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Nebula NGC 3372 in the Carene - NGC 3372, Eta Carinae nebula - The nebula of the Carene is located about 8000 years - light from the Earth. It is home to many hot massive stars, including the star Eta Carinae in the centre of the nebula. This nebula is larger than the Great Nebula in Orion, but is not visible from most northern latitudes. It is a giant complex of emission and dark nebulae surrounding the unique variable star Eta Carinae, which scientists believe is the most massive and energetic star in the Milky Way galaxy. Located about 8,500 light years from the Earth, the star is about 100 times as massive as our own Sun, but produces 6 million times the light output. It was observed producing a remarkable burst of X - ray emissions that doubled its X - ray output in only four months. In the 1840's, Eta Carinae erupted visibly and was the second brightest star in the sky during this time

Nebula NGC 3372 in the Carene - NGC 3372, Eta Carinae nebula - The nebula of the Carene is located about 8000 years - light from the Earth. It is home to many hot massive stars, including the star Eta Carinae in the centre of the nebula. This nebula is larger than the Great Nebula in Orion, but is not visible from most northern latitudes. It is a giant complex of emission and dark nebulae surrounding the unique variable star Eta Carinae, which scientists believe is the most massive and energetic star in the Milky Way galaxy. Located about 8,500 light years from the Earth, the star is about 100 times as massive as our own Sun, but produces 6 million times the light output. It was observed producing a remarkable burst of X - ray emissions that doubled its X - ray output in only four months. In the 1840's, Eta Carinae erupted visibly and was the second brightest star in the sky during this time

Jerry Lodriguss

PIX4618875

Visvamitra visits Vasishtha's hermitage, Kulu, Punjab Hills, 1700 (w/c & gold on paper)

Visvamitra visits Vasishtha's hermitage, Kulu, Punjab Hills, 1700 (w/c & gold on paper)

Indian School, (18th century)

UEA420214

Mahmud in his bloodstained Jibba, captured at the Battle of Atbara, 8th April 1898 (b/w photo)

Mahmud in his bloodstained Jibba, captured at the Battle of Atbara, 8th April 1898 (b/w photo)

NAM2973859

Spiral Galaxy M31 in Andromede - Spiral galaxy M31 in Andromeda - The galaxy of Andromede is located about 2 million years ago - light from Earth. Two satellite galaxies accompany it: M32 (NGC 221) in the center left, and M110 (NGC 205) below. Like the lactee path, the Andromede galaxy belongs to the local group, making up about thirty galaxies. M31, the Great galaxy in Andromeda, is a gigantic collection of more than 300 billion stars and is located about 2 million light years from Earth. Companion dwarf elliptical galaxies M32 and M110 are also visible. M31 and its companions are part of our local group of galaxies, which includes the Milky Way and Magellanic Clouds, and M33. The Andromeda Galaxy is headed towards our Milky Way Galaxy and is expected to collide with it and possibly merge into a gigantic elliptical galaxy in about 3 billion years

Spiral Galaxy M31 in Andromede - Spiral galaxy M31 in Andromeda - The galaxy of Andromede is located about 2 million years ago - light from Earth. Two satellite galaxies accompany it: M32 (NGC 221) in the center left, and M110 (NGC 205) below. Like the lactee path, the Andromede galaxy belongs to the local group, making up about thirty galaxies. M31, the Great galaxy in Andromeda, is a gigantic collection of more than 300 billion stars and is located about 2 million light years from Earth. Companion dwarf elliptical galaxies M32 and M110 are also visible. M31 and its companions are part of our local group of galaxies, which includes the Milky Way and Magellanic Clouds, and M33. The Andromeda Galaxy is headed towards our Milky Way Galaxy and is expected to collide with it and possibly merge into a gigantic elliptical galaxy in about 3 billion years

R. Gendler

PIX4608810

Spiral Galaxy M31 in Andromede - Spiral galaxy M31 in Andromeda - The galaxy of Andromede is located about 2 million years ago - light from Earth. Two satellite galaxies accompany it: M32 (NGC 221) in the center left, and M110 (NGC 205) below. Like the lactee path, the Andromede galaxy belongs to the local group, making up about thirty galaxies. Image made with an amateur instrument, a 130 mm bezel, several composite images. M31, the Great galaxy in Andromeda, is a gigantic collection of more than 300 billion stars and is located about 2 million light years from Earth. Companion dwarf elliptical galaxies M32 and M110 are also visible. M31 and its companions are part of our local group of galaxies, which includes the Milky Way and Magellanic Clouds, and M33. The Andromeda Galaxy is headed towards our Milky Way Galaxy and is expected to collide with it and possibly merge into a gigantic elliptical galaxy in about 3 billion years

Spiral Galaxy M31 in Andromede - Spiral galaxy M31 in Andromeda - The galaxy of Andromede is located about 2 million years ago - light from Earth. Two satellite galaxies accompany it: M32 (NGC 221) in the center left, and M110 (NGC 205) below. Like the lactee path, the Andromede galaxy belongs to the local group, making up about thirty galaxies. Image made with an amateur instrument, a 130 mm bezel, several composite images. M31, the Great galaxy in Andromeda, is a gigantic collection of more than 300 billion stars and is located about 2 million light years from Earth. Companion dwarf elliptical galaxies M32 and M110 are also visible. M31 and its companions are part of our local group of galaxies, which includes the Milky Way and Magellanic Clouds, and M33. The Andromeda Galaxy is headed towards our Milky Way Galaxy and is expected to collide with it and possibly merge into a gigantic elliptical galaxy in about 3 billion years

