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Dying Gaul - The Dying Galatian - “” Dying Galatian Warrior”” Marble sculpture of Ludovisi Group after original bronze from 220-210 BC. Sun. h. 93 cm Rome, Musei Capitolini
Dying Gaul - The Dying Galatian - “” Dying Galatian Warrior”” Marble sculpture of Ludovisi Group after original bronze from 220-210 BC. Sun. h. 93 cm Rome, Musei Capitolini

LRI4625343: Dying Gaul - The Dying Galatian - “” Dying Galatian Warrior”” Marble sculpture of Ludovisi Group after original bronze from 220-210 BC. Sun. h. 93 cm Rome, Musei Capitolini, Roman, (1st century AD) / Bridgeman Images

ID: LRI4625343

Dying Gaul - The Dying Galatian - “” Dying Galatian Warrior”” Marble sculpture of Ludovisi Group after original bronze from 220-210 BC. Sun. h. 93 cm Rome, Musei Capitolini

Roman, (1st century AD)

The site of the Musee des Monuments Francais, Cite de l'architecture et du patrimoine, Palais de Chaillot, 1 place du Trocadero, Paris 16th. All the renovation and renovation works were entrusted to the architect Jean Francois Bodin, at the end of 2007. Photography 2003.
The site of the Musee des Monuments Francais, Cite de l'architecture et du patrimoine, Palais de Chaillot, 1 place du Trocadero, Paris 16th. All the renovation and renovation works were entrusted to the architect Jean Francois Bodin, at the end of 2007. Photography 2003.

JSN4625394: The site of the Musee des Monuments Francais, Cite de l'architecture et du patrimoine, Palais de Chaillot, 1 place du Trocadero, Paris 16th. All the renovation and renovation works were entrusted to the architect Jean Francois Bodin, at the end of 2007. Photography 2003., Salmon, Jacqueline / Bridgeman Images

ID: JSN4625394

The site of the Musee des Monuments Francais, Cite de l'architecture et du patrimoine, Palais de Chaillot, 1 place du Trocadero, Paris 16th. All the renovation and renovation works were entrusted to the architect Jean Francois Bodin, at the end of 2007. Photography 2003.

Salmon, Jacqueline

Illustration from the book
Illustration from the book

JLJ4625425: Illustration from the book "Le bon roy Henri": Portrait of Charles de Lorraine (1554-1611) (litho), Job, pseudonym for Onfray de Breville, Jacques (1858-1931) / Bridgeman Images

ID: JLJ4625425

Illustration from the book "Le bon roy Henri": Portrait of Charles de Lorraine (1554-1611) (litho)

Job, pseudonym for Onfray de Breville, Jacques (1858-1931)

The site of the Musee des Monuments Francais, Cite de l'architecture et du patrimoine, Palais de Chaillot, 1 place du Trocadero, Paris 16th. All the renovation and renovation works were entrusted to the architect Jean Francois Bodin, at the end of 2007. Photography 2003.
The site of the Musee des Monuments Francais, Cite de l'architecture et du patrimoine, Palais de Chaillot, 1 place du Trocadero, Paris 16th. All the renovation and renovation works were entrusted to the architect Jean Francois Bodin, at the end of 2007. Photography 2003.

JSN4625434: The site of the Musee des Monuments Francais, Cite de l'architecture et du patrimoine, Palais de Chaillot, 1 place du Trocadero, Paris 16th. All the renovation and renovation works were entrusted to the architect Jean Francois Bodin, at the end of 2007. Photography 2003., Salmon, Jacqueline / Bridgeman Images

ID: JSN4625434

The site of the Musee des Monuments Francais, Cite de l'architecture et du patrimoine, Palais de Chaillot, 1 place du Trocadero, Paris 16th. All the renovation and renovation works were entrusted to the architect Jean Francois Bodin, at the end of 2007. Photography 2003.

Salmon, Jacqueline

The site of the Musee des Monuments Francais, Cite de l'architecture et du patrimoine, Palais de Chaillot, 1 place du Trocadero, Paris 16th. All the renovation and renovation works were entrusted to the architect Jean Francois Bodin, at the end of 2007. Photography 2003.
The site of the Musee des Monuments Francais, Cite de l'architecture et du patrimoine, Palais de Chaillot, 1 place du Trocadero, Paris 16th. All the renovation and renovation works were entrusted to the architect Jean Francois Bodin, at the end of 2007. Photography 2003.

JSN4625468: The site of the Musee des Monuments Francais, Cite de l'architecture et du patrimoine, Palais de Chaillot, 1 place du Trocadero, Paris 16th. All the renovation and renovation works were entrusted to the architect Jean Francois Bodin, at the end of 2007. Photography 2003., Salmon, Jacqueline / Bridgeman Images

ID: JSN4625468

The site of the Musee des Monuments Francais, Cite de l'architecture et du patrimoine, Palais de Chaillot, 1 place du Trocadero, Paris 16th. All the renovation and renovation works were entrusted to the architect Jean Francois Bodin, at the end of 2007. Photography 2003.

Salmon, Jacqueline

The site of the Musee des Monuments Francais, Cite de l'architecture et du patrimoine, Palais de Chaillot, 1 place du Trocadero, Paris 16th. All the renovation and renovation works were entrusted to the architect Jean Francois Bodin, at the end of 2007. Photography 2003.
The site of the Musee des Monuments Francais, Cite de l'architecture et du patrimoine, Palais de Chaillot, 1 place du Trocadero, Paris 16th. All the renovation and renovation works were entrusted to the architect Jean Francois Bodin, at the end of 2007. Photography 2003.

