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Nebulae IC 1283 - 84 and NGC 6589 - 90 in Sagittarius - Nebulosity in Sagittarius, NGC 6589 - 90 - These nebulae are located in Sagittarius at a distance of about 5900 light years from Earth. Image made with Siding Spring's 3.9m telescope. Our view towards the centre of the Galaxy is obscured by extensive clouds of interstellar dust in the direction of the constellation of Sagittarius. The large - scale, patchy nature of the obscuration can be seen with the unaided eye and it is evident on smaller scales from the uneven distribution of background stars across this picture. Light from bright stars within the dust produces the two blue reflection nebulae (NGC 6589 and 6590), and these stars are members of a loose open cluster of stars, NGC 6595 (Sharpless 37) which is at a distance of about 5,900 light years. A large, almost transparent cloud of hydrogen, mixed with traces of dust, glows with a characteristic magenta hue over most of the field of view. This is known as IC 1283, 1284 and

Nebulae IC 1283 - 84 and NGC 6589 - 90 in Sagittarius - Nebulosity in Sagittarius, NGC 6589 - 90 - These nebulae are located in Sagittarius at a distance of about 5900 light years from Earth. Image made with Siding Spring's 3.9m telescope. Our view towards the centre of the Galaxy is obscured by extensive clouds of interstellar dust in the direction of the constellation of Sagittarius. The large - scale, patchy nature of the obscuration can be seen with the unaided eye and it is evident on smaller scales from the uneven distribution of background stars across this picture. Light from bright stars within the dust produces the two blue reflection nebulae (NGC 6589 and 6590), and these stars are members of a loose open cluster of stars, NGC 6595 (Sharpless 37) which is at a distance of about 5,900 light years. A large, almost transparent cloud of hydrogen, mixed with traces of dust, glows with a characteristic magenta hue over most of the field of view. This is known as IC 1283, 1284 and

PIX4619870

Mme Darsonval, Paris, 1897-99 (wool, silk & lace)

Mme Darsonval, Paris, 1897-99 (wool, silk & lace)

French School, (19th century)

MAN7069628

Mme Darsonval, Paris, 1897-99 (wool, silk & lace)

Mme Darsonval, Paris, 1897-99 (wool, silk & lace)

French School, (19th century)

MAN7069636

Mme Darsonval, Paris, 1897-99 (wool, silk & lace)

Mme Darsonval, Paris, 1897-99 (wool, silk & lace)

French School, (19th century)

MAN7069641

Mme Darsonval, Paris, 1897-99 (wool, silk & lace)

Mme Darsonval, Paris, 1897-99 (wool, silk & lace)

French School, (19th century)

MAN7069642

Elephant tube nebula (VDB 142) in Cephee - The Elephant Trunk Nebula (VDB 142) in Cepheus - IC1396, VDB 142. Nebula located about 2700 years - light from Earth. The Elephant Trunk Nebula (IC 1396A) in Cepheus is part of the larger IC 1396 complex which spans a large area of the sky measuring 170 by 140 arc - minutes and is one of the brightest emission nebulae with a magnitude of 3.5. The western portion of IC 1396 contains the Elephant Trunk Nebula (IC 1396A) which is characterized with H - II emissions, dark lanes and globules as well as a small reflection nebula. The IC 1396 complex is technically a star cluster (aka Cr 439, Trumpler 37) owing to the presence of a developing open but loose cluster at the heart of this rich nebulosity. This open star cluster is comprised of 50 - 100 member stars which vary in brightness spanning an area of approximately 50 'in diameter and which are not very well detached from the background sky. This stellar nursery lies at a distance of 2,720 light

Elephant tube nebula (VDB 142) in Cephee - The Elephant Trunk Nebula (VDB 142) in Cepheus - IC1396, VDB 142. Nebula located about 2700 years - light from Earth. The Elephant Trunk Nebula (IC 1396A) in Cepheus is part of the larger IC 1396 complex which spans a large area of the sky measuring 170 by 140 arc - minutes and is one of the brightest emission nebulae with a magnitude of 3.5. The western portion of IC 1396 contains the Elephant Trunk Nebula (IC 1396A) which is characterized with H - II emissions, dark lanes and globules as well as a small reflection nebula. The IC 1396 complex is technically a star cluster (aka Cr 439, Trumpler 37) owing to the presence of a developing open but loose cluster at the heart of this rich nebulosity. This open star cluster is comprised of 50 - 100 member stars which vary in brightness spanning an area of approximately 50 'in diameter and which are not very well detached from the background sky. This stellar nursery lies at a distance of 2,720 light

Sebastian Voltmer

PIX4622327

(Whole folio) End of Psalm 34. Psalm 35 beginning with initial 'D', the head of a young queen with a gold crown. Border decoration including, in the lower margin, a bearded hooded man pulling aside his tunic to reveal the body of a hybrid grotesque with foliate tail. In the upper margin, an old man or woman in a cloak and a youth sit, conversing in sign language, using their hands. At the side, a young male acrobat, one leg raised, balances on his shoulders the swaying figure of a young woman. She is viewed from behind, and is wearing a fashionable purple gown with long loose sleeves

