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The "Capital of the Judge" or "of the Upright Judge and of the Corrupt Judge", work by Campionesi masters, XII - XIII centur, Torresani Hall, Ghirlandina Tower, Modena, Italy (photo)y.

The "Capital of the Judge" or "of the Upright Judge and of the Corrupt Judge", work by Campionesi masters, XII - XIII centur, Torresani Hall, Ghirlandina Tower, Modena, Italy (photo)y.

Ghigo Roli

GRL5974131

The "Capital of the Judge" or "of the Upright Judge and of the Corrupt Judge", work by Campionesi masters, XII - XIII century, Torresani Hall, Ghirlandina Tower, Modena, Italy (photo)

The "Capital of the Judge" or "of the Upright Judge and of the Corrupt Judge", work by Campionesi masters, XII - XIII century, Torresani Hall, Ghirlandina Tower, Modena, Italy (photo)

Ghigo Roli

GRL5974081

The "Capital of the Judge" or "of the Upright Judge and of the Corrupt Judge", work by Campionesi masters, XII - XIII century, Torresani Hall, Ghirlandina Tower, Modena, Italy (photo)

The "Capital of the Judge" or "of the Upright Judge and of the Corrupt Judge", work by Campionesi masters, XII - XIII century, Torresani Hall, Ghirlandina Tower, Modena, Italy (photo)

Ghigo Roli

GRL5974084

The "Capital of the Judge" or "of the Upright Judge and of the Corrupt Judge", work by Campionesi masters, XII - XIII century, Torresani Hall, Ghirlandina Tower, Modena, Italy (photo), Torresani Hall, Ghirlandina Tower, Modena, Italy (photo)

The "Capital of the Judge" or "of the Upright Judge and of the Corrupt Judge", work by Campionesi masters, XII - XIII century, Torresani Hall, Ghirlandina Tower, Modena, Italy (photo), Torresani Hall, Ghirlandina Tower, Modena, Italy (photo)

Ghigo Roli

GRL5974086

The "Capital of the Judge" or "of the Upright Judge and of the Corrupt Judge", work by Campionesi masters, XII - XIII century, Torresani Hall, Ghirlandina Tower, Modena, Italy (photo)

The "Capital of the Judge" or "of the Upright Judge and of the Corrupt Judge", work by Campionesi masters, XII - XIII century, Torresani Hall, Ghirlandina Tower, Modena, Italy (photo)

Ghigo Roli

GRL5974088

The "Capital of the Judge" or "of the Upright Judge and of the Corrupt Judge", work by Campionesi masters, XII - XIII century, Torresani Hall, Ghirlandina Tower, Modena, Italy (photo)

The "Capital of the Judge" or "of the Upright Judge and of the Corrupt Judge", work by Campionesi masters, XII - XIII century, Torresani Hall, Ghirlandina Tower, Modena, Italy (photo)

Ghigo Roli

GRL5974090

The "Capital of the Judge" or "of the Upright Judge and of the Corrupt Judge", work by Campionesi masters, XII - XIII century, Torresani Hall, Ghirlandina Tower, Modena, Italy (photo)

The "Capital of the Judge" or "of the Upright Judge and of the Corrupt Judge", work by Campionesi masters, XII - XIII century, Torresani Hall, Ghirlandina Tower, Modena, Italy (photo)

Ghigo Roli

GRL5974105

Planetary nebula M57 (NGC 6720) in Lyra - The Ring nebula M57 in Lyra - The planetary nebula of Lyra (M57) is located about 2000 years - light from Earth. 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. Image obtained by the Hubble Space Telescope. This close - up, visible - light view by Nasa's Hubble Space Telescope reveals new details of the Ring Nebula. The object is tilted towards Earth so that astronomers see the ring face - on. The Hubble observations reveal that the nebula's shape is more complicated than astronomers thought. The blue gas in the nebula's center is actually a football - shaped structure that pierces the red doughnut - shaped material. Hubble also uncovers the detailed structure of the dark, irregular knots of dense gas embedded along the inner rim of the ring. The knots look like spokes in a bicycle. The Hubble images have allowed the research team to match u

Planetary nebula M57 (NGC 6720) in Lyra - The Ring nebula M57 in Lyra - The planetary nebula of Lyra (M57) is located about 2000 years - light from Earth. 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. Image obtained by the Hubble Space Telescope. This close - up, visible - light view by Nasa's Hubble Space Telescope reveals new details of the Ring Nebula. The object is tilted towards Earth so that astronomers see the ring face - on. The Hubble observations reveal that the nebula's shape is more complicated than astronomers thought. The blue gas in the nebula's center is actually a football - shaped structure that pierces the red doughnut - shaped material. Hubble also uncovers the detailed structure of the dark, irregular knots of dense gas embedded along the inner rim of the ring. The knots look like spokes in a bicycle. The Hubble images have allowed the research team to match u

