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Telescope Gemini south - Gemini South Telescope - The 8.2 m Gemini south telescope. Cerro Pachon, Chile. Gemini south telescope. Cerro Pachon, Chile
Telescope Gemini south - Gemini South Telescope - The 8.2 m Gemini south telescope. Cerro Pachon, Chile. Gemini south telescope. Cerro Pachon, Chile

PIX4652758: Telescope Gemini south - Gemini South Telescope - The 8.2 m Gemini south telescope. Cerro Pachon, Chile. Gemini south telescope. Cerro Pachon, Chile / Bridgeman Images

ID: PIX4652758

Telescope Gemini south - Gemini South Telescope - The 8.2 m Gemini south telescope. Cerro Pachon, Chile. Gemini south telescope. Cerro Pachon, Chile

Telescope SOAR - Chile - SOAR Telescope - The dome of the 4 m telescope SOAR (Southern Astrophysical Research Telescope). Cerro Pachon, Chile. SOAR (Southern Astrophysical Research Telescope) is a 4 - meter telescope located on Cerro Pachon in Chile
Telescope SOAR - Chile - SOAR Telescope - The dome of the 4 m telescope SOAR (Southern Astrophysical Research Telescope). Cerro Pachon, Chile. SOAR (Southern Astrophysical Research Telescope) is a 4 - meter telescope located on Cerro Pachon in Chile

PIX4652805: Telescope SOAR - Chile - SOAR Telescope - The dome of the 4 m telescope SOAR (Southern Astrophysical Research Telescope). Cerro Pachon, Chile. SOAR (Southern Astrophysical Research Telescope) is a 4 - meter telescope located on Cerro Pachon in Chile / Bridgeman Images

ID: PIX4652805

Telescope SOAR - Chile - SOAR Telescope - The dome of the 4 m telescope SOAR (Southern Astrophysical Research Telescope). Cerro Pachon, Chile. SOAR (Southern Astrophysical Research Telescope) is a 4 - meter telescope located on Cerro Pachon in Chile

Hotel de Ville de Boulogne Billancourt (Hauts de Seine). Architect Tony Garnier (1869-1948), 1931-1934. Built of weapon concrete, the building is seen as an exemplary town hall for the 20th century, a municipal factory characterized by the transparency of the counter hall with its three levels of suspended galleries.
Hotel de Ville de Boulogne Billancourt (Hauts de Seine). Architect Tony Garnier (1869-1948), 1931-1934. Built of weapon concrete, the building is seen as an exemplary town hall for the 20th century, a municipal factory characterized by the transparency of the counter hall with its three levels of suspended galleries.

TEC4652811: Hotel de Ville de Boulogne Billancourt (Hauts de Seine). Architect Tony Garnier (1869-1948), 1931-1934. Built of weapon concrete, the building is seen as an exemplary town hall for the 20th century, a municipal factory characterized by the transparency of the counter hall with its three levels of suspended galleries., Garnier, Tony (1869-1948) / Bridgeman Images

ID: TEC4652811

Hotel de Ville de Boulogne Billancourt (Hauts de Seine). Architect Tony Garnier (1869-1948), 1931-1934. Built of weapon concrete, the building is seen as an exemplary town hall for the 20th century, a municipal factory characterized by the transparency of the counter hall with its three levels of suspended galleries.

Garnier, Tony (1869-1948)

Cerro Tololo Observatory - Chile - Cerro Tololo Observatory - Chile - Cerro Tololo Observatory seen from Cerro Pachon, Chile. Cerro Tololo observatory seen from Cerro Pachon. Chile
Cerro Tololo Observatory - Chile - Cerro Tololo Observatory - Chile - Cerro Tololo Observatory seen from Cerro Pachon, Chile. Cerro Tololo observatory seen from Cerro Pachon. Chile

PIX4652829: Cerro Tololo Observatory - Chile - Cerro Tololo Observatory - Chile - Cerro Tololo Observatory seen from Cerro Pachon, Chile. Cerro Tololo observatory seen from Cerro Pachon. Chile / Bridgeman Images

ID: PIX4652829

Cerro Tololo Observatory - Chile - Cerro Tololo Observatory - Chile - Cerro Tololo Observatory seen from Cerro Pachon, Chile. Cerro Tololo observatory seen from Cerro Pachon. Chile

Hotel de Ville de Boulogne Billancourt (Hauts de Seine). Architect Tony Garnier (1869-1948), 1931-1934. Built of weapon concrete, the building is seen as an exemplary town hall for the 20th century, a municipal factory characterized by the transparency of the counter hall with its three levels of suspended galleries.
Hotel de Ville de Boulogne Billancourt (Hauts de Seine). Architect Tony Garnier (1869-1948), 1931-1934. Built of weapon concrete, the building is seen as an exemplary town hall for the 20th century, a municipal factory characterized by the transparency of the counter hall with its three levels of suspended galleries.

MDA4652837: Hotel de Ville de Boulogne Billancourt (Hauts de Seine). Architect Tony Garnier (1869-1948), 1931-1934. Built of weapon concrete, the building is seen as an exemplary town hall for the 20th century, a municipal factory characterized by the transparency of the counter hall with its three levels of suspended galleries., Garnier, Tony (1869-1948) / Bridgeman Images

ID: MDA4652837

Hotel de Ville de Boulogne Billancourt (Hauts de Seine). Architect Tony Garnier (1869-1948), 1931-1934. Built of weapon concrete, the building is seen as an exemplary town hall for the 20th century, a municipal factory characterized by the transparency of the counter hall with its three levels of suspended galleries.

