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The interurban road station of Brasilia (Brazil). Architect Lucio Costa, 1960. Photography 2007.
The interurban road station of Brasilia (Brazil). Architect Lucio Costa, 1960. Photography 2007.

TEC4629462: The interurban road station of Brasilia (Brazil). Architect Lucio Costa, 1960. Photography 2007. / Bridgeman Images

ID: TEC4629462

The interurban road station of Brasilia (Brazil). Architect Lucio Costa, 1960. Photography 2007.

The interurban road station of Brasilia (Brazil). Architect Lucio Costa, 1960. Photography 2007.
The interurban road station of Brasilia (Brazil). Architect Lucio Costa, 1960. Photography 2007.

TEC4629478: The interurban road station of Brasilia (Brazil). Architect Lucio Costa, 1960. Photography 2007. / Bridgeman Images

ID: TEC4629478

The interurban road station of Brasilia (Brazil). Architect Lucio Costa, 1960. Photography 2007.

Saint Anthony of Padua known as the Thaumaturge (print)
Saint Anthony of Padua known as the Thaumaturge (print)

LRI4629496: Saint Anthony of Padua known as the Thaumaturge (print), Anonymous / Bridgeman Images

ID: LRI4629496

Saint Anthony of Padua known as the Thaumaturge (print)

Anonymous

The interurban road station of Brasilia (Brazil). Architect Lucio Costa, 1960. Photography 2007.
The interurban road station of Brasilia (Brazil). Architect Lucio Costa, 1960. Photography 2007.

TEC4629517: The interurban road station of Brasilia (Brazil). Architect Lucio Costa, 1960. Photography 2007. / Bridgeman Images

ID: TEC4629517

The interurban road station of Brasilia (Brazil). Architect Lucio Costa, 1960. Photography 2007.

The dwarf planet Eris and its satellite Dysnomie - The dwarf planet Eris and its satellite Dysnomie seen by the Hubble space telescope on August 30, 2006
The dwarf planet Eris and its satellite Dysnomie - The dwarf planet Eris and its satellite Dysnomie seen by the Hubble space telescope on August 30, 2006

PIX4629533: The dwarf planet Eris and its satellite Dysnomie - The dwarf planet Eris and its satellite Dysnomie seen by the Hubble space telescope on August 30, 2006 / Bridgeman Images

ID: PIX4629533

The dwarf planet Eris and its satellite Dysnomie - The dwarf planet Eris and its satellite Dysnomie seen by the Hubble space telescope on August 30, 2006

Night Eve in Paris, First World War (stereoscopic glass plate)
Night Eve in Paris, First World War (stereoscopic glass plate)

JLJ4629653: Night Eve in Paris, First World War (stereoscopic glass plate), Anonymous / Bridgeman Images

ID: JLJ4629653

Night Eve in Paris, First World War (stereoscopic glass plate)

Anonymous

To offer your heart to Mary, of what virtues you adorn it, are you sweet, modest, charitable. 19th century (print)
To offer your heart to Mary, of what virtues you adorn it, are you sweet, modest, charitable. 19th century (print)

LRI4629760: To offer your heart to Mary, of what virtues you adorn it, are you sweet, modest, charitable. 19th century (print), Anonymous / Bridgeman Images

ID: LRI4629760

To offer your heart to Mary, of what virtues you adorn it, are you sweet, modest, charitable. 19th century (print)

Anonymous

Terre et Mars: comparison of sizes - Terre et Mars: comparison of sizes - Photomontag
Terre et Mars: comparison of sizes - Terre et Mars: comparison of sizes - Photomontag

PIX4629784: Terre et Mars: comparison of sizes - Terre et Mars: comparison of sizes - Photomontag / Bridgeman Images

ID: PIX4629784

Terre et Mars: comparison of sizes - Terre et Mars: comparison of sizes - Photomontag

Earth and Mars - Earth and Mars - Artist's view of Earth and Mars. The diameter of the planet Mars is half the diameter of the Earth. Artwork showing the Earth and Mars (in foreground). Mars' diameter is half that of the Earth's
Earth and Mars - Earth and Mars - Artist's view of Earth and Mars. The diameter of the planet Mars is half the diameter of the Earth. Artwork showing the Earth and Mars (in foreground). Mars' diameter is half that of the Earth's

