The World We Live In…. What is the Universe? How old is it? How big is it? What is it made of? What laws of nature govern it? What was happening to it in the past? What will happen to it in the future?. Assembled by Sergei Zverev. What is the Universe?.
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What is the Universe?
How old is it?
How big is it?
What is it made of?
What laws of nature govern it?
What was happening to it in the past?
What will happen to it in the future?
Assembled by Sergei Zverev
Demonstration which shows that our Universe is not thought to be a set of objects moving in a space away from a certain point at which the explosion occurred
Our Universe is three-dimensional but you can picture a universe that consists onlyof the surface of a balloon (get a balloon, prepare it in advance: inflate it and draw the galaxies on the surface; make sure you have plenty of galaxies; let the air out). You inflate the balloon just a little bit and note the galaxies on the surface of the balloon. Then start inflating the balloon more and more. You will see that, while the balloon is inflating, the galaxies are moving farther away from each other and, if you measure the distance between the galaxies before and after the inflation of the balloon, you will see that more distant galaxies will appear to move apart faster.
In this model it is easy to see that every galaxy will observe the same effect, and no one galaxy is in a special location. Then you can ask yourself if you can find the center of expansion on the surface of the balloon, and you will not find it. This will help you make a conclusion that there is no location on the surface of the balloon that can be identified as the "center" of the universe or a point of the Big Bang “explosion.”
FROM MACRO to MEGA to MICRO COSMOS
We will start with 100 (equivalent to 1 meter), and will increase the size of observable area by a factor of 10, or 101 (10 meters), 102 (10x10 = 100 meters), 103 (10x10x10 = 1,000 meters), 104 (10x10x10x10 = 10,000 meters), so on, until we get close to the limit of our imagination in the direction of the mega cosmos.
Later we will return, a little faster, back to the point where we started and continue our trip in the opposite direction reducing observable distances by factors of 10 into the micro cosmos.
We will see how much the human race still needs to learn...
Distance to a bunch of leaves in the garden
Starting our trip upwards .... We can see the foliage
At this distance we can see the limits of the forest and the edifications
We will pass from meters to kilometers...
Now it is possible to jump with a parachute
The city could be observed but we really can’t see the houses
At this height, the state of Florida is just coming into view...
Typical sight from a satellite
The northern hemisphere of Earth, and part of South America
The Earth starts looking small...
1 million km
The Earth and the Moon’s orbit in white...
10 million km
Part of the Earth’s Orbit in blue
100 million km
Venus and Earth...
1 billion km
Orbits of Mercury, Venus, Earth, Mars and Jupiter
10 billion km
At this height of our trip, we could observe the Solar System and the orbits of the planets
100 billion km
The Solar System starts looking small...
1 trillion km
The Sun now is a small star in the middle of thousands of stars...
At one light-year the little Sun star is very small
Here we will see just stars in the infinity...
a light-year is the distance that light travels in a vacuum
in one year at a speed of 3.0 x 108 m/s or 190,000 mi/s
A lot of stars and Nebulae...
At this distance we are travelling in the Milky Way, our galaxy
We continue our travel inside the Milky Way
We begin reaching the periphery of the Milky Way
At this tremendous distance we can see the entire Milky Way and other galaxies as well
From this distance, all the galaxies look small with immense empty spaces in betweenThe same laws are ruling all bodies of the UniverseWe could continue traveling upwards (up to 100 billion light years) with our imagination, but now let’s return home
In this trip “upwards” we went to the power of 23 of 10
Now we are going to dig inside of matter in a reverse trip...
10 centimeters or 4 inches
We arrive at our starting point. We could touch it with our hands...
Getting closer at 10 cm ... We can delineate the leaves
At this distance it is possible to observe the structure of the leaf
The cellular structures begin to show...
The cells can be delineatedYou can see the union between them
Starting our trip inside the cell...
The nucleus of the cell is visible.
Again we changed the measuring unit to adapt to the miniscule sizeYou can see the chromosomes
In this micro universe the DNA chain is visible
...the chromosome blocks can be observed.
It appears like clouds of electrons... These are carbon atoms, one of the organic componentsIs there some resemblance of the micro cosmos with the mega cosmos? cosmos ...
In this miniature world we can observe the electron cloud
You can see a small nucleus in the middle of the atom and an empty space between the nucleus and the electron orbits
At this incredible and minuscule size we could observe the nucleus of the atom
Now we can observe the nucleus of the carbon atom: 6 protons and 6 neutrons
Here we are in the field of the scientific imagination, face to face with a proton
Examine the proton in the nucleus
There is nowhere further to go...We are at the limits of current scientific knowledge
A period of "inflation" produced a burst of exponential growth in the universe. For the next several billion years, the expansion of the universe gradually slowed down as the matter in the universe pulled on itself via gravity. More recently, the expansion has begun to speed up again as the repulsive effects of dark energy have come to dominate the expansion of the universe.
A representation of the evolution of the Universe over 13.7 billion years.
Observations suggest that the universe as we know it began around 13.7 billion years ago. Since then, the evolution of the universe has passed through three phases:
1. The very early universe was the split second in which the universe was so hot that particles had energies higher than those currently accessible in particle accelerators on Earth (particles had no mass, only one force existed).