Garnier, Tony (1869-1948)

Telescope Gemini south - Gemini South Telescope - The dome of the 8.2 m Gemini south telescope on Cerro Pachon in Chile. Gemini south telescope at summit of Cerro Pachon in Chile
Telescope Gemini south - Gemini South Telescope - The dome of the 8.2 m Gemini south telescope on Cerro Pachon in Chile. Gemini south telescope at summit of Cerro Pachon in Chile

PIX4652783: Telescope Gemini south - Gemini South Telescope - The dome of the 8.2 m Gemini south telescope on Cerro Pachon in Chile. Gemini south telescope at summit of Cerro Pachon in Chile / Bridgeman Images

ID: PIX4652783

Telescope Gemini south - Gemini South Telescope - The dome of the 8.2 m Gemini south telescope on Cerro Pachon in Chile. Gemini south telescope at summit of Cerro Pachon in Chile

Ancient Greece: Perirrhanterion of Delphi in marble with three Cores 6th century BC (marble)
Ancient Greece: Perirrhanterion of Delphi in marble with three Cores 6th century BC (marble)

JLJ4652789: Ancient Greece: Perirrhanterion of Delphi in marble with three Cores 6th century BC (marble), Greek school, (6th century BC) / Bridgeman Images

ID: JLJ4652789

Ancient Greece: Perirrhanterion of Delphi in marble with three Cores 6th century BC (marble)

Greek school, (6th century BC)

Agias Sculpture of Lysipus of Sicyone (395-305 BC) 355 BC (marble)
Agias Sculpture of Lysipus of Sicyone (395-305 BC) 355 BC (marble)

JLJ4652804: Agias Sculpture of Lysipus of Sicyone (395-305 BC) 355 BC (marble), Lysippos (fl.370-310 BC) (attributed to) / Bridgeman Images

ID: JLJ4652804

Agias Sculpture of Lysipus of Sicyone (395-305 BC) 355 BC (marble)

Lysippos (fl.370-310 BC) (attributed to)

Hotel de Ville de Boulogne Billancourt (Hauts de Seine). Architect Tony Garnier (1869-1948), 1931-1934. Built of weapon concrete, the building is seen as an exemplary town hall for the 20th century, a municipal factory characterized by the transparency of the counter hall with its three levels of suspended galleries.
Hotel de Ville de Boulogne Billancourt (Hauts de Seine). Architect Tony Garnier (1869-1948), 1931-1934. Built of weapon concrete, the building is seen as an exemplary town hall for the 20th century, a municipal factory characterized by the transparency of the counter hall with its three levels of suspended galleries.

MDA4652906: Hotel de Ville de Boulogne Billancourt (Hauts de Seine). Architect Tony Garnier (1869-1948), 1931-1934. Built of weapon concrete, the building is seen as an exemplary town hall for the 20th century, a municipal factory characterized by the transparency of the counter hall with its three levels of suspended galleries., Garnier, Tony (1869-1948) / Bridgeman Images

ID: MDA4652906

Hotel de Ville de Boulogne Billancourt (Hauts de Seine). Architect Tony Garnier (1869-1948), 1931-1934. Built of weapon concrete, the building is seen as an exemplary town hall for the 20th century, a municipal factory characterized by the transparency of the counter hall with its three levels of suspended galleries.

Garnier, Tony (1869-1948)

Hotel de Ville de Boulogne Billancourt (Hauts de Seine). Architect Tony Garnier (1869-1948), 1931-1934. Built of weapon concrete, the building is seen as an exemplary town hall for the 20th century, a municipal factory characterized by the transparency of the counter hall with its three levels of suspended galleries.
Hotel de Ville de Boulogne Billancourt (Hauts de Seine). Architect Tony Garnier (1869-1948), 1931-1934. Built of weapon concrete, the building is seen as an exemplary town hall for the 20th century, a municipal factory characterized by the transparency of the counter hall with its three levels of suspended galleries.

MDA4652970: Hotel de Ville de Boulogne Billancourt (Hauts de Seine). Architect Tony Garnier (1869-1948), 1931-1934. Built of weapon concrete, the building is seen as an exemplary town hall for the 20th century, a municipal factory characterized by the transparency of the counter hall with its three levels of suspended galleries., Garnier, Tony (1869-1948) / Bridgeman Images

ID: MDA4652970

Hotel de Ville de Boulogne Billancourt (Hauts de Seine). Architect Tony Garnier (1869-1948), 1931-1934. Built of weapon concrete, the building is seen as an exemplary town hall for the 20th century, a municipal factory characterized by the transparency of the counter hall with its three levels of suspended galleries.

Garnier, Tony (1869-1948)

Accommodation, 65 rue La Fontaine in Paris 75016. Architect Henri Sauvage (1873-1932), realisation 1926-1928.Known as the Studio Building, this remarkable building is made up of fifty duplex apartments each containing an artist's studio. Ceram gres coating by Gentil and Bourdet.
Accommodation, 65 rue La Fontaine in Paris 75016. Architect Henri Sauvage (1873-1932), realisation 1926-1928.Known as the Studio Building, this remarkable building is made up of fifty duplex apartments each containing an artist's studio. Ceram gres coating by Gentil and Bourdet.

