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Constellations of Cephee, Cassiopee and Little Bear - Across the North Celestial Pole, Cassiopeia to Ursa Mino

Constellations of Cephee, Cassiopee and Little Bear - Across the North Celestial Pole, Cassiopeia to Ursa Mino

PIX4589859

Orion Nebula (M42 - 43) - The Orion Nebula - Located 1500 years ago - the Orion Nebula is the closest region to the formation of stars of the Sun. Image obtained with Siding Spring's 3.9m telescope. The Orion Nebula is famous for a number of reasons. It is the nearest bright nebula to us and can be seen with the naked eye. Its brightness led to it being the first nebula ever photographed (in 1882) and its proximity (1500 light years) means that we know more about it than any other star - forming region. It is also in a very active stage of star formation and it is perfectly placed for us to explore the intimate details of the birth of stars. The inner regions are glowing mainly in the red light of excited hydrogen, which together with some green emission from oxygen give the centre of the nebula a yellowish colour. The energy for this spectacular display comes from the small cluster of stars in the brightest part of the nebula. Three, five - minute exposures were used to make this pict

Orion Nebula (M42 - 43) - The Orion Nebula - Located 1500 years ago - the Orion Nebula is the closest region to the formation of stars of the Sun. Image obtained with Siding Spring's 3.9m telescope. The Orion Nebula is famous for a number of reasons. It is the nearest bright nebula to us and can be seen with the naked eye. Its brightness led to it being the first nebula ever photographed (in 1882) and its proximity (1500 light years) means that we know more about it than any other star - forming region. It is also in a very active stage of star formation and it is perfectly placed for us to explore the intimate details of the birth of stars. The inner regions are glowing mainly in the red light of excited hydrogen, which together with some green emission from oxygen give the centre of the nebula a yellowish colour. The energy for this spectacular display comes from the small cluster of stars in the brightest part of the nebula. Three, five - minute exposures were used to make this pict

PIX4617657

Spiral Galaxy NGC 253 in Sculptor - Spiral galaxy NGC 253 in Sculptor - NGC 253 is the brightest galaxy of the Sculptor's group, the closest galaxy group to the Local Group. It is about 10 million light years away. Image made with Siding Spring's 3.9m telescope in 1975. A mere 10 million light years away, NGC 253 is one of the nearest spiral galaxies, a member of a small group straggling across the southern constellation of Sculptor. It appears elongated because we see it almost edge - on. This galaxy is also one of the dustiest galaxies known and much of its internal detail is hidden by obscuring matter which can be seen as dark patches against the background stars. Despite the obscuration, two spiral arms and many bluish clusters of stars can be seen around the edge of the galaxy. NGC 253 is so close to us that some of the brightest stars are apparent as individuals within the spiral arms

Spiral Galaxy NGC 253 in Sculptor - Spiral galaxy NGC 253 in Sculptor - NGC 253 is the brightest galaxy of the Sculptor's group, the closest galaxy group to the Local Group. It is about 10 million light years away. Image made with Siding Spring's 3.9m telescope in 1975. A mere 10 million light years away, NGC 253 is one of the nearest spiral galaxies, a member of a small group straggling across the southern constellation of Sculptor. It appears elongated because we see it almost edge - on. This galaxy is also one of the dustiest galaxies known and much of its internal detail is hidden by obscuring matter which can be seen as dark patches against the background stars. Despite the obscuration, two spiral arms and many bluish clusters of stars can be seen around the edge of the galaxy. NGC 253 is so close to us that some of the brightest stars are apparent as individuals within the spiral arms

PIX4609065

Constellation of Taurus - Constellation of Taurus - Taurus, (the Bull) is one of the most ancient constellations, and appears in artefacts as old as western civilisation itself. The bull is still a figure of strength and fertility in cultures around the world. In the sky the distinctive 'V' shape of his head and long horns tipped by beta (ss) and zeta Tau is easily recognised. If the purpose of the horns was in doubt, the English name for ss Tau is Alnath, meaning 'the butting one'. The bull's glowing red eye of Aldebaran completes the picture, and its location between the delicate Pleiades and the aggressive stance of Orion makes Taurus hard to overlook. Despite its masculine connotations, the constellation is rich in female icons; both the Hyades and Pleiades star clusters are daughters of Atlas and both are important astronomically. The Pleiades (or the Seven Sisters) are a group of young stars at a distance of about 440 light years and on long exposure photographs are seen to be em