PIX4623343

Royal Hunt at the pond of Tour Rambouillet, 18th September, 1826 (w/c)

Royal Hunt at the pond of Tour Rambouillet, 18th September, 1826 (w/c)

Champin, Jean-Jacques (1796-1860)

XIR904815

The "Capital of the Judge" or "of the Upright Judge and of the Corrupt Judge", work by Campionesi masters, XII - XIII century, Torresani Hall, Ghirlandina Tower, Modena, Italy (photo)

The "Capital of the Judge" or "of the Upright Judge and of the Corrupt Judge", work by Campionesi masters, XII - XIII century, Torresani Hall, Ghirlandina Tower, Modena, Italy (photo)

Ghigo Roli

GRL5974098

The "Capital of the Judge" or "of the Upright Judge and of the Corrupt Judge", work by Campionesi masters, XII - XIII century, Torresani Hall, Ghirlandina Tower, Modena, Italy (photo)

The "Capital of the Judge" or "of the Upright Judge and of the Corrupt Judge", work by Campionesi masters, XII - XIII century, Torresani Hall, Ghirlandina Tower, Modena, Italy (photo)

Ghigo Roli

GRL5974102

The "Capital of the Judge" or "of the Upright Judge and of the Corrupt Judge", work by Campionesi masters, XII - XIII century, Torresani Hall, Ghirlandina Tower, Modena, Italy (photo)

The "Capital of the Judge" or "of the Upright Judge and of the Corrupt Judge", work by Campionesi masters, XII - XIII century, Torresani Hall, Ghirlandina Tower, Modena, Italy (photo)

Ghigo Roli

GRL5974107

Planetary nebula IC 418 dans le Lievre/HST - IC 418: The “” Spirograph” Nebula Glowing like a multi - faceted jewel, the planetary nebula IC 418 lies about 2,000 light - years from Earth in the direction of the constellation Lepus. This photograph is from Nasa's Hubble Space Telescope, obtained with the Wide Field Planetary Camera 2. A planetary nebula represents the final stage in the evolution of a star similar to our Sun. The star at the center of IC 418 was a red giant a few thousand years ago, but then ejected its outer layers into space to form the nebula, which has now expanded to a diameter of about 0.1 light - year. The stellar remnant at the center is the hot core of the red giant, from which ultraviolet radiation floods out into the surrounding gas, causing it to fluoresce. Over the next several thousand years, the nebula will gradually disperse into space, and then the star will cool and fade away for billions of years as a white dwarf. Our own Sun is expected to undergo a

Planetary nebula IC 418 dans le Lievre/HST - IC 418: The “” Spirograph” Nebula Glowing like a multi - faceted jewel, the planetary nebula IC 418 lies about 2,000 light - years from Earth in the direction of the constellation Lepus. This photograph is from Nasa's Hubble Space Telescope, obtained with the Wide Field Planetary Camera 2. A planetary nebula represents the final stage in the evolution of a star similar to our Sun. The star at the center of IC 418 was a red giant a few thousand years ago, but then ejected its outer layers into space to form the nebula, which has now expanded to a diameter of about 0.1 light - year. The stellar remnant at the center is the hot core of the red giant, from which ultraviolet radiation floods out into the surrounding gas, causing it to fluoresce. Over the next several thousand years, the nebula will gradually disperse into space, and then the star will cool and fade away for billions of years as a white dwarf. Our own Sun is expected to undergo a

PIX4623677

Distant galaxies in the Fornax constellation - Distant galaxies in the Fornax constellation - Image of distant galaxies obtained by the Hubble space telescope in the constellation Forneau in September 2003. This image represents a typical view of our distant universe. In taking this picture, Hubble is looking down a long corridor of galaxies stretching billions of light - years distant in space, corresponding to looking billions of years back in time. The field shown in this picture covers a relatively small patch of sky, a fraction of the area of the full moon, yet it is richly populated with a variety of galaxy types. A handful of large fully formed galaxies are scattered throughout the image. These galaxies are easy to see because they are relatively close to us. Several of the galaxies are spirals with flat disks that are oriented edge - on or face - on to our line of sight, or somewhere in between. Elliptical galaxies and more exotic galaxies with bars or tidal tails are also visi

