A select group of hemipterans within the suborder Auchenorrhyncha are the only animals that feed exclusively on xylem sap – a nutritionally poor liquid that exists under negative pressure within a plant's xylem vessels. To consume it, xylem-feeding bugs have evolved enlarged cibarial pumps capable of generating enormous negative pressures. A previous study examining the allometry of this feeding model suggested that small xylem feeders pay relatively higher energetic costs while feeding, favouring the evolution of larger-bodied species. However, this interspecific analysis only considered adult xylem-feeding insects and neglected the considerable intraspecific change in size that occurs across the insect's development. Here, we examine the changes in cibarial pump morphology and function that occur during the development of Philaenus spumarius, the common meadow spittlebug. We show that the cibarial pump scales largely as expected from isometry and that the maximum negative pressure is mass independent, indicating that size has no effect on the xylem-feeding capacity of juvenile spittlebugs. We conclude that a first instar nymph with a body mass 2% of the adult can still feed at the >1 MPa tension present in a plant's xylem vessels without a substantial energetic disadvantage.

The dilute sap within a plant's xylem vessels is under negative pressure (tension), as it consists primarily of water that is being pulled from the soil and through the plant before evaporating into the atmosphere. These negative pressures can be immense, routinely exceeding −1 MPa. Despite xylem sap being both nutrient poor and hard to extract, some insects within the sub-order Auchenorrhyncha (order Hemiptera) feed exclusively on this liquid. These insects likely all evolved from a single xylem-feeding ancestor and as a group they represent the sole origin of this mode of feeding in the animal kingdom (Bell-Roberts et al., 2019). To extract xylem sap, they possess an enlarged muscular cibarial pump that can produce negative pressures exceeding those within a xylem vessel. The cibarial pump consists of a bipennate cibarial dilator muscle (CDM) which attaches to an apodeme extending from the midline of a flexible diaphragm covering the top half of a rigid cibarial chamber (Fig. 1). Contraction of the CDM lifts the apodeme and attached diaphragm away from the floor of the chamber, drawing liquid inward. The negative pressure generated within the cibarial chamber can be calculated by dividing the component of the CDM's force acting in the direction of the cibarial diaphragm's displacement by the area of the diaphragm (Fig. 1B–D). As the biomechanical and energetic challenges involved in this mode of feeding are clearly enormous, there may be geometric or energetic constraints on cibarial pump function associated with changes in the insect's size.

Fig. 1.

Micro-computed tomography (micro-CT) scans of Philaenus spumarius. (A) Philaenus spumarius heads (left) and their internal cibarial dilator muscle (purple) and cibarial chamber (yellow; right) across development from third instar to adult. (B) Frontal plane section showing pennation angle θ of the bipennate cibarial dilator muscle (CDM) relative to the muscle contraction vector and apodeme movement vector . (C) Area of the cibarial diaphragm (left) and a cross-section through the chamber (right) showing the height h of the diaphragm above the chamber floor. (D) Schematic diagram of the cibarial pump. FCDM, total force produced by the contracting CDM; FCiBD, component of the FCDM acting in the direction of the apodeme and cibarial diaphragm's displacement; PCSA, physiological cross-sectional area; Cib. diaph., cibarial diaphragm.

Fig. 1.

Micro-computed tomography (micro-CT) scans of Philaenus spumarius. (A) Philaenus spumarius heads (left) and their internal cibarial dilator muscle (purple) and cibarial chamber (yellow; right) across development from third instar to adult. (B) Frontal plane section showing pennation angle θ of the bipennate cibarial dilator muscle (CDM) relative to the muscle contraction vector and apodeme movement vector . (C) Area of the cibarial diaphragm (left) and a cross-section through the chamber (right) showing the height h of the diaphragm above the chamber floor. (D) Schematic diagram of the cibarial pump. FCDM, total force produced by the contracting CDM; FCiBD, component of the FCDM acting in the direction of the apodeme and cibarial diaphragm's displacement; PCSA, physiological cross-sectional area; Cib. diaph., cibarial diaphragm.