2. Following this period, in the early universe, the evolution of the universe proceeded according to known high energy physics. This is when the particle acquired mass, one force split in four, first protons, electrons and neutrons formed, then nuclei and finally atoms.
3. With the formation of neutral hydrogen, the cosmic microwave background was emitted. Then matter started to aggregate into the first stars and ultimately galaxies, quasars, and clusters of galaxies formed.
after the Big Bang?
The Planck epoch - up to 10–43 seconds after the Big Bang: only one fundamental force exists.
The grand unification epoch - 10–43 - 10–36 seconds, gravity separates from the fundamental force.
The electroweak epoch - between 10–36 seconds and 10–12 seconds: strong force separates from the electroweak force.
The inflationary epoch - between 10–36 seconds and 10–32 seconds: inflation (rapid exponential expansion) occurs. In the end the universe is filled with a quark-gluon plasma.
The quark epoch - between 10–12 seconds and 10–6 seconds: particles acquire a mass, fundamental interactions of gravitation, electromagnetism, the strong interaction and the weak interaction have taken their present forms.
The hadron epoch - between 10–6 seconds and 1 second: The quark-gluon plasma cools, protons and neutrons and other hadrons form, neutrinos decouple and begin traveling freely through space.
The lepton epoch - between 1 second and 3 minutes: The majority of hadrons and anti-hadrons annihilate each other, leptons and anti-leptons dominating the mass of the universe, then most leptons and anti-leptons
annihilate leaving a small residue of leptons.
The photon epoch - between 3 minutes and 380,000 years: universe is dominated by photons. These photons are still interacting frequently with charged protons, electrons and later with the nuclei, and continue to do so for the next 300,000 years. After 17 minutes the nuclear fusion stops. In the end of the epoch most of the atoms in the universe become neutral, and the photons can now travel freely: the universe has become transparent for radiation.
Dark ages -380,000 – 500 million years: the universe is filled with neutral hydrogen and helium and is relatively opaque at certain wavelengths, and does not emit radiation.
Structure formation: after 150 million years: first stars and quasars formed, large volumes of matter form galaxies.
Reionization- 150 million to 1 billion years: intense quasar radiation re-ionizes the surrounding universe. From this point on, most of the universe is composed of plasma and is transparent.
5.4 billion years after the Big Bang – the Milky Way formed.
8.5 billion years after the Big Bang – the Solar System formed.
13.7 billion years after the Big Bang - you were born. Expansion of the Universe is accelerating.
Big freeze: 1014 years (100,000,000,000,000 = 100,000 billion = 100 trillion) and beyond.This scenario is generally considered to be the most likely, as it occurs if the universe continues expanding as it has been.
1. Over a time scale on the order of 100 trillion years or less, existing stars burn out, new stars cease to be created, and the universe goes dark;
2. Over a much longer time scale in the eras following this, the galaxy evaporates as the stellar remnants comprising it escape into space, and black holes evaporate via Hawking radiation;
3. In some grand unified theories, proton decay will convert the remaining interstellar gas and stellar remnants into leptons (such as positrons and electrons) and photons. Some positrons and electrons will then recombine into photons. In this case, the universe has reached a maximum-entropy state consisting of a bath of particles and low-energy radiation at thermodynamic equilibrium.
4. No changes after that.
Big rip: 200+ billion years
This scenario is possible only if the energy density of dark energy actually increases without limit over time. Such dark energy is called phantom energy and is unlike any known kind of energy. In this case, the expansion rate of the universe will increase without limit. Gravitationally bound systems, such as clusters of galaxies, galaxies, and ultimately the solar system will be torn apart. Eventually the expansion will be so rapid as to overcome the electromagnetic forces holding molecules and atoms together. Finally even atomic nuclei will be torn apart and the universe as we know it will end in an unusual kind of gravitational singularity. In other words, the universe will expand so much that the electromagnetic force holding things together will fall to this expansion, making things fall apart.
1. What is the Universe?
Space, time, matter, energy and laws of nature
13.7 billion (13,700,000,000) years old
3. How big is our Universe?
96 billion light years wide
Atoms and radiation, dark matter and dark energy
4. What is it made of?
2. How old is our Universe?
5. What is the largest
object in our Universe?
Super clusters of galaxies up to 500 million light years (or 5x1024 meters) in size and containing up to 10,000 galaxies
6. What is the smallest object
in our Universe?
A quark and an electron – both are less than 10-18 meters in size
5. What was happening to
the Universe after the Big
It was expanding from a tiny dot,
it is expanding now,
and will keep expanding in the future
And now ... Note that going downwards we could only go to the power of minus 16 of 10 to reach the known limits of matter... and upwards we went to the power of 23 of 10 but we could have continued our trip up to the size of our universe – 1027 meters (power of 27 of 10)then ...What is behind those limits? Are there any limits?What initiated the Big Bang? What are the dark matter and dark energy? Why zillions of elementary particles of the same kind (for example electrons) in the universe are absolutely identical? Are we alone in the universe or there is life in other solar systems and galaxies? How long can the mankind survive on Earth? – etc., etc., etc.Do you want to find answers to these questions?