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Images of 'Broad Bottom' found, 65

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Necklace belonging to Princess Neferuptah, from the Pyramid of Princess Neferuptah at Hawara, Middle Kingdom (gold, carnelian, feldspar & glass paste)

Necklace belonging to Princess Neferuptah, from the Pyramid of Princess Neferuptah at Hawara, Middle Kingdom (gold, carnelian, feldspar & glass paste)

Egyptian 12th Dynasty (1991-1786 BC)

Sandro Vannini

SVA660124

Broad Bottom Drones storming the Hive, Wasps, Hornets & Bumble-Bees joining in the Attack, published by Hannah Humphrey in 1808 (hand-coloured etching)

Broad Bottom Drones storming the Hive, Wasps, Hornets & Bumble-Bees joining in the Attack, published by Hannah Humphrey in 1808 (hand-coloured etching)

Gillray, James (1757-1815)

NCO192595

'A Pair of Broad Bottoms' (coloured engraving)

'A Pair of Broad Bottoms' (coloured engraving)

English School, (18th century)

STC229787

'Where William Blake was born (engraving)

'Where William Blake was born (engraving)

XLA3776991

Part of a Poleyn for the Left Knee, probably Milanese, c.1450 (steel)

Part of a Poleyn for the Left Knee, probably Milanese, c.1450 (steel)

Italian School, (15th century)

CH7212574

A Kick at the Broad-Bottoms' George III kicking Lord Grenville's bottom and dismissing Grenville's ministry. King opposed Roman Catholic Army and Navy Service Bill. James Gilray cartoon 1807. Religion Anti-Catholic

A Kick at the Broad-Bottoms' George III kicking Lord Grenville's bottom and dismissing Grenville's ministry. King opposed Roman Catholic Army and Navy Service Bill. James Gilray cartoon 1807. Religion Anti-Catholic

UIG528553

Broad Bottoms, 1745 (etching)

Broad Bottoms, 1745 (etching)

English School, (18th century)

XJF863021

Sketch for a Monument of Disappointed Justice, published by Hannah Humphrey in 1806 (hand-coloured etching)

Sketch for a Monument of Disappointed Justice, published by Hannah Humphrey in 1806 (hand-coloured etching)

Gillray, James (1757-1815)

NCO192599

The Funeral Procession of Broad-Bottom, published by Hannah Humphrey in 1807 (hand-coloured etching)

The Funeral Procession of Broad-Bottom, published by Hannah Humphrey in 1807 (hand-coloured etching)

Gillray, James (1757-1815)

NCO191215

A Tub for the Whale! published by Hannah Humphrey in 1806 (hand-coloured etching)

A Tub for the Whale! published by Hannah Humphrey in 1806 (hand-coloured etching)

Gillray, James (1757-1815)

NCO193185

L'Enfant Trouve: a Sample of Roman Charity, or the misfortune of not being born with Marks of 'the Talents', published by Hannah Humphrey in 1808 (hand-coloured etching)

L'Enfant Trouve: a Sample of Roman Charity, or the misfortune of not being born with Marks of 'the Talents', published by Hannah Humphrey in 1808 (hand-coloured etching)

Gillray, James (1757-1815)

NCO193192

The Pigs Possessed, or The Broad bottom'd Litter running headlong into ye Sea of Perdition, 1807 (coloured engraving)

The Pigs Possessed, or The Broad bottom'd Litter running headlong into ye Sea of Perdition, 1807 (coloured engraving)

Gillray, James (1757-1815)

HRP2624943

Patriotic Petitions on the Convention, published by Hannah Humphrey (hand-coloured etching)

Patriotic Petitions on the Convention, published by Hannah Humphrey (hand-coloured etching)

Gillray, James (1757-1815)

NCO193107

The Pigs Possessed: or the Broad bottom'd Litter running headlong into the Sea of Perdition, pub. 1807 (hand coloured engraving)

The Pigs Possessed: or the Broad bottom'd Litter running headlong into the Sea of Perdition, pub. 1807 (hand coloured engraving)

Gillray, James (1757-1815)

STC3035657

Posting to the Election: a scene on the road to Brentford, published by Hannah Humphrey in 1806 (hand-coloured etching)

Posting to the Election: a scene on the road to Brentford, published by Hannah Humphrey in 1806 (hand-coloured etching)

Gillray, James (1757-1815)

NCO193119

The Triumph of Quassia, published by Hannah Humphrey in 1806 (hand-coloured etching)

The Triumph of Quassia, published by Hannah Humphrey in 1806 (hand-coloured etching)

Gillray, James (1757-1815)

NCO193108

French costumes of the late 15th century, 1889 (chromolithograph)

French costumes of the late 15th century, 1889 (chromolithograph)

FLO5912648

Disciples catching the Mantle: the Spirit of Darkness overshadowing the Priests of Baal, published by Hannah Humphrey in 1808 (hand-coloured etching)

Disciples catching the Mantle: the Spirit of Darkness overshadowing the Priests of Baal, published by Hannah Humphrey in 1808 (hand-coloured etching)

Gillray, James (1757-1815)

NCO193135

The stock exchange on Broad Street, 1885 (sepia photo)

The stock exchange on Broad Street, 1885 (sepia photo)

American Photographer, (19th century)

GLC696189

Bottom of a moulded bowl with a broad rim (glass)

Bottom of a moulded bowl with a broad rim (glass)

Erich Lessing

ELS9145343

The Introduction of the Pope to the Convocation at Oxford by the cardinal Broad-Bottom, published by Hannah Humphrey in 1809 (hand-coloured etching)

The Introduction of the Pope to the Convocation at Oxford by the cardinal Broad-Bottom, published by Hannah Humphrey in 1809 (hand-coloured etching)

Gillray, James (1757-1815)

NCO191749

Broad Street, Oxford (w/c on paper)

Broad Street, Oxford (w/c on paper)

Gotch, Bernard Cecil (1876-1964)

NCO931215

British Tars towing the Danish Fleet into Harbour: the Borad bottom Leviathan trying to swamp Billy's old Boat, & the little Corsican tottering on the Clouds of Ambition, pub. 1807 (hand coloured engraving)

British Tars towing the Danish Fleet into Harbour: the Borad bottom Leviathan trying to swamp Billy's old Boat, & the little Corsican tottering on the Clouds of Ambition, pub. 1807 (hand coloured engraving)

