1. Home
  2. All Artists
  4. All Assets

Assets (798986 in total)

Search options

Orientation
Colour

Display options

View

Print

To print search results, use print friendly version of this page.

Results

Pierre de Coubertin, c.1930s (b/w photo)
Pierre de Coubertin, c.1930s (b/w photo)

DGC3106966: Pierre de Coubertin, c.1930s (b/w photo) / Bridgeman Images

ID: DGC3106966

Pierre de Coubertin, c.1930s (b/w photo)

E.Sharp and son's Toffee advert featuring rememberance poppy, c.1942 (litho)
E.Sharp and son's Toffee advert featuring rememberance poppy, c.1942 (litho)

DGC3113899: E.Sharp and son's Toffee advert featuring rememberance poppy, c.1942 (litho) / Bridgeman Images

ID: DGC3113899

E.Sharp and son's Toffee advert featuring rememberance poppy, c.1942 (litho)

Biology and pregnancy: amniotic pocket containing the human embryo (then fetus) at the second week of fecondation (photo)
Biology and pregnancy: amniotic pocket containing the human embryo (then fetus) at the second week of fecondation (photo)

LRI4672569: Biology and pregnancy: amniotic pocket containing the human embryo (then fetus) at the second week of fecondation (photo) / Bridgeman Images

ID: LRI4672569

Biology and pregnancy: amniotic pocket containing the human embryo (then fetus) at the second week of fecondation (photo)

Detroit d'Ormuz - 02/2011 - Strait of Hormuz - 02/2011 - Detroit d'Ormuz seen by Envisat satellite on February 4, 2011. The south - eastern parts of Iran (top) and the Arabian Peninsula are featured in this image, acquired by Envisat's Medium Resolution Imaging Spectrometer on 4 February 2011. The closest point between the two Middle Eastern countries is the Strait of Hormuz (centre), which links the Persian Gulf (left) with the Gulf of Oman (upper right) and the Arabian Sea (lower right). Several countries are visible on the peninsula: the United Arab Emirates (top left), Oman (tip and bottom right) and Saudi Arabia (far left and bottom)
Detroit d'Ormuz - 02/2011 - Strait of Hormuz - 02/2011 - Detroit d'Ormuz seen by Envisat satellite on February 4, 2011. The south - eastern parts of Iran (top) and the Arabian Peninsula are featured in this image, acquired by Envisat's Medium Resolution Imaging Spectrometer on 4 February 2011. The closest point between the two Middle Eastern countries is the Strait of Hormuz (centre), which links the Persian Gulf (left) with the Gulf of Oman (upper right) and the Arabian Sea (lower right). Several countries are visible on the peninsula: the United Arab Emirates (top left), Oman (tip and bottom right) and Saudi Arabia (far left and bottom)

PIX4660195: Detroit d'Ormuz - 02/2011 - Strait of Hormuz - 02/2011 - Detroit d'Ormuz seen by Envisat satellite on February 4, 2011. The south - eastern parts of Iran (top) and the Arabian Peninsula are featured in this image, acquired by Envisat's Medium Resolution Imaging Spectrometer on 4 February 2011. The closest point between the two Middle Eastern countries is the Strait of Hormuz (centre), which links the Persian Gulf (left) with the Gulf of Oman (upper right) and the Arabian Sea (lower right). Several countries are visible on the peninsula: the United Arab Emirates (top left), Oman (tip and bottom right) and Saudi Arabia (far left and bottom) / Bridgeman Images

ID: PIX4660195

Detroit d'Ormuz - 02/2011 - Strait of Hormuz - 02/2011 - Detroit d'Ormuz seen by Envisat satellite on February 4, 2011. The south - eastern parts of Iran (top) and the Arabian Peninsula are featured in this image, acquired by Envisat's Medium Resolution Imaging Spectrometer on 4 February 2011. The closest point between the two Middle Eastern countries is the Strait of Hormuz (centre), which links the Persian Gulf (left) with the Gulf of Oman (upper right) and the Arabian Sea (lower right). Several countries are visible on the peninsula: the United Arab Emirates (top left), Oman (tip and bottom right) and Saudi Arabia (far left and bottom)

Ichthyosaurus - Ichthyosaurus (fish body lezard) is a marine reptile living from the early Jurassic in Lower Cretace. Ichthyosaurus is an extinct genus of ichthyosaur from the Early Jurassic
Ichthyosaurus - Ichthyosaurus (fish body lezard) is a marine reptile living from the early Jurassic in Lower Cretace. Ichthyosaurus is an extinct genus of ichthyosaur from the Early Jurassic

PIX4662175: Ichthyosaurus - Ichthyosaurus (fish body lezard) is a marine reptile living from the early Jurassic in Lower Cretace. Ichthyosaurus is an extinct genus of ichthyosaur from the Early Jurassic / Bridgeman Images

