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Star Trains - Celestial Ecuador - Photographic pose of several hours on the constellation Orion. Orion, northern hemisphere setting trails. Few hours exposure

Star Trains - Celestial Ecuador - Photographic pose of several hours on the constellation Orion. Orion, northern hemisphere setting trails. Few hours exposure

PIX4580287

Open cluster NGC 3293 in Carene - Open star cluster NGC 3293 in Carina - Star cluster located in the constellation Carene about 8500 years ago - light from Earth. Unlike the Sun, many stars are found in brilliant clusters such as NGC 3293 where they spend their lives. At birth, which should have been at much the same time for all the stars in NGC 3293, the most massive stars are hot and very luminous and therefore appear as the brightest blue stars. With time they deplete their supplies of nuclear fuel, hydrogen. This evolutionary process involves cooling, so that the stars become redder, and would ordinarily disappear from view, but they also swell to gigantic proportions and so remain visible. The bright orange star in NGC 3293 is the member of the cluster which has aged fastest. This cluster is in the constellation of Carina at a distance of about 8500 light years

Open cluster NGC 3293 in Carene - Open star cluster NGC 3293 in Carina - Star cluster located in the constellation Carene about 8500 years ago - light from Earth. Unlike the Sun, many stars are found in brilliant clusters such as NGC 3293 where they spend their lives. At birth, which should have been at much the same time for all the stars in NGC 3293, the most massive stars are hot and very luminous and therefore appear as the brightest blue stars. With time they deplete their supplies of nuclear fuel, hydrogen. This evolutionary process involves cooling, so that the stars become redder, and would ordinarily disappear from view, but they also swell to gigantic proportions and so remain visible. The bright orange star in NGC 3293 is the member of the cluster which has aged fastest. This cluster is in the constellation of Carina at a distance of about 8500 light years

PIX4568236

Barree spiral galaxy NGC 2442 in Flying Fish - NGC 2442, a barred spiral galaxy in Volans - NGC 2442 is a barree spiral galaxy located about 50 million years ago - light. Its asymmetrical shape suggests that a galaxy interacts with it. Image made with Siding Spring's 3.9m telescope. This unusual barred spiral galaxy is in the far southern constellation of Volans and was discovered by Sir John Herschel who described one of its spiral arms as hook - like. Although not seen here, (but evident on very deep images) NGC 2442 appears to have a less massive, distant companion that is also distorted, and it seems likely that the two have had a close encounter in the recent past. If there are no further meetings, the forces that hold NGC 2442 together will restore galaxy to a more symmetrical spiral form. However, much more likely is that the companion has been captured by the distorted spiral and will eventually be devoured by it, triggering a dramatic bout of star formation. NGC 2442 is about

Barree spiral galaxy NGC 2442 in Flying Fish - NGC 2442, a barred spiral galaxy in Volans - NGC 2442 is a barree spiral galaxy located about 50 million years ago - light. Its asymmetrical shape suggests that a galaxy interacts with it. Image made with Siding Spring's 3.9m telescope. This unusual barred spiral galaxy is in the far southern constellation of Volans and was discovered by Sir John Herschel who described one of its spiral arms as hook - like. Although not seen here, (but evident on very deep images) NGC 2442 appears to have a less massive, distant companion that is also distorted, and it seems likely that the two have had a close encounter in the recent past. If there are no further meetings, the forces that hold NGC 2442 together will restore galaxy to a more symmetrical spiral form. However, much more likely is that the companion has been captured by the distorted spiral and will eventually be devoured by it, triggering a dramatic bout of star formation. NGC 2442 is about

PIX4610090

Nebula N70 in the Great Magellan Cloud - The N 70 nebula in Large Magellanic Cloud (LMC) - The Henize 70 nebula extends for about 400 years - light, it is located in the Great Magellan Cloud. In the center, a small group of very massive and extremely hot stars, stars of Wolf - Rayet. Image obtained by Siding Spring's 3.9m telescope. At the centre of this remarkable bubble - like nebula nebula is a small group of extremely hot stars. Some of these stars are rapdly losing mass and have stellar winds blowing from their surfaces with velocities that approach 4000 kilometers per second. Such stars are known as Wolf - Rayet stars and are found in galaxies capable of forming massive stars. There are many such stars in the Large Magellanic Cloud (LMC) but not all of them are associated with distinctive nebulae. The outward flowing streams of energetic particles from Wolf - Rayet (and other energetic stars) eventually interact with the relatively stationary interstellar medium pervading the LMC

Nebula N70 in the Great Magellan Cloud - The N 70 nebula in Large Magellanic Cloud (LMC) - The Henize 70 nebula extends for about 400 years - light, it is located in the Great Magellan Cloud. In the center, a small group of very massive and extremely hot stars, stars of Wolf - Rayet. Image obtained by Siding Spring's 3.9m telescope. At the centre of this remarkable bubble - like nebula nebula is a small group of extremely hot stars. Some of these stars are rapdly losing mass and have stellar winds blowing from their surfaces with velocities that approach 4000 kilometers per second. Such stars are known as Wolf - Rayet stars and are found in galaxies capable of forming massive stars. There are many such stars in the Large Magellanic Cloud (LMC) but not all of them are associated with distinctive nebulae. The outward flowing streams of energetic particles from Wolf - Rayet (and other energetic stars) eventually interact with the relatively stationary interstellar medium pervading the LMC

PIX4620865

Irregular Galaxy of the Little Magellan Cloud (NGC 292) - The Small Magellanic Cloud - The galaxy of the Little Magellan Cloud is about 240,000 light years from Earth in the southern constellation of Toucan. It's one of the closest galaxies of the Lactee Way. Two globular clusters are visible in this image, on the right the Toucan cluster, at the top of the galaxy the NGC 362 cluster. Image obtained by the 1.2m UK Schmidt telescope from Siding Spring, Australia. The Small Magellanic Cloud (SMC) is the second nearest galaxy to the Milky Way, (the LMC being the nearest) and is at the distance of about 240,000 light years, quite close enough for it to be resolved into individual stars on this colour picture made from plates taken on the UK Schmidt Telescope. The shape of the SMC defies description and it is therefore classified as an 'irregular' galaxy. The large globular cluster at right is 47 Tucanae, while a smaller one at the top of the picture is NGC 362. It is about 30,000 light yea

Irregular Galaxy of the Little Magellan Cloud (NGC 292) - The Small Magellanic Cloud - The galaxy of the Little Magellan Cloud is about 240,000 light years from Earth in the southern constellation of Toucan. It's one of the closest galaxies of the Lactee Way. Two globular clusters are visible in this image, on the right the Toucan cluster, at the top of the galaxy the NGC 362 cluster. Image obtained by the 1.2m UK Schmidt telescope from Siding Spring, Australia. The Small Magellanic Cloud (SMC) is the second nearest galaxy to the Milky Way, (the LMC being the nearest) and is at the distance of about 240,000 light years, quite close enough for it to be resolved into individual stars on this colour picture made from plates taken on the UK Schmidt Telescope. The shape of the SMC defies description and it is therefore classified as an 'irregular' galaxy. The large globular cluster at right is 47 Tucanae, while a smaller one at the top of the picture is NGC 362. It is about 30,000 light yea

