X-ray diffraction is used to solve the low-resolution
structures of fully hydrated aqueous dispersions of seven different diacyl phosphatidylethanolamines (PEs) whose hydrocarbon chains have
the same effective chain length but whose structures vary widely. Both
the lower-temperature, liquid-crystalline lamellar (L
)
and the higher-temperature, inverted hexagonal (HII) phase
structures are solved, and the resultant internal dimensions (d-spacing, water layer thickness, average lipid length, and headgroup area at the lipid-water interface) of each phase are determined as a
function of temperature. The magnitude of the L
and HII phase d-spacings on either side of the
L
/HII phase transition temperature
(Th) depends significantly on the structure of
the PE hydrocarbon chains. The L
phase d-spacings range
from 51.2 to 56.4 Å, whereas those of the HII phase range
from 74.9 to 82.7 Å. These new results differ from our earlier
measurements of these PEs (Lewis et al., Biochemistry,
28:541-548, 1989), which found near constant d-spacings of 52.5 and
77.0-78.0 Å for the L
and HII phases,
respectively. In both phases, the d-spacings decrease with increasing
temperature independent of chain structure, but, in both phases, the
rate of decrease in the L
phase is smaller than that in
the HII phase. A detailed molecular description of the
L
/HII phase transition in these PEs is also presented.
 |
INTRODUCTION |
A complete understanding of the physical
properties of specific membrane lipids requires a determination of the
phase structures that are formed by these lipids under defined
conditions. Because the lipid phases of biological interest are fully
hydrated liquid-crystal mesophases, such a structural measurement
involves a determination of the electron density distribution of the
lipid/water system from a small number of powder-pattern-averaged
orders of x-ray diffraction. In this article, we describe such a
structure determination method that is then applied to aqueous
dispersions of various phosphatidylethanolamines (PEs). In an
accompanying article to be published elsewhere (D. A. Mannock,
R. N. A. H. Lewis, R. N. McElhaney, P. E. Harper, and S. M. Gruner, submitted for publication), these
results will be used in a comparative study of PEs and
diacyl-
-D-glucosyl-glycerols containing fatty acyl
chains of various lengths and structures.
To illuminate the physical principles at work in these systems, it is
important to study systems with a variety of chemical structures to
differentiate between general physical behavior and physical behavior
that varies with the lipid chemical structure. In this paper, we
determine the structural parameters of seven PEs with hydrocarbon
chains having different chemical structures, but the same effective
chain length (ECL).
The ECL of a hydrocarbon chain is defined by the total number of
carbons in the "main chain." For linear saturated and unsaturated fatty acyl groups, the ECL equals the total number of carbon atoms present, whereas for the branched fatty acyl chains, the ECLs equal the
total number of carbon atoms minus those present in the branch(es). For
-cyclohexyl fatty acyl groups, where three carbon atoms of the
terminal six-membered ring actually form part of the main chain, the
ECL is equal to the total number of carbon atoms present minus three.
Although the unit cell basis vector lengths (d-spacings) of both the
lamellar liquid-crystalline (L
) and inverted hexagonal phases (HII) are readily measured, additional information
about the specific chemical structures of these lipids may be used to compute the electron density reconstructions to determine such quantities as average lipid length (
l
) and water layer
thickness (w and r). We first detail the theory
and practice of this method of performing the reconstructions and then
apply the method to various PEs. The results presented here also serve
to correct earlier measurements (Lewis et al., 1989
), in which some of
the structural dimensions versus temperature were incorrect by as much
as 10% due to a faulty temperature calibration arising from a voltage
bias in the temperature controller.
