| 10.3 |
Star properties
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As we said earlier, the principle
reaction that occurs within stars to produce light particles and other
particles is strong-nuclear fusion. Strong nuclear fusion (as defined and
discussed in previous chapters) is a reaction whereby sub-atomic particles
configure and/or re-configure new atomic structures and as a result, certain
atomic and sub-atomic particles are repulsed into nearby space.
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| 10.3.1
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Revisit of the relative temperatures
required for strong-nuclear fusion
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As we also discussed earlier,
the relative levels of kinesis to cause firstly atomic structures to become
unstable and secondly for atomic structures to reconfigure into more complex
and/or less complex shapes are huge. |
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Strong Nuclear Fusion
Reaction
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Temperature Required |
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Proton-Proton
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20 million degrees K |
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Photons (3 Quarks) |
18.2 million degrees K |
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Hetons (3 Down Quarks)
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7.3 million degrees K |
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Protoactives |
7 million degrees K |
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Protons
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5 million degrees K |
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Magnetons
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5 million degrees K |
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Positrons |
3.5 million degrees K |
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Neutrons
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2.1 million degrees K |
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Neutroactives |
1.3 million degrees K |
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Electrons
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678,000 degrees K |
| 10.3.2 |
The actual process of chain reaction- ergon
levels and therefore strength
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As we now understand, the relative
conditions for strong nuclear fusion occur only under certain conditions to
produce such het. These conditions are limited to: o the creation boundary of
the Universe (creation of Quarks and Neutrinos), o collapsing nebulae (the
birth of stars), o inside stars themselves, o the collapse of stars (black
holes, supernova). |
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As we have discussed previously, a fusion
reaction is when groups of like spin and strength particles are in sufficient
quantities and close proximity that they form close orbits. This process means
that the relative velocity of these particles drops to O and at that moment,
their kinesis rates are at maximum. This creates a wave of intense kinesis rise
and therefore a chain reaction of like particles forming new bonds. If the
kinesis levels are high enough and in sync, the like particles can form more
geometrically complex and perfect shape. |
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These newly "fused" like particle groups
and their huge release of kinesis act as a magnet for other particles to come
in. The resultant rush, pushes the newly formed and heavier particles outwards,
thereby creation a chain reaction of kinesis, release and motion of particles
inwards and outwards. |
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Photon-Photon core fusion requires the
second greatest level of kinesis (temperature). Proton-Proton (hydrogen to
helium) is the highest, while electrons and neutrons are often enough to kick
off a chain reaction to start-up a star. |
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When we look at a Star emitting light
particles, we are seeing a series of simultaneous chain reactions of the fusion
of different particles ranging from electrons through to photons- the
electromagnetic spectrum. Hydrogen to Helium fusion is merely one of many
different particle chain fusion reactions occurring in our Sun at the same
time. |
| 10.3.3 |
How do stars get the first chain reaction
to occur?
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Stars are huge compared to the size of
planets. Stars, being many hundreds of thousands of kilometres in diameter
compared to a few thousand kilometres for planets. |
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Because of the general forces of
attraction, the further inward we travel into a star, the higher the density.
