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Images of 'Quite Red' found, 94

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Mary, Mary, Quite Contrary, How does Your Garden Grow? The Nursery, 1886 (stained glass)

Mary, Mary, Quite Contrary, How does Your Garden Grow? The Nursery, 1886 (stained glass)

Holmes Jewitt, Edward (1849-1929)

Alastair Carew-Cox

CCX3475493

Ambrose Dudley, Earl of Warwick, late 1590s (oil on panel)

Ambrose Dudley, Earl of Warwick, late 1590s (oil on panel)

English School, (16th century)

MOU5322329

Aquarius Constellation - Constellation of Aquarius - Field around the Aquarius constelllation. The Helix planetary nebula appears as a red dot towards the center of the image. Aquarius (The Water Carrier) is a large but relatively insconspicuous southern zodiacal constellation and has an area of about 980 square degrees, which makes it the 10th largest. Its origins as a constellation can be traced back to Babylonian times and has usually been delineated as a figure pouring water from a jar in the general direction of Capricornus and Piscis Austrinus, themselves quite watery constellations. The Sun is in this part of the sky in February and March, following the Ecliptic. The constellation embraces many objects of telescopic interest, including the Helix nebula and the Mira - like variable star R Aquarii. Also notable are the globular clusters M2 (NGC 7089) and the Saturn planetary nebula NGC 7009. Best seen in the early evening in August

Aquarius Constellation - Constellation of Aquarius - Field around the Aquarius constelllation. The Helix planetary nebula appears as a red dot towards the center of the image. Aquarius (The Water Carrier) is a large but relatively insconspicuous southern zodiacal constellation and has an area of about 980 square degrees, which makes it the 10th largest. Its origins as a constellation can be traced back to Babylonian times and has usually been delineated as a figure pouring water from a jar in the general direction of Capricornus and Piscis Austrinus, themselves quite watery constellations. The Sun is in this part of the sky in February and March, following the Ecliptic. The constellation embraces many objects of telescopic interest, including the Helix nebula and the Mira - like variable star R Aquarii. Also notable are the globular clusters M2 (NGC 7089) and the Saturn planetary nebula NGC 7009. Best seen in the early evening in August

PIX4594332

Our Cheeks Have Got Quite Rosy (colour litho)

Our Cheeks Have Got Quite Rosy (colour litho)

English School, (20th century)

LLM3094671

An Afternoon Dance on Board a Man-of-War (engraving)

An Afternoon Dance on Board a Man-of-War (engraving)

English School, (19th century)

LIP1061368

Why, my lady, you're quite a stranger (litho)

Why, my lady, you're quite a stranger (litho)

Armour, George Denholm (1864-1949)

IL3611082

Factory lamp, quite purified red-orange ceramic body

Factory lamp, quite purified red-orange ceramic body

MEV7080338

No Violencia Machista - No Violence Against Women (photo)

No Violencia Machista - No Violence Against Women (photo)

Ken Welsh

KW6373443

Open cluster NGC 4755 - Jewel Box - The Jewel Box cluster, NGC 4755 - NGC 4755 is located in the constellation of the Southern Cross at a distance of 7800 years - light from Earth. The bright orange star is Kappa Crucis, a supergiant red star. This famous group of young bright stars is an open cluster some 7800 light years from the Sun. It was named the Jewel Box from its description by Sir John Herschel as 'a casket of variously coloured precious stones', which refers to its appearance in the telescope. The bright orange star is kappa Crucis, and it contrasts strongly against its predominantly blue, hot companions. Kappa Cru is a very large, (hence very luminous) quite young star in its red supergiant stage, which paradoxically indicates that its life is drawing to a close. The cluster is looks like a star to the unaided eye and appears close to the eastern - most star of the Southern Cross, so is only visible from southern latitude

Open cluster NGC 4755 - Jewel Box - The Jewel Box cluster, NGC 4755 - NGC 4755 is located in the constellation of the Southern Cross at a distance of 7800 years - light from Earth. The bright orange star is Kappa Crucis, a supergiant red star. This famous group of young bright stars is an open cluster some 7800 light years from the Sun. It was named the Jewel Box from its description by Sir John Herschel as 'a casket of variously coloured precious stones', which refers to its appearance in the telescope. The bright orange star is kappa Crucis, and it contrasts strongly against its predominantly blue, hot companions. Kappa Cru is a very large, (hence very luminous) quite young star in its red supergiant stage, which paradoxically indicates that its life is drawing to a close. The cluster is looks like a star to the unaided eye and appears close to the eastern - most star of the Southern Cross, so is only visible from southern latitude

PIX4568295

And the eagle looked quite regal, illustration from 'Johnny Crow's Party', c.1930 (colour litho)

And the eagle looked quite regal, illustration from 'Johnny Crow's Party', c.1930 (colour litho)

Brooke, Leonard Leslie (1862-1940)

IL616645

Line of kids paddling in the sea (colour litho)

Line of kids paddling in the sea (colour litho)

English School, (20th century)

LLM8649518

Squat Lekythos (oil jug), 400-375 BC (red-figure terracotta)

Squat Lekythos (oil jug), 400-375 BC (red-figure terracotta)

Greek school, (4th century BC)

XCL5867626

Summer, Head of Woman, 1916 (red sandstone)

premium — Summer, Head of Woman, 1916 (red sandstone)

Summer, Head of Woman, 1916 (red sandstone)

Fergusson, John Duncan (1874-1961)

PRK6201219

Figures from Children’s Books: Little Red Riding Hood (colour litho)

Figures from Children’s Books: Little Red Riding Hood (colour litho)

Trier, Walter (1890-1951)

LLM8646598

Oslo 19580531: 40 days with the loose red lows RUSSE CELEBRATION: Broke ball at the University Square …, 1958 (photo)

Oslo 19580531: 40 days with the loose red lows RUSSE CELEBRATION: Broke ball at the University Square …, 1958 (photo)

Sverre A. Børretzen

NTB8734154

The Enchantress, 1912 (Watercolour)

The Enchantress, 1912 (Watercolour)

