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' Emissionen' Bilder und Clips Suchergebnisse page 1 of 2

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Bilder zu ' Emissionen' gefunden, 128

Celestial objects, electromagnetic emissions and observation technology
 
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Celestial objects, electromagnetic emissions and observation technology

DGA572707

Celestial objects, electromagnetic emissions and observation technology

DGA572707

Factory near Helmstedt (b/w photo)
 
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Factory near Helmstedt (b/w photo)

Alfred Strobel

SZT3515701

Factory near Helmstedt (b/w photo)

Alfred Strobel

SZT3515701

United States 1950s: A lab technician uses a radiation testing machine to read the emissions from a stack of gallium blocks
 
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United States 1950s: A lab technician uses a radiation testing machine to read the emissions from a stack of gallium blocks

AVE6324225

United States 1950s: A lab technician uses a radiation testing machine to read the emissions from a stack of gallium blocks

AVE6324225

France, River Seine, view of nuclear plants.
 
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France, River Seine, view of nuclear plants.

UDK841833

France, River Seine, view of nuclear plants.

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Japan, Kyushu, Mount Aso caldera, fuming crater of Mount Nakadake.
 
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Japan, Kyushu, Mount Aso caldera, fuming crater of Mount Nakadake.

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Japan, Kyushu, Mount Aso caldera, fuming crater of Mount Nakadake.

UDK844034

At “Don Camillo” The Review By Jacqueline Joubert And Roger Lanzac Parodiant The TV Emissions On December 9, 1966 Here With Pierre Roussel (b/w photo)
 
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At “Don Camillo” The Review By Jacqueline Joubert And Roger Lanzac Parodiant The TV Emissions On December 9, 1966 Here With Pierre Roussel (b/w photo)

XRA1667942

At “Don Camillo” The Review By Jacqueline Joubert And Roger Lanzac Parodiant The TV Emissions On December 9, 1966 Here With Pierre Roussel (b/w photo)

XRA1667942

USA, Illinois, Chicago, nr Union Station, front of a train in train yard, steam rising from side of tracks, high angle view.
 
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USA, Illinois, Chicago, nr Union Station, front of a train in train yard, steam rising from side of tracks, high angle view.

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USA, Illinois, Chicago, nr Union Station, front of a train in train yard, steam rising from side of tracks, high angle view.

UDK847189

In Pleumeur Bodou (Brittany), The Spacel Centre : White Sphere 50 Meters Diameter, It Recorded The Emissions Relayed By Satellite "Telstar" on July 19, 1962 (b/w photo)
 
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In Pleumeur Bodou (Brittany), The Spacel Centre : White Sphere 50 Meters Diameter, It Recorded The Emissions Relayed By Satellite "Telstar" on July 19, 1962 (b/w photo)

XRA1658662

In Pleumeur Bodou (Brittany), The Spacel Centre : White Sphere 50 Meters Diameter, It Recorded The Emissions Relayed By Satellite "Telstar" on July 19, 1962 (b/w photo)

XRA1658662

At the “Don Camillo” The Review Of Jacqueline Joubert And Roger Lanzac Parodiant The Emissions Of Tv Here Roger Lanzac (Right) And Jean Valton In “Readings For All” September 9, 1966 (b/w photo)
 
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At the “Don Camillo” The Review Of Jacqueline Joubert And Roger Lanzac Parodiant The Emissions Of Tv Here Roger Lanzac (Right) And Jean Valton In “Readings For All” September 9, 1966 (b/w photo)

XRA1667272

At the “Don Camillo” The Review Of Jacqueline Joubert And Roger Lanzac Parodiant The Emissions Of Tv Here Roger Lanzac (Right) And Jean Valton In “Readings For All” September 9, 1966 (b/w photo)

XRA1667272

Eco Anxiety
 
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Eco Anxiety

Huntley, Claire

AJO7143534

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Eco Anxiety

Huntley, Claire

AJO7143534

Elephant tube nebula (VDB 142) in Cephee - The Elephant Trunk Nebula (VDB 142) in Cepheus: IC1396, VDB 142. Nebula located about 2700 light years from Earth. Image obtained with a bezel Tele Vue NP127iS, through 3 different filters that demonstrate oxygen, hydrogen, and sulfur - The Elephant Trunk Nebula (IC 1396A) in Cepheus is part of the larger IC 1396 complex which spans a large area of the sky measuring 170 by 140 arc-minutes and is one of the brightest emission nebulae with a magnitude of 3.5. The western portion of IC 1396 contains the Elephant Trunk Nebula (IC 1396A) which is characterized with H-II emissions, dark lanes and globules as well as a small reflection nebula. The IC 1396 complex is technically a star cluster (aka Cr 439, Trumpler 37) owing to the presence of a developing open but loose cluster at the heart of this rich nebulosity. This open star cluster is comprised of 50-100 member stars which vary in brightness spanning an area of approximately 50 'in diameter and which are not very well detached from the background sky. This stellar nursery lies at a distance of 2,720 light-years away - Image taken in combining the light from 3 different filters tracing emission from oxygen, hydrogen, and sulphur
 
Elephant tube nebula (VDB 142) in Cephee - The Elephant Trunk Nebula (VDB 142) in Cepheus: IC1396, VDB 142. Nebula located about 2700 light years from Earth. Image obtained with a bezel Tele Vue NP127iS, through 3 different filters that demonstrate oxygen, hydrogen, and sulfur - The Elephant Trunk Nebula (IC 1396A) in Cepheus is part of the larger IC 1396 complex which spans a large area of the sky measuring 170 by 140 arc-minutes and is one of the brightest emission nebulae with a magnitude of 3.5. The western portion of IC 1396 contains the Elephant Trunk Nebula (IC 1396A) which is characterized with H-II emissions, dark lanes and globules as well as a small reflection nebula. The IC 1396 complex is technically a star cluster (aka Cr 439, Trumpler 37) owing to the presence of a developing open but loose cluster at the heart of this rich nebulosity. This open star cluster is comprised of 50-100 member stars which vary in brightness spanning an area of approximately 50 'in diameter and

W. Promper

PIX4622329

Elephant tube nebula (VDB 142) in Cephee - The Elephant Trunk Nebula (VDB 142) in Cepheus: IC1396, VDB 142. Nebula located about 2700 light years from Earth. Image obtained with a bezel Tele Vue NP127iS, through 3 different filters that demonstrate oxygen, hydrogen, and sulfur - The Elephant Trunk Nebula (IC 1396A) in Cepheus is part of the larger IC 1396 complex which spans a large area of the sky measuring 170 by 140 arc-minutes and is one of the brightest emission nebulae with a magnitude of 3.5. The western portion of IC 1396 contains the Elephant Trunk Nebula (IC 1396A) which is characterized with H-II emissions, dark lanes and globules as well as a small reflection nebula. The IC 1396 complex is technically a star cluster (aka Cr 439, Trumpler 37) owing to the presence of a developing open but loose cluster at the heart of this rich nebulosity. This open star cluster is comprised of 50-100 member stars which vary in brightness spanning an area of approximately 50 'in diameter and

W. Promper

PIX4622329

Patagonia, Chile (photo)
 
Patagonia, Chile (photo)

UIG807769

Patagonia, Chile (photo)

UIG807769

Dessert and Fork on Placemat, Chile (photo)
 
Dessert and Fork on Placemat, Chile (photo)

UIG807775

Dessert and Fork on Placemat, Chile (photo)

UIG807775

Field, Patagonia, Chile (photo)
 
Field, Patagonia, Chile (photo)

UIG807782

Field, Patagonia, Chile (photo)

UIG807782

Snow-covered Mountains and Lake, Patagonia, Chile (photo)
 
Snow-covered Mountains and Lake, Patagonia, Chile (photo)

UIG807765

Snow-covered Mountains and Lake, Patagonia, Chile (photo)

UIG807765

Snow-covered Mountains and Lake, Patagonia, Chile (photo)
 
Snow-covered Mountains and Lake, Patagonia, Chile (photo)

UIG807789

Snow-covered Mountains and Lake, Patagonia, Chile (photo)

UIG807789

Snow-covered Mountains and lake, Patagonia, Chile (photo)
 
Snow-covered Mountains and lake, Patagonia, Chile (photo)

