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The ambulatory of the choir was only covered with slabs forming a terrace in the 14th century. Cathedrale Notre Dame de Paris - Paris 4 - XIIIth, XIIIth, XIXth, rehabilitation by Viollet-le-Duc -
The ambulatory of the choir was only covered with slabs forming a terrace in the 14th century. Cathedrale Notre Dame de Paris - Paris 4 - XIIIth, XIIIth, XIXth, rehabilitation by Viollet-le-Duc -

ITR4553529: The ambulatory of the choir was only covered with slabs forming a terrace in the 14th century. Cathedrale Notre Dame de Paris - Paris 4 - XIIIth, XIIIth, XIXth, rehabilitation by Viollet-le-Duc - / Bridgeman Images

ID: ITR4553529

The ambulatory of the choir was only covered with slabs forming a terrace in the 14th century. Cathedrale Notre Dame de Paris - Paris 4 - XIIIth, XIIIth, XIXth, rehabilitation by Viollet-le-Duc -

Open cluster M26 in the ECU of Sobieski - Open cluster M26 in Scutum - M26 (NGC 6694) is located about 5000 years - light from Earth and is about 90 million years old. M26 is an open cluster in the constellation Scutum. A fairly tight cluster, in this deep image it has to compete with a very populous background of Milky Way stars. It is about 5000 light - years away and around 90 million years old
Open cluster M26 in the ECU of Sobieski - Open cluster M26 in Scutum - M26 (NGC 6694) is located about 5000 years - light from Earth and is about 90 million years old. M26 is an open cluster in the constellation Scutum. A fairly tight cluster, in this deep image it has to compete with a very populous background of Milky Way stars. It is about 5000 light - years away and around 90 million years old

PIX4568402: Open cluster M26 in the ECU of Sobieski - Open cluster M26 in Scutum - M26 (NGC 6694) is located about 5000 years - light from Earth and is about 90 million years old. M26 is an open cluster in the constellation Scutum. A fairly tight cluster, in this deep image it has to compete with a very populous background of Milky Way stars. It is about 5000 light - years away and around 90 million years old / Bridgeman Images

ID: PIX4568402

Open cluster M26 in the ECU of Sobieski - Open cluster M26 in Scutum - M26 (NGC 6694) is located about 5000 years - light from Earth and is about 90 million years old. M26 is an open cluster in the constellation Scutum. A fairly tight cluster, in this deep image it has to compete with a very populous background of Milky Way stars. It is about 5000 light - years away and around 90 million years old

The port of Rotterdam, Netherlands (Netherlands) is the first European port and is located at the mouth of the Meuse and the Rhine.
The port of Rotterdam, Netherlands (Netherlands) is the first European port and is located at the mouth of the Meuse and the Rhine.

TEC4568449: The port of Rotterdam, Netherlands (Netherlands) is the first European port and is located at the mouth of the Meuse and the Rhine. / Bridgeman Images

ID: TEC4568449

The port of Rotterdam, Netherlands (Netherlands) is the first European port and is located at the mouth of the Meuse and the Rhine.

Open cluster M11 in the ECU of Sobieski - M11 open cluster in Scutum - M11 (NGC 6705) is a cluster of about 3000 stars. Image obtained by Siding Spring Clusters of bright blue stars like M11 are found scattered among the spiral arms of the Milky Way and other galaxies like it. They are a clear sign that star formation is active, because such clusters are usually very young and short lived. The stars in M11 all formed from the same material and at about the same time, a few million years ago. In 100 million years or so, all the brightest stars in the group will have evolved into cool supergiants and exploded as supernovae, leaving behind large numbers of low mass, relatively faint stars whose lives will be much longer and whose end will be much less dramatic. Located in the constellation of Scutum, it is sometimes mistaken for a loose globular cluster. M11 is also called the “” Wild Duck Cluster”” because of it's resemblance to a flight of wild ducks when viewed in a telescope. M11, with an overall brightness of magnitude 5.8, contains as many as 500 stars ranging from 8th magnitude down to 14th magnitude
Open cluster M11 in the ECU of Sobieski - M11 open cluster in Scutum - M11 (NGC 6705) is a cluster of about 3000 stars. Image obtained by Siding Spring Clusters of bright blue stars like M11 are found scattered among the spiral arms of the Milky Way and other galaxies like it. They are a clear sign that star formation is active, because such clusters are usually very young and short lived. The stars in M11 all formed from the same material and at about the same time, a few million years ago. In 100 million years or so, all the brightest stars in the group will have evolved into cool supergiants and exploded as supernovae, leaving behind large numbers of low mass, relatively faint stars whose lives will be much longer and whose end will be much less dramatic. Located in the constellation of Scutum, it is sometimes mistaken for a loose globular cluster. M11 is also called the “” Wild Duck Cluster”” because of it's resemblance to a flight of wild ducks when viewed in a telescope. M11, with an overall brightness of magnitude 5.8, contains as many as 500 stars ranging from 8th magnitude down to 14th magnitude

PIX4568454: Open cluster M11 in the ECU of Sobieski - M11 open cluster in Scutum - M11 (NGC 6705) is a cluster of about 3000 stars. Image obtained by Siding Spring Clusters of bright blue stars like M11 are found scattered among the spiral arms of the Milky Way and other galaxies like it. They are a clear sign that star formation is active, because such clusters are usually very young and short lived. The stars in M11 all formed from the same material and at about the same time, a few million years ago. In 100 million years or so, all the brightest stars in the group will have evolved into cool supergiants and exploded as supernovae, leaving behind large numbers of low mass, relatively faint stars whose lives will be much longer and whose end will be much less dramatic. Located in the constellation of Scutum, it is sometimes mistaken for a loose globular cluster. M11 is also called the “” Wild Duck Cluster”” because of it's resemblance to a flight of wild ducks when viewed in a telescope. M11, with an overall brightness of magnitude 5.8, contains as many as 500 stars ranging from 8th magnitude down to 14th magnitude / Bridgeman Images

