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Bilbao in Spain. Photography 05/05/06.
Bilbao in Spain. Photography 05/05/06.

TEC4607973: Bilbao in Spain. Photography 05/05/06. / Bridgeman Images

ID: TEC4607973

Bilbao in Spain. Photography 05/05/06.

Deauville (Calvados, Lower Normandy).
Deauville (Calvados, Lower Normandy).

TEC4608148: Deauville (Calvados, Lower Normandy). / Bridgeman Images

ID: TEC4608148

Deauville (Calvados, Lower Normandy).

Museum in the city of Chandigarh, India. Photography 23/01/06.
Museum in the city of Chandigarh, India. Photography 23/01/06.

TEC4608256: Museum in the city of Chandigarh, India. Photography 23/01/06. / Bridgeman Images

ID: TEC4608256

Museum in the city of Chandigarh, India. Photography 23/01/06.

Museum in the city of Chandigarh, India. Photography 23/01/06.
Museum in the city of Chandigarh, India. Photography 23/01/06.

TEC4608273: Museum in the city of Chandigarh, India. Photography 23/01/06. / Bridgeman Images

ID: TEC4608273

Museum in the city of Chandigarh, India. Photography 23/01/06.

K.C cinema in sector 17 in Chandigarh, India.
K.C cinema in sector 17 in Chandigarh, India.

TEC4608286: K.C cinema in sector 17 in Chandigarh, India. / Bridgeman Images

ID: TEC4608286

K.C cinema in sector 17 in Chandigarh, India.

Building facade in Chandigarh, India. Photography 23/01/06.
Building facade in Chandigarh, India. Photography 23/01/06.

TEC4608367: Building facade in Chandigarh, India. Photography 23/01/06. / Bridgeman Images

ID: TEC4608367

Building facade in Chandigarh, India. Photography 23/01/06.

Signage of sector 21 in Chandigarh, India.
Signage of sector 21 in Chandigarh, India.

TEC4608405: Signage of sector 21 in Chandigarh, India. / Bridgeman Images

ID: TEC4608405

Signage of sector 21 in Chandigarh, India.

Detail of a claustra of a residential building in Chandigarh, India.
Detail of a claustra of a residential building in Chandigarh, India.

TEC4608463: Detail of a claustra of a residential building in Chandigarh, India. / Bridgeman Images

ID: TEC4608463

Detail of a claustra of a residential building in Chandigarh, India.

Housing building under construction in Chandigarh, India.
Housing building under construction in Chandigarh, India.

TEC4608503: Housing building under construction in Chandigarh, India. / Bridgeman Images

ID: TEC4608503

Housing building under construction in Chandigarh, India.

Delta II rocket decolving 04/01 - Delta II rocket carrying the Mars Odyssey probe. 07/04/2001
Delta II rocket decolving 04/01 - Delta II rocket carrying the Mars Odyssey probe. 07/04/2001

PIX4605095: Delta II rocket decolving 04/01 - Delta II rocket carrying the Mars Odyssey probe. 07/04/2001 / Bridgeman Images

ID: PIX4605095

Delta II rocket decolving 04/01 - Delta II rocket carrying the Mars Odyssey probe. 07/04/2001

Alexandria, Egypt. Photograph 22/05/02.
Alexandria, Egypt. Photograph 22/05/02.

TEC4583937: Alexandria, Egypt. Photograph 22/05/02. / Bridgeman Images

ID: TEC4583937

Alexandria, Egypt. Photograph 22/05/02.

The entrance of the Ministry of Culture, Jardins du Palais Royal, Paris.
The entrance of the Ministry of Culture, Jardins du Palais Royal, Paris.

TEC4605288: The entrance of the Ministry of Culture, Jardins du Palais Royal, Paris. / Bridgeman Images

ID: TEC4605288

The entrance of the Ministry of Culture, Jardins du Palais Royal, Paris.

Pekin, China. Photograph 01/10/02.
Pekin, China. Photograph 01/10/02.

