1. Home
  2. Search Results

Search options

Orientation
Colour

Display options

View

Print

To print search results, use print friendly version of this page.

2497570 Search Results

Nebula NGC 6914 in the Swan - A vast region of 200-year-old star formation - light situated about 5000 years ago - light from Earth. Image obtained by Isaac Newton 2.5m telescope from La Palma
Nebula NGC 6914 in the Swan - A vast region of 200-year-old star formation - light situated about 5000 years ago - light from Earth. Image obtained by Isaac Newton 2.5m telescope from La Palma

PIX4620405: Nebula NGC 6914 in the Swan - A vast region of 200-year-old star formation - light situated about 5000 years ago - light from Earth. Image obtained by Isaac Newton 2.5m telescope from La Palma / Bridgeman Images

ID: PIX4620405

Nebula NGC 6914 in the Swan - A vast region of 200-year-old star formation - light situated about 5000 years ago - light from Earth. Image obtained by Isaac Newton 2.5m telescope from La Palma

Nebula NGC 7000 North America and Pelican in the swan - NGC7000 - The North American Nebula Complex Lens: Nikon 300 mm ED f/Stop: 2.8 Exposure: 25 minutes Film: Hypered Fujichrome 50 RFP Exposure start: 3:22 am Date: June 4, 1989 Location: Cloudcroft, NM, US
Nebula NGC 7000 North America and Pelican in the swan - NGC7000 - The North American Nebula Complex Lens: Nikon 300 mm ED f/Stop: 2.8 Exposure: 25 minutes Film: Hypered Fujichrome 50 RFP Exposure start: 3:22 am Date: June 4, 1989 Location: Cloudcroft, NM, US

PIX4620410: Nebula NGC 7000 North America and Pelican in the swan - NGC7000 - The North American Nebula Complex Lens: Nikon 300 mm ED f/Stop: 2.8 Exposure: 25 minutes Film: Hypered Fujichrome 50 RFP Exposure start: 3:22 am Date: June 4, 1989 Location: Cloudcroft, NM, US / Bridgeman Images

ID: PIX4620410

Nebula NGC 7000 North America and Pelican in the swan - NGC7000 - The North American Nebula Complex Lens: Nikon 300 mm ED f/Stop: 2.8 Exposure: 25 minutes Film: Hypered Fujichrome 50 RFP Exposure start: 3:22 am Date: June 4, 1989 Location: Cloudcroft, NM, US

Brandenburg Gate, Mitte district in Berlin (Germany). 1788- 1791, architect Carl Gotthard Langhans.Photography 10/06/95.
Brandenburg Gate, Mitte district in Berlin (Germany). 1788- 1791, architect Carl Gotthard Langhans.Photography 10/06/95.

TEC4620488: Brandenburg Gate, Mitte district in Berlin (Germany). 1788- 1791, architect Carl Gotthard Langhans.Photography 10/06/95. / Bridgeman Images

ID: TEC4620488

Brandenburg Gate, Mitte district in Berlin (Germany). 1788- 1791, architect Carl Gotthard Langhans.Photography 10/06/95.

Nebula NGC 7129 in Cephee - Reflection nebula NGC 7129 in Cepheus - Nebula by reflexion located 3300 years - light of the Earth. This nebula houses very young stars, aged less than a million years old. NGC 7129 is a star forming region located in Cepheus constellation, 3300 light years from us. Several Herbig Haro objects are visible in this nebula. Herbig - Haro objects are small emission nebulae found around young developing stars (protostars) and which are believed to be transient in their nature, for they only exist for a few thousand years
Nebula NGC 7129 in Cephee - Reflection nebula NGC 7129 in Cepheus - Nebula by reflexion located 3300 years - light of the Earth. This nebula houses very young stars, aged less than a million years old. NGC 7129 is a star forming region located in Cepheus constellation, 3300 light years from us. Several Herbig Haro objects are visible in this nebula. Herbig - Haro objects are small emission nebulae found around young developing stars (protostars) and which are believed to be transient in their nature, for they only exist for a few thousand years

