'High-angle' Bilder und Clips Suchergebnisse

Type # for projects,to access projects, > for users, and ? for help.

Ihre AuswahlIhre aktuelle Auswahl

{"event":"ecommerce_event","event_name":"view_item","event_category":"browse_catalog","ecommerce":{"items":[{"item_id":"PIX4574942","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"infrared_jupiter_seen_by_the_new_horizons_probe_jupiter_seen_by_new_horizons_spacecraft_view_of_jupi","item_variant":"undefined"},{"item_id":"PIX4670945","item_category2":"no_copyright","item_category3":"standard","item_category4":"laurent_laveder","item_category5":"not_balown","item_list_name":"search_results","item_name":"halo_around_the_sun_sun_halo_halos_are_due_to_the_light_of_the_sun_reflected_by_high_altitude_clouds","item_variant":"undefined"},{"item_id":"PIX4596489","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"fusee_saturn_v_apollo_12_apollo_12_spacecraft_at_launch_complex_39_the_saturn_v_rocket_leaves_the_as","item_variant":"undefined"},{"item_id":"UIS5064048","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"jean_baptiste_biot_french_physicist_and_astronomer_c_1850_1862","item_variant":"undefined"},{"item_id":"FLM1266924","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"city_of_treasures_part_8_children_buy_cradle_at_market_market_closing_paris_1951","item_variant":"undefined"},{"item_id":"PIX4670921","item_category2":"no_copyright","item_category3":"standard","item_category4":"laurent_laveder","item_category5":"not_balown","item_list_name":"search_results","item_name":"halo_around_the_sun_sun_halo_halos_are_due_to_the_light_of_the_sun_reflected_by_high_altitude_clouds","item_variant":"undefined"},{"item_id":"PIX4670979","item_category2":"no_copyright","item_category3":"standard","item_category4":"laurent_laveder","item_category5":"not_balown","item_list_name":"search_results","item_name":"halo_around_the_sun_sun_halo_halos_are_due_to_the_light_of_the_sun_reflected_by_high_altitude_clouds","item_variant":"undefined"},{"item_id":"PIX4582276","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"titan_saturn_satellite_seen_by_cassini_saturn_s_moon_titan_as_seen_by_cassini_spacecraft_titan_image","item_variant":"undefined"},{"item_id":"PIX4671758","item_category2":"no_copyright","item_category3":"standard","item_category4":"alex_tudorica","item_category5":"not_balown","item_list_name":"search_results","item_name":"halo_and_light_column_ice_halos_near_zeel_am_see_austria_a_light_column_is_created_by_the_reflection","item_variant":"undefined"},{"item_id":"LAL300748","item_category2":"no_copyright","item_category3":"standard","item_category4":"hardy_wilf_wilfred_20th_century","item_category5":"not_balown","item_list_name":"search_results","item_name":"measuring_time","item_variant":"undefined"},{"item_id":"CH3057859","item_category2":"out_of_copyright","item_category3":"standard","item_category4":"french_school_18th_century","item_category5":"not_balown","item_list_name":"search_results","item_name":"royal_louis_xv_commode_c_1757_ormolu_mounted_tulipwood_amaranth_sycamore_marquetry","item_variant":"undefined"},{"item_id":"MMM7342589","item_category2":"out_of_copyright","item_category3":"standard","item_category4":"velde_willem_van_de_the_younger_1633_1707","item_category5":"not_balown","item_list_name":"search_results","item_name":"a_mediterranean_brigantine_drifting_onto_a_rocky_coast_in_a_storm_c_1700_oil_on_canvas","item_variant":"undefined"},{"item_id":"PFH3085655","item_category2":"out_of_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"hawaii_a_young_girl_of_the_sandwich_islands_watercolour_over_pencil_mikhail_tikhonovich_tikhanov_178","item_variant":"undefined"},{"item_id":"PIX4574952","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"jupiter_and_io_seen_by_the_new_horizons_probe","item_variant":"undefined"},{"item_id":"PIX4625583","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"tethys_saturn_satellite_seen_by_the_cassini_probe_saturn_s_moon_tethys_seen_by_cassini_spacecraft_th","item_variant":"undefined"},{"item_id":"PIX4675641","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"christchurch_and_the_peninsula_of_banks_new_zealand_from_space_christchurch_and_banks_peninsula_new_","item_variant":"undefined"},{"item_id":"PIX4622776","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"neptune_voyager_2_image_of_neptune_obtained_by_the_voyager_2_probe_on_august_14_1989_at_14_8_million","item_variant":"undefined"},{"item_id":"PIX4612202","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"galaxy_centaurus_a_ngc_5128_x_ray_view_radio_visible_galaxy_centaurus_a_in_different_wavelengths_fal","item_variant":"undefined"},{"item_id":"PIX4625007","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"saturn_en_jour_seen_by_cassini_backlit_saturn_seen_by_cassini_image_obtained_by_the_cassini_probe_on","item_variant":"undefined"},{"item_id":"IMO2708822","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"interieur_du_trump_tower","item_variant":"undefined"},{"item_id":"PIX4625026","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"saturn_rings_seen_by_cassini_saturn_s_rings_from_cassini_image_obtained_by_the_cassini_probe_on_janu","item_variant":"undefined"},{"item_id":"BAF7424512","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"vernede_collection_3_military_parade_girl_guiders_inspection_and_society_wedding","item_variant":"undefined"},{"item_id":"PIX4615862","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"march_opportunity_panorama_05_2007_march_d_star_panorama_by_opportunity_false_color_panorama_in_fake","item_variant":"undefined"},{"item_id":"PIX4615851","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"march_opportunity_panorama_05_2007_march_d_star_panorama_by_opportunity_false_color_panorama_in_fake","item_variant":"undefined"}]}}