TEC4583976: Pekin, China. Photograph 01/10/02. / Bridgeman Images

ID: TEC4583976

Pekin, China. Photograph 01/10/02.

Inhabited mission to an asteroid - Artist's view - Asteroid Lander prepares for touchdown - A living spaceship lands on the surface of an asteroid. A manned Asteroid Lander descends towards the rugged and cratered surface of an ancient asteroid. Orbiting the asteroid on the upper left is a Deep Space Vehicle (DSV) and Extended Stay Module (ESM)
Inhabited mission to an asteroid - Artist's view - Asteroid Lander prepares for touchdown - A living spaceship lands on the surface of an asteroid. A manned Asteroid Lander descends towards the rugged and cratered surface of an ancient asteroid. Orbiting the asteroid on the upper left is a Deep Space Vehicle (DSV) and Extended Stay Module (ESM)

PIX4584017: Inhabited mission to an asteroid - Artist's view - Asteroid Lander prepares for touchdown - A living spaceship lands on the surface of an asteroid. A manned Asteroid Lander descends towards the rugged and cratered surface of an ancient asteroid. Orbiting the asteroid on the upper left is a Deep Space Vehicle (DSV) and Extended Stay Module (ESM) / Bridgeman Images

ID: PIX4584017

Inhabited mission to an asteroid - Artist's view - Asteroid Lander prepares for touchdown - A living spaceship lands on the surface of an asteroid. A manned Asteroid Lander descends towards the rugged and cratered surface of an ancient asteroid. Orbiting the asteroid on the upper left is a Deep Space Vehicle (DSV) and Extended Stay Module (ESM)

Pioneer plate placed on Pioneer 10 - Pioneer 10 and Pioneer 11 probes have embarked on a plate, called the Pioneer plate, containing a message intended for potential aliens. On this engraved metal plate are depicted a naked man and woman, the location of our Sun as well as 14 pulsars, the trajectory of the probe in the solar system... Pioneer 10 was launched on 3 March 1972 with as its first destination, the Jupiter planet, which it flew over on 3 December 1973; it was the first space probe to approach this planet; it was also the first space probe to leave the solar system.
Pioneer plate placed on Pioneer 10 - Pioneer 10 and Pioneer 11 probes have embarked on a plate, called the Pioneer plate, containing a message intended for potential aliens. On this engraved metal plate are depicted a naked man and woman, the location of our Sun as well as 14 pulsars, the trajectory of the probe in the solar system... Pioneer 10 was launched on 3 March 1972 with as its first destination, the Jupiter planet, which it flew over on 3 December 1973; it was the first space probe to approach this planet; it was also the first space probe to leave the solar system.

PIX4605586: Pioneer plate placed on Pioneer 10 - Pioneer 10 and Pioneer 11 probes have embarked on a plate, called the Pioneer plate, containing a message intended for potential aliens. On this engraved metal plate are depicted a naked man and woman, the location of our Sun as well as 14 pulsars, the trajectory of the probe in the solar system... Pioneer 10 was launched on 3 March 1972 with as its first destination, the Jupiter planet, which it flew over on 3 December 1973; it was the first space probe to approach this planet; it was also the first space probe to leave the solar system. / Bridgeman Images

ID: PIX4605586

Pioneer plate placed on Pioneer 10 - Pioneer 10 and Pioneer 11 probes have embarked on a plate, called the Pioneer plate, containing a message intended for potential aliens. On this engraved metal plate are depicted a naked man and woman, the location of our Sun as well as 14 pulsars, the trajectory of the probe in the solar system... Pioneer 10 was launched on 3 March 1972 with as its first destination, the Jupiter planet, which it flew over on 3 December 1973; it was the first space probe to approach this planet; it was also the first space probe to leave the solar system.

Pekin, China. Photograph 01/10/02.
Pekin, China. Photograph 01/10/02.

TEC4584071: Pekin, China. Photograph 01/10/02. / Bridgeman Images

ID: TEC4584071

Pekin, China. Photograph 01/10/02.

Rue Duphot with in perspective the church of the Madeleine in Paris.
Rue Duphot with in perspective the church of the Madeleine in Paris.

