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Nijhum Dwip (Nijhum island) once known as Char Osman is a small island under Hatiya Upazila in Noakhali district in Bangladesh. There was no settlement on the island until 1970 before which people used to come to the island on seasonal basis. The island was included in the Hatiya constituency in the early 70s. At that time a large number of people from Hatiya, Shahbajpur and Ramgati, losing their lands and homes in riverbank erosion migrated to the island as new settlers. The Forest Department of the government of Bangladesh created mangrove forest on the island and in 2001 declared it as National Park. The main attraction of the park is a herd of about 25,000 spotted dear or Chitra Horin. Nijhum Dwip, Noakhali, Bangladesh. December 10, 2009. (photo)

UIG802189

Nijhum Dwip (Nijhum island) once known as Char Osman is a small island under Hatiya Upazila in Noakhali district in Bangladesh. There was no settlement on the island until 1970 before which people used to come to the island on seasonal basis. The island was included in the Hatiya constituency in the early 70s. At that time a large number of people from Hatiya, Shahbajpur and Ramgati, losing their lands and homes in riverbank erosion migrated to the island as new settlers. The Forest Department of the government of Bangladesh created mangrove forest on the island and in 2001 declared it as National Park. The main attraction of the park is a herd of about 25,000 spotted dear or Chitra Horin. Nijhum Dwip, Noakhali, Bangladesh. December 10, 2009. (photo)

UIG802189

 
Nijhum Dwip (Nijhum island) once known as Char Osman is a small island under Hatiya Upazila in Noakhali district in Bangladesh. There was no settlement on the island until 1970 before which people used to come to the island on seasonal basis. The island was included in the Hatiya constituency in the early 70s. At that time a large number of people from Hatiya, Shahbajpur and Ramgati, losing their lands and homes in riverbank erosion migrated to the island as new settlers. The Forest Department of the government of Bangladesh created mangrove forest on the island and in 2001 declared it as National Park. The main attraction of the park is a herd of about 25,000 spotted dear or Chitra Horin. Nijhum Dwip, Noakhali, Bangladesh. December 10, 2009. (photo)

UIG802191

Nijhum Dwip (Nijhum island) once known as Char Osman is a small island under Hatiya Upazila in Noakhali district in Bangladesh. There was no settlement on the island until 1970 before which people used to come to the island on seasonal basis. The island was included in the Hatiya constituency in the early 70s. At that time a large number of people from Hatiya, Shahbajpur and Ramgati, losing their lands and homes in riverbank erosion migrated to the island as new settlers. The Forest Department of the government of Bangladesh created mangrove forest on the island and in 2001 declared it as National Park. The main attraction of the park is a herd of about 25,000 spotted dear or Chitra Horin. Nijhum Dwip, Noakhali, Bangladesh. December 10, 2009. (photo)

UIG802191

 
Nebula N70 in the Great Magellan Cloud - The N 70 nebula in Large Magellanic Cloud (LMC) - The Henize 70 nebula extends for about 400 years - light, it is located in the Great Magellan Cloud. In the center, a small group of very massive and extremely hot stars, stars of Wolf - Rayet. Image obtained by Siding Spring's 3.9m telescope. At the centre of this remarkable bubble - like nebula nebula is a small group of extremely hot stars. Some of these stars are rapdly losing mass and have stellar winds blowing from their surfaces with velocities that approach 4000 kilometers per second. Such stars are known as Wolf - Rayet stars and are found in galaxies capable of forming massive stars. There are many such stars in the Large Magellanic Cloud (LMC) but not all of them are associated with distinctive nebulae. The outward flowing streams of energetic particles from Wolf - Rayet (and other energetic stars) eventually interact with the relatively stationary interstellar medium pervading the LMC

PIX4620865

Nebula N70 in the Great Magellan Cloud - The N 70 nebula in Large Magellanic Cloud (LMC) - The Henize 70 nebula extends for about 400 years - light, it is located in the Great Magellan Cloud. In the center, a small group of very massive and extremely hot stars, stars of Wolf - Rayet. Image obtained by Siding Spring's 3.9m telescope. At the centre of this remarkable bubble - like nebula nebula is a small group of extremely hot stars. Some of these stars are rapdly losing mass and have stellar winds blowing from their surfaces with velocities that approach 4000 kilometers per second. Such stars are known as Wolf - Rayet stars and are found in galaxies capable of forming massive stars. There are many such stars in the Large Magellanic Cloud (LMC) but not all of them are associated with distinctive nebulae. The outward flowing streams of energetic particles from Wolf - Rayet (and other energetic stars) eventually interact with the relatively stationary interstellar medium pervading the LMC