Browne, Gordon Frederick (1858-1932)

MAI7261491

Water Monitor Lizard on the Chobe River, Chobe National Park, Botswana (photo)

Water Monitor Lizard on the Chobe River, Chobe National Park, Botswana (photo)

Sergi Reboredo

SRB1202632

Muse (Musa), by Bramantino, 1499-1503, 15th-16th century (fresco)

Muse (Musa), by Bramantino, 1499-1503, 15th-16th century (fresco)

Bramantino, Bartolomeo Suardi (1450/55-c.1536)

Mauro Magliani & Barbara Piovan

MEP1267123

"Rose Window", from The Art work of Louis C. Tiffany, Garden City, New York : Doubleday, Page, & Company, 1914 (colour litho)

"Rose Window", from The Art work of Louis C. Tiffany, Garden City, New York : Doubleday, Page, & Company, 1914 (colour litho)

Tiffany, Louis Comfort (1848-1933)

SMT1217234

Turkey: A levha or panel honouring Imam 'Ali ibn Abi Talib I(r. 656-661 CE) and his celebrated bifurcated sword Dhu'l-fiqar (Zulfiqar), 'The Cleaver of Vertebrae'. Calligraphy attributed to Farid al-Din, early 19th century

Turkey: A levha or panel honouring Imam 'Ali ibn Abi Talib I(r. 656-661 CE) and his celebrated bifurcated sword Dhu'l-fiqar (Zulfiqar), 'The Cleaver of Vertebrae'. Calligraphy attributed to Farid al-Din, early 19th century

PFH1774311

Open Cluster of Pleiades - The Pleiades star cluster - The Pleiades cluster is a cluster of about 500 young stars nees 150 million years ago. Visible in the constellation Taurus, this cluster is 440 years from the Earth. The Pleiades are a reflection nebula associated with a cluster of young stars. The cluster itself is a group of many hundreds of stars about 400 light years from Earth in the northern constellation of Taurus.Seven of the brightest stars are quite easy to see with the unaided eye.The nebulosity seen here is light reflected from the particles in a cloud of cold gas and dust into which the cluster has drifted. It appears blue because these tiny interstellar particles scatter blue light more efficiently than the longer wavelengths of red light and it is streaky because of the distribution of dust particles in space

Open Cluster of Pleiades - The Pleiades star cluster - The Pleiades cluster is a cluster of about 500 young stars nees 150 million years ago. Visible in the constellation Taurus, this cluster is 440 years from the Earth. The Pleiades are a reflection nebula associated with a cluster of young stars. The cluster itself is a group of many hundreds of stars about 400 light years from Earth in the northern constellation of Taurus.Seven of the brightest stars are quite easy to see with the unaided eye.The nebulosity seen here is light reflected from the particles in a cloud of cold gas and dust into which the cluster has drifted. It appears blue because these tiny interstellar particles scatter blue light more efficiently than the longer wavelengths of red light and it is streaky because of the distribution of dust particles in space

PIX4568736

Aquarius Constellation - Constellation of Aquarius - Field around the Aquarius constelllation. The Helix planetary nebula appears as a red dot towards the center of the image. Aquarius (The Water Carrier) is a large but relatively insconspicuous southern zodiacal constellation and has an area of about 980 square degrees, which makes it the 10th largest. Its origins as a constellation can be traced back to Babylonian times and has usually been delineated as a figure pouring water from a jar in the general direction of Capricornus and Piscis Austrinus, themselves quite watery constellations. The Sun is in this part of the sky in February and March, following the Ecliptic. The constellation embraces many objects of telescopic interest, including the Helix nebula and the Mira - like variable star R Aquarii. Also notable are the globular clusters M2 (NGC 7089) and the Saturn planetary nebula NGC 7009. Best seen in the early evening in August

Aquarius Constellation - Constellation of Aquarius - Field around the Aquarius constelllation. The Helix planetary nebula appears as a red dot towards the center of the image. Aquarius (The Water Carrier) is a large but relatively insconspicuous southern zodiacal constellation and has an area of about 980 square degrees, which makes it the 10th largest. Its origins as a constellation can be traced back to Babylonian times and has usually been delineated as a figure pouring water from a jar in the general direction of Capricornus and Piscis Austrinus, themselves quite watery constellations. The Sun is in this part of the sky in February and March, following the Ecliptic. The constellation embraces many objects of telescopic interest, including the Helix nebula and the Mira - like variable star R Aquarii. Also notable are the globular clusters M2 (NGC 7089) and the Saturn planetary nebula NGC 7009. Best seen in the early evening in August

PIX4594337

Aquarius Constellation - Constellation of Aquarius - Field around the Aquarius constelllation. The Helix planetary nebula appears as a red dot towards the center of the image. Aquarius (The Water Carrier) is a large but relatively insconspicuous southern zodiacal constellation and has an area of about 980 square degrees, which makes it the 10th largest. Its origins as a constellation can be traced back to Babylonian times and has usually been delineated as a figure pouring water from a jar in the general direction of Capricornus and Piscis Austrinus, themselves quite watery constellations. The Sun is in this part of the sky in February and March, following the Ecliptic. The constellation embraces many objects of telescopic interest, including the Helix nebula and the Mira - like variable star R Aquarii. Also notable are the globular clusters M2 (NGC 7089) and the Saturn planetary nebula NGC 7009. Best seen in the early evening in August

Aquarius Constellation - Constellation of Aquarius - Field around the Aquarius constelllation. The Helix planetary nebula appears as a red dot towards the center of the image. Aquarius (The Water Carrier) is a large but relatively insconspicuous southern zodiacal constellation and has an area of about 980 square degrees, which makes it the 10th largest. Its origins as a constellation can be traced back to Babylonian times and has usually been delineated as a figure pouring water from a jar in the general direction of Capricornus and Piscis Austrinus, themselves quite watery constellations. The Sun is in this part of the sky in February and March, following the Ecliptic. The constellation embraces many objects of telescopic interest, including the Helix nebula and the Mira - like variable star R Aquarii. Also notable are the globular clusters M2 (NGC 7089) and the Saturn planetary nebula NGC 7009. Best seen in the early evening in August

