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{"event":"custom_event","event_name":"view_search_result","event_category":"browse_catalog","keyword":"saturne","search_type":"standard","search_bridgeman_artists":"false","search_mode":"automatic","search_zero_result":"false","search_results":1067,"search_results_page_number":18}

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Images of 'Saturne' found, 1,067

 
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Launch Vehicles, USA Saturn V rocket on the launch pad, 1969

UIS5074423

Launch Vehicles, USA Saturn V rocket on the launch pad, 1969

UIS5074423

 
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A Modern Picture Gallery

Witherington, William Frederick (1785-1865)

USB1159740

A Modern Picture Gallery

Witherington, William Frederick (1785-1865)

USB1159740

 
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Launch Vehicles, USA Saturn V rocket for the Apollo 12 mission on mobile launch platform, 1969

UIS5070225

Launch Vehicles, USA Saturn V rocket for the Apollo 12 mission on mobile launch platform, 1969

UIS5070225

 
Saturn seen by the Cassini probe on 23/07/2008 - Saturn seen by Cassini spacecraft on july 23 2008 - Saturn seen by the Cassini probe on 23 July 2008 at a distance of 1.1 million km from the planet. Mosaic of 30 images. Several satellites are visible in this image: Titan, Janus, Mimas, Pandora, Epimethee and Enceladus. As Saturn advances in its orbit toward equinox and the sun gradually moves northward on the planet, the motion of Saturn's ring shadows and the changing colors of its atmosphere continue to transform the face of Saturn as seen by Cassini. This captivating natural color view was created from images collected shortly after Cassini began its extended Equinox Mission in July 2008. This mosaic combines 30 images - - 10 each of red, green and blue light - - taken over the course of approximately two hours as Cassini panned its wide - angle camera across the entire planet and ring system on July 23, 2008, from a southerly elevation of 6 degrees. Six moons complete this construc

PIX4625214

Saturn seen by the Cassini probe on 23/07/2008 - Saturn seen by Cassini spacecraft on july 23 2008 - Saturn seen by the Cassini probe on 23 July 2008 at a distance of 1.1 million km from the planet. Mosaic of 30 images. Several satellites are visible in this image: Titan, Janus, Mimas, Pandora, Epimethee and Enceladus. As Saturn advances in its orbit toward equinox and the sun gradually moves northward on the planet, the motion of Saturn's ring shadows and the changing colors of its atmosphere continue to transform the face of Saturn as seen by Cassini. This captivating natural color view was created from images collected shortly after Cassini began its extended Equinox Mission in July 2008. This mosaic combines 30 images - - 10 each of red, green and blue light - - taken over the course of approximately two hours as Cassini panned its wide - angle camera across the entire planet and ring system on July 23, 2008, from a southerly elevation of 6 degrees. Six moons complete this construc

PIX4625214

 
Japet, satellite of Saturn, seen by Cassini - Saturn's moon Iapetus seen by Cassini spacecraft. - Mosaic in false colors of Japet, a satellite of 1436 kilometers in diameter, taken by the Cassini probe on 10 September 2007 has a distance of 73,000 km from the satellite. The image shows the bright side of the satellite; a large 450 km wide impact basin is visible towards the bottom of the image. This false - color mosaic shows the entire hemisphere of Iapetus (1,468 kilometers, or 912 miles across) visible from Cassini on Sept. 10 2007 at a distance of about 73,000 kilometers (45,000 miles) from Iapetus. Near the top of the mosaic, numerous impact features are visible, including the craters Ogier and Charlemagne. The most prominent topographic feature in this view, in the bottom half of the mosaic, is a 450 - kilometer (280 - mile) wide impact basin

PIX4625416

Japet, satellite of Saturn, seen by Cassini - Saturn's moon Iapetus seen by Cassini spacecraft. - Mosaic in false colors of Japet, a satellite of 1436 kilometers in diameter, taken by the Cassini probe on 10 September 2007 has a distance of 73,000 km from the satellite. The image shows the bright side of the satellite; a large 450 km wide impact basin is visible towards the bottom of the image. This false - color mosaic shows the entire hemisphere of Iapetus (1,468 kilometers, or 912 miles across) visible from Cassini on Sept. 10 2007 at a distance of about 73,000 kilometers (45,000 miles) from Iapetus. Near the top of the mosaic, numerous impact features are visible, including the craters Ogier and Charlemagne. The most prominent topographic feature in this view, in the bottom half of the mosaic, is a 450 - kilometer (280 - mile) wide impact basin

