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Centre de la nebula de la Lagoon (M8) dans le Sagittarius - In the heart of the Lagoon Nebula - Centre de la nebula de la Lagoon (M8) vue par le telescope Hubble (HST). This close - up shot of the centre of the Lagoon Nebula (Messier 8) clearly shows the delicate structures formed when the powerful radiation of young stars interacts with the hydrogen cloud they formed from. This image was created from exposures taken with the Wide Field Channel of the Advanced Camera for Surveys on Hubble. Light from glowing hydrogen (through the F658N filter) is coloured red. Light from ionised nitrogen (through the F660N filter) is coloured green and light through a yellow filter (F550M) is coloured blue. The exposure times through each filter are 1560 s, 1600 s and 400 s respectively. The blue - white flare at the upper - left of the image is scattered light from a bright star just outside the field of view. The field of view is about 3.3 by 1.7 arcminutes
Centre de la nebula de la Lagoon (M8) dans le Sagittarius - In the heart of the Lagoon Nebula - Centre de la nebula de la Lagoon (M8) vue par le telescope Hubble (HST). This close - up shot of the centre of the Lagoon Nebula (Messier 8) clearly shows the delicate structures formed when the powerful radiation of young stars interacts with the hydrogen cloud they formed from. This image was created from exposures taken with the Wide Field Channel of the Advanced Camera for Surveys on Hubble. Light from glowing hydrogen (through the F658N filter) is coloured red. Light from ionised nitrogen (through the F660N filter) is coloured green and light through a yellow filter (F550M) is coloured blue. The exposure times through each filter are 1560 s, 1600 s and 400 s respectively. The blue - white flare at the upper - left of the image is scattered light from a bright star just outside the field of view. The field of view is about 3.3 by 1.7 arcminutes

PIX4619692: Centre de la nebula de la Lagoon (M8) dans le Sagittarius - In the heart of the Lagoon Nebula - Centre de la nebula de la Lagoon (M8) vue par le telescope Hubble (HST). This close - up shot of the centre of the Lagoon Nebula (Messier 8) clearly shows the delicate structures formed when the powerful radiation of young stars interacts with the hydrogen cloud they formed from. This image was created from exposures taken with the Wide Field Channel of the Advanced Camera for Surveys on Hubble. Light from glowing hydrogen (through the F658N filter) is coloured red. Light from ionised nitrogen (through the F660N filter) is coloured green and light through a yellow filter (F550M) is coloured blue. The exposure times through each filter are 1560 s, 1600 s and 400 s respectively. The blue - white flare at the upper - left of the image is scattered light from a bright star just outside the field of view. The field of view is about 3.3 by 1.7 arcminutes / Bridgeman Images

The Church of Remembrance in the Charlottenburg district of Berlin (Germany). Renovation1963, architect Eiermann Egon, construction 1895, architect Franz Schwechten. Photography 15/10/96.
The Church of Remembrance in the Charlottenburg district of Berlin (Germany). Renovation1963, architect Eiermann Egon, construction 1895, architect Franz Schwechten. Photography 15/10/96.

TEC4619737: The Church of Remembrance in the Charlottenburg district of Berlin (Germany). Renovation1963, architect Eiermann Egon, construction 1895, architect Franz Schwechten. Photography 15/10/96. / Bridgeman Images

Cemetery in Berlin (Germany).
Cemetery in Berlin (Germany).

TEC4619751: Cemetery in Berlin (Germany). / Bridgeman Images

Kunstgewerbmuseum Martin Gropius Bau (former Museum of Decorative Arts) æa Kreutzberg, Stresemannstasse 110, Berlin, Germany. Construction 1877-1881, architects Martin Gropius (1824-1880) and Heino Schmieden (1835-1913). Photography 2003.
Kunstgewerbmuseum Martin Gropius Bau (former Museum of Decorative Arts) æa Kreutzberg, Stresemannstasse 110, Berlin, Germany. Construction 1877-1881, architects Martin Gropius (1824-1880) and Heino Schmieden (1835-1913). Photography 2003.

