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Andromede and Triangle Constellations - Constellations of Andromeda and Triangulum - The constellation of Andromede begins at the brilliant star Alpheratz, or Alpha Andromedae, one of the corners of the great square of Pegase. Alpheratz is the brightest star in the picture, on the right, and is located about 97 light years away from Earth. Mirach star, in the center of the image, is a giant red star situated about 200 years ago - light. The galaxy of Andromede, M31, is visible at the top of the picture. At the bottom of the mage, in the middle, the galaxy M33. The large open cluster NGC 752 is at the bottom left. The constellations of Andromeda, the Princess, and Triangulum, the Triangle, point the way to several deep - sky delights in the fall sky. Andromeda begins at the bright star Alpheratz, or Alpha Andromedae, one of the corners of the great square of Pegasus. Alpheratz is the brightest star in the image, near the right side of the frame and is located about 97 light years away f

Andromede and Triangle Constellations - Constellations of Andromeda and Triangulum - The constellation of Andromede begins at the brilliant star Alpheratz, or Alpha Andromedae, one of the corners of the great square of Pegase. Alpheratz is the brightest star in the picture, on the right, and is located about 97 light years away from Earth. Mirach star, in the center of the image, is a giant red star situated about 200 years ago - light. The galaxy of Andromede, M31, is visible at the top of the picture. At the bottom of the mage, in the middle, the galaxy M33. The large open cluster NGC 752 is at the bottom left. The constellations of Andromeda, the Princess, and Triangulum, the Triangle, point the way to several deep - sky delights in the fall sky. Andromeda begins at the bright star Alpheratz, or Alpha Andromedae, one of the corners of the great square of Pegasus. Alpheratz is the brightest star in the image, near the right side of the frame and is located about 97 light years away f

Jerry Lodriguss

PIX4588973

Andromede and Triangle Constellations - Constellations of Andromeda and Triangulum - The constellation of Andromede begins at the brilliant star Alpheratz, or Alpha Andromedae, one of the corners of the great square of Pegase. Alpheratz is the brightest star in the picture, on the right, and is located about 97 light years away from Earth. Mirach star, in the center of the image, is a giant red star situated about 200 years ago - light. The galaxy of Andromede, M31, is visible at the top of the picture. At the bottom of the mage, in the middle, the galaxy M33. The large open cluster NGC 752 is at the bottom left. The constellations of Andromeda, the Princess, and Triangulum, the Triangle, point the way to several deep - sky delights in the fall sky. Andromeda begins at the bright star Alpheratz, or Alpha Andromedae, one of the corners of the great square of Pegasus. Alpheratz is the brightest star in the image, near the right side of the frame and is located about 97 light years away f

Andromede and Triangle Constellations - Constellations of Andromeda and Triangulum - The constellation of Andromede begins at the brilliant star Alpheratz, or Alpha Andromedae, one of the corners of the great square of Pegase. Alpheratz is the brightest star in the picture, on the right, and is located about 97 light years away from Earth. Mirach star, in the center of the image, is a giant red star situated about 200 years ago - light. The galaxy of Andromede, M31, is visible at the top of the picture. At the bottom of the mage, in the middle, the galaxy M33. The large open cluster NGC 752 is at the bottom left. The constellations of Andromeda, the Princess, and Triangulum, the Triangle, point the way to several deep - sky delights in the fall sky. Andromeda begins at the bright star Alpheratz, or Alpha Andromedae, one of the corners of the great square of Pegasus. Alpheratz is the brightest star in the image, near the right side of the frame and is located about 97 light years away f

Jerry Lodriguss

PIX4588980

Open Cluster of Pleiades - The Pleiades star cluster - The Pleiades cluster is a cluster of about 500 young stars nees 150 million years ago. Visible in the constellation Taurus, this cluster is 440 years from the Earth. The Pleiades star cluster, also known as the Seven Sisters and Messier 45, is one of the brightest and famous star clusters visible in the northern hemisphere. It consists of about 500 bright, hot, young stars that were all born at the same time between 75 and 150 million years ago within a large cloud of dust and gas. The cluster contains many stars, of which only a handful are commonly visible to the naked eye. The blue haze that accompanies them is due to very fine dust which still remains and preferentially reflects the blue light from the stars. This star cluster lie some 440 light years away from the Earth, in the constellation of Taurus

Open Cluster of Pleiades - The Pleiades star cluster - The Pleiades cluster is a cluster of about 500 young stars nees 150 million years ago. Visible in the constellation Taurus, this cluster is 440 years from the Earth. The Pleiades star cluster, also known as the Seven Sisters and Messier 45, is one of the brightest and famous star clusters visible in the northern hemisphere. It consists of about 500 bright, hot, young stars that were all born at the same time between 75 and 150 million years ago within a large cloud of dust and gas. The cluster contains many stars, of which only a handful are commonly visible to the naked eye. The blue haze that accompanies them is due to very fine dust which still remains and preferentially reflects the blue light from the stars. This star cluster lie some 440 light years away from the Earth, in the constellation of Taurus

R. Gendler

PIX4568697

Spectacles & Contact Lenses NHS gold-plated plastic rest spectacles, 1948-1960

Spectacles & Contact Lenses NHS gold-plated plastic rest spectacles, 1948-1960

UIS5083984

Oslo 19521020. The German war cemetery at Ekeberg ..., 1952 (photo)

Oslo 19521020. The German war cemetery at Ekeberg ..., 1952 (photo)

Odd Nicolaysen

NTB8681658

Oslo 19521020. The German war cemetery at Ekeberg has since 1940 been a thorn in …, 1952 (photo)

Oslo 19521020. The German war cemetery at Ekeberg has since 1940 been a thorn in …, 1952 (photo)

Odd Nicolaysen

NTB8948647

Oslo 19521020. The German war cemetery at Ekeberg has since 1940 been a thorn in …, 1952 (photo)

Oslo 19521020. The German war cemetery at Ekeberg has since 1940 been a thorn in …, 1952 (photo)

Odd Nicolaysen

NTB8946042

Centaur Omega globular cluster - The globular cluster Omega Centauri NGC 5139 - Located 17,000 years ago - light from Earth in the southern constellation of Centaur, Omega Centauri contains several million stars and is one of the oldest objects in our galaxy. To the unaided eye this glorious globular cluster has the appearance of a hazy star and was frequently confused with Halley's comet when it drifted through Centaurus in 1986. One of the richest in the Milky Way, Omega Cen contains several million stars, but unlike its southern rival, 47 Tucanae, it has a relatively open structure. Like most galactic globular clusters, the stellar population of Omega Cen identifies it as one of the oldest objects associated with the Milky Way, indeed its age is comparable to that of the Universe itself. The cluster contains a large number of RR Lyrae variable stars which enable its distance to be determined as 17,000 light years

Centaur Omega globular cluster - The globular cluster Omega Centauri NGC 5139 - Located 17,000 years ago - light from Earth in the southern constellation of Centaur, Omega Centauri contains several million stars and is one of the oldest objects in our galaxy. To the unaided eye this glorious globular cluster has the appearance of a hazy star and was frequently confused with Halley's comet when it drifted through Centaurus in 1986. One of the richest in the Milky Way, Omega Cen contains several million stars, but unlike its southern rival, 47 Tucanae, it has a relatively open structure. Like most galactic globular clusters, the stellar population of Omega Cen identifies it as one of the oldest objects associated with the Milky Way, indeed its age is comparable to that of the Universe itself. The cluster contains a large number of RR Lyrae variable stars which enable its distance to be determined as 17,000 light years