PIX4625416

 
Saturn seen by the Cassini probe on 10 - 09 - 2007 - Saturn seen by Cassini spacecraft Sept. 10 2007. - Saturn seen by the Cassini probe on 10 - 09 - 2007 at a distance of 3.3 million km from the planet shortly before it flew over the Japet satellite. Mosaic of 45 images. Several satellites are visible in this image; from right to left: Titan, Tethys, Rhea, Mimas, Enceladus and Dione. While on final approach for its Sept. 2007 close encounter with Saturn's moon Iapetus, Cassini spun around to take in a sweeping view of the Saturn System. Iapetus (1,468 kilometers, or 912 miles across) is the only major moon of Saturn with a significant inclination to its orbit. From the other major satellites, the rings would appear almost edge - on, but from Iapetus, the rings usually appear at a tilt, as seen here. This natural color mosaic consists of 15 red, green and blue spectral filter images acquired in five wide - angle camera footprints that swept across the scene. Moons visible in this image

PIX4625105

Saturn seen by the Cassini probe on 10 - 09 - 2007 - Saturn seen by Cassini spacecraft Sept. 10 2007. - Saturn seen by the Cassini probe on 10 - 09 - 2007 at a distance of 3.3 million km from the planet shortly before it flew over the Japet satellite. Mosaic of 45 images. Several satellites are visible in this image; from right to left: Titan, Tethys, Rhea, Mimas, Enceladus and Dione. While on final approach for its Sept. 2007 close encounter with Saturn's moon Iapetus, Cassini spun around to take in a sweeping view of the Saturn System. Iapetus (1,468 kilometers, or 912 miles across) is the only major moon of Saturn with a significant inclination to its orbit. From the other major satellites, the rings would appear almost edge - on, but from Iapetus, the rings usually appear at a tilt, as seen here. This natural color mosaic consists of 15 red, green and blue spectral filter images acquired in five wide - angle camera footprints that swept across the scene. Moons visible in this image

PIX4625105

 
Saturn seen by the Cassini probe on 9 - 05 - 2007 - Saturn in natural colors seen by Cassini spacecraft May 9 2007. - Saturn seen by the Cassini probe on 9 - 05 - 2007 at a distance of 1.1 million km from the planet. Mosaic of 45 images. Three satellites are visible in this image: Mimas (upper right), Janus (lower right) and Pandora (barely visible, near ring F, lower left). This natural color mosaic was acquired by the Cassini spacecraft as it soared 39 degrees above the unilluminated side of the rings. Little light makes its way through the rings to be scattered in Cassini's direction in this viewing geometry, making the rings appear somewhat dark compared to the reflective planet. Bright clouds play in the blue - gray skies of the north. The ring shadows continue to caress the planet as they slide farther south toward their momentary disappearance during equinox in 2009. The rings' reflected light illuminates the southern hemisphere on Saturn's night side. Three of Saturn's moons ar

PIX4625121

Saturn seen by the Cassini probe on 9 - 05 - 2007 - Saturn in natural colors seen by Cassini spacecraft May 9 2007. - Saturn seen by the Cassini probe on 9 - 05 - 2007 at a distance of 1.1 million km from the planet. Mosaic of 45 images. Three satellites are visible in this image: Mimas (upper right), Janus (lower right) and Pandora (barely visible, near ring F, lower left). This natural color mosaic was acquired by the Cassini spacecraft as it soared 39 degrees above the unilluminated side of the rings. Little light makes its way through the rings to be scattered in Cassini's direction in this viewing geometry, making the rings appear somewhat dark compared to the reflective planet. Bright clouds play in the blue - gray skies of the north. The ring shadows continue to caress the planet as they slide farther south toward their momentary disappearance during equinox in 2009. The rings' reflected light illuminates the southern hemisphere on Saturn's night side. Three of Saturn's moons ar

PIX4625121

 
Saturn seen by the Cassini probe 04/2007 - Saturn from Cassini spacecraft 04/2007 - Image obtained by the Cassini probe on 13 April 2007 at a distance of 1.8 million km from the planet. Colorful Saturn tilts its darkened ringplane towards Cassini. Against the dark sky, the rings are made visible by the light that scatters through them towards the camera. The F ring shepherd moon Pandora (84 kilometers, or 52 miles across) is faintly visible at the top, left of center. Pandora's brightness was increased by a factor of three to aid its visibility. This view looks toward the unilluminated side of the rings from about 18 degrees above the ringplane. The planet is visible through the innermost and outermost portions of the rings. The images were obtained by the Cassini spacecraft wide - angle camera on April 13, 2007, at a distance of approximately 1.8 million kilometers (1.1 million miles) from Saturn

