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The Journal of Neuroscience, January 15, 2001, 21(2):477-484
Cytosolic Calcium Oscillations in Astrocytes May Regulate
Exocytotic Release of Glutamate
Lucia
Pasti1,
Micaela
Zonta1,
Tullio
Pozzan1,
Stefano
Vicini2, and
Giorgio
Carmignoto1
1 Department of Experimental Biomedical Sciences and
Consiglio Nazionale delle Ricerche Center for the Study of
Biomembranes, University of Padova, 35121 Padova, Italy, and
2 Department of Physiology and Biophysics, Georgetown
University, Washington, DC 20007
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ABSTRACT |
To obtain insights into the spatiotemporal characteristics and
mechanism of Ca2+-dependent glutamate release from
astrocytes, we developed a new experimental approach using human
embryonic kidney (HEK) 293 cells transfected with the
NMDA receptor (NMDAR), which act as glutamate biosensors, plated
on cultured astrocytes. We here show that oscillations of intracellular
Ca2+ concentration
([Ca2+]i) in astrocytes trigger
synchronous and repetitive [Ca2+]i
elevations in sensor HEK cells, and that these elevations are sensitive
to NMDAR inhibition. By whole-cell patch-clamp recordings, we
demonstrate that the activation of NMDARs in HEK cells results in
inward currents that often have extremely fast kinetics, comparable with those of glutamate-mediated NMDAR currents in postsynaptic neurons. We also show that the release of glutamate from stimulated astrocytes is drastically reduced by agents that are known to reduce
neuronal exocytosis, i.e., tetanus toxin and bafilomycin A1. We conclude that
[Ca2+]i oscillations represent a
frequency-encoded signaling system that controls a pulsatile release of
glutamate from astrocytes. The fast activation of NMDARs in the sensor
cells and the dependence of glutamate release on the functional
integrity of both synaptobrevin and vacuolar H+
ATPase suggest that astrocytes are endowed with an exocytotic mechanism
of glutamate release that resembles that of neurons.
Key words:
glia; calcium oscillations; transmitter release; exocytosis; SNARE protein; green fluorescent protein
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INTRODUCTION |
Astrocytes can synthesize and
release a large number of neuroactive compounds, including peptides,
eicosanoids, and neurotrophins (Martin, 1992 ). The recent observation
that astrocytes can also release neurotransmitters, such as the
excitatory amino acid glutamate (Parpura et al., 1994 ), has attracted
considerable interest for the possible involvement of glial cells in
the modulation of neuronal function (Smith, 1994 ; Pfrieger and Barres,
1996 ). Furthermore, over the past decade, a growing body of evidence
has emerged on the existence in the brain of a close bidirectional
communication between neurons and astrocytes that may affect neuronal
excitability and synaptic transmission. The existence of a signaling
pathway from neurons to astrocytes was demonstrated by the observation that glutamate released from synaptic terminals after episodes of
intense neuronal activity can activate metabotropic glutamate receptors
(mGluRs) in the astrocyte membrane and trigger repetitive elevations in
intracellular Ca2+
([Ca2+]i) (Dani et
al., 1992 ; Porter and McCarthy, 1996 ; Pasti et al., 1997 ).
Interestingly, an increase in the firing rate of neuronal afferents
results in an increased frequency of
[Ca2+]i
oscillations in astrocytes (Pasti et al., 1997 ), demonstrating that the
frequency of oscillations is under the dynamic control of neuronal
activity and raising the possibility that it represents the code for
the transfer of information from neurons to astrocytes. However,
astrocytes can also signal back to neurons. In fact, astrocyte
[Ca2+]i elevations
can induce the release of glutamate which causes [Ca2+]i elevations
in adjacent neurons both in culture (Parpura et al., 1994 ; Hassingher
et al., 1995 ) and in acute brain slices (Pasti et al., 1997 ). The
release of glutamate from astrocytes was recently shown to modulate
synaptic transmission in cultured hippocampal neurons (Araque et al.,
1998a ,b ) as well as in the intact retina (Newman and Zahs, 1998 ). A
physiologically relevant phenomenon, such as the activity-dependent
potentiation of inhibitory synaptic transmission in the hippocampus
between interneurons and pyramidal neurons, is critically dependent on
glutamate release from astrocytes (Kang et al., 1998 ). The
intracellular signaling transduction pathway mediating
Ca2+-dependent glutamate release from
astrocytes is still poorly defined. We recently found that activation
of the mGluR in astrocytes from acute brain slices can trigger the
release of glutamate from these cells (Pasti et al., 1997 ), whereas its
coactivation with the AMPA receptor in cultured astrocytes powerfully
enhanced the release through a signaling transduction system involving
prostaglandin formation (Bezzi et al., 1998 ).