(Whole folio) End of Psalm 34. Psalm 35 beginning with initial 'D', the head of a young queen with a gold crown. Border decoration including, in the lower margin, a bearded hooded man pulling aside his tunic to reveal the body of a hybrid grotesque with foliate tail. In the upper margin, an old man or woman in a cloak and a youth sit, conversing in sign language, using their hands. At the side, a young male acrobat, one leg raised, balances on his shoulders the swaying figure of a young woman. She is viewed from behind, and is wearing a fashionable purple gown with long loose sleeves

BL3276449

Spiral Galaxy NGC 247 in the Whale - Spiral galaxy NGC 247 in Cetus - Dwarf spiral galaxy in the Whale, located about 11 million years ago - light from Earth. Image obtained with the 2.2 meter MPG/ESO telescope at the La Silla Observatory. The spiral galaxy NGC 247 is one of the closest spiral galaxies of the southern sky. In this view from the Wide Field Imager on the MPG/ESO 2.2 - metre telescope in Chile large numbers of the galaxy's component stars are clearly resolved and many glowing pink clouds of hydrogen, marking regions of active star formation, can be made out in the loose and ragged spiral arms. NGC 247 is part of the Sculptor Group. This is the nearest group of galaxies to our Local Group, which includes the Milky Way, but putting a precise value on such celestial distances is inherently difficult. Astronomers have reported that NGC 247 is more than a million light - years closer to the Milky Way than was previously thought, bringing its distance down to just over 11 milli

Spiral Galaxy NGC 247 in the Whale - Spiral galaxy NGC 247 in Cetus - Dwarf spiral galaxy in the Whale, located about 11 million years ago - light from Earth. Image obtained with the 2.2 meter MPG/ESO telescope at the La Silla Observatory. The spiral galaxy NGC 247 is one of the closest spiral galaxies of the southern sky. In this view from the Wide Field Imager on the MPG/ESO 2.2 - metre telescope in Chile large numbers of the galaxy's component stars are clearly resolved and many glowing pink clouds of hydrogen, marking regions of active star formation, can be made out in the loose and ragged spiral arms. NGC 247 is part of the Sculptor Group. This is the nearest group of galaxies to our Local Group, which includes the Milky Way, but putting a precise value on such celestial distances is inherently difficult. Astronomers have reported that NGC 247 is more than a million light - years closer to the Milky Way than was previously thought, bringing its distance down to just over 11 milli

PIX4609139

The Penitent Magdalene,previously inscribed 1599 (oil on canvas)

The Penitent Magdalene,previously inscribed 1599 (oil on canvas)

Palma Il Giovane (Jacopo Negretti) (1548-1628)

ROC3709176

Full dress uniform worn by Major-General C J B Hay,The Queen's Own Corps of Guides, Punjab Frontier Force Infantry, 1903 circa (fabric)

Full dress uniform worn by Major-General C J B Hay,The Queen's Own Corps of Guides, Punjab Frontier Force Infantry, 1903 circa (fabric)

British School, (20th century)

NAM5925562

Full dress uniform worn by Major-General C J B Hay,The Queen's Own Corps of Guides, Punjab Frontier Force Infantry, 1903 circa (fabric)

Full dress uniform worn by Major-General C J B Hay,The Queen's Own Corps of Guides, Punjab Frontier Force Infantry, 1903 circa (fabric)

British School, (20th century)

NAM5925565

West Indian Waitresses, c.1955 (oil on paper)

West Indian Waitresses, c.1955 (oil on paper)

Frankfurther, Eva (1930-58)

BUG3588347

Martian dunes in summer - Mars: Summer view of Dunes: Detail on dunes near the northern polar cap of Mars in summer. Image obtained by the HIRISE camera of the Mars Reconnaissance probe orbiter on 1 September 2008. HIRISE is a 50 cm telescope that observes visible and near infrared. This dune field formed near the base of the North Polar cap. Dunes require a source of loose particulate material to form. The source of the northern dune fields around the polar cap may be from the layers of dusty ice that are eroded by strong polar winds. This image was taken during the Martian northern summer, so there is no frost present on the dunes. The dunes closest to the base of the polar cap are long and parallel, indicating strong winds from the direction of the cap. As they get farther away from the polar cap, they start to form more crescent shaped dunes, called barchan dunes. Repeated observations by HiRise of dunes like these show measurable changes in some locations. This discovery adds to t

Martian dunes in summer - Mars: Summer view of Dunes: Detail on dunes near the northern polar cap of Mars in summer. Image obtained by the HIRISE camera of the Mars Reconnaissance probe orbiter on 1 September 2008. HIRISE is a 50 cm telescope that observes visible and near infrared. This dune field formed near the base of the North Polar cap. Dunes require a source of loose particulate material to form. The source of the northern dune fields around the polar cap may be from the layers of dusty ice that are eroded by strong polar winds. This image was taken during the Martian northern summer, so there is no frost present on the dunes. The dunes closest to the base of the polar cap are long and parallel, indicating strong winds from the direction of the cap. As they get farther away from the polar cap, they start to form more crescent shaped dunes, called barchan dunes. Repeated observations by HiRise of dunes like these show measurable changes in some locations. This discovery adds to t

PIX4580056

Full dress uniform worn by Major-General C J B Hay,The Queen's Own Corps of Guides, Punjab Frontier Force Infantry, 1903 circa (fabric)