TEC4652969: Accommodation, 65 rue La Fontaine in Paris 75016. Architect Henri Sauvage (1873-1932), realisation 1926-1928.Known as the Studio Building, this remarkable building is made up of fifty duplex apartments each containing an artist's studio. Ceram gres coating by Gentil and Bourdet. / Bridgeman Images

ID: TEC4652969

Accommodation, 65 rue La Fontaine in Paris 75016. Architect Henri Sauvage (1873-1932), realisation 1926-1928.Known as the Studio Building, this remarkable building is made up of fifty duplex apartments each containing an artist's studio. Ceram gres coating by Gentil and Bourdet.

Accommodation, 65 rue La Fontaine in Paris 75016. Architect Henri Sauvage (1873-1932), realisation 1926-1928.Known as the Studio Building, this remarkable building is made up of fifty duplex apartments each containing an artist's studio. Ceram gres coating by Gentil and Bourdet.
Accommodation, 65 rue La Fontaine in Paris 75016. Architect Henri Sauvage (1873-1932), realisation 1926-1928.Known as the Studio Building, this remarkable building is made up of fifty duplex apartments each containing an artist's studio. Ceram gres coating by Gentil and Bourdet.

TEC4652977: Accommodation, 65 rue La Fontaine in Paris 75016. Architect Henri Sauvage (1873-1932), realisation 1926-1928.Known as the Studio Building, this remarkable building is made up of fifty duplex apartments each containing an artist's studio. Ceram gres coating by Gentil and Bourdet. / Bridgeman Images

ID: TEC4652977

Accommodation, 65 rue La Fontaine in Paris 75016. Architect Henri Sauvage (1873-1932), realisation 1926-1928.Known as the Studio Building, this remarkable building is made up of fifty duplex apartments each containing an artist's studio. Ceram gres coating by Gentil and Bourdet.

Accommodation, 65 rue La Fontaine in Paris 75016. Architect Henri Sauvage (1873-1932), realisation 1926-1928.Known as the Studio Building, this remarkable building is made up of fifty duplex apartments each containing an artist's studio. Ceram gres coating by Gentil and Bourdet.
Accommodation, 65 rue La Fontaine in Paris 75016. Architect Henri Sauvage (1873-1932), realisation 1926-1928.Known as the Studio Building, this remarkable building is made up of fifty duplex apartments each containing an artist's studio. Ceram gres coating by Gentil and Bourdet.

TEC4653001: Accommodation, 65 rue La Fontaine in Paris 75016. Architect Henri Sauvage (1873-1932), realisation 1926-1928.Known as the Studio Building, this remarkable building is made up of fifty duplex apartments each containing an artist's studio. Ceram gres coating by Gentil and Bourdet. / Bridgeman Images

ID: TEC4653001

Accommodation, 65 rue La Fontaine in Paris 75016. Architect Henri Sauvage (1873-1932), realisation 1926-1928.Known as the Studio Building, this remarkable building is made up of fifty duplex apartments each containing an artist's studio. Ceram gres coating by Gentil and Bourdet.

Hotel de Ville de Boulogne Billancourt (Hauts de Seine). Architect Tony Garnier (1869-1948), 1931-1934. Built of weapon concrete, the building is seen as an exemplary town hall for the 20th century, a municipal factory characterized by the transparency of the counter hall with its three levels of suspended galleries.
Hotel de Ville de Boulogne Billancourt (Hauts de Seine). Architect Tony Garnier (1869-1948), 1931-1934. Built of weapon concrete, the building is seen as an exemplary town hall for the 20th century, a municipal factory characterized by the transparency of the counter hall with its three levels of suspended galleries.

TEC4652782: Hotel de Ville de Boulogne Billancourt (Hauts de Seine). Architect Tony Garnier (1869-1948), 1931-1934. Built of weapon concrete, the building is seen as an exemplary town hall for the 20th century, a municipal factory characterized by the transparency of the counter hall with its three levels of suspended galleries., Garnier, Tony (1869-1948) / Bridgeman Images

ID: TEC4652782

Hotel de Ville de Boulogne Billancourt (Hauts de Seine). Architect Tony Garnier (1869-1948), 1931-1934. Built of weapon concrete, the building is seen as an exemplary town hall for the 20th century, a municipal factory characterized by the transparency of the counter hall with its three levels of suspended galleries.

Garnier, Tony (1869-1948)

Hotel de Ville de Boulogne Billancourt (Hauts de Seine). Architect Tony Garnier (1869-1948), 1931-1934. Built of weapon concrete, the building is seen as an exemplary town hall for the 20th century, a municipal factory characterized by the transparency of the counter hall with its three levels of suspended galleries.
Hotel de Ville de Boulogne Billancourt (Hauts de Seine). Architect Tony Garnier (1869-1948), 1931-1934. Built of weapon concrete, the building is seen as an exemplary town hall for the 20th century, a municipal factory characterized by the transparency of the counter hall with its three levels of suspended galleries.

MDA4652830: Hotel de Ville de Boulogne Billancourt (Hauts de Seine). Architect Tony Garnier (1869-1948), 1931-1934. Built of weapon concrete, the building is seen as an exemplary town hall for the 20th century, a municipal factory characterized by the transparency of the counter hall with its three levels of suspended galleries., Garnier, Tony (1869-1948) / Bridgeman Images

ID: MDA4652830

Hotel de Ville de Boulogne Billancourt (Hauts de Seine). Architect Tony Garnier (1869-1948), 1931-1934. Built of weapon concrete, the building is seen as an exemplary town hall for the 20th century, a municipal factory characterized by the transparency of the counter hall with its three levels of suspended galleries.

