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Gazing at the stars - Observation of the sky with a bezel
Gazing at the stars - Observation of the sky with a bezel

PIX4565936: Gazing at the stars - Observation of the sky with a bezel / Bridgeman Images

ID: PIX4565936

Gazing at the stars - Observation of the sky with a bezel

Tenryu-ji, a Buddhist temple in Kyoto, Japan.
Tenryu-ji, a Buddhist temple in Kyoto, Japan.

TEC4562909: Tenryu-ji, a Buddhist temple in Kyoto, Japan. / Bridgeman Images

ID: TEC4562909

Tenryu-ji, a Buddhist temple in Kyoto, Japan.

Lenin Mausolee (Vladimir Ilich Ulyaniov, 1870-1924) on the Red Square in Moscow (Russia)
Lenin Mausolee (Vladimir Ilich Ulyaniov, 1870-1924) on the Red Square in Moscow (Russia)

TEC4566463: Lenin Mausolee (Vladimir Ilich Ulyaniov, 1870-1924) on the Red Square in Moscow (Russia) / Bridgeman Images

ID: TEC4566463

Lenin Mausolee (Vladimir Ilich Ulyaniov, 1870-1924) on the Red Square in Moscow (Russia)

Star watching - Night sky observation - Two girls look at the sky sitting in the dunes, with the Big Bear in the background. Two girls watching the starry sky
Star watching - Night sky observation - Two girls look at the sky sitting in the dunes, with the Big Bear in the background. Two girls watching the starry sky

PIX4566248: Star watching - Night sky observation - Two girls look at the sky sitting in the dunes, with the Big Bear in the background. Two girls watching the starry sky / Bridgeman Images

ID: PIX4566248

Star watching - Night sky observation - Two girls look at the sky sitting in the dunes, with the Big Bear in the background. Two girls watching the starry sky

Photographer silhouette leans on the photographic chamber, made of wire, trade sign in Paris.
Photographer silhouette leans on the photographic chamber, made of wire, trade sign in Paris.

TEC4566281: Photographer silhouette leans on the photographic chamber, made of wire, trade sign in Paris. / Bridgeman Images

ID: TEC4566281

Photographer silhouette leans on the photographic chamber, made of wire, trade sign in Paris.

Gardener pushing his wheelbarrow full of plants, for the weekend house, trade sign in Paris.
Gardener pushing his wheelbarrow full of plants, for the weekend house, trade sign in Paris.

TEC4566304: Gardener pushing his wheelbarrow full of plants, for the weekend house, trade sign in Paris. / Bridgeman Images

ID: TEC4566304

Gardener pushing his wheelbarrow full of plants, for the weekend house, trade sign in Paris.

Amateur astronomer - Amateur astronomer - Amateur astronomer and astronomical bezel. Amateur astronomer and refractor
Amateur astronomer - Amateur astronomer - Amateur astronomer and astronomical bezel. Amateur astronomer and refractor

PIX4566340: Amateur astronomer - Amateur astronomer - Amateur astronomer and astronomical bezel. Amateur astronomer and refractor / Bridgeman Images

ID: PIX4566340

Amateur astronomer - Amateur astronomer - Amateur astronomer and astronomical bezel. Amateur astronomer and refractor

Amateur astronomer - Amateur astronomer - Amateur astronomer and astronomical bezel. Amateur astronomer and refractor
Amateur astronomer - Amateur astronomer - Amateur astronomer and astronomical bezel. Amateur astronomer and refractor

PIX4566346: Amateur astronomer - Amateur astronomer - Amateur astronomer and astronomical bezel. Amateur astronomer and refractor / Bridgeman Images

ID: PIX4566346

Amateur astronomer - Amateur astronomer - Amateur astronomer and astronomical bezel. Amateur astronomer and refractor

The Gum department store, one of the largest stores in Russia, stretches 252 metres long and 88 metres deep. It consists of three passages joined together by corridors and bridges and covered by a large glass that lets the light filter. Built in 1894, on Red Square, Moscow (Russia)
The Gum department store, one of the largest stores in Russia, stretches 252 metres long and 88 metres deep. It consists of three passages joined together by corridors and bridges and covered by a large glass that lets the light filter. Built in 1894, on Red Square, Moscow (Russia)

TEC4566531: The Gum department store, one of the largest stores in Russia, stretches 252 metres long and 88 metres deep. It consists of three passages joined together by corridors and bridges and covered by a large glass that lets the light filter. Built in 1894, on Red Square, Moscow (Russia) / Bridgeman Images

ID: TEC4566531

The Gum department store, one of the largest stores in Russia, stretches 252 metres long and 88 metres deep. It consists of three passages joined together by corridors and bridges and covered by a large glass that lets the light filter. Built in 1894, on Red Square, Moscow (Russia)

Catherine's palace in Pushkin (Russia). Construction 1756, architect Francesco Bartolomeo Rastrelli (1700-1771).
Catherine's palace in Pushkin (Russia). Construction 1756, architect Francesco Bartolomeo Rastrelli (1700-1771).

