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Laguna Cejar - Desert d'Atacama - Chile - Cejar Lagoon - Chile - Reflections on Laguna Cejar, a dirty water hole located about 20 km from San Pedro de Atacama. August 2014. Salar de Atacama's Cejar Lagoon is a giant sinkhole, the dark blue is actually super deep water. It has a salt concentration that ranges from 5 to 28%, producing at the higher end of the range an effect of floating like the Dead Sea

Laguna Cejar - Desert d'Atacama - Chile - Cejar Lagoon - Chile - Reflections on Laguna Cejar, a dirty water hole located about 20 km from San Pedro de Atacama. August 2014. Salar de Atacama's Cejar Lagoon is a giant sinkhole, the dark blue is actually super deep water. It has a salt concentration that ranges from 5 to 28%, producing at the higher end of the range an effect of floating like the Dead Sea

Alex Tudorica

PIX4676142

Laguna Cejar - Desert d'Atacama - Chile - Cejar Lagoon - Chile - La Laguna Cejar, a dirty water hole located about 20 km from San Pedro de Atacama. August 2014. Salar de Atacama's Cejar Lagoon is a giant sinkhole, the dark blue is actually super deep water. It has a salt concentration that ranges from 5 to 28%, producing at the higher end of the range an effect of floating like the Dead Sea

Laguna Cejar - Desert d'Atacama - Chile - Cejar Lagoon - Chile - La Laguna Cejar, a dirty water hole located about 20 km from San Pedro de Atacama. August 2014. Salar de Atacama's Cejar Lagoon is a giant sinkhole, the dark blue is actually super deep water. It has a salt concentration that ranges from 5 to 28%, producing at the higher end of the range an effect of floating like the Dead Sea

Alex Tudorica

PIX4676120

Remains of the supernova of the Sails - Detail - Vela supernova remnant. Detail - Detail of the rest of the supernova of the Sails. The supernova exploded 12,000 years ago. A supernova event marks the catastrophic end - point in the life of a massive star. The self - destruction of the star releases a huge amount of energy as radiation of all kinds, but a substantial fraction of the force of the explosion blasts the outer part of the supernova into an expanding shell of matter that travels through the almost empty space between the stars. As the rapidly moving blast wave encounters the relatively stationary interstellar medium it creates a very narrow, luminous shock front that appears as a faint nebula. Because the shock front is very convoluted the nebulosity appears to be highly structured and the various colours define different energy levels within the interaction. Although the star responsible for the Vela supernova remnant exploded 12,000 years ago, it is still affecting its env

Remains of the supernova of the Sails - Detail - Vela supernova remnant. Detail - Detail of the rest of the supernova of the Sails. The supernova exploded 12,000 years ago. A supernova event marks the catastrophic end - point in the life of a massive star. The self - destruction of the star releases a huge amount of energy as radiation of all kinds, but a substantial fraction of the force of the explosion blasts the outer part of the supernova into an expanding shell of matter that travels through the almost empty space between the stars. As the rapidly moving blast wave encounters the relatively stationary interstellar medium it creates a very narrow, luminous shock front that appears as a faint nebula. Because the shock front is very convoluted the nebulosity appears to be highly structured and the various colours define different energy levels within the interaction. Although the star responsible for the Vela supernova remnant exploded 12,000 years ago, it is still affecting its env

PIX4582820

Remains of the supernova of the Sails - Detail - Vela supernova remnant. Detail - Detail of the rest of the supernova of the Sails. The supernova exploded 12,000 years ago. A supernova event marks the catastrophic end - point in the life of a massive star. The self - destruction of the star releases a huge amount of energy as radiation of all kinds, but a substantial fraction of the force of the explosion blasts the outer part of the supernova into an expanding shell of matter that travels through the almost empty space between the stars. As the rapidly moving blast wave encounters the relatively stationary interstellar medium it creates a very narrow, luminous shock front that appears as a faint nebula. Because the shock front is very convoluted the nebulosity appears to be highly structured and the various colours define different energy levels within the interaction. Although the star responsible for the Vela supernova remnant exploded 12,000 years ago, it is still affecting its env

Remains of the supernova of the Sails - Detail - Vela supernova remnant. Detail - Detail of the rest of the supernova of the Sails. The supernova exploded 12,000 years ago. A supernova event marks the catastrophic end - point in the life of a massive star. The self - destruction of the star releases a huge amount of energy as radiation of all kinds, but a substantial fraction of the force of the explosion blasts the outer part of the supernova into an expanding shell of matter that travels through the almost empty space between the stars. As the rapidly moving blast wave encounters the relatively stationary interstellar medium it creates a very narrow, luminous shock front that appears as a faint nebula. Because the shock front is very convoluted the nebulosity appears to be highly structured and the various colours define different energy levels within the interaction. Although the star responsible for the Vela supernova remnant exploded 12,000 years ago, it is still affecting its env

PIX4582885

Planetary nebula NGC 5189 in the Fly - NGC 5189 - Planetary nebula in Musca - This nebula is located about 3000 light years from Earth in the southern constellation of Fly. Image obtained by the Gemini telescope. NGC 5189 is a planetary nebula. At the end of its life, a star with a mass less than eight times that of the Sun will blow its outer layers away, giving rise to a planetary nebula. Some of these stellar puffballs are almost round, resembling huge soap bubbles or giant planets (hence the name), but others, such as NGC 5189 are more intricate. In particular, this planetary nebula exhibits a curious S” - shaped profile, with a central bar that is most likely the projection of an inner ring of gas discharged by the star, seen edge on. The details of the physical processes producing such a complex symmetry from a simple, spherical star are still the object of astronomical controversy. One possibility is that the star has a very close (but unseen) companion. Over time the orbits dri

Planetary nebula NGC 5189 in the Fly - NGC 5189 - Planetary nebula in Musca - This nebula is located about 3000 light years from Earth in the southern constellation of Fly. Image obtained by the Gemini telescope. NGC 5189 is a planetary nebula. At the end of its life, a star with a mass less than eight times that of the Sun will blow its outer layers away, giving rise to a planetary nebula. Some of these stellar puffballs are almost round, resembling huge soap bubbles or giant planets (hence the name), but others, such as NGC 5189 are more intricate. In particular, this planetary nebula exhibits a curious S” - shaped profile, with a central bar that is most likely the projection of an inner ring of gas discharged by the star, seen edge on. The details of the physical processes producing such a complex symmetry from a simple, spherical star are still the object of astronomical controversy. One possibility is that the star has a very close (but unseen) companion. Over time the orbits dri

PIX4623091

Remains of the supernova of the Sails - Detail - Vela supernova remnant. Detail - Detail of the rest of the supernova of the Sails. The supernova exploded 12,000 years ago. The line that crosses the image is the trace left by the passage of a satellite during the photo shoot. Image obtained with Siding Spring's 3.9m telescope. A supernova event marks the catastrophic end - point in the life of a massive star. The self - destruction of the star releases a huge amount of energy as radiation of all kinds, but a substantial fraction of the force of the explosion blasts the outer part of the supernova into an expanding shell of matter that travels through the almost empty space between the stars. As the rapidly moving blast wave encounters the relatively stationary interstellar medium it creates a very narrow, luminous shock front that appears as a faint nebula. Because the shock front is very convoluted the nebulosity appears to be highly structured and the various colours define different

Remains of the supernova of the Sails - Detail - Vela supernova remnant. Detail - Detail of the rest of the supernova of the Sails. The supernova exploded 12,000 years ago. The line that crosses the image is the trace left by the passage of a satellite during the photo shoot. Image obtained with Siding Spring's 3.9m telescope. A supernova event marks the catastrophic end - point in the life of a massive star. The self - destruction of the star releases a huge amount of energy as radiation of all kinds, but a substantial fraction of the force of the explosion blasts the outer part of the supernova into an expanding shell of matter that travels through the almost empty space between the stars. As the rapidly moving blast wave encounters the relatively stationary interstellar medium it creates a very narrow, luminous shock front that appears as a faint nebula. Because the shock front is very convoluted the nebulosity appears to be highly structured and the various colours define different

