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Panoramic Camera of Jet Propulsion Laboratory (JPL)
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Spirit Stuck in Soft Soil on
This view from the panoramic
11/2/09
| Description |
This view from the panoramic camera on NASA's Mars Exploration Rover Spirit shows the terrain surrounding the location called "Troy," where Spirit became embedded in soft soil during the spring of 2009. The hundreds of images combined into this view were taken beginning on the 1,906th Martian day (or sol) of Spirit's mission on Mars (May 14, 2009) and ending on Sol 1943 (June 20, 2009). Near the center of the image, in the distance, lies Husband Hill, where Spirit recorded views from the summit in 2005. For scale, the parallel tracks are about 1 meter (39 inches) apart. The track on the right is more evident because Spirit was driving backwards, dragging its right-front wheel, which no longer rotates. The bright soil in the center foreground is soft material in which Spirit became embedded after the wheels on that side cut through a darker top layer. The composition of different layers in the soil at the site became the subject of intense investigation by tools on Spirit's robotic arm. In recent weeks, Engineers have been using test rovers on Earth to prepare for extracting the sand-trapped Spirit rover. While amnesia-like symptoms in recent days might delay the start of planned drives by Spirit geared towards extricating it, the Mars Exploration Rover team remains hopeful. "If they are intermittent and infrequent, they are a nuisance that would set us back a day or two when they occur. If the condition becomes persistent or frequent, we will need to go to an alternate strategy that avoids depending on flash memory, " said Project Manager John Callas of NASA's Jet Propulsion Laboratory. In these amnesia events, Spirit fails to record data from the day's activities onto the type of computer memory -- non-volatile "flash" memory -- that can retain the data when the rover powers down for its energy-conserving periods of "sleep." Spirit has worked on Mars for more than 69 months in what was originally planned as a three-month mission. |
| Date |
11/2/09 |
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Mars 2003 Rover
This artist's rendering show
7/27/00
| Date |
7/27/00 |
| Description |
This artist's rendering shows a view of NASA's Mars 2003 Rover as it sets off roam the surface of the red planet. The rover is scheduled for launch in June 2003 and will arrive in January 2004, shielded in its landing by an airbag shell. The airbag/lander structure, which has no scientific instruments of its own, is shown to the right in this image, behind the rover. The rover will carry five scientific instruments and rock abrading device. The Panoramic Camera and the Miniature Thermal Emission Spectrometer are located on the large mast shown on the front of the rover. The camera will be supplied by NASA's Jet Propulsion Laboratory, Pasadena, Calif., and the spectrometer will be supplied by Arizona State University in Tempe. The payload also includes magnetic targets, provided by the Niels Bohr Institute in Copenhagen, Denmark, that will collect magnetic dust for further study by the science instruments. The Rock Abrasion Tool is located on a robotic arm that can be deployed to study rocks and soil.(In this view, the robotic arm is tucked under the front of the rover.) The tool, provided by Honeybee Robotics Ltd., New York, N.Y., will grind away the outer surfaces of rocks, which may be dusty and weathered, allowing the science instruments to determine the nature of rock interiors. The three instruments that will study the abraded rocks are a Mossbauer Spectrometer, provided by the Johannes Gutenberg- University Mainz, Germany, an Alpha-Proton X-ray Spectrometer provided by Max Planck Institute for Chemistry, also in Mainz, Germany, and a Microscopic Imager, supplied by JPL. The payload also includes magnetic targets, provided by the Niels Bohr Institute in Copenhagen, Denmark, that will collect magnetic dust for further study by the science instruments. In a landing similar to that of the 1997 Mars Pathfinder spacecraft, a parachute will deploy to slow the spacecraft down and airbags will inflate to cushion the landing. Petals of the landing structure will unfold to release the rover, which will drive off to begin its exploration. JPL manages the Mars 2003 Rover for NASA's Office of Space Science, Washington, D.C. JPL is a division of the California Institute of Technology in Pasadena. Cornell University, Ithaca, NY is the lead institution for the science payload. ##### |
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Mars 2003 Rover
This artist's rendering show
7/27/00
| Date |
7/27/00 |
| Description |
This artist's rendering shows a side view of NASA's Mars 2003 Rover as it sets off on its exploration of the red planet. The rover is scheduled for launch in June 2003 and will arrive at Mars in January 2004 with an airbag-shielded landing shell. The Mars 2003 Rover will carry five scientific instruments and a rock abrading tool. The instruments include a Panoramic Camera and a Miniature Thermal Emission Spectrometer, both on the large mast shown on the front of the rover. A Mossbauer Spectrometer, an Alpha-Proton X-ray Spectrometer, and a Microscopic Imager are located on a robotic arm that is tucked under the front of the rover, as is a Rock Abrasion Tool that will grind away the outer surfaces of rocks to determine the nature of rock interiors. NASA's Jet Propulsion Laboratory, Pasadena, Calif., manages the Mars 2003 Rover for NASA's Office of Space Science, Washington, D.C. JPL is a division of the California Institute of Technology in Pasadena. Cornell University, Ithaca, NY is the lead institution for the science payload. ##### |
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Empty Nest
| title |
Empty Nest |
| date |
01.18.2004 |
| description |
This image mosaic taken by the panoramic camera onboard the Mars Exploration Rover Spirit shows the rover's landing site, the Columbia Memorial Station, at Gusev Crater, Mars. This spectacular view may encapsulate Spirit's entire journey, from lander to its possible final destination toward the east hills. On its way, the rover will travel 250 meters (820 feet) northeast to a large crater approximately 200 meters (660 feet) across, the ridge of which can be seen to the left of this image. To the right are the east hills, about 3 kilometers (2 miles) away from the lander. The picture was taken on the 16th martian day, or sol, of the mission (Jan. 18/19, 2004). A portion of Spirit's solar panels appear in the foreground. Data from the panoramic camera's green, blue and infrared filters were combined to create this approximate true color image. *Image Credit*: NASA/JPL/Cornell |
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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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Rover Spirit Gets a Cleaning
| title |