PIX4594347

Nebula NGC 6334 in the Scorpion - The 'reddened' nebulosity of NGC 6334 - The nebula NGC 6334 is located about 5500 years - light from Earth. Image made with the 1.2m Telescope of Schmidt UK from Siding Spring. The star - forming nebula NGC 6334 shows no evidence of a blue component in their colour - indeed, the blue - light plate used in these 3 - colour pictures had no nebulous image at all - nor is there any obvious sign of the bright blue stars normally found in these objects. They are excellent examples of the phenomenon known as 'interstellar reddening', the selective removal of blue light by minute particles of dust in the line of sight. This accounts for both the ruddy hue and apparent absence of blue stars. The hot stars are present but only some of the red part of their light is seen so they are not conspicuous. This nebula is quite nearby (5500 light years) but located close to the Galactic plane and are buried in the dust of the Milky Way. Careful measurement of the colour

Nebula NGC 6334 in the Scorpion - The 'reddened' nebulosity of NGC 6334 - The nebula NGC 6334 is located about 5500 years - light from Earth. Image made with the 1.2m Telescope of Schmidt UK from Siding Spring. The star - forming nebula NGC 6334 shows no evidence of a blue component in their colour - indeed, the blue - light plate used in these 3 - colour pictures had no nebulous image at all - nor is there any obvious sign of the bright blue stars normally found in these objects. They are excellent examples of the phenomenon known as 'interstellar reddening', the selective removal of blue light by minute particles of dust in the line of sight. This accounts for both the ruddy hue and apparent absence of blue stars. The hot stars are present but only some of the red part of their light is seen so they are not conspicuous. This nebula is quite nearby (5500 light years) but located close to the Galactic plane and are buried in the dust of the Milky Way. Careful measurement of the colour

PIX4619360

Open Cluster of Pleiades - The Pleiades star cluster - The Pleiades cluster is a cluster of about 500 young stars nees 150 million years ago. Visible in the constellation Taurus, this cluster is 440 years from the Earth. The Pleiades are one of the finest and nearest examples of a reflection nebula associated with a cluster of young stars. The cluster itself is a group of many hundreds of stars about 400 light years from Earth in the northern constellation of Taurus and has been recognised since ancient times. Seven of the brightest stars are quite easy to see with the unaided eye and bear the names of the Seven Sisters, the daughters of Atlas. The nebulosity seen here is light reflected from the particles in a cloud of cold gas and dust into which the cluster has drifted. It appears blue because these tiny interstellar particles scatter blue light more efficiently than the longer wavelengths of red light and it is streaky because of the distribution of dust particles in space

Open Cluster of Pleiades - The Pleiades star cluster - The Pleiades cluster is a cluster of about 500 young stars nees 150 million years ago. Visible in the constellation Taurus, this cluster is 440 years from the Earth. The Pleiades are one of the finest and nearest examples of a reflection nebula associated with a cluster of young stars. The cluster itself is a group of many hundreds of stars about 400 light years from Earth in the northern constellation of Taurus and has been recognised since ancient times. Seven of the brightest stars are quite easy to see with the unaided eye and bear the names of the Seven Sisters, the daughters of Atlas. The nebulosity seen here is light reflected from the particles in a cloud of cold gas and dust into which the cluster has drifted. It appears blue because these tiny interstellar particles scatter blue light more efficiently than the longer wavelengths of red light and it is streaky because of the distribution of dust particles in space

PIX4568850

Aquarius Constellations, Capricorn, Austral Fish and Microscope - Constellations of Aquarius, Capricorn, Piscis Austrinus, Microscopium - Field around the Aquarius constellation. The Helix planetary nebula appears as a red dot towards the center of the image. Aquarius (The Water Carrier) is a large but relatively insconspicuous southern zodiacal constellation and has an area of about 980 square degrees, which makes it the 10th largest. Its origins as a constellation can be traced back to Babylonian times and has usually been delineated as a figure pouring water from a jar in the general direction of Capricornus and Piscis Austrinus, themselves quite watery constellations. The Sun is in this part of the sky in February and March, following the Ecliptic. The constellation embraces many objects of telescopic interest, including the Helix nebula and the Mira - like variable star R Aquarii. Also notable are the globular clusters M2 (NGC 7089) and the Saturn planetary nebula NGC 7009. Best s

Aquarius Constellations, Capricorn, Austral Fish and Microscope - Constellations of Aquarius, Capricorn, Piscis Austrinus, Microscopium - Field around the Aquarius constellation. The Helix planetary nebula appears as a red dot towards the center of the image. Aquarius (The Water Carrier) is a large but relatively insconspicuous southern zodiacal constellation and has an area of about 980 square degrees, which makes it the 10th largest. Its origins as a constellation can be traced back to Babylonian times and has usually been delineated as a figure pouring water from a jar in the general direction of Capricornus and Piscis Austrinus, themselves quite watery constellations. The Sun is in this part of the sky in February and March, following the Ecliptic. The constellation embraces many objects of telescopic interest, including the Helix nebula and the Mira - like variable star R Aquarii. Also notable are the globular clusters M2 (NGC 7089) and the Saturn planetary nebula NGC 7009. Best s

PIX4594319

Open Cluster of Pleiades - The Pleiades star cluster - The Pleiades cluster is a cluster of about 500 young stars nees 150 million years ago. Visible in the constellation Taurus, this cluster is 440 years from the Earth. The Pleiades are one of the finest and nearest examples of a reflection nebula associated with a cluster of young stars. The cluster itself is a group of many hundreds of stars about 400 light years from Earth in the northern constellation of Taurus and has been recognised since ancient times. Seven of the brightest stars are quite easy to see with the unaided eye and bear the names of the Seven Sisters, the daughters of Atlas. The nebulosity seen here is light reflected from the particles in a cloud of cold gas and dust into which the cluster has drifted. It appears blue because these tiny interstellar particles scatter blue light more efficiently than the longer wavelengths of red light and it is streaky because of the distribution of dust particles in space