PIX4620579: Nebula NGC 7129 in Cephee - Reflection nebula NGC 7129 in Cepheus - Nebula by reflexion located 3300 years - light of the Earth. This nebula houses very young stars, aged less than a million years old. NGC 7129 is a star forming region located in Cepheus constellation, 3300 light years from us. Several Herbig Haro objects are visible in this nebula. Herbig - Haro objects are small emission nebulae found around young developing stars (protostars) and which are believed to be transient in their nature, for they only exist for a few thousand years / Bridgeman Images

ID: PIX4620579

Nebula NGC 7129 in Cephee - Reflection nebula NGC 7129 in Cepheus - Nebula by reflexion located 3300 years - light of the Earth. This nebula houses very young stars, aged less than a million years old. NGC 7129 is a star forming region located in Cepheus constellation, 3300 light years from us. Several Herbig Haro objects are visible in this nebula. Herbig - Haro objects are small emission nebulae found around young developing stars (protostars) and which are believed to be transient in their nature, for they only exist for a few thousand years

Nebula NGC 7635 and M52 clusters in Cassiopee - Nebula NGC 7635 and M52 clusters in Cassiopee - Nebula NGC 7635 is located about 7800 years - light from Earth. A massive star, called Wolf - Rayet, is responsible for the formation of this bubble; it is the star BD+60* 2522, 40 times more massive than our Sun. M52, top left, is an open cluster containing about 200 stars
Nebula NGC 7635 and M52 clusters in Cassiopee - Nebula NGC 7635 and M52 clusters in Cassiopee - Nebula NGC 7635 is located about 7800 years - light from Earth. A massive star, called Wolf - Rayet, is responsible for the formation of this bubble; it is the star BD+60* 2522, 40 times more massive than our Sun. M52, top left, is an open cluster containing about 200 stars

PIX4620626: Nebula NGC 7635 and M52 clusters in Cassiopee - Nebula NGC 7635 and M52 clusters in Cassiopee - Nebula NGC 7635 is located about 7800 years - light from Earth. A massive star, called Wolf - Rayet, is responsible for the formation of this bubble; it is the star BD+60* 2522, 40 times more massive than our Sun. M52, top left, is an open cluster containing about 200 stars / Bridgeman Images

ID: PIX4620626

Nebula NGC 7635 and M52 clusters in Cassiopee - Nebula NGC 7635 and M52 clusters in Cassiopee - Nebula NGC 7635 is located about 7800 years - light from Earth. A massive star, called Wolf - Rayet, is responsible for the formation of this bubble; it is the star BD+60* 2522, 40 times more massive than our Sun. M52, top left, is an open cluster containing about 200 stars

Artist squat (Kunsthaus), Tacheles district in Berlinae (Germany).
Artist squat (Kunsthaus), Tacheles district in Berlinae (Germany).

LBY4620662: Artist squat (Kunsthaus), Tacheles district in Berlinae (Germany). / Bridgeman Images

ID: LBY4620662

Artist squat (Kunsthaus), Tacheles district in Berlinae (Germany).

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

PIX4620681: Nebula NGC 7635 in Cassiopee - Bubble Nebula (NGC 7635) in Cassiopeia - This nebula is located about 7100 years - light from Earth. A massive star, called Wolf - Rayet, is responsible for the formation of this bubble; it is the star BD+60* 2522. The Bubble Nebula in Cassiopeia is one of the most dramatic emission nebulae visible in the northern hemisphere. Lying at a distance of about 7,000 light - years away and spanning six light - years in diameter, NGC 7635 is quite bright with a magnitude of 7.0. The star in the middle of the bubble, BD+602522, is responsible for this stunning site, for this very hot star emits so much UV radiation that it is able to also heat and excite the surrounding dust and gas, thus emitting its own radiation. It is a Wolf - Rayet star, a very luminous star and also very short - lived. This Wolf - Rayet star is 40 times as massive than our sun / Bridgeman Images

ID: PIX4620681

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

Brandenburg Gate in Berlin, Germany. Architecteae Carl Gotthard Langhans, 1788-1791. Photography 15/10/99.
Brandenburg Gate in Berlin, Germany. Architecteae Carl Gotthard Langhans, 1788-1791. Photography 15/10/99.

