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Bard in distinctive sky-blue robes with 12-string harp, Briton in the Roman fashion of multicolored cape and red tunic, and two female Britons in tunic and skirts. Handcoloured copperplate engraving by Verico from Giulio Ferrario's Costumes Ancient and Modern of the Peoples of the World, 1847.
Bard in distinctive sky-blue robes with 12-string harp, Briton in the Roman fashion of multicolored cape and red tunic, and two female Britons in tunic and skirts. Handcoloured copperplate engraving by Verico from Giulio Ferrario's Costumes Ancient and Modern of the Peoples of the World, 1847.

FLO4623166: Bard in distinctive sky-blue robes with 12-string harp, Briton in the Roman fashion of multicolored cape and red tunic, and two female Britons in tunic and skirts. Handcoloured copperplate engraving by Verico from Giulio Ferrario's Costumes Ancient and Modern of the Peoples of the World, 1847. / Bridgeman Images

ID: FLO4623166

Bard in distinctive sky-blue robes with 12-string harp, Briton in the Roman fashion of multicolored cape and red tunic, and two female Britons in tunic and skirts. Handcoloured copperplate engraving by Verico from Giulio Ferrario's Costumes Ancient and Modern of the Peoples of the World, 1847.

Section through a dome-shaped Lapp (Sami) fishermen's house, with hearth in centre. Handcoloured copperplate engraving by Giarre and Stanghi from Giulio Ferrario's Costumes Ancient and Modern of the Peoples of the World, 1847.
Section through a dome-shaped Lapp (Sami) fishermen's house, with hearth in centre. Handcoloured copperplate engraving by Giarre and Stanghi from Giulio Ferrario's Costumes Ancient and Modern of the Peoples of the World, 1847.

FLO4623181: Section through a dome-shaped Lapp (Sami) fishermen's house, with hearth in centre. Handcoloured copperplate engraving by Giarre and Stanghi from Giulio Ferrario's Costumes Ancient and Modern of the Peoples of the World, 1847. / Bridgeman Images

ID: FLO4623181

Section through a dome-shaped Lapp (Sami) fishermen's house, with hearth in centre. Handcoloured copperplate engraving by Giarre and Stanghi from Giulio Ferrario's Costumes Ancient and Modern of the Peoples of the World, 1847.

Dome-shaped house of the Sami people, Lapland. Handcoloured copperplate engraving by Giarre from Giulio Ferrario's Costumes Ancient and Modern of the Peoples of the World, 1847.
Dome-shaped house of the Sami people, Lapland. Handcoloured copperplate engraving by Giarre from Giulio Ferrario's Costumes Ancient and Modern of the Peoples of the World, 1847.

FLO4623191: Dome-shaped house of the Sami people, Lapland. Handcoloured copperplate engraving by Giarre from Giulio Ferrario's Costumes Ancient and Modern of the Peoples of the World, 1847. / Bridgeman Images

ID: FLO4623191

Dome-shaped house of the Sami people, Lapland. Handcoloured copperplate engraving by Giarre from Giulio Ferrario's Costumes Ancient and Modern of the Peoples of the World, 1847.

Planetary nebula NGC 6369 in Ophiuchus/HST - NGC 6369 is known to amateur astronomers as the “” Little Ghost Nebula,”” because it appears as a small, ghostly cloud surrounding the faint, dying central star. NGC 6369 lies in the direction of the constellation Ophiuchus, at a distance estimated to be between about 2,000 and 5,000 light - years from Earth. When a star with a mass similar to that of our own Sun nears the end of its lifetime, it expands in size to become a red giant. The red - giant stage ends when the star expels its outer layers into space, producing a faintly glowing nebula. Astronomers call such an object a planetary nebula, because its round shape resembles that of a planet when viewed with a small telescope. The Hubble photograph of NGC 6369, captured with the Wide Field Planetary Camera 2 (WFPC2) in February 2002, reveals remarkable details of the ejection process that are not visible from ground - based telescopes because of the blurring produced by the Earth's atmosphere. The remnant stellar core in the center is now sending out a flood of ultraviolet (UV) light into the surrounding gas. The prominent blue - green ring, nearly a light - year in diameter, marks the location where the energetic UV light has stripped electrons off of atoms in the gas. This process is called ionization. In the redder gas at larger distances from the star, where the UV light is less intense, the ionization process is less advanced. Even farther outside the main body of the nebula, one can see fainter wisps of gas that were lost from the star at the beginning of the ejection process. The color image has been produced by combining WFPC2 pictures taken through filters that isolate light emitted by three different chemical elements with different degrees of ionization. The doughnut - shaped blue - green ring represents light from ionized oxygen atoms that have lost two electrons (blue) and from hydrogen atoms that have lost their single electrons (green). Red marks
Planetary nebula NGC 6369 in Ophiuchus/HST - NGC 6369 is known to amateur astronomers as the “” Little Ghost Nebula,”” because it appears as a small, ghostly cloud surrounding the faint, dying central star. NGC 6369 lies in the direction of the constellation Ophiuchus, at a distance estimated to be between about 2,000 and 5,000 light - years from Earth. When a star with a mass similar to that of our own Sun nears the end of its lifetime, it expands in size to become a red giant. The red - giant stage ends when the star expels its outer layers into space, producing a faintly glowing nebula. Astronomers call such an object a planetary nebula, because its round shape resembles that of a planet when viewed with a small telescope. The Hubble photograph of NGC 6369, captured with the Wide Field Planetary Camera 2 (WFPC2) in February 2002, reveals remarkable details of the ejection process that are not visible from ground - based telescopes because of the blurring produced by the Earth's atmosphere. The remnant stellar core in the center is now sending out a flood of ultraviolet (UV) light into the surrounding gas. The prominent blue - green ring, nearly a light - year in diameter, marks the location where the energetic UV light has stripped electrons off of atoms in the gas. This process is called ionization. In the redder gas at larger distances from the star, where the UV light is less intense, the ionization process is less advanced. Even farther outside the main body of the nebula, one can see fainter wisps of gas that were lost from the star at the beginning of the ejection process. The color image has been produced by combining WFPC2 pictures taken through filters that isolate light emitted by three different chemical elements with different degrees of ionization. The doughnut - shaped blue - green ring represents light from ionized oxygen atoms that have lost two electrons (blue) and from hydrogen atoms that have lost their single electrons (green). Red marks

PIX4623194: Planetary nebula NGC 6369 in Ophiuchus/HST - NGC 6369 is known to amateur astronomers as the “” Little Ghost Nebula,”” because it appears as a small, ghostly cloud surrounding the faint, dying central star. NGC 6369 lies in the direction of the constellation Ophiuchus, at a distance estimated to be between about 2,000 and 5,000 light - years from Earth. When a star with a mass similar to that of our own Sun nears the end of its lifetime, it expands in size to become a red giant. The red - giant stage ends when the star expels its outer layers into space, producing a faintly glowing nebula. Astronomers call such an object a planetary nebula, because its round shape resembles that of a planet when viewed with a small telescope. The Hubble photograph of NGC 6369, captured with the Wide Field Planetary Camera 2 (WFPC2) in February 2002, reveals remarkable details of the ejection process that are not visible from ground - based telescopes because of the blurring produced by the Earth's atmosphere. The remnant stellar core in the center is now sending out a flood of ultraviolet (UV) light into the surrounding gas. The prominent blue - green ring, nearly a light - year in diameter, marks the location where the energetic UV light has stripped electrons off of atoms in the gas. This process is called ionization. In the redder gas at larger distances from the star, where the UV light is less intense, the ionization process is less advanced. Even farther outside the main body of the nebula, one can see fainter wisps of gas that were lost from the star at the beginning of the ejection process. The color image has been produced by combining WFPC2 pictures taken through filters that isolate light emitted by three different chemical elements with different degrees of ionization. The doughnut - shaped blue - green ring represents light from ionized oxygen atoms that have lost two electrons (blue) and from hydrogen atoms that have lost their single electrons (green). Red marks / Bridgeman Images