Jerry Lodriguss

PIX4608685

Visible Crab Nebula - Infrared and X - The Crab Nebula - M1, the Crab Nebula, is the rest of a supernova that exploded on July 4, 1054. It is located about 7000 light years from Earth in the constellation Taurus. At the heart of this nebula is a pulsar. To obtain this photo, three spatial observatories combined their observations: the Hubble telescope for the visible part (here in red and yellow), the Chandra telescope for the X-ray data (blue) and the Spitzer telescope for the infrared image (purple). The pulsar is the bright spot in the center of the image. The Crab Nebula (M1) is a supernova remnant at about 7,000 light - year from Earth in the constellation Taurus. The star explosion occured on July 04 1054. At the center of this nebula lies a pulsar. This composite image uses data from three of Nasa's Great Observatories. The Chandra X - ray image is shown in blue, the Hubble Space Telescope optical images are in red and yellow, and the Spitzer Space Telescope's infrared image is

Visible Crab Nebula - Infrared and X - The Crab Nebula - M1, the Crab Nebula, is the rest of a supernova that exploded on July 4, 1054. It is located about 7000 light years from Earth in the constellation Taurus. At the heart of this nebula is a pulsar. To obtain this photo, three spatial observatories combined their observations: the Hubble telescope for the visible part (here in red and yellow), the Chandra telescope for the X-ray data (blue) and the Spitzer telescope for the infrared image (purple). The pulsar is the bright spot in the center of the image. The Crab Nebula (M1) is a supernova remnant at about 7,000 light - year from Earth in the constellation Taurus. The star explosion occured on July 04 1054. At the center of this nebula lies a pulsar. This composite image uses data from three of Nasa's Great Observatories. The Chandra X - ray image is shown in blue, the Hubble Space Telescope optical images are in red and yellow, and the Spitzer Space Telescope's infrared image is

PIX4583130

Spiral Galaxy M31 in Andromede - Spiral galaxy M31 in Andromeda - The galaxy of Andromede is located about 2 million years ago - light from Earth. Two satellite galaxies accompany it: M32 (NGC 221) at the top center, and M110 (NGC 205) at the bottom. Like the lactee path, the Andromede galaxy belongs to the local group, making up about thirty galaxies. Image obtained with an apochromatic bezel Televue 127is. 22 hours of laying. M31, the Great galaxy in Andromeda, is a gigantic collection of more than 300 billion stars and is located about 2 million light years from Earth. Companion dwarf elliptical galaxies M32 and M110 are also visible. M31 and its companions are part of our local group of galaxies, which includes the Milky Way and Magellanic Clouds, and M33. The Andromeda Galaxy is headed towards our Milky Way Galaxy and is expected to collide with it and possibly merge into a gigantic elliptical galaxy in about 3 billion years

Spiral Galaxy M31 in Andromede - Spiral galaxy M31 in Andromeda - The galaxy of Andromede is located about 2 million years ago - light from Earth. Two satellite galaxies accompany it: M32 (NGC 221) at the top center, and M110 (NGC 205) at the bottom. Like the lactee path, the Andromede galaxy belongs to the local group, making up about thirty galaxies. Image obtained with an apochromatic bezel Televue 127is. 22 hours of laying. M31, the Great galaxy in Andromeda, is a gigantic collection of more than 300 billion stars and is located about 2 million light years from Earth. Companion dwarf elliptical galaxies M32 and M110 are also visible. M31 and its companions are part of our local group of galaxies, which includes the Milky Way and Magellanic Clouds, and M33. The Andromeda Galaxy is headed towards our Milky Way Galaxy and is expected to collide with it and possibly merge into a gigantic elliptical galaxy in about 3 billion years

PIX4608828

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

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

PIX4620865

Andromede and Triangle Constellations - Constellations of Andromeda and Triangulum - The constellation of Andromede begins at the brilliant star Alpheratz, or Alpha Andromedae, one of the corners of the great square of Pegase. Alpheratz is the brightest star in the picture, on the right, and is located about 97 light years away from Earth. Mirach star, in the center of the image, is a giant red star situated about 200 years ago - light. The galaxy of Andromede, M31, is visible at the top of the picture. At the bottom of the mage, in the middle, the galaxy M33. The large open cluster NGC 752 is at the bottom left. The constellations of Andromeda, the Princess, and Triangulum, the Triangle, point the way to several deep - sky delights in the fall sky. Andromeda begins at the bright star Alpheratz, or Alpha Andromedae, one of the corners of the great square of Pegasus. Alpheratz is the brightest star in the image, near the right side of the frame and is located about 97 light years away f

