computer-generated movie of the rover's final 30 seconds before landing at Gusev Crater, Mars. Just seconds before the rover touched down and its airbags were inflated, a gust of wind threatened to significantly increase the rover's horizontal speed. But the firing of a lateral rocket, called the Tranverse Impulse Rocket System (blue), kept the rover on course, orienting the main retrorockets (white) to the their correct upright position. Subsequent igniting of these rockets reduced the rover's speed to near zero, 23 feet (7 meters) above the martian surface. The telemetry was acquired through the Mars Global Surveyor. |
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'McMurdo' Panorama from Spir
title |
'McMurdo' Panorama from Spirit's 'Winter Haven' |
description |
This 360-degree view, called the "McMurdo" panorama, comes from the panoramic camera (Pancam) on NASA's Mars Exploration Rover Spirit. From April through October 2006, Spirit has stayed on a small hill known as "Low Ridge." There, the rover's solar panels are tilted toward the sun to maintain enough solar power for Spirit to keep making scientific observations throughout the winter on southern Mars. This view of the surroundings from Spirit's "Winter Haven" is presented in approximately true color. Oct. 26, 2006, marks Spirit's 1,000th sol of what was planned as a 90-sol mission. (A sol is a Martian day, which lasts 24 hours, 39 minutes, 35 seconds). The rover has lived through the most challenging part of its second Martian winter. Its solar power levels are rising again. Spring in the southern hemisphere of Mars will begin in early 2007. Before that, the rover team hopes to start driving Spirit again toward scientifically interesting places in the "Inner Basin" and "Columbia Hills" inside Gusev crater. The McMurdo panorama is providing team members with key pieces of scientific and topographic information for choosing where to continue Spirit's exploration adventure. The Pancam began shooting component images of this panorama during Spirit's sol 814 (April 18, 2006) and completed the part shown here on sol 932 (Aug. 17, 2006). The panorama was acquired using all 13 of the Pancam's color filters, using lossless compression for the red and blue stereo filters, and only modest levels of compression on the remaining filters. The overall panorama consists of 1,449 Pancam images and represents a raw data volume of nearly 500 megabytes. It is thus the largest, highest-fidelity view of Mars acquired from either rover. Additional photo coverage of the parts of the rover deck not shown here was completed on sol 980 (Oct. 5 , 2006). The team is completing the processing and mosaicking of those final pieces of the panorama, and that image will be released on the Web shortly to augment this McMurdo panorama view. This beautiful scene reveals a tremendous amount of detail in Spirit's surroundings. Many dark, porous-textured volcanic rocks can be seen around the rover, including many on Low Ridge. Two rocks to the right of center, brighter and smoother-looking in this image and more reflective in infrared observations by Spirit's miniature thermal emission spectrometer, are thought to be meteorites. On the right, "Husband Hill" on the horizon, the rippled "El Dorado" sand dune field near the base of that hill, and lighter-toned "Home Plate" below the dunes provide context for Spirit's travels since mid-2005. Left of center, tracks and a trench dug by Spirit's right-front wheel, which no longer rotates, have exposed bright underlying material. This bright material is evidence of sulfur-rich salty minerals in the subsurface, which may provide clues about the watery past of this part of Gusev Crater. Spirit has stayed busy at Winter Haven during the past, six months even without driving. In addition to acquiring this spectacular panorama, the rover team has also acquired significant new assessments of the elemental chemistry and mineralogy of rocks and soil targets within reach of the rover's arm. The team plans soon to have Spirit drive to a very nearby spot on Low Ridge to access different rock and soil samples while maintaining a good solar panel tilt toward the sun for the rest of the Martian winter. Despite the long span of time needed for acquiring this 360-degree view -- a few images at a time every few sols over a total of 119 sols because the available power was so low -- the lighting and color remain remarkably uniform across the mosaic. This fact attests to the repeatability of wintertime sols on Mars in the southern hemisphere. |
