According to the nebular theory, did the planets start forming before or after the Sun ignited

According to the nebular theory, did the planets start forming before or after the Sun ignited?

The Correct Answer and Explanation is :

According to the nebular theory, the planets started forming after the Sun began to ignite.

The nebular theory suggests that the solar system formed from a giant cloud of gas and dust, known as a solar nebula, about 4.6 billion years ago. Initially, this cloud was mostly hydrogen and helium, with traces of heavier elements. The process began with the gravitational collapse of a part of this nebula under its own weight, leading to the formation of the Sun at the core of the collapsing material.

As the nebula collapsed, it began to spin faster and flatten into a disk, known as the protoplanetary disk, with the Sun forming at its center. The Sun’s formation process involved the contraction of material under gravity, which increased the temperature and pressure in the core of the Sun until nuclear fusion ignited. This ignition marks the point at which the Sun became a full-fledged star, emitting light and heat.

After the Sun ignited, the leftover material in the surrounding disk started to cool and condense into solid particles. These particles coalesced through a process called accretion, gradually forming larger bodies. Over time, these bodies grew into the planets, moons, asteroids, and other components of the solar system.

This sequence of events highlights that the initial stages of the Sun’s formation and its subsequent ignition preceded the formation of the planets. The energy and solar wind from the newly formed Sun influenced the material in the protoplanetary disk, helping to shape the environment in which the planets formed. This process ensured that the planets formed in a stable orbit around the Sun, creating the organized system we observe today.

Now, let’s generate an image that illustrates this process of the nebular theory:

  • Image Description: A vibrant representation of the early solar system according to the nebular theory. The image shows a central bright young Sun emitting light and solar winds, surrounded by a swirling protoplanetary disk filled with gas, dust, and forming planetesimals. The background is a starry space, enhancing the cosmic setting. The colors should be vivid, with oranges and yellows for the Sun, and various shades of blues and grays for the disk and forming materials.
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