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Io, one of the moons of Jupiter, showing a volcanic eruption on the horizon, 1979

UIS5071892

Io, one of the moons of Jupiter, showing a volcanic eruption on the horizon, 1979

UIS5071892

 
Mars - Illustration - Mars - Illustration - Artist's view of the planet Mars. The three volcanoes of Tharsis and Olympus Mons are visible on the left. In the centre is the great canyon Valles Marineris. A “” full””” Mars. In this image the massive volcano Olympus Mons is clearly visible upper left of center, while near center are the three Tharsis Montes volcanoes. All these volcanoes are believed to be extinct. To the right of the Tharsis Montes are the deep canyons of Valles Marineris, a meandering network of channels as long as the United States is wide. Mars has been known historically as a bright, reddish “” star”” in Earth's sky. The ruddy hue is due to the presence of iron oxide (i.e., rust) on the martian surface. Mars is often host to white clouds of water - ice crystals (like the high - altitude cirrus clouds on Earth) and experiences seasonal dust storms that can cover the entire planet

Walter B Myers

PIX4616786

Mars - Illustration - Mars - Illustration - Artist's view of the planet Mars. The three volcanoes of Tharsis and Olympus Mons are visible on the left. In the centre is the great canyon Valles Marineris. A “” full””” Mars. In this image the massive volcano Olympus Mons is clearly visible upper left of center, while near center are the three Tharsis Montes volcanoes. All these volcanoes are believed to be extinct. To the right of the Tharsis Montes are the deep canyons of Valles Marineris, a meandering network of channels as long as the United States is wide. Mars has been known historically as a bright, reddish “” star”” in Earth's sky. The ruddy hue is due to the presence of iron oxide (i.e., rust) on the martian surface. Mars is often host to white clouds of water - ice crystals (like the high - altitude cirrus clouds on Earth) and experiences seasonal dust storms that can cover the entire planet

Walter B Myers

PIX4616786

 
La Palma Observatory: Telescope FACT - La Palma Observatory: The FACT telescope: FACT (First G-APD Cherenkov Telescope) is a telescope located at the Roque de los Muchachos Observatory in La Palma, Canary Islands. One of the MAGIC telescopes is visible in the background. The First G-APD Cherenkov Telescope (FACT) is the first imaging atmospheric Cherenkov telescope using Geiger-mode avalanche photodiods (G-APDs) as photo sensors. The rather small, low-cost telescope will not only serve as a test bench for this technology in Cherenkov astronomy, but also monitor bright active galactic nuclei (AGN) in the TeV energy range. Image taken at Observatorio del Roque de Los Muchachos, Canary Islands, Spain. One of the MAGIC (Major Atmospheric Gamma-ray Imaging Cherenkov Telescopes) is visible in the background. The Canary Islands are volcanic in origin and the whole observatory lies on the edge of the Taburiente volcano

Alex Tudorica

PIX4654590

La Palma Observatory: Telescope FACT - La Palma Observatory: The FACT telescope: FACT (First G-APD Cherenkov Telescope) is a telescope located at the Roque de los Muchachos Observatory in La Palma, Canary Islands. One of the MAGIC telescopes is visible in the background. The First G-APD Cherenkov Telescope (FACT) is the first imaging atmospheric Cherenkov telescope using Geiger-mode avalanche photodiods (G-APDs) as photo sensors. The rather small, low-cost telescope will not only serve as a test bench for this technology in Cherenkov astronomy, but also monitor bright active galactic nuclei (AGN) in the TeV energy range. Image taken at Observatorio del Roque de Los Muchachos, Canary Islands, Spain. One of the MAGIC (Major Atmospheric Gamma-ray Imaging Cherenkov Telescopes) is visible in the background. The Canary Islands are volcanic in origin and the whole observatory lies on the edge of the Taburiente volcano

