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Maldives: Women of Malé, the Maldivian capital, embroidering a traditional dress, North Malé Atoll, 1980

Maldives: Women of Malé, the Maldivian capital, embroidering a traditional dress, North Malé Atoll, 1980

PFH4072386

Maldives: Plaiting coir fibre to make rope, Maradhoo Island, Addu Atoll, 1976

Maldives: Plaiting coir fibre to make rope, Maradhoo Island, Addu Atoll, 1976

PFH2561701

At least 9,000 people including 3000 women and 1000 children work as stone laborer, on the bank of the Dholai river, in Bholaganj, Sylhet. Millions of tons of boulders, pebbles and stones slide along the strong current of the Mari river, coming from the great Himalayas of India. The average income of the stone laborers is less then 150 taka per day, about 2 US Dollars. Stone extraction goes on in the area for about eight months a year, except the rainy season. On an average 300 truck load of stones are sent to Sylhet and other parts of Bangladesh everyday. Bangladesh. July 25, 2008. (photo)

At least 9,000 people including 3000 women and 1000 children work as stone laborer, on the bank of the Dholai river, in Bholaganj, Sylhet. Millions of tons of boulders, pebbles and stones slide along the strong current of the Mari river, coming from the great Himalayas of India. The average income of the stone laborers is less then 150 taka per day, about 2 US Dollars. Stone extraction goes on in the area for about eight months a year, except the rainy season. On an average 300 truck load of stones are sent to Sylhet and other parts of Bangladesh everyday. Bangladesh. July 25, 2008. (photo)

UIG799900

At least 9,000 people including 3000 women and 1000 children work as stone laborer, on the bank of the Dholai river, in Bholaganj, Sylhet. Millions of tons of boulders, pebbles and stones slide along the strong current of the Mari river, coming from the great Himalayas of India. The average income of the stone laborers is less then 150 taka per day, about 2 US Dollars. Stone extraction goes on in the area for about eight months a year, except the rainy season. On an average 300 truck load of stones are sent to Sylhet and other parts of Bangladesh everyday. Bangladesh. July 25, 2008. (photo)

At least 9,000 people including 3000 women and 1000 children work as stone laborer, on the bank of the Dholai river, in Bholaganj, Sylhet. Millions of tons of boulders, pebbles and stones slide along the strong current of the Mari river, coming from the great Himalayas of India. The average income of the stone laborers is less then 150 taka per day, about 2 US Dollars. Stone extraction goes on in the area for about eight months a year, except the rainy season. On an average 300 truck load of stones are sent to Sylhet and other parts of Bangladesh everyday. Bangladesh. July 25, 2008. (photo)

UIG799904

At least 9,000 people including 3000 women and 1000 children work as stone laborer, on the bank of the Dholai river, in Bholaganj, Sylhet. Millions of tons of boulders, pebbles and stones slide along the strong current of the Mari river, coming from the great Himalayas of India. The average income of the stone laborers is less then 150 taka per day, about 2 US Dollars. Stone extraction goes on in the area for about eight months a year, except the rainy season. On an average 300 truck load of stones are sent to Sylhet and other parts of Bangladesh everyday. Bangladesh. July 25, 2008. (photo)

At least 9,000 people including 3000 women and 1000 children work as stone laborer, on the bank of the Dholai river, in Bholaganj, Sylhet. Millions of tons of boulders, pebbles and stones slide along the strong current of the Mari river, coming from the great Himalayas of India. The average income of the stone laborers is less then 150 taka per day, about 2 US Dollars. Stone extraction goes on in the area for about eight months a year, except the rainy season. On an average 300 truck load of stones are sent to Sylhet and other parts of Bangladesh everyday. Bangladesh. July 25, 2008. (photo)

UIG799899

At least 9,000 people including 3000 women and 1000 children work as stone laborer, on the bank of the Dholai river, in Bholaganj, Sylhet. Millions of tons of boulders, pebbles and stones slide along the strong current of the Mari river, coming from the great Himalayas of India. The average income of the stone laborers is less then 150 taka per day, about 2 US Dollars. Stone extraction goes on in the area for about eight months a year, except the rainy season. On an average 300 truck load of stones are sent to Sylhet and other parts of Bangladesh everyday. Bangladesh. July 25, 2008. (photo)

At least 9,000 people including 3000 women and 1000 children work as stone laborer, on the bank of the Dholai river, in Bholaganj, Sylhet. Millions of tons of boulders, pebbles and stones slide along the strong current of the Mari river, coming from the great Himalayas of India. The average income of the stone laborers is less then 150 taka per day, about 2 US Dollars. Stone extraction goes on in the area for about eight months a year, except the rainy season. On an average 300 truck load of stones are sent to Sylhet and other parts of Bangladesh everyday. Bangladesh. July 25, 2008. (photo)

