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Galerie de photos de Europe, satellite galiléen de la planète Jupiter

<h1>PIA01183:  Europa Wedge Region</h1><div class="PIA01183" lang="en" style="width:798px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;">This image shows an area of crustal separation on Jupiter's moon, Europa. Lower resolution pictures taken earlier in the tour of NASA's Galileo spacecraft revealed that dark wedge-shaped bands in this region are areas where the icy crust has completely pulled apart. Dark material has filled up from below and filled the void created by this separation.<p>In the lower left corner of this image, taken by Galileo's onboard camera on December 16, 1997, a portion of one dark wedge area is visible, revealing a linear texture along the trend of the wedge. The lines of the texture change orientation slightly and reflect the fact that we are looking at a bend in the wedge. The older, bright background, visible on the right half of the image, is criss-crossed with ridges. A large, bright ridge runs east-west through the upper part of the image, cutting across both the older background plains and the wedge. This ridge is rough in texture, with numerous small terraces and troughs containing dark material.<p>North is to the top of the picture and the sun illuminates the surface from the northwest. This image, centered at approximately 16.5 degrees south latitude and 196.5 degrees west longitude, covers an area approximately 10 kilometers square (about 6.5 miles square). The resolution of this image is about 26 meters per picture element. This image was taken by the solid state imaging system from a distance of 1250 kilometers (750 miles).<p>The Jet Propulsion Laboratory, Pasadena, CA manages the Galileo mission for NASA's Office of Space Science, Washington, DC. JPL is an operating division of California Institute of Technology (Caltech).<p>This image and other images and data received from Galileo are posted on the World Wide Web, on the Galileo mission home page at URL http://www.jpl.nasa.gov/ galileo.<br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01183" onclick="window.open(this.href); return false;" title="Voir l'image 	 PIA01183:  Europa Wedge Region	  sur le site de la NASA">Voir l'image 	 PIA01183:  Europa Wedge Region	  sur le site de la NASA.</a></div>
PIA01183: Europa Wedge Region
<h1>PIA01211:  Pwyll Crater on Europa</h1><div class="PIA01211" lang="en" style="width:800px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;">This enhanced color image of the region surrounding the young impact crater Pwyll on Jupiter's moon Europa was produced by combining low resolution color data with a higher resolution mosaic of images obtained on December 19, 1996 by the Solid State Imaging (CCD) system aboard NASA's Galileo spacecraft. This region is on the trailing hemisphere of the satellite, centered at 11 degrees South and 276 degrees West, and is about 1240 kilometers across. North is toward the top of the image, and the sun illuminates the surface from the east.<p>The 26 kilometer diameter impact crater Pwyll, just below the center of the image, is thought to be one of the youngest features on the surface of Europa. The diameter of the central dark spot, ejecta blasted from beneath Europa's surface, is approximately 40 kilometers, and bright white rays extend for over a thousand kilometers in all directions from the impact site. These rays cross over many different terrain types, indicating that they are younger than anything they cross. Their bright white color may indicate that they are composed of fresh, fine water ice particles, as opposed to the blue and brown tints of older materials elsewhere in the image.<p>Also visible in this image are a number of the dark lineaments which are called "triple bands" because they have a bright central stripe surrounded by darker material. Scientists can use the order in which these bands cross each other to determine their relative ages, as they attempt to reconstruct the geologic history of Europa.<p>The Jet Propulsion Laboratory, Pasadena, CA manages the mission for NASA's Office of Space Science, Washington, DC.<p>This image and other images and data received from Galileo are posted on the World Wide Web, on the Galileo mission home page at URL http://galileo.jpl.nasa.gov. Background information and educational context for the images can be found at <a href="http://www2.jpl.nasa.gov/galileo/sepo/" target="_blank">http://www.jpl.nasa.gov/galileo/sepo</a>..<br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01211" onclick="window.open(this.href); return false;" title="Voir l'image 	 PIA01211:  Pwyll Crater on Europa	  sur le site de la NASA">Voir l'image 	 PIA01211:  Pwyll Crater on Europa	  sur le site de la NASA.</a></div>
PIA01211: Pwyll Crater on Europa
<h1>PIA01212:  Near-Terminator Image of Europa</h1><div class="PIA01212" lang="en" style="width:800px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;">This image of Europa's surface was obtained by the Solid State Imaging (CCD) system on board NASA's Galileo spacecraft during its fourth orbit of Jupiter, Linear features with bright central stripes referred to as "triple bands" are seen to transect the surface of Europa. Several of these triple bands are over 700 kilometers in length. In the left side of the image the surface of Europa is seen to be locally pitted and irregular. Ridges less than 100 kilometers in length are also visible in this region.<p>The area seen in this image, centered near 27 degrees South, 300 degrees West, is 760 kilometers (456 miles) by 850 kilometers (510 miles) across, which is approximately the size of the state of Texas or the country of France. North is to the top of the image, with the sun illuminating the surface from the left. The image which has a resolution of 1.3 kilometers per picture element (pixel) was obtained on December 19th, 1996 (Universal Time).<p>The Jet Propulsion Laboratory, Pasadena, CA manages the mission for NASA's Office of Space Science, Washington, DC.<p>This image and other images and data received from Galileo are posted on the World Wide Web, on the Galileo mission home page at URL http://galileo.jpl.nasa.gov. Background information and educational context for the images can be found at <a href="http://www2.jpl.nasa.gov/galileo/sepo/" target="_blank">http://www.jpl.nasa.gov/galileo/sepo</a>..<br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01212" onclick="window.open(this.href); return false;" title="Voir l'image 	 PIA01212:  Near-Terminator Image of Europa	  sur le site de la NASA">Voir l'image 	 PIA01212:  Near-Terminator Image of Europa	  sur le site de la NASA.</a></div>
PIA01212: Near-Terminator Image of Europa
<h1>PIA01216:  Very High Resolution Image of Icy Cliffs on Europa and Similar Scales on Earth (Providence, RI)</h1><div class="PIA01216" lang="en" style="width:760px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;">The top image is a very high resolution view of the Conamara Chaos region on Jupiter's moon Europa, showing an area where icy plates have been broken apart and moved around laterally. The top of this image is dominated by corrugated plateaus ending in icy cliffs over a hundred meters (a few hundred feet) high. Debris piled at the base of the cliffs. The bottom image is an aerial photograph of downtown Providence, Rhode Island at the same scale. The bright white circular feature in the top center of the Providence image is an indoor hockey rink, and one can find many craters in the Europa image about the same size. Blocks of debris which have fallen from the cliffs on the Europa image are about the same size as houses seen in the Providence image, and the largest blocks are almost as large as the Rhode Island state capitol building (large white building in upper left of Providence image). A fracture that runs horizontally across the center of the Europa image is about the same width as the freeway which runs along the bottom of the Providence image.<p>North is to the top right of the Europa image, and the sun illuminates the surface from the east. The Europa image is centered at approximately 9 degrees north latitude and 274 degrees west longitude. The images each cover an area approximately 1.7 kilometers by 4 kilometers (1 mile by 2.5 miles). The resolution is 9 meters (30 feet) per picture element. The Europa image was taken on December 16, 1997 at a range of 900 kilometers (540 miles) by the solid state imaging system on NASA's Galileo spacecraft.<p>The Jet Propulsion Laboratory, Pasadena, CA manages the Galileo mission for NASA's Office of Space Science, Washington, DC. JPL is an operating division of California Institute of Technology (Caltech).<p>This image and other images and data received from Galileo are posted on the World Wide Web, on the Galileo mission home page at URL http://www.jpl.nasa.gov/ galileo.<br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01216" onclick="window.open(this.href); return false;" title="Voir l'image 	 PIA01216:  Very High Resolution Image of Icy Cliffs on Europa and Similar Scales on Earth (Providence, RI)	  sur le site de la NASA">Voir l'image 	 PIA01216:  Very High Resolution Image of Icy Cliffs on Europa and Similar Scales on Earth (Providence, RI)	  sur le site de la NASA.</a></div>
PIA01216: Very High Resolution Image of Icy Cliffs on Europa and Similar Scales on Earth (Providence, RI)