 |
MATERIALS |
The seven PEs used in this study were
1,2-di-O-[cis-9,10-octadecenoyl("oleoyl")]-3-O-phosphatidylethanolamine-sn-glycerol (18:1c
9-PE),
1,2-di-O-[trans-9,10-octadecenoyl("elaidoyl")]-3-O-phosphatidylethanolamine-sn-glycerol (18:1t
9-PE),
1,2-di-O-[16'-ethyl-octadecanoyl]-3-O-phosphatidylethanolamine-sn-glycerol (20:0eai-PE),
1,2-di-O-[17',17'-dimethyl-octadecanoyl]-3-O-phosphatidylethanolamine-sn-glycerol (20:0dmi-PE),
1,2-di-O-[16'-methyl-octadecanoyl]-3-O-phosphatidylethanolamine-sn-glycerol (19:0ai-PE),
1,2-di-O-[15-cyclohexyl-pentadecanoyl]-3-O-phosphatidylethanolamine-sn-glycerol (21:0ch-PE), and
1,2-di-O-[17'-methyl-octadecanoyl]-3-O-phosphatidylethanolamine-sn-glycerol (19:0i-PE). The numbers in the above abbreviated chemical
nomenclature indicate the total number of carbon atoms in the
hydrocarbon chain and the number, configuration, and position of any
double bonds in the chain, whereas the subscripts indicate the type and
position of the branches in the hydrocarbon chain (Lewis et al., 1989
). The 18:1c
9-PE and 18:1t
9-PE were purchased
from Avanti Polar Lipids (Alabaster, AL) and used as received. The
remaining lipids were synthesized as described earlier (Lewis et al.,
1989
).
 |
METHODS |
Lipid molecular volumes
To determine the structural parameters of the various PEs
studied, estimations of their molecular volumes are required. The volumes of 18:1c
9-PE and 18:1t
9-PE as a
function of temperature and pressure have been measured by a
combination of the method of neutral buoyancy in
H2O/D2O mixtures (Nagle and Wilkinson, 1978
)
and high-pressure dilatometry (So et al., 1992
). These methods require
>100 mg of lipid, which is much more than the available supply of the
other 18 carbon ECL PEs. Alternatively, the molecular volumes of the
lipids can be estimated to the required accuracy by using the volumes
of similar constituent hydrocarbons (see Table
1), along with the measured value for
18:1c
9-PE and the assumption that the headgroup volumes
of all the PEs are identical. For the temperature dependence, it is
known that lipids like 18:1c
9-PE and
18:1t
9-PE in their L
phases have a
coefficient of expansion of
V/V = 7 × 10
4/°C and that the
L
/HII phase transition involves a
V/V of approximately 0.33% (So, 1992
). Therefore, if the
volume of a lipid is known at one temperature, the linear approximation
given above can be used to determine the volume at any other
temperature in the L
portion of the phase diagram to an
accuracy of better than 1% (So, 1992
; So et al., 1993
).
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TABLE 1
Measured volumes of the hydrocarbons used to calculate the
volumes of the diacyl phosphatidylethanolamines in
Table 2
|
|
As a specific example and as a test of the accuracy of such an
estimation, consider the two PCs for which the specific volumes are
known, 15:0i-PC (1.01 ml/g at 45°C; Yang et al., 1986
)
and 16:0-PC (1.004 ml/g at 45°C; Melchior et al., 1980
). The
molecular weights of 15:0i-PC and 16:0-PC are 762.11 and
734.05, respectively, yielding volumes of 1278 and 1224 Å3, respectively. We can estimate the specific volume of
15:0i-PC, v15i-PC, by considering it
to be the volume
which is in good agreement with the measured value of 1278 Å3. A similar calculation for 18:1t
9-PE,
starting from the measured value of 18:1c
9-PE, yields a
value that is within 2% of the measured value for
18:1t
9-PE. Volumes for the other lipids are evaluated similarly and are presented in Table 2.
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TABLE 2
Estimated volumes for several 18-carbon atom ECL
hydrocarbon chain structural variants of diacyl
phosphatidylethanolamine
|
|
General electron density reconstruction theory
Our concern is with the L
and the HII
phases, both of which are centrosymmetric. If one has a centrosymmetric
unit cell (i.e.,
e(r) =
e(
r), where
is the electron density and
r is the vector to the position in the unit cell), the
electron density can be written as a Fourier series of cosines. With
Aq being the Fourier coefficients and
q the Fourier vector, the electron density,
e, as function of position r can be written,
|
(1)
|
where
avg is the average electron density. For a
powder sample of crystals, one will see a pattern of concentric rings
of diffraction, each ring corresponding to a Fourier component
q of the electron density. The integrated intensity
Iq of a ring is related to its Fourier
coefficient Aq by
|
(1a)
|
where m is the multiplicity factor for the
coefficient and the sin
factor is the Lorentz correction (see
Warren, 1969
). The multiplicity is the number of orientations of a
crystal relative to the incoming x-rays that will yield a given
reflection. The approximation sin
is made because all
data are in the small angle region,
< 0.1.