Open Cluster of Pleiades - The Pleiades star cluster - The Pleiades cluster is a cluster of about 500 young stars nees 150 million years ago. Visible in the constellation Taurus, this cluster is 440 years from the Earth. The Pleiades are one of the finest and nearest examples of a reflection nebula associated with a cluster of young stars. The cluster itself is a group of many hundreds of stars about 400 light years from Earth in the northern constellation of Taurus and has been recognised since ancient times. Seven of the brightest stars are quite easy to see with the unaided eye and bear the names of the Seven Sisters, the daughters of Atlas. The nebulosity seen here is light reflected from the particles in a cloud of cold gas and dust into which the cluster has drifted. It appears blue because these tiny interstellar particles scatter blue light more efficiently than the longer wavelengths of red light and it is streaky because of the distribution of dust particles in space

PIX4568732

Open Cluster of Pleiades - The Pleiades star cluster - The Pleiades cluster is a cluster of about 500 young stars nees 150 million years ago. Visible in the constellation Taurus, this cluster is 440 years from the Earth. The Pleiades are one of the finest and nearest examples of a reflection nebula associated with a cluster of young stars. The cluster itself is a group of many hundreds of stars about 400 light years from Earth in the northern constellation of Taurus and has been recognised since ancient times. Seven of the brightest stars are quite easy to see with the unaided eye and bear the names of the Seven Sisters, the daughters of Atlas. The nebulosity seen here is light reflected from the particles in a cloud of cold gas and dust into which the cluster has drifted. It appears blue because these tiny interstellar particles scatter blue light more efficiently than the longer wavelengths of red light and it is streaky because of the distribution of dust particles in space

Open Cluster of Pleiades - The Pleiades star cluster - The Pleiades cluster is a cluster of about 500 young stars nees 150 million years ago. Visible in the constellation Taurus, this cluster is 440 years from the Earth. The Pleiades are one of the finest and nearest examples of a reflection nebula associated with a cluster of young stars. The cluster itself is a group of many hundreds of stars about 400 light years from Earth in the northern constellation of Taurus and has been recognised since ancient times. Seven of the brightest stars are quite easy to see with the unaided eye and bear the names of the Seven Sisters, the daughters of Atlas. The nebulosity seen here is light reflected from the particles in a cloud of cold gas and dust into which the cluster has drifted. It appears blue because these tiny interstellar particles scatter blue light more efficiently than the longer wavelengths of red light and it is streaky because of the distribution of dust particles in space

PIX4568852

Spiral galaxy M74 in Pisces - Spiral galaxy M74 in Pisces - Image of the spiral galaxy M74 (NGC 628). This galaxy is about 80,000 light years and is 30 million light years apart. Viewed face on, as it appeared about 30 million years ago, M74 is considered to be one of the most photogenic spiral galaxies in the sky. The galaxy is rich in young bright blue stars and glowing red regions of dust and molecular hydrogen where new stars are being created. M74, however, is quite camera shy - it has a low surface brightness that makes it challenging for both visual observers and astrophotographers to see it's entire form. The Chandra X - Ray observatory, discovered M74 to be the home of a super massive black hole, tucked away in one of it's outer arms. This black hole is one of the largest ever discovered and has the mass of over 10,000 suns

Spiral galaxy M74 in Pisces - Spiral galaxy M74 in Pisces - Image of the spiral galaxy M74 (NGC 628). This galaxy is about 80,000 light years and is 30 million light years apart. Viewed face on, as it appeared about 30 million years ago, M74 is considered to be one of the most photogenic spiral galaxies in the sky. The galaxy is rich in young bright blue stars and glowing red regions of dust and molecular hydrogen where new stars are being created. M74, however, is quite camera shy - it has a low surface brightness that makes it challenging for both visual observers and astrophotographers to see it's entire form. The Chandra X - Ray observatory, discovered M74 to be the home of a super massive black hole, tucked away in one of it's outer arms. This black hole is one of the largest ever discovered and has the mass of over 10,000 suns

Adam Block

PIX4609424

Nebulae NGC 3576 and 3603 in Carene. - Star formation regions NGC 3576 and 3603 in Carina - NGC 3576 (right) is located about 7000 years - light from Earth; NGC 3603 (left) is twice as far away. These two nebulae are located in the constellation Carene. These two star - formation regions appear side by side in the sky and seem to be linked as parts of an extensive nebula. However, the apparent intimacy is line - of - sight effect because these two objects are at quite different distances from the Sun. The curious looped nebula NGC 3576 is about 7000 light years from us while its neighbour NGC 3603 is more than twice as far away. That NGC 3603 is the more distant is confirmed by its colour, which is a ruddier red than the pinkish hue of NGC 3576. The change in colour is due to absorption of the blue - light component of the nebulosity by dust particles in the much longer line of sight

Nebulae NGC 3576 and 3603 in Carene. - Star formation regions NGC 3576 and 3603 in Carina - NGC 3576 (right) is located about 7000 years - light from Earth; NGC 3603 (left) is twice as far away. These two nebulae are located in the constellation Carene. These two star - formation regions appear side by side in the sky and seem to be linked as parts of an extensive nebula. However, the apparent intimacy is line - of - sight effect because these two objects are at quite different distances from the Sun. The curious looped nebula NGC 3576 is about 7000 light years from us while its neighbour NGC 3603 is more than twice as far away. That NGC 3603 is the more distant is confirmed by its colour, which is a ruddier red than the pinkish hue of NGC 3576. The change in colour is due to absorption of the blue - light component of the nebulosity by dust particles in the much longer line of sight