Close modal

A previous allometric analysis of cibarial pump function by Novotny and Wilson (1997) examined a wide range of adult xylem-feeding hemipteran species and concluded that feeding on xylem sap may become more energetically favourable with increasing body size, potentially promoting the evolution of larger-bodied xylem-feeding insects. Based on analysis of external cibarial and mouthpart morphology, this earlier study concluded that ‘cibarial pump load’ L (volumetric flow rate of xylem sap Q divided by CDM volume) scaled with body volume (equivalent to body mass Mb) as Mb−0.17, while the pressure difference (Δp) required to move xylem at flow rate Q through the insects’ tube-like stylets scaled as Mb−0.21. Thus, both L and Δp were predicted to diminish as Mb increases, enhancing the efficiency of xylem extraction in larger insects. Crucially, however, this study's focus on adult xylem-feeding bugs did not consider the substantial change in size that occurs in all these species as they develop from a first instar nymph into an adult: all xylem-feeding bugs begin their lives small! We re-examined these conclusions from an intraspecific analysis of cibarial pump function across ontogeny.

One of the most studied xylem-feeding insects is Philaenus spumarius, a globally distributed spittlebug species that is an important vector of the plant disease Xylella fastidiosa (Cornara et al., 2017). Adult P. spumarius have been found to produce pressures of −1.3 MPa within their cibarium (Bergman et al., 2021), allowing them to extract the xylem sap from over 300 herbaceous and woody plant species (Bodino et al., 2020; Hamilton, 1982; Weaver and King, 1954). While the first instar hatches out with a body mass of just ∼0.2 mg, it eventually grows into an adult weighing between 8 and 9.5 mg, equivalent to a 40–45 times increase in body mass (Horsfield, 1978). Yet even the newly hatched first instars apparently feed by inserting their mouthparts into xylem vessels (Horsfield, 1978) and so must encounter the same hydraulic challenges as the adults. Here, we used micro-computed tomography (micro-CT) scans of P. spumarius heads (third instar to adult) to investigate whether the morphology of their cibarial pump displays isometric scaling across ontogeny (where variables scale with body mass Mb according to the square-cube law: length Mb0.33, area Mb0.67, volume Mb1.0), and whether changes in body size are related to changes in the pump's function.

Study animals

Nymphs and adults of Philaenus spumarius (Linnaeus 1758) (n=1 third instar, n=6 fourth instars, n=8 fifth instars and n=5 adults, as determined from eye width comparisons with a developmental data series in Weaver and King, 1954) were collected from around the UBC Point Grey campus, Vancouver, BC, Canada, between May 2019 and June 2023. Nymphs were first placed on a piece of tissue paper to remove any adhering spittle mass, then all specimens were weighed individually to 0.01 mg on an electronic balance (XPE205 DeltaRange, Mettler Toledo, Greifensee, Switzerland). They were then narcotized in pure CO2 and photographed on a stereomicroscope to determine their maximum head width (measured from a dorsal image as the maximum distance across the eyes) before their heads were removed and prepared for micro-CT scanning.

Micro-CT scanning

Philaenus spumarius nymphs and adults were decapitated with a double-edged razor blade and their heads were placed in fixative (4% PFA and 2.5% glutaraldehyde in a 0.1 mol l−1, pH 7 sodium phosphate buffer) before being transferred into 70% ethanol for storage. Fixed heads were stained in 1% phosphotungstic acid in 70% ethanol and scanned at resolutions of 1–4 µm using a 3D X-ray microscope (Xradia Versa 520, Zeiss, Oberkochen, Germany). Scan slices were compiled and stacked with image analysis software (Dragonfly v.4.5.0.711, Object Research Systems Inc., Montreal, QC, Canada) to generate 3D reconstructions of the heads (Fig. 1). The CDM and cibarial chamber were digitally highlighted as regions of interest (ROI) for relevant length, area and volume measurements used for calculating the suction capacity of each specimen. Cibarial chamber and CDM volume were generated from the total highlighted voxels of the respective ROI. The cibarial diaphragm cross-sectional area was calculated by outlining the largest-diameter cross-section of the cibarium perpendicular to the apodeme – the area over which the force of the CDM is exerted (Fig. 1C). Muscle fibre length l was measured as the distance between two points placed at either end of a chosen muscle fibre (from its insertion on the apodeme to its origin on the interior of the postclypeus; Fig. 1B). A muscle fibre in one of the middle sheets of muscle and close to the centre of a sheet was chosen as the representative muscle fibre for each individual. Pennation angle was calculated using four points – one each at the rostral and caudal ends of the apodeme and the other previously defined points for a single muscle fibre. The angle between the apodeme and muscle fibre vectors was calculated using:
(1)
As some individuals displayed post-mortem contraction of their CDM, as indicated by the displacement of their cibarial diaphragm away from the floor of the cibarial chamber, both the muscle fibre length and pennation angle were corrected to the relaxed muscle fibre conditions. The relaxed muscle fibre length (l′) was calculated using:
(2)
where l is the uncorrected muscle fibre length, θ is the original pennation angle and h is the measured displacement of the cibarial diaphragm away from the floor of the cibarial chamber (Fig. 1C). The relaxed pennation angle θ′ was calculated as:
(3)
Food canal length was measured by generating a continuous path from the distal end of the proboscis, through the stylets, to the point where the food canal enters the cibarial chamber. Physiological cross-sectional area of the CDM was calculated using an image plane that was oriented perpendicular to the majority of the muscle fibres in one-half of the CDM. The CDM was then sectioned into a stack of 1-voxel-thick slices parallel to the chosen plane with the physiological cross-sectional area of the CDM generated for each slice. If the difference between slices was positive, the areas were summed, giving the physiological cross-sectional area of one half of the bipennate CDM, which was then multiplied by 2 to give the total cross-sectional area of the CDM. This was then multiplied by the estimated specific tension of the muscle (assumed to be 297 kN m−2, as determined previously for this species; Bergman et al., 2021), giving the total force produced by the contracting CDM (FCDM). The component of the FCDM acting in the direction of the apodeme and cibarial diaphragm's displacement (FCibD) was calculated using the corrected pennation angle θ′:
(4)
The maximum suction pressure each insect could generate within its cibarial pump was then calculated by dividing FCibD by the area of the cibarial diaphragm (Fig. 1C).