TEC4567943: Catherine's palace in Pushkin (Russia). Construction 1756, architect Francesco Bartolomeo Rastrelli (1700-1771). / Bridgeman Images

ID: TEC4567943

Catherine's palace in Pushkin (Russia). Construction 1756, architect Francesco Bartolomeo Rastrelli (1700-1771).

Open cluster M41 in the Great Dog - Open cluster M41 in Canis Major - M41 (NGC 2287), is a cluster of a hundred stars located about 2300 years - light from Earth. This open cluster contains about one hundred stars; it is located at about 2300 light year away. This skyview is corresponding to binoculars and small telescopes
Open cluster M41 in the Great Dog - Open cluster M41 in Canis Major - M41 (NGC 2287), is a cluster of a hundred stars located about 2300 years - light from Earth. This open cluster contains about one hundred stars; it is located at about 2300 light year away. This skyview is corresponding to binoculars and small telescopes

PIX4568016: Open cluster M41 in the Great Dog - Open cluster M41 in Canis Major - M41 (NGC 2287), is a cluster of a hundred stars located about 2300 years - light from Earth. This open cluster contains about one hundred stars; it is located at about 2300 light year away. This skyview is corresponding to binoculars and small telescopes / Bridgeman Images

ID: PIX4568016

Open cluster M41 in the Great Dog - Open cluster M41 in Canis Major - M41 (NGC 2287), is a cluster of a hundred stars located about 2300 years - light from Earth. This open cluster contains about one hundred stars; it is located at about 2300 light year away. This skyview is corresponding to binoculars and small telescopes

Place Jacques Duclos in Montreuil (Seine Saint Denis)
Place Jacques Duclos in Montreuil (Seine Saint Denis)

EPA4570136: Place Jacques Duclos in Montreuil (Seine Saint Denis) / Bridgeman Images

ID: EPA4570136

Place Jacques Duclos in Montreuil (Seine Saint Denis)

Core of the Hartley 2 comet seen by the Epoxi probe - Comet Hartley 2 nucleus seen by Deep impact spacecraft - Composite of images of the nucleus of the Hartley 2 comet obtained on November 4, 2010 during its approach by the Epoxi probe (Deep Impact). The core is 2 km long. This image montage shows comet Hartley 2 as NASA'S EPOXI mission approached and flew under the comet. The images progress in time clockwise, starting at the top left. The image was taken by Epoxi's Medium - Resolution Instrument on Nov. 4, 2010. The sun is to the right. The comet's nucleus, or main body, is approximately 2 kilometers (1.2 miles) long and 0.4 kilometers (0.25 miles) at the “” neck,””” or most narrow portion. Jets can be seen streaming out of the nucleus
Core of the Hartley 2 comet seen by the Epoxi probe - Comet Hartley 2 nucleus seen by Deep impact spacecraft - Composite of images of the nucleus of the Hartley 2 comet obtained on November 4, 2010 during its approach by the Epoxi probe (Deep Impact). The core is 2 km long. This image montage shows comet Hartley 2 as NASA'S EPOXI mission approached and flew under the comet. The images progress in time clockwise, starting at the top left. The image was taken by Epoxi's Medium - Resolution Instrument on Nov. 4, 2010. The sun is to the right. The comet's nucleus, or main body, is approximately 2 kilometers (1.2 miles) long and 0.4 kilometers (0.25 miles) at the “” neck,””” or most narrow portion. Jets can be seen streaming out of the nucleus

PIX4570260: Core of the Hartley 2 comet seen by the Epoxi probe - Comet Hartley 2 nucleus seen by Deep impact spacecraft - Composite of images of the nucleus of the Hartley 2 comet obtained on November 4, 2010 during its approach by the Epoxi probe (Deep Impact). The core is 2 km long. This image montage shows comet Hartley 2 as NASA'S EPOXI mission approached and flew under the comet. The images progress in time clockwise, starting at the top left. The image was taken by Epoxi's Medium - Resolution Instrument on Nov. 4, 2010. The sun is to the right. The comet's nucleus, or main body, is approximately 2 kilometers (1.2 miles) long and 0.4 kilometers (0.25 miles) at the “” neck,””” or most narrow portion. Jets can be seen streaming out of the nucleus / Bridgeman Images

