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Bilder zu 'Scala' gefunden, 20,468

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Sonde Jupiter Icy Moon Explorer (JUICE) (2023-2030) (illustration)

Sonde Jupiter Icy Moon Explorer (JUICE) (2023-2030) (illustration)

D. Ducros

PIX8702153

Nebula N44 in the Large Magellan Cloud - Superbubble LHA 120 - N 44 in the Large Magellanic Cloud - This image obtained by the Very Large Telescope (VLT) shows the nebula N44 surrounding the cluster of stars NGC 1929. It is a star-forming region located in the galaxy of the Great Magellan Cloud, about 170,000 light years from Earth. Eso's Very Large Telescope captured this striking view of the nebula around the star cluster NGC 1929 within the Large Magellanic Cloud, a satellite galaxy of our own Milky Way. A colossal example of what astronomers call a superbubble dominates this stellar nursery. It is being carved by the winds from bright young stars and the shockwaves from supernova explosions. This nebula is officially known as LHA 120 - N 44, or just N 44 for short. Hot young stars in NGC 1929 are emitting intense ultraviolet light and causing the gas to glow. This effect highlights the aptly - named superbubble, a vast shell of material around 325 by 250 light - years across. For c

Nebula N44 in the Large Magellan Cloud - Superbubble LHA 120 - N 44 in the Large Magellanic Cloud - This image obtained by the Very Large Telescope (VLT) shows the nebula N44 surrounding the cluster of stars NGC 1929. It is a star-forming region located in the galaxy of the Great Magellan Cloud, about 170,000 light years from Earth. Eso's Very Large Telescope captured this striking view of the nebula around the star cluster NGC 1929 within the Large Magellanic Cloud, a satellite galaxy of our own Milky Way. A colossal example of what astronomers call a superbubble dominates this stellar nursery. It is being carved by the winds from bright young stars and the shockwaves from supernova explosions. This nebula is officially known as LHA 120 - N 44, or just N 44 for short. Hot young stars in NGC 1929 are emitting intense ultraviolet light and causing the gas to glow. This effect highlights the aptly - named superbubble, a vast shell of material around 325 by 250 light - years across. For c

PIX4620802

Caister Castle, Norfolk

Caister Castle, Norfolk

Beaumont, George Howland (1753-1827)

USB1159949

Enceladus, Saturn's satellite, seen by Cassini - Saturn's moon Enceladus from Cassini - Mosaic of false-coloured images obtained by the Cassini probe during the flight over this satellite on 11 August 2008. The image shows a fractured region in the southern hemisphere of the satellite. This mosaic of Saturn's moon Enceladus provides broad regional context for the ultra - sharp, close - up views Nasa's Cassini spacecraft acquired minutes earlier, during its flyby on Aug. 11, 2008. This false - color mosaic combines Imaging Science Subsystem (ISS) narrow - angle camera images obtained through ultraviolet, green, and near - infrared camera filters. Areas that are greenish in appearance are believed to represent deposits of coarser grained ice and solid boulders that are too small to be seen at this scale, but which are visible in the higher resolution views, while whitish deposits represent finer grained ice. The mosaic shows that coarse - grained and solid ice are concentrated along vall

Enceladus, Saturn's satellite, seen by Cassini - Saturn's moon Enceladus from Cassini - Mosaic of false-coloured images obtained by the Cassini probe during the flight over this satellite on 11 August 2008. The image shows a fractured region in the southern hemisphere of the satellite. This mosaic of Saturn's moon Enceladus provides broad regional context for the ultra - sharp, close - up views Nasa's Cassini spacecraft acquired minutes earlier, during its flyby on Aug. 11, 2008. This false - color mosaic combines Imaging Science Subsystem (ISS) narrow - angle camera images obtained through ultraviolet, green, and near - infrared camera filters. Areas that are greenish in appearance are believed to represent deposits of coarser grained ice and solid boulders that are too small to be seen at this scale, but which are visible in the higher resolution views, while whitish deposits represent finer grained ice. The mosaic shows that coarse - grained and solid ice are concentrated along vall

PIX4625460

The yard at the rear of no. 4 St Barnabas' Square, Douglas, Isle of Man, 1932-34 (b/w photo)

