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Peru Machu Picchu (photo)

Peru Machu Picchu (photo)

Sergi Reboredo

SRB3585221

Bloomdale China Clay and Stone Works, St. Stephen-in-Brannel, Cornwall, UK (b/w photo)

Bloomdale China Clay and Stone Works, St. Stephen-in-Brannel, Cornwall, UK (b/w photo)

EHT6948185

Ultraviolet view of the galaxies M81 and M82 - Ultraviolet image of M81 and M82 - M81 (left) is a spiral galaxy. M82 (right) an irregular galaxy. Separated for about 150,000 light years, these two galaxies belong to the galaxy cluster closest to our local group. These galaxies are approximately 10 - 12 million light years away from Earth. In ultraviolet, the Galex satellite highlights star-forming regions. Ultraviolet image of Messier 81 and Messier 82 (NGC 3031 and 3034), a pair of galaxies lying 10 million light - years distant. The stars in M81 spiral arms have formed within the last 100 million years, as have most of the stars in a nearby dwarf galaxy just to the left of M81. GALEX reveals that star formation is occurring quite distant from the nucleus of M81 in the faint blue extensions to the brighter spiral arms. The upper half of the full GALEX field of view shows the remarkable star forming galaxy M82

Ultraviolet view of the galaxies M81 and M82 - Ultraviolet image of M81 and M82 - M81 (left) is a spiral galaxy. M82 (right) an irregular galaxy. Separated for about 150,000 light years, these two galaxies belong to the galaxy cluster closest to our local group. These galaxies are approximately 10 - 12 million light years away from Earth. In ultraviolet, the Galex satellite highlights star-forming regions. Ultraviolet image of Messier 81 and Messier 82 (NGC 3031 and 3034), a pair of galaxies lying 10 million light - years distant. The stars in M81 spiral arms have formed within the last 100 million years, as have most of the stars in a nearby dwarf galaxy just to the left of M81. GALEX reveals that star formation is occurring quite distant from the nucleus of M81 in the faint blue extensions to the brighter spiral arms. The upper half of the full GALEX field of view shows the remarkable star forming galaxy M82

PIX4610320

March - Volcanos Ceraunius Tholus and Uranius Tholus - Mars - Volcanos Ceraunius Tholus and Uranius Tholus - Image obtained by the Mars Global Surveyor probe in March 2002. This image shows the volcanoes Ceraunius Tholus (bottom) and Uranius Tholus (top). The presence of impact crateres on these volcanoes indicates that these volcanoes are old. The crater at the top of Ceraunius Tholus is about 25 km in diameter. Acquired in March 2002, this Mars Global Surveyor (MGS) Mars Orbiter Camera wide angle view shows the martian volcanoes, Ceraunius Tholus (lower) and Uranius Tholus (upper). The presence of impact craters on these volcanoes, particularly on Uranius Tholus; indicates that they are quite ancient and are not active today. The light - toned area on the southeastern face (towards lower right) of Ceraunius Tholus is a remnant of a once more extensive deposit of dust from the global dust storm events that occurred in 2001. The crater at the summit of Ceraunius Tholus is about 25 km (

March - Volcanos Ceraunius Tholus and Uranius Tholus - Mars - Volcanos Ceraunius Tholus and Uranius Tholus - Image obtained by the Mars Global Surveyor probe in March 2002. This image shows the volcanoes Ceraunius Tholus (bottom) and Uranius Tholus (top). The presence of impact crateres on these volcanoes indicates that these volcanoes are old. The crater at the top of Ceraunius Tholus is about 25 km in diameter. Acquired in March 2002, this Mars Global Surveyor (MGS) Mars Orbiter Camera wide angle view shows the martian volcanoes, Ceraunius Tholus (lower) and Uranius Tholus (upper). The presence of impact craters on these volcanoes, particularly on Uranius Tholus; indicates that they are quite ancient and are not active today. The light - toned area on the southeastern face (towards lower right) of Ceraunius Tholus is a remnant of a once more extensive deposit of dust from the global dust storm events that occurred in 2001. The crater at the summit of Ceraunius Tholus is about 25 km (

PIX4615439

Globular cluster NGC 3201 in Veles - Globular cluster NGC 3201 in Vela - This cluster of stars is located about 15,000 years ago - light from Earth

Globular cluster NGC 3201 in Veles - Globular cluster NGC 3201 in Vela - This cluster of stars is located about 15,000 years ago - light from Earth

PIX4564350

Pegase Constellation - Constellation of Pegasus - Pegasus represents a winged horse of Greek mythology, a figure that appears quite often, most spectacularly as the great winged steed of Bellerophon. The word Pegasus itself is derived from the Greek meaning 'strong'. Pegasus was the son of Neptune and Medusa the Gorgon, and sprang from the blood of his mother when her head had been severed by Perseus. Because Pegasus was considered a mortal, when he died he was placed in the heavens as a constellation by Zeus. Adjoining Pegasus is Equuleus, the foal. The most distinctive part of constellation is the Great Square of Pegasus. Its northernmost star, Sirrah, was incorparated into Andromeda when the constellation boundaries were formalized in the 1930s; it used to be delta (d) Pegasi. Because of its position in the sky, the first two objects in the New General Catalogue (NGC) appear in the Pegasus. NGC 1 and NGC 2 are distant, unremarkable galaxies, indeed this large constellation as a whol

Pegase Constellation - Constellation of Pegasus - Pegasus represents a winged horse of Greek mythology, a figure that appears quite often, most spectacularly as the great winged steed of Bellerophon. The word Pegasus itself is derived from the Greek meaning 'strong'. Pegasus was the son of Neptune and Medusa the Gorgon, and sprang from the blood of his mother when her head had been severed by Perseus. Because Pegasus was considered a mortal, when he died he was placed in the heavens as a constellation by Zeus. Adjoining Pegasus is Equuleus, the foal. The most distinctive part of constellation is the Great Square of Pegasus. Its northernmost star, Sirrah, was incorparated into Andromeda when the constellation boundaries were formalized in the 1930s; it used to be delta (d) Pegasi. Because of its position in the sky, the first two objects in the New General Catalogue (NGC) appear in the Pegasus. NGC 1 and NGC 2 are distant, unremarkable galaxies, indeed this large constellation as a whol

PIX4593125

Star formation regions NGC 3576 and 3603 in Carina - NGC 3576 (right) is located about 7000 years - light from Earth; NGC 3603 (left) is twice as far away. These two nebulae are located in the constellation Carene. Image obtained by Siding Spring's 3.9m telescope. These two star - formation regions appear side by side in the sky and seem to be linked as parts of an extensive nebula. However, the apparent intimacy is line - of - sight effect because these two objects are at quite different distances from the Sun. The curious looped nebula NGC 3576 is about 7000 light years from us while its neighbour NGC 3603 is more than twice as far away. That NGC 3603 is the more distant is confirmed by its colour, which is a ruddier red than the pinkish hue of NGC 3576. The change in colour is due to absorption of the blue - light component of the nebulosity by dust particles in the much longer line of sight. This effect is known as interstellar reddening, though it would be better described as 'de

Star formation regions NGC 3576 and 3603 in Carina - NGC 3576 (right) is located about 7000 years - light from Earth; NGC 3603 (left) is twice as far away. These two nebulae are located in the constellation Carene. Image obtained by Siding Spring's 3.9m telescope. These two star - formation regions appear side by side in the sky and seem to be linked as parts of an extensive nebula. However, the apparent intimacy is line - of - sight effect because these two objects are at quite different distances from the Sun. The curious looped nebula NGC 3576 is about 7000 light years from us while its neighbour NGC 3603 is more than twice as far away. That NGC 3603 is the more distant is confirmed by its colour, which is a ruddier red than the pinkish hue of NGC 3576. The change in colour is due to absorption of the blue - light component of the nebulosity by dust particles in the much longer line of sight. This effect is known as interstellar reddening, though it would be better described as 'de

PIX4619187

Nebulae NGC 3603 and NGC 3576 in Carene - NGC 3576 and 3603 in Carina - NGC 3576 (right) is located about 7000 years - light from Earth; NGC 3603 (left) is twice as far away. These two nebulae are located in the constellation Carene. Image obtained by Siding Spring's 3.9m telescope. These two star - formation regions appear side by side in the sky and seem to be linked as parts of an extensive nebula. However, the apparent intimacy is line - of - sight effect because these two objects are at quite different distances from the Sun. The curious looped nebula NGC 3576 is about 7000 light years from us while its neighbour NGC 3603 is more than twice as far away. That NGC 3603 is the more distant is confirmed by its colour, which is a ruddier red than the pinkish hue of NGC 3576. The change in colour is due to absorption of the blue - light component of the nebulosity by dust particles in the much longer line of sight. This effect is known as interstellar reddening, though it would be bette

Nebulae NGC 3603 and NGC 3576 in Carene - NGC 3576 and 3603 in Carina - NGC 3576 (right) is located about 7000 years - light from Earth; NGC 3603 (left) is twice as far away. These two nebulae are located in the constellation Carene. Image obtained by Siding Spring's 3.9m telescope. These two star - formation regions appear side by side in the sky and seem to be linked as parts of an extensive nebula. However, the apparent intimacy is line - of - sight effect because these two objects are at quite different distances from the Sun. The curious looped nebula NGC 3576 is about 7000 light years from us while its neighbour NGC 3603 is more than twice as far away. That NGC 3603 is the more distant is confirmed by its colour, which is a ruddier red than the pinkish hue of NGC 3576. The change in colour is due to absorption of the blue - light component of the nebulosity by dust particles in the much longer line of sight. This effect is known as interstellar reddening, though it would be bette

