Two (recurrant) strange circles at Capella     Strange circles at Vega  
GIC - PLANETS1 PAGE

YOU SHOULD HAVE A LOOK AT THESE - STRANGE CIRCLES AROUND GIANT STARS

FEATURED LINKS:       thugs mugshots     tidal planets     tidally distended planets     tidally extended planets     tidal rounds and tidal circulars     izar ringworld planetary system     double star mizar     comment on izar dss images     visible quarks at Betelgeuse     migration in orbit reveals aphelion     coffee accident splash pattern creates island ovals     Alpha Andromeda ringworld
    Part 1     Part 2     Special

  to bottom   PART 3.   ANNOUNCING 'TIDAL' PLANETS - IN ORBITS AROUND GIANT STARS

Giant stars featured are:   Aldebaran   Alphecca   Altair   Arcturus   Betelgeuse   Delboo   Izar   Mizar   Phi Persei   R aquarii   Regulus   Sigma Scorpii   Sirius   Vega


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Composite of two plate zooms - Ist gen image left (green), 2nd gen (red) image right (white).

Four tidal trios in orbit around giant star Betelgeuse. Each orbital structure has two tidal trios in synchronous positions on either side of the sun.

First learned insight is that rules for planetary orbiting around giant stars are not the same as rules determined solely from normal stars such as our Sun and planets.

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In the time frame between photograph for Dss 1st gen plate, and 2nd gen (red) plate, the tidal trio seen at left in the 1st gen plate, has mirgrated to a more aphelion position in orbit on the right side of the star.

The Betelgeus tidal trio migration in orbit, is explored in detail.

MIGRATING TIDAL TRIO AT REGULUS


Migrating tidal trio at Regulus. Details here 1 and here 2.

A discussion under qualifications addresses questions such as 'migrating objects', and ' orbital velocity reversal'.

WHY NO PLANETS ARE BEING SEEN BY WOBBLE

If large planetoid -aka- sundry object clumps, are orbiting stars on either side of the star's centerpoints, optical phase shift 'vibrations' in fractional degrees of star displacements looking for planets will not work.

When Jupiter is on one side of the Sun, then the other, our Sun will be seen to displace in space by a minute phase shift variance, due to the gravitational pull of Jupiter pulling the Sun to the East, then West, by slight degrees, as Jupiter orbits from one side to the other side of the Sun. This 'visualization' is standard astronomy proceedure. The wiggle of the Sun reveals the planet, ergo its orbital period.

If two Jupiters are orbiting the Sun in tidal locked array - one on either side of the Sun - no phase shift displacements can be seen, because of opposite equal pulls in two opposite directions upon the Sun. Science fiction movies have exploited the prospect of two Earths, one each on either side of the Sun, so that the second Earth cannot be seen its view blocked from us by the sun itself, and no wobble in the Sun's position is seen because pull of Earth1 cancels pull of Earth 2.

Thus, astronomers would conclude that NO planets are orbiting the Sun, because vibration cancels vibration, (and, in fact, astronomers have concluded this, that no planets are orbiting nearby giant stars, ignoring the possibility that vibrations cancel vibrations).

If several giant planets are scattered in orbits around all sides of a giant star at any given moment in time, no star vibrations can be seen.

The solution is to look for the 'planets' by other means then wiggle or wobble, such as by actual photographs that reveal the planets. Such photographs seem to be existing aplenty in the Dss archives of nearby giant stars.

When many sundry planetoid objects are orbiting a star, little to no phase shift variances can be seen, due to obvious logics in fundamental physics principles. The voidancies do not, however, rule out presences of sundry objects orbiting giant stars. The plain fact is, there are many, and many, and many, sundry objects existing around giant stars.




DIFFERENT TIDALLY BONDED SYNCHRONOUS ORBITS IN PLANET TRIO GROUPS


It seems planets can form tidally bonded synchronous orbits when locked in groups of three, each member in its own orbit, and at its own tilt, but all three revolving in a sustained trio around an orbital circumpherence, in a state of temporary gravitational tide stability.

Oblong and tube shaped planets are not an impossibility. Very rapid spinners with spin axis tilted along the orbital axis will be elongated assuming spins rapid enough. For that matter, the planets do not even need to be spheroidically coherent. A cluster of tube worms knotted at the center can comprise a planet if destructive forces striking them are fierce enough.

Tidally interractive planets are in three forms, distended (island ovals) extended (stretched into swaths), and mugs (two curved tubes face to face close together). When not tidally interractive, a planet can be spherical. Note that synchronous bound tidal planets occur in strings of three.

