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Mars - Hellas Basin - Mosaic of images obtained by the Viking probe 1. To the north, the large clear circular region is Arabia. Below, the white spot represents the Hellas Basin, an impact crater of 2000 km in diameter and 6 km deep covered with carbon dioxide gele
Mars - Hellas Basin - Mosaic of images obtained by the Viking probe 1. To the north, the large clear circular region is Arabia. Below, the white spot represents the Hellas Basin, an impact crater of 2000 km in diameter and 6 km deep covered with carbon dioxide gele

PIX4615133: Mars - Hellas Basin - Mosaic of images obtained by the Viking probe 1. To the north, the large clear circular region is Arabia. Below, the white spot represents the Hellas Basin, an impact crater of 2000 km in diameter and 6 km deep covered with carbon dioxide gele / Bridgeman Images

Mars - Dust Tempete - These two images show the same view of Mars before and during a dust storm. Images obtained by the Mars Global Surveyor probe on 10 June 2001 on the left and on 31 July 2001 on the right
Mars - Dust Tempete - These two images show the same view of Mars before and during a dust storm. Images obtained by the Mars Global Surveyor probe on 10 June 2001 on the left and on 31 July 2001 on the right

PIX4615244: Mars - Dust Tempete - These two images show the same view of Mars before and during a dust storm. Images obtained by the Mars Global Surveyor probe on 10 June 2001 on the left and on 31 July 2001 on the right / Bridgeman Images

Labour Exchange in Paris. Construction 1890.
Labour Exchange in Paris. Construction 1890.

TEC4615345: Labour Exchange in Paris. Construction 1890. / Bridgeman Images

Untitled, 1912 (Watercolour)
Untitled, 1912 (Watercolour)

LRI4615401: Untitled, 1912 (Watercolour), Haussmann, Raoul (1886-1970) / Bridgeman Images

March - Spirit - Panorama - Husband Hill - Panorama of 360 degres consists of 243 images obtained by Spirit from November 24 to December 2, 2004. The hill in the center left of the image is Husband Hill. The Rover Spirit landed on Mars in the Gusev crater area, July 4, 2004
March - Spirit - Panorama - Husband Hill - Panorama of 360 degres consists of 243 images obtained by Spirit from November 24 to December 2, 2004. The hill in the center left of the image is Husband Hill. The Rover Spirit landed on Mars in the Gusev crater area, July 4, 2004

PIX4615615: March - Spirit - Panorama - Husband Hill - Panorama of 360 degres consists of 243 images obtained by Spirit from November 24 to December 2, 2004. The hill in the center left of the image is Husband Hill. The Rover Spirit landed on Mars in the Gusev crater area, July 4, 2004 / Bridgeman Images

Pointed Silence, 1933 (Tempera on paper)
Pointed Silence, 1933 (Tempera on paper)

LRI4615653: Pointed Silence, 1933 (Tempera on paper), Kandinsky, Wassily (1866-1944) / Bridgeman Images

The moon during the totality of the lunar eclipse of 27 October, 2004: Eclipse totale de Lune. 27/10/2004 - Total lunar eclipse. October 27 2004
The moon during the totality of the lunar eclipse of 27 October, 2004: Eclipse totale de Lune. 27/10/2004 - Total lunar eclipse. October 27 2004

PIX4614683: The moon during the totality of the lunar eclipse of 27 October, 2004: Eclipse totale de Lune. 27/10/2004 - Total lunar eclipse. October 27 2004 / Bridgeman Images

Square Alban Satragne in Paris 10th.
Square Alban Satragne in Paris 10th.

TEC4614864: Square Alban Satragne in Paris 10th. / Bridgeman Images

Wall painting in Paris 10th. Photography 10/06/99.
Wall painting in Paris 10th. Photography 10/06/99.

TEC4614908: Wall painting in Paris 10th. Photography 10/06/99. / Bridgeman Images

Fluxkit, 1965-1966 (Assemblage with small black case)
Fluxkit, 1965-1966 (Assemblage with small black case)

LRI4614930: Fluxkit, 1965-1966 (Assemblage with small black case), Fluxus (International contemporary art community) / Bridgeman Images

Porte Saint Denis in Paris 10th. Construction 1672, architect Francois Blondel (1618-1686).
Porte Saint Denis in Paris 10th. Construction 1672, architect Francois Blondel (1618-1686).