PIX4613306

Nebula NGC 2359 in the Big Dog - A Wolf - Rayet star in NGC 2359 - NGC 2359 is a nebula in the Big Dog that houses a star Wolf - Rayet, HD 56925. Image obtained by Siding Spring's 3.9m telescope. NGC 2359 is the nebula produced by a single, extremely hot star HD 56925. This is one of the rare Wolf - Rayet stars, whose intrinsic brilliance is combined with high rates of mass loss from its surface. This material is ejected from the star with velocities which approach 2000 kilometers per second. This violent activity quickly reduces the mass of the star which in turn reduces the instability. The rapidly - moving ejected material interacts with the gas and dust around the star producing the cosmic bubble seen here. Such stars are unusual, largely because extreme behaviour of this kind cannot be sustained for long. This particular example is spectacular because it happens to inhabit a part of our Galaxy rich in interstellar gas

Nebula NGC 2359 in the Big Dog - A Wolf - Rayet star in NGC 2359 - NGC 2359 is a nebula in the Big Dog that houses a star Wolf - Rayet, HD 56925. Image obtained by Siding Spring's 3.9m telescope. NGC 2359 is the nebula produced by a single, extremely hot star HD 56925. This is one of the rare Wolf - Rayet stars, whose intrinsic brilliance is combined with high rates of mass loss from its surface. This material is ejected from the star with velocities which approach 2000 kilometers per second. This violent activity quickly reduces the mass of the star which in turn reduces the instability. The rapidly - moving ejected material interacts with the gas and dust around the star producing the cosmic bubble seen here. Such stars are unusual, largely because extreme behaviour of this kind cannot be sustained for long. This particular example is spectacular because it happens to inhabit a part of our Galaxy rich in interstellar gas

PIX4618821

Globular cluster 47 Toucan - 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 oldest stars known today. Image obtained from the 3.9m telescope of Siding Spring, Australia. Among the many spectacular objects in the southern skies are two magnificent naked - eye globular clusters, omega Centauri and 47 Tucanae. These ancient cities of stars are captives of the Milky Way but were formed long before our Galaxy assumed its present shape, indeed these clusters have some of the oldest known stars. 47 Tuc is about 15,000 light years distant and contains several million stars, as many as some minor galaxies. The crowded central region leads to occasional stellar encounters and it is in 47 Tuc that rapidly - spinning pulsars have been discovered by radio astronomers. Although the light of globular clus

Globular cluster 47 Toucan - 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 oldest stars known today. Image obtained from the 3.9m telescope of Siding Spring, Australia. Among the many spectacular objects in the southern skies are two magnificent naked - eye globular clusters, omega Centauri and 47 Tucanae. These ancient cities of stars are captives of the Milky Way but were formed long before our Galaxy assumed its present shape, indeed these clusters have some of the oldest known stars. 47 Tuc is about 15,000 light years distant and contains several million stars, as many as some minor galaxies. The crowded central region leads to occasional stellar encounters and it is in 47 Tuc that rapidly - spinning pulsars have been discovered by radio astronomers. Although the light of globular clus

PIX4564283

Constellation of the Berenice Hair - Constellation of Coma Berenices - The constellation of the Berenice Hair contains a cluster of stars, Melotte 111. Coma Berenice's (Berenices Hair) would be as insignificant as many of Lacaille's southern sky inventions if it were not for the subtle but distinctive Coma Star Cluster (Melotte 111), 270 light years away. The constellation's name alludes to the flowing hair of Queen Berenices of Egypt, allegedly cut off in gratitude for the safe return of her husband from some military escapade. This constellation was once considered to be part of Leo, where the hairy smudge of the open cluster was regarded as the tuft of the lion's tail. Melotte 111 is a large, open cluster of stars ranging between 5th magnitude (barely visible) to 10th magnitude, 100 times fainter. It extends over 5 degrees and despite the faintness of its constituent stars is clearly visible as a hazy patch in an otherwise undistinguished part of the sky. Coma is the direction of th

Constellation of the Berenice Hair - Constellation of Coma Berenices - The constellation of the Berenice Hair contains a cluster of stars, Melotte 111. Coma Berenice's (Berenices Hair) would be as insignificant as many of Lacaille's southern sky inventions if it were not for the subtle but distinctive Coma Star Cluster (Melotte 111), 270 light years away. The constellation's name alludes to the flowing hair of Queen Berenices of Egypt, allegedly cut off in gratitude for the safe return of her husband from some military escapade. This constellation was once considered to be part of Leo, where the hairy smudge of the open cluster was regarded as the tuft of the lion's tail. Melotte 111 is a large, open cluster of stars ranging between 5th magnitude (barely visible) to 10th magnitude, 100 times fainter. It extends over 5 degrees and despite the faintness of its constituent stars is clearly visible as a hazy patch in an otherwise undistinguished part of the sky. Coma is the direction of th

PIX4589943

Constellations of Lievre, Orion, Burin and part of Eridan - Eridanus, Orion, Lepus, and Caelum constellations - In the center left, the constellation of Lievre, above, Orion, from the center up to the bottom, the constellation of Eridan, down to the left, the Burin. At the top of the picture, the bright star is Aldebaran

Constellations of Lievre, Orion, Burin and part of Eridan - Eridanus, Orion, Lepus, and Caelum constellations - In the center left, the constellation of Lievre, above, Orion, from the center up to the bottom, the constellation of Eridan, down to the left, the Burin. At the top of the picture, the bright star is Aldebaran

PIX4592025

Globular cluster M5 in Serpens - Globular cluster M5 in Serpens - This cluster of stars is located about 25,000 light years away from Earth. It is one of the most extensive (165 years - light) and one of the oldest known globular clusters.

Globular cluster M5 in Serpens - Globular cluster M5 in Serpens - This cluster of stars is located about 25,000 light years away from Earth. It is one of the most extensive (165 years - light) and one of the oldest known globular clusters.

PIX4564527

Mars retrograde in the Taurus from 03/09/1990 to 17/03/1991 - The reversal of the motion of Mars in Taurus. September 23, 1990 - Photo series showing the retrograde movement of Mars in the Taurus. September 23, 1990. The reversal of the motion of Mars, between the Hyades and Pleiades, September 3, 1990 to March 17, 199

Mars retrograde in the Taurus from 03/09/1990 to 17/03/1991 - The reversal of the motion of Mars in Taurus. September 23, 1990 - Photo series showing the retrograde movement of Mars in the Taurus. September 23, 1990. The reversal of the motion of Mars, between the Hyades and Pleiades, September 3, 1990 to March 17, 199

PIX4587634

Mars retrograde in the Taurus from 03/09/1990 to 17/03/1991 - The reversal of the motion of Mars in Taurus. October 23, 1990. - Photo series showing the retrograde movement of Mars in the Taurus. October 23, 1990. The reversal of the motion of Mars, between the Hyades and Pleiades, September 3, 1990 to March 17, 199

Mars retrograde in the Taurus from 03/09/1990 to 17/03/1991 - The reversal of the motion of Mars in Taurus. October 23, 1990. - Photo series showing the retrograde movement of Mars in the Taurus. October 23, 1990. The reversal of the motion of Mars, between the Hyades and Pleiades, September 3, 1990 to March 17, 199

PIX4587645

March Retrograde in the Taurus from 03/09/1990 to 17/03/1991 - Reversal motion of Mars in Taurus, January 6, 1991 - Photo series showing the retrograde movement of Mars in the Taurus. 6 January 1991. The reversal of the motion of Mars, between the Hyades and Pleiades, September 3, 1990 to March 17, 199