Alex Tudorica

PIX4654590

 
Jupiter and Io seen by the New Horizons probe

PIX4574952

Jupiter and Io seen by the New Horizons probe

PIX4574952

 
Tenoumer impact crater, Mauritania - Tenoumer impact crater, Mauritania - The Tenoumer impact crater in Mauritania is said to have been formed 10,000 to 30,000 years ago and has a diameter of 1.9 km. Image made from the International Space Station on 1 March 2007. Tenoumer impact crater, Mauritania, as seen by the International Space Station on march 1st 2007. Nearly a perfect circle, it is 1.9 kilometers (1.2 miles) wide, and sports a rim 100 meters (330 feet) high. The crater sits in a vast plain of rocks so ancient they were deposited hundreds of millions of years before the first dinosaurs walked the Earth. Modern geologists long debated what caused this crater, some of them favoring a volcano. But closer examination of the structure revealed that the crater's hardened lava”” was actually rock that had melted from a meteorite impact. Although it resides in ancient rock, Tenoumer is geologically young, ranging in age between roughly 10,000 and 30,000 years old.

PIX4630656

Tenoumer impact crater, Mauritania - Tenoumer impact crater, Mauritania - The Tenoumer impact crater in Mauritania is said to have been formed 10,000 to 30,000 years ago and has a diameter of 1.9 km. Image made from the International Space Station on 1 March 2007. Tenoumer impact crater, Mauritania, as seen by the International Space Station on march 1st 2007. Nearly a perfect circle, it is 1.9 kilometers (1.2 miles) wide, and sports a rim 100 meters (330 feet) high. The crater sits in a vast plain of rocks so ancient they were deposited hundreds of millions of years before the first dinosaurs walked the Earth. Modern geologists long debated what caused this crater, some of them favoring a volcano. But closer examination of the structure revealed that the crater's hardened lava”” was actually rock that had melted from a meteorite impact. Although it resides in ancient rock, Tenoumer is geologically young, ranging in age between roughly 10,000 and 30,000 years old.

PIX4630656

 
Frescos on the wall of Sigiriya rock, in Matale district of Sri Lanka. This 370 meter high lava mound of an ancient volcano is famous for the fortified palace complex, built during the reign of King Kasyapa, 477 Ð 495 AD. After his death, the place was turned into a Buddhist monetary. The paintings, very similar to the paintings of India's Ajanta Cave, cover an area of 140 meters long and 40 meters high on the wall of the rock. It is one of the seven World Heritage sites in Sri Lanka and is also a popular tourist destination. June 27, 2008. (photo)

UIG801127

Frescos on the wall of Sigiriya rock, in Matale district of Sri Lanka. This 370 meter high lava mound of an ancient volcano is famous for the fortified palace complex, built during the reign of King Kasyapa, 477 Ð 495 AD. After his death, the place was turned into a Buddhist monetary. The paintings, very similar to the paintings of India's Ajanta Cave, cover an area of 140 meters long and 40 meters high on the wall of the rock. It is one of the seven World Heritage sites in Sri Lanka and is also a popular tourist destination. June 27, 2008. (photo)

UIG801127

 
Fresco on the wall of Sigiriya rock, in Matale district of Sri Lanka. This 370 meter high lava mound of an ancient volcano is famous for the fortified palace complex, built during the reign of King Kasyapa, 477 Ð 495 AD. After his death, the place was turned into a Buddhist monetary. The paintings, very similar to the paintings of India's Ajanta Cave, cover an area of 140 meters long and 40 meters high on the wall of the rock. It is one of the seven World Heritage sites in Sri Lanka and is also a popular tourist destination. June 27, 2008. (photo)

UIG801124

Fresco on the wall of Sigiriya rock, in Matale district of Sri Lanka. This 370 meter high lava mound of an ancient volcano is famous for the fortified palace complex, built during the reign of King Kasyapa, 477 Ð 495 AD. After his death, the place was turned into a Buddhist monetary. The paintings, very similar to the paintings of India's Ajanta Cave, cover an area of 140 meters long and 40 meters high on the wall of the rock. It is one of the seven World Heritage sites in Sri Lanka and is also a popular tourist destination. June 27, 2008. (photo)

