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Nebula NGC 6334 in the Scorpion - The 'reddened' nebulosity of NGC 6334 - The nebula NGC 6334 is located about 5500 years - light from Earth. Image made with the 1.2m Telescope of Schmidt UK from Siding Spring. The star - forming nebula NGC 6334 shows 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. This nebula is quite nearby (5500 light years) but located close to the Galactic plane and are buried in the dust of the Milky Way. Careful measurement of the colour

Nebula NGC 6334 in the Scorpion - The 'reddened' nebulosity of NGC 6334 - The nebula NGC 6334 is located about 5500 years - light from Earth. Image made with the 1.2m Telescope of Schmidt UK from Siding Spring. The star - forming nebula NGC 6334 shows 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. This nebula is quite nearby (5500 light years) but located close to the Galactic plane and are buried in the dust of the Milky Way. Careful measurement of the colour

PIX4619360

Thousands of people in the coastal area took shelter on the embankment and buildings nearby after five to seven feet high tidal surge flooded their homes, during hurricane Aila. The cyclone struck the coastal areas of Bangladesh on May 25, 2009 causing severe damage to crops, homes and lives. About 200 people died and more than thousand are missing. Nearly 200,000 people are still trapped in water. More than 500 shrimp farms washed away in five to seven feet high tidal surge. Thousands of people are made homeless and there is a severe crisis of food and pure drinking water. Satkhira, Bangladesh. May 28, 2009. (photo)

Thousands of people in the coastal area took shelter on the embankment and buildings nearby after five to seven feet high tidal surge flooded their homes, during hurricane Aila. The cyclone struck the coastal areas of Bangladesh on May 25, 2009 causing severe damage to crops, homes and lives. About 200 people died and more than thousand are missing. Nearly 200,000 people are still trapped in water. More than 500 shrimp farms washed away in five to seven feet high tidal surge. Thousands of people are made homeless and there is a severe crisis of food and pure drinking water. Satkhira, Bangladesh. May 28, 2009. (photo)

UIG800031

Thousands of people in the coastal area took shelter on the embankment and buildings nearby after five to seven feet high tidal surge flooded their homes, during hurricane Aila. The cyclone struck the coastal areas of Bangladesh on May 25, 2009 causing severe damage to crops, homes and lives. About 200 people died and more than thousand are missing. Nearly 200,000 people are still trapped in water. More than 500 shrimp farms washed away in five to seven feet high tidal surge. Thousands of people are made homeless and there is a severe crisis of food and pure drinking water. Satkhira, Bangladesh. May 28, 2009. (photo)

Thousands of people in the coastal area took shelter on the embankment and buildings nearby after five to seven feet high tidal surge flooded their homes, during hurricane Aila. The cyclone struck the coastal areas of Bangladesh on May 25, 2009 causing severe damage to crops, homes and lives. About 200 people died and more than thousand are missing. Nearly 200,000 people are still trapped in water. More than 500 shrimp farms washed away in five to seven feet high tidal surge. Thousands of people are made homeless and there is a severe crisis of food and pure drinking water. Satkhira, Bangladesh. May 28, 2009. (photo)

UIG800029

People in the coastal area took shelter on the embankment and buildings nearby after five to seven feet high tidal surge flooded their homes, during hurricane Aila. The cyclone struck the coastal areas of Bangladesh on May 25, 2009 causing severe damage to crops, homes and lives. About 200 people died and more than thousand are missing. Nearly 200,000 people are still trapped in water. More than 500 shrimp farms washed away in five to seven feet high tidal surge. Thousands of people are made homeless and there is a severe crisis of food and pure drinking water. Satkhira, Bangladesh. May 28, 2009. (photo)

People in the coastal area took shelter on the embankment and buildings nearby after five to seven feet high tidal surge flooded their homes, during hurricane Aila. The cyclone struck the coastal areas of Bangladesh on May 25, 2009 causing severe damage to crops, homes and lives. About 200 people died and more than thousand are missing. Nearly 200,000 people are still trapped in water. More than 500 shrimp farms washed away in five to seven feet high tidal surge. Thousands of people are made homeless and there is a severe crisis of food and pure drinking water. Satkhira, Bangladesh. May 28, 2009. (photo)

UIG800028

Two Views of a Dead Boar with a Mastiff and two other Dogs

Two Views of a Dead Boar with a Mastiff and two other Dogs

Hackert, Jacob-Philippe (1737-1807)

USB1160438

Boats on the Sangker River, Cambodia (photo)

Boats on the Sangker River, Cambodia (photo)

Sergi Reboredo

SRB1202740

Irregular galaxy NGC 3239 in the Lion - Irregular galaxy NGC 3239 in Leo - The irregular galaxy NGC 3239 is located 25 million light years ago in the constellation Lion. Also visible on this image is the supernova SN 2012a (under the bright star in the center of the image). About 40,000 light - years across, irregular galaxy NGC 3239 lies near the center of this field of galaxies in the galaxy rich constellation Leo. At a distance of only 25 million light - years it dominates the frame, sporting a peculiar arrangement of structures, young blue star clusters and star forming regions, suggesting that NGC 3239 (aka Arp 263) is the result of a galaxy merger. Appearing almost on top of the pretty galaxy is a bright, spiky, foreground star, a nearby member of our own Milky Way galaxy almost directly along our line - of - sight to NGC 3239. Still, NGC 3239 is notable for hosting this year's first confirmed supernova, designated SN 2012A. SN 2012A is just below and right of the bright foregrou

Irregular galaxy NGC 3239 in the Lion - Irregular galaxy NGC 3239 in Leo - The irregular galaxy NGC 3239 is located 25 million light years ago in the constellation Lion. Also visible on this image is the supernova SN 2012a (under the bright star in the center of the image). About 40,000 light - years across, irregular galaxy NGC 3239 lies near the center of this field of galaxies in the galaxy rich constellation Leo. At a distance of only 25 million light - years it dominates the frame, sporting a peculiar arrangement of structures, young blue star clusters and star forming regions, suggesting that NGC 3239 (aka Arp 263) is the result of a galaxy merger. Appearing almost on top of the pretty galaxy is a bright, spiky, foreground star, a nearby member of our own Milky Way galaxy almost directly along our line - of - sight to NGC 3239. Still, NGC 3239 is notable for hosting this year's first confirmed supernova, designated SN 2012A. SN 2012A is just below and right of the bright foregrou