TEC4619774: Kunstgewerbmuseum Martin Gropius Bau (former Museum of Decorative Arts) æa Kreutzberg, Stresemannstasse 110, Berlin, Germany. Construction 1877-1881, architects Martin Gropius (1824-1880) and Heino Schmieden (1835-1913). Photography 2003. / Bridgeman Images

Nebula NGC 6559 in Sagittarius - Nebula NGC 6559 in Sagittarius - Located in Sagittarius, this nebula is located at a distance of about 5000 years - light from Earth. Mosaic of images obtained with a telescope of 35 cm, 22 hours of poses. This nebula is located at about 5000 light years from the Earth. Mosaic of images taken with 14.5”” RCOS telescope, 22 hours of exposure
Nebula NGC 6559 in Sagittarius - Nebula NGC 6559 in Sagittarius - Located in Sagittarius, this nebula is located at a distance of about 5000 years - light from Earth. Mosaic of images obtained with a telescope of 35 cm, 22 hours of poses. This nebula is located at about 5000 light years from the Earth. Mosaic of images taken with 14.5”” RCOS telescope, 22 hours of exposure

PIX4619810: Nebula NGC 6559 in Sagittarius - Nebula NGC 6559 in Sagittarius - Located in Sagittarius, this nebula is located at a distance of about 5000 years - light from Earth. Mosaic of images obtained with a telescope of 35 cm, 22 hours of poses. This nebula is located at about 5000 light years from the Earth. Mosaic of images taken with 14.5”” RCOS telescope, 22 hours of exposure / Bridgeman Images

Wittenbergplatz Metro Station in Schoneberg, Berlin (Germany). First underground metro station in Berlin, on the first electric line. Built in reference to the classical buildings of the 18th century, especially Schinkel, it retains an abundant decor designed in a more contemporary style that survived the war. Architect Alfred Grenander (1863-1931), construction 1911-1913.
Wittenbergplatz Metro Station in Schoneberg, Berlin (Germany). First underground metro station in Berlin, on the first electric line. Built in reference to the classical buildings of the 18th century, especially Schinkel, it retains an abundant decor designed in a more contemporary style that survived the war. Architect Alfred Grenander (1863-1931), construction 1911-1913.

TEC4619833: Wittenbergplatz Metro Station in Schoneberg, Berlin (Germany). First underground metro station in Berlin, on the first electric line. Built in reference to the classical buildings of the 18th century, especially Schinkel, it retains an abundant decor designed in a more contemporary style that survived the war. Architect Alfred Grenander (1863-1931), construction 1911-1913. / Bridgeman Images

Dust in Iris Nebula - Dust in Iris Nebula - The Iris Nebula (NGC 7023) is a reflexion nebula illuminated by the star HD 200775. This image obtained by the Hubble Space Telescope shows a detail of the nebula or HD star 200775 (at the top of the image, out of the field) illuminates tiny particles of dust. This close - up of an area in the northwest region of the large Iris Nebula (NGC 7023) seems to be clogged with cosmic dust. With bright light from the nearby star HD 200775 illuminating it from above, the dust resemble thick mounds of billowing cotton. It is actually made up of tiny particles of solid matter, with sizes from ten to a hundred times smaller than those of the dust grains we find at home. Both background and foreground stars are dotted throughout the image. North is down, East is right. The field of view is 3.3 arcminutes. The image is a composite of four images obtained by the Hubble space Telescope through blue, green, near - infrared and H - alpha filters
Dust in Iris Nebula - Dust in Iris Nebula - The Iris Nebula (NGC 7023) is a reflexion nebula illuminated by the star HD 200775. This image obtained by the Hubble Space Telescope shows a detail of the nebula or HD star 200775 (at the top of the image, out of the field) illuminates tiny particles of dust. This close - up of an area in the northwest region of the large Iris Nebula (NGC 7023) seems to be clogged with cosmic dust. With bright light from the nearby star HD 200775 illuminating it from above, the dust resemble thick mounds of billowing cotton. It is actually made up of tiny particles of solid matter, with sizes from ten to a hundred times smaller than those of the dust grains we find at home. Both background and foreground stars are dotted throughout the image. North is down, East is right. The field of view is 3.3 arcminutes. The image is a composite of four images obtained by the Hubble space Telescope through blue, green, near - infrared and H - alpha filters

