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Ascetic devotees hang from a spinning wheel attached with 'Charhak tree' on the occasion of Charak Puja at Shah Dhamrai, Dhaka, Bangladesh on April 15, 2006. Charhak Puja is observed on the last days of the Bangla month of Chaitra (April) called Chatitra Sangkranti. Farmers celebrate during this festival with the devotees singing and dancing without any care. The Charak Puja is well-known for the rites of piercing the body with nails, and swirling from a high pole. A 'charhak tree' is built on the occasion, consisting of a long pole atop which a wheel is fixed. An ascetic devotee is hung from this wheel with a hook. The wheel then spins around with him at high speed. Small nails, at times red hot ones, pierce all parts of his body including his tongue. The devotee thus spinning spreads prasad (handmade sweetmeats blessed with chants) among the curious spectators and onlookers. At the root of the celebration of Charhak Puja is a belief in spirits and the cult of rebirth. Its rites sugge

UIG798118

Ascetic devotees hang from a spinning wheel attached with 'Charhak tree' on the occasion of Charak Puja at Shah Dhamrai, Dhaka, Bangladesh on April 15, 2006. Charhak Puja is observed on the last days of the Bangla month of Chaitra (April) called Chatitra Sangkranti. Farmers celebrate during this festival with the devotees singing and dancing without any care. The Charak Puja is well-known for the rites of piercing the body with nails, and swirling from a high pole. A 'charhak tree' is built on the occasion, consisting of a long pole atop which a wheel is fixed. An ascetic devotee is hung from this wheel with a hook. The wheel then spins around with him at high speed. Small nails, at times red hot ones, pierce all parts of his body including his tongue. The devotee thus spinning spreads prasad (handmade sweetmeats blessed with chants) among the curious spectators and onlookers. At the root of the celebration of Charhak Puja is a belief in spirits and the cult of rebirth. Its rites sugge

UIG798118

 
Spiral galaxy NGC 2683 in Lynx - Spiral galaxy NGC 2683 in Lynx - Spiral galaxy NGC 2683 distant about 16 million years - light in the constellation Lynx. Image obtained by the Hubble Space Telescope (HST). NGC 2683 is a spiral galaxy seen almost edge - on, giving it the shape of a classic science fiction spaceship. The delicate dusty lanes of the spiral arms are silhouetted against the golden haze of the galaxy's core. In addition, brilliant clusters of young blue stars shine scattered throughout the disc, mapping the galaxy's star - forming regions. Perhaps surprisingly, side - on views of galaxies like this one do not prevent astronomers from deducing their structures. Studies of the properties of the light coming from NGC 2683 suggest that this is a barred spiral galaxy, even though the angle we see it at does not let us see this directly. NGC 2683, discovered on 5 February 1788 by the famous astronomer William Herschel, lies in the Northern constellation of Lynx. A constellation n

PIX4610165

Spiral galaxy NGC 2683 in Lynx - Spiral galaxy NGC 2683 in Lynx - Spiral galaxy NGC 2683 distant about 16 million years - light in the constellation Lynx. Image obtained by the Hubble Space Telescope (HST). NGC 2683 is a spiral galaxy seen almost edge - on, giving it the shape of a classic science fiction spaceship. The delicate dusty lanes of the spiral arms are silhouetted against the golden haze of the galaxy's core. In addition, brilliant clusters of young blue stars shine scattered throughout the disc, mapping the galaxy's star - forming regions. Perhaps surprisingly, side - on views of galaxies like this one do not prevent astronomers from deducing their structures. Studies of the properties of the light coming from NGC 2683 suggest that this is a barred spiral galaxy, even though the angle we see it at does not let us see this directly. NGC 2683, discovered on 5 February 1788 by the famous astronomer William Herschel, lies in the Northern constellation of Lynx. A constellation n

PIX4610165

 
Insertion of hooks on the back for hanging from a spinning wheel attached with 'Charhak tree' on the occasion of Charak Puja at Dhamrai, Dhaka, Bangladesh on April 15, 2006. Bangladesh on April 2006. Charhak Puja is observed on the last days of the Bangla month of Chaitra (April) called Chatitra Sangkranti. Farmers celebrate during this festival with the devotees singing and dancing without any care. The Charak Puja is well-known for the rites of piercing the body with nails, and swirling from a high pole. A 'charhak tree' is built on the occasion, consisting of a long pole atop which a wheel is fixed. An ascetic devotee is hung from this wheel with a hook. The wheel then spins around with him at high speed. Small nails, at times red hot ones, pierce all parts of his body including his tongue. The devotee thus spinning spreads prasad (handmade sweetmeats blessed with chants) among the curious spectators and onlookers. At the root of the celebration of Charhak Puja is a belief in spirit