TEC4614991: Porte Saint Denis in Paris 10th. Construction 1672, architect Francois Blondel (1618-1686). / Bridgeman Images

Porte Saint Denis in Paris 10th. Construction 1672, architect Francois Blondel (1618-1686).
Porte Saint Denis in Paris 10th. Construction 1672, architect Francois Blondel (1618-1686).

TEC4614996: Porte Saint Denis in Paris 10th. Construction 1672, architect Francois Blondel (1618-1686). / Bridgeman Images

Mars - Olympus Mons Volcano - False colors - Altimetric data obtained by the Mars Global Surveyor probe in 2000. The Olympus Mons volcano is 600 km in diameter and 27 km high
Mars - Olympus Mons Volcano - False colors - Altimetric data obtained by the Mars Global Surveyor probe in 2000. The Olympus Mons volcano is 600 km in diameter and 27 km high

PIX4615442: Mars - Olympus Mons Volcano - False colors - Altimetric data obtained by the Mars Global Surveyor probe in 2000. The Olympus Mons volcano is 600 km in diameter and 27 km high / Bridgeman Images

The Canal Saint Martin in Paris 10th. Inaugurated in 1825, the Saint-Martinae Canal connects the Villette basin to the Seine. It has 9 locks and 2 turntables. Photography 2005.
The Canal Saint Martin in Paris 10th. Inaugurated in 1825, the Saint-Martinae Canal connects the Villette basin to the Seine. It has 9 locks and 2 turntables. Photography 2005.

TEC4615495: The Canal Saint Martin in Paris 10th. Inaugurated in 1825, the Saint-Martinae Canal connects the Villette basin to the Seine. It has 9 locks and 2 turntables. Photography 2005. / Bridgeman Images

Canal Saint Martin in Paris 10th. Inaugurated in 1825, the Saint Martin Canal connects the basin of the Villette with the Seine. It has 9 locks and 2 turntables. Photograph 2005.
Canal Saint Martin in Paris 10th. Inaugurated in 1825, the Saint Martin Canal connects the basin of the Villette with the Seine. It has 9 locks and 2 turntables. Photograph 2005.

TEC4615504: Canal Saint Martin in Paris 10th. Inaugurated in 1825, the Saint Martin Canal connects the basin of the Villette with the Seine. It has 9 locks and 2 turntables. Photograph 2005. / Bridgeman Images

Quai de Valmy, Paris 10th. Photography 2005.
Quai de Valmy, Paris 10th. Photography 2005.

TEC4615526: Quai de Valmy, Paris 10th. Photography 2005. / Bridgeman Images

Detail of the 1st color panorama of the Martian soil obtained by Spirit. The Rover Spirit landed on Mars in the area of the crater Gusev, July 4, 2004 - Detail of the first panorama taken by Spirit.: Surface de Mars: detail of the first panorama obtained by Spirit - The martian surface seen by Spirit. 07/2004
Detail of the 1st color panorama of the Martian soil obtained by Spirit. The Rover Spirit landed on Mars in the area of the crater Gusev, July 4, 2004 - Detail of the first panorama taken by Spirit.: Surface de Mars: detail of the first panorama obtained by Spirit - The martian surface seen by Spirit. 07/2004

PIX4615535: Detail of the 1st color panorama of the Martian soil obtained by Spirit. The Rover Spirit landed on Mars in the area of the crater Gusev, July 4, 2004 - Detail of the first panorama taken by Spirit.: Surface de Mars: detail of the first panorama obtained by Spirit - The martian surface seen by Spirit. 07/2004 / Bridgeman Images

A cafe on the Quai de Valmy in Paris 10th.
A cafe on the Quai de Valmy in Paris 10th.

TEC4615590: A cafe on the Quai de Valmy in Paris 10th. / Bridgeman Images

A Velib station, avenue de Verdun, in Paris 10th. Photography 18/08/07.
A Velib station, avenue de Verdun, in Paris 10th. Photography 18/08/07.

TEC4615621: A Velib station, avenue de Verdun, in Paris 10th. Photography 18/08/07. / Bridgeman Images

A bicycle path, boulevard Magenta in Paris 10th. Photography 18/08/07.
A bicycle path, boulevard Magenta in Paris 10th. Photography 18/08/07.

