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Woman with Chrysanthemums or, The Sphinx, c.1925 (oil on canvas)
Woman with Chrysanthemums or, The Sphinx, c.1925 (oil on canvas)

JLJ4611378: Woman with Chrysanthemums or, The Sphinx, c.1925 (oil on canvas), Dongen, Kees van (1877-1968) / Bridgeman Images

ID: JLJ4611378

Woman with Chrysanthemums or, The Sphinx, c.1925 (oil on canvas)

Dongen, Kees van (1877-1968)

Spiral galaxy of Sombrero M104 in the Virgin - The Sombrero galaxy (M104) in Virgo - The spiral galaxy M104 (NGC 4594, Sombrero galaxy) is located about 28 million years ago - light. Image obtained with the ANTU telescope of the VLT on January 30, 2000. The light from this remarkable spiral system is dominated by the billions of old, faint stars that form the vast 'bulge' around its tiny hidden nucleus. Most spirals, including the Milky Way, have clouds of old, faint stars around their nuclei, but in M104 the galaxy's light is dominated by them. This effect is enhanced because disk of the galaxy is seen nearly edge - on and dust in its outer parts is in silhouette as it crosses the picture. The galaxy is about 28 million light years distant. This image was obtained with FORS1 instrument on ANTU telescope at Paranal observatory on January 30 2000
Spiral galaxy of Sombrero M104 in the Virgin - The Sombrero galaxy (M104) in Virgo - The spiral galaxy M104 (NGC 4594, Sombrero galaxy) is located about 28 million years ago - light. Image obtained with the ANTU telescope of the VLT on January 30, 2000. The light from this remarkable spiral system is dominated by the billions of old, faint stars that form the vast 'bulge' around its tiny hidden nucleus. Most spirals, including the Milky Way, have clouds of old, faint stars around their nuclei, but in M104 the galaxy's light is dominated by them. This effect is enhanced because disk of the galaxy is seen nearly edge - on and dust in its outer parts is in silhouette as it crosses the picture. The galaxy is about 28 million light years distant. This image was obtained with FORS1 instrument on ANTU telescope at Paranal observatory on January 30 2000

PIX4611598: Spiral galaxy of Sombrero M104 in the Virgin - The Sombrero galaxy (M104) in Virgo - The spiral galaxy M104 (NGC 4594, Sombrero galaxy) is located about 28 million years ago - light. Image obtained with the ANTU telescope of the VLT on January 30, 2000. The light from this remarkable spiral system is dominated by the billions of old, faint stars that form the vast 'bulge' around its tiny hidden nucleus. Most spirals, including the Milky Way, have clouds of old, faint stars around their nuclei, but in M104 the galaxy's light is dominated by them. This effect is enhanced because disk of the galaxy is seen nearly edge - on and dust in its outer parts is in silhouette as it crosses the picture. The galaxy is about 28 million light years distant. This image was obtained with FORS1 instrument on ANTU telescope at Paranal observatory on January 30 2000 / Bridgeman Images

ID: PIX4611598

Spiral galaxy of Sombrero M104 in the Virgin - The Sombrero galaxy (M104) in Virgo - The spiral galaxy M104 (NGC 4594, Sombrero galaxy) is located about 28 million years ago - light. Image obtained with the ANTU telescope of the VLT on January 30, 2000. The light from this remarkable spiral system is dominated by the billions of old, faint stars that form the vast 'bulge' around its tiny hidden nucleus. Most spirals, including the Milky Way, have clouds of old, faint stars around their nuclei, but in M104 the galaxy's light is dominated by them. This effect is enhanced because disk of the galaxy is seen nearly edge - on and dust in its outer parts is in silhouette as it crosses the picture. The galaxy is about 28 million light years distant. This image was obtained with FORS1 instrument on ANTU telescope at Paranal observatory on January 30 2000

Fuller Building facade, 41East 57th Street in Manhattan, construction 1928-1929, architects Walker Morrisae & Gilette. New York, United States. Photography 10/04/03.
Fuller Building facade, 41East 57th Street in Manhattan, construction 1928-1929, architects Walker Morrisae & Gilette. New York, United States. Photography 10/04/03.

TEC4611483: Fuller Building facade, 41East 57th Street in Manhattan, construction 1928-1929, architects Walker Morrisae & Gilette. New York, United States. Photography 10/04/03. / Bridgeman Images

ID: TEC4611483

Fuller Building facade, 41East 57th Street in Manhattan, construction 1928-1929, architects Walker Morrisae & Gilette. New York, United States. Photography 10/04/03.

Tower LVMH 57th Street/Madison Avenue, construction 1999-2001, architect Christian de Protzamparc. New York, United States. Photography 15/10/03.
Tower LVMH 57th Street/Madison Avenue, construction 1999-2001, architect Christian de Protzamparc. New York, United States. Photography 15/10/03.

TEC4611553: Tower LVMH 57th Street/Madison Avenue, construction 1999-2001, architect Christian de Protzamparc. New York, United States. Photography 15/10/03., Portzamparc, de Christian (b.1944) / Bridgeman Images

ID: TEC4611553

Tower LVMH 57th Street/Madison Avenue, construction 1999-2001, architect Christian de Protzamparc. New York, United States. Photography 15/10/03.