UIG801124

 
Fresco on the wall of Sigiriya rock, in Matale district of Sri Lanka. This 370 meter high lava mound of an ancient volcano is famous for the fortified palace complex, built during the reign of King Kasyapa, 477 Ð 495 AD. After his death, the place was turned into a Buddhist monetary. The paintings, very similar to the paintings of India's Ajanta Cave, cover an area of 140 meters long and 40 meters high on the wall of the rock. It is one of the seven World Heritage sites in Sri Lanka and is also a popular tourist destination. June 27, 2008. (photo)

UIG801125

Fresco on the wall of Sigiriya rock, in Matale district of Sri Lanka. This 370 meter high lava mound of an ancient volcano is famous for the fortified palace complex, built during the reign of King Kasyapa, 477 Ð 495 AD. After his death, the place was turned into a Buddhist monetary. The paintings, very similar to the paintings of India's Ajanta Cave, cover an area of 140 meters long and 40 meters high on the wall of the rock. It is one of the seven World Heritage sites in Sri Lanka and is also a popular tourist destination. June 27, 2008. (photo)

UIG801125

 
Frescos on the wall of Sigiriya rock, in Matale district of Sri Lanka. This 370 meter high lava mound of an ancient volcano is famous for the fortified palace complex, built during the reign of King Kasyapa, 477 Ð 495 AD. After his death, the place was turned into a Buddhist monetary. The paintings, very similar to the paintings of India's Ajanta Cave, cover an area of 140 meters long and 40 meters high on the wall of the rock. It is one of the seven World Heritage sites in Sri Lanka and is also a popular tourist destination. June 27, 2008. (photo)

UIG801126

Frescos on the wall of Sigiriya rock, in Matale district of Sri Lanka. This 370 meter high lava mound of an ancient volcano is famous for the fortified palace complex, built during the reign of King Kasyapa, 477 Ð 495 AD. After his death, the place was turned into a Buddhist monetary. The paintings, very similar to the paintings of India's Ajanta Cave, cover an area of 140 meters long and 40 meters high on the wall of the rock. It is one of the seven World Heritage sites in Sri Lanka and is also a popular tourist destination. June 27, 2008. (photo)

UIG801126

 
A Cognocenti Contemplating Ye Beauties of Ye Antique, Gillray, James, 1756-1815, Engraver, [London]: H. Humphrey, 1801, an Elderly Sir William Hamilton Inspecting His Antiquities, All of which Refer to His Wife, Lady Emma Hamilton and Her Lover, Lord Horatio Nelson. In the Background Hang Four Pictures on the Wall: Cleopatra, a Picture of Lady Hamilton with Her Breasts Exposed, Holding a Gin Bottle; Mark Anthony, Lord Nelson with a Sea Battle in Background: An Erupting Volcano; and a Portrait of Hamilton, Facing Away from the Other Paintings.

LZT1012649

A Cognocenti Contemplating Ye Beauties of Ye Antique, Gillray, James, 1756-1815, Engraver, [London]: H. Humphrey, 1801, an Elderly Sir William Hamilton Inspecting His Antiquities, All of which Refer to His Wife, Lady Emma Hamilton and Her Lover, Lord Horatio Nelson. In the Background Hang Four Pictures on the Wall: Cleopatra, a Picture of Lady Hamilton with Her Breasts Exposed, Holding a Gin Bottle; Mark Anthony, Lord Nelson with a Sea Battle in Background: An Erupting Volcano; and a Portrait of Hamilton, Facing Away from the Other Paintings.