PIX4582923

Open cluster M93 (NGC 2447) in Puppis - Open cluster M93 (NGC 2447) in Puppis - M93 (NGC 2447) is a cluster of age stars located 3000 years - light. Image obtained by the 3.9m telescope of Siding Spring In March, 1871 Charles Messier noted as number 93 in his famous catalogue this conspicuous group as a cluster of small stars. It was one of the last objects that Messier himself listed though he lived until 1817. The cluster is in the southern constellation of Puppis (known to Messier as Argo Puppis) and is in a rich part of the Milky Way, almost on the Galactic equator. The group is quite compact and is on the threshold of naked - eye visibility under good conditions. It is at a distance of over 3000 light years. About 80 stars have been identified as being members of the cluster, however, as in most open clusters, a mere handful contribute most of the light, reflecting the broad distribution of stellar luminosities (and thus stellar masses) found in objects of this kind. M93 is at the

Open cluster M93 (NGC 2447) in Puppis - Open cluster M93 (NGC 2447) in Puppis - M93 (NGC 2447) is a cluster of age stars located 3000 years - light. Image obtained by the 3.9m telescope of Siding Spring In March, 1871 Charles Messier noted as number 93 in his famous catalogue this conspicuous group as a cluster of small stars. It was one of the last objects that Messier himself listed though he lived until 1817. The cluster is in the southern constellation of Puppis (known to Messier as Argo Puppis) and is in a rich part of the Milky Way, almost on the Galactic equator. The group is quite compact and is on the threshold of naked - eye visibility under good conditions. It is at a distance of over 3000 light years. About 80 stars have been identified as being members of the cluster, however, as in most open clusters, a mere handful contribute most of the light, reflecting the broad distribution of stellar luminosities (and thus stellar masses) found in objects of this kind. M93 is at the

PIX4568102

Barree spiral galaxy NGC 7098 - Barred spiral galaxy NGC 7098: The barree spiral galaxy NGC 7098 is located about 95 million light years away from Earth in the southern constellation of the octant. Image obtained by the Very Large Telescope (VLT). Approximately 95 million light-years away, in the southern constellation of Octans (The Octant), lies NGC 7098 - an intriguing spiral galaxy with numerous sets of double features. The first of NGC 7098's double features is a duo of distinct ring-like structures that loop around the galaxy's hazy heart. This central region hosts a second double feature: a double bar. NGC 7098 has also developed features known as ansae, visible as small, bright streaks at each end of the central region. Ansae are visible areas of overdensity - they commonly take looping, linear, or circular shapes, and can be found at the extremities of planetary ring systems, in nebulous clouds, and, as is the case with NGC 7098, in parts of galaxies that are packed to the bri

Barree spiral galaxy NGC 7098 - Barred spiral galaxy NGC 7098: The barree spiral galaxy NGC 7098 is located about 95 million light years away from Earth in the southern constellation of the octant. Image obtained by the Very Large Telescope (VLT). Approximately 95 million light-years away, in the southern constellation of Octans (The Octant), lies NGC 7098 - an intriguing spiral galaxy with numerous sets of double features. The first of NGC 7098's double features is a duo of distinct ring-like structures that loop around the galaxy's hazy heart. This central region hosts a second double feature: a double bar. NGC 7098 has also developed features known as ansae, visible as small, bright streaks at each end of the central region. Ansae are visible areas of overdensity - they commonly take looping, linear, or circular shapes, and can be found at the extremities of planetary ring systems, in nebulous clouds, and, as is the case with NGC 7098, in parts of galaxies that are packed to the bri

PIX4574313

Queue d'étoiles - Moonset in the Warrumbungles - Photographic pose of several hours on the stars and the crescent moon. The picture here was made on one partially cloudy night at Siding Spring. In the foreground are the distinctive shapes of the Warrumbungle mountains in outback New South Wales. The exposure, on 400 ISO transparency film, was begun at the end of astronomical twilight, when the sun has descended 18 degrees below the horizon. There was a crescent moon and cloud around the south - western horizon. The exposure continued for several hours after the moon had set, and breaks in the star trails reveal that cloud had come and gone during the night

Queue d'étoiles - Moonset in the Warrumbungles - Photographic pose of several hours on the stars and the crescent moon. The picture here was made on one partially cloudy night at Siding Spring. In the foreground are the distinctive shapes of the Warrumbungle mountains in outback New South Wales. The exposure, on 400 ISO transparency film, was begun at the end of astronomical twilight, when the sun has descended 18 degrees below the horizon. There was a crescent moon and cloud around the south - western horizon. The exposure continued for several hours after the moon had set, and breaks in the star trails reveal that cloud had come and gone during the night

PIX4581124

Planetary nebula NGC 5189 in the fly - This nebula is located about 3000 light years from Earth in the southern constellation of the fly. Image obtained by the Gemini and Hubble telescopes (HST). NGC 5189 is a planetary nebula. At the end of its life, a star with a mass less than eight times that of the Sun will blow its outer layers away, giving rise to a planetary nebula. Some of these stellar puffballs are almost round, resembling huge soap bubbles or giant planets (hence the name), but others, such as NGC 5189 are more intricate. In particular, this planetary nebula exhibits a curious S” - shaped profile, with a central bar that is most likely the projection of an inner ring of gas discharged by the star, seen edge on. The details of the physical processes producing such a complex symmetry from a simple, spherical star are still the object of astronomical controversy. One possibility is that the star has a very close (but unseen) companion. Over time the orbits drift due to precess

Planetary nebula NGC 5189 in the fly - This nebula is located about 3000 light years from Earth in the southern constellation of the fly. Image obtained by the Gemini and Hubble telescopes (HST). NGC 5189 is a planetary nebula. At the end of its life, a star with a mass less than eight times that of the Sun will blow its outer layers away, giving rise to a planetary nebula. Some of these stellar puffballs are almost round, resembling huge soap bubbles or giant planets (hence the name), but others, such as NGC 5189 are more intricate. In particular, this planetary nebula exhibits a curious S” - shaped profile, with a central bar that is most likely the projection of an inner ring of gas discharged by the star, seen edge on. The details of the physical processes producing such a complex symmetry from a simple, spherical star are still the object of astronomical controversy. One possibility is that the star has a very close (but unseen) companion. Over time the orbits drift due to precess

PIX4623115

Open cluster NGC 4755 - Jewel box - The Jewel Box cluster - The NGC 4755 cluster 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 cluster contains about fifty stars formed about 14 million years ago. NGC4755 (Caldwell 94) is called the Jewel Box, based on John Herschel's comment in the 1830's that it looked like a superb piece of jewelry. There are about 50 stars in this cluster which formed some 14 million years ago. Most of the cluster members are blue giants which in a few million years will exhaust their hydrogen fuel and become red giants on their way to a cataclysmic end as supernovae. One red giant can already be seen at the center of the cluster

Open cluster NGC 4755 - Jewel box - The Jewel Box cluster - The NGC 4755 cluster 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 cluster contains about fifty stars formed about 14 million years ago. NGC4755 (Caldwell 94) is called the Jewel Box, based on John Herschel's comment in the 1830's that it looked like a superb piece of jewelry. There are about 50 stars in this cluster which formed some 14 million years ago. Most of the cluster members are blue giants which in a few million years will exhaust their hydrogen fuel and become red giants on their way to a cataclysmic end as supernovae. One red giant can already be seen at the center of the cluster

R. Gendler

PIX4568254

Old open cluster NGC 2818 and planetary nebula NGC 2818A - Old Open cluster NGC 2818 and planetary nebula in Pyxis - The open cluster NGC 2818 in the southern constellation of the Compsole is distinguished by the fact that most of its bright stars have already become supernovae; this indicates that this cluster must be very old, perhaps a billion years. It has a planetary nebula, NGC 2818A, a star at the end of life. These objects are located approximately 10,000 light years away from Earth. The open cluster NGC 2818 is not very conspicuous because most of the brilliant, massive stars that normally distinguish such groupings have vanished as supernovae, indicating that the cluster is quite mature. The massive stars dominating the scene in young clusters leaving the fainter, long - lived stars behind. Eventually, they too come to the end of their lives, throwing off their outer layers as planetary nebulae. This one, identified as NGC 2818A, is particularly graceful, and its existence su