R. Gendler

PIX4619230

Open Cluster of Pleiades - The Pleiades star cluster - The Pleiades cluster is a cluster of about 500 young stars nees 150 million years ago. Visible in the constellation Taurus, this cluster is 440 years from the Earth. The Pleiades are one of the finest and nearest examples of a reflection nebula associated with a cluster of young stars. The cluster itself is a group of many hundreds of stars about 400 light years from Earth in the northern constellation of Taurus and has been recognised since ancient times. Seven of the brightest stars are quite easy to see with the unaided eye and bear the names of the Seven Sisters, the daughters of Atlas. The nebulosity seen here is light reflected from the particles in a cloud of cold gas and dust into which the cluster has drifted. It appears blue because these tiny interstellar particles scatter blue light more efficiently than the longer wavelengths of red light and it is streaky because of the distribution of dust particles in space

Open Cluster of Pleiades - The Pleiades star cluster - The Pleiades cluster is a cluster of about 500 young stars nees 150 million years ago. Visible in the constellation Taurus, this cluster is 440 years from the Earth. The Pleiades are one of the finest and nearest examples of a reflection nebula associated with a cluster of young stars. The cluster itself is a group of many hundreds of stars about 400 light years from Earth in the northern constellation of Taurus and has been recognised since ancient times. Seven of the brightest stars are quite easy to see with the unaided eye and bear the names of the Seven Sisters, the daughters of Atlas. The nebulosity seen here is light reflected from the particles in a cloud of cold gas and dust into which the cluster has drifted. It appears blue because these tiny interstellar particles scatter blue light more efficiently than the longer wavelengths of red light and it is streaky because of the distribution of dust particles in space

PIX4568741

Nebulae NGC 6334 and NGC 6357 in Scorpio - Nebulae NGC 6334 and NGC 6357 in Scorpius - These nebulae are located approximately 5500 years - light from Earth. Image made with the 1.2m Telescope of Schmidt UK from Siding Spring. The star - forming nebulae NGC 6334 and NGC 6357 show no evidence of a blue component in their colour - indeed, the blue - light plate used in these 3 - colour pictures had no nebulous image at all - nor is there any obvious sign of the bright blue stars normally found in these objects. They are excellent examples of the phenomenon known as 'interstellar reddening', the selective removal of blue light by minute particles of dust in the line of sight. This accounts for both the ruddy hue and apparent absence of blue stars. The hot stars are present but only some of the red part of their light is seen so they are not conspicuous. These nebulae are quite nearby (5500 light years) but located close to the Galactic plane and are buried in the dust of the Milky Way. Ca

Nebulae NGC 6334 and NGC 6357 in Scorpio - Nebulae NGC 6334 and NGC 6357 in Scorpius - These nebulae are located approximately 5500 years - light from Earth. Image made with the 1.2m Telescope of Schmidt UK from Siding Spring. The star - forming nebulae NGC 6334 and NGC 6357 show no evidence of a blue component in their colour - indeed, the blue - light plate used in these 3 - colour pictures had no nebulous image at all - nor is there any obvious sign of the bright blue stars normally found in these objects. They are excellent examples of the phenomenon known as 'interstellar reddening', the selective removal of blue light by minute particles of dust in the line of sight. This accounts for both the ruddy hue and apparent absence of blue stars. The hot stars are present but only some of the red part of their light is seen so they are not conspicuous. These nebulae are quite nearby (5500 light years) but located close to the Galactic plane and are buried in the dust of the Milky Way. Ca

PIX4619350

Nebula IC 4628 in Scorpio - Nebula IC 4628 in Scorpius - Nebula has a low light emission, IC 4628 (or Gum 56) is alongside the open cluster Collinder 316, which houses many young hot stars. Image obtained through 3 different filters that highlight oxygen (blue), hydrogen (green), and sulfur (red). This beautiful, arc - like rim of nebulosity is in the far southern sky, out of sight from most of the USA and Europe. It is quite faint and has often been overlooked because of it, even by southern observers. However, it is in a rich region in Scorpius. This richness is reflected in the number of names associated with the objects in the field illustrated here. There is a large scattered star cluster, Collinder 316 which extends over most of the picture. It encloses Trumpler 24, more or less the same cluster under another name, and all of this is part of the Sco OB1 association, a much larger gathering of very hot, intrinsically luminous stars in this part of the sky. The nebula itself is als

Nebula IC 4628 in Scorpio - Nebula IC 4628 in Scorpius - Nebula has a low light emission, IC 4628 (or Gum 56) is alongside the open cluster Collinder 316, which houses many young hot stars. Image obtained through 3 different filters that highlight oxygen (blue), hydrogen (green), and sulfur (red). This beautiful, arc - like rim of nebulosity is in the far southern sky, out of sight from most of the USA and Europe. It is quite faint and has often been overlooked because of it, even by southern observers. However, it is in a rich region in Scorpius. This richness is reflected in the number of names associated with the objects in the field illustrated here. There is a large scattered star cluster, Collinder 316 which extends over most of the picture. It encloses Trumpler 24, more or less the same cluster under another name, and all of this is part of the Sco OB1 association, a much larger gathering of very hot, intrinsically luminous stars in this part of the sky. The nebula itself is als

Tom Davis

PIX4622673

Nebulae NGC 3603 and NGC 3576 in Carene - NGC 3576 and 3603 in Carina - NGC 3576 (right) is located about 7000 years - light from Earth; NGC 3603 (left) is twice as far away. These two nebulae are located in the constellation Carene. Image obtained by Siding Spring's 3.9m telescope. These two star - formation regions appear side by side in the sky and seem to be linked as parts of an extensive nebula. However, the apparent intimacy is line - of - sight effect because these two objects are at quite different distances from the Sun. The curious looped nebula NGC 3576 is about 7000 light years from us while its neighbour NGC 3603 is more than twice as far away. That NGC 3603 is the more distant is confirmed by its colour, which is a ruddier red than the pinkish hue of NGC 3576. The change in colour is due to absorption of the blue - light component of the nebulosity by dust particles in the much longer line of sight. This effect is known as interstellar reddening, though it would be bette