March Retrograde in the Taurus from 03/09/1990 to 17/03/1991 - Reversal motion of Mars in Taurus, January 6, 1991 - Photo series showing the retrograde movement of Mars in the Taurus. 6 January 1991. The reversal of the motion of Mars, between the Hyades and Pleiades, September 3, 1990 to March 17, 199

PIX4587664

Spiral galaxy NGC 1313 in the Reticule - The starburst galaxy NGC 1313 - NGC 1313 is a galaxy located about 15 million years ago - light. Intense star formations are observed. Image made with Siding Spring's 3.9m telescope. In visible light, NGC 1313 seems dominated by scattered patches of star formation which give our picture a rather ragged appearance. The clouds of bluish stars seem to have burst into existence at random, without the normal trigger gravitational interaction or even a distinct spiral to prompt them. Star formation seems to have occurred in a series of irregular, self-sustaining bursts. However, a very deep image shows that the outer parts of galaxy are also very disturbed. Seen with a radio telescope, the galaxy is rich in hydrogen, the raw material of stars, and the gas circulates around the centre of the galaxy in a well ordered way, apparently hardly affected by the starburst activity or other irregularities that so colour our visual impression of this unusual gal

Spiral galaxy NGC 1313 in the Reticule - The starburst galaxy NGC 1313 - NGC 1313 is a galaxy located about 15 million years ago - light. Intense star formations are observed. Image made with Siding Spring's 3.9m telescope. In visible light, NGC 1313 seems dominated by scattered patches of star formation which give our picture a rather ragged appearance. The clouds of bluish stars seem to have burst into existence at random, without the normal trigger gravitational interaction or even a distinct spiral to prompt them. Star formation seems to have occurred in a series of irregular, self-sustaining bursts. However, a very deep image shows that the outer parts of galaxy are also very disturbed. Seen with a radio telescope, the galaxy is rich in hydrogen, the raw material of stars, and the gas circulates around the centre of the galaxy in a well ordered way, apparently hardly affected by the starburst activity or other irregularities that so colour our visual impression of this unusual gal

PIX4609773

Barree spiral galaxy NGC 6744 in the constellation Peacock - Barred spiral galaxy NGC 6744 in Pavo - The galaxy NGC 6744 is located about 25 million years ago - light from Earth. The morphology of this galaxy is very similar to that of our galaxy, the Lactee Way. Image obtained from the 3.9m telescope of Siding Spring, Australia. This beautiful galaxy is about 25 million light years away in the direction of Pavo, a constellation of the southern hemisphere winter. NGC 6744 is believed to one of the most Milky Way - like of all the nearby spirals, with fluffy (flocculent) spiral arms and a large and distinctly elongated nucleus. It also has other similarities to the Milky Way that are not visible here (but seen on a deep image) with at least one distorted companion galaxy superficially similar to one of the Magellanic Clouds. The CCD chip that made this picture at the prime focus of the AAT (Siding Spring) covers about 7 arc minutes of sky. But the galaxy has a much bigger angular size t

Barree spiral galaxy NGC 6744 in the constellation Peacock - Barred spiral galaxy NGC 6744 in Pavo - The galaxy NGC 6744 is located about 25 million years ago - light from Earth. The morphology of this galaxy is very similar to that of our galaxy, the Lactee Way. Image obtained from the 3.9m telescope of Siding Spring, Australia. This beautiful galaxy is about 25 million light years away in the direction of Pavo, a constellation of the southern hemisphere winter. NGC 6744 is believed to one of the most Milky Way - like of all the nearby spirals, with fluffy (flocculent) spiral arms and a large and distinctly elongated nucleus. It also has other similarities to the Milky Way that are not visible here (but seen on a deep image) with at least one distorted companion galaxy superficially similar to one of the Magellanic Clouds. The CCD chip that made this picture at the prime focus of the AAT (Siding Spring) covers about 7 arc minutes of sky. But the galaxy has a much bigger angular size t

PIX4612955

Elliptical galaxy Centaurus A (NGC 5128) in the Centaurus - Galaxy Centaurus A (NGC 5128). Wide field - The NGC 5128 galaxy is about 13 million light years away from Earth. Image obtained from the 1.2m telescope of Siding Spring, Australia. Centaurus A is a most unusual galaxy, set in a rich part of the southern sky. not only are there plenty of stars here to catch the eye, but the region is rich in galaxies as well. One of the nearer galaxies, at 13 million light years away, Centaurus A is the most powerful nearby radio source and is also a copious source of X - and gamma rays as well as visible and infrared radiation

Elliptical galaxy Centaurus A (NGC 5128) in the Centaurus - Galaxy Centaurus A (NGC 5128). Wide field - The NGC 5128 galaxy is about 13 million light years away from Earth. Image obtained from the 1.2m telescope of Siding Spring, Australia. Centaurus A is a most unusual galaxy, set in a rich part of the southern sky. not only are there plenty of stars here to catch the eye, but the region is rich in galaxies as well. One of the nearer galaxies, at 13 million light years away, Centaurus A is the most powerful nearby radio source and is also a copious source of X - and gamma rays as well as visible and infrared radiation

PIX4612296

Flying Fish Constellation - Constellation of Volans - Flying Fish is a small constellation in the southern hemisphere. The bright star on its left is Miaplacidus, in Carene. Volans was introduced by Johann Bayer in 1603 as Piscis Volans, the Flying Fish and in old star atlases is seen flying alongside the ancient sailing ship Argo Navis. However, the fish has flown and only the adjective Volans (flying) remains. The stars form a distinctive pattern but at magnitudes between 3.7 and 4.0 they are not bright. On the other hand the constellation is easily found between the bright stars Avior (epsilon Carinae) and Miaplacidus (beta Carinae) with the fish apparently flying towards the LM

Flying Fish Constellation - Constellation of Volans - Flying Fish is a small constellation in the southern hemisphere. The bright star on its left is Miaplacidus, in Carene. Volans was introduced by Johann Bayer in 1603 as Piscis Volans, the Flying Fish and in old star atlases is seen flying alongside the ancient sailing ship Argo Navis. However, the fish has flown and only the adjective Volans (flying) remains. The stars form a distinctive pattern but at magnitudes between 3.7 and 4.0 they are not bright. On the other hand the constellation is easily found between the bright stars Avior (epsilon Carinae) and Miaplacidus (beta Carinae) with the fish apparently flying towards the LM

PIX4593469

Constellation Pegase - detail - Contellation of Pegasus - detail - The great square of Pegase. The Great Square of Pegasu

Constellation Pegase - detail - Contellation of Pegasus - detail - The great square of Pegase. The Great Square of Pegasu

PIX4593186

Galaxy NGC 4027 in the Raven - Galaxy NGC 4027 in Corvus - NGC 4027 is a spiral galaxy located about 80 million years ago - light. The photo shows some nearby dwarf galaxies. Image made with Siding Spring's 3.9m telescope. This galaxy is of interest because of its similarity to the Large Magellanic Cloud, (LMC) our nearest extra - galactic neighbour. Like the LMC, its light comes predominantly from young stars, which are hotter than the Sun and give the galaxy a bluish colour. However, because this galaxy is over 80 million light - years distant we see only the integrated light of millions of unresolved stars, rather than the individuals we see in the LMC. NGC 4027 has a somewhat distorted appearance and an elongated spiral arm, probably due to the gravitational effect of a smaller companion galaxy, not visible in this photograph but rather obvious on a much deeper image. NGC 4027 is less than half a degree south of the Antennae interacting galaxies

