Introduction
The presence of secretory vesicles (synaptic-like microvesicles or SLMVs) in astrocytes capable of fine-tuning synaptic transmission, has been a topic of debate in the field. While some studies have suggested that astrocytes release gliotransmitters through SNARE-dependent vesicular exocytosis, other studies presented contradictory data suggesting that astrocytes release in a non-regulated manner, such as through lysosomes, or non-vesicular pathways such as channels (reviewed in Hamilton and Attwell, ; Savtchouk and Volterra, 2018). Evidence showing the presence of secretory vesicles in astrocytes in situ would support regulated exocytosis; nevertheless, efforts to investigate the presence of these organelles at the ultrastructural level, using electron microscopy, failed to convince skeptical scientists so far (Bezzi et al., ; Bergersen et al., ). Two important studies (Petravicz et al., 2008; Agulhon et al., ) heated the debate, by showing that astrocytic calcium signaling has no impact on synaptic activity (Smith, 2010). Moreover, murine models developed to impair astrocytic SLMVs exocytosis such as the dnSnare or IP3RKO (Pascual et al., 2005; Sherwood et al., 2021) show weak behavioral phenotype. Nevertheless, we still use genetic models to study astrocytic impact on synaptic activity, somehow upstreaming SLMVs exocytosis (Petrelli et al., 2020, 2023). Indeed, calcium signaling has been largely used as a proxy to study the dynamics of SLMVs release in culture (Calì et al., ; Cali et al., ; Marchaland et al., 2008; Vardjan et al., 2019; Stenovec et al., 2020; Mielnicka and Michaluk, 2021), leading to in vivo studies with the assumption that neuroglia functional interactions might be due to astrocytic SLMVs exocytosis (Kirchhoff, ; Wiedemann, 2010; Bindocci et al., ; de Ceglia et al., ). Aforementioned reasons led to a progressive abandonment of this quest, leaving the problem almost as a religious question, where believers don't need further proofs, and conversely no evidence will be enough for those who don't believe in it. Here, we review the current state of the art regarding our knowledge of exocytotic SLMVs in astrocytes.
Ultrastructural evidence using EM
To date, the best way to study cellular ultrastructure from a morphological level, is by far Electron Microscopy (EM). In fact, by increasing resolution limit by a factor of two compared to fluorescence microscopy, it is the only technique capable of unequivocally identify nanometer-sized structures (Knott and Genoud, ; Boges et al., ). This includes small, astrocytic perisynaptic astrocytic processes (PAPs), and their organelles.
The use of volume EM to characterize astrocytes fine morphology
Identifying processes on a single section EM micrograph could be misleading. Depending on the direction and position of the cut, a cellular process could be mistaken for something similar in its cross-section (e.g., small axons and microglial processes on a single section might have a similar round morphology and diameter). Volume Electron Microscopy (VEM) allows navigating along z-stacks, and observing single processes at multiple heights to make sure about who-is-what (Titze and Genoud, 2016). VEM became more and more common since a seminal paper was published in 2004 (Denk and Horstmann, ). Taking on a concept from 1981 (Leighton, ), it has been shown how SEM combined with an ultramicrotome and a high-resolution back scattered detector for block face imaging could be used to observe large portion of tissues with similar quality and resolution to classic serial-section TEM for biological application, and automatically cut serial sections at the same time (Denk and Horstmann, ). Although this technique has been originally developed to solve the so-called connectome (DeFelipe, ; Oh et al., 2014; Fua and Knott, ; Wanner et al., 2015), few papers managed to produce high-resolution 3D reconstructions of full morphologies of astrocytes by adapting VolumeEM to study glial cells (Coggan et al., ).
By using this approach, several labs interested in astrocytes have started an important work in the field, describing the astrocytic ultrastructure in three dimension, and quantifying parameters such as synaptic ensheathment, surface are to volume ratio (SVR), and working on ontologies to define a proper nomenclature of astrocytic processes in the parenchyma (reviewed in Calì, ). In the last 5 years, three of them focused on escheatment of full astrocytes on neurites, such as Calyx of Held (Heller et al., ), or relationships with vasculature, one of the most distinctive hallmarks of astrocytes in all regions of the CNS (Albargothy et al., ). Nevertheless, astrocytes participate to parenchymal homeostasis at many levels, hence many works have analyzed general aspects of structural neuro-glia relationships (Cali et al., ; Shapson-Coe et al., 2021; Møller et al., 2022; Turner et al., 2022; Salmon et al., 2023).
In a beautiful piece of work, authors have quantified the finest nanoarchitecture of diverse astrocytic processes, using computer vision methods specifically tailored for astrocytes (Salmon et al., 2023). To this regard, the use of VEM, combined with state-of-the-art computer vision techniques (Agus et al., ), could be a novel unbiased tool to identify astrocytic microdomains hosting SLMVs.