ID: PIX4662175

Ichthyosaurus - Ichthyosaurus (fish body lezard) is a marine reptile living from the early Jurassic in Lower Cretace. Ichthyosaurus is an extinct genus of ichthyosaur from the Early Jurassic

Laguna Cejar - Atacama Desert - Chile - Cejar Lagoon - Chile: The lake path and the clouds of Magellan are reflected in the salt water of Laguna Cejar. August 2014. Salar of Atacama's Cejar Lagoon and the Milky Way
Laguna Cejar - Atacama Desert - Chile - Cejar Lagoon - Chile: The lake path and the clouds of Magellan are reflected in the salt water of Laguna Cejar. August 2014. Salar of Atacama's Cejar Lagoon and the Milky Way

PIX4676123: Laguna Cejar - Atacama Desert - Chile - Cejar Lagoon - Chile: The lake path and the clouds of Magellan are reflected in the salt water of Laguna Cejar. August 2014. Salar of Atacama's Cejar Lagoon and the Milky Way / Bridgeman Images

ID: PIX4676123

Laguna Cejar - Atacama Desert - Chile - Cejar Lagoon - Chile: The lake path and the clouds of Magellan are reflected in the salt water of Laguna Cejar. August 2014. Salar of Atacama's Cejar Lagoon and the Milky Way

Anchiornis huxleyi - Anchiornis huxleyi is a small dinosaur of the troodontid family dating from mid-Jurassic (160 to 155 Million years). A pre-archaeopteryx troodontid theropod from China with long feathers on the metatarsus
Anchiornis huxleyi - Anchiornis huxleyi is a small dinosaur of the troodontid family dating from mid-Jurassic (160 to 155 Million years). A pre-archaeopteryx troodontid theropod from China with long feathers on the metatarsus

PIX4662183: Anchiornis huxleyi - Anchiornis huxleyi is a small dinosaur of the troodontid family dating from mid-Jurassic (160 to 155 Million years). A pre-archaeopteryx troodontid theropod from China with long feathers on the metatarsus / Bridgeman Images

ID: PIX4662183

Anchiornis huxleyi - Anchiornis huxleyi is a small dinosaur of the troodontid family dating from mid-Jurassic (160 to 155 Million years). A pre-archaeopteryx troodontid theropod from China with long feathers on the metatarsus

Thirty Years' War (1618-1648): double page of the Treaty of Westphalia signed on 24/10/1648, 1648
Thirty Years' War (1618-1648): double page of the Treaty of Westphalia signed on 24/10/1648, 1648

JLJ4682761: Thirty Years' War (1618-1648): double page of the Treaty of Westphalia signed on 24/10/1648, 1648 / Bridgeman Images

ID: JLJ4682761

Thirty Years' War (1618-1648): double page of the Treaty of Westphalia signed on 24/10/1648, 1648

LHC: Installation of the ATLAS calorimeter - LHC: Installing the ATLAS calorimeter - Central view of the ATLAS detector with its eight toroid magnets surrounding the calorimeter before it is moved to the center of the detector. The calorimeter measures the energy of the particles produced during the collision between the protons in the center of the detector. The eight toroid magnets can be seen surrounding the calorimeter that is later moved into the middle of the detector. This calorimeter will measure the energies of particles produced when protons collide in the centre of the detector
LHC: Installation of the ATLAS calorimeter - LHC: Installing the ATLAS calorimeter - Central view of the ATLAS detector with its eight toroid magnets surrounding the calorimeter before it is moved to the center of the detector. The calorimeter measures the energy of the particles produced during the collision between the protons in the center of the detector. The eight toroid magnets can be seen surrounding the calorimeter that is later moved into the middle of the detector. This calorimeter will measure the energies of particles produced when protons collide in the centre of the detector

PIX4650532: LHC: Installation of the ATLAS calorimeter - LHC: Installing the ATLAS calorimeter - Central view of the ATLAS detector with its eight toroid magnets surrounding the calorimeter before it is moved to the center of the detector. The calorimeter measures the energy of the particles produced during the collision between the protons in the center of the detector. The eight toroid magnets can be seen surrounding the calorimeter that is later moved into the middle of the detector. This calorimeter will measure the energies of particles produced when protons collide in the centre of the detector / Bridgeman Images

ID: PIX4650532

LHC: Installation of the ATLAS calorimeter - LHC: Installing the ATLAS calorimeter - Central view of the ATLAS detector with its eight toroid magnets surrounding the calorimeter before it is moved to the center of the detector. The calorimeter measures the energy of the particles produced during the collision between the protons in the center of the detector. The eight toroid magnets can be seen surrounding the calorimeter that is later moved into the middle of the detector. This calorimeter will measure the energies of particles produced when protons collide in the centre of the detector