Garnier, Tony (1869-1948)

Theatre accessories: fan and binoculars. 18th century. Paris, decorative arts (photo)
Theatre accessories: fan and binoculars. 18th century. Paris, decorative arts (photo)

JLJ4652918: Theatre accessories: fan and binoculars. 18th century. Paris, decorative arts (photo), Unknown artist, (18th century) / Bridgeman Images

ID: JLJ4652918

Theatre accessories: fan and binoculars. 18th century. Paris, decorative arts (photo)

Unknown artist, (18th century)

Hotel de Ville de Boulogne Billancourt (Hauts de Seine). Architect Tony Garnier (1869-1948), 1931-1934. Built of weapon concrete, the building is seen as an exemplary town hall for the 20th century, a municipal factory characterized by the transparency of the counter hall with its three levels of suspended galleries.
Hotel de Ville de Boulogne Billancourt (Hauts de Seine). Architect Tony Garnier (1869-1948), 1931-1934. Built of weapon concrete, the building is seen as an exemplary town hall for the 20th century, a municipal factory characterized by the transparency of the counter hall with its three levels of suspended galleries.

MDA4652931: Hotel de Ville de Boulogne Billancourt (Hauts de Seine). Architect Tony Garnier (1869-1948), 1931-1934. Built of weapon concrete, the building is seen as an exemplary town hall for the 20th century, a municipal factory characterized by the transparency of the counter hall with its three levels of suspended galleries., Garnier, Tony (1869-1948) / Bridgeman Images

ID: MDA4652931

Hotel de Ville de Boulogne Billancourt (Hauts de Seine). Architect Tony Garnier (1869-1948), 1931-1934. Built of weapon concrete, the building is seen as an exemplary town hall for the 20th century, a municipal factory characterized by the transparency of the counter hall with its three levels of suspended galleries.

Garnier, Tony (1869-1948)

View of the island of Saint Helene with the tomb of Emperor Napoleon I (1769-1821) Watercolour c.1821, 19th century (watercolour)
View of the island of Saint Helene with the tomb of Emperor Napoleon I (1769-1821) Watercolour c.1821, 19th century (watercolour)

JLJ4652959: View of the island of Saint Helene with the tomb of Emperor Napoleon I (1769-1821) Watercolour c.1821, 19th century (watercolour), French School, (19th century) / Bridgeman Images

ID: JLJ4652959

View of the island of Saint Helene with the tomb of Emperor Napoleon I (1769-1821) Watercolour c.1821, 19th century (watercolour)

French School, (19th century)

Milky Way above Cerro Armazones - Star sky at the top of Cerro Armazones. This 3060-metre mountain in Chile will host the giant telescope E - ELT (European Extremely Large Telescope). The construction of this 42-metre telescope is expected to start at the end of 2010 and will be inaugurated around 2018. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. On 26 April 2010, the ESO Council selected Cerro Armazones as the baseline site for the planned 42 - metre European Extremely Large Telescope (E - ELT). Cerro Armazones is a mountain at an altitude of 3060 metres in the central part of Child's Atacama Desert, some 130 kilometres south of the town of Antofagasta and about 20 kilometres from Cerro Paranal, home of Eso's Very Large Telescope
Milky Way above Cerro Armazones - Star sky at the top of Cerro Armazones. This 3060-metre mountain in Chile will host the giant telescope E - ELT (European Extremely Large Telescope). The construction of this 42-metre telescope is expected to start at the end of 2010 and will be inaugurated around 2018. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. On 26 April 2010, the ESO Council selected Cerro Armazones as the baseline site for the planned 42 - metre European Extremely Large Telescope (E - ELT). Cerro Armazones is a mountain at an altitude of 3060 metres in the central part of Child's Atacama Desert, some 130 kilometres south of the town of Antofagasta and about 20 kilometres from Cerro Paranal, home of Eso's Very Large Telescope

PIX4652988: Milky Way above Cerro Armazones - Star sky at the top of Cerro Armazones. This 3060-metre mountain in Chile will host the giant telescope E - ELT (European Extremely Large Telescope). The construction of this 42-metre telescope is expected to start at the end of 2010 and will be inaugurated around 2018. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. On 26 April 2010, the ESO Council selected Cerro Armazones as the baseline site for the planned 42 - metre European Extremely Large Telescope (E - ELT). Cerro Armazones is a mountain at an altitude of 3060 metres in the central part of Child's Atacama Desert, some 130 kilometres south of the town of Antofagasta and about 20 kilometres from Cerro Paranal, home of Eso's Very Large Telescope / Bridgeman Images

ID: PIX4652988

Milky Way above Cerro Armazones - Star sky at the top of Cerro Armazones. This 3060-metre mountain in Chile will host the giant telescope E - ELT (European Extremely Large Telescope). The construction of this 42-metre telescope is expected to start at the end of 2010 and will be inaugurated around 2018. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. On 26 April 2010, the ESO Council selected Cerro Armazones as the baseline site for the planned 42 - metre European Extremely Large Telescope (E - ELT). Cerro Armazones is a mountain at an altitude of 3060 metres in the central part of Child's Atacama Desert, some 130 kilometres south of the town of Antofagasta and about 20 kilometres from Cerro Paranal, home of Eso's Very Large Telescope