TEC4605670: Rue Duphot with in perspective the church of the Madeleine in Paris. / Bridgeman Images

ID: TEC4605670

Rue Duphot with in perspective the church of the Madeleine in Paris.

Pioneer Venus orbiter - Artist view - Pioneer Venus orbiter - Artist view - The Pioneer Venus Project was a NASA space exploration mission to Venus launched in 1978. It consisted of two separate probes, one to study Venus from its orbit (Pioneer Venus Orbiter) and the other to analyze the atmosphere of the planet through 4 atmospheric probes (Pioneer Venus Multiprobe). An artist concept of the orbiter approaching Venus is shown here
Pioneer Venus orbiter - Artist view - Pioneer Venus orbiter - Artist view - The Pioneer Venus Project was a NASA space exploration mission to Venus launched in 1978. It consisted of two separate probes, one to study Venus from its orbit (Pioneer Venus Orbiter) and the other to analyze the atmosphere of the planet through 4 atmospheric probes (Pioneer Venus Multiprobe). An artist concept of the orbiter approaching Venus is shown here

PIX4605693: Pioneer Venus orbiter - Artist view - Pioneer Venus orbiter - Artist view - The Pioneer Venus Project was a NASA space exploration mission to Venus launched in 1978. It consisted of two separate probes, one to study Venus from its orbit (Pioneer Venus Orbiter) and the other to analyze the atmosphere of the planet through 4 atmospheric probes (Pioneer Venus Multiprobe). An artist concept of the orbiter approaching Venus is shown here / Bridgeman Images

ID: PIX4605693

Pioneer Venus orbiter - Artist view - Pioneer Venus orbiter - Artist view - The Pioneer Venus Project was a NASA space exploration mission to Venus launched in 1978. It consisted of two separate probes, one to study Venus from its orbit (Pioneer Venus Orbiter) and the other to analyze the atmosphere of the planet through 4 atmospheric probes (Pioneer Venus Multiprobe). An artist concept of the orbiter approaching Venus is shown here

Pekin, China. Photograph 01/10/02.
Pekin, China. Photograph 01/10/02.

TEC4584264: Pekin, China. Photograph 01/10/02. / Bridgeman Images

ID: TEC4584264

Pekin, China. Photograph 01/10/02.

Artist's view of a black hole
Artist's view of a black hole

PIX4584364: Artist's view of a black hole / Bridgeman Images

ID: PIX4584364

Artist's view of a black hole

Huygens probe en route to Titan. - Artist's view of the Cassini probe during the separation of the European module Huygens on 25 December 2004. Huygens landed on the Titan satellite on 14 January 2005. The Cassini-Huygens probe was launched on 15 October 1997 and has been placed in orbit around Saturn since 1 July 200
Huygens probe en route to Titan. - Artist's view of the Cassini probe during the separation of the European module Huygens on 25 December 2004. Huygens landed on the Titan satellite on 14 January 2005. The Cassini-Huygens probe was launched on 15 October 1997 and has been placed in orbit around Saturn since 1 July 200

PIX4605992: Huygens probe en route to Titan. - Artist's view of the Cassini probe during the separation of the European module Huygens on 25 December 2004. Huygens landed on the Titan satellite on 14 January 2005. The Cassini-Huygens probe was launched on 15 October 1997 and has been placed in orbit around Saturn since 1 July 200 / Bridgeman Images

ID: PIX4605992

Huygens probe en route to Titan. - Artist's view of the Cassini probe during the separation of the European module Huygens on 25 December 2004. Huygens landed on the Titan satellite on 14 January 2005. The Cassini-Huygens probe was launched on 15 October 1997 and has been placed in orbit around Saturn since 1 July 200