ID: PIX4568454

Open cluster M11 in the ECU of Sobieski - M11 open cluster in Scutum - M11 (NGC 6705) is a cluster of about 3000 stars. Image obtained by Siding Spring Clusters of bright blue stars like M11 are found scattered among the spiral arms of the Milky Way and other galaxies like it. They are a clear sign that star formation is active, because such clusters are usually very young and short lived. The stars in M11 all formed from the same material and at about the same time, a few million years ago. In 100 million years or so, all the brightest stars in the group will have evolved into cool supergiants and exploded as supernovae, leaving behind large numbers of low mass, relatively faint stars whose lives will be much longer and whose end will be much less dramatic. Located in the constellation of Scutum, it is sometimes mistaken for a loose globular cluster. M11 is also called the “” Wild Duck Cluster”” because of it's resemblance to a flight of wild ducks when viewed in a telescope. M11, wit

The port of Rotterdam, Netherlands (Netherlands) is the first European port and is located at the mouth of the Meuse and the Rhine.
The port of Rotterdam, Netherlands (Netherlands) is the first European port and is located at the mouth of the Meuse and the Rhine.

TEC4568459: The port of Rotterdam, Netherlands (Netherlands) is the first European port and is located at the mouth of the Meuse and the Rhine. / Bridgeman Images

ID: TEC4568459

The port of Rotterdam, Netherlands (Netherlands) is the first European port and is located at the mouth of the Meuse and the Rhine.

Page of musical score of Psalm 23, op 132, D 706 by Franz Schubert
Page of musical score of Psalm 23, op 132, D 706 by Franz Schubert

LRI4568506: Page of musical score of Psalm 23, op 132, D 706 by Franz Schubert / Bridgeman Images

ID: LRI4568506

Page of musical score of Psalm 23, op 132, D 706 by Franz Schubert

The northern fence of the Cathedrale Notre-Dame de Paris tells the life of Jesus: The Flight in Egypt Cathedrale Notre Dame de Paris - Paris 4 - XIIIth, XIIIth, XIXth, rehabilitation by Viollet-le-Duc -
The northern fence of the Cathedrale Notre-Dame de Paris tells the life of Jesus: The Flight in Egypt Cathedrale Notre Dame de Paris - Paris 4 - XIIIth, XIIIth, XIXth, rehabilitation by Viollet-le-Duc -

ITR4553687: The northern fence of the Cathedrale Notre-Dame de Paris tells the life of Jesus: The Flight in Egypt Cathedrale Notre Dame de Paris - Paris 4 - XIIIth, XIIIth, XIXth, rehabilitation by Viollet-le-Duc - / Bridgeman Images

ID: ITR4553687

The northern fence of the Cathedrale Notre-Dame de Paris tells the life of Jesus: The Flight in Egypt Cathedrale Notre Dame de Paris - Paris 4 - XIIIth, XIIIth, XIXth, rehabilitation by Viollet-le-Duc -

Spiral Galaxy NGC 4450 - Spiral Galaxy NGC 4450 in Coma Berenices. Image obtained with a telescope of 80 cm. NGC 4450 is a spiral galaxy in the constellation Coma Berenices. Image was taken with a 32 - inch Schulman Telescope (RC Optical Systems)
Spiral Galaxy NGC 4450 - Spiral Galaxy NGC 4450 in Coma Berenices. Image obtained with a telescope of 80 cm. NGC 4450 is a spiral galaxy in the constellation Coma Berenices. Image was taken with a 32 - inch Schulman Telescope (RC Optical Systems)

PIX4611379: Spiral Galaxy NGC 4450 - Spiral Galaxy NGC 4450 in Coma Berenices. Image obtained with a telescope of 80 cm. NGC 4450 is a spiral galaxy in the constellation Coma Berenices. Image was taken with a 32 - inch Schulman Telescope (RC Optical Systems) / Bridgeman Images

ID: PIX4611379

Spiral Galaxy NGC 4450 - Spiral Galaxy NGC 4450 in Coma Berenices. Image obtained with a telescope of 80 cm. NGC 4450 is a spiral galaxy in the constellation Coma Berenices. Image was taken with a 32 - inch Schulman Telescope (RC Optical Systems)

M87 elliptical galaxy in Virgo - M87 elliptical galaxy in Virgo - The M87 galaxy (NGC 4486) is located about 52 million years away - light from Earth, in the heart of the Virgin's cluster. M87 is the brightest radio source in the constellation, it is also called Virgo A. Gigantic elliptical galaxy M87 is located at the heart of the Virgo Cluster of galaxies. Also known as radio source Virgo A, M87 is located about 60 million light years away. It appears to have a linear size of 120,000 light years and a mass estimated at 2.7 trillion solar masses, and an extreme luminosity, with an absolute magnitude of about - 22
M87 elliptical galaxy in Virgo - M87 elliptical galaxy in Virgo - The M87 galaxy (NGC 4486) is located about 52 million years away - light from Earth, in the heart of the Virgin's cluster. M87 is the brightest radio source in the constellation, it is also called Virgo A. Gigantic elliptical galaxy M87 is located at the heart of the Virgo Cluster of galaxies. Also known as radio source Virgo A, M87 is located about 60 million light years away. It appears to have a linear size of 120,000 light years and a mass estimated at 2.7 trillion solar masses, and an extreme luminosity, with an absolute magnitude of about - 22

PIX4611436: M87 elliptical galaxy in Virgo - M87 elliptical galaxy in Virgo - The M87 galaxy (NGC 4486) is located about 52 million years away - light from Earth, in the heart of the Virgin's cluster. M87 is the brightest radio source in the constellation, it is also called Virgo A. Gigantic elliptical galaxy M87 is located at the heart of the Virgo Cluster of galaxies. Also known as radio source Virgo A, M87 is located about 60 million light years away. It appears to have a linear size of 120,000 light years and a mass estimated at 2.7 trillion solar masses, and an extreme luminosity, with an absolute magnitude of about - 22 / Bridgeman Images

