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Mars: crater in Myers Valles - Mars: crater in Myers Valles - Mamers Valles is a valley about 1000 km long located in the region of Deuteronilus Mensae, north of Arabia Terra. The image obtained by the Mars Express probe on 5 August 2006 shows a crater at the end of this valley. This circular formation measures about thirty kilometres in diameter and is 1400 metres deep. There are traces of flow of material probably composed of water ice, similar to the relief left by the passage of glaciers on Earth. The darker area could be caused by local erosion or wind-driven material. The High - Resolution Stereo Camera (HRSC) onboard the ESA spacecraft Mars Express obtained images focusing on a depression that displays a crater at the end of the long, winding valley, Mamers Valles. The data was obtained on 5 August 2006 with a ground resolution of approximately 14 m/per pixel. The image is centred at approximately 39* north and 17* east on the planet. The valley of Mamers Valles is approximately

Mars: crater in Myers Valles - Mars: crater in Myers Valles - Mamers Valles is a valley about 1000 km long located in the region of Deuteronilus Mensae, north of Arabia Terra. The image obtained by the Mars Express probe on 5 August 2006 shows a crater at the end of this valley. This circular formation measures about thirty kilometres in diameter and is 1400 metres deep. There are traces of flow of material probably composed of water ice, similar to the relief left by the passage of glaciers on Earth. The darker area could be caused by local erosion or wind-driven material. The High - Resolution Stereo Camera (HRSC) onboard the ESA spacecraft Mars Express obtained images focusing on a depression that displays a crater at the end of the long, winding valley, Mamers Valles. The data was obtained on 5 August 2006 with a ground resolution of approximately 14 m/per pixel. The image is centred at approximately 39* north and 17* east on the planet. The valley of Mamers Valles is approximately

PIX4616090

Remains of supernova SN 1006 - Supernova remnant SN 1006 - Remains of supernova SN 1006 located 7000 years ago - light in the constellation Wolf. This supernova that appeared in 1006 is the result of a white dwarf star that absorbs the matter of a companion star became unstable and eventually exploded. This image is a composite of X-ray images obtained by the Chandra telescope (blue), by Cerro Tololo's 90 cm telescope (yellow) and by the Digitized Sky Survey (orange and light blue), and by the VLA and the Green Bank's telescope radio (red). Just over a thousand years ago, the stellar explosion known as supernova SN 1006 was observed. It was brighter than Venus, and visible during the day for weeks. The brightest supernova ever recorded on Earth, this spectacular light show was documented in China, Japan, Europe, and the Arab world. Astronomers now understand that SN 1006 was caused by a white dwarf star that captured mass from a companion star until the white dwarf became unstable and

Remains of supernova SN 1006 - Supernova remnant SN 1006 - Remains of supernova SN 1006 located 7000 years ago - light in the constellation Wolf. This supernova that appeared in 1006 is the result of a white dwarf star that absorbs the matter of a companion star became unstable and eventually exploded. This image is a composite of X-ray images obtained by the Chandra telescope (blue), by Cerro Tololo's 90 cm telescope (yellow) and by the Digitized Sky Survey (orange and light blue), and by the VLA and the Green Bank's telescope radio (red). Just over a thousand years ago, the stellar explosion known as supernova SN 1006 was observed. It was brighter than Venus, and visible during the day for weeks. The brightest supernova ever recorded on Earth, this spectacular light show was documented in China, Japan, Europe, and the Arab world. Astronomers now understand that SN 1006 was caused by a white dwarf star that captured mass from a companion star until the white dwarf became unstable and

PIX4583213

Galaxy NGC 4631 in Hunting Dogs - Spiral galaxy NGC 4631 in Canes Venatici - Spiral galaxy seen by the slice located at a distance of 30 million years - light. Image obtained by the Hubble Space Telescope (HST). The NASA/ESA Hubble Space Telescope has peered deep into NGC 4631, better known as the Whale Galaxy. Here, a profusion of starbirth lights up the galactic centre, revealing bands of dark material between us and the starburst. The galaxy's activity tapers off in its outer regions where there are fewer stars and less dust, but these are still punctuated by pockets of star formation. The Whale Galaxy is about 30 million light - years away from us in the constellation of Canes Venatici (The Hunting Dogs) and is a spiral galaxy much like the Milky Way. From our vantage point, however, we see the Whale Galaxy edge - on, seeing its glowing centre through dusty spiral arms. The galaxy's central bulge and asymmetric tapering disc have suggested the shape of a whale or a herring to past