PIX4629805: Earth and Mars - Earth and Mars - Artist's view of Earth and Mars. The diameter of the planet Mars is half the diameter of the Earth. Artwork showing the Earth and Mars (in foreground). Mars' diameter is half that of the Earth's / Bridgeman Images

ID: PIX4629805

Earth and Mars - Earth and Mars - Artist's view of Earth and Mars. The diameter of the planet Mars is half the diameter of the Earth. Artwork showing the Earth and Mars (in foreground). Mars' diameter is half that of the Earth's

Saint Desideratus. 19th century (engraving)
Saint Desideratus. 19th century (engraving)

LRI4629831: Saint Desideratus. 19th century (engraving), Anonymous / Bridgeman Images

ID: LRI4629831

Saint Desideratus. 19th century (engraving)

Anonymous

Saint Luke 19th century (engraving)
Saint Luke 19th century (engraving)

LRI4629909: Saint Luke 19th century (engraving), Anonymous / Bridgeman Images

ID: LRI4629909

Saint Luke 19th century (engraving)

Anonymous

Illustration from the book
Illustration from the book

JLJ4625458: Illustration from the book "Le bon roy Henri" (litho), Job, pseudonym for Onfray de Breville, Jacques (1858-1931) / Bridgeman Images

ID: JLJ4625458

Illustration from the book "Le bon roy Henri" (litho)

Job, pseudonym for Onfray de Breville, Jacques (1858-1931)

Enceladus, satellite of Saturn, seen by Cassini - Enceladus, satellite of Saturn, seen by Cassini - Mosaic of 16 images obtained by the Cassini probe during the flight over this satellite on 17 February 2005. The image shows the hemisphere of Enceladus center on Sarandib Planitia
Enceladus, satellite of Saturn, seen by Cassini - Enceladus, satellite of Saturn, seen by Cassini - Mosaic of 16 images obtained by the Cassini probe during the flight over this satellite on 17 February 2005. The image shows the hemisphere of Enceladus center on Sarandib Planitia

PIX4625492: Enceladus, satellite of Saturn, seen by Cassini - Enceladus, satellite of Saturn, seen by Cassini - Mosaic of 16 images obtained by the Cassini probe during the flight over this satellite on 17 February 2005. The image shows the hemisphere of Enceladus center on Sarandib Planitia / Bridgeman Images

ID: PIX4625492

Enceladus, satellite of Saturn, seen by Cassini - Enceladus, satellite of Saturn, seen by Cassini - Mosaic of 16 images obtained by the Cassini probe during the flight over this satellite on 17 February 2005. The image shows the hemisphere of Enceladus center on Sarandib Planitia

The site of the Musee des Monuments Francais, Cite de l'architecture et du patrimoine, Palais de Chaillot, 1 place du Trocadero, Paris 16th. All the renovation and renovation works were entrusted to the architect Jean Francois Bodin, at the end of 2007. Photography 2003.
The site of the Musee des Monuments Francais, Cite de l'architecture et du patrimoine, Palais de Chaillot, 1 place du Trocadero, Paris 16th. All the renovation and renovation works were entrusted to the architect Jean Francois Bodin, at the end of 2007. Photography 2003.

JSN4625505: The site of the Musee des Monuments Francais, Cite de l'architecture et du patrimoine, Palais de Chaillot, 1 place du Trocadero, Paris 16th. All the renovation and renovation works were entrusted to the architect Jean Francois Bodin, at the end of 2007. Photography 2003., Salmon, Jacqueline / Bridgeman Images

ID: JSN4625505

The site of the Musee des Monuments Francais, Cite de l'architecture et du patrimoine, Palais de Chaillot, 1 place du Trocadero, Paris 16th. All the renovation and renovation works were entrusted to the architect Jean Francois Bodin, at the end of 2007. Photography 2003.

Salmon, Jacqueline

The site of the Musee des Monuments Francais, Cite de l'architecture et du patrimoine, Palais de Chaillot, 1 place du Trocadero, Paris 16th. All the renovation and renovation works were entrusted to the architect Jean Francois Bodin, at the end of 2007. Photography 2003.
The site of the Musee des Monuments Francais, Cite de l'architecture et du patrimoine, Palais de Chaillot, 1 place du Trocadero, Paris 16th. All the renovation and renovation works were entrusted to the architect Jean Francois Bodin, at the end of 2007. Photography 2003.