THROUGH THE GLASS QUICKLY

  Click image Regulus     Click image Aldebaran     Click image Izar     Click image Regulus     Click image Aldebaran     Click image Betelgeuse     Click image Vega     Click image Alphecca     Click image Betelgeuse     Click image Regulusn     Click image Aldebaran     Click image Aldebaran     Click image Vega     Click image Vega     Click image Altair     Click image Vega     Click image Vega     Click image Vega  

Notice in the above thugshots the following - three planetoids pairs in a single long string, and three planetoid pairs each planetoid side by side in a pair.

  Bound pairs at Aldebaran     Bound pairs at Betelgeuse  

SILLY PUTTY SHAPES

The above thugshot gallery shows objects transmuting, transfiguring, and transforming, in silly putty shapes as tidal planets in orbits around nearby giant stars. (Nearby means within naked eyesight or binnocular range around our own average star the Sun. Silly Putty means to say the planet's shape is never constant one day to the next, one orbit to the next. Tidal means the planetoid positions are governed by the actions of gravitational tides as three planets close to each other act together as one system).

Anyone who wants to still argue that these are, and can only be, image errors and plate flaws, can look again to the planet being occulted in the top image, and in a pale green image part way down, six rivets in three groups of two each, form a tidal trio along orbital ellipse tilt planes along an ecliptic axis line. How can you beat those odds.

TIDALLY DISTENDED PLANETS

Illustrated as well as any, by these planetary island ovals off the left hemisphere of giant star Vega.

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TIDALLY EXTENDED PLANETS

   

It can now be predicted by conjecture, that tidal planets extend in orbits not only sequentially outward locked in the synchronous orbit of tidal grip, but also vertically in separate elevations via orbital tilts.

The vertical tilt in orbits causing stacked laddering of tidal planets, need not be incremental, for instance not (O1+inc=O2+inc=O3). In 3d (merge the above image pair together to see stereo), the smallest tide planet is down farthest, and seems closest in to the star. The largest tide planet, in the middle position, is closest to use in an orbital tilt slightly raised up in our direction. The 3rd tidal planet proceeding outward, is down slightly in elevation height from the 2nd (largest) object.

This tidal trio at Aldebaran is similarly stacked vertically in elevation in an add hoc way.





I must freely confess that the 'prediction' indicated above was slightly off the mark (more than slightly, but basically correct). I had somehow seen in mind's eye driving to the grocery store and back, that the largest tide planet would be farthest out and highest up in orbital tilt, visa versa for the smallest tide planet.

It seems size has little to do with it (nothing to do with it), except, the largest member of a trio tends to be in the middle, in the nunber 2 position.

VEGA TWIN TIDAL TRIOS

This twin pair of tidal trios are stereo, that is, there is vertical elevation separation 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 tide planet is highest, which is lowest, in the orbital tilt planes.





The question mark, if you haven't caught on, is someone's nose hair in the film.

Tidal circular in Vega halo is a thug - two bound tubular planets in a close together tidal embrace.

   

Here is a larger view, showing three Vega 'thugs', two are clearly seen, the third lower center is blurred.

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Here is a tidal 'thug' pair further apart at Alphecca showing how the oval shapes become extended into vertical blood cell shapes when mutually locked together (in mono, seen as two tubes whirling around each other end to end).

   

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Click on image for large

In this Vega plate, other larger 'circular rounds' appear concentrated along the left side hemisphere. These seem like they could be related to tidal planets but perhaps spread out much more so, and, somehow, in a distinctly noticable bias in concentration seeming out of place there. Why there should be a concentration is not clear.

By clicking on the image immediately above, you will see nine circular rounds concentrated in a vertical strip down the Vega left hemisphere. This is an anomaly. Image error of complete unknown kind is one of the suspects for interrogation in the hot seat of heavy brainwork .

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Click for large red enhanced

Oh but wait a minute - the image error suspect has been told it is free to go, no longer a suspect. I have just noticed a total coherence in the larger circulars.

The initial pair in a line above, are lined on an axis in complete mirror image to the axis of the lower pair. Similarly for the middle to pair, the polar planar axis of one pair (above the plate's horizontal horizon, is the mirror image of the other pair immediately below the horizontal horizon.

This is news that is HUGE.

Also, the smallest member of each pair on an axis is inside, closest to the star. Such property management coherencies as this cannot go unnoticed. The coherent properties still do not explain how the group of eight is clustered to one hemisphere. That the cluster orbits as a whole in some self contained way keeps springing to mind as the little white rabbit in the brain leaps out, fleeing for its life.

Click for stereo panel of the eight circular ovals.

