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Images of 'South West View' found, 1,726

 
Exterior view, Clifford's Tower, York (photo)

John Bethell

JB24504

Exterior view, Clifford's Tower, York (photo)

John Bethell

JB24504

 
View of Whitby Abbey, North Yorkshire (photo)

John Bethell

JB55606

View of Whitby Abbey, North Yorkshire (photo)

John Bethell

JB55606

 
Mimas, satellite of Saturn, seen by the Cassini probe on 13/02/2010 - Saturn's moon Mimas seen by Cassini spacecraft - February 13 2010 - The Mimas satellite photographed by the Cassini probe on 13 February 2010 has a distance of 50,000 km from the satellite. Mimas is about 400 km in diameter. At the right centre is the large impact crater Herschel, 130 km wide. In this view captured by Nasa's Cassini spacecraft on its closest - ever flyby of Saturn's moon Mimas, large Herschel Crater dominates Mimas, making the moon look like the Death Star in the movie “” Star Wars.”” Herschel Crater is 130 kilometers, or 80 miles, wide and covers most of the right of this image. Cassini came within about 9,500 kilometers (5,900 miles) of Mimas on Feb. 13, 2010.This mosaic was created from six images taken that day in visible light with Cassini's narrow - angle camera on Feb. 13, 2010. The images were re - projected into an orthographic map projection. This view looks toward the area between the regi

PIX4625548

Mimas, satellite of Saturn, seen by the Cassini probe on 13/02/2010 - Saturn's moon Mimas seen by Cassini spacecraft - February 13 2010 - The Mimas satellite photographed by the Cassini probe on 13 February 2010 has a distance of 50,000 km from the satellite. Mimas is about 400 km in diameter. At the right centre is the large impact crater Herschel, 130 km wide. In this view captured by Nasa's Cassini spacecraft on its closest - ever flyby of Saturn's moon Mimas, large Herschel Crater dominates Mimas, making the moon look like the Death Star in the movie “” Star Wars.”” Herschel Crater is 130 kilometers, or 80 miles, wide and covers most of the right of this image. Cassini came within about 9,500 kilometers (5,900 miles) of Mimas on Feb. 13, 2010.This mosaic was created from six images taken that day in visible light with Cassini's narrow - angle camera on Feb. 13, 2010. The images were re - projected into an orthographic map projection. This view looks toward the area between the regi

PIX4625548

 
Tempete sur Saturn seen by the Cassini probe - Huge Storm on Saturn seen by Cassini spacecraft - Evolution of a huge tempete on Saturn seen by the Cassini probe from December 5, 2010 to August 12, 2011. This series of images from Nasa's Cassini spacecraft shows the development of the largest storm seen on the planet since 1990. These true - color and composite near - true - color views chronicle the storm from its start in late 2010 through mid - 2011, showing how the distinct head of the storm quickly grew large but eventually became engulfed by the storm's tail. The earliest image of the storm, taken Dec. 5, 2010, is in the top left of the panel. The storm appears only as a small, white cloud on the terminator between the day side and night side of the planet. The next view, in the top middle of the panel and taken Jan. 2, 2011, shows that the head quickly grew much larger and a tail began to trail a great distance eastward. Some of the clouds moved south and got caught up in a curre

PIX4625230

Tempete sur Saturn seen by the Cassini probe - Huge Storm on Saturn seen by Cassini spacecraft - Evolution of a huge tempete on Saturn seen by the Cassini probe from December 5, 2010 to August 12, 2011. This series of images from Nasa's Cassini spacecraft shows the development of the largest storm seen on the planet since 1990. These true - color and composite near - true - color views chronicle the storm from its start in late 2010 through mid - 2011, showing how the distinct head of the storm quickly grew large but eventually became engulfed by the storm's tail. The earliest image of the storm, taken Dec. 5, 2010, is in the top left of the panel. The storm appears only as a small, white cloud on the terminator between the day side and night side of the planet. The next view, in the top middle of the panel and taken Jan. 2, 2011, shows that the head quickly grew much larger and a tail began to trail a great distance eastward. Some of the clouds moved south and got caught up in a curre