JSN4625522: The site of the Musee des Monuments Francais, Cite de l'architecture et du patrimoine, Palais de Chaillot, 1 place du Trocadero, Paris 16th. All the renovation and renovation works were entrusted to the architect Jean Francois Bodin, at the end of 2007. Photography 2003., Salmon, Jacqueline / Bridgeman Images

ID: JSN4625522

The site of the Musee des Monuments Francais, Cite de l'architecture et du patrimoine, Palais de Chaillot, 1 place du Trocadero, Paris 16th. All the renovation and renovation works were entrusted to the architect Jean Francois Bodin, at the end of 2007. Photography 2003.

Salmon, Jacqueline

Illustration from the book
Illustration from the book

JLJ4625547: Illustration from the book "Le bon roy Henri": Henri IV (litho), Job, pseudonym for Onfray de Breville, Jacques (1858-1931) / Bridgeman Images

ID: JLJ4625547

Illustration from the book "Le bon roy Henri": Henri IV (litho)

Job, pseudonym for Onfray de Breville, Jacques (1858-1931)

Mimas, satellite of Saturn, seen by the Cassini probe on 13/02/2010 - Saturn's moon Mimas seen by Cassini spacecraft - February 13 2010 - The Mimas satellite photographed by the Cassini probe on 13 February 2010 has a distance of 16,000 km from the satellite. Mimas is about 400 km in diameter. In the centre left, the large impact crater Herschel, 130 km wide. Relatively dark regions below bright crater walls and streaks on some of the walls are seen in this mosaic of Saturn's moon Mimas, created from images taken by Nasa's Cassini spacecraft during its closest flyby of the moon. The crater floors and surroundings are about 20 percent darker than the steep crater walls in this view. Mimas 'original surface, like the surfaces of most of the other major Saturnian moons without atmospheres, is not pure ice but contains some dark impurities. The relatively dark markings appear along the lower portion of the walls of Herschel Crater (130 kilometers, 80 miles wide) and some of the smaller craters and are marked in green in the annotated version of the image. Cassini scientists interpret this darkening as evidence for the gradual concentration of impurities from evaporating icy materials in areas where the dark impurities slide slowly down the crater wall. There, the bright ice is baked away by the sun and the vacuum of space. At Herschel, the edge where the darker regions contact the crater floor is interrupted by an extensive hummocky area. Scientists believe the hummocky texture came from the flow of melted ice that occurred during the impact that created the crater. That melt filled the bottom of the crater around the central peak. Dark streaks are seen making their way down the sides of some craters and often originated from pockets of dark contaminants embedded just below the rim of the crater wall. The pockets themselves likely represent small, pre - existing, dark - floored craters that were buried by the blanket of material thrown out from the newer im
Mimas, satellite of Saturn, seen by the Cassini probe on 13/02/2010 - Saturn's moon Mimas seen by Cassini spacecraft - February 13 2010 - The Mimas satellite photographed by the Cassini probe on 13 February 2010 has a distance of 16,000 km from the satellite. Mimas is about 400 km in diameter. In the centre left, the large impact crater Herschel, 130 km wide. Relatively dark regions below bright crater walls and streaks on some of the walls are seen in this mosaic of Saturn's moon Mimas, created from images taken by Nasa's Cassini spacecraft during its closest flyby of the moon. The crater floors and surroundings are about 20 percent darker than the steep crater walls in this view. Mimas 'original surface, like the surfaces of most of the other major Saturnian moons without atmospheres, is not pure ice but contains some dark impurities. The relatively dark markings appear along the lower portion of the walls of Herschel Crater (130 kilometers, 80 miles wide) and some of the smaller craters and are marked in green in the annotated version of the image. Cassini scientists interpret this darkening as evidence for the gradual concentration of impurities from evaporating icy materials in areas where the dark impurities slide slowly down the crater wall. There, the bright ice is baked away by the sun and the vacuum of space. At Herschel, the edge where the darker regions contact the crater floor is interrupted by an extensive hummocky area. Scientists believe the hummocky texture came from the flow of melted ice that occurred during the impact that created the crater. That melt filled the bottom of the crater around the central peak. Dark streaks are seen making their way down the sides of some craters and often originated from pockets of dark contaminants embedded just below the rim of the crater wall. The pockets themselves likely represent small, pre - existing, dark - floored craters that were buried by the blanket of material thrown out from the newer im

