The stability of an idealized climate system is investigated using a s
imple coupled atmosphere-ocean box model. Motivated by the results fro
m general circulation models, the main physical constraint imposed on
the system is that the net radiation at the top of the atmosphere is f
ixed. The specification of an invariant equatorial atmospheric tempera
ture, consistent with paleoclimatic data, allows the hydrological cycl
e to be internally determined from the poleward heat transport budget,
resulting in a model that has a plausible representation of the hydro
logical cycle-thermohaline circulation interaction. The model suggests
that the stability and variability of the climate system depends fund
amentally on the mean climatic state (total heat content of the system
). When the total heat content of the climate system is low, a stable
present-day equilibrum exists with high-latitude sinking. Conversely,
when the total heat content is high, a stable equatorial sinking equil
ibrium exists. For a range of intermediate values of the total heat co
ntent, internal climatic oscillations can occur through a hydrological
cycle-thermohaline circulation feedback process. Experiments conducte
d with the model reveal that under a 100-year 2xCO(2) warming, the the
rmohaline circulation first collapses but then recovers. Under a 100-y
ear 4xCO(2) warming, the thermohaline circulation collapses and remain
s collapsed. Recent paleoclimatic data suggest that the climate system
may behave very differently for a warmer climate. Our results suggest
that this may be attributed to the enhanced poleward freshwater trans
port, which causes increased instability of the present-day thermohal
ine circulation.