Rover Spirit Gets a Cleaning |
| date |
03.23.2005 |
| description |
These two images from 10 days apart show that dust was removed from the panoramic camera's calibration target on NASA's Mars Exploration Rover Spirit. Spirit's panoramic camera took the picture on the left on the rover's 416th martian day, or sol, (March 5, 2005) and took the picture on the right on sol 426 (March 15, 2005). During the time in-between, other evidence of dust-lifting winds were a jump in power output by Spirit's solar arrays on sol 420 from removal of some accumulated dust, and sighting of two dust devils in sol 421 images from Spirit. The size of the base plate on the calibration target shown in both of these images is 8 centimeters (3.15 inches) on each side. These are the panoramic camera team's best current attempt at generating "true color" views of what these scenes would look like if viewed by a human on Mars. They were generated from mathematical combinations of six calibrated, left-eye Pancam images for each sequence, using filters ranging from 430-nanometer to 750-nanometer wavelengths. Image credit: NASA/JPL/Cornell |
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Two Moons Passing in the Nig
| title |
Two Moons Passing in the Night |
| date |
08.26.2005 |
| description |
Taking advantage of extra solar energy collected during the day, NASA's Mars Exploration Rover Spirit settled in for an evening of stargazing, photographing the two moons of Mars as they crossed the night sky. "It is incredibly cool to be running an observatory on another planet," said planetary scientist Jim Bell of Cornell University, Ithaca, N.Y., lead scientist for the panoramic cameras on Spirit and Opportunity. In this animation, both martian moons, Deimos on the left and Phobos on the right, travel across the night sky in front of the constellation Sagittarius. Part of Sagittarius resembles an upside-down teapot. Phobos is the brighter object on the right, Deimos is on the left. Spirit acquired these enhanced-brightness images with the panoramic camera on the night of sol 585 (Aug. 26, 2005). Scientists will use images of the two moons to better map their orbital positions, learn more about their composition, and monitor the presence of nighttime clouds or haze. Spirit took the six images that make up this animation using the camera's broadband filter, which was designed specifically for acquiring images under low-light conditions. *Image credit:* NASA/JPL/Cornell/ Texas A&M |
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Mars Rover Panorama Shows Vi
| title |
Mars Rover Panorama Shows Vista From 'Lookout' Point |
| date |
04.29.2005 |
| description |
From a ridgeline vantage point overlooking slopes, valleys and plains, NASA's Mars Exploration Rover Spirit has returned its latest color panorama of the martian landscape. The approximately true color image shows a full 360-degree view from a site informally named "Larry's Lookout," about halfway up "Husband Hill." Dr. Jim Bell of Cornell University, Ithaca, N.Y., lead scientist for the panoramic cameras on both the Spirit and Opportunity Mars rovers, said, "Spirit and the rover team worked hard over many weeks to get to this vantage point along the flanks of Husband Hill. The rugged ridge and valley terrain seen here is similar in some respects to the view seen months earlier at the 'West Spur,' but the chemistry and mineralogy here are significantly different. Specifically, some of the areas seen here amid the outcrop rocks and in places where the subsurface was exposed by the rover wheels contain the highest sulfur abundances ever measured by Spirit." The view includes the summit of Husband Hill about 200 meters (about 660 feet) southward and about 45 meters (about 150 feet) higher. As Spirit continues uphill, scientists are looking for evidence about whether the intensity of water- related alteration increases with elevation or whether there are pockets of more heavily altered rocks and soils scattered throughout the hills. Spirit's panoramic camera took more than 300 individual frames between Feb. 27 and March 2 that are combined into the big picture. Downloading the frames to Earth took several weeks, and processing took additional time. Imaging specialists at Cornell and at NASA's Jet Propulsion Laboratory, Pasadena, Calif., calibrated the color and assembled the image. Spirit and its twin, Opportunity, successfully completed three-month primary missions a year ago. In extended missions since then, they have been exploring at increasing distances from their landing sites. JPL, a division of the California Institute of Technology in Pasadena, manages NASA's Mars Exploration Rover project for NASA's Science Mission Directorate, Washington. Spirit's "Lookout" panorama is also available online at http://www.nasa.gov/vision/universe/solarsystem/mer_main.html [ http://www.nasa.gov/vision/universe/solarsystem/mer_main.html ]and http://marsrovers.jpl.nasa.gov [ http://marsrovers.jpl.nasa.gov/ ] . |
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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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Earth From Mars
| title |
Earth From Mars |
| date |
03.08.2004 |
| description |
This is the first image ever taken of Earth from the surface of a planet beyond the Moon. It was taken by the Mars Exploration Rover Spirit one hour before sunrise on the 63rd Martian day, or sol, of its mission. The image is a mosaic of images taken by the rover's navigation camera showing a broad view of the sky, and an image taken by the rover's panoramic camera of Earth. The contrast in the panoramic camera image was increased two times to make Earth easier to see.The inset shows a combination of four panoramic camera images zoomed in on Earth. The arrow points to Earth. Earth was too faint to be detected in images taken with the panoramic camera's color filters. *Image Credit*: NASA/JPL/Cornell/Texas A&M |
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A Bird's-Eye View of Erebus
| title |
A Bird's-Eye View of Erebus |
| date |
11.23.2005 |
| description |
This false-color view combines frames taken by the panoramic camera on NASA's Mars Exploration Rover Opportunity on the rover's 652 through 663 Martian days, or sols (Nov. 23 to Dec. 5, 2005), at the edge of Erebus Crater. The mosaic is presented as a vertical projection. This type of projection provides a true-to-scale overhead view of the rover deck and nearby surrounding terrain. The view here shows outcrop rocks, sand dunes, and other features out to a distance of about 25 meters (82 feet) from the rover. Opportunity examined targets on the outcrop called "Rimrock" in front of the rover, testing the mobility and operation of Opportunity's robotic arm. The view shows examples of the dunes and ripples that Opportunity has been crossing as the rover drives on the Meridiani plains. Image credit: NASA/JPL-Caltech/Cornell |
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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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Opportunity's Second Martian