UIG807771

Snow-covered Mountains and lake, Patagonia, Chile (photo)

UIG807771

Darwin's Rhea, Rhea pennata, Chile (photo)
 
Darwin's Rhea, Rhea pennata, Chile (photo)

UIG807777

Darwin's Rhea, Rhea pennata, Chile (photo)

UIG807777

Snow-covered Mountains, Patagonia, Chile (photo)
 
Snow-covered Mountains, Patagonia, Chile (photo)

UIG807779

Snow-covered Mountains, Patagonia, Chile (photo)

UIG807779

Snow-covered Mountains, Patagonia, Chile (photo)
 
Snow-covered Mountains, Patagonia, Chile (photo)

UIG807781

Snow-covered Mountains, Patagonia, Chile (photo)

UIG807781

Snow-covered Mountains, Patagonia, Chile (photo)
 
Snow-covered Mountains, Patagonia, Chile (photo)

UIG807770

Snow-covered Mountains, Patagonia, Chile (photo)

UIG807770

Snow-covered Mountains and Lake, Patagonia, Chile (photo)
 
Snow-covered Mountains and Lake, Patagonia, Chile (photo)

UIG807783

Snow-covered Mountains and Lake, Patagonia, Chile (photo)

UIG807783

Snow-covered Mountains and Lake, Patagonia, Chile (photo)
 
Snow-covered Mountains and Lake, Patagonia, Chile (photo)

UIG807788

Snow-covered Mountains and Lake, Patagonia, Chile (photo)

UIG807788

Volcanic ash cloud in Iceland - Volcanic ash cloud from Iceland - The volcanic ash cloud caused by the eruption of the Eyjafjoell volcano in Iceland seen by the Envisat satellite on 19 April 2010. In this image taken on 19 April 2010 by ESA's Envisat satellite, a heavy plume of ash from the Eyjafjallajoekull Volcano in Iceland is seen travelling in a roughly southeasterly direction. The volcano has been emitting steam and ash since its recent eruptions began on 20 March, and as observable, the emissions continue. The plume, visible in brownish - grey, is approximately 400 km long
 
Volcanic ash cloud in Iceland - Volcanic ash cloud from Iceland - The volcanic ash cloud caused by the eruption of the Eyjafjoell volcano in Iceland seen by the Envisat satellite on 19 April 2010. In this image taken on 19 April 2010 by ESA's Envisat satellite, a heavy plume of ash from the Eyjafjallajoekull Volcano in Iceland is seen travelling in a roughly southeasterly direction. The volcano has been emitting steam and ash since its recent eruptions began on 20 March, and as observable, the emissions continue. The plume, visible in brownish - grey, is approximately 400 km long

PIX4666194

Volcanic ash cloud in Iceland - Volcanic ash cloud from Iceland - The volcanic ash cloud caused by the eruption of the Eyjafjoell volcano in Iceland seen by the Envisat satellite on 19 April 2010. In this image taken on 19 April 2010 by ESA's Envisat satellite, a heavy plume of ash from the Eyjafjallajoekull Volcano in Iceland is seen travelling in a roughly southeasterly direction. The volcano has been emitting steam and ash since its recent eruptions began on 20 March, and as observable, the emissions continue. The plume, visible in brownish - grey, is approximately 400 km long

PIX4666194

South American Fox, Culpeo, Chile (photo)
 
South American Fox, Culpeo, Chile (photo)

UIG807786

South American Fox, Culpeo, Chile (photo)

UIG807786

Etoile filante -Perseide - Perseid meteor - Rain d'étoiles filantes vue le 12/08/2008. Perseid meteor seem to radiate out of the same point in the constellation of Perseus in this composite exposure taken on August 12, 2008 during the Perseid Meteor Shower. The Perseids are tiny bits of dust left behind by Comet Swift-Tuttle on one of its day's through the Solar system. Although the comet is now far away, the dust left behind stays in orbit around the Sun, and sometimes the Earth passes through this dust trail, causing a meteor shower. The colors in the meteor's path come from different emissions as the meteor, speeding at 132,000 miles per hour, burns up and interacts with molecules in the upper atmosphere
 
Etoile filante -Perseide - Perseid meteor - Rain d'étoiles filantes vue le 12/08/2008. Perseid meteor seem to radiate out of the same point in the constellation of Perseus in this composite exposure taken on August 12, 2008 during the Perseid Meteor Shower. The Perseids are tiny bits of dust left behind by Comet Swift-Tuttle on one of its day's through the Solar system. Although the comet is now far away, the dust left behind stays in orbit around the Sun, and sometimes the Earth passes through this dust trail, causing a meteor shower. The colors in the meteor's path come from different emissions as the meteor, speeding at 132,000 miles per hour, burns up and interacts with molecules in the upper atmosphere

Jerry Lodriguss

PIX4598868

Etoile filante -Perseide - Perseid meteor - Rain d'étoiles filantes vue le 12/08/2008. Perseid meteor seem to radiate out of the same point in the constellation of Perseus in this composite exposure taken on August 12, 2008 during the Perseid Meteor Shower. The Perseids are tiny bits of dust left behind by Comet Swift-Tuttle on one of its day's through the Solar system. Although the comet is now far away, the dust left behind stays in orbit around the Sun, and sometimes the Earth passes through this dust trail, causing a meteor shower. The colors in the meteor's path come from different emissions as the meteor, speeding at 132,000 miles per hour, burns up and interacts with molecules in the upper atmosphere

Jerry Lodriguss

PIX4598868

Icebergs, Patagonia, Chile (photo)
 
Icebergs, Patagonia, Chile (photo)

UIG807773

Icebergs, Patagonia, Chile (photo)

UIG807773

South American Fox, Culpeo, Chile (photo)
 
South American Fox, Culpeo, Chile (photo)

UIG807787

South American Fox, Culpeo, Chile (photo)

UIG807787

Cascades and Snow-covered Mountains, Patagonia, Chile (photo)
 
Cascades and Snow-covered Mountains, Patagonia, Chile (photo)

UIG807785

Cascades and Snow-covered Mountains, Patagonia, Chile (photo)

UIG807785

Snow-covered Mountains and Lake, Patagonia, Chile (photo)
 
Snow-covered Mountains and Lake, Patagonia, Chile (photo)

UIG807772

Snow-covered Mountains and Lake, Patagonia, Chile (photo)

UIG807772

Cascades and Snow-covered Mountains, Patagonia, Chile (photo)
 
Cascades and Snow-covered Mountains, Patagonia, Chile (photo)

UIG807784

Cascades and Snow-covered Mountains, Patagonia, Chile (photo)

UIG807784

Elephant tube nebula (VDB 142) in Cephee - The Elephant Trunk Nebula (VDB 142) in Cepheus - IC1396, VDB 142. Nebula located about 2700 years - light from Earth. Image obtained with a telescope 40 cm in diameter, through 3 different filters that highlight oxygen, hydrogen, and sulfur. The Elephant Trunk Nebula (IC 1396A) in Cepheus is part of the larger IC 1396 complex which spans a large area of the sky measuring 170 by 140 arc - minutes and is one of the brightest emission nebulae with a magnitude of 3.5. The western portion of IC 1396 contains the Elephant Trunk Nebula (IC 1396A) which is characterized with H - II emissions, dark lanes and globules as well as a small reflection nebula. The IC 1396 complex is technically a star cluster (aka Cr 439, Trumpler 37) owing to the presence of a developing open but loose cluster at the heart of this rich nebulosity. This open star cluster is comprised of 50 - 100 member stars which vary in brightness spanning an area of approximately 50 'in diameter and which are not very well detached from the background sky. This stellar nursery lies at a distance of 2,720 light - years away. Image taken with a 16 inch telescope in combining the light from 3 different filters tracing emission from oxygen, hydrogen, and sulphur
 
