  We show that it is possible to embed the 1+1 dimensional reduction of certain
spherically symmetric black hole spacetimes into 2+1 Minkowski space. The
spacetimes of interest (Schwarzschild de-Sitter, Schwarzschild anti de-Sitter,
and Reissner-Nordstrom near the outer horizon) represent a class of metrics
whose geometries allow for such embeddings. The embedding diagrams have a
dynamic character which allows one to represent the motion of test particles.
We also analyze various features of the embedding construction, deriving the
general conditions under which our procedure provides a smooth embedding. These
conditions also yeild an embedding constant related to the surface gravity of
the relevant horizon.
