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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

Dissection of the human diaphragm, chest cavity, and details of the pharynx and larynx. Copperplate engraving by Robert Benard after an illustration by Albrecht von Haller from Denis Diderot's Encyclopedia, Pellet, Geneva, 1779.
Dissection of the human diaphragm, chest cavity, and details of the pharynx and larynx. Copperplate engraving by Robert Benard after an illustration by Albrecht von Haller from Denis Diderot's Encyclopedia, Pellet, Geneva, 1779.

FLO4611580: Dissection of the human diaphragm, chest cavity, and details of the pharynx and larynx. Copperplate engraving by Robert Benard after an illustration by Albrecht von Haller from Denis Diderot's Encyclopedia, Pellet, Geneva, 1779. / Bridgeman Images

ID: FLO4611580

Dissection of the human diaphragm, chest cavity, and details of the pharynx and larynx. Copperplate engraving by Robert Benard after an illustration by Albrecht von Haller from Denis Diderot's Encyclopedia, Pellet, Geneva, 1779.

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

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

Trunk of the hepatic portal vein. Copperplate engraving by Robert Benard from Denis Diderot's Encyclopedia, Pellet, Geneva, 1779.
Trunk of the hepatic portal vein. Copperplate engraving by Robert Benard from Denis Diderot's Encyclopedia, Pellet, Geneva, 1779.

FLO4611607: Trunk of the hepatic portal vein. Copperplate engraving by Robert Benard from Denis Diderot's Encyclopedia, Pellet, Geneva, 1779. / Bridgeman Images

ID: FLO4611607

Trunk of the hepatic portal vein. Copperplate engraving by Robert Benard from Denis Diderot's Encyclopedia, Pellet, Geneva, 1779.

Arteries in the face. Copperplate engraving by Robert Benard after an illustration by Albrecht von Haller from Denis Diderot's Encyclopedia, Pellet, Geneva, 1779.
Arteries in the face. Copperplate engraving by Robert Benard after an illustration by Albrecht von Haller from Denis Diderot's Encyclopedia, Pellet, Geneva, 1779.

FLO4611624: Arteries in the face. Copperplate engraving by Robert Benard after an illustration by Albrecht von Haller from Denis Diderot's Encyclopedia, Pellet, Geneva, 1779. / Bridgeman Images

ID: FLO4611624

Arteries in the face. Copperplate engraving by Robert Benard after an illustration by Albrecht von Haller from Denis Diderot's Encyclopedia, Pellet, Geneva, 1779.

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

Second position of the disarm in tierce, disarm on the carte or seconde thrust, and second position of the disarm on the carte. Copperplate engraving by Robert Benard from the Fencing fencing section of Denis Diderot's Encyclopedia, Pellet, Geneva, 1779.
Second position of the disarm in tierce, disarm on the carte or seconde thrust, and second position of the disarm on the carte. Copperplate engraving by Robert Benard from the Fencing fencing section of Denis Diderot's Encyclopedia, Pellet, Geneva, 1779.

FLO4611696: Second position of the disarm in tierce, disarm on the carte or seconde thrust, and second position of the disarm on the carte. Copperplate engraving by Robert Benard from the Fencing fencing section of Denis Diderot's Encyclopedia, Pellet, Geneva, 1779. / Bridgeman Images

ID: FLO4611696

Second position of the disarm in tierce, disarm on the carte or seconde thrust, and second position of the disarm on the carte. Copperplate engraving by Robert Benard from the Fencing fencing section of Denis Diderot's Encyclopedia, Pellet, Geneva, 1779.

Galaxy NGC 4631 in Hunting Dogs - Spiral galaxy NGC 4631 in Canes Venatici - Spiral galaxy seen by the slice located at a distance of 30 million years - light. His small companion, the elliptical galaxy NGC 4627, is visible just above it. This huge edge - on galaxy has a small companion, an elliptical galaxy, NGC 4627, which seems to interact strongly with it
Galaxy NGC 4631 in Hunting Dogs - Spiral galaxy NGC 4631 in Canes Venatici - Spiral galaxy seen by the slice located at a distance of 30 million years - light. His small companion, the elliptical galaxy NGC 4627, is visible just above it. This huge edge - on galaxy has a small companion, an elliptical galaxy, NGC 4627, which seems to interact strongly with it

PIX4611703: Galaxy NGC 4631 in Hunting Dogs - Spiral galaxy NGC 4631 in Canes Venatici - Spiral galaxy seen by the slice located at a distance of 30 million years - light. His small companion, the elliptical galaxy NGC 4627, is visible just above it. This huge edge - on galaxy has a small companion, an elliptical galaxy, NGC 4627, which seems to interact strongly with it / Bridgeman Images

ID: PIX4611703

Galaxy NGC 4631 in Hunting Dogs - Spiral galaxy NGC 4631 in Canes Venatici - Spiral galaxy seen by the slice located at a distance of 30 million years - light. His small companion, the elliptical galaxy NGC 4627, is visible just above it. This huge edge - on galaxy has a small companion, an elliptical galaxy, NGC 4627, which seems to interact strongly with it

Fencers in outside guard/thrust positions, tierce and carte positions, tierce and second positions. Copperplate engraving by Robert Benard from the Fencing fencing section of Denis Diderot's Encyclopedia, Pellet, Geneva, 1779.
Fencers in outside guard/thrust positions, tierce and carte positions, tierce and second positions. Copperplate engraving by Robert Benard from the Fencing fencing section of Denis Diderot's Encyclopedia, Pellet, Geneva, 1779.

FLO4611726: Fencers in outside guard/thrust positions, tierce and carte positions, tierce and second positions. Copperplate engraving by Robert Benard from the Fencing fencing section of Denis Diderot's Encyclopedia, Pellet, Geneva, 1779. / Bridgeman Images

ID: FLO4611726

Fencers in outside guard/thrust positions, tierce and carte positions, tierce and second positions. Copperplate engraving by Robert Benard from the Fencing fencing section of Denis Diderot's Encyclopedia, Pellet, Geneva, 1779.

Second, third, fourth and fifth positions of the salute, and inside parade. Copperplate engraving by Robert Benard from the Fencing fencing section of Denis Diderot's Encyclopedia, Pellet, Geneva, 1779.
Second, third, fourth and fifth positions of the salute, and inside parade. Copperplate engraving by Robert Benard from the Fencing fencing section of Denis Diderot's Encyclopedia, Pellet, Geneva, 1779.

FLO4611738: Second, third, fourth and fifth positions of the salute, and inside parade. Copperplate engraving by Robert Benard from the Fencing fencing section of Denis Diderot's Encyclopedia, Pellet, Geneva, 1779. / Bridgeman Images

ID: FLO4611738

Second, third, fourth and fifth positions of the salute, and inside parade. Copperplate engraving by Robert Benard from the Fencing fencing section of Denis Diderot's Encyclopedia, Pellet, Geneva, 1779.

