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French and Germans, Anecdotal History of the War of 1870-1871, 1888 (engraving)
French and Germans, Anecdotal History of the War of 1870-1871, 1888 (engraving)

JLJ4635874: French and Germans, Anecdotal History of the War of 1870-1871, 1888 (engraving), Lonlay, Dick de (Hardouin Georges pseud.) (1846-1893) / Bridgeman Images

ID: JLJ4635874

French and Germans, Anecdotal History of the War of 1870-1871, 1888 (engraving)

Lonlay, Dick de (Hardouin Georges pseud.) (1846-1893)

La voie lactee de l'Aigle à la Carene. - Extreme wide angle view of the Milky Way, from Aquila to Carina, including the Galactic Centre, Southern Cross, Antares - and jupite
La voie lactee de l'Aigle à la Carene. - Extreme wide angle view of the Milky Way, from Aquila to Carina, including the Galactic Centre, Southern Cross, Antares - and jupite

PIX4635793: La voie lactee de l'Aigle à la Carene. - Extreme wide angle view of the Milky Way, from Aquila to Carina, including the Galactic Centre, Southern Cross, Antares - and jupite / Bridgeman Images

ID: PIX4635793

La voie lactee de l'Aigle à la Carene. - Extreme wide angle view of the Milky Way, from Aquila to Carina, including the Galactic Centre, Southern Cross, Antares - and jupite

Marina City, The River, Chicago, USA. Architect Bertrand Goldberg, 1964-1967. Photography 10/04/90.
Marina City, The River, Chicago, USA. Architect Bertrand Goldberg, 1964-1967. Photography 10/04/90.

TEC4635856: Marina City, The River, Chicago, USA. Architect Bertrand Goldberg, 1964-1967. Photography 10/04/90. / Bridgeman Images

ID: TEC4635856

Marina City, The River, Chicago, USA. Architect Bertrand Goldberg, 1964-1967. Photography 10/04/90.

Aurora on Saturn by Hubble - 01 - 2004 - Evolution of a Southern Aurora seen in ultraviolet (and Saturn seen in visible) by the Hubble Space Telescope on 24 (bottom), 26 and 28 January (top) 2004
Aurora on Saturn by Hubble - 01 - 2004 - Evolution of a Southern Aurora seen in ultraviolet (and Saturn seen in visible) by the Hubble Space Telescope on 24 (bottom), 26 and 28 January (top) 2004

PIX4624873: Aurora on Saturn by Hubble - 01 - 2004 - Evolution of a Southern Aurora seen in ultraviolet (and Saturn seen in visible) by the Hubble Space Telescope on 24 (bottom), 26 and 28 January (top) 2004 / Bridgeman Images

ID: PIX4624873

Aurora on Saturn by Hubble - 01 - 2004 - Evolution of a Southern Aurora seen in ultraviolet (and Saturn seen in visible) by the Hubble Space Telescope on 24 (bottom), 26 and 28 January (top) 2004

Saturn and satellites seen by the Hubble space telescope - Saturn rings edge - on with satellites - Saturn observed by the Hubble space telescope on February 24, 2009 when the Earth is in the same plane as the rings, seen by the slice. This phenomene occurs every 15 years. This sequence of images taken for just over three hours shows the movement from left to right of four satellites in front of the planet. From left to right on the top image we see the satellites Enceladus, Dione (the brightest ice satellite), Mimas and the largest satellite, Titan, orange. This sequence of images captures the parade of several of Saturn's moons transiting the face of the gas giant planet from left to right during more than three hours. This is a rare event because the rings are tilted edge on to Earth every 15 years. The top frame captures the giant moon Titan and its shadow near Saturn's northern polar hood. Tiny Mimas and its shadow have just entered the left limb of Saturn, slightly above the rings. To the far left off the disk, Dione, the brightest of the icy moons in this view - and Enceladus, fainter and farther to the left - can easily be seen just above the rings. This picture sequence was taken with Hubble's Wide Field Planetary Camera 2 on February 24, 2009, when Saturn was at a distance of roughly 775 million miles (1.25 billion kilometers) from Earth. Hubble can see details as small as 190 miles (300 km) across on Saturn
Saturn and satellites seen by the Hubble space telescope - Saturn rings edge - on with satellites - Saturn observed by the Hubble space telescope on February 24, 2009 when the Earth is in the same plane as the rings, seen by the slice. This phenomene occurs every 15 years. This sequence of images taken for just over three hours shows the movement from left to right of four satellites in front of the planet. From left to right on the top image we see the satellites Enceladus, Dione (the brightest ice satellite), Mimas and the largest satellite, Titan, orange. This sequence of images captures the parade of several of Saturn's moons transiting the face of the gas giant planet from left to right during more than three hours. This is a rare event because the rings are tilted edge on to Earth every 15 years. The top frame captures the giant moon Titan and its shadow near Saturn's northern polar hood. Tiny Mimas and its shadow have just entered the left limb of Saturn, slightly above the rings. To the far left off the disk, Dione, the brightest of the icy moons in this view - and Enceladus, fainter and farther to the left - can easily be seen just above the rings. This picture sequence was taken with Hubble's Wide Field Planetary Camera 2 on February 24, 2009, when Saturn was at a distance of roughly 775 million miles (1.25 billion kilometers) from Earth. Hubble can see details as small as 190 miles (300 km) across on Saturn