LBY4620721: Brandenburg Gate in Berlin, Germany. Architecteae Carl Gotthard Langhans, 1788-1791. Photography 15/10/99. / Bridgeman Images

ID: LBY4620721

Brandenburg Gate in Berlin, Germany. Architecteae Carl Gotthard Langhans, 1788-1791. Photography 15/10/99.

Nebuleuse Ced 214 in Cephe
Nebuleuse Ced 214 in Cephe

PIX4620727: Nebuleuse Ced 214 in Cephe / Bridgeman Images

ID: PIX4620727

Nebuleuse Ced 214 in Cephe

Nebulae Ced 214 and NGC 7822 in Cephee - Nebulae Ced 214 and NGC 7822 in Cephee - Cederblad 214 and NGC 7822 are vast star-forming regions located about 2750 years away - light from Earth
Nebulae Ced 214 and NGC 7822 in Cephee - Nebulae Ced 214 and NGC 7822 in Cephee - Cederblad 214 and NGC 7822 are vast star-forming regions located about 2750 years away - light from Earth

PIX4620732: Nebulae Ced 214 and NGC 7822 in Cephee - Nebulae Ced 214 and NGC 7822 in Cephee - Cederblad 214 and NGC 7822 are vast star-forming regions located about 2750 years away - light from Earth / Bridgeman Images

ID: PIX4620732

Nebulae Ced 214 and NGC 7822 in Cephee - Nebulae Ced 214 and NGC 7822 in Cephee - Cederblad 214 and NGC 7822 are vast star-forming regions located about 2750 years away - light from Earth

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

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

ID: PIX4625788

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

Astronauts on Titan - Illustration - First steps on Titan - Astronauts explore Titan's surface. Perhaps some day in the far future humans will set foot on Saturn's mysterious moon Titan, one of the most interesting worlds in the Solar System. Larger than the planet Mercury, Earth's moon, and the dwarf planet Pluto, and second only in size to Jupiter's satellite Ganymede, Titan is the only known extraterrestrial world with a dense atmosphere that realistically could be visited by humans. A visit to Titan would require a space journey of a year or more and traverse over 700 million miles. Beneath Titan's 350 miles of atmosphere, intrepid explorers would likely find a dark, forbidding landscape of rock, ice, and possibly tarry layers of hydrocarbons and lakes of liquid ethane and/or methane (AKA natural gas). The Surface temperature would be around minus 300* F, cold enough to freeze exposed human tissue within seconds. There would be no oxygen to breathe, and any water to be found would be as hard and dense as granite. Despite these harsh conditions, Titan could yet yield secrets regarding the origin of life itself as it is believed that, with the exception of the extreme cold, Titan resemble the primordial Earth at the time living organisms first appeared. In this image, Titan's first human visitors are protected by thick suits and helmets to shield them from the extreme cold - - and possibly toxic compounds such as hydrogen cyanide. They carry their own oxygen as Titan's atmosphere is primarily nitrogen with lesser amounts of argon, methane and other gases. Each explorer also carries “” head”” lights attached to their helmets to help them navigate a terrain that receives only 1/1000th the Sun's illumination on the Earth; while this means that noon on Titan would appear relatively dim, it would yet be over 300 times brighter than the Earth under a full moon
Astronauts on Titan - Illustration - First steps on Titan - Astronauts explore Titan's surface. Perhaps some day in the far future humans will set foot on Saturn's mysterious moon Titan, one of the most interesting worlds in the Solar System. Larger than the planet Mercury, Earth's moon, and the dwarf planet Pluto, and second only in size to Jupiter's satellite Ganymede, Titan is the only known extraterrestrial world with a dense atmosphere that realistically could be visited by humans. A visit to Titan would require a space journey of a year or more and traverse over 700 million miles. Beneath Titan's 350 miles of atmosphere, intrepid explorers would likely find a dark, forbidding landscape of rock, ice, and possibly tarry layers of hydrocarbons and lakes of liquid ethane and/or methane (AKA natural gas). The Surface temperature would be around minus 300* F, cold enough to freeze exposed human tissue within seconds. There would be no oxygen to breathe, and any water to be found would be as hard and dense as granite. Despite these harsh conditions, Titan could yet yield secrets regarding the origin of life itself as it is believed that, with the exception of the extreme cold, Titan resemble the primordial Earth at the time living organisms first appeared. In this image, Titan's first human visitors are protected by thick suits and helmets to shield them from the extreme cold - - and possibly toxic compounds such as hydrogen cyanide. They carry their own oxygen as Titan's atmosphere is primarily nitrogen with lesser amounts of argon, methane and other gases. Each explorer also carries “” head”” lights attached to their helmets to help them navigate a terrain that receives only 1/1000th the Sun's illumination on the Earth; while this means that noon on Titan would appear relatively dim, it would yet be over 300 times brighter than the Earth under a full moon