Galaxies NGC 4631 and NGC 4656 - 57 in Hunting Dogs - Galaxies NGC 4631 and NGC 4656 - 57 - The spiral galaxy NGC 4631 (upper right) is a galaxy seen by the slice that is located at a distance of 30 million years - light. His small companion, the elliptical galaxy NGC 4627, is visible just above it. Below the irregular galaxies NGC 4656 and NGC 4657. Galaxies NGC 4631 (top right) and NGC 4656 (bottom left) are two unusual galaxies in Canes Venatici. A small companion galaxy, NGC 4627, can be seen next to NGC 4631. The galaxies, which are located about 30 million lights years away, get their unusual shapes from gravitational interactions with each other. NGC 6431 and NGC 4627 are also listed in ARP's Atlas of Peculiar Galaxies as Arp 281
Galaxies NGC 4631 and NGC 4656 - 57 in Hunting Dogs - Galaxies NGC 4631 and NGC 4656 - 57 - The spiral galaxy NGC 4631 (upper right) is a galaxy seen by the slice that is located at a distance of 30 million years - light. His small companion, the elliptical galaxy NGC 4627, is visible just above it. Below the irregular galaxies NGC 4656 and NGC 4657. Galaxies NGC 4631 (top right) and NGC 4656 (bottom left) are two unusual galaxies in Canes Venatici. A small companion galaxy, NGC 4627, can be seen next to NGC 4631. The galaxies, which are located about 30 million lights years away, get their unusual shapes from gravitational interactions with each other. NGC 6431 and NGC 4627 are also listed in ARP's Atlas of Peculiar Galaxies as Arp 281

PIX4611740: Galaxies NGC 4631 and NGC 4656 - 57 in Hunting Dogs - Galaxies NGC 4631 and NGC 4656 - 57 - The spiral galaxy NGC 4631 (upper right) is a galaxy seen by the slice that is located at a distance of 30 million years - light. His small companion, the elliptical galaxy NGC 4627, is visible just above it. Below the irregular galaxies NGC 4656 and NGC 4657. Galaxies NGC 4631 (top right) and NGC 4656 (bottom left) are two unusual galaxies in Canes Venatici. A small companion galaxy, NGC 4627, can be seen next to NGC 4631. The galaxies, which are located about 30 million lights years away, get their unusual shapes from gravitational interactions with each other. NGC 6431 and NGC 4627 are also listed in ARP's Atlas of Peculiar Galaxies as Arp 281 / Bridgeman Images

ID: PIX4611740

Galaxies NGC 4631 and NGC 4656 - 57 in Hunting Dogs - Galaxies NGC 4631 and NGC 4656 - 57 - The spiral galaxy NGC 4631 (upper right) is a galaxy seen by the slice that is located at a distance of 30 million years - light. His small companion, the elliptical galaxy NGC 4627, is visible just above it. Below the irregular galaxies NGC 4656 and NGC 4657. Galaxies NGC 4631 (top right) and NGC 4656 (bottom left) are two unusual galaxies in Canes Venatici. A small companion galaxy, NGC 4627, can be seen next to NGC 4631. The galaxies, which are located about 30 million lights years away, get their unusual shapes from gravitational interactions with each other. NGC 6431 and NGC 4627 are also listed in ARP's Atlas of Peculiar Galaxies as Arp 281

Galaxies NGC 4631 and NGC 4656 - 57 in Hunting Dogs - Galaxies NGC 4631 and NGC 4656 - 57 - The spiral galaxy NGC 4631 (upper right) is a galaxy seen by the slice that is located at a distance of 30 million years - light. His small companion, the elliptical galaxy NGC 4627, is visible just above it. Below the irregular galaxies NGC 4656 and NGC 4657. Galaxies NGC 4631 (top right) and NGC 4656 (bottom left) are two unusual galaxies in Canes Venatici. A small companion galaxy, NGC 4627, can be seen next to NGC 4631. The galaxies, which are located about 30 million lights years away, get their unusual shapes from gravitational interactions with each other. NGC 6431 and NGC 4627 are also listed in ARP's Atlas of Peculiar Galaxies as Arp 281
Galaxies NGC 4631 and NGC 4656 - 57 in Hunting Dogs - Galaxies NGC 4631 and NGC 4656 - 57 - The spiral galaxy NGC 4631 (upper right) is a galaxy seen by the slice that is located at a distance of 30 million years - light. His small companion, the elliptical galaxy NGC 4627, is visible just above it. Below the irregular galaxies NGC 4656 and NGC 4657. Galaxies NGC 4631 (top right) and NGC 4656 (bottom left) are two unusual galaxies in Canes Venatici. A small companion galaxy, NGC 4627, can be seen next to NGC 4631. The galaxies, which are located about 30 million lights years away, get their unusual shapes from gravitational interactions with each other. NGC 6431 and NGC 4627 are also listed in ARP's Atlas of Peculiar Galaxies as Arp 281

PIX4611764: Galaxies NGC 4631 and NGC 4656 - 57 in Hunting Dogs - Galaxies NGC 4631 and NGC 4656 - 57 - The spiral galaxy NGC 4631 (upper right) is a galaxy seen by the slice that is located at a distance of 30 million years - light. His small companion, the elliptical galaxy NGC 4627, is visible just above it. Below the irregular galaxies NGC 4656 and NGC 4657. Galaxies NGC 4631 (top right) and NGC 4656 (bottom left) are two unusual galaxies in Canes Venatici. A small companion galaxy, NGC 4627, can be seen next to NGC 4631. The galaxies, which are located about 30 million lights years away, get their unusual shapes from gravitational interactions with each other. NGC 6431 and NGC 4627 are also listed in ARP's Atlas of Peculiar Galaxies as Arp 281 / Bridgeman Images

ID: PIX4611764

Galaxies NGC 4631 and NGC 4656 - 57 in Hunting Dogs - Galaxies NGC 4631 and NGC 4656 - 57 - The spiral galaxy NGC 4631 (upper right) is a galaxy seen by the slice that is located at a distance of 30 million years - light. His small companion, the elliptical galaxy NGC 4627, is visible just above it. Below the irregular galaxies NGC 4656 and NGC 4657. Galaxies NGC 4631 (top right) and NGC 4656 (bottom left) are two unusual galaxies in Canes Venatici. A small companion galaxy, NGC 4627, can be seen next to NGC 4631. The galaxies, which are located about 30 million lights years away, get their unusual shapes from gravitational interactions with each other. NGC 6431 and NGC 4627 are also listed in ARP's Atlas of Peculiar Galaxies as Arp 281

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

Rectum with seistule, syringotome (syringe) for incising the anal fistula, several bandages - Plate from “” L'Encyclopedie”” by Denis Diderot (1713-1784) and Jean Le Rond D'Alembert (1717-1783), 1779 - Rectum with sistule 1, syringotome scalpel 2, solar bandage 3, eye bandages 4,5, face mask 6, upperlip bandage 7, head divider 8, hernia bandages 9,10 and T bandages 11-14. Copperplate engraving by Robert Benard from Denis Diderot's Encyclopedia, Pellet, Geneva, 1779.
Rectum with seistule, syringotome (syringe) for incising the anal fistula, several bandages - Plate from “” L'Encyclopedie”” by Denis Diderot (1713-1784) and Jean Le Rond D'Alembert (1717-1783), 1779 - Rectum with sistule 1, syringotome scalpel 2, solar bandage 3, eye bandages 4,5, face mask 6, upperlip bandage 7, head divider 8, hernia bandages 9,10 and T bandages 11-14. Copperplate engraving by Robert Benard from Denis Diderot's Encyclopedia, Pellet, Geneva, 1779.

