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Tunic worn by Lieutenant Campbell Clark, 2nd Bengal European Fusiliers, 1857 (tunic)

Tunic worn by Lieutenant Campbell Clark, 2nd Bengal European Fusiliers, 1857 (tunic)

British School, (19th century)

NAM5929439

Pressure Suit, A7-L, Armstrong, Apollo 11, Flown, 1969 (mixed media)

Pressure Suit, A7-L, Armstrong, Apollo 11, Flown, 1969 (mixed media)

American School, (20th century)

SMT3741591

Pressure Suit, A7-L, Armstrong, Apollo 11, Flown, 1969 (mixed media)

Pressure Suit, A7-L, Armstrong, Apollo 11, Flown, 1969 (mixed media)

American School, (20th century)

SMT3741596

Pressure Suit, A7-L, Armstrong, Apollo 11, Flown, 1969 (mixed media)

Pressure Suit, A7-L, Armstrong, Apollo 11, Flown, 1969 (mixed media)

American School, (20th century)

SMT3741598

Barnard's loop and constellation Orion - Barnard's loop and Orion constellation - The constellation Orion and its nebulae. The main stars of this constellation are two supergeants, Betelgeuse (red) on the top left and Rigel (blue) on the bottom right. In the center of the constellation are the three stars forming Orion's Belt (or Baldrier) and the dark nebula of the horse's head (IC434 - B33). Further down, the large Orion nebula (M42) vast star-forming region. Wrapping these nebulae, Barnard's loop, a circle-arch nebula that would come from the explosion of a supernova more than two million years ago. The Orion constellation and its nebulae. The two Orion's bright stars are both supergiant stars: Betelgeuse (a red one) and Rigel (blue one). The center of this constellation is the Orion Belt with the Horsehead nebula (IC 434 - B33). Lower, the great Orion nebula, M42, a large star forming region. Also visible on this image, the Barnard's loop, a very faint nebula. This is composite mos

Barnard's loop and constellation Orion - Barnard's loop and Orion constellation - The constellation Orion and its nebulae. The main stars of this constellation are two supergeants, Betelgeuse (red) on the top left and Rigel (blue) on the bottom right. In the center of the constellation are the three stars forming Orion's Belt (or Baldrier) and the dark nebula of the horse's head (IC434 - B33). Further down, the large Orion nebula (M42) vast star-forming region. Wrapping these nebulae, Barnard's loop, a circle-arch nebula that would come from the explosion of a supernova more than two million years ago. The Orion constellation and its nebulae. The two Orion's bright stars are both supergiant stars: Betelgeuse (a red one) and Rigel (blue one). The center of this constellation is the Orion Belt with the Horsehead nebula (IC 434 - B33). Lower, the great Orion nebula, M42, a large star forming region. Also visible on this image, the Barnard's loop, a very faint nebula. This is composite mos

R. Gendler

PIX4617896

Infantry officer thought to be Lord John Douglas Campbell, 7th Duke of Argyle (1777-1847), 1806 circa (miniature on ivory)

Infantry officer thought to be Lord John Douglas Campbell, 7th Duke of Argyle (1777-1847), 1806 circa (miniature on ivory)

Housom, George (fl. 1796-1806)

NAM5927536

Sir Ralph Ellerker of Risby (b.1548/9) at the age of 73 (after British (English) School of 1632)

Sir Ralph Ellerker of Risby (b.1548/9) at the age of 73 (after British (English) School of 1632)

Orpen, Rebecca Dulcibella (1830-1923)

USB1160566

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

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

PFH3277801

Grand Trou bleu, Lighthouse reef, Belize - Satellite image of Belize's Lighthouse Reef with the Great Blue Hole - Satellite photo of Lighthouse Reef obtained by EO satellite - 1 March 24, 2009. Lighthouse Reef is a small atoll located 80 km from the mainland and Belize City. It belongs to the network of reserves of the Belize Barriere Reef, a UNESCO World Heritage Site. In the center of the image is the Great Blue Hole, an ancient, collapsed limestone cave, almost circular, with a diameter of more than 300 m and 120 m deep. The Advanced Land Imager (ALI) on Nasa's Earth Observing - 1 satellite captured this image of Lighthouse Reef in the Caribbean Sea on March 24, 2009. In the middle of the image lies a giant circle of deep blue. Roughly 300 meters (1,000 feet) across and 125 meters (400 feet) deep, the feature is known as the Great Blue Hole. The Great Blue Hole is surrounded by a ring of lighter color caused by elevated coral. In fact, parts of the ring surrounding this feature actu

Grand Trou bleu, Lighthouse reef, Belize - Satellite image of Belize's Lighthouse Reef with the Great Blue Hole - Satellite photo of Lighthouse Reef obtained by EO satellite - 1 March 24, 2009. Lighthouse Reef is a small atoll located 80 km from the mainland and Belize City. It belongs to the network of reserves of the Belize Barriere Reef, a UNESCO World Heritage Site. In the center of the image is the Great Blue Hole, an ancient, collapsed limestone cave, almost circular, with a diameter of more than 300 m and 120 m deep. The Advanced Land Imager (ALI) on Nasa's Earth Observing - 1 satellite captured this image of Lighthouse Reef in the Caribbean Sea on March 24, 2009. In the middle of the image lies a giant circle of deep blue. Roughly 300 meters (1,000 feet) across and 125 meters (400 feet) deep, the feature is known as the Great Blue Hole. The Great Blue Hole is surrounded by a ring of lighter color caused by elevated coral. In fact, parts of the ring surrounding this feature actu

PIX4672819

Trial Piece Worked on Both Sides, c.1391-1353 BC (limestone)

Trial Piece Worked on Both Sides, c.1391-1353 BC (limestone)

Egyptian 18th Dynasty (c.1567-1320 BC)

XCL491037

Nebula Sh2 - 106 in the Swan - Sh2 - 106 nebula in Cygnus - Sharpless 106 (Sh2 - 106) is a star-forming region in the constellation Swan. Image obtained by Hubble Space Telescope (HST) and Subaru Telescope. The bipolar star - forming region, called Sharpless 2 - 106, or S106 for short, looks like a soaring, celestial snow angel. The outstretched “” wings”” of the nebula record the contrasting imprint of heat and motion against the backdrop of a colder medium. Twin lobes of super - hot gas, glowing blue in this image, stretch outward from the central star. This hot gas creates the “” wings”” of our angel. A ring of dust and gas orbiting the star acts like a belt, cinching the expanding nebula into an “” hourglass””” shape. This composite image combines optical and near - infrared astronomical data from the Hubble Space Telescope with mid - infrared data from the ground - based Subaru Telescope, located on Mauna Kea in Hawaii. The Hubble data (H - alpha, J, and H) were taken as part of H