JSN4625487: The site of the Musee des Monuments Francais, Cite de l'architecture et du patrimoine, Palais de Chaillot, 1 place du Trocadero, Paris 16th. All the renovation and renovation works were entrusted to the architect Jean Francois Bodin, at the end of 2007. Photography 2003., Salmon, Jacqueline / Bridgeman Images

ID: JSN4625487

The site of the Musee des Monuments Francais, Cite de l'architecture et du patrimoine, Palais de Chaillot, 1 place du Trocadero, Paris 16th. All the renovation and renovation works were entrusted to the architect Jean Francois Bodin, at the end of 2007. Photography 2003.

Salmon, Jacqueline

Tethys, Saturn satellite, seen by the Cassini probe - Saturn's moon Tethys seen by Cassini spacecraft - The southern pole of the Tethys satellite photographed by the Cassini probe on September 24, 2005. Mosaic of nine images. With this full - disk mosaic, Cassini presents the best view yet of the south pole of Saturn's moon Tethys. The giant rift Ithaca Chasma cuts across the disk. Much of the topography seen here, including that of Ithaca Chasma, has a soft, muted appearance. It is clearly very old and has been heavily bombarded by impacts over time. Many of the fresh - appearing craters (ones with crisp relief) exhibit unusually bright crater floors. The origin of the apparent brightness (or “” albedo”) contrast is not known. It is possible that impacts punched through to a brighter layer underneath, or perhaps it is brighter because of different grain sizes or textures of the crater floor material in comparison to material along the crater walls and surrounding surface. The moon's high southern latitudes, seen here at the bottom, were not imaged by Nasa's Voyager spacecraft during their flybys of Tethys 25 years ago. The mosaic is composed of nine images taken during Cassini's close flyby of Tethys (1,071 kilometers, or 665 miles across) on Sept. 24, 2005, during which the spacecraft passed approximately 1,500 kilometers (930 miles) above the Moon's surface. This view is centered on terrain at approximately 1.2 degrees south latitude and 342 degrees west longitude on Tethys. It has been rotated so that north is up. The clear filter images in this mosaic were taken with the Cassini spacecraft narrow - angle camera at distances ranging from 71,600 kilometers (44,500 miles) to 62,400 kilometers (38,800 miles) from Tethys and at a Sun - Tethys - spacecraft, or phase, angle of 21 degrees. The image scale is 370 meters (1,200 feet) per pixel
Tethys, Saturn satellite, seen by the Cassini probe - Saturn's moon Tethys seen by Cassini spacecraft - The southern pole of the Tethys satellite photographed by the Cassini probe on September 24, 2005. Mosaic of nine images. With this full - disk mosaic, Cassini presents the best view yet of the south pole of Saturn's moon Tethys. The giant rift Ithaca Chasma cuts across the disk. Much of the topography seen here, including that of Ithaca Chasma, has a soft, muted appearance. It is clearly very old and has been heavily bombarded by impacts over time. Many of the fresh - appearing craters (ones with crisp relief) exhibit unusually bright crater floors. The origin of the apparent brightness (or “” albedo”) contrast is not known. It is possible that impacts punched through to a brighter layer underneath, or perhaps it is brighter because of different grain sizes or textures of the crater floor material in comparison to material along the crater walls and surrounding surface. The moon's high southern latitudes, seen here at the bottom, were not imaged by Nasa's Voyager spacecraft during their flybys of Tethys 25 years ago. The mosaic is composed of nine images taken during Cassini's close flyby of Tethys (1,071 kilometers, or 665 miles across) on Sept. 24, 2005, during which the spacecraft passed approximately 1,500 kilometers (930 miles) above the Moon's surface. This view is centered on terrain at approximately 1.2 degrees south latitude and 342 degrees west longitude on Tethys. It has been rotated so that north is up. The clear filter images in this mosaic were taken with the Cassini spacecraft narrow - angle camera at distances ranging from 71,600 kilometers (44,500 miles) to 62,400 kilometers (38,800 miles) from Tethys and at a Sun - Tethys - spacecraft, or phase, angle of 21 degrees. The image scale is 370 meters (1,200 feet) per pixel

PIX4625583: Tethys, Saturn satellite, seen by the Cassini probe - Saturn's moon Tethys seen by Cassini spacecraft - The southern pole of the Tethys satellite photographed by the Cassini probe on September 24, 2005. Mosaic of nine images. With this full - disk mosaic, Cassini presents the best view yet of the south pole of Saturn's moon Tethys. The giant rift Ithaca Chasma cuts across the disk. Much of the topography seen here, including that of Ithaca Chasma, has a soft, muted appearance. It is clearly very old and has been heavily bombarded by impacts over time. Many of the fresh - appearing craters (ones with crisp relief) exhibit unusually bright crater floors. The origin of the apparent brightness (or “” albedo”) contrast is not known. It is possible that impacts punched through to a brighter layer underneath, or perhaps it is brighter because of different grain sizes or textures of the crater floor material in comparison to material along the crater walls and surrounding surface. The moon's high southern latitudes, seen here at the bottom, were not imaged by Nasa's Voyager spacecraft during their flybys of Tethys 25 years ago. The mosaic is composed of nine images taken during Cassini's close flyby of Tethys (1,071 kilometers, or 665 miles across) on Sept. 24, 2005, during which the spacecraft passed approximately 1,500 kilometers (930 miles) above the Moon's surface. This view is centered on terrain at approximately 1.2 degrees south latitude and 342 degrees west longitude on Tethys. It has been rotated so that north is up. The clear filter images in this mosaic were taken with the Cassini spacecraft narrow - angle camera at distances ranging from 71,600 kilometers (44,500 miles) to 62,400 kilometers (38,800 miles) from Tethys and at a Sun - Tethys - spacecraft, or phase, angle of 21 degrees. The image scale is 370 meters (1,200 feet) per pixel / Bridgeman Images

