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'Cat's Eye' immagini e video risultati page 1 of 1

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Immagini di 'Cat's Eye' trovate, 34

Cat's Eye (chrysoberyl)
Cat's Eye by LewisTeague with Drew Barrymore, 1984 (d'apres StephenKing, after StephenKing) (photo)
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The Cat's Eye Nebula, 1994
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Cat's Eye by Lewis Teague, 1985
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Weeping Cat's Eye, 2020 (digital photograph)
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Chrysoberyl (photo)
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Pendant, two rings and pair of studs in cat's eye chrysoberyl
Close up on a cat's head with orange eyes.
Close-up on yellow-eyed cat's head.
Watching (acrylic on canvas)
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Chrysoberyl cat's eye in the rough (part polished), from Edwin Streeter's "Precious Stones and Gems," London, George Bell & Sons, 1892 (chromolitho)
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Cat's eyes - tiger, 2012 (acrylic on board)
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Cat's eyes - snow leopard, 2012 (acrylic on board)
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Bus to Kehlsteinhaus (Eagle's Nest), 1960 (b/w photo)
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Gem scarf pins with diamond, ruby, sapphire, pearl, and cat's eye. Chromolithograph from Edwin Street's Gems Catalog, Bond Street, London, circa 1895.
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Chrysoberyl cat's eye raw (partly polished)). Chromolithography, in Precious Stones and Gems by Edwin Streeter, published in London, England, by George Bell and Sons, 1892.
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Bus to Kehlsteinhaus (Eagle's Nest), 1960 (b/w photo)
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The false eye, 2025 (oil on canvas)
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Planetary nebula NGC 6543 in the Dragon - Planetary nebula NGC 6543 in Draco - Composite view of the planetary nebula NGC 6543 in the Dragon obtained by the Hubble space telescope and X-ray (blue) by the Chandra satellite. NGC 6543 is located about 3000 years of light from Earth. This composite of data from Nasa's Chandra X - ray Observatory and Hubble Space Telescope is a new look for NGC 6543, better known as the Cat's Eye nebula. This famous object is a so - called planetary nebula that represents a phase of stellar evolution that the Sun should experience several billion years from now. When a star like the Sun begins to run out of fuel, it becomes what is known as a red giant. In this phase, a star sheds some of its outer layers, eventually leaving behind a hot core that collapses to form a dense white dwarf star. A fast wind emanating from the hot core rams into the ejected atmosphere, pushes it outward, and creates the graceful filamentary structures seen with optical telescopes. Chandra's X - ray data (colored in blue) of NGC 6543 shows that its central star is surrounded by a cloud of multi - million - degree gas. By comparing where the X - rays lie in relation to the structures seen in optical light by Hubble (red and purple), astronomers were able to deduce that the chemical abundances in the region of hot gas were like those in the wind from the central star and different from the outer cooler material. In the case of the Cat's Eye, material shed by the star is flying away at a speed of about 4 million miles per hour. The star itself is expected to collapse to become a white dwarf star in a few million years
Planetary nebula NGC 6543 dans le Dragon/HST - The nebula, formally cataloged NGC 6543 was one of the first planetary nebulae to be discovered; it is one of the most complex such nebulae seen in space. A planetary nebula forms when Sun - like stars gently eject their outer gaseous layers that form bright nebulae with amazing and confounding shapes. In 1994, Hubble first revealed NGC 6543's surprisingly intricate structures, including concentric gas shells, jets of high - speed gas, and unusual shock - induced knots of gas. As if the Cat's Eye itself isn't spectacular enough, this new image taken with Hubble's Advanced Camera for Surveys (ACS) reveals the full beauty of a bull's eye pattern of eleven or even more concentric rings, or shells, around the Cat's Eye. Each 'ring' is actually the edge of a spherical bubble seen projected onto the sky - - that's why it appears bright along its outer edge. Observations suggest the star ejected its mass in a series of pulses at 1,500 - year intervals. These convulsions created dust shells, each of which contain as much mass as all of the planets in our solar system combined (still only one percent of the Sun's mass). These concentric shells make a layered, onion - skin structure around the dying star. The view from Hubble is like seeing an onion cut in half, where each skin layer is discernible. Until recently, it was thought that such shells around planetary nebulae were a rare phenomenon. However, Romano Corradi (Isaac Newton Group of Telescopes, Spain) and collaborators, in a paper published in the European journal Astronomy and Astrophysics in April 2004, have instead shown that the formation of these rings is likely to be the rule rather than the exception. The bull's - eye patterns seen around planetary nebulae come as a surprise to astronomers because they had no expectation that episodes of mass loss at the end of stellar lives would repeat every 1,500 years. Several explanations have been proposed, including cy
German infra-red equipment by G. H. Davis, 1946 (print)
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Indonesian geologist Mahardi Paramita checks the radioactive levels of a gemstone set in a gold ring.., 1997-11-14 (photo)
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Indonesian gemologist Mahardi Paramita holds up three rings set with gemstones at his office in Jak.., 1997-11-14 (photo)
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The constellation Draco, 1603
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Planetary nebula NGC 6543 in the Dragon/HST - This NASA Hubble Space Telescope image shows one of the most complex planetary nebulae ever seen, NGC 6543, nicknamed the “Cat's Eye Nebula.””” Hubble reveals surprisingly intricate structures including concentric gas shells, jets of high - speed gas and unusual shock - induced knots of gas. Estimated to be 1,000 years old, the nebula is a visual “” fossil record”” of the dynamics and late evolution of a dying star. A preliminary interpretation suggests that the star might be a double - star system. The dynamical effects of two stars orbiting one another most easily explains the intricate structures, which are much more complicated than features seen in most planetary nebulae. (The two stars are too close together to be individually resolved by Hubble, and instead, appear as a single point of light at the center of the nebula.) According to this model, a fast “” stellar wind””” of gas blown off the central star created the elongated shell of dense, glowing gas. This structure is embedded inside two larger lobes of gas blown off the star at an earlier phase. These lobes are “” pinched”” by a ring of denser gas, presumably ejected along the orbital plane of the binary companion. The suspected companion star also might be responsible for a pair of high - speed jets of gas that lie at right angles to this equatorial ring. If the companion were pulling in material from a neighboring star, jets escaping along the company's rotation axis could be produced. These jets would explain several puzzling features along the periphery of the gas lobes. Like a stream of water hitting a sand pile, the jets compress gas ahead of them, creating the “” curlicue”” features and bright arcs near the outer edge of the lobes. The twin jets are now pointing in different directions than these features. This suggests the jets are wobbling, or precessing, and turning on and off episodically. This color picture, taken with the Wide Field Planetary Camera - 2
Iridis, 2016 (digital photo)
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Blue eye of Cat (Felis sylvestris catus), side close up
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