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Virgis Puodziunas as 'Aeneas'
Virgis Puodziunas as 'Aeneas'

LEL3892097: Virgis Puodziunas as 'Aeneas' / Bridgeman Images

Bass Trombone - with
Bass Trombone - with

SKC3892333: Bass Trombone - with / Bridgeman Images

Ingo Maurer - portrait
Ingo Maurer - portrait

BAU3885710: Ingo Maurer - portrait / Bridgeman Images

Sonia Rykiel - portrait
Sonia Rykiel - portrait

BAU3885733: Sonia Rykiel - portrait / Bridgeman Images

Cowbell - percussion instrument
Cowbell - percussion instrument

SKC3889205: Cowbell - percussion instrument / Bridgeman Images

Benedict Mason
Benedict Mason

LEL3869327: Benedict Mason / Bridgeman Images

Literature - a pile
Literature - a pile

SKC3890088: Literature - a pile / Bridgeman Images

WIND MACHINE being played
WIND MACHINE being played

SKC3862656: WIND MACHINE being played / Bridgeman Images

Rihm Wolfgang (photo)
Rihm Wolfgang (photo)

BYF3879904: Rihm Wolfgang (photo) / Bridgeman Images

Circumpolar - Star trails around north celestial pole - Photographic pose around the polar star. Long exposure image; because the earth rotates on it's own axis, during the exposure the stars seem to revolve around a point in the sky very near to Polaris
Circumpolar - Star trails around north celestial pole - Photographic pose around the polar star. Long exposure image; because the earth rotates on it's own axis, during the exposure the stars seem to revolve around a point in the sky very near to Polaris

PIX4580204: Circumpolar - Star trails around north celestial pole - Photographic pose around the polar star. Long exposure image; because the earth rotates on it's own axis, during the exposure the stars seem to revolve around a point in the sky very near to Polaris / Bridgeman Images

Remnants of the supernova Cassiopee A in X-rays - visible and infrared - This stunning picture of the supernova remnant Cassiopeia A (Cas A) is a composite of images taken by three of Nasa's Great Observatories. Infrared data from the Spitzer Space Telescope are colored red; optical data from the Hubble Space Telescope are yellow; and X - ray data from the Chandra X - ray Observatory are green and blue. Cas A is the 300 - year - old remnant created by the supernova explosion of a massive star. Each Great Observatory image highlights different characteristics of the remnant. Spitzer reveals warm dust in the outer shell with temperatures of about 10 degrees Celsius (80 degrees Fahrenheit), and Hubble sees the delicate filamentary structures of warmer gases about 10,000 degrees Celsius. Chandra shows hot gases at about 10 million degrees Celsius. This hot gas was created when ejected material from the supernova smashed into surrounding gas and dust at speeds of about ten million miles per hour. A comparison of the infrared and X - ray images of Cas A should enable astronomers to better understand how relatively cool dust grains can coexist in the superhot gas that produces the X - rays. It should also help to determine whether most of the dust in the supernova remnant came from the massive star before it exploded, or from the rapidly expanding supernova ejecta. The turquoise dot at the center of the shell may be a neutron star created during the supernova. Blue Chandra data were acquired using broadband X - rays (low through high energies); green Chandra data correspond only to intermediate energy X - rays; yellow Hubble data were taken using a 900 nanometer - wavelength filter, and red Spitzer data are from the telescope's 24 - micron detector. Observation Dates 9 pointings between Feb 8 - May 5, 2004 Observation Time 11 days, 14 hours Distance Estimate About 10,000 light year
Remnants of the supernova Cassiopee A in X-rays - visible and infrared - This stunning picture of the supernova remnant Cassiopeia A (Cas A) is a composite of images taken by three of Nasa's Great Observatories. Infrared data from the Spitzer Space Telescope are colored red; optical data from the Hubble Space Telescope are yellow; and X - ray data from the Chandra X - ray Observatory are green and blue. Cas A is the 300 - year - old remnant created by the supernova explosion of a massive star. Each Great Observatory image highlights different characteristics of the remnant. Spitzer reveals warm dust in the outer shell with temperatures of about 10 degrees Celsius (80 degrees Fahrenheit), and Hubble sees the delicate filamentary structures of warmer gases about 10,000 degrees Celsius. Chandra shows hot gases at about 10 million degrees Celsius. This hot gas was created when ejected material from the supernova smashed into surrounding gas and dust at speeds of about ten million miles per hour. A comparison of the infrared and X - ray images of Cas A should enable astronomers to better understand how relatively cool dust grains can coexist in the superhot gas that produces the X - rays. It should also help to determine whether most of the dust in the supernova remnant came from the massive star before it exploded, or from the rapidly expanding supernova ejecta. The turquoise dot at the center of the shell may be a neutron star created during the supernova. Blue Chandra data were acquired using broadband X - rays (low through high energies); green Chandra data correspond only to intermediate energy X - rays; yellow Hubble data were taken using a 900 nanometer - wavelength filter, and red Spitzer data are from the telescope's 24 - micron detector. Observation Dates 9 pointings between Feb 8 - May 5, 2004 Observation Time 11 days, 14 hours Distance Estimate About 10,000 light year