PIX4564400

USA Hometown, 1940s B&W

USA Hometown, 1940s B&W

LTT7239415

Clubs R136 in the Tarantula Nebula (NGC 2070) - Central region of the Tarantula Nebula - The Tarantula Nebula (or 30 Bream) is the largest star-forming region of the Magellan Cloud. It is located 170,000 light years ago in the constellation Dorado (southern hemisphere). In the center of this nebula, the open cluster of R136 stars (on the right), clusters of young, hot and massive stars, age barely 5 million years. Image obtained by the Hubble Space Telescope in October 2009. The Tarantula is situated 170,000 light - years away in the Large Magellanic Cloud (LMC) in the southern sky and is clearly visible to the naked eye as a large milky patch. To thr right of the image there is a huge cluster of very hot stars called R136. The stars in R136 are also among the most massive stars we know. R136 is also a very young cluster, its oldest stars being 'just' 5 million years old or so. Its smallest stars, however, are still forming. The image, taken in ultraviolet, visible, and red light by Hu

Clubs R136 in the Tarantula Nebula (NGC 2070) - Central region of the Tarantula Nebula - The Tarantula Nebula (or 30 Bream) is the largest star-forming region of the Magellan Cloud. It is located 170,000 light years ago in the constellation Dorado (southern hemisphere). In the center of this nebula, the open cluster of R136 stars (on the right), clusters of young, hot and massive stars, age barely 5 million years. Image obtained by the Hubble Space Telescope in October 2009. The Tarantula is situated 170,000 light - years away in the Large Magellanic Cloud (LMC) in the southern sky and is clearly visible to the naked eye as a large milky patch. To thr right of the image there is a huge cluster of very hot stars called R136. The stars in R136 are also among the most massive stars we know. R136 is also a very young cluster, its oldest stars being 'just' 5 million years old or so. Its smallest stars, however, are still forming. The image, taken in ultraviolet, visible, and red light by Hu

PIX4618335

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

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

Sächsische Zeitung

IMO8765817

Saxony, GDR, historical, hotel, restaurants, restaurants, cafes, Beer gardens Dresden, House Old market, View …, 1985 (photo)

Saxony, GDR, historical, hotel, restaurants, restaurants, cafes, Beer gardens Dresden, House Old market, View …, 1985 (photo)

Sächsische Zeitung

IMO8765793

The wall of the coalyard in New Bond Street, Douglas, Isle of Man, 1932-34 (b/w photo)

The wall of the coalyard in New Bond Street, Douglas, Isle of Man, 1932-34 (b/w photo)

Frowde, John James (1868-1946)

MNX5053493

Almshouse Lane, Douglas, after demolition, Isle of Man, 1932-34 (b/w photo)

Almshouse Lane, Douglas, after demolition, Isle of Man, 1932-34 (b/w photo)

Frowde, John James (1868-1946)

MNX5052347

Open cluster NGC 4755 - Jewel Box - The Jewel Box cluster, NGC 4755 - NGC 4755 is located in the constellation of the Southern Cross at a distance of 7800 years - light from Earth. The bright orange star is Kappa Crucis, a supergiant red star. This famous group of young bright stars is an open cluster some 7800 light years from the Sun. It was named the Jewel Box from its description by Sir John Herschel as 'a casket of variously coloured precious stones', which refers to its appearance in the telescope. The bright orange star is kappa Crucis, and it contrasts strongly against its predominantly blue, hot companions. Kappa Cru is a very large, (hence very luminous) quite young star in its red supergiant stage, which paradoxically indicates that its life is drawing to a close. The cluster is looks like a star to the unaided eye and appears close to the eastern - most star of the Southern Cross, so is only visible from southern latitude

Open cluster NGC 4755 - Jewel Box - The Jewel Box cluster, NGC 4755 - NGC 4755 is located in the constellation of the Southern Cross at a distance of 7800 years - light from Earth. The bright orange star is Kappa Crucis, a supergiant red star. This famous group of young bright stars is an open cluster some 7800 light years from the Sun. It was named the Jewel Box from its description by Sir John Herschel as 'a casket of variously coloured precious stones', which refers to its appearance in the telescope. The bright orange star is kappa Crucis, and it contrasts strongly against its predominantly blue, hot companions. Kappa Cru is a very large, (hence very luminous) quite young star in its red supergiant stage, which paradoxically indicates that its life is drawing to a close. The cluster is looks like a star to the unaided eye and appears close to the eastern - most star of the Southern Cross, so is only visible from southern latitude

PIX4568295

The Jungle Myna (Acridotheres fuscus), a common resident bird of Bangladesh in Mathbari, Sundarbans. People also pet them. The bird is a member of the starling family, typically found in forest and cultivation. The Jungle Myna builds a nest in hole. The normal clutch is 3-6 eggs. These 23cm long birds have grey plumage, darker on the head and wings. There are large white wing patches obvious in flight, and a white tail tip. The head has a forehead tuft. The bill and strong legs are bright yellow, and there is no bare skin around eye. Like most starlings, the Jungle Myna is fairly omnivorous, eating fruit, grain and insects. May 4, 2007. (photo)

The Jungle Myna (Acridotheres fuscus), a common resident bird of Bangladesh in Mathbari, Sundarbans. People also pet them. The bird is a member of the starling family, typically found in forest and cultivation. The Jungle Myna builds a nest in hole. The normal clutch is 3-6 eggs. These 23cm long birds have grey plumage, darker on the head and wings. There are large white wing patches obvious in flight, and a white tail tip. The head has a forehead tuft. The bill and strong legs are bright yellow, and there is no bare skin around eye. Like most starlings, the Jungle Myna is fairly omnivorous, eating fruit, grain and insects. May 4, 2007. (photo)

UIG798547

Open Cluster of Pleiades - The Pleiades star cluster - The Pleiades cluster (M45) is a cluster of about 500 young stars nees 150 million years ago. Visible in the constellation Taurus, this cluster is 440 years from the Earth. Brown dwarfs have been observed in this cluster. The Pleiades star cluster, also known as the Seven Sisters and Messier 45 (M45), is one of the brightest and famous star clusters visible in the northern hemisphere. It consists of about 500 bright, hot, young stars that were all born at the same time between 75 and 150 million years ago within a large cloud of dust and gas. The cluster contains many stars, of which only a handful are commonly visible to the naked eye. The blue haze that accompanies them is due to very fine dust which still remains and preferentially reflects the blue light from the stars. This star cluster lie some 440 light years away from the Earth, in the constellation of Taurus

Open Cluster of Pleiades - The Pleiades star cluster - The Pleiades cluster (M45) is a cluster of about 500 young stars nees 150 million years ago. Visible in the constellation Taurus, this cluster is 440 years from the Earth. Brown dwarfs have been observed in this cluster. The Pleiades star cluster, also known as the Seven Sisters and Messier 45 (M45), is one of the brightest and famous star clusters visible in the northern hemisphere. It consists of about 500 bright, hot, young stars that were all born at the same time between 75 and 150 million years ago within a large cloud of dust and gas. The cluster contains many stars, of which only a handful are commonly visible to the naked eye. The blue haze that accompanies them is due to very fine dust which still remains and preferentially reflects the blue light from the stars. This star cluster lie some 440 light years away from the Earth, in the constellation of Taurus

PIX4568835

The Jungle Myna (Acridotheres fuscus), a common resident bird of Bangladesh in Mathbari, Sundarbans. People also pet them. The bird is a member of the starling family, typically found in forest and cultivation. The Jungle Myna builds a nest in hole. The normal clutch is 3-6 eggs. These 23cm long birds have grey plumage, darker on the head and wings. There are large white wing patches obvious in flight, and a white tail tip. The head has a forehead tuft. The bill and strong legs are bright yellow, and there is no bare skin around eye. Like most starlings, the Jungle Myna is fairly omnivorous, eating fruit, grain and insects. May 4, 2007. (photo)

The Jungle Myna (Acridotheres fuscus), a common resident bird of Bangladesh in Mathbari, Sundarbans. People also pet them. The bird is a member of the starling family, typically found in forest and cultivation. The Jungle Myna builds a nest in hole. The normal clutch is 3-6 eggs. These 23cm long birds have grey plumage, darker on the head and wings. There are large white wing patches obvious in flight, and a white tail tip. The head has a forehead tuft. The bill and strong legs are bright yellow, and there is no bare skin around eye. Like most starlings, the Jungle Myna is fairly omnivorous, eating fruit, grain and insects. May 4, 2007. (photo)

