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The March Revolution of 1848 in Munich
The March Revolution of 1848 in Munich

SZT2989951: The March Revolution of 1848 in Munich / Bridgeman Images

Leni Riefenstahl during the filming of Triumph of the Will, 1934 (b/w photo)
Leni Riefenstahl during the filming of Triumph of the Will, 1934 (b/w photo)

SZT2994575: Leni Riefenstahl during the filming of Triumph of the Will, 1934 (b/w photo) / Bridgeman Images

Howard Carter and George Carnarvon, 1922 (b/w photo)
Howard Carter and George Carnarvon, 1922 (b/w photo)

SZT2994809: Howard Carter and George Carnarvon, 1922 (b/w photo) / Bridgeman Images

Franz Marc, c.1910 (b/w photo)
Franz Marc, c.1910 (b/w photo)

SZT2959989: Franz Marc, c.1910 (b/w photo) / Bridgeman Images

Prime Minister Nehru, Yugoslav President Tito, and Egyptian President Nasser in a conference. July 18, 1956. The non-aligned leaders met at a fishermen's hut on an islet near of President Tito's summer residence in Brioni
Prime Minister Nehru, Yugoslav President Tito, and Egyptian President Nasser in a conference. July 18, 1956. The non-aligned leaders met at a fishermen's hut on an islet near of President Tito's summer residence in Brioni

EVB2925589: Prime Minister Nehru, Yugoslav President Tito, and Egyptian President Nasser in a conference. July 18, 1956. The non-aligned leaders met at a fishermen's hut on an islet near of President Tito's summer residence in Brioni / Bridgeman Images

Swiss scientist Jacques Piccard and Navy Lieutenant Don Walsh aboard the bathyscaphe Trieste, San Diego, CA 01-23-1960.
Swiss scientist Jacques Piccard and Navy Lieutenant Don Walsh aboard the bathyscaphe Trieste, San Diego, CA 01-23-1960.

EVB2951517: Swiss scientist Jacques Piccard and Navy Lieutenant Don Walsh aboard the bathyscaphe Trieste, San Diego, CA 01-23-1960. / Bridgeman Images

Bonnie Parker and Clyde Barrow, 1933
Bonnie Parker and Clyde Barrow, 1933

EVB2949721: Bonnie Parker and Clyde Barrow, 1933 / Bridgeman Images

Notting Hill Carnival, 1982 (b/w photo)
Notting Hill Carnival, 1982 (b/w photo)

PLD3251801: Notting Hill Carnival, 1982 (b/w photo) / Bridgeman Images

Notting Hill Carnival, 1982 (b/w photo)
Notting Hill Carnival, 1982 (b/w photo)

PLD3251802: Notting Hill Carnival, 1982 (b/w photo) / Bridgeman Images

Julia Donaldson
Julia Donaldson

WAN3845174: Julia Donaldson / Bridgeman Images

St Petersburg MARIINSKY THEATRE
St Petersburg MARIINSKY THEATRE

LEL3854194: St Petersburg MARIINSKY THEATRE / Bridgeman Images

Dietrich Fischer-Dieskau, German baritone, singing in concert - accompanied by Gerald Moore on the piano, 1967
Dietrich Fischer-Dieskau, German baritone, singing in concert - accompanied by Gerald Moore on the piano, 1967

FLL3921716: Dietrich Fischer-Dieskau, German baritone, singing in concert - accompanied by Gerald Moore on the piano, 1967 / Bridgeman Images

Observation night - Amateur astronomer
Observation night - Amateur astronomer

PIX4565916: Observation night - Amateur astronomer / Bridgeman Images

Constellations of the Great Bear and Little Bear - Constellations of Ursa Major and Ursa Minor - On the right, the large trolley, asterism of the Great Bear; on the left, the small trolley, asterism of the Little Bear that houses the polar star, the star that currently indicates the position of the northern Celestial pole, at the end of the handle of the pan
Constellations of the Great Bear and Little Bear - Constellations of Ursa Major and Ursa Minor - On the right, the large trolley, asterism of the Great Bear; on the left, the small trolley, asterism of the Little Bear that houses the polar star, the star that currently indicates the position of the northern Celestial pole, at the end of the handle of the pan