FLO4611875: Rectum with seistule, syringotome (syringe) for incising the anal fistula, several bandages - Plate from “” L'Encyclopedie”” by Denis Diderot (1713-1784) and Jean Le Rond D'Alembert (1717-1783), 1779 - Rectum with sistule 1, syringotome scalpel 2, solar bandage 3, eye bandages 4,5, face mask 6, upperlip bandage 7, head divider 8, hernia bandages 9,10 and T bandages 11-14. Copperplate engraving by Robert Benard from Denis Diderot's Encyclopedia, Pellet, Geneva, 1779. / Bridgeman Images

ID: FLO4611875

Rectum with seistule, syringotome (syringe) for incising the anal fistula, several bandages - Plate from “” L'Encyclopedie”” by Denis Diderot (1713-1784) and Jean Le Rond D'Alembert (1717-1783), 1779 - Rectum with sistule 1, syringotome scalpel 2, solar bandage 3, eye bandages 4,5, face mask 6, upperlip bandage 7, head divider 8, hernia bandages 9,10 and T bandages 11-14. Copperplate engraving by Robert Benard from Denis Diderot's Encyclopedia, Pellet, Geneva, 1779.

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

PIX4611880: Spiral Galaxy NGC 4725 in Berenice's Hair - Spiral galaxy NGC 4725 in Coma Berenice / Bridgeman Images

ID: PIX4611880

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

Trocade a tracheotomy, brush for the stomach, tumour in the chest after Lorenz Heister, scar after the elimination of the tumour, and ancient harmful and painful method of tracheotomy - Plate drawn from “” The Encyclopedie”” by Denis Diderot (1713-1784) and Jean Le Rond D'Alembert (1717-1783), 1779 - chotomy trocar 1, stomach brush 2, breast tumor after Lorenz Heister 3, scar after tumor removal 4, large breast tumor 5 and old mastectomy method more painful and harmful than useful 6. Copperplate engraving by Robert Benard from Denis Diderot's Encyclopedia, Pellet, Geneva, 1779.
Trocade a tracheotomy, brush for the stomach, tumour in the chest after Lorenz Heister, scar after the elimination of the tumour, and ancient harmful and painful method of tracheotomy - Plate drawn from “” The Encyclopedie”” by Denis Diderot (1713-1784) and Jean Le Rond D'Alembert (1717-1783), 1779 - chotomy trocar 1, stomach brush 2, breast tumor after Lorenz Heister 3, scar after tumor removal 4, large breast tumor 5 and old mastectomy method more painful and harmful than useful 6. Copperplate engraving by Robert Benard from Denis Diderot's Encyclopedia, Pellet, Geneva, 1779.

FLO4611930: Trocade a tracheotomy, brush for the stomach, tumour in the chest after Lorenz Heister, scar after the elimination of the tumour, and ancient harmful and painful method of tracheotomy - Plate drawn from “” The Encyclopedie”” by Denis Diderot (1713-1784) and Jean Le Rond D'Alembert (1717-1783), 1779 - chotomy trocar 1, stomach brush 2, breast tumor after Lorenz Heister 3, scar after tumor removal 4, large breast tumor 5 and old mastectomy method more painful and harmful than useful 6. Copperplate engraving by Robert Benard from Denis Diderot's Encyclopedia, Pellet, Geneva, 1779. / Bridgeman Images

ID: FLO4611930

Trocade a tracheotomy, brush for the stomach, tumour in the chest after Lorenz Heister, scar after the elimination of the tumour, and ancient harmful and painful method of tracheotomy - Plate drawn from “” The Encyclopedie”” by Denis Diderot (1713-1784) and Jean Le Rond D'Alembert (1717-1783), 1779 - chotomy trocar 1, stomach brush 2, breast tumor after Lorenz Heister 3, scar after tumor removal 4, large breast tumor 5 and old mastectomy method more painful and harmful than useful 6. Copperplate engraving by Robert Benard from Denis Diderot's Encyclopedia, Pellet, Geneva, 1779.

Spiral Galaxy M94 in Hunting Dogs - Spiral galaxy M94 in Canes Venatici - The spiral galaxy M94 (NGC 4736) is located about 15 million years ago - light from Earth. The M94 spiral galaxy was classified as Sab because of the extreme luminosite of its central region. This galaxy has several ring zones of star formation, one of which is very active. Image obtained with a 50 cm telescope, composite of several poses. M94 is a spiral galaxy located 15 million light - year away. Several active regions of star formation have been identified there
Spiral Galaxy M94 in Hunting Dogs - Spiral galaxy M94 in Canes Venatici - The spiral galaxy M94 (NGC 4736) is located about 15 million years ago - light from Earth. The M94 spiral galaxy was classified as Sab because of the extreme luminosite of its central region. This galaxy has several ring zones of star formation, one of which is very active. Image obtained with a 50 cm telescope, composite of several poses. M94 is a spiral galaxy located 15 million light - year away. Several active regions of star formation have been identified there

PIX4611934: Spiral Galaxy M94 in Hunting Dogs - Spiral galaxy M94 in Canes Venatici - The spiral galaxy M94 (NGC 4736) is located about 15 million years ago - light from Earth. The M94 spiral galaxy was classified as Sab because of the extreme luminosite of its central region. This galaxy has several ring zones of star formation, one of which is very active. Image obtained with a 50 cm telescope, composite of several poses. M94 is a spiral galaxy located 15 million light - year away. Several active regions of star formation have been identified there / Bridgeman Images

ID: PIX4611934

Spiral Galaxy M94 in Hunting Dogs - Spiral galaxy M94 in Canes Venatici - The spiral galaxy M94 (NGC 4736) is located about 15 million years ago - light from Earth. The M94 spiral galaxy was classified as Sab because of the extreme luminosite of its central region. This galaxy has several ring zones of star formation, one of which is very active. Image obtained with a 50 cm telescope, composite of several poses. M94 is a spiral galaxy located 15 million light - year away. Several active regions of star formation have been identified there

Dodo of the Scotch House, Veere, 1561, and dodo from the Florence Codex, circa 1703. Heliotype by Van Leer from Dr. Anthonie Cornelis Oudemans' Dodo Studies, Amsterdam, Johannes Muller, 1917.
Dodo of the Scotch House, Veere, 1561, and dodo from the Florence Codex, circa 1703. Heliotype by Van Leer from Dr. Anthonie Cornelis Oudemans' Dodo Studies, Amsterdam, Johannes Muller, 1917.