Old open cluster NGC 2818 and planetary nebula NGC 2818A - Old Open cluster NGC 2818 and planetary nebula in Pyxis - The open cluster NGC 2818 in the southern constellation of the Compsole is distinguished by the fact that most of its bright stars have already become supernovae; this indicates that this cluster must be very old, perhaps a billion years. It has a planetary nebula, NGC 2818A, a star at the end of life. These objects are located approximately 10,000 light years away from Earth. The open cluster NGC 2818 is not very conspicuous because most of the brilliant, massive stars that normally distinguish such groupings have vanished as supernovae, indicating that the cluster is quite mature. The massive stars dominating the scene in young clusters leaving the fainter, long - lived stars behind. Eventually, they too come to the end of their lives, throwing off their outer layers as planetary nebulae. This one, identified as NGC 2818A, is particularly graceful, and its existence su

PIX4622981

Atacama Desert - Chile - Atacama desert - Chile - Star sky on the Atacama desert, between San Pedro and the Tatio geysers. August 2014. End of night above Atacama desert close to El Tatio

Atacama Desert - Chile - Atacama desert - Chile - Star sky on the Atacama desert, between San Pedro and the Tatio geysers. August 2014. End of night above Atacama desert close to El Tatio

Alex Tudorica

PIX4676149

Detail of the globular cluster 47 Toucan - Starfield in the globular cluster 47 Tucanae, NGC 104 - The globular cluster 47 Toucan (or NGC 104) is visible to the naked eye from the southern hemisphere. Located about 15000 years ago - light it contains several million stars, some of which are among the older stars known today. This image obtained by the Hubble Space Telescope shows a detail of this cluster near its center; about 35,000 stars are visible. This image shows the Hubble telescope's close - up look at a swarm of 35, 000 stars near the club's central region. The stars are tightly packed together: They are much closer together than our Sun and its closest stars. The picture, taken by the Wide Field and Planetary Camera 2, depicts the stars' natural colors and tells scientists about their composition and age. For example, the red stars denote bright red giants nearing the end of their lives; the more common yellow stars are similar to our middle - aged Sun

Detail of the globular cluster 47 Toucan - Starfield in the globular cluster 47 Tucanae, NGC 104 - The globular cluster 47 Toucan (or NGC 104) is visible to the naked eye from the southern hemisphere. Located about 15000 years ago - light it contains several million stars, some of which are among the older stars known today. This image obtained by the Hubble Space Telescope shows a detail of this cluster near its center; about 35,000 stars are visible. This image shows the Hubble telescope's close - up look at a swarm of 35, 000 stars near the club's central region. The stars are tightly packed together: They are much closer together than our Sun and its closest stars. The picture, taken by the Wide Field and Planetary Camera 2, depicts the stars' natural colors and tells scientists about their composition and age. For example, the red stars denote bright red giants nearing the end of their lives; the more common yellow stars are similar to our middle - aged Sun

PIX4564266

Stars in the globular cluster Omega Centauri - Omega Centauri seen by Hubble space telescope - Located 16,000 years ago - light from Earth in the southern constellation of Centaur, Omega Centauri contains several million stars and is one of the most ancient objects in our galaxy. This image obtained by the Hubble Space Telescope in July 2009 shows only a small part of this cluster, where 100,000 stars are visible. Hubble Space Telescope snapped this panoramic view of a colorful assortment of 100,000 stars residing in the crowded core of a giant star cluster. The image reveals a small region inside the massive globular cluster Omega Centauri, which boasts nearly 10 million stars. The stars in Omega Centauri are between 10 billion and 12 billion years old. The cluster lies about 16,000 light - years from Earth. This is one of the first images taken by the new Wide Field Camera 3 (WFC3), installed aboard Hubble in May 2009, during Servicing Mission 4. The majority of the stars in the imag

Stars in the globular cluster Omega Centauri - Omega Centauri seen by Hubble space telescope - Located 16,000 years ago - light from Earth in the southern constellation of Centaur, Omega Centauri contains several million stars and is one of the most ancient objects in our galaxy. This image obtained by the Hubble Space Telescope in July 2009 shows only a small part of this cluster, where 100,000 stars are visible. Hubble Space Telescope snapped this panoramic view of a colorful assortment of 100,000 stars residing in the crowded core of a giant star cluster. The image reveals a small region inside the massive globular cluster Omega Centauri, which boasts nearly 10 million stars. The stars in Omega Centauri are between 10 billion and 12 billion years old. The cluster lies about 16,000 light - years from Earth. This is one of the first images taken by the new Wide Field Camera 3 (WFC3), installed aboard Hubble in May 2009, during Servicing Mission 4. The majority of the stars in the imag

PIX4564450

The Large Magellanic Cloud - The Large Magellanic Cloud - The Great Magellan Cloud galaxy is located about 160,000 light years away from Earth in the southern constellation of Dorado. Visible with the naked eye in the southern hemishere it is one of the closest galaxies to us. It contains large star-forming zones such as the Tarantula Nebula (30 Sea bream, visible to the left), the most active star-forming regions of the local group. Image obtained by the 1.2m UK Schmidt telescope from Siding Spring, Australia. The Large Magellanic Cloud (LMC) is the nearest galaxy to the Milky Way but less than one tenth as massive; even so it contains the equivalent of over ten billion solar masses of material in the form of stars, gas and dust. The LMC is at a distance of 160,000 light years and is visible to the unaided eye from southern latitudes, rather like a detached piece of the Milky Way. The nearness of the LMC ensures that it is well resolved into stars in quite a modest telescope, and deep

The Large Magellanic Cloud - The Large Magellanic Cloud - The Great Magellan Cloud galaxy is located about 160,000 light years away from Earth in the southern constellation of Dorado. Visible with the naked eye in the southern hemishere it is one of the closest galaxies to us. It contains large star-forming zones such as the Tarantula Nebula (30 Sea bream, visible to the left), the most active star-forming regions of the local group. Image obtained by the 1.2m UK Schmidt telescope from Siding Spring, Australia. The Large Magellanic Cloud (LMC) is the nearest galaxy to the Milky Way but less than one tenth as massive; even so it contains the equivalent of over ten billion solar masses of material in the form of stars, gas and dust. The LMC is at a distance of 160,000 light years and is visible to the unaided eye from southern latitudes, rather like a detached piece of the Milky Way. The nearness of the LMC ensures that it is well resolved into stars in quite a modest telescope, and deep

PIX4613427

Irregular Galaxy IC 5152 in the Indian - A nearby galaxy, IC 5152 - IC 5152 is an irregular galaxy located about 5.8 million years ago - light. In the foreground, a star in our galaxy of 8th magnitude. Image made in 1982 with the 3.9m telescope of Siding Spring. This small blue galaxy is resolved into stars in this deep AAT picture, which means that it is relatively nearby. However despite its proximity, it is probably just beyond the Local Group, which is a loose collection of 30 or so galaxies within 2 or 3 million light years of the Milky Way. Apart from the Milky Way and the similarly massive M31 galaxy in Andromeda, most of our immediate extra - galactic neighbours are light - weight collections of stars and gas like IC 5152, though few (except the Large Magellanic Cloud) show such strong evidence of recent star formation The bright object which appears at the eastern end of the galaxy is an 8th magnitude blue star in the Milky Way