UIG798546

Nebula NGC 3372 in the Carene - The Carina nebula, NGC 3372 - The Carene nebula is located about 7000 years from the Earth. It is home to many hot stars, including the star Eta Carinae in the centre of the nebula. Image obtained by Siding Spring's 3.9m telescope. The brightest part of the Milky Way, as seen by the unaided eye, lies in the southern constellation Carina. Here there are an unusually large number of young, hot stars. Their radiation is rich in energetic ultraviolet light. Many of these stars were born within the spectacular Carinae nebula, seen here. The nebula is a cloud of glowing gas composed mostly of hydrogen. It excited by ultrviolet light from the embedded stars. This dostictive emission radiation is responsible for the red colour. About a quarter of the nebula is made of helium gas, the second most abundant element in the universe after hydrogen, and all the other chemical elements account for only a few percent of the total mass. The brightest star in the nebula i

Nebula NGC 3372 in the Carene - The Carina nebula, NGC 3372 - The Carene nebula is located about 7000 years from the Earth. It is home to many hot stars, including the star Eta Carinae in the centre of the nebula. Image obtained by Siding Spring's 3.9m telescope. The brightest part of the Milky Way, as seen by the unaided eye, lies in the southern constellation Carina. Here there are an unusually large number of young, hot stars. Their radiation is rich in energetic ultraviolet light. Many of these stars were born within the spectacular Carinae nebula, seen here. The nebula is a cloud of glowing gas composed mostly of hydrogen. It excited by ultrviolet light from the embedded stars. This dostictive emission radiation is responsible for the red colour. About a quarter of the nebula is made of helium gas, the second most abundant element in the universe after hydrogen, and all the other chemical elements account for only a few percent of the total mass. The brightest star in the nebula i

PIX4618887

Spiral galaxy M33 in the Triangle - Spiral galaxy M33 in Triangulum - M33, (NGC 598), the galaxy of the Triangle, is located about 2 million years ago - light from Earth. It belongs to the local group, just like our galaxy or Andromede galaxy. Image made with an amateur instrument, a 130 mm bezel. The Pinwheel Galaxy, M33, is a very large, beautiful, face - on spiral galaxy. It is more difficult to observe at magnification than its size and magnitude would indicate under skies that are not dark because of it's fairly low surface brightness. Still, under very dark and transparent skies, M33 can be seen with the unaided eye by keen - eyed observers. Several emission nebulae inside of M33 can be seen as pink patches in this photo. The largest and most prominent emission nebula is NGC 604 which is almost 1,500 light - years in diameter. Such clouds are star factories where gas condenses under gravitational attraction and stars are born. It is one of the largest clouds of ionized hydrogen g

Spiral galaxy M33 in the Triangle - Spiral galaxy M33 in Triangulum - M33, (NGC 598), the galaxy of the Triangle, is located about 2 million years ago - light from Earth. It belongs to the local group, just like our galaxy or Andromede galaxy. Image made with an amateur instrument, a 130 mm bezel. The Pinwheel Galaxy, M33, is a very large, beautiful, face - on spiral galaxy. It is more difficult to observe at magnification than its size and magnitude would indicate under skies that are not dark because of it's fairly low surface brightness. Still, under very dark and transparent skies, M33 can be seen with the unaided eye by keen - eyed observers. Several emission nebulae inside of M33 can be seen as pink patches in this photo. The largest and most prominent emission nebula is NGC 604 which is almost 1,500 light - years in diameter. Such clouds are star factories where gas condenses under gravitational attraction and stars are born. It is one of the largest clouds of ionized hydrogen g

Jerry Lodriguss

PIX4609277

Comete 17P/Holmes 29/10/2007 - Comet 17P/Holmes October 29 2007 - View of comete 17P/Holmes and its weak hair. The faint outer coma of Comet 17P/Homes is seen here in a composite exposures on 29 October 2007. Holmes is currently located in the solar system between the orbits of Mars and Jupiter, and it moving away from the Earth since it's closest approach to the Sun at 191 million miles in May of 2007. At its closest approach to the Sun, it was still outside of the orbit of Mars. It is currently about 151 million miles from the Earth. The comet was discovered more than 100 years ago in 1892 by Edwin Holmes in London, England when it was probably undergoing a previous outburst when it became visible to the unaided eye at 4th magnitude.The reason for the outburst is unknown, but it is speculated that an internal chamber in the porous comet may have collapsed, exposing a large area of fresh ice to sunlight, causing a giant sublimation event that created the cloud around the nucleus that

Comete 17P/Holmes 29/10/2007 - Comet 17P/Holmes October 29 2007 - View of comete 17P/Holmes and its weak hair. The faint outer coma of Comet 17P/Homes is seen here in a composite exposures on 29 October 2007. Holmes is currently located in the solar system between the orbits of Mars and Jupiter, and it moving away from the Earth since it's closest approach to the Sun at 191 million miles in May of 2007. At its closest approach to the Sun, it was still outside of the orbit of Mars. It is currently about 151 million miles from the Earth. The comet was discovered more than 100 years ago in 1892 by Edwin Holmes in London, England when it was probably undergoing a previous outburst when it became visible to the unaided eye at 4th magnitude.The reason for the outburst is unknown, but it is speculated that an internal chamber in the porous comet may have collapsed, exposing a large area of fresh ice to sunlight, causing a giant sublimation event that created the cloud around the nucleus that

Jerry Lodriguss

PIX4570911

Trial Piece Worked on Both Sides, c.1391-1353 BC (limestone)

Trial Piece Worked on Both Sides, c.1391-1353 BC (limestone)

Egyptian 18th Dynasty (c.1567-1320 BC)

XCL491038

Detail of the Tarantula Nebula (NGC 2070) in the Dorado - Central region of the Tarantula Nebula - The Tarantula Nebula (or 30 Dorado) is the largest star-forming region of the Magellan Cloud. It is located 170,000 light years ago in the constellation Dorado (southern hemisphere). At the center of this nebula, the open cluster of R136 stars, clusters of young, hot and massive stars, aged just 5 million years. Mosaic of 15 images obtained by the Hubble Space Telescope. The Tarantula is situated 170,000 light - years away in the Large Magellanic Cloud (LMC) in the Southern sky and is clearly visible to the naked eye as a large milky patch. Astronomers believe that this smallish irregular galaxy is currently going through a violent period in its life. It is orbiting around the Milky Way and has had several close encounters with it. It is believed that the interaction with the Milky Way has caused an episode of energetic star formation - part of which is visible as the Tarantula Nebula. Ju

Detail of the Tarantula Nebula (NGC 2070) in the Dorado - Central region of the Tarantula Nebula - The Tarantula Nebula (or 30 Dorado) is the largest star-forming region of the Magellan Cloud. It is located 170,000 light years ago in the constellation Dorado (southern hemisphere). At the center of this nebula, the open cluster of R136 stars, clusters of young, hot and massive stars, aged just 5 million years. Mosaic of 15 images obtained by the Hubble Space Telescope. The Tarantula is situated 170,000 light - years away in the Large Magellanic Cloud (LMC) in the Southern sky and is clearly visible to the naked eye as a large milky patch. Astronomers believe that this smallish irregular galaxy is currently going through a violent period in its life. It is orbiting around the Milky Way and has had several close encounters with it. It is believed that the interaction with the Milky Way has caused an episode of energetic star formation - part of which is visible as the Tarantula Nebula. Ju

PIX4618229

Constellation Cancer - Cancer constellation - At the top right, the star Pollux des Gemeaux. Cancer (the Crab) is a rather small constellation of 506 square degrees without any bright stars, however, the stick figure above strongly hints at a crab - like shape. The ecliptic runs through the middle of the main stars, which makes it one of the 12 zodiacal constellations. It is best seen in the early evening in March. The most obvious feature in the image above is the large open cluster Messier 44, also known as Praesepe, which appears to the unaided eye as a fuzzy patch. It is easly resolved into numerous faint stars in binoculars, hence its popular name, the Beehive cluster. Although inconspicuous, the constellation gave its name to the Tropic of Cancer. In ancient times Cancer was where the Sun appeared at its maximum mid - day elevation at the time of the (northern) summer solstice. Because of the precession of the equinoxes the northern summer solstice now occurs when the Sun is in T