UIG799901

At least 9,000 people including 3000 women and 1000 children work as stone laborer, on the bank of the Dholai river, in Bholaganj, Sylhet. Millions of tons of boulders, pebbles and stones slide along the strong current of the Mari river, coming from the great Himalayas of India. The average income of the stone laborers is less then 150 taka per day, about 2 US Dollars. Stone extraction goes on in the area for about eight months a year, except the rainy season. On an average 300 truck load of stones are sent to Sylhet and other parts of Bangladesh everyday. Bangladesh. July 25, 2008. (photo)

At least 9,000 people including 3000 women and 1000 children work as stone laborer, on the bank of the Dholai river, in Bholaganj, Sylhet. Millions of tons of boulders, pebbles and stones slide along the strong current of the Mari river, coming from the great Himalayas of India. The average income of the stone laborers is less then 150 taka per day, about 2 US Dollars. Stone extraction goes on in the area for about eight months a year, except the rainy season. On an average 300 truck load of stones are sent to Sylhet and other parts of Bangladesh everyday. Bangladesh. July 25, 2008. (photo)

UIG799902

At least 9,000 people including 3000 women and 1000 children work as stone laborer, on the bank of the Dholai river, in Bholaganj, Sylhet. Millions of tons of boulders, pebbles and stones slide along the strong current of the Mari river, coming from the great Himalayas of India. The average income of the stone laborers is less then 150 taka per day, about 2 US Dollars. Stone extraction goes on in the area for about eight months a year, except the rainy season. On an average 300 truck load of stones are sent to Sylhet and other parts of Bangladesh everyday. Bangladesh. July 25, 2008. (photo)

At least 9,000 people including 3000 women and 1000 children work as stone laborer, on the bank of the Dholai river, in Bholaganj, Sylhet. Millions of tons of boulders, pebbles and stones slide along the strong current of the Mari river, coming from the great Himalayas of India. The average income of the stone laborers is less then 150 taka per day, about 2 US Dollars. Stone extraction goes on in the area for about eight months a year, except the rainy season. On an average 300 truck load of stones are sent to Sylhet and other parts of Bangladesh everyday. Bangladesh. July 25, 2008. (photo)

UIG798804

India: The red Digambara Jain Temple and white Sikh temple on busy Chandni Chowk, Old Delhi

India: The red Digambara Jain Temple and white Sikh temple on busy Chandni Chowk, Old Delhi

David Henley

PFH1189590

India: Diwan-i-Khas (Hall of Private Audiences), Red Fort, Old Delhi

India: Diwan-i-Khas (Hall of Private Audiences), Red Fort, Old Delhi

David Henley

PFH1189482

India: The walls of the Red Fort (Lahore Gate to the left) seen in the late afternoon, Delhi

India: The walls of the Red Fort (Lahore Gate to the left) seen in the late afternoon, Delhi

David Henley

PFH1189484

Maldives: Carved spar from a Maldivian mosque

Maldives: Carved spar from a Maldivian mosque

PFH4072315

Maldives: A boy uses a sand tray and stick pen to practise his writing skills. In the past a traditional way to learn to write. Addu Atoll (Seenu Atoll) 1980

Maldives: A boy uses a sand tray and stick pen to practise his writing skills. In the past a traditional way to learn to write. Addu Atoll (Seenu Atoll) 1980

PFH4072380

Maldives: Island style baby seats with rattle, Addu Atoll (Seena Atoll) 1980

Maldives: Island style baby seats with rattle, Addu Atoll (Seena Atoll) 1980

PFH4072388

India: The Lahore Gate at the massive Red Fort, Old Delhi

India: The Lahore Gate at the massive Red Fort, Old Delhi

David Henley

PFH1189276

Maldives: Carved spar from a Maldivian mosque

Maldives: Carved spar from a Maldivian mosque

PFH4072317

Maldives: A father instructs his two sons in the use of traditional drums, Addu Atoll (Seenu Atoll) 1980

Maldives: A father instructs his two sons in the use of traditional drums, Addu Atoll (Seenu Atoll) 1980

PFH4072347

Maldives: A woman smoking a traditional hookah (shisha) pipe, Addu Atoll (Seenu Atoll) 1980

Maldives: A woman smoking a traditional hookah (shisha) pipe, Addu Atoll (Seenu Atoll) 1980

PFH4072350

India: Moti Masjid (Pearl Mosque), Red Fort, Old Delhi

India: Moti Masjid (Pearl Mosque), Red Fort, Old Delhi

David Henley

PFH1189364

India: White marble hall (diwan) north of the Moti Masjid, Red Fort, Old Delhi

India: White marble hall (diwan) north of the Moti Masjid, Red Fort, Old Delhi

David Henley

PFH1189366

Maldives: Plaiting leaves to make matting, Feydhoo Island, Addu Atoll, 1976

Maldives: Plaiting leaves to make matting, Feydhoo Island, Addu Atoll, 1976

PFH2561700

Maldives: Maldivian drummers repairing their intruments, Hithadhoo Island, Addu Atoll, 1976

Maldives: Maldivian drummers repairing their intruments, Hithadhoo Island, Addu Atoll, 1976