Type # for projects,to access projects, > for users, and ? for help.

Erweiterte Suche Search Tips

Bilder zu 'High-angle' gefunden, 6,924

«
1
…
114
115
116
»

Infrared Jupiter seen by the New Horizons probe. - Jupiter seen by New Horizons spacecraft - View of Jupiter obtained on February 28, 2007 by the New Horizons probe. This infrared image shows the different altitudes of the Jovian clouds; in blue, the high altitudes clouds, in red, the lower clouds. Jupiter seen by New Horizons spacecraft during the Jupiter flyby in early 2007. This image is an infrared color composite taken by the spacecraft's near - infrared imaging spectrometer, the Linear Etalon Imaging Spectral Array (LEISA) at 1:40 UT on Feb. 28, 2007. The infrared wavelengths used (red: 1.59 um, green: 1.94 um, blue: 1.85 um) highlight variations in the altitude of the Jovian cloud tops, with blue denoting high - altitude clouds and hazes, and red indicating deeper clouds. The prominent bluish - white oval is the Great Red Spot. The observation was made at a solar phase angle of 75 degrees but has been projected onto a crescent to remove distortion caused by Jupiter's rotation du

Infrared Jupiter seen by the New Horizons probe. - Jupiter seen by New Horizons spacecraft - View of Jupiter obtained on February 28, 2007 by the New Horizons probe. This infrared image shows the different altitudes of the Jovian clouds; in blue, the high altitudes clouds, in red, the lower clouds. Jupiter seen by New Horizons spacecraft during the Jupiter flyby in early 2007. This image is an infrared color composite taken by the spacecraft's near - infrared imaging spectrometer, the Linear Etalon Imaging Spectral Array (LEISA) at 1:40 UT on Feb. 28, 2007. The infrared wavelengths used (red: 1.59 um, green: 1.94 um, blue: 1.85 um) highlight variations in the altitude of the Jovian cloud tops, with blue denoting high - altitude clouds and hazes, and red indicating deeper clouds. The prominent bluish - white oval is the Great Red Spot. The observation was made at a solar phase angle of 75 degrees but has been projected onto a crescent to remove distortion caused by Jupiter's rotation du

PIX4574942

Halo around the Sun - Sun Halo - Halos are due to the light of the Sun reflected by high-altitude clouds, cirrostratus, composed of ice crystals. They bend the light and cause a perfect circle around the Sun. Here we can see: - around the Sun, the halo of 22* radius, rather little contrast. - on the left of the Sun, a brilliant parhely but little colour. - on the top of the halo of 22* radius, the upper arc tangent in the shape of a U evase. - on the left, the arc of Parry. - near the zenith, the arc circumzenithal, colour. 28 October 2006, Quimper O are caused by sunlight being refracted by cirro - stratus clouds. These are thin clouds, very high in the atmosphere, and are composed of ice crystals. They bend light at a 22 degree angle, which creates a halo around the sun that is 44 degrees in diameter. In brief: - around the Sun, the 22* halo, not very contrasted. - on the left of the Sun, a bright parhelia uncolored. - atop the 22* halo, the upper tangent arc. - on the left, the Parr

