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Lycee Louis le Grand has Paris 6th arrondissement.
Lycee Louis le Grand has Paris 6th arrondissement.

TEC4559519: Lycee Louis le Grand has Paris 6th arrondissement. / Bridgeman Images

Conversion of the Halle aux Flours in Paris 13th arrondissement. Built in 1950 by Denis Honneger, pupil of Auguste Perret, to receive from the 2006 rent the UFR of physics and chemistry. Under the leadership of Nicolas Michelin, creation in 2004, of thirteen amphitheatres and twenty-six classrooms. Photography 2005.
Conversion of the Halle aux Flours in Paris 13th arrondissement. Built in 1950 by Denis Honneger, pupil of Auguste Perret, to receive from the 2006 rent the UFR of physics and chemistry. Under the leadership of Nicolas Michelin, creation in 2004, of thirteen amphitheatres and twenty-six classrooms. Photography 2005.

TEC4579396: Conversion of the Halle aux Flours in Paris 13th arrondissement. Built in 1950 by Denis Honneger, pupil of Auguste Perret, to receive from the 2006 rent the UFR of physics and chemistry. Under the leadership of Nicolas Michelin, creation in 2004, of thirteen amphitheatres and twenty-six classrooms. Photography 2005. / Bridgeman Images

Lycee technique Raspail, Paris 14th arrondissement.
Lycee technique Raspail, Paris 14th arrondissement.

TEC4559537: Lycee technique Raspail, Paris 14th arrondissement. / Bridgeman Images

Annexe of the Lycee Victor Hugo, Paris 3rd arrondissement. Architect Anatole de Baudot (1834-1915).
Annexe of the Lycee Victor Hugo, Paris 3rd arrondissement. Architect Anatole de Baudot (1834-1915).

TEC4559543: Annexe of the Lycee Victor Hugo, Paris 3rd arrondissement. Architect Anatole de Baudot (1834-1915). / Bridgeman Images

Salon du Ministere des Affaires Etrangeres et Europeennes, 37 quai d'Orsay, Paris 7, architect Jacques Lacornee, 1856.
Salon du Ministere des Affaires Etrangeres et Europeennes, 37 quai d'Orsay, Paris 7, architect Jacques Lacornee, 1856.

TEC4547476: Salon du Ministere des Affaires Etrangeres et Europeennes, 37 quai d'Orsay, Paris 7, architect Jacques Lacornee, 1856. / Bridgeman Images

Statuary in the park of the castle of Versailles (Yvelines, Ile de France), amenagement Andre Le Notre (1613-1700).
Statuary in the park of the castle of Versailles (Yvelines, Ile de France), amenagement Andre Le Notre (1613-1700).

TEC4561665: Statuary in the park of the castle of Versailles (Yvelines, Ile de France), amenagement Andre Le Notre (1613-1700). / Bridgeman Images

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).

TEC4561677: Le Peer Trianon a Versailles, architect Jacques Anges Gabriel, 1760-1764. Parc du Chateau de Versailles (Yvelines, Ile de France). / Bridgeman Images

Le Peer Trianon, garden side, park of the castle of Versailles (Yveline, Ile de France). Architect Jacques Anges Gabriel, 1760-1764.
Le Peer Trianon, garden side, park of the castle of Versailles (Yveline, Ile de France). Architect Jacques Anges Gabriel, 1760-1764.

TEC4561692: Le Peer Trianon, garden side, park of the castle of Versailles (Yveline, Ile de France). Architect Jacques Anges Gabriel, 1760-1764. / Bridgeman Images

Visible Crab Nebula - Infrared and X - The Crab Nebula - M1, the Crab Nebula, is the rest of a supernova that exploded on July 4, 1054. It is located about 7000 light years from Earth in the constellation Taurus. At the heart of this nebula is a pulsar. To obtain this photo, three spatial observatories combined their observations: the Hubble telescope for the visible part (here in red and yellow), the Chandra telescope for the X-ray data (blue) and the Spitzer telescope for the infrared image (purple). The pulsar is the bright spot in the center of the image. The Crab Nebula (M1) is a supernova remnant at about 7,000 light - year from Earth in the constellation Taurus. The star explosion occured on July 04 1054. At the center of this nebula lies a pulsar. This composite image uses data from three of Nasa's Great Observatories. The Chandra X - ray image is shown in blue, the Hubble Space Telescope optical images are in red and yellow, and the Spitzer Space Telescope's infrared image is in purple
Visible Crab Nebula - Infrared and X - The Crab Nebula - M1, the Crab Nebula, is the rest of a supernova that exploded on July 4, 1054. It is located about 7000 light years from Earth in the constellation Taurus. At the heart of this nebula is a pulsar. To obtain this photo, three spatial observatories combined their observations: the Hubble telescope for the visible part (here in red and yellow), the Chandra telescope for the X-ray data (blue) and the Spitzer telescope for the infrared image (purple). The pulsar is the bright spot in the center of the image. The Crab Nebula (M1) is a supernova remnant at about 7,000 light - year from Earth in the constellation Taurus. The star explosion occured on July 04 1054. At the center of this nebula lies a pulsar. This composite image uses data from three of Nasa's Great Observatories. The Chandra X - ray image is shown in blue, the Hubble Space Telescope optical images are in red and yellow, and the Spitzer Space Telescope's infrared image is in purple

