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Planetary nebula NGC 6302 in Scorpio - Planetary nebula NGC 6302 in Scorpius - NGC...
Editorial (Books, magazines and newspaper) - extended
Print and/or digital. Single use, any size, inside only. Single language only. Single territory rights for trade books; worldwide rights for academic books. Print run up to 5000. 7 years. (excludes advertising)
$175.00
Editorial (Books, magazines and newspaper) - standard
Print and/or digital. Single use, any size, inside only. Single language only. Single territory rights for trade books; worldwide rights for academic books. Print run up to 1500. 7 years. (excludes advertising)
$100.00
Corporate website, social media or presentation/talk
Web display, social media, apps or blogs.
Not for advertising. All languages. 1 year + archival rights
$190.00
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Web display, social media, apps, or blogs. Use in academic and non-commercial presentations/talks included. Not for commercial use or advertising. All languages. 5 years
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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 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