Gillray, James (1757-1815)

STC3025367

Broad Street, Lyme Regis, Dorset, 22/05/1925 (b/w photo)

Broad Street, Lyme Regis, Dorset, 22/05/1925 (b/w photo)

Macfee, Katherine Jean (1881-1952)

EHT7306574

‘The New Broad Sword Exercise’ cotton handkerchief, 1798 (cotton)

‘The New Broad Sword Exercise’ cotton handkerchief, 1798 (cotton)

English School, (18th century)

NAM3062538

Broad Bottom Drones storming the Hive: Wasps, Hornets, & Bumble Bees joinig the attack, pub. 1808 (hand coloured engraving)

Broad Bottom Drones storming the Hive: Wasps, Hornets, & Bumble Bees joinig the attack, pub. 1808 (hand coloured engraving)

Gillray, James (1757-1815)

STC3025927

Tankard, c.1590 (salt-glazed stoneware and pewter)

Tankard, c.1590 (salt-glazed stoneware and pewter)

German School, (16th century)

TWC8701900

A Stretch of the Seine (oil on canvas)

A Stretch of the Seine (oil on canvas)

Daubigny, Charles Francois (1817-78) (attr. to)

USB1155426

GERMAN CHANCELLOR SCHROEDER AND DEFENSE MINISTER SCHARPING ATTEND
PARLIMENTARY DEBATE IN BERLIN, 2001-08-29 (photo) — GERMAN CHANCELLOR SCHROEDER AND DEFENSE MINISTER SCHARPING ATTEND PARLIMENTARY DEBATE IN BERLIN, 2001-08-29 (photo)

GERMAN CHANCELLOR SCHROEDER AND DEFENSE MINISTER SCHARPING ATTEND PARLIMENTARY DEBATE IN BERLIN, 2001-08-29 (photo)

Alexandra Beier

REU7979002

GERMAN CHANCELLOR SCHROEDER AND DEFENSE MINISTER SCHARPING ATTEND
PARLIMENTARY DEBATE IN BERLIN, 2001-08-29 (photo) — GERMAN CHANCELLOR SCHROEDER AND DEFENSE MINISTER SCHARPING ATTEND PARLIMENTARY DEBATE IN BERLIN, 2001-08-29 (photo)

GERMAN CHANCELLOR SCHROEDER AND DEFENSE MINISTER SCHARPING ATTEND PARLIMENTARY DEBATE IN BERLIN, 2001-08-29 (photo)

Alexandra Beier

REU8021613

A Polished Brass 80-A Victor Cornet And A 20-A Flugelhorn

A Polished Brass 80-A Victor Cornet And A 20-A Flugelhorn

SIC830493

Jun. 06, 1953 - M. Andre Marie the new premier designate four expressions of M. Andre aerie, the fourth” premier designate” shaped as he was leaving the Elysee palace this morning. (Left to right and top to bottom) 1st” i must think it over before saying yes. 2nd. yes it takes deep thinking. 3rd: I think i will have a try (smiling). and i will Do my best (broad smile)

Jun. 06, 1953 - M. Andre Marie the new premier designate four expressions of M. Andre aerie, the fourth” premier designate” shaped as he was leaving the Elysee palace this morning. (Left to right and top to bottom) 1st” i must think it over before saying yes. 2nd. yes it takes deep thinking. 3rd: I think i will have a try (smiling). and i will Do my best (broad smile)

ZUM4851304

Candle snuffer and stand, 1710-15 (brass)

Candle snuffer and stand, 1710-15 (brass)

English School, (18th century)

JEF3084423

GERMAN CHANCELLOR SCHROEDER AND PARLIAMENTARY FLOOR LEADER STRUCK IN
BERLIN, 2001-08-28 (photo) — GERMAN CHANCELLOR SCHROEDER AND PARLIAMENTARY FLOOR LEADER STRUCK IN BERLIN, 2001-08-28 (photo)

GERMAN CHANCELLOR SCHROEDER AND PARLIAMENTARY FLOOR LEADER STRUCK IN BERLIN, 2001-08-28 (photo)

Fabrizio Bensch

REU8017412

New London Bridge from Billingsgate (Low Water), 1833 (etching on paper)

New London Bridge from Billingsgate (Low Water), 1833 (etching on paper)

Cooke, Edward William (1811-80)

IGM7485341

The Dutch Fleet

The Dutch Fleet

Witmont, Heerman (c.1605-c.83)

USB1160303

CHRISTIAN DEMOCRATIC UNION PARTY MILITARY EXPERT RUEHE DELIVERS HIS
SPEECH DURING PARLIMENTARY ..., 2001-08-29 (photo) — CHRISTIAN DEMOCRATIC UNION PARTY MILITARY EXPERT RUEHE DELIVERS HIS SPEECH DURING PARLIMENTARY ..., 2001-08-29 (photo)

CHRISTIAN DEMOCRATIC UNION PARTY MILITARY EXPERT RUEHE DELIVERS HIS SPEECH DURING PARLIMENTARY ..., 2001-08-29 (photo)

Fabrizio Bensch

REU8152899

The cluster of galaxies in Fornax - The cluster of galaxies in Fornax - The cluster of galaxies in the Furnace is located about 55 million years away from Earth. This image shows only a detail of the cluster. Lower right, the barred spiral galaxy NGC 1365

The cluster of galaxies in Fornax - The cluster of galaxies in Fornax - The cluster of galaxies in the Furnace is located about 55 million years away from Earth. This image shows only a detail of the cluster. Lower right, the barred spiral galaxy NGC 1365

PIX4565382

The Milky Way, looking towards the Galactic Centre - The Milky Way, looking towards the Galactic Centre - The bright point at the bottom left is Jupiter Planet The Milky Way is best seen on winter nights (May to August) from the southern hemisphere. This wide-angle picture shows a broad span of the southern Milky Way and is a photograph made using colour film in a conventional camera. The camera which was pointed towards the centre of our Galaxy, in the direction of the constellation of Sagittarius. The Galactic centre itself is totally hidden at visible wavelengths by the band of dust which divides the Milky Way along much of its length. The dust lane is only visible because it blots out background stars. Embedded in the dust are many star-forming regions, seen as bright red emission nebulae. The brightest, left of the centre of the picture, is Messier 8, the Lagoon Nebula, which is visible to the unaided eye. The bright 'star' at lower left is the planet Jupiter