PIX4619197

Nebula IC 4628 in Scorpio - Nebula IC 4628 in Scorpius - Nebula with low light emission, IC 4628 (or Gum 56) is alongside the open cluster Collinder 316, which houses many hot young stars. This beautiful, arc - like rim of nebulosity is in the far southern sky, out of sight from most of the USA and Europe. It is quite faint and has often been overlooked because of it, even by southern observers. However, it is in a rich region in Scorpius. This richness is reflected in the number of names associated with the objects in the field illustrated here. There is a large scattered star cluster, Collinder 316 which extends over most of the picture. It encloses Trumpler 24, more or less the same cluster under another name, and all of this is part of the Sco OB1 association, a much larger gathering of very hot, intrinsically luminous stars in this part of the sky. The nebula itself is also known as Gum 56, after the Australian Colin Gum who catalogued emission nebulae in the southern sky using wi

Nebula IC 4628 in Scorpio - Nebula IC 4628 in Scorpius - Nebula with low light emission, IC 4628 (or Gum 56) is alongside the open cluster Collinder 316, which houses many hot young stars. This beautiful, arc - like rim of nebulosity is in the far southern sky, out of sight from most of the USA and Europe. It is quite faint and has often been overlooked because of it, even by southern observers. However, it is in a rich region in Scorpius. This richness is reflected in the number of names associated with the objects in the field illustrated here. There is a large scattered star cluster, Collinder 316 which extends over most of the picture. It encloses Trumpler 24, more or less the same cluster under another name, and all of this is part of the Sco OB1 association, a much larger gathering of very hot, intrinsically luminous stars in this part of the sky. The nebula itself is also known as Gum 56, after the Australian Colin Gum who catalogued emission nebulae in the southern sky using wi

PIX4622627

Globular cluster NGC 3201 in Veles - Globular cluster NGC 3201 in Vela - This cluster of stars is located about 15,000 years ago - light from Earth

Globular cluster NGC 3201 in Veles - Globular cluster NGC 3201 in Vela - This cluster of stars is located about 15,000 years ago - light from Earth

PIX4564372

Virgin and Child with Angel and Donor, after Memling, between 1499 and 1509 (oil on wood)

Virgin and Child with Angel and Donor, after Memling, between 1499 and 1509 (oil on wood)

Unknown Artist, (16th century)

XOS8985569

People of Dohar, an upajila (subdistrict) beside the River Padma, 65 km. from the capital city Dhaka, are quite well used to with the highs and lows of flood water. Every year they adjust the height of their homes according to the rise of flood water. But this year they have to shift their homes to safer places. As the northern districts see the receding of flood waters, Dhaka and its surrounding regions are facing a terrible threat of disaster. Waters of the rivers, such as the Padma and the Dhaleshwari, surrounding Dhaka are swelling rapidly. At the same time new areas of Manikganj, Munshiganj, and Dohar upazilas of Dhaka are facing imminent inundation. Dohar, Munshiganj , Bangladesh. August 5, 2007. (photo)

People of Dohar, an upajila (subdistrict) beside the River Padma, 65 km. from the capital city Dhaka, are quite well used to with the highs and lows of flood water. Every year they adjust the height of their homes according to the rise of flood water. But this year they have to shift their homes to safer places. As the northern districts see the receding of flood waters, Dhaka and its surrounding regions are facing a terrible threat of disaster. Waters of the rivers, such as the Padma and the Dhaleshwari, surrounding Dhaka are swelling rapidly. At the same time new areas of Manikganj, Munshiganj, and Dohar upazilas of Dhaka are facing imminent inundation. Dohar, Munshiganj , Bangladesh. August 5, 2007. (photo)

UIG797096

Nebulae NGC 3603 and NGC 3576 in Carene - NGC 3576 and 3603 in Carina - NGC 3576 (right) is located about 7000 years - light from Earth; NGC 3603 (left) is twice as far away. These two nebulae are located in the constellation Carene. Image obtained by Siding Spring's 3.9m telescope. These two star - formation regions appear side by side in the sky and seem to be linked as parts of an extensive nebula. However, the apparent intimacy is line - of - sight effect because these two objects are at quite different distances from the Sun. The curious looped nebula NGC 3576 is about 7000 light years from us while its neighbour NGC 3603 is more than twice as far away. That NGC 3603 is the more distant is confirmed by its colour, which is a ruddier red than the pinkish hue of NGC 3576. The change in colour is due to absorption of the blue - light component of the nebulosity by dust particles in the much longer line of sight. This effect is known as interstellar reddening, though it would be bette

Nebulae NGC 3603 and NGC 3576 in Carene - NGC 3576 and 3603 in Carina - NGC 3576 (right) is located about 7000 years - light from Earth; NGC 3603 (left) is twice as far away. These two nebulae are located in the constellation Carene. Image obtained by Siding Spring's 3.9m telescope. These two star - formation regions appear side by side in the sky and seem to be linked as parts of an extensive nebula. However, the apparent intimacy is line - of - sight effect because these two objects are at quite different distances from the Sun. The curious looped nebula NGC 3576 is about 7000 light years from us while its neighbour NGC 3603 is more than twice as far away. That NGC 3603 is the more distant is confirmed by its colour, which is a ruddier red than the pinkish hue of NGC 3576. The change in colour is due to absorption of the blue - light component of the nebulosity by dust particles in the much longer line of sight. This effect is known as interstellar reddening, though it would be bette

PIX4619201

Cruise liner poster: Royal Mail Line, Atlantic Cruises, 'Cruise with the Sun'. c. 1930 (poster)

Cruise liner poster: Royal Mail Line, Atlantic Cruises, 'Cruise with the Sun'. c. 1930 (poster)

Shoesmith, Kenneth (1890-1939)

MMM7342544

Mural scene from the Buddhist Jataka tales, Wat Hang Dong, Chiang Mai, northern Thailand

Mural scene from the Buddhist Jataka tales, Wat Hang Dong, Chiang Mai, northern Thailand

David Henley

PFH4822623

Mural scene from the Buddhist Jataka tales, Wat Hang Dong, Chiang Mai, northern Thailand

Mural scene from the Buddhist Jataka tales, Wat Hang Dong, Chiang Mai, northern Thailand

David Henley

PFH4822628

Pegase Constellation - Constellation of Pegasus - Pegasus represents a winged horse of Greek mythology, a figure that appears quite often, most spectacularly as the great winged steed of Bellerophon. The word Pegasus itself is derived from the Greek meaning 'strong'. Pegasus was the son of Neptune and Medusa the Gorgon, and sprang from the blood of his mother when her head had been severed by Perseus. Because Pegasus was considered a mortal, when he died he was placed in the heavens as a constellation by Zeus. Adjoining Pegasus is Equuleus, the foal. The most distinctive part of constellation is the Great Square of Pegasus. Its northernmost star, Sirrah, was incorparated into Andromeda when the constellation boundaries were formalized in the 1930s; it used to be delta (d) Pegasi. Because of its position in the sky, the first two objects in the New General Catalogue (NGC) appear in the Pegasus. NGC 1 and NGC 2 are distant, unremarkable galaxies, indeed this large constellation as a whol

Pegase Constellation - Constellation of Pegasus - Pegasus represents a winged horse of Greek mythology, a figure that appears quite often, most spectacularly as the great winged steed of Bellerophon. The word Pegasus itself is derived from the Greek meaning 'strong'. Pegasus was the son of Neptune and Medusa the Gorgon, and sprang from the blood of his mother when her head had been severed by Perseus. Because Pegasus was considered a mortal, when he died he was placed in the heavens as a constellation by Zeus. Adjoining Pegasus is Equuleus, the foal. The most distinctive part of constellation is the Great Square of Pegasus. Its northernmost star, Sirrah, was incorparated into Andromeda when the constellation boundaries were formalized in the 1930s; it used to be delta (d) Pegasi. Because of its position in the sky, the first two objects in the New General Catalogue (NGC) appear in the Pegasus. NGC 1 and NGC 2 are distant, unremarkable galaxies, indeed this large constellation as a whol

PIX4593156

Newly Married Couple Dressed For The Ceremony With Flower Garland And Traditional Clothing Near The Mahamaham Tank, Kumbakonam, India, 2008 (photo)

Newly Married Couple Dressed For The Ceremony With Flower Garland And Traditional Clothing Near The Mahamaham Tank, Kumbakonam, India, 2008 (photo)

Eric Lafforgue

LFG7355732

Relatives Dressed For The Ceremony Following The Bride And Groom In The Street During The Wedding, Kanadukathan Chettinad, India, 2008 (photo)

Relatives Dressed For The Ceremony Following The Bride And Groom In The Street During The Wedding, Kanadukathan Chettinad, India, 2008 (photo)

Eric Lafforgue

LFG7357972

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

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

PIX4568102

Bride In Sari Wearing A Colorful Flower Garland On Her Head For Her Wedding, Pondicherry, India, 2008 (photo)

