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Japan: Bugaku mask of the Chikyu type, painted wood, c. 16th - 18th century, Tokyo National Museum

Japan: Bugaku mask of the Chikyu type, painted wood, c. 16th - 18th century, Tokyo National Museum

PFH3122376

The Seilern Triptych - The Entombment, c.1425 (paint, gold leaf on panel)

The Seilern Triptych - The Entombment, c.1425 (paint, gold leaf on panel)

Master of Flemalle, (Robert Campin) (1375/8-1444) (attr.to)

COU5892279

Calligraphic manuscript, Augsburg, c.1720-30 (pen & ink on paper)

Calligraphic manuscript, Augsburg, c.1720-30 (pen & ink on paper)

German School, (18th century)

CH2921860

Japan: A young woman in Bugaku costume. Bugaku performers are always male, so this was certainly a studio photograph, hand-coloured albumen silver print, 1880s.

Japan: A young woman in Bugaku costume. Bugaku performers are always male, so this was certainly a studio photograph, hand-coloured albumen silver print, 1880s.

PFH3122392

Belt Buckle, c.525-560 (bronze with garnets, glass, mother of pearl, gold foil, traces of gilding; bronze and glass)

Belt Buckle, c.525-560 (bronze with garnets, glass, mother of pearl, gold foil, traces of gilding; bronze and glass)

Visigothic (6th century AD)

XCL500298

Elliptical galaxy NGC 1275 in Perseus

Elliptical galaxy NGC 1275 in Perseus

PIX5620129

Tomb of the Emperor Akbur at Secundra (w/c and ink on paper)

Tomb of the Emperor Akbur at Secundra (w/c and ink on paper)

XCF276479

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

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

Markarian Galaxy 273 - Galaxy Markarian 273 - The Markarian galaxy 273 is about 500 million light years away from Earth in the constellation of the Great Bear. The presence of a 130,000-year-long maree tail suggests that Markarian 273 is the fusion of two galaxies. The collision caused a burst of star formations. This galaxy has a double core and is one of the brightest infrared galaxies. Image obtained by the Hubble Space Telescope on November 16, 2001. Markarian 273 shows an intricate central region and a striking tail that extends diagonally towards the bottom - right of the image. The tail is about 130 thousand light - years long and is strongly indicative of a merger between two galaxies. Markarian 273 has an intense region of starburst, where 60 solar masses of new stars are born each year. Near - infrared observations reveal a nucleus with two components. Markarian 273 is one of the most luminous galaxies when observed in the infrared, and is located 500 million light - years aw

Markarian Galaxy 273 - Galaxy Markarian 273 - The Markarian galaxy 273 is about 500 million light years away from Earth in the constellation of the Great Bear. The presence of a 130,000-year-long maree tail suggests that Markarian 273 is the fusion of two galaxies. The collision caused a burst of star formations. This galaxy has a double core and is one of the brightest infrared galaxies. Image obtained by the Hubble Space Telescope on November 16, 2001. Markarian 273 shows an intricate central region and a striking tail that extends diagonally towards the bottom - right of the image. The tail is about 130 thousand light - years long and is strongly indicative of a merger between two galaxies. Markarian 273 has an intense region of starburst, where 60 solar masses of new stars are born each year. Near - infrared observations reveal a nucleus with two components. Markarian 273 is one of the most luminous galaxies when observed in the infrared, and is located 500 million light - years aw

PIX4613690

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

Facade of the prefecture of Montpellier, France, Place des Martyrs de la Résistance, Prefecture de l'Herault, It is one of the main tourist attractions in Montpellier, The Prefecture, Montpellier, which dates back to the 19th century will give you pure tourism pleasure with its arched architecture and intricate design, The Prefecture, Montpellier also has the added advantage of having excellent transport facilities, along with accommodation facilities that guarantee the comfort and ease of tourists, The facade of the Prefecture, Montpellier, as mentioned is a creation of the 19th century, Data on Montpellier inform that the structure is seen along the Resistance Place the martyrs of the des, In 1718, the Prefecture, Montpellier, which had previously occupied the site of the evening Ganges Hotel, became the Hotel de l'Intendencia in 1718, 2020 (photo)