The Milky Way, looking towards the Galactic Centre - The Milky Way, looking towards the Galactic Centre - The bright point at the bottom left is Jupiter Planet The Milky Way is best seen on winter nights (May to August) from the southern hemisphere. This wide-angle picture shows a broad span of the southern Milky Way and is a photograph made using colour film in a conventional camera. The camera which was pointed towards the centre of our Galaxy, in the direction of the constellation of Sagittarius. The Galactic centre itself is totally hidden at visible wavelengths by the band of dust which divides the Milky Way along much of its length. The dust lane is only visible because it blots out background stars. Embedded in the dust are many star-forming regions, seen as bright red emission nebulae. The brightest, left of the centre of the picture, is Messier 8, the Lagoon Nebula, which is visible to the unaided eye. The bright 'star' at lower left is the planet Jupiter

PIX4637870

Phaeton alarm'd, 1808 (etching)

Phaeton alarm'd, 1808 (etching)

Gillray, James (1757-1815)

MMM7340077

The Presentation of the Virgin

The Presentation of the Virgin

Giovanni di Paolo di Grazia (1403-82)

USB1159432

March: Promethei Planum - Mars: Promethei Planum - Promethei Planum is a region located near the southern pole of Mars. This region is seasonally covered with a thick layer of ice up to 3500 metres thick. On this perspective image obtained by the Mars Express probe on September 22, 2005, an impact crater about 100 km wide and 800 metres deep is visible at the bottom of the image. It is partially covered with ice. On top, structures formed by lava flows; at the top of the picture, ice, which is an extension of the southern polar cap. Promethei Planum, an area seasonally covered with layer of ice more than 3500 m thick layer of ice in the martian south polar region, was the subject of the High Resolution Stereo Camera's focus on 22 September 2005 as Mars Express was in orbit above the Red Planet. Promethei Planum lies at approximately 76* south and 105* east. An approximately 100 km - large and 800 m - deep impact crater is visible in the bottom of the image. The crater's interior is partly covered in ice. Above, are structures that may have been created by basaltic lava flow from a volcano. This area is covered in ice. The dark dunes towards the left side of the image are most likely made up of dust originating from this lava flow or volcanic ash. A broad sheet of ice, which is an extension of the south polar ice cap is visible in the higher part of the image. The steep flanks clearly show white, clean ice. The thickness of the ice is between 900 and 1100 m — March: Promethei Planum - Mars: Promethei Planum - Promethei Planum is a region located near the southern pole of Mars. This region is seasonally covered with a thick layer of ice up to 3500 metres thick. On this perspective image obtained by the Mars Express probe on September 22, 2005, an impact crater about 100 km wide and 800 metres deep is visible at the bottom of the image. It is partially covered with ice. On top, structures formed by lava flows; at the top of the picture, ice, which is an extension of the southern polar cap. Promethei Planum, an area seasonally covered with layer of ice more than 3500 m thick layer of ice in the martian south polar region, was the subject of the High Resolution Stereo Camera's focus on 22 September 2005 as Mars Express was in orbit above the Red Planet. Promethei Planum lies at approximately 76* south and 105* east. An approximately 100 km - large and 800 m - deep impact crater is visible in the bottom of the image. The crater's interior is par

March: Promethei Planum - Mars: Promethei Planum - Promethei Planum is a region located near the southern pole of Mars. This region is seasonally covered with a thick layer of ice up to 3500 metres thick. On this perspective image obtained by the Mars Express probe on September 22, 2005, an impact crater about 100 km wide and 800 metres deep is visible at the bottom of the image. It is partially covered with ice. On top, structures formed by lava flows; at the top of the picture, ice, which is an extension of the southern polar cap. Promethei Planum, an area seasonally covered with layer of ice more than 3500 m thick layer of ice in the martian south polar region, was the subject of the High Resolution Stereo Camera's focus on 22 September 2005 as Mars Express was in orbit above the Red Planet. Promethei Planum lies at approximately 76* south and 105* east. An approximately 100 km - large and 800 m - deep impact crater is visible in the bottom of the image. The crater's interior is par

PIX4616138

Mars: dunes and ice in Chasma Boreale - Mars: dunes and ice in Chasma Boreale - Chasma Boreale is a huge canyon located in the northern polar cap of Mars. This image, obtained in light visible by the probe 2001 Mars Odyssey, shows Tenuis Cavus, the end of this valley or the canyon is only 35 km wide. The cliffs s'elevent 1400 meters above ground. The walls are covered with ice, while at the bottom of the bowl many sand dunes are present. 3D recomposed view, vertical exaggeration: 2.5 times. Chasma Boreale is a huge canyon in the northern polar cap. It runs into the ice cap for 570 kilometers (350 miles), making a broad valley that ends at a point called Tenuis Cavus, shown in this THEMIS image taken at visible wavelengths.tapering from a width of 120 km (75 miles) at its mouth, Chasma Boreale is only about 35 km (22 miles) wide here. The cliffs rise about 1,400 meters (4,600 feet) above the base. On the inside walls of this gigantic amphitheater are stacked layers of ice, while on its floor lie a dark sheet of what is likely frozen sand and a horde of sand dunes marching down - canyon under the winds' direction. 3D image, vertical exaggeration: X2. — Mars: dunes and ice in Chasma Boreale - Mars: dunes and ice in Chasma Boreale - Chasma Boreale is a huge canyon located in the northern polar cap of Mars. This image, obtained in light visible by the probe 2001 Mars Odyssey, shows Tenuis Cavus, the end of this valley or the canyon is only 35 km wide. The cliffs s'elevent 1400 meters above ground. The walls are covered with ice, while at the bottom of the bowl many sand dunes are present. 3D recomposed view, vertical exaggeration: 2.5 times. Chasma Boreale is a huge canyon in the northern polar cap. It runs into the ice cap for 570 kilometers (350 miles), making a broad valley that ends at a point called Tenuis Cavus, shown in this THEMIS image taken at visible wavelengths.tapering from a width of 120 km (75 miles) at its mouth, Chasma Boreale is only about 35 km (22 miles) wide here. The cliffs rise about 1,400 meters (4,600 feet) above the base. On the inside walls of this gigantic amphitheater are stacked layers of ice, while on its