| title |
Opportunity's Second Martian Birthday at Cape Verde |
| date |
10.20.2007 |
| description |
A promontory nicknamed "Cape Verde" can be seen jutting out from the walls of Victoria Crater in this approximate true-color picture taken by the panoramic camera on NASA's Mars Exploration Rover Opportunity. The rover took this picture on martian day, or sol, 1329 (Oct. 20, 2007), more than a month after it began descending down the crater walls - and just 9 sols shy of its second Martian birthday on sol 1338 (Oct. 29, 2007). Opportunity landed on the Red Planet on Jan. 25, 2004. That's nearly four years ago on Earth, but only two on Mars because Mars takes longer to travel around the sun than Earth. One Martian year equals 687 Earth days. The overall soft quality of the image, and the "haze" seen in the lower right portion, are the result of scattered light from dust on the front sapphire window of the rover's camera. This view was taken using three panoramic-camera filters, admitting light with wavelengths centered at 750 nanometers (near infrared), 530 nanometers (green) and 430 nanometers (violet). Image Credit: NASA/JPL-Caltech/Cornell |
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Red Planet
| title |
Red Planet |
| description |
This is the first color image of Mars taken by the panoramic camera on the Mars Exploration Rover Spirit. It is the highest resolution image ever taken on the surface of another planet. A high-resolution TIFF version of this image is available at http://photojournal.jpl.nasa.gov/catalog/?IDNumber=pia04995. *Image credit*: NASA/JPL/Cornell University |
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Peeking Out
| title |
Peeking Out |
| description |
From its new location at the inner edge of the small crater surrounding it, the Mars Exploration Rover Opportunity was able to look out to the plains where its backshell (left) and parachute (right) landed. This approximate true-color image was created by combining data from the panoramic camera's red, green and blue filters. *Image credit*: NASA/JPL/Cornell |
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Rover Eyes
| title |
Rover Eyes |
| description |
This image taken shows the panoramic camera used onboard both Mars Exploration Rovers. The panel to the lower right highlights the multicolored filter wheel that allows the camera to see a rainbow of colors, in addition to infrared bands of light. By seeing Mars in all its colors, scientists can gain insight into the different minerals that constitute its rocks and soil. *Image Credit*: NASA/JPL |
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Still Going
| title |
Still Going |
| date |
09.26.2004 |
| description |
This frame from Spirit's panoramic camera is the 50,000th image from NASA's pair of Mars Exploration Rovers. It shows the camera's calibration target, the most photographed subject on Mars, with a glimpse past it to rocks and soil at the location in the "Columbia Hills" where Spirit was examining soil during its 260th martian day, or sol (Sept. 25, 2004). The outer circle of the calibration target is 8 centimeters (3.15 inches) in diameter. The target includes reference colors and a shadow-casting post. Most days when the panoramic camera is used, it takes a series of images of the calibration target through different filters to aid in accurate interpretation of the other images it takes. This frame was taken by the left eye of the camera's stereo pair, through a red-orange filter admitting light with wavelengths centered at 600 nanometers. *Image Credit*: NASA/JPL/Cornell |
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Size Comparison, Mars Scienc
| title |
Size Comparison, Mars Science Laboratory and Mars Exploration Rover |
| description |
An artist's concept of NASA's Mars Science Laboratory (left) serves to compare it with Spirit, one of NASA's twin Mars Exploration Rovers. Mars Science Laboratory is in development for a launch opportunity in 2009, a landing on Mars in 2010 and investigation of that planet's past or present ability to sustain microbial life. The images of Spirit and the more advanced rover are both superimposed by special effects on a scene from Mars'"Columbia Hills," photographed by Spirit's panoramic camera on April 13, 2005, and presented here in false color (see Next Stop: Methuselah [PIA07855]). Image Credit: NASA/JPL-Caltech |
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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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Attacking Mars
| Title |
Attacking Mars |
| Explanation |
The Spirit rover [ http://marsrovers.jpl.nasa.gov/overview/ ] attacked Mars again in 2005 September. What might look, above, like a military attack, though, was once again just a scientific one - Spirit was instructed to closely inspect some interesting rocks near the summit of Husband Hill [ http://antwrp.gsfc.nasa.gov/apod/ap060703.html ]. Spirit's Panoramic Camera [ http://pancam.astro.cornell.edu/pancam_instrument/projects_2.html ] captured the rover's Instrument Deployment Device above as moved to get a closer look at an outcrop of rocks [ http://antwrp.gsfc.nasa.gov/apod/ap991030.html ] named Hillary [ http://en.wikipedia.org/wiki/Sir_Edmund_Hillary ]. The Spirit rover [ http://antwrp.gsfc.nasa.gov/apod/ap061206.html ], and its twin rover Opportunity [ http://antwrp.gsfc.nasa.gov/apod/ap051214.html ], have now been exploring the red planet [ http://www.nineplanets.org/mars.html ] for over three years [ http://marsrovers.jpl.nasa.gov/newsroom/pressreleases/20061228a.html ]. Both Spirit and Opportunity have found evidence that parts of Mars were once wet [ http://antwrp.gsfc.nasa.gov/apod/ap040310.html ]. |
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Red Mars from Spirit
| Title |
Red Mars from Spirit |
| Explanation |
Rocks are strewn across the broad, flat Gusev crater floor in this sharp color picture [ http://www.jpl.nasa.gov/mer2004/rover-images/jan-06-2004/ captions/image-1.html ] from NASA's Spirit rover [ http://marsrovers.jpl.nasa.gov/mission/ spacecraft_surface_rover.html ]. Recorded by the rover's panoramic camera [ http://marsrovers.jpl.nasa.gov/mission/ spacecraft_instru_pancam.html ], the picture is part of Spirit's first color image [ http://www.jpl.nasa.gov/releases/2004/10.cfm ] of Mars - the highest resolution picture yet taken on the surface of another planet. Already revealing alluring and perplexing [ http://www.jpl.nasa.gov/mer2004/rover-images/jan-06-2004/ captions/image-5.html ] details of an apparently windswept [ http://www.jpl.nasa.gov/mer2004/rover-images/jan-06-2004/ captions/image-4.html ] plain thought to be an ancient lake bed [ http://antwrp.gsfc.nasa.gov/apod/ap020627.html ], this stunning view represents only a small fraction of the color image data mission scientists expect to be transmitted in the coming days. As the robotic Spirit rover is preparing [ http://marsrovers.jpl.nasa.gov/mission/tl_rover.html ] to stand up, roll off the lander, and explore [ http://marsrovers.jpl.nasa.gov/science/goals.html ] the geology of the crater floor, NASA has announced plans to rename the landing site the Columbia Memorial Station [ http://www.jpl.nasa.gov/releases/2004/6.cfm ] in honor of the astronauts [ http://antwrp.gsfc.nasa.gov/apod/ap030203.html ] lost in the Columbia space shuttle accident. |