PIX4626158: Astronauts on Titan - Illustration - First steps on Titan - Astronauts explore Titan's surface. Perhaps some day in the far future humans will set foot on Saturn's mysterious moon Titan, one of the most interesting worlds in the Solar System. Larger than the planet Mercury, Earth's moon, and the dwarf planet Pluto, and second only in size to Jupiter's satellite Ganymede, Titan is the only known extraterrestrial world with a dense atmosphere that realistically could be visited by humans. A visit to Titan would require a space journey of a year or more and traverse over 700 million miles. Beneath Titan's 350 miles of atmosphere, intrepid explorers would likely find a dark, forbidding landscape of rock, ice, and possibly tarry layers of hydrocarbons and lakes of liquid ethane and/or methane (AKA natural gas). The Surface temperature would be around minus 300* F, cold enough to freeze exposed human tissue within seconds. There would be no oxygen to breathe, and any water to be found would be as hard and dense as granite. Despite these harsh conditions, Titan could yet yield secrets regarding the origin of life itself as it is believed that, with the exception of the extreme cold, Titan resemble the primordial Earth at the time living organisms first appeared. In this image, Titan's first human visitors are protected by thick suits and helmets to shield them from the extreme cold - - and possibly toxic compounds such as hydrogen cyanide. They carry their own oxygen as Titan's atmosphere is primarily nitrogen with lesser amounts of argon, methane and other gases. Each explorer also carries “” head”” lights attached to their helmets to help them navigate a terrain that receives only 1/1000th the Sun's illumination on the Earth; while this means that noon on Titan would appear relatively dim, it would yet be over 300 times brighter than the Earth under a full moon / Bridgeman Images

ID: PIX4626158

Astronauts on Titan - Illustration - First steps on Titan - Astronauts explore Titan's surface. Perhaps some day in the far future humans will set foot on Saturn's mysterious moon Titan, one of the most interesting worlds in the Solar System. Larger than the planet Mercury, Earth's moon, and the dwarf planet Pluto, and second only in size to Jupiter's satellite Ganymede, Titan is the only known extraterrestrial world with a dense atmosphere that realistically could be visited by humans. A visit to Titan would require a space journey of a year or more and traverse over 700 million miles. Beneath Titan's 350 miles of atmosphere, intrepid explorers would likely find a dark, forbidding landscape of rock, ice, and possibly tarry layers of hydrocarbons and lakes of liquid ethane and/or methane (AKA natural gas). The Surface temperature would be around minus 300* F, cold enough to freeze exposed human tissue within seconds. There would be no oxygen to breathe, and any water to be found would

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

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

ID: PIX4626499

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

A plane passes by the Sun - A plane in front of the Sun - A plane passes by the solar disk. Image obtained by an astronomical bezel ed 102/1320 and an eos 60d cannon. A plane is silhouetted in front of the Sun
A plane passes by the Sun - A plane in front of the Sun - A plane passes by the solar disk. Image obtained by an astronomical bezel ed 102/1320 and an eos 60d cannon. A plane is silhouetted in front of the Sun

PIX4626743: A plane passes by the Sun - A plane in front of the Sun - A plane passes by the solar disk. Image obtained by an astronomical bezel ed 102/1320 and an eos 60d cannon. A plane is silhouetted in front of the Sun / Bridgeman Images

