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Peru Machu Picchu (photo)

Sergi Reboredo

SRB3585208

Peru Machu Picchu (photo)

Sergi Reboredo

SRB3585208

 
Mount Everest seen from space - Himalaya Mountains, Nepal March 1996 - Part of the Himalayan chain with Mount Everest (below the center, on the left), observed by the shuttle Atlantis in March 1996. At the top of the picture, the foggy plains of northern India, at the bottom the Tibetan plateau. The Himalaya Mountains provide a formidable physical barrier between the hazy environmental conditions of north central India (top) and Nepal (middle), and the clear atmosphere of the Tibetan Plateau (lower third of image). Elevation disparities in this region of the world are tremendous. For example the elevations on the Gangetic Plain in India averages about 300 feet (92 meters) above sea level, the foothills (dark - looking features that run laterally across the image) in Nepal average about 2500 feet (762 meters), and finally the snow capped Himalayas average around 24000 feet (7315 meters). Mt. Everest, highest mountain peak in the world at 29028 feet (8848 meters), is visible as an identi

PIX4661176

Mount Everest seen from space - Himalaya Mountains, Nepal March 1996 - Part of the Himalayan chain with Mount Everest (below the center, on the left), observed by the shuttle Atlantis in March 1996. At the top of the picture, the foggy plains of northern India, at the bottom the Tibetan plateau. The Himalaya Mountains provide a formidable physical barrier between the hazy environmental conditions of north central India (top) and Nepal (middle), and the clear atmosphere of the Tibetan Plateau (lower third of image). Elevation disparities in this region of the world are tremendous. For example the elevations on the Gangetic Plain in India averages about 300 feet (92 meters) above sea level, the foothills (dark - looking features that run laterally across the image) in Nepal average about 2500 feet (762 meters), and finally the snow capped Himalayas average around 24000 feet (7315 meters). Mt. Everest, highest mountain peak in the world at 29028 feet (8848 meters), is visible as an identi

PIX4661176

 
Nepal: A depiction of Shiva on a carved temple roof strut at the Buddhist Rudra Varna Mahavihar (Uku Bahal) temple, Patan, Kathmandu

Chaweewan Chuchuay

PFH2635066

Nepal: A depiction of Shiva on a carved temple roof strut at the Buddhist Rudra Varna Mahavihar (Uku Bahal) temple, Patan, Kathmandu

Chaweewan Chuchuay

PFH2635066

 
Nepal: A depiction of Shiva on a carved temple roof strut at the Buddhist Rudra Varna Mahavihar (Uku Bahal) temple, Patan, Kathmandu

Chaweewan Chuchuay

PFH2635069

Nepal: A depiction of Shiva on a carved temple roof strut at the Buddhist Rudra Varna Mahavihar (Uku Bahal) temple, Patan, Kathmandu

Chaweewan Chuchuay

PFH2635069

 
Nepal: Carved temple roof strut at the Buddhist Rudra Varna Mahavihar (Uku Bahal) temple, Patan, Kathmandu

Chaweewan Chuchuay

PFH2635070

Nepal: Carved temple roof strut at the Buddhist Rudra Varna Mahavihar (Uku Bahal) temple, Patan, Kathmandu

Chaweewan Chuchuay

PFH2635070

 
Mars - Volcanoes Ceraunius Tholus and Uranius Tholus - Mosaic of images obtained by the Mars Express probe between November 25, 2004 and June 22, 2006 during three different orbits. This image shows the volcanoes Ceraunius Tholus (left) and Uranius Tholus (right). These volcanoes measure 130 and 62 km respectively, and s'elevent is 5500m and 4500m. In the second orbit, a cloud was present near the summit of Ceraunius Tholus volcano; in the final mosaic it appears cut in a straight line because the cloud had disappeared in the last image. Ceraunius Tholus and Uranius Tholus are two volcanoes in the Tharsis region of Mars. Ceraunius Tholus is 130 km across and rises 5.5 km above its surroundings. The flanks of this volcano are etched with many valleys. Its neighbour, Uranius Tholus is a smaller volcano, with a base diameter of 62 km and a height of 4.5 km. This image is derived from data acquired during three separate orbits of Mars Express, which took place between 25 November 2004 and