Galaxy NGC 4631 in Hunting Dogs - Spiral galaxy NGC 4631 in Canes Venatici - Spiral galaxy seen by the slice located at a distance of 30 million years - light. Image obtained by the Hubble Space Telescope (HST). The NASA/ESA Hubble Space Telescope has peered deep into NGC 4631, better known as the Whale Galaxy. Here, a profusion of starbirth lights up the galactic centre, revealing bands of dark material between us and the starburst. The galaxy's activity tapers off in its outer regions where there are fewer stars and less dust, but these are still punctuated by pockets of star formation. The Whale Galaxy is about 30 million light - years away from us in the constellation of Canes Venatici (The Hunting Dogs) and is a spiral galaxy much like the Milky Way. From our vantage point, however, we see the Whale Galaxy edge - on, seeing its glowing centre through dusty spiral arms. The galaxy's central bulge and asymmetric tapering disc have suggested the shape of a whale or a herring to past

PIX4611784

Mimas, satellite of Saturn, seen by the Cassini probe on 13/02/2010 - Saturn's moon Mimas seen by Cassini spacecraft - February 13 2010 - The Mimas satellite seen in false colours by the Cassini probe on 13 February 2010 has a distance of 16,000 km from the satellite. Color differences reveal differences in terrain nature. Mimas is about 400 km in diameter. At the right centre is the large impact crater Herschel, 130 km wide. Subtle color differences on Saturn's moon Mimas are apparent in this false - color view of Herschel Crater captured by Nasa's Cassini spacecraft during its closest - ever flyby of that moon. The image shows terrain - dependent color variations, particularly the contrast between the bluish materials in and around Herschel Crater (130 kilometers, or 80 miles, wide) and the greenish cast on older, more heavily cratered terrain elsewhere. The origin of the color differences is not yet understood, but may be caused by subtle differences in the surface composition betwe

Mimas, satellite of Saturn, seen by the Cassini probe on 13/02/2010 - Saturn's moon Mimas seen by Cassini spacecraft - February 13 2010 - The Mimas satellite seen in false colours by the Cassini probe on 13 February 2010 has a distance of 16,000 km from the satellite. Color differences reveal differences in terrain nature. Mimas is about 400 km in diameter. At the right centre is the large impact crater Herschel, 130 km wide. Subtle color differences on Saturn's moon Mimas are apparent in this false - color view of Herschel Crater captured by Nasa's Cassini spacecraft during its closest - ever flyby of that moon. The image shows terrain - dependent color variations, particularly the contrast between the bluish materials in and around Herschel Crater (130 kilometers, or 80 miles, wide) and the greenish cast on older, more heavily cratered terrain elsewhere. The origin of the color differences is not yet understood, but may be caused by subtle differences in the surface composition betwe

PIX4625563

Crab Pulsar in Nebula M1 - The Crab pulsar: This false-colored image obtained by the Hubble Space Telescope shows the central region of the Crab Nebula or resides its pulsar. The pulsar is visible in the center of the image. It is a very dense neutron star from the explosion of a massive supernova star. This star quickly rotates on itself developing a powerful magnetic field, emitting beams of light and radio waves. M1 is located about 6000 light-years in the constellation Taurus.. In 1054 AD, during the Song dynasty, Chinese astronomers spotted a bright new star in the night sky. This newcomer turned out to be a violent explosion within the Milky Way, caused by the spectacular death of a star some 1600 light-years away. This explosion created one of the most well-studied and beautiful objects in the night sky - the Crab Nebula. The beautiful result of this cataclysmic Type II supernova is shown here, imaged by the NASA/ESA Hubble Space Telescope's Advanced Camera for Surveys. Unlike m

Crab Pulsar in Nebula M1 - The Crab pulsar: This false-colored image obtained by the Hubble Space Telescope shows the central region of the Crab Nebula or resides its pulsar. The pulsar is visible in the center of the image. It is a very dense neutron star from the explosion of a massive supernova star. This star quickly rotates on itself developing a powerful magnetic field, emitting beams of light and radio waves. M1 is located about 6000 light-years in the constellation Taurus.. In 1054 AD, during the Song dynasty, Chinese astronomers spotted a bright new star in the night sky. This newcomer turned out to be a violent explosion within the Milky Way, caused by the spectacular death of a star some 1600 light-years away. This explosion created one of the most well-studied and beautiful objects in the night sky - the Crab Nebula. The beautiful result of this cataclysmic Type II supernova is shown here, imaged by the NASA/ESA Hubble Space Telescope's Advanced Camera for Surveys. Unlike m

