Missing mass is explored in detail in M74.
Missing mass is thick, thick, thick, in an image of Ngc 4258.
Missing mass is a residual small galaxy jetting into M87
Source of several images shown next below.
NGC 891
As suspected,
Ngc 891 is a wide
body object, the width
glimpsed inconclusively in
images enhanced, this one, out
in full smash from Japanese sources
shows the wide body as if a polar ring
galaxy whose 'ring' is in very dim medias
M65-66
Two
nearby
galaxies M65
and M66 have a closeby
neighbor, not even suspected in
first look, enhancement clearly shows a
large dim object in between, direct contact
between it and the upper spiral galaxy
seen in dim yet distinct tendrils
trailing upward, the dark
object has the shape
and size to
be a dark
elliptical
galaxy except
one would expect
something bright from
the center at least but this
large object is even darker in the center
NGC 253 (SCULPTOR)
A larger
diffuse oversize
is revealed for the Sculptor
galaxy in these enhancements, certain
features revealed more in blue, other features
including more of the diffuse surrounding haze is
revealed in red. Histogram shows what seem to be
gravitic waves
in concentric formation around
the upper right end and above the lower
left. Turbulence trailing away below
indicates upward drifting motion
HUGE SUPERFORM FOR NGC 3628
A very
diffuse very
grainy image does help
when enhanced, revealing a vertical
circular cyclonnic sweeping over the right
flank and dimly senses deep space turbulences above
and below the left flank
LONG ANTENNA ARMS FOR NGC 4676
Very
long range
antenna arms are
revealed in this Noao
image of Ngc 4676, the details too
blurry to bother with further image adjustments
M88 - SURPRISE
Huge
superform
hidden in faint
image of M88 which
swells to major galaxy size.
Windings are very cinched up, deeply
indented core, pronounced twists in lateral planes,
result in a very torqued object lacking a smooth generic dish or disk
Three
clustere large
vertical upright areas
which seem geometric perhaps 6
sided tympani resonator cavities, are
seen beyond the right end of the core socket,
and are sure signs of major collision but
who can say how long ago, but perhaps
recent, at least one object on
a long rod out into space
in the upper right
seems to be an
intruder or
jet engine
SUCCESS - CONFIRMATION
Dss
images
show similar
features as seen in
some above color enhancements.
Click on thumbnails for large images
Dark stretch between M65 and M66
Larger diffuse areas and space drift turbulence at Ngc 253
Huge superform of dim media contents immensly swells Ngc 3628 into an
intriguing superform, it was spotted partially off screen at the top of
the M65 Dss image of M65-m66. Smuged circular blurrs are seen at both
ends, the right end blur drifts into deep space in faint sonic collars.
WHEN NGC 4414 BECOMES AN INSECT
Scientists
and newspaper
publishers like to talk
about amazing co-incidences in the
form of total solar eclipses. Here is one, two
chance screen captures happened to land a pair of images
together in such a way they combine perfectly in virtual 3D
to give us a glimpse of the 'insect', a deep space
configuration in which it may be what we
are seeing is where another
galaxy went in,
darker
oval just
lower right of
the main Ngc 4414 body, and
where it came out, darker oval above Ngc 4414.
The cat whiskers which give the whole construction its 'insect'
appearance are also seen rather well and the only thing these
seem to be is tracks left in a sailpast by something
giving a slight glancing blow to the outer
left edge, the fact that the cat
whiskers are pulled in at
the point of contact
means Ngc 4414's
strong gravity collapsed
(concentrated) the shape of the
fast travelling by passer (gravity does
this - the stronger the gravity, the smaller
the cross sectional area, and the greater
concentration of rest state mass). In
fact the collider might have
sailed in ploughing
under the
core
advancing
to the rear where
there it resides now, the
actual collision event is not clear,
but, no contest, a choatic collison has occurred
TWO SLIM STREAKS NEED EXPLAINING
See large display of M94 images in context here.
In the next images, of M94, (from this Dss image),
the small slash is at further depth and a different angle its right end
dipping away, whereas the right end of the larger slash is angled sharply
toward us in deep space.