ID: PIX4623194

Planetary nebula NGC 6369 in Ophiuchus/HST - NGC 6369 is known to amateur astronomers as the “” Little Ghost Nebula,”” because it appears as a small, ghostly cloud surrounding the faint, dying central star. NGC 6369 lies in the direction of the constellation Ophiuchus, at a distance estimated to be between about 2,000 and 5,000 light - years from Earth. When a star with a mass similar to that of our own Sun nears the end of its lifetime, it expands in size to become a red giant. The red - giant stage ends when the star expels its outer layers into space, producing a faintly glowing nebula. Astronomers call such an object a planetary nebula, because its round shape resembles that of a planet when viewed with a small telescope. The Hubble photograph of NGC 6369, captured with the Wide Field Planetary Camera 2 (WFPC2) in February 2002, reveals remarkable details of the ejection process that are not visible from ground - based telescopes because of the blurring produced by the Earth's atmo

Planetary nebula NGC 6563 in Sagittarius - Planetary nebula NGC 6563 in Sagittarius - Image obtained on 1 June 2008 with a telescope 61 cm in diameter. Image taken on June 1st 2008 with a 24 - inch telescope
Planetary nebula NGC 6563 in Sagittarius - Planetary nebula NGC 6563 in Sagittarius - Image obtained on 1 June 2008 with a telescope 61 cm in diameter. Image taken on June 1st 2008 with a 24 - inch telescope

PIX4623282: Planetary nebula NGC 6563 in Sagittarius - Planetary nebula NGC 6563 in Sagittarius - Image obtained on 1 June 2008 with a telescope 61 cm in diameter. Image taken on June 1st 2008 with a 24 - inch telescope / Bridgeman Images

ID: PIX4623282

Planetary nebula NGC 6563 in Sagittarius - Planetary nebula NGC 6563 in Sagittarius - Image obtained on 1 June 2008 with a telescope 61 cm in diameter. Image taken on June 1st 2008 with a 24 - inch telescope

Planetary nebula M57 (NGC 6720) in the Lyr
Planetary nebula M57 (NGC 6720) in the Lyr

PIX4623287: Planetary nebula M57 (NGC 6720) in the Lyr / Bridgeman Images

ID: PIX4623287

Planetary nebula M57 (NGC 6720) in the Lyr

Planetary Nebula M57 (NGC 6720) in the Lyre/HST - The Hubble Space Telescope has captured the sharpest view yet of M57, the Ring Nebula in Lyra, which is the most famous of all planetary nebulae. In this image, the telescope has looked down a tunnel of gas cast off by a dying star thousands of years ago. This photo reveals elongated dark clumps of material embedded in the gas at the edge of the nebula, and the dying central star floating in a blue haze of hot gas. The nebula is about a light - year in diameter, and is located some 2,000 light - years from Earth in the direction of the constellation Lyra. The colors are approximately true colors, and represent three different chemical elements: helium (blue), oxygen (green), and nitrogen (red). 16/10/1998 1hour exhibition
Planetary Nebula M57 (NGC 6720) in the Lyre/HST - The Hubble Space Telescope has captured the sharpest view yet of M57, the Ring Nebula in Lyra, which is the most famous of all planetary nebulae. In this image, the telescope has looked down a tunnel of gas cast off by a dying star thousands of years ago. This photo reveals elongated dark clumps of material embedded in the gas at the edge of the nebula, and the dying central star floating in a blue haze of hot gas. The nebula is about a light - year in diameter, and is located some 2,000 light - years from Earth in the direction of the constellation Lyra. The colors are approximately true colors, and represent three different chemical elements: helium (blue), oxygen (green), and nitrogen (red). 16/10/1998 1hour exhibition

PIX4623298: Planetary Nebula M57 (NGC 6720) in the Lyre/HST - The Hubble Space Telescope has captured the sharpest view yet of M57, the Ring Nebula in Lyra, which is the most famous of all planetary nebulae. In this image, the telescope has looked down a tunnel of gas cast off by a dying star thousands of years ago. This photo reveals elongated dark clumps of material embedded in the gas at the edge of the nebula, and the dying central star floating in a blue haze of hot gas. The nebula is about a light - year in diameter, and is located some 2,000 light - years from Earth in the direction of the constellation Lyra. The colors are approximately true colors, and represent three different chemical elements: helium (blue), oxygen (green), and nitrogen (red). 16/10/1998 1hour exhibition / Bridgeman Images

ID: PIX4623298

Planetary Nebula M57 (NGC 6720) in the Lyre/HST - The Hubble Space Telescope has captured the sharpest view yet of M57, the Ring Nebula in Lyra, which is the most famous of all planetary nebulae. In this image, the telescope has looked down a tunnel of gas cast off by a dying star thousands of years ago. This photo reveals elongated dark clumps of material embedded in the gas at the edge of the nebula, and the dying central star floating in a blue haze of hot gas. The nebula is about a light - year in diameter, and is located some 2,000 light - years from Earth in the direction of the constellation Lyra. The colors are approximately true colors, and represent three different chemical elements: helium (blue), oxygen (green), and nitrogen (red). 16/10/1998 1hour exhibition

Jousting helm 1, horned helmet of the Earl of Dammartin 2, winged helm of the Constable of Clisson 3, royal helm 4 and chainmail hood and cap 5, and flat-headed helms circa 1230 during the reign of King Philip II, 6,7. Handcoloured copperplate engraving by Verico from Giulio Ferrario's Ancient and Modern Costumes of all the Peoples of the World, 1844.
Jousting helm 1, horned helmet of the Earl of Dammartin 2, winged helm of the Constable of Clisson 3, royal helm 4 and chainmail hood and cap 5, and flat-headed helms circa 1230 during the reign of King Philip II, 6,7. Handcoloured copperplate engraving by Verico from Giulio Ferrario's Ancient and Modern Costumes of all the Peoples of the World, 1844.

FLO4623313: Jousting helm 1, horned helmet of the Earl of Dammartin 2, winged helm of the Constable of Clisson 3, royal helm 4 and chainmail hood and cap 5, and flat-headed helms circa 1230 during the reign of King Philip II, 6,7. Handcoloured copperplate engraving by Verico from Giulio Ferrario's Ancient and Modern Costumes of all the Peoples of the World, 1844. / Bridgeman Images

ID: FLO4623313

Jousting helm 1, horned helmet of the Earl of Dammartin 2, winged helm of the Constable of Clisson 3, royal helm 4 and chainmail hood and cap 5, and flat-headed helms circa 1230 during the reign of King Philip II, 6,7. Handcoloured copperplate engraving by Verico from Giulio Ferrario's Ancient and Modern Costumes of all the Peoples of the World, 1844.

