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'Nucleus' Bilder und Clips Suchergebnisse page 181 of 7

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Bilder zu 'Nucleus' gefunden, 559

 
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Controlling Atomic Energy 6, 1950s

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Controlling Atomic Energy 6, 1950s

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Controlling Atomic Energy 12, 1950s

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Controlling Atomic Energy 12, 1950s

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Controlling Atomic Energy 14, 1950s

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Controlling Atomic Energy 14, 1950s

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Controlling Atomic Energy 17, 1950s

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Controlling Atomic Energy 17, 1950s

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Controlling Atomic Energy 21, 1950s

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Controlling Atomic Energy 21, 1950s

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United States, 1960s: animation of molecules entering muscle cell

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United States, 1960s: animation of molecules entering muscle cell

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Sun cutaway - Sun cutaway - At the bottom left, the Earth is represented. Bottom left is the Earth

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Sun cutaway - Sun cutaway - At the bottom left, the Earth is represented. Bottom left is the Earth

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M87 elliptical galaxy in Virgo - M87 elliptical galaxy in Virgo - The M87 galaxy (NGC 4486) is 54 million years ago - light from Earth, in the heart of the Virgin's cluster. This image is a composite obtained in X-rays, radio and visible. Gas material is ejected from the heart of the galaxy. A supermassive black hole would have caused this jet. This image is a composite of visible (or optical), radio, and X - ray data of the giant elliptical galaxy, M87. M87 lies at a distance of 54 million light years and is the largest galaxy in the Virgo cluster of galaxies. Bright jets moving at close to the speed of light are seen at all wavelengths coming from the massive black hole at the center of the galaxy. It has also been identified with the strong radio source, Virgo A, and is a powerful source of X - rays as it resides near the center of a hot, X - ray emitting cloud that extends over much of the Virgo cluster. The extended radio emission consists of plumes of fast - moving gas from the j

PIX4611440

M87 elliptical galaxy in Virgo - M87 elliptical galaxy in Virgo - The M87 galaxy (NGC 4486) is 54 million years ago - light from Earth, in the heart of the Virgin's cluster. This image is a composite obtained in X-rays, radio and visible. Gas material is ejected from the heart of the galaxy. A supermassive black hole would have caused this jet. This image is a composite of visible (or optical), radio, and X - ray data of the giant elliptical galaxy, M87. M87 lies at a distance of 54 million light years and is the largest galaxy in the Virgo cluster of galaxies. Bright jets moving at close to the speed of light are seen at all wavelengths coming from the massive black hole at the center of the galaxy. It has also been identified with the strong radio source, Virgo A, and is a powerful source of X - rays as it resides near the center of a hot, X - ray emitting cloud that extends over much of the Virgo cluster. The extended radio emission consists of plumes of fast - moving gas from the j

PIX4611440

 
Centaurus A elliptical galaxy (NGC 5128) in the Centaurus - Galaxy Centaurus A (NGC 5128) - The galaxy NGC 5128 is located about 13 million years away from Earth. This Giant Galaxy is a powerful radio source known as Centaurus A. It is an active galaxy whose energy comes from a supermassive black hole. This image obtained by the Kueyen telescope of the VLT in Chile on 1 February 2000 shows the star flames that occur in the dark band of the galaxy. Centaurus A is one of the foremost examples of a radio - loud active galactic nucleus (AGN). On images obtained at optical wavelengths, thick dust layers almost completely obscure the galaxy's centre. Until 1949, NGC 5128 was thought to be a strange object in the Milky Way, but it was then identified as a powerful radio galaxy and designated Centaurus A. The distance is about 10 - 13 million light - years (3 - 4 Mpc) and the apparent visual magnitude is about 8, or 5 times too faint to be seen with the unaided eye. There is strong evidence th

PIX4612179

Centaurus A elliptical galaxy (NGC 5128) in the Centaurus - Galaxy Centaurus A (NGC 5128) - The galaxy NGC 5128 is located about 13 million years away from Earth. This Giant Galaxy is a powerful radio source known as Centaurus A. It is an active galaxy whose energy comes from a supermassive black hole. This image obtained by the Kueyen telescope of the VLT in Chile on 1 February 2000 shows the star flames that occur in the dark band of the galaxy. Centaurus A is one of the foremost examples of a radio - loud active galactic nucleus (AGN). On images obtained at optical wavelengths, thick dust layers almost completely obscure the galaxy's centre. Until 1949, NGC 5128 was thought to be a strange object in the Milky Way, but it was then identified as a powerful radio galaxy and designated Centaurus A. The distance is about 10 - 13 million light - years (3 - 4 Mpc) and the apparent visual magnitude is about 8, or 5 times too faint to be seen with the unaided eye. There is strong evidence th