PIX4582940: Remnants of the supernova Cassiopee A in X-rays - visible and infrared - This stunning picture of the supernova remnant Cassiopeia A (Cas A) is a composite of images taken by three of Nasa's Great Observatories. Infrared data from the Spitzer Space Telescope are colored red; optical data from the Hubble Space Telescope are yellow; and X - ray data from the Chandra X - ray Observatory are green and blue. Cas A is the 300 - year - old remnant created by the supernova explosion of a massive star. Each Great Observatory image highlights different characteristics of the remnant. Spitzer reveals warm dust in the outer shell with temperatures of about 10 degrees Celsius (80 degrees Fahrenheit), and Hubble sees the delicate filamentary structures of warmer gases about 10,000 degrees Celsius. Chandra shows hot gases at about 10 million degrees Celsius. This hot gas was created when ejected material from the supernova smashed into surrounding gas and dust at speeds of about ten million miles per hour. A comparison of the infrared and X - ray images of Cas A should enable astronomers to better understand how relatively cool dust grains can coexist in the superhot gas that produces the X - rays. It should also help to determine whether most of the dust in the supernova remnant came from the massive star before it exploded, or from the rapidly expanding supernova ejecta. The turquoise dot at the center of the shell may be a neutron star created during the supernova. Blue Chandra data were acquired using broadband X - rays (low through high energies); green Chandra data correspond only to intermediate energy X - rays; yellow Hubble data were taken using a 900 nanometer - wavelength filter, and red Spitzer data are from the telescope's 24 - micron detector. Observation Dates 9 pointings between Feb 8 - May 5, 2004 Observation Time 11 days, 14 hours Distance Estimate About 10,000 light year / Bridgeman Images

Impact of asteroides on Earth - Asteroids impacting the Earth- Artwork - Artist's view
Impact of asteroides on Earth - Asteroids impacting the Earth- Artwork - Artist's view

PIX4583678: Impact of asteroides on Earth - Asteroids impacting the Earth- Artwork - Artist's view / Bridgeman Images

Artist view of Cygnus X-1 - Cygnus X-1 is a binary star X and was the first black hole candidate. This system consists of the 226868 HD star, a supergeant star, orbiting around a black hole. A stellar black hole is born from the gravitational collapse of a massive star. The stellar black holes have a mass of some solar masses. A black hole is a region of space whose gravitation is so strong that it will prevent any form of material or radiation from escaping. Cygnus X-1 is an X-ray binary system and the first black hole candidates to be discovered
Artist view of Cygnus X-1 - Cygnus X-1 is a binary star X and was the first black hole candidate. This system consists of the 226868 HD star, a supergeant star, orbiting around a black hole. A stellar black hole is born from the gravitational collapse of a massive star. The stellar black holes have a mass of some solar masses. A black hole is a region of space whose gravitation is so strong that it will prevent any form of material or radiation from escaping. Cygnus X-1 is an X-ray binary system and the first black hole candidates to be discovered

PIX4584791: Artist view of Cygnus X-1 - Cygnus X-1 is a binary star X and was the first black hole candidate. This system consists of the 226868 HD star, a supergeant star, orbiting around a black hole. A stellar black hole is born from the gravitational collapse of a massive star. The stellar black holes have a mass of some solar masses. A black hole is a region of space whose gravitation is so strong that it will prevent any form of material or radiation from escaping. Cygnus X-1 is an X-ray binary system and the first black hole candidates to be discovered / Bridgeman Images

Constellation of the Southern Cross - The Southern Cross - The Southern Cross and the Alpha and Beta stars of Centaurus. Crux, the Southern Cross, is the smallest constellation in the sky yet one of the most distinctive, at least to those of us who live in the southern hemisphere. It was once part of Centaurus, where the bright stars Acrux and Mimosa could easly be imagined as the rear hooves of the rearing mythical centaur. However, when Christian sailors began to explore southwards in the 16th century, this memorable asterism took on a new significance. The cross appears on the national flags of several southern hemisphere countries, including Australia, though it can be seen on the southern horizon from the tropic of Cancer, 23.5 degrees north of the equator. Along with the Southern Cross is a very distinctive dark shape known as the Coalsack, much used by southern hemisphere astronomers as an indicator of a dark sky, especially if the sixth magnitude star embedded in it is visible. The long axis of the southern cross points towards the south celestial pole, so the cross itself acts as a very convenient circumpolar clock, compasset and calendar
Constellation of the Southern Cross - The Southern Cross - The Southern Cross and the Alpha and Beta stars of Centaurus. Crux, the Southern Cross, is the smallest constellation in the sky yet one of the most distinctive, at least to those of us who live in the southern hemisphere. It was once part of Centaurus, where the bright stars Acrux and Mimosa could easly be imagined as the rear hooves of the rearing mythical centaur. However, when Christian sailors began to explore southwards in the 16th century, this memorable asterism took on a new significance. The cross appears on the national flags of several southern hemisphere countries, including Australia, though it can be seen on the southern horizon from the tropic of Cancer, 23.5 degrees north of the equator. Along with the Southern Cross is a very distinctive dark shape known as the Coalsack, much used by southern hemisphere astronomers as an indicator of a dark sky, especially if the sixth magnitude star embedded in it is visible. The long axis of the southern cross points towards the south celestial pole, so the cross itself acts as a very convenient circumpolar clock, compasset and calendar

PIX4590268: Constellation of the Southern Cross - The Southern Cross - The Southern Cross and the Alpha and Beta stars of Centaurus. Crux, the Southern Cross, is the smallest constellation in the sky yet one of the most distinctive, at least to those of us who live in the southern hemisphere. It was once part of Centaurus, where the bright stars Acrux and Mimosa could easly be imagined as the rear hooves of the rearing mythical centaur. However, when Christian sailors began to explore southwards in the 16th century, this memorable asterism took on a new significance. The cross appears on the national flags of several southern hemisphere countries, including Australia, though it can be seen on the southern horizon from the tropic of Cancer, 23.5 degrees north of the equator. Along with the Southern Cross is a very distinctive dark shape known as the Coalsack, much used by southern hemisphere astronomers as an indicator of a dark sky, especially if the sixth magnitude star embedded in it is visible. The long axis of the southern cross points towards the south celestial pole, so the cross itself acts as a very convenient circumpolar clock, compasset and calendar / Bridgeman Images

Constellation of Ophiuchus - Constellation of Ophiuchus - Constellation of Ophiuchus extracted from the Uranographia of Hevelius. Recolorised image. Map showing the constellation of Ophiuchus with its mythological form from “” Uranographia”” star atlas by Hevelius (1690). Recolored Image
Constellation of Ophiuchus - Constellation of Ophiuchus - Constellation of Ophiuchus extracted from the Uranographia of Hevelius. Recolorised image. Map showing the constellation of Ophiuchus with its mythological form from “” Uranographia”” star atlas by Hevelius (1690). Recolored Image