Although it has been demonstrated that astrocytes are capable of
releasing glutamate, through the reverse operation of the glutamate
transporter (Szatkowski et al., 1990 ) or by a swelling-induced mechanism (Kimelberg et al., 1990 ), none of these mechanisms accounts for the Ca2+-dependent release of
glutamate triggered by stimuli such as bradykinin, agonists of
AMPA/mGluRs, and prostaglandins (Parpura et al., 1994 ; Bezzi et al.,
1998 ; Araque et al., 2000 ). To further explore the mechanism and
spatiotemporal features of glutamate release from astrocytes, we
devised a new experimental approach. HEK cells were cotransfected with
the NMDA receptor and green fluorescent protein (GFP). Whereas the
latter enables the positive identification of transfected cells, the
former renders these cells sensitive to glutamate. When plated onto
cultured astrocytes, the cotransfected cells act as biosensors for
glutamate release from the astrocytes. By combining different
experimental approaches, we demonstrate that
[Ca2+]i
oscillations mediated by activation of AMPA/mGluRs trigger in
astrocytes a pulsatile, most likely vesicle-mediated, release of glutamate.
Part of this work has been reported in abstract form (Carmignoto et
al., 1999 )
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MATERIALS AND METHODS |
Tissue preparations. Primary cultures of cortical
astrocytes were prepared from neonatal Wistar rats as previously
described (Pasti et al., 1995 ). For purification of the astrocyte
culture, 14 d after plating, cells were subjected to 12 hr of
continuous shaking and then incubated for 5 min with 0.2% trypsin.
Detached cells were then collected and replated on 24-mm-diameter
coverslips. Human embryonic kidney (HEK) 293 cells (American Type
Culture Collection, Manassas, VA) were cotransfected with cDNAs
encoding NMDAR subunits 1-2A (Vicini et al., 1998 ) and GFP (Prasher et al., 1992 ; Rizzuto et al., 1995 ), in the presence of 2 mM kynurenic acid and 500 µM ketamine (Vicini et al., 1998 ); these cells
will be henceforth referred to as NR-GFP cells. Cells were
trypsinized 12-16 hr after transfection and replated on 2-week-old
astrocyte secondary cultures. For confocal microscope experiments,
after 1-3 d, both types of cells were loaded with the
Ca2+ indicator indo-1. SDS-PAGE and
immunoblotting were performed according to standard procedures
(Laemmli, 1970 ; Rossetto et al., 1996 ). Proteins (50 µg/lane) were
loaded on SDS-PAGE and transferred to nitrocellulose. Purified TeNT and
antibodies against synaptobrevin (Rossetto et al., 1996 ) were kindly
provided by O. Rossetto (Department of Experimental Biomedical
Sciences, University of Padova, Padova, Italy). Antibodies against the
glial fibrillar acidic protein (GFAP) and bafilomycin A1 were from
Boehringer Mannheim (Indianapolis, IN) and Sigma (St. Louis, MO), respectively.
Confocal microscopy. Digital fluorescence microscopy (Nikon,
RCM8000) was used for monitoring the change in indo-1 emission after
cell loading with indo-1/AM (Molecular Probes, Eugene, OR) as
previously described (Pasti et al., 1997 ). After excitation at 351 nm
wavelength, the emitted light was separated into its two components
(405 and 485 nm), and the ratio (405/485) was displayed as a
pseudocolor scale. During experiments, cultured cells were continuously
perfused (1.5-3 ml/min) at room temperature with a
Mg2+-free extracellular solution
consisting of (in mM): 145 NaCl, 5 KCl, 2 CaCl2, 1 Na3PO4, 5.5 glucose, 0.01 glycine, and 10 HEPES, pH 7.4, with NaOH. Sampling rate was 2 sec, and
16 images were averaged for each frame. Occasionally, very bright
fluorescent NR-GFP cells were apparently less loaded with
Indo-1. Fluorescent resonant energy transfer between GFP and Indo-1,
and/or inner filtering effect may account for this observation; the
405/485 nm ratio obtained in basal and stimulating conditions was not significantly affected by this phenomenon, and stimulated ratio was,
however, not significantly changed. Calibration was performed intracellularly as described (Scheenen et al., 1998 ).
Patch-clamp recordings and analysis. Cells were viewed with
an upright Axioskop FS microscope (Zeiss, Oberkochen, Germany) equipped
with differential interference contrast Nomarski optics and an
electrically insulated water immersion 40× objective with a long
working distance (2 mm). Standard procedures for pipette preparation
and patch-clamp recordings in the whole-cell configuration were used
(Hamill et al., 1981 ). In brief, electrodes were pulled in two stages
on a vertical pipette puller from borosilicate glass capillaries
(Wiretrol II; Drummond, Broomall, PA). Typical pipette resistance was
5-8 M . The recording pipette contained (in
mM): 145 CsCl, 2 MgCl2, 10 EGTA, 3 Na2ATP, and 10 HEPES, pH 7.2, with CsOH.
