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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

ID: 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)

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

ID: 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 nor

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

ID: LRI4616085

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

Longhi, Pietro (c.1701-85)

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

ID: MDA4616250

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

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

ID: LRI4616699

Landscape (oil on canvas, 20th century)

Mattioli, Carlo (1911-94)

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

ID: MDA4616780

Corner building, Porte de Bagnolet in Paris 20th.

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

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

ID: OMG4616915

Paris seen from the 20th arrondissement.

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

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

ID: OMG4616925

Paris seen from the 20th arrondissement.

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

ID: 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

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

ID: LBY4616697

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

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

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

ID: OMG4616866

Paris seen from the 20th arrondissement.

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

ID: 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

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

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

ID: OMG4616914

Paris seen from the 20th arrondissement.

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

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

ID: LRI4617908

Grotesque (Wood Sculpture, 1923)

Schlemmer, Oskar (1888-1943)

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

ID: TEC4618043

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

Nebula M78 in Orion - M78 nebula in Orion - The nebula M78 (NGC 2068) is located about 1300 years - light from Earth and extends over 4 years - light. M78, (NGC2068) is part of the Orion complex, a large region of star - forming gas and dust centred around M42 and M43. It is the brightest diffuse reflection nebula in the sky. M78 is some 1600 light - years away and around 4 light - years across
Nebula M78 in Orion - M78 nebula in Orion - The nebula M78 (NGC 2068) is located about 1300 years - light from Earth and extends over 4 years - light. M78, (NGC2068) is part of the Orion complex, a large region of star - forming gas and dust centred around M42 and M43. It is the brightest diffuse reflection nebula in the sky. M78 is some 1600 light - years away and around 4 light - years across

PIX4618137: Nebula M78 in Orion - M78 nebula in Orion - The nebula M78 (NGC 2068) is located about 1300 years - light from Earth and extends over 4 years - light. M78, (NGC2068) is part of the Orion complex, a large region of star - forming gas and dust centred around M42 and M43. It is the brightest diffuse reflection nebula in the sky. M78 is some 1600 light - years away and around 4 light - years across / Bridgeman Images

ID: PIX4618137

Nebula M78 in Orion - M78 nebula in Orion - The nebula M78 (NGC 2068) is located about 1300 years - light from Earth and extends over 4 years - light. M78, (NGC2068) is part of the Orion complex, a large region of star - forming gas and dust centred around M42 and M43. It is the brightest diffuse reflection nebula in the sky. M78 is some 1600 light - years away and around 4 light - years across

The passage Joffroy in Paris 9th.
The passage Joffroy in Paris 9th.

TEC4618158: The passage Joffroy in Paris 9th. / Bridgeman Images

ID: TEC4618158

The passage Joffroy in Paris 9th.

La rue Scribe in Paris 9th. Photography 25/08/07.
La rue Scribe in Paris 9th. Photography 25/08/07.

TEC4618177: La rue Scribe in Paris 9th. Photography 25/08/07. / Bridgeman Images

ID: TEC4618177

La rue Scribe in Paris 9th. Photography 25/08/07.

Le department store Old England, 12 boulevard des Capucines, Paris 9th.
Le department store Old England, 12 boulevard des Capucines, Paris 9th.

TEC4618220: Le department store Old England, 12 boulevard des Capucines, Paris 9th. / Bridgeman Images

ID: TEC4618220

Le department store Old England, 12 boulevard des Capucines, Paris 9th.

Rue Edouard VII in Paris 9th. Photography 30/08/99.
Rue Edouard VII in Paris 9th. Photography 30/08/99.

TEC4617893: Rue Edouard VII in Paris 9th. Photography 30/08/99. / Bridgeman Images

ID: TEC4617893

Rue Edouard VII in Paris 9th. Photography 30/08/99.

Pear. 1938 (Collage)
Pear. 1938 (Collage)

LRI4617933: Pear. 1938 (Collage), Schwitters, Kurt (1887-1948) / Bridgeman Images

ID: LRI4617933

Pear. 1938 (Collage)

Schwitters, Kurt (1887-1948)

Avenue Frochot in Paris 9th.
Avenue Frochot in Paris 9th.