A fifth set of circular objects has been spotted, 15 degrees clockwise off the bottom center axis, this group has three objects in lineal order.

  Bound pairs at Aldebaran     Bound pairs at Betelgeuse  

Click for red enhanced with five axis
Click for grey original with five axis

Other Vega images are here




STRANGE CIRCULARS


  Bubbles around new massive star Mwc1080   Round circulars seem to be in the process of formation around fierce active star .... The rounds are not seen until the original image is very highly enhanced, when, then, nearby objects appear which have the very look and field of mysterious circular rounds seen at other large stars itemized below.

Strange circular 'rounds' are seen in the neaby vacinity of some large stars, and seem to be intrinsically involved in the star activities. Their shapes suggest a proto sphere, or perhaps proto disks seen face on.

For instance, left, will a 'stretch' pancake object like this at Beta Pollux, be a circular round when seen face on, or is it sausage shaped no matter which orientation viewed.

Enough circulars have been spotted for use in GIC (in Dss images), to declare that a phenomena is present.

Besides those shown near Vega further above, next are two more examples near another giant star, named Capella.

Next, left, a strange circular round at Capella, spotted at a 10 o'clock position in this Dss 2nd gen (red) image.



Another round (right) is also spotted, at a 5 o'clock position in the Dss 2nd gen (blue) image of Capella. This second round is either the same - migrated around to a 5 o'clock position during the time between the two photos - or it is a second circular round. Only a return for time-lapse photography at Capella will tell.

In either case, the second object seen at 5 o'clock in the other Dss image, is somewhat larger than the first seen in a 10 o'clock position. If it is the same circular, migrated, it is now closer to the camera, appearing, thus, larger, and, revealing an orbit.

Tidal trios can be seen in the Capella images. Tidal trios are explored aplenty in the immediate above link. Tidal Trios can also be seen in both of the next two links.

Click for 2nd gen (red) full size
Click for 2nd gen (blue) full size

I have also included the Capella 1st gen Dss plate so you can have a look at it for retrospect. The picture quality is very poor, not bright, the star halo itself very dull.

However two small dark dots close together in the 9:30 o'clock position (see left image) suggest a binary planet pair, and diffuse ovals (marked in a highlighted window) in the 6:30 o'clock position suggest planetoid objects orbiting through dense haze or dust. Also, several tiny white dots - one particularly bright on the star face itself, see right image - could be comets transiting across the star. Click for star closeup.

BETA POLLUX

Near Beta Pollux, in a Dss 2nd gen (red) image (left) is an irregular form which appears to be at least three objects merged in a conglomerate.

Objects can be seen infesting space around Beta Pollux in the Dss 1st gen image. More objects can be seen in the Beta Pollux Dss 2nd gen (blue) plate.

More strange circles are seen at Vega




DOUBLE STAR MIZAR

Next, zooms from Miza Dss 2nd gen (red), and at the right Dss 2nd gen (blue), plates. Each zoom shows planetoids clustered in a different area between the two stars.



Double star Mizar has neither tidal planet trios, nor planetoids coherently ordered in recognizable orbital disks. Instead, Mizar (the double planet) has planetoids ordered into select areas between the two stars comprising the Mizar double star system.

Mizar scans

Click for 1st gen enhanced 2

Click for 2nd gen enhanced 1 (red)
Click for 2nd gen enhanced 2 (red)
Click for 2nd gen enhanced 3 (red)

Click for 2nd gen enhanced 1 (blue)
Click for 2nd gen enhanced 2 (blue)

Click for 2nd gen original (blue)
Click for 2nd gen original (red)
Click for 1st gen original




SINGLE STAR IZAR


Outloud!
A bark of surprise!
A bark loud enough that a reliable witness elsewhere in the dwelling heard it and come to see, knowing that such barks never happen unless something extra-ordinary has just been seen.

A 1st generation of star Izar, shows nothing but a bright telescope light ring around a small star large in full sized mid screen. An enhacement jolt by me changed little. A second jolt of the same strong enhancing power still revealed little. And a third jolt of the same, executed with ruthless abandon, produced a trio of tubular tidal planets in a synchronous orbit, a complete surprise, ergo the complete loud bark!.

A perfect trio, in that their existence in midsts of totally black domain is unargueable, and, their existence adds one more find to a rapidly accumulating list of tidal planets (bound together as three in a synchronous orbit by gravitational tides).

A cross orbit planets check, showed nothing in the polar opposite orbit position to the trio of tides, however the 2nd gen (blue) plate shows three ovals in the right position to co-incide with the 3 tidals, assuming not much time has passed (hardly any) between photo shoots of the 2nd (red) and 2nd (blue) plates.