PIX4583169

WWII Propaganda poster Royal Air Force, Royal Auxiliary Air Force

WWII Propaganda poster Royal Air Force, Royal Auxiliary Air Force

UIG2620934

Jupiter and Io seen by the New Horizons probe

Jupiter and Io seen by the New Horizons probe

PIX4574952

The Alps seen by satellite Envisat - The Alps as seen from satellite Envisat - Les Alpes seen by satellite ENVISAT on 8 December 2008. The snow - capped, crescent - shaped Alps and Italy's Apennines mountain chain are shown in this Envisat image. Snowfall in early winter - for meteorologists winter begins on the 1 December - covered the whole mountain areas with fresh snow, while the lower lands in the south and north of the mountains remained snow - free. Due to this snow cover and a relatively low illumination angle of the sun, the ranges and valleys of the mountains stand out in the image. Much of the whiteness seen in the top of the image is cloud cover, but fog is visible in the valleys such as the Rhine. The Alps - central Europe's major mountain range - extend some 1,200 km through France, Switzerland, Italy and Austria and down through Slovenia, Croatia, Bosnia and Herzegovina, Serbia and Montenegro and Albania as the Dinaric Alps. The Alps occupy an area of about 200,000 km an

The Alps seen by satellite Envisat - The Alps as seen from satellite Envisat - Les Alpes seen by satellite ENVISAT on 8 December 2008. The snow - capped, crescent - shaped Alps and Italy's Apennines mountain chain are shown in this Envisat image. Snowfall in early winter - for meteorologists winter begins on the 1 December - covered the whole mountain areas with fresh snow, while the lower lands in the south and north of the mountains remained snow - free. Due to this snow cover and a relatively low illumination angle of the sun, the ranges and valleys of the mountains stand out in the image. Much of the whiteness seen in the top of the image is cloud cover, but fog is visible in the valleys such as the Rhine. The Alps - central Europe's major mountain range - extend some 1,200 km through France, Switzerland, Italy and Austria and down through Slovenia, Croatia, Bosnia and Herzegovina, Serbia and Montenegro and Albania as the Dinaric Alps. The Alps occupy an area of about 200,000 km an

PIX4665079

Portrait of a Woman, said to be Marie Miraille, ca. 1574 (oil)

Portrait of a Woman, said to be Marie Miraille, ca. 1574 (oil)

Unknown Artist, (16th century)

XOS8984927

Centaurus A Elliptical Galaxy (NGC 5128) in the Centaur - Galaxy Centaurus A - The NGC 5128 galaxy is about 11 million years away - light from Earth. This image from the Hubble Space Telescope (HST) shows the star flames that occur in the dark band of the galaxy. This giant galaxy is a powerful radio source known as Centaurus A. It is an active galaxy whose energy comes from a supermassive black hole. Centaurus A, also known as NGC 5128, is well known for its dramatic dusty lanes of dark material. Hubble's observations, using its most advanced instrument, the Wide Field Camera 3, are the most detailed ever made of this galaxy. They have been combined here in a multi - wavelength image that reveals never - before - seen detail in the dusty portion of the galaxy. As well as features in the visible spectrum, this composite shows ultraviolet light from young stars, and near - infrared light, which lets us glimpse some of the detail otherwise obscured by the dust. The dark dust lane that cr

Centaurus A Elliptical Galaxy (NGC 5128) in the Centaur - Galaxy Centaurus A - The NGC 5128 galaxy is about 11 million years away - light from Earth. This image from the Hubble Space Telescope (HST) shows the star flames that occur in the dark band of the galaxy. This giant galaxy is a powerful radio source known as Centaurus A. It is an active galaxy whose energy comes from a supermassive black hole. Centaurus A, also known as NGC 5128, is well known for its dramatic dusty lanes of dark material. Hubble's observations, using its most advanced instrument, the Wide Field Camera 3, are the most detailed ever made of this galaxy. They have been combined here in a multi - wavelength image that reveals never - before - seen detail in the dusty portion of the galaxy. As well as features in the visible spectrum, this composite shows ultraviolet light from young stars, and near - infrared light, which lets us glimpse some of the detail otherwise obscured by the dust. The dark dust lane that cr