The yard at the rear of no. 4 St Barnabas' Square, Douglas, Isle of Man, 1932-34 (b/w photo)

Frowde, John James (1868-1946)

MNX5052662

Europe - Jupiter Satellite - View of the surface of the Europe satellite obtained from images made by the Galileo probe in 1995 and 1998. Jupiter's icy moon Europa looms large in this newly - reprocessed color view, made from images taken by Nasa's Galileo spacecraft in the late 1990s. This is the color view of Europa from Galileo that shows the largest portion of the moon's surface at the highest resolution. To create this new version, the images were assembled into a realistic color view of the surface that approximates how Europa would appear to the human eye. The scene shows the stunning diversity of Europa's surface geology. Long, linear cracks and ridges crisscross the surface, interrupted by regions of disrupted terrain where the surface ice crust has been broken up and re - frozen into new patterns. Color variations across the surface are associated with differences in geologic feature type and location. For example, areas that appear blue or white contain relatively pure water

Europe - Jupiter Satellite - View of the surface of the Europe satellite obtained from images made by the Galileo probe in 1995 and 1998. Jupiter's icy moon Europa looms large in this newly - reprocessed color view, made from images taken by Nasa's Galileo spacecraft in the late 1990s. This is the color view of Europa from Galileo that shows the largest portion of the moon's surface at the highest resolution. To create this new version, the images were assembled into a realistic color view of the surface that approximates how Europa would appear to the human eye. The scene shows the stunning diversity of Europa's surface geology. Long, linear cracks and ridges crisscross the surface, interrupted by regions of disrupted terrain where the surface ice crust has been broken up and re - frozen into new patterns. Color variations across the surface are associated with differences in geologic feature type and location. For example, areas that appear blue or white contain relatively pure water

PIX4574821

Self-Portrait, c.1590 (w/c on vellum laid on card)

Self-Portrait, c.1590 (w/c on vellum laid on card)

Oliver, Isaac (c.1565-1617)

ROC5672284

Rice Terraces, Tirta Gangga, Bali, Indonesia (photo)

Rice Terraces, Tirta Gangga, Bali, Indonesia (photo)

Sergi Reboredo

SRB1202714

A three-masted ship under sail, c.1470 (engraving)

A three-masted ship under sail, c.1470 (engraving)

Venetian School, (15th century)

MMM7341689

Passenger liner SS 'Normandie' (1932), c.1932 (wood, brass;silver, steel, paint;varnish)

Passenger liner SS 'Normandie' (1932), c.1932 (wood, brass;silver, steel, paint;varnish)

Montera, J. (fl.c.1932)

MMM7339843

Southern constellations around the Clock - Southern constellations around Horologium - Southern constellations around the Clock. The two bright stars are Canopus (bottom) and Achernar. This wide angle image includes Horologium, Phoenix and Pictor, insignificant constellations roughly centred on an arc of delination 50* south, but at a scale too small to show the star identifications and stick figures. Horologium, the Pendulum Clock (originally l'Horloge and then Horologium Oscillitorium), was a constellation introduced by Abbe Nicolas Louis de Lacaille during his stay at the Cape of Good Hope between 1751 and 1752. It was named to honor Christian Huygens as the inventor of this type of clock, but the idea for such a method of regulating time came from Galileo. Lacaille's constellation drawing shows a remarkably detailed dial, weights and a pendulum that has little apparent connection with the scattering of faint stars in this part of the sky. There are no named stars and little else in

Southern constellations around the Clock - Southern constellations around Horologium - Southern constellations around the Clock. The two bright stars are Canopus (bottom) and Achernar. This wide angle image includes Horologium, Phoenix and Pictor, insignificant constellations roughly centred on an arc of delination 50* south, but at a scale too small to show the star identifications and stick figures. Horologium, the Pendulum Clock (originally l'Horloge and then Horologium Oscillitorium), was a constellation introduced by Abbe Nicolas Louis de Lacaille during his stay at the Cape of Good Hope between 1751 and 1752. It was named to honor Christian Huygens as the inventor of this type of clock, but the idea for such a method of regulating time came from Galileo. Lacaille's constellation drawing shows a remarkably detailed dial, weights and a pendulum that has little apparent connection with the scattering of faint stars in this part of the sky. There are no named stars and little else in