Stellar black hole - Artist view - Stellar black hole - Artist view - A stellar black hole is born from the gravitational collapse of a massive star. The stellar black holes have a mass of some solar masses. A black hole is a region of space whose gravitation is so strong that it will prevent any form of material or radiation from escaping. A stellar black hole is a black hole formed by the gravitational collapse of a massive star; it is also a region of space in which the gravitational field is so powerful that nothing can escape
Stellar black hole - Artist view - Stellar black hole - Artist view - A stellar black hole is born from the gravitational collapse of a massive star. The stellar black holes have a mass of some solar masses. A black hole is a region of space whose gravitation is so strong that it will prevent any form of material or radiation from escaping. A stellar black hole is a black hole formed by the gravitational collapse of a massive star; it is also a region of space in which the gravitational field is so powerful that nothing can escape

PIX4584774: Stellar black hole - Artist view - Stellar black hole - Artist view - A stellar black hole is born from the gravitational collapse of a massive star. The stellar black holes have a mass of some solar masses. A black hole is a region of space whose gravitation is so strong that it will prevent any form of material or radiation from escaping. A stellar black hole is a black hole formed by the gravitational collapse of a massive star; it is also a region of space in which the gravitational field is so powerful that nothing can escape / Bridgeman Images

ID: PIX4584774

Stellar black hole - Artist view - Stellar black hole - Artist view - A stellar black hole is born from the gravitational collapse of a massive star. The stellar black holes have a mass of some solar masses. A black hole is a region of space whose gravitation is so strong that it will prevent any form of material or radiation from escaping. A stellar black hole is a black hole formed by the gravitational collapse of a massive star; it is also a region of space in which the gravitational field is so powerful that nothing can escape

Porte de Versailles, Paris 15th arrondissement.
Porte de Versailles, Paris 15th arrondissement.

TEC4584923: Porte de Versailles, Paris 15th arrondissement. / Bridgeman Images

ID: TEC4584923

Porte de Versailles, Paris 15th arrondissement.

SMART Probe - 1 - Artist View - SMART Probe - 1 - Artist View - SMART - 1 (Small Missions for Advanced Research in Technology) is a European probe that maps the Moon and tests new technologies such as ion propulsion. The mission took place from 27 September 2003 to 3 September 2006
SMART Probe - 1 - Artist View - SMART Probe - 1 - Artist View - SMART - 1 (Small Missions for Advanced Research in Technology) is a European probe that maps the Moon and tests new technologies such as ion propulsion. The mission took place from 27 September 2003 to 3 September 2006

PIX4606133: SMART Probe - 1 - Artist View - SMART Probe - 1 - Artist View - SMART - 1 (Small Missions for Advanced Research in Technology) is a European probe that maps the Moon and tests new technologies such as ion propulsion. The mission took place from 27 September 2003 to 3 September 2006 / Bridgeman Images

ID: PIX4606133

SMART Probe - 1 - Artist View - SMART Probe - 1 - Artist View - SMART - 1 (Small Missions for Advanced Research in Technology) is a European probe that maps the Moon and tests new technologies such as ion propulsion. The mission took place from 27 September 2003 to 3 September 2006

Porte de Versailles, Paris 15th arrondissement.
Porte de Versailles, Paris 15th arrondissement.

TEC4584927: Porte de Versailles, Paris 15th arrondissement. / Bridgeman Images

ID: TEC4584927

Porte de Versailles, Paris 15th arrondissement.

Sundial - Paris - Sundial in Paris - Sundial de la rue Saint Maur, à Paris (Xeme) Dial dating from 1907, decorated with a Tournesol. Sundial in Paris, rue Saint Maur, 75010
Sundial - Paris - Sundial in Paris - Sundial de la rue Saint Maur, à Paris (Xeme) Dial dating from 1907, decorated with a Tournesol. Sundial in Paris, rue Saint Maur, 75010

PIX4585009: Sundial - Paris - Sundial in Paris - Sundial de la rue Saint Maur, à Paris (Xeme) Dial dating from 1907, decorated with a Tournesol. Sundial in Paris, rue Saint Maur, 75010 / Bridgeman Images

ID: PIX4585009

Sundial - Paris - Sundial in Paris - Sundial de la rue Saint Maur, à Paris (Xeme) Dial dating from 1907, decorated with a Tournesol. Sundial in Paris, rue Saint Maur, 75010