PIX4612191

Galaxy UGC 10214 in the Dragon - Galaxy UGC 10214 in Draco - The galaxy UGC 10214 is about 420 million years away - light from Earth. The shape of this galaxy is due to a collision with another galaxy, the small galaxy, blue, visible in the upper left corner of the image. Powerful gravitational forces are responsible for the formation of the tail, consisting of stars of dust and gas, which stretches over nearly 28,000 light years and is composed of recently formed and extremely bright blue stars. In the background, more than 6000 galaxies are visible, some more than 12 billion years apart - light. Image obtained by the Hubble Space Telescope in April 2002. This picture of the galaxy UGC 10214 was taken by the Advanced Camera for Surveys (ACS), which was installed aboard Nasa's Hubble Space Telescope in March during Servicing Mission 3B. Its distorted shape was caused by a small interloper, a very blue, compact galaxy visible in the upper left corner of the more massive Tadpole. The Tad

Galaxy UGC 10214 in the Dragon - Galaxy UGC 10214 in Draco - The galaxy UGC 10214 is about 420 million years away - light from Earth. The shape of this galaxy is due to a collision with another galaxy, the small galaxy, blue, visible in the upper left corner of the image. Powerful gravitational forces are responsible for the formation of the tail, consisting of stars of dust and gas, which stretches over nearly 28,000 light years and is composed of recently formed and extremely bright blue stars. In the background, more than 6000 galaxies are visible, some more than 12 billion years apart - light. Image obtained by the Hubble Space Telescope in April 2002. This picture of the galaxy UGC 10214 was taken by the Advanced Camera for Surveys (ACS), which was installed aboard Nasa's Hubble Space Telescope in March during Servicing Mission 3B. Its distorted shape was caused by a small interloper, a very blue, compact galaxy visible in the upper left corner of the more massive Tadpole. The Tad

PIX4613605

Pollution in the Gulf of Mexico - Gulf of Mexico oil spill - On April 20, 2010, following an explosion, an oil platform sank into the sea. The black maree stretching in the Gulf of Mexico is photographed here on 4 May 2010 from the International Space Station. In the center of the picture the oil table is visible south of the Mississippi Delta. On April 20, 2010, the oil rig Deepwater Horizon suffered an explosion and sank two days later. Soon thereafter, oil began leaking into the Gulf of Mexico from ruptured pipes deep on the ocean floor.

Pollution in the Gulf of Mexico - Gulf of Mexico oil spill - On April 20, 2010, following an explosion, an oil platform sank into the sea. The black maree stretching in the Gulf of Mexico is photographed here on 4 May 2010 from the International Space Station. In the center of the picture the oil table is visible south of the Mississippi Delta. On April 20, 2010, the oil rig Deepwater Horizon suffered an explosion and sank two days later. Soon thereafter, oil began leaking into the Gulf of Mexico from ruptured pipes deep on the ocean floor.

PIX4673142

Royal Naval uniform: pattern 1795-1812, Nelson's Trafalgar coat, c.1805 (wool, silk, brass, metal thread, gold alloy)

Royal Naval uniform: pattern 1795-1812, Nelson's Trafalgar coat, c.1805 (wool, silk, brass, metal thread, gold alloy)

Unknown Artist, (19th century)

MMM7340662

Galaxy UGC 10214 in the Dragon - Galaxy UGC 10214 in Draco - The galaxy UGC 10214 is about 420 million years away - light from Earth. The shape of this galaxy is due to a collision with another galaxy, the small galaxy, blue, visible in the upper left corner of the image. Powerful gravitational forces are responsible for the formation of the tail, consisting of stars of dust and gas, which stretches over nearly 28,000 light years and is composed of recently formed and extremely bright blue stars. In the background, more than 6000 galaxies are visible, some more than 12 billion years apart - light. Image obtained by the Hubble Space Telescope in April 2002. This picture of the galaxy UGC 10214 was taken by the Advanced Camera for Surveys (ACS), which was installed aboard Nasa's Hubble Space Telescope in March during Servicing Mission 3B. Its distorted shape was caused by a small interloper, a very blue, compact galaxy visible in the upper left corner of the more massive Tadpole. The Tad