UIG798112

Insertion of hooks on the back for hanging from a spinning wheel attached with 'Charhak tree' on the occasion of Charak Puja at Dhamrai, Dhaka, Bangladesh on April 15, 2006. Bangladesh on April 2006. Charhak Puja is observed on the last days of the Bangla month of Chaitra (April) called Chatitra Sangkranti. Farmers celebrate during this festival with the devotees singing and dancing without any care. The Charak Puja is well-known for the rites of piercing the body with nails, and swirling from a high pole. A 'charhak tree' is built on the occasion, consisting of a long pole atop which a wheel is fixed. An ascetic devotee is hung from this wheel with a hook. The wheel then spins around with him at high speed. Small nails, at times red hot ones, pierce all parts of his body including his tongue. The devotee thus spinning spreads prasad (handmade sweetmeats blessed with chants) among the curious spectators and onlookers. At the root of the celebration of Charhak Puja is a belief in spirit

UIG798112

 
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St Christopher carrying the Christ Child

Borgianni, Orazio (1578-1616) (after)

USB1158026

St Christopher carrying the Christ Child

Borgianni, Orazio (1578-1616) (after)

USB1158026

 
Ocean level rise - North America - North America with sea level+100m - Artist's view showing North America as it would appear if the ocean level increased by 100 metres. This would happen if all glaciers on Earth melt. This is how North America may appear with mean sea level about 100 meters (330 feet) above today's. Such a dramatic rise in sea level could occur if all of the Earth's glaciers were to melt. In this image the Gulf of Mexico and Atlantic ocean have inundated almost all of southeastern United State including the entire state of Florida, almost all of Louisiana, and significant portions of the other southeastern states and the District of Columbia. Major US cities submerged include New York City, Boston and Houston, and on the west coast Los Angeles, San Francisco, and much of San Diego. To the north the Hudson Bay has grown to claim much of the Canadian provinces of Ontario, Quebec, Manitoba and Nunavut. Further north Greenland's entire ice sheet, 110,000 years old and hol

Walter B Myers

PIX4633123

Ocean level rise - North America - North America with sea level+100m - Artist's view showing North America as it would appear if the ocean level increased by 100 metres. This would happen if all glaciers on Earth melt. This is how North America may appear with mean sea level about 100 meters (330 feet) above today's. Such a dramatic rise in sea level could occur if all of the Earth's glaciers were to melt. In this image the Gulf of Mexico and Atlantic ocean have inundated almost all of southeastern United State including the entire state of Florida, almost all of Louisiana, and significant portions of the other southeastern states and the District of Columbia. Major US cities submerged include New York City, Boston and Houston, and on the west coast Los Angeles, San Francisco, and much of San Diego. To the north the Hudson Bay has grown to claim much of the Canadian provinces of Ontario, Quebec, Manitoba and Nunavut. Further north Greenland's entire ice sheet, 110,000 years old and hol

Walter B Myers

PIX4633123

 
Mars: craters and channels in Hephaestus Fossae - Mars: craters and channels in Hephaestus Fossae - Impact crateres and channel system in Hephaestus Fossae, a region on Mars located on the western flank of Elysium Mons. The large impact crater at the top of the picture is 20 km in diameter. The image covering an area of about 150 square km was obtained by the Mars Express probe on 28 December 2007. This image of Hephaestus Fossae was obtained by Esa's Mars Express orbiter on 28 December 2007. The region is dotted with craters and channel systems and lies at about 21* North and 126* East on the Red Planet. Named after the Greek god of fire, Hephaestus Fossae extends for more than 600 km on the western flank of Elysium Mons in the Utopia Planitia region. The surface is mostly smooth, and is covered by several small impact craters measuring 800 to 2800 m in diameter. Smaller craters are scattered across the entire region. A larger impact crater measuring 20 km in diameter is a prominent f