PIX4594625

Heart of the Nebula of the Lagoon (M8) in Sagittarius seen by HST - This NASA Hubble Space Telescope (HST) image reveals a pair of one - half light - year long interstellar “” twisters”” - - eerie funnels and twisted - rope structures (upper left) - - in the heart of the Lagoon Nebula (Messier 8) which lies 5,000 years - - away in the direction of the constellation Sagittarius. The central hot O type star, Herschel 36 (upper left in photo), is the primary source of the ionizing radiation for the brightest region in the nebula, called the Hourglass. Other hot stars, also present in the nebula, are ionizing the extended optical nebulosity. The ionizing radiation induces photo - evaporation of the surfaces of the clouds (seen as a blue “” mist”” at the right of the image), and drives away violent stellar winds tearing into the cool clouds.Analogous to the spectacular phenomena of Earth tornadoes, the large difference in temperature between the hot surface and cold interior of the clouds,

Heart of the Nebula of the Lagoon (M8) in Sagittarius seen by HST - This NASA Hubble Space Telescope (HST) image reveals a pair of one - half light - year long interstellar “” twisters”” - - eerie funnels and twisted - rope structures (upper left) - - in the heart of the Lagoon Nebula (Messier 8) which lies 5,000 years - - away in the direction of the constellation Sagittarius. The central hot O type star, Herschel 36 (upper left in photo), is the primary source of the ionizing radiation for the brightest region in the nebula, called the Hourglass. Other hot stars, also present in the nebula, are ionizing the extended optical nebulosity. The ionizing radiation induces photo - evaporation of the surfaces of the clouds (seen as a blue “” mist”” at the right of the image), and drives away violent stellar winds tearing into the cool clouds.Analogous to the spectacular phenomena of Earth tornadoes, the large difference in temperature between the hot surface and cold interior of the clouds,

PIX4619680

Star Formation in the DR21 Region - Star Formation in the DR21 Region - This star-forming region is about 6200 years old - light. Hidden in light visible by interstellar dust, this region rises in infrared light. Gas filaments appear in red; they emphasize the presence of aromatic polycyclic hydrocarbons (PAH); they are organic molecules composed of carbon atoms and hydrogen that could be the germs on which the first bricks of life appeared. Image obtained by the Spitzer space telescope in 2003. Hidden behind a shroud of dust in the constellation Cygnus is a stellar nursery called DR21, which is giving birth to some of the most massive stars in our galaxy. Visible light images reveal no trace of this interstellar cauldron because of heavy dust obscuration. This image from Nasa's Spitzer Space Telescope allow us to peek behind the cosmic veil and pinpoint one of the most massive natal stars yet seen in our Milky Way galaxy. The never - before - seen star is 100,000 times as bright as th

Star Formation in the DR21 Region - Star Formation in the DR21 Region - This star-forming region is about 6200 years old - light. Hidden in light visible by interstellar dust, this region rises in infrared light. Gas filaments appear in red; they emphasize the presence of aromatic polycyclic hydrocarbons (PAH); they are organic molecules composed of carbon atoms and hydrogen that could be the germs on which the first bricks of life appeared. Image obtained by the Spitzer space telescope in 2003. Hidden behind a shroud of dust in the constellation Cygnus is a stellar nursery called DR21, which is giving birth to some of the most massive stars in our galaxy. Visible light images reveal no trace of this interstellar cauldron because of heavy dust obscuration. This image from Nasa's Spitzer Space Telescope allow us to peek behind the cosmic veil and pinpoint one of the most massive natal stars yet seen in our Milky Way galaxy. The never - before - seen star is 100,000 times as bright as th

PIX4621130

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

Diana, 1892-94 (copper sheets)

Diana, 1892-94 (copper sheets)

Saint-Gaudens, Augustus (1848-1907)

