Direct visualization of hemolymph flow in the heart of a grasshopper (Schistocerca americana)

Background

Hemolymph flow patterns in opaque insects have never been directly visualized due to the lack of an appropriate imaging technique. The required spatial and temporal resolutions, together with the lack of contrast between the hemolymph and the surrounding soft tissue, are major challenges. Previously, indirect techniques have been used to infer insect heart motion and hemolymph flow, but such methods fail to reveal fine-scale kinematics of heartbeat and details of intra-heart flow patterns.

Results

With the use of microbubbles as high contrast tracer particles, we directly visualized hemolymph flow in a grasshopper (Schistocerca americana) using synchrotron x-ray phase-contrast imaging. In-vivo intra-heart flow patterns and the relationship between respiratory (tracheae and air sacs) and circulatory (heart) systems were directly observed for the first time.

Conclusion

Synchrotron x-ray phase contrast imaging is the only generally applicable technique that has the necessary spatial, temporal resolutions and sensitivity to directly visualize heart dynamics and flow patterns inside opaque animals. This technique has the potential to illuminate many long-standing questions regarding small animal circulation, encompassing topics such as retrograde heart flow in some insects and the development of flow in embryonic vertebrates.

Direct visualization of blood flow in small (millimeter-centimeter scale) animals remains a major challenge. Generally, spatial and temporal resolutions better than 50 μm and 0.1 s are required for studies in insect physiology. Current techniques, including x-ray, MRI, and ultrasound or visible light probes, suffer from insufficient spatial or temporal resolutions, lack of sensitivity, or inability to penetrate the animal's opaque body. For example, MRI has recently been used to visualize the internal dynamics of circulation, respiration, and digestion in tobacco hornworm pupae, but the temporal resolution (~300 ms) and spatial resolution (~150 μm, laterally) of MRI are insufficient to distinguish fine kinematic details of motion [1]. Consequently, internal movements in small animals such as insects remain poorly understood. One prominent example is the movement of hemolymph in the insect circulatory system. Real-time synchrotron x-ray phase-contrast imaging [2] has recently been demonstrated to be an excellent technique for the study of respiratory and digestive systems in small animals, and it has the necessary resolution to study blood flow as well. This technique is capable of spatial and temporal resolutions of ~1 μm and ~100 ps, respectively, although these parameters have to be weighed against the detrimental effects on the animal because higher temporal resolutions require higher beam intensities. Despite the capabilities of synchrotron x-ray imaging, this imaging technique alone cannot distinguish blood from the rest of the soft tissue because density differences are minimal. Here, we demonstrate a new method of visualizing blood flow at the micrometer scale in intact small animals using microbubble injection combined with synchrotron x-ray imaging.

For transparent or semi-transparent animals, visible light imaging techniques have been used successfully to study gross patterns of heart activity and blood flow in small animals. Movement of hemolymph, the insect 'blood', from the abdomen to the wings of a butterfly has been visualized by introducing a visible-light dye into the hemolymph [3]. Confocal microscopy has shed new light on the heart activity and blood flow in a zebrafish embryo, showing that pumping is not peristaltic, as was previously thought [4]. Optical coherence tomography (OCT) has been used to image heartbeat in Drosophila melanogaster [5], and Doppler OCT has been used to visualize blood flow in frog embryos [6]. Although these recent developments are promising, they remain ultimately limited by the transmission of light: many small animals have opaque exteriors and/or the heart is located sufficiently deep that there is insufficient visible light transmission to form an image. More importantly, none of these visible light techniques have demonstrated the ability to measure intra-heart flow patterns in animals with millimeter-centimeter-scale body size.