<h1>PIA01295:  Europa Global Views in Natural and Enhanced Colors</h1><div class="PIA01295" lang="en" style="width:520px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p>This color composite view combines violet, green, and infrared images of Jupiter's intriguing moon, Europa, for a view of the moon in natural color (left) and in enhanced color designed to bring out subtle color differences in the surface (right). The bright white and bluish part of Europa's surface is composed mostly of water ice, with very few non-ice materials. In contrast, the brownish mottled regions on the right side of the image may be covered by hydrated salts and an unknown red component. The yellowish mottled terrain on the left side of the image is caused by some other unknown component. Long, dark lines are fractures in the crust, some of which are more than 3,000 kilometers (1,850 miles) long.<p>North is to the top of the picture and the sun fully illuminates the surface. Europa is about 3,160 kilometers (1,950 miles) in diameter, or about the size of Earth's moon. The finest details that can be discerned are 25 kilometers across. The images in this global view were taken in June 1997 at a range of 1.25 million kilometers by the Solid State Imaging (SSI) system on NASA's Galileo spacecraft, during its ninth orbit of Jupiter.<p>The Jet Propulsion Laboratory, Pasadena, CA manages the Galileo mission for NASA's Office of Space Science, Washington, DC. JPL is an operating division of California Institute of Technology (Caltech).<p>This image and other images and data received from Galileo are posted on the World Wide Web, on the Galileo mission home page at URL http://galileo.jpl.nasa.gov. Background information and educational context for the images can be found at <a href="http://www2.jpl.nasa.gov/galileo/sepo/" target="_blank">http://www.jpl.nasa.gov/galileo/sepo</a>..<br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01295" onclick="window.open(this.href); return false;" title="Voir l'image 	 PIA01295:  Europa Global Views in Natural and Enhanced Colors	  sur le site de la NASA">Voir l'image 	 PIA01295:  Europa Global Views in Natural and Enhanced Colors	  sur le site de la NASA.</a></div>
PIA01295: Europa Global Views in Natural and Enhanced Colors
<h1>PIA01296:  Europa "Ice Rafts" in Local and Color Context</h1><div class="PIA01296" lang="en" style="width:800px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p>This image of Jupiter's icy satellite Europa shows surface features such as domes and ridges, as well as a region of disrupted terrain including crustal plates which are thought to have broken apart and "rafted" into new positions. The image covers an area of Europa's surface about 250 by 200 kilometer (km) and is centered at 10 degrees latitude, 271 degrees longitude. The color information allows the surface to be divided into three distinct spectral units. The bright white areas are ejecta rays from the relatively young crater Pwyll, which is located about 1000 km to the south (bottom) of this image. These patchy deposits appear to be superposed on other areas of the surface, and thus are thought to be the youngest features present. Also visible are reddish areas which correspond to locations where non-ice components are present. This coloring can be seen along the ridges, in the region of disrupted terrain in the center of the image, and near the dome-like features where the surface may have been thermally altered. Thus, areas associated with internal geologic activity appear reddish. The third distinct color unit is bright blue, and corresponds to the relatively old icy plains.<p>This product combines data taken by the Solid State Imaging (SSI) system on NASA's Galileo spacecraft during three separate flybys of Europa. Low resolution color data (violet, green, and 1 micron) acquired in September 1996 were combined with medium resolution images from December 1996, to produce synthetic color images. These were then combined with a high resolution mosaic of images acquired in February 1997.<p>The Jet Propulsion Laboratory, Pasadena, CA manages the Galileo mission for NASA's Office of Space Science, Washington, DC. JPL is an operating division of California Institute of Technology (Caltech).<p>This image and other images and data received from Galileo are posted on the World Wide Web, on the Galileo mission home page at URL http://galileo.jpl.nasa.gov. Background information and educational context for the images can be found at <a href="http://www2.jpl.nasa.gov/galileo/sepo/" target="_blank">http://www.jpl.nasa.gov/galileo/sepo</a>..<br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01296" onclick="window.open(this.href); return false;" title="Voir l'image 	 PIA01296:  Europa "Ice Rafts" in Local and Color Context	  sur le site de la NASA">Voir l'image 	 PIA01296:  Europa "Ice Rafts" in Local and Color Context	  sur le site de la NASA.</a></div>
PIA01296: Europa "Ice Rafts" in Local and Color Context
<h1>PIA01401:  Scrambled Ice</h1><div class="PIA01401" lang="en" style="width:800px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;">This complex area on the side of Europa which faces away from Jupiter shows several types of features which are formed by disruptions of Europa's icy crust. North is to the top of the image, taken by NASA's Galileo spacecraft, and the Sun illuminates the surface from the left. The prominent wide, dark bands are up to 20 kilometers (12 miles) wide and over 50 kilometers (30 miles) long. They are believed to have formed when Europa's icy crust fractured, separated and filled in with darker, "dirtier" ice or slush from below. A relatively rare type of feature on Europa is the 15-kilometer-diameter (9.3-mile) impact crater in the lower left corner. The small number of impact craters on Europa's surface is an indication of its relatively young age. A region of chaotic terrain south of this impact crater contains crustal plates which have broken apart and rafted into new positions. Some of these "ice rafts" are nearly 1 kilometer (about half a mile) across. Other regions of chaotic terrain are visible and indicate heating and disruption of Europa's icy crust from below. The youngest features in this scene are the long, narrow cracks in the ice which cut across all other features. One of these cracks is about 30 kilometers (18 miles) to the right of the impact crater and extends for hundreds of miles from the top to the bottom of the image.<p>The image, centered near 23 degrees south latitude and 179 degrees longitude, covers an area about 240 by 215 kilometers (150 by 130 miles) across. The finest details that can be discerned in this picture are about 460 meters (500 yards) across. The image was taken as Galileo flew by Europa on March 29, 1998. The image was taken by the onboard solid state imaging system camera from an altitude of 23,000 kilometers (14,000 miles).<p>The Jet Propulsion Laboratory, Pasadena, CA manages the Galileo mission for NASA's Office of Space Science, Washington, DC. JPL is an operating division of California Institute of Technology (Caltech).<p>This image and other images and data received from Galileo are posted on the World Wide Web, on the Galileo mission home page at URL http://galileo.jpl.nasa.gov. Background information and educational context for the images can be found at <a href="http://www2.jpl.nasa.gov/galileo/sepo/" target="_blank">http://www.jpl.nasa.gov/galileo/sepo</a>..<br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01401" onclick="window.open(this.href); return false;" title="Voir l'image 	 PIA01401:  Scrambled Ice	  sur le site de la NASA">Voir l'image 	 PIA01401:  Scrambled Ice	  sur le site de la NASA.</a></div>
PIA01401: Scrambled Ice
<h1>PIA01403:  A closer look at Chaos on Europa</h1><div class="PIA01403" lang="en" style="width:800px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;">This mosaic of the Conamara Chaos region on Jupiter's moon, Europa, clearly indicates relatively recent resurfacing of Europa's surface. Irregularly shaped blocks of water ice were formed by the break up and movement of the existing crust. The blocks were shifted, rotated, and even tipped and partially submerged within a mobile material that was either liquid water, warm mobile ice, or an ice and water slush. The presence of young fractures cutting through this region indicates that the surface froze again into solid, brittle ice.<p>The background image in this picture was taken during Galileo's sixth orbit of Jupiter in February, 1997. Five very high resolution images which were taken during the spacecraft's twelfth orbit in December, 1997 provide an even closer look at some of the details. This mosaic shows some of the high resolution data inset into the context of this tumultuous region.<p>North is to the top of the picture, and the sun illuminates the scene from the east (right). The picture, centered at 9 degrees north latitude and 274 degrees west longitude, covers an area approximately 35 by 50 kilometers (20 by 30 miles). The finest details visible in the very high resolution insets are about 20 meters (22 yards) across, and in the background image, 100 meters (110 yards) across. The insets were taken on December 16, 1997, at ranges as close as 880 kilometers (550 miles) by the Solid State Imaging (SSI) system on NASA's Galileo spacecraft.<p>The Jet Propulsion Laboratory, Pasadena, CA manages the Galileo mission for NASA's Office of Space Science, Washington, DC. JPL is an operating division of California Institute of Technology (Caltech).<p>This image and other images and data received from Galileo are posted on the World Wide Web, on the Galileo mission home page at URL http://galileo.jpl.nasa.gov. Background information and educational context for the images can be found at <a href="http://www2.jpl.nasa.gov/galileo/sepo/" target="_blank">http://www.jpl.nasa.gov/galileo/sepo</a>..<br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01403" onclick="window.open(this.href); return false;" title="Voir l'image 	 PIA01403:  A closer look at Chaos on Europa	  sur le site de la NASA">Voir l'image 	 PIA01403:  A closer look at Chaos on Europa	  sur le site de la NASA.</a></div>
PIA01403: A closer look at Chaos on Europa