Galaxy UGC 10214 in the Dragon - Galaxy UGC 10214 in Draco - The galaxy UGC 10214 is about 420 million years away - light from Earth. The shape of this galaxy is due to a collision with another galaxy, the small galaxy, blue, visible in the upper left corner of the image. Powerful gravitational forces are responsible for the formation of the tail, consisting of stars of dust and gas, which stretches over nearly 28,000 light years and is composed of recently formed and extremely bright blue stars. In the background, more than 6000 galaxies are visible, some more than 12 billion years apart - light. Image obtained by the Hubble Space Telescope in April 2002. This picture of the galaxy UGC 10214 was taken by the Advanced Camera for Surveys (ACS), which was installed aboard Nasa's Hubble Space Telescope in March during Servicing Mission 3B. Its distorted shape was caused by a small interloper, a very blue, compact galaxy visible in the upper left corner of the more massive Tadpole. The Tad

PIX4613581

Barree spiral galaxy NGC 4319 and Markarian quasar 205 - Galaxy NGC 4319 and quasar Markarian 205 - The barree spiral galaxy NGC 4319, in the center, is 80 million years - light in the constellation of the Dragon. The Markarian 205 quasar, on the top right, is 14 times further at about 1 billion light years. These two objects are therefore not interacting; on the other hand, the galaxy NGC 4319 is probably interacting with the galaxy NGC 4291, out of field, as the weak arm at the bottom left allows. Quasars are galaxies that create an extremely bright core. Image made by the Hubble Space Telescope in 2002. In this NASA Hubble Space Telescope image, an odd celestial duo, the spiral galaxy NGC 4319 (center) and a quasar called Markarian 205 (upper right), appear to be neighbors. In reality, the two objects don't even live in the same city. NGC 4319 is 80 million light - years from Earth. Markarian 205 (Mrk 205) is more than 14 times farther away, residing 1 billion light - years from Ear

Barree spiral galaxy NGC 4319 and Markarian quasar 205 - Galaxy NGC 4319 and quasar Markarian 205 - The barree spiral galaxy NGC 4319, in the center, is 80 million years - light in the constellation of the Dragon. The Markarian 205 quasar, on the top right, is 14 times further at about 1 billion light years. These two objects are therefore not interacting; on the other hand, the galaxy NGC 4319 is probably interacting with the galaxy NGC 4291, out of field, as the weak arm at the bottom left allows. Quasars are galaxies that create an extremely bright core. Image made by the Hubble Space Telescope in 2002. In this NASA Hubble Space Telescope image, an odd celestial duo, the spiral galaxy NGC 4319 (center) and a quasar called Markarian 205 (upper right), appear to be neighbors. In reality, the two objects don't even live in the same city. NGC 4319 is 80 million light - years from Earth. Markarian 205 (Mrk 205) is more than 14 times farther away, residing 1 billion light - years from Ear

PIX4611257

Flying Star Zeta Ophiuchi - Runaway Star Zeta Ophiuchi - The blue star near the center of the image is Zeta Ophiuchi, a very massive star moving at 24 km per second. It is a “” fleeing star”, a star ejected by the explosion of his companion star. In this infrared image obtained by the WISE (Wide - field Infrared Survey Explorer) satellite, the interstellar dust traversed by the star appears, as well as an arc-shaped shock wave caused by the powerful stellar winds that the star breaks. The blue star near the center of this image is Zeta Ophiuchi. When seen in visible light it appears as a relatively dim red star surrounded by other dim stars and no dust. However, in this infrared image taken with Nasa's Wide - field Infrared Survey Explorer, or WISE, a completely different view emerges. Zeta Ophiuchi is actually a very massive, hot, bright blue star plowing its way through a large cloud of interstellar dust and gas. Astronomers theorize that this stellar juggernaut was likely once part