Bride In Sari Wearing A Colorful Flower Garland On Her Head For Her Wedding, Pondicherry, India, 2008 (photo)

Eric Lafforgue

LFG7355717

Young Bride And Groom Dressed For The Ceremony And Adorned With Flower Garlands Posing Surrounded By Family, Pondicherry, India, 2008 (photo)

Young Bride And Groom Dressed For The Ceremony And Adorned With Flower Garlands Posing Surrounded By Family, Pondicherry, India, 2008 (photo)

Eric Lafforgue

LFG7355720

Lance-Corporal David Finlay, V.C, 2nd bn. Black Watch. David Finlay VC (20 January 1893 - 21 January 1916) was a Scottish recipient of the Victoria Cross. On 9 May 1915 near Rue du Bois, France, Lance-Corporal Finlay led a bombing party of 12 men in the attack until 10 of them had fallen. He then ordered the two survivors to crawl back and he himself went to the assistance of a wounded man and carried him over a distance of 100 yards of fire-swept ground into cover, quite regardless of his own safety. He was killed in action in Mesopotamia on 21 January 1916 and is remembered on the Basra Memorial.[

Lance-Corporal David Finlay, V.C, 2nd bn. Black Watch. David Finlay VC (20 January 1893 - 21 January 1916) was a Scottish recipient of the Victoria Cross. On 9 May 1915 near Rue du Bois, France, Lance-Corporal Finlay led a bombing party of 12 men in the attack until 10 of them had fallen. He then ordered the two survivors to crawl back and he himself went to the assistance of a wounded man and carried him over a distance of 100 yards of fire-swept ground into cover, quite regardless of his own safety. He was killed in action in Mesopotamia on 21 January 1916 and is remembered on the Basra Memorial.[

BL3310477

Young Groom Dressed For The Ceremony With Flower Garland Surrounded By Men In White In Procession For The Wedding, Kanadukathan Chettinad, India, 2008 (photo)

Young Groom Dressed For The Ceremony With Flower Garland Surrounded By Men In White In Procession For The Wedding, Kanadukathan Chettinad, India, 2008 (photo)

Eric Lafforgue

LFG7357973

Young Bride And Groom Sitting On A Bank Dressed For The Ceremony And Adorned With Flower Garlands, Pondicherry, India, 2008 (photo)

Young Bride And Groom Sitting On A Bank Dressed For The Ceremony And Adorned With Flower Garlands, Pondicherry, India, 2008 (photo)

Eric Lafforgue

LFG7355611

Passengers on RMS Titanic. Photograph of Mr Bride, the young wireless operator who assisted Phillips, the Chief Operator, during the crisis. Mr Bride, like most of the operators on board ships, was quite young. He apparently assisted Phillips very efficiently during the critical hours on the Titanic. Titanic was built by Harland & Wolff in Belfast Ireland during 1910 - 1911 and later sank on April 15th, 1912 off the coast of New Foundland after striking an iceberg during her maiden voyage from Southampton, England to New York, USA, with the loss of 1,522 passengers and crew. (Photo by Titanic Images/Universal Images Group) Photographie. ©UIG/Leemage

Passengers on RMS Titanic. Photograph of Mr Bride, the young wireless operator who assisted Phillips, the Chief Operator, during the crisis. Mr Bride, like most of the operators on board ships, was quite young. He apparently assisted Phillips very efficiently during the critical hours on the Titanic. Titanic was built by Harland & Wolff in Belfast Ireland during 1910 - 1911 and later sank on April 15th, 1912 off the coast of New Foundland after striking an iceberg during her maiden voyage from Southampton, England to New York, USA, with the loss of 1,522 passengers and crew. (Photo by Titanic Images/Universal Images Group) Photographie. ©UIG/Leemage

UIG5447049

Ganges, Varanasi, India (photo)

Ganges, Varanasi, India (photo)

Sergi Reboredo

SRB3036637

The Magnificent Omega Centauri, 2014 (digital photo)

The Magnificent Omega Centauri, 2014 (digital photo)

Bobillo, Ignacio Diaz (20th-21st century)

MMM7340386

Group Of Musician Men Dressed In White In Procession During A Wedding With Nadaswaram And Thavil In Kanadukathan Chettinad's Street, India, 2008 (photo)

Group Of Musician Men Dressed In White In Procession During A Wedding With Nadaswaram And Thavil In Kanadukathan Chettinad's Street, India, 2008 (photo)

Eric Lafforgue

LFG7355772

Young Bride And Groom Standing In Front Of A House Dressed For The Ceremony And Adorned With Flower Garlands, Pondicherry, India, 2008 (photo)

Young Bride And Groom Standing In Front Of A House Dressed For The Ceremony And Adorned With Flower Garlands, Pondicherry, India, 2008 (photo)

Eric Lafforgue

LFG7357897

Planetary nebula NGC 2899 dans les Voiles - A distorted planetary nebula, NGC 2899 - This nebula is located about 3000 years from Earth. Image obtained by the 3.9m telescope of Siding Spring Planetary nebulae present a wide variety of forms on the sky, partly because of the random orientation of their parent stars but also because the nebulae themselves can have quite different intrinsic shapes. Theories about the shapes of planetaries range from the influence of binary companions to the central star to the distribution of material around the stars during its red giant phase, before the final outburst. Whatever the mechanism, most planetaries are symmetrical about one or more axes and only rarely do they appear curved like NGC 2899. A possible explanation is that the star from which the nebula was ejected had a large proper motion through space. The resulting nebula has the same velocity but vastly lower density than the star so is distorted by its encounter with the tenuous interstell

Planetary nebula NGC 2899 dans les Voiles - A distorted planetary nebula, NGC 2899 - This nebula is located about 3000 years from Earth. Image obtained by the 3.9m telescope of Siding Spring Planetary nebulae present a wide variety of forms on the sky, partly because of the random orientation of their parent stars but also because the nebulae themselves can have quite different intrinsic shapes. Theories about the shapes of planetaries range from the influence of binary companions to the central star to the distribution of material around the stars during its red giant phase, before the final outburst. Whatever the mechanism, most planetaries are symmetrical about one or more axes and only rarely do they appear curved like NGC 2899. A possible explanation is that the star from which the nebula was ejected had a large proper motion through space. The resulting nebula has the same velocity but vastly lower density than the star so is distorted by its encounter with the tenuous interstell

PIX4622995

With the Swiss partner NESTLÉ and many, many colorful smarties as encore, the TV magazine HÖRZU promotes itself and Germany's television prize 'Golden Camera', which will be presented again on 4 February 2003 in Berlin. At the time of the economic miracle HÖRZU and mascot MECKI were the real stars of the still young television family: Launched in December 1946 (250,000 copies), the weekly program sheet became Europe's largest magazine (1962: 4.2 million copies). Since 1949, the dear Mecki on the advertising drum and made it several times on the title page (our photo from December 1955). In the Chinese look, he advertises quite casually for his book series, which is still popular among old and young, 2003 (photo)

With the Swiss partner NESTLÉ and many, many colorful smarties as encore, the TV magazine HÖRZU promotes itself and Germany's television prize 'Golden Camera', which will be presented again on 4 February 2003 in Berlin. At the time of the economic miracle HÖRZU and mascot MECKI were the real stars of the still young television family: Launched in December 1946 (250,000 copies), the weekly program sheet became Europe's largest magazine (1962: 4.2 million copies). Since 1949, the dear Mecki on the advertising drum and made it several times on the title page (our photo from December 1955). In the Chinese look, he advertises quite casually for his book series, which is still popular among old and young, 2003 (photo)

SZT5863516

The Lawes of Virginia. Virginia was the first permanent English colony in North America, established by the London Company in 1607. The foundation charter of that new colony, drafted by Sir Edward Coke (d. 1634), stated that English law should be applied to the settlers. However, by the time that The Lawes of Virginia was published in 1662, it had become evident that certain principles of English law, which took their inspiration from Magna Carta, were no longer recognised in Virginia. This was especially the case regarding 'Tryals by Juryes', which were limited by the legal procedures instituted in that colony. The Lawes of Virginia therefore directed that, as this 'restriction is quite contrary to the Law of England "¦ by which we are to be governed', trial by jury was to be reinstated, and a jury empanelled to attend court on a daily basis

The Lawes of Virginia. Virginia was the first permanent English colony in North America, established by the London Company in 1607. The foundation charter of that new colony, drafted by Sir Edward Coke (d. 1634), stated that English law should be applied to the settlers. However, by the time that The Lawes of Virginia was published in 1662, it had become evident that certain principles of English law, which took their inspiration from Magna Carta, were no longer recognised in Virginia. This was especially the case regarding 'Tryals by Juryes', which were limited by the legal procedures instituted in that colony. The Lawes of Virginia therefore directed that, as this 'restriction is quite contrary to the Law of England "¦ by which we are to be governed', trial by jury was to be reinstated, and a jury empanelled to attend court on a daily basis