A ring of rocks and dust is orbiting the Earth. The massive continent below is Pangee and the ocean to the west is Panthalassa. This is what Earth was supposed to look like at the end of Permian, about 260 million years ago, before the first dinosaurs appeared. This ring around the Earth was of earthly origin, constitutes debris thrown into orbit by collision with a meteorite or comet. Over time, these debris have fallen or fallen to Earth in a meteorite rain - A dusty ring arc orbits four thousand miles above Earth's equator. The massive continent below is Pangea and the ocean to the west is Panthalassa. This is how the Earth may have appeared during the end of the Permian period, a time just prior to the appearance of the dinosaurs, when continental drift was pulling Pangea apart into the seven continents we know today - 260 million years ago the Earth may have been host to ring arcs similar to the incomplete rings that currently circumscribe the planet Neptune . Unlike Neptune's rings, the ring arcs around the Earth were of terrestrial origin, debris thrown into orbit by a collision with a large meteorite or comet. The debris consisted of tiny pebbles that were once molten droplets of ejecta, long since cooled in the vacuum of space. The orbit of the ring arc would eventually decay, returning the debris back to Earth as a shower of meteorites. This debris is found on Earth's surface today in the form of dark, glassy objects known as tektites.: La Terre à la fin du Permien - Ring arcs over the Permian Earth
A ring of rocks and dust is orbiting the Earth. The massive continent below is Pangee and the ocean to the west is Panthalassa. This is what Earth was supposed to look like at the end of Permian, about 260 million years ago, before the first dinosaurs appeared. This ring around the Earth was of earthly origin, constitutes debris thrown into orbit by collision with a meteorite or comet. Over time, these debris have fallen or fallen to Earth in a meteorite rain - A dusty ring arc orbits four thousand miles above Earth's equator. The massive continent below is Pangea and the ocean to the west is Panthalassa. This is how the Earth may have appeared during the end of the Permian period, a time just prior to the appearance of the dinosaurs, when continental drift was pulling Pangea apart into the seven continents we know today - 260 million years ago the Earth may have been host to ring arcs similar to the incomplete rings that currently circumscribe the planet Neptune . Unlike Neptune's rings, the ring arcs around the Earth were of terrestrial origin, debris thrown into orbit by a collision with a large meteorite or comet. The debris consisted of tiny pebbles that were once molten droplets of ejecta, long since cooled in the vacuum of space. The orbit of the ring arc would eventually decay, returning the debris back to Earth as a shower of meteorites. This debris is found on Earth's surface today in the form of dark, glassy objects known as tektites.: La Terre à la fin du Permien - Ring arcs over the Permian Earth

PIX4669572: A ring of rocks and dust is orbiting the Earth. The massive continent below is Pangee and the ocean to the west is Panthalassa. This is what Earth was supposed to look like at the end of Permian, about 260 million years ago, before the first dinosaurs appeared. This ring around the Earth was of earthly origin, constitutes debris thrown into orbit by collision with a meteorite or comet. Over time, these debris have fallen or fallen to Earth in a meteorite rain - A dusty ring arc orbits four thousand miles above Earth's equator. The massive continent below is Pangea and the ocean to the west is Panthalassa. This is how the Earth may have appeared during the end of the Permian period, a time just prior to the appearance of the dinosaurs, when continental drift was pulling Pangea apart into the seven continents we know today - 260 million years ago the Earth may have been host to ring arcs similar to the incomplete rings that currently circumscribe the planet Neptune . Unlike Neptune's rings, the ring arcs around the Earth were of terrestrial origin, debris thrown into orbit by a collision with a large meteorite or comet. The debris consisted of tiny pebbles that were once molten droplets of ejecta, long since cooled in the vacuum of space. The orbit of the ring arc would eventually decay, returning the debris back to Earth as a shower of meteorites. This debris is found on Earth's surface today in the form of dark, glassy objects known as tektites.: La Terre à la fin du Permien - Ring arcs over the Permian Earth / Bridgeman Images

ID: PIX4669572

A ring of rocks and dust is orbiting the Earth. The massive continent below is Pangee and the ocean to the west is Panthalassa. This is what Earth was supposed to look like at the end of Permian, about 260 million years ago, before the first dinosaurs appeared. This ring around the Earth was of earthly origin, constitutes debris thrown into orbit by collision with a meteorite or comet. Over time, these debris have fallen or fallen to Earth in a meteorite rain - A dusty ring arc orbits four thousand miles above Earth's equator. The massive continent below is Pangea and the ocean to the west is Panthalassa. This is how the Earth may have appeared during the end of the Permian period, a time just prior to the appearance of the dinosaurs, when continental drift was pulling Pangea apart into the seven continents we know today - 260 million years ago the Earth may have been host to ring arcs similar to the incomplete rings that currently circumscribe the planet Neptune . Unlike Neptune's rin