Halo around the Sun - Sun Halo - Halos are due to the light of the Sun reflected by high-altitude clouds, cirrostratus, composed of ice crystals. They bend the light and cause a perfect circle around the Sun. Here we can see: - around the Sun, the halo of 22* radius, rather little contrast. - on the left of the Sun, a brilliant parhely but little colour. - on the top of the halo of 22* radius, the upper arc tangent in the shape of a U evase. - on the left, the arc of Parry. - near the zenith, the arc circumzenithal, colour. 28 October 2006, Quimper O are caused by sunlight being refracted by cirro - stratus clouds. These are thin clouds, very high in the atmosphere, and are composed of ice crystals. They bend light at a 22 degree angle, which creates a halo around the sun that is 44 degrees in diameter. In brief: - around the Sun, the 22* halo, not very contrasted. - on the left of the Sun, a bright parhelia uncolored. - atop the 22* halo, the upper tangent arc. - on the left, the Parr

Laurent Laveder

PIX4670945

Fusee Saturn V - Apollo 12 - Apollo 12 spacecraft at Launch Complex 39 - The Saturn V rocket leaves the assembly building to be brought to its firing pitch. 08/09/1969. High - angle view at Launch Complex 39, Kennedy Space Center (KSC), showing the Apollo 12 (Spacecraft 108/Lunar Module 6/Saturn 507) space vehicle leaving the Vehicle Assembly Building (VAB) on the way to Pad A. The Saturn V stack and its mobile launch tower are atop a huge crawler - transporter. Apollo 12 is scheduled as the second lunar landing mission. The crew will be astronauts Charles Conrad Jr., commander; Richard F. Gordon Jr., command module pilot; and Alan L. Bean, lunar module pilot. Sep 8 1969

Fusee Saturn V - Apollo 12 - Apollo 12 spacecraft at Launch Complex 39 - The Saturn V rocket leaves the assembly building to be brought to its firing pitch. 08/09/1969. High - angle view at Launch Complex 39, Kennedy Space Center (KSC), showing the Apollo 12 (Spacecraft 108/Lunar Module 6/Saturn 507) space vehicle leaving the Vehicle Assembly Building (VAB) on the way to Pad A. The Saturn V stack and its mobile launch tower are atop a huge crawler - transporter. Apollo 12 is scheduled as the second lunar landing mission. The crew will be astronauts Charles Conrad Jr., commander; Richard F. Gordon Jr., command module pilot; and Alan L. Bean, lunar module pilot. Sep 8 1969

PIX4596489

Jean-Baptiste Biot, French physicist and astronomer, c 1850-1862

Jean-Baptiste Biot, French physicist and astronomer, c 1850-1862

UIS5064048

City of Treasures part 8 - children buy cradle at market. Market closing Paris 1951

City of Treasures part 8 - children buy cradle at market. Market closing Paris 1951

FLM1266924

Halo around the Sun - Sun Halo - Halos are due to the light of the Sun reflected by high-altitude clouds, cirrostratus, composed of ice crystals. They bend the light and cause a perfect circle around the Sun. Here we can see: - around the Sun, the halo of 22* radius, rather little contrast. - on the right of the Sun, a brilliant parhely but little colour. - at the top of the halo of 22* radius, the upper arc tangent in the shape of a U evase. - above, “” parallele””” to the halo of 22* radius, the arc of Parry. - near the zenith, the cirucmzenithal arc, very colorful. - just in below, tangent and very discreet, l'arc supralateral. 28 October 2006, Quimper Halos are caused by sunlight being refracted by cirro - stratus clouds. These are thin clouds, very high in the atmosphere, and are composed of ice crystals. They bend light at a 22 degree angle, which creates a halo around the sun that is 44 degrees in diameter. In brief: - around the Sun, the 22* halo, not very contrasted. - on the

Halo around the Sun - Sun Halo - Halos are due to the light of the Sun reflected by high-altitude clouds, cirrostratus, composed of ice crystals. They bend the light and cause a perfect circle around the Sun. Here we can see: - around the Sun, the halo of 22* radius, rather little contrast. - on the right of the Sun, a brilliant parhely but little colour. - at the top of the halo of 22* radius, the upper arc tangent in the shape of a U evase. - above, “” parallele””” to the halo of 22* radius, the arc of Parry. - near the zenith, the cirucmzenithal arc, very colorful. - just in below, tangent and very discreet, l'arc supralateral. 28 October 2006, Quimper Halos are caused by sunlight being refracted by cirro - stratus clouds. These are thin clouds, very high in the atmosphere, and are composed of ice crystals. They bend light at a 22 degree angle, which creates a halo around the sun that is 44 degrees in diameter. In brief: - around the Sun, the 22* halo, not very contrasted. - on the