PIX4624891: Saturn and satellites seen by the Hubble space telescope - Saturn rings edge - on with satellites - Saturn observed by the Hubble space telescope on February 24, 2009 when the Earth is in the same plane as the rings, seen by the slice. This phenomene occurs every 15 years. This sequence of images taken for just over three hours shows the movement from left to right of four satellites in front of the planet. From left to right on the top image we see the satellites Enceladus, Dione (the brightest ice satellite), Mimas and the largest satellite, Titan, orange. This sequence of images captures the parade of several of Saturn's moons transiting the face of the gas giant planet from left to right during more than three hours. This is a rare event because the rings are tilted edge on to Earth every 15 years. The top frame captures the giant moon Titan and its shadow near Saturn's northern polar hood. Tiny Mimas and its shadow have just entered the left limb of Saturn, slightly above the rings. To the far left off the disk, Dione, the brightest of the icy moons in this view - and Enceladus, fainter and farther to the left - can easily be seen just above the rings. This picture sequence was taken with Hubble's Wide Field Planetary Camera 2 on February 24, 2009, when Saturn was at a distance of roughly 775 million miles (1.25 billion kilometers) from Earth. Hubble can see details as small as 190 miles (300 km) across on Saturn / Bridgeman Images

ID: PIX4624891

Saturn and satellites seen by the Hubble space telescope - Saturn rings edge - on with satellites - Saturn observed by the Hubble space telescope on February 24, 2009 when the Earth is in the same plane as the rings, seen by the slice. This phenomene occurs every 15 years. This sequence of images taken for just over three hours shows the movement from left to right of four satellites in front of the planet. From left to right on the top image we see the satellites Enceladus, Dione (the brightest ice satellite), Mimas and the largest satellite, Titan, orange. This sequence of images captures the parade of several of Saturn's moons transiting the face of the gas giant planet from left to right during more than three hours. This is a rare event because the rings are tilted edge on to Earth every 15 years. The top frame captures the giant moon Titan and its shadow near Saturn's northern polar hood. Tiny Mimas and its shadow have just entered the left limb of Saturn, slightly above the ring

Illustration from the book
Illustration from the book

JLJ4624920: Illustration from the book "Jeanne d'Arc", On February 25, 1429 (litho), Semant, Paul de (1855-1915) / Bridgeman Images

ID: JLJ4624920

Illustration from the book "Jeanne d'Arc", On February 25, 1429 (litho)

Semant, Paul de (1855-1915)

Saturn - Rings - by Voyager 2 - 23 - 08 - 1981 - Image in false colors made by the probe Voyager 2 on August 23, 1981 at a distance of 2.7 million km from the planet. This image has been reconstructed from 3 black and white photos taken through the UV, green and orange filters. The contrasts were exaggerated. The C ring, in blue on the image, is actually a gray color. The different colors correspond to differences in the chemical composition of the particles that make up the rings
Saturn - Rings - by Voyager 2 - 23 - 08 - 1981 - Image in false colors made by the probe Voyager 2 on August 23, 1981 at a distance of 2.7 million km from the planet. This image has been reconstructed from 3 black and white photos taken through the UV, green and orange filters. The contrasts were exaggerated. The C ring, in blue on the image, is actually a gray color. The different colors correspond to differences in the chemical composition of the particles that make up the rings

PIX4624947: Saturn - Rings - by Voyager 2 - 23 - 08 - 1981 - Image in false colors made by the probe Voyager 2 on August 23, 1981 at a distance of 2.7 million km from the planet. This image has been reconstructed from 3 black and white photos taken through the UV, green and orange filters. The contrasts were exaggerated. The C ring, in blue on the image, is actually a gray color. The different colors correspond to differences in the chemical composition of the particles that make up the rings / Bridgeman Images

ID: PIX4624947

Saturn - Rings - by Voyager 2 - 23 - 08 - 1981 - Image in false colors made by the probe Voyager 2 on August 23, 1981 at a distance of 2.7 million km from the planet. This image has been reconstructed from 3 black and white photos taken through the UV, green and orange filters. The contrasts were exaggerated. The C ring, in blue on the image, is actually a gray color. The different colors correspond to differences in the chemical composition of the particles that make up the rings

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.

JSN4624962: 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: JSN4624962

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.

JSN4624978: 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: JSN4624978

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

Nebula of the crescent NGC 6888 in the Swan - NGC 6888 Crescent Nebula - NGC 6888 Nebula of the Crescent. This nebula is a gas shell located in the constellation Swan. The bright star in the center of the nebula is the star WR 136, a star of Wolf - Rayet, massive, very hot. Image obtained by combining light through 3 different filters that highlight oxygen, hydrogen, and sulfur. The nebula is a shell of gas that is being energized by the strong stellar wind from the Wolf - Rayet star WR 136, the bright star at the center of the nebula. It is located in the constellation of Cygnus, the Swan. Wolf - Rayet stars are very hot, massive stars that are blowing off their outer layers. Narrowband false color composite H - alpha, OIII, SII
Nebula of the crescent NGC 6888 in the Swan - NGC 6888 Crescent Nebula - NGC 6888 Nebula of the Crescent. This nebula is a gas shell located in the constellation Swan. The bright star in the center of the nebula is the star WR 136, a star of Wolf - Rayet, massive, very hot. Image obtained by combining light through 3 different filters that highlight oxygen, hydrogen, and sulfur. The nebula is a shell of gas that is being energized by the strong stellar wind from the Wolf - Rayet star WR 136, the bright star at the center of the nebula. It is located in the constellation of Cygnus, the Swan. Wolf - Rayet stars are very hot, massive stars that are blowing off their outer layers. Narrowband false color composite H - alpha, OIII, SII