Mars: dunes and ice in Chasma Boreale - Mars: dunes and ice in Chasma Boreale - Chasma Boreale is a huge canyon located in the northern polar cap of Mars. This image, obtained in light visible by the probe 2001 Mars Odyssey, shows Tenuis Cavus, the end of this valley or the canyon is only 35 km wide. The cliffs s'elevent 1400 meters above ground. The walls are covered with ice, while at the bottom of the bowl many sand dunes are present. 3D recomposed view, vertical exaggeration: 2.5 times. Chasma Boreale is a huge canyon in the northern polar cap. It runs into the ice cap for 570 kilometers (350 miles), making a broad valley that ends at a point called Tenuis Cavus, shown in this THEMIS image taken at visible wavelengths.tapering from a width of 120 km (75 miles) at its mouth, Chasma Boreale is only about 35 km (22 miles) wide here. The cliffs rise about 1,400 meters (4,600 feet) above the base. On the inside walls of this gigantic amphitheater are stacked layers of ice, while on its

PIX4616341

Mars: dunes and ice in Chasma Boreale - Mars: dunes and ice in Chasma Boreale - Chasma Boreale is a huge canyon located in the northern polar cap of Mars. This image, obtained in light visible by the probe 2001 Mars Odyssey, shows Tenuis Cavus, the end of this valley or the canyon is only 35 km wide. The cliffs to the north (top) and to the east (right) s'elevent 1400 meters above ground. The walls are covered with ice, while at the bottom of the bowl many sand dunes are present. Chasma Boreale is a huge canyon in the northern polar cap. It runs into the ice cap for 570 kilometers (350 miles), making a broad valley that ends at a point called Tenuis Cavus, shown in this THEMIS image taken at visible wavelengths.tapering from a width of 120 km (75 miles) at its mouth, Chasma Boreale is only about 35 km (22 miles) wide here. The cliffs on the northern (top) and eastern (right) sides of the image rise about 1,400 meters (4,600 feet) above the base. On the inside walls of this gigantic amphitheater are stacked layers of ice, while on its floor lie a dark sheet of what is likely frozen sand and a horde of sand dunes marching down - canyon under the winds' direction — Mars: dunes and ice in Chasma Boreale - Mars: dunes and ice in Chasma Boreale - Chasma Boreale is a huge canyon located in the northern polar cap of Mars. This image, obtained in light visible by the probe 2001 Mars Odyssey, shows Tenuis Cavus, the end of this valley or the canyon is only 35 km wide. The cliffs to the north (top) and to the east (right) s'elevent 1400 meters above ground. The walls are covered with ice, while at the bottom of the bowl many sand dunes are present. Chasma Boreale is a huge canyon in the northern polar cap. It runs into the ice cap for 570 kilometers (350 miles), making a broad valley that ends at a point called Tenuis Cavus, shown in this THEMIS image taken at visible wavelengths.tapering from a width of 120 km (75 miles) at its mouth, Chasma Boreale is only about 35 km (22 miles) wide here. The cliffs on the northern (top) and eastern (right) sides of the image rise about 1,400 meters (4,600 feet) above the base. On the inside walls of this gigantic amp

Mars: dunes and ice in Chasma Boreale - Mars: dunes and ice in Chasma Boreale - Chasma Boreale is a huge canyon located in the northern polar cap of Mars. This image, obtained in light visible by the probe 2001 Mars Odyssey, shows Tenuis Cavus, the end of this valley or the canyon is only 35 km wide. The cliffs to the north (top) and to the east (right) s'elevent 1400 meters above ground. The walls are covered with ice, while at the bottom of the bowl many sand dunes are present. Chasma Boreale is a huge canyon in the northern polar cap. It runs into the ice cap for 570 kilometers (350 miles), making a broad valley that ends at a point called Tenuis Cavus, shown in this THEMIS image taken at visible wavelengths.tapering from a width of 120 km (75 miles) at its mouth, Chasma Boreale is only about 35 km (22 miles) wide here. The cliffs on the northern (top) and eastern (right) sides of the image rise about 1,400 meters (4,600 feet) above the base. On the inside walls of this gigantic amp

PIX4616330

The cluster of galaxies in Fornax - The cluster of galaxies in Fornax - clusters of galaxies situated about 55 million years ago - light. In the center of the image is the barree spiral galaxy NGC 1365; at the bottom right of the image, the interaction galaxy NGC 1316 - 17 (Fornax A), which is one of the strongest known radiosource. Galaxies can be separated by their appearance into two broad groups, spirals and ellipticals. An example of a spiral galaxy, NGC 1365, is seen in center of this picture. In contrast, most of the galaxies in this cluster are ellipticals, which contain little or no gas or evidence of star formation; indeed they are composed millions of rather old, yellowish stars. Unlike many of the stars in spiral systems, those in ellipticals have orbits which are not confined to a narrow plane, so the galaxy can have a shape anywhere between a perfect sphere and an American football. This kind of galaxy is the most common type in the photograph as it is in all of the nearby Universe. The picture also illustrates another distinctive property of ellipticals, their gregarious nature - they congregate in clusters, like this group of galaxies in Fornax, 55 million light years distant. This image also shows us another, less common kind of galaxy. In the lower right corner is NGC 1316 - 17. This is interacting pair of galaxies is one of the strongest nearby radio galaxies, known as Fornax A. Finally, in the opposite corner is a bright yellow (K5) 4.5 magnitude star in the adjoining constellation of Eridanus — The cluster of galaxies in Fornax - The cluster of galaxies in Fornax - clusters of galaxies situated about 55 million years ago - light. In the center of the image is the barree spiral galaxy NGC 1365; at the bottom right of the image, the interaction galaxy NGC 1316 - 17 (Fornax A), which is one of the strongest known radiosource. Galaxies can be separated by their appearance into two broad groups, spirals and ellipticals. An example of a spiral galaxy, NGC 1365, is seen in center of this picture. In contrast, most of the galaxies in this cluster are ellipticals, which contain little or no gas or evidence of star formation; indeed they are composed millions of rather old, yellowish stars. Unlike many of the stars in spiral systems, those in ellipticals have orbits which are not confined to a narrow plane, so the galaxy can have a shape anywhere between a perfect sphere and an American football. This kind of galaxy is the most common type in the photograph as it is in all of the nearb