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The Second Rover Image
PIA04315
Sol (our sun)
Imager for Mars Pathfinder
Title |
The Second Rover Image |
Original Caption Released with Image |
This image of the Mars Pathfinder Lander on the surface of Mars was imaged by Sojourner as it looks back. Sojourners tracks are visible in the foreground. |
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Pathfinder Rover Atop Mermai
PIA01132
Sol (our sun)
Imager for Mars Pathfinder
Title |
Pathfinder Rover Atop Mermaid Dune |
Original Caption Released with Image |
Mars Pathfinder Lander camera image of Sojourner Rover atop the Mermaid "dune" on Sol 30. Note the dark material excavated by the rover wheels. These, and other excavations brought materials to the surface for examination and allowed estimates of mechanical properties of the deposits. NOTE: original caption as published in Science Magazine Mars Pathfinder is the second in NASA's Discovery program of low-cost spacecraft with highly focused science goals. The Jet Propulsion Laboratory, Pasadena, CA, developed and manages the Mars Pathfinder mission for NASA's Office of Space Science, Washington, D.C. JPL is a division of the California Institute of Technology (Caltech). |
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May 2000 Nevada Field Test
The Field Integrated Design
5/15/00
Date |
5/15/00 |
Description |
The Field Integrated Design and Operations (FIDO) rover extends the large mast that carries its panoramic camera. The FIDO is being used in ongoing NASA field tests to simulate driving conditions on Mars. FIDO is at a geologically interesting site in central Nevada while it is controlled from the mission control room at JPL's Planetary Robotics Laboratory in Pasadena. FIDO is about the size of a St. Bernard. It weighs about 70 kilograms (154 pounds) and is approximately 85 centimeters (about 33 inches) wide, 105 centimeters (41 inches) long, and 55 centimeters (22 inches) high. The rover moves at an average speed of about 200 meters an hour (about one tenth a mile per hour) over smooth terrain, using its onboard stereo vision systems to detect and avoid obstacles "on- the-fly." During these tests, FIDO is powered by both solar panels that cover the top of the rover and by replaceable, rechargeable batteries. FIDO is about twice the size of Mars Pathfinder's Sojourner rover and is far more capable of performing its job without frequent human help. |
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May 2000 Nevada Field Test
The Field Integrated Design
5/15/00
Date |
5/15/00 |
Description |
The Field Integrated Design and Operations (FIDO) rover extends the large mast that carries its panoramic camera. The FIDO is being used in ongoing NASA field tests to simulate driving conditions on Mars. FIDO is at a geologically interesting site in central Nevada while it is controlled from the mission control room at JPL's Planetary Robotics Laboratory in Pasadena. FIDO is about the size of a St. Bernard. It weighs about 70 kilograms (154 pounds) and is approximately 85 centimeters (about 33 inches) wide, 105 centimeters (41 inches) long, and 55 centimeters (22 inches) high. The rover moves at an average speed of about 200 meters an hour (about one tenth a mile per hour) over smooth terrain, using its onboard stereo vision systems to detect and avoid obstacles "on- the-fly." During these tests, FIDO is powered by both solar panels that cover the top of the rover and by replaceable, rechargeable batteries. FIDO is about twice the size of Mars Pathfinder's Sojourner rover and is far more capable of performing its job without frequent human help. |
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May 2000 Nevada Field Test
The Field Integrated Design
5/16/00
Date |
5/16/00 |
Description |
The Field Integrated Design and Operations (FIDO) rover is being used in ongoing NASA field tests to simulate driving conditions on Mars. FIDO is at a geologically interesting site in central Nevada while it is controlled from the mission control room at JPL's Planetary Robotics Laboratory in Pasadena. FIDO is about the size of a St. Bernard. It weighs about 70 kilograms (154 pounds) and is approximately 85 centimeters (about 33 inches) wide, 105 centimeters (41 inches) long, and 55 centimeters (22 inches) high. The rover moves at an average speed of about 200 meters an hour (about one tenth a mile per hour) over smooth terrain, using its onboard stereo vision systems to detect and avoid obstacles "on- the-fly." During these tests, FIDO is powered by both solar panels that cover the top of the rover and by replaceable, rechargeable batteries. FIDO is about twice the size of Mars Pathfinder's Sojourner rover and is far more capable of performing its job without frequent human help. |
