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Anaea tyrianthina.

Anaea tyrianthina.

NHM1457325

Arhopala hercules

Arhopala hercules

NHM1457322

Arhopala hercules

Arhopala hercules

NHM1457323

Zerene eurydice

Zerene eurydice

NHM1457326

Euphaedra zampa

Euphaedra zampa

NHM1457328

Graphium agamemnon

Graphium agamemnon

NHM1457317

Teinopalpus imperialis

Teinopalpus imperialis

NHM1457324

Cyrestis thyodamas

Cyrestis thyodamas

NHM1457318

Graphium weiskei

Graphium weiskei

NHM1457319

Cymothoe sangaris

Cymothoe sangaris

NHM1457327

Graphium weiskei

Graphium weiskei

NHM1457320

Water Belt Butterfly and Reed Cutter Butterfly from St. Domingo (print)

Water Belt Butterfly and Reed Cutter Butterfly from St. Domingo (print)

PRX11860458

Runner, Guatemala, Sacatepequez, 2005 (cotton & dye)

Runner, Guatemala, Sacatepequez, 2005 (cotton & dye)

Guatemalan School, (20th century)

LWE410791

Wallflower with blue butterfly (watercolour on vellum), 1710-1705

Wallflower with blue butterfly (watercolour on vellum), 1710-1705

Merian, Maria Sibylla Graff (1647-1717)

ROC11992674

The Garden of Unearthly Delights, 2009 (Steel, aluminium, plaster, resin, LED lights, motor)

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The Garden of Unearthly Delights, 2009 (Steel, aluminium, plaster, resin, LED lights, motor)

Collishaw, Mat (b.1966)

MCW7316053

The Garden of Unearthly Delights, 2009 (Steel, aluminium, plaster, resin, LED lights, motor)

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The Garden of Unearthly Delights, 2009 (Steel, aluminium, plaster, resin, LED lights, motor)

Collishaw, Mat (b.1966)

MCW7316056

The Garden of Unearthly Delights, 2009 (Steel, aluminium, plaster, resin, LED lights, motor)

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The Garden of Unearthly Delights, 2009 (Steel, aluminium, plaster, resin, LED lights, motor)

Collishaw, Mat (b.1966)

MCW7316057

The Garden of Unearthly Delights, 2009 (Steel, aluminium, plaster, resin, LED lights, motor)

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The Garden of Unearthly Delights, 2009 (Steel, aluminium, plaster, resin, LED lights, motor)

Collishaw, Mat (b.1966)

MCW7316055

The Garden of Unearthly Delights, 2009 (Steel, aluminium, plaster, resin, LED lights, motor)

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The Garden of Unearthly Delights, 2009 (Steel, aluminium, plaster, resin, LED lights, motor)

Collishaw, Mat (b.1966)

MCW7316054

Planetary nebula NGC 6302 in Scorpio - Planetary nebula NGC 6302 in Scorpius - NGC 6302 is a planetary nebula located about 4000 years from Earth. In the center of the nebula, an extremely hot dying star. Image obtained by the Hubble Space Telescope with the new WFC 3 (Wide Field Camera 3) camera, July 27, 2009. A dying star that was once about five times the mass of the Sun is at the center of this nebula. It has ejected its envelope of gases and is now unleashing a stream of ultraviolet radiation that is making the cast - off material glow. This object is an example of a planetary nebula, so - named because many of them have a round appearance resembling that of a planet when viewed through a small telescope. The Wide Field Camera 3 (WFC3), a new camera aboard Nasa's Hubble Space Telescope, snapped this image of the planetary nebula, catalogued as NGC 6302, but more popularly called the Bug Nebula or the Butterfly Nebula. WFC3 was installed by NASA astronauts in May 2009, during the servicing mission to upgrade and repair the 19 - year - old Hubble telescope. NGC 6302 lies within our Milky Way galaxy, roughly 3,800 light - years away in the constellation Scorpius. The glowing gas is the star's outer layers, expelled over about 2,200 years. The “” butterfly”” stretches for more than two light - years, which is about half the distance from the Sun to the nearest star, Alpha Centauri. The central star itself cannot be seen, because it is hidden within a doughnut - shaped ring of dust, which appears as a dark band pinching the nebula in the center. The thick dust belt constricts the star's outflow, creating the classic “” bipolar”” or hourglass shape displayed by some planetary nebulae. The star's surface temperature is estimated to be about 400,000 degrees Fahrenheit, making it one of the hottest known stars in our galaxy. Spectroscopic observations made with ground - based telescopes show that the gas is roughly 36,000 d — Planetary nebula NGC 6302 in Scorpio - Planetary nebula NGC 6302 in Scorpius - NGC 6302 is a planetary nebula located about 4000 years from Earth. In the center of the nebula, an extremely hot dying star. Image obtained by the Hubble Space Telescope with the new WFC 3 (Wide Field Camera 3) camera, July 27, 2009. A dying star that was once about five times the mass of the Sun is at the center of this nebula. It has ejected its envelope of gases and is now unleashing a stream of ultraviolet radiation that is making the cast - off material glow. This object is an example of a planetary nebula, so - named because many of them have a round appearance resembling that of a planet when viewed through a small telescope. The Wide Field Camera 3 (WFC3), a new camera aboard Nasa's Hubble Space Telescope, snapped this image of the planetary nebula, catalogued as NGC 6302, but more popularly called the Bug Nebula or the Butterfly Nebula. WFC3 was installed by NASA astronauts in May 2009, during the