PIX4592385: Constellation of Ophiuchus - Constellation of Ophiuchus - Constellation of Ophiuchus extracted from the Uranographia of Hevelius. Recolorised image. Map showing the constellation of Ophiuchus with its mythological form from “” Uranographia”” star atlas by Hevelius (1690). Recolored Image / Bridgeman Images

Winter Sky - Winter Sky - Star sky above the Alps. In the sky, the constellations of the Taurus (right), Orion (center), and the bright star Sirius (lower left). A shooting star crosses the constellation of Taurus. January 3, 2011. Starry sky above english Alps. In the sky, constellations of Taurus (at right), Orion (centre), and bright star Sirius (bottom left). A shooting star is crossing Taurus constellation. January 3rd 2011
Winter Sky - Winter Sky - Star sky above the Alps. In the sky, the constellations of the Taurus (right), Orion (center), and the bright star Sirius (lower left). A shooting star crosses the constellation of Taurus. January 3, 2011. Starry sky above english Alps. In the sky, constellations of Taurus (at right), Orion (centre), and bright star Sirius (bottom left). A shooting star is crossing Taurus constellation. January 3rd 2011

PIX4592866: Winter Sky - Winter Sky - Star sky above the Alps. In the sky, the constellations of the Taurus (right), Orion (center), and the bright star Sirius (lower left). A shooting star crosses the constellation of Taurus. January 3, 2011. Starry sky above english Alps. In the sky, constellations of Taurus (at right), Orion (centre), and bright star Sirius (bottom left). A shooting star is crossing Taurus constellation. January 3rd 2011 / Bridgeman Images

Rocket Ariane 5 GS - 12/2009 - Ariane 5 GS liftoff - 12/2009 - Decolving the Ariane 5 GS rocket with the military satellite Helios - 2B on board. Flight V193 was launched on 18 December 2009. On 18 December 2009, an Ariane 5 GS launcher lifted off from Europe's Spaceport in English Guiana on a journey to place the French military reconnaissance satellite Helios - 2B into Sun - synchronous polar orbit. Flight V193 was the seventh Ariane 5 launch of 2009 and used the last of the GS variant of the launcher. Liftoff of the 49th Ariane 5 mission took place at 17:26 CET/Paris (16:26 UTC; 13:26 English Guiana). The satellite was accurately injected into its target orbit about 59 minutes later. The payload mass for this launch was 5954 kg; the satellite mass was 4200 kg, with payload adapters and dispensers making up the additional 1754 kg
Rocket Ariane 5 GS - 12/2009 - Ariane 5 GS liftoff - 12/2009 - Decolving the Ariane 5 GS rocket with the military satellite Helios - 2B on board. Flight V193 was launched on 18 December 2009. On 18 December 2009, an Ariane 5 GS launcher lifted off from Europe's Spaceport in English Guiana on a journey to place the French military reconnaissance satellite Helios - 2B into Sun - synchronous polar orbit. Flight V193 was the seventh Ariane 5 launch of 2009 and used the last of the GS variant of the launcher. Liftoff of the 49th Ariane 5 mission took place at 17:26 CET/Paris (16:26 UTC; 13:26 English Guiana). The satellite was accurately injected into its target orbit about 59 minutes later. The payload mass for this launch was 5954 kg; the satellite mass was 4200 kg, with payload adapters and dispensers making up the additional 1754 kg

PIX4604377: Rocket Ariane 5 GS - 12/2009 - Ariane 5 GS liftoff - 12/2009 - Decolving the Ariane 5 GS rocket with the military satellite Helios - 2B on board. Flight V193 was launched on 18 December 2009. On 18 December 2009, an Ariane 5 GS launcher lifted off from Europe's Spaceport in English Guiana on a journey to place the French military reconnaissance satellite Helios - 2B into Sun - synchronous polar orbit. Flight V193 was the seventh Ariane 5 launch of 2009 and used the last of the GS variant of the launcher. Liftoff of the 49th Ariane 5 mission took place at 17:26 CET/Paris (16:26 UTC; 13:26 English Guiana). The satellite was accurately injected into its target orbit about 59 minutes later. The payload mass for this launch was 5954 kg; the satellite mass was 4200 kg, with payload adapters and dispensers making up the additional 1754 kg / Bridgeman Images

Constellations of Cassiopee and Cephee - Cassiopeia and Cepheus with constellation lines - Constellations Cassiopeia and Cepheus are two of the most famous constellations in the Northern skies. The shapes of the constellations were drawn on top and some important objects were highlited
Constellations of Cassiopee and Cephee - Cassiopeia and Cepheus with constellation lines - Constellations Cassiopeia and Cepheus are two of the most famous constellations in the Northern skies. The shapes of the constellations were drawn on top and some important objects were highlited

PIX4589747: Constellations of Cassiopee and Cephee - Cassiopeia and Cepheus with constellation lines - Constellations Cassiopeia and Cepheus are two of the most famous constellations in the Northern skies. The shapes of the constellations were drawn on top and some important objects were highlited / Bridgeman Images