ID: PIX4570260

Core of the Hartley 2 comet seen by the Epoxi probe - Comet Hartley 2 nucleus seen by Deep impact spacecraft - Composite of images of the nucleus of the Hartley 2 comet obtained on November 4, 2010 during its approach by the Epoxi probe (Deep Impact). The core is 2 km long. This image montage shows comet Hartley 2 as NASA'S EPOXI mission approached and flew under the comet. The images progress in time clockwise, starting at the top left. The image was taken by Epoxi's Medium - Resolution Instrument on Nov. 4, 2010. The sun is to the right. The comet's nucleus, or main body, is approximately 2 kilometers (1.2 miles) long and 0.4 kilometers (0.25 miles) at the “” neck,””” or most narrow portion. Jets can be seen streaming out of the nucleus

Core of Comet 67P/Churyumov - Gerasimenkovu by the Rosetta probe - Comet 67P/Churyumov - Gerasimenko nucleus seen by Rosetta - Image of the nucleus of Comet 67P/Churyumov - Gerasimenko seen on November 22, 2014 by the Rosetta probe at a distance of 30 km. OSIRIS wide - angle camera image acquired on 22 November 2014 from a distance of 30 km from Comet 67P/Churyumov - Gerasimenko. The image resolution is 2.8 m/pixel. The nucleus is deliberately overexposed in order to reveal the faint jets of activity
Core of Comet 67P/Churyumov - Gerasimenkovu by the Rosetta probe - Comet 67P/Churyumov - Gerasimenko nucleus seen by Rosetta - Image of the nucleus of Comet 67P/Churyumov - Gerasimenko seen on November 22, 2014 by the Rosetta probe at a distance of 30 km. OSIRIS wide - angle camera image acquired on 22 November 2014 from a distance of 30 km from Comet 67P/Churyumov - Gerasimenko. The image resolution is 2.8 m/pixel. The nucleus is deliberately overexposed in order to reveal the faint jets of activity

PIX4570311: Core of Comet 67P/Churyumov - Gerasimenkovu by the Rosetta probe - Comet 67P/Churyumov - Gerasimenko nucleus seen by Rosetta - Image of the nucleus of Comet 67P/Churyumov - Gerasimenko seen on November 22, 2014 by the Rosetta probe at a distance of 30 km. OSIRIS wide - angle camera image acquired on 22 November 2014 from a distance of 30 km from Comet 67P/Churyumov - Gerasimenko. The image resolution is 2.8 m/pixel. The nucleus is deliberately overexposed in order to reveal the faint jets of activity / Bridgeman Images

ID: PIX4570311

Core of Comet 67P/Churyumov - Gerasimenkovu by the Rosetta probe - Comet 67P/Churyumov - Gerasimenko nucleus seen by Rosetta - Image of the nucleus of Comet 67P/Churyumov - Gerasimenko seen on November 22, 2014 by the Rosetta probe at a distance of 30 km. OSIRIS wide - angle camera image acquired on 22 November 2014 from a distance of 30 km from Comet 67P/Churyumov - Gerasimenko. The image resolution is 2.8 m/pixel. The nucleus is deliberately overexposed in order to reveal the faint jets of activity

Open Cluster of Pleiades - The Pleiades star cluster - The Pleiades cluster is a cluster of about 500 young stars nees 150 million years ago. Visible in the constellation Taurus, this cluster is 440 years from the Earth. The Pleiades star cluster, also known as the Seven Sisters and Messier 45, is one of the brightest and famous star clusters visible in the northern hemisphere. It consists of about 500 bright, hot, young stars that were all born at the same time between 75 and 150 million years ago within a large cloud of dust and gas. The cluster contains many stars, of which only a handful are commonly visible to the naked eye. The blue haze that accompanies them is due to very fine dust which still remains and preferentially reflects the blue light from the stars. This star cluster lie some 440 light years away from the Earth, in the constellation of Taurus
Open Cluster of Pleiades - The Pleiades star cluster - The Pleiades cluster is a cluster of about 500 young stars nees 150 million years ago. Visible in the constellation Taurus, this cluster is 440 years from the Earth. The Pleiades star cluster, also known as the Seven Sisters and Messier 45, is one of the brightest and famous star clusters visible in the northern hemisphere. It consists of about 500 bright, hot, young stars that were all born at the same time between 75 and 150 million years ago within a large cloud of dust and gas. The cluster contains many stars, of which only a handful are commonly visible to the naked eye. The blue haze that accompanies them is due to very fine dust which still remains and preferentially reflects the blue light from the stars. This star cluster lie some 440 light years away from the Earth, in the constellation of Taurus

PIX4568697: Open Cluster of Pleiades - The Pleiades star cluster - The Pleiades cluster is a cluster of about 500 young stars nees 150 million years ago. Visible in the constellation Taurus, this cluster is 440 years from the Earth. The Pleiades star cluster, also known as the Seven Sisters and Messier 45, is one of the brightest and famous star clusters visible in the northern hemisphere. It consists of about 500 bright, hot, young stars that were all born at the same time between 75 and 150 million years ago within a large cloud of dust and gas. The cluster contains many stars, of which only a handful are commonly visible to the naked eye. The blue haze that accompanies them is due to very fine dust which still remains and preferentially reflects the blue light from the stars. This star cluster lie some 440 light years away from the Earth, in the constellation of Taurus / Bridgeman Images