Nebulae NGC 3603 and NGC 3576 in Carene - NGC 3576 and 3603 in Carina - NGC 3576 (right) is located about 7000 years - light from Earth; NGC 3603 (left) is twice as far away. These two nebulae are located in the constellation Carene. Image obtained by Siding Spring's 3.9m telescope. These two star - formation regions appear side by side in the sky and seem to be linked as parts of an extensive nebula. However, the apparent intimacy is line - of - sight effect because these two objects are at quite different distances from the Sun. The curious looped nebula NGC 3576 is about 7000 light years from us while its neighbour NGC 3603 is more than twice as far away. That NGC 3603 is the more distant is confirmed by its colour, which is a ruddier red than the pinkish hue of NGC 3576. The change in colour is due to absorption of the blue - light component of the nebulosity by dust particles in the much longer line of sight. This effect is known as interstellar reddening, though it would be bette

PIX4619197

Globular cluster NGC 3201 in Veles - Globular cluster NGC 3201 in Vela - This cluster of stars is located about 15,000 years ago - light from Earth

Globular cluster NGC 3201 in Veles - Globular cluster NGC 3201 in Vela - This cluster of stars is located about 15,000 years ago - light from Earth

PIX4564350

Star formation regions NGC 3576 and 3603 in Carina - NGC 3576 (right) is located about 7000 years - light from Earth; NGC 3603 (left) is twice as far away. These two nebulae are located in the constellation Carene. Image obtained by Siding Spring's 3.9m telescope. These two star - formation regions appear side by side in the sky and seem to be linked as parts of an extensive nebula. However, the apparent intimacy is line - of - sight effect because these two objects are at quite different distances from the Sun. The curious looped nebula NGC 3576 is about 7000 light years from us while its neighbour NGC 3603 is more than twice as far away. That NGC 3603 is the more distant is confirmed by its colour, which is a ruddier red than the pinkish hue of NGC 3576. The change in colour is due to absorption of the blue - light component of the nebulosity by dust particles in the much longer line of sight. This effect is known as interstellar reddening, though it would be better described as 'de

Star formation regions NGC 3576 and 3603 in Carina - NGC 3576 (right) is located about 7000 years - light from Earth; NGC 3603 (left) is twice as far away. These two nebulae are located in the constellation Carene. Image obtained by Siding Spring's 3.9m telescope. These two star - formation regions appear side by side in the sky and seem to be linked as parts of an extensive nebula. However, the apparent intimacy is line - of - sight effect because these two objects are at quite different distances from the Sun. The curious looped nebula NGC 3576 is about 7000 light years from us while its neighbour NGC 3603 is more than twice as far away. That NGC 3603 is the more distant is confirmed by its colour, which is a ruddier red than the pinkish hue of NGC 3576. The change in colour is due to absorption of the blue - light component of the nebulosity by dust particles in the much longer line of sight. This effect is known as interstellar reddening, though it would be better described as 'de

PIX4619187

Globular cluster NGC 3201 in Veles - Globular cluster NGC 3201 in Vela - This cluster of stars is located about 15,000 years ago - light from Earth

Globular cluster NGC 3201 in Veles - Globular cluster NGC 3201 in Vela - This cluster of stars is located about 15,000 years ago - light from Earth

PIX4564372

Nebula IC 2948 in Centaurus - Nebula IC 2948 and IC 2944 in Centaurus - Nebula IC 2948 is a vast nebula located about 6000 years from Earth in the southern constellation of Centaurus. It is associated with the cluster of stars IC 2944 near which Bok's blood cells are visible. A Bok's blood cell is a dark interstellar cloud of gases and dust that absorb light. If it condenses enough, it gives birth to new stars. Image obtained through 3 different filters that highlight oxygen (blue), hydrogen (green), and sulfur (red). Between the Southern Cross and the rich Carina region, on the southern border of Centaurus, is a large, almost featureless emission nebula, IC 2948, with a sprinkling of bright stars, Collinder 249. It is against this uniform, backdrop that we see a brighter region (IC 2944) which hosts small group of dark clouds of the kind known as 'Bok globules'. They are named for the Dutch - American astronomer who first drew attention to them as the possible sites of star formation.

Nebula IC 2948 in Centaurus - Nebula IC 2948 and IC 2944 in Centaurus - Nebula IC 2948 is a vast nebula located about 6000 years from Earth in the southern constellation of Centaurus. It is associated with the cluster of stars IC 2944 near which Bok's blood cells are visible. A Bok's blood cell is a dark interstellar cloud of gases and dust that absorb light. If it condenses enough, it gives birth to new stars. Image obtained through 3 different filters that highlight oxygen (blue), hydrogen (green), and sulfur (red). Between the Southern Cross and the rich Carina region, on the southern border of Centaurus, is a large, almost featureless emission nebula, IC 2948, with a sprinkling of bright stars, Collinder 249. It is against this uniform, backdrop that we see a brighter region (IC 2944) which hosts small group of dark clouds of the kind known as 'Bok globules'. They are named for the Dutch - American astronomer who first drew attention to them as the possible sites of star formation.

Tom Davis

PIX4622599

Planetary nebula NGC 2899 dans les Voiles - A distorted planetary nebula, NGC 2899 - This nebula is located about 3000 years from Earth. Image obtained by the 3.9m telescope of Siding Spring Planetary nebulae present a wide variety of forms on the sky, partly because of the random orientation of their parent stars but also because the nebulae themselves can have quite different intrinsic shapes. Theories about the shapes of planetaries range from the influence of binary companions to the central star to the distribution of material around the stars during its red giant phase, before the final outburst. Whatever the mechanism, most planetaries are symmetrical about one or more axes and only rarely do they appear curved like NGC 2899. A possible explanation is that the star from which the nebula was ejected had a large proper motion through space. The resulting nebula has the same velocity but vastly lower density than the star so is distorted by its encounter with the tenuous interstell

Planetary nebula NGC 2899 dans les Voiles - A distorted planetary nebula, NGC 2899 - This nebula is located about 3000 years from Earth. Image obtained by the 3.9m telescope of Siding Spring Planetary nebulae present a wide variety of forms on the sky, partly because of the random orientation of their parent stars but also because the nebulae themselves can have quite different intrinsic shapes. Theories about the shapes of planetaries range from the influence of binary companions to the central star to the distribution of material around the stars during its red giant phase, before the final outburst. Whatever the mechanism, most planetaries are symmetrical about one or more axes and only rarely do they appear curved like NGC 2899. A possible explanation is that the star from which the nebula was ejected had a large proper motion through space. The resulting nebula has the same velocity but vastly lower density than the star so is distorted by its encounter with the tenuous interstell