PIX4591367: Constellations of the Great Bear and Little Bear - Constellations of Ursa Major and Ursa Minor - On the right, the large trolley, asterism of the Great Bear; on the left, the small trolley, asterism of the Little Bear that houses the polar star, the star that currently indicates the position of the northern Celestial pole, at the end of the handle of the pan / Bridgeman Images

Very Large Array Radio Observatory - New Mexico - USA - Very Large Array - Radio observatory in New Mexico - Radio Observatory consists of 27 antennas of 25m diameter. Very Large Array - Radio observatory in New Mexico The Very Large Array, one of the world's premier astronomical radio observatories, consists of 27 radio antennas in a Y - shaped configuration. Each antenna is 25 meters (82 feet) in diameter
Very Large Array Radio Observatory - New Mexico - USA - Very Large Array - Radio observatory in New Mexico - Radio Observatory consists of 27 antennas of 25m diameter. Very Large Array - Radio observatory in New Mexico The Very Large Array, one of the world's premier astronomical radio observatories, consists of 27 radio antennas in a Y - shaped configuration. Each antenna is 25 meters (82 feet) in diameter

PIX4656578: Very Large Array Radio Observatory - New Mexico - USA - Very Large Array - Radio observatory in New Mexico - Radio Observatory consists of 27 antennas of 25m diameter. Very Large Array - Radio observatory in New Mexico The Very Large Array, one of the world's premier astronomical radio observatories, consists of 27 radio antennas in a Y - shaped configuration. Each antenna is 25 meters (82 feet) in diameter / Bridgeman Images

Ardipithecus ramidus - Reconstitution of Ardipithecus ramidus, a species faint from the order of Primates and probably from the family Hominides. He lived about 4.4 million years ago at the lower Pliocene. Portrait of a Ardipithecus ramidus. This restoration, based on the newly described Ethiopian specimen nicknamed “” Ardi””, illustrates a basal hominid that resides near the common ancestor of apes and humans. It lived about 4.4 million years ago during the early Pliocene
Ardipithecus ramidus - Reconstitution of Ardipithecus ramidus, a species faint from the order of Primates and probably from the family Hominides. He lived about 4.4 million years ago at the lower Pliocene. Portrait of a Ardipithecus ramidus. This restoration, based on the newly described Ethiopian specimen nicknamed “” Ardi””, illustrates a basal hominid that resides near the common ancestor of apes and humans. It lived about 4.4 million years ago during the early Pliocene

PIX4675717: Ardipithecus ramidus - Reconstitution of Ardipithecus ramidus, a species faint from the order of Primates and probably from the family Hominides. He lived about 4.4 million years ago at the lower Pliocene. Portrait of a Ardipithecus ramidus. This restoration, based on the newly described Ethiopian specimen nicknamed “” Ardi””, illustrates a basal hominid that resides near the common ancestor of apes and humans. It lived about 4.4 million years ago during the early Pliocene / Bridgeman Images

Centre of the Milky Way Central Region - Center of the Milky Way: Central part of the lactee route seen in New Zealand. Planet Saturn is the bright white dot towards the center of the image (near the nebula of the pipe). The central part of our Milky Way photographed from New Zealand. Lots of emission and obscure nebulae are visible in the image. Planet Saturn in the bright white “” star”” close to the center of the image.
Centre of the Milky Way Central Region - Center of the Milky Way: Central part of the lactee route seen in New Zealand. Planet Saturn is the bright white dot towards the center of the image (near the nebula of the pipe). The central part of our Milky Way photographed from New Zealand. Lots of emission and obscure nebulae are visible in the image. Planet Saturn in the bright white “” star”” close to the center of the image.

PIX4636579: Centre of the Milky Way Central Region - Center of the Milky Way: Central part of the lactee route seen in New Zealand. Planet Saturn is the bright white dot towards the center of the image (near the nebula of the pipe). The central part of our Milky Way photographed from New Zealand. Lots of emission and obscure nebulae are visible in the image. Planet Saturn in the bright white “” star”” close to the center of the image. / Bridgeman Images

The Kuiper Belt - Illustration - The Kuiper Belt is an area beyond the orbit of Neptune with small ice bodies. The orbits of planets Jupiter, Saturn, Uranus, Neptune and Pluto are represented
The Kuiper Belt - Illustration - The Kuiper Belt is an area beyond the orbit of Neptune with small ice bodies. The orbits of planets Jupiter, Saturn, Uranus, Neptune and Pluto are represented