Galaxy NGC 4027 in the Raven - Galaxy NGC 4027 in Corvus - NGC 4027 is a spiral galaxy located about 80 million years ago - light. The photo shows some nearby dwarf galaxies. Image made with Siding Spring's 3.9m telescope. This galaxy is of interest because of its similarity to the Large Magellanic Cloud, (LMC) our nearest extra - galactic neighbour. Like the LMC, its light comes predominantly from young stars, which are hotter than the Sun and give the galaxy a bluish colour. However, because this galaxy is over 80 million light - years distant we see only the integrated light of millions of unresolved stars, rather than the individuals we see in the LMC. NGC 4027 has a somewhat distorted appearance and an elongated spiral arm, probably due to the gravitational effect of a smaller companion galaxy, not visible in this photograph but rather obvious on a much deeper image. NGC 4027 is less than half a degree south of the Antennae interacting galaxies

PIX4611058

Design with Decorative Vessels, 1915 (pen & ink with pencil on paper & board)

Design with Decorative Vessels, 1915 (pen & ink with pencil on paper & board)

Berson, Lazar (1882-1954)

BUG2970092

Jupiter and Saturn in the Taurus -06/11/1999 - Jupiter and Saturn between the Hyades and Pleiades - Jupiter and Saturn between the Hyades and Pleiades, 1999-2000. November 6, 199

Jupiter and Saturn in the Taurus -06/11/1999 - Jupiter and Saturn between the Hyades and Pleiades - Jupiter and Saturn between the Hyades and Pleiades, 1999-2000. November 6, 199

PIX4587736

Constellation Ursa - Constellation of Ursa Major - Grand Chariot, asterism of the constellation Ursa Ursa

Constellation Ursa - Constellation of Ursa Major - Grand Chariot, asterism of the constellation Ursa Ursa

PIX4591217

Galaxy seen by the slice NGC 55 in the Sculptor - Edge - on galaxy NGC 55 in Sculptor - The irregular galaxy NGC 55 is located 5 million years ago - light of the Earth and resides in a grouping of several galaxies calls the Sculptor's Group

Galaxy seen by the slice NGC 55 in the Sculptor - Edge - on galaxy NGC 55 in Sculptor - The irregular galaxy NGC 55 is located 5 million years ago - light of the Earth and resides in a grouping of several galaxies calls the Sculptor's Group

PIX4608616

Spiral Galaxy M83 in Hydra - Spiral galaxy M83 in Hydra - The galaxy M83 (NGC 5236) is located about 15 million years away from Earth. This galaxy is intermediate between a classic spiral and a barree spiral. Image obtained from the 3.9m telescope of Siding Spring, Australia. M83 is thought to be very like our own Galaxy, the Milky Way, but seen from above one of its poles and at a distance of about 15 million light years. Composed of billions of stars and huge clouds of dust and gas, this object is one of the finest examples of a spiral galaxy and shows a concentration of older, yellow stars in its central nucleus with younger, blue stars and patchy red clouds of glowing gas and dark dust lanes in the trailing spiral arms. The massive blue stars occasionally explode as supernovae; at least eight have been seen in Messier 83 in the last 70 years

Spiral Galaxy M83 in Hydra - Spiral galaxy M83 in Hydra - The galaxy M83 (NGC 5236) is located about 15 million years away from Earth. This galaxy is intermediate between a classic spiral and a barree spiral. Image obtained from the 3.9m telescope of Siding Spring, Australia. M83 is thought to be very like our own Galaxy, the Milky Way, but seen from above one of its poles and at a distance of about 15 million light years. Composed of billions of stars and huge clouds of dust and gas, this object is one of the finest examples of a spiral galaxy and shows a concentration of older, yellow stars in its central nucleus with younger, blue stars and patchy red clouds of glowing gas and dark dust lanes in the trailing spiral arms. The massive blue stars occasionally explode as supernovae; at least eight have been seen in Messier 83 in the last 70 years

PIX4612481

Spiral Galaxy M83 in Hydra - Spiral galaxy M83 in Hydra - The galaxy M83 (NGC 5236) is located about 15 million years away from Earth. This galaxy is intermediate between a classic spiral and a barree spiral. Image obtained from the 3.9m telescope of Siding Spring, Australia. M83 is thought to be very like our own Galaxy, the Milky Way, but seen from above one of its poles and at a distance of about 15 million light years. Composed of billions of stars and huge clouds of dust and gas, this object is one of the finest examples of a spiral galaxy and shows a concentration of older, yellow stars in its central nucleus with younger, blue stars and patchy red clouds of glowing gas and dark dust lanes in the trailing spiral arms. The massive blue stars occasionally explode as supernovae; at least eight have been seen in Messier 83 in the last 70 years

Spiral Galaxy M83 in Hydra - Spiral galaxy M83 in Hydra - The galaxy M83 (NGC 5236) is located about 15 million years away from Earth. This galaxy is intermediate between a classic spiral and a barree spiral. Image obtained from the 3.9m telescope of Siding Spring, Australia. M83 is thought to be very like our own Galaxy, the Milky Way, but seen from above one of its poles and at a distance of about 15 million light years. Composed of billions of stars and huge clouds of dust and gas, this object is one of the finest examples of a spiral galaxy and shows a concentration of older, yellow stars in its central nucleus with younger, blue stars and patchy red clouds of glowing gas and dark dust lanes in the trailing spiral arms. The massive blue stars occasionally explode as supernovae; at least eight have been seen in Messier 83 in the last 70 years

PIX4612513

Cephee Constellation - Constellation of Cepheus - At the bottom left, the constellation Cassiopee; at the top, the bright star is the polar star. Cepheus is a representation of King Cepheus of Ethiopia, who has stellar connections, being husband to Cassiopeia and the father of Andromeda. It is a large northern constellation of 588 square degrees, 27th out of 88 in size and is best seen in the early evening in November. It is distinguished by having two unusual stars that are easily seen. Delta Cephei is the prototype for an intrinsically bright class of regularly pulsating variable stars whose period of variability is closely related to their absolute magnitudes. The brightest stars have the longest period, so distance can be estimated by measuring the period and the apparent magnitude of a star. And these stars are bright, so the method can be extended to nearby galaxies. Mu (u) Cephei is an extremely red, irregular variable star easily seen in binoculars. This too is a prototype, of

Cephee Constellation - Constellation of Cepheus - At the bottom left, the constellation Cassiopee; at the top, the bright star is the polar star. Cepheus is a representation of King Cepheus of Ethiopia, who has stellar connections, being husband to Cassiopeia and the father of Andromeda. It is a large northern constellation of 588 square degrees, 27th out of 88 in size and is best seen in the early evening in November. It is distinguished by having two unusual stars that are easily seen. Delta Cephei is the prototype for an intrinsically bright class of regularly pulsating variable stars whose period of variability is closely related to their absolute magnitudes. The brightest stars have the longest period, so distance can be estimated by measuring the period and the apparent magnitude of a star. And these stars are bright, so the method can be extended to nearby galaxies. Mu (u) Cephei is an extremely red, irregular variable star easily seen in binoculars. This too is a prototype, of