BL3289721

Spiral galaxy M74 in Pisces - Spiral galaxy M74 in Pisces - Image of the spiral galaxy M74 (NGC 628). This galaxy is about 80,000 light years and is 30 million light years apart. Viewed face on, as it appeared about 30 million years ago, M74 is considered to be one of the most photogenic spiral galaxies in the sky. The galaxy is rich in young bright blue stars and glowing red regions of dust and molecular hydrogen where new stars are being created. M74, however, is quite camera shy - it has a low surface brightness that makes it challenging for both visual observers and astrophotographers to see it's entire form. The Chandra X - Ray observatory, discovered M74 to be the home of a super massive black hole, tucked away in one of it's outer arms. This black hole is one of the largest ever discovered and has the mass of over 10,000 suns. Thirty six, fifteen minute photographs were combined to create this picture, with a total exposure time of almost nine hours. The images were taken with a

Spiral galaxy M74 in Pisces - Spiral galaxy M74 in Pisces - Image of the spiral galaxy M74 (NGC 628). This galaxy is about 80,000 light years and is 30 million light years apart. Viewed face on, as it appeared about 30 million years ago, M74 is considered to be one of the most photogenic spiral galaxies in the sky. The galaxy is rich in young bright blue stars and glowing red regions of dust and molecular hydrogen where new stars are being created. M74, however, is quite camera shy - it has a low surface brightness that makes it challenging for both visual observers and astrophotographers to see it's entire form. The Chandra X - Ray observatory, discovered M74 to be the home of a super massive black hole, tucked away in one of it's outer arms. This black hole is one of the largest ever discovered and has the mass of over 10,000 suns. Thirty six, fifteen minute photographs were combined to create this picture, with a total exposure time of almost nine hours. The images were taken with a

R. Jay GaBany

PIX4609403

Spiral galaxy NGC 7424 in the Crane - Galaxy NGC 7424 in Grus - The barree spiral galaxy NGC 7424 is located about 40 million years away from Earth. NGC 7424 extends over nearly 100,000 light years, like our galaxy. Numerous bright blue clusters of massive young stars are visible along the spiral arms. Image obtained by the telescope MELIPAL of the VLT on October 9, 2004 Composite colour - coded image of spiral galaxy, NGC 7424, at a distance of 40 million light - years. This galaxy is classified as “” SAB (rs) cd””, meaning that it is intermediate between normal spirals (SA) and strongly barred galaxies (SB) and that it has rather open arms with a small central region. It also shows many ionised regions as well as clusters of young and massive stars. Ten young massive star clusters can be identified whose size span the range from 1 to 200 light - years. The galaxy itself is roughly 100,000 light - years across, that is, quite similar in size to our own Milky Way galaxy. Images obtaine

Spiral galaxy NGC 7424 in the Crane - Galaxy NGC 7424 in Grus - The barree spiral galaxy NGC 7424 is located about 40 million years away from Earth. NGC 7424 extends over nearly 100,000 light years, like our galaxy. Numerous bright blue clusters of massive young stars are visible along the spiral arms. Image obtained by the telescope MELIPAL of the VLT on October 9, 2004 Composite colour - coded image of spiral galaxy, NGC 7424, at a distance of 40 million light - years. This galaxy is classified as “” SAB (rs) cd””, meaning that it is intermediate between normal spirals (SA) and strongly barred galaxies (SB) and that it has rather open arms with a small central region. It also shows many ionised regions as well as clusters of young and massive stars. Ten young massive star clusters can be identified whose size span the range from 1 to 200 light - years. The galaxy itself is roughly 100,000 light - years across, that is, quite similar in size to our own Milky Way galaxy. Images obtaine

PIX4613160

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

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

PIX4622981

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

Turkey: A levha or panel honouring Imam 'Ali ibn Abi Talib I(r. 656-661 CE) and his celebrated bifurcated sword Dhu'l-fiqar (Zulfiqar), 'The Cleaver of Vertebrae'. Calligraphy attributed to Farid al-Din, early 19th century

Turkey: A levha or panel honouring Imam 'Ali ibn Abi Talib I(r. 656-661 CE) and his celebrated bifurcated sword Dhu'l-fiqar (Zulfiqar), 'The Cleaver of Vertebrae'. Calligraphy attributed to Farid al-Din, early 19th century

PFH1774311

Comet C2013US10 Catalina, 2015 (digital photo)

Comet C2013US10 Catalina, 2015 (digital photo)

Rhemann, Gerald (21st century)

MMM7340356

Sep. 24, 1953 - Miracle 'boy walks after eight years.: Mrs. Jean Palmer, 38-tear-old housewife of Cramlington, Northumberland, believes that a miracle happened in the parlour of her new Council house. Her eight year old son, John, cripples from birth by deformed hips, was playing on the rug. Suddenly he grabbed a tor cricket bat and a toy spade - and stood up. While Mrs. Palmer watched breathlessly, John hobbled across the room to her. The he turned round and went back. When we had an operation three years ago, doctors told Mrs. Palmer that John, who had never walked might not do so as long as he lived. A doctor at the Royal Victoria Infirmary, Newcastle, where John has been attending twice a week, said last night:” Operations for congenital hip dislocations are quite common, and their success is not unusual. But for a child to recover his power who walk after three years lapse is something we do not come across frequently.” Photo shows John Palmer, the little boy who was crippled from

Sep. 24, 1953 - Miracle 'boy walks after eight years.: Mrs. Jean Palmer, 38-tear-old housewife of Cramlington, Northumberland, believes that a miracle happened in the parlour of her new Council house. Her eight year old son, John, cripples from birth by deformed hips, was playing on the rug. Suddenly he grabbed a tor cricket bat and a toy spade - and stood up. While Mrs. Palmer watched breathlessly, John hobbled across the room to her. The he turned round and went back. When we had an operation three years ago, doctors told Mrs. Palmer that John, who had never walked might not do so as long as he lived. A doctor at the Royal Victoria Infirmary, Newcastle, where John has been attending twice a week, said last night:” Operations for congenital hip dislocations are quite common, and their success is not unusual. But for a child to recover his power who walk after three years lapse is something we do not come across frequently.” Photo shows John Palmer, the little boy who was crippled from

ZUM4882177

The Lawes of Virginia. Virginia was the first permanent English colony in North America, established by the London Company in 1607. The foundation charter of that new colony, drafted by Sir Edward Coke (d. 1634), stated that English law should be applied to the settlers. However, by the time that The Lawes of Virginia was published in 1662, it had become evident that certain principles of English law, which took their inspiration from Magna Carta, were no longer recognised in Virginia. This was especially the case regarding 'Tryals by Juryes', which were limited by the legal procedures instituted in that colony. The Lawes of Virginia therefore directed that, as this 'restriction is quite contrary to the Law of England "¦ by which we are to be governed', trial by jury was to be reinstated, and a jury empanelled to attend court on a daily basis

The Lawes of Virginia. Virginia was the first permanent English colony in North America, established by the London Company in 1607. The foundation charter of that new colony, drafted by Sir Edward Coke (d. 1634), stated that English law should be applied to the settlers. However, by the time that The Lawes of Virginia was published in 1662, it had become evident that certain principles of English law, which took their inspiration from Magna Carta, were no longer recognised in Virginia. This was especially the case regarding 'Tryals by Juryes', which were limited by the legal procedures instituted in that colony. The Lawes of Virginia therefore directed that, as this 'restriction is quite contrary to the Law of England "¦ by which we are to be governed', trial by jury was to be reinstated, and a jury empanelled to attend court on a daily basis

BL3289718

Ganges, Varanasi, India (photo)

Ganges, Varanasi, India (photo)

Sergi Reboredo

SRB3036636

Malaysia / China: Carving of Zheng Lun, depicting his role in the 16th Century Ming Dynasty novel 'Fengshen Yanyi' ('Investiture of the Gods'). From Ping Sien Si Temple, Pasir Panjang Laut

Malaysia / China: Carving of Zheng Lun, depicting his role in the 16th Century Ming Dynasty novel 'Fengshen Yanyi' ('Investiture of the Gods'). From Ping Sien Si Temple, Pasir Panjang Laut

PFH3277878

May 18, 1953 - St. Gangolf's Pilgrimage and Ride in Neudenau. As may be followed back in historical sources the farmers of Neudenau are riding out for centuries. to the old Gangolf's chapel, about tow kilometers outside the gates of the small town, every year in May. The old chapel is one of the oldest buildings of Frankonia originating from the 9th century. Probably this old chapel may be traced back to be an old German source - sanctuary and also the St. Gangolf's ride may have its origin in an old German habit of blessing the spring and the horses. Every year 150 to 200 horses and thousands of people are taking part in this horse - pilgrimage. St. Gangolf's ride is especially meant for the adoration of this saint of the Frankonian knights who is regarded from the oldest times to be the helper in need among the Christian people and to be also the patron saint of the horses. saint Gangolf's ride is one of the oldest German horse-pilgrimages and it always preserved its special characte

May 18, 1953 - St. Gangolf's Pilgrimage and Ride in Neudenau. As may be followed back in historical sources the farmers of Neudenau are riding out for centuries. to the old Gangolf's chapel, about tow kilometers outside the gates of the small town, every year in May. The old chapel is one of the oldest buildings of Frankonia originating from the 9th century. Probably this old chapel may be traced back to be an old German source - sanctuary and also the St. Gangolf's ride may have its origin in an old German habit of blessing the spring and the horses. Every year 150 to 200 horses and thousands of people are taking part in this horse - pilgrimage. St. Gangolf's ride is especially meant for the adoration of this saint of the Frankonian knights who is regarded from the oldest times to be the helper in need among the Christian people and to be also the patron saint of the horses. saint Gangolf's ride is one of the oldest German horse-pilgrimages and it always preserved its special characte