Portzamparc, de Christian (b.1944)

Spiral galaxy of the Sombrero M104 infrared view - Sombrero galaxy seen in infrared - Infrared image of the spiral galaxy M104 (Sombrero galaxy), located about 28 million years ago - light, obtained with the Spitzer space telescope in 2004 and January 2005. Infrared radiation shows the dust of the disc visible throughout the circumference. A high emission also comes from the center of the galaxy where a supermassive black hole is thought to reside there. This spiral galaxy is located some 28 million light - years away. The infrared image obtained by Spitzer space telescope in 2004 and 2005 pierces through the obscuring dust, along with the bulge of stars. It shows that the disk is warped, which is often the result of a gravitational encounter with another galaxy; clumpy areas spotted in the far edges of the ring indicate young star - forming regions. Spitzer detected infrared emission not only from the ring, but from the center of the galaxy too, where there is a huge black hole, believed to be a billion times more massive than our Sun
Spiral galaxy of the Sombrero M104 infrared view - Sombrero galaxy seen in infrared - Infrared image of the spiral galaxy M104 (Sombrero galaxy), located about 28 million years ago - light, obtained with the Spitzer space telescope in 2004 and January 2005. Infrared radiation shows the dust of the disc visible throughout the circumference. A high emission also comes from the center of the galaxy where a supermassive black hole is thought to reside there. This spiral galaxy is located some 28 million light - years away. The infrared image obtained by Spitzer space telescope in 2004 and 2005 pierces through the obscuring dust, along with the bulge of stars. It shows that the disk is warped, which is often the result of a gravitational encounter with another galaxy; clumpy areas spotted in the far edges of the ring indicate young star - forming regions. Spitzer detected infrared emission not only from the ring, but from the center of the galaxy too, where there is a huge black hole, believed to be a billion times more massive than our Sun

PIX4611595: Spiral galaxy of the Sombrero M104 infrared view - Sombrero galaxy seen in infrared - Infrared image of the spiral galaxy M104 (Sombrero galaxy), located about 28 million years ago - light, obtained with the Spitzer space telescope in 2004 and January 2005. Infrared radiation shows the dust of the disc visible throughout the circumference. A high emission also comes from the center of the galaxy where a supermassive black hole is thought to reside there. This spiral galaxy is located some 28 million light - years away. The infrared image obtained by Spitzer space telescope in 2004 and 2005 pierces through the obscuring dust, along with the bulge of stars. It shows that the disk is warped, which is often the result of a gravitational encounter with another galaxy; clumpy areas spotted in the far edges of the ring indicate young star - forming regions. Spitzer detected infrared emission not only from the ring, but from the center of the galaxy too, where there is a huge black hole, believed to be a billion times more massive than our Sun / Bridgeman Images

ID: PIX4611595

Spiral galaxy of the Sombrero M104 infrared view - Sombrero galaxy seen in infrared - Infrared image of the spiral galaxy M104 (Sombrero galaxy), located about 28 million years ago - light, obtained with the Spitzer space telescope in 2004 and January 2005. Infrared radiation shows the dust of the disc visible throughout the circumference. A high emission also comes from the center of the galaxy where a supermassive black hole is thought to reside there. This spiral galaxy is located some 28 million light - years away. The infrared image obtained by Spitzer space telescope in 2004 and 2005 pierces through the obscuring dust, along with the bulge of stars. It shows that the disk is warped, which is often the result of a gravitational encounter with another galaxy; clumpy areas spotted in the far edges of the ring indicate young star - forming regions. Spitzer detected infrared emission not only from the ring, but from the center of the galaxy too, where there is a huge black hole, belie

Subdivision in Marcoussis (Essonne).
Subdivision in Marcoussis (Essonne).

LBY4610071: Subdivision in Marcoussis (Essonne). / Bridgeman Images

ID: LBY4610071

Subdivision in Marcoussis (Essonne).

Moses and the tables of the Law, detail of the hand of Moses showing the ten commandments, 1663 (oil on canvas)
Moses and the tables of the Law, detail of the hand of Moses showing the ten commandments, 1663 (oil on canvas)

JLJ4610003: Moses and the tables of the Law, detail of the hand of Moses showing the ten commandments, 1663 (oil on canvas), Champaigne, Philippe de (1602-74) / Bridgeman Images

ID: JLJ4610003

Moses and the tables of the Law, detail of the hand of Moses showing the ten commandments, 1663 (oil on canvas)

Champaigne, Philippe de (1602-74)

Subdivision in Nozay (Essonne).
Subdivision in Nozay (Essonne).

LBY4610084: Subdivision in Nozay (Essonne). / Bridgeman Images

ID: LBY4610084

Subdivision in Nozay (Essonne).