Constellation of Taurus - Constellation of Taurus - Taurus, (the Bull) is one of the most ancient constellations, and appears in artefacts as old as western civilisation itself. The bull is still a figure of strength and fertility in cultures around the world. In the sky the distinctive 'V' shape of his head and long horns tipped by beta (ss) and zeta Tau is easily recognised. If the purpose of the horns was in doubt, the English name for ss Tau is Alnath, meaning 'the butting one'. The bull's glowing red eye of Aldebaran completes the picture, and its location between the delicate Pleiades and the aggressive stance of Orion makes Taurus hard to overlook. Despite its masculine connotations, the constellation is rich in female icons; both the Hyades and Pleiades star clusters are daughters of Atlas and both are important astronomically. The Pleiades (or the Seven Sisters) are a group of young stars at a distance of about 440 light years and on long exposure photographs are seen to be em

PIX4594065

Vote for the Zionist Party #6, 1917 (poster)

Vote for the Zionist Party #6, 1917 (poster)

SSI2526762

Globular cluster NGC 6723 in Sagittarius - Globular cluster NGC 6723 in Sagittarius - This cluster of stars is located about 30,000 years ago - light from Earth

Globular cluster NGC 6723 in Sagittarius - Globular cluster NGC 6723 in Sagittarius - This cluster of stars is located about 30,000 years ago - light from Earth

PIX4565034

President Dwight D. Eisenhower (b/w photo)

President Dwight D. Eisenhower (b/w photo)

UIG2621459

President Eisenhower Golfing (b/w photo)

President Eisenhower Golfing (b/w photo)

UIG2621454

Germany, Berlin: Golden Cupola of the New Synagogue

Germany, Berlin: Golden Cupola of the New Synagogue

DPA2535901

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

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

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

Christ In Majesty, c.1867 (stained glass)

Christ In Majesty, c.1867 (stained glass)

Hassam, Alfred (1842-69)

Alastair Carew-Cox

CCX3474781

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

Constellation of Belier - Constellation of Aries - Constellation of Belier and clusters of Pleiades (in the Taurus). Although inconspicuous, Aries is one of the constellations of the zodiac and from ancient times has been represented by a ram, the same ram whose golden fleece was sought by Jason and the Argonauts in the great ship Argo Navis. For more than 2000 years it also of astronomical importance because it was the constellation where the Sun crossed the celestial equator (ecliptic) each year at the vernal equinox, marking the first point in Aries from which right ascension is measured. Precession has now carried this point into Pisces. The constellation is the 39th largest in the sky and covers about 440 square degrees. The best - known object in this field is the Pleiades star cluster (M45 in Taurus)

Constellation of Belier - Constellation of Aries - Constellation of Belier and clusters of Pleiades (in the Taurus). Although inconspicuous, Aries is one of the constellations of the zodiac and from ancient times has been represented by a ram, the same ram whose golden fleece was sought by Jason and the Argonauts in the great ship Argo Navis. For more than 2000 years it also of astronomical importance because it was the constellation where the Sun crossed the celestial equator (ecliptic) each year at the vernal equinox, marking the first point in Aries from which right ascension is measured. Precession has now carried this point into Pisces. The constellation is the 39th largest in the sky and covers about 440 square degrees. The best - known object in this field is the Pleiades star cluster (M45 in Taurus)

PIX4589193

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

PIX4609776

Constellation of the Southern Cross - The Southern cross - Image obtained from Kangaroo Island, Australia. The Southern Cross and Carina from Kangaroo Island, Australia

Constellation of the Southern Cross - The Southern cross - Image obtained from Kangaroo Island, Australia. The Southern Cross and Carina from Kangaroo Island, Australia

David Miller

PIX4590228

French passport and interfaith. Symbols of islam, judaism and christianity. (photo)

French passport and interfaith. Symbols of islam, judaism and christianity. (photo)

GNG5937620

Interior of the Great Synagogue in Budapest (Dohany Street Synagogue)., Budapest, Hongrie

Interior of the Great Synagogue in Budapest (Dohany Street Synagogue)., Budapest, Hongrie

GNG5279271

Interior of the Great Synagogue in Budapest (Dohany Street Synagogue)., Budapest, Hongrie

Interior of the Great Synagogue in Budapest (Dohany Street Synagogue)., Budapest, Hongrie