Elephant tube nebula (VDB 142) in Cephee - The Elephant Trunk Nebula (VDB 142) in Cepheus - IC1396, VDB 142. Nebula located about 2700 years - light from Earth. Image obtained with a telescope 40 cm in diameter, through 3 different filters that highlight oxygen, hydrogen, and sulfur. The Elephant Trunk Nebula (IC 1396A) in Cepheus is part of the larger IC 1396 complex which spans a large area of the sky measuring 170 by 140 arc - minutes and is one of the brightest emission nebulae with a magnitude of 3.5. The western portion of IC 1396 contains the Elephant Trunk Nebula (IC 1396A) which is characterized with H - II emissions, dark lanes and globules as well as a small reflection nebula. The IC 1396 complex is technically a star cluster (aka Cr 439, Trumpler 37) owing to the presence of a developing open but loose cluster at the heart of this rich nebulosity. This open star cluster is comprised of 50 - 100 member stars which vary in brightness spanning an area of approximately 50 'in d

PIX4622303

Elephant tube nebula (VDB 142) in Cephee - The Elephant Trunk Nebula (VDB 142) in Cepheus - IC1396, VDB 142. Nebula located about 2700 years - light from Earth. Image obtained with a telescope 40 cm in diameter, through 3 different filters that highlight oxygen, hydrogen, and sulfur. The Elephant Trunk Nebula (IC 1396A) in Cepheus is part of the larger IC 1396 complex which spans a large area of the sky measuring 170 by 140 arc - minutes and is one of the brightest emission nebulae with a magnitude of 3.5. The western portion of IC 1396 contains the Elephant Trunk Nebula (IC 1396A) which is characterized with H - II emissions, dark lanes and globules as well as a small reflection nebula. The IC 1396 complex is technically a star cluster (aka Cr 439, Trumpler 37) owing to the presence of a developing open but loose cluster at the heart of this rich nebulosity. This open star cluster is comprised of 50 - 100 member stars which vary in brightness spanning an area of approximately 50 'in d

PIX4622303

Icebergs, Patagonia, Chile (photo)
 
Icebergs, Patagonia, Chile (photo)

UIG807774

Icebergs, Patagonia, Chile (photo)

UIG807774

Upland Geese, Chloephaga picta, Chile (photo)
 
Upland Geese, Chloephaga picta, Chile (photo)

UIG807778

Upland Geese, Chloephaga picta, Chile (photo)

UIG807778

Group of Guanacos, Lama guanicoe, Chile (photo)
 
Group of Guanacos, Lama guanicoe, Chile (photo)

UIG807780

Group of Guanacos, Lama guanicoe, Chile (photo)

UIG807780

Yurt Interior, Patagonia Camp, Chile (photo)
 
Yurt Interior, Patagonia Camp, Chile (photo)

UIG807776

Yurt Interior, Patagonia Camp, Chile (photo)

UIG807776

United States, 1960s: cartoon animation of positive crank case ventilation valve
 
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United States, 1960s: cartoon animation of positive crank case ventilation valve

AVE6323772

United States, 1960s: cartoon animation of positive crank case ventilation valve

AVE6323772

Patagonia Camp, Chile (photo)
 
Patagonia Camp, Chile (photo)

UIG807763

Patagonia Camp, Chile (photo)

UIG807763

Patagonia Camp, Chile (photo)
 
Patagonia Camp, Chile (photo)

UIG807764

Patagonia Camp, Chile (photo)

UIG807764

Children of choir fainting because of carbon monoxide emanations from the stove of the church of Charquemont, in the Doubs, 1927 (print)
 
Children of choir fainting because of carbon monoxide emanations from the stove of the church of Charquemont, in the Doubs, 1927 (print)

Anonymous

Stefano Bianchetti

XEE4183876

Children of choir fainting because of carbon monoxide emanations from the stove of the church of Charquemont, in the Doubs, 1927 (print)

Anonymous

Stefano Bianchetti

XEE4183876

Elephant tube nebula (VDB 142) in Cephee - The Elephant Trunk Nebula (VDB 142) in Cepheus - IC1396, VDB 142. Nebula located about 2700 years - light from Earth. Image obtained with a telescope 61 cm in diameter. The Elephant Trunk Nebula (IC 1396A) in Cepheus is part of the larger IC 1396 complex which spans a large area of the sky measuring 170 by 140 arc - minutes and is one of the brightest emission nebulae with a magnitude of 3.5. The western portion of IC 1396 contains the Elephant Trunk Nebula (IC 1396A) which is characterized with H - II emissions, dark lanes and globules as well as a small reflection nebula. This stellar nursery lies at a distance of 2,720 light - years away. Image taken with a 24 - inch telescope
 
Elephant tube nebula (VDB 142) in Cephee - The Elephant Trunk Nebula (VDB 142) in Cepheus - IC1396, VDB 142. Nebula located about 2700 years - light from Earth. Image obtained with a telescope 61 cm in diameter. The Elephant Trunk Nebula (IC 1396A) in Cepheus is part of the larger IC 1396 complex which spans a large area of the sky measuring 170 by 140 arc - minutes and is one of the brightest emission nebulae with a magnitude of 3.5. The western portion of IC 1396 contains the Elephant Trunk Nebula (IC 1396A) which is characterized with H - II emissions, dark lanes and globules as well as a small reflection nebula. This stellar nursery lies at a distance of 2,720 light - years away. Image taken with a 24 - inch telescope

Adam Block

PIX4622392

Elephant tube nebula (VDB 142) in Cephee - The Elephant Trunk Nebula (VDB 142) in Cepheus - IC1396, VDB 142. Nebula located about 2700 years - light from Earth. Image obtained with a telescope 61 cm in diameter. The Elephant Trunk Nebula (IC 1396A) in Cepheus is part of the larger IC 1396 complex which spans a large area of the sky measuring 170 by 140 arc - minutes and is one of the brightest emission nebulae with a magnitude of 3.5. The western portion of IC 1396 contains the Elephant Trunk Nebula (IC 1396A) which is characterized with H - II emissions, dark lanes and globules as well as a small reflection nebula. This stellar nursery lies at a distance of 2,720 light - years away. Image taken with a 24 - inch telescope

Adam Block

PIX4622392

Oslo 19850308. The natural protections Geir Arne Bore t …, 1985 (photo)
 
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Oslo 19850308. The natural protections Geir Arne Bore t …, 1985 (photo)

Bjørn Sigurdsøn

NTB8699698

Oslo 19850308. The natural protections Geir Arne Bore t …, 1985 (photo)

Bjørn Sigurdsøn

NTB8699698

'Summer petrol campaign 1995' - Bartenstein and Schenz, 1995 (photo)
 
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'Summer petrol campaign 1995' - Bartenstein and Schenz, 1995 (photo)

Harald Schneider

PAA8904194

'Summer petrol campaign 1995' - Bartenstein and Schenz, 1995 (photo)

Harald Schneider

PAA8904194

Military satellite DSP - Military satellite DSP tilted to predeployment position - Deploiement d'un satellite militaire DSP (Defense Support Program) on board the space shuttle Atlantis on 1 December 1991. These American spy satellites detect missile and spacecraft launches and nuclear explosions thanks to their infrared sensor that detects heat emissions. Defense Support Program (DSP)/Inertial Upper Stage (IUS) spacecraft, with forward airborne support equipment payload retention latch actuator released (foreground), is raised to a 29 degree predeployment position by the ASE aft frame tilt actuator (AFTA) table in the payload bay of Atlantis, Orbiter Vehicle 104. DSP components include Infrared sensor (top), AR I, SHF Antenna, EHF Antenna, Link 2 High - Gain Antenna, star sensor, and stowed solar paddles (box - like structure around the base). The Earth's limb and the blackness of space create the backdrop for this deployment scene. DSP satellites detect missile or spacecraft launches and nuclear explosions using sensors that detect the infrared emissions from these intense sources of heat
 
Military satellite DSP - Military satellite DSP tilted to predeployment position - Deploiement d'un satellite militaire DSP (Defense Support Program) on board the space shuttle Atlantis on 1 December 1991. These American spy satellites detect missile and spacecraft launches and nuclear explosions thanks to their infrared sensor that detects heat emissions. Defense Support Program (DSP)/Inertial Upper Stage (IUS) spacecraft, with forward airborne support equipment payload retention latch actuator released (foreground), is raised to a 29 degree predeployment position by the ASE aft frame tilt actuator (AFTA) table in the payload bay of Atlantis, Orbiter Vehicle 104. DSP components include Infrared sensor (top), AR I, SHF Antenna, EHF Antenna, Link 2 High - Gain Antenna, star sensor, and stowed solar paddles (box - like structure around the base). The Earth's limb and the blackness of space create the backdrop for this deployment scene. DSP satellites detect missile or spacecraft launches