Telescope E - ELT - Artist's view - European Extremely Large Telescope - Artwork - Artist's view of the E - ELT (European Extremely Large Telescope), a telescope project measuring 42 metres in diameter. Construction of this European project could start in 2010, with a planned inauguration around 2017. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. With a 42 - m diameter primary mirror, the present baseline, its total rotating mass is 5500 tons. The two platforms on each side of the structure hold large instruments. The telescope features a novel, innovative design, based on 5 mirrors. The primary 42 - m mirror is composed of 906 segments, each 1.45 m wide, while the secondary mirror is as large as 6 m in diameter. A tertiary mirror, 4.2 m in diameter, relays the light to the adaptive optics system, composed of two mirrors: a 2.5 - m mirror supported by 5000 or more actuators so as to be able to distort its own shape a thousand times per second, and one 2.7 m in diameter that allows for the final image corrections. This five mirror approach results in an exceptional image quality, with no significant aberrations in the field of view
Telescope E - ELT - Artist's view - European Extremely Large Telescope - Artwork - Artist's view of the E - ELT (European Extremely Large Telescope), a telescope project measuring 42 metres in diameter. Construction of this European project could start in 2010, with a planned inauguration around 2017. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. With a 42 - m diameter primary mirror, the present baseline, its total rotating mass is 5500 tons. The two platforms on each side of the structure hold large instruments. The telescope features a novel, innovative design, based on 5 mirrors. The primary 42 - m mirror is composed of 906 segments, each 1.45 m wide, while the secondary mirror is as large as 6 m in diameter. A tertiary mirror, 4.2 m in diameter, relays the light to the adaptive optics system, composed of two mirrors: a 2.5 - m mirror supported by 5000 or more actuators so as to be able to distort its own shape a thousand times per second, and one 2.7 m in diameter that allows for the final image corrections. This five mirror approach results in an exceptional image quality, with no significant aberrations in the field of view

PIX4653068: Telescope E - ELT - Artist's view - European Extremely Large Telescope - Artwork - Artist's view of the E - ELT (European Extremely Large Telescope), a telescope project measuring 42 metres in diameter. Construction of this European project could start in 2010, with a planned inauguration around 2017. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. With a 42 - m diameter primary mirror, the present baseline, its total rotating mass is 5500 tons. The two platforms on each side of the structure hold large instruments. The telescope features a novel, innovative design, based on 5 mirrors. The primary 42 - m mirror is composed of 906 segments, each 1.45 m wide, while the secondary mirror is as large as 6 m in diameter. A tertiary mirror, 4.2 m in diameter, relays the light to the adaptive optics system, composed of two mirrors: a 2.5 - m mirror supported by 5000 or more actuators so as to be able to distort its own shape a thousand times per second, and one 2.7 m in diameter that allows for the final image corrections. This five mirror approach results in an exceptional image quality, with no significant aberrations in the field of view / Bridgeman Images

ID: PIX4653068

Telescope E - ELT - Artist's view - European Extremely Large Telescope - Artwork - Artist's view of the E - ELT (European Extremely Large Telescope), a telescope project measuring 42 metres in diameter. Construction of this European project could start in 2010, with a planned inauguration around 2017. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. With a 42 - m diameter primary mirror, the present baseline, its total rotating mass is 5500 tons. The two platforms on each side of the structure hold large instruments. The telescope features a novel, innovative design, based on 5 mirrors. The primary 42 - m mirror is composed of 906 segments, each 1.45 m wide, while the secondary mirror is as large as 6 m in diameter. A tertiary mirror, 4.2 m in diameter, relays the light to the adaptive optics system, composed of two mirrors: a 2.5 - m mirror supported by 5000 or more actuators so as to be able to

Telescope ELT - Artist's view. - 3 - dimensional model of the European Extremely Large Telescope - Artist's view of the ELT (Extremely Large Telescope), a telescope project measuring 42 metres in diameter. Construction of this European project could start in 2010, with a planned inauguration around 2017. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. With a 42 - m diameter primary mirror, the present baseline, its total rotating mass is 5500 tons. The two platforms on each side of the structure hold large instruments. The telescope features a novel, innovative design, based on 5 mirrors. The primary 42 - m mirror is composed of 906 segments, each 1.45 m wide, while the secondary mirror is as large as 6 m in diameter. A tertiary mirror, 4.2 m in diameter, relays the light to the adaptive optics system, composed of two mirrors: a 2.5 - m mirror supported by 5000 or more actuators so as to be able to distort its own shape a thousand times per second, and one 2.7 m in diameter that allows for the final image corrections. This five mirror approach results in an exceptional image quality, with no significant aberrations in the field of view
Telescope ELT - Artist's view. - 3 - dimensional model of the European Extremely Large Telescope - Artist's view of the ELT (Extremely Large Telescope), a telescope project measuring 42 metres in diameter. Construction of this European project could start in 2010, with a planned inauguration around 2017. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. With a 42 - m diameter primary mirror, the present baseline, its total rotating mass is 5500 tons. The two platforms on each side of the structure hold large instruments. The telescope features a novel, innovative design, based on 5 mirrors. The primary 42 - m mirror is composed of 906 segments, each 1.45 m wide, while the secondary mirror is as large as 6 m in diameter. A tertiary mirror, 4.2 m in diameter, relays the light to the adaptive optics system, composed of two mirrors: a 2.5 - m mirror supported by 5000 or more actuators so as to be able to distort its own shape a thousand times per second, and one 2.7 m in diameter that allows for the final image corrections. This five mirror approach results in an exceptional image quality, with no significant aberrations in the field of view

