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Immagini di 'Crescent' trovate, 2,197

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Silver mounted desk set of two polo ponys hooves, Captain J F Sherer, 1865 circa (silver)

Silver mounted desk set of two polo ponys hooves, Captain J F Sherer, 1865 circa (silver)

Indian School, (19th century)

NAM5924947

Silver mounted desk set of two polo ponys hooves, Captain J F Sherer, 1865 circa (silver)

Silver mounted desk set of two polo ponys hooves, Captain J F Sherer, 1865 circa (silver)

Indian School, (19th century)

NAM5924953

Silver mounted desk set of two polo ponys hooves, Captain J F Sherer, 1865 circa (silver)

Silver mounted desk set of two polo ponys hooves, Captain J F Sherer, 1865 circa (silver)

Indian School, (19th century)

NAM5924954

Silver mounted desk set of two polo ponys hooves, Captain J F Sherer, 1865 circa (silver)

Silver mounted desk set of two polo ponys hooves, Captain J F Sherer, 1865 circa (silver)

Indian School, (19th century)

NAM5924955

Infrared Jupiter seen by the New Horizons probe. - Jupiter seen by New Horizons spacecraft - View of Jupiter obtained on February 28, 2007 by the New Horizons probe. This infrared image shows the different altitudes of the Jovian clouds; in blue, the high altitudes clouds, in red, the lower clouds. Jupiter seen by New Horizons spacecraft during the Jupiter flyby in early 2007. This image is an infrared color composite taken by the spacecraft's near - infrared imaging spectrometer, the Linear Etalon Imaging Spectral Array (LEISA) at 1:40 UT on Feb. 28, 2007. The infrared wavelengths used (red: 1.59 um, green: 1.94 um, blue: 1.85 um) highlight variations in the altitude of the Jovian cloud tops, with blue denoting high - altitude clouds and hazes, and red indicating deeper clouds. The prominent bluish - white oval is the Great Red Spot. The observation was made at a solar phase angle of 75 degrees but has been projected onto a crescent to remove distortion caused by Jupiter's rotation du

Infrared Jupiter seen by the New Horizons probe. - Jupiter seen by New Horizons spacecraft - View of Jupiter obtained on February 28, 2007 by the New Horizons probe. This infrared image shows the different altitudes of the Jovian clouds; in blue, the high altitudes clouds, in red, the lower clouds. Jupiter seen by New Horizons spacecraft during the Jupiter flyby in early 2007. This image is an infrared color composite taken by the spacecraft's near - infrared imaging spectrometer, the Linear Etalon Imaging Spectral Array (LEISA) at 1:40 UT on Feb. 28, 2007. The infrared wavelengths used (red: 1.59 um, green: 1.94 um, blue: 1.85 um) highlight variations in the altitude of the Jovian cloud tops, with blue denoting high - altitude clouds and hazes, and red indicating deeper clouds. The prominent bluish - white oval is the Great Red Spot. The observation was made at a solar phase angle of 75 degrees but has been projected onto a crescent to remove distortion caused by Jupiter's rotation du

PIX4574942

A tower furnace enclosing two conjoined flasks that separate 'spiritus' (above) from 'anima' and 'corpus' (below); Latin verses on either side. - verse in English, in one stanza; beneath, a banded circle containing the signs of the zodiac, enclosing a sun and crescent moons and two dragons, each devoring the other's tail; inscriptions to the left and right and beneath. - a moon and a sun, both with human faces; between them, a cloud raining golden droplets upon a golden reclining male figure, from whose side a woman is emerging; on the left, a flowered bush, and on the right, a rose bush.

A tower furnace enclosing two conjoined flasks that separate 'spiritus' (above) from 'anima' and 'corpus' (below); Latin verses on either side. - verse in English, in one stanza; beneath, a banded circle containing the signs of the zodiac, enclosing a sun and crescent moons and two dragons, each devoring the other's tail; inscriptions to the left and right and beneath. - a moon and a sun, both with human faces; between them, a cloud raining golden droplets upon a golden reclining male figure, from whose side a woman is emerging; on the left, a flowered bush, and on the right, a rose bush.