Planetary nebula NGC 6302 in Scorpio - Planetary nebula NGC 6302 in Scorpius - NGC 6302 is a planetary nebula located about 4000 years from Earth. In the center of the nebula, an extremely hot dying star. Image obtained by the Hubble Space Telescope with the new WFC 3 (Wide Field Camera 3) camera, July 27, 2009. A dying star that was once about five times the mass of the Sun is at the center of this nebula. It has ejected its envelope of gases and is now unleashing a stream of ultraviolet radiation that is making the cast - off material glow. This object is an example of a planetary nebula, so - named because many of them have a round appearance resembling that of a planet when viewed through a small telescope. The Wide Field Camera 3 (WFC3), a new camera aboard Nasa's Hubble Space Telescope, snapped this image of the planetary nebula, catalogued as NGC 6302, but more popularly called the Bug Nebula or the Butterfly Nebula. WFC3 was installed by NASA astronauts in May 2009, during the

PIX4623200

Planetary nebula M2 - 9 in Ophiuchus/HST - M2 - 9 is a striking example of a “” butterfly”” or a bipolar planetary nebula. Another more revealing name might be the “Twin Jet Nebula.”” If the nebula is sliced across the star, each side of it appears much like a pair of exhausts from jet engines. Indeed, because of the nebula's shape and the measured velocity of the gas, in excess of 200 miles per second, astronomers believe that the description as a super - super - sonic jet exhaust is quite apt. Ground - based studies have shown that the nebula's size increases with time, suggesting that the stellar outburst that formed the lobes occurred just 1,200 years ago. The central star in M2 - 9 is known to be one of a very close pair which orbit one another at perilously close distances. It is even possible that one star is being engulfed by the other. Astronomers suspect the gravity of one star pulls weakly bound gas from the surface of the other and flings it into a thin, dense disk which surrounds both stars and extends well into space. The disk can actually be seen in shorter exposure images obtained with the Hubble telescope. It measures approximately 10 times the diameter of Pluto's orbit. Models of the type that are used to design jet engines (“hydrodynamics”) show that such a disk can successfully account for the jet - exhaust - like appearance of M2 - 9. The high - speed wind from one of the stars rams into the surrounding disk, which serves as a nozzle. The wind is deflected in a perpendicular direction and forms the pair of jets that we see in the nebula's image. This is much the same process that takes place in a jet engine: The burning and expanding gases are deflected by the engine walls through a nozzle to form long, collimated jets of hot air at high speeds. M2 - 9 is 2,100 light - years away in the constellation Ophiucus. The observation was taken Aug. 2, 1997 by the Hubble telescope's Wide Field and Planetary Camera 2. In this image, neutral oxygen is — Planetary nebula M2 - 9 in Ophiuchus/HST - M2 - 9 is a striking example of a “” butterfly”” or a bipolar planetary nebula. Another more revealing name might be the “Twin Jet Nebula.”” If the nebula is sliced across the star, each side of it appears much like a pair of exhausts from jet engines. Indeed, because of the nebula's shape and the measured velocity of the gas, in excess of 200 miles per second, astronomers believe that the description as a super - super - sonic jet exhaust is quite apt. Ground - based studies have shown that the nebula's size increases with time, suggesting that the stellar outburst that formed the lobes occurred just 1,200 years ago. The central star in M2 - 9 is known to be one of a very close pair which orbit one another at perilously close distances. It is even possible that one star is being engulfed by the other. Astronomers suspect the gravity of one star pulls weakly bound gas from the surface of the other and flings it into a thin, dense disk which su

Planetary nebula M2 - 9 in Ophiuchus/HST - M2 - 9 is a striking example of a “” butterfly”” or a bipolar planetary nebula. Another more revealing name might be the “Twin Jet Nebula.”” If the nebula is sliced across the star, each side of it appears much like a pair of exhausts from jet engines. Indeed, because of the nebula's shape and the measured velocity of the gas, in excess of 200 miles per second, astronomers believe that the description as a super - super - sonic jet exhaust is quite apt. Ground - based studies have shown that the nebula's size increases with time, suggesting that the stellar outburst that formed the lobes occurred just 1,200 years ago. The central star in M2 - 9 is known to be one of a very close pair which orbit one another at perilously close distances. It is even possible that one star is being engulfed by the other. Astronomers suspect the gravity of one star pulls weakly bound gas from the surface of the other and flings it into a thin, dense disk which su

PIX4623720

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