Eagle Crater Traverse Area

Looking Back at Eagle Crater

The bright landing platform left behind by NASA's Mars Exploration Rover Opportunity in 2004 is visible inside Eagle Crater, at upper right in this April 8, 2017, observation by NASA's Mars Reconnaissance Orbiter. Mars Reconnaissance Orbiter arrived at Mars in March 2006, more than two years after Opportunity's landing on Jan. 25, 2004, Universal Time (Jan. 24, PDT). This is the first image of Eagle Crater from the orbiter's High Resolution Imaging Science Experiment (HiRISE) camera, which has optics that include the most powerful telescope ever sent to Mars. Eagle Crater is about 72 feet (22 meters) in diameter, at 1.95 degrees south latitude, 354.47 degrees east longitude, in the Meridiani Planum region of Mars. The airbag-cushioned lander, with Opportunity folded-up inside, first hit Martian ground near the crater, then bounced and rolled right into the crater. The lander structure was four triangles, folded into a tetrahedron until after the airbags deflated. The triangular petals then opened, exposing the rover. A week later, the rover drove off (see PIA05214), and the landing platform's job was done. The spacecraft's backshell and parachute, jettisoned during final descent, are visible near the lower left corner of this scene. The blue tint of the backshell is an effect of exaggerated color, because HiRISE combines color information from red, blue-green and infrared portions of the spectrum, rather than three different visible-light colors, so its color images are not true color. Opportunity examined Eagle Crater for more than half of the rover's originally planned three-month mission, before driving east and south to larger craters. At Eagle, it found headline-making evidence that water once flowed over the surface and soaked the subsurface of the area. By the time this orbital image of the landing site was taken, about 13 years after the rover departed Eagle, Opportunity had driven more than 27 miles (44 kilometers) and was actively exploring the rim of Endeavour Crater, which is about 1,000 times as wide as Eagle. https://photojournal.jpl.nasa.gov/catalog/PIA21494

Hamersley : Not Quite Like Eagle Crater

A Well-Traveled Eagle Crater right-eye

A Well-Traveled Eagle Crater left-eye

This is the 3-D version of NASA Mars Exploration Rover Opportunity view on its 56th sol on Mars, before it left Eagle Crater. 3D glasses are necessary to view this image.

This image maps out the travels of NASA Mars Exploration Rover Opportunity, from is landing site at Eagle Crater to the rim of Victoria Crater about six miles 9.7 kilometers away in September of 2006.

This is a 3-D version of the first 360-degree view from NASA Mars Exploration Rover Opportunity position outside Eagle Crater. 3D glasses are necessary to view this image.

The yellow line on this map shows where NASA Mars Rover Opportunity has driven from the place where it landed in January 2004, inside Eagle crater, upper left end of track, to a point about 2.2 miles away from reaching the rim of Endeavour crater.

This map shows the route driven by NASA Opportunity rover from the site of its landing, inside Eagle crater, to its location more than 112 months later, in late May 2013, departing the Cape York section of the rim of Endeavour crater.

The yellow line on this map shows where NASA Mars Rover Opportunity has driven from the place where it landed in January 2004, inside Eagle crater, at the upper left end of the track, to a point approaching the rim of Endeavour crater.

This map shows route driven by NASA Mars Exploration Rover Opportunity from the site of its landing, inside Eagle crater at the upper left, to its location more than 91 months later, on the Cape York section of the rim of Endeavour crater.

The yellow line on this map shows where NASA Mars Rover Opportunity has driven from the place where it landed in January 2004, inside Eagle crater, at the upper left end of the track, to a point approaching the rim of Endeavour crater.

The white line on this map shows where NASA Mars Rover Opportunity has driven from the place where it landed in January 2004 -- inside Eagle Crater, at the upper left end of the track -- to where it reached on the 2,442nd Martian day, or sol.

NASA Opportunity rover, working on Mars since January 2004, passed 25 miles of total driving on the July 27, 2014. The gold line on this map shows Opportunity route from the landing site inside Eagle Crater, in upper left.