PIX4625578: Mimas, satellite of Saturn, seen by the Cassini probe on 13/02/2010 - Saturn's moon Mimas seen by Cassini spacecraft - February 13 2010 - The Mimas satellite photographed by the Cassini probe on 13 February 2010 has a distance of 16,000 km from the satellite. Mimas is about 400 km in diameter. In the centre left, the large impact crater Herschel, 130 km wide. Relatively dark regions below bright crater walls and streaks on some of the walls are seen in this mosaic of Saturn's moon Mimas, created from images taken by Nasa's Cassini spacecraft during its closest flyby of the moon. The crater floors and surroundings are about 20 percent darker than the steep crater walls in this view. Mimas 'original surface, like the surfaces of most of the other major Saturnian moons without atmospheres, is not pure ice but contains some dark impurities. The relatively dark markings appear along the lower portion of the walls of Herschel Crater (130 kilometers, 80 miles wide) and some of the smaller craters and are marked in green in the annotated version of the image. Cassini scientists interpret this darkening as evidence for the gradual concentration of impurities from evaporating icy materials in areas where the dark impurities slide slowly down the crater wall. There, the bright ice is baked away by the sun and the vacuum of space. At Herschel, the edge where the darker regions contact the crater floor is interrupted by an extensive hummocky area. Scientists believe the hummocky texture came from the flow of melted ice that occurred during the impact that created the crater. That melt filled the bottom of the crater around the central peak. Dark streaks are seen making their way down the sides of some craters and often originated from pockets of dark contaminants embedded just below the rim of the crater wall. The pockets themselves likely represent small, pre - existing, dark - floored craters that were buried by the blanket of material thrown out from the newer im / Bridgeman Images

ID: PIX4625578

Mimas, satellite of Saturn, seen by the Cassini probe on 13/02/2010 - Saturn's moon Mimas seen by Cassini spacecraft - February 13 2010 - The Mimas satellite photographed by the Cassini probe on 13 February 2010 has a distance of 16,000 km from the satellite. Mimas is about 400 km in diameter. In the centre left, the large impact crater Herschel, 130 km wide. Relatively dark regions below bright crater walls and streaks on some of the walls are seen in this mosaic of Saturn's moon Mimas, created from images taken by Nasa's Cassini spacecraft during its closest flyby of the moon. The crater floors and surroundings are about 20 percent darker than the steep crater walls in this view. Mimas 'original surface, like the surfaces of most of the other major Saturnian moons without atmospheres, is not pure ice but contains some dark impurities. The relatively dark markings appear along the lower portion of the walls of Herschel Crater (130 kilometers, 80 miles wide) and some of the smaller cra

Enceladus, satellite of Saturn, seen by Cassini - Enceladus, satellite of Saturn, seen by Cassini - Mosaic of 21 images obtained by the Cassini probe during the overflights of this satellite on 9 March and 14 July 2005. The image shows the southern hemisphere of Enceladus. Many faults are visible and the area near the south pole is zebree of blue faults that would house pockets of liquid water.
Enceladus, satellite of Saturn, seen by Cassini - Enceladus, satellite of Saturn, seen by Cassini - Mosaic of 21 images obtained by the Cassini probe during the overflights of this satellite on 9 March and 14 July 2005. The image shows the southern hemisphere of Enceladus. Many faults are visible and the area near the south pole is zebree of blue faults that would house pockets of liquid water.