LCROSS Probe - Artist View - LCROSS - Artist view - LCROSS (Lunar Crater Observation and Sensing Satellite) is a space probe of NASA whose aim is to discover the presence of water ice in a crater perpetually in the shade of the Sun at the southern pole of the Moon. LCROSS must analyze the impact created by the top floor of its Atlas 5 launcher precipitates in this crater. LCROSS (Lunar Crater Observation and Sensing Satellite) should be launched in June 2009 with Lunar Reconnaissance Orbiter (LRO) payload aboard an Atlas V rocket from Cape Canaveral Air Force Station in Florida. LCROSS will seek a definitive answer about the presence of water ice at the lunar south pole using the spent second stage Atlas Centaur rocket that will impact on the moon's surface
LCROSS Probe - Artist View - LCROSS - Artist view - LCROSS (Lunar Crater Observation and Sensing Satellite) is a space probe of NASA whose aim is to discover the presence of water ice in a crater perpetually in the shade of the Sun at the southern pole of the Moon. LCROSS must analyze the impact created by the top floor of its Atlas 5 launcher precipitates in this crater. LCROSS (Lunar Crater Observation and Sensing Satellite) should be launched in June 2009 with Lunar Reconnaissance Orbiter (LRO) payload aboard an Atlas V rocket from Cape Canaveral Air Force Station in Florida. LCROSS will seek a definitive answer about the presence of water ice at the lunar south pole using the spent second stage Atlas Centaur rocket that will impact on the moon's surface

PIX4606162: LCROSS Probe - Artist View - LCROSS - Artist view - LCROSS (Lunar Crater Observation and Sensing Satellite) is a space probe of NASA whose aim is to discover the presence of water ice in a crater perpetually in the shade of the Sun at the southern pole of the Moon. LCROSS must analyze the impact created by the top floor of its Atlas 5 launcher precipitates in this crater. LCROSS (Lunar Crater Observation and Sensing Satellite) should be launched in June 2009 with Lunar Reconnaissance Orbiter (LRO) payload aboard an Atlas V rocket from Cape Canaveral Air Force Station in Florida. LCROSS will seek a definitive answer about the presence of water ice at the lunar south pole using the spent second stage Atlas Centaur rocket that will impact on the moon's surface / Bridgeman Images

ID: PIX4606162

LCROSS Probe - Artist View - LCROSS - Artist view - LCROSS (Lunar Crater Observation and Sensing Satellite) is a space probe of NASA whose aim is to discover the presence of water ice in a crater perpetually in the shade of the Sun at the southern pole of the Moon. LCROSS must analyze the impact created by the top floor of its Atlas 5 launcher precipitates in this crater. LCROSS (Lunar Crater Observation and Sensing Satellite) should be launched in June 2009 with Lunar Reconnaissance Orbiter (LRO) payload aboard an Atlas V rocket from Cape Canaveral Air Force Station in Florida. LCROSS will seek a definitive answer about the presence of water ice at the lunar south pole using the spent second stage Atlas Centaur rocket that will impact on the moon's surface

Meridienne de l'église Saint Eustache (Paris 1er) - Noon Mark on Church Saint Eustache (Paris 1er) - Located on the meridional facade of the church, under the sundial of the eardrum, this Meridian no longer works due to the disappearance of the disc that served as her style
Meridienne de l'église Saint Eustache (Paris 1er) - Noon Mark on Church Saint Eustache (Paris 1er) - Located on the meridional facade of the church, under the sundial of the eardrum, this Meridian no longer works due to the disappearance of the disc that served as her style

PIX4585098: Meridienne de l'église Saint Eustache (Paris 1er) - Noon Mark on Church Saint Eustache (Paris 1er) - Located on the meridional facade of the church, under the sundial of the eardrum, this Meridian no longer works due to the disappearance of the disc that served as her style / Bridgeman Images

ID: PIX4585098

Meridienne de l'église Saint Eustache (Paris 1er) - Noon Mark on Church Saint Eustache (Paris 1er) - Located on the meridional facade of the church, under the sundial of the eardrum, this Meridian no longer works due to the disappearance of the disc that served as her style

