  The compositional and morphological evolution of minor bodies in the Solar
System is primarily driven by the evolution of their heliocentric distances, as
the level of incident solar radiation regulates cometary activity. We
investigate the dynamical transfer of Centaurs into the inner Solar System,
facilitated by mean motion resonances with Jupiter and Saturn. The recently
discovered object, P/2019 LD2, will transition from the Centaur region to the
inner Solar System in 2063. In order to contextualize LD2, we perform N-body
simulations of a population of Centaurs and JFCs. Objects between Jupiter and
Saturn with Tisserand parameter $T_J\sim$3 are transferred onto orbits with
perihelia $q<4$au within the next 1000 years with notably high efficiency. Our
simulations show that there may be additional LD2-like objects transitioning
into the inner Solar System in the near-term future, all of which have low
$\Delta$V with respect to Jupiter. We calculate the distribution of orbital
elements resulting from a single Jovian encounter and show that objects with
initial perihelia close to Jupiter are efficiently scattered to $q<4$au.
Moreover, approximately $55\%$ of the transitioning objects in our simulated
population experience at least 1 Jovian encounter prior to reaching $q<4$au. We
demonstrate that a spacecraft stationed near Jupiter would be well-positioned
to rendezvous, orbit match, and accompany LD2 into the inner Solar System,
providing an opportunity to observe the onset of intense activity in a pristine
comet $\textit{in situ}$. Finally, we discuss the prospect of identifying
additional targets for similar measurements with forthcoming observational
facilities.