PIX4625230

 
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A view of the reservoir and artificial mount in the gardens of Studley, the seat of William Aislabie, Esq., with a distant view of Fountains Abbey, 1758 (coloured mezzotint)

Nebot, Balthasar (fl.1730-65) (after)

USB393059

A view of the reservoir and artificial mount in the gardens of Studley, the seat of William Aislabie, Esq., with a distant view of Fountains Abbey, 1758 (coloured mezzotint)

Nebot, Balthasar (fl.1730-65) (after)

USB393059

 
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  • Permission required for non-editorial use (inc book and magazine covers). Please contact us
High Level Bridge, Newcastle Upon Tyne, UK (b/w photo)

EHT6948482

High Level Bridge, Newcastle Upon Tyne, UK (b/w photo)

EHT6948482

 
Puffing Billy, 1862 (photo mounted on card)

IGM7426826

Puffing Billy, 1862 (photo mounted on card)

IGM7426826

 
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The Battle of Solebay, 28 May-7 June 1672 (graphite)

Velde, Willem van de, the Elder (1611-93)

MMM7295531

The Battle of Solebay, 28 May-7 June 1672 (graphite)

Velde, Willem van de, the Elder (1611-93)

MMM7295531

 
Apollo 15: J. Irwin on the Moon - Jim Irwin works at the LRV during Apollo 15 EVA - 1 - Irwin works near the Lunar Roving Vehicle. 31/07/1971. Astronaut James B. Irwin, lunar module pilot, works at the Lunar Roving Vehicle (LRV) during the first Apollo 15 lunar surface extravehicular activity (EVA) at the Hadley - Apennine landing site (31 July 1971). The Lunar Module (LM) “” Falcon””” is on the left. The undeployed Laser Ranging Reflector (LR - 3) lies atop the LM's modular equipment stowage assembly (MESA). This view is looking slightly west of south. Hadley Delta and the Apennine Front are in the background to the left. St. George crater is approximately five kilometers (about three statute miles) in the distance behind Irwin's head. This photograph was taken by astronaut David R. Scott, commander. While astronauts Scott and Irwin descended in the LM to explore the moon, astronaut Alfred M. Worden, command module pilot, remained with the Command and Service Modules (CSM) in lunar or

PIX4597336

Apollo 15: J. Irwin on the Moon - Jim Irwin works at the LRV during Apollo 15 EVA - 1 - Irwin works near the Lunar Roving Vehicle. 31/07/1971. Astronaut James B. Irwin, lunar module pilot, works at the Lunar Roving Vehicle (LRV) during the first Apollo 15 lunar surface extravehicular activity (EVA) at the Hadley - Apennine landing site (31 July 1971). The Lunar Module (LM) “” Falcon””” is on the left. The undeployed Laser Ranging Reflector (LR - 3) lies atop the LM's modular equipment stowage assembly (MESA). This view is looking slightly west of south. Hadley Delta and the Apennine Front are in the background to the left. St. George crater is approximately five kilometers (about three statute miles) in the distance behind Irwin's head. This photograph was taken by astronaut David R. Scott, commander. While astronauts Scott and Irwin descended in the LM to explore the moon, astronaut Alfred M. Worden, command module pilot, remained with the Command and Service Modules (CSM) in lunar or

PIX4597336

 
View of Caerphilly Castle, Glamorgan, Wales, built 1268-77 (photo)

John Bethell

JB24641

View of Caerphilly Castle, Glamorgan, Wales, built 1268-77 (photo)

John Bethell

JB24641

 
View looking north across the River Ure towards the house (photo)

John Bethell

JB137624

View looking north across the River Ure towards the house (photo)

John Bethell

JB137624

 
View across the north lake towards the house, Castle Howard, North Yorkshire (photo)

John Bethell

JB137610

View across the north lake towards the house, Castle Howard, North Yorkshire (photo)