PIX4616151

Mars: craters and channels in Hephaestus Fossae - Mars: craters and channels in Hephaestus Fossae - Impact crateres and channel system in Hephaestus Fossae, a region on Mars located on the western flank of Elysium Mons. The large impact crater at the top of the picture is 20 km in diameter. The image covering an area of about 150 square km was obtained by the Mars Express probe on 28 December 2007. This image of Hephaestus Fossae was obtained by Esa's Mars Express orbiter on 28 December 2007. The region is dotted with craters and channel systems and lies at about 21* North and 126* East on the Red Planet. Named after the Greek god of fire, Hephaestus Fossae extends for more than 600 km on the western flank of Elysium Mons in the Utopia Planitia region. The surface is mostly smooth, and is covered by several small impact craters measuring 800 to 2800 m in diameter. Smaller craters are scattered across the entire region. A larger impact crater measuring 20 km in diameter is a prominent f

PIX4616151

 
An ascetic devotee hangs from a spinning wheel attached with 'Charhak tree' on the occasion of Charak Puja at Shah Para village, Tangail, Bangladesh on April 15, 2006. Charhak Puja is observed on the last days of the Bangla month of Chaitra (April) called Chatitra Sangkranti. Farmers celebrate during this festival with the devotees singing and dancing without any care. The Charak Puja is well-known for the rites of piercing the body with nails, and swirling from a high pole. A 'charhak tree' is built on the occasion, consisting of a long pole atop which a wheel is fixed. An ascetic devotee is hung from this wheel with a hook. The wheel then spins around with him at high speed. Small nails, at times red hot ones, pierce all parts of his body including his tongue. The devotee thus spinning spreads prasad (handmade sweetmeats blessed with chants) among the curious spectators and onlookers. At the root of the celebration of Charhak Puja is a belief in spirits and the cult of rebirth. Its r

UIG798114

An ascetic devotee hangs from a spinning wheel attached with 'Charhak tree' on the occasion of Charak Puja at Shah Para village, Tangail, Bangladesh on April 15, 2006. Charhak Puja is observed on the last days of the Bangla month of Chaitra (April) called Chatitra Sangkranti. Farmers celebrate during this festival with the devotees singing and dancing without any care. The Charak Puja is well-known for the rites of piercing the body with nails, and swirling from a high pole. A 'charhak tree' is built on the occasion, consisting of a long pole atop which a wheel is fixed. An ascetic devotee is hung from this wheel with a hook. The wheel then spins around with him at high speed. Small nails, at times red hot ones, pierce all parts of his body including his tongue. The devotee thus spinning spreads prasad (handmade sweetmeats blessed with chants) among the curious spectators and onlookers. At the root of the celebration of Charhak Puja is a belief in spirits and the cult of rebirth. Its r

UIG798114

 
Barree spiral galaxy UGC 12158 - Galaxy UGC 12158 - The galaxy UGC 12158, is about 400 million light years away from Earth in the constellation Pegase. In this image obtained by the Hubble space telescope, a blue star is visible near the center of the galaxy (lower left), it is a supernova, SN 2004ef. The galaxy captured in this image, called UGC 12158, certainly isn't camera - shy: this spiral stunner is posing face - on to the NASA/ESA Hubble Space Telescope's Advanced Camera for Surveys, revealing its structure in fine detail. UGC 12158 is an excellent example of a barred spiral galaxy in the Hubble sequence - - a scheme used to categorise galaxies based on their shapes. Barred spirals, as the name suggest, feature spectacular swirling arms of stars that emanate from a bar - shaped centre. Such bar structures are common, being found in about two thirds of spiral galaxies, and are thought to act as funnels, guiding gas to their galactic centres where it accumulates to form newborn st

PIX4613612

Barree spiral galaxy UGC 12158 - Galaxy UGC 12158 - The galaxy UGC 12158, is about 400 million light years away from Earth in the constellation Pegase. In this image obtained by the Hubble space telescope, a blue star is visible near the center of the galaxy (lower left), it is a supernova, SN 2004ef. The galaxy captured in this image, called UGC 12158, certainly isn't camera - shy: this spiral stunner is posing face - on to the NASA/ESA Hubble Space Telescope's Advanced Camera for Surveys, revealing its structure in fine detail. UGC 12158 is an excellent example of a barred spiral galaxy in the Hubble sequence - - a scheme used to categorise galaxies based on their shapes. Barred spirals, as the name suggest, feature spectacular swirling arms of stars that emanate from a bar - shaped centre. Such bar structures are common, being found in about two thirds of spiral galaxies, and are thought to act as funnels, guiding gas to their galactic centres where it accumulates to form newborn st

