  We introduce two new diagnostics of dark energy (DE). The first, Om, is a
combination of the Hubble parameter and the cosmological redshift and provides
a "null test" of dark energy being a cosmological constant. Namely, if the
value of Om(z) is the same at different redshifts, then DE is exactly
cosmological constant. The slope of Om(z) can differentiate between different
models of dark energy even if the value of the matter density is not accurately
known. For DE with an unevolving equation of state, a positive slope of Om(z)
is suggestive of Phantom (w < -1) while a negative slope indicates Quintessence
(w > -1). The second diagnostic, "acceleration probe"(q-probe), is the mean
value of the deceleration parameter over a small redshift range. It can be used
to determine the cosmological redshift at which the universe began to
accelerate, again without reference to the current value of the matter density.
We apply the "Om" and "q-probe" diagnostics to the Union data set of type Ia
supernovae combined with recent data from the cosmic microwave background
(WMAP5) and baryon acoustic oscillations.
