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Some image
redundancy herein
is deliberate - different
themes. Think of it as similar
equations in different parts
of a thick physics
textbook
Another
poke at the
Andromeda core
takes place here
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No
one has
seen the Andromeda
core since it is a flattish
oblong laying in a canted angle aimed
rearward in a depression like an egg settled
in a nest, the core itself canted at a sharp angle
its main slope cammed turned toward us, the cam due
to contained different angular momentums than in the
immediate arm swirls surrounding, the result a
slow turning out of synch of the core to
the rest of the galaxy. In fact
two slow motions are
involved: that
which cams
the core
toward us,
and that which
is causing the end
to settle in the socket.
A swath of haze drifts rearward
above the core, gently curving to the
right to join rear rim flows to the right
The cam
is not the
point. The point
is that one side of the
core flares up, the other curls
down. In Andromeda the upcurl is actually
from the lower (west) end of the core settled down
in the socket. How is this known? A picture which has
been around for a long time, when enhanced properly,
instantly reveals the core's bi-lateral s-shaped
symmetry. The s-shape is a standard form
seen in galaxies in general,
nothing unusual here.
The enhancement
occurs in
the blink of
an eye simply by adjusting
the original image with histogram equalize
Very important image
In the
original,
the core face
can be seen to drop
down a vertical slope (like
Niagra Falls). This is correct. A
vertical drop down a steep slope is often
found in galaxy cores viewed in 3D. In Andromeda's
case the question is this is image of such poor quality it
hardly counts as astronomy. None the less it seems the
only image around able to show the nuclear core. The
problem is that Andromeda's core is so intensely
bright, relative to the whole rest of the
poor radiating galaxy, that the core
invariably shows as a hot globe
glowing no matter how much
the core's light was down
filtered, and astronomers
accept this. Here with this
image is a unique opportunity to
see more of the core, and its surrounding
s-shape configuration. The image was very early when
pros new little the real look of Andromeda and this one
was the best to be had at that time. It's capture of
slow radiant photons gives us a unique view
into the Andromeda interior
Here we see a little clearer how the bright core area is skewed sideways and partically standing up, plus the upper end is heaving forward the lower end dipping back.
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So
you see,
there are two
s-shapes. Bi-lateral
symmetry acts twice: the
Niagra falls effect clearly
the bottom shooting out and up,
the top pouring over and curling
down, and around the sides the
rear sweeping up and away,
the near sweeping dn and
around in the opposite
direction. Plenty of
properties to see
in one throw
away image
Click here to see movie showing hot points of light in the
middle of Andromeda's double nucleus core
Andromeda's double core - two black holes in speculation.
A sizeable sinkhole occupies the lower left - cause unknown
The
smaller
core (to the
rear) is actually
the more energetic, it's
counter intuitive smallness due
to intervening dust and clutter between
the black hole at the rear vrs the second
(larger) black hole more toward us
closer to the camera
If the
yellow halos
are appearing correctly
(not imager processing extra from
Hubble headquarters) the two halos are
joined by a sweeping arc from the larger
(forground) back into the rear halo
(smaller) the curve a classic
sci fi accretian disk
image which in
this case is real,
where two nuclear black
holes are visibly inter-engaged.
At the borderline of perception is the following:
In 'virtual' stereo, the forward larger hoves backward at a
tilted angle it's lower edge jutting toward us. From behind at
the upper left, the yellow accretion tether winds around going
backward to approach the smaller object from the rear, coming
forward to join the smaller behind its left side. To see
the wind in the accretian tether requires diligent
focusing and ideal viewing conditions (glare
right on screen from lights will
spoil, dark room is best)
Hubble
has noticed
two cores, both
assumed black holes, the
inner arrangement not in plain
view except the smaller noted core is
actually the largest. I have managed
to coax some more info via image
enhancements and have arrived
at one which seems to show
hot spots winking on
and off but the
prospect is
high that
the hot
spots are
over exaggerated
image hotpoints rather than
actual new-seen goodies winking in the core
A dark
hole has turned
up in the enhancements
by Greydon Moore (who also did
the animations). The nature of the dark
hole is simply not known within the context
of this Hubble image, but, it is
unquestionably there
S-SHAPED CORES IN GALAXIES
An
s-shape
core can hardly
be better illustrated
than with these views of M100
by Hubble. The first is of course the
famous inner (nuclear) core made by Hubble
as one of Hubble's first
new images verifying
that the original myopic lens problem had been
solved. Note in the next image a profound
s-shaped arm up the center almost
over the hot center core
kernal
Notice
the abrupt
punch-out at the
lower foot of the core, a
round cavity cape with a prong
jutting out. Prongs jutting from one
end of a black hole core are not uncommon,
once you have seen one (here) you will
see others. The 'prong' seems to
have something to do with
black hole polarity
dynamics
S-SHAPE IN THE CORE OF NGC 1365
No
discussion
of s-shaped cores
can go by without the obvious
s-shape in the core of Ngc 1365
as pointed to by Hubble, for instance
a strong 'prong' froths out from the
foot of the core up jutting a
short distance
A maple
leaf stands
up in the middle
of a long shank, the
forward part of the shank
coming toward the camera from
below the maple leaf, the rear
geared shank from the top of
the maple leaf. Care to
count the number of
symmetry item
points, in
this
When
these pair
images are focused
together they will be in stereo.