TEC4618025: Avenue Frochot in Paris 9th. / Bridgeman Images

ID: TEC4618025

Avenue Frochot in Paris 9th.

Impasse de la tour d'Auvergne à Paris 9th.
Impasse de la tour d'Auvergne à Paris 9th.

TEC4618033: Impasse de la tour d'Auvergne à Paris 9th. / Bridgeman Images

ID: TEC4618033

Impasse de la tour d'Auvergne à Paris 9th.

Detail in the Tarantula Nebula - Part of the Tarantula Nebula - The Tarantula Nebula (or 30 Bream bream) is the largest star-forming region of the Magellan Cloud. It is located 170,000 light years ago in the constellation Dorado (southern hemisphere). This image obtained by the Hubble Space Telescope (HST) shows a detail of the nebula around NGC 2060, a cluster of stars associated with a remnant of supernova (N157b) housing a pulsar. The part of the Tarentula nebula visible in this image from Hubble's Advanced Camera for Surveys is criss - crossed with tendrils of dust and gas churned up by recent supernovae. These supernova remnants include NGC 2060, visible above and to the left of the centre of this image, which contains the brightest known pulsar. The tarantula's bite goes beyond NGC 2060. Near the edge of the nebula, outside the frame, below and to the right, lie the remains of supernova SN 1987a, the closest supernova to Earth to be observed since the invention of telescopes in the 17th century. Together with dying stars, the Tarantula Nebula is packed with young stars which have recently formed from the nebula's supply of hydrogen gas. These toddler - stars shine forth with intense ultraviolet light that ionises the gas, making it light up red. The light is so intense that although around 170,000 light - years distant, and outside the Milky Way, the Tarantula Nebula is nevertheless visible without a telescope on a dark night to Earth - bound observers. This nebula might be far away, but it is the most luminous example of its type that astronomers have observed in the local Universe
Detail in the Tarantula Nebula - Part of the Tarantula Nebula - The Tarantula Nebula (or 30 Bream bream) is the largest star-forming region of the Magellan Cloud. It is located 170,000 light years ago in the constellation Dorado (southern hemisphere). This image obtained by the Hubble Space Telescope (HST) shows a detail of the nebula around NGC 2060, a cluster of stars associated with a remnant of supernova (N157b) housing a pulsar. The part of the Tarentula nebula visible in this image from Hubble's Advanced Camera for Surveys is criss - crossed with tendrils of dust and gas churned up by recent supernovae. These supernova remnants include NGC 2060, visible above and to the left of the centre of this image, which contains the brightest known pulsar. The tarantula's bite goes beyond NGC 2060. Near the edge of the nebula, outside the frame, below and to the right, lie the remains of supernova SN 1987a, the closest supernova to Earth to be observed since the invention of telescopes in the 17th century. Together with dying stars, the Tarantula Nebula is packed with young stars which have recently formed from the nebula's supply of hydrogen gas. These toddler - stars shine forth with intense ultraviolet light that ionises the gas, making it light up red. The light is so intense that although around 170,000 light - years distant, and outside the Milky Way, the Tarantula Nebula is nevertheless visible without a telescope on a dark night to Earth - bound observers. This nebula might be far away, but it is the most luminous example of its type that astronomers have observed in the local Universe