GNG5279284

Banknotes of euro currency. Christianity, Islamic and Judaism finance and economy concept with Jewish Star, Prayer Beads and Crucifix. Interreligious ( interfaith ) symbols. (photo)

Banknotes of euro currency. Christianity, Islamic and Judaism finance and economy concept with Jewish Star, Prayer Beads and Crucifix. Interreligious ( interfaith ) symbols. (photo)

GNG5936255

Germany: Propaganda poster portraying jazz and especially saxophone music as 'entartete musik' or 'degenerate music', complete with stereotyped black musician and Star of David, c. 1938

Germany: Propaganda poster portraying jazz and especially saxophone music as 'entartete musik' or 'degenerate music', complete with stereotyped black musician and Star of David, c. 1938

David Henley

PFH1189765

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

Constellation of Sextant - Constellation of Sextans - Constellation of Sextant; below part of the constellation Hydra. At the top of the picture, the bright star is Regulus, of the Lion. Sextans, and part of Hydra. Top of image, the bright star is Regulus in Leo. Sextans, (the Sextant, originally Sextans Uraniae), is small, faint, equatorial constellation south of Leo, framed by the bright stars Regulus to the north and Alphard to the west. It was introduced by Johannes Hevelius in 1687 to commemorate the instrument with which he continued to measure star positions for long after the telescope had been invented. This small and insignificant constellation measures a little more than 17 degrees on a side (about 313 degrees square) and is ranked 45th in area out of the 88 modern constellations. In contrast is the winding collection of stars that make up the head of the Hydra, the Water Snake. This is the largest constellation in the sky, extending over 1300 square degrees, and though the

Constellation of Sextant - Constellation of Sextans - Constellation of Sextant; below part of the constellation Hydra. At the top of the picture, the bright star is Regulus, of the Lion. Sextans, and part of Hydra. Top of image, the bright star is Regulus in Leo. Sextans, (the Sextant, originally Sextans Uraniae), is small, faint, equatorial constellation south of Leo, framed by the bright stars Regulus to the north and Alphard to the west. It was introduced by Johannes Hevelius in 1687 to commemorate the instrument with which he continued to measure star positions for long after the telescope had been invented. This small and insignificant constellation measures a little more than 17 degrees on a side (about 313 degrees square) and is ranked 45th in area out of the 88 modern constellations. In contrast is the winding collection of stars that make up the head of the Hydra, the Water Snake. This is the largest constellation in the sky, extending over 1300 square degrees, and though the

PIX4594016

Nebuleuse Barnard 86 & open cluster NGC 6520 - Dark nebula Barnard 86 and open cluster NGC 6520 - NGC 6520, is a cluster of young stars, aged a few million years. To its right is the dark nebula, Barnard 86, a cloud of molecular gas and dust, very cold, in which these stars have become formed. In the background, the billions of years old stars of Sagittarius. NGC 6520 is a small cluster of young blue stars. In the same region is a dark cloud, Barnard 86. The cluster and cloud are probably associated and the dust is visible only because it blocks out light from the myriads of stars beyond. On the distant background, old yellowish stars in Sagittarius are visible in vast numbers

Nebuleuse Barnard 86 & open cluster NGC 6520 - Dark nebula Barnard 86 and open cluster NGC 6520 - NGC 6520, is a cluster of young stars, aged a few million years. To its right is the dark nebula, Barnard 86, a cloud of molecular gas and dust, very cold, in which these stars have become formed. In the background, the billions of years old stars of Sagittarius. NGC 6520 is a small cluster of young blue stars. In the same region is a dark cloud, Barnard 86. The cluster and cloud are probably associated and the dust is visible only because it blocks out light from the myriads of stars beyond. On the distant background, old yellowish stars in Sagittarius are visible in vast numbers

PIX4621326

Nebula Trifide (M20) in the constellation Sagittarius - Trifid nebula (M20) in Sagittarius - View 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. The spectacular Trifid nebula (Messier 20) is one of the best known in the sky. It is a striking mixture of brilliant red light emitted from excited hydrogen gas and the soft blue glow of a reflection nebula. The blue arises from starlight, scattered by dust particles between the stars. The size of the particles is minute, similar to those of smoke, which also has a bluish hue. However, the scattered light is not a pure blue, and if we see it through a medium that is yellow (i.e. absorbs blue light) some green colouration remains. This effect can be seen in some of the darker parts of the faint reflection nebula that surrounds the Trifid, where partial absorption of light by foreground dust provides a yellow 'filte

