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Lady Phyllis Hervey, later Lady Phyllis MacRae (1899-1990)

Lady Phyllis Hervey, later Lady Phyllis MacRae (1899-1990)

Miller, William Edwards (1873-1903)

USB1156560

Nebula IC 2948 in Centaurus - Nebula IC 2948 and IC 2944 in Centaurus: IC2944 - SHO 70 70 70 Bin 2 - Nebula IC 2948 is a vast nebula located about 6000 light years from Earth in the southern constellation of Centaurus. It is associated with the cluster of stars IC 2944 near which Bok's blood cells are visible. A Bok's blood cell is a dark interstellar cloud of gases and dust that absorb light. If it condenses enough, it gives birth to new stars - Image obtained through 3 different filters that highlight oxygen (in blue), hydrogen (in green), and sulfur (in red) - Between the Southern Cross and the rich Carina region, on the southern border of Centaurus, is a large, almost featureless emission nebula, IC 2948, with a sprinkling of bright stars, Collinder 249. It is against this uniform, backdrop that we see a brighter region (IC 2944) which hosts small group of dark clouds of the kind known as 'Bok globules'. They are named for the Dutch-American astronomer who first drew attention to t

Nebula IC 2948 in Centaurus - Nebula IC 2948 and IC 2944 in Centaurus: IC2944 - SHO 70 70 70 Bin 2 - Nebula IC 2948 is a vast nebula located about 6000 light years from Earth in the southern constellation of Centaurus. It is associated with the cluster of stars IC 2944 near which Bok's blood cells are visible. A Bok's blood cell is a dark interstellar cloud of gases and dust that absorb light. If it condenses enough, it gives birth to new stars - Image obtained through 3 different filters that highlight oxygen (in blue), hydrogen (in green), and sulfur (in red) - Between the Southern Cross and the rich Carina region, on the southern border of Centaurus, is a large, almost featureless emission nebula, IC 2948, with a sprinkling of bright stars, Collinder 249. It is against this uniform, backdrop that we see a brighter region (IC 2944) which hosts small group of dark clouds of the kind known as 'Bok globules'. They are named for the Dutch-American astronomer who first drew attention to t

W. Promper

PIX4622580

Sir David Baird Bart GCB, KC Colonel of the 24th Regiment, 1811 (mezzotint)

Sir David Baird Bart GCB, KC Colonel of the 24th Regiment, 1811 (mezzotint)

Raeburn, Henry (1756-1823) (after)

NAM5920729

China / USA: Anna May Wong, Chinese-American movie star, c. 1938

China / USA: Anna May Wong, Chinese-American movie star, c. 1938

PFH3061478

Thomas Hesketh, MP (1698-1735), his wife Martha St Amand, Mrs Thomas Hesketh (d.1782) and a Son

Thomas Hesketh, MP (1698-1735), his wife Martha St Amand, Mrs Thomas Hesketh (d.1782) and a Son

Kneller, Godfrey (1646-1723) (studio of)

USB1158016

Clive at Plassey (1757), circa 1821 (w/c and ink)

Clive at Plassey (1757), circa 1821 (w/c and ink)

Heath, William (1795-1840)

NAM5919939

Dark stars and nebulae in Sagittarius and Ophiuchus - Dark Nebulae in Sagittarius and Scorpius - Dark nebulae on the edge of the Pipe nebula. This complex of dust clouds that block the light of the stars is located between the Sagittarius and the Scorpio, near the center of our lactee road. Also visible, the nebulae emitted from the Lagoon, Trifide, and Omega. Image obtained with Canon 20Da, 50 mm f/1.4, 6 x 5 min ISO 1600 poses. This amazing complex of dark nebulae and dust in Sagittarius and Ophiuchus lies near the central bulge of our own galaxy, the Milky Way. Dark nebulae are non - luminous clouds of obscuring matter and dust which block the light from stars behind them. Many of the dark nebulae seen here are listed in E.E. Barnard's catalog of dark nebulae and are given a “” B” designation, such as B72, the Snake Nebula. Almost the entire complex of dark nebulae seen on the right hand side of the image make up the “Dark Horse and Rider””. The Pipe Nebula, Lynds Dark Nebula 1773,

Dark stars and nebulae in Sagittarius and Ophiuchus - Dark Nebulae in Sagittarius and Scorpius - Dark nebulae on the edge of the Pipe nebula. This complex of dust clouds that block the light of the stars is located between the Sagittarius and the Scorpio, near the center of our lactee road. Also visible, the nebulae emitted from the Lagoon, Trifide, and Omega. Image obtained with Canon 20Da, 50 mm f/1.4, 6 x 5 min ISO 1600 poses. This amazing complex of dark nebulae and dust in Sagittarius and Ophiuchus lies near the central bulge of our own galaxy, the Milky Way. Dark nebulae are non - luminous clouds of obscuring matter and dust which block the light from stars behind them. Many of the dark nebulae seen here are listed in E.E. Barnard's catalog of dark nebulae and are given a “” B” designation, such as B72, the Snake Nebula. Almost the entire complex of dark nebulae seen on the right hand side of the image make up the “Dark Horse and Rider””. The Pipe Nebula, Lynds Dark Nebula 1773,

Jerry Lodriguss

PIX4621393

Margaret Lemon, c.1638 (oil on canvas)

Margaret Lemon, c.1638 (oil on canvas)

Dyck, Anthony van (1599-1641)

ROC3707666

Warsaw Ghetto Uprising - Photo from Jürgen Stroop Report to Heinrich …, 1945 (photo)

Warsaw Ghetto Uprising - Photo from Jürgen Stroop Report to Heinrich …, 1945 (photo)

IMO8738210

New Horizons closest approach to Pluto - Artist's view of the New Horizons probe near Pluto and its largest satellite Charon. The New Horizons probe was launched on 19 January 2006 to Jupiter, then Pluto and Charon, which it will reach in 2015 and Kuiper's objects in 2020. Nasa's New Horizons unmanned spacecraft flies into the shadow of dwarf planet Pluto and its moon Charon. New Horizons has been en route to Pluto since its launch from Earth in 2006 and is scheduled to make its closest approach on 14 July 2015. New Horizons will be traveling at a velocity relative to Pluto of 30,800 mph, far too fast for it to enter orbit around and become a satellite of Pluto. Instead after passing Pluto, New Horizons will continue farther into the Kuiper belt searching for other objects with diameters of 30 to 60 miles. New Horizons is about the size and shape of a grand piano and weighed 1,054 pounds at launch. The high - gain dish antenna is about 7 feet in diameter and is employed for communicati