Andromede and Triangle Constellations - Constellations of Andromeda and Triangulum - The constellation of Andromede begins at the brilliant star Alpheratz, or Alpha Andromedae, one of the corners of the great square of Pegase. Alpheratz is the brightest star in the picture, on the right, and is located about 97 light years away from Earth. Mirach star, in the center of the image, is a giant red star situated about 200 years ago - light. The galaxy of Andromede, M31, is visible at the top of the picture. At the bottom of the mage, in the middle, the galaxy M33. The large open cluster NGC 752 is at the bottom left. The constellations of Andromeda, the Princess, and Triangulum, the Triangle, point the way to several deep - sky delights in the fall sky. Andromeda begins at the bright star Alpheratz, or Alpha Andromedae, one of the corners of the great square of Pegasus. Alpheratz is the brightest star in the image, near the right side of the frame and is located about 97 light years away f

Jerry Lodriguss

PIX4588980

The First Council of Queen Victoria, 1838 (oil on canvas)

The First Council of Queen Victoria, 1838 (oil on canvas)

Wilkie, David (1785-1841)

ROC399116

Andromede and Triangle Constellations - Constellations of Andromeda and Triangulum - The constellation of Andromede begins at the brilliant star Alpheratz, or Alpha Andromedae, one of the corners of the great square of Pegase. Alpheratz is the brightest star in the picture, on the right, and is located about 97 light years away from Earth. Mirach star, in the center of the image, is a giant red star situated about 200 years ago - light. The galaxy of Andromede, M31, is visible at the top of the picture. At the bottom of the mage, in the middle, the galaxy M33. The large open cluster NGC 752 is at the bottom left. The constellations of Andromeda, the Princess, and Triangulum, the Triangle, point the way to several deep - sky delights in the fall sky. Andromeda begins at the bright star Alpheratz, or Alpha Andromedae, one of the corners of the great square of Pegasus. Alpheratz is the brightest star in the image, near the right side of the frame and is located about 97 light years away f

Andromede and Triangle Constellations - Constellations of Andromeda and Triangulum - The constellation of Andromede begins at the brilliant star Alpheratz, or Alpha Andromedae, one of the corners of the great square of Pegase. Alpheratz is the brightest star in the picture, on the right, and is located about 97 light years away from Earth. Mirach star, in the center of the image, is a giant red star situated about 200 years ago - light. The galaxy of Andromede, M31, is visible at the top of the picture. At the bottom of the mage, in the middle, the galaxy M33. The large open cluster NGC 752 is at the bottom left. The constellations of Andromeda, the Princess, and Triangulum, the Triangle, point the way to several deep - sky delights in the fall sky. Andromeda begins at the bright star Alpheratz, or Alpha Andromedae, one of the corners of the great square of Pegasus. Alpheratz is the brightest star in the image, near the right side of the frame and is located about 97 light years away f

Jerry Lodriguss

PIX4588973

Tarantula Nebula (NGC 2070) in the river bream - The Tarantula Nebula, around the 30 Dor cluster - The Tarantula Nebula (or 30 Bream) is the largest star-forming region of the Great Magellan Cloud. It is located 170,000 light years ago in the constellation Dorado (southern hemisphere). At the center of this nebula, the open cluster of R136 stars, clusters of hot and massive stars. Image obtained with Siding Spring's 3.9m telescope. This object is the only extra - galactic nebula which can be seen with the unaided eye. It is a faint patch of light at the eastern end of the Large Magellanic Cloud, 170,000 light years distant. A small telescope reveals narrow spindly tendrils of glowing gas which have been likened to the legs of a spider. The 'body' of the spider is the bright nebula seen at the centre of the photograph, while at its core is an extremely dense clump of very hot stars, until recently thought to a single, unusually massive star known as 30 Doradus. The very hot stars of 30

Tarantula Nebula (NGC 2070) in the river bream - The Tarantula Nebula, around the 30 Dor cluster - The Tarantula Nebula (or 30 Bream) is the largest star-forming region of the Great Magellan Cloud. It is located 170,000 light years ago in the constellation Dorado (southern hemisphere). At the center of this nebula, the open cluster of R136 stars, clusters of hot and massive stars. Image obtained with Siding Spring's 3.9m telescope. This object is the only extra - galactic nebula which can be seen with the unaided eye. It is a faint patch of light at the eastern end of the Large Magellanic Cloud, 170,000 light years distant. A small telescope reveals narrow spindly tendrils of glowing gas which have been likened to the legs of a spider. The 'body' of the spider is the bright nebula seen at the centre of the photograph, while at its core is an extremely dense clump of very hot stars, until recently thought to a single, unusually massive star known as 30 Doradus. The very hot stars of 30

PIX4618255

The Three Stars of Happiness, Wealth, and Longevity, Ming dynasty (1368–1644) c.1500 (ink & light colours on silk)

The Three Stars of Happiness, Wealth, and Longevity, Ming dynasty (1368–1644) c.1500 (ink & light colours on silk)

Wang Zhao (fl.1480-1540)

KFW3743040

Vortigern, King of Britain, enamoured with Rowena at the Banquet of Hengist, the Saxon General, 18th century (oil on canvas)

Vortigern, King of Britain, enamoured with Rowena at the Banquet of Hengist, the Saxon General, 18th century (oil on canvas)

Kauffman, Angelica (1741-1807)

USB1156278

Britain As It Was Devided In The Tyme of the Englishe Saxons especially during their Heptarchy (hand coloured copper engraving)

Britain As It Was Devided In The Tyme of the Englishe Saxons especially during their Heptarchy (hand coloured copper engraving)

Speed, John (1552-1629)