The cluster of galaxies in Fornax - The cluster of galaxies in Fornax - clusters of galaxies situated about 55 million years ago - light. In the center of the image is the barree spiral galaxy NGC 1365; at the bottom right of the image, the interaction galaxy NGC 1316 - 17 (Fornax A), which is one of the strongest known radiosource. Galaxies can be separated by their appearance into two broad groups, spirals and ellipticals. An example of a spiral galaxy, NGC 1365, is seen in center of this picture. In contrast, most of the galaxies in this cluster are ellipticals, which contain little or no gas or evidence of star formation; indeed they are composed millions of rather old, yellowish stars. Unlike many of the stars in spiral systems, those in ellipticals have orbits which are not confined to a narrow plane, so the galaxy can have a shape anywhere between a perfect sphere and an American football. This kind of galaxy is the most common type in the photograph as it is in all of the nearb

PIX4565370

Earth view from space: California and Mexico - Northwest Mexico and Southern California seen from space - View extending from southern California with dirty Lake Salton Sea at the bottom of the image, at the southern tip of Baja California in Mexico. Image obtained from Shuttle Columbia in June 1991. Rugged mountains along the spine of Baja California, the deep blue water of the Gulf of California (also known as the Sea of Cortez), and the deserts of northwestern Mexico and southern California highlight this photograph. This southerly view provides an excellent panorama extending from the Salton Sea in the Imperial Valley of southern California almost to the southern tip of Baja California. Human imprint on this landscape is primarily found along the rivers and their floodplains, where intensive irrigated agriculture exists. The Colorado River, with its cultivated field patterns (darker areas), can be seen to flow from the north toward the southwest and finally to empty into the broad delta at the center of the photograph and to enter the northern end of the Gulf of California. The international border between the United States and Mexico can be identified by the differences in land management, farming practices, and sizes of fields. The border is the east - west straight line approximately 35 miles (56 kilometers) south of the Salton Sea. The Altar Desert is the arid - looking area with no visible vegetation east of the mouth of the Colorado River. June 5, 1991 — Earth view from space: California and Mexico - Northwest Mexico and Southern California seen from space - View extending from southern California with dirty Lake Salton Sea at the bottom of the image, at the southern tip of Baja California in Mexico. Image obtained from Shuttle Columbia in June 1991. Rugged mountains along the spine of Baja California, the deep blue water of the Gulf of California (also known as the Sea of Cortez), and the deserts of northwestern Mexico and southern California highlight this photograph. This southerly view provides an excellent panorama extending from the Salton Sea in the Imperial Valley of southern California almost to the southern tip of Baja California. Human imprint on this landscape is primarily found along the rivers and their floodplains, where intensive irrigated agriculture exists. The Colorado River, with its cultivated field patterns (darker areas), can be seen to flow from the north toward the southwest and finally to empty into the broad

Earth view from space: California and Mexico - Northwest Mexico and Southern California seen from space - View extending from southern California with dirty Lake Salton Sea at the bottom of the image, at the southern tip of Baja California in Mexico. Image obtained from Shuttle Columbia in June 1991. Rugged mountains along the spine of Baja California, the deep blue water of the Gulf of California (also known as the Sea of Cortez), and the deserts of northwestern Mexico and southern California highlight this photograph. This southerly view provides an excellent panorama extending from the Salton Sea in the Imperial Valley of southern California almost to the southern tip of Baja California. Human imprint on this landscape is primarily found along the rivers and their floodplains, where intensive irrigated agriculture exists. The Colorado River, with its cultivated field patterns (darker areas), can be seen to flow from the north toward the southwest and finally to empty into the broad

PIX4673252

Mars: dunes and ice in Chasma Boreal, a huge canyon located in the northern polar cap of Mars, image obtained in light visible by the probe Mars Odyssey, 2001

Mars: dunes and ice in Chasma Boreal, a huge canyon located in the northern polar cap of Mars, image obtained in light visible by the probe Mars Odyssey, 2001

PIX4616353

Figure 194: Black beaver hat, trimmed a la militaire, Military habit of superfine scarlet cloth, turned up with blue; gilt buttons and gold epaulettes. Large gold ear-rings. Crinson sash. Purple shoes. Buff gloves.
Figure 195: Patent demi-poke straw bonnet, trimmed round the crown with a narrow blue riband. Frock of muslin, embroidered in shell pattern, and trimmed round the neck with lace. Bow of pink riband on the left side. Yellow shoes and gloves.
Figure 196: Turban bonnet of fine muslin. Round dress of striped British muslin, scalloped at the bottom, and frock sleeves. Long gold rear-rings. Black figured gauze cloak, trimmed with broad lace. Clear book muslin veil, the border richly embroidered. — Figure 194: Black beaver hat, trimmed a la militaire, Military habit of superfine scarlet cloth, turned up with blue; gilt buttons and gold epaulettes. Large gold ear-rings. Crinson sash. Purple shoes. Buff gloves. Figure 195: Patent demi-poke straw bonnet, trimmed round the crown with a narrow blue riband. Frock of muslin, embroidered in shell pattern, and trimmed round the neck with lace. Bow of pink riband on the left side. Yellow shoes and gloves. Figure 196: Turban bonnet of fine muslin. Round dress of striped British muslin, scalloped at the bottom, and frock sleeves. Long gold rear-rings. Black figured gauze cloak, trimmed with broad lace. Clear book muslin veil, the border richly embroidered.

Figure 194: Black beaver hat, trimmed a la militaire, Military habit of superfine scarlet cloth, turned up with blue; gilt buttons and gold epaulettes. Large gold ear-rings. Crinson sash. Purple shoes. Buff gloves. Figure 195: Patent demi-poke straw bonnet, trimmed round the crown with a narrow blue riband. Frock of muslin, embroidered in shell pattern, and trimmed round the neck with lace. Bow of pink riband on the left side. Yellow shoes and gloves. Figure 196: Turban bonnet of fine muslin. Round dress of striped British muslin, scalloped at the bottom, and frock sleeves. Long gold rear-rings. Black figured gauze cloak, trimmed with broad lace. Clear book muslin veil, the border richly embroidered.