The next image is faked, three tidal ovals (upper right) copied from a Dss 2nd gen (blue) enhancement, are pasted into place opposite three tidal tubes (lower left) from a Dss 2nd gen (red) enhancement.

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There are oscillating hems within the telescope light ring halo of this star, indicating the star is oscillating. Oscillations in stars are featured in their own page, here.


Click for large zoom
Click for large enhanced 1
Click for large enhanced 2
Click for 2nd gen original (blue)
Click for 1st gen original




ALPHECCA

A pair of tubular swatches facing each other, a two-body object, similar to the same shape seen at Vega.

   



A thug in Vega (left), at Aphecca (right).

Click for 2nd gen (blue) enhanced (large)
Click for 2nd gen (blue) original





DELBOO

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A few ovals seen in the Dss 2nd gen (red) plate. The star is not actually oval. A chance incorrect value for height resulted in a nice looking picture - why throw it away.

Click for 1st gen original
Click for 2nd gen (red) original
Click for 2nd gen (blue) original




PHI PERSEI

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A few ovals seen above (click) in the Dss 2nd gen (blue) plate.

Click for 2nd gen (blue) enhanced (zoom)
Click for 2nd gen (blue) enhanced (large)
Click for 2nd gen (blue) original




REGULUS

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Regulus has been kind enough to give us our first glimpse of an occluding planet.

A very interesting eventing in motion, at giant star Regulus. Three broad swatches have migrated between when the Dss 2nd gen (red) and Dss 2nd gen (blue) photo plates were taken.

In the composite next, the (red) swatches are large and bold in the left hand view, the (blue) swatches have migrated counterclockwise, are smaller, a little further out, and have aquired bends, as they drop in orbit farther away behind Regulus.

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Click for large enhanced 1 (red)
Click for large enhanced 2 (blue)

No orbital counterparts for the swatches are readily seen (in these Dss images) in the orbitally opposite side of Regulus.

Click for 1st gen original
Click for 2nd gen (red) original
Click for 2nd gen (blue) original

Related important information is here, in a collaborating page dealing with a planetary host star named Fomalhaut.

TIDAL PLANETS

Perhaps the swatches are gravitationally powerful enough to keep each other lock stepped in synchronous orbits, that is, all three are orbiting in the same time, not velocity, with each object's period identical, even though their velocities must vary to keep the swathes lineally progressively cojoined outward from Regulus in synchronous periods of revolution. This would be a violation of Kepler's Laws though not a violation of physics.

Except, not a Kepler violation. If fierce gravitational tides between the three bodies stretch each body out to compensate, in this case, the physics equations description for these 'swatches' (gravitationally streched tidal planets), would include terms for spherical radii as a control factor for how much stretching by tides is reguired for the three, as a group, to attain synchronous orbits. (At age 40 I could have probably done the tide stretching equations. At age 63 with my only powerful enough calculator in pieces in a plastic bag, I have not the brain cells or other elements necessary to go ahead and do the equations. Therefore, you do them, see if synchronous orbits for two or more planets can be achieved by mutual stretchings in mutual gravitational tides).

Noticably, the swatch closest to the star is smallest, the swatch furthest out is largest. Is this consistent with fierce gravitational tide forces causing synchronous orbits of stretched out giant planets. I don't know. I sure hope so, for the sake of better rather than bad conjecture. A basic rule is that the larger is probably closer in a tidal orbit.

I have no way of knowing just by inspecting these images, if the migration of the swatchs has been right to left, or left to right. Clearly, however, if indeed migration due to movement in orbit(s), the swatches in the left panel (red) are swung around closer to the camera, more out front toward us.

Whereas, the swatches in the right view have moved down, closer in to the central vertical star axis, have dropped down, and have diminished in size, all events consistent with objects now gliding around the rear ellipse of orbit and are receeding on the rear outswing of the orbit(s) to soon disappear down around behind the star, if counterclockwise revolution is in effect. If not, see all motions and object shifting in reverse, that is, the objects just coming out from behind the star (right view) are now swinging forward toward the high point of the orbital ellipse(s).

The above paragraph confirms a well known Murphy's Law, that descriptions tend to complex exponentially with each extra item to describe a lockstep with the fewest known facts. Fewest facts descriptions tend to be like dragging black holes along through the description.

