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Department of Neurobiology, Physiology, and Behavior, College of Biological Sciences, University of California, Davis, Davis, California 95616
Address all correspondence and requests for reprints to: Lynnette Gerhold, Ph.D., Northwestern University, Department of Neurobiology and Physiology, 2205 Tech Drive, Evanston, Illinois 60208. E-mail: l-gerhold{at}northwestern.edu.
| Abstract |
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| Introduction |
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Studies from our laboratory (16) demonstrate that the surface area of astrocytes that surround GnRH neuronal cell bodies in the organun vasculosum of the lamina terminalis (OVLT) and the rostral region of the medial preoptic nucleus (rMPN) exhibit diurnal rhythms: surface area is high on the morning of proestrus and decreases throughout the afternoon. This retraction of processes and reduction in surface area is thought to allow stimulatory inputs to GnRH neurons to induce preovulatory GnRH synthesis and secretion. Vasoactive intestinal polypeptide (VIP) is a neurotransmitter and neurotrophic factor (17, 18, 19) that exerts broad and diverse actions in several brain regions by acting on neurons and astrocytes to stimulate the release of one or more factors that directly or indirectly affect synaptogenesis of neurons (17, 19). In the suprachiasmatic nucleus (SCN) within the hypothalamus, VIP entrains diurnal rhythms in the SCN and GnRH neurons (20); whereas, in the cortex, VIP acts as a neurotrophic factor. Originally, VIP was thought to act predominantly by directly modulating neuronal activity. More recently it has become clear that VIP influences neurons in the cortex through activation of VIP receptors located on astrocytes (17, 19). However, it is not known whether and/or how VIP influences diurnal rhythms in the morphometry of astrocytes that surround GnRH neurons.
Aging involves changes in GnRH neuronal activation (21, 22, 23), and VIP is critical to the activation of GnRH neurons (20). In the SCN, VIP mRNA decreases with age (24). Aging also attenuates dynamic changes in astrocyte morphometry (16). This age-related attenuation in diurnal rhythms of VIP and astrocyte morphometry has been correlated with diminution of diurnal rhythms in GnRH neuronal synthesis and activity (21, 22, 23, 25) and an attenuated and delayed LH surge (26).
The goal of this study was to assess whether there is a functional relationship between the diurnal rhythmicity in VIP activity in the SCN and the rhythmicity in astrocyte morphometry. We hypothesized that VIP may indirectly affect GnRH neurons by influencing astrocytes that are associated with these neurons. Furthermore, we tested the hypothesis that blockade of VIP rhythms would result in aging-like changes in the diurnal rhythm of the morphometry of astrocytes surrounding GnRH neurons, which in turn may lead to a decline in GnRH neuronal function.
| Materials and Methods |
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Stereotaxic surgery
Stereotaxic surgeries in young animals were performed based on the protocols of Harney et al. (31) and Gerhold et al. (20), which are briefly described below. Five days after OVX (d 5), rats were anesthetized with ketamine (49 mg/ml)/xylazine (1.8 mg/ml) and implanted with bilateral guide tubes directed stereotaxically at the SCN (1.5 mm apart; 9 mm in length; 26 gauge; Plastics One Inc., Roanoke, VA). Two days after bilateral guide tube implantation (d 7), VIP antisense or random sequence oligos (0.5 µg in 0.5 µl saline per side; Invitrogen Life Technologies, Carlsbad, CA) were infused over a 4-min interval at 0800 h through cannulae implanted bilaterally in the guide tubes. The antisense oligonucleotides were 20-mers complementary to the cap site (5'-GCTCTGCACTACAACCTGAC-3') and translation start site (5'-TTGCTTCTGGATTCCATCTC-3') of the rat VIP mRNA (32). Control oligonucleotides had the same ATGC content as antisense oligonucleotides but in random order that had no significant homology to any known peptide localized in the SCN. At the same time, rats were implanted with SILASTIC brand capsules containing E2 dissolved in sesame oil. Rats were killed 2 d later (d 9) at 43 h (0400 h), 53 h (1400 h), and 57 h (1800 h) after injection. Antisense and random sequence oligo-treated rats as well as a group of middle-aged regularly cycling female rats (OVX, d 0, E2 implanted d 7, and killed d 9) were transcardially perfused with 4% paraformaldehyde (Sigma), and the brains were removed, sectioned coronally, and stored in cyroprotectant at 20 C until processed for immunocytochemistry. The SCN was checked for correct cannulae placement as the brains were sectioned (n = 610 rats per time point per treatment). VIP antisense treatment effectively suppresses VIP concentrations in the SCN (20).