PIX4613612

 
Jeju volcanic island, South Korea - Jeju volcanic island, South Korea - Jeju volcanic island seen by Landsat satellite - 7 on April 6, 2000. This island, classified as a World Heritage Site, is home to the highest peak of South Korea, Mount Halla (1950 m), a volcano shield whose last eruption dates back to 1007. Cheju Island, is an oval - shaped volcanic landmass covering 1,845 square kilometers (712 square miles) off the southern tip of the Korean Peninsula. Geologists estimate the island's age at 2 million years, and archaeological finds suggest that people have lived on the island since prehistoric times. Today, Cheju is both a tourist attraction and home to an UNESCO World Heritage site. The Enhanced Thematic Mapper Plus on Nasa's Landsat - 7 satellite captured this image of Cheju Island on April 6, 2000. In this photo - like image, cloudless skies allow a clear view of the island and the swirling blue hues of the surrounding waters. Urbanized areas, such as the capital city, Cheju

PIX4660095

Jeju volcanic island, South Korea - Jeju volcanic island, South Korea - Jeju volcanic island seen by Landsat satellite - 7 on April 6, 2000. This island, classified as a World Heritage Site, is home to the highest peak of South Korea, Mount Halla (1950 m), a volcano shield whose last eruption dates back to 1007. Cheju Island, is an oval - shaped volcanic landmass covering 1,845 square kilometers (712 square miles) off the southern tip of the Korean Peninsula. Geologists estimate the island's age at 2 million years, and archaeological finds suggest that people have lived on the island since prehistoric times. Today, Cheju is both a tourist attraction and home to an UNESCO World Heritage site. The Enhanced Thematic Mapper Plus on Nasa's Landsat - 7 satellite captured this image of Cheju Island on April 6, 2000. In this photo - like image, cloudless skies allow a clear view of the island and the swirling blue hues of the surrounding waters. Urbanized areas, such as the capital city, Cheju

PIX4660095

 
Galaxies NGC 1316 and 1317 in the Furnace - Galaxies NGC 1316 and NGC 1317 in Fornax - The giant elliptical galaxy NGC 1316 (below) absorbed a spiral galaxy a few billion years ago. A few bands of dust visible in the centre are the traces of this feast. A spiral galaxy, NGC 1317, is visible just above it. These galaxies resident more than 60 million years ago - light in the array of galaxies of the Furnace. Also called Fornax A, NGC 1316 is one of the strongest radio sources in the sky. Image made with Siding Spring's 3.9m telescope. NGC 1316 - 17 are on the outskirts of a nearby cluster of galaxies in the southern constellation of Fornax, at a distance of about 60 million light years. At first glance, the optical image of these galaxies does not seem to be very unusual. However, closer inspection shows that the larger galaxy, the elliptical NGC 1316, has distinct dust lanes in its inner regions, and NGC 1317 is a strangely distorted spiral. The dust lanes strongly suggest that NGC 131

PIX4609824

Galaxies NGC 1316 and 1317 in the Furnace - Galaxies NGC 1316 and NGC 1317 in Fornax - The giant elliptical galaxy NGC 1316 (below) absorbed a spiral galaxy a few billion years ago. A few bands of dust visible in the centre are the traces of this feast. A spiral galaxy, NGC 1317, is visible just above it. These galaxies resident more than 60 million years ago - light in the array of galaxies of the Furnace. Also called Fornax A, NGC 1316 is one of the strongest radio sources in the sky. Image made with Siding Spring's 3.9m telescope. NGC 1316 - 17 are on the outskirts of a nearby cluster of galaxies in the southern constellation of Fornax, at a distance of about 60 million light years. At first glance, the optical image of these galaxies does not seem to be very unusual. However, closer inspection shows that the larger galaxy, the elliptical NGC 1316, has distinct dust lanes in its inner regions, and NGC 1317 is a strangely distorted spiral. The dust lanes strongly suggest that NGC 131