XCF291063

Dublin And S Ireland

Dublin And S Ireland

LTT7238297

Barnard's loop and constellation Orion - Barnard's loop and Orion constellation - The constellation Orion and its nebulae. The main stars of this constellation are two supergeants, Betelgeuse (red) on the top left and Rigel (blue) on the bottom right. In the center of the constellation are the three stars forming Orion's Belt (or Baldrier) and the dark nebula of the horse's head (IC434 - B33). Further down, the large Orion nebula (M42) vast star-forming region. Wrapping these nebulae, Barnard's loop, a circle-arch nebula that would come from the explosion of a supernova more than two million years ago. The Orion constellation and its nebulae. The two Orion's bright stars are both supergiant stars: Betelgeuse (a red one) and Rigel (blue one). The center of this constellation is the Orion Belt with the Horsehead nebula (IC 434 - B33). Lower, the great Orion nebula, M42, a large star forming region. Also visible on this image, the Barnard's loop, a very faint nebula. This is composite mos

Barnard's loop and constellation Orion - Barnard's loop and Orion constellation - The constellation Orion and its nebulae. The main stars of this constellation are two supergeants, Betelgeuse (red) on the top left and Rigel (blue) on the bottom right. In the center of the constellation are the three stars forming Orion's Belt (or Baldrier) and the dark nebula of the horse's head (IC434 - B33). Further down, the large Orion nebula (M42) vast star-forming region. Wrapping these nebulae, Barnard's loop, a circle-arch nebula that would come from the explosion of a supernova more than two million years ago. The Orion constellation and its nebulae. The two Orion's bright stars are both supergiant stars: Betelgeuse (a red one) and Rigel (blue one). The center of this constellation is the Orion Belt with the Horsehead nebula (IC 434 - B33). Lower, the great Orion nebula, M42, a large star forming region. Also visible on this image, the Barnard's loop, a very faint nebula. This is composite mos

R. Gendler

PIX4617896

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

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

PIX4620872

Charles II dancing at a ball at court, 1660 (oil on canvas)

Charles II dancing at a ball at court, 1660 (oil on canvas)

Janssens, Hieronymus (1624-93)

ROC412945

The Fortress of Gingee, Madras, 1816 A stronghold in the South Arcot District, about 80 miles south-west of Madras. In the centre of the picture is seen the Great Mountain (Rajagiri), a precipitous bluff some 600 feet high, crowned by a citadel. At the foot is the inner (principal) fort. On the right hand side of the picture rises the English Mountain (Kistnagiri), and on the left the hill of St. George (Chandraya Drug). Both were strongly fortified; and all three hills were linked by granite walls five feet thick and several miles in length. In the foreground, on the bank of what was once the moat, stand two Indian villagers, one of whom points to the ruins of Kistnagiri.

The Fortress of Gingee, Madras, 1816 A stronghold in the South Arcot District, about 80 miles south-west of Madras. In the centre of the picture is seen the Great Mountain (Rajagiri), a precipitous bluff some 600 feet high, crowned by a citadel. At the foot is the inner (principal) fort. On the right hand side of the picture rises the English Mountain (Kistnagiri), and on the left the hill of St. George (Chandraya Drug). Both were strongly fortified; and all three hills were linked by granite walls five feet thick and several miles in length. In the foreground, on the bank of what was once the moat, stand two Indian villagers, one of whom points to the ruins of Kistnagiri.

BL3304378

Cannon ball, 1704 (lead)

Cannon ball, 1704 (lead)

English School, (18th century)

NAM5921243

China: The tomb of Abakh Khoja, 17th century Sufi mystic, Kashgar, Xinjiang

China: The tomb of Abakh Khoja, 17th century Sufi mystic, Kashgar, Xinjiang

David Henley

PFH4072181

China: The tomb of Abakh Khoja, 17th century Sufi mystic, Kashgar, Xinjiang

China: The tomb of Abakh Khoja, 17th century Sufi mystic, Kashgar, Xinjiang

David Henley

PFH4072182

China: Pillar detail, Mosque at the tomb of Abakh Khoja, 17th century Sufi mystic, Kashgar, Xinjiang

China: Pillar detail, Mosque at the tomb of Abakh Khoja, 17th century Sufi mystic, Kashgar, Xinjiang

David Henley

PFH4072184

China: Mosque at the tomb of Abakh Khoja, 17th century Sufi mystic, Kashgar, Xinjiang

China: Mosque at the tomb of Abakh Khoja, 17th century Sufi mystic, Kashgar, Xinjiang

David Henley

PFH4072186

Feb. 11, 1954 - Suspended Girton Girl Students Arrive In London. The Indian girl students from Girton College, who were “rusticated” for four days were worried yesterday - about what their relatives in India will say. Anita Chakravarty said as she caught a train for London” We don't want our people in India to hear about this. a suspension of this kind is viewed with greater gravity in India”. Miss Chakravarty and Miss Ranjana Ray were with four other students when two men undergraduates knocked on the window of a ground-floor room in the women's college after midnight. The girls let them in, though men are not allowed in the college after 10 p.m. A tutor heard men's voices and investigated. the girls were suspended. (“Rusticating” means that a student must not approach within 25 miles of Great St. Mary's Church in the centre of Cambridge). Keystone Photo Shows: - Ranjana Ray (Left), and Anita Chakravarty, seen on their arrival in London yesterday. they will stay at the Y.W.C.A until t