PIX4612179

 
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Sun cutaway - Sun cutaway - At the bottom left, the Earth is represented. Bottom left is the Earth

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Sun cutaway - Sun cutaway - At the bottom left, the Earth is represented. Bottom left is the Earth

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Spiral galaxy M81 in the Great Bear - Spiral galaxy M81 in Ursa Major: The spiral galaxy M81 is located 12 million light years from Earth. Its arms are home to star-forming regions while its core is surrounded by much older yellow stars. An irregular dwarf galaxy, PGC 28757 (Holmberg IX), is visible at the top of the picture. - M81 is the brightest member of the nearby galactic group called the M81 group. This group contains at least 25 other members including the peculiar starburst galaxy M82, the peculiar galaxy NGC 3077 and many dwarfs galaxies. The core galaxies of the group (M81, M82, NGC 3077, NGC 2976) are strongly interacting and are all imbedded within a large and extended molecular gas cloud. The Dwarf irregular Holmberg IX (seen above M81 in the image) most likely condensed from tidal debri existing between M81 and M82. M81 has the distinction of being the nearest spiral galaxy to have an active galactic nucleus (AGN). AGN galaxies are luminous galaxies that demonstrate much

PIX4610399

Spiral galaxy M81 in the Great Bear - Spiral galaxy M81 in Ursa Major: The spiral galaxy M81 is located 12 million light years from Earth. Its arms are home to star-forming regions while its core is surrounded by much older yellow stars. An irregular dwarf galaxy, PGC 28757 (Holmberg IX), is visible at the top of the picture. - M81 is the brightest member of the nearby galactic group called the M81 group. This group contains at least 25 other members including the peculiar starburst galaxy M82, the peculiar galaxy NGC 3077 and many dwarfs galaxies. The core galaxies of the group (M81, M82, NGC 3077, NGC 2976) are strongly interacting and are all imbedded within a large and extended molecular gas cloud. The Dwarf irregular Holmberg IX (seen above M81 in the image) most likely condensed from tidal debri existing between M81 and M82. M81 has the distinction of being the nearest spiral galaxy to have an active galactic nucleus (AGN). AGN galaxies are luminous galaxies that demonstrate much

PIX4610399

 
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Spine and back cover of an early printed book, with the inscription 'Bessarionis-Card-Opa', 1503 (leather)

Italian School, (16th century)

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Spine and back cover of an early printed book, with the inscription 'Bessarionis-Card-Opa', 1503 (leather)

Italian School, (16th century)

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Controlling Atomic Energy 38, 1950s

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Controlling Atomic Energy 38, 1950s

AVE7296713

 
Spiral galaxy NGC 1566 in the bream - The Seyfert Galaxy NGC 1566: NGC 1566 is a spiral galaxy located about 40 million light years ago. Its core is very bright. It is an active galaxy called Seyfert, which probably houses a black hole in its heart. Image obtained with the Hubble telescope - NGC 1566 is a galaxy located approximately 40 million light-years away in the constellation of Dorado (The Dolphinfish). NGC 1566 is an intermediate spiral galaxy, meaning that while it does not have a well defined bar-shaped region of stars at its centre - like barred spirals - it is not quite an unbarred spiral either (heic9902o). The small but extremely bright nucleus of NGC 1566 is clearly visible in this image, a telltale sign of its membership of the Seyfert class of galaxies. The centres of such galaxies are very active and luminous, emitting strong bursts of radiation and potentially harbouring supermassive black holes that are many millions of times the mass of the Sun. NGC 1566 is not jus