PIX4618146: Detail in the Tarantula Nebula - Part of the Tarantula Nebula - The Tarantula Nebula (or 30 Bream bream) is the largest star-forming region of the Magellan Cloud. It is located 170,000 light years ago in the constellation Dorado (southern hemisphere). This image obtained by the Hubble Space Telescope (HST) shows a detail of the nebula around NGC 2060, a cluster of stars associated with a remnant of supernova (N157b) housing a pulsar. The part of the Tarentula nebula visible in this image from Hubble's Advanced Camera for Surveys is criss - crossed with tendrils of dust and gas churned up by recent supernovae. These supernova remnants include NGC 2060, visible above and to the left of the centre of this image, which contains the brightest known pulsar. The tarantula's bite goes beyond NGC 2060. Near the edge of the nebula, outside the frame, below and to the right, lie the remains of supernova SN 1987a, the closest supernova to Earth to be observed since the invention of telescopes in the 17th century. Together with dying stars, the Tarantula Nebula is packed with young stars which have recently formed from the nebula's supply of hydrogen gas. These toddler - stars shine forth with intense ultraviolet light that ionises the gas, making it light up red. The light is so intense that although around 170,000 light - years distant, and outside the Milky Way, the Tarantula Nebula is nevertheless visible without a telescope on a dark night to Earth - bound observers. This nebula might be far away, but it is the most luminous example of its type that astronomers have observed in the local Universe / Bridgeman Images

ID: PIX4618146

Detail in the Tarantula Nebula - Part of the Tarantula Nebula - The Tarantula Nebula (or 30 Bream bream) is the largest star-forming region of the Magellan Cloud. It is located 170,000 light years ago in the constellation Dorado (southern hemisphere). This image obtained by the Hubble Space Telescope (HST) shows a detail of the nebula around NGC 2060, a cluster of stars associated with a remnant of supernova (N157b) housing a pulsar. The part of the Tarentula nebula visible in this image from Hubble's Advanced Camera for Surveys is criss - crossed with tendrils of dust and gas churned up by recent supernovae. These supernova remnants include NGC 2060, visible above and to the left of the centre of this image, which contains the brightest known pulsar. The tarantula's bite goes beyond NGC 2060. Near the edge of the nebula, outside the frame, below and to the right, lie the remains of supernova SN 1987a, the closest supernova to Earth to be observed since the invention of telescopes in t

Rue des Martyrs in Paris 9th.
Rue des Martyrs in Paris 9th.

TEC4617291: Rue des Martyrs in Paris 9th. / Bridgeman Images

ID: TEC4617291

Rue des Martyrs in Paris 9th.

Place de Toutwelve in Paris 9th.
Place de Toutwelve in Paris 9th.

TEC4617331: Place de Toutwelve in Paris 9th. / Bridgeman Images

ID: TEC4617331

Place de Toutwelve in Paris 9th.

Rue de la tower des dames in Paris 9e.
Rue de la tower des dames in Paris 9e.

TEC4617425: Rue de la tower des dames in Paris 9e. / Bridgeman Images

ID: TEC4617425

Rue de la tower des dames in Paris 9e.

Nebula NGC 281 in Cassiopee - This region of stole formation is located about 10,000 light years from Earth. Image obtained by Isaac Newton 2.5m telescope from La Palma
Nebula NGC 281 in Cassiopee - This region of stole formation is located about 10,000 light years from Earth. Image obtained by Isaac Newton 2.5m telescope from La Palma

PIX4617450: Nebula NGC 281 in Cassiopee - This region of stole formation is located about 10,000 light years from Earth. Image obtained by Isaac Newton 2.5m telescope from La Palma / Bridgeman Images

ID: PIX4617450

Nebula NGC 281 in Cassiopee - This region of stole formation is located about 10,000 light years from Earth. Image obtained by Isaac Newton 2.5m telescope from La Palma

Nebula NGC 1333 in Persee - Nebula NGC 1333 in Persee - NGC 1333 is a nebula located 720 years - light from Earth. It's a reflexion nebula and a star-forming region.
Nebula NGC 1333 in Persee - Nebula NGC 1333 in Persee - NGC 1333 is a nebula located 720 years - light from Earth. It's a reflexion nebula and a star-forming region.

PIX4617527: Nebula NGC 1333 in Persee - Nebula NGC 1333 in Persee - NGC 1333 is a nebula located 720 years - light from Earth. It's a reflexion nebula and a star-forming region. / Bridgeman Images

ID: PIX4617527

Nebula NGC 1333 in Persee - Nebula NGC 1333 in Persee - NGC 1333 is a nebula located 720 years - light from Earth. It's a reflexion nebula and a star-forming region.