In the small angle regime, the Lorentz correction (up to an overall
scaling factor) is made by dividing the integrated intensities of the
diffraction orders by the magnitude of the reciprocal lattice vector.
For instance, the intensity of the second-order peak in the
L
phase is divided by 2. In the HII phase,
the reciprocal lattice vectors also form a hexagonal lattice, and so,
from geometry, the magnitude of the vector (h, k) is
(h2 + hk + k2).
Therefore, the (1, 1) peak in the HII phase is divided by
. (For more information on the Lorentz correction, see
Warren (1969)
and Turner (1990)
). The peak intensity is divided by the
multiplicity of the reflection. For example, in the HII
phase, the (1, 0) peak has the same magnitude and reciprocal vector
length as the (0, 1), (1,
1), (
1, 1), (
1, 0), and (0,
1)
peaks, and so has a multiplicity of 6. Therefore, the peak intensity of
(1, 0) peak is divided by 6. For the L
phase, all the
peaks have a multiplicity of 1. For the HII phase, the
peaks (2, 1), (3, 1), (3, 2), and (4, 1) each have a multiplicity
of 12 and the remaining peaks have a multiplicity of 6 (Turner, 1990
).
This is almost enough information to reconstruct the electron density
of the liquid crystals from x-ray diffraction. What is missing are the
signs of the Aq, e.g., the relative phases of
the diffracted orders. Several methods have been developed to deal with
this difficulty. One method is to construct a model of the electron
density consistent with a known lipid chemical structure and then to
pick the phasing that comes closest to reproducing the model, subject
to the constraint that the rejected choices are clearly unphysical.
Conversely, one can Fourier transform the model and then use the
resulting phases in the reconstruction. Extensive work in modeling
lamellar structures has been done by Wiener et al. (1992)
and the
HII structure has been modeled by Turner and Gruner (1992)
.
Another means to determine the phases is the swelling method, in which
structures at slightly different hydrations are compared. Because the
electron density should only be shifted slightly by a small change in
hydration, it is a reasonable assumption that the integrated difference
of the square of the electron densities should be at a minimum for the
proper phasing. This method was used by Stamatoff and Krimm (1976)
for
lamellar systems and was extended to HII systems by Turner
(1990)
and Turner and Gruner (1992)
. Yet another method is the



technique of Luzzati and co-workers, where
e is the electron density. They stated that, if one
compares two structures of identical chemical composition, the value of



should be the same for both. If one
structure has a known phasing, this can be used to determine the
phasing for the other structure. A recent example of this method is
contained in Mariani et al. (1990)
. A new phasing technique, the methyl
trough search, has recently been described by our groups (Harper and
Gruner, 2000
; Harper et al., 2000
).
Lamellar phase reconstruction
A first step in determining a proper phasing for the
L
system is to construct a simple model of what a
correct phasing should yield, based on an estimate of the molecular
volume for each of the seven PEs studied here. These volumes were
estimated by assuming that all of the PE polar headgroups have a single invariant volume and that the acyl chain volume may be estimated from
known molecular volumes of the "constituent" hydrocarbons, as
described above. The hydrocarbons that were used are listed in Table 1
and the estimated lipid molecular volumes are given in Table 2.
18:1c
9-PE may be used as an example of the treatment of
each of the seven lipids: The volume of 18:1c
9-PE is 1190 Å at 25°C (Tate and Gruner, 1989
). The methyls on the two
hydrocarbon chains occupy a total of 2 × 56 Å3 = 112 Å3, or about 10% of the lipid volume. There are a
total of 18 electrons in the methyl groups, yielding an electron
density of 0.16 e/Å3. The volume of the methylene portion
of chains minus the terminal methyls can be estimated by comparison to
the known molecular volumes of the constituent hydrocarbons measured at
25°C shown in Table 1,
|
(2)
|
From Eq. 2, it is seen that the hydrocarbon chains minus the
methyl groups occupy about 70% of the lipid volume and that the
remaining 20% is taken up by the headgroup. From the chemical composition of 18:1c
9-PE, it is a simple matter to
calculate the electron densities for these regions, which are 0.30 e/Å3 for the hydrocarbon chains and 0.54 e/Å3
for the polar headgroup. A diagram of this simple model is shown in
Fig. 1. The model illustrates the basic
features of a correct reconstruction, namely a methyl trough bounded by
the headgroup peaks, which give way to the water region, which is of
intermediate electron density. Note that this model is appropriate to
all of the lipids under study here except for 21:0ch-PE,
which has no terminal methyls. Because there is no methyl trough for
21:0ch-PE, the electron density in the tail region should
be fairly flat.