For animals with opaque bodies, a variety of indirect, non-imaging methods have been devised to deduce heart activity and circulation patterns. To study heart activity, researchers have implanted electrodes near the heart and used the impedance between them as a proxy for heart pulsations [7, 8]. This electrocardiogram technique is invasive and requires considerable skill in the implantation of the electrodes; moreover, it is not feasible for millimeter-sized animals. Alternatively, visible or infrared light transmission or reflected intensity has been used to detect heart pulsations [9, 10], and by using multiple probes, it is possible to deduce the temporal relationship between different heart segments [11]. Broad patterns of hemolymph flow have been inferred using 'thermography' in which thermistors are attached to the exterior dorsal surface near the heart [12] and flow is deduced by small temperature fluctuations in the thermistor. Indirect techniques have also provided inferential evidence for the relationship between hemolymph flow and CO₂ exchange [13–15], the retrograde flow through the insect heart [10, 11], and for the function of accessory pulsatile organs that are hypothesized to help circulation [16]. Although these non-imaging techniques provide evidence of bulk flow, they do not provide quantitative structural information involved in heartbeat (e.g., amount of compression or shape change) or circulation (e.g., flow patterns). Furthermore, because they are inferential, these indirect techniques face common challenges involving data interpretation. For example, insects can telescope the abdomen, compress internal air sacs, and contract the gut, and these movements may occur independently from the heartbeat, making it difficult to distinguish the 'true' signal from artifact with certainty (however, see [11]). Lastly, because these are 'point' techniques, they cannot provide the contextual spatial information provided by direct imaging techniques. For example, using thermography, it is not possible to differentiate between hemolymph flow in an insect's heart versus flow in the surrounding pericardial sinus [17].

The insect circulatory system is profoundly different than its mammalian counterpart. Instead of flow occurring in a closed system of tubes and produced by a large central pump, the insect system is open, consisting of a single, open-ended tube (the heart and aorta) that runs dorsally from the abdomen to the thorax or head [18]. The tube contains slit-like incurrent and excurrent valves (ostia) that run laterally along the length of the heart. Circumferential muscles ring the heart, and fan-like alary muscles connect it laterally to the body wall. Insects pump hemolymph through the heart toward the head (anterograde flow), and, in some species, reverse the flow toward the abdomen (retrograde flow) [10, 11]. However, the detailed flow patterns that result, both within the heart and body, and how exactly they are produced are almost entirely unknown. Thus the detailed mechanics of the circulatory system of perhaps the most speciose and abundant animal group on earth remains largely unknown. The ability to directly visualize the fundamental physiological functions of microfluid flow in situ will be extremely valuable in advancing our understanding of circulatory systems in insects and other small animals.

In this study, we visualized heart flow directly with synchrotron x-ray phase-contrast imaging combined with the use of microbubbles as high-contrast tracer particles. Microbubbles are used in clinical environments as contrast agents for ultrasound imaging [19, 20]; however, the spatial resolution for in-vivo ultrasound imaging is wavelength limited to about 100 μm [21]. Our technique allows for direct simultaneous visualization of hemolymph flow and heart and tracheal activity with micrometer-level spatial resolution and excellent image contrast. Although MRI [1] and OCT [5] have been used to study the structural dynamics of internal heart activity in insects, these techniques do not measure actual flow rates. As far as we know, this is the first measurement of intra-heart flow rates, patterns and dynamics with micrometer-level spatial resolution in an insect. Although the results presented here are taken with video rate (30 Hz) acquisition, much faster exposure times and frame rates are possible at the cost of increased damage to the animal [2]. This technique extends the capability of synchrotron x-ray phase-contrast imaging to study all three essential fluid transport systems in insects: respiration (air), feeding (liquid food), and circulation (hemolymph).

Microbubbles ranging from 10–150 μm in diameter were clearly visualized, as were air sacs and numerous tracheae, including a main longitudinal tracheal trunk that runs adjacent to the heart (Fig. 1C and Additional files 1, 2, 3, 4, 5, 6 and 7). The buoyant bubbles accumulated along the ventral edge of the dorsal diaphragm, which partially compartmentalizes the dorsal heart region. Within the heart, the buoyant bubbles demarcated the dorsal edge of the heart lumen. The ventral edge of the heart lumen could not be clearly identified, but the paths of microbubbles during flow within the heart suggested its ventral extent. Microbubble flow, compression of the pericardial sinus and changes in the tracheal diameters were all clearly visualized (Additional files 2, 3, 4, 5, 6 and 7).