PIX4630360: The Kuiper Belt - Illustration - The Kuiper Belt is an area beyond the orbit of Neptune with small ice bodies. The orbits of planets Jupiter, Saturn, Uranus, Neptune and Pluto are represented / Bridgeman Images

European launchers - Illustration - European launch vehicles family in 2009 - Illustration - Artist's view of the various fusees used by the European Space Agency and launches from the Guyanese Space Centre. From left to right, the Vega launcher, Soyuz - ST, Ariane 5 ES ATV and Ariane 5 ECA. Artist view of the family of launchers to be operated on behalf of ESA from the Guiana Space Center, Europe's Spaceport, in Kourou, English Guiana. From left to right: Vega, ESA's new small launcher, is designed to loft single or multiple payloads to orbits up to 1,500 km in altitude. Its reference payload capability is about 1,500 kg to a circular 500 - km - high Sun - synchronous orbit but it can also loft satellites from 300 kg to more than 2 metric tons, as well as piggyback microsatellites of less than 100 kg each. Soyuz - ST, the improved version of Russia's Soyuz workhorse launcher with a new digital avionics and a wider, Ariane 4 - type payload fairing. A new launch pad is being built in the CSG for Soyuz vehicles. Ariane 5 ES, another version of the Ariane 5E featuring a restartable version of Ariane 5G's storable propellant upper stage. One of its primary payloads is the Autonomous Transfer Vehicle (ATV) for resupply and reboost missions to the International Space Station. Ariane 5 ECA, the most powerful version of the Ariane 5E, an evolution of the generic Ariane 5 launcher with an increased propellant load in its solid booster stages and an improved capacity for the liquid oxygen tank of its cryogenic core stage to feed its new Vulcain 2 main engine. The Ariane 5 ECA was first launched on December 11, 2002. Its payload capacity to geostationary transfer orbit reaches 10 metric tons
European launchers - Illustration - European launch vehicles family in 2009 - Illustration - Artist's view of the various fusees used by the European Space Agency and launches from the Guyanese Space Centre. From left to right, the Vega launcher, Soyuz - ST, Ariane 5 ES ATV and Ariane 5 ECA. Artist view of the family of launchers to be operated on behalf of ESA from the Guiana Space Center, Europe's Spaceport, in Kourou, English Guiana. From left to right: Vega, ESA's new small launcher, is designed to loft single or multiple payloads to orbits up to 1,500 km in altitude. Its reference payload capability is about 1,500 kg to a circular 500 - km - high Sun - synchronous orbit but it can also loft satellites from 300 kg to more than 2 metric tons, as well as piggyback microsatellites of less than 100 kg each. Soyuz - ST, the improved version of Russia's Soyuz workhorse launcher with a new digital avionics and a wider, Ariane 4 - type payload fairing. A new launch pad is being built in the CSG for Soyuz vehicles. Ariane 5 ES, another version of the Ariane 5E featuring a restartable version of Ariane 5G's storable propellant upper stage. One of its primary payloads is the Autonomous Transfer Vehicle (ATV) for resupply and reboost missions to the International Space Station. Ariane 5 ECA, the most powerful version of the Ariane 5E, an evolution of the generic Ariane 5 launcher with an increased propellant load in its solid booster stages and an improved capacity for the liquid oxygen tank of its cryogenic core stage to feed its new Vulcain 2 main engine. The Ariane 5 ECA was first launched on December 11, 2002. Its payload capacity to geostationary transfer orbit reaches 10 metric tons