PIX4609939

Spiral galaxy NGC 1566 in the bream - The Seyfert Galaxy NGC 1566: NGC 1566 is a spiral galaxy located about 40 million light years ago. Its core is very bright. It is an active galaxy called Seyfert, which probably houses a black hole in its heart. Image obtained with the Hubble telescope - NGC 1566 is a galaxy located approximately 40 million light-years away in the constellation of Dorado (The Dolphinfish). NGC 1566 is an intermediate spiral galaxy, meaning that while it does not have a well defined bar-shaped region of stars at its centre - like barred spirals - it is not quite an unbarred spiral either (heic9902o). The small but extremely bright nucleus of NGC 1566 is clearly visible in this image, a telltale sign of its membership of the Seyfert class of galaxies. The centres of such galaxies are very active and luminous, emitting strong bursts of radiation and potentially harbouring supermassive black holes that are many millions of times the mass of the Sun. NGC 1566 is not jus

PIX4609939

 
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Controlling Atomic Energy 8, 1950s

AVE7296683

Controlling Atomic Energy 8, 1950s

AVE7296683

 
Centaurus A Elliptical Galaxy (NGC 5128) in the Centaur - Galaxy Centaurus A - The NGC 5128 galaxy is about 11 million years away - light from Earth. This image from the Hubble Space Telescope (HST) shows the star flames that occur in the dark band of the galaxy. This giant galaxy is a powerful radio source known as Centaurus A. It is an active galaxy whose energy comes from a supermassive black hole. Centaurus A, also known as NGC 5128, is well known for its dramatic dusty lanes of dark material. Hubble's observations, using its most advanced instrument, the Wide Field Camera 3, are the most detailed ever made of this galaxy. They have been combined here in a multi - wavelength image that reveals never - before - seen detail in the dusty portion of the galaxy. As well as features in the visible spectrum, this composite shows ultraviolet light from young stars, and near - infrared light, which lets us glimpse some of the detail otherwise obscured by the dust. The dark dust lane that cr

PIX4612191

Centaurus A Elliptical Galaxy (NGC 5128) in the Centaur - Galaxy Centaurus A - The NGC 5128 galaxy is about 11 million years away - light from Earth. This image from the Hubble Space Telescope (HST) shows the star flames that occur in the dark band of the galaxy. This giant galaxy is a powerful radio source known as Centaurus A. It is an active galaxy whose energy comes from a supermassive black hole. Centaurus A, also known as NGC 5128, is well known for its dramatic dusty lanes of dark material. Hubble's observations, using its most advanced instrument, the Wide Field Camera 3, are the most detailed ever made of this galaxy. They have been combined here in a multi - wavelength image that reveals never - before - seen detail in the dusty portion of the galaxy. As well as features in the visible spectrum, this composite shows ultraviolet light from young stars, and near - infrared light, which lets us glimpse some of the detail otherwise obscured by the dust. The dark dust lane that cr

PIX4612191

 
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1950s: Animated diagram of copper atoms

AVE6329366

1950s: Animated diagram of copper atoms

AVE6329366

 
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Controlling Atomic Energy 32, 1950s

AVE7296707

Controlling Atomic Energy 32, 1950s

AVE7296707

 
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Controlling Atomic Energy 35, 1950s

AVE7296710

Controlling Atomic Energy 35, 1950s

AVE7296710

 
Centaurus A Elliptical Galaxy (NGC 5128) in the Centaur - Galaxy Centaurus A - The NGC 5128 galaxy is about 13 million years away - light from Earth. This image obtained by the Hubble Space Telescope in 1998 shows the star flames that occur in the dark band of the galaxy. In blue, these are the clusters of newly shaped young stars. At the top left, a photo of the galaxy obtained from the ground. This giant galaxy is a powerful radio source known as Centaurus A. It is an active galaxy whose energy comes from a supermassive black hole. NGC 5128 is the nearest large elliptical galaxies to our sun. It is also the nearest of the giant radio galaxies, possessing an active galactic nucleus (AGN) and optically one of the most luminous galaxies in the sky. Among many other things NGC 5128 is also the prototypical postmerger elliptical galaxy. Structural peculiarities including the prominent rotating disk of stars and gas and the complex shell structure of its halo point to a large scale merger