PFH2561702

Maldives: A man holds a simple indigenous percussion instrument, Addu Atoll (Seenu Atoll) 1980

Maldives: A man holds a simple indigenous percussion instrument, Addu Atoll (Seenu Atoll) 1980

PFH4072349

Maldives: Children, eyes darkened with "kohl" makeup, Addu Atoll (Seenu Atoll) 1980

Maldives: Children, eyes darkened with "kohl" makeup, Addu Atoll (Seenu Atoll) 1980

PFH4072387

A woman carries freshly molded brick, at a brick factory, in Joydebpur, on the outskirts of Dhaka. There are hundreds of brick factories around the country that employ women and children as laborer. In and around urban areas, they are paid Taka 50, about US$ 0.70, for carrying 1000 bricks from one site to another, usually between 50 to 100 meters apart. Adult women can carry 1500-1800 bricks. Young children can carry between 200-400 bricks. Factories that are located in rural areas pay almost half as much. Mostly they earn just enough to be able to have three basic meals everyday. Bangladesh. February 12, 2007. (photo)

A woman carries freshly molded brick, at a brick factory, in Joydebpur, on the outskirts of Dhaka. There are hundreds of brick factories around the country that employ women and children as laborer. In and around urban areas, they are paid Taka 50, about US$ 0.70, for carrying 1000 bricks from one site to another, usually between 50 to 100 meters apart. Adult women can carry 1500-1800 bricks. Young children can carry between 200-400 bricks. Factories that are located in rural areas pay almost half as much. Mostly they earn just enough to be able to have three basic meals everyday. Bangladesh. February 12, 2007. (photo)

UIG799410

The three foot theodolite made by Cary for the Great Survey of India, 1802

The three foot theodolite made by Cary for the Great Survey of India, 1802

UIS5085678

Basement 19580815 Frederic's calculator is installed on Kjeller. The calculator developed …, 1958 (photo)

Basement 19580815 Frederic's calculator is installed on Kjeller. The calculator developed …, 1958 (photo)

Jan Nordby

NTB8910021

Dale in Hordaland 19530425. Dale Fabrikker is Norway's largest textile factory with …, 1953 (photo)

Dale in Hordaland 19530425. Dale Fabrikker is Norway's largest textile factory with …, 1953 (photo)

Sverre A. Børretzen

NTB8930265

Maldives: Gravestones (pointed for men) are covered with incised designs

Maldives: Gravestones (pointed for men) are covered with incised designs

PFH4072366

Remains of the Crab Supernova (M1) in the Taurus - This image, made by the Very Large Telescope in November 1999, shows in detail the gas remains of the supernova that exploded in 1054. In the center of the picture, the pulsar of the Crab. M1 with the FORS2 instrument in imaging mode in the morning of November 10, 1999. It is the remnant of a supernova explosion at a distance of about 6,000 light - years, observed almost 1000 years ago, in the year 1054. It contains a neutron star near its center that spins 30 times per second around its axis In this picture, the red light is predominantly produced by hydrogen emission from material ejected by the star that exploded. The blue light is predominantly emitted by very high - energy (“relativistic”) electrons that spiral in a large - scale magnetic field (so - called syncrotron emission). It is believed that these electrons are continuously accelerated and ejected by the rapidly spinning neutron star at the centre of the nebula and which is

Remains of the Crab Supernova (M1) in the Taurus - This image, made by the Very Large Telescope in November 1999, shows in detail the gas remains of the supernova that exploded in 1054. In the center of the picture, the pulsar of the Crab. M1 with the FORS2 instrument in imaging mode in the morning of November 10, 1999. It is the remnant of a supernova explosion at a distance of about 6,000 light - years, observed almost 1000 years ago, in the year 1054. It contains a neutron star near its center that spins 30 times per second around its axis In this picture, the red light is predominantly produced by hydrogen emission from material ejected by the star that exploded. The blue light is predominantly emitted by very high - energy (“relativistic”) electrons that spiral in a large - scale magnetic field (so - called syncrotron emission). It is believed that these electrons are continuously accelerated and ejected by the rapidly spinning neutron star at the centre of the nebula and which is

PIX4582982

Constellation of Centaurus - Constellation of Centaurus - Also visible are the constellations of the Compas, the Southern Cross, the Rulle and the Wolf. Centaurus (the Centaur), is in one of the richest parts of the southern sky. At over 1000 square degrees it is the ninth largest constellation. It represents a centaur in Greek mythology, a half - man half - horse creature (Sagittarius is another). The learned centaur is the legendary inventor of the main constellations. Apart from a sparkling scattering of stars, the constellation also embraces one of the finest globular clusters, Omega Centauri and a few degrees north of it NGC 5128, the radio galaxy Centaurus A. Close to a Centaurus, the brightest star in the picture and, with ss Centaurus, one of the Pointers to the Southern Cross, is Proxima Cen. This faint star is not seen in this image, but at 4 light years distant is the closest star to the Sun. Norma, (originally Norma and Regula, the builder's level and set square) is an insi