Distant galaxies in the Fornax constellation - Distant galaxies in the Fornax constellation - Image of distant galaxies obtained by the Hubble space telescope in the constellation Forneau in September 2003. This image represents a typical view of our distant universe. In taking this picture, Hubble is looking down a long corridor of galaxies stretching billions of light - years distant in space, corresponding to looking billions of years back in time. The field shown in this picture covers a relatively small patch of sky, a fraction of the area of the full moon, yet it is richly populated with a variety of galaxy types. A handful of large fully formed galaxies are scattered throughout the image. These galaxies are easy to see because they are relatively close to us. Several of the galaxies are spirals with flat disks that are oriented edge - on or face - on to our line of sight, or somewhere in between. Elliptical galaxies and more exotic galaxies with bars or tidal tails are also visi

PIX4613828

Pioneer Plate - The Pioneer Plate - The Pioneer 10 and Pioneer 11 probes have embarked on a plate, called the Pioneer Plate, containing a message intended for potential aliens. On this engraved metal plate are depicted a naked man and woman, the location of our Sun as well as 14 pulsars, the trajectory of the probe in the solar system... Pioneer 10 was launched on 3 March 1972 with as its first destination, the Jupiter Planet, which it flew over on 3 December 1973; it was the first space probe to approach this planet; it was also the first space probe to leave the solar system. The Pioneer F spacecraft, destined to be the first man made object to escape from the solar system into interstellar space, carries this pictorial plaque. It is designed to show scientifically educated inhabitants of some other star system, who might intercept it millions of years from now, when Pioneer was launched, from where, and by what kind of beings. The design is etched into a 6 inch by 9 inch gold - anod

Pioneer Plate - The Pioneer Plate - The Pioneer 10 and Pioneer 11 probes have embarked on a plate, called the Pioneer Plate, containing a message intended for potential aliens. On this engraved metal plate are depicted a naked man and woman, the location of our Sun as well as 14 pulsars, the trajectory of the probe in the solar system... Pioneer 10 was launched on 3 March 1972 with as its first destination, the Jupiter Planet, which it flew over on 3 December 1973; it was the first space probe to approach this planet; it was also the first space probe to leave the solar system. The Pioneer F spacecraft, destined to be the first man made object to escape from the solar system into interstellar space, carries this pictorial plaque. It is designed to show scientifically educated inhabitants of some other star system, who might intercept it millions of years from now, when Pioneer was launched, from where, and by what kind of beings. The design is etched into a 6 inch by 9 inch gold - anod

PIX4605578

Capt. Offin Boardman, 1787 (oil on canvas)

Capt. Offin Boardman, 1787 (oil on canvas)

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

WAM3690704

Antares star and the nebula Rho Ophiuchi - Antares and Rho Ophiuchi cloud - This coloree nebula represents the visible part of a very large molecule cloud, the cloud of Ophiuchus. This star-forming region is about 520 years old - light. The brightest star at the bottom left is the star Antares, from the Scorpio. The triple star Rho Ophiuchus is located in the middle of the blue cloud at the top of the picture. On the right, surrounded by a nebula, the star Sigma Scorpii. The globular clusters M4 (at the bottom of the image) and NGC 6144 (near Antares) are also visible on this image obtained with the UK Schmidt telescope of 1.2m. This photograph shows a portion of a great swath of obscuring gas and dust in the constellations Ophiuchus and Scorpius, and illustrates what is probably the most colourful region in the entire sky. The almost garish colours are due to the brilliance and contrasting colours of the stars, by whose reflected light we see the dust clouds. Dominating the picture is

Antares star and the nebula Rho Ophiuchi - Antares and Rho Ophiuchi cloud - This coloree nebula represents the visible part of a very large molecule cloud, the cloud of Ophiuchus. This star-forming region is about 520 years old - light. The brightest star at the bottom left is the star Antares, from the Scorpio. The triple star Rho Ophiuchus is located in the middle of the blue cloud at the top of the picture. On the right, surrounded by a nebula, the star Sigma Scorpii. The globular clusters M4 (at the bottom of the image) and NGC 6144 (near Antares) are also visible on this image obtained with the UK Schmidt telescope of 1.2m. This photograph shows a portion of a great swath of obscuring gas and dust in the constellations Ophiuchus and Scorpius, and illustrates what is probably the most colourful region in the entire sky. The almost garish colours are due to the brilliance and contrasting colours of the stars, by whose reflected light we see the dust clouds. Dominating the picture is

