to bottom  
VAST HORIZONTAL EXPANSE MEANS A CIRCULAR DISH

These
stereo views
are able to show the
circular breadth of Andromeda
reaching far across a wide circular
tableau to reaches long and away behind out in
deep space. The view shows that our Andromeda is
circular, rather than a mere fluke-shaped
elongation along a long east-west axis
(as is suggested by all Andromeda
images viewed in 2D mono)

The
real shape
of Andromed is
more circular, not
rather an elongated liver
fluke. You can not know this
until viewing stereo images. The
best stereo views are here, in
which a look across a wide
expanse across the mid
section best tells
the breadth of
Andromeda

Missing mass looms over the horizon in stereo

Other
stereo views
of the Andromeda
lead little left to the
imagination, as stereoscopically
seen in an immense horizontal distance
spanning far into rearspace across the top
of the plateau, the stereo showing a wide active
region comprising the crown on the top of a wisdom
tooth where the central part normally thought
to be Andromeda is hot rings with a deep
inset core bole, and a wide skirt
spreading out not unlike the
disk of a comsically
altered frisbee



Frills
dance up along
the far distant rear
edge, conciderable turblence
and chaos indicated by such tiny
compact coherent frills as if
very rough rapids are
here in stereo
view

SLIGHTLY WARPED FRISBEE





Stereo
reveals much
bunching up on the
right, each rim bunching
up even as it drops down lower
than the proceeding inner rim, the
outermost dim rim lowest down
in the horizontal plane

The
fact of
a circular
aspect (not thin
fluke), and deep (not a
thin doily like the rings of
Saturn) dramatically increases the
amount of mass the whole shell of Andromeda
contains. Calculate the difference in area between
a flattened collapsed sickle cell, and a healthy round
cell, to get a grasp of how much more mass will
be contained in a deep cell-shaped suck
candy with indented center





REGARDS M110

Alignment
of haze at both
ends suggests the small
galaxy may be slowly flipping
in the air, the forward end (south)
moving up, the rear end (north) moving down,
and also a slew - the elongated shape may
be rotating counterclockwise very slowly
around an inner center point, flat
tongue shape, and horizontal
distance from Andromeda
better seen in stereo
by focusing the two
images together



Indications
in stereo are that
the left flank is not an
'ideal' circle, it seems more
jogged up, with a bending kink, more
irregular than is the much wider seeming
right flank, in this case the east side is
more horizontally spread out, the west
side more vertical. Such asymmetry
in a galaxy's fundamental
compent shape shape is
not untypical for
many forms
of spiral galaxies.
In the case of Andromeda
the asymmetry in planar topology
is not pronounced. Here next is one image
which shows in a self evident way that a horizontal -
vertical component exists in galaxies, in this case a partial
elliptical galaxy reveals a flattened horizontal portal into a
wall of haze at the left side of the central rim band, and
a vertical rise into the haze at the right side, the
fact of galactic 'topolical asymmetry' thus
proven by this single enhanced image
of Ngc 4526. This is a 'warped'
galaxy with the warp
at either side.
A 'warped' galaxy
with the warp crossing the
centerplane axis in the middle is here



Image source for Ngc 4526 is here



  email     home   Web site/display/designs/image enhancements - Greydon Moore
World's largest cosmic teaching site - Ottawa 2001/2004    

    form   A & O 3 3                 to top  

                  Click google logo for site search
  Click for site search  

For the world's most comprehensive searches use   Visit Webcrawl


  Click for Industrial Strength Astronomy home  
  New Proton Page     New Physics Index  
  Crash course   Fast crash course in astronomy
More advanced at top of home




Available Downloads

DRUMBALLIA    ODDESSY    CLIFFR    CONTACT