Aurora boreale - Finland - Aurora borealis in Finland - Aurora boreale observed in Lapland (Finland). Aurora borealis seen in Lapland (Finland)
Aurora boreale - Finland - Aurora borealis in Finland - Aurora boreale observed in Lapland (Finland). Aurora borealis seen in Lapland (Finland)

PIX4670380: Aurora boreale - Finland - Aurora borealis in Finland - Aurora boreale observed in Lapland (Finland). Aurora borealis seen in Lapland (Finland) / Bridgeman Images

ID: PIX4670380

Aurora boreale - Finland - Aurora borealis in Finland - Aurora boreale observed in Lapland (Finland). Aurora borealis seen in Lapland (Finland)

Circumpolar above the dome of the 1.93 m of the Observatory of Haute - Provence - Haute - Provence Observatory, the 1.93 m telescope dome - Photographic pose showing the apparent rotation of stars around the polar star (circumpolar). Below, the dome of the 1.93 m telescope of the Observatory of Haute Provence. This is where the first exoplanet was discovered in 1995. The Observatory of Haute-Provence is located in the south-east of France, near the village of St. Michel l'Observatoire, a hundred kilometers north of Marseille, on a plateau with an average altitude of 650 meters. Long exposure image of starry sky around the pole star (circumpolar). Below, the 1.93 m telescope dome. Here has been discovered the first extrasolar planet (51 Peg b) in 1995. OHP is situated in the southeast of France, it lies at an altitude of about 650 m, near the village of Saint-Michel l'Observatoire
Circumpolar above the dome of the 1.93 m of the Observatory of Haute - Provence - Haute - Provence Observatory, the 1.93 m telescope dome - Photographic pose showing the apparent rotation of stars around the polar star (circumpolar). Below, the dome of the 1.93 m telescope of the Observatory of Haute Provence. This is where the first exoplanet was discovered in 1995. The Observatory of Haute-Provence is located in the south-east of France, near the village of St. Michel l'Observatoire, a hundred kilometers north of Marseille, on a plateau with an average altitude of 650 meters. Long exposure image of starry sky around the pole star (circumpolar). Below, the 1.93 m telescope dome. Here has been discovered the first extrasolar planet (51 Peg b) in 1995. OHP is situated in the southeast of France, it lies at an altitude of about 650 m, near the village of Saint-Michel l'Observatoire

PIX4655293: Circumpolar above the dome of the 1.93 m of the Observatory of Haute - Provence - Haute - Provence Observatory, the 1.93 m telescope dome - Photographic pose showing the apparent rotation of stars around the polar star (circumpolar). Below, the dome of the 1.93 m telescope of the Observatory of Haute Provence. This is where the first exoplanet was discovered in 1995. The Observatory of Haute-Provence is located in the south-east of France, near the village of St. Michel l'Observatoire, a hundred kilometers north of Marseille, on a plateau with an average altitude of 650 meters. Long exposure image of starry sky around the pole star (circumpolar). Below, the 1.93 m telescope dome. Here has been discovered the first extrasolar planet (51 Peg b) in 1995. OHP is situated in the southeast of France, it lies at an altitude of about 650 m, near the village of Saint-Michel l'Observatoire / Bridgeman Images

ID: PIX4655293

Circumpolar above the dome of the 1.93 m of the Observatory of Haute - Provence - Haute - Provence Observatory, the 1.93 m telescope dome - Photographic pose showing the apparent rotation of stars around the polar star (circumpolar). Below, the dome of the 1.93 m telescope of the Observatory of Haute Provence. This is where the first exoplanet was discovered in 1995. The Observatory of Haute-Provence is located in the south-east of France, near the village of St. Michel l'Observatoire, a hundred kilometers north of Marseille, on a plateau with an average altitude of 650 meters. Long exposure image of starry sky around the pole star (circumpolar). Below, the 1.93 m telescope dome. Here has been discovered the first extrasolar planet (51 Peg b) in 1995. OHP is situated in the southeast of France, it lies at an altitude of about 650 m, near the village of Saint-Michel l'Observatoire

Sun and sunspots, the 27/10/2003 - Sun with sunspots - Le Soleil vu le 27 October 2003. Two giant sunspots are visible. Two giant sunspots, easily visible to the unaided eye with proper filtration, are visible in this color image taken on October 27, 2003
Sun and sunspots, the 27/10/2003 - Sun with sunspots - Le Soleil vu le 27 October 2003. Two giant sunspots are visible. Two giant sunspots, easily visible to the unaided eye with proper filtration, are visible in this color image taken on October 27, 2003

PIX4626631: Sun and sunspots, the 27/10/2003 - Sun with sunspots - Le Soleil vu le 27 October 2003. Two giant sunspots are visible. Two giant sunspots, easily visible to the unaided eye with proper filtration, are visible in this color image taken on October 27, 2003 / Bridgeman Images

ID: PIX4626631

Sun and sunspots, the 27/10/2003 - Sun with sunspots - Le Soleil vu le 27 October 2003. Two giant sunspots are visible. Two giant sunspots, easily visible to the unaided eye with proper filtration, are visible in this color image taken on October 27, 2003

The sinking of the USS Merrimac, 2 June 1898, during the Spanish–American War.
The sinking of the USS Merrimac, 2 June 1898, during the Spanish–American War.