LZT1012649

 
Saint Denis, Reunion island (photo)

Sergi Reboredo

SRB1202707

Saint Denis, Reunion island (photo)

Sergi Reboredo

SRB1202707

 
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Monastery on the Island of Santorini, Greece

Prince Nicholas of Greece and Denmark (1872-1938)

USB1160302

Monastery on the Island of Santorini, Greece

Prince Nicholas of Greece and Denmark (1872-1938)

USB1160302

 
Mars seen by the Hubble Space Telescope - 2016 - Mars in opposition 2016 - Image obtained on 12 May 2016 a few days before the opposition of Mars when the planet was only 80 million km away from Earth. This image shows planet Mars, as it was observed shortly before opposition in 2016, taken when the planet was 50 million miles from Earth on May 12, 2016. by the NASA/ESA Hubble Space Telescope. The photo reveals details as small as 20 miles to 30 miles across. This observation was made just a few days before March opposition on May 22, when the sun and Mars will be on exact opposite sides of Earth. Mars also will be 47.4 million miles from Earth. On May 30, Mars will be the closest it has been to Earth in 11 years, at a distance of 46.8 million miles. Some prominent features of the planet are clearly visible: the ancient and inactive shield volcano Syrtis Major; the bright and oval Hellas Planitia basin; the heavily eroded Arabia Terra in the centre of the image; the dark features of Si

PIX4614997

Mars seen by the Hubble Space Telescope - 2016 - Mars in opposition 2016 - Image obtained on 12 May 2016 a few days before the opposition of Mars when the planet was only 80 million km away from Earth. This image shows planet Mars, as it was observed shortly before opposition in 2016, taken when the planet was 50 million miles from Earth on May 12, 2016. by the NASA/ESA Hubble Space Telescope. The photo reveals details as small as 20 miles to 30 miles across. This observation was made just a few days before March opposition on May 22, when the sun and Mars will be on exact opposite sides of Earth. Mars also will be 47.4 million miles from Earth. On May 30, Mars will be the closest it has been to Earth in 11 years, at a distance of 46.8 million miles. Some prominent features of the planet are clearly visible: the ancient and inactive shield volcano Syrtis Major; the bright and oval Hellas Planitia basin; the heavily eroded Arabia Terra in the centre of the image; the dark features of Si

PIX4614997

 
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Vesuvius 1944

BOF6289580

Vesuvius 1944

BOF6289580

 
Saint Denis, Reuinion Island (photo)

Sergi Reboredo

SRB1202705

Saint Denis, Reuinion Island (photo)

Sergi Reboredo

SRB1202705

 
March: Promethei Planum - Mars: Promethei Planum - Promethei Planum is a region located near the southern pole of Mars. This region is seasonally covered with a thick layer of ice up to 3500 metres thick. On this image obtained by the Mars Express probe on September 22, 2005, an impact crater about 100 km wide and 800 metres deep is visible to the right (north). It is partially covered with ice. In the center of the image, structures formed by lava flows; on the left of the image, ice, which is an extension of the southern polar cap. Promethei Planum, an area seasonally covered with layer of ice more than 3500 m thick layer of ice in the martian south polar region, was the subject of the High Resolution Stereo Camera's focus on 22 September 2005 as Mars Express was in orbit above the Red Planet. Promethei Planum lies at approximately 76* south and 105* east. An approximately 100 km - large and 800 m - deep impact crater is visible in the northern part of the image. The crater's interio

PIX4616118

March: Promethei Planum - Mars: Promethei Planum - Promethei Planum is a region located near the southern pole of Mars. This region is seasonally covered with a thick layer of ice up to 3500 metres thick. On this image obtained by the Mars Express probe on September 22, 2005, an impact crater about 100 km wide and 800 metres deep is visible to the right (north). It is partially covered with ice. In the center of the image, structures formed by lava flows; on the left of the image, ice, which is an extension of the southern polar cap. Promethei Planum, an area seasonally covered with layer of ice more than 3500 m thick layer of ice in the martian south polar region, was the subject of the High Resolution Stereo Camera's focus on 22 September 2005 as Mars Express was in orbit above the Red Planet. Promethei Planum lies at approximately 76* south and 105* east. An approximately 100 km - large and 800 m - deep impact crater is visible in the northern part of the image. The crater's interio