Facade of the prefecture of Montpellier, France, Place des Martyrs de la Résistance, Prefecture de l'Herault, It is one of the main tourist attractions in Montpellier, The Prefecture, Montpellier, which dates back to the 19th century will give you pure tourism pleasure with its arched architecture and intricate design, The Prefecture, Montpellier also has the added advantage of having excellent transport facilities, along with accommodation facilities that guarantee the comfort and ease of tourists, The facade of the Prefecture, Montpellier, as mentioned is a creation of the 19th century, Data on Montpellier inform that the structure is seen along the Resistance Place the martyrs of the des, In 1718, the Prefecture, Montpellier, which had previously occupied the site of the evening Ganges Hotel, became the Hotel de l'Intendencia in 1718, 2020 (photo)

Sergi Reboredo

SRB6367756

Galaxies clusters Abell 370 - Abell 370 cluster of galaxies with gravitational arcs - This cluster of galaxies is located about 5 billion years away from Earth. This image obtained by the Hubble Space Telescope on July 16, 2009 shows gravitational arcs among galaxies. These mirages are deformed images of farther galaxies located behind the cluster. The NASA/ESA Hubble Space Telescope's newly repaired Advanced Camera for Surveys (ACS) has peered across almost five billion light - years to resolve intricate details in the galaxy cluster Abell 370. Abell 370 is one of the very first galaxy clusters where astronomers observed the phenomenon of gravitational lensing, the warping of space - time by the cluster's gravitational field that distorts the light from galaxies lying far behind it. This is manifested as arcs and streaks in the picture, which are the stretched images of background galaxies. Gravitational lensing is a vital tool for astronomers when measuring the dark matter distributi

Galaxies clusters Abell 370 - Abell 370 cluster of galaxies with gravitational arcs - This cluster of galaxies is located about 5 billion years away from Earth. This image obtained by the Hubble Space Telescope on July 16, 2009 shows gravitational arcs among galaxies. These mirages are deformed images of farther galaxies located behind the cluster. The NASA/ESA Hubble Space Telescope's newly repaired Advanced Camera for Surveys (ACS) has peered across almost five billion light - years to resolve intricate details in the galaxy cluster Abell 370. Abell 370 is one of the very first galaxy clusters where astronomers observed the phenomenon of gravitational lensing, the warping of space - time by the cluster's gravitational field that distorts the light from galaxies lying far behind it. This is manifested as arcs and streaks in the picture, which are the stretched images of background galaxies. Gravitational lensing is a vital tool for astronomers when measuring the dark matter distributi

PIX4565651

Ceremonial Cross of Countess Gertrude, Lower Saxony, c.1038, Reliquary Bag, 1200s and Ceremonial Cross of Count Liudolf, shortly after 1038 (mixed media)

Ceremonial Cross of Countess Gertrude, Lower Saxony, c.1038, Reliquary Bag, 1200s and Ceremonial Cross of Count Liudolf, shortly after 1038 (mixed media)

European School

XCL491168

The Happy Instruments of Englands Preservation, published by Benjamin Combe after Francis Barlow, April 1681 (engraving)

The Happy Instruments of Englands Preservation, published by Benjamin Combe after Francis Barlow, April 1681 (engraving)

Barlow, Francis (1626-1702) (after)

XJF884282

Chliara cresus, Croesus Prominent, mounted male moth, an exquisite croesus prominent moth, patterned network of dark brown lines and golden brown scales, striking pale hindwings (photo)

Chliara cresus, Croesus Prominent, mounted male moth, an exquisite croesus prominent moth, patterned network of dark brown lines and golden brown scales, striking pale hindwings (photo)

UDK5001223

Spiral galaxy NGC 3370 in the Lion - Spiral galaxy NGC 3370 in Leo - The spiral galaxy NGC 3370 is located about 100 million years away - light from Earth. In November 1994, light emitting from a supernova type Ia, SN 1994ae, part of this galaxy, reached Earth. In this image taken by the Hubble space telescope in May 2003, this supernova is no longer detectable. On the other hand, the telescope was able to observe in this galaxy cepheides, variable stars used to accurately measure distances in the universe and calculate the rate of expansion of the universe. Many galaxies are visible in the background. The majestic dusty spiral, NGC 3370, looms in the foreground in this NASA Hubble Space Telescope image. Recent observations taken with the Advanced Camera for Surveys show intricate spiral arm structure spotted with hot areas of new star formation. In November 1994, the light of a supernova in nearby NGC 3370 reached Earth. This stellar outburst briefly outshone all of the tens of billio