Click for large enhanced 1 (red)
Click for large enhanced 2 (blue)

Click for 1st gen original
Click for 2nd gen (red) original
Click for 2nd gen (blue) original




BETELGEUSE

A cluster of 3 tidal stars in the lower left, matched by a tidal-planet cluster on the opposite side (right) indicates an orbital shell disk. Another cluster of 3 tidal planets further up nearer the centerline, is matched by small ovals in sequence in the left below the horizontal centerline. This means we know there can be more than one trio in an orbital ring. And, the parety polarity of each trio shifts, as each group of three wings on around the star.

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Click for full enhanced large
Click for original

These add to the accumulating account of large planets stretched out along the circumpherence of orbit by interactive gravitationally tides (ergo tide planets), keeping the 3 each group in synchronous orbit, as first identified above in studying orbiting objects at Regulus.

The 2nd gen (red) image has a tidal trio, as shown. Nothing on the left side of the star is seen to match the trio.

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Click for large zoom

Click for full large

A strong show of drop-shaped ovals in the lower right of the Dss 2nd gen (red) plate, is not clearly met by bodies orbiting in a proper position on the opposite side of the star.

The green enhancement in midscreen above, shows the strong show of 6 ovals in 3 sets of two each. Click on 'large' and see that numerous objects can be dimily seen in the upper right, perhaps there is a lot of haze and anything up there that is orbitally consistent is in the rear, masked by overlaying haze.


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Click for large

DSS 2ND GEN (BLUE)

In the Dss 2nd gen (blue) plate, a polar plane pair of orbiting ovals, each a group of 3, each on opposite side of the star, seems in a disk aligned along a North/west, South/east, ecliptic. Another show of lineal ovals is below, but this planetary string if a planetary string) is not in handshake above the star in the right field area, there seems nothing out there to be seen that shouts "the other planets".


VISIBLE QUARKS

Tidal trio groups of three are eerily close to 'quark' sets in elementary particles. For instance, Protons, classed as 'Baryon Hadron' particles (hadrons having 1/2 units of spin per particle, baryons having 3 quarks), might be in image here at Betelqeuse.

If images here at Betelgeuse are correct - that elementary particle wavelength harmonics can be modelled by solar system planet formations and distances apart - then Betegeuse should in like kind, be showing us some things about 'quarks'.

Unfortunately, these Dss images do not show us exact tidal trio radii, which are necessary in understanding if radial distances from a parent star, and radial separations between each entity in a tidal trio, match the Compton wavelengths of known elementary particles and their higher energy resonances, regards Baryon quark trios. Of interest would be, in terms of quark trios, (+ or 0 or -) charge states for a particle, and 1/3, 3/2. 5/2 spins, etc., resonance states of a particle.

Click for 1st gen original
Click for 2nd gen (red) zoom
Click for 2nd gen (red) enhanced
Click for 2nd gen (blue) enhanced
Click for 2nd gen (blue) original
Click for 2nd gen (red) original

ORBITAL MIGRATION OVER TIME REVEALS ORBITAL APHELION

If trios are in orbit, they would be migrating over time, and this is exactly what is seen between the time the Dss 1st gen plate was taken, and the Dss 2nd gen (red) plate was taken.

A first image next shows a trio of three oscillating saddle shaped objects in a left side position near the star in the 1st gen plate, in the 2nd gen (red) plate composited at right the trio has migrated to the opposite side of the star, is further out, and the saddles have re-oriented spin axis positions to appear more stretched out and smaller, indicating being further away as well as further out from the star.

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In closeup, the saddle shaped trio objects at left from the Dss 1st gen plate, and at right the trio migrated to the other side of the star in the Dss 2nd gen (red) plate.

  Tital trio (saddle shaped) orbiting Betelgeuse     Tital trio (saddle shaped) orbiting Betelgeuse  

  Tital trio (saddle shaped) orbiting Betelgeuse     Tital trio (saddle shaped) orbiting Betelgeuse  

  Tital trio (saddle shaped) orbiting Betelgeuse     Tital trio (saddle shaped) orbiting Betelgeuse  



Everything about the layout of the migrating trios confirms an orbit, that is, on the right side the trio is more spread out indicating an aphelion of a highly eccentricic orbit, and being smaller indicate the aphelion edge of the orbital ellipse is in rearspace, in a plane out to the right and behind the star.

In fairness to physics logics, it cannot be said that the trio in the left hemisphere is in the perhihelion position of eccentric orbit, but certainly the trio appears closer to us. For that matter, it cannot be said that the trio in the right hemisphere is in aphelion position, but certainly, it is an ellipse edge that is further out, further back, and the trio of objects is more spread out.

Until proper stereo rendering of these objects is possible on large screen, the parallax factor regards just what angle and just what view plane is in our view, left side vrs right side, is a hung up telephone long distance call.

