The formula relating the synodic period of Venus to its sidereal period is
$$\frac1P = \frac1E + \frac1S$$
Where $P$ is the sidereal period, $S$ is the synodic period, and $E$ is the orbital period of Earth (1 year).
Now both E and P can be calculated from Kepler's law, explicitly
$$P = 2\pi\sqrt{\frac{r_P^3}{\mu}}$$
Where $r_P$ is the semi-major-axis of Venus (distance to sun), and $\mu$ is the sun's gravitational parameter $\mu=1.33\times 10^{20}$ in SI units (m,kg,s). The same formula works for $E$
So now you can use this law to work out $P$ and $E$ for Venus and Earth in their new positions, and with that find $S$. Take care with units you can't use metres and seconds in one part of the formula and km - years in another.