|
Taxon
NUCLEOGALAXIES
TAXA Galactides Objects with blackstars in their nuclei.
TAXON Elliptogalaxies Galactides with a one blackstar, standard, nucleus.
TAXON Electrogalaxies Galactides with a two blackstar, electroidal, nucleus.
TAXON Nucleogalaxies Galactides with a three blackstar, nucleonic, nucleus. |
|
|
CONTENTS
- TAXONOMY - a hierarchical presentation.
- GALAXY - a large structure that may be photonic, electroidic, nucleonic, or isotopic.
- G3 GALAXY - a nucleonically structured galaxy.
- G3NUCLEUS - a quarkcore and a blackhole inside an aurasphere.
- G3nucleus - elementals
- G3quarkcores
- G3axiquarks
- G3centriquarks
- G3teeloceans
- G3nucleus - physicals
- G3nucleus principal measurements
- Mass measurements
- Repellence measurements
- G3nucleus principal features
- G3nucleus stability
- G3nucleus mass constancy
- G3nucleus morphidity
- G3nucleus - mechanicals
- G3quark teelstream systems
- G3nucleus teelstream systems
- G3quark attunement
- G3nucleus stabilisation turbines
- G3nucleus north polar jets
- G3nucleus south polar jets
- G3nucleus blackholes
- G3TEELOSPHERE - a region of gasbonded teels that is a kaosphere inside a halosphere.
- G3 teelosphere - elementals
- KAOSPHERE - that part of the teelosphere that is bound to the nucleus.
- Elementals
- Physicals
- Mechanicals
- Eventuals
- Interactuals
- HALOSPHERE - that part of the teelosphere that is bound to the galaxy.
- Elementals
- Physicals
- Mechanicals
- Eventuals
- Interactuals.
- VOIDOSPHERE - a region that is outside the galaxy but inside the galaxy's gravitysheath.
|
|
NARRATIVES
Broadly,
a G3 galaxy equates to the large elliptical galaxies of the
Current Paradigm. However, not all large ellipticals are G3s. G1
galaxies, for example, can become more massive than a G3 and be
superficially indistinguishable from one. Conversely, not all G3s
have the expected appearance of a large elliptical. The
nucleus of a G3 is small, relatively, and the often extensive
teelosphere of a large elliptical is not essential for it
to endure.
* * * * *
G3
galaxies form when a G2 galaxy accretes a G1 galaxy. Collisions between
such galaxies don't always result in a union but if the alignment is
satisfactory, the mass of the two quarkcores is enough to strongforce
them together without need of a third party mechanism.
* * * * *
Empirical
facts about galaxies are all observational. That galaxies come
in a wide range of sizes is clearly seen and the masses
underlying these variations can be calculated.
However, the reasons offered for their variations are
necessarily conjectural. It doesn't help that all that can be
seen of large/giant ellipticals is an ellipsoid with a smooth
and nearly featureless image.
* * * * *
In
the taxonomy below, G3 galaxies have a sophisticated structure.
This is deduced evolutionarily, the assumption being that the patterns
established in earlier taxons are replicated in galaxies. There
is, of course, no empirical confirmation for much of the taxonomy
but it is encouraging that some current galactic conundrums are
resolved in it.
* * * * *
A
G3 galaxy has three g3quarks in its nucleus. Thus it has a
nucleonic structure. Nucleons are morphides, able to be as
neutrons or protons. Thus G3 galaxies are structured neutronically or
protonically. In the lifecycle description below, G3
galaxies begin life as neutronics and then transmute
permanently to protonics. If the nucleon is a true precedent, this
may not be so. It is so here to keep matters simple but in
practice G3s may well have an enduring neutronic form,
especially when near the centre of large galaxy clusters..
* * * * *
In
the Current Paradigm, there is concern that the blackholes in
supergiant galaxies would require more than 13.8 billion years to
accrete to their present mass - 13.8 billion year being the estimated
time since the big bang. G3 galaxies form by the coming together of
three G1s or a G1 and a G2. The mass of stable G1s is not a constant
but that of stable G2s is. Thus it is more than likely that the
resulting trio is overstable. This is especially so if a G2 is
involved. An overstable object is a mass sink. It absorbs and does not
eject until it is stable and if there is absorbable matter available
the absorption is rapid. 13.8 billion years may or may not be a viable
timespan but the currently observed G3s are all understable and
most are extensively cloaked in absorbables. There is no good
reason why a G3 cannot reach that condition well within the 13.8.
* * * * *
Nucleons have
three quarks in their nuclei and no more. In the description below, G3
galaxies echo that. However, there is no immediately apparent
reason why galaxies cannot contain four quarks or more. A galaxy
nucleus with two axial quarks and two centrifugal quarks is an
especially satisfying notion. It would be a neutral and very dense
object and thus an ideal building block in the same manner that
dense and neutral heliums are the building blocks for complex isotopes.
A notion not explored here but worth considering is the
bonding together of numbers of G3 galaxy nuclei to form "galactic
isotopes".
* * * * *
A
G3 galaxy has a stabilisation turbine identical in every way bar one to
that found in a proton. The one difference is size with a G3
turbine being enormous relative to a proton turbine. In the
description below, no comment is made as to the types of stabilisation
objects emitted by a G3 turbine but it can be reasonably
assumed that everything a proton turbine can emit is also
emittable by a G3 turbine - with the greater size of the G3
enabling the emission of even larger objects.
* * * * *
The
possible emission of larger objects by G3 stabilisation turbines may
raise conflict with the Current Paradigm which assumes that
most protons, deuteriums, and heliums formed in the first moments of
the Universe. The most massive objects formed in a proton stabilisation
turbine are electroids. The next massive objects after electroids are
nucleons, deuteriums, and heliums and the stabilisation turbine in
a G3 galaxy is suited to their creation. It might explain
why gas clouds are detected close to some astrophysical jets (the
clouds need to be "lit" to be detected so there may be "unlit" clouds
close to all astrophysical jets). It would explain why many
astrophysical jets emit photons - something not possible without
there being understable protons inside the jets. Whether "most"
protons, deuteriums, and heliums were produced in the first moments of
the Universe, or are are being continuously produced in G3
turbines, is a matter for further research.