The red line on this map shows where NASA Mars Rover Opportunity has driven from the place where it landed in January 2004, inside Eagle Crater, at the upper left end of the track, to where it reached on Nov. 30, 2010.

AS11-40-5881 (20 July 1969) --- This 70mm handheld camera's image on the Sea of Tranquility's lunar surface is the first of a multi-framed panorama photographed from a point some 30 or 40 feet west of the plus-Z (west) footpad of the Lunar Module "Eagle." The view is looking toward the southwest showing part of the horizon crater rim that was pointed out as being visible from the Eagle's window.

Panoramas of Apollo sites are required to familiarize various Constellation projects with the actual nature of the lunar surface. This image is the first of a multi-framed panorama photographed from a point some 30 or 40 feet west of the plus-Z (west) footpad of the Lunar Module "Eagle." The view is looking toward the southwest showing part of the horizon crater rim that was pointed out as being visible from the Eagle's window. Image taken at Tranquility Base. View was created using Apollo 11 images - mag 40 frames 5881 thru 5891.

This is a mosaic assembled from some of the images taken by the panoramic camera on NASA's Mars Exploration Rover Opportunity during the rover's 590th sol (Sept. 21, 2005). The view is toward the south and includes rock exposures north of "Erebus Crater," with the crater in the background. The rover will investigate the exposed rocks in the foreground and will take additional panoramic-camera images of Erebus Crater, which is about 300 meters (about 984 feet) across. Erebus Crater dwarfs the landing-site crater, "Eagle Crater," which measures about 22 meters (72 feet) in diameter. And, it is nearly twice the diameter of "Endurance Crater," which, at 130 meters (430 feet) wide, has been compared to a stadium. The camera's red filter was used for taking the images in this mosaic. It admits light with a wavelength of 750 nanometers http://photojournal.jpl.nasa.gov/catalog/PIA06341

This final traverse map for NASA's Opportunity rover shows where the rover was located within Perseverance Valley on June 10, 2018, the last date it made contact with its engineering team. Visible in this map is a yellow traverse route beginning at Opportunity's landing site, Eagle Crater, and ranging 28.06 miles (45.16 kilometers) to its final resting spot on the rim of Endeavour Crater. The rover was descending down into the crater in Perseverance Valley when the dust storm ended its mission. This map is made from several images taken by the Context Camera on NASA's Mars Reconnaissance Orbiter. Those images are: B02_010486_1779_XN_02S005W, P15_006847_1770_XN_03S005W, and P13_006135_1789_XN_01S005W. Malin Space Science Systems in San Diego built and operates the camera. https://photojournal.jpl.nasa.gov/catalog/PIA23178

AS11-44-6609 (16-24 July 1969) --- An oblique of the Crater Daedalus on the lunar farside as seen from the Apollo 11 spacecraft in lunar orbit. The view looks southwest. Daedalus (formerly referred to as I.A.U. Crater No. 308) is located at 179 degrees east longitude and 5.5 degrees south latitude. Daedalus has a diameter of about 50 statute miles. This is a typical scene showing the rugged terrain on the farside of the moon. While astronauts Neil A. Armstrong, commander, and Edwin E. Aldrin Jr., lunar module pilot, descended in the Lunar Module (LM) "Eagle" to explore the Sea of Tranquility region of the moon, astronaut Michael Collins, command module pilot, remained with the Command and Service Modules (CSM) "Columbia" in lunar orbit.