PIX4589805

Globular cluster 47 Toucan - 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 oldest stars known today. Image obtained from the 3.9m telescope of Siding Spring, Australia. Among the many spectacular objects in the southern skies are two magnificent naked - eye globular clusters, omega Centauri and 47 Tucanae. These ancient cities of stars are captives of the Milky Way but were formed long before our Galaxy assumed its present shape, indeed these clusters have some of the oldest known stars. 47 Tuc is about 15,000 light years distant and contains several million stars, as many as some minor galaxies. The crowded central region leads to occasional stellar encounters and it is in 47 Tuc that rapidly - spinning pulsars have been discovered by radio astronomers. Although the light of globular clust

Globular cluster 47 Toucan - 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 oldest stars known today. Image obtained from the 3.9m telescope of Siding Spring, Australia. Among the many spectacular objects in the southern skies are two magnificent naked - eye globular clusters, omega Centauri and 47 Tucanae. These ancient cities of stars are captives of the Milky Way but were formed long before our Galaxy assumed its present shape, indeed these clusters have some of the oldest known stars. 47 Tuc is about 15,000 light years distant and contains several million stars, as many as some minor galaxies. The crowded central region leads to occasional stellar encounters and it is in 47 Tuc that rapidly - spinning pulsars have been discovered by radio astronomers. Although the light of globular clust

PIX4564310

Captain January de David Butler avec Temple Shirley en 1936

Captain January de David Butler avec Temple Shirley en 1936

XRD1715114

Persee Constellation - Constellation of Persia

Persee Constellation - Constellation of Persia

PIX4593202

Venus in the Pleiades - Venus among the Pleiades, April 3 1999 - Venus among the Pleiades, April 3

Venus in the Pleiades - Venus among the Pleiades, April 3 1999 - Venus among the Pleiades, April 3

PIX4586749

Nebula IC 2948 in Centaur - Bok's cells - A group of Bok globules in IC 2948 - View of a detail of nebula IC 2948 in the center Centaur on Bok's cells. A Bok's blood cell is a dark interstellar cloud of gases and dust that absorb light. If it condenses enough, it gives birth to new stars. The dark spots in the picture are not photographic defects but an unusual type of interstellar cloud known as a Bok globule. Bok globules, named after astronomer Bart Bok who studied them extensively, are small dark clouds made of gas and dust that are typically condensing to form a star or stars. These Bok globules are located at a distance of about 6000 light years near IC 2944 cluster in the emission nebula IC 2948

Nebula IC 2948 in Centaur - Bok's cells - A group of Bok globules in IC 2948 - View of a detail of nebula IC 2948 in the center Centaur on Bok's cells. A Bok's blood cell is a dark interstellar cloud of gases and dust that absorb light. If it condenses enough, it gives birth to new stars. The dark spots in the picture are not photographic defects but an unusual type of interstellar cloud known as a Bok globule. Bok globules, named after astronomer Bart Bok who studied them extensively, are small dark clouds made of gas and dust that are typically condensing to form a star or stars. These Bok globules are located at a distance of about 6000 light years near IC 2944 cluster in the emission nebula IC 2948

PIX4622532

Barree spiral galaxy NGC 6744 in the constellation Peacock - Barred spiral galaxy NGC 6744 in Pavo - The galaxy NGC 6744 is located about 25 million years ago - light from Earth. Image obtained from the 3.9m telescope of Siding Spring, Australia. This beautiful galaxy is about 25 million light years away in the direction of Pavo, a constellation of the southern hemisphere winter. It sits in a rich starfield, and is strongly inclined to our line of sight. NGC 6744 is believed to one of the most Milky Way - like of all the nearby spirals, with fluffy (flocculent) spiral arms and a large and distinctly elongated nucleus. It also has other similarities to the Milky Way that are not visible here with at least one distorted companion galaxy superficially similar to one of the Magellanic Clouds

Barree spiral galaxy NGC 6744 in the constellation Peacock - Barred spiral galaxy NGC 6744 in Pavo - The galaxy NGC 6744 is located about 25 million years ago - light from Earth. Image obtained from the 3.9m telescope of Siding Spring, Australia. This beautiful galaxy is about 25 million light years away in the direction of Pavo, a constellation of the southern hemisphere winter. It sits in a rich starfield, and is strongly inclined to our line of sight. NGC 6744 is believed to one of the most Milky Way - like of all the nearby spirals, with fluffy (flocculent) spiral arms and a large and distinctly elongated nucleus. It also has other similarities to the Milky Way that are not visible here with at least one distorted companion galaxy superficially similar to one of the Magellanic Clouds

PIX4612966

Jewish grave in military cemetery. Second World War II. Annecy. France.

Jewish grave in military cemetery. Second World War II. Annecy. France.

Pascal Deloche

GNG6949611

Jerusalem XIV-D, Girls with Flutes

premium — Jerusalem XIV-D, Girls with Flutes

Jerusalem XIV-D, Girls with Flutes

Hodges, Elizabeth Barakah (b.1938)

SSI2211433

An Israeli Jew prays at the Western Wall, Jerusalem, Israel

An Israeli Jew prays at the Western Wall, Jerusalem, Israel

GNG5280145

Old Bible in french, 18 th century, Old Testament, Deuteronomy, The Fith Book of Moses, France (photo)

Old Bible in french, 18 th century, Old Testament, Deuteronomy, The Fith Book of Moses, France (photo)

Fred de Noyelle

GNG6279590

A man selling goods in a ghetto street, Lodz, Poland, 1942 (photo)

A man selling goods in a ghetto street, Lodz, Poland, 1942 (photo)

GBW3246135

Christ In Majesty, c.1867 (stained glass)

Christ In Majesty, c.1867 (stained glass)

Hassam, Alfred (1842-69)

Alastair Carew-Cox

CCX3474781

Mars retrograde in the Taurus from 03/09/1990 to 17/03/1991 - The reversal of the motion of Mars in Taurus. September 3, 1990 - Photo series showing the retrograde movement of Mars in the Taurus. September 3, 1990. The reversal of the motion of Mars, between the Hyades and Pleiades, September 3, 1990 to March 17, 199

Mars retrograde in the Taurus from 03/09/1990 to 17/03/1991 - The reversal of the motion of Mars in Taurus. September 3, 1990 - Photo series showing the retrograde movement of Mars in the Taurus. September 3, 1990. The reversal of the motion of Mars, between the Hyades and Pleiades, September 3, 1990 to March 17, 199

PIX4587629

Galaxies NGC 5078 and IC 879 in Hydra - Galaxies NGC 5078 and IC 879 in Hydra - NGC 5078 is a spiral galaxy located about 95 million years ago - light. A small galaxy, IC 879, at the bottom of the picture, is probably interacting with it. Image made with Siding Spring's 3.9m telescope. NGC 5078 is a lenticular (lens - shaped) galaxy crossed by a distinct dusty band which is seen against the bright background of the galaxy itself. The dust lane is warped and broadened, probably by interaction with the faint companion galaxy IC 879, which is itself distorted into an 'S' shape by the interaction. The slightly bluish colour of parts of the fainter galaxy is suggestive of star formation, probably triggered by the interaction. Encounters between galaxies such as this are common, and often lead to them merging into a single entity. It is likely that the dust lane of NGC 5078 is the remnant of a dusty spiral which fell into it long ago. The galaxies are about 80 million light years distant