<h1>PIA01404:  Small Craters on Europa</h1><div class="PIA01404" lang="en" style="width:800px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;">This high resolution view of the Conamara Chaos region on Jupiter's icy moon, Europa, reveals craters which range in size from about 30 meters to over 450 meters (slightly over a quarter of a mile) in diameter. The large number of craters seen here is unusual for Europa. This section of Conamara Chaos lies inside a bright ray of material which was ejected by the large impact crater, Pwyll, 1000 kilometers (620 miles) to the south. The presence of craters within the bright ray suggests that many are secondaries which formed from chunks of material that were thrown out by the enormous energy of the impact which formed Pwyll.<p>North is to the upper right of the picture and the sun illuminates the surface from the east. The image, centered at 9 degrees latitude and 274 degrees longitude, covers an area approximately 8 by 4 kilometers (5 by 2.5 miles). The finest details that can be discerned in this picture are about 20 meters (66 feet) across. The images were taken on December 16, 1997 at a range of 960 kilometers (590 miles) by the Solid State Imaging (SSI) system on NASA's Galileo spacecraft.<p>The Jet Propulsion Laboratory, Pasadena, CA manages the Galileo mission for NASA's Office of Space Science, Washington, DC. JPL is an operating division of California Institute of Technology (Caltech).<p>This image and other images and data received from Galileo are posted on the World Wide Web, on the Galileo mission home page at URL http://galileo.jpl.nasa.gov. Background information and educational context for the images can be found at <a href="http://www2.jpl.nasa.gov/galileo/sepo/" target="_blank">http://www.jpl.nasa.gov/galileo/sepo</a>..<br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01404" onclick="window.open(this.href); return false;" title="Voir l'image 	 PIA01404:  Small Craters on Europa	  sur le site de la NASA">Voir l'image 	 PIA01404:  Small Craters on Europa	  sur le site de la NASA.</a></div>
PIA01404: Small Craters on Europa
<h1>PIA01405:  A Dark Spot on Europa</h1><div class="PIA01405" lang="en" style="width:800px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;">This view taken by NASA's Galileo spacecraft of Jupiter's icy moon Europa focuses on a dark, smooth region whose center is the lowest area in this image. To the west (left), it is bounded by a cliff and terraces, which might have been formed by normal faulting. The slopes toward the east (right) leading into the dark spot are gentle.<p>Near the center of the dark area, it appears the dark materials have covered some of the bright terrain and ridges. This suggests that when the dark material was deposited, it may have been a fluid or an icy slush.<p>Only a few impact craters are visible, with some of them covered or flooded by dark material. Some appear in groups, which may indicate that they are secondary craters formed by debris excavated during a larger impact event. A potential source for these is the nearby crater Mannann`an.<p>North is to the top of the picture which is centered at 1 degree south latitude and 225 degrees west longitude. The images in this mosaic have been re-projected to 50 meters (55 yards) per picture element. They were obtained by the Solid State Imaging (SSI) system on March 29, 1998, during Galileo's fourteenth orbit of Jupiter, at ranges as close as 1940 kilometers (1,200 miles) from Europa.<p>The Jet Propulsion Laboratory, Pasadena, CA manages the Galileo mission for NASA's Office of Space Science, Washington, DC. JPL is an operating division of California Institute of Technology (Caltech).<p>This image and other images and data received from Galileo are posted on the World Wide Web, on the Galileo mission home page at URL http://galileo.jpl.nasa.gov. Background information and educational context for the images can be found at <a href="http://www2.jpl.nasa.gov/galileo/sepo/" target="_blank">http://www.jpl.nasa.gov/galileo/sepo</a>..<br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01405" onclick="window.open(this.href); return false;" title="Voir l'image 	 PIA01405:  A Dark Spot on Europa	  sur le site de la NASA">Voir l'image 	 PIA01405:  A Dark Spot on Europa	  sur le site de la NASA.</a></div>
PIA01405: A Dark Spot on Europa
<h1>PIA01406:  Topography within Europa's Mannann'an crater</h1><div class="PIA01406" lang="en" style="width:800px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;">This three dimensional effect is created by superimposing images of Jupiter's icy moon, Europa, which were taken from slightly different perspectives. When viewed through red (left eye) and blue (right eye) filters, this product, a stereo anaglyph, shows variations in height of surface features.<p>This view shows the rim and interior of the impact crater Mannann'an, on Jupiter's moon Europa. The stereo image reveals the rim of the crater which appears as a tall ridge near the left edge of the image, as well as and numerous small hills on the bottom of the crater. One of the most striking features is the large pit surrounded by circular cracks on the right side of the image, with dark radiating fractures in its center.<p>The right (blue) image is a high resolution image (20 meters per picture element) taken through a clear filter. The left (red) image is composed of lower resolution (80 meters per picture element) color images taken through violet, green, and near-infrared filters and averaged to approximate an unfiltered view.<p>North is to the top of the picture and the sun illuminates the scene from the east (right). The image, centered at 3 degrees north latitude and 120 degrees west longitude, covers an area approximately 18 by 4 kilometers (11 by 2.5 miles). The finest details that can be discerned in this picture are about 40 meters (44 yards) across. The images were taken on March 29th, 1998 at 13 hours, 17 minutes, 29 seconds Universal Time at a range of 1934 kilometers by the Solid State Imaging (SSI) system on NASA's Galileo spacecraft.<p>The Jet Propulsion Laboratory, Pasadena, CA manages the Galileo mission for NASA's Office of Space Science, Washington, DC. JPL is an operating division of California Institute of Technology (Caltech).<p>This image and other images and data received from Galileo are posted on the World Wide Web, on the Galileo mission home page at URL http://galileo.jpl.nasa.gov. Background information and educational context for the images can be found at <a href="http://www2.jpl.nasa.gov/galileo/sepo/" target="_blank">http://www.jpl.nasa.gov/galileo/sepo</a>..<br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01406" onclick="window.open(this.href); return false;" title="Voir l'image 	 PIA01406:  Topography within Europa's Mannann'an crater	  sur le site de la NASA">Voir l'image 	 PIA01406:  Topography within Europa's Mannann'an crater	  sur le site de la NASA.</a></div>
PIA01406: Topography within Europa's Mannann'an crater
<h1>PIA01407:  Europa Imaging Highlights during GEM</h1><div class="PIA01407" lang="en" style="width:800px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p>During the two year Galileo Europa Mission (GEM), NASA's Galileo spacecraft will focus intensively on Jupiter's intriguing moon, Europa. This montage shows samples of some of the features that will be imaged during eight successive orbits. The images in this montage are in order of increasing orbit from the upper left (orbit 11) to the lower right (orbit 19).<p>DESCRIPTIONS AND APPROXIMATE RESOLUTIONSTriple bands and dark spots<p>1.6 kilometers/pixelConamara Chaos<p>1.6 kilometers/pixelMannan'an Crater<p>1.6 kilometers/ pixelCilix<p>1.6 kilometers/pixelAgenor Linea and Thrace Macula<p>2 kilometers/pixelSouth polar terrain<p>2 kilometers/pixelRhadamanthys Linea<p>1.6 kilometers/pixelEuropa plume search<p>7 kilometers/pixel< /tr><p>1. Triple bands and dark spots were the focus of some images from Galileo's eleventh orbit of Jupiter. Triple bands are multiple ridges with dark deposits along the outer margins. Some extend for thousands of kilometers across Europa's icy surface. They are cracks in the ice sheet and indicate the great stresses imposed on Europa by tides raised by Jupiter, as well as Europa's neighboring moons, Ganymede and Io. The dark spots or "lenticulae" are spots of localized disruption.<p>2. The Conamara Chaos region reveals icy plates which have broken up, moved, and rafted into new positions. This terrain suggests that liquid water or ductile ice was present near the surface. On Galileo's twelfth orbit of Jupiter, sections of this region with resolutions as high as 10 meters per picture element will be obtained.<p>3. Mannann'an Crater is a feature newly discovered by Galileo in June 1996. Color and high resolution images (to 40 meters per picture element) from Galileo's fourteenth orbit of Jupiter will offer a close look at the crater and help characterize how impacts affect the icy surface of this moon.<p>4. Cilix, a large mound about 1.5 kilometers high, is the center of Europa's coordinate system. Its concave top and what may be flow like features to the southwest of the mound are especially intriguing. The origin of this feature is unknown at present. Color, stereo, and high resolution images (to 65 meters per picture element) from Galileo's fifteenth orbit of Jupiter will offer new insights and resolve questions about its origin.<p>5. Images of Agenor Linea (white arrow) and Thrace Macula (black arrow) with resolutions as high as 30 meters per picture element will be obtained during Galileo's sixteenth orbit of Jupiter. Agenor is an unusually bright lineament on Europa. Is the brightness due to new ice, and if so, does it represent recent activity? Could the dark region of Thrace Macula be a flow from ice volcanism?<p>6. Images of Europa's south polar terrain obtained during Galileo's seventeenth orbit of Jupiter will offer insights into the processes which are active in this region. Is the ice crust thicker near Europa's poles than near the equator? The prominent dark line running from upper left to lower right through the center of this image is Astypalaea Linea. It is a fault about the length of the San Andreas fault in California and is the largest such fault known on Europa. Images with resolutions of 48 meters per picture element will be obtained to examine its geologic structure.