KWE3116262: The sinking of the USS Merrimac, 2 June 1898, during the Spanish–American War. / Bridgeman Images

ID: KWE3116262

The sinking of the USS Merrimac, 2 June 1898, during the Spanish–American War.

American naval bombardment of Santiago de Cuba's harbour defences July 2, 1898 during the Spanish-American War.
American naval bombardment of Santiago de Cuba's harbour defences July 2, 1898 during the Spanish-American War.

KWE3116341: American naval bombardment of Santiago de Cuba's harbour defences July 2, 1898 during the Spanish-American War. / Bridgeman Images

ID: KWE3116341

American naval bombardment of Santiago de Cuba's harbour defences July 2, 1898 during the Spanish-American War.

Making the Titanic's anchor chain at Hingley & Sons, c.1909 (photo)
Making the Titanic's anchor chain at Hingley & Sons, c.1909 (photo)

DGC3088181: Making the Titanic's anchor chain at Hingley & Sons, c.1909 (photo) / Bridgeman Images

ID: DGC3088181

Making the Titanic's anchor chain at Hingley & Sons, c.1909 (photo)

Second World War (1939-1945): Stohlberg (Germany) September 1944: The city is three-quarter in the hands of the 1st US Army. Treve evacuates civilians
Second World War (1939-1945): Stohlberg (Germany) September 1944: The city is three-quarter in the hands of the 1st US Army. Treve evacuates civilians

ETE4881705: Second World War (1939-1945): Stohlberg (Germany) September 1944: The city is three-quarter in the hands of the 1st US Army. Treve evacuates civilians / Bridgeman Images

ID: ETE4881705

Second World War (1939-1945): Stohlberg (Germany) September 1944: The city is three-quarter in the hands of the 1st US Army. Treve evacuates civilians

Second World War (1939-1945): two inhabitants of Brest (Brittany) in front of the ruins of their house after the liberation of the city on 20 September 1944. Photograph of the same day.
Second World War (1939-1945): two inhabitants of Brest (Brittany) in front of the ruins of their house after the liberation of the city on 20 September 1944. Photograph of the same day.

ETE4842306: Second World War (1939-1945): two inhabitants of Brest (Brittany) in front of the ruins of their house after the liberation of the city on 20 September 1944. Photograph of the same day. / Bridgeman Images

ID: ETE4842306

Second World War (1939-1945): two inhabitants of Brest (Brittany) in front of the ruins of their house after the liberation of the city on 20 September 1944. Photograph of the same day.

Statue of Maimonides in Cordoba, Andalusia, Spain
Statue of Maimonides in Cordoba, Andalusia, Spain

GNG4989467: Statue of Maimonides in Cordoba, Andalusia, Spain / Bridgeman Images

ID: GNG4989467

Statue of Maimonides in Cordoba, Andalusia, Spain

WWII:Lorient (France) May 10, 1945: Poche de Lorient (France) May 10, 1945: After the surrender of German General Fahrmbacher (Commander of the German Forces of La Poche), the garrison was assembled under the custody of the soldiers of the 25th French DI of General Chomel
WWII:Lorient (France) May 10, 1945: Poche de Lorient (France) May 10, 1945: After the surrender of German General Fahrmbacher (Commander of the German Forces of La Poche), the garrison was assembled under the custody of the soldiers of the 25th French DI of General Chomel

ETE4931822: WWII:Lorient (France) May 10, 1945: Poche de Lorient (France) May 10, 1945: After the surrender of German General Fahrmbacher (Commander of the German Forces of La Poche), the garrison was assembled under the custody of the soldiers of the 25th French DI of General Chomel / Bridgeman Images

ID: ETE4931822

WWII:Lorient (France) May 10, 1945: Poche de Lorient (France) May 10, 1945: After the surrender of German General Fahrmbacher (Commander of the German Forces of La Poche), the garrison was assembled under the custody of the soldiers of the 25th French DI of General Chomel

Second World War (1939-1945): aerian view of the ship terminal in ruins on the port of Cherbourg after its liberation by the troops of the 7th US Corps. Photography 27 June 1944.
Second World War (1939-1945): aerian view of the ship terminal in ruins on the port of Cherbourg after its liberation by the troops of the 7th US Corps. Photography 27 June 1944.