Irregular Galaxy IC 5152 in the Indian - A nearby galaxy, IC 5152 - IC 5152 is an irregular galaxy located about 5.8 million years ago - light. In the foreground, a star in our galaxy of 8th magnitude. Image made in 1982 with the 3.9m telescope of Siding Spring. This small blue galaxy is resolved into stars in this deep AAT picture, which means that it is relatively nearby. However despite its proximity, it is probably just beyond the Local Group, which is a loose collection of 30 or so galaxies within 2 or 3 million light years of the Milky Way. Apart from the Milky Way and the similarly massive M31 galaxy in Andromeda, most of our immediate extra - galactic neighbours are light - weight collections of stars and gas like IC 5152, though few (except the Large Magellanic Cloud) show such strong evidence of recent star formation The bright object which appears at the eastern end of the galaxy is an 8th magnitude blue star in the Milky Way

PIX4613299

Tarantula Nebula and Supernova 1987A - The Tarantula Nebula and supernova 1987a in the LMC - Tarantula Nebula photographed in 1987, two weeks after the appearance of the 1987A supernova. Image obtained with Siding Spring's 3.9m telescope. Supernova 1987A appeared in the constellation Doradus on February 23, 1987. The brightest star in this picture is the first supernova to be visible to the unaided eye for almost 400 years. It occured in a region rich in young, blue stars and it was one of these which destroyed itself. When this picture was taken, about 2 weeks after the supernova was discovered, at the end of February, 1987, the expanding shell of material had already changed from blue to orange - red as it cooled. The location of the supernova in the Large Magellanic Cloud (LMC) means that it can only be seen from the southern hemisphere

Tarantula Nebula and Supernova 1987A - The Tarantula Nebula and supernova 1987a in the LMC - Tarantula Nebula photographed in 1987, two weeks after the appearance of the 1987A supernova. Image obtained with Siding Spring's 3.9m telescope. Supernova 1987A appeared in the constellation Doradus on February 23, 1987. The brightest star in this picture is the first supernova to be visible to the unaided eye for almost 400 years. It occured in a region rich in young, blue stars and it was one of these which destroyed itself. When this picture was taken, about 2 weeks after the supernova was discovered, at the end of February, 1987, the expanding shell of material had already changed from blue to orange - red as it cooled. The location of the supernova in the Large Magellanic Cloud (LMC) means that it can only be seen from the southern hemisphere

PIX4582389

Around the Tarantula Nebula - Around the Tarantula nebula in the Large Magellanic Cloud - The Tarantula Nebula (or 30 Bream) is the largest star-forming region of the Great 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 hot and massive stars. Image obtained with the 1.2m Schmidt UK Telescope from Siding Spring. In this picture we see the eastern end of the Large Magellanic Cloud where lies one of the most active star formation regions known. If this enormous complex of stars, gas and dust were at the distance of the better - known Orion Nebula the brightest parts of it would visible during the day and would cover a quarter of the sky at night. While the Orion Nebula contains a mere handful of the hot blue stars which energise it, the Tarantula nebula has spawned many thousands in the bright central region, which surrounds a compact, brilliant cluster known

Around the Tarantula Nebula - Around the Tarantula nebula in the Large Magellanic Cloud - The Tarantula Nebula (or 30 Bream) is the largest star-forming region of the Great 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 hot and massive stars. Image obtained with the 1.2m Schmidt UK Telescope from Siding Spring. In this picture we see the eastern end of the Large Magellanic Cloud where lies one of the most active star formation regions known. If this enormous complex of stars, gas and dust were at the distance of the better - known Orion Nebula the brightest parts of it would visible during the day and would cover a quarter of the sky at night. While the Orion Nebula contains a mere handful of the hot blue stars which energise it, the Tarantula nebula has spawned many thousands in the bright central region, which surrounds a compact, brilliant cluster known

PIX4618257

Pedestrian area; Karlstor gate; western end of the Neuhauser Strasse street with view of Stachus square; Karlsplatz square; through the arch; old town; city centre; Munich; Upper Bavaria; Germany; Europe

Pedestrian area; Karlstor gate; western end of the Neuhauser Strasse street with view of Stachus square; Karlsplatz square; through the arch; old town; city centre; Munich; Upper Bavaria; Germany; Europe

Stefan Auth

IMB4894857

Tarantula Nebula (NGC 2070) in the river bream - The Tarantula Nebula, around the 30 Dor cluster - The Tarantula Nebula (or 30 Bream) is the largest star-forming region of the Great 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 hot and massive stars. Image obtained with Siding Spring's 3.9m telescope. This object is the only extra - galactic nebula which can be seen with the unaided eye. It is a faint patch of light at the eastern end of the Large Magellanic Cloud, 170,000 light years distant. A small telescope reveals narrow spindly tendrils of glowing gas which have been likened to the legs of a spider. The 'body' of the spider is the bright nebula seen at the centre of the photograph, while at its core is an extremely dense clump of very hot stars, until recently thought to a single, unusually massive star known as 30 Doradus. The very hot stars of 30

Tarantula Nebula (NGC 2070) in the river bream - The Tarantula Nebula, around the 30 Dor cluster - The Tarantula Nebula (or 30 Bream) is the largest star-forming region of the Great 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 hot and massive stars. Image obtained with Siding Spring's 3.9m telescope. This object is the only extra - galactic nebula which can be seen with the unaided eye. It is a faint patch of light at the eastern end of the Large Magellanic Cloud, 170,000 light years distant. A small telescope reveals narrow spindly tendrils of glowing gas which have been likened to the legs of a spider. The 'body' of the spider is the bright nebula seen at the centre of the photograph, while at its core is an extremely dense clump of very hot stars, until recently thought to a single, unusually massive star known as 30 Doradus. The very hot stars of 30

PIX4618255

Open cluster NGC 4755 - Jewel Box - The Jewel Box star cluster - The NGC 4755 cluster is located in the constellation of the Southern Cross at a distance of 6400 years - light from Earth. The bright orange star on the top right is Kappa Crucis, a supergiant red star. This cluster contains about fifty stars formed about 16 million years ago. This close-up of the center of the cluster was obtained with the Hubble Space Telescope. This image is a “” close - up 'view from the NASA/ESA Hubble Space Telescope of NGC 4755, or the Jewel Box cluster. Several very bright, pale blue supergiant stars, a solitary ruby - red supergiant and a variety of other brilliantly coloured stars are visible in the image, as well as many much fainter ones, often with intriguing colours. The huge variety in brightness exists because the brighter stars are 15 to 20 times the mass of the Sun, while the dimmest stars are less than half the mass of the Sun. This is the first image of an open galactic cluster with im

Open cluster NGC 4755 - Jewel Box - The Jewel Box star cluster - The NGC 4755 cluster is located in the constellation of the Southern Cross at a distance of 6400 years - light from Earth. The bright orange star on the top right is Kappa Crucis, a supergiant red star. This cluster contains about fifty stars formed about 16 million years ago. This close-up of the center of the cluster was obtained with the Hubble Space Telescope. This image is a “” close - up 'view from the NASA/ESA Hubble Space Telescope of NGC 4755, or the Jewel Box cluster. Several very bright, pale blue supergiant stars, a solitary ruby - red supergiant and a variety of other brilliantly coloured stars are visible in the image, as well as many much fainter ones, often with intriguing colours. The huge variety in brightness exists because the brighter stars are 15 to 20 times the mass of the Sun, while the dimmest stars are less than half the mass of the Sun. This is the first image of an open galactic cluster with im

PIX4568246

Detail of the nebula NGC 3603 in the Carene - Star life cycle in NGC 3603 - In the center of the picture is a cluster of massive young stars formed from the gas surrounding them. Two pillars of gas and dust visible on the right at the top and bottom will one day form other stars, as probably the dark cloud at the top right of the image called Bok's globule. Above the left of the star cluster, an old blue supergiant star, Sher 25, arrives at the end of life. The nebula NGC 3603 is located approximately 20,000 light years from Earth in the southern constellation of Carene. Image obtained by the Hubble Space Telescope. This image made by the Hubble space telescope nicely illustrates the entire stellar life cycle of stars, starting with the Bok globules (dark clouds at the upper right) and giant gaseous pillars, followed by circumstellar disks and progressing to evolved massive stars in the young starburst cluster (center). The blue supergiant star Sher 25 with its ring and bipolar outflow

