Hubble Watches Star Tear Apart its Neighborhood
NASA/ESA Hubble Space Telescope has snapped a view of a stellar demolition zone in our Milky Way Galaxy: a massive star, nearing the end of its life, tearing apart the shell of surrounding material it blew off 250, 000 years ago with its strong stellar wind. The shell of material, dubbed the Crescent Nebula (NGC 6888), surrounds the 'hefty', aging star WR 136, an extremely rare and short-lived class of super-hot star called a Wolf-Rayet. Hubble's multicolored picture reveals with unprecedented clarity that the shell of matter is a network of filaments and dense knots, all enshrouded in a thin 'skin' of gas [seen in blue]. The whole structure looks like oatmeal trapped inside a balloon. The skin is glowing because it is being blasted by ultraviolet light from WR 136.
Credit:About the Image
About the Object
Name: | Crescent Nebula, NGC 6888, WR 136 |
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Type: | Milky Way : Star : Type : Wolf-Rayet Milky Way : Nebula : Appearance : Emission |
Distance: | 4500 light years |
Constellation: | Cygnus |
Category: | Stars |
Coordinates
Position (RA): | 20 12 32.26 |
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Position (Dec): | 38° 27' 14.71" |
Field of view: | 2.47 x 2.51 arcminutes |
Orientation: | North is 9.9° right of vertical |
Colours & filters
Band | Wavelength | Telescope |
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Optical OIII | 502 nm |
Hubble Space Telescope
WFPC2 |
Optical H-alpha | 656 nm |
Hubble Space Telescope
WFPC2 |
Optical SII | 673 nm |
Hubble Space Telescope
WFPC2 |