For the L
phase, the electron density is given by
|
(3)
|
where d is the repeat spacing of the crystal and
x is in a direction perpendicular to the membrane surface.
The
avg cannot be determined from the reflection data
alone, and may be set to zero for the reconstructions on an arbitrary
electron density scale.
Inverted hexagonal phase reconstruction
A method of Turner and Gruner (1992)
was used to reconstruct the
HII phase. This technique is based on earlier work by
Stamatoff and Krimm (1976)
, who applied it to the lamellar phase. These methods are based on the observation that, if one compares the electron
densities of two lamellar phases with slightly different water
contents, the correct phasing should yield the electron density that
changes the least in going from one hydration to another. This is known
as the swelling method of phasing.
Quantitatively, one can define the difference in electron densities as
|
(4)
|
where
is a measure of the deviation, A is the
area of the unit cell,
'e is the electron density
at one hydration,
e is the electron density at another
hydration,
is the small difference in the radii of the two water
cores, and B and C are constants to take into
account differences in absolute and relative scaling, and the integral
is performed over the unit cell (Turner and Gruner, 1992
). Minimizing
with respect to B and C yields the following formulas for those quantities:
|
(5)
|
|
(6)
|
For the HII phase, the electron density is given by
|
(7)
|
where
|
(8)
|
|
(9)
|
For h or k equal to 0 or h = k, the multiplicity for the Ahk is 6. For
the remaining cases, the multiplicity is 12.
X-ray diffraction
X-ray diffraction data were acquired as described in Lewis et
al. (1989)
but with the intensifier/lens/CCD detector described in Tate
et al. (1997)
. Briefly, x-rays were generated on a Rigaku RU-200
rotating anode x-ray generator using a copper anode. The beam was
Ni-filtered, point focused via two orthogonal Franks mirrors and the
data were recorded on a two-dimensional x-ray detector based on an
intensified CCD. Samples consisted of unoriented dispersions of fully
hydrated lipid and water, generally in an ~1:1 weight ratio,
contained in 1.5 mm glass x-ray capillaries. The x-ray stage was
thermostatically controlled to ~0.5°C and a stability of
~0.1°C. Equilibration of the samples was checked by varying the
equilibration time between temperature steps until the diffraction was
stable when the time was increased. Repeat spacings were calibrated
with silver stearate, which has a lamellar repeat of 48.68 Å (Vand et
al., 1949
).
 |
RESULTS |
Lamellar reconstructions
Diffraction is seen to fourth order for lipids in the
L
phase. The Lorentz-corrected amplitudes as a function
of temperature are listed for each lipid in Table
3. Note that the amplitudes have been
normalized to the first-order amplitude and that the multiplicity for
each of these peaks is the same.
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TABLE 3
Temperature (T, °C), measured amplitudes,
d, w, l , v, and
A for several hydrocarbon chain structural variants of
diacyl phosphatidylethanolamine in the L phase
|
|
Four diffracted orders can have 24 = 16 possible
combinations of sign; however, eight of these are simply the negative
of the remaining eight combinations (cf. Figs.
2 and 3).
Choosing a phasing that is centered on the midplane of the bilayer
requires that the middle of the electron density profile be coincident
with the terminal methyl dip, thereby eliminating 8 of the 16 possible phase combinations. The remaining combinations are shown in Fig. 2. The
minimum must also be bounded by maxima due to the phospholipid headgroups, followed by a decrease in electron density in the water
region. The average electron density is set to zero, as noted earlier,
and because the electron density of water is about equal to the average
electron density of the system, one expects a substantial decrease in
the electron density toward zero in the water region. This leaves only

+
and
++
as viable choices, with a preference toward 
+
,
because the dip in the water region is slightly deeper. To resolve this
choice satisfactorily, note that it has been shown that
18:1c
9-PE has a phasing of 
+
(So et al., 1993
).
Because 18:1c
9-PE is practically identical to 18:1t
9-PE in terms of electron density, it seems clear
that this is the proper phasing for 18:1t
9-PE as well.