Nebula Sh2 - 106 in the Swan - Sh2 - 106 nebula in Cygnus - Sharpless 106 (Sh2 - 106) is a star-forming region in the constellation Swan. Image obtained by Hubble Space Telescope (HST) and Subaru Telescope. The bipolar star - forming region, called Sharpless 2 - 106, or S106 for short, looks like a soaring, celestial snow angel. The outstretched “” wings”” of the nebula record the contrasting imprint of heat and motion against the backdrop of a colder medium. Twin lobes of super - hot gas, glowing blue in this image, stretch outward from the central star. This hot gas creates the “” wings”” of our angel. A ring of dust and gas orbiting the star acts like a belt, cinching the expanding nebula into an “” hourglass””” shape. This composite image combines optical and near - infrared astronomical data from the Hubble Space Telescope with mid - infrared data from the ground - based Subaru Telescope, located on Mauna Kea in Hawaii. The Hubble data (H - alpha, J, and H) were taken as part of H

PIX4620999

A George III mahogany and brass-mounted quarter-chiming musical and automaton table clock by Eardley Norton, London

A George III mahogany and brass-mounted quarter-chiming musical and automaton table clock by Eardley Norton, London

English School, (18th century)

CH6424322

Agnes Enthroned and Scenes from Her Legend. Historiated miniature of Agnes enthroned flanked by two musician angels, below (left) the saint's statue holding out its finger to receive an emerald ring from Paulinus, a priest of the church of Saint Agnes who wished to be allowed to marry, and (right) Agnes appearing to relatives maintaining a vigil besides her tomb. Historiated full-page border in colours and gold, of foliage and birds with three medallions in the lower margin containing two scenes of Agnes surviving being thrown into flames at the order of Aspasius and a male and female member of the Compagnia di Sant'Agnese kneeling in prayer. Beneath the miniature is a single four-line red stave, musical notation and a single line of text in gold capitals 'Sancta Agnese da dio'.

Agnes Enthroned and Scenes from Her Legend. Historiated miniature of Agnes enthroned flanked by two musician angels, below (left) the saint's statue holding out its finger to receive an emerald ring from Paulinus, a priest of the church of Saint Agnes who wished to be allowed to marry, and (right) Agnes appearing to relatives maintaining a vigil besides her tomb. Historiated full-page border in colours and gold, of foliage and birds with three medallions in the lower margin containing two scenes of Agnes surviving being thrown into flames at the order of Aspasius and a male and female member of the Compagnia di Sant'Agnese kneeling in prayer. Beneath the miniature is a single four-line red stave, musical notation and a single line of text in gold capitals 'Sancta Agnese da dio'.

BL3293390

Planetary nebula NGC 5189 in the fly - This nebula is located about 3000 light years from Earth in the southern constellation of the fly. Image obtained by the Gemini and Hubble telescopes (HST). NGC 5189 is a planetary nebula. At the end of its life, a star with a mass less than eight times that of the Sun will blow its outer layers away, giving rise to a planetary nebula. Some of these stellar puffballs are almost round, resembling huge soap bubbles or giant planets (hence the name), but others, such as NGC 5189 are more intricate. In particular, this planetary nebula exhibits a curious S” - shaped profile, with a central bar that is most likely the projection of an inner ring of gas discharged by the star, seen edge on. The details of the physical processes producing such a complex symmetry from a simple, spherical star are still the object of astronomical controversy. One possibility is that the star has a very close (but unseen) companion. Over time the orbits drift due to precess

Planetary nebula NGC 5189 in the fly - This nebula is located about 3000 light years from Earth in the southern constellation of the fly. Image obtained by the Gemini and Hubble telescopes (HST). NGC 5189 is a planetary nebula. At the end of its life, a star with a mass less than eight times that of the Sun will blow its outer layers away, giving rise to a planetary nebula. Some of these stellar puffballs are almost round, resembling huge soap bubbles or giant planets (hence the name), but others, such as NGC 5189 are more intricate. In particular, this planetary nebula exhibits a curious S” - shaped profile, with a central bar that is most likely the projection of an inner ring of gas discharged by the star, seen edge on. The details of the physical processes producing such a complex symmetry from a simple, spherical star are still the object of astronomical controversy. One possibility is that the star has a very close (but unseen) companion. Over time the orbits drift due to precess

PIX4623115

Astrolabe, c.1570 (gilt brass)

Astrolabe, c.1570 (gilt brass)

Flemish School, (16th century)

CH3057865

Planetary nebula NGC 5189 in the Fly - NGC 5189 - Planetary nebula in Musca - This nebula is located about 3000 light years from Earth in the southern constellation of Fly. Image obtained by the Gemini telescope. NGC 5189 is a planetary nebula. At the end of its life, a star with a mass less than eight times that of the Sun will blow its outer layers away, giving rise to a planetary nebula. Some of these stellar puffballs are almost round, resembling huge soap bubbles or giant planets (hence the name), but others, such as NGC 5189 are more intricate. In particular, this planetary nebula exhibits a curious S” - shaped profile, with a central bar that is most likely the projection of an inner ring of gas discharged by the star, seen edge on. The details of the physical processes producing such a complex symmetry from a simple, spherical star are still the object of astronomical controversy. One possibility is that the star has a very close (but unseen) companion. Over time the orbits dri

Planetary nebula NGC 5189 in the Fly - NGC 5189 - Planetary nebula in Musca - This nebula is located about 3000 light years from Earth in the southern constellation of Fly. Image obtained by the Gemini telescope. NGC 5189 is a planetary nebula. At the end of its life, a star with a mass less than eight times that of the Sun will blow its outer layers away, giving rise to a planetary nebula. Some of these stellar puffballs are almost round, resembling huge soap bubbles or giant planets (hence the name), but others, such as NGC 5189 are more intricate. In particular, this planetary nebula exhibits a curious S” - shaped profile, with a central bar that is most likely the projection of an inner ring of gas discharged by the star, seen edge on. The details of the physical processes producing such a complex symmetry from a simple, spherical star are still the object of astronomical controversy. One possibility is that the star has a very close (but unseen) companion. Over time the orbits dri

PIX4623091

Trial Piece Worked on Both Sides, c.1391-1353 BC (limestone)

Trial Piece Worked on Both Sides, c.1391-1353 BC (limestone)

Egyptian 18th Dynasty (c.1567-1320 BC)

XCL491038

New York, New York: c. 1922 A sectional view of the Holland Tunnel, a marvel of modern science, and all its features: 1. Exhaust airports. 2. Telephone & telegraph cables. 3. Fire extinguisher. 4. Water supply pipe. 5. Continuous duct for fresh air supply. 6. Fresh air flues every 15 feet. 7. Exhaust air ducts running the length of the tunnel. 8. Tunnel segment weighing 3000 pounds. 9. Weight of complete ring 21.6 tons. 10. Concrete. 11. Sidewalk. 12. Power cables for tunnel. 13. Fresh air expansion chamber. 14. Fresh air flues every 15 feet. 15. Drain. 16. Fresh air duct running entire length of tunnel.

New York, New York: c. 1922 A sectional view of the Holland Tunnel, a marvel of modern science, and all its features: 1. Exhaust airports. 2. Telephone & telegraph cables. 3. Fire extinguisher. 4. Water supply pipe. 5. Continuous duct for fresh air supply. 6. Fresh air flues every 15 feet. 7. Exhaust air ducts running the length of the tunnel. 8. Tunnel segment weighing 3000 pounds. 9. Weight of complete ring 21.6 tons. 10. Concrete. 11. Sidewalk. 12. Power cables for tunnel. 13. Fresh air expansion chamber. 14. Fresh air flues every 15 feet. 15. Drain. 16. Fresh air duct running entire length of tunnel.