Flow visualization in the heart of a grasshopper ( Schistocerca americana ) using synchrotron x-ray phase-contrast imaging. (A) Side view of the grasshopper abdomen showing the approximate location of the heart (blue) and the relative size of the imaging window (white rectangle, 1.3 × 0.9 mm). The abdomen is encapsulated in an x-ray transparent Kapton tube. Scale bar, 5 mm. (B), Cross-sectional schematic of the dorsal abdomen showing the relative sizes and locations of the heart (H), dorsal diaphragm (DD), and pericardial sinus (PS). The red arrow indicates the orientation of the x-ray beam. (C) X-ray video still of a region in the dorsal 3rd abdominal segment in lateral view. Round structures are air bubbles used to visualize patterns of heartbeat and hemolymph flow.

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As seen within the field of view (1.3 H × 0.9 V mm), the flow patterns were complex and dependent on location. At any particular location along the heart, general flow patterns were repetitive, but not strictly time-periodic, over the course of the measurement (10's of seconds). For most pulsations (e.g., Fig. 2), forward flows coincided with local pericardial compressions (see Methods). Interestingly, back flows, when they occurred, began during pericardial compression, and ended at or after the end of the compression. However, this could be due to a phase lag between the hemolymph and the bubble (see Discussion). The amplitude of pericardial sinus compression varied locally (Additional file 2). Compressions of the longitudinal tracheal trunk were not synchronized with the pericardial sinus compressions (e.g., Fig. 3); however, their frequencies were similar (0.8–1.0 Hz). Air sac compressions also appeared to be independent of pericardial sinus compressions (Additional file 1). Flow within the heart was pulsatile, but did not appear to be bolus-like. Unlike previously observed peristaltic transport in the gut [2] in which the bolus-like transport of food and gut peristaltic waves were readily apparent, the hemolymph transport mechanism within the heart remains unknown from this preliminary study.

Relationship between heart movements and hemolymph flow (3rd abdominal segment) in the grasshopper Schistocerca americana. (A) Side view x-ray video image indicating the color conventions used in (B). Anterior is to the right; dorsal is to the top. (B) Time series from one video sequence showing the relationship between pericardial sinus depth (blue) and hemolymph flow direction (green, yellow, white). Decrease in pericardial sinus depth corresponds to compression. Green represents net forward (anterograde) flow, yellow represents backflow, and white indicates zero flow. Average compression frequency was 55 cycles/min (0.92 Hz). In most instances, forward flow occurred only during compressive movements of the pericardial sinus, and presumably of the heart itself. Backflow did not occur with each forward flow event, but when it did, it occurred directly after the forward flow event. Note that there was no observable hemolymph movement for roughly half the time.

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Relative timing of compression of the pericardial sinus (blue) and a main longitudinal trachea (red) in the dorsal abdomen (4th segment) of the grasshopper Schistocerca americana. This sequence shows that the movements of the pericardial sinus and the trachea are not phase locked.

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The power of this technique is exemplified in the ability to track small-scale flow patterns. For example, bubbles can apparently be seen to enter the heart by moving through incurrent ostia (Fig. 4, Additional files 6 and 7). However, it was not possible to differentiate if the incurrent ostia were opening actively or passively, nor were we able to positively identify movement of bubbles out of the heart through excurrent ostia [22]. The local flow patterns near the ostia, but external to the heart, were complex. In general, bubbles were observed to enter the ostia originating both posteriorly (e.g., Fig. 4a, Additional file 6) and anteriorly (e.g., Fig. 4b, Additional file 7). In either case, once they entered the heart, the bubbles were swept anteriorly with the heartflow. Another example shows the complexity of flow within the heart. In Figure 5, four microbubbles are tracked over the course of 25 frames (~0.83 s) in one section of the heart. This sequence suggests that the bubbles were pulled towards the middle of the image during diaphragm dilation, and upon compression, hemolymph was transported towards the head. The ability to image individual microbubbles allowed us to quantify instantaneous velocities and potentially to map complex flow fields. Such detailed flow information cannot be obtained from any other technique.