Experiments were performed at room temperature, and cells were
continuously perfused (1.5-3 ml/min) with the same solution used in
the confocal microscope experiments (see above). To stimulate glutamate
release from astrocytes, 10 or 20 µM
L-quisqualate (at the concentration more
effective in eliciting oscillations in parallel experiments at the
confocal microscope) was added to the perfusate. Recordings were
performed in voltage clamp with an Axopatch-200B amplifier (Axon
Instruments, Foster City, CA), sampled at 10 or 20 kHz, filtered at
1-2 kHz, and digitized by the interface Digidata1200A and pClamp 8 software (Axon Instruments). Off-line data analysis, curve fitting, and
figure preparation were performed with Clampfit-8 (Axon Instruments)
and Origin 5 (Microcal Software, Northampton, MA) software. Rise times
represent the time elapsed from 20 to 80% of the peak amplitude of the
response. Fitting of decay times of currents recorded from
NR-GFP cells was performed using a simplex algorithm
based on a least squares exponential fitting routine. Double
exponential equations of the form I(t) = If × exp( t/ f) + Is × exp( t/ s), where
If and
Is are the amplitudes of the fast and
slow decay components, and f and
s are their respective decay time constants
used to fit the data. A comparison of the summed square deviation was
used to estimate the quality of single versus double exponential fits. To compare decay time between different currents, we used a weighted mean decay time constant w = [If/(If + Is)] × tf + [Is/(If + Is)] × ts. Data values are expressed as
mean ± SEM. To investigate the possible presence of gap junction
communication between astrocytes and transfected HEK cells, Lucifer
yellow (4 mg/ml) was included in the patch pipette in some experiments.
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RESULTS |
Calcium oscillations trigger a pulsatile release of glutamate
Our experimental approach allowed us to monitor simultaneously
both the agonist-mediated
[Ca2+]i
oscillations in astrocytes and the release of glutamate. The latter
could be detected as a
[Ca2+]i increase
in NR-GFP cells caused by Ca2+
influx through glutamate-activated NMDARs. Activation of metabotropic glutamate receptors (mGluRs) and AMPA receptors with either
L-quisqualate or the selective agonists
1-aminocyclopentane-1,3-dicarboxylic acid (t-ACPD) and AMPA
was used to trigger
[Ca2+]i
oscillations in astrocytes. Stimulation of wild-type HEK cells (plated
alone) with NMDA (200 µM; n = 67), AMPA (50 µM; n = 60), t-ACPD (100 µM; n = 55), or L-quisqualate (30 µM; n = 36) failed to evoke any
[Ca2+]i increase.
On the contrary, NR-GFP cells plated alone displayed large
[Ca2+]i increases
after NMDA but not L-quisqualate or
t-ACPD/AMPA.
Figure 1 shows a typical example of the
results obtained by stimulating
[Ca2+]i
oscillations in astrocytes. NR-GFP cells plated onto
astrocytes could be easily recognized by both their GFP fluorescence
(Fig. 1Aa) and their response to NMDA (Fig.
1Ab). Stimulation with 3 µM
L-quisqualate induced in one of the astrocytes
two successive [Ca2+]i elevations
(Fig. 1Ac,d). The
[Ca2+]i change
initiated at the level of the process (spot 1) and then spread to the
soma (spot 2; Fig. 1Ac). In the NR-GFP
cells close to the stimulated astrocyte,
[Ca2+]i elevations
synchronous with those occurring in the astrocyte were observed. The
response in NR-GFP cells was attributable to activation of
the NMDAR because it was abolished by the NMDAR antagonist
D-2-amino-5-phosphonopentanoic acid
(D-AP-5; Fig. 1B). The
[Ca2+]i rise in
NR-GFP cells (spots 3 and 4) initiated concurrently with the
[Ca2+]i peak in
the process and before that in the soma (Fig. 1Ac,Ad,B, inset), suggesting that the site of glutamate release is localized at the level of the process. We analyzed a total of 52 NR-GFP cells that displayed
[Ca2+]i elevations
after either t-ACPD/AMPA or
L-quisqualate-induced [Ca2+]i
oscillations in astrocytes: 87.2% (82 of 94) of
D-AP-5-sensitive [Ca2+]i transients
occurred in temporal correlation with a
[Ca2+]i transient
in nearby astrocytes. After the wash-out of
D-AP-5, in all cells tested (n = 3), we observed a full recovery of the response to
L-quisqualate. The
[Ca2+]i rise in
NR-GFP cells could not be attributed to gap junction communication between astrocytes and NR-GFP cells because
Lucifer yellow included in a patch pipette never diffused from patched NR-GFP cells (n = 10) to surrounding
astrocytes or from patched astrocytes (n = 3) to
NR-GFP cells. Taken together, the above results directly
demonstrate that
[Ca2+]i
oscillations in astrocytes, mediated by AMPA and mGlu receptors, lead
to a pulsatile release of glutamate that triggers NMDAR-mediated [Ca2+]i elevations
in NR-GFP cells.