Suspect these are galaxies. Sharp clues are
as follows, seen only in 3D by overlaying the two images together - the
small slash is far distant back in deep space, very far, and the larger
slash has a sharp elbow jog, which is common
in galaxy arms and rims, and cannot be
made by some mad astronomer's razor blades on a film negative or whipping
the mouse around on an image altering computer. In fact the upper broom
tail, which bends this way, has parallel layers, as seen in the low
resolution zooms enhanced above as best as I can get them (see the
three 'slash' images above again). A wide ranging look at slashes is
here.
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'low radiance' hidden mass |
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This rotated image above was used to solve a major mystery involving
slingshots, here.
Good 'slingshot' views in galaxy examples are here 1 and
here 2.
A histogram view (dark blue) shows that faint streaks are streaming
upward from the top, and, there are faint concentric arcs in deep
space radiating upward above the small galaxy.
An ESO image of Ngc 1232 explodes
into stupendous size, most of it on the outer right flank, the left
flank where a small remote galaxy named
Little Rudolpho hoves nearby does not explode with the same push when
the original image is given one hit of Histogram Equalize.
SUPERGALAXIES Forms of well known galaxy objects are usually rich in abundant surrounding mass at larger area, the abundant outer field mass usually not seen being very low radiant compared to the brightness of the main galaxy which is usually the only form of a galaxy known, as bright and colored against a pitch black deep space background. However, each of these galaxies extend far out from their optically most bright inner regions, the outer superforms captured in photo medias too dim to be discerned by normal eyesight and when enhanced to reveal the superform the inner optically bright mainform becomes overwhite which is of no good to astronomers. However, the superform actually reveals the whole of a galaxy's scope, not just its pretty picture. Histogram Equalize in an image processor (such as Paint Shop Pro) can reveal in an instant what lays afield though producing a product with few fine or exquisite details remaining, due to overbright, yet, how much more of the galaxy is seen, is well worth the effort. Enhancing an image density with 'gamma correction' may reveal more in an image but usually produces a grey or smurred background and in most cases cannot reveal the true extent of residual faint captured photons such as are instantly revealed in the maximum light-dark contrasts revealed by Histogram Equalize (3rd images at right in the above composite panel). The following is a photo show designed only to show and tell, each, a 3-picture trio, showing an original image enhanced by 'gamma correction, and a 3rd view enhanced by 'histogram equalize'. You can see the superforms of the galaxies in an instant, perhaps even you may recognize a galaxy or two since most of these object are well known and well studied by astronomers |
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Notice
how a drift
extends from the
upper end of small eliptical
galaxy Ngc 205 to a disturbed area under
the rim of Andromeda, revealing that small Ngc 205
is emerging into the open from a recent flyby
under the body of Andromeda. Such instant
finds in enhancing an image are
nicely worthwhile and can
at once put aside
fields of
paperwork
(football field
size) hammering theories
back and forth regards the activities of
small elliptical galaxy Ngc 205 and its relationship
to mighty Andromeda. The above Andromeda image is not
to scale the height exaggeration more immediately
revealing the drift's band of blue matter
See more about the drift, and about Andromeda itself
An
advantage
of viewing a 'superform'
is new arms or other dramatic dynamic
features can be seen in an instant, particularly when
an image is viewed fullsized (not the 'thumbnail' scale used
for the images above). Not currently under study or known by
astronomers in a given galaxy, the superform is a leading
seeme guide to galaxy superstardom and will certainly
shave a few points at least off the missing
mass percentages of the universe
AN ANTENNA REVEALED
Click here for antenna 'time signature' images
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ENHANCING PROTOCALLS Astronomy photographer David Malin of Australia has reported that attenuating the 'contrasts' in developing prints from emulsion photographs of astronomy objects can reveal new details not prior known to be in the emulsion - he called these finds "finding little white buggers all over the place" I have found that 'contrast' in an image processor, interferes with an image's latent contents, that use of 'contrast' rubs out much of the finer details which can or may be coaxed from an image by using enhancing adjusters such as 'gamma correction' (density), 'colors' (richness), and 'histogram equalize' (fundamental dark-light contrasts) I rarely (hardly ever) use 'contrast' in playing with enhancing adjusters when looking for hidden or dim 'missing mass or new details' contents in an astronomy image, including digital captured images from Hubble, ESO, and Chandra, in which (for these three digital telescope sources) color density and gamma correction are the most useful way to go since 'histogram equalize' for images from these three sources tend to produce only a pixilated amorphous background field and extreme washouts of the central image. You will see what I mean if you try enhancing images yourself GM. |
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I would
like to use this
Andromeda endhalf image
but cannot, too few dpi's in what
originally is a large image. The only thing
usefull is to show how much missing mass drifts
beyond the east hard border, and to assume this
image from Noao is one of the scenes used here
by an astronomer to suggest the drifts meant a
collision with
Triangulum
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A pause to wonder what constitutes this door handle -
Hmmmmm? what is it. Enhancements (by GM) show it is associated
with some extremely dynamic circumstances lurking in the
darks of obscuring dense low-luminous matter
888888
The Studebaker door handle is seen (more dimly), in a Dss plate, of
'Coronae Australis'.