PIX4620558: Dust in Iris Nebula - Dust in Iris Nebula - The Iris Nebula (NGC 7023) is a reflexion nebula illuminated by the star HD 200775. This image obtained by the Hubble Space Telescope shows a detail of the nebula or HD star 200775 (at the top of the image, out of the field) illuminates tiny particles of dust. This close - up of an area in the northwest region of the large Iris Nebula (NGC 7023) seems to be clogged with cosmic dust. With bright light from the nearby star HD 200775 illuminating it from above, the dust resemble thick mounds of billowing cotton. It is actually made up of tiny particles of solid matter, with sizes from ten to a hundred times smaller than those of the dust grains we find at home. Both background and foreground stars are dotted throughout the image. North is down, East is right. The field of view is 3.3 arcminutes. The image is a composite of four images obtained by the Hubble space Telescope through blue, green, near - infrared and H - alpha filters / Bridgeman Images

Friedrichstrasse Station, Mitte Quarter aae Berlin (Germany).
Friedrichstrasse Station, Mitte Quarter aae Berlin (Germany).

LBY4620623: Friedrichstrasse Station, Mitte Quarter aae Berlin (Germany). / Bridgeman Images

The 17th June Street and the Brandenburg Gate (Architect Carl Gotthard Langhans, 1788-1791) in Berlin, Germany. Photography 15/101/99.
The 17th June Street and the Brandenburg Gate (Architect Carl Gotthard Langhans, 1788-1791) in Berlin, Germany. Photography 15/101/99.

LBY4620682: The 17th June Street and the Brandenburg Gate (Architect Carl Gotthard Langhans, 1788-1791) in Berlin, Germany. Photography 15/101/99. / Bridgeman Images

The deposition of Christ (oil on canvas, circa 1651)
The deposition of Christ (oil on canvas, circa 1651)

LRI4621309: The deposition of Christ (oil on canvas, circa 1651), Le Sueur, Eustache (1617-55) / Bridgeman Images

Nebula in the galaxy NGC 6822 - Bubble nebulae in NGC 6822 - Nebula in the irregular galaxy NGC 6822, adjacent to our galaxy. This gas bubble houses massive stars known as Wolf - Rayet. NGC 6822 is a nearby irregular galaxy reminiscent of the Large Magellanic Cloud (LMC). Like the LMC it contains many, extremely hot stars of the Wolf - Rayet type, stars which often have intense stellar winds blasting from their surfaces. Small groups of such stars are found at the centres of the bubble nebulae seen here, which are the result of the stellar winds colliding with the more or less stationary interstellar medium in NGC 6822. At the interface of the collision, the interstellar medium glows, producing a thin, luminous bubble. Such bubbles are rare in the more turbulent Milky Way galaxy, but Henize 70 in the Large Magellanic Cloud is similar
Nebula in the galaxy NGC 6822 - Bubble nebulae in NGC 6822 - Nebula in the irregular galaxy NGC 6822, adjacent to our galaxy. This gas bubble houses massive stars known as Wolf - Rayet. NGC 6822 is a nearby irregular galaxy reminiscent of the Large Magellanic Cloud (LMC). Like the LMC it contains many, extremely hot stars of the Wolf - Rayet type, stars which often have intense stellar winds blasting from their surfaces. Small groups of such stars are found at the centres of the bubble nebulae seen here, which are the result of the stellar winds colliding with the more or less stationary interstellar medium in NGC 6822. At the interface of the collision, the interstellar medium glows, producing a thin, luminous bubble. Such bubbles are rare in the more turbulent Milky Way galaxy, but Henize 70 in the Large Magellanic Cloud is similar