Detail of the nebula NGC 3603 in the Carene - Star life cycle in NGC 3603 - In the center of the picture is a cluster of massive young stars formed from the gas surrounding them. Two pillars of gas and dust visible on the right at the top and bottom will one day form other stars, as probably the dark cloud at the top right of the image called Bok's globule. Above the left of the star cluster, an old blue supergiant star, Sher 25, arrives at the end of life. The nebula NGC 3603 is located approximately 20,000 light years from Earth in the southern constellation of Carene. Image obtained by the Hubble Space Telescope. This image made by the Hubble space telescope nicely illustrates the entire stellar life cycle of stars, starting with the Bok globules (dark clouds at the upper right) and giant gaseous pillars, followed by circumstellar disks and progressing to evolved massive stars in the young starburst cluster (center). The blue supergiant star Sher 25 with its ring and bipolar outflow

PIX4619146

Constellation of Eridan - Constellation of Eridanus - View from the Hyadas to the Hydra Male. In the center is the great constellation of Eridan. The brightest stars visible here are Rigel, Sirius, Canopus and Achernar. In the center of image is the Eridanus constellation. Brightest stars visible are Rigel (top in Orion); Sirius (top left); Canopus (below) and Achernar (bottom center). Eridanus (the Celestial River) is very well named; since it winds its way over an enormous area of the sky. It is the 6th largest constellation (almost 1140 square degrees) and wanders over a huge range of Declination. The river runs from close to the celestial equator (which runs through Orion's Belt) to its brightest star Achernar (a Eri; from the English for 'river's end'); which is at 57* south declination

Constellation of Eridan - Constellation of Eridanus - View from the Hyadas to the Hydra Male. In the center is the great constellation of Eridan. The brightest stars visible here are Rigel, Sirius, Canopus and Achernar. In the center of image is the Eridanus constellation. Brightest stars visible are Rigel (top in Orion); Sirius (top left); Canopus (below) and Achernar (bottom center). Eridanus (the Celestial River) is very well named; since it winds its way over an enormous area of the sky. It is the 6th largest constellation (almost 1140 square degrees) and wanders over a huge range of Declination. The river runs from close to the celestial equator (which runs through Orion's Belt) to its brightest star Achernar (a Eri; from the English for 'river's end'); which is at 57* south declination

PIX4590607

Constellation of Eridan - Constellation of Eridanus - View from the Hyadas to the Hydra Male. In the center is the great constellation of Eridan. The brightest stars visible here are Rigel, Sirius, Canopus and Achernar. In the center of image is the Eridanus constellation. Brightest stars visible are Rigel (top in Orion); Sirius (top left); Canopus (below) and Achernar (bottom center). Eridanus (the Celestial River) is very well named; since it winds its way over an enormous area of the sky. It is the 6th largest constellation (almost 1140 square degrees) and wanders over a huge range of Declination. The river runs from close to the celestial equator (which runs through Orion's Belt) to its brightest star Achernar (a Eri; from the English for 'river's end'); which is at 57* south declination

Constellation of Eridan - Constellation of Eridanus - View from the Hyadas to the Hydra Male. In the center is the great constellation of Eridan. The brightest stars visible here are Rigel, Sirius, Canopus and Achernar. In the center of image is the Eridanus constellation. Brightest stars visible are Rigel (top in Orion); Sirius (top left); Canopus (below) and Achernar (bottom center). Eridanus (the Celestial River) is very well named; since it winds its way over an enormous area of the sky. It is the 6th largest constellation (almost 1140 square degrees) and wanders over a huge range of Declination. The river runs from close to the celestial equator (which runs through Orion's Belt) to its brightest star Achernar (a Eri; from the English for 'river's end'); which is at 57* south declination

PIX4590625

South Carolina: The South in 1880 East Battery the Promenade on the Southern End of East Bay Street. Charleston

South Carolina: The South in 1880 East Battery the Promenade on the Southern End of East Bay Street. Charleston

LZT1034718

Star Chart made and published by C. Allard, Amsterdam

Star Chart made and published by C. Allard, Amsterdam

XLF3786738

Anatomical cuirass breast plate, end 4th century BC (bronze lamina)

Anatomical cuirass breast plate, end 4th century BC (bronze lamina)

Greek school, (4th century BC)

Luisa Ricciarini

LRI4686946

Posterior part of a double armor. End of 4th century BC (bronze)

Posterior part of a double armor. End of 4th century BC (bronze)

Greek school, (4th century BC)

Luisa Ricciarini

LRI4686918

Jun 06, 1954 - MOTHER OF TWO BIDS FOR ATHLETICS TITLE. Mrs. Iris Pond, Southern Countries and Middlesex champion and International Hurdler, is competing at the Women's A.A.A. meeting at the White City on Saturday. Apart from her ordinary training on the track at Alperton, Iris has the assistance of her two sons, Barry, aged 6 and Anthony, aged 8. at her home at Uxbridge when it was discovered that, when sitting on two bricks, Barry exactly measured up to the regulation hurdle height of 2 feet six inches. The yard broom with Anthony at the other end - completed the obstacle

Jun 06, 1954 - MOTHER OF TWO BIDS FOR ATHLETICS TITLE. Mrs. Iris Pond, Southern Countries and Middlesex champion and International Hurdler, is competing at the Women's A.A.A. meeting at the White City on Saturday. Apart from her ordinary training on the track at Alperton, Iris has the assistance of her two sons, Barry, aged 6 and Anthony, aged 8. at her home at Uxbridge when it was discovered that, when sitting on two bricks, Barry exactly measured up to the regulation hurdle height of 2 feet six inches. The yard broom with Anthony at the other end - completed the obstacle

ZUM4935941

Capture of the town of Seringapatam (or Srirangapatna), capital of Mysore (Maissour) in India by the British army commanded by the Duke Arthur Wellesley of Wellington (1769-1852) in 1799. This event marked the end of the Anglo-mysore war and the domination of the English in southern India. Srirangapatna (Seringapatam), the chief city of Mysore, India, was captured by the British army commanded by the Duke of Wellington in 1799. The battle and the death of Tipu Sultan marked the end of the Fourth Anglo-Mysore War and the confirmation of British domination of southern India.

Capture of the town of Seringapatam (or Srirangapatna), capital of Mysore (Maissour) in India by the British army commanded by the Duke Arthur Wellesley of Wellington (1769-1852) in 1799. This event marked the end of the Anglo-mysore war and the domination of the English in southern India. Srirangapatna (Seringapatam), the chief city of Mysore, India, was captured by the British army commanded by the Duke of Wellington in 1799. The battle and the death of Tipu Sultan marked the end of the Fourth Anglo-Mysore War and the confirmation of British domination of southern India.

English School, (19th century)

Stefano Bianchetti

XEE4188390

Earth view from space: California and Mexico - Northwest Mexico and Southern California seen from space - View extending from southern California with dirty Lake Salton Sea at the bottom of the image, at the southern tip of Baja California in Mexico. Image obtained from Shuttle Columbia in June 1991. Rugged mountains along the spine of Baja California, the deep blue water of the Gulf of California (also known as the Sea of Cortez), and the deserts of northwestern Mexico and southern California highlight this photograph. This southerly view provides an excellent panorama extending from the Salton Sea in the Imperial Valley of southern California almost to the southern tip of Baja California. Human imprint on this landscape is primarily found along the rivers and their floodplains, where intensive irrigated agriculture exists. The Colorado River, with its cultivated field patterns (darker areas), can be seen to flow from the north toward the southwest and finally to empty into the broad

Earth view from space: California and Mexico - Northwest Mexico and Southern California seen from space - View extending from southern California with dirty Lake Salton Sea at the bottom of the image, at the southern tip of Baja California in Mexico. Image obtained from Shuttle Columbia in June 1991. Rugged mountains along the spine of Baja California, the deep blue water of the Gulf of California (also known as the Sea of Cortez), and the deserts of northwestern Mexico and southern California highlight this photograph. This southerly view provides an excellent panorama extending from the Salton Sea in the Imperial Valley of southern California almost to the southern tip of Baja California. Human imprint on this landscape is primarily found along the rivers and their floodplains, where intensive irrigated agriculture exists. The Colorado River, with its cultivated field patterns (darker areas), can be seen to flow from the north toward the southwest and finally to empty into the broad