TEC4615681: A bicycle path, boulevard Magenta in Paris 10th. Photography 18/08/07. / Bridgeman Images

March - Spirit - View during the descent of Husband Hill - Detail of the 360 degres panorama obtained by Spirit from 23 to 28 November 2005. The summit of Husband Hill is 100m above the surrounding plateau. The Rover Spirit landed on Mars in the Gusev crater area, July 4, 2004
March - Spirit - View during the descent of Husband Hill - Detail of the 360 degres panorama obtained by Spirit from 23 to 28 November 2005. The summit of Husband Hill is 100m above the surrounding plateau. The Rover Spirit landed on Mars in the Gusev crater area, July 4, 2004

PIX4615689: March - Spirit - View during the descent of Husband Hill - Detail of the 360 degres panorama obtained by Spirit from 23 to 28 November 2005. The summit of Husband Hill is 100m above the surrounding plateau. The Rover Spirit landed on Mars in the Gusev crater area, July 4, 2004 / Bridgeman Images

Pont sur le quai Valmy in Paris 10th.
Pont sur le quai Valmy in Paris 10th.

TEC4615779: Pont sur le quai Valmy in Paris 10th. / Bridgeman Images

March - Opportunity - Cratere Victoria 09 - 2006 - March: Victoria crater seen from rover Opportunity - Panorama obtained by the rover Opportunity on 28 and 29 September 2006. The Rover Opportunity landed on Mars in the Meridiani Planum region on January 25, 2004. Opportunity reached the Victoria crater on September 27, 2006 after travelling more than 9 km on the surface of Mars. The Victoria crater is about 800 metres wide and its south face on the left is about 6 metres above ground. This image taken by the panoramic camera on the Mars Exploration Rover Opportunity shows the view of Victoria Crater from Duck Bay. Opportunity reached Victoria Crater on Sol 951 (September 27, 2006) after traversing 9.28 kilometers (5.77 miles) since her landing site at Eagle Crater. Victoria Crater is roughly 800 meters (one - half mile) wide - - about five times wider than Endurance Crater, and 40 times as wide as Eagle crater. The south face of the 6 meter (20 foot) tall layered Cape Verde promontory can be seen in the left side of the inner crater wall, about 50 meters (about 165 feet) away from the rover at the time of the imaging. The north face of the 15 meter (50 foot) tall stack of layered rocks called Cabo Frio can be seen on the right side of the inner crater wall. This mosaic was taken on Sols 952 and 953 (September 28 and 29, 2006). There are 30 separate pointings through 6 different filters at each pointing
March - Opportunity - Cratere Victoria 09 - 2006 - March: Victoria crater seen from rover Opportunity - Panorama obtained by the rover Opportunity on 28 and 29 September 2006. The Rover Opportunity landed on Mars in the Meridiani Planum region on January 25, 2004. Opportunity reached the Victoria crater on September 27, 2006 after travelling more than 9 km on the surface of Mars. The Victoria crater is about 800 metres wide and its south face on the left is about 6 metres above ground. This image taken by the panoramic camera on the Mars Exploration Rover Opportunity shows the view of Victoria Crater from Duck Bay. Opportunity reached Victoria Crater on Sol 951 (September 27, 2006) after traversing 9.28 kilometers (5.77 miles) since her landing site at Eagle Crater. Victoria Crater is roughly 800 meters (one - half mile) wide - - about five times wider than Endurance Crater, and 40 times as wide as Eagle crater. The south face of the 6 meter (20 foot) tall layered Cape Verde promontory can be seen in the left side of the inner crater wall, about 50 meters (about 165 feet) away from the rover at the time of the imaging. The north face of the 15 meter (50 foot) tall stack of layered rocks called Cabo Frio can be seen on the right side of the inner crater wall. This mosaic was taken on Sols 952 and 953 (September 28 and 29, 2006). There are 30 separate pointings through 6 different filters at each pointing

PIX4615845: March - Opportunity - Cratere Victoria 09 - 2006 - March: Victoria crater seen from rover Opportunity - Panorama obtained by the rover Opportunity on 28 and 29 September 2006. The Rover Opportunity landed on Mars in the Meridiani Planum region on January 25, 2004. Opportunity reached the Victoria crater on September 27, 2006 after travelling more than 9 km on the surface of Mars. The Victoria crater is about 800 metres wide and its south face on the left is about 6 metres above ground. This image taken by the panoramic camera on the Mars Exploration Rover Opportunity shows the view of Victoria Crater from Duck Bay. Opportunity reached Victoria Crater on Sol 951 (September 27, 2006) after traversing 9.28 kilometers (5.77 miles) since her landing site at Eagle Crater. Victoria Crater is roughly 800 meters (one - half mile) wide - - about five times wider than Endurance Crater, and 40 times as wide as Eagle crater. The south face of the 6 meter (20 foot) tall layered Cape Verde promontory can be seen in the left side of the inner crater wall, about 50 meters (about 165 feet) away from the rover at the time of the imaging. The north face of the 15 meter (50 foot) tall stack of layered rocks called Cabo Frio can be seen on the right side of the inner crater wall. This mosaic was taken on Sols 952 and 953 (September 28 and 29, 2006). There are 30 separate pointings through 6 different filters at each pointing / Bridgeman Images