PIX4616192

Mars - Volcanoes Ceraunius Tholus and Uranius Tholus - Mosaic of images obtained by the Mars Express probe between November 25, 2004 and June 22, 2006 during three different orbits. This image shows the volcanoes Ceraunius Tholus (left) and Uranius Tholus (right). These volcanoes measure 130 and 62 km respectively, and s'elevent is 5500m and 4500m. In the second orbit, a cloud was present near the summit of Ceraunius Tholus volcano; in the final mosaic it appears cut in a straight line because the cloud had disappeared in the last image. Ceraunius Tholus and Uranius Tholus are two volcanoes in the Tharsis region of Mars. Ceraunius Tholus is 130 km across and rises 5.5 km above its surroundings. The flanks of this volcano are etched with many valleys. Its neighbour, Uranius Tholus is a smaller volcano, with a base diameter of 62 km and a height of 4.5 km. This image is derived from data acquired during three separate orbits of Mars Express, which took place between 25 November 2004 and

PIX4616192

 
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

 
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

SRB3584745

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

Sergi Reboredo

SRB3584745

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

Sergi Reboredo

SRB3584744

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

Sergi Reboredo

SRB3584744

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

Sergi Reboredo

SRB3584743

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

Sergi Reboredo

SRB3584743

 
Peru Machu Picchu (photo)

Sergi Reboredo

SRB3585204

Peru Machu Picchu (photo)

Sergi Reboredo

SRB3585204

 
Mars: crater in Myers Valles - Mars: crater in Myers Valles - Mamers Valles is a valley about 1000 km long located in the region of Deuteronilus Mensae, north of Arabia Terra. The image obtained by the Mars Express probe on 5 August 2006 shows a crater at the end of this valley. This circular formation measures about thirty kilometres in diameter and is 1400 metres deep. There are traces of flow of material probably composed of water ice, similar to the relief left by the passage of glaciers on Earth. The High - Resolution Stereo Camera (HRSC) onboard the ESA spacecraft Mars Express obtained images focusing on a depression that displays a crater at the end of the long, winding valley, Mamers Valles. The data was obtained on 5 August 2006 with a ground resolution of approximately 14 m/per pixel. The image is centred at approximately 39* north and 17* east on the planet. The valley of Mamers Valles is approximately 1000 km long, running along the boundary between the northern lowlands an

PIX4616082

Mars: crater in Myers Valles - Mars: crater in Myers Valles - Mamers Valles is a valley about 1000 km long located in the region of Deuteronilus Mensae, north of Arabia Terra. The image obtained by the Mars Express probe on 5 August 2006 shows a crater at the end of this valley. This circular formation measures about thirty kilometres in diameter and is 1400 metres deep. There are traces of flow of material probably composed of water ice, similar to the relief left by the passage of glaciers on Earth. The High - Resolution Stereo Camera (HRSC) onboard the ESA spacecraft Mars Express obtained images focusing on a depression that displays a crater at the end of the long, winding valley, Mamers Valles. The data was obtained on 5 August 2006 with a ground resolution of approximately 14 m/per pixel. The image is centred at approximately 39* north and 17* east on the planet. The valley of Mamers Valles is approximately 1000 km long, running along the boundary between the northern lowlands an

PIX4616082

 
Mars: crater in Myers Valles - Mars: crater in Myers Valles - Mamers Valles is a valley about 1000 km long located in the region of Deuteronilus Mensae, north of Arabia Terra. The image obtained by the Mars Express probe on 5 August 2006 shows a crater at the end of this valley. This circular formation measures about thirty kilometres in diameter and is 1400 metres deep. There are traces of flow of material probably composed of water ice, similar to the relief left by the passage of glaciers on Earth. The darker area could be caused by local erosion or wind-driven material. The High - Resolution Stereo Camera (HRSC) onboard the ESA spacecraft Mars Express obtained images focusing on a depression that displays a crater at the end of the long, winding valley, Mamers Valles. The data was obtained on 5 August 2006 with a ground resolution of approximately 14 m/per pixel. The image is centred at approximately 39* north and 17* east on the planet. The valley of Mamers Valles is approximately