PIX4616118

 
March: Promethei Planum - Mars: Promethei Planum - Promethei Planum is a region located near the southern pole of Mars. This region is seasonally covered with a thick layer of ice up to 3500 metres thick. On this perspective image obtained by the Mars Express probe on September 22, 2005, an impact crater about 100 km wide and 800 metres deep is visible at the bottom of the image. It is partially covered with ice. On top, structures formed by lava flows; at the top of the picture, ice, which is an extension of the southern polar cap. Promethei Planum, an area seasonally covered with layer of ice more than 3500 m thick layer of ice in the martian south polar region, was the subject of the High Resolution Stereo Camera's focus on 22 September 2005 as Mars Express was in orbit above the Red Planet. Promethei Planum lies at approximately 76* south and 105* east. An approximately 100 km - large and 800 m - deep impact crater is visible in the bottom of the image. The crater's interior is par

PIX4616138

March: Promethei Planum - Mars: Promethei Planum - Promethei Planum is a region located near the southern pole of Mars. This region is seasonally covered with a thick layer of ice up to 3500 metres thick. On this perspective image obtained by the Mars Express probe on September 22, 2005, an impact crater about 100 km wide and 800 metres deep is visible at the bottom of the image. It is partially covered with ice. On top, structures formed by lava flows; at the top of the picture, ice, which is an extension of the southern polar cap. Promethei Planum, an area seasonally covered with layer of ice more than 3500 m thick layer of ice in the martian south polar region, was the subject of the High Resolution Stereo Camera's focus on 22 September 2005 as Mars Express was in orbit above the Red Planet. Promethei Planum lies at approximately 76* south and 105* east. An approximately 100 km - large and 800 m - deep impact crater is visible in the bottom of the image. The crater's interior is par

PIX4616138

 
Atafu Atoll - Tokelau Islands, South Pacific - Atafu Atoll, Tokelau, Southern Pacific Ocean - Atafu is a small atoll belonging to the Tokelau Archipelago, in the South Pacific Ocean. With an elevation of two metres above the water, this coral reef is still vulnerable to cyclones and to the rise of water due to global warming. At roughly eight kilometers wide, Atafu Atoll is the smallest of three atolls and one island (Nukunonu and Fakaofo Atoll to the southeast and Swains Island to the south are not shown) comprising the Tokelau Islands group located in the southern Pacific Ocean. The primary settlement on Atafu is a village located at the northwestern corner of the atoll - - indicated by an area of light gray dots in this astronaut photograph. The typical ring shape of the atoll is the result of coral reefs building up around a former volcanic island. Over geologic time, the central volcano has subsided beneath the water surface, leaving the fringing reefs and a central lagoon that co

PIX4675640

Atafu Atoll - Tokelau Islands, South Pacific - Atafu Atoll, Tokelau, Southern Pacific Ocean - Atafu is a small atoll belonging to the Tokelau Archipelago, in the South Pacific Ocean. With an elevation of two metres above the water, this coral reef is still vulnerable to cyclones and to the rise of water due to global warming. At roughly eight kilometers wide, Atafu Atoll is the smallest of three atolls and one island (Nukunonu and Fakaofo Atoll to the southeast and Swains Island to the south are not shown) comprising the Tokelau Islands group located in the southern Pacific Ocean. The primary settlement on Atafu is a village located at the northwestern corner of the atoll - - indicated by an area of light gray dots in this astronaut photograph. The typical ring shape of the atoll is the result of coral reefs building up around a former volcanic island. Over geologic time, the central volcano has subsided beneath the water surface, leaving the fringing reefs and a central lagoon that co

