AT GIANT STAR CAPELLA


Chortles - round, tapeworm coiled inside - orbiting giant stars





Focus two images together to see some stereo, which is enough to reveal a none smooth, none round, none flat surface

Not enough is known about chortles to describe this item in real terms, other than that a square oval is an unusual shape for any solar body, and these may be transitory, with brief lifetimes

It may be possible we are looking at two separate chortles, formed one then dissolved then another. How this may be possible is suggested in insight by a star's rotating powerful magnetic field downloaded from an unrecorded internet site

On the other side of the coin, is proof that chortles can also be resident as tidal objects in radial orbits (radial orbits extend straight out from a star like spokes of a bicyle wheel, festooned with fixed beads along the spoke - the outer bead rotates around on the wheel at a faster clip than the inner bead)

MORE CHORTLES GALORE AT GIANT STAR VEGA

Six chortle events festoon six spokes of a bicycle wheel revolving in radial straight lines out from Vega


Four chortle sets are pairs, outer larger, inner significantky smaller. The lower two sets are tidal trios which have two beads split in the middle by dogbones (an entirely different object somatotype). Each of the 12 chortles is round, none are square

Click on the above image to see chortles to correct scale in the universal deep space reference frame recorded by Dss telescope focal lengths. Shift image to the right to see the chortles

Dogbone is in the middle

The Vega chortles are detailed further in the Trios.htm page

It is possible to suggest the chortle is in orbit, because six different sets of chortles are in orbit around giant star Vega

The Vega chortles are seen in a Dss Poss2 plate

There are four sets of a pair of chortles in each set, in space on a radial orbit axis vectored to the middle of Vega

Two dogbones in the Vega halo

Two other chortle sets occur in tidal trios of 3, split in line with a dogbone in the middle


If not already investigated by astronomers, this proto disk will make a prime candidate in that it is (though small) well seen in a poor quality archived black and white Dss plate. Imagine what it might reveal when scoped by a super duper telescope. (There is possibility it is a nebula (exploding star))



EXPLODED COMETS

One stray thought drifting through consciousness half awake - half asleep - is chortles may be exploded comets. A comet has been said to have a head 50 to 500 miles in diameter through a wide range, one of these big ones close enough to a giant fierce star to overheat fast more than its cohesive binding can handle can explode, leaving a chortle as a signature of its former existence. Even on Earth, meteors can explode with violent disinvolvement when impacting the atmosphere at too high a velocity. Why not comets at giant stars. Sure, then, to sleep, then to awake to think again remembering, this time, words are the result. Speculations are cheap, worth more than penny when correct

At Capella

A comet was occuring (near horizontal light spike) when the photo with the proto was taken



Three more comets close together are crossing the face of Capella in another plate



In a Dss Poss1 plate, 6 comets are seen at once at the same time crossing the face of the giant star Capella



At Pollux



Planets (dark) comets (white)

Back to Capella

Tidal trios are plentiful at Capella



A trio upper left (blue grey) and in olive lower right a trio with two ovals and whose third member is a planet

Tidal trios is the subject of its own Trios.htm page

Tidal trios are a very big subject, well over 100 have been documented at giant stars

At Capella in infrared large planets giving off heat have been captured on film in distinct furry profiles



A tiny planet is seen up in the disk, along with a comet

AT OTHER GIANT STARS WE FIND


At Canopus, a large oval with fringe



At Alpha Cassiopeiae

Over at left image, an unusually large oval with a fringe (shown to scale) is seen in Poss2 red filter at the top in a downshifted declension view, click for large plate (the oval's location shown in silver - the object is officially known as Lkha 198

Above, at Alpha Cassiopeiae, obviously a celestial artifact, a star may be superimposed giving an odd indent extra that is not real, except, no pure round (a star) the bright hottie seems to be on the edge of the deep dish oval. Click image for large picture, (the luminous bird bath is at lower left). Three tidal trios are dimly discerned in the musks of the star's solar surroundings

An extra large island with inside light halo, either crossing a superimposed star or a bird (hottie) is on the edge, in either case it is not plate flaw assuming Cassiopeiae's halo would have no effect on a media matter in the plate itself


At Lambda SCO

Peculiar object near star, could be a plate flaw however irregular glowing edge is furred not stark, suggesting a barnacle shaped nebula


At Mizar



Image of dim tidal trio comprising three small ovals in a straight line, between two stars - seen through obscuring lens light interference prooving these ovals are celestial reals in radial orbit at Mizar (bigger star at right)

Poss2 UK photos characteristically have twin lens spikes shooting out long distances in the four compass cardinal points around the star. Poss1 UK plates from another deep space sky survey, characteristically have only one spike comprising the compass four point cardinal lens artifacts in the images of bright stars. In the blue toned view of Mizar above, the stars have twin light spikes


Is this, at Alpha Phoenicis, a dark sinkhole?

Poss1 UK plate of Iota Ceti has in view a sinkhole which seems similar to well known large cold sinkhole (lightless molecular cloud) named Barnard 68, and what appears to be a colliding galaxy situation with longarms. Click on grey sinkhole for large overview




AROUND GIANT STAR CAPELLA - A WHOLE NEW CLASS OF PLANET ORBITER

Any begrudges that planetary orbiters around stars cannot be found by simply viewing old photo plates can be instantly put to rest by the following find - as said as succinctly as possible - What A Score!