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FIGURE 2
Electron density reconstructions of the
L phase for 18:1t 9-PE at 55°C. The
phasing is shown above the reconstruction. Only phasing combinations in
which the first phase is negative are shown in this figure. The
y-axis is the electron density in arbitrary units and the
x-axis is in angstroms.
|
|

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FIGURE 3
Electron density reconstructions of the
L phase for 18:1t 9-PE at 55°C. The
phasing is shown above the reconstruction. Only phasing combinations in
which the first phase is positive are shown in this figure. The
y-axis is the electron density in arbitrary units and the
x-axis is in angstroms.
|
|
For the other lipids studied besides 18:1c
9-PE and
18:1t
9-PE (except for 21:0ch-PE), the weak
second-order reflection was missing, and so it was straightforward to
pick the correct phasing, which was
0+
. The correct phasing for
21:0ch-PE was
++
, as shown by the following reasoning.
The strong first-order peak must have a minus phasing for the
hydrocarbon region to have a lower electron density than the headgroups
and the water. A plot of the remaining phase combinations is shown in
Fig. 4. The 21:0ch-PE has no
terminal methyls and must therefore have a relatively uniform electron
density in the hydrocarbon region. The only phase combination that
satisfies this is
++
. It is not surprising that most of these
lipids have the same phasing because the overall chemical structure of
all these lipids is quite similar. Finally, note that these phase
choices yield water-layer thicknesses that are the same to within an
angstrom for all of the lipids. Because it is reasonable that lipids
with the same headgroup and similar hydrocarbon chains should have the
same water-layer spacing, this helps confirm these phasing choices.

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FIGURE 4
Electron density reconstructions of the
L phase for 21:0ch-PE at 70°C. The phasing
is shown above the reconstruction. The y-axis is the
electron density in arbitrary units and the x-axis is in
angstroms.
|
|
Inverted hexagonal reconstructions
This method was applied to 18:1c
9-PE using the
amplitudes at 85°C and 95°C. The amplitudes for
18:1c
9-PE in the HII phase are shown in Table
4 and the amplitudes for the other lipids in the HII phase are shown in Table
5. According to the phasing criteria
developed by Turner and Gruner (1992)
, the best phasing is selected by
first eliminating from consideration all phase sets with a scale factor
C that varies from 1 by more than 0.05 and then picking the
phasing with the lowest
from the remaining choices. The best
phasing choice was (+
++++) according to the above criteria, with
the second-best phase choice having a value of
that was twice as
large. This is also the phasing found for the HII phases of
18:1c
9-PE by Turner and Gruner (1992)
. A reconstruction of 18:1t
9-PE using the +
++++ phasing is shown in a 3D
plot in Fig. 5. The electron density
shown is similar to that of 18:1c
9-PE (Turner and Gruner,
1992
).
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TABLE 4
Temperature (T, °C), measured amplitudes,
d, r, l , v, and
A for
1,2-di-O-oleoyl-3-O-phosphatidylethanolamine-sn-glycerol in
the HII phase
|
|
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TABLE 5
Temperature (T, °C), measured amplitudes,
d, r, l , v and
A for several hydrocarbon chain structural variants of
diacyl phosphatidylethanolamine in the HII phase
|
|
The phasing +
++++ was also found to be the correct phasing for the
other PEs studied, using the same phasing method. This is a reasonable
result, considering the similarity of the lipids. As will be shown in
the following section, several patterns emerge in the structural
parameters that also help confirm this phasing choice. For example, the
average lipid length appears to decrease by roughly the same amount
(1-1.5 Å) across the L
/HII phase transition for all the lipids studied. Additionally, the headgroup areas at the lipid-water interface assume similar values. This physically plausible behavior lends support to the phasing choice.
Structural parameters
The structural parameters of the L
and
HII phases are defined in Fig.
6. The dimensions that were found, as
described below, are listed in Tables 4-6 and Figs. 6-10. The value
of d is readily measured to an accuracy of ±1/2 Å and the position of the lipid-water interface can also be calculated
from the electron density reconstruction to a relative accuracy of
±1/2 Å (Turner and Gruner, 1992
). Though disorder is certainly
present in these systems, the method used to determine the lipid-water
interface uses experimental amplitudes that have not been altered to
correct for disorder. The values of d are given in Fig.