PIX4653083: Telescope ELT - Artist's view. - 3 - dimensional model of the European Extremely Large Telescope - Artist's view of the ELT (Extremely Large Telescope), a telescope project measuring 42 metres in diameter. Construction of this European project could start in 2010, with a planned inauguration around 2017. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. With a 42 - m diameter primary mirror, the present baseline, its total rotating mass is 5500 tons. The two platforms on each side of the structure hold large instruments. The telescope features a novel, innovative design, based on 5 mirrors. The primary 42 - m mirror is composed of 906 segments, each 1.45 m wide, while the secondary mirror is as large as 6 m in diameter. A tertiary mirror, 4.2 m in diameter, relays the light to the adaptive optics system, composed of two mirrors: a 2.5 - m mirror supported by 5000 or more actuators so as to be able to distort its own shape a thousand times per second, and one 2.7 m in diameter that allows for the final image corrections. This five mirror approach results in an exceptional image quality, with no significant aberrations in the field of view / Bridgeman Images

ID: PIX4653083

Telescope ELT - Artist's view. - 3 - dimensional model of the European Extremely Large Telescope - Artist's view of the ELT (Extremely Large Telescope), a telescope project measuring 42 metres in diameter. Construction of this European project could start in 2010, with a planned inauguration around 2017. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. With a 42 - m diameter primary mirror, the present baseline, its total rotating mass is 5500 tons. The two platforms on each side of the structure hold large instruments. The telescope features a novel, innovative design, based on 5 mirrors. The primary 42 - m mirror is composed of 906 segments, each 1.45 m wide, while the secondary mirror is as large as 6 m in diameter. A tertiary mirror, 4.2 m in diameter, relays the light to the adaptive optics system, composed of two mirrors: a 2.5 - m mirror supported by 5000 or more actuators so as to be able

Representation of Saint James the Major in pelerine Sculpture in limestone of the Burgundy school, 1475-1500 (limestone)
Representation of Saint James the Major in pelerine Sculpture in limestone of the Burgundy school, 1475-1500 (limestone)

JLJ4653103: Representation of Saint James the Major in pelerine Sculpture in limestone of the Burgundy school, 1475-1500 (limestone), French School, (15th century) / Bridgeman Images

ID: JLJ4653103

Representation of Saint James the Major in pelerine Sculpture in limestone of the Burgundy school, 1475-1500 (limestone)

French School, (15th century)

Bauhaus building in Dessau (Germany) designed in 1925 (photo)
Bauhaus building in Dessau (Germany) designed in 1925 (photo)

TEC4653155: Bauhaus building in Dessau (Germany) designed in 1925 (photo) / Bridgeman Images

ID: TEC4653155

Bauhaus building in Dessau (Germany) designed in 1925 (photo)

The stained glass windows by Fernand Leger (1881-1955) and the tapestry by Jean Lurcat (1892-1966), in the church of Saint Germain d'Auxerre in Courfaivre in Switzerland. Photography 2000.
The stained glass windows by Fernand Leger (1881-1955) and the tapestry by Jean Lurcat (1892-1966), in the church of Saint Germain d'Auxerre in Courfaivre in Switzerland. Photography 2000.

JSN4653264: The stained glass windows by Fernand Leger (1881-1955) and the tapestry by Jean Lurcat (1892-1966), in the church of Saint Germain d'Auxerre in Courfaivre in Switzerland. Photography 2000., Leger, Fernand (1881-1955) / Bridgeman Images

ID: JSN4653264

The stained glass windows by Fernand Leger (1881-1955) and the tapestry by Jean Lurcat (1892-1966), in the church of Saint Germain d'Auxerre in Courfaivre in Switzerland. Photography 2000.

Leger, Fernand (1881-1955)

The Merchant of Eventails, 18th century (oil on canvas)
The Merchant of Eventails, 18th century (oil on canvas)

JLJ4653280: The Merchant of Eventails, 18th century (oil on canvas), Castillo, Jose del (1737-93) / Bridgeman Images

ID: JLJ4653280

The Merchant of Eventails, 18th century (oil on canvas)

Castillo, Jose del (1737-93)

Gamma ray telescope HESS - Gamma rays telescope HESS - High Energy Stereoscopic System (HESS) telescope located in Namibia near Gamsberg. This network of telescopes is dedicated to the study of high energy gamma rays. High Energy Stereoscopic System or HESS is a system of Imaging Atmospheric Cherenkov Telescopes (IACT) for the investigation of cosmic gamma rays. It is located in Namibia, near Gamsberg
Gamma ray telescope HESS - Gamma rays telescope HESS - High Energy Stereoscopic System (HESS) telescope located in Namibia near Gamsberg. This network of telescopes is dedicated to the study of high energy gamma rays. High Energy Stereoscopic System or HESS is a system of Imaging Atmospheric Cherenkov Telescopes (IACT) for the investigation of cosmic gamma rays. It is located in Namibia, near Gamsberg

PIX4653309: Gamma ray telescope HESS - Gamma rays telescope HESS - High Energy Stereoscopic System (HESS) telescope located in Namibia near Gamsberg. This network of telescopes is dedicated to the study of high energy gamma rays. High Energy Stereoscopic System or HESS is a system of Imaging Atmospheric Cherenkov Telescopes (IACT) for the investigation of cosmic gamma rays. It is located in Namibia, near Gamsberg / Bridgeman Images

ID: PIX4653309

Gamma ray telescope HESS - Gamma rays telescope HESS - High Energy Stereoscopic System (HESS) telescope located in Namibia near Gamsberg. This network of telescopes is dedicated to the study of high energy gamma rays. High Energy Stereoscopic System or HESS is a system of Imaging Atmospheric Cherenkov Telescopes (IACT) for the investigation of cosmic gamma rays. It is located in Namibia, near Gamsberg