EM sample preparation: stained or unstained?
When someone wants to approach the problem of studying astrocytes using EM, the first problem is clearly to identify them. While immunohistochemistry (IHC) allows the identification of astrocytes using specific markers [e.g., GFAP, S100Beta, glutamate transporters GLT-1 or GLAST... (Figure 1A)], it also requires a permeabilization step needed to allow antibodies to penetrate the tissue. Permeabilization physically damages membranes; while this is hardly a problem for fluorescence microscopy, it visibly degrades image quality under EM. Hence, in order to study proper ultrastructure, one should rather observe unstained tissue, with perfectly preserved membranes. Classic staining protocols allows to study brain ultrastructure (Titze and Genoud, 2016), but tissue dehydration is known to induce artifacts in particular in the preservation of extracellular matrix. Recent advancements include the use of high-pressure freezing, a technique which vitrifies tissue, using water from the sample itself fix the sample (Schertel et al., 2013; Korogod et al., ), supposedly preserving sample in their most natural state. Nevertheless, this technique is difficult to set up, and fails in staining large volumes of samples.
Figure 1
Identification of PAPs and ultrastructural organelles in unstained tissue
Either way, identification of astrocytic processes in unstained tissue requires some training and understanding of electron micrographs. A good practice for beginners is to use empiric criteria that can be inferred from solid, well cited literature. If one has to look for astrocytes in EM micrographs then, one of the oft quoted sentences to this regard, is that astrocytic processes usually have an irregular shape, and a relatively clear cytoplasm (Ventura and Harris, 1999; Witcher et al., 2007; Nahirney and Tremblay, 2021). This sentence in particular comes from the classic “The fine structure of the nervous system,” from Peters et al. (1976) and possibly led to the misbelief that astrocytes are rather devoid of intracellular organelles, including ER, cisterns, or vesicles, especially in PAPs in close apposition to synapses.
Ultrastructural basis of Ca2+ signaling to show rich intracellular content in PAPs
As previously mentioned, the study of astrocytic Ca2+ waves have been used as a proxy to characterize SLMVs dynamics, which are hard to study in vivo. In fact, a rich body of literature, in the first decade of 2000, has studied SLMVs exocytosis in vitro using astrocytic cell cultures (Calì et al.,
Evidence for SLMVs in astrocytes
SLMVs are round, clear, with a diameter of 50 nm, and resemble glutamatergic vesicles in excitatory boutons (Bezzi et al.,
State of the art on the quest of exocytotic organelles
In the last 10 years, only a few research papers have specifically characterized exocytosis of synaptic-like microvesicles from astrocytes (Cali et al.,
Large-scale VEM to look for SLMVs
One very elegant study (Kiyoshi et al.,
Conclusions
The presence of secretory synaptic-like microvesicles in astrocytes has a solid base of correlative data, suggesting that astrocytes participate to neuronal signaling by fine tuning synaptic transmission in a fast and highly-regulated manner. Nevertheless, ultimate proof, to show them under electron microscopy in independent studies from different labs, is still missing. Few recent studies (Aboufares El Alaoui et al.,
Questions that might help to find an answer are:
Do exocytotic microdomains in astrocytes exists?
Which types of synapses benefit from gliotransmission?
Are astrocytic SLMVs clustered like in synaptic boutons?
Are SLMVs an exclusive feature of hippocampal synapses?
In the end, those who don't believe we went to the moon often cite the lack of photos of the landing sites, and that we can't really see any equipment left there using our imaging systems. This does not really mean that Neil Amstrong did not put his foot on the moon in 1969; simply, we are still not that good at looking into it.
Statements
Author contributions
CC: Conceptualization, Funding acquisition, Visualization, Writing – original draft, Writing – review & editing.
Funding
The author(s) declare that financial support was received for the research, authorship, and/or publication of this article. This work was supported by the GFI to CC.
Conflict of interest
The author declares that the research was conducted in the absence of any commercial or financial relationships that could be construed as a potential conflict of interest.
Publisher’s note
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Summary
Keywords
synaptic-like microvesicles, SLMVs, astrocyte, gliotransmission, exocytosis, volume electron microscopy, vEM, 3D reconstruction
Citation
Calì C (2024) Regulated exocytosis from astrocytes: a matter of vesicles?. Front. Neurosci. 18:1393165. doi: 10.3389/fnins.2024.1393165
Received
28 February 2024
Accepted
30 April 2024
Published
10 May 2024
Volume
18 - 2024
Edited by
Renaud Blaise Jolivet, University of Geneva, Switzerland
Reviewed by
Irma Lorena Arancibia Carcamo, University College London, United Kingdom
Linda Hildegard Bergersen, University of Oslo, Norway
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© 2024 Calì.
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*Correspondence: Corrado Calì corrado.cali@unito.it
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