Barree spiral galaxy NGC 2442 in Flying Fish - NGC 2442, a barred spiral galaxy in Volans - NGC 2442 is a barree spiral galaxy located about 50 million years ago - light. Its asymmetrical shape suggests that a galaxy interacts with it. Image made with Siding Spring's 3.9m telescope. This unusual barred spiral galaxy is in the far southern constellation of Volans and was discovered by Sir John Herschel who described one of its spiral arms as hook - like. Although not seen here, (but evident on very deep images) NGC 2442 appears to have a less massive, distant companion that is also distorted, and it seems likely that the two have had a close encounter in the recent past. If there are no further meetings, the forces that hold NGC 2442 together will restore galaxy to a more symmetrical spiral form. However, much more likely is that the companion has been captured by the distorted spiral and will eventually be devoured by it, triggering a dramatic bout of star formation. NGC 2442 is about 50 million light years distant
Barree spiral galaxy NGC 2442 in Flying Fish - NGC 2442, a barred spiral galaxy in Volans - NGC 2442 is a barree spiral galaxy located about 50 million years ago - light. Its asymmetrical shape suggests that a galaxy interacts with it. Image made with Siding Spring's 3.9m telescope. This unusual barred spiral galaxy is in the far southern constellation of Volans and was discovered by Sir John Herschel who described one of its spiral arms as hook - like. Although not seen here, (but evident on very deep images) NGC 2442 appears to have a less massive, distant companion that is also distorted, and it seems likely that the two have had a close encounter in the recent past. If there are no further meetings, the forces that hold NGC 2442 together will restore galaxy to a more symmetrical spiral form. However, much more likely is that the companion has been captured by the distorted spiral and will eventually be devoured by it, triggering a dramatic bout of star formation. NGC 2442 is about 50 million light years distant

PIX4610090: Barree spiral galaxy NGC 2442 in Flying Fish - NGC 2442, a barred spiral galaxy in Volans - NGC 2442 is a barree spiral galaxy located about 50 million years ago - light. Its asymmetrical shape suggests that a galaxy interacts with it. Image made with Siding Spring's 3.9m telescope. This unusual barred spiral galaxy is in the far southern constellation of Volans and was discovered by Sir John Herschel who described one of its spiral arms as hook - like. Although not seen here, (but evident on very deep images) NGC 2442 appears to have a less massive, distant companion that is also distorted, and it seems likely that the two have had a close encounter in the recent past. If there are no further meetings, the forces that hold NGC 2442 together will restore galaxy to a more symmetrical spiral form. However, much more likely is that the companion has been captured by the distorted spiral and will eventually be devoured by it, triggering a dramatic bout of star formation. NGC 2442 is about 50 million light years distant / Bridgeman Images

ID: PIX4610090

Barree spiral galaxy NGC 2442 in Flying Fish - NGC 2442, a barred spiral galaxy in Volans - NGC 2442 is a barree spiral galaxy located about 50 million years ago - light. Its asymmetrical shape suggests that a galaxy interacts with it. Image made with Siding Spring's 3.9m telescope. This unusual barred spiral galaxy is in the far southern constellation of Volans and was discovered by Sir John Herschel who described one of its spiral arms as hook - like. Although not seen here, (but evident on very deep images) NGC 2442 appears to have a less massive, distant companion that is also distorted, and it seems likely that the two have had a close encounter in the recent past. If there are no further meetings, the forces that hold NGC 2442 together will restore galaxy to a more symmetrical spiral form. However, much more likely is that the companion has been captured by the distorted spiral and will eventually be devoured by it, triggering a dramatic bout of star formation. NGC 2442 is about

Bouquet of flowers. Anonymous painting, 18th century (oil on canvas)
Bouquet of flowers. Anonymous painting, 18th century (oil on canvas)

JLJ4610107: Bouquet of flowers. Anonymous painting, 18th century (oil on canvas), Unknown artist, (18th century) / Bridgeman Images

ID: JLJ4610107

Bouquet of flowers. Anonymous painting, 18th century (oil on canvas)

Unknown artist, (18th century)

Spiral galaxy NGC 2460 in Giraffe - NGC 2460 spiral galaxy in Camelopardalis - Spiral galaxy NGC 2460 in the constellation Giraffe. To its right is the galaxy IC 2209. NGC 2460 spiral galaxy in Camelopardalis; to its right, galaxy IC 2209
Spiral galaxy NGC 2460 in Giraffe - NGC 2460 spiral galaxy in Camelopardalis - Spiral galaxy NGC 2460 in the constellation Giraffe. To its right is the galaxy IC 2209. NGC 2460 spiral galaxy in Camelopardalis; to its right, galaxy IC 2209

PIX4610118: Spiral galaxy NGC 2460 in Giraffe - NGC 2460 spiral galaxy in Camelopardalis - Spiral galaxy NGC 2460 in the constellation Giraffe. To its right is the galaxy IC 2209. NGC 2460 spiral galaxy in Camelopardalis; to its right, galaxy IC 2209 / Bridgeman Images

ID: PIX4610118

Spiral galaxy NGC 2460 in Giraffe - NGC 2460 spiral galaxy in Camelopardalis - Spiral galaxy NGC 2460 in the constellation Giraffe. To its right is the galaxy IC 2209. NGC 2460 spiral galaxy in Camelopardalis; to its right, galaxy IC 2209

The toilet. A woman in a bathroom near her bathtub is about to take a bath, 19th century (litho)
The toilet. A woman in a bathroom near her bathtub is about to take a bath, 19th century (litho)

JLJ4610138: The toilet. A woman in a bathroom near her bathtub is about to take a bath, 19th century (litho), Unknown Artist, (19th century) / Bridgeman Images

ID: JLJ4610138

The toilet. A woman in a bathroom near her bathtub is about to take a bath, 19th century (litho)

Unknown Artist, (19th century)

French soldiers after victory (I Empire), 19th century (engraving)
French soldiers after victory (I Empire), 19th century (engraving)