Examples of bubble movement through presumed ostial openings in the heart wall of the grasshopper Schistocerca americana. Yellow bubbles represent single bubbles tracked through one video sequence (30 Hz), with the start of the sequence indicated in white and bubble positions corrected for whole-body movement. The blue arrows represent the apparent locations of ostia, inferred from the movements of the bubbles. (A) Heart entrance event in which the bubble traveled dorsally and anteriorly in the pericardial sinus, moved through the ostium, then was transported anteriorly within the heart (5th abdominal segment). For corresponding video, see Additional File 6. Scale bar, 200 μm. (B) Entrance event in which the bubble moved posteriorly in the pericardial sinus, dorsally through the ostium, and anteriorly after entering the heart (6th abdominal segment, same individual as above). For corresponding video, see Additional File 7.

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Examples of non-uniform flow patterns in the heart of the grasshopper Schistocerca americana. This schematic depicts the paths of four bubbles digitized in one video sequence (duration, 0.83 s) moving within the heart (white background, 6th abdominal segment). Each color represents a different bubble. Time between points is 0.033 s; the start of the sequence is indicated with black and white circles. The overall motion of the flow is from left to right (anterograde; toward the head), but the microscale flow is non-uniform. For example, the red and green bubbles begin moving to the left while the blue bubble was moving to the right; these bubbles also reverse direction to the left at the end of their sequences. Note that the purple bubble displays a counterclockwise vortical movement (shown with greater detail, inset box). The corresponding movement of the pericardial sinus is depicted in the graph (lower right). Note that the purple bubble enters the frame from the left at t = 0.20 s, 5 frames later than the other bubbles. Scale bar, 200 μm.

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Although the main purpose of this paper is to present this new technique, our measurements allow us to make a few preliminary observations on the hemolymph flow in the heart of the grasshopper Schistocerca americana.

1. In general, flow patterns are complex, and are time and location dependent. Furthermore, some flows appear to be three-dimensional. In some observations, there appeared to be no overall transport, but simply a back-and-forth oscillation of the hemolymph (Additional files 4 and 5). This preliminary study suggests that the origin of hemolymph transport may be more complicated than the commonly assumed peristaltic motion [10, 11, 14].

The maximum speed of bubbles that could be tracked was 9.5 mm/s; faster moving bubbles were observed but could not be reliably measured due to motion blur (exposure, 16 ms). Based on this maximum speed, a heart diameter of 0.5 mm, and using the viscosity of water as an estimate of that of hemolymph, we calculate a Reynolds number of 4.8, suggesting that flows are in the laminar regime.

3. For two individuals that were imaged for 20–30 minutes each, there was no evidence of a sustained retrograde fluid transport. The microbubble motion was either pulsatile with overall forward transport, or oscillatory with no net transport.

4. Respiratory structures (tracheae and/or air sacs) were compressed in patterns both synchronous and asynchronous to the local heartbeat.

5. No immediate detrimental effects on the animal were observed, either from the x-rays or from the microbubbles. The animals that were injected with microbubbles and under x-ray irradiation of the heart for up to an hour were alive 24 hours later. This is consistent with our previous results [2] which showed that there were no observable negative effects in insects at similar x-ray intensities under irradiation of the abdomen. Local x-ray damage must have occurred, but effects on heart, tracheal, or abdominal movements and behavior were not apparent within this time frame.

Prior work on grasshopper hearts consists of optical cardiography (Schistocerca gregaria, [9]), electrocardiography and mechanography (Melanoplus differentialis, [23]), and direct observation through live dissection (multiple species, [22]). These studies quantified heart activity, but did not measure hemolymph flow patterns within the heart. One valid comparison that can be made among studies is between mechanography (pulsations detected using an electromechanical setup) and our measured pericardial compressions. Among studies, measured pulsation frequencies (0.8–1.0 Hz) and waveform shapes are similar. Additionally, Jahn and colleagues [24] showed that the shapes and frequencies of the optical, electrical and mechano cardiography signals can vary greatly, from individual to individual, and show large dependence on temperature, further reinforcing the need for understanding the link between electrocardiography and actual flow.