BL3294785

Caspian sea area seen from space - Caspian sea area seen from space - Satellite photo of the Caspian Sea obtained by Aqua satellite on 30 September 2004. The borders are drawn. In the upper left portion of the image, the southwestern - most portion of Russia spreads across the broad plains north of the Caucasus Mountains. Georgia runs along the southern face of the Caucasus Mountains and part of the southeastern shore of the Black Sea. In the small valley and plains south of Russia and on the central shore of the Caspian Sea, Azerbaijan sprawls until butting up against the mountains of Armenia and northern Iran. Another small piece of Azerbaijan is tucked away on the far side of Armenia. Stretching far from the southern shores of the Black Sea into the mountains and deserts of the Middle East is eastern Turkey, while in the bottom right corner, Syria and Iraq mark the northern edges of the Syrian Desert. The Reshteh - ye Kuhha - ye Alborz Mountains curve in a bright green arc around the southern end of the Caspian Sea in northwestern Iran, while on the far side of the Caspian Sea, Kazakhstan (upper right) and Turkmenistan (lower right) sprawl across the Urstyurt Plateau. Three major lakes stand out like jewels against the mountains in the lower left portion of the image - Lake Van in eastern Turkey, Lake Sevana in Armenia, and the turquoise - hued Lake Urmia in northwestern Iran. Like the Caspian Sea, the bright colors are likely due to sediment in the waters. Image taken by satellite Aqua on September 30, 2004. NB: borders are marked — Caspian sea area seen from space - Caspian sea area seen from space - Satellite photo of the Caspian Sea obtained by Aqua satellite on 30 September 2004. The borders are drawn. In the upper left portion of the image, the southwestern - most portion of Russia spreads across the broad plains north of the Caucasus Mountains. Georgia runs along the southern face of the Caucasus Mountains and part of the southeastern shore of the Black Sea. In the small valley and plains south of Russia and on the central shore of the Caspian Sea, Azerbaijan sprawls until butting up against the mountains of Armenia and northern Iran. Another small piece of Azerbaijan is tucked away on the far side of Armenia. Stretching far from the southern shores of the Black Sea into the mountains and deserts of the Middle East is eastern Turkey, while in the bottom right corner, Syria and Iraq mark the northern edges of the Syrian Desert. The Reshteh - ye Kuhha - ye Alborz Mountains curve in a bright green arc around th

Caspian sea area seen from space - Caspian sea area seen from space - Satellite photo of the Caspian Sea obtained by Aqua satellite on 30 September 2004. The borders are drawn. In the upper left portion of the image, the southwestern - most portion of Russia spreads across the broad plains north of the Caucasus Mountains. Georgia runs along the southern face of the Caucasus Mountains and part of the southeastern shore of the Black Sea. In the small valley and plains south of Russia and on the central shore of the Caspian Sea, Azerbaijan sprawls until butting up against the mountains of Armenia and northern Iran. Another small piece of Azerbaijan is tucked away on the far side of Armenia. Stretching far from the southern shores of the Black Sea into the mountains and deserts of the Middle East is eastern Turkey, while in the bottom right corner, Syria and Iraq mark the northern edges of the Syrian Desert. The Reshteh - ye Kuhha - ye Alborz Mountains curve in a bright green arc around th

PIX4660580

March: Promethei Planum - Mars: Promethei Planum - Promethei Planum is a region located near the southern pole of Mars. This region is seasonally covered with a thick layer of ice up to 3500 metres thick. On this image obtained by the Mars Express probe on September 22, 2005, an impact crater about 100 km wide and 800 metres deep is visible to the right (north). It is partially covered with ice. In the center of the image, structures formed by lava flows; on the left of the image, ice, which is an extension of the southern polar cap. Promethei Planum, an area seasonally covered with layer of ice more than 3500 m thick layer of ice in the martian south polar region, was the subject of the High Resolution Stereo Camera's focus on 22 September 2005 as Mars Express was in orbit above the Red Planet. Promethei Planum lies at approximately 76* south and 105* east. An approximately 100 km - large and 800 m - deep impact crater is visible in the northern part of the image. The crater's interior is partly covered in ice. In the centre of the image are structures that may have been created by basaltic lava flow from a volcano. This area is covered in ice. The dark dunes towards the bottom of the image are most likely made up of dust originating from this lava flow or volcanic ash. A broad sheet of ice, which is an extension of the south polar ice cap is located south of the lava flow, to the left in the (nadir) image. The steep flanks clearly show white, clean ice. The thickness of the ice is between 900 and 1100 m — March: Promethei Planum - Mars: Promethei Planum - Promethei Planum is a region located near the southern pole of Mars. This region is seasonally covered with a thick layer of ice up to 3500 metres thick. On this image obtained by the Mars Express probe on September 22, 2005, an impact crater about 100 km wide and 800 metres deep is visible to the right (north). It is partially covered with ice. In the center of the image, structures formed by lava flows; on the left of the image, ice, which is an extension of the southern polar cap. Promethei Planum, an area seasonally covered with layer of ice more than 3500 m thick layer of ice in the martian south polar region, was the subject of the High Resolution Stereo Camera's focus on 22 September 2005 as Mars Express was in orbit above the Red Planet. Promethei Planum lies at approximately 76* south and 105* east. An approximately 100 km - large and 800 m - deep impact crater is visible in the northern part of the image. The crater's interio

March: Promethei Planum - Mars: Promethei Planum - Promethei Planum is a region located near the southern pole of Mars. This region is seasonally covered with a thick layer of ice up to 3500 metres thick. On this image obtained by the Mars Express probe on September 22, 2005, an impact crater about 100 km wide and 800 metres deep is visible to the right (north). It is partially covered with ice. In the center of the image, structures formed by lava flows; on the left of the image, ice, which is an extension of the southern polar cap. Promethei Planum, an area seasonally covered with layer of ice more than 3500 m thick layer of ice in the martian south polar region, was the subject of the High Resolution Stereo Camera's focus on 22 September 2005 as Mars Express was in orbit above the Red Planet. Promethei Planum lies at approximately 76* south and 105* east. An approximately 100 km - large and 800 m - deep impact crater is visible in the northern part of the image. The crater's interio

PIX4616118

Lieutenant James Wilcox (d. 1811), c.1806-09 (watercolour, ivory, glass, gilt, human hair)