PIX4612157

Centaurus A Elliptical Galaxy (NGC 5128) in the Centaur - Galaxy Centaurus A - The NGC 5128 galaxy is about 13 million years away - light from Earth. This image obtained by the Hubble Space Telescope in 1998 shows the star flames that occur in the dark band of the galaxy. In blue, these are the clusters of newly shaped young stars. At the top left, a photo of the galaxy obtained from the ground. This giant galaxy is a powerful radio source known as Centaurus A. It is an active galaxy whose energy comes from a supermassive black hole. NGC 5128 is the nearest large elliptical galaxies to our sun. It is also the nearest of the giant radio galaxies, possessing an active galactic nucleus (AGN) and optically one of the most luminous galaxies in the sky. Among many other things NGC 5128 is also the prototypical postmerger elliptical galaxy. Structural peculiarities including the prominent rotating disk of stars and gas and the complex shell structure of its halo point to a large scale merger

PIX4612157

 
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Controlling Atomic Energy 7, 1950s

AVE7296682

Controlling Atomic Energy 7, 1950s

AVE7296682

 
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Controlling Atomic Energy 18, 1950s

AVE7296693

Controlling Atomic Energy 18, 1950s

AVE7296693

 
Urheberrecht
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Triangulate, 1936 (gouache on board)

Thomas, Charles (1884-1958)

SAV329303

Triangulate, 1936 (gouache on board)

Thomas, Charles (1884-1958)

SAV329303

 
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Controlling Atomic Energy 1, 1950s

AVE7296676

Controlling Atomic Energy 1, 1950s

AVE7296676

 
Interacting galaxies Markarian 533 - Interacting galaxies Markarian 533 - The galaxy NGC 7674 (Markarian 533 or Arp 182) is located about 400 million years ago - light from Earth in the constellation Pegase. It is the most important member of a group of galaxies called Hickson 96 (HCG 96). This spiral galaxy seen from the front is in interaction with other companion galaxies. It has an active core. Image obtained by the Hubble Space Telescope on June 9, 2002. NGC 7674 (seen just above the center), also known as Markarian 533, is the brightest and largest member of the so - called Hickson 96 compact group of galaxies, consisting of four galaxies. This stunning Hubble image shows a spiral galaxy nearly face - on. The central bar - shaped structure is made up of stars. The shape of NGC 7674, including the long narrow streamers seen to the left of and below the galaxy can be accounted for by tidal interactions with its companions. NGC 7674 has a powerful active nucleus of the kind known as

PIX4613210

Interacting galaxies Markarian 533 - Interacting galaxies Markarian 533 - The galaxy NGC 7674 (Markarian 533 or Arp 182) is located about 400 million years ago - light from Earth in the constellation Pegase. It is the most important member of a group of galaxies called Hickson 96 (HCG 96). This spiral galaxy seen from the front is in interaction with other companion galaxies. It has an active core. Image obtained by the Hubble Space Telescope on June 9, 2002. NGC 7674 (seen just above the center), also known as Markarian 533, is the brightest and largest member of the so - called Hickson 96 compact group of galaxies, consisting of four galaxies. This stunning Hubble image shows a spiral galaxy nearly face - on. The central bar - shaped structure is made up of stars. The shape of NGC 7674, including the long narrow streamers seen to the left of and below the galaxy can be accounted for by tidal interactions with its companions. NGC 7674 has a powerful active nucleus of the kind known as

PIX4613210

 
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Inserting nucleus into oyster during cultivation of cultured pearls, Japan

DGA1081574

Inserting nucleus into oyster during cultivation of cultured pearls, Japan

DGA1081574

 
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Controlling Atomic Energy 26, 1950s

AVE7296701

Controlling Atomic Energy 26, 1950s

AVE7296701

 
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Controlling Atomic Energy 2, 1950s

AVE7296677

Controlling Atomic Energy 2, 1950s

AVE7296677

 
Active Galaxy NGC 1068 in the Whale - Active galaxy NGC 1068 - This composite image shows that a strong stellar wind escapes from the heart of the galaxy NGC 1068 or resides a massive black hole. NGC 1068 is located about 50 million light years away from Earth. Images obtained in X-ray by the Chandra satellite (red), visible by the Hubble space telescope (green) and radio waves (blue). This is a composite image of NGC 1068, one of the nearest and brightest galaxies containing a rapidly growing supermassive black hole. X - ray data from the Chandra X - ray Observatory are shown in red, optical data from the Hubble Space Telescope in green and radio data from the Very Large Array in blue. The spiral structure of NGC 1068 is shown by the X - ray and optical data, and a jet powered by the central supermassive black hole is shown by the radio data. The X - ray images and spectra obtained using Chandra's High Energy Transmission Grating Spectrometer show that a strong wind is being driven aw

