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Le Peer Trianon a Versailles, architect Jacques Anges Gabriel, 1760-1764. Parc du Chateau de Versailles (Yvelines, Ile de France).
Le Peer Trianon a Versailles, architect Jacques Anges Gabriel, 1760-1764. Parc du Chateau de Versailles (Yvelines, Ile de France).

TEC4561685: Le Peer Trianon a Versailles, architect Jacques Anges Gabriel, 1760-1764. Parc du Chateau de Versailles (Yvelines, Ile de France). / Bridgeman Images

Vault with Corinthian columns of LaChapelle royale began by Jules Hardouin Mansart (1646-1708) in 1699 and completed in 1710 by Robert De Cotte (1656-1735).Chateau de Versailles (Les Yvelines). Principal architects: Louis Le Vau (1612-1670) and Jules Hardouin Mansart (1646-1708), 1660-1700.
Vault with Corinthian columns of LaChapelle royale began by Jules Hardouin Mansart (1646-1708) in 1699 and completed in 1710 by Robert De Cotte (1656-1735).Chateau de Versailles (Les Yvelines). Principal architects: Louis Le Vau (1612-1670) and Jules Hardouin Mansart (1646-1708), 1660-1700.

ITR4561887: Vault with Corinthian columns of LaChapelle royale began by Jules Hardouin Mansart (1646-1708) in 1699 and completed in 1710 by Robert De Cotte (1656-1735).Chateau de Versailles (Les Yvelines). Principal architects: Louis Le Vau (1612-1670) and Jules Hardouin Mansart (1646-1708), 1660-1700. / Bridgeman Images

La Colonnade in the Parc du Chateau de Versailles (Les Yvelines), 1660-1700. Gardens of Andre Le Notre (1613-1700) and principal architects: Louis Le Vau (1612-1670) and Jules Hardouin Mansart (1646-1708).
La Colonnade in the Parc du Chateau de Versailles (Les Yvelines), 1660-1700. Gardens of Andre Le Notre (1613-1700) and principal architects: Louis Le Vau (1612-1670) and Jules Hardouin Mansart (1646-1708).

ITR4561970: La Colonnade in the Parc du Chateau de Versailles (Les Yvelines), 1660-1700. Gardens of Andre Le Notre (1613-1700) and principal architects: Louis Le Vau (1612-1670) and Jules Hardouin Mansart (1646-1708). / Bridgeman Images

Apollo basin. Chateau de Versailles (Les Yvelines), 1660-1700. Gardens of Andre Le Notre (1613-1700) and principal architects: Louis Le Vau (1612-1670) and Jules Hardouin Mansart (1646-1708).
Apollo basin. Chateau de Versailles (Les Yvelines), 1660-1700. Gardens of Andre Le Notre (1613-1700) and principal architects: Louis Le Vau (1612-1670) and Jules Hardouin Mansart (1646-1708).

ITR4562018: Apollo basin. Chateau de Versailles (Les Yvelines), 1660-1700. Gardens of Andre Le Notre (1613-1700) and principal architects: Louis Le Vau (1612-1670) and Jules Hardouin Mansart (1646-1708). / Bridgeman Images

Belem Tower in Lisbon (Portugal), built in 1521.
Belem Tower in Lisbon (Portugal), built in 1521.

LBY4562222: Belem Tower in Lisbon (Portugal), built in 1521. / Bridgeman Images

The Port of Hong Kong (China)
The Port of Hong Kong (China)

TEC4562306: The Port of Hong Kong (China) / Bridgeman Images

Kowloon District, Hong Kong, China.
Kowloon District, Hong Kong, China.

TEC4562350: Kowloon District, Hong Kong, China. / Bridgeman Images

Victoria Island to Hong Kong (China).
Victoria Island to Hong Kong (China).

TEC4562407: Victoria Island to Hong Kong (China). / Bridgeman Images

Hong Kong City Hong Kong - China -
Hong Kong City Hong Kong - China -

TEC4562577: Hong Kong City Hong Kong - China - / Bridgeman Images

Hong Kong City Hong Kong - China -
Hong Kong City Hong Kong - China -

TEC4562622: Hong Kong City Hong Kong - China - / Bridgeman Images

Kinkaku-ji Temple, a gold-covered building, in Kyoto, Japan.
Kinkaku-ji Temple, a gold-covered building, in Kyoto, Japan.

TEC4562783: Kinkaku-ji Temple, a gold-covered building, in Kyoto, Japan. / Bridgeman Images

Frontispiece of the score for the opera Alessandro Nell'Indie by Johan Christian Bach (Fac-simile from the original of 1761)
Frontispiece of the score for the opera Alessandro Nell'Indie by Johan Christian Bach (Fac-simile from the original of 1761)

LRI4562881: Frontispiece of the score for the opera Alessandro Nell'Indie by Johan Christian Bach (Fac-simile from the original of 1761) / Bridgeman Images

Tenryu-ji, a Buddhist temple in Kyoto, Japan.
Tenryu-ji, a Buddhist temple in Kyoto, Japan.