PIX4620865

 
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The Battle of Lowestoft, 3 June 1665, Showing HMS 'Royal Charles' and the 'Eendracht', mid-17th century (oil on wood)

Minderhout, Hendrik van (1632-96)

MMM7337616

The Battle of Lowestoft, 3 June 1665, Showing HMS 'Royal Charles' and the 'Eendracht', mid-17th century (oil on wood)

Minderhout, Hendrik van (1632-96)

MMM7337616

 
Nebula N70 in the Great Magellan Cloud - The N 70 nebula in Large Magellanic Cloud (LMC) - The Henize 70 nebula extends for about 400 years - light, it is located in the Great Magellan Cloud. In the center, a small group of very massive and extremely hot stars, stars of Wolf - Rayet. Image obtained by Siding Spring's 3.9m telescope. At the centre of this remarkable bubble - like nebula nebula is a small group of extremely hot stars. Some of these stars are rapdly losing mass and have stellar winds blowing from their surfaces with velocities that approach 4000 kilometers per second. Such stars are known as Wolf - Rayet stars and are found in galaxies capable of forming massive stars. There are many such stars in the Large Magellanic Cloud (LMC) but not all of them are associated with distinctive nebulae. The outward flowing streams of energetic particles from Wolf - Rayet (and other energetic stars) eventually interact with the relatively stationary interstellar medium pervading the LMC

PIX4620872

Nebula N70 in the Great Magellan Cloud - The N 70 nebula in Large Magellanic Cloud (LMC) - The Henize 70 nebula extends for about 400 years - light, it is located in the Great Magellan Cloud. In the center, a small group of very massive and extremely hot stars, stars of Wolf - Rayet. Image obtained by Siding Spring's 3.9m telescope. At the centre of this remarkable bubble - like nebula nebula is a small group of extremely hot stars. Some of these stars are rapdly losing mass and have stellar winds blowing from their surfaces with velocities that approach 4000 kilometers per second. Such stars are known as Wolf - Rayet stars and are found in galaxies capable of forming massive stars. There are many such stars in the Large Magellanic Cloud (LMC) but not all of them are associated with distinctive nebulae. The outward flowing streams of energetic particles from Wolf - Rayet (and other energetic stars) eventually interact with the relatively stationary interstellar medium pervading the LMC

PIX4620872

 
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Phaeton alarm'd, 1808 (etching)

Gillray, James (1757-1815)

MMM7340077

Phaeton alarm'd, 1808 (etching)

Gillray, James (1757-1815)

MMM7340077

 
A’ Squadron 3rd County of London Yeomanry (Sharpshooters) preparing for action near the German Radar Station near Douvres, Normandy, June 1944 (b/w photo)

Sale, Wilfred Herbert James

NAM5922003

A’ Squadron 3rd County of London Yeomanry (Sharpshooters) preparing for action near the German Radar Station near Douvres, Normandy, June 1944 (b/w photo)

Sale, Wilfred Herbert James

NAM5922003

 
A’ Squadron 3rd County of London Yeomanry (Sharpshooters), and infantry of the Black Watch, Normandy, 7 June 1944 (b/w photo)

Sale, Wilfred Herbert James

NAM5922004

A’ Squadron 3rd County of London Yeomanry (Sharpshooters), and infantry of the Black Watch, Normandy, 7 June 1944 (b/w photo)

Sale, Wilfred Herbert James

NAM5922004

 
Pulsar of Crab in Taurus seen in X - The Crab nebula pulsar - Pulsar of Crab in Taurus seen in X by satellite Chandra. The pulsar is the white dot in the center of the image. This neutron star generates a powerful magnetic field creating material jets at the poles, as well as a strong stellar wind. This image gives the first clear view of the faint boundary of the Crab Nebula's X - ray - emitting pulsar wind nebula. The nebula is powered by a rapidly rotating, highly magnetized neutron star, or pulsar (white dot near the center). The combination of rapid rotating and strong magnetic field generates an intense electromagnetic field that creates jets of matter and anti - matter moving away from the north and south poles of the pulsar, and an intense wind flowing out in the equatorial direction. The inner X - ray ring is thought to be a shock wave that marks the boundary between the surrounding nebula and the flow of matter and antimatter particles from the pulsar. Energetic electrons and