Flying Star Zeta Ophiuchi - Runaway Star Zeta Ophiuchi - The blue star near the center of the image is Zeta Ophiuchi, a very massive star moving at 24 km per second. It is a “” fleeing star”, a star ejected by the explosion of his companion star. In this infrared image obtained by the WISE (Wide - field Infrared Survey Explorer) satellite, the interstellar dust traversed by the star appears, as well as an arc-shaped shock wave caused by the powerful stellar winds that the star breaks. The blue star near the center of this image is Zeta Ophiuchi. When seen in visible light it appears as a relatively dim red star surrounded by other dim stars and no dust. However, in this infrared image taken with Nasa's Wide - field Infrared Survey Explorer, or WISE, a completely different view emerges. Zeta Ophiuchi is actually a very massive, hot, bright blue star plowing its way through a large cloud of interstellar dust and gas. Astronomers theorize that this stellar juggernaut was likely once part

PIX4572156

Star formation in the Sails - Star formation in Vela - Infrared view of the nebulae Gum 22 (top right), Gum 23, IRAS 09002 - 4732 (orange cloud near center), Bran 226 (bottom left), and Gum 25 (bottom left). These star-forming regions are located between 4000 and 10,000 light years of the Earth. The bright green star, down to the right of the image, is a carbon star, IRAS 08535 - 4724. Image obtained by the WISE telescope (Wide - field Infrared Explorer). This image from Nasa's Wide - field Infrared Survey Explorer, or WISE, highlights several star - forming regions. There are five distinct centers of star birth in this one image alone. Star - forming nebulae (called HII regions by astronomers) are clouds of gas and dust that have been heated up by nearby stars recently formed from the same cloud. The largest, brightest cloud, in the upper right is known as Gum 22. It's named after Colin Gum, an Australian astronomer who surveyed the southern hemisphere sky in the early 1950's looking

Star formation in the Sails - Star formation in Vela - Infrared view of the nebulae Gum 22 (top right), Gum 23, IRAS 09002 - 4732 (orange cloud near center), Bran 226 (bottom left), and Gum 25 (bottom left). These star-forming regions are located between 4000 and 10,000 light years of the Earth. The bright green star, down to the right of the image, is a carbon star, IRAS 08535 - 4724. Image obtained by the WISE telescope (Wide - field Infrared Explorer). This image from Nasa's Wide - field Infrared Survey Explorer, or WISE, highlights several star - forming regions. There are five distinct centers of star birth in this one image alone. Star - forming nebulae (called HII regions by astronomers) are clouds of gas and dust that have been heated up by nearby stars recently formed from the same cloud. The largest, brightest cloud, in the upper right is known as Gum 22. It's named after Colin Gum, an Australian astronomer who surveyed the southern hemisphere sky in the early 1950's looking

PIX4621545

Grand Trou bleu, Lighthouse reef, Belize - Satellite image of Belize's Lighthouse Reef with the Great Blue Hole - Satellite photo of Lighthouse Reef obtained by EO satellite - 1 March 24, 2009. Lighthouse Reef is a small atoll located 80 km from the mainland and Belize City. It belongs to the network of reserves of the Belize Barriere Reef, a UNESCO World Heritage Site. In the center of the image is the Great Blue Hole, an ancient, collapsed limestone cave, almost circular, with a diameter of more than 300 m and 120 m deep. The Advanced Land Imager (ALI) on Nasa's Earth Observing - 1 satellite captured this image of Lighthouse Reef in the Caribbean Sea on March 24, 2009. In the middle of the image lies a giant circle of deep blue. Roughly 300 meters (1,000 feet) across and 125 meters (400 feet) deep, the feature is known as the Great Blue Hole. The Great Blue Hole is surrounded by a ring of lighter color caused by elevated coral. In fact, parts of the ring surrounding this feature actu

Grand Trou bleu, Lighthouse reef, Belize - Satellite image of Belize's Lighthouse Reef with the Great Blue Hole - Satellite photo of Lighthouse Reef obtained by EO satellite - 1 March 24, 2009. Lighthouse Reef is a small atoll located 80 km from the mainland and Belize City. It belongs to the network of reserves of the Belize Barriere Reef, a UNESCO World Heritage Site. In the center of the image is the Great Blue Hole, an ancient, collapsed limestone cave, almost circular, with a diameter of more than 300 m and 120 m deep. The Advanced Land Imager (ALI) on Nasa's Earth Observing - 1 satellite captured this image of Lighthouse Reef in the Caribbean Sea on March 24, 2009. In the middle of the image lies a giant circle of deep blue. Roughly 300 meters (1,000 feet) across and 125 meters (400 feet) deep, the feature is known as the Great Blue Hole. The Great Blue Hole is surrounded by a ring of lighter color caused by elevated coral. In fact, parts of the ring surrounding this feature actu

