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Barree spiral galaxy NGC 1300 in Eridan - NGC 1300, barred spiral galaxy in Eridanus - The galaxy NGC 1300 is located about 60 million years ago - light and extends over about 85 000 years - light. Spiral galaxies appear in a variety of guises, but none are more intriguing than the barred variety. As their name suggests, these galaxies are distinguished by a bar, extending (in this case) like two more of less straight assemblies of stars either side of the bright nucleus. Caught up in the bar are two dust lanes, emerging on either side of the nuclear mass. At some distance from the nucleus, the straight, almost structurreless bar and dust lanes abruptly turn at a sharp angle. It is here that the delicately curved arms of the spiral begin, and it is here that star formation is at its most concentrated. Many spirals have such bars, including the Milky Way, where it is a subtle feature, very difficult to detect. NGC 1300, in the southern constellation of Eridanus is among the finest examp

Barree spiral galaxy NGC 1300 in Eridan - NGC 1300, barred spiral galaxy in Eridanus - The galaxy NGC 1300 is located about 60 million years ago - light and extends over about 85 000 years - light. Spiral galaxies appear in a variety of guises, but none are more intriguing than the barred variety. As their name suggests, these galaxies are distinguished by a bar, extending (in this case) like two more of less straight assemblies of stars either side of the bright nucleus. Caught up in the bar are two dust lanes, emerging on either side of the nuclear mass. At some distance from the nucleus, the straight, almost structurreless bar and dust lanes abruptly turn at a sharp angle. It is here that the delicately curved arms of the spiral begin, and it is here that star formation is at its most concentrated. Many spirals have such bars, including the Milky Way, where it is a subtle feature, very difficult to detect. NGC 1300, in the southern constellation of Eridanus is among the finest examp

PIX4609731

An artist of tangka showing his creation at his workroom in Kangding County in Ganzi Tibetan Autonomous Prefecture, southwest China's Sichuan Province, October 21, 2005

An artist of tangka showing his creation at his workroom in Kangding County in Ganzi Tibetan Autonomous Prefecture, southwest China's Sichuan Province, October 21, 2005

UIG3903046

The photo taken on Oct. 28, 2005 shows the highway linking Sichuan and Tibet zigzagging its way up Mount Jianziwan (curve of scissors), with its bealock at 4, 659 meters high above sea level, in Ganzi Tibetan Autonomous Prefecture of southwest China's Sichuan Province

The photo taken on Oct. 28, 2005 shows the highway linking Sichuan and Tibet zigzagging its way up Mount Jianziwan (curve of scissors), with its bealock at 4, 659 meters high above sea level, in Ganzi Tibetan Autonomous Prefecture of southwest China's Sichuan Province

UIG3903018

Nebula Trifide (M20) in the constellation Sagittarius - Trifid nebula (M20) in Sagittarius - View of the Trifide nebula (M20 or NGC 6514) located in the constellation Sagittarius between 5000 and 10,000 years - light from Earth. Image obtained by Siding Spring's 3.9m telescope. Trifid nebula is located in Sagittarius constellation between 5000 and 10 000 light - years away. Stars, the Sun included, were born within clouds of dusty gas such as the Trifid Nebula. Within it a number of young hot stars have already formed. The hottest cause the gas, mostly hydrogen, to emit its characteristic red light. Around the red emission nebula the gas contains many dust grains which preferentially reflect the blue component of starlight, and to the north (top) of the nebula can be seen a bright star which illuminates part of the dust to create a region of blue reflection. In some parts of the nebula there are so many dust grains that they hide the glowing gas, producing the three dark lanes which gi

Nebula Trifide (M20) in the constellation Sagittarius - Trifid nebula (M20) in Sagittarius - View of the Trifide nebula (M20 or NGC 6514) located in the constellation Sagittarius between 5000 and 10,000 years - light from Earth. Image obtained by Siding Spring's 3.9m telescope. Trifid nebula is located in Sagittarius constellation between 5000 and 10 000 light - years away. Stars, the Sun included, were born within clouds of dusty gas such as the Trifid Nebula. Within it a number of young hot stars have already formed. The hottest cause the gas, mostly hydrogen, to emit its characteristic red light. Around the red emission nebula the gas contains many dust grains which preferentially reflect the blue component of starlight, and to the north (top) of the nebula can be seen a bright star which illuminates part of the dust to create a region of blue reflection. In some parts of the nebula there are so many dust grains that they hide the glowing gas, producing the three dark lanes which gi

PIX4619538

Saxony, GDR, historical, Sale, Shopping, Businesses, stores, Trade, Retail …, 1988 (photo)

Saxony, GDR, historical, Sale, Shopping, Businesses, stores, Trade, Retail …, 1988 (photo)

Sächsische Zeitung

IMO8755162

Nebula Trifide (M20) in the constellation Sagittarius - Trifid nebula (M20) in Sagittarius - View of the Trifide nebula (M20 or NGC 6514) located in the constellation Sagittarius between 5000 and 10,000 years - light from Earth. Image obtained by Siding Spring's 3.9m telescope. Trifid nebula is located in Sagittarius constellation between 5000 and 10 000 light - years away. Stars, the Sun included, were born within clouds of dusty gas such as the Trifid Nebula. Within it a number of young hot stars have already formed. The hottest cause the gas, mostly hydrogen, to emit its characteristic red light. Around the red emission nebula the gas contains many dust grains which preferentially reflect the blue component of starlight, and to the north (top) of the nebula can be seen a bright star which illuminates part of the dust to create a region of blue reflection. In some parts of the nebula there are so many dust grains that they hide the glowing gas, producing the three dark lanes which gi

Nebula Trifide (M20) in the constellation Sagittarius - Trifid nebula (M20) in Sagittarius - View of the Trifide nebula (M20 or NGC 6514) located in the constellation Sagittarius between 5000 and 10,000 years - light from Earth. Image obtained by Siding Spring's 3.9m telescope. Trifid nebula is located in Sagittarius constellation between 5000 and 10 000 light - years away. Stars, the Sun included, were born within clouds of dusty gas such as the Trifid Nebula. Within it a number of young hot stars have already formed. The hottest cause the gas, mostly hydrogen, to emit its characteristic red light. Around the red emission nebula the gas contains many dust grains which preferentially reflect the blue component of starlight, and to the north (top) of the nebula can be seen a bright star which illuminates part of the dust to create a region of blue reflection. In some parts of the nebula there are so many dust grains that they hide the glowing gas, producing the three dark lanes which gi

PIX4619434

Nebula Trifide (M20) in the constellation Sagittarius - Trifid nebula (M20) in Sagittarius - View of the Trifide nebula (M20 or NGC 6514) located in the constellation Sagittarius between 5000 and 10,000 years - light from Earth. Image obtained with a telescope of 61 cm. Trifid nebula is located in Sagittarius constellation between 5000 and 10 000 light - years away. Stars, the Sun included, were born within clouds of dusty gas such as the Trifid Nebula. Within it a number of young hot stars have already formed. The hottest cause the gas, mostly hydrogen, to emit its characteristic red light. Around the red emission nebula the gas contains many dust grains which preferentially reflect the blue component of starlight, and to the north (top) of the nebula can be seen a bright star which illuminates part of the dust to create a region of blue reflection. In some parts of the nebula there are so many dust grains that they hide the glowing gas, producing the three dark lanes which give the o

