How Big is the Universe?
How
Big is the Universe?
For
the understanding of the structure of the Universe – the outer world, or the
Sky – the same role as Aristotelis system for the structure of matter was
played by the Ptolemaic geocentric system of SPHERES.
According
to it, the Universe reminds the well-known Russian doll – matrioshka. It is a
set of moving spheres, placed one inside the other and the Earth is resting in
the center of the construction (like the egg yolk). The size of the
Universe is comparable to the Earth alone.
Each
sphere was considered to be solid, transparent and carrying just one attached
to it planet – Moon, Mercury, Venus, Sun, Mars, Jupiter, Saturn and the sphere
carrying all the rest of immovable stars.
All spheres are circling around the Earth with
less (for the Sun, the Moon and Stars) or more (for other planets) complicated
cyclic regularity.
The
system also included the last outer sphere – the sphere of the PRIME MOOVER –
which was understood as the source of any motion noticeable at the sky.
IMPORTANT:
the size of the Universe in this system is comparable to the Earth alone (!)
In
the first half of 16-th century Polish astronomer, priest, doctor,
fortification engineer, mathematician and amateur astronomer Nikolai Copernicus
(in Polish Mikolaj Kopernik, 1473-1543) proposed the system, which
mathematically looked much simpler: in his system the Sun was placed in the
center and the Earth became just one of the planets with only Moon circling
around it.
This
system was really a problem for the Catholic Church, as it RELEGATED the Earth
down to the level of one of many Planets.
Kopernik
himself, being the catholic priest, understood it very well. That is why he was
not in a hurry to publish his research. His book De revolutionibus orbium
coelestium was published in Nuernberg (Germany) just several days before his
death. It has a FOREWORD, where the author (or, probably, one of his disciples
Retic) specially noted that the book contains just the description of a new
mathematical approach to calculate the orbits of planets, which is much simpler
than the old one, and that is all. NO REVOLUTION!
But
the Chirch understood everything right and in 1616 forbid to all the Catholics
to study or to teach the new system.
At
the end of 16-th century the Danish astronomer Tycho Brahe (1546–1601) proposed
a compromise system – with the immovable Earth at the very center, which served
the center for the spheres of Moon, Sun and Stars, but the rest 5 spheres with
planets are circling around the Sun. This system did not contradict to Catholic
dogmas but from the mathematical point of view it preserves all the advantages
of Copernicus system.
The
revolution continued with the discoveries of Italian physicist, mathematician
and – very important – a very good glass maker – Galileo Galilei (1564–1642).
He
built very good optical tools – telescopes – which he was successfully selling
to rulers, military and seamen. And he was probably the first, who used this
tool to look at the sky! And immediately made plenty of discoveries.
1. He saw mountains and planes at the surface
of the Moon – they looked just like on Earth!
2. He definitely saw that the dark parts of the
Moon are simply in a shade (here You may see at the picture of shaded Moon,
drawn by Halileo himself). And the light, coming from the Moon, actually is the
reflection of the Sun light.
3. Finally he saw 4 more Moons, circling around
Jupiter. That was a crash for the “system of spheres”! How many more spheres we
will need when we investigate the sky more thoroughly?
In
1624 a good friend of Galileo Matheo Barbierini was elected the new Pope (he
took the name of Urban the 8-th), and the 60 years old Galileo made a childish
mistake. Being sure that the new Pope will keep a stack hand on him, he
published in 1632 in Italian language a book in defense of the banned
Copernicus system: “The Dialogue about two Major Systems – Ptolemaic and
Copernican”.
The
result was better than could be. In 1633 he was convicted by the inquisition
court not as “heretic” but as “strongly suspected in herecy” and was not burnt
on fire (like Giordano Bruno several years before that), but just kept under
home arrest for the rest of his years.
One
year after Galileo has died (January 1642, in Arcetri, near Florence, Italy) in
Lincolnshire (England) on the 4-th of January, 1643 a child was born, named
Isaac, who’s destiny was to perform an ultimate revolution in physics,
astronomy and mathematics.