PIX4642655

Military satellite DSP - Military satellite DSP tilted to predeployment position - Deploiement d'un satellite militaire DSP (Defense Support Program) on board the space shuttle Atlantis on 1 December 1991. These American spy satellites detect missile and spacecraft launches and nuclear explosions thanks to their infrared sensor that detects heat emissions. Defense Support Program (DSP)/Inertial Upper Stage (IUS) spacecraft, with forward airborne support equipment payload retention latch actuator released (foreground), is raised to a 29 degree predeployment position by the ASE aft frame tilt actuator (AFTA) table in the payload bay of Atlantis, Orbiter Vehicle 104. DSP components include Infrared sensor (top), AR I, SHF Antenna, EHF Antenna, Link 2 High - Gain Antenna, star sensor, and stowed solar paddles (box - like structure around the base). The Earth's limb and the blackness of space create the backdrop for this deployment scene. DSP satellites detect missile or spacecraft launches

PIX4642655

Orion Nebula (M42 - 43) - The Orion Nebula - Located 1500 years ago - the Orion Nebula is the closest region to the formation of stars of the Sun. Image obtained with Siding Spring's 3.9m telescope. The Orion Nebula is famous for a number of reasons. It is the nearest bright nebula to us and can be seen with the naked eye. Its brightness led to it being the first nebula ever photographed (in 1882) and its proximity (1500 light years) means that we know more about it than any other star - forming region. It is also in a very active stage of star formation and it is perfectly placed for us to explore the intimate details of the birth of stars. The inner regions are glowing mainly in the red light of excited hydrogen, which together with some green emission from oxygen give the centre of the nebula a yellowish colour. The energy for this spectacular display comes from the small cluster of stars in the brightest part of the nebula. Three, five - minute exposures were used to make this picture using the Anglo - Australian Telescope at Siding Spring
 
Orion Nebula (M42 - 43) - The Orion Nebula - Located 1500 years ago - the Orion Nebula is the closest region to the formation of stars of the Sun. Image obtained with Siding Spring's 3.9m telescope. The Orion Nebula is famous for a number of reasons. It is the nearest bright nebula to us and can be seen with the naked eye. Its brightness led to it being the first nebula ever photographed (in 1882) and its proximity (1500 light years) means that we know more about it than any other star - forming region. It is also in a very active stage of star formation and it is perfectly placed for us to explore the intimate details of the birth of stars. The inner regions are glowing mainly in the red light of excited hydrogen, which together with some green emission from oxygen give the centre of the nebula a yellowish colour. The energy for this spectacular display comes from the small cluster of stars in the brightest part of the nebula. Three, five - minute exposures were used to make this pict

PIX4617657

Orion Nebula (M42 - 43) - The Orion Nebula - Located 1500 years ago - the Orion Nebula is the closest region to the formation of stars of the Sun. Image obtained with Siding Spring's 3.9m telescope. The Orion Nebula is famous for a number of reasons. It is the nearest bright nebula to us and can be seen with the naked eye. Its brightness led to it being the first nebula ever photographed (in 1882) and its proximity (1500 light years) means that we know more about it than any other star - forming region. It is also in a very active stage of star formation and it is perfectly placed for us to explore the intimate details of the birth of stars. The inner regions are glowing mainly in the red light of excited hydrogen, which together with some green emission from oxygen give the centre of the nebula a yellowish colour. The energy for this spectacular display comes from the small cluster of stars in the brightest part of the nebula. Three, five - minute exposures were used to make this pict

PIX4617657

Spiral galaxy of the Sombrero M104 infrared view - Sombrero galaxy seen in infrared - Infrared image of the spiral galaxy M104 (Sombrero galaxy), located about 28 million years ago - light, obtained with the Spitzer space telescope in 2004 and January 2005. Infrared radiation shows the dust of the disc visible throughout the circumference. A high emission also comes from the center of the galaxy where a supermassive black hole is thought to reside there. This spiral galaxy is located some 28 million light - years away. The infrared image obtained by Spitzer space telescope in 2004 and 2005 pierces through the obscuring dust, along with the bulge of stars. It shows that the disk is warped, which is often the result of a gravitational encounter with another galaxy; clumpy areas spotted in the far edges of the ring indicate young star - forming regions. Spitzer detected infrared emission not only from the ring, but from the center of the galaxy too, where there is a huge black hole, believed to be a billion times more massive than our Sun
 
Spiral galaxy of the Sombrero M104 infrared view - Sombrero galaxy seen in infrared - Infrared image of the spiral galaxy M104 (Sombrero galaxy), located about 28 million years ago - light, obtained with the Spitzer space telescope in 2004 and January 2005. Infrared radiation shows the dust of the disc visible throughout the circumference. A high emission also comes from the center of the galaxy where a supermassive black hole is thought to reside there. This spiral galaxy is located some 28 million light - years away. The infrared image obtained by Spitzer space telescope in 2004 and 2005 pierces through the obscuring dust, along with the bulge of stars. It shows that the disk is warped, which is often the result of a gravitational encounter with another galaxy; clumpy areas spotted in the far edges of the ring indicate young star - forming regions. Spitzer detected infrared emission not only from the ring, but from the center of the galaxy too, where there is a huge black hole, belie

PIX4611595

Spiral galaxy of the Sombrero M104 infrared view - Sombrero galaxy seen in infrared - Infrared image of the spiral galaxy M104 (Sombrero galaxy), located about 28 million years ago - light, obtained with the Spitzer space telescope in 2004 and January 2005. Infrared radiation shows the dust of the disc visible throughout the circumference. A high emission also comes from the center of the galaxy where a supermassive black hole is thought to reside there. This spiral galaxy is located some 28 million light - years away. The infrared image obtained by Spitzer space telescope in 2004 and 2005 pierces through the obscuring dust, along with the bulge of stars. It shows that the disk is warped, which is often the result of a gravitational encounter with another galaxy; clumpy areas spotted in the far edges of the ring indicate young star - forming regions. Spitzer detected infrared emission not only from the ring, but from the center of the galaxy too, where there is a huge black hole, belie

PIX4611595

The Formation of the Earth and the Moon - Young Earth and Moon - The young Earth draped with thick clouds is illuminated by lightning and the reddish glow of volcanoes. Still surrounded by the remains of the primitive nebula, it will wait another 500 million years to cool sufisciously, form a solid crust and develop a primitive atmosphere. Top right is the Moon, still covered in molten lava. A young Earth is shrouded in turbulent, roiling clouds, while under the shadow of its night side can be seen flashes of lightning and the ruddy glow of volcanoes and lava fields illuminating the clouds from beneath. The space around the Earth is highlighted by remnants of the nebula from which the Solar System was born. On the upper right is the Earth's Moon whose lava - filled scars from massive impacts are still cooling. 500 million years after its molten birth the Earth's surface would have cooled enough for a solid crust to form, and gases delivered by comets and emissions from within would have contributed to the Earth's first, albeit primitive, atmosphere
 
The Formation of the Earth and the Moon - Young Earth and Moon - The young Earth draped with thick clouds is illuminated by lightning and the reddish glow of volcanoes. Still surrounded by the remains of the primitive nebula, it will wait another 500 million years to cool sufisciously, form a solid crust and develop a primitive atmosphere. Top right is the Moon, still covered in molten lava. A young Earth is shrouded in turbulent, roiling clouds, while under the shadow of its night side can be seen flashes of lightning and the ruddy glow of volcanoes and lava fields illuminating the clouds from beneath. The space around the Earth is highlighted by remnants of the nebula from which the Solar System was born. On the upper right is the Earth's Moon whose lava - filled scars from massive impacts are still cooling. 500 million years after its molten birth the Earth's surface would have cooled enough for a solid crust to form, and gases delivered by comets and emissions from within would hav

