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GALAXY HIDDEN SUPERSIZES ARE SUPRISINGLY BIG More     in Superbig.htm More     in Bigger-1.htm This is a browse page, read at leisure EXAMPLES Supersize Ngc 613 Supersize Ngc 1097 Supersize M66 SUPERSIZE NGC 1097 By Eso's Vlt Melipal+Vmos telescope. A winding longarms galaxy with cat's eye central core, it's diaphanous long arms not visible until strong image enhancement reveals them. The long winding arms are very diaphanous, rearward beyond, myriads of small distant galaxies can be seen between and through the arms. Except for a short distance through the central cat's eye there is no ecliptic axis, this galaxy hugely fills three dimensional space. In particular, the lenticular central core is a lopsided lozenge in two parts, not flat.

Opposed thin ridgebacks curving out from the core circle in opposite directions occupy more than one vector each. If the image is rotated leftward so the upper arm swinging upward from the core lays now horizontally, after a 90 degree planar rotation the lower arm like a fin on an arrow will now be arcing upward foward toward us. 90 degrees is said for convenience.







Vertical lineal striations along the left flank are a telltale sign of an image chisling collision. Two different thermodynamics folding along the ridge of the lower dark rift spinning off from the core, plus a smoothed flattened platten of different plasma latent heat (bluer), standing up and dominating the lower right wing, are also guaranteed to be consequences of collision where one galaxy has slide over areas of another.

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The 3 dimensional size in bulk contributes heavily to 'missing mass' yearned if the whole is viewed as a two dimensional object only. Even more missing mass 'vanishes' if estimates of bulk are made using the original image plus the most enhanced image possible, comparing small details in the hulks of 3d vrs mono.





Next a slight zoom.









ORIGINAL



The bilateral ridgebacks of the central core are a standard formula found in any galaxy that has spiral. See both the bilatera.htm page and the symmetry.htm page for descriptions and examples of standard bilateral symmetry and cosmically related symmetry principles.

THE REAL SUPERSIZE - AND COLLISON

A Dss image when suitably enhanced leaves little to the imagination.







A huge scattergun rooster tail engulphs the little galaxy standing remote in the color picture. the roostertail is commonly seen in energetic collisions. Stephans Quintet is an excellent example. So are the 'Fish' Ngc 2207. Use key F11 if the above two links display image pairs vertically instead of side by side in your browser.

Stephans Quintet rooster tails



The 'Fish' (Ngc 2207)



If the little critter is the jitterbug responsible for all of the fuss, it has come out behind the core, moving further away north/west spotted centered through an opening in the scattergun clouds, and is at some distance in deep space behind, but not far enough that it has untangled completely its engagement with Ngc 1097.

It would be interesting to see little superboy in ultra violet and x-ray, to see how invisibly massive it might be. New born galaxies have been found aged on the order of 1 billion light years which can hardly be seen in visible (optical) light but are powerfully compact huge masses in higher plasma frequencies.

As an interesting aside, a Dss infra red picture shows nearly nothing at all for Ngc 1097 but enhancements enough to bring forth an outline of the large galaxy, is also enough to expose gravity waves pervading space with Ngc 1097 in view.





The bright image with bold waves is the dim lumens version converted by histogram equalize so that great contrast occurs between peaks and valleys of the waves.

In the Dss infra red original, galaxy Ngc 1097 is seen midscreen as a small white ball with faint flanges.

Gravity waves have been seen elsewhere. Other gravity wave pages.

Page Epsilon.htm explores moire wave grills extending across the borders of different Dss photo plates having different medias.

SUPERSIZE NGC 613

By Eso's Vlt Melipal/Yepun+Fors1/Fors2 telescope.

Another tonging longarm large galaxy with oblong lozenge central core.

Where are its arms (left). Here they are (right).



Large spiral/bar galaxy Ngc 613. Original at left, gamma enhanced at right. Probably several tangloid long arm spiral galaxies involved, with intermixing of colors making it awkard to try and separate one galaxy from another. A long thin arm, perhaps an original antenna longarm, extends from the left arcing a long way through deep space this way toward the camera (best seen in 3D where the extensive length of the longarm is unmistakable - focus the two images together by eyesight to see stereo).

In stereo, the right end of the core is farther away meaning the central core vectors along an axis from near left to rearward right.







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

Be assured that despite what can be enhanced, there is still a lot more missing mass to this bulky long ago collided galaxy than what has been captured in this photo.

Merger, of similar materials - probably one galaxy was rotating in contra direction to the other, the result a heaving deck not unlike choppy waters which momentarily spring up at the change of tides when insurging oceon or sea waters fall idle as outsurge of waters begin - at that interface the water surface becomes very vertically choppy for some minutes due to the inherent separations of two distinct angular momemtums before the waters have had time to merge anew in a tide whose direction of flow has abruptly changed.



Next, zooms.









Because the galaxy was photographed in only one directional perspective, the 3d profile can change when the original photograph's perspective is arbitrarily changed. For instance if the image is rotated by 180 degrees, left side and right side forground and rearward aspecta switch places, whereas foreward and rearward spacials remain unchanged along the picture's bottom to top vertical axis.





Structurally, this galaxy is similar to Ngc 1365 which is a well known bar galaxy. The (lower portion) hub of intersections where parts of one galaxy sticking out are joined from another galaxy can be seen in both nubs in the comparative side by side views next, bar galaxy Ngc 1365 is on the left.

More Ngc 1365 here and here.



Each has a differential transvector changing hub (gearbox) off an end of the core, in this case the lower end of each core, the gearbox directing the arms abruptly to the right.

THE CENTRAL CORE OF NGC 613





Similar constructions are noticed in comparing the central cores of Ngc 613, and Ngc 1097, next. Mainly, Ngc 1097 has a more disorganized differential transvector changing hub off an end its core.



An unusual small 'curl' occurs near the end of the core area, where the ridgeback crack abruptly ends. Zoom from original image at left, strongly enhanced at right reveals great unevenness in media textures.







Organization is similar in both Ngc 1097, and Ngc 1365 differential gearboxes.





Ngc 613 (right) is re-oriented by 180 degrees.



The two re-oriented views of Ngc 613 immediately caste bold light on the thicknesses and degrees in declensions amongst the arms. A gordian knot suggests both incredible slow motion and fast changes.

SUPERSIZE M66

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

Where are its arms (left). Here they are (right).



Original Chft authority image at left - the supersize is missing completely. Supersize via home enhanced at right.

Diffuse swish-around extras are perhaps long lasting residuals of a former galaxy in collision. The diffuse matter is assumed to be positively charged in having few if any distinct feature highlights or elements of information, no thin upthrusts or hot star formation clumps. It is possible the diffuse reaches had too much momentum to congeil into the start of an elliptical galaxy halo.



More M66 images are in the recent.htm page.

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