UIG5449596

China: Xiang Ying (c. 1895-1941) was a war-time Chinese communist leader reaching the rank of political chief of staff of the New Fourth Army during World War II. He was assassinated by a member of his staff in 1941

China: Xiang Ying (c. 1895-1941) was a war-time Chinese communist leader reaching the rank of political chief of staff of the New Fourth Army during World War II. He was assassinated by a member of his staff in 1941

PFH2635742

Impact on the Moon at the Cretace - Cretaceous lunar strike - Artist's view of an asteroid impact on the Moon illuminating a nocturnal landscape of the cretace. In the foreground, a spinosaur, a theropod dinosaur who lived in what is now Egypt 95 to 93 million years ago. What may appear here as a diamond ring effect from a solar eclipse is in fact a brilliant and momentary flash of light signaling a massive asteroid impact on the Moon. The Moon and all the inner planets of the Solar System show evidence of a long and violent history of encounters with meteorites and asteroids - leftover debris from the formation of the Solar System. This image depicts an asteroid colliding with the Moon about 95 million years ago. The perspective is from the surface of the Earth in what today is Egypt. The impact would have released millions of times more energy than today's largest nuclear weapon, creating a flash of light that would be far brighter than any star in the sky. In the foreground of this

Impact on the Moon at the Cretace - Cretaceous lunar strike - Artist's view of an asteroid impact on the Moon illuminating a nocturnal landscape of the cretace. In the foreground, a spinosaur, a theropod dinosaur who lived in what is now Egypt 95 to 93 million years ago. What may appear here as a diamond ring effect from a solar eclipse is in fact a brilliant and momentary flash of light signaling a massive asteroid impact on the Moon. The Moon and all the inner planets of the Solar System show evidence of a long and violent history of encounters with meteorites and asteroids - leftover debris from the formation of the Solar System. This image depicts an asteroid colliding with the Moon about 95 million years ago. The perspective is from the surface of the Earth in what today is Egypt. The impact would have released millions of times more energy than today's largest nuclear weapon, creating a flash of light that would be far brighter than any star in the sky. In the foreground of this

Walter B Myers

PIX4662978

Titan, Saturn satellite seen by Cassini - Saturn's moon Titan as seen by Cassini spacecraft: Visible and infrared composite image of Titan taken by the Cassini probe on August 21, 2014. View of methane and ethane lakes lit by the Sun. - This near-infrared, color mosaic from Nasa's Cassini spacecraft shows the sun glinting off of Titan's north polar seas. - The sunglint, also called a specular reflection, is the bright area near the 11 o'clock position at upper left. This mirror-like reflection, known as the specular point, is in the south of Titan's largest sea, Kraken Mare, just north of an island archipelago separating two separate parts of the sea - This particular sunglint was so bright as to saturate the detector of Cassini's Visual and Infrared Mapping Spectrometer (VIMS) instrument, which captures the view. - The southern portion of Kraken Mare (the area surrounding the specular feature toward upper left) displays a “” bathtub ring”” - a bright margin of evaporate deposits - whi

Titan, Saturn satellite seen by Cassini - Saturn's moon Titan as seen by Cassini spacecraft: Visible and infrared composite image of Titan taken by the Cassini probe on August 21, 2014. View of methane and ethane lakes lit by the Sun. - This near-infrared, color mosaic from Nasa's Cassini spacecraft shows the sun glinting off of Titan's north polar seas. - The sunglint, also called a specular reflection, is the bright area near the 11 o'clock position at upper left. This mirror-like reflection, known as the specular point, is in the south of Titan's largest sea, Kraken Mare, just north of an island archipelago separating two separate parts of the sea - This particular sunglint was so bright as to saturate the detector of Cassini's Visual and Infrared Mapping Spectrometer (VIMS) instrument, which captures the view. - The southern portion of Kraken Mare (the area surrounding the specular feature toward upper left) displays a “” bathtub ring”” - a bright margin of evaporate deposits - whi

PIX4625340

Saturn above the clouds of Titan - Illustration - Saturn from atop Titan's hydrocarbon haze - Artist's view of the planet Saturn view 80 km above the surface of his satellite Titan. In the plane of the rings of the planet appear from left to right the satellites Enceladus, Dione, Tethys and Rhea. Saturn and its rings would be a majestic sight lording over Titan's hydrocarbon haze. The viewpoint is from 50 miles above Titan's surface and three - quarters of a million miles away from Saturn itself. Four of Saturn's smaller satellites can also be seen along the ring plane: left to right are Enceladus, Dione, Tethys and Rhea. Technically, the orange clouds mark the beginning of Titan's condensate haze, which consists of ethane, methane, nitrogen, and a variety of hydrocarbons known collectively as tholin. These gases and hydrocarbons extend upward another 250 miles, resulting in a bluish, earthlike sky, albeit darker due to Titan's great distance from the Sun. Tholin is created by the inte

Saturn above the clouds of Titan - Illustration - Saturn from atop Titan's hydrocarbon haze - Artist's view of the planet Saturn view 80 km above the surface of his satellite Titan. In the plane of the rings of the planet appear from left to right the satellites Enceladus, Dione, Tethys and Rhea. Saturn and its rings would be a majestic sight lording over Titan's hydrocarbon haze. The viewpoint is from 50 miles above Titan's surface and three - quarters of a million miles away from Saturn itself. Four of Saturn's smaller satellites can also be seen along the ring plane: left to right are Enceladus, Dione, Tethys and Rhea. Technically, the orange clouds mark the beginning of Titan's condensate haze, which consists of ethane, methane, nitrogen, and a variety of hydrocarbons known collectively as tholin. These gases and hydrocarbons extend upward another 250 miles, resulting in a bluish, earthlike sky, albeit darker due to Titan's great distance from the Sun. Tholin is created by the inte

Walter B Myers

PIX4626034

(Figures from left to right): Fig. 19: Rohand, Earl of Warwick. In chain armour, with shield. Fig.20: Dame Felice, his daughter, wife of Sir Guy (in her right), Earl of Warwick. She receives from the herdsman the ring sent to her by her husband, just before his death. Fig.21: Guy, Earl of Warwick. In chain armour; holding a battle-axe and shield. At his feet lies a group of monsters of which he rid the world. Fig.22: Guy, Earl of Warwick, holding a staff and rosary; his head irradiated. At his feet, Colbrond the Danish giant whom he slew at Winchester. Fig.23: Rainburn, Earl of Warwick, son of Sir Guy and Lady Felice. He hold a sword. Unknown slain figure at his feet. He earned for himself in Russia the reputation of a valiant knight, from having slain many giants in single combat.