PIX4622995

Nebulae NGC 3603 and NGC 3576 in Carene - NGC 3576 and 3603 in Carina - NGC 3576 (right) is located about 7000 years - light from Earth; NGC 3603 (left) is twice as far away. These two nebulae are located in the constellation Carene. Image obtained by Siding Spring's 3.9m telescope. These two star - formation regions appear side by side in the sky and seem to be linked as parts of an extensive nebula. However, the apparent intimacy is line - of - sight effect because these two objects are at quite different distances from the Sun. The curious looped nebula NGC 3576 is about 7000 light years from us while its neighbour NGC 3603 is more than twice as far away. That NGC 3603 is the more distant is confirmed by its colour, which is a ruddier red than the pinkish hue of NGC 3576. The change in colour is due to absorption of the blue - light component of the nebulosity by dust particles in the much longer line of sight. This effect is known as interstellar reddening, though it would be bette

Nebulae NGC 3603 and NGC 3576 in Carene - NGC 3576 and 3603 in Carina - NGC 3576 (right) is located about 7000 years - light from Earth; NGC 3603 (left) is twice as far away. These two nebulae are located in the constellation Carene. Image obtained by Siding Spring's 3.9m telescope. These two star - formation regions appear side by side in the sky and seem to be linked as parts of an extensive nebula. However, the apparent intimacy is line - of - sight effect because these two objects are at quite different distances from the Sun. The curious looped nebula NGC 3576 is about 7000 light years from us while its neighbour NGC 3603 is more than twice as far away. That NGC 3603 is the more distant is confirmed by its colour, which is a ruddier red than the pinkish hue of NGC 3576. The change in colour is due to absorption of the blue - light component of the nebulosity by dust particles in the much longer line of sight. This effect is known as interstellar reddening, though it would be bette

PIX4619201

Spiral galaxy M74 in Pisces - Spiral galaxy M74 in Pisces - Image of the spiral galaxy M74 (NGC 628). This galaxy is about 80,000 light years and is 30 million light years apart. Viewed face on, as it appeared about 30 million years ago, M74 is considered to be one of the most photogenic spiral galaxies in the sky. The galaxy is rich in young bright blue stars and glowing red regions of dust and molecular hydrogen where new stars are being created. M74, however, is quite camera shy - it has a low surface brightness that makes it challenging for both visual observers and astrophotographers to see it's entire form. The Chandra X - Ray observatory, discovered M74 to be the home of a super massive black hole, tucked away in one of it's outer arms. This black hole is one of the largest ever discovered and has the mass of over 10,000 suns. Thirty six, fifteen minute photographs were combined to create this picture, with a total exposure time of almost nine hours. The images were taken with a

Spiral galaxy M74 in Pisces - Spiral galaxy M74 in Pisces - Image of the spiral galaxy M74 (NGC 628). This galaxy is about 80,000 light years and is 30 million light years apart. Viewed face on, as it appeared about 30 million years ago, M74 is considered to be one of the most photogenic spiral galaxies in the sky. The galaxy is rich in young bright blue stars and glowing red regions of dust and molecular hydrogen where new stars are being created. M74, however, is quite camera shy - it has a low surface brightness that makes it challenging for both visual observers and astrophotographers to see it's entire form. The Chandra X - Ray observatory, discovered M74 to be the home of a super massive black hole, tucked away in one of it's outer arms. This black hole is one of the largest ever discovered and has the mass of over 10,000 suns. Thirty six, fifteen minute photographs were combined to create this picture, with a total exposure time of almost nine hours. The images were taken with a

R. Jay GaBany

PIX4609403

The Large Magellanic Cloud - The Large Magellanic Cloud - The Great Magellan Cloud galaxy is located about 160,000 light years away from Earth in the southern constellation of Dorado. Visible with the naked eye in the southern hemishere it is one of the closest galaxies to us. It contains large star-forming zones such as the Tarantula Nebula (30 Sea bream, visible to the left), the most active star-forming regions of the local group. Image obtained by the 1.2m UK Schmidt telescope from Siding Spring, Australia. The Large Magellanic Cloud (LMC) is the nearest galaxy to the Milky Way but less than one tenth as massive; even so it contains the equivalent of over ten billion solar masses of material in the form of stars, gas and dust. The LMC is at a distance of 160,000 light years and is visible to the unaided eye from southern latitudes, rather like a detached piece of the Milky Way. The nearness of the LMC ensures that it is well resolved into stars in quite a modest telescope, and deep

The Large Magellanic Cloud - The Large Magellanic Cloud - The Great Magellan Cloud galaxy is located about 160,000 light years away from Earth in the southern constellation of Dorado. Visible with the naked eye in the southern hemishere it is one of the closest galaxies to us. It contains large star-forming zones such as the Tarantula Nebula (30 Sea bream, visible to the left), the most active star-forming regions of the local group. Image obtained by the 1.2m UK Schmidt telescope from Siding Spring, Australia. The Large Magellanic Cloud (LMC) is the nearest galaxy to the Milky Way but less than one tenth as massive; even so it contains the equivalent of over ten billion solar masses of material in the form of stars, gas and dust. The LMC is at a distance of 160,000 light years and is visible to the unaided eye from southern latitudes, rather like a detached piece of the Milky Way. The nearness of the LMC ensures that it is well resolved into stars in quite a modest telescope, and deep

PIX4613427

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

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

W. Promper

PIX4622580

Vietnam: The Opera House by night, Hanoi

Vietnam: The Opera House by night, Hanoi

David Henley

PFH4072407

Family of Khmer Leu Ethnic Group, Kateung village, Ratanakiri, Cambodia (photo)

Family of Khmer Leu Ethnic Group, Kateung village, Ratanakiri, Cambodia (photo)

