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Images of 'Peaks' found, 1,762

 
Christchurch and the Peninsula of Banks (New Zealand) from space - Christchurch and Banks Peninsula, New Zealand - The Peninsula of Banks and the City of Christchurch seen from the International Space Station (ISS) on August 15, 2006. The Banks Peninsula is an ancient erode volcano forming a peninsula on the east coast of the South Island. Oblique view (the photograph was taken from a side angle) of the city of Christchurch, New Zealand. Snow highlights the peaks of the Banks Peninsula to the southeast of the city. The peninsula has a radically different landscape compared to the adjoining, flat Canterbury Plains, where Christchurch (gray patch to the north) is located. The Banks Peninsula is formed from the overlapping cones of the extinct Lyttelton and Akaroa volcanoes. Subsequent erosion of the cones formed the heavily dissected terrain visible in the image, and sea level rise led to the creation of several harbors around the Peninsula. Erosion continues unabated today, as evidenced

PIX4675641

Christchurch and the Peninsula of Banks (New Zealand) from space - Christchurch and Banks Peninsula, New Zealand - The Peninsula of Banks and the City of Christchurch seen from the International Space Station (ISS) on August 15, 2006. The Banks Peninsula is an ancient erode volcano forming a peninsula on the east coast of the South Island. Oblique view (the photograph was taken from a side angle) of the city of Christchurch, New Zealand. Snow highlights the peaks of the Banks Peninsula to the southeast of the city. The peninsula has a radically different landscape compared to the adjoining, flat Canterbury Plains, where Christchurch (gray patch to the north) is located. The Banks Peninsula is formed from the overlapping cones of the extinct Lyttelton and Akaroa volcanoes. Subsequent erosion of the cones formed the heavily dissected terrain visible in the image, and sea level rise led to the creation of several harbors around the Peninsula. Erosion continues unabated today, as evidenced

PIX4675641

 
Lake Orumieh in Iran seen from space - Lake Urmia in Iran seen from space - Lake Orumieh is the largest lake in Iran. This dirty lake is a UNESCO biosphere reserve. Image obtained from the International Space Station (ISS) on 23 August 2002. Lake Urmia is an isolated lake in Azerbaijan Province in northwest Iran. The total area of the lake is 1815 square miles (4700 square kilometers), and the north - south length is about 90 miles (145 kilometers). The maximum depth of the shallow, saline lake is approximately 50 feet (15 meters). Climatically, the lake region is located in a semiarid, almost desert environment, with general precipitation averaging 12 inches (30 centimeters) per year. Topographically, the entire region is either plateau or mountain. The surface of the lake is approximately 4100 feet (1250 meters) above sea level with several of the individual volcanic peaks reaching more than 7000 feet (2134 meters) above sea level. The massive, rugged mountain range west of the lake

PIX4660548

Lake Orumieh in Iran seen from space - Lake Urmia in Iran seen from space - Lake Orumieh is the largest lake in Iran. This dirty lake is a UNESCO biosphere reserve. Image obtained from the International Space Station (ISS) on 23 August 2002. Lake Urmia is an isolated lake in Azerbaijan Province in northwest Iran. The total area of the lake is 1815 square miles (4700 square kilometers), and the north - south length is about 90 miles (145 kilometers). The maximum depth of the shallow, saline lake is approximately 50 feet (15 meters). Climatically, the lake region is located in a semiarid, almost desert environment, with general precipitation averaging 12 inches (30 centimeters) per year. Topographically, the entire region is either plateau or mountain. The surface of the lake is approximately 4100 feet (1250 meters) above sea level with several of the individual volcanic peaks reaching more than 7000 feet (2134 meters) above sea level. The massive, rugged mountain range west of the lake

PIX4660548

 
St. Helene Island - St. Helena Island - St. Helene Island seen from the International Space Station (ISS) on 7 May 2009. Sainte-Helene is located 1860 km off the African coast in the Atlantic Ocean. Saint Helena Island, located in the South Atlantic Ocean approximately 1,860 kilometers (1,156 miles) west of Africa, was one of the many isolated islands that naturalist Charles Darwin visited during his scientific voyages in the nineteenth century. This image was acquired by astronauts onboard the International Space Station on May 7, 2009. This astronaut photograph shows the island's sharp peaks and deep ravines; the rugged topography results from erosion of the volcanic rocks that make up the island. The change in elevation from the coast to the interior creates a climate gradient. The higher, wetter center is covered with green vegetation, whereas the lower coastal areas are drier and hotter, with little vegetation cover. Human presence on the island has also caused dramatic changes to

PIX4659322

St. Helene Island - St. Helena Island - St. Helene Island seen from the International Space Station (ISS) on 7 May 2009. Sainte-Helene is located 1860 km off the African coast in the Atlantic Ocean. Saint Helena Island, located in the South Atlantic Ocean approximately 1,860 kilometers (1,156 miles) west of Africa, was one of the many isolated islands that naturalist Charles Darwin visited during his scientific voyages in the nineteenth century. This image was acquired by astronauts onboard the International Space Station on May 7, 2009. This astronaut photograph shows the island's sharp peaks and deep ravines; the rugged topography results from erosion of the volcanic rocks that make up the island. The change in elevation from the coast to the interior creates a climate gradient. The higher, wetter center is covered with green vegetation, whereas the lower coastal areas are drier and hotter, with little vegetation cover. Human presence on the island has also caused dramatic changes to