* * * * *
The
nucleus of a stable G3 galaxy has a specific mass. The G3 galaxy
does not. The jets of a G3 nucleus stabilise the nucleus and that part
of the teelosphere that is inside the gravityhorizon. The part of
the galaxy outside the gravityhorizon is primarily held by the
intrinsic gravitypull of the galaxy and not by the extrinsic
gravitypull of the nucleus. Thus the growth potential of outer galaxy
is considerable without affecting the mass of a stable nucleus.
There is a limit to the growth but within that limit large/giant
ellipticals are observed in a wide range of masses and sizes.
* * * * *
Some large/giant
elliptical galaxies are observed to have an astrophysical jet. Some
have two although most have none that are readily apparent. The jets
serve to stabilise the galaxy nucleus. Thus a less understable
nucleus discharges the content of its jet into the teelosphere or the
halosphere where it is difficult or impossible to observe. A more
understable nucleus discharges the content of its northern
astrophysical jet into its voidosphere or even beyond its gravitysheath
interface. Such discharges continue until the understability of
the nucleus has fallen enough to retreat the jet back inside the
halosphere. A nucleus sufficiently understable can
have southern astrophysical jet discharges beyond the halosphere
but southern jets have less heft and so this is less
common. |
|
SUMMARY - G3 GALAXY - NUCLEUS
|
TAXONOMY - G3 GALAXY - NUCLEUS
TAXONOMY - G3 GALAXY - TEELOSPHERE
G3teelosphere - contents
- G3teelosphere content -
- Teelosphere teelstream systems -
- Polar jets.
- Atmospheres.
- Stellarspheres.
- Voidospheres.
|
G3teelosphere - Physicals
Principal measurements
- Teelosphere extrinsic gravitypull.
- Teelosphere extrinsic inertia.
- Teelosphere intrinsic gravitypull.
- Teelosphere intrinsic inertia.
- Teelosphere extrinsic motion -
- Teelosphere extrinsic velocity.
- Teelosphere extrinsic spinrate.
- Teelosphere intrinsic motion -
- Teelosphere intrinsic velocity.
- Teelosphere intrinsic spinrate.
Principal features
Stability
- Teelosphere stability is either -
- Overstable -
- Energyvelocity less than massvelocity.
- Stable -
- Energyvelocity same as massvelocity -
- Understable -
- Energyvelocity more than massvelocity.
|
The
teelosphere is the outer region of a G3 galaxy. It is the gasbonded
teelstream system that surrounds the G3 nucleus. When the galaxy is
stable, the teelosphere is mostly subphotonics. When it is understable,
it also has significant quantities of superphotonics and stars.
In
a stable G3, the teelosphere is a stable semiaxial
structure, densely bound to the nucleus. Being stable, its
energyvelocity is the same as its massvelocity and so, subject to
stabilisation lag, it counters any absorptions by the ejection of the
equivalent in teel EMV from its surface.
In an understable G3,
the teelosphere is also understable. Now, while it is still primarily
semiaxial, there is a significant secondary chaotic element. This
teelosphere is more substantial and more extensive. It is also more
complex, the lower region being the kaosphere and the upper region
being the halosphere. The kaosphere and the halosphere differ in the
way their content is held inside the galaxy.
Kaosphere content is -
- Extrinsically gravitypulled by the nucleus.
- Extrinsically gravitypulled by the halosphere.
- Intrinsically gravitypulled by the galaxy.
- The extrinsic gravitypull of the nucleus dominates.
Halosphere content is -
- Intrinsically gravitypulled by the galaxy.
- Extrinsically gravitypulled by the nucleus.
- Extrinsically gravitypulled by the kaosphere.
- The intrinsic gravitypull of the galaxy dominates.
The stars
of an understable teelosphere interact with the teelosphere
teelstream system. The heft of the teelstreams is not constant.
- It increases with increases in the understability of the galaxy.
- It decreases with upward distance from the surface of the aurasphere.
In
the kaosphere, the heft is such that its stars are strongly engorged
with those toward the surface of the aurasphere being overengorged. In
the halosphere, while the stars are less strongly engorged their
engorgement is still such that evolutions beyond S1 stars does not
happen.
An understable G3 stabilises if conditions allow. The
teelosphere is a mechanism in the stabilisation process. The process
results in the ejection of the excess teel EMV out of the galaxy in the
polar jets - principally from the north polar jet.
- The content of a north polar jet is -
- A core of subphotonics, photons, and superphotonics.
- A sheath of aerospiking subphotonics.
- The jet discharges a proportion of its content into the halosphere as byflow.
- The byflow becomes star nurseries for the manufacture of star clusters.
- The byflow becomes solo stars and binaries.
- The stars are engorged by the teelstreams.
- The stars migrate over time into the kaosphere.
- The stars are overengorged in the kaosphere.
- The overengorged stars dissipate.
- The dissipated content migrates over time into the aurasphere.
- The aurasphere content migrates into the quarkcore stabilisation turbine.
- The turbine manufactures the content into subphotonics, photons and superphotonics.
- The turbine content is ejected as the north polar jet.
- The jet discharged a proportion of its content out of the galaxy.
- The jet discharges a proportion of its content into the halosphere as byflow.
The process continues to cycle until the G3 is stable.
|
TAXONOMY - G3 GALAXY - TEELOSPHERE - KAOSPHERE
Kaosphere - elementals
Kaosphere synopsis
- A kaosphere is -
- The inner region of an understable teelosphere.
- Above the aurasphere.
- Below the halosphere.
- Kaosphere contents are -
- A teelstream system.
- Numbers of superphotonics.
- Numbers of stars.
- Kaospheres are gravitationally bound to the galaxy -
- Primarily -
- By extrinsic gravitypull -
- A kaosphere mutually gravitypulls the galaxy nucleus.
- Secondarily -
- By intrinsic gravitypull -
- Every kaosphere object mutually gravitypulls every galaxy object.
Kaosphere teelstream system
- A kaosphere teelstream system is -
- The lower part of the teelosphere teelstream system -
- Teelosphere teelstream systems are semiaxial -
- Northern hemisphere teelstreams -
- Rise at northpole -
- Move at high level to equator -
- Fall at equator -
- Move at low level to northpole.
