If astronomers are using images such as the following originals to factor concepts of plastic mass and missing mass conjectures, it is no wonder that puzzlement abounds. Each of the images has enormous contents when enhanced beyond original public release specifications. More missing mass and galaxy superforms are at these pages. missmass.htm missmas1.htm superfor.htm anomaly.htm anomaly1.htm |
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MISSING MASS AND GLIMPSE OF SUPERFORM IN NGC 4603
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A very hard splash of red, which turns the center area details solid with color, is incredibly useful nonetheless in merger 3D where the best of both images merge into one and lesser effects (such as solid red color) vanish.
Hst source site
Hst blk & wht original
Hst color original
The galaxy hardly shows in either Hst original, the no-show in the blk & wht may be due to frequency study photo (a specific single radiant frequency captured in the blk & wht photo).
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This is what Ngc 4603 can look like in full (left), clipped from a highly enhanced Dss 1st gen image of Ngc 4603.
The Dss original shows less mass (right).
The enhanced view (left) shows what seems like a galactic sized comet heading into the galaxy from the lower right, the comet's tail sweeping a path between vertical vectors, through galaxy arms.
A spray of small arms is seen in the comet tail arcing lower right from the comet head located in the right midst of the galaxy. This seems sure evidence of former active status in collision(s).
A RING GALAXY?
There is what looks like a ring galaxy in the extreme lower right corner of the picture. The 'ring' is spotted in the extreme lower right corner of an HST blk & wht image.
The ring turned up after very high enhancement of the original, in which no sign of the ring is seen (see lower right corner - nothing is there).
A histogram of the original reveals the ring, very faint but definately there. The small size rules out determining if this is a false positive in a bad spot in the negative. The ring is proportionately very small, suggesting, if it is a ring galaxy, that it is much farther away.
The corner containing the 'ring' has been cropped out of Hst color views. Different Ngc 4603 images by Hst have been released in different orientations, which is rather unusual for Hst.
Click for histogram view showing ring
Click for close ring view
Click for full ring view
Click for original view
More 4603 images can be seen here, here, and here.
INTERGALACTIC RUBBLE STREWS TO GREAT DISTANCES IN THE PERSEUS GALAXY BLUSTER
Ngc 1275 - also known as Perseus A - in the Perseus Galaxy Cluster.
These next images (and others) are shown elsewhere.
Hubble 'preview' original
Enhanced at home
Images of Perseus A in the Perseus galaxy cluster, the Hubble view showing fiercly active moments of dense matter between the galaxies.
Perseus A is officially classed at a 'cannibal' galaxy. More of its voracious surroundings are revealed in the above enhancement, some of that revealed is completely unexpected if just viewing the HST original shown first.
3D indicates that the strew path is extending toward us, the flaming hot object on an upward trajectory slanting away. The amount of spoiled brew in the strew path indicates the hot galaxy is travelling away fast.
When you concider that some of the construction site boils are vertical, there is conciderable mass (missing if not counted) in this seething display, the whole region of the image is packed with mass, it is thick, as well as spread out on a horizontal plane slanting away from us.
Note - in the imaging processes by which the above image was produced and posted for download, the image takes on a destructive checkerboard mesh when reduced in display beyond a certain point, for this reason it is not possible to show a full image in 3D. Two partial images are shown instead. The two partial images were also rotated left by 90 degrees to fit them into the display without checker boarding.
More about boiling galaxy Ngc 1275 here
More about Perseus galaxy cluster here
FLOW STREAMS REVEALED IN ORION
This image of nebula M78 (one of the several bright clumps in Orion) contains a great scene on the nebula's flow streams and long curls, when highly enhanced, particularly in its red content hidden within a publically released dim image.
This image was studied a second time a short while later, with result as its own Globe.htm page. Read if you dare.
Red content above, original (with it's dim content) next.