ID: PIX4626743

A plane passes by the Sun - A plane in front of the Sun - A plane passes by the solar disk. Image obtained by an astronomical bezel ed 102/1320 and an eos 60d cannon. A plane is silhouetted in front of the Sun

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

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

ID: PIX4626906

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

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

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

ID: PIX4626948

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

The Sun seen in ultraviolet by SOHO 01 - 07 - 2002 - A protuberance, a plasma cloud, escapes from the Sun. White regions are the hottest and most active areas
The Sun seen in ultraviolet by SOHO 01 - 07 - 2002 - A protuberance, a plasma cloud, escapes from the Sun. White regions are the hottest and most active areas

PIX4626965: The Sun seen in ultraviolet by SOHO 01 - 07 - 2002 - A protuberance, a plasma cloud, escapes from the Sun. White regions are the hottest and most active areas / Bridgeman Images

ID: PIX4626965

The Sun seen in ultraviolet by SOHO 01 - 07 - 2002 - A protuberance, a plasma cloud, escapes from the Sun. White regions are the hottest and most active areas

The Moon passes in front of the Sun - 25 - 02 - 2007 - Transit of the Moon in front of the Sun observed by STEREO - B satellite on 25 February 2007. The Sun is seen in different wavelengths of the ultraviolet
The Moon passes in front of the Sun - 25 - 02 - 2007 - Transit of the Moon in front of the Sun observed by STEREO - B satellite on 25 February 2007. The Sun is seen in different wavelengths of the ultraviolet

PIX4627109: The Moon passes in front of the Sun - 25 - 02 - 2007 - Transit of the Moon in front of the Sun observed by STEREO - B satellite on 25 February 2007. The Sun is seen in different wavelengths of the ultraviolet / Bridgeman Images

ID: PIX4627109

The Moon passes in front of the Sun - 25 - 02 - 2007 - Transit of the Moon in front of the Sun observed by STEREO - B satellite on 25 February 2007. The Sun is seen in different wavelengths of the ultraviolet

Keizersgracht in Amsterdam (Netherlands). Photographed 05/04/07.
Keizersgracht in Amsterdam (Netherlands). Photographed 05/04/07.

OMG4627167: Keizersgracht in Amsterdam (Netherlands). Photographed 05/04/07. / Bridgeman Images

ID: OMG4627167

Keizersgracht in Amsterdam (Netherlands). Photographed 05/04/07.

Westelijke eilanden a Priseneiland, Amsterdam (Netherlands).
Westelijke eilanden a Priseneiland, Amsterdam (Netherlands).

OMG4627184: Westelijke eilanden a Priseneiland, Amsterdam (Netherlands). / Bridgeman Images

ID: OMG4627184

Westelijke eilanden a Priseneiland, Amsterdam (Netherlands).

Tramway in Amsterdam (Netherlands).
Tramway in Amsterdam (Netherlands).

OMG4627236: Tramway in Amsterdam (Netherlands). / Bridgeman Images

ID: OMG4627236

Tramway in Amsterdam (Netherlands).

Amsterdam Central Station (Netherlands). Construction 1889, architects Cuypers and Van Gendt. Photography 05/04/07.
Amsterdam Central Station (Netherlands). Construction 1889, architects Cuypers and Van Gendt. Photography 05/04/07.

OMG4627283: Amsterdam Central Station (Netherlands). Construction 1889, architects Cuypers and Van Gendt. Photography 05/04/07. / Bridgeman Images

ID: OMG4627283

Amsterdam Central Station (Netherlands). Construction 1889, architects Cuypers and Van Gendt. Photography 05/04/07.

