No, the relationship that Kepler discovered was between the length of the long axis of the ellipse, and the period of the planet.
It is possible for a comet with a very long skinny orbit, and an asteroid with a nearly circular orbit to have the same minor axis length, but obviously, the comet will have a much longer orbital period. For example, Halley's comet has a semiminor axis of about 3.5AU. An asteroid in a circular orbit with the same semi-minor axis would have a period of about 6 years, compared to Halley's period of 76 years.
I don't fully understand whyIf you ask about various types of meanknow the semi-minor axis, and the perihelion distance (for example), then it would be possible to work out the semi-major axis, and the relative orbital period, but I can't think of anything relatedyou would need more information than just the semi-minor axis.