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A Mars Panorama from the Spi
| Title |
A Mars Panorama from the Spirit Rover |
| Explanation |
If you could stand on Mars -- what would you see? Scrolling right will reveal a full color 360-degree panoramic [ http://marsrovers.jpl.nasa.gov/gallery/press/spirit/20040113a.html ] view from NASA's Spirit Rover [ http://marsrovers.jpl.nasa.gov/overview/ ] that landed on Mars just 10 days ago. The image [ http://photojournal.jpl.nasa.gov/catalog/PIA05058 ] is a digital mosaic from the panoramic camera that shows the view in every direction. Annotated on the image [ http://marsrovers.jpl.nasa.gov/gallery/press/spirit/20040113a.html ] are the directions and distances to various hills along the horizon [ http://marsoweb.nas.nasa.gov/landingsites/mer2003/topsites/final/Gusev/ ]. These hills are valuable for orienting Spirit since they are also visible to the Mars Global Surveyor [ http://antwrp.gsfc.nasa.gov/apod/ap970911.html ] and Mars Odyssey [ http://antwrp.gsfc.nasa.gov/apod/ap011025.html ] spacecraft orbiting high overhead. Visible in the foreground are several instruments and airbags around Columbia Memorial Station [ http://www.jpl.nasa.gov/releases/2004/6.cfm ]. Spirit will attempt to roll [ http://antwrp.gsfc.nasa.gov/apod/ap991030.html ] onto the red planet [ http://www.nineplanets.org/mars.html ] in the next few days and explore interesting features [ http://antwrp.gsfc.nasa.gov/apod/ap040109.html ]. |
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The Hills of Mars
| Title |
The Hills of Mars |
| Explanation |
Distant hills rise above a rocky, windswept plain in this sharp stereo scene [ http://www.jpl.nasa.gov/mer2004/rover-images/jan-07-2004/ captions/image-1.html ] from the Spirit rover on Mars [ http://www.giss.nasa.gov/tools/mars24/ ]. When viewed with red/blue glasses, the picture combines left and right images from Spirit's high resolution panoramic camera [ http://marsrovers.jpl.nasa.gov/mission/ spacecraft_instru_pancam.html ] to yield a dramatic 3D perspective. The hills were estimated to lie about 2 kilometers away and be approximately 50 to 100 meters high. Along with other features of the landscape, determining their direction and distance will help pinpoint the exact location [ http://www.msss.com/mer_mission/finding_mer/ ] of the Spirit landing site when compared with high resolution images of the region taken from Mars orbit [ http://www.msss.com/mars_images/moc/2004/01/03/ ]. Much stereo [ http://antwrp.gsfc.nasa.gov/apod/ap030111.html ] image data, allowing important estimates of three dimensional shapes, sizes, and distances, is anticipated from the rover's cameras. ("Editor's note:" Red/blue glasses for viewing stereo pictures can be purchased [ http://photojournal.jpl.nasa.gov/Help/ VendorList.html#Glasses ] or simply constructed [ http://faxmentis.org/html/ ana-howto.html#glasses ] using red and blue plastic for filters. Try it! To view this image, the red filter is used for the left eye.) |
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Opportunity's Horizon
| Title |
Opportunity's Horizon |
| Explanation |
Remarkably, the Opportunity Mars rover lies in a small martian impact crater [ http://www.jpl.nasa.gov/mer2004/rover-images/jan-30-2004/ captions/image-3.html ] about 3 meters deep and 22 meters wide. For 360 degrees, Opportunity's horizon stretches to the right in this new color mosaic image [ http://www.jpl.nasa.gov/mer2004/rover-images/feb-02-2004/ captions/image-1.html ] from the rover's panoramic camera. Notable in this view of the generally dark, smooth terrain [ http://antwrp.gsfc.nasa.gov/apod/ap040126.html ] are surface imprints left by the lander's airbags [ http://www.jpl.nasa.gov/mer2004/rover-images/jan-28-2004/ captions/image-6.html ] and an outcropping of light-colored, layered rock about 8 meters away toward the northwest. Though they look imposing, the rocks in the tantalizing outcrop are only a few centimeters high and will be dwarfed by the cart-sized rover [ http://marsrovers.jpl.nasa.gov/mission/ spacecraft_surface_rover.html ] itself during future close-up investigations. Opportunity has now rolled off its lander and, along with the restored Spirit rover [ http://antwrp.gsfc.nasa.gov/apod/ap040114.html ], is directly exploring the martian surface [ http://www.jpl.nasa.gov/releases/2004/49.cfm ]. |
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Razorbacks in Endurance Crat
| Title |
Razorbacks in Endurance Crater |
| Explanation |
Over one year after its launch, robot geologist Opportunity [ http://marsrovers.jpl.nasa.gov/mission/ status_opportunity.html ] has been spending recent sols on Mars inching its way down the slopes of Endurance crater [ http://antwrp.gsfc.nasa.gov/apod/ap040510.html ]. Littered with martian blueberries [ http://antwrp.gsfc.nasa.gov/apod/ap040405.html ], some flat rocks within the crater also seem to have surprising razorbacks [ http://marsrovers.jpl.nasa.gov/gallery/press/ opportunity/20040716a.html ] -- narrow slabs sticking up along their edges. Like the blueberries, it's possible that the sharp, narrow features are related to water. They could be formed by minerals deposited by water in cracks, with the surrounding softer material subsequently eroded away. How narrow are they? The ones pictured here in an enhanced color image [ http://photojournal.jpl.nasa.gov/catalog/PIA06692 ] from Opportunity's [ http://marsrovers.jpl.nasa.gov/gallery/all/ opportunity.html ] panoramic camera are actually only a few centimeters high and about half a centimeter wide. Impressive 3D views [ http://antwrp.gsfc.nasa.gov/apod/lib/razorback_anaglyphs.html ] have been constructed by stereo experimenter P. Vantuyne based on the camera's left and right eye images of the region. |
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Martian Eclipses: Deimos and
| Title |
Martian Eclipses: Deimos and Phobos |
| Description |
[figure removed for brevity, see original site] [figure removed for brevity, see original site] [figure removed for brevity, see original site] Deimos [figure removed for brevity, see original site] Phobos This panel combines the first photographs of solar eclipses by Mars' two moons. The panoramic camera on NASA's Mars Exploration Rover Opportunity captured the images as the first in a planned series of eclipse observations by Opportunity and Spirit. The Deimos image was taken at 03:04 Universal Time on March 4, 2004. This irregularly shaped moon is only 15 kilometers (9 miles) across in its longest dimension. It appears as just a speck in front of the disc of the Sun. The Phobos image was taken as that moon grazed the edge of the solar disc at 02:46 Universal Time on March 7, 2004. Phobos is 27 kilometers (17 miles) in its longest dimension. Its apparent size relative to Deimos is even greater because it orbits much closer to Mars' surface than Deimos does. |