Constellation of Centaurus - Constellation of Centaurus - Also visible are the constellations of the Compas, the Southern Cross, the Rulle and the Wolf. Centaurus (the Centaur), is in one of the richest parts of the southern sky. At over 1000 square degrees it is the ninth largest constellation. It represents a centaur in Greek mythology, a half - man half - horse creature (Sagittarius is another). The learned centaur is the legendary inventor of the main constellations. Apart from a sparkling scattering of stars, the constellation also embraces one of the finest globular clusters, Omega Centauri and a few degrees north of it NGC 5128, the radio galaxy Centaurus A. Close to a Centaurus, the brightest star in the picture and, with ss Centaurus, one of the Pointers to the Southern Cross, is Proxima Cen. This faint star is not seen in this image, but at 4 light years distant is the closest star to the Sun. Norma, (originally Norma and Regula, the builder's level and set square) is an insi

PIX4589824

Constellation of Centaurus - Constellation of Centaurus - Also visible are the constellations of the Compas, the Southern Cross, the Rulle and the Wolf. Centaurus (the Centaur), is in one of the richest parts of the southern sky. At over 1000 square degrees it is the ninth largest constellation. It represents a centaur in Greek mythology, a half - man half - horse creature (Sagittarius is another). The learned centaur is the legendary inventor of the main constellations. Apart from a sparkling scattering of stars, the constellation also embraces one of the finest globular clusters, Omega Centauri and a few degrees north of it NGC 5128, the radio galaxy Centaurus A. Close to a Centaurus, the brightest star in the picture and, with ss Centaurus, one of the Pointers to the Southern Cross, is Proxima Cen. This faint star is not seen in this image, but at 4 light years distant is the closest star to the Sun. Norma, (originally Norma and Regula, the builder's level and set square) is an insi

Constellation of Centaurus - Constellation of Centaurus - Also visible are the constellations of the Compas, the Southern Cross, the Rulle and the Wolf. Centaurus (the Centaur), is in one of the richest parts of the southern sky. At over 1000 square degrees it is the ninth largest constellation. It represents a centaur in Greek mythology, a half - man half - horse creature (Sagittarius is another). The learned centaur is the legendary inventor of the main constellations. Apart from a sparkling scattering of stars, the constellation also embraces one of the finest globular clusters, Omega Centauri and a few degrees north of it NGC 5128, the radio galaxy Centaurus A. Close to a Centaurus, the brightest star in the picture and, with ss Centaurus, one of the Pointers to the Southern Cross, is Proxima Cen. This faint star is not seen in this image, but at 4 light years distant is the closest star to the Sun. Norma, (originally Norma and Regula, the builder's level and set square) is an insi

PIX4589782

Maldives: Gravestones (rounded for women) are covered with incised designs

Maldives: Gravestones (rounded for women) are covered with incised designs

PFH4072367

Nebula NGC 3372 in the Carene in fake colors - NGC 3372 Carina nebula in narrow band - The nebula of the Carene is located about 8000 years - light from Earth. It is home to many hot stars, including the massive star Eta Carinae in the centre of the nebula. Image obtained by the 1.2m Schmidt UK Telescope of Siding Spring through 3 different filters that highlight oxygen, hydrogen, and sulfur. Although no bright naked - eye stars are associated with the Carina nebula now, 150 years ago there blazed forth here one of the most unusual and peculiar stars ever seen. The star is known as Eta Carinae and for a few months in 1843 it was the second or third brightest star in the sky. Since then it has faded and is today about 1000 times fainter than it was at its brightest as the nebula it created during its outburst has cooled and become opaque. The whole region around Eta Carinae is rich in hot stars of which Eta is an extreme example and it is their combined radiation that produces the spect

Nebula NGC 3372 in the Carene in fake colors - NGC 3372 Carina nebula in narrow band - The nebula of the Carene is located about 8000 years - light from Earth. It is home to many hot stars, including the massive star Eta Carinae in the centre of the nebula. Image obtained by the 1.2m Schmidt UK Telescope of Siding Spring through 3 different filters that highlight oxygen, hydrogen, and sulfur. Although no bright naked - eye stars are associated with the Carina nebula now, 150 years ago there blazed forth here one of the most unusual and peculiar stars ever seen. The star is known as Eta Carinae and for a few months in 1843 it was the second or third brightest star in the sky. Since then it has faded and is today about 1000 times fainter than it was at its brightest as the nebula it created during its outburst has cooled and become opaque. The whole region around Eta Carinae is rich in hot stars of which Eta is an extreme example and it is their combined radiation that produces the spect

PIX4619010

The bombardment of Algiers, 27 August 1816, c.1836 (oil painting)

The bombardment of Algiers, 27 August 1816, c.1836 (oil painting)

Chambers, George the Elder (1803-40)

MMM7337712

L'ingenieur anglais Charles Stewart Rolls (1877-1910), deguise en policier, mettant une amende au pilote automobile John Moore Brabazon (1884-1964)

