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La fontaine Agam a La defense (Hauts de Seine).
La fontaine Agam a La defense (Hauts de Seine).

TEC4573453: La fontaine Agam a La defense (Hauts de Seine). / Bridgeman Images

ID: TEC4573453

La fontaine Agam a La defense (Hauts de Seine).

View of the square of Mercato Vecchio in Florence -oil on canvas, 17th century
View of the square of Mercato Vecchio in Florence -oil on canvas, 17th century

LRI4573567: View of the square of Mercato Vecchio in Florence -oil on canvas, 17th century, D'Angeli, Filippo (Il Napoletano) (c.1660-c.40) / Bridgeman Images

ID: LRI4573567

View of the square of Mercato Vecchio in Florence -oil on canvas, 17th century

D'Angeli, Filippo (Il Napoletano) (c.1660-c.40)

The hell from Dante's The Divine Comedy - Detail - Fresco, 19th century
The hell from Dante's The Divine Comedy - Detail - Fresco, 19th century

LRI4573609: The hell from Dante's The Divine Comedy - Detail - Fresco, 19th century, Koch, Joseph Anton (1768-1839) / Bridgeman Images

ID: LRI4573609

The hell from Dante's The Divine Comedy - Detail - Fresco, 19th century

Koch, Joseph Anton (1768-1839)

Tour of the Societe Generale à la Defense (Hauts de Seine). Construction 1995, architects Michel Andrault and Pierre Parat.
Tour of the Societe Generale à la Defense (Hauts de Seine). Construction 1995, architects Michel Andrault and Pierre Parat.

TEC4573157: Tour of the Societe Generale à la Defense (Hauts de Seine). Construction 1995, architects Michel Andrault and Pierre Parat., Andrault, Michel (1926-2020) & Parat, Pierre (b.1928) / Bridgeman Images

ID: TEC4573157

Tour of the Societe Generale à la Defense (Hauts de Seine). Construction 1995, architects Michel Andrault and Pierre Parat.

Andrault, Michel (1926-2020) & Parat, Pierre (b.1928)

Tour of the Societe Generale à la Defense (Hauts de Seine). Construction 1995, architects Michel Andrault and Pierre Parat.
Tour of the Societe Generale à la Defense (Hauts de Seine). Construction 1995, architects Michel Andrault and Pierre Parat.

TEC4573165: Tour of the Societe Generale à la Defense (Hauts de Seine). Construction 1995, architects Michel Andrault and Pierre Parat., Andrault, Michel (1926-2020) & Parat, Pierre (b.1928) / Bridgeman Images

ID: TEC4573165

Tour of the Societe Generale à la Defense (Hauts de Seine). Construction 1995, architects Michel Andrault and Pierre Parat.

Andrault, Michel (1926-2020) & Parat, Pierre (b.1928)

View of the clouds towers, in Nanterre (Hauts de Seine). Architect Emile Aillaud (1902-1988), construction 1977.
View of the clouds towers, in Nanterre (Hauts de Seine). Architect Emile Aillaud (1902-1988), construction 1977.

TEC4573199: View of the clouds towers, in Nanterre (Hauts de Seine). Architect Emile Aillaud (1902-1988), construction 1977. / Bridgeman Images

ID: TEC4573199

View of the clouds towers, in Nanterre (Hauts de Seine). Architect Emile Aillaud (1902-1988), construction 1977.

Life of John the Baptist: st John the baptist in prison, detail, 1435 (fresco)
Life of John the Baptist: st John the baptist in prison, detail, 1435 (fresco)

LRI4573342: Life of John the Baptist: st John the baptist in prison, detail, 1435 (fresco), Masolino da Panicale, Tommaso (1383-c.1447) / Bridgeman Images

ID: LRI4573342

Life of John the Baptist: st John the baptist in prison, detail, 1435 (fresco)

Masolino da Panicale, Tommaso (1383-c.1447)

Planete extrasolaire - Artist view - Extrasolar planet - Artist vie
Planete extrasolaire - Artist view - Extrasolar planet - Artist vie

PIX4573350: Planete extrasolaire - Artist view - Extrasolar planet - Artist vie / Bridgeman Images

ID: PIX4573350

Planete extrasolaire - Artist view - Extrasolar planet - Artist vie

Les Catacombes, Paris 14th arrondissement. The origin of the catacombs dates back to the end of the 18th century, and collected all the bones found in the soil of Paris until around 1950. Anonymity is complete. It is estimated that six million of the individuals whose remains were collected in the catacombs.
Les Catacombes, Paris 14th arrondissement. The origin of the catacombs dates back to the end of the 18th century, and collected all the bones found in the soil of Paris until around 1950. Anonymity is complete. It is estimated that six million of the individuals whose remains were collected in the catacombs.