Mars Exploration Rover - Mars Exploration Rover is a Martian exploration mission composed of two probes housing two identical rovers, Spirit and Opportunity MER - A, the Spirit robot launched on June 10, 2003, landed on January 3, 2004 in the crater Gusev. MER - B, the Opportunity robot launched on July 8, 2003, landed on January 24, 2004 on Meridiani Planum. The sun rises behind one of the Mars Exploration Rovers as it prepares to analyse a rock with its RAT tool. Mars Exploration Rover (MER) is a robotic mission which aims to explore the Martian surface and geology. The mission began with the sending of two twin rovers: MER - A (Spirit), launched on June 10 2003 and landed on January 03 2004 in Gusev crater; MER - B (Opportunity) launched on July 08 2003 and landed on January 24 2004 at Meridiani Planum
Mars Exploration Rover - Mars Exploration Rover is a Martian exploration mission composed of two probes housing two identical rovers, Spirit and Opportunity MER - A, the Spirit robot launched on June 10, 2003, landed on January 3, 2004 in the crater Gusev. MER - B, the Opportunity robot launched on July 8, 2003, landed on January 24, 2004 on Meridiani Planum. The sun rises behind one of the Mars Exploration Rovers as it prepares to analyse a rock with its RAT tool. Mars Exploration Rover (MER) is a robotic mission which aims to explore the Martian surface and geology. The mission began with the sending of two twin rovers: MER - A (Spirit), launched on June 10 2003 and landed on January 03 2004 in Gusev crater; MER - B (Opportunity) launched on July 08 2003 and landed on January 24 2004 at Meridiani Planum

PIX4606584: Mars Exploration Rover - Mars Exploration Rover is a Martian exploration mission composed of two probes housing two identical rovers, Spirit and Opportunity MER - A, the Spirit robot launched on June 10, 2003, landed on January 3, 2004 in the crater Gusev. MER - B, the Opportunity robot launched on July 8, 2003, landed on January 24, 2004 on Meridiani Planum. The sun rises behind one of the Mars Exploration Rovers as it prepares to analyse a rock with its RAT tool. Mars Exploration Rover (MER) is a robotic mission which aims to explore the Martian surface and geology. The mission began with the sending of two twin rovers: MER - A (Spirit), launched on June 10 2003 and landed on January 03 2004 in Gusev crater; MER - B (Opportunity) launched on July 08 2003 and landed on January 24 2004 at Meridiani Planum / Bridgeman Images

Planetary system around Trappist-1 - Artist's impressions of the TRAPPIST-1 planetary system: Artist's view of extrasolar planets around the red dwarf star TRAPPIST-1. At least seven exoplanets the size of the Earth are orbiting this star 40 light years ago in the constellation Aquarius. All could contain water. This artist's impression shows several of the planets orbiting the ultra-cool red dwarf star TRAPPIST-1. New observations, when combined with very sophisticated analysis, have now yielded good estimates of the densities of all seven of the Earth-sized planets and suggest that they are rich in volatile materials, probably water
Planetary system around Trappist-1 - Artist's impressions of the TRAPPIST-1 planetary system: Artist's view of extrasolar planets around the red dwarf star TRAPPIST-1. At least seven exoplanets the size of the Earth are orbiting this star 40 light years ago in the constellation Aquarius. All could contain water. This artist's impression shows several of the planets orbiting the ultra-cool red dwarf star TRAPPIST-1. New observations, when combined with very sophisticated analysis, have now yielded good estimates of the densities of all seven of the Earth-sized planets and suggest that they are rich in volatile materials, probably water

PIX4608442: Planetary system around Trappist-1 - Artist's impressions of the TRAPPIST-1 planetary system: Artist's view of extrasolar planets around the red dwarf star TRAPPIST-1. At least seven exoplanets the size of the Earth are orbiting this star 40 light years ago in the constellation Aquarius. All could contain water. This artist's impression shows several of the planets orbiting the ultra-cool red dwarf star TRAPPIST-1. New observations, when combined with very sophisticated analysis, have now yielded good estimates of the densities of all seven of the Earth-sized planets and suggest that they are rich in volatile materials, probably water / Bridgeman Images

Leo 1 dwarf galaxy in the Lion - Leo 1 dwarf galaxy - Leo 1 is located about 900,000 light years from Earth. It belongs to the local group, just like our galaxy or Andromede galaxy. It has only been known since the 1950s; it is difficult to observe due to the proximity of the Regulus star, thousands of times brighter. Image obtained from the 3.9m telescope of Siding Spring. The 'Local Group' of galaxies, to which the Milky Way belongs, contains more dwarf galaxies than any other type. The low surface brightness and lack of bright stars makes them difficult to study, even with a large telescope. Leo I presents particular problems because the galaxy appears only 20 arc minutes (less than the apparent diameter of the Moon) from the brilliant star Regulus and special precautions had to be taken to prevent scattered light from the star obliterating its feeble image. The plates from which this picture was made (the first in colour of a dwarf elliptical galaxy) will be used to learn more about the origins of star formation in these light - weight objects
Leo 1 dwarf galaxy in the Lion - Leo 1 dwarf galaxy - Leo 1 is located about 900,000 light years from Earth. It belongs to the local group, just like our galaxy or Andromede galaxy. It has only been known since the 1950s; it is difficult to observe due to the proximity of the Regulus star, thousands of times brighter. Image obtained from the 3.9m telescope of Siding Spring. The 'Local Group' of galaxies, to which the Milky Way belongs, contains more dwarf galaxies than any other type. The low surface brightness and lack of bright stars makes them difficult to study, even with a large telescope. Leo I presents particular problems because the galaxy appears only 20 arc minutes (less than the apparent diameter of the Moon) from the brilliant star Regulus and special precautions had to be taken to prevent scattered light from the star obliterating its feeble image. The plates from which this picture was made (the first in colour of a dwarf elliptical galaxy) will be used to learn more about the origins of star formation in these light - weight objects

PIX4613932: Leo 1 dwarf galaxy in the Lion - Leo 1 dwarf galaxy - Leo 1 is located about 900,000 light years from Earth. It belongs to the local group, just like our galaxy or Andromede galaxy. It has only been known since the 1950s; it is difficult to observe due to the proximity of the Regulus star, thousands of times brighter. Image obtained from the 3.9m telescope of Siding Spring. The 'Local Group' of galaxies, to which the Milky Way belongs, contains more dwarf galaxies than any other type. The low surface brightness and lack of bright stars makes them difficult to study, even with a large telescope. Leo I presents particular problems because the galaxy appears only 20 arc minutes (less than the apparent diameter of the Moon) from the brilliant star Regulus and special precautions had to be taken to prevent scattered light from the star obliterating its feeble image. The plates from which this picture was made (the first in colour of a dwarf elliptical galaxy) will be used to learn more about the origins of star formation in these light - weight objects / Bridgeman Images