L'ingenieur anglais Charles Stewart Rolls (1877-1910), deguise en policier, mettant une amende au pilote automobile John Moore Brabazon (1884-1964)

UIS5070047

Tarantula (NGC 2070) in the LMC - The nebula around 30 Doradus (NGC 2070) in the LMC - The Tarantula Nebula (or 30 Bream) is the largest star-forming region of the Great Magellan Cloud. It is located 170,000 light years ago in the constellation Dorado (southern hemisphere). At the center of this nebula, the open cluster of R136 stars, clusters of hot and massive stars. Image obtained with Siding Spring's 3.9m telescope. The brightest cluster of stars in this picture was believed until recently to contain a single, uniquely massive object with the mass equivalent to 1000 suns, and was named as a star, 30 Doradus. Sophisticated image analysis techniques have been used to show that 30 Doradus is a very compact group of stars, many of which are massive, but not unimaginably so. The radiation from this star cluster is sufficient to excite a huge cloud of hydrogen gas in its vicinity so that it glows with its distinctive red colour. This picture is essentially a one minute exposure. A longer

Tarantula (NGC 2070) in the LMC - The nebula around 30 Doradus (NGC 2070) in the LMC - The Tarantula Nebula (or 30 Bream) is the largest star-forming region of the Great Magellan Cloud. It is located 170,000 light years ago in the constellation Dorado (southern hemisphere). At the center of this nebula, the open cluster of R136 stars, clusters of hot and massive stars. Image obtained with Siding Spring's 3.9m telescope. The brightest cluster of stars in this picture was believed until recently to contain a single, uniquely massive object with the mass equivalent to 1000 suns, and was named as a star, 30 Doradus. Sophisticated image analysis techniques have been used to show that 30 Doradus is a very compact group of stars, many of which are massive, but not unimaginably so. The radiation from this star cluster is sufficient to excite a huge cloud of hydrogen gas in its vicinity so that it glows with its distinctive red colour. This picture is essentially a one minute exposure. A longer

PIX4618266

Maldives: Gravestones (pointed for men) are covered with incised designs

Maldives: Gravestones (pointed for men) are covered with incised designs

PFH4072365

Maldives: Gravestones (pointed for men) are covered with incised designs, this stone has been damaged and the point has gone

Maldives: Gravestones (pointed for men) are covered with incised designs, this stone has been damaged and the point has gone

PFH4072368

Nebula NGC 3372 in the Carene in false colours - NGC 3372 Carina nebula - The nebula of the Carene is located about 8000 years - light from the Earth. It is home to many hot stars, including the massive star Eta Carinae in the centre of the nebula. Top right is the cluster of stars NGC 3293. Image obtained from the 1.2m Schmidt UK telescope of Siding Spring. Although no bright naked - eye stars are associated with the Carina nebula now, 150 years ago there blazed forth here one of the most unusual and peculiar stars ever seen. The star is known as Eta Carinae and for a few months in 1843 it was the second or third brightest star in the sky. Since then it has faded and is today about 1000 times fainter than it was at its brightest as the nebula it created during its outburst has cooled and become opaque. The whole region around Eta Carinae is rich in hot stars of which Eta is an extreme example and it is their combined radiation that produces the spectacular Carina nebula that dominates

Nebula NGC 3372 in the Carene in false colours - NGC 3372 Carina nebula - The nebula of the Carene is located about 8000 years - light from the Earth. It is home to many hot stars, including the massive star Eta Carinae in the centre of the nebula. Top right is the cluster of stars NGC 3293. Image obtained from the 1.2m Schmidt UK telescope of Siding Spring. Although no bright naked - eye stars are associated with the Carina nebula now, 150 years ago there blazed forth here one of the most unusual and peculiar stars ever seen. The star is known as Eta Carinae and for a few months in 1843 it was the second or third brightest star in the sky. Since then it has faded and is today about 1000 times fainter than it was at its brightest as the nebula it created during its outburst has cooled and become opaque. The whole region around Eta Carinae is rich in hot stars of which Eta is an extreme example and it is their combined radiation that produces the spectacular Carina nebula that dominates

PIX4618867

India: The remains of the Alai Minar, originally built to be twice as high as the Qutb Minar, the Qutb Minar complex, Delhi

India: The remains of the Alai Minar, originally built to be twice as high as the Qutb Minar, the Qutb Minar complex, Delhi

David Henley

PFH1189429

India: A crafted stone pillar in the Quwwat-ul-Islam Mosque at the ancient Qutb Minar complex, Delhi

India: A crafted stone pillar in the Quwwat-ul-Islam Mosque at the ancient Qutb Minar complex, Delhi

David Henley

PFH1189430

India: Mahatma Gandhi mural at the Gandhi Smriti Museum (formerly Birla House), New Delhi

India: Mahatma Gandhi mural at the Gandhi Smriti Museum (formerly Birla House), New Delhi

David Henley

PFH1189593

India: The Martyr's Column marking the spot where Mahatma Gandhi was assassinated on January 30, 1948, Gandhi Smriti Museum (formerly Birla House), New Delhi