Venus Express Probe - Artist's View - Venus Express spacecraft - Artwork - The European Venus Express probe was launched on 9 November 2005 and has been placed in orbit around Venus since 11 April 2006. The european spacecraft Venus Express has been launched from Baikonur in november 2005 and orbits the planet Venus since april 11 2006
Venus Express Probe - Artist's View - Venus Express spacecraft - Artwork - The European Venus Express probe was launched on 9 November 2005 and has been placed in orbit around Venus since 11 April 2006. The european spacecraft Venus Express has been launched from Baikonur in november 2005 and orbits the planet Venus since april 11 2006

PIX4606234: Venus Express Probe - Artist's View - Venus Express spacecraft - Artwork - The European Venus Express probe was launched on 9 November 2005 and has been placed in orbit around Venus since 11 April 2006. The european spacecraft Venus Express has been launched from Baikonur in november 2005 and orbits the planet Venus since april 11 2006 / Bridgeman Images

ID: PIX4606234

Venus Express Probe - Artist's View - Venus Express spacecraft - Artwork - The European Venus Express probe was launched on 9 November 2005 and has been placed in orbit around Venus since 11 April 2006. The european spacecraft Venus Express has been launched from Baikonur in november 2005 and orbits the planet Venus since april 11 2006

Le Ritz, 15 place Vendome, Paris. Built in 1705 for Jean Baillet de la Cour, the mansion was transformed into a palace by Charles Mewes for Cesar Ritz in 1896.
Le Ritz, 15 place Vendome, Paris. Built in 1705 for Jean Baillet de la Cour, the mansion was transformed into a palace by Charles Mewes for Cesar Ritz in 1896.

OMG4606477: Le Ritz, 15 place Vendome, Paris. Built in 1705 for Jean Baillet de la Cour, the mansion was transformed into a palace by Charles Mewes for Cesar Ritz in 1896. / Bridgeman Images

ID: OMG4606477

Le Ritz, 15 place Vendome, Paris. Built in 1705 for Jean Baillet de la Cour, the mansion was transformed into a palace by Charles Mewes for Cesar Ritz in 1896.

Mars Global Surveyor - The probe was launched on November 7, 1996 and put into orbit around March in September 1997. Predicted to observe Mars for two years, it was not until November 2006 that the probe stopped working
Mars Global Surveyor - The probe was launched on November 7, 1996 and put into orbit around March in September 1997. Predicted to observe Mars for two years, it was not until November 2006 that the probe stopped working

PIX4606491: Mars Global Surveyor - The probe was launched on November 7, 1996 and put into orbit around March in September 1997. Predicted to observe Mars for two years, it was not until November 2006 that the probe stopped working / Bridgeman Images

ID: PIX4606491

Mars Global Surveyor - The probe was launched on November 7, 1996 and put into orbit around March in September 1997. Predicted to observe Mars for two years, it was not until November 2006 that the probe stopped working

Mars Pathfinder Probe - View of the Mars Pathfinder probe and its small Sojourner rover at the Kennedy space center in October 1996. The probe was launched on 4 December 1996 and landed on March 4 July 1997 in Ares Vallis. Teleguide from Earth, the Sojourner rover was the first robot to survey Martian soil. He explored about 250 m2 of the surface of Mars and returned 550 photographs. Contact was definitively lost with the Mars Pathfinder probe on 27 September 1997
Mars Pathfinder Probe - View of the Mars Pathfinder probe and its small Sojourner rover at the Kennedy space center in October 1996. The probe was launched on 4 December 1996 and landed on March 4 July 1997 in Ares Vallis. Teleguide from Earth, the Sojourner rover was the first robot to survey Martian soil. He explored about 250 m2 of the surface of Mars and returned 550 photographs. Contact was definitively lost with the Mars Pathfinder probe on 27 September 1997