Laurent Laveder

PIX4670921

Halo around the Sun - Sun Halo - Halos are due to the light of the Sun reflected by high-altitude clouds, cirrostratus, composed of ice crystals. They bend the light and cause a perfect circle around the Sun. Here we can see: - around the Sun, the halo of 22* radius, rather little contrast. - on the right of the Sun, a brilliant parhely but little colour. - at the top of the halo of 22* radius, the upper arc tangent in the shape of a U evase. - above, “” parallele””” to the halo of 22* radius, the arc of Parry. - near the zenith, the cirucmzenithal arc, very colorful. - just in below, tangent and very discreet, l'arc supralateral. 28 October 2006, Quimper Halos are caused by sunlight being refracted by cirro - stratus clouds. These are thin clouds, very high in the atmosphere, and are composed of ice crystals. They bend light at a 22 degree angle, which creates a halo around the sun that is 44 degrees in diameter. In brief: - around the Sun, the 22* halo, not very contrasted. - on the

Halo around the Sun - Sun Halo - Halos are due to the light of the Sun reflected by high-altitude clouds, cirrostratus, composed of ice crystals. They bend the light and cause a perfect circle around the Sun. Here we can see: - around the Sun, the halo of 22* radius, rather little contrast. - on the right of the Sun, a brilliant parhely but little colour. - at the top of the halo of 22* radius, the upper arc tangent in the shape of a U evase. - above, “” parallele””” to the halo of 22* radius, the arc of Parry. - near the zenith, the cirucmzenithal arc, very colorful. - just in below, tangent and very discreet, l'arc supralateral. 28 October 2006, Quimper Halos are caused by sunlight being refracted by cirro - stratus clouds. These are thin clouds, very high in the atmosphere, and are composed of ice crystals. They bend light at a 22 degree angle, which creates a halo around the sun that is 44 degrees in diameter. In brief: - around the Sun, the 22* halo, not very contrasted. - on the

Laurent Laveder

PIX4670979

Titan, Saturn satellite seen by Cassini - Saturn's moon Titan as seen by Cassini spacecraft: Titan images obtained by the Cassini probe on 21 March 2017. On the left, Titan seen in real colors. On the right, infrared image showing surface details as well as clouds in the northern hemisphere. These views were obtained with the Cassini spacecraft narrow-angle camera on March 21, 2017. Images taken using red, green and blue spectral filters were combined to create the natural-color view at left. The false-color view at right was made by substituting an infrared image (centered at 938 nanometers) for the red color channel. A large, bright and feathery band of summer clouds can be seen arcing across high northern latitudes in the view at right. The views were acquired at a distance of approximately 613,000 miles (986,000 kilometers) from Titan. Image scale is about 4 miles (6 kilometers) per pixel

Titan, Saturn satellite seen by Cassini - Saturn's moon Titan as seen by Cassini spacecraft: Titan images obtained by the Cassini probe on 21 March 2017. On the left, Titan seen in real colors. On the right, infrared image showing surface details as well as clouds in the northern hemisphere. These views were obtained with the Cassini spacecraft narrow-angle camera on March 21, 2017. Images taken using red, green and blue spectral filters were combined to create the natural-color view at left. The false-color view at right was made by substituting an infrared image (centered at 938 nanometers) for the red color channel. A large, bright and feathery band of summer clouds can be seen arcing across high northern latitudes in the view at right. The views were acquired at a distance of approximately 613,000 miles (986,000 kilometers) from Titan. Image scale is about 4 miles (6 kilometers) per pixel

PIX4582276

Halo and Light Column- Ice halos near Zeel am See, Austria - A light column is created by the reflection of a light source on the horizontal faces of ice crystals. So it takes a fairly stable atmosphere to keep these crystals parallel to the horizon. Lunar halo. The ice crystals in the cirrus decompose the lunar light (in fact, the solar light reflected by the lunar surface) as small prisms and can give rise to a large coloured circle. A paraselene consists of light spots located on the left and right at the height of the Moon. Austria, January 2016. A light pillar is created by the reflection of light on the horizontal face of ice cristals. So, a quiet atmosphere is needed in order that this cristals stay parallel to the horizon. Lunar halos are caused by moonlight being refracted by cirro-stratus clouds. These thin clouds are located very high in the atmosphere, and are composed of ice crystals. They bend light at a 22 degree angle, which creates a halo that is 44 degrees in diameter