ZUM4847131

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

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

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

PIX4613427

The Village of Amed and View of Mount Gunung Agung, Bali (photo)

The Village of Amed and View of Mount Gunung Agung, Bali (photo)

Sergi Reboredo

SRB1202672

Tureens (part of The Grand Service), hallmark 1826/7 (silver gilt)

Tureens (part of The Grand Service), hallmark 1826/7 (silver gilt)

Bridge, John (1755-1834)

ROC6151249

'Suspension Bridge of hide thongs (but repaired with chain) over the Maypu, five leagues south of Santiago, Chile, Jany 11th 1851', 1851 (watercolour)

'Suspension Bridge of hide thongs (but repaired with chain) over the Maypu, five leagues south of Santiago, Chile, Jany 11th 1851', 1851 (watercolour)

Fanshawe, Admiral Sir Edward Gennys (1814-1906)

MMM7295626

Nebulae IC 2948 and 2944 in Centaur - A large southern emission nebula, IC 2948 - Nebula IC 2948 is a vast nebula located about 6000 years from Earth in the southern constellation of Centaur. It is associated with the cluster of stars IC 2944 near which Bok's blood cells are visible. 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. Between the Southern Cross and the rich Carina region, on the southern border of Centaurus, is a large, almost featureless emission nebula, IC 2948, with a sprinkling of bright stars, Collinder 249. It is against this uniform, backdrop that we see a brighter region (IC 2944) which hosts small group of dark clouds of the kind known as 'Bok globules'. They are named for the Dutch - American astronomer who first drew attention to them as the possible sites of star formation. There are young stars scattered through the nebula and these stars are responsible for its existence

Nebulae IC 2948 and 2944 in Centaur - A large southern emission nebula, IC 2948 - Nebula IC 2948 is a vast nebula located about 6000 years from Earth in the southern constellation of Centaur. It is associated with the cluster of stars IC 2944 near which Bok's blood cells are visible. 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. Between the Southern Cross and the rich Carina region, on the southern border of Centaurus, is a large, almost featureless emission nebula, IC 2948, with a sprinkling of bright stars, Collinder 249. It is against this uniform, backdrop that we see a brighter region (IC 2944) which hosts small group of dark clouds of the kind known as 'Bok globules'. They are named for the Dutch - American astronomer who first drew attention to them as the possible sites of star formation. There are young stars scattered through the nebula and these stars are responsible for its existence

PIX4622607

Galaxy NGC 891 in Andromede - Edge - on spiral galaxy NGC 891 in Andromeda - Spiral galaxy seen by the slice located at a distance of 10 million years - light. This image was obtained with the Isaac Newton 2.5m telescope of La Palma. If we could view the Milky Way from a distance of about 30 million light years it would look something like NGC 891. But galaxies that look like this are quite rare because the chance alignment of the thin disk of a spiral galaxy with our line of sight is unusual. A few degrees either side of its orientation and NGC 891 would be just another highly inclined spiral galaxy. From this unusual vantage point we can see in NGC 891 the surprising narrowness of the obscuring dust lane, a dark, slightly irregular band across the galaxy. We also see that it is yellowish, confirming that it is dust, which absorbs blue light, as in the Milky Way. Also similar to the Milky Way is the prominent central 'bulge' corresponding to the rich star clouds in Sagittarius. Howeve

Galaxy NGC 891 in Andromede - Edge - on spiral galaxy NGC 891 in Andromeda - Spiral galaxy seen by the slice located at a distance of 10 million years - light. This image was obtained with the Isaac Newton 2.5m telescope of La Palma. If we could view the Milky Way from a distance of about 30 million light years it would look something like NGC 891. But galaxies that look like this are quite rare because the chance alignment of the thin disk of a spiral galaxy with our line of sight is unusual. A few degrees either side of its orientation and NGC 891 would be just another highly inclined spiral galaxy. From this unusual vantage point we can see in NGC 891 the surprising narrowness of the obscuring dust lane, a dark, slightly irregular band across the galaxy. We also see that it is yellowish, confirming that it is dust, which absorbs blue light, as in the Milky Way. Also similar to the Milky Way is the prominent central 'bulge' corresponding to the rich star clouds in Sagittarius. Howeve

PIX4609474

Tureens (part of The Grand Service), hallmark 1826/7 (silver gilt)

Tureens (part of The Grand Service), hallmark 1826/7 (silver gilt)

Bridge, John (1755-1834)

ROC6151232

The Southern Milky Way and south celestial pole - The Southern Milky Way and south celestial pole - The Octant constellation houses the south celeste pole (mark of a cross) This part of the sky was mostly uncharted by Europeans until the 17th and 18th centuries, so many of the constellations in the southern (lower) half of the image are relatively modern constructions without mythlogical connotations. Octans, the Octant (a forerunner of the sextant) is an Enlightenment - period instrument whose outline was constructed on the sky by the vivid imagination of the Abbe Lacaille. The constellation is quite large but totally undistinguished. Its only notable feature is the South Celestial Pole, with is marked (within a degree or so) by the faint star s Octantis. Apus, the Bird of Paradise, first appeared in the star charts of the German astronomer Johann Bayer in 1603. It contains no named stars. Chameleon, a type of lizard. The stars here are even fainter than those in Apus. Mensa, the cons

The Southern Milky Way and south celestial pole - The Southern Milky Way and south celestial pole - The Octant constellation houses the south celeste pole (mark of a cross) This part of the sky was mostly uncharted by Europeans until the 17th and 18th centuries, so many of the constellations in the southern (lower) half of the image are relatively modern constructions without mythlogical connotations. Octans, the Octant (a forerunner of the sextant) is an Enlightenment - period instrument whose outline was constructed on the sky by the vivid imagination of the Abbe Lacaille. The constellation is quite large but totally undistinguished. Its only notable feature is the South Celestial Pole, with is marked (within a degree or so) by the faint star s Octantis. Apus, the Bird of Paradise, first appeared in the star charts of the German astronomer Johann Bayer in 1603. It contains no named stars. Chameleon, a type of lizard. The stars here are even fainter than those in Apus. Mensa, the cons

PIX4594601

Galaxy NGC 891 in Andromede - Edge - on spiral galaxy NGC 891 in Andromeda - Spiral galaxy seen by the slice located at a distance of 10 million years - light.. This image obtained with the 2.5m Isaac Newton telescope of La Palma. If we could view the Milky Way from a distance of about 30 million light years it would look something like NGC 891. But galaxies that look like this are quite rare because the chance alignment of the thin disk of a spiral galaxy with our line of sight is unusual. A few degrees either side of its orientation and NGC 891 would be just another highly inclined spiral galaxy. From this unusual vantage point we can see in NGC 891 the surprising narrowness of the obscuring dust lane, a dark, slightly irregular band across the galaxy. We also see that it is yellowish, confirming that it is dust, which absorbs blue light, as in the Milky Way. Also similar to the Milky Way is the prominent central 'bulge' corresponding to the rich star clouds in Sagittarius. However,

Galaxy NGC 891 in Andromede - Edge - on spiral galaxy NGC 891 in Andromeda - Spiral galaxy seen by the slice located at a distance of 10 million years - light.. This image obtained with the 2.5m Isaac Newton telescope of La Palma. If we could view the Milky Way from a distance of about 30 million light years it would look something like NGC 891. But galaxies that look like this are quite rare because the chance alignment of the thin disk of a spiral galaxy with our line of sight is unusual. A few degrees either side of its orientation and NGC 891 would be just another highly inclined spiral galaxy. From this unusual vantage point we can see in NGC 891 the surprising narrowness of the obscuring dust lane, a dark, slightly irregular band across the galaxy. We also see that it is yellowish, confirming that it is dust, which absorbs blue light, as in the Milky Way. Also similar to the Milky Way is the prominent central 'bulge' corresponding to the rich star clouds in Sagittarius. However,

PIX4609481

Shibu Onsen, Shimotakai district (photo)

Shibu Onsen, Shimotakai district (photo)

Catherine Shepard

SHD8330427

Visitors in Shibu Onsen, Shimotakai district (photo)

Visitors in Shibu Onsen, Shimotakai district (photo)

Catherine Shepard

SHD8330370

Vietnam: The Opera House by night, Hanoi

Vietnam: The Opera House by night, Hanoi

David Henley

PFH4072407

Shibu Onsen, Shimotakai district (photo)

Shibu Onsen, Shimotakai district (photo)

Catherine Shepard

SHD8330423

Shinmeidaki-no-yu Onsen in Yamanouchi (photo)

Shinmeidaki-no-yu Onsen in Yamanouchi (photo)

Catherine Shepard

SHD8330441

Magna Carta is frequently mentioned in children's history books where traditionally it has been taught as one of the foundations of British liberty. Such books include Our Island Story, first published in 1905, in which 'the Story of the Great Charter' is presented as an important chapter in the nation's democratic development. Combining history with vivid story-telling, Our Island Story portrays King John as a maniac who 'gnashed his teeth, growling and snarling like a wild animal mad with rage "¦ These things seem to us now quite natural and right, so you can imagine what evil times these were when the King was unwilling to grant such liberty to his people'. Our Island Story was nominated by Conservative Prime Minister David Cameron in 2010 as his favourite childhood book, saying that it 'nurtured my interest in the history of our great nation'.