Nebula Trifide (M20) in the constellation Sagittarius - Trifid nebula (M20) in Sagittarius - View of the Trifide nebula (M20 or NGC 6514) located in the constellation Sagittarius between 5000 and 10,000 years - light from Earth. Image obtained with a telescope of 61 cm. Trifid nebula is located in Sagittarius constellation between 5000 and 10 000 light - years away. Stars, the Sun included, were born within clouds of dusty gas such as the Trifid Nebula. Within it a number of young hot stars have already formed. The hottest cause the gas, mostly hydrogen, to emit its characteristic red light. Around the red emission nebula the gas contains many dust grains which preferentially reflect the blue component of starlight, and to the north (top) of the nebula can be seen a bright star which illuminates part of the dust to create a region of blue reflection. In some parts of the nebula there are so many dust grains that they hide the glowing gas, producing the three dark lanes which give the o

Adam Block

PIX4619510

Center of the Trifid Nebula (M20) - Center of the Trifid Nebula - The Trifid Nebula (M20) is located between 5000 and 10,000 years - light of the Earth in the constellation of Sagittarius. This image obtained by the Hubble space telescope shows the center of this nebula. A group of bright stars is visible in the center of the image near the dark bands of interstellar dust. These stars are young, blue, massive and extremely hot stars; they are O-type stars and the radiation they emit influence the evolution and structure of the nebula. Trifid Nebula, also known as Messier 20 and NGC 6514, lies within our own Milky Way Galaxy between 5000 and 10 000 light - years from Earth, in the constellation Sagittarius. This image from the Hubble Space Telescope offers a close - up view of the center of the Trifid Nebula, near the intersection of the dust bands, where a group of recently formed, massive, bright stars is easily visible. These stars, which astronomers classify as belonging to the hott

Center of the Trifid Nebula (M20) - Center of the Trifid Nebula - The Trifid Nebula (M20) is located between 5000 and 10,000 years - light of the Earth in the constellation of Sagittarius. This image obtained by the Hubble space telescope shows the center of this nebula. A group of bright stars is visible in the center of the image near the dark bands of interstellar dust. These stars are young, blue, massive and extremely hot stars; they are O-type stars and the radiation they emit influence the evolution and structure of the nebula. Trifid Nebula, also known as Messier 20 and NGC 6514, lies within our own Milky Way Galaxy between 5000 and 10 000 light - years from Earth, in the constellation Sagittarius. This image from the Hubble Space Telescope offers a close - up view of the center of the Trifid Nebula, near the intersection of the dust bands, where a group of recently formed, massive, bright stars is easily visible. These stars, which astronomers classify as belonging to the hott

PIX4619552

Saxony, GDR, historical, Sale, Shopping, Businesses, stores, Trade, Retail …, 1988 (photo)

Saxony, GDR, historical, Sale, Shopping, Businesses, stores, Trade, Retail …, 1988 (photo)

Sächsische Zeitung

IMO8755157

There are more than 175 factories employing about 80, 000 workers, 80% of whom are females in the Chittagong Export Processing Zone (CEPZ) in Chittagong, Bangladesh. The ready made garment industry has been the key export division and the chief source of foreign exchange for about 25 years. Not only does the country generate about 5 billion dollars worth of products each year but the industry itself provides employment to about 3 million workers throughout the country. Chittagong, Bangladesh. November 22, 2008. . (photo)

There are more than 175 factories employing about 80, 000 workers, 80% of whom are females in the Chittagong Export Processing Zone (CEPZ) in Chittagong, Bangladesh. The ready made garment industry has been the key export division and the chief source of foreign exchange for about 25 years. Not only does the country generate about 5 billion dollars worth of products each year but the industry itself provides employment to about 3 million workers throughout the country. Chittagong, Bangladesh. November 22, 2008. . (photo)

UIG801720

Nebula NGC 7635 in Cassiopee - The Bubble Nebula: This nebula is located about 8000 light years from Earth. A star 40 times more massive than our Sun, called Wolf-Rayet, is responsible for the formation of this bubble; it is the star BD+60* 2522. Image obtained by the space telescope Hubble - The Bubble Nebula, also known as NGC 7635, is an emission nebula located 8 000 light-years away - This complete view of the Bubble Nebula allows us to fully appreciate the almost perfectly symmetrical shell which gives the nebula its name. This shell is the result of a powerful flow of gas - known as a stellar wind - from the bright star visible just to the left of centre in this image. The star, SAO 20575, is between ten and twenty times the mass of the Sun and the pressure created by its stellar wind forces the surrounding interstellar material outwards into this bubble-like form - The giant molecular cloud that surrounds the star - glowing in the star's intense ultraviolet radiation - tries to

Nebula NGC 7635 in Cassiopee - The Bubble Nebula: This nebula is located about 8000 light years from Earth. A star 40 times more massive than our Sun, called Wolf-Rayet, is responsible for the formation of this bubble; it is the star BD+60* 2522. Image obtained by the space telescope Hubble - The Bubble Nebula, also known as NGC 7635, is an emission nebula located 8 000 light-years away - This complete view of the Bubble Nebula allows us to fully appreciate the almost perfectly symmetrical shell which gives the nebula its name. This shell is the result of a powerful flow of gas - known as a stellar wind - from the bright star visible just to the left of centre in this image. The star, SAO 20575, is between ten and twenty times the mass of the Sun and the pressure created by its stellar wind forces the surrounding interstellar material outwards into this bubble-like form - The giant molecular cloud that surrounds the star - glowing in the star's intense ultraviolet radiation - tries to

PIX4620728

Barree spiral galaxy NGC 1300 in Eridan - Barred spiral galaxy NGC 1300 in Eridanus - The galaxy NGC1300 is located about 60 million years ago - light and extends over about 85 000 years - light. This image was obtained by the Hubble Space Telescope in September 2004. NGC 1300 is considered to be prototypical of barred spiral galaxies. Barred spirals differ from normal spiral galaxies in that the arms of the galaxy do not spiral all the way into the center, but are connected to the two ends of a straight bar of stars containing the nucleus at its center. At Hubble's resolution, a myriad of fine details, some of which have never before been seen, is seen throughout the galaxy's arms, disk, bulge, and nucleus. Blue and red supergiant stars, star clusters, and star - forming regions are well resolved across the spiral arms, and dust lanes trace out fine structures in the disk and bar. Numerous more distant galaxies are visible in the background, and are seen even through the densest regio

Barree spiral galaxy NGC 1300 in Eridan - Barred spiral galaxy NGC 1300 in Eridanus - The galaxy NGC1300 is located about 60 million years ago - light and extends over about 85 000 years - light. This image was obtained by the Hubble Space Telescope in September 2004. NGC 1300 is considered to be prototypical of barred spiral galaxies. Barred spirals differ from normal spiral galaxies in that the arms of the galaxy do not spiral all the way into the center, but are connected to the two ends of a straight bar of stars containing the nucleus at its center. At Hubble's resolution, a myriad of fine details, some of which have never before been seen, is seen throughout the galaxy's arms, disk, bulge, and nucleus. Blue and red supergiant stars, star clusters, and star - forming regions are well resolved across the spiral arms, and dust lanes trace out fine structures in the disk and bar. Numerous more distant galaxies are visible in the background, and are seen even through the densest regio