ID: PIX4568697

Open Cluster of Pleiades - The Pleiades star cluster - The Pleiades cluster is a cluster of about 500 young stars nees 150 million years ago. Visible in the constellation Taurus, this cluster is 440 years from the Earth. The Pleiades star cluster, also known as the Seven Sisters and Messier 45, is one of the brightest and famous star clusters visible in the northern hemisphere. It consists of about 500 bright, hot, young stars that were all born at the same time between 75 and 150 million years ago within a large cloud of dust and gas. The cluster contains many stars, of which only a handful are commonly visible to the naked eye. The blue haze that accompanies them is due to very fine dust which still remains and preferentially reflects the blue light from the stars. This star cluster lie some 440 light years away from the Earth, in the constellation of Taurus

Dowtown Los Angeles Central Library 630 West 5th Street, Los Angeles, California, USA.
Dowtown Los Angeles Central Library 630 West 5th Street, Los Angeles, California, USA.

TEC4568797: Dowtown Los Angeles Central Library 630 West 5th Street, Los Angeles, California, USA. / Bridgeman Images

ID: TEC4568797

Dowtown Los Angeles Central Library 630 West 5th Street, Los Angeles, California, USA.

Open Cluster of Pleiades - The Pleiades star cluster - The Pleiades cluster is a cluster of about 500 young stars nees 150 million years ago. Visible in the constellation Taurus, this cluster is 440 years from the Earth. The Pleiades are one of the finest and nearest examples of a reflection nebula associated with a cluster of young stars. The cluster itself is a group of many hundreds of stars about 400 light years from Earth in the northern constellation of Taurus and has been recognised since ancient times. Seven of the brightest stars are quite easy to see with the unaided eye and bear the names of the Seven Sisters, the daughters of Atlas. The nebulosity seen here is light reflected from the particles in a cloud of cold gas and dust into which the cluster has drifted. It appears blue because these tiny interstellar particles scatter blue light more efficiently than the longer wavelengths of red light and it is streaky because of the distribution of dust particles in space
Open Cluster of Pleiades - The Pleiades star cluster - The Pleiades cluster is a cluster of about 500 young stars nees 150 million years ago. Visible in the constellation Taurus, this cluster is 440 years from the Earth. The Pleiades are one of the finest and nearest examples of a reflection nebula associated with a cluster of young stars. The cluster itself is a group of many hundreds of stars about 400 light years from Earth in the northern constellation of Taurus and has been recognised since ancient times. Seven of the brightest stars are quite easy to see with the unaided eye and bear the names of the Seven Sisters, the daughters of Atlas. The nebulosity seen here is light reflected from the particles in a cloud of cold gas and dust into which the cluster has drifted. It appears blue because these tiny interstellar particles scatter blue light more efficiently than the longer wavelengths of red light and it is streaky because of the distribution of dust particles in space

PIX4568850: Open Cluster of Pleiades - The Pleiades star cluster - The Pleiades cluster is a cluster of about 500 young stars nees 150 million years ago. Visible in the constellation Taurus, this cluster is 440 years from the Earth. The Pleiades are one of the finest and nearest examples of a reflection nebula associated with a cluster of young stars. The cluster itself is a group of many hundreds of stars about 400 light years from Earth in the northern constellation of Taurus and has been recognised since ancient times. Seven of the brightest stars are quite easy to see with the unaided eye and bear the names of the Seven Sisters, the daughters of Atlas. The nebulosity seen here is light reflected from the particles in a cloud of cold gas and dust into which the cluster has drifted. It appears blue because these tiny interstellar particles scatter blue light more efficiently than the longer wavelengths of red light and it is streaky because of the distribution of dust particles in space / Bridgeman Images

ID: PIX4568850

Open Cluster of Pleiades - The Pleiades star cluster - The Pleiades cluster is a cluster of about 500 young stars nees 150 million years ago. Visible in the constellation Taurus, this cluster is 440 years from the Earth. The Pleiades are one of the finest and nearest examples of a reflection nebula associated with a cluster of young stars. The cluster itself is a group of many hundreds of stars about 400 light years from Earth in the northern constellation of Taurus and has been recognised since ancient times. Seven of the brightest stars are quite easy to see with the unaided eye and bear the names of the Seven Sisters, the daughters of Atlas. The nebulosity seen here is light reflected from the particles in a cloud of cold gas and dust into which the cluster has drifted. It appears blue because these tiny interstellar particles scatter blue light more efficiently than the longer wavelengths of red light and it is streaky because of the distribution of dust particles in space