Magna Carta is frequently mentioned in children's history books where traditionally it has been taught as one of the foundations of British liberty. Such books include Our Island Story, first published in 1905, in which 'the Story of the Great Charter' is presented as an important chapter in the nation's democratic development. Combining history with vivid story-telling, Our Island Story portrays King John as a maniac who 'gnashed his teeth, growling and snarling like a wild animal mad with rage "¦ These things seem to us now quite natural and right, so you can imagine what evil times these were when the King was unwilling to grant such liberty to his people'. Our Island Story was nominated by Conservative Prime Minister David Cameron in 2010 as his favourite childhood book, saying that it 'nurtured my interest in the history of our great nation'.

BL3261257

The Southern Milky Way and south celestial pole - The Octant constellation houses the southern Celestial pole. See annotee image a - cst98 - 00005 to identify the different constellations present in the image. This part of the sky was mostly uncharted by Europeans until the 17th and 18th centuries, so many of the constellations in the southern (lower) half of the image are relatively modern constructions without mythlogical connotations. Octans, the Octant (a forerunner of the sextant) is an Enlightenment - period instrument whose outline was constructed on the sky by the vivid imagination of the Abbe Lacaille. The constellation is quite large but totally undistinguished. Its only notable feature is the South Celestial Pole, with is marked (within a degree or so) by the faint star s Octantis. Apus, the Bird of Paradise, first appeared in the star charts of the German astronomer Johann Bayer in 1603. It contains no named stars. Chameleon, a type of lizard. The stars here are even fainte

The Southern Milky Way and south celestial pole - The Octant constellation houses the southern Celestial pole. See annotee image a - cst98 - 00005 to identify the different constellations present in the image. This part of the sky was mostly uncharted by Europeans until the 17th and 18th centuries, so many of the constellations in the southern (lower) half of the image are relatively modern constructions without mythlogical connotations. Octans, the Octant (a forerunner of the sextant) is an Enlightenment - period instrument whose outline was constructed on the sky by the vivid imagination of the Abbe Lacaille. The constellation is quite large but totally undistinguished. Its only notable feature is the South Celestial Pole, with is marked (within a degree or so) by the faint star s Octantis. Apus, the Bird of Paradise, first appeared in the star charts of the German astronomer Johann Bayer in 1603. It contains no named stars. Chameleon, a type of lizard. The stars here are even fainte

PIX4594597

Magna Carta is frequently mentioned in children's history books where traditionally it has been taught as one of the foundations of British liberty. Such books include Our Island Story, first published in 1905, in which 'the Story of the Great Charter' is presented as an important chapter in the nation's democratic development. Combining history with vivid story-telling, Our Island Story portrays King John as a maniac who 'gnashed his teeth, growling and snarling like a wild animal mad with rage "¦ These things seem to us now quite natural and right, so you can imagine what evil times these were when the King was unwilling to grant such liberty to his people'. Our Island Story was nominated by Conservative Prime Minister David Cameron in 2010 as his favourite childhood book, saying that it 'nurtured my interest in the history of our great nation'.

Magna Carta is frequently mentioned in children's history books where traditionally it has been taught as one of the foundations of British liberty. Such books include Our Island Story, first published in 1905, in which 'the Story of the Great Charter' is presented as an important chapter in the nation's democratic development. Combining history with vivid story-telling, Our Island Story portrays King John as a maniac who 'gnashed his teeth, growling and snarling like a wild animal mad with rage "¦ These things seem to us now quite natural and right, so you can imagine what evil times these were when the King was unwilling to grant such liberty to his people'. Our Island Story was nominated by Conservative Prime Minister David Cameron in 2010 as his favourite childhood book, saying that it 'nurtured my interest in the history of our great nation'.

BL3261248

Feet With Rings Of A Just Married Man Surrounded By Rose Petals At His Wedding In Trichy, India, 2008 (photo)

Feet With Rings Of A Just Married Man Surrounded By Rose Petals At His Wedding In Trichy, India, 2008 (photo)

Eric Lafforgue

LFG7355783

Nebula IC 4628 in Scorpio - Nebula IC 4628 in Scorpius - Nebula has a low light emission, IC 4628 (or Gum 56) is alongside the open cluster Collinder 316, which houses many young hot stars. Image obtained through 3 different filters that highlight oxygen (blue), hydrogen (green), and sulfur (red). This beautiful, arc - like rim of nebulosity is in the far southern sky, out of sight from most of the USA and Europe. It is quite faint and has often been overlooked because of it, even by southern observers. However, it is in a rich region in Scorpius. This richness is reflected in the number of names associated with the objects in the field illustrated here. There is a large scattered star cluster, Collinder 316 which extends over most of the picture. It encloses Trumpler 24, more or less the same cluster under another name, and all of this is part of the Sco OB1 association, a much larger gathering of very hot, intrinsically luminous stars in this part of the sky. The nebula itself is als

Nebula IC 4628 in Scorpio - Nebula IC 4628 in Scorpius - Nebula has a low light emission, IC 4628 (or Gum 56) is alongside the open cluster Collinder 316, which houses many young hot stars. Image obtained through 3 different filters that highlight oxygen (blue), hydrogen (green), and sulfur (red). This beautiful, arc - like rim of nebulosity is in the far southern sky, out of sight from most of the USA and Europe. It is quite faint and has often been overlooked because of it, even by southern observers. However, it is in a rich region in Scorpius. This richness is reflected in the number of names associated with the objects in the field illustrated here. There is a large scattered star cluster, Collinder 316 which extends over most of the picture. It encloses Trumpler 24, more or less the same cluster under another name, and all of this is part of the Sco OB1 association, a much larger gathering of very hot, intrinsically luminous stars in this part of the sky. The nebula itself is als

Tom Davis

PIX4622673

The Christening of Victoria, Princess Royal, 10 February 1841, c.1841-2 (oil on canvas)

The Christening of Victoria, Princess Royal, 10 February 1841, c.1841-2 (oil on canvas)

Leslie, Charles Robert (1794-1859)

ROC828751

Spiral galaxy NGC 1566 in the bream - The Seyfert Galaxy NGC 1566: NGC 1566 is a spiral galaxy located about 40 million light years ago. Its core is very bright. It is an active galaxy called Seyfert, which probably houses a black hole in its heart. Image obtained with the Hubble telescope - NGC 1566 is a galaxy located approximately 40 million light-years away in the constellation of Dorado (The Dolphinfish). NGC 1566 is an intermediate spiral galaxy, meaning that while it does not have a well defined bar-shaped region of stars at its centre - like barred spirals - it is not quite an unbarred spiral either (heic9902o). The small but extremely bright nucleus of NGC 1566 is clearly visible in this image, a telltale sign of its membership of the Seyfert class of galaxies. The centres of such galaxies are very active and luminous, emitting strong bursts of radiation and potentially harbouring supermassive black holes that are many millions of times the mass of the Sun. NGC 1566 is not jus

Spiral galaxy NGC 1566 in the bream - The Seyfert Galaxy NGC 1566: NGC 1566 is a spiral galaxy located about 40 million light years ago. Its core is very bright. It is an active galaxy called Seyfert, which probably houses a black hole in its heart. Image obtained with the Hubble telescope - NGC 1566 is a galaxy located approximately 40 million light-years away in the constellation of Dorado (The Dolphinfish). NGC 1566 is an intermediate spiral galaxy, meaning that while it does not have a well defined bar-shaped region of stars at its centre - like barred spirals - it is not quite an unbarred spiral either (heic9902o). The small but extremely bright nucleus of NGC 1566 is clearly visible in this image, a telltale sign of its membership of the Seyfert class of galaxies. The centres of such galaxies are very active and luminous, emitting strong bursts of radiation and potentially harbouring supermassive black holes that are many millions of times the mass of the Sun. NGC 1566 is not jus

PIX4609939

Camps near the fishing village of Amed East Bali, Bali (photo)

Camps near the fishing village of Amed East Bali, Bali (photo)

Sergi Reboredo

SRB1202674

Water Monitor Lizard on the Chobe River, Chobe National Park, Botswana (photo)

Water Monitor Lizard on the Chobe River, Chobe National Park, Botswana (photo)

Sergi Reboredo

SRB1202632

King Charles IX of France (1550-1574)

King Charles IX of France (1550-1574)

Clouet, Francois (c.1510-72) (after)

USB1159912

Nebula IC 2948 in Centaurus - Nebula IC 2948 and IC 2944 in Centaurus - Nebula IC 2948 is a vast nebula located about 6000 years from Earth in the southern constellation of Centaurus. It is associated with the cluster of stars IC 2944 near which Bok's blood cells are visible. 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. Image obtained through 3 different filters that highlight oxygen (blue), hydrogen (green), and sulfur (red). Between the Southern Cross and the rich Carina region, on the southern border of Centaurus, is a large, almost featureless emission nebula, IC 2948, with a sprinkling of bright stars, Collinder 249. It is against this uniform, backdrop that we see a brighter region (IC 2944) which hosts small group of dark clouds of the kind known as 'Bok globules'. They are named for the Dutch - American astronomer who first drew attention to them as the possible sites of star formation.