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May 2000 Nevada Field Test
The Field Integrated Design
5/17/00
Date |
5/17/00 |
Description |
The Field Integrated Design and Operations (FIDO) rover is being used in ongoing NASA field tests to simulate driving conditions on Mars. FIDO is at a geologically interesting site in central Nevada while it is controlled from the mission control room at JPL's Planetary Robotics Laboratory in Pasadena. FIDO is about the size of a St. Bernard. It weighs about 70 kilograms (154 pounds) and is approximately 85 centimeters (about 33 inches) wide, 105 centimeters (41 inches) long, and 55 centimeters (22 inches) high. The rover moves at an average speed of about 200 meters an hour (about one tenth a mile per hour) over smooth terrain, using its onboard stereo vision systems to detect and avoid obstacles "on- the-fly." During these tests, FIDO is powered by both solar panels that cover the top of the rover and by replaceable, rechargeable batteries. FIDO is about twice the size of Mars Pathfinder's Sojourner rover and is far more capable of performing its job without frequent human help. |
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Hole in One
title |
Hole in One |
description |
The interior of a crater surrounding the Mars Exploration Rover Opportunity at Meridiani Planum on Mars can be seen in this color image from the rover's panoramic camera. This is the darkest landing site ever visited by a spacecraft on Mars. The rim of the crater is approximately 10 meters (32 feet) from the rover. The crater is estimated to be 20 meters (65 feet) in diameter. Scientists are intrigued by the abundance of rock outcrops dispersed throughout the crater, as well as the crater's soil, which appears to be a mixture of coarse gray grains and fine reddish grains. Data taken from the camera's near-infrared, green and blue filters were combined to create this approximate true color picture, taken on the first day of Opportunity's journey. The view is to the west-southwest of the rover. *Image Credit*: NASA/JPL/Cornell |
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Spirit Celebration
title |
Spirit Celebration |
date |
01.03.2004 |
description |
NASA's Mars Exploration Rover team reacts after getting the first signals from the Spirit rover on the surface of Mars. Spirit landed at Mars' Gusev Carter at 8:52 p.m. (PST) on Saturday, Jan. 3. *Image Credit*: NASA |
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Martian Meteorite
title |
Martian Meteorite |
description |
NASA's Mars Exploration Rover Opportunity has found an iron meteorite, the first meteorite of any type ever identified on another planet. The pitted, basketball-size object is mostly made of iron and nickel according to readings from spectrometers on the rover. Only a small fraction of the meteorites fallen on Earth are similarly metal-rich. Others are rockier. As an example, the meteorite that blasted the famous Meteor Crater in Arizona is similar in composition. "This is a huge surprise, though maybe it shouldn't have been," said Dr. Steve Squyres of Cornell University, Ithaca, N.Y., principal investigator for the science instruments on Opportunity and its twin, Spirit. The meteorite, dubbed "Heat Shield Rock," sits near debris of Opportunity's heat shield on the surface of Meridiani Planum, a cratered flatland that has been Opportunity's home since the robot landed on Mars nearly one year ago. "I never thought we would get to use our instruments on a rock from someplace other than Mars," Squyres said. "Think about where an iron meteorite comes from: a destroyed planet or planetesimal that was big enough to differentiate into a metallic core and a rocky mantle." Rover-team scientists are wondering whether some rocks that Opportunity has seen atop the ground surface are rocky meteorites. "Mars should be hit by a lot more rocky meteorites than iron meteorites," Squyres said. "We've been seeing lots of cobbles out on the plains, and this raises the possibility that some of them may in fact be meteorites. We may be investigating some of those in coming weeks. The key is not what we'll learn about meteorites -- we have lots of meteorites on Earth -- but what the meteorites can tell us about Meridiani Planum." The numbers of exposed meteorites could be an indication of whether the plain is gradually