PIX4620956: Nebula in the galaxy NGC 6822 - Bubble nebulae in NGC 6822 - Nebula in the irregular galaxy NGC 6822, adjacent to our galaxy. This gas bubble houses massive stars known as Wolf - Rayet. NGC 6822 is a nearby irregular galaxy reminiscent of the Large Magellanic Cloud (LMC). Like the LMC it contains many, extremely hot stars of the Wolf - Rayet type, stars which often have intense stellar winds blasting from their surfaces. Small groups of such stars are found at the centres of the bubble nebulae seen here, which are the result of the stellar winds colliding with the more or less stationary interstellar medium in NGC 6822. At the interface of the collision, the interstellar medium glows, producing a thin, luminous bubble. Such bubbles are rare in the more turbulent Milky Way galaxy, but Henize 70 in the Large Magellanic Cloud is similar / Bridgeman Images

The Berliner Ensemble in Berlin (Germany). 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 Berliner Ensemble in Berlin (Germany). 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.

JSN4620531: The Berliner Ensemble in Berlin (Germany). 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

Nebula NGC 7023 in Cephee - NGC 7023 (The Iris Nebula) in Cepheus - The Iris Nebula (NGC 7023) is a reflexion nebula illuminated by the massive star HD 200775. The bright star HD 200775 shining through the nebula NGC 7023 is a 10 solar mass star centrally imbedded in a region surrounded by ambient molecular cloud material. Suns are born from vast clouds of dust and gas that gather in the dark places between the stars. Gravity causes these interstellar vapors to collapse inward until the pressure causes high enough temperatures at its center to fuse hydrogen, the university's basic building block, into helium - an event that also releases gamma - ray photons. These photons can take a million years to travel outward through the overlying matter until they reach the surface and escape into space as visible light. The push of the photon's rush to make an exit also stops the cloud's collapse and thus what began as thin gas and dust becomes a brilliant star illuminating the heavens and possibly warming near - by planets. This picture shows a place in deep space where these kinds of events have occurred. The brilliant star near the center of the picture is young and very hot - in relative terms, it was only recently created. The cloud from which it formed still surrounds this young Sun but is being blown away by the push of star's massive radiation. This picture shows the way it looked 1,300 years ago due to the distance that separates it from Earth and the speed that light travels
Nebula NGC 7023 in Cephee - NGC 7023 (The Iris Nebula) in Cepheus - The Iris Nebula (NGC 7023) is a reflexion nebula illuminated by the massive star HD 200775. The bright star HD 200775 shining through the nebula NGC 7023 is a 10 solar mass star centrally imbedded in a region surrounded by ambient molecular cloud material. Suns are born from vast clouds of dust and gas that gather in the dark places between the stars. Gravity causes these interstellar vapors to collapse inward until the pressure causes high enough temperatures at its center to fuse hydrogen, the university's basic building block, into helium - an event that also releases gamma - ray photons. These photons can take a million years to travel outward through the overlying matter until they reach the surface and escape into space as visible light. The push of the photon's rush to make an exit also stops the cloud's collapse and thus what began as thin gas and dust becomes a brilliant star illuminating the heavens and possibly warming near - by planets. This picture shows a place in deep space where these kinds of events have occurred. The brilliant star near the center of the picture is young and very hot - in relative terms, it was only recently created. The cloud from which it formed still surrounds this young Sun but is being blown away by the push of star's massive radiation. This picture shows the way it looked 1,300 years ago due to the distance that separates it from Earth and the speed that light travels