Constellation Cancer - Cancer constellation - At the top right, the star Pollux des Gemeaux. Cancer (the Crab) is a rather small constellation of 506 square degrees without any bright stars, however, the stick figure above strongly hints at a crab - like shape. The ecliptic runs through the middle of the main stars, which makes it one of the 12 zodiacal constellations. It is best seen in the early evening in March. The most obvious feature in the image above is the large open cluster Messier 44, also known as Praesepe, which appears to the unaided eye as a fuzzy patch. It is easly resolved into numerous faint stars in binoculars, hence its popular name, the Beehive cluster. Although inconspicuous, the constellation gave its name to the Tropic of Cancer. In ancient times Cancer was where the Sun appeared at its maximum mid - day elevation at the time of the (northern) summer solstice. Because of the precession of the equinoxes the northern summer solstice now occurs when the Sun is in T

PIX4589405

Constellation Cancer - Cancer constellation - At the top right, the star Pollux des Gemeaux. Cancer (the Crab) is a rather small constellation of 506 square degrees without any bright stars, however, the stick figure above strongly hints at a crab - like shape. The ecliptic runs through the middle of the main stars, which makes it one of the 12 zodiacal constellations. It is best seen in the early evening in March. The most obvious feature in the image above is the large open cluster Messier 44, also known as Praesepe, which appears to the unaided eye as a fuzzy patch. It is easly resolved into numerous faint stars in binoculars, hence its popular name, the Beehive cluster. Although inconspicuous, the constellation gave its name to the Tropic of Cancer. In ancient times Cancer was where the Sun appeared at its maximum mid - day elevation at the time of the (northern) summer solstice. Because of the precession of the equinoxes the northern summer solstice now occurs when the Sun is in T

Constellation Cancer - Cancer constellation - At the top right, the star Pollux des Gemeaux. Cancer (the Crab) is a rather small constellation of 506 square degrees without any bright stars, however, the stick figure above strongly hints at a crab - like shape. The ecliptic runs through the middle of the main stars, which makes it one of the 12 zodiacal constellations. It is best seen in the early evening in March. The most obvious feature in the image above is the large open cluster Messier 44, also known as Praesepe, which appears to the unaided eye as a fuzzy patch. It is easly resolved into numerous faint stars in binoculars, hence its popular name, the Beehive cluster. Although inconspicuous, the constellation gave its name to the Tropic of Cancer. In ancient times Cancer was where the Sun appeared at its maximum mid - day elevation at the time of the (northern) summer solstice. Because of the precession of the equinoxes the northern summer solstice now occurs when the Sun is in T

PIX4589441

Oslo 1954-03: Filmball at the Grand Hotel. In the middle of the snow slap and Mondays, Oslo gets the frivolous whim to want to play Hollywood for an evening and one night …, 1954 (photo)

Oslo 1954-03: Filmball at the Grand Hotel. In the middle of the snow slap and Mondays, Oslo gets the frivolous whim to want to play Hollywood for an evening and one night …, 1954 (photo)

Sverre A. Børretzen

NTB8700053

Spiral galaxy NGC 1964 in the constellation Lievre - Spiral galaxy NGC 1964 in Lepus: The galaxy NGC 1964 is located about 70 million light years away from Earth. Image obtained by the 2.2 meter MPG/ESO telescope at the La Silla Observatory. This spectacular spiral galaxy, known as NGC 1964, resides approximately 70 million light-years away in the constellation of Lepus (The Hare). NGC 1964 has a bright and dense core. In addition to containing stars, NGC 1964 lives in a star-sprinkled section of the sky. In this view from the Wide Field Imager (WFI) - an instrument mounted on the MPG/ESO 2.2-metre telescope at Eso's La Silla Observatory, Chile - the star HD 36785 can be seen to the galaxy's immediate right. Above it reside two other prominent stars named HD 36784 and TYC 5928-368-1 - and the large bright star below NGC 1964 is known as BD-22 1147. This view of NGC 1964 also contains an array of galaxies, visible in the background. The WFI is able to observe the light from these distan

Spiral galaxy NGC 1964 in the constellation Lievre - Spiral galaxy NGC 1964 in Lepus: The galaxy NGC 1964 is located about 70 million light years away from Earth. Image obtained by the 2.2 meter MPG/ESO telescope at the La Silla Observatory. This spectacular spiral galaxy, known as NGC 1964, resides approximately 70 million light-years away in the constellation of Lepus (The Hare). NGC 1964 has a bright and dense core. In addition to containing stars, NGC 1964 lives in a star-sprinkled section of the sky. In this view from the Wide Field Imager (WFI) - an instrument mounted on the MPG/ESO 2.2-metre telescope at Eso's La Silla Observatory, Chile - the star HD 36785 can be seen to the galaxy's immediate right. Above it reside two other prominent stars named HD 36784 and TYC 5928-368-1 - and the large bright star below NGC 1964 is known as BD-22 1147. This view of NGC 1964 also contains an array of galaxies, visible in the background. The WFI is able to observe the light from these distan

PIX4609997

Detail of the Tarantula nebula (NGC 2070) in the Dorado - Detail of the Tarentula nebula in Dorado - Image of a detail of the Tarantula nebula obtained in December 2001 with the WFI instrument of the ESO/MPG 2.2 telescope - m at the La Silla Observatory. The Tarantula Nebula (or 30 Dorada) is the largest star-forming region of the Great Magellan Cloud, a galaxy adjacent to ours. It is located 170,000 light years ago in the constellation Dorado (southern hemisphere). This image shows the turbulent region around the ring - shaped nebula DEM L 299 in the Large Magellanic Cloud, a satellite galaxy of the Milky Way system. It was produced by combining three monochromatic images obtained in December 2001 with the Wide - Field - Imager (WFI) at the ESO/MPG 2.2 - m telescope at the La Silla Observatory. North is up and East is left. The coloured rings seen near some of the brighter stars in the field result from light reflections in the telescope optics. The Tarantula Nebula is one of the most

Detail of the Tarantula nebula (NGC 2070) in the Dorado - Detail of the Tarentula nebula in Dorado - Image of a detail of the Tarantula nebula obtained in December 2001 with the WFI instrument of the ESO/MPG 2.2 telescope - m at the La Silla Observatory. The Tarantula Nebula (or 30 Dorada) is the largest star-forming region of the Great Magellan Cloud, a galaxy adjacent to ours. It is located 170,000 light years ago in the constellation Dorado (southern hemisphere). This image shows the turbulent region around the ring - shaped nebula DEM L 299 in the Large Magellanic Cloud, a satellite galaxy of the Milky Way system. It was produced by combining three monochromatic images obtained in December 2001 with the Wide - Field - Imager (WFI) at the ESO/MPG 2.2 - m telescope at the La Silla Observatory. North is up and East is left. The coloured rings seen near some of the brighter stars in the field result from light reflections in the telescope optics. The Tarantula Nebula is one of the most

PIX4618269

Galaxy of the Wheel of the Charette in the Sculptor - The Cartwheel Galaxy - The ring galaxy of the Wheel of the Charette is about 500 million years away - light from Earth. It is surrounded by a ring of 150,000 years - light of diameter composed of young and very bright stars (detail at the top left). This particular form is the result of a collision, probably with one of the two galaxies on the right. Bottom left, close-up on the nucleus of the galaxy. Image obtained by the Hubble Space Telescope in October 1994. A rare and spectacular head - on collision between two galaxies appears in this NASA Hubble Space Telescope true - color image of the Cartwheel Galaxy, located 500 million light - years away in the constellation Sculptor. The details of star birth resolved by Hubble provide an opportunity to study how extremely massive stars are born in large fragmented gas clouds. The striking ring - like feature is a direct result of a smaller intruder galaxy - - possibly one of two object