Statistical analysis

Data were analysed and stats were performed in R v.3.5.1 (http://www.R-project.org/) running in RStudio v.1.1.463 (https://posit.co/products/open-source/rstudio/). Each variable was tested for normality using quantile–quantile plots and the Shapiro–Wilk normality test. Body mass and all the variables of interest were log transformed before generating linear regression models with 95% confidence intervals for each variable using the stats (v.3.5.1) package.

The dimensions of the cibarial chamber scale isometrically across development, with neither the volume of the chamber nor the cross-sectional area of the cibarial diaphragm scaling with exponents distinguishable from Mb1.0 or Mb0.67, respectively (Fig. 2A,B, Table 1). However, the dimensions of the CDM do differ from isometry in two aspects: CDM volume scales less than predicted with an exponent of Mb0.85, and this may be attributed to the lower exponent for CDM muscle fibre length (Mb0.23) (Fig. 2C,E, Table 1). CDM physiological cross-sectional area scales as Mb0.64 (Fig. 2D), but this exponent is not significantly different from isometry, indicating that relatively shorter muscle fibres explain the reduced CDM volume rather than a reduction in their cross-sectional area and force production capacity. Likewise, the scaling of pennation angle is independent of body mass (Mb−0.07), with an average empty-cibarium corrected angle of 28.39±1.2 deg (Fig. 2F). Finally, the scaling of maximum suction pressure calculated from these variables is also independent of body mass, scaling with Mb0.05, which is not significantly different from Mb0 (Fig. 2G).

Fig. 2.

Relationship between various cibarial pump parameters and body mass plotted on log–log axes. (A) Cibarial chamber volume; (B) cibarial diaphragm cross-sectional area (CSA); (C) CDM volume; CDM physiological cross-sectional area (PCSA); (E) CDM muscle fibre length; (F) pennation angle; (G) maximum pressure; (H) food canal length. Solid lines show linear regressions while grey bands indicate 95% confidence interval limits. n=20 for all regressions, except food canal length (n=13).

Fig. 2.

Relationship between various cibarial pump parameters and body mass plotted on log–log axes. (A) Cibarial chamber volume; (B) cibarial diaphragm cross-sectional area (CSA); (C) CDM volume; CDM physiological cross-sectional area (PCSA); (E) CDM muscle fibre length; (F) pennation angle; (G) maximum pressure; (H) food canal length. Solid lines show linear regressions while grey bands indicate 95% confidence interval limits. n=20 for all regressions, except food canal length (n=13).

Close modal
Table 1.
Slope and intercept from linear regressions of log10 transformed variables versus body mass according to the equation: log(y)=log(a)+blog(Mb)
Slope and intercept from linear regressions of log10 transformed variables versus body mass according to the equation: log(y)=log(a)+blog(Mb)

