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Rhea, satellite of Saturn, seen by Cassini - Saturn's moon Rhea seen by Cassini - Mosaic of images obtained by the Cassini probe in March 2015. Rhea is the second largest satellite in Saturn (1528 km in diameter). After a couple of years in high - inclination orbits that limited its ability to encounter Saturn's moons, Nasa's Cassini spacecraft returned to Saturn's equatorial plane in March 2015.Image taken using clear, green, infrared and ultraviolet spectral filters were combined to create these enhanced color views, which offer an expanded range of the colors visible to human eyes in order to highlight subtle color differences across Rhea's surface. The moon's surface is fairly uniform in natural color.This view at right is centered at 9 degrees north latitude, 254 degrees west longitude. Resolution in this mosaic is 300 meters (984 feet) per pixel. The image was acquired at a distance that ranged from about 36,000 to 32.100 miles (57,900 to 51,700 kilometers) from Rhea

Rhea, satellite of Saturn, seen by Cassini - Saturn's moon Rhea seen by Cassini - Mosaic of images obtained by the Cassini probe in March 2015. Rhea is the second largest satellite in Saturn (1528 km in diameter). After a couple of years in high - inclination orbits that limited its ability to encounter Saturn's moons, Nasa's Cassini spacecraft returned to Saturn's equatorial plane in March 2015.Image taken using clear, green, infrared and ultraviolet spectral filters were combined to create these enhanced color views, which offer an expanded range of the colors visible to human eyes in order to highlight subtle color differences across Rhea's surface. The moon's surface is fairly uniform in natural color.This view at right is centered at 9 degrees north latitude, 254 degrees west longitude. Resolution in this mosaic is 300 meters (984 feet) per pixel. The image was acquired at a distance that ranged from about 36,000 to 32.100 miles (57,900 to 51,700 kilometers) from Rhea

PIX4625591

Reindeer farm in Salla, Lapland Finland, 2022 (photography)

Reindeer farm in Salla, Lapland Finland, 2022 (photography)

Sergi Reboredo

SRB7333234

Reindeer farm in Salla, Lapland Finland, 2022 (photography)

Reindeer farm in Salla, Lapland Finland, 2022 (photography)

Sergi Reboredo

SRB7333233

Dione, satellite of Saturn, seen by Cassini - Dione, moon of Saturn, as seen by Cassini - Mosaic of images obtained by the Cassini probe on 11 October 2005 at a distance of about 25,000 km from the satellite. As it departed its encounter with Saturn's moon Dione, Cassini sailed above an unreal landscape blasted by impacts. The rising Sun throws craters into sharp contrast and reveals steep crater walls. At the far right, a medium - sized crater is bisected by a fracture, revealing a cross section of the impact site. The seven clear - filter images in this mosaic were taken with the Cassini spacecraft narrow - angle camera on Oct. 11, 2005, at distances ranging from 21.650 to 25.580 kilometers (13,450 to 15,890 miles) from Dione and at a Sun - Dione - spacecraft, or phase, angle of 154 degrees. Resolution in the original images ranges from 126 to 154 meters (413 to 505 feet) per pixel. The images have been re - sized to have an image scale of about 100 meters (330 feet) per pixel. North

Dione, satellite of Saturn, seen by Cassini - Dione, moon of Saturn, as seen by Cassini - Mosaic of images obtained by the Cassini probe on 11 October 2005 at a distance of about 25,000 km from the satellite. As it departed its encounter with Saturn's moon Dione, Cassini sailed above an unreal landscape blasted by impacts. The rising Sun throws craters into sharp contrast and reveals steep crater walls. At the far right, a medium - sized crater is bisected by a fracture, revealing a cross section of the impact site. The seven clear - filter images in this mosaic were taken with the Cassini spacecraft narrow - angle camera on Oct. 11, 2005, at distances ranging from 21.650 to 25.580 kilometers (13,450 to 15,890 miles) from Dione and at a Sun - Dione - spacecraft, or phase, angle of 154 degrees. Resolution in the original images ranges from 126 to 154 meters (413 to 505 feet) per pixel. The images have been re - sized to have an image scale of about 100 meters (330 feet) per pixel. North