Feb. 11, 1954 - Suspended Girton Girl Students Arrive In London. The Indian girl students from Girton College, who were “rusticated” for four days were worried yesterday - about what their relatives in India will say. Anita Chakravarty said as she caught a train for London” We don't want our people in India to hear about this. a suspension of this kind is viewed with greater gravity in India”. Miss Chakravarty and Miss Ranjana Ray were with four other students when two men undergraduates knocked on the window of a ground-floor room in the women's college after midnight. The girls let them in, though men are not allowed in the college after 10 p.m. A tutor heard men's voices and investigated. the girls were suspended. (“Rusticating” means that a student must not approach within 25 miles of Great St. Mary's Church in the centre of Cambridge). Keystone Photo Shows: - Ranjana Ray (Left), and Anita Chakravarty, seen on their arrival in London yesterday. they will stay at the Y.W.C.A until t

ZUM4915198

China: Mosque at the tomb of Abakh Khoja, 17th century Sufi mystic, Kashgar, Xinjiang

China: Mosque at the tomb of Abakh Khoja, 17th century Sufi mystic, Kashgar, Xinjiang

David Henley

PFH4072185

Tomb of the Emperor Akbur at Secundra (w/c and ink on paper)

Tomb of the Emperor Akbur at Secundra (w/c and ink on paper)

XCF276479

China: The tomb of Abakh Khoja, 17th century Sufi mystic, Kashgar, Xinjiang

China: The tomb of Abakh Khoja, 17th century Sufi mystic, Kashgar, Xinjiang

David Henley

PFH4072183

A Dutch ship close-hauled, c.1610 (oil on panel)

A Dutch ship close-hauled, c.1610 (oil on panel)

Anthonisz, Aert (c.1579/80-1620)

MMM7337734

Admiral Sir George Brydges Rodney, 1st Baron Rodney (1719-1792) with French Captive Ships after the Battle of the Saints, 12 April 1782

Admiral Sir George Brydges Rodney, 1st Baron Rodney (1719-1792) with French Captive Ships after the Battle of the Saints, 12 April 1782

Serres, Dominic (1722-93)

USB1156574

Add 15296 (1) f.68r, At the top centre, the three spend the night in the forest. Sita and Rama lie on one mat, his sword and bow beside him, while Laksmana seated on his mat reproves Rama for giving way to grief. At the bottom, they then proceed to the hermitage of Bharadvaja, on the bank of the Ganga at Prayaga where the Ganga and Yamuna meet. In this peaceful place, abounding in deer and bird life, they offer homage to the hermits and ask the advice of the great sage aSita where they might fix their dwelling in the forest, so that they might not be disturbed. He advises the travellers to seek out the Citrakuta mountain sixty miles to the west, a lovely spot abounding in fruit, flowers and animals, and much frequented by hermits.

Add 15296 (1) f.68r, At the top centre, the three spend the night in the forest. Sita and Rama lie on one mat, his sword and bow beside him, while Laksmana seated on his mat reproves Rama for giving way to grief. At the bottom, they then proceed to the hermitage of Bharadvaja, on the bank of the Ganga at Prayaga where the Ganga and Yamuna meet. In this peaceful place, abounding in deer and bird life, they offer homage to the hermits and ask the advice of the great sage aSita where they might fix their dwelling in the forest, so that they might not be disturbed. He advises the travellers to seek out the Citrakuta mountain sixty miles to the west, a lovely spot abounding in fruit, flowers and animals, and much frequented by hermits.

Indian School, (17th century)

BL3283003

Peace Celebrations, Indian Troops Marching Down Whitehall, 1919 (oil on canvas)

Peace Celebrations, Indian Troops Marching Down Whitehall, 1919 (oil on canvas)

Meeson, Dora (1869-1955)

NAM237637

Sir William Heathcote, Rev. William Heathcote and Major Gilbert out Hunting (oil on canvas)

Sir William Heathcote, Rev. William Heathcote and Major Gilbert out Hunting (oil on canvas)

Gardner, Daniel (1750-1805)

USB392845

NGC 1850 Star Cluster in Dorado - Double Cluster NGC 1850 in Dorado - The double cluster NGC 1850 is located in the galaxy of the Great Magellan Cloud. It contains a cluster of globular form, but young, 50 million years, in the center of the image and another cluster, at the bottom right, even younger (4 million years), consists of warm and blue stars and a few T - Tauri stars. NGC 1850, imaged here with the NASA/ESA Hubble Space Telescope, is an unusual double cluster that lies in the bar of the Large Magellanic Cloud, a satellite galaxy of our own Milky Way. After the 30 Doradus complex, NGC 1850 is the brightest star cluster in the Large Magellanic Cloud. It is representative of a special class of objects - young, globular - like star clusters - that have no counterpart in our own Galaxy. The two components of the cluster are both relatively young and consist of a main globular - like cluster in the centre and an even younger, smaller cluster, seen below and to the right, composed o