Adam Block

PIX4610534

M87 elliptical galaxy in Virgo - M87 elliptical galaxy in Virgo - The M87 galaxy (NGC 4486) is located about 60 million years ago - light from Earth, in the heart of the Virgin's cluster. M87 is the brightest radio source in the constellation, it is also called Virgo A. Image made with Siding Spring's 3.9m telescope. Messier 87 (NGC 4486) lies near the centre of the nearby cluster of galaxies in Virgo at a distance of about 60 million light years. Although the physical boundaries of elliptical galaxies are not well defined, their mass can be, and by any standards M87 is enormous. It contains several thousand billion stars. Associated with this giant galaxy are large numbers of globular clusters, visible in this photograph as the cloud of slightly fuzzy objects around it. Like all ellipticals, M 87 is composed mainly of old stars and is largely devoid of the materials needed to make new ones. The galaxy is not inert however; high energy X - rays have been detected from an extensive oute

M87 elliptical galaxy in Virgo - M87 elliptical galaxy in Virgo - The M87 galaxy (NGC 4486) is located about 60 million years ago - light from Earth, in the heart of the Virgin's cluster. M87 is the brightest radio source in the constellation, it is also called Virgo A. Image made with Siding Spring's 3.9m telescope. Messier 87 (NGC 4486) lies near the centre of the nearby cluster of galaxies in Virgo at a distance of about 60 million light years. Although the physical boundaries of elliptical galaxies are not well defined, their mass can be, and by any standards M87 is enormous. It contains several thousand billion stars. Associated with this giant galaxy are large numbers of globular clusters, visible in this photograph as the cloud of slightly fuzzy objects around it. Like all ellipticals, M 87 is composed mainly of old stars and is largely devoid of the materials needed to make new ones. The galaxy is not inert however; high energy X - rays have been detected from an extensive oute

PIX4611461

Exoplanete GJ 1214 b - Exoplanet GJ 1214 b - Illustration showing the transit of the extrasolar planet GJ 1214 b in front of its star, the red dwarf GJ 1214, in the constellation Ophiuchus. GJ 1214 b is a super Earth, six times the mass of the Earth, which has an atmosphere but is too inhospitable to shelter life as we know it. This artist's impression shows how the super - Earth surrounding the nearby star GJ1214 may look. Discovered by the Mearth project and investigated further by the HARPS spectrograph on ESO's 3.6 - metre telescope at La Silla, GJ1214b is the second super - Earth exoplanet for which astronomers have determined the mass and radius, giving vital clues about its structure. It is also the first super - Earth around which an atmosphere has been found. The exoplanet, orbiting a small star only 40 light - years away from us, thus opens dramatic new perspectives in the quest for habitable worlds. The planet, GJ1214b, has a mass about six times that of Earth and its interi

Exoplanete GJ 1214 b - Exoplanet GJ 1214 b - Illustration showing the transit of the extrasolar planet GJ 1214 b in front of its star, the red dwarf GJ 1214, in the constellation Ophiuchus. GJ 1214 b is a super Earth, six times the mass of the Earth, which has an atmosphere but is too inhospitable to shelter life as we know it. This artist's impression shows how the super - Earth surrounding the nearby star GJ1214 may look. Discovered by the Mearth project and investigated further by the HARPS spectrograph on ESO's 3.6 - metre telescope at La Silla, GJ1214b is the second super - Earth exoplanet for which astronomers have determined the mass and radius, giving vital clues about its structure. It is also the first super - Earth around which an atmosphere has been found. The exoplanet, orbiting a small star only 40 light - years away from us, thus opens dramatic new perspectives in the quest for habitable worlds. The planet, GJ1214b, has a mass about six times that of Earth and its interi

PIX4573892

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

Thailand: Ganesh image at Chiang Mai College of Drama and Arts, Suriyawong Soi 5, Chiang Mai

Thailand: Ganesh image at Chiang Mai College of Drama and Arts, Suriyawong Soi 5, Chiang Mai

David Henley

PFH1184600

Nebula N159 in the Great Magellan Cloud - N159 star forming region in Large Magellanic Cloud (LMC): N159 is a star-forming region located in the galaxy of the Great Magellan Cloud. Image obtained by the Hubble Space Telescope (HST) - This shot from the NASA/ESA Hubble Space Telescope shows a maelstrom of glowing gas and dark dust within one of the Milky Way's satellite galaxies, the Large Magellanic Cloud (LMC). This stormy scene shows a stellar nursery known as N159, an HII region over 150 light-years across. N159 contains many hot young stars. These stars are emitting intense ultraviolet light, which causes nearby hydrogen gas to glow, and torrential stellar winds, which are carving out ridges, arcs, and filaments from the surrounding material. At the heart of this cosmic cloud lies the Papillon Nebula, a butterfly-shaped region of nebulosity. This small, dense object is classified as a High-Excitation Blob, and is thought to be tightly linked to the early stages of massive star form

Nebula N159 in the Great Magellan Cloud - N159 star forming region in Large Magellanic Cloud (LMC): N159 is a star-forming region located in the galaxy of the Great Magellan Cloud. Image obtained by the Hubble Space Telescope (HST) - This shot from the NASA/ESA Hubble Space Telescope shows a maelstrom of glowing gas and dark dust within one of the Milky Way's satellite galaxies, the Large Magellanic Cloud (LMC). This stormy scene shows a stellar nursery known as N159, an HII region over 150 light-years across. N159 contains many hot young stars. These stars are emitting intense ultraviolet light, which causes nearby hydrogen gas to glow, and torrential stellar winds, which are carving out ridges, arcs, and filaments from the surrounding material. At the heart of this cosmic cloud lies the Papillon Nebula, a butterfly-shaped region of nebulosity. This small, dense object is classified as a High-Excitation Blob, and is thought to be tightly linked to the early stages of massive star form

PIX4620798

Cloth with Procession of Figures, 100 BC-200 (cotton and pigment (field); camelid fiber (borders and fringe))

Cloth with Procession of Figures, 100 BC-200 (cotton and pigment (field); camelid fiber (borders and fringe))