PIX4625507

Spiral galaxy of the Sombrero M104 infrared view - Sombrero galaxy seen in infrared - Infrared image of the spiral galaxy M104 (Sombrero galaxy), located about 28 million years ago - light, obtained with the Spitzer space telescope in 2004 and January 2005. Infrared radiation shows the dust of the disc visible throughout the circumference. A high emission also comes from the center of the galaxy where a supermassive black hole is thought to reside there. This spiral galaxy is located some 28 million light - years away. The infrared image obtained by Spitzer space telescope in 2004 and 2005 pierces through the obscuring dust, along with the bulge of stars. It shows that the disk is warped, which is often the result of a gravitational encounter with another galaxy; clumpy areas spotted in the far edges of the ring indicate young star - forming regions. Spitzer detected infrared emission not only from the ring, but from the center of the galaxy too, where there is a huge black hole, belie

Spiral galaxy of the Sombrero M104 infrared view - Sombrero galaxy seen in infrared - Infrared image of the spiral galaxy M104 (Sombrero galaxy), located about 28 million years ago - light, obtained with the Spitzer space telescope in 2004 and January 2005. Infrared radiation shows the dust of the disc visible throughout the circumference. A high emission also comes from the center of the galaxy where a supermassive black hole is thought to reside there. This spiral galaxy is located some 28 million light - years away. The infrared image obtained by Spitzer space telescope in 2004 and 2005 pierces through the obscuring dust, along with the bulge of stars. It shows that the disk is warped, which is often the result of a gravitational encounter with another galaxy; clumpy areas spotted in the far edges of the ring indicate young star - forming regions. Spitzer detected infrared emission not only from the ring, but from the center of the galaxy too, where there is a huge black hole, belie

PIX4611595

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

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

PIX4610090

Photocopies of credit card receipts giving waitress Colleen Gallagher a $1,000 tip (L) and $10,000 t.., 2001-07-12 (photo)

Photocopies of credit card receipts giving waitress Colleen Gallagher a $1,000 tip (L) and $10,000 t.., 2001-07-12 (photo)

Sue Ogrocki

REU7532600

Galaxy clusters Abell 1060 in Hydra - The Hydra cluster of galaxies (Abell 1060) - The galaxy in the center is the spiral galaxy NGC 3312. To its right, the brightest elliptical galaxies of this cluster: NGC 3311. The two bright stars are closer and belong to our galaxy. This splendid cluster of galaxies in Hydra is framed by two nearby, cool stars in our own Milky Way. The brightest is about 5th magnitude, visible to the unaided eye only under a dark sky; the second brightest is below naked - eye visibility. In contrast the galaxies appear featureless in all but the largest telescopes. The bluish, elongated galaxy is an edge - on spiral, NGC 3312. It has been distorted by interactions with its neighbours. They in turn have been affected, and the brightest of the two adjacent yellow elliptical galaxies (NGC 3311) has an assymetrical envelope, perhaps as a result of this encounter. It's hard to tell who is jostling who in a crowded group of galaxies such as this. Among the most interest

Galaxy clusters Abell 1060 in Hydra - The Hydra cluster of galaxies (Abell 1060) - The galaxy in the center is the spiral galaxy NGC 3312. To its right, the brightest elliptical galaxies of this cluster: NGC 3311. The two bright stars are closer and belong to our galaxy. This splendid cluster of galaxies in Hydra is framed by two nearby, cool stars in our own Milky Way. The brightest is about 5th magnitude, visible to the unaided eye only under a dark sky; the second brightest is below naked - eye visibility. In contrast the galaxies appear featureless in all but the largest telescopes. The bluish, elongated galaxy is an edge - on spiral, NGC 3312. It has been distorted by interactions with its neighbours. They in turn have been affected, and the brightest of the two adjacent yellow elliptical galaxies (NGC 3311) has an assymetrical envelope, perhaps as a result of this encounter. It's hard to tell who is jostling who in a crowded group of galaxies such as this. Among the most interest

