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MUCH LARGER GALAXIES ARE CONCIELED IN WELL KNOWN ASTRONOMY IMAGES This is a browse page, read at leisure EXAMPLES Massive M74 Supersize M33 Supernova galaxy Ngc 6946 Sunflower galaxy Ngc 3949

All these images proport to do is report more missing mass in routinely accepted astronomy images which have failed to reveal an object's greater superform bulk in the form of dim and very dim media contents, in images revealed to the public from major telescope installations described and interpreted according to what is seen in images lacking their major contents of missing mass.

SUPERSIZE NGC 6946

A January 1 2005 new years day gift from Gemini North telescope shows the center region the rest off screen. Enhancement heightens the awareness of straight lines vectoring to the left in a subliminal rooster tail, with a blue bob near the end of the scattergun straight lines.



Supernova galaxy Ngc 6946 is said to be about half the size of the Milky Way. This estimate begs the question as to if the whole of its supersize is known. Supersize images follow next. This galaxy is one of the most prolific supernova sources known. Read literature on the Internet if curious about this particular galaxy's prolific supernova output. It has had 8 supernovas this century. The Milky Way has not had one for 4 hundred years.

The Ngc 6946 supersize is seen in an enhanced Dss blue filter image, which swells to show a large reaching tangle of bent thick arms.



This histogram equalize version of the Dss image shows faint arms extending even further to the south, probably showing big in infra red.



This next view, downloaded in the name n6946levy.jpg, source unknown, brightens remarkably in enhancements to show a great deal of detail, including a good look at the blue bob. The levy image was rotated 225 degrees counterclockwise then flipped, to bring it to the same view alignment as the Gemini image.









The parallel tracks suggest the blue bob is a very fast tracker hurtling out to the west so fast it has not had time to bend into an arcing orbit, and may leave the galaxy entirely. If compressions lead to crunch, the blue color is due to prolific hot new blue star births of large and giant stars.



On the opposite side on an axis through the core another clumps of hot blue stars this in a scattergun facing the fringe of deep space, with a fringe of red star clumps a little further out. A first impression is the two (red, and blue) formations are somehow related, the red travelling at slightly greater velocity outward than the blue. A second impression is the two (red and blue) are co-incidentally in the same area in the arm.

SUPERSIZE M33

A supersize glimpse of the Triangulum galaxy M33 is available in a Gendler image where Gendler chose to record dim medias as well as the inner spiral clustered hot spots most astronomers focus on.

For instance Ngc 604 the 'strawberry' (in highlighted window brighter image pair below) is close to the inner fuss with a very large shell of diffuse dim matter in an oblong north/west south/east elongation is the true size of the galaxy in visible light.









The M33 supersize is so big it extends beyond the top and bottom of the picture frame. An incise down the left edge is seen, though a vague straight line, as a telltale showing where a sideswipe collision occured once upon a time.

The Gendler Triangulum image is particularly successful in revealing that Triangulum lacks a central core, and is dramatically wrinkled in a chaotic state, the right side noticably different than the left, both sides noticably absent standard arm formation typically seen around core regions of galaxy's containing massively energetic central structure(s), Triangulum is absent any such structure(s). It seems the core has been lost along the way in a former collision, a free wheeler can speculate, (without too much difficulty) that the Triangulum core was ripped away and left behind in Andromeda.

MASSIVE M74

A Gemini telescope image of spiral galaxy M74 contains the galaxy's supersize, the image has to be enhanced to reveal the galaxy total mass, much of which is 'missing' in the Gemini original.

The M74 supersize is so big it extends beyond the top and bottom of the picture frame.

SUNFLOWER GALAXY NGC 3949

Ngc 3949 original.



Ngc 3949 superform.













NGC 3949 - HUBBLE HERITAGE IMAGE

Click for original full size.
Click for enhanced full size.



At left the public view, a serene galaxy centered midscreen on a pitch black nighsky background. At right a huge dense galaxy so large it floods offscreen overflowing the picture's borders.

THICK GALAXY 3949

Most of its thickness is not seen in the Hubble heritage original image.

In the original only the bright center area is seen, the rest is illuminated but hidden in unenhanced dark medias.

Enhanced - huge body - hidden mass in this photo is revealed.

Focusing any two images together by eyesight is the best way to view these images.







The wrap around wall structure is deep, in places vertical. The center is a deep insink much deeper and more abrupt than a flat eyed disk.

You can model the galaxy in mind's eye as a magnetic field around an extremely powerful small permamagnet whose thick field extends a long distance around a tiny central permamagnet at the core of the giant field.

Prominant vertical galaxy upthrusts (toward the camera) are seen at both ends, emphasizing the thickness.



Next, two right endviews enhanced slightly differently cast more light on a ribbon of active star clumps stewn across the lower part of the image.

Web site/display/designs/image enhancements - Greydon Moore World's largest cosmic teaching site - Ottawa 2001/2004         form   A & O 3 3