Nebula Trifide (M20) in the constellation Sagittarius - Trifid nebula (M20) in Sagittarius - View 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. The spectacular Trifid nebula (Messier 20) is one of the best known in the sky. It is a striking mixture of brilliant red light emitted from excited hydrogen gas and the soft blue glow of a reflection nebula. The blue arises from starlight, scattered by dust particles between the stars. The size of the particles is minute, similar to those of smoke, which also has a bluish hue. However, the scattered light is not a pure blue, and if we see it through a medium that is yellow (i.e. absorbs blue light) some green colouration remains. This effect can be seen in some of the darker parts of the faint reflection nebula that surrounds the Trifid, where partial absorption of light by foreground dust provides a yellow 'filte

PIX4619447

Hubble Nebula (NGC 2261) in Unicorn - NGC 2261, Hubble's variable nebula - The Hubble Nebula is a weak nebulosite that surrounds the star R Monocerotis (R Mon), the bright star at the bottom of the nebula. The mass of the star R Mon is about 10 times that of the sun. It is approximately 2600 light years away and is only 300,000 years old. Image obtained by Siding Spring's 3.9m telescope. Hubble's variable nebula is in Monoceros and was the first object to be photographed with the famous 200 inch Hale Telescope at Palomar in 1948. This curious object is a reflection nebula in which is embedded the star R Monocerotis. Variations in the appearance of the nebula were noted by the American astronomer Edwin Hubble in 1916. They are probably caused by opaque clouds of dust passing between the hidden star and the outskirts of the nebula we see, the moving shadows changing the apparent form of the glowing dust in an irregular way. This picture was made from three AAT plates taken over several y

Hubble Nebula (NGC 2261) in Unicorn - NGC 2261, Hubble's variable nebula - The Hubble Nebula is a weak nebulosite that surrounds the star R Monocerotis (R Mon), the bright star at the bottom of the nebula. The mass of the star R Mon is about 10 times that of the sun. It is approximately 2600 light years away and is only 300,000 years old. Image obtained by Siding Spring's 3.9m telescope. Hubble's variable nebula is in Monoceros and was the first object to be photographed with the famous 200 inch Hale Telescope at Palomar in 1948. This curious object is a reflection nebula in which is embedded the star R Monocerotis. Variations in the appearance of the nebula were noted by the American astronomer Edwin Hubble in 1916. They are probably caused by opaque clouds of dust passing between the hidden star and the outskirts of the nebula we see, the moving shadows changing the apparent form of the glowing dust in an irregular way. This picture was made from three AAT plates taken over several y

PIX4618577

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

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

Constellations of the Great Bear and Little Bear - Constellations of Ursa Major and Ursa Minor - On the right, the large trolley, asterism of the Great Bear; on the left, the small trolley, asterism of the Little Bear that houses the polar star, the star that currently indicates the position of the northern Celestial pole, at the end of the handle of the pan

Constellations of the Great Bear and Little Bear - Constellations of Ursa Major and Ursa Minor - On the right, the large trolley, asterism of the Great Bear; on the left, the small trolley, asterism of the Little Bear that houses the polar star, the star that currently indicates the position of the northern Celestial pole, at the end of the handle of the pan

PIX4591367

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

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

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

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

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

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. 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

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

Venus pres des Pleiades - Venus among the Pleiades, April 6, 1999 - Venus pres de l'amas des Pleiades April 6, 1999. Venus among the Pleiades, April 6, 1999

Venus pres des Pleiades - Venus among the Pleiades, April 6, 1999 - Venus pres de l'amas des Pleiades April 6, 1999. Venus among the Pleiades, April 6, 1999

PIX4586759

Dragon Constellation - Constellation of Draco - Dragon Constellation with part of the Big Bear and Little Bear. Draco (the Dragon) is said to represent Ladon, the multi - headed dragon slaughtered by Hercules, an act necessary to obtain the golden apples from the garden of Hesperides as the 11th of his 12 labours. Other ancient, dragonocentric legends exist. The constellation itself is rather indistinct with few bright stars, but it is a large and rambling construction wrapped around the north celestial pole. It extends from close to the Pole Star to more than 40 degrees of delination south of it and wanders over 11 hours of Right Ascension between Hercules and the Big Dipper. It is the 8th largest constelation in terms of area, which is over 1000 square degrees. This image also contains the constellation of Ursa Minor

