Astrocytes are morphologically complex cells, exemplified by their multiple processes and bushy territories. To analyze their elaborate morphology, we present a reliable protocol to perform intracellular Lucifer yellow iontophoresis in lightly fixed tissue.
Astrocytes are essential components of neural circuits. They tile the entire central nervous system (CNS) and are involved in a variety of functions, which include neurotransmitter clearance, ion regulation, synaptic modulation, metabolic support to neurons, and blood flow regulation. Astrocytes are complex cells that have a soma, several major branches, and numerous fine processes that contact diverse cellular elements within the neuropil. In order to assess the morphology of astrocytes, it is necessary to have a reliable and reproducible method to visualize their structure. We report a reliable protocol to perform intracellular iontophoresis of astrocytes using fluorescent Lucifer yellow (LY) dye in lightly fixed brain tissue from adult mice. This method has several features that are useful to characterize astrocyte morphology. It allows for three-dimensional reconstruction of individual astrocytes, which is useful to perform morphological analyses on different aspects of their structure. Immunohistochemistry together with LY iontophoresis can also be utilized to understand the interaction of astrocytes with different components of nervous system and to evaluate the expression of proteins within the labelled astrocytes. This protocol can be implemented in a variety of mouse models of CNS disorders to rigorously examine astrocyte morphology with light microscopy. LY iontophoresis provides an experimental approach to evaluate astrocyte structure, especially in the context of injury or disease where these cells are proposed to undergo significant morphological changes.
Astrocytes are the most abundant glial cells in the central nervous system (CNS). They play roles in ion homeostasis, blood flow regulation, synapse formation as well as elimination, and neurotransmitter uptake1. The wide range of astrocyte functions is reflected in their complex morphological structure2,3. Astrocytes contain several primary and secondary branches which divide into thousands of finer branchlets and leaflets that directly interact with synapses, dendrites, axons, blood vessels, and other glial cells. Astrocyte morphology varies across different brain regions, which may hint at their ability to perform their functions differentially in neuronal circuits4. Moreover, astrocytes are known to alter their morphology during development, during physiological conditions, and in multiple disease states3,5,6.
A consistent, reproducible method is needed to accurately resolve the complexity of astrocyte morphology. Traditionally, immunohistochemistry has been used to visualize astrocytes with the use of astrocyte specific or astrocyte enriched protein markers. However, these methods reveal the pattern of protein expression rather than the structure of the astrocyte. The commonly used markers, such as glial fibrillary acidic protein (GFAP) and S100 calcium binding protein β (S100β), do not express in the entire cell volume and thus do not resolve complete morphology7. Genetic approaches to express fluorescent proteins ubiquitously in astrocytes (viral injections or transgenic mouse reporter lines) can identify the finer branches and overall territory. However, it is difficult to differentiate individual astrocytes, and analyses may be biased by the astrocyte population targeted by the specific promoter8. Serial section electron microscopy has been used to reveal a detailed picture of the interactions of astrocyte processes with synapses. Due to the thousands of astrocyte processes contacting synapses, it is currently not possible to reconstruct an entire cell with this technique9, although this is expected to change with the use of machine learning approaches for data analysis.
In this report, we focus on a procedure to characterize mouse astrocytes using intracellular iontophoresis with Lucifer yellow (LY) dye, using the CA1 stratum radiatum as an example. The method is based on pioneering past work by Eric Bushong and Mark Ellisman10,11. Astrocytes from lightly fixed brain slices are identified by their distinctive soma shape and filled with LY. The cells are then imaged with confocal microscopy. We demonstrate how LY iontophoresis can be used to reconstruct individual astrocytes and perform detailed morphological analyses of their processes and territory. Also, this method can be applied in conjunction with immunohistochemistry to identify spatial relationships and interactions between astrocytes and neurons, other glial cells, and brain vasculature. We consider LY iontophoresis to be a very suitable tool to analyze morphology in different brain regions and mouse models of healthy or disease conditions7,12,13.
The animal experiments in this study were performed in accordance with the National Institute of Health Guide for the Care and Use of Laboratory Animals and were approved by the Chancellor's Animal Research Committee at the University of California, Los Angeles. Adult mice (6−8 weeks old) of mixed gender were used in all experiments.