PIX4609752

Helen Joseph, Brave fighter of Racism - Helen was born in 1905, in Britain. She beca…, 1956 (photo)

Helen Joseph, Brave fighter of Racism - Helen was born in 1905, in Britain. She beca…, 1956 (photo)

AMD8679322

Bushman rock paintings, at Kagga Kamma Reserve, South Africa. March 29, 2009. The Bushman rock paintings, dating back to thousands of years ago, are one of South Africas greatest cultural treasures. Some 20, 000 individual rock paintings have been recorded at 500 different cave and overhang sites. The paintings range from animals (mainly elands) to humans, therianthropes to ox-wagons and mounted men with weapons. The Kagga Kamma Private Game Reserve, lying in an untouched wilderness, south of Cederberg mountains, has hundreds of Bushman rock paintings up to 6000 years old and is a unique safari in South Africa. (photo)

Bushman rock paintings, at Kagga Kamma Reserve, South Africa. March 29, 2009. The Bushman rock paintings, dating back to thousands of years ago, are one of South Africas greatest cultural treasures. Some 20, 000 individual rock paintings have been recorded at 500 different cave and overhang sites. The paintings range from animals (mainly elands) to humans, therianthropes to ox-wagons and mounted men with weapons. The Kagga Kamma Private Game Reserve, lying in an untouched wilderness, south of Cederberg mountains, has hundreds of Bushman rock paintings up to 6000 years old and is a unique safari in South Africa. (photo)

UIG800916

There are more than 175 factories employing about 80, 000 workers, 80% of whom are females in the Chittagong Export Processing Zone (CEPZ) in Chittagong, Bangladesh. The ready made garment industry has been the key export division and the chief source of foreign exchange for about 25 years. Not only does the country generate about 5 billion dollars worth of products each year but the industry itself provides employment to about 3 million workers throughout the country. Chittagong, Bangladesh. November 22, 2008. . (photo)

There are more than 175 factories employing about 80, 000 workers, 80% of whom are females in the Chittagong Export Processing Zone (CEPZ) in Chittagong, Bangladesh. The ready made garment industry has been the key export division and the chief source of foreign exchange for about 25 years. Not only does the country generate about 5 billion dollars worth of products each year but the industry itself provides employment to about 3 million workers throughout the country. Chittagong, Bangladesh. November 22, 2008. . (photo)

UIG801718

There are more than 175 factories employing about 80, 000 workers, 80% of whom are females in the Chittagong Export Processing Zone (CEPZ) in Chittagong, Bangladesh. The ready made garment industry has been the key export division and the chief source of foreign exchange for about 25 years. Not only does the country generate about 5 billion dollars worth of products each year but the industry itself provides employment to about 3 million workers throughout the country. Chittagong, Bangladesh. November 22, 2008. . (photo)

There are more than 175 factories employing about 80, 000 workers, 80% of whom are females in the Chittagong Export Processing Zone (CEPZ) in Chittagong, Bangladesh. The ready made garment industry has been the key export division and the chief source of foreign exchange for about 25 years. Not only does the country generate about 5 billion dollars worth of products each year but the industry itself provides employment to about 3 million workers throughout the country. Chittagong, Bangladesh. November 22, 2008. . (photo)

UIG801719

There are more than 175 factories employing about 80, 000 workers, 80% of whom are females in the Chittagong Export Processing Zone (CEPZ) in Chittagong, Bangladesh. The ready made garment industry has been the key export division and the chief source of foreign exchange for about 25 years. Not only does the country generate about 5 billion dollars worth of products each year but the industry itself provides employment to about 3 million workers throughout the country. Chittagong, Bangladesh. November 22, 2008. (photo)

There are more than 175 factories employing about 80, 000 workers, 80% of whom are females in the Chittagong Export Processing Zone (CEPZ) in Chittagong, Bangladesh. The ready made garment industry has been the key export division and the chief source of foreign exchange for about 25 years. Not only does the country generate about 5 billion dollars worth of products each year but the industry itself provides employment to about 3 million workers throughout the country. Chittagong, Bangladesh. November 22, 2008. (photo)

UIG801721

Helen Joseph, Brave fighter of Racism - Helen was born in 1905, in Britain. She beca…, 1956 (photo)

Helen Joseph, Brave fighter of Racism - Helen was born in 1905, in Britain. She beca…, 1956 (photo)

AMD8679319

Cluster of stars NGC 299 in Toucan - Open cluster NGC 299 in Tucana: NGC 299 is an open cluster located in the galaxy of the Little Magellan Cloud. Image obtained by the Hubble Space Telescope (HST). NGC 299 is an open star cluster located within the Small Magellanic Cloud just under 200 000 light-years away. Open clusters such as this are collections of stars weakly bound by the shackles of gravity, all of which formed from the same massive molecular cloud of gas and dust. Because of this, all the stars have the same age and composition, but vary in their mass because they formed at different positions within the cloud. This unique property not only ensures a spectacular sight when viewed through a sophisticated instrument attached to a telescope such as Hubble's Advanced Camera for Surveys, but gives astronomers a cosmic laboratory in which to study the formation and evolution of stars - a process that is thought to depend strongly on a star's mass

Cluster of stars NGC 299 in Toucan - Open cluster NGC 299 in Tucana: NGC 299 is an open cluster located in the galaxy of the Little Magellan Cloud. Image obtained by the Hubble Space Telescope (HST). NGC 299 is an open star cluster located within the Small Magellanic Cloud just under 200 000 light-years away. Open clusters such as this are collections of stars weakly bound by the shackles of gravity, all of which formed from the same massive molecular cloud of gas and dust. Because of this, all the stars have the same age and composition, but vary in their mass because they formed at different positions within the cloud. This unique property not only ensures a spectacular sight when viewed through a sophisticated instrument attached to a telescope such as Hubble's Advanced Camera for Surveys, but gives astronomers a cosmic laboratory in which to study the formation and evolution of stars - a process that is thought to depend strongly on a star's mass

PIX4580152

Detail of the nebula NGC 3603 in the Carene - Star life cycle in NGC 3603 - In the center of the picture is a cluster of massive young stars formed from the gas surrounding them. Two pillars of gas and dust visible on the right at the top and bottom will one day form other stars, as probably the dark cloud at the top right of the image called Bok's globule. Above the left of the star cluster, an old blue supergiant star, Sher 25, arrives at the end of life. The nebula NGC 3603 is located approximately 20,000 light years from Earth in the southern constellation of Carene. Image obtained by the Hubble Space Telescope. This image made by the Hubble space telescope nicely illustrates the entire stellar life cycle of stars, starting with the Bok globules (dark clouds at the upper right) and giant gaseous pillars, followed by circumstellar disks and progressing to evolved massive stars in the young starburst cluster (center). The blue supergiant star Sher 25 with its ring and bipolar outflow

Detail of the nebula NGC 3603 in the Carene - Star life cycle in NGC 3603 - In the center of the picture is a cluster of massive young stars formed from the gas surrounding them. Two pillars of gas and dust visible on the right at the top and bottom will one day form other stars, as probably the dark cloud at the top right of the image called Bok's globule. Above the left of the star cluster, an old blue supergiant star, Sher 25, arrives at the end of life. The nebula NGC 3603 is located approximately 20,000 light years from Earth in the southern constellation of Carene. Image obtained by the Hubble Space Telescope. This image made by the Hubble space telescope nicely illustrates the entire stellar life cycle of stars, starting with the Bok globules (dark clouds at the upper right) and giant gaseous pillars, followed by circumstellar disks and progressing to evolved massive stars in the young starburst cluster (center). The blue supergiant star Sher 25 with its ring and bipolar outflow