Planetary nebula M57 (NGC 6720) in Lyra - The Ring nebula M57 in Lyra - The planetary nebula of Lyra (M57) is located about 2000 years - light from Earth. A planetary nebula is a gas shell from a small late-life star whose heart collapsed to become a white dwarf and expelled the outer layers of its matter. Image obtained by the Hubble Space Telescope. This close - up, visible - light view by Nasa's Hubble Space Telescope reveals new details of the Ring Nebula. The object is tilted towards Earth so that astronomers see the ring face - on. The Hubble observations reveal that the nebula's shape is more complicated than astronomers thought. The blue gas in the nebula's center is actually a football - shaped structure that pierces the red doughnut - shaped material. Hubble also uncovers the detailed structure of the dark, irregular knots of dense gas embedded along the inner rim of the ring. The knots look like spokes in a bicycle. The Hubble images have allowed the research team to match up the knots with the spikes of light around the bright, main ring, which are a shadow effect. The Ring Nebula is a well - known planetary nebula, the glowing remains of a Sun - like star. The tiny white dot in the center of the nebula is the star's hot core, called a white dwarf. The nebula is about 2,000 light - years away in the constellation Lyra. The structure measures roughly one light - year across. The Hubble observations were taken Sept. 19, 2011, by the Wide Field Camera 3. In the image, the deep blue color in the center represents helium; the cyan color of the inner ring is the glow of hydrogen and oxygen; and the reddish color of the outer ring is from nitrogen and sulfur
Planetary nebula M57 (NGC 6720) in Lyra - The Ring nebula M57 in Lyra - The planetary nebula of Lyra (M57) is located about 2000 years - light from Earth. A planetary nebula is a gas shell from a small late-life star whose heart collapsed to become a white dwarf and expelled the outer layers of its matter. Image obtained by the Hubble Space Telescope. This close - up, visible - light view by Nasa's Hubble Space Telescope reveals new details of the Ring Nebula. The object is tilted towards Earth so that astronomers see the ring face - on. The Hubble observations reveal that the nebula's shape is more complicated than astronomers thought. The blue gas in the nebula's center is actually a football - shaped structure that pierces the red doughnut - shaped material. Hubble also uncovers the detailed structure of the dark, irregular knots of dense gas embedded along the inner rim of the ring. The knots look like spokes in a bicycle. The Hubble images have allowed the research team to match up the knots with the spikes of light around the bright, main ring, which are a shadow effect. The Ring Nebula is a well - known planetary nebula, the glowing remains of a Sun - like star. The tiny white dot in the center of the nebula is the star's hot core, called a white dwarf. The nebula is about 2,000 light - years away in the constellation Lyra. The structure measures roughly one light - year across. The Hubble observations were taken Sept. 19, 2011, by the Wide Field Camera 3. In the image, the deep blue color in the center represents helium; the cyan color of the inner ring is the glow of hydrogen and oxygen; and the reddish color of the outer ring is from nitrogen and sulfur

PIX4623343: Planetary nebula M57 (NGC 6720) in Lyra - The Ring nebula M57 in Lyra - The planetary nebula of Lyra (M57) is located about 2000 years - light from Earth. A planetary nebula is a gas shell from a small late-life star whose heart collapsed to become a white dwarf and expelled the outer layers of its matter. Image obtained by the Hubble Space Telescope. This close - up, visible - light view by Nasa's Hubble Space Telescope reveals new details of the Ring Nebula. The object is tilted towards Earth so that astronomers see the ring face - on. The Hubble observations reveal that the nebula's shape is more complicated than astronomers thought. The blue gas in the nebula's center is actually a football - shaped structure that pierces the red doughnut - shaped material. Hubble also uncovers the detailed structure of the dark, irregular knots of dense gas embedded along the inner rim of the ring. The knots look like spokes in a bicycle. The Hubble images have allowed the research team to match up the knots with the spikes of light around the bright, main ring, which are a shadow effect. The Ring Nebula is a well - known planetary nebula, the glowing remains of a Sun - like star. The tiny white dot in the center of the nebula is the star's hot core, called a white dwarf. The nebula is about 2,000 light - years away in the constellation Lyra. The structure measures roughly one light - year across. The Hubble observations were taken Sept. 19, 2011, by the Wide Field Camera 3. In the image, the deep blue color in the center represents helium; the cyan color of the inner ring is the glow of hydrogen and oxygen; and the reddish color of the outer ring is from nitrogen and sulfur / Bridgeman Images

ID: PIX4623343

Planetary nebula M57 (NGC 6720) in Lyra - The Ring nebula M57 in Lyra - The planetary nebula of Lyra (M57) is located about 2000 years - light from Earth. A planetary nebula is a gas shell from a small late-life star whose heart collapsed to become a white dwarf and expelled the outer layers of its matter. Image obtained by the Hubble Space Telescope. This close - up, visible - light view by Nasa's Hubble Space Telescope reveals new details of the Ring Nebula. The object is tilted towards Earth so that astronomers see the ring face - on. The Hubble observations reveal that the nebula's shape is more complicated than astronomers thought. The blue gas in the nebula's center is actually a football - shaped structure that pierces the red doughnut - shaped material. Hubble also uncovers the detailed structure of the dark, irregular knots of dense gas embedded along the inner rim of the ring. The knots look like spokes in a bicycle. The Hubble images have allowed the research team to match u

Planetary nebula M57 (NGC 6720) in Lyra - M57 (NGC 6720) planetary nebula in Lyra - The planetary nebula of Lyra (M57) is located about 2000 years - light from Earth. With a magnitude of 9.0, this nebula is easily observed with a small telescope. A planetary nebula is a gas shell from a small late-life star whose heart collapsed to become a white dwarf and expelled the outer layers of its matter. Composite image obtained by different telescopes. The Ring Nebula, M57, is the most famous example of a planetary nebula. Located about 2,000 light years away, it has an apparent diameter of 1 arc minute and a real diameter of about one light year. At magnitude 9.0 its high surface brightness makes it an easy object, even from the city and even with small telescopes. Planetary nebula are shells of gas shed by stars late in their life cycles after using up all of their nuclear fuel. The star then ejects a significant portion of its mass in a gaseous shell, which is illuminated by its extremely hot central star, which is just the core left from the original star. The star at the center of the Ring nebula has a surface temperature of 216,000 degrees Farenheit or 120,000 degrees Celsius. Our own star, the Sun, is expected to undergo the same process in a couple of billion years. Planetary nebulae do not last long at all in cosmic terms, the shell of gas expands and diffuse, becoming invisible, and the star turns into a white dwarf. Composite image from three data sources: HST, LBT, Subaru
Planetary nebula M57 (NGC 6720) in Lyra - M57 (NGC 6720) planetary nebula in Lyra - The planetary nebula of Lyra (M57) is located about 2000 years - light from Earth. With a magnitude of 9.0, this nebula is easily observed with a small telescope. A planetary nebula is a gas shell from a small late-life star whose heart collapsed to become a white dwarf and expelled the outer layers of its matter. Composite image obtained by different telescopes. The Ring Nebula, M57, is the most famous example of a planetary nebula. Located about 2,000 light years away, it has an apparent diameter of 1 arc minute and a real diameter of about one light year. At magnitude 9.0 its high surface brightness makes it an easy object, even from the city and even with small telescopes. Planetary nebula are shells of gas shed by stars late in their life cycles after using up all of their nuclear fuel. The star then ejects a significant portion of its mass in a gaseous shell, which is illuminated by its extremely hot central star, which is just the core left from the original star. The star at the center of the Ring nebula has a surface temperature of 216,000 degrees Farenheit or 120,000 degrees Celsius. Our own star, the Sun, is expected to undergo the same process in a couple of billion years. Planetary nebulae do not last long at all in cosmic terms, the shell of gas expands and diffuse, becoming invisible, and the star turns into a white dwarf. Composite image from three data sources: HST, LBT, Subaru

PIX4623359: Planetary nebula M57 (NGC 6720) in Lyra - M57 (NGC 6720) planetary nebula in Lyra - The planetary nebula of Lyra (M57) is located about 2000 years - light from Earth. With a magnitude of 9.0, this nebula is easily observed with a small telescope. A planetary nebula is a gas shell from a small late-life star whose heart collapsed to become a white dwarf and expelled the outer layers of its matter. Composite image obtained by different telescopes. The Ring Nebula, M57, is the most famous example of a planetary nebula. Located about 2,000 light years away, it has an apparent diameter of 1 arc minute and a real diameter of about one light year. At magnitude 9.0 its high surface brightness makes it an easy object, even from the city and even with small telescopes. Planetary nebula are shells of gas shed by stars late in their life cycles after using up all of their nuclear fuel. The star then ejects a significant portion of its mass in a gaseous shell, which is illuminated by its extremely hot central star, which is just the core left from the original star. The star at the center of the Ring nebula has a surface temperature of 216,000 degrees Farenheit or 120,000 degrees Celsius. Our own star, the Sun, is expected to undergo the same process in a couple of billion years. Planetary nebulae do not last long at all in cosmic terms, the shell of gas expands and diffuse, becoming invisible, and the star turns into a white dwarf. Composite image from three data sources: HST, LBT, Subaru / Bridgeman Images