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Figure 1.
[Ca2+]i
oscillations trigger synchronous
[Ca2+]i elevations in sensor cells.
A, Four NR-GFP cells, identified by their
GFP fluorescence at 488 nm excitation wavelength
(a), but not astrocytes, display
[Ca2+]i elevations after 100 µM NMDA stimulation (b).
c, d, Sequence of pseudocolor images
showing the [Ca2+]i changes after
stimulation with 3 µM quisqualate in one astrocyte (spot
2), its process (spot 1), and in two of
the NR-GFP cells (spots 3 and
4). Sampling rate, 2 sec. Scale bar, 10 µm. The
ratio (405/485) is displayed as a pseudocolor scale. B,
Kinetics of the 405/485 changes from the same cells.
Arrows (b) and bars
(c, d) underline the pattern of
[Ca2+]i changes corresponding to
images in Ab, Ac, and Ad.
To better distinguish the response from each cell, in this as well as
in the other figures, traces are shifted on the y-axis.
The onset of the [Ca2+]i change in
NR-GFP cells clearly occurred after the
[Ca2+]i elevation in the process and
before that in the soma (see the three-dimensional inset
reporting the responses at expanded time scale). Basal 405/485 values
in astrocytes and NR-GFP cells were similar and ranged
from 0.61 to 0.95. After the wash-out of D-AP-5, in all
cells tested (n = 3), we observed a full recovery
of the response to L-quisqualate (0.40 ± 0.14 and
0.42 ± 0.12, after the first and third challenge, respectively;
mean 405/485 change ± SEM; relative change of response amplitude
in the third with respect to the first challenge, +6%;
n = 3). Two successive stimulations also elicited
comparable responses (0.49 ± 0.12 and 0.60 ± 0.15; +22%;
n = 4).
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The dependence of the response of NR-GFP cells on the
pattern of astrocyte
[Ca2+]i
oscillations was next investigated. Challenge with agonists of
AMPA/mGlu receptors at high concentration, which induces a single
[Ca2+]i peak
followed by a sustained plateau in astrocytes, triggers only a single
[Ca2+]i transient
in the neighboring NR-GFP cells (Fig.
2A). A repetitive response in NR-GFP cells was never observed under these
conditions. Furthermore, high- but not low-amplitude
[Ca2+]i peaks in
the astrocyte result in effective stimulation of
[Ca2+]i changes in
the adjacent NR-GFP cell (Fig. 2B). In
Figure 2C the amplitudes of the
[Ca2+]i peaks in
stimulated astrocytes are grouped according to the presence (success)
or absence (failure) of response in nearby NR-GFP cells.
[Ca2+]i peaks,
measured at the soma, with amplitude of >550 nM
always triggered a
[Ca2+]i increase
in NR-GFP cells; below this value, successes were sometimes
observed. Furthermore, we confirmed that prostaglandin formation
represents a crucial step in the signaling transduction system
regulating in astrocytes the
Ca2+-dependent release of glutamate (Bezzi
et al., 1998 ). NR-GFP cells (n = 8), which
displayed [Ca2+]i
increases on a first AMPA/mGluRs stimulation, failed to respond to a
second challenge after preincubation with 5 µM
indomethacin, an inhibitor of the prostaglandin-forming enzyme
cyclo-oxygenase. Finally, after depletion of
Ca2+ from astrocyte intracellular stores
by preincubation with 10 µM cyclopiazonic acid,
activation of AMPA/mGluRs failed to trigger [Ca2+]i changes in
astrocytes, and no response was observed in NR-GFP cells
(n = 11).

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Figure 2.
The glutamate-mediated response in
NR-GFP cells depends on the pattern and amplitude of
[Ca2+]i oscillations.
A, A sustained [Ca2+]i
increase in the astrocyte (black area) evokes only a
single [Ca2+]i transient in the
adjacent NR-GFP cell (gray area).