Halo and Light Column- Ice halos near Zeel am See, Austria - A light column is created by the reflection of a light source on the horizontal faces of ice crystals. So it takes a fairly stable atmosphere to keep these crystals parallel to the horizon. Lunar halo. The ice crystals in the cirrus decompose the lunar light (in fact, the solar light reflected by the lunar surface) as small prisms and can give rise to a large coloured circle. A paraselene consists of light spots located on the left and right at the height of the Moon. Austria, January 2016. A light pillar is created by the reflection of light on the horizontal face of ice cristals. So, a quiet atmosphere is needed in order that this cristals stay parallel to the horizon. Lunar halos are caused by moonlight being refracted by cirro-stratus clouds. These thin clouds are located very high in the atmosphere, and are composed of ice crystals. They bend light at a 22 degree angle, which creates a halo that is 44 degrees in diameter

Alex Tudorica

PIX4671758

Measuring time

Hardy, Wilf (Wilfred) (20th century)

LAL300748

Royal Louis XV commode, c.1757 (ormolu-mounted tulipwood, amaranth, sycamore & marquetry)

Royal Louis XV commode, c.1757 (ormolu-mounted tulipwood, amaranth, sycamore & marquetry)

French School, (18th century)

CH3057859

A Mediterranean Brigantine Drifting Onto a Rocky Coast in a Storm, c.1700 (oil on canvas)

A Mediterranean Brigantine Drifting Onto a Rocky Coast in a Storm, c.1700 (oil on canvas)

Velde, Willem van de, the Younger (1633-1707)

MMM7342589

Hawaii: 'A Young Girl of the Sandwich Islands', watercolour over pencil, Mikhail Tikhonovich Tikhanov (1789-1862), 1818

Hawaii: 'A Young Girl of the Sandwich Islands', watercolour over pencil, Mikhail Tikhonovich Tikhanov (1789-1862), 1818

PFH3085655

Jupiter and Io seen by the New Horizons probe

Jupiter and Io seen by the New Horizons probe

PIX4574952

Tethys, Saturn satellite, seen by the Cassini probe - Saturn's moon Tethys seen by Cassini spacecraft - The southern pole of the Tethys satellite photographed by the Cassini probe on September 24, 2005. Mosaic of nine images. With this full - disk mosaic, Cassini presents the best view yet of the south pole of Saturn's moon Tethys. The giant rift Ithaca Chasma cuts across the disk. Much of the topography seen here, including that of Ithaca Chasma, has a soft, muted appearance. It is clearly very old and has been heavily bombarded by impacts over time. Many of the fresh - appearing craters (ones with crisp relief) exhibit unusually bright crater floors. The origin of the apparent brightness (or “” albedo”) contrast is not known. It is possible that impacts punched through to a brighter layer underneath, or perhaps it is brighter because of different grain sizes or textures of the crater floor material in comparison to material along the crater walls and surrounding surface. The moon's h

Tethys, Saturn satellite, seen by the Cassini probe - Saturn's moon Tethys seen by Cassini spacecraft - The southern pole of the Tethys satellite photographed by the Cassini probe on September 24, 2005. Mosaic of nine images. With this full - disk mosaic, Cassini presents the best view yet of the south pole of Saturn's moon Tethys. The giant rift Ithaca Chasma cuts across the disk. Much of the topography seen here, including that of Ithaca Chasma, has a soft, muted appearance. It is clearly very old and has been heavily bombarded by impacts over time. Many of the fresh - appearing craters (ones with crisp relief) exhibit unusually bright crater floors. The origin of the apparent brightness (or “” albedo”) contrast is not known. It is possible that impacts punched through to a brighter layer underneath, or perhaps it is brighter because of different grain sizes or textures of the crater floor material in comparison to material along the crater walls and surrounding surface. The moon's h

PIX4625583

Christchurch and the Peninsula of Banks (New Zealand) from space - Christchurch and Banks Peninsula, New Zealand - The Peninsula of Banks and the City of Christchurch seen from the International Space Station (ISS) on August 15, 2006. The Banks Peninsula is an ancient erode volcano forming a peninsula on the east coast of the South Island. Oblique view (the photograph was taken from a side angle) of the city of Christchurch, New Zealand. Snow highlights the peaks of the Banks Peninsula to the southeast of the city. The peninsula has a radically different landscape compared to the adjoining, flat Canterbury Plains, where Christchurch (gray patch to the north) is located. The Banks Peninsula is formed from the overlapping cones of the extinct Lyttelton and Akaroa volcanoes. Subsequent erosion of the cones formed the heavily dissected terrain visible in the image, and sea level rise led to the creation of several harbors around the Peninsula. Erosion continues unabated today, as evidenced