John Bethell

JB137610

 
Galaxies Group: Stephan's Quintet in Pegase - Stephan's Quintet group of galaxies - Image obtained with the Hubble space telescope. This group of 5 galaxies is located about 270 million light years away from Earth. In this image three star-forming regions are visible: in the long arm of NGC 7319 (near the center); the gas debris of two galaxies, NGC 7318B and NGC 7318A (upper right); and in the upper left. Blue indicates that these stars are young. This NASA/ESA Hubble Space Telescope image is a close - up view of the central part of Stephan's Quintet, giving a magnificent view of a gigantic cosmic collision. Stephan's Quintet, as its name implies, is a group of five galaxies (NGC7317, 7318A, 7318B, 7319 and 7320) and lies about 270 million light - years away in the constellation of Pegasus (North - west of the Great Square of Pegasus). A sixth galaxy (NGC 7320C) lies south - east of the other five (upper left - hand corner of the overview image). The galaxy group was the first of its

PIX4565462

Galaxies Group: Stephan's Quintet in Pegase - Stephan's Quintet group of galaxies - Image obtained with the Hubble space telescope. This group of 5 galaxies is located about 270 million light years away from Earth. In this image three star-forming regions are visible: in the long arm of NGC 7319 (near the center); the gas debris of two galaxies, NGC 7318B and NGC 7318A (upper right); and in the upper left. Blue indicates that these stars are young. This NASA/ESA Hubble Space Telescope image is a close - up view of the central part of Stephan's Quintet, giving a magnificent view of a gigantic cosmic collision. Stephan's Quintet, as its name implies, is a group of five galaxies (NGC7317, 7318A, 7318B, 7319 and 7320) and lies about 270 million light - years away in the constellation of Pegasus (North - west of the Great Square of Pegasus). A sixth galaxy (NGC 7320C) lies south - east of the other five (upper left - hand corner of the overview image). The galaxy group was the first of its

PIX4565462

 
Shanghai, China (photo)

Sergi Reboredo

SRB3036713

Shanghai, China (photo)

Sergi Reboredo

SRB3036713

 
View the from eastern side of Caerphilly Castle, Glamorgan, Wales, completed 1277 (photo)

John Bethell

JB24623

View the from eastern side of Caerphilly Castle, Glamorgan, Wales, completed 1277 (photo)

John Bethell

JB24623

 
Volcano Arsia Mons - Arsia Mons volcano. - Arsia Mons is one of the largest known volcanoes. It rises more than 9 km above the Martian surface and its caldera extends for 110 km. Image obtained by the Mars Global Surveyor probe. Arsia Mons is one of the largest volcanoes known. This shield volcano is part of an aligned trio known as the Tharsis Montes (the others are Pavonis Mons and Ascraeus Mons). Arsia Mons is rivaled only by Olympus Mons in terms of its volume. The summit of Arsia Mons is more than 9 kilometers (5.6 miles) higher than the surrounding plains. The crater (or caldera) at the volcano summit is approximately 110 km (68 mi) across. This view of Arsia Mons was taken by the red and blue wide angle cameras of the Mars Global Surveyor Mars Orbiter Camera (MOC) system. Bright water ice clouds (the whitish/bluish wisps) hang above the volcano, a common sight every martian afternoon in this region. Arsia Mons is located at 120* west longitude and 9* south latitude. Illumination

PIX4615335

Volcano Arsia Mons - Arsia Mons volcano. - Arsia Mons is one of the largest known volcanoes. It rises more than 9 km above the Martian surface and its caldera extends for 110 km. Image obtained by the Mars Global Surveyor probe. Arsia Mons is one of the largest volcanoes known. This shield volcano is part of an aligned trio known as the Tharsis Montes (the others are Pavonis Mons and Ascraeus Mons). Arsia Mons is rivaled only by Olympus Mons in terms of its volume. The summit of Arsia Mons is more than 9 kilometers (5.6 miles) higher than the surrounding plains. The crater (or caldera) at the volcano summit is approximately 110 km (68 mi) across. This view of Arsia Mons was taken by the red and blue wide angle cameras of the Mars Global Surveyor Mars Orbiter Camera (MOC) system. Bright water ice clouds (the whitish/bluish wisps) hang above the volcano, a common sight every martian afternoon in this region. Arsia Mons is located at 120* west longitude and 9* south latitude. Illumination