We
know this great person now as Sir Isaac Newton (1643-1727). In 1665-1666, being
still a student of Trinity College in Cambridge, the 22-23-years old Isaac,
inspired by lectures and ideas of his teacher of mathematics Isaac Barrow, as
well as by works of Galileo, Descartes, Fermat, Huygens, Wallis and other
mathematicians, has worked out the new method of mathematical computations- the
differential and integral Calculus, Which in UK and USA
universities
programs is usually denominated as simply “Calculus”. The strongest analytical
research tool the humanity ever invented! Neither before nor after Newton.
Probably this we may assume as the greatest achievement of Isaac Newton, but
not the only one!
In
September 1682 the exciting appearance of Galley comet in European sky raised
an interest to Celestial mechanics. Edmond Galley, who calculated the period
and predicted appearance of this commit proposed Newton to use his super-tool
Calculus to calculate the orbits of all planets, based on available very
detailed tables of observations and previously done calculations from Copernicus,
Johan Kepler and others.
Newton
published his results for celestial mechanics together with his general theory
of motion, which we now call the Classical (Newton) Mechanics in his
outstanding work “Mathematical Principles of Natural Philosophy” in 1686. Since
this publication all the previous “Systems of Spheres” lost any sense.
According
to Newton’s Classical Mechanics the motion of any body, having mass m. speed v
and pulse p = mv is defined by the equation (2-nd Newton’s Law):
mdv/dt
= dp/dt = F
where
F is the integral force affecting this body from other physical bodies.
dv/dt
= (v(t+dt) – v(t))/dt – is the mathematical derivative of the vector function
v(t), which by itself consists of three coordinate components, each of them
being also a derivative from corresponding coordinate.
vx(t)
= dx/dt, vy(t) = dx/dt, vz(t) = dx/dt
Thus,
knowing the coordinates and velocities of a body at some initial moment t = 0,
using the equation of the 2-nd Newton’s Law and the Calculus one can precisely
calculate what coordinates and velocities had or will have the body at any
other moment t < 0 or t > 0, given it is known, how the acting force F
depends on time and coordinates!
For
Celestial mechanics Newton assumed that the force, acting between the Sun and
each planet depends only on their masses and the distance between them, exactly
as:
F(r)=
Gm1m2/r2
and
is directed exactly along the line, connecting their centers. Here G is the
Gravitation constant, which has to be defined experimentally. Today we know
that its value is
G = 6.67•10–11 N•m2/kg2
Based
on this assumption, one can precisely calculated the orbits of all planets in
Solar system and find their shape (they are ellipses) and time characteristics
(the period of rotation for each planets depends on its average distance r from
the Sun proportional to r3/2. Everything exactly in compliance with
observations and observation tables, collected by Johan Kepler and all other
astronomers.
Only
one question remained unclear: how the gravitation force affects the body
through absolutely empty space? How it works? This question remained open until
the General Relativity Theory, created by another genius Albert Einstein
(1879–1955) in 1915, which we will discuss later.
Calculations
based on the Newton Laws and observations of astronomers allowed to define the
parameters of the Solar system and the planets in it. In short, they are listed
in a table below:
Planet Distance
from the Year (rotation Diameter, related Relative mass
Sun period around the to the
diameter of (related to the
(in astronomic Sun) Earth
= Earth mass =
units. In terrestrial years 12,74•103
km 6•1024 kg)
1 a.u. = 1,5•108 km)
0. SUN 0 - 220 3.3•105
1. Mercury 0.3
– 0.47 0.24 0.38 0,055
2. Venus 0.718–0.728 0.615 0.95 0,815
3. EARTH 1 1 1 1
4. Mars 1.38-1.52 1.88 0.532 0.107
5. Jupiter 5-5.2 11.86 11 318
6. Saturn 9-10 29.46 9.14 95
7. Uranus 18.4-20 84 3.98 14
8. Neptune 30 164,8 3.86 17
After
Newton and basing on his theory astronomers had discovered and calculated
parameters of at least two new big planets (Neptune and Uranus), very many
smaller planets, asteroids, comets and moons, circling around bigger planets.
The complete updated list and all the interesting parameters anyone can
nowadays found in reference books or on the Internet.
Just
only note some peculiar facts: The mass of the Sun exceeds the Mass of the
Earth approximately million times! And the total mass of all the planets in
Solar system makes just 0.14% percent of the mass of the whole system. The rest
99.86% belongs to the Sun. Isn’t it reminding You about atoms and their nuclei?