This increasing inward pressure causes increased levels of kinesis to a point
that a kinesis level is reached between similar particle shapes and a chain
reaction occurs. |
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This sets up a reaction whereby the forces
inwards are dramatically increased with a tangible increased attraction of the
core to like particles, while at the same time creating an equally strong
pressure outwards. It is therefore the number of particles, their size, kinesis
rates and the relative pressures that start the sequence of chain reactions to
occur. |
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An excellent example of a star trying to
start a chain reactions is Jupiter. Jupiter for its size (144,000km across)
rotates at phenomenal speed (around 1 rotation in around 10 hours). This speed
increases the pressures within the atmosphere of Jupiter tremendously. |
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Sadly for Jupiter though, its size and
rotation rate is only sufficient to cause fusion reactions to the magneton
stage at its core. Interestingly, during its life cycle, it is possible to see
Jupiter lighten in colour. This would indicate limited success in producing
certain fusion reactions, but not of sufficient quantity to set of a chain
reaction and convection particle field around Jupiter of Photons. |
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However, it does indicate that at some
point, Jupiter via its continued growth (attraction as a magnet of small
particles throughout the solar system), will reach a critical point where
photon-photon and proton-proton chain reactions can be established with limited
success. This is likely towards the end of life of our Sun. |
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That Jupiter lightens and darkens
significantly during the course of its orbit of the Sun indicates that Jupiter
is much closer to being a photon producing star than contemporary science
thinks. |
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That in ten million, possibly one hundred
million years that Jupiter might fulfil its destiny and become our second Sun
is an important understanding of the path of evolution yet to unfold in our
very own immediate neighborhood. |
| 10.3.4 |
The return of particles to the Sun and their curved
path
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As we have mentioned earlier, it is only in the past fifty years that
contemporary science conceded that light does not travel in straight lines. |
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Yet we have a further way to go in understanding just how particles from a Sun
travel to a planet and then what happens next?. The first question to tackle
is: do particles that emanate from the Sun ever return? |
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Particle fields |
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We have already discussed that ergon
particles behave in fields. We now know that the Sun has huge magnetic particle
fields, gravity fields, electrical fields. |
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But what about photon fields? What we mean is that, there is nothing to suggest
to the contrary that the majority of light particles circulate back to the Sun
once hitting a planet. This is in spite of a high degree of entropy of photon
particles into deep space. Particle fields also explain why the levels of light
further out from the Sun diminish. Because Photons are on a path to return to
the Sun. |
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That photons, electrons, magnetons behave in particle fields through, out and
back to the Sun explains why the Sun remains relatively stable in size and
output for so long. That is because it is a self regulating system. It is much
more advanced set of process than simply something blowing up. |
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For instance, we know stars do not grow at an exponential rate from birth. We
know this because our Sun has been the same approximate size for several
billion years. If particle fields did not exist and we simply saw the random
explosion of particles from the Sun without any regulation- one of two things
would happen: |
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Suns would expand very quickly into chain reactions that spread larger and
larger;
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or Suns would burn out very quickly (millions of years).
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| 10.3.5 |
Answering an anomaly of science- does a star just burn on its original fuel
base?
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Just as so many hundreds of other models of science, the Sun has been
considered a "closed system" for much of this century- that is the Sun burns by
virtue of its own original fuel reserves (hydrogen). |
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This model seems to make perfect sense, until closer analysis of the "rate" of
fuel consumption by our Sun points to an anomaly as to the precise proportion
of helium present. |
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If we project back in time to the original birth and beginnings of the
strong-nuclear fusion reactions at the core of our Sun, then the levels of
helium should by rights be in greater proportions- in other words, the fuel
tanks should be emptier than they are. |
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The search for neutrinos and "thick" space have given us clues |
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It has only been through the greater understanding of the formation of stars
from nebulae and the general "attraction" of large structures to smaller
sub-atomic and atomic structures, that we have come to understand that the Sun
is actually attracting sub-atomic particles from nearby space (up to 1.5 light
years away) while at the same time, releasing particles such as photons (light
particles). |
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The difference is that the amount of sub-atomic and atomic particles attracted
to the Sun's atmosphere is less than the rate of nuclear fusion. If it was the
same, the fuel tanks of hydrogen would never run dry. |
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This way, we see a counter balance between the gradual acceleration of nuclear
fusion at the core of stars as their density increases and the attraction of
new particles from nearby space. When we look at the evolution and gradual
death of stars, we must also consider the amount of matter attracted to the
star, that in turn slows the date of death. |
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One more controversy- the loss of hydrogen |
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One loop that hasn't fully been resolved
by science is that nuclear fusion of hydrogen into helium does not match up
with replenishment rates. In other words, Stars lose hydrogen not only by
fusion but by the attachment of hydrogen to other particles such as Photons. |
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What this means is that the Sun loses
Hydrogen on two fronts- nuclear conversion as well as being part of particle
packages such as light. |
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However, on the return journey, light
particles "pick-up" stray hydrogen particles back to the Sun as new fuel. This
additional hydrogen loss explains the exponential changes in Suns when hydrogen
levels versus size reach critical points. |
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The same process for helium will occur
once the size and temperature of the core of the Sun reaches sufficient
temperatures to start a photon-photon core reaction, producing stronger light
particles capable of carrying helium. |
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