Immunocytochemistry: VPAC2 receptor/glial fibrillary acidic protein (GFAP)
Coronal brain sections (40 µm) were cut in a cryostat (Microm, Kalamazoo, MI) starting at the level of the medial diagonal band of Broca (bregma 0.20 mm) (33) through the arcuate nucleus (bregma 3.80 mm) (33). Each brain was collected in a series of six sets with every sixth section represented in a group and stored in cyroprotectant until processed for immunocytochemistry. Antibodies against GFAP (Sigma) and VPAC2 receptor (VIP receptor subtype) (Santa Cruz Biotechnology, Santa Cruz, CA) were used to determine whether astrocytes express this VIP receptor subtype. On d 1, sections from one series that contains every sixth section were rinsed in 0.1 M Tris-buffered saline (TBS) and blocked with 10% normal horse serum plus 0.4% Triton X-100 (NHS-X) for 1 h at room temperature. Next, sections were incubated in mouse anti-GFAP (1:50,000) in 2% NHS-X overnight at 4 C. On d 2, sections were rinsed in TBS and incubated in Cy2-conjugated antimouse IgG (Jackson ImmunoReseach Laboratories, West Grove, PA) diluted 1:500 in 2% NHS-X for 1 h at room temperature. Sections were rinsed in TBS and incubated in goat anti-VPAC2 receptor (1:1000) in 2% NHS-X for 2 d at 4 C. On d 4, sections were rinsed in TBS and incubated in Cy3-conjugated antigoat IgG (Jackson ImmunoReseach Laboratories) diluted 1:500 in 2% NHS-X for 1 h at room temperature. Sections were rinsed and mounted on slides and coverslips were applied using Permount (Fisher Scientific, Pittsburgh, PA). For a control experiment, a separate set of sections was processed for GFAP immunoreactivity; however, the primary antibody, VPAC2, was omitted from the 2% NHS-X, whereas incubating for 2 d before incubating with the secondary Cy3-conjugated antigoat IgG for 1 h. No VPAC2 receptor immunoreactivity was detected with omission of the antibody. In addition, we used the blocking peptide supplied (Santa Cruz Biotechnology) with this antibody and added it to the antibody to determine specificity of the antibody. No VPAC2 receptor immunoreactivity was detected.
Immunocytochemistry: GFAP/GnRH
Antibodies against GnRH (LR-5, Benoit, Montreal, Canada) and GFAP (Sigma) were used to identify astrocytes surrounding GnRH neurons. Identifying astrocytes by using the structural protein GFAP accounts for only a percentage of the total astrocyte cell body and processes. However, small changes in this structural protein may lead to correlative changes in the astrocyte processes. On d 1, sections from one series that contains every sixth section were rinsed in TBS and blocked with 10% NHS-X for 1 h at room temperature. Next, sections were incubated in mouse anti-GFAP (1:50,000) in 2% NHS-X overnight at 4 C. On d 2, sections were rinsed in TBS, incubated in biotinylated antimouse IgG diluted 1:500 in 2% NHS-X for 1 h at room temperature, followed by incubation in avidin-biotin complex (Vectastain kit, Vector Laboratories, Burlingame, CA) in TBS plus 0.4% Triton X-100 for 1 h at room temperature. Finally, sections were incubated in 0.025% diaminobenzidine (DAB; Sigma) with 0.02% ammonium nickel sulfate (Fisher Scientific) and 0.1 µl/ml of 30% hydrogen peroxide in TBS for 10 min at room temperature. After the DAB reaction, sections were rinsed in TBS and then incubated in rabbit anti-GnRH (1:100,000) in 2% NHS-X overnight at 4 C. On d 3, sections were rinsed in TBS, incubated in biotinylated antirabbit IgG diluted 1:500 in 2% NHS-X for 1 h at room temperature, followed by incubation in avidin-biotin complex (Vectastain kit, Vector Laboratories) in TBS plus 0.4% Triton X-100 for 1 h at room temperature. Finally, sections were incubated in 0.025% DAB (Sigma) with 0.1 µl/ml of 30% hydrogen peroxide in TBS for 10 min at room temperature. Each step was followed by rinses in TBS (3 x 5 min). Sections were mounted on slides and coverslips were applied using Permount.