Instantly seen will be bi-lateral synmmetry,
where one side of the core flares up, the
other curls down. To one degree or
another, bi-lateral symmetry
is found in every galaxy.
Rooster tail is the
larger outer
form
Ngc 1365 image collection. Ngc 5236
image collection.
| S-SHAPED CORE IN M101 |
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Small
toggles
spin off the
core of M101, aimed
in two opposed directions
and with bi-laeral symmetry, that is,
one toggle aimed upward, the other down
In
any search
through an astronomy
site via you surf there is no
documentations (except occasional techno
dense abstract) citing thickness in galaxies or arms
that are 2 dimenionally flat. Occasionally an artist for an
agency such as NASA or JPL has produced an illustration used in
reference showing an indented arm at below the disk line or easing
above the disk but no waggling like a worm out of an apple in 3D
space. The above M101 core views clearly show coils winding
in thick vertically slanted sheets around the central
energy source, the look not unsimilar to a
cinammon roll. Missing mass screams
to be recognized
| ANROMEDA EXPOSED CORE AGAIN - EARLIER STUDY |
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Bi-lateral
symmetry, in this
case asymmetry found at
the core, cannot be more self
evident the instant the above image
is viewed in stereo by focusing the two
images together. All galaxy cores seem to
have bi-lateral symmetry to one degree or
another, in the case of Andromeda the
bi-lateral symmetry seems slight
for appearances of the large
glowing ball, but when
appeared exposed
the bi-lateral
symmetry is
far more
obvious
The
core a
flattish glowing
orb socked in a cavity the
orb so bright so intense it is lighting
up part of the rim, so hot it usually masks
out to white in any photo designed to
capture the far less radiant
rest of Andromeda
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Original a diffuse vague shape, enhancements reveal core dynamics
Even
if you
disagree with
the concept of stereo
in mono images you have to agree
that superimposing together two images of
extremely different densities produces
an excellent concequence in new
details revealed
Original a dot, enhancements reveal core dynamics
These
cores views
may be the first
ever shown of Andromeda's
actual core. It is similar in fact
typical of cores seen in other massive or
super massive galaxies, hidden under the vale of
glow, Andromeda's core is no different than any other
The
elongated
s-shaped core is
most noticable, one side
flaring Up, the other curling Down, in
a core bole sitting 'cammed' off angle (out of kilter)
to the swirling arms that surround it, revealing that core
forces as are these are rotating at different velocities
each on different vectors than the velocity of
the outer swirling arms
Ngc 1365 image collection.
Ngc 5236 image collection.
M101 image collection
if you
disagree with
the concept of stereo
in mono images you have to agree
that superimposing together two images of
extremely different densities produces
an excellent concequence in new
details revealed
Original a dot, enhancements reveal core dynamics
These
cores views
may be the first
ever shown of Andromeda's
actual core. It is similar in fact
typical of cores seen in other massive or
super massive galaxies, hidden under the vale of
glow, Andromeda's core is no different than any other
The
elongated
s-shaped core is
most noticable, one side
flaring Up, the other curling Down, in
a core bole sitting 'cammed' off angle (out of kilter)
to the swirling arms that surround it, revealing that core
forces as are these are rotating at different velocities
each on different vectors than the velocity of
the outer swirling arms
Ngc 1365 image collection. Ngc 5236 image collection. M101 image collection
Web site/display/designs/image enhancements - Greydon Moore World's largest cosmic teaching site - Ottawa 2001/2004 form A & O 3 3
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