LBY4572739: Les Catacombes, Paris 14th arrondissement. The origin of the catacombs dates back to the end of the 18th century, and collected all the bones found in the soil of Paris until around 1950. Anonymity is complete. It is estimated that six million of the individuals whose remains were collected in the catacombs. / Bridgeman Images

ID: LBY4572739

Les Catacombes, Paris 14th arrondissement. The origin of the catacombs dates back to the end of the 18th century, and collected all the bones found in the soil of Paris until around 1950. Anonymity is complete. It is estimated that six million of the individuals whose remains were collected in the catacombs.

Binary pulsar and gravitational waves - Artist's impression of the pulsar PSR J0348+0432 and its white dwarf companion - Artist's view of a gravitational wave generated by a system of a neutron star associated with a white dwarf, spreading on the fabric of space - time. This artist's impression shows the exotic double object that consists of a tiny, but very heavy neutron star that spins 25 times each second, orbited every two and a half hours by a white dwarf star. The neutron star is a pulsar named PSR J0348+0432 that is giving off radio waves that can be picked up on Earth by radio telescopes. Although this unusual pair is very interesting in its own right it is also a unique laboratory for testing the limits of physical theories. This system is radiating gravitational radiation, ripples in spacetime. Although these waves cannot be detected directly by astronomers on Earth they can be detected indirectly by measuring the change in the orbit of the system as it loses energy. As the pulsar is so small the relative sizes of the two objects are not drawn to scale
Binary pulsar and gravitational waves - Artist's impression of the pulsar PSR J0348+0432 and its white dwarf companion - Artist's view of a gravitational wave generated by a system of a neutron star associated with a white dwarf, spreading on the fabric of space - time. This artist's impression shows the exotic double object that consists of a tiny, but very heavy neutron star that spins 25 times each second, orbited every two and a half hours by a white dwarf star. The neutron star is a pulsar named PSR J0348+0432 that is giving off radio waves that can be picked up on Earth by radio telescopes. Although this unusual pair is very interesting in its own right it is also a unique laboratory for testing the limits of physical theories. This system is radiating gravitational radiation, ripples in spacetime. Although these waves cannot be detected directly by astronomers on Earth they can be detected indirectly by measuring the change in the orbit of the system as it loses energy. As the pulsar is so small the relative sizes of the two objects are not drawn to scale

PIX4572892: Binary pulsar and gravitational waves - Artist's impression of the pulsar PSR J0348+0432 and its white dwarf companion - Artist's view of a gravitational wave generated by a system of a neutron star associated with a white dwarf, spreading on the fabric of space - time. This artist's impression shows the exotic double object that consists of a tiny, but very heavy neutron star that spins 25 times each second, orbited every two and a half hours by a white dwarf star. The neutron star is a pulsar named PSR J0348+0432 that is giving off radio waves that can be picked up on Earth by radio telescopes. Although this unusual pair is very interesting in its own right it is also a unique laboratory for testing the limits of physical theories. This system is radiating gravitational radiation, ripples in spacetime. Although these waves cannot be detected directly by astronomers on Earth they can be detected indirectly by measuring the change in the orbit of the system as it loses energy. As the pulsar is so small the relative sizes of the two objects are not drawn to scale / Bridgeman Images

ID: PIX4572892

Binary pulsar and gravitational waves - Artist's impression of the pulsar PSR J0348+0432 and its white dwarf companion - Artist's view of a gravitational wave generated by a system of a neutron star associated with a white dwarf, spreading on the fabric of space - time. This artist's impression shows the exotic double object that consists of a tiny, but very heavy neutron star that spins 25 times each second, orbited every two and a half hours by a white dwarf star. The neutron star is a pulsar named PSR J0348+0432 that is giving off radio waves that can be picked up on Earth by radio telescopes. Although this unusual pair is very interesting in its own right it is also a unique laboratory for testing the limits of physical theories. This system is radiating gravitational radiation, ripples in spacetime. Although these waves cannot be detected directly by astronomers on Earth they can be detected indirectly by measuring the change in the orbit of the system as it loses energy. As the p

Tour of the Societe Generale à la Defense (Hauts de Seine). Construction 1995, architects Michel Andrault and Pierre Parat.
Tour of the Societe Generale à la Defense (Hauts de Seine). Construction 1995, architects Michel Andrault and Pierre Parat.