More generally, we can compare this x-ray imaging method with other techniques that have recently been used to study small animal circulation. Confocal microscopy provides 2D depth-resolved images with micrometer-level spatial resolution, with depth of focus usually no more than a few micrometers, and high speed confocal microscopy has been demonstrated at 1000 frames per second (fps) [25]. Microscopic flow patterns can be quantified through the use of fluorescent tags, although depth of focus can be a limitation if the flow is not parallel to the focal plane. OCT provides cross-sectional images of the sample with spatial resolution in the tens of micrometers [26], and framing rates of 1000 fps have also been demonstrated [6]. Doppler OCT can provide information on bulk flow, but it is not quantitative [6]. Both confocal microscopy and OCT are visible light techniques and therefore are limited by light transmission. Recently, MRI has been used to image the cross-sectional structure and flow in the pupae of the tobacco hornworm caterpillar (Manduca sexta) [1]. However, the spatial resolutions (156 μm with a slice thickness of 500 μm) are still not comparable to synchrotron x-ray phase contrast imaging or visible light techniques. MRI cross-sectional images can be obtained at a frequency of about 3 Hz [1]. In contrast, the x-ray technique described in this paper has spatial resolution that is comparable to visible light techniques (μm-level), and high-speed x-ray imaging is possible as well. Compared to visible light techniques, x-ray imaging has the advantage of high penetration and can be used for opaque samples. X-ray images are 2D transmission projections and therefore depth information is lost, but this has the advantage that one can see through the entire animal without the need to adjust a 'depth of focus'. Transverse flow (perpendicular to x-ray direction), when imaged with tracer particles, can be quantified at the micrometer-level, which cannot be done with MRI or OCT. Two disadvantages of this technique compared to visible light or MRI are that (1) the x-rays can have a detrimental effect on the animal [2] and (2) the need for contrast agents or tracer particles.

Several challenges and improvements need to be addressed to make this technique more accessible. First, it is necessary to tailor the contrast agent to the animal or species. In particular, it is important to limit the amount of bubbles within the volume of interest; otherwise, the projected overlapping bubbles will overwhelm specific features of interest. Second, it is important to generate bubbles of the proper size; obviously, for visualization of internal heart flow, the sizes should be substantially smaller than the cross-sectional heart dimensions. Third, different species may require different injection protocols depending on anatomy and physiology. Finally, there is the question of bubble buoyancy and differences between bubble and fluid motion, which may be a major limitation on the quantification of flow. In our experiments, we oriented the insect's abdomen horizontally so that any observed posterior-to-anterior bubble flow could be definitively attributed to fluid flow, rather than to buoyancy. The buoyancy issue can be addressed in future studies by using tracer particles that have a more comparable density with hemolymph, such as metal-coated hollow glass spheres. Differences between actual fluid motion and bubble/tracer particle motion, and the effects of the bubbles themselves on the fluid motion, are complex questions that are beyond the scope of this paper, especially in the realm of non-uniform pulsating flow that we see here. Nonetheless, for the parameters used here, the speed of the bubble should reflect the speed of the fluid, although there may be a phase difference between the two [27, 28]. The use of neutrally buoyant and smaller tracer particles should solve this problem. Finally, although we were able to quantify representative instances of individual bubble speed, the frame rate (30 fps) of our camera was not fast enough for a more complete velocity map. Planned future work includes the use of a high speed video camera (> 500 fps), which should enable us to directly measure peak hemolymph flow velocities; the addition of flow-through respirometry, which would allow further insight into circulation-respiration coupling; and combination of this technique with available indirect techniques (e.g., thermography, light transmission) for purposes of verification and for generating complementary data.

For the first time, detailed fluid flow patterns in small animals can be imaged at the micrometer scale. In addition to insects, this technique should find applications in areas including vertebrate development (in such model systems as zebrafish or chick), and any other field in which the understanding of moving fluids behind opaque anatomy, at small scales, is key to answering outstanding questions of physiology. The potential applications of this technique are very broad.