New Horizons closest approach to Pluto - Artist's view of the New Horizons probe near Pluto and its largest satellite Charon. The New Horizons probe was launched on 19 January 2006 to Jupiter, then Pluto and Charon, which it will reach in 2015 and Kuiper's objects in 2020. Nasa's New Horizons unmanned spacecraft flies into the shadow of dwarf planet Pluto and its moon Charon. New Horizons has been en route to Pluto since its launch from Earth in 2006 and is scheduled to make its closest approach on 14 July 2015. New Horizons will be traveling at a velocity relative to Pluto of 30,800 mph, far too fast for it to enter orbit around and become a satellite of Pluto. Instead after passing Pluto, New Horizons will continue farther into the Kuiper belt searching for other objects with diameters of 30 to 60 miles. New Horizons is about the size and shape of a grand piano and weighed 1,054 pounds at launch. The high - gain dish antenna is about 7 feet in diameter and is employed for communicati

Walter B Myers

PIX4607362

Faustina, 150-175 (marble)

Faustina, 150-175 (marble)

Roman, (2nd century)

ROC3706869

Globular cluster NGC 6397 in the Altar - Stars in globular cluster NGC 6397 in Ara - Image of the center of the globular cluster NGC 6397 located 8200 years - light in the southern constellation of the Altar. The density of stars is very important, the stars are distant from each other only a few weeks light (the star closest to our Sun is four years away - light). Sometimes a collision between two stars occurs; they merge into a single, young, bright and warm star called a blue straggler; some of these stars are visible near the center of the image. This Hubble Space Telescope view of the core of one of the nearest globular star clusters, called NGC 6397, located 8,200 light - years away in the constellation Ara. The stellar density is about a million times greater than in our Sun's stellar neighborhood. The stars are only a few light - weeks apart, while the nearest star to our Sun is over four light - years away. The ancient stars are so crowded together that a few of them inevitabl

Globular cluster NGC 6397 in the Altar - Stars in globular cluster NGC 6397 in Ara - Image of the center of the globular cluster NGC 6397 located 8200 years - light in the southern constellation of the Altar. The density of stars is very important, the stars are distant from each other only a few weeks light (the star closest to our Sun is four years away - light). Sometimes a collision between two stars occurs; they merge into a single, young, bright and warm star called a blue straggler; some of these stars are visible near the center of the image. This Hubble Space Telescope view of the core of one of the nearest globular star clusters, called NGC 6397, located 8,200 light - years away in the constellation Ara. The stellar density is about a million times greater than in our Sun's stellar neighborhood. The stars are only a few light - weeks apart, while the nearest star to our Sun is over four light - years away. The ancient stars are so crowded together that a few of them inevitabl

PIX4564803

Gladstone collection 3: Northern Territories, Ghana Part 1 c.1961

Gladstone collection 3: Northern Territories, Ghana Part 1 c.1961

BAF8619157

The Colossus, in Dardanelles (oil painting)

The Colossus, in Dardanelles (oil painting)

Nibbs, Richard Henry (c.1816-93)

MMM7337707

Sir Robert Davers, 5th Bt (1729-1763) [aged 21]

Sir Robert Davers, 5th Bt (1729-1763) [aged 21]

Batoni, Pompeo Girolamo (1708-87)

USB1156516

Liquid mirror telescope on the Moon - Lunar liquid mirror telescope - Illustration of an astronomical observatory on the Moon. Installs near the southern pole of the Moon, a giant telescope with liquid mirror, one kilometre in diameter. A giant liquid mirror telescope 1 kilometer wide (6 tenths of a mile) and 1 kilometer tall lies nestled in an approximately 1 kilometer wide crater near the Moon's south pole. In the foreground is a kind of lunar city for human habitation composed of pressurized and radiation-hardened living units. On the upper right are landing pads for transports arriving to and departing from the lunar surface. A liquid mirror telescope is a Newtonian reflecting type telescope that employs a reflecting liquid as the primary mirror. A concept first identified 300 years ago by Isaac Newton himself, the reflecting liquid assumes the proper paraboloidal shape by rotating the container the liquid is in. On Earth working liquid mirror telescopes have been created with diam

Liquid mirror telescope on the Moon - Lunar liquid mirror telescope - Illustration of an astronomical observatory on the Moon. Installs near the southern pole of the Moon, a giant telescope with liquid mirror, one kilometre in diameter. A giant liquid mirror telescope 1 kilometer wide (6 tenths of a mile) and 1 kilometer tall lies nestled in an approximately 1 kilometer wide crater near the Moon's south pole. In the foreground is a kind of lunar city for human habitation composed of pressurized and radiation-hardened living units. On the upper right are landing pads for transports arriving to and departing from the lunar surface. A liquid mirror telescope is a Newtonian reflecting type telescope that employs a reflecting liquid as the primary mirror. A concept first identified 300 years ago by Isaac Newton himself, the reflecting liquid assumes the proper paraboloidal shape by rotating the container the liquid is in. On Earth working liquid mirror telescopes have been created with diam

Walter B Myers

PIX4639385

Milky way all around the horizon and Gegenschein - Fisheye view of the southern sky. The lactee path blends with the horizon line. In the sky, the three brightest galaxies visible on Earth: the two galaxies of the Magellan Cloud, and opposite it towards the right middle of the image, the galaxy of Andromede. Crossing the image on the right, the gegenschein, the blade glow made up of dust reflecting the light of the sun, observable only in a dense sky of any parasite light. The bright spot near the center of the image is Jupiter Planet. The following image was taken at new Moon (No Moon light), middle of the night (minimum zodiacal light effect), in the Atacama desert close to Paranal observatory (no light pollution). The chosen place for this picture has the particularity to be located at a latitude which value is close to the declination of the galactic southern pole. The picture was therefore also taken when the galactic pole passes at zenith, ensuring that there is no Milky Way up i

Milky way all around the horizon and Gegenschein - Fisheye view of the southern sky. The lactee path blends with the horizon line. In the sky, the three brightest galaxies visible on Earth: the two galaxies of the Magellan Cloud, and opposite it towards the right middle of the image, the galaxy of Andromede. Crossing the image on the right, the gegenschein, the blade glow made up of dust reflecting the light of the sun, observable only in a dense sky of any parasite light. The bright spot near the center of the image is Jupiter Planet. The following image was taken at new Moon (No Moon light), middle of the night (minimum zodiacal light effect), in the Atacama desert close to Paranal observatory (no light pollution). The chosen place for this picture has the particularity to be located at a latitude which value is close to the declination of the galactic southern pole. The picture was therefore also taken when the galactic pole passes at zenith, ensuring that there is no Milky Way up i

Stephane Guisard

PIX4636032

CYRIL STINNETT: Left handed fiddle champion, Spring 1981

CYRIL STINNETT: Left handed fiddle champion, Spring 1981

OZA8610369

Lakota Territory at the Wounded Knee, 1984.