B, Astrocyte [Ca2+]i
peaks of large amplitudes resulted in synchronous
[Ca2+]i elevations in the
NR-GFP cell. C, Values of the astrocyte
[Ca2+]i peaks (n = 48) that failed (failure) or succeeded (success) to trigger a
correlated [Ca2+]i elevations in the
NR-GFP cells. Only astrocytes displaying an oscillatory
pattern comprised of both low- and large-amplitude
[Ca2+]i peaks were considered
(n = 13). The mean values of the
[Ca2+]i change from the two groups are
significantly different (280 ± 30 vs 764 ± 100 nM; p < 0.005, one-way ANOVA).
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In 35% of NR-GFP cells responsive to
L-quisqualate stimulation of astrocytes,
D-AP-5 was unable to block the
[Ca2+]i increase,
suggesting that astrocytes can release, besides glutamate, other agents
that can trigger
[Ca2+]i elevations
in HEK cells. Similarly, a number of nontransfected (GFP-negative) HEK
cells (46 of 119; 38.6%) also displayed
[Ca2+]i elevations
after astrocyte stimulation. The
D-AP-5-insensitive responses in HEK cells were
caused by the release from stimulated astrocytes of prostaglandins,
most likely PGE2 (data not shown).
On the mechanism of glutamate release from astrocytes
The mechanism of glutamate release from activated astrocytes was
next investigated. To this end we used the patch-clamp recording technique that ensures a higher temporal resolution of
glutamate-mediated activation of NMDARs in NR-GFP cells. The
rationale is as follows. If glutamate release occurs via an exocytotic
mechanism, the resulting sudden increase of glutamate concentration in
the proximity of the recorded NR-GFP cell should trigger a
rapid activation of the NMDAR. Conversely, other release mechanisms
(e.g., a carrier-mediated process), should generate much slower
kinetics. Figure 3A shows an NR-GFP cell
plated on astrocytes and identified by its GFP fluorescence. After a
challenge with L-quisqualate, this cell displayed
pulsatile, inward current events that resemble NMDA EPSCs (Fig.
3B). Many currents had rise
times as fast as a few milliseconds and decay time constants comparable
with those of NMDA EPSCs (Collingridge et al., 1988 ; Lester et al.,
1990 ; Carmignoto and Vicini, 1992 ) (Fig. 3C, events 1 and 2, D). Some events characterized by a peak followed by a
sustained current (Fig. 3C, event 2), i.e., similar to those
obtained by prolonged applications of NMDA in neurons (Lester and Jahr,
1992 ; Vicini et al., 1998 ), were occasionally observed. Currents with
slower kinetics were also recorded (Fig. 3C, event 3).
Currents with fast kinetics were observed in 13 NR-GFP cells
from a total of 52 recorded cells and were regularly blocked by 10 µM D-AP-5. In Figure
3D the rise time values of the currents recorded from
NR-GFP cells are expressed as a function of the current
decay time constant w. The significant degree
of correlation between these two values is noteworthy. Thirty-two cells
of our sample displayed on astrocyte stimulation either very slow
current events or repetitive episodes of noise increase resembling
bursts of NMDAR channel openings. These types of response were also
regularly blocked by D-AP-5 (10 µM). No responses were observed in the
remaining seven cells. In the absence of astrocytes, no inward currents
were recorded from NR-GFP cells (n = 15)
after stimulation with 20 µM
L-quisqualate.

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Figure 3.
Stimulation of astrocytes results in
glutamate-mediated, fast activation of NMDARs in the sensor cell.
A, NR-GFP cell plated on cultured
astrocytes. Scale bar, 10 µm. B, The
NR-GFP cell shown in A responded with
repetitive, inward currents after stimulation of astrocytes with 10 µM quisqualate. Holding potential, 55 mV. Calibration:
20 pA, 10 sec. C, Events 1,
2, and 3 are reported at expanded scales.
Calibration: 5 pA, 500 msec. Rise time value of the current and decay
time constant w of the curve best describing the decay
are reported. The fitting curve (white line) is
superimposed to the currents. D, Scatter plot of rise
time values of the currents recorded from 13 NR-GFP
cells expressed as a function of the current decay time constant
w (mean ± SEM; rise time, 20.2 ± 3.75 msec;
range, 1.5-167 msec; w 563 ± 74.9 msec; range,
37-2896 msec; amplitude, 20.2 ± 6.7 pA; range, 3.2-272 pA;
n = 65). Very slow currents (rise and decay times
>200 msec and 3 sec, respectively) such as event 3,
were not included in our sample. The line is the linear fit to the data
(r = 0.61; p < 0.0001).