PIX4675640

 
Geyser sur Enceladus - Artist's view - Water geyser on Enceladus - Artist's view of an ice geyser on the surface of the Enceladus satellite. In the sky, the planet Saturn and its satellite Mimas. Liquid water reaches the surface of Enceladus' south pole and drives a massive plume of ice crystals into the sky. The combination of Enceladus' low surface gravity and the geyser's force accelerate the crystals to escape velocity, where sunlight breaks the water molecules down into their constituent atoms of hydrogen and oxygen. Saturn itself appears low on the horizon due to the proximity to Enceladus' pole. The small object immediately to Saturn's left is another icy moon named Mimas. Somewhat smaller than Enceladus and closer to Saturn, Mimas sprints around Saturn in slightly less than one Earth day. In March 2006 Nasa's Cassini probe revealed evidence of water - driven geysers on the surface of Enceladus. At first glance Enceladus doesn't seem to be a likely host for liquid water as the s

Walter B Myers

PIX4625896

Geyser sur Enceladus - Artist's view - Water geyser on Enceladus - Artist's view of an ice geyser on the surface of the Enceladus satellite. In the sky, the planet Saturn and its satellite Mimas. Liquid water reaches the surface of Enceladus' south pole and drives a massive plume of ice crystals into the sky. The combination of Enceladus' low surface gravity and the geyser's force accelerate the crystals to escape velocity, where sunlight breaks the water molecules down into their constituent atoms of hydrogen and oxygen. Saturn itself appears low on the horizon due to the proximity to Enceladus' pole. The small object immediately to Saturn's left is another icy moon named Mimas. Somewhat smaller than Enceladus and closer to Saturn, Mimas sprints around Saturn in slightly less than one Earth day. In March 2006 Nasa's Cassini probe revealed evidence of water - driven geysers on the surface of Enceladus. At first glance Enceladus doesn't seem to be a likely host for liquid water as the s

Walter B Myers

PIX4625896

 
The Alps seen by satellite Envisat - The Alps as seen from satellite Envisat - Les Alpes seen by satellite ENVISAT on 8 December 2008. The snow - capped, crescent - shaped Alps and Italy's Apennines mountain chain are shown in this Envisat image. Snowfall in early winter - for meteorologists winter begins on the 1 December - covered the whole mountain areas with fresh snow, while the lower lands in the south and north of the mountains remained snow - free. Due to this snow cover and a relatively low illumination angle of the sun, the ranges and valleys of the mountains stand out in the image. Much of the whiteness seen in the top of the image is cloud cover, but fog is visible in the valleys such as the Rhine. The Alps - central Europe's major mountain range - extend some 1,200 km through France, Switzerland, Italy and Austria and down through Slovenia, Croatia, Bosnia and Herzegovina, Serbia and Montenegro and Albania as the Dinaric Alps. The Alps occupy an area of about 200,000 km an

PIX4665079

The Alps seen by satellite Envisat - The Alps as seen from satellite Envisat - Les Alpes seen by satellite ENVISAT on 8 December 2008. The snow - capped, crescent - shaped Alps and Italy's Apennines mountain chain are shown in this Envisat image. Snowfall in early winter - for meteorologists winter begins on the 1 December - covered the whole mountain areas with fresh snow, while the lower lands in the south and north of the mountains remained snow - free. Due to this snow cover and a relatively low illumination angle of the sun, the ranges and valleys of the mountains stand out in the image. Much of the whiteness seen in the top of the image is cloud cover, but fog is visible in the valleys such as the Rhine. The Alps - central Europe's major mountain range - extend some 1,200 km through France, Switzerland, Italy and Austria and down through Slovenia, Croatia, Bosnia and Herzegovina, Serbia and Montenegro and Albania as the Dinaric Alps. The Alps occupy an area of about 200,000 km an

PIX4665079

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