Christchurch and the Peninsula of Banks (New Zealand) from space - Christchurch and Banks Peninsula, New Zealand - The Peninsula of Banks and the City of Christchurch seen from the International Space Station (ISS) on August 15, 2006. The Banks Peninsula is an ancient erode volcano forming a peninsula on the east coast of the South Island. Oblique view (the photograph was taken from a side angle) of the city of Christchurch, New Zealand. Snow highlights the peaks of the Banks Peninsula to the southeast of the city. The peninsula has a radically different landscape compared to the adjoining, flat Canterbury Plains, where Christchurch (gray patch to the north) is located. The Banks Peninsula is formed from the overlapping cones of the extinct Lyttelton and Akaroa volcanoes. Subsequent erosion of the cones formed the heavily dissected terrain visible in the image, and sea level rise led to the creation of several harbors around the Peninsula. Erosion continues unabated today, as evidenced

PIX4675641

Neptune - Voyager 2 - Image of Neptune obtained by the Voyager 2 probe on August 14, 1989 at 14.8 million km from the planet. Neptune has an equatorial diameter of about 49,000 kilometres. Its blue color is due to the abundance of methane in its atmosphere. On this photo, on the right, the Great Dark Spot, which is the size of the Earth where winds are blowing at 300 m/s. This spot has now disappeared but other dark spots have been detected since then. This contrast enhanced color photograph of Neptune was produced from images taken through the orange, green, and violet filters of the narrow angle camera. As Voyager 2 approaches Neptune, rapidly increasing image resolution is revealing striking new details in the planet's atmosphere, and this picture shows features as small as a few hundred kilometers in extent. Bright, wispy “” cirrus - type”” clouds are seen overlying the Great Dark Spot (GDS) at its southern (lower) margin and over its northwest (upper left) boundary. This is the fi

Neptune - Voyager 2 - Image of Neptune obtained by the Voyager 2 probe on August 14, 1989 at 14.8 million km from the planet. Neptune has an equatorial diameter of about 49,000 kilometres. Its blue color is due to the abundance of methane in its atmosphere. On this photo, on the right, the Great Dark Spot, which is the size of the Earth where winds are blowing at 300 m/s. This spot has now disappeared but other dark spots have been detected since then. This contrast enhanced color photograph of Neptune was produced from images taken through the orange, green, and violet filters of the narrow angle camera. As Voyager 2 approaches Neptune, rapidly increasing image resolution is revealing striking new details in the planet's atmosphere, and this picture shows features as small as a few hundred kilometers in extent. Bright, wispy “” cirrus - type”” clouds are seen overlying the Great Dark Spot (GDS) at its southern (lower) margin and over its northwest (upper left) boundary. This is the fi

PIX4622776

Galaxy Centaurus A (NGC 5128) x-ray view - radio - visible - Galaxy Centaurus A in different wavelengths - false-coloured view of the 30,000-year long jet - light escaping from the nucleus of the Centaurus A galaxy where a massive black hole is suspected. On this composite image obtained in X, radio, and visible, two large X-emission arcs surround this jet over a diameter of 25,000 years - light. These hot arcs could be the result of a gigantic explosion that occurred 10 million years ago in the nucleus of the galaxy. The galaxy NGC 5128 is located about 13 million light years away from Earth. A composite X - ray (blue), radio (pink and green), and optical (orange and yellow) image of the galaxy Centaurus A presents a stunning view of a galaxy in turmoil. A broad band of dust and cold gas is bisected at an angle by opposing jets of high - energy particles blasting away from the supermassive black hole in the nucleus. Two large arcs of X - ray emitting hot gas were discovered in the out