Measuring astrocyte surface area
Bright-field photomicrographs using a x40 objective were taken of astrocytes that surround GnRH neurons using a Leica DC 500 camera attached to a Leica DMLB microscope (JH Technologies, San Jose, CA). Photomicrographs were analyzed using Metamorph Image Analysis software 6.1 (Universal Imaging Corp., Downing, PA). Astrocyte surface area was obtained by using the tracing tool to outline the astrocyte and all processes, and Metamorph was calibrated to determine the area in the outlined region. Only astrocytes that were in close apposition to GnRH neurons were measured (two astrocytes each per five GnRH neurons in the OVLT and two astrocytes each per 10 GnRH neurons in the rMPN).
Statistical analysis
Two-way ANOVA followed by Bonferronis post hoc test were used to analyze surface area significance of astrocytes that surround GnRH in antisense and random sequence oligo-treated rats and middle-aged rats for effects of treatment, time, and treatment x time interactions. All statistics were performed using Prism 4.0 software (GraphPad, San Diego, CA).
| Results |
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Aging affects the surface area of astrocytes in the OVLT and rMPN
In the OVLT of middle-aged rats, the surface area of astrocytes that surround GnRH neurons no longer demonstrates a diurnal rhythm (Fig. 3A
). The astrocyte surface area did not decline at 1400 or 1800 h in these rats, and the area of astrocytes seen in middle-aged animals across the day resembled the surface area of astrocytes measured in animals treated with antisense oligos (Fig. 2A
). This lack of diurnal rhythms in the surface area of astrocytes that surround GnRH neurons is also seen in the rMPN of middle-aged rats, in that no decline in astrocyte surface area was seen at 1400 or 1800 h (Fig. 3B
). The surface area of astrocytes in the rMPN of middle-aged rats was similar to the surface area of astrocytes observed in the rMPN of antisense oligo-treated rats (Fig. 2B
).
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| Discussion |
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The SCN contains an extensive network of astrocytes (34), and neurons in this brain region exhibit more coverage by astrocytes than neurons in the anterior hypothalamic areas (35). In the SCN, astrocyte processes are found between neuronal cell bodies and adjacent to presynaptic and postsynaptic sites (36). Astrocyte processes ensheath VIP and vasopressin neurons, with a greater percent of VIP neurons ensheathed by astrocytes (36). Treatment with agents that prevent glial metabolism or block astrocyte gap junction formation in the SCN disrupts circadian rhythms in neuronal activity, suggesting that astrocytes play a crucial role in maintaining circadian rhythms (37). However, conflicting results have been reported on whether diurnal rhythms in astrocyte morphology exist (35, 36, 38).
Astrocytes have been shown to play a role in the regulation of GnRH neurons and secretion. Astrocytes in close apposition to GnRH neurons, which may influence GnRH neuronal activation and release, display region-specific characteristics that are regulated differentially by circulating estradiol levels (10, 15). Astrocytes in the arcuate nucleus along with tanycytes that send processes to the median eminence increase their ensheathment of GnRH terminals on the afternoon of proestrus when estradiol levels are elevated, which limits inhibitory inputs that suppress GnRH release into the median eminence (13, 14). In contrast, our laboratory has demonstrated that astrocytes in the rMPN and OVLT, which regulate synaptic input to the GnRH neuronal cell bodies, exhibit a different diurnal pattern. During the afternoon of proestrus, astrocytes decrease their GFAP immunoreactivity, and this may lead to a decrease in the degree of ensheathment of GnRH neurons, which may lead to an increase in stimulatory inputs that induce GnRH synthesis and release (16) and thereby may limit inputs that may influence GnRH neurons.
Astrocyte-neuron interactions are bidirectional. Araque et al. (39) proposed the tripartite synapse consisting of the presynaptic and postsynaptic neurons along with astrocyte processes that can either physically modify synaptic communication or chemically alter synapse firing due to the close proximity of astrocytes around synapses. In the current study, we observed VPAC2 receptor-IR in GFAP-IR cells in the OVLT and rMPN as well as VPAC2 receptor-IR colocalized with cells with neuronal-like morphology (data not shown) that were in close apposition to GFAP-IR astrocytes. Our demonstration of VPAC2 receptors on astrocytes and neuron-like cells in conjunction with previous observations of the presence of VPAC2 receptors on GnRH neurons (40) suggest that VIP may influence GnRH neurons in numerous ways by affecting GnRH neurons directly, other neuronal phenotypes that communicate with GnRH neurons, and astrocytes that are in close proximity to GnRH or other neurons. We explored the possibility that one mechanism by which VIP affects GnRH neuronal activity is by modulating the surface area of astrocytes that surround GnRH neurons, which thereby influences the density of synapses on GnRH neurons.