- Southern hemisphere teelstreams -
- Rise at southpole -
- Move at high level to equator -
- Fall at equator -
- Move at low level to southpole.
- Semiaxial teelstream system equators increasingly move toward the southpole with increasing galaxy understability.
- Kaosphere teelstream systems are modified by galaxy understability -
- Teelospheres of understable galaxies contain engorged stars -
- Engorged star numbers increase with increasing galaxy understability.
- Engorged stars bind to the aurasphere surface.
- Engorged stars extend farther from the aurasphere surface as numbers increase.
- Engorged stars extend from the aurasphere surface into the halosphere if numbers increase sufficiently.
- Engorged stars in sufficient numbers render the teelstream system around them chaotic.
- Kaosphere teelstream systems are -
- Primarily: semiaxial.
- Secondarily: chaotic.
Kaosphere superphotonics
- A kaosphere's superphotonics are -
- Electroids, nucleons, deuteriums, and heliums.
- Kaosphere superphotonics are -
- Primarily: bound to the galaxy nucleus by extrinsic gravitypull.
- Secondarily: bound to the galaxy by intrinsic gravitypull..
- Kaosphere superphotonics are -
- Primarily: discharges or byflows from the polar jets.
- Secondarily: ejections from the aurasphere.
- Secondarily: absorptions from the halosphere.
- Kaosphere superphotonics migrate into the aurasphere over time -
- Primarily: extrinsically gravitypulled by the galaxy nucleus.
- Secondarily: intrinsically gravitypulled by the galaxy.
- Kaosphere superphotonics are stripped of their teelospheres as they migrate -
- A
consequence of the galaxy's increasing gravitypull with with increasing
nearness to the aurasphere and the resulting decrease in
the volume of their gravitysheaths -
- Superphotonic stripping can be 100% on entry into the aurasphere.
Kaosphere stars
- A kaosphere's stars are -
- Primarily: absorbed from the halosphere.
- Secondarily: formed from the discharge or byflow of the polar jets.
- Kaosphere stars absorbed from the halosphere are already engorged -
- Stars formed in the kaosphere are formed engorged.
- Kaosphere stars are -
- Primarily: bound to the galaxy nucleus by extrinsic gravitypull.
- Secondarily: bound to the galaxy by intrinsic gravitypull.
- Kaosphere stars migrate to the aurasphere over time -
- Primarily: extrinsically gravitypulled by the galaxy nucleus.
- Secondarily: intrinsically gravitypulled by the galaxy.
- Kaosphere stars become overengorged as they migrate toward the aurasphere -
- A consequence of -
- The heft of the teelstream system increasing with increasing nearness to the aurasphere.
- The increasing transmutation of potential motion to motion with increasing nearness to the aurasphere.
- Kaosphere stars are overengorged to dissipation on nearing the aurasphere -
- Most stars are wholly dissipated to nucleons or subphotonics before entering the aurasphere.
- Dissipation is accompanied by high levels of photon emission.
- Stars not wholly dissipated before entering the aurasphere are dissipated shortly thereafter.
|
Kaosphere - Physicals
Principal measurements
- Kaosphere mass measurements
- Kaosphere extrinsic gravitypull -
- Kaosphere gravitypull strength on something external, eg -
- A point or object outside the kaosphere.
- The galaxy masscentre.
- The halosphere.
- The combined gravitypull strength of the nucleus and teelosphere is the extrinsic gravitypull strength of the galaxy.
- Kaosphere extrinsic inertia -
- Kaosphere resistance strength to being gravitypulled toward something external, eg -
- A point or object outside the kaosphere.
- The galaxy nucleus.
- The halosphere.
- The
combined resistance strength of the nucleus and the teelosphere to
being gravitypulled toward something external is the extrinsic inertia
of the galaxy.
- Kaosphere intrinsic gravitypull -
- Kaosphere gravitypull strength on something internal, eg -
- A point or object inside the kaosphere.
- Its own masscentre.
- The kaosphere is a "shell" so its masscentre is a "shell within a shell".
- Kaosphere intrinsic inertia -
- Kaosphere resistance strength to being gravitypulled toward something internal, eg -
- A point or object inside the kaosphere.
- Its own masscentre.
- The kaosphere is a "shell" so its masscentre is a "shell within a shell".
- Kaosphere extrinsic motion -
- Kaosphere extrinsic velocity plus kaosphere extrinsic spinrate -
- Kaosphere extrinsic velocity -
- Kaosphere velocity relative to something external, eg -
- A point or object outside the kaosphere.
- The
kaosphere extrinsic velocity and the galaxy extrinsic velocity coincide
when relative to the same object outside the galaxy.
- Kaosphere extrinsic spinrate -
- Kaosphere spinrate relative to something external, eg -
- A point or object outside the kaosphere.
- The galaxy masscentre.
- The galaxy nucleus.
- The
kaosphere extrinsic spinrate and the extrinsic spinrate of the nucleus
may or may not coincide when relative to the same object outside the
galaxy.
- Kaosphere intrinsic motion -
- Kaosphere intrinsic velocity plus kaosphere intrinsic spinrate -
- Kaosphere intrinsic velocity -
- The velocities of the teels in a kaosphere relative to something internal, eg -
- A point or object inside the kaosphere.
- The kaosphere masscentre.
- The kaosphere is a "shell" so its masscentre is a "shell within a shell".
- Kaosphere intrinsic spinrate -
- The spinrates of the teels in a kaosphere relative to something internal, eg -
- A point or object inside the kaosphere.
- The kaosphere masscentre.
- The kaosphere is a "shell" so its masscentre is a "shell within a shell".
- Kaosphere repellence measurements
- Kaosphere density -
- Absolute: the sum of the volumes of the teels in a kaosphere relative to the volume of the kaosphere.
- Practical: the sum of the volumes of the stars in a kaosphere relative to the volume of the kaosphere.
- Kaosphere dimensions -
- Depth.
- Duration.
- Height.
- Volume.
- Width.
- Etc.