PIX4565253

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

Galaxy clusters Abell 1060 in Hydra - The Hydra cluster of galaxies (Abell 1060) - The galaxy in the center is the spiral galaxy NGC 3312. To its right, the brightest elliptical galaxies of this cluster: NGC 3311. The two bright stars are closer and belong to our galaxy. This splendid cluster of galaxies in Hydra is framed by two nearby, cool stars in our own Milky Way. The brightest is about 5th magnitude, visible to the unaided eye only under a dark sky; the second brightest is below naked - eye visibility. In contrast the galaxies appear featureless in all but the largest telescopes. The bluish, elongated galaxy is an edge - on spiral, NGC 3312. It has been distorted by interactions with its neighbours. They in turn have been affected, and the brightest of the two adjacent yellow elliptical galaxies (NGC 3311) has an assymetrical envelope, perhaps as a result of this encounter. It's hard to tell who is jostling who in a crowded group of galaxies such as this. Among the most interest

Galaxy clusters Abell 1060 in Hydra - The Hydra cluster of galaxies (Abell 1060) - The galaxy in the center is the spiral galaxy NGC 3312. To its right, the brightest elliptical galaxies of this cluster: NGC 3311. The two bright stars are closer and belong to our galaxy. This splendid cluster of galaxies in Hydra is framed by two nearby, cool stars in our own Milky Way. The brightest is about 5th magnitude, visible to the unaided eye only under a dark sky; the second brightest is below naked - eye visibility. In contrast the galaxies appear featureless in all but the largest telescopes. The bluish, elongated galaxy is an edge - on spiral, NGC 3312. It has been distorted by interactions with its neighbours. They in turn have been affected, and the brightest of the two adjacent yellow elliptical galaxies (NGC 3311) has an assymetrical envelope, perhaps as a result of this encounter. It's hard to tell who is jostling who in a crowded group of galaxies such as this. Among the most interest

PIX4565268

Nov 29, 1943 - Tehran, Iran - Historical encounter between General Secretary of the Communist Party JOSEPH STALIN, the U.S. President FRANKLIN D. ROOSEVELT and U.K. Prime Minister Sir WINSTON CHURCHILL during the Teheran Conference. The Tehran Conference (codenamed Eureka) was a strategy meeting held between Joseph Stalin, Franklin D. Roosevelt, and Winston Churchill from November 28 to December 1, 1943. It was held in the Soviet Embassy in Tehran, Iran and was the first of the World War II conferences held between all of the 'Big Three' Allied leaders (the Soviet Union, the United States, and the United Kingdom). During the Conference, the three leaders coordinated their military strategy against Germany and Japan and made a number of important decisions concerning the post World War II era. The most notable achievements of the Conference focused on the next phases of the war against the Axis powers in Europe and Asia. Roosevelt, Churchill, and Stalin engaged in discussions concerning

Nov 29, 1943 - Tehran, Iran - Historical encounter between General Secretary of the Communist Party JOSEPH STALIN, the U.S. President FRANKLIN D. ROOSEVELT and U.K. Prime Minister Sir WINSTON CHURCHILL during the Teheran Conference. The Tehran Conference (codenamed Eureka) was a strategy meeting held between Joseph Stalin, Franklin D. Roosevelt, and Winston Churchill from November 28 to December 1, 1943. It was held in the Soviet Embassy in Tehran, Iran and was the first of the World War II conferences held between all of the 'Big Three' Allied leaders (the Soviet Union, the United States, and the United Kingdom). During the Conference, the three leaders coordinated their military strategy against Germany and Japan and made a number of important decisions concerning the post World War II era. The most notable achievements of the Conference focused on the next phases of the war against the Axis powers in Europe and Asia. Roosevelt, Churchill, and Stalin engaged in discussions concerning

ZUM4869724

Replica Victoria Cross awarded to Private John Connors VC, 3rd (The East Kent) Regiment of Foot (The Buffs) (metal)