Dragon Constellation - Constellation of Draco - Dragon Constellation with part of the Big Bear and Little Bear. Draco (the Dragon) is said to represent Ladon, the multi - headed dragon slaughtered by Hercules, an act necessary to obtain the golden apples from the garden of Hesperides as the 11th of his 12 labours. Other ancient, dragonocentric legends exist. The constellation itself is rather indistinct with few bright stars, but it is a large and rambling construction wrapped around the north celestial pole. It extends from close to the Pole Star to more than 40 degrees of delination south of it and wanders over 11 hours of Right Ascension between Hercules and the Big Dipper. It is the 8th largest constelation in terms of area, which is over 1000 square degrees. This image also contains the constellation of Ursa Minor

PIX4590525

French passport and interfaith. Symbols of islam, judaism and christianity. (photo)

French passport and interfaith. Symbols of islam, judaism and christianity. (photo)

GNG5937619

Kippas, Jerusalem, Israel

Kippas, Jerusalem, Israel

GNG5280237

Nebula in the galaxy NGC 6822 - Bubble nebulae in NGC 6822 - Nebula in the irregular galaxy NGC 6822, adjacent to our galaxy. This gas bubble houses massive stars known as Wolf - Rayet. NGC 6822 is a nearby irregular galaxy reminiscent of the Large Magellanic Cloud (LMC). Like the LMC it contains many, extremely hot stars of the Wolf - Rayet type, stars which often have intense stellar winds blasting from their surfaces. Small groups of such stars are found at the centres of the bubble nebulae seen here, which are the result of the stellar winds colliding with the more or less stationary interstellar medium in NGC 6822. At the interface of the collision, the interstellar medium glows, producing a thin, luminous bubble. Such bubbles are rare in the more turbulent Milky Way galaxy, but Henize 70 in the Large Magellanic Cloud is similar

Nebula in the galaxy NGC 6822 - Bubble nebulae in NGC 6822 - Nebula in the irregular galaxy NGC 6822, adjacent to our galaxy. This gas bubble houses massive stars known as Wolf - Rayet. NGC 6822 is a nearby irregular galaxy reminiscent of the Large Magellanic Cloud (LMC). Like the LMC it contains many, extremely hot stars of the Wolf - Rayet type, stars which often have intense stellar winds blasting from their surfaces. Small groups of such stars are found at the centres of the bubble nebulae seen here, which are the result of the stellar winds colliding with the more or less stationary interstellar medium in NGC 6822. At the interface of the collision, the interstellar medium glows, producing a thin, luminous bubble. Such bubbles are rare in the more turbulent Milky Way galaxy, but Henize 70 in the Large Magellanic Cloud is similar

PIX4620956

Globular cluster Hodge 11 - Globular cluster Hodge 11 - This cluster of stars is located about 160,000 years ago - light in the Big Magellan Cloud

Globular cluster Hodge 11 - Globular cluster Hodge 11 - This cluster of stars is located about 160,000 years ago - light in the Big Magellan Cloud

PIX4565244

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

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

Stars - The Southern Cross - Alpha and Beta of Centaur - Southern Cross and pointers - Star trails - Because of the Earth's rotation, leaving the camera open, the stars advance towards the background of the sky. During the installation, gradually changing the focal length of the lens, the stars spread out and reveal their true color. Here it is the constellation of the Southern Cross (center right) and the Centaurus Alpha and Beta stars, in the center below, that are photographed in this way during a 30-minute pose. Star images are point sources of light of widely varying intensity. Normally, no single photographic exposure on colour film can capture their subtle colours. Those stars whose intensity is just right for their colour to be recorded appear insignificant on the photograph, while anything brighter is overexposed and washed out. By changing the focus of the lens during a star trail exposure, star images are spread out over the film surface. This effectively changes the amount

Stars - The Southern Cross - Alpha and Beta of Centaur - Southern Cross and pointers - Star trails - Because of the Earth's rotation, leaving the camera open, the stars advance towards the background of the sky. During the installation, gradually changing the focal length of the lens, the stars spread out and reveal their true color. Here it is the constellation of the Southern Cross (center right) and the Centaurus Alpha and Beta stars, in the center below, that are photographed in this way during a 30-minute pose. Star images are point sources of light of widely varying intensity. Normally, no single photographic exposure on colour film can capture their subtle colours. Those stars whose intensity is just right for their colour to be recorded appear insignificant on the photograph, while anything brighter is overexposed and washed out. By changing the focus of the lens during a star trail exposure, star images are spread out over the film surface. This effectively changes the amount