1. Solution Preparation
2. Mouse Transcardial Perfusion and Brain Dissection
3. Slice Preparation
4. Electrode Preparation
5. Filling Astrocytes with Iontophoresis
6. Staining with Immunohistochemistry (Optional)
The data reported in this study are from 7−12 cells from 4 mice in each experiment. Average data are reported in the figure panels where appropriate.
To assess astrocyte morphology, we performed intracellular iontophoresis using LY dye to fill astrocytes in the CA1 stratum radiatum, which is summarized in Figure 1. Figure 2 depicts a representative astrocyte and its elaborate morphological structure. The cell was imaged post-fixation with the 60x oil immersion lens on a confocal laser-scanning microscope using the 488 nm laser line (step size of 0.3 µm and 3.0−3.5x digital zoom). The photomultiplier tube (PMT), offset, and gain functions of the confocal microscope were adjusted to create a high signal/ background ratio in the final image. In Figure 2A, single optical plane images from different z-steps (shown every 10 µm, labeled in order from 1−6) reveal the central soma and several major branches which divided into a dense network of processes. By generating a maximum intensity projection (stack size of 85 µm) we observed a detailed view of the structure of the astrocyte and its domain (Figure 2B). The main components of the astrocyte’s structure have also been noted. Figure 2C shows a zoom in (x4) maximum intensity projection of one major branch, several secondary branches, and the distribution of the surrounding branchlets and leaflets.
Morphological analyses and reconstructions of astrocytes were performed with Imaris analysis software (Table of Materials) using the post-fixation images of LY-filled astrocytes (other software such as ImageJ could also be used). After the reconstruction of each astrocyte was completed, the volumes of the soma, major branches, processes, and territory were quantified. The soma was created first with a surface smoothing set to the x-y plane resolution limit (0.25 µm). The minimum object diameter was set at 3.0 µm to remove other objects not associated with the cell body. To create the major branches, the intensity of the soma was masked, due to its brightness relative to the rest of the cell. The surface smoothing and minimum object diameter of the major branches was set to 0.3 µm (z plane step size). To create the processes, the intensity of the major branches was also masked. Surface smoothing was set to 0.18 µm and minimum object diameter was set to 0.3 µm. The territory of the astrocyte was created using a lower intensity threshold and surface smoothing set to 0.75 µm. Figure 3A shows the original image of a CA1 astrocyte. The cell body, the major branches, the processes, and the territory volume enclosed by the astrocyte are reconstructed in Figure 3B-E. After the reconstructions of the cells were created, the volumes of the soma, entire cell, and territory were quantified and the number of major branches was counted (Table 1). CA1 astrocytes from the stratum radiatum had an average soma volume of 488.91 µm3, average of ~7 primary branches, average cell volume of 5.58 x 103 µm3, and average territory volume of 2.94 x 104 µm3.
The well-characterized astrocyte marker, GFAP, is a cytoskeletal protein that labels the intermediate filaments of an astrocyte8. After astrocytes were dye filled, we performed immunostaining for GFAP to visualize expression in individual astrocytes (Figure 4). We found that GFAP was expressed in the cell soma, major branches, and some secondary branches of astrocytes, but not in the finer branches and processes (Figure 4A). No significant difference was found in the number of primary branches labeled by GFAP and those visualized by LY (p = 0.1573; Figure 4B). The cell area and volume of the astrocyte labeled by GFAP were significantly smaller than the area and volume visualized with LY (p < 0.0001; Figure 4C,D). This demonstrates that GFAP is a reliable marker for labeling major branches, but is not useful for determining the overall area or volume of the cell.