Full dress uniform worn by Major-General C J B Hay,The Queen's Own Corps of Guides, Punjab Frontier Force Infantry, 1903 circa (fabric)

British School, (20th century)

NAM5925561

Full dress uniform worn by Major-General C J B Hay,The Queen's Own Corps of Guides, Punjab Frontier Force Infantry, 1903 circa (fabric)

Full dress uniform worn by Major-General C J B Hay,The Queen's Own Corps of Guides, Punjab Frontier Force Infantry, 1903 circa (fabric)

British School, (20th century)

NAM5925563

Full dress uniform worn by Major-General C J B Hay,The Queen's Own Corps of Guides, Punjab Frontier Force Infantry, 1903 circa (fabric)

Full dress uniform worn by Major-General C J B Hay,The Queen's Own Corps of Guides, Punjab Frontier Force Infantry, 1903 circa (fabric)

British School, (20th century)

NAM5925564

A design by Paquin. 'A new and very pretty skirt which is suitable for wearing at the sea-side, of lavender blue piqué, made for ... Mademoiselle Cécile Sorel. Width is given to the dress by the machine stictched folds which are left loose a little below the skirt. The bodice which is slightly pouched is cut in battlements, each square or tab being edged with tiny tucks and fastened by a crystal button: the yoke is entirely covered with guipure lace, while the bodice and sleeves are embroidered in white. The hat ... is of black rice straw trimmed with a wired velvet ribbon true lovers knot and a plume of black cocks feather'.

A design by Paquin. 'A new and very pretty skirt which is suitable for wearing at the sea-side, of lavender blue piqué, made for ... Mademoiselle Cécile Sorel. Width is given to the dress by the machine stictched folds which are left loose a little below the skirt. The bodice which is slightly pouched is cut in battlements, each square or tab being edged with tiny tucks and fastened by a crystal button: the yoke is entirely covered with guipure lace, while the bodice and sleeves are embroidered in white. The hat ... is of black rice straw trimmed with a wired velvet ribbon true lovers knot and a plume of black cocks feather'.

BL3302208

A Barn with a Still Life of Kitchen Utensils and a Sleeping Cook

A Barn with a Still Life of Kitchen Utensils and a Sleeping Cook

Teniers, David the Younger (1610-90) & Saftleven, Herman (1609-85)

USB1158799

Nebulae IC 1283 - 84 and NGC 6589 - 90 in Sagittarius - Nebulosity in Sagittarius, NGC 6589 - 90 - These nebulae are located in Sagittarius at a distance of about 5900 light years from Earth. Mosaic of images obtained with a telescope of 35 cm, 22 hours of poses. This rich nebula complex is located near the center of the galaxy where dust is ubiquitous and often partially obscures the view at visible wavelengths. The two bright blue clouds are NGC 6589 and NGC 6590. The clouds represent scattered starlight from two imbedded young blue stars. The two bright stars are part of a loose cluster known as NGC 6595. The diffuse magenta cloud is a complex HII region which absorbs the energy from the nearby bright stars and releases it in the visible red light of excited hydrogen. The HII clouds are known as IC 1283, IC 1284 and IC 4700. This region of our galaxy is rich with dust clouds and young stars which together produce the stunning reflection nebulae we see in the image. Mosaic of images

Nebulae IC 1283 - 84 and NGC 6589 - 90 in Sagittarius - Nebulosity in Sagittarius, NGC 6589 - 90 - These nebulae are located in Sagittarius at a distance of about 5900 light years from Earth. Mosaic of images obtained with a telescope of 35 cm, 22 hours of poses. This rich nebula complex is located near the center of the galaxy where dust is ubiquitous and often partially obscures the view at visible wavelengths. The two bright blue clouds are NGC 6589 and NGC 6590. The clouds represent scattered starlight from two imbedded young blue stars. The two bright stars are part of a loose cluster known as NGC 6595. The diffuse magenta cloud is a complex HII region which absorbs the energy from the nearby bright stars and releases it in the visible red light of excited hydrogen. The HII clouds are known as IC 1283, IC 1284 and IC 4700. This region of our galaxy is rich with dust clouds and young stars which together produce the stunning reflection nebulae we see in the image. Mosaic of images

R. Gendler

PIX4619883

Apr. 04, 1953 - When still being a millionaire - - I invited every year some hundered people at the anniversary of my firm and prepared Thuringian sausages for them. That's wh, I can it so excellently!” The man who says so does not have a screw loose. Werner Singer now selling hot and roasted sausages in Frankfort/Main was really millionaire - at least theoretioally on the paper. They called him the bus-king of Thuringia for he owned the largest bus-pool of Thuringia and the largest repair-shop now being” in the possession of the people” after the Russians had expropriated his propriety. Besides he also had two houses and extended estate. All this he had to leave behind him and behind the Iron Curtain when he came to Frankfort some weeks ago. As a man of energy he would notarouble anyone and opened a booth where he is selling hot sausage. Sow we can only. wait until Mr. Singer will be millionaire again for he is a man who can never be beaten. KEYSTONE MUNICH EXCLUSIVE PICTURE