PIX4673252

Shikotan island seen from space - Shikotan island seen from space - Shikotan island (Shikotan) is one of the largest islands of the Kuril archipelago, located in the Pacific Ocean between the Kamchatka Peninsula and northern Japan. In this image obtained by the EO-1 satellite on 14 February 2011, this volcanic island is surrounded by ice forming spirals in the wind. Ostrov Shikotan (or Shikotan - to) is a volcanic island at the southern end of the Kuril chain. Shikotan lies along the extreme southern edge of winter sea ice in the Northern Hemisphere. The Advanced Land Imager (ALI) on NASA's Earth Observing - 1 (EO - 1) satellite captured this natural - color image of Shikotan on February 14, 2011. The island is surrounded by sea ice - - swirling shapes of ghostly blue - gray. The ice in this image may have formed in a matter of several days, and it is prone to moving with currents. North of the western end of Shikotan, eddies have shaped the ice into rough circles. The eddies may resul

Shikotan island seen from space - Shikotan island seen from space - Shikotan island (Shikotan) is one of the largest islands of the Kuril archipelago, located in the Pacific Ocean between the Kamchatka Peninsula and northern Japan. In this image obtained by the EO-1 satellite on 14 February 2011, this volcanic island is surrounded by ice forming spirals in the wind. Ostrov Shikotan (or Shikotan - to) is a volcanic island at the southern end of the Kuril chain. Shikotan lies along the extreme southern edge of winter sea ice in the Northern Hemisphere. The Advanced Land Imager (ALI) on NASA's Earth Observing - 1 (EO - 1) satellite captured this natural - color image of Shikotan on February 14, 2011. The island is surrounded by sea ice - - swirling shapes of ghostly blue - gray. The ice in this image may have formed in a matter of several days, and it is prone to moving with currents. North of the western end of Shikotan, eddies have shaped the ice into rough circles. The eddies may resul

PIX4661440

Mulaku and Felidhu Atoll - Maldives, Image taken from the space shuttle Atlantis in january 1997

Mulaku and Felidhu Atoll - Maldives, Image taken from the space shuttle Atlantis in january 1997

PIX4661056

Onekotan volcanic island seen from space - Onekotan volcanic island seen from space - Onekotan Island is an uninhabited volcanic island north of the Kuril Islands chain (Russia). About 40 kilometres long, this island is home to two stratovolcanoes, on the right (north), the Nemo volcano, on the left (south), the Krenitsyn volcano with the caldera Tao - Rusyr. Image obtained from the International Space Station (ISS) on January 9, 2011. Snow cover highlights the calderas and volcanic cones that form the northern and southern ends of Onekotan Island, part of the Russian Federation in the western Pacific Ocean. Calderas are depressions formed when a volcano empties its magma chamber in an explosive eruption and then the overlaying material collapses into the evacuated space. In this astronaut photograph taken from the International Space Station (ISS) on January 9, 2011, the northern end of the island (image right) is dominated by the Nemo Peak volcano, which began forming within an older

Onekotan volcanic island seen from space - Onekotan volcanic island seen from space - Onekotan Island is an uninhabited volcanic island north of the Kuril Islands chain (Russia). About 40 kilometres long, this island is home to two stratovolcanoes, on the right (north), the Nemo volcano, on the left (south), the Krenitsyn volcano with the caldera Tao - Rusyr. Image obtained from the International Space Station (ISS) on January 9, 2011. Snow cover highlights the calderas and volcanic cones that form the northern and southern ends of Onekotan Island, part of the Russian Federation in the western Pacific Ocean. Calderas are depressions formed when a volcano empties its magma chamber in an explosive eruption and then the overlaying material collapses into the evacuated space. In this astronaut photograph taken from the International Space Station (ISS) on January 9, 2011, the northern end of the island (image right) is dominated by the Nemo Peak volcano, which began forming within an older

PIX4661424

Glacier Viedma, Argentina - Viedma Glacier in Argentina - The Viedma Glacier in Argentina, observed from the International Space Station on January 10, 2004. This detailed view was taken with an 800 mm lens from the International Space Station on 10 January, 2004. The image shows the lower end of the Viedma Glacier that flows into Lake Viedma, one of three major glacially formed lakes on the Patagonian side of the southern Andean ice sheet, at 50 degrees South. The image reveals the slender dark lines of rock material (moraine) which is carried in the slowly flowing ice. Lighter lines at right angles are patterns of crevasse. The glacier diverges into two lakes where calved icebergs can be seen floating in the lakes. The glacier here is about 1.8 km wide

Glacier Viedma, Argentina - Viedma Glacier in Argentina - The Viedma Glacier in Argentina, observed from the International Space Station on January 10, 2004. This detailed view was taken with an 800 mm lens from the International Space Station on 10 January, 2004. The image shows the lower end of the Viedma Glacier that flows into Lake Viedma, one of three major glacially formed lakes on the Patagonian side of the southern Andean ice sheet, at 50 degrees South. The image reveals the slender dark lines of rock material (moraine) which is carried in the slowly flowing ice. Lighter lines at right angles are patterns of crevasse. The glacier diverges into two lakes where calved icebergs can be seen floating in the lakes. The glacier here is about 1.8 km wide

PIX4675760

Caspian sea area seen from space - Caspian sea area seen from space - Satellite photo of the Caspian Sea obtained by Aqua satellite on 30 September 2004. The borders are drawn. In the upper left portion of the image, the southwestern - most portion of Russia spreads across the broad plains north of the Caucasus Mountains. Georgia runs along the southern face of the Caucasus Mountains and part of the southeastern shore of the Black Sea. In the small valley and plains south of Russia and on the central shore of the Caspian Sea, Azerbaijan sprawls until butting up against the mountains of Armenia and northern Iran. Another small piece of Azerbaijan is tucked away on the far side of Armenia. Stretching far from the southern shores of the Black Sea into the mountains and deserts of the Middle East is eastern Turkey, while in the bottom right corner, Syria and Iraq mark the northern edges of the Syrian Desert. The Reshteh - ye Kuhha - ye Alborz Mountains curve in a bright green arc around th

Caspian sea area seen from space - Caspian sea area seen from space - Satellite photo of the Caspian Sea obtained by Aqua satellite on 30 September 2004. The borders are drawn. In the upper left portion of the image, the southwestern - most portion of Russia spreads across the broad plains north of the Caucasus Mountains. Georgia runs along the southern face of the Caucasus Mountains and part of the southeastern shore of the Black Sea. In the small valley and plains south of Russia and on the central shore of the Caspian Sea, Azerbaijan sprawls until butting up against the mountains of Armenia and northern Iran. Another small piece of Azerbaijan is tucked away on the far side of Armenia. Stretching far from the southern shores of the Black Sea into the mountains and deserts of the Middle East is eastern Turkey, while in the bottom right corner, Syria and Iraq mark the northern edges of the Syrian Desert. The Reshteh - ye Kuhha - ye Alborz Mountains curve in a bright green arc around th

PIX4660580

Southern Crown Nebula - The tail of the CRA reflection nebula - R Coronae Australis is a region of star formations visible in the southern hemisphere. It is located about 500 light years away from Earth. On the right, the globular cluster NGC 6723, located 30 000 light years from Earth in Sagittarius. Image made with the 1.2m Telescope of Schmidt UK from Siding Spring. Corona Australis (the southern crown, CRA) is in the far southern sky but visible from the southern states of the USA. The constellation is small but distinctive. The conspicuous globular cluster NGC 6723 is at the western (right) edge of the photograph, but it is in Sagittarius, and is about 30,000 light years distant. Our picture is about 4.5 degrees across and the extremely faint Corona Australis nebula meanders along the Sgr - CRA border nebula in the same E - W direction. Almost all the nebulosity here is starlight, reflected from minute grains of dust, some of which gather into darker condensations ('molecular clou