PIX4619146

Globular cluster M5 in Serpens - Globular cluster M5 in Serpens - This cluster of stars is located about 25,000 light years away from Earth. It is one of the most extensive (165 years - light) and one of the oldest known globular clusters. Globular clusters are generally peoples of very old stars, but here the Hubble space telescope has identified some young stars, blue stragglers. The globular cluster Messier 5, shown here in this NASA/ESA Hubble Space Telescope image, is one of the oldest belonging to the Milky Way. The majority of its stars formed more than 12 billion years ago, but there are some unexpected newcomers on the scene, adding some vitality to this aging population. Stars in globular clusters form in the same stellar nursery and grow old together. The most massive stars age quickly, exhausting their fuel supply in less than a million years, and end their lives in spectacular supernovae explosions. This process should have left the ancient cluster Messier 5 with only old,

Globular cluster M5 in Serpens - Globular cluster M5 in Serpens - This cluster of stars is located about 25,000 light years away from Earth. It is one of the most extensive (165 years - light) and one of the oldest known globular clusters. Globular clusters are generally peoples of very old stars, but here the Hubble space telescope has identified some young stars, blue stragglers. The globular cluster Messier 5, shown here in this NASA/ESA Hubble Space Telescope image, is one of the oldest belonging to the Milky Way. The majority of its stars formed more than 12 billion years ago, but there are some unexpected newcomers on the scene, adding some vitality to this aging population. Stars in globular clusters form in the same stellar nursery and grow old together. The most massive stars age quickly, exhausting their fuel supply in less than a million years, and end their lives in spectacular supernovae explosions. This process should have left the ancient cluster Messier 5 with only old,

PIX4564490

Jet of the Galaxy Centaurus A (NGC 5128) seen in X-rays - Galaxy Centaurus A X - ray jet - View in false colours of a 30 000-year long jet - light that escapes from the nucleus of the Galaxy Centaurus A where a massive black hole is suspected. The galaxy NGC 5128 is located about 13 million light years away from Earth. Image obtained by the Chandra Space Telescope in May 2000. Chandra space telescope detects a jet emanating from the NGC 5128 core and numerous point - like X - ray sources, all bathed in diffuse X - rays produced by several - million - degree gas that fills the galaxy. It is believed that most of these sources are X - ray binaries in which a neutron star or stellar - sized black hole is accreting matter from a nearby companion star. The Cen A image was created from Chandra observations taken on December 5, 1999 and May 17, 2000

Jet of the Galaxy Centaurus A (NGC 5128) seen in X-rays - Galaxy Centaurus A X - ray jet - View in false colours of a 30 000-year long jet - light that escapes from the nucleus of the Galaxy Centaurus A where a massive black hole is suspected. The galaxy NGC 5128 is located about 13 million light years away from Earth. Image obtained by the Chandra Space Telescope in May 2000. Chandra space telescope detects a jet emanating from the NGC 5128 core and numerous point - like X - ray sources, all bathed in diffuse X - rays produced by several - million - degree gas that fills the galaxy. It is believed that most of these sources are X - ray binaries in which a neutron star or stellar - sized black hole is accreting matter from a nearby companion star. The Cen A image was created from Chandra observations taken on December 5, 1999 and May 17, 2000

PIX4612176

Ireland between Londonderry and Dublin, 1595 (linen, paper)

Ireland between Londonderry and Dublin, 1595 (linen, paper)

Thomas, John (16th century)

MMM7339818

Globular cluster NGC 6752 - Stars in globular cluster NGC 6752 - Image of the center of the globular cluster NGC 6752 located in the constellation Peacock. The Hubble Space Telescope (HST) observed blue straggler. NGC 6752 is a globular cluster, and at over 10 billion years old is one the most ancient collections of stars known. It has been blazing for well over twice as long as our Solar System has existed. NGC 6752 contains a high number of blue straggler”” stars, some of which are visible in this image. These stars display characteristics of stars younger than their neighbours, despite models suggesting that most of the stars within globular clusters should have formed at approximately the same time. Their origin is therefore something of a mystery. Studies of NGC 6752 may shed light on this situation. It appears that a very high number - - up to 38% - - of the stars within its core region are binary systems. Collisions between stars in this turbulent area could produce the blue str

Globular cluster NGC 6752 - Stars in globular cluster NGC 6752 - Image of the center of the globular cluster NGC 6752 located in the constellation Peacock. The Hubble Space Telescope (HST) observed blue straggler. NGC 6752 is a globular cluster, and at over 10 billion years old is one the most ancient collections of stars known. It has been blazing for well over twice as long as our Solar System has existed. NGC 6752 contains a high number of blue straggler”” stars, some of which are visible in this image. These stars display characteristics of stars younger than their neighbours, despite models suggesting that most of the stars within globular clusters should have formed at approximately the same time. Their origin is therefore something of a mystery. Studies of NGC 6752 may shed light on this situation. It appears that a very high number - - up to 38% - - of the stars within its core region are binary systems. Collisions between stars in this turbulent area could produce the blue str

PIX4565015

Globular cluster M72 in Aquarius - Globular cluster M72 in Aquarius - M72 (NGC 6981) is a cluster of stars located about 50,000 years from Earth. Image obtained by the Hubble Space Telescope. This rich collection of scattered stars, known as Messier 72, is actually a globular cluster, an ancient spherical collection of old stars packed much closer together at its centre. As well as huge numbers of stars in the cluster itself the picture also captures the images of many much more distant galaxies seen between and around the cluster stars. English astronomer Pierre Megchain discovered this rich cluster in August of 1780, but we take Messier 72's most common name from Mechain's colleague Charles Messier, who recorded it as the 72nd entry in his famous catalog of comet - like objects just two months later. This globular cluster lies in the constellation of Aquarius (the Water Bearer) about 50 000 light - years from Earth. This image was taken with the Wide Field Channel of the Advanced Cam

Globular cluster M72 in Aquarius - Globular cluster M72 in Aquarius - M72 (NGC 6981) is a cluster of stars located about 50,000 years from Earth. Image obtained by the Hubble Space Telescope. This rich collection of scattered stars, known as Messier 72, is actually a globular cluster, an ancient spherical collection of old stars packed much closer together at its centre. As well as huge numbers of stars in the cluster itself the picture also captures the images of many much more distant galaxies seen between and around the cluster stars. English astronomer Pierre Megchain discovered this rich cluster in August of 1780, but we take Messier 72's most common name from Mechain's colleague Charles Messier, who recorded it as the 72nd entry in his famous catalog of comet - like objects just two months later. This globular cluster lies in the constellation of Aquarius (the Water Bearer) about 50 000 light - years from Earth. This image was taken with the Wide Field Channel of the Advanced Cam