McNaught Comet McNaught - View of McNaught Comet in January 2007 in Chile. On the left, a laser shot from the Paranal Observatory. Comet McNaught (C/2006 P1) with laser beam from Paranal observatory in Chile. January 2007
McNaught Comet McNaught - View of McNaught Comet in January 2007 in Chile. On the left, a laser shot from the Paranal Observatory. Comet McNaught (C/2006 P1) with laser beam from Paranal observatory in Chile. January 2007

PIX4570558: McNaught Comet McNaught - View of McNaught Comet in January 2007 in Chile. On the left, a laser shot from the Paranal Observatory. Comet McNaught (C/2006 P1) with laser beam from Paranal observatory in Chile. January 2007 / Bridgeman Images

Gemini 8: Neil Armstrong - Portrait of Astronaut Neil Armstrong, Gemini Mission 8. September 1964 Portrait of Astronaut Neil A. Armstron
Gemini 8: Neil Armstrong - Portrait of Astronaut Neil Armstrong, Gemini Mission 8. September 1964 Portrait of Astronaut Neil A. Armstron

PIX4599462: Gemini 8: Neil Armstrong - Portrait of Astronaut Neil Armstrong, Gemini Mission 8. September 1964 Portrait of Astronaut Neil A. Armstron / Bridgeman Images

Apollo - Soyuz: A. Leonov and D. Slayton - Apollo - Soyuz: Donald Slayton and Aleksey Leonov - Donald Slayton (left) and Aleksey Leonov photographs in the Soyuz during the junction of the Apollo module and the Soyuz spaceship. 17/07/1975. Donald Slayton and Aleksey Leonov photographed in the Soyuz Orbital Module during the joint US - USSR Apollo Soyuz Test Project. Jul 17 1975
Apollo - Soyuz: A. Leonov and D. Slayton - Apollo - Soyuz: Donald Slayton and Aleksey Leonov - Donald Slayton (left) and Aleksey Leonov photographs in the Soyuz during the junction of the Apollo module and the Soyuz spaceship. 17/07/1975. Donald Slayton and Aleksey Leonov photographed in the Soyuz Orbital Module during the joint US - USSR Apollo Soyuz Test Project. Jul 17 1975

PIX4598461: Apollo - Soyuz: A. Leonov and D. Slayton - Apollo - Soyuz: Donald Slayton and Aleksey Leonov - Donald Slayton (left) and Aleksey Leonov photographs in the Soyuz during the junction of the Apollo module and the Soyuz spaceship. 17/07/1975. Donald Slayton and Aleksey Leonov photographed in the Soyuz Orbital Module during the joint US - USSR Apollo Soyuz Test Project. Jul 17 1975 / Bridgeman Images

Barree spiral galaxy M109 in the Great Bear - Barred spiral galaxy M109 in Ursa Major - The barree spiral galaxy M109 (NGC 3992) is located about 45 million years away - light from Earth. The barred spiral galaxy M109 (NGC 3992) is located at about 45 million light year from the Earth
Barree spiral galaxy M109 in the Great Bear - Barred spiral galaxy M109 in Ursa Major - The barree spiral galaxy M109 (NGC 3992) is located about 45 million years away - light from Earth. The barred spiral galaxy M109 (NGC 3992) is located at about 45 million light year from the Earth

PIX4611025: Barree spiral galaxy M109 in the Great Bear - Barred spiral galaxy M109 in Ursa Major - The barree spiral galaxy M109 (NGC 3992) is located about 45 million years away - light from Earth. The barred spiral galaxy M109 (NGC 3992) is located at about 45 million light year from the Earth / Bridgeman Images

Artist's view of the New Horizons probe and a Kuiper object - The New Horizons spacecraft near Kuiper Belt Object - Artist's view of the New Horizons probe approaching a Kuiper object. The Sun shines more than 6 billion km surrounded by a disc of dust. Jupiter and Neptune appear as two stars to the right of the Sun. The New Horizons probe was launched on 19 January 2006 to Jupiter, then Pluto and Charon, which it will reach in 2015 and Kuiper's objects in 2020. Artist's impression of the New Horizons spacecraft encountering a Kuiper Belt object. The Sun, more than 4.1 billion miles (6.7 billion kilometers) away, shines as a bright star embedded in the glow of the zodiacal dust cloud. Jupiter and Neptune are visible as orange and blue “” stars””” to the right of the Sun. Although you would not actually see the myriad other objects that make up the Kuiper Belt because they are so far apart, they are shown here to give the impression of an extensive disk of icy worlds beyond Neptune
Artist's view of the New Horizons probe and a Kuiper object - The New Horizons spacecraft near Kuiper Belt Object - Artist's view of the New Horizons probe approaching a Kuiper object. The Sun shines more than 6 billion km surrounded by a disc of dust. Jupiter and Neptune appear as two stars to the right of the Sun. The New Horizons probe was launched on 19 January 2006 to Jupiter, then Pluto and Charon, which it will reach in 2015 and Kuiper's objects in 2020. Artist's impression of the New Horizons spacecraft encountering a Kuiper Belt object. The Sun, more than 4.1 billion miles (6.7 billion kilometers) away, shines as a bright star embedded in the glow of the zodiacal dust cloud. Jupiter and Neptune are visible as orange and blue “” stars””” to the right of the Sun. Although you would not actually see the myriad other objects that make up the Kuiper Belt because they are so far apart, they are shown here to give the impression of an extensive disk of icy worlds beyond Neptune