PHL434261

Star Formation in the DR21 Region - Star Formation in the DR21 Region - This star formation region is about 6200 years old - light. Hidden in light visible by interstellar dust, this region rises in infrared light. Gas filaments appear in red; they emphasize the presence of aromatic polycyclic hydrocarbons (PAH); they are organic molecules composed of carbon atoms and hydrogen that could be the germs on which the first bricks of life appeared. Composite image in different wavelengths obtained by the Spitzer space telescope; in blue the visible light, in yellow and red the infrared light. Hidden behind a shroud of dust in the constellation Cygnus is a stellar nursery called DR21, which is giving birth to some of the most massive stars in our galaxy. Visible light images reveal no trace of this interstellar cauldron because of heavy dust obscuration. This image from Nasa's Spitzer Space Telescope allow us to peek behind the cosmic veil and pinpoint one of the most massive natal stars yet

Star Formation in the DR21 Region - Star Formation in the DR21 Region - This star formation region is about 6200 years old - light. Hidden in light visible by interstellar dust, this region rises in infrared light. Gas filaments appear in red; they emphasize the presence of aromatic polycyclic hydrocarbons (PAH); they are organic molecules composed of carbon atoms and hydrogen that could be the germs on which the first bricks of life appeared. Composite image in different wavelengths obtained by the Spitzer space telescope; in blue the visible light, in yellow and red the infrared light. Hidden behind a shroud of dust in the constellation Cygnus is a stellar nursery called DR21, which is giving birth to some of the most massive stars in our galaxy. Visible light images reveal no trace of this interstellar cauldron because of heavy dust obscuration. This image from Nasa's Spitzer Space Telescope allow us to peek behind the cosmic veil and pinpoint one of the most massive natal stars yet

PIX4621115

Passenger liner SS 'Normandie' (1932), c.1932 (wood, organic, metal: brass, metal: silver, metal: steel, inorganic, paint, coating: varnish)

Passenger liner SS 'Normandie' (1932), c.1932 (wood, organic, metal: brass, metal: silver, metal: steel, inorganic, paint, coating: varnish)

Montera, J. (fl.c.1932)

MMM7339845

Richat structure - Mauritania - satellite view - Richat structure, Mauritania, seen by satellite - Richat structure is a geological formation of volcanic origin in Mauritania. This “eye” measures 50 km in diameter. This image is a combination of an image obtained by the Landsat satellite in 1987 and a radar image obtained from the Space Shuttle (SRTM) in 2000. The relief is exaggerated by about 6 times. The picture covers an area of 68 km by 112 km. This prominent circular feature, known as the Richat Structure, in the Sahara desert of Mauritania is often noted by astronauts because it forms a conspicuous 50 - kilometer - wide (30 - mile - wide) bull's - eye on the otherwise rather featureless expanse of the desert. Initially mistaken for a possible impact crater, it is now known to be an eroded circular anticline (structural dome) of layered sedimentary rocks. Extensive sand dunes occur in this region and the interaction of bedrock topography, wind, and moving sand is evident in this

Richat structure - Mauritania - satellite view - Richat structure, Mauritania, seen by satellite - Richat structure is a geological formation of volcanic origin in Mauritania. This “eye” measures 50 km in diameter. This image is a combination of an image obtained by the Landsat satellite in 1987 and a radar image obtained from the Space Shuttle (SRTM) in 2000. The relief is exaggerated by about 6 times. The picture covers an area of 68 km by 112 km. This prominent circular feature, known as the Richat Structure, in the Sahara desert of Mauritania is often noted by astronauts because it forms a conspicuous 50 - kilometer - wide (30 - mile - wide) bull's - eye on the otherwise rather featureless expanse of the desert. Initially mistaken for a possible impact crater, it is now known to be an eroded circular anticline (structural dome) of layered sedimentary rocks. Extensive sand dunes occur in this region and the interaction of bedrock topography, wind, and moving sand is evident in this

PIX4659064

Waterline model; Miniature model (sculpture)

Waterline model; Miniature model (sculpture)

Carpenter, Reginald (20th century)

MMM7340611

Hôtel de Balzac. Entrance and façade on rue Fortunée, now rue Balzac, 1880 (painting)

Hôtel de Balzac. Entrance and façade on rue Fortunée, now rue Balzac, 1880 (painting)

Dargaud, Paul Joseph Victor (fl.1873-1920)