7, and the values of the water layer
thickness (w and r, as defined in Fig. 6) are given in Fig. 8.

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FIGURE 6
Typical terminology used in this study. (A)
The L dimensions, d is the d-spacing,
l is the lipid length, and w is the thickness of
the water layer between the lipid bilayers. (B) The
HII dimensions, d is the d-spacing,
lmin is the minimum lipid length,
lmax is the maximum lipid length, and
r is the water core radius. Note that in both diagrams,
A is the headgroup area at the lipid-water interface and
S is the area of the hatched region.
|
|

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FIGURE 7
Unit cell lengths (d in Fig. 6) for some
hydrocarbon chain structural variants of diacyl
phosphatidylethanolamine. Solid lines connect the L data
points and dotted lines connect the HII data points.
Representative error bars for each phase are plotted for
18:1c 9-PE at one data point per phase. ,
18:1c 9-PE; , 18:1t 9-PE; ,
20:0eai-PE; , 20:0dmi-PE; ,
19:0i-PE; , 19:0ai-PE; ,
21:0ch-PE.
|
|

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FIGURE 8
Water layer thickness (w or r in
Fig. 6) for some hydrocarbon chain structural variants of diacyl
phosphatidylethanolamine. Solid lines connect the L data
points and dotted lines connect the HII data points.
Representative error bars for each phase are plotted for
18:1c 9-PE at one data point per phase. The symbols have
the same meaning as in Fig. 7.
|
|
The d-spacings for the L
and HII phases
formed by the various PEs are presented in Fig. 7. In both phases, they
decrease as a function of increasing temperature, although, in general, the rate of decrease is smaller in the L
phase than in
the HII phase. The rate of decrease of the d-spacings with
temperature in both phases does not depend significantly on chain
structure. However, as shown in Table 6,
the magnitudes of the d-spacings of the L
and
HII phases at temperatures either side of their L
/HII phase transitions do depend
significantly on the structure of the hydrocarbon chains. In
particular, the d-spacings in the L
phase varied from
51.2 to 56.4 Å and those in the HII phase from 74.9 to
82.7 Å. These results differ from those reported in our earlier study
(Lewis et al., 1989
), where near-constant d-spacings of 52.5 and
77.0-78.0 Å for the L
and HII phases, respectively, were reported for these PEs. Interestingly, the values of
the d-spacings for the 18:1c
9- and
18:1t
9-PEs are the smallest in both the
L
and HII phases, whereas those for
19:0i and 19:0ai-PE are intermediate, and those
for the 20:0eai, 20:0dmi and
21:0ch-PE are largest. The possible molecular basis for
these observations will be discussed in a forthcoming paper to be
presented elsewhere (D. A. Mannock, R. N. A. H. Lewis, R. N. McElhaney, P. E. Harper, and S. M. Gruner,
submitted for publication).
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TABLE 6
Lipid dimensions (d-spacing, w, r,
l and A) at the
L /HII phase transition for the hydrocarbon
chain structural variants of diacyl phosphatidylethanolamine used in
this study
|
|
The dependence of the water-layer dimensions for the
L
and HII phases formed by the various PEs
studied here as a function of temperature are presented in Fig. 8. In
general, the thickness of the water layer separating adjoining bilayers
in the L
phase is much less than the radius of the
central water core in the HII phase, as expected. The
L
phase water-layer thickness (12.2-13.1 Å) also
varies less with changes in the structure of the hydrocarbon chains
than does the radius of the water core in the HII phase,
which varies from 20.9 to 23.1 Å (Table 6). Nevertheless, these values
vary much less with PE hydrocarbon chain structure than do the
d-spacings, indicating that variations in average lipid length and
headgroup area at the lipid-water interface must account for most of
the observed variations in the bilayer d-spacing. However, the small
variations in the radius of the water cylinders in the HII
phase formed by the various PEs follow the same trends as those
observed in the d-spacings of the L
and HII
phases, suggesting that the structure of the chains also plays a part
in determining the monolayer curvature in the HII phase.