PIX4583131

Pulsar of Crab in Taurus seen in X - The Crab nebula pulsar - Pulsar of Crab in Taurus seen in X by satellite Chandra. The pulsar is the white dot in the center of the image. This neutron star generates a powerful magnetic field creating material jets at the poles, as well as a strong stellar wind. This image gives the first clear view of the faint boundary of the Crab Nebula's X - ray - emitting pulsar wind nebula. The nebula is powered by a rapidly rotating, highly magnetized neutron star, or pulsar (white dot near the center). The combination of rapid rotating and strong magnetic field generates an intense electromagnetic field that creates jets of matter and anti - matter moving away from the north and south poles of the pulsar, and an intense wind flowing out in the equatorial direction. The inner X - ray ring is thought to be a shock wave that marks the boundary between the surrounding nebula and the flow of matter and antimatter particles from the pulsar. Energetic electrons and

PIX4583131

 
Egypt: Coin of Cleopatra VII (69-30 BCE), 32 BCE

PFH3085690

Egypt: Coin of Cleopatra VII (69-30 BCE), 32 BCE

PFH3085690

 
Galaxy cluster Abell 2667 - Galaxy cluster Abell 2667 - In this image of the galaxy cluster Abell 2667, a spiral galaxy, at the top left of the image, seems to leave a trail of gas and stars in its wake. Attracted by the high gravity of Abell 2667, this “galaxy - comete” plunges into the cluster at a speed of 3.5 million km/h, losing its gas and young stars. This phenomene may explain the presence of isolated stars in the centre of galaxy clusters. On the right, a further galaxy appears as a gravitational arc. Image obtained by the Hubble Space Telescope in October 2001. The NASA/ESA Hubble Space Telescope, in collaboration with several other ground - and space - based telescopes, has captured a galaxy being ripped apart by a galaxy cluster's gravitational field and harsh environment. The finding sheds light on the mysterious process by which gas - rich spiral - shaped galaxies might evolve into gas - poor irregular - or elliptical - shaped galaxies over billions of years. The new obse

PIX4565700

Galaxy cluster Abell 2667 - Galaxy cluster Abell 2667 - In this image of the galaxy cluster Abell 2667, a spiral galaxy, at the top left of the image, seems to leave a trail of gas and stars in its wake. Attracted by the high gravity of Abell 2667, this “galaxy - comete” plunges into the cluster at a speed of 3.5 million km/h, losing its gas and young stars. This phenomene may explain the presence of isolated stars in the centre of galaxy clusters. On the right, a further galaxy appears as a gravitational arc. Image obtained by the Hubble Space Telescope in October 2001. The NASA/ESA Hubble Space Telescope, in collaboration with several other ground - and space - based telescopes, has captured a galaxy being ripped apart by a galaxy cluster's gravitational field and harsh environment. The finding sheds light on the mysterious process by which gas - rich spiral - shaped galaxies might evolve into gas - poor irregular - or elliptical - shaped galaxies over billions of years. The new obse

PIX4565700

 
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Add 15296 (2) f.18r, Outside the palace, Sugriva and Bali buffet each other furiously with fists and nails and then tear up trees and rocks, but Bali is the stronger and slowly Sugriva is forced to give ground. When Rama sees that Sugriva is losing, he keeps his promise to assist his ally by aiming his deadly arrow into Bali's chest. Bali sinks dying to the ground and the exhausted Sugriva too falls down. Bali bitterly reproaches Rama for his treacherous action in basely and surreptitiously killing him when engaged in fighting another. But Rama tells him that for stealing his younger brother Sugriva's wife Rama, whom he should have regarded as a daughter-in-law, he deserves death. The earth and all that is in it belong to the Iksvaku race and Rama is doing his warrior duty by upholding the rule of law on behalf of his brother Bharata the king. Bali accepts his fate and commends his young son Angada to Rama's protection.

