STAR AND GALAXY BIRTHING , LIFE SPAN, AND DEATH SPRIAL

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    • THE LAW THAT CONTROLS ALL PARTICLE INTERACTIONS IS THIS:
    • ALL THINGS ARE TRIUNE, WITH BINARY INTERACTIVES.  THIS IS THE LINKAGE BETWEEN MATTER AND FORCE CARRYING PARTICLES. THE LINKAGE BETWEEN THE PARTICLE ZOO IS CONTROLLED BY FERMIONS AND BOSONS. 
    • THE REALITY OF HOW LIFE FORMS CAME ABOUT ON THIS REMOTE BLUE MARBLE IS THIS:  THE EVENT ORIGINATOR WROTE THE CODE, PRODUCED THE BLUEPRINT, AND USED AN EVOLVEMENT PROCESS TO OBTAIN THE REQUISITE RESULT.  IT’S ALL JUST A BINARY SOFTWARE PROGRAM.
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      • Symmetry is the causal structure built into the creation module.  The creation module has a two-way arrow of time that is built into it.  All current information is always passed back into the versatile storage unit.  These informational totals can’t be changed or deleted.
      • The closed subatomic quantum system is a duplicate of the macro quantum system.  The two systems interact on a binary basis.
        • CONSCIOUSNESS CREATES SPACE/TIME.
      • Every symmetry of physics laws leads to a conservation law, and every conservation law arises from a symmetry in the laws of physics. 
      • Symmetry is the casual structure built into the creation module.  The creation module has a two-way arrow of time that is built into it.  All current information is always passed back into the versatile storage unit.  These informational totals can’t be changed or deleted.
      • The closed sub-atomic quantum system is a duplicate of the macro quantum system.  The two systems interact on a binary basis.
    • The triune combined functions of consciousness, quantum gravity, and quantum entanglement act as one from the underside of the fabric of space-time.
  • The graceful, winding arms of the majestic spiral galaxy M51 (NGC 5194) appear like a grand spiral staircase sweeping through space. They are actually long lanes of stars and gas laced with dust. This sharpest-ever image, taken in January 2005 with the Advanced Camera for Surveys aboard the NASA/ESA Hubble Space Telescope, illustrates a spiral galaxy’s grand design, from its curving spiral arms, where young stars reside, to its yellowish central core, a home of older stars. The galaxy is nicknamed the Whirlpool because of its swirling structure. The Whirlpool’s most striking feature is its two curving arms, a hallmark of so-called grand-design spiral galaxies. Many spiral galaxies possess numerous, loosely shaped arms that make their spiral structure less pronounced. These arms serve an important purpose in spiral galaxies. They are star-formation factories, compressing hydrogen gas, and creating clusters of new stars. In the Whirlpool, the assembly line begins with the dark clouds of gas on the inner edge, then moves to bright pink star-forming regions, and ends with the brilliant blue star clusters along the outer edge. Some astronomers believe that the Whirlpool’s arms are so prominent because of the effects of a close encounter with NGC 5195, the small, yellowish galaxy at the outermost tip of one of the Whirlpool’s arms. At first glance, the compact galaxy appears to be tugging on the arm. Hubble’s clear view, however, shows that NGC 5195 is passing behind the Whirlpool. The small galaxy has been gliding past the Whirlpool for hundreds of millions of years. As NGC 5195 drifts by, its gravitational muscle pumps up waves within the Whirlpool’s pancake-shaped disk. The waves are like ripples in a pond generated when a rock is thrown in the water. When the waves pass through orbiting gas clouds within the disk, they squeeze the gaseous material along each arm’s inner edge. The dark dusty material looks like gathering storm clouds. These dense clouds then collapse.

    The Horsehead Nebula viewed in infrared wavelengths. The nebula, shadowy in optical light, appears transparent and ethereal when seen in the infrared, represented here with visible shades. The backlit wisps along the Horsehead’s upper ridge are being illuminated by Sigma Orionis, a young five-star system just off the top of the Hubble image. A harsh ultraviolet glare from one of these bright stars is slowly evaporating the nebula. Along the nebula’s top ridge, two fledgling stars peek out from their now-exposed nurseries. The Horsehead Nebula is part of a much larger complex in the constellation Orion. Known collectively as the Orion Molecular Cloud, it also houses other famous objects such as the Great Orion Nebula (M42), the Flame Nebula, and Barnard’s Loop. At about 1,500 light-years away, this complex is one of the nearest and most easily photographed regions in which massive stars are being formed. (NASA, ESA, and the Hubble Heritage Team, STScI/AURA)

    The Hubble image unveils a very cluttered-looking universe filled with galaxies near and far. Some are distorted like a funhouse mirror through a warping-of-space phenomenon first predicted by Einstein a century ago. In the center of the image is the immense galaxy cluster Abell S1063, located 4 billion light-years away, and surrounded by magnified images of galaxies much farther. Thanks to Hubble’s exquisite sharpness, the photo unveils the effect of space warping due to gravity. The huge mass of the cluster distorts and magnifies the light from galaxies that lie far behind it due to an effect called gravitational lensing. This phenomenon allows Hubble to see galaxies that would otherwise be too small and faint to observe. This “warp field” makes it possible to get a peek at the very first generation of galaxies. Already, an infant galaxy has been found in the field, as it looked 1 billion years after the big bang. This frontier image provides a sneak peek of the early universe, and gives us a taste of what the James Webb Space Telescope will be capable of seeing in greater detail when it launches in 2018. The cluster contains approximately 100 million-million solar masses and contains 51 confirmed galaxies and perhaps over 400 more. (NASA, ESA, and J. Lotz, STScI)

    The Bubble Nebula is seen in an image captured in February 2016, by the Hubble Space Telescope’s Wide Field Camera 3 and released April 21, 2016. The nebula is 7 light-years across? about one-and-a-half times the distance from our sun to its nearest stellar neighbor, Alpha Centauri ? and resides 7,100 light-years from Earth in the constellation Cassiopeia.

    OUR NEIGHBORHOOD STAR (THE BIRTH AND DEATH OF THE SUN).
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    • More than 5 Billion years ago, there was no Sun, no Earth, no solar system at all.  instead, just a huge, thin cloud of gas and dust slowly turning and drifting through space.   Gradually, the cloud became smaller, as gravity pulled it together.  Concurrently, it was getting hotter and denser.  The fuzzy ball at the center of the cloud got hot enough for fusion to start.  Hydrogen began to turn into helium, making light and heat.
    • the litany of events (for a star of the sun’s size).
    • First, A cloud of diffuse gas.
    •  Second, a protostar evolves (the star releases energy from gravitational contraction).
    • Becomes the main-sequence star. (Fuse’s hydrogen to helium in the core, stabilized and long-lived).
    • After the nuclear fuel is gone, it expands into a red giant, consuming its planets.
    • Then, it becomes a small and dim star, called a white dwarf.
    Larger sized stars in the neighborhood:
    • Larger mass stars become supergiants, once an iron core develops.
    • If large enough, they can become a supernova.
    • A few can become a Neutron star. (small, dim, and extremely dense).
    • Fewer yet, become black holes.