PIX4609662

Active Galaxy NGC 1068 in the Whale - Active galaxy NGC 1068 - This composite image shows that a strong stellar wind escapes from the heart of the galaxy NGC 1068 or resides a massive black hole. NGC 1068 is located about 50 million light years away from Earth. Images obtained in X-ray by the Chandra satellite (red), visible by the Hubble space telescope (green) and radio waves (blue). This is a composite image of NGC 1068, one of the nearest and brightest galaxies containing a rapidly growing supermassive black hole. X - ray data from the Chandra X - ray Observatory are shown in red, optical data from the Hubble Space Telescope in green and radio data from the Very Large Array in blue. The spiral structure of NGC 1068 is shown by the X - ray and optical data, and a jet powered by the central supermassive black hole is shown by the radio data. The X - ray images and spectra obtained using Chandra's High Energy Transmission Grating Spectrometer show that a strong wind is being driven aw

PIX4609662

 
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Controlling Atomic Energy 11, 1950s

AVE7296686

Controlling Atomic Energy 11, 1950s

AVE7296686

 
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Controlling Atomic Energy, 31

AVE7296706

Controlling Atomic Energy, 31

AVE7296706

 
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Controlling Atomic Energy 30, 1950s

AVE7296705

Controlling Atomic Energy 30, 1950s

AVE7296705

 
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Nuclear power plant Lubmin reactor in block 4 (17 hours in operation) ..., 2000 (photo)

Rolf Zöllner

IMO8823065

Nuclear power plant Lubmin reactor in block 4 (17 hours in operation) ..., 2000 (photo)

Rolf Zöllner

IMO8823065

 
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Lubmin nuclear power plant remote control via screen of the so-called manipulator ..., 2000 (photo)

Rolf Zöllner

IMO8823093

Lubmin nuclear power plant remote control via screen of the so-called manipulator ..., 2000 (photo)

Rolf Zöllner

IMO8823093

 
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Controlling Atomic Energy 22, 1950s

AVE7296697

Controlling Atomic Energy 22, 1950s

AVE7296697

 
Portrait of Ernest Rutherford (1871 - 1937), Nobel Prize in 1908

FGL5456642

Portrait of Ernest Rutherford (1871 - 1937), Nobel Prize in 1908

FGL5456642

 
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Controlling Atomic Energy 29, 1950s

AVE7296704

Controlling Atomic Energy 29, 1950s

AVE7296704

 
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Controlling Atomic Energy 37, 1950s

AVE7296712

Controlling Atomic Energy 37, 1950s

AVE7296712

 
Sir John Douglas Cockcroft, 1950

UIG3330249

Sir John Douglas Cockcroft, 1950

UIG3330249

 
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Nuclear power plant Lubmin irradiated boiler, ZLN (Zwischenlager Nord) ..., 2000 (photo)

Rolf Zöllner

IMO8823053

Nuclear power plant Lubmin irradiated boiler, ZLN (Zwischenlager Nord) ..., 2000 (photo)

Rolf Zöllner

IMO8823053

 
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Lubmin Nuclear Power Plant Block 5, former Lubmin Nuclear Power Plant, now Energiewerke ..., 2000 (photo)

Rolf Zöllner

IMO8823080

Lubmin Nuclear Power Plant Block 5, former Lubmin Nuclear Power Plant, now Energiewerke ..., 2000 (photo)

Rolf Zöllner

IMO8823080

 
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Nuclear power plant Lubmin director of the interim storage north Juergen Fischer points ..., 2000 (photo)

Rolf Zöllner

IMO8823092

Nuclear power plant Lubmin director of the interim storage north Juergen Fischer points ..., 2000 (photo)

Rolf Zöllner

IMO8823092

 
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Nuclear power plant Lubmin safety lock, leaving the reactor rooms ..., 2000 (photo)

Rolf Zöllner

IMO8823090

Nuclear power plant Lubmin safety lock, leaving the reactor rooms ..., 2000 (photo)

Rolf Zöllner

IMO8823090

 
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Nuclear power plant Lubmin two workers in protective suits in block 5, ehm ..., 2000 (photo)

Rolf Zöllner

IMO8823094

Nuclear power plant Lubmin two workers in protective suits in block 5, ehm ..., 2000 (photo)