PIX4609824

 
Planetary nebula CRL 2688 dans le Swan/HST - This image of the Egg Nebula, also known as CRL2688 and located roughly 3,000 light - years from us, was taken in red light with the Wide Field and Planetary Camera 2 (WFPC2) aboard Nasa's Hubble Space Telescope.The image shows a pair of mysterious “” searchlight” beams emerging from a hidden star, criss - Yeah. crossed by numerous bright arcs. This image sheds new light on the poorly understood ejection of stellar matter which accompanies the slow death of Sun - like stars. The image is shown in false color. The central star in CRL2688 was a red giant a few hundred years ago. The nebula is really a large cloud of dust and gas ejected by the star, expanding at a speed of 20 km/s (115,000 mph). A dense cocoon of dust (the dark band in the image center) enshrouds the star and hides it from our view. Starlight escapes more easily in directions where the cocoon is thinner, and is reflected towards us by dust particles in the cloud, giving it its

PIX4623752

Planetary nebula CRL 2688 dans le Swan/HST - This image of the Egg Nebula, also known as CRL2688 and located roughly 3,000 light - years from us, was taken in red light with the Wide Field and Planetary Camera 2 (WFPC2) aboard Nasa's Hubble Space Telescope.The image shows a pair of mysterious “” searchlight” beams emerging from a hidden star, criss - Yeah. crossed by numerous bright arcs. This image sheds new light on the poorly understood ejection of stellar matter which accompanies the slow death of Sun - like stars. The image is shown in false color. The central star in CRL2688 was a red giant a few hundred years ago. The nebula is really a large cloud of dust and gas ejected by the star, expanding at a speed of 20 km/s (115,000 mph). A dense cocoon of dust (the dark band in the image center) enshrouds the star and hides it from our view. Starlight escapes more easily in directions where the cocoon is thinner, and is reflected towards us by dust particles in the cloud, giving it its

PIX4623752

 
Planetary nebula NGC 6543 dans le Dragon/HST - The nebula, formally cataloged NGC 6543 was one of the first planetary nebulae to be discovered; it is one of the most complex such nebulae seen in space. A planetary nebula forms when Sun - like stars gently eject their outer gaseous layers that form bright nebulae with amazing and confounding shapes. In 1994, Hubble first revealed NGC 6543's surprisingly intricate structures, including concentric gas shells, jets of high - speed gas, and unusual shock - induced knots of gas. As if the Cat's Eye itself isn't spectacular enough, this new image taken with Hubble's Advanced Camera for Surveys (ACS) reveals the full beauty of a bull's eye pattern of eleven or even more concentric rings, or shells, around the Cat's Eye. Each 'ring' is actually the edge of a spherical bubble seen projected onto the sky - - that's why it appears bright along its outer edge. Observations suggest the star ejected its mass in a series of pulses at 1,500 - year inte

PIX4623222

Planetary nebula NGC 6543 dans le Dragon/HST - The nebula, formally cataloged NGC 6543 was one of the first planetary nebulae to be discovered; it is one of the most complex such nebulae seen in space. A planetary nebula forms when Sun - like stars gently eject their outer gaseous layers that form bright nebulae with amazing and confounding shapes. In 1994, Hubble first revealed NGC 6543's surprisingly intricate structures, including concentric gas shells, jets of high - speed gas, and unusual shock - induced knots of gas. As if the Cat's Eye itself isn't spectacular enough, this new image taken with Hubble's Advanced Camera for Surveys (ACS) reveals the full beauty of a bull's eye pattern of eleven or even more concentric rings, or shells, around the Cat's Eye. Each 'ring' is actually the edge of a spherical bubble seen projected onto the sky - - that's why it appears bright along its outer edge. Observations suggest the star ejected its mass in a series of pulses at 1,500 - year inte

PIX4623222

 
Seyfert's Sextet Group of Galaxies in the Snake - Seyfert's Sextet group of galaxies - This group of interacting galaxies resides approximately 190 million years ago - light in the constellation of the Snake and extends over 100,000 years - light. The small spiral galaxy seen from the front does not belong to this group. The small face - on spiral with the prominent arms [center] of gas and stars is a background galaxy almost five times farther away than the other four. Only a chance alignment makes it appear as if it is part of the group. The sixth member of the sextet isn't a galaxy at all but a long “” tidal tail””” of stars [below, right] torn from one of the galaxies. The group resides 190 million light - years away in the constellation Serpens. This densely packed grouping spans just 100,000 light - years, occupying less volume than the Milky Way galaxy. Each galaxy is about 35,000 light - years wide. Three of the galaxies [the elliptical galaxy, second from top, and the two spir