Tarantula Nebula in the Great Magellan Cloud - Tarantula Nebula in the Great Magellan Cloud - NGC 2070, the Tarantula Nebula is a vast star-forming region located north of the Great Magellan Cloud galaxy, in the southern hemisphere about 170,000 years - light from Earth. Mosaic of images obtained by the 2.2m telescope of La Silla - Chile
Tarantula Nebula in the Great Magellan Cloud - Tarantula Nebula in the Great Magellan Cloud - NGC 2070, the Tarantula Nebula is a vast star-forming region located north of the Great Magellan Cloud galaxy, in the southern hemisphere about 170,000 years - light from Earth. Mosaic of images obtained by the 2.2m telescope of La Silla - Chile

PIX4618279: Tarantula Nebula in the Great Magellan Cloud - Tarantula Nebula in the Great Magellan Cloud - NGC 2070, the Tarantula Nebula is a vast star-forming region located north of the Great Magellan Cloud galaxy, in the southern hemisphere about 170,000 years - light from Earth. Mosaic of images obtained by the 2.2m telescope of La Silla - Chile / Bridgeman Images

ID: PIX4618279

Tarantula Nebula in the Great Magellan Cloud - Tarantula Nebula in the Great Magellan Cloud - NGC 2070, the Tarantula Nebula is a vast star-forming region located north of the Great Magellan Cloud galaxy, in the southern hemisphere about 170,000 years - light from Earth. Mosaic of images obtained by the 2.2m telescope of La Silla - Chile

Nebula NGC 2170 in Unicorn - Nebula NGC 2170 in Monoceros - Nebula by reflexion located in the constellation Unicorn. This rich collection of predominantly reflection and sparse emission nebulosity exists in the western part of a vast star forming region known as the Mon R 2 association. The “” R”” designation stands for reflection and indicates an association of stars illuminating reflection nebulae. Most of the members of Mon R 2 are type B stars located along an east - west line stretching across 2 degrees of the winter sky, situated about 8 degrees east of the Orion Nebula. The Mon R 2 association resides at a distance of 830 pc and formed about 6 to 10 million years ago along the edge of the Mon R2 molecular cloud. NGC2170 is a common nebula imaged and yet with long exposures it takes on a whole new look. Many of the nebulae seen here appear to be uncataloged and not previously imaged. This image has been carefully processed to reveal the many faint and dusty nebulae in this region of Monoceros
Nebula NGC 2170 in Unicorn - Nebula NGC 2170 in Monoceros - Nebula by reflexion located in the constellation Unicorn. This rich collection of predominantly reflection and sparse emission nebulosity exists in the western part of a vast star forming region known as the Mon R 2 association. The “” R”” designation stands for reflection and indicates an association of stars illuminating reflection nebulae. Most of the members of Mon R 2 are type B stars located along an east - west line stretching across 2 degrees of the winter sky, situated about 8 degrees east of the Orion Nebula. The Mon R 2 association resides at a distance of 830 pc and formed about 6 to 10 million years ago along the edge of the Mon R2 molecular cloud. NGC2170 is a common nebula imaged and yet with long exposures it takes on a whole new look. Many of the nebulae seen here appear to be uncataloged and not previously imaged. This image has been carefully processed to reveal the many faint and dusty nebulae in this region of Monoceros

PIX4618385: Nebula NGC 2170 in Unicorn - Nebula NGC 2170 in Monoceros - Nebula by reflexion located in the constellation Unicorn. This rich collection of predominantly reflection and sparse emission nebulosity exists in the western part of a vast star forming region known as the Mon R 2 association. The “” R”” designation stands for reflection and indicates an association of stars illuminating reflection nebulae. Most of the members of Mon R 2 are type B stars located along an east - west line stretching across 2 degrees of the winter sky, situated about 8 degrees east of the Orion Nebula. The Mon R 2 association resides at a distance of 830 pc and formed about 6 to 10 million years ago along the edge of the Mon R2 molecular cloud. NGC2170 is a common nebula imaged and yet with long exposures it takes on a whole new look. Many of the nebulae seen here appear to be uncataloged and not previously imaged. This image has been carefully processed to reveal the many faint and dusty nebulae in this region of Monoceros / Bridgeman Images

