Open Access Article
Khaled
Khairy
*a and
Jonathon
Howard
*b
aJanelia Farm Research Campus, 19700 Helix Drive, Ashburn, VA, USA. E-mail: khairyk@janelia.hhmi.org; Tel: +1 571 209 4217
bMax-Planck Institute of Molecular Cell Biology and Genetics, Pfotenhauerstrasse 108, Dresden, Germany. E-mail: howard@mpi-cbg.de; Fax: +49 351 210 2020; Tel: +49 351 210 2500
First published on 21st January 2011
An important open question in biophysics is to understand how mechanical forces shape membrane-bounded cells and their organelles. A general solution to this problem is to calculate the bending energy of an arbitrarily shaped membrane surface, which can include both lipids and cytoskeletal proteins, and minimize the energy subject to all mechanical constraints. However, the calculations are difficult to perform, especially for shapes that do not possess axial symmetry. We show that the spherical harmonics parameterization (SHP) provides an analytic description of shape that can be used to quickly and reliably calculate minimum energy shapes of both symmetric and asymmetric surfaces. Using this method, we probe the entire set of shapes predicted by the bilayer couple model, unifying work based on different computational approaches, and providing additional details of the transitions between different shape classes. In addition, we present new minimum-energy morphologies based on non-linear models of membrane skeletal elasticity that closely mimic extreme shapes of red blood cells. The SHP thus provides a versatile shape description that can be used to investigate forces that shape cells.
There are three general categories of methods for calculating minimum-energy membrane conformations.18 The first is solving the Euler–Lagrange equations constructed from the integrals of the energy and constraint expressions.2,19 This method has so far been restricted to shapes that are axially symmetric.13,14 The second is a brute force technique in which the surface is represented as a simply connected triangular mesh.9,20–22 It permits general (nonaxisymmetric) shapes, but limits the accuracy of geometric property calculations and renders energy minimization CPU-intensive. This approach may become more attractive with future developments of faster computer clusters and clouds. The third approach is to use an appropriate set of basis functions.17,18,23 The parameter set is small and can be varied within a numerical optimization strategy to minimize the energy expression directly. An especially intuitive basis is provided by the spherical harmonics basis functions.24 This basis was used for vesicle mechanics studies in the pioneering work of Heinrich et al.25 The spherical harmonics are the three dimensional equivalent of the one dimensional Fourier series, they form an orthonormal basis and their characteristics are well studied. However, they can only represent stellar objects, i.e. objects that have a point inside that can see all points on the surface without crossing the surface (Fig. 1a, left). This poses a serious limitation to modeling cells and vesicles because only nearly spherical shapes can be represented.
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| Fig. 1 The spherical harmonics parameterization (SHP). (a) Spherical harmonics functions are single-valued; their direct combinations can only represent stellar surfaces, i.e., surfaces that contain a point inside that can “see” every point on the surface. SHP, however, can represent both stellar and non-stellar objects. Left: stellar object, right: non-stellar object. (b) Surface reconstruction of a human red blood cell discocyte segmented from 3D confocal microscopy images.30 The top row and lower left shapes represent direct spherical harmonic expansions (eqn (1)) with approximations of increasing Lmax values; number of coefficients = (Lmax + 1)2. Even at the high order of Lmax = 22 (lower left), the centre of the discocyte suffers from artefacts (ringing). Colour: local curvature. Lower right: SHP of the cell at Lmax = 10. 30 non-zero coefficients capture the essential features of the cell with no apparent artefacts. | ||
To circumvent the above problems, we implemented the spherical harmonics method in parametric form (spherical harmonics parameterization SHP).26,27 SHP represents both stellar and non-stellar closed surfaces (Fig. 1a, right), and requires far fewer parameters than the direct spherical harmonics representation even for stellar objects (Fig. 1b). SHP has been used successfully in computer vision for performing quantitative shape analysis.28,29
In this work, we use SHP to map out shape space defined by the bilayer couple model. In this model, the bending energy is minimized for fixed values of the reduced volume (the volume normalized by that of a sphere of equal surface area) and the relative area difference between the bilayers. Due to the computational advantages of SHP, we explore transitions from one class of shapes to another, finding that the transitions are smooth. We also use SHP to calculate minimum-energy surfaces produced by a lipid–cytoskeletal composite membrane with highly non-linear elastic properties, such as that of the human red blood cell. Recently, RBC shapes were obtained for particular resting shapes of the membrane associated cytoskeleton.9,17 However, the influence of the resting shape on the final morphology has not been fully investigated. We have used the SHP method to show that a prolate resting shape for the membrane-associated cytoskeleton is able to predict observed detailed morphological features that do not appear for oblate or biconcave resting shapes.
