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Some images show inserted ecliptic axis lines. Ignore white dots in these lines, the dots are stars captured when the dark lines were cut from dark sky patches and pasted into place elsewhere.
Mantles, coronas, and light halos around giant stars are rich in objects photographed in high resolution black and white Dss images through two separate (red, and blue) frequency filters (two unique indepentent images). The two, red and blue, are entirely separate images. Only a few red vrs blue images are specified in the following, a duality made more complex by dint of three separate Dss surveys in the 60's and 70's. The first survey, a precursor, produced blotchy images only a few used in this page. The third survey homogenized the deep field backgrounds so that little to nothing was seen in them besides the giant stars themselves. Most of the images next are from the second Dss black and white survey. Colors are false, added here by image editing to better highlight dim features.
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Tidal trios along more than one ecliptic axis passing through the center. In this Dss image there is a major discontinuity in radiance along the upper east side of the giant star.
Click on Betelgeuse image for full size
Click on Betelgeuse image for full size - earlier lower resolution Dss image shows tidal trios in different positions.
At the moment this Dss photo was taken, a gob with a small hot center is partially occluded by giant star Betelgeuse.
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Two coiled rounds in the solar wind field of giant star Capella.
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Objects of unusual shapes are gathered around giant star Sirius. The long axis of the unusual shapes point to the center of Sirus.
Click on Sirius image for full size
TIDAL TRIOS
Three objects is a row, the largest further out, may be locked in steady state figures (three in a row - largest furthest out) by tidal gravity forces in 'tidal' orbital dynamics, a tug of war accelarates the furthest out, which is then dragged back, similar for the other two tidals in a tidal figure, all three slingshotting each other then dragging back in a repeated steady state that evens out to a tidal lock of three in a row, the heaviest mass the furthest out.
Click on Sirius image for full size
No comment.
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In this Dss view of giant star Vega, ditrus in the form of islands, ovals, and coiled rounds surround Vega. The ditrus objects are scattered, with a bias to the west side of the image. Click for the large image to see ditrus details.
Click on Vega image for large details
Oval islands, and coiled rounds, at Vega. Oval islands have oblong hot centers whose long axis point to the center of giant star Vega. Coiled rounds have internal swirl.
OVAL ISLANDS
COILED ROUNDS
Stereo panel of the eight circular ovals. Inserted ecliptic vectors are focused through the center of Vega. A planet (solid black dot) is seen at the left edge half way down the tall image.
Dim descending trails indicate these rounds are on the move clockwise through thick unorganized nebula materials.
VEGA TWIN TIDAL TRIOS
This twin pair of tidal trios are stereo, that is,
there is vertical separation in elevation in orbital tilts between each
single member of a trio, however, the background texture is so touchy
it is hard to tell (in this case at Vega), exactly which tidal planet is
highest, which is lowest, in each if the the orbital tilt planes.
The twin strings lay across their ecliptic axis, at right angles to the vector orbiter signature to the center of the star. Most tidal trios lay parallel along their ecliptic vectors, each trio member's long axis pointing toward the star, though not necessarily at the center, an off shift consistent with a planetary disk of matter in orbit(s) around the star. Giant stars can have more than one orbiting disk.
At Vega, a pair of tidal trios are at right angles to the direction of orbit.
Thread from lint (artificial) is seen in a stark curve in the upper right.
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A partially occluded dark orb at giant star Regulus, tells us the dark orb is an orbiter, currently around to the rear nearly behind the east edge of Regulas.
There is a hint of a small moon in the two oclock position on the edge of the orbiting orb. A proto planet with a dark disk may explain why the oval further out has a bright center.
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Regulus - change in position of tidal trio between two different Dss plates shows orbiting. Change in shape of the trio's three objects, from rectangular to flapjack, shows the trio objects tumbling while working to maintain the trio in a lineal alignment straight out along an ecliptic axis.
In a straight line, the inner body is orbiting slower than it should, the outer body is orbiting faster than it should. The orbital slipstreams are not sequential, that is, the orbiting velocity times distance of the outer body is different than the ratio for the innermost body. Because of influence of the outer heavier body, the middle body is also in a zone outside the perfect fit of Newtonian gravity.
Click on Regulus image for full size
Slew perhaps an unravelled tidal trio - there are three objects, heads out right, long tails trailing toward the star, the tails not smooth containing an oblong energy transferring vortice near the middle object.
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Oval openings in strew at giant star Alpha Peg proove that slew is not randomly chaotic, slews can contain stringent engineering physics.
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Giant star Procyon has a surrounding field densly occupied with irregular oval and circular gobs. Small to large dark precisely circular objects are more likely established planets of different sizes.
Click on Procyon image for full size
Procyon has a rill system extending in short outsprays around the telescope's inner brighter light circle interference area. A telescope's light circle typically amplifies information within it's circle.
Click on Procyon image for full size
Click on Procyon image for full size
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Ditrus around giant star Arcturus includes strews, like flings of slime. The strews are substantially off angle to the Star's center. The off angled orbital trajectories suggest another star, unseen, is altering the Arcturus zodiac. In theory, the farthest end out of a fling is orbiting at a lesser rate, this should be pulling the flings apart and dissolving their lengths.
Click on Arcturus image for full size
Photon frequencies used in an earlier cruder Dss image show dense bright flings closer to the surface of Arcturus. The flings inhabit a crude central disk across the star's horizon.
Click on Arcturus image for full size
Material is thrown out by stars in slews, this slew is at Arcturus.
Two tiny planets (small dots) in vertical position off the lower left of the telescope light spike, are in the foreground transiting over Arcturus.
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BRIGHT FLYERS - amplified in the telescope light halo around giant star Alpha Andromeda
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CALLED 'RINGWORLD' - A FAMILY OF PLANETS IS IDENTIFIED AT ALPHA ANDROMEDA
A line drawn in, shows east-side west-side consistency, that is, ovals on the east side are in place concistent to be in a ring with ovals on the west side. The east side ovals are less bold compared to the lineal progressive order of the west side ovals.
In the large image, a small oval at the right within the star's halo is exactly in a lineup position to be a planet dimmed, seen in a rear orbit through the haze of the star's telescope bright light halo.
Because the string of ovals highlighted on the left side are so much bigger, and bolder seen, this suggests that we are looking at the ellipse of the disk, which, on the left side, is closest to the camera and therefore most free of any masking haze.
Click for large study image without highlighted windows
Large study image - small gobs are copious.
Notice, using the inserted line as an indicator, that the lineal ovals on the west side slope slightly away, toward the star, the same with the ovals on the east side. These slopes are entirely consistent with a ring arcing around the star, seen nearly on edge at a very shallow angle.
There is nothing in these Dss images which tell us if the gobs are merely dew on the telescope's front.
In the ring, larger ovals may be nearer in current circling in the disk, smaller ovals may be farther back in the disk, behind the plane of the star. Just a guess, a lucky guess I hope. The point is, nothing described in the above sentences is contradicted by anything otherwise seen.
The seeming 'ring' is also consistent with planets in a specific ecliptic axis orbiting very near the giant star. One, 'ring disk', or the other, 'tight orbits', system is revealed in the above grey image with the inserted line.
An actual family of planets in tight ecliptic orbit, or else in a ring system containing planets around the star, is seen and shown in detail. At least seven planets are firmly identified in this 'family' called Ringworld, in orbit around giant star Alpha Andromdeda.
The Ringworld family of planets can be seen in the Dss 2nd gen (blue) orignal plate. The bright 'flyers' imaged further above are easily seen in the Dss 2nd gen (red) original plate.