ID: PIX4623359

Planetary nebula M57 (NGC 6720) in Lyra - M57 (NGC 6720) planetary nebula in Lyra - The planetary nebula of Lyra (M57) is located about 2000 years - light from Earth. With a magnitude of 9.0, this nebula is easily observed with a small telescope. A planetary nebula is a gas shell from a small late-life star whose heart collapsed to become a white dwarf and expelled the outer layers of its matter. Composite image obtained by different telescopes. The Ring Nebula, M57, is the most famous example of a planetary nebula. Located about 2,000 light years away, it has an apparent diameter of 1 arc minute and a real diameter of about one light year. At magnitude 9.0 its high surface brightness makes it an easy object, even from the city and even with small telescopes. Planetary nebula are shells of gas shed by stars late in their life cycles after using up all of their nuclear fuel. The star then ejects a significant portion of its mass in a gaseous shell, which is illuminated by its extremely

Planetary nebula NGC 6826 in Swan - Planetary nebula NGC 6826 in Cygnus - Planetary nebula NGC 6826 is located about 2000 years - light from Earth in the constellation Swan. A planetary nebula is a gas shell from a small late-life star whose heart collapsed to become a white dwarf and expelled the outer layers of its matter. Image obtained by the Hubble Space Telescope on January 27, 1996. NGC 6826's eye - like appearance is marred by two sets of blood - red “” fliers”” that lie horizontally across the image. The surrounding faint green “” white”” of the eye is believed to be gas that made up almost half of the star's mass for most of its life. The hot remnant star (in the center of the green oval) drives a fast wind into older material, forming a hot interior bubble which pushes the older gas ahead of it to form a bright rim. (The star is one of the brightest stars in any planetary.) NGC 6826 is 2,200 light - years away in the constellation Cygnus. The Hubble telescope observation was taken Jan. 27, 1996 with the Wide Field and Planetary Camera
Planetary nebula NGC 6826 in Swan - Planetary nebula NGC 6826 in Cygnus - Planetary nebula NGC 6826 is located about 2000 years - light from Earth in the constellation Swan. A planetary nebula is a gas shell from a small late-life star whose heart collapsed to become a white dwarf and expelled the outer layers of its matter. Image obtained by the Hubble Space Telescope on January 27, 1996. NGC 6826's eye - like appearance is marred by two sets of blood - red “” fliers”” that lie horizontally across the image. The surrounding faint green “” white”” of the eye is believed to be gas that made up almost half of the star's mass for most of its life. The hot remnant star (in the center of the green oval) drives a fast wind into older material, forming a hot interior bubble which pushes the older gas ahead of it to form a bright rim. (The star is one of the brightest stars in any planetary.) NGC 6826 is 2,200 light - years away in the constellation Cygnus. The Hubble telescope observation was taken Jan. 27, 1996 with the Wide Field and Planetary Camera

PIX4623390: Planetary nebula NGC 6826 in Swan - Planetary nebula NGC 6826 in Cygnus - Planetary nebula NGC 6826 is located about 2000 years - light from Earth in the constellation Swan. A planetary nebula is a gas shell from a small late-life star whose heart collapsed to become a white dwarf and expelled the outer layers of its matter. Image obtained by the Hubble Space Telescope on January 27, 1996. NGC 6826's eye - like appearance is marred by two sets of blood - red “” fliers”” that lie horizontally across the image. The surrounding faint green “” white”” of the eye is believed to be gas that made up almost half of the star's mass for most of its life. The hot remnant star (in the center of the green oval) drives a fast wind into older material, forming a hot interior bubble which pushes the older gas ahead of it to form a bright rim. (The star is one of the brightest stars in any planetary.) NGC 6826 is 2,200 light - years away in the constellation Cygnus. The Hubble telescope observation was taken Jan. 27, 1996 with the Wide Field and Planetary Camera / Bridgeman Images

ID: PIX4623390

Planetary nebula NGC 6826 in Swan - Planetary nebula NGC 6826 in Cygnus - Planetary nebula NGC 6826 is located about 2000 years - light from Earth in the constellation Swan. A planetary nebula is a gas shell from a small late-life star whose heart collapsed to become a white dwarf and expelled the outer layers of its matter. Image obtained by the Hubble Space Telescope on January 27, 1996. NGC 6826's eye - like appearance is marred by two sets of blood - red “” fliers”” that lie horizontally across the image. The surrounding faint green “” white”” of the eye is believed to be gas that made up almost half of the star's mass for most of its life. The hot remnant star (in the center of the green oval) drives a fast wind into older material, forming a hot interior bubble which pushes the older gas ahead of it to form a bright rim. (The star is one of the brightest stars in any planetary.) NGC 6826 is 2,200 light - years away in the constellation Cygnus. The Hubble telescope observation was

Knights in armour on horseback at a medieval tournament. Handcoloured copperplate engraving by Verico from Giulio Ferrario's Ancient and Modern Costumes of all the Peoples of the World, 1844.
Knights in armour on horseback at a medieval tournament. Handcoloured copperplate engraving by Verico from Giulio Ferrario's Ancient and Modern Costumes of all the Peoples of the World, 1844.

FLO4623493: Knights in armour on horseback at a medieval tournament. Handcoloured copperplate engraving by Verico from Giulio Ferrario's Ancient and Modern Costumes of all the Peoples of the World, 1844. / Bridgeman Images

ID: FLO4623493

Knights in armour on horseback at a medieval tournament. Handcoloured copperplate engraving by Verico from Giulio Ferrario's Ancient and Modern Costumes of all the Peoples of the World, 1844.

King and knights in armour on horseback at a medieval tournament. Handcoloured copperplate engraving by Verico after A. Monticelli from Giulio Ferrario's Ancient and Modern Costumes of all the Peoples of the World, 1844.
King and knights in armour on horseback at a medieval tournament. Handcoloured copperplate engraving by Verico after A. Monticelli from Giulio Ferrario's Ancient and Modern Costumes of all the Peoples of the World, 1844.

FLO4623504: King and knights in armour on horseback at a medieval tournament. Handcoloured copperplate engraving by Verico after A. Monticelli from Giulio Ferrario's Ancient and Modern Costumes of all the Peoples of the World, 1844. / Bridgeman Images

ID: FLO4623504

King and knights in armour on horseback at a medieval tournament. Handcoloured copperplate engraving by Verico after A. Monticelli from Giulio Ferrario's Ancient and Modern Costumes of all the Peoples of the World, 1844.

Paladins, warriors of Charlemagne's court, saying their last goodbyes to their bridesmaids in the gallery of the Palace of Bourgtheroude, Normandy. Handcoloured copperplate engraving by Verico after Alessandro Sanquirico from Giulio Ferrario's Ancient and Modern Costumes of all the Peoples of the World, 1844.
Paladins, warriors of Charlemagne's court, saying their last goodbyes to their bridesmaids in the gallery of the Palace of Bourgtheroude, Normandy. Handcoloured copperplate engraving by Verico after Alessandro Sanquirico from Giulio Ferrario's Ancient and Modern Costumes of all the Peoples of the World, 1844.

FLO4623514: Paladins, warriors of Charlemagne's court, saying their last goodbyes to their bridesmaids in the gallery of the Palace of Bourgtheroude, Normandy. Handcoloured copperplate engraving by Verico after Alessandro Sanquirico from Giulio Ferrario's Ancient and Modern Costumes of all the Peoples of the World, 1844. / Bridgeman Images

ID: FLO4623514

Paladins, warriors of Charlemagne's court, saying their last goodbyes to their bridesmaids in the gallery of the Palace of Bourgtheroude, Normandy. Handcoloured copperplate engraving by Verico after Alessandro Sanquirico from Giulio Ferrario's Ancient and Modern Costumes of all the Peoples of the World, 1844.