Eleven years and two months after its landing on Mars, the total driving distance of NASA's Mars Exploration Rover Opportunity surpassed the length of a marathon race: 26.219 miles (42.195 kilometers). This map shows the southward path driven by Opportunity from late December 2014 until it passed marathon distance on March 24, 2015, during the 3,968th Martian day, or sol, of the rover's work on Mars. Recent drives bring the vehicle close to a science destination called "Marathon Valley" on the west rim of Endeavour Crater. The rover team is using instruments on Opportunity to study "Spirit of St. Louis Crater" before entry into Marathon Valley. Opportunity reached the Sol 3881 location near the top of the map on Dec. 24, 2015. A map showing wider context of Opportunity's route from its January 2004 landing in Eagle Crater to Endeavour Crater is at PIA18404. A view from the Sol 3893 location at the summit of "Cape Tribulation," taken the following sol, is at PIA19109. The rover's traverse shown here has been mapped onto an image from the High Resolution Imaging Science Experiment (HiRISE) camera on NASA's Mars Reconnaissance Orbiter. http://photojournal.jpl.nasa.gov/catalog/PIA19157

Eleven years and two months after its landing on Mars, the total driving distance of NASA's Mars Exploration Rover Opportunity surpassed the length of a marathon race: 26.219 miles (42.195 kilometers). This map shows the southward path driven by Opportunity from late December 2014 until it passed marathon distance on March 24, 2015, during the 3,968th Martian day, or sol, of the rover's work on Mars. Recent drives bring the vehicle close to a science destination called "Marathon Valley" on the west rim of Endeavour Crater. The rover team is using instruments on Opportunity to study "Spirit of St. Louis Crater" before entry into Marathon Valley. Opportunity reached the Sol 3881 location near the top of the map on Dec. 24, 2015. A map showing wider context of Opportunity's route from its January 2004 landing in Eagle Crater to Endeavour Crater is at PIA18404. A view from the Sol 3893 location at the summit of "Cape Tribulation," taken the following sol, is at PIA19109. The rover's traverse shown here has been mapped onto an image from the High Resolution Imaging Science Experiment (HiRISE) camera on NASA's Mars Reconnaissance Orbiter. http://photojournal.jpl.nasa.gov/catalog/PIA19158

NASA's Mars Exploration Rover Opportunity, working on Mars since January 2004, passed marathon distance in total driving on March 24, 2015, during the mission's 3,968th Martian day, or sol. A drive of 153 feet (46.5 meters) on Sol 3968 brought Opportunity's total odometry to 26.221 miles (42.198 kilometers). Olympic marathon distance is 26.219 miles (42.195 kilometers). The gold line on this image shows Opportunity's route from the landing site inside Eagle Crater, in upper left, to its location after the Sol 3968 drive. The mission has been investigating on the western rim of Endeavour Crater since August 2011. This crater spans about 14 miles (22 kilometers) in diameter. The mapped area is all within the Meridiani Planum region of equatorial Mars, which was chosen as Opportunity's landing area because of earlier detection of the mineral hematite from orbit. North is up. The base image for the map is a mosaic of images taken by the Context Camera on NASA's Mars Reconnaissance Orbiter. http://photojournal.jpl.nasa.gov/catalog/PIA19154

This map show a portion of Endeavour Crater's western rim that includes the "Marathon Valley" area investigated intensively by NASA's Mars Exploration Rover Opportunity in 2015 and 2016, and a fluid-carved gully that is a destination to the south for the mission. The width of the area covered in the map is about half a mile (about 800 meters). North is up. Opportunity entered the northern end of the mapped area in January 2015 and entered Marathon Valley in July 2015. A gold line on the map, which may not be visible without zooming into the image, shows the rover's route. Curiosity departed Marathon Valley in September 2016 by driving southward through "Lewis and Clark Gap" into "Bitterroot Valley." The gully near the south end of the map was incised into Endeavour's rim long ago by a fluid, possibly a water-lubricated debris flow or a flow with mostly water. Driving into this gully to learn more about that flow is one of the goals for a two-year mission extension taking Opportunity through September 2018. A map showing wider context of Opportunity's route from its January 2004 landing in Eagle Crater to Endeavour Crater and Marathon Valley is at PIA19154. The rover's traverse shown here has been mapped by Tim Parker of NASA's Jet Propulsion Laboratory, Pasadena, California, onto an image from the High Resolution Imaging Science Experiment (HiRISE) camera on NASA's Mars Reconnaissance Orbiter. http://photojournal.jpl.nasa.gov/catalog/PIA20854