TEC4573135: Tour of the Societe Generale à la Defense (Hauts de Seine). Construction 1995, architects Michel Andrault and Pierre Parat., Andrault, Michel (1926-2020) & Parat, Pierre (b.1928) / Bridgeman Images

ID: TEC4573135

Tour of the Societe Generale à la Defense (Hauts de Seine). Construction 1995, architects Michel Andrault and Pierre Parat.

Andrault, Michel (1926-2020) & Parat, Pierre (b.1928)

Exoplanets around 70 Virginis - A jovian planet orbiting 70 Virginis - Artist's view of the extrasolar planet 70 Vir B, a giant gas planet orbiting around a solar star, about 78 years old - light from the Sun. This exoplanet has about 6 times the mass of Jupiter and its distance from its star 70 Virginis is almost the same as that of Mercury from the Sun. A ringed 70 Vir B presides over the hot and airless terrain of a hypothetical moon. While it is not known if 70 Vir B has rings, it is certainly possible. 70 Vir B's rings would have no ice in them due to is proximity to its sun. Such rings would likely be less than 100 million years old and could have been formed from the shattered remnants of an asteroid that wondered too close to this giant planet. 70 Vir B's eccentric orbit would increase the likelihood of its encountering other objects in orbit around 70 Virginis. About 78 light years from the Earth astronomers believe that there is a large planet orbiting 70 Virginis, a type G5V star (similar to our own sun). Designated 70 Vir B, this planet is believed to have over six times the mass of the planet Jupiter and orbits around its sun in an eccentric orbit once every 116 days. 70 Vir B's average distance from its sun is about the same as that of the planet Mercury from our own sun
Exoplanets around 70 Virginis - A jovian planet orbiting 70 Virginis - Artist's view of the extrasolar planet 70 Vir B, a giant gas planet orbiting around a solar star, about 78 years old - light from the Sun. This exoplanet has about 6 times the mass of Jupiter and its distance from its star 70 Virginis is almost the same as that of Mercury from the Sun. A ringed 70 Vir B presides over the hot and airless terrain of a hypothetical moon. While it is not known if 70 Vir B has rings, it is certainly possible. 70 Vir B's rings would have no ice in them due to is proximity to its sun. Such rings would likely be less than 100 million years old and could have been formed from the shattered remnants of an asteroid that wondered too close to this giant planet. 70 Vir B's eccentric orbit would increase the likelihood of its encountering other objects in orbit around 70 Virginis. About 78 light years from the Earth astronomers believe that there is a large planet orbiting 70 Virginis, a type G5V star (similar to our own sun). Designated 70 Vir B, this planet is believed to have over six times the mass of the planet Jupiter and orbits around its sun in an eccentric orbit once every 116 days. 70 Vir B's average distance from its sun is about the same as that of the planet Mercury from our own sun

PIX4573224: Exoplanets around 70 Virginis - A jovian planet orbiting 70 Virginis - Artist's view of the extrasolar planet 70 Vir B, a giant gas planet orbiting around a solar star, about 78 years old - light from the Sun. This exoplanet has about 6 times the mass of Jupiter and its distance from its star 70 Virginis is almost the same as that of Mercury from the Sun. A ringed 70 Vir B presides over the hot and airless terrain of a hypothetical moon. While it is not known if 70 Vir B has rings, it is certainly possible. 70 Vir B's rings would have no ice in them due to is proximity to its sun. Such rings would likely be less than 100 million years old and could have been formed from the shattered remnants of an asteroid that wondered too close to this giant planet. 70 Vir B's eccentric orbit would increase the likelihood of its encountering other objects in orbit around 70 Virginis. About 78 light years from the Earth astronomers believe that there is a large planet orbiting 70 Virginis, a type G5V star (similar to our own sun). Designated 70 Vir B, this planet is believed to have over six times the mass of the planet Jupiter and orbits around its sun in an eccentric orbit once every 116 days. 70 Vir B's average distance from its sun is about the same as that of the planet Mercury from our own sun / Bridgeman Images