Saddle shaped objects such as the above 6 - three repeated in two orbital positions - are difficult to picture in terms of what each object actually might look like close up - certainly they might not look like Jupiter or Saturm.

A polarized view of the Crab Nebula (by Malin of Australia) shows similar saddle shapes. This does not necessarily extrapolate to the saddles of Betelgeuse, on the other hand perhaps strong or even intense polarizing fields at each object is distorting their light reaching us, into polarized intensities forming the tidal trio's 'saddle' seeming shapes.





Numerous tidal trios are seen in the Dss 2nd (red) plate. Most all of the groups in highlighted windows in the next view are trios.

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VEGA

Two groups of tidal planets, each a characteristic 3 object trio in elongated shape, stacked one before the other (synchronous orbits) are seen in giant star Vega. These two tidal planet trios are each also stretched in a line side by side (orbiting necklaces - each of the three is trailing along in the same orbit behind another).

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Therefore, two fundamental orbital modes are demonstrated visually in view. The image is an enhanced version of a Dss 2nd gen (red) plate of giant star Vega.

Gravitationally adjusting tides may have created two sets of synchonous orbits in Vega, in this case, a string of three swatches following each other in a row like beads of a necklace, and a short jump further out another string of swatches following each other in a row like beads of a necklace.


Vega has many long strong planetary ovals in surrounds out to a very long distance.

There may be more than one multi-planet ringworld in orbital disk.

One orbital disk can be shown by an inserted axis. The disk starts in the upper left with a chain of ovals, on the other side of the star a number of ovals are seen, falling on both sides of the inserted line. The upper chain is curved slightly one way, (consistent with the ellipse of a disk), the lower chain is slightly curved in the opposite direction (consistent with being the opposite side of the disk's ellipse.

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A second axis is inserted, at an opposite slant, underscoring two opposed island groups of just a couple of ovals each.

PLANET NECKLACES

I am suggesting that the occurrence of two sets of three ovals, each in a line at odds with the sun-focus axis of orbital radii, could be planets in the same orbits following each other around like beads in a necklace. Each orbit necklace of three is in its own orbit.

The above three images are from the Dss 2nd gen (red) plate for Vega.

I have to confess in having had some (conciderable) difficulty in landing the inserted lines exactly where I wanted them, no line actually fall exactly into place. Secondly, lines would click off out of action before I had moved them into best co-ordinates, and thirdly in the middle of my master composition a spurious vertical line appeared. So I just left it. Then after over a dozen attempts to land one of the canted lines I gave up and just left it too, in fact both canted orbital axis indicator lines are not exactly where I wanted them.

And, not liking that last paragraph I went back and spent 3/4 of an hour composing another version which I think is the best there will be from me.

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NEXT

Here we see that ovals identified in the highlighted window are uniformly pointing away from the star, straight to the two sets of necklaces in the lower right. It means the anomalous point direction has meaning if these anonomously pointing ovals in the upper right are involved in the same orbital disk as are the two necklace groups.

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All other ovals seen in this Sirius image are small, and unformly pointing to the center of the star, as exampled by a few seen in the dim medias beyond the highlighted window.

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Vega's Dss 1st gen plate is interesting. The large shell of an oval looms in from the left. Several dark sinkholes of unknown kind are noticed. Ovals and gobettes pepper the whole region right out to where it gets dark, all of the objects without round shape are pointing to the center of Vega.

Vega's Dss 2nd gen (blue) is different than the 2nd gen (red) in having hordes of ovals all facing the star center, but also, peculiar large rounds are concentrated in the left hemisphere near and inside the bright star area, what these circular rounds are anybody's guess, mine is perhaps planets with moon systems or bright disks akin to Saturn, perhaps however these disks may be more like hordes of astereoids rather than thin films of disky dust. But, in truth, my best ten cent bet is that these are tidal round (planetoid pairs) which have concentrated momentarily in an orbiting cluster on the west rear side of Vega.

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A small thug is seen in the Vega halo, to the lower right. Click on large. Thugs are two planetoids which have come together and orbit each other like two hemoglobin cells nearly together.

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Thugs are seen in the above sequence of mugshots.

TIDAL ROUNDS AND TIDAL CIRCULARS





The question mark, if you haven't caught on, is someone's nose hair in the film.

Myserious large rounds are mysterious. Three familiar rounds lower in the left are familiar, these are tidal pairs (rounds) when two ovals come together or at least attain a systained two body faceoff at very close quarters, almost merged.

Tidal circular in Vega halo is a thug - two bound tubular planets in a close together tidal embrace.

   

Click for round circulars and tidal rounds (large)

Another tidal pair has been spotted in the halo of Alphecca.