FLO4611958: Dodo of the Scotch House, Veere, 1561, and dodo from the Florence Codex, circa 1703. Heliotype by Van Leer from Dr. Anthonie Cornelis Oudemans' Dodo Studies, Amsterdam, Johannes Muller, 1917. / Bridgeman Images

ID: FLO4611958

Dodo of the Scotch House, Veere, 1561, and dodo from the Florence Codex, circa 1703. Heliotype by Van Leer from Dr. Anthonie Cornelis Oudemans' Dodo Studies, Amsterdam, Johannes Muller, 1917.

17th century copies of the white dodo by Salomon Savery, male: Gerrit van Goedesberg, 1662 (13), Joost Hartgers, 1650 (14), Abraham and Jan de Wees, 1651 (15) and Gijsbert Sijbes, 1651 (16). Heliotype by Van Leer from Dr. Anthonie Cornelis Oudemans' Dodo Studies, Amsterdam, Johannes Muller, 1917.
17th century copies of the white dodo by Salomon Savery, male: Gerrit van Goedesberg, 1662 (13), Joost Hartgers, 1650 (14), Abraham and Jan de Wees, 1651 (15) and Gijsbert Sijbes, 1651 (16). Heliotype by Van Leer from Dr. Anthonie Cornelis Oudemans' Dodo Studies, Amsterdam, Johannes Muller, 1917.

FLO4611990: 17th century copies of the white dodo by Salomon Savery, male: Gerrit van Goedesberg, 1662 (13), Joost Hartgers, 1650 (14), Abraham and Jan de Wees, 1651 (15) and Gijsbert Sijbes, 1651 (16). Heliotype by Van Leer from Dr. Anthonie Cornelis Oudemans' Dodo Studies, Amsterdam, Johannes Muller, 1917. / Bridgeman Images

ID: FLO4611990

17th century copies of the white dodo by Salomon Savery, male: Gerrit van Goedesberg, 1662 (13), Joost Hartgers, 1650 (14), Abraham and Jan de Wees, 1651 (15) and Gijsbert Sijbes, 1651 (16). Heliotype by Van Leer from Dr. Anthonie Cornelis Oudemans' Dodo Studies, Amsterdam, Johannes Muller, 1917.

Elliptical galaxy NGC 4881 and distant galaxies - Elliptical galaxy NGC 4881 and distant galaxies - The elliptical galaxy NGC 4881 (upper left) is about 300 million years away - light from Earth. NGC 4881 is located in the Coma galaxy cluster that contains at least 1,000 galaxies and is five times farther from us than the Virgin's cluster. Almost all the objects visible in this photo are located far behind the Coma cluster, except for the spiral galaxy to the right of Ngc 4881. Image obtained by the Hubble Space Telescope in 1994. This photo mosaic, which shows a field of distant galaxies, is a computer enhanced reproduction of a picture taken 4 March 1994 with the repaired Hubble Space Telescope. The brightest object in this picture is NGC 4881. It is a 13th - magnitude elliptical galaxy in the outskirts of the Coma Cluster, a great cluster of galaxies more than 5 times farther away than the Virgo Cluster. Except for a 16th - magnitude Coma spiral at the right and a few foreground stars of the Milky Way, almost everything else in this field lies far beyond the Coma Cluster. There is a fascinating assortment of background galaxies, including an apparent galaxian merger in progress
Elliptical galaxy NGC 4881 and distant galaxies - Elliptical galaxy NGC 4881 and distant galaxies - The elliptical galaxy NGC 4881 (upper left) is about 300 million years away - light from Earth. NGC 4881 is located in the Coma galaxy cluster that contains at least 1,000 galaxies and is five times farther from us than the Virgin's cluster. Almost all the objects visible in this photo are located far behind the Coma cluster, except for the spiral galaxy to the right of Ngc 4881. Image obtained by the Hubble Space Telescope in 1994. This photo mosaic, which shows a field of distant galaxies, is a computer enhanced reproduction of a picture taken 4 March 1994 with the repaired Hubble Space Telescope. The brightest object in this picture is NGC 4881. It is a 13th - magnitude elliptical galaxy in the outskirts of the Coma Cluster, a great cluster of galaxies more than 5 times farther away than the Virgo Cluster. Except for a 16th - magnitude Coma spiral at the right and a few foreground stars of the Milky Way, almost everything else in this field lies far beyond the Coma Cluster. There is a fascinating assortment of background galaxies, including an apparent galaxian merger in progress

PIX4611992: Elliptical galaxy NGC 4881 and distant galaxies - Elliptical galaxy NGC 4881 and distant galaxies - The elliptical galaxy NGC 4881 (upper left) is about 300 million years away - light from Earth. NGC 4881 is located in the Coma galaxy cluster that contains at least 1,000 galaxies and is five times farther from us than the Virgin's cluster. Almost all the objects visible in this photo are located far behind the Coma cluster, except for the spiral galaxy to the right of Ngc 4881. Image obtained by the Hubble Space Telescope in 1994. This photo mosaic, which shows a field of distant galaxies, is a computer enhanced reproduction of a picture taken 4 March 1994 with the repaired Hubble Space Telescope. The brightest object in this picture is NGC 4881. It is a 13th - magnitude elliptical galaxy in the outskirts of the Coma Cluster, a great cluster of galaxies more than 5 times farther away than the Virgo Cluster. Except for a 16th - magnitude Coma spiral at the right and a few foreground stars of the Milky Way, almost everything else in this field lies far beyond the Coma Cluster. There is a fascinating assortment of background galaxies, including an apparent galaxian merger in progress / Bridgeman Images

ID: PIX4611992

Elliptical galaxy NGC 4881 and distant galaxies - Elliptical galaxy NGC 4881 and distant galaxies - The elliptical galaxy NGC 4881 (upper left) is about 300 million years away - light from Earth. NGC 4881 is located in the Coma galaxy cluster that contains at least 1,000 galaxies and is five times farther from us than the Virgin's cluster. Almost all the objects visible in this photo are located far behind the Coma cluster, except for the spiral galaxy to the right of Ngc 4881. Image obtained by the Hubble Space Telescope in 1994. This photo mosaic, which shows a field of distant galaxies, is a computer enhanced reproduction of a picture taken 4 March 1994 with the repaired Hubble Space Telescope. The brightest object in this picture is NGC 4881. It is a 13th - magnitude elliptical galaxy in the outskirts of the Coma Cluster, a great cluster of galaxies more than 5 times farther away than the Virgo Cluster. Except for a 16th - magnitude Coma spiral at the right and a few foreground sta