Hyades and Pleiades open clusters - Hyades and Pleiades open clusters - The Hyades cluster, on the left, with the brilliant star Aldebaran. On the right, the Pleiades cluster. These two clusters belong to the constellation of the Taurus of which Aldebaran is the brightest star; it is a red giante. The Hyades is seen at left, containing the bright star Aldeberan. The Pleiades is at right. Both are open clusters in the constellation of Taurus. This skyview is corresponding to binoculars and small telescopes
Hyades and Pleiades open clusters - Hyades and Pleiades open clusters - The Hyades cluster, on the left, with the brilliant star Aldebaran. On the right, the Pleiades cluster. These two clusters belong to the constellation of the Taurus of which Aldebaran is the brightest star; it is a red giante. The Hyades is seen at left, containing the bright star Aldeberan. The Pleiades is at right. Both are open clusters in the constellation of Taurus. This skyview is corresponding to binoculars and small telescopes

PIX4568855: Hyades and Pleiades open clusters - Hyades and Pleiades open clusters - The Hyades cluster, on the left, with the brilliant star Aldebaran. On the right, the Pleiades cluster. These two clusters belong to the constellation of the Taurus of which Aldebaran is the brightest star; it is a red giante. The Hyades is seen at left, containing the bright star Aldeberan. The Pleiades is at right. Both are open clusters in the constellation of Taurus. This skyview is corresponding to binoculars and small telescopes / Bridgeman Images

ID: PIX4568855

Hyades and Pleiades open clusters - Hyades and Pleiades open clusters - The Hyades cluster, on the left, with the brilliant star Aldebaran. On the right, the Pleiades cluster. These two clusters belong to the constellation of the Taurus of which Aldebaran is the brightest star; it is a red giante. The Hyades is seen at left, containing the bright star Aldeberan. The Pleiades is at right. Both are open clusters in the constellation of Taurus. This skyview is corresponding to binoculars and small telescopes

Open cluster M44 in cancer - Open star cluster M44 in Cancer - M44 is a cluster of stars located only 600 years - light from Earth, in the constellation Cancer. This field corresponds to the one obtained with binoculars or a small telescope. This star cluster is located about 600 light year away in Cancer.This skyview is corresponding to binoculars and small telescopes
Open cluster M44 in cancer - Open star cluster M44 in Cancer - M44 is a cluster of stars located only 600 years - light from Earth, in the constellation Cancer. This field corresponds to the one obtained with binoculars or a small telescope. This star cluster is located about 600 light year away in Cancer.This skyview is corresponding to binoculars and small telescopes

PIX4568192: Open cluster M44 in cancer - Open star cluster M44 in Cancer - M44 is a cluster of stars located only 600 years - light from Earth, in the constellation Cancer. This field corresponds to the one obtained with binoculars or a small telescope. This star cluster is located about 600 light year away in Cancer.This skyview is corresponding to binoculars and small telescopes / Bridgeman Images

ID: PIX4568192

Open cluster M44 in cancer - Open star cluster M44 in Cancer - M44 is a cluster of stars located only 600 years - light from Earth, in the constellation Cancer. This field corresponds to the one obtained with binoculars or a small telescope. This star cluster is located about 600 light year away in Cancer.This skyview is corresponding to binoculars and small telescopes

Open cluster M11 in the Sobieski ECU - M11 open cluster in Scutum - M11, NGC6705, is a particularly compact and star-rich open cluster (about 2900), located in the constellation Sobieski ECU. The image is of a young cluster of stars located in the direction of the constellation named Scutum. This tight gathering of stars, known as the Wild Duck Cluster or M11, features about 2,900 individual members - most of them are approximately 250 million years old - the newest stars appear white - blue, the older ones have a yellowed appearance. This group of stars hangs in space about 5,000 light - years from Earth
Open cluster M11 in the Sobieski ECU - M11 open cluster in Scutum - M11, NGC6705, is a particularly compact and star-rich open cluster (about 2900), located in the constellation Sobieski ECU. The image is of a young cluster of stars located in the direction of the constellation named Scutum. This tight gathering of stars, known as the Wild Duck Cluster or M11, features about 2,900 individual members - most of them are approximately 250 million years old - the newest stars appear white - blue, the older ones have a yellowed appearance. This group of stars hangs in space about 5,000 light - years from Earth

PIX4568468: Open cluster M11 in the Sobieski ECU - M11 open cluster in Scutum - M11, NGC6705, is a particularly compact and star-rich open cluster (about 2900), located in the constellation Sobieski ECU. The image is of a young cluster of stars located in the direction of the constellation named Scutum. This tight gathering of stars, known as the Wild Duck Cluster or M11, features about 2,900 individual members - most of them are approximately 250 million years old - the newest stars appear white - blue, the older ones have a yellowed appearance. This group of stars hangs in space about 5,000 light - years from Earth / Bridgeman Images