Kaosphere principal features
- Kaosphere axis -
- The notional straight line through a kaosphere around which it spins -
- May or may not coincides with the axis of the nucleus.
- Kaosphere equator -
- The notional line on the surface of a kaosphere that is 90° from the axis and equidistant from its poles -
- May or may not coincide with the equator of the nucleus.
- Kaosphere northpole -
- The axiquark end of a kaosphere's axis.
- Kaosphere southpole -
- The centriquark end of a kaosphere's axis.
- Kaosphere surface -
- The outer face of a kaosphere -
Kaosphere stability
- A kaosphere is understable -
- Kaospheres cease to exist on becoming stable.
- Kaosphere understability -
- Kaosphere energyvelocity is more than its massvelocity.
- Kaospheres automatically stabilise out of existence if conditions allow.
- Can only become stable when the nucleus is stable.
- Kaospheres become stable by ejecting teel EMV more quickly than it is absorbed.
- All stars and superphonics have dissipated into the aurasphere.
Kaosphere mass constancy
- Kaosphere mass is not a constant -
- Rule of thumb -
- The greater the understability of the galaxy, the greater the volume of its kaosphere.
|
Kaosphere - mechanicals
Kaosphere teelstream system
- Kaosphere teelstream systems have heft -
- Kaosphere teelstream heft decreases from the aurasphere surface upward.
- Kaosphere teelstream systems have a primary structure and a secondary structure -
- Primary structure -
- Semiaxial - driven by discharge or byflow from the polar jets.
- North polar jet discharge or byflow has more heft than that of the south polar jet.
- South polar jet discharge or byflow has less heft than that of the north polar jet.
- With increasing galaxy understability, the heft disparity between the north polar jet and the south polar jet increases -
- With increasing galaxy understability, the equatorial downflow moves increasingly south.
- Secondary structure -
- Chaotic - driven by ejections and emissions from engorged and overengorged stars -
- Star packing density increases with nearness to the aurasphere.
- Star engorgement increases with nearness to the aurasphere.
- Star overengorgement and dissipation increases with nearness to the aurasphere.
- Star repellence increases with nearness to the aurasphere.
- Star velocity increases with nearness to the aurasphere.
- Transmutation of potential velocity to velocity.
Kaosphere superphotonics
- Kaospheres contain superphotonics -
- Superphotonic numbers increase as the understability of a galaxy increases.
- Kaosphere superphotonics are sourced -
- Primarily - as downflow from the halosphere -
- Most are stripped of some or all of their teelospheres before they enter the kaosphere.
- Secondarily - from the polar jets -
- As discharge if a jet does not breach the kaosphere surface.
- As byflow if a jet breaches the kaosphere surface.
Kaosphere superphotonics processing
- Kaosphere superphotonics processing is interactions between the superphotonics and the kaosphere teelstream system.
- Kaosphere are mostly neutrons which either -
- Migrate into the aurasphere over time, or
- Dissipate before reaching the aurasphere.
- Kaosphere neutrons are progressively stripped of the remains of their teelospheres -
- By the increasing heft of the kaosphere teelstream system.
- By the decreasing volume of their gravitysheath due to the increasing gravitypull strength of the nucleus.
- Kaosphere stripped neutrons have reduced interaction with star teelospheres -
- Having no teelosphere their only repellence is contact with the nucleus.
- Kaosphere stripped neutrons are engorged becoming overengorged -
- Continuously overengorged neutrons dissipate to quarks -
- The quarks then dissipate to teels.
- Neutrons that enter the aurasphere dissipate there.
Kaosphere stars
- Kaospheres contain stars -
- Star numbers increase with the understability of the galaxy -
- Kaosphere stars are sourced -
- From the halosphere -
- Halosphere stars migrate into the Kaosphere over time.
Kaosphere star processing
- Kaosphere star processing is interactions between its stars and its teelstream system.
- Stars are engorged by the heft of the teelstreams -
- Teelstream heft increases from kaosphere surface to the aurasphere surface.
- Star engorgement increases with decreasing distance from the aurasphere -
- Becoming overengorgement before the aurasphere is reached.
- Star velocity increases with decreasing distance from the aurasphere.
- As potential velocity transmutes to velocity.
- Star repellence increases with decreasing distance from the aurasphere -
- Star teelosphere increases in density and volume.
- Star teelosphere contracts by being stripped -
- By the increasing heft of the kaosphere teelstream system.
- By the increasing gravitypull strength of the nucleus.
- Star packing density increases with decreasing distance from the aurasphere.
- Stars dissipate over time with overengorgement -
- By increased photon emission.
- By subphotonic and superphotonic ejection.
- Stars dissipate into superphotonics -
- The superphotonics dissipate into quarks.
- The quarks decay and dissipate into teels.
- Star dissipation content migrates into the aurasphere.
|
TAXONOMY - G3 GALAXY - TEELOSPHERE - HALOSPHERE
Halosphere - elementals
Halosphere synopsis
- A halosphere is -
- The outer region of an understable teelosphere -
- Below the voidosphere or gravitysheath interface.
- Halosphere contents are -
- A teelstream system.
- Numbers of superphotonics.
- Numbers of stars.
- Halospheres are gravitationally bound to the galaxy -
- By intrinsic gravitypull -
- Every halosphere object mutually gravitypulls every galaxy object.
- By extrinsic gravitypull -
- A halosphere mutually gravitypulls the galaxy nucleus.
- Intrinsic gravitypull dominates.
Halosphere teelstream system
- A halosphere teelstream system is -
- The upper part of the teelosphere teelstream system.
- Teelosphere teelstream systems are semiaxial -
- Northern hemisphere teelstreams -
- Move at high level to equator -
- Move at low level to northpole.
- Southern hemisphere teelstreams -
- Move at high level to equator -
- Move at low level to southpole.
- Semiaxial teelstream system equators increasingly move toward the southpole with increasing galaxy understability.
- Halosphere teelstream systems are modified by galaxy understability -
- Teelospheres of understable galaxies contain engorged stars -
- Engorged star numbers increase with increasing galaxy understability.
- Engorged stars bind to the aurasphere surface.
- Engorged stars extend farther from the aurasphere surface as numbers increase.