| Date |
03.08.2004 |
|
Martian Moon Eclipses Sun, i
| Title |
Martian Moon Eclipses Sun, in Stages |
| Description |
This panel illustrates the transit of the martian moon Phobos across the Sun. It is made up of images taken by the Mars Exploration Rover Opportunity on the morning of the 45th martian day, or sol, of its mission. This observation will help refine our knowledge of the orbit and position of Phobos. Other spacecraft may be able to take better images of Phobos using this new information. This event is similar to solar eclipses seen on Earth in which our Moon passes in front of the Sun. The images were taken by the rover's panoramic camera. |
| Date |
03.13.2004 |
|
Martian Sunsets More Than Ju
| Title |
Martian Sunsets More Than Just Pretty |
| Description |
This image shows the Sun as it appears on Mars throughout the day. Scientists monitor the dimming of the setting Sun to assess how much dust is in the martian atmosphere. The pictures were taken by the Mars Exploration Rover Spirit's panoramic camera. |
| Date |
01.10.2004 |
|
Hills Over Yonder
| Title |
Hills Over Yonder |
| Description |
[figure removed for brevity, see original site]*Click on the image for Hills Over Yonder (QTVR)* The arrows in this 360-degree panoramic view of the martian surface identify hills and craters on the martian horizon that scientists can easily find with orbiters Mars Global Surveyor and Mars Odyssey. The image was taken on Mars by the panoramic camera on the Mars Exploration Rover Spirit. |
| Date |
01.13.2004 |
|
2003 Rover
| title |
2003 Rover |
| Description |
This artist's rendering shows a view of NASA's Mars 2003 Rover as it sets off roam the surface of the red planet. The rover is scheduled for launch in June 2003 and will arrive in January 2004, shielded in its landing by an airbag shell. The airbag/lander structure, which has no scientific instruments of its own, is shown to the right in this image, behind the rover. The rover will carry five scientific instruments and rock abrading device. The Panoramic Camera and the Miniature Thermal Emission Spectrometer are located on the large mast shown on the front of the rover. The camera will be supplied by NASA's Jet Propulsion Laboratory, Pasadena, Calif., and the spectrometer will be supplied by Arizona State University in Tempe. The payload also includes magnetic targets, provided by the Niels Bohr Institute in Copenhagen, Denmark, that will collect magnetic dust for further study by the science instruments. The Rock Abrasion Tool is located on a robotic arm that can be deployed to study rocks and soil.(In this view, the robotic arm is tucked under the front of the rover.) The tool, provided by Honeybee Robotics Ltd., New York, N.Y., will grind away the outer surfaces of rocks, which may be dusty and weathered, allowing the science instruments to determine the nature of rock interiors. The three instruments that will study the abraded rocks are a Mossbauer Spectrometer, provided by the Johannes Gutenberg- University Mainz, Germany, an Alpha-Proton X-ray Spectrometer provided by Max Planck Institute for Chemistry, also in Mainz, Germany, and a Microscopic Imager, supplied by JPL. The payload also includes magnetic targets, provided by the Niels Bohr Institute in Copenhagen, Denmark, that will collect magnetic dust for further study by the science instruments. In a landing similar to that of the 1997 Mars Pathfinder spacecraft, a parachute will deploy to slow the spacecraft down and airbags will inflate to cushion the landing. Petals of the landing structure will unfold to release the rover, which will drive off to begin its exploration. JPL manages the Mars 2003 Rover for NASA's Office of Space Science, Washington, D.C. JPL is a division of the California Institute of Technology in Pasadena. Cornell University, Ithaca, NY is the lead institution for the science payload. |
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| Description |
Browse Image | Medium Image (129 kB) | Large (20.4 MB) Hi-Res (NASA's Planetary Photojournal) [ http://photojournal.jpl.nasa.gov/catalog/PIA08813 ] |
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Covered Ground
PIA05441
Sol (our sun)
Panoramic Camera
| Title |
Covered Ground |
| Original Caption Released with Image |
This image is a traverse map, illustrating Spirit's path over the last 45 sols. When the rover reached the point called "Laguna Hollow," it had driven 131 meters (430 feet) from Columbia Memorial Station. The rover heading is 45 degrees to the northeast. On the horizon behind the lander looms the landmark informally named "Grissom Hill." Over the relatively flat traverse, Spirit has made observations of rocks such as "Adirondack" and utilized the tools on its arm to investigate soil in several locations. Spirit stayed at "Laguna Hollow" for 3 sols, dug a trench and observed the floor and wall of it with three of the instruments on its arm: the Moessbauer spectrometer, the alpha particle X-ray spectrometer and the microscopic imager. Spirit is about halfway to the edge of the crater dubbed "Bonneville. |
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Spirit Says Goodbye to 'Home
PIA02044
Sol (our sun)
Panoramic Camera
| Title |
Spirit Says Goodbye to 'Home Plate' (False Color) |
| Original Caption Released with Image |
For the past several weeks, Spirit has been examining spectacular layered rocks exposed at "Home Plate." The rover has been driving around the northern and eastern edges of Home Plate, on the way to "McCool Hill." Before departing, Spirit took this image showing some of the most complex layering patterns seen so far at this location. The layered nature of these rocks presents new questions for the rover team. In addition to their chemical properties, which scientists can study using Spirit's spectrometers, these rocks record a detailed history of the physical properties that formed them. In the center of this image, one group of layers slopes downward to the right. The layers above and below this group are more nearly horizontal. Where layers of different orientations intersect, other layers are truncated. This indicates that there were complex patterns of alternating erosion and deposition occurring when these layers were being deposited. Similar patterns can be found in some sedimentary rocks on Earth. Physical relationships among the various layers exposed at Home Plate are crucial evidence in understanding how these Martian rocks formed. Scientists suspect that the rocks at Home Plate were formed in the aftermath of a volcanic explosion or impact event, and they are investigating the possibility that wind may also have played a role in redistributing materials after such an event. Images like this one from panoramic camera (Pancam), which shows larger-scale layering, as well as those from the microscopic imager, which reveal the individual sand-sized grains that make up these rocks, are essential to understanding the geologic history of Home Plate. This view is a false-color rendering that combines separate images taken through the Pancam's 753-nanometer, 535-namometer, and 432-nanometer filters, enhanced to emphasize color differences among the rocks and soils. It was taken during Spirit's 774th Martian day (March 8, 2006). |