The previous intraspecific analysis of adult xylem-feeding insects focused on two metrics to evaluate the impact of changes in scale on cibarial pump energetics: Pump load L [volumetric flow of xylem sap (Q)/CDM volume] and pressure drop across the mouthparts for a given Qp) (Novotny and Wilson, 1997). Pump load L was predicted to scale as Mb−0.17 (Novotny and Wilson, 1997), indicating that the energetic requirements of xylem sap extraction decreased with increasing size. However, this result assumes that Q is proportional to the insect's metabolic rate, assumed to be Mb0.75, while CDM volume was estimated from measurements of the exterior of the frontoclypeus, giving a scaling exponent of Mb0.94 for cercopids and cicadas. The P. spumarius data presented here, however, show that their CDM volume scales across development as Mb0.85, significantly lower than predicted from isometry. Using this exponent, and assuming pumping frequency is mass independent, Q should scale with cibarial chamber volume (Mb0.90), giving an L of Mb0.05. Xylem excretion rate (also equal to Q) has also been measured empirically across all P. spumarius life stages by Horsfield (1978) and plotting these data shows Q scales with mass as Mb0.89. Using this value of Q then gives an L of Mb0.04. These exponents are both close to zero, suggesting it is no more difficult for a newly hatched first instar spittlebug to extract xylem sap than it is for the adult. The close agreement between the scaling exponents for measured values of Q and cibarial chamber volume (0.89 and 0.90, respectively) further supports the assumption that pumping frequency is mass independent.

An allometric analysis of the pressure drop (Δp) required to move xylem sap through the insect's proboscis at a given volumetric flow rate Q can be made using the Hagen–Poiseuille (H–P) equation:
(5)
Assuming geometric similarity (dynamic viscosity µ=Mb0.0, proboscis length lprob.=Mb0.33, Q=Mb1.0, π=Mb0.0 and r=Mb0.33×4), Δp should be mass independent (Mb0.0). The analysis of Novotny and Wilson (1997) assumed Q was proportional to metabolic rate or Mb0.75, and so concluded that Δp should scale as Mb−0.25. Factoring in the average scaling exponent for proboscis length lprob. measured from both adult cercopids and cicadas (lMb0.29 and Mb0.41, respectively; Novotny and Wilson, 1997) reduced this exponent to Mb−0.21.

For P. spumarius, the length of their food canal (the distance from the tip of the stylets to where it joins with the cibarial chamber) lFC scales as Mb0.30 [the average of Mb0.29 from this study (Fig. 2H) and Mb0.31 for external stylet length measured by Hoffman across all instars; Hoffman, 1983] while its internal radius r is assumed to follow geometric similarity: Mb0.33 (Novotny and Wilson, 1997). If it is assumed cibarial pumping frequency is mass independent, then Q should scale with the same exponent as cibarial chamber volume (Mb0.90), resulting in Δp scaling as Mb−0.13. Or, if Q scales the same as the rates of xylem excretion measured across ontogeny by Horsfeld (Mb0.89; Horsfield, 1978), Δp then scales as Mb−0.14. Thus, P. spumarius likely experience a more moderate decrease in Δp across their development than predicted from looking across adult xylem-feeding species (Novotny and Wilson, 1997). However, the importance of this parameter Δp on the energetic requirements of xylem feeding needs additional context: the pressure gradient needed to drive xylem sap through the insects’ stylets is very small relative to negative pressures encountered within the xylem vessel (Δp<0.025 MPa or less than 2% of the maximum calculated cibarial pressure generated by an adult P. spumarius; Ranieri et al., 2020). Thus, it may be concluded that a reduction in the proboscis’ already relatively minor resistance to xylem sap flow will not substantially reduce the cost of xylem sap extraction as body mass increases.