Galaxy of the Wheel of the Charette in the Sculptor - The Cartwheel Galaxy - The ring galaxy of the Wheel of the Charette is about 500 million years away - light from Earth. It is surrounded by a ring of 150,000 years - light of diameter composed of young and very bright stars (detail at the top left). This particular form is the result of a collision, probably with one of the two galaxies on the right. Bottom left, close-up on the nucleus of the galaxy. Image obtained by the Hubble Space Telescope in October 1994. A rare and spectacular head - on collision between two galaxies appears in this NASA Hubble Space Telescope true - color image of the Cartwheel Galaxy, located 500 million light - years away in the constellation Sculptor. The details of star birth resolved by Hubble provide an opportunity to study how extremely massive stars are born in large fragmented gas clouds. The striking ring - like feature is a direct result of a smaller intruder galaxy - - possibly one of two object

PIX4613572

Nebula of the Lagoon (M8) in Sagittarius - The Hourglass Nebula in M8, NGC 6523 - View of the Nebula of the Lagoon (M8/NGC 6523). Located in Sagittarius, at a distance of 5800 years - light, it is visible to the naked eye in good conditions. It is a star-forming region illuminated by several large O-type stars that belong to the open cluster NGC 6530 visible on the left of the image. The brightest part of the nebula is called the hourglass nebula whose gases are excited mainly by two massive supergeant stars Herschel 36 and 9 Sagittarii. At the heart of the Lagoon Nebula in Sagittarius lies the diminutive Hourglass Nebula. This extremely bright object is associated with the blue star alongside it, named Herschel 36 after its discoverer. Herschel described M8 as 'A noble nebula' and 'a fine and complicated nebula', but he was clearly intrigued by the Hourglass which he compared to the nucleus of the Andromeda nebula, M31 as 'decidedly not stellar'. The tiny bright nebula that captures H

Nebula of the Lagoon (M8) in Sagittarius - The Hourglass Nebula in M8, NGC 6523 - View of the Nebula of the Lagoon (M8/NGC 6523). Located in Sagittarius, at a distance of 5800 years - light, it is visible to the naked eye in good conditions. It is a star-forming region illuminated by several large O-type stars that belong to the open cluster NGC 6530 visible on the left of the image. The brightest part of the nebula is called the hourglass nebula whose gases are excited mainly by two massive supergeant stars Herschel 36 and 9 Sagittarii. At the heart of the Lagoon Nebula in Sagittarius lies the diminutive Hourglass Nebula. This extremely bright object is associated with the blue star alongside it, named Herschel 36 after its discoverer. Herschel described M8 as 'A noble nebula' and 'a fine and complicated nebula', but he was clearly intrigued by the Hourglass which he compared to the nucleus of the Andromeda nebula, M31 as 'decidedly not stellar'. The tiny bright nebula that captures H

Adam Block

PIX4619672

Space Exploration: Soyuz and Orion Ships - Artist's View - CEV-Soyuz Joint Mission - An American Orion ship mooring has a Soyuz TMA-M spaceship during a distant space exploration mission. Here, the ship is approaching a satellite stationed at a point in Lagrange. Illustration. An Orion class Crew Exploration Vehicle (AKA Deep Space Vehicle) is paired with a Soyuz TMA-M manned spacecraft for a joint deep space rendezvous with a satellite parked in a gravitationally stable Lagrangian point about 1 million miles beyond the orbit of the Earth's Moon. At this position, in this case a Lagrangian point 2, or L2, the Earth is between the spacecraft and the Sun resulting in the Earth eclipsing much of the Sun's light, however at this distance the Earth does not subtend an angle large enough to cover the entire disk of the Sun. What's visible of the Sun is a brilliant ring of light illuminating the spacecraft. (The streamers of light around the Sun are not the Sun's corona, but rather a way of i

Space Exploration: Soyuz and Orion Ships - Artist's View - CEV-Soyuz Joint Mission - An American Orion ship mooring has a Soyuz TMA-M spaceship during a distant space exploration mission. Here, the ship is approaching a satellite stationed at a point in Lagrange. Illustration. An Orion class Crew Exploration Vehicle (AKA Deep Space Vehicle) is paired with a Soyuz TMA-M manned spacecraft for a joint deep space rendezvous with a satellite parked in a gravitationally stable Lagrangian point about 1 million miles beyond the orbit of the Earth's Moon. At this position, in this case a Lagrangian point 2, or L2, the Earth is between the spacecraft and the Sun resulting in the Earth eclipsing much of the Sun's light, however at this distance the Earth does not subtend an angle large enough to cover the entire disk of the Sun. What's visible of the Sun is a brilliant ring of light illuminating the spacecraft. (The streamers of light around the Sun are not the Sun's corona, but rather a way of i

Walter B Myers

PIX4639150

Spiral galaxy M101 in the Great Bear - Large field - Wide field view of the Pinwheel Galaxy (M101) - The galaxy M101 (NGC 5457) is located about 27 million years away - light from Earth. It spans more than 170,000 light years, almost double the size of our galaxy. We think that of the trillion stars in it, 100 billion stars could be similar to our Sun. In this image, other galaxies are visible: NGC 5474 (below M101), NGC 5473 (just above M101), NGC 5485 (upper left), NGC 5422 (upper center) and UGC 8837 (near star 86 uA, lower left). Image obtained by the Oschin telescope of Mount Palomar through several filters and composed. Catalogued as M101, the Pinwheel is a nice face - on spiral galaxy. It lies in the northern circumpolar constellation Ursa Major (The Big Bear), at a distance of about 25 million light - years from Earth. The bright blue star at right is 86 Uma, barely visible at the naked eye from a dark site. Also visible some other nice galaxies like NGC 5474 (below under M101)

Spiral galaxy M101 in the Great Bear - Large field - Wide field view of the Pinwheel Galaxy (M101) - The galaxy M101 (NGC 5457) is located about 27 million years away - light from Earth. It spans more than 170,000 light years, almost double the size of our galaxy. We think that of the trillion stars in it, 100 billion stars could be similar to our Sun. In this image, other galaxies are visible: NGC 5474 (below M101), NGC 5473 (just above M101), NGC 5485 (upper left), NGC 5422 (upper center) and UGC 8837 (near star 86 uA, lower left). Image obtained by the Oschin telescope of Mount Palomar through several filters and composed. Catalogued as M101, the Pinwheel is a nice face - on spiral galaxy. It lies in the northern circumpolar constellation Ursa Major (The Big Bear), at a distance of about 25 million light - years from Earth. The bright blue star at right is 86 Uma, barely visible at the naked eye from a dark site. Also visible some other nice galaxies like NGC 5474 (below under M101)

D. De Martin

PIX4612725

Nebula of the Lagoon (M8) in Sagittarius - The Hourglass Nebula in M8, NGC 6523 - View of the Nebula of the Lagoon (M8/NGC 6523). Located in Sagittarius, at a distance of 5800 years - light, it is visible to the naked eye in good conditions. It is a star-forming region illuminated by several large O-type stars that belong to the open cluster NGC 6530 visible on the left of the image. The brightest part of the nebula is called the hourglass nebula whose gases are excited mainly by two massive supergeant stars Herschel 36 and 9 Sagittarii. Image made with Siding Spring's 3.9m telescope. At the heart of the Lagoon Nebula in Sagittarius lies the diminutive Hourglass Nebula. This extremely bright object is associated with the blue star alongside it, named Herschel 36 after its discoverer. Herschel described M8 as 'A noble nebula' and 'a fine and complicated nebula', but he was clearly intrigued by the Hourglass which he compared to the nucleus of the Andromeda nebula, M31 as 'decidedly not