Lakota Territory at the Wounded Knee, 1984.

LCS7223860

Saturn seen by the Cassini probe on 9 - 05 - 2007 - Saturn in natural colors seen by Cassini spacecraft May 9 2007. - Saturn seen by the Cassini probe on 9 - 05 - 2007 at a distance of 1.1 million km from the planet. Mosaic of 45 images. Three satellites are visible in this image: Mimas (upper right), Janus (lower right) and Pandora (barely visible, near ring F, lower left). This natural color mosaic was acquired by the Cassini spacecraft as it soared 39 degrees above the unilluminated side of the rings. Little light makes its way through the rings to be scattered in Cassini's direction in this viewing geometry, making the rings appear somewhat dark compared to the reflective planet. Bright clouds play in the blue - gray skies of the north. The ring shadows continue to caress the planet as they slide farther south toward their momentary disappearance during equinox in 2009. The rings' reflected light illuminates the southern hemisphere on Saturn's night side. Three of Saturn's moons ar

Saturn seen by the Cassini probe on 9 - 05 - 2007 - Saturn in natural colors seen by Cassini spacecraft May 9 2007. - Saturn seen by the Cassini probe on 9 - 05 - 2007 at a distance of 1.1 million km from the planet. Mosaic of 45 images. Three satellites are visible in this image: Mimas (upper right), Janus (lower right) and Pandora (barely visible, near ring F, lower left). This natural color mosaic was acquired by the Cassini spacecraft as it soared 39 degrees above the unilluminated side of the rings. Little light makes its way through the rings to be scattered in Cassini's direction in this viewing geometry, making the rings appear somewhat dark compared to the reflective planet. Bright clouds play in the blue - gray skies of the north. The ring shadows continue to caress the planet as they slide farther south toward their momentary disappearance during equinox in 2009. The rings' reflected light illuminates the southern hemisphere on Saturn's night side. Three of Saturn's moons ar

PIX4625121

Taurus Molecular Cloud - Taurus Molecular Cloud - This region is located on the border of the Taurus and Persee constellations. Covering about 20 x 30 degres, this image shows a complex of emitted nebulae, star clusters, reflexion nebulae and dark nebulae. A molecular cloud is a region of dense gas and dust composed mainly of molecular hydrogen and helium. It's a birthplace of stars. The Molecular Cloud of Taurus is located about 400 years ago - light, and is one of the closest molecular clouds to our solar system. The California Nebula (NGC 1499), an emission nebula located about 1000 years ago - is visible at the top right. The dark nebulae B7, B18 and B19 are visible near the center of the image. Les Pleiades, M45, is the open cluster at the bottom right center. The open clusters NGC 1817, NGC 1746, NGC 1647 are on the left side of the image. The Hyades, Melotte 25, is a V-shaped cluster at the bottom left. It is the closest open cluster, located at a distance of about 151 light yea

Taurus Molecular Cloud - Taurus Molecular Cloud - This region is located on the border of the Taurus and Persee constellations. Covering about 20 x 30 degres, this image shows a complex of emitted nebulae, star clusters, reflexion nebulae and dark nebulae. A molecular cloud is a region of dense gas and dust composed mainly of molecular hydrogen and helium. It's a birthplace of stars. The Molecular Cloud of Taurus is located about 400 years ago - light, and is one of the closest molecular clouds to our solar system. The California Nebula (NGC 1499), an emission nebula located about 1000 years ago - is visible at the top right. The dark nebulae B7, B18 and B19 are visible near the center of the image. Les Pleiades, M45, is the open cluster at the bottom right center. The open clusters NGC 1817, NGC 1746, NGC 1647 are on the left side of the image. The Hyades, Melotte 25, is a V-shaped cluster at the bottom left. It is the closest open cluster, located at a distance of about 151 light yea

Jerry Lodriguss

PIX4621177

Master Middleton (?) preparing to Shoot for the Silver Arrow at Harrow, 5th August, 1758

Master Middleton (?) preparing to Shoot for the Silver Arrow at Harrow, 5th August, 1758

Craskell, Thomas (18th century)

USB1160170

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 UGC 12158 - Galaxy UGC 12158 - The galaxy UGC 12158, is about 400 million light years away from Earth in the constellation Pegase. In this image obtained by the Hubble space telescope, a blue star is visible near the center of the galaxy (lower left), it is a supernova, SN 2004ef. The galaxy captured in this image, called UGC 12158, certainly isn't camera - shy: this spiral stunner is posing face - on to the NASA/ESA Hubble Space Telescope's Advanced Camera for Surveys, revealing its structure in fine detail. UGC 12158 is an excellent example of a barred spiral galaxy in the Hubble sequence - - a scheme used to categorise galaxies based on their shapes. Barred spirals, as the name suggest, feature spectacular swirling arms of stars that emanate from a bar - shaped centre. Such bar structures are common, being found in about two thirds of spiral galaxies, and are thought to act as funnels, guiding gas to their galactic centres where it accumulates to form newborn st

Barree spiral galaxy UGC 12158 - Galaxy UGC 12158 - The galaxy UGC 12158, is about 400 million light years away from Earth in the constellation Pegase. In this image obtained by the Hubble space telescope, a blue star is visible near the center of the galaxy (lower left), it is a supernova, SN 2004ef. The galaxy captured in this image, called UGC 12158, certainly isn't camera - shy: this spiral stunner is posing face - on to the NASA/ESA Hubble Space Telescope's Advanced Camera for Surveys, revealing its structure in fine detail. UGC 12158 is an excellent example of a barred spiral galaxy in the Hubble sequence - - a scheme used to categorise galaxies based on their shapes. Barred spirals, as the name suggest, feature spectacular swirling arms of stars that emanate from a bar - shaped centre. Such bar structures are common, being found in about two thirds of spiral galaxies, and are thought to act as funnels, guiding gas to their galactic centres where it accumulates to form newborn st

PIX4613612

Mosaic of a Vine Scroll Border with Peacocks, Antioch, 526-540 (marble and limestone tesserae embedded in lime mortar)