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To provide further insights into the mechanism of glutamate release,
astrocytes were incubated for 24 hr with 100 nM tetanus neurotoxin (TeNT), a specific neurotoxin that blocks the
exocytotic release of neurotransmitters. In neurons, the effects of
TeNT depends on receptor-mediated endocytosis of the toxin followed by
release of the active subunit into the cytoplasm and proteolytic cleavage of the vesicle protein synaptobrevin (Schiavo et al., 1992 ).
No inward current events were recorded from NR-GFP cells (n = 19) plated on TeNT-treated astrocytes and
stimulated with L-quisqualate (Fig.
4A). Only in three
cells were a few episodes of noise increase observed. The dramatic
reduction of the response in NR-GFP cells after stimulation
was accompanied by the cleavage of synaptobrevin, as demonstrated by
the reduction in specific immunoreactivity in TeNT-treated astrocytes
as compared with controls (Fig. 4B). The amplitude
and pattern of L-quisqualate-induced [Ca2+]i
oscillations were not affected by TeNT treatment (Fig.
5A-C). It should be noted
that prolonged incubations with the toxins are necessary to inhibit
glutamate release from astrocytes, whereas inhibition of presynaptic
release of neurotransmitters is complete in ~30 min (Pasti et al.,
1997 ; Bezzi et al., 1998 ).

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Figure 4.
TeNT and bafilomycin (BA1) reduce the
response of NR-GFP cells. A, Histograms
reporting the number and relative percentage of NR-GFP
cells responsive to astrocyte stimulation under different experimental
conditions (see Results for details). B,
Synaptobrevin immunoreactivity was reduced in Western blots of
TeNT-treated astrocytes as compared with untreated astrocytes
( 47.5 ± 6.3%; n = 2; Gel Doc 2000 multianalyst densitometric assay; Bio-Rad, Hercules, CA). A protein
stain of the nitrocellulose revealed no differences in amount and
pattern of proteins loaded. GFAP immunoreactivity was unaffected by
TeNT.
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Figure 5.
TeNT and bafilomycin do not affect
[Ca2+]i elevations triggered in
astrocytes by stimulation with L-quisqualate.
A, B, Sequence of pseudocolor images
illustrating the [Ca2+]i increase
triggered in indo-1-loaded astrocytes by a challenge with 20 µM L-quisqualate in control astrocytes
(A) and in astrocytes incubated for 24 hr in TeNT
(B). C, D, Kinetics of the
[Ca2+]i elevations in three
representative astrocytes before and after incubation with either TeNT
(C) or bafilomycin (D). The
amplitude of [Ca2+]i elevations in
response to L-quisqualate stimulation in the different
experimental conditions was unchanged (0.59 ± 0.01, n = 21 and 0.61 ± 0.03, n = 26, in control astrocytes and after TeNT, respectively; 0.46 ± 0.02, n = 74 and 0.45 ± 0.02, n = 61, before and after bafilomycin,
respectively). Bars indicate the duration of L-quisqualate
stimulation. The ratio (405/485) is displayed as a pseudocolor
scale.
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We next investigated the effects of bafilomycin, a specific inhibitor
of the vacuolar H+ ATPase (v-ATPase)
(Bowman et al., 1988 ; Stevens and Forgac, 1997 ), which blocks glutamate
release in stimulated neurons (Araque et al., 2000 ; Zhou et al., 2000 ).
By inhibiting H+ pumping, this drug causes
the collapse of the H+ gradient across the
membrane that is necessary for the uptake of glutamate into the
synaptic vesicle lumen (Maycox et al., 1990 ). In a first series of
experiments, astrocytes and NR-GFP cells were incubated in
4.5 µM bafilomycin for 1 hr. After quisqualate stimulation, 2 of 11 NR-GFP cells displayed a single episode
of fast kinetic glutamate-mediated currents, and two other cells displayed episodes of bursts of NMDAR channel openings, whereas no
activity was observed in the remaining seven NR-GFP cells
(Fig. 4A). In the second group of experiments, a
challenge with L-quisqualate (to trigger
glutamate release) was applied during the period of bafilomycin
incubation. After a second application of
L-quisqualate, neither inward current events nor
noise increases were observed from NR-GFP recorded cells
(Fig. 4A). The inhibitory effects of bafilomycin were
not accompanied by any alteration in the pattern or amplitude of
quisqualate-mediated
[Ca2+]i elevations
in astrocytes which, under control conditions, trigger repetitive
episodes of glutamate release (Fig. 5D). The activation of
NMDARs was not unspecifically affected by bafilomycin because NR-GFP cells (n = 8) displayed regular
[Ca2+]i elevations
after bath application of 200 µM NMDA.