India: The Martyr's Column marking the spot where Mahatma Gandhi was assassinated on January 30, 1948, Gandhi Smriti Museum (formerly Birla House), New Delhi

David Henley

PFH1189594

India: A crafted stone pillar in the Quwwat-ul-Islam Mosque at the ancient Qutb Minar complex, Delhi

India: A crafted stone pillar in the Quwwat-ul-Islam Mosque at the ancient Qutb Minar complex, Delhi

David Henley

PFH1189427

India: The Alai Darwaza (Alai Gate, built 1311 CE) next to the soaring minaret of the Qutb Minar, built in 1193, Delhi

India: The Alai Darwaza (Alai Gate, built 1311 CE) next to the soaring minaret of the Qutb Minar, built in 1193, Delhi

David Henley

PFH1189401

Galaxy Cluster Abell 1656 - Coma Cluster - Wide - field image around the Coma galaxy cluster - Large field around the Coma galaxy cluster. This cluster consists of about a thousand galaxies and is located 330 million light years away in the constellation Coma Berenices (Berenice hair). This cluster is dominated by two large elliptical galaxies (NGC 4874 on the right and NGC 4889 on the left). Below the middle of the image, to the right, is the galaxy NGC 4921. Mosaic of images obtained by the Oschin telescope of 1.2m from Mount Palomar through several filters and composed. The Coma cluster (Abell 1656) is a particularly rich cluster of individual galaxies (over 1000 members), most prominently the two giant ellipticals, NGC 4874 (right) and NGC 4889 (left). NGC 4921 is the small circular galaxy below and a little to the right of the centre of the image. The remaining members are mostly smaller ellipticals. The cluster is seen towards the constellation Coma Berenices, and is actually at

Galaxy Cluster Abell 1656 - Coma Cluster - Wide - field image around the Coma galaxy cluster - Large field around the Coma galaxy cluster. This cluster consists of about a thousand galaxies and is located 330 million light years away in the constellation Coma Berenices (Berenice hair). This cluster is dominated by two large elliptical galaxies (NGC 4874 on the right and NGC 4889 on the left). Below the middle of the image, to the right, is the galaxy NGC 4921. Mosaic of images obtained by the Oschin telescope of 1.2m from Mount Palomar through several filters and composed. The Coma cluster (Abell 1656) is a particularly rich cluster of individual galaxies (over 1000 members), most prominently the two giant ellipticals, NGC 4874 (right) and NGC 4889 (left). NGC 4921 is the small circular galaxy below and a little to the right of the centre of the image. The remaining members are mostly smaller ellipticals. The cluster is seen towards the constellation Coma Berenices, and is actually at

PIX4565314

India: Gandhi Smriti Museum (formerly Birla House), New Delhi

India: Gandhi Smriti Museum (formerly Birla House), New Delhi

David Henley

PFH1189592

India: Personalised number plate at the Gandhi Smriti Museum (formerly Birla House), New Delhi

India: Personalised number plate at the Gandhi Smriti Museum (formerly Birla House), New Delhi

David Henley

PFH1189598

Open cluster NGC 6242 in Scorpio - Open star cluster NGC 6242 in Scorpius - This cluster is about 3500 years old - light from the Sun and is about 50 million years old. A bright yellow star is in the foreground. This cluster is one of many in the sparkling southern constellation of Scorpius. It is marked by a bright yellow star (spectral type K5) which happens to be in the foreground at a distance of about 1000 light years. The cluster itself is about 3,500 light years from the sun. The cluster is slightly dimmed by foreground dust. This so - called interstellar extinction is common with object close to the Galactic plane. Despite this, it is possible to estimate the age of the cluster by measuring the color and relative brightness of its stars. The age turns out to be about 50 million years, which is quite mature for an open cluster of this type. By now, most of the brightest stars will have turned into supernovae and vanished, leaving this quite modest group to compete with the many

Open cluster NGC 6242 in Scorpio - Open star cluster NGC 6242 in Scorpius - This cluster is about 3500 years old - light from the Sun and is about 50 million years old. A bright yellow star is in the foreground. This cluster is one of many in the sparkling southern constellation of Scorpius. It is marked by a bright yellow star (spectral type K5) which happens to be in the foreground at a distance of about 1000 light years. The cluster itself is about 3,500 light years from the sun. The cluster is slightly dimmed by foreground dust. This so - called interstellar extinction is common with object close to the Galactic plane. Despite this, it is possible to estimate the age of the cluster by measuring the color and relative brightness of its stars. The age turns out to be about 50 million years, which is quite mature for an open cluster of this type. By now, most of the brightest stars will have turned into supernovae and vanished, leaving this quite modest group to compete with the many

PIX4568311

Dale in Hordaland 19530425. Dale Fabrikker is Norway's largest textile factory with …, 1953 (photo)

Dale in Hordaland 19530425. Dale Fabrikker is Norway's largest textile factory with …, 1953 (photo)