- Engorged stars extend from the kaosphere into the halosphere if their numbers increase sufficiently.
- Engorged stars in sufficient numbers render the surrounding teelstream system chaotic.
- Halosphere teelstream systems are -
- Primarily: semiaxial.
- Secondarily: chaotic.
Halosphere superphotonics
- A halosphere's superphotonics are -
- Electroids, nucleons, deuteriums, and heliums.
- Halosphere superphotonics are -
- Primarily: bound to the galaxy -
- Secondarily: bound to the galaxy nucleus.
- Halosphere superphotonics are -
- Primarily: discharges or byflows from the polar jets -
- Secondarily: ejections from the kaosphere.
- Secondarily: absorptions from the outside the halosphere surface.
- Halosphere superphotonics migrate to the kaosphere over time -
- Primarily: intrinsically gravitypulled by the galaxy.
- Secondarily: extrinsically gravitypulled by the galaxy nucleus.
- Halosphere superphotonics are stripped of their teelospheres as they migrate -
- A
consequence of the galaxy's increasing gravitypull with increasing
nearness to the aurasphere and the resulting decrease in
the volume of their gravitysheaths -
- The stripping is usually less than 100% on entry into the kaosphere.
Halosphere stars
- A halosphere's stars are -
- Primarily: formed from the discharge or byflow of the polar jets.
- Secondarily: absorbed from outside the halosphere surface.
- Halosphere stars are -
- Primarily; bound to the galaxy -
- Secondarily bound to the galaxy nucleus.
- Halosphere stars migrate to the kaosphere over time -
- Primarily: intrinsically gravitypulled by the galaxy.
- Secondarily: extrinsically gravitypulled by the galaxy nucleus.
- Halosphere stars are engorged as they migrate -
- A consequence of -
- The heft of the teelstream system increases with increasing nearness to the kaosphere.
- The increasing transmutation of potential motion to motion with increasing nearness to the kaosphere.
|
Halosphere - physicals
Principal measurements
- Halosphere mass measurements
- Halosphere extrinsic gravitypull -
- Halosphere gravitypull strength on something external, eg -
- A point or an object outside the halosphere.
- The combined gravitypull strength of the nucleus and the teelosphere is the extrinsic gravitypull strength of the galaxy.
- Halosphere extrinsic inertia -
- Halosphere resistance strength to being gravitypulled toward something external, eg -
- A point or an object outside the halosphere.
- The galaxy nucleus.
- The kaosphere.
- The
combined resistance strength of the nucleus and the teelosphere to
being gravitypulled toward something external is the extrinsic inertia
of the galaxy.
- Halosphere intrinsic gravitypull -
- Halosphere gravitypull strength on something internal, eg -
- A point or an object inside the halosphere.
- Its own masscentre.
- The halosphere is a "shell" so its masscentre is a "shell within a shell".
- Halosphere intrinsic inertia -
- Halosphere resistance strength to being gravitypulled toward something internal, eg -
- A point or an object inside the halosphere.
- Its own masscentre.
- The halosphere is a "shell" so its masscentre is a "shell within a shell".
- Halosphere extrinsic motion -
- Halosphere extrinsic velocity plus halosphere extrinsic spinrate -
- Halosphere extrinsic velocity -
- Halosphere velocity relative to something external, eg -
- A point or object outside the halosphere.
- The galaxy masscentre.
- The galaxy nucleus.
- The
halosphere extrinsic velocity and the galaxy extrinsic velocity
coincide when relative to the same object outside the galaxy.
- Halosphere extrinsic spinrate -
- Halosphere spinrate relative to something external, eg -
- A point or object outside the halosphere.
- The galaxy masscentre.
- The galaxy nucleus.
- The
halosphere extrinsic spinrate and the extrinsic spinrate of the nucleus
may or may not coincide when relative to the same object outside the
galaxy.
- Halosphere intrinsic motion -
- Halosphere intrinsic velocity plus halosphere intrinsic spinrate -
- Halosphere intrinsic velocity -
- The velocities of the teels in a halosphere relative to something internal, eg -
- A point or object inside the halosphere.
- The halosphere masscentre.
- The halosphere is a "shell" so its masscentre is a "shell within a shell".
- Halosphere intrinsic spinrate -
- The spinrates of the teels in a halosphere relative to something internal, eg -
- A point or object inside the halosphere.
- The halosphere masscentre.
- The halosphere is a "shell" so its masscentre is a "shell within a shell".
- Halosphere repellence measurements
- Halosphere density -
- Absolute: the sum of the volumes of the teels in a halosphere relative to the volume of the halosphere.
- Practical: the sum of the volumes of the stars in a halosphere relative to the volume of halosphere.
- Halosphere dimensions -
- Depth.
- Duration.
- Height.
- Volume.
- Width.
- Etc.
Principal features
- Halosphere axis -
- The notional straight line through a halosphere around which it spins -
- May or may not coincide with the axis of the nucleus.
- Halosphere equator -
- The notional line on the surface of a halosphere that is 90° from the axis and equidistant from its poles.
- May or may not coincide with the equator of the nucleus.
- Halosphere northpole -
- The axiquark end of a halosphere's axis.
- Halosphere southpole -
- The centriquark end of a halosphere's axis.
- Halosphere surface -
- The outer face of a halosphere -
- Coincides with the surface of the teelosphere.
- Coincides with the surface of the galaxy.
- Abuts the voidosphere or coincides with the gravitysheath interface.
Stability
- A halospheres is understable -
- Halospheres cease to exist on becoming stable.
- Halosphere understability -
- Energy velocity is more than massvelocity.
- Automatically stabilises out of existence if conditions allow.
- Can only become stable when the nucleus is stable.
- Becomes stable by ejecting teel EMV more quickly than it is absorbed.
- Rids itself of all stars and superphotonics.
Mass constancy
- Halosphere mass is not a constant.
- Rule of thumb -
- The greater the understability of the galaxy, the greater the mass of its halosphere.
|
Halosphere - mechanicals
Halosphere teelstream system
- Halosphere teelstream systems have heft -
- Halosphere teelstream heft increases from the kaosphere surface upward.