ID: PIX4625583

Tethys, Saturn satellite, seen by the Cassini probe - Saturn's moon Tethys seen by Cassini spacecraft - The southern pole of the Tethys satellite photographed by the Cassini probe on September 24, 2005. Mosaic of nine images. With this full - disk mosaic, Cassini presents the best view yet of the south pole of Saturn's moon Tethys. The giant rift Ithaca Chasma cuts across the disk. Much of the topography seen here, including that of Ithaca Chasma, has a soft, muted appearance. It is clearly very old and has been heavily bombarded by impacts over time. Many of the fresh - appearing craters (ones with crisp relief) exhibit unusually bright crater floors. The origin of the apparent brightness (or “” albedo”) contrast is not known. It is possible that impacts punched through to a brighter layer underneath, or perhaps it is brighter because of different grain sizes or textures of the crater floor material in comparison to material along the crater walls and surrounding surface. The moon's h

Tethys, Saturn satellite, seen by the Cassini probe - Saturn's moon Tethys seen by Cassini spacecraft: The Tethys satellite photographed by the Cassini probe on 11 April 2015 has a distance of 53,000 km from the satellite. Tethys is about 1070 km in diameter. - This enhancement-color mosaic of Saturn's icy moon Tethys shows a range of features on the moon's trailing hemisphere. Tethys is tidally locked to Saturn, so the trailing hemisphere is the side of the moon that always faces opposite its direction of motion as it orbits the planet - Images taken using clear, green, infrared and ultraviolet spectral filters were combined to create the view, which highlights subtle color differences across Tethys' surface at wavelengths not visible to human eyes. The moon's surface is fairly uniform in natural color - The color of the surface changes conspicuously across the disk, from yellowish hues to nearly white. These broad color changes are affected by a number of external processes. First, Saturn's diffuse E-ring preferentially bombards Tethys' leading hemisphere, towards the right side of this image, with ice bright ice grains. At the same time, charged particles from Saturn's radiation belt bombard the surface on the trailing side, causing color changes due to chemical alteration of the materials there. The albedo - a measure of the surface's reflectivity - drops by 10 to 15 percent from the moon's leading side to the trailing side. Similar global color patterns exist on other Saturnian moons - Mountains on the floor of the 280 mile- (450 km-) wide Odysseus impact basin are visible at upper right, around the two o'clock position - This mosaic is an orthographic projection constructed from 52 Cassini images obtained on April 11, 2015 with the Cassini spacecraft narrow-angle camera. Resolution is about 1,000 feet (300 meters) per pixel. The images were obtained at a distance of approximately 33,000 miles (53,000 kilometers) from Tethys
Tethys, Saturn satellite, seen by the Cassini probe - Saturn's moon Tethys seen by Cassini spacecraft: The Tethys satellite photographed by the Cassini probe on 11 April 2015 has a distance of 53,000 km from the satellite. Tethys is about 1070 km in diameter. - This enhancement-color mosaic of Saturn's icy moon Tethys shows a range of features on the moon's trailing hemisphere. Tethys is tidally locked to Saturn, so the trailing hemisphere is the side of the moon that always faces opposite its direction of motion as it orbits the planet - Images taken using clear, green, infrared and ultraviolet spectral filters were combined to create the view, which highlights subtle color differences across Tethys' surface at wavelengths not visible to human eyes. The moon's surface is fairly uniform in natural color - The color of the surface changes conspicuously across the disk, from yellowish hues to nearly white. These broad color changes are affected by a number of external processes. First, Saturn's diffuse E-ring preferentially bombards Tethys' leading hemisphere, towards the right side of this image, with ice bright ice grains. At the same time, charged particles from Saturn's radiation belt bombard the surface on the trailing side, causing color changes due to chemical alteration of the materials there. The albedo - a measure of the surface's reflectivity - drops by 10 to 15 percent from the moon's leading side to the trailing side. Similar global color patterns exist on other Saturnian moons - Mountains on the floor of the 280 mile- (450 km-) wide Odysseus impact basin are visible at upper right, around the two o'clock position - This mosaic is an orthographic projection constructed from 52 Cassini images obtained on April 11, 2015 with the Cassini spacecraft narrow-angle camera. Resolution is about 1,000 feet (300 meters) per pixel. The images were obtained at a distance of approximately 33,000 miles (53,000 kilometers) from Tethys

PIX4625616: Tethys, Saturn satellite, seen by the Cassini probe - Saturn's moon Tethys seen by Cassini spacecraft: The Tethys satellite photographed by the Cassini probe on 11 April 2015 has a distance of 53,000 km from the satellite. Tethys is about 1070 km in diameter. - This enhancement-color mosaic of Saturn's icy moon Tethys shows a range of features on the moon's trailing hemisphere. Tethys is tidally locked to Saturn, so the trailing hemisphere is the side of the moon that always faces opposite its direction of motion as it orbits the planet - Images taken using clear, green, infrared and ultraviolet spectral filters were combined to create the view, which highlights subtle color differences across Tethys' surface at wavelengths not visible to human eyes. The moon's surface is fairly uniform in natural color - The color of the surface changes conspicuously across the disk, from yellowish hues to nearly white. These broad color changes are affected by a number of external processes. First, Saturn's diffuse E-ring preferentially bombards Tethys' leading hemisphere, towards the right side of this image, with ice bright ice grains. At the same time, charged particles from Saturn's radiation belt bombard the surface on the trailing side, causing color changes due to chemical alteration of the materials there. The albedo - a measure of the surface's reflectivity - drops by 10 to 15 percent from the moon's leading side to the trailing side. Similar global color patterns exist on other Saturnian moons - Mountains on the floor of the 280 mile- (450 km-) wide Odysseus impact basin are visible at upper right, around the two o'clock position - This mosaic is an orthographic projection constructed from 52 Cassini images obtained on April 11, 2015 with the Cassini spacecraft narrow-angle camera. Resolution is about 1,000 feet (300 meters) per pixel. The images were obtained at a distance of approximately 33,000 miles (53,000 kilometers) from Tethys / Bridgeman Images