Total Eclipse of Sun 11 - 07 - 1991 - Total Eclipse of Sun 11 - 07 - 199
Total Eclipse of Sun 11 - 07 - 1991 - Total Eclipse of Sun 11 - 07 - 199

PIX4627341: Total Eclipse of Sun 11 - 07 - 1991 - Total Eclipse of Sun 11 - 07 - 199 / Bridgeman Images

ID: PIX4627341

Total Eclipse of Sun 11 - 07 - 1991 - Total Eclipse of Sun 11 - 07 - 199

Total Eclipse of Sun 11 - 07 - 1991 - Detail on solar protuberances
Total Eclipse of Sun 11 - 07 - 1991 - Detail on solar protuberances

PIX4627350: Total Eclipse of Sun 11 - 07 - 1991 - Detail on solar protuberances / Bridgeman Images

ID: PIX4627350

Total Eclipse of Sun 11 - 07 - 1991 - Detail on solar protuberances

Total Eclipse of Sun - Zambia 21/06/2001 - The beginning of totalite, grains of Lease
Total Eclipse of Sun - Zambia 21/06/2001 - The beginning of totalite, grains of Lease

PIX4627687: Total Eclipse of Sun - Zambia 21/06/2001 - The beginning of totalite, grains of Lease / Bridgeman Images

ID: PIX4627687

Total Eclipse of Sun - Zambia 21/06/2001 - The beginning of totalite, grains of Lease

Total Eclipse of Sun - Zambia 21 - 06 - 2001 - End of eclips
Total Eclipse of Sun - Zambia 21 - 06 - 2001 - End of eclips

PIX4627694: Total Eclipse of Sun - Zambia 21 - 06 - 2001 - End of eclips / Bridgeman Images

ID: PIX4627694

Total Eclipse of Sun - Zambia 21 - 06 - 2001 - End of eclips

Church of the Holy Spirit, Avenue Daumesnil in Paris. Architect Paul Tournon (1881-1964), 1935.
Church of the Holy Spirit, Avenue Daumesnil in Paris. Architect Paul Tournon (1881-1964), 1935.

TEC4627842: Church of the Holy Spirit, Avenue Daumesnil in Paris. Architect Paul Tournon (1881-1964), 1935. / Bridgeman Images

ID: TEC4627842

Church of the Holy Spirit, Avenue Daumesnil in Paris. Architect Paul Tournon (1881-1964), 1935.

Rue de Bercy in Paris.
Rue de Bercy in Paris.

TEC4627850: Rue de Bercy in Paris. / Bridgeman Images

ID: TEC4627850

Rue de Bercy in Paris.

Total solar eclipse - Turkey 29 March 2006 - Total solar eclipse - Turkey - March 29, 2006 - Total solar eclipse observed in Side, Turkey on 29 March 2006. Venus is visible at the bottom right. Total solar eclipse seen in Side, Turkey on March 29, 2006. Venus is visible at bottom right
Total solar eclipse - Turkey 29 March 2006 - Total solar eclipse - Turkey - March 29, 2006 - Total solar eclipse observed in Side, Turkey on 29 March 2006. Venus is visible at the bottom right. Total solar eclipse seen in Side, Turkey on March 29, 2006. Venus is visible at bottom right

PIX4627908: Total solar eclipse - Turkey 29 March 2006 - Total solar eclipse - Turkey - March 29, 2006 - Total solar eclipse observed in Side, Turkey on 29 March 2006. Venus is visible at the bottom right. Total solar eclipse seen in Side, Turkey on March 29, 2006. Venus is visible at bottom right / Bridgeman Images

ID: PIX4627908

Total solar eclipse - Turkey 29 March 2006 - Total solar eclipse - Turkey - March 29, 2006 - Total solar eclipse observed in Side, Turkey on 29 March 2006. Venus is visible at the bottom right. Total solar eclipse seen in Side, Turkey on March 29, 2006. Venus is visible at bottom right

Concert area of Reuilly overlooking Parc de la Coulee verte in Paris.
Concert area of Reuilly overlooking Parc de la Coulee verte in Paris.

TEC4627993: Concert area of Reuilly overlooking Parc de la Coulee verte in Paris. / Bridgeman Images

ID: TEC4627993

Concert area of Reuilly overlooking Parc de la Coulee verte in Paris.

Concert area in Paris 12th.
Concert area in Paris 12th.

TEC4628039: Concert area in Paris 12th. / Bridgeman Images

ID: TEC4628039

Concert area in Paris 12th.