Rue Albert Thomas in Paris 10th photograph 10/05/02.
Rue Albert Thomas in Paris 10th photograph 10/05/02.

TEC4615129: Rue Albert Thomas in Paris 10th photograph 10/05/02. / Bridgeman Images

Mars: panorama of Chryse Planitia by Viking 1 - Mars: Chryse Planitia panorama by Viking 1 - Panorama of the surface of Mars obtained by the probe Viking 1 on 23 July 1976. The big rock on the left, nicknamed Big Joe, is about three metres long. Panoramic image of Chryse Planitia taken by camera 1 on the Viking 1 Lander. The image was taken on 23 July 1976, three days after Viking 1 landed. The dark rock at the left of the frame, nicknamed “” Big Joe”””, is about 3 meters across and 8 meters from the lander
Mars: panorama of Chryse Planitia by Viking 1 - Mars: Chryse Planitia panorama by Viking 1 - Panorama of the surface of Mars obtained by the probe Viking 1 on 23 July 1976. The big rock on the left, nicknamed Big Joe, is about three metres long. Panoramic image of Chryse Planitia taken by camera 1 on the Viking 1 Lander. The image was taken on 23 July 1976, three days after Viking 1 landed. The dark rock at the left of the frame, nicknamed “” Big Joe”””, is about 3 meters across and 8 meters from the lander

PIX4615194: Mars: panorama of Chryse Planitia by Viking 1 - Mars: Chryse Planitia panorama by Viking 1 - Panorama of the surface of Mars obtained by the probe Viking 1 on 23 July 1976. The big rock on the left, nicknamed Big Joe, is about three metres long. Panoramic image of Chryse Planitia taken by camera 1 on the Viking 1 Lander. The image was taken on 23 July 1976, three days after Viking 1 landed. The dark rock at the left of the frame, nicknamed “” Big Joe”””, is about 3 meters across and 8 meters from the lander / Bridgeman Images

Mars: dunes and ice in Chasma Boreale - Mars: dunes and ice in Chasma Boreale - Chasma Boreale is a huge canyon located in the northern polar cap of Mars. This image, obtained by the Mars Express probe, shows Tenuis Cavus, the end of this canyon, where layers of water ice mix with Mars dust. At the bottom of the bowl there are numerous sand dunes. Chasma Boreale is a huge canyon in the northern polar cap. The images taken by Mars Express spacecraft show sharp detail of a series of scarps at the head of Chasma Boreale, a giant trough that almost divides the north polar ice cap in two. The trough is about 318 kilometers long and has cliffs that are almost two kilometers high. The images show layers of water ice and dust possibly for the first time in perspective view. Chasma Boreale is cut into the layered material that lies beneath the water ice of the polar cap. For decades, these layered materials were assumed to consist of a mixture of ice and dust. Recent observations could mean that some of the layers are a source for windblown sand. The floor of the trough and the caldera - like structures are covered by dark sand dunes. This dark material could be volcanic ash or it is possible that it is dark sand eroding out of the polar layered materials. These pictures were taken in mid - summer, a time when the dark sand dunes on the trough floor were still partially covered by a white frost left over from the winter season. The frost is most definitely frozen water, rather than carbon dioxide, because the temperatures even in spring are too high for solid carbon dioxide to be present. This frost is not likely to defrost much beyond this extent. The shapes of the dunes indicate transport in a direction parallel to the chasma incision. The main wind direction is not clear at present but likely to be north - east to south - west, parallel to the chasma walls
Mars: dunes and ice in Chasma Boreale - Mars: dunes and ice in Chasma Boreale - Chasma Boreale is a huge canyon located in the northern polar cap of Mars. This image, obtained by the Mars Express probe, shows Tenuis Cavus, the end of this canyon, where layers of water ice mix with Mars dust. At the bottom of the bowl there are numerous sand dunes. Chasma Boreale is a huge canyon in the northern polar cap. The images taken by Mars Express spacecraft show sharp detail of a series of scarps at the head of Chasma Boreale, a giant trough that almost divides the north polar ice cap in two. The trough is about 318 kilometers long and has cliffs that are almost two kilometers high. The images show layers of water ice and dust possibly for the first time in perspective view. Chasma Boreale is cut into the layered material that lies beneath the water ice of the polar cap. For decades, these layered materials were assumed to consist of a mixture of ice and dust. Recent observations could mean that some of the layers are a source for windblown sand. The floor of the trough and the caldera - like structures are covered by dark sand dunes. This dark material could be volcanic ash or it is possible that it is dark sand eroding out of the polar layered materials. These pictures were taken in mid - summer, a time when the dark sand dunes on the trough floor were still partially covered by a white frost left over from the winter season. The frost is most definitely frozen water, rather than carbon dioxide, because the temperatures even in spring are too high for solid carbon dioxide to be present. This frost is not likely to defrost much beyond this extent. The shapes of the dunes indicate transport in a direction parallel to the chasma incision. The main wind direction is not clear at present but likely to be north - east to south - west, parallel to the chasma walls