NGC 1850 Star Cluster in Dorado - Double Cluster NGC 1850 in Dorado - The double cluster NGC 1850 is located in the galaxy of the Great Magellan Cloud. It contains a cluster of globular form, but young, 50 million years, in the center of the image and another cluster, at the bottom right, even younger (4 million years), consists of warm and blue stars and a few T - Tauri stars. NGC 1850, imaged here with the NASA/ESA Hubble Space Telescope, is an unusual double cluster that lies in the bar of the Large Magellanic Cloud, a satellite galaxy of our own Milky Way. After the 30 Doradus complex, NGC 1850 is the brightest star cluster in the Large Magellanic Cloud. It is representative of a special class of objects - young, globular - like star clusters - that have no counterpart in our own Galaxy. The two components of the cluster are both relatively young and consist of a main globular - like cluster in the centre and an even younger, smaller cluster, seen below and to the right, composed o

PIX4567832

Palm Trees at Le Cannet, c.1924 (oil on canvas)

Palm Trees at Le Cannet, c.1924 (oil on canvas)

Bonnard, Pierre (1867-1947)

MAN5890580

March: Hebes Chasma - Mars: Hebes Chasma - Hebes Chasma is a basin of almost 8000 m deep located in the northern part of Valles Marineris, the great Martian canyon. At the centre of this depression is a stratified plateau that constitutes sedimentary deposits. Image obtained by the Mars Express probe in 2005. View of Hebes Chasma obtained by the High Resolution Stereo Camera (HRSC) on ESA's Mars Express spacecraft. Hebes Chasma is an enclosed trough, almost 8000 m deep, in Valles Marineris, the Grand Canyon of Mars. A mesa - like mountain is located in the center of Hebes Chasma. It reaches 8000 meters above the graben floor and extends almost to the top of the surrounding plain. The mountain is made up by numerous stacked rock layers. The layering may consists of remnants of the older plateau, lake sediments, wind blown sediments or volcanic rock. The rock layers were exposed by erosional processes. Newest data acquired by the OMEGA spectrometer on - board Mars Express revealed hydrat

March: Hebes Chasma - Mars: Hebes Chasma - Hebes Chasma is a basin of almost 8000 m deep located in the northern part of Valles Marineris, the great Martian canyon. At the centre of this depression is a stratified plateau that constitutes sedimentary deposits. Image obtained by the Mars Express probe in 2005. View of Hebes Chasma obtained by the High Resolution Stereo Camera (HRSC) on ESA's Mars Express spacecraft. Hebes Chasma is an enclosed trough, almost 8000 m deep, in Valles Marineris, the Grand Canyon of Mars. A mesa - like mountain is located in the center of Hebes Chasma. It reaches 8000 meters above the graben floor and extends almost to the top of the surrounding plain. The mountain is made up by numerous stacked rock layers. The layering may consists of remnants of the older plateau, lake sediments, wind blown sediments or volcanic rock. The rock layers were exposed by erosional processes. Newest data acquired by the OMEGA spectrometer on - board Mars Express revealed hydrat

PIX4616152

Globular cluster M71 in the Fleche - Globular cluster M71 in Sagitta - M71 is located about 12,000 light years away from Earth. Image of the central region of the cluster obtained by the Hubble space telescope. This NASA/ESA Hubble Space Telescope image shows a bright scattering of stars in the small constellation of Sagitta (the Arrow). This is the centre of the globular cluster Messier 71, a great ball of ancient stars on the edge of our galaxy around 13,000 light - years from Earth. M71 is around 27 light - years across. Globular clusters are like galactic suburbs, pockets of stars that exist on the edge of major galaxies. These clusters are tightly bound together by their gravitational attraction, hence their spherical shape and their name: globulus means little sphere”” in Latin. Around 150 such globular clusters are known to exist around our Milky Way, each one of them containing several hundred thousand stars. Despite being a familiar object, Messier 71's precise nature was disp

Globular cluster M71 in the Fleche - Globular cluster M71 in Sagitta - M71 is located about 12,000 light years away from Earth. Image of the central region of the cluster obtained by the Hubble space telescope. This NASA/ESA Hubble Space Telescope image shows a bright scattering of stars in the small constellation of Sagitta (the Arrow). This is the centre of the globular cluster Messier 71, a great ball of ancient stars on the edge of our galaxy around 13,000 light - years from Earth. M71 is around 27 light - years across. Globular clusters are like galactic suburbs, pockets of stars that exist on the edge of major galaxies. These clusters are tightly bound together by their gravitational attraction, hence their spherical shape and their name: globulus means little sphere”” in Latin. Around 150 such globular clusters are known to exist around our Milky Way, each one of them containing several hundred thousand stars. Despite being a familiar object, Messier 71's precise nature was disp

PIX4565068

The Holy Parent. (Saint Anne, surrounded by her three successive husbands, Salome (blue tunic, with pointed index finger), Cleophas (with red coat, father of Marie Cleophas) and Joachim, father of the Virgin (red coat, head resting on the fist). In the centre, Christ child jugs on his cradle, the Virgin Mary who supports him, Saint Anne wearing a bloody white and behind them, with his hands raised, Saint Joseph. The child facing Christ is Saint John the Evangelist, supported by his mother Mary Salome (daughter of Saint Anne and Salome, wife of Zebedee), with his left his groin son, Saint James the middle one leans on his pelerin stick and at the back, Saint Anthony the Great (or Saint Anthony the Hermit or Saint Anthony the Abbe) recognizable with his bell, which with Saint Francois of Assisi, visible to the extreme right, are the only ones who do not belong to the line of Saint Anne. Mary Cleophas is surrounded by her sons, from right to left Saint Jude, Saint Simon, Joseph the righte

