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North America and Pelican Nebulae in the Swan - North America and Pelican Nebulae in the Swan - The North America Nebula (NGC 7000) is a large emission nebula located near the Deneb star (the bright star to the right of the image) in the constellation of Swan. Between NGC 7000 and Deneb, the Pelican nebula, IC 5070
North America and Pelican Nebulae in the Swan - North America and Pelican Nebulae in the Swan - The North America Nebula (NGC 7000) is a large emission nebula located near the Deneb star (the bright star to the right of the image) in the constellation of Swan. Between NGC 7000 and Deneb, the Pelican nebula, IC 5070

PIX4620436: North America and Pelican Nebulae in the Swan - North America and Pelican Nebulae in the Swan - The North America Nebula (NGC 7000) is a large emission nebula located near the Deneb star (the bright star to the right of the image) in the constellation of Swan. Between NGC 7000 and Deneb, the Pelican nebula, IC 5070 / Bridgeman Images

ID: PIX4620436

North America and Pelican Nebulae in the Swan - North America and Pelican Nebulae in the Swan - The North America Nebula (NGC 7000) is a large emission nebula located near the Deneb star (the bright star to the right of the image) in the constellation of Swan. Between NGC 7000 and Deneb, the Pelican nebula, IC 5070

North America nebula in Cygnus - North America nebula in Cygnus - The North America nebula (NGC 7000) is a large emission nebula located near the star Deneb in the constellation Swan. NGC 7000 is the North America Nebula in Cygnus. Located just 3 degrees east - southeast of Deneb, the brightest star in Cygnus, this large 2 x 3 degree area of red hydrogen - alpha emission nebulosity is a complex star - forming region choked with gas and obscuring dust. It is located about 1,500 light years away
North America nebula in Cygnus - North America nebula in Cygnus - The North America nebula (NGC 7000) is a large emission nebula located near the star Deneb in the constellation Swan. NGC 7000 is the North America Nebula in Cygnus. Located just 3 degrees east - southeast of Deneb, the brightest star in Cygnus, this large 2 x 3 degree area of red hydrogen - alpha emission nebulosity is a complex star - forming region choked with gas and obscuring dust. It is located about 1,500 light years away

PIX4620499: North America nebula in Cygnus - North America nebula in Cygnus - The North America nebula (NGC 7000) is a large emission nebula located near the star Deneb in the constellation Swan. NGC 7000 is the North America Nebula in Cygnus. Located just 3 degrees east - southeast of Deneb, the brightest star in Cygnus, this large 2 x 3 degree area of red hydrogen - alpha emission nebulosity is a complex star - forming region choked with gas and obscuring dust. It is located about 1,500 light years away / Bridgeman Images

ID: PIX4620499

North America nebula in Cygnus - North America nebula in Cygnus - The North America nebula (NGC 7000) is a large emission nebula located near the star Deneb in the constellation Swan. NGC 7000 is the North America Nebula in Cygnus. Located just 3 degrees east - southeast of Deneb, the brightest star in Cygnus, this large 2 x 3 degree area of red hydrogen - alpha emission nebulosity is a complex star - forming region choked with gas and obscuring dust. It is located about 1,500 light years away

Nebuleuse NGC 7023 in Cephe
Nebuleuse NGC 7023 in Cephe

PIX4620512: Nebuleuse NGC 7023 in Cephe / Bridgeman Images

ID: PIX4620512

Nebuleuse NGC 7023 in Cephe

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

PIX4620654: Nebula NGC 7635 in Cassiopee - This nebula is located about 7800 light years from Earth. A massive star, called Wolf - Rayet, is responsible for the formation of this bubble; it is the star BD+60* 2522, 40 times more massive than our Sun. Image obtained by Isaac Newton 2.5m telescope from La Palma / Bridgeman Images

ID: PIX4620654

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

Nebula N70 in the Great Magellan Cloud - The N 70 nebula in Large Magellanic Cloud (LMC) - The Henize 70 nebula extends for about 400 years - light, it is located in the Great Magellan Cloud. In the center, a small group of very massive and extremely hot stars, stars of Wolf - Rayet. Image obtained by Siding Spring's 3.9m telescope. At the centre of this remarkable bubble - like nebula nebula is a small group of extremely hot stars. Some of these stars are rapdly losing mass and have stellar winds blowing from their surfaces with velocities that approach 4000 kilometers per second. Such stars are known as Wolf - Rayet stars and are found in galaxies capable of forming massive stars. There are many such stars in the Large Magellanic Cloud (LMC) but not all of them are associated with distinctive nebulae. The outward flowing streams of energetic particles from Wolf - Rayet (and other energetic stars) eventually interact with the relatively stationary interstellar medium pervading the LMC, releasing much of their energy as a thin spherical shell of luminous material. The hollow structure accounts for the shape we see in the sky. This nebula is almost 400 light years across, about 100 times the distance from the Sun to the nearest star. The LMC is about 160,000 light years away and is the closest galaxy to the Milky Way
Nebula N70 in the Great Magellan Cloud - The N 70 nebula in Large Magellanic Cloud (LMC) - The Henize 70 nebula extends for about 400 years - light, it is located in the Great Magellan Cloud. In the center, a small group of very massive and extremely hot stars, stars of Wolf - Rayet. Image obtained by Siding Spring's 3.9m telescope. At the centre of this remarkable bubble - like nebula nebula is a small group of extremely hot stars. Some of these stars are rapdly losing mass and have stellar winds blowing from their surfaces with velocities that approach 4000 kilometers per second. Such stars are known as Wolf - Rayet stars and are found in galaxies capable of forming massive stars. There are many such stars in the Large Magellanic Cloud (LMC) but not all of them are associated with distinctive nebulae. The outward flowing streams of energetic particles from Wolf - Rayet (and other energetic stars) eventually interact with the relatively stationary interstellar medium pervading the LMC, releasing much of their energy as a thin spherical shell of luminous material. The hollow structure accounts for the shape we see in the sky. This nebula is almost 400 light years across, about 100 times the distance from the Sun to the nearest star. The LMC is about 160,000 light years away and is the closest galaxy to the Milky Way