Apr. 04, 1953 - When still being a millionaire - - I invited every year some hundered people at the anniversary of my firm and prepared Thuringian sausages for them. That's wh, I can it so excellently!” The man who says so does not have a screw loose. Werner Singer now selling hot and roasted sausages in Frankfort/Main was really millionaire - at least theoretioally on the paper. They called him the bus-king of Thuringia for he owned the largest bus-pool of Thuringia and the largest repair-shop now being” in the possession of the people” after the Russians had expropriated his propriety. Besides he also had two houses and extended estate. All this he had to leave behind him and behind the Iron Curtain when he came to Frankfort some weeks ago. As a man of energy he would notarouble anyone and opened a booth where he is selling hot sausage. Sow we can only. wait until Mr. Singer will be millionaire again for he is a man who can never be beaten. KEYSTONE MUNICH EXCLUSIVE PICTURE

ZUM4832952

Lucy Harington, Countess of Bedford, c.1612-16 (w/c on vellum)

Lucy Harington, Countess of Bedford, c.1612-16 (w/c on vellum)

Oliver, Isaac (c.1565-1617)

ROC5672288

Codex Arundel, MS 263 f.229v, Notes, displayed as an open bifolium with f. 226: text page, 1503 (pen & ink on paper)

Codex Arundel, MS 263 f.229v, Notes, displayed as an open bifolium with f. 226: text page, 1503 (pen & ink on paper)

Vinci, Leonardo da (1452-1519)

BL3067821

St Patrick's Isle Necklace, mid-late 10th century (glass, amber & jet)

St Patrick's Isle Necklace, mid-late 10th century (glass, amber & jet)

Viking, (10th century)

MNX3701178

Open cluster M11 in the ECU of Sobieski - M11 open cluster in Scutum - M11 (NGC 6705) is a cluster of about 3000 stars. Image obtained by Siding Spring Clusters of bright blue stars like M11 are found scattered among the spiral arms of the Milky Way and other galaxies like it. They are a clear sign that star formation is active, because such clusters are usually very young and short lived. The stars in M11 all formed from the same material and at about the same time, a few million years ago. In 100 million years or so, all the brightest stars in the group will have evolved into cool supergiants and exploded as supernovae, leaving behind large numbers of low mass, relatively faint stars whose lives will be much longer and whose end will be much less dramatic. Located in the constellation of Scutum, it is sometimes mistaken for a loose globular cluster. M11 is also called the “” Wild Duck Cluster”” because of it's resemblance to a flight of wild ducks when viewed in a telescope. M11, wit

Open cluster M11 in the ECU of Sobieski - M11 open cluster in Scutum - M11 (NGC 6705) is a cluster of about 3000 stars. Image obtained by Siding Spring Clusters of bright blue stars like M11 are found scattered among the spiral arms of the Milky Way and other galaxies like it. They are a clear sign that star formation is active, because such clusters are usually very young and short lived. The stars in M11 all formed from the same material and at about the same time, a few million years ago. In 100 million years or so, all the brightest stars in the group will have evolved into cool supergiants and exploded as supernovae, leaving behind large numbers of low mass, relatively faint stars whose lives will be much longer and whose end will be much less dramatic. Located in the constellation of Scutum, it is sometimes mistaken for a loose globular cluster. M11 is also called the “” Wild Duck Cluster”” because of it's resemblance to a flight of wild ducks when viewed in a telescope. M11, wit

PIX4568454

Sir Ralph Bankes, MP (?1631-1677)

Sir Ralph Bankes, MP (?1631-1677)

Lely, Peter (1618-80)

USB1156998

Madonna della sedia (after Raphael)

Madonna della sedia (after Raphael)

Raphael (Raffaello Sanzio of Urbino) (1483-1520) (after)

USB1161054

Queen Silvia of Sweden, 1981 (photo)

Queen Silvia of Sweden, 1981 (photo)

SJB8685063

Queen Silvia of Sweden, 1978 (photo)

Queen Silvia of Sweden, 1978 (photo)

SJB8685053

Queen Silvia of Sweden, 1983 (photo)

Queen Silvia of Sweden, 1983 (photo)

SJB8685067

Queen Silvia of Sweden, 1981 (photo)

Queen Silvia of Sweden, 1981 (photo)

SJB8685018

Two Chinese men carrying a load suspended from a pole between them, 1900 (Gelatine dry plate)

Two Chinese men carrying a load suspended from a pole between them, 1900 (Gelatine dry plate)

Jones, Kenneth Hurlstone (fl.c.1900)

MMM7341046

Elephant tube nebula (VDB 142) in Cephee - The Elephant Trunk Nebula (VDB 142) in Cepheus: IC1396, VDB 142. Nebula located about 2700 light years from Earth. Image obtained with a bezel Tele Vue NP127iS, through 3 different filters that demonstrate oxygen, hydrogen, and sulfur - The Elephant Trunk Nebula (IC 1396A) in Cepheus is part of the larger IC 1396 complex which spans a large area of the sky measuring 170 by 140 arc-minutes and is one of the brightest emission nebulae with a magnitude of 3.5. The western portion of IC 1396 contains the Elephant Trunk Nebula (IC 1396A) which is characterized with H-II emissions, dark lanes and globules as well as a small reflection nebula. The IC 1396 complex is technically a star cluster (aka Cr 439, Trumpler 37) owing to the presence of a developing open but loose cluster at the heart of this rich nebulosity. This open star cluster is comprised of 50-100 member stars which vary in brightness spanning an area of approximately 50 'in diameter and