XCL5869626

Spiral Galaxy NGC 1566 in the Dorado - The Seyfert Galaxy NGC 1566 - NGC 1566 is a spiral galaxy located about 50 million years ago - light. Its core is very bright. It is an active galaxy called Seyfert, which probably houses a black hole in its heart. Image made with Siding Spring's 3.9m telescope. NGC 1566 is the brightest member of a nearby group of galaxies in Dorado and is at a distance of about 50 million light years. It has beautifully symmetrical, tightly - wound spiral arms, which on deep images appear to almost encircle the galaxy. This striking galaxy is also of interest because it has a very luminous nucleus which has many of the characteristics of a quasar, though it is much less energetic. Galaxies of this type are known as Seyfert galaxies, after Carl Seyfert who first recognised their peculiar nature in 1943. The active region at the centre of NGC 1566 has recently been found to vary on a timescale of less than a month, which indicates that it is extremely compact. Spe

Spiral Galaxy NGC 1566 in the Dorado - The Seyfert Galaxy NGC 1566 - NGC 1566 is a spiral galaxy located about 50 million years ago - light. Its core is very bright. It is an active galaxy called Seyfert, which probably houses a black hole in its heart. Image made with Siding Spring's 3.9m telescope. NGC 1566 is the brightest member of a nearby group of galaxies in Dorado and is at a distance of about 50 million light years. It has beautifully symmetrical, tightly - wound spiral arms, which on deep images appear to almost encircle the galaxy. This striking galaxy is also of interest because it has a very luminous nucleus which has many of the characteristics of a quasar, though it is much less energetic. Galaxies of this type are known as Seyfert galaxies, after Carl Seyfert who first recognised their peculiar nature in 1943. The active region at the centre of NGC 1566 has recently been found to vary on a timescale of less than a month, which indicates that it is extremely compact. Spe

PIX4609942

La chasse au buffle. Planche representant trois hommes caches dans un fosse pres d'un troupeau de buffles. ""Catlin's North American Indian Portfolio. Hunting scenes and amusements of the Rocky Mountains and Prairies of America"" par George Catlin, 1844. The British Library Institution Reference: Shelfmark ID: 1788.c.7. Buffalo Hunt. Approaching in a Ravine', 1844. In the lush, green prairies three armed men crouch down in a ravine, while a herd of buffalo graze nearby. Plate 11 from ""Catlin's North American Indian Portfolio. Hunting scenes and amusements of the Rocky Mountains and Prairies of America"" by George Catlin. (London, 1844).

La chasse au buffle. Planche representant trois hommes caches dans un fosse pres d'un troupeau de buffles. ""Catlin's North American Indian Portfolio. Hunting scenes and amusements of the Rocky Mountains and Prairies of America"" par George Catlin, 1844. The British Library Institution Reference: Shelfmark ID: 1788.c.7. Buffalo Hunt. Approaching in a Ravine', 1844. In the lush, green prairies three armed men crouch down in a ravine, while a herd of buffalo graze nearby. Plate 11 from ""Catlin's North American Indian Portfolio. Hunting scenes and amusements of the Rocky Mountains and Prairies of America"" by George Catlin. (London, 1844).

BL5337105

A woman and a child walk over a makeshift bamboo bridge to reach their home at the slum built directly over a puddle of chemical waste from nearby tanneries. It stinks and attracts mosquitoes and other insects day and night. Even though living condition in this slum is extremely difficult and hard to tolerate, a tiny room in the slum still cost about Taka one thousand, about $ 15 per month. Like many other industries unconcerned about the environmental factors, tanneries also cause serious damage to the environment. Hazaribagh, Dhakas biggest leather processing zone, is right in the middle of one of the most densely populated residential areas. February 20, 2007. (photo)

A woman and a child walk over a makeshift bamboo bridge to reach their home at the slum built directly over a puddle of chemical waste from nearby tanneries. It stinks and attracts mosquitoes and other insects day and night. Even though living condition in this slum is extremely difficult and hard to tolerate, a tiny room in the slum still cost about Taka one thousand, about $ 15 per month. Like many other industries unconcerned about the environmental factors, tanneries also cause serious damage to the environment. Hazaribagh, Dhakas biggest leather processing zone, is right in the middle of one of the most densely populated residential areas. February 20, 2007. (photo)

UIG798683

Close up of Ma Than Aye's weaving work in Heya Ywa Ma village on Lake Inle in Shan State. Ko Myint Swe (37 years old) makes silver jewellery and handcrafts at home-based workshop, while his wife, Ma Than Aye (40 years), weave cloths for bags and lungi, etc. Between them, they earn about 1800 Kyats per day (.00). They are both Inthar, a ethnic group, and have two children, both boys. Saw San Tin is 7 years old and studies in grade 2. Pyae Htu is 5 years old and has just started going to kindergarten in a nearby government school. (photo)

Close up of Ma Than Aye's weaving work in Heya Ywa Ma village on Lake Inle in Shan State. Ko Myint Swe (37 years old) makes silver jewellery and handcrafts at home-based workshop, while his wife, Ma Than Aye (40 years), weave cloths for bags and lungi, etc. Between them, they earn about 1800 Kyats per day (.00). They are both Inthar, a ethnic group, and have two children, both boys. Saw San Tin is 7 years old and studies in grade 2. Pyae Htu is 5 years old and has just started going to kindergarten in a nearby government school. (photo)

UIG795731

Thailand: The viharn (assembly hall) and main chedi at Wat Suan Dok, Chiang Mai, northern Thailand

Thailand: The viharn (assembly hall) and main chedi at Wat Suan Dok, Chiang Mai, northern Thailand

David Henley

PFH3519116

Thailand: The western end of the viharn (assembly hall) at Wat Suan Dok, Chiang Mai, northern Thailand

Thailand: The western end of the viharn (assembly hall) at Wat Suan Dok, Chiang Mai, northern Thailand

David Henley

PFH3519118

Thailand: Buddhist monks inside the viharn (assembly hall) at Wat Suan Dok, Chiang Mai, northern Thailand

Thailand: Buddhist monks inside the viharn (assembly hall) at Wat Suan Dok, Chiang Mai, northern Thailand

David Henley

PFH3519120

Thailand: "Thewada" (angels) adorn an inner wall in the viharn (assembly hall) at Wat Suan Dok, Chiang Mai, northern Thailand

Thailand: "Thewada" (angels) adorn an inner wall in the viharn (assembly hall) at Wat Suan Dok, Chiang Mai, northern Thailand

David Henley

PFH3519125

Thailand: "Thewada" (angels) adorn an inner wall in the viharn (assembly hall) at Wat Suan Dok, Chiang Mai, northern Thailand