PIX4606522: Mars Pathfinder Probe - View of the Mars Pathfinder probe and its small Sojourner rover at the Kennedy space center in October 1996. The probe was launched on 4 December 1996 and landed on March 4 July 1997 in Ares Vallis. Teleguide from Earth, the Sojourner rover was the first robot to survey Martian soil. He explored about 250 m2 of the surface of Mars and returned 550 photographs. Contact was definitively lost with the Mars Pathfinder probe on 27 September 1997 / Bridgeman Images

ID: PIX4606522

Mars Pathfinder Probe - View of the Mars Pathfinder probe and its small Sojourner rover at the Kennedy space center in October 1996. The probe was launched on 4 December 1996 and landed on March 4 July 1997 in Ares Vallis. Teleguide from Earth, the Sojourner rover was the first robot to survey Martian soil. He explored about 250 m2 of the surface of Mars and returned 550 photographs. Contact was definitively lost with the Mars Pathfinder probe on 27 September 1997

Terrace planted in Salzburg (Austria).
Terrace planted in Salzburg (Austria).

TEC4606701: Terrace planted in Salzburg (Austria). / Bridgeman Images

ID: TEC4606701

Terrace planted in Salzburg (Austria).

Galaxy NGC 891 in Andromede - Edge - on spiral galaxy NGC 891 in Andromeda - Spiral galaxy seen by the slice located at a distance of 10 million years - light. Composite image (Subaru, HST and a 90 cm telescope). Located about 10 million light years from Earth, NGC 891 is one of the most photographed edge - on spiral galaxies in the northern skies. Composite Image made from Three Data Sources: 8.2 Meter Subaru Telescope (NAOJ), Hubble Space Telescope, West Mountain Observatory, BYU
Galaxy NGC 891 in Andromede - Edge - on spiral galaxy NGC 891 in Andromeda - Spiral galaxy seen by the slice located at a distance of 10 million years - light. Composite image (Subaru, HST and a 90 cm telescope). Located about 10 million light years from Earth, NGC 891 is one of the most photographed edge - on spiral galaxies in the northern skies. Composite Image made from Three Data Sources: 8.2 Meter Subaru Telescope (NAOJ), Hubble Space Telescope, West Mountain Observatory, BYU

PIX4609518: Galaxy NGC 891 in Andromede - Edge - on spiral galaxy NGC 891 in Andromeda - Spiral galaxy seen by the slice located at a distance of 10 million years - light. Composite image (Subaru, HST and a 90 cm telescope). Located about 10 million light years from Earth, NGC 891 is one of the most photographed edge - on spiral galaxies in the northern skies. Composite Image made from Three Data Sources: 8.2 Meter Subaru Telescope (NAOJ), Hubble Space Telescope, West Mountain Observatory, BYU / Bridgeman Images

ID: PIX4609518

Galaxy NGC 891 in Andromede - Edge - on spiral galaxy NGC 891 in Andromeda - Spiral galaxy seen by the slice located at a distance of 10 million years - light. Composite image (Subaru, HST and a 90 cm telescope). Located about 10 million light years from Earth, NGC 891 is one of the most photographed edge - on spiral galaxies in the northern skies. Composite Image made from Three Data Sources: 8.2 Meter Subaru Telescope (NAOJ), Hubble Space Telescope, West Mountain Observatory, BYU

Development in San Diego (United States).
Development in San Diego (United States).

TEC4609711: Development in San Diego (United States). / Bridgeman Images

ID: TEC4609711

Development in San Diego (United States).