Elephant tube nebula (VDB 142) in Cephee - The Elephant Trunk Nebula (VDB 142) in Cepheus: IC1396, VDB 142. Nebula located about 2700 light years from Earth. Image obtained with a bezel Tele Vue NP127iS, through 3 different filters that demonstrate oxygen, hydrogen, and sulfur - The Elephant Trunk Nebula (IC 1396A) in Cepheus is part of the larger IC 1396 complex which spans a large area of the sky measuring 170 by 140 arc-minutes and is one of the brightest emission nebulae with a magnitude of 3.5. The western portion of IC 1396 contains the Elephant Trunk Nebula (IC 1396A) which is characterized with H-II emissions, dark lanes and globules as well as a small reflection nebula. The IC 1396 complex is technically a star cluster (aka Cr 439, Trumpler 37) owing to the presence of a developing open but loose cluster at the heart of this rich nebulosity. This open star cluster is comprised of 50-100 member stars which vary in brightness spanning an area of approximately 50 'in diameter and

W. Promper

PIX4622329

Queen Silvia of Sweden, 1987 (photo)

Queen Silvia of Sweden, 1987 (photo)

SJB8685050

Queen Silvia of Sweden, 1987 (photo)

Queen Silvia of Sweden, 1987 (photo)

SJB8685051

Queen Silvia of Sweden, 1987 (photo)

Queen Silvia of Sweden, 1987 (photo)

SJB8685052

Rare and massive punchbowl, c.1775 (ceramic) (see also 3084896)

Rare and massive punchbowl, c.1775 (ceramic) (see also 3084896)

Chinese School (18th century)

CH3084896

Barree spiral galaxy NGC 1483 in Dorado - Barred spiral galaxy NGC 1483 in Dorado - NGC 1483 is a barree spiral galaxy located about 60 million years ago - light in the southern constellation of Dorado. Image obtained by the Hubble Space Telescope (HST). NGC 1483 is a barred spiral galaxy located in the southern constellation of Dorado. The nebulous galaxy features a bright central bulge and diffuse arms with distinct star - forming regions. In the background, many other distant galaxies can be seen. The constellation Dorado is home to the Dorado Group of galaxies, a loose group comprising an estimated 70 galaxies and located some 62 million light - years away. The Dorado group is much larger than the Local Group that includes the Milky Way (and which contains around 30 galaxies) and approaches the size of a galaxy cluster. Galaxy clusters are the largest groupings of galaxies (and indeed the largest structures of any type) in the Universe to be held together by their gravity. Barred s

Barree spiral galaxy NGC 1483 in Dorado - Barred spiral galaxy NGC 1483 in Dorado - NGC 1483 is a barree spiral galaxy located about 60 million years ago - light in the southern constellation of Dorado. Image obtained by the Hubble Space Telescope (HST). NGC 1483 is a barred spiral galaxy located in the southern constellation of Dorado. The nebulous galaxy features a bright central bulge and diffuse arms with distinct star - forming regions. In the background, many other distant galaxies can be seen. The constellation Dorado is home to the Dorado Group of galaxies, a loose group comprising an estimated 70 galaxies and located some 62 million light - years away. The Dorado group is much larger than the Local Group that includes the Milky Way (and which contains around 30 galaxies) and approaches the size of a galaxy cluster. Galaxy clusters are the largest groupings of galaxies (and indeed the largest structures of any type) in the Universe to be held together by their gravity. Barred s

PIX4609879

Queen Silvia of Sweden, 1987 (photo)

Queen Silvia of Sweden, 1987 (photo)

SJB8685049

Queen Silvia of Sweden, 1992 (photo)

Queen Silvia of Sweden, 1992 (photo)

SJB8685055

Phyllis 1st Lieutenant spaniel dog on top of barrel with hat and pipe. From an album relating to the Royal Naval Service of Cdr John Rodolph Peronet Thompson RN., 1909-16 (photo, paper)

Phyllis 1st Lieutenant spaniel dog on top of barrel with hat and pipe. From an album relating to the Royal Naval Service of Cdr John Rodolph Peronet Thompson RN., 1909-16 (photo, paper)

Thompson, John Rodolph (1892-1965)

MMM7342509

A Boy and a Girl and a Blackamoor Page

A Boy and a Girl and a Blackamoor Page

Anglo-Dutch School, (17th century)

USB1157783

Rare and massive punchbowl, c.1775 (ceramic) (see also 3084896)

Rare and massive punchbowl, c.1775 (ceramic) (see also 3084896)

Chinese School (18th century)

CH3084897

Elephant tube nebula (VDB 142) in Cephee - The Elephant Trunk Nebula (VDB 142) in Cepheus - IC1396, VDB 142. Nebula located about 2700 years - light from Earth. Image obtained with a telescope 40 cm in diameter, through 3 different filters that highlight oxygen, hydrogen, and sulfur. The Elephant Trunk Nebula (IC 1396A) in Cepheus is part of the larger IC 1396 complex which spans a large area of the sky measuring 170 by 140 arc - minutes and is one of the brightest emission nebulae with a magnitude of 3.5. The western portion of IC 1396 contains the Elephant Trunk Nebula (IC 1396A) which is characterized with H - II emissions, dark lanes and globules as well as a small reflection nebula. The IC 1396 complex is technically a star cluster (aka Cr 439, Trumpler 37) owing to the presence of a developing open but loose cluster at the heart of this rich nebulosity. This open star cluster is comprised of 50 - 100 member stars which vary in brightness spanning an area of approximately 50 'in d