Walter B Myers

PIX4633451

The Formation of the Earth and the Moon - Young Earth and Moon - The young Earth draped with thick clouds is illuminated by lightning and the reddish glow of volcanoes. Still surrounded by the remains of the primitive nebula, it will wait another 500 million years to cool sufisciously, form a solid crust and develop a primitive atmosphere. Top right is the Moon, still covered in molten lava. A young Earth is shrouded in turbulent, roiling clouds, while under the shadow of its night side can be seen flashes of lightning and the ruddy glow of volcanoes and lava fields illuminating the clouds from beneath. The space around the Earth is highlighted by remnants of the nebula from which the Solar System was born. On the upper right is the Earth's Moon whose lava - filled scars from massive impacts are still cooling. 500 million years after its molten birth the Earth's surface would have cooled enough for a solid crust to form, and gases delivered by comets and emissions from within would hav

Walter B Myers

PIX4633451

Elephant tube nebula (VDB 142) in Cephee - The Elephant Trunk Nebula (VDB 142) in Cepheus - IC1396, VDB 142. Nebula located about 2700 years - light from Earth. The Elephant Trunk Nebula (IC 1396A) in Cepheus is part of the larger IC 1396 complex which spans a large area of the sky measuring 170 by 140 arc - minutes and is one of the brightest emission nebulae with a magnitude of 3.5. The western portion of IC 1396 contains the Elephant Trunk Nebula (IC 1396A) which is characterized with H - II emissions, dark lanes and globules as well as a small reflection nebula. The IC 1396 complex is technically a star cluster (aka Cr 439, Trumpler 37) owing to the presence of a developing open but loose cluster at the heart of this rich nebulosity. This open star cluster is comprised of 50 - 100 member stars which vary in brightness spanning an area of approximately 50 'in diameter and which are not very well detached from the background sky. This stellar nursery lies at a distance of 2,720 light - years away
 
Elephant tube nebula (VDB 142) in Cephee - The Elephant Trunk Nebula (VDB 142) in Cepheus - IC1396, VDB 142. Nebula located about 2700 years - light from Earth. The Elephant Trunk Nebula (IC 1396A) in Cepheus is part of the larger IC 1396 complex which spans a large area of the sky measuring 170 by 140 arc - minutes and is one of the brightest emission nebulae with a magnitude of 3.5. The western portion of IC 1396 contains the Elephant Trunk Nebula (IC 1396A) which is characterized with H - II emissions, dark lanes and globules as well as a small reflection nebula. The IC 1396 complex is technically a star cluster (aka Cr 439, Trumpler 37) owing to the presence of a developing open but loose cluster at the heart of this rich nebulosity. This open star cluster is comprised of 50 - 100 member stars which vary in brightness spanning an area of approximately 50 'in diameter and which are not very well detached from the background sky. This stellar nursery lies at a distance of 2,720 light

Sebastian Voltmer

PIX4622327

Elephant tube nebula (VDB 142) in Cephee - The Elephant Trunk Nebula (VDB 142) in Cepheus - IC1396, VDB 142. Nebula located about 2700 years - light from Earth. The Elephant Trunk Nebula (IC 1396A) in Cepheus is part of the larger IC 1396 complex which spans a large area of the sky measuring 170 by 140 arc - minutes and is one of the brightest emission nebulae with a magnitude of 3.5. The western portion of IC 1396 contains the Elephant Trunk Nebula (IC 1396A) which is characterized with H - II emissions, dark lanes and globules as well as a small reflection nebula. The IC 1396 complex is technically a star cluster (aka Cr 439, Trumpler 37) owing to the presence of a developing open but loose cluster at the heart of this rich nebulosity. This open star cluster is comprised of 50 - 100 member stars which vary in brightness spanning an area of approximately 50 'in diameter and which are not very well detached from the background sky. This stellar nursery lies at a distance of 2,720 light

Sebastian Voltmer

PIX4622327

Physical Therapies Jugum penis, 1901-1930
 
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Physical Therapies Jugum penis, 1901-1930

UIS5101960

Physical Therapies Jugum penis, 1901-1930

UIS5101960

PENA ANNOUNCES ANNOUNCES BREAKTHROUGH, 1997-10-21 (photo)
 
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PENA ANNOUNCES ANNOUNCES BREAKTHROUGH, 1997-10-21 (photo)

Gary Cameron

REU8035785

PENA ANNOUNCES ANNOUNCES BREAKTHROUGH, 1997-10-21 (photo)

Gary Cameron

REU8035785

Energy Secretary Federico-Pena announced October 21 that U.S. scientists have made a breakthrough di.., 1997 (photo)
 
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Energy Secretary Federico-Pena announced October 21 that U.S. scientists have made a breakthrough di.., 1997 (photo)

Gary Cameron

REU7476626

Energy Secretary Federico-Pena announced October 21 that U.S. scientists have made a breakthrough di.., 1997 (photo)

Gary Cameron

REU7476626

Planetary nebula NGC 5189 in the Fly - NGC 5189 - Planetary nebula in Musca - This nebula is located about 3000 light years from Earth in the southern constellation of Fly. Image obtained by the Hubble Space Telescope (HST). The colors used in this image correspond to the emissions of different gases: sulfur in green, hydrogen in orange and oxygen in blue. Hubble Space Telescope have photographed a festive - looking nearby planetary nebula called NGC 5189. Planetary nebulae represent the final brief stage in the life of a medium - sized star like our Sun. While consuming the last of the fuel in its core, the dying star expels a large portion of its outer envelope. This material then becomes heated by the radiation from the stellar remnant and radiates, producing glowing clouds of gas that can show complex structures, as the ejection of mass from the star is uneven in both time and direction. This image was taken with Hubble's Wide Field Camera 3 on October 8, 2012, in filters tuned to the specific colors of fluorescing sulfur, hydrogen, and oxygen atoms. Broad filters in the visible and near - infrared were used to capture the star colors
 
Planetary nebula NGC 5189 in the Fly - NGC 5189 - Planetary nebula in Musca - This nebula is located about 3000 light years from Earth in the southern constellation of Fly. Image obtained by the Hubble Space Telescope (HST). The colors used in this image correspond to the emissions of different gases: sulfur in green, hydrogen in orange and oxygen in blue. Hubble Space Telescope have photographed a festive - looking nearby planetary nebula called NGC 5189. Planetary nebulae represent the final brief stage in the life of a medium - sized star like our Sun. While consuming the last of the fuel in its core, the dying star expels a large portion of its outer envelope. This material then becomes heated by the radiation from the stellar remnant and radiates, producing glowing clouds of gas that can show complex structures, as the ejection of mass from the star is uneven in both time and direction. This image was taken with Hubble's Wide Field Camera 3 on October 8, 2012, in filters tuned to

PIX4623125

Planetary nebula NGC 5189 in the Fly - NGC 5189 - Planetary nebula in Musca - This nebula is located about 3000 light years from Earth in the southern constellation of Fly. Image obtained by the Hubble Space Telescope (HST). The colors used in this image correspond to the emissions of different gases: sulfur in green, hydrogen in orange and oxygen in blue. Hubble Space Telescope have photographed a festive - looking nearby planetary nebula called NGC 5189. Planetary nebulae represent the final brief stage in the life of a medium - sized star like our Sun. While consuming the last of the fuel in its core, the dying star expels a large portion of its outer envelope. This material then becomes heated by the radiation from the stellar remnant and radiates, producing glowing clouds of gas that can show complex structures, as the ejection of mass from the star is uneven in both time and direction. This image was taken with Hubble's Wide Field Camera 3 on October 8, 2012, in filters tuned to

PIX4623125

Orion Nebula (M42 - 43) - The Orion Nebula - Located 1500 years ago - the Orion Nebula is the closest region to the formation of stars of the Sun. Image obtained with Siding Spring's 3.9m telescope. The Orion Nebula is famous for a number of reasons. It is the nearest bright nebula to us and can be seen with the naked eye. Its brightness led to it being the first nebula ever photographed (in 1882) and its proximity (1500 light years) means that we know more about it than any other star - forming region. It is also in a very active stage of star formation and it is perfectly placed for us to explore the intimate details of the birth of stars. The inner regions are glowing mainly in the red light of excited hydrogen, which together with some green emission from oxygen give the centre of the nebula a yellowish colour. The energy for this spectacular display comes from the small cluster of stars in the brightest part of the nebula. Three, five - minute exposures were used to make this picture using the Anglo - Australian Telescope at Siding Spring
 
