The moment of “opposition” is not the moment that a planet is closest or brightest, but is (if I recall) the moment when the elliptical longitude of the planet is 180° — exactly halfway across the sky, which is as far as possible — away from that of the Sun from the point of view of Earth.
If the planets traveled in perfect circles centered on the sun and at a uniform velocity, then the moment of opposition would also be the moment when the planet is closest and brightest. But since the planets are in elliptical orbits and move at a non-uniform rate, they can pass opposition but still be moving toward each other — or already be moving away from each other.
Magnitude is affected by both the phase of the planet and its distance, so we would expect the maximum magnitude to fall between the moment when the phase is greatest (at the moment of opposition) and the moment when the distance is smallest — and that is in fact what your numbers seem to indicate.