to bottom   GALAXY   NGC 1365   IS A BIG SUBJECT IN GALAXIES IN CHAOS.
EACH OF THESE PAGES INCLUDES   NGC 1365.
   Tympanum bus bar couples charge states between two merged galaxies

   3314.htm                   Hotblue.htm               Property.htm
   3d-optic.htm               Hubble.htm                Purpose.htm
   Bilatera.htm               Lookhere.htm              Rattles.htm
   Blare.htm                  Missmass.htm              Spindle.htm
   Core-m31.htm               Momentum.htm              Stream.htm
   Cores.htm                  Ngc5236.htm               Symmetry.htm
   Globular.htm               Preview.htm               Vortex.htm


THE FABULOUS BAR GALAXY NGC 1365 IS A LINK CHAIN

First,
a self evident
stereo model for Ngc 1365


Super
Nova 1987
in the LMC has two
major topological conformities
to Ngc 1365. First is that one of the helix
rings in Sn87 spins off in a horizontal plane, arcing
around to the upper rear, the other helix ring spins off in
a vertical plane and arcs around into the lower foreground.
Secondly, each helix spins off from an opposite side of
the core. Both of these dynamic properties
are maintained in Ngc 1365



Compare.
Here is the Dss
original used to achieve the
above spectacular color tone enhancements


If you
want to talk
about missing mass,
finger waggling a few stray
hairs scintillating the bald spot,
the profesional mentally mulling 'what
missing mass, its a particle we haven't
discovered yet that saturates space',
have a look at this next image,
enhanced from a Dss original



An image by ESO




Now
that you
have seen it,
you cannot ignore
the missing mass which has a
major symmetry principle - the galaxy's
main arms continue around to more or less rejoin
source, and, one arm is oriented at a distinct
rotation from the other, as if, two
links in a link chain

  click on image for full size  

Window in DSS deep space view shows full size of galaxy.

There
are galaxies out
there, very small smudges faint
tiny blurs, barely seen in the Dss original.
Here is how to see them at once without having to
book time on a major telescope. At least 9 galaxies
can be seen. The scenes in the 'preview' imaged further
below are rather hard to be definative, so here next
is a zoom from which the 'preview' shots
were made. Galaxies can be
counted in the zoom


PREVIEWS

Traces
of deep space
gravitic excitement
(rippling lines and ellipses)
have turned up in 'preview' views.
A cleft in deep space forms a folded arc
over the head of NGC 1365, where entropy
is flowing in streams. There is much still to
be learned about this galaxy, the bi-lateral
asymmetric planar phase rotation of its
two arms for starters, and the major
bi-symmetric left/right form of
the s-shaped core

   

   

The
more I
get used to these
deep space and hidden mass
images of Ngc 1365, the more I can
form a picture of it as a more normal or
standard spiral galaxy with two long wound arms
if re-oriented to be looking upon the core
sideways except the core would now
have changed dramatically
still looking as a
core because of
its 4 poles, and
the swirled matter drifts
seen filling space on either side of
the core would become the central inner bands of
arms in angular momentum that typically surround galaxy cores
Pillars of fire rising from the core

The
zoom views
come from a Hubble
Antennae colliding galaxies image



Pillars
of fire seem
to be an entirely
unrelated phenomena, that
is, not caused by galaxy remnent
projectiles rather, by perhaps strong arcs
in magnetic fields. For example not one but two
pillars of fire are self evident, one spins off
from end of a core and rises in a huge
backcurving tranversing the whole
face of its galaxy. Some core
phenomena seems explicitly
involved and no rattle
points to a telltale





Further
enhancements
in color tones of
the Antennae pillars of
fire reveals little new except
more of their stupendous size
in arc bending through
3D space













A magnification
straight into where
the core is splitting in
half does not reveal a great deal
about how the pillar of fire originates





Notice
the crescent
moon shape in the
inner bar, a sub crescent
moon in the upper bar partition







A noticable
crescent moon shape similar
to Ngc 1365 is seen in Ngc 5236


NGC 1365 CORE - BI-LATERAL SYMMETRY - ONE SIDE OF THE CORE
FLARES UP, THE OTHER SIDE CURLS DOWN

For
comparison
the core of
NGC 1365,
a very different galaxy, in an
extreme closeup view by Hubble,
has a similar look and feel to
Andromeda's s-shape core



One
noticable
difference is the
core of NGC 1365 is more
thrust up like pushing shards piling
into mountains, whereas Andromeda's core
to the extent we can see it is more
long sweeping and evenly
serene, less chaos

Now
is a good
opportunity to show
off what virtual 3D can really
do. The core is deeply cleaved and crevassed,
you cannot see how deep until accepting the inevitable
and look at the image in 3D by focusing the two images
together. There is a small hole at the base of
the core mount, the hole may not be
an actual hole just a place
where lumonics are
not radiating,
but also
may be
a glimpse of
a void which might
surround a mighty black hole
though stupendously powerful the black
hole occupies an extremely small area and is
(black hole) conjectured by theorists to sweep
clear an area surrounding its event horizon,
also, degrees of separation due to image
patching inconsistencies are easily
seen in thin straight lines, the
flaws hard to see in mono



WHAT A HUGE GALAXY























The above enhancements came from this image, which came from here.



  email     home   Web site/display/designs/image enhancements - Greydon Moore
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