ID: PIX4625616

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

Artist's view of the planet Saturn
Artist's view of the planet Saturn

PIX4625707: Artist's view of the planet Saturn / Bridgeman Images

ID: PIX4625707

Artist's view of the planet Saturn

Housing building, Avenue de Versailles, Paris 16th arrondissement.
Housing building, Avenue de Versailles, Paris 16th arrondissement.

MDA4626252: Housing building, Avenue de Versailles, Paris 16th arrondissement., Denance, Michel / Bridgeman Images

ID: MDA4626252

Housing building, Avenue de Versailles, Paris 16th arrondissement.

Denance, Michel

Housing building, Avenue Dode de de la Brunerie, Paris 16th arrondissement.
Housing building, Avenue Dode de de la Brunerie, Paris 16th arrondissement.

MDA4626259: Housing building, Avenue Dode de de la Brunerie, Paris 16th arrondissement., Denance, Michel / Bridgeman Images

ID: MDA4626259

Housing building, Avenue Dode de de la Brunerie, Paris 16th arrondissement.

Denance, Michel

Gothic Art: detail of the central portal of the Cathedrale Notre Dame de Paris, (1163-1330), Paris
Gothic Art: detail of the central portal of the Cathedrale Notre Dame de Paris, (1163-1330), Paris

LRI4626274: Gothic Art: detail of the central portal of the Cathedrale Notre Dame de Paris, (1163-1330), Paris, Unknown Artist, (14th century) / Bridgeman Images

ID: LRI4626274

Gothic Art: detail of the central portal of the Cathedrale Notre Dame de Paris, (1163-1330), Paris

Unknown Artist, (14th century)

Vue de l'Hotel-Dieu (Hotel Dieu) hospital realized between 1866 and 1878 on the Ile de la Cite in Paris.
Vue de l'Hotel-Dieu (Hotel Dieu) hospital realized between 1866 and 1878 on the Ile de la Cite in Paris.

LRI4626285: Vue de l'Hotel-Dieu (Hotel Dieu) hospital realized between 1866 and 1878 on the Ile de la Cite in Paris., French School, (19th century) / Bridgeman Images

ID: LRI4626285

Vue de l'Hotel-Dieu (Hotel Dieu) hospital realized between 1866 and 1878 on the Ile de la Cite in Paris.

French School, (19th century)

View of the fountain made by Jacques Ignace Hittorff and the obelic of Place de la Concorde in Paris.
View of the fountain made by Jacques Ignace Hittorff and the obelic of Place de la Concorde in Paris.

LRI4626296: View of the fountain made by Jacques Ignace Hittorff and the obelic of Place de la Concorde in Paris., Hittorff, Jacques Ignace (1792-1867) / Bridgeman Images

ID: LRI4626296

View of the fountain made by Jacques Ignace Hittorff and the obelic of Place de la Concorde in Paris.

Hittorff, Jacques Ignace (1792-1867)

View of the Arc de Triomphe realized by Jean Francois Chalgrin (1739-1811) between 1806 and 1836 on the Place de l'Etoile in Paris
View of the Arc de Triomphe realized by Jean Francois Chalgrin (1739-1811) between 1806 and 1836 on the Place de l'Etoile in Paris

LRI4626329: View of the Arc de Triomphe realized by Jean Francois Chalgrin (1739-1811) between 1806 and 1836 on the Place de l'Etoile in Paris, Chalgrin, Jean Francois Therese (1739-1811) / Bridgeman Images

ID: LRI4626329

View of the Arc de Triomphe realized by Jean Francois Chalgrin (1739-1811) between 1806 and 1836 on the Place de l'Etoile in Paris

Chalgrin, Jean Francois Therese (1739-1811)

“The Memorial of Saint Helene
“The Memorial of Saint Helene

JLJ4626214: “The Memorial of Saint Helene": Portrait of Pierre Andre de Suffren (1729-1788) (litho), Bombled, Louis Charles (1862-1927) / Bridgeman Images

ID: JLJ4626214

“The Memorial of Saint Helene": Portrait of Pierre Andre de Suffren (1729-1788) (litho)

Bombled, Louis Charles (1862-1927)

“The Memorial se Sainte Helene
“The Memorial se Sainte Helene

JLJ4626368: “The Memorial se Sainte Helene": Hudson Lowe (1769-1844) makes the papers of Las Cases searched (litho), Bombled, Louis Charles (1862-1927) / Bridgeman Images

ID: JLJ4626368

“The Memorial se Sainte Helene": Hudson Lowe (1769-1844) makes the papers of Las Cases searched (litho)

Bombled, Louis Charles (1862-1927)