Spiral Galaxy NGC 4911 - Galaxy Spiral NGC 4911 - The NGC 4911 galaxy photographed here by the Hubble Space Telescope (HST) is located in the Coma galaxy cluster (Abell 1656) about 320 million light years ago. Image obtained from different cliches obtained from 2006 to 2009, 28 hours of installation in total. A long - exposure Hubble Space Telescope image shows a majestic face - on spiral galaxy located deep within the Coma Cluster of galaxies, which lies 320 million light - years away in the northern constellation Coma Berenices. The galaxy, known as NGC 4911, contains rich lanes of dust and gas near its center. These are silhouetted against glowing newborn star clusters and iridescent pink clouds of hydrogen, the existence of which indicates ongoing star formation. Hubble has also captured the outer spiral arms of NGC 4911, along with thousands of other galaxies of varying sizes. This natural - color Hubble image, which combines data obtained in 2006, 2007, and 2009 from the Wide Field Planetary Camera 2 and the Advanced Camera for Surveys, required 28 hours of exposure time
Spiral Galaxy NGC 4911 - Galaxy Spiral NGC 4911 - The NGC 4911 galaxy photographed here by the Hubble Space Telescope (HST) is located in the Coma galaxy cluster (Abell 1656) about 320 million light years ago. Image obtained from different cliches obtained from 2006 to 2009, 28 hours of installation in total. A long - exposure Hubble Space Telescope image shows a majestic face - on spiral galaxy located deep within the Coma Cluster of galaxies, which lies 320 million light - years away in the northern constellation Coma Berenices. The galaxy, known as NGC 4911, contains rich lanes of dust and gas near its center. These are silhouetted against glowing newborn star clusters and iridescent pink clouds of hydrogen, the existence of which indicates ongoing star formation. Hubble has also captured the outer spiral arms of NGC 4911, along with thousands of other galaxies of varying sizes. This natural - color Hubble image, which combines data obtained in 2006, 2007, and 2009 from the Wide Field Planetary Camera 2 and the Advanced Camera for Surveys, required 28 hours of exposure time

PIX4612005: Spiral Galaxy NGC 4911 - Galaxy Spiral NGC 4911 - The NGC 4911 galaxy photographed here by the Hubble Space Telescope (HST) is located in the Coma galaxy cluster (Abell 1656) about 320 million light years ago. Image obtained from different cliches obtained from 2006 to 2009, 28 hours of installation in total. A long - exposure Hubble Space Telescope image shows a majestic face - on spiral galaxy located deep within the Coma Cluster of galaxies, which lies 320 million light - years away in the northern constellation Coma Berenices. The galaxy, known as NGC 4911, contains rich lanes of dust and gas near its center. These are silhouetted against glowing newborn star clusters and iridescent pink clouds of hydrogen, the existence of which indicates ongoing star formation. Hubble has also captured the outer spiral arms of NGC 4911, along with thousands of other galaxies of varying sizes. This natural - color Hubble image, which combines data obtained in 2006, 2007, and 2009 from the Wide Field Planetary Camera 2 and the Advanced Camera for Surveys, required 28 hours of exposure time / Bridgeman Images

ID: PIX4612005

Spiral Galaxy NGC 4911 - Galaxy Spiral NGC 4911 - The NGC 4911 galaxy photographed here by the Hubble Space Telescope (HST) is located in the Coma galaxy cluster (Abell 1656) about 320 million light years ago. Image obtained from different cliches obtained from 2006 to 2009, 28 hours of installation in total. A long - exposure Hubble Space Telescope image shows a majestic face - on spiral galaxy located deep within the Coma Cluster of galaxies, which lies 320 million light - years away in the northern constellation Coma Berenices. The galaxy, known as NGC 4911, contains rich lanes of dust and gas near its center. These are silhouetted against glowing newborn star clusters and iridescent pink clouds of hydrogen, the existence of which indicates ongoing star formation. Hubble has also captured the outer spiral arms of NGC 4911, along with thousands of other galaxies of varying sizes. This natural - color Hubble image, which combines data obtained in 2006, 2007, and 2009 from the Wide Fie

White dodo I by Pieter II Holsteyn, female, 1638. Heliotype by Van Leer from Dr. Anthonie Cornelis Oudemans' Dodo Studies, Amsterdam, Johannes Muller, 1917.
White dodo I by Pieter II Holsteyn, female, 1638. Heliotype by Van Leer from Dr. Anthonie Cornelis Oudemans' Dodo Studies, Amsterdam, Johannes Muller, 1917.

FLO4612010: White dodo I by Pieter II Holsteyn, female, 1638. Heliotype by Van Leer from Dr. Anthonie Cornelis Oudemans' Dodo Studies, Amsterdam, Johannes Muller, 1917. / Bridgeman Images

ID: FLO4612010

White dodo I by Pieter II Holsteyn, female, 1638. Heliotype by Van Leer from Dr. Anthonie Cornelis Oudemans' Dodo Studies, Amsterdam, Johannes Muller, 1917.

Spiral Galaxy NGC 4945 in Centaurus - Spiral galaxy NGC 4945 in Centaurus - The barree spiral galaxy NGC 4945 is located about 13 million years ago - light from Earth. This remarkable spiral galaxy seen almost edge - on is located at about 13 million years away in southern constellation of Centaurus. The galaxy is extremely dusty, and it is seen through dust in the Milky Way
Spiral Galaxy NGC 4945 in Centaurus - Spiral galaxy NGC 4945 in Centaurus - The barree spiral galaxy NGC 4945 is located about 13 million years ago - light from Earth. This remarkable spiral galaxy seen almost edge - on is located at about 13 million years away in southern constellation of Centaurus. The galaxy is extremely dusty, and it is seen through dust in the Milky Way

PIX4612036: Spiral Galaxy NGC 4945 in Centaurus - Spiral galaxy NGC 4945 in Centaurus - The barree spiral galaxy NGC 4945 is located about 13 million years ago - light from Earth. This remarkable spiral galaxy seen almost edge - on is located at about 13 million years away in southern constellation of Centaurus. The galaxy is extremely dusty, and it is seen through dust in the Milky Way / Bridgeman Images

ID: PIX4612036

Spiral Galaxy NGC 4945 in Centaurus - Spiral galaxy NGC 4945 in Centaurus - The barree spiral galaxy NGC 4945 is located about 13 million years ago - light from Earth. This remarkable spiral galaxy seen almost edge - on is located at about 13 million years away in southern constellation of Centaurus. The galaxy is extremely dusty, and it is seen through dust in the Milky Way

White dodo by Johann Walther, female, 1657 (27) and white dodo by Jacob Hoefnagel, young male, 1609 (28). Heliotype by Van Leer from Dr. Anthonie Cornelis Oudemans' Dodo Studies, Amsterdam, Johannes Muller, 1917.
White dodo by Johann Walther, female, 1657 (27) and white dodo by Jacob Hoefnagel, young male, 1609 (28). Heliotype by Van Leer from Dr. Anthonie Cornelis Oudemans' Dodo Studies, Amsterdam, Johannes Muller, 1917.