PIX4583130: Visible Crab Nebula - Infrared and X - The Crab Nebula - M1, the Crab Nebula, is the rest of a supernova that exploded on July 4, 1054. It is located about 7000 light years from Earth in the constellation Taurus. At the heart of this nebula is a pulsar. To obtain this photo, three spatial observatories combined their observations: the Hubble telescope for the visible part (here in red and yellow), the Chandra telescope for the X-ray data (blue) and the Spitzer telescope for the infrared image (purple). The pulsar is the bright spot in the center of the image. The Crab Nebula (M1) is a supernova remnant at about 7,000 light - year from Earth in the constellation Taurus. The star explosion occured on July 04 1054. At the center of this nebula lies a pulsar. This composite image uses data from three of Nasa's Great Observatories. The Chandra X - ray image is shown in blue, the Hubble Space Telescope optical images are in red and yellow, and the Spitzer Space Telescope's infrared image is in purple / Bridgeman Images

Crab pulsar in nebula M1 - The Crab pulsar: This image from the Hubble space telescope shows the central region of the Crab nebula or resides its pulsar. The pulsar is visible in the center of the image. It is a very dense neutron star from the explosion of a massive supernova star. This star quickly rotates on itself developing a powerful magnetic field, emitting beams of light and radio waves. M1 is located about 6000 light-years in the constellation Taurus.. While many other images of the famous Crab Nebula have focused on the filaments in the outer part of the nebula, this image shows the very heart of the Crab Nebula including the central neutron star - it is the rightmost of the two bright stars near the centre of this image. The rapid motion of the material nearest to the central star is revealed by the subtle rainbow of colours in this time-lapse image, the rainbow effect being due to the movement of material over the time between one image and another
Crab pulsar in nebula M1 - The Crab pulsar: This image from the Hubble space telescope shows the central region of the Crab nebula or resides its pulsar. The pulsar is visible in the center of the image. It is a very dense neutron star from the explosion of a massive supernova star. This star quickly rotates on itself developing a powerful magnetic field, emitting beams of light and radio waves. M1 is located about 6000 light-years in the constellation Taurus.. While many other images of the famous Crab Nebula have focused on the filaments in the outer part of the nebula, this image shows the very heart of the Crab Nebula including the central neutron star - it is the rightmost of the two bright stars near the centre of this image. The rapid motion of the material nearest to the central star is revealed by the subtle rainbow of colours in this time-lapse image, the rainbow effect being due to the movement of material over the time between one image and another

PIX4583135: Crab pulsar in nebula M1 - The Crab pulsar: This image from the Hubble space telescope shows the central region of the Crab nebula or resides its pulsar. The pulsar is visible in the center of the image. It is a very dense neutron star from the explosion of a massive supernova star. This star quickly rotates on itself developing a powerful magnetic field, emitting beams of light and radio waves. M1 is located about 6000 light-years in the constellation Taurus.. While many other images of the famous Crab Nebula have focused on the filaments in the outer part of the nebula, this image shows the very heart of the Crab Nebula including the central neutron star - it is the rightmost of the two bright stars near the centre of this image. The rapid motion of the material nearest to the central star is revealed by the subtle rainbow of colours in this time-lapse image, the rainbow effect being due to the movement of material over the time between one image and another / Bridgeman Images

L'hotel del Coronado in San Diego (California, United States).
L'hotel del Coronado in San Diego (California, United States).

TEC4583730: L'hotel del Coronado in San Diego (California, United States). / Bridgeman Images

The group of 6 Mosquees in Alexandria (Egypt).
The group of 6 Mosquees in Alexandria (Egypt).