Total Eclipse of Sun. 01/08/2008 - Total Solar Eclipse of 2008 august 01 - Composite of images showing the solar crown, the ash light (the Moon lit by the Earth) the stars around the Sun (with the cluster of stars M44 at the top right) and the planet Mercury (bright dot on the left). 01/08/2008, Mongolia. Data from two different cameras were used for this image creation. The open cluster M 44 Praesepae (NGC 2632) dominates the star field. The bright object in the left part of the image is Mercury. The solar corona is traceable up to the distance of 20 solar radii. The position of the Moon represents the situation 62 seconds after the second contact (18:04:37 mongolia local time). Display of the solar corona, lunar surface and stars in the resulting image are highly beyond the ability of human vision during the eclipse
Total Eclipse of Sun. 01/08/2008 - Total Solar Eclipse of 2008 august 01 - Composite of images showing the solar crown, the ash light (the Moon lit by the Earth) the stars around the Sun (with the cluster of stars M44 at the top right) and the planet Mercury (bright dot on the left). 01/08/2008, Mongolia. Data from two different cameras were used for this image creation. The open cluster M 44 Praesepae (NGC 2632) dominates the star field. The bright object in the left part of the image is Mercury. The solar corona is traceable up to the distance of 20 solar radii. The position of the Moon represents the situation 62 seconds after the second contact (18:04:37 mongolia local time). Display of the solar corona, lunar surface and stars in the resulting image are highly beyond the ability of human vision during the eclipse

PIX4628063: Total Eclipse of Sun. 01/08/2008 - Total Solar Eclipse of 2008 august 01 - Composite of images showing the solar crown, the ash light (the Moon lit by the Earth) the stars around the Sun (with the cluster of stars M44 at the top right) and the planet Mercury (bright dot on the left). 01/08/2008, Mongolia. Data from two different cameras were used for this image creation. The open cluster M 44 Praesepae (NGC 2632) dominates the star field. The bright object in the left part of the image is Mercury. The solar corona is traceable up to the distance of 20 solar radii. The position of the Moon represents the situation 62 seconds after the second contact (18:04:37 mongolia local time). Display of the solar corona, lunar surface and stars in the resulting image are highly beyond the ability of human vision during the eclipse / Bridgeman Images

ID: PIX4628063

Total Eclipse of Sun. 01/08/2008 - Total Solar Eclipse of 2008 august 01 - Composite of images showing the solar crown, the ash light (the Moon lit by the Earth) the stars around the Sun (with the cluster of stars M44 at the top right) and the planet Mercury (bright dot on the left). 01/08/2008, Mongolia. Data from two different cameras were used for this image creation. The open cluster M 44 Praesepae (NGC 2632) dominates the star field. The bright object in the left part of the image is Mercury. The solar corona is traceable up to the distance of 20 solar radii. The position of the Moon represents the situation 62 seconds after the second contact (18:04:37 mongolia local time). Display of the solar corona, lunar surface and stars in the resulting image are highly beyond the ability of human vision during the eclipse

Entrepots de Bercy, Paris 12th arondissement. Louis XIV (1638-1715) built the first wine warehouses in Bercy because Paris was home to one of the largest vineyards in Europe. These warehouses reached their peak in the 19th century, becoming the world's largest centre for wine and spirits trade. The activities of the warehouses began to declinate in the 20th century with the destruction of the fortifications of Thiers, 1920-1929, the success of the railway and the evolution of storage techniques. It is now Bercy Village and Bercy Park that settled on the old warehouses. The surrounding area still resonate with the memory of old activities: rue de Pommard, rue de Chablis, rue de Macon...
Entrepots de Bercy, Paris 12th arondissement. Louis XIV (1638-1715) built the first wine warehouses in Bercy because Paris was home to one of the largest vineyards in Europe. These warehouses reached their peak in the 19th century, becoming the world's largest centre for wine and spirits trade. The activities of the warehouses began to declinate in the 20th century with the destruction of the fortifications of Thiers, 1920-1929, the success of the railway and the evolution of storage techniques. It is now Bercy Village and Bercy Park that settled on the old warehouses. The surrounding area still resonate with the memory of old activities: rue de Pommard, rue de Chablis, rue de Macon...