JLJ4610241: French soldiers after victory (I Empire), 19th century (engraving), Paquier, A. (19th century) / Bridgeman Images

ID: JLJ4610241

French soldiers after victory (I Empire), 19th century (engraving)

Paquier, A. (19th century)

The elliptical galaxy NGC 4458 - The elliptical galaxy NGC 4458 - The galaxy NGC 4458 is 53 million years away - light from Earth, in the Virgin's cluster. Image obtained by the Hubble Space Telescope. The elliptical galaxy NGC 4458 lies at a distance of 53 million light - years from the Sun in the spring constellation Virgo. This image was made from data taken with Hubble space telescope
The elliptical galaxy NGC 4458 - The elliptical galaxy NGC 4458 - The galaxy NGC 4458 is 53 million years away - light from Earth, in the Virgin's cluster. Image obtained by the Hubble Space Telescope. The elliptical galaxy NGC 4458 lies at a distance of 53 million light - years from the Sun in the spring constellation Virgo. This image was made from data taken with Hubble space telescope

PIX4611377: The elliptical galaxy NGC 4458 - The elliptical galaxy NGC 4458 - The galaxy NGC 4458 is 53 million years away - light from Earth, in the Virgin's cluster. Image obtained by the Hubble Space Telescope. The elliptical galaxy NGC 4458 lies at a distance of 53 million light - years from the Sun in the spring constellation Virgo. This image was made from data taken with Hubble space telescope / Bridgeman Images

ID: PIX4611377

The elliptical galaxy NGC 4458 - The elliptical galaxy NGC 4458 - The galaxy NGC 4458 is 53 million years away - light from Earth, in the Virgin's cluster. Image obtained by the Hubble Space Telescope. The elliptical galaxy NGC 4458 lies at a distance of 53 million light - years from the Sun in the spring constellation Virgo. This image was made from data taken with Hubble space telescope

Elliptical Galaxy M49 - Elliptical galaxy M49 in Virgo - M49 (NGC 4472) is an E4 elliptical galaxy located in the Virgin's cluster. Elliptical galaxy M49 (NGC 4472) located in the Virgo cluster of galaxies
Elliptical Galaxy M49 - Elliptical galaxy M49 in Virgo - M49 (NGC 4472) is an E4 elliptical galaxy located in the Virgin's cluster. Elliptical galaxy M49 (NGC 4472) located in the Virgo cluster of galaxies

PIX4611387: Elliptical Galaxy M49 - Elliptical galaxy M49 in Virgo - M49 (NGC 4472) is an E4 elliptical galaxy located in the Virgin's cluster. Elliptical galaxy M49 (NGC 4472) located in the Virgo cluster of galaxies / Bridgeman Images

ID: PIX4611387

Elliptical Galaxy M49 - Elliptical galaxy M49 in Virgo - M49 (NGC 4472) is an E4 elliptical galaxy located in the Virgin's cluster. Elliptical galaxy M49 (NGC 4472) located in the Virgo cluster of galaxies

The Metropolitan Museum, 1000 Fifth Avenue New York (United States).
The Metropolitan Museum, 1000 Fifth Avenue New York (United States).

TEC4611419: The Metropolitan Museum, 1000 Fifth Avenue New York (United States). / Bridgeman Images

ID: TEC4611419

The Metropolitan Museum, 1000 Fifth Avenue New York (United States).

M87 elliptical galaxy in Virgo - M87 elliptical galaxy in Virgo - The M87 galaxy (NGC 4486) is located about 60 million years ago - light from Earth, in the heart of the Virgin's cluster. M87 is the brightest radio source in the constellation, it is also called Virgo A. Image made with Siding Spring's 3.9m telescope. Messier 87 (NGC 4486) is at the heart of the Virgo cluster and has a mass many times that of the Milky Way, itself no lightweight. Unlike our galaxy however, M87 is an elliptical galaxy. Though it appears more - or - less spherical on this photograph, a deep image shows it to be markedly elongated. Also unlike the Milky Way, M87 contains relatively little gas and dust. It is composed mainly of cool stars, which gives it a yellowish colour, in contrast to the blue of spiral galaxies. Despite the lack of star - forming materials, M87 is not a quiescent backwater. It is a powerful source of radio waves and the orbits of stars near its nucleus suggest they are held by a very massive, extremely compact core. Also, from the nucleus (but not seen here) extends a curious jet, all of which suggests that a massive black hole is hidden in the bright core of the galaxy
M87 elliptical galaxy in Virgo - M87 elliptical galaxy in Virgo - The M87 galaxy (NGC 4486) is located about 60 million years ago - light from Earth, in the heart of the Virgin's cluster. M87 is the brightest radio source in the constellation, it is also called Virgo A. Image made with Siding Spring's 3.9m telescope. Messier 87 (NGC 4486) is at the heart of the Virgo cluster and has a mass many times that of the Milky Way, itself no lightweight. Unlike our galaxy however, M87 is an elliptical galaxy. Though it appears more - or - less spherical on this photograph, a deep image shows it to be markedly elongated. Also unlike the Milky Way, M87 contains relatively little gas and dust. It is composed mainly of cool stars, which gives it a yellowish colour, in contrast to the blue of spiral galaxies. Despite the lack of star - forming materials, M87 is not a quiescent backwater. It is a powerful source of radio waves and the orbits of stars near its nucleus suggest they are held by a very massive, extremely compact core. Also, from the nucleus (but not seen here) extends a curious jet, all of which suggests that a massive black hole is hidden in the bright core of the galaxy