(Figures from left to right): Fig. 19: Rohand, Earl of Warwick. In chain armour, with shield. Fig.20: Dame Felice, his daughter, wife of Sir Guy (in her right), Earl of Warwick. She receives from the herdsman the ring sent to her by her husband, just before his death. Fig.21: Guy, Earl of Warwick. In chain armour; holding a battle-axe and shield. At his feet lies a group of monsters of which he rid the world. Fig.22: Guy, Earl of Warwick, holding a staff and rosary; his head irradiated. At his feet, Colbrond the Danish giant whom he slew at Winchester. Fig.23: Rainburn, Earl of Warwick, son of Sir Guy and Lady Felice. He hold a sword. Unknown slain figure at his feet. He earned for himself in Russia the reputation of a valiant knight, from having slain many giants in single combat.

BL3298959

Detail of the nebula NGC 3603 in the Carene - Star life cycle in NGC 3603 - In the center of the picture is a cluster of massive young stars formed from the gas surrounding them. Two pillars of gas and dust visible on the right at the top and bottom will one day form other stars, as probably the dark cloud at the top right of the image called Bok's globule. Above the left of the star cluster, an old blue supergiant star, Sher 25, arrives at the end of life. The nebula NGC 3603 is located approximately 20,000 light years from Earth in the southern constellation of Carene. Image obtained by the Hubble Space Telescope. This image made by the Hubble space telescope nicely illustrates the entire stellar life cycle of stars, starting with the Bok globules (dark clouds at the upper right) and giant gaseous pillars, followed by circumstellar disks and progressing to evolved massive stars in the young starburst cluster (center). The blue supergiant star Sher 25 with its ring and bipolar outflow

Detail of the nebula NGC 3603 in the Carene - Star life cycle in NGC 3603 - In the center of the picture is a cluster of massive young stars formed from the gas surrounding them. Two pillars of gas and dust visible on the right at the top and bottom will one day form other stars, as probably the dark cloud at the top right of the image called Bok's globule. Above the left of the star cluster, an old blue supergiant star, Sher 25, arrives at the end of life. The nebula NGC 3603 is located approximately 20,000 light years from Earth in the southern constellation of Carene. Image obtained by the Hubble Space Telescope. This image made by the Hubble space telescope nicely illustrates the entire stellar life cycle of stars, starting with the Bok globules (dark clouds at the upper right) and giant gaseous pillars, followed by circumstellar disks and progressing to evolved massive stars in the young starburst cluster (center). The blue supergiant star Sher 25 with its ring and bipolar outflow

PIX4619146

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

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

PIX4619201

Saturn seen by the Cassin probe - Saturn seen by Cassini spacecraft on october 10 2013: Saturn seen by the Cassini probe on October 10, 2013. - A swing high above Saturn by Nasa's Cassini spacecraft revealed this stately view of the golden-hued planet and its main rings. The view is in natural color, as human eyes would have seen it. This mosaic was made from 36 images in three color filters obtained by Cassini's imaging science subsystem on Oct. 10, 2013 - A bright, narrow wave of clouds around 42 degrees north latitude appears to be some of the turbulent aftermath of a giant storm that reached its violent peak in early 2011. The mysterious six-sided weather pattern known as the hexagon is visible around Saturn's north pole - The rings shown here include Saturn's main rings. The rings known as the C, B and A rings - listed here in order of closeness to Saturn - are easily seen. The F ring is also there, but not easily seen without enhancing the contrast of the image. (Rings were named

Saturn seen by the Cassin probe - Saturn seen by Cassini spacecraft on october 10 2013: Saturn seen by the Cassini probe on October 10, 2013. - A swing high above Saturn by Nasa's Cassini spacecraft revealed this stately view of the golden-hued planet and its main rings. The view is in natural color, as human eyes would have seen it. This mosaic was made from 36 images in three color filters obtained by Cassini's imaging science subsystem on Oct. 10, 2013 - A bright, narrow wave of clouds around 42 degrees north latitude appears to be some of the turbulent aftermath of a giant storm that reached its violent peak in early 2011. The mysterious six-sided weather pattern known as the hexagon is visible around Saturn's north pole - The rings shown here include Saturn's main rings. The rings known as the C, B and A rings - listed here in order of closeness to Saturn - are easily seen. The F ring is also there, but not easily seen without enhancing the contrast of the image. (Rings were named

PIX4625303

Cratere Manicouagan - Quebec - January 2014 - The Manicouagan Impact Crater reservoir in Quebec, Canada - Cratere d'impact Manicouagan, Quebec, seen from the International Space Station (ISS) on January 2, 2014. This 100-kilometre crater formed 212 million years ago, following the fall of an asteroid on Earth. One of the Expedition 38 crew members aboard the Earth - orbiting International Space Station recorded this image which features the Manicouagan Crater and reservoir located primarily in Manicouagan Regional County Municipality in the Cote - Nord region of Quebec, Canada. Scientists believe the crater was caused by the impact of a 5 kilometer (3 mile) diameter asteroid about 215.5 million years ago (Triassic Period). The crater is a multiple - ring structure about 100 kilometers (60 miles) across, with its 70 kilometer (40 mile) diameter inner ring as its most prominent feature; it contains a 70 kilometer (40 mile) diameter annular lake, the Manicouagan Reservoir, surrounding an

Cratere Manicouagan - Quebec - January 2014 - The Manicouagan Impact Crater reservoir in Quebec, Canada - Cratere d'impact Manicouagan, Quebec, seen from the International Space Station (ISS) on January 2, 2014. This 100-kilometre crater formed 212 million years ago, following the fall of an asteroid on Earth. One of the Expedition 38 crew members aboard the Earth - orbiting International Space Station recorded this image which features the Manicouagan Crater and reservoir located primarily in Manicouagan Regional County Municipality in the Cote - Nord region of Quebec, Canada. Scientists believe the crater was caused by the impact of a 5 kilometer (3 mile) diameter asteroid about 215.5 million years ago (Triassic Period). The crater is a multiple - ring structure about 100 kilometers (60 miles) across, with its 70 kilometer (40 mile) diameter inner ring as its most prominent feature; it contains a 70 kilometer (40 mile) diameter annular lake, the Manicouagan Reservoir, surrounding an

PIX4630745

Shikotan island seen from space - Shikotan island seen from space - Shikotan island (Shikotan) is one of the largest islands of the Kuril archipelago, located in the Pacific Ocean between the Kamchatka Peninsula and northern Japan. In this image obtained by the EO-1 satellite on 14 February 2011, this volcanic island is surrounded by ice forming spirals in the wind. Ostrov Shikotan (or Shikotan - to) is a volcanic island at the southern end of the Kuril chain. Shikotan lies along the extreme southern edge of winter sea ice in the Northern Hemisphere. The Advanced Land Imager (ALI) on NASA's Earth Observing - 1 (EO - 1) satellite captured this natural - color image of Shikotan on February 14, 2011. The island is surrounded by sea ice - - swirling shapes of ghostly blue - gray. The ice in this image may have formed in a matter of several days, and it is prone to moving with currents. North of the western end of Shikotan, eddies have shaped the ice into rough circles. The eddies may resul