Galaxies NGC 5078 and IC 879 in Hydra - Galaxies NGC 5078 and IC 879 in Hydra - NGC 5078 is a spiral galaxy located about 95 million years ago - light. A small galaxy, IC 879, at the bottom of the picture, is probably interacting with it. Image made with Siding Spring's 3.9m telescope. NGC 5078 is a lenticular (lens - shaped) galaxy crossed by a distinct dusty band which is seen against the bright background of the galaxy itself. The dust lane is warped and broadened, probably by interaction with the faint companion galaxy IC 879, which is itself distorted into an 'S' shape by the interaction. The slightly bluish colour of parts of the fainter galaxy is suggestive of star formation, probably triggered by the interaction. Encounters between galaxies such as this are common, and often lead to them merging into a single entity. It is likely that the dust lane of NGC 5078 is the remnant of a dusty spiral which fell into it long ago. The galaxies are about 80 million light years distant

PIX4612223

Nebula Trifide (M20) in the constellation Sagittarius - Trifid nebula (M20) in Sagittarius - View of the center of the Trifide nebula (M20/NGC 6514) located in the constellation Sagittarius between 5000 and 10,000 years - light from Earth. Image obtained by Siding Spring's 3.9m telescope. Vast clouds of hydrogen mixed with tiny dust grains are distributed throughout the Milky Way. The hydrogen can only be seen at visible wavelengths when it is illuminated by very hot stars. The light from these stars is sufficiently rich in ultraviolet light to cause the gas to glow with its characteristic red colour. In most cases, such as here, the hot stars formed recently from the hydrogen cloud. The stars found at the heart of the Trifid Nebula are here seen associated with dust lanes which are silhouetted against the glowing background. This nebula is in the constellation of Sagittarius at a distance between 5000 and 10,000 light years

Nebula Trifide (M20) in the constellation Sagittarius - Trifid nebula (M20) in Sagittarius - View of the center of the Trifide nebula (M20/NGC 6514) located in the constellation Sagittarius between 5000 and 10,000 years - light from Earth. Image obtained by Siding Spring's 3.9m telescope. Vast clouds of hydrogen mixed with tiny dust grains are distributed throughout the Milky Way. The hydrogen can only be seen at visible wavelengths when it is illuminated by very hot stars. The light from these stars is sufficiently rich in ultraviolet light to cause the gas to glow with its characteristic red colour. In most cases, such as here, the hot stars formed recently from the hydrogen cloud. The stars found at the heart of the Trifid Nebula are here seen associated with dust lanes which are silhouetted against the glowing background. This nebula is in the constellation of Sagittarius at a distance between 5000 and 10,000 light years

PIX4619647

Jupiter and Saturn in the Taurus. 29/12/2000 - Jupiter and Saturn move into Taurus - Jupiter and Saturn move into Taurus, 1999-2000. 29 December, 200

Jupiter and Saturn in the Taurus. 29/12/2000 - Jupiter and Saturn move into Taurus - Jupiter and Saturn move into Taurus, 1999-2000. 29 December, 200

PIX4587719

Jupiter and Saturn in the Taurus. 29/12/2000 - Jupiter and Saturn move into Taurus - Jupiter and Saturn move into Taurus, 1999-2000. 29 December, 200

Jupiter and Saturn in the Taurus. 29/12/2000 - Jupiter and Saturn move into Taurus - Jupiter and Saturn move into Taurus, 1999-2000. 29 December, 200

PIX4587782

Spiral galaxy NGC 6744 in the constellation Peacock - Spiral galaxy NGC 6744 in Pavo - The galaxy NGC 6744 is about 25 million years away - light from Earth. Image obtained from the 3.9m telescope of Siding Spring, Australia. This beautiful galaxy is about 25 million light years away in the direction of Pavo, a constellation of the southern hemisphere winter. It sits in a rich starfield, and is strongly inclined to our line of sight. NGC 6744 is believed to one of the most Milky Way - like of all the nearby spirals, with fluffy (flocculent) spiral arms and a large and distinctly elongated nucleus. It also has other similarities to the Milky Way that are not visible here with at least one distorted companion galaxy superficially similar to one of the Magellanic Clouds

Spiral galaxy NGC 6744 in the constellation Peacock - Spiral galaxy NGC 6744 in Pavo - The galaxy NGC 6744 is about 25 million years away - light from Earth. Image obtained from the 3.9m telescope of Siding Spring, Australia. This beautiful galaxy is about 25 million light years away in the direction of Pavo, a constellation of the southern hemisphere winter. It sits in a rich starfield, and is strongly inclined to our line of sight. NGC 6744 is believed to one of the most Milky Way - like of all the nearby spirals, with fluffy (flocculent) spiral arms and a large and distinctly elongated nucleus. It also has other similarities to the Milky Way that are not visible here with at least one distorted companion galaxy superficially similar to one of the Magellanic Clouds

PIX4612996

Untitled, 1905-38 (gelatin silver print)

Untitled, 1905-38 (gelatin silver print)

Van Der Zee, James (1886-1983)

CH5055793

Jacques Martin Kissing Pascale Hazan For her Wedding With David Martin August 1989 (photo)

Jacques Martin Kissing Pascale Hazan For her Wedding With David Martin August 1989 (photo)

XRA1663057

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

Constellation of Big Bear - Constellation of Ursa Major - The constellation of Big Bear with the constellations of Hunting Dogs and Little Lion. Ursa Major is the third largest constellation in the sky but is not seen by skywatchers in the far southern hemisphere. However, it is the most recognisable of all constellations for those who can see it, mainly because of the asterism formed by the seven brightest stars. This is known as the Big Dipper in the USA, the Plough in Britain, various kinds of carts in Europe and a range of other objects in other cultures. Not surprisingly the constellation as a whole has a rich mythology associated with it, with many peoples projecting their stories among these beautiful stars. Greatly abbreviated, one ancient Greek version has Zeus romancing Callisto. His wife Hera changed Callisto into a bear out of jealousy. Hera's son Arcus found Callisto (the bear) by chance in the forest and was about to kill her, so to save her, Zeus turned Arcus into a smal

Constellation of Big Bear - Constellation of Ursa Major - The constellation of Big Bear with the constellations of Hunting Dogs and Little Lion. Ursa Major is the third largest constellation in the sky but is not seen by skywatchers in the far southern hemisphere. However, it is the most recognisable of all constellations for those who can see it, mainly because of the asterism formed by the seven brightest stars. This is known as the Big Dipper in the USA, the Plough in Britain, various kinds of carts in Europe and a range of other objects in other cultures. Not surprisingly the constellation as a whole has a rich mythology associated with it, with many peoples projecting their stories among these beautiful stars. Greatly abbreviated, one ancient Greek version has Zeus romancing Callisto. His wife Hera changed Callisto into a bear out of jealousy. Hera's son Arcus found Callisto (the bear) by chance in the forest and was about to kill her, so to save her, Zeus turned Arcus into a smal

PIX4591228

Nebulae NGC 6334 and NGC 6357 in Scorpio - Nebulae NGC 6334 and NGC 6357 in Scorpius - These nebulae are located approximately 5500 years - light from Earth. Image made with the 1.2m Telescope of Schmidt UK from Siding Spring. The star - forming nebulae NGC 6334 and NGC 6357 show no evidence of a blue component in their colour - indeed, the blue - light plate used in these 3 - colour pictures had no nebulous image at all - nor is there any obvious sign of the bright blue stars normally found in these objects. They are excellent examples of the phenomenon known as 'interstellar reddening', the selective removal of blue light by minute particles of dust in the line of sight. This accounts for both the ruddy hue and apparent absence of blue stars. The hot stars are present but only some of the red part of their light is seen so they are not conspicuous. These nebulae are quite nearby (5500 light years) but located close to the Galactic plane and are buried in the dust of the Milky Way. Ca