An important feature of astrocytes is their endfeet, which contact blood vessels and are proposed to help regulate blood flow in the CNS. To further understand the spatial relationship between astrocytes and brain vasculature, we stained with antibodies against aquaporin-4 following dye filling. Aquaporin-4 is a water channel protein found on astrocytes and ependymal cells, and is highly expressed in areas near ventricles and blood vessels15. We found that aquaporin-4 is expressed on astrocyte endfeet in close proximity to brain vasculature (Figure 5A). The image depicts three astrocyte endfeet contacting a blood vessel at different locations (indicated by the white arrows). In the CA1 stratum radiatum, the average number of endfeet per astrocyte was ~2 (Figure 5B). Interestingly, the branches containing endfeet were significantly thicker than the other primary branches of the astrocyte, using the major branch reconstructions (p = 0.0038; Figure 5C). We also measured the length of the branches containing endfeet from the center of the soma to the blood vessel and compared that to the shortest, direct path to the blood vessel. The actual length of the branches to the blood vessel was significantly greater than the shortest path (p = 0.0333; Figure 5D), which suggests that these branches tend to take a longer, circuitous route to the blood vessel. Movie 1 depicts a movie of a reconstruction of a LY-filled astrocyte and aquaporin-4 staining. The different structural components of the astrocyte (soma, major branches, processes, and territory) are represented in three dimensions. The LY-filled astrocyte together with the aquaporin-4 staining depict the astrocyte endfeet encircling the blood vessel. From the reconstruction of the major branches and the blood vessel, the branches that contain endfeet can be visualized extending from the soma to the vessel.
In the preceding sections, where p values are reported we used an unpaired Student’s t test, with significance at p < 0.05.
Figure 1: Diagram of workflow in LY iontophoresis. Schematic representation of protocol highlighting the critical steps. After the mouse was perfused with fixative, the brain was dissected. Following a short post-fixation period, coronal sections were cut with a vibratome. Electrode was backfilled with 1.5% LY dye. Astrocytes were identified in the CA1 stratum radiatum using IR-DIC on a light microscope. The soma of the cell was impaled by the electrode, and dye was injected into the cell by applying 0.5−1 V until the finer processes were completely filled. The slice was imaged with confocal microscopy using a 40x water immersion lens and then processed for immunohistochemistry. Further imaging was completed with a 60x oil immersion lens to perform cell reconstruction and morphological analysis. Shown is an example reconstruction of the processes. Please click here to view a larger version of this figure.
Figure 2: LY-filled astrocyte of CA1 stratum radiatum. (A) Single optical plane images from an astrocyte shown every 10 µm (labeled 1−6). (B) Maximum projection of the astrocyte, depicting the cell soma, several major branches, and numerous processes which make up its bushy territory. (C) Maximum projection (zoom x4) of one major branch (from section outlined in yellow), two secondary branches, several branchets, and the organization of the surrounding processes. Scale bar = 10 µm. Please click here to view a larger version of this figure.
Figure 3: Reconstruction of a LY-filled astrocyte and its components. (A) CA1 astrocyte filled with LY. (B-E) Three-dimensional reconstruction of the soma (B), soma and major branches (C), processes (D), and territory (E) at 0° and 45° orientation. Scale bar = 10 µm. Please click here to view a larger version of this figure.
Figure 4: GFAP immunostaining in LY-filled astrocytes. (A) Representative z-projection of LY (green) and GFAP (magenta) staining. GFAP is expressed primarily in the primary and some secondary branches of the astrocyte, but was not found within the entire astrocyte territory. Scale bar = 10 µm. (B) Graph of number of primary branches labeled by LY and GFAP. (C) Cell area denoted by LY and GFAP staining. (D) Cell volume denoted by LY and GFAP staining. Open circles are raw data with closed squares indicating mean ± SEM. Data was collected from 12 cells from 4 mice. Please click here to view a larger version of this figure.
Figure 5: Aquaporin-4 immunostaining in LY-filled astrocytes. (A) Representative z-projection of LY (green) and aquaporin-4 staining (magenta). Aquaporin-4 is expressed mainly in the endfeet of the astrocyte. White arrows denote the three endfeet as they contact a nearby blood vessel. Scale bar = 10 µm. (B) Number of branches with endfeet per astrocyte. (C) Thickness of branches with endfeet in comparison to the other primary branches of astrocytes. (D) Length of branches with endfeet in comparison to the shortest path to the blood vessel. Open circles are raw data with closed squares indicating mean ± SEM. Data was collected from 7 cells from 4 mice. Please click here to view a larger version of this figure.