Shikotan island seen from space - Shikotan island seen from space - Shikotan island (Shikotan) is one of the largest islands of the Kuril archipelago, located in the Pacific Ocean between the Kamchatka Peninsula and northern Japan. In this image obtained by the EO-1 satellite on 14 February 2011, this volcanic island is surrounded by ice forming spirals in the wind. Ostrov Shikotan (or Shikotan - to) is a volcanic island at the southern end of the Kuril chain. Shikotan lies along the extreme southern edge of winter sea ice in the Northern Hemisphere. The Advanced Land Imager (ALI) on NASA's Earth Observing - 1 (EO - 1) satellite captured this natural - color image of Shikotan on February 14, 2011. The island is surrounded by sea ice - - swirling shapes of ghostly blue - gray. The ice in this image may have formed in a matter of several days, and it is prone to moving with currents. North of the western end of Shikotan, eddies have shaped the ice into rough circles. The eddies may resul

PIX4661440

Singing-bird box, c.1840 (gold, diamonds & enamel)

Singing-bird box, c.1840 (gold, diamonds & enamel)

Bruguier, Charles (1788-1862)

CH3025211

Supernova 1987A in the Great Magellan Cloud View by HST - Glittering stars and wisps of gas create a breathtaking backdrop for the self - destruction of a massive star, called supernova 1987A, in the Large Magellanic Cloud, a nearby galaxy. Astronomers in the Southern hemisphere witnessed the brilliant explosion of this star on Feb. 23, 1987. Shown in this NASA Hubble Space Telescope image, the supernova remnant, surrounded by inner and outer rings of material, is set in a forest of ethereal, diffuse clouds of gas. This three - color image is composed of several pictures of the supernova and its neighboring region taken with the Wide Field and Planetary Camera 2 in Sept. 1994, Feb. 1996 and July 1997. The many bright blue stars nearby the supernova are massive stars, each more than six times heftier than our Sun. With ages of about 12 million years old, they are members of the same generation of stars as the star that went supernova. The presence of bright gas clouds is another sign of

Supernova 1987A in the Great Magellan Cloud View by HST - Glittering stars and wisps of gas create a breathtaking backdrop for the self - destruction of a massive star, called supernova 1987A, in the Large Magellanic Cloud, a nearby galaxy. Astronomers in the Southern hemisphere witnessed the brilliant explosion of this star on Feb. 23, 1987. Shown in this NASA Hubble Space Telescope image, the supernova remnant, surrounded by inner and outer rings of material, is set in a forest of ethereal, diffuse clouds of gas. This three - color image is composed of several pictures of the supernova and its neighboring region taken with the Wide Field and Planetary Camera 2 in Sept. 1994, Feb. 1996 and July 1997. The many bright blue stars nearby the supernova are massive stars, each more than six times heftier than our Sun. With ages of about 12 million years old, they are members of the same generation of stars as the star that went supernova. The presence of bright gas clouds is another sign of

PIX4582360

Sirius A and Sirius B in the Big Dog - Sirius A and Sirius B in Canis Major - Sirius A and Sirius B in the Big Dog seen by the Hubble space telescope in February 2004. The brightest source in this image is Sirius A, the brightest star in the sky in visible light, here overexposed to his companion, Sirius B (lower left), a white dwarf star orbiting Sirius A in 50 years. Sirius is located 8.6 years of light from Earth. This Hubble Space Telescope image shows Sirius, the brightest star in our nighttime sky, along with its faint, tiny stellar companion, Sirius B. Astronomers overexposed the image of Sirius (at center) so that the dim Sirius B (tiny dot at lower left) could be seen. The cross - shaped diffraction spikes and concentric rings around Sirius, and the small ring around Sirius B, are artifacts produced within the telescope's imaging system. Sirius B is a white dwarf that orbits around Sirius every 50 years. Sirius, only 8.6 light - years from Earth, is the fifth closest star syst

Sirius A and Sirius B in the Big Dog - Sirius A and Sirius B in Canis Major - Sirius A and Sirius B in the Big Dog seen by the Hubble space telescope in February 2004. The brightest source in this image is Sirius A, the brightest star in the sky in visible light, here overexposed to his companion, Sirius B (lower left), a white dwarf star orbiting Sirius A in 50 years. Sirius is located 8.6 years of light from Earth. This Hubble Space Telescope image shows Sirius, the brightest star in our nighttime sky, along with its faint, tiny stellar companion, Sirius B. Astronomers overexposed the image of Sirius (at center) so that the dim Sirius B (tiny dot at lower left) could be seen. The cross - shaped diffraction spikes and concentric rings around Sirius, and the small ring around Sirius B, are artifacts produced within the telescope's imaging system. Sirius B is a white dwarf that orbits around Sirius every 50 years. Sirius, only 8.6 light - years from Earth, is the fifth closest star syst

PIX4571735

May 05, 1953 - LIFESAVER SARAH... SARAH - short for Search and Rescue and Homing - is a new radio device for saving air-crash survivors, shipwrecked seamen and stranded personnel in mountains, jungle and in desert. A radio beacon weighing only 20 ounces with a 32-ounce battery fitted to the survivor's life-jacket, transmits a signal to guide searching aircraft. The stranded man pulls a ring which releases a 31-inch flexible aerial and starts the transmitter. Transmission can be maintained for 20 hours with a maximum range of 66 miles to an aircraft at 10,000 feet. A distress signal at see can thus be picked up by an aircraft within an area of 10,000 square miles. The signals are displayed on a cathode ray tube in the rescuing aircraft. The rescuing craft then” homes” on to the signal which suddenly vanishes when the aircraft is above the stranded man. A two-way speech unit provides means of verbal communication in between rescuer and survivor at close range. Keystone Photo Shows: - On

May 05, 1953 - LIFESAVER SARAH... SARAH - short for Search and Rescue and Homing - is a new radio device for saving air-crash survivors, shipwrecked seamen and stranded personnel in mountains, jungle and in desert. A radio beacon weighing only 20 ounces with a 32-ounce battery fitted to the survivor's life-jacket, transmits a signal to guide searching aircraft. The stranded man pulls a ring which releases a 31-inch flexible aerial and starts the transmitter. Transmission can be maintained for 20 hours with a maximum range of 66 miles to an aircraft at 10,000 feet. A distress signal at see can thus be picked up by an aircraft within an area of 10,000 square miles. The signals are displayed on a cathode ray tube in the rescuing aircraft. The rescuing craft then” homes” on to the signal which suddenly vanishes when the aircraft is above the stranded man. A two-way speech unit provides means of verbal communication in between rescuer and survivor at close range. Keystone Photo Shows: - On

ZUM4842034

Singing-bird box, c.1840 (gold, diamonds & enamel)

Singing-bird box, c.1840 (gold, diamonds & enamel)

Bruguier, Charles (1788-1862)

CH3025207

Singing-bird box, c.1840 (gold, diamonds & enamel)

Singing-bird box, c.1840 (gold, diamonds & enamel)

Bruguier, Charles (1788-1862)

CH3025210

Ferry Carondolet (1473-1528) and his Secretary (after Sebastiano)