Rolf Zöllner

IMO8823094

 
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Controlling Atomic Energy 5, 1950s

AVE7296680

Controlling Atomic Energy 5, 1950s

AVE7296680

 
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Nuclear power plant Lubmin Castor container for radioactive waste, in the ZLN ..., 2000 (photo)

Rolf Zöllner

IMO8823066

Nuclear power plant Lubmin Castor container for radioactive waste, in the ZLN ..., 2000 (photo)

Rolf Zöllner

IMO8823066

 
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Nuclear power plant Lubmin special saw in the former nuclear power plant Lubmin, now ..., 2000 (photo)

Rolf Zöllner

IMO8823085

Nuclear power plant Lubmin special saw in the former nuclear power plant Lubmin, now ..., 2000 (photo)

Rolf Zöllner

IMO8823085

 
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Controlling Atomic Energy 40, 1950s

AVE7296715

Controlling Atomic Energy 40, 1950s

AVE7296715

 
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Nuclear power plant Lubmin decommissioned and dismantled reactor in the former nuclear power plant ..., 2000 (photo)

Rolf Zöllner

IMO8823070

Nuclear power plant Lubmin decommissioned and dismantled reactor in the former nuclear power plant ..., 2000 (photo)

Rolf Zöllner

IMO8823070

 
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Kernkraftwerk Lubmin Direktor des Zwischenlager Nord Juergen Fischer weist …, 2000 (photo)

Rolf Zöllner

IMO8823074

Kernkraftwerk Lubmin Direktor des Zwischenlager Nord Juergen Fischer weist …, 2000 (photo)

Rolf Zöllner

IMO8823074

 
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Nuclear power plant Lubmin irradiated boiler, ZLN (Zwischenlager Nord) ..., 2000 (photo)

Rolf Zöllner

IMO8823087

Nuclear power plant Lubmin irradiated boiler, ZLN (Zwischenlager Nord) ..., 2000 (photo)

Rolf Zöllner

IMO8823087

 
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Nuclear power plant Lubmin so-called manipulator in the former nuclear power plant Lubmin, now ..., 2000 (photo)

Rolf Zöllner

IMO8822996

Nuclear power plant Lubmin so-called manipulator in the former nuclear power plant Lubmin, now ..., 2000 (photo)

Rolf Zöllner

IMO8822996

 
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Lubmin nuclear power plant radioactive waste from Rheinsberg NPP in the ZLN ..., 2000 (photo)

Rolf Zöllner

IMO8823017

Lubmin nuclear power plant radioactive waste from Rheinsberg NPP in the ZLN ..., 2000 (photo)

Rolf Zöllner

IMO8823017

 
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Nuclear power plant Lubmin destroyed reactor in the former nuclear power plant Lubmin ..., 2000 (photo)

Rolf Zöllner

IMO8823018

Nuclear power plant Lubmin destroyed reactor in the former nuclear power plant Lubmin ..., 2000 (photo)

Rolf Zöllner

IMO8823018

 
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Atomwiederaufbereitungsanlage La Hague Atomwiederaufbereitungsanlage La …, 2000 (photo)

Rolf Zöllner

IMO8824277

Atomwiederaufbereitungsanlage La Hague Atomwiederaufbereitungsanlage La …, 2000 (photo)

Rolf Zöllner

IMO8824277

 
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BUND - Energiesparen Groesster Stecker der Welt, BUND and Federal Ministry for the Environment ..., 1999 (photo)

Rolf Zöllner

IMO8826626

BUND - Energiesparen Groesster Stecker der Welt, BUND and Federal Ministry for the Environment ..., 1999 (photo)

Rolf Zöllner

IMO8826626

 
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BUND - Energiesparen Pressekonferenz im Roten Rathaus, BUND und Bundesumweltministerium …, 1999 (photo)

Rolf Zöllner

IMO8826690

BUND - Energiesparen Pressekonferenz im Roten Rathaus, BUND und Bundesumweltministerium …, 1999 (photo)

Rolf Zöllner

IMO8826690

 
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Comet nucleus and planet - Illustration - Comet nucleus and a planet Artwor

Dixon, Don (b.1951)

PIX4571530

Comet nucleus and planet - Illustration - Comet nucleus and a planet Artwor

Dixon, Don (b.1951)

