INTERESTING FINDS IN HUBBLE IMAGES

Hubble images enhanced by eager amateur have more air miles than Hubble images enhanced by Hubble image engineers alone. Read on.

BAR GALAXY NGC 1365 Before - original - astronomer use the hot blue stars they see to gage theoretical ideas referenced internationally After - teeming thousands (if not millions) of hot blue stars not included in the theories Luminance=10 Gamma Corection=1.80 Blue color=+70

ANTENNAE COLLIDING GALAXIES Before - the original - astronomer achieves instant international fame by counting more than 1000! individual hot blue star clusters After - thousands more (if not millions more) hot blue stars are revealed Luminance=10 Gamma Corection=1.25 Blue color=+70 Both hot blue star finding images above, are used in context on how to find more hot blue new stars, here

NGC 1808 Skimpy little Ngc 1808 explodes to life when suitably enhanced with high luminating power activating latent dim media content in the original image (far left). When you superimpose the red and blue images, you will see a large form boring into the galaxy below the core, a gap the size of Alaska alongside the core borer These Ngc 1808 images are used in context regarding galaxy cores here

THE CARTWHEEL GALAXY Analysis of motions and rotary 'camshaft' aka 'vibratory' core rotations are described here. Analysis of a four body Cartwheel collision is here.

Missing content in Hubble images of Ngc 1512 are investigated here, two Hubble image examples of the investigation are shown next.

First is a near visible light UV photo in blue false color.



Click for original, and compare how much is missing in the Hubble original.

Second is a Hubble large outer view area shown enhanced beside a view maximally enhanced by histogram equalize.



Click for original, and compare how much is missing in the Hubble original.

Thackery's Globules are given a GIC industrial strength astronomy examination.



Since a 'pillar' is noticable, other pillars in nebula are also examined in context of being coherent reproducable objects with an underlying blueprint. Click for links to other GIC nebula studies.

CONTINUE

There are many other Hubble images shown their contents amplified, but what is the point of trying to show them all, all it will do is clog the page. Let's call Hubble show'n tell quits after this next sequence under the theme Hubble Heritage Images

INTERESTING FINDS IN HUBBLE HERITAGE IMAGES

Hubble Heritage image gallery

HUBBLE GALAXY SUPERFORM IMAGES     Galaxies in Chaos Hubble superforms appear   when Hubble images are highly enhanced.   Link here for Hubble Heritage main site, which sourced Hubble images herein investigated.   Investigation of other galaxy Superforms and Superstructures   More missing mass observations.   Hubble reasons   You must set your computer desktop to its largest width to view image pairs side by side. By forcing your eyes to focus two images together (for instance by gently going crosseyed) you will see remarkable intensifications of details and depth in each image pair.

HUBBLE IMAGES SUPERFORMS

Several Hubble images - particularly noticed by myself to swell beyond anything anticipated when enhanced by myself - are the following.

NGC 4414

High levels of blue enhancement reveals huge reaches of extra mass beyond the left bright flank, and an overall explosion of new mass in all of the black outer reaches in the Hubble original. A small region in different color within a large bloom of diffuse area in the upper right may be matter from a different galaxy which has collided and is now behind the scenes, a show of it peeking through as the different colored clump.

More Ngc 4414 missing mass is here.

THE FISH

Here called 'the fish' because it looks like a fish, colliding galaxies Ngc 2207 is huge! Vertical sheets in horizon planes at right angles to the face plane shoot up between the two colliders - at left at midcenter in the above thumbnail view. These sheets are examined in several locations in Galaxies in Chaos.

More Ngc 2207 is here 1 and here 2 and here 3

NGC 6745

This Ngc 6745 collision event shows a streaming long tail still connected to the departing small galaxy that was cause of a new 'yo-yo' restructure to the large cigar shaped galaxy.

More Ngc 6745 are   here   and   here.

Stephan's Quintet colliding galaxies explodes to brillience with long streaming tails amongst dancing galaxies having yo-yo appearances. 'Yo-yo' means parallel bright thin arms circumvent around a galaxy and can string out into tails. These characteristic long thin wrapping bright arms are the result of collision, but are usually of lower luminant dimmer media so are sometimes missed in normal careful image enhancements designed for a bright object on a pitch black background.

More stephan's Quintet is here.

A description of how 'antenna' arms form in colliding galaxies is here.

NGC 4603

A massive swollen image seen for Ngc 4603 may not be a superform since the original swells entirely beyond the picture frame, suggesting that much more (which would be the superform) lies beyond the picture borders.

COLLIDING GALAXIES NGC 3314

Enhanced and highly enhanced images of Ngc 3314, are used to demonstate that these are colliding galaxies (and are not two galaxies co-incidentally separated in deep space). The complete detective work concluding that these are colliding galaxies is here.

HALF SMASHED GALAXY NGC 3310

Monumentally deep indented core being pushed toward us, and chopped off arm leaving a long skeleton, are among the obvious and factual evidence that Ngc 3310 is probably in latter stages of merging.

WARPED SPIRAL GALAXY ESO 510-13

The warped panama hat brim horizontally grows out toward the picture borders, and the diffuse elliptical halo bursts beyond the picture frame when the Hubble original is highly enhanced with 'Gamma Correction' in a PC Windows graphics editor such as Paint Shop Pro.

Notice a sharp incise where the brown band vectoring right issues out of a larger growth at the left. In other words this left warpage is not a tip of a propellor, it is two arm bands, the brown band issuing from behind a hot star foreward edge from an inner source unseen.

FAINT YELLOW OBJECTS SEEN THROUGH HAZE

Note that many faint, more distant objects, (in dark yellow) can be seen through the haze when the original is highly enhanced, meaning the haze - like Earth's atmosphere - filters out certain colors leaving yellow color as dominant. Some of the faint yellow objects can be seen in the original, which does not indicate that most of the faint yellow objects are being filtered to yellowish huse through the warped galaxy's atmospheric haze.