PIX4625600: Enceladus, satellite of Saturn, seen by Cassini - Enceladus, satellite of Saturn, seen by Cassini - Mosaic of 21 images obtained by the Cassini probe during the overflights of this satellite on 9 March and 14 July 2005. The image shows the southern hemisphere of Enceladus. Many faults are visible and the area near the south pole is zebree of blue faults that would house pockets of liquid water. / Bridgeman Images

ID: PIX4625600

Enceladus, satellite of Saturn, seen by Cassini - Enceladus, satellite of Saturn, seen by Cassini - Mosaic of 21 images obtained by the Cassini probe during the overflights of this satellite on 9 March and 14 July 2005. The image shows the southern hemisphere of Enceladus. Many faults are visible and the area near the south pole is zebree of blue faults that would house pockets of liquid water.

Illustration from the book
Illustration from the book

JLJ4625607: Illustration from the book "Le bon roy Henri": In front of the Spanish ambassador (litho), Job, pseudonym for Onfray de Breville, Jacques (1858-1931) / Bridgeman Images

ID: JLJ4625607

Illustration from the book "Le bon roy Henri": In front of the Spanish ambassador (litho)

Job, pseudonym for Onfray de Breville, Jacques (1858-1931)

Tethys, Saturn satellite, seen by the Cassini probe - Saturn's moon Tethys seen by Cassini spacecraft: The Tethys satellite photographed by the Cassini probe on 11 April 2015 has a distance of 53,000 km from the satellite. Tethys is about 1070 km in diameter. - This enhancement-color mosaic of Saturn's icy moon Tethys shows a range of features on the moon's trailing hemisphere. Tethys is tidally locked to Saturn, so the trailing hemisphere is the side of the moon that always faces opposite its direction of motion as it orbits the planet - Images taken using clear, green, infrared and ultraviolet spectral filters were combined to create the view, which highlights subtle color differences across Tethys' surface at wavelengths not visible to human eyes. The moon's surface is fairly uniform in natural color - The color of the surface changes conspicuously across the disk, from yellowish hues to nearly white. These broad color changes are affected by a number of external processes. First, Saturn's diffuse E-ring preferentially bombards Tethys' leading hemisphere, towards the right side of this image, with ice bright ice grains. At the same time, charged particles from Saturn's radiation belt bombard the surface on the trailing side, causing color changes due to chemical alteration of the materials there. The albedo - a measure of the surface's reflectivity - drops by 10 to 15 percent from the moon's leading side to the trailing side. Similar global color patterns exist on other Saturnian moons - This mosaic is an orthographic projection constructed from 52 Cassini images obtained on April 11, 2015 with the Cassini spacecraft narrow-angle camera. Resolution is about 1,000 feet (300 meters) per pixel. The images were obtained at a distance of approximately 33,000 miles (53,000 kilometers) from Tethys
Tethys, Saturn satellite, seen by the Cassini probe - Saturn's moon Tethys seen by Cassini spacecraft: The Tethys satellite photographed by the Cassini probe on 11 April 2015 has a distance of 53,000 km from the satellite. Tethys is about 1070 km in diameter. - This enhancement-color mosaic of Saturn's icy moon Tethys shows a range of features on the moon's trailing hemisphere. Tethys is tidally locked to Saturn, so the trailing hemisphere is the side of the moon that always faces opposite its direction of motion as it orbits the planet - Images taken using clear, green, infrared and ultraviolet spectral filters were combined to create the view, which highlights subtle color differences across Tethys' surface at wavelengths not visible to human eyes. The moon's surface is fairly uniform in natural color - The color of the surface changes conspicuously across the disk, from yellowish hues to nearly white. These broad color changes are affected by a number of external processes. First, Saturn's diffuse E-ring preferentially bombards Tethys' leading hemisphere, towards the right side of this image, with ice bright ice grains. At the same time, charged particles from Saturn's radiation belt bombard the surface on the trailing side, causing color changes due to chemical alteration of the materials there. The albedo - a measure of the surface's reflectivity - drops by 10 to 15 percent from the moon's leading side to the trailing side. Similar global color patterns exist on other Saturnian moons - This mosaic is an orthographic projection constructed from 52 Cassini images obtained on April 11, 2015 with the Cassini spacecraft narrow-angle camera. Resolution is about 1,000 feet (300 meters) per pixel. The images were obtained at a distance of approximately 33,000 miles (53,000 kilometers) from Tethys