PIX4611429: M87 elliptical galaxy in Virgo - M87 elliptical galaxy in Virgo - The M87 galaxy (NGC 4486) is located about 60 million years ago - light from Earth, in the heart of the Virgin's cluster. M87 is the brightest radio source in the constellation, it is also called Virgo A. Image made with Siding Spring's 3.9m telescope. Messier 87 (NGC 4486) is at the heart of the Virgo cluster and has a mass many times that of the Milky Way, itself no lightweight. Unlike our galaxy however, M87 is an elliptical galaxy. Though it appears more - or - less spherical on this photograph, a deep image shows it to be markedly elongated. Also unlike the Milky Way, M87 contains relatively little gas and dust. It is composed mainly of cool stars, which gives it a yellowish colour, in contrast to the blue of spiral galaxies. Despite the lack of star - forming materials, M87 is not a quiescent backwater. It is a powerful source of radio waves and the orbits of stars near its nucleus suggest they are held by a very massive, extremely compact core. Also, from the nucleus (but not seen here) extends a curious jet, all of which suggests that a massive black hole is hidden in the bright core of the galaxy / Bridgeman Images

ID: PIX4611429

M87 elliptical galaxy in Virgo - M87 elliptical galaxy in Virgo - The M87 galaxy (NGC 4486) is located about 60 million years ago - light from Earth, in the heart of the Virgin's cluster. M87 is the brightest radio source in the constellation, it is also called Virgo A. Image made with Siding Spring's 3.9m telescope. Messier 87 (NGC 4486) is at the heart of the Virgo cluster and has a mass many times that of the Milky Way, itself no lightweight. Unlike our galaxy however, M87 is an elliptical galaxy. Though it appears more - or - less spherical on this photograph, a deep image shows it to be markedly elongated. Also unlike the Milky Way, M87 contains relatively little gas and dust. It is composed mainly of cool stars, which gives it a yellowish colour, in contrast to the blue of spiral galaxies. Despite the lack of star - forming materials, M87 is not a quiescent backwater. It is a powerful source of radio waves and the orbits of stars near its nucleus suggest they are held by a very m

Hudson Bar at the Hudson Hotel, 356 West 58th Street in Manhattan, architect Philippe Starck, New York (United States). Photography 10/04/03.
Hudson Bar at the Hudson Hotel, 356 West 58th Street in Manhattan, architect Philippe Starck, New York (United States). Photography 10/04/03.

TEC4611451: Hudson Bar at the Hudson Hotel, 356 West 58th Street in Manhattan, architect Philippe Starck, New York (United States). Photography 10/04/03., Starck, Philippe (b.1949) / Bridgeman Images

ID: TEC4611451

Hudson Bar at the Hudson Hotel, 356 West 58th Street in Manhattan, architect Philippe Starck, New York (United States). Photography 10/04/03.

Starck, Philippe (b.1949)

The Whitney Museum, 945 Madison Avenue at 75th Street in Manhattan, architect Marcel Breuer, 1966. New York, United States. Photography 10/04/03.
The Whitney Museum, 945 Madison Avenue at 75th Street in Manhattan, architect Marcel Breuer, 1966. New York, United States. Photography 10/04/03.

TEC4611509: The Whitney Museum, 945 Madison Avenue at 75th Street in Manhattan, architect Marcel Breuer, 1966. New York, United States. Photography 10/04/03., Breuer, Marcel (1902-81) / Bridgeman Images

ID: TEC4611509

The Whitney Museum, 945 Madison Avenue at 75th Street in Manhattan, architect Marcel Breuer, 1966. New York, United States. Photography 10/04/03.

Breuer, Marcel (1902-81)

Spiral galaxy NGC 4565 in Berenice's Hair - Spiral galaxy NGC 4565 in Coma Berenices - The galaxy NGC 4565 is located about 30 million years ago - light from Earth. It's a spiral galaxy seen by the slice. Image obtained with a 50 cm telescope, composite of several poses. Edge - on galaxy located at about 30 million light years away
Spiral galaxy NGC 4565 in Berenice's Hair - Spiral galaxy NGC 4565 in Coma Berenices - The galaxy NGC 4565 is located about 30 million years ago - light from Earth. It's a spiral galaxy seen by the slice. Image obtained with a 50 cm telescope, composite of several poses. Edge - on galaxy located at about 30 million light years away

PIX4611532: Spiral galaxy NGC 4565 in Berenice's Hair - Spiral galaxy NGC 4565 in Coma Berenices - The galaxy NGC 4565 is located about 30 million years ago - light from Earth. It's a spiral galaxy seen by the slice. Image obtained with a 50 cm telescope, composite of several poses. Edge - on galaxy located at about 30 million light years away / Bridgeman Images

ID: PIX4611532

Spiral galaxy NGC 4565 in Berenice's Hair - Spiral galaxy NGC 4565 in Coma Berenices - The galaxy NGC 4565 is located about 30 million years ago - light from Earth. It's a spiral galaxy seen by the slice. Image obtained with a 50 cm telescope, composite of several poses. Edge - on galaxy located at about 30 million light years away

