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   The background image of this document features star formation in the Orion Nebula as captured by NASA

   Summary::

   The heavenly power organizers are nebular organizers; in the realms of their spatial presence they are capable of initiating colossal cyclones of force which - once set in motion - can never be stopped or tamed until the mobilization of the all-pervading forces necessary for the ultimatonic units of universal matter to arise. Thus appear the spiral and other nebulae, the star-forming disks, directly giving rise to the suns and their diverse systems. Ten different types of nebulae can be observed in outer space, representing stages of primordial evolution of the universes, and these vast energy disks (or vortices) had the same origin as those that gave rise to the seven superuniverses.

 

   Nebulae differ substantially in size, number and combined mass of their stellar and planetary progeny. A star-forming nebula north of Orvonton's borders, but within the spatial plane of the superuniverses, has already produced approximately 40,000 suns, but this star-forming disk continues to eject suns, most of which are many times the size of our luminary. Some of the largest nebulae in outer space spawn as many as 100 million suns.

 

   Not all spiral nebulae are involved in solar formation. Some have retained control of many stars, and their spiral shape is explained by their suns emerging from the arms of the nebulae in a narrow array, but returning by different paths, so it is easy to observe them in the first case, and more complicated then , as they return to the nebula, scattered over vast distances by its sleeves. There are currently few active Sun-forming nebulae in Orvonton, although Andromeda, which is outside the habitable part of the superuniverse, is very active. This distant nebula is visible to the naked eye, and when you observe it, consider that the light you see left these distant luminaries almost a million years ago.

 

   The Milky Way consists of a large number of former spiral and other nebulae, and many of them still retain their original configuration. But as a result of internal catastrophes and external attraction, many of them have undergone such deformations and rearrangements that these huge clusters resemble giant luminous masses of bright suns like the Magellanic Cloud. The globular appearance of star clusters dominates near the outer limits of Orvonton

 

   The vast Orvonton star clouds should be viewed as individual clumps of matter, comparable to the individual nebulae that can be observed in the spatial regions beyond the Milky Way. But many of the so-called star clouds of space consist only of gaseous matter. The energy potential of these stellar gas clouds is simply enormous, and part of it is absorbed by neighboring suns and redistributed into space in the form of solar radiation.