PIX4620865: Nebula N70 in the Great Magellan Cloud - The N 70 nebula in Large Magellanic Cloud (LMC) - The Henize 70 nebula extends for about 400 years - light, it is located in the Great Magellan Cloud. In the center, a small group of very massive and extremely hot stars, stars of Wolf - Rayet. Image obtained by Siding Spring's 3.9m telescope. At the centre of this remarkable bubble - like nebula nebula is a small group of extremely hot stars. Some of these stars are rapdly losing mass and have stellar winds blowing from their surfaces with velocities that approach 4000 kilometers per second. Such stars are known as Wolf - Rayet stars and are found in galaxies capable of forming massive stars. There are many such stars in the Large Magellanic Cloud (LMC) but not all of them are associated with distinctive nebulae. The outward flowing streams of energetic particles from Wolf - Rayet (and other energetic stars) eventually interact with the relatively stationary interstellar medium pervading the LMC, releasing much of their energy as a thin spherical shell of luminous material. The hollow structure accounts for the shape we see in the sky. This nebula is almost 400 light years across, about 100 times the distance from the Sun to the nearest star. The LMC is about 160,000 light years away and is the closest galaxy to the Milky Way / Bridgeman Images

ID: PIX4620865

Nebula N70 in the Great Magellan Cloud - The N 70 nebula in Large Magellanic Cloud (LMC) - The Henize 70 nebula extends for about 400 years - light, it is located in the Great Magellan Cloud. In the center, a small group of very massive and extremely hot stars, stars of Wolf - Rayet. Image obtained by Siding Spring's 3.9m telescope. At the centre of this remarkable bubble - like nebula nebula is a small group of extremely hot stars. Some of these stars are rapdly losing mass and have stellar winds blowing from their surfaces with velocities that approach 4000 kilometers per second. Such stars are known as Wolf - Rayet stars and are found in galaxies capable of forming massive stars. There are many such stars in the Large Magellanic Cloud (LMC) but not all of them are associated with distinctive nebulae. The outward flowing streams of energetic particles from Wolf - Rayet (and other energetic stars) eventually interact with the relatively stationary interstellar medium pervading the LMC

Galerie Victor Emmanuel II in Milan, Italy. Architect Giuseppe Mengoni (1829-1877).
Galerie Victor Emmanuel II in Milan, Italy. Architect Giuseppe Mengoni (1829-1877).

TEC4620883: Galerie Victor Emmanuel II in Milan, Italy. Architect Giuseppe Mengoni (1829-1877). / Bridgeman Images

ID: TEC4620883

Galerie Victor Emmanuel II in Milan, Italy. Architect Giuseppe Mengoni (1829-1877).

Nebuleuse Sh2 - 142 in Cephee - Nebuleuse Sh2 - 142 in Cephee - Region of star formation in Cephee and star clusters NGC 7380
Nebuleuse Sh2 - 142 in Cephee - Nebuleuse Sh2 - 142 in Cephee - Region of star formation in Cephee and star clusters NGC 7380

PIX4621043: Nebuleuse Sh2 - 142 in Cephee - Nebuleuse Sh2 - 142 in Cephee - Region of star formation in Cephee and star clusters NGC 7380 / Bridgeman Images

ID: PIX4621043

Nebuleuse Sh2 - 142 in Cephee - Nebuleuse Sh2 - 142 in Cephee - Region of star formation in Cephee and star clusters NGC 7380

Nebula NGC 3372 and cluster of stars in the Carene - The nebula of the Carene is located about 7000 years from the Earth. It houses many hot stars, including the star Eta Carinae. On its right, the cluster of stars NGC 3532
Nebula NGC 3372 and cluster of stars in the Carene - The nebula of the Carene is located about 7000 years from the Earth. It houses many hot stars, including the star Eta Carinae. On its right, the cluster of stars NGC 3532

PIX4618914: Nebula NGC 3372 and cluster of stars in the Carene - The nebula of the Carene is located about 7000 years from the Earth. It houses many hot stars, including the star Eta Carinae. On its right, the cluster of stars NGC 3532 / Bridgeman Images

ID: PIX4618914

Nebula NGC 3372 and cluster of stars in the Carene - The nebula of the Carene is located about 7000 years from the Earth. It houses many hot stars, including the star Eta Carinae. On its right, the cluster of stars NGC 3532

Wooden frame construction in the La Petite France district in Strasbourg (Alsace). Photography 20/04/89.
Wooden frame construction in the La Petite France district in Strasbourg (Alsace). Photography 20/04/89.

LBY4618970: Wooden frame construction in the La Petite France district in Strasbourg (Alsace). Photography 20/04/89. / Bridgeman Images

ID: LBY4618970

Wooden frame construction in the La Petite France district in Strasbourg (Alsace). Photography 20/04/89.