Spiral galaxy NGC 4565 in Berenice's Hair - Spiral galaxy NGC 4565 in Coma Berenices - The galaxy NGC 4565 is located about 30 million years ago - light from Earth. It's a spiral galaxy seen by the slice. Edge - on galaxy located at about 30 million light years away
Spiral galaxy NGC 4565 in Berenice's Hair - Spiral galaxy NGC 4565 in Coma Berenices - The galaxy NGC 4565 is located about 30 million years ago - light from Earth. It's a spiral galaxy seen by the slice. Edge - on galaxy located at about 30 million light years away

PIX4611545: Spiral galaxy NGC 4565 in Berenice's Hair - Spiral galaxy NGC 4565 in Coma Berenices - The galaxy NGC 4565 is located about 30 million years ago - light from Earth. It's a spiral galaxy seen by the slice. Edge - on galaxy located at about 30 million light years away / Bridgeman Images

ID: PIX4611545

Spiral galaxy NGC 4565 in Berenice's Hair - Spiral galaxy NGC 4565 in Coma Berenices - The galaxy NGC 4565 is located about 30 million years ago - light from Earth. It's a spiral galaxy seen by the slice. Edge - on galaxy located at about 30 million light years away

Saint Roch The saint carries the bubon of plague on his leg. Painting by Tanzio da Varallo (Antonio d'Enrico) (1580 ~ 1635) Pinacoteca de Varallo
Saint Roch The saint carries the bubon of plague on his leg. Painting by Tanzio da Varallo (Antonio d'Enrico) (1580 ~ 1635) Pinacoteca de Varallo

LRI4611610: Saint Roch The saint carries the bubon of plague on his leg. Painting by Tanzio da Varallo (Antonio d'Enrico) (1580 ~ 1635) Pinacoteca de Varallo, Varallo, Tanzio da (c.1575/80-c.1633) / Bridgeman Images

ID: LRI4611610

Saint Roch The saint carries the bubon of plague on his leg. Painting by Tanzio da Varallo (Antonio d'Enrico) (1580 ~ 1635) Pinacoteca de Varallo

Varallo, Tanzio da (c.1575/80-c.1633)

The Adoration of the Shepherds Detail representing the angels, 1635 (painting)
The Adoration of the Shepherds Detail representing the angels, 1635 (painting)

JLJ4611635: The Adoration of the Shepherds Detail representing the angels, 1635 (painting), La Hyre, Laurent de (1606-56) / Bridgeman Images

ID: JLJ4611635

The Adoration of the Shepherds Detail representing the angels, 1635 (painting)

La Hyre, Laurent de (1606-56)

Spiral galaxy of Sombrero M104 in the Virgin - The Sombrero galaxy (M104) in Virgo - Image of the spiral galaxy M104 or NGC 4594 (Sombrero galaxy), located between 28 and 40 million years - light. Image obtained with a telescope 61 cm in diameter, 3h40 laying. The Sombrero, named after the broad - brimmed Mexican hat it superficially resembles, is probably the most famous galaxy in the sky. The spiral galaxy is between 28 to 40 million light years distant. Image taken with a 24 - inch telescope, total exposure time: 3 hours 40 minutes
Spiral galaxy of Sombrero M104 in the Virgin - The Sombrero galaxy (M104) in Virgo - Image of the spiral galaxy M104 or NGC 4594 (Sombrero galaxy), located between 28 and 40 million years - light. Image obtained with a telescope 61 cm in diameter, 3h40 laying. The Sombrero, named after the broad - brimmed Mexican hat it superficially resembles, is probably the most famous galaxy in the sky. The spiral galaxy is between 28 to 40 million light years distant. Image taken with a 24 - inch telescope, total exposure time: 3 hours 40 minutes

PIX4611656: Spiral galaxy of Sombrero M104 in the Virgin - The Sombrero galaxy (M104) in Virgo - Image of the spiral galaxy M104 or NGC 4594 (Sombrero galaxy), located between 28 and 40 million years - light. Image obtained with a telescope 61 cm in diameter, 3h40 laying. The Sombrero, named after the broad - brimmed Mexican hat it superficially resembles, is probably the most famous galaxy in the sky. The spiral galaxy is between 28 to 40 million light years distant. Image taken with a 24 - inch telescope, total exposure time: 3 hours 40 minutes / Bridgeman Images

ID: PIX4611656

Spiral galaxy of Sombrero M104 in the Virgin - The Sombrero galaxy (M104) in Virgo - Image of the spiral galaxy M104 or NGC 4594 (Sombrero galaxy), located between 28 and 40 million years - light. Image obtained with a telescope 61 cm in diameter, 3h40 laying. The Sombrero, named after the broad - brimmed Mexican hat it superficially resembles, is probably the most famous galaxy in the sky. The spiral galaxy is between 28 to 40 million light years distant. Image taken with a 24 - inch telescope, total exposure time: 3 hours 40 minutes

Times Square in New York (United States).
Times Square in New York (United States).

TEC4611672: Times Square in New York (United States). / Bridgeman Images

ID: TEC4611672

Times Square in New York (United States).