TEC4562885: Tenryu-ji, a Buddhist temple in Kyoto, Japan. / Bridgeman Images

Villa Kujoyama in Kyoto, Japan.
Villa Kujoyama in Kyoto, Japan.

TEC4562926: Villa Kujoyama in Kyoto, Japan. / Bridgeman Images

Villa Kujoyama in Kyoto, Japan.
Villa Kujoyama in Kyoto, Japan.

TEC4562945: Villa Kujoyama in Kyoto, Japan. / Bridgeman Images

First page of the partition of the opening of the Coriolanus Overture, Op. 62, by Ludwig van Beethoven
First page of the partition of the opening of the Coriolanus Overture, Op. 62, by Ludwig van Beethoven

LRI4562985: First page of the partition of the opening of the Coriolanus Overture, Op. 62, by Ludwig van Beethoven / Bridgeman Images

Shibuya District in Tokyo, Japan.
Shibuya District in Tokyo, Japan.

TEC4563132: Shibuya District in Tokyo, Japan. / Bridgeman Images

Panoramic view of Tokyo (Japan).
Panoramic view of Tokyo (Japan).

TEC4563217: Panoramic view of Tokyo (Japan). / Bridgeman Images

Panoramic view of Tokyo (Japan).
Panoramic view of Tokyo (Japan).

TEC4563229: Panoramic view of Tokyo (Japan). / Bridgeman Images

Panoramic view of Tokyo (Japan).
Panoramic view of Tokyo (Japan).

TEC4563237: Panoramic view of Tokyo (Japan). / Bridgeman Images

Panoramic view of Tokyo (Japan).
Panoramic view of Tokyo (Japan).

TEC4563267: Panoramic view of Tokyo (Japan). / Bridgeman Images

Ginza District in Tokyo, Japan Ginza - Tokyo - Japan -
Ginza District in Tokyo, Japan Ginza - Tokyo - Japan -

TEC4563492: Ginza District in Tokyo, Japan Ginza - Tokyo - Japan - / Bridgeman Images

Ginza District in Tokyo, Japan Ginza - Tokyo - Japan -
Ginza District in Tokyo, Japan Ginza - Tokyo - Japan -

TEC4563535: Ginza District in Tokyo, Japan Ginza - Tokyo - Japan - / Bridgeman Images

Omotesando Avenue in Shibuya District in Tokyo, Japan Omotesando-Shibuya-Tokyo-Japan-
Omotesando Avenue in Shibuya District in Tokyo, Japan Omotesando-Shibuya-Tokyo-Japan-

TEC4563634: Omotesando Avenue in Shibuya District in Tokyo, Japan Omotesando-Shibuya-Tokyo-Japan- / Bridgeman Images

Shinjuku District in Tokyo, Japan Shinjuku - Tokyo - Japan -
Shinjuku District in Tokyo, Japan Shinjuku - Tokyo - Japan -

TEC4563739: Shinjuku District in Tokyo, Japan Shinjuku - Tokyo - Japan - / Bridgeman Images

Shinjuku District in Tokyo, Japan Shinjuku - Tokyo - Japan -
Shinjuku District in Tokyo, Japan Shinjuku - Tokyo - Japan -

TEC4563843: Shinjuku District in Tokyo, Japan Shinjuku - Tokyo - Japan - / Bridgeman Images

The Lyon tram. Parilly universal station, Saint Priest (Rhone).
The Lyon tram. Parilly universal station, Saint Priest (Rhone).

LBY4564203: The Lyon tram. Parilly universal station, Saint Priest (Rhone). / Bridgeman Images

Detail of the globular cluster 47 Toucan - Starfield in the globular cluster 47 Tucanae, NGC 104 - The globular cluster 47 Toucan (or NGC 104) is visible to the naked eye from the southern hemisphere. Located about 15000 years ago - light it contains several million stars, some of which are among the older stars known today. This image obtained by the Hubble Space Telescope shows a detail of this cluster near its center; about 35,000 stars are visible. This image shows the Hubble telescope's close - up look at a swarm of 35, 000 stars near the club's central region. The stars are tightly packed together: They are much closer together than our Sun and its closest stars. The picture, taken by the Wide Field and Planetary Camera 2, depicts the stars' natural colors and tells scientists about their composition and age. For example, the red stars denote bright red giants nearing the end of their lives; the more common yellow stars are similar to our middle - aged Sun
Detail of the globular cluster 47 Toucan - Starfield in the globular cluster 47 Tucanae, NGC 104 - The globular cluster 47 Toucan (or NGC 104) is visible to the naked eye from the southern hemisphere. Located about 15000 years ago - light it contains several million stars, some of which are among the older stars known today. This image obtained by the Hubble Space Telescope shows a detail of this cluster near its center; about 35,000 stars are visible. This image shows the Hubble telescope's close - up look at a swarm of 35, 000 stars near the club's central region. The stars are tightly packed together: They are much closer together than our Sun and its closest stars. The picture, taken by the Wide Field and Planetary Camera 2, depicts the stars' natural colors and tells scientists about their composition and age. For example, the red stars denote bright red giants nearing the end of their lives; the more common yellow stars are similar to our middle - aged Sun