ID: PIX4568468

Open cluster M11 in the Sobieski ECU - M11 open cluster in Scutum - M11, NGC6705, is a particularly compact and star-rich open cluster (about 2900), located in the constellation Sobieski ECU. The image is of a young cluster of stars located in the direction of the constellation named Scutum. This tight gathering of stars, known as the Wild Duck Cluster or M11, features about 2,900 individual members - most of them are approximately 250 million years old - the newest stars appear white - blue, the older ones have a yellowed appearance. This group of stars hangs in space about 5,000 light - years from Earth

Open cluster NGC 6830 in the Little Fox - Open cluster NGC 6830 in Vulpecula - The NGC 6830 cluster is a cluster composed of 20 to 30 very scattered stars; its distance is estimated at 5,500 years - light. This cluster of 20 to 30 stars is located 5 500 light years away
Open cluster NGC 6830 in the Little Fox - Open cluster NGC 6830 in Vulpecula - The NGC 6830 cluster is a cluster composed of 20 to 30 very scattered stars; its distance is estimated at 5,500 years - light. This cluster of 20 to 30 stars is located 5 500 light years away

PIX4568519: Open cluster NGC 6830 in the Little Fox - Open cluster NGC 6830 in Vulpecula - The NGC 6830 cluster is a cluster composed of 20 to 30 very scattered stars; its distance is estimated at 5,500 years - light. This cluster of 20 to 30 stars is located 5 500 light years away / Bridgeman Images

ID: PIX4568519

Open cluster NGC 6830 in the Little Fox - Open cluster NGC 6830 in Vulpecula - The NGC 6830 cluster is a cluster composed of 20 to 30 very scattered stars; its distance is estimated at 5,500 years - light. This cluster of 20 to 30 stars is located 5 500 light years away

The McNaught comet seen over Santiago - Chile - Comet McNaught (C/2006 P1) over Santiago 01/2007 - View of the McNaught comet obtained on January 20, 2007 above the city of Santiago in Chile. Comet McNaught (C/2006 P1) as seen over Santiago, Chile, on January 20 2007
The McNaught comet seen over Santiago - Chile - Comet McNaught (C/2006 P1) over Santiago 01/2007 - View of the McNaught comet obtained on January 20, 2007 above the city of Santiago in Chile. Comet McNaught (C/2006 P1) as seen over Santiago, Chile, on January 20 2007

PIX4570602: The McNaught comet seen over Santiago - Chile - Comet McNaught (C/2006 P1) over Santiago 01/2007 - View of the McNaught comet obtained on January 20, 2007 above the city of Santiago in Chile. Comet McNaught (C/2006 P1) as seen over Santiago, Chile, on January 20 2007 / Bridgeman Images

ID: PIX4570602

The McNaught comet seen over Santiago - Chile - Comet McNaught (C/2006 P1) over Santiago 01/2007 - View of the McNaught comet obtained on January 20, 2007 above the city of Santiago in Chile. Comet McNaught (C/2006 P1) as seen over Santiago, Chile, on January 20 2007

View of Comet McNaught on January 26, 2007 - Comet McNaught (C/2006 P1) Jan 26, 2007 - View of Comet McNaught obtained on January 26, 2007 at 23:55 in Queenstown, New Zealand. View of the Comet McNaught on Jan 26 2007 over Queenstown, South Island, New Zealand
View of Comet McNaught on January 26, 2007 - Comet McNaught (C/2006 P1) Jan 26, 2007 - View of Comet McNaught obtained on January 26, 2007 at 23:55 in Queenstown, New Zealand. View of the Comet McNaught on Jan 26 2007 over Queenstown, South Island, New Zealand

PIX4570650: View of Comet McNaught on January 26, 2007 - Comet McNaught (C/2006 P1) Jan 26, 2007 - View of Comet McNaught obtained on January 26, 2007 at 23:55 in Queenstown, New Zealand. View of the Comet McNaught on Jan 26 2007 over Queenstown, South Island, New Zealand / Bridgeman Images

ID: PIX4570650

View of Comet McNaught on January 26, 2007 - Comet McNaught (C/2006 P1) Jan 26, 2007 - View of Comet McNaught obtained on January 26, 2007 at 23:55 in Queenstown, New Zealand. View of the Comet McNaught on Jan 26 2007 over Queenstown, South Island, New Zealand

Comete McNaught 01/2007 - Comet McNaught 01/2007 - View of the McNaught comet obtained on January 19, 2007 from Australia. Chiro Observatory - Western Australia. Comet McNaught as seen from Chiro Observatory, W. Australia. Jan 19 2007
Comete McNaught 01/2007 - Comet McNaught 01/2007 - View of the McNaught comet obtained on January 19, 2007 from Australia. Chiro Observatory - Western Australia. Comet McNaught as seen from Chiro Observatory, W. Australia. Jan 19 2007