Spiral galaxy NGC 3370 in the Lion - Spiral galaxy NGC 3370 in Leo - The spiral galaxy NGC 3370 is located about 100 million years away - light from Earth. In November 1994, light emitting from a supernova type Ia, SN 1994ae, part of this galaxy, reached Earth. In this image taken by the Hubble space telescope in May 2003, this supernova is no longer detectable. On the other hand, the telescope was able to observe in this galaxy cepheides, variable stars used to accurately measure distances in the universe and calculate the rate of expansion of the universe. Many galaxies are visible in the background. The majestic dusty spiral, NGC 3370, looms in the foreground in this NASA Hubble Space Telescope image. Recent observations taken with the Advanced Camera for Surveys show intricate spiral arm structure spotted with hot areas of new star formation. In November 1994, the light of a supernova in nearby NGC 3370 reached Earth. This stellar outburst briefly outshone all of the tens of billio

PIX4610713

Spiral galaxy NGC 3370 in the Lion - Spiral galaxy NGC 3370 in Leo - The spiral galaxy NGC 3370 is located about 100 million years away - light from Earth. In November 1994, light emitting from a supernova type Ia, SN 1994ae, part of this galaxy, reached Earth. In this image taken by the Hubble space telescope in May 2003, this supernova is no longer detectable. On the other hand, the telescope was able to observe in this galaxy cepheides, variable stars used to accurately measure distances in the universe and calculate the rate of expansion of the universe. Many galaxies are visible in the background. The majestic dusty spiral, NGC 3370, looms in the foreground in this NASA Hubble Space Telescope image. Recent observations taken with the Advanced Camera for Surveys show intricate spiral arm structure spotted with hot areas of new star formation. In November 1994, the light of a supernova in nearby NGC 3370 reached Earth. This stellar outburst briefly outshone all of the tens of billio

Spiral galaxy NGC 3370 in the Lion - Spiral galaxy NGC 3370 in Leo - The spiral galaxy NGC 3370 is located about 100 million years away - light from Earth. In November 1994, light emitting from a supernova type Ia, SN 1994ae, part of this galaxy, reached Earth. In this image taken by the Hubble space telescope in May 2003, this supernova is no longer detectable. On the other hand, the telescope was able to observe in this galaxy cepheides, variable stars used to accurately measure distances in the universe and calculate the rate of expansion of the universe. Many galaxies are visible in the background. The majestic dusty spiral, NGC 3370, looms in the foreground in this NASA Hubble Space Telescope image. Recent observations taken with the Advanced Camera for Surveys show intricate spiral arm structure spotted with hot areas of new star formation. In November 1994, the light of a supernova in nearby NGC 3370 reached Earth. This stellar outburst briefly outshone all of the tens of billio

PIX4610684

Gold pocket watch, open-Photo by Clive Streeter, Courtesy of The Science Museum, London

Gold pocket watch, open-Photo by Clive Streeter, Courtesy of The Science Museum, London

UDK5430400

Elliptical galaxy NGC 1275 in Persee - Elliptical galaxy NGC 1275 in Perseus - This image obtained by the Hubble space telescope in 1995 shows a system of two colliding galaxies; in the foreground, a spiral galaxy seen almost from the edge, with many stars forming in the background, a giant, very bright elliptical galaxy, special because it has a spiral structure in its center. Its core probably houses a black hole. NGC 1275 is located about 230 million years ago - light; it belongs to the large cluster of galaxies of Persee. These images, taken with Hubble's Wide Field Planetary Camera 2 (WFPC2), show traces of spiral structure accompanied by dramatic dust lanes and bright blue regions that mark areas of active star formation. Detailed observations of NGC 1275 indicate that the dusty material belongs to a spiral system seen nearly edge - on in the foreground. The second galaxy, lying beyond the first, is actually a giant elliptical with peculiar faint spiral structure in its nucleus.

Elliptical galaxy NGC 1275 in Persee - Elliptical galaxy NGC 1275 in Perseus - This image obtained by the Hubble space telescope in 1995 shows a system of two colliding galaxies; in the foreground, a spiral galaxy seen almost from the edge, with many stars forming in the background, a giant, very bright elliptical galaxy, special because it has a spiral structure in its center. Its core probably houses a black hole. NGC 1275 is located about 230 million years ago - light; it belongs to the large cluster of galaxies of Persee. These images, taken with Hubble's Wide Field Planetary Camera 2 (WFPC2), show traces of spiral structure accompanied by dramatic dust lanes and bright blue regions that mark areas of active star formation. Detailed observations of NGC 1275 indicate that the dusty material belongs to a spiral system seen nearly edge - on in the foreground. The second galaxy, lying beyond the first, is actually a giant elliptical with peculiar faint spiral structure in its nucleus.