TEC4583837: The group of 6 Mosquees in Alexandria (Egypt). / Bridgeman Images

Pekin, China. Photograph 01/10/02.
Pekin, China. Photograph 01/10/02.

TEC4583984: Pekin, China. Photograph 01/10/02. / Bridgeman Images

The hamlet of the Queen, in the Parc du Chateau de Versailles (Yvelines, Ile de France). Architect Richard Mic 1783-1785.
The hamlet of the Queen, in the Parc du Chateau de Versailles (Yvelines, Ile de France). Architect Richard Mic 1783-1785.

TEC4561713: The hamlet of the Queen, in the Parc du Chateau de Versailles (Yvelines, Ile de France). Architect Richard Mic 1783-1785. / Bridgeman Images

Large apartment, queen's room. Ceiling by Francois Boucher. Chateau de Versailles (Les Yvelines). Principal architects Louis Le Vau (1612-1670) and Jules Hardouin Mansart (1646-1708), 1660-1700.
Large apartment, queen's room. Ceiling by Francois Boucher. Chateau de Versailles (Les Yvelines). Principal architects Louis Le Vau (1612-1670) and Jules Hardouin Mansart (1646-1708), 1660-1700.

ITR4561854: Large apartment, queen's room. Ceiling by Francois Boucher. Chateau de Versailles (Les Yvelines). Principal architects Louis Le Vau (1612-1670) and Jules Hardouin Mansart (1646-1708), 1660-1700. / Bridgeman Images

North wing, Crusades Hall. Chateau de Versailles (Les Yvelines). Principal architects: Louis Le Vau (1612-1670) and Jules Hardouin Mansart (1646-1708), 1660-1700.
North wing, Crusades Hall. Chateau de Versailles (Les Yvelines). Principal architects: Louis Le Vau (1612-1670) and Jules Hardouin Mansart (1646-1708), 1660-1700.

ITR4561869: North wing, Crusades Hall. Chateau de Versailles (Les Yvelines). Principal architects: Louis Le Vau (1612-1670) and Jules Hardouin Mansart (1646-1708), 1660-1700. / Bridgeman Images

Midi Wing, Battle Gallery. Chateau de Versailles (Les Yvelines). Principal architects: Louis Le Vau (1612-1670) and Jules Hardouin Mansart (1646-1708), 1660-1700.
Midi Wing, Battle Gallery. Chateau de Versailles (Les Yvelines). Principal architects: Louis Le Vau (1612-1670) and Jules Hardouin Mansart (1646-1708), 1660-1700.

ITR4561878: Midi Wing, Battle Gallery. Chateau de Versailles (Les Yvelines). Principal architects: Louis Le Vau (1612-1670) and Jules Hardouin Mansart (1646-1708), 1660-1700. / Bridgeman Images

The Queen's hamlet around her pond. Built in 1782 in the northwest part of the garden of the Peer Trianon, Chateau de Versailles (Les Yvelines), 1660-1700. Principal architects: Louis Le Vau (1612-1670) and Jules Hardouin Mansart (1646-1708).
The Queen's hamlet around her pond. Built in 1782 in the northwest part of the garden of the Peer Trianon, Chateau de Versailles (Les Yvelines), 1660-1700. Principal architects: Louis Le Vau (1612-1670) and Jules Hardouin Mansart (1646-1708).

ITR4561940: The Queen's hamlet around her pond. Built in 1782 in the northwest part of the garden of the Peer Trianon, Chateau de Versailles (Les Yvelines), 1660-1700. Principal architects: Louis Le Vau (1612-1670) and Jules Hardouin Mansart (1646-1708). / Bridgeman Images

Latone basin realized by the Marsy brothers in 1670.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).
Latone basin realized by the Marsy brothers in 1670.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).

ITR4562005: Latone basin realized by the Marsy brothers in 1670.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).

ITR4562011: 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

The Temple of Love, architect Richard Mic (1728-1794), 1777-1778, in the gardens of the Trianon of the 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).
The Temple of Love, architect Richard Mic (1728-1794), 1777-1778, in the gardens of the Trianon of the 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).