PIX4604567: European launchers - Illustration - European launch vehicles family in 2009 - Illustration - Artist's view of the various fusees used by the European Space Agency and launches from the Guyanese Space Centre. From left to right, the Vega launcher, Soyuz - ST, Ariane 5 ES ATV and Ariane 5 ECA. Artist view of the family of launchers to be operated on behalf of ESA from the Guiana Space Center, Europe's Spaceport, in Kourou, English Guiana. From left to right: Vega, ESA's new small launcher, is designed to loft single or multiple payloads to orbits up to 1,500 km in altitude. Its reference payload capability is about 1,500 kg to a circular 500 - km - high Sun - synchronous orbit but it can also loft satellites from 300 kg to more than 2 metric tons, as well as piggyback microsatellites of less than 100 kg each. Soyuz - ST, the improved version of Russia's Soyuz workhorse launcher with a new digital avionics and a wider, Ariane 4 - type payload fairing. A new launch pad is being built in the CSG for Soyuz vehicles. Ariane 5 ES, another version of the Ariane 5E featuring a restartable version of Ariane 5G's storable propellant upper stage. One of its primary payloads is the Autonomous Transfer Vehicle (ATV) for resupply and reboost missions to the International Space Station. Ariane 5 ECA, the most powerful version of the Ariane 5E, an evolution of the generic Ariane 5 launcher with an increased propellant load in its solid booster stages and an improved capacity for the liquid oxygen tank of its cryogenic core stage to feed its new Vulcain 2 main engine. The Ariane 5 ECA was first launched on December 11, 2002. Its payload capacity to geostationary transfer orbit reaches 10 metric tons / Bridgeman Images

E.DEORBIT: a satellite to clean up space - E.Deorbit grabbing debris - Artist view of the satellite e.deorbit (right) catching a satellite with a net to take it to consume in the Earth's atmosphere. e.Deorbit is a European mission project that if approved in 2019 will start in 2024. This satellite will be the first to clean up space debris. He would recapture the larger objects with his articulated arm or a net, before discharging them into the atmosphere, or they would be destroyed. ESA's proposed e.Deorbit mission, shown right, using a net to catch a derelict satellite - the baseline capture method for what would be the world's first active space debris removal mission, in 2024. The mission would first rendezvous with a large, drifting ESA satellite, then capture and secure it safely ahead of steering the combination down for a controlled burn-up in the atmosphere. As well as the baselined robot arm, additional capture technologies are being investigated, including a net and harpon. In any case, grappling the derelict satellite would have to be done in a very rapid and precise manner to prevent E.Deorbit and its target rebounding apart. The mission, being developed through ESA's Clean Space initiative - tasked with safeguarding terrestrial and orbital environments - will be proposed for final agreement at ESA's next Council at Ministerial Level, in 2019. It will place European industry at the forefront of the world's active debris removal efforts and multipurpose space tugs
E.DEORBIT: a satellite to clean up space - E.Deorbit grabbing debris - Artist view of the satellite e.deorbit (right) catching a satellite with a net to take it to consume in the Earth's atmosphere. e.Deorbit is a European mission project that if approved in 2019 will start in 2024. This satellite will be the first to clean up space debris. He would recapture the larger objects with his articulated arm or a net, before discharging them into the atmosphere, or they would be destroyed. ESA's proposed e.Deorbit mission, shown right, using a net to catch a derelict satellite - the baseline capture method for what would be the world's first active space debris removal mission, in 2024. The mission would first rendezvous with a large, drifting ESA satellite, then capture and secure it safely ahead of steering the combination down for a controlled burn-up in the atmosphere. As well as the baselined robot arm, additional capture technologies are being investigated, including a net and harpon. In any case, grappling the derelict satellite would have to be done in a very rapid and precise manner to prevent E.Deorbit and its target rebounding apart. The mission, being developed through ESA's Clean Space initiative - tasked with safeguarding terrestrial and orbital environments - will be proposed for final agreement at ESA's next Council at Ministerial Level, in 2019. It will place European industry at the forefront of the world's active debris removal efforts and multipurpose space tugs

PIX4605506: E.DEORBIT: a satellite to clean up space - E.Deorbit grabbing debris - Artist view of the satellite e.deorbit (right) catching a satellite with a net to take it to consume in the Earth's atmosphere. e.Deorbit is a European mission project that if approved in 2019 will start in 2024. This satellite will be the first to clean up space debris. He would recapture the larger objects with his articulated arm or a net, before discharging them into the atmosphere, or they would be destroyed. ESA's proposed e.Deorbit mission, shown right, using a net to catch a derelict satellite - the baseline capture method for what would be the world's first active space debris removal mission, in 2024. The mission would first rendezvous with a large, drifting ESA satellite, then capture and secure it safely ahead of steering the combination down for a controlled burn-up in the atmosphere. As well as the baselined robot arm, additional capture technologies are being investigated, including a net and harpon. In any case, grappling the derelict satellite would have to be done in a very rapid and precise manner to prevent E.Deorbit and its target rebounding apart. The mission, being developed through ESA's Clean Space initiative - tasked with safeguarding terrestrial and orbital environments - will be proposed for final agreement at ESA's next Council at Ministerial Level, in 2019. It will place European industry at the forefront of the world's active debris removal efforts and multipurpose space tugs / Bridgeman Images