ID: PIX4573224

Exoplanets around 70 Virginis - A jovian planet orbiting 70 Virginis - Artist's view of the extrasolar planet 70 Vir B, a giant gas planet orbiting around a solar star, about 78 years old - light from the Sun. This exoplanet has about 6 times the mass of Jupiter and its distance from its star 70 Virginis is almost the same as that of Mercury from the Sun. A ringed 70 Vir B presides over the hot and airless terrain of a hypothetical moon. While it is not known if 70 Vir B has rings, it is certainly possible. 70 Vir B's rings would have no ice in them due to is proximity to its sun. Such rings would likely be less than 100 million years old and could have been formed from the shattered remnants of an asteroid that wondered too close to this giant planet. 70 Vir B's eccentric orbit would increase the likelihood of its encountering other objects in orbit around 70 Virginis. About 78 light years from the Earth astronomers believe that there is a large planet orbiting 70 Virginis, a type G5V

Urban wasteland in Courbevoie (Hauts de Seine).
Urban wasteland in Courbevoie (Hauts de Seine).

TEC4573205: Urban wasteland in Courbevoie (Hauts de Seine). / Bridgeman Images

ID: TEC4573205

Urban wasteland in Courbevoie (Hauts de Seine).

Shopping centre Les Quatre Temps, (architectesJean Dimitrijevic and Guy Lagneau, construction 1981) in La Defense (Hauts de Seine).
Shopping centre Les Quatre Temps, (architectesJean Dimitrijevic and Guy Lagneau, construction 1981) in La Defense (Hauts de Seine).

TEC4573214: Shopping centre Les Quatre Temps, (architectesJean Dimitrijevic and Guy Lagneau, construction 1981) in La Defense (Hauts de Seine). / Bridgeman Images

ID: TEC4573214

Shopping centre Les Quatre Temps, (architectesJean Dimitrijevic and Guy Lagneau, construction 1981) in La Defense (Hauts de Seine).

Villa Adrienne, 19 avenue du General Leclerc in Paris. Set up in 1780, this villa was originally intended to receive military and ecclesiastic.
Villa Adrienne, 19 avenue du General Leclerc in Paris. Set up in 1780, this villa was originally intended to receive military and ecclesiastic.

TEC4572060: Villa Adrienne, 19 avenue du General Leclerc in Paris. Set up in 1780, this villa was originally intended to receive military and ecclesiastic. / Bridgeman Images

ID: TEC4572060

Villa Adrienne, 19 avenue du General Leclerc in Paris. Set up in 1780, this villa was originally intended to receive military and ecclesiastic.

The Maine Montparnasse tower, seen from the boulevard du Maine in Paris. Construction 1969-1972, architects Jean Saubot, Eugene Beaudouin, Urbain Cassan and Louis Hoy
The Maine Montparnasse tower, seen from the boulevard du Maine in Paris. Construction 1969-1972, architects Jean Saubot, Eugene Beaudouin, Urbain Cassan and Louis Hoy

TEC4572389: The Maine Montparnasse tower, seen from the boulevard du Maine in Paris. Construction 1969-1972, architects Jean Saubot, Eugene Beaudouin, Urbain Cassan and Louis Hoy / Bridgeman Images

ID: TEC4572389

The Maine Montparnasse tower, seen from the boulevard du Maine in Paris. Construction 1969-1972, architects Jean Saubot, Eugene Beaudouin, Urbain Cassan and Louis Hoy

Building Plaisance in Paris. Construction 1966, architect Jean Dubuisson.
Building Plaisance in Paris. Construction 1966, architect Jean Dubuisson.

TEC4572320: Building Plaisance in Paris. Construction 1966, architect Jean Dubuisson., Dubuisson, Jean (1914-2011) / Bridgeman Images

ID: TEC4572320

Building Plaisance in Paris. Construction 1966, architect Jean Dubuisson.