Planetary nebula NGC 7008 in the Cygn
Planetary nebula NGC 7008 in the Cygn

PIX4623521: Planetary nebula NGC 7008 in the Cygn / Bridgeman Images

ID: PIX4623521

Planetary nebula NGC 7008 in the Cygn

Planetary nebula NGC 7008 in Swan - Planetary nebula NGC 7008 in Cygnu
Planetary nebula NGC 7008 in Swan - Planetary nebula NGC 7008 in Cygnu

PIX4623544: Planetary nebula NGC 7008 in Swan - Planetary nebula NGC 7008 in Cygnu / Bridgeman Images

ID: PIX4623544

Planetary nebula NGC 7008 in Swan - Planetary nebula NGC 7008 in Cygnu

Planetary nebula NGC 7027 in the Swan/HST - This NASA Hubble Space Telescope image of planetary nebula NGC 7027 shows remarkable new details of the process by which a star like the Sun dies. New features include: faint, blue, concentric shells surrounding the nebula; an extensive network of red dust clouds throughout the bright inner region; and the hot central white dwarf, visible as a white dot at the center. The nebula is a record of the star's final death throes. Initially the ejection of the star's outer layers, when it was at its red giant stage of evolution, occurred at a low rate and was spherical. The Hubble photo reveals that the initial ejections occurred episodically to produce the concentric shells. This culminated in a vigorous ejection of all of the remaining outer layers, which produced the bright inner regions. At this later stage the ejection was non - spherical, and dense clouds of dust condensed from the ejected material. NGC 7027 is located about 3,000 light - years from Earth in the direction of the summer constellation Cygnus. When a star like the Sun nears the end of its life, it expands to more than 50 times its original diameter, becoming a red giant star. Then its outer layers are ejected into space, exposing the small, extremely hot core of the star, which cools off to become a white dwarf. Although stars like the Sun can live for up to 10 billion years before becoming a red giant and ejecting a nebula, the actual ejection process takes only a few thousand years. The NGC 7027 photograph is a composite of two Hubble images, taken in visible and infrared light, and is shown in “” pseudo - color.
Planetary nebula NGC 7027 in the Swan/HST - This NASA Hubble Space Telescope image of planetary nebula NGC 7027 shows remarkable new details of the process by which a star like the Sun dies. New features include: faint, blue, concentric shells surrounding the nebula; an extensive network of red dust clouds throughout the bright inner region; and the hot central white dwarf, visible as a white dot at the center. The nebula is a record of the star's final death throes. Initially the ejection of the star's outer layers, when it was at its red giant stage of evolution, occurred at a low rate and was spherical. The Hubble photo reveals that the initial ejections occurred episodically to produce the concentric shells. This culminated in a vigorous ejection of all of the remaining outer layers, which produced the bright inner regions. At this later stage the ejection was non - spherical, and dense clouds of dust condensed from the ejected material. NGC 7027 is located about 3,000 light - years from Earth in the direction of the summer constellation Cygnus. When a star like the Sun nears the end of its life, it expands to more than 50 times its original diameter, becoming a red giant star. Then its outer layers are ejected into space, exposing the small, extremely hot core of the star, which cools off to become a white dwarf. Although stars like the Sun can live for up to 10 billion years before becoming a red giant and ejecting a nebula, the actual ejection process takes only a few thousand years. The NGC 7027 photograph is a composite of two Hubble images, taken in visible and infrared light, and is shown in “” pseudo - color.

PIX4623552: Planetary nebula NGC 7027 in the Swan/HST - This NASA Hubble Space Telescope image of planetary nebula NGC 7027 shows remarkable new details of the process by which a star like the Sun dies. New features include: faint, blue, concentric shells surrounding the nebula; an extensive network of red dust clouds throughout the bright inner region; and the hot central white dwarf, visible as a white dot at the center. The nebula is a record of the star's final death throes. Initially the ejection of the star's outer layers, when it was at its red giant stage of evolution, occurred at a low rate and was spherical. The Hubble photo reveals that the initial ejections occurred episodically to produce the concentric shells. This culminated in a vigorous ejection of all of the remaining outer layers, which produced the bright inner regions. At this later stage the ejection was non - spherical, and dense clouds of dust condensed from the ejected material. NGC 7027 is located about 3,000 light - years from Earth in the direction of the summer constellation Cygnus. When a star like the Sun nears the end of its life, it expands to more than 50 times its original diameter, becoming a red giant star. Then its outer layers are ejected into space, exposing the small, extremely hot core of the star, which cools off to become a white dwarf. Although stars like the Sun can live for up to 10 billion years before becoming a red giant and ejecting a nebula, the actual ejection process takes only a few thousand years. The NGC 7027 photograph is a composite of two Hubble images, taken in visible and infrared light, and is shown in “” pseudo - color. / Bridgeman Images

ID: PIX4623552

Planetary nebula NGC 7027 in the Swan/HST - This NASA Hubble Space Telescope image of planetary nebula NGC 7027 shows remarkable new details of the process by which a star like the Sun dies. New features include: faint, blue, concentric shells surrounding the nebula; an extensive network of red dust clouds throughout the bright inner region; and the hot central white dwarf, visible as a white dot at the center. The nebula is a record of the star's final death throes. Initially the ejection of the star's outer layers, when it was at its red giant stage of evolution, occurred at a low rate and was spherical. The Hubble photo reveals that the initial ejections occurred episodically to produce the concentric shells. This culminated in a vigorous ejection of all of the remaining outer layers, which produced the bright inner regions. At this later stage the ejection was non - spherical, and dense clouds of dust condensed from the ejected material. NGC 7027 is located about 3,000 light - year

Mustard plant with cochineal beetles, jackfruit tree, water buffalo and orangutan. Handcoloured copperplate drawn and engraved by Andrea Bernieri after Francois Solvyns from Giulio Ferrario's Ancient and Modern Costumes of all the Peoples of the World, Florence, Italy, 1844.
Mustard plant with cochineal beetles, jackfruit tree, water buffalo and orangutan. Handcoloured copperplate drawn and engraved by Andrea Bernieri after Francois Solvyns from Giulio Ferrario's Ancient and Modern Costumes of all the Peoples of the World, Florence, Italy, 1844.

FLO4623556: Mustard plant with cochineal beetles, jackfruit tree, water buffalo and orangutan. Handcoloured copperplate drawn and engraved by Andrea Bernieri after Francois Solvyns from Giulio Ferrario's Ancient and Modern Costumes of all the Peoples of the World, Florence, Italy, 1844., Bernieri, Andrea (1792-1849) / Bridgeman Images

ID: FLO4623556

Mustard plant with cochineal beetles, jackfruit tree, water buffalo and orangutan. Handcoloured copperplate drawn and engraved by Andrea Bernieri after Francois Solvyns from Giulio Ferrario's Ancient and Modern Costumes of all the Peoples of the World, Florence, Italy, 1844.

Bernieri, Andrea (1792-1849)

Planetary nebula Helix (NGC 7293) in Aquarius - Planetary nebula Helix (NGC 7293) - This nebula is located 690 years - light from Earth. Image obtained by Siding Spring's 3.9m telescope This faint object is the nearest planetary nebula to the Sun and on deep photographs has a diameter of about half a degree - - the same apparent size as the Sun in the sky. The AAT colour picture shows the brighter parts of the nebula, revealing various ionization levels within the shell of matter ejected from the central star. This picture was made without unsharp masking. Unsharp masking emphasises the smallest of the radial blobs inside the red shell, which are about 150 astronomical units across (150 times the Earth - Sun distance). These radial streaks give this beautiful object its alternative name, the Sunflower Nebula. The Helix is about 400 light years away, or about 100 times more distant than the nearest stars
Planetary nebula Helix (NGC 7293) in Aquarius - Planetary nebula Helix (NGC 7293) - This nebula is located 690 years - light from Earth. Image obtained by Siding Spring's 3.9m telescope This faint object is the nearest planetary nebula to the Sun and on deep photographs has a diameter of about half a degree - - the same apparent size as the Sun in the sky. The AAT colour picture shows the brighter parts of the nebula, revealing various ionization levels within the shell of matter ejected from the central star. This picture was made without unsharp masking. Unsharp masking emphasises the smallest of the radial blobs inside the red shell, which are about 150 astronomical units across (150 times the Earth - Sun distance). These radial streaks give this beautiful object its alternative name, the Sunflower Nebula. The Helix is about 400 light years away, or about 100 times more distant than the nearest stars