- Halosphere teelstream systems have a primary structure and a secondary structure -
- Primary structure -
- Semiaxial - driven by discharge or byflow from the polar jets -
- North polar jet discharge or byflow has more heft than that of the south polar jet.
- South polar jet discharge or byflow has less heft than that of the north polar jet.
- With increasing galaxy understability, the heft disparity between the north polar jet and the south polar jet increases -
- With increasing galaxy understability, the equatorial downflow moves increasingly south.
- Secondary structure -
- Chaotic - driven by ejections from engorged stars -
- Star packing density increases with nearness to the kaosphere.
- Star engorgement increases with nearness to the kaosphere.
- Star repellence increases with nearness to the kaosphere.
- Star velocity increases with nearness to the kaosphere -
- Transmutation of potential velocity to velocity.
Halosphere superphotonics
- Halospheres contain superphotonics -
- Superphotonic numbers increase as the understability of a galaxy increases.
- Halosphere superphotonics are sourced -
- Primarily - from the polar jets -
- As discharge if a jet does not breach the halosphere surface.
- As byflow if a jet breaches the halosphere surface.
- Secondarily - from beyond the halosphere surface.
- Secondarily - from the kaosphere.
- Halosphere superphotonics are mostly nucleons -
- Deuteriums and heliums only form in the jets of a strongly understable galaxy.
- Strongly understable galaxy jets usually breach the halosphere surface and discharge beyond -
- Deuteriums and heliums may or may not byflow into the halosphere.
Superphotonics processing
- Halosphere superphotonic processing is interaction between its superphotonics and its teelstream system.
- Halosphere superphotonics are drawn toward the kaosphere over time
- Superphotonics become increasingly engorged with increasing nearness to the kaosphere.
- Due to the increasing heft of the teelstream system.
- Halosphere superphotonics are mostly nucleons
- Nucleons in the outer halosphere are mostly protons.
- Protons transmute to neutrons with increasing nearness to the kaosphere.
- Halosphere protons alter with increasing nearness to the kaosphere -
- Proton teelospheres expand due to increasing engorgement.
- Proton teelosphere contract due to contraction of its gravitysheath interface.
- The contraction dominates.
- Proton teelosphere repellence decreases with increasing nearness to the kaosphere -
- Commensurate with the contraction of its gravitysheath interface.
- Halosphere protons transmute to neutrons with increasing nearness to the kaosphere -
- Due to increasing engorgement.
- Halosphere neutrons are stripped neutrons due to decreased teelosphere volume and repellence -
- Stripped neutrons are relatively less affected by adjacent star gravitypull.
- Stripped neutrons are better able to pass unhindered through successive star teelospheres without being absorbed.
Halosphere stars
- Halospheres contains stars -
- Star numbers increase with the understability of the galaxy -
- Halosphere stars are sourced -
- Primarily: from halosphere star nurseries -
- Star nurseries create stars, binaries, and star clusters.
- Secondarily: spontaneously inside the halosphere -
- Spontaneous creations are stars and binaries.
- Secondarily: from outside the halosphere surface -
- As absorbed stars and binaries.
- In lesser galaxies (which become globular clusters once inside the halosphere).
Star processing
- Halosphere star processing is interaction between its stars and its teelstream system.
- Stars are engorged by the heft of the teelstreams -
- Teelstream heft increases from the halosphere surface to the kaosphere surface.
- Star engorgement increases from the halosphere surface to the kaosphere surface.
- Halosphere stars may or may not be in star clusters or globular clusters.
- Clusters are engorged by teelstream heft -
- Teelstream heft increases with increasing nearness to the kaosphere surface.
- Cluster engorgement increases with increasing nearness to the kaosphere surface.
- Cluster engorgement becomes overengorgement between the halosphere surface and the kaosphere surface.
- Cluster overengorgement may or may not result in cluster dispersal before the kaosphere surface is reached.
- Halosphere stars may or may not be metalrich.
- Stars created in the halosphere are metalpoor S1 stars.
- Stars from outside the halosphere surface may or may not be metalrich.
- Metalrich stars engorge as they move toward the kaosphere -
- Their isotopes overengorge.
- Their isotopes dissipate to superphotonics.
- The stars are metalpoor before they reach the kaosphere surface.
Halosphere star nurseries
- Halosphere star nurseries are dense clouds of superphotonics -
- Star nursery content is mostly protons -
- Deuteriums and heliums may or may not be present.
- Halosphere star nursery content is sourced -
- Primarily: star nursery content is polar jet discharge or byflow -
- Discharge -
- When the jets do not breach the halosphere surface -
- Galaxies with lower understability.
- Byflow -
- When the jets breach the halosphere surface -
- Galaxies with higher understability.
- Secondarily: star nursery content is downflow or upflow -
- Downflow -
- Superphotonics absorbed from outside the halosphere surface.
- Upflow -
- Superphotonics ejected from the kaosphere.
- Halosphere star nurseries mostly form in the outer halosphere -
- Star nurseries move with the teelstream system toward the equator.
- Star nurseries downwell with the teelstream system -
- Into the chaotic inner halosphere to disperse -
- Insubstantial star nurseries disperse before they downwell.
- Halosphere star nurseries may or may not endure -
- Star nursery endurance is prolonged by either -
- Rapid growth to a substantial mass.
- Continuing content replenishment by the jets, replacing that downwelling.
|
VOIDOSPHERE ???????
- A gravitysheath has two regions:
- A G3gravitysheath interface's position relative to the surface of the teelosphere dictates the stability of the galaxy.
- Overstable:
- The surface of the teelosphere is wholly inside the gravitysheath interface.
- Stable:
- The surface of the teelosphere and the gravitysheath interface coincide.
- Understable:
- The surface of the teelosphere partly or wholly extends across the gravitysheath interface.
|
LIFECYCLE
A G3GALAXY FORMS WHEN A G2GALAXY ACCRETES A G1GALAXY.- A G2quarkcore consists of one G2axiquark and one G2centriquark.
- A G2quarkcore is stable.
- The G2quarks are understable and engorged.
- A G1quarkcore consists of a single G1centriquark.
- A G1quarkcore is stable.