THE DUSTING GALAXIES

Another faint object 'atmospherically' filtered to a dark yellow color, appears through the very large blue haze envelope of the 'Dusting' colliding galaxies.

The 'Dusting' colliding, galaxies with snub, is illustrated in important context here. A separate comment regards debateable peculiarities in the 'dusting' galaxies is here. Similarities with the Sombrero galaxy are here 1 and here 2. A third spherical galaxy (Ngc 4526) galaxy-speaks a similar language many of the words a brand new language to human's plugged ears.

NGC 4526

The toroidal shape of the 'Warped Galaxy' means that Ngc 4526 is also probably a 'warped' galaxy. In the case of Ngc 4526 the warp, if it exists, is not seen by being at the left and right ends of the encircling band rather than in the middle as the warped encircling band seen further above in the 'Warped' galaxy by Hubble. Instead, Ngc 4526 presents a toroid in horizontal plane on the left side, vertical plane on the right side.

NEXT

A dark smudge (lower left corner) appears in a dark area absent of deep space drifts when the original ESO image is highly enhanced by 'Gamma Correction' and a second version highly enhanced by 'Histogram Equalize'. The dark smudge seems coherent so something is out there, perhaps a dark galaxy, or, the dark area contains photon absorbing materials, or, the dark area is empty compared to the deep space drifts which irregularly surround ESO 510-13.

The even edges of the dark area make it suspicious as if something cooked up in the skunk works of the ESO image factory but the dark smudge inside the dark area seems coherent enough to be non-skunk.

The fact that the green haze on the left drifts meandering backward into rear space toward the top of the picture makes the green haze per se less skunkish. The green haze seems something valid, a form of deep space sheeting being trafficed by ESO 510-13 and captured in low luminant quantities in the ESO image.

This is the same galaxy featured by Hubble heritage and called the 'warped' galaxy, profiled above. Watch what happens to the large original ESO image when it is highly enhanced, and zoomed.

Have a look at some images I have prepared in attempt to make sense of the dark hole (lower left) it seems to have its own collection of globular clusters, and wisps of a meteror trail drift northward.

1   2   3   4  

After all that I definately don't understand that dark hole. It can't be the digital camera because electrons don't fart. A wrong cross shot of light in the lens seems ruled out since the dark hole has absorbed light not increased it. The very fine filamental nature inside the dark hole is not regular or coherent like a spiral or elliptical galaxy but a small pimple sized prong at the lowest edge inside the dark hole juts forward toward us and locking on that we see the strange tangled wires inside the hole are tilted backward, in this sense behaving like a galaxy core deck which can tilt at any angle.

In the solid black original square (number 4 above) not even any stars or clusters or see-through deep distant galaxies are seen. When enhanced, many objects pop out of the dark media which brings us back to the arguement that those objects were there all along, the dark hole in ESO 510-13 absorbing their bright light.

HUBBLE REASONS

Hubble images more typically focus in on some unique feature typically found well within a galaxy's bounds - even the center. However, Hubble images are also cited in astronomy remarks as revealing an object's intrinsic mass, which cannot be accurate if far more mass in dim medias exists hidden in a Hubble photo.

The point of showing here dim media masses missed in Hubble public images is to suggest that Hubble (and other telescopes) might also be used to explore a celestial object's farthest outer reaches, letting go of intents to explore oxygen or nitrogen content or clear views of center regions, and go for the whole thing in one complete image, ignoring wishes to capture fine line inner details or details of any unique portion of an object. The whole object in its maximum superform size will reveal quantities of 'missing mass', how much missing mass remains to be seen.

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LO AND BEHOLD - THE 'KEYHOLE NEBULA' IS RIDDLED WITH HEXAGRAMS - BOTH LARGE AND SMALL - and laced with criss crossing fractal lines

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WARNING - LONG LOAD !

Hubble's
Keyhole Nebula image
enhances to reveal these aspects of
interest - content in a dark cavity which had
just stars peeking out - and a collar around an outhrust,
the collar not caused by two masses moving slowly
together, not compressing in a none fluid
compression way, rather by two nebula
pieces drifting by each other
and scrubbing each other

From the original - a Tympani Resonator is discovered hiding in a dark crevice

ORIGINAL

TYMPANI IN DARK CREVICE

A red platelette stands up (in the left) near ridges (to the right) that are like incises cut into cream cheese by movements at different velocities crunching, one movement perhaps pushing outward.

Another 'cheesy' incise is seen in the Rosette Nebula.

And
where
did we get
these fancy Keyhole
Nebula views shown above,
from this Hubble Heritage Site, which
also has the master image of the Keyhole Nebula

Original

IN THE ORION TRAPEZIUM

A huge plume gushes upward to the right from what seems a tympani in the trapezium in Orion.

WHAT IS THIS

   

GRRRRRR



Astronomy's only mythological character, the Horsehead Nebula. Because it looks like a horse's head it is made to look like a horse's head, but it is not a horse's head nor does it actually resemble one when seen in full light. If anything, the above black on dark more resembles a dragon's head. If fact, it is not a solid object at all it is a sinkhole.



I my be rubbing rear ends somewhat too vigorously in the above image pair comparisons, the first the Hubble Heritage celebration original, and the second mine. I wanted to see as much as I could what the Horsehead really looked like in effort to dispell its myth in astronomy mythology from mind, and, it seems, succeeded.

Here is the horsehead in a larger Orion overview, the horsehead is a little toggle sticking out midway down the left edge in a huge 'materials' star forming field.



I lied.
I didn't tell
you this was going
to be a long file. Sue me
if you didn't learn anything

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