Whether astrocytes predominantly express ohmic K+ channels in vivo, and how expression of different K+ channels affects [K+]ohomeostasis in the CNS have been long-standing questions for how astrocytes function. In the present study, we have addressed some of these questions in glial fibrillary acidic protein [GFAP(+)], freshly isolated astrocytes (FIAs) from CA1 and CA3 regions of P7–15 rat hippocampus. As isolated, these astrocytes were uncoupled allowing a higher resolution of electrophysiological study. FIAs showed two distinct ion current profiles, with neither showing a purely linear I-V relationship. One population of astrocytes had a combined expression of outward potassium currents ( I Ka, I Kd) and inward sodium currents ( I Na). We term these outwardly rectifying astrocytes (ORA). Another population of astrocytes is characterized by a relatively symmetric potassium current pattern, comprising outward I Kdr, I Ka, and abundant inward potassium currents ( I Kin), and a larger membrane capacitance ( C m ) and more negative resting membrane potential (RMP) than ORAs. We term these variably rectifying astrocytes (VRA). The I Kin in 70% of the VRAs was essentially insensitive to Cs+, while I Kin in the remaining 30% of VRAs was sensitive. The I Ka of VRAs was most sensitive to 4-aminopyridine (4-AP), while I Kdr of ORAs was more sensitive to tetraethylammonium (TEA). ORAs and VRAs occurred approximately equally in FIAs isolated from the CA1 region (52% ORAs versus 48% VRAs), but ORAs were enriched in FIAs isolated from the CA3 region (71% ORAs versus 29% VRAs), suggesting an anatomical segregation of these two types of astrocytes within the hippocampus. VRAs, but not ORAs, showed robust inward currents in response to an increase in extracellular K+ from 5 to 10 mM. As VRAs showed a similar current pattern and other passive membrane properties (e.g., RMP, R in) to “passive astrocytes”in situ (i.e., these showing linear I-V curves), such passive astrocytes possibly represent VRAs influenced by extensive gap-junction coupling in situ. Thus, our data suggest that, at least in CA1 and CA3 regions from P7–15 rats, there are two classes of GFAP(+) astrocytes which possess different K+ currents. Only VRAs seem suited to uptake of extracellular K+ via I Kin channels at physiological membrane potentials and increases of [K+]o. ORAs show abundant outward potassium currents with more depolarized RMP. Thus VRAs and ORAs may cooperate in vivo for uptake and release of K+, respectively.
Muscle Velocity Recovery Cycles to Examine Muscle Membrane Properties