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DISCUSSION |
Oscillations of the
[Ca2+]i represent
a widespread mode of signaling in eukaryotic cells (Berridge, 1993 ). In
astrocytes, the main glial population of the CNS,
[Ca2+]i,
oscillations induced by the neurotransmitter glutamate released from
activated synapses have been proposed to represent the key aspect of
the communication with neurons (Cornell-Bell et al., 1990 ; Smith, 1994 ;
Pasti et al., 1997 ). The output of astrocytes in response to this
neuronal signaling remains, however, largely undetermined.
The key finding of the present study is that, in cultured astrocytes,
activation of AMPA/mGluRs triggers a pulsatile release of glutamate
that depends on the frequency of
[Ca2+]i
oscillations. Indeed, the great majority of NMDA receptor-mediated [Ca2+]i elevations
in NR-GFP cells (glutamate release biosensors) occurred in
temporal correlation with
[Ca2+]i increases
in neighboring astrocytes. Given that
[Ca2+]i
oscillations of astrocytes from acute brain slices are under the
control of neuronal activity (Pasti et al., 1997 ), it is expected that
a pulsatile release of glutamate by astrocytes will follow episodes of
high neuronal activity.
Although the frequency of the
[Ca2+]i
oscillations controls the frequency of the release, the amplitude of
the [Ca2+]i
increases controls its efficacy. In particular, below an average level
of [Ca2+]i (550 nM), the probability of triggering an episode of glutamate release is significantly decreased. It should be stressed that this
threshold not only refers to the value recorded in the cell soma
(although the release may occur from the processes) but also reflects
the average cytosolic values. It is not unlikely that [Ca2+]i increases
higher than those measured here may be reached in restricted regions,
close to the release sites. Support for this possibility derives from
the recent observation that Ca2+ release
from the endoplasmic reticulum can result in highly localized [Ca2+]i increase
of concentrations >15 µM (Csordas et al., 1999 ).
The second major conclusion of our work is that the release of
glutamate in astrocytes occurs via a mechanism that shares common
properties with the exocytosis of glutamate-containing vesicles in
neurons. We found that the NMDAR-mediated inward currents elicited by
activated astrocytes in NR-GFP cells have kinetic characteristics comparable with those of NMDA currents activated by
glutamate released from synaptic terminals. These currents have rise
times as fast as 1.5 msec, indicating that the activation of the NMDAR
in NR-GFP cells is triggered by an abrupt increase in the
extracellular concentration of glutamate. The only process known to
cause such a rapid increase in concentration of a neurotransmitter is
the fusion of vesicles with the plasma membrane.
Currents with slower kinetics (as compared with the kinetics of NMDAR
EPSCs) were also recorded. A likely explanation for the variability in
current kinetics relies on the geometry of the contacts between
stimulated astrocytes and NR-GFP cells. Indeed, the
significant degree of correlation observed between rise and decay time
values suggests that the distance between the site of glutamate release
and the recorded cell determines the time course of the response. The
presence of currents with both fast and slow kinetics in the same cell
further suggests that glutamate is released either from multiple sites
of the same astrocyte and/or from many stimulated astrocytes located at
different distances from the recorded NR-GFP cell. The
absence of a membrane apposition with a site of release may also
account for both the very slow current events and the noise increase
resembling bursts of NMDAR channel openings. Currents with slow rise
and decay times may, therefore, reflect the kinetics of glutamate
diffusion, i.e., slow rising and decaying of glutamate concentration at
a given site.
Further evidence in favor of a glutamate release process dependent on
vesicle exocytosis derives from the results obtained with TeNT and
bafilomycin. These two compounds are known to inhibit neuronal
exocytosis by two independent mechanisms: the former through its
capacity of selectively proteolysing the v-SNARE protein synaptobrevin (Schiavo et al., 1992 ; Söllner et al., 1993 ; Dolly et al., 1994 ), the latter by inhibiting the v-ATPase that provides the
driving force for neurotransmitter accumulation in the secretory vesicles (Bowman et al., 1988 ; Maycox et al., 1990 ; Stevens and Forgac,
1997 ; Araque et al., 2000 ; Zhou et al., 2000 ).
As far as TeNT is concerned, its effect is highly specific on the
release of glutamate because it did not affect the astrocyte Ca2+ response to AMPA/mGluRs stimulation,
while suppressing the
[Ca2+]i elevations
in the NR-GFP cells. Two aspects of the inhibition by TeNT
are worth stressing: (1) unlike in neurons, the inhibition requires
several hours of incubation with the toxin, presumably because of lack
of specific membrane receptors for TeNT in astrocytes (Bezzi et al.,
1998 ; Verderio et al., 1999 ); (2) the inhibition of glutamate release
was accompanied by cleavage of synaptobrevin. Synaptobrevin is known to
be expressed in astrocytes (Parpura et al., 1995 ; Maienschein et al.,
1999 ), together with other components of the neuronal secretory
apparatus, i.e., syntaxin, cellubrevin (Parpura et al., 1995 ),
SNAP-23 (Hepp et al., 1999 ), and rab3 (Madison et al., 1996 ;
Maienschein et al., 1999 ).