PIX4620372: Nebula of the crescent NGC 6888 in the Swan - NGC 6888 Crescent Nebula - NGC 6888 Nebula of the Crescent. This nebula is a gas shell located in the constellation Swan. The bright star in the center of the nebula is the star WR 136, a star of Wolf - Rayet, massive, very hot. Image obtained by combining light through 3 different filters that highlight oxygen, hydrogen, and sulfur. The nebula is a shell of gas that is being energized by the strong stellar wind from the Wolf - Rayet star WR 136, the bright star at the center of the nebula. It is located in the constellation of Cygnus, the Swan. Wolf - Rayet stars are very hot, massive stars that are blowing off their outer layers. Narrowband false color composite H - alpha, OIII, SII / Bridgeman Images

ID: PIX4620372

Nebula of the crescent NGC 6888 in the Swan - NGC 6888 Crescent Nebula - NGC 6888 Nebula of the Crescent. This nebula is a gas shell located in the constellation Swan. The bright star in the center of the nebula is the star WR 136, a star of Wolf - Rayet, massive, very hot. Image obtained by combining light through 3 different filters that highlight oxygen, hydrogen, and sulfur. The nebula is a shell of gas that is being energized by the strong stellar wind from the Wolf - Rayet star WR 136, the bright star at the center of the nebula. It is located in the constellation of Cygnus, the Swan. Wolf - Rayet stars are very hot, massive stars that are blowing off their outer layers. Narrowband false color composite H - alpha, OIII, SII

The French Church, Platz der Akademie, Berlin (Germany). Construction 1701-1780, architects Louis Gayard and Karl v. Gonard. Photography 2003.
The French Church, Platz der Akademie, Berlin (Germany). Construction 1701-1780, architects Louis Gayard and Karl v. Gonard. Photography 2003.

TEC4620380: The French Church, Platz der Akademie, Berlin (Germany). Construction 1701-1780, architects Louis Gayard and Karl v. Gonard. Photography 2003. / Bridgeman Images

ID: TEC4620380

The French Church, Platz der Akademie, Berlin (Germany). Construction 1701-1780, architects Louis Gayard and Karl v. Gonard. Photography 2003.

Nebulae North America (NGC7000) and Pelican (IC 5070) in the swan - The north is at top. The North America nebula (left) is named because recall the shape of the American continent. The smaller Pelican nebula (IC 5067/70) is at right. These nebulae are certainly part of the same complex of hydrogen gas and dust that is crossed by a dark nebula (called LDN935) in the foreground. The distance to these nebulae is uncertain, although it is commonly accepted they lie at about 1600 light years from our Sun. It is also unknown which star ionises the nebulae and causes them to glow. This nebular complex is found in the Cygnus constellation, just west of the bright star Deneb. This image is based on data acquired by the Oschin Telescope at the Mount Palomar Observatory
Nebulae North America (NGC7000) and Pelican (IC 5070) in the swan - The north is at top. The North America nebula (left) is named because recall the shape of the American continent. The smaller Pelican nebula (IC 5067/70) is at right. These nebulae are certainly part of the same complex of hydrogen gas and dust that is crossed by a dark nebula (called LDN935) in the foreground. The distance to these nebulae is uncertain, although it is commonly accepted they lie at about 1600 light years from our Sun. It is also unknown which star ionises the nebulae and causes them to glow. This nebular complex is found in the Cygnus constellation, just west of the bright star Deneb. This image is based on data acquired by the Oschin Telescope at the Mount Palomar Observatory

PIX4620421: Nebulae North America (NGC7000) and Pelican (IC 5070) in the swan - The north is at top. The North America nebula (left) is named because recall the shape of the American continent. The smaller Pelican nebula (IC 5067/70) is at right. These nebulae are certainly part of the same complex of hydrogen gas and dust that is crossed by a dark nebula (called LDN935) in the foreground. The distance to these nebulae is uncertain, although it is commonly accepted they lie at about 1600 light years from our Sun. It is also unknown which star ionises the nebulae and causes them to glow. This nebular complex is found in the Cygnus constellation, just west of the bright star Deneb. This image is based on data acquired by the Oschin Telescope at the Mount Palomar Observatory / Bridgeman Images

ID: PIX4620421

Nebulae North America (NGC7000) and Pelican (IC 5070) in the swan - The north is at top. The North America nebula (left) is named because recall the shape of the American continent. The smaller Pelican nebula (IC 5067/70) is at right. These nebulae are certainly part of the same complex of hydrogen gas and dust that is crossed by a dark nebula (called LDN935) in the foreground. The distance to these nebulae is uncertain, although it is commonly accepted they lie at about 1600 light years from our Sun. It is also unknown which star ionises the nebulae and causes them to glow. This nebular complex is found in the Cygnus constellation, just west of the bright star Deneb. This image is based on data acquired by the Oschin Telescope at the Mount Palomar Observatory

Joan of Albret or Joan III of Albret (1528-1572) and her son Henry IV (1553-1610) before her Protestant troops, 1907 (illustration)
Joan of Albret or Joan III of Albret (1528-1572) and her son Henry IV (1553-1610) before her Protestant troops, 1907 (illustration)

JLJ4620500: Joan of Albret or Joan III of Albret (1528-1572) and her son Henry IV (1553-1610) before her Protestant troops, 1907 (illustration), Vogel, Hermann (1856-1918) / Bridgeman Images

ID: JLJ4620500

Joan of Albret or Joan III of Albret (1528-1572) and her son Henry IV (1553-1610) before her Protestant troops, 1907 (illustration)

Vogel, Hermann (1856-1918)

The Brandenburg Gate (1788-1791, architect Karl Gotthard Langhans) and the Pariser Platz, Mitte district in Berlin (Germany). Photographei 15/10/03.
The Brandenburg Gate (1788-1791, architect Karl Gotthard Langhans) and the Pariser Platz, Mitte district in Berlin (Germany). Photographei 15/10/03.