Lieutenant James Wilcox (d. 1811), c.1806-09 (watercolour, ivory, glass, gilt, human hair)

Unknown Artist, (19th century)

MMM7340101

Weymouth and Great Western Galop, c1870 (lithograph on paper)

Weymouth and Great Western Galop, c1870 (lithograph on paper)

Sherren, John (1846-1922)

IGM8836227

Birth of stars in the nebula NGC 3372 - Star formation in the Carina Nebula - Detail of the nebula of the Carene seen in visible light (top) and infrared (bottom) by the Hubble space telescope. The top image shows a column of gas and dust eroded by ultraviolet radiation emitted by young stars. Jets are also visible, showing the presence of a nascent star. In the infrared image, the dust clouds radiate little, the nascent star responsible for these jets appears. NGC 3372 is located about 7000 light years away from Earth. Images obtained in July 2009. The pictures demonstrate one example of the broad wavelength range of the new Wide Field Camera 3 (WFC3) aboard the Hubble telescope, extending from ultraviolet to visible to infrared light. Composed of gas and dust, the pillar resides in a tempestuous stellar nursery called the Carina Nebula, located 7500 light - years away in the southern constellation of Carina. The pair of images shows that astronomers are given a much more complete view of the pillar and its contents when distinct details not seen at visible wavelengths are uncovered in near - infrared light. The top image, taken in visible light, shows the tip of the three - light - year - long pillar, bathed in the glow of light from hot, massive stars off the top of the image. Scorching radiation and fast winds (streams of charged particles) from these stars are sculpting the pillar and causing new stars to form within it. Streamers of gas and dust can be seen flowing off the top of the structure. Nestled inside this dense structure are fledgling stars. They cannot be seen in this image because they are hidden by a wall of gas and dust. Although the stars themselves are invisible, one of them is providing evidence of its existence. Thin puffs of material can be seen travelling to the left and to the right of a dark notch in the centre of the pillar. The matter is part of — Birth of stars in the nebula NGC 3372 - Star formation in the Carina Nebula - Detail of the nebula of the Carene seen in visible light (top) and infrared (bottom) by the Hubble space telescope. The top image shows a column of gas and dust eroded by ultraviolet radiation emitted by young stars. Jets are also visible, showing the presence of a nascent star. In the infrared image, the dust clouds radiate little, the nascent star responsible for these jets appears. NGC 3372 is located about 7000 light years away from Earth. Images obtained in July 2009. The pictures demonstrate one example of the broad wavelength range of the new Wide Field Camera 3 (WFC3) aboard the Hubble telescope, extending from ultraviolet to visible to infrared light. Composed of gas and dust, the pillar resides in a tempestuous stellar nursery called the Carina Nebula, located 7500 light - years away in the southern constellation of Carina. The pair of images shows that astronomers are given a much more complete vie

Birth of stars in the nebula NGC 3372 - Star formation in the Carina Nebula - Detail of the nebula of the Carene seen in visible light (top) and infrared (bottom) by the Hubble space telescope. The top image shows a column of gas and dust eroded by ultraviolet radiation emitted by young stars. Jets are also visible, showing the presence of a nascent star. In the infrared image, the dust clouds radiate little, the nascent star responsible for these jets appears. NGC 3372 is located about 7000 light years away from Earth. Images obtained in July 2009. The pictures demonstrate one example of the broad wavelength range of the new Wide Field Camera 3 (WFC3) aboard the Hubble telescope, extending from ultraviolet to visible to infrared light. Composed of gas and dust, the pillar resides in a tempestuous stellar nursery called the Carina Nebula, located 7500 light - years away in the southern constellation of Carina. The pair of images shows that astronomers are given a much more complete vie

PIX4619072

Enceladus, Saturn's satellite, seen by Cassini - Saturn's moon Enceladus from Cassini - Mosaic of false-coloured images obtained by the Cassini probe during the flight over this satellite on 11 August 2008. The image shows a fractured region in the southern hemisphere of the satellite. This mosaic of Saturn's moon Enceladus provides broad regional context for the ultra - sharp, close - up views Nasa's Cassini spacecraft acquired minutes earlier, during its flyby on Aug. 11, 2008. This false - color mosaic combines Imaging Science Subsystem (ISS) narrow - angle camera images obtained through ultraviolet, green, and near - infrared camera filters. Areas that are greenish in appearance are believed to represent deposits of coarser grained ice and solid boulders that are too small to be seen at this scale, but which are visible in the higher resolution views, while whitish deposits represent finer grained ice. The mosaic shows that coarse - grained and solid ice are concentrated along valley floors and walls, as well as along the upraised flanks of the “” tiger stripe”” fractures, which may be covered with plume fallout that landed not far from the sources. Elsewhere on Enceladus, this coarse water ice is concentrated within outcrops along cliff faces and at the top of ridges. The sinuous boundary of scarps and ridges that encircles the south polar terrain at about 55 degrees south latitude is conspicuous. Much of the coarse - grained or solid ice along this boundary may be blocky rubble that has crumbled off of cliff faces as a result of ongoing seismic activity. The lighting conditions over the polar region highlight features, such as fractures and ridges, that are barely visible in the July 2005 views, and vice versa. The four most prominent sulci (from top to bottom: Damascus, Baghdad, Alexandria and Cairo) appear as generally horizontal fractures near lower right, and they extend into the moon's night side. The mosaic is an orthographic projection centered at 63.0 degrees south — Enceladus, Saturn's satellite, seen by Cassini - Saturn's moon Enceladus from Cassini - Mosaic of false-coloured images obtained by the Cassini probe during the flight over this satellite on 11 August 2008. The image shows a fractured region in the southern hemisphere of the satellite. This mosaic of Saturn's moon Enceladus provides broad regional context for the ultra - sharp, close - up views Nasa's Cassini spacecraft acquired minutes earlier, during its flyby on Aug. 11, 2008. This false - color mosaic combines Imaging Science Subsystem (ISS) narrow - angle camera images obtained through ultraviolet, green, and near - infrared camera filters. Areas that are greenish in appearance are believed to represent deposits of coarser grained ice and solid boulders that are too small to be seen at this scale, but which are visible in the higher resolution views, while whitish deposits represent finer grained ice. The mosaic shows that coarse - grained and solid ice are concentrated along vall