TEC4628196: Entrepots de Bercy, Paris 12th arondissement. Louis XIV (1638-1715) built the first wine warehouses in Bercy because Paris was home to one of the largest vineyards in Europe. These warehouses reached their peak in the 19th century, becoming the world's largest centre for wine and spirits trade. The activities of the warehouses began to declinate in the 20th century with the destruction of the fortifications of Thiers, 1920-1929, the success of the railway and the evolution of storage techniques. It is now Bercy Village and Bercy Park that settled on the old warehouses. The surrounding area still resonate with the memory of old activities: rue de Pommard, rue de Chablis, rue de Macon... / Bridgeman Images

ID: TEC4628196

Entrepots de Bercy, Paris 12th arondissement. Louis XIV (1638-1715) built the first wine warehouses in Bercy because Paris was home to one of the largest vineyards in Europe. These warehouses reached their peak in the 19th century, becoming the world's largest centre for wine and spirits trade. The activities of the warehouses began to declinate in the 20th century with the destruction of the fortifications of Thiers, 1920-1929, the success of the railway and the evolution of storage techniques. It is now Bercy Village and Bercy Park that settled on the old warehouses. The surrounding area still resonate with the memory of old activities: rue de Pommard, rue de Chablis, rue de Macon...

Total Eclipse of Sun - Easter Island 11/07/2010 - Easter Island Total Solar Eclipse - July 11 2010 - Total Eclipse of Sun from 11 July 2010 seen on Easter Island. The total solar eclipse of 11 July 2010 seen in Easter Island
Total Eclipse of Sun - Easter Island 11/07/2010 - Easter Island Total Solar Eclipse - July 11 2010 - Total Eclipse of Sun from 11 July 2010 seen on Easter Island. The total solar eclipse of 11 July 2010 seen in Easter Island

PIX4628238: Total Eclipse of Sun - Easter Island 11/07/2010 - Easter Island Total Solar Eclipse - July 11 2010 - Total Eclipse of Sun from 11 July 2010 seen on Easter Island. The total solar eclipse of 11 July 2010 seen in Easter Island / Bridgeman Images

ID: PIX4628238

Total Eclipse of Sun - Easter Island 11/07/2010 - Easter Island Total Solar Eclipse - July 11 2010 - Total Eclipse of Sun from 11 July 2010 seen on Easter Island. The total solar eclipse of 11 July 2010 seen in Easter Island

Partial Eclipse of Soleil 20/03/2015 - Partial Solar Eclipse - March 20 2015 - Partial Eclipse of Sun of 20 March 2015 seen in Italy. The partially eclipsed Sun seen in Italy. Mar 20, 201
Partial Eclipse of Soleil 20/03/2015 - Partial Solar Eclipse - March 20 2015 - Partial Eclipse of Sun of 20 March 2015 seen in Italy. The partially eclipsed Sun seen in Italy. Mar 20, 201

PIX4628372: Partial Eclipse of Soleil 20/03/2015 - Partial Solar Eclipse - March 20 2015 - Partial Eclipse of Sun of 20 March 2015 seen in Italy. The partially eclipsed Sun seen in Italy. Mar 20, 201 / Bridgeman Images

ID: PIX4628372

Partial Eclipse of Soleil 20/03/2015 - Partial Solar Eclipse - March 20 2015 - Partial Eclipse of Sun of 20 March 2015 seen in Italy. The partially eclipsed Sun seen in Italy. Mar 20, 201

The Parc Floral de Vincennes, Paris 12th arrondissement. Located on the edge of the Bois de Vincennes, this botanical garden was created in 1969 by landscape architect David Collin. Photography 2002.
The Parc Floral de Vincennes, Paris 12th arrondissement. Located on the edge of the Bois de Vincennes, this botanical garden was created in 1969 by landscape architect David Collin. Photography 2002.

LBY4628573: The Parc Floral de Vincennes, Paris 12th arrondissement. Located on the edge of the Bois de Vincennes, this botanical garden was created in 1969 by landscape architect David Collin. Photography 2002. / Bridgeman Images

ID: LBY4628573

The Parc Floral de Vincennes, Paris 12th arrondissement. Located on the edge of the Bois de Vincennes, this botanical garden was created in 1969 by landscape architect David Collin. Photography 2002.


Back to top