TEC4620501: The Brandenburg Gate (1788-1791, architect Karl Gotthard Langhans) and the Pariser Platz, Mitte district in Berlin (Germany). Photographei 15/10/03. / Bridgeman Images

ID: TEC4620501

The Brandenburg Gate (1788-1791, architect Karl Gotthard Langhans) and the Pariser Platz, Mitte district in Berlin (Germany). Photographei 15/10/03.

The Schiller Theater in Berlin (Germany). Architect Max Littmann, 1905-1906. This photographic work came from the exhibition Berlin, urban mutations presented at the Musee Carnavalet in Paris in 1997. A catalogue is available in the Open City editions. Photography 10/06/95.
The Schiller Theater in Berlin (Germany). Architect Max Littmann, 1905-1906. This photographic work came from the exhibition Berlin, urban mutations presented at the Musee Carnavalet in Paris in 1997. A catalogue is available in the Open City editions. Photography 10/06/95.

JSN4620509: The Schiller Theater in Berlin (Germany). Architect Max Littmann, 1905-1906. This photographic work came from the exhibition Berlin, urban mutations presented at the Musee Carnavalet in Paris in 1997. A catalogue is available in the Open City editions. Photography 10/06/95., Salmon, Jacqueline / Bridgeman Images

ID: JSN4620509

The Schiller Theater in Berlin (Germany). Architect Max Littmann, 1905-1906. This photographic work came from the exhibition Berlin, urban mutations presented at the Musee Carnavalet in Paris in 1997. A catalogue is available in the Open City editions. Photography 10/06/95.

Salmon, Jacqueline

The Hebbel Theater in Berlin (Germany). Architect Oskar Kaufmann, 1908.This photographic work came from the exhibition Berlin, urban mutations presented at the Musee Carnavalet in Paris in 1997. A catalogue is available in the Open City editions. Photography 10/06/95.
The Hebbel Theater in Berlin (Germany). Architect Oskar Kaufmann, 1908.This photographic work came from the exhibition Berlin, urban mutations presented at the Musee Carnavalet in Paris in 1997. A catalogue is available in the Open City editions. Photography 10/06/95.

JSN4620577: The Hebbel Theater in Berlin (Germany). Architect Oskar Kaufmann, 1908.This photographic work came from the exhibition Berlin, urban mutations presented at the Musee Carnavalet in Paris in 1997. A catalogue is available in the Open City editions. Photography 10/06/95., Salmon, Jacqueline / Bridgeman Images

ID: JSN4620577

The Hebbel Theater in Berlin (Germany). Architect Oskar Kaufmann, 1908.This photographic work came from the exhibition Berlin, urban mutations presented at the Musee Carnavalet in Paris in 1997. A catalogue is available in the Open City editions. Photography 10/06/95.

Salmon, Jacqueline

La Nouvelle Synagogue, 30 Oranienburger strasse, qaurtier Mitte in Berlin (Germany). Architects Eduard Knoblauch and Friedrich August Stuler, 1866, reconstruction Bernard Leisering, 1991. Photography 15/10/99.
La Nouvelle Synagogue, 30 Oranienburger strasse, qaurtier Mitte in Berlin (Germany). Architects Eduard Knoblauch and Friedrich August Stuler, 1866, reconstruction Bernard Leisering, 1991. Photography 15/10/99.

LBY4620646: La Nouvelle Synagogue, 30 Oranienburger strasse, qaurtier Mitte in Berlin (Germany). Architects Eduard Knoblauch and Friedrich August Stuler, 1866, reconstruction Bernard Leisering, 1991. Photography 15/10/99. / Bridgeman Images

ID: LBY4620646

La Nouvelle Synagogue, 30 Oranienburger strasse, qaurtier Mitte in Berlin (Germany). Architects Eduard Knoblauch and Friedrich August Stuler, 1866, reconstruction Bernard Leisering, 1991. Photography 15/10/99.

Einstein Cafe on Unter den Linden a Berlinae (Germany).
Einstein Cafe on Unter den Linden a Berlinae (Germany).

LBY4620680: Einstein Cafe on Unter den Linden a Berlinae (Germany). / Bridgeman Images

ID: LBY4620680

Einstein Cafe on Unter den Linden a Berlinae (Germany).

Nebula NGC 7635 in Cassiopee - North is at top. Seemingly adrift in a cosmic sea of stars and glowing gas, the delicate, floating apparition near the center (next to a blue tinted star) of this widefield view is cataloged as NGC 7635 - The Bubble Nebula. A mere 10 light - years wide, the tiny Bubble Nebula and the larger complex of interstellar gas and dust clouds are found about 11,000 light - years distant, straddling the boundary between the parental constellations Cepheus and Cassiopeia. Also included in the vista is open star cluster M52 (upper left), some 5,000 light - years away. The image spans about 2.7 degrees on the sky corresponding to a width of just over 500 light - years at the estimated distance of the Bubble Nebula. This image is based on data acquired by the Oschin Telescope at the Mount Palomar Observatory
Nebula NGC 7635 in Cassiopee - North is at top. Seemingly adrift in a cosmic sea of stars and glowing gas, the delicate, floating apparition near the center (next to a blue tinted star) of this widefield view is cataloged as NGC 7635 - The Bubble Nebula. A mere 10 light - years wide, the tiny Bubble Nebula and the larger complex of interstellar gas and dust clouds are found about 11,000 light - years distant, straddling the boundary between the parental constellations Cepheus and Cassiopeia. Also included in the vista is open star cluster M52 (upper left), some 5,000 light - years away. The image spans about 2.7 degrees on the sky corresponding to a width of just over 500 light - years at the estimated distance of the Bubble Nebula. This image is based on data acquired by the Oschin Telescope at the Mount Palomar Observatory