On
the picture to the left one may estimate the relative sizes of different
planets. On the other picture the Venus planet (having approximately the same size
as the Earth) is plotted over the Solar disk.
The
radius of all Solar system (from the Sun to the most remote smaller planets and
comets)
exceeds
5 billion kilometers (~ 35 times the distance from the Earth to the Sun). The
message is:
the
Solar system proved to be much bigger, than it was previously (before Newton)
thought to be!
And
the distances beyond the borders of the Solar system are even much-much bigger!
The
distances in far space is not convenient to measure in kilometers or even in
astronomical units, as it is convenient to do within the Solar system (1 a.u. =
1,5•108 km equals the average distance between the Sun and the Earth).
Like moles are more convenient to calculate molecules, the LIGHT YEARs are more convenient to calculate distances in the Universe. 1 LIGHT YEAR is the distance, that the light passes in one year. 1 light year = 9.46•1015 m ( ~103 the diameter of the Solar system).
Like moles are more convenient to calculate molecules, the LIGHT YEARs are more convenient to calculate distances in the Universe. 1 LIGHT YEAR is the distance, that the light passes in one year. 1 light year = 9.46•1015 m ( ~103 the diameter of the Solar system).
Even
the nearest to the Sun stars are located at the distances of many light years!
(The nearest one – the Proxima of Centaurus – 4.2 light years)
And
the most far away known objects in the Universe are divided from us by the
distances of ~ 109 – 1010 light years! The Universe is really big!
The
question is: why it is so big? Or even we may put it in another way: why it HAS
TO BE so big?
Let
us for a while return back to molecular physics and thermodynamics. The systems
of molecules, due to chaotic character of their motion, tend to go into a state
with maximum possible (under this or that conditions) disorder. In physics
there is a special value, that measures the degree of disorder in a system.
This value has a name Entropy.
The higher is disorder – the higher is the entropy of the system. And there is a the 2-nd Great Law of Thermodynamics, which states that any macroscopic system being taken out from the equilibrium state (means the state with maximal entropy and degree of disorder) and then left to itself (means the system is isolated from any external interference) will always change its state towards equilibrium.
It means that the ENTROPY of the isolated system can either grow (towards equilibrium state) or remain constant (in equilibrium state, which has maximal possible value of entropy). ENTROPY is the measure of disorder of matter. The higher is the entropy – the less is the order.
The higher is disorder – the higher is the entropy of the system. And there is a the 2-nd Great Law of Thermodynamics, which states that any macroscopic system being taken out from the equilibrium state (means the state with maximal entropy and degree of disorder) and then left to itself (means the system is isolated from any external interference) will always change its state towards equilibrium.
It means that the ENTROPY of the isolated system can either grow (towards equilibrium state) or remain constant (in equilibrium state, which has maximal possible value of entropy). ENTROPY is the measure of disorder of matter. The higher is the entropy – the less is the order.
If
to apply the Second Great Law to the Universe taken as a whole, we may note,
that
1. The Universe is by definition the isolated
system, as there is nothing beyond it, no external forces or influences are
possible. According to the 2-nd Law the entropy (means
–
disorder) in isolated systems MUST grow or remain constant. .
2. Life (proteins, DNA, biological cells,
living creatures and human beings) are definitely more ordered systems than any
gas or liquid. It has incomparable less entropy, than the same set of atoms
being dispersed (as it happens after it dies)
3. Moreover – the Earth itself, being a
complicated self-developing system, is much more ordered than a gas of atoms,
from which it origins. The same we may say about the Sun and other stars. How
it may happen, if the 2-nd Law of Therm. is true?
4. The only chance: the entropy of a big system
MUST only grow, but it is possible that in some small part of it the entropy
may locally decrease.
5. For existing of ordered self-organized
systems (islands of order) it is necessary that they shall be surrounded by
much bigger volume of disordered matter (ocean of disorder), where the excess
entropy can be spread.
It
means: Universe has to be BIG!
The
old System of Spheres was not big enough and was thought to be very harmonious.
The ORDER and HARMONY were ruling the system. Such a system cannot evolve from
initial chaos by the laws of physics. It can be only created – and created
directly into the final shape.
To
have a chance to evolve from initial chaos and to have enough space to disperse
excess quantity of entropy the Universe MUST be BIG! And MUST be from the very
beginning NON-Equilibrium!
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