ITR4562095: The Temple of Love, architect Richard Mic (1728-1794), 1777-1778, in the gardens of the Trianon of the 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

Le CENTQURE in Paris, 104 rue d'Aubervilliers, 75019 Paris. CENTQURE, the new artistic establishment of the City of Paris, opens its doors on 11 October 2008 in the old buildings of the Municipal Funebres, located between 5 rue Curial and 104 rue d'Aubervilliers. This place of creation and production unique in the world, both in its architecture and in its surface area of 39,000 square metres, offers artists working spaces adapted, in terms of surfaces and equipment, to the contemporary requirements of creation. It will host about thirty artists a year in residences for periods ranging from 2 to 12 months. Architecture of the November Workshop completed in 2008
Le CENTQURE in Paris, 104 rue d'Aubervilliers, 75019 Paris. CENTQURE, the new artistic establishment of the City of Paris, opens its doors on 11 October 2008 in the old buildings of the Municipal Funebres, located between 5 rue Curial and 104 rue d'Aubervilliers. This place of creation and production unique in the world, both in its architecture and in its surface area of 39,000 square metres, offers artists working spaces adapted, in terms of surfaces and equipment, to the contemporary requirements of creation. It will host about thirty artists a year in residences for periods ranging from 2 to 12 months. Architecture of the November Workshop completed in 2008

OMG4548518: Le CENTQURE in Paris, 104 rue d'Aubervilliers, 75019 Paris. CENTQURE, the new artistic establishment of the City of Paris, opens its doors on 11 October 2008 in the old buildings of the Municipal Funebres, located between 5 rue Curial and 104 rue d'Aubervilliers. This place of creation and production unique in the world, both in its architecture and in its surface area of 39,000 square metres, offers artists working spaces adapted, in terms of surfaces and equipment, to the contemporary requirements of creation. It will host about thirty artists a year in residences for periods ranging from 2 to 12 months. Architecture of the November Workshop completed in 2008 / Bridgeman Images

Le CENTQURE in Paris, 104 rue d'Aubervilliers, 75019 Paris. CENTQURE, the new artistic establishment of the City of Paris, opens its doors on 11 October 2008 in the old buildings of the Municipal Funebres, located between 5 rue Curial and 104 rue d'Aubervilliers. This place of creation and production unique in the world, both in its architecture and in its surface area of 39,000 square metres, offers artists working spaces adapted, in terms of surfaces and equipment, to the contemporary requirements of creation. It will host about thirty artists a year in residences for periods ranging from 2 to 12 months. Architecture of the November Workshop completed in 2008
Le CENTQURE in Paris, 104 rue d'Aubervilliers, 75019 Paris. CENTQURE, the new artistic establishment of the City of Paris, opens its doors on 11 October 2008 in the old buildings of the Municipal Funebres, located between 5 rue Curial and 104 rue d'Aubervilliers. This place of creation and production unique in the world, both in its architecture and in its surface area of 39,000 square metres, offers artists working spaces adapted, in terms of surfaces and equipment, to the contemporary requirements of creation. It will host about thirty artists a year in residences for periods ranging from 2 to 12 months. Architecture of the November Workshop completed in 2008

OMG4548547: Le CENTQURE in Paris, 104 rue d'Aubervilliers, 75019 Paris. CENTQURE, the new artistic establishment of the City of Paris, opens its doors on 11 October 2008 in the old buildings of the Municipal Funebres, located between 5 rue Curial and 104 rue d'Aubervilliers. This place of creation and production unique in the world, both in its architecture and in its surface area of 39,000 square metres, offers artists working spaces adapted, in terms of surfaces and equipment, to the contemporary requirements of creation. It will host about thirty artists a year in residences for periods ranging from 2 to 12 months. Architecture of the November Workshop completed in 2008 / Bridgeman Images

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

TEC4562296: Tour to Victoria Island in Hong Kong (China). / Bridgeman Images

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

TEC4562438: Victoria Island to Hong Kong (China). / Bridgeman Images

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

TEC4562532: Hong Kong City Hong Kong - China - / Bridgeman Images

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

TEC4562636: Hong Kong City Hong Kong - China - / Bridgeman Images

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

TEC4562656: Hong Kong City Hong Kong - China - / Bridgeman Images

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

TEC4562679: Hong Kong City Hong Kong - China - / Bridgeman Images

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

TEC4563792: Shinjuku District in Tokyo, Japan Shinjuku - Tokyo - Japan - / Bridgeman Images