PIX4616090

Mars: crater in Myers Valles - Mars: crater in Myers Valles - Mamers Valles is a valley about 1000 km long located in the region of Deuteronilus Mensae, north of Arabia Terra. The image obtained by the Mars Express probe on 5 August 2006 shows a crater at the end of this valley. This circular formation measures about thirty kilometres in diameter and is 1400 metres deep. There are traces of flow of material probably composed of water ice, similar to the relief left by the passage of glaciers on Earth. The darker area could be caused by local erosion or wind-driven material. The High - Resolution Stereo Camera (HRSC) onboard the ESA spacecraft Mars Express obtained images focusing on a depression that displays a crater at the end of the long, winding valley, Mamers Valles. The data was obtained on 5 August 2006 with a ground resolution of approximately 14 m/per pixel. The image is centred at approximately 39* north and 17* east on the planet. The valley of Mamers Valles is approximately

PIX4616090

 
Tyndall Glacier, Chile - Tyndall Glacier, Chile - The Tyndall Glacier in Torres del Paine National Park in Chile, observed from the International Space Station in November 2007. Tyndall Glacier is located in the Torres del Paine National Park in Chile. This glacier, which has a total area of 331 square kilometers and a length of 32 kilometers (based on 1996 measurements), begins in the Patagonian Andes Mountains to the west and terminates in Lago Geikie. The digital astronaut photograph taken in november 2007 records visible light in red, green, and blue wavelengths (true color). The Tyndall Glacier terminus has retreated significantly during the past 17 years. Significant ice loss was also observed earlier this year at Grey Glacier, about 30 kilometers to the north - northeast, suggesting both glaciers are responding similarly to regional changes in temperature and precipitation. A medial moraine is visible in the center of the glacier, extending along its length (top image, center le

PIX4675989

Tyndall Glacier, Chile - Tyndall Glacier, Chile - The Tyndall Glacier in Torres del Paine National Park in Chile, observed from the International Space Station in November 2007. Tyndall Glacier is located in the Torres del Paine National Park in Chile. This glacier, which has a total area of 331 square kilometers and a length of 32 kilometers (based on 1996 measurements), begins in the Patagonian Andes Mountains to the west and terminates in Lago Geikie. The digital astronaut photograph taken in november 2007 records visible light in red, green, and blue wavelengths (true color). The Tyndall Glacier terminus has retreated significantly during the past 17 years. Significant ice loss was also observed earlier this year at Grey Glacier, about 30 kilometers to the north - northeast, suggesting both glaciers are responding similarly to regional changes in temperature and precipitation. A medial moraine is visible in the center of the glacier, extending along its length (top image, center le

PIX4675989

 
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  • Content within this photograph may require additional clearances (eg: trademark and personality rights) depending on Licensee's specific use of material, which may include book and magazine cover use.
Saxony, GDR, historical, hotel, restaurants, restaurants, cafes, Beer …, 1985 (photo)

Sächsische Zeitung

IMO8758572

Saxony, GDR, historical, hotel, restaurants, restaurants, cafes, Beer …, 1985 (photo)

Sächsische Zeitung

IMO8758572

 
Africa by satellite. Chad - Possible impact crateres - radar view - 20/03/1996 The impact of an asteroid or comet several hundred million years ago left scars in the landscape that are still visible in this spaceborne radar image of an area in the Sahara Desert of northern Chad. The concentric ring structure left of center is the Aorounga impact crater with a diameter of about 17 kilometers (10.5 miles). Scientists are using radar images to investigate the possibility that Aorounga formed as part of a multiple impact event. A proposed second crater, similar in size to the main structure, appears as a circular trough surrounding a central peak in the center of the image. A third structure, also about the same size, is seen as a dark, partial circular trough with a possible central structure in the right center of the image. The proposed crater “” chain”” could have formed when a 1 km to 2 km (0.5 mile to 1 mile) diameter object broke apart before impact. The dark streaks are deposits of

PIX4659396

Africa by satellite. Chad - Possible impact crateres - radar view - 20/03/1996 The impact of an asteroid or comet several hundred million years ago left scars in the landscape that are still visible in this spaceborne radar image of an area in the Sahara Desert of northern Chad. The concentric ring structure left of center is the Aorounga impact crater with a diameter of about 17 kilometers (10.5 miles). Scientists are using radar images to investigate the possibility that Aorounga formed as part of a multiple impact event. A proposed second crater, similar in size to the main structure, appears as a circular trough surrounding a central peak in the center of the image. A third structure, also about the same size, is seen as a dark, partial circular trough with a possible central structure in the right center of the image. The proposed crater “” chain”” could have formed when a 1 km to 2 km (0.5 mile to 1 mile) diameter object broke apart before impact. The dark streaks are deposits of