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Spirit Says Goodbye to 'Home
PIA02055
Sol (our sun)
Panoramic Camera
| Title |
Spirit Says Goodbye to 'Home Plate' |
| Original Caption Released with Image |
For the past several weeks, Spirit has been examining spectacular layered rocks exposed at "Home Plate." The rover has been driving around the northern and eastern edges of Home Plate, on the way to "McCool Hill." Before departing, Spirit took this image showing some of the most complex layering patterns seen so far at this location. The layered nature of these rocks presents new questions for the rover team. In addition to their chemical properties, which scientists can study using Spirit's spectrometers, these rocks record a detailed history of the physical properties that formed them. In the center of this image, one group of layers slopes downward to the right. The layers above and below this group are more nearly horizontal. Where layers of different orientations intersect, other layers are truncated. This indicates that there were complex patterns of alternating erosion and deposition occurring when these layers were being deposited. Similar patterns can be found in some sedimentary rocks on Earth. Physical relationships among the various layers exposed at Home Plate are crucial evidence in understanding how these Martian rocks formed. Scientists suspect that the rocks at Home Plate were formed in the aftermath of a volcanic explosion or impact event, and they are investigating the possibility that wind may also have played a role in redistributing materials after such an event. Images like this one from panoramic camera (Pancam), which shows larger-scale layering, as well as those from the microscopic imager, which reveal the individual sand-sized grains that make up these rocks, are essential to understanding the geologic history of Home Plate. This view is an approximately true-color rendering that combines separate images taken through the Pancam's 753-nanometer, 535-namometer, and 432-nanometer filters during Spirit's 774th Martian day (March 8, 2006). |
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Martian Eclipses: Deimos and
PIA05518
Panoramic Camera
| Title |
Martian Eclipses: Deimos and Phobos |
| Original Caption Released with Image |
This panel combines the first photographs of solar eclipses by Mars' two moons. The panoramic camera on NASA's Mars Exploration Rover Opportunity captured the images as the first in a planned series of eclipse observations by Opportunity and Spirit. The Deimos image was taken at 03:04 Universal Time on March 4, 2004. This irregularly shaped moon is only 15 kilometers (9 miles) across in its longest dimension. It appears as just a speck in front of the disc of the Sun. The Phobos image was taken as that moon grazed the edge of the solar disc at 02:46 Universal Time on March 7, 2004. Phobos is 27 kilometers (17 miles) in its longest dimension. Its apparent size relative to Deimos is even greater because it orbits much closer to Mars' surface than Deimos does. |
|
Martian Eclipses: Deimos and
PIA05518
Panoramic Camera
| Title |
Martian Eclipses: Deimos and Phobos |
| Original Caption Released with Image |
This panel combines the first photographs of solar eclipses by Mars' two moons. The panoramic camera on NASA's Mars Exploration Rover Opportunity captured the images as the first in a planned series of eclipse observations by Opportunity and Spirit. The Deimos image was taken at 03:04 Universal Time on March 4, 2004. This irregularly shaped moon is only 15 kilometers (9 miles) across in its longest dimension. It appears as just a speck in front of the disc of the Sun. The Phobos image was taken as that moon grazed the edge of the solar disc at 02:46 Universal Time on March 7, 2004. Phobos is 27 kilometers (17 miles) in its longest dimension. Its apparent size relative to Deimos is even greater because it orbits much closer to Mars' surface than Deimos does. |
|
Martian Eclipses: Deimos and
PIA05518
Panoramic Camera
| Title |
Martian Eclipses: Deimos and Phobos |
| Original Caption Released with Image |
This panel combines the first photographs of solar eclipses by Mars' two moons. The panoramic camera on NASA's Mars Exploration Rover Opportunity captured the images as the first in a planned series of eclipse observations by Opportunity and Spirit. The Deimos image was taken at 03:04 Universal Time on March 4, 2004. This irregularly shaped moon is only 15 kilometers (9 miles) across in its longest dimension. It appears as just a speck in front of the disc of the Sun. The Phobos image was taken as that moon grazed the edge of the solar disc at 02:46 Universal Time on March 7, 2004. Phobos is 27 kilometers (17 miles) in its longest dimension. Its apparent size relative to Deimos is even greater because it orbits much closer to Mars' surface than Deimos does. |
|
Martian Eclipses: Deimos and
PIA05518
Panoramic Camera
| Title |
Martian Eclipses: Deimos and Phobos |
| Original Caption Released with Image |
This panel combines the first photographs of solar eclipses by Mars' two moons. The panoramic camera on NASA's Mars Exploration Rover Opportunity captured the images as the first in a planned series of eclipse observations by Opportunity and Spirit. The Deimos image was taken at 03:04 Universal Time on March 4, 2004. This irregularly shaped moon is only 15 kilometers (9 miles) across in its longest dimension. It appears as just a speck in front of the disc of the Sun. The Phobos image was taken as that moon grazed the edge of the solar disc at 02:46 Universal Time on March 7, 2004. Phobos is 27 kilometers (17 miles) in its longest dimension. Its apparent size relative to Deimos is even greater because it orbits much closer to Mars' surface than Deimos does. |
|
Martian Eclipses: Deimos and
PIA05518
Panoramic Camera
| Title |
Martian Eclipses: Deimos and Phobos |
| Original Caption Released with Image |
This panel combines the first photographs of solar eclipses by Mars' two moons. The panoramic camera on NASA's Mars Exploration Rover Opportunity captured the images as the first in a planned series of eclipse observations by Opportunity and Spirit. The Deimos image was taken at 03:04 Universal Time on March 4, 2004. This irregularly shaped moon is only 15 kilometers (9 miles) across in its longest dimension. It appears as just a speck in front of the disc of the Sun. The Phobos image was taken as that moon grazed the edge of the solar disc at 02:46 Universal Time on March 7, 2004. Phobos is 27 kilometers (17 miles) in its longest dimension. Its apparent size relative to Deimos is even greater because it orbits much closer to Mars' surface than Deimos does. |