Southern Crown Nebula - The tail of the CRA reflection nebula - R Coronae Australis is a region of star formations visible in the southern hemisphere. It is located about 500 light years away from Earth. On the right, the globular cluster NGC 6723, located 30 000 light years from Earth in Sagittarius. Image made with the 1.2m Telescope of Schmidt UK from Siding Spring. Corona Australis (the southern crown, CRA) is in the far southern sky but visible from the southern states of the USA. The constellation is small but distinctive. The conspicuous globular cluster NGC 6723 is at the western (right) edge of the photograph, but it is in Sagittarius, and is about 30,000 light years distant. Our picture is about 4.5 degrees across and the extremely faint Corona Australis nebula meanders along the Sgr - CRA border nebula in the same E - W direction. Almost all the nebulosity here is starlight, reflected from minute grains of dust, some of which gather into darker condensations ('molecular clou

PIX4620260

Millennium Island - Millennium Island - Millennium Island, or Carolina Island, is an uninhabited atoll belonging to the Republic of Kiribati and is the most eastern island in the Pacific Ocean. In 1999, for celebrations marking the arrival of the year 2000, the island of Carolina was officially renamed the island of the Millennium, being one of the points on earth closest to the date change line. This island, whose highest point is about 6 metres, is particularly threatened by rising sea levels. Image obtained on 1 July 2009 from the International Space Station (ISS). Millennium Island is located at the southern end of the Line Islands in the South Pacific Ocean. This uninhabited island is part of the Republic of Kiribati. At a maximum height of approximately 6 meters (19.7 feet) above sea level, Millennium Island has been identified as being at great risk from sea level rise by the United Nations. Millennium Island was known as Caroline Island prior to 2000. The name was changed becau

Millennium Island - Millennium Island - Millennium Island, or Carolina Island, is an uninhabited atoll belonging to the Republic of Kiribati and is the most eastern island in the Pacific Ocean. In 1999, for celebrations marking the arrival of the year 2000, the island of Carolina was officially renamed the island of the Millennium, being one of the points on earth closest to the date change line. This island, whose highest point is about 6 metres, is particularly threatened by rising sea levels. Image obtained on 1 July 2009 from the International Space Station (ISS). Millennium Island is located at the southern end of the Line Islands in the South Pacific Ocean. This uninhabited island is part of the Republic of Kiribati. At a maximum height of approximately 6 meters (19.7 feet) above sea level, Millennium Island has been identified as being at great risk from sea level rise by the United Nations. Millennium Island was known as Caroline Island prior to 2000. The name was changed becau

PIX4675565

Palm islands, Dubai 10/2002 - Palm islands, artificial islands built on the coast of the Emirates of Dubai. False colour image obtained by the Terra satellite in October 2002. The vegetation appears in red, the water in dark blue, the constructions in light blue or grey, the desert in beige. This image, acquired in October 2002 by Terra satellite, shows the early stages of Palm Jumeirah, also known as The Palm”” in Dubai. The circular outline of the archipelago is largely completed, and the palm fronds are beginning to take shape. Inland, cityscape begins to push eastward into the desert, with a combination of roads and buildings. The conspicuously vegetated area southeast of Palm Jumeirah is a golf course. East of this course, however, the land is mostly undeveloped desert. In this false - color image, bare ground appears light brown, vegetation appears red, water appears dark blue, and buildings and paved surfaces appear light blue or gray. The United Arab Emirates falls within the E

Palm islands, Dubai 10/2002 - Palm islands, artificial islands built on the coast of the Emirates of Dubai. False colour image obtained by the Terra satellite in October 2002. The vegetation appears in red, the water in dark blue, the constructions in light blue or grey, the desert in beige. This image, acquired in October 2002 by Terra satellite, shows the early stages of Palm Jumeirah, also known as The Palm”” in Dubai. The circular outline of the archipelago is largely completed, and the palm fronds are beginning to take shape. Inland, cityscape begins to push eastward into the desert, with a combination of roads and buildings. The conspicuously vegetated area southeast of Palm Jumeirah is a golf course. East of this course, however, the land is mostly undeveloped desert. In this false - color image, bare ground appears light brown, vegetation appears red, water appears dark blue, and buildings and paved surfaces appear light blue or gray. The United Arab Emirates falls within the E

PIX4660143

Tue 03, 1953 - Law-suit against iron profiteers with 70 accused.: The center of the lawsuit which takes at present place in town-hall of Rheinhausen are the iron-works Rheinhausen which have lost several tons of iron stolen by workers in the time form the end of 1950 to the middle of 1952. By a generous agreement of the work every worker could get bricks, cement and construction iron up to three tons from the works directly. With the iron which was not always needed the workers made agood business. The accused swindlers gave false order-forms, used once more old order-forms and the master at the weighing-machine sometimes gave them twice as much as they had to get. Buyers and receivers of the stolen iron from the whole Ruhr District and from Southern Germany met each other now before the court. More than 30 little profiters, 18 middle and 5 great cheaters and 11 receivers are expecting the sentence

Tue 03, 1953 - Law-suit against iron profiteers with 70 accused.: The center of the lawsuit which takes at present place in town-hall of Rheinhausen are the iron-works Rheinhausen which have lost several tons of iron stolen by workers in the time form the end of 1950 to the middle of 1952. By a generous agreement of the work every worker could get bricks, cement and construction iron up to three tons from the works directly. With the iron which was not always needed the workers made agood business. The accused swindlers gave false order-forms, used once more old order-forms and the master at the weighing-machine sometimes gave them twice as much as they had to get. Buyers and receivers of the stolen iron from the whole Ruhr District and from Southern Germany met each other now before the court. More than 30 little profiters, 18 middle and 5 great cheaters and 11 receivers are expecting the sentence

ZUM4874153

Mars: crater in Myers Valles - Mars: crater in Myers Valles - Mamers Valles is a valley about 1000 km long located in the region of Deuteronilus Mensae, north of Arabia Terra. The image obtained by the Mars Express probe on 5 August 2006 shows a crater at the end of this valley. This circular formation measures about thirty kilometres in diameter and is 1400 metres deep. There are traces of flow of material probably composed of water ice, similar to the relief left by the passage of glaciers on Earth. The High - Resolution Stereo Camera (HRSC) onboard the ESA spacecraft Mars Express obtained images focusing on a depression that displays a crater at the end of the long, winding valley, Mamers Valles. The data was obtained on 5 August 2006 with a ground resolution of approximately 14 m/per pixel. The image is centred at approximately 39* north and 17* east on the planet. The valley of Mamers Valles is approximately 1000 km long, running along the boundary between the northern lowlands an

Mars: crater in Myers Valles - Mars: crater in Myers Valles - Mamers Valles is a valley about 1000 km long located in the region of Deuteronilus Mensae, north of Arabia Terra. The image obtained by the Mars Express probe on 5 August 2006 shows a crater at the end of this valley. This circular formation measures about thirty kilometres in diameter and is 1400 metres deep. There are traces of flow of material probably composed of water ice, similar to the relief left by the passage of glaciers on Earth. The High - Resolution Stereo Camera (HRSC) onboard the ESA spacecraft Mars Express obtained images focusing on a depression that displays a crater at the end of the long, winding valley, Mamers Valles. The data was obtained on 5 August 2006 with a ground resolution of approximately 14 m/per pixel. The image is centred at approximately 39* north and 17* east on the planet. The valley of Mamers Valles is approximately 1000 km long, running along the boundary between the northern lowlands an