PIX4623608: Planetary nebula Helix (NGC 7293) in Aquarius - Planetary nebula Helix (NGC 7293) - This nebula is located 690 years - light from Earth. Image obtained by Siding Spring's 3.9m telescope This faint object is the nearest planetary nebula to the Sun and on deep photographs has a diameter of about half a degree - - the same apparent size as the Sun in the sky. The AAT colour picture shows the brighter parts of the nebula, revealing various ionization levels within the shell of matter ejected from the central star. This picture was made without unsharp masking. Unsharp masking emphasises the smallest of the radial blobs inside the red shell, which are about 150 astronomical units across (150 times the Earth - Sun distance). These radial streaks give this beautiful object its alternative name, the Sunflower Nebula. The Helix is about 400 light years away, or about 100 times more distant than the nearest stars / Bridgeman Images

ID: PIX4623608

Planetary nebula Helix (NGC 7293) in Aquarius - Planetary nebula Helix (NGC 7293) - This nebula is located 690 years - light from Earth. Image obtained by Siding Spring's 3.9m telescope This faint object is the nearest planetary nebula to the Sun and on deep photographs has a diameter of about half a degree - - the same apparent size as the Sun in the sky. The AAT colour picture shows the brighter parts of the nebula, revealing various ionization levels within the shell of matter ejected from the central star. This picture was made without unsharp masking. Unsharp masking emphasises the smallest of the radial blobs inside the red shell, which are about 150 astronomical units across (150 times the Earth - Sun distance). These radial streaks give this beautiful object its alternative name, the Sunflower Nebula. The Helix is about 400 light years away, or about 100 times more distant than the nearest stars

Planetary nebula Helix (NGC 7293) in Aquarius - Planetary nebula Helix (NGC 7293) - The planetary nebula of Helice, located in Aquarius, is one of the closest to Earth (about 690 years - light) and is also one of the most extended; its apparent diameter is about half of the full moon. Image made with the 1.5m Danish telescope of La Silla in Chile in 2009. Helix is our closest planetary nebula at about 690 light years distance. Image taken with the ESO/Danish 1.5m telescope at La Silla observatory in Chile
Planetary nebula Helix (NGC 7293) in Aquarius - Planetary nebula Helix (NGC 7293) - The planetary nebula of Helice, located in Aquarius, is one of the closest to Earth (about 690 years - light) and is also one of the most extended; its apparent diameter is about half of the full moon. Image made with the 1.5m Danish telescope of La Silla in Chile in 2009. Helix is our closest planetary nebula at about 690 light years distance. Image taken with the ESO/Danish 1.5m telescope at La Silla observatory in Chile

PIX4623669: Planetary nebula Helix (NGC 7293) in Aquarius - Planetary nebula Helix (NGC 7293) - The planetary nebula of Helice, located in Aquarius, is one of the closest to Earth (about 690 years - light) and is also one of the most extended; its apparent diameter is about half of the full moon. Image made with the 1.5m Danish telescope of La Silla in Chile in 2009. Helix is our closest planetary nebula at about 690 light years distance. Image taken with the ESO/Danish 1.5m telescope at La Silla observatory in Chile / Bridgeman Images

ID: PIX4623669

Planetary nebula Helix (NGC 7293) in Aquarius - Planetary nebula Helix (NGC 7293) - The planetary nebula of Helice, located in Aquarius, is one of the closest to Earth (about 690 years - light) and is also one of the most extended; its apparent diameter is about half of the full moon. Image made with the 1.5m Danish telescope of La Silla in Chile in 2009. Helix is our closest planetary nebula at about 690 light years distance. Image taken with the ESO/Danish 1.5m telescope at La Silla observatory in Chile

Planetary nebula IC 418 dans le Lievre/HST - IC 418: The “” Spirograph” Nebula Glowing like a multi - faceted jewel, the planetary nebula IC 418 lies about 2,000 light - years from Earth in the direction of the constellation Lepus. This photograph is from Nasa's Hubble Space Telescope, obtained with the Wide Field Planetary Camera 2. A planetary nebula represents the final stage in the evolution of a star similar to our Sun. The star at the center of IC 418 was a red giant a few thousand years ago, but then ejected its outer layers into space to form the nebula, which has now expanded to a diameter of about 0.1 light - year. The stellar remnant at the center is the hot core of the red giant, from which ultraviolet radiation floods out into the surrounding gas, causing it to fluoresce. Over the next several thousand years, the nebula will gradually disperse into space, and then the star will cool and fade away for billions of years as a white dwarf. Our own Sun is expected to undergo a similar fate, but fortunately this will not occur until some 5 billion years from now. The Hubble image of IC 418 is shown in a false - color representation, based on Wide Field Planetary Camera 2 exposures taken in February and September, 1999 through filters that isolate light from various chemical elements. Red shows emission from ionized nitrogen (the coolest gas in the nebula, located furthest from the hot nucleus), green shows emission from hydrogen, and blue traces the emission from ionized oxygen (the hottest gas, closest to the central star)
Planetary nebula IC 418 dans le Lievre/HST - IC 418: The “” Spirograph” Nebula Glowing like a multi - faceted jewel, the planetary nebula IC 418 lies about 2,000 light - years from Earth in the direction of the constellation Lepus. This photograph is from Nasa's Hubble Space Telescope, obtained with the Wide Field Planetary Camera 2. A planetary nebula represents the final stage in the evolution of a star similar to our Sun. The star at the center of IC 418 was a red giant a few thousand years ago, but then ejected its outer layers into space to form the nebula, which has now expanded to a diameter of about 0.1 light - year. The stellar remnant at the center is the hot core of the red giant, from which ultraviolet radiation floods out into the surrounding gas, causing it to fluoresce. Over the next several thousand years, the nebula will gradually disperse into space, and then the star will cool and fade away for billions of years as a white dwarf. Our own Sun is expected to undergo a similar fate, but fortunately this will not occur until some 5 billion years from now. The Hubble image of IC 418 is shown in a false - color representation, based on Wide Field Planetary Camera 2 exposures taken in February and September, 1999 through filters that isolate light from various chemical elements. Red shows emission from ionized nitrogen (the coolest gas in the nebula, located furthest from the hot nucleus), green shows emission from hydrogen, and blue traces the emission from ionized oxygen (the hottest gas, closest to the central star)

PIX4623677: Planetary nebula IC 418 dans le Lievre/HST - IC 418: The “” Spirograph” Nebula Glowing like a multi - faceted jewel, the planetary nebula IC 418 lies about 2,000 light - years from Earth in the direction of the constellation Lepus. This photograph is from Nasa's Hubble Space Telescope, obtained with the Wide Field Planetary Camera 2. A planetary nebula represents the final stage in the evolution of a star similar to our Sun. The star at the center of IC 418 was a red giant a few thousand years ago, but then ejected its outer layers into space to form the nebula, which has now expanded to a diameter of about 0.1 light - year. The stellar remnant at the center is the hot core of the red giant, from which ultraviolet radiation floods out into the surrounding gas, causing it to fluoresce. Over the next several thousand years, the nebula will gradually disperse into space, and then the star will cool and fade away for billions of years as a white dwarf. Our own Sun is expected to undergo a similar fate, but fortunately this will not occur until some 5 billion years from now. The Hubble image of IC 418 is shown in a false - color representation, based on Wide Field Planetary Camera 2 exposures taken in February and September, 1999 through filters that isolate light from various chemical elements. Red shows emission from ionized nitrogen (the coolest gas in the nebula, located furthest from the hot nucleus), green shows emission from hydrogen, and blue traces the emission from ionized oxygen (the hottest gas, closest to the central star) / Bridgeman Images

ID: PIX4623677

Planetary nebula IC 418 dans le Lievre/HST - IC 418: The “” Spirograph” Nebula Glowing like a multi - faceted jewel, the planetary nebula IC 418 lies about 2,000 light - years from Earth in the direction of the constellation Lepus. This photograph is from Nasa's Hubble Space Telescope, obtained with the Wide Field Planetary Camera 2. A planetary nebula represents the final stage in the evolution of a star similar to our Sun. The star at the center of IC 418 was a red giant a few thousand years ago, but then ejected its outer layers into space to form the nebula, which has now expanded to a diameter of about 0.1 light - year. The stellar remnant at the center is the hot core of the red giant, from which ultraviolet radiation floods out into the surrounding gas, causing it to fluoresce. Over the next several thousand years, the nebula will gradually disperse into space, and then the star will cool and fade away for billions of years as a white dwarf. Our own Sun is expected to undergo a

Hindu gods including Trimurti, Shiva, Vishnu and Brahma. Handcoloured copperplate drawn and engraved by Andrea Bernieri from Giulio Ferrario's Ancient and Modern Costumes of all the Peoples of the World, Florence, Italy, 1844.
Hindu gods including Trimurti, Shiva, Vishnu and Brahma. Handcoloured copperplate drawn and engraved by Andrea Bernieri from Giulio Ferrario's Ancient and Modern Costumes of all the Peoples of the World, Florence, Italy, 1844.