With the lipid volumes, V, discussed in the Methods section
and a coefficient of expansion of
V/V
7 × 10
4/°C, one can use geometry to calculate the
headgroup area at the lipid-water interface. For the L
case, the headgroup area is given by
|
(10)
|
and, for the HII case,
|
(11)
|
where A is headgroup area at the lipid-water
interface, V is the lipid volume, d is d-spacing,
and r is the water core radius, all of which are defined in
Fig. 6. As expected, the headgroup areas at the lipid-water interface
(Fig. 9) are considerably larger and
increase more rapidly with increases in temperature in the L
phase than in the HII phase. However, the
most important feature of this plot, and the data in Table 6, is that
the headgroup areas at the lipid-water interface in both the
L
and HII phases just below and just above
the L
/HII phase transition are quite similar
for each PE hydrocarbon chain variant. These results suggest that the
effects emanating from the variation in the structure of hydrocarbon
chains on the headgroup area at the lipid-water interface are
relatively small.

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|
FIGURE 9
Headgroup area at lipid-water interface (A
in Fig. 6) for some hydrocarbon chain structural variants of diacyl
phosphatidylethanolamine. Solid lines connect the L data
points and dotted lines connect the HII data points.
Representative error bars for each phase are plotted for
18:1c 9-PE at one data point per phase. The symbols have
the same meaning as in Fig. 7.
|
|
The average lipid lengths are shown in Fig.
10. In calculating the average lipid
length for the HII phase, each length was weighted by the
volume of lipid for that length. If one assumes that the volume of each
lipid in a given phase at a given temperature is constant, then
weighting averages by volume is equivalent to averaging over all the
lipids. The derivation for the formula for the average length in the
HII phase is as follows. From Fig. 6, it is noted that
l(
), the lipid length as a function of
(in radians),
is defined
|
(12)
|
|
(13)
|
From geometry,
|
(14)
|
where r is the water core radius, l is lipid
length as a function of
, and lmin is minimum
value of l(
), as shown in Fig. 6. Define
|
(15)
|
for computational convenience. Solving for l yields
|
(16)
|
|
(17)
|
For the area S, as in Fig. 6,
|
(18)
|
|
(19)
|
|
(20)
|
Finally,
l
, the average lipid length, is given by
|
(21)
|
|
(22)
|
which to first order in (
1), is
|
(23)
|
Note that the expansion for
l
is accurate to
±0.2% for 0.5 <
< 1.5.

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FIGURE 10
Average lipid length ( l in Fig. 6)
for some hydrocarbon chain structural variants of diacyl
phosphatidylethanolamine. Solid lines connect the L data
points and dotted lines connect the HII data points.
Representative error bars for each phase are plotted for
18:1c 9-PE at one data point per phase. The symbols have
the same meaning as in Fig. 7.
|
|
The dependence of lipid length on temperature in the L
and HII phases formed by the various PEs studied here is
presented in Fig. 10. In all cases, the lipid lengths decrease with
increasing temperature in both phases at roughly comparable rates with
an abrupt decrease of 1.5-2.0 Å at the
L
/HII phase transition, as expected (Table
6). The magnitude of the lipid length values also changes with
hydrocarbon chain structure as was observed with the d-spacings.
Typically, the lipid lengths in both the L
and
HII phases of the 18:1c
9- and
18:1t
9-PEs are smallest, those for 19:0i and
19:0ai-PE are intermediate, and those for the
20:0eai, 20:0dmi, and 21:0ch-PE are
the largest. Thus, the bulk and position of the substituent branch on
the hydrocarbon chain determine Th by moderating
the ability of the hydrocarbon chains to shorten as a function of
increasing temperature. Once again, the possible molecular basis for
these observations will be discussed in a forthcoming paper to be
presented elsewhere (D. A. Mannock, R. N. A. H. Lewis, R. N. McElhaney,
P. E. Harper, and S. M. Gruner, submitted for publication).
 |
DISCUSSION |
The original impetus for this study came from an observation that,
at the L
/HII phase transition, all of these
PEs had very similar L
and HII d-spacings
(Lewis et al., 1989
). The goal of this study was to check whether the
internal dimensions followed the same pattern. In fact, it turns out
that the dimensions, both internal and external, vary by over 10%. The
difference with our earlier measurements (Lewis et al., 1989
) has been
traced to faulty temperature calibration. This result underscores the need for accurate temperature calibrations.
