Astronomers
of old called them
"planets"
because they
looked like planets when viewed with earth bound telescopes. Recently,
higher resolution telescopes showed them to be distant nebulae; results
of stars in their later life stages, cooling, and loosing much of their
gassy exterior. A magnetic field of the core
caused by orbiting ions restrains the jet to move only out of the
poles. These jets send particles into
that gas causing the gas to glow and to also move out with increased
velocity. There can also be an unseen companion that drags material
away from the dying
star, causing spiral/ring effects. Black holes are not necessarily
involved. Theories as to the true nature of these strangely shaped
nebulae are still being developed.
Ultraviolet images in 1978 showed that dying stars
continue to blow winds long after they eject their outer gaseous
layers. Then, from 1994 onward, startling detailed images by the
orbiting Hubble telescope emerged. Private discussions about them
circulated in the astronomy world, but not much was said publicly as
these images completely upset previous theories on the disposition of
stars. See
Hubble
Image nebula 0828 ("Calabash")
Hubble
Image
MyCn18 (MyCn18)
Hubble Image MZ3
("Ant Nebula"; Menzel 3)
Hubble
Image (Jodrell) ("Bug")
Hubble Image
("Boomerang")
Hubble
Image
("Butterfly")
Hubble
Image
("Eta Cartinae")
Good reproductions of the Calabash, the Ant nebula
and
other nebula images
were published in the July, 2004
Scientific
American (some of these facts and images are copied from that
article). I came across the 0828 image by accident a few years ago
"somewhere on the internet".
Our
present ignorance about how these nebula work is often obscured
by journalistic babble. E.g.: "New information ultimately upends the
best of theories. Progress is often disruptive. It clears out old
niches and prepares the way for big (and often disorientating ) leaps
forward" (babble continues).
One characteristic evident of these hour-glass
shaped
nebulae is that the are magnetically controlled. The nature and origin
of such magnetic fields have not been discussed in public as far as I
can tell. So I will venture an explanation:
Up to the present
such a star has been fusing hydrogen into nuclei of larger atomic
number (Z) along with the accompanying neutrons to make nuclei of
atomic
weights (W) ever greater. The main star body has been so hot that
electrons no longer associate with the proton/neutron
nuclei, so the nuclei bundle together as gravity may attract them to
one another while their positive charge has also established a stable
standoff distance. Thermal agitation adds some standoff distance, on
the average.
Fusion has advanced far past the atomic number of
iron
Z=26, W=55, which we know on earth to divide exothermic fusions from
the exothermic FISSION of heavy atoms. There is so much extra energy,
pressure and density in the star interior, that it has become the
natatorium for heavy
elements in my opinion. It is even likely that nuclei have been fused
that are
beyond the highest Z (Neptunium, 93/237) that we know to exist on
our cool earth. Such higher Z nuclei are formed and decay
with some equilibrium and concentration, and likely have congregated
near the center of a large core.
.
Mid-life: First,
it is presumed that this sun-like star is now in a later stage of its
life.
Previously, it enjoyed the above mentioned sun like life, being
relatively large in
diameter and engaged in hydrogen gathering and hydrogen fusion for some
time. But of late it
is becoming starved of hydrogen on its journey through space. It has
not encountered a fresh bounty of drifting hydrogen fuel. So it
decays, using up whatever hydrogen it previously stored. Or it might be
in a late cookie monster stage where it ate too much, got too big, and
can no longer satisfy its appetite for hydrogen cookies.
This aging star will have some rotational angular
momentum, as nothing is ever so still as to not possess any. The
heavier nuclei gravitate to the aging star's center in proportion to
their atomic weight W; the heaviest toward the core's center. At that
moment, this is not important. Some shells or strata of various
radii may develop according to some
preferred groupings of similar nuclei.
Mid-life Crisis: Having
the misfortune in its journey through space to not recently encounter
some drifting clouds of fresh hydrogen, this star begins to cool. In so
cooling, it shrinks in diameter as lower temperatures all around
justify a smaller radius. Soon, the rotational rate (spin)
increases. The outer spinning lamina shells will most certainly contain
an excess of electrons. Such a rotating shell of charges will evolve a
magnetic field aligned along the average axis of spin. Sub shells or
spheres might develop where the angular momentum was too small to
homogenize or consolidate, so that a multipole star mass will develop.
But we will just concentrate on a one-body dipole-like spin model,
Death Throes:
As cooling progresses, the star's overall radius shrinks, the
spin rate
of those lamina, especially the core, that have shrunken increases
dramatically just as
exhibition ice skaters demonstrate by drawing
in their arms. The charged lamina, likely gasses heavily charge with
electrons that long ago were stripped from their nucleus, comprise a
strong circulating current that creates a strong magnetic field with
poles on the spin axis.
At the same time many high Z nuclei, really unstable
isotopes, will come to prominence as core
density increases.
Now it does matter that the Highest Z nuclei are concentrated near the
core
center++; as they
are the least stable of the lot and most prone to
fission. As the core also cools, it's greater pressure and
density cause the high Z nuclei to be compressed ever closer together,
tending toward a critical mass Eventually, this core goes into a
soft critical condition
where profuse and perhaps prolonged fission occurs. The product
nucleons are charged; each
fission propels charged particles having various velocities. The spun
magnetic
field is strong enough to constrain their average journey to be only
along the magnetic field lines; along either direction of the the spin
axis. Though launched in
random directions, the final velocity of these launched and positively
charged nucleons is only along the spin axis, in either direction.
Calabash Lives:
Thus, the planetary nebulae Calabash evolves; Calabash lives!
The expelled particle jet encounters the low pressure of free space,
expansion as a gas cloud occurs as in the jet of a rocket, into a
parabola of rotation. Similar jets occur as we see in either end of
this dying star, Calabash. A precursor, faint, far ahead of the main
plume and nearly on the projected spin axis, is seen a signature of the
"trigger" fission explosion responsible for generating this
impressive display. And we now know the evolution of the
hour glass pattern of planetary
nebulae.
10 February, 2008 AJC.