Nebulae NGC 6334 and NGC 6357 in Scorpio - Nebulae NGC 6334 and NGC 6357 in Scorpius - These nebulae are located approximately 5500 years - light from Earth. Image made with the 1.2m Telescope of Schmidt UK from Siding Spring. The star - forming nebulae NGC 6334 and NGC 6357 show no evidence of a blue component in their colour - indeed, the blue - light plate used in these 3 - colour pictures had no nebulous image at all - nor is there any obvious sign of the bright blue stars normally found in these objects. They are excellent examples of the phenomenon known as 'interstellar reddening', the selective removal of blue light by minute particles of dust in the line of sight. This accounts for both the ruddy hue and apparent absence of blue stars. The hot stars are present but only some of the red part of their light is seen so they are not conspicuous. These nebulae are quite nearby (5500 light years) but located close to the Galactic plane and are buried in the dust of the Milky Way. Ca

PIX4619350

Whale Constellation - Constellation of Cetus - Also visible, the constellation Belier at the top of the picture. Cetus (the Whale or Sea Monster) is an ancient constellation in the northern sky depicting a whale - like creature basking on the shores of the fabled stream Eridanus, which flows from the celestial equator far into the southern sky. Cetus is extensive but not very distinctive, containing few bright stars. However, some of the stars are exceptionally interesting, particlarly Mira the wonderful, the prototype variable star, whose variability was first noted 400 years ago. The constellation of Aries is visible at the top of the image

Whale Constellation - Constellation of Cetus - Also visible, the constellation Belier at the top of the picture. Cetus (the Whale or Sea Monster) is an ancient constellation in the northern sky depicting a whale - like creature basking on the shores of the fabled stream Eridanus, which flows from the celestial equator far into the southern sky. Cetus is extensive but not very distinctive, containing few bright stars. However, some of the stars are exceptionally interesting, particlarly Mira the wonderful, the prototype variable star, whose variability was first noted 400 years ago. The constellation of Aries is visible at the top of the image

PIX4589136

Peacock Constellation - Constellation of Pavo - Pavo, the Peacock, lies south of Sagittarius and Corona Australis, and is one of Johann Bayer's twelve constellations, introduced in 1603. It is one of several birds in the southern sky, including Apus, Grus, Phoenix and Tucanae. The legends say that the goddess of the heavens, Juno (the Greek Hera) ordered a hundred - eyed giant, Argos Panoptes, to keep his eyes on her wandering husband, Jupiter. He ordered Argos slain and Juno transformed the 100 eyes into the Peacock's tail. These eyes are also meant to represent the starry sky

Peacock Constellation - Constellation of Pavo - Pavo, the Peacock, lies south of Sagittarius and Corona Australis, and is one of Johann Bayer's twelve constellations, introduced in 1603. It is one of several birds in the southern sky, including Apus, Grus, Phoenix and Tucanae. The legends say that the goddess of the heavens, Juno (the Greek Hera) ordered a hundred - eyed giant, Argos Panoptes, to keep his eyes on her wandering husband, Jupiter. He ordered Argos slain and Juno transformed the 100 eyes into the Peacock's tail. These eyes are also meant to represent the starry sky

PIX4593100

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

Nebula of the Lagoon (M8) in Sagittarius - The Lagoon Nebula, M8, NGC 6523 - View of the Nebula of the Lagoon (M8/NGC 6523). Located in Sagittarius, at a distance of 6500 years - light, it extends over a diameter of 60 AL. Image made with the 1.2m Telescope of Schmidt UK from Siding Spring. The irregular distribution of light in this beautiful part of the sky is due mainly to clouds of dust that dim the light of vast clouds of stars that make Sagittarius one of the brightest parts of the Milky Way. The Lagoon nebula is an illuminated part of such a dark ('molecule') cloud and it reveals the dust as dark lanes and globules silhouetted against the luminous gas. Within the nebula is the scattered young star cluster NGC 6530, recently formed from this material, though the centre of star - forming activity has now shifted westwards from the cluster to the brightest part of the nebula, around the tiny Hourglass Nebula

Nebula of the Lagoon (M8) in Sagittarius - The Lagoon Nebula, M8, NGC 6523 - View of the Nebula of the Lagoon (M8/NGC 6523). Located in Sagittarius, at a distance of 6500 years - light, it extends over a diameter of 60 AL. Image made with the 1.2m Telescope of Schmidt UK from Siding Spring. The irregular distribution of light in this beautiful part of the sky is due mainly to clouds of dust that dim the light of vast clouds of stars that make Sagittarius one of the brightest parts of the Milky Way. The Lagoon nebula is an illuminated part of such a dark ('molecule') cloud and it reveals the dust as dark lanes and globules silhouetted against the luminous gas. Within the nebula is the scattered young star cluster NGC 6530, recently formed from this material, though the centre of star - forming activity has now shifted westwards from the cluster to the brightest part of the nebula, around the tiny Hourglass Nebula

PIX4619624

Centaurus A elliptical galaxy (NGC 5128) in Centaurus - Galaxy Centaurus A (NGC 5128) - The galaxy NGC 5128 is located about 13 million light years away from Earth in the southern constellation of Centaurus. A broad dark band crosses it in the middle, a probable vestige of a collision with a spiral galaxy. This Giant Galaxy is a powerful radio source known as Centaurus A. It is an active galaxy whose energy comes from a supermassive black hole. The green dot visible in the dust strip is a supernova, the supernova 1986g. It appears green because the red filter image that made this trichromy image was only taken a year after the event and the supernova had weakened. Image obtained from the 3.9m telescope of Siding Spring, Australia. Centaurus A is a most unusual galaxy. The circular, uniformly bright portion is composed of several thousand million stars, most of them old and yellowish. The galaxy is girded by a dense dust lane which obscures and reddens the light of stars behind it. Some

Centaurus A elliptical galaxy (NGC 5128) in Centaurus - Galaxy Centaurus A (NGC 5128) - The galaxy NGC 5128 is located about 13 million light years away from Earth in the southern constellation of Centaurus. A broad dark band crosses it in the middle, a probable vestige of a collision with a spiral galaxy. This Giant Galaxy is a powerful radio source known as Centaurus A. It is an active galaxy whose energy comes from a supermassive black hole. The green dot visible in the dust strip is a supernova, the supernova 1986g. It appears green because the red filter image that made this trichromy image was only taken a year after the event and the supernova had weakened. Image obtained from the 3.9m telescope of Siding Spring, Australia. Centaurus A is a most unusual galaxy. The circular, uniformly bright portion is composed of several thousand million stars, most of them old and yellowish. The galaxy is girded by a dense dust lane which obscures and reddens the light of stars behind it. Some

PIX4612278

Dark Stars and Nebulae in Sagittarius - The Star Clouds of Sagittarius - Star Field towards the center of our galaxy. The bright star towards the center of the image is Gamma of Sagittarius. Image obtained from the 1.2m Schmidt UK telescope of Siding Spring. Orbiting round the centre of our Galaxy are found huge numbers of stars which are mostly faint, cool and often billions of years old. They are as ancient as the Galaxy itself. These stars are seen with the unaided eye as the hazy star clouds of the southern Milky Way, especially rich in Sagittarius. Our line of sight in this direction is strongly affected by dust, which reveals itself by both dimming the starlight passing through it and by selectively removing the blue light, changing the apparent colour to a deeper yellow. Though the colour change is only seen in photographs such as this, the dustiness of the Milky Way is obvious to the unaided eye. Near the centre of the picture is a region known as Baade's Window after the astro

