The steps of the solar system formation according to the nebula hypothesis will be 1,2,3,4,5,6,7.
What is solar system formation?
The solar system consists of the planet's satellites, as well as numerous comets, asteroids, and meteoroids, as well as the interplanetary medium.
The following are the steps to the nebular hypothesis. A nebula becomes a solar nebula when a patch of gas and dust within the cloud condenses into a core and becomes a protostar.
A nearby supernova blast might have created the condensing material. An accretion disc forms as the material surrounding the protostar falls.
The steps in the development of the solar system are as follows:
1. A giant nebula exists in space.
2. As the contraction continues a proto-star will form at the center which eventually becomes the star in the solar system
3. The contraction creates kinetic energy within the cloud
4. It begins to contract under its own gravity.
5. The entire nebula will flatten into a disk as a result and small back currents or eddies will form in the disk.
6. The cloud begins to heat up, flatten and spin or rotate.
7. Material builds up or accretes in eddies to form planets.
Hence, the steps of the solar system formation according to the nebula hypothesis will be 1,2,3,4,5,6,7.
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