Nebula NGC 3372 in the Carene in fake colors - NGC 3372 Carina nebula in narrow band - The nebula of the Carene is located about 8000 years - light from Earth. It is home to many hot stars, including the massive star Eta Carinae in the centre of the nebula. Image obtained by the 1.2m Schmidt UK Telescope of Siding Spring through 3 different filters that highlight oxygen, hydrogen, and sulfur. Although no bright naked - eye stars are associated with the Carina nebula now, 150 years ago there blazed forth here one of the most unusual and peculiar stars ever seen. The star is known as Eta Carinae and for a few months in 1843 it was the second or third brightest star in the sky. Since then it has faded and is today about 1000 times fainter than it was at its brightest as the nebula it created during its outburst has cooled and become opaque. The whole region around Eta Carinae is rich in hot stars of which Eta is an extreme example and it is their combined radiation that produces the spectacular Carina nebula that dominates this picture. The nebula and its peculiar star are about 8000 light years away
Nebula NGC 3372 in the Carene in fake colors - NGC 3372 Carina nebula in narrow band - The nebula of the Carene is located about 8000 years - light from Earth. It is home to many hot stars, including the massive star Eta Carinae in the centre of the nebula. Image obtained by the 1.2m Schmidt UK Telescope of Siding Spring through 3 different filters that highlight oxygen, hydrogen, and sulfur. Although no bright naked - eye stars are associated with the Carina nebula now, 150 years ago there blazed forth here one of the most unusual and peculiar stars ever seen. The star is known as Eta Carinae and for a few months in 1843 it was the second or third brightest star in the sky. Since then it has faded and is today about 1000 times fainter than it was at its brightest as the nebula it created during its outburst has cooled and become opaque. The whole region around Eta Carinae is rich in hot stars of which Eta is an extreme example and it is their combined radiation that produces the spectacular Carina nebula that dominates this picture. The nebula and its peculiar star are about 8000 light years away

PIX4619010: Nebula NGC 3372 in the Carene in fake colors - NGC 3372 Carina nebula in narrow band - The nebula of the Carene is located about 8000 years - light from Earth. It is home to many hot stars, including the massive star Eta Carinae in the centre of the nebula. Image obtained by the 1.2m Schmidt UK Telescope of Siding Spring through 3 different filters that highlight oxygen, hydrogen, and sulfur. Although no bright naked - eye stars are associated with the Carina nebula now, 150 years ago there blazed forth here one of the most unusual and peculiar stars ever seen. The star is known as Eta Carinae and for a few months in 1843 it was the second or third brightest star in the sky. Since then it has faded and is today about 1000 times fainter than it was at its brightest as the nebula it created during its outburst has cooled and become opaque. The whole region around Eta Carinae is rich in hot stars of which Eta is an extreme example and it is their combined radiation that produces the spectacular Carina nebula that dominates this picture. The nebula and its peculiar star are about 8000 light years away / Bridgeman Images

ID: PIX4619010

Nebula NGC 3372 in the Carene in fake colors - NGC 3372 Carina nebula in narrow band - The nebula of the Carene is located about 8000 years - light from Earth. It is home to many hot stars, including the massive star Eta Carinae in the centre of the nebula. Image obtained by the 1.2m Schmidt UK Telescope of Siding Spring through 3 different filters that highlight oxygen, hydrogen, and sulfur. Although no bright naked - eye stars are associated with the Carina nebula now, 150 years ago there blazed forth here one of the most unusual and peculiar stars ever seen. The star is known as Eta Carinae and for a few months in 1843 it was the second or third brightest star in the sky. Since then it has faded and is today about 1000 times fainter than it was at its brightest as the nebula it created during its outburst has cooled and become opaque. The whole region around Eta Carinae is rich in hot stars of which Eta is an extreme example and it is their combined radiation that produces the spect

Birth of stars in the nebula NGC 3372 - Star formation in the Carina Nebula - Detail of the Carene nebula (NGC 3372) obtained by the Hubble space telescope. The image shows a column of gas eroded by ultraviolet radiation emitted by young stars. Jets are also visible, showing the presence of emerging stars. NGC 3372 is located about 7500 light years away from Earth. The colors used in this image correspond to the emissions of different gases: sulfur in red, hydrogen in green and oxygen in blue. The NASA Hubble Space Telescope photograph captures the chaotic activity atop a three - light - year - tall pillar of gas and dust that is being eaten away by the brilliant light from nearby bright stars. The pillar is also being assaulted from within, as infant stars buried inside it fire off jets of gas that can be seen streaming from towering peaks. This turbulent cosmic pinnacle lies within a tempestuous stellar nursery called the Carina Nebula, located 7,500 light - years away in the southern constellation Carina. Hubble's Wide Field Camera 3 observed the pillar on Feb. 1 - 2, 2010. The colors in this composite image correspond to the glow of oxygen (blue), hydrogen and nitrogen (green), and sulfur (red)
Birth of stars in the nebula NGC 3372 - Star formation in the Carina Nebula - Detail of the Carene nebula (NGC 3372) obtained by the Hubble space telescope. The image shows a column of gas eroded by ultraviolet radiation emitted by young stars. Jets are also visible, showing the presence of emerging stars. NGC 3372 is located about 7500 light years away from Earth. The colors used in this image correspond to the emissions of different gases: sulfur in red, hydrogen in green and oxygen in blue. The NASA Hubble Space Telescope photograph captures the chaotic activity atop a three - light - year - tall pillar of gas and dust that is being eaten away by the brilliant light from nearby bright stars. The pillar is also being assaulted from within, as infant stars buried inside it fire off jets of gas that can be seen streaming from towering peaks. This turbulent cosmic pinnacle lies within a tempestuous stellar nursery called the Carina Nebula, located 7,500 light - years away in the southern constellation Carina. Hubble's Wide Field Camera 3 observed the pillar on Feb. 1 - 2, 2010. The colors in this composite image correspond to the glow of oxygen (blue), hydrogen and nitrogen (green), and sulfur (red)