PIX4570754: Comete McNaught 01/2007 - Comet McNaught 01/2007 - View of the McNaught comet obtained on January 19, 2007 from Australia. Chiro Observatory - Western Australia. Comet McNaught as seen from Chiro Observatory, W. Australia. Jan 19 2007 / Bridgeman Images

ID: PIX4570754

Comete McNaught 01/2007 - Comet McNaught 01/2007 - View of the McNaught comet obtained on January 19, 2007 from Australia. Chiro Observatory - Western Australia. Comet McNaught as seen from Chiro Observatory, W. Australia. Jan 19 2007

Comete 17P/Holmes 29/10/2007 - Comet 17P/Holmes October 29 2007 - View of comet 17P/Holmes on October 29, 2007. On October 24, 2007, Comete 17P/Holmes suddenly increased luminosite and became visible to the naked eye. The false nucleus and inner coma of Comet 17P/Holmes is seen here in a composite exposures on 29 October 2007. Comet 17P/Holmes began a spectacular outburst in brightness on October 24th, brightening from 17th magnitude to 2.5th magnitude, an increase of more than 1 million times brighter to become a unaided - eye object in the constellation of Perseus
Comete 17P/Holmes 29/10/2007 - Comet 17P/Holmes October 29 2007 - View of comet 17P/Holmes on October 29, 2007. On October 24, 2007, Comete 17P/Holmes suddenly increased luminosite and became visible to the naked eye. The false nucleus and inner coma of Comet 17P/Holmes is seen here in a composite exposures on 29 October 2007. Comet 17P/Holmes began a spectacular outburst in brightness on October 24th, brightening from 17th magnitude to 2.5th magnitude, an increase of more than 1 million times brighter to become a unaided - eye object in the constellation of Perseus

PIX4570924: Comete 17P/Holmes 29/10/2007 - Comet 17P/Holmes October 29 2007 - View of comet 17P/Holmes on October 29, 2007. On October 24, 2007, Comete 17P/Holmes suddenly increased luminosite and became visible to the naked eye. The false nucleus and inner coma of Comet 17P/Holmes is seen here in a composite exposures on 29 October 2007. Comet 17P/Holmes began a spectacular outburst in brightness on October 24th, brightening from 17th magnitude to 2.5th magnitude, an increase of more than 1 million times brighter to become a unaided - eye object in the constellation of Perseus / Bridgeman Images

ID: PIX4570924

Comete 17P/Holmes 29/10/2007 - Comet 17P/Holmes October 29 2007 - View of comet 17P/Holmes on October 29, 2007. On October 24, 2007, Comete 17P/Holmes suddenly increased luminosite and became visible to the naked eye. The false nucleus and inner coma of Comet 17P/Holmes is seen here in a composite exposures on 29 October 2007. Comet 17P/Holmes began a spectacular outburst in brightness on October 24th, brightening from 17th magnitude to 2.5th magnitude, an increase of more than 1 million times brighter to become a unaided - eye object in the constellation of Perseus

La Meridienne de l'Hotel Chenizot - Paris - Sundial in Paris: This meridian dates back to 1730. It indicates noon, as well as the shifts and half hours before and after. A Meridian is based on the well-known principle of the sundial, but only preys to determine the exact time of noon (Meridian = half of the day). 51 Rue Saint-Louis, 75004
La Meridienne de l'Hotel Chenizot - Paris - Sundial in Paris: This meridian dates back to 1730. It indicates noon, as well as the shifts and half hours before and after. A Meridian is based on the well-known principle of the sundial, but only preys to determine the exact time of noon (Meridian = half of the day). 51 Rue Saint-Louis, 75004

PIX4569237: La Meridienne de l'Hotel Chenizot - Paris - Sundial in Paris: This meridian dates back to 1730. It indicates noon, as well as the shifts and half hours before and after. A Meridian is based on the well-known principle of the sundial, but only preys to determine the exact time of noon (Meridian = half of the day). 51 Rue Saint-Louis, 75004 / Bridgeman Images

ID: PIX4569237

La Meridienne de l'Hotel Chenizot - Paris - Sundial in Paris: This meridian dates back to 1730. It indicates noon, as well as the shifts and half hours before and after. A Meridian is based on the well-known principle of the sundial, but only preys to determine the exact time of noon (Meridian = half of the day). 51 Rue Saint-Louis, 75004

Sundial - Paris - Sundial in Paris: Recent sundial on the facade of a building located at 45 rue Letellier (75015)
Sundial - Paris - Sundial in Paris: Recent sundial on the facade of a building located at 45 rue Letellier (75015)

PIX4569355: Sundial - Paris - Sundial in Paris: Recent sundial on the facade of a building located at 45 rue Letellier (75015) / Bridgeman Images

ID: PIX4569355

Sundial - Paris - Sundial in Paris: Recent sundial on the facade of a building located at 45 rue Letellier (75015)

Office real estate in Los Angeles (California, United States).
Office real estate in Los Angeles (California, United States).