BL3292663

China / Philippines: An aerial view of Chinese development on Woody Island in the disputed Paracel Islands, currently controlled by China and claimed by Taiwan and Vietnam, c. 2015

China / Philippines: An aerial view of Chinese development on Woody Island in the disputed Paracel Islands, currently controlled by China and claimed by Taiwan and Vietnam, c. 2015

PFH3085455

Nebula IC 1318 in the Swan - Gamma Cygnus, IC 1318, NGC 6888 - IC 1318 is a very extended emission nebula that surrounds the star Gamma Cygni (Sadr), visible towards the middle of the image. Lower right is the nebula NGC 6888 which surrounds a star Wolf - Rayet. This large area of emission nebulosity surrounds Sadr, Gamma Cygni, the brightest star in this photo and the heart of the constellation of Cygnus the Swan. Numerous star clusters can also be found embedded in the nebulosity. The two sections of nebulosity to the left of Sadr are called the Butterfly Nebula, and have the catalog designation of IC 1318. The large area of dark nebulosity that separates the two halves of the Butterfly is LDN 889, and B343 is the small but very dense dark nebula at the center right of the image. The small open cluster NGC 6910 is just above Sadr. The Crescent Nebula, NGC 6888, is at the lower right. The small patches of blue reflection nebulosity at top left are part of the NGC 6914/van den Berg 131

Nebula IC 1318 in the Swan - Gamma Cygnus, IC 1318, NGC 6888 - IC 1318 is a very extended emission nebula that surrounds the star Gamma Cygni (Sadr), visible towards the middle of the image. Lower right is the nebula NGC 6888 which surrounds a star Wolf - Rayet. This large area of emission nebulosity surrounds Sadr, Gamma Cygni, the brightest star in this photo and the heart of the constellation of Cygnus the Swan. Numerous star clusters can also be found embedded in the nebulosity. The two sections of nebulosity to the left of Sadr are called the Butterfly Nebula, and have the catalog designation of IC 1318. The large area of dark nebulosity that separates the two halves of the Butterfly is LDN 889, and B343 is the small but very dense dark nebula at the center right of the image. The small open cluster NGC 6910 is just above Sadr. The Crescent Nebula, NGC 6888, is at the lower right. The small patches of blue reflection nebulosity at top left are part of the NGC 6914/van den Berg 131

Jerry Lodriguss

PIX4622203

Martian dunes in summer - Mars: Summer view of Dunes: Detail on dunes near the northern polar cap of Mars in summer. Image obtained by the HIRISE camera of the Mars Reconnaissance probe orbiter on 1 September 2008. HIRISE is a 50 cm telescope that observes visible and near infrared. This dune field formed near the base of the North Polar cap. Dunes require a source of loose particulate material to form. The source of the northern dune fields around the polar cap may be from the layers of dusty ice that are eroded by strong polar winds. This image was taken during the Martian northern summer, so there is no frost present on the dunes. The dunes closest to the base of the polar cap are long and parallel, indicating strong winds from the direction of the cap. As they get farther away from the polar cap, they start to form more crescent shaped dunes, called barchan dunes. Repeated observations by HiRise of dunes like these show measurable changes in some locations. This discovery adds to t

Martian dunes in summer - Mars: Summer view of Dunes: Detail on dunes near the northern polar cap of Mars in summer. Image obtained by the HIRISE camera of the Mars Reconnaissance probe orbiter on 1 September 2008. HIRISE is a 50 cm telescope that observes visible and near infrared. This dune field formed near the base of the North Polar cap. Dunes require a source of loose particulate material to form. The source of the northern dune fields around the polar cap may be from the layers of dusty ice that are eroded by strong polar winds. This image was taken during the Martian northern summer, so there is no frost present on the dunes. The dunes closest to the base of the polar cap are long and parallel, indicating strong winds from the direction of the cap. As they get farther away from the polar cap, they start to form more crescent shaped dunes, called barchan dunes. Repeated observations by HiRise of dunes like these show measurable changes in some locations. This discovery adds to t