PIX4659322

 
Mars - View of the south pole - Mars South pole - Image of part of the southern polar cap of Mars obtained by the Mars Express probe on December 17, 2012. The bright white region of this image shows the icy cap that covers Mars' south pole, composed of frozen water and carbon dioxide. While it looks smooth in this image, at close quarters the cap is a layered mix of peaks, troughs and flat plains, and has been likened in appearance to swiss cheese. The southern cap reaches some 3 km thick in places, and is around 350 km in diameter. This icy region is permanent; in the martian winter another, thinner ice cap forms over the top of it, stretching further out across the planet and disappearing again when the weather warms up. The cap is around 150 km north of Mars' geographical south pole and Mars Express has shed light on why this ice cap is displaced. Deep impact craters - notably the Hellas Basin, the largest impact structure on the entire planet at 7 km deep and 2300 km across - funne

PIX4616189

Mars - View of the south pole - Mars South pole - Image of part of the southern polar cap of Mars obtained by the Mars Express probe on December 17, 2012. The bright white region of this image shows the icy cap that covers Mars' south pole, composed of frozen water and carbon dioxide. While it looks smooth in this image, at close quarters the cap is a layered mix of peaks, troughs and flat plains, and has been likened in appearance to swiss cheese. The southern cap reaches some 3 km thick in places, and is around 350 km in diameter. This icy region is permanent; in the martian winter another, thinner ice cap forms over the top of it, stretching further out across the planet and disappearing again when the weather warms up. The cap is around 150 km north of Mars' geographical south pole and Mars Express has shed light on why this ice cap is displaced. Deep impact craters - notably the Hellas Basin, the largest impact structure on the entire planet at 7 km deep and 2300 km across - funne

PIX4616189

 
Inside the archaeological complex of Machu Picchu, Peru (photo)

Sergi Reboredo

SRB3584745

Inside the archaeological complex of Machu Picchu, Peru (photo)

Sergi Reboredo

SRB3584745

 
Lake Orumieh in Iran seen from space - Lake Urmia in Iran seen from space - Lake Orumieh is the largest lake in Iran. This dirty lake is a UNESCO biosphere reserve. Image obtained by Space Shuttle Challenger in October 1984. Lake Urmia is an isolated lake in Azerbaijan Province in northwest Iran. The total area of the lake is 1815 square miles (4700 square kilometers), and the north - south length is about 90 miles (145 kilometers). The maximum depth of the shallow, saline lake is approximately 50 feet (15 meters). Climatically, the lake region is located in a semiarid, almost desert environment, with general precipitation averaging 12 inches (30 centimeters) per year. Topographically, the entire region is either plateau or mountain. The surface of the lake is approximately 4100 feet (1250 meters) above sea level with several of the individual volcanic peaks reaching more than 7000 feet (2134 meters) above sea level. The massive, rugged mountain range west of the lake has ridges that e

PIX4660581

Lake Orumieh in Iran seen from space - Lake Urmia in Iran seen from space - Lake Orumieh is the largest lake in Iran. This dirty lake is a UNESCO biosphere reserve. Image obtained by Space Shuttle Challenger in October 1984. Lake Urmia is an isolated lake in Azerbaijan Province in northwest Iran. The total area of the lake is 1815 square miles (4700 square kilometers), and the north - south length is about 90 miles (145 kilometers). The maximum depth of the shallow, saline lake is approximately 50 feet (15 meters). Climatically, the lake region is located in a semiarid, almost desert environment, with general precipitation averaging 12 inches (30 centimeters) per year. Topographically, the entire region is either plateau or mountain. The surface of the lake is approximately 4100 feet (1250 meters) above sea level with several of the individual volcanic peaks reaching more than 7000 feet (2134 meters) above sea level. The massive, rugged mountain range west of the lake has ridges that e

PIX4660581

 
View of the winding road leading to the train des train the archaeological complex of Machu Picchu, Peru (photo)

Sergi Reboredo

SRB3584746

View of the winding road leading to the train des train the archaeological complex of Machu Picchu, Peru (photo)

Sergi Reboredo

SRB3584746

 
Inside the archaeological complex of Machu Picchu, Peru (photo)

Sergi Reboredo

SRB3584744

Inside the archaeological complex of Machu Picchu, Peru (photo)

Sergi Reboredo

SRB3584744

 
Terraces inside the archaeological complex of Machu Picchu, Peru (photo)

Sergi Reboredo

SRB3584747

Terraces inside the archaeological complex of Machu Picchu, Peru (photo)

Sergi Reboredo

SRB3584747

 
Peru Machu Picchu (photo)