Saturn seen from its satellite Japet - Saturn from Iapetus - The planet Saturn accompanied by three satellites (from left to right Tethys, Rhea and Dione) seen from the icy surface of Japet. In this image Saturn dominates Iapetus' velvet black sky framed by three inner moons. Left to right are Tethys, Rhea and Dione. Less than half the size of the Earth's moon, ice - covered Iapetus is one of the few places in the Solar System that offers a good view of Saturn's rings. This is because Iapetus' orbit is inclined almost 15 degrees to Saturn's equator. With the exception of Phoebe, none of Saturn's other satellites offer such a vantage point. Unlike haze - shrouded Titan, Iapetus has no atmosphere to speak of and is believed to be composed almost entirely of water ice
Saturn seen from its satellite Japet - Saturn from Iapetus - The planet Saturn accompanied by three satellites (from left to right Tethys, Rhea and Dione) seen from the icy surface of Japet. In this image Saturn dominates Iapetus' velvet black sky framed by three inner moons. Left to right are Tethys, Rhea and Dione. Less than half the size of the Earth's moon, ice - covered Iapetus is one of the few places in the Solar System that offers a good view of Saturn's rings. This is because Iapetus' orbit is inclined almost 15 degrees to Saturn's equator. With the exception of Phoebe, none of Saturn's other satellites offer such a vantage point. Unlike haze - shrouded Titan, Iapetus has no atmosphere to speak of and is believed to be composed almost entirely of water ice

PIX4626289: Saturn seen from its satellite Japet - Saturn from Iapetus - The planet Saturn accompanied by three satellites (from left to right Tethys, Rhea and Dione) seen from the icy surface of Japet. In this image Saturn dominates Iapetus' velvet black sky framed by three inner moons. Left to right are Tethys, Rhea and Dione. Less than half the size of the Earth's moon, ice - covered Iapetus is one of the few places in the Solar System that offers a good view of Saturn's rings. This is because Iapetus' orbit is inclined almost 15 degrees to Saturn's equator. With the exception of Phoebe, none of Saturn's other satellites offer such a vantage point. Unlike haze - shrouded Titan, Iapetus has no atmosphere to speak of and is believed to be composed almost entirely of water ice / Bridgeman Images

ID: PIX4626289

Saturn seen from its satellite Japet - Saturn from Iapetus - The planet Saturn accompanied by three satellites (from left to right Tethys, Rhea and Dione) seen from the icy surface of Japet. In this image Saturn dominates Iapetus' velvet black sky framed by three inner moons. Left to right are Tethys, Rhea and Dione. Less than half the size of the Earth's moon, ice - covered Iapetus is one of the few places in the Solar System that offers a good view of Saturn's rings. This is because Iapetus' orbit is inclined almost 15 degrees to Saturn's equator. With the exception of Phoebe, none of Saturn's other satellites offer such a vantage point. Unlike haze - shrouded Titan, Iapetus has no atmosphere to speak of and is believed to be composed almost entirely of water ice

Portrait of Benjamin Franklin (1706-1790), 19th century (oil on canvas)
Portrait of Benjamin Franklin (1706-1790), 19th century (oil on canvas)

JLJ4626421: Portrait of Benjamin Franklin (1706-1790), 19th century (oil on canvas), Healy, George Peter Alexander (1813-1894) / Bridgeman Images

ID: JLJ4626421

Portrait of Benjamin Franklin (1706-1790), 19th century (oil on canvas)

Healy, George Peter Alexander (1813-1894)

Unjust kings are invited by an angel to enter the Underworld 13th Century Orthodox Monastery of Milesevo, Serbia
Unjust kings are invited by an angel to enter the Underworld 13th Century Orthodox Monastery of Milesevo, Serbia

LRI4626452: Unjust kings are invited by an angel to enter the Underworld 13th Century Orthodox Monastery of Milesevo, Serbia, Unknown Artist, (13th century) / Bridgeman Images

ID: LRI4626452

Unjust kings are invited by an angel to enter the Underworld 13th Century Orthodox Monastery of Milesevo, Serbia

Unknown Artist, (13th century)

Illustration from the book
Illustration from the book

JLJ4626484: Illustration from the book "The Memorial of Saint Helene", Mamluk of the Imperiale Guard (litho), Bombled, Louis Charles (1862-1927) / Bridgeman Images

ID: JLJ4626484

Illustration from the book "The Memorial of Saint Helene", Mamluk of the Imperiale Guard (litho)

Bombled, Louis Charles (1862-1927)