Dark Stars and Nebulae in Sagittarius - The Star Clouds of Sagittarius - Star Field towards the center of our galaxy. The bright star towards the center of the image is Gamma of Sagittarius. Image obtained from the 1.2m Schmidt UK telescope of Siding Spring. Orbiting round the centre of our Galaxy are found huge numbers of stars which are mostly faint, cool and often billions of years old. They are as ancient as the Galaxy itself. These stars are seen with the unaided eye as the hazy star clouds of the southern Milky Way, especially rich in Sagittarius. Our line of sight in this direction is strongly affected by dust, which reveals itself by both dimming the starlight passing through it and by selectively removing the blue light, changing the apparent colour to a deeper yellow. Though the colour change is only seen in photographs such as this, the dustiness of the Milky Way is obvious to the unaided eye. Near the centre of the picture is a region known as Baade's Window after the astro

PIX4621371

The Swift Comet - Tuttle 12/1992 - Comet Swift - Tuttle 12/1992 - In August 2126, this comet is expected to pass very close to Earth; however, the risks of a collision with the Earth are very low. Comet Swift - Tuttle is expected to make an impressive pass near the earth in the year 2126. Dec 12 1992

The Swift Comet - Tuttle 12/1992 - Comet Swift - Tuttle 12/1992 - In August 2126, this comet is expected to pass very close to Earth; however, the risks of a collision with the Earth are very low. Comet Swift - Tuttle is expected to make an impressive pass near the earth in the year 2126. Dec 12 1992

PIX4570256

Constellation of Sobieski's ECU - Constellation of Scutum - Scutum (The Shield) was originally Scutum Sobiescianum, Sobieski's Shield, and was introduced in 1690 by the astronomer/cartographer Johannes Hevelius, one - time mayor of Gdansk (Danzig), in honour of Polish warrior - King John Sobieski. King John distiguished himself in defending his land against the Turks in 1683, turning them back at the gates of Vienna. For this he was hailed by the Pope and others as the savior of Vienna and Western European Civilization. Scutum was created in honor of this victory, and alpha Scuti named Ioannina (Greek for John) in his honor. Scutum is small, 84th in size out of the 88 modern constellation. It contains no bright stars, and seems to have been carved out of adjoining Aquila and Serpens simply embrace a fine piece of the Milky Way. However, the open clusters M11 and M26 can be found here

Constellation of Sobieski's ECU - Constellation of Scutum - Scutum (The Shield) was originally Scutum Sobiescianum, Sobieski's Shield, and was introduced in 1690 by the astronomer/cartographer Johannes Hevelius, one - time mayor of Gdansk (Danzig), in honour of Polish warrior - King John Sobieski. King John distiguished himself in defending his land against the Turks in 1683, turning them back at the gates of Vienna. For this he was hailed by the Pope and others as the savior of Vienna and Western European Civilization. Scutum was created in honor of this victory, and alpha Scuti named Ioannina (Greek for John) in his honor. Scutum is small, 84th in size out of the 88 modern constellation. It contains no bright stars, and seems to have been carved out of adjoining Aquila and Serpens simply embrace a fine piece of the Milky Way. However, the open clusters M11 and M26 can be found here

PIX4590553

Constellations of Lievre, Orion, Burin and part of Eridan - Eridanus, Orion, Lepus, and Caelum constellations - In the center left, the constellation of Lievre, above, Orion, from the center top to the bottom, the constellation of Eridan, down to the left, the Burin. At the top of the picture, the bright star is Aldebaran

Constellations of Lievre, Orion, Burin and part of Eridan - Eridanus, Orion, Lepus, and Caelum constellations - In the center left, the constellation of Lievre, above, Orion, from the center top to the bottom, the constellation of Eridan, down to the left, the Burin. At the top of the picture, the bright star is Aldebaran

PIX4592041

Constellation Ophiuchus - Constellation of Ophiuchus - The constellation Ophiuchus separates the constellation of the Snake into two parts. The constellation of Ophiuchus is located between Serpens Caput and Serpens Cauda, two parts of the constellation of Serpens. The southern part of Ophiuchus contains one of the darkest and most visually distinctive dark clouds of the Miky Way. It is popularly known as the Dark Horse nebula - - the body of the horse runs north - south and its legs point towards the bright star Antares. The hind quarters of the horse make up the (smoker's) Pipe nebula, with the stem pointing to Antares. The dust of forelegs reaches a long way in the direction of Antares, where it is illuminated by stars associated with Rho Ophiuchi to make a distinctive reflection nebula. The dusty clouds of the Dark Horse nebula hide the northern part of the Milky Way's central bulge. The southern part (in Sagittarius) is relatively unobscured. Without this dust the extent of the Mi

Constellation Ophiuchus - Constellation of Ophiuchus - The constellation Ophiuchus separates the constellation of the Snake into two parts. The constellation of Ophiuchus is located between Serpens Caput and Serpens Cauda, two parts of the constellation of Serpens. The southern part of Ophiuchus contains one of the darkest and most visually distinctive dark clouds of the Miky Way. It is popularly known as the Dark Horse nebula - - the body of the horse runs north - south and its legs point towards the bright star Antares. The hind quarters of the horse make up the (smoker's) Pipe nebula, with the stem pointing to Antares. The dust of forelegs reaches a long way in the direction of Antares, where it is illuminated by stars associated with Rho Ophiuchi to make a distinctive reflection nebula. The dusty clouds of the Dark Horse nebula hide the northern part of the Milky Way's central bulge. The southern part (in Sagittarius) is relatively unobscured. Without this dust the extent of the Mi

PIX4592342

Pisces Constellation - Constellation of Pisces - Pisces (the Fishes) is a large constellation of mostly quite faint stars at the edge of an ancient and huge part of the sky known as 'the Sea'. Pisces is said to resemble two fish, which are tied to a (alpha) Piscium by long lines. Alpha Piscium is known as Al Rischa in English, where it means 'the cord'. Some Greek mythologies have two men tethered to this star, though some of the other stars have fishy names. The Sun is in Pisces from March 13 to April 19, and it crosses the ecliptic on March 21, which marks the vernal Equinox, the first day of autumn in the southern hemisphere. This used to be called the first point in Aries, but precession has now moved it into Pisces. However, this point in the sky is the origin of right ascension (RA) in the astronomical equatorial coordinate sytem, and because it moves with precession, RA and Dec are defined at a certain date

Pisces Constellation - Constellation of Pisces - Pisces (the Fishes) is a large constellation of mostly quite faint stars at the edge of an ancient and huge part of the sky known as 'the Sea'. Pisces is said to resemble two fish, which are tied to a (alpha) Piscium by long lines. Alpha Piscium is known as Al Rischa in English, where it means 'the cord'. Some Greek mythologies have two men tethered to this star, though some of the other stars have fishy names. The Sun is in Pisces from March 13 to April 19, and it crosses the ecliptic on March 21, which marks the vernal Equinox, the first day of autumn in the southern hemisphere. This used to be called the first point in Aries, but precession has now moved it into Pisces. However, this point in the sky is the origin of right ascension (RA) in the astronomical equatorial coordinate sytem, and because it moves with precession, RA and Dec are defined at a certain date

PIX4593517

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