PIX4607276: Artist's view of the New Horizons probe and a Kuiper object - The New Horizons spacecraft near Kuiper Belt Object - Artist's view of the New Horizons probe approaching a Kuiper object. The Sun shines more than 6 billion km surrounded by a disc of dust. Jupiter and Neptune appear as two stars to the right of the Sun. The New Horizons probe was launched on 19 January 2006 to Jupiter, then Pluto and Charon, which it will reach in 2015 and Kuiper's objects in 2020. Artist's impression of the New Horizons spacecraft encountering a Kuiper Belt object. The Sun, more than 4.1 billion miles (6.7 billion kilometers) away, shines as a bright star embedded in the glow of the zodiacal dust cloud. Jupiter and Neptune are visible as orange and blue “” stars””” to the right of the Sun. Although you would not actually see the myriad other objects that make up the Kuiper Belt because they are so far apart, they are shown here to give the impression of an extensive disk of icy worlds beyond Neptune / Bridgeman Images

Vincennes, Festival America, (North American Literature Festival), 30/09/2006: portrait of Canadian writer David Albahari.
Vincennes, Festival America, (North American Literature Festival), 30/09/2006: portrait of Canadian writer David Albahari.

AUL4125479: Vincennes, Festival America, (North American Literature Festival), 30/09/2006: portrait of Canadian writer David Albahari. / Bridgeman Images

ISS: astronaut exit and Cupola - Astronaut with Cupola module on ISS - Astronaut Nicholas Patrick participates in a space trip to continue the construction and maintenance of the International Space Station (ISS). He works here on Cupola, the new observation module. 17 February 2010. NASA astronaut Nicholas Patrick participates in the mission's third and final session of extravehicular activity (EVA) as construction and maintenance continue on the International Space Station. During the five - hour, 48 - minute spacewalk, Patrick and astronaut Behnken completed all of their planned tasks, removing insulation blankets and removing launch restraint bolts from each of the Cupola's seven windows. February 17, 2010
ISS: astronaut exit and Cupola - Astronaut with Cupola module on ISS - Astronaut Nicholas Patrick participates in a space trip to continue the construction and maintenance of the International Space Station (ISS). He works here on Cupola, the new observation module. 17 February 2010. NASA astronaut Nicholas Patrick participates in the mission's third and final session of extravehicular activity (EVA) as construction and maintenance continue on the International Space Station. During the five - hour, 48 - minute spacewalk, Patrick and astronaut Behnken completed all of their planned tasks, removing insulation blankets and removing launch restraint bolts from each of the Cupola's seven windows. February 17, 2010

PIX4602719: ISS: astronaut exit and Cupola - Astronaut with Cupola module on ISS - Astronaut Nicholas Patrick participates in a space trip to continue the construction and maintenance of the International Space Station (ISS). He works here on Cupola, the new observation module. 17 February 2010. NASA astronaut Nicholas Patrick participates in the mission's third and final session of extravehicular activity (EVA) as construction and maintenance continue on the International Space Station. During the five - hour, 48 - minute spacewalk, Patrick and astronaut Behnken completed all of their planned tasks, removing insulation blankets and removing launch restraint bolts from each of the Cupola's seven windows. February 17, 2010 / 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. A diffusing filter was used to enhance star color and general shape of the constellations.
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. A diffusing filter was used to enhance star color and general shape of the constellations.

PIX4636541: 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. A diffusing filter was used to enhance star color and general shape of the constellations. / Bridgeman Images

Earth seen by satellite DSCOVR - Earth seen by satellite DSCOVR: Earth photo obtained by satellite Deep Space Climate Observatory (DSCOVR) on July 6, 2015. This satellite, launched on 11 February 2015, and placed in orbit 1.6 million km, at the point of Lagrange L1 (about 4 times farther than the Moon's orbit), provides views of the Earth as a whole - The journey has been a long one for the Deep Space Climate Observatory (DSCOVR). Once known as Triana, the satellite was conceived in 1998 to provide continuous views of Earth, to monitor the solar wind, and to measure fluctuations in Earth's albedo. The mission was put on hold in 2001, and the part-built satellite ended up in storage for several years with an uncertain future. In 2008, the National Oceanic and Atmospheric Administration (NOAA), NASA, and the U.S. Air Force decided to refurbish and update the spacecraft for launch - On February 11, 2015, DSCOVR was finally lofted into space by a SpaceX Falcon 9 rocket. After journey of about 1.6 million kilometers (1 million miles) to the L1 Lagrange Point, the satellite and its Earth Polychromatic Imaging Camera (EPIC) has returned its first view of the entire sunlit side of Earth. At L1-four times farther than the orbit of the Moon - the gravitational pull of the Sun and Earth cancel out, providing a stable orbit and a continuous view of Earth. The image above was made by combining information from Epic's red, green, and blue bands. (Bands are narrow regions of the electromagnetic spectrum to which a remote sensing instrument responds. When EPIC collects data, it takes a series of 10 images at different bands - from ultraviolet to near infrared.)
Earth seen by satellite DSCOVR - Earth seen by satellite DSCOVR: Earth photo obtained by satellite Deep Space Climate Observatory (DSCOVR) on July 6, 2015. This satellite, launched on 11 February 2015, and placed in orbit 1.6 million km, at the point of Lagrange L1 (about 4 times farther than the Moon's orbit), provides views of the Earth as a whole - The journey has been a long one for the Deep Space Climate Observatory (DSCOVR). Once known as Triana, the satellite was conceived in 1998 to provide continuous views of Earth, to monitor the solar wind, and to measure fluctuations in Earth's albedo. The mission was put on hold in 2001, and the part-built satellite ended up in storage for several years with an uncertain future. In 2008, the National Oceanic and Atmospheric Administration (NOAA), NASA, and the U.S. Air Force decided to refurbish and update the spacecraft for launch - On February 11, 2015, DSCOVR was finally lofted into space by a SpaceX Falcon 9 rocket. After journey of about 1.6 million kilometers (1 million miles) to the L1 Lagrange Point, the satellite and its Earth Polychromatic Imaging Camera (EPIC) has returned its first view of the entire sunlit side of Earth. At L1-four times farther than the orbit of the Moon - the gravitational pull of the Sun and Earth cancel out, providing a stable orbit and a continuous view of Earth. The image above was made by combining information from Epic's red, green, and blue bands. (Bands are narrow regions of the electromagnetic spectrum to which a remote sensing instrument responds. When EPIC collects data, it takes a series of 10 images at different bands - from ultraviolet to near infrared.)