Nebula of the Lagoon (M8) in Sagittarius - The Hourglass Nebula in M8, NGC 6523 - View of the Nebula of the Lagoon (M8/NGC 6523). Located in Sagittarius, at a distance of 5800 years - light, it is visible to the naked eye in good conditions. It is a star-forming region illuminated by several large O-type stars that belong to the open cluster NGC 6530 visible on the left of the image. The brightest part of the nebula is called the hourglass nebula whose gases are excited mainly by two massive supergeant stars Herschel 36 and 9 Sagittarii. Image made with Siding Spring's 3.9m telescope. At the heart of the Lagoon Nebula in Sagittarius lies the diminutive Hourglass Nebula. This extremely bright object is associated with the blue star alongside it, named Herschel 36 after its discoverer. Herschel described M8 as 'A noble nebula' and 'a fine and complicated nebula', but he was clearly intrigued by the Hourglass which he compared to the nucleus of the Andromeda nebula, M31 as 'decidedly not

PIX4619615

Une larme pour une goutte d'eau (Notre-Dame de Paris), 1903 (oil on canvas)

Une larme pour une goutte d'eau (Notre-Dame de Paris), 1903 (oil on canvas)

Merson, Luc-Oliver (1846-1920)

XOS8985231

The Lagoon nebula (M8) without stars - The Lagoon nebula (M8) with stars removed - In this image, the stars were removed by computer processing. Located in Sagittarius, at a distance of 5800 years - light, M8 is visible to the naked eye in good conditions. It is a star-forming region illuminated by several large O-type stars that belong to the open cluster NGC 6530 visible in the center of the image. The brightest part of the nebula is called the hourglass nebula whose gases are excited mainly by two massive supergeant stars Herschel 36 and 9 Sagittarii. M8 has at least 60 Giant B stars, 3 to 4 times more than the Orion Nebula. This image was processed to remove the stars so the incredible complex of dark and light nebulosity could more easily be seen. M8 is an amazing stellar nursery. Hot young stars that formed out of the hydrogen gas in the nebula cause it to glow in the light of ionized hydrogen at the hydrogen - alpha wavelength of 656nm. The Lagoon Nebula gets its name from the d

The Lagoon nebula (M8) without stars - The Lagoon nebula (M8) with stars removed - In this image, the stars were removed by computer processing. Located in Sagittarius, at a distance of 5800 years - light, M8 is visible to the naked eye in good conditions. It is a star-forming region illuminated by several large O-type stars that belong to the open cluster NGC 6530 visible in the center of the image. The brightest part of the nebula is called the hourglass nebula whose gases are excited mainly by two massive supergeant stars Herschel 36 and 9 Sagittarii. M8 has at least 60 Giant B stars, 3 to 4 times more than the Orion Nebula. This image was processed to remove the stars so the incredible complex of dark and light nebulosity could more easily be seen. M8 is an amazing stellar nursery. Hot young stars that formed out of the hydrogen gas in the nebula cause it to glow in the light of ionized hydrogen at the hydrogen - alpha wavelength of 656nm. The Lagoon Nebula gets its name from the d

Jerry Lodriguss

PIX4619678

(First section) A medallion, partly damaged but containing some drawing in the lower half, atop a blank panel. - a monk-like figure reclining on a grassy platform, clothed in a white hooded robe, with his left eye closed; an angel standing at his feet, bearing a platter of unidentified objects. - a monk-like figure reclining on a grassy platform, clothed in a white hooded robe, awake; an angel standing at his feet, bearing a platter containing a heart with a knife stuck in it. A speech scroll accompanies the angel; the text is partially legible: 'Collirio inunge oculus tuos vi videns'. - a scroll, bearing a largely illegible inscription (from Ashmole Roll 53: 'Est lapis occultus secreto fonte sepultus fermentu variat lapide qui conta colora'); beneath, a frog. (There is a join at this location between two sheets of paper. Comparison with Ashmole Roll 53 shows a small section is missing.) - within a ribboned section, seven roundels connected by laureal wreaths/ropes to a central red sha

(First section) A medallion, partly damaged but containing some drawing in the lower half, atop a blank panel. - a monk-like figure reclining on a grassy platform, clothed in a white hooded robe, with his left eye closed; an angel standing at his feet, bearing a platter of unidentified objects. - a monk-like figure reclining on a grassy platform, clothed in a white hooded robe, awake; an angel standing at his feet, bearing a platter containing a heart with a knife stuck in it. A speech scroll accompanies the angel; the text is partially legible: 'Collirio inunge oculus tuos vi videns'. - a scroll, bearing a largely illegible inscription (from Ashmole Roll 53: 'Est lapis occultus secreto fonte sepultus fermentu variat lapide qui conta colora'); beneath, a frog. (There is a join at this location between two sheets of paper. Comparison with Ashmole Roll 53 shows a small section is missing.) - within a ribboned section, seven roundels connected by laureal wreaths/ropes to a central red sha

BL3292691

Motion of the Star Proxima of Centauri - The proper motion of Proxima Centauri - Proxima of Centauri (in the center of the image) is the closest star to the Sun, located at a distance of 4.2 years - light. This star is a red dwarf, 10,000 times less luminous than our Sun, and is invisible to the naked eye. Its proximity makes it move quickly ahead of the other stars. This composite image made from three images taken in 1976 (blue), 1982 (red) and 1993 (green) shows the shift of the star in 17 years. Image obtained from the 1.2m Schmidt UK telescope of Siding Spring. Proxima Centauri is the nearest known star to the sun, at a distance of about 4.2 light years. It is an intrinsically faint red star, more than ten magnitudes (ten thousand times) fainter than the Sun. It is also much cooler, with a surface temperature of about 3100 C. Its visual (apparent) magnitude is eleven, so it is only visible with a good telescope, and only then from southern latitudes. Proxima is about one - tenth t

Motion of the Star Proxima of Centauri - The proper motion of Proxima Centauri - Proxima of Centauri (in the center of the image) is the closest star to the Sun, located at a distance of 4.2 years - light. This star is a red dwarf, 10,000 times less luminous than our Sun, and is invisible to the naked eye. Its proximity makes it move quickly ahead of the other stars. This composite image made from three images taken in 1976 (blue), 1982 (red) and 1993 (green) shows the shift of the star in 17 years. Image obtained from the 1.2m Schmidt UK telescope of Siding Spring. Proxima Centauri is the nearest known star to the sun, at a distance of about 4.2 light years. It is an intrinsically faint red star, more than ten magnitudes (ten thousand times) fainter than the Sun. It is also much cooler, with a surface temperature of about 3100 C. Its visual (apparent) magnitude is eleven, so it is only visible with a good telescope, and only then from southern latitudes. Proxima is about one - tenth t

PIX4571842

Seneschal Lane, Douglas, Isle of Man, 1932 (b/w photo)

Seneschal Lane, Douglas, Isle of Man, 1932 (b/w photo)

Frowde, John James (1868-1946)

MNX5052739

Close-up of a Broad-breasted Bronze Turkey

Close-up of a Broad-breasted Bronze Turkey

SSI2175699

Star field in the halo of the Andromede galaxy - Deep field image in the halo of Andromeda galaxy - Deep field in the halo of the Andromede galaxy obtained by the Hubble space telescope in 2003. 300,000 stars as well as thousands of background galaxies are visible. Astronomers using Nasa's Hubble Space Telescope (HST) have reliably measured the age of the spherical halo of stars surrounding the neighboring Andromeda galaxy (M31). To their surprise, they have discovered that approximately one - third of the stars in Andromeda's halo formed only 6 to 8 billion years ago. That's a far cry from the 11 - to - 13 billion - year age of the stars in the Milky Way's halo. Why the difference in halo ages? Apparently, M31 must have gone through a major “” corporate merger”” with another large galaxy, or a series of mergers with smaller galaxies, billions of years ago. Astronomers cannot yet tell whether this was one tumultuous event or a more continual acquisition of smaller galaxies. The newly d