  Click image for large  
Click on image for large

In this Vega plate, other larger 'circular rounds' appear concentrated along the left side hemisphere. These seem like they could be related to tidal planets but perhaps spread out much more so, and, somehow, in a distinctly noticable bias in concentration seeming out of place there. Why there should be a concentration is not clear.

Click for large with axis lines 1
Click for large with axis lines 2
Click for large with axis lines 3
Click for large without axis lines 2
Click for large original Dss 2nd (red)

Click for large enhanced Dss 1st gen
Click for large original Dss 1st gen

Click for large enhanced Dss 2nd gen (blue)
Click for large original Dss 2nd gen (blue)




ALTAIR

Two groups of three objects in a Dss 2nd gen (blue) plate. A trio of 3 tidal planets, well stretched out, are in the lower left. A group of three round ovals is in the upper left.

  Click image for large  
Click for large

Regards 'tidal' planets. No one ever said planets had to be perfectly round, or pumpkin. Picture a rubber balloon filled with water and hurtled through the air. It wobbles and slogs, oscillates and bobs, the more is the throw off canted from center thrust, the more the slosh and elongated stretched out flogging in the gob of water contained in the oscillating balloon.

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ALDEBARAN

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A matching pair of tidal planet trios. Three long thin tidal planets are in synchronous orbit in the upper right. In polar plane opposition on the other side of the star, it looks to be the ellipsoil far end edge of a disk, in a deep 'U' with tidal planets, small and far away seeming, on both prongs of the 'U'. This meets criteria to be the same orbital plane as for the upper right tidal trio.

If the second string (upper left) are 3 tidal planets in a synchronous orbit, there nothing visible on the opposite side of the planet (lower right) that would meet any criteria to be in related orbit. The worms in the upper right, if they are tidal planets, are (it may be possible) in the process of being torn apart, slingshotted further out?, driven further out by hoary solar blasts?. Slung by their own velocities as 3-way tidal synchronous grip suddenly let go?.

A trio of oval pairs, forming a synchronous orbit structure with subset, that is, instead of one object at each gravitational tide point, there are two close together as if each on either side of a tide line.

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In each of the pairs, the larger appearing member is higher up in tilt elevation than the smaller, and each larger is farther away. Mechanic properties regards synchronous orbit tital planets, are starting to accumulate in a text book list.

It seems now established without doubt, that for gravitational tide synchronous orbiting structures to occur, that three bodies are required, and that the synchronous gravitational tides grab the three in orbits that are separated both by small increments horizontally, and also by small increments in vertical tilt. The concentric rings around a conally expanding sound tunnel can give a quick mental model if first having difficulty with the concept.

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SIRIUS

Other gobs, other planets, seen in one but not another Dss generation plate of an image, is not uncommon, and not to be unexexpected. In giant star Izar, a fully evolved Ringworld planetary system is seen in a ringworld orbit around Izar, the lower left planetoids seen in the Dss 1st gen plate only, the upper right planetoids seen only in the Dss 2nd gen (blue) plate.

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For Sirius - oh sob Sahebe - the nearest and largest brightest star in the sky, there is no Dss 2nd gen (red) or 2nd gen (blue) image plates. Oh how I would like to see if island ovals extend into the upper right quadrant in orbital positions opposite to those big gobs flailing away out in the lower left quadrant in the Dss 1st gen image.

The little monkey in the cage in a different brain region than the little squirrel, starting going owoooot! woooot! woooot! so, I went back to the Dss site, and downloaded the 2nd (red) plate under the co-ordinate name 'Sirius b'. Nice surprise that the higher level plates were there, under a different set of call letters.

Nowwwww, I can tell you what I have found in toto at Sirius.

Okay the 1st step is backward, here is the famed Dss 2nd gen (red) platge in which the janitor who did not have enough money yet to patent, put a amateurishly trimmed piece of cutout paper over the star to factor its image, proving the patent was a valid idea.

The last step ended in a bummer, however, as the little monkey in the cage ran out of hot poop. There is no Dss 2nd gen (blue) scan, either under 'Sirius B', or 'Sirius A', or 'Sirius'.

Now down to serious business.

Very large swatches are missing their third partner to complete a tidal trio. It seems there should be three, in keeping with other tidal trios. If wish turned to granted, there could be a trace of the third, lower down, partially masked by a small bright star shining through it. It can hardly be read, it is either the third, or imps of eyesight playing impish wish urges.

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Island ovals are everywhere around the star though those readily visible tend to be on the left side indicating extreme eccentricies perhaps sustained in synchronous geocentric orbits by the pumping action of the second star.

