Origin Of The Universe

Big Bang Theory

• Also called the expanding universe hypothesis.
• In the beginning, all matter forming the universe existed in one place in the form of a “tiny ball” (singular atom) with an unimaginably small volume, infinite temperature and infinite density.
• At the Big Bang the “tiny ball” exploded violently. This led to a huge expansion.
• took place 13.7 billion years before
• The expansion continues even to the present day.
• There was particularly rapid expansion within fractions of a second after the bang.
• Thereafter, the expansion has slowed down. Within first 3 minutes from the Big Bang event, the first atom began to form.
• Within 300,000 years from the Big Bang, temperature dropped to 4,500 K (Kelvin) and gave rise to atomic matter.
• The expansion of universe means increase in space between the galaxies.
• An alternative to this was Hoyle’s concept of steady state.
• It considered the universe to be roughly the same at any point of time.
• However, with greater evidence becoming available about the expanding universe, scientific community at present favours argument of expanding universe.

The Star Formation

• • The distribution of matter and energy was not even in the early universe.
  • These initial density differences gave rise to differences in gravitational forces and it caused the matter to get drawn together. These formed the bases for development of galaxies.
  • A galaxy contains a large number of stars. Galaxies spread over vast distances that are measured in thousands of light-years.
  • A galaxy starts to form by accumulation of hydrogen gas in the form of a very large cloud called nebula.
  • Eventually, growing nebula develops localized clumps of gas.
  • These clumps continue to grow into even denser gaseous bodies, giving rise to formation of stars.
• A light year is a measure of distance and not of time.

• Light travels at a speed of 300,000 km/second.
• One light year- 9.461 1012 km.
• The mean distance between the sun and the earth is 149,598,000 km. In terms of light years, it is 8.311minutes.

Formation Of Planets

• The stars are localised lumps of gas within a nebula.
• The gravitational force within the lumps leads to the formation of a core to the gas cloud and a huge rotating disc of gas and dust develops around the gas core.
• The gas cloud starts getting condensed and the matter around the core develops into small- rounded objects.
• These small-rounded objects by the process of cohesion develop in the same period sometime about 4.6 billion years ago.
• Planetesimals are a large number of smaller bodies.
• Till recently (August 2006), Pluto was also considered a planet.
• However, in a meeting of the International Astronomical Union, a decision was taken that Pluto like other celestial into what is called planetesimals objects
• These large number of small planetesimals accrete to form a fewer large bodies in the form of planets

Our Solar System

Details

• 8 planets
• The nebula, from which our Solar system is supposed to have been formed, started its collapse and core formation some time 5-5.6 billion years ago and the planets were formed about 4.6 billion years ago.
• Sun (the star), 8 planets, 63 moons, millions of smaller bodies like asteroids and comets and huge quantity of dust-grains and gases.
• Out of the eight planets, mercury, Venus, earth and mars are called as the inner planets as they lie between the sun and the belt of asteroids the other four planets are called the outer planets.
• Alternatively, the first four are called Terrestrial, meaning earth-like as they are made up of rock and metals, and have relatively high densities.
• The rest four are called Jovian or Gas Giant planets. Jovian means Jupiter-like. Most of them are much larger than the terrestrial planets and have thick atmosphere, mostly of helium and hydrogen.
• All the planets were formed may be called ‘dwarf planet’

Evolution Of The Earth-

Details

• The planet earth initially was a barren, rocky and hot object with a thin atmosphere of hydrogen and helium.
• The earth has a layered structure.
• From the outermost end of the atmosphere to the centre of the earth, the material that exists is not uniform.
• The atmospheric matter has the least density.
• From the surface to deeper depths, the earth’s interior has different zones and each of these contains materials with different characteristics.

Evolution Of Lithosphere

• The earth was mostly in a volatile state during its primordial stage.
• Due to gradual increase in density the temperature inside has increased.
• As a result the material inside started getting separated depending on their densities.
• This allowed heavier materials (like iron) to sink towards the centre of the earth and the lighter ones to move towards the surface.
• With passage of time it cooled further and solidified and condensed into a smaller size.
• This later led to the development of the outer surface in the form of a crust.
• During the formation of the moon, due to the giant impact, the earth was further heated up.
• It is through the process of differentiation that the earth forming material got separated into different layers.
• Starting from the surface to the central parts, we have layers like the crust, mantle, outer core and inner core.
• From the crust to the core, the density of the material increases

Evolution Of Atmosphere And Hydrosphere

• • The present composition of earth’s atmosphere is chiefly contributed by nitrogen and oxygen.
  • There are three stages in the evolution of the present atmosphere.
  • The first stage is marked by the loss of primordial atmosphere.
  • In the second stage, the hot interior of the earth contributed to the evolution of the atmosphere.
  • Finally, the composition of the atmosphere was modified by the living world through the process of photosynthesis.
  • The early atmosphere, with hydrogen and helium, is supposed to have been stripped off as a result of the solar winds.
  • This happened not only in case of the earth, but also in all the terrestrial planets, which were supposed to have lost their primordial atmosphere through the impact of solar winds.
• During the cooling of the earth, gases and water vapour were released from the interior solid earth.

• This started the evolution of the present atmosphere.
• The early atmosphere largely contained water vapour, nitrogen, carbon dioxide, methane, ammonia and very little of free oxygen.
• The process through which the gases were outpoured from the interior is called degassing.
• Continuous volcanic eruptions contributed water vapour and gases to the atmosphere.
• As the earth cooled, the water vapour released started getting condensed.
• The carbon dioxide in the atmosphere got dissolved in rainwater and the temperature further decreased causing more condensation and more rains.
• The rainwater falling onto the surface got collected in the depressions to give rise to oceans.
• The earth’s oceans were formed within 500 million years from the formation of the earth.
• This tells us that the oceans are as old as 4,000 million years.
• Sometime around 3,800 million years ago, life began to evolve.
• However, around 2,500-3,000 million years before the present, the process of photosynthesis got evolved.
• Life was confined to the oceans for a long time.
• Oceans began to have the contribution of oxygen through the process of photosynthesis.
• Eventually, oceans were saturated with oxygen, and 2,000 million years ago, oxygen began to flood the atmosphere.