Orion Nebula (M42 - 43) - The Orion Nebula - Located 1500 years ago - the Orion Nebula is the closest region to the formation of stars of the Sun. Image obtained with Siding Spring's 3.9m telescope. The Orion Nebula is famous for a number of reasons. It is the nearest bright nebula to us and can be seen with the naked eye. Its brightness led to it being the first nebula ever photographed (in 1882) and its proximity (1500 light years) means that we know more about it than any other star - forming region. It is also in a very active stage of star formation and it is perfectly placed for us to explore the intimate details of the birth of stars. The inner regions are glowing mainly in the red light of excited hydrogen, which together with some green emission from oxygen give the centre of the nebula a yellowish colour. The energy for this spectacular display comes from the small cluster of stars in the brightest part of the nebula. Three, five - minute exposures were used to make this pict

PIX4617852

Orion Nebula (M42 - 43) - The Orion Nebula - Located 1500 years ago - the Orion Nebula is the closest region to the formation of stars of the Sun. Image obtained with Siding Spring's 3.9m telescope. The Orion Nebula is famous for a number of reasons. It is the nearest bright nebula to us and can be seen with the naked eye. Its brightness led to it being the first nebula ever photographed (in 1882) and its proximity (1500 light years) means that we know more about it than any other star - forming region. It is also in a very active stage of star formation and it is perfectly placed for us to explore the intimate details of the birth of stars. The inner regions are glowing mainly in the red light of excited hydrogen, which together with some green emission from oxygen give the centre of the nebula a yellowish colour. The energy for this spectacular display comes from the small cluster of stars in the brightest part of the nebula. Three, five - minute exposures were used to make this pict

PIX4617852

BREAKTHROUGH ELECTRIC CELL UNVEILED, 1997-10-21 (photo)
 
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BREAKTHROUGH ELECTRIC CELL UNVEILED, 1997-10-21 (photo)

Gary Cameron

REU8085839

BREAKTHROUGH ELECTRIC CELL UNVEILED, 1997-10-21 (photo)

Gary Cameron

REU8085839

The harmful substance Rhoca-Gil used in the construction of the tunnel work on …, 1997 (photo)
 
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The harmful substance Rhoca-Gil used in the construction of the tunnel work on …, 1997 (photo)

Knut Fjeldstad

NTB8965408

The harmful substance Rhoca-Gil used in the construction of the tunnel work on …, 1997 (photo)

Knut Fjeldstad

NTB8965408

TRADERS SIGNAL TRADES IN THE DOW INDEX PIT AT THE CBOT, 2000-01-05 (photo)
 
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TRADERS SIGNAL TRADES IN THE DOW INDEX PIT AT THE CBOT, 2000-01-05 (photo)

Scott Olson

REU7998008

TRADERS SIGNAL TRADES IN THE DOW INDEX PIT AT THE CBOT, 2000-01-05 (photo)

Scott Olson

REU7998008

SHARE PRICES DROP IN TOKYO, 2003-11-19 (photo)
 
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SHARE PRICES DROP IN TOKYO, 2003-11-19 (photo)

Issei Kato

REU7763680

SHARE PRICES DROP IN TOKYO, 2003-11-19 (photo)

Issei Kato

REU7763680

A JAPANESE BUSINESSMAN WALKS PAST STOCK QUOTATION BOARD IN TOKYO, 2000-04-24 (photo)
 
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A JAPANESE BUSINESSMAN WALKS PAST STOCK QUOTATION BOARD IN TOKYO, 2000-04-24 (photo)

Susumu Toshiyuki

REU8008124

A JAPANESE BUSINESSMAN WALKS PAST STOCK QUOTATION BOARD IN TOKYO, 2000-04-24 (photo)

Susumu Toshiyuki

REU8008124

PASSERSBY ARE REFLECTED ON AN STOCK QUOTATION BOARD IN TOKYO, 2003-07-02 (photo)
 
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PASSERSBY ARE REFLECTED ON AN STOCK QUOTATION BOARD IN TOKYO, 2003-07-02 (photo)

Issei Kato

REU7717625

PASSERSBY ARE REFLECTED ON AN STOCK QUOTATION BOARD IN TOKYO, 2003-07-02 (photo)

Issei Kato

REU7717625

PASSERBY IS REFLECTED ON A GLASS WINDOW DISPLAYING THE STOCK PRICE IN TOKYO, 2003-07-02 (photo)
 
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PASSERBY IS REFLECTED ON A GLASS WINDOW DISPLAYING THE STOCK PRICE IN TOKYO, 2003-07-02 (photo)

Issei Kato

REU7813853

PASSERBY IS REFLECTED ON A GLASS WINDOW DISPLAYING THE STOCK PRICE IN TOKYO, 2003-07-02 (photo)

Issei Kato

REU7813853

A TOKYO BUSINESSMAN WIPES SWEAT AS HE WALKS PAST A QUOTATION BOARD, 2002-07-26 (photo)
 
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A TOKYO BUSINESSMAN WIPES SWEAT AS HE WALKS PAST A QUOTATION BOARD, 2002-07-26 (photo)

Kimimasa Mayama

REU8023761

A TOKYO BUSINESSMAN WIPES SWEAT AS HE WALKS PAST A QUOTATION BOARD, 2002-07-26 (photo)

Kimimasa Mayama

REU8023761

PRESIDENT OF THE CLIMATE CONFERENCE JAN PRONK ADDRESSES DELEGATES, 2000-11-24 (photo)
 
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PRESIDENT OF THE CLIMATE CONFERENCE JAN PRONK ADDRESSES DELEGATES, 2000-11-24 (photo)

Fred Ernst

REU8003490

PRESIDENT OF THE CLIMATE CONFERENCE JAN PRONK ADDRESSES DELEGATES, 2000-11-24 (photo)

Fred Ernst

REU8003490

AN ELDERLY INVESTOR WATCHES THE STOCK MARKET RISE IN SEOUL, 1997-12-17 (photo)
 
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AN ELDERLY INVESTOR WATCHES THE STOCK MARKET RISE IN SEOUL, 1997-12-17 (photo)

Str Old

REU8012476

AN ELDERLY INVESTOR WATCHES THE STOCK MARKET RISE IN SEOUL, 1997-12-17 (photo)

Str Old

REU8012476

Sombrero M104 Spiral Galaxy - Visible Composite - Infrared - The Sombrero galaxy. Composite of visible and infrared views - Composite image of the spiral galaxy M104 (Sombrero galaxy), located about 28 million years ago - light. Infrared image obtained with the Spitzer space telescope in 2004 and January 2005 superimposed on the image made by the Hubble space telescope visible in May and June 2003. The dark band of girders in this galaxy is visible throughout the circumference. Composite image of a visible image and an infrared image of the galaxy M104. The visible image was obtained by the Hubble space telescope in 2003, the infrared view by Spitzer telescope in 2004 and 2005. This spiral galaxy is located some 28 million light - years away. The infrared image obtained by Spitzer space telescope pierces through the obscuring dust, along with the bulge of stars. It shows that the disk is warped, which is often the result of a gravitational encounter with another galaxy; clumpy areas spotted in the far edges of the ring indicate young star - forming regions. Spitzer detected infrared emission not only from the ring, but from the center of the galaxy too, where there is a huge black hole, believed to be a billion times more massive than our Sun
 
Sombrero M104 Spiral Galaxy - Visible Composite - Infrared - The Sombrero galaxy. Composite of visible and infrared views - Composite image of the spiral galaxy M104 (Sombrero galaxy), located about 28 million years ago - light. Infrared image obtained with the Spitzer space telescope in 2004 and January 2005 superimposed on the image made by the Hubble space telescope visible in May and June 2003. The dark band of girders in this galaxy is visible throughout the circumference. Composite image of a visible image and an infrared image of the galaxy M104. The visible image was obtained by the Hubble space telescope in 2003, the infrared view by Spitzer telescope in 2004 and 2005. This spiral galaxy is located some 28 million light - years away. The infrared image obtained by Spitzer space telescope pierces through the obscuring dust, along with the bulge of stars. It shows that the disk is warped, which is often the result of a gravitational encounter with another galaxy; clumpy areas sp