PIX4609694

Peru Machu Picchu (photo)

Peru Machu Picchu (photo)

Sergi Reboredo

SRB3585210

Peru Machu Picchu (photo)

Peru Machu Picchu (photo)

Sergi Reboredo

SRB3585211

Nebuleuse N44 in the Great Magellan Cloud - This photo shows the southern part of the spectacular N44 region in the Large Magellanic Cloud. The green colour indicates areas that are particularly hot. The field measures 27.5 x 26.5 arcmin2., North is up and East is left. The two best known satellite galaxies of the Milky Way, the Magellanic Clouds, are located in the southern sky at a distance of about 170,000 light - years. They host many giant nebular complexes with very hot and luminous stars whose intense ultraviolet radiation causes the surrounding interstellar gas to glow. The intricate and colourful nebulae are produced by ionised gas that shines as electrons and positively charged atomic nuclei recombine, emitting a cascade of photons at well defined wavelengths. Such nebulae are called “” H II regions””, signifying ionised hydrogen, i.e. hydrogen atoms that have lost one electron (protons). Their spectra are characterized by emission lines whose relative intensities carry usefu

Nebuleuse N44 in the Great Magellan Cloud - This photo shows the southern part of the spectacular N44 region in the Large Magellanic Cloud. The green colour indicates areas that are particularly hot. The field measures 27.5 x 26.5 arcmin2., North is up and East is left. The two best known satellite galaxies of the Milky Way, the Magellanic Clouds, are located in the southern sky at a distance of about 170,000 light - years. They host many giant nebular complexes with very hot and luminous stars whose intense ultraviolet radiation causes the surrounding interstellar gas to glow. The intricate and colourful nebulae are produced by ionised gas that shines as electrons and positively charged atomic nuclei recombine, emitting a cascade of photons at well defined wavelengths. Such nebulae are called “” H II regions””, signifying ionised hydrogen, i.e. hydrogen atoms that have lost one electron (protons). Their spectra are characterized by emission lines whose relative intensities carry usefu

PIX4620812

Nebulae NGC 6334 and NGC 6357 in Scorpio - Nebulae NGC 6334 and NGC 6357 in Scorpius: These nebulae are located about 5500 light years from Earth - Located in the constellation of Scorpius, the Cat's Paw Nebula resemble a faint, luminous paw-print on the sky. Deep images reveal that the nebula is about a degree across in the sky. At a distance of about 5500 light-years away it is a truly vast structure spanning almost 100 light-years across. The sculpted gases of NGC 6334 are illuminated by the light of numerous powerful stars, some exceeding 10 solar masses. The two brilliant blue stars in the upper left are Lambda and Kappa Scorpii. Many of these luminous hot stars are surprisingly not visible because they lie within the dusty plane of our galaxy. At infrared wavelengths the numerous hot stars are revealed and the nature of this object as a region of massive star formation becomes clear. In the past decade water masers, molecular outflows, and x-ray sources have provided direct evide

Nebulae NGC 6334 and NGC 6357 in Scorpio - Nebulae NGC 6334 and NGC 6357 in Scorpius: These nebulae are located about 5500 light years from Earth - Located in the constellation of Scorpius, the Cat's Paw Nebula resemble a faint, luminous paw-print on the sky. Deep images reveal that the nebula is about a degree across in the sky. At a distance of about 5500 light-years away it is a truly vast structure spanning almost 100 light-years across. The sculpted gases of NGC 6334 are illuminated by the light of numerous powerful stars, some exceeding 10 solar masses. The two brilliant blue stars in the upper left are Lambda and Kappa Scorpii. Many of these luminous hot stars are surprisingly not visible because they lie within the dusty plane of our galaxy. At infrared wavelengths the numerous hot stars are revealed and the nature of this object as a region of massive star formation becomes clear. In the past decade water masers, molecular outflows, and x-ray sources have provided direct evide

R. Gendler

PIX4619391

Crab Pulsar in Nebula M1 - The Crab pulsar: This false-colored image obtained by the Hubble Space Telescope shows the central region of the Crab Nebula or resides its pulsar. The pulsar is visible in the center of the image. It is a very dense neutron star from the explosion of a massive supernova star. This star quickly rotates on itself developing a powerful magnetic field, emitting beams of light and radio waves. M1 is located about 6000 light-years in the constellation Taurus.. In 1054 AD, during the Song dynasty, Chinese astronomers spotted a bright new star in the night sky. This newcomer turned out to be a violent explosion within the Milky Way, caused by the spectacular death of a star some 1600 light-years away. This explosion created one of the most well-studied and beautiful objects in the night sky - the Crab Nebula. The beautiful result of this cataclysmic Type II supernova is shown here, imaged by the NASA/ESA Hubble Space Telescope's Advanced Camera for Surveys. Unlike m