- A G1quark is stable and not engorged.
|
AS FIRST FORMED, THE QUARKCORE OF A G3galaxy CONSISTS OF:
- one G1centriquark,
- one G2centriquark,
- one G2axiquark.
EACH OF THE QUARKS IS INSIDE ITS OWN TEELOCEAN
- Each teelocean is a teelstream system.
- Centriquarks have centrifugal teelstream systems.
- Axiquarks have axial teelstream systems.
THE QUARKS ARE STRONGFORCED TOGETHER THUS:
- Held together by their mutual gravitypull.
- Held apart by the mutual repellence of their teeloceans.
THE AURASPHERE IS THE TWO PREVIOUS AURASPHERES CONJOINED
- The G1aurasphere was a centrifugal teelstream system.
- The G2aurasphere was an axial teelstream system.
- The G3aurasphere is chaotic.
- The G3aurasphere is understable.
THE QUARKCORE CONFIGURATION IS STRESSED
- The quarks are three different sizes.
- The quarks are three different masses.
- The quarks are overstable and thus:
- Their teelospheres are tightly bound.
- Their teelospheres are very repellent.
- The axiquark and centriquark teelospheres mismatch do the quarks tumble about each other.
THE QUARKCORE ADOPTS ITS LEAST STRESSFUL CONFIGURATION
- The least stressful configuration is neutronic thus:
- The centriquarks are bound pole to pole
- Their equators cant toward the quarkcore northpole.
- They are dual spinning.
- Each around its own axis.
- Each around their mutual masscentre.
- The axiquark southpole is lodged north of the canted centriquark equators.
- It is spinning around its axis.
- The axiquark northpole is the northpole of the quarkcore.
- The quarks are overstable and thus teel interchange between them is minimal.
THE QUARKCORE'S LEAST STRESSFUL CONFIGURATION CANNOT ENDURE
- The quarkcore is overstable.
- The aurasphere is understable.
THE QUARKCORE ABSORBS TEELS FROM THE AURASPHERE
- Per the energy/mass differential mechanism
- More energyvelocity is absorbed than massvelocity.
- More energy and mass is absorbed than is ejected.
- The energy, mass and size of the quarks increases.
- The centriquarks equalise their energy, mass and size.
- The quarks become stable
- The quarkcore is not yet stable.
- The quarkcore continues to absorb teels.
- The quarks continue to absorb teels.
- The quarks become understable.
- The quarks become increasingly understable.
- The quarkcore is still not yet stable.
THE QUARKCORE'S LEAST STRESSFUL CONFIGURATION IS OVERSTRESSED
- The quark teelstream systems rearrange.
- The axiquark teelstream system becomes centrifugal.
- The axiquark is now a centriquark.
- The centriquark teelstream systems become axial.
- The centriquarks are now axiquarks.
THE QUARKCORE'S STRUCTURE IS TRANSMUTED FROM NEUTRONIC TO PROTONIC
- The axiquarks are bound equator to equator.
- Their northpoles are canted inward.
- Their southpoles are canted outward.
- Each around its own axis.
- Each around their mutual masscentre.
- Their northpoles face the quarkcore northpole.
- The axiquarks are a torus.
- The centriquark is lodged between the outward canted southpoles of the axiquarks.
- Its equator is aligned with the quarkcore axis.
- Its capricorn-tropic faces the axiquark southpoles.
- It is spinning around its axis.
THE QUARKCORE'S PROTONIC LEAST STRESSFUL CONFIGURATION IS UNDERSTABLE
- The quarks are understable.
- Understable quarks eject teels.
- The axiquarks eject teels at their northpoles.
- Ejections from the canted northpoles coalesce to form a polar jet.
- The polar jet is emitted into the aurasphere.
- The centriquark ejects teels at its equator.
- The equatorial north ejects teels into the axiquark torus.
- The teels pass through the torus and are emitted.
- The emitted teels conjoin with the axiquark polar jet.
- The equatorial east, south, and west teel ejections are directly into the aurasphere.
* * * * *
THE AXIQUARK TORUS IS THE QUARKCORE'S STABILISATION TURBINE
- The stabilisation turbine is a compressor, a choke, and an exhaust.
- Teels flowing through the turbine are a teelstream.
- The compressor accelerates the teelstream, compresses it, and laterally spins it.
- The choke reduces the teelstream to its smallest lateral diameter.
- The expansion is aerospiked by the outflow from the axiquark northpoles into a coherent jet.
- This is the northern polar jet.
- The northern polar jet is the quarkcore's primary stabilisation mechanism.
- The southern polar jet (see below) has less heft, less coherence, and less importance.
* * * * *
THE AURASPHERE IS UNDERSTABLE
- The aurasphere teelstream system is chaotic.
- It is ejecting teels randomly into the teelosphere.
- It is ejecting teels randomly into into the quarkcore.
THE QUARKCORE RESISTS TEEL ABSORPTION FROM THE AURASPHERE
- The quark teeloceans resist absorption from the aurasphere.
THE QUARKCORE'S EQUATOR IS A WEAKPOINT IN THE RESISTANCE TO TEEL ABSORPTION.
- The axiquark southpoles and the centriquark capricorn-tropic face each other at the equator.
- They repel each other strongly.
- The axiquarks are spinning around their mutual masscentre.
- The centriquark is spinning around its axis.
- The mutual gravitypull of aurasphere and the quarkcore is strong.
- The aurasphere is chaotic, dense, and energetic.
- The cannot prevent aurasphere teels forcing in between the axiquarks and the centriquark.
- The weakpoint is an annular intake.
- The heft of the teels entering the intake is commensurate to aurasphere understability.
THE AURASPHERE ENTERS THE QUARKCORE TO FORM THE NORTHERN POLAR JET- The aurasphere teels coalesce with the north centriquark equatorial ejection.
- They form a teelstream.
- The heft of the combined teelstream is commensurate with the understability of the nucleus.
- The teelstream the stabilisation turbine.
- In the turbine it is accelerated, compressed, and given a lateral spin.
- It emerges from the turbine exhaust into the teel ejections from the understable axiquarks.
- The axiquark ejections aerospike the teelstream to become the northern polar jet.