PIX4669145: Earth seen by satellite DSCOVR - Earth seen by satellite DSCOVR: Earth photo obtained by satellite Deep Space Climate Observatory (DSCOVR) on July 6, 2015. This satellite, launched on 11 February 2015, and placed in orbit 1.6 million km, at the point of Lagrange L1 (about 4 times farther than the Moon's orbit), provides views of the Earth as a whole - The journey has been a long one for the Deep Space Climate Observatory (DSCOVR). Once known as Triana, the satellite was conceived in 1998 to provide continuous views of Earth, to monitor the solar wind, and to measure fluctuations in Earth's albedo. The mission was put on hold in 2001, and the part-built satellite ended up in storage for several years with an uncertain future. In 2008, the National Oceanic and Atmospheric Administration (NOAA), NASA, and the U.S. Air Force decided to refurbish and update the spacecraft for launch - On February 11, 2015, DSCOVR was finally lofted into space by a SpaceX Falcon 9 rocket. After journey of about 1.6 million kilometers (1 million miles) to the L1 Lagrange Point, the satellite and its Earth Polychromatic Imaging Camera (EPIC) has returned its first view of the entire sunlit side of Earth. At L1-four times farther than the orbit of the Moon - the gravitational pull of the Sun and Earth cancel out, providing a stable orbit and a continuous view of Earth. The image above was made by combining information from Epic's red, green, and blue bands. (Bands are narrow regions of the electromagnetic spectrum to which a remote sensing instrument responds. When EPIC collects data, it takes a series of 10 images at different bands - from ultraviolet to near infrared.) / Bridgeman Images

Aurore Boreale - Iceland - Akureyri Fjord lights - Iceland: Aurora boreale on Eyjafjoer fjord at the end of Akureyri Bay. March 2016. A wonderful display of the northern lights at the end of the Akureyri bay
Aurore Boreale - Iceland - Akureyri Fjord lights - Iceland: Aurora boreale on Eyjafjoer fjord at the end of Akureyri Bay. March 2016. A wonderful display of the northern lights at the end of the Akureyri bay

PIX4670679: Aurore Boreale - Iceland - Akureyri Fjord lights - Iceland: Aurora boreale on Eyjafjoer fjord at the end of Akureyri Bay. March 2016. A wonderful display of the northern lights at the end of the Akureyri bay / Bridgeman Images

Umnak Island - Aleutian Islands - Alaska - Umnak Island - Aleutian Islands - Alaska: Umnak Island is one of the Fox Islands, belonging to the Aleutian Islands in Alaska, USA. With an area of more than 1,776 km, it is the third largest of the Aleutian Islands. At the top right is the Okmok caldera (erupted in 2008), below the Vsevidof volcano; below the left, the Ile des Quatre Montagnes. Image obtained on 3 May 2014 by the Landsat-8 satellite. On May 3, 2014, the Landsat 8 satellite acquired this natural-color image of Umnak Island and its volcanic neighbors in the Aleutian Island chain. Part of the Fox Islands, Umnak is the third largest in the Aleutian chain and lies just southwest of Unalaska. Umnak is mostly unpopulated, with roughly 40 people living in the village of Nikolski near the southwest tip of the island. Being a volcanic island, Umnak has numerous mud pots, hot springs, and the only geysers in Alaska. The landscape is dominated by volcanoes. On the northern half of the island, Okmok - site of the 2008 eruption - rises 1073 meters (3,520 feet) above sea level as a broad shield volcano with a caldera nestled near the top. A crater lake sits amidst the volcanic ash and debris in the caldera. Mount Vsevidof, a symmetrical stratovolcano, rises 2149 meters (7,050 feet) and dominates the skyline of the southern portion of Umnak Island. The volcanic Islands of the Four Mountains are also visible in the lower left of the wide image
Umnak Island - Aleutian Islands - Alaska - Umnak Island - Aleutian Islands - Alaska: Umnak Island is one of the Fox Islands, belonging to the Aleutian Islands in Alaska, USA. With an area of more than 1,776 km, it is the third largest of the Aleutian Islands. At the top right is the Okmok caldera (erupted in 2008), below the Vsevidof volcano; below the left, the Ile des Quatre Montagnes. Image obtained on 3 May 2014 by the Landsat-8 satellite. On May 3, 2014, the Landsat 8 satellite acquired this natural-color image of Umnak Island and its volcanic neighbors in the Aleutian Island chain. Part of the Fox Islands, Umnak is the third largest in the Aleutian chain and lies just southwest of Unalaska. Umnak is mostly unpopulated, with roughly 40 people living in the village of Nikolski near the southwest tip of the island. Being a volcanic island, Umnak has numerous mud pots, hot springs, and the only geysers in Alaska. The landscape is dominated by volcanoes. On the northern half of the island, Okmok - site of the 2008 eruption - rises 1073 meters (3,520 feet) above sea level as a broad shield volcano with a caldera nestled near the top. A crater lake sits amidst the volcanic ash and debris in the caldera. Mount Vsevidof, a symmetrical stratovolcano, rises 2149 meters (7,050 feet) and dominates the skyline of the southern portion of Umnak Island. The volcanic Islands of the Four Mountains are also visible in the lower left of the wide image

