Embargoed Until: 1:00 a.m. (EDT) July 13, 2000
The Hubble 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.
Credits: NASA, Brian D. Moore, Jeff Hester, Paul
Scowen (Arizona State University), Reginald Dufour (Rice University)