PIX4620555: Nebula NGC 7023 in Cephee - NGC 7023 (The Iris Nebula) in Cepheus - The Iris Nebula (NGC 7023) is a reflexion nebula illuminated by the massive star HD 200775. The bright star HD 200775 shining through the nebula NGC 7023 is a 10 solar mass star centrally imbedded in a region surrounded by ambient molecular cloud material. Suns are born from vast clouds of dust and gas that gather in the dark places between the stars. Gravity causes these interstellar vapors to collapse inward until the pressure causes high enough temperatures at its center to fuse hydrogen, the university's basic building block, into helium - an event that also releases gamma - ray photons. These photons can take a million years to travel outward through the overlying matter until they reach the surface and escape into space as visible light. The push of the photon's rush to make an exit also stops the cloud's collapse and thus what began as thin gas and dust becomes a brilliant star illuminating the heavens and possibly warming near - by planets. This picture shows a place in deep space where these kinds of events have occurred. The brilliant star near the center of the picture is young and very hot - in relative terms, it was only recently created. The cloud from which it formed still surrounds this young Sun but is being blown away by the push of star's massive radiation. This picture shows the way it looked 1,300 years ago due to the distance that separates it from Earth and the speed that light travels / Bridgeman Images

Nebula NGC 7538 in Cassiope
Nebula NGC 7538 in Cassiope

PIX4620603: Nebula NGC 7538 in Cassiope / Bridgeman Images

La cathedrale de Sens Painting by Jean Baptiste Camille Corot (1796-1875) 1874 Dim. 61x40 cm Paris, Musee du Louvre
La cathedrale de Sens Painting by Jean Baptiste Camille Corot (1796-1875) 1874 Dim. 61x40 cm Paris, Musee du Louvre

LRI4620714: La cathedrale de Sens Painting by Jean Baptiste Camille Corot (1796-1875) 1874 Dim. 61x40 cm Paris, Musee du Louvre, Corot, Jean Baptiste Camille (1796-1875) / Bridgeman Images

The Volksbank in Berlin (Germany). Construction 1994-1998, architects Arata Isozaki and Steffen Lehmann. Photography 15/10/99.
The Volksbank in Berlin (Germany). Construction 1994-1998, architects Arata Isozaki and Steffen Lehmann. Photography 15/10/99.

LBY4620759: The Volksbank in Berlin (Germany). Construction 1994-1998, architects Arata Isozaki and Steffen Lehmann. Photography 15/10/99. / Bridgeman Images

Place du Pantheon in Paris.
Place du Pantheon in Paris.

TEC4622703: Place du Pantheon in Paris. / Bridgeman Images

Ancient channels on Mars - Ancient channels on planet Mars. Ares Vallis - View of the area of Ares Vallis and Tiu Vallis obtained by the probe 2001 Mars Odyssey. This region seems to have been shaped by the passage of water. Channels scoured by ancient outbursts of flood waters are seen in this orbital view from Odyssey's Thermal Emission Imaging System.The channels are billions of years old and have likely been affected by multiple processes over time. Here, two channels, Tiu Vallis on the left and Ares Vallis on the right, flow northward from the highlands of the southern hemisphere of Mars.The stark difference between today's cold, dry Mars and the evidence of flood waters in the past tells scientists that the Martian climate has seen great changes
Ancient channels on Mars - Ancient channels on planet Mars. Ares Vallis - View of the area of Ares Vallis and Tiu Vallis obtained by the probe 2001 Mars Odyssey. This region seems to have been shaped by the passage of water. Channels scoured by ancient outbursts of flood waters are seen in this orbital view from Odyssey's Thermal Emission Imaging System.The channels are billions of years old and have likely been affected by multiple processes over time. Here, two channels, Tiu Vallis on the left and Ares Vallis on the right, flow northward from the highlands of the southern hemisphere of Mars.The stark difference between today's cold, dry Mars and the evidence of flood waters in the past tells scientists that the Martian climate has seen great changes