Mirrors of one of the gamma ray telescopes HESS - Mirror of Gamma rays telescope HESS - Telescope of the High Energy Stereoscopic System (HESS) network located in Namibia near Gamsberg. This network of telescopes is dedicated to the study of high energy gamma rays. High Energy Stereoscopic System or HESS is a system of Imaging Atmospheric Cherenkov Telescopes (IACT) for the investigation of cosmic gamma rays. It is located in Namibia, near Gamsberg
Mirrors of one of the gamma ray telescopes HESS - Mirror of Gamma rays telescope HESS - Telescope of the High Energy Stereoscopic System (HESS) network located in Namibia near Gamsberg. This network of telescopes is dedicated to the study of high energy gamma rays. High Energy Stereoscopic System or HESS is a system of Imaging Atmospheric Cherenkov Telescopes (IACT) for the investigation of cosmic gamma rays. It is located in Namibia, near Gamsberg

PIX4653323: Mirrors of one of the gamma ray telescopes HESS - Mirror of Gamma rays telescope HESS - Telescope of the High Energy Stereoscopic System (HESS) network located in Namibia near Gamsberg. This network of telescopes is dedicated to the study of high energy gamma rays. High Energy Stereoscopic System or HESS is a system of Imaging Atmospheric Cherenkov Telescopes (IACT) for the investigation of cosmic gamma rays. It is located in Namibia, near Gamsberg / Bridgeman Images

ID: PIX4653323

Mirrors of one of the gamma ray telescopes HESS - Mirror of Gamma rays telescope HESS - Telescope of the High Energy Stereoscopic System (HESS) network located in Namibia near Gamsberg. This network of telescopes is dedicated to the study of high energy gamma rays. High Energy Stereoscopic System or HESS is a system of Imaging Atmospheric Cherenkov Telescopes (IACT) for the investigation of cosmic gamma rays. It is located in Namibia, near Gamsberg

The last supper, c. 1250 (High relief)
The last supper, c. 1250 (High relief)

LRI4653333: The last supper, c. 1250 (High relief), German School, (13th century) / Bridgeman Images

ID: LRI4653333

The last supper, c. 1250 (High relief)

German School, (13th century)

View of the antiquarium of the Royal Palace, 1569-1586 (photography)
View of the antiquarium of the Royal Palace, 1569-1586 (photography)

LRI4653345: View of the antiquarium of the Royal Palace, 1569-1586 (photography), Sustris, Friedrich (c.1540-99) / Bridgeman Images

ID: LRI4653345

View of the antiquarium of the Royal Palace, 1569-1586 (photography)

Sustris, Friedrich (c.1540-99)

Telescope E - ELT - Artist's view - European Extremely Large Telescope - Artwork - Artist's view of the E - ELT (European Extremely Large Telescope), a telescope project measuring 42 metres in diameter. Construction of this European project could start in 2010, with a planned inauguration around 2017. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. With a 42 - m diameter primary mirror, the present baseline, its total rotating mass is 5500 tons. The two platforms on each side of the structure hold large instruments. The telescope features a novel, innovative design, based on 5 mirrors. The primary 42 - m mirror is composed of 906 segments, each 1.45 m wide, while the secondary mirror is as large as 6 m in diameter. A tertiary mirror, 4.2 m in diameter, relays the light to the adaptive optics system, composed of two mirrors: a 2.5 - m mirror supported by 5000 or more actuators so as to be able to distort its own shape a thousand times per second, and one 2.7 m in diameter that allows for the final image corrections. This five mirror approach results in an exceptional image quality, with no significant aberrations in the field of view
Telescope E - ELT - Artist's view - European Extremely Large Telescope - Artwork - Artist's view of the E - ELT (European Extremely Large Telescope), a telescope project measuring 42 metres in diameter. Construction of this European project could start in 2010, with a planned inauguration around 2017. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. With a 42 - m diameter primary mirror, the present baseline, its total rotating mass is 5500 tons. The two platforms on each side of the structure hold large instruments. The telescope features a novel, innovative design, based on 5 mirrors. The primary 42 - m mirror is composed of 906 segments, each 1.45 m wide, while the secondary mirror is as large as 6 m in diameter. A tertiary mirror, 4.2 m in diameter, relays the light to the adaptive optics system, composed of two mirrors: a 2.5 - m mirror supported by 5000 or more actuators so as to be able to distort its own shape a thousand times per second, and one 2.7 m in diameter that allows for the final image corrections. This five mirror approach results in an exceptional image quality, with no significant aberrations in the field of view

PIX4653061: Telescope E - ELT - Artist's view - European Extremely Large Telescope - Artwork - Artist's view of the E - ELT (European Extremely Large Telescope), a telescope project measuring 42 metres in diameter. Construction of this European project could start in 2010, with a planned inauguration around 2017. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. With a 42 - m diameter primary mirror, the present baseline, its total rotating mass is 5500 tons. The two platforms on each side of the structure hold large instruments. The telescope features a novel, innovative design, based on 5 mirrors. The primary 42 - m mirror is composed of 906 segments, each 1.45 m wide, while the secondary mirror is as large as 6 m in diameter. A tertiary mirror, 4.2 m in diameter, relays the light to the adaptive optics system, composed of two mirrors: a 2.5 - m mirror supported by 5000 or more actuators so as to be able to distort its own shape a thousand times per second, and one 2.7 m in diameter that allows for the final image corrections. This five mirror approach results in an exceptional image quality, with no significant aberrations in the field of view / Bridgeman Images