PIX4620650: Nebula NGC 7635 in Cassiopee - North is at top. Seemingly adrift in a cosmic sea of stars and glowing gas, the delicate, floating apparition near the center (next to a blue tinted star) of this widefield view is cataloged as NGC 7635 - The Bubble Nebula. A mere 10 light - years wide, the tiny Bubble Nebula and the larger complex of interstellar gas and dust clouds are found about 11,000 light - years distant, straddling the boundary between the parental constellations Cepheus and Cassiopeia. Also included in the vista is open star cluster M52 (upper left), some 5,000 light - years away. The image spans about 2.7 degrees on the sky corresponding to a width of just over 500 light - years at the estimated distance of the Bubble Nebula. This image is based on data acquired by the Oschin Telescope at the Mount Palomar Observatory / Bridgeman Images

ID: PIX4620650

Nebula NGC 7635 in Cassiopee - North is at top. Seemingly adrift in a cosmic sea of stars and glowing gas, the delicate, floating apparition near the center (next to a blue tinted star) of this widefield view is cataloged as NGC 7635 - The Bubble Nebula. A mere 10 light - years wide, the tiny Bubble Nebula and the larger complex of interstellar gas and dust clouds are found about 11,000 light - years distant, straddling the boundary between the parental constellations Cepheus and Cassiopeia. Also included in the vista is open star cluster M52 (upper left), some 5,000 light - years away. The image spans about 2.7 degrees on the sky corresponding to a width of just over 500 light - years at the estimated distance of the Bubble Nebula. This image is based on data acquired by the Oschin Telescope at the Mount Palomar Observatory

Nebula NGC 7635 in Cassiopee - This nebula is located about 7800 light years from Earth. A massive star, called Wolf - Rayet, is responsible for the formation of this bubble; it is the star BD+60* 2522, 40 times more massive than our Sun. Image obtained by Isaac Newton 2.5m telescope from La Palma
Nebula NGC 7635 in Cassiopee - This nebula is located about 7800 light years from Earth. A massive star, called Wolf - Rayet, is responsible for the formation of this bubble; it is the star BD+60* 2522, 40 times more massive than our Sun. Image obtained by Isaac Newton 2.5m telescope from La Palma

PIX4620665: Nebula NGC 7635 in Cassiopee - This nebula is located about 7800 light years from Earth. A massive star, called Wolf - Rayet, is responsible for the formation of this bubble; it is the star BD+60* 2522, 40 times more massive than our Sun. Image obtained by Isaac Newton 2.5m telescope from La Palma / Bridgeman Images

ID: PIX4620665

Nebula NGC 7635 in Cassiopee - This nebula is located about 7800 light years from Earth. A massive star, called Wolf - Rayet, is responsible for the formation of this bubble; it is the star BD+60* 2522, 40 times more massive than our Sun. Image obtained by Isaac Newton 2.5m telescope from La Palma

Nebula N119 in the Great Magellan Cloud - N119 is a “” H II region”” in the LMC
Nebula N119 in the Great Magellan Cloud - N119 is a “” H II region”” in the LMC

PIX4620774: Nebula N119 in the Great Magellan Cloud - N119 is a “” H II region”” in the LMC / Bridgeman Images

ID: PIX4620774

Nebula N119 in the Great Magellan Cloud - N119 is a “” H II region”” in the LMC

Nebula NGC 7635 in Cassiopee - The Bubble Nebula: This nebula is located about 8000 light years from Earth. A star 40 times more massive than our Sun, called Wolf-Rayet, is responsible for the formation of this bubble; it is the star BD+60* 2522. Image obtained by the space telescope Hubble - The Bubble Nebula, also known as NGC 7635, is an emission nebula located 8 000 light-years away - This complete view of the Bubble Nebula allows us to fully appreciate the almost perfectly symmetrical shell which gives the nebula its name. This shell is the result of a powerful flow of gas - known as a stellar wind - from the bright star visible just to the left of centre in this image. The star, SAO 20575, is between ten and twenty times the mass of the Sun and the pressure created by its stellar wind forces the surrounding interstellar material outwards into this bubble-like form - The giant molecular cloud that surrounds the star - glowing in the star's intense ultraviolet radiation - tries to stop the expansion of the bubble. However, although the sphere already measures around ten light-years in diameter, it is still growing, owing to the constant pressure of the stellar wind - currently at more than 100,000 kilometers per hour! - This stunning new image was observed by the NASA/ESA Hubble Space Telescope
Nebula NGC 7635 in Cassiopee - The Bubble Nebula: This nebula is located about 8000 light years from Earth. A star 40 times more massive than our Sun, called Wolf-Rayet, is responsible for the formation of this bubble; it is the star BD+60* 2522. Image obtained by the space telescope Hubble - The Bubble Nebula, also known as NGC 7635, is an emission nebula located 8 000 light-years away - This complete view of the Bubble Nebula allows us to fully appreciate the almost perfectly symmetrical shell which gives the nebula its name. This shell is the result of a powerful flow of gas - known as a stellar wind - from the bright star visible just to the left of centre in this image. The star, SAO 20575, is between ten and twenty times the mass of the Sun and the pressure created by its stellar wind forces the surrounding interstellar material outwards into this bubble-like form - The giant molecular cloud that surrounds the star - glowing in the star's intense ultraviolet radiation - tries to stop the expansion of the bubble. However, although the sphere already measures around ten light-years in diameter, it is still growing, owing to the constant pressure of the stellar wind - currently at more than 100,000 kilometers per hour! - This stunning new image was observed by the NASA/ESA Hubble Space Telescope