PIX4565111

Nebula N159 in the Great Magellan Cloud - N159 star forming region in Large Magellanic Cloud (LMC): N159 is a star-forming region located in the galaxy of the Great Magellan Cloud. Image obtained by the Hubble Space Telescope (HST) - This shot from the NASA/ESA Hubble Space Telescope shows a maelstrom of glowing gas and dark dust within one of the Milky Way's satellite galaxies, the Large Magellanic Cloud (LMC). This stormy scene shows a stellar nursery known as N159, an HII region over 150 light-years across. N159 contains many hot young stars. These stars are emitting intense ultraviolet light, which causes nearby hydrogen gas to glow, and torrential stellar winds, which are carving out ridges, arcs, and filaments from the surrounding material. At the heart of this cosmic cloud lies the Papillon Nebula, a butterfly-shaped region of nebulosity. This small, dense object is classified as a High-Excitation Blob, and is thought to be tightly linked to the early stages of massive star form

Nebula N159 in the Great Magellan Cloud - N159 star forming region in Large Magellanic Cloud (LMC): N159 is a star-forming region located in the galaxy of the Great Magellan Cloud. Image obtained by the Hubble Space Telescope (HST) - This shot from the NASA/ESA Hubble Space Telescope shows a maelstrom of glowing gas and dark dust within one of the Milky Way's satellite galaxies, the Large Magellanic Cloud (LMC). This stormy scene shows a stellar nursery known as N159, an HII region over 150 light-years across. N159 contains many hot young stars. These stars are emitting intense ultraviolet light, which causes nearby hydrogen gas to glow, and torrential stellar winds, which are carving out ridges, arcs, and filaments from the surrounding material. At the heart of this cosmic cloud lies the Papillon Nebula, a butterfly-shaped region of nebulosity. This small, dense object is classified as a High-Excitation Blob, and is thought to be tightly linked to the early stages of massive star form

PIX4620798

Southern Crown Nebula - The tail of the CRA reflection nebula - R Coronae Australis is a region of star formations visible in the southern hemisphere. It is located about 500 light years away from Earth. On the right, the globular cluster NGC 6723, located 30 000 light years from Earth in Sagittarius. Image made with the 1.2m Telescope of Schmidt UK from Siding Spring. Corona Australis (the southern crown, CRA) is in the far southern sky but visible from the southern states of the USA. The constellation is small but distinctive. The conspicuous globular cluster NGC 6723 is at the western (right) edge of the photograph, but it is in Sagittarius, and is about 30,000 light years distant. Our picture is about 4.5 degrees across and the extremely faint Corona Australis nebula meanders along the Sgr - CRA border nebula in the same E - W direction. Almost all the nebulosity here is starlight, reflected from minute grains of dust, some of which gather into darker condensations ('molecular clou

Southern Crown Nebula - The tail of the CRA reflection nebula - R Coronae Australis is a region of star formations visible in the southern hemisphere. It is located about 500 light years away from Earth. On the right, the globular cluster NGC 6723, located 30 000 light years from Earth in Sagittarius. Image made with the 1.2m Telescope of Schmidt UK from Siding Spring. Corona Australis (the southern crown, CRA) is in the far southern sky but visible from the southern states of the USA. The constellation is small but distinctive. The conspicuous globular cluster NGC 6723 is at the western (right) edge of the photograph, but it is in Sagittarius, and is about 30,000 light years distant. Our picture is about 4.5 degrees across and the extremely faint Corona Australis nebula meanders along the Sgr - CRA border nebula in the same E - W direction. Almost all the nebulosity here is starlight, reflected from minute grains of dust, some of which gather into darker condensations ('molecular clou

PIX4620260

People Washing And Putting Dry Clothes Under A Painted Bridge, Madurai, India, 2008 (photo)

People Washing And Putting Dry Clothes Under A Painted Bridge, Madurai, India, 2008 (photo)

Eric Lafforgue

LFG7355807

Detail of the globular cluster 47 Toucan - Starfield in the globular cluster 47 Tucanae, NGC 104 - The globular cluster 47 Toucan (or NGC 104) is visible to the naked eye from the southern hemisphere. Located about 15000 years ago - light it contains several million stars, some of which are among the older stars known today. This image obtained by the Hubble Space Telescope shows a detail of this cluster near its center; about 35,000 stars are visible. This image shows the Hubble telescope's close - up look at a swarm of 35, 000 stars near the club's central region. The stars are tightly packed together: They are much closer together than our Sun and its closest stars. The picture, taken by the Wide Field and Planetary Camera 2, depicts the stars' natural colors and tells scientists about their composition and age. For example, the red stars denote bright red giants nearing the end of their lives; the more common yellow stars are similar to our middle - aged Sun

Detail of the globular cluster 47 Toucan - Starfield in the globular cluster 47 Tucanae, NGC 104 - The globular cluster 47 Toucan (or NGC 104) is visible to the naked eye from the southern hemisphere. Located about 15000 years ago - light it contains several million stars, some of which are among the older stars known today. This image obtained by the Hubble Space Telescope shows a detail of this cluster near its center; about 35,000 stars are visible. This image shows the Hubble telescope's close - up look at a swarm of 35, 000 stars near the club's central region. The stars are tightly packed together: They are much closer together than our Sun and its closest stars. The picture, taken by the Wide Field and Planetary Camera 2, depicts the stars' natural colors and tells scientists about their composition and age. For example, the red stars denote bright red giants nearing the end of their lives; the more common yellow stars are similar to our middle - aged Sun

PIX4564266

Open cluster Westerlund 1 in the Altar - Open cluster Westerlund 1 in Ara - The open cluster Westerlund 1 is located about 16,000 years - light in the southern constellation of the Altar. It contains hundreds of very young massive stars as well as the supergiant red star W26. Image obtained by the VST telescope in Chile. This exceptionally bright cluster lies about 16 000 light - years from Earth in the southern constellation of Ara (The Altar). It contains hundreds of very massive and brilliant stars, all of which are just a few million years old - - babies by stellar standards. But our view of this cluster is hampered by gas and dust that prevents most of the visible light from the cluster's stars from getting to Earth. Around one of the stars - - known as W26, a red supergiant and possibly the biggest star known - - astronomers have discovered clouds of glowing hydrogen gas, shown as green features in this new image. Such glowing clouds around massive stars are very rare, and are ev

Open cluster Westerlund 1 in the Altar - Open cluster Westerlund 1 in Ara - The open cluster Westerlund 1 is located about 16,000 years - light in the southern constellation of the Altar. It contains hundreds of very young massive stars as well as the supergiant red star W26. Image obtained by the VST telescope in Chile. This exceptionally bright cluster lies about 16 000 light - years from Earth in the southern constellation of Ara (The Altar). It contains hundreds of very massive and brilliant stars, all of which are just a few million years old - - babies by stellar standards. But our view of this cluster is hampered by gas and dust that prevents most of the visible light from the cluster's stars from getting to Earth. Around one of the stars - - known as W26, a red supergiant and possibly the biggest star known - - astronomers have discovered clouds of glowing hydrogen gas, shown as green features in this new image. Such glowing clouds around massive stars are very rare, and are ev