Indian School, (17th century)

BL3283050

Add 15296 (2) f.18r, Outside the palace, Sugriva and Bali buffet each other furiously with fists and nails and then tear up trees and rocks, but Bali is the stronger and slowly Sugriva is forced to give ground. When Rama sees that Sugriva is losing, he keeps his promise to assist his ally by aiming his deadly arrow into Bali's chest. Bali sinks dying to the ground and the exhausted Sugriva too falls down. Bali bitterly reproaches Rama for his treacherous action in basely and surreptitiously killing him when engaged in fighting another. But Rama tells him that for stealing his younger brother Sugriva's wife Rama, whom he should have regarded as a daughter-in-law, he deserves death. The earth and all that is in it belong to the Iksvaku race and Rama is doing his warrior duty by upholding the rule of law on behalf of his brother Bharata the king. Bali accepts his fate and commends his young son Angada to Rama's protection.

Indian School, (17th century)

BL3283050

 
Hurricane on Earth - 09/2008 - Hurricane season on earth - 09/2008 - Image of Earth from GOES satellites - 12 September 3, 2008. Four hurricanes were visible on the Atlantic and one on the Pacific. Near the African coast, the tropical storm Josephine. In the middle of the Atlantic, Hurricane Ike. Near Cuba and the Bahamas, Hurricane Hanna. Above Arkansas, the tropical storm Gustav. Well, west of Baja California, Karina depression. The Atlantic hurricane season typically peaks in early to mid - September after the ocean's surface has had time to heat up in the summer sun. When the GOES satellite captured this view of the atmosphere at 1:45 p.m. Eastern Daylight Time on September 3, four storms were lined up across the Atlantic, and one had developed in the Eastern Pacific. Goes' view of the clouds are overlaid on the NASA Blue Marble. Near the African coast, Tropical Storm Josephine was slowly losing power under the influence of dry air and contrary winds. The storm is little more than

PIX4631836

Hurricane on Earth - 09/2008 - Hurricane season on earth - 09/2008 - Image of Earth from GOES satellites - 12 September 3, 2008. Four hurricanes were visible on the Atlantic and one on the Pacific. Near the African coast, the tropical storm Josephine. In the middle of the Atlantic, Hurricane Ike. Near Cuba and the Bahamas, Hurricane Hanna. Above Arkansas, the tropical storm Gustav. Well, west of Baja California, Karina depression. The Atlantic hurricane season typically peaks in early to mid - September after the ocean's surface has had time to heat up in the summer sun. When the GOES satellite captured this view of the atmosphere at 1:45 p.m. Eastern Daylight Time on September 3, four storms were lined up across the Atlantic, and one had developed in the Eastern Pacific. Goes' view of the clouds are overlaid on the NASA Blue Marble. Near the African coast, Tropical Storm Josephine was slowly losing power under the influence of dry air and contrary winds. The storm is little more than

PIX4631836

 
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The Battle of Quiberon Bay, 20 November 1759, 1779 (oil painting)

Serres, Dominic (1722-93)

MMM7337655

The Battle of Quiberon Bay, 20 November 1759, 1779 (oil painting)

Serres, Dominic (1722-93)

MMM7337655

 
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The Battle of Quiberon Bay, 20 November 1759, 1812 (oil painting)

Pocock, Nicholas (1741-1821)

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The Battle of Quiberon Bay, 20 November 1759, 1812 (oil painting)

Pocock, Nicholas (1741-1821)

MMM7337656

 
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The Battle of Quiberon Bay, 20 November 1759 (oil painting)

Paton, Richard (1717-91)

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The Battle of Quiberon Bay, 20 November 1759 (oil painting)

Paton, Richard (1717-91)

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This representation of His Majesty's Ship 'Magnificent', 74 Guns..., 1830 (hand-coloured aquatint)

British School, (19th century)

MMM7342225

This representation of His Majesty's Ship 'Magnificent', 74 Guns..., 1830 (hand-coloured aquatint)

British School, (19th century)

MMM7342225

 
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View around Abraham Trossel's House, no. 248 from 'Photographic Incidents of the War, the Battle-Field of Gettysburg (albumen print)

O'Sullivan, Timothy (1840-82)

VAH427616

View around Abraham Trossel's House, no. 248 from 'Photographic Incidents of the War, the Battle-Field of Gettysburg (albumen print)

O'Sullivan, Timothy (1840-82)

VAH427616

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