Our studies demonstrate that VIP decreases astrocyte surface area around GnRH neurons at the time of the LH surge and could therefore indirectly enhance stimulatory inputs to synapse on GnRH neurons. One of these stimulatory inputs is VIP (30, 40). Work from our laboratory (20) demonstrated a stimulatory role of VIP from the SCN in inducing GnRH neuronal activation. One possibility is that VIP may also be able to influence GnRH neurons to induce changes in astrocyte morphology. Another example is estrogen receptor-containing neurons located in the AVPV (41), which project to the OVLT near GnRH neurons (42). This pathway may explain how estrogens stimulatory effects on the LH surge are communicated to GnRH neurons. Furthermore, some estrogen receptor-containing neurons in the AVPV have recently been shown to also contain
-aminobutyric acid and glutamate vesicles, in which an increase in glutamate-containing vesicles and a decrease in
-aminobutyric acid -containing vesicles occur at the time of the LH surge (43) and therefore potentially stimulate GnRH neurons.
It is interesting to note that Cashion et al. (16) did not see a decrease in astrocyte surface area on the afternoon of estrus when estradiol concentrations are low, even though VIP concentrations in the SCN are elevated at this time (44). It is possible that an increase in estradiol and the diurnal increase in VIP are both necessary to induce plastic changes in the surface area of astrocytes that surround GnRH neurons. In our studies, rats were implanted with E2-containing capsules to elucidate whether a daily signal is necessary to induce changes in astrocyte morphology. Indeed, blockade of VIP in the SCN prevented the afternoon decline in the surface area of astrocytes that surround GnRH neurons in E2-primed rats.
Aging dampens SCN VIP rhythmicity, which in turn decreases the diurnal plasticity of astrocytes. Cashion et al. (16), in agreement with our data, demonstrate that middle-aged rats no longer exhibit diurnal changes in the surface area of astrocytes that surround GnRH neurons. When we blocked the VIP rhythm and suppressed its concentrations in the SCN using antisense oligo methodology, we inhibited the diurnal changes in the surface area of astrocytes that are closely apposed to GnRH neuronal cell bodies. The absence of the astrocytes morphometry rhythm in our VIP antisense-treated rats is strikingly similar to what we observe in middle-aged rats that experience attenuated GnRH neuronal activation (20). Therefore, we conclude that VIP is necessary to induce cyclic changes in astrocyte morphometry and that the age-related loss of VIP in the SCN leads to a loss in the diurnal rhythm in astrocyte surface area.
In summary, VIP from the SCN plays a crucial role in regulating GnRH neuronal activity by directly influencing GnRH neurons (20, 30, 31, 40) and indirectly modulating the surface area of astrocytes that surround GnRH neurons, which allows for stimulatory inputs to GnRH neurons to occur at the right time to induce an LH surge. Furthermore, maintenance of VIPs daily rhythm is of great importance to the synchronization of the SCN with GnRH neurons and astrocytes that surround GnRH neurons. Subtle changes in the ability of the biological clock to drive reproductive rhythms in middle-aged rats may underlie the transition to acyclicity and decline in reproductive function.
| Footnotes |
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Disclosure: L.M.G. and P.M.W. have nothing to declare.
First Published Online February 9, 2006
Abbreviations: DAB, Diaminobenzidine; E2, 17ß-estradiol; GFAP, glial fibrillary acidic protein; IR, immunoreactivity; NHS-X, normal horse serum plus Triton X-100; OVLT, organun vasculosum of the lamina terminalis; OVX, ovariectomized; rMPN, rostral region of the medial preoptic nucleus; SCN, suprachiasmatic nucleus; TBS, Tris-buffered saline; VIP, vasoactive intestinal polypeptide; VPAC2, VIP receptor subtype.
Received October 4, 2005.
Accepted for publication February 1, 2006.
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