The structure of the universe --- the
structure of the particles - the structure of life (human special high-level
wisdom of life form) ----- natural universe eternal great topic (FangRuida)
What is the structure of the
galaxy outside the galaxy
Human vision and observable cosmic
spatial homogeneity and heterogeneity
Overview of the cosmic panorama
Macro universe
Microcosmic universe
Elements and particles
Galaxies dust particles "black
hole" "white hole", dark matter, big bang, steady state and variants
of antimatter between objects of cosmic stars
Interplanetary interplanetary interlocking
mechanism of space interplanetary space cosmic space network intermodal network
basic expression
Super universe super - super - interstellar
material super - interstellar structure functional network
Gravitational gravitational field
gravitational wave cosmic kinetic energy
The initial state of the universe, the
final state and the basic modal mathematical expression
Particle initial state, final state and
basic expression, mathematical expression
** Substance - species - organic matter -
inorganic - intermediate life generation and evolution of the basic conditions
of life
Animal-animal evolution of the various options
- monkey to human evolution of the spontaneous combustion of the particularity
and inevitability of the long evolutionary process, a variety of evolutionary
species of competition and natural selection of human evolution of the
particularity
** In the natural universe the universality
of particles and substances produced by the inevitability of spontaneous
combustion of animal life and evolution of the objectivity and natural life in
the universe of necessity and particularity of advanced intelligence life and
low-level extreme microbial survival
* Super-spin - super-dynamic - super-spin -
super-spin vector - ultra-polar field ------- the basic static static, dynamic
mode
Silver ball heart
Helical arm man - bottom arm ▪ shield -
south cross arm ▪ ruler - swan arm ▪ angel arm ▪ hunting arm
Silver halo silver crown
. Kepler's third law: T2 / R3 = K (= 4π2 /
GM) {R: orbital radius, T: period, K: constant (independent of the mass of the
planet, depending on the quality of the center celestial body)}
2. Gravitational law: F = Gm1m2 / r2 (G =
6.67 × 10-11N? M2 / kg2, the direction of their connection)
3. Gravitational and gravitational
acceleration: GMm / R2 = mg; g = GM / R2 {R: celestial radius (m), M: celestial
mass (kg)}
(GM / r3) 1/2; T = 2π (r3 / GM) 1/2 {M:
center celestial mass }
The first (second, third) cosmic velocity
V1 = (g = r) 1/2 = (GM / r) 1/2 = 7.9km / s; V2 = 11.2km / s; V3 = 16.7km / S
6. Earth Synchronous satellite GMm / (r =
h4) = 2, m4π2 (r = h) /
T2 {h ≈ 36000km, h:
height from the Earth's surface, r: radius of the earth}
Cosmic physics, physical cosmology,
cosmology, gravity and relativity: general theory of relativity; astrophysical
relativity. (2) classical cosmology: isotropic universe; gravitational lens;
age and distance scale. (3) Quantum field basis: quantum mechanics and
relativity; quantum field theory; standard model. (D) early universe: hot big
bang; topological loss; expansion cosmology. (5) observing cosmology: matter in
the universe; galaxies and their evolution; running galaxies. (6) galaxy
formation and formation: structural formation dynamics; cosmic density field;
galaxy formation; cosmic background ups and downs
Launching the Nebula The Lagoon Nebula ▪ North America Nebula
Reflecting Nebula Variation Nebula ▪
Diffuse Nebula ▪ Witch Nebula
Dark Nebula Coal Bag Nebula ▪ Horse Head
Nebula ▪ Dark Horse Nebula
Spider Cluster Butterfly Cluster ▪
Butterfly Cluster ▪ M52 ▪ Pleiades Cluster
Globular cluster Centaurus ▪ Rhododendron
47 ▪ M5 ▪ M19 ▪ M54 ▪ M75 ▪ M80 ▪ Paloma 5 ▪ Paloma 12
Star Alliance
OB Star Association ▪ T Star Association ▪ R
Star Association
Ant Nebula ▪ Eskimo Nebula ▪ Spiral Nebula ▪
Respirator Nebula ▪ Hourglass Nebula ▪ NGC 3132
Sagittarius Stellar Clouds ▪ Magellan Star
Streams ▪ Centaurus Dwarf Galaxy ▪ Kirin Seat
Ring ▪ Virgo Star Stream ▪
Gould band ▪ Local bubble ▪ The
interstellar cloud
Evolution of the concept of elements The oldest
philosophers believe that all the material is composed of a few elements that
are air, soil, fire, water, and some that the element is the four most
primitive properties (heat, Cold, dry, wet) constitute a combination of all
things. The first scientific definition for the chemical element is the British
R. In 1661, he pointed out in the book "The Paintist Chemist" that
"they (elements) should be something that is not made up of any other
substance or that is composed of the original and the simplest ";"
Should be some of the nature of a certain, real, can be perceived in kind, with
the general chemical method can not be broken down into some of the more simple
kind. " With the emergence of atomic theory and atomic structure theory,
it is clear that the main factors that determine the nature of chemical
elements are the number of electrons outside the nucleus and the number of
nuclear charges have elucidated the modern definition of the essence of
elements: "the same kind of atoms with the same nuclear charge The general
name. "
The origin of the chemical element {the
origin of the chemical element and the evolution of the particle-cosmic
structure are closely related. Regardless of physics, regardless of chemistry,
physical chemistry, chemical physics, particle structure, element origin,
cosmic origin, often connected together. Although the scope of the study is
different, but the link is very tight. Vertical profile, cross-section,
three-dimensional profile, multi-dimensional perspective study to understand
its mystery. Before the production of various chemical elements and the
generation of particles change can not be completely separated. That is, one of
the issues of particular importance to cosmic physics and cosmic chemistry. }
"The proton fusion and neutron capture
are two main processes in the formation of chemical elements in the
universe." This hypothesis holds that all elements of the universe
originate from hydrogen, which is very high (Lithium, boron, beryllium, etc.),
this process is proton fusion, followed by the formation of heavy nuclei, the
first is helium, followed by light elements (lithium, boron, beryllium, etc.)