An asteroid hits the Earth - An asteroid hits the Earth - An asteroid enters the Earth's atmosphere. An asteroid enters the earth's atmosphere
An asteroid hits the Earth - An asteroid hits the Earth - An asteroid enters the Earth's atmosphere. An asteroid enters the earth's atmosphere

PIX4583761: An asteroid hits the Earth - An asteroid hits the Earth - An asteroid enters the Earth's atmosphere. An asteroid enters the earth's atmosphere / Bridgeman Images

Arecibo Message - Arecibo Message: Arecibo Message is a radio message that was sent to space on November 16, 1974 towards the globular cluster M13, 25 000 light-years from Earth - When this binary message is divided into 73 groups of 23 characters it forms this drawing that includes the numbers from one to ten, the atomic numbers of the hydrogen, carbon, nitrogen, oxygen and phosphorus, DNA structure, a 1.76m man, Earth's population, our solar system, and a representation of the Arecibo radiotelescope - Arecibo message is a radio message that was sent into space, at the globular star cluster M13 on november 16 1974. This binary message describes numbers, atomic numbers, DNA, man dimension, our solar system and the Arecibo radiotelescope
Arecibo Message - Arecibo Message: Arecibo Message is a radio message that was sent to space on November 16, 1974 towards the globular cluster M13, 25 000 light-years from Earth - When this binary message is divided into 73 groups of 23 characters it forms this drawing that includes the numbers from one to ten, the atomic numbers of the hydrogen, carbon, nitrogen, oxygen and phosphorus, DNA structure, a 1.76m man, Earth's population, our solar system, and a representation of the Arecibo radiotelescope - Arecibo message is a radio message that was sent into space, at the globular star cluster M13 on november 16 1974. This binary message describes numbers, atomic numbers, DNA, man dimension, our solar system and the Arecibo radiotelescope

PIX4651737: Arecibo Message - Arecibo Message: Arecibo Message is a radio message that was sent to space on November 16, 1974 towards the globular cluster M13, 25 000 light-years from Earth - When this binary message is divided into 73 groups of 23 characters it forms this drawing that includes the numbers from one to ten, the atomic numbers of the hydrogen, carbon, nitrogen, oxygen and phosphorus, DNA structure, a 1.76m man, Earth's population, our solar system, and a representation of the Arecibo radiotelescope - Arecibo message is a radio message that was sent into space, at the globular star cluster M13 on november 16 1974. This binary message describes numbers, atomic numbers, DNA, man dimension, our solar system and the Arecibo radiotelescope / Bridgeman Images

Bologna-Florence Motorway, Rio Della Piazza Viaduct, 1964 (b/w photo)
Bologna-Florence Motorway, Rio Della Piazza Viaduct, 1964 (b/w photo)

UIT6191820: Bologna-Florence Motorway, Rio Della Piazza Viaduct, 1964 (b/w photo) / Bridgeman Images

Shooting star rain on LAMOST telescope - China - Geminids over LAMOST telescope - China: Geminides shooting star rain above LAMOST telescope (Large Sky Area Multi-Object Fibre Spectroscopic Telescope), a 4-metre optical telescope, located on the site of the Xinglong Observatory in the Hebei region of China. December 2015. Space dust from asteroid 3200 Phaethon rained into the Earth's atmosphere, and burnt as meteors at about 100 km above Xinglong Station of National Astronomical Observatories of China, piercing the night sky over the Guoshoujing LAMOST telescope. All meteors seemed to radiate from the same point, which lies at Gemini, and that's how the meteor shower named Geminids.Over 100 meteors were captured in the composed image taken on the peak night of the 2015 Geminid meteor shower, and the brightest bolide even instantly lit up the landscape.
Shooting star rain on LAMOST telescope - China - Geminids over LAMOST telescope - China: Geminides shooting star rain above LAMOST telescope (Large Sky Area Multi-Object Fibre Spectroscopic Telescope), a 4-metre optical telescope, located on the site of the Xinglong Observatory in the Hebei region of China. December 2015. Space dust from asteroid 3200 Phaethon rained into the Earth's atmosphere, and burnt as meteors at about 100 km above Xinglong Station of National Astronomical Observatories of China, piercing the night sky over the Guoshoujing LAMOST telescope. All meteors seemed to radiate from the same point, which lies at Gemini, and that's how the meteor shower named Geminids.Over 100 meteors were captured in the composed image taken on the peak night of the 2015 Geminid meteor shower, and the brightest bolide even instantly lit up the landscape.