Schistocerca americana grasshoppers (mass, 1.3–1.7 g) were obtained from the laboratory colony of Prof. Jon Harrison (Arizona State University) and were supplied with food and water ad libitum prior to the experiment. Only males were used. We used clinical grade microbubbles (lipid/octafluoropropane bubbles; Definity, Bristol-Meyers Squibb) as the contrast agent. The average size of the microbubbles in the contrast agent (98% < 10 μm, 2.4–3.1 μm median) was near the spatial resolution of our system and therefore was at the limit of visibility. These clinical grade microbubbles could indeed be seen in the grasshopper, but they did not provide the degree of flow visualization that we were seeking. To achieve larger, more easily tracked bubbles in the animal, we purposely left air (roughly the same volume as the Definity solution) in the tip of the needle when loading the syringe with the microbubble solution; during injection, both air and solution were then transferred into the grasshopper, creating additional 10–150 μm sized bubbles in the hemolymph. For the creation of the larger bubbles, the Definity solution merely acted as a non-toxic surfactant to reduce surface tension, and it is likely that other cheaper alternatives may work as well. We experimented with different injection protocols; for the data presented in this paper, we injected the animal both on the dorsal and ventral sides of the abdomen, near the third to last segment. On the dorsal side, we attempted to inject into the pericardial sinus, but were unable to verify placement due to hemolymph circulation between the time of injection and the start of imaging. Bubbles appeared stable over the course of the measurements (20 min to 1 hr), and disappeared within 24 hours.

Animals were held in place with a clip attached to the wings, with the abdomen oriented parallel to the ground and orthogonal to the x-ray beam, providing a lateral view image (Fig. 1). The legs and abdomen were inserted into separate Kapton (Dupont) tubes with slightly larger diameters, permitting small movements but precluding large-scale movements for stable imaging. The tubes were arranged to position the legs out of view. The animal was mounted on a translation stage, allowing movement relative to the x-ray beam, and translation was controlled remotely.

For x-ray imaging, the x-ray energy was 25 keV and the incident power density was 80 W mm^-2, similar to that used in our previous work [2]. The x-rays passing through the insect were converted to a visible light image using a cerium doped Y₃Al₅O₁₂ scintillator, which was then imaged onto a video camera (Cohu 2700) using a Mitutoyo 5× microscope objective together with a tube lens. The field of view was approximately 1.3 mm × 0.9 mm. Video images were recorded onto miniDV tapes. iMovie (Apple, OSX) was used to convert movie clips into still image stacks (30 frames per second) and then analyzed using MATLAB (Mathworks, MA, USA). A 400-mesh transmission electron microscope grid was used for image calibration. The data were collected at the X-ray Operations and Research beamline 32-ID-C at the Advanced Photon Source, Argonne National Laboratory.

For image analysis, the following protocol was used. To quantify pericardial compression, we identified locations along the heart with the most pronounced movement and digitized two points: one on the dorsal diaphragm, which moved dorsoventrally during compression, and one near the dorsal cuticle, which was static relative to compression. We defined pericardial depth as the vertical distance between these points; decreasing pericardial depth indicates compression. For tracheal compression analyses, we measured the diameter of the trachea by digitizing the dorsal and ventral edges of the tube. For some sequences, we scored flow discretely as forward (bubbles moving anteriorly), backward (bubbles moving posteriorly) or none (no overall translation of bubbles). Due to bubble buoyancy, our flow quantification was restricted to the dorsal regions of the heart.

We thank Jon F. Harrison of Arizona State University for providing the grasshoppers used in this study, and Mark Stremler for discussion. Use of the Advanced Photon Source was supported by the U. S. Department of Energy, Office of Science, Office of Basic Energy Sciences, under Contract No. DE-AC02-06CH11357.

Author notes

Affiliations

1. X-ray Science Division, Argonne National Laboratory, 9700 S. Cass Avenue, Argonne, IL, 60439, USA

   • Wah-Keat Lee
   •  & John J Socha

2. Current address : Department of Engineering Science and Mechanics, Virginia Polytechnic Institute and State University, Blacksburg, VA, 24061, USA

   • John J Socha

Corresponding author

Correspondence to Wah-Keat Lee.

Authors' contributions

Both authors contributed equally to the conception, data collection, analysis and writing of this work, and have read and approved the final manuscript.

Wah-Keat Lee and John J Socha contributed equally to this work.

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