Besides correcting the earlier study, there are a number of
interesting features of the data that add insight into PE phase behavior. The first is that the water-layer thickness in the
L
phase is the same to within one angstrom for all of
these PEs (Fig. 8). This suggests that the headgroup plays the dominant role in setting the interlamellar water-layer thickness, with the
hydrocarbon chains playing a secondary role. It is also interesting to
note that the water layer shrinks at roughly the same rate as the
increase of the headgroup area at the lipid-water interface, implying that the property of the headgroups that sets the
water-layer spacing varies inversely with the headgroup area.
The rate of contraction of the hydrocarbon chains with increasing
temperature for a given lipid is roughly the same in both the
L
and HII phases. There is also a small
decrease in
l
of ~1.0-2.0 Å across the phase
transition, an amount that is approximately the same for all the PEs
under study (Fig. 10). The behavior of the headgroup area at the
lipid-water interface is far more dramatic, as the headgroup area
increases in the L
phase, and then drops dramatically
across the L
/HII phase transition. The headgroup areas at the lipid-water interface also tend to
have similar values in the HII phase (Fig. 9) regardless of
the hydrocarbon chain structure.
Comparison of the headgroup area at the lipid-water interface in these
PEs shows that the values of A are considerably larger and
increase more rapidly with an increase in temperature in the L
phase than in the HII phase. However, at
temperatures just below and just above the Th,
the values of A in both the L
phase and the
HII phase are largely independent of hydrocarbon chain
structure. These results indicate that, although differences in
hydrocarbon chain structure may determine the Th
on the absolute temperature scale by virtue of differences in the rate
of hydrocarbon chain shortening, the structure of the hydrocarbon
chains probably makes only a small contribution to the limiting area
per molecule at the lipid-water interface in both the L
and HII phases of these PEs. An overview of the
l
and A data suggests that these two
parameters are in direct competition, with the decreasing lipid length
driving the lipid-water interface to larger and larger areas in the
L
phase. Eventually, the lamellar morphology becomes too
costly energetically, and the system is forced to adopt the
HII phase, where the extra degree of geometric freedom allows both the hydrocarbon chains and polar headgroups to assume their
desired states.
The following picture is suggested as an explanation for this behavior
(Tate and Gruner, 1989
). There are two main free energies in the
system, one driving the hydrocarbon chains to a desired length that
decreases with increasing temperature and the other free energy pushing
the headgroup to an optimum area that is relatively temperature
independent. In the L
phase (for a nearly constant molecular volume), the lipid length and headgroup area at the lipid-water interface are uniquely related (see Eq. 10). Hence, these
two free energies are in direct competition, with the decreasing lipid
length and concomitant splaying of the hydrocarbon chains driving the
lipid-water interface to larger and larger areas. Eventually, this
becomes too costly and the system is forced into the HII
phase, where the extra degree of geometric freedom allows both the
hydrocarbon chains and headgroups to assume (on average) their desired
states. The only free energy cost keeping the system out of the
HII phase is that the lipid hydrocarbon chains are forced
to assume a variety of lengths to fill the hexagon (see Fig. 6). This
free energy cost due to the packing of the lipid chains in the
HII phase was demonstrated by Kirk et al. (1984)
.
These observations will be extended in another paper to be presented
elsewhere by considering lipids with a similar spectrum of hydrocarbon
chain structures but different chain lengths and polar headgroups
(D. A. Mannock, R. N. A. H. Lewis, R. N. McElhaney, P. E. Harper, and S. M. Gruner, submitted for publication).
This work was supported by operating and major equipment grants
from the Canadian Institute of Health Research (R.N.M.), the Alberta
Heritage Foundation for Medical Research (R.N.M.), National Institutes of Health grant GM32614 (S.M.G.) and Department of Energy
grant DE-FGO287ER60522 (S.M.G.). D.A.M. was funded by a postdoctoral fellowship from the Alberta Heritage Foundation for Medical Research. P.E.H. gratefully acknowledges fellowship support from both the National Science Foundation and the Liposome Co.
Address reprint requests to Sol. M. Gruner, Laboratory of Atomic and
Solid-State Physics, 162 Clark Hall, Cornell University, Ithaca, NY
14853-2501. Tel.: 607-255-3441; Fax: 607-255-8751; E-mail:
smg26{at}cornell.edu.
Dr. Paul E. Harper's present address is Department of Physics and
Astronomy, Calvin College, 3201 Burton SE, Grand Rapids, MI 49546.
Dr. Sol M. Gruner's present address is Dept. of Physics, Cornell
University, Ithaca, NY 14853.