Crab Nebula seen in different wavelength - The Crab Nebula in multi wavelength: M1, the Crab Nebula, is the rest of a supernova that exploded on July 4, 1054. It is located about 6500 light years from Earth in the constellation Taurus. At the heart of this nebula is a pulsar. To obtain this photo, different observatories and telescopes combined their observations; the VLA provided the radio image (in red), the Spitzer telescope the infrared image (in yellow), the Hubble telescope for the visible part (here in green), XMM-Newton the ultraviolet image (in blue) and the Chandra telescope for X-ray data (purple). The pulsar is the bright spot in the center of the image. The unusual image was produced by combining data from telescopes spanning almost the entire electromagnetic spectrum, from radio waves to X-rays. The Karl G. Jansky Very Large Array (VLA) provided information about the nebula gathered in the radio regime (colored in red). Nasa's Spitzer Space Telescope took images in the infrared (yellow). The NASA/ESA Hubble Space Telescope provided the images made in optical wavelengths (colored in green). ESA's XMM-Newton telescope observed the Crab Nebula in the ultraviolet (blue) and Nasa's Chandra X-ray Observatory provided the data for X-ray radiation (purple). The Crab Nebula, located 6500 light-years from Earth in the constellation of Taurus, is the result of a supernova explosion which was observed by Chinese and other astronomers in 1054. At its centre is a pulsar: a super-dense neutron star, spinning once every 33 milliseconds, shooting out rotating light-like beams of radio waves and visible light. Surrounding the pulsar lies a mix of material; some of it was originally expelled from the star before it went supernova, and the rest was ejected during the explosion itself. Fast-moving winds of particles fly off from the neutron star, energising the dust and gas around it.
Crab Nebula seen in different wavelength - The Crab Nebula in multi wavelength: M1, the Crab Nebula, is the rest of a supernova that exploded on July 4, 1054. It is located about 6500 light years from Earth in the constellation Taurus. At the heart of this nebula is a pulsar. To obtain this photo, different observatories and telescopes combined their observations; the VLA provided the radio image (in red), the Spitzer telescope the infrared image (in yellow), the Hubble telescope for the visible part (here in green), XMM-Newton the ultraviolet image (in blue) and the Chandra telescope for X-ray data (purple). The pulsar is the bright spot in the center of the image. The unusual image was produced by combining data from telescopes spanning almost the entire electromagnetic spectrum, from radio waves to X-rays. The Karl G. Jansky Very Large Array (VLA) provided information about the nebula gathered in the radio regime (colored in red). Nasa's Spitzer Space Telescope took images in the infrared (yellow). The NASA/ESA Hubble Space Telescope provided the images made in optical wavelengths (colored in green). ESA's XMM-Newton telescope observed the Crab Nebula in the ultraviolet (blue) and Nasa's Chandra X-ray Observatory provided the data for X-ray radiation (purple). The Crab Nebula, located 6500 light-years from Earth in the constellation of Taurus, is the result of a supernova explosion which was observed by Chinese and other astronomers in 1054. At its centre is a pulsar: a super-dense neutron star, spinning once every 33 milliseconds, shooting out rotating light-like beams of radio waves and visible light. Surrounding the pulsar lies a mix of material; some of it was originally expelled from the star before it went supernova, and the rest was ejected during the explosion itself. Fast-moving winds of particles fly off from the neutron star, energising the dust and gas around it.

PIX4626499: Crab Nebula seen in different wavelength - The Crab Nebula in multi wavelength: M1, the Crab Nebula, is the rest of a supernova that exploded on July 4, 1054. It is located about 6500 light years from Earth in the constellation Taurus. At the heart of this nebula is a pulsar. To obtain this photo, different observatories and telescopes combined their observations; the VLA provided the radio image (in red), the Spitzer telescope the infrared image (in yellow), the Hubble telescope for the visible part (here in green), XMM-Newton the ultraviolet image (in blue) and the Chandra telescope for X-ray data (purple). The pulsar is the bright spot in the center of the image. The unusual image was produced by combining data from telescopes spanning almost the entire electromagnetic spectrum, from radio waves to X-rays. The Karl G. Jansky Very Large Array (VLA) provided information about the nebula gathered in the radio regime (colored in red). Nasa's Spitzer Space Telescope took images in the infrared (yellow). The NASA/ESA Hubble Space Telescope provided the images made in optical wavelengths (colored in green). ESA's XMM-Newton telescope observed the Crab Nebula in the ultraviolet (blue) and Nasa's Chandra X-ray Observatory provided the data for X-ray radiation (purple). The Crab Nebula, located 6500 light-years from Earth in the constellation of Taurus, is the result of a supernova explosion which was observed by Chinese and other astronomers in 1054. At its centre is a pulsar: a super-dense neutron star, spinning once every 33 milliseconds, shooting out rotating light-like beams of radio waves and visible light. Surrounding the pulsar lies a mix of material; some of it was originally expelled from the star before it went supernova, and the rest was ejected during the explosion itself. Fast-moving winds of particles fly off from the neutron star, energising the dust and gas around it. / Bridgeman Images

ID: PIX4626499

Crab Nebula seen in different wavelength - The Crab Nebula in multi wavelength: M1, the Crab Nebula, is the rest of a supernova that exploded on July 4, 1054. It is located about 6500 light years from Earth in the constellation Taurus. At the heart of this nebula is a pulsar. To obtain this photo, different observatories and telescopes combined their observations; the VLA provided the radio image (in red), the Spitzer telescope the infrared image (in yellow), the Hubble telescope for the visible part (here in green), XMM-Newton the ultraviolet image (in blue) and the Chandra telescope for X-ray data (purple). The pulsar is the bright spot in the center of the image. The unusual image was produced by combining data from telescopes spanning almost the entire electromagnetic spectrum, from radio waves to X-rays. The Karl G. Jansky Very Large Array (VLA) provided information about the nebula gathered in the radio regime (colored in red). Nasa's Spitzer Space Telescope took images in the in

“The Memorial of Saint Helene
“The Memorial of Saint Helene

JLJ4625738: “The Memorial of Saint Helene": Portrait of General Joubert (1769-1799) (litho), Bombled, Louis Charles (1862-1927) / Bridgeman Images

ID: JLJ4625738

“The Memorial of Saint Helene": Portrait of General Joubert (1769-1799) (litho)

Bombled, Louis Charles (1862-1927)

Temple of Zeus (photography)
Temple of Zeus (photography)

LRI4625744: Temple of Zeus (photography), Greek / Bridgeman Images

ID: LRI4625744

Temple of Zeus (photography)

Greek

Head of a woman (fragment), from the palace of Tirynthe, 1300 BC (fresco)
Head of a woman (fragment), from the palace of Tirynthe, 1300 BC (fresco)

LRI4625766: Head of a woman (fragment), from the palace of Tirynthe, 1300 BC (fresco), Mycenaean, (14th century BC) / Bridgeman Images

ID: LRI4625766

Head of a woman (fragment), from the palace of Tirynthe, 1300 BC (fresco)

Mycenaean, (14th century BC)