PIX4625625: Tethys, Saturn satellite, seen by the Cassini probe - Saturn's moon Tethys seen by Cassini spacecraft: The Tethys satellite photographed by the Cassini probe on 11 April 2015 has a distance of 53,000 km from the satellite. Tethys is about 1070 km in diameter. - This enhancement-color mosaic of Saturn's icy moon Tethys shows a range of features on the moon's trailing hemisphere. Tethys is tidally locked to Saturn, so the trailing hemisphere is the side of the moon that always faces opposite its direction of motion as it orbits the planet - Images taken using clear, green, infrared and ultraviolet spectral filters were combined to create the view, which highlights subtle color differences across Tethys' surface at wavelengths not visible to human eyes. The moon's surface is fairly uniform in natural color - The color of the surface changes conspicuously across the disk, from yellowish hues to nearly white. These broad color changes are affected by a number of external processes. First, Saturn's diffuse E-ring preferentially bombards Tethys' leading hemisphere, towards the right side of this image, with ice bright ice grains. At the same time, charged particles from Saturn's radiation belt bombard the surface on the trailing side, causing color changes due to chemical alteration of the materials there. The albedo - a measure of the surface's reflectivity - drops by 10 to 15 percent from the moon's leading side to the trailing side. Similar global color patterns exist on other Saturnian moons - This mosaic is an orthographic projection constructed from 52 Cassini images obtained on April 11, 2015 with the Cassini spacecraft narrow-angle camera. Resolution is about 1,000 feet (300 meters) per pixel. The images were obtained at a distance of approximately 33,000 miles (53,000 kilometers) from Tethys / Bridgeman Images

ID: PIX4625625

Tethys, Saturn satellite, seen by the Cassini probe - Saturn's moon Tethys seen by Cassini spacecraft: The Tethys satellite photographed by the Cassini probe on 11 April 2015 has a distance of 53,000 km from the satellite. Tethys is about 1070 km in diameter. - This enhancement-color mosaic of Saturn's icy moon Tethys shows a range of features on the moon's trailing hemisphere. Tethys is tidally locked to Saturn, so the trailing hemisphere is the side of the moon that always faces opposite its direction of motion as it orbits the planet - Images taken using clear, green, infrared and ultraviolet spectral filters were combined to create the view, which highlights subtle color differences across Tethys' surface at wavelengths not visible to human eyes. The moon's surface is fairly uniform in natural color - The color of the surface changes conspicuously across the disk, from yellowish hues to nearly white. These broad color changes are affected by a number of external processes. First, S

The molding gallery of the Musee des monuments francais de la Cité de l'architecture et du patrimoine, 1 place du Trocadero and 11 November, Paris. Architect Jean Francois Bodin, rehabilitation 2007. Photography 20/10/07.
The molding gallery of the Musee des monuments francais de la Cité de l'architecture et du patrimoine, 1 place du Trocadero and 11 November, Paris. Architect Jean Francois Bodin, rehabilitation 2007. Photography 20/10/07.

MDA4626377: The molding gallery of the Musee des monuments francais de la Cité de l'architecture et du patrimoine, 1 place du Trocadero and 11 November, Paris. Architect Jean Francois Bodin, rehabilitation 2007. Photography 20/10/07. / Bridgeman Images

ID: MDA4626377

The molding gallery of the Musee des monuments francais de la Cité de l'architecture et du patrimoine, 1 place du Trocadero and 11 November, Paris. Architect Jean Francois Bodin, rehabilitation 2007. Photography 20/10/07.

The molding gallery of the Musee des monuments francais de la Cité de l'architecture et du patrimoine, 1 place du Trocadero and 11 November, Paris. Architect Jean Francois Bodin, rehabilitation 2007. Photography 20/10/07.
The molding gallery of the Musee des monuments francais de la Cité de l'architecture et du patrimoine, 1 place du Trocadero and 11 November, Paris. Architect Jean Francois Bodin, rehabilitation 2007. Photography 20/10/07.

MDA4626392: The molding gallery of the Musee des monuments francais de la Cité de l'architecture et du patrimoine, 1 place du Trocadero and 11 November, Paris. Architect Jean Francois Bodin, rehabilitation 2007. Photography 20/10/07. / Bridgeman Images

ID: MDA4626392

The molding gallery of the Musee des monuments francais de la Cité de l'architecture et du patrimoine, 1 place du Trocadero and 11 November, Paris. Architect Jean Francois Bodin, rehabilitation 2007. Photography 20/10/07.