PIX4581418

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

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

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

PIX4612513

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

Central region of the spiral galaxy NGC 300 in the Sculptor - Nucleus of spiral galaxy NGC 300 in Sculptor - Located about 7 million years ago - light from Earth, the spiral galaxy NGC 300 belongs to the Sculptor's group. The photo taken by Siding Spring's 3.9m telescope highlights the nucleus of this galaxy. At the centre of the spiral arms of NGC 300 is an unusually compact, star - like nucleus. It is surrounded by a faint but extensive yellow haze, consisting of millions of faint, cool stars. This is the older population, or 'bulge' of NGC 300, a distant equivalent to the (much more numerous) stars that we see in our own galaxy as the brightest part of the Milky Way in Sagittarius

Central region of the spiral galaxy NGC 300 in the Sculptor - Nucleus of spiral galaxy NGC 300 in Sculptor - Located about 7 million years ago - light from Earth, the spiral galaxy NGC 300 belongs to the Sculptor's group. The photo taken by Siding Spring's 3.9m telescope highlights the nucleus of this galaxy. At the centre of the spiral arms of NGC 300 is an unusually compact, star - like nucleus. It is surrounded by a faint but extensive yellow haze, consisting of millions of faint, cool stars. This is the older population, or 'bulge' of NGC 300, a distant equivalent to the (much more numerous) stars that we see in our own galaxy as the brightest part of the Milky Way in Sagittarius

PIX4609189

Centaurus A elliptical galaxy (NGC 5128) in the Centaurus - Galaxy Centaurus A (NGC 5128) - The galaxy NGC 5128 is located about 13 million years away from Earth. 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. 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 younger, blue stars can be seen at the edges of the dust cloud. One of the nearer galaxies, 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

Centaurus A elliptical galaxy (NGC 5128) in the Centaurus - Galaxy Centaurus A (NGC 5128) - The galaxy NGC 5128 is located about 13 million years away from Earth. 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. 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 younger, blue stars can be seen at the edges of the dust cloud. One of the nearer galaxies, 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

PIX4612201

Globular clusters NGC 6522 and NGC 6528 in Sagittarius - Baade's Window around NGC 6522 - NGC 6522 (right) and NGC 6528 (left) are two clusters located about 25,000 years ago - light from Earth towards the center of our galaxy

Globular clusters NGC 6522 and NGC 6528 in Sagittarius - Baade's Window around NGC 6522 - NGC 6522 (right) and NGC 6528 (left) are two clusters located about 25,000 years ago - light from Earth towards the center of our galaxy

PIX4564863

Constellations of Cephee, Cassiopee and Little Bear - Across the North Celestial Pole, Cassiopeia to Ursa Mino

Constellations of Cephee, Cassiopee and Little Bear - Across the North Celestial Pole, Cassiopeia to Ursa Mino

PIX4589857

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

Constellation Belier - Aries constellation - Constellation Belier and cluster of Pleiades (in the Taurus). Although inconspicuous, Aries is one of the constellations of the zodiac and from ancient times has been represented by a ram, the same ram whose golden fleece was sought by Jason and the Argonauts in the great ship Argo Navis. For more than 2000 years it also of astronomical importance because it was the constellation where the Sun crossed the celestial equator (ecliptic) each year at the vernal equinox, marking the first point in Aries from which right ascension is measured. Precession has now carried this point into Pisces. The constellation is the 39th largest in the sky and covers about 440 square degrees. The best - known object in this field is the Pleiades star cluster (M45 in Taurus)

Constellation Belier - Aries constellation - Constellation Belier and cluster of Pleiades (in the Taurus). Although inconspicuous, Aries is one of the constellations of the zodiac and from ancient times has been represented by a ram, the same ram whose golden fleece was sought by Jason and the Argonauts in the great ship Argo Navis. For more than 2000 years it also of astronomical importance because it was the constellation where the Sun crossed the celestial equator (ecliptic) each year at the vernal equinox, marking the first point in Aries from which right ascension is measured. Precession has now carried this point into Pisces. The constellation is the 39th largest in the sky and covers about 440 square degrees. The best - known object in this field is the Pleiades star cluster (M45 in Taurus)

PIX4589253

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