Nebula IC 2948 in Centaurus - Nebula IC 2948 and IC 2944 in Centaurus - Nebula IC 2948 is a vast nebula located about 6000 years from Earth in the southern constellation of Centaurus. It is associated with the cluster of stars IC 2944 near which Bok's blood cells are visible. 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. Image obtained through 3 different filters that highlight oxygen (blue), hydrogen (green), and sulfur (red). Between the Southern Cross and the rich Carina region, on the southern border of Centaurus, is a large, almost featureless emission nebula, IC 2948, with a sprinkling of bright stars, Collinder 249. It is against this uniform, backdrop that we see a brighter region (IC 2944) which hosts small group of dark clouds of the kind known as 'Bok globules'. They are named for the Dutch - American astronomer who first drew attention to them as the possible sites of star formation.

Tom Davis

PIX4622599

Galaxies NGC 5426 and NGC 5427 in the Virgin - Galaxies NGC 5426 and NGC 5427 in Virgo - Arp 271 desks the two spiral galaxies of similar sizes in interaction NGC 5426 and NGC 5427. Located 90 million years ago - light in the constellation of Virgo, Arp 271 is about 130,000 years - light in diameter. Although it is uncertain whether this interaction leads to a fusion of galaxies, the galaxies are already gravitationally affected by each other and a bridge of matter has formed between the two. Image obtained with a telescope of 80 cm. NGC 5426 and NGC 5427 are two spiral galaxies of similar sizes engaged in a dramatic dance. It is not certain that this interaction will end in a collision and ultimately a merging of the two galaxies, although the galaxies have already been affected. Together known as Arp 271, this dance will last for tens of millions of years, creating new stars as a result of the mutual gravitational attraction between the galaxies, a pull seen in the bridge of stars al

Galaxies NGC 5426 and NGC 5427 in the Virgin - Galaxies NGC 5426 and NGC 5427 in Virgo - Arp 271 desks the two spiral galaxies of similar sizes in interaction NGC 5426 and NGC 5427. Located 90 million years ago - light in the constellation of Virgo, Arp 271 is about 130,000 years - light in diameter. Although it is uncertain whether this interaction leads to a fusion of galaxies, the galaxies are already gravitationally affected by each other and a bridge of matter has formed between the two. Image obtained with a telescope of 80 cm. NGC 5426 and NGC 5427 are two spiral galaxies of similar sizes engaged in a dramatic dance. It is not certain that this interaction will end in a collision and ultimately a merging of the two galaxies, although the galaxies have already been affected. Together known as Arp 271, this dance will last for tens of millions of years, creating new stars as a result of the mutual gravitational attraction between the galaxies, a pull seen in the bridge of stars al

Adam Block

PIX4612650

Camps near the fishing village of Amed East Bali, Bali (photo)

Camps near the fishing village of Amed East Bali, Bali (photo)

Sergi Reboredo

SRB1202687

Nebula IC 2948 in Centaurus - Nebula IC 2948 and IC 2944 in Centaurus: IC2944 - SHO 70 70 70 Bin 2 - Nebula IC 2948 is a vast nebula located about 6000 light years from Earth in the southern constellation of Centaurus. It is associated with the cluster of stars IC 2944 near which Bok's blood cells are visible. 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 - Image obtained through 3 different filters that highlight oxygen (in blue), hydrogen (in green), and sulfur (in red) - Between the Southern Cross and the rich Carina region, on the southern border of Centaurus, is a large, almost featureless emission nebula, IC 2948, with a sprinkling of bright stars, Collinder 249. It is against this uniform, backdrop that we see a brighter region (IC 2944) which hosts small group of dark clouds of the kind known as 'Bok globules'. They are named for the Dutch-American astronomer who first drew attention to t

Nebula IC 2948 in Centaurus - Nebula IC 2948 and IC 2944 in Centaurus: IC2944 - SHO 70 70 70 Bin 2 - Nebula IC 2948 is a vast nebula located about 6000 light years from Earth in the southern constellation of Centaurus. It is associated with the cluster of stars IC 2944 near which Bok's blood cells are visible. 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 - Image obtained through 3 different filters that highlight oxygen (in blue), hydrogen (in green), and sulfur (in red) - Between the Southern Cross and the rich Carina region, on the southern border of Centaurus, is a large, almost featureless emission nebula, IC 2948, with a sprinkling of bright stars, Collinder 249. It is against this uniform, backdrop that we see a brighter region (IC 2944) which hosts small group of dark clouds of the kind known as 'Bok globules'. They are named for the Dutch-American astronomer who first drew attention to t

W. Promper

PIX4622580

Poland / Palestine: Moses Wilhelm Shapira (1830-1884), Jerusalem antiquities dealer, forger and purveyor of fake Biblical artifacts, date not known but probably c. 1870

Poland / Palestine: Moses Wilhelm Shapira (1830-1884), Jerusalem antiquities dealer, forger and purveyor of fake Biblical artifacts, date not known but probably c. 1870

David Henley

PFH2561634

The Virgin and Child with the Infant St John, c.1505 (metalpoint (much faded) and white heightening on pink-buff prepared paper)

The Virgin and Child with the Infant St John, c.1505 (metalpoint (much faded) and white heightening on pink-buff prepared paper)

Raphael (Raffaello Sanzio of Urbino) (1483-1520)

ROC3552292

Poland / Palestine: Moses Wilhelm Shapira (1830-1884), Jerusalem antiquities dealer, forger and purveyor of fake Biblical artifacts, date not known but probably c. 1870

Poland / Palestine: Moses Wilhelm Shapira (1830-1884), Jerusalem antiquities dealer, forger and purveyor of fake Biblical artifacts, date not known but probably c. 1870

David Henley

PFH2561635

In billets at Flesselles. A member of the Australian 2nd Battalion "carrying on" with his correspondence, 17-30 November 1916 (b/w photo)

In billets at Flesselles. A member of the Australian 2nd Battalion "carrying on" with his correspondence, 17-30 November 1916 (b/w photo)

Australian Photographer (20th century)

MEM1268206

Portrait of Thomas Eakins, c.1920-25 (oil on canvas)

Portrait of Thomas Eakins, c.1920-25 (oil on canvas)

Eakins, Susan Macdowell (1851-1938)

PHL434332

Abell 383 galaxy cluster and primitive galaxy - Abell 383 cluster of galaxies with gravitational arcs - Abell 383 is a cluster of galaxies located in the constellation Eridan. This image obtained by the Hubble Space Telescope (HST) in 2011 shows gravitational arcs among galaxies. These mirages are deformed images of farther galaxies located behind the cluster. Thanks to this magnifying effect, the resulting image revealed the presence of a primitive galaxy, nee 200 million years after the big blow. Astronomers have uncovered one of the youngest galaxies in the distant universe, with stars that formed 13.5 billion years ago, a mere 200 million years after the Big Bang. The finding addresses questions about when the first galaxies arose, and how the early universe evolved. Nasa's Hubble Space Telescope was the first to spot the newfound galaxy. Detailed observations from the W.M. Keck Observatory on Mauna Kea in Hawaii revealed the observed light dates to when the universe was only 950 m

Abell 383 galaxy cluster and primitive galaxy - Abell 383 cluster of galaxies with gravitational arcs - Abell 383 is a cluster of galaxies located in the constellation Eridan. This image obtained by the Hubble Space Telescope (HST) in 2011 shows gravitational arcs among galaxies. These mirages are deformed images of farther galaxies located behind the cluster. Thanks to this magnifying effect, the resulting image revealed the presence of a primitive galaxy, nee 200 million years after the big blow. Astronomers have uncovered one of the youngest galaxies in the distant universe, with stars that formed 13.5 billion years ago, a mere 200 million years after the Big Bang. The finding addresses questions about when the first galaxies arose, and how the early universe evolved. Nasa's Hubble Space Telescope was the first to spot the newfound galaxy. Detailed observations from the W.M. Keck Observatory on Mauna Kea in Hawaii revealed the observed light dates to when the universe was only 950 m

PIX4565712

Family of Khmer Leu Ethnic Group, Kateung village, Ratanakiri, Cambodia (photo)

Family of Khmer Leu Ethnic Group, Kateung village, Ratanakiri, Cambodia (photo)

Sergi Reboredo

SRB1202779

Dolly Rathebe - Dolly and Her Men! - The World Does Not Suspect That Film Star Dolly…, 1957 (photo)

Dolly Rathebe - Dolly and Her Men! - The World Does Not Suspect That Film Star Dolly…, 1957 (photo)

Jürgen Schadeberg

AMD8679362

Spiral galaxy M31 in Andromede - First color photo - The first color image of spiral galaxy M31 in Andromeda - The galaxy of Andromede is located about 2 million years ago - light from Earth. Two satellite galaxies accompany him: M32 (NGC 221) on the left, and M110 (NGC 205) on the bottom right. Like the lactee path, the Andromede galaxy belongs to the local group, making up about thirty galaxies. This photo is the first color photo of M31. It was obtained on 11 August 1958 at the Schmidt telescope of Mount Palomar. M31 (NGC 224) is the finest and nearest large spiral galaxy in the sky, about 2 million light years away. It has several close companions, the most obvious of which are the compact elliptical galaxy M32 (NGC 221) at lower left centre here, and M110 (NGC 205) at lower right. M 31 is a member of the Local Group of about 30 galaxies that includes the Milky Way and M31 as its most massive members as well as the two Magellanic Clouds. This particular picture is of interest becau