PIX4565516

Seyfert's Sextet Group of Galaxies in the Snake - Seyfert's Sextet group of galaxies - This group of interacting galaxies resides approximately 190 million years ago - light in the constellation of the Snake and extends over 100,000 years - light. The small spiral galaxy seen from the front does not belong to this group. The small face - on spiral with the prominent arms [center] of gas and stars is a background galaxy almost five times farther away than the other four. Only a chance alignment makes it appear as if it is part of the group. The sixth member of the sextet isn't a galaxy at all but a long “” tidal tail””” of stars [below, right] torn from one of the galaxies. The group resides 190 million light - years away in the constellation Serpens. This densely packed grouping spans just 100,000 light - years, occupying less volume than the Milky Way galaxy. Each galaxy is about 35,000 light - years wide. Three of the galaxies [the elliptical galaxy, second from top, and the two spir

PIX4565516

 
Spiral galaxy M33 infrared view - Spiral galaxy M33 seen in infrared - M33, (NGC 598), the galaxy of the Triangle, is located about 2.9 million years ago - light from Earth. It belongs to the local group, just like our galaxy or Andromede galaxy. This infrared image from the Spitzer space telescope shows stars in blue, gas in green, star formations in red - orange. Red dots are distant galaxies. In infrared, the galaxy appears larger than visible light, revealing cold gas and dust that spread around the galaxy. Also known as M33 or NGC 598, the Triangulum Galaxy is part of the Local Group of galaxies, which includes the Andromeda Galaxy (M31) and our galaxy, the Milky Way. M33 is over thirty thousand light - years across, and more than two million light - years away. Viewed here with Spitzer's infrared eyes, this elegant spiral galaxy sparkles with color and detail. Stars appear as glistening blue gems (several of which are actually foreground stars in our own galaxy), while dust rich

PIX4609334

Spiral galaxy M33 infrared view - Spiral galaxy M33 seen in infrared - M33, (NGC 598), the galaxy of the Triangle, is located about 2.9 million years ago - light from Earth. It belongs to the local group, just like our galaxy or Andromede galaxy. This infrared image from the Spitzer space telescope shows stars in blue, gas in green, star formations in red - orange. Red dots are distant galaxies. In infrared, the galaxy appears larger than visible light, revealing cold gas and dust that spread around the galaxy. Also known as M33 or NGC 598, the Triangulum Galaxy is part of the Local Group of galaxies, which includes the Andromeda Galaxy (M31) and our galaxy, the Milky Way. M33 is over thirty thousand light - years across, and more than two million light - years away. Viewed here with Spitzer's infrared eyes, this elegant spiral galaxy sparkles with color and detail. Stars appear as glistening blue gems (several of which are actually foreground stars in our own galaxy), while dust rich

PIX4609334

 
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Holland House, Kensington (watercolour)

Varley, John (1778-1842)

CBE8833657

Holland House, Kensington (watercolour)

Varley, John (1778-1842)

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Admiral Sir William Parker (1743-1802), c.1777 (watercolour, gilt)

Scouler, James (c.1740-1812)

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Admiral Sir William Parker (1743-1802), c.1777 (watercolour, gilt)

Scouler, James (c.1740-1812)

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Colonel William Windham I, MP (1647-1689)

Kneller, Godfrey (1646-1723)

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Colonel William Windham I, MP (1647-1689)

Kneller, Godfrey (1646-1723)

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Bust of a 'Barbary pirate', c.1700 (terracotta)

Unknown artist, (18th century)

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Bust of a 'Barbary pirate', c.1700 (terracotta)

Unknown artist, (18th century)

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Seru Thakombau [Seru Epenisa Cakobau], 1815 - 83; King of Fiji, 1852-74, 1849 (watercolour, graphite)

Fanshawe, Admiral Sir Edward Gennys (1814-1906)

MMM7295608

Seru Thakombau [Seru Epenisa Cakobau], 1815 - 83; King of Fiji, 1852-74, 1849 (watercolour, graphite)

Fanshawe, Admiral Sir Edward Gennys (1814-1906)

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Called 'Bungay', the Favourite Dog of Sir John Harington (1561-1612)

English School

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Called 'Bungay', the Favourite Dog of Sir John Harington (1561-1612)

English School

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Federal President Schaerf on his way to the swearing-in into parliament

Fritz Kern

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Federal President Schaerf on his way to the swearing-in into parliament

Fritz Kern

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