PIX4616321: Ancient channels on Mars - Ancient channels on planet Mars. Ares Vallis - View of the area of Ares Vallis and Tiu Vallis obtained by the probe 2001 Mars Odyssey. This region seems to have been shaped by the passage of water. Channels scoured by ancient outbursts of flood waters are seen in this orbital view from Odyssey's Thermal Emission Imaging System.The channels are billions of years old and have likely been affected by multiple processes over time. Here, two channels, Tiu Vallis on the left and Ares Vallis on the right, flow northward from the highlands of the southern hemisphere of Mars.The stark difference between today's cold, dry Mars and the evidence of flood waters in the past tells scientists that the Martian climate has seen great changes / Bridgeman Images

The cemetery of Pere Lachaise in Paris. The cemetery opened around 1804 on a land formerly owned by the Jesuit. The architect Alexandre Theodore Brongniart conceived the plans of 1810. Many artists worked at Pere-Lachaise in the first half of the 19th century. With an area of almost 44 hectares, it counts about 70 000 monuments.ÆPhotograph 06/06/05.
The cemetery of Pere Lachaise in Paris. The cemetery opened around 1804 on a land formerly owned by the Jesuit. The architect Alexandre Theodore Brongniart conceived the plans of 1810. Many artists worked at Pere-Lachaise in the first half of the 19th century. With an area of almost 44 hectares, it counts about 70 000 monuments.ÆPhotograph 06/06/05.

TEC4616567: The cemetery of Pere Lachaise in Paris. The cemetery opened around 1804 on a land formerly owned by the Jesuit. The architect Alexandre Theodore Brongniart conceived the plans of 1810. Many artists worked at Pere-Lachaise in the first half of the 19th century. With an area of almost 44 hectares, it counts about 70 000 monuments.ÆPhotograph 06/06/05. / Bridgeman Images

The three (Trio) (Lithography, 1913)
The three (Trio) (Lithography, 1913)

LRI4616336: The three (Trio) (Lithography, 1913), Malevich, Kazimir Severinovich (1878-1935) / Bridgeman Images

Houses in the district of Mouzaia in Parisæ20e.
Houses in the district of Mouzaia in Parisæ20e.

TEC4616369: Houses in the district of Mouzaia in Parisæ20e. / Bridgeman Images

Landscape with red houses Painting by Kasimir Severinovich Malevich (Malevich, Malevic) (1878-1935) Sun 107x106 cm 1910 Sun Kunstmuseum Bale
Landscape with red houses Painting by Kasimir Severinovich Malevich (Malevich, Malevic) (1878-1935) Sun 107x106 cm 1910 Sun Kunstmuseum Bale

LRI4616380: Landscape with red houses Painting by Kasimir Severinovich Malevich (Malevich, Malevic) (1878-1935) Sun 107x106 cm 1910 Sun Kunstmuseum Bale, Malevich, Kazimir Severinovich (1878-1935) / Bridgeman Images