Dubuisson, Jean (1914-2011)

Variable star Mira Ceti view in ultraviolet - Star Mira Ceti seen in ultraviolet - Ultraviolet view of the star Mira of the Whale revealing a long train of material ejected by the large red star. This trail extends over 13 years - light. Mosaic of images obtained by the Galex satellite in November and December 2006. Ultraviolet image of the star Mira taken with the Galex satellite in November and December 2006. In this image, Mira is moving from left to right. It is visible as the small white dot in the bulb shape at right. The shed material can be seen in light blue. The dots in the picture are stars and distant galaxies. The large blue dot at left is a star that is closer to us than Mira. Mira is traveling so fast (130 kilometers per second) that it's creating a bow shock, or build - up of gas, in front of it, as can be seen here at right
Variable star Mira Ceti view in ultraviolet - Star Mira Ceti seen in ultraviolet - Ultraviolet view of the star Mira of the Whale revealing a long train of material ejected by the large red star. This trail extends over 13 years - light. Mosaic of images obtained by the Galex satellite in November and December 2006. Ultraviolet image of the star Mira taken with the Galex satellite in November and December 2006. In this image, Mira is moving from left to right. It is visible as the small white dot in the bulb shape at right. The shed material can be seen in light blue. The dots in the picture are stars and distant galaxies. The large blue dot at left is a star that is closer to us than Mira. Mira is traveling so fast (130 kilometers per second) that it's creating a bow shock, or build - up of gas, in front of it, as can be seen here at right

PIX4572330: Variable star Mira Ceti view in ultraviolet - Star Mira Ceti seen in ultraviolet - Ultraviolet view of the star Mira of the Whale revealing a long train of material ejected by the large red star. This trail extends over 13 years - light. Mosaic of images obtained by the Galex satellite in November and December 2006. Ultraviolet image of the star Mira taken with the Galex satellite in November and December 2006. In this image, Mira is moving from left to right. It is visible as the small white dot in the bulb shape at right. The shed material can be seen in light blue. The dots in the picture are stars and distant galaxies. The large blue dot at left is a star that is closer to us than Mira. Mira is traveling so fast (130 kilometers per second) that it's creating a bow shock, or build - up of gas, in front of it, as can be seen here at right / Bridgeman Images

ID: PIX4572330

Variable star Mira Ceti view in ultraviolet - Star Mira Ceti seen in ultraviolet - Ultraviolet view of the star Mira of the Whale revealing a long train of material ejected by the large red star. This trail extends over 13 years - light. Mosaic of images obtained by the Galex satellite in November and December 2006. Ultraviolet image of the star Mira taken with the Galex satellite in November and December 2006. In this image, Mira is moving from left to right. It is visible as the small white dot in the bulb shape at right. The shed material can be seen in light blue. The dots in the picture are stars and distant galaxies. The large blue dot at left is a star that is closer to us than Mira. Mira is traveling so fast (130 kilometers per second) that it's creating a bow shock, or build - up of gas, in front of it, as can be seen here at right

Tours to the Defense (Hauts de Seine) with the circular boulevard in the foreground.
Tours to the Defense (Hauts de Seine) with the circular boulevard in the foreground.

TEC4573521: Tours to the Defense (Hauts de Seine) with the circular boulevard in the foreground. / Bridgeman Images

ID: TEC4573521

Tours to the Defense (Hauts de Seine) with the circular boulevard in the foreground.

Urban layout, the Terrasse de Nanterre and Puteaux (Hauts de Seine).
Urban layout, the Terrasse de Nanterre and Puteaux (Hauts de Seine).

TEC4573616: Urban layout, the Terrasse de Nanterre and Puteaux (Hauts de Seine). / Bridgeman Images

ID: TEC4573616

Urban layout, the Terrasse de Nanterre and Puteaux (Hauts de Seine).

Conjunction Moon-Pleiades -06/2006 - Moon and Pleiades conjunction-06/2006 - The Moon in conjunction with the Pleiades cluster. On the right, on the horizon, Venus rises. June 23, 2006, Sainte Marine (Finistere-France). Moon in close conjunction with Pleiades star cluster. Venus is rising at right. June 23 2006, Sainte Marine (Finistere-France)
Conjunction Moon-Pleiades -06/2006 - Moon and Pleiades conjunction-06/2006 - The Moon in conjunction with the Pleiades cluster. On the right, on the horizon, Venus rises. June 23, 2006, Sainte Marine (Finistere-France). Moon in close conjunction with Pleiades star cluster. Venus is rising at right. June 23 2006, Sainte Marine (Finistere-France)

PIX4587841: Conjunction Moon-Pleiades -06/2006 - Moon and Pleiades conjunction-06/2006 - The Moon in conjunction with the Pleiades cluster. On the right, on the horizon, Venus rises. June 23, 2006, Sainte Marine (Finistere-France). Moon in close conjunction with Pleiades star cluster. Venus is rising at right. June 23 2006, Sainte Marine (Finistere-France) / Bridgeman Images