Ferry Carondolet (1473-1528) and his Secretary (after Sebastiano)

Piombo, Sebastiano del (S. Luciani) (c.1485-1547) (after)

USB1161108

Singing-bird box, c.1840 (gold, diamonds & enamel)

Singing-bird box, c.1840 (gold, diamonds & enamel)

Bruguier, Charles (1788-1862)

CH3025208

Interacting galaxies Arp 297 - Interacting galaxies Arp 297 - Arp 297 is located about 200 million light years away from Earth in the constellation Bovier. This pair of interacting galaxies consists of a large spiral galaxy, NGC 5754, and a small spiral galaxy, NGC 5752, at the bottom of the image. This interaction causes intense star flames within the small galaxy. Image obtained by the Hubble Space Telescope on March 14, 1999. This beautiful pair of interacting galaxies consists of NGC 5754, the large spiral on the right, and NGC 5752, the smaller companion in the bottom left corner of the image. NGC 5754's internal structure has hardly been disturbed by the interaction. The outer structure does exhibit tidal features, as does the symmetry of the inner spiral pattern and the kinked arms just beyond its inner ring. In contrast, NGC 5752 has undergone a starburst episode, with a rich population of massive and luminous star clusters clumping around the core and intertwined with intricat

Interacting galaxies Arp 297 - Interacting galaxies Arp 297 - Arp 297 is located about 200 million light years away from Earth in the constellation Bovier. This pair of interacting galaxies consists of a large spiral galaxy, NGC 5754, and a small spiral galaxy, NGC 5752, at the bottom of the image. This interaction causes intense star flames within the small galaxy. Image obtained by the Hubble Space Telescope on March 14, 1999. This beautiful pair of interacting galaxies consists of NGC 5754, the large spiral on the right, and NGC 5752, the smaller companion in the bottom left corner of the image. NGC 5754's internal structure has hardly been disturbed by the interaction. The outer structure does exhibit tidal features, as does the symmetry of the inner spiral pattern and the kinked arms just beyond its inner ring. In contrast, NGC 5752 has undergone a starburst episode, with a rich population of massive and luminous star clusters clumping around the core and intertwined with intricat

PIX4612781

Augustus Keppel, Viscount Keppel (1725-1786), early to mid 19th century (watercolour, bodycolour, ivory, wood, gilt)

Augustus Keppel, Viscount Keppel (1725-1786), early to mid 19th century (watercolour, bodycolour, ivory, wood, gilt)

Unknown Artist, (19th century)

MMM7340100

Singing-bird box, c.1840 (gold, diamonds & enamel)

Singing-bird box, c.1840 (gold, diamonds & enamel)

Bruguier, Charles (1788-1862)

CH3025209

Sigurd Cross Slab (Manx Cross 121) (stone)

Sigurd Cross Slab (Manx Cross 121) (stone)

MNX5934749

Space Exploration: Soyuz and Orion Ships - Artist's View - CEV-Soyuz Joint Mission - An American Orion ship mooring has a Soyuz TMA-M spaceship during a distant space exploration mission. Here, the ship is approaching a satellite stationed at a point in Lagrange. Illustration. An Orion class Crew Exploration Vehicle (AKA Deep Space Vehicle) is paired with a Soyuz TMA-M manned spacecraft for a joint deep space rendezvous with a satellite parked in a gravitationally stable Lagrangian point about 1 million miles beyond the orbit of the Earth's Moon. At this position, in this case a Lagrangian point 2, or L2, the Earth is between the spacecraft and the Sun resulting in the Earth eclipsing much of the Sun's light, however at this distance the Earth does not subtend an angle large enough to cover the entire disk of the Sun. What's visible of the Sun is a brilliant ring of light illuminating the spacecraft. (The streamers of light around the Sun are not the Sun's corona, but rather a way of i

Space Exploration: Soyuz and Orion Ships - Artist's View - CEV-Soyuz Joint Mission - An American Orion ship mooring has a Soyuz TMA-M spaceship during a distant space exploration mission. Here, the ship is approaching a satellite stationed at a point in Lagrange. Illustration. An Orion class Crew Exploration Vehicle (AKA Deep Space Vehicle) is paired with a Soyuz TMA-M manned spacecraft for a joint deep space rendezvous with a satellite parked in a gravitationally stable Lagrangian point about 1 million miles beyond the orbit of the Earth's Moon. At this position, in this case a Lagrangian point 2, or L2, the Earth is between the spacecraft and the Sun resulting in the Earth eclipsing much of the Sun's light, however at this distance the Earth does not subtend an angle large enough to cover the entire disk of the Sun. What's visible of the Sun is a brilliant ring of light illuminating the spacecraft. (The streamers of light around the Sun are not the Sun's corona, but rather a way of i

Walter B Myers

PIX4639150

Phaeton alarm'd, 1808 (etching)

Phaeton alarm'd, 1808 (etching)

Gillray, James (1757-1815)

MMM7340077

Aug 08, 1954 - Inquest In Film Star's Mother In-Law: In a London Coroner's Court today a man was asked:” Did you murder Mrs. McGrath”. The question put by Mr. Neville Stafford, the Westminster Coroner, came at the end of 60 minutes evidence by Walter Henry Hensby, 46-year old electrician. In a low voice, he replied:” No, sir” Hensby was giving evidence at the inquest on his friend, 64-year old Mrs. Violet McGrath, mother-in-law of film star Michael Rennie. She was found strangled in a South Kansington flat. Hensby, now living at Cricket-inll, Pately, near Cambarley, was said yesterday to have a healed scar on his right hand consistent with the measurement of a metal suspender clip and scartch marks consistent with being caused by fingernails. All, it was said in evidence could have been caused between 11 p.m. and midnight on Sunday, May 9, the night Mrs. McGrath died. Today, Hensby, as the coroner questioned him, said that he did not know where he got the scratch marks and the healed s

Aug 08, 1954 - Inquest In Film Star's Mother In-Law: In a London Coroner's Court today a man was asked:” Did you murder Mrs. McGrath”. The question put by Mr. Neville Stafford, the Westminster Coroner, came at the end of 60 minutes evidence by Walter Henry Hensby, 46-year old electrician. In a low voice, he replied:” No, sir” Hensby was giving evidence at the inquest on his friend, 64-year old Mrs. Violet McGrath, mother-in-law of film star Michael Rennie. She was found strangled in a South Kansington flat. Hensby, now living at Cricket-inll, Pately, near Cambarley, was said yesterday to have a healed scar on his right hand consistent with the measurement of a metal suspender clip and scartch marks consistent with being caused by fingernails. All, it was said in evidence could have been caused between 11 p.m. and midnight on Sunday, May 9, the night Mrs. McGrath died. Today, Hensby, as the coroner questioned him, said that he did not know where he got the scratch marks and the healed s

ZUM4939539

Charlotte Gilding, Lady Iliffe (1881 -1972)

Charlotte Gilding, Lady Iliffe (1881 -1972)

Jameson, Cecil Stuart (1883-c.1937)

USB1160671

Sigurd Cross Slab, c.1906 (ink & pencil on paper)