PIX4672819

Airy's transit circle telescope, 1850 (photo)

Airy's transit circle telescope, 1850 (photo)

British School, (19th century)

MMM7340621

Battle of Midway, WWII defense of Midway Island from Japanese attack, battle scenes, Navy pilots, marines and burial ceremonies, 1942

Battle of Midway, WWII defense of Midway Island from Japanese attack, battle scenes, Navy pilots, marines and burial ceremonies, 1942

BOF3833239

The English and Dutch fleets on the day after the Battle of Solebay, 1672, late 17th century (drawing)

The English and Dutch fleets on the day after the Battle of Solebay, 1672, late 17th century (drawing)

Velde, Willem van de, the Elder (1611-93)

MMM7341582

The Hon. Sir John Cust, 3rd Bt of Pinchbeck and 6th Bt of Humby (1718-1770) in Speaker's Robes

The Hon. Sir John Cust, 3rd Bt of Pinchbeck and 6th Bt of Humby (1718-1770) in Speaker's Robes

Reynolds, Joshua (1723-92)

USB1160784

Where the Anzacs dug themselves in on the shelterless slopes of barren hills exposed to enemy fire, 1915 (b/w photo)

Where the Anzacs dug themselves in on the shelterless slopes of barren hills exposed to enemy fire, 1915 (b/w photo)

Unknown photographer, (20th century)

NAM5923026

Lord Fairfax, 1650 circa (line engraving)

Lord Fairfax, 1650 circa (line engraving)

English School, (17th century)

NAM5929101

Sir Thomas Fairfax, c.1645 (engraving)

Sir Thomas Fairfax, c.1645 (engraving)

Walker, Robert (1599-1658) (after)

NAM5929098

Sepoy Ali Haidar VC, 13th Frontier Force Rifles, 13 August 1945 (b/w photo)

Sepoy Ali Haidar VC, 13th Frontier Force Rifles, 13 August 1945 (b/w photo)

Unknown photographer, (20th century)

NAM5923535

Lord Robert Spencer (1747-1831)

Lord Robert Spencer (1747-1831)

Reynolds, Joshua (1723-92)

USB1159772

Sepoy Ali Haidar VC (right) at the Frontier Force Rifles depot, Abbottabad, 13 August 1945 (b/w photo)

Sepoy Ali Haidar VC (right) at the Frontier Force Rifles depot, Abbottabad, 13 August 1945 (b/w photo)

Unknown photographer, (20th century)

NAM5923536

The Days of Brescia, 1974 (16mm positive, 2K/Sound scan)

The Days of Brescia, 1974 (16mm positive, 2K/Sound scan)

MOD6428912

Wolf, 2018 (mixed media on paper)

premium — Wolf, 2018 (mixed media on paper)

Wolf, 2018 (mixed media on paper)

Adlington, Mark

MAD6219141

A Subtle Intelligence, 2018 (mixed media on paper)

premium — A Subtle Intelligence, 2018 (mixed media on paper)

A Subtle Intelligence, 2018 (mixed media on paper)

Adlington, Mark

MAD6219139

Not For Conquest 3of3

Not For Conquest 3of3

BOF6283319

Not For Conquest 2of3

Not For Conquest 2of3

BOF6285240

Release Of Watergate Tapes - President Richard M. Nixon

Release Of Watergate Tapes - President Richard M. Nixon

BOF7336651

Switzerland Basel Carnival, 1959 (b/w photo)

Switzerland Basel Carnival, 1959 (b/w photo)

Stringer (STR)

KES6245725

Stereoscopic glass plate, First World War: Aisne, after a raid by enemy aircraft, 1918 (photo)

Stereoscopic glass plate, First World War: Aisne, after a raid by enemy aircraft, 1918 (photo)

Unknown photographer, (20th century)

Photo Josse

JLJ5619239

Switzerland Gottlieb Duttweiler (b/w photo)

Switzerland Gottlieb Duttweiler (b/w photo)

Stringer (STR)

KES6249898

Straits of Gibraltar seen by the Envisat satellite with the ASAR instrument on 20 May 2002

Straits of Gibraltar seen by the Envisat satellite with the ASAR instrument on 20 May 2002

PIX4665861

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