PIX4569073

Nebula N90 in the Little Magellan Cloud - N90 nebula in the Small Magellanic Cloud - View of nebula N90 in the Little Magellan Cloud, a galaxy next to our located 200 000 years - light from Earth. At the heart of this star-forming region is the cluster of stars NGC 602. These young stars have emerge from their cocoon of gas blowing the surrounding matter; the gas pillars pointing towards these stars are a sign of this erosion. In the dark clouds, other stars are forming. In the background, many galaxies are visible. Composite images obtained by the Hubble Space Telescope in July 2004. N90 is one of the star - forming regions in the Small Magellanic Cloud approximately 200,000 light - years away from the Earth.. The rich populations of infant stars found here enable astronomers to examine star forming processes in an environment that is very different from that in our own Milky Way. The high energy radiation blazing out from the hot young stars in N90 is eroding the outer portions of th

Nebula N90 in the Little Magellan Cloud - N90 nebula in the Small Magellanic Cloud - View of nebula N90 in the Little Magellan Cloud, a galaxy next to our located 200 000 years - light from Earth. At the heart of this star-forming region is the cluster of stars NGC 602. These young stars have emerge from their cocoon of gas blowing the surrounding matter; the gas pillars pointing towards these stars are a sign of this erosion. In the dark clouds, other stars are forming. In the background, many galaxies are visible. Composite images obtained by the Hubble Space Telescope in July 2004. N90 is one of the star - forming regions in the Small Magellanic Cloud approximately 200,000 light - years away from the Earth.. The rich populations of infant stars found here enable astronomers to examine star forming processes in an environment that is very different from that in our own Milky Way. The high energy radiation blazing out from the hot young stars in N90 is eroding the outer portions of th

R. Gendler

PIX4620932

Spiral galaxy NGC 6503 in the Dragon - Spiral galaxy NGC 6503 in Draco - The dwarf spiral galaxy NGC 6503 is located about 17 million years ago - light from Earth. It spans 30,000 light years and shows many star-forming regions. Image obtained by the Hubble Space Telescope. Fresh starbirth infuses the galaxy NGC 6503 with a vital pink glow in this image from the NASA/ESA Hubble Space Telescope. This galaxy, a smaller version of the Milky Way, is perched near a great void in space where few other galaxies reside. This new image from Hubble's Advanced Camera for Surveys displays, with particular clarity, the pink - colored puffs marking where stars have recently formed in NGC 6503's swirling spiral arms. Although structurally similar to the Milky Way, the disc of NGC 6503 spans just 30 000 light - years, or just about a third of the size of the Milky Way, leading astronomers to classify NGC 6503 as a dwarf spiral galaxy. NGC 6503 lies approximately 17 million light - years away in the co

Spiral galaxy NGC 6503 in the Dragon - Spiral galaxy NGC 6503 in Draco - The dwarf spiral galaxy NGC 6503 is located about 17 million years ago - light from Earth. It spans 30,000 light years and shows many star-forming regions. Image obtained by the Hubble Space Telescope. Fresh starbirth infuses the galaxy NGC 6503 with a vital pink glow in this image from the NASA/ESA Hubble Space Telescope. This galaxy, a smaller version of the Milky Way, is perched near a great void in space where few other galaxies reside. This new image from Hubble's Advanced Camera for Surveys displays, with particular clarity, the pink - colored puffs marking where stars have recently formed in NGC 6503's swirling spiral arms. Although structurally similar to the Milky Way, the disc of NGC 6503 spans just 30 000 light - years, or just about a third of the size of the Milky Way, leading astronomers to classify NGC 6503 as a dwarf spiral galaxy. NGC 6503 lies approximately 17 million light - years away in the co

PIX4612940

Spiral galaxy NGC 406 in Toucan - Spiral galaxy NGC 406 in Tucana - NGC 406 is a spiral galaxy located at a distance of about 65 million light years in the southern constellation of Toucan. Image obtained by the Hubble Space Telescope. The spiral galaxy NGC 406 was discovered in 1834 by John Herschel and is here imaged in great detail by the NASA/ESA Hubble Space Telescope. Located some 65 million light - years away, in the southern constellation of Tucana (the Toucan), NGC 406 is about 60 000 light - years across, roughly half the diameter of our galaxy, the Milky Way. In a moderate - sized amateur telescope NGC 406 would appear as a faint hazy blob, like thousands of others across the sky, and none of the spectacular fine detail in the Hubble picture could be made out. In this image the galaxy exhibits spiral arms that are mainly populated by young, massive, bluish stars and crossed by dark dust lanes. As is typically observed in this kind of spiral galaxy, the yellowish central bulg

Spiral galaxy NGC 406 in Toucan - Spiral galaxy NGC 406 in Tucana - NGC 406 is a spiral galaxy located at a distance of about 65 million light years in the southern constellation of Toucan. Image obtained by the Hubble Space Telescope. The spiral galaxy NGC 406 was discovered in 1834 by John Herschel and is here imaged in great detail by the NASA/ESA Hubble Space Telescope. Located some 65 million light - years away, in the southern constellation of Tucana (the Toucan), NGC 406 is about 60 000 light - years across, roughly half the diameter of our galaxy, the Milky Way. In a moderate - sized amateur telescope NGC 406 would appear as a faint hazy blob, like thousands of others across the sky, and none of the spectacular fine detail in the Hubble picture could be made out. In this image the galaxy exhibits spiral arms that are mainly populated by young, massive, bluish stars and crossed by dark dust lanes. As is typically observed in this kind of spiral galaxy, the yellowish central bulg

PIX4609197

Calloused Hands Of A Blacksmith In Pondicherry, India, 2008 (photo)

Calloused Hands Of A Blacksmith In Pondicherry, India, 2008 (photo)

Eric Lafforgue

LFG7355608

Squatting Blacksmith Forging Tools Near Pondicherry, India, 2008 (photo)

Squatting Blacksmith Forging Tools Near Pondicherry, India, 2008 (photo)

Eric Lafforgue

LFG7355722

Barree spiral galaxy NGC 2146 in the Giraffe - Barred spiral galaxy NGC 2146 in Camelopardalis - NGC 2146 is a barree spiral galaxy located about 70 million years ago - light from Earth in the constellation Giraffe (Camelopardalis). Image obtained by the Hubble Space Telescope (HST). NGC 2146 is classified as a barred spiral due to its shape, but the most distinctive feature is the dusty spiral arm that has looped in front of the galaxy's core as seen from our perspective. The forces required to pull this structure out of its natural shape and twist it up to 45 degrees are colossal. The most likely explanation is that a neighbouring galaxy is gravitationally perturbing it and distorting the orbits of many of NGC 2146's stars. It is probable that we are currently witnessing the end stages of a process which has been occurring for tens of millions of years. NCG 2146 is undergoing intense bouts of star formation, to such an extent that it is referred to as a starburst galaxy. This is a co

Barree spiral galaxy NGC 2146 in the Giraffe - Barred spiral galaxy NGC 2146 in Camelopardalis - NGC 2146 is a barree spiral galaxy located about 70 million years ago - light from Earth in the constellation Giraffe (Camelopardalis). Image obtained by the Hubble Space Telescope (HST). NGC 2146 is classified as a barred spiral due to its shape, but the most distinctive feature is the dusty spiral arm that has looped in front of the galaxy's core as seen from our perspective. The forces required to pull this structure out of its natural shape and twist it up to 45 degrees are colossal. The most likely explanation is that a neighbouring galaxy is gravitationally perturbing it and distorting the orbits of many of NGC 2146's stars. It is probable that we are currently witnessing the end stages of a process which has been occurring for tens of millions of years. NCG 2146 is undergoing intense bouts of star formation, to such an extent that it is referred to as a starburst galaxy. This is a co