PIX4621421

Planetary nebula NGC 6543 in the Dragon - Planetary nebula NGC 6543 in Draco - Composite view of the planetary nebula NGC 6543 in the Dragon obtained by the Hubble space telescope and X-ray (blue) by the Chandra satellite. NGC 6543 is located about 3000 years of light from Earth. This composite of data from Nasa's Chandra X - ray Observatory and Hubble Space Telescope is a new look for NGC 6543, better known as the Cat's Eye nebula. This famous object is a so - called planetary nebula that represents a phase of stellar evolution that the Sun should experience several billion years from now. When a star like the Sun begins to run out of fuel, it becomes what is known as a red giant. In this phase, a star sheds some of its outer layers, eventually leaving behind a hot core that collapses to form a dense white dwarf star. A fast wind emanating from the hot core rams into the ejected atmosphere, pushes it outward, and creates the graceful filamentary structures seen with optical telescopes

Planetary nebula NGC 6543 in the Dragon - Planetary nebula NGC 6543 in Draco - Composite view of the planetary nebula NGC 6543 in the Dragon obtained by the Hubble space telescope and X-ray (blue) by the Chandra satellite. NGC 6543 is located about 3000 years of light from Earth. This composite of data from Nasa's Chandra X - ray Observatory and Hubble Space Telescope is a new look for NGC 6543, better known as the Cat's Eye nebula. This famous object is a so - called planetary nebula that represents a phase of stellar evolution that the Sun should experience several billion years from now. When a star like the Sun begins to run out of fuel, it becomes what is known as a red giant. In this phase, a star sheds some of its outer layers, eventually leaving behind a hot core that collapses to form a dense white dwarf star. A fast wind emanating from the hot core rams into the ejected atmosphere, pushes it outward, and creates the graceful filamentary structures seen with optical telescopes

PIX4623257

Les branches de la connaissance 16e siecle: chacune representee par differentes personnalites: en haut, Aristote (384-322 avant JC) pour la philosophie et Seneque (Lucius Annaeus Seneca, 4 avant JC-65) pour la morale

Les branches de la connaissance 16e siecle: chacune representee par differentes personnalites: en haut, Aristote (384-322 avant JC) pour la philosophie et Seneque (Lucius Annaeus Seneca, 4 avant JC-65) pour la morale

UIS5064676

Galaxy clusters Abell 2744 - Black material - X - rays, dark matter and galaxies in cluster Abell 2744

Galaxy clusters Abell 2744 - Black material - X - rays, dark matter and galaxies in cluster Abell 2744

PIX4565787

Shanghai, China (photo)

Shanghai, China (photo)

Sergi Reboredo

SRB3036715

Remains of the supernova Kepler in Ophiuchus - Nasa's three Great Observatories - - the Hubble Space Telescope, the Spitzer Space Telescope, and the Chandra X - ray Observatory - joined forces to probe the expanding remains of a supernova, called Kepler's supernova remnant, first seen 400 years ago by sky watchers, including famous astronomer Johannes Kepler. The combined image unveils a bubble - shaped shroud of gas and dust that is 14 light - years wide and is expanding at 4 million miles per hour (2,000 kilometers per second). Observations from each telescope highlight distinct features of the supernova remnant, a fast - moving shell of iron - rich material from the exploded star, surrounded by an expanding shock wave that is sweeping up interstellar gas and dust. Each color in this image represents a different region of the electromagnetic spectrum, from X - rays to infrared light. The X - ray and infrared data cannot be seen with the human eye. By color - coding those data and com

Remains of the supernova Kepler in Ophiuchus - Nasa's three Great Observatories - - the Hubble Space Telescope, the Spitzer Space Telescope, and the Chandra X - ray Observatory - joined forces to probe the expanding remains of a supernova, called Kepler's supernova remnant, first seen 400 years ago by sky watchers, including famous astronomer Johannes Kepler. The combined image unveils a bubble - shaped shroud of gas and dust that is 14 light - years wide and is expanding at 4 million miles per hour (2,000 kilometers per second). Observations from each telescope highlight distinct features of the supernova remnant, a fast - moving shell of iron - rich material from the exploded star, surrounded by an expanding shock wave that is sweeping up interstellar gas and dust. Each color in this image represents a different region of the electromagnetic spectrum, from X - rays to infrared light. The X - ray and infrared data cannot be seen with the human eye. By color - coding those data and com

PIX4582960

Shanghai, China (photo)

Shanghai, China (photo)

Sergi Reboredo

SRB3036716

The Procession to Calvary

The Procession to Calvary

Brueghel, Pieter the Younger (c.1564-1638)

USB1162139

Family Sorrows (oil on canvas)

Family Sorrows (oil on canvas)

Wieschebrink, Franz (1818-84)