Click for Dss Coronae small
Click for Dss Coronae large
It was
hoped that a
Dss Deep Space Sky
Survery image of Ngc 4414 would
reveal more insight as to the nature of how it
came to have such a huge far ranged vertical underskirt.
The image Dss image doesn't of course. It is interesting however
for another reason, in what it reveals about the deep space sitting of
Ngc 4414. A small version shows long horizontal drifts across the frame
in bands of differing media density, and slanted vertical sheeting plus
swirls around bright objects indicating motions, or gravity
wave interactions, or both. A larger version
of the same histogram enhanced Dss
image reveals thin tracks
even cracks crossing
space, and a
long thick
twisted helix
rises vertically
from the left snout of
Ngc 4414 where cat whiskers
criss cross at the snout itself. This
twisted helix and the cat whiskers may have
something to do with Ngc 4414's odd nature (most of
it's stuff is hidden from all but insect's eyes - insects
see in other frequencies than those most used by
humans). Two zooms show extended oblong
mantles around the outer body, the
outermost mantle very faint
Thugshots
from a graphic
editor's preview window,
show sheeting and cell walls which
cannot be seen in an obvious way in
the larger images. Ngc 4414 is
the round black spot in
the middle
RESIDUE OF ANOTHER GALAXY WHICH ARCED UNDER NGC 4414 ?
A 'mosque'
(swirling oinion)
above the insect seems
to have probable cause in the
insect's circumstances. In thugshots
the 'mosque' is an oval cavity with ribs
radiating into to a point at a hot object,
the oval seemingly a vacuum in the
media density of space there
The 'mosque'
is in a perfect
position to be all that
is left of a smaller galaxy that
arced under Ngc 4414 causing the deep cleft
in the front edge of Ngc 4414, the cleft is very
deep but if a galaxy sailed through there, it
did not seem to disturb the core by much,
suggesting it may have dived in,
swinging in a gravity grab
arcing downward, as it
it entered like
a comet in
orbit
in closest
approach to a Sun,
and came out the other side
hardly anything left of it, slinging
on out in an uprising hyperbolic path, or perhaps
on an elliptical orbit bringing what is left
(residue) back to Ngc 4414, eventually
Images
used above also
appear in the Ngc 4414 page.
The slightly rotated image above
is a surprise discovery on
how to improve 3D
COMMENT
Images
such as the
'mosque' showing a
vacuum caused by a dense
small object are not to be trusted. In
an image as grainy as these views, however,
it usually happens that 'grainy' views are in
fact showing something and later what that
is can be revealed by another released
image of great mew professional
interest. In fact, ovals
like this may be a
faint residue
of a spiral
galaxy totally
stripped of dust and
gas leaving only clumps in rings
showing where the galaxy's breadth once existed.
For instance oblong diffuse galaxy M110, neighbor of Andromeda,
has oval rings made only of small bright dots sweeping out long distances
at oblique angles to the plane of M110, the oval necklaces are consistent with
a spiral galaxy (larger than M100) stripped of everything but it's star
fields, which is entirely possible since M110
itself is just now
emerging from a vigorous piranha attact under the
hemskirt of Andromeda. And this puts entirely
new meaning to the words 'missing mass'
since they include skeleton arms
Missing mass, a great deal of it, shows up in outer left
flanges of galaxy Ngc 4414
Click here for very revealing Deep Space Sky survey images of Ngc 4414
The
blue matte
in the lower left
is actually more galaxy
a whole lot more of it, in dim media
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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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