Replica Victoria Cross awarded to Private John Connors VC, 3rd (The East Kent) Regiment of Foot (The Buffs) (metal)

British School, (19th century)

NAM5925143

Replica Victoria Cross awarded to Private John Connors VC, 3rd (The East Kent) Regiment of Foot (The Buffs) (metal)

Replica Victoria Cross awarded to Private John Connors VC, 3rd (The East Kent) Regiment of Foot (The Buffs) (metal)

British School, (19th century)

NAM5925144

Sombrero M104 Spiral Galaxy - Visible Composite - Infrared - The Sombrero galaxy. Composite of visible and infrared views - Composite image of the spiral galaxy M104 (Sombrero galaxy), located about 28 million years ago - light. Infrared image obtained with the Spitzer space telescope in 2004 and January 2005 superimposed on the image made by the Hubble space telescope visible in May and June 2003. The dark band of girders in this galaxy is visible throughout the circumference. Composite image of a visible image and an infrared image of the galaxy M104. The visible image was obtained by the Hubble space telescope in 2003, the infrared view by Spitzer telescope in 2004 and 2005. This spiral galaxy is located some 28 million light - years away. The infrared image obtained by Spitzer space telescope pierces through the obscuring dust, along with the bulge of stars. It shows that the disk is warped, which is often the result of a gravitational encounter with another galaxy; clumpy areas sp

Sombrero M104 Spiral Galaxy - Visible Composite - Infrared - The Sombrero galaxy. Composite of visible and infrared views - Composite image of the spiral galaxy M104 (Sombrero galaxy), located about 28 million years ago - light. Infrared image obtained with the Spitzer space telescope in 2004 and January 2005 superimposed on the image made by the Hubble space telescope visible in May and June 2003. The dark band of girders in this galaxy is visible throughout the circumference. Composite image of a visible image and an infrared image of the galaxy M104. The visible image was obtained by the Hubble space telescope in 2003, the infrared view by Spitzer telescope in 2004 and 2005. This spiral galaxy is located some 28 million light - years away. The infrared image obtained by Spitzer space telescope pierces through the obscuring dust, along with the bulge of stars. It shows that the disk is warped, which is often the result of a gravitational encounter with another galaxy; clumpy areas sp

PIX4611601

Silver Regimental Medal, Private John Connors, 3rd (The East Kent) Regiment of Foot (The Buffs), 1855 (metal)

Silver Regimental Medal, Private John Connors, 3rd (The East Kent) Regiment of Foot (The Buffs), 1855 (metal)

British School, (19th century)

NAM5925150

Silver Regimental Medal, Private John Connors, 3rd (The East Kent) Regiment of Foot (The Buffs), 1855 (metal)

Silver Regimental Medal, Private John Connors, 3rd (The East Kent) Regiment of Foot (The Buffs), 1855 (metal)

British School, (19th century)

NAM5925149

Henry VIII's deposition to convocation on his marriage with Anne of Cleves and questions to be put to Thomas Cromwell, 1540. In Henry's hand. Determined to nullify his marriage to Anne, Henry drafted in evidence a deposition and a series of questions to be put to Cromwell, who had been arrested on 10 June on charges of high treason. Henry testified that, when Cromwell asked how he liked Anne after their first encounter at Rochester, he had responded 'nothyng soo well as she was spokyn off and ... that yff [I] had knowne so moche before, she shuld nott have come hyt[her]'. The King also claimed that when Cromwell asked him the day after the wedding if he liked Anne better, he replied, not at all for by her breasts and belly he thought her no maid, and when he touched her he had no will to prove otherwise

Henry VIII's deposition to convocation on his marriage with Anne of Cleves and questions to be put to Thomas Cromwell, 1540. In Henry's hand. Determined to nullify his marriage to Anne, Henry drafted in evidence a deposition and a series of questions to be put to Cromwell, who had been arrested on 10 June on charges of high treason. Henry testified that, when Cromwell asked how he liked Anne after their first encounter at Rochester, he had responded 'nothyng soo well as she was spokyn off and ... that yff [I] had knowne so moche before, she shuld nott have come hyt[her]'. The King also claimed that when Cromwell asked him the day after the wedding if he liked Anne better, he replied, not at all for by her breasts and belly he thought her no maid, and when he touched her he had no will to prove otherwise