XAL885725

Galaxy UGC 10214 in the Dragon - Galaxy UGC 10214 in Draco - The galaxy UGC 10214 is about 420 million years away - light from Earth. The shape of this galaxy is due to a collision with another galaxy, the small galaxy, blue, visible in the upper left corner of the image. Powerful gravitational forces are responsible for the formation of the tail, consisting of stars of dust and gas, which stretches over nearly 28,000 light years and is composed of recently formed and extremely bright blue stars. In the background, more than 6000 galaxies are visible, some more than 12 billion years apart - light. Image obtained by the Hubble Space Telescope in April 2002. This picture of the galaxy UGC 10214 was taken by the Advanced Camera for Surveys (ACS), which was installed aboard Nasa's Hubble Space Telescope in March during Servicing Mission 3B. Its distorted shape was caused by a small interloper, a very blue, compact galaxy visible in the upper left corner of the more massive Tadpole. The Tad

Galaxy UGC 10214 in the Dragon - Galaxy UGC 10214 in Draco - The galaxy UGC 10214 is about 420 million years away - light from Earth. The shape of this galaxy is due to a collision with another galaxy, the small galaxy, blue, visible in the upper left corner of the image. Powerful gravitational forces are responsible for the formation of the tail, consisting of stars of dust and gas, which stretches over nearly 28,000 light years and is composed of recently formed and extremely bright blue stars. In the background, more than 6000 galaxies are visible, some more than 12 billion years apart - light. Image obtained by the Hubble Space Telescope in April 2002. This picture of the galaxy UGC 10214 was taken by the Advanced Camera for Surveys (ACS), which was installed aboard Nasa's Hubble Space Telescope in March during Servicing Mission 3B. Its distorted shape was caused by a small interloper, a very blue, compact galaxy visible in the upper left corner of the more massive Tadpole. The Tad

PIX4613605

Shanghai, China (photo)

Shanghai, China (photo)

Sergi Reboredo

SRB3036724

Apsidal arch: Etymasia (preparation for the throne) with the instruments of passion, restored in 1979; Byzantine school mosaic with a golden background (mosaic)

Apsidal arch: Etymasia (preparation for the throne) with the instruments of passion, restored in 1979; Byzantine school mosaic with a golden background (mosaic)

Byzantine, (12th-13th century)

Ghigo Roli

GRL6166444

Galaxy UGC 10214 in the Dragon - Galaxy UGC 10214 in Draco - The galaxy UGC 10214 is about 420 million years away - light from Earth. The shape of this galaxy is due to a collision with another galaxy, the small galaxy, blue, visible in the upper left corner of the image. Powerful gravitational forces are responsible for the formation of the tail, consisting of stars of dust and gas, which stretches over nearly 28,000 light years and is composed of recently formed and extremely bright blue stars. In the background, more than 6000 galaxies are visible, some more than 12 billion years apart - light. Image obtained by the Hubble Space Telescope in April 2002. This picture of the galaxy UGC 10214 was taken by the Advanced Camera for Surveys (ACS), which was installed aboard Nasa's Hubble Space Telescope in March during Servicing Mission 3B. Its distorted shape was caused by a small interloper, a very blue, compact galaxy visible in the upper left corner of the more massive Tadpole. The Tad

Galaxy UGC 10214 in the Dragon - Galaxy UGC 10214 in Draco - The galaxy UGC 10214 is about 420 million years away - light from Earth. The shape of this galaxy is due to a collision with another galaxy, the small galaxy, blue, visible in the upper left corner of the image. Powerful gravitational forces are responsible for the formation of the tail, consisting of stars of dust and gas, which stretches over nearly 28,000 light years and is composed of recently formed and extremely bright blue stars. In the background, more than 6000 galaxies are visible, some more than 12 billion years apart - light. Image obtained by the Hubble Space Telescope in April 2002. This picture of the galaxy UGC 10214 was taken by the Advanced Camera for Surveys (ACS), which was installed aboard Nasa's Hubble Space Telescope in March during Servicing Mission 3B. Its distorted shape was caused by a small interloper, a very blue, compact galaxy visible in the upper left corner of the more massive Tadpole. The Tad

