Formation of Solar System (original) (raw)

Last Updated : 23 Jul, 2025

The formation of solar system was very energetic and unique. The Sun and the planets produced the solar nebula, made of cloud of gas and dust, some 4.6 billion years ago. The collapse of the solar nebula was mostly due to a supernova explosion. The planets formed in a thin disk circling the Sun, which formed at its center. Moons evolved around the gas giant planets in a similar way. In the outer regions of the solar system, comets consolidated and were propelled to considerable distances by near gravitational collisions with the massive planets. A powerful solar wind removed gas and dust from the system after the Sun began. The stony remains are represented by the asteroids.

We will answer a few of the questions in this article, such as what are planets? from where did they originate? why are some things gaseous and some stony? How does our planet look like?

Table of Content

History:

Formation:

Presolar nebula

Solar system birth environment:

Formation of the planets:

The different planets are remembered to have framed from the sun oriented cloud, the circle molded haze of gas and residue left over from the Sun's formation.The right now acknowledged strategy by which the planets shaped is gradual addition, in which the planets started as residue grains in circle around the focal protostar. Through direct contact and self-association, these grains shaped into bunches up to 200 m (660 ft) in distance across, which thus crashed to frame bigger bodies (planetesimals) of ~10 km (6.2 mi) in size. These step by step expanded through additional impacts, developing at the pace of centimeters each year throughout the following couple of million years.

Subsequent evolution:

The planets were initially remembered to have framed in or close to their ongoing circles. This has been addressed during the most recent 20 years. Right now, numerous planetary researchers believe that the Planetary group could have looked altogether different after its underlying development: a few articles as gigantic as Mercury might have been available in the inward Nearby planet group, the external Planetary group might have been substantially more minimized than it is currently, and the Kuiper belt might have been a lot nearer to the Sun.

Terrestrial planets:

Asteroid belt:

Planetary migration:

Late Heavy Bombardment and after:

The Birth of the Sun:

The Birth of the Planets:

Earth’s Moon:

Pluto and Beyond:

  1. Before 2006, students discovered that our planetary group had nine planets, not eight. The one considered the 10th, Pluto, circles uttermost from our Sun.
  2. In any case, in 2006, the International Astronomical Union proclaimed that Pluto doesn't consider a planet. It is more smaller than Earth's Moon.
  3. It circles far out in a belt of space rocks past Neptune (however Pluto occasionally draws nearer to the Sun than Neptune), and needs more gravity to clear the area around its way.
  4. In this way, it was downsized to a "dwarf planet," or a planetesimal.
  1. Solar System Planets, Orders and Formation
  2. Solar System – Introduction, Planets, Earth, FAQs
  3. Solar Energy

Conclusion:

In summary, planets are bodies circling a star. Planets sform from particles in a plate of gas and residue, impacting and staying together as they circle the star. The planets closest to the star will generally be rockier in light of the fact that the star's breeze blows away their gases and on the grounds that they are made of heavier materials pulled in by the star's gravity. In the Sun's framework, Earth is one of four rough planets, however an extraordinary one, with unbending and liquid layers.