BL3287728

Interacting galaxies Arp 81 - Interacting galaxies Arp 81 - Arp 81 is located about 300 million light years away from Earth in the constellation Dragon. This pair of interacting galaxies is composed of NGC 6621 on the left and NGC 6622 on the right. NGC 6621 is the largest of the two galaxies. The collision, seen here about 100 million years later, caused intense star flames. Image obtained by the Hubble Space Telescope on 15 March 1999. NGC 6621/2 (VV 247, Arp 81) is a strongly interacting pair of galaxies, seen about 100 million years after their closest approach. It consists of NGC 6621 (to the left) and NGC 6622 (to the right). NGC 6621 is the larger of the two, and is a very disturbed spiral galaxy. The encounter has pulled a long tail out of NGC 6621 that has now wrapped behind its body. The collision has also triggered extensive star formation between the two galaxies. Scientists believe that Arp 81 has a richer collection of young massive star clusters than the notable Antennae

Interacting galaxies Arp 81 - Interacting galaxies Arp 81 - Arp 81 is located about 300 million light years away from Earth in the constellation Dragon. This pair of interacting galaxies is composed of NGC 6621 on the left and NGC 6622 on the right. NGC 6621 is the largest of the two galaxies. The collision, seen here about 100 million years later, caused intense star flames. Image obtained by the Hubble Space Telescope on 15 March 1999. NGC 6621/2 (VV 247, Arp 81) is a strongly interacting pair of galaxies, seen about 100 million years after their closest approach. It consists of NGC 6621 (to the left) and NGC 6622 (to the right). NGC 6621 is the larger of the two, and is a very disturbed spiral galaxy. The encounter has pulled a long tail out of NGC 6621 that has now wrapped behind its body. The collision has also triggered extensive star formation between the two galaxies. Scientists believe that Arp 81 has a richer collection of young massive star clusters than the notable Antennae

PIX4612937

Fridtjof Nansen, 1893 (photo)

Fridtjof Nansen, 1893 (photo)

SJB8899753

Mungo Park, 1771 To 1806, Scottish Explorer, Encountering A Lion Whilst On His Way To The Village Of Modiboo During His Exploration Of Africa In 1795. From The Life And Travels Of Mungo Park Published 1875 ©UIG/Leemage

Mungo Park, 1771 To 1806, Scottish Explorer, Encountering A Lion Whilst On His Way To The Village Of Modiboo During His Exploration Of Africa In 1795. From The Life And Travels Of Mungo Park Published 1875 ©UIG/Leemage

UIG5420144

Interacting galaxies NGC 4038 - 4039 in the Raven - The Antennae galaxy in Corvus - On the left, seen from the ground of the galaxy NGC 4038 - 39 (antenna galaxy), located about 45 million years ago - light. These two galaxies are interacting. The collision started at least 100 million years ago causes intense star formation. On the right, the image made by the space telescope Hubble on 20 January 1996 shows in detail the nuclei of these two twin galaxies surrounded by young clusters of blue stars, more than 1000, made up of young and massive stars. At left, a ground - based telescopic view of the Antennae galaxies (known formally as NGC 4038/4039) - so named because a pair of long tails of luminous matter, formed by the gravitational tidal forces of their encounter, resemble an insect's antennae. The galaxies are located 45 million light - years away in the southern constellation Corvus. At right, the respective cores of the twin galaxies are the orange blobs, left and right of image

Interacting galaxies NGC 4038 - 4039 in the Raven - The Antennae galaxy in Corvus - On the left, seen from the ground of the galaxy NGC 4038 - 39 (antenna galaxy), located about 45 million years ago - light. These two galaxies are interacting. The collision started at least 100 million years ago causes intense star formation. On the right, the image made by the space telescope Hubble on 20 January 1996 shows in detail the nuclei of these two twin galaxies surrounded by young clusters of blue stars, more than 1000, made up of young and massive stars. At left, a ground - based telescopic view of the Antennae galaxies (known formally as NGC 4038/4039) - so named because a pair of long tails of luminous matter, formed by the gravitational tidal forces of their encounter, resemble an insect's antennae. The galaxies are located 45 million light - years away in the southern constellation Corvus. At right, the respective cores of the twin galaxies are the orange blobs, left and right of image