Sigurd Cross Slab, c.1906 (ink & pencil on paper)

Kermode, Philip Moore Callow (1855-1932)

MNX3594335

Sep. 09, 1954 - Demonstration of British military vehicles. first gas turbine powered track vehicle on show. A special and unique demonstration of British military vehicle was held at the fighting vehicles research and development establishment (F.V.R.D.E), at chertsey, surrey today. staged primarily to promote sales in this special channel of our export trade, the display included little short of 100 different vehicles giving an immense range of usage. load and personal carrying motor workshop lorries, mobile cranes, tankers triers up to 60 tons for tank transpiration, and even armored ears were among the exhibits to be seen either on the display center or taking part in spectacular demonstration of their qualities on test circuits. The event has been orgainsed jointly by the ministry of Supply, to who are calcification the vehicles are built and by the society of motor manufacturers and traders, certain of whose members are responsible for the carrying out of the production programme

Sep. 09, 1954 - Demonstration of British military vehicles. first gas turbine powered track vehicle on show. A special and unique demonstration of British military vehicle was held at the fighting vehicles research and development establishment (F.V.R.D.E), at chertsey, surrey today. staged primarily to promote sales in this special channel of our export trade, the display included little short of 100 different vehicles giving an immense range of usage. load and personal carrying motor workshop lorries, mobile cranes, tankers triers up to 60 tons for tank transpiration, and even armored ears were among the exhibits to be seen either on the display center or taking part in spectacular demonstration of their qualities on test circuits. The event has been orgainsed jointly by the ministry of Supply, to who are calcification the vehicles are built and by the society of motor manufacturers and traders, certain of whose members are responsible for the carrying out of the production programme

ZUM4941587

Barree spiral galaxy NGC 7098 - Barred spiral galaxy NGC 7098: The barree spiral galaxy NGC 7098 is located about 95 million light years away from Earth in the southern constellation of the octant. Image obtained by the Very Large Telescope (VLT). Approximately 95 million light-years away, in the southern constellation of Octans (The Octant), lies NGC 7098 - an intriguing spiral galaxy with numerous sets of double features. The first of NGC 7098's double features is a duo of distinct ring-like structures that loop around the galaxy's hazy heart. This central region hosts a second double feature: a double bar. NGC 7098 has also developed features known as ansae, visible as small, bright streaks at each end of the central region. Ansae are visible areas of overdensity - they commonly take looping, linear, or circular shapes, and can be found at the extremities of planetary ring systems, in nebulous clouds, and, as is the case with NGC 7098, in parts of galaxies that are packed to the bri

Barree spiral galaxy NGC 7098 - Barred spiral galaxy NGC 7098: The barree spiral galaxy NGC 7098 is located about 95 million light years away from Earth in the southern constellation of the octant. Image obtained by the Very Large Telescope (VLT). Approximately 95 million light-years away, in the southern constellation of Octans (The Octant), lies NGC 7098 - an intriguing spiral galaxy with numerous sets of double features. The first of NGC 7098's double features is a duo of distinct ring-like structures that loop around the galaxy's hazy heart. This central region hosts a second double feature: a double bar. NGC 7098 has also developed features known as ansae, visible as small, bright streaks at each end of the central region. Ansae are visible areas of overdensity - they commonly take looping, linear, or circular shapes, and can be found at the extremities of planetary ring systems, in nebulous clouds, and, as is the case with NGC 7098, in parts of galaxies that are packed to the bri

PIX4574313

Planetary nebula M57 (NGC 6720) in Lyra - M57 (NGC 6720) planetary nebula in Lyra - The planetary nebula of Lyra (M57) is located about 2000 years - light from Earth. With a magnitude of 9.0, this nebula is easily observed with a small telescope. A planetary nebula is a gas shell from a small late-life star whose heart collapsed to become a white dwarf and expelled the outer layers of its matter. Composite image obtained by different telescopes. The Ring Nebula, M57, is the most famous example of a planetary nebula. Located about 2,000 light years away, it has an apparent diameter of 1 arc minute and a real diameter of about one light year. At magnitude 9.0 its high surface brightness makes it an easy object, even from the city and even with small telescopes. Planetary nebula are shells of gas shed by stars late in their life cycles after using up all of their nuclear fuel. The star then ejects a significant portion of its mass in a gaseous shell, which is illuminated by its extremely

Planetary nebula M57 (NGC 6720) in Lyra - M57 (NGC 6720) planetary nebula in Lyra - The planetary nebula of Lyra (M57) is located about 2000 years - light from Earth. With a magnitude of 9.0, this nebula is easily observed with a small telescope. A planetary nebula is a gas shell from a small late-life star whose heart collapsed to become a white dwarf and expelled the outer layers of its matter. Composite image obtained by different telescopes. The Ring Nebula, M57, is the most famous example of a planetary nebula. Located about 2,000 light years away, it has an apparent diameter of 1 arc minute and a real diameter of about one light year. At magnitude 9.0 its high surface brightness makes it an easy object, even from the city and even with small telescopes. Planetary nebula are shells of gas shed by stars late in their life cycles after using up all of their nuclear fuel. The star then ejects a significant portion of its mass in a gaseous shell, which is illuminated by its extremely

PIX4623359

Onekotan volcanic island seen from space - Onekotan volcanic island seen from space - Onekotan Island is an uninhabited volcanic island north of the Kuril Islands chain (Russia). About 40 kilometres long, this island is home to two stratovolcanoes, on the right (north), the Nemo volcano, on the left (south), the Krenitsyn volcano with the caldera Tao - Rusyr. Image obtained from the International Space Station (ISS) on January 9, 2011. Snow cover highlights the calderas and volcanic cones that form the northern and southern ends of Onekotan Island, part of the Russian Federation in the western Pacific Ocean. Calderas are depressions formed when a volcano empties its magma chamber in an explosive eruption and then the overlaying material collapses into the evacuated space. In this astronaut photograph taken from the International Space Station (ISS) on January 9, 2011, the northern end of the island (image right) is dominated by the Nemo Peak volcano, which began forming within an older

Onekotan volcanic island seen from space - Onekotan volcanic island seen from space - Onekotan Island is an uninhabited volcanic island north of the Kuril Islands chain (Russia). About 40 kilometres long, this island is home to two stratovolcanoes, on the right (north), the Nemo volcano, on the left (south), the Krenitsyn volcano with the caldera Tao - Rusyr. Image obtained from the International Space Station (ISS) on January 9, 2011. Snow cover highlights the calderas and volcanic cones that form the northern and southern ends of Onekotan Island, part of the Russian Federation in the western Pacific Ocean. Calderas are depressions formed when a volcano empties its magma chamber in an explosive eruption and then the overlaying material collapses into the evacuated space. In this astronaut photograph taken from the International Space Station (ISS) on January 9, 2011, the northern end of the island (image right) is dominated by the Nemo Peak volcano, which began forming within an older

PIX4661424

Heitengi (Astronomical Volvelle), possibly Izumi province, southern Osaka, 1801 (colour woodblock print)