Sverre A. Børretzen

NTB8929738

India: The almost 2,000 year old Iron Pillar at the Qutb Minar complex, Delhi

India: The almost 2,000 year old Iron Pillar at the Qutb Minar complex, Delhi

David Henley

PFH1189587

India: A crafted stone pillar in the Quwwat-ul-Islam Mosque at the ancient Qutb Minar complex, Delhi

India: A crafted stone pillar in the Quwwat-ul-Islam Mosque at the ancient Qutb Minar complex, Delhi

David Henley

PFH1189431

India: Gandhi Smriti Museum (formerly Birla House), New Delhi

India: Gandhi Smriti Museum (formerly Birla House), New Delhi

David Henley

PFH1189879

Malaspina Glacier, Alaska. 08/1989 - Malaspina Glacier, Alaska, U.S.A. August 1989 - Malaspina Glacier, Alaska, observes from Space Shuttle Columbia. Malaspina Glacier can be seen just left of the center of this northeast - looking, low - oblique photograph. Located in southern Alaska on the shore of the Gulf of Alaska, Malaspina Glacier is a classic example of a piedmont glacier lying at the foot of a mountain range - - in this case, the Saint Elias Mountains (just north of the glacier). The glacier covers an area of 1500 square miles (3900 square kilometers) on the coastal plain, is almost 60 miles (97 kilometers) long, and is more than 1000 feet (300 meters) thick. The Seward Ice Field is the main source of ice for the glacier. The glacier moves in surges that push earlier - formed moraines outward into expanding concentric patterns, which you can see along the flanks of the ice mass. To the northwest of Malaspina Glacier is the curved and pointed Agassiz Glacier, which is also fed

Malaspina Glacier, Alaska. 08/1989 - Malaspina Glacier, Alaska, U.S.A. August 1989 - Malaspina Glacier, Alaska, observes from Space Shuttle Columbia. Malaspina Glacier can be seen just left of the center of this northeast - looking, low - oblique photograph. Located in southern Alaska on the shore of the Gulf of Alaska, Malaspina Glacier is a classic example of a piedmont glacier lying at the foot of a mountain range - - in this case, the Saint Elias Mountains (just north of the glacier). The glacier covers an area of 1500 square miles (3900 square kilometers) on the coastal plain, is almost 60 miles (97 kilometers) long, and is more than 1000 feet (300 meters) thick. The Seward Ice Field is the main source of ice for the glacier. The glacier moves in surges that push earlier - formed moraines outward into expanding concentric patterns, which you can see along the flanks of the ice mass. To the northwest of Malaspina Glacier is the curved and pointed Agassiz Glacier, which is also fed

PIX4672451

Galapagos Islands - The Galapagos Islands seen from the space shuttle - Galapagos Islands (Isabela, the largest, Fernandina, San Salvador and part of Santa Cruz) seen by the space shuttle Endeavour in May 1996. The Galapagos Islands seen from the space shuttle Endeavour in May 1996. Isabela, the largest of the Galapagos Islands; Fernandina; San Salvador; and a partial view of Santa Cruz, are apparent in this southwest - looking, low - oblique photograph. Located on the equator 600 miles (1000 kilometers) west of Ecuador, the rugged volcanic islands began forming 4 to 5 million years ago. Sea - horse - shaped Isabela Island covers 1771 square miles (4588 square kilometers) and has five active volcanoes. Fernandina Island, west - southwest of Isabela, covers 248 square miles (642 square kilometers) and has a single large active volcano with a very distinct caldera that is sometimes filled with water. East - northeast of Isabella lies San Salvador that covers 226 square miles (585 square

Galapagos Islands - The Galapagos Islands seen from the space shuttle - Galapagos Islands (Isabela, the largest, Fernandina, San Salvador and part of Santa Cruz) seen by the space shuttle Endeavour in May 1996. The Galapagos Islands seen from the space shuttle Endeavour in May 1996. Isabela, the largest of the Galapagos Islands; Fernandina; San Salvador; and a partial view of Santa Cruz, are apparent in this southwest - looking, low - oblique photograph. Located on the equator 600 miles (1000 kilometers) west of Ecuador, the rugged volcanic islands began forming 4 to 5 million years ago. Sea - horse - shaped Isabela Island covers 1771 square miles (4588 square kilometers) and has five active volcanoes. Fernandina Island, west - southwest of Isabela, covers 248 square miles (642 square kilometers) and has a single large active volcano with a very distinct caldera that is sometimes filled with water. East - northeast of Isabella lies San Salvador that covers 226 square miles (585 square

PIX4676441

Battle near the village of Sorauren, 1813 (aquatint)

Battle near the village of Sorauren, 1813 (aquatint)

Heath, William (1795-1840) (after)