The Holy Parent. (Saint Anne, surrounded by her three successive husbands, Salome (blue tunic, with pointed index finger), Cleophas (with red coat, father of Marie Cleophas) and Joachim, father of the Virgin (red coat, head resting on the fist). In the centre, Christ child jugs on his cradle, the Virgin Mary who supports him, Saint Anne wearing a bloody white and behind them, with his hands raised, Saint Joseph. The child facing Christ is Saint John the Evangelist, supported by his mother Mary Salome (daughter of Saint Anne and Salome, wife of Zebedee), with his left his groin son, Saint James the middle one leans on his pelerin stick and at the back, Saint Anthony the Great (or Saint Anthony the Hermit or Saint Anthony the Abbe) recognizable with his bell, which with Saint Francois of Assisi, visible to the extreme right, are the only ones who do not belong to the line of Saint Anne. Mary Cleophas is surrounded by her sons, from right to left Saint Jude, Saint Simon, Joseph the righte

Chalons, Simon de (active 1532-62)

Leonard de Selva

LSE4313983

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. This NASA/ESA Hubble Space Telescope image is a close - up view of the central part of Stephan's Quintet, giving a magnificent view of a gigantic cosmic collision. Stephan's Quintet, as its name implies, is a group of five galaxies (NGC7317, 7318A, 7318B, 7319 and 7320) and lies about 270 million light - years away in the constellation of Pegasus (North - west of the Great Square of Pegasus). A sixth galaxy (NGC 7320C) lies south - east of the other five (upper left - hand corner of the overview image). The galaxy group was the first of its

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. This NASA/ESA Hubble Space Telescope image is a close - up view of the central part of Stephan's Quintet, giving a magnificent view of a gigantic cosmic collision. Stephan's Quintet, as its name implies, is a group of five galaxies (NGC7317, 7318A, 7318B, 7319 and 7320) and lies about 270 million light - years away in the constellation of Pegasus (North - west of the Great Square of Pegasus). A sixth galaxy (NGC 7320C) lies south - east of the other five (upper left - hand corner of the overview image). The galaxy group was the first of its

PIX4565462

Historic center, the former Mail street, postcards shop in a pedestrian alle in the city centre Montpellier France. Sale of postcards in an alley near the Palace of Justice, Montpellier at a good price Traveling to Montpellier on a low budget is more than possible! The city itself is an open-air museum, Just look around to discover statues and works of art in every corner of the city, The most curious will only have to push the doors of the private mansions to discover authentic architectural wonders, In addition, with the beach 11 km away and public transport, the journey to the sea is made in no time, And if your weakness is nature, you can rent a bike at Vélomagg, for just € 1! As for shows, saying that culture is accessible to everyone is not a mere phrase, All festivals offer free shows and, for museum and show lovers, the Tourist Office has created the City Card, a card that will allow you to discover the city at a great price, 2020 (photo)

Historic center, the former Mail street, postcards shop in a pedestrian alle in the city centre Montpellier France. Sale of postcards in an alley near the Palace of Justice, Montpellier at a good price Traveling to Montpellier on a low budget is more than possible! The city itself is an open-air museum, Just look around to discover statues and works of art in every corner of the city, The most curious will only have to push the doors of the private mansions to discover authentic architectural wonders, In addition, with the beach 11 km away and public transport, the journey to the sea is made in no time, And if your weakness is nature, you can rent a bike at Vélomagg, for just € 1! As for shows, saying that culture is accessible to everyone is not a mere phrase, All festivals offer free shows and, for museum and show lovers, the Tourist Office has created the City Card, a card that will allow you to discover the city at a great price, 2020 (photo)

Sergi Reboredo

SRB6367755

Nebula NGC 3372 in the Carene - NGC 3372 Carina nebula - The Carene Nebula (NGC 3372) is a very large region of star formation visible in the southern hemisphere. Image obtained through 3 different filters that highlight oxygen (blue), hydrogen (green), and sulfur (red). The bright star in the center of the image is Eta Carinae, a super massive star. The Carina Nebula (also known as the Great Nebula in Carina, the Eta Carinae Nebula, or NGC 3372) is a large bright nebula that surrounds several open clusters of stars. Eta Carinae and HD 93129A, two of the most massive and luminous stars in our Milky Way galaxy, are among them. The nebula lies at an estimated distance between 6,500 and 10,000 light years from Earth. It is located in the constellation of Carina. The nebula contains multiple O - type stars. This nebula is one of the largest H II regions in the Milky Way. It has a visual magnitude of 1.0. The nebula is one of the largest diffuse nebulae in our skies. Although it is some fou

Nebula NGC 3372 in the Carene - NGC 3372 Carina nebula - The Carene Nebula (NGC 3372) is a very large region of star formation visible in the southern hemisphere. Image obtained through 3 different filters that highlight oxygen (blue), hydrogen (green), and sulfur (red). The bright star in the center of the image is Eta Carinae, a super massive star. The Carina Nebula (also known as the Great Nebula in Carina, the Eta Carinae Nebula, or NGC 3372) is a large bright nebula that surrounds several open clusters of stars. Eta Carinae and HD 93129A, two of the most massive and luminous stars in our Milky Way galaxy, are among them. The nebula lies at an estimated distance between 6,500 and 10,000 light years from Earth. It is located in the constellation of Carina. The nebula contains multiple O - type stars. This nebula is one of the largest H II regions in the Milky Way. It has a visual magnitude of 1.0. The nebula is one of the largest diffuse nebulae in our skies. Although it is some fou

