  The Vera C. Rubin Observatory is expected to start the Legacy Survey of Space
and Time (LSST) in early to mid-2025. This multi-band wide-field synoptic
survey will transform our view of the solar system, with the discovery and
monitoring of over 5 million small bodies.The final survey strategy chosen for
LSST has direct implications on the discoverability and characterization of
solar system minor planets and passing interstellar objects. Creating an
inventory of the solar system is one of the four main LSST science drivers. The
LSST observing cadence is a complex optimization problem that must balance the
priorities and needs of all the key LSST science areas. To design the best LSST
survey strategy, a series of operation simulations using the Rubin Observatory
scheduler have been generated to explore the various options for tuning
observing parameters and prioritizations. We explore the impact of the various
simulated LSST observing strategies on studying the solar system's small body
reservoirs. We examine what are the best observing scenarios and review what
are the important considerations for maximizing LSST solar system science. In
general, most of the LSST cadence simulations produce +/-5% or less variations
in our chosen key metrics, but a subset of the simulations significantly hinder
science returns with much larger losses in the discovery and light curve
metrics.