Mosaic of a Vine Scroll Border with Peacocks, Antioch, 526-540 (marble and limestone tesserae embedded in lime mortar)

Roman, (6th century AD)

WAM5911438

Mr Charles Melville Hays, passenger on the Titanic, was 55 - born at Rock Island, Illinois, USA, on 16 May 1856. He was educated at the public schools of Rock Island, and went to work for the Atlantic and Pacific Railway when he was 17. At 22 he was appointed secretary to the Manager of the Missouri Pacific Railway. In 1896 he moved to Montreal to become general manager of the Grand Trunk Pacific Railway. It was Hays who convinced the Canadian Prime Minister, Sir Wilfrid Laurier, of the need for a second transcontinental railroad. Hays and his wife and daughter were on the Titanic and when it struck the iceberg. As he put his wife and daughter into a lifeboat, he assured them Titanic would stay 'afloat for at least 10 hours' - he never believed it would sink so quickly. Hays drowned in the disaster, but the Minia recovered his body on 26 April. His coffin was brought back to Montreal for burial aboard his private railway car, Canada. The car is still preserved and on display at the C

Mr Charles Melville Hays, passenger on the Titanic, was 55 - born at Rock Island, Illinois, USA, on 16 May 1856. He was educated at the public schools of Rock Island, and went to work for the Atlantic and Pacific Railway when he was 17. At 22 he was appointed secretary to the Manager of the Missouri Pacific Railway. In 1896 he moved to Montreal to become general manager of the Grand Trunk Pacific Railway. It was Hays who convinced the Canadian Prime Minister, Sir Wilfrid Laurier, of the need for a second transcontinental railroad. Hays and his wife and daughter were on the Titanic and when it struck the iceberg. As he put his wife and daughter into a lifeboat, he assured them Titanic would stay 'afloat for at least 10 hours' - he never believed it would sink so quickly. Hays drowned in the disaster, but the Minia recovered his body on 26 April. His coffin was brought back to Montreal for burial aboard his private railway car, Canada. The car is still preserved and on display at the C

UIG5447129

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

Arcadion, ca. 1893 (oil on canvas)

Arcadion, ca. 1893 (oil on canvas)

Constant, Jean Joseph Benjamin (1845-1902)

XOS8985915

Lady Louisa Tollemache, Countess of Dysart (1745-1840) (after Reynolds)

Lady Louisa Tollemache, Countess of Dysart (1745-1840) (after Reynolds)

Hoppner, John (1758-1810)

USB1155790

Copper Mines in Arizona - USA - Open pit Copper mines - Arizona: Three open-air copper mines near the city of Green Valley in Arizona. Image taken from the International Space Station (ISS) on January 14, 2010. This astronaut photograph illustrates three open-pit mines located west-northwest of the town of Green Valley, Arizona. While the mines appear to be close to each other, each exploits a separate porphyry copper deposit. The mine pits are recognizable by the concentric lines of benches cut into the pit sides. The benches allow equipment and personnel access to the fresh ore (gray) exposed at the bottom of the excavation. Water may also pool at the bottom of inactive pits, such as in the Twin Buttes Mine at image upper right (black areas). The open pit areas are surrounded by an array of sculpted tailings ponds and mine dump areas; these receive mine waste rock for storage and later leaching for further recovery of metals. The green color of the water in the tailings pond at image

Copper Mines in Arizona - USA - Open pit Copper mines - Arizona: Three open-air copper mines near the city of Green Valley in Arizona. Image taken from the International Space Station (ISS) on January 14, 2010. This astronaut photograph illustrates three open-pit mines located west-northwest of the town of Green Valley, Arizona. While the mines appear to be close to each other, each exploits a separate porphyry copper deposit. The mine pits are recognizable by the concentric lines of benches cut into the pit sides. The benches allow equipment and personnel access to the fresh ore (gray) exposed at the bottom of the excavation. Water may also pool at the bottom of inactive pits, such as in the Twin Buttes Mine at image upper right (black areas). The open pit areas are surrounded by an array of sculpted tailings ponds and mine dump areas; these receive mine waste rock for storage and later leaching for further recovery of metals. The green color of the water in the tailings pond at image

PIX4672551

Blue stragglers in cluster 47 Toucan - Blue stragglers in globular cluster 47 Tucanae - This image obtained by the Hubble space telescope shows a detail of the 47 Toucan cluster near its center (the field is indicated on the left image taken from the ground). The yellow circles on the right image indicate the position of stars identified by the telescope as blue trainers. Because of the high density of stars within a globular cluster, a collision between two stars sometimes occurs, merging into a single young, bright and warm star called a blue straggler. The core of globular cluster 47 Tucanae is home to many blue stragglers, rejuvenated stars that glow with the blue light of young stars. A ground - based telescope image (on the left) shows the entire crowded core of 47 Tucanae, located 15,000 light - years away in the constellation Tucana. Peering into the heart of the globular cluster's bright core, the Hubble Space Telescope's Wide Field and Planetary Camera 2 separated the dense c

Blue stragglers in cluster 47 Toucan - Blue stragglers in globular cluster 47 Tucanae - This image obtained by the Hubble space telescope shows a detail of the 47 Toucan cluster near its center (the field is indicated on the left image taken from the ground). The yellow circles on the right image indicate the position of stars identified by the telescope as blue trainers. Because of the high density of stars within a globular cluster, a collision between two stars sometimes occurs, merging into a single young, bright and warm star called a blue straggler. The core of globular cluster 47 Tucanae is home to many blue stragglers, rejuvenated stars that glow with the blue light of young stars. A ground - based telescope image (on the left) shows the entire crowded core of 47 Tucanae, located 15,000 light - years away in the constellation Tucana. Peering into the heart of the globular cluster's bright core, the Hubble Space Telescope's Wide Field and Planetary Camera 2 separated the dense c

PIX4564265

Jupiter's Fusion Spots seen by the Hubble Space Telescope - Sequence of images of Jupiter's atmosphere obtained on May 15, June 28 and July 8, 2008 by the Hubble Space Telescope. The Great Red Spot of Jupiter is a gigantic permanent tempete measuring nearly 25,000 km in diameter. It's been observed for over 400 years. A second red spot half smaller, appeared in 2006; visible at the bottom of the image, we see it passing on this series below the Great red spot without being disturbed by the huge cyclone. A third red spot, visible at the extreme left on the first image appeared at the beginning of 2008. We see her heading towards the Great red spot to appear on the last clash deformed and almost colorless. It seems his destiny is to be totally swallowed by the Great Red Spot. The time series shows the passage of the “” Red Spot Jr.”” in a band of clouds below (south) of the Great Red Spot (GRS). “” Red Spot Jr.”” first appeared on Jupiter in early 2006 when a previously white storm turne