ID: PIX4618385

Nebula NGC 2170 in Unicorn - Nebula NGC 2170 in Monoceros - Nebula by reflexion located in the constellation Unicorn. This rich collection of predominantly reflection and sparse emission nebulosity exists in the western part of a vast star forming region known as the Mon R 2 association. The “” R”” designation stands for reflection and indicates an association of stars illuminating reflection nebulae. Most of the members of Mon R 2 are type B stars located along an east - west line stretching across 2 degrees of the winter sky, situated about 8 degrees east of the Orion Nebula. The Mon R 2 association resides at a distance of 830 pc and formed about 6 to 10 million years ago along the edge of the Mon R2 molecular cloud. NGC2170 is a common nebula imaged and yet with long exposures it takes on a whole new look. Many of the nebulae seen here appear to be uncataloged and not previously imaged. This image has been carefully processed to reveal the many faint and dusty nebulae in this regio

L'Hotel des Ventes Drouot Richelieu, 9 Rue Drouot in Paris 9e. The aluminium panels of the facades are designed to evoke the curtains of the concierges.Construction 1980, architectesæ Jean Jacques Fernier and Andre Biro. Photography 11/09/07.
L'Hotel des Ventes Drouot Richelieu, 9 Rue Drouot in Paris 9e. The aluminium panels of the facades are designed to evoke the curtains of the concierges.Construction 1980, architectesæ Jean Jacques Fernier and Andre Biro. Photography 11/09/07.

TEC4618394: L'Hotel des Ventes Drouot Richelieu, 9 Rue Drouot in Paris 9e. The aluminium panels of the facades are designed to evoke the curtains of the concierges.Construction 1980, architectesæ Jean Jacques Fernier and Andre Biro. Photography 11/09/07., Biro, Andre (b.1926) & Fernier, Jean-Jacques (1931-2020) / Bridgeman Images

ID: TEC4618394

L'Hotel des Ventes Drouot Richelieu, 9 Rue Drouot in Paris 9e. The aluminium panels of the facades are designed to evoke the curtains of the concierges.Construction 1980, architectesæ Jean Jacques Fernier and Andre Biro. Photography 11/09/07.

Biro, Andre (b.1926) & Fernier, Jean-Jacques (1931-2020)

La Place de l'Opera in Paris 9th. Photography 10/05/02.
La Place de l'Opera in Paris 9th. Photography 10/05/02.

LBY4618505: La Place de l'Opera in Paris 9th. Photography 10/05/02. / Bridgeman Images

ID: LBY4618505

La Place de l'Opera in Paris 9th. Photography 10/05/02.