PIX4620728: Nebula NGC 7635 in Cassiopee - The Bubble Nebula: This nebula is located about 8000 light years from Earth. A star 40 times more massive than our Sun, called Wolf-Rayet, is responsible for the formation of this bubble; it is the star BD+60* 2522. Image obtained by the space telescope Hubble - The Bubble Nebula, also known as NGC 7635, is an emission nebula located 8 000 light-years away - This complete view of the Bubble Nebula allows us to fully appreciate the almost perfectly symmetrical shell which gives the nebula its name. This shell is the result of a powerful flow of gas - known as a stellar wind - from the bright star visible just to the left of centre in this image. The star, SAO 20575, is between ten and twenty times the mass of the Sun and the pressure created by its stellar wind forces the surrounding interstellar material outwards into this bubble-like form - The giant molecular cloud that surrounds the star - glowing in the star's intense ultraviolet radiation - tries to stop the expansion of the bubble. However, although the sphere already measures around ten light-years in diameter, it is still growing, owing to the constant pressure of the stellar wind - currently at more than 100,000 kilometers per hour! - This stunning new image was observed by the NASA/ESA Hubble Space Telescope / Bridgeman Images

ID: PIX4620728

Nebula NGC 7635 in Cassiopee - The Bubble Nebula: This nebula is located about 8000 light years from Earth. A star 40 times more massive than our Sun, called Wolf-Rayet, is responsible for the formation of this bubble; it is the star BD+60* 2522. Image obtained by the space telescope Hubble - The Bubble Nebula, also known as NGC 7635, is an emission nebula located 8 000 light-years away - This complete view of the Bubble Nebula allows us to fully appreciate the almost perfectly symmetrical shell which gives the nebula its name. This shell is the result of a powerful flow of gas - known as a stellar wind - from the bright star visible just to the left of centre in this image. The star, SAO 20575, is between ten and twenty times the mass of the Sun and the pressure created by its stellar wind forces the surrounding interstellar material outwards into this bubble-like form - The giant molecular cloud that surrounds the star - glowing in the star's intense ultraviolet radiation - tries to

Nebula NGC 346 in the Small Magellan Cloud - Nebula NGC 346 in the Small Magellanic Cloud - Photo of the nebula NGC 346, located about 210,000 years ago - light in the galaxy of the Little Magellan Cloud, obtained by the 2.2-metre MPG/ESO telescope. Nebula NGC 346 in the Small Magellanic Cloud, a nearby irregular galaxy, seen by the 2.2 - metre MPG/ESO telescope at the La Silla Observatory in Chile
Nebula NGC 346 in the Small Magellan Cloud - Nebula NGC 346 in the Small Magellanic Cloud - Photo of the nebula NGC 346, located about 210,000 years ago - light in the galaxy of the Little Magellan Cloud, obtained by the 2.2-metre MPG/ESO telescope. Nebula NGC 346 in the Small Magellanic Cloud, a nearby irregular galaxy, seen by the 2.2 - metre MPG/ESO telescope at the La Silla Observatory in Chile

PIX4620841: Nebula NGC 346 in the Small Magellan Cloud - Nebula NGC 346 in the Small Magellanic Cloud - Photo of the nebula NGC 346, located about 210,000 years ago - light in the galaxy of the Little Magellan Cloud, obtained by the 2.2-metre MPG/ESO telescope. Nebula NGC 346 in the Small Magellanic Cloud, a nearby irregular galaxy, seen by the 2.2 - metre MPG/ESO telescope at the La Silla Observatory in Chile / Bridgeman Images

ID: PIX4620841

Nebula NGC 346 in the Small Magellan Cloud - Nebula NGC 346 in the Small Magellanic Cloud - Photo of the nebula NGC 346, located about 210,000 years ago - light in the galaxy of the Little Magellan Cloud, obtained by the 2.2-metre MPG/ESO telescope. Nebula NGC 346 in the Small Magellanic Cloud, a nearby irregular galaxy, seen by the 2.2 - metre MPG/ESO telescope at the La Silla Observatory in Chile

The Duomo (Cathedrale) of Milan, Italy. Photograph 10/08/90.
The Duomo (Cathedrale) of Milan, Italy. Photograph 10/08/90.

LBY4620921: The Duomo (Cathedrale) of Milan, Italy. Photograph 10/08/90. / Bridgeman Images

ID: LBY4620921

The Duomo (Cathedrale) of Milan, Italy. Photograph 10/08/90.

N66 Nebula in the Little Magellan Cloud - Photo of the N66 nebula in the galaxy of the Small Magellan Cloud obtained by the Hubble space telescope. At the center of this nebula, a cluster of very young stars, NGC 346 in which some stars are only 5 million years old.
N66 Nebula in the Little Magellan Cloud - Photo of the N66 nebula in the galaxy of the Small Magellan Cloud obtained by the Hubble space telescope. At the center of this nebula, a cluster of very young stars, NGC 346 in which some stars are only 5 million years old.

PIX4620847: N66 Nebula in the Little Magellan Cloud - Photo of the N66 nebula in the galaxy of the Small Magellan Cloud obtained by the Hubble space telescope. At the center of this nebula, a cluster of very young stars, NGC 346 in which some stars are only 5 million years old. / Bridgeman Images

ID: PIX4620847

N66 Nebula in the Little Magellan Cloud - Photo of the N66 nebula in the galaxy of the Small Magellan Cloud obtained by the Hubble space telescope. At the center of this nebula, a cluster of very young stars, NGC 346 in which some stars are only 5 million years old.