Thailand: "Thewada" (angels) adorn an inner wall in the viharn (assembly hall) at Wat Suan Dok, Chiang Mai, northern Thailand

David Henley

PFH3519130

Portrait Bust of an Aristocratic Man and Portrait Bust of an Aristocratic Woman, c.270-280 (marble)

Portrait Bust of an Aristocratic Man and Portrait Bust of an Aristocratic Woman, c.270-280 (marble)

Roman Imperial Period (27 BC-476 AD)

XCL499618

Thailand: The western end of the viharn (assembly hall) at Wat Suan Dok, Chiang Mai, northern Thailand

Thailand: The western end of the viharn (assembly hall) at Wat Suan Dok, Chiang Mai, northern Thailand

David Henley

PFH3519119

Thailand: Inside the roof of the viharn (assembly hall) at Wat Suan Dok, Chiang Mai, northern Thailand

Thailand: Inside the roof of the viharn (assembly hall) at Wat Suan Dok, Chiang Mai, northern Thailand

David Henley

PFH3519123

Thailand: Inside the roof of the viharn (assembly hall) at Wat Suan Dok, Chiang Mai, northern Thailand

Thailand: Inside the roof of the viharn (assembly hall) at Wat Suan Dok, Chiang Mai, northern Thailand

David Henley

PFH3519124

Thailand: Buddha statues in the viharn (assembly hall) at Wat Suan Dok, Chiang Mai, northern Thailand

Thailand: Buddha statues in the viharn (assembly hall) at Wat Suan Dok, Chiang Mai, northern Thailand

David Henley

PFH3519127

Thailand: Buddha statues in the viharn (assembly hall) at Wat Suan Dok, Chiang Mai, northern Thailand

Thailand: Buddha statues in the viharn (assembly hall) at Wat Suan Dok, Chiang Mai, northern Thailand

David Henley

PFH3519135

Thailand: The interior roof of the viharn (assembly hall) at Wat Suan Dok, Chiang Mai, northern Thailand

Thailand: The interior roof of the viharn (assembly hall) at Wat Suan Dok, Chiang Mai, northern Thailand

David Henley

PFH3519137

Birth of stars in the nebula NGC 3372 - Star formation in the Carina Nebula - Detail of the Carene nebula (NGC 3372) obtained by the Hubble space telescope. The image shows a column of gas eroded by ultraviolet radiation emitted by young stars. Jets are also visible, showing the presence of emerging stars. NGC 3372 is located about 7500 light years away from Earth. The colors used in this image correspond to the emissions of different gases: sulfur in red, hydrogen in green and oxygen in blue. The NASA Hubble Space Telescope photograph captures the chaotic activity atop a three - light - year - tall pillar of gas and dust that is being eaten away by the brilliant light from nearby bright stars. The pillar is also being assaulted from within, as infant stars buried inside it fire off jets of gas that can be seen streaming from towering peaks. This turbulent cosmic pinnacle lies within a tempestuous stellar nursery called the Carina Nebula, located 7,500 light - years away in the souther

Birth of stars in the nebula NGC 3372 - Star formation in the Carina Nebula - Detail of the Carene nebula (NGC 3372) obtained by the Hubble space telescope. The image shows a column of gas eroded by ultraviolet radiation emitted by young stars. Jets are also visible, showing the presence of emerging stars. NGC 3372 is located about 7500 light years away from Earth. The colors used in this image correspond to the emissions of different gases: sulfur in red, hydrogen in green and oxygen in blue. The NASA Hubble Space Telescope photograph captures the chaotic activity atop a three - light - year - tall pillar of gas and dust that is being eaten away by the brilliant light from nearby bright stars. The pillar is also being assaulted from within, as infant stars buried inside it fire off jets of gas that can be seen streaming from towering peaks. This turbulent cosmic pinnacle lies within a tempestuous stellar nursery called the Carina Nebula, located 7,500 light - years away in the souther

PIX4619114

Supernova 1987A in the Great Magellan Cloud before and after explosion - Sometime during 23 February 1987 a supernova exploded in the Large Magellanic Cloud (LMC), a nearby galaxy. However, the LMC is about 170,000 light years distant, so the supernova exploded 170,000 years ago. It was discovered the following day and brightened rapidly to become the first supernova to be easily visible to the unaided eye for almost 400 years. This photograph shows the field around the site of the supernova in great detail, both before the supernova exploded (right) and about 10 days afterwards, when it was still brightening. The image of the star that exploded to create the supernova (mouseover the image) is elongated (better seen on this bigger image). This does not necessarily indicate any peculiarity or a close companion, rather it is the effect of stars being by chance aligned along the line of sight. Several other examples can be seen in this picture and other, different, blended images are seen

Supernova 1987A in the Great Magellan Cloud before and after explosion - Sometime during 23 February 1987 a supernova exploded in the Large Magellanic Cloud (LMC), a nearby galaxy. However, the LMC is about 170,000 light years distant, so the supernova exploded 170,000 years ago. It was discovered the following day and brightened rapidly to become the first supernova to be easily visible to the unaided eye for almost 400 years. This photograph shows the field around the site of the supernova in great detail, both before the supernova exploded (right) and about 10 days afterwards, when it was still brightening. The image of the star that exploded to create the supernova (mouseover the image) is elongated (better seen on this bigger image). This does not necessarily indicate any peculiarity or a close companion, rather it is the effect of stars being by chance aligned along the line of sight. Several other examples can be seen in this picture and other, different, blended images are seen

PIX4582330

Thailand: The viharn (assembly hall) at Wat Suan Dok, Chiang Mai, northern Thailand

Thailand: The viharn (assembly hall) at Wat Suan Dok, Chiang Mai, northern Thailand

David Henley

PFH3519115

Thailand: A woman meditates in the viharn (assembly hall) at Wat Suan Dok, Chiang Mai, northern Thailand

Thailand: A woman meditates in the viharn (assembly hall) at Wat Suan Dok, Chiang Mai, northern Thailand

David Henley

PFH3519129

Thailand: Buddha statues in the viharn (assembly hall) at Wat Suan Dok, Chiang Mai, northern Thailand

Thailand: Buddha statues in the viharn (assembly hall) at Wat Suan Dok, Chiang Mai, northern Thailand

David Henley

PFH3519133

Thailand: The interior roof of the viharn (assembly hall) at Wat Suan Dok, Chiang Mai, northern Thailand