View of the Eiffel Tower made in 1889 by Gustave Eiffel (1832-1923). Paris
View of the Eiffel Tower made in 1889 by Gustave Eiffel (1832-1923). Paris

LRI4626396: View of the Eiffel Tower made in 1889 by Gustave Eiffel (1832-1923). Paris, Eiffel, Gustave (1832-1923) / Bridgeman Images

ID: LRI4626396

View of the Eiffel Tower made in 1889 by Gustave Eiffel (1832-1923). Paris

Eiffel, Gustave (1832-1923)

“The Memorial of Saint Helene
“The Memorial of Saint Helene

JLJ4626575: “The Memorial of Saint Helene": Armee Francaise: Line infantry: fusilier, grenadier and voltiger (litho), Bombled, Louis Charles (1862-1927) / Bridgeman Images

ID: JLJ4626575

“The Memorial of Saint Helene": Armee Francaise: Line infantry: fusilier, grenadier and voltiger (litho)

Bombled, Louis Charles (1862-1927)

Sun and spot
Sun and spot

PIX4626618: Sun and spot / Bridgeman Images

ID: PIX4626618

Sun and spot

La rue de Ranelagh in Paris.
La rue de Ranelagh in Paris.

RCT4626623: La rue de Ranelagh in Paris., Castan, Remy / Bridgeman Images

ID: RCT4626623

La rue de Ranelagh in Paris.

Castan, Remy

JLJ4626556: "The Memorial of Saint Helene", Aide de camp of a division general of the French army (litho), Bombled, Louis Charles (1862-1927) / Bridgeman Images

ID: JLJ4626556

"The Memorial of Saint Helene", Aide de camp of a division general of the French army (litho)

Bombled, Louis Charles (1862-1927)

“The Memorial of Saint Helene
“The Memorial of Saint Helene

JLJ4626589: “The Memorial of Saint Helene": Student of the Polytechnic School (litho), Bombled, Louis Charles (1862-1927) / Bridgeman Images

ID: JLJ4626589

“The Memorial of Saint Helene": Student of the Polytechnic School (litho)

Bombled, Louis Charles (1862-1927)

Real estate on the boulevard de Beausejour in Paris. Photography 07/05/08
Real estate on the boulevard de Beausejour in Paris. Photography 07/05/08

RCT4626616: Real estate on the boulevard de Beausejour in Paris. Photography 07/05/08, Castan, Remy / Bridgeman Images

ID: RCT4626616

Real estate on the boulevard de Beausejour in Paris. Photography 07/05/08

Castan, Remy

Head of a woman (fragment), from the palace of Tirynthe, 1300 BC (fresco)
Head of a woman (fragment), from the palace of Tirynthe, 1300 BC (fresco)

LRI4625770: Head of a woman (fragment), from the palace of Tirynthe, 1300 BC (fresco), Mycenaean, (14th century BC) / Bridgeman Images

ID: LRI4625770

Head of a woman (fragment), from the palace of Tirynthe, 1300 BC (fresco)

Mycenaean, (14th century BC)

The site of the Musee des Monuments Francais in Paris. Cite of architecture and heritage, Palais de Chaillot, 1 place du Trocadero, Paris 16th arrondissement. All the renovation and renovation works were entrusted to the architect Jean Francois Bodin, 2007. Photography 2003.
The site of the Musee des Monuments Francais in Paris. Cite of architecture and heritage, Palais de Chaillot, 1 place du Trocadero, Paris 16th arrondissement. All the renovation and renovation works were entrusted to the architect Jean Francois Bodin, 2007. Photography 2003.

JSN4625791: The site of the Musee des Monuments Francais in Paris. Cite of architecture and heritage, Palais de Chaillot, 1 place du Trocadero, Paris 16th arrondissement. All the renovation and renovation works were entrusted to the architect Jean Francois Bodin, 2007. Photography 2003., Salmon, Jacqueline / Bridgeman Images

ID: JSN4625791

The site of the Musee des Monuments Francais in Paris. Cite of architecture and heritage, Palais de Chaillot, 1 place du Trocadero, Paris 16th arrondissement. All the renovation and renovation works were entrusted to the architect Jean Francois Bodin, 2007. Photography 2003.