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Click for Sirius enhanced 3

Click for Sirius 1st gen original
Click for Sirius up 1st gen original
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Click for Sirius left 1st gen original
Click for Sirius right 1st gen original




DOUBLE STAR MIZAR

Mizar is an interesting situation. There are planetary ovals, most are concentrated between the two stars, suggesting a gravitation null grip in a Lagrane point area.



In the Dss 2nd gen (red) plate, the ovals are seen concentrated within an area that lies inside the bounds of the big star's light shell.

In the Dss 2nd gen (blue) plate, a different concentration of ovals is seen this second cluster concentrated in an empty area just above where the two star's light shells touch.

See this click for more information on the nature of telescope light shells which surround bright stars, and how the light bending causing the shells is also secondarily amplifying information inside the shell.

Click for 2nd gen (red) original
Click for 2nd gen (red) enhanced
Click for 2nd gen (red) enhanced

Click for 2nd gen (blue) enhanced 1
Click for 2nd gen (blue) enhanced 2
Click for 2nd gen (blue) original

More Mizar views are looked at here




SINGLE STAR IZAR

IZAR RINGWORLD PLANETARY SYSTEM



Here we are, another planetary ringworld system, this one around giant star Izar. This system is bifurcated. It is seen in two different images, one part in one image, the second part in another image.

The 1st gen image shows a lineal string of irregular ovals stepping out from the center shell into the lower left. Nothing at all is seen in the opposed upper right.

The 2nd gen (blue) shows large strong ovals progressing out in the upper right, and nothing is seen in the lower left.

Paste and copy a merged version of the two separate image states, and there are the planets in an orbiting shell. Perhaps. The great godmaker known as human does not like inserts from another's trains - there may be two oribital systems, but the likelyhood is high that this is one.

Click on image for full size

COMMENT ON IZAR DSS IMAGES

The intrinsic media of the 2nd gen (blue) image of giant star Izar is very weak, requiring unual degrees of enhancements to fully bring forth a show'n'tell at his star. Many small gobettes are seen particularly to the lower left of the central star shell. Three very large ovals in a progressive sequence, with, nearby, a second progressive sequence of smaller ovals, suggests two planetary rings, in two separate orbital shells around the star.

Click for 1st gen original
Click for 1st gen enhanced
Click for 2nd gen (blue) enhanced 1
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Click for 2nd gen (blue) enhanced 3
Click for 2nd gen (blue) enhanced 4

More Izar views are looked at here




SIGMA SCORPII



Scorpii, a giant wisp covered cloud in the Antares group in the Pipe Nebula, has just a few indications of planet activity, either because main shows are covered in wisps, or only a few gobules of tiny size inhabit Scorpii's corona. A tiny dark dot highlighted in the halo may be a planet (thought perhaps a planet because it is diffuse dark and not solid dark as would be seen if merely a plate flaw.

For instance to the right in Sigma Scorpii Dss 2nd gen (red), a large solid black plate flaw is an obvious no brainer (if you can find it).

Further to the right, and above the centerline, an anomalous long streak has been highlighted in yellow. The streak bends at its upper end, ruling out a satellite track. There are two short re-appearances of the streak further down. It looks at if something strong in the way of a lazer coherent ray is firing through diaphanous matter drifts, appearing, disappearing, and reappearing again. But nothing is ruled out by the image that makes this long thin anomalous streak a false positive (fake).

A dark dot (shown in blue, to the right of the main star, in the 1st gen image), seems to be overlaying a star behind, in which case a black solid dot such as this is concidered a plate flaw (error in the image).

Click for 1st gen original
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Click for 2nd gen (red) original
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R AQUARII

This very strange tangle turns up in a Dss 2nd gen (red) plate of R Aquarii, the object is small at the center of the plate and is a photo of a star of that name.

1a

The object has the look and feel of rilldisks (which are thought to be proto planet disk arrays forming at long distance around stars.




ARCTURUS

A huge dark hole is found in the Dss 2nd gen (blue) plate of giant star Arcturus, the hole is shown highlighted near the centerline at the bottom. Many small island ovals facing the star, are seen in the dim surroundings.

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Dark holes are a subject of their own page.

Click for Dss 2nd gen (blue) enhanced 1
Click for Dss 2nd gen (blue) enhanced 2
Click for Dss 2nd gen (blue) original
Click for Dss 2nd gen (red) original
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  Saturn-like, by artist  

Click for detailed description of how confirming clues accumulated into a picture of a ringworld family of planetoids in a disk around nearby giant star Alpha Andromeda.



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