Nebula N55 in the Great Magellan Cloud - Star forming region north of the Great Magellan Cloud. Image from the 1.2m Schmidt UK Telescope of Siding Spring
Nebula N55 in the Great Magellan Cloud - Star forming region north of the Great Magellan Cloud. Image from the 1.2m Schmidt UK Telescope of Siding Spring

PIX4620885: Nebula N55 in the Great Magellan Cloud - Star forming region north of the Great Magellan Cloud. Image from the 1.2m Schmidt UK Telescope of Siding Spring / Bridgeman Images

ID: PIX4620885

Nebula N55 in the Great Magellan Cloud - Star forming region north of the Great Magellan Cloud. Image from the 1.2m Schmidt UK Telescope of Siding Spring

Nebula N55 in the Great Magellan Cloud - Henize 55 (NGC 2014) is a star-forming region located north of the Great Magellan Cloud. Image obtained by Siding Spring's 3.9m telescope
Nebula N55 in the Great Magellan Cloud - Henize 55 (NGC 2014) is a star-forming region located north of the Great Magellan Cloud. Image obtained by Siding Spring's 3.9m telescope

PIX4620894: Nebula N55 in the Great Magellan Cloud - Henize 55 (NGC 2014) is a star-forming region located north of the Great Magellan Cloud. Image obtained by Siding Spring's 3.9m telescope / Bridgeman Images

ID: PIX4620894

Nebula N55 in the Great Magellan Cloud - Henize 55 (NGC 2014) is a star-forming region located north of the Great Magellan Cloud. Image obtained by Siding Spring's 3.9m telescope

On July 16, 1789, when King Louis XVI (1754-1793) en route to the town hall to receive the cocarde, 1907 (illustration)
On July 16, 1789, when King Louis XVI (1754-1793) en route to the town hall to receive the cocarde, 1907 (illustration)

JLJ4620907: On July 16, 1789, when King Louis XVI (1754-1793) en route to the town hall to receive the cocarde, 1907 (illustration), Vogel, Hermann (1856-1918) / Bridgeman Images

ID: JLJ4620907

On July 16, 1789, when King Louis XVI (1754-1793) en route to the town hall to receive the cocarde, 1907 (illustration)

Vogel, Hermann (1856-1918)

The Duomo di San Lorenzo of the Cathedral of Genes Duomo di San Lorenzo - Cathedrale de Genes - 1181
The Duomo di San Lorenzo of the Cathedral of Genes Duomo di San Lorenzo - Cathedrale de Genes - 1181

LBY4620931: The Duomo di San Lorenzo of the Cathedral of Genes Duomo di San Lorenzo - Cathedrale de Genes - 1181 / Bridgeman Images

ID: LBY4620931

The Duomo di San Lorenzo of the Cathedral of Genes Duomo di San Lorenzo - Cathedrale de Genes - 1181

La Nouvelle Synagogue, 30 Oranienburger strasse, qaurtier Mitte in Berlin (Germany). Architects Eduard Knoblauch and Friedrich August Stuler, 1866, reconstruction Bernard Leisering, 1991. Photography 15/10/99.
La Nouvelle Synagogue, 30 Oranienburger strasse, qaurtier Mitte in Berlin (Germany). Architects Eduard Knoblauch and Friedrich August Stuler, 1866, reconstruction Bernard Leisering, 1991. Photography 15/10/99.

LBY4620657: La Nouvelle Synagogue, 30 Oranienburger strasse, qaurtier Mitte in Berlin (Germany). Architects Eduard Knoblauch and Friedrich August Stuler, 1866, reconstruction Bernard Leisering, 1991. Photography 15/10/99. / Bridgeman Images

ID: LBY4620657

La Nouvelle Synagogue, 30 Oranienburger strasse, qaurtier Mitte in Berlin (Germany). Architects Eduard Knoblauch and Friedrich August Stuler, 1866, reconstruction Bernard Leisering, 1991. Photography 15/10/99.

Nebula NGC 7635 in Cassiopee - The Bubble Nebula (NGC 7635) in Cassiopeia - This nebula is located about 7100 years - light from Earth. A star 40 times more massive than our Sun, called Wolf - Rayet, is responsible for the formation of this bubble; it is the star BD+60* 2522. The Bubble Nebula in Cassiopeia is one of the most dramatic emission nebulae visible in the northern hemisphere. Lying at a distance of about 7,000 light - years away and spanning six light - years in diameter, NGC 7635 is quite bright with a magnitude of 7.0. The star in the middle of the bubble, BD+602522, is responsible for this stunning site, for this very hot star emits so much UV radiation that it is able to also heat and excite the surrounding dust and gas, thus emitting its own radiation. It is a Wolf - Rayet star, a very luminous star and also very short - lived. This Wolf - Rayet star is 40 times as massive than our sun
Nebula NGC 7635 in Cassiopee - The Bubble Nebula (NGC 7635) in Cassiopeia - This nebula is located about 7100 years - light from Earth. A star 40 times more massive than our Sun, called Wolf - Rayet, is responsible for the formation of this bubble; it is the star BD+60* 2522. The Bubble Nebula in Cassiopeia is one of the most dramatic emission nebulae visible in the northern hemisphere. Lying at a distance of about 7,000 light - years away and spanning six light - years in diameter, NGC 7635 is quite bright with a magnitude of 7.0. The star in the middle of the bubble, BD+602522, is responsible for this stunning site, for this very hot star emits so much UV radiation that it is able to also heat and excite the surrounding dust and gas, thus emitting its own radiation. It is a Wolf - Rayet star, a very luminous star and also very short - lived. This Wolf - Rayet star is 40 times as massive than our sun