PIX4615335

 
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Helmsley Castle - aerial view of the castle in the 16th century, 2004 (w/c on paper)

Dunn, Peter (20th Century)

EHT369084

Helmsley Castle - aerial view of the castle in the 16th century, 2004 (w/c on paper)

Dunn, Peter (20th Century)

EHT369084

 
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General view showing barges moored on the Leeds Liverpool Canal, 1947 (b/w photo)

Ashley, Hallam (20th Century)

EHT368628

General view showing barges moored on the Leeds Liverpool Canal, 1947 (b/w photo)

Ashley, Hallam (20th Century)

EHT368628

 
Enceladus, Saturn's satellite, seen by the Cassini probe - Saturn's moon Enceladus seen by Cassini spacecraft - Mosaic of false-coloured images obtained by the Cassini probe during the flight over this satellite on 5 October 2008. The image shows a fractured region in the southern hemisphere of the satellite. On Oct. 5, 2008, just after coming within 25 kilometers (15.6 miles) of the surface of Enceladus, Nasa's Cassini captured this stunning mosaic as the spacecraft sped away from this geologically active moon of Saturn. Craters and cratered terrains are rare in this view of the southern region of the moon's Saturn - facing hemisphere. Instead, the surface is replete with fractures, folds, and ridges - - all hallmarks of remarkable tectonic activity for a relatively small world. In this enhanced - color view, regions that appear blue - green are thought to be coated with larger grains than those that appear white or gray. Portions of the tiger stripe fractures, or sulci, are visible a

PIX4625451

Enceladus, Saturn's satellite, seen by the Cassini probe - Saturn's moon Enceladus seen by Cassini spacecraft - Mosaic of false-coloured images obtained by the Cassini probe during the flight over this satellite on 5 October 2008. The image shows a fractured region in the southern hemisphere of the satellite. On Oct. 5, 2008, just after coming within 25 kilometers (15.6 miles) of the surface of Enceladus, Nasa's Cassini captured this stunning mosaic as the spacecraft sped away from this geologically active moon of Saturn. Craters and cratered terrains are rare in this view of the southern region of the moon's Saturn - facing hemisphere. Instead, the surface is replete with fractures, folds, and ridges - - all hallmarks of remarkable tectonic activity for a relatively small world. In this enhanced - color view, regions that appear blue - green are thought to be coated with larger grains than those that appear white or gray. Portions of the tiger stripe fractures, or sulci, are visible a

PIX4625451

 
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Shibden Hall, Shibden, Halifax, Calderdale, UK (b/w photo)

EHT6947971

Shibden Hall, Shibden, Halifax, Calderdale, UK (b/w photo)

EHT6947971

 
Martian panorama taken by the rover Opportunity - Martian panorama seen from rover Opportunity - 360 degres panorama obtained by the rover Opportunity from the position where the rover remained for five weeks in November and December 2008. The 276 images that make up this panorama were taken from November 21 to 24, 2008. In this image the rover, whose top of its antenna can be seen in the center of the image, is located about 1 km southwest of the Victoria crater. Opportunity returned to Endeavour crater on December 23, 2008. The Rover Opportunity landed on Mars in the Meridiani Planum region on January 25, 2004. This 360 - degree panorama shows the vista from the location where Nasa's Mars Exploration Rover Opportunity spent five weeks in November and December 2008 while the sun was almost directly in between Mars and Earth, limiting communications. Opportunity is approaching the fifth Earth - year anniversary of its landing on Mars, continuing a surface mission that was initially sch