ETE4849086: Second World War (1939-1945): aerian view of the ship terminal in ruins on the port of Cherbourg after its liberation by the troops of the 7th US Corps. Photography 27 June 1944. / Bridgeman Images

ID: ETE4849086

Second World War (1939-1945): aerian view of the ship terminal in ruins on the port of Cherbourg after its liberation by the troops of the 7th US Corps. Photography 27 June 1944.

WWII:Near Aachen (Aachen) Germany around September 16, 1944: A Sherman M4 tank of the 5th DB US crosses the dragon teeth of the Siegried line
WWII:Near Aachen (Aachen) Germany around September 16, 1944: A Sherman M4 tank of the 5th DB US crosses the dragon teeth of the Siegried line

ETE4888636: WWII:Near Aachen (Aachen) Germany around September 16, 1944: A Sherman M4 tank of the 5th DB US crosses the dragon teeth of the Siegried line / Bridgeman Images

ID: ETE4888636

WWII:Near Aachen (Aachen) Germany around September 16, 1944: A Sherman M4 tank of the 5th DB US crosses the dragon teeth of the Siegried line

Lakshman temple in Rishikesh : Nara simha (man lion), 4th incarnation of Vishnu
Lakshman temple in Rishikesh : Nara simha (man lion), 4th incarnation of Vishnu

GNG5281095: Lakshman temple in Rishikesh : Nara simha (man lion), 4th incarnation of Vishnu / Bridgeman Images

ID: GNG5281095

Lakshman temple in Rishikesh : Nara simha (man lion), 4th incarnation of Vishnu

WWII:Ulm (Germany) at the end of May 1945: Young boys and teenagers rebuild their school (Keppler Mittelschule) destroyed by Allied bombing
WWII:Ulm (Germany) at the end of May 1945: Young boys and teenagers rebuild their school (Keppler Mittelschule) destroyed by Allied bombing

ETE4930452: WWII:Ulm (Germany) at the end of May 1945: Young boys and teenagers rebuild their school (Keppler Mittelschule) destroyed by Allied bombing / Bridgeman Images

ID: ETE4930452

WWII:Ulm (Germany) at the end of May 1945: Young boys and teenagers rebuild their school (Keppler Mittelschule) destroyed by Allied bombing

20151022, Abu Dhabi, United Arab Emirates : Sheikh Zayed Grand Mosque, Abu Dhabi. Veiled woman. Veiled woman
20151022, Abu Dhabi, United Arab Emirates : Sheikh Zayed Grand Mosque, Abu Dhabi. Veiled woman. Veiled woman

GNG5246869: 20151022, Abu Dhabi, United Arab Emirates : Sheikh Zayed Grand Mosque, Abu Dhabi. Veiled woman. Veiled woman / Bridgeman Images

ID: GNG5246869

20151022, Abu Dhabi, United Arab Emirates : Sheikh Zayed Grand Mosque, Abu Dhabi. Veiled woman. Veiled woman

WWII - Battle of the Bulge (WWII): A 57 mm anti-tank gun served by soldiers of the 83rd DI of the 1st US Army monitors a snow corridor between two fir forests on the road halfway between Houffalize and Saint Vith (Saint Vith) - Photograph taken in Bovigny (Belgium), January 21, 1945
WWII - Battle of the Bulge (WWII): A 57 mm anti-tank gun served by soldiers of the 83rd DI of the 1st US Army monitors a snow corridor between two fir forests on the road halfway between Houffalize and Saint Vith (Saint Vith) - Photograph taken in Bovigny (Belgium), January 21, 1945

ETE4865502: WWII - Battle of the Bulge (WWII): A 57 mm anti-tank gun served by soldiers of the 83rd DI of the 1st US Army monitors a snow corridor between two fir forests on the road halfway between Houffalize and Saint Vith (Saint Vith) - Photograph taken in Bovigny (Belgium), January 21, 1945 / Bridgeman Images

ID: ETE4865502

WWII - Battle of the Bulge (WWII): A 57 mm anti-tank gun served by soldiers of the 83rd DI of the 1st US Army monitors a snow corridor between two fir forests on the road halfway between Houffalize and Saint Vith (Saint Vith) - Photograph taken in Bovigny (Belgium), January 21, 1945

WWII:Near Cologne (Germany) beginning March 1945: On the road to the Rhenan city, this Sherman M4 of the 3rd DB US has just been hit by enemy artillery
WWII:Near Cologne (Germany) beginning March 1945: On the road to the Rhenan city, this Sherman M4 of the 3rd DB US has just been hit by enemy artillery

ETE4914079: WWII:Near Cologne (Germany) beginning March 1945: On the road to the Rhenan city, this Sherman M4 of the 3rd DB US has just been hit by enemy artillery / Bridgeman Images