PIX4611601

Sombrero M104 Spiral Galaxy - Visible Composite - Infrared - The Sombrero galaxy. Composite of visible and infrared views - Composite image of the spiral galaxy M104 (Sombrero galaxy), located about 28 million years ago - light. Infrared image obtained with the Spitzer space telescope in 2004 and January 2005 superimposed on the image made by the Hubble space telescope visible in May and June 2003. The dark band of girders in this galaxy is visible throughout the circumference. Composite image of a visible image and an infrared image of the galaxy M104. The visible image was obtained by the Hubble space telescope in 2003, the infrared view by Spitzer telescope in 2004 and 2005. This spiral galaxy is located some 28 million light - years away. The infrared image obtained by Spitzer space telescope pierces through the obscuring dust, along with the bulge of stars. It shows that the disk is warped, which is often the result of a gravitational encounter with another galaxy; clumpy areas sp

PIX4611601

TRADERS AT NEW YORK STOCK EXCHANGE, 2000-02-28 (photo)
 
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TRADERS AT NEW YORK STOCK EXCHANGE, 2000-02-28 (photo)

Peter Morgan

REU7786773

TRADERS AT NEW YORK STOCK EXCHANGE, 2000-02-28 (photo)

Peter Morgan

REU7786773

TOKYO STOCKS TUMBLE TO 5-MONTH LOW, 2002-07-26 (photo)
 
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TOKYO STOCKS TUMBLE TO 5-MONTH LOW, 2002-07-26 (photo)

Kimimasa Mayama

REU7983659

TOKYO STOCKS TUMBLE TO 5-MONTH LOW, 2002-07-26 (photo)

Kimimasa Mayama

REU7983659

US PRESIDENT BUSH SPEAKS ON CLEAR SKIES, 2003-09-16 (photo)
 
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US PRESIDENT BUSH SPEAKS ON CLEAR SKIES, 2003-09-16 (photo)

William Philpott

REU7689567

US PRESIDENT BUSH SPEAKS ON CLEAR SKIES, 2003-09-16 (photo)

William Philpott

REU7689567

US PRESIDENT BUSH TALKS ABOUT CLEAN SKIES, 2003-09-16 (photo)
 
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US PRESIDENT BUSH TALKS ABOUT CLEAN SKIES, 2003-09-16 (photo)

William Philpott

REU7736433

US PRESIDENT BUSH TALKS ABOUT CLEAN SKIES, 2003-09-16 (photo)

William Philpott

REU7736433

Birth of stars in the nebula NGC 3372 - Star formation in the Carina Nebula - Detail of the Carene nebula (NGC 3372) obtained by the Hubble space telescope. The image shows a column of gas eroded by ultraviolet radiation emitted by young stars. Jets are also visible, showing the presence of emerging stars. NGC 3372 is located about 7500 light years away from Earth. The colors used in this image correspond to the emissions of different gases: sulfur in red, hydrogen in green and oxygen in blue. The NASA Hubble Space Telescope photograph captures the chaotic activity atop a three - light - year - tall pillar of gas and dust that is being eaten away by the brilliant light from nearby bright stars. The pillar is also being assaulted from within, as infant stars buried inside it fire off jets of gas that can be seen streaming from towering peaks. This turbulent cosmic pinnacle lies within a tempestuous stellar nursery called the Carina Nebula, located 7,500 light - years away in the southern constellation Carina. Hubble's Wide Field Camera 3 observed the pillar on Feb. 1 - 2, 2010. The colors in this composite image correspond to the glow of oxygen (blue), hydrogen and nitrogen (green), and sulfur (red)
 
Birth of stars in the nebula NGC 3372 - Star formation in the Carina Nebula - Detail of the Carene nebula (NGC 3372) obtained by the Hubble space telescope. The image shows a column of gas eroded by ultraviolet radiation emitted by young stars. Jets are also visible, showing the presence of emerging stars. NGC 3372 is located about 7500 light years away from Earth. The colors used in this image correspond to the emissions of different gases: sulfur in red, hydrogen in green and oxygen in blue. The NASA Hubble Space Telescope photograph captures the chaotic activity atop a three - light - year - tall pillar of gas and dust that is being eaten away by the brilliant light from nearby bright stars. The pillar is also being assaulted from within, as infant stars buried inside it fire off jets of gas that can be seen streaming from towering peaks. This turbulent cosmic pinnacle lies within a tempestuous stellar nursery called the Carina Nebula, located 7,500 light - years away in the souther

PIX4619114

Birth of stars in the nebula NGC 3372 - Star formation in the Carina Nebula - Detail of the Carene nebula (NGC 3372) obtained by the Hubble space telescope. The image shows a column of gas eroded by ultraviolet radiation emitted by young stars. Jets are also visible, showing the presence of emerging stars. NGC 3372 is located about 7500 light years away from Earth. The colors used in this image correspond to the emissions of different gases: sulfur in red, hydrogen in green and oxygen in blue. The NASA Hubble Space Telescope photograph captures the chaotic activity atop a three - light - year - tall pillar of gas and dust that is being eaten away by the brilliant light from nearby bright stars. The pillar is also being assaulted from within, as infant stars buried inside it fire off jets of gas that can be seen streaming from towering peaks. This turbulent cosmic pinnacle lies within a tempestuous stellar nursery called the Carina Nebula, located 7,500 light - years away in the souther

PIX4619114

Promotion girls show off Mitsubishi Motors' concept car SUWadvance on display at Tokyo Motor Show pr.., 1999-10-20 (photo)
 
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Promotion girls show off Mitsubishi Motors' concept car SUWadvance on display at Tokyo Motor Show pr.., 1999-10-20 (photo)

Eriko Sugita

REU7517445

Promotion girls show off Mitsubishi Motors' concept car SUWadvance on display at Tokyo Motor Show pr.., 1999-10-20 (photo)

Eriko Sugita

REU7517445

US PRESIDENT BUSH URGES PASSING OF CLEAR SKIES, 2003-09-16 (photo)
 
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US PRESIDENT BUSH URGES PASSING OF CLEAR SKIES, 2003-09-16 (photo)

William Philpott

REU7691071

US PRESIDENT BUSH URGES PASSING OF CLEAR SKIES, 2003-09-16 (photo)

William Philpott

REU7691071

TOKYO STOCKS TUMBLE TO 5-MONTH LOW, 2002-07-26 (photo)
 
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TOKYO STOCKS TUMBLE TO 5-MONTH LOW, 2002-07-26 (photo)

Kimimasa Mayama

REU7983604

TOKYO STOCKS TUMBLE TO 5-MONTH LOW, 2002-07-26 (photo)

Kimimasa Mayama

REU7983604

HONDA MOTOR UNVEILS NEW MODEL MINICAR "LIFE" IN TOKYO, 2003 (photo)
 
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HONDA MOTOR UNVEILS NEW MODEL MINICAR "LIFE" IN TOKYO, 2003 (photo)

Toshiyuki Aizawa

REU7468406

HONDA MOTOR UNVEILS NEW MODEL MINICAR "LIFE" IN TOKYO, 2003 (photo)

Toshiyuki Aizawa

REU7468406

HONDA MOTOR PRESIDENT AND CEO FUKUI POSES WITH NEW MODEL MINICAR "LIFE" IN TOKYO, 2003-09-04 (photo)
 
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HONDA MOTOR PRESIDENT AND CEO FUKUI POSES WITH NEW MODEL MINICAR "LIFE" IN TOKYO, 2003-09-04 (photo)

Toshiyuki Aizawa

REU7780967

HONDA MOTOR PRESIDENT AND CEO FUKUI POSES WITH NEW MODEL MINICAR "LIFE" IN TOKYO, 2003-09-04 (photo)

Toshiyuki Aizawa

REU7780967

PASSERSBY ARE REFLECTED ON AN STOCK QUOTATION BOARD IN TOKYO, 2003-07-02 (photo)
 
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PASSERSBY ARE REFLECTED ON AN STOCK QUOTATION BOARD IN TOKYO, 2003-07-02 (photo)

Issei Kato

REU7816303

PASSERSBY ARE REFLECTED ON AN STOCK QUOTATION BOARD IN TOKYO, 2003-07-02 (photo)

Issei Kato

REU7816303

HONDA MOTOR PRESIDENT AND CEO FUKUI POSES WITH NEW MODEL MINICAR "LIFE" IN TOKYO, 2003 (photo)
 