PIX4580056

Spiral galaxy NGC 4651 in Berenice's Hair - Spiral galaxy NGC 4651 in Coma Berenices - The galaxy NGC 4651 (Arp 189) is located about 50 million years away - light from Earth. The Umbrella Galaxy (NGC 4651 or Arp 189) exhibits a jet like spear that's strikingly coherent and narrow. The structure was previously reported by Boris Vorontsov Velyaminov in 1959 but never interpreted as a stellar tidal stream. This deep image additionally shows a spectacular crescent shaped shell surrounding the east side of the star system that corresponds to the apocenter of the dwarf galaxy. Interestingly, a possible second arc on the western side of the galaxy can also be seen in this image. This feature is less obvious because it's partially hidden by the galaxy's disk and suggests we are observing a moderately inclined structure projected into the halo of NGC 4651. This image was produced by combining an hour of exposure through the Isaac Newton Telescope, located on the Spanish island of La Palma, wit

Spiral galaxy NGC 4651 in Berenice's Hair - Spiral galaxy NGC 4651 in Coma Berenices - The galaxy NGC 4651 (Arp 189) is located about 50 million years away - light from Earth. The Umbrella Galaxy (NGC 4651 or Arp 189) exhibits a jet like spear that's strikingly coherent and narrow. The structure was previously reported by Boris Vorontsov Velyaminov in 1959 but never interpreted as a stellar tidal stream. This deep image additionally shows a spectacular crescent shaped shell surrounding the east side of the star system that corresponds to the apocenter of the dwarf galaxy. Interestingly, a possible second arc on the western side of the galaxy can also be seen in this image. This feature is less obvious because it's partially hidden by the galaxy's disk and suggests we are observing a moderately inclined structure projected into the halo of NGC 4651. This image was produced by combining an hour of exposure through the Isaac Newton Telescope, located on the Spanish island of La Palma, wit

R. Jay GaBany

PIX4611786

Lyon Astronomical Clock - Astronomical clock in Lyon - France - L'Astrolabe The outer circle allows you to know the time. It is divided into 2 parts of 12 Roman numerals (noon at the top, midnight at the bottom). The time is indicated by the alidade ending with a fleur-de-lis (here, 12:25). The crescent has the opposite is only a counterweight. Then we find the calendar with the days of the week as well as the months in Latin. The inner circle represents the zodiac, with the 12 signs. In the central part, the Sun moves over the ecliptic circle during the year. Inside the latter, the circle of the Moon and its phases (here in the last quarter). In the background, the map of the sky. Located in the Cathedrale Saint John, the clock dates back to 1379. Writings witness his presence in the cathedrale since 1383, making it one of the oldest astronomical clocks in Europe. It consists of a 1.80m square tower, surmounted by an octagonal turret presenting the automatons and a dome supporting a r

Lyon Astronomical Clock - Astronomical clock in Lyon - France - L'Astrolabe The outer circle allows you to know the time. It is divided into 2 parts of 12 Roman numerals (noon at the top, midnight at the bottom). The time is indicated by the alidade ending with a fleur-de-lis (here, 12:25). The crescent has the opposite is only a counterweight. Then we find the calendar with the days of the week as well as the months in Latin. The inner circle represents the zodiac, with the 12 signs. In the central part, the Sun moves over the ecliptic circle during the year. Inside the latter, the circle of the Moon and its phases (here in the last quarter). In the background, the map of the sky. Located in the Cathedrale Saint John, the clock dates back to 1379. Writings witness his presence in the cathedrale since 1383, making it one of the oldest astronomical clocks in Europe. It consists of a 1.80m square tower, surmounted by an octagonal turret presenting the automatons and a dome supporting a r