This is a detailed view of the back side of Moon in the vicinity of Crater No. 308 taken during the Apollo 11 mission. Apollo 11, the first manned lunar mission, launched from The Kennedy Space Center, Florida via a Saturn V launch vehicle on July 16, 1969 and safely returned to Earth on July 24, 1969. The Saturn V vehicle was developed by the Marshall Space Flight Center (MSFC) under the direction of Dr. Wernher von Braun. The 3-man crew aboard the flight consisted of Neil A. Armstrong, commander; Michael Collins, Command Module pilot; and Edwin E. Aldrin Jr., Lunar Module pilot. The Lunar Module (LM), named “Eagle, carrying astronauts Neil Armstrong and Edwin Aldrin, was the first crewed vehicle to land on the Moon. Meanwhile, astronaut Collins piloted the Command Module in a parking orbit around the Moon. Armstrong was the first human to ever stand on the lunar surface, followed by Edwin (Buzz) Aldrin. The crew collected 47 pounds of lunar surface material which was returned to Earth for analysis. The surface exploration was concluded in 2½ hours. With the success of Apollo 11, the national objective to land men on the Moon and return them safely to Earth had been accomplished.

Capri Chasma is located in the eastern portion of the Valles Marineris canyon system, the largest known canyon system in the Solar System. Deeply incised canyons such as this are excellent targets for studying the Martian crust, as the walls may reveal many distinct types of bedrock. This section of the canyon was targeted by HiRISE based on a previous spectral detection of hematite-rich deposits in the area. Hematite, a common iron-oxide mineral, was first identified here by the Mars Global Surveyor Thermal Emission Spectrometer (TES). In this TES image, red pixels indicate higher abundances of hematite, while the blue and green pixels represent different types of volcanic rocks (e.g., basalt). Hematite in the Meridiani Planum region was also detected with the TES instrument (which we can see with the bright red spot on the Global TES mineral map). As a consequence, Meridiani Planum was the first landing site selected on Mars due to the spectral detection of a mineral that may have formed in the presence of liquid water. Shortly after landing, the Opportunity rover detected the presence of hematite in the form of concretions called "blueberries." The blueberries are found in association with layers of sulfate salt-rich rocks. The salts are hypothesized to have formed through the raising and lowering of the groundwater table. During one such an event, the rock altered to form the hematite-rich blueberries. As the rock was eroded away, the more resistant hematite-rich blueberries were plucked out and concentrated on the plains as a "lag" deposit. Martian blueberries are observed to be scattered across the plains of Meridiani along Opportunity's traverse from Eagle Crater to Endeavor Crater, where Opportunity continues to explore after its mission began over 10 years ago. This infrared-color image close-up highlights what is possibly the hematite-rich deposits nestled between different types of bedrock terraces in Capri Chasma. The bluish terrace is likely volcanic in origin, possibly basaltic, whereas the greenish rocks remain unidentified. The central reddish terrace is possibly where some of the hematite may be concentrated. The higher elevation terrace with the lighter-colored materials is likely a sulfate-rich rock (based on CRISM data in the area). Given the presence of both sulfate salts and hematite in this area, akin to the deposits and associations explored by the Opportunity rover in Meridiani Planum, it might be that these materials in Capri Chasma may share a similar origin. The yellow rectangular box shown on the TES spectral map outlines the corresponding location of the HiRISE image. Although the outline does not appear to contain a high hematite abundance, we note that the lower resolution of TES (about 3 to 6 kilometers per pixel) may exclude smaller exposures and finer sub-pixel details not-yet captured, but could be with HiRISE. A follow-up observation by the CRISM spectrometer may reveal additional details and a spectral signature for hematite in the vicinity at a finer resolution than TES. http://photojournal.jpl.nasa.gov/catalog/PIA21274