PIX4571530

 
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Renate Kuenast, new federal chairwoman of Buendnis 90 Die Gruenen Start of a ..., 2000 (photo)

Rolf Zöllner

IMO8824272

Renate Kuenast, new federal chairwoman of Buendnis 90 Die Gruenen Start of a ..., 2000 (photo)

Rolf Zöllner

IMO8824272

 
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Nuclear power plant Lubmin destroyed reactor in the former nuclear power plant Lubmin ..., 2000 (photo)

Rolf Zöllner

IMO8823075

Nuclear power plant Lubmin destroyed reactor in the former nuclear power plant Lubmin ..., 2000 (photo)

Rolf Zöllner

IMO8823075

 
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Renate Kuenast, new federal chairwoman of Buendnis 90 Die Gruenen Start of a ..., 2000 (photo)

Rolf Zöllner

IMO8824260

Renate Kuenast, new federal chairwoman of Buendnis 90 Die Gruenen Start of a ..., 2000 (photo)

Rolf Zöllner

IMO8824260

 
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Renate Kuenast, new federal chairwoman of Buendnis 90 Die Gruenen Start of a ..., 2000 (photo)

Rolf Zöllner

IMO8824288

Renate Kuenast, new federal chairwoman of Buendnis 90 Die Gruenen Start of a ..., 2000 (photo)

Rolf Zöllner

IMO8824288

 
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Kernkraftwerk Lubmin stillgelegter Reaktor im ehm. Kernkraftwerk Lubmin ..., 2000 (photo)

Rolf Zöllner

IMO8823072

Kernkraftwerk Lubmin stillgelegter Reaktor im ehm. Kernkraftwerk Lubmin ..., 2000 (photo)

Rolf Zöllner

IMO8823072

 
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Renate Kuenast, new federal chairwoman of Buendnis 90 Die Gruenen Start of a ..., 2000 (photo)

Rolf Zöllner

IMO8824323

Renate Kuenast, new federal chairwoman of Buendnis 90 Die Gruenen Start of a ..., 2000 (photo)

Rolf Zöllner

IMO8824323

 
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The wedding of the atom, 1955 (oil and tempera on canvas)

Tulli, Wladimiro (1922-2003)

SBL7293953

The wedding of the atom, 1955 (oil and tempera on canvas)

Tulli, Wladimiro (1922-2003)

SBL7293953

 
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Neckar GKN II joint nuclear power plant in Neckarwestheim !RECORD DATE ..., 1988 (photo)

Detlev Konnerth

IMO8823119

Neckar GKN II joint nuclear power plant in Neckarwestheim !RECORD DATE ..., 1988 (photo)

Detlev Konnerth

IMO8823119

 
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Nuclear power plant Neckar GKN II in Neckarwestheim! ESTIMATED DATE OF INCLUSION! …, 1988 (photo)

Detlev Konnerth

IMO8823121

Nuclear power plant Neckar GKN II in Neckarwestheim! ESTIMATED DATE OF INCLUSION! …, 1988 (photo)

Detlev Konnerth

IMO8823121

 
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BUND - Energiesparen Groesster Stecker der Welt, BUND and Federal Ministry for the Environment ..., 1999 (photo)

Rolf Zöllner

IMO8826740

BUND - Energiesparen Groesster Stecker der Welt, BUND and Federal Ministry for the Environment ..., 1999 (photo)

Rolf Zöllner

IMO8826740

 
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1960s: Small part of the model of a complex molecule.

AVE8908649

1960s: Small part of the model of a complex molecule.

AVE8908649

 
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BUND - Energiesparen Groesster Stecker der Welt, BUND und Bundesumweltministerium …, 1999 (photo)

Rolf Zöllner

IMO8827186

BUND - Energiesparen Groesster Stecker der Welt, BUND und Bundesumweltministerium …, 1999 (photo)

Rolf Zöllner

IMO8827186

 
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Controlling Atomic Energy 16, 1950s

AVE7296691

Controlling Atomic Energy 16, 1950s

AVE7296691

 
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BUND - Energiesparen Groesster Stecker der Welt, BUND und Bundesumweltministerium …, 1999 (photo)

Rolf Zöllner

IMO8826688

BUND - Energiesparen Groesster Stecker der Welt, BUND und Bundesumweltministerium …, 1999 (photo)

