Ајде да ги видам доказите. Кога е докажано дека не постои Бог кој бил координатор на тој проект и со кои единици мерки е измерено дека не постои Бог

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Сега ќе биде дечко не по 20 години, кај да е ќе го пуштат пак акцелераторот во Швајцарија, минатиот пат масло му немаа турено па му зариба на кривина


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1) the universe has evolved
2) we are a result of that evolution.
“We are the first generation of human beings to glimpse the full
sweep of cosmic history, from the universe's fiery origin in the Big
Bang to the silent, stately flight of galaxies through the intergalactic
night.
Order in the Universe
Cosmology is the study of the evolution of the universe from its first moments to
the present. In cosmology the most fundamental question we can ask is: Does our
universe have intelligible regularities that we can understand—is it ordered? This
question lies at the heart of the scientific revolution beginning in the sixteenth century.
That revolution began with the discoveries by Copernicus, Galileo, and Newton of order
in our world. Today our scientific understanding of nature’s order has reached a critical
threshold. Only now can we begin to piece together a coherent picture of the whole.
Only now can we begin to see the deep order of our universe.
понатаму.....
By determining how fast the universe is expanding now, and then "running the
movie of the universe" backwards in time, we can determine the age of the universe.
The result is that space started expanding 13.7 billion years ago. This number has now
been experimentally determined to within 1% accuracy.
It's a common misconception that the entire universe began from a point. If the
whole universe is infinitely large today (and we don't know yet), then it would have
been infinitely large in the past, including during the Big Bang. But any finite chunk of
the universe—such as the part of the universe we can observe today—is predicted to
have started from an extremely small volume.
Part of the confusion is that scientists sometimes use the term "universe" when
they're referring to just the part we can see ("the observable universe"). And sometimes
they use the term universe to refer to everything, including the part of the universe
beyond what we can see.
It's also a common misconception that the Big Bang was an "explosion" that took
place somewhere in space. But the Big Bang was an expansion of space itself. Every
part of space participated in it. For example, the part of space occupied by the Earth, the
Sun, and our Milky Way galaxy was once, during the Big Bang, incredibly hot and
dense. The same holds true of every other part of the universe we can see.
We observe that galaxies are rushing apart in just the way predicted by the Big
Bang model. But there are other important observations that support the Big Bang.
Astronomers have detected, throughout the universe, two chemical elements that
could only have been created during the Big Bang: hydrogen and helium. Furthermore,
these elements are observed in just the proportions (roughly 75% hydrogen, 25%
helium) predicted to have been produced during the Big Bang. This is the
nucleosynthesis of the light elements. This prediction is based on our well-established
understanding of nuclear reactions—independent of Einstein's theory of gravity.
Second, we can actually detect the light left over from the era of the Big Bang.
This is the origin of the cosmic microwave background radiation. The blinding light that
was present in our region of space has long since traveled off to the far reaches of the
universe. But light from distant parts of the universe is just now arriving here at Earth,
billions of years after the Big Bang. This light is observed to have all the characteristics
expected from the Big Bang scenario and from our understanding of heat and light.
The standard Hot Big Bang model also provides a framework in which to
understand the collapse of matter to form galaxies and other large-scale structures
observed in the Universe today. At about 10,000 years after the Big Bang, the
temperature had fallen to such an extent that the energy density of the Universe began to
be dominated by massive particles, rather than the light and other radiation which had
predominated earlier. This change in the form of matter density meant that the
gravitational forces between the massive particles could begin to take effect, so that any
small perturbations in their density would grow. Thirteen point seven billion years later
we see the results of this collapse in the structure and distribution of the galaxies.
пази гокииииииии НЕМА МАГНЕТИЗАМ!!!!!!!!!
Dr. Allan Sandage, the Carnegie Observatories astronomer, once called
cosmology "the search for two numbers" The first number is the Hubble constant, which
tells how fast the universe is expanding. Together with the other number telling how fast
the expansion is slowing, they determine whether the universe will expand forever or
not.
The second number, known as the deceleration parameter, indicates how much
the cosmos had been warped by the density of its contents. In a high-density universe,
space would be curved around on itself like a ball. Such a universe would eventually
stop expanding and fall back together in a big crunch that would extinguish space and
time, as well as the galaxies and stars that inhabit them. A low-density universe, on the
other hand, would have an opposite or "open" curvature like a saddle, harder to
envision, and would expand forever.
In between with no overall warpage at all was a "Goldilocks" universe with just
the right density to expand forever but more and more slowly, so that after an infinite
time it would coast to a stop. This was a "flat" universe in the cosmological parlance,
and to many theorists the simplest and most mathematically beautiful solution of all.
This solution has now been confirmed by the Wilkinson Microwave Anisotropy Probe.
ПАЗИ ТУКА
It is now thought that Omega (
Ω), the ratio of the density of matter in the universe
to the density of matter required for a flat universe, is equal to one. That is, the universe
is flat so it will expand forever but more and more slowly, so that after an infinite time it
will coast to a stop.
ете го твојот магнетизам во центарот бе тууууу:t app:
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