Heitengi (Astronomical Volvelle), possibly Izumi province, southern Osaka, 1801 (colour woodblock print)

Iwahashi Kobodo (fl.1801)

CH3281678

Louis XVI month-going mean and solar time mantel regulator with remontoire, 1778 (ormolu & enamel)

Louis XVI month-going mean and solar time mantel regulator with remontoire, 1778 (ormolu & enamel)

Coteau, Joseph (1740-1801) & Robin, Robert (1741-99)

CH3502610

Atafu Atoll - Tokelau Islands, South Pacific - Atafu Atoll, Tokelau, Southern Pacific Ocean - Atafu is a small atoll belonging to the Tokelau Archipelago, in the South Pacific Ocean. With an elevation of two metres above the water, this coral reef is still vulnerable to cyclones and to the rise of water due to global warming. At roughly eight kilometers wide, Atafu Atoll is the smallest of three atolls and one island (Nukunonu and Fakaofo Atoll to the southeast and Swains Island to the south are not shown) comprising the Tokelau Islands group located in the southern Pacific Ocean. The primary settlement on Atafu is a village located at the northwestern corner of the atoll - - indicated by an area of light gray dots in this astronaut photograph. The typical ring shape of the atoll is the result of coral reefs building up around a former volcanic island. Over geologic time, the central volcano has subsided beneath the water surface, leaving the fringing reefs and a central lagoon that co

Atafu Atoll - Tokelau Islands, South Pacific - Atafu Atoll, Tokelau, Southern Pacific Ocean - Atafu is a small atoll belonging to the Tokelau Archipelago, in the South Pacific Ocean. With an elevation of two metres above the water, this coral reef is still vulnerable to cyclones and to the rise of water due to global warming. At roughly eight kilometers wide, Atafu Atoll is the smallest of three atolls and one island (Nukunonu and Fakaofo Atoll to the southeast and Swains Island to the south are not shown) comprising the Tokelau Islands group located in the southern Pacific Ocean. The primary settlement on Atafu is a village located at the northwestern corner of the atoll - - indicated by an area of light gray dots in this astronaut photograph. The typical ring shape of the atoll is the result of coral reefs building up around a former volcanic island. Over geologic time, the central volcano has subsided beneath the water surface, leaving the fringing reefs and a central lagoon that co

PIX4675640

Louis XVI month-going mean and solar time mantel regulator with remontoire, 1778 (ormolu & enamel)

Louis XVI month-going mean and solar time mantel regulator with remontoire, 1778 (ormolu & enamel)

Coteau, Joseph (1740-1801) & Robin, Robert (1741-99)

CH3502612

Saturn seen by the Cassini probe on 23/07/2008 - Saturn seen by Cassini spacecraft on july 23 2008 - Saturn seen by the Cassini probe on 23 July 2008 at a distance of 1.1 million km from the planet. Mosaic of 30 images. Several satellites are visible in this image: Titan, Janus, Mimas, Pandora, Epimethee and Enceladus. As Saturn advances in its orbit toward equinox and the sun gradually moves northward on the planet, the motion of Saturn's ring shadows and the changing colors of its atmosphere continue to transform the face of Saturn as seen by Cassini. This captivating natural color view was created from images collected shortly after Cassini began its extended Equinox Mission in July 2008. This mosaic combines 30 images - - 10 each of red, green and blue light - - taken over the course of approximately two hours as Cassini panned its wide - angle camera across the entire planet and ring system on July 23, 2008, from a southerly elevation of 6 degrees. Six moons complete this construc

Saturn seen by the Cassini probe on 23/07/2008 - Saturn seen by Cassini spacecraft on july 23 2008 - Saturn seen by the Cassini probe on 23 July 2008 at a distance of 1.1 million km from the planet. Mosaic of 30 images. Several satellites are visible in this image: Titan, Janus, Mimas, Pandora, Epimethee and Enceladus. As Saturn advances in its orbit toward equinox and the sun gradually moves northward on the planet, the motion of Saturn's ring shadows and the changing colors of its atmosphere continue to transform the face of Saturn as seen by Cassini. This captivating natural color view was created from images collected shortly after Cassini began its extended Equinox Mission in July 2008. This mosaic combines 30 images - - 10 each of red, green and blue light - - taken over the course of approximately two hours as Cassini panned its wide - angle camera across the entire planet and ring system on July 23, 2008, from a southerly elevation of 6 degrees. Six moons complete this construc

PIX4625214

Louis XVI month-going mean and solar time mantel regulator with remontoire, 1778 (ormolu & enamel)

Louis XVI month-going mean and solar time mantel regulator with remontoire, 1778 (ormolu & enamel)

Coteau, Joseph (1740-1801) & Robin, Robert (1741-99)

CH3502609

Louis XVI month-going mean and solar time mantel regulator with remontoire, 1778 (ormolu & enamel)

Louis XVI month-going mean and solar time mantel regulator with remontoire, 1778 (ormolu & enamel)

Coteau, Joseph (1740-1801) & Robin, Robert (1741-99)

CH3502611

Tethys, Saturn satellite, seen by the Cassini probe - Saturn's moon Tethys seen by Cassini spacecraft: The Tethys satellite photographed by the Cassini probe on 11 April 2015 has a distance of 53,000 km from the satellite. Tethys is about 1070 km in diameter. - This enhancement-color mosaic of Saturn's icy moon Tethys shows a range of features on the moon's trailing hemisphere. Tethys is tidally locked to Saturn, so the trailing hemisphere is the side of the moon that always faces opposite its direction of motion as it orbits the planet - Images taken using clear, green, infrared and ultraviolet spectral filters were combined to create the view, which highlights subtle color differences across Tethys' surface at wavelengths not visible to human eyes. The moon's surface is fairly uniform in natural color - The color of the surface changes conspicuously across the disk, from yellowish hues to nearly white. These broad color changes are affected by a number of external processes. First, S

Tethys, Saturn satellite, seen by the Cassini probe - Saturn's moon Tethys seen by Cassini spacecraft: The Tethys satellite photographed by the Cassini probe on 11 April 2015 has a distance of 53,000 km from the satellite. Tethys is about 1070 km in diameter. - This enhancement-color mosaic of Saturn's icy moon Tethys shows a range of features on the moon's trailing hemisphere. Tethys is tidally locked to Saturn, so the trailing hemisphere is the side of the moon that always faces opposite its direction of motion as it orbits the planet - Images taken using clear, green, infrared and ultraviolet spectral filters were combined to create the view, which highlights subtle color differences across Tethys' surface at wavelengths not visible to human eyes. The moon's surface is fairly uniform in natural color - The color of the surface changes conspicuously across the disk, from yellowish hues to nearly white. These broad color changes are affected by a number of external processes. First, S

PIX4625625

marriage

marriage

IMO2037498

Stephen Gardiner (1483 1555), Bishop of Winchester

Stephen Gardiner (1483 1555), Bishop of Winchester

USB1157749

Capt. Offin Boardman, 1787 (oil on canvas)

Capt. Offin Boardman, 1787 (oil on canvas)

Gullager, Christian (1759-1826) (attr. to)

WAM3690704

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