Jupiter's Fusion Spots seen by the Hubble Space Telescope - Sequence of images of Jupiter's atmosphere obtained on May 15, June 28 and July 8, 2008 by the Hubble Space Telescope. The Great Red Spot of Jupiter is a gigantic permanent tempete measuring nearly 25,000 km in diameter. It's been observed for over 400 years. A second red spot half smaller, appeared in 2006; visible at the bottom of the image, we see it passing on this series below the Great red spot without being disturbed by the huge cyclone. A third red spot, visible at the extreme left on the first image appeared at the beginning of 2008. We see her heading towards the Great red spot to appear on the last clash deformed and almost colorless. It seems his destiny is to be totally swallowed by the Great Red Spot. The time series shows the passage of the “” Red Spot Jr.”” in a band of clouds below (south) of the Great Red Spot (GRS). “” Red Spot Jr.”” first appeared on Jupiter in early 2006 when a previously white storm turne

PIX4574511

The 'Resolution' In a Gale, c.1678 (oil on canvas)

The 'Resolution' In a Gale, c.1678 (oil on canvas)

Velde, Willem van de, the Younger (1633-1707)

MMM7342591

The Battle of the Texel, 11-21 August 1673, late 17th century - early 18th century (oil on canvas on panel)

The Battle of the Texel, 11-21 August 1673, late 17th century - early 18th century (oil on canvas on panel)

Velde, Willem van de, the Younger (1633-1707)

MMM7337627

Portrait of a Man, probably Isaac Holmes, c.1755 (oil on canvas)

Portrait of a Man, probably Isaac Holmes, c.1755 (oil on canvas)

Theus, Jeremiah (1719-74)

WAM5321914

1940s WW2 documentary 'The Big Red One'

1940s WW2 documentary 'The Big Red One'

BOF6285984

Nebulae IC 2948 and 2944 in Centaur - A large southern emission nebula, IC 2948 - Nebula IC 2948 is a vast nebula located about 6000 years from Earth in the southern constellation of Centaur. It is associated with the cluster of stars IC 2944 near which Bok's blood cells are visible. A Bok's blood cell is a dark interstellar cloud of gases and dust that absorb light. If it condenses enough, it gives birth to new stars. IC2944 is a large HII region (star forming cloud) in the southern constellation of Centaurus. The bright blue star in the upper right is Lambda Centauri, one of the brightest stars in the southern sky.The cluster of hot blue stars to the right of center are illuminating the gases of IC2944 and causing it to glow in the red and magenta light of excited hydrogen. The compact black objects adjacent to the bright blue stars are called Thackeray's Globules named for the astronomer A.D. Thackeray who described these in 1950. Thackeray Globules are similar to Bok Globules which

Nebulae IC 2948 and 2944 in Centaur - A large southern emission nebula, IC 2948 - Nebula IC 2948 is a vast nebula located about 6000 years from Earth in the southern constellation of Centaur. It is associated with the cluster of stars IC 2944 near which Bok's blood cells are visible. A Bok's blood cell is a dark interstellar cloud of gases and dust that absorb light. If it condenses enough, it gives birth to new stars. IC2944 is a large HII region (star forming cloud) in the southern constellation of Centaurus. The bright blue star in the upper right is Lambda Centauri, one of the brightest stars in the southern sky.The cluster of hot blue stars to the right of center are illuminating the gases of IC2944 and causing it to glow in the red and magenta light of excited hydrogen. The compact black objects adjacent to the bright blue stars are called Thackeray's Globules named for the astronomer A.D. Thackeray who described these in 1950. Thackeray Globules are similar to Bok Globules which

R. Gendler

PIX4622567

Antares star and the nebula Rho Ophiuchi - Antares and Rho Ophiuchi cloud - This coloree nebula represents the visible part of a very large molecule cloud, the cloud of Ophiuchus. This star-forming region is about 520 years old - light. The brightest star at the bottom left is the star Antares, from the Scorpio. The triple star Rho Ophiuchus is located in the middle of the blue cloud at the top of the picture. On the right, surrounded by a nebula, the star Sigma Scorpii. The globular clusters M4 (at the bottom of the image) and NGC 6144 (near Antares) are also visible on this image obtained with the UK Schmidt telescope of 1.2m. This photograph shows a portion of a great swath of obscuring gas and dust in the constellations Ophiuchus and Scorpius, and illustrates what is probably the most colourful region in the entire sky. The almost garish colours are due to the brilliance and contrasting colours of the stars, by whose reflected light we see the dust clouds. Dominating the picture is

Antares star and the nebula Rho Ophiuchi - Antares and Rho Ophiuchi cloud - This coloree nebula represents the visible part of a very large molecule cloud, the cloud of Ophiuchus. This star-forming region is about 520 years old - light. The brightest star at the bottom left is the star Antares, from the Scorpio. The triple star Rho Ophiuchus is located in the middle of the blue cloud at the top of the picture. On the right, surrounded by a nebula, the star Sigma Scorpii. The globular clusters M4 (at the bottom of the image) and NGC 6144 (near Antares) are also visible on this image obtained with the UK Schmidt telescope of 1.2m. This photograph shows a portion of a great swath of obscuring gas and dust in the constellations Ophiuchus and Scorpius, and illustrates what is probably the most colourful region in the entire sky. The almost garish colours are due to the brilliance and contrasting colours of the stars, by whose reflected light we see the dust clouds. Dominating the picture is

PIX4621421

Pistol star - Massive star in the constellation Sagittarius - The massive star Pistol star in Sagittarius - Pistol star is one of the most massive stars in our galaxy. Located about 25,000 years ago - the light of the Earth in the constellation of Sagittarius, this star shines like 10 million Sun consuming in six seconds as much energy as our star in a year. This star is masked by the numerous interstellar dust present in the Sagittarius near the galactic center and appears only in infrared wavelengths, as in this image obtained with the NICMOS instrument embark on the Hubble space telescope. The nebula that surrounds it (in the shape of a gun), extends over 4 years - light. Image obtained in 1997. Astronomers using Nasa's Hubble Space Telescope have identified what may be the most luminous star known “” a celestial mammoth which releases up to 10 million times the power of the Sun and is big enough to fill the diameter of Earth's orbit. The star unleashes as much energy in six seconds