Mars: faults in Claritas Fossae. - Mars: fractures in Claritas Fossae - Fracture system in Claritas Fossae, a region south of the Tharsis volcanoes. These fractures, ranging from a few kilometres to a hundred kilometres, are probably associated with the tectonic activity that led to elevation of the Tharsis plateau. Perspective image obtained by the Mars Express probe in 2004. On 29 June 2004 the High Resolution Stereo Camera (HRSC) onboard the ESA spacecraft Mars Express obtained image data in orbit 563 with a ground resolution of approximately 62 metres per pixel. The images cover Claritas Fossae at approximately 25* southern latitude and 253* eastern longitude. Claritas Fossae is located on the Tharsis rise, south of the three large volcanoes known as the Tharsis Montes, and extends roughly north to south for approximately 1800 km. Claritas Fossae, which is composed of a series of linear fractures with widths ranging from a few kilometres to 100 km, is roughly 150 km wide in the north and 550 km wide in the south. The series of fractures comprising Claritas Fossae are radial to the Tharsis rise, consistent with the idea that they are the result of enormous stresses associated with formation of the 8 to 10 km high Tharsis rise. In the east of the color image, a prominent linear feature exhibiting a dark shadow is visible. This is most likely a normal fault, the eastern edge of a 100 km wide graben, a block of terrain that drops relative to its surroundings as a result of extension. The graben is characterized by a smooth surface and the elevation difference between the eastern edge of the graben and the plains east of the normal fault is roughly 2.3 km. Alternatively, this 100 km wide feature may have resulted from surface collapse due to magma withdrawal
Mars: faults in Claritas Fossae. - Mars: fractures in Claritas Fossae - Fracture system in Claritas Fossae, a region south of the Tharsis volcanoes. These fractures, ranging from a few kilometres to a hundred kilometres, are probably associated with the tectonic activity that led to elevation of the Tharsis plateau. Perspective image obtained by the Mars Express probe in 2004. On 29 June 2004 the High Resolution Stereo Camera (HRSC) onboard the ESA spacecraft Mars Express obtained image data in orbit 563 with a ground resolution of approximately 62 metres per pixel. The images cover Claritas Fossae at approximately 25* southern latitude and 253* eastern longitude. Claritas Fossae is located on the Tharsis rise, south of the three large volcanoes known as the Tharsis Montes, and extends roughly north to south for approximately 1800 km. Claritas Fossae, which is composed of a series of linear fractures with widths ranging from a few kilometres to 100 km, is roughly 150 km wide in the north and 550 km wide in the south. The series of fractures comprising Claritas Fossae are radial to the Tharsis rise, consistent with the idea that they are the result of enormous stresses associated with formation of the 8 to 10 km high Tharsis rise. In the east of the color image, a prominent linear feature exhibiting a dark shadow is visible. This is most likely a normal fault, the eastern edge of a 100 km wide graben, a block of terrain that drops relative to its surroundings as a result of extension. The graben is characterized by a smooth surface and the elevation difference between the eastern edge of the graben and the plains east of the normal fault is roughly 2.3 km. Alternatively, this 100 km wide feature may have resulted from surface collapse due to magma withdrawal

PIX4616037: Mars: faults in Claritas Fossae. - Mars: fractures in Claritas Fossae - Fracture system in Claritas Fossae, a region south of the Tharsis volcanoes. These fractures, ranging from a few kilometres to a hundred kilometres, are probably associated with the tectonic activity that led to elevation of the Tharsis plateau. Perspective image obtained by the Mars Express probe in 2004. On 29 June 2004 the High Resolution Stereo Camera (HRSC) onboard the ESA spacecraft Mars Express obtained image data in orbit 563 with a ground resolution of approximately 62 metres per pixel. The images cover Claritas Fossae at approximately 25* southern latitude and 253* eastern longitude. Claritas Fossae is located on the Tharsis rise, south of the three large volcanoes known as the Tharsis Montes, and extends roughly north to south for approximately 1800 km. Claritas Fossae, which is composed of a series of linear fractures with widths ranging from a few kilometres to 100 km, is roughly 150 km wide in the north and 550 km wide in the south. The series of fractures comprising Claritas Fossae are radial to the Tharsis rise, consistent with the idea that they are the result of enormous stresses associated with formation of the 8 to 10 km high Tharsis rise. In the east of the color image, a prominent linear feature exhibiting a dark shadow is visible. This is most likely a normal fault, the eastern edge of a 100 km wide graben, a block of terrain that drops relative to its surroundings as a result of extension. The graben is characterized by a smooth surface and the elevation difference between the eastern edge of the graben and the plains east of the normal fault is roughly 2.3 km. Alternatively, this 100 km wide feature may have resulted from surface collapse due to magma withdrawal / Bridgeman Images

The cosmorama, exhibition of perspective pictures (Painting, 1757)
The cosmorama, exhibition of perspective pictures (Painting, 1757)

LRI4616085: The cosmorama, exhibition of perspective pictures (Painting, 1757), Longhi, Pietro (c.1701-85) / Bridgeman Images

Parisian corner building, on rue Pierre Dupont, Paris 10th. Photography 1990.
Parisian corner building, on rue Pierre Dupont, Paris 10th. Photography 1990.

