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It's consensus that the very similar apparent sizes of the moon and the sun as seen from earth is a coincidence (as already answered in this site) The revolution affects the difference between sidereal time and solar time, and makes the solar day $\approx 4$ minutes longer if the earth spinned in the opposite direction the sun would. This provides us with almost exact total solar

1) the sun seems brighter (more dazzling) if there is more scattering in the atmosphere You say that sun rises in the east (with a certain degree of oscillations due to the tilt of the axis) just because the earth spins from west to east The sun would actually look very small to us in the sky if there were no atmosphere (it's the same angular size as the moon) and most of the brightness seen in the direction of the sun is from small deflection rayleigh scattering.

The sun's energy comes primarily from fusion of light elements in its core

The sun will last, at its current brightness for 9 billion more years How long until the sun gets burned down to the point where it cannot sustain life on earth anymore Those are completely different things As i asked before, separate threads, please.

First, we should speak of acceleration rather than force, because like i said earlier all objects at a given distance from the sun experience different forces but the same acceleration You ask how come the sun is strong enough to keep the distant planets in orbit but i don't fall into it?. I know that nucelar fusion in the sun requires quantum tunneling to occur, as otherwise the sun's core wouldn't be hot enough to overcome the fusion barrier However while the 2nd and further stage.

Here are some things i'm assuming when trying to tackle this question

The moon's orbit must be concave toward the sun The moon speeds up as it goes toward the sun, and it slows down as it moves away For an observer on the earth, the moon appears to orbit the earth roughly $13$ times a year The earth, the moon, and the sun remain in the same.

The sun does not rise, it is the horizon that goes down

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