<p>7. This long lineament, Rhadamanthys Linea. is spotted with dark "freckles." Are these freckle features formed by icy volcanism? Is this an early form of a triple band? Stereo and high resolution (to 46 meters per picture element) obtained during Galileo's eighteenth orbit of Jupiter may indicate whether the lineament is the result of volcanic processes or is formed by other surface processes.<p>8. During Galileo's nineteenth orbit of Jupiter, images of Europa will be taken with very low sun illuminations, similar to taking a picture at sunset or sunrise. The object will be to search for backlit plumes issuing from icy volcanic vents. Such plumes would be direct evidence of a liquid ocean beneath the ice. Resolutions will be as high as 40 meters per picture element. This picture was simulated image from Galileo data obtained during the spacecraft's second orbit of Jupiter in September 1996.<p>North is to the top of the pictures. During orbit 13, the Galileo spacecraft was behind the sun from our vantage point on Earth so it did not obtain or transmit data from that orbit. The left two images in the bottom row were obtained by NASA's Voyager 2 spacecraft in 1979; the remaining images were obtained by the Solid State Imaging (SSI) system on NASA's Galileo spacecraft in 1996.<p>The Jet Propulsion Laboratory, Pasadena, CA manages the Galileo mission for NASA's Office of Space Science, Washington, DC. JPL is an operating division of California Institute of Technology (Caltech).<p>This image and other images and data received from Galileo are posted on the World Wide Web, on the Galileo mission home page at URL http://galileo.jpl.nasa.gov. Background information and educational context for the images can be found at <a href="http://www2.jpl.nasa.gov/galileo/sepo/" target="_blank">http://www.jpl.nasa.gov/galileo/sepo</a>..<br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01407" onclick="window.open(this.href); return false;" title="Voir l'image 	 PIA01407:  Europa Imaging Highlights during GEM	  sur le site de la NASA">Voir l'image 	 PIA01407:  Europa Imaging Highlights during GEM	  sur le site de la NASA.</a></div>
PIA01407: Europa Imaging Highlights during GEM
<h1>PIA01503:  Europa's Fractured Surface</h1><div class="PIA01503" lang="en" style="width:790px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p>This image of Europa, smallest of Jupiter's four Galilean satellites, was acquired by Voyager 2 on July 9, 1979, from a (150,600 miles). Europa, the brightest range of 241,000 kilometers of the Galilean satellites, has a density slightly less than Io, suggesting it has a substantial quantity of water. Scientists previously speculated that the water must have cooled from the interior and formed a mantle of ice perhaps 100 kilometers thick. The complex patterns on its surface suggest that the icy surface was fractured, and that the cracks filled with dark material from below. Very few impact craters are visible on the surface, suggesting that active processes on the surface are still modifying Europa. The tectonic pattern seen on its surface differs drastically from the fault systems seen on Ganymede where pieces of the crust have moved relative to each other. On Europa, the crust evidently fractures but the pieces remain in roughly their original position.<br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01503" onclick="window.open(this.href); return false;" title="Voir l'image 	 PIA01503:  Europa's Fractured Surface	  sur le site de la NASA">Voir l'image 	 PIA01503:  Europa's Fractured Surface	  sur le site de la NASA.</a></div>
PIA01503: Europa's Fractured Surface
<h1>PIA01504:  Europa's Evening Terminator</h1><div class="PIA01504" lang="en" style="width:800px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;">This image of the Jovian moon Europa was taken by Voyager 2 the spacecraft passed within 225,000 kilometers. The area shown is about 600 by 800 kilometers, July 9, 1979, as (140,625 miles). and the smallest features visible are about 4 kllometers in size. This image was taken along the evening terminator, which best shows the surface topography of complex narrow ridges, seen as curved bright streaks, 5 to 10 kilometers wide, andAlso visible are dark bands, typically 100 kilometers in length. more diffuse in character, 20 to 40 kilometers wide and hundreds to thousands of kilometers in length. A few features are suggestive of impact craters but are rare, indicating that the surface thought to be dominantly ice is still active, perhaps warmed by tidal heating like Io. The larger icy satellites, Callisto and Ganymede, are evidently colder with much more rigid crusts and ancient impact craters. The complex intersecting of dark markings and bright ridges suggest that the surface has been fractured and material from beneath has welled up to fill the cracks.<br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01504" onclick="window.open(this.href); return false;" title="Voir l'image 	 PIA01504:  Europa's Evening Terminator	  sur le site de la NASA">Voir l'image 	 PIA01504:  Europa's Evening Terminator	  sur le site de la NASA.</a></div>
PIA01504: Europa's Evening Terminator
<h1>PIA01523:  Europa Linear Features from 246,000 kilometers</h1><div class="PIA01523" lang="en" style="width:790px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;">The first close look ever obtained of Jupiter's satellite, Europa, was taken today, July 9, by Voyager 2 as the spacecraft approached the planet. The linear crack-like features had been seen from a much greater distance last March by Voyager 1. This picture was made at a range of 246,000 kilometers (152,000 miles) and provides a resolution of about four kilometers (2.5 miles). The complicated linear features appear even more like cracks or huge fractures in these images. Also seen are somewhat darker mottled regions which appear to have a slightly pitted appearance, perhaps due to small scale craters. No large craters (more than five kilometers in diameter) are easily identifiable in the Europa photographs to date, suggesting that this satellite has a young surface relative to Ganymede and Callisto, although not perhaps as young as Io's. Various models for Europa's structure will be tested during analysis of these images, including the possibility that the surface is a thin ice crust overlying water or softer ice and that the fracture systems seen are breaks in that crust. Resurfacing mechanisms such as production of fresh ice or snow along the cracks and cold glacier-like flows are being considered as possibilities for removing evidence of impact events. Europa thus appears to truly be a satellite with many properties intermediate between Ganymede and Io.<br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01523" onclick="window.open(this.href); return false;" title="Voir l'image 	 PIA01523:  Europa Linear Features from 246,000 kilometers	  sur le site de la NASA">Voir l'image 	 PIA01523:  Europa Linear Features from 246,000 kilometers	  sur le site de la NASA.</a></div>
PIA01523: Europa Linear Features from 246,000 kilometers
<h1>PIA01633:  The Tyre multi-ring Structure on Europa</h1><div class="PIA01633" lang="en" style="width:800px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p>This mosaic shows the Tyre multi-ring structure which is thought to have been formed by a large impact onto Jupiter's moon Europa. The effective crater (large bull's-eye feature) is about 40 kilometers (25 miles) across while the entire structure is much larger. The feature was formerly known as Tyre Macula. The concentric rings, of which five to seven can be discerned easily, consist of troughs and ridges. Tyre is one of the few impact structures on Europa that has concentric rings and may indicate an area where fluid material, perhaps liquid water, lay below the surface at the time of impact. A few ridges within Tyre appear to have been partly destroyed at the time of impact.</p><p>North is to the top of the picture and the sun illuminates the surface from the left. The mosaic is centered at 34 degrees north latitude and 144 degrees west longitude and covers an area approximately 424 by 456 kilometers (265 by 285 miles). The resolution is 170 meters (185 feet) across. The horizontal and vertical black lines in the mosaic indicate gaps in the data received for this image. The images were taken on March 29, 1998 at a range of approximately 18,000 kilometers (11,250 miles) by the Solid State Imaging (SSI) system on NASA's Galileo spacecraft.</p><p>The Jet Propulsion Laboratory, Pasadena, CA manages the Galileo mission or NASA's Office of Space Science, Washington, DC.</p><p>This image and other images and data received from Galileo are posted on the World Wide Web, on the Galileo mission home page at URL <a href="http://galileo.jpl.nasa.gov"> http://galileo.jpl.nasa.gov</a>. Background information and educational context for the images can be found at <a href="http://www2.jpl.nasa.gov/galileo/sepo/" target="_blank">http://www.jpl.nasa.gov/galileo/sepo</a>.<br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01633" onclick="window.open(this.href); return false;" title="Voir l'image 	 PIA01633:  The Tyre multi-ring Structure on Europa	  sur le site de la NASA">Voir l'image 	 PIA01633:  The Tyre multi-ring Structure on Europa	  sur le site de la NASA.</a></div>
PIA01633: The Tyre multi-ring Structure on Europa