eroding away or being built up. NASA Chief Scientist Dr. Jim Garvin said, "Exploring meteorites is a vital part of NASA's scientific agenda, and discovering whether there are storehouses of them on Mars opens new research possibilities, including further incentives for robotic and then human-based sample-return missions. Mars continues to provide unexpected science 'gold,' and our rovers have proven the value of mobile exploration with this latest finding." Initial observation of Heat Shield Rock from a distance with Opportunity's miniature thermal emission spectrometer suggested a metallic composition and raised speculation last week that it was a meteorite. The rover drove close enough to use its Moessbauer and alpha particle X-ray spectrometers, confirming the meteorite identification over the weekend. Opportunity and Spirit successfully completed their primary three-month missions on Mars in April 2004. NASA has extended their missions twice because the rovers have remained in good condition to continue exploring Mars longer than anticipated. They have found geological evidence of past wet environmental conditions that might have, been hospitable to life. Opportunity has driven a total of 2.10 kilometers (1.30 miles). Minor mottling from dust has appeared in images from the rover's rear hazard-identification camera since Opportunity entered the area of its heat-shield debris, said Jim Erickson of NASA's Jet Propulsion Laboratory, Pasadena, Calif., rover project manager. The rover team plans to begin driving Opportunity south toward a circular feature called "Vostok" within about a week. Spirit has driven a total of 4.05 kilometers (2.52 miles). It has been making slow progress uphill toward a ridge on "Husband Hill" inside Gusev Crater. *Image Credit*: NASA |
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Lower portions of Yogi & rov
PIA00643
Sol (our sun)
Rover Cameras
Title |
Lower portions of Yogi & rover wheel |
Original Caption Released with Image |
The image was taken by a camera aboard the Sojourner rover on Sol 4. The large rock Yogi can be seen at the upper right portion of the image. Sojourner's Alpha Proton X-Ray Spectrometer instrument is currently studying the sand around Yogi, and may study Yogi itself later on. One of Sojourner's cleated wheels is visible at lower right. Mars Pathfinder is the second in NASA's Discovery program of low-cost spacecraft with highly focused science goals. The Jet Propulsion Laboratory, Pasadena, CA, developed and manages the Mars Pathfinder mission for NASA's Office of Space Science, Washington, D.C. JPL is an operating division of the California Institute of Technology (Caltech). The Imager for Mars Pathfinder (IMP) was developed by the University of Arizona Lunar and Planetary Laboratory under contract to JPL. Peter Smith is the Principal Investigator. |
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Sojourner Doing a Wheelie on
PIA01556
Sol (our sun)
Rover Cameras
Title |
Sojourner Doing a Wheelie on Wedge - Left Eye |
Original Caption Released with Image |
Sojourner's left rear wheel is perched on the rock "Wedge" in this image, taken on Sol 47 by the Imager for Mars Pathfinder (IMP). The rover's Alpha Proton X-ray Spectrometer (APXS) is the cylindrical object extending from the back of the rover. This image and PIA01557 [ http://photojournal.jpl.nasa.gov/catalog/PIA01557 ](right eye) make up a stereo pair. Mars Pathfinder is the second in NASA's Discovery program of low-cost spacecraft with highly focused science goals. The Jet Propulsion Laboratory, Pasadena, CA, developed and manages the Mars Pathfinder mission for NASA's Office of Space Science, Washington, D.C. JPL is an operating division of the California Institute of Technology (Caltech). |
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Eyeing Eagle Crater
title |
Eyeing Eagle Crater |
description |
This image mosaic, compiled from navigation and panoramic camera images during the Mars Exploration Rover Opportunity's 33rd, 35th, and 36th sols on Mars, shows a panoramic view of the crater where the rover had been exploring since its dramatic arrival in late January 2004. The crater, now informally referred to as "Eagle Crater," is approximately 22 meters (72 feet) in diameter. Opportunity's lander is visible in the center of the image. Track marks reveal the rover's progress. The rover cameras recorded this view as Opportunity climbed close to the crater rim as part of a soil survey campaign. *Image credit*: NASA/JPL/Cornell |
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