In the case of bafilomycin, the inhibition of glutamate release
is stronger if during the period of preincubation the cells are
challenged with agonists. The simplest explanation of this finding is
that the drug does not prevent the release of glutamate-containing vesicles but inhibits their refilling with the transmitter. Similarly to TeNT, bafilomycin affected neither the pattern nor the amplitude of
quisqualate-mediated
[Ca2+]i elevations
in astrocytes. Consistent with our observations, it was recently shown
that bafilomycin reduces the slow inward current elicited in neurons by
glutamate released from mechanically stimulated astrocytes (Araque et
al., 2000 ). Taken together, the above results indicate that stimulated
astrocytes can release glutamate by an exocytotic mechanism similar in
its pharmacological sensitivity and, at least in part, in its kinetic
characteristics to that of stimulated neurons. A number of important
questions remain to be clarified. First of all, given that astrocytes
in culture may differ from astrocytes in the intact brain, our
observations do not necessarily indicate that astrocytes in
situ release glutamate through the same mechanism operative in
cultured astrocyte. However, the ability astrocytes from acute brain
slices to release glutamate after activation of their GluRs was
previously demonstrated (Pasti et al., 1997 ; Bezzi et al., 1998 ). In
addition, we need more information on the cellular and molecular
characteristics of the vesicular compartments containing glutamate. In
this respect, immunoelectron microscopic analysis revealed that
synaptobrevin and synaptophysin are associated with vesicular
structures in cultured astrocytes (Maienschein et al., 1999 ).
Furthermore, Calegari et al. (1999) not only have shown that a
subpopulation of hippocampal astrocytes in culture possess dense core
as well as less dense, smaller vesicles, but they also showed that
these cells can release the vesicle-associated protein secretogranin II
via a Ca2+-regulated process. Further
ultrastructural studies, if possible, combined with immunogold
techniques, are necessary to obtain direct evidence for the presence of
glutamate-containing vesicles in astrocytes in situ.
Despite these general similarities with the neuronal
glutamate-containing vesicles, it is also clear that the astrocyte
compartment containing the neurotransmitter may significantly differ
from the neuronal one, at least in the mechanism of glutamate
accumulation. In fact, because of the high glutamine synthetase
activity in astrocytes, it is predicted that the cytoplasmic glutamate
concentration should be much lower in astrocytes than in neurons. The
kinetic characteristics of the vesicular transporter for the
neurotransmitter might be accordingly quite distinct in the two cell types.
The physiological consequences of the exocytotic release of glutamate
from astrocytes on neuronal function remain to be investigated. If such
a release occurs through an exocytotic mechanism, it will have effects
on neurons far more complex than those suggested on the basis of the
available data.
In summary, our results demonstrate that the release of glutamate by
astrocytes results in a fast activation of the NMDAR in the sensor
cells. Moreover, this activation depends on the functional integrity of
synaptobrevin as well as of v-ATPase. These data are consistent with
the presence of a regulated, secretory pathway for glutamate-containing
vesicles under the control of [Ca2+]i
oscillations. Our findings add a new level of spatial and temporal complexity to the action of glutamate in the brain and hint at the
existence of a regulated, vesicle-mediated glutamatergic communication between astrocytes and neurons.
 |
FOOTNOTES |
Received Aug. 9, 2000; revised Oct. 18, 2000; accepted Oct. 20, 2000.
This work was supported by Grants 845 and 850 from the
Armenise-Harvard University Foundation, the Italian University and Health Ministries, the Italian Association for Cancer Research, Human
Frontier Science Program Grant RG520/95, and Telethon-Italy Grants 845 and 850 (T.P.) and 1095 (G.C.). We thank P. Magalhães and C. Angulo for helpful discussion and critical reading of this manuscript
and M. Nowycky and D. Janigro for critical reading of an early version
of this manuscript, C. Montecucco and O. Rossetto for the gift of
purified tetanus toxin and antibodies for synaptobrevin, and R. Pellizzari for collaborating in the immunoblotting experiments.
Correspondence should be addressed to Giorgio Carmignoto, Consiglio
Nazionale delle Ricerche Center for the Study of Biomembranes and
Department of Experimental Biomedical Sciences, University of Padova,
Via G. Colombo 3, 35121 Padova, Italy. E-mail:
gcarmi{at}civ.bio.unipd.it.
 |
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