Thailand: The interior roof of the viharn (assembly hall) at Wat Suan Dok, Chiang Mai, northern Thailand

David Henley

PFH3519136

Asafo flag (silk brocade and cotton fabric)

Asafo flag (silk brocade and cotton fabric)

Fante people, (19th century)

DTR3611188

Thailand: Buddhist monks inside the viharn (assembly hall) at Wat Suan Dok, Chiang Mai, northern Thailand

Thailand: Buddhist monks inside the viharn (assembly hall) at Wat Suan Dok, Chiang Mai, northern Thailand

David Henley

PFH3519121

Thailand: Buddha statues in the viharn (assembly hall) at Wat Suan Dok, Chiang Mai, northern Thailand

Thailand: Buddha statues in the viharn (assembly hall) at Wat Suan Dok, Chiang Mai, northern Thailand

David Henley

PFH3519128

Thailand: Buddha statues in the viharn (assembly hall) at Wat Suan Dok, Chiang Mai, northern Thailand

Thailand: Buddha statues in the viharn (assembly hall) at Wat Suan Dok, Chiang Mai, northern Thailand

David Henley

PFH3519131

Thailand: Buddha statues in the viharn (assembly hall) at Wat Suan Dok, Chiang Mai, northern Thailand

Thailand: Buddha statues in the viharn (assembly hall) at Wat Suan Dok, Chiang Mai, northern Thailand

David Henley

PFH3519132

Thailand: Buddha statues in the viharn (assembly hall) at Wat Suan Dok, Chiang Mai, northern Thailand

Thailand: Buddha statues in the viharn (assembly hall) at Wat Suan Dok, Chiang Mai, northern Thailand

David Henley

PFH3519134

Thailand: The entrance to the viharn (assembly hall) at Wat Suan Dok, Chiang Mai, northern Thailand

Thailand: The entrance to the viharn (assembly hall) at Wat Suan Dok, Chiang Mai, northern Thailand

David Henley

PFH3519114

Thailand: Inside the roof of the viharn (assembly hall) at Wat Suan Dok, Chiang Mai, northern Thailand

Thailand: Inside the roof of the viharn (assembly hall) at Wat Suan Dok, Chiang Mai, northern Thailand

David Henley

PFH3519122

Thailand: Buddha statues in the viharn (assembly hall) at Wat Suan Dok, Chiang Mai, northern Thailand

Thailand: Buddha statues in the viharn (assembly hall) at Wat Suan Dok, Chiang Mai, northern Thailand

David Henley

PFH3519126

Ouranosaurs and Sarcosuchus - Ouranosaurus stalked by Sarcosuchus - Three Ouranosaurus water a pond while a sarcosuchus approaches, threatening. Ouranosaurus nigeriensis is a herbivorous dinosaur of the order of ornithisdogs who lived in Africa 110 million years ago in Cretace. Sarcosuchus is a distant parent from crocodiles, measuring about ten metres in length. Three Ouranosaurus drink at a watering hole while a menacing Sarcosuchus floats nearby 110 million years ago in what is today Africa. The environment is moderately arid with Prickly Juniper and other hardy conifers dominating the ruddy landscape. Ouranosaurus was a variety of Iguanodont, a group of large plant-eating dinosaurs that also includes the well-known “” duck-billed””” hadrosaurs. At about 24 feet long and 4 tons, Ouranosaurus was unusual in that its skeleton suggests it had a large hump on its back. The hump may have served as a reservoir for water and/or source of nutrition for lean times as they do for modern bison

Ouranosaurs and Sarcosuchus - Ouranosaurus stalked by Sarcosuchus - Three Ouranosaurus water a pond while a sarcosuchus approaches, threatening. Ouranosaurus nigeriensis is a herbivorous dinosaur of the order of ornithisdogs who lived in Africa 110 million years ago in Cretace. Sarcosuchus is a distant parent from crocodiles, measuring about ten metres in length. Three Ouranosaurus drink at a watering hole while a menacing Sarcosuchus floats nearby 110 million years ago in what is today Africa. The environment is moderately arid with Prickly Juniper and other hardy conifers dominating the ruddy landscape. Ouranosaurus was a variety of Iguanodont, a group of large plant-eating dinosaurs that also includes the well-known “” duck-billed””” hadrosaurs. At about 24 feet long and 4 tons, Ouranosaurus was unusual in that its skeleton suggests it had a large hump on its back. The hump may have served as a reservoir for water and/or source of nutrition for lean times as they do for modern bison

Walter B Myers

PIX4662764

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

Cepheides in the barree spiral galaxy NGC 1365 - Cepheids in the barred spiral galaxy NGC 1365 - Detail on a star-forming zone in the barree spiral galaxy NGC 1365. Approximately 50 cepheides were discovered, allowing it to calculate its distance and estimate it at 60 million light years. NGC 1365 is a barred spiral galaxy that extends over 200,000 years - light. It belongs to the cluster of galaxies in the Furnace. Image obtained in 1996 by the Hubble space telescope A left image obtained by a ground telescope. This color image from the Hubble Space Telescope shows a region in NGC 1365, a barred spiral galaxy located in a cluster of galaxies called Fornax. A barred spiral galaxy is characterized by a “” bar””” of stars, dust and gas across its center. The black and white photograph from a ground - based telescope shows the entire galaxy, which is visible from the Southern Hemisphere. Astronomers who have been measuring the distance to the Fornax cluster, have estimated it to be 60 mil

Cepheides in the barree spiral galaxy NGC 1365 - Cepheids in the barred spiral galaxy NGC 1365 - Detail on a star-forming zone in the barree spiral galaxy NGC 1365. Approximately 50 cepheides were discovered, allowing it to calculate its distance and estimate it at 60 million light years. NGC 1365 is a barred spiral galaxy that extends over 200,000 years - light. It belongs to the cluster of galaxies in the Furnace. Image obtained in 1996 by the Hubble space telescope A left image obtained by a ground telescope. This color image from the Hubble Space Telescope shows a region in NGC 1365, a barred spiral galaxy located in a cluster of galaxies called Fornax. A barred spiral galaxy is characterized by a “” bar””” of stars, dust and gas across its center. The black and white photograph from a ground - based telescope shows the entire galaxy, which is visible from the Southern Hemisphere. Astronomers who have been measuring the distance to the Fornax cluster, have estimated it to be 60 mil