ID: PIX4611436

M87 elliptical galaxy in Virgo - M87 elliptical galaxy in Virgo - The M87 galaxy (NGC 4486) is located about 52 million years away - light from Earth, in the heart of the Virgin's cluster. M87 is the brightest radio source in the constellation, it is also called Virgo A. Gigantic elliptical galaxy M87 is located at the heart of the Virgo Cluster of galaxies. Also known as radio source Virgo A, M87 is located about 60 million light years away. It appears to have a linear size of 120,000 light years and a mass estimated at 2.7 trillion solar masses, and an extreme luminosity, with an absolute magnitude of about - 22

M87 elliptical galaxy in Virgo - M87 elliptical galaxy in Virgo - The M87 galaxy (NGC 4486) is 54 million years ago - light from Earth, in the heart of the Virgin's cluster. This image is a composite obtained in X-rays, radio and visible. Gas material is ejected from the heart of the galaxy. A supermassive black hole would have caused this jet. This image is a composite of visible (or optical), radio, and X - ray data of the giant elliptical galaxy, M87. M87 lies at a distance of 54 million light years and is the largest galaxy in the Virgo cluster of galaxies. Bright jets moving at close to the speed of light are seen at all wavelengths coming from the massive black hole at the center of the galaxy. It has also been identified with the strong radio source, Virgo A, and is a powerful source of X - rays as it resides near the center of a hot, X - ray emitting cloud that extends over much of the Virgo cluster. The extended radio emission consists of plumes of fast - moving gas from the jets rising into the X - ray emitting cluster medium. Chandra X - ray image in X - rays, M87 also reveals evidence for a series of outbursts from the central supermassive black hole. The loops and bubbles in the hot, X - ray emitting gas are relics of small outbursts from close to the black hole. Other interesting features in M87 are narrow filaments of X - ray emission, which may be due to hot gas trapped by magnetic fields. One of these filaments is over 100,000 light years long, and extends below and to the right of the center of M87 in almost a straight line. The optical data of M87 were obtained with Hubble's Advanced Camera for Surveys in visible and infrared filters
M87 elliptical galaxy in Virgo - M87 elliptical galaxy in Virgo - The M87 galaxy (NGC 4486) is 54 million years ago - light from Earth, in the heart of the Virgin's cluster. This image is a composite obtained in X-rays, radio and visible. Gas material is ejected from the heart of the galaxy. A supermassive black hole would have caused this jet. This image is a composite of visible (or optical), radio, and X - ray data of the giant elliptical galaxy, M87. M87 lies at a distance of 54 million light years and is the largest galaxy in the Virgo cluster of galaxies. Bright jets moving at close to the speed of light are seen at all wavelengths coming from the massive black hole at the center of the galaxy. It has also been identified with the strong radio source, Virgo A, and is a powerful source of X - rays as it resides near the center of a hot, X - ray emitting cloud that extends over much of the Virgo cluster. The extended radio emission consists of plumes of fast - moving gas from the jets rising into the X - ray emitting cluster medium. Chandra X - ray image in X - rays, M87 also reveals evidence for a series of outbursts from the central supermassive black hole. The loops and bubbles in the hot, X - ray emitting gas are relics of small outbursts from close to the black hole. Other interesting features in M87 are narrow filaments of X - ray emission, which may be due to hot gas trapped by magnetic fields. One of these filaments is over 100,000 light years long, and extends below and to the right of the center of M87 in almost a straight line. The optical data of M87 were obtained with Hubble's Advanced Camera for Surveys in visible and infrared filters

PIX4611440: M87 elliptical galaxy in Virgo - M87 elliptical galaxy in Virgo - The M87 galaxy (NGC 4486) is 54 million years ago - light from Earth, in the heart of the Virgin's cluster. This image is a composite obtained in X-rays, radio and visible. Gas material is ejected from the heart of the galaxy. A supermassive black hole would have caused this jet. This image is a composite of visible (or optical), radio, and X - ray data of the giant elliptical galaxy, M87. M87 lies at a distance of 54 million light years and is the largest galaxy in the Virgo cluster of galaxies. Bright jets moving at close to the speed of light are seen at all wavelengths coming from the massive black hole at the center of the galaxy. It has also been identified with the strong radio source, Virgo A, and is a powerful source of X - rays as it resides near the center of a hot, X - ray emitting cloud that extends over much of the Virgo cluster. The extended radio emission consists of plumes of fast - moving gas from the jets rising into the X - ray emitting cluster medium. Chandra X - ray image in X - rays, M87 also reveals evidence for a series of outbursts from the central supermassive black hole. The loops and bubbles in the hot, X - ray emitting gas are relics of small outbursts from close to the black hole. Other interesting features in M87 are narrow filaments of X - ray emission, which may be due to hot gas trapped by magnetic fields. One of these filaments is over 100,000 light years long, and extends below and to the right of the center of M87 in almost a straight line. The optical data of M87 were obtained with Hubble's Advanced Camera for Surveys in visible and infrared filters / Bridgeman Images

ID: PIX4611440

M87 elliptical galaxy in Virgo - M87 elliptical galaxy in Virgo - The M87 galaxy (NGC 4486) is 54 million years ago - light from Earth, in the heart of the Virgin's cluster. This image is a composite obtained in X-rays, radio and visible. Gas material is ejected from the heart of the galaxy. A supermassive black hole would have caused this jet. This image is a composite of visible (or optical), radio, and X - ray data of the giant elliptical galaxy, M87. M87 lies at a distance of 54 million light years and is the largest galaxy in the Virgo cluster of galaxies. Bright jets moving at close to the speed of light are seen at all wavelengths coming from the massive black hole at the center of the galaxy. It has also been identified with the strong radio source, Virgo A, and is a powerful source of X - rays as it resides near the center of a hot, X - ray emitting cloud that extends over much of the Virgo cluster. The extended radio emission consists of plumes of fast - moving gas from the j

Barclay Capital, Times Square in New York, United States.
Barclay Capital, Times Square in New York, United States.