- The heft of the northern polar jet increases commensurately with the understability of the nucleus.
THE NORTHERN POLAR JET DISCHARGES OUTSIDE THE NUCLEUS
- The reach of the northern jet increases with the understability of the nucleus.
- The reach of the northern jet is modified by the stability of the galaxy.
- With an understable nucleus and an overstable galaxy, the discharge is into the teelosphere.
- With an understable nucleus and a stable galaxy, the discharge is into the teelosphere.
- With an understable nucleus and an understable galaxy, the discharge is beyond the teelosphere.
- Depending
on the understability of the galaxy, the discharge can be into the
outer gravitysheath or across the gravitysheath interface.
AN UNDERSTABLE NUCLEUS ALSO FORMS A SOUTHERN POLAR JET- The quarks in an understable nucleus are understable.
- The centriquark is understable.
- The centriquark absorbs teels from the aurasphere.
- The centriquark ejects excess teels equatorially.
- The north equatorial ejection is into the axiquark torus.
- The east west and south equatorial ejection is ejected into the aurasphere.
- The aurasphere resists the ejection and marshals the ejection toward the southpole.
- The greater the aurasphere understability, the more forceful the marshalling.
- The aurasphere, when sufficiently understable, marshals the ejection into a southern polar jet.
- The heft of the polar jet is less than that of the northern polar jet.
- The speed, compression, and lateral spin of the southern polar jet is less than that of the northern polar jet.
- The southern polar jet, when the galaxy is sufficiently understable, can discharge beyond the galaxy teelosphere.
* * * * *
THE NUCLEUS STABILISES
- Aurasphere teels stream into the quarkcore.
- Aurasphere teels combine with teels ejected by the quarkcore as a single teelstream.
- The teelstream enters the stabilisation turbine.
- The teelstream emerges from the stabilisation turbine as the northern polar jet.
- The northern polar jet discharges excess teels outside the teelosphere.
- Per
the energy/mass differential mechanism, the discharged teels
differentially remove energyvelocity and massvelocity from the nucleus.
- The discharging continues until the nucleus is stable.
- When the nucleus is stable, the discharging stops.
THE STABILISATION IS A COLLAPSE- The northern polar jet is discharging teels from the nucleus outside the galaxy teelosphere.
- The jet is differentially discharging energyvelocity and massvelocity.
- The quark masses decrease as they differentially eject energyvelocity and massvelocity.
- The quark volumes contract commensurately.
- The quarkcore mass decreases as quark masses decrease.
- The quarkcore's volume contracts commensurately.
- The aurasphere responds to the contraction in quarkcore volume.
- The aurasphere is gravitypulled into the space vacated by the contracting quarkcore.
- The aurasphere volume contracts commensurately.
- The aurasphere is simultaneously contracting due to teel loss.
- The bulge responds to the contraction in aurasphere volume.
- The bulge stars are gravitypulled into the space vacated by the contracting aurasphere.
- The bulge emits a stabilising photonic flash.
- The bulge stars move toward the aurasphere.
- Potentialspeed transmutes to speed.
- The bulge star overengorgement increases.
- Photon emissions increase commensurately.
- There is an intense, relatively brief, photonic flash.
- The flash exceeds the galaxy's normal photonic output and is detectable at a distance.MORNING
THE NUCLEUS STABILISES- The quarkcore stabilises.
- The quarkcore is in engorgement stasis.
- The quarks are understable and engorged.
- The quarkcore is a closed cycle.
- The quark teelstream systems circulate in harmony.
- The massdensity of the aurasphere is not enough for penetration to the stabilisation turbine.
- The stabilisation turbine does not discharge into the aurasphere.
- The aurasphere stabilises.
- The aurasphere volume is constant.
- The interface with the bulge is constant.
- The aurasphere teelstream system is axial overall.
- It was made axial by the jet.
- It retains its axiality.
THE NUCLEUS IS NEVER TRULY STABLE- Bulge stars are overengorged and dissipating.
- Bulge content is continually gravitypulled into the aurasphere.
- Subphotonics, stripped neutrons, stripped deuteriums, and stripped heliums.
- The bulge content understabilises the aurasphere.
- Understabilisation restarts the stabilisation turbine.
- The understable aurasphere penetrates the quarkcore.
- The penetration starts the stabilisation turbine.
- The stabilisation turbine emits a polar jet.
- The polar jet discharges into the galaxy teelosphere.
- The G3galaxy is a closed system.
THE GALAXY AS A CLOSED SYSTEM
- If the polar jet discharges into the lower teelosphere, the galaxy is overstable.
- An overstable galaxy is a closed system.
- If the polar jet discharges into the upper teelosphere, the galaxy is stable.
- A stable galaxy is a closed system.
- The closed system of a stable galaxy is thus:
- Polar jet content coalesces and accretes in the upper teelosphere.
- Stars and star clusters form.
- The stars and the star clusters are gravitypulled into the bulge.
- In the bulge, the stars and the star clusters are overengorged and dissipated.
- The dissipation debris is gravitypulled into the aurasphere where it is further dissipated into teels.
- The teels are penetrated into the quarkcore's stabilisation turbine.
- The stabilisation ejects the teels as a polar jet into the upper teelosphere.
- The stable closed system cycles and recycles until something happens to change it..
THE GALAXY AS AN OPEN SYSTEM
- A stable galaxy endures in isolation.
- Isolation for a galaxy is, relative to a benchmark, temporary.
- Lesser galaxies and other lesser content abound in the outer gravitysheaths of galaxies.
- When a stable galaxy absorbs content from beyond its teelosphere:
- Its mass increases.
- Its energyvelocity and massvelocity increases differentially.
- It becomes understable.
- Its closed system becomes an open system.
- In an open system, the polar jet discharges beyond the teelosphere.
- The polar jet continues to discharge beyond the teelosphere until the galaxy is stable once more.
- Stability for a galaxy is, relative to a benchmark, temporary.
THE LIFECYCLE END FOR A G3GALAXY. |
|
|
|
Comments and suggestions:
peter.ed.winchester@gmail.com
Copyright 2022 - Sian Luise Winchester
|
|
|
|