Pistol star - Massive star in the constellation Sagittarius - The massive star Pistol star in Sagittarius - Pistol star is one of the most massive stars in our galaxy. Located about 25,000 years ago - the light of the Earth in the constellation of Sagittarius, this star shines like 10 million Sun consuming in six seconds as much energy as our star in a year. This star is masked by the numerous interstellar dust present in the Sagittarius near the galactic center and appears only in infrared wavelengths, as in this image obtained with the NICMOS instrument embark on the Hubble space telescope. The nebula that surrounds it (in the shape of a gun), extends over 4 years - light. Image obtained in 1997. Astronomers using Nasa's Hubble Space Telescope have identified what may be the most luminous star known “” a celestial mammoth which releases up to 10 million times the power of the Sun and is big enough to fill the diameter of Earth's orbit. The star unleashes as much energy in six seconds

PIX4572084

Djorgovski globular cluster 1 in Scorpio - Globular cluster Djorgovski 1 in Scorpius - The Djorgovski globular cluster 1 is a cluster of light stars located near the galactic center, 40,000 years - light from Earth. Its discovery is recent (1987) and studies show that its stars are composed only of hydrogene and helium. The absence of heavier elements that are usually present in stars remains an enigma. Image obtained by the Hubble Space Telescope (HST). The NASA/ESA Hubble Space Telescope has imaged an area so jam - packed with stars that they almost overwhelm the inky blackness of space. This includes the globular star cluster Djorgovski 1, which was only discovered in 1987 Djorgovski 1 is located close to the centre of our Milky Way Galaxy, within the bulge. If the galaxy is thought of as being like a city, then this bulge is the very busiest district at its centre. Djorgovski 1's proximity to this hub - - within just a few degrees - - explains why the picture is teeming with stars.

Djorgovski globular cluster 1 in Scorpio - Globular cluster Djorgovski 1 in Scorpius - The Djorgovski globular cluster 1 is a cluster of light stars located near the galactic center, 40,000 years - light from Earth. Its discovery is recent (1987) and studies show that its stars are composed only of hydrogene and helium. The absence of heavier elements that are usually present in stars remains an enigma. Image obtained by the Hubble Space Telescope (HST). The NASA/ESA Hubble Space Telescope has imaged an area so jam - packed with stars that they almost overwhelm the inky blackness of space. This includes the globular star cluster Djorgovski 1, which was only discovered in 1987 Djorgovski 1 is located close to the centre of our Milky Way Galaxy, within the bulge. If the galaxy is thought of as being like a city, then this bulge is the very busiest district at its centre. Djorgovski 1's proximity to this hub - - within just a few degrees - - explains why the picture is teeming with stars.

PIX4565206

Marcus Aurelius, 139-150 (marble)

Marcus Aurelius, 139-150 (marble)

Roman, (2nd century)

ROC3706866

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

Centaur Omega globular cluster - NGC 5139 Omega Centauri globular cluster - Visible to the naked eye in the southern hemisphere, Centaurus Omega is the most massive globular cluster in the galaxy. About 17,000 light years ago, millions of stars nearly 12 billion years old are concentrated here. This image obtained by the Spitzer space telescope reveals in yellow and red the big red stars, whose dust radiates infrared, and in blue the smaller and less evoluted stars. Omega Centauri is the biggest and brightest of the more than 150 similar objects, called globular clusters, that orbit around the outside of our Milky Way galaxy. Stargazers at southern latitudes can spot the stellar gem with the naked eye in the constellation Centaurus. While the visible - light observations highlight the cluster's millions of jam - packed stars, Spitzer's infrared eyes reveal the dustier, more evolved stars tossed throughout the region. Globular clusters are some of the oldest objects in our universe. The

Centaur Omega globular cluster - NGC 5139 Omega Centauri globular cluster - Visible to the naked eye in the southern hemisphere, Centaurus Omega is the most massive globular cluster in the galaxy. About 17,000 light years ago, millions of stars nearly 12 billion years old are concentrated here. This image obtained by the Spitzer space telescope reveals in yellow and red the big red stars, whose dust radiates infrared, and in blue the smaller and less evoluted stars. Omega Centauri is the biggest and brightest of the more than 150 similar objects, called globular clusters, that orbit around the outside of our Milky Way galaxy. Stargazers at southern latitudes can spot the stellar gem with the naked eye in the constellation Centaurus. While the visible - light observations highlight the cluster's millions of jam - packed stars, Spitzer's infrared eyes reveal the dustier, more evolved stars tossed throughout the region. Globular clusters are some of the oldest objects in our universe. The

PIX4564424

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

Star Formation in Galaxy M83 - Star Birth in Spiral galaxy M83 - Close-up of star-forming zones in the arms and near the nucleus (white region on the right) of the M83 galaxy. In red appear the hydrogen clouds in which the stars are born. The new stars are concentrated in blue clusters visible by hundreds on this image. The galaxy M83 (NGC 5236) is located about 15 million light years away from Earth in the constellation Hydra. This galaxy is intermediate between a classic spiral and a barree spiral. Image obtained by the Hubble space telescope with its wide field camera 3 (WFC3) in August 2009. Nicknamed the Southern Pinwheel, M83 is undergoing more rapid star formation than our own Milky Way galaxy, especially in its nucleus. The sharp “” eye”” of the Wide Field Camera 3 (WFC3) has captured hundreds of young star clusters, ancient swarms of globular star clusters, and hundreds of thousands of individual stars, mostly blue supergiants and red supergiants. The image, taken in August 20

Star Formation in Galaxy M83 - Star Birth in Spiral galaxy M83 - Close-up of star-forming zones in the arms and near the nucleus (white region on the right) of the M83 galaxy. In red appear the hydrogen clouds in which the stars are born. The new stars are concentrated in blue clusters visible by hundreds on this image. The galaxy M83 (NGC 5236) is located about 15 million light years away from Earth in the constellation Hydra. This galaxy is intermediate between a classic spiral and a barree spiral. Image obtained by the Hubble space telescope with its wide field camera 3 (WFC3) in August 2009. Nicknamed the Southern Pinwheel, M83 is undergoing more rapid star formation than our own Milky Way galaxy, especially in its nucleus. The sharp “” eye”” of the Wide Field Camera 3 (WFC3) has captured hundreds of young star clusters, ancient swarms of globular star clusters, and hundreds of thousands of individual stars, mostly blue supergiants and red supergiants. The image, taken in August 20