Tom Davis

PIX4619112

The Bell Shrine of St Mura, 11th - 16th century (bronze, brass, silver, parcel-gilt, rock crystal and amber)

The Bell Shrine of St Mura, 11th - 16th century (bronze, brass, silver, parcel-gilt, rock crystal and amber)

TWC5863249

The Bell Shrine of St Mura, 11th - 16th century (bronze, brass, silver, parcel-gilt, rock crystal and amber)

The Bell Shrine of St Mura, 11th - 16th century (bronze, brass, silver, parcel-gilt, rock crystal and amber)

TWC5863248

The Bell Shrine of St Mura, 11th - 16th century (bronze, brass, silver, parcel-gilt, rock crystal and amber)

The Bell Shrine of St Mura, 11th - 16th century (bronze, brass, silver, parcel-gilt, rock crystal and amber)

TWC5863250

Globular cluster NGC 7006 - Globular cluster NGC 7006 - The globular cluster NGC 7006 is located in the constellation Dauphin about 135,000 years old - light from Earth. Image obtained by the Hubble Space Telescope (HST). This NASA/ESA Hubble Space Telescope image shows a compact and remote globular star cluster that lies in one of the smallest constellations in the night sky, Delphinus (The Dolphin). Due to its modest size, great distance and relatively low brightness, NGC 7006 is often ignored by amateur astronomers. But even remote globular clusters such as this one appear bright and clear when imaged by Hubble's Advanced Camera for Surveys. NGC 7006 resides in the outskirts of the Milky Way. It is about 135,000 light - years away, five times the distance between the Sun and the centre of the galaxy, and it is part of the galactic halo. This roughly spherical region of the Milky Way is made up of dark matter, gas and sparsely distributed stellar clusters. Like other remote globular

Globular cluster NGC 7006 - Globular cluster NGC 7006 - The globular cluster NGC 7006 is located in the constellation Dauphin about 135,000 years old - light from Earth. Image obtained by the Hubble Space Telescope (HST). This NASA/ESA Hubble Space Telescope image shows a compact and remote globular star cluster that lies in one of the smallest constellations in the night sky, Delphinus (The Dolphin). Due to its modest size, great distance and relatively low brightness, NGC 7006 is often ignored by amateur astronomers. But even remote globular clusters such as this one appear bright and clear when imaged by Hubble's Advanced Camera for Surveys. NGC 7006 resides in the outskirts of the Milky Way. It is about 135,000 light - years away, five times the distance between the Sun and the centre of the galaxy, and it is part of the galactic halo. This roughly spherical region of the Milky Way is made up of dark matter, gas and sparsely distributed stellar clusters. Like other remote globular

PIX4565129

After the Battle of Atbara, April 8th 1898 (oil on canvas)

After the Battle of Atbara, April 8th 1898 (oil on canvas)

Giles, Godfrey Douglas (1857-1941)

NAM5920204

Basement of the Savoy Hotel, c.1904 (b/w photo)

Basement of the Savoy Hotel, c.1904 (b/w photo)

CWA124896

Corner of the forecourt of the Savoy Hotel, c.1904 (b/w photo)

Corner of the forecourt of the Savoy Hotel, c.1904 (b/w photo)

CWA124895

General, The Hon. William Hervey (1732-1815)

General, The Hon. William Hervey (1732-1815)

Zoffany, Johann (1733-1810) (attr. to)

USB1156585

View of the back of the Savoy Hotel with shades on the windows, and the statue of Robert Raikes (1735-1811) in the Victoria Embankment Gardens, c.1904 (b&w photo)

View of the back of the Savoy Hotel with shades on the windows, and the statue of Robert Raikes (1735-1811) in the Victoria Embankment Gardens, c.1904 (b&w photo)

CWA124893

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

The Forecourt of the Savoy Hotel, c.1904 (b/w photo)

The Forecourt of the Savoy Hotel, c.1904 (b/w photo)

CWA124894

A Dining Room at the Savoy Hotel, c.1904 (b/w photo)

A Dining Room at the Savoy Hotel, c.1904 (b/w photo)

CWA124898

A Drawing Room in the Savoy Hotel, c.1904 (b/w photo)

A Drawing Room in the Savoy Hotel, c.1904 (b/w photo)

CWA124897

The back of the Savoy Hotel and Victoria Embankment Gardens, c.1904 (b/w photo)

The back of the Savoy Hotel and Victoria Embankment Gardens, c.1904 (b/w photo)

CWA124892

Grimspound II, 1995 (w/c on paper)

Grimspound II, 1995 (w/c on paper)

Stevens, Philip (b.1953)

UEA420504

Standing Stones I, Avebury, 1994 (oil on canvas)

Standing Stones I, Avebury, 1994 (oil on canvas)

Stevens, Philip (b.1953)

UEA420496

Postbridge, 1998 (oil on canvas)

Postbridge, 1998 (oil on canvas)

Stevens, Philip (b.1953)

UEA420523

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