Egyptian antiquite: statuette representing the Divine Adorator Karomama. Gold bronze sculpture. 850 BC (gold, bronze)
Egyptian antiquite: statuette representing the Divine Adorator Karomama. Gold bronze sculpture. 850 BC (gold, bronze)

JLJ4611826: Egyptian antiquite: statuette representing the Divine Adorator Karomama. Gold bronze sculpture. 850 BC (gold, bronze), Egyptian School / Bridgeman Images

ID: JLJ4611826

Egyptian antiquite: statuette representing the Divine Adorator Karomama. Gold bronze sculpture. 850 BC (gold, bronze)

Egyptian School

Mongolian rider chasing a horse. Detail. Silk (oil on canvas)
Mongolian rider chasing a horse. Detail. Silk (oil on canvas)

JLJ4611862: Mongolian rider chasing a horse. Detail. Silk (oil on canvas), Chao Meng-Fu or, Zhao Mengfu (1254-1322) / Bridgeman Images

ID: JLJ4611862

Mongolian rider chasing a horse. Detail. Silk (oil on canvas)

Chao Meng-Fu or, Zhao Mengfu (1254-1322)

Mongolian rider chasing a horse. Detail. Silk (oil on canvas)
Mongolian rider chasing a horse. Detail. Silk (oil on canvas)

JLJ4611871: Mongolian rider chasing a horse. Detail. Silk (oil on canvas), Chao Meng-Fu or, Zhao Mengfu (1254-1322) / Bridgeman Images

ID: JLJ4611871

Mongolian rider chasing a horse. Detail. Silk (oil on canvas)

Chao Meng-Fu or, Zhao Mengfu (1254-1322)

Spiral Galaxy NGC 4725 in Berenice's Hair - Spiral galaxy NGC 4725 in Coma Berenice
Spiral Galaxy NGC 4725 in Berenice's Hair - Spiral galaxy NGC 4725 in Coma Berenice

PIX4611872: Spiral Galaxy NGC 4725 in Berenice's Hair - Spiral galaxy NGC 4725 in Coma Berenice / Bridgeman Images

ID: PIX4611872

Spiral Galaxy NGC 4725 in Berenice's Hair - Spiral galaxy NGC 4725 in Coma Berenice

Oriental art: woulette tau (end of the shepherd's stick) with ivory animal head. Detail, 15th century (ivory)
Oriental art: woulette tau (end of the shepherd's stick) with ivory animal head. Detail, 15th century (ivory)

JLJ4611916: Oriental art: woulette tau (end of the shepherd's stick) with ivory animal head. Detail, 15th century (ivory), Unknown Artist, (15th century) / Bridgeman Images

ID: JLJ4611916

Oriental art: woulette tau (end of the shepherd's stick) with ivory animal head. Detail, 15th century (ivory)

Unknown Artist, (15th century)

Spiral galaxy NGC 2841 in the Great Bear - Spiral galaxy NGC 2841 in Ursa Major - NGC 2841 is a spiral galaxy located 46 million years ago - light. The spiral galaxy NGC 2841 lies 46 million light - years away in the constellation of Ursa Major (The Great Bear)
Spiral galaxy NGC 2841 in the Great Bear - Spiral galaxy NGC 2841 in Ursa Major - NGC 2841 is a spiral galaxy located 46 million years ago - light. The spiral galaxy NGC 2841 lies 46 million light - years away in the constellation of Ursa Major (The Great Bear)

PIX4610193: Spiral galaxy NGC 2841 in the Great Bear - Spiral galaxy NGC 2841 in Ursa Major - NGC 2841 is a spiral galaxy located 46 million years ago - light. The spiral galaxy NGC 2841 lies 46 million light - years away in the constellation of Ursa Major (The Great Bear) / Bridgeman Images

ID: PIX4610193

Spiral galaxy NGC 2841 in the Great Bear - Spiral galaxy NGC 2841 in Ursa Major - NGC 2841 is a spiral galaxy located 46 million years ago - light. The spiral galaxy NGC 2841 lies 46 million light - years away in the constellation of Ursa Major (The Great Bear)

Railway right-of-way at Ivry sur Seine (Val de Marne).
Railway right-of-way at Ivry sur Seine (Val de Marne).

MDA4610200: Railway right-of-way at Ivry sur Seine (Val de Marne). / Bridgeman Images

ID: MDA4610200

Railway right-of-way at Ivry sur Seine (Val de Marne).

The French soldier (Grenadier I empire wesse), 19th century (engraving)
The French soldier (Grenadier I empire wesse), 19th century (engraving)

JLJ4610231: The French soldier (Grenadier I empire wesse), 19th century (engraving), Charlet, Nicolas Toussaint (1792-1845) / Bridgeman Images

ID: JLJ4610231

The French soldier (Grenadier I empire wesse), 19th century (engraving)

Charlet, Nicolas Toussaint (1792-1845)