PIX4609849

Spiral galaxy M81 in the Great Bear - Spiral galaxy M81 in Ursa Major - The spiral galaxy M81 is located 12 million years ago - light from Earth. Its arms are home to star-forming regions while its core is surrounded by much older yellow stars. An irregular dwarf galaxy, PGC 28757 (Holmberg IX), is visible at the top of the picture. M81 is the brightest member of the nearby galactic group called the M81 group. This group contains at least 25 other members including the peculiar starburst galaxy M82, the peculiar galaxy NGC 3077 and many dwarfs galaxies. The core galaxies of the group (M81, M82, NGC 3077, NGC 2976) are strongly interacting and are all imbedded within a large and extended molecular gas cloud. The Dwarf irregular Holmberg IX (seen above M81 in the image) most likely condensed from tidal debri existing between M81 and M82. M81 has the distinction of being the nearest spiral galaxy to have an active galactic nucleus (AGN). AGN galaxies are luminous galaxies that demonstrate

Spiral galaxy M81 in the Great Bear - Spiral galaxy M81 in Ursa Major - The spiral galaxy M81 is located 12 million years ago - light from Earth. Its arms are home to star-forming regions while its core is surrounded by much older yellow stars. An irregular dwarf galaxy, PGC 28757 (Holmberg IX), is visible at the top of the picture. M81 is the brightest member of the nearby galactic group called the M81 group. This group contains at least 25 other members including the peculiar starburst galaxy M82, the peculiar galaxy NGC 3077 and many dwarfs galaxies. The core galaxies of the group (M81, M82, NGC 3077, NGC 2976) are strongly interacting and are all imbedded within a large and extended molecular gas cloud. The Dwarf irregular Holmberg IX (seen above M81 in the image) most likely condensed from tidal debri existing between M81 and M82. M81 has the distinction of being the nearest spiral galaxy to have an active galactic nucleus (AGN). AGN galaxies are luminous galaxies that demonstrate

R. Gendler

PIX4610379

Spiral galaxy M81 in the Great Bear - Spiral galaxy M81 in Ursa Major: The spiral galaxy M81 is located 12 million light years from Earth. Its arms are home to star-forming regions while its core is surrounded by much older yellow stars. An irregular dwarf galaxy, PGC 28757 (Holmberg IX), is visible at the top of the picture. - M81 is the brightest member of the nearby galactic group called the M81 group. This group contains at least 25 other members including the peculiar starburst galaxy M82, the peculiar galaxy NGC 3077 and many dwarfs galaxies. The core galaxies of the group (M81, M82, NGC 3077, NGC 2976) are strongly interacting and are all imbedded within a large and extended molecular gas cloud. The Dwarf irregular Holmberg IX (seen above M81 in the image) most likely condensed from tidal debri existing between M81 and M82. M81 has the distinction of being the nearest spiral galaxy to have an active galactic nucleus (AGN). AGN galaxies are luminous galaxies that demonstrate much

Spiral galaxy M81 in the Great Bear - Spiral galaxy M81 in Ursa Major: The spiral galaxy M81 is located 12 million light years from Earth. Its arms are home to star-forming regions while its core is surrounded by much older yellow stars. An irregular dwarf galaxy, PGC 28757 (Holmberg IX), is visible at the top of the picture. - M81 is the brightest member of the nearby galactic group called the M81 group. This group contains at least 25 other members including the peculiar starburst galaxy M82, the peculiar galaxy NGC 3077 and many dwarfs galaxies. The core galaxies of the group (M81, M82, NGC 3077, NGC 2976) are strongly interacting and are all imbedded within a large and extended molecular gas cloud. The Dwarf irregular Holmberg IX (seen above M81 in the image) most likely condensed from tidal debri existing between M81 and M82. M81 has the distinction of being the nearest spiral galaxy to have an active galactic nucleus (AGN). AGN galaxies are luminous galaxies that demonstrate much

PIX4610399

Spiral Galaxy M33 in the Triangle - Spiral galaxy M33 in Triangulum - The Galaxy of the Triangle (M33, NGC598) is located about 2 million years ago - light from Earth. It belongs to the local group, just like our galaxy or Andromede galaxy. In red, the star-forming regions appear, especially at the top left NGC 604 one of the largest and most active star-forming regions. It extends over 150 years of light. Image obtained from the Isaac Newton telescope of La Palma. M33 is a large, almost face - on spiral galaxy about 2.5 million light years distant in the northern constellation of Triangulum. It is a member of the 'Local Group' of galaxies, which is dominated by the Milky Way and M31. Like M31, M33 is approaching the Milky Way at a velocity of about 180km/s. Although the total light M33 galaxy is that of a star of magnitude 5.3, its large diameter makes it hard to see. However, despite its low surface brightness, this galaxy was among the first to be identified as a 'spiral nebula' by

Spiral Galaxy M33 in the Triangle - Spiral galaxy M33 in Triangulum - The Galaxy of the Triangle (M33, NGC598) is located about 2 million years ago - light from Earth. It belongs to the local group, just like our galaxy or Andromede galaxy. In red, the star-forming regions appear, especially at the top left NGC 604 one of the largest and most active star-forming regions. It extends over 150 years of light. Image obtained from the Isaac Newton telescope of La Palma. M33 is a large, almost face - on spiral galaxy about 2.5 million light years distant in the northern constellation of Triangulum. It is a member of the 'Local Group' of galaxies, which is dominated by the Milky Way and M31. Like M31, M33 is approaching the Milky Way at a velocity of about 180km/s. Although the total light M33 galaxy is that of a star of magnitude 5.3, its large diameter makes it hard to see. However, despite its low surface brightness, this galaxy was among the first to be identified as a 'spiral nebula' by

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Cepheide RS Puppis - Cepheides are very bright variable stars that serve as cosmic beacons to measure the distance of nearby galaxies. Their pulse period is measured and their absolute luminosite is calculated. By comparing the result to their apparent luminosite in the sky, they can be calculated accurately. Here, the space telescope photographed one of the brightest cepheids, RS Puppis (in the center of the image), located 6500 years - light in the southern constellation of the Puppi. The bright southern hemisphere star RS Puppis, at the center of the image, is swaddled in a gossamer cocoon of reflective dust illuminated by the glittering star. The super star is ten times more massive than our Sun and 200 times larger. RS Puppis rhythmically brightens and dims over a six - week cycle. It is one of the most luminous in the class of so - called Cepheid variable stars. Its average intrinsic brightness is 15,000 times greater than our Sun's luminosity. The nebula flickers in brightness a

