How Was the Solar System Formed

A Solar System is a collection of heavenly bodies comprising a star, with planets and other objects orbiting around it. Our Solar System consists of the Sun which is orbited by 8 planets (including our very own Earth), and many other objects like moons (which orbit planets), asteroids and meteors. Several heavenly bodies of the Solar System like the Sun, Moon, Mercury, Venus, Mars, Jupiter and Saturn are visible to the naked eye, while the rest of the planets are visible through telescopes. There are also various bright asteroids, comets and meteors which are visible.

The Sun is the most important member of the Solar System because it provides most of the light, heat and other energy vital for existence of life. The eight known planets orbit around the Sun in slightly oval orbits, of which the first four planets: Mercury, Venus, Earth and Mars are rocky planets, whereas the next four: Jupiter, Saturn, Uranus and Neptune are gaseous planets. Pluto was the ninth planet earlier and as it is very small in size, scientists from around the world collectively demoted it. Hence, now it is no longer considered to be a planet.

How Was the Solar System Formed?

By analyzing the radioactive decay of radioactive elements in the meteorites, astronomers have said that the origin of the Solar System can be traced back to 4.6 billion years ago. This was when a gravitational collapse of a small portion of a giant molecular cloud occurred. This is known as 'Nebular Hypothesis' which was developed for the first time by Emanuel Swedenborg, Immanuel Kant and Pierre-Simon Laplace in the 18th century, and is a theory widely accepted across the globe. However, this theory has been challenged and refined after the dawn of the space age and the discovery of extra solar planets in the 1950s and 1990s respectively.

According to this Nebular theory, the Solar System was formed from a massive, rotating cloud of dust and gas called the Solar Nebula. It so happened that the Solar Nebula began collapsing under its own gravitational force. Several scientists believe that the collapse of this giant gas cloud was triggered by a supernova (exploding star) near it, resulting into the contraction of the Nebula. As the cloud collapsed, heat increased causing the dust particles to vaporize and resulting in the compression of the cloud at the center.

As the Nebula collapsed, a large fragment separated itself from it to form the Solar System. The Sun emerged from the largest collection of mass at the center of the Nebula. The pressure at the center of the Nebula became high enough to trigger nuclear reactions that could power the Sun. As the Nebula shrunk in size, it spun faster and faster and got flattened into a disk. Therefore, the mass around the Sun aggregated and formed a disk around it.

Further, the particles within the flattened disk collided against each other with increased frequency and got fused, so as to form asteroid-shaped objects known as planetesimals. Some of these planetesimals further collided and combined with each other to form the planets that we know today. The rest of the planetesimals combined to form moons, meteors, comets and asteroids.

As solar eruptions took place, solar winds were created. These winds were so powerful in nature that they swept away most of the lighter elements such as Helium and Hydrogen from the Solar System. However, these winds were weaker in the outer regions of the Solar System and thus the outer planets were left with a large amount of Hydrogen and Helium. This explains the gaseous nature of the outer planets and the contrasting rocky nature of the inner four planets.

Scientists believe that stars continue changing and do not remain constant. They believe that in the next 5 billion years, the outer layers of the Sun will expand, making the Sun larger and hotter. The expansion of the Sun will cause it to become a red ball of fire which will consume all the inner planets including the Earth. Scientists also believe that after a period of 100 million years, the Sun will lose its capacity to make energy and will end up as a small planet.

The above mentioned 'Nebular Hypothesis' is the most widely accepted theory of formation of the Solar System. However, it has not been agreed upon as the ultimate theory due to the emergence of various theoretical problems which is causing difficulties to reconcile it with new observations.