FLO4612042: White dodo by Johann Walther, female, 1657 (27) and white dodo by Jacob Hoefnagel, young male, 1609 (28). Heliotype by Van Leer from Dr. Anthonie Cornelis Oudemans' Dodo Studies, Amsterdam, Johannes Muller, 1917. / Bridgeman Images

ID: FLO4612042

White dodo by Johann Walther, female, 1657 (27) and white dodo by Jacob Hoefnagel, young male, 1609 (28). Heliotype by Van Leer from Dr. Anthonie Cornelis Oudemans' Dodo Studies, Amsterdam, Johannes Muller, 1917.

Images of a male Rodrigues solitaire, Pezophaps solitaria, from Francois Lequat's Voyages, 1708. Heliotype by Van Leer from Dr. Anthonie Cornelis Oudemans' Dodo Studies, Amsterdam, Johannes Muller, 1917.
Images of a male Rodrigues solitaire, Pezophaps solitaria, from Francois Lequat's Voyages, 1708. Heliotype by Van Leer from Dr. Anthonie Cornelis Oudemans' Dodo Studies, Amsterdam, Johannes Muller, 1917.

FLO4612049: Images of a male Rodrigues solitaire, Pezophaps solitaria, from Francois Lequat's Voyages, 1708. Heliotype by Van Leer from Dr. Anthonie Cornelis Oudemans' Dodo Studies, Amsterdam, Johannes Muller, 1917. / Bridgeman Images

ID: FLO4612049

Images of a male Rodrigues solitaire, Pezophaps solitaria, from Francois Lequat's Voyages, 1708. Heliotype by Van Leer from Dr. Anthonie Cornelis Oudemans' Dodo Studies, Amsterdam, Johannes Muller, 1917.

Head and tail of the dodo by Roelandt Savery, Johan Neiuhof, Jacob de Bondt, Ludwig Schmoor von Carolsfeld, G. Krause, etc. Heliotype by Van Leer from Dr. Anthonie Cornelis Oudemans' Dodo Studies, Amsterdam, Johannes Muller, 1917.
Head and tail of the dodo by Roelandt Savery, Johan Neiuhof, Jacob de Bondt, Ludwig Schmoor von Carolsfeld, G. Krause, etc. Heliotype by Van Leer from Dr. Anthonie Cornelis Oudemans' Dodo Studies, Amsterdam, Johannes Muller, 1917.

FLO4612057: Head and tail of the dodo by Roelandt Savery, Johan Neiuhof, Jacob de Bondt, Ludwig Schmoor von Carolsfeld, G. Krause, etc. Heliotype by Van Leer from Dr. Anthonie Cornelis Oudemans' Dodo Studies, Amsterdam, Johannes Muller, 1917. / Bridgeman Images

ID: FLO4612057

Head and tail of the dodo by Roelandt Savery, Johan Neiuhof, Jacob de Bondt, Ludwig Schmoor von Carolsfeld, G. Krause, etc. Heliotype by Van Leer from Dr. Anthonie Cornelis Oudemans' Dodo Studies, Amsterdam, Johannes Muller, 1917.

Title page with Willem Ysbrantsz Bontekoe's illustration of the dodo. Title page from Hugh Edwin Strickland and Alexander Gordon Melville's The Dodo and its Kindred, London, Reeve, Benham and Reeve, 1848.
Title page with Willem Ysbrantsz Bontekoe's illustration of the dodo. Title page from Hugh Edwin Strickland and Alexander Gordon Melville's The Dodo and its Kindred, London, Reeve, Benham and Reeve, 1848.

FLO4612063: Title page with Willem Ysbrantsz Bontekoe's illustration of the dodo. Title page from Hugh Edwin Strickland and Alexander Gordon Melville's The Dodo and its Kindred, London, Reeve, Benham and Reeve, 1848. / Bridgeman Images

ID: FLO4612063

Title page with Willem Ysbrantsz Bontekoe's illustration of the dodo. Title page from Hugh Edwin Strickland and Alexander Gordon Melville's The Dodo and its Kindred, London, Reeve, Benham and Reeve, 1848.

Spiral Galaxy NGC 4921 - Unusual Spiral NGC 4921 in the Coma Galaxy Cluster - Galaxy NGC 4921 photographed by the Hubble Space Telescope (HST). Located in the cluster of Coma galaxies (Abell 1656) is about 320 million light years old, this spiral galaxy presents an unusual structure with poorly marked arms; some young blue stars are visible but the activity of star formation here is much less strong than in other spiral galaxies. In the background, many more distant galaxies appear. This very deep image taken with the NASA/ESA Hubble Space Telescope shows the spiral galaxy NGC 4921 along with a spectacular backdrop of more distant galaxies. It was created from a total of 80 separate pictures through yellow and near - infrared filters. The Coma Galaxy Cluster, in the northern constellation of Coma Berenices, the hair of Queen Berenice, is one of the closest very rich collections of galaxies in the nearby Universe. The cluster, also known as Abell 1656, is about 320 million light - years from Earth and contains more than 1000 members. The brightest galaxies, including NGC 4921 shown here, were discovered back in the late 18th century by William Herschel. The galaxies in rich clusters undergo many interactions and mergers that tend to gradually turn gas - rich spirals into elliptical systems without much active star formation. As a result there are far more ellipticals and fewer spirals in the Coma Cluster than are found in quieter corners of the Universe. NGC 4921 is one of the rare spirals in Coma, and a rather unusual one - - it is an example of an “” anaemic spiral”” where the normal vigorous star formation that creates a spiral galaxy's familiar bright arms is much less intense. As a result there is just a delicate swirl of dust in a ring around the galaxy, accompanied by some bright young blue stars that are clearly separated out by Hubble's sharp vision. Much of the pale spiral structure in the outer
Spiral Galaxy NGC 4921 - Unusual Spiral NGC 4921 in the Coma Galaxy Cluster - Galaxy NGC 4921 photographed by the Hubble Space Telescope (HST). Located in the cluster of Coma galaxies (Abell 1656) is about 320 million light years old, this spiral galaxy presents an unusual structure with poorly marked arms; some young blue stars are visible but the activity of star formation here is much less strong than in other spiral galaxies. In the background, many more distant galaxies appear. This very deep image taken with the NASA/ESA Hubble Space Telescope shows the spiral galaxy NGC 4921 along with a spectacular backdrop of more distant galaxies. It was created from a total of 80 separate pictures through yellow and near - infrared filters. The Coma Galaxy Cluster, in the northern constellation of Coma Berenices, the hair of Queen Berenice, is one of the closest very rich collections of galaxies in the nearby Universe. The cluster, also known as Abell 1656, is about 320 million light - years from Earth and contains more than 1000 members. The brightest galaxies, including NGC 4921 shown here, were discovered back in the late 18th century by William Herschel. The galaxies in rich clusters undergo many interactions and mergers that tend to gradually turn gas - rich spirals into elliptical systems without much active star formation. As a result there are far more ellipticals and fewer spirals in the Coma Cluster than are found in quieter corners of the Universe. NGC 4921 is one of the rare spirals in Coma, and a rather unusual one - - it is an example of an “” anaemic spiral”” where the normal vigorous star formation that creates a spiral galaxy's familiar bright arms is much less intense. As a result there is just a delicate swirl of dust in a ring around the galaxy, accompanied by some bright young blue stars that are clearly separated out by Hubble's sharp vision. Much of the pale spiral structure in the outer