PIX4619114: Birth of stars in the nebula NGC 3372 - Star formation in the Carina Nebula - Detail of the Carene nebula (NGC 3372) obtained by the Hubble space telescope. The image shows a column of gas eroded by ultraviolet radiation emitted by young stars. Jets are also visible, showing the presence of emerging stars. NGC 3372 is located about 7500 light years away from Earth. The colors used in this image correspond to the emissions of different gases: sulfur in red, hydrogen in green and oxygen in blue. The NASA Hubble Space Telescope photograph captures the chaotic activity atop a three - light - year - tall pillar of gas and dust that is being eaten away by the brilliant light from nearby bright stars. The pillar is also being assaulted from within, as infant stars buried inside it fire off jets of gas that can be seen streaming from towering peaks. This turbulent cosmic pinnacle lies within a tempestuous stellar nursery called the Carina Nebula, located 7,500 light - years away in the southern constellation Carina. Hubble's Wide Field Camera 3 observed the pillar on Feb. 1 - 2, 2010. The colors in this composite image correspond to the glow of oxygen (blue), hydrogen and nitrogen (green), and sulfur (red) / Bridgeman Images

ID: PIX4619114

Birth of stars in the nebula NGC 3372 - Star formation in the Carina Nebula - Detail of the Carene nebula (NGC 3372) obtained by the Hubble space telescope. The image shows a column of gas eroded by ultraviolet radiation emitted by young stars. Jets are also visible, showing the presence of emerging stars. NGC 3372 is located about 7500 light years away from Earth. The colors used in this image correspond to the emissions of different gases: sulfur in red, hydrogen in green and oxygen in blue. The NASA Hubble Space Telescope photograph captures the chaotic activity atop a three - light - year - tall pillar of gas and dust that is being eaten away by the brilliant light from nearby bright stars. The pillar is also being assaulted from within, as infant stars buried inside it fire off jets of gas that can be seen streaming from towering peaks. This turbulent cosmic pinnacle lies within a tempestuous stellar nursery called the Carina Nebula, located 7,500 light - years away in the souther

Quai des boateliers, Pont Saint Thomas in Strasbourg (Alsace).
Quai des boateliers, Pont Saint Thomas in Strasbourg (Alsace).

LBY4619119: Quai des boateliers, Pont Saint Thomas in Strasbourg (Alsace). / Bridgeman Images

ID: LBY4619119

Quai des boateliers, Pont Saint Thomas in Strasbourg (Alsace).

The tram in Strasbourg (Bas Rhin, Alsace).
The tram in Strasbourg (Bas Rhin, Alsace).

LBY4619251: The tram in Strasbourg (Bas Rhin, Alsace). / Bridgeman Images

ID: LBY4619251

The tram in Strasbourg (Bas Rhin, Alsace).

Place Kleber in Strasbourg (Bas Rhin, Alsace).
Place Kleber in Strasbourg (Bas Rhin, Alsace).

LBY4619319: Place Kleber in Strasbourg (Bas Rhin, Alsace). / Bridgeman Images

ID: LBY4619319

Place Kleber in Strasbourg (Bas Rhin, Alsace).

Nebulae NGC 6334 and NGC 6357 in Scorpio
Nebulae NGC 6334 and NGC 6357 in Scorpio

PIX4619363: Nebulae NGC 6334 and NGC 6357 in Scorpio / Bridgeman Images

ID: PIX4619363

Nebulae NGC 6334 and NGC 6357 in Scorpio

Nebula NGC 6334 in Scorpio - Cat's Paw nebula (NGC 6334) in Scorpius - The nebula NGC 6334 is located about 5500 years - light from Earth. It is a vast region of star formation. The Cat's Paw Nebula (NGC 6334) is a vast region of star formation. NGC 6334 lies about 5500 light - years from Earth in the constellation of Scorpius. The whole gas cloud is about 50 light - years across. NGC 6334 is one of the most active nurseries of massive stars in our galaxy and has been extensively studied by astronomers
Nebula NGC 6334 in Scorpio - Cat's Paw nebula (NGC 6334) in Scorpius - The nebula NGC 6334 is located about 5500 years - light from Earth. It is a vast region of star formation. The Cat's Paw Nebula (NGC 6334) is a vast region of star formation. NGC 6334 lies about 5500 light - years from Earth in the constellation of Scorpius. The whole gas cloud is about 50 light - years across. NGC 6334 is one of the most active nurseries of massive stars in our galaxy and has been extensively studied by astronomers

PIX4619380: Nebula NGC 6334 in Scorpio - Cat's Paw nebula (NGC 6334) in Scorpius - The nebula NGC 6334 is located about 5500 years - light from Earth. It is a vast region of star formation. The Cat's Paw Nebula (NGC 6334) is a vast region of star formation. NGC 6334 lies about 5500 light - years from Earth in the constellation of Scorpius. The whole gas cloud is about 50 light - years across. NGC 6334 is one of the most active nurseries of massive stars in our galaxy and has been extensively studied by astronomers / Bridgeman Images