PIX4657602: Shooting star rain on LAMOST telescope - China - Geminids over LAMOST telescope - China: Geminides shooting star rain above LAMOST telescope (Large Sky Area Multi-Object Fibre Spectroscopic Telescope), a 4-metre optical telescope, located on the site of the Xinglong Observatory in the Hebei region of China. December 2015. Space dust from asteroid 3200 Phaethon rained into the Earth's atmosphere, and burnt as meteors at about 100 km above Xinglong Station of National Astronomical Observatories of China, piercing the night sky over the Guoshoujing LAMOST telescope. All meteors seemed to radiate from the same point, which lies at Gemini, and that's how the meteor shower named Geminids.Over 100 meteors were captured in the composed image taken on the peak night of the 2015 Geminid meteor shower, and the brightest bolide even instantly lit up the landscape. / Bridgeman Images

Portrait of Leo Ferre (1916-1993) in 1962 on Duguesclin Island - September 1962
Portrait of Leo Ferre (1916-1993) in 1962 on Duguesclin Island - September 1962

JPS4959082: Portrait of Leo Ferre (1916-1993) in 1962 on Duguesclin Island - September 1962 / Bridgeman Images

The printing and delivery of the Berliner Tageblatt, 1920s
The printing and delivery of the Berliner Tageblatt, 1920s

CMD6288288: The printing and delivery of the Berliner Tageblatt, 1920s / Bridgeman Images

Grey-headed flying fox: Grey-headed flying fox (Pteropus poliocephalus) in flight photography in Australia, south of Cairns, Queensland. Grey-headed flying fox (Pteropus poliocephalus) seen in Australia.
Grey-headed flying fox: Grey-headed flying fox (Pteropus poliocephalus) in flight photography in Australia, south of Cairns, Queensland. Grey-headed flying fox (Pteropus poliocephalus) seen in Australia.

PIX4677857: Grey-headed flying fox: Grey-headed flying fox (Pteropus poliocephalus) in flight photography in Australia, south of Cairns, Queensland. Grey-headed flying fox (Pteropus poliocephalus) seen in Australia. / Bridgeman Images

Lava flow on volcano Pacaya - Guatemala - Lava flow on volcano Pacaya - Guatemala - Lava flow on volcano Pacaya in Guatemala. In the background the volcanoes Agua and Fuego (in the background). Lava flow on volcano Pacaya in Guatemala. In background are volcanoes Agua and Fuego
Lava flow on volcano Pacaya - Guatemala - Lava flow on volcano Pacaya - Guatemala - Lava flow on volcano Pacaya in Guatemala. In the background the volcanoes Agua and Fuego (in the background). Lava flow on volcano Pacaya in Guatemala. In background are volcanoes Agua and Fuego

PIX4677346: Lava flow on volcano Pacaya - Guatemala - Lava flow on volcano Pacaya - Guatemala - Lava flow on volcano Pacaya in Guatemala. In the background the volcanoes Agua and Fuego (in the background). Lava flow on volcano Pacaya in Guatemala. In background are volcanoes Agua and Fuego / Bridgeman Images

The lava dome Santiaguito active -Guatemala - Santiaguito lava dome - Guatemala - The eruption of the Santiaguito, the active lava dome (or volcanic dome) of the Santa Maria volcano in Guatemala. January 2009. Volcanic eruption at lava dome (or volcanic dome) of Santiaguito, an active part of volcano Santa Maria in Guatemala. January 2009
The lava dome Santiaguito active -Guatemala - Santiaguito lava dome - Guatemala - The eruption of the Santiaguito, the active lava dome (or volcanic dome) of the Santa Maria volcano in Guatemala. January 2009. Volcanic eruption at lava dome (or volcanic dome) of Santiaguito, an active part of volcano Santa Maria in Guatemala. January 2009