ID: ETE4914079

WWII:Near Cologne (Germany) beginning March 1945: On the road to the Rhenan city, this Sherman M4 of the 3rd DB US has just been hit by enemy artillery

Sign has poetic joust. Iran, Isfahan, mid-17th century. Ceramic, decor of black lines. Louvre Museum
Sign has poetic joust. Iran, Isfahan, mid-17th century. Ceramic, decor of black lines. Louvre Museum

SYC4193783: Sign has poetic joust. Iran, Isfahan, mid-17th century. Ceramic, decor of black lines. Louvre Museum / Bridgeman Images

ID: SYC4193783

Sign has poetic joust. Iran, Isfahan, mid-17th century. Ceramic, decor of black lines. Louvre Museum

Russian soldiers loading ammunition
Russian soldiers loading ammunition

XLF3788880: Russian soldiers loading ammunition / Bridgeman Images

ID: XLF3788880

Russian soldiers loading ammunition

Mauna Kea Observatory. Radiotelescopes - Radiotelescopes at Mauna Kea Observatory - View of the Mauna Kea Observatory located 4200 metres above sea level in Hawaii, USA. Here, the radiotelescopes with in the foreground the CSO (Caltech Submillimeter Observatory), then the JCMT (James Clerk Maxwell Telescope) and the SMA antenna network (Sub - Millimeter Array). Foreground is CSO (Caltech Submillimeter Observatory), then, JCMT (James Clerk Maxwell Telescope) and background is the antennas network SMA (Sub - Millimeter Array)
Mauna Kea Observatory. Radiotelescopes - Radiotelescopes at Mauna Kea Observatory - View of the Mauna Kea Observatory located 4200 metres above sea level in Hawaii, USA. Here, the radiotelescopes with in the foreground the CSO (Caltech Submillimeter Observatory), then the JCMT (James Clerk Maxwell Telescope) and the SMA antenna network (Sub - Millimeter Array). Foreground is CSO (Caltech Submillimeter Observatory), then, JCMT (James Clerk Maxwell Telescope) and background is the antennas network SMA (Sub - Millimeter Array)

PIX4655209: Mauna Kea Observatory. Radiotelescopes - Radiotelescopes at Mauna Kea Observatory - View of the Mauna Kea Observatory located 4200 metres above sea level in Hawaii, USA. Here, the radiotelescopes with in the foreground the CSO (Caltech Submillimeter Observatory), then the JCMT (James Clerk Maxwell Telescope) and the SMA antenna network (Sub - Millimeter Array). Foreground is CSO (Caltech Submillimeter Observatory), then, JCMT (James Clerk Maxwell Telescope) and background is the antennas network SMA (Sub - Millimeter Array) / Bridgeman Images

ID: PIX4655209

Mauna Kea Observatory. Radiotelescopes - Radiotelescopes at Mauna Kea Observatory - View of the Mauna Kea Observatory located 4200 metres above sea level in Hawaii, USA. Here, the radiotelescopes with in the foreground the CSO (Caltech Submillimeter Observatory), then the JCMT (James Clerk Maxwell Telescope) and the SMA antenna network (Sub - Millimeter Array). Foreground is CSO (Caltech Submillimeter Observatory), then, JCMT (James Clerk Maxwell Telescope) and background is the antennas network SMA (Sub - Millimeter Array)

Artist View of a Galactic Black Hole
Artist View of a Galactic Black Hole

PIX4584461: Artist View of a Galactic Black Hole / Bridgeman Images

ID: PIX4584461

Artist View of a Galactic Black Hole

Saturn - Illustration - Saturn - Illustration - Artist's view of the planet Saturn. The ring system is composed from the closest to Saturn to the furthest by ring D, then C, B, the division of Cassini, A with the division of Encke, F, G and E. The brightest part of the rings is ring B. This image suggests how Saturn might look from high above the ring plane and at a right angle to the Sun, a perspective that we could never get from the Earth nor from the Hubble Space Telescope
Saturn - Illustration - Saturn - Illustration - Artist's view of the planet Saturn. The ring system is composed from the closest to Saturn to the furthest by ring D, then C, B, the division of Cassini, A with the division of Encke, F, G and E. The brightest part of the rings is ring B. This image suggests how Saturn might look from high above the ring plane and at a right angle to the Sun, a perspective that we could never get from the Earth nor from the Hubble Space Telescope

PIX4625712: Saturn - Illustration - Saturn - Illustration - Artist's view of the planet Saturn. The ring system is composed from the closest to Saturn to the furthest by ring D, then C, B, the division of Cassini, A with the division of Encke, F, G and E. The brightest part of the rings is ring B. This image suggests how Saturn might look from high above the ring plane and at a right angle to the Sun, a perspective that we could never get from the Earth nor from the Hubble Space Telescope / Bridgeman Images