PIX4612521

Gladstone collection 3: Northern Territories, Ghana Part 3 c.1961

Gladstone collection 3: Northern Territories, Ghana Part 3 c.1961

BAF8619159

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

Saturday Sunday Monday, 1968

Saturday Sunday Monday, 1968

MOD6437289

Fromings Collection: Production of Malawi Darkfired Tobacco Part 3 1956

Fromings Collection: Production of Malawi Darkfired Tobacco Part 3 1956

BAF8619153

Portrait of Raja Ram Roy, son of Raja Ram Mohan Roy, 1833 A half-length portrait. He wears a pink turban with touches of green, yellow and white, a blue tunic with gold trimmings and a pink gold-spotted under-vest. He holds a map of Bengal in his right hand and is pointing with his left to Calcutta and Bengal. Raja Ram Roy is a somewhat mysterious figure. He appears to have been a Muslim orphan adopted by Raja Ram Mohan Roy (1772-1833). He accompanied his 'father' to England in 1831 and was present at his death at Stapleton Grove near Bristol on September 27, 1833. During this period Raja Ram Mohan Roy's portrait was also painted by H.P. Briggs, R.A. Raja Ram Roy stayed on in England and in August, 1835, was appointed 'for one year as an extra Clerk at the Board of Control at East India House with a salary of Â£100, to be charged among the contingencies of the office'. This appointment was a result of the interest taken in him by John Hobhouse (Lord Broughton), who had recently become

Portrait of Raja Ram Roy, son of Raja Ram Mohan Roy, 1833 A half-length portrait. He wears a pink turban with touches of green, yellow and white, a blue tunic with gold trimmings and a pink gold-spotted under-vest. He holds a map of Bengal in his right hand and is pointing with his left to Calcutta and Bengal. Raja Ram Roy is a somewhat mysterious figure. He appears to have been a Muslim orphan adopted by Raja Ram Mohan Roy (1772-1833). He accompanied his 'father' to England in 1831 and was present at his death at Stapleton Grove near Bristol on September 27, 1833. During this period Raja Ram Mohan Roy's portrait was also painted by H.P. Briggs, R.A. Raja Ram Roy stayed on in England and in August, 1835, was appointed 'for one year as an extra Clerk at the Board of Control at East India House with a salary of Â£100, to be charged among the contingencies of the office'. This appointment was a result of the interest taken in him by John Hobhouse (Lord Broughton), who had recently become

BL3304755

Bok's cells in NGC 281 (Cassiopee) - Bok globules in NGC 281 - View of a detail of the nebula NGC 281 in Cassiopee center on Bok's Globules. A Bok's blood cell is a dark interstellar cloud of gases and dust that absorb light. If it condenses enough, it gives birth to new stars. Near these blood cells shine blue stars; they belong to the young cluster of stars IC 1590. Image obtained by the Hubble Space Telescope in October 2005. These opaque, dark knots of gas and dust are called “” Bok globules,””” and they are absorbing light in the center of the nearby emission nebula and star - forming region. Bok hypothesized that giant molecular clouds, on the order of hundreds of light - years in size, can become perturbed and form small pockets where the dust and gas are highly concentrated. These small pockets become gravitationally bound and accumulate dust and gas from the surrounding area. If they can capture enough mass, they have the potential of creating stars in their cores; however, no

Bok's cells in NGC 281 (Cassiopee) - Bok globules in NGC 281 - View of a detail of the nebula NGC 281 in Cassiopee center on Bok's Globules. A Bok's blood cell is a dark interstellar cloud of gases and dust that absorb light. If it condenses enough, it gives birth to new stars. Near these blood cells shine blue stars; they belong to the young cluster of stars IC 1590. Image obtained by the Hubble Space Telescope in October 2005. These opaque, dark knots of gas and dust are called “” Bok globules,””” and they are absorbing light in the center of the nearby emission nebula and star - forming region. Bok hypothesized that giant molecular clouds, on the order of hundreds of light - years in size, can become perturbed and form small pockets where the dust and gas are highly concentrated. These small pockets become gravitationally bound and accumulate dust and gas from the surrounding area. If they can capture enough mass, they have the potential of creating stars in their cores; however, no

PIX4617491

Tenerife. 1978

LCS7223903

Galaxies Group: Stephan's Quintet in Pegase - Stephan's Quintet group of galaxies - Image obtained with the Hubble space telescope. This group of 5 galaxies is located about 270 million light years away from Earth. In this image three star-forming regions are visible: in the long arm of NGC 7319 (near the center); the gas debris of two galaxies, NGC 7318B and NGC 7318A (upper right); and in the upper left. Blue indicates that these stars are young. The NASA Hubble Space Telescope photo shows three regions of star birth: the long, sweeping tail and spiral arms of NGC 7319 [near center]; the gaseous debris of two galaxies, NGC 7318B and NGC 7318A [top right]; and the area north of those galaxies, dubbed the northern starburst region [top left]. The clusters' bluish color indicates that they're relatively young. Their ages span from about 2 million to more than 1 billion years old. The brilliant star clusters in NGC 7318B's spiral arm (about 30,000 light - years long) and the northern sta

Galaxies Group: Stephan's Quintet in Pegase - Stephan's Quintet group of galaxies - Image obtained with the Hubble space telescope. This group of 5 galaxies is located about 270 million light years away from Earth. In this image three star-forming regions are visible: in the long arm of NGC 7319 (near the center); the gas debris of two galaxies, NGC 7318B and NGC 7318A (upper right); and in the upper left. Blue indicates that these stars are young. The NASA Hubble Space Telescope photo shows three regions of star birth: the long, sweeping tail and spiral arms of NGC 7319 [near center]; the gaseous debris of two galaxies, NGC 7318B and NGC 7318A [top right]; and the area north of those galaxies, dubbed the northern starburst region [top left]. The clusters' bluish color indicates that they're relatively young. Their ages span from about 2 million to more than 1 billion years old. The brilliant star clusters in NGC 7318B's spiral arm (about 30,000 light - years long) and the northern sta

PIX4565466

'Jubilee', Herongate, Essex, 1935 (part 1)

'Jubilee', Herongate, Essex, 1935 (part 1)

ESS3483013

Daddy Deer, 1969 (16mm negative, 2K/Sound scan)

Daddy Deer, 1969 (16mm negative, 2K/Sound scan)

MOD6428975

'Jubilee', Herongate, Essex, 1935 (part 1)

'Jubilee', Herongate, Essex, 1935 (part 1)

ESS3483012

Six of the Duke of Newcastles Manège Horses

Six of the Duke of Newcastles Manège Horses

Anglo-Flemish School, (17th century)