TEC4611758: Barclay Capital, Times Square in New York, United States. / Bridgeman Images

ID: TEC4611758

Barclay Capital, Times Square in New York, United States.

Stock market indices on a building facade in Times Square in New York, USA. Photography 20/10/08.
Stock market indices on a building facade in Times Square in New York, USA. Photography 20/10/08.

TEC4611770: Stock market indices on a building facade in Times Square in New York, USA. Photography 20/10/08. / Bridgeman Images

ID: TEC4611770

Stock market indices on a building facade in Times Square in New York, USA. Photography 20/10/08.

Galaxy NGC 4631 in Hunting Dogs - Spiral galaxy NGC 4631 in Canes Venatici - Spiral galaxy seen by the slice located at a distance of 30 million years - light. Image obtained by the Hubble Space Telescope (HST). The NASA/ESA Hubble Space Telescope has peered deep into NGC 4631, better known as the Whale Galaxy. Here, a profusion of starbirth lights up the galactic centre, revealing bands of dark material between us and the starburst. The galaxy's activity tapers off in its outer regions where there are fewer stars and less dust, but these are still punctuated by pockets of star formation. The Whale Galaxy is about 30 million light - years away from us in the constellation of Canes Venatici (The Hunting Dogs) and is a spiral galaxy much like the Milky Way. From our vantage point, however, we see the Whale Galaxy edge - on, seeing its glowing centre through dusty spiral arms. The galaxy's central bulge and asymmetric tapering disc have suggested the shape of a whale or a herring to past observers. Many supernovae - - the explosions of hot, blue, short - lived stars at least eight times the mass of the Sun - - have gone off in the core of the Whale Galaxy. The stellar pyrotechnics have bathed the galaxy in hot gas, visible to X - ray telescopes like ESA's XMM - Newton. Comparing the optical and near - infrared observations from Hubble with other telescopes sensitive to different wavelengths of light helps astronomers gather the full story behind celestial phenomena. From such work, the triggers of the starburst in the Whale Galaxy and others can be elucidated. The gravitational “” feeding”” on intergalactic material, as well as clumping caused by the gravitational interactions with its galactic neighbours, creates the areas of greater density where stars start to coalesce. Just as blue whales, the biggest creatures on Earth, can gorge themselves on comparatively tiny bits of plankton, so the Whale Galaxy has become filled with the gas and dust that p
Galaxy NGC 4631 in Hunting Dogs - Spiral galaxy NGC 4631 in Canes Venatici - Spiral galaxy seen by the slice located at a distance of 30 million years - light. Image obtained by the Hubble Space Telescope (HST). The NASA/ESA Hubble Space Telescope has peered deep into NGC 4631, better known as the Whale Galaxy. Here, a profusion of starbirth lights up the galactic centre, revealing bands of dark material between us and the starburst. The galaxy's activity tapers off in its outer regions where there are fewer stars and less dust, but these are still punctuated by pockets of star formation. The Whale Galaxy is about 30 million light - years away from us in the constellation of Canes Venatici (The Hunting Dogs) and is a spiral galaxy much like the Milky Way. From our vantage point, however, we see the Whale Galaxy edge - on, seeing its glowing centre through dusty spiral arms. The galaxy's central bulge and asymmetric tapering disc have suggested the shape of a whale or a herring to past observers. Many supernovae - - the explosions of hot, blue, short - lived stars at least eight times the mass of the Sun - - have gone off in the core of the Whale Galaxy. The stellar pyrotechnics have bathed the galaxy in hot gas, visible to X - ray telescopes like ESA's XMM - Newton. Comparing the optical and near - infrared observations from Hubble with other telescopes sensitive to different wavelengths of light helps astronomers gather the full story behind celestial phenomena. From such work, the triggers of the starburst in the Whale Galaxy and others can be elucidated. The gravitational “” feeding”” on intergalactic material, as well as clumping caused by the gravitational interactions with its galactic neighbours, creates the areas of greater density where stars start to coalesce. Just as blue whales, the biggest creatures on Earth, can gorge themselves on comparatively tiny bits of plankton, so the Whale Galaxy has become filled with the gas and dust that p

PIX4611784: Galaxy NGC 4631 in Hunting Dogs - Spiral galaxy NGC 4631 in Canes Venatici - Spiral galaxy seen by the slice located at a distance of 30 million years - light. Image obtained by the Hubble Space Telescope (HST). The NASA/ESA Hubble Space Telescope has peered deep into NGC 4631, better known as the Whale Galaxy. Here, a profusion of starbirth lights up the galactic centre, revealing bands of dark material between us and the starburst. The galaxy's activity tapers off in its outer regions where there are fewer stars and less dust, but these are still punctuated by pockets of star formation. The Whale Galaxy is about 30 million light - years away from us in the constellation of Canes Venatici (The Hunting Dogs) and is a spiral galaxy much like the Milky Way. From our vantage point, however, we see the Whale Galaxy edge - on, seeing its glowing centre through dusty spiral arms. The galaxy's central bulge and asymmetric tapering disc have suggested the shape of a whale or a herring to past observers. Many supernovae - - the explosions of hot, blue, short - lived stars at least eight times the mass of the Sun - - have gone off in the core of the Whale Galaxy. The stellar pyrotechnics have bathed the galaxy in hot gas, visible to X - ray telescopes like ESA's XMM - Newton. Comparing the optical and near - infrared observations from Hubble with other telescopes sensitive to different wavelengths of light helps astronomers gather the full story behind celestial phenomena. From such work, the triggers of the starburst in the Whale Galaxy and others can be elucidated. The gravitational “” feeding”” on intergalactic material, as well as clumping caused by the gravitational interactions with its galactic neighbours, creates the areas of greater density where stars start to coalesce. Just as blue whales, the biggest creatures on Earth, can gorge themselves on comparatively tiny bits of plankton, so the Whale Galaxy has become filled with the gas and dust that p / Bridgeman Images

