We consider two proposals for defining black hole entropy in spherical symm
etry, where the horizon is defined locally as a trapping horizon. The first
case! boundary:terms in a dual-null form df the reduced action in two dime
nsions, gives a result that is proportional to the area. The second case, W
ald's Noether current method, is generalized to dynamic black holes giving
an entropy that is just the area of the trapping horizon. These results are
compared with a generalized first law of thermodynamics. [S0556-2821(99)03
918-1].