Artist's view of the ice fountains on Enceladus - Artist's view of the ice jets on the surface of the Encelade satellite observed by the Cassini probe. It would appear that these particles feed the E ring of Saturn, which was previously unknown
Artist's view of the ice fountains on Enceladus - Artist's view of the ice jets on the surface of the Encelade satellite observed by the Cassini probe. It would appear that these particles feed the E ring of Saturn, which was previously unknown

PIX4625788: Artist's view of the ice fountains on Enceladus - Artist's view of the ice jets on the surface of the Encelade satellite observed by the Cassini probe. It would appear that these particles feed the E ring of Saturn, which was previously unknown / Bridgeman Images

ID: PIX4625788

Artist's view of the ice fountains on Enceladus - Artist's view of the ice jets on the surface of the Encelade satellite observed by the Cassini probe. It would appear that these particles feed the E ring of Saturn, which was previously unknown

Gold lion's head rhyton from Grave IV, Mycenae. 16th century BC.
Gold lion's head rhyton from Grave IV, Mycenae. 16th century BC.

LRI4625830: Gold lion's head rhyton from Grave IV, Mycenae. 16th century BC., Mycenaean, (16th century BC) / Bridgeman Images

ID: LRI4625830

Gold lion's head rhyton from Grave IV, Mycenae. 16th century BC.

Mycenaean, (16th century BC)

The site of the Musee des Monuments Francais in Paris. Cite of architecture and heritage, Palais de Chaillot, 1 place du Trocadero, Paris 16th arrondissement. All the renovation and renovation works were entrusted to the architect Jean Francois Bodin, 2007. Photography 2003.
The site of the Musee des Monuments Francais in Paris. Cite of architecture and heritage, Palais de Chaillot, 1 place du Trocadero, Paris 16th arrondissement. All the renovation and renovation works were entrusted to the architect Jean Francois Bodin, 2007. Photography 2003.

JSN4625866: The site of the Musee des Monuments Francais in Paris. Cite of architecture and heritage, Palais de Chaillot, 1 place du Trocadero, Paris 16th arrondissement. All the renovation and renovation works were entrusted to the architect Jean Francois Bodin, 2007. Photography 2003., Salmon, Jacqueline / Bridgeman Images

ID: JSN4625866

The site of the Musee des Monuments Francais in Paris. Cite of architecture and heritage, Palais de Chaillot, 1 place du Trocadero, Paris 16th arrondissement. All the renovation and renovation works were entrusted to the architect Jean Francois Bodin, 2007. Photography 2003.

Salmon, Jacqueline

Illustration for 'The Memorial of Saint Helene' by Count Emmanuel de Las Cases (lithograph)
Illustration for 'The Memorial of Saint Helene' by Count Emmanuel de Las Cases (lithograph)

JLJ4625972: Illustration for 'The Memorial of Saint Helene' by Count Emmanuel de Las Cases (lithograph), Bombled, Louis Charles (1862-1927) / Bridgeman Images

ID: JLJ4625972

Illustration for 'The Memorial of Saint Helene' by Count Emmanuel de Las Cases (lithograph)

Bombled, Louis Charles (1862-1927)

The Decorative Art Collection of the Musee d'Art Moderne de la Ville de Paris, Avenue du President Wilson, Paris 75016. Architecture by Jean-Claude Dondel, Andre Aubert, Paul Viard and Marcel Dastugue, 1937. Artist Jean Dunand (1877 - 1942) and Andre Arbus
The Decorative Art Collection of the Musee d'Art Moderne de la Ville de Paris, Avenue du President Wilson, Paris 75016. Architecture by Jean-Claude Dondel, Andre Aubert, Paul Viard and Marcel Dastugue, 1937. Artist Jean Dunand (1877 - 1942) and Andre Arbus

ITR4626547: The Decorative Art Collection of the Musee d'Art Moderne de la Ville de Paris, Avenue du President Wilson, Paris 75016. Architecture by Jean-Claude Dondel, Andre Aubert, Paul Viard and Marcel Dastugue, 1937. Artist Jean Dunand (1877 - 1942) and Andre Arbus, Lemaitre, Pascal / Bridgeman Images

ID: ITR4626547

The Decorative Art Collection of the Musee d'Art Moderne de la Ville de Paris, Avenue du President Wilson, Paris 75016. Architecture by Jean-Claude Dondel, Andre Aubert, Paul Viard and Marcel Dastugue, 1937. Artist Jean Dunand (1877 - 1942) and Andre Arbus

Lemaitre, Pascal

“The Memorial of Saint Helene
“The Memorial of Saint Helene

JLJ4626617: “The Memorial of Saint Helene": English Armee: Scottish Dragons (scotch greys) (litho), Bombled, Louis Charles (1862-1927) / Bridgeman Images

ID: JLJ4626617

“The Memorial of Saint Helene": English Armee: Scottish Dragons (scotch greys) (litho)

Bombled, Louis Charles (1862-1927)

“The Memorial of Saint Helene
“The Memorial of Saint Helene

JLJ4626766: “The Memorial of Saint Helene": Portrait of the marechal Jean Mathieu Philibert Serurier (1742-1819) (litho), Bombled, Louis Charles (1862-1927) / Bridgeman Images

ID: JLJ4626766

“The Memorial of Saint Helene": Portrait of the marechal Jean Mathieu Philibert Serurier (1742-1819) (litho)

Bombled, Louis Charles (1862-1927)

Theological virtues and Hercules on the left Detail of sculpted groups supporting the pulpit. Marble sculpture by Giovanni Pisano (1248-1314). 1302-1311 Cathedrale of Pisa (Duomo di Santa Maria Assunta di Pisa), Italy
Theological virtues and Hercules on the left Detail of sculpted groups supporting the pulpit. Marble sculpture by Giovanni Pisano (1248-1314). 1302-1311 Cathedrale of Pisa (Duomo di Santa Maria Assunta di Pisa), Italy