PIX4613581

Planetary nebula NGC 6369 in Ophiuchus/HST - NGC 6369 is known to amateur astronomers as the “” Little Ghost Nebula,”” because it appears as a small, ghostly cloud surrounding the faint, dying central star. NGC 6369 lies in the direction of the constellation Ophiuchus, at a distance estimated to be between about 2,000 and 5,000 light - years from Earth. When a star with a mass similar to that of our own Sun nears the end of its lifetime, it expands in size to become a red giant. The red - giant stage ends when the star expels its outer layers into space, producing a faintly glowing nebula. Astronomers call such an object a planetary nebula, because its round shape resembles that of a planet when viewed with a small telescope. The Hubble photograph of NGC 6369, captured with the Wide Field Planetary Camera 2 (WFPC2) in February 2002, reveals remarkable details of the ejection process that are not visible from ground - based telescopes because of the blurring produced by the Earth's atmo

Planetary nebula NGC 6369 in Ophiuchus/HST - NGC 6369 is known to amateur astronomers as the “” Little Ghost Nebula,”” because it appears as a small, ghostly cloud surrounding the faint, dying central star. NGC 6369 lies in the direction of the constellation Ophiuchus, at a distance estimated to be between about 2,000 and 5,000 light - years from Earth. When a star with a mass similar to that of our own Sun nears the end of its lifetime, it expands in size to become a red giant. The red - giant stage ends when the star expels its outer layers into space, producing a faintly glowing nebula. Astronomers call such an object a planetary nebula, because its round shape resembles that of a planet when viewed with a small telescope. The Hubble photograph of NGC 6369, captured with the Wide Field Planetary Camera 2 (WFPC2) in February 2002, reveals remarkable details of the ejection process that are not visible from ground - based telescopes because of the blurring produced by the Earth's atmo

PIX4623194

Young stars in Rho Ophiuchi - Young stars in Rho Ophiuchi - Image of the central part of Rho Ophiuchi obtained in infrared by the Spitzer space telescope. Rho Ophiuchi is a vast dark cloud of molecular hydrogen located 407 years - light from Earth in the constellations of Ophiuchus and Scorpio. More than 300 young stars aged only 300,000 years have been observed. On this picture in false colors highlighting the temperature differences present in this cloud, the younger stars appear in red, the more evolute stars in blue. Newborn stars peek out from beneath their natal blanket of dust in this dynamic image of the Rho Ophiuchi dark cloud from Nasa's Spitzer Space Telescope. Called “” Rho Oph””” by astronomers, it's one of the closest star - forming regions to our own solar system. Located near the constellations Scorpius and Ophiuchus, the nebula is about 407 light years away from Earth. Rho Oph is a complex made up of a large main cloud of molecular hydrogen, a key molecule allowing new

Young stars in Rho Ophiuchi - Young stars in Rho Ophiuchi - Image of the central part of Rho Ophiuchi obtained in infrared by the Spitzer space telescope. Rho Ophiuchi is a vast dark cloud of molecular hydrogen located 407 years - light from Earth in the constellations of Ophiuchus and Scorpio. More than 300 young stars aged only 300,000 years have been observed. On this picture in false colors highlighting the temperature differences present in this cloud, the younger stars appear in red, the more evolute stars in blue. Newborn stars peek out from beneath their natal blanket of dust in this dynamic image of the Rho Ophiuchi dark cloud from Nasa's Spitzer Space Telescope. Called “” Rho Oph””” by astronomers, it's one of the closest star - forming regions to our own solar system. Located near the constellations Scorpius and Ophiuchus, the nebula is about 407 light years away from Earth. Rho Oph is a complex made up of a large main cloud of molecular hydrogen, a key molecule allowing new

PIX4621537

Mont Blanc: Great rock-Mules and Chamonix Valley (b/w Photo before 1912)

Mont Blanc: Great rock-Mules and Chamonix Valley (b/w Photo before 1912)

LRS887743

Quasars seen by the Hubble Space Telescope - Quasars seen by the Hubble Space Telescope - Gallery of quasars observed in different types of galaxies; left column, quasars in normal galaxies, center in colliding galaxies, right in particular galaxies. Top left: quasar PG 0052+251, has about 1.4 billion years - light. Bottom left: Quasar PHL 909 has about 1.5 billion years - light. High center: quasar IRAS04505 - 2958, has about 3 billion years - light. Low center: quasar PG 1012+008, has about 1.6 billion years - light. High right: quasar 0316 - 346, has about 2.2 billion years - light. Low right: quasar IRAS13218+0552. has about 2 billion years - light. Images obtained by the Hubble Space Telescope in 1996. Quasars reside in a variety of galaxies, from normal to highly disturbed. When seen through ground - based telescopes, these compact, enigmatic light sources resemble stars, yet they are billions of light - years away and several hundred billion times brighter than normal stars. The