<h1>PIA01640:  Mitten shaped region of Chaotic Terrain on Europa</h1><div class="PIA01640" lang="en" style="width:747px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p>This view of Jupiter's icy moon Europa shows a region shaped like a mitten that has a texture similar to the matrix of chaotic terrain, which is seen in medium and high resolution images of numerous locations across Europa's surface. Development of such terrain may be one of the major processes for resurfacing the moon. North is to the top and the sun illuminates the surface from the left. The material in the "catcher's mitt" has the appearance of frozen slush and seems to bulge upward from the adjacent surface, which has been bent downward and cracked, especially along the southwest (lower left) margins. Scientists on the Galileo imaging team are exploring various hypotheses for the formation of such terrain including solid-state convection (vertical movement between areas which differ in density due to heating), upwelling of viscous icy "lava," or liquid water melting through from a subsurface ocean.</p><p>The image, centered at 20 degrees north latitude, 80 degrees west longitude covers an area approximately 175 by 180 kilometers (108 by 112 miles). The resolution is 235 meters per picture element. The images were taken on 31 May, 1998 Universal Time at a range of 23 thousand kilometers (14 thousand miles) by the Solid State Imaging (SSI) system on NASA's Galileo spacecraft.</p><p>The Jet Propulsion Laboratory, Pasadena, CA manages the Galileo mission for NASA's Office of Space Science, Washington, DC.</p><p>This image and other images and data received from Galileo are posted on the World Wide Web, on the Galileo mission home page at URL <a href="http://galileo.jpl.nasa.gov ">http://galileo.jpl.nasa.gov</a>. Background information and educational context for the images can be found at <a href="http://www2.jpl.nasa.gov/galileo/sepo/" target="_blank">http://www.jpl.nasa.gov/galileo/sepo</a>.<br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01640" onclick="window.open(this.href); return false;" title="Voir l'image 	 PIA01640:  Mitten shaped region of Chaotic Terrain on Europa	  sur le site de la NASA">Voir l'image 	 PIA01640:  Mitten shaped region of Chaotic Terrain on Europa	  sur le site de la NASA.</a></div>
PIA01640: Mitten shaped region of Chaotic Terrain on Europa
<h1>PIA01641:  Double Ridges, Dark Spots, and Smooth Icy Plains on Europa</h1><div class="PIA01641" lang="en" style="width:800px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p>This mosaic of a region in the northern hemisphere of Jupiter's moon, Europa, displays many of the features which are typical on the satellite's icy surface. Brown, linear (double) ridges extend prominently across the scene. They could be frozen remnants of cryovolcanic activity which occurred when water or partly molten water ice erupted on the Europan surface, freezing almost instantly in the extremely low temperatures so far from our sun. Dark spots, several kilometers in diameter, are distributed over the surface. A geologically older, smoother surface, bluish in tone, underlies the ridge system. The blue surface is composed of almost pure water ice, whereas the composition of the dark, brownish spots and ridges is not certain. One possibility is that they contain evaporites such as mineral salts in a matrix of high water content.</p><p>North is to the lower left of the picture and the sun illuminates the surface from the upper left. The image, centered at 40 degrees north latitude and 225 degrees west longitude, covers an area approximately 800 by 350 kilometers(500 by 220 miles). The resolution is 230 meters (250 yards) per picture element. The colors have been enhanced to bring out the details. An astronaut orbiting this smallest of the four Galilean satellites would seethe icy surface of Europa somewhat brighter, but with less intense colors. The images were obtained during two separate orbits of Jupiter by the Solid State Imaging (SSI) system on NASA's Galileo spacecraft. High resolution images obtained at a range of about 25,000 kilometers(15,000 miles) during the spacecraft's 15th orbit of Jupiter on May 31st, 1998 are combined with <a href="http://www2.jpl.nasa.gov/galileo/sepo/" target="_blank">http://www.jpl.nasa.gov/galileo/sepo</a>./atjup/europa/G1.html">lower resolution images</a> obtained during the spacecraft's first orbit of Jupiter on June 28th, 1996. Combining the lower resolution and high resolution images enables scientists to investigate both the surface features in great detail as well as the color or compositional information in a regional context.</p><p>The Jet Propulsion Laboratory, Pasadena, CA manages the Galileo mission or NASA's Office of Space Science, Washington, DC.</p><p>This image and other images and data received from Galileo are posted on the World Wide Web, on the Galileo mission home page at URL<a href="http://solarsystem.nasa.gov/galileo/" target="_blank">http://solarsystem.nasa.gov/galileo/</a>. Background information and educational context for the images can be found at URL<a href="http://www2.jpl.nasa.gov/galileo/sepo/" target="_blank">http://www.jpl.nasa.gov/galileo/sepo</a><br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01641" onclick="window.open(this.href); return false;" title="Voir l'image 	 PIA01641:  Double Ridges, Dark Spots, and Smooth Icy Plains on Europa	  sur le site de la NASA">Voir l'image 	 PIA01641:  Double Ridges, Dark Spots, and Smooth Icy Plains on Europa	  sur le site de la NASA.</a></div>
PIA01641: Double Ridges, Dark Spots, and Smooth Icy Plains on Europa
<h1>PIA01642:  Cracks and Ridges Distorted by Europan Fault Motion</h1><div class="PIA01642" lang="en" style="width:633px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p>These cracks and ridges in the south polar region of Jupiter's moon Europa have been rotated into sigmoidal or "S" shapes by the motion of <a href="/catalog/PIA01644">Astypalaea Linea, a strike-slip fault</a> in the moon's icy surface. These cracks and ridges are located within Cyclades Macula, a region of the fault which has been pulled apart and created openings through which warmer, softer ice from below Europa's brittle ice shell surface, or frozen water from a possible subsurface ocean, could reach the surface. This upwelling of material formed large areas of new ice within the boundaries of the original fault. North is to the top of the picture. The once active fault structure is a barely visible line (right of center) that trends approximately north to south in this image.</p><p>An earlier northwest to southeast trending generation of rotated cracks underlies the more recent set. Such rotated structure is typical of a process known as "simple shear," and characterizes many large strike-slip faults on Earth. In this case, however, simple shear structures seem limited to the interior of the Cyclades Macula pull apart region and do not appear to border the elongate trunk of the fault, Astypalaea Linea. Comparisons between these structures related to faults on Europa and those on Earth may generate ideas useful in the study of terrestrial faulting.</p><p>The sun illuminates the surface from the top. The image, centered at 63 degrees south latitude and 191 degrees west longitude, covers an area approximately 15 by 10 kilometers (9 by 6 miles). The resolution is 40 meters (131 feet) per picture element. The images were taken on September 26, 1998 at a range of less than 4200 kilometers (2600 miles) by the Solid State Imaging (SSI) system on NASA's Galileo spacecraft.</p><p>The Jet Propulsion Laboratory, Pasadena, CA manages the Galileo mission for NASA's Office of Space Science, Washington, DC.</p><p>This image and other images and data received from Galileo are posted on the World Wide Web, on the Galileo mission home page at URL<a href="http://solarsystem.nasa.gov/galileo/" target="_blank">http://solarsystem.nasa.gov/galileo/</a>. Background information and educational context for the images can be found at URL<a href="http://www2.jpl.nasa.gov/galileo/sepo/" target="_blank">http://www.jpl.nasa.gov/galileo/sepo</a>."><a href="http://www2.jpl.nasa.gov/galileo/sepo/" target="_blank">http://www.jpl.nasa.gov/galileo/sepo</a>.</a></p><br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01642" onclick="window.open(this.href); return false;" title="Voir l'image 	 PIA01642:  Cracks and Ridges Distorted by Europan Fault Motion	  sur le site de la NASA">Voir l'image 	 PIA01642:  Cracks and Ridges Distorted by Europan Fault Motion	  sur le site de la NASA.</a></div>
PIA01642: Cracks and Ridges Distorted by Europan Fault Motion
<h1>PIA01643:  A Record of Crustal Movement on Europa</h1><div class="PIA01643" lang="en" style="width:453px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p>This view of the south polar region of Jupiter's moon Europa shows part of a gray band that formed as plates on the icy surface separated and material filled in the widening gap. North is to the top of the picture. In the center of the image, a gently curving linear crack runs north to south and appears to be the location where the fault originally opened. Successive layers, like tree rings, form as material enters the gap periodically from below and hardens.</p><p>The relative motion of the two opposing sides of the band is mostly "strike-slip," where two crustal blocks move horizontally past one another, similar to two opposing lanes of traffic. However, since this motion is not exactly parallel to the active crack, the opposite sides also pull apart to create openings through which warmer, softer ice from below Europa's brittle ice shell surface, or frozen water from a possible subsurface ocean, could reach the surface. The band surface accumulates layer by layer. A rough symmetry with respect to the active central linear crack can be seen in these layers.</p><p>The large, segmented crack paralleling the west (left) side of the band cuts the original north to south fault shown in the center of the image. This suggests that the central fault has not been active since the large, segmented crack formed.</p><p>The curved, lined area is a small part of a much larger <a href="/catalog/PIA01644">strike-slip fault called Astypalaea Linea.</a> This fault extends over 800 kilometers (500 miles), roughly the distance of the portion of California's San Andreas fault from the Mexican border to the San Francisco Bay. Galileo images show that the Europan fault has slipped about 50 kilometers (30 miles).</p><p>The Sun illuminates the surface from the top. The image, centered at 66 degrees south latitude and 195 degrees west longitude, covers an area approximately 24 by 16 kilometers (15 by 10 miles). The resolution is 40 meters (131 feet) per picture element. The images were taken on September 26, 1998 at a range of less than 4,200 kilometers (2,600 miles) by Galileo's solid-state imaging system.</p><p>This image and other images and data received from Galileo are posted on the World Wide Web, on the Galileo mission home page at URL<a href="http://solarsystem.nasa.gov/galileo/" target="_blank">http://solarsystem.nasa.gov/galileo/</a>. Background information and educational context for the images can be found at URL<a href="http://www2.jpl.nasa.gov/galileo/sepo/" target="_blank">http://www.jpl.nasa.gov/galileo/sepo</a>."><a href="http://www2.jpl.nasa.gov/galileo/sepo/" target="_blank">http://www.jpl.nasa.gov/galileo/sepo</a>.</a></p><br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01643" onclick="window.open(this.href); return false;" title="Voir l'image 	 PIA01643:  A Record of Crustal Movement on Europa	  sur le site de la NASA">Voir l'image 	 PIA01643:  A Record of Crustal Movement on Europa	  sur le site de la NASA.</a></div>