XOS8984314

An Angling Party

An Angling Party

Smith, Edward (fl.1773)

USB1159715

Large pair of library globes, the terrestrial 1645/48, the celestial after c.1630 (plaster, wood & engraved paper)

Large pair of library globes, the terrestrial 1645/48, the celestial after c.1630 (plaster, wood & engraved paper)

Blaeu, Willem (1571-1638)

CH3482878

Large pair of library globes, the terrestrial 1645/48, the celestial after c.1630 (plaster, wood & engraved paper)

Large pair of library globes, the terrestrial 1645/48, the celestial after c.1630 (plaster, wood & engraved paper)

Blaeu, Willem (1571-1638)

CH3482880

Large pair of library globes, the terrestrial 1645/48, the celestial after c.1630 (plaster, wood & engraved paper)

Large pair of library globes, the terrestrial 1645/48, the celestial after c.1630 (plaster, wood & engraved paper)

Blaeu, Willem (1571-1638)

CH3482890

Large pair of library globes, the terrestrial 1645/48, the celestial after c.1630 (plaster, wood & engraved paper)

Large pair of library globes, the terrestrial 1645/48, the celestial after c.1630 (plaster, wood & engraved paper)

Blaeu, Willem (1571-1638)

CH3482891

Large pair of library globes, the terrestrial 1645/48, the celestial after c.1630 (plaster, wood & engraved paper)

Large pair of library globes, the terrestrial 1645/48, the celestial after c.1630 (plaster, wood & engraved paper)

Blaeu, Willem (1571-1638)

CH3482892

Large pair of library globes, the terrestrial 1645/48, the celestial after c.1630 (plaster, wood & engraved paper)

Large pair of library globes, the terrestrial 1645/48, the celestial after c.1630 (plaster, wood & engraved paper)

Blaeu, Willem (1571-1638)

CH3482885

Airy's transit circle telescope, 1850 (photo)

Airy's transit circle telescope, 1850 (photo)

British School, (19th century)

MMM7340621

Large pair of library globes, the terrestrial 1645/48, the celestial after c.1630 (plaster, wood & engraved paper)

Large pair of library globes, the terrestrial 1645/48, the celestial after c.1630 (plaster, wood & engraved paper)

Blaeu, Willem (1571-1638)

CH3482882

Large pair of library globes, the terrestrial 1645/48, the celestial after c.1630 (plaster, wood & engraved paper)

Large pair of library globes, the terrestrial 1645/48, the celestial after c.1630 (plaster, wood & engraved paper)

Blaeu, Willem (1571-1638)

CH3482886

Large pair of library globes, the terrestrial 1645/48, the celestial after c.1630 (plaster, wood & engraved paper)

Large pair of library globes, the terrestrial 1645/48, the celestial after c.1630 (plaster, wood & engraved paper)

Blaeu, Willem (1571-1638)

CH3482887

Large pair of library globes, the terrestrial 1645/48, the celestial after c.1630 (plaster, wood & engraved paper)

Large pair of library globes, the terrestrial 1645/48, the celestial after c.1630 (plaster, wood & engraved paper)

Blaeu, Willem (1571-1638)

CH3482889

Coast Of Vietnam 1966

Coast Of Vietnam 1966

BOF6283753

President Bill Clinton - Affirmative Action Speech, 1995

President Bill Clinton - Affirmative Action Speech, 1995

BOF6286734

Our Indian Contingent at Malta (engraving)

Our Indian Contingent at Malta (engraving)

Dollman, John Charles (1851-1934) (after)

LIP1059758

Tatton Park, Knutsford, Cheshire, the Seat of Lord Egerton of Tatton (engraving)

Tatton Park, Knutsford, Cheshire, the Seat of Lord Egerton of Tatton (engraving)

Brewer, Henry Charles (1866-1950)

LIP1050499

Royal Family of Sweden

Royal Family of Sweden

Unknown photographer, (20th century)

XRE2034729

The Battle of Culloden was the last full-scale combat fought on British soil

The Battle of Culloden was the last full-scale combat fought on British soil

Nicolle, Pat (Patrick) (1907-95)

LAL295763

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