PIX4677391: The lava dome Santiaguito active -Guatemala - Santiaguito lava dome - Guatemala - The eruption of the Santiaguito, the active lava dome (or volcanic dome) of the Santa Maria volcano in Guatemala. January 2009. Volcanic eruption at lava dome (or volcanic dome) of Santiaguito, an active part of volcano Santa Maria in Guatemala. January 2009 / Bridgeman Images

The lava dome Santiaguito active -Guatemala - Santiaguito lava dome - Guatemala - The eruption of the Santiaguito, the active lava dome (or volcanic dome) of the Santa Maria volcano in Guatemala. January 2009. Volcanic eruption at lava dome (or volcanic dome) of Santiaguito, an active part of volcano Santa Maria in Guatemala. January 2009
The lava dome Santiaguito active -Guatemala - Santiaguito lava dome - Guatemala - The eruption of the Santiaguito, the active lava dome (or volcanic dome) of the Santa Maria volcano in Guatemala. January 2009. Volcanic eruption at lava dome (or volcanic dome) of Santiaguito, an active part of volcano Santa Maria in Guatemala. January 2009

PIX4677443: The lava dome Santiaguito active -Guatemala - Santiaguito lava dome - Guatemala - The eruption of the Santiaguito, the active lava dome (or volcanic dome) of the Santa Maria volcano in Guatemala. January 2009. Volcanic eruption at lava dome (or volcanic dome) of Santiaguito, an active part of volcano Santa Maria in Guatemala. January 2009 / Bridgeman Images

The lava dome of the Soufriere-Ile de Montserrat - Soufriere hills lava dome - Montserrat - The lava dome (or volcanic dome) of the volcano of the Soufriere in activity seen from the valley of the river Tar. Montserrat Island. Active Soufriere Hills lava dome (or volcanic dome) seen from Tar river valley. Montserrat
The lava dome of the Soufriere-Ile de Montserrat - Soufriere hills lava dome - Montserrat - The lava dome (or volcanic dome) of the volcano of the Soufriere in activity seen from the valley of the river Tar. Montserrat Island. Active Soufriere Hills lava dome (or volcanic dome) seen from Tar river valley. Montserrat

PIX4677444: The lava dome of the Soufriere-Ile de Montserrat - Soufriere hills lava dome - Montserrat - The lava dome (or volcanic dome) of the volcano of the Soufriere in activity seen from the valley of the river Tar. Montserrat Island. Active Soufriere Hills lava dome (or volcanic dome) seen from Tar river valley. Montserrat / Bridgeman Images

Francis Scott Fitzgerald smoking, 1920 (b/w photo)
Francis Scott Fitzgerald smoking, 1920 (b/w photo)

MEP3510968: Francis Scott Fitzgerald smoking, 1920 (b/w photo) / Bridgeman Images

Member of the Hungarian secret police surrounded by the crowd, Hungary, 1956 (b/w photo)
Member of the Hungarian secret police surrounded by the crowd, Hungary, 1956 (b/w photo)

MEP3063016: Member of the Hungarian secret police surrounded by the crowd, Hungary, 1956 (b/w photo) / Bridgeman Images

Revolutionaries at the border between Austria and Hungary, Unspecified, 1950 (b/w photo)
Revolutionaries at the border between Austria and Hungary, Unspecified, 1950 (b/w photo)

MEP3269992: Revolutionaries at the border between Austria and Hungary, Unspecified, 1950 (b/w photo) / Bridgeman Images

A tank in Budapest streets, Ungheria, 1950 (b/w photo)
A tank in Budapest streets, Ungheria, 1950 (b/w photo)

MEP3270005: A tank in Budapest streets, Ungheria, 1950 (b/w photo) / Bridgeman Images

Young Hungarian revolutionaries, Ungheria, 1950 (b/w photo)
Young Hungarian revolutionaries, Ungheria, 1950 (b/w photo)

MEP3270020: Young Hungarian revolutionaries, Ungheria, 1950 (b/w photo) / Bridgeman Images


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