ID: PIX4625712

Saturn - Illustration - Saturn - Illustration - Artist's view of the planet Saturn. The ring system is composed from the closest to Saturn to the furthest by ring D, then C, B, the division of Cassini, A with the division of Encke, F, G and E. The brightest part of the rings is ring B. This image suggests how Saturn might look from high above the ring plane and at a right angle to the Sun, a perspective that we could never get from the Earth nor from the Hubble Space Telescope

Mars Express probe - Artist's View - Mars Express artist's view - The European probe Mars Express leaves the Earth propelled by the upper floor Fregat. This probe was launched on 2 June 2003 and began its observations in early 2004. Mars Express left Earth for Mars on 2 June 2003 when the positions of the two planets made for the shortest possible route, a condition that occurs once every twenty - six months. The european spaceprobe began its March observations in 2004. Mars Express was mounted on the Fregat upper stage. Most of the energy needed to propel Mars Express from Earth to Mars is provided by the four - stage Soyuz/Fregat launcher. The Fregat upper stage separated from the spacecraft after placed it on a Mars - bound trajectory
Mars Express probe - Artist's View - Mars Express artist's view - The European probe Mars Express leaves the Earth propelled by the upper floor Fregat. This probe was launched on 2 June 2003 and began its observations in early 2004. Mars Express left Earth for Mars on 2 June 2003 when the positions of the two planets made for the shortest possible route, a condition that occurs once every twenty - six months. The european spaceprobe began its March observations in 2004. Mars Express was mounted on the Fregat upper stage. Most of the energy needed to propel Mars Express from Earth to Mars is provided by the four - stage Soyuz/Fregat launcher. The Fregat upper stage separated from the spacecraft after placed it on a Mars - bound trajectory

PIX4606628: Mars Express probe - Artist's View - Mars Express artist's view - The European probe Mars Express leaves the Earth propelled by the upper floor Fregat. This probe was launched on 2 June 2003 and began its observations in early 2004. Mars Express left Earth for Mars on 2 June 2003 when the positions of the two planets made for the shortest possible route, a condition that occurs once every twenty - six months. The european spaceprobe began its March observations in 2004. Mars Express was mounted on the Fregat upper stage. Most of the energy needed to propel Mars Express from Earth to Mars is provided by the four - stage Soyuz/Fregat launcher. The Fregat upper stage separated from the spacecraft after placed it on a Mars - bound trajectory / Bridgeman Images

ID: PIX4606628

Mars Express probe - Artist's View - Mars Express artist's view - The European probe Mars Express leaves the Earth propelled by the upper floor Fregat. This probe was launched on 2 June 2003 and began its observations in early 2004. Mars Express left Earth for Mars on 2 June 2003 when the positions of the two planets made for the shortest possible route, a condition that occurs once every twenty - six months. The european spaceprobe began its March observations in 2004. Mars Express was mounted on the Fregat upper stage. Most of the energy needed to propel Mars Express from Earth to Mars is provided by the four - stage Soyuz/Fregat launcher. The Fregat upper stage separated from the spacecraft after placed it on a Mars - bound trajectory

Europe at night - 2016 - Europe by night - 2016 - View of Europe at night consisting of images taken by the Suomi NPP satellite in 2016. This image of Europe at night is a composite assembled from data acquired by the Suomi NPP satellite in 2016.
Europe at night - 2016 - Europe by night - 2016 - View of Europe at night consisting of images taken by the Suomi NPP satellite in 2016. This image of Europe at night is a composite assembled from data acquired by the Suomi NPP satellite in 2016.

PIX4667181: Europe at night - 2016 - Europe by night - 2016 - View of Europe at night consisting of images taken by the Suomi NPP satellite in 2016. This image of Europe at night is a composite assembled from data acquired by the Suomi NPP satellite in 2016. / Bridgeman Images

ID: PIX4667181

Europe at night - 2016 - Europe by night - 2016 - View of Europe at night consisting of images taken by the Suomi NPP satellite in 2016. This image of Europe at night is a composite assembled from data acquired by the Suomi NPP satellite in 2016.

Pious image: Our Lady of the Rosary, early 20th century (notched card)
Pious image: Our Lady of the Rosary, early 20th century (notched card)

LRI4628954: Pious image: Our Lady of the Rosary, early 20th century (notched card) / Bridgeman Images

ID: LRI4628954

Pious image: Our Lady of the Rosary, early 20th century (notched card)

Aerial view of Pentagon (1988 - Photography)
Aerial view of Pentagon (1988 - Photography)

LRI4597991: Aerial view of Pentagon (1988 - Photography) / Bridgeman Images

ID: LRI4597991

Aerial view of Pentagon (1988 - Photography)


Back to top