Elephant tube nebula (VDB 142) in Cephee - The Elephant Trunk Nebula (VDB 142) in Cepheus - IC1396, VDB 142. Nebula located about 2700 years - light from Earth. Image obtained with a telescope 40 cm in diameter, through 3 different filters that highlight oxygen, hydrogen, and sulfur. The Elephant Trunk Nebula (IC 1396A) in Cepheus is part of the larger IC 1396 complex which spans a large area of the sky measuring 170 by 140 arc - minutes and is one of the brightest emission nebulae with a magnitude of 3.5. The western portion of IC 1396 contains the Elephant Trunk Nebula (IC 1396A) which is characterized with H - II emissions, dark lanes and globules as well as a small reflection nebula. The IC 1396 complex is technically a star cluster (aka Cr 439, Trumpler 37) owing to the presence of a developing open but loose cluster at the heart of this rich nebulosity. This open star cluster is comprised of 50 - 100 member stars which vary in brightness spanning an area of approximately 50 'in d

PIX4622303

Henrietta Georgiana Marcia Lascelles Iremonger, Lady Chatterton (1806 1876), Mrs Edward Heneage Dering

Henrietta Georgiana Marcia Lascelles Iremonger, Lady Chatterton (1806 1876), Mrs Edward Heneage Dering

Orpen, Rebecca Dulcibella (1830-1923)

USB1160637

Charlotte Gilding, Lady Iliffe (1881 -1972)

Charlotte Gilding, Lady Iliffe (1881 -1972)

Jameson, Cecil Stuart (1883-c.1937)

USB1160671

A Collector in his Study

A Collector in his Study

Verlin, Venceslao (fl.1768-d.1780)

USB1159703

Sigurd Cross Slab, c.1906 (ink & pencil on paper)

Sigurd Cross Slab, c.1906 (ink & pencil on paper)

Kermode, Philip Moore Callow (1855-1932)

MNX3594335

Barree spiral galaxy NGC 1345 in Eridan - Barred Spiral galaxy NGC 1345 in Eridanus - Located about 85 million years ago - light from Earth, NGC 1345 is a barree spiral galaxy located in the constellation Eridan. This galaxy belongs to the Eridan galaxy cluster, a group of 70 galaxies. Many galaxies are visible in the background. The spiral galaxy NGC 1345 and its loose and ragged arms dominate this rich image from the NASA/ESA Hubble Space Telescope. It is a member of the Eridanus Galaxy Cluster - - a group of about 70 galaxies that lies 85 million light - years away in the constellation of Eridanus (the River). This region of the night sky is well populated with bright galaxies, with the Fornax Cluster of galaxies also nearby on the celestial sphere, although the two clusters are actually separated by about 20 million light - years. Collectively, they are known as the Fornax Supercluster or the Southern Supercluster. Apart from the main galaxy that dominates the picture, lots more di

Barree spiral galaxy NGC 1345 in Eridan - Barred Spiral galaxy NGC 1345 in Eridanus - Located about 85 million years ago - light from Earth, NGC 1345 is a barree spiral galaxy located in the constellation Eridan. This galaxy belongs to the Eridan galaxy cluster, a group of 70 galaxies. Many galaxies are visible in the background. The spiral galaxy NGC 1345 and its loose and ragged arms dominate this rich image from the NASA/ESA Hubble Space Telescope. It is a member of the Eridanus Galaxy Cluster - - a group of about 70 galaxies that lies 85 million light - years away in the constellation of Eridanus (the River). This region of the night sky is well populated with bright galaxies, with the Fornax Cluster of galaxies also nearby on the celestial sphere, although the two clusters are actually separated by about 20 million light - years. Collectively, they are known as the Fornax Supercluster or the Southern Supercluster. Apart from the main galaxy that dominates the picture, lots more di

PIX4609816

Dwarf galaxy Holmberg IX in the Great Bear - Dwarf galaxy Holmberg IX in Ursa Major - The dwarf galaxy Holmberg IX is located 12 million years - light from Earth in the constellation of the Great Bear, just above the spiral galaxy M81. Of the 20,000 stars visible on this image obtained by the Hubble space telescope, more than 90% are young stars aged between 10 and 200 million years. The proximity of other galaxies, including M81, is believed to be at the origin of this recent star formation. This loose collection of stars is actually a dwarf irregular galaxy, called Holmberg IX. It resides just off the outer edge of M81, a large spiral galaxy in Ursa Major. This image was taken with Hubble's Advanced Camera for Surveys in early 2006. Holmberg IX is of the so - called Magellanic type of galaxy, as its size and irregularity in structure are similar to the Small Magellanic Cloud, a neighbour to our own Milky Way. It is suspected that the dwarf galaxy was created as a result of a galactic

