To celebrate the Hubble Space Telescope's 30th birthday, Gentside has prepared a collection of its greatest achievements. A csillag külső rétegeiből nagy sebességgel kiáramló hidrogén és nitrogén gáz szárnyformákat alkot a térben. New 6 cm continuum and radio recombination line VLA observations as well as CO observations are presented of the bright PN NGC 6302. With an estimated surface temperature of about 250,000 degrees C, the dying central star of this particular planetary nebula has become exceptionally hot. NGC 6302, a butterfly-shaped nebula, surrounds a dying star.


NGC 6302 Bug, nebula classification: planetary, nebula position: 17h 13m, –37° 06′ (Scorpius), distance from Earth: 3,800 ly, instrument/year: WFC3/UVIS, 2009. Explanation: The bright clusters and nebulae of planet Earth's night sky are often named for flowers or insects, and NGC 6302 … The bright clusters and nebulae of planet Earth's night sky are often named for flowers or insects. The outflowing proper motions of 15 knots in the dominant northwestern lobe of the high-excitation poly-polar planetary nebula NGC 6302 have been determined by comparing their positions relative to those of faint stars in an image taken at the San Pedro Martir Observatory in 2007 to those in a South African Astronomical Observatory archival plate obtained by Evans in 1956. NGC 6302, image: NASA, ESA and A.Zijlstra (UMIST, Manchester, UK) The dust cloud around the star has an estimated temperature of 18,000°C.

Last Update: 1 September 2019 5-Jun-2020 12:10 UT Aims:We measure the mass and kinematics of the massive molecular torus in the the proto-typical butterfly planetary nebula NGC 6302.

WFC3 was installed by NASA astronauts in May 2009, during the servicing mission to upgrade and repair the 19-year-old Hubble 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. Corradi. NGC 6302 lies within our Milky Way galaxy, roughly 3,800 light-years away in the constellation Scorpius. With an estimated surface temperature of about 250,000 degrees C, the dying central star of this particular planetary nebula has become exceptionally hot. Felfedezése.

We present the combined Infrared Space Observatory Short-Wavelength Spectrometer and Long-Wavelength Spectrometer 2.4-197 mu m spectrum of the Planetary Nebula NGC 6302 which contains in addition to strong atomic lines, a series of emission features due to solid state components.

The broad wavelength coverage enables us to more accurately identify and determine the properties of both …

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.
The glowing gas is the …

Though its wingspan covers over 3 light-years, NGC 6302 is no exception. NGC 6302: Big, Bright, Bug Nebula Credit: A. Zijlstra et al., ESA, NASA. WFC3 was installed by NASA astronauts in May 2009, during the servicing mission to upgrade and repair the 19-year-old Hubble telescope. Photo of the Butterfly Nebula. NGC 6302 (také známá jako Bug Nebula nebo Caldwell 69) je bipolární planetární mlhovina v souhvězdí Štíra.Objevil ji americký astronom Edward Emerson Barnard v roce 1880. The bright clusters and nebulae of planet Earth's night sky are often named for flowers or insects. The bright clusters and nebulae of planet Earth's night sky are often named for flowers or insects. Vnitřním uspořádáním se řadí mezi nejsložitější pozorované planetární mlhoviny. The H110-alpha line is significantly broader than the H76-alpha line, an effect which is attributed to electron pressure broadening. Lines of very highly ionized silicon recently discovered in the type I planetary nebula NGC 6302 implied a central star temperature of 450,000 K assuming that the high ionization lines were the result of photoionization.

The gas in the nebula is moving very quickly across space at over 600,000 miles (965,606 kilometres) per hour.

NGC 6302 is among the first observations made by the new Wide Field Camera 3 aboard the upgraded NASA Hubble Space Telescope. Though its wingspan covers over 3 light-years, NGC 6302 is no exception.


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