Sebastien Beaucourt

PIX4586006

Saturn view of Enceladus - Illustration - Saturn from the surface of Enceladus - The planet Saturn seen from the ice surface of Enceladus. This is how Saturn may appear from the icy surface of Enceladus, one of Saturn's eight major satellites. At a distance of 148 thousand miles, Saturn would subtend an angle of 29o in Enceladus' sky, about the same width as 58 Earth moon's lined up side - by - side. While the surface of Enceladus is as reflective as new fallen snow, it would probably appear leaden about an hour before sunrise with a crescent Saturn as the only source of illumination. Like all of Saturn's major satellites, Enceladus always keeps the same side facing its host planet. From the perspective of a stationary observer on Enceladus, Saturn would always appear in the same position in the sky, cycling through its phases in about one - and - half Earth days. This image also illustrates a phenomenon only recently discovered by Nasa's Cassini probe: sunlight reflecting off of Satur

Saturn view of Enceladus - Illustration - Saturn from the surface of Enceladus - The planet Saturn seen from the ice surface of Enceladus. This is how Saturn may appear from the icy surface of Enceladus, one of Saturn's eight major satellites. At a distance of 148 thousand miles, Saturn would subtend an angle of 29o in Enceladus' sky, about the same width as 58 Earth moon's lined up side - by - side. While the surface of Enceladus is as reflective as new fallen snow, it would probably appear leaden about an hour before sunrise with a crescent Saturn as the only source of illumination. Like all of Saturn's major satellites, Enceladus always keeps the same side facing its host planet. From the perspective of a stationary observer on Enceladus, Saturn would always appear in the same position in the sky, cycling through its phases in about one - and - half Earth days. This image also illustrates a phenomenon only recently discovered by Nasa's Cassini probe: sunlight reflecting off of Satur

Walter B Myers

PIX4625835

Earth's atmosphere and night clouds - Earth's atmosphere, noctilucent clouds and Moon - View of the Earth's atmosphere and a crescent moon photographs from the International Space Station on July 27, 2003. Night clouds are also visible. These clouds look like cirrus but are much higher, between 75 and 90 km from the Earth's surface. Noctilucent clouds are very high clouds that look like cirrus clouds, but are much higher (75 - 90 km above the Earth's surface) than clouds that we observe every day. They are optically thin and can only be observed during twilight hours, when the sun is just below the horizon and only shines on the uppermost atmosphere. In this image, the limb of the Earth at the bottom transitions into the orange - colored troposphere, the lowest and most dense portion of the Earth's atmosphere. The troposphere ends abruptly at the tropopause, which appears in the image as the sharp boundary between the orange - and blue - colored atmosphere. The silvery - blue noctiluce

Earth's atmosphere and night clouds - Earth's atmosphere, noctilucent clouds and Moon - View of the Earth's atmosphere and a crescent moon photographs from the International Space Station on July 27, 2003. Night clouds are also visible. These clouds look like cirrus but are much higher, between 75 and 90 km from the Earth's surface. Noctilucent clouds are very high clouds that look like cirrus clouds, but are much higher (75 - 90 km above the Earth's surface) than clouds that we observe every day. They are optically thin and can only be observed during twilight hours, when the sun is just below the horizon and only shines on the uppermost atmosphere. In this image, the limb of the Earth at the bottom transitions into the orange - colored troposphere, the lowest and most dense portion of the Earth's atmosphere. The troposphere ends abruptly at the tropopause, which appears in the image as the sharp boundary between the orange - and blue - colored atmosphere. The silvery - blue noctiluce

PIX4675194

Shoulder headdress (Zigiren-wunde), possibly Baga, late 19th-early 20th century (wood & metal)

Shoulder headdress (Zigiren-wunde), possibly Baga, late 19th-early 20th century (wood & metal)

TBM3708323

A burst of flame and on either side a lion salient before a wall, and two scrolls ('The mouth of the Collorick beware' and 'Heare is the last of the red stone and the beginning to put away the dead the elixir vita'). A sun above a crowned male Bird of Hermes, standing on a dark, sea-filled orb and surrounded by droplets of fire; the border of the orb is inscribed with the words 'aquila anima spiritus' in various combinations, and is stuck with eight feathers. A large scroll bearing verses in two stanzas. A scroll bearing an inscription ('The Red Sea, The Red Sol, The Red Elixir Vitae'), above a yellow sun containing three interlinked orbs (red, white and black). A crescent moon, being bitten by a large brown dragon, beneath.