PIA01643: A Record of Crustal Movement on Europa
<h1>PIA01644:  San Andreas-sized Strike-slip Fault on Europa</h1><div class="PIA01644" lang="en" style="width:678px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p>This mosaic of the south polar region of Jupiter's moon Europa shows the northern 290 kilometers (180 miles) of a strike-slip fault named Astypalaea Linea. The entire fault is about 810 kilometers (500 miles) long, about the size of the California portion of the San Andreas fault, which runs from the California-Mexico border north to the San Francisco Bay.</p><p>In a strike-slip fault, two crustal blocks move horizontally past one another, similar to two opposing lanes of traffic. Overall motion along the fault seems to have followed a continuous narrow crack along the feature's entire length, with a path resembling steps on a staircase crossing zones that have been pulled apart. The images show that about 50 kilometers (30 miles) of displacement have taken place along the fault. The fault's opposite sides can be reconstructed like a puzzle, matching the shape of the sides and older, individual cracks and ridges broken by its movements.</p><p><a href="/figures/graphic_full.jpg"></a></p><p>The red line marks the once active central crack of the fault. The black line outlines the fault zone, including material accumulated in the regions which have been pulled apart.</p><p>Bends in the fault have allowed the surface to be pulled apart. This process created openings through which warmer, softer ice from below Europa's brittle ice shell surface, or frozen water from a possible subsurface ocean, could reach the surface. This upwelling of material formed large areas of new ice within the boundaries of the original fault. A similar pulling-apart phenomenon can be observed in the geological trough surrounding California's Salton Sea, in Death Valley and the Dead Sea. In those cases, the pulled-apart regions can include upwelled materials, but may be filled mostly by sedimentary and eroded material from above.</p><p>One theory is that fault motion on Europa is induced by the pull of variable daily tides generated by Jupiter's gravitational tug on Europa. Tidal tension opens the fault and subsequent tidal stress causes it to move lengthwise in one direction. Then tidal forces close the fault again, preventing the area from moving back to its original position. Daily tidal cycles produce a steady accumulation of lengthwise offset motions. Here on Earth, unlike Europa, large strike-slip faults like the San Andreas are set in motion by plate tectonic forces.</p><p>North is to the top of the picture and the sun illuminates the surface from the top. The image, centered at 66 degrees south latitude and 195 degrees west longitude, covers an area approximately 300 by 203 kilometers(185 by 125 miles). The pictures were taken on September 26, 1998by Galileo's solid-state imaging system.</p><p>This image and other images and data received from Galileo are posted on the World Wide Web, on the Galileo mission home page at URL http://galileo.jpl.nasa.gov. Background information and educational context for the images can be found at <a href="http://www2.jpl.nasa.gov/galileo/sepo/" target="_blank">http://www.jpl.nasa.gov/galileo/sepo</a>..</p><br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01644" onclick="window.open(this.href); return false;" title="Voir l'image 	 PIA01644:  San Andreas-sized Strike-slip Fault on Europa	  sur le site de la NASA">Voir l'image 	 PIA01644:  San Andreas-sized Strike-slip Fault on Europa	  sur le site de la NASA.</a></div>
PIA01644: San Andreas-sized Strike-slip Fault on Europa
<h1>PIA01645:  The San Andreas Fault and a Strike-slip Fault on Europa</h1><div class="PIA01645" lang="en" style="width:800px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p>The mosaic on the right of the south polar region of Jupiter's moon Europa shows the northern 290 kilometers (180 miles) of a strike-slip fault named Astypalaea Linea. The entire fault is about 810 kilometers (500 miles) long, the size of the California portion of the San Andreas fault on Earth which runs from the California-Mexico border north to the San Francisco Bay.</p><p>The left mosaic shows the portion of the San Andreas fault near California's san Francisco Bay that has been scaled to the same size and resolution as the Europa image. Each covers an area approximately 170 by 193 kilometers(105 by 120 miles). The red line marks the once active central crack of the Europan fault (right) and the line of the San Andreas fault (left).</p><p>A strike-slip fault is one in which two crustal blocks move horizontally past one another, similar to two opposing lanes of traffic. The overall motion along the Europan fault seems to have followed a continuous narrow crack along the entire length of the feature, with a path resembling stepson a staircase crossing zones which have been pulled apart. The images show that about 50 kilometers (30 miles) of displacement have taken place along the fault. Opposite sides of the fault can be reconstructed like a puzzle, matching the shape of the sides as well as older individual cracks and ridges that had been broken by its movements.</p><p>Bends in the Europan fault have allowed the surface to be pulled apart. This pulling-apart along the fault's bends created openings through which warmer, softer ice from below Europa's brittle ice shell surface, or frozen water from a possible subsurface ocean, could reach the surface. This upwelling of material formed large areas of new ice within the boundaries of the original fault. A similar pulling apart phenomenon can be observed in the geological trough surrounding California's Salton Sea, and in Death Valley and the Dead Sea. In those cases, the pulled apart regions can include upwelled materials, but may be filled in mostly by sedimentary and erosional material deposited from above. Comparisons between faults on Europa and Earth may generate ideas useful in the study of terrestrial faulting.</p><p>One theory is that fault motion on Europa is induced by the pull of variable daily tides generated by Jupiter's gravitational tug on Europa. The tidal tension opens the fault; subsequent tidal stress causes it to move lengthwise in one direction. Then the tidal forces close the fault up again. This prevents the area from moving back to its original position. If it moves forward with the next daily tidal cycle, the result is a steady accumulation of these lengthwise offset motions.</p><p>Unlike Europa, here on Earth, large strike-slip faults such as the San Andreas are set in motion not by tidal pull, but by plate tectonic forces from the planet's mantle.</p><p>North is to the top of the picture. The Earth picture (left) shows a LandSat Thematic Mapper image acquired in the infrared (1.55 to 1.75 micrometers) by LandSat5 on Friday, October 20th 1989 at 10:21 am. The original resolution was 28.5 meters per picture element.</p><p>The Europa picture (right) is centered at 66 degrees south latitude and 195 degrees west longitude. The highest resolution frames, obtained at 40 meters per picture element with a spacecraft range of less than 4200 kilometers (2600 miles), are set in the context of lower resolution regional frames obtained at 200 meters per picture element and a range of 22,000 kilometers (13,600 miles). The images were taken on September 26, 1998 by the Solid State Imaging (SSI) system on NASA's Galileo spacecraft.</p><p>The Jet Propulsion Laboratory, Pasadena, CA manages the Galileo mission for NASA's Office of Space Science, Washington, DC.</p><p>This image and other images and data received from Galileo are posted on the World Wide Web, on the Galileo mission home page at URL http://galileo.jpl.nasa.gov. Background information and educational context for the images can be found at URL HTTP://www.jpl.nasa.gov/galileo/sepo.<br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01645" onclick="window.open(this.href); return false;" title="Voir l'image 	 PIA01645:  The San Andreas Fault and a Strike-slip Fault on Europa	  sur le site de la NASA">Voir l'image 	 PIA01645:  The San Andreas Fault and a Strike-slip Fault on Europa	  sur le site de la NASA.</a></div>
PIA01645: The San Andreas Fault and a Strike-slip Fault on Europa