ID: PIX4611784

Galaxy NGC 4631 in Hunting Dogs - Spiral galaxy NGC 4631 in Canes Venatici - Spiral galaxy seen by the slice located at a distance of 30 million years - light. Image obtained by the Hubble Space Telescope (HST). The NASA/ESA Hubble Space Telescope has peered deep into NGC 4631, better known as the Whale Galaxy. Here, a profusion of starbirth lights up the galactic centre, revealing bands of dark material between us and the starburst. The galaxy's activity tapers off in its outer regions where there are fewer stars and less dust, but these are still punctuated by pockets of star formation. The Whale Galaxy is about 30 million light - years away from us in the constellation of Canes Venatici (The Hunting Dogs) and is a spiral galaxy much like the Milky Way. From our vantage point, however, we see the Whale Galaxy edge - on, seeing its glowing centre through dusty spiral arms. The galaxy's central bulge and asymmetric tapering disc have suggested the shape of a whale or a herring to past

Advertised in Times Square in New York (United States).
Advertised in Times Square in New York (United States).

TEC4611797: Advertised in Times Square in New York (United States). / Bridgeman Images

ID: TEC4611797

Advertised in Times Square in New York (United States).

Colliding galaxies NGC 4676 in Berenice's Hair - Colliding galaxies NGC 4676 - The galaxy NGC 4676 is located about 300 million years away - light from Earth. It is a system of two spiral galaxies that collide and eventually become one galaxy. Image obtained on May 31, 2008 with a telescope 61 cm in diameter. Located 300 million light - years away in the constellation Coma Berenices, the colliding galaxies have been nicknamed “” The Mice”” because of the long tails of stars and gas emanating from each galaxy. Otherwise known as NGC 4676, the pair will eventually merge into a single giant galaxy. Image taken on May 31 2008 with a 24 - inch telescope
Colliding galaxies NGC 4676 in Berenice's Hair - Colliding galaxies NGC 4676 - The galaxy NGC 4676 is located about 300 million years away - light from Earth. It is a system of two spiral galaxies that collide and eventually become one galaxy. Image obtained on May 31, 2008 with a telescope 61 cm in diameter. Located 300 million light - years away in the constellation Coma Berenices, the colliding galaxies have been nicknamed “” The Mice”” because of the long tails of stars and gas emanating from each galaxy. Otherwise known as NGC 4676, the pair will eventually merge into a single giant galaxy. Image taken on May 31 2008 with a 24 - inch telescope

PIX4611833: Colliding galaxies NGC 4676 in Berenice's Hair - Colliding galaxies NGC 4676 - The galaxy NGC 4676 is located about 300 million years away - light from Earth. It is a system of two spiral galaxies that collide and eventually become one galaxy. Image obtained on May 31, 2008 with a telescope 61 cm in diameter. Located 300 million light - years away in the constellation Coma Berenices, the colliding galaxies have been nicknamed “” The Mice”” because of the long tails of stars and gas emanating from each galaxy. Otherwise known as NGC 4676, the pair will eventually merge into a single giant galaxy. Image taken on May 31 2008 with a 24 - inch telescope / Bridgeman Images

ID: PIX4611833

Colliding galaxies NGC 4676 in Berenice's Hair - Colliding galaxies NGC 4676 - The galaxy NGC 4676 is located about 300 million years away - light from Earth. It is a system of two spiral galaxies that collide and eventually become one galaxy. Image obtained on May 31, 2008 with a telescope 61 cm in diameter. Located 300 million light - years away in the constellation Coma Berenices, the colliding galaxies have been nicknamed “” The Mice”” because of the long tails of stars and gas emanating from each galaxy. Otherwise known as NGC 4676, the pair will eventually merge into a single giant galaxy. Image taken on May 31 2008 with a 24 - inch telescope

The New York Stock Exchange in Manhattan, New Yorkæ (USA).
The New York Stock Exchange in Manhattan, New Yorkæ (USA).

TEC4611868: The New York Stock Exchange in Manhattan, New Yorkæ (USA). / Bridgeman Images

ID: TEC4611868

The New York Stock Exchange in Manhattan, New Yorkæ (USA).

Wall Street in Manhattan, New York (United States).
Wall Street in Manhattan, New York (United States).

TEC4611885: Wall Street in Manhattan, New York (United States). / Bridgeman Images

ID: TEC4611885

Wall Street in Manhattan, New York (United States).

Central Park in Manhattan, New York, United States.
Central Park in Manhattan, New York, United States.

TEC4611985: Central Park in Manhattan, New York, United States. / Bridgeman Images

ID: TEC4611985

Central Park in Manhattan, New York, United States.

