Water: One of the most significant oxides of hydrogen is water. The speciality of water is that most life forms on Earth cannot survive without...
Water Structure and Properties: Hydrogen Bonding, Dipole Moment
December 11, 2024Universe and Origin of Solar System: How and when did the universe begin? Even after centuries of research, this fundamental question remains as intriguing as other scientific theories. The term universe makes us think about unimaginable things that we haven’t seen with naked eyes or space and time. It is curious to think and understand the theories of the origin of the universe and, by extension, our solar system, the earth and life as we know it. Read further to learn much more about the enigma of the Universe and the Origin of the Solar System.
The universe is a composition of matter, energy and gasses in all of space and time. Space is completely silent, as there is no medium for sound to travel in space. There are various cosmological theories about the origin of the universe, but The Big bang Theory proposed by Georges Lemaître is the most accepted one. Discussion of the universe starts with the big bang hypothesis, which is another controversial topic among astrologers. It all began as a red hot, dense, revolving gaseous cloud of cosmic dust called Ylem or primaeval matter about 10 to 13 billion years ago. The Ylem was made up of matter particles (such as neutrons, protons, and electrons) and antimatter antiparticles.
Fig: The Bigbang Theory
The chronological order of the evolution of the universe can be categorised in the following stages:
Earth formed around 4.5 billion years ago, as gravity drew spinning gas and dust into the third planet after stabilising the solar system into its current shape. The formation of the earth occurred in three stages.
The primitive earth existed only as an enormous cloud of dust and gas. The earth began to cool over a few hundred million years, and oceans of liquid water emerged. Heavier elements like iron started plunging through the seas and magma to the planet’s core. Earth became divided into layers as a result of this, with the topmost layer consisting of a solid crust coating of a comparatively lighter material and the denser, molten stuff sinking to the centre. Water molecules on earth were broken into hydrogen and oxygen, oxygen combined with other compounds. The ozone layer was created naturally by the sun’s interaction of ultraviolet (UV) light with molecular oxygen.
Earth has a central core, a rocky mantle, and a solid crust, just like its other terrestrial planets. The incredible gaseous atmosphere composition of 21% oxygen (which we need to breathe), 78% nitrogen, and.9% argon. Water vapour exists in our atmosphere and serves to keep our daily temperatures temperate.
Fig: Evolution of Present Day Earth
According to scientists, bacteria may have been the first life on land 3.22 billion years ago. Evidence of microbial life on land was discovered in 3.48-billion-year-old geyserite in Western Australia’s Pilbara Craton in May 2017.
The emergence of the simplest primordial life from non-living elements is referred to as the origin of life. The gradual creation of sophisticated species from simpler organisms is referred to as the evolution of life. These early species have to be simpler than those that exist now. On Earth, all living things were single-celled organisms.
The earliest living forms were prokaryotes, which were primitive animals that ate carbon compounds that accumulated in Earth’s early oceans. Other species gradually emerged that used the Sun’s light, as well as chemicals like sulfides, to make their own energy. The first multicellular species appeared much later, and Earth’s biodiversity increased dramatically as a result leading to the evolution of man and earth of the present.
The universe is a composition of matter, energy and gasses in all of space and time. Space is completely silent, as there is no medium for sound to travel in space. According to the most accepted big bang theory, it all began as a red hot, dense, revolving gaseous cloud of cosmic dust called Ylem or primaeval matter about 10 to 13 billion years ago. The chronological order of evolution of the universe can be categorised into four: (i) Early Universe, which constituted fundamental particles like quarks, electrons, photons, and neutrinos. (ii) The Dark Ages, during which the cosmos was devoid of light. (iii) Appearance of the first star and galaxies and (iv) Formation of the solar system. The Sun and the planets were born from a cloud of gas and dust called the solar nebula 4.6 billion years ago. A powerful solar wind cleansed the system of gas and dust after the Sun began. The asteroids represent the remaining stony debris. Earth formed around 4.5 billion years ago, as gravity drew spinning gas and dust into becoming the third planet after the solar system stabilized into its current shape. According to scientists, the first life on earth appeared around 3.22 billion years ago which finally led to present-day earth.
Q.1. What is the most accepted theory of the origin of the Earth?
Ans: The nebular hypothesis is the most commonly accepted theory of planetary creation.
Q.2. How old is our universe?
Ans: About 13.8 billion years old.
Q.3. How long will our universe last?
Ans: The earliest conceivable end of the Universe is 22 billion years in the future.
Q.4. What does the Solar System Comprise?
Ans: Our solar system is composed of the planets Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune, as well as dozens of moons and millions of asteroids, comets, and meteoroids that are all gravitationally linked to the Sun.
Q.5. What is another theory for the origin of the universe?
Ans: Although the most accepted theory is the big bang, alternate theories like the Steady State universe also exist.
Hope this detailed article on the Universe and the Origin of the Solar System helps you in your exam preparation. If you have any queries or doubts, drop them in the comments section and we will get back to you at the earliest.