Elliptical galaxy NGC 1275 in Persee - Elliptical galaxy NGC 1275 in Perseus - View of the giant elliptical galaxy NGC 1275 located 230 million years ago - light in the center of the cluster of Persee galaxies. This image obtained by the Hubble Space Telescope in 2006 reveals filamentary structures surrounding the galaxy. These gas filaments would come from the interaction between the cold gas of the center of the galaxy or resides a supermassive black hole and the warmer gas present in the galaxy cluster. This Hubble Space Telescope image of galaxy NGC 1275 reveals the fine, thread - like filamentary structures in the gas surrounding the galaxy. The red filaments are composed of cool gas being suspended by a magnetic field, and are surrounded by the 100 - million - degree Fahrenheit hot gas in the center of the Perseus galaxy cluster. The filaments are dramatic markers of the feedback process through which energy is transferred from the central massive black hole to the surrounding gas. The filaments originate when cool gas is transported from the center of the galaxy by radio bubbles that rise in the hot interstellar gas. At a distance of 230 million light - years, NGC 1275 is one of the closest giant elliptical galaxies and lies at the center of the Perseus cluster of galaxies. The galaxy was photographed in July and August 2006 with the Advanced Camera for Surveys in three color filters
Elliptical galaxy NGC 1275 in Persee - Elliptical galaxy NGC 1275 in Perseus - View of the giant elliptical galaxy NGC 1275 located 230 million years ago - light in the center of the cluster of Persee galaxies. This image obtained by the Hubble Space Telescope in 2006 reveals filamentary structures surrounding the galaxy. These gas filaments would come from the interaction between the cold gas of the center of the galaxy or resides a supermassive black hole and the warmer gas present in the galaxy cluster. This Hubble Space Telescope image of galaxy NGC 1275 reveals the fine, thread - like filamentary structures in the gas surrounding the galaxy. The red filaments are composed of cool gas being suspended by a magnetic field, and are surrounded by the 100 - million - degree Fahrenheit hot gas in the center of the Perseus galaxy cluster. The filaments are dramatic markers of the feedback process through which energy is transferred from the central massive black hole to the surrounding gas. The filaments originate when cool gas is transported from the center of the galaxy by radio bubbles that rise in the hot interstellar gas. At a distance of 230 million light - years, NGC 1275 is one of the closest giant elliptical galaxies and lies at the center of the Perseus cluster of galaxies. The galaxy was photographed in July and August 2006 with the Advanced Camera for Surveys in three color filters

PIX4609732: Elliptical galaxy NGC 1275 in Persee - Elliptical galaxy NGC 1275 in Perseus - View of the giant elliptical galaxy NGC 1275 located 230 million years ago - light in the center of the cluster of Persee galaxies. This image obtained by the Hubble Space Telescope in 2006 reveals filamentary structures surrounding the galaxy. These gas filaments would come from the interaction between the cold gas of the center of the galaxy or resides a supermassive black hole and the warmer gas present in the galaxy cluster. This Hubble Space Telescope image of galaxy NGC 1275 reveals the fine, thread - like filamentary structures in the gas surrounding the galaxy. The red filaments are composed of cool gas being suspended by a magnetic field, and are surrounded by the 100 - million - degree Fahrenheit hot gas in the center of the Perseus galaxy cluster. The filaments are dramatic markers of the feedback process through which energy is transferred from the central massive black hole to the surrounding gas. The filaments originate when cool gas is transported from the center of the galaxy by radio bubbles that rise in the hot interstellar gas. At a distance of 230 million light - years, NGC 1275 is one of the closest giant elliptical galaxies and lies at the center of the Perseus cluster of galaxies. The galaxy was photographed in July and August 2006 with the Advanced Camera for Surveys in three color filters / Bridgeman Images

ID: PIX4609732

Elliptical galaxy NGC 1275 in Persee - Elliptical galaxy NGC 1275 in Perseus - View of the giant elliptical galaxy NGC 1275 located 230 million years ago - light in the center of the cluster of Persee galaxies. This image obtained by the Hubble Space Telescope in 2006 reveals filamentary structures surrounding the galaxy. These gas filaments would come from the interaction between the cold gas of the center of the galaxy or resides a supermassive black hole and the warmer gas present in the galaxy cluster. This Hubble Space Telescope image of galaxy NGC 1275 reveals the fine, thread - like filamentary structures in the gas surrounding the galaxy. The red filaments are composed of cool gas being suspended by a magnetic field, and are surrounded by the 100 - million - degree Fahrenheit hot gas in the center of the Perseus galaxy cluster. The filaments are dramatic markers of the feedback process through which energy is transferred from the central massive black hole to the surrounding ga


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