PIX4612079: Spiral Galaxy NGC 4921 - Unusual Spiral NGC 4921 in the Coma Galaxy Cluster - Galaxy NGC 4921 photographed by the Hubble Space Telescope (HST). Located in the cluster of Coma galaxies (Abell 1656) is about 320 million light years old, this spiral galaxy presents an unusual structure with poorly marked arms; some young blue stars are visible but the activity of star formation here is much less strong than in other spiral galaxies. In the background, many more distant galaxies appear. This very deep image taken with the NASA/ESA Hubble Space Telescope shows the spiral galaxy NGC 4921 along with a spectacular backdrop of more distant galaxies. It was created from a total of 80 separate pictures through yellow and near - infrared filters. The Coma Galaxy Cluster, in the northern constellation of Coma Berenices, the hair of Queen Berenice, is one of the closest very rich collections of galaxies in the nearby Universe. The cluster, also known as Abell 1656, is about 320 million light - years from Earth and contains more than 1000 members. The brightest galaxies, including NGC 4921 shown here, were discovered back in the late 18th century by William Herschel. The galaxies in rich clusters undergo many interactions and mergers that tend to gradually turn gas - rich spirals into elliptical systems without much active star formation. As a result there are far more ellipticals and fewer spirals in the Coma Cluster than are found in quieter corners of the Universe. NGC 4921 is one of the rare spirals in Coma, and a rather unusual one - - it is an example of an “” anaemic spiral”” where the normal vigorous star formation that creates a spiral galaxy's familiar bright arms is much less intense. As a result there is just a delicate swirl of dust in a ring around the galaxy, accompanied by some bright young blue stars that are clearly separated out by Hubble's sharp vision. Much of the pale spiral structure in the outer / Bridgeman Images

ID: PIX4612079

Spiral Galaxy NGC 4921 - Unusual Spiral NGC 4921 in the Coma Galaxy Cluster - Galaxy NGC 4921 photographed by the Hubble Space Telescope (HST). Located in the cluster of Coma galaxies (Abell 1656) is about 320 million light years old, this spiral galaxy presents an unusual structure with poorly marked arms; some young blue stars are visible but the activity of star formation here is much less strong than in other spiral galaxies. In the background, many more distant galaxies appear. This very deep image taken with the NASA/ESA Hubble Space Telescope shows the spiral galaxy NGC 4921 along with a spectacular backdrop of more distant galaxies. It was created from a total of 80 separate pictures through yellow and near - infrared filters. The Coma Galaxy Cluster, in the northern constellation of Coma Berenices, the hair of Queen Berenice, is one of the closest very rich collections of galaxies in the nearby Universe. The cluster, also known as Abell 1656, is about 320 million light - years

Spiral galaxy M63 (NGC 5055) in Hunting Dogs - Spiral galaxy M63 - The spiral galaxy M63 (NGC 5055) is about 35 million years away - light from Earth. Image obtained with a 50 cm telescope, composite of several poses. M63 (NGC 5055) is a spiral glaxy in the contellation Canes Venatici at about 35 million light - years from Earth
Spiral galaxy M63 (NGC 5055) in Hunting Dogs - Spiral galaxy M63 - The spiral galaxy M63 (NGC 5055) is about 35 million years away - light from Earth. Image obtained with a 50 cm telescope, composite of several poses. M63 (NGC 5055) is a spiral glaxy in the contellation Canes Venatici at about 35 million light - years from Earth

PIX4612096: Spiral galaxy M63 (NGC 5055) in Hunting Dogs - Spiral galaxy M63 - The spiral galaxy M63 (NGC 5055) is about 35 million years away - light from Earth. Image obtained with a 50 cm telescope, composite of several poses. M63 (NGC 5055) is a spiral glaxy in the contellation Canes Venatici at about 35 million light - years from Earth / Bridgeman Images

ID: PIX4612096

Spiral galaxy M63 (NGC 5055) in Hunting Dogs - Spiral galaxy M63 - The spiral galaxy M63 (NGC 5055) is about 35 million years away - light from Earth. Image obtained with a 50 cm telescope, composite of several poses. M63 (NGC 5055) is a spiral glaxy in the contellation Canes Venatici at about 35 million light - years from Earth

Illustration of a Rodrigues solitaire, 1848 (lithograph)
Illustration of a Rodrigues solitaire, 1848 (lithograph)

FLO4612102: Illustration of a Rodrigues solitaire, 1848 (lithograph) / Bridgeman Images

ID: FLO4612102

Illustration of a Rodrigues solitaire, 1848 (lithograph)

Spiral Galaxy M63 in Hunting Dogs - Spiral galaxy M63 in Canes Venatici - The spiral galaxy M63 (NGC 5055) is located about 35 million years ago - light from Earth. Image obtained with a 61 cm telescope, composite of several poses. M63 (NGC 5055) is a spiral glaxy in the contellation Canes Venatici at about 35 million light - years from Earth. Image taken with a 24 - inch telescope
Spiral Galaxy M63 in Hunting Dogs - Spiral galaxy M63 in Canes Venatici - The spiral galaxy M63 (NGC 5055) is located about 35 million years ago - light from Earth. Image obtained with a 61 cm telescope, composite of several poses. M63 (NGC 5055) is a spiral glaxy in the contellation Canes Venatici at about 35 million light - years from Earth. Image taken with a 24 - inch telescope

PIX4612151: Spiral Galaxy M63 in Hunting Dogs - Spiral galaxy M63 in Canes Venatici - The spiral galaxy M63 (NGC 5055) is located about 35 million years ago - light from Earth. Image obtained with a 61 cm telescope, composite of several poses. M63 (NGC 5055) is a spiral glaxy in the contellation Canes Venatici at about 35 million light - years from Earth. Image taken with a 24 - inch telescope / Bridgeman Images

ID: PIX4612151

Spiral Galaxy M63 in Hunting Dogs - Spiral galaxy M63 in Canes Venatici - The spiral galaxy M63 (NGC 5055) is located about 35 million years ago - light from Earth. Image obtained with a 61 cm telescope, composite of several poses. M63 (NGC 5055) is a spiral glaxy in the contellation Canes Venatici at about 35 million light - years from Earth. Image taken with a 24 - inch telescope