Dwarf galaxy Holmberg IX in the Great Bear - Dwarf galaxy Holmberg IX in Ursa Major - The dwarf galaxy Holmberg IX is located 12 million years - light from Earth in the constellation of the Great Bear, just above the spiral galaxy M81. Of the 20,000 stars visible on this image obtained by the Hubble space telescope, more than 90% are young stars aged between 10 and 200 million years. The proximity of other galaxies, including M81, is believed to be at the origin of this recent star formation. This loose collection of stars is actually a dwarf irregular galaxy, called Holmberg IX. It resides just off the outer edge of M81, a large spiral galaxy in Ursa Major. This image was taken with Hubble's Advanced Camera for Surveys in early 2006. Holmberg IX is of the so - called Magellanic type of galaxy, as its size and irregularity in structure are similar to the Small Magellanic Cloud, a neighbour to our own Milky Way. It is suspected that the dwarf galaxy was created as a result of a galactic

PIX4613880

Sigurd Cross Slab (Manx Cross 121) (stone)

Sigurd Cross Slab (Manx Cross 121) (stone)

MNX5934749

Spiral galaxy NGC 1566 in the bream - The Seyfert Galaxy NGC 1566: NGC 1566 is a spiral galaxy located about 40 million light years ago. Its core is very bright. It is an active galaxy called Seyfert, which probably houses a black hole in its heart. Image obtained with the Hubble telescope - NGC 1566 is a galaxy located approximately 40 million light-years away in the constellation of Dorado (The Dolphinfish). NGC 1566 is an intermediate spiral galaxy, meaning that while it does not have a well defined bar-shaped region of stars at its centre - like barred spirals - it is not quite an unbarred spiral either (heic9902o). The small but extremely bright nucleus of NGC 1566 is clearly visible in this image, a telltale sign of its membership of the Seyfert class of galaxies. The centres of such galaxies are very active and luminous, emitting strong bursts of radiation and potentially harbouring supermassive black holes that are many millions of times the mass of the Sun. NGC 1566 is not jus

Spiral galaxy NGC 1566 in the bream - The Seyfert Galaxy NGC 1566: NGC 1566 is a spiral galaxy located about 40 million light years ago. Its core is very bright. It is an active galaxy called Seyfert, which probably houses a black hole in its heart. Image obtained with the Hubble telescope - NGC 1566 is a galaxy located approximately 40 million light-years away in the constellation of Dorado (The Dolphinfish). NGC 1566 is an intermediate spiral galaxy, meaning that while it does not have a well defined bar-shaped region of stars at its centre - like barred spirals - it is not quite an unbarred spiral either (heic9902o). The small but extremely bright nucleus of NGC 1566 is clearly visible in this image, a telltale sign of its membership of the Seyfert class of galaxies. The centres of such galaxies are very active and luminous, emitting strong bursts of radiation and potentially harbouring supermassive black holes that are many millions of times the mass of the Sun. NGC 1566 is not jus

PIX4609939

Eighty percent of the world's high quality jute grows in Bangladesh. Jute plant, the fiber of which is known as the golden fiber of Bangladesh, grows six to ten feet in height. It takes two to three months for the plants to grow up for harvest. After cutting, the plants are tied up in bundles and kept under water for a few weeks. When the stems rot and their bark become loose, farmers pull off the fiber from the bark and wash very carefully. Then the fiber is dried in the sun and put in bundles for sale. Jute grows well in moist and swampy lands. Bangladesh has plenty of low lands that go under water during rainy season. Jute is used for making cloth, shawl, ropes, carpet, bags and many other useful things. Jute sacks are very suitable for packing food grains. May 7, 2005. (photo)

Eighty percent of the world's high quality jute grows in Bangladesh. Jute plant, the fiber of which is known as the golden fiber of Bangladesh, grows six to ten feet in height. It takes two to three months for the plants to grow up for harvest. After cutting, the plants are tied up in bundles and kept under water for a few weeks. When the stems rot and their bark become loose, farmers pull off the fiber from the bark and wash very carefully. Then the fiber is dried in the sun and put in bundles for sale. Jute grows well in moist and swampy lands. Bangladesh has plenty of low lands that go under water during rainy season. Jute is used for making cloth, shawl, ropes, carpet, bags and many other useful things. Jute sacks are very suitable for packing food grains. May 7, 2005. (photo)

UIG795044

Mars: craters and channels in Hephaestus Fossae - Mars: craters and channels in Hephaestus Fossae - Impact crateres and channel system in Hephaestus Fossae, a region on Mars located on the western flank of Elysium Mons. The large impact crater at the top of the picture is 20 km in diameter. The image covering an area of about 150 square km was obtained by the Mars Express probe on 28 December 2007. This image of Hephaestus Fossae was obtained by Esa's Mars Express orbiter on 28 December 2007. The region is dotted with craters and channel systems and lies at about 21* North and 126* East on the Red Planet. Named after the Greek god of fire, Hephaestus Fossae extends for more than 600 km on the western flank of Elysium Mons in the Utopia Planitia region. The surface is mostly smooth, and is covered by several small impact craters measuring 800 to 2800 m in diameter. Smaller craters are scattered across the entire region. A larger impact crater measuring 20 km in diameter is a prominent f