Crab Pulsar in Nebula M1 - The Crab pulsar: This false-colored image obtained by the Hubble Space Telescope shows the central region of the Crab Nebula or resides its pulsar. The pulsar is visible in the center of the image. It is a very dense neutron star from the explosion of a massive supernova star. This star quickly rotates on itself developing a powerful magnetic field, emitting beams of light and radio waves. M1 is located about 6000 light-years in the constellation Taurus.. In 1054 AD, during the Song dynasty, Chinese astronomers spotted a bright new star in the night sky. This newcomer turned out to be a violent explosion within the Milky Way, caused by the spectacular death of a star some 1600 light-years away. This explosion created one of the most well-studied and beautiful objects in the night sky - the Crab Nebula. The beautiful result of this cataclysmic Type II supernova is shown here, imaged by the NASA/ESA Hubble Space Telescope's Advanced Camera for Surveys. Unlike m

PIX4583169

Peru Machu Picchu (photo)

Peru Machu Picchu (photo)

Sergi Reboredo

SRB3585209

Planetary nebula myCN18 dans la Mouche/HST - This is an image of MyCN18, a young planetary nebula located about 8,000 light - years away, taken with the Wide Field and Planetary Camera 2 (WFPC2) aboard Nasa's Hubble Space Telescope (HST). This picture has been composed from three separate images taken in the light of ionized nitrogen (represented by red), hydrogen (green), and doubly - ionized oxygen (blue). The results are of great interest because they shed new light on the poorly understood ejection of stellar matter which accompanies the slow death of Sun - like stars. According to one theory for the formation of planetary nebulae, the hourglass shape is produced by the expansion of a fast stellar wind within a slowly expanding cloud which is more dense near its equator than near its poles. What appears as a bright elliptical ring in the center, and at first sight might be mistaken for an equatorially dense region, is seen on closer inspection to be a potato shaped structure with a

Planetary nebula myCN18 dans la Mouche/HST - This is an image of MyCN18, a young planetary nebula located about 8,000 light - years away, taken with the Wide Field and Planetary Camera 2 (WFPC2) aboard Nasa's Hubble Space Telescope (HST). This picture has been composed from three separate images taken in the light of ionized nitrogen (represented by red), hydrogen (green), and doubly - ionized oxygen (blue). The results are of great interest because they shed new light on the poorly understood ejection of stellar matter which accompanies the slow death of Sun - like stars. According to one theory for the formation of planetary nebulae, the hourglass shape is produced by the expansion of a fast stellar wind within a slowly expanding cloud which is more dense near its equator than near its poles. What appears as a bright elliptical ring in the center, and at first sight might be mistaken for an equatorially dense region, is seen on closer inspection to be a potato shaped structure with a

PIX4623735

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

France Paris Musee d Orsay The Great Clock

France Paris Musee d Orsay The Great Clock

UIG5382427

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

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

PIX4623222

Marcus Aurelius, 139-150 (marble)

Marcus Aurelius, 139-150 (marble)

Roman, (2nd century)

ROC3706866

North Africa, Morocco, Karaouiyine Quarter, Fes el-Bali, Bou Inania Medersa, doorway richly decorated with Zellij tilework, stuccowork and sculpted wood, man wearing hooded cloak entering.-Photo by Cecile Treal and Jean-Michel Ruiz

North Africa, Morocco, Karaouiyine Quarter, Fes el-Bali, Bou Inania Medersa, doorway richly decorated with Zellij tilework, stuccowork and sculpted wood, man wearing hooded cloak entering.-Photo by Cecile Treal and Jean-Michel Ruiz

UDK5430525

1960s Mexico: Bell ringing between the intricately detailed columns of the church tower.

1960s Mexico: Bell ringing between the intricately detailed columns of the church tower.