FLO4623689: Hindu gods including Trimurti, Shiva, Vishnu and Brahma. Handcoloured copperplate drawn and engraved by Andrea Bernieri from Giulio Ferrario's Ancient and Modern Costumes of all the Peoples of the World, Florence, Italy, 1844. / Bridgeman Images

ID: FLO4623689

Hindu gods including Trimurti, Shiva, Vishnu and Brahma. Handcoloured copperplate drawn and engraved by Andrea Bernieri from Giulio Ferrario's Ancient and Modern Costumes of all the Peoples of the World, Florence, Italy, 1844.

South-east view of the Kailasa temple, Ellora rock cut temple caves, India. Handcoloured copperplate drawn and engraved by Andrea Bernieri from Giulio Ferrario's Ancient and Modern Costumes of all the Peoples of the World, Florence, Italy, 1844.
South-east view of the Kailasa temple, Ellora rock cut temple caves, India. Handcoloured copperplate drawn and engraved by Andrea Bernieri from Giulio Ferrario's Ancient and Modern Costumes of all the Peoples of the World, Florence, Italy, 1844.

FLO4623819: South-east view of the Kailasa temple, Ellora rock cut temple caves, India. Handcoloured copperplate drawn and engraved by Andrea Bernieri from Giulio Ferrario's Ancient and Modern Costumes of all the Peoples of the World, Florence, Italy, 1844. / Bridgeman Images

ID: FLO4623819

South-east view of the Kailasa temple, Ellora rock cut temple caves, India. Handcoloured copperplate drawn and engraved by Andrea Bernieri from Giulio Ferrario's Ancient and Modern Costumes of all the Peoples of the World, Florence, Italy, 1844.

Planetary Nebula Abell 24 in Little Chie
Planetary Nebula Abell 24 in Little Chie

PIX4623825: Planetary Nebula Abell 24 in Little Chie / Bridgeman Images

ID: PIX4623825

Planetary Nebula Abell 24 in Little Chie

Pagoda of Brihadeeswarar Temple or Peruvudaiyar Kovil, Thanjavur, India. Handcoloured copperplate drawn and engraved by Andrea Bernieri from Giulio Ferrario's Ancient and Modern Costumes of all the Peoples of the World, Florence, Italy, 1844.
Pagoda of Brihadeeswarar Temple or Peruvudaiyar Kovil, Thanjavur, India. Handcoloured copperplate drawn and engraved by Andrea Bernieri from Giulio Ferrario's Ancient and Modern Costumes of all the Peoples of the World, Florence, Italy, 1844.

FLO4623830: Pagoda of Brihadeeswarar Temple or Peruvudaiyar Kovil, Thanjavur, India. Handcoloured copperplate drawn and engraved by Andrea Bernieri from Giulio Ferrario's Ancient and Modern Costumes of all the Peoples of the World, Florence, Italy, 1844. / Bridgeman Images

ID: FLO4623830

Pagoda of Brihadeeswarar Temple or Peruvudaiyar Kovil, Thanjavur, India. Handcoloured copperplate drawn and engraved by Andrea Bernieri from Giulio Ferrario's Ancient and Modern Costumes of all the Peoples of the World, Florence, Italy, 1844.

Interior of the Thirumalai Nayak Palace, ancient residence of Raja Raja Thirumalai sowri at Madurai, India. Handcoloured copperplate drawn and engraved by Andrea Bernieri from Giulio Ferrario's Ancient and Modern Costumes of all the Peoples of the World, Florence, Italy, 1844.
Interior of the Thirumalai Nayak Palace, ancient residence of Raja Raja Thirumalai sowri at Madurai, India. Handcoloured copperplate drawn and engraved by Andrea Bernieri from Giulio Ferrario's Ancient and Modern Costumes of all the Peoples of the World, Florence, Italy, 1844.

FLO4623835: Interior of the Thirumalai Nayak Palace, ancient residence of Raja Raja Thirumalai sowri at Madurai, India. Handcoloured copperplate drawn and engraved by Andrea Bernieri from Giulio Ferrario's Ancient and Modern Costumes of all the Peoples of the World, Florence, Italy, 1844. / Bridgeman Images

ID: FLO4623835

Interior of the Thirumalai Nayak Palace, ancient residence of Raja Raja Thirumalai sowri at Madurai, India. Handcoloured copperplate drawn and engraved by Andrea Bernieri from Giulio Ferrario's Ancient and Modern Costumes of all the Peoples of the World, Florence, Italy, 1844.

Entrance to the Kailasa temple, Ellora rock cut temple caves, India. Handcoloured copperplate drawn and engraved by Andrea Bernieri from Giulio Ferrario's Ancient and Modern Costumes of all the Peoples of the World, Florence, Italy, 1844.
Entrance to the Kailasa temple, Ellora rock cut temple caves, India. Handcoloured copperplate drawn and engraved by Andrea Bernieri from Giulio Ferrario's Ancient and Modern Costumes of all the Peoples of the World, Florence, Italy, 1844.

FLO4623846: Entrance to the Kailasa temple, Ellora rock cut temple caves, India. Handcoloured copperplate drawn and engraved by Andrea Bernieri from Giulio Ferrario's Ancient and Modern Costumes of all the Peoples of the World, Florence, Italy, 1844. / Bridgeman Images

ID: FLO4623846

Entrance to the Kailasa temple, Ellora rock cut temple caves, India. Handcoloured copperplate drawn and engraved by Andrea Bernieri from Giulio Ferrario's Ancient and Modern Costumes of all the Peoples of the World, Florence, Italy, 1844.

Planetary Nebula Abell 36 in the Virgin
Planetary Nebula Abell 36 in the Virgin

PIX4623852: Planetary Nebula Abell 36 in the Virgin / Bridgeman Images

ID: PIX4623852

Planetary Nebula Abell 36 in the Virgin

Carved pillars in the Thirumalai Nayak Palace, ancient residence of Raja Raja Thirumalai sowri at Madurai, India. Copperplate drawn and engraved by Andrea Bernieri from Giulio Ferrario's Ancient and Modern Costumes of all the Peoples of the World, Florence, Italy, 1844.
Carved pillars in the Thirumalai Nayak Palace, ancient residence of Raja Raja Thirumalai sowri at Madurai, India. Copperplate drawn and engraved by Andrea Bernieri from Giulio Ferrario's Ancient and Modern Costumes of all the Peoples of the World, Florence, Italy, 1844.

FLO4623862: Carved pillars in the Thirumalai Nayak Palace, ancient residence of Raja Raja Thirumalai sowri at Madurai, India. Copperplate drawn and engraved by Andrea Bernieri from Giulio Ferrario's Ancient and Modern Costumes of all the Peoples of the World, Florence, Italy, 1844. / Bridgeman Images

ID: FLO4623862

Carved pillars in the Thirumalai Nayak Palace, ancient residence of Raja Raja Thirumalai sowri at Madurai, India. Copperplate drawn and engraved by Andrea Bernieri from Giulio Ferrario's Ancient and Modern Costumes of all the Peoples of the World, Florence, Italy, 1844.