Star field in the halo of the Andromede galaxy - Deep field image in the halo of Andromeda galaxy - Deep field in the halo of the Andromede galaxy obtained by the Hubble space telescope in 2003. 300,000 stars as well as thousands of background galaxies are visible. Astronomers using Nasa's Hubble Space Telescope (HST) have reliably measured the age of the spherical halo of stars surrounding the neighboring Andromeda galaxy (M31). To their surprise, they have discovered that approximately one - third of the stars in Andromeda's halo formed only 6 to 8 billion years ago. That's a far cry from the 11 - to - 13 billion - year age of the stars in the Milky Way's halo. Why the difference in halo ages? Apparently, M31 must have gone through a major “” corporate merger”” with another large galaxy, or a series of mergers with smaller galaxies, billions of years ago. Astronomers cannot yet tell whether this was one tumultuous event or a more continual acquisition of smaller galaxies. The newly d

PIX4572242

Mimas, satellite of Saturn, seen by the Cassini probe on 13/02/2010 - Saturn's moon Mimas seen by Cassini spacecraft - February 13 2010 - The Mimas satellite seen in false colours by the Cassini probe on 13 February 2010 has a distance of 16,000 km from the satellite. Color differences reveal differences in terrain nature. Mimas is about 400 km in diameter. At the right centre is the large impact crater Herschel, 130 km wide. Subtle color differences on Saturn's moon Mimas are apparent in this false - color view of Herschel Crater captured by Nasa's Cassini spacecraft during its closest - ever flyby of that moon. The image shows terrain - dependent color variations, particularly the contrast between the bluish materials in and around Herschel Crater (130 kilometers, or 80 miles, wide) and the greenish cast on older, more heavily cratered terrain elsewhere. The origin of the color differences is not yet understood, but may be caused by subtle differences in the surface composition betwe

Mimas, satellite of Saturn, seen by the Cassini probe on 13/02/2010 - Saturn's moon Mimas seen by Cassini spacecraft - February 13 2010 - The Mimas satellite seen in false colours by the Cassini probe on 13 February 2010 has a distance of 16,000 km from the satellite. Color differences reveal differences in terrain nature. Mimas is about 400 km in diameter. At the right centre is the large impact crater Herschel, 130 km wide. Subtle color differences on Saturn's moon Mimas are apparent in this false - color view of Herschel Crater captured by Nasa's Cassini spacecraft during its closest - ever flyby of that moon. The image shows terrain - dependent color variations, particularly the contrast between the bluish materials in and around Herschel Crater (130 kilometers, or 80 miles, wide) and the greenish cast on older, more heavily cratered terrain elsewhere. The origin of the color differences is not yet understood, but may be caused by subtle differences in the surface composition betwe

PIX4625563

Europe - Jupiter Satellite - View of the surface of the Europe satellite obtained from images made by the Galileo probe in 1995 and 1998. Jupiter's icy moon Europa looms large in this newly - reprocessed color view, made from images taken by Nasa's Galileo spacecraft in the late 1990s. This is the color view of Europa from Galileo that shows the largest portion of the moon's surface at the highest resolution. To create this new version, the images were assembled into a realistic color view of the surface that approximates how Europa would appear to the human eye. The scene shows the stunning diversity of Europa's surface geology. Long, linear cracks and ridges crisscross the surface, interrupted by regions of disrupted terrain where the surface ice crust has been broken up and re - frozen into new patterns. Color variations across the surface are associated with differences in geologic feature type and location. For example, areas that appear blue or white contain relatively pure water

Europe - Jupiter Satellite - View of the surface of the Europe satellite obtained from images made by the Galileo probe in 1995 and 1998. Jupiter's icy moon Europa looms large in this newly - reprocessed color view, made from images taken by Nasa's Galileo spacecraft in the late 1990s. This is the color view of Europa from Galileo that shows the largest portion of the moon's surface at the highest resolution. To create this new version, the images were assembled into a realistic color view of the surface that approximates how Europa would appear to the human eye. The scene shows the stunning diversity of Europa's surface geology. Long, linear cracks and ridges crisscross the surface, interrupted by regions of disrupted terrain where the surface ice crust has been broken up and re - frozen into new patterns. Color variations across the surface are associated with differences in geologic feature type and location. For example, areas that appear blue or white contain relatively pure water

PIX4574821

Page from Dala'il al-Khayrat (Collection of Prayers for the Prophet Muhammad), c.1660 (opaque w/c & gold on paper) (verso of 3702784)

Page from Dala'il al-Khayrat (Collection of Prayers for the Prophet Muhammad), c.1660 (opaque w/c & gold on paper) (verso of 3702784)

Indian School, (17th century)

SD3702788

Miniature Pinscher (Canis familiaris) standing, head turned to left, side view

Miniature Pinscher (Canis familiaris) standing, head turned to left, side view

UDK5444323

Royal Naval uniform: pattern 1843, c.1843 (textile)

Royal Naval uniform: pattern 1843, c.1843 (textile)

British School, (19th century)

MMM7339913

Royal Naval uniform: pattern 1843, c.1843 (textile)

Royal Naval uniform: pattern 1843, c.1843 (textile)

British School, (19th century)

MMM7339915

Royal Naval uniform: pattern 1843, c.1843 (textile)

Royal Naval uniform: pattern 1843, c.1843 (textile)

British School, (19th century)

MMM7339914

Stars cluster in the Nebula of the Eagle - Young stars in the Eagle nebula - Detail on young stars located in the cluster of stars NGC 6611 of the Nebula of the Eagle (M16). Image obtained by the Hubble Space Telescope. A spectacular section of the well - known Eagle Nebula has been targeted by the NASA/ESA Hubble Space Telescope. This collection of dazzling stars is called NGC 6611, an open star cluster that formed about 5.5 million years ago and is found approximately 6500 light - years from the Earth. It is a very young cluster, containing many hot, blue stars, whose fierce ultraviolet glow make the surrounding Eagle Nebula glow brightly. The cluster and the associated nebula together are also known as Messier 16. Astronomers refer to areas like the Eagle Nebula as HII regions. This is the scientific notation for ionised hydrogen from which the region is largely made. Extrapolating far into the future, this HII region will eventually disperse, helped along by shockwaves from superno

Stars cluster in the Nebula of the Eagle - Young stars in the Eagle nebula - Detail on young stars located in the cluster of stars NGC 6611 of the Nebula of the Eagle (M16). Image obtained by the Hubble Space Telescope. A spectacular section of the well - known Eagle Nebula has been targeted by the NASA/ESA Hubble Space Telescope. This collection of dazzling stars is called NGC 6611, an open star cluster that formed about 5.5 million years ago and is found approximately 6500 light - years from the Earth. It is a very young cluster, containing many hot, blue stars, whose fierce ultraviolet glow make the surrounding Eagle Nebula glow brightly. The cluster and the associated nebula together are also known as Messier 16. Astronomers refer to areas like the Eagle Nebula as HII regions. This is the scientific notation for ionised hydrogen from which the region is largely made. Extrapolating far into the future, this HII region will eventually disperse, helped along by shockwaves from superno

PIX4620069

Flying Star Zeta Ophiuchi - Runaway Star Zeta Ophiuchi - The blue star near the center of the image is Zeta Ophiuchi, a very massive star moving at 24 km per second. It is a “” fleeing star”, a star ejected by the explosion of his companion star. In this infrared image obtained by the WISE (Wide - field Infrared Survey Explorer) satellite, the interstellar dust traversed by the star appears, as well as an arc-shaped shock wave caused by the powerful stellar winds that the star breaks. The blue star near the center of this image is Zeta Ophiuchi. When seen in visible light it appears as a relatively dim red star surrounded by other dim stars and no dust. However, in this infrared image taken with Nasa's Wide - field Infrared Survey Explorer, or WISE, a completely different view emerges. Zeta Ophiuchi is actually a very massive, hot, bright blue star plowing its way through a large cloud of interstellar dust and gas. Astronomers theorize that this stellar juggernaut was likely once part