PIX4609999

Blacksmith Holding His Tools Near A Flame In Pondicherry, India, 2008 (photo)

Blacksmith Holding His Tools Near A Flame In Pondicherry, India, 2008 (photo)

Eric Lafforgue

LFG7355721

Chat

Chat

IMO2255738

Spiral Galaxy M66 in the Lion - Spiral galaxy M66 in Leo - M66 (NGC 3627) is a spiral galaxy located at a distance of about 35 million years - light. M66, with its neighbors M65 and NGC 3628, forms a remarkable triplet of galaxies, called the Lion Triplet or the M66 Group. Image obtained by the Hubble Space Telescope. The unusual spiral galaxy, Messier 66, is located at a distance of about 35 million light - years in the constellation of Leo. Together with Messier 65 and NGC 3628, Messier 66 is one third of the Leo Triplet, a trio of interacting spiral galaxies, part of the larger Messier 66 group. Messier 66 wins out in size over its fellow triplets - - it is about 100 000 light - years across. Messier 66 is the proud owner of exclusive asymmetric spiral arms which seem to climb above the galaxy's main disc and an apparently displaced nucleus. This asymmetry is unusual; most often, dense waves of gas, dust and newly born stars wind about the galaxy's centre in a symmetric way. Astrono

Spiral Galaxy M66 in the Lion - Spiral galaxy M66 in Leo - M66 (NGC 3627) is a spiral galaxy located at a distance of about 35 million years - light. M66, with its neighbors M65 and NGC 3628, forms a remarkable triplet of galaxies, called the Lion Triplet or the M66 Group. Image obtained by the Hubble Space Telescope. The unusual spiral galaxy, Messier 66, is located at a distance of about 35 million light - years in the constellation of Leo. Together with Messier 65 and NGC 3628, Messier 66 is one third of the Leo Triplet, a trio of interacting spiral galaxies, part of the larger Messier 66 group. Messier 66 wins out in size over its fellow triplets - - it is about 100 000 light - years across. Messier 66 is the proud owner of exclusive asymmetric spiral arms which seem to climb above the galaxy's main disc and an apparently displaced nucleus. This asymmetry is unusual; most often, dense waves of gas, dust and newly born stars wind about the galaxy's centre in a symmetric way. Astrono

PIX4610836

Globular cluster M54 in Sagittarius - Globular cluster M54 in Sagittarius - The globular cluster M54 photographed by the Hubble space telescope (HST). M54 resides about 90,000 light years from Earth, in the dwarf galaxy of Sagittarius. The object shown in this beautiful Hubble image, dubbed Messier 54, could be just another globular cluster, but this dense and faint group of stars was in fact the first globular cluster found that is outside our galaxy. Discovered by the famous astronomer Charles Messier in 1778, Messier 54 belongs to a satellite of the Milky Way called the Sagittarius Dwarf Elliptical Galaxy. Messier had no idea of the significance of his discovery at the time, and it wasn't until over two centuries later, in 1994, that astronomers found Messier 54 to be part of the miniature galaxy and not our own. Current estimates indicate that the Sagittarius dwarf, and hence the cluster, is situated almost 90 000 light - years away - - more than three times as far from the centre

Globular cluster M54 in Sagittarius - Globular cluster M54 in Sagittarius - The globular cluster M54 photographed by the Hubble space telescope (HST). M54 resides about 90,000 light years from Earth, in the dwarf galaxy of Sagittarius. The object shown in this beautiful Hubble image, dubbed Messier 54, could be just another globular cluster, but this dense and faint group of stars was in fact the first globular cluster found that is outside our galaxy. Discovered by the famous astronomer Charles Messier in 1778, Messier 54 belongs to a satellite of the Milky Way called the Sagittarius Dwarf Elliptical Galaxy. Messier had no idea of the significance of his discovery at the time, and it wasn't until over two centuries later, in 1994, that astronomers found Messier 54 to be part of the miniature galaxy and not our own. Current estimates indicate that the Sagittarius dwarf, and hence the cluster, is situated almost 90 000 light - years away - - more than three times as far from the centre

PIX4565011

Dresden, historical, GDR, Film Theatre Round Cinema Prague Street, 25 …, 1978 (photo)

Dresden, historical, GDR, Film Theatre Round Cinema Prague Street, 25 …, 1978 (photo)

Sächsische Zeitung

IMO8755019

Homo sapiens crania

Homo sapiens crania

NHM1453618

Homo erectus (Sangiran 17)

Homo erectus (Sangiran 17)

NHM1454757

Globular cluster M55 in Sagittarius - Globular cluster M55 in Sagittarius - Star cluster located about 17,000 years away from Earth. Star cluster located at about 17,000 light years away

Globular cluster M55 in Sagittarius - Globular cluster M55 in Sagittarius - Star cluster located about 17,000 years away from Earth. Star cluster located at about 17,000 light years away

Vincent Toporenko

PIX4565045

NGC 6541 in the Southern Crown - Globular cluster NGC 6541 in Corona Australis - This cluster of stars is located about 23,000 years from Earth. Globular cluster located at about 23,000 light years away

NGC 6541 in the Southern Crown - Globular cluster NGC 6541 in Corona Australis - This cluster of stars is located about 23,000 years from Earth. Globular cluster located at about 23,000 light years away

Vincent Toporenko

PIX4564884

Trifide nebula (M20) in the constellation Sagittarius: View of the Trifide nebula (M20/NGC 6514) located in the constellation Sagittarius between 5000 and 10,000 light years from Earth. Measuring some forty light years across, this nebula contains enough gas to make many thousands of suns. Trifid is located in Sagittarius constellation between 5000 and 10,000 light-years away

Trifide nebula (M20) in the constellation Sagittarius: View of the Trifide nebula (M20/NGC 6514) located in the constellation Sagittarius between 5000 and 10,000 light years from Earth. Measuring some forty light years across, this nebula contains enough gas to make many thousands of suns. Trifid is located in Sagittarius constellation between 5000 and 10,000 light-years away

Sebastian Voltmer

PIX4619532

Neanderthal man - Neanderthal man - Reconstitution of the face of the Neanderthal man (Homo neanderthalensis). The Neanderthals lived in Europe and Western Asia in the Middle Paleolithic, between about 250,000 and 28,000 years BC. Portrait of a Neanderthal man (Homo neanderthalensis). This hominid inhabited Europe and parts of western Asia between 250,000 and 28,000 years ago

Neanderthal man - Neanderthal man - Reconstitution of the face of the Neanderthal man (Homo neanderthalensis). The Neanderthals lived in Europe and Western Asia in the Middle Paleolithic, between about 250,000 and 28,000 years BC. Portrait of a Neanderthal man (Homo neanderthalensis). This hominid inhabited Europe and parts of western Asia between 250,000 and 28,000 years ago

Gregoire Cirade

PIX4675718

Man of Neanderthal - Neanderthal man - Scene of daily life of a group of Neanderthalians (Homo neanderthalensis). The Neanderthal Man lived in Europe and Western Asia in Middle Paleolithic, between about 250,000 and 28,000 years BC. Everyday life of Neanderthal men (Homo neanderthalensis). This hominid inhabited Europe and parts of western Asia between 250,000 and 28,000 years ago