Mars: craters and channels in Hephaestus Fossae - Mars: craters and channels in Hephaestus Fossae - Impact crateres and channel system in Hephaestus Fossae, a region on Mars located on the western flank of Elysium Mons. The large impact crater at the top of the picture is 20 km in diameter. The image covering an area of about 150 square km was obtained by the Mars Express probe on 28 December 2007. This image of Hephaestus Fossae was obtained by Esa's Mars Express orbiter on 28 December 2007. The region is dotted with craters and channel systems and lies at about 21* North and 126* East on the Red Planet. Named after the Greek god of fire, Hephaestus Fossae extends for more than 600 km on the western flank of Elysium Mons in the Utopia Planitia region. The surface is mostly smooth, and is covered by several small impact craters measuring 800 to 2800 m in diameter. Smaller craters are scattered across the entire region. A larger impact crater measuring 20 km in diameter is a prominent f

PIX4616151

Mr Yorick and Maria ('A Sentimental Journey' by Laurence Sterne)

Mr Yorick and Maria ('A Sentimental Journey' by Laurence Sterne)

Stothard, Thomas (1755-1834) (after)

USB1159560

Barree spiral galaxy NGC 1097 in the Furnace - Barred spiral galaxy NGC 1097 in Fornax - Located at a distance of about 45 million years - light, NGC 1097 is the object of intense star formation and is an active core galaxy with a supermassive black hole in its heart. Image obtained by the Hubble Space Telescope (HST). The NASA/ESA Hubble Space Telescope provides us with a spectacular image of the bright star - forming ring that surrounds the heart of the barred spiral galaxy NGC 1097. In this image, the larger - scale structure of the galaxy is barely visible: its comparatively dim spiral arms, which surround its heart in a loose embrace, reach out beyond the edges of this frame. This face - on galaxy, lying 45 million light - years away from Earth in the southern constellation of Fornax (The Furnace), is particularly attractive for astronomers. NGC 1097 is a Seyfert galaxy. Lurking at the very centre of the galaxy, a supermassive black hole 100 million times the mass of our Sun is gr

Barree spiral galaxy NGC 1097 in the Furnace - Barred spiral galaxy NGC 1097 in Fornax - Located at a distance of about 45 million years - light, NGC 1097 is the object of intense star formation and is an active core galaxy with a supermassive black hole in its heart. Image obtained by the Hubble Space Telescope (HST). The NASA/ESA Hubble Space Telescope provides us with a spectacular image of the bright star - forming ring that surrounds the heart of the barred spiral galaxy NGC 1097. In this image, the larger - scale structure of the galaxy is barely visible: its comparatively dim spiral arms, which surround its heart in a loose embrace, reach out beyond the edges of this frame. This face - on galaxy, lying 45 million light - years away from Earth in the southern constellation of Fornax (The Furnace), is particularly attractive for astronomers. NGC 1097 is a Seyfert galaxy. Lurking at the very centre of the galaxy, a supermassive black hole 100 million times the mass of our Sun is gr

PIX4609655

Figure 3: Head-dress of white satin. One purple and two white feathers placed in the bandeau on the left side. The hair, light frizzed, thrown into easy curls, falling over the bandeau. Long ear-rings of pearls. One string of pearls and one chain of gold round the neck. The petticoat of white satin, embroidered in colours. A Circassian robe, of purple and orange-striped satin; the train cut in bias and rounded. The corset of white satin, with long sleeves of the same, tied round the wrist with two purple ribands. The short-sleeves of the robe, and the robe itself trimmed with fur... Figure 4: A Scotch bonnet of garnet-coloured satin, the ends trimmed with a gold fringe, and the bonnet with blue fox fur; a heron feather of gold on the left side. Chemise of clear-worked muslin, trimmed round the neck with a broad lace, and flounced with white fringe; long close sleeves, equally trimmed with lace, and tied with garnet-coloured riband; over them loose sleeves. The sash of a broad garnet-co

Figure 3: Head-dress of white satin. One purple and two white feathers placed in the bandeau on the left side. The hair, light frizzed, thrown into easy curls, falling over the bandeau. Long ear-rings of pearls. One string of pearls and one chain of gold round the neck. The petticoat of white satin, embroidered in colours. A Circassian robe, of purple and orange-striped satin; the train cut in bias and rounded. The corset of white satin, with long sleeves of the same, tied round the wrist with two purple ribands. The short-sleeves of the robe, and the robe itself trimmed with fur... Figure 4: A Scotch bonnet of garnet-coloured satin, the ends trimmed with a gold fringe, and the bonnet with blue fox fur; a heron feather of gold on the left side. Chemise of clear-worked muslin, trimmed round the neck with a broad lace, and flounced with white fringe; long close sleeves, equally trimmed with lace, and tied with garnet-coloured riband; over them loose sleeves. The sash of a broad garnet-co

BL3294757

Woman's Dressing Gown (Tea Gown) Liberty & Co., 1906 (silk, lace & net)

Woman's Dressing Gown (Tea Gown) Liberty & Co., 1906 (silk, lace & net)

English School, (20th century)

PHL2909232

1940s WW2 documentary 'The Big Red One'

1940s WW2 documentary 'The Big Red One'

BOF6285984

Apollo crowning a Poet and joining him with a Consort, witnessed by Hercules and by four other Females

Apollo crowning a Poet and joining him with a Consort, witnessed by Hercules and by four other Females

Tintoretto, Jacopo Robusti (1518-94)

USB1157020

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

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