Movie 1: Reconstruction of a LY-filled astrocyte and aquaporin-4 staining. Representative movie of a CA1 astrocyte in proximity to a blood vessel. The soma, major branches, processes, and territory were reconstructed to analyze the morphology of the cell. The reconstruction of the major branches together with aquaporin-4 depict two astrocyte endfeet directly contacting the blood vessel. Please click here to view this video. (Right-click to download.)
Morphological characteristics | Mean ± SEM |
Soma volume (µm3) | 489 ± 30 |
Number of primary branches | 7.0 ± 0.5 |
Cell volume (µm3) | 5580 ± 425 |
Territory volume (µm3) | 29391 ± 8150 |
Number of cells | 14 |
Table 1: Morphological analysis of astrocyte structure. The astrocyte soma volume, number of primary branches per astrocyte, astrocyte cell volume, and volume enclosed by astrocyte territory are shown. Data was collected from 14 cells from 7 mice.
The method outlined in this paper describes a way to visualize astrocyte morphology using intracellular iontophoresis of LY dye in lightly fixed brain slices. There are several critical factors highlighted in this protocol that contribute to successful LY iontophoresis and morphological reconstruction of the cells. One factor is the quality and reproducibility of the images, which is determined largely by the age of the mouse and the outcome of the perfusion. In this study, we used C57/BL6N mice 6−8 weeks old. A successful perfusion (highly dependent on the proper placement of the perfusing needle and noted by a white-colored brain and absence of blood in brain vasculature) is necessary for the most detailed and clearly filled cells. After impalement by an electrode, the cell membrane should maintain a tight seal around the tip of the electrode and prevent dye from leaking out. Despite best efforts, occasionally other structures outside of the cell will be filled as the pipette is advanced through brain tissue: we excluded these cells from the analysis. The resistance of the electrodes is an additional key factor. The high resistance only allows a steady ejection of dye from the electrode tip upon voltage stimulation. More technically, it is important to maintain gentle, slow movements when impaling the soma of the cell with the electrode. Electrode penetration through the cell can lead to dye leakage from the soma. A successful impalement followed by voltage application should result in almost immediate dye filling of the cell body and processes (i.e., within a few seconds). The time required to completely fill an astrocyte is related to the territory it encompasses; however, wait to ensure the finer processes are completely filled (at least 15 min).
We found this protocol to be a most faithful way to study astrocyte morphology in detail, nonetheless, the method has its limitations. Identifying a cell can be time-consuming and error prone. Under IR-DIC, one should identify distinctive features that mark the specific cell type (soma shape and size). Alternatively, the expression of red fluorescent reporters specifically in astrocytes, by viral injection or a transgenic mouse reporter line, allows for easier identification of these cells before filling. Also, LY is limited as a cytosolic dye because it cannot be used to label the astrocyte membrane, in comparison to labeling with a membrane-tethered GFP, such as Lck-GFP16. Lck-GFP would give a more accurate representation of the entire territory area, as LY iontophoresis reveals the internal volume of an astrocyte. However, depending on the experimental design, LY iontophoresis is better suited to resolve the entire astrocyte internal volume, develop three-dimensional reconstructions, and quantify the anatomical components that make up an astrocyte’s structure6. Finally, as with all forms of confocal microscopy, spatial resolution is limited by diffraction, noted as the point spread function of the microscope optics17. Altering components of the imaging system, such as decreasing pinhole diameter, will help improve the images, but the true resolution is determined by the wavelength of light and the numerical aperture of the objective lens. In our case, we estimate the best resolution possible is probably around 300 nm, which is likely to be worse in the z-axis.
LY iontophoresis offers several advantages over other commonly used methods to label astrocytes. The protocol can be applied in any established mouse model, cell population, or brain region18,19,20 as it is not limited by an astrocyte specific promoter or a transgenic mouse line. Genetic approaches to express fluorescent proteins ubiquitously in astrocytes by viral injections or transgenic mouse reporter lines (i.e., td-Tomato) require the use of an astrocyte promoter, which, in some regions, can be expressed in other cell types or not include all the astrocytes21. LY iontophoresis is also time-efficient, as viral injections of fluorescent proteins require surgery and time to express the specific virus, and transgenic mouse lines require breeding. Finally, LY iontophoresis is a useful method to distinguish individual cells, while other strategies would also need to be combined with a method for sparse labeling to visualize the territories of individual astrocytes22,23,24. However, no one method is a panacea and the choice of which is used needs to be tailored to the specific question being addressed.