PIX4616082

Lake Orumieh in Iran seen from space - Lake Urmia in Iran seen from space - Lake Orumieh is the largest lake in Iran. This dirty lake is a UNESCO biosphere reserve. Image obtained by Space Shuttle Challenger in October 1984. Lake Urmia is an isolated lake in Azerbaijan Province in northwest Iran. The total area of the lake is 1815 square miles (4700 square kilometers), and the north - south length is about 90 miles (145 kilometers). The maximum depth of the shallow, saline lake is approximately 50 feet (15 meters). Climatically, the lake region is located in a semiarid, almost desert environment, with general precipitation averaging 12 inches (30 centimeters) per year. Topographically, the entire region is either plateau or mountain. The surface of the lake is approximately 4100 feet (1250 meters) above sea level with several of the individual volcanic peaks reaching more than 7000 feet (2134 meters) above sea level. The massive, rugged mountain range west of the lake has ridges that e

Lake Orumieh in Iran seen from space - Lake Urmia in Iran seen from space - Lake Orumieh is the largest lake in Iran. This dirty lake is a UNESCO biosphere reserve. Image obtained by Space Shuttle Challenger in October 1984. Lake Urmia is an isolated lake in Azerbaijan Province in northwest Iran. The total area of the lake is 1815 square miles (4700 square kilometers), and the north - south length is about 90 miles (145 kilometers). The maximum depth of the shallow, saline lake is approximately 50 feet (15 meters). Climatically, the lake region is located in a semiarid, almost desert environment, with general precipitation averaging 12 inches (30 centimeters) per year. Topographically, the entire region is either plateau or mountain. The surface of the lake is approximately 4100 feet (1250 meters) above sea level with several of the individual volcanic peaks reaching more than 7000 feet (2134 meters) above sea level. The massive, rugged mountain range west of the lake has ridges that e

PIX4660581

Mars: crater in Myers Valles - Mars: crater in Myers Valles - Mamers Valles is a valley about 1000 km long located in the region of Deuteronilus Mensae, north of Arabia Terra. The image obtained by the Mars Express probe on 5 August 2006 shows a crater at the end of this valley. This circular formation measures about thirty kilometres in diameter and is 1400 metres deep. There are traces of flow of material probably composed of water ice, similar to the relief left by the passage of glaciers on Earth. The darker area could be caused by local erosion or wind-driven material. The High - Resolution Stereo Camera (HRSC) onboard the ESA spacecraft Mars Express obtained images focusing on a depression that displays a crater at the end of the long, winding valley, Mamers Valles. The data was obtained on 5 August 2006 with a ground resolution of approximately 14 m/per pixel. The image is centred at approximately 39* north and 17* east on the planet. The valley of Mamers Valles is approximately

Mars: crater in Myers Valles - Mars: crater in Myers Valles - Mamers Valles is a valley about 1000 km long located in the region of Deuteronilus Mensae, north of Arabia Terra. The image obtained by the Mars Express probe on 5 August 2006 shows a crater at the end of this valley. This circular formation measures about thirty kilometres in diameter and is 1400 metres deep. There are traces of flow of material probably composed of water ice, similar to the relief left by the passage of glaciers on Earth. The darker area could be caused by local erosion or wind-driven material. The High - Resolution Stereo Camera (HRSC) onboard the ESA spacecraft Mars Express obtained images focusing on a depression that displays a crater at the end of the long, winding valley, Mamers Valles. The data was obtained on 5 August 2006 with a ground resolution of approximately 14 m/per pixel. The image is centred at approximately 39* north and 17* east on the planet. The valley of Mamers Valles is approximately

PIX4616090

Mars: crater in Myers Valles - Mars: crater in Myers Valles - Mamers Valles is a valley about 1000 km long located in the region of Deuteronilus Mensae, north of Arabia Terra. The image obtained by the Mars Express probe on 5 August 2006 shows a crater at the end of this valley. This circular formation measures about thirty kilometres in diameter and is 1400 metres deep. There are traces of flow of material probably composed of water ice, similar to the relief left by the passage of glaciers on Earth. The darker area could be caused by local erosion or wind-driven material. The High - Resolution Stereo Camera (HRSC) onboard the ESA spacecraft Mars Express obtained images focusing on a depression that displays a crater at the end of the long, winding valley, Mamers Valles. The data was obtained on 5 August 2006 with a ground resolution of approximately 14 m/per pixel. The image is centred at approximately 39* north and 17* east on the planet. The valley of Mamers Valles is approximately

Mars: crater in Myers Valles - Mars: crater in Myers Valles - Mamers Valles is a valley about 1000 km long located in the region of Deuteronilus Mensae, north of Arabia Terra. The image obtained by the Mars Express probe on 5 August 2006 shows a crater at the end of this valley. This circular formation measures about thirty kilometres in diameter and is 1400 metres deep. There are traces of flow of material probably composed of water ice, similar to the relief left by the passage of glaciers on Earth. The darker area could be caused by local erosion or wind-driven material. The High - Resolution Stereo Camera (HRSC) onboard the ESA spacecraft Mars Express obtained images focusing on a depression that displays a crater at the end of the long, winding valley, Mamers Valles. The data was obtained on 5 August 2006 with a ground resolution of approximately 14 m/per pixel. The image is centred at approximately 39* north and 17* east on the planet. The valley of Mamers Valles is approximately

PIX4616083

Ruined Cities of Ceylon: West End of Southern Altar, Abhayagiriya Dagaba (b/w photo)

Ruined Cities of Ceylon: West End of Southern Altar, Abhayagiriya Dagaba (b/w photo)

Cave, Henry W. (1854-1913)

LLM6009258

Excavation of the Great Temple of Luxor, Upper Egypt (engraving)

Excavation of the Great Temple of Luxor, Upper Egypt (engraving)

English School, (19th century)

LIP1614139

Ruined Cities of Ceylon: East End of Southern Altar, Abhayagiriya Dagaba (b/w photo)

Ruined Cities of Ceylon: East End of Southern Altar, Abhayagiriya Dagaba (b/w photo)

Cave, Henry W. (1854-1913)

LLM6009268

Battle of Copenhagen, 1801 (aquatint)

Battle of Copenhagen, 1801 (aquatint)

UIG1579743

A Young Collared Tamandua sitting at the end of a branch holding on with its prehensile tail, London Zoo, 24th April 1925 (b/w photo)

A Young Collared Tamandua sitting at the end of a branch holding on with its prehensile tail, London Zoo, 24th April 1925 (b/w photo)

Bond, Frederick William (1887-1942)

ZSL3073891

Female Warori slave from the Southern end of Lake Tanganyika (engraving)

Female Warori slave from the Southern end of Lake Tanganyika (engraving)

English School, (19th century)

LLM967293

Emancipation of Southern slaves at the end of the Civil War, 19th century (engraving)

Emancipation of Southern slaves at the end of the Civil War, 19th century (engraving)

UIG2623859

The 1965 emancipation of Southern slaves and the end of the American Civil War

The 1965 emancipation of Southern slaves and the end of the American Civil War

UIG2912394

Thomas Nast's celebration of the emancipation of Southern slaves with the end of the Civil War

Thomas Nast's celebration of the emancipation of Southern slaves with the end of the Civil War

UIG2623858

Seated statue of Gudea, prince of Lagash. Neo-Sumerian period (c. 2125-2110 BC) Gudea was a ruler (ensi) of the state of Lagash in Southern Mesopotamia at the end of the 3rd millennium b.c.

Seated statue of Gudea, prince of Lagash. Neo-Sumerian period (c. 2125-2110 BC) Gudea was a ruler (ensi) of the state of Lagash in Southern Mesopotamia at the end of the 3rd millennium b.c.

UIG529027

Row's End (litho)

Row's End (litho)

Mauzey, Merritt (1898-1973)

DMA1066714

Slave auction

UIG2624001

Ruins of a Roman siege fort (photo)

Ruins of a Roman siege fort (photo)

UIG1580195

Ruins of Herod's Palace at Masada (photo)

Ruins of Herod's Palace at Masada (photo)

UIG1580201

Bath night for evacuees in a cathedral in Southern England (b/w photo)

Bath night for evacuees in a cathedral in Southern England (b/w photo)

English Photographer, (20th century)

LLM6011777

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