![]() | (1) |
| yLK(θ,ϕ) = NLKPL,K(cos θ)cos (Kϕ), when K ≥ 0 |
| yLK(θ,ϕ) = NLKPL,K(cos θ)sin (|K|ϕ), when K < 0 | (2) |
As stated above, this representation is limited to stellar surfaces. We represent a general surface
that is topologically equivalent to the sphere, parametrically26 by expanding, in spherical harmonics basis functions, its individual Cartesian coordinates,
![]() | (3) |
![]() | (4) |
, and reduced area difference Δa = M/4πRo3, with
. For a sphere v = Δa = 1. We implemented the above simplified model to demonstrate the numerical power of SHP and for comparison with established work. However, the accurate modeling of a bilayer vesicle requires the “generalized bilayer couple model” in which the hard constraint of area difference is relaxed by replacing it with an explicit area-difference-elasticity term.2,25,33
![]() | (5) |
/kb, where
is the modulus corresponding to the stretching of the membrane leaflets due to the deviation from the preferred area difference. Co, ΔA and ΔAo are the spontaneous curvature, the difference in area between the outer and inner leaflets and the preferred difference respectively. Integration of the first term of eqn (5) is performed over the whole shape. EMS is the energy associated with the stretch and shear of the membrane skeleton. Here we closely follow the expression given in ref. 9 and 34,![]() | (6) |
. Δa0 is a measure of the tendency of the membrane to bend in or outwards and combines local and non-local effects (ESI, S6†).
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| Fig. 2 Phase diagram of the bilayer coupling model (adapted from the phase diagram of Fig. 3 in ref. 14), and simulated morphologies. (a) Part of the phase diagram adapted from Seifert et al. with the main morphological regions (phases) labeled. This part has been studied by Seifert et al. 1991 and Ziherl and Svetina 2005. Lines I, II and III show the fixed reduced volumes of 0.8, 0.7 and 0.59 along which we calculated minimum energy shapes using the bilayer coupling model and SHP shape representation. The three lines correspond to right, middle and left columns in (b) respectively. Dark circles indicate the locations at which shapes are shown in (b). (b) Right column: v = 0.8. Middle column: v = 0.7. Left column: v = 0.59. Numbers next to the shapes are Δa values. | ||
For the more spherical family of shapes corresponding to v = 0.8, we used Lmax = 3; this has 48 parameters. As the area difference was reduced from 1.3 to 0.6 in 0.1% steps, the minimum energy shape changed from bowling-pin morphology through dumbbell to ellipsoid, discocyte and stomatocyte (Fig. 2b, right column, corresponding top Fig. 2a, line I). The computational procedure was as follows. We started with a sphere and the first part of the optimization consisted of a series of steepest descent steps to satisfy the reduced volume and area difference constraints. This required 30 seconds. The second part consisted of bending energy minimizations satisfying those constraints at all times (ESI, S8†). A minimum energy shape resulting from one step was then used as starting shape for the next. The complete series was generated in 70 minutes. To test that a sufficiently broad range of shapes was explored for the minimization procedure, we raised Lmax to 5, with a total of 108 parameters. The same sequence was obtained with no significant decrease in the minimum bending energy, and no significant amplitudes in L orders above 3. The shape sequence in the right most column of Fig. 2b is in accord with the findings of Seifert et al. (1991) for the axisymmetric part, and with the findings of Ziherl and Svetina (2005)20 for the nonaxisymmetric part (fourth shape from the bottom).
Although axisymmetric shapes require only (Lmax + 1)2 + 2 parameters, starting with such a restricted set of parameters is only acceptable if the symmetry of the minimum energy shape is known beforehand. Usually, it is not. Therefore we kept our calculations general and made the full set available for optimization. Nevertheless, the number, order (L) and degree (K) of non-zero coefficients reflect symmetry, and result in a sparse representation for symmetric and smooth shapes. For example, the number of coefficients with amplitude >1% of the largest coefficient, for the top five shapes in the v = 0.8 sequence, was from top to bottom of Fig. 2b right: 13, 13, 11, 8 and 11. This clearly represents only a subset of the available 48. Truncating these coefficients from the series resulted in less than 0.01% increase in bending energy.