<h1>PIA01646:  Agenor Linea at High Resolution</h1><div class="PIA01646" lang="en" style="width:800px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p>Agenor Linea is an unusual feature on Jupiter's icy moon Europa since it is brighter than its surroundings while most of Europa's ridges and bands are relatively dark. During the Galileo spacecraft's 17th orbit of Jupiter, high resolution images were obtained of Agenor Linea near Europa's day/night boundary so as to emphasize fine surface details. This mosaic shows high resolution images embedded in slightly lower resolution images which were also acquired during the 17th orbit. The Galileo images show that Agenoris not a ridge, but is relatively flat. Its interior consists of several long bands, just one of which is the very bright feature known as Agenor. Each long band shows fine striations along its length. A few very small craters pockmark Agenor Linea and its surroundings. Agenor is cut by some narrow fractures, and by some small subcircular features called lenticulae. Rough chaotic terrain is visible at the top and bottom of this photo, and appears to be "eating away" at the edges of Agenor. Though previously it was suspected that Agenor Linea might be one of the youngest features on Europa, this new view shows that it is probably not.</p><p>North is to the upper right of the picture and the sun illuminates the surface from the east. The image, centered at 44 degrees south latitude and 219 degrees west longitude, covers an area approximately 130 by 95 kilometers (80 by 60 miles). The highest resolution images were obtained at a resolution of about 50 meters (165 feet) per picture element and are shown here in context at about 220 meters per picture element. The images were taken on September 26th, 1998 at ranges as close as 5000 kilometers (3100 miles) by the Solid State Imaging (SSI) system on NASA's Galileo spacecraft.</p><p>The Jet Propulsion Laboratory, Pasadena, CA manages the Galileo mission for NASA's Office of Space Science, Washington, DC.</p><p>This image and other images and data received from Galileo are posted on the World Wide Web, on the Galileo mission home page at URL<a href="http://solarsystem.nasa.gov/galileo/" target="_blank">http://solarsystem.nasa.gov/galileo/</a>. Background information and educational context for the images can be found at URL<a href="http://www2.jpl.nasa.gov/galileo/sepo/" target="_blank">http://www.jpl.nasa.gov/galileo/sepo</a>."><a href="http://www2.jpl.nasa.gov/galileo/sepo/" target="_blank">http://www.jpl.nasa.gov/galileo/sepo</a>.</a></p><br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01646" onclick="window.open(this.href); return false;" title="Voir l'image 	 PIA01646:  Agenor Linea at High Resolution	  sur le site de la NASA">Voir l'image 	 PIA01646:  Agenor Linea at High Resolution	  sur le site de la NASA.</a></div>
PIA01646: Agenor Linea at High Resolution
<h1>PIA01647:  Agenor Linea in Color</h1><div class="PIA01647" lang="en" style="width:800px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p>Agenor Linea is an unusually bright, white band on Jupiter's icy moon Europa. This mosaic uses color images to "paint" high resolution images of Agenor, and then places the colorized images within lower resolution images of the surrounding area. All data was obtained on September 26th, 1998 during the 17th orbit of Jupiter by NASA's Galileo spacecraft. Along this portion of Agenor is a "triple band," flanked by dark, reddish material of uncertain origin. On the right side of this image, Agenor splits into two sections. These color images will help scientists understand why Agenor Linea is unusually bright and white compared to Europa's other ridges and bands.</p><p>North is to the upper right of the picture and the sun illuminates the surface from the east. The image, centered at 41 degrees south latitude and 189 degrees west longitude, covers an area approximately 135 by 60 kilometers (84 by 37 miles). The highest resolution images were obtained at a resolution of about 50 meters (165 feet) per picture element and are shown here in context at about 220 meters per picture element. The images were taken by the Solid State Imaging (SSI) system on NASA's Galileo spacecraft at a range of about 4700 kilometers (2900 miles) for the highest resolution images and less than 20000 kilometers (12,400 miles) for the lower resolution color images.</p><p>The Jet Propulsion Laboratory, Pasadena, CA manages the Galileo mission for NASA's Office of Space Science, Washington, DC.</p><p>This image and other images and data received from Galileo are posted on the World Wide Web, on the Galileo mission home page at URL<a href="http://solarsystem.nasa.gov/galileo/" target="_blank">http://solarsystem.nasa.gov/galileo/</a>. Background information and educational context for the images can be found at <a href="http://www2.jpl.nasa.gov/galileo/sepo/" target="_blank">http://www.jpl.nasa.gov/galileo/sepo</a>.<br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01647" onclick="window.open(this.href); return false;" title="Voir l'image 	 PIA01647:  Agenor Linea in Color	  sur le site de la NASA">Voir l'image 	 PIA01647:  Agenor Linea in Color	  sur le site de la NASA.</a></div>
PIA01647: Agenor Linea in Color
<h1>PIA01653:  Rugged Terrain on Europa</h1><div class="PIA01653" lang="en" style="width:800px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p>This mosaic of an area just southeast of the <a href="/catalog/PIA01633">Tyre multi-ring structure</a> on Jupiter's moon Europa combines two sets of images taken by NASA's Galileo spacecraft. Features in this area include pits, plains, and regions of chaotic terrain. The circular to oval shaped pits that contain dark material are secondary craters formed by debris from the Tyre impact. While the origin of the dark material is uncertain, it could be subsurface material that was excavated by impacts or a deposit left behind as surface ice turned to vapor. Two types of plains can be distinguished: lineated and ridged. Ridged plains are composed of numerous small ridges which trend from northwest to southeast while lineated plains appear finer in texture with more closely spaced north to south trending ridges. Two types of chaotic terrain can be distinguished: hummocky and blocky. Hummocky chaos regions appear to contain very fine textured matrix material with a few small "rafts" that are commonly seen in other chaos regions. Blocky chaos regions contain the large (greater than 2 kilometers or 1.25 miles across) "rafts" of the pre-existing crustal material which are similar to those seen in the <a href="/catalog/PIA01127">Conamara Chaos</a> region of Europa.</p><p>North is to the top of the image and the sun illuminates the surface from the left. The image is in an orthographic projection, centered at 13 degrees north latitude and 110 degrees west longitude, and covers an area approximately 45 by 64 kilometers (28 by 40 miles). The resolution is about 30 meters (100 feet) across. The images were taken on May 31, 1998 at a range of approximately 4200 kilometers (2625 miles) by the Solid State Imaging (SSI) system on NASA's Galileo spacecraft.</p><p>The Jet Propulsion Laboratory, Pasadena, CA manages the Galileo mission or NASA's Office of Space Science, Washington, DC.</p><p>This image and other images and data received from Galileo are posted on the World Wide Web, on the Galileo mission home page at URL<a href="http://solarsystem.nasa.gov/galileo/" target="_blank">http://solarsystem.nasa.gov/galileo/</a>. Background information and educational context for the images can be found at <a href="http://www2.jpl.nasa.gov/galileo/sepo/" target="_blank">http://www.jpl.nasa.gov/galileo/sepo</a>.<br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01653" onclick="window.open(this.href); return false;" title="Voir l'image 	 PIA01653:  Rugged Terrain on Europa	  sur le site de la NASA">Voir l'image 	 PIA01653:  Rugged Terrain on Europa	  sur le site de la NASA.</a></div>
PIA01653: Rugged Terrain on Europa
<h1>PIA01661:  Large Impact Structures on Europa</h1><div class="PIA01661" lang="en" style="width:800px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p>The picture compares four large impact structures on Jupiter's icy moon, Europa. Clockwise, from top left, are Pwyll, Cilix, Tyre, and Mannann'an. Impact structures with diameters of more than 20 kilometers are rather rare on Europa. Tyre is most unusual. While the effective crater, which is somewhat larger than the prominent large bull's eye feature, is about 40 kilometers (25 miles) across, the entire structure is much larger. The concentric rings display relatively little relief. Some of the smaller craters near Tyre were formed by material ejected by and then redeposited from the impact which formed Tyre. One hypothesis for such characteristics is that the impactor which formed Tyre penetrated through an icy crust into a less brittle layer. While Pwyll, Cilix, and Mannann'an also display shallow crater depths for their size, they more closely resemble similar sized craters on two neighboring moons of Jupiter, Ganymede and Callisto. Perhaps the impactor did not punch through the upper crust during these events. This might have been the case if the impacting body was smaller or weaker than in the case of Tyre or if the crust was thinner at the location of Tyre during the impact event.</p><p>North is to the top of the picture. The sun illuminates the surfaces from the right, except for Tyre, where the sun illuminates the surface from the left. The horizontal and vertical grey lines in the Tyre mosaic indicate gaps in the data received for this image. The Pwyll image was taken on December 16, 1997, Cilix on May 31, 1998,Tyre on March 29, 1998, and Mannann'an on March 29, 1998. All images were taken by the Solid State Imaging (SSI) system on NASA's Galileo spacecraft.</p><p>The Jet Propulsion Laboratory, Pasadena, CA manages the Galileo mission for NASA's Office of Space Science, Washington, DC.</p><p>This image and other images and data received from Galileo are posted on the World Wide Web, on the Galileo mission home page at URL<a href="http://solarsystem.nasa.gov/galileo/" target="_blank">http://solarsystem.nasa.gov/galileo/</a>. Background information and educational context for the images can be found at URL<a href="http://www2.jpl.nasa.gov/galileo/sepo/" target="_blank">http://www.jpl.nasa.gov/galileo/sepo</a>."><a href="http://www2.jpl.nasa.gov/galileo/sepo/" target="_blank">http://www.jpl.nasa.gov/galileo/sepo</a>.</a><p><br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01661" onclick="window.open(this.href); return false;" title="Voir l'image 	 PIA01661:  Large Impact Structures on Europa	  sur le site de la NASA">Voir l'image 	 PIA01661:  Large Impact Structures on Europa	  sur le site de la NASA.</a></div>