PIX4611051

Dwarf galaxy Holmberg IX in the Great Bear - Dwarf galaxy Holmberg IX in Ursa Major - The dwarf galaxy Holmberg IX is located 12 million years - light from Earth in the constellation of the Great Bear, just above the spiral galaxy M81. Of the 20,000 stars visible on this image obtained by the Hubble space telescope, more than 90% are young stars aged between 10 and 200 million years. The proximity of other galaxies, including M81, is believed to be at the origin of this recent star formation. This loose collection of stars is actually a dwarf irregular galaxy, called Holmberg IX. It resides just off the outer edge of M81, a large spiral galaxy in Ursa Major. This image was taken with Hubble's Advanced Camera for Surveys in early 2006. Holmberg IX is of the so - called Magellanic type of galaxy, as its size and irregularity in structure are similar to the Small Magellanic Cloud, a neighbour to our own Milky Way. It is suspected that the dwarf galaxy was created as a result of a galactic

Dwarf galaxy Holmberg IX in the Great Bear - Dwarf galaxy Holmberg IX in Ursa Major - The dwarf galaxy Holmberg IX is located 12 million years - light from Earth in the constellation of the Great Bear, just above the spiral galaxy M81. Of the 20,000 stars visible on this image obtained by the Hubble space telescope, more than 90% are young stars aged between 10 and 200 million years. The proximity of other galaxies, including M81, is believed to be at the origin of this recent star formation. This loose collection of stars is actually a dwarf irregular galaxy, called Holmberg IX. It resides just off the outer edge of M81, a large spiral galaxy in Ursa Major. This image was taken with Hubble's Advanced Camera for Surveys in early 2006. Holmberg IX is of the so - called Magellanic type of galaxy, as its size and irregularity in structure are similar to the Small Magellanic Cloud, a neighbour to our own Milky Way. It is suspected that the dwarf galaxy was created as a result of a galactic

PIX4613880

King Francois I Of France Advances To Meet King Henry Viii Of England At The Field Of The Cloth Of Gold In June, 1520. From Les Artes Au Moyen Age, Published Paris 1873 ©UIG/Leemage

King Francois I Of France Advances To Meet King Henry Viii Of England At The Field Of The Cloth Of Gold In June, 1520. From Les Artes Au Moyen Age, Published Paris 1873 ©UIG/Leemage

UIG5420225

Chibe National Park, Botswana (photo)

Chibe National Park, Botswana (photo)

Sergi Reboredo

SRB1202626

Elephants, Chobe National Park (Zambia) (photo)

Elephants, Chobe National Park (Zambia) (photo)

Sergi Reboredo

SRB1202874

Elephants, Chobe National Park (Zambia) (photo)

Elephants, Chobe National Park (Zambia) (photo)

Sergi Reboredo

SRB1202875

Elephants, Chobe National Park (Zambia) (photo)

Elephants, Chobe National Park (Zambia) (photo)

Sergi Reboredo

SRB1202876

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

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

Galaxy M82 view in different wavelength - Galaxy M82 in multi - wavelength - Composite of different images: in blue the image obtained by Chandra in X-rays, in red the infrared image obtained by Spitzer, in yellow, orange, green, the image of Hubble. M82 is an irregular galaxy distant about 12 million years - light from Earth. Its nucleus, which appears to have suffered from the passage of the neighbouring galaxy M81, is in a phase of violent star activity. Its central regions are rich in star formation. These hot stars blow a stellar wind that becomes a very violent galactic wind. Composite of multi - wavelength images of the active galaxy M82 from the three Great Observatories. X - ray data recorded by Chandra appears here in blue; infrared light recorded by Spitzer appears in red; Hubble's observations of hydrogen emission appears in orange, and the bluest visible light appears in yellow - green. Another Hubble observation designed to image 10,000 degree Celsius hydrogen gas (orange