Put simply, a huge pancake of indeterminate matter and planetary sciences has migrated, from one photo, to the other side of the star in a second photo taken at a different time.

Note that there can be no doubt of planetary orbital migration, the object is topologically the same (square circle) on both sides of the star. The fact that the object is square cornered is rough stuff for very accute physics theories to come from this important planetary mechanics discovery. This is a whole new class of star orbiter.

The object is the size of a star, but definately is not a nuclear reactor. What it is, is your domain to discovery. All I can do with my puny IQ and techniques is point it out. Let's just say very deft creative enhancing techniques 'a la a moi' make it much easier to point it out, plus a curiousity that probes far out in left field leaving dogmas and preconcieved beliefs behind in dust. This kind of curiousity definately helps to justify hours wasted in fruitless efforts looking out in the left fields of astronomy. Those long hours add up.

However, I have come to trust intuition. I do not waste time unless I am secure in knowing that inevitably someday something will turn up making the hours worthwhile. This orbiting meat patty certainly fills the bill for adding up to something worthwhile, found. (That intuition would not let go, I kept looking at every single star name I could find. Then one day recently, a star map of Orion stars with a few names I had not seen before. Capella was one of the names). History complete.

A large gob of diaphonous matter in a rough shaped loose sphere is in orbit around giant star Capella, which is in the Orion constellation. Capella is estimated at 20 times the mass of the Sun, the shape has changed noticably during its period of orbit

Two Dss Deep Space Sky Survey photos one 'red', one 'blue', from the Poss1 Ukstu survey show the orbiting gob, in a orbital position in the upper left near the star in the red filter photo, and again in a blue filter photo, across the star in a lower right position near the star on the other side of orbit. Blue was chosen to show the red filter position only because the object's details showed up more clearly in blue enhancement, and visa versa for the object shown in pink Click on image for full size The gob appears larger in the right side position, meaning it is closer to us in orbit, in a current orbital position forward from the star at the moment the blue filter black and white Dss photo was taken The two colors, blue, and pink, have been arbitrarily chosen to reveal more details in enhancement. The original Dss Poss1 plates are black and white The nature of the gob is unknown. It is too large to be a planet (say, of Jupiter size)

Gobs of this kind have been spotted (by GM) hording in a school around Vega. In this instance the diaphonous gobs are visible clustered on the west side of Vega. It is assumed others (if in orbits) may also be in the farside, that is, the east side but perhaps further back obscured by dusy haze which surrounds giant active star Vegus. The plain fact is that none others can be seen in any enhancements

CHORTLES AT VEGA

Two zooms enhanced, showing the eerie circles

Click for 3rd zoom in which the gamma correction (density) was reduced to darken thus make more visible the chortles




Notice the two dogbones, (enhanced in magenta the dogbones could barely be seen in dark dim media in the original)



This distorted dogbone is in a Dss infrared image of Vega. A dot on the face of Vega may be a planet in transit





Giant star Alnitak here. Objects such as these are offered as planets in transit across the face of the star. Traditional wisdom holds that the odds of a planet spotted crossing a star in transit are extremely remote at best, due to tilts and lineups in co-incidental perfect line of site along ecliptic axis, all lucky strikes are required etc

Leading edge wisdom suggests that if the star is surrounded by planets in quantities approaching a horde of hornets whirling around in different tilts including polar orbits, with no single clearcut ecliptic, transits (even multi transits) across the face of the star will be, ho hum, routine

Click on image for full size



Each of the rectangles has a hard dot of planet scale. The Flame nebula is at the left, the snout of the Horsehead peaks up from the bottom edge. This 60x60 arcminutes picture is of a small area of Orion

The big superscoop on teeming planets orbiting the spacescape of giant stars is linked directly here in the Trios.htm page

EERIE CIRCLES AT FIERCE STAR MWC1080

Every so often I do an enhancement that reveals startling content in an otherwise non startling image and this (next) is one, of fierce giant star MWC1080, an enhancement reveals ovals more or less of exact similar kind to those shown above for stars Capella and Vega. I have not been able to recreate the MWC1080 enhancement a second time

More Mwc1080 in the Special.htm page



It is not possible for an ordinary PC Windows image graphic editor to input content of such articulate nature, in other words the content is in the image. Where, in the image, I cannot say. I have not been able to bring forth again the ovals a second time. Yet, since the ovals are apparent in the image, I am showing them here, head bowed, just slightly. GM.

2 TIDAL TRIOS AT CAPELLA



Click for large view



OTHER INTERESTING OBJECTS AROUND CAPELLA

Click for large



Click for large



These may be two planets close together on the west side of Capella, seen in a very dim Dss Poss1 image



CAPELLA TIDAL TRIO ZOOMS

Two tidal trios requiring very high enhancement to see, in the upper right region around Capella



Two more tidal trios, in the south region below star Capella, also impossible to see without very high image enhancing. The trio in green is a straight line, another oval more clearly seen nearby to the left of the 3rd oval out in the trio's string



A tidal trio at Dubhe, vectored south/west from the giant star Dubhe offscreen to the right. A very dim object of indeterminant kind has been included (at bottom as a record of its present photo existence)

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