Galaxy Centaurus A (NGC 5128) x-ray view - radio - visible - Galaxy Centaurus A in different wavelengths - false-coloured view of the 30,000-year long jet - light escaping from the nucleus of the Centaurus A galaxy where a massive black hole is suspected. On this composite image obtained in X, radio, and visible, two large X-emission arcs surround this jet over a diameter of 25,000 years - light. These hot arcs could be the result of a gigantic explosion that occurred 10 million years ago in the nucleus of the galaxy. The galaxy NGC 5128 is located about 13 million light years away from Earth. A composite X - ray (blue), radio (pink and green), and optical (orange and yellow) image of the galaxy Centaurus A presents a stunning view of a galaxy in turmoil. A broad band of dust and cold gas is bisected at an angle by opposing jets of high - energy particles blasting away from the supermassive black hole in the nucleus. Two large arcs of X - ray emitting hot gas were discovered in the out

PIX4612202

Saturn en jour seen by Cassini - Backlit Saturn seen by Cassini - Image obtained by the Cassini probe on October 17, 2012 at a distance of 800,000 km from the planet. At the bottom left of the image, the two brilliant dots are the Enceladus and Tethys satellites. Nasa's Cassini spacecraft has delivered a glorious view of Saturn, taken while the spacecraft was in Saturn's shadow. The cameras were turned toward Saturn and the sun so that the planet and rings are backlit. (The sun is behind the planet, which is shielding the cameras from direct sunlight.) In addition to the visual splendor, this special, very - high - phase viewing geometry lets scientists study ring and atmosphere phenomena not easily seen at a lower phase. Also captured in this image are two of Saturn's moons: Enceladus and Tethys. Both appear on the left side of the planet, below the rings. Enceladus is closer to the rings; Tethys is below and to the left. This view looks toward the non - illuminated side of the rings

Saturn en jour seen by Cassini - Backlit Saturn seen by Cassini - Image obtained by the Cassini probe on October 17, 2012 at a distance of 800,000 km from the planet. At the bottom left of the image, the two brilliant dots are the Enceladus and Tethys satellites. Nasa's Cassini spacecraft has delivered a glorious view of Saturn, taken while the spacecraft was in Saturn's shadow. The cameras were turned toward Saturn and the sun so that the planet and rings are backlit. (The sun is behind the planet, which is shielding the cameras from direct sunlight.) In addition to the visual splendor, this special, very - high - phase viewing geometry lets scientists study ring and atmosphere phenomena not easily seen at a lower phase. Also captured in this image are two of Saturn's moons: Enceladus and Tethys. Both appear on the left side of the planet, below the rings. Enceladus is closer to the rings; Tethys is below and to the left. This view looks toward the non - illuminated side of the rings

PIX4625007

Interieur du Trump Tower

Interieur du Trump Tower

IMO2708822

Saturn rings seen by Cassini - Saturn's rings from Cassini - Image obtained by the Cassini probe on January 21, 2007 at a distance of 1.6 million km from the planet. This view in natural colors shows Saturn's ring system. The planet, overexposed on this image, has been deliberately erased from the image but its shadow decouts the rings on the right. Some satellites are visible: Epimethee (at 1 hour), Pandora (at 5 o'clock) and Janus (at 10 o'clock). Mosaic of 27 images. The ring system is composed from closest to Saturn to outermost by ring D, then C, B, the division of Cassini, A with division of Encke, F, G and E. The Cassini spacecraft, flying high above Saturn, captured this view of an alien copper - colored ring world. The overexposed planet has deliberately been removed to show the unlit rings alone, seen from an elevation of 60 degrees. The view is a mosaic of 27 images - - nine separate sets of red, green and blue images - - taken over the course of about 45 minutes, as Cassini

Saturn rings seen by Cassini - Saturn's rings from Cassini - Image obtained by the Cassini probe on January 21, 2007 at a distance of 1.6 million km from the planet. This view in natural colors shows Saturn's ring system. The planet, overexposed on this image, has been deliberately erased from the image but its shadow decouts the rings on the right. Some satellites are visible: Epimethee (at 1 hour), Pandora (at 5 o'clock) and Janus (at 10 o'clock). Mosaic of 27 images. The ring system is composed from closest to Saturn to outermost by ring D, then C, B, the division of Cassini, A with division of Encke, F, G and E. The Cassini spacecraft, flying high above Saturn, captured this view of an alien copper - colored ring world. The overexposed planet has deliberately been removed to show the unlit rings alone, seen from an elevation of 60 degrees. The view is a mosaic of 27 images - - nine separate sets of red, green and blue images - - taken over the course of about 45 minutes, as Cassini

PIX4625026

Vernede Collection 3: Military Parade, Girl Guiders inspection and Society wedding

Vernede Collection 3: Military Parade, Girl Guiders inspection and Society wedding