Spiral galaxy NGC 4910 - Spiral galaxy NGC 4910 in the constellation Virginis. Spiral galaxy NGC 4910 in Virgo
Spiral galaxy NGC 4910 - Spiral galaxy NGC 4910 in the constellation Virginis. Spiral galaxy NGC 4910 in Virgo

PIX4612002: Spiral galaxy NGC 4910 - Spiral galaxy NGC 4910 in the constellation Virginis. Spiral galaxy NGC 4910 in Virgo / Bridgeman Images

ID: PIX4612002

Spiral galaxy NGC 4910 - Spiral galaxy NGC 4910 in the constellation Virginis. Spiral galaxy NGC 4910 in Virgo

The promenade planted on the High Line in New York (New York), United States (United States). Photography 26/09/10
The promenade planted on the High Line in New York (New York), United States (United States). Photography 26/09/10

TEC4612033: The promenade planted on the High Line in New York (New York), United States (United States). Photography 26/09/10 / Bridgeman Images

ID: TEC4612033

The promenade planted on the High Line in New York (New York), United States (United States). Photography 26/09/10

Barree spiral galaxy NGC 4945 in Centaurus - Barred spiral galaxy NGC 4945 in Centaurus - The barree spiral galaxy NGC 4945 is located about 13 million years away - light from Earth. This remarkable spiral galaxy seen almost edge - on is located at about 13 million years away in southern constellation of Centaurus. The galaxy is extremely dusty, and it is seen through dust in the Milky Way
Barree spiral galaxy NGC 4945 in Centaurus - Barred spiral galaxy NGC 4945 in Centaurus - The barree spiral galaxy NGC 4945 is located about 13 million years away - light from Earth. This remarkable spiral galaxy seen almost edge - on is located at about 13 million years away in southern constellation of Centaurus. The galaxy is extremely dusty, and it is seen through dust in the Milky Way

PIX4612037: Barree spiral galaxy NGC 4945 in Centaurus - Barred spiral galaxy NGC 4945 in Centaurus - The barree spiral galaxy NGC 4945 is located about 13 million years away - light from Earth. This remarkable spiral galaxy seen almost edge - on is located at about 13 million years away in southern constellation of Centaurus. The galaxy is extremely dusty, and it is seen through dust in the Milky Way / Bridgeman Images

ID: PIX4612037

Barree spiral galaxy NGC 4945 in Centaurus - Barred spiral galaxy NGC 4945 in Centaurus - The barree spiral galaxy NGC 4945 is located about 13 million years away - light from Earth. This remarkable spiral galaxy seen almost edge - on is located at about 13 million years away in southern constellation of Centaurus. The galaxy is extremely dusty, and it is seen through dust in the Milky Way

Vals in Switzerland.
Vals in Switzerland.

LBY4631905: Vals in Switzerland. / Bridgeman Images

ID: LBY4631905

Vals in Switzerland.

Earth on star background - North America - Earth with starry sky - North America - Image of Earth recomposed from different satellite images. A star background has been added. Composite images obtained with data collected from several satellites. A starry sky background was added
Earth on star background - North America - Earth with starry sky - North America - Image of Earth recomposed from different satellite images. A star background has been added. Composite images obtained with data collected from several satellites. A starry sky background was added

PIX4631925: Earth on star background - North America - Earth with starry sky - North America - Image of Earth recomposed from different satellite images. A star background has been added. Composite images obtained with data collected from several satellites. A starry sky background was added / Bridgeman Images

ID: PIX4631925

Earth on star background - North America - Earth with starry sky - North America - Image of Earth recomposed from different satellite images. A star background has been added. Composite images obtained with data collected from several satellites. A starry sky background was added

Earth on star background - Pole Sud - Earth with starry sky - South Pole - Image of the Earth recomposed from different satellite images. A star background has been added. Composite images obtained with data collected from several satellites. A starry sky background was added
Earth on star background - Pole Sud - Earth with starry sky - South Pole - Image of the Earth recomposed from different satellite images. A star background has been added. Composite images obtained with data collected from several satellites. A starry sky background was added

PIX4631931: Earth on star background - Pole Sud - Earth with starry sky - South Pole - Image of the Earth recomposed from different satellite images. A star background has been added. Composite images obtained with data collected from several satellites. A starry sky background was added / Bridgeman Images

ID: PIX4631931

Earth on star background - Pole Sud - Earth with starry sky - South Pole - Image of the Earth recomposed from different satellite images. A star background has been added. Composite images obtained with data collected from several satellites. A starry sky background was added

The Earth - Topographic View - Altimetric view of earth. - Bathymetric and topographic map of the Earth. Image made from radar data. The topography of the seabed was obtained from boat surveys, as well as from data obtained from ERS-1, ERS-2 and Geosat satellites. Altimetric data on the continents come from observations from the ERS-1 satellite. Color code uses: purple (- 8000m) to white (+ 3000m to+8000m); green 0 to 400 meters altitude. This global map was realized by merging a bathymetry model and the Altimetry Corrected Elevations (ACE). For the ocean, the global bathymetry was constructed by blending depth soundings collected from ships with detailed gravity anomaly information obtained from the Geosat (US Navy) and ERS - 1/2 (ESA) satellite altimetry missions. For the land elevation, database of ERS - 1 satellite altimeter were reprocessed
The Earth - Topographic View - Altimetric view of earth. - Bathymetric and topographic map of the Earth. Image made from radar data. The topography of the seabed was obtained from boat surveys, as well as from data obtained from ERS-1, ERS-2 and Geosat satellites. Altimetric data on the continents come from observations from the ERS-1 satellite. Color code uses: purple (- 8000m) to white (+ 3000m to+8000m); green 0 to 400 meters altitude. This global map was realized by merging a bathymetry model and the Altimetry Corrected Elevations (ACE). For the ocean, the global bathymetry was constructed by blending depth soundings collected from ships with detailed gravity anomaly information obtained from the Geosat (US Navy) and ERS - 1/2 (ESA) satellite altimetry missions. For the land elevation, database of ERS - 1 satellite altimeter were reprocessed

PIX4632061: The Earth - Topographic View - Altimetric view of earth. - Bathymetric and topographic map of the Earth. Image made from radar data. The topography of the seabed was obtained from boat surveys, as well as from data obtained from ERS-1, ERS-2 and Geosat satellites. Altimetric data on the continents come from observations from the ERS-1 satellite. Color code uses: purple (- 8000m) to white (+ 3000m to+8000m); green 0 to 400 meters altitude. This global map was realized by merging a bathymetry model and the Altimetry Corrected Elevations (ACE). For the ocean, the global bathymetry was constructed by blending depth soundings collected from ships with detailed gravity anomaly information obtained from the Geosat (US Navy) and ERS - 1/2 (ESA) satellite altimetry missions. For the land elevation, database of ERS - 1 satellite altimeter were reprocessed / Bridgeman Images