Spiral Galaxy NGC 3079 in the Great Bear - Spiral galaxy NGC 3079 - NGC 3079 is a spiral galaxy distant about 50 million years - light from Earth. His disc measures about 70,000 years - light. This false-colored image obtained by the Hubble Space Telescope in 1998 shows that a huge gas bubble escapes from the galaxy. This bubble rises more than 3500 years ago - light above the disk of the galaxy. It is a wind from hot stars and blends with very hot gas from supernovae explosions that would cause this bubble. The picture shows the bubble in the center of the NGC 3079 galaxy's disk. The structure is more than 3,000 light - years wide and rises 3,500 light - years above the galaxy's disk. Astronomers suspect that the bubble is being blown by “” winds”” (high - speed streams of particles) released during a burst of star formation. Eventually, this gas will rain down upon the galaxy's disk where it may collide with gas clouds, compress them, and form a new generation of stars. The two white dots just above the bubble are probably stars in the galaxy. According to theoretical models, the bubble formed when ongoing winds from hot stars mixed with small bubbles of very hot gas from supernova explosions. NGC 3079 is 50 million light - years from Earth in the constellation Ursa Major. The colors in this image accentuate important details in the bubble. Glowing gas is red and starlight is blue/green. Hubble's Wide Field and Planetary Camera 2 snapped this picture in 1998
Spiral Galaxy NGC 3079 in the Great Bear - Spiral galaxy NGC 3079 - NGC 3079 is a spiral galaxy distant about 50 million years - light from Earth. His disc measures about 70,000 years - light. This false-colored image obtained by the Hubble Space Telescope in 1998 shows that a huge gas bubble escapes from the galaxy. This bubble rises more than 3500 years ago - light above the disk of the galaxy. It is a wind from hot stars and blends with very hot gas from supernovae explosions that would cause this bubble. The picture shows the bubble in the center of the NGC 3079 galaxy's disk. The structure is more than 3,000 light - years wide and rises 3,500 light - years above the galaxy's disk. Astronomers suspect that the bubble is being blown by “” winds”” (high - speed streams of particles) released during a burst of star formation. Eventually, this gas will rain down upon the galaxy's disk where it may collide with gas clouds, compress them, and form a new generation of stars. The two white dots just above the bubble are probably stars in the galaxy. According to theoretical models, the bubble formed when ongoing winds from hot stars mixed with small bubbles of very hot gas from supernova explosions. NGC 3079 is 50 million light - years from Earth in the constellation Ursa Major. The colors in this image accentuate important details in the bubble. Glowing gas is red and starlight is blue/green. Hubble's Wide Field and Planetary Camera 2 snapped this picture in 1998

PIX4610471: Spiral Galaxy NGC 3079 in the Great Bear - Spiral galaxy NGC 3079 - NGC 3079 is a spiral galaxy distant about 50 million years - light from Earth. His disc measures about 70,000 years - light. This false-colored image obtained by the Hubble Space Telescope in 1998 shows that a huge gas bubble escapes from the galaxy. This bubble rises more than 3500 years ago - light above the disk of the galaxy. It is a wind from hot stars and blends with very hot gas from supernovae explosions that would cause this bubble. The picture shows the bubble in the center of the NGC 3079 galaxy's disk. The structure is more than 3,000 light - years wide and rises 3,500 light - years above the galaxy's disk. Astronomers suspect that the bubble is being blown by “” winds”” (high - speed streams of particles) released during a burst of star formation. Eventually, this gas will rain down upon the galaxy's disk where it may collide with gas clouds, compress them, and form a new generation of stars. The two white dots just above the bubble are probably stars in the galaxy. According to theoretical models, the bubble formed when ongoing winds from hot stars mixed with small bubbles of very hot gas from supernova explosions. NGC 3079 is 50 million light - years from Earth in the constellation Ursa Major. The colors in this image accentuate important details in the bubble. Glowing gas is red and starlight is blue/green. Hubble's Wide Field and Planetary Camera 2 snapped this picture in 1998 / Bridgeman Images

ID: PIX4610471

Spiral Galaxy NGC 3079 in the Great Bear - Spiral galaxy NGC 3079 - NGC 3079 is a spiral galaxy distant about 50 million years - light from Earth. His disc measures about 70,000 years - light. This false-colored image obtained by the Hubble Space Telescope in 1998 shows that a huge gas bubble escapes from the galaxy. This bubble rises more than 3500 years ago - light above the disk of the galaxy. It is a wind from hot stars and blends with very hot gas from supernovae explosions that would cause this bubble. The picture shows the bubble in the center of the NGC 3079 galaxy's disk. The structure is more than 3,000 light - years wide and rises 3,500 light - years above the galaxy's disk. Astronomers suspect that the bubble is being blown by “” winds”” (high - speed streams of particles) released during a burst of star formation. Eventually, this gas will rain down upon the galaxy's disk where it may collide with gas clouds, compress them, and form a new generation of stars. The two white

Codex Atlanticus, sheet 964 recto, 1478-1518 (pen & ink)
Codex Atlanticus, sheet 964 recto, 1478-1518 (pen & ink)

MEV5047120: Codex Atlanticus, sheet 964 recto, 1478-1518 (pen & ink), Vinci, Leonardo da (1452-1519) / Bridgeman Images

ID: MEV5047120

Codex Atlanticus, sheet 964 recto, 1478-1518 (pen & ink)

Vinci, Leonardo da (1452-1519)

Codex Atlanticus, sheet 968 verso, 1478-1518 (pen & ink)
Codex Atlanticus, sheet 968 verso, 1478-1518 (pen & ink)

MEV5047129: Codex Atlanticus, sheet 968 verso, 1478-1518 (pen & ink), Vinci, Leonardo da (1452-1519) / Bridgeman Images

ID: MEV5047129

Codex Atlanticus, sheet 968 verso, 1478-1518 (pen & ink)

Vinci, Leonardo da (1452-1519)


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