Quasars seen by the Hubble Space Telescope - Quasars seen by the Hubble Space Telescope - Gallery of quasars observed in different types of galaxies; left column, quasars in normal galaxies, center in colliding galaxies, right in particular galaxies. Top left: quasar PG 0052+251, has about 1.4 billion years - light. Bottom left: Quasar PHL 909 has about 1.5 billion years - light. High center: quasar IRAS04505 - 2958, has about 3 billion years - light. Low center: quasar PG 1012+008, has about 1.6 billion years - light. High right: quasar 0316 - 346, has about 2.2 billion years - light. Low right: quasar IRAS13218+0552. has about 2 billion years - light. Images obtained by the Hubble Space Telescope in 1996. Quasars reside in a variety of galaxies, from normal to highly disturbed. When seen through ground - based telescopes, these compact, enigmatic light sources resemble stars, yet they are billions of light - years away and several hundred billion times brighter than normal stars. The

PIX4613552

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

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

PIX4609334

Salle de spectacle (fol. 11 detail), from 'Atlas du Comte du Nord', 1784 (w/c & ink on paper)

Salle de spectacle (fol. 11 detail), from 'Atlas du Comte du Nord', 1784 (w/c & ink on paper)

Chambe, (fl.1784)

CND898774

Old town and Faculty or University of Medicine in the background Montpellier France. The Guilhem dynasty ends with the incorporation of Montpellier into the Crown of Aragon, In the fourteenth century, the sale of Montpellier to the Kingdom of France represents a period of decline during the following two centuries with various religious conflicts (the Holy War), However, a man named Jacques Coeur will stand out during this period: he is an excellent businessman who, apart from managing the royal treasury, is dedicated to trade in the Mediterranean, restoring Montpellier to its economic development, Today, you can still visit his palace, In the 15th century, Montpellier underwent an essential evolution with the creation of four royal chairs at the University of Medicine awarded by oppositions, Simple doctors see their role as an educator progressively harmed and in fact disappeared in the 18th century, The Renaissance is characterized by a profound renewal of teaching, Montpellier beco

Old town and Faculty or University of Medicine in the background Montpellier France. The Guilhem dynasty ends with the incorporation of Montpellier into the Crown of Aragon, In the fourteenth century, the sale of Montpellier to the Kingdom of France represents a period of decline during the following two centuries with various religious conflicts (the Holy War), However, a man named Jacques Coeur will stand out during this period: he is an excellent businessman who, apart from managing the royal treasury, is dedicated to trade in the Mediterranean, restoring Montpellier to its economic development, Today, you can still visit his palace, In the 15th century, Montpellier underwent an essential evolution with the creation of four royal chairs at the University of Medicine awarded by oppositions, Simple doctors see their role as an educator progressively harmed and in fact disappeared in the 18th century, The Renaissance is characterized by a profound renewal of teaching, Montpellier beco

Sergi Reboredo

SRB6367757

Twenty Star American "Abolitionist Flag", c.1859 (textile flag)

Twenty Star American "Abolitionist Flag", c.1859 (textile flag)

American School, (19th century)

GLC696125

Twenty Star American "Abolitionist Flag", c.1859 (textile flag)

Twenty Star American "Abolitionist Flag", c.1859 (textile flag)

American School, (19th century)

GLC696123

Sir Robert Davers, 5th Bt (1729-1763) [aged 21]

Sir Robert Davers, 5th Bt (1729-1763) [aged 21]

Batoni, Pompeo Girolamo (1708-87)

USB1156516

The Unannounced Return by Night of L. Tarquinius Collatinus and his Companions to find his Wife Lucretia Weaving (oil on canvas)

The Unannounced Return by Night of L. Tarquinius Collatinus and his Companions to find his Wife Lucretia Weaving (oil on canvas)

Baleschoux, Jehan Balechouse John (fl.1570) (attr.to)

USB1161917

The centre figure represents a Lama acting as 'Gnéchungchui-kyong'' [gNas-chun-chos-skyon]' a Deota. All the actors are supposed to represent servants of the Deota'. 'No.2 & 3 are two Gyelongs' [dge-slon] '4 & 5 are called Todpakyashil representing skeletons. Todpa is a head & kyashil or naked bones'. '6 & 7 King, supposed to be Rakhus attendants on the Deota'. '8 & 9 Dudhmo' [bdud-mo]' or cannibals'. [? she-devils] '10 & 11 Tsongtsong other attendants on the Deota. They are all in pairs, and were supposed in former times to have attended as these characters are represented before they had the shape of common human beings'. '12 & 13 Kerba, as above'. '14 & 15 Kiwho, as above'. '16 & 17 Dutot' [bdud- ]' cannibals'. '18 & 19 Zhanag' [zva-nag]' or black hats'. '20. Alpélkur' [ -dpal-dkar?]' supposed to be the wife of the Deota no.1'. '21. Zhugti' [bzugs-sti]' the seat of the Deota, spread with a human skin'. '22. Tongchin, the name of the instrument the men are sounding'. '23. Gyaling, na