ID: PIX4619380

Nebula NGC 6334 in Scorpio - Cat's Paw nebula (NGC 6334) in Scorpius - The nebula NGC 6334 is located about 5500 years - light from Earth. It is a vast region of star formation. The Cat's Paw Nebula (NGC 6334) is a vast region of star formation. NGC 6334 lies about 5500 light - years from Earth in the constellation of Scorpius. The whole gas cloud is about 50 light - years across. NGC 6334 is one of the most active nurseries of massive stars in our galaxy and has been extensively studied by astronomers

Nebula NGC 6357 in Scorpio - Nebula NGC 6357 in Scorpius - This nebulae is located about 5500 years - light from Earth. Image made with the 1.2m Telescope of Schmidt UK from Siding Spring. Star - forming region located 5500 light year away
Nebula NGC 6357 in Scorpio - Nebula NGC 6357 in Scorpius - This nebulae is located about 5500 years - light from Earth. Image made with the 1.2m Telescope of Schmidt UK from Siding Spring. Star - forming region located 5500 light year away

PIX4619393: Nebula NGC 6357 in Scorpio - Nebula NGC 6357 in Scorpius - This nebulae is located about 5500 years - light from Earth. Image made with the 1.2m Telescope of Schmidt UK from Siding Spring. Star - forming region located 5500 light year away / Bridgeman Images

ID: PIX4619393

Nebula NGC 6357 in Scorpio - Nebula NGC 6357 in Scorpius - This nebulae is located about 5500 years - light from Earth. Image made with the 1.2m Telescope of Schmidt UK from Siding Spring. Star - forming region located 5500 light year away

Nebula NGC 6357 in Scorpio - Nebula NGC 6357 in Scorpio
Nebula NGC 6357 in Scorpio - Nebula NGC 6357 in Scorpio

PIX4619403: Nebula NGC 6357 in Scorpio - Nebula NGC 6357 in Scorpio / Bridgeman Images

ID: PIX4619403

Nebula NGC 6357 in Scorpio - Nebula NGC 6357 in Scorpio

Nebula NGC 6357 in Scorpio
Nebula NGC 6357 in Scorpio

PIX4619428: Nebula NGC 6357 in Scorpio / Bridgeman Images

ID: PIX4619428

Nebula NGC 6357 in Scorpio

Nebula M20 in Sagittarius - View of the nebula Trifide (M20/ngc 6514) in the constellation Sagittarius
Nebula M20 in Sagittarius - View of the nebula Trifide (M20/ngc 6514) in the constellation Sagittarius

PIX4619445: Nebula M20 in Sagittarius - View of the nebula Trifide (M20/ngc 6514) in the constellation Sagittarius / Bridgeman Images

ID: PIX4619445

Nebula M20 in Sagittarius - View of the nebula Trifide (M20/ngc 6514) in the constellation Sagittarius

Tram to Strasbourg (Bas Rhin, Alsace).
Tram to Strasbourg (Bas Rhin, Alsace).

LBY4619449: Tram to Strasbourg (Bas Rhin, Alsace). / Bridgeman Images

ID: LBY4619449

Tram to Strasbourg (Bas Rhin, Alsace).

Trifide nebula (M20) in Sagittarius. - View of the Trifide nebula (M20/ngc 6514) located in the constellation of Sagittarius between 5000 and 10,000 years - light of the Earth
Trifide nebula (M20) in Sagittarius. - View of the Trifide nebula (M20/ngc 6514) located in the constellation of Sagittarius between 5000 and 10,000 years - light of the Earth

PIX4619461: Trifide nebula (M20) in Sagittarius. - View of the Trifide nebula (M20/ngc 6514) located in the constellation of Sagittarius between 5000 and 10,000 years - light of the Earth / Bridgeman Images

ID: PIX4619461

Trifide nebula (M20) in Sagittarius. - View of the Trifide nebula (M20/ngc 6514) located in the constellation of Sagittarius between 5000 and 10,000 years - light of the Earth

