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Darkmatter Selfproofs |
SELFPROOF 0505
- GLOBULAR CLUSTERS
CURRENT COSMOLOGY MODEL
A
globular cluster is a spherical collection of stars that orbits a
galactic core as a satellite. Globular clusters are very tightly
bound by gravity which gives them their spherical shapes and
relatively high stellar densities toward their centres. Globular
clusters, which are found in the halo of a galaxy contain
considerably more stars and are much older than the less dense
galactic, or open clusters, which are found in the disk.
Every
galaxy of sufficient mass in the Local Group has an associated group
of globular clusters, and almost every large galaxy surveyed has been
found to possess a system of globular clusters. The Sagittarius Dwarf
and Canis Major Dwarf galaxies appear to be in the process of
donating their associated globular clusters to the Milky Way. This
demonstrates how many of this galaxy's globular clusters might have
been acquired in the past.
Although
it appears that globular clusters contain some of the first stars to
be produced in the galaxy, their origins and their role in galactic
evolution are still unclear. It does appear clear that globular
clusters are significantly different from dwarf elliptical galaxies
and were formed as part of the star formation of the parent galaxy
rather than as a separate galaxy. However, recent conjectures by
astronomers suggest that globular clusters and dwarf spheroidals may
not be clearly separate and distinct types of objects. (Wikipedia 19
Aug 2012)
Globular
clusters, which are found in the halo of a galaxy contain considerably
more stars and are much older than the less dense galactic or open
clusters, which are found in the disk. Globular clusters are fairly
common; there are about 150 to 158 currently known globular clusters in
the Milky Way, with perhaps 10 to 20 more still undiscovered. Large
galaxies can have more: Andromeda, for instance, may have as many
as 500. Some giant elliptical galaxies, such as M87, have as many as
13,000 globular clusters. These globular clusters orbit the galaxy out
to large radii, 40 kiloparsecs (approximately 131,000 lightyears) or
more. (Wikipedia08 Jun 2014)
MALTA COSMOLOGY TEMPLATE
- Every
blackhole in the Universe is within the gravitysheath of a larger
object. (see Argument 0336)
- Many blackholes are within the teelospheres of larger objects.
(see Argument 0337)
- Blackholes absorb teels from the teelosphere they are within which
alters the blackhole's measures of mass and energy. (see Argument 0338)
- A
stable blackhole within the teelosphere of a larger object becomes
understable due to the differential absorption of mass and energy
from the teelosphere. The stability of already overstable or
understable blackholes alters commensurately. (see Argument 0339)
- A
stable blackhole within a teelosphere, made understable through the
differential absorption of mass and energy, ejects more than it
absorbs until it returns to stability. The stability of already
overstable or understable blackholes alters commensurately. (see Argument 0340)
- The
average realspeed of the teels in a teelosphere decreases with
distance from its parent object's centre of gravity. (see Argument 0341)
- A
stable blackhole moving toward the centre of gravity of the
teelosphere it is within maintains its stability by differentially
losing mass and energy, thus decreasing its ratio of energy over
mass. (see Argument 0342)
- A
stable blackhole moving away from the centre of gravity of the
teelosphere it is within maintains its stability by differentially
gaining mass and energy, thus increasing its ratio of energy over
mass. (see Argument 0343)
COMMENTARY
- Globular
clusters are galaxies, protogalaxies, or starclusters.
- Globular clusters either circulate within, or are passing through, a larger galaxy's gravitysheath interface.
- Every globular cluster has its own gravitysheath and gravitysheath interface.
- Every globular cluster has an accretion of understable stars which form the cluster's "blackhole core".
- Every globular cluster's blackhole core is surrounded by a teelosphere.
- Every
star within a globular cluster has its own blackhole core, its own
teelosphere, its own gravitysheath, and its own gravitysheath
interface.
- A typical galaxy contains numbers of clusters, sometimes a great many of them.