Sergi Reboredo

SRB1202779

Tyndall Glacier, Chile - Tyndall Glacier, Chile - The Tyndall Glacier in Torres del Paine National Park in Chile, observed from the International Space Station in November 2007. Tyndall Glacier is located in the Torres del Paine National Park in Chile. This glacier, which has a total area of 331 square kilometers and a length of 32 kilometers (based on 1996 measurements), begins in the Patagonian Andes Mountains to the west and terminates in Lago Geikie. The digital astronaut photograph taken in november 2007 records visible light in red, green, and blue wavelengths (true color). The Tyndall Glacier terminus has retreated significantly during the past 17 years. Significant ice loss was also observed earlier this year at Grey Glacier, about 30 kilometers to the north - northeast, suggesting both glaciers are responding similarly to regional changes in temperature and precipitation. A medial moraine is visible in the center of the glacier, extending along its length (top image, center le

Tyndall Glacier, Chile - Tyndall Glacier, Chile - The Tyndall Glacier in Torres del Paine National Park in Chile, observed from the International Space Station in November 2007. Tyndall Glacier is located in the Torres del Paine National Park in Chile. This glacier, which has a total area of 331 square kilometers and a length of 32 kilometers (based on 1996 measurements), begins in the Patagonian Andes Mountains to the west and terminates in Lago Geikie. The digital astronaut photograph taken in november 2007 records visible light in red, green, and blue wavelengths (true color). The Tyndall Glacier terminus has retreated significantly during the past 17 years. Significant ice loss was also observed earlier this year at Grey Glacier, about 30 kilometers to the north - northeast, suggesting both glaciers are responding similarly to regional changes in temperature and precipitation. A medial moraine is visible in the center of the glacier, extending along its length (top image, center le

PIX4675989

Nebula Trifide (M20) in Sagittarius view in visible and infrared - This image composite compares the well - known visible - light picture of the glowing Trifid Nebula (left panel) with infrared views from Nasa's Spitzer Space Telescope (remaining three panels). The Trifid Nebula is a giant star - forming cloud of gas and dust located 5,400 light - years away in the constellation Sagittarius. The false - color Spitzer images reveal a different side of the Trifid Nebula. Where dark lanes of dust are visible trisecting the nebula in the visible - light picture, bright regions of star - forming activity are seen in the Spitzer pictures. All together, Spitzer uncovered 30 massive embryonic stars and 120 smaller newborn stars throughout the Trifid Nebula, in both its dark lanes and luminous clouds. These stars are visible in all the Spitzer images, mainly as yellow or red spots. Embryonic stars are developing stars about to burst into existence. Ten of the 30 massive embryos discovered by Sp

Nebula Trifide (M20) in Sagittarius view in visible and infrared - This image composite compares the well - known visible - light picture of the glowing Trifid Nebula (left panel) with infrared views from Nasa's Spitzer Space Telescope (remaining three panels). The Trifid Nebula is a giant star - forming cloud of gas and dust located 5,400 light - years away in the constellation Sagittarius. The false - color Spitzer images reveal a different side of the Trifid Nebula. Where dark lanes of dust are visible trisecting the nebula in the visible - light picture, bright regions of star - forming activity are seen in the Spitzer pictures. All together, Spitzer uncovered 30 massive embryonic stars and 120 smaller newborn stars throughout the Trifid Nebula, in both its dark lanes and luminous clouds. These stars are visible in all the Spitzer images, mainly as yellow or red spots. Embryonic stars are developing stars about to burst into existence. Ten of the 30 massive embryos discovered by Sp

PIX4619569

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

English Photographer, (19th century)

LMG3744835

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

English Photographer, (19th century)

LMG3744927

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

English Photographer, (19th century)

LMG3744951

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

English Photographer, (19th century)

LMG3744916

Frontispiece from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (pen & ink on paper)

Frontispiece from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (pen & ink on paper)

English School, (19th century)

LMG3744839

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

English Photographer, (19th century)

LMG3744840

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

English Photographer, (19th century)

LMG3744842

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

English Photographer, (19th century)

LMG3744844

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

English Photographer, (19th century)

LMG3744855

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

English Photographer, (19th century)

LMG3744862

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

English Photographer, (19th century)

LMG3744870

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

English Photographer, (19th century)

LMG3744882

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

English Photographer, (19th century)

LMG3744953

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

English Photographer, (19th century)

LMG3744973

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

English Photographer, (19th century)

LMG3744988

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

English Photographer, (19th century)

LMG3744865

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

English Photographer, (19th century)

LMG3744952

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

English Photographer, (19th century)

LMG3744955

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

English Photographer, (19th century)

LMG3744971

Binding of a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (leather)

Binding of a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (leather)

English School, (19th century)

LMG3744838

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

English Photographer, (19th century)

LMG3744849

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

English Photographer, (19th century)

LMG3744885

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

English Photographer, (19th century)

LMG3744920

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

English Photographer, (19th century)

LMG3744923

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

English Photographer, (19th century)

LMG3744961

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

English Photographer, (19th century)

LMG3744970

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

English Photographer, (19th century)

LMG3744843

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

English Photographer, (19th century)

LMG3744847

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

English Photographer, (19th century)

LMG3744877

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

English Photographer, (19th century)

LMG3744878

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

English Photographer, (19th century)

LMG3744895

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

English Photographer, (19th century)

LMG3744908

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

English Photographer, (19th century)

LMG3744921

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

English Photographer, (19th century)

LMG3744974

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

English Photographer, (19th century)

LMG3744954

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

English Photographer, (19th century)

LMG3744956

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

English Photographer, (19th century)

LMG3744981

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

English Photographer, (19th century)

LMG3744837

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

English Photographer, (19th century)

LMG3744841

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

English Photographer, (19th century)

LMG3744851

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

English Photographer, (19th century)

LMG3744872

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

English Photographer, (19th century)

LMG3744879

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

Page from a souvenir album of the Juvenile Fancy Dress Ball, Leeds, 12th January 1891 (b/w photo)

English Photographer, (19th century)

LMG3744880

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