ID: PIX4632061

The Earth - Topographic View - Altimetric view of earth. - Bathymetric and topographic map of the Earth. Image made from radar data. The topography of the seabed was obtained from boat surveys, as well as from data obtained from ERS-1, ERS-2 and Geosat satellites. Altimetric data on the continents come from observations from the ERS-1 satellite. Color code uses: purple (- 8000m) to white (+ 3000m to+8000m); green 0 to 400 meters altitude. This global map was realized by merging a bathymetry model and the Altimetry Corrected Elevations (ACE). For the ocean, the global bathymetry was constructed by blending depth soundings collected from ships with detailed gravity anomaly information obtained from the Geosat (US Navy) and ERS - 1/2 (ESA) satellite altimetry missions. For the land elevation, database of ERS - 1 satellite altimeter were reprocessed

Evolution of the ozone hole at the southern pole from 1979 to 2004 - Ozole hole evolution - The image shows the ozone hole on the southern pole from 1979 to 2004 (except 1995) at its maximum level each year. Image based on Earth Probe - TOMS satellite data. The image shows the maximum stratospheric ozone hole over the Antarctic for years 1979 to 2004 (except 1995). Datas from Earth Probe, TOMS instrument
Evolution of the ozone hole at the southern pole from 1979 to 2004 - Ozole hole evolution - The image shows the ozone hole on the southern pole from 1979 to 2004 (except 1995) at its maximum level each year. Image based on Earth Probe - TOMS satellite data. The image shows the maximum stratospheric ozone hole over the Antarctic for years 1979 to 2004 (except 1995). Datas from Earth Probe, TOMS instrument

PIX4632155: Evolution of the ozone hole at the southern pole from 1979 to 2004 - Ozole hole evolution - The image shows the ozone hole on the southern pole from 1979 to 2004 (except 1995) at its maximum level each year. Image based on Earth Probe - TOMS satellite data. The image shows the maximum stratospheric ozone hole over the Antarctic for years 1979 to 2004 (except 1995). Datas from Earth Probe, TOMS instrument / Bridgeman Images

ID: PIX4632155

Evolution of the ozone hole at the southern pole from 1979 to 2004 - Ozole hole evolution - The image shows the ozone hole on the southern pole from 1979 to 2004 (except 1995) at its maximum level each year. Image based on Earth Probe - TOMS satellite data. The image shows the maximum stratospheric ozone hole over the Antarctic for years 1979 to 2004 (except 1995). Datas from Earth Probe, TOMS instrument

The Earth seen by Apollo 13 - Ocean Pacifiqu
The Earth seen by Apollo 13 - Ocean Pacifiqu

PIX4632214: The Earth seen by Apollo 13 - Ocean Pacifiqu / Bridgeman Images

ID: PIX4632214

The Earth seen by Apollo 13 - Ocean Pacifiqu

La Terre vue par satellite - Flying over 700 km above the Earth onboard the Terra satellite, MODIS provides an integrated tool for observing a variety of terrestrial, oceanic, and atmospheric features of the Earth. The land and coastal ocean portions of these images are based on surface observations collected from June through September 2001 and combined, or composited, every eight days to compensate for clouds that might block the sensor's view of the surface on any single day. Two different types of ocean data were used in these images: shallow water true color data, and global ocean color (or chlorophyll) data. Topographic shading is based on the GTOPO 30 elevation dataset compiled by the U.S. Geological Survey's EROS Data Center. MODIS observations of polar sea ice were combined with observations of Antarctica made by the National Oceanic and Atmospheric Administration's AVHRR sensor - - the Advanced Very High Resolution Radiometer
La Terre vue par satellite - Flying over 700 km above the Earth onboard the Terra satellite, MODIS provides an integrated tool for observing a variety of terrestrial, oceanic, and atmospheric features of the Earth. The land and coastal ocean portions of these images are based on surface observations collected from June through September 2001 and combined, or composited, every eight days to compensate for clouds that might block the sensor's view of the surface on any single day. Two different types of ocean data were used in these images: shallow water true color data, and global ocean color (or chlorophyll) data. Topographic shading is based on the GTOPO 30 elevation dataset compiled by the U.S. Geological Survey's EROS Data Center. MODIS observations of polar sea ice were combined with observations of Antarctica made by the National Oceanic and Atmospheric Administration's AVHRR sensor - - the Advanced Very High Resolution Radiometer

PIX4632280: La Terre vue par satellite - Flying over 700 km above the Earth onboard the Terra satellite, MODIS provides an integrated tool for observing a variety of terrestrial, oceanic, and atmospheric features of the Earth. The land and coastal ocean portions of these images are based on surface observations collected from June through September 2001 and combined, or composited, every eight days to compensate for clouds that might block the sensor's view of the surface on any single day. Two different types of ocean data were used in these images: shallow water true color data, and global ocean color (or chlorophyll) data. Topographic shading is based on the GTOPO 30 elevation dataset compiled by the U.S. Geological Survey's EROS Data Center. MODIS observations of polar sea ice were combined with observations of Antarctica made by the National Oceanic and Atmospheric Administration's AVHRR sensor - - the Advanced Very High Resolution Radiometer / Bridgeman Images

ID: PIX4632280

La Terre vue par satellite - Flying over 700 km above the Earth onboard the Terra satellite, MODIS provides an integrated tool for observing a variety of terrestrial, oceanic, and atmospheric features of the Earth. The land and coastal ocean portions of these images are based on surface observations collected from June through September 2001 and combined, or composited, every eight days to compensate for clouds that might block the sensor's view of the surface on any single day. Two different types of ocean data were used in these images: shallow water true color data, and global ocean color (or chlorophyll) data. Topographic shading is based on the GTOPO 30 elevation dataset compiled by the U.S. Geological Survey's EROS Data Center. MODIS observations of polar sea ice were combined with observations of Antarctica made by the National Oceanic and Atmospheric Administration's AVHRR sensor - - the Advanced Very High Resolution Radiometer

Source Cachat to Evian les Bains in Haute Savoie.
Source Cachat to Evian les Bains in Haute Savoie.

