Infrared Helix
Credit:
ESA/ISO,
ISOCAM Team and P. Cox et al.
Five hundred light years from Earth, in
the constellation Aquarius,
a sun-like star is dying.
Its last few thousand years have produced
the Helix, a
well studied and nearby
example of a Planetary Nebula - typical
of this
final phase of stellar evolution.
The emission in this
Infrared Space Observatory image of the Helix nebula
comes mostly from the expanding shells of molecular hydrogen gas.
Dust, normally expected in such nebulae, should also radiate strongly
at infrared wavelengths but
mysteriously seems to be absent here.
The culprit may
may well be the Helix's central star, a contracting
white dwarf.
This small but extremely hot star radiates most of its
energy at
short Ultraviolet wavelengths and
is invisible in this infrared mage.
Astronomers suspect that over time,
this intense Ultraviolet radiation may have destroyed
the dust.
The Sun is expected to go through
its own Planetary Nebula phase ...
in another 5 billion years.