Galaxy M82 view in different wavelength - Galaxy M82 in multi - wavelength - Composite of different images: in blue the image obtained by Chandra in X-rays, in red the infrared image obtained by Spitzer, in yellow, orange, green, the image of Hubble. M82 is an irregular galaxy distant about 12 million years - light from Earth. Its nucleus, which appears to have suffered from the passage of the neighbouring galaxy M81, is in a phase of violent star activity. Its central regions are rich in star formation. These hot stars blow a stellar wind that becomes a very violent galactic wind. Composite of multi - wavelength images of the active galaxy M82 from the three Great Observatories. X - ray data recorded by Chandra appears here in blue; infrared light recorded by Spitzer appears in red; Hubble's observations of hydrogen emission appears in orange, and the bluest visible light appears in yellow - green. Another Hubble observation designed to image 10,000 degree Celsius hydrogen gas (orange

PIX4610442

Saturn seen by the Cassini probe on 10 - 09 - 2007 - Saturn seen by Cassini spacecraft Sept. 10 2007. - Saturn seen by the Cassini probe on 10 - 09 - 2007 at a distance of 3.3 million km from the planet shortly before it flew over the Japet satellite. Mosaic of 45 images. Several satellites are visible in this image; from right to left: Titan, Tethys, Rhea, Mimas, Enceladus and Dione. While on final approach for its Sept. 2007 close encounter with Saturn's moon Iapetus, Cassini spun around to take in a sweeping view of the Saturn System. Iapetus (1,468 kilometers, or 912 miles across) is the only major moon of Saturn with a significant inclination to its orbit. From the other major satellites, the rings would appear almost edge - on, but from Iapetus, the rings usually appear at a tilt, as seen here. This natural color mosaic consists of 15 red, green and blue spectral filter images acquired in five wide - angle camera footprints that swept across the scene. Moons visible in this image

Saturn seen by the Cassini probe on 10 - 09 - 2007 - Saturn seen by Cassini spacecraft Sept. 10 2007. - Saturn seen by the Cassini probe on 10 - 09 - 2007 at a distance of 3.3 million km from the planet shortly before it flew over the Japet satellite. Mosaic of 45 images. Several satellites are visible in this image; from right to left: Titan, Tethys, Rhea, Mimas, Enceladus and Dione. While on final approach for its Sept. 2007 close encounter with Saturn's moon Iapetus, Cassini spun around to take in a sweeping view of the Saturn System. Iapetus (1,468 kilometers, or 912 miles across) is the only major moon of Saturn with a significant inclination to its orbit. From the other major satellites, the rings would appear almost edge - on, but from Iapetus, the rings usually appear at a tilt, as seen here. This natural color mosaic consists of 15 red, green and blue spectral filter images acquired in five wide - angle camera footprints that swept across the scene. Moons visible in this image

PIX4625105

The Battle of Quiberon Bay, 20 November 1759, 1779 (oil painting)

The Battle of Quiberon Bay, 20 November 1759, 1779 (oil painting)

Serres, Dominic (1722-93)

MMM7337655

The Battle of Quiberon Bay, 20 November 1759, 1812 (oil painting)

The Battle of Quiberon Bay, 20 November 1759, 1812 (oil painting)

Pocock, Nicholas (1741-1821)

MMM7337656

The Battle of Quiberon Bay, 20 November 1759 (oil painting)

The Battle of Quiberon Bay, 20 November 1759 (oil painting)

Paton, Richard (1717-91)

MMM7337654

Cinderella tries the glass shoe found by the prince. Illustration of Charles Perrault's tale “Cinderella or La petite slipper de verre”, 1697. In “” Tales from the home for the little ones””. Anonymous engraving of the 19th century.

Cinderella tries the glass shoe found by the prince. Illustration of Charles Perrault's tale “Cinderella or La petite slipper de verre”, 1697. In “” Tales from the home for the little ones””. Anonymous engraving of the 19th century.