Open cluster M35 and NGC 2158 in Gemeaux - Open clusters M35 and NGC 2158 in Gemini - Open cluster M35 (NGC 2168) is visible to the naked eye under good conditions. NGC 2158, lower right, is weaker and is only observed at the telescope. M35 is about 2800 years of light from Earth and is about 110 million years old. M35 (NGC 2168), at left, is a spectacular large open cluster containing about 200 stars located in Gemini. Shining at magnitude 5, it is visible to the unaided eye off the foot of Gemini. It is accompanied by a jewel - like smaller companion, open cluster NGC 2158, seen at the lower right of the photo
Open cluster M35 and NGC 2158 in Gemeaux - Open clusters M35 and NGC 2158 in Gemini - Open cluster M35 (NGC 2168) is visible to the naked eye under good conditions. NGC 2158, lower right, is weaker and is only observed at the telescope. M35 is about 2800 years of light from Earth and is about 110 million years old. M35 (NGC 2168), at left, is a spectacular large open cluster containing about 200 stars located in Gemini. Shining at magnitude 5, it is visible to the unaided eye off the foot of Gemini. It is accompanied by a jewel - like smaller companion, open cluster NGC 2158, seen at the lower right of the photo

PIX4567936: Open cluster M35 and NGC 2158 in Gemeaux - Open clusters M35 and NGC 2158 in Gemini - Open cluster M35 (NGC 2168) is visible to the naked eye under good conditions. NGC 2158, lower right, is weaker and is only observed at the telescope. M35 is about 2800 years of light from Earth and is about 110 million years old. M35 (NGC 2168), at left, is a spectacular large open cluster containing about 200 stars located in Gemini. Shining at magnitude 5, it is visible to the unaided eye off the foot of Gemini. It is accompanied by a jewel - like smaller companion, open cluster NGC 2158, seen at the lower right of the photo / Bridgeman Images

La Basilique du Sacre Coeur (Sacre Coeur), Paris 18. Architects Paul Abadie and Lucien Magne, 1877-1923.
La Basilique du Sacre Coeur (Sacre Coeur), Paris 18. Architects Paul Abadie and Lucien Magne, 1877-1923.

TEC4552901: La Basilique du Sacre Coeur (Sacre Coeur), Paris 18. Architects Paul Abadie and Lucien Magne, 1877-1923. / Bridgeman Images

Title page of musical score of symphony for piano in Semiramide by Gioacchino Rossini
Title page of musical score of symphony for piano in Semiramide by Gioacchino Rossini

LRI4568181: Title page of musical score of symphony for piano in Semiramide by Gioacchino Rossini / Bridgeman Images

Open cluster NGC 3293 in Carene - Open star cluster NGC 3293 in Carina - Star cluster located in the constellation Carene about 8500 years ago - light from Earth. Unlike the Sun, many stars are found in brilliant clusters such as NGC 3293 where they spend their lives. At birth, which should have been at much the same time for all the stars in NGC 3293, the most massive stars are hot and very luminous and therefore appear as the brightest blue stars. With time they deplete their supplies of nuclear fuel, hydrogen. This evolutionary process involves cooling, so that the stars become redder, and would ordinarily disappear from view, but they also swell to gigantic proportions and so remain visible. The bright orange star in NGC 3293 is the member of the cluster which has aged fastest. This cluster is in the constellation of Carina at a distance of about 8500 light years
Open cluster NGC 3293 in Carene - Open star cluster NGC 3293 in Carina - Star cluster located in the constellation Carene about 8500 years ago - light from Earth. Unlike the Sun, many stars are found in brilliant clusters such as NGC 3293 where they spend their lives. At birth, which should have been at much the same time for all the stars in NGC 3293, the most massive stars are hot and very luminous and therefore appear as the brightest blue stars. With time they deplete their supplies of nuclear fuel, hydrogen. This evolutionary process involves cooling, so that the stars become redder, and would ordinarily disappear from view, but they also swell to gigantic proportions and so remain visible. The bright orange star in NGC 3293 is the member of the cluster which has aged fastest. This cluster is in the constellation of Carina at a distance of about 8500 light years

PIX4568196: Open cluster NGC 3293 in Carene - Open star cluster NGC 3293 in Carina - Star cluster located in the constellation Carene about 8500 years ago - light from Earth. Unlike the Sun, many stars are found in brilliant clusters such as NGC 3293 where they spend their lives. At birth, which should have been at much the same time for all the stars in NGC 3293, the most massive stars are hot and very luminous and therefore appear as the brightest blue stars. With time they deplete their supplies of nuclear fuel, hydrogen. This evolutionary process involves cooling, so that the stars become redder, and would ordinarily disappear from view, but they also swell to gigantic proportions and so remain visible. The bright orange star in NGC 3293 is the member of the cluster which has aged fastest. This cluster is in the constellation of Carina at a distance of about 8500 light years / Bridgeman Images