Cepheide RS Puppis - Cepheides are very bright variable stars that serve as cosmic beacons to measure the distance of nearby galaxies. Their pulse period is measured and their absolute luminosite is calculated. By comparing the result to their apparent luminosite in the sky, they can be calculated accurately. Here, the space telescope photographed one of the brightest cepheids, RS Puppis (in the center of the image), located 6500 years - light in the southern constellation of the Puppi. The bright southern hemisphere star RS Puppis, at the center of the image, is swaddled in a gossamer cocoon of reflective dust illuminated by the glittering star. The super star is ten times more massive than our Sun and 200 times larger. RS Puppis rhythmically brightens and dims over a six - week cycle. It is one of the most luminous in the class of so - called Cepheid variable stars. Its average intrinsic brightness is 15,000 times greater than our Sun's luminosity. The nebula flickers in brightness a

PIX4572188

Jul 07, 1953 - Village of Beautiful Girls- Girls Outnumber men by Four to one: Bramber with a population of 400 is decreed in guide books as one of the most picturesque villages in Sussex. But it isn't one of the most romantic. The reason for that is because there is only one eligible bachelor for every four of its glamorous girls. Mrs. Peggy Glenie, manageress of the Castle Hotel said, “The shortage of men is terrible”. Every evening groups of two or three girls go into Mrs. Glene's her just to pass away the time. Their other sources of amusement are nearby river, a ruined castle and a hall - and a deserted Lover's Lane. Some of the young man of the village are lured away by the towns when they start work, but return to claim their childhood sweethearts. But with that four-to-one ratio there are a lot of girls without sweethearts to return. The reactor, The Rev. Ernest Street has about 25 wedding a year in Bramber and adjoining village of Beeding

Jul 07, 1953 - Village of Beautiful Girls- Girls Outnumber men by Four to one: Bramber with a population of 400 is decreed in guide books as one of the most picturesque villages in Sussex. But it isn't one of the most romantic. The reason for that is because there is only one eligible bachelor for every four of its glamorous girls. Mrs. Peggy Glenie, manageress of the Castle Hotel said, “The shortage of men is terrible”. Every evening groups of two or three girls go into Mrs. Glene's her just to pass away the time. Their other sources of amusement are nearby river, a ruined castle and a hall - and a deserted Lover's Lane. Some of the young man of the village are lured away by the towns when they start work, but return to claim their childhood sweethearts. But with that four-to-one ratio there are a lot of girls without sweethearts to return. The reactor, The Rev. Ernest Street has about 25 wedding a year in Bramber and adjoining village of Beeding

ZUM4859860

Ma Than Aye assists her children to do their home work in her house in Heya Ywa Ma village on Lake Inle in Shan State. Ko Myint Swe (37 years old) makes silver jeweleries and handcrafts at home-based workshop, while his wife, Ma Than Aye (40 years), weave cloths for bags and lungi, etc. Between them, they earn about 1800 Kyats per day (.00). They are both Inthar, a ethnic group, and have two children, both boys. Saw San Tin is 7 years old and studies in grade 2. Pyae Htu is 5 years old and has just started going to kindergarten in a nearby government school. (photo)

Ma Than Aye assists her children to do their home work in her house in Heya Ywa Ma village on Lake Inle in Shan State. Ko Myint Swe (37 years old) makes silver jeweleries and handcrafts at home-based workshop, while his wife, Ma Than Aye (40 years), weave cloths for bags and lungi, etc. Between them, they earn about 1800 Kyats per day (.00). They are both Inthar, a ethnic group, and have two children, both boys. Saw San Tin is 7 years old and studies in grade 2. Pyae Htu is 5 years old and has just started going to kindergarten in a nearby government school. (photo)

UIG795713

Ma Than Aye weaves cloth for school bags using a tradional loom in her house in in Heya Ywa Ma village on Lake Inle in Shan State. Ko Myint Swe (37 years old) makes silver jewellery and handcrafts at home-based workshop, while his wife, Ma Than Aye (40 years), weave cloths for bags and lungi, etc. Between them, they earn about 1800 Kyats per day (.00). They are both Inthar, a ethnic group, and have two children, both boys. Saw San Tin is 7 years old and studies in grade 2. Pyae Htu is 5 years old and has just started going to kindergarten in a nearby government school. (photo)

Ma Than Aye weaves cloth for school bags using a tradional loom in her house in in Heya Ywa Ma village on Lake Inle in Shan State. Ko Myint Swe (37 years old) makes silver jewellery and handcrafts at home-based workshop, while his wife, Ma Than Aye (40 years), weave cloths for bags and lungi, etc. Between them, they earn about 1800 Kyats per day (.00). They are both Inthar, a ethnic group, and have two children, both boys. Saw San Tin is 7 years old and studies in grade 2. Pyae Htu is 5 years old and has just started going to kindergarten in a nearby government school. (photo)

UIG795730

Rāvaṇa assigns the defence of Laṅkā's eastern gate to his general Prahasta; the southern gate to his brothers MahÄpÄrÅ›va and Mahodara; the western gate to his son Indrajit; and the northern gate, where he himself would also go, to the spies Åšuka and SÄraá¹‡a. The centre he leaves to VirūpÄká¹£a. Having thus directed Laṅkā's key defences, he retires to his chamber. Along with his allies, Rāma has now decided to climb the nearby Mount Suvela, from which there is a splendid view of the city of Laṅkā 'as if suspended in the sky'. All of Rāvaṇa's dispositions are soon known to VibhÄ«á¹£aá¹‡a through the birds he has sent out as spies.

Rāvaṇa assigns the defence of Laṅkā's eastern gate to his general Prahasta; the southern gate to his brothers MahÄpÄrÅ›va and Mahodara; the western gate to his son Indrajit; and the northern gate, where he himself would also go, to the spies Åšuka and SÄraá¹‡a. The centre he leaves to VirūpÄká¹£a. Having thus directed Laṅkā's key defences, he retires to his chamber. Along with his allies, Rāma has now decided to climb the nearby Mount Suvela, from which there is a splendid view of the city of Laṅkā 'as if suspended in the sky'. All of Rāvaṇa's dispositions are soon known to VibhÄ«á¹£aá¹‡a through the birds he has sent out as spies.