Helium atoms bombard the elements of the light element, it will produce
neutrons, these neutrons are light element nucleus capture, the formation of
heavier elements, from carbon, nitrogen, iron until the atomic number of 82 and
83 lead and bismuth, This process is neutron capture. The two elements of the
process of generating elements still continue within the stars.
There are only a few chemical elements
present in the free state
The Milky Way is the solar system where the
solar system is located, including 1500 to 400 billion stars and a large number
of stars, nebulae, and various types of interstellar and interstellar dust,
black holes, and its total mass is 210 billion times the mass of the sun.
Outer galaxies are outside the Milky Way,
composed of a large number of stars, but because of the distance, in the
appearance of the performance of the fuzzy spots, which is also known as
"river nebula." People have observed about 1 billion galaxies similar
to the Milky Way. According to their shape and structure, can be divided into:
spiral galaxies, rods galaxies, elliptical galaxies and irregular galaxies. It
is estimated that the total number of galaxies outside the river in more than
100 billion. (Wikipedia website, Wikipedia)
Outside the galaxy - the total galaxy (the
breadth of the universe): the naked eye and the unobtrusive galaxy outside the
galaxy, the total galaxy range: planets, celestial bodies, interstellar
material, dust, nebula, clusters, galaxies, black holes. The The The The The
The The The Etc., etc. {Astrophysics, celestial chemistry, cosmic physics,
cosmic chemistry, galactic physics, galactic chemistry, extraterrestrial
galaxies physics, extraterrestrial galaxies chemistry The The The The The The
The In any case, for human beings, how the extraterrestrial galaxies and the
extraterrestrial galaxies are directly connected to the galaxy and the universe
are very important. The chemical abundance of the universe, the physical
homogeneity or heterogeneity of the universe, is essential for the astronomy
cosmology science. The extraterrestrial galaxies and the total galaxies need
great exploration and exploration of human beings, but it is very difficult.
Theoretical hypotheses can be created, but this does not represent the true
universe of the whole picture. In fact, regardless of the solar system,
galaxies, galaxies, clusters, galaxies, extraterrestrial galaxies, interstellar
material, nebula, black hole ------- and so on, many changes in physical
chemistry, and difficult to be recognized by human beings, or Is mysterious and
mysterious so many unknowns. Crack these mysteries, it is not easy.
Interstellar chemistry: It is also
important to observe and confirm astronomical molecules (cosmic chemistry,
astrophysics, cosmic chemistry, interstellar chemistry, and so on, involving
all aspects of the chemical universe.) As with cosmic physics, cosmic chemistry
is extremely important, Moon Science, Lunar Chemistry, Mars Chemistry,
Geochemistry, Galaxy Chemistry, Hetai Galaxy Chemical Physics, etc.).
Cosmic chemistry is divided into several
aspects according to celestial bodies and research methods: meteorite
chemistry: the chemical composition of various meteorites. Planetary chemistry:
studies the chemical composition and chemical evolution of planets (including
earth), satellites, asteroids, meteoroids, comets, and interplanetary
substances;
Stellar Chemistry: Study the chemical
composition of stars and their chemical evolution. The sun is the nearest star
from the people, and accounts for 99.86% of the total mass of the solar system.
Therefore, solar chemistry is of great significance to the study of stars and
the solar system.
Interstellar chemistry: the main
observation and identification of interstellar molecules, to study their
formation and disintegration; other chemical branches and cutting-edge
research, and so on.
particles - the beginning
of the super-particles
The beginning and ending of
the universe
the end of the species
The outcome and evolution
of animals and advanced wisdom
Survival and development of
rare species and high intelligence in the solar system
Earth - Moon - Mars -
Jupiter - Venus - Mercury - Saturn Jupiter in the solar system in the special
status and significant role
Galactic structure and basic structure
Galaxy outside the universe
of large scale cosmic small scale universe
the reality and possibility
of human migration on the moon, Mars and other stars
The basic outline of the
future world planet society The basic survival mode of the planet society
Survival Mo Modes Planetary society management and operation Planetary society
interpersonal relationship Planetary society Basic framework Planetary society
Natural selection (500 - 1000 years time, 5-10 The process of the century or
longer)
human flying out of the
solar system, can survive in the Galaxy? Galaxy Planet Can humans survive
human nature and social
properties of evolutionary genetic and variation
planet and the collapse of
the universe after the collapse of the destruction of the universe is all gone,
everything is empty, completely back to the origin?
Natural science, natural
philosophy - philosophy and social sciences, permanent subjects, constantly
refreshing the natural study of great philosophy or natural philosophy can not
replace the most realistic existence of natural science research and detection
of various discoveries. And even if any major scientific discovery will
inevitably be a slightest flaw or fallacy. Thus, the understanding of
understanding the universe, the material - the particle - life, requires
constant innovation and continuous development. Zeus, God of War, the moon, and
gradually be recognized by human understanding. Tens of millions of years
later, if the human beings still exist, we will today's awareness and discovery
as a laughing stock or joke, as far away from the ancient ancient culture of ancient
ancient.
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