PIX4564266: Detail of the globular cluster 47 Toucan - Starfield in the globular cluster 47 Tucanae, NGC 104 - The globular cluster 47 Toucan (or NGC 104) is visible to the naked eye from the southern hemisphere. Located about 15000 years ago - light it contains several million stars, some of which are among the older stars known today. This image obtained by the Hubble Space Telescope shows a detail of this cluster near its center; about 35,000 stars are visible. This image shows the Hubble telescope's close - up look at a swarm of 35, 000 stars near the club's central region. The stars are tightly packed together: They are much closer together than our Sun and its closest stars. The picture, taken by the Wide Field and Planetary Camera 2, depicts the stars' natural colors and tells scientists about their composition and age. For example, the red stars denote bright red giants nearing the end of their lives; the more common yellow stars are similar to our middle - aged Sun / Bridgeman Images

Portrait of Niccolo Paganini (engraving)
Portrait of Niccolo Paganini (engraving)

LRI4564611: Portrait of Niccolo Paganini (engraving) / Bridgeman Images

Globular cluster M13 - Hercules cluster - The Great Globular Cluster in Hercules M13 - M13 (NGC6205), extends for about 150 years - light and is 22,000 years - light from Earth in the constellation of Hercules. M13 (NGC 6205) in the Hercules constellation has a diameter of about 150 light - years and is 22,000 light - years away from Earth
Globular cluster M13 - Hercules cluster - The Great Globular Cluster in Hercules M13 - M13 (NGC6205), extends for about 150 years - light and is 22,000 years - light from Earth in the constellation of Hercules. M13 (NGC 6205) in the Hercules constellation has a diameter of about 150 light - years and is 22,000 light - years away from Earth

PIX4564624: Globular cluster M13 - Hercules cluster - The Great Globular Cluster in Hercules M13 - M13 (NGC6205), extends for about 150 years - light and is 22,000 years - light from Earth in the constellation of Hercules. M13 (NGC 6205) in the Hercules constellation has a diameter of about 150 light - years and is 22,000 light - years away from Earth / Bridgeman Images

Globular cluster M13 - Hercules cluster - The Great Globular Cluster in Hercules M13 - M13 (NGC6205), extends for about 150 years - light and is 22,000 years - light from Earth in the constellation of Hercules. M13 (NGC 6205) in the Hercules constellation has a diameter of about 150 light - years and is 22,000 light - years away from Earth
Globular cluster M13 - Hercules cluster - The Great Globular Cluster in Hercules M13 - M13 (NGC6205), extends for about 150 years - light and is 22,000 years - light from Earth in the constellation of Hercules. M13 (NGC 6205) in the Hercules constellation has a diameter of about 150 light - years and is 22,000 light - years away from Earth

PIX4564635: Globular cluster M13 - Hercules cluster - The Great Globular Cluster in Hercules M13 - M13 (NGC6205), extends for about 150 years - light and is 22,000 years - light from Earth in the constellation of Hercules. M13 (NGC 6205) in the Hercules constellation has a diameter of about 150 light - years and is 22,000 light - years away from Earth / Bridgeman Images

Portrait of Giovanni Paisiello (engraving)
Portrait of Giovanni Paisiello (engraving)