Man of Neanderthal - Neanderthal man - Scene of daily life of a group of Neanderthalians (Homo neanderthalensis). The Neanderthal Man lived in Europe and Western Asia in Middle Paleolithic, between about 250,000 and 28,000 years BC. Everyday life of Neanderthal men (Homo neanderthalensis). This hominid inhabited Europe and parts of western Asia between 250,000 and 28,000 years ago

Gregoire Cirade

PIX4675757

Neanderthal man - Neanderthal man - Group of Neanderthal men (Homo neanderthalensis) hunting. The Neanderthals lived in Europe and Western Asia in the Middle Paleolithic, between about 250,000 and 28,000 years BC. A tribe of Neanderthal men (Homo neanderthalensis) hunting. This hominid inhabited Europe and parts of western Asia between 250,000 and 28,000 years ago

Neanderthal man - Neanderthal man - Group of Neanderthal men (Homo neanderthalensis) hunting. The Neanderthals lived in Europe and Western Asia in the Middle Paleolithic, between about 250,000 and 28,000 years BC. A tribe of Neanderthal men (Homo neanderthalensis) hunting. This hominid inhabited Europe and parts of western Asia between 250,000 and 28,000 years ago

Gregoire Cirade

PIX4675747

Globular cluster M12 in Ophiuchus - Globular cluster M12 in Ophiuchus - M12 (NGC 6218) is a cluster of stars located about 16,000 years from Earth. M12 (NGC 6218) is a star cluster located at about 16,000 light years away

Globular cluster M12 in Ophiuchus - Globular cluster M12 in Ophiuchus - M12 (NGC 6218) is a cluster of stars located about 16,000 years from Earth. M12 (NGC 6218) is a star cluster located at about 16,000 light years away

Jim Misti

PIX4564690

Globular cluster M3 in Hunting Dogs - Globular cluster M3 in Canes Venatici - This cluster contains about 500,000 stars and is located 100,000 years - light from Earth. This globular cluster is about 100,000 light - years from us and contains approximately 555,000 stars

Globular cluster M3 in Hunting Dogs - Globular cluster M3 in Canes Venatici - This cluster contains about 500,000 stars and is located 100,000 years - light from Earth. This globular cluster is about 100,000 light - years from us and contains approximately 555,000 stars

PIX4564461

Globular cluster M3 in Hunting Dogs - Globular cluster M3 in Canes Venatici - This cluster contains about 500,000 stars and is located 100,000 years - light from Earth. This globular cluster is about 100,000 light - years from us and contains approximately 555,000 stars

Globular cluster M3 in Hunting Dogs - Globular cluster M3 in Canes Venatici - This cluster contains about 500,000 stars and is located 100,000 years - light from Earth. This globular cluster is about 100,000 light - years from us and contains approximately 555,000 stars

Jim Misti

PIX4564462

A Slave Kaffle, from 'Narrative of Travels in Northern Africa in the Years 1818-19 and 1820', engraved by Denis Dighton (1792-1827) published 1821 (colour litho)

A Slave Kaffle, from 'Narrative of Travels in Northern Africa in the Years 1818-19 and 1820', engraved by Denis Dighton (1792-1827) published 1821 (colour litho)

Lyon, Captain George Francis (1795-1832) (after)

STC209624

Globular cluster M70 in Sagittarius - Globular cluster M70 in Sagittarius - Star cluster located about 29,300 years - light from Earth. Star cluster located at about 29,000 light years away

Globular cluster M70 in Sagittarius - Globular cluster M70 in Sagittarius - Star cluster located about 29,300 years - light from Earth. Star cluster located at about 29,000 light years away

Vincent Toporenko

PIX4564945

Globular cluster M13 - Hercules cluster - The Great Globular Cluster in Hercules M13 - M13 (NGC 6205) extends for about 150 years - light and is 22,000 years - light from Earth in the constellation Hercules. M13 (NGC 6205) appearing in the constellation Ophiuchus at approximately 22,000 light - years away and about 150 light - years across

Globular cluster M13 - Hercules cluster - The Great Globular Cluster in Hercules M13 - M13 (NGC 6205) extends for about 150 years - light and is 22,000 years - light from Earth in the constellation Hercules. M13 (NGC 6205) appearing in the constellation Ophiuchus at approximately 22,000 light - years away and about 150 light - years across

Jim Misti

PIX4564654

President Bill Clinton - Affirmative Action Speech, 1995

President Bill Clinton - Affirmative Action Speech, 1995

BOF6286734

Globular cluster M13 - Hercules cluster - The Great Globular Cluster in Hercules M13 - M13 (NGC6205), extends for about 150 years - light and is 22,000 years - light from Earth in the constellation of Hercules. M13 (NGC 6205) in the Hercules constellation has a diameter of about 150 light - years and is 22,000 light - years away from Earth

Globular cluster M13 - Hercules cluster - The Great Globular Cluster in Hercules M13 - M13 (NGC6205), extends for about 150 years - light and is 22,000 years - light from Earth in the constellation of Hercules. M13 (NGC 6205) in the Hercules constellation has a diameter of about 150 light - years and is 22,000 light - years away from Earth

R. Gendler

PIX4564639

Globular cluster M13 - Hercules cluster - The Great Globular Cluster in Hercules M13 - M13 (NGC6205), extends for about 150 years - light and is 22,000 years - light from Earth in the constellation of Hercules. M13 (NGC 6205) in the Hercules constellation has a diameter of about 150 light - years and is 22,000 light - years away from Earth

Globular cluster M13 - Hercules cluster - The Great Globular Cluster in Hercules M13 - M13 (NGC6205), extends for about 150 years - light and is 22,000 years - light from Earth in the constellation of Hercules. M13 (NGC 6205) in the Hercules constellation has a diameter of about 150 light - years and is 22,000 light - years away from Earth

E Mouquet

PIX4564624

Globular cluster M13 - Hercules cluster - The Great Globular Cluster in Hercules M13 - M13 (NGC6205), extends for about 150 years - light and is 22,000 years - light from Earth in the constellation of Hercules. M13 (NGC 6205) in the Hercules constellation has a diameter of about 150 light - years and is 22,000 light - years away from Earth

Globular cluster M13 - Hercules cluster - The Great Globular Cluster in Hercules M13 - M13 (NGC6205), extends for about 150 years - light and is 22,000 years - light from Earth in the constellation of Hercules. M13 (NGC 6205) in the Hercules constellation has a diameter of about 150 light - years and is 22,000 light - years away from Earth

E Mouquet

PIX4564635

Globular cluster M28 in Sagittarius - Globular cluster M28 in Sagittarius - The globular cluster M28 (NGC 6626) is located approximately 18,000 light years away from Earth. M28 (NGC 6626) is a globular cluster in the constellation Sagittarius. Slightly elliptical in shape, it is around 80 light - years across and some 18000 light - years away

Globular cluster M28 in Sagittarius - Globular cluster M28 in Sagittarius - The globular cluster M28 (NGC 6626) is located approximately 18,000 light years away from Earth. M28 (NGC 6626) is a globular cluster in the constellation Sagittarius. Slightly elliptical in shape, it is around 80 light - years across and some 18000 light - years away

Jim Misti

PIX4564899

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