BL3283073

Ma Than Aye assit her children to do their home work in her house in Heya Ywa Ma village on Lake Inle in Shan State. Ko Myint Swe (37 years old) makes silver jeweleries and handcrafts at home-based workshop, while his wife, Ma Than Aye (40 years), weave cloths for bags and lungi, etc. Between them, they earn about 1800 Kyats per day (.00). They are both Inthar, a ethnic group, and have two children, both boys. Saw San Tin is 7 years old and studies in grade 2. Pyae Htu is 5 years old and has just started going to kindergarten in a nearby government school. (photo)

Ma Than Aye assit her children to do their home work in her house in Heya Ywa Ma village on Lake Inle in Shan State. Ko Myint Swe (37 years old) makes silver jeweleries and handcrafts at home-based workshop, while his wife, Ma Than Aye (40 years), weave cloths for bags and lungi, etc. Between them, they earn about 1800 Kyats per day (.00). They are both Inthar, a ethnic group, and have two children, both boys. Saw San Tin is 7 years old and studies in grade 2. Pyae Htu is 5 years old and has just started going to kindergarten in a nearby government school. (photo)

UIG798403

St. Odo of Canterbury, Patron saint of dealers in antiques and old clothes, c.1910 (colour litho)

St. Odo of Canterbury, Patron saint of dealers in antiques and old clothes, c.1910 (colour litho)

French School, (20th century)

KDC488444

Spiral galaxy M81 in the Great Bear - Spiral galaxy M81 in Ursa Major - The spiral galaxy M81 is located 12 million years ago - light from Earth. Its arms are home to star-forming regions while its core is surrounded by much older yellow stars. An irregular dwarf galaxy, PGC 28757 (Holmberg IX), is visible at the top of the picture. Image obtained with a 50 cm telescope through different filters, total of different poses: 20h. M81 is the brightest member of the nearby galactic group called the M81 group. This group contains at least 25 other members including the peculiar starburst galaxy M82, the peculiar galaxy NGC 3077 and many dwarfs galaxies. The core galaxies of the group (M81, M82, NGC 3077, NGC 2976) are strongly interacting and are all imbedded within a large and extended molecular gas cloud. The Dwarf irregular Holmberg IX (seen above M81 in the image) most likely condensed from tidal debri existing between M81 and M82. M81 has the distinction of being the nearest spiral gala

Spiral galaxy M81 in the Great Bear - Spiral galaxy M81 in Ursa Major - The spiral galaxy M81 is located 12 million years ago - light from Earth. Its arms are home to star-forming regions while its core is surrounded by much older yellow stars. An irregular dwarf galaxy, PGC 28757 (Holmberg IX), is visible at the top of the picture. Image obtained with a 50 cm telescope through different filters, total of different poses: 20h. M81 is the brightest member of the nearby galactic group called the M81 group. This group contains at least 25 other members including the peculiar starburst galaxy M82, the peculiar galaxy NGC 3077 and many dwarfs galaxies. The core galaxies of the group (M81, M82, NGC 3077, NGC 2976) are strongly interacting and are all imbedded within a large and extended molecular gas cloud. The Dwarf irregular Holmberg IX (seen above M81 in the image) most likely condensed from tidal debri existing between M81 and M82. M81 has the distinction of being the nearest spiral gala

R. Gendler

PIX4610335

Globular cluster G1 (Mayall II) - Globular cluster G1 (Mayall II) - The G1 globular cluster is the brightest globular cluster in the group of about thirty galaxies known as the Local Group (including the Lactee Way). It is orbiting the Andromede galaxy and contains at least 300,000 stars. This image is a composite of visible and near infrared images obtained by the Hubble Space Telescope in July 1994. Hubble Space Telescope has captured a view of a globular cluster called G1, a large, bright ball of light in the center of the photograph consisting of at least 300,000 old stars. G1, also known as Mayall II, orbits the Andromeda galaxy (M31), the nearest major spiral galaxy to our Milky Way. Located 130,000 light - years from Andromeda's nucleus, G1 is the brightest globular cluster in the Local Group of galaxies. The Local Group consists of about 20 nearby galaxies, including the Milky Way. A glimpse into the cluster's finer details allow astronomers to see its fainter helium - burning

Globular cluster G1 (Mayall II) - Globular cluster G1 (Mayall II) - The G1 globular cluster is the brightest globular cluster in the group of about thirty galaxies known as the Local Group (including the Lactee Way). It is orbiting the Andromede galaxy and contains at least 300,000 stars. This image is a composite of visible and near infrared images obtained by the Hubble Space Telescope in July 1994. Hubble Space Telescope has captured a view of a globular cluster called G1, a large, bright ball of light in the center of the photograph consisting of at least 300,000 old stars. G1, also known as Mayall II, orbits the Andromeda galaxy (M31), the nearest major spiral galaxy to our Milky Way. Located 130,000 light - years from Andromeda's nucleus, G1 is the brightest globular cluster in the Local Group of galaxies. The Local Group consists of about 20 nearby galaxies, including the Milky Way. A glimpse into the cluster's finer details allow astronomers to see its fainter helium - burning

PIX4565191

Ko Myint Swe and Ma Than Aye take their evening meal with their two children in their house in Heya Ywa Ma village on Lake Inle in Shan State. Myanmar. Ko Myint Swe (37 years old) makes silver jeweleries and handcrafts at home-based workshop, while his wife, Ma Than Aye (40 years), weave cloths for bags and lungi, etc. Between them, they earn about 1800 Kyats per day (.00). They are both Inthar, a ethnic group, and have two children, both boys. Saw San Tin is 7 years old and studies in grade 2. Pyae Htu is 5 years old and has just started going to kindergarten in a nearby government school. (photo)

Ko Myint Swe and Ma Than Aye take their evening meal with their two children in their house in Heya Ywa Ma village on Lake Inle in Shan State. Myanmar. Ko Myint Swe (37 years old) makes silver jeweleries and handcrafts at home-based workshop, while his wife, Ma Than Aye (40 years), weave cloths for bags and lungi, etc. Between them, they earn about 1800 Kyats per day (.00). They are both Inthar, a ethnic group, and have two children, both boys. Saw San Tin is 7 years old and studies in grade 2. Pyae Htu is 5 years old and has just started going to kindergarten in a nearby government school. (photo)

UIG795851

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