LRI4564649: Portrait of Giovanni Paisiello (engraving) / Bridgeman Images

Globular cluster M13 - Hercules cluster - The Great Globular Cluster in Hercules M13 - M13 (NGC 6205), extends for about 150 years - light and is approximately 25,000 years - light from Earth in the constellation of Hercules. Image obtained by the Hubble Space Telescope. M13 is home to over 100,000 stars and located at a distance of 25,000 light - years. These stars are packed so closely together in a ball, approximately 150 light - years across, that they will spend their entire lives whirling around in the cluster. Near the core of this cluster, the density of stars is about a hundred times greater than the density in the neighborhood of our sun. These stars are so crowded that they can, at times, slam into each other and even form a new star, called a “blue straggler.” The brightest reddish stars in the cluster are ancient red giants. These aging stars have expanded to many times their original diameters and cooled. The blue - white stars are the hottest in the cluster. Globular clusters can be found spread largely in a vast halo around our galaxy. M13 is one of nearly 150 known globular clusters surrounding our Milky Way galaxy. Globular clusters have some of the oldest stars in the universe. They likely formed before the disk of our Milky Way, so they are older than nearly all other stars in our galaxy. Studying globular clusters therefore tells us about the history of our galaxy. This image is a composite of archival Hubble data taken with the Wide Field Planetary Camera 2 and the Advanced Camera for Surveys. Observations from four separate science proposals taken in November 1999, April 2000, August 2005, and April 2006 were used. The image includes broadband filters that isolate light from the blue, visible, and infrared portions of the spectrum
Globular cluster M13 - Hercules cluster - The Great Globular Cluster in Hercules M13 - M13 (NGC 6205), extends for about 150 years - light and is approximately 25,000 years - light from Earth in the constellation of Hercules. Image obtained by the Hubble Space Telescope. M13 is home to over 100,000 stars and located at a distance of 25,000 light - years. These stars are packed so closely together in a ball, approximately 150 light - years across, that they will spend their entire lives whirling around in the cluster. Near the core of this cluster, the density of stars is about a hundred times greater than the density in the neighborhood of our sun. These stars are so crowded that they can, at times, slam into each other and even form a new star, called a “blue straggler.” The brightest reddish stars in the cluster are ancient red giants. These aging stars have expanded to many times their original diameters and cooled. The blue - white stars are the hottest in the cluster. Globular clusters can be found spread largely in a vast halo around our galaxy. M13 is one of nearly 150 known globular clusters surrounding our Milky Way galaxy. Globular clusters have some of the oldest stars in the universe. They likely formed before the disk of our Milky Way, so they are older than nearly all other stars in our galaxy. Studying globular clusters therefore tells us about the history of our galaxy. This image is a composite of archival Hubble data taken with the Wide Field Planetary Camera 2 and the Advanced Camera for Surveys. Observations from four separate science proposals taken in November 1999, April 2000, August 2005, and April 2006 were used. The image includes broadband filters that isolate light from the blue, visible, and infrared portions of the spectrum

PIX4564712: Globular cluster M13 - Hercules cluster - The Great Globular Cluster in Hercules M13 - M13 (NGC 6205), extends for about 150 years - light and is approximately 25,000 years - light from Earth in the constellation of Hercules. Image obtained by the Hubble Space Telescope. M13 is home to over 100,000 stars and located at a distance of 25,000 light - years. These stars are packed so closely together in a ball, approximately 150 light - years across, that they will spend their entire lives whirling around in the cluster. Near the core of this cluster, the density of stars is about a hundred times greater than the density in the neighborhood of our sun. These stars are so crowded that they can, at times, slam into each other and even form a new star, called a “blue straggler.” The brightest reddish stars in the cluster are ancient red giants. These aging stars have expanded to many times their original diameters and cooled. The blue - white stars are the hottest in the cluster. Globular clusters can be found spread largely in a vast halo around our galaxy. M13 is one of nearly 150 known globular clusters surrounding our Milky Way galaxy. Globular clusters have some of the oldest stars in the universe. They likely formed before the disk of our Milky Way, so they are older than nearly all other stars in our galaxy. Studying globular clusters therefore tells us about the history of our galaxy. This image is a composite of archival Hubble data taken with the Wide Field Planetary Camera 2 and the Advanced Camera for Surveys. Observations from four separate science proposals taken in November 1999, April 2000, August 2005, and April 2006 were used. The image includes broadband filters that isolate light from the blue, visible, and infrared portions of the spectrum / Bridgeman Images

NGC 6541 in the Southern Crown - Globular cluster NGC 6541 in Corona Australis - This cluster of stars is located about 23,000 years from Earth. Globular cluster located at about 23,000 light years away
NGC 6541 in the Southern Crown - Globular cluster NGC 6541 in Corona Australis - This cluster of stars is located about 23,000 years from Earth. Globular cluster located at about 23,000 light years away

PIX4564884: NGC 6541 in the Southern Crown - Globular cluster NGC 6541 in Corona Australis - This cluster of stars is located about 23,000 years from Earth. Globular cluster located at about 23,000 light years away / Bridgeman Images

Implosion of a bar HLM to the Cité des 4000 de La Courneuve (Seine Saint Denis), in 2000.
Implosion of a bar HLM to the Cité des 4000 de La Courneuve (Seine Saint Denis), in 2000.

OMG4564923: Implosion of a bar HLM to the Cité des 4000 de La Courneuve (Seine Saint Denis), in 2000. / Bridgeman Images

Implosion of bars HLM, Les Minguettes (Rhone).
Implosion of bars HLM, Les Minguettes (Rhone).

OMG4564958: Implosion of bars HLM, Les Minguettes (Rhone). / Bridgeman Images


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