We then explored shapes with smaller reduced volume v = 0.7, in which the morphologies are more “deflated”. As the relative area difference was decreased from 1.25 to 0.6, the minimum energy shapes changed from dumbbell, biconcave discoid, discocyte to stomatocyte (Fig. 2a, line II, and Fig. 2b, middle column). This series is again in close agreement with the Seifert et al. phase diagram for the axisymmetric shapes. Non-axisymmetric morphologies for this constant reduced volume line are also in agreement with Heinrich et al. 199325 (Fig. 2b, middle column; second and third shapes from the top), as well as the values for the minimum bending energy Eb(S) (data not shown). The sequence 0.6 < Δa < 1.25 required 60 minutes, and was generated with Lmax = 3.
The third reduced volume that we explored was v = 0.59, corresponding to even more deflated morphologies (Fig. 2a, line III and Fig. 2b, column left). As the relative area difference was reduced from 1.4 to 0.6, the minimum-energy shapes ranged from dumbbell, through paddle-shape, plectrum, to discocyte and finally stomatocyte. The changing symmetry was handled naturally with SHP, and we found a smooth morphing of one shape into another. Our results agree with those of Seifert et al. (1991) for the axisymmetric shapes at Lmax = 3, including the dumbbell shape (Fig. 2b, left column: top shape). Our nonaxisymmetric sequence (Fig. 2b, left column: shapes 2–4 from the top), for which we used Lmax = 5, agreed with Fig. 1 of ref. 20.
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| Fig. 3 Experimentally induced and theoretically predicted sequences of RBC morphology. (a) 3D confocal images of DiI-labeled RBCs in solutions of increasing concentrations of NaCl (concentrations in mM shown on the images). (b) Theoretically predicted shapes that minimize the shape energy of eqn (5) under constraints of total surface area 140 µm2, and volume 100 µm3. The sequence was obtained by changing the value of the effective reduced area difference Δa0; from top to bottom by [%]: 0.072, 0.143, 1.717, 1.788 and 2.003. Δa0 indicates the tendency of the membrane towards blebbing (small values) or budding (large values). All calculations assumed a prolate ellipsoidal relaxed membrane skeleton with a reduced volume of 0.95. | ||
For simulating RBC morphology, we calculated minimum energy shapes corresponding to eqn (5) for a range of Δa0values. When using a prolate ellipsoid, our results are in excellent qualitative agreement with the observed RBC morphologies (Fig. 3b). As in the case of the bilayer coupling, the number of parameters was small, so the calculations were fast (40–60 minutes). For example, a discocyte requires only 4 nonzero parameters and is readily calculated at Lmax = 3. A flat spiculated cell (echinocyte I) contains features available at Lmax = 10, yet only 6 nonzero coefficients essentially capture the morphology. For more complicated shapes (Fig. 3b, bottom 2), Lmax was set to 12, and the optimization was performed overnight (12 hours). However, only 13% of the coefficients are nonzero.
Importantly, our simulations reproduced the out-of-plane spicules of the echinocyte I (Fig. 3, middle panels) when we introduced the prolate ellipsoidal undeformed membrane skeleton geometry. We did not computationally observe such out-of-plane spicules when oblate or discocytic resting skeleton shapes were assumed. It should be noted that out-of-plane spicules can be clearly experimentally observed in about half the cells (ESI, S9†), and the features persist over the time span of an imaging experiment (0.5 to 1 hours).
SHP can describe arbitrary genus-zero morphologies. It is not restricted to symmetric shapes and has an advantage over methods that calculate shape properties from surface triangular meshes in terms of accuracy and efficiency. Its primary limitation is that it is an approximation up to some expansion order. This limitation, however, will become less of a problem as computational power increases.
Footnote |
| † Electronic supplementary information (ESI) available: S1: the spherical harmonics series expansion; S2: calculation of associated Legendre functions and derivatives; S3: calculation of surface properties from SHP description; S4: testing convergence of SHP calculations with Gaussian quadrature; S5: testing accuracy of SHP with Gaussian quadrature against analytical methods; S6: a note on the preferred curvature and area difference; S7: numerical implementation of the membrane skeleton energy; S8: numerical optimization under constraints using sequential quadratic programming; S9: examples of echinocyte type I shapes. See DOI: 10.1039/c0sm01193b |
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