PIX4620709: Nebula NGC 7635 in Cassiopee - The Bubble Nebula (NGC 7635) in Cassiopeia - This nebula is located about 7100 years - light from Earth. A star 40 times more massive than our Sun, called Wolf - Rayet, is responsible for the formation of this bubble; it is the star BD+60* 2522. The Bubble Nebula in Cassiopeia is one of the most dramatic emission nebulae visible in the northern hemisphere. Lying at a distance of about 7,000 light - years away and spanning six light - years in diameter, NGC 7635 is quite bright with a magnitude of 7.0. The star in the middle of the bubble, BD+602522, is responsible for this stunning site, for this very hot star emits so much UV radiation that it is able to also heat and excite the surrounding dust and gas, thus emitting its own radiation. It is a Wolf - Rayet star, a very luminous star and also very short - lived. This Wolf - Rayet star is 40 times as massive than our sun / Bridgeman Images

ID: PIX4620709

Nebula NGC 7635 in Cassiopee - The Bubble Nebula (NGC 7635) in Cassiopeia - This nebula is located about 7100 years - light from Earth. A star 40 times more massive than our Sun, called Wolf - Rayet, is responsible for the formation of this bubble; it is the star BD+60* 2522. The Bubble Nebula in Cassiopeia is one of the most dramatic emission nebulae visible in the northern hemisphere. Lying at a distance of about 7,000 light - years away and spanning six light - years in diameter, NGC 7635 is quite bright with a magnitude of 7.0. The star in the middle of the bubble, BD+602522, is responsible for this stunning site, for this very hot star emits so much UV radiation that it is able to also heat and excite the surrounding dust and gas, thus emitting its own radiation. It is a Wolf - Rayet star, a very luminous star and also very short - lived. This Wolf - Rayet star is 40 times as massive than our sun

Portrait of Philippe Coypel, brother of the artist Painting by Charles Antoine Coypel (1696-1752) 1732 Dim. 75x61 cm Paris, musee du Louvre
Portrait of Philippe Coypel, brother of the artist Painting by Charles Antoine Coypel (1696-1752) 1732 Dim. 75x61 cm Paris, musee du Louvre

LRI4620764: Portrait of Philippe Coypel, brother of the artist Painting by Charles Antoine Coypel (1696-1752) 1732 Dim. 75x61 cm Paris, musee du Louvre, Coypel, Antoine (1661-1722) / Bridgeman Images

ID: LRI4620764

Portrait of Philippe Coypel, brother of the artist Painting by Charles Antoine Coypel (1696-1752) 1732 Dim. 75x61 cm Paris, musee du Louvre

Coypel, Antoine (1661-1722)

The Dutch Nobles Walk on horseback. Painting by Albert (Aelbert or Aelbrecht) Cuyp (1620-1691) 17th century Sun. 119x152,5 cm Paris, musee du Louvre
The Dutch Nobles Walk on horseback. Painting by Albert (Aelbert or Aelbrecht) Cuyp (1620-1691) 17th century Sun. 119x152,5 cm Paris, musee du Louvre

LRI4620800: The Dutch Nobles Walk on horseback. Painting by Albert (Aelbert or Aelbrecht) Cuyp (1620-1691) 17th century Sun. 119x152,5 cm Paris, musee du Louvre, Cuyp, Aelbert (1620-91) / Bridgeman Images

ID: LRI4620800

The Dutch Nobles Walk on horseback. Painting by Albert (Aelbert or Aelbrecht) Cuyp (1620-1691) 17th century Sun. 119x152,5 cm Paris, musee du Louvre

Cuyp, Aelbert (1620-91)

The Victor Emmanuel II gallery in Milan, Italy. Architect Giuseppe Mengoni. Photography 10/08/90.
The Victor Emmanuel II gallery in Milan, Italy. Architect Giuseppe Mengoni. Photography 10/08/90.

LBY4620925: The Victor Emmanuel II gallery in Milan, Italy. Architect Giuseppe Mengoni. Photography 10/08/90. / Bridgeman Images

ID: LBY4620925

The Victor Emmanuel II gallery in Milan, Italy. Architect Giuseppe Mengoni. Photography 10/08/90.

The field concert Musicians on the grass, women are naked. Detail. Painting attributed to Tiziano Vecellio known as the Titian (1485-1576) or to Giorgio da Castelfranco called Giorgione (1476/1478-1510) Sun. 1,05 X 1.36 m Paris, Museum of the Louvre
The field concert Musicians on the grass, women are naked. Detail. Painting attributed to Tiziano Vecellio known as the Titian (1485-1576) or to Giorgio da Castelfranco called Giorgione (1476/1478-1510) Sun. 1,05 X 1.36 m Paris, Museum of the Louvre

LRI4621066: The field concert Musicians on the grass, women are naked. Detail. Painting attributed to Tiziano Vecellio known as the Titian (1485-1576) or to Giorgio da Castelfranco called Giorgione (1476/1478-1510) Sun. 1,05 X 1.36 m Paris, Museum of the Louvre, Titian (Tiziano Vecellio) (c.1488-1576) (attr. to) / Bridgeman Images

ID: LRI4621066

The field concert Musicians on the grass, women are naked. Detail. Painting attributed to Tiziano Vecellio known as the Titian (1485-1576) or to Giorgio da Castelfranco called Giorgione (1476/1478-1510) Sun. 1,05 X 1.36 m Paris, Museum of the Louvre

Titian (Tiziano Vecellio) (c.1488-1576) (attr. to)

St Bonaventure Enters the Franciscan Order (oil on canvas, 1628)
St Bonaventure Enters the Franciscan Order (oil on canvas, 1628)

LRI4621138: St Bonaventure Enters the Franciscan Order (oil on canvas, 1628), Herrera, Francisco (1576-1656) / Bridgeman Images

ID: LRI4621138

St Bonaventure Enters the Franciscan Order (oil on canvas, 1628)

Herrera, Francisco (1576-1656)


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