The Red Spider Planetary Nebula
Explanation:
Oh what a
tangled web
a
planetary nebula can weave.
The
Red Spider Planetary Nebula
shows the complex structure that can result when a
normal star ejects
its outer gases and becomes a
white dwarf star.
Officially tagged
NGC
6537, this two-lobed symmetric
planetary nebula
houses one of the
hottest white dwarfs ever observed,
probably as part of
binary star system.
Internal
winds emanating from the central stars, shown
in the central inset, have been measured in excess of
1000 kilometers per second.
These
winds expand the
nebula, flow along the nebula's walls, and cause waves of hot
gas and
dust to collide.
Atoms
caught in these colliding shocks radiate light shown in the
above representative-color picture.
The
Red Spider Nebula lies toward the
constellation of
Sagittarius.
It's distance is not well known but
estimated by some to be about 4000
light-years.
Authors & editors:
Robert Nemiroff
(MTU) &
Jerry Bonnell
(USRA)
NASA Web Site Statements, Warnings,
and Disclaimers
NASA Official: Jay Norris.
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rights apply.
A service of:
LHEA at
NASA /
GSFC
& Michigan Tech. U.