PIX4615964: Mars: dunes and ice in Chasma Boreale - Mars: dunes and ice in Chasma Boreale - Chasma Boreale is a huge canyon located in the northern polar cap of Mars. This image, obtained by the Mars Express probe, shows Tenuis Cavus, the end of this canyon, where layers of water ice mix with Mars dust. At the bottom of the bowl there are numerous sand dunes. Chasma Boreale is a huge canyon in the northern polar cap. The images taken by Mars Express spacecraft show sharp detail of a series of scarps at the head of Chasma Boreale, a giant trough that almost divides the north polar ice cap in two. The trough is about 318 kilometers long and has cliffs that are almost two kilometers high. The images show layers of water ice and dust possibly for the first time in perspective view. Chasma Boreale is cut into the layered material that lies beneath the water ice of the polar cap. For decades, these layered materials were assumed to consist of a mixture of ice and dust. Recent observations could mean that some of the layers are a source for windblown sand. The floor of the trough and the caldera - like structures are covered by dark sand dunes. This dark material could be volcanic ash or it is possible that it is dark sand eroding out of the polar layered materials. These pictures were taken in mid - summer, a time when the dark sand dunes on the trough floor were still partially covered by a white frost left over from the winter season. The frost is most definitely frozen water, rather than carbon dioxide, because the temperatures even in spring are too high for solid carbon dioxide to be present. This frost is not likely to defrost much beyond this extent. The shapes of the dunes indicate transport in a direction parallel to the chasma incision. The main wind direction is not clear at present but likely to be north - east to south - west, parallel to the chasma walls / Bridgeman Images

Coprates Chasma - This image shows a detail of Valles Marineris, Coprates Chasma. Image obtained by the Mars Global Surveyor probe
Coprates Chasma - This image shows a detail of Valles Marineris, Coprates Chasma. Image obtained by the Mars Global Surveyor probe

PIX4615270: Coprates Chasma - This image shows a detail of Valles Marineris, Coprates Chasma. Image obtained by the Mars Global Surveyor probe / Bridgeman Images

Melisenda, 1971 (collage, painting)
Melisenda, 1971 (collage, painting)

LRI4612860: Melisenda, 1971 (collage, painting), Baj, Enrico (1924-2003) / Bridgeman Images

Large Magellanic Cloud galaxy - Large Magellanic Cloud galaxy - The galaxy of the Great Magellan Cloud is about 160,000 light years away from Earth in the southern constellation of Dorado. Visible with the naked eye in the southern hemishere it is one of the closest galaxies to ours. Mosaic of 10 images, 30 hours of poses. The irregular galaxy Large Magellanic Cloud (LMC) is located at a distance of 160,000 light years in the southern constellation of Dorado. It is one of the nearest galaxy, visible to naked eye. 10 frame mosaic image, 30 hours of exposure
Large Magellanic Cloud galaxy - Large Magellanic Cloud galaxy - The galaxy of the Great Magellan Cloud is about 160,000 light years away from Earth in the southern constellation of Dorado. Visible with the naked eye in the southern hemishere it is one of the closest galaxies to ours. Mosaic of 10 images, 30 hours of poses. The irregular galaxy Large Magellanic Cloud (LMC) is located at a distance of 160,000 light years in the southern constellation of Dorado. It is one of the nearest galaxy, visible to naked eye. 10 frame mosaic image, 30 hours of exposure