BAF7424512

March - Opportunity - Panorama - 05/2007 - March: D - Star Panorama by Opportunity (False Color) - Panorama in fake colors obtained by the rover Opportunity on 1st May 2007. The Rover Opportunity landed on Mars in the Meridiani Planum region on January 25, 2004. Opportunity reached the Victoria crater (in the background, at the top of the picture) on September 27, 2006 after having travelled more than 9 km on the surface of Mars. On April 29, 2007, the rover tested a new navigation software to optimize its driving. The traces left on Martian soil are visible to the left of the image. The rocks towards the center of the image are 7 to 10 cm high. This view from Opportunity shows the tracks left by a drive executed with more onboard autonomy than has been used on any other drive by a Mars rover. Opportunity made the curving, 15.8 - meter (52 - foot) drive during its 1,160th Martian day, or sol (April 29, 2007). It was testing a navigational capability called “Field D - star,””” which ena

March - Opportunity - Panorama - 05/2007 - March: D - Star Panorama by Opportunity (False Color) - Panorama in fake colors obtained by the rover Opportunity on 1st May 2007. The Rover Opportunity landed on Mars in the Meridiani Planum region on January 25, 2004. Opportunity reached the Victoria crater (in the background, at the top of the picture) on September 27, 2006 after having travelled more than 9 km on the surface of Mars. On April 29, 2007, the rover tested a new navigation software to optimize its driving. The traces left on Martian soil are visible to the left of the image. The rocks towards the center of the image are 7 to 10 cm high. This view from Opportunity shows the tracks left by a drive executed with more onboard autonomy than has been used on any other drive by a Mars rover. Opportunity made the curving, 15.8 - meter (52 - foot) drive during its 1,160th Martian day, or sol (April 29, 2007). It was testing a navigational capability called “Field D - star,””” which ena

PIX4615862

March - Opportunity - Panorama - 05/2007 - March: D - Star Panorama by Opportunity (False Color) - Panorama in fake colors obtained by the rover Opportunity on 1st May 2007. The Rover Opportunity landed on Mars in the Meridiani Planum region on January 25, 2004. Opportunity reached the Victoria crater (in the background, at the top of the picture) on September 27, 2006 after having travelled more than 9 km on the surface of Mars. On April 29, 2007, the rover tested a new navigation software to optimize its driving. The traces left on Martian soil are visible to the left of the image. The rocks towards the center of the image are 7 to 10 cm high. This view from Opportunity shows the tracks left by a drive executed with more onboard autonomy than has been used on any other drive by a Mars rover. Opportunity made the curving, 15.8 - meter (52 - foot) drive during its 1,160th Martian day, or sol (April 29, 2007). It was testing a navigational capability called “Field D - star,””” which ena

March - Opportunity - Panorama - 05/2007 - March: D - Star Panorama by Opportunity (False Color) - Panorama in fake colors obtained by the rover Opportunity on 1st May 2007. The Rover Opportunity landed on Mars in the Meridiani Planum region on January 25, 2004. Opportunity reached the Victoria crater (in the background, at the top of the picture) on September 27, 2006 after having travelled more than 9 km on the surface of Mars. On April 29, 2007, the rover tested a new navigation software to optimize its driving. The traces left on Martian soil are visible to the left of the image. The rocks towards the center of the image are 7 to 10 cm high. This view from Opportunity shows the tracks left by a drive executed with more onboard autonomy than has been used on any other drive by a Mars rover. Opportunity made the curving, 15.8 - meter (52 - foot) drive during its 1,160th Martian day, or sol (April 29, 2007). It was testing a navigational capability called “Field D - star,””” which ena

PIX4615851

«
1
…
114
115
116
»

Warum Bridgeman Images?

Kunst. Kultur. Geschichte.

Wir arbeiten mit den weltweit führenden Museen, Galerien und Künstlern zusammen, so dass Sie Zugang zu qualitativ hochwertigem Bildmaterial haben.

Entdecken Sie unsere Kollektion FAQs durchsuchen

Einfach. Schnell. Zuverlässig.

Unsere Teams helfen Ihnen bei der Suche nach den perfekten Inhalten und kümmern sich um alle urheberrechtlichen und lizenzrechtlichen Anforderungen.

Kontaktieren Sie uns

Entdecken Sie Millionen von Bildern und Clips für Ihre kreativen Projekte.

Starten Sie Ihre Suche

© Copyright 2024 Bridgeman Art Library Limited. Registriert in England und Wales unter der Firmennummer 01056394.