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Spirit Hits a Home Run
PIA02187
Sol (our sun)
Panoramic Camera
| Title |
Spirit Hits a Home Run |
| Original Caption Released with Image |
This week, NASA's Mars Exploration Rover Spirit arrived at "Home Plate," a feature that, when seen from orbit, looks like the home plate of a baseball diamond. Home Plate is a roughly circular feature about 80 meters (260 feet) in diameter that might be an old impact crater or volcanic feature. The Spirit team has been eager to get to Home Plate and has been enjoying distant views of the feature and a curious "bathtub ring" of light-colored materials along its edges. The team has pushed the rover hard to get here before the deep Martian winter sets in. After scientists had identified Home Plate from orbit, they had many theories about what it could be and what they might see. But when Spirit's panoramic camera (Pancam) took this and other images, the science team was stunned. This Pancam image is of an outcrop nicknamed "Barnhill" and surrounding rocks on the north side of Home Plate, showing the most spectacular layering that Spirit has seen. Pancam and microscopic imager views of the layers in the rocks reveal a range of grain sizes and textures that change from the lower to the upper part of the outcrop. This may help scientists figure out how the material was emplaced. Spirit is also conducting work with its arm instruments to figure out the chemistry and mineralogy of the rocks. Scientists have several hypotheses about what Home Plate could be, including features made by volcanoes and impact craters, and ways that water could have played a role. They are busy trying to figure out what the data from Spirit is really telling us. As Spirit works at Home Plate during February, the science team is choosing informal names for rocks from the great players and managers of the Negro Leagues of baseball. This outcrop, "Barnhill," is informally named for David Barnhill, the ace of the New York Cubans' pitching staff during the early 1940s. He compiled an 18-3 record in 1941 and defeated Satchel Paige in the 1942 East-West all-star game. Other rocks in the area are informally named for Josh Gibson, "Bullet Joe" Rogan, and Cumberland Posey. Stay tuned this month, as the Baseball Hall of Fame elects more players from the Negro Leagues and Spirit continues to examine these spectacular rocks. Spirit took this mosaic of images using the panoramic camera on the rover's 746th day, or sol (Feb. 7, 2006), of exploring Mars. Scientists are acquiring and processing image data for more views of the same terrain in approximate true color. |
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Spirit Studies Rock Outcrop
PIA02686
Sol (our sun)
Panoramic Camera, Rock Abras
| Title |
Spirit Studies Rock Outcrop at 'Home Plate' |
| Original Caption Released with Image |
NASA's Mars Exploration Rover Spirit acquired this false-color image at 11:48 local true solar time on Mars on the rover's 746th Martian day, or sol (Feb. 26, 2006), after using the rock abrasion tool to brush the surfaces of rock targets informally named "Stars" (left) and "Crawfords" (right). Small streaks of dust extend for several centimeters behind the small rock chips and pebbles in the dusty, red soils. Because the rover was looking southwest when this image was taken, the wind streaks indicate that the dominant wind direction was from the southeast. The targets Stars and Crawfords are on a rock outcrop located on top of "Home Plate." The outcrop is informally named "James 'Cool Papa' Bell," after a Negro Leagues Hall of Famer who played for both the Pittsburgh Crawfords and the Kansas City Stars. To some science team members, the two brushed spots resemble the eyes of a face, with rocks below and between the eyes as a nose and layered rocks at the bottom of the image as a mouth. The image combines frames taken by Spirit's panoramic camera through the camera's 753-nanometer, 535-namometer, and 432-nanometer filters. It is enhanced to emphasize color differences among the rocks, soils and brushed areas. The blue circular area on the left, Stars, was brushed on 761 (Feb. 22, 2006). The one on the right, Crawfords, was brushed on sol 763 (Feb. 25, 2006). |
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Stargazing at 'Husband Hill
PIA03070
Sol (our sun)
Panoramic Camera
| Title |
Stargazing at 'Husband Hill Observatory' on Mars |
| Original Caption Released with Image |
NASA's Mars Exploration Rover Spirit continues to take advantage of extra solar energy by occasionally turning its cameras upward for night sky observations. Most recently, Spirit made a series of observations of bright star fields from the summit of "Husband Hill" in Gusev Crater on Mars. Scientists use the images to assess the cameras' sensitivity and to search for evidence of nighttime clouds or haze. The image on the left is a computer simulation of the stars in the constellation Orion. The next three images are actual views of Orion captured with Spirit's panoramic camera during exposures of 10, 30, and 60 seconds. Because Spirit is in the southern hemisphere of Mars, Orion appears upside down compared to how it would appear to viewers in the Northern Hemisphere of Earth. "Star trails" in the longer exposures are a result of the planet's rotation. The faintest stars visible in the 60-second exposure are about as bright as the faintest stars visible with the naked eye from Earth (about magnitude 6 in astronomical terms). The Orion Nebula, famous as a nursery of newly forming stars, is also visible in these images. Bright streaks in some parts of the images aren't stars or meteors or unidentified flying objects, but are caused by solar and galactic cosmic rays striking the camera's detector. Spirit acquired these images with the panoramic camera on Martian day, or sol, 632 (Oct. 13, 2005) at around 45 minutes past midnight local time, using the camera's broadband filter (wavelengths of 739 nanometers plus or minus 338 nanometers). |
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Dodging the Drifts
PIA03065
Sol (our sun)
Panoramic Camera
| Title |
Dodging the Drifts |
| Original Caption Released with Image |
This image taken by NASA's Mars Exploration Rover Opportunity is a portion of a mosaic acquired by the panoramic camera. The picture highlights the light-toned outcrop on the rim of "Erebus Crater" and large, dark, wind-deposited drifts that have filled the center of the crater. Opportunity took this image on the rover's 608th sol (Oct. 9, 2005). The rover is driving west, avoiding the large drifts and crossing the low ripples and outcrop to the right. After traversing to the north of the large drift on the horizon (near the center of the image), Opportunity will drive south to the western rim of the crater. |
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Spirit View of Phobos Eclips
PIA03612
Mars
Panoramic Camera
| Title |