ID: PIX4587841

Conjunction Moon-Pleiades -06/2006 - Moon and Pleiades conjunction-06/2006 - The Moon in conjunction with the Pleiades cluster. On the right, on the horizon, Venus rises. June 23, 2006, Sainte Marine (Finistere-France). Moon in close conjunction with Pleiades star cluster. Venus is rising at right. June 23 2006, Sainte Marine (Finistere-France)

Detail of the Nilotic mosaic of Preneste (Palestrina) from the shrine of the deity of Fortune Primigenia, 80 BC
Detail of the Nilotic mosaic of Preneste (Palestrina) from the shrine of the deity of Fortune Primigenia, 80 BC

LRI4587901: Detail of the Nilotic mosaic of Preneste (Palestrina) from the shrine of the deity of Fortune Primigenia, 80 BC, Roman, (1st century BC) / Bridgeman Images

ID: LRI4587901

Detail of the Nilotic mosaic of Preneste (Palestrina) from the shrine of the deity of Fortune Primigenia, 80 BC

Roman, (1st century BC)

Representation of a manufacturer of crowns (relief)
Representation of a manufacturer of crowns (relief)

LRI4587831: Representation of a manufacturer of crowns (relief), Roman / Bridgeman Images

ID: LRI4587831

Representation of a manufacturer of crowns (relief)

Roman

The Metropolis building in Madrid (Spain), at the intersection of Calle Gran Via and Calle de Incala. Building realized in 1905 by Jules (1842-1037) and Raymond February. Photography 22/09/2005.
The Metropolis building in Madrid (Spain), at the intersection of Calle Gran Via and Calle de Incala. Building realized in 1905 by Jules (1842-1037) and Raymond February. Photography 22/09/2005.

LBY4587839: The Metropolis building in Madrid (Spain), at the intersection of Calle Gran Via and Calle de Incala. Building realized in 1905 by Jules (1842-1037) and Raymond February. Photography 22/09/2005. / Bridgeman Images

ID: LBY4587839

The Metropolis building in Madrid (Spain), at the intersection of Calle Gran Via and Calle de Incala. Building realized in 1905 by Jules (1842-1037) and Raymond February. Photography 22/09/2005.

Pediment decorated with knives and butcher objects, 1st century BC (low relief)
Pediment decorated with knives and butcher objects, 1st century BC (low relief)

LRI4587854: Pediment decorated with knives and butcher objects, 1st century BC (low relief), Roman, (1st century BC) / Bridgeman Images

ID: LRI4587854

Pediment decorated with knives and butcher objects, 1st century BC (low relief)

Roman, (1st century BC)

La Capitania General, Calle Mayor in Madrid, Spain.
La Capitania General, Calle Mayor in Madrid, Spain.

LBY4587898: La Capitania General, Calle Mayor in Madrid, Spain. / Bridgeman Images

ID: LBY4587898

La Capitania General, Calle Mayor in Madrid, Spain.

Plaza Mayor, architect Juan de Villanueva, 18th century, in Madrid (Spain). In the background, Casa de la Panaderia, 16th century. Photography 22/09/2005.
Plaza Mayor, architect Juan de Villanueva, 18th century, in Madrid (Spain). In the background, Casa de la Panaderia, 16th century. Photography 22/09/2005.

LBY4587954: Plaza Mayor, architect Juan de Villanueva, 18th century, in Madrid (Spain). In the background, Casa de la Panaderia, 16th century. Photography 22/09/2005. / Bridgeman Images

ID: LBY4587954

Plaza Mayor, architect Juan de Villanueva, 18th century, in Madrid (Spain). In the background, Casa de la Panaderia, 16th century. Photography 22/09/2005.

Church of San Jeronimo El Real in Madrid, Spain.
Church of San Jeronimo El Real in Madrid, Spain.

LBY4587984: Church of San Jeronimo El Real in Madrid, Spain. / Bridgeman Images

ID: LBY4587984

Church of San Jeronimo El Real in Madrid, Spain.

La plaza del Canalejas, Calle de Sevila in Madrid (Spain).
La plaza del Canalejas, Calle de Sevila in Madrid (Spain).

LBY4587913: La plaza del Canalejas, Calle de Sevila in Madrid (Spain). / Bridgeman Images

ID: LBY4587913

La plaza del Canalejas, Calle de Sevila in Madrid (Spain).