In 3D - merge two images together by eyesight to see true 3D - reveals all thrusts forward, primarily in a vector aimed over your right shoulder. Two 3D views are shown. Subtle differences between the two views reveals more of the seething topology in the flows and the portals from which issue bursts, and within which thin narrow slipstreams are sucked in to disappear. In particular, distinguishing finer details are seen along and behind the long narrow curl above and left of the main nebula.
Oops, tried to find the image source again on the internet, no luck, it means the source of the above Orion image is not cited herein.
Ooops found it again, do not know how I missed the traffic lights searching first time around.
M78 image source at APOD
Click for original
Click for enhanced 1
Click for enhanced 2
M78 in the fields of orion by Sloan digital Sky Survey.
Click for enahnced 1
Click for enahnced 2
M78 original at left (small), enhanced at right (small).
Now I plead innocent ignorance - I have not been able to find an official reference which states that M78 is, or is not, the small glow whose overhanging fronds show that the arc made by the smooth gliding motion of the horsehead is an arc, since the fronds spill over the arc proving the arc is not an artifact falsely reflected by mere telescope lenses.
Ooops, nearly stabbed myself in both feet, M78 is... isn't...
Seds has this to show regards M78 (Ngc 2023). No street map shows where M78 actually drifts in regards to the horsehead. Yes, there is one, homemade, at the top of the Orion-2.htm page.
LINEAL STRIATIONS SEEN MAKING CONTACT WITH THE ANTENNA COLLIDING GALAXIES
Antenna colliding galaxies from ESO.
A very dim Antenna view by ESO enhances to reveal diagonal striations, which may be deep space indications of gravity waves present in the Antenna vacinity including making contact with the galaxies. For reference, see gravity waves at M101.
Although the striations seem at first glance to be too coherent to be natural, perhaps thus caused by digital rastering scanning the galaxies, the striations are not lineally coherent enough to rule out natural causes, such as large scale gravity waves.
Even if the striations are bogus, the image itself reveals the collider's true size, which includes large surrounding areas of diffuse very disturbed material. This image contains the largest super structure containing details seen for these galaxies.
Six sided 'tympani resonator' cavities, hunkered in dark areas between the two galaxies, and are in fact poorly seen in the VLT image above, are detailed here.
ESO original
Even though blurred, it is obvious that the inner valley up the chasm is a caldron of tympanic formations. A huge arm stump with two short woggles sticking out (below the valley of caldrons) shows major whumpage where a thick arm has been cut as clean as the arm of an octupus.
A black and white by Hubble shows more detail, less of the whole structure. Note the line of stitching along the lower right, as a spume of disturbed galaxy material on the north side of the stitch rises faster than material on the south side of the stitch, not a hint of the stitching is visible in the Hubble original, seen by clicking on the next image. Look to the lower right corner and up a bit diagonally a faint irregular line crosses upward to the right.
The Hubble image is rotated to the right by (a guess) about 20 degrees from the ESO view above, where cleavage into the valley is straight up, not over at the right. How Hubble managed to do this rotation is a bonanza for speculators who love conspiracy theories.
Click for ESO enhanced 1
Click for ESO enhanced 2
Click for Hubble original
VLT CAMERA LINEAL STRIATIONS AT M100
Lineal striations are also seen at M100, these on an opposite diagonal, taken at the same ESO telescope installation, suggesting digital scanning rastering as perhaps their cause.
Click here to see a small version of its original.
More M100 images can be seen here and here.
Click for enhanced small
Click for enhanced large
Click for original
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MAJOR CONTENTS MISSING IN COLLIDING GALAXIES IMAGE |
Colliding galaxies so vast, so conflagrated they burst right out of the picture frame when their true expanse is exposed by extra strong measures of enhancements.
Click for small original
Click for large original
Click for large enhanced 1
Click for large enhanced 2
The subject of the 'fish' colliding galaxies is covered here.
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OBVIOUSLY DISTURBED GALAXY OF UNKNOWN NAME |
An obviously disturbed galaxy of unknown name is well enhanced in the Dss 2nd gen (red) image, the galaxy (shown next) is not one seen in public lagoons and canals where public astronomy images are present.
Click for galaxy in original
Click for galaxy in enhanced
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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