Spirit View of Phobos Eclipse, Sol 675 |
| Original Caption Released with Image |
Annotated Spirit View of Phobos Eclipse, Sol 675 NASA's Mars Exploration Rover Spirit observed the Martian moon Phobos entering the shadow of Mars during the night of the rover's 675th sol (Nov. 27, 2005). The panoramic camera captured 16 images, spaced 10 seconds apart, covering the period from when Phobos was in full sunlight to when it was entirely in shadow. As with our own Moon during lunar eclipses on Earth, even when in the planet's shadow, Phobos was not entirely dark. The small amount of light still visible from Phobos is a kind of "Mars-shine" -- sunlight reflected through Mars' atmosphere and into the shadowed region. This view is a time-lapse composite of images taken 20 seconds apart, showing the movement of Phobos from left to right. (At 10 seconds apart, the images of the moon overlap each other.) Scientists are using information about the precise timing of Martian moon eclipses gained from observations such as these to refine calculations about the orbital path of Phobos. The precise position of Phobos will be important to any future spacecraft taking detailed pictures of the moon or landing on its surface. |
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Spirit View of Phobos Eclips
PIA03612
Mars
Panoramic Camera
| Title |
Spirit View of Phobos Eclipse, Sol 675 |
| Original Caption Released with Image |
Annotated Spirit View of Phobos Eclipse, Sol 675 NASA's Mars Exploration Rover Spirit observed the Martian moon Phobos entering the shadow of Mars during the night of the rover's 675th sol (Nov. 27, 2005). The panoramic camera captured 16 images, spaced 10 seconds apart, covering the period from when Phobos was in full sunlight to when it was entirely in shadow. As with our own Moon during lunar eclipses on Earth, even when in the planet's shadow, Phobos was not entirely dark. The small amount of light still visible from Phobos is a kind of "Mars-shine" -- sunlight reflected through Mars' atmosphere and into the shadowed region. This view is a time-lapse composite of images taken 20 seconds apart, showing the movement of Phobos from left to right. (At 10 seconds apart, the images of the moon overlap each other.) Scientists are using information about the precise timing of Martian moon eclipses gained from observations such as these to refine calculations about the orbital path of Phobos. The precise position of Phobos will be important to any future spacecraft taking detailed pictures of the moon or landing on its surface. |
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Partial 'Seminole' Panorama
PIA03617
Sol (our sun)
Panoramic Camera
| Title |
Partial 'Seminole' Panorama (False Color) |
| Original Caption Released with Image |
This view from Spirit's panoramic camera is assembled from frames acquired on Martian days, or sols, 672 and 673 (Nov. 23 and 24, 2005) from the rover's position near an outcrop called "Seminole." The view is a southward-looking portion of a larger panorama still being completed. This is a false-color version to emphasize geological differences. It is a composite of images shot through three different filters, admitting light of wavelengths 750 nanometers, 530 nanometers and 430 nanometers. |
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Partial 'Seminole' Panorama
PIA03623
Sol (our sun)
Panoramic Camera
| Title |
Partial 'Seminole' Panorama |
| Original Caption Released with Image |
This view from Spirit's panoramic camera is assembled from frames acquired on Martian days, or sols, 672 and 673 (Nov. 23 and 24, 2005) from the rover's position near an outcrop called "Seminole." The view is a southward-looking portion of a larger panorama still being completed. This approximately true-color view is a composite of images shot through three different filters, admitting light of wavelengths 750 nanometers, 530 nanometers and 430 nanometers. |
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Spirit Movie of Phobos Eclip
PIA03611
Mars
Panoramic Camera
| Title |
Spirit Movie of Phobos Eclipse, Sol 675 |
| Original Caption Released with Image |
" Spirit Phobos Eclipse Animation NASA's Mars Exploration Rover Spirit observed the Martian moon Phobos entering the shadow of Mars during the night of the rover's 675th sol (Nov. 27, 2005). The panoramic camera captured 16 images, spaced 10 seconds apart, covering the period from when Phobos was in full sunlight to when it was entirely in shadow. As with our own Moon during lunar eclipses on Earth, even when in the planet's shadow, Phobos was not entirely dark. The small amount of light still visible from Phobos is a kind of "Mars-shine" -- sunlight reflected through Mars' atmosphere and into the shadowed region. This clip is a sequence of the 16 images showing the eclipse at about 10 times normal speed. It shows the movement of Phobos from left to right as the moon enters the shadow. Scientists are using information about the precise timing of Martian moon eclipses gained from observations such as these to refine calculations about the orbital path of Phobos. The precise position of Phobos will be important to any future spacecraft taking detailed pictures of the moon or landing on its surface. |
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Spirit Movie of Phobos Eclip
PIA03611
Mars
Panoramic Camera
| Title |
Spirit Movie of Phobos Eclipse, Sol 675 |
| Original Caption Released with Image |
" Spirit Phobos Eclipse Animation NASA's Mars Exploration Rover Spirit observed the Martian moon Phobos entering the shadow of Mars during the night of the rover's 675th sol (Nov. 27, 2005). The panoramic camera captured 16 images, spaced 10 seconds apart, covering the period from when Phobos was in full sunlight to when it was entirely in shadow. As with our own Moon during lunar eclipses on Earth, even when in the planet's shadow, Phobos was not entirely dark. The small amount of light still visible from Phobos is a kind of "Mars-shine" -- sunlight reflected through Mars' atmosphere and into the shadowed region. This clip is a sequence of the 16 images showing the eclipse at about 10 times normal speed. It shows the movement of Phobos from left to right as the moon enters the shadow. Scientists are using information about the precise timing of Martian moon eclipses gained from observations such as these to refine calculations about the orbital path of Phobos. The precise position of Phobos will be important to any future spacecraft taking detailed pictures of the moon or landing on its surface. |
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'Algonquin' Outcrop on Spiri
PIA03614
Sol (our sun)
Panoramic Camera
| Title |
'Algonquin' Outcrop on Spirit's Sol 680 |
| Original Caption Released with Image |
This view combines four frames from Spirit's panoramic camera, looking in the drive direction on the rover's 680th Martian day, or sol (Dec. 1, 2005). The outcrop of apparently layered bedrock has the informal name "Algonquin." |
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