Tomb of Hyder Ali Khan, Sultan of Mysore, India. Handcoloured copperplate drawn and engraved by Andrea Bernieri from Giulio Ferrario's Ancient and Modern Costumes of all the Peoples of the World, Florence, Italy, 1844.
Tomb of Hyder Ali Khan, Sultan of Mysore, India. Handcoloured copperplate drawn and engraved by Andrea Bernieri from Giulio Ferrario's Ancient and Modern Costumes of all the Peoples of the World, Florence, Italy, 1844.

FLO4623877: Tomb of Hyder Ali Khan, Sultan of Mysore, India. Handcoloured copperplate drawn and engraved by Andrea Bernieri from Giulio Ferrario's Ancient and Modern Costumes of all the Peoples of the World, Florence, Italy, 1844. / Bridgeman Images

ID: FLO4623877

Tomb of Hyder Ali Khan, Sultan of Mysore, India. Handcoloured copperplate drawn and engraved by Andrea Bernieri from Giulio Ferrario's Ancient and Modern Costumes of all the Peoples of the World, Florence, Italy, 1844.

Planetary nebula PK164+31.1 in Lyn
Planetary nebula PK164+31.1 in Lyn

PIX4623891: Planetary nebula PK164+31.1 in Lyn / Bridgeman Images

ID: PIX4623891

Planetary nebula PK164+31.1 in Lyn

Indian musicians with musical instruments. Man playing bell and conch shell, sankh and ghanta, bansi flutist, surmandal player, dholak drummer, kartal cymbalist, dhak drummer, and jagajhampa drummer. Handcoloured copperplate drawn and engraved by Andrea Bernieri after Francois Solvyns from Giulio Ferrario's Ancient and Modern Costumes of all the Peoples of the World, Florence, Italy, 1844.
Indian musicians with musical instruments. Man playing bell and conch shell, sankh and ghanta, bansi flutist, surmandal player, dholak drummer, kartal cymbalist, dhak drummer, and jagajhampa drummer. Handcoloured copperplate drawn and engraved by Andrea Bernieri after Francois Solvyns from Giulio Ferrario's Ancient and Modern Costumes of all the Peoples of the World, Florence, Italy, 1844.

FLO4623901: Indian musicians with musical instruments. Man playing bell and conch shell, sankh and ghanta, bansi flutist, surmandal player, dholak drummer, kartal cymbalist, dhak drummer, and jagajhampa drummer. Handcoloured copperplate drawn and engraved by Andrea Bernieri after Francois Solvyns from Giulio Ferrario's Ancient and Modern Costumes of all the Peoples of the World, Florence, Italy, 1844., Bernieri, Andrea (1792-1849) / Bridgeman Images

ID: FLO4623901

Indian musicians with musical instruments. Man playing bell and conch shell, sankh and ghanta, bansi flutist, surmandal player, dholak drummer, kartal cymbalist, dhak drummer, and jagajhampa drummer. Handcoloured copperplate drawn and engraved by Andrea Bernieri after Francois Solvyns from Giulio Ferrario's Ancient and Modern Costumes of all the Peoples of the World, Florence, Italy, 1844.

Bernieri, Andrea (1792-1849)

Planetary nebula PK164+31.1 in Lynx - Planetary nebula PKS164+31.1 in Lyn
Planetary nebula PK164+31.1 in Lynx - Planetary nebula PKS164+31.1 in Lyn

PIX4623905: Planetary nebula PK164+31.1 in Lynx - Planetary nebula PKS164+31.1 in Lyn / Bridgeman Images

ID: PIX4623905

Planetary nebula PK164+31.1 in Lynx - Planetary nebula PKS164+31.1 in Lyn

Nautch or Ramjani girls dancing to music from kuplyans or bin, dhol drums, tabla, and other string and percussion instruments. Handcoloured copperplate drawn and engraved by Andrea Bernieri after Francois Solvyns from Giulio Ferrario's Ancient and Modern Costumes of all the Peoples of the World, Florence, Italy, 1844.
Nautch or Ramjani girls dancing to music from kuplyans or bin, dhol drums, tabla, and other string and percussion instruments. Handcoloured copperplate drawn and engraved by Andrea Bernieri after Francois Solvyns from Giulio Ferrario's Ancient and Modern Costumes of all the Peoples of the World, Florence, Italy, 1844.

FLO4623910: Nautch or Ramjani girls dancing to music from kuplyans or bin, dhol drums, tabla, and other string and percussion instruments. Handcoloured copperplate drawn and engraved by Andrea Bernieri after Francois Solvyns from Giulio Ferrario's Ancient and Modern Costumes of all the Peoples of the World, Florence, Italy, 1844., Bernieri, Andrea (1792-1849) / Bridgeman Images

ID: FLO4623910

Nautch or Ramjani girls dancing to music from kuplyans or bin, dhol drums, tabla, and other string and percussion instruments. Handcoloured copperplate drawn and engraved by Andrea Bernieri after Francois Solvyns from Giulio Ferrario's Ancient and Modern Costumes of all the Peoples of the World, Florence, Italy, 1844.

Bernieri, Andrea (1792-1849)

Planetary nebula ESO 166 - 21 dans les Voiles - The faint planetary nebula ESO 166 - 21 - This planetary nebula was discovered in the rich southern constellation of Vela in 1966, which is why it does not have an NGC number. The 'Ack' designation refers to its identification in the catalogue of planetary nebulae edited by Agnes Acker. This beautifully structured delicate sphere of glowing gas is about 2 arc minutes in diameter and is extremely faint. Both these characteristics have contributed to the conspicuous grain 'noise' in the photograph, and attempts to emphasise the faint nebulosity also bring out the many faint stars in this direction, including the markedly blue central star of visual magnitude 18 which is seen here sandwiched between two other, brighter stars
Planetary nebula ESO 166 - 21 dans les Voiles - The faint planetary nebula ESO 166 - 21 - This planetary nebula was discovered in the rich southern constellation of Vela in 1966, which is why it does not have an NGC number. The 'Ack' designation refers to its identification in the catalogue of planetary nebulae edited by Agnes Acker. This beautifully structured delicate sphere of glowing gas is about 2 arc minutes in diameter and is extremely faint. Both these characteristics have contributed to the conspicuous grain 'noise' in the photograph, and attempts to emphasise the faint nebulosity also bring out the many faint stars in this direction, including the markedly blue central star of visual magnitude 18 which is seen here sandwiched between two other, brighter stars

PIX4623916: Planetary nebula ESO 166 - 21 dans les Voiles - The faint planetary nebula ESO 166 - 21 - This planetary nebula was discovered in the rich southern constellation of Vela in 1966, which is why it does not have an NGC number. The 'Ack' designation refers to its identification in the catalogue of planetary nebulae edited by Agnes Acker. This beautifully structured delicate sphere of glowing gas is about 2 arc minutes in diameter and is extremely faint. Both these characteristics have contributed to the conspicuous grain 'noise' in the photograph, and attempts to emphasise the faint nebulosity also bring out the many faint stars in this direction, including the markedly blue central star of visual magnitude 18 which is seen here sandwiched between two other, brighter stars / Bridgeman Images

ID: PIX4623916

Planetary nebula ESO 166 - 21 dans les Voiles - The faint planetary nebula ESO 166 - 21 - This planetary nebula was discovered in the rich southern constellation of Vela in 1966, which is why it does not have an NGC number. The 'Ack' designation refers to its identification in the catalogue of planetary nebulae edited by Agnes Acker. This beautifully structured delicate sphere of glowing gas is about 2 arc minutes in diameter and is extremely faint. Both these characteristics have contributed to the conspicuous grain 'noise' in the photograph, and attempts to emphasise the faint nebulosity also bring out the many faint stars in this direction, including the markedly blue central star of visual magnitude 18 which is seen here sandwiched between two other, brighter stars

Cocon Nebula (IC 5146) in the Cygn
Cocon Nebula (IC 5146) in the Cygn

PIX4622732: Cocon Nebula (IC 5146) in the Cygn / Bridgeman Images

ID: PIX4622732

Cocon Nebula (IC 5146) in the Cygn


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