Around the Tarantula Nebula - Around the Tarantula nebula in the Large Magellanic Cloud - The Tarantula Nebula (or 30 Bream) is the largest star-forming region of the Great Magellan Cloud. It is located 170,000 light years ago in the constellation Dorado (southern hemisphere). At the center of this nebula, the open cluster of R136 stars, clusters of hot and massive stars. Image obtained with the 1.2m Schmidt UK Telescope from Siding Spring. In this picture we see the eastern end of the Large Magellanic Cloud where lies one of the most active star formation regions known. If this enormous complex of stars, gas and dust were at the distance of the better - known Orion Nebula the brightest parts of it would visible during the day and would cover a quarter of the sky at night. While the Orion Nebula contains a mere handful of the hot blue stars which energise it, the Tarantula nebula has spawned many thousands in the bright central region, which surrounds a compact, brilliant cluster known as 30 Doradus. Like the Orion Nebula, the 30 Doradus region is a naked eye object for the keen sighted. It is however over one hundred times more distant! Surrounding this nebula is a huge and much fainter series of interlocking bubbles and shells of gas and dust blow away from the center of activity by intense stellar winds and supernova explosions
Around the Tarantula Nebula - Around the Tarantula nebula in the Large Magellanic Cloud - The Tarantula Nebula (or 30 Bream) is the largest star-forming region of the Great Magellan Cloud. It is located 170,000 light years ago in the constellation Dorado (southern hemisphere). At the center of this nebula, the open cluster of R136 stars, clusters of hot and massive stars. Image obtained with the 1.2m Schmidt UK Telescope from Siding Spring. In this picture we see the eastern end of the Large Magellanic Cloud where lies one of the most active star formation regions known. If this enormous complex of stars, gas and dust were at the distance of the better - known Orion Nebula the brightest parts of it would visible during the day and would cover a quarter of the sky at night. While the Orion Nebula contains a mere handful of the hot blue stars which energise it, the Tarantula nebula has spawned many thousands in the bright central region, which surrounds a compact, brilliant cluster known as 30 Doradus. Like the Orion Nebula, the 30 Doradus region is a naked eye object for the keen sighted. It is however over one hundred times more distant! Surrounding this nebula is a huge and much fainter series of interlocking bubbles and shells of gas and dust blow away from the center of activity by intense stellar winds and supernova explosions

PIX4618257: Around the Tarantula Nebula - Around the Tarantula nebula in the Large Magellanic Cloud - The Tarantula Nebula (or 30 Bream) is the largest star-forming region of the Great Magellan Cloud. It is located 170,000 light years ago in the constellation Dorado (southern hemisphere). At the center of this nebula, the open cluster of R136 stars, clusters of hot and massive stars. Image obtained with the 1.2m Schmidt UK Telescope from Siding Spring. In this picture we see the eastern end of the Large Magellanic Cloud where lies one of the most active star formation regions known. If this enormous complex of stars, gas and dust were at the distance of the better - known Orion Nebula the brightest parts of it would visible during the day and would cover a quarter of the sky at night. While the Orion Nebula contains a mere handful of the hot blue stars which energise it, the Tarantula nebula has spawned many thousands in the bright central region, which surrounds a compact, brilliant cluster known as 30 Doradus. Like the Orion Nebula, the 30 Doradus region is a naked eye object for the keen sighted. It is however over one hundred times more distant! Surrounding this nebula is a huge and much fainter series of interlocking bubbles and shells of gas and dust blow away from the center of activity by intense stellar winds and supernova explosions / Bridgeman Images

ID: PIX4618257

Around the Tarantula Nebula - Around the Tarantula nebula in the Large Magellanic Cloud - The Tarantula Nebula (or 30 Bream) is the largest star-forming region of the Great Magellan Cloud. It is located 170,000 light years ago in the constellation Dorado (southern hemisphere). At the center of this nebula, the open cluster of R136 stars, clusters of hot and massive stars. Image obtained with the 1.2m Schmidt UK Telescope from Siding Spring. In this picture we see the eastern end of the Large Magellanic Cloud where lies one of the most active star formation regions known. If this enormous complex of stars, gas and dust were at the distance of the better - known Orion Nebula the brightest parts of it would visible during the day and would cover a quarter of the sky at night. While the Orion Nebula contains a mere handful of the hot blue stars which energise it, the Tarantula nebula has spawned many thousands in the bright central region, which surrounds a compact, brilliant cluster known

Metro Richelieu Drout in Paris 9th.
Metro Richelieu Drout in Paris 9th.

TEC4618330: Metro Richelieu Drout in Paris 9th. / Bridgeman Images

ID: TEC4618330

Metro Richelieu Drout in Paris 9th.

Urban display in Paris. Photography 11/09/07.
Urban display in Paris. Photography 11/09/07.

TEC4618361: Urban display in Paris. Photography 11/09/07. / Bridgeman Images

ID: TEC4618361

Urban display in Paris. Photography 11/09/07.


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