PIX4615883

Martian panorama taken by the rover Opportunity - Martian panorama seen from rover Opportunity - 360 degres panorama obtained by the rover Opportunity from the position where the rover remained for five weeks in November and December 2008. The 276 images that make up this panorama were taken from November 21 to 24, 2008. In this image the rover, whose top of its antenna can be seen in the center of the image, is located about 1 km southwest of the Victoria crater. Opportunity returned to Endeavour crater on December 23, 2008. The Rover Opportunity landed on Mars in the Meridiani Planum region on January 25, 2004. This 360 - degree panorama shows the vista from the location where Nasa's Mars Exploration Rover Opportunity spent five weeks in November and December 2008 while the sun was almost directly in between Mars and Earth, limiting communications. Opportunity is approaching the fifth Earth - year anniversary of its landing on Mars, continuing a surface mission that was initially sch

PIX4615883

 
Mars: dunes and ice in Chasma Boreale - Mars: dunes and ice in Chasma Boreale - Chasma Boreale is a huge canyon located in the northern polar cap of Mars. This image, obtained by the Mars Express probe, shows Tenuis Cavus, the end of this canyon, where layers of water ice mix with Mars dust. At the bottom of the bowl there are numerous sand dunes. Chasma Boreale is a huge canyon in the northern polar cap. The images taken by Mars Express spacecraft show sharp detail of a series of scarps at the head of Chasma Boreale, a giant trough that almost divides the north polar ice cap in two. The trough is about 318 kilometers long and has cliffs that are almost two kilometers high. The images show layers of water ice and dust possibly for the first time in perspective view. Chasma Boreale is cut into the layered material that lies beneath the water ice of the polar cap. For decades, these layered materials were assumed to consist of a mixture of ice and dust. Recent observations could mean tha

PIX4615964

Mars: dunes and ice in Chasma Boreale - Mars: dunes and ice in Chasma Boreale - Chasma Boreale is a huge canyon located in the northern polar cap of Mars. This image, obtained by the Mars Express probe, shows Tenuis Cavus, the end of this canyon, where layers of water ice mix with Mars dust. At the bottom of the bowl there are numerous sand dunes. Chasma Boreale is a huge canyon in the northern polar cap. The images taken by Mars Express spacecraft show sharp detail of a series of scarps at the head of Chasma Boreale, a giant trough that almost divides the north polar ice cap in two. The trough is about 318 kilometers long and has cliffs that are almost two kilometers high. The images show layers of water ice and dust possibly for the first time in perspective view. Chasma Boreale is cut into the layered material that lies beneath the water ice of the polar cap. For decades, these layered materials were assumed to consist of a mixture of ice and dust. Recent observations could mean tha

PIX4615964

 
1762, Janvier Map of North America and South America, Sea of the West

LZT5456193

1762, Janvier Map of North America and South America, Sea of the West

LZT5456193

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

Paton, Richard (1717-91)

MMM7337654

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

Paton, Richard (1717-91)

MMM7337654

 
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The Black Soldier, WWII

BOF6375136

The Black Soldier, WWII

BOF6375136

 
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A general view of the Catholic church of Shangyanjing (Upper Salt Well) village in Markam county, southwest China's Tibet Autonomous Region Oct 22, 2005

UIG3902992

A general view of the Catholic church of Shangyanjing (Upper Salt Well) village in Markam county, southwest China's Tibet Autonomous Region Oct 22, 2005

UIG3902992

 
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A view of salt fields near the Lancang River at Naxi nationality township of Markam county, southwest China's Tibet Autonomous Region Oct 20, 2005

UIG3901200

A view of salt fields near the Lancang River at Naxi nationality township of Markam county, southwest China's Tibet Autonomous Region Oct 20, 2005

UIG3901200

 
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An exterior view of the Catholic church of Shangyanjing (Upper Salt Well) village in Markam county, southwest China's Tibet Autonomous Region Oct 22, 2005

UIG3902996

An exterior view of the Catholic church of Shangyanjing (Upper Salt Well) village in Markam county, southwest China's Tibet Autonomous Region Oct 22, 2005

UIG3902996

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