Lune et amas des Pleiades - Moon and Pleiades star cluster - The Moon near the Pleiades cluster above the castle of Savaillan in the Gers. 30 March 2009. Moon close to the Pleiades star cluster above the castle of Savaillan in Gers, France. March 30, 2009
Lune et amas des Pleiades - Moon and Pleiades star cluster - The Moon near the Pleiades cluster above the castle of Savaillan in the Gers. 30 March 2009. Moon close to the Pleiades star cluster above the castle of Savaillan in Gers, France. March 30, 2009

PIX4587965: Lune et amas des Pleiades - Moon and Pleiades star cluster - The Moon near the Pleiades cluster above the castle of Savaillan in the Gers. 30 March 2009. Moon close to the Pleiades star cluster above the castle of Savaillan in Gers, France. March 30, 2009 / Bridgeman Images

ID: PIX4587965

Lune et amas des Pleiades - Moon and Pleiades star cluster - The Moon near the Pleiades cluster above the castle of Savaillan in the Gers. 30 March 2009. Moon close to the Pleiades star cluster above the castle of Savaillan in Gers, France. March 30, 2009

The extension of the Museo del Prado in Madrid (Spain). Architects of the Museum, in 1808: Juan de Villanueva, in 1918, renovated by Antonio Lopez Aguado and in 2005, extended by Rafael Moneo.
The extension of the Museo del Prado in Madrid (Spain). Architects of the Museum, in 1808: Juan de Villanueva, in 1918, renovated by Antonio Lopez Aguado and in 2005, extended by Rafael Moneo.

OMG4588082: The extension of the Museo del Prado in Madrid (Spain). Architects of the Museum, in 1808: Juan de Villanueva, in 1918, renovated by Antonio Lopez Aguado and in 2005, extended by Rafael Moneo., Moneo, Jose Rafael (b.1937) / Bridgeman Images

ID: OMG4588082

The extension of the Museo del Prado in Madrid (Spain). Architects of the Museum, in 1808: Juan de Villanueva, in 1918, renovated by Antonio Lopez Aguado and in 2005, extended by Rafael Moneo.

Moneo, Jose Rafael (b.1937)

Conjunction Venus-Saturn 13/10/2009 - Conjunction Venus-Saturn - October 13 2009 - The bright spot in the sky is the planet Venus. To his left is the planet Saturn. On the right, a plane leaves a condensation train. Kerogan Bay, Finistere. Venus (bright dot) with Saturn (close to Venus, at left), and a plane above the bay of Kerogan (Finistere, Brittany)
Conjunction Venus-Saturn 13/10/2009 - Conjunction Venus-Saturn - October 13 2009 - The bright spot in the sky is the planet Venus. To his left is the planet Saturn. On the right, a plane leaves a condensation train. Kerogan Bay, Finistere. Venus (bright dot) with Saturn (close to Venus, at left), and a plane above the bay of Kerogan (Finistere, Brittany)

PIX4588110: Conjunction Venus-Saturn 13/10/2009 - Conjunction Venus-Saturn - October 13 2009 - The bright spot in the sky is the planet Venus. To his left is the planet Saturn. On the right, a plane leaves a condensation train. Kerogan Bay, Finistere. Venus (bright dot) with Saturn (close to Venus, at left), and a plane above the bay of Kerogan (Finistere, Brittany) / Bridgeman Images

ID: PIX4588110

Conjunction Venus-Saturn 13/10/2009 - Conjunction Venus-Saturn - October 13 2009 - The bright spot in the sky is the planet Venus. To his left is the planet Saturn. On the right, a plane leaves a condensation train. Kerogan Bay, Finistere. Venus (bright dot) with Saturn (close to Venus, at left), and a plane above the bay of Kerogan (Finistere, Brittany)

The theatre Valle Inclön, Plaza de Lavapies in Madrid (Spain). Architects Angela Garcia de Paredes and Ignacio Garcia Pedrosa, 2005. Photography 30/12/07.
The theatre Valle Inclön, Plaza de Lavapies in Madrid (Spain). Architects Angela Garcia de Paredes and Ignacio Garcia Pedrosa, 2005. Photography 30/12/07.

RCT4588581: The theatre Valle Inclön, Plaza de Lavapies in Madrid (Spain). Architects Angela Garcia de Paredes and Ignacio Garcia Pedrosa, 2005. Photography 30/12/07., Castan, Remy / Bridgeman Images

ID: RCT4588581

The theatre Valle Inclön, Plaza de Lavapies in Madrid (Spain). Architects Angela Garcia de Paredes and Ignacio Garcia Pedrosa, 2005. Photography 30/12/07.