View of the nebula of the Lagoon (M8/NGC 6523). Located in Sagittarius, at a distance of 5800 light years, it is visible to the naked eye in good conditions. It is a star-forming region illuminated by several large O-type stars that belong to the open cluster NGC 6530 visible in the center of the image. The brightest part of the nebula is called the hourglass nebula whose gases are excited mainly by two massive supergeant stars Herschel 36 and 9 Sagittarii. M8 has at least 60 Giant B stars, 3 to 4 times more than the Orion nebula - The Lagoon nebula (M8), can be visible to the unaided eye as a small bright patch above the large Sagittarius star cloud in the Milky Way. The Lagoon nebula is a star-forming region about 5800 light years from us. The nebula is illuminated by several O-type giants within the open cluster NGC 6530 near the center of the nebula. The brightest part of the nebula is known as the “hourglass nebula”” and its gases are excited primarily by two massive O-type supergiants designated Herschel 36 and 9 Sagittarii. These two stars lie to the west of NGC 6530 and are separated from it by a dark lane dividing the nebula like a black lagoon, giving it its name. Twisted funnel shaped clouds are visible close to the illuminating stars, especially Herschel 36. They are due to shear forces between the hot excited gases at the surface and the cold interior of the clouds. At least 60 B-type giants are embedded in the nebula which make M8 3 to 4 times richer in massive stars than the Orion nebula: Nebula of the Lagoon (M8) in Sagittarius
View of the nebula of the Lagoon (M8/NGC 6523). Located in Sagittarius, at a distance of 5800 light years, it is visible to the naked eye in good conditions. It is a star-forming region illuminated by several large O-type stars that belong to the open cluster NGC 6530 visible in the center of the image. The brightest part of the nebula is called the hourglass nebula whose gases are excited mainly by two massive supergeant stars Herschel 36 and 9 Sagittarii. M8 has at least 60 Giant B stars, 3 to 4 times more than the Orion nebula - The Lagoon nebula (M8), can be visible to the unaided eye as a small bright patch above the large Sagittarius star cloud in the Milky Way. The Lagoon nebula is a star-forming region about 5800 light years from us. The nebula is illuminated by several O-type giants within the open cluster NGC 6530 near the center of the nebula. The brightest part of the nebula is known as the “hourglass nebula”” and its gases are excited primarily by two massive O-type supergiants designated Herschel 36 and 9 Sagittarii. These two stars lie to the west of NGC 6530 and are separated from it by a dark lane dividing the nebula like a black lagoon, giving it its name. Twisted funnel shaped clouds are visible close to the illuminating stars, especially Herschel 36. They are due to shear forces between the hot excited gases at the surface and the cold interior of the clouds. At least 60 B-type giants are embedded in the nebula which make M8 3 to 4 times richer in massive stars than the Orion nebula: Nebula of the Lagoon (M8) in Sagittarius

PIX4619585: View of the nebula of the Lagoon (M8/NGC 6523). Located in Sagittarius, at a distance of 5800 light years, it is visible to the naked eye in good conditions. It is a star-forming region illuminated by several large O-type stars that belong to the open cluster NGC 6530 visible in the center of the image. The brightest part of the nebula is called the hourglass nebula whose gases are excited mainly by two massive supergeant stars Herschel 36 and 9 Sagittarii. M8 has at least 60 Giant B stars, 3 to 4 times more than the Orion nebula - The Lagoon nebula (M8), can be visible to the unaided eye as a small bright patch above the large Sagittarius star cloud in the Milky Way. The Lagoon nebula is a star-forming region about 5800 light years from us. The nebula is illuminated by several O-type giants within the open cluster NGC 6530 near the center of the nebula. The brightest part of the nebula is known as the “hourglass nebula”” and its gases are excited primarily by two massive O-type supergiants designated Herschel 36 and 9 Sagittarii. These two stars lie to the west of NGC 6530 and are separated from it by a dark lane dividing the nebula like a black lagoon, giving it its name. Twisted funnel shaped clouds are visible close to the illuminating stars, especially Herschel 36. They are due to shear forces between the hot excited gases at the surface and the cold interior of the clouds. At least 60 B-type giants are embedded in the nebula which make M8 3 to 4 times richer in massive stars than the Orion nebula: Nebula of the Lagoon (M8) in Sagittarius / Bridgeman Images

ID: PIX4619585

View of the nebula of the Lagoon (M8/NGC 6523). Located in Sagittarius, at a distance of 5800 light years, it is visible to the naked eye in good conditions. It is a star-forming region illuminated by several large O-type stars that belong to the open cluster NGC 6530 visible in the center of the image. The brightest part of the nebula is called the hourglass nebula whose gases are excited mainly by two massive supergeant stars Herschel 36 and 9 Sagittarii. M8 has at least 60 Giant B stars, 3 to 4 times more than the Orion nebula - The Lagoon nebula (M8), can be visible to the unaided eye as a small bright patch above the large Sagittarius star cloud in the Milky Way. The Lagoon nebula is a star-forming region about 5800 light years from us. The nebula is illuminated by several O-type giants within the open cluster NGC 6530 near the center of the nebula. The brightest part of the nebula is known as the “hourglass nebula”” and its gases are excited primarily by two massive O-type superg

Nebula of the Lagoon (M8) in the Sagittair
Nebula of the Lagoon (M8) in the Sagittair

PIX4619635: Nebula of the Lagoon (M8) in the Sagittair / Bridgeman Images

ID: PIX4619635

Nebula of the Lagoon (M8) in the Sagittair

Nebula of the Lagoon (M8) in the Sagittair
Nebula of the Lagoon (M8) in the Sagittair

PIX4619653: Nebula of the Lagoon (M8) in the Sagittair / Bridgeman Images

ID: PIX4619653

Nebula of the Lagoon (M8) in the Sagittair

The International Space Station (ISS) 09 - 2006 - View of the station after the start of the shuttle Atlantis on 17 - 09 - 2006. Mission STS-115 (09 - 21 Sep 2006
The International Space Station (ISS) 09 - 2006 - View of the station after the start of the shuttle Atlantis on 17 - 09 - 2006. Mission STS-115 (09 - 21 Sep 2006

PIX4601485: The International Space Station (ISS) 09 - 2006 - View of the station after the start of the shuttle Atlantis on 17 - 09 - 2006. Mission STS-115 (09 - 21 Sep 2006 / Bridgeman Images

ID: PIX4601485

The International Space Station (ISS) 09 - 2006 - View of the station after the start of the shuttle Atlantis on 17 - 09 - 2006. Mission STS-115 (09 - 21 Sep 2006

Paris 4th arrondissement. Photography 25/08/07.
Paris 4th arrondissement. Photography 25/08/07.