A burst of flame and on either side a lion salient before a wall, and two scrolls ('The mouth of the Collorick beware' and 'Heare is the last of the red stone and the beginning to put away the dead the elixir vita'). A sun above a crowned male Bird of Hermes, standing on a dark, sea-filled orb and surrounded by droplets of fire; the border of the orb is inscribed with the words 'aquila anima spiritus' in various combinations, and is stuck with eight feathers. A large scroll bearing verses in two stanzas. A scroll bearing an inscription ('The Red Sea, The Red Sol, The Red Elixir Vitae'), above a yellow sun containing three interlinked orbs (red, white and black). A crescent moon, being bitten by a large brown dragon, beneath.

BL3292652

Viscount Horatio Nelson (1758-1805), before the Battle of Trafalgar, 21 October 1805, c.1854 (oil on canvas)

Viscount Horatio Nelson (1758-1805), before the Battle of Trafalgar, 21 October 1805, c.1854 (oil on canvas)

Lucy, Charles (1814-73) (after)

MMM7339092

Lady Mary Herbert, Vicountess Molyneux, Vicountess Montagu and Lady Maxwell (1659-1744), as Diana

Lady Mary Herbert, Vicountess Molyneux, Vicountess Montagu and Lady Maxwell (1659-1744), as Diana

Troy, Francois de (1645-1730)

USB1162035

Japet, satellite of Saturn, seen by Cassini - Crescent of Iapetus seen by Cassini spacecraft. - Mosaic in fake colors of Japet, a satellite of 1436 kilometers in diameter, taken by the Cassini probe on 10 September 2007 has a distance of 83 000 km from the satellite. Iapetus, 1,468 kilometers (912 miles) across, seen here in false color, is unique in its dramatic variation in brightness between the northern polar region and the middle and low latitudes. Equally prominent is the moon's equatorial ridge of towering mountains. The profile of the ridge against the darkness of space reveals that it is topped by a cratered plateau approximately 15 kilometers (9 miles) wide. Further west, the profile of the ridge changes from a long plateau to discrete peaks. The mosaic consists of four image footprints across the surface of Iapetus and has a resolution of 489 meters (0.3 miles) per pixel. The color seen in this view represents an expansion of the wavelength region of the electromagnetic spec

Japet, satellite of Saturn, seen by Cassini - Crescent of Iapetus seen by Cassini spacecraft. - Mosaic in fake colors of Japet, a satellite of 1436 kilometers in diameter, taken by the Cassini probe on 10 September 2007 has a distance of 83 000 km from the satellite. Iapetus, 1,468 kilometers (912 miles) across, seen here in false color, is unique in its dramatic variation in brightness between the northern polar region and the middle and low latitudes. Equally prominent is the moon's equatorial ridge of towering mountains. The profile of the ridge against the darkness of space reveals that it is topped by a cratered plateau approximately 15 kilometers (9 miles) wide. Further west, the profile of the ridge changes from a long plateau to discrete peaks. The mosaic consists of four image footprints across the surface of Iapetus and has a resolution of 489 meters (0.3 miles) per pixel. The color seen in this view represents an expansion of the wavelength region of the electromagnetic spec

PIX4625407

Union Flag made at Chitral during the siege, 1895 (fabric)

Union Flag made at Chitral during the siege, 1895 (fabric)

British School, (19th century)

NAM5926633

Attic red-figured bell-krater, c.410-400 BC (ceramic)