Sergi Reboredo

SRB3585204

Peru Machu Picchu (photo)

Sergi Reboredo

SRB3585204

 
Inside the archaeological complex of Machu Picchu, Peru (photo)

Sergi Reboredo

SRB3584743

Inside the archaeological complex of Machu Picchu, Peru (photo)

Sergi Reboredo

SRB3584743

 
Angkor Wat Temple, Cambodia (photo)

Sergi Reboredo

SRB1202561

Angkor Wat Temple, Cambodia (photo)

Sergi Reboredo

SRB1202561

 
Birth of stars in the nebula NGC 3372 - Star formation in the Carina Nebula - Detail of the Carene nebula (NGC 3372) obtained by the Hubble space telescope. The image shows a column of gas eroded by ultraviolet radiation emitted by young stars. Jets are also visible, showing the presence of emerging stars. NGC 3372 is located about 7500 light years away from Earth. The colors used in this image correspond to the emissions of different gases: sulfur in red, hydrogen in green and oxygen in blue. The NASA Hubble Space Telescope photograph captures the chaotic activity atop a three - light - year - tall pillar of gas and dust that is being eaten away by the brilliant light from nearby bright stars. The pillar is also being assaulted from within, as infant stars buried inside it fire off jets of gas that can be seen streaming from towering peaks. This turbulent cosmic pinnacle lies within a tempestuous stellar nursery called the Carina Nebula, located 7,500 light - years away in the souther

PIX4619129

Birth of stars in the nebula NGC 3372 - Star formation in the Carina Nebula - Detail of the Carene nebula (NGC 3372) obtained by the Hubble space telescope. The image shows a column of gas eroded by ultraviolet radiation emitted by young stars. Jets are also visible, showing the presence of emerging stars. NGC 3372 is located about 7500 light years away from Earth. The colors used in this image correspond to the emissions of different gases: sulfur in red, hydrogen in green and oxygen in blue. The NASA Hubble Space Telescope photograph captures the chaotic activity atop a three - light - year - tall pillar of gas and dust that is being eaten away by the brilliant light from nearby bright stars. The pillar is also being assaulted from within, as infant stars buried inside it fire off jets of gas that can be seen streaming from towering peaks. This turbulent cosmic pinnacle lies within a tempestuous stellar nursery called the Carina Nebula, located 7,500 light - years away in the souther

PIX4619129

 
Planetary nebula NGC 6537 in Sagittarius - Hubble observations have revealed huge waves sculpted in the Red Spider nebula. This warm and windy planetary nebula harbours one of the hottest stars in the Universe and its powerful stellar winds generate waves 100 billion kilometers high - intimidating for even the bravest space surfers. The Red Spider Nebula, NGC 6537, is a striking 'butterfly' or bipolar (two - lobed) planetary nebula. Planetary nebulae are the glowing embers of ordinary stars, such as our Sun. At the end of their lives these stars expel most of their material into space, often forming a two - lobed structure as in the case of the Red Spider. These waves are driven by stellar winds radiating from the hot central star, much as a wind passing over a lake can generate waves on the water. The waves reach peaks 100 billion kilometers high and must have been produced by a powerful wind blowing with a speed of 2000 - 4500 kilometers per second (about 7 - 16 million km/hr). The w

PIX4623214

Planetary nebula NGC 6537 in Sagittarius - Hubble observations have revealed huge waves sculpted in the Red Spider nebula. This warm and windy planetary nebula harbours one of the hottest stars in the Universe and its powerful stellar winds generate waves 100 billion kilometers high - intimidating for even the bravest space surfers. The Red Spider Nebula, NGC 6537, is a striking 'butterfly' or bipolar (two - lobed) planetary nebula. Planetary nebulae are the glowing embers of ordinary stars, such as our Sun. At the end of their lives these stars expel most of their material into space, often forming a two - lobed structure as in the case of the Red Spider. These waves are driven by stellar winds radiating from the hot central star, much as a wind passing over a lake can generate waves on the water. The waves reach peaks 100 billion kilometers high and must have been produced by a powerful wind blowing with a speed of 2000 - 4500 kilometers per second (about 7 - 16 million km/hr). The w

PIX4623214

 
CHILE SKORPIOS, 2022 (photography)

Sergi Reboredo

SRB7333674

CHILE SKORPIOS, 2022 (photography)

Sergi Reboredo

SRB7333674

 
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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China, Lijiang, Heilong Tan, Yulong Xue Shan or Jade Dragon Snow Mountain, view from Black Dragon Pool

UDK5432245

China, Lijiang, Heilong Tan, Yulong Xue Shan or Jade Dragon Snow Mountain, view from Black Dragon Pool

UDK5432245

 
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Searching for immortality

BL3264048

Searching for immortality

BL3264048

 
Queen's Road Central, Hong Kong, c.1910 (b/w photo) [1998/028/1/1/136]

BRV3509656

Queen's Road Central, Hong Kong, c.1910 (b/w photo) [1998/028/1/1/136]

BRV3509656

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