Rolf Zöllner

IMO8826688

 
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Renate Kuenast, new federal chairwoman of Buendnis 90 Die Gruenen Start of a ..., 2000 (photo)

Rolf Zöllner

IMO8824273

Renate Kuenast, new federal chairwoman of Buendnis 90 Die Gruenen Start of a ..., 2000 (photo)

Rolf Zöllner

IMO8824273

 
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Renate Kuenast, new federal chairwoman of Buendnis 90 Die Gruenen Start of a ..., 2000 (photo)

Rolf Zöllner

IMO8824309

Renate Kuenast, new federal chairwoman of Buendnis 90 Die Gruenen Start of a ..., 2000 (photo)

Rolf Zöllner

IMO8824309

 
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BUND - Energiesparen Groesster Stecker der Welt, BUND and Federal Ministry for the Environment ..., 1999 (photo)

Rolf Zöllner

IMO8826798

BUND - Energiesparen Groesster Stecker der Welt, BUND and Federal Ministry for the Environment ..., 1999 (photo)

Rolf Zöllner

IMO8826798

 
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BUND - Energiesparen Groesster Stecker der Welt, BUND und Bundesumweltministerium …, 1999 (photo)

Rolf Zöllner

IMO8827071

BUND - Energiesparen Groesster Stecker der Welt, BUND und Bundesumweltministerium …, 1999 (photo)

Rolf Zöllner

IMO8827071

 
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Controlling Atomic Energy 36, 1950s

AVE7296711

Controlling Atomic Energy 36, 1950s

AVE7296711

 
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Anti-nuclear power plant assembly of the Greens in Nuremberg..., 1987 (photo)

Dieter Bauer

IMO8815365

Anti-nuclear power plant assembly of the Greens in Nuremberg..., 1987 (photo)

Dieter Bauer

IMO8815365

 
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Controlling Atomic Energy 24, 1950s

AVE7296699

Controlling Atomic Energy 24, 1950s

AVE7296699

 
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Le Soleil vu en coupe - Sun cutaway: Cutaway of the sun, showing core, radiative and convective zones, and corona

Dixon, Don (b.1951)

PIX4629374

Le Soleil vu en coupe - Sun cutaway: Cutaway of the sun, showing core, radiative and convective zones, and corona

Dixon, Don (b.1951)

PIX4629374

 
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The first galaxies - The first galaxies - Artist's view of the appearance of giant stars at the intersection of hydrogen filaments, which will form the nuclei of the first galaxies. Giant stars form at the intersections of great filaments of primordial hydrogen, forming the nuclei of the first galaxies

Dixon, Don (b.1951)

PIX4634481

The first galaxies - The first galaxies - Artist's view of the appearance of giant stars at the intersection of hydrogen filaments, which will form the nuclei of the first galaxies. Giant stars form at the intersections of great filaments of primordial hydrogen, forming the nuclei of the first galaxies

Dixon, Don (b.1951)

PIX4634481

 
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Anti-nuclear power plant assembly of the Greens in Nuremberg..., 1987 (photo)

Dieter Bauer

IMO8815374

Anti-nuclear power plant assembly of the Greens in Nuremberg..., 1987 (photo)

Dieter Bauer

IMO8815374

 
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Anti-nuclear power plant assembly of the Greens at the KOMM youth center in Nuremberg..., 1987 (photo)

Dieter Bauer

IMO8815378

Anti-nuclear power plant assembly of the Greens at the KOMM youth center in Nuremberg..., 1987 (photo)

Dieter Bauer

IMO8815378

 
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Anti-nuclear power plant assembly of the Greens at the KOMM youth center in Nuremberg..., 1987 (photo)

Dieter Bauer

IMO8815382

Anti-nuclear power plant assembly of the Greens at the KOMM youth center in Nuremberg..., 1987 (photo)

Dieter Bauer

IMO8815382

 
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Neckar GKN II joint nuclear power plant in Neckarwestheim !RECORD DATE ..., 1988 (photo)

Detlev Konnerth

IMO8823120

Neckar GKN II joint nuclear power plant in Neckarwestheim !RECORD DATE ..., 1988 (photo)

Detlev Konnerth

IMO8823120

 
Equipment created to diseintegrate the atom

FGL7272476

Equipment created to diseintegrate the atom

FGL7272476

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