ID: PIX4653061

Telescope E - ELT - Artist's view - European Extremely Large Telescope - Artwork - Artist's view of the E - ELT (European Extremely Large Telescope), a telescope project measuring 42 metres in diameter. Construction of this European project could start in 2010, with a planned inauguration around 2017. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. With a 42 - m diameter primary mirror, the present baseline, its total rotating mass is 5500 tons. The two platforms on each side of the structure hold large instruments. The telescope features a novel, innovative design, based on 5 mirrors. The primary 42 - m mirror is composed of 906 segments, each 1.45 m wide, while the secondary mirror is as large as 6 m in diameter. A tertiary mirror, 4.2 m in diameter, relays the light to the adaptive optics system, composed of two mirrors: a 2.5 - m mirror supported by 5000 or more actuators so as to be able to

Bauhaus building in Dessau (Germany) designed in 1925 (photo)
Bauhaus building in Dessau (Germany) designed in 1925 (photo)

TEC4653136: Bauhaus building in Dessau (Germany) designed in 1925 (photo) / Bridgeman Images

ID: TEC4653136

Bauhaus building in Dessau (Germany) designed in 1925 (photo)

Circle Gallery Building in San Francisco, California (United States). Architect Frank Lloyd Wright (1867-1959), 1949.
Circle Gallery Building in San Francisco, California (United States). Architect Frank Lloyd Wright (1867-1959), 1949.

LBY4653205: Circle Gallery Building in San Francisco, California (United States). Architect Frank Lloyd Wright (1867-1959), 1949., Wright, Frank Lloyd (1867-1959) / Bridgeman Images

ID: LBY4653205

Circle Gallery Building in San Francisco, California (United States). Architect Frank Lloyd Wright (1867-1959), 1949.

Wright, Frank Lloyd (1867-1959)

View of the Royal Salon, 1734-1739 (photography)
View of the Royal Salon, 1734-1739 (photography)

LRI4653273: View of the Royal Salon, 1734-1739 (photography), Cuvillies, Francois de (1695-1768) / Bridgeman Images

ID: LRI4653273

View of the Royal Salon, 1734-1739 (photography)

Cuvillies, Francois de (1695-1768)

View of the interior of the Royal Palace, 1751-1755 (photography)
View of the interior of the Royal Palace, 1751-1755 (photography)

LRI4653283: View of the interior of the Royal Palace, 1751-1755 (photography), Cuvillies, Francois de (1695-1768) / Bridgeman Images

ID: LRI4653283

View of the interior of the Royal Palace, 1751-1755 (photography)

Cuvillies, Francois de (1695-1768)

View of the interior of the royal palace, 1728-1730 (photography)
View of the interior of the royal palace, 1728-1730 (photography)

LRI4653304: View of the interior of the royal palace, 1728-1730 (photography), Zimmermann, Johann Baptist (1680-1758) / Bridgeman Images

ID: LRI4653304

View of the interior of the royal palace, 1728-1730 (photography)

Zimmermann, Johann Baptist (1680-1758)

The church of Notre Dame de Tout Grace at the Plateau d'Assy in Passy (Haute Savoie). Architect Maurice Novarina (1907-2002), 1946. Decor Fernand Leger (1881-1955). The village, located at 1200 meters above sea level, was the village of sanatoriums. In 1935, Canon Devemy, Chaplain of the Sanatarium of Sancellemoz, had the idea of building the church of the sick on the Plateau d'Assy. The entrance facade recalls the famous and robust Savoyard chalets of the Vallee d'Abondance built with the stone of the country. Photography 1989.
The church of Notre Dame de Tout Grace at the Plateau d'Assy in Passy (Haute Savoie). Architect Maurice Novarina (1907-2002), 1946. Decor Fernand Leger (1881-1955). The village, located at 1200 meters above sea level, was the village of sanatoriums. In 1935, Canon Devemy, Chaplain of the Sanatarium of Sancellemoz, had the idea of building the church of the sick on the Plateau d'Assy. The entrance facade recalls the famous and robust Savoyard chalets of the Vallee d'Abondance built with the stone of the country. Photography 1989.

JSN4653318: The church of Notre Dame de Tout Grace at the Plateau d'Assy in Passy (Haute Savoie). Architect Maurice Novarina (1907-2002), 1946. Decor Fernand Leger (1881-1955). The village, located at 1200 meters above sea level, was the village of sanatoriums. In 1935, Canon Devemy, Chaplain of the Sanatarium of Sancellemoz, had the idea of building the church of the sick on the Plateau d'Assy. The entrance facade recalls the famous and robust Savoyard chalets of the Vallee d'Abondance built with the stone of the country. Photography 1989., Leger, Fernand (1881-1955) / Bridgeman Images

ID: JSN4653318

The church of Notre Dame de Tout Grace at the Plateau d'Assy in Passy (Haute Savoie). Architect Maurice Novarina (1907-2002), 1946. Decor Fernand Leger (1881-1955). The village, located at 1200 meters above sea level, was the village of sanatoriums. In 1935, Canon Devemy, Chaplain of the Sanatarium of Sancellemoz, had the idea of building the church of the sick on the Plateau d'Assy. The entrance facade recalls the famous and robust Savoyard chalets of the Vallee d'Abondance built with the stone of the country. Photography 1989.

Leger, Fernand (1881-1955)


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