Attic red-figured bell-krater, c.410-400 BC (ceramic)

Nikias Painter (fl.c.420-c.400 BC) (attr. to)

CH3619102

Destruction of the American Fleet at Penobscot Bay, 14 August 1779, 1780s (oil on canvas)

Destruction of the American Fleet at Penobscot Bay, 14 August 1779, 1780s (oil on canvas)

Serres, Dominic (1722-93)

MMM7337659

Union Flag made at Chitral during the siege, 1895 (fabric)

Union Flag made at Chitral during the siege, 1895 (fabric)

British School, (19th century)

NAM5926634

Collection of snuff boxes (enamel, gold & tortoiseshell)

Collection of snuff boxes (enamel, gold & tortoiseshell)

European School

CH3025206

Vice-Admiral Horatio Nelson (1758-1805), 1894 (coloured lithograph, oil on canvas)

Vice-Admiral Horatio Nelson (1758-1805), 1894 (coloured lithograph, oil on canvas)

Abbott, Lemuel Francis (c.1760-1803) (after)

MMM7342309

Action between the Dutch fleet and barbary pirates, c.1670 (oil painting)

Action between the Dutch fleet and barbary pirates, c.1670 (oil painting)

Verschuier, Lieve (1630-86)

MMM7337743

Star T - Tauri in Orion - Bow Shock around T - Tauri Star in the Orion Nebula - LL Ori is a star T - Tauri located about 1500 years ago - light from Earth in Orion's nebula. This young star emits a powerful stellar wind that hits the surrounding gas creating an arc-shaped shock wave Image obtained by the Hubble space telescope in February 1995. A bow shock can be created in space when two streams of gas collide. The star LL Ori emits a vigorous solar wind, a stream of charged particles moving rapidly outward from the star. Our own Sun has a less energetic version of this wind that is responsible for auroral displays on the Earth. The material in the fast wind from LL Ori collides with slow - moving gas evaporating away from the center of the Orion Nebula, which is located to the lower right in this Heritage image. The surface where the two winds collide is the crescent - shaped bow shock seen in the image. Unlike a water wave made by a ship, this interstellar bow shock is a three - dim

Star T - Tauri in Orion - Bow Shock around T - Tauri Star in the Orion Nebula - LL Ori is a star T - Tauri located about 1500 years ago - light from Earth in Orion's nebula. This young star emits a powerful stellar wind that hits the surrounding gas creating an arc-shaped shock wave Image obtained by the Hubble space telescope in February 1995. A bow shock can be created in space when two streams of gas collide. The star LL Ori emits a vigorous solar wind, a stream of charged particles moving rapidly outward from the star. Our own Sun has a less energetic version of this wind that is responsible for auroral displays on the Earth. The material in the fast wind from LL Ori collides with slow - moving gas evaporating away from the center of the Orion Nebula, which is located to the lower right in this Heritage image. The surface where the two winds collide is the crescent - shaped bow shock seen in the image. Unlike a water wave made by a ship, this interstellar bow shock is a three - dim

PIX4572363

Jupiter and Io seen by the New Horizons probe

Jupiter and Io seen by the New Horizons probe

PIX4574952

Royal Naval uniform: pattern 1795-1812, Nelson's Trafalgar coat, c.1805 (wool, silk, brass, metal thread, gold alloy)

Royal Naval uniform: pattern 1795-1812, Nelson's Trafalgar coat, c.1805 (wool, silk, brass, metal thread, gold alloy)

Unknown Artist, (19th century)

MMM7340662

The Alps seen by satellite Envisat - The Alps as seen from satellite Envisat - Les Alpes seen by satellite ENVISAT on 8 December 2008. The snow - capped, crescent - shaped Alps and Italy's Apennines mountain chain are shown in this Envisat image. Snowfall in early winter - for meteorologists winter begins on the 1 December - covered the whole mountain areas with fresh snow, while the lower lands in the south and north of the mountains remained snow - free. Due to this snow cover and a relatively low illumination angle of the sun, the ranges and valleys of the mountains stand out in the image. Much of the whiteness seen in the top of the image is cloud cover, but fog is visible in the valleys such as the Rhine. The Alps - central Europe's major mountain range - extend some 1,200 km through France, Switzerland, Italy and Austria and down through Slovenia, Croatia, Bosnia and Herzegovina, Serbia and Montenegro and Albania as the Dinaric Alps. The Alps occupy an area of about 200,000 km an

