This thread is really messy. If one is talking about Newtonian gravity - or for that matter, SR - one should not muddy the waters discussing spacetime curvature. The nit that the sun's mass is not exactly constant is singularly unhelpful. It's also negligible, as it is less than a part per trillion per decade.
Ibix answer is right - you cannot take Newtonian gravity, make it travel at c rather than instantaneously, and match observations. However, this is not (directly) due to "the position of the sun in the sky 8 minutes ago". First, that's dominated by the Earth's rotation. Second, as pointed out, insofar as the sun is stationary, the gravitational field at point X is the same as it was 8 minutes ago, so the field the Earth traverses is the same as it was 8 minutes ago, so how can the orbit be different?
The answer to this apparent paradox is that the sun is not exactly stationary. Even in a one-planet solar system, the Earth and Sun revolve around their common center of mass. If you put in a propagation delay, the Earth sees its own gravity through the Sun's (small) motion with a 16 minute delay. This tends to perturb the orbit, and as described earlier, results in an instability over many millions of years. When you add the other 8 - sorry, 7 - planets, this instability just gets worse.
GR doesn't actually have to fix this up. There's no reason to demand that it give you stable orbits (although if you want to consider it as a viable description of nature you do, but the theory itself doesn't have to). It does and it doesn't - orbits in GR are not ellipses but rosettes, but these rosettes are stable over long time scales. It is a success of GR that it matches the data, both the long-term stability and the rosette nature of the orbits.