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Astrocytic IP(3)Rs: Beyond IP(3)R2

Astrocytes are sensitive to ongoing neuronal/network activities and, accordingly, regulate neuronal functions (synaptic transmission, synaptic plasticity, behavior, etc.) by the context-dependent release of several gliotransmitters (e.g., glutamate, glycine, D-serine, ATP). To sense diverse input, a...

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Autores principales: Sherwood, Mark W., Arizono, Misa, Panatier, Aude, Mikoshiba, Katsuhiko, Oliet, Stéphane H. R.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Frontiers Media S.A. 2021
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8363081/
https://www.ncbi.nlm.nih.gov/pubmed/34393726
http://dx.doi.org/10.3389/fncel.2021.695817
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author Sherwood, Mark W.
Arizono, Misa
Panatier, Aude
Mikoshiba, Katsuhiko
Oliet, Stéphane H. R.
author_facet Sherwood, Mark W.
Arizono, Misa
Panatier, Aude
Mikoshiba, Katsuhiko
Oliet, Stéphane H. R.
author_sort Sherwood, Mark W.
collection PubMed
description Astrocytes are sensitive to ongoing neuronal/network activities and, accordingly, regulate neuronal functions (synaptic transmission, synaptic plasticity, behavior, etc.) by the context-dependent release of several gliotransmitters (e.g., glutamate, glycine, D-serine, ATP). To sense diverse input, astrocytes express a plethora of G-protein coupled receptors, which couple, via G(i/o) and G(q), to the intracellular Ca(2+) release channel IP(3)-receptor (IP(3)R). Indeed, manipulating astrocytic IP(3)R-Ca(2+) signaling is highly consequential at the network and behavioral level: Depleting IP(3)R subtype 2 (IP(3)R2) results in reduced GPCR-Ca(2+) signaling and impaired synaptic plasticity; enhancing IP(3)R-Ca(2+) signaling affects cognitive functions such as learning and memory, sleep, and mood. However, as a result of discrepancies in the literature, the role of GPCR-IP(3)R-Ca(2+) signaling, especially under physiological conditions, remains inconclusive. One primary reason for this could be that IP(3)R2 has been used to represent all astrocytic IP(3)Rs, including IP(3)R1 and IP(3)R3. Indeed, IP(3)R1 and IP(3)R3 are unique Ca(2+) channels in their own right; they have unique biophysical properties, often display distinct distribution, and are differentially regulated. As a result, they mediate different physiological roles to IP(3)R2. Thus, these additional channels promise to enrich the diversity of spatiotemporal Ca(2+) dynamics and provide unique opportunities for integrating neuronal input and modulating astrocyte–neuron communication. The current review weighs evidence supporting the existence of multiple astrocytic-IP(3)R isoforms, summarizes distinct sub-type specific properties that shape spatiotemporal Ca(2+) dynamics. We also discuss existing experimental tools and future refinements to better recapitulate the endogenous activities of each IP(3)R isoform.
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spelling pubmed-83630812021-08-14 Astrocytic IP(3)Rs: Beyond IP(3)R2 Sherwood, Mark W. Arizono, Misa Panatier, Aude Mikoshiba, Katsuhiko Oliet, Stéphane H. R. Front Cell Neurosci Cellular Neuroscience Astrocytes are sensitive to ongoing neuronal/network activities and, accordingly, regulate neuronal functions (synaptic transmission, synaptic plasticity, behavior, etc.) by the context-dependent release of several gliotransmitters (e.g., glutamate, glycine, D-serine, ATP). To sense diverse input, astrocytes express a plethora of G-protein coupled receptors, which couple, via G(i/o) and G(q), to the intracellular Ca(2+) release channel IP(3)-receptor (IP(3)R). Indeed, manipulating astrocytic IP(3)R-Ca(2+) signaling is highly consequential at the network and behavioral level: Depleting IP(3)R subtype 2 (IP(3)R2) results in reduced GPCR-Ca(2+) signaling and impaired synaptic plasticity; enhancing IP(3)R-Ca(2+) signaling affects cognitive functions such as learning and memory, sleep, and mood. However, as a result of discrepancies in the literature, the role of GPCR-IP(3)R-Ca(2+) signaling, especially under physiological conditions, remains inconclusive. One primary reason for this could be that IP(3)R2 has been used to represent all astrocytic IP(3)Rs, including IP(3)R1 and IP(3)R3. Indeed, IP(3)R1 and IP(3)R3 are unique Ca(2+) channels in their own right; they have unique biophysical properties, often display distinct distribution, and are differentially regulated. As a result, they mediate different physiological roles to IP(3)R2. Thus, these additional channels promise to enrich the diversity of spatiotemporal Ca(2+) dynamics and provide unique opportunities for integrating neuronal input and modulating astrocyte–neuron communication. The current review weighs evidence supporting the existence of multiple astrocytic-IP(3)R isoforms, summarizes distinct sub-type specific properties that shape spatiotemporal Ca(2+) dynamics. We also discuss existing experimental tools and future refinements to better recapitulate the endogenous activities of each IP(3)R isoform. Frontiers Media S.A. 2021-07-30 /pmc/articles/PMC8363081/ /pubmed/34393726 http://dx.doi.org/10.3389/fncel.2021.695817 Text en Copyright © 2021 Sherwood, Arizono, Panatier, Mikoshiba and Oliet. https://creativecommons.org/licenses/by/4.0/This is an open-access article distributed under the terms of the Creative Commons Attribution License (CC BY). The use, distribution or reproduction in other forums is permitted, provided the original author(s) and the copyright owner(s) are credited and that the original publication in this journal is cited, in accordance with accepted academic practice. No use, distribution or reproduction is permitted which does not comply with these terms.
spellingShingle Cellular Neuroscience
Sherwood, Mark W.
Arizono, Misa
Panatier, Aude
Mikoshiba, Katsuhiko
Oliet, Stéphane H. R.
Astrocytic IP(3)Rs: Beyond IP(3)R2
title Astrocytic IP(3)Rs: Beyond IP(3)R2
title_full Astrocytic IP(3)Rs: Beyond IP(3)R2
title_fullStr Astrocytic IP(3)Rs: Beyond IP(3)R2
title_full_unstemmed Astrocytic IP(3)Rs: Beyond IP(3)R2
title_short Astrocytic IP(3)Rs: Beyond IP(3)R2
title_sort astrocytic ip(3)rs: beyond ip(3)r2
topic Cellular Neuroscience
url https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8363081/
https://www.ncbi.nlm.nih.gov/pubmed/34393726
http://dx.doi.org/10.3389/fncel.2021.695817
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