The Alps seen by satellite Envisat - The Alps as seen from satellite Envisat - Les Alpes seen by satellite ENVISAT on 8 December 2008. The snow - capped, crescent - shaped Alps and Italy's Apennines mountain chain are shown in this Envisat image. Snowfall in early winter - for meteorologists winter begins on the 1 December - covered the whole mountain areas with fresh snow, while the lower lands in the south and north of the mountains remained snow - free. Due to this snow cover and a relatively low illumination angle of the sun, the ranges and valleys of the mountains stand out in the image. Much of the whiteness seen in the top of the image is cloud cover, but fog is visible in the valleys such as the Rhine. The Alps - central Europe's major mountain range - extend some 1,200 km through France, Switzerland, Italy and Austria and down through Slovenia, Croatia, Bosnia and Herzegovina, Serbia and Montenegro and Albania as the Dinaric Alps. The Alps occupy an area of about 200,000 km an

PIX4665079

Pluto seen by the New Horizons probe - Pluto seen by New Horizons - Pluto's atmosphere seen by the New Horizons probe. Image obtained on July 14, 2015 at a distance of 200,000 km from the dwarf planet. Mosaic of six images. This is the high-resolution color departure shot of Pluto's receding crescent from Nasa's New Horizons spacecraft, taken when the spacecraft was 120,000 miles (200,000 kilometers) away from Pluto. Shown in approximate true color, the picture was constructed from a mosaic of six black-and-white images from the Long Range Reconnaissance Imager (LORRI), with color added from a lower resolution Ralph/Multispectral Visible Imaging Camera (MVIC) color image, all acquired between 15:20 and 15:45 UT - about 3.5 hours after closest approach to Pluto - on July 14, 2015. The resolution of the LORRI images is about 0.6 miles (1 kilometer) per pixel; the sun illuminates the scene from the other side of Pluto and somewhat towards the top of this image. The image is dominated by s

Pluto seen by the New Horizons probe - Pluto seen by New Horizons - Pluto's atmosphere seen by the New Horizons probe. Image obtained on July 14, 2015 at a distance of 200,000 km from the dwarf planet. Mosaic of six images. This is the high-resolution color departure shot of Pluto's receding crescent from Nasa's New Horizons spacecraft, taken when the spacecraft was 120,000 miles (200,000 kilometers) away from Pluto. Shown in approximate true color, the picture was constructed from a mosaic of six black-and-white images from the Long Range Reconnaissance Imager (LORRI), with color added from a lower resolution Ralph/Multispectral Visible Imaging Camera (MVIC) color image, all acquired between 15:20 and 15:45 UT - about 3.5 hours after closest approach to Pluto - on July 14, 2015. The resolution of the LORRI images is about 0.6 miles (1 kilometer) per pixel; the sun illuminates the scene from the other side of Pluto and somewhat towards the top of this image. The image is dominated by s

PIX4582251

(Fourth section): An orange sun with a human face; beneath, three animals: to the left, a red lion, affronté , a white eagle perching on its head and holding a horseshoe in its beak; in the centre, a red lion, affronté , a cockatrice perching on its head; to the right, a green lion, affronté , a crow perching on its head and holding a horseshoe in its beak. - from the belly of the red lion, a red strand is descending into a large flask; around it, eleven suns (to the left) and eleven moons (to the right), each with a human face, all enclosed by another black-, white- and green-banded crescent moon. - a crowned figure with a red mantle, holding in his right hand a sun caduceus or wand (a serpent is entwined around his arm), and holding in his left hand a moon caduceus; he has seven feet and is standing atop a blank pedestal, to the left of which is standing a pilgrim with a crutch and forked staff (a horseshoe dangling from the fork), and to right a crowned and mitred figure holding a s

