Did the sun evolve from the moon?

Answer 1

No.
there are many theories that how did the sun and moon evolved i think its the theories that i read

1. long time ago there are no stars nor anything in the outer space but there is a meteor so big it crash in the solar system and because its burning the eye or the center of the meteor is become the sun and other planets and because of the gravitational pull of the sun there is gravity and there is the the order of how for example the venus pass in the earth its the order it only happens twice in your lifetime

Answer 2

Protostar, main-sequence, red giant, white dwarf

• A cloud of gas and dust begins to contract under the force of gravity. In regions of star birth, we find gaseous nebulae and molecular clouds. These sites of pre-birth are dark patches called globules.

• The protosun collapsed. As it did, its temperature rose to about 150,000 degrees and the sun appeared very red. Its radius was about 50 present solar radii.

When the central temperature reaches 10 million degrees, nuclear burning of hydrogen into helium commences

• The star settles into a stable existence on the Main Sequence, generating energy via hydrogen burning. This is the longest single stage in the evolutionary history of a star, typically lasting 90% of its lifetime.Thermonuclear fusion within the Sun is a stable process, controlled by its internal structure.

Answer 3

There are several theories. The most widely accepted is that our solar system existed as a huge cloud of gas and dust, and a supernova shock-wave struck this cloud, causing it to condense. As the cloud condensed, a large portion of the gas and dust gathered in the center. This caused it to start spinning. As it spun, it continued to gather mass in the center. Eventually the gravity within this mass would cause the conditions needed (extreme heat and pressure) for fusion to occur, and our sun was born. Once the sun began producing energy from this process, the outward pressure of its radiation cleared out much of the smaller debris. The rest of the materials continued to spiral around the star and began forming bigger and bigger masses that would eventually, through a very violent process, form the planets. A large portion of this material that did not form the sun or the planets would remain in a distant orbit around the sun, and form what is called the Kuiper belt (Pluto is a Kuiper belt object), and the even more distant Oort cloud (believed to be a source of comets).