Salmon, Jacqueline

The site of the Musee des Monuments Francais, Cite de l'architecture et du patrimoine, Palais de Chaillot, 1 place du Trocadero, Paris 16th. All the renovation and renovation works were entrusted to the architect Jean Francois Bodin, the end of the 2007 works. Photography 2003.
The site of the Musee des Monuments Francais, Cite de l'architecture et du patrimoine, Palais de Chaillot, 1 place du Trocadero, Paris 16th. All the renovation and renovation works were entrusted to the architect Jean Francois Bodin, the end of the 2007 works. Photography 2003.

JSN4625880: The site of the Musee des Monuments Francais, Cite de l'architecture et du patrimoine, Palais de Chaillot, 1 place du Trocadero, Paris 16th. All the renovation and renovation works were entrusted to the architect Jean Francois Bodin, the end of the 2007 works. Photography 2003., Salmon, Jacqueline / Bridgeman Images

ID: JSN4625880

The site of the Musee des Monuments Francais, Cite de l'architecture et du patrimoine, Palais de Chaillot, 1 place du Trocadero, Paris 16th. All the renovation and renovation works were entrusted to the architect Jean Francois Bodin, the end of the 2007 works. Photography 2003.

Salmon, Jacqueline

The site of the Musee des Monuments Francais in Paris. Cite of architecture and heritage, Palais de Chaillot, 1 place du Trocadero, Paris 16th arrondissement. All the renovation and renovation works were entrusted to the architect Jean Francois Bodin, 2007. Photography 2003.
The site of the Musee des Monuments Francais in Paris. Cite of architecture and heritage, Palais de Chaillot, 1 place du Trocadero, Paris 16th arrondissement. All the renovation and renovation works were entrusted to the architect Jean Francois Bodin, 2007. Photography 2003.

JSN4625950: The site of the Musee des Monuments Francais in Paris. Cite of architecture and heritage, Palais de Chaillot, 1 place du Trocadero, Paris 16th arrondissement. All the renovation and renovation works were entrusted to the architect Jean Francois Bodin, 2007. Photography 2003., Salmon, Jacqueline / Bridgeman Images

ID: JSN4625950

The site of the Musee des Monuments Francais in Paris. Cite of architecture and heritage, Palais de Chaillot, 1 place du Trocadero, Paris 16th arrondissement. All the renovation and renovation works were entrusted to the architect Jean Francois Bodin, 2007. Photography 2003.

Salmon, Jacqueline

Illustration for 'The Memorial of Saint Helene' by Count Emmanuel de Las Cases (lithograph)
Illustration for 'The Memorial of Saint Helene' by Count Emmanuel de Las Cases (lithograph)

JLJ4625986: Illustration for 'The Memorial of Saint Helene' by Count Emmanuel de Las Cases (lithograph), Bombled, Louis Charles (1862-1927) / Bridgeman Images

ID: JLJ4625986

Illustration for 'The Memorial of Saint Helene' by Count Emmanuel de Las Cases (lithograph)

Bombled, Louis Charles (1862-1927)

Illustration for 'The Memorial of Saint Helene' by Count Emmanuel de Las Cases (lithograph)
Illustration for 'The Memorial of Saint Helene' by Count Emmanuel de Las Cases (lithograph)

JLJ4626015: Illustration for 'The Memorial of Saint Helene' by Count Emmanuel de Las Cases (lithograph), Bombled, Louis Charles (1862-1927) / Bridgeman Images

ID: JLJ4626015

Illustration for 'The Memorial of Saint Helene' by Count Emmanuel de Las Cases (lithograph)

Bombled, Louis Charles (1862-1927)

“The Memorial of Saint Helene
“The Memorial of Saint Helene

JLJ4626029: “The Memorial of Saint Helene": Portrait of military surgeons and nurses of the Great Armee (litho), Bombled, Louis Charles (1862-1927) / Bridgeman Images

ID: JLJ4626029

“The Memorial of Saint Helene": Portrait of military surgeons and nurses of the Great Armee (litho)

Bombled, Louis Charles (1862-1927)


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