Flying Star Zeta Ophiuchi - Runaway Star Zeta Ophiuchi - The blue star near the center of the image is Zeta Ophiuchi, a very massive star moving at 24 km per second. It is a “” fleeing star”, a star ejected by the explosion of his companion star. In this infrared image obtained by the WISE (Wide - field Infrared Survey Explorer) satellite, the interstellar dust traversed by the star appears, as well as an arc-shaped shock wave caused by the powerful stellar winds that the star breaks. The blue star near the center of this image is Zeta Ophiuchi. When seen in visible light it appears as a relatively dim red star surrounded by other dim stars and no dust. However, in this infrared image taken with Nasa's Wide - field Infrared Survey Explorer, or WISE, a completely different view emerges. Zeta Ophiuchi is actually a very massive, hot, bright blue star plowing its way through a large cloud of interstellar dust and gas. Astronomers theorize that this stellar juggernaut was likely once part

PIX4572156

Clip from THE RIGHT MAN, 1970

Clip from THE RIGHT MAN, 1970

IWF7405551

Eyewitness News Library: April 4, 1978 7PM and 11PM

Eyewitness News Library: April 4, 1978 7PM and 11PM

MOV8614352

The Crucifix, ca. 1887 (oil on canvas)

The Crucifix, ca. 1887 (oil on canvas)

Martin, Henri Jean Guillaume (1860-1943)

XOS8982791

Cyclone Inigo, Australia, In 2003, True Colour Satellite Image. Tropical Cyclone Inigo off the coast of Western Australia on 8 April 2003. True-colour satellite image using MODIS data ©Planet Observer/UIG/Leemage

Cyclone Inigo, Australia, In 2003, True Colour Satellite Image. Tropical Cyclone Inigo off the coast of Western Australia on 8 April 2003. True-colour satellite image using MODIS data ©Planet Observer/UIG/Leemage

UIG5422065

Cyclone Larry, Australia, In 2006, True Colour Satellite Image. Tropical Cyclone Larry over the Coral Sea off the coast of Queensland, Australia, on 21 March 2006. True-colour satellite image using MODIS data ©Planet Observer/UIG/Leemage

Cyclone Larry, Australia, In 2006, True Colour Satellite Image. Tropical Cyclone Larry over the Coral Sea off the coast of Queensland, Australia, on 21 March 2006. True-colour satellite image using MODIS data ©Planet Observer/UIG/Leemage

UIG5422079

Cyclone Billy, Australia, In 2008, True Colour Satellite Image. Tropical Cyclone Billy over the Indian Ocean, off the coast of Western Australia, on 25 December 2008. True-colour satellite image using MODIS data ©Planet Observer/UIG/Leemage

Cyclone Billy, Australia, In 2008, True Colour Satellite Image. Tropical Cyclone Billy over the Indian Ocean, off the coast of Western Australia, on 25 December 2008. True-colour satellite image using MODIS data ©Planet Observer/UIG/Leemage

UIG5422071

Cyclone Hamish, Australia, In 2009, True Colour Satellite Image. Tropical Cyclone Hamish over the Coral Sea just off the coast of Queensland, Australia, on 9 March 2009. True-colour satellite image using MODIS data ©Planet Observer/UIG/Leemage

Cyclone Hamish, Australia, In 2009, True Colour Satellite Image. Tropical Cyclone Hamish over the Coral Sea just off the coast of Queensland, Australia, on 9 March 2009. True-colour satellite image using MODIS data ©Planet Observer/UIG/Leemage

UIG5422074

Bird's-Eye View of Exeter College, Oxford University (engraving)

Bird's-Eye View of Exeter College, Oxford University (engraving)

English School, (19th century)

LIP1609855

Cyclone Izilda, Madagascar, Africa, In 2009, True Colour Satellite Image. Cyclone Izilda in the Mozambique Channel off the coast of Southern Magadascar on 25 March 2009. True-colour satellite image using MODIS data ©Planet Observer/UIG/Leemage

Cyclone Izilda, Madagascar, Africa, In 2009, True Colour Satellite Image. Cyclone Izilda in the Mozambique Channel off the coast of Southern Magadascar on 25 March 2009. True-colour satellite image using MODIS data ©Planet Observer/UIG/Leemage

UIG5422081

Hurricane Andres, Mexico, In 2009, True Colour Satellite Image. Hurricane Andres on 23 June 2009 off the coast of Mexico over the Pacific ocean. True-colour satellite image using MODIS data ©Planet Observer/UIG/Leemage

Hurricane Andres, Mexico, In 2009, True Colour Satellite Image. Hurricane Andres on 23 June 2009 off the coast of Mexico over the Pacific ocean. True-colour satellite image using MODIS data ©Planet Observer/UIG/Leemage

UIG5422080

Hurricane Norbert, Pacific Ocean, In 2008, True Colour Satellite Image. Hurricane Norbert on 8 October 2008 over the Pacific ocean off Mexico. True-colour satellite image using MODIS data ©Planet Observer/UIG/Leemage

Hurricane Norbert, Pacific Ocean, In 2008, True Colour Satellite Image. Hurricane Norbert on 8 October 2008 over the Pacific ocean off Mexico. True-colour satellite image using MODIS data ©Planet Observer/UIG/Leemage

UIG5422106

Cyclone Nargis, Myanmar, In 2008, True Colour Satellite Image. Tropical Cyclone Nargis on May 1st 2008 off the coast of Burma (Myanmar). True-colour satellite image using MODIS data ©Planet Observer/UIG/Leemage

Cyclone Nargis, Myanmar, In 2008, True Colour Satellite Image. Tropical Cyclone Nargis on May 1st 2008 off the coast of Burma (Myanmar). True-colour satellite image using MODIS data ©Planet Observer/UIG/Leemage

UIG5422073

Tropical Storm Edouard, Gulf Of Mexico, In 2008, True Colour Satellite Image. Tropical storm Edouard on 4 August 2008 in the Gulf of Mexico off Louisana, US. True-colour satellite image using MODIS data ©Planet Observer/UIG/Leemage

Tropical Storm Edouard, Gulf Of Mexico, In 2008, True Colour Satellite Image. Tropical storm Edouard on 4 August 2008 in the Gulf of Mexico off Louisana, US. True-colour satellite image using MODIS data ©Planet Observer/UIG/Leemage

UIG5422114

Hurricane Hernan, Pacific Ocean, On 01/09/2002, True Colour Satellite Image. Hurricane Hernan on 1st September 2002 over the Pacific ocean, off of Baja California peninsula, Mexico (top right on the image). True-colour satellite image using MODIS data ©Planet Observer/UIG/Leemage

Hurricane Hernan, Pacific Ocean, On 01/09/2002, True Colour Satellite Image. Hurricane Hernan on 1st September 2002 over the Pacific ocean, off of Baja California peninsula, Mexico (top right on the image). True-colour satellite image using MODIS data ©Planet Observer/UIG/Leemage

UIG5422090

Hurricanes Kenneth, Jova And Max, Pacific Ocean, In 2005, True Colour Satellite Image. Satellite image of Hurricane Jova (left), Kenneth (center), and Tropical Storm Max (right) on 21 September 2005 over the Pacific ocean, off the coast of Baja California, Mexico. True-colour satellite image using MODIS data ©Planet Observer/UIG/Leemage

Hurricanes Kenneth, Jova And Max, Pacific Ocean, In 2005, True Colour Satellite Image. Satellite image of Hurricane Jova (left), Kenneth (center), and Tropical Storm Max (right) on 21 September 2005 over the Pacific ocean, off the coast of Baja California, Mexico. True-colour satellite image using MODIS data ©Planet Observer/UIG/Leemage

UIG5422105

Long, Broad, and Quick-Eye (litho)

Long, Broad, and Quick-Eye (litho)

Lavrin, Nora Fry (1897-1985)

LLM5991971

Houses of Parliament and London Eye at dusk, London, England, UK (photo)

Houses of Parliament and London Eye at dusk, London, England, UK (photo)

Charles Bowman

DSP3591862

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