Centaurus A Elliptical Galaxy (NGC 5128) in the Centaur - Galaxy Centaurus A - The NGC 5128 galaxy is about 13 million years away - light from Earth. This image obtained by the Hubble Space Telescope in 1998 shows the star flames that occur in the dark band of the galaxy. In blue, these are the clusters of newly shaped young stars. At the top left, a photo of the galaxy obtained from the ground. This giant galaxy is a powerful radio source known as Centaurus A. It is an active galaxy whose energy comes from a supermassive black hole. NGC 5128 is the nearest large elliptical galaxies to our sun. It is also the nearest of the giant radio galaxies, possessing an active galactic nucleus (AGN) and optically one of the most luminous galaxies in the sky. Among many other things NGC 5128 is also the prototypical postmerger elliptical galaxy. Structural peculiarities including the prominent rotating disk of stars and gas and the complex shell structure of its halo point to a large scale merger within the last billion years. Tidal streams of young stars have also been identified in the halo of NGC 5128 thought to have occurred by cannibalization of a nearby gas rich dwarf galaxy some 300 million years ago, long after the large scale merger. Elliptical galaxies are typically devoid of gas, dust and young stars. The unexpected presence of gas rich disk elements within the structure of NGC 5128 supports the current belief that accretions and mergers of low mass galaxies may be an important agent in the evolution of galaxy formation. As a radio galaxy, NGC 5128 belongs to the subgroup of galaxies called Active Galaxies, which include Quasars, Seyfert galaxies, Blazars and Radio Galaxies. Active galaxies are distinguished by their prodigious energy output which cannot be explained by their stellar populations and must have another source. Active galaxies have in common an “Active Galactic Nucleus (AGN)”” which is beli
Centaurus A Elliptical Galaxy (NGC 5128) in the Centaur - Galaxy Centaurus A - The NGC 5128 galaxy is about 13 million years away - light from Earth. This image obtained by the Hubble Space Telescope in 1998 shows the star flames that occur in the dark band of the galaxy. In blue, these are the clusters of newly shaped young stars. At the top left, a photo of the galaxy obtained from the ground. This giant galaxy is a powerful radio source known as Centaurus A. It is an active galaxy whose energy comes from a supermassive black hole. NGC 5128 is the nearest large elliptical galaxies to our sun. It is also the nearest of the giant radio galaxies, possessing an active galactic nucleus (AGN) and optically one of the most luminous galaxies in the sky. Among many other things NGC 5128 is also the prototypical postmerger elliptical galaxy. Structural peculiarities including the prominent rotating disk of stars and gas and the complex shell structure of its halo point to a large scale merger within the last billion years. Tidal streams of young stars have also been identified in the halo of NGC 5128 thought to have occurred by cannibalization of a nearby gas rich dwarf galaxy some 300 million years ago, long after the large scale merger. Elliptical galaxies are typically devoid of gas, dust and young stars. The unexpected presence of gas rich disk elements within the structure of NGC 5128 supports the current belief that accretions and mergers of low mass galaxies may be an important agent in the evolution of galaxy formation. As a radio galaxy, NGC 5128 belongs to the subgroup of galaxies called Active Galaxies, which include Quasars, Seyfert galaxies, Blazars and Radio Galaxies. Active galaxies are distinguished by their prodigious energy output which cannot be explained by their stellar populations and must have another source. Active galaxies have in common an “Active Galactic Nucleus (AGN)”” which is beli

PIX4612157: Centaurus A Elliptical Galaxy (NGC 5128) in the Centaur - Galaxy Centaurus A - The NGC 5128 galaxy is about 13 million years away - light from Earth. This image obtained by the Hubble Space Telescope in 1998 shows the star flames that occur in the dark band of the galaxy. In blue, these are the clusters of newly shaped young stars. At the top left, a photo of the galaxy obtained from the ground. This giant galaxy is a powerful radio source known as Centaurus A. It is an active galaxy whose energy comes from a supermassive black hole. NGC 5128 is the nearest large elliptical galaxies to our sun. It is also the nearest of the giant radio galaxies, possessing an active galactic nucleus (AGN) and optically one of the most luminous galaxies in the sky. Among many other things NGC 5128 is also the prototypical postmerger elliptical galaxy. Structural peculiarities including the prominent rotating disk of stars and gas and the complex shell structure of its halo point to a large scale merger within the last billion years. Tidal streams of young stars have also been identified in the halo of NGC 5128 thought to have occurred by cannibalization of a nearby gas rich dwarf galaxy some 300 million years ago, long after the large scale merger. Elliptical galaxies are typically devoid of gas, dust and young stars. The unexpected presence of gas rich disk elements within the structure of NGC 5128 supports the current belief that accretions and mergers of low mass galaxies may be an important agent in the evolution of galaxy formation. As a radio galaxy, NGC 5128 belongs to the subgroup of galaxies called Active Galaxies, which include Quasars, Seyfert galaxies, Blazars and Radio Galaxies. Active galaxies are distinguished by their prodigious energy output which cannot be explained by their stellar populations and must have another source. Active galaxies have in common an “Active Galactic Nucleus (AGN)”” which is beli / Bridgeman Images

ID: PIX4612157

Centaurus A Elliptical Galaxy (NGC 5128) in the Centaur - Galaxy Centaurus A - The NGC 5128 galaxy is about 13 million years away - light from Earth. This image obtained by the Hubble Space Telescope in 1998 shows the star flames that occur in the dark band of the galaxy. In blue, these are the clusters of newly shaped young stars. At the top left, a photo of the galaxy obtained from the ground. This giant galaxy is a powerful radio source known as Centaurus A. It is an active galaxy whose energy comes from a supermassive black hole. NGC 5128 is the nearest large elliptical galaxies to our sun. It is also the nearest of the giant radio galaxies, possessing an active galactic nucleus (AGN) and optically one of the most luminous galaxies in the sky. Among many other things NGC 5128 is also the prototypical postmerger elliptical galaxy. Structural peculiarities including the prominent rotating disk of stars and gas and the complex shell structure of its halo point to a large scale merger

Back view of skull, upper and lower view of lower jaw, inner view of jaw, and circle of sclerotic bones in the dodo. Lithograph from Hugh Edwin Strickland and Alexander Gordon Melville's The Dodo and its Kindred, London, Reeve, Benham and Reeve, 1848.
Back view of skull, upper and lower view of lower jaw, inner view of jaw, and circle of sclerotic bones in the dodo. Lithograph from Hugh Edwin Strickland and Alexander Gordon Melville's The Dodo and its Kindred, London, Reeve, Benham and Reeve, 1848.

FLO4612158: Back view of skull, upper and lower view of lower jaw, inner view of jaw, and circle of sclerotic bones in the dodo. Lithograph from Hugh Edwin Strickland and Alexander Gordon Melville's The Dodo and its Kindred, London, Reeve, Benham and Reeve, 1848. / Bridgeman Images

ID: FLO4612158

Back view of skull, upper and lower view of lower jaw, inner view of jaw, and circle of sclerotic bones in the dodo. Lithograph from Hugh Edwin Strickland and Alexander Gordon Melville's The Dodo and its Kindred, London, Reeve, Benham and Reeve, 1848.

Galaxy NGC 5101 in Hydra - Galaxy NGC 5101 in Hydr
Galaxy NGC 5101 in Hydra - Galaxy NGC 5101 in Hydr

PIX4612187: Galaxy NGC 5101 in Hydra - Galaxy NGC 5101 in Hydr / Bridgeman Images

ID: PIX4612187

Galaxy NGC 5101 in Hydra - Galaxy NGC 5101 in Hydr


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