Although the H–P equation has been applied to understand flow through the food canal of P. spumarius (e.g. Novotny and Wilson, 1997; Ranieri et al., 2020), its correct application requires certain assumptions are approximately satisfied, including that the flow velocity profile within the tube is parabolic and laminar, and that flow is continuous (Loudon and McCulloh, 1999). A parabolic velocity profile forms when laminar flow enters a tube and becomes fully developed some distance from the entrance. That distance is termed the ‘entrance length’ lE. If lE is large relative to the tube's total length (e.g. lE>10% total length), then the pressure and flow relationships predicted using the H–P equation will become increasingly inaccurate. lE can be calculated as:
(6)
using Q (m3 s−1) and the liquid's kinematic viscosity, ν (m2 s−1) (Loudon and McCulloh, 1999). Assuming a Q of 0.57 μl min−1 as the rate of flow through the food canal of a feeding adult P. spumarius (Bergman et al., 2021) and that xylem sap has the same density and viscosity as water (ν=1×10−6 m2 s−1) gives an lE of 0.70 μm. This is smaller than the internal diameter d of the food canal (given as an ellipse with major and minor axis d of 9 and 7 μm, respectively; Malone et al., 1999). But as lE has a lower bound of ∼0.6d (i.e. the minimum distance a fluid must flow within a tube to develop a parabolic velocity profile is 0.6 times the tube's diameter; Loudon and McCulloh, 1999), it is safe to assume parabolic flow is fully developed within ∼5.4 μm from the entrance of the food canal. Even if Q was an order of magnitude larger, lE would still be less than 1% of the total length of a ∼1.575 mm long food canal, meaning entrance effects may be safely ignored. Does this change across ontogeny? As the calculated lE is proportional to Q, it must scale with the same exponent of Mb0.89, while food canal diameter scales as Mb0.33. The result is that the calculated lE must decrease with body mass faster than the food canal diameter, resulting in lE≈0.6d and negligible entrance effects for all nymphs.
While the H–P assumption of continuous flow is clearly violated by the pulsatile suction generated by the cibarial pump, the Womersley number (Wo) can be used to evaluate whether the flow remains in phase with the oscillating pressure gradient (Wo<1) or becomes unsteady (Wo>1). In the Wo<1 flow regime, the greatest oscillation in fluid velocity occurs furthest from the walls of the tube, resulting in a parabolic velocity gradient. Wo is calculated as:
(7)
where d is the tube's diameter (m), ω is the oscillation frequency (rad s−1) and ν is kinematic viscosity of the xylem sap (1×10−6 m2 s−1) (Loudon and Tordesillas, 1998). Using a d of 9 μm (Malone et al., 1999) and considering the range of pumping frequencies recorded for adult P. spumarius (4.40–10.68 rad s−1) (Bergman et al., 2021; Cornara et al., 2018; Malone et al., 1999) gives a range of Wo from 0.009 to 0.015. As Wo≪1, the flow's velocity remains in phase with the pressure oscillations generated by the cibarial pump, producing a parabolic velocity profile as it flows through the food canal. As the food canal's d is smaller in nymphs and ω is assumed to be mass independent, Wo must be even lower in juveniles. This analysis suggests that although the pressure gradient and flow velocity oscillate over time, the instantaneous relationship between pressure and flow within the food canal are essentially what they would be during steady Poiseuille flow (Zamir, 2000), supporting the use of the H–P equation to examine the scaling of Δp.

Conclusion

This study reveals that all P. spumarius nymphs generate the same maximum cibarial pressures as the adult bug, and that the energetic requirements of xylem sap extraction are essentially independent of body mass. Thus, contrary to a previous intraspecific analysis of adult xylem-feeding insects (Novotny and Wilson, 1997), across development there is no size-dependent change in the costs associated with this feeding strategy. This conclusion is consistent with the observation that P. spumarius nymphs and adults both insert their mouthparts into xylem vessels (Horsfield, 1978) and largely feed on the same plant species (Weaver and King, 1954). While some changes in host plant preference have been observed to occur across development (Cornara et al., 2017), this can be attributed to changes in the length of the mouthparts: larger individuals possess a longer proboscis housing longer stylets, giving them access to xylem vessels located more deeply within a plant's stem or beneath a thicker layer of trichomes (Hoffman and McEvoy, 1985). Repeating this study on those xylem-feeding species that undergo a switch in feeding location (e.g. from subterranean roots to aerial stems) or plant host species (e.g. from herbaceous plants to trees) when they transition from nymph to adult (e.g. cicadas) could be an important test to determine whether this isometric pattern of cibarial development is common to all xylem-feeding bugs, or whether there are cases where cibarial development does not result in functional equivalence to accommodate changes in the xylem tensions encountered at different stages of development.

Our thanks to the two anonymous reviewers for their constructive comments and suggestions.

Author contributions

Conceptualization: P.G.D.M.; Methodology: E.A.B., P.G.D.M.; Validation: E.A.B.; Formal analysis: E.A.B.; Investigation: E.A.B.; Data curation: E.A.B.; Writing - original draft: E.A.B., P.G.D.M.; Writing - review & editing: E.A.B., P.G.D.M.; Visualization: E.A.B.; Supervision: P.G.D.M.; Project administration: P.G.D.M.; Funding acquisition: P.G.D.M.

Funding

This work was supported by Natural Sciences and Engineering Research Council of Canada Discovery grant RGPIN-2020-07089 and Accelerator RGPAS-2020-00039 to P.G.D.M.

Data availability

The morphological data extracted from the micro-CT scans are available from figshare: https://doi.org/10.6084/m9.figshare.26012821.v1

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Competing interests

The authors declare no competing or financial interests.