- A typical visible galaxy galaxy is understable and thus shedding fast teels from its
teelcore as it seeks stability.
- A typical understable galaxy has a dense and energetic
teelosphere.
- Typically, a galaxy's teelosphere teelstreams are denser
and more energetic than the teelosphere teelstreams of its globular clusters.
- Consequently the galaxy teelosphere engorges the teelospheres of the globular clusters.
- Consequently the teelospheres of the globular clusters are diminished as the fastest teels escape.
- The teelosphere of a globular cluster protects the teelospheres of the stars within.
- If
the teelosphere of a globular cluster is diminished, the teelospheres
of the stars within are exposed to the energy and density of the
teelosphere of the galaxy outside.
- Consequently the galaxy teelosphere now engorges the teelosphere of the stars within the globular cluster.
- Consequently the teelospheres of the stars within the globular clusters are diminished as the fastest teels escape.
- The stars in a globular cluster are densely packed, especially at the centre.
- In
part this dense packing is enabled by the dense and energetic
teelospheres that surround stars in a globular cluster. (The same
effect is seen in the densely packed stars at a galactic centre (see Selfproof C0504) and in the dense packing of quarks within an electron on nucleon (the strong force).)
- The
teelosphere of the galaxy diminishes the teelospheres of the stars
within the globular cluster which in turn reduces their rejectivity vis
a vis other stars.
- With
the reduced rejectivity of the stars within a globular cluster, they
cannot help but be drawn closer together by their mutual
gravitypull.
- The teelosphere of a star is a consequence of activity within its blackhole core.
- However, it also provides protection for that blackhole core.
- When
the teelosphere of a star within a globular cluster is diminished by
the teelosphere of the galaxy, the protection of the blackhole core is
also diminished.
- The
engorgement of the star's teelosphere leads to the engorgement of the
teelosphere of the nucleons that are the star's blackhole core.
- Consequently the teelospheres of the star's nucleons is diminished.
- The diminishing of the teelospheres of the nucleons reduces their rejectivity.
- Consequently the nucleons pack more densely due to their mutual gravitypull.
- Packing nucleons more densely leads to nuclear fusion.
- Consequently the stars become"low-metal" stars.
- In
the Current Cosmology Model, globular cluster stars are thought to be
old when compared to the overall age of the stars in the galaxy
outside.
- In
the Malta Cosmology Template, globular cluster stars are "aged" through having
their teelospheres, and the teelospheres of their nucleons, diminished.
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GLOSSARY
- galaxy:
A galaxy is a high mass blackhole. As with all
blackholes, a galaxy can be overstable, stable, or understable. A
galaxy consists of a solidbonded teelcore, (perhaps) a liquidbonded
teelocean, and a gasbonded teelosphere. An overstable or stable galaxy
may or may not be "bald". An understable galaxy is unlikely to be bald,
Instead it will be surrounded by stars, gas, and dust. Depending on the
mass of the teelcore, an understable galaxy can be elliptical, spiral,
or dwarf elliptical.
- protogalaxy:
A protogalaxy is an accretion of stars and/or dust and/or gas
held together by mutual gravitypull. A protogalaxy doesn't have a
dominant blackhole but it does have the sufficiently high
mass and the sufficiently low energy needed to evolve one.
- starcluster: A starcluster
is an accretion of stars, together with any associated dust and gas
that is held together by mutual gravitypull. A starcluster doesn't have
a dominant blackhole. Nor does it have mass and energy measures
sufficient to evolve one.
- strong force:
(Also known as the "strong interaction") (1) The
interaction responsible for binding quarks, antiquarks, and gluons to
make hadrons. Residual strong interactions provide the nuclear binding
force (particleadventure.org). (2) The force that binds two
blackholes (quarks) together within an electron and three blackholes
(quarks) together within a nucleon. The strong force is a multiprocess
in which the mutual gravitational attraction of the quarks is countered
by the rejectivity of their teelospheres.
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