Future studies can employ specific experimental manipulations and examine different components of astrocyte structure (soma, branches, processes, territory, etc.) to answer morphological questions. This could provide insight and direction into astrocyte morphology and its functional implications, which could be analyzed further by super resolution light microscopy or electron microscopy4. For example, LY iontophoresis provides a means to visualize fine astrocyte processes, which contact thousands of synapses and are involved in synaptic functions. Studying how the structure of these processes changes in different pathological conditions could help elucidate the roles of astrocytes in health and disease. LY iontophoresis is an important technique to visualize detailed cell morphology and characterize astrocyte properties to better understand their functions in the central nervous system.
The authors have nothing to disclose.
The authors thank Ms. Soto, Dr. Yu, and Dr. Octeau for guidance as well as comments on the text. This work is supported by NS060677.
10% Buffered Formalin Phosphate | Fisher | SF 100-20 | An identical alternative can be used |
Acrodisc Syringe Filters with Supor Membrane | Pall | 4692 | An identical alternative can be used |
Ag/AgCl ground pellet | WPI | EP2 | A similar alternative can be used |
Alexa Fluor 546 goat anti-chicken IgG (H+L) | Thermo Scientific | A-11040 | A similar alternative can be used |
Alexa Fluor 647 goat anti-rabbit IgG (H+L) | Thermo Scientific | A27040 | A similar alternative can be used |
Anti Aquaporin-4 antibody | Novus Biologicals | NBP1-87679 | A similar alternative can be used |
Anti GFAP antibody | Abcam | ab4674 | A similar alternative can be used |
Borosilicate glass pipettes with filament | World precision instruments | 1B150F-4 | |
C57BL/6NTac mice | Taconic Stock | B6 | A similar alternative can be used |
Calcium Chloride | Sigma | 21108 | An identical alternative can be used |
Confocal laser-scanning microscope | Olympus | FV1000MPE | A similar alternative can be used |
D-glucose | Sigma | G7528 | An identical alternative can be used |
Disodium Phosphate | Sigma | 255793 | An identical alternative can be used |
Electrode puller- Model P-97 | Sutter | P-97 | A similar alternative can be used |
Fluoromount-G | Southern Biotech | 0100-01 | An identical alternative can be used |
Heparin sodium injection (1,000 USP per mL) | Sagent Pharmaceuticals | 400-10 | An identical alternative can be used |
Imaris software (Version 7.6.5) | Bitplane Inc. | A similar alternative can be used | |
Isofluorane | Henry Schein Animal Health | 29404 | An identical alternative can be used |
Lidocaine Hydrochloride Injectable (2%) | Clipper | 1050035 | An identical alternative can be used |
Lucifer Yellow CH dilithium salt | Sigma | L0259 | |
Lucifer Yellow CH dipotassium salt | Sigma | L0144 | |
Magnesium Chloride | Sigma | M8266 | An identical alternative can be used |
Microscope Cover Glass | Thermo Scientific | 24X60-1 | An identical alternative can be used |
Microscope Slides | Fisher | 12-544-2 | An identical alternative can be used |
Normal Goat Serum | Vector Laboratories | S-1000 | An identical alternative can be used |
Objective lens (40x) | Olympus | LUMPLFLN 40XW | A similar alternative can be used |
Objective lens (60x) | Olympus | PlanAPO 60X | A similar alternative can be used |
PBS tablets, 100 mL | VWR | VWRVE404 | An identical alternative can be used |
Pipette micromanipulator- Model ROE-200 | Sutter | MP-285 / ROE-200 / MPC-200 | A similar alternative can be used |
Potassium Chloride | Sigma | P3911 | An identical alternative can be used |
Sodium Bicarbonate | Sigma | S5761 | An identical alternative can be used |
Sodium Chloride | Sigma | S5886 | An identical alternative can be used |
Stimulator- Model Omnical 2010 | World precision instruments | Omnical 2010 | A similar alternative can be used |
Triton X 100 | Sigma | T8787 | An identical alternative can be used |
Vibratome- Model #3000 | Pelco | 100-S | A similar alternative can be used |