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HONDA MOTOR PRESIDENT AND CEO FUKUI POSES WITH NEW MODEL MINICAR "LIFE" IN TOKYO, 2003 (photo)

Toshiyuki Aizawa

REU7468398

HONDA MOTOR PRESIDENT AND CEO FUKUI POSES WITH NEW MODEL MINICAR "LIFE" IN TOKYO, 2003 (photo)

Toshiyuki Aizawa

REU7468398

Trevor Creed, senior vice president of design for Dodge, discusses the Dodge Powerbox SUV at the 200.., 2001 (photo)
 
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Trevor Creed, senior vice president of design for Dodge, discusses the Dodge Powerbox SUV at the 200.., 2001 (photo)

Sam Mircovich

REU7480303

Trevor Creed, senior vice president of design for Dodge, discusses the Dodge Powerbox SUV at the 200.., 2001 (photo)

Sam Mircovich

REU7480303

JAPANESE OLD MAN LOOKS AT STOCK QUOTATION BOARD FLSHING RISE IN SHARE PRICES IN TOKYO, 2003-09-01 (photo)
 
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JAPANESE OLD MAN LOOKS AT STOCK QUOTATION BOARD FLSHING RISE IN SHARE PRICES IN TOKYO, 2003-09-01 (photo)

Toshiyuki Aizawa

REU7781718

JAPANESE OLD MAN LOOKS AT STOCK QUOTATION BOARD FLSHING RISE IN SHARE PRICES IN TOKYO, 2003-09-01 (photo)

Toshiyuki Aizawa

REU7781718

Barree spiral galaxy NGC 1300 in Eridan - Barred spiral galaxy NGC 1300 in Eridanus - The galaxy NGC1300 is located about 60 million years ago - light and extends over about 85 000 years - light. This image was obtained by the Hubble Space Telescope in September 2004. NGC 1300 is considered to be prototypical of barred spiral galaxies. Barred spirals differ from normal spiral galaxies in that the arms of the galaxy do not spiral all the way into the center, but are connected to the two ends of a straight bar of stars containing the nucleus at its center. At Hubble's resolution, a myriad of fine details, some of which have never before been seen, is seen throughout the galaxy's arms, disk, bulge, and nucleus. Blue and red supergiant stars, star clusters, and star - forming regions are well resolved across the spiral arms, and dust lanes trace out fine structures in the disk and bar. Numerous more distant galaxies are visible in the background, and are seen even through the densest regions of NGC 1300. The image was constructed from exposures taken in September 2004 by the Advanced Camera for Surveys onboard Hubble in four filters. Starlight and dust are seen in blue, visible, and infrared light. Bright star clusters are highlighted in red by their associated emission from glowing hydrogen gas. The galaxy lies roughly 69 million light - years away (21 megaparsecs) in the direction of the constellation Eridanus
 
Barree spiral galaxy NGC 1300 in Eridan - Barred spiral galaxy NGC 1300 in Eridanus - The galaxy NGC1300 is located about 60 million years ago - light and extends over about 85 000 years - light. This image was obtained by the Hubble Space Telescope in September 2004. NGC 1300 is considered to be prototypical of barred spiral galaxies. Barred spirals differ from normal spiral galaxies in that the arms of the galaxy do not spiral all the way into the center, but are connected to the two ends of a straight bar of stars containing the nucleus at its center. At Hubble's resolution, a myriad of fine details, some of which have never before been seen, is seen throughout the galaxy's arms, disk, bulge, and nucleus. Blue and red supergiant stars, star clusters, and star - forming regions are well resolved across the spiral arms, and dust lanes trace out fine structures in the disk and bar. Numerous more distant galaxies are visible in the background, and are seen even through the densest regio

PIX4609752

Barree spiral galaxy NGC 1300 in Eridan - Barred spiral galaxy NGC 1300 in Eridanus - The galaxy NGC1300 is located about 60 million years ago - light and extends over about 85 000 years - light. This image was obtained by the Hubble Space Telescope in September 2004. NGC 1300 is considered to be prototypical of barred spiral galaxies. Barred spirals differ from normal spiral galaxies in that the arms of the galaxy do not spiral all the way into the center, but are connected to the two ends of a straight bar of stars containing the nucleus at its center. At Hubble's resolution, a myriad of fine details, some of which have never before been seen, is seen throughout the galaxy's arms, disk, bulge, and nucleus. Blue and red supergiant stars, star clusters, and star - forming regions are well resolved across the spiral arms, and dust lanes trace out fine structures in the disk and bar. Numerous more distant galaxies are visible in the background, and are seen even through the densest regio

PIX4609752

00362888
 
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00362888

IMO2000180

00362888

IMO2000180

TOKYO STOCK EXCHANGE OFFICIALS EXCHANGE BOWS AFTER FINAL CLOSING SESSION, 1998-12-30 (photo)
 
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TOKYO STOCK EXCHANGE OFFICIALS EXCHANGE BOWS AFTER FINAL CLOSING SESSION, 1998-12-30 (photo)

Susumu Toshiyuki

REU8014900

TOKYO STOCK EXCHANGE OFFICIALS EXCHANGE BOWS AFTER FINAL CLOSING SESSION, 1998-12-30 (photo)

Susumu Toshiyuki

REU8014900

JAPANESE OLD MAN LOOKS AT STOCK QUOTATION BOARD FLSHING RISE IN SHARE PRICES IN TOKYO, 2003-09-01 (photo)
 
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JAPANESE OLD MAN LOOKS AT STOCK QUOTATION BOARD FLSHING RISE IN SHARE PRICES IN TOKYO, 2003-09-01 (photo)

Toshiyuki Aizawa

REU7764359

JAPANESE OLD MAN LOOKS AT STOCK QUOTATION BOARD FLSHING RISE IN SHARE PRICES IN TOKYO, 2003-09-01 (photo)

Toshiyuki Aizawa

REU7764359

JAPANESE BUSINESSMEN WALK IN FRONT OF STOCK QUOTATION BOARD FLSHING RISE IN SHARE PRICES IN TOKYO, 2003-09-01 (photo)
 
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JAPANESE BUSINESSMEN WALK IN FRONT OF STOCK QUOTATION BOARD FLSHING RISE IN SHARE PRICES IN TOKYO, 2003-09-01 (photo)

Toshiyuki Aizawa

REU7889199

JAPANESE BUSINESSMEN WALK IN FRONT OF STOCK QUOTATION BOARD FLSHING RISE IN SHARE PRICES IN TOKYO, 2003-09-01 (photo)

Toshiyuki Aizawa

REU7889199

JAPANESE BUSINESSMEN WALK BEFORE STOCK QUOTATION BOARD FLASHING JUMP OF SHARE PRICES IN TOKYO, 2000-10-20 (photo)
 
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JAPANESE BUSINESSMEN WALK BEFORE STOCK QUOTATION BOARD FLASHING JUMP OF SHARE PRICES IN TOKYO, 2000-10-20 (photo)

Toshiyuki Aizawa

REU7914319

JAPANESE BUSINESSMEN WALK BEFORE STOCK QUOTATION BOARD FLASHING JUMP OF SHARE PRICES IN TOKYO, 2000-10-20 (photo)

Toshiyuki Aizawa

REU7914319

NISSAN SENTRA CA OFFERS ULTRA-GREEN CA MODEL IN CALIFORNIA, 2000-01-12 (photo)
 
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NISSAN SENTRA CA OFFERS ULTRA-GREEN CA MODEL IN CALIFORNIA, 2000-01-12 (photo)

Reuters Photographer

REU7974594

NISSAN SENTRA CA OFFERS ULTRA-GREEN CA MODEL IN CALIFORNIA, 2000-01-12 (photo)

Reuters Photographer

REU7974594

SMILING MAN WALKS BY ELECTRONIC STOCK QUOTATION BOARD IN TOKYO, 2003-07-08 (photo)
 
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SMILING MAN WALKS BY ELECTRONIC STOCK QUOTATION BOARD IN TOKYO, 2003-07-08 (photo)

Haruyoshi Yamaguchi

REU7831427

SMILING MAN WALKS BY ELECTRONIC STOCK QUOTATION BOARD IN TOKYO, 2003-07-08 (photo)

Haruyoshi Yamaguchi

REU7831427

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