TEC4632446: Source Cachat to Evian les Bains in Haute Savoie. / Bridgeman Images

ID: TEC4632446

Source Cachat to Evian les Bains in Haute Savoie.

Primitive Land - Artist's View
Primitive Land - Artist's View

PIX4632624: Primitive Land - Artist's View / Bridgeman Images

ID: PIX4632624

Primitive Land - Artist's View

Star sky above the snow-covered Pyrenean chain - Starry sky above pyrenees - Photo taken from the observatory of the Pic du Midi. Lighting from the Moon. Pyrenees in moonlight seen from Pic du Midi observatory
Star sky above the snow-covered Pyrenean chain - Starry sky above pyrenees - Photo taken from the observatory of the Pic du Midi. Lighting from the Moon. Pyrenees in moonlight seen from Pic du Midi observatory

PIX4590955: Star sky above the snow-covered Pyrenean chain - Starry sky above pyrenees - Photo taken from the observatory of the Pic du Midi. Lighting from the Moon. Pyrenees in moonlight seen from Pic du Midi observatory / Bridgeman Images

ID: PIX4590955

Star sky above the snow-covered Pyrenean chain - Starry sky above pyrenees - Photo taken from the observatory of the Pic du Midi. Lighting from the Moon. Pyrenees in moonlight seen from Pic du Midi observatory

The Bund has Shanghai, China. Photography 21/04/05.
The Bund has Shanghai, China. Photography 21/04/05.

OMG4591253: The Bund has Shanghai, China. Photography 21/04/05. / Bridgeman Images

ID: OMG4591253

The Bund has Shanghai, China. Photography 21/04/05.

The Bund, Zhongshan andong yilu Puxi in Shanghai, China.
The Bund, Zhongshan andong yilu Puxi in Shanghai, China.

OMG4591276: The Bund, Zhongshan andong yilu Puxi in Shanghai, China. / Bridgeman Images

ID: OMG4591276

The Bund, Zhongshan andong yilu Puxi in Shanghai, China.

Walk on the Bund, Puxi to Shanghai, China. Photography 21/04/05.
Walk on the Bund, Puxi to Shanghai, China. Photography 21/04/05.

OMG4591357: Walk on the Bund, Puxi to Shanghai, China. Photography 21/04/05. / Bridgeman Images

ID: OMG4591357

Walk on the Bund, Puxi to Shanghai, China. Photography 21/04/05.

Old town district, Puxi, Shanghai, China.
Old town district, Puxi, Shanghai, China.

OMG4591390: Old town district, Puxi, Shanghai, China. / Bridgeman Images

ID: OMG4591390

Old town district, Puxi, Shanghai, China.

Spiral Galaxy M51 in Hunting Dogs - Galaxy Spiral M51 - The spiral galaxy M51 (NGC 5194) is located about 37 million years away - light from Earth. Image made with an amateur instrument, a 130 mm bezel. M51 is a wonderful bright face - on spiral galaxy located about 37 million light years away from us. It was one of the first discoveries made by Charles Messier in 1773, and it was the first galaxy where spiral structure was observed, by Lord Rosse in 1845. A faint companion galaxy, NGC 5195, seen here to the right of M51, seems to be interacting with M51. NGC 5195 shines at 9.6 magnitude and is about 5 arc minutes in diameter
Spiral Galaxy M51 in Hunting Dogs - Galaxy Spiral M51 - The spiral galaxy M51 (NGC 5194) is located about 37 million years away - light from Earth. Image made with an amateur instrument, a 130 mm bezel. M51 is a wonderful bright face - on spiral galaxy located about 37 million light years away from us. It was one of the first discoveries made by Charles Messier in 1773, and it was the first galaxy where spiral structure was observed, by Lord Rosse in 1845. A faint companion galaxy, NGC 5195, seen here to the right of M51, seems to be interacting with M51. NGC 5195 shines at 9.6 magnitude and is about 5 arc minutes in diameter

PIX4612294: Spiral Galaxy M51 in Hunting Dogs - Galaxy Spiral M51 - The spiral galaxy M51 (NGC 5194) is located about 37 million years away - light from Earth. Image made with an amateur instrument, a 130 mm bezel. M51 is a wonderful bright face - on spiral galaxy located about 37 million light years away from us. It was one of the first discoveries made by Charles Messier in 1773, and it was the first galaxy where spiral structure was observed, by Lord Rosse in 1845. A faint companion galaxy, NGC 5195, seen here to the right of M51, seems to be interacting with M51. NGC 5195 shines at 9.6 magnitude and is about 5 arc minutes in diameter / Bridgeman Images

ID: PIX4612294

Spiral Galaxy M51 in Hunting Dogs - Galaxy Spiral M51 - The spiral galaxy M51 (NGC 5194) is located about 37 million years away - light from Earth. Image made with an amateur instrument, a 130 mm bezel. M51 is a wonderful bright face - on spiral galaxy located about 37 million light years away from us. It was one of the first discoveries made by Charles Messier in 1773, and it was the first galaxy where spiral structure was observed, by Lord Rosse in 1845. A faint companion galaxy, NGC 5195, seen here to the right of M51, seems to be interacting with M51. NGC 5195 shines at 9.6 magnitude and is about 5 arc minutes in diameter


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