Unknown Artist, (19th century)

Stefano Bianchetti

XEE4404543

Sleeping Beauty: illustration of Charles Perrault's tale. The prince enters the room and sees the young woman asleep. Chromolithography of the late 19th century

Sleeping Beauty: illustration of Charles Perrault's tale. The prince enters the room and sees the young woman asleep. Chromolithography of the late 19th century

Jaime Abecasis

JAB5036977

The Marquis of Carabas, the princess and the king in the castle. Illustration of the tale “The cat botte” by Charles Perrault, 1697. In “” Tales from the home for the little ones””. Anonymous engraving of the 19th century.

The Marquis of Carabas, the princess and the king in the castle. Illustration of the tale “The cat botte” by Charles Perrault, 1697. In “” Tales from the home for the little ones””. Anonymous engraving of the 19th century.

Unknown Artist, (19th century)

Stefano Bianchetti

XEE4404563

The prince picks up the glass shoe by Cinderella. Illustration of Charles Perrault's tale “Cinderella or La petite slipper de verre”, 1697. In “” Tales from the home for the little ones””. Anonymous engraving of the 19th century.

The prince picks up the glass shoe by Cinderella. Illustration of Charles Perrault's tale “Cinderella or La petite slipper de verre”, 1697. In “” Tales from the home for the little ones””. Anonymous engraving of the 19th century.

Unknown Artist, (19th century)

Stefano Bianchetti

XEE4404553

Tale by Charles Perrault: Riquet has the crown. The little prince addresses the beautiful and witty princess and announces that he has the power to give spirit to the woman he is in love with. Chromolithography of the late 19th century

Tale by Charles Perrault: Riquet has the crown. The little prince addresses the beautiful and witty princess and announces that he has the power to give spirit to the woman he is in love with. Chromolithography of the late 19th century

Jaime Abecasis

JAB5037006

The two boys (litho)

The two boys (litho)

English School, (19th century)

LLM5207663

Meeting between the Russian Tsar Alexander II (1818-1881) and the Austrian Emperor Francois Joseph I (1830-1916) at the Belvedere in Weimar (Germany). From left to right are Alexander II, Francois Joseph I, Charles Alexander Duke of Saxony-Weimar-Eisenach (Charles Alexander Duke of Saxony Weimar Eisenach) (1818-1901), Prince Alexander of Hesse Darmstadt (Hesse-Darmstadt) (1823-1898) and Count Grunne. Engraving In “” The illustrated London News”” of 31 October 1857.

Meeting between the Russian Tsar Alexander II (1818-1881) and the Austrian Emperor Francois Joseph I (1830-1916) at the Belvedere in Weimar (Germany). From left to right are Alexander II, Francois Joseph I, Charles Alexander Duke of Saxony-Weimar-Eisenach (Charles Alexander Duke of Saxony Weimar Eisenach) (1818-1901), Prince Alexander of Hesse Darmstadt (Hesse-Darmstadt) (1823-1898) and Count Grunne. Engraving In “” The illustrated London News”” of 31 October 1857.

Unknown Artist, (19th century)

Stefano Bianchetti

XEE4143998

Anonymous illustration for “La belle au bois dormant”, tale by Charles Perrault (1628-1703), French writer. Wood engraving of Imaging Pellerin - Epinal, sd. Late 19th century.

Anonymous illustration for “La belle au bois dormant”, tale by Charles Perrault (1628-1703), French writer. Wood engraving of Imaging Pellerin - Epinal, sd. Late 19th century.

French School, (19th century)

Stefano Bianchetti

XEE4133094

Interview between Marlborough and Charles XII of Sweden, Altranstadt (1707), c.1890 (engraving)

Interview between Marlborough and Charles XII of Sweden, Altranstadt (1707), c.1890 (engraving)

Ken Welsh

KWE7212151

The Queen and Chariot (colour litho)

The Queen and Chariot (colour litho)

Molino, Walter (1915-1997)

LLM2785247

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