TEC4601534: Paris 4th arrondissement. Photography 25/08/07. / Bridgeman Images

ID: TEC4601534

Paris 4th arrondissement. Photography 25/08/07.

Anousheh Ansari in Soyuz 09/2006 - Anousheh Ansari in Soyuz 09/2006 - Anousheh Ansari, the first woman space tourist, sitting in the Soyuz TMA - 9 on its way to the international space station. ISS Expedition 14
Anousheh Ansari in Soyuz 09/2006 - Anousheh Ansari in Soyuz 09/2006 - Anousheh Ansari, the first woman space tourist, sitting in the Soyuz TMA - 9 on its way to the international space station. ISS Expedition 14

PIX4601556: Anousheh Ansari in Soyuz 09/2006 - Anousheh Ansari in Soyuz 09/2006 - Anousheh Ansari, the first woman space tourist, sitting in the Soyuz TMA - 9 on its way to the international space station. ISS Expedition 14 / Bridgeman Images

ID: PIX4601556

Anousheh Ansari in Soyuz 09/2006 - Anousheh Ansari in Soyuz 09/2006 - Anousheh Ansari, the first woman space tourist, sitting in the Soyuz TMA - 9 on its way to the international space station. ISS Expedition 14

Astronaut Daniel Tani resting in ISS - Daniel Tani rests in the international space station - Astronaut Daniel Tani sleeps in his sleeping bag in the Unity module of the International Space Station. Mission STS - 120 - 2 November 2007. 2 Nov. 2007. Astronaut Daniel Tani, Expedition 16 flight engineer, sleeps in his sleeping bag in the Unity node of the International Space Station while Space Shuttle Discovery is docked with the station
Astronaut Daniel Tani resting in ISS - Daniel Tani rests in the international space station - Astronaut Daniel Tani sleeps in his sleeping bag in the Unity module of the International Space Station. Mission STS - 120 - 2 November 2007. 2 Nov. 2007. Astronaut Daniel Tani, Expedition 16 flight engineer, sleeps in his sleeping bag in the Unity node of the International Space Station while Space Shuttle Discovery is docked with the station

PIX4601779: Astronaut Daniel Tani resting in ISS - Daniel Tani rests in the international space station - Astronaut Daniel Tani sleeps in his sleeping bag in the Unity module of the International Space Station. Mission STS - 120 - 2 November 2007. 2 Nov. 2007. Astronaut Daniel Tani, Expedition 16 flight engineer, sleeps in his sleeping bag in the Unity node of the International Space Station while Space Shuttle Discovery is docked with the station / Bridgeman Images

ID: PIX4601779

Astronaut Daniel Tani resting in ISS - Daniel Tani rests in the international space station - Astronaut Daniel Tani sleeps in his sleeping bag in the Unity module of the International Space Station. Mission STS - 120 - 2 November 2007. 2 Nov. 2007. Astronaut Daniel Tani, Expedition 16 flight engineer, sleeps in his sleeping bag in the Unity node of the International Space Station while Space Shuttle Discovery is docked with the station

The International Space Station (ISS) 02/2008 - The International Space Station (ISS) 02/2008 - The International Space Station (ISS) seen from Shuttle Atlantis before returning to Earth on February 18, 2008. Backdropped by Earth's horizon and the blackness of space, the International Space Station is seen from Space Shuttle Atlantis as the two spacecraft begin their relative separation. Earlier the STS - 122 and Expedition 16 crews concluded almost nine days of cooperative work onboard the shuttle and station. Undocking of the two spacecraft occurred at 3:24 a.m. (CST) on Feb. 18, 2008
The International Space Station (ISS) 02/2008 - The International Space Station (ISS) 02/2008 - The International Space Station (ISS) seen from Shuttle Atlantis before returning to Earth on February 18, 2008. Backdropped by Earth's horizon and the blackness of space, the International Space Station is seen from Space Shuttle Atlantis as the two spacecraft begin their relative separation. Earlier the STS - 122 and Expedition 16 crews concluded almost nine days of cooperative work onboard the shuttle and station. Undocking of the two spacecraft occurred at 3:24 a.m. (CST) on Feb. 18, 2008

PIX4601875: The International Space Station (ISS) 02/2008 - The International Space Station (ISS) 02/2008 - The International Space Station (ISS) seen from Shuttle Atlantis before returning to Earth on February 18, 2008. Backdropped by Earth's horizon and the blackness of space, the International Space Station is seen from Space Shuttle Atlantis as the two spacecraft begin their relative separation. Earlier the STS - 122 and Expedition 16 crews concluded almost nine days of cooperative work onboard the shuttle and station. Undocking of the two spacecraft occurred at 3:24 a.m. (CST) on Feb. 18, 2008 / Bridgeman Images

ID: PIX4601875

The International Space Station (ISS) 02/2008 - The International Space Station (ISS) 02/2008 - The International Space Station (ISS) seen from Shuttle Atlantis before returning to Earth on February 18, 2008. Backdropped by Earth's horizon and the blackness of space, the International Space Station is seen from Space Shuttle Atlantis as the two spacecraft begin their relative separation. Earlier the STS - 122 and Expedition 16 crews concluded almost nine days of cooperative work onboard the shuttle and station. Undocking of the two spacecraft occurred at 3:24 a.m. (CST) on Feb. 18, 2008