TEC4568761: Office real estate in Los Angeles (California, United States). / Bridgeman Images

ID: TEC4568761

Office real estate in Los Angeles (California, United States).

Frontispiece of Non me lo dite, opera by Francesco Paolo Tosti
Frontispiece of Non me lo dite, opera by Francesco Paolo Tosti

LRI4568890: Frontispiece of Non me lo dite, opera by Francesco Paolo Tosti / Bridgeman Images

ID: LRI4568890

Frontispiece of Non me lo dite, opera by Francesco Paolo Tosti

Sundial - Riquewihr - Sundial - Riquewihr - Sundial - 1971 sundial
Sundial - Riquewihr - Sundial - Riquewihr - Sundial - 1971 sundial

PIX4569392: Sundial - Riquewihr - Sundial - Riquewihr - Sundial - 1971 sundial / Bridgeman Images

ID: PIX4569392

Sundial - Riquewihr - Sundial - Riquewihr - Sundial - 1971 sundial

Sundial - Valloire - Sundial in France - Valloire - Dial realised by Zarbula, restored in 1998. Hameau Les Verneys, Savoie
Sundial - Valloire - Sundial in France - Valloire - Dial realised by Zarbula, restored in 1998. Hameau Les Verneys, Savoie

PIX4569412: Sundial - Valloire - Sundial in France - Valloire - Dial realised by Zarbula, restored in 1998. Hameau Les Verneys, Savoie / Bridgeman Images

ID: PIX4569412

Sundial - Valloire - Sundial in France - Valloire - Dial realised by Zarbula, restored in 1998. Hameau Les Verneys, Savoie

L'immeuble du Parisien Libere, 124rue Reaumur, Paris 2nd arrondissement. Construction 1905, architect Georges Chedanne.
L'immeuble du Parisien Libere, 124rue Reaumur, Paris 2nd arrondissement. Construction 1905, architect Georges Chedanne.

TEC4571183: L'immeuble du Parisien Libere, 124rue Reaumur, Paris 2nd arrondissement. Construction 1905, architect Georges Chedanne. / Bridgeman Images

ID: TEC4571183

L'immeuble du Parisien Libere, 124rue Reaumur, Paris 2nd arrondissement. Construction 1905, architect Georges Chedanne.

The passage of the Grand Cerf in Paris 2nd arrondissement.
The passage of the Grand Cerf in Paris 2nd arrondissement.

TEC4571345: The passage of the Grand Cerf in Paris 2nd arrondissement. / Bridgeman Images

ID: TEC4571345

The passage of the Grand Cerf in Paris 2nd arrondissement.

Comete Hale - Bopp and Nebula North America - Comet Hale - Bopp and the North America Nebula - March 7, 1997. Hale - Bopp and the North American Nebula on 7 March 1997
Comete Hale - Bopp and Nebula North America - Comet Hale - Bopp and the North America Nebula - March 7, 1997. Hale - Bopp and the North American Nebula on 7 March 1997

PIX4569683: Comete Hale - Bopp and Nebula North America - Comet Hale - Bopp and the North America Nebula - March 7, 1997. Hale - Bopp and the North American Nebula on 7 March 1997 / Bridgeman Images

ID: PIX4569683

Comete Hale - Bopp and Nebula North America - Comet Hale - Bopp and the North America Nebula - March 7, 1997. Hale - Bopp and the North American Nebula on 7 March 1997

Aerial view on vineyards in the east of Mendoza (photography, 1983)
Aerial view on vineyards in the east of Mendoza (photography, 1983)

LRI4569736: Aerial view on vineyards in the east of Mendoza (photography, 1983) / Bridgeman Images

ID: LRI4569736

Aerial view on vineyards in the east of Mendoza (photography, 1983)

Open cluster CR 399 in Little Fox - The Coathanger (CR 399) in Vulpecula - The Hanger cluster or Brocchi cluster is not a true cluster of stars but an asterism located in the constellation Little Fox
Open cluster CR 399 in Little Fox - The Coathanger (CR 399) in Vulpecula - The Hanger cluster or Brocchi cluster is not a true cluster of stars but an asterism located in the constellation Little Fox

PIX4569023: Open cluster CR 399 in Little Fox - The Coathanger (CR 399) in Vulpecula - The Hanger cluster or Brocchi cluster is not a true cluster of stars but an asterism located in the constellation Little Fox / Bridgeman Images

ID: PIX4569023

Open cluster CR 399 in Little Fox - The Coathanger (CR 399) in Vulpecula - The Hanger cluster or Brocchi cluster is not a true cluster of stars but an asterism located in the constellation Little Fox


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