Spiral galaxy M31 in Andromede - First color photo - The first color image of spiral galaxy M31 in Andromeda - The galaxy of Andromede is located about 2 million years ago - light from Earth. Two satellite galaxies accompany him: M32 (NGC 221) on the left, and M110 (NGC 205) on the bottom right. Like the lactee path, the Andromede galaxy belongs to the local group, making up about thirty galaxies. This photo is the first color photo of M31. It was obtained on 11 August 1958 at the Schmidt telescope of Mount Palomar. M31 (NGC 224) is the finest and nearest large spiral galaxy in the sky, about 2 million light years away. It has several close companions, the most obvious of which are the compact elliptical galaxy M32 (NGC 221) at lower left centre here, and M110 (NGC 205) at lower right. M 31 is a member of the Local Group of about 30 galaxies that includes the Milky Way and M31 as its most massive members as well as the two Magellanic Clouds. This particular picture is of interest becau

PIX4608699

Colliding galaxy Ngc 6745 in Lyra - Colliding galaxy NGC 6745 in Lyra - The spiral galaxy NGC 6745 is located about 206 million years away - light from Earth. This galaxy is double; a second galaxy at the bottom right of the image collides with it, causing star formation. Image obtained by the Hubble Space Telescope in 1996. A large spiral galaxy, with its nucleus still intact, peers at the smaller passing galaxy (almost out of the field of view at lower right). These galaxies did not merely interact gravitationally as they passed one another, they actually collided. When galaxies collide, the stars that normally comprise the major portion of the luminous mass of each of the two galaxies will almost never collide with each other but will pass rather freely between each other with little damage. This occurs because the physical size of individual stars is tiny compared to their typical separations, making the chance of physical encounter relatively small. In our own Milky Way galaxy, th

Colliding galaxy Ngc 6745 in Lyra - Colliding galaxy NGC 6745 in Lyra - The spiral galaxy NGC 6745 is located about 206 million years away - light from Earth. This galaxy is double; a second galaxy at the bottom right of the image collides with it, causing star formation. Image obtained by the Hubble Space Telescope in 1996. A large spiral galaxy, with its nucleus still intact, peers at the smaller passing galaxy (almost out of the field of view at lower right). These galaxies did not merely interact gravitationally as they passed one another, they actually collided. When galaxies collide, the stars that normally comprise the major portion of the luminous mass of each of the two galaxies will almost never collide with each other but will pass rather freely between each other with little damage. This occurs because the physical size of individual stars is tiny compared to their typical separations, making the chance of physical encounter relatively small. In our own Milky Way galaxy, th

PIX4612985

HMS 'Cardiff' leading the German fleet to surrender, 1918, 1919 (paper, watercolour)

HMS 'Cardiff' leading the German fleet to surrender, 1918, 1919 (paper, watercolour)

Dixon, Charles Edward (1872-1934)

MMM7342504

Dolly Rathebe - Dolly and Her Men! - The World Does Not Suspect That Film Star Dolly…, 1957 (photo)

Dolly Rathebe - Dolly and Her Men! - The World Does Not Suspect That Film Star Dolly…, 1957 (photo)

Jürgen Schadeberg

AMD8679363

Landscape with Two Figures dancing with Tambourines (after Claude Lorrain)

Landscape with Two Figures dancing with Tambourines (after Claude Lorrain)

Hackert, Jacob-Philippe (1737-1807) (attr. to)

USB1156681

Tyndall Glacier, Chile - Tyndall Glacier, Chile - The Tyndall Glacier in Torres del Paine National Park in Chile, observed from the International Space Station in November 2007. Tyndall Glacier is located in the Torres del Paine National Park in Chile. This glacier, which has a total area of 331 square kilometers and a length of 32 kilometers (based on 1996 measurements), begins in the Patagonian Andes Mountains to the west and terminates in Lago Geikie. The digital astronaut photograph taken in november 2007 records visible light in red, green, and blue wavelengths (true color). The Tyndall Glacier terminus has retreated significantly during the past 17 years. Significant ice loss was also observed earlier this year at Grey Glacier, about 30 kilometers to the north - northeast, suggesting both glaciers are responding similarly to regional changes in temperature and precipitation. A medial moraine is visible in the center of the glacier, extending along its length (top image, center le

Tyndall Glacier, Chile - Tyndall Glacier, Chile - The Tyndall Glacier in Torres del Paine National Park in Chile, observed from the International Space Station in November 2007. Tyndall Glacier is located in the Torres del Paine National Park in Chile. This glacier, which has a total area of 331 square kilometers and a length of 32 kilometers (based on 1996 measurements), begins in the Patagonian Andes Mountains to the west and terminates in Lago Geikie. The digital astronaut photograph taken in november 2007 records visible light in red, green, and blue wavelengths (true color). The Tyndall Glacier terminus has retreated significantly during the past 17 years. Significant ice loss was also observed earlier this year at Grey Glacier, about 30 kilometers to the north - northeast, suggesting both glaciers are responding similarly to regional changes in temperature and precipitation. A medial moraine is visible in the center of the glacier, extending along its length (top image, center le

PIX4675989

Nebula NGC 6726 - 27 - 29 in the Southern Crown - The Corona Australis nebula (NGC 6726 - 27 - 29) Image of R Coronae Australis region in the southern Milky Way, obtained with the Wide Field Imager (WFI) (camera) at the 2.2 - m MPG/ESO Telescope on La Silla (Chile). The sky field shown measures approx. 33.7 x 31.9 arcmin2 (about the diameter of the full moon). The R Coronae Australis complex of young stars and interstellar gas clouds is one of the nearest star - forming regions, at a distance of approx. 500 light - years from the Sun. It is seen in the southern constellation of that name (The “Southern Crown”). R Coronae Australis, the bright star from which the entire complex is named, is located at the center of the field and illuminates the reddish nebula around it. The bright star in the lower part, illuminating a somewhat bluer nebula, is known as TY Coronae Australis. The brightness of these two stars and several others in the same field is variable. They belong to the so - calle

Nebula NGC 6726 - 27 - 29 in the Southern Crown - The Corona Australis nebula (NGC 6726 - 27 - 29) Image of R Coronae Australis region in the southern Milky Way, obtained with the Wide Field Imager (WFI) (camera) at the 2.2 - m MPG/ESO Telescope on La Silla (Chile). The sky field shown measures approx. 33.7 x 31.9 arcmin2 (about the diameter of the full moon). The R Coronae Australis complex of young stars and interstellar gas clouds is one of the nearest star - forming regions, at a distance of approx. 500 light - years from the Sun. It is seen in the southern constellation of that name (The “Southern Crown”). R Coronae Australis, the bright star from which the entire complex is named, is located at the center of the field and illuminates the reddish nebula around it. The bright star in the lower part, illuminating a somewhat bluer nebula, is known as TY Coronae Australis. The brightness of these two stars and several others in the same field is variable. They belong to the so - calle

PIX4620222

Dolly Rathebe - Dolly and Her Men! - The World Does Not Suspect That Film Star Dolly…, 1957 (photo)

Dolly Rathebe - Dolly and Her Men! - The World Does Not Suspect That Film Star Dolly…, 1957 (photo)

Jürgen Schadeberg

AMD8679285

Southern Crown Nebula - The Corona Australis nebula (NGC 6726 - 27 - 29) - R Coronae Australis is one of the closest and most intense star-forming regions; visible in the southern hemisphere, it is located about 500 years from Earth. R Coronae Australis is the star in the center of the image that illuminates a reddish nebula around it. Image obtained in Chile at the observatory of La Silla with the 2.2 meter MPG/ESO telescope. Image of R Coronae Australis region in the southern Milky Way, obtained with the Wide Field Imager (WFI) (camera) at the 2.2 - m MPG/ESO Telescope on La Silla (Chile). The R Coronae Australis complex of young stars and interstellar gas clouds is one of the nearest star - forming regions, at a distance of approx. 500 light - years from the Sun. It is seen in the southern constellation of that name (The “Southern Crown”). R Coronae Australis, the bright star from which the entire complex is named, is located at the center of the field and illuminates the reddish ne

Southern Crown Nebula - The Corona Australis nebula (NGC 6726 - 27 - 29) - R Coronae Australis is one of the closest and most intense star-forming regions; visible in the southern hemisphere, it is located about 500 years from Earth. R Coronae Australis is the star in the center of the image that illuminates a reddish nebula around it. Image obtained in Chile at the observatory of La Silla with the 2.2 meter MPG/ESO telescope. Image of R Coronae Australis region in the southern Milky Way, obtained with the Wide Field Imager (WFI) (camera) at the 2.2 - m MPG/ESO Telescope on La Silla (Chile). The R Coronae Australis complex of young stars and interstellar gas clouds is one of the nearest star - forming regions, at a distance of approx. 500 light - years from the Sun. It is seen in the southern constellation of that name (The “Southern Crown”). R Coronae Australis, the bright star from which the entire complex is named, is located at the center of the field and illuminates the reddish ne

PIX4620317

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