USB1159685

Group portrait of all the original officers and men of the 11th Battalion, 3rd Brigade, AIF, 10 January 1915 (b/w photo)

Group portrait of all the original officers and men of the 11th Battalion, 3rd Brigade, AIF, 10 January 1915 (b/w photo)

Australian Photographer (20th century)

MEM1268284

Victoria Cross, 2nd Lieutenant R P Hallowes, Duke of Cambridge's Own (Middlesex Regiment), 1915 (metal)

Victoria Cross, 2nd Lieutenant R P Hallowes, Duke of Cambridge's Own (Middlesex Regiment), 1915 (metal)

British School, (20th century)

NAM5921596

Victoria Cross, 2nd Lieutenant R P Hallowes, Duke of Cambridge's Own (Middlesex Regiment), 1915 (metal)

Victoria Cross, 2nd Lieutenant R P Hallowes, Duke of Cambridge's Own (Middlesex Regiment), 1915 (metal)

British School, (20th century)

NAM5921595

Supposed Portrait of Mary of Guise, Queen of Scotland (15151560)

Supposed Portrait of Mary of Guise, Queen of Scotland (15151560)

English School, (17th century)

USB1160072

Called 'Bungay', the Favourite Dog of Sir John Harington (1561-1612)

Called 'Bungay', the Favourite Dog of Sir John Harington (1561-1612)

USB1159908

Lady Elizabeth Christiana Hervey, Lady Elizabeth Foster, later Duchess of Devonshire (1759-1824), 18th century (oil on canvas)

Lady Elizabeth Christiana Hervey, Lady Elizabeth Foster, later Duchess of Devonshire (1759-1824), 18th century (oil on canvas)

Kauffman, Angelica (1741-1807)

USB1156547

The Crucifix, ca. 1887 (oil on canvas)

The Crucifix, ca. 1887 (oil on canvas)

Martin, Henri Jean Guillaume (1860-1943)

XOS8982791

Chisman collection 14: Footage taken in Waziristan, 1937

Chisman collection 14: Footage taken in Waziristan, 1937

BAF7424521

Malecki Home Movie, 1952

Malecki Home Movie, 1952

MOV8613787

Astrolabe, c.1570 (gilt brass)

Astrolabe, c.1570 (gilt brass)

Flemish School, (16th century)

CH3057865

Naik Yeshwant Ghadge VC (1921-1944), 3/5th Mahratta Light Infantry, 1944 (b/w photo)

Naik Yeshwant Ghadge VC (1921-1944), 3/5th Mahratta Light Infantry, 1944 (b/w photo)

Unknown photographer, (20th century)

NAM5923543

Clip from THE RIGHT MAN, 1970

Clip from THE RIGHT MAN, 1970

IWF7405551

This representation of His Majesty's Ship 'Magnificent', 74 Guns..., 1830 (hand-coloured aquatint)

This representation of His Majesty's Ship 'Magnificent', 74 Guns..., 1830 (hand-coloured aquatint)

British School, (19th century)

MMM7342225

Chisman collection 15: Footage taken in Waziristan, 1937

Chisman collection 15: Footage taken in Waziristan, 1937

BAF7424519

Early flights of the North American X-15 rocket powered aircraft, 1959

Early flights of the North American X-15 rocket powered aircraft, 1959

BOF6284113

Liberation Of Rome, 1944

Liberation Of Rome, 1944

BOF8966955

Portugal. Birth of freedom, 1974

Portugal. Birth of freedom, 1974

MOD6437291

Parvenez Means Spring, 1976

Parvenez Means Spring, 1976

MOD6437288

News Events Post-War Japan 1946

News Events Post-War Japan 1946

BOF6286456

Battipaglia, 1969

Battipaglia, 1969

MOD6428900

From the north and south to Vietnam, 1967

From the north and south to Vietnam, 1967

MOD6437277

Release Of Watergate Tapes - President Richard M. Nixon

Release Of Watergate Tapes - President Richard M. Nixon

BOF7336651

President Bill Clinton - Affirmative Action Speech, 1995

President Bill Clinton - Affirmative Action Speech, 1995

BOF6286734

The Head-Quarters of Prince Frederick Charles at Corny, near Metz (engraving)

The Head-Quarters of Prince Frederick Charles at Corny, near Metz (engraving)

English School, (19th century)

LIP2773937

The Queen's Visit to the Prince of Wales, Arrival at Wolferton Station, near Sandringham (engraving)

The Queen's Visit to the Prince of Wales, Arrival at Wolferton Station, near Sandringham (engraving)

Robinson, Charles (1840-81)

LIP1626068

A Representation of the Battle on Drunmossie [sic] Moor near Culloden, 16 April 1746 (line engraving)

A Representation of the Battle on Drunmossie [sic] Moor near Culloden, 16 April 1746 (line engraving)

Bowles, John (1701-79)

NAM5919999

Residence of H.R.H. the Prince of Wales, Highgrove House, Doughton, Near Tetbury, 1981 (pencil & w/c on paper)

Residence of H.R.H. the Prince of Wales, Highgrove House, Doughton, Near Tetbury, 1981 (pencil & w/c on paper)

Tart, Spencer (b.1942)

XZL151590

Visit of Prince Albert (1819-61) to the Emperor Napoleon III (1808-73) on the heights near Boulogne, 8th September 1854 (oil on canvas)

Visit of Prince Albert (1819-61) to the Emperor Napoleon III (1808-73) on the heights near Boulogne, 8th September 1854 (oil on canvas)

Prades, Alfred de (fl.c.1862-79)

CH256932

Benrath Castle, 1806 (oil on canvas)

Benrath Castle, 1806 (oil on canvas)

Vernet, Antoine Charles Horace (Carle) (1758-1836)

XIR415746

Culloden moor battlefield memorial, early 21st century (photo)

Culloden moor battlefield memorial, early 21st century (photo)

PNP3697328

The woodcutters, 1779 (oil on canvas)

The woodcutters, 1779 (oil on canvas)

Goya y Lucientes, Francisco Jose de (1746-1828)

XIR488625

The meeting of the Duke of Wellington and Prince Bluecher, 1818 (watercolour on paper)

The meeting of the Duke of Wellington and Prince Bluecher, 1818 (watercolour on paper)

Warren, Charles Turner (1762-1823)

FIA5395903

Vase with flowers, c.1670-80 (oil on canvas)

Vase with flowers, c.1670-80 (oil on canvas)

Heem, Cornelis de (1631-95)

RTR5891868

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