Castan, Remy

Comet 67P/Churyumov-Gerasimenko and Philae - Comet 67P/Churyumov-Gerasimenko nucleus with Philae: Detail of the surface of the nucleus of Comet 67P/Churyumov-Gerasimenko as seen on September 2, 2016 by the Rosetta probe. The Philae lander appears pose on the comet - Rosetta's lander Philae has been identified in OSIRIS narrow-angle camera images taken on 2 September 2016 from a distance of 2.7 km. The image scale is about 5 cm/pixel - Philae's 1 m-wide body and two of its three legs can be seen extended from the body. The images also provide proof of Philae's orientation - A Rosetta Navigation Camera image taken on 16 April 2015 is shown at top right for context, with the approximate location of Philae on the small lobe of Comet Churyumov-Gerasimenko marked
Comet 67P/Churyumov-Gerasimenko and Philae - Comet 67P/Churyumov-Gerasimenko nucleus with Philae: Detail of the surface of the nucleus of Comet 67P/Churyumov-Gerasimenko as seen on September 2, 2016 by the Rosetta probe. The Philae lander appears pose on the comet - Rosetta's lander Philae has been identified in OSIRIS narrow-angle camera images taken on 2 September 2016 from a distance of 2.7 km. The image scale is about 5 cm/pixel - Philae's 1 m-wide body and two of its three legs can be seen extended from the body. The images also provide proof of Philae's orientation - A Rosetta Navigation Camera image taken on 16 April 2015 is shown at top right for context, with the approximate location of Philae on the small lobe of Comet Churyumov-Gerasimenko marked

PIX4588652: Comet 67P/Churyumov-Gerasimenko and Philae - Comet 67P/Churyumov-Gerasimenko nucleus with Philae: Detail of the surface of the nucleus of Comet 67P/Churyumov-Gerasimenko as seen on September 2, 2016 by the Rosetta probe. The Philae lander appears pose on the comet - Rosetta's lander Philae has been identified in OSIRIS narrow-angle camera images taken on 2 September 2016 from a distance of 2.7 km. The image scale is about 5 cm/pixel - Philae's 1 m-wide body and two of its three legs can be seen extended from the body. The images also provide proof of Philae's orientation - A Rosetta Navigation Camera image taken on 16 April 2015 is shown at top right for context, with the approximate location of Philae on the small lobe of Comet Churyumov-Gerasimenko marked / Bridgeman Images

ID: PIX4588652

Comet 67P/Churyumov-Gerasimenko and Philae - Comet 67P/Churyumov-Gerasimenko nucleus with Philae: Detail of the surface of the nucleus of Comet 67P/Churyumov-Gerasimenko as seen on September 2, 2016 by the Rosetta probe. The Philae lander appears pose on the comet - Rosetta's lander Philae has been identified in OSIRIS narrow-angle camera images taken on 2 September 2016 from a distance of 2.7 km. The image scale is about 5 cm/pixel - Philae's 1 m-wide body and two of its three legs can be seen extended from the body. The images also provide proof of Philae's orientation - A Rosetta Navigation Camera image taken on 16 April 2015 is shown at top right for context, with the approximate location of Philae on the small lobe of Comet Churyumov-Gerasimenko marked

The Parque del Retiro in Madrid (Spain).Photography 29/12/07.
The Parque del Retiro in Madrid (Spain).Photography 29/12/07.

RCT4588704: The Parque del Retiro in Madrid (Spain).Photography 29/12/07., Castan, Remy / Bridgeman Images

ID: RCT4588704

The Parque del Retiro in Madrid (Spain).Photography 29/12/07.

Castan, Remy

Extension of Atocha Station in Madrid (Spain). Realisation 1992, architect Rafael Moneo. Photography 30/12/07.
Extension of Atocha Station in Madrid (Spain). Realisation 1992, architect Rafael Moneo. Photography 30/12/07.

RCT4588694: Extension of Atocha Station in Madrid (Spain). Realisation 1992, architect Rafael Moneo. Photography 30/12/07., Moneo, Jose Rafael (b.1937) / Bridgeman Images

ID: RCT4588694

Extension of Atocha Station in Madrid (Spain). Realisation 1992, architect Rafael Moneo. Photography 30/12/07.

Moneo, Jose Rafael (b.1937)


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