PIX4672476: Umnak Island - Aleutian Islands - Alaska - Umnak Island - Aleutian Islands - Alaska: Umnak Island is one of the Fox Islands, belonging to the Aleutian Islands in Alaska, USA. With an area of more than 1,776 km, it is the third largest of the Aleutian Islands. At the top right is the Okmok caldera (erupted in 2008), below the Vsevidof volcano; below the left, the Ile des Quatre Montagnes. Image obtained on 3 May 2014 by the Landsat-8 satellite. On May 3, 2014, the Landsat 8 satellite acquired this natural-color image of Umnak Island and its volcanic neighbors in the Aleutian Island chain. Part of the Fox Islands, Umnak is the third largest in the Aleutian chain and lies just southwest of Unalaska. Umnak is mostly unpopulated, with roughly 40 people living in the village of Nikolski near the southwest tip of the island. Being a volcanic island, Umnak has numerous mud pots, hot springs, and the only geysers in Alaska. The landscape is dominated by volcanoes. On the northern half of the island, Okmok - site of the 2008 eruption - rises 1073 meters (3,520 feet) above sea level as a broad shield volcano with a caldera nestled near the top. A crater lake sits amidst the volcanic ash and debris in the caldera. Mount Vsevidof, a symmetrical stratovolcano, rises 2149 meters (7,050 feet) and dominates the skyline of the southern portion of Umnak Island. The volcanic Islands of the Four Mountains are also visible in the lower left of the wide image / Bridgeman Images

Image obtained from the International Space Station (ISS). Tambora Volcano is a huge stratovolcano 60 km in diameter. His eruption on April 10, 1815 was the deadliest in history.
Image obtained from the International Space Station (ISS). Tambora Volcano is a huge stratovolcano 60 km in diameter. His eruption on April 10, 1815 was the deadliest in history.

PIX4661498: Image obtained from the International Space Station (ISS). Tambora Volcano is a huge stratovolcano 60 km in diameter. His eruption on April 10, 1815 was the deadliest in history. / Bridgeman Images

Sinosauropteryx - View of a Sinosauropteryx prima, a small theropod dinosaur who lived in China 130 million years ago, at the beginning of Cretace. A metre-long compsognathid dinosaur, Sinosauropteryx prima, drilling for prey in a Cretaceous Chinese forest. This dinosaur is among the growing number whose remains include preserved feather-like integumentary structures, strongly suggesting their close kinship with birds
Sinosauropteryx - View of a Sinosauropteryx prima, a small theropod dinosaur who lived in China 130 million years ago, at the beginning of Cretace. A metre-long compsognathid dinosaur, Sinosauropteryx prima, drilling for prey in a Cretaceous Chinese forest. This dinosaur is among the growing number whose remains include preserved feather-like integumentary structures, strongly suggesting their close kinship with birds

PIX4662478: Sinosauropteryx - View of a Sinosauropteryx prima, a small theropod dinosaur who lived in China 130 million years ago, at the beginning of Cretace. A metre-long compsognathid dinosaur, Sinosauropteryx prima, drilling for prey in a Cretaceous Chinese forest. This dinosaur is among the growing number whose remains include preserved feather-like integumentary structures, strongly suggesting their close kinship with birds / Bridgeman Images

Sulfur flow in molten - Kawah Ijen volcano -Java, Indonesia - Sulfur burning flow at Kawah Ijen volcano -Java, Indonesia - Sulfur flow in molten on Kawah Ijen volcano. Sulphur on fire emits a blue glow. This active stratovolcano is located on the island of Java in Indonesia, on the Pacific belt of fire. Sulfur burning flow at Kawah Ijen volcano seen at night. Burning sulfur is emitting blue light. This active stratovolcano is located on the island of Java in Indonesia on the Pacific Ring of fire
Sulfur flow in molten - Kawah Ijen volcano -Java, Indonesia - Sulfur burning flow at Kawah Ijen volcano -Java, Indonesia - Sulfur flow in molten on Kawah Ijen volcano. Sulphur on fire emits a blue glow. This active stratovolcano is located on the island of Java in Indonesia, on the Pacific belt of fire. Sulfur burning flow at Kawah Ijen volcano seen at night. Burning sulfur is emitting blue light. This active stratovolcano is located on the island of Java in Indonesia on the Pacific Ring of fire

PIX4677108: Sulfur flow in molten - Kawah Ijen volcano -Java, Indonesia - Sulfur burning flow at Kawah Ijen volcano -Java, Indonesia - Sulfur flow in molten on Kawah Ijen volcano. Sulphur on fire emits a blue glow. This active stratovolcano is located on the island of Java in Indonesia, on the Pacific belt of fire. Sulfur burning flow at Kawah Ijen volcano seen at night. Burning sulfur is emitting blue light. This active stratovolcano is located on the island of Java in Indonesia on the Pacific Ring of fire / Bridgeman Images

Sulphur miner on the volcano Kawah Ijen -Java, Indonesia - Sulfer miner on Kawah Ijen volcano -Java, Indonesia - A sulfur miner in the solfatare of the volcano Kawah Ijen on the island of Java in Indonesia. Sulphur on fire emits a blue glow. Sulfur miner on Kawah Ijen volcano seen at night. Burning sulfur is emitting blue light. Island of Java, Indonesia
Sulphur miner on the volcano Kawah Ijen -Java, Indonesia - Sulfer miner on Kawah Ijen volcano -Java, Indonesia - A sulfur miner in the solfatare of the volcano Kawah Ijen on the island of Java in Indonesia. Sulphur on fire emits a blue glow. Sulfur miner on Kawah Ijen volcano seen at night. Burning sulfur is emitting blue light. Island of Java, Indonesia

PIX4677114: Sulphur miner on the volcano Kawah Ijen -Java, Indonesia - Sulfer miner on Kawah Ijen volcano -Java, Indonesia - A sulfur miner in the solfatare of the volcano Kawah Ijen on the island of Java in Indonesia. Sulphur on fire emits a blue glow. Sulfur miner on Kawah Ijen volcano seen at night. Burning sulfur is emitting blue light. Island of Java, Indonesia / Bridgeman Images


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