(Fourth section): An orange sun with a human face; beneath, three animals: to the left, a red lion, affronté , a white eagle perching on its head and holding a horseshoe in its beak; in the centre, a red lion, affronté , a cockatrice perching on its head; to the right, a green lion, affronté , a crow perching on its head and holding a horseshoe in its beak. - from the belly of the red lion, a red strand is descending into a large flask; around it, eleven suns (to the left) and eleven moons (to the right), each with a human face, all enclosed by another black-, white- and green-banded crescent moon. - a crowned figure with a red mantle, holding in his right hand a sun caduceus or wand (a serpent is entwined around his arm), and holding in his left hand a moon caduceus; he has seven feet and is standing atop a blank pedestal, to the left of which is standing a pilgrim with a crutch and forked staff (a horseshoe dangling from the fork), and to right a crowned and mitred figure holding a s

BL3292677

A large figure, most likely representing Hermes Trismegistus; at his head, a scroll bearing an inscription ('Est lapis occultus secreto fonte sepultus; he is embracing a large, stoppered flask (the arms of which bear writing), which contains a black frog, feathers and tadpoles or droplets of liquid at the top, and eight roundels, seven of which are connected to a central roundel by gold bands, which represent stages in the alchemical process. Seven of the roundels depict figures conducting alchemical experiments involving a large flask containing homunculi atop a furnace; the eighth (detached) roundel contains a sun and moon, corresponding silver and gold figures (Adam and Eve beside the Tree of Knowledge, around which a serpent is entwined), and two figures dressed in red robes wielding tools. The central roundel depicts two men holding a large book, to which the connecting bands are attached. All of the roundels contain inscriptions around their borders. a title 'An Alkemye Scrowle,

A large figure, most likely representing Hermes Trismegistus; at his head, a scroll bearing an inscription ('Est lapis occultus secreto fonte sepultus; he is embracing a large, stoppered flask (the arms of which bear writing), which contains a black frog, feathers and tadpoles or droplets of liquid at the top, and eight roundels, seven of which are connected to a central roundel by gold bands, which represent stages in the alchemical process. Seven of the roundels depict figures conducting alchemical experiments involving a large flask containing homunculi atop a furnace; the eighth (detached) roundel contains a sun and moon, corresponding silver and gold figures (Adam and Eve beside the Tree of Knowledge, around which a serpent is entwined), and two figures dressed in red robes wielding tools. The central roundel depicts two men holding a large book, to which the connecting bands are attached. All of the roundels contain inscriptions around their borders. a title 'An Alkemye Scrowle,

BL3292641

The Churning of the Ocean of Milk, c.1825 (opaque w/c & gold on paper)

The Churning of the Ocean of Milk, c.1825 (opaque w/c & gold on paper)

Indian School, (19th century)

SD5863973

Astrolabe, c.1570 (gilt brass)

Astrolabe, c.1570 (gilt brass)

Flemish School, (16th century)

CH3057865

The Republican Court (Lady Washington's Reception) 1861 (oil on canvas)

The Republican Court (Lady Washington's Reception) 1861 (oil on canvas)

Huntington, Daniel (1816-1906)

TBM143859

The Prince of Wales at Cowes, Arrival of the Prince on Saturday Evening, 30 July, Royal Salute by HMS "Crescent," Captain the Duke of York (litho)

The Prince of Wales at Cowes, Arrival of the Prince on Saturday Evening, 30 July, Royal Salute by HMS "Crescent," Captain the Duke of York (litho)

Lacy, Charles John de (c.1860-1936) (after)

LIP1606329

Types of the British Navy (litho)

Types of the British Navy (litho)

Wright, Henry Charles Seppings (1850-1937)

LIP1615850

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