PIX4659396

 
Mars: crater in Myers Valles - Mars: crater in Myers Valles - Mamers Valles is a valley about 1000 km long located in the region of Deuteronilus Mensae, north of Arabia Terra. The image obtained by the Mars Express probe on 5 August 2006 shows a crater at the end of this valley. This circular formation measures about thirty kilometres in diameter and is 1400 metres deep. There are traces of flow of material probably composed of water ice, similar to the relief left by the passage of glaciers on Earth. The darker area could be caused by local erosion or wind-driven material. The High - Resolution Stereo Camera (HRSC) onboard the ESA spacecraft Mars Express obtained images focusing on a depression that displays a crater at the end of the long, winding valley, Mamers Valles. The data was obtained on 5 August 2006 with a ground resolution of approximately 14 m/per pixel. The image is centred at approximately 39* north and 17* east on the planet. The valley of Mamers Valles is approximately

PIX4616083

Mars: crater in Myers Valles - Mars: crater in Myers Valles - Mamers Valles is a valley about 1000 km long located in the region of Deuteronilus Mensae, north of Arabia Terra. The image obtained by the Mars Express probe on 5 August 2006 shows a crater at the end of this valley. This circular formation measures about thirty kilometres in diameter and is 1400 metres deep. There are traces of flow of material probably composed of water ice, similar to the relief left by the passage of glaciers on Earth. The darker area could be caused by local erosion or wind-driven material. The High - Resolution Stereo Camera (HRSC) onboard the ESA spacecraft Mars Express obtained images focusing on a depression that displays a crater at the end of the long, winding valley, Mamers Valles. The data was obtained on 5 August 2006 with a ground resolution of approximately 14 m/per pixel. The image is centred at approximately 39* north and 17* east on the planet. The valley of Mamers Valles is approximately

PIX4616083

 
Open cluster Westerlund 2 in Carene - Open cluster Westerlund 2 in Carina - The open cluster Westerlund 2 is located about 20,000 years - light in the southern constellation of Carene, within the nebula Gum 29. About 3000 stars form this cluster. It contains a significant number of massive stars including one of the most massive stars known to date: WR 20a. Image obtained by the Hubble Space Telescope. The sparkling centerpiece of this image taken by the Hubble space telescope is a giant cluster of about 3,000 stars called Westerlund 2, named for Swedish astronomer Bengt Westerlund, who discovered the grouping in the 1960s. The cluster resides in a raucous stellar breeding ground known as Gum 29, located 20,000 light - years away from Earth in the constellation Carina. To capture this image, Hubble's near - infrared Wide Field Camera 3 near - infrared pierced through the dusty veil shrouding the stellar nursery, giving astronomers a clear view of the nebula and the dense concentration

PIX4569094

Open cluster Westerlund 2 in Carene - Open cluster Westerlund 2 in Carina - The open cluster Westerlund 2 is located about 20,000 years - light in the southern constellation of Carene, within the nebula Gum 29. About 3000 stars form this cluster. It contains a significant number of massive stars including one of the most massive stars known to date: WR 20a. Image obtained by the Hubble Space Telescope. The sparkling centerpiece of this image taken by the Hubble space telescope is a giant cluster of about 3,000 stars called Westerlund 2, named for Swedish astronomer Bengt Westerlund, who discovered the grouping in the 1960s. The cluster resides in a raucous stellar breeding ground known as Gum 29, located 20,000 light - years away from Earth in the constellation Carina. To capture this image, Hubble's near - infrared Wide Field Camera 3 near - infrared pierced through the dusty veil shrouding the stellar nursery, giving astronomers a clear view of the nebula and the dense concentration

PIX4569094

 
CHILE SKORPIOS, 2022 (photography)

Sergi Reboredo

SRB7333674

CHILE SKORPIOS, 2022 (photography)

Sergi Reboredo

SRB7333674

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