PIA01661: Large Impact Structures on Europa
<h1>PIA01662:  Topography around Europa's Cilix crater</h1><div class="PIA01662" lang="en" style="width:700px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p>This shaded relief highlights relative elevations around Cilix crater on Jupiter's moon, Europa. North is to the top of the picture which was created by shading a model of the surface with the brightnesses resulting from artificial illumination. The sun illumination was artificially computed to be shining from the right (east) while 60 degrees above the horizon. Several images of Cilix, obtained at varying viewing geometries are combined to calculate a three dimensional surface model.</p><p>The Cilix impact structure is situated at about 180 degrees longitude near Europa's equator. The crater is 20 kilometers (12 miles) across, with rims as high as 500 meters (545 yards). The massif near the crater center is as high as the rim. While the western portion of the rim shows pronounced slumping of the crater walls, the opposite rim does not. The crater floor appears to have rebounded into a domed shape. Linear ridges in the shaded relief may be double ridges which are not fully resolved by the topographic model.</p><p>The stereo perspective combines images obtained from different camera positions. Such a three dimensional model is similar to the three dimensional scenes our brains construct from images seen by the left and right eyes. The figure uses uniformly grey patches, outlined in black, to indicate locations where gaps in the data prevented three dimensional modelling. The best resolution is 65 meters per picture element. The stereo images were taken on May 31st, 1998 at ranges of 12,300 kilometers (7,650 miles) and 4,500 kilometers (2,800 miles) by the Solid State Imaging (SSI) system on NASA's Galileo spacecraft.</p><p>The Jet Propulsion Laboratory, Pasadena, CA manages the Galileo mission for NASA's Office of Space Science, Washington, DC.</p> This image and other images and data received from Galileo are posted on the World Wide Web, on the Galileo mission home page at URL<a href="http://solarsystem.nasa.gov/galileo/" target="_blank">http://solarsystem.nasa.gov/galileo/</a>. Background information and educational context for the images can be found at <a href="http://www2.jpl.nasa.gov/galileo/sepo/" target="_blank">http://www.jpl.nasa.gov/galileo/sepo</a>.<br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01662" onclick="window.open(this.href); return false;" title="Voir l'image 	 PIA01662:  Topography around Europa's Cilix crater	  sur le site de la NASA">Voir l'image 	 PIA01662:  Topography around Europa's Cilix crater	  sur le site de la NASA.</a></div>
PIA01662: Topography around Europa's Cilix crater
<h1>PIA01664:  Three dimensional view of Double Ridges on Europa</h1><div class="PIA01664" lang="en" style="width:800px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p>These images reveal the dramatic topography of Europa's icy crust. North is to the right. An east-west running double ridge with a deep intervening trough cuts across older background plains and the darker wedge shaped band. The numerous cracks and bands of such terrain may indicate where the crust has pulled apart and sometimes allowed dark material from beneath the surface to well up and fill the cracks. A computer generated three dimensional perspective (upper right) shows that bright material, probably pure water ice, prevails at the ridge crests and slopes while most dark material (perhaps ice mixed with silicates or hydrated salts) is confined to lower areas such as valley floors. The northernmost (right) slope which faces north, however, has a larger concentration of dark material than south facing slopes. The model on the lower right has been color coded to accentuate elevations. The red tones indicate that the crests of the ridge system reach elevations of more than 300 meters (330 yards) above the surrounding furrowed plains (blue and purple tones). The two ridges are separated by a valley about 1.5 kilometers (0.9 miles) wide.</p><p>The stereo perspective combines high resolution images obtained from two different viewing angles. Such a three dimensional model is similar to the three dimensional scenes our brains construct when both eyes view something from two angles.</p><p>North is to the right, and the sun illuminates the scene from northwest. The images were taken by the Solid State Imaging (SSI) system on NASA's Galileo spacecraft. The regional context (left), centered at about 16 degrees south latitude, 195 degrees west longitude, was imaged on November 6th, 1996 at a range of about 41,000 kilometers (25,500 miles). The higher resolution stereo images were taken on December 16th, 1997, at ranges of 5,800 kilometers(3,600 miles) and 2,600 kilometers (1,600 miles) leading to a best resolution of 26 meters per picture element.</p><p>The Jet Propulsion Laboratory, Pasadena, CA manages the Galileo mission for NASA's Office of Space Science, Washington, DC.</p><p>This image and other images and data received from Galileo are posted on the World Wide Web, on the Galileo mission home page at URL<a href="http://solarsystem.nasa.gov/galileo/" target="_blank">http://solarsystem.nasa.gov/galileo/</a>. Background information and educational context for the images can be found at URL<a href="http://www2.jpl.nasa.gov/galileo/sepo/" target="_blank">http://www.jpl.nasa.gov/galileo/sepo</a>."><a href="http://www2.jpl.nasa.gov/galileo/sepo/" target="_blank">http://www.jpl.nasa.gov/galileo/sepo</a>.</a></p><br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01664" onclick="window.open(this.href); return false;" title="Voir l'image 	 PIA01664:  Three dimensional view of Double Ridges on Europa	  sur le site de la NASA">Voir l'image 	 PIA01664:  Three dimensional view of Double Ridges on Europa	  sur le site de la NASA.</a></div>
PIA01664: Three dimensional view of Double Ridges on Europa
<h1>PIA01665:  Red-Blue Three dimensional view of Pwyll crater</h1><div class="PIA01665" lang="en" style="width:800px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p>This three dimensional effect is created by superimposing images of Jupiter's moon, Europa, which were taken from two slightly different perspectives. When viewed through red (left eye) and blue (right eye) filters, the product, an anaglyph, shows variations in height of surface features.</p><p>The anaglyph shows Pwyll crater on Jupiter's icy satellite Europa. The crater is about 26 kilometers (16 miles) across and has a central peak which rises approximately 600 meters (almost 2,000 feet) above the crater floor. The heavily degraded rim reaches a height of only 300 meters. A central peak that is higher than the crater rim is unusual among other craters in the Solar System. A continuous ejecta blanket around the impact structure rises above the surrounding landscape and is at about the same topographic level as the crater floor. The Pwyll impact appears to have occurred on a northwest to southeast (upper left to lower right) trending slope.</p><p>North is to the top of the picture. Pwyll is located at about 25 degrees south latitude and 271 degrees west longitude. The stereo perspective combines high resolution images obtained from two different camera positions. Such a three dimensional model is similar to the three dimensional scenes our brains construct from images seen by the left and right eyes. The picture is based on such a computer generated model using images taken by the Solid State Imaging (SSI) system on NASA's Galileo spacecraft on two separate orbits. The grey band running completely across the image just north of Pwyllis where a gap in the data prevented three dimensional modelling. The images of Pwyll were taken from different viewing geometries on February 20, 1997 and December 16, 1997 at ranges of 13,200 kilometers (8,200 miles) and 13,500 kilometers (8,400 miles).</p><p>The Jet Propulsion Laboratory, Pasadena, CA manages the Galileo mission for NASA's Office of Space Science, Washington, DC.</p><p>This image and other images and data received from Galileo are posted on the World Wide Web, on the Galileo mission home page at URL<a href="http://solarsystem.nasa.gov/galileo/" target="_blank">http://solarsystem.nasa.gov/galileo/</a>. Background information and educational context for the images can be found at <a href="http://www2.jpl.nasa.gov/galileo/sepo/" target="_blank">http://www.jpl.nasa.gov/galileo/sepo</a>.<br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01665" onclick="window.open(this.href); return false;" title="Voir l'image 	 PIA01665:  Red-Blue Three dimensional view of Pwyll crater	  sur le site de la NASA">Voir l'image 	 PIA01665:  Red-Blue Three dimensional view of Pwyll crater	  sur le site de la NASA.</a></div>
PIA01665: Red-Blue Three dimensional view of Pwyll crater
<h1>PIA01970:  Europa from 2,869,252 kilometers</h1><div class="PIA01970" lang="en" style="width:450px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;">View of Europa taken from a range of 2,869,252 kilometers (1.6 million miles) on March 2 at 2:00 PM. The color composite is made from three black and white images taken through the orange, green and violet filters. The 170 longitude is at the center of the picture; this is the face away from Jupiter. Irregular dark and bright patches on the surface are different from the patterns on the other satellites of Jupiter and those on the Moon, Mars and Mercury. Dark intersecting lines may be faults that break the crust. JPL manages and controls the Voyager Project for NASA's Office of Space Science.<br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01970" onclick="window.open(this.href); return false;" title="Voir l'image 	 PIA01970:  Europa from 2,869,252 kilometers	  sur le site de la NASA">Voir l'image 	 PIA01970:  Europa from 2,869,252 kilometers	  sur le site de la NASA.</a></div>
PIA01970: Europa from 2,869,252 kilometers

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