PIX4613538: Large Magellanic Cloud galaxy - Large Magellanic Cloud galaxy - The galaxy of the Great Magellan Cloud is about 160,000 light years away from Earth in the southern constellation of Dorado. Visible with the naked eye in the southern hemishere it is one of the closest galaxies to ours. Mosaic of 10 images, 30 hours of poses. The irregular galaxy Large Magellanic Cloud (LMC) is located at a distance of 160,000 light years in the southern constellation of Dorado. It is one of the nearest galaxy, visible to naked eye. 10 frame mosaic image, 30 hours of exposure / Bridgeman Images

The mosquee Adda'wa in Paris.
The mosquee Adda'wa in Paris.

TEC4613615: The mosquee Adda'wa in Paris. / Bridgeman Images

Spiral galaxy NGC 6946 in Cephee - Spiral galaxy NGC 6946 in Cepheus - Spiral galaxy NGC 6946 located about 10 million years ago - light in Cephee. NGC 6946 is a nearby spiral galaxy, located at 10 million light years from us
Spiral galaxy NGC 6946 in Cephee - Spiral galaxy NGC 6946 in Cepheus - Spiral galaxy NGC 6946 located about 10 million years ago - light in Cephee. NGC 6946 is a nearby spiral galaxy, located at 10 million light years from us

PIX4613059: Spiral galaxy NGC 6946 in Cephee - Spiral galaxy NGC 6946 in Cepheus - Spiral galaxy NGC 6946 located about 10 million years ago - light in Cephee. NGC 6946 is a nearby spiral galaxy, located at 10 million light years from us / Bridgeman Images

Spiral galaxy NGC 7331 in Pegase - Spiral galaxy NGC 7331 in Pegasus - The galaxy NGC 7331 is located about 50 million years away - light from Earth. The small galaxies around them form a cluster much farther away. Image obtained with a 50 cm telescope, composite of several images. NGC 7331 is located 49 million light years away. The smaller galaxies visible are much farer
Spiral galaxy NGC 7331 in Pegase - Spiral galaxy NGC 7331 in Pegasus - The galaxy NGC 7331 is located about 50 million years away - light from Earth. The small galaxies around them form a cluster much farther away. Image obtained with a 50 cm telescope, composite of several images. NGC 7331 is located 49 million light years away. The smaller galaxies visible are much farer

PIX4613118: Spiral galaxy NGC 7331 in Pegase - Spiral galaxy NGC 7331 in Pegasus - The galaxy NGC 7331 is located about 50 million years away - light from Earth. The small galaxies around them form a cluster much farther away. Image obtained with a 50 cm telescope, composite of several images. NGC 7331 is located 49 million light years away. The smaller galaxies visible are much farer / Bridgeman Images

House through the trees. 1895-1900. (Watercolour)
House through the trees. 1895-1900. (Watercolour)

LRI4614072: House through the trees. 1895-1900. (Watercolour), Cezanne, Paul (1839-1906) / Bridgeman Images

House building, Quai de Seine in Paris 19th. Detached house on 4 levels, built on a residue of land between 2 gables. Architects Olivier Fassio and Jean Brice Viaud, construction 2002. Photography 2005.
House building, Quai de Seine in Paris 19th. Detached house on 4 levels, built on a residue of land between 2 gables. Architects Olivier Fassio and Jean Brice Viaud, construction 2002. Photography 2005.

LBY4614109: House building, Quai de Seine in Paris 19th. Detached house on 4 levels, built on a residue of land between 2 gables. Architects Olivier Fassio and Jean Brice Viaud, construction 2002. Photography 2005. / Bridgeman Images

Social housing tour, Place des fetes, in Paris in the 19th arrondissement. Photography 09/12/07.
Social housing tour, Place des fetes, in Paris in the 19th arrondissement. Photography 09/12/07.

LBY4614152: Social housing tour, Place des fetes, in Paris in the 19th arrondissement. Photography 09/12/07. / Bridgeman Images

Social housing tour, place des fetes, in Paris in the 19th arrondissement. Photography 09/12/07.
Social housing tour, place des fetes, in Paris in the 19th arrondissement. Photography 09/12/07.

LBY4614176: Social housing tour, place des fetes, in Paris in the 19th arrondissement. Photography 09/12/07. / Bridgeman Images


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