Regiomontanus
Ματαιοδοξία ματαιοδοξιών! Όλα είναι ματαιοδοξία.
The Sun puts out a solar wind of particles, and you can come up with an average rate per thousand years. That rate might relate to its surface temperature, surface activity, surface area. Over time this will slightly decrease the mass of the Sun and therefore its gravitational force, but by how much?
Is the Sun Losing Mass? | by Brian Koberlein
The above article says its losing 174 trillion tons per year. You just multiply that by 5 billion years (or however many years) and then recalculate the strength of the Sun's gravitational pull. Then you can recalculate the shape and size of the planetary circuits.
Over the lifetime of a star like ours (spectral type G2), that mass loss is about 0.06% of what it started with. So planetary orbits will not change a huge amount.