Enceladus, Saturn's satellite, seen by Cassini - Saturn's moon Enceladus from Cassini - Mosaic of false-coloured images obtained by the Cassini probe during the flight over this satellite on 11 August 2008. The image shows a fractured region in the southern hemisphere of the satellite. This mosaic of Saturn's moon Enceladus provides broad regional context for the ultra - sharp, close - up views Nasa's Cassini spacecraft acquired minutes earlier, during its flyby on Aug. 11, 2008. This false - color mosaic combines Imaging Science Subsystem (ISS) narrow - angle camera images obtained through ultraviolet, green, and near - infrared camera filters. Areas that are greenish in appearance are believed to represent deposits of coarser grained ice and solid boulders that are too small to be seen at this scale, but which are visible in the higher resolution views, while whitish deposits represent finer grained ice. The mosaic shows that coarse - grained and solid ice are concentrated along vall

PIX4625460

Machine gunner's body armour (Sappenpanzer), 1916-17 (steel)

Machine gunner's body armour (Sappenpanzer), 1916-17 (steel)

German School, (20th century)

AMR3548830

An Allegorical Posthumous Portrait of Algernon Sidney (1622-1683) en grisaille

An Allegorical Posthumous Portrait of Algernon Sidney (1622-1683) en grisaille

Dutch School, (18th century)

USB1159907

A Kick at the Broad-bottoms! - i.e. - Emancipation of 'All the Talents', published by Hannah Humphrey in 1807 (hand-coloured etching with aquatint)

A Kick at the Broad-bottoms! - i.e. - Emancipation of 'All the Talents', published by Hannah Humphrey in 1807 (hand-coloured etching with aquatint)

Gillray, James (1757-1815)

NCO190144

Private conversation or a peep behind the curtain, 1807 (coloured engraving)

Private conversation or a peep behind the curtain, 1807 (coloured engraving)

English School, (19th century)

HRP2624944

A kick at the broad-bottoms!-i.e.-Emancipation of all the talents!, 1807 (coloured engraving)

A kick at the broad-bottoms!-i.e.-Emancipation of all the talents!, 1807 (coloured engraving)

Gillray, James (1757-1815)

HRP2624942

A Plumper for Paul! or The Little Taylor done over! i.e The terrible effects of provoking a Red-hot shot from the Broad Bottom'd Whig Battery, published by Hannah Humphrey in 1807 (hand-coloured etching)

A Plumper for Paul! or The Little Taylor done over! i.e The terrible effects of provoking a Red-hot shot from the Broad Bottom'd Whig Battery, published by Hannah Humphrey in 1807 (hand-coloured etching)

Gillray, James (1757-1815)

NCO193171

The Cabinetical Balance, published by Hannah Humphrey in 1806 (hand-coloured etching)

The Cabinetical Balance, published by Hannah Humphrey in 1806 (hand-coloured etching)

Gillray, James (1757-1815)

NCO190494

Charon's Boat or the Ghosts of All the Talents Taking Their Last Voyage, from the Pope's Gallery at Rome, a Group of Naked Whig Politicians, Including Three Grenvilles, Sheridan, St. Vincent, Moira, Temple, Erskine, Howick, Petty, Whitbread, Sheridan, Windham,and Tomline, Bishop of Lincoln, Crossing the River Styx in a Boat Named the Broad Bottom Packet. Sidmouth's Head Emerges from the Water Next to the Boat. The Boat's Torn Sail Has Inscription Catholic Emancipation and the Center Mast is Crowned with the Prince of Wales Feathers and Motto Ich Dien. On the Far Side the Shades of Cromwell, Charles Fox and Robespierre Wave to Them. Overhead, on Brooms, Are the Three Fates; to the Left a Three-Headed Dog. Above the Boat Three Birds Soil the Boat and Politicians.

Charon's Boat or the Ghosts of All the Talents Taking Their Last Voyage, from the Pope's Gallery at Rome, a Group of Naked Whig Politicians, Including Three Grenvilles, Sheridan, St. Vincent, Moira, Temple, Erskine, Howick, Petty, Whitbread, Sheridan, Windham,and Tomline, Bishop of Lincoln, Crossing the River Styx in a Boat Named the Broad Bottom Packet. Sidmouth's Head Emerges from the Water Next to the Boat. The Boat's Torn Sail Has Inscription Catholic Emancipation and the Center Mast is Crowned with the Prince of Wales Feathers and Motto Ich Dien. On the Far Side the Shades of Cromwell, Charles Fox and Robespierre Wave to Them. Overhead, on Brooms, Are the Three Fates; to the Left a Three-Headed Dog. Above the Boat Three Birds Soil the Boat and Politicians.

LZT1012535

Charon's Boat, or The Ghost's of the 'All Talents' Taking their Last Voyage, published by Hannah Humphrey, 1807 (hand-coloured etching)

Charon's Boat, or The Ghost's of the 'All Talents' Taking their Last Voyage, published by Hannah Humphrey, 1807 (hand-coloured etching)

Gillray, James (1757-1815)

STC2489003

L'assemblée nationale: - or - grand co-operation meeting at St. Ann's Hill, pub. 1804 (hand coloured engraving)

L'assemblée nationale: - or - grand co-operation meeting at St. Ann's Hill, pub. 1804 (hand coloured engraving)

Gillray, James (1757-1815)

STC2655347

L'Assemblee Nationale or Grand Cooperation Meeting at St. Ann's Hill. Respectfully Dedicated to the Admirers of a Broad-Bottom'D Administration, Gillray, James, 1756-1815, Artist, [London] : Published by H. Humphrey, 1804 June 18., 1 Print : Etching, Hand-Colored., Print Shows a Reception Given by Charles James Fox and Wife for Various Groups and Friends of the Prince of Wales, All Opposed to the Government.

L'Assemblee Nationale or Grand Cooperation Meeting at St. Ann's Hill. Respectfully Dedicated to the Admirers of a Broad-Bottom'D Administration, Gillray, James, 1756-1815, Artist, [London] : Published by H. Humphrey, 1804 June 18., 1 Print : Etching, Hand-Colored., Print Shows a Reception Given by Charles James Fox and Wife for Various Groups and Friends of the Prince of Wales, All Opposed to the Government.

LZT1012674

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