MDA4616250: Parisian corner building, on rue Pierre Dupont, Paris 10th. Photography 1990. / Bridgeman Images

Landscape (oil on canvas, 20th century)
Landscape (oil on canvas, 20th century)

LRI4616699: Landscape (oil on canvas, 20th century), Mattioli, Carlo (1911-94) / Bridgeman Images

Corner building, Porte de Bagnolet in Paris 20th.
Corner building, Porte de Bagnolet in Paris 20th.

MDA4616780: Corner building, Porte de Bagnolet in Paris 20th. / Bridgeman Images

Paris seen from the 20th arrondissement.
Paris seen from the 20th arrondissement.

OMG4616915: Paris seen from the 20th arrondissement. / Bridgeman Images

Paris seen from the 20th arrondissement.
Paris seen from the 20th arrondissement.

OMG4616925: Paris seen from the 20th arrondissement. / Bridgeman Images

Sol de Mars seen by the Phoenix - Mars probe: Phoenix landing site - Image of the region around the Phoenix probe. The probe landed on a vast plain north of the planet in the Vastitas Borealis region. This approximate color view was obtained on sol 2 by the Surface Stereo Imager (SSI) on board the Phoenix lander. The view is toward the northwest, showing polygonal terrain near the lander and out to the horizon
Sol de Mars seen by the Phoenix - Mars probe: Phoenix landing site - Image of the region around the Phoenix probe. The probe landed on a vast plain north of the planet in the Vastitas Borealis region. This approximate color view was obtained on sol 2 by the Surface Stereo Imager (SSI) on board the Phoenix lander. The view is toward the northwest, showing polygonal terrain near the lander and out to the horizon

PIX4616607: Sol de Mars seen by the Phoenix - Mars probe: Phoenix landing site - Image of the region around the Phoenix probe. The probe landed on a vast plain north of the planet in the Vastitas Borealis region. This approximate color view was obtained on sol 2 by the Surface Stereo Imager (SSI) on board the Phoenix lander. The view is toward the northwest, showing polygonal terrain near the lander and out to the horizon / Bridgeman Images

The Parc de Belleville in Paris 20th. Amenagement 1988, architect Francois Debulois and Michel Viollet (landscape designer).
The Parc de Belleville in Paris 20th. Amenagement 1988, architect Francois Debulois and Michel Viollet (landscape designer).

LBY4616697: The Parc de Belleville in Paris 20th. Amenagement 1988, architect Francois Debulois and Michel Viollet (landscape designer). / Bridgeman Images

Paris seen from the 20th arrondissement.
Paris seen from the 20th arrondissement.

OMG4616866: Paris seen from the 20th arrondissement. / Bridgeman Images

Mars with water - Artist's view - Mars with ocean - Artwork - View of Mars at the time she had an ocean. In the foreground, a passing asteroid. Mars as it may have appeared from a passing asteroid during a warmer wetter period in its past
Mars with water - Artist's view - Mars with ocean - Artwork - View of Mars at the time she had an ocean. In the foreground, a passing asteroid. Mars as it may have appeared from a passing asteroid during a warmer wetter period in its past

PIX4616883: Mars with water - Artist's view - Mars with ocean - Artwork - View of Mars at the time she had an ocean. In the foreground, a passing asteroid. Mars as it may have appeared from a passing asteroid during a warmer wetter period in its past / Bridgeman Images

Paris seen from the 20th arrondissement.
Paris seen from the 20th arrondissement.

OMG4616914: Paris seen from the 20th arrondissement. / Bridgeman Images

Grotesque (Wood Sculpture, 1923)
Grotesque (Wood Sculpture, 1923)

LRI4617908: Grotesque (Wood Sculpture, 1923), Schlemmer, Oskar (1888-1943) / Bridgeman Images

A Morris column in front of the Opera Garnier, Paris 9th.
A Morris column in front of the Opera Garnier, Paris 9th.

TEC4618043: A Morris column in front of the Opera Garnier, Paris 9th. / Bridgeman Images


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