NAM5920969

Spiral Galaxy NGC 4921 - Galaxy Spiral NGC 4921 - Galaxy NGC 4921 photographed by the Hubble Space Telescope (HST). Located in the cluster of Coma galaxies (Abell 1656) is about 320 million light years old, this spiral galaxy presents an unusual structure with poorly marked arms; some young blue stars are visible but the activity of star formation here is much less strong than in other spiral galaxies. In the background, many more distant galaxies appear. This very deep image taken with the NASA/ESA Hubble Space Telescope shows the spiral galaxy NGC 4921 along with a spectacular backdrop of more distant galaxies. The Coma Galaxy Cluster, in the northern constellation of Coma Berenices, the hair of Queen Berenice, is one of the closest very rich collections of galaxies in the nearby Universe. The cluster, also known as Abell 1656, is about 320 million light - years from Earth and contains more than 1000 members. The brightest galaxies, including NGC 4921 shown here, were discovered back

Spiral Galaxy NGC 4921 - Galaxy Spiral NGC 4921 - Galaxy NGC 4921 photographed by the Hubble Space Telescope (HST). Located in the cluster of Coma galaxies (Abell 1656) is about 320 million light years old, this spiral galaxy presents an unusual structure with poorly marked arms; some young blue stars are visible but the activity of star formation here is much less strong than in other spiral galaxies. In the background, many more distant galaxies appear. This very deep image taken with the NASA/ESA Hubble Space Telescope shows the spiral galaxy NGC 4921 along with a spectacular backdrop of more distant galaxies. The Coma Galaxy Cluster, in the northern constellation of Coma Berenices, the hair of Queen Berenice, is one of the closest very rich collections of galaxies in the nearby Universe. The cluster, also known as Abell 1656, is about 320 million light - years from Earth and contains more than 1000 members. The brightest galaxies, including NGC 4921 shown here, were discovered back

PIX4612034

Super massive star Eta Carinae - Super massive star Eta Carinae - Eta Carinae is one of the most massive stars in our galaxy. Its mass would be about 120 times that of the Sun with a diameter 1000 times larger than our star. The image obtained by the Hubble space telescope reveals two expanding gas lobes; it is the nebula called the Homuncule, vestige of a huge explosion that the star experienced 150 years ago. The star blows its exterior atmosphere and will eventually explode in a supernova. Eta Carinae is located approximately 8000 light years from Earth in the southern constellation of Carene. A huge, billowing pair of gas and dust clouds is captured in this stunning Hubble telescope picture of the super - massive star Eta Carinae. Even though Eta Carinae is more than 8,000 light - years away, features 10 billion miles across (about the diameter of our solar system) can be distinguished. Eta Carinae suffered giant outburst about 150 years ago, when it became one of the brightest sta

Super massive star Eta Carinae - Super massive star Eta Carinae - Eta Carinae is one of the most massive stars in our galaxy. Its mass would be about 120 times that of the Sun with a diameter 1000 times larger than our star. The image obtained by the Hubble space telescope reveals two expanding gas lobes; it is the nebula called the Homuncule, vestige of a huge explosion that the star experienced 150 years ago. The star blows its exterior atmosphere and will eventually explode in a supernova. Eta Carinae is located approximately 8000 light years from Earth in the southern constellation of Carene. A huge, billowing pair of gas and dust clouds is captured in this stunning Hubble telescope picture of the super - massive star Eta Carinae. Even though Eta Carinae is more than 8,000 light - years away, features 10 billion miles across (about the diameter of our solar system) can be distinguished. Eta Carinae suffered giant outburst about 150 years ago, when it became one of the brightest sta

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Interacting galaxies NGC 4038 - 4039 in the Raven - The Antennae galaxy in Corvus - On the left, seen from the ground of the galaxy NGC 4038 - 39 (antenna galaxy), located about 45 million years ago - light. These two galaxies are interacting. The collision started at least 100 million years ago causes intense star formation. On the right, the image made by the space telescope Hubble on 20 January 1996 shows in detail the nuclei of these two twin galaxies surrounded by young clusters of blue stars, more than 1000, made up of young and massive stars. At left, a ground - based telescopic view of the Antennae galaxies (known formally as NGC 4038/4039) - so named because a pair of long tails of luminous matter, formed by the gravitational tidal forces of their encounter, resemble an insect's antennae. The galaxies are located 45 million light - years away in the southern constellation Corvus. At right, the respective cores of the twin galaxies are the orange blobs, left and right of image

Interacting galaxies NGC 4038 - 4039 in the Raven - The Antennae galaxy in Corvus - On the left, seen from the ground of the galaxy NGC 4038 - 39 (antenna galaxy), located about 45 million years ago - light. These two galaxies are interacting. The collision started at least 100 million years ago causes intense star formation. On the right, the image made by the space telescope Hubble on 20 January 1996 shows in detail the nuclei of these two twin galaxies surrounded by young clusters of blue stars, more than 1000, made up of young and massive stars. At left, a ground - based telescopic view of the Antennae galaxies (known formally as NGC 4038/4039) - so named because a pair of long tails of luminous matter, formed by the gravitational tidal forces of their encounter, resemble an insect's antennae. The galaxies are located 45 million light - years away in the southern constellation Corvus. At right, the respective cores of the twin galaxies are the orange blobs, left and right of image

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