The International Space Station (ISS) 02/2008 - The International Space Station (ISS) 02/2008 - Detail of the international space station with its new element, the European Columbus laboratory connects to the Harmony module, seen from the Atlantis shuttle before returning to Earth on 18 February 2008. A close - up view of the Columbus laboratory (top right), the newest addition to the International Space Station, is featured in this image photographed by a STS - 122 crewmember on Space Shuttle Atlantis shortly after the undocking of the two spacecraft. Undocking of the two spacecraft occurred at 3:24 a.m. (CST) on Feb. 18, 2008
The International Space Station (ISS) 02/2008 - The International Space Station (ISS) 02/2008 - Detail of the international space station with its new element, the European Columbus laboratory connects to the Harmony module, seen from the Atlantis shuttle before returning to Earth on 18 February 2008. A close - up view of the Columbus laboratory (top right), the newest addition to the International Space Station, is featured in this image photographed by a STS - 122 crewmember on Space Shuttle Atlantis shortly after the undocking of the two spacecraft. Undocking of the two spacecraft occurred at 3:24 a.m. (CST) on Feb. 18, 2008

PIX4601901: The International Space Station (ISS) 02/2008 - The International Space Station (ISS) 02/2008 - Detail of the international space station with its new element, the European Columbus laboratory connects to the Harmony module, seen from the Atlantis shuttle before returning to Earth on 18 February 2008. A close - up view of the Columbus laboratory (top right), the newest addition to the International Space Station, is featured in this image photographed by a STS - 122 crewmember on Space Shuttle Atlantis shortly after the undocking of the two spacecraft. Undocking of the two spacecraft occurred at 3:24 a.m. (CST) on Feb. 18, 2008 / Bridgeman Images

ID: PIX4601901

The International Space Station (ISS) 02/2008 - The International Space Station (ISS) 02/2008 - Detail of the international space station with its new element, the European Columbus laboratory connects to the Harmony module, seen from the Atlantis shuttle before returning to Earth on 18 February 2008. A close - up view of the Columbus laboratory (top right), the newest addition to the International Space Station, is featured in this image photographed by a STS - 122 crewmember on Space Shuttle Atlantis shortly after the undocking of the two spacecraft. Undocking of the two spacecraft occurred at 3:24 a.m. (CST) on Feb. 18, 2008

La rue du Roi de Sicily in Paris 4th arrondissement.
La rue du Roi de Sicily in Paris 4th arrondissement.

TEC4601484: La rue du Roi de Sicily in Paris 4th arrondissement. / Bridgeman Images

ID: TEC4601484

La rue du Roi de Sicily in Paris 4th arrondissement.

Place de l'Hotel de Ville in Paris during the commemorations of the Liberation of Paris. Photography 25/08/07.
Place de l'Hotel de Ville in Paris during the commemorations of the Liberation of Paris. Photography 25/08/07.

TEC4601555: Place de l'Hotel de Ville in Paris during the commemorations of the Liberation of Paris. Photography 25/08/07. / Bridgeman Images

ID: TEC4601555

Place de l'Hotel de Ville in Paris during the commemorations of the Liberation of Paris. Photography 25/08/07.

The International Space Station (ISS) 12 - 2006 - The International Space Station (ISS) 12 - 2006 - View of the station after the start of the shuttle Discovery on 19 - 12 - 2006. Mission STS-11
The International Space Station (ISS) 12 - 2006 - The International Space Station (ISS) 12 - 2006 - View of the station after the start of the shuttle Discovery on 19 - 12 - 2006. Mission STS-11

PIX4601601: The International Space Station (ISS) 12 - 2006 - The International Space Station (ISS) 12 - 2006 - View of the station after the start of the shuttle Discovery on 19 - 12 - 2006. Mission STS-11 / Bridgeman Images

ID: PIX4601601

The International Space Station (ISS) 12 - 2006 - The International Space Station (ISS) 12 - 2006 - View of the station after the start of the shuttle Discovery on 19 - 12 - 2006. Mission STS-11

Extravehicular exit of Sunita L. Williams. ISS - Expedition 14. 31 - 01 - 2007 - Extravehicular release of Sunita L. Williams. ISS - Expedition 14. 31 - 01 - 200
Extravehicular exit of Sunita L. Williams. ISS - Expedition 14. 31 - 01 - 2007 - Extravehicular release of Sunita L. Williams. ISS - Expedition 14. 31 - 01 - 200

PIX4601614: Extravehicular exit of Sunita L. Williams. ISS - Expedition 14. 31 - 01 - 2007 - Extravehicular release of Sunita L. Williams. ISS - Expedition 14. 31 - 01 - 200 / Bridgeman Images

ID: PIX4601614

Extravehicular exit of Sunita L. Williams. ISS - Expedition 14. 31 - 01 - 2007 - Extravehicular release of Sunita L. Williams. ISS - Expedition 14. 31 - 01 - 200

International Space Station (ISS) 06 - 2007 - View of the station after the start of the shuttle Atlantis on 19 - 06 - 2007. Mission STS-11
International Space Station (ISS) 06 - 2007 - View of the station after the start of the shuttle Atlantis on 19 - 06 - 2007. Mission STS-11

PIX4601700: International Space Station (ISS) 06 - 2007 - View of the station after the start of the shuttle Atlantis on 19 - 06 - 2007. Mission STS-11 / Bridgeman Images

ID: PIX4601700

International Space Station (ISS) 06 - 2007 - View of the station after the start of the shuttle Atlantis on 19 - 06 - 2007. Mission STS-11


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