AVE8927328

Ceiling with intricately painted tiles; floral pattern; Vakil Mosque; Shiraz; Iran; Asia

Ceiling with intricately painted tiles; floral pattern; Vakil Mosque; Shiraz; Iran; Asia

Stefan Auth

IMB4914323

Allegory of religion, 16th century (drawing)

Allegory of religion, 16th century (drawing)

Delaune, Etienne (1518-83)

Photo Josse

JLJ4670008

The Life and Strange Surprising Adventures of Robinson Crusoe, 18th century (engraving)

The Life and Strange Surprising Adventures of Robinson Crusoe, 18th century (engraving)

Stothard, Thomas (1755-1834)

AFF3614723

Stele of Iku and Mer-Imat, probably from Naga-ed-Deir, First Intermediate Period, c.2100 BC (painted limestone)

Stele of Iku and Mer-Imat, probably from Naga-ed-Deir, First Intermediate Period, c.2100 BC (painted limestone)

Egyptian 11th Dynasty (2061-2010 BC)

SSI2211184

Rose from the transept of the south coast of the Cathedrale Notre Dame of Chartres, 13th century (photo)

Rose from the transept of the south coast of the Cathedrale Notre Dame of Chartres, 13th century (photo)

French School, (13th century)

Photo Josse

JLJ4670423

Ottoman art: the taste of princesses, Turkish manuscript page, 16th century (miniature)

Ottoman art: the taste of princesses, Turkish manuscript page, 16th century (miniature)

Ottoman School, (16th century)

Photo Josse

JLJ4581071

Carving Of The Goddess Parvati At Keshava Temple, Somnathpur, India, 2008 (photo)

Carving Of The Goddess Parvati At Keshava Temple, Somnathpur, India, 2008 (photo)

Eric Lafforgue

LFG7357771

Rows Of Carvings Of Hindu God At Keshava Temple, Somnathpur, India, 2008 (photo)

Rows Of Carvings Of Hindu God At Keshava Temple, Somnathpur, India, 2008 (photo)

Eric Lafforgue

LFG7357770

Bas-relief Of Carved Riders On Horse-back At Keshava Temple, Somnathpur, India, 2008 (photo)

Bas-relief Of Carved Riders On Horse-back At Keshava Temple, Somnathpur, India, 2008 (photo)

Eric Lafforgue

LFG7357772

Carving Cut In Rock Of Lord Shiva And The Goddess Parvati At Keshava Temple, Somnathpur, India, 2008 (photo)

Carving Cut In Rock Of Lord Shiva And The Goddess Parvati At Keshava Temple, Somnathpur, India, 2008 (photo)

Eric Lafforgue

LFG7355857

One Of The Three Sanctuaries Of The 12Th Century Keshava Temple, Somnathpur, India, 2008 (photo)

One Of The Three Sanctuaries Of The 12Th Century Keshava Temple, Somnathpur, India, 2008 (photo)

Eric Lafforgue

LFG7357774

Carvings Cuts In Rock At Keshava Temple, Somnathpur, India, 2008 (photo)

Carvings Cuts In Rock At Keshava Temple, Somnathpur, India, 2008 (photo)

Eric Lafforgue

LFG7357773

The Main Shrines And Its Intricately Carved Rock At Keshava Temple, Somnathpur, India, 2008 (photo)

The Main Shrines And Its Intricately Carved Rock At Keshava Temple, Somnathpur, India, 2008 (photo)

Eric Lafforgue

LFG7355858

Shivaji, Khana, 1996 (mixed media on paper)

premium — Shivaji, Khana, 1996 (mixed media on paper)

Shivaji, Khana, 1996 (mixed media on paper)

Adlington, Mark

MAD116392

Cathedral of Chartres: life of Saint John the Evangelist detail bas, 13th century (stained glass)

Cathedral of Chartres: life of Saint John the Evangelist detail bas, 13th century (stained glass)

French School, (13th century)

Photo Josse

JLJ4696885

Porringer (silver)

Porringer (silver)

Coney, John (1655-1722)

BAL1070

A Subtle Intelligence, 2018 (mixed media on paper)

premium — A Subtle Intelligence, 2018 (mixed media on paper)

A Subtle Intelligence, 2018 (mixed media on paper)

Adlington, Mark

MAD6219139

Social Realism: "The Human Machine", 1902 (bronze relief)

Social Realism: "The Human Machine", 1902 (bronze relief)

Hoetger, Bernhard (1874-1949)

Photo Josse

JLJ4678908

Procession of the Sablon girls in Brussels, c.1635 (oil on wood)

Procession of the Sablon girls in Brussels, c.1635 (oil on wood)

Sallaert, Antoine or Anthonis (c.1590-c.1658)

Ernani Orcorte

RTR5891885

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