PIX4625102

Saturn seen by the Cassini probe 04/2007 - Saturn from Cassini spacecraft 04/2007 - Image obtained by the Cassini probe on 13 April 2007 at a distance of 1.8 million km from the planet. Colorful Saturn tilts its darkened ringplane towards Cassini. Against the dark sky, the rings are made visible by the light that scatters through them towards the camera. The F ring shepherd moon Pandora (84 kilometers, or 52 miles across) is faintly visible at the top, left of center. Pandora's brightness was increased by a factor of three to aid its visibility. This view looks toward the unilluminated side of the rings from about 18 degrees above the ringplane. The planet is visible through the innermost and outermost portions of the rings. The images were obtained by the Cassini spacecraft wide - angle camera on April 13, 2007, at a distance of approximately 1.8 million kilometers (1.1 million miles) from Saturn

PIX4625102

 
Saturn by Voyager 2 - Rings in fake colors - Composition differences within Saturn's rings. Voyager 2 - Image in false colors made by the Voyager 2 probe on August 17, 1981 at a distance of 8.9 million km from the planet. This image has been reconstructed from 3 black and white photos taken through the UV, green and orange filters. The contrasts were exaggerated. The different colors correspond to differences in the chemical composition of the particles that make up the rings. Possible variations in chemical composition from one part of Saturn's ring system to another are visible in this Voyager 2 picture as subtle color variations that can be recorded with special computer - processing techniques. This highly enhanced color view was assembled from clear, orange and ultraviolet frames obtained Aug. 17 from a distance of 8.9 million kilometers (5.5 million miles). In addition to the previously known blue color of the C - ring and the Cassini Division, the picture shows additional color

PIX4624957

Saturn by Voyager 2 - Rings in fake colors - Composition differences within Saturn's rings. Voyager 2 - Image in false colors made by the Voyager 2 probe on August 17, 1981 at a distance of 8.9 million km from the planet. This image has been reconstructed from 3 black and white photos taken through the UV, green and orange filters. The contrasts were exaggerated. The different colors correspond to differences in the chemical composition of the particles that make up the rings. Possible variations in chemical composition from one part of Saturn's ring system to another are visible in this Voyager 2 picture as subtle color variations that can be recorded with special computer - processing techniques. This highly enhanced color view was assembled from clear, orange and ultraviolet frames obtained Aug. 17 from a distance of 8.9 million kilometers (5.5 million miles). In addition to the previously known blue color of the C - ring and the Cassini Division, the picture shows additional color

PIX4624957

 
Japet, satellite of Saturn, seen by Cassini - Crescent of Iapetus seen by Cassini spacecraft. - Mosaic in fake colors of Japet, a satellite of 1436 kilometers in diameter, taken by the Cassini probe on 10 September 2007 has a distance of 83 000 km from the satellite. Iapetus, 1,468 kilometers (912 miles) across, seen here in false color, is unique in its dramatic variation in brightness between the northern polar region and the middle and low latitudes. Equally prominent is the moon's equatorial ridge of towering mountains. The profile of the ridge against the darkness of space reveals that it is topped by a cratered plateau approximately 15 kilometers (9 miles) wide. Further west, the profile of the ridge changes from a long plateau to discrete peaks. The mosaic consists of four image footprints across the surface of Iapetus and has a resolution of 489 meters (0.3 miles) per pixel. The color seen in this view represents an expansion of the wavelength region of the electromagnetic spec

PIX4625407

Japet, satellite of Saturn, seen by Cassini - Crescent of Iapetus seen by Cassini spacecraft. - Mosaic in fake colors of Japet, a satellite of 1436 kilometers in diameter, taken by the Cassini probe on 10 September 2007 has a distance of 83 000 km from the satellite. Iapetus, 1,468 kilometers (912 miles) across, seen here in false color, is unique in its dramatic variation in brightness between the northern polar region and the middle and low latitudes. Equally prominent is the moon's equatorial ridge of towering mountains. The profile of the ridge against the darkness of space reveals that it is topped by a cratered plateau approximately 15 kilometers (9 miles) wide. Further west, the profile of the ridge changes from a long plateau to discrete peaks. The mosaic consists of four image footprints across the surface of Iapetus and has a resolution of 489 meters (0.3 miles) per pixel. The color seen in this view represents an expansion of the wavelength region of the electromagnetic spec

PIX4625407

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