The centre figure represents a Lama acting as 'Gnéchungchui-kyong'' [gNas-chun-chos-skyon]' a Deota. All the actors are supposed to represent servants of the Deota'. 'No.2 & 3 are two Gyelongs' [dge-slon] '4 & 5 are called Todpakyashil representing skeletons. Todpa is a head & kyashil or naked bones'. '6 & 7 King, supposed to be Rakhus attendants on the Deota'. '8 & 9 Dudhmo' [bdud-mo]' or cannibals'. [? she-devils] '10 & 11 Tsongtsong other attendants on the Deota. They are all in pairs, and were supposed in former times to have attended as these characters are represented before they had the shape of common human beings'. '12 & 13 Kerba, as above'. '14 & 15 Kiwho, as above'. '16 & 17 Dutot' [bdud- ]' cannibals'. '18 & 19 Zhanag' [zva-nag]' or black hats'. '20. Alpélkur' [ -dpal-dkar?]' supposed to be the wife of the Deota no.1'. '21. Zhugti' [bzugs-sti]' the seat of the Deota, spread with a human skin'. '22. Tongchin, the name of the instrument the men are sounding'. '23. Gyaling, na

BL3304994

Study for 'Deserted - a Foundling' (oil on canvas)

Study for 'Deserted - a Foundling' (oil on canvas)

Holl, Frank (1845-88)

MAA2956891

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

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

Dutch School, (18th century)

USB1159907

Portrait of Terentius Neo and his wife, formerly titled The Proculus baker and his wife (fresco)

Portrait of Terentius Neo and his wife, formerly titled The Proculus baker and his wife (fresco)

Roman (1st century AD)

XAL886745

Poster of Nazi propaganda representing the good Aryen on the left and the bad Jew on the right, 20th century (engraving)

Poster of Nazi propaganda representing the good Aryen on the left and the bad Jew on the right, 20th century (engraving)

German School, (20th century)

Photo Josse

JLJ4683772

News Events Post-War Japan 1946

News Events Post-War Japan 1946

BOF6286456

Morenci Mine is an open pit mine located in Arizona, United States

Morenci Mine is an open pit mine located in Arizona, United States

PIX6318749

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

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

Gillray, James (1757-1815)

NCO190494

Prince Charles Louis, Elector Palatine of the Rhine, and Duke of Bavaria (oil on canvas)

Prince Charles Louis, Elector Palatine of the Rhine, and Duke of Bavaria (oil on canvas)

Honthorst, Gerrit van (1590-1656)

USB1160403

Prince Charles Edward Stuart, c.1750 (oil on canvas)

Prince Charles Edward Stuart, c.1750 (oil on canvas)

Mosman, William (c.1700-71)

NGS3552110

Baby cot of the Prince Imperial, given by the City of Paris to Empress Eugénie in 1856 (b/w photo)

Baby cot of the Prince Imperial, given by the City of Paris to Empress Eugénie in 1856 (b/w photo)

Baltard, Victor (1805-74)

KDC498765

Royal Artillery Memorial, Hyde Park Corner, London, photographed in 2015 (photo)

Royal Artillery Memorial, Hyde Park Corner, London, photographed in 2015 (photo)

NAM5927024

Royal Artillery Memorial, Hyde Park Corner, London, photographed in 2015 (photo)

Royal Artillery Memorial, Hyde Park Corner, London, photographed in 2015 (photo)

NAM5927030

Royal Artillery Memorial, Hyde Park Corner, London, photographed in 2015 (photo)

Royal Artillery Memorial, Hyde Park Corner, London, photographed in 2015 (photo)

NAM5927028

Royal Artillery Memorial, Hyde Park Corner, London, photographed in 2015 (photo)

Royal Artillery Memorial, Hyde Park Corner, London, photographed in 2015 (photo)

NAM5927027

Royal Artillery Memorial, Hyde Park Corner, London, photographed in 2015 (photo)

Royal Artillery Memorial, Hyde Park Corner, London, photographed in 2015 (photo)

NAM5927031

Royal Artillery Memorial, Hyde Park Corner, London, photographed in 2015 (photo)

Royal Artillery Memorial, Hyde Park Corner, London, photographed in 2015 (photo)

NAM5927026

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