Cl. Dumke et al., ROD OUTER SEGMENT STRUCTURE INFLUENCES THE APPARENT KINETIC-PARAMETERS OF CYCLIC-GMP PHOSPHODIESTERASE, The Journal of general physiology, 103(6), 1994, pp. 1071-1098
Cyclic GMP hydrolysis by the phosphodiesterase (PDE) of retinal rod ou
ter segments (ROS) is a key amplification step in phototransduction. D
efinitive estimates of the turnover number, k(cat), and of the K-m are
crucial to quantifying the amplification contributed by the PDE. Publ
ished estimates for these kinetic param eters vary widely; moreover, l
ight-dependent changes in the K-m of PDE have been reported. The exper
iments and analyses reported here account for most observed variations
in apparent K-m, and they lead to definitive estimates of the intrins
ic kinetic parameters in amphibian rods. We first obtained a new and h
ighly accurate estimate of the ratio of holo-PDE to rhodopsin in the a
mphibian ROS, 1:270. We then estimated the apparent kinetic parameters
of light-activated PDE of suspensions of disrupted frog ROS whose str
uctural integrity was systematically varied. Tn the most severely disr
upted ROS preparation, we found K-m = 95 mu M and k(cat) = 4,400 cGMP.
s(-1). In suspensions of disc-stack fragments of greater integrity, th
e apparent K-m increased to similar to 600 mu M, though k(cat) remaine
d unchanged. In contrast, the K-m for cAMP was not shifted in the disc
stack preparations. A theoretical analysis shows that the elevated ap
parent K-m of suspensions of disc stacks can be explained as a consequ
ence of diffusion with hydrolysis in the disc stack, which causes acti
ve PDEs nearer the center of the stack to be exposed to a lower concen
tration of cyclic GMP than PDEs at the disc stack rim. The analysis pr
edicts our observation that the apparent K-m for cGMP is elevated with
no accompanying decrease in k(cat). The analysis also predicts the la
ck of a K-m shift for cAMP and the previously reported light dependenc
e of the apparent K-m for cGMP. We conclude that the intrinsic kinetic
parameters of the PDE do not vary with light or structural integrity,
and are those of the most severely disrupted disc stacks.