Open cluster NGC 4755 - Jewel Box - The Jewel Box star cluster - The NGC 4755 cluster is located in the constellation of the Southern Cross at a distance of 6400 years - light from Earth. The bright orange star on the top right is Kappa Crucis, a supergiant red star. This cluster contains about fifty stars formed about 16 million years ago. This close-up of the center of the cluster was obtained with the Hubble Space Telescope. This image is a “” close - up 'view from the NASA/ESA Hubble Space Telescope of NGC 4755, or the Jewel Box cluster. Several very bright, pale blue supergiant stars, a solitary ruby - red supergiant and a variety of other brilliantly coloured stars are visible in the image, as well as many much fainter ones, often with intriguing colours. The huge variety in brightness exists because the brighter stars are 15 to 20 times the mass of the Sun, while the dimmest stars are less than half the mass of the Sun. This is the first image of an open galactic cluster with imaging extending from the far ultraviolet to the near - infrared. NGC 4755 (Caldwell 94) is called the Jewel Box, based on John Herschel's comment in the 1830's that it looked like a superb piece of jewelry. There are about 50 stars in this cluster which formed some 14 million years ago. Most of the cluster members are blue giants which in a few million years will exhaust their hydrogen fuel and become red giants on their way to a cataclysmic end as supernovae. One red giant can already be seen at the center of the cluster (top right)
Open cluster NGC 4755 - Jewel Box - The Jewel Box star cluster - The NGC 4755 cluster is located in the constellation of the Southern Cross at a distance of 6400 years - light from Earth. The bright orange star on the top right is Kappa Crucis, a supergiant red star. This cluster contains about fifty stars formed about 16 million years ago. This close-up of the center of the cluster was obtained with the Hubble Space Telescope. This image is a “” close - up 'view from the NASA/ESA Hubble Space Telescope of NGC 4755, or the Jewel Box cluster. Several very bright, pale blue supergiant stars, a solitary ruby - red supergiant and a variety of other brilliantly coloured stars are visible in the image, as well as many much fainter ones, often with intriguing colours. The huge variety in brightness exists because the brighter stars are 15 to 20 times the mass of the Sun, while the dimmest stars are less than half the mass of the Sun. This is the first image of an open galactic cluster with imaging extending from the far ultraviolet to the near - infrared. NGC 4755 (Caldwell 94) is called the Jewel Box, based on John Herschel's comment in the 1830's that it looked like a superb piece of jewelry. There are about 50 stars in this cluster which formed some 14 million years ago. Most of the cluster members are blue giants which in a few million years will exhaust their hydrogen fuel and become red giants on their way to a cataclysmic end as supernovae. One red giant can already be seen at the center of the cluster (top right)

PIX4568246: Open cluster NGC 4755 - Jewel Box - The Jewel Box star cluster - The NGC 4755 cluster is located in the constellation of the Southern Cross at a distance of 6400 years - light from Earth. The bright orange star on the top right is Kappa Crucis, a supergiant red star. This cluster contains about fifty stars formed about 16 million years ago. This close-up of the center of the cluster was obtained with the Hubble Space Telescope. This image is a “” close - up 'view from the NASA/ESA Hubble Space Telescope of NGC 4755, or the Jewel Box cluster. Several very bright, pale blue supergiant stars, a solitary ruby - red supergiant and a variety of other brilliantly coloured stars are visible in the image, as well as many much fainter ones, often with intriguing colours. The huge variety in brightness exists because the brighter stars are 15 to 20 times the mass of the Sun, while the dimmest stars are less than half the mass of the Sun. This is the first image of an open galactic cluster with imaging extending from the far ultraviolet to the near - infrared. NGC 4755 (Caldwell 94) is called the Jewel Box, based on John Herschel's comment in the 1830's that it looked like a superb piece of jewelry. There are about 50 stars in this cluster which formed some 14 million years ago. Most of the cluster members are blue giants which in a few million years will exhaust their hydrogen fuel and become red giants on their way to a cataclysmic end as supernovae. One red giant can already be seen at the center of the cluster (top right) / Bridgeman Images

The Erasmus bridge in Rotterdam (Netherlands). Construction 1990-1996, Arcchitecte Van Berkel and Bos Architecten.
The Erasmus bridge in Rotterdam (Netherlands). Construction 1990-1996, Arcchitecte Van Berkel and Bos Architecten.

TEC4568283: The Erasmus bridge in Rotterdam (Netherlands). Construction 1990-1996, Arcchitecte Van Berkel and Bos Architecten. / Bridgeman Images


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