LRI4626780: Theological virtues and Hercules on the left Detail of sculpted groups supporting the pulpit. Marble sculpture by Giovanni Pisano (1248-1314). 1302-1311 Cathedrale of Pisa (Duomo di Santa Maria Assunta di Pisa), Italy, Pisano, Giovanni (c.1245-p.1314) / Bridgeman Images

ID: LRI4626780

Theological virtues and Hercules on the left Detail of sculpted groups supporting the pulpit. Marble sculpture by Giovanni Pisano (1248-1314). 1302-1311 Cathedrale of Pisa (Duomo di Santa Maria Assunta di Pisa), Italy

Pisano, Giovanni (c.1245-p.1314)

Solar protuberance seen in ultraviolet by SOHO on 25 - 10 - 2002 - A protuberance, a plasma cloud, escapes from the Sun
Solar protuberance seen in ultraviolet by SOHO on 25 - 10 - 2002 - A protuberance, a plasma cloud, escapes from the Sun

PIX4626906: Solar protuberance seen in ultraviolet by SOHO on 25 - 10 - 2002 - A protuberance, a plasma cloud, escapes from the Sun / Bridgeman Images

ID: PIX4626906

Solar protuberance seen in ultraviolet by SOHO on 25 - 10 - 2002 - A protuberance, a plasma cloud, escapes from the Sun

Le Soleil 12/04/2003 seen by SOHO - Le Soleil 12/04/2003 seen by SOHO - Le Soleil 12/04/2003 seen by SOHO in the band centree on 284 A, the ray emailed by the ion Fe X
Le Soleil 12/04/2003 seen by SOHO - Le Soleil 12/04/2003 seen by SOHO - Le Soleil 12/04/2003 seen by SOHO in the band centree on 284 A, the ray emailed by the ion Fe X

PIX4626948: Le Soleil 12/04/2003 seen by SOHO - Le Soleil 12/04/2003 seen by SOHO - Le Soleil 12/04/2003 seen by SOHO in the band centree on 284 A, the ray emailed by the ion Fe X / Bridgeman Images

ID: PIX4626948

Le Soleil 12/04/2003 seen by SOHO - Le Soleil 12/04/2003 seen by SOHO - Le Soleil 12/04/2003 seen by SOHO in the band centree on 284 A, the ray emailed by the ion Fe X

Astronauts on Titan - Illustration - Releasing a weather balloon on Titan - Astronauts make meteorological measurements on the surface of Titan. A titanian explorer prepares to release a weather balloon while another direct a flood lamp to illuminate the activity. On the left is a supply cart with a portable weather station, featuring an interactive control panel designed to accommodate hands enclosed in thick gloves. All exposed hardware would have to function at temperatures of minus 300* F and below. With an atmosphere 10 times denser than the Earth's, weather would be of keen interest to Titan's visitors. High in Titan's atmosphere wind velocities in excess of 400 mph have been detected. While not much is known about winds and weather at Triton's surface, terrain features resembling dune fields have been observed, suggesting surface winds have occurred at some locations. Fogs of methane gas would likely be present at the surface as well
Astronauts on Titan - Illustration - Releasing a weather balloon on Titan - Astronauts make meteorological measurements on the surface of Titan. A titanian explorer prepares to release a weather balloon while another direct a flood lamp to illuminate the activity. On the left is a supply cart with a portable weather station, featuring an interactive control panel designed to accommodate hands enclosed in thick gloves. All exposed hardware would have to function at temperatures of minus 300* F and below. With an atmosphere 10 times denser than the Earth's, weather would be of keen interest to Titan's visitors. High in Titan's atmosphere wind velocities in excess of 400 mph have been detected. While not much is known about winds and weather at Triton's surface, terrain features resembling dune fields have been observed, suggesting surface winds have occurred at some locations. Fogs of methane gas would likely be present at the surface as well

PIX4626113: Astronauts on Titan - Illustration - Releasing a weather balloon on Titan - Astronauts make meteorological measurements on the surface of Titan. A titanian explorer prepares to release a weather balloon while another direct a flood lamp to illuminate the activity. On the left is a supply cart with a portable weather station, featuring an interactive control panel designed to accommodate hands enclosed in thick gloves. All exposed hardware would have to function at temperatures of minus 300* F and below. With an atmosphere 10 times denser than the Earth's, weather would be of keen interest to Titan's visitors. High in Titan's atmosphere wind velocities in excess of 400 mph have been detected. While not much is known about winds and weather at Triton's surface, terrain features resembling dune fields have been observed, suggesting surface winds have occurred at some locations. Fogs of methane gas would likely be present at the surface as well / Bridgeman Images

ID: PIX4626113

Astronauts on Titan - Illustration - Releasing a weather balloon on Titan - Astronauts make meteorological measurements on the surface of Titan. A titanian explorer prepares to release a weather balloon while another direct a flood lamp to illuminate the activity. On the left is a supply cart with a portable weather station, featuring an interactive control panel designed to accommodate hands enclosed in thick gloves. All exposed hardware would have to function at temperatures of minus 300* F and below. With an atmosphere 10 times denser than the Earth's, weather would be of keen interest to Titan's visitors. High in Titan's atmosphere wind velocities in excess of 400 mph have been detected. While not much is known about winds and weather at Triton's surface, terrain features resembling dune fields have been observed, suggesting surface winds have occurred at some locations. Fogs of methane gas would likely be present at the surface as well


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