M = mass of the Sun
m = mass of the Earth
r = distance between the Earth and the Sun
The sun is converting mass into energy by nuclear fusion.
F=GMmr2=mv2r→r=GMv2
ΔE=ΔMc2=(Mt−Mt+Δt)c2→ΔM=ΔE/c2
→ΔrΔt=Gv2c2.ΔEΔt
Sun radiates 3.9×1026 W=ΔE/Δt
Velocity of the earth v=29.8km/s
There is nothing that is stopping the earth from moving with the same velocity so for centripetal force to balance gravitational force r must change.
Is r increasing? (Δr/Δt=3.26070717×10−10m/s)
Answer
I think the reasoning has an error. It assumes v is constant, but instead we ought to assume the angular momentum is constant.
By dimensional analysis that leads to
r∝L2GM
so as M decreases, r increases (the original post had r∝M, not r∝1/M.
On the other hand, assuming a circular orbit seems dubious.
As the other commenters said, this effect is minute. A significant effect on the orbit of the moon around the earth is tidal evolution, which does actually push the moon further away.
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