- Research article
- Open Access
The growth pattern of the human intestine and its mesentery
BMC Developmental Biology volume 15, Article number: 31 (2015)
It remains unclear to what extent midgut rotation determines human intestinal topography and pathology. We reinvestigated the midgut during its looping and herniation phases of development, using novel 3D visualization techniques.
We distinguished 3 generations of midgut loops. The topography of primary and secondary loops was constant, but that of tertiary loops not. The orientation of the primary loop changed from sagittal to transverse due to the descent of ventral structures in a body with a still helical body axis. The 1st secondary loop (duodenum, proximal jejunum) developed intraabdominally towards a left-sided position. The 2nd secondary loop (distal jejunum) assumed a left-sided position inside the hernia before returning, while the 3rd and 4th secondary loops retained near-midline positions. Intestinal return into the abdomen resembled a backward sliding movement. Only after return, the 4th secondary loop (distal ileum, cecum) rapidly “slid” into the right lower abdomen. The seemingly random position of the tertiary small-intestinal loops may have a biomechanical origin.
The interpretation of “intestinal rotation” as a mechanistic rather than a descriptive concept underlies much of the confusion accompanying the physiological herniation. We argue, instead, that the concept of “en-bloc rotation” of the developing midgut is a fallacy of schematic drawings. Primary, secondary and tertiary loops arise in a hierarchical fashion. The predictable position and growth of secondary loops is pre-patterned and determines adult intestinal topography. We hypothesize based on published accounts that malrotations result from stunted development of secondary loops.
Congenital intestinal malrotations are thought to be present in 1:200–500 live births . Malrotations are considered as incomplete or abnormal rotations of the midgut around the vitelline/superior mesenteric artery (SMA). The symptoms of malrotation are not well understood and not all malrotations become symptomatic [2, 3]. If malrotations become symptomatic, it is usually in the early months of life, with 75–85 % of cases diagnosed within one year of age . If one assumes that malrotations represent “frozen” stages of normal development , it becomes important to establish how the intestine develops.
The standard description of normal intestinal “rotation” encompasses a couple of sequential developmental steps. Initially, the midgut loop forms and extends into the extra-abdominal cavity due to rapid growth of this part of the intestine. This process is known as physiological intestinal herniation. Further development of this loop is associated with a change in position of the small intestine from cranial to right-sided, and of the cecum from caudal to left-sided, that is, with an apparent ~90° counterclockwise rotation. The duodenojejunal junction acquires its left-sided position during the herniation phase of development, whereas the cecum acquires its right-sided position upon return of the gut into the abdominal cavity. Together, these changes in position would represent an additional ~180° counterclockwise rotation. However, few of these largely schematic descriptions and illustrations are based on original studies (e.g., [6–8]. Moreover, the authors of one of the first studies already cautioned that “it must not been assumed that the main vessel, the SMA, actually forms an axis around which the loop twists” . This so-called rope model with an “en-bloc rotation” of the gut over 270° around the SMA has, nevertheless, become the current paradigm in virtually all texts. Despite a century of studies, it remains unclear to what extent active rotation, or its absence, contributes to intestinal development .
Another hallmark of intestinal development is the formation of the intestinal coils. Although the shape and position of the early loops appear very constant [10–13], it is widely assumed that the number and position of the small intestinal coils are random. An invariable pattern of loop formation during the early herniation period implies the presence of a pre-pattern, whereas a random pattern is compatible with a stochastic control of loop formation. The tensile interaction between the intestinal tube and its suspending mesentery was recently proposed as a potential mechanism for stochastic coil formation .
If we are to resolve these apparent contradictions, it becomes important to establish what part of intestinal looping is hard-wired in a genetically determined pre-pattern and what part is not. We, therefore, reinvestigated the looping pattern of the human intestine and provide virtual 3D reconstructions of the intestinal loops, their blood supply and mesenteric suspension in human embryos during and after herniation into the hernial sac. The results support the existence of a pre-pattern for the establishment of the intestinal loops during the early herniation period, which in turn largely determines the topography of the intestine in the abdominal cavity after the umbilical herniation has resolved. In contrast, the loops that are formed during and after the late herniation period appear to form under stochastic control.
The pre-herniation period
The foregut could first be identified in Carnegie Stage (CS) 9 embryos (25–27 days post fertilization) and the hindgut at CS10 (28–30 days). The rapid longitudinal growth of the embryo in the 5th developmental week, reflected in a 5-fold increase in greatest length , resulted in a corkscrew-like appearance of the longitudinal body axis. The caudal portion of the embryo was always located to the right of the head (Fig. 1a). Since both fore- and hindgut were midline structures in this period, their longitudinal axis followed that of the body (see 3D-PDF CS14). The initial connection of the intestine with the yolk sac was wide and located at the right side. This connection grew less rapidly than the embryo proper and became the tubular vitelline duct (Fig. 1a; ).
The formation of the midgut (week 5)
The intestine started to loop ventrally during CS14 (33–35 days), with the connection with the vitelline duct at its apex (Fig. 1a, Fig. 2a,b). The connection of this “primary” loop with the dorsal body wall was visibly thinner than the comparable connections of more cranial or caudal parts of the gut, and was, therefore, already identifiable as the dorsal mesentery of the midgut (Fig. 1b,c). The cranial end of the midgut loop (color coded orange) was located between segments 11 and 13 (corresponding to Th4-6; for numbering of segments, see Methods) between the confluence of both vitelline veins and the origin of the vitelline artery from the aorta (Fig. 1a; see also 3D-PDF CS14). The caudal end of the midgut loop was found caudal to a local widening of the midgut, the future cecum, at the level of segments 17–18 (Th10-11; Fig. 1a,c). The plane through the midgut loop and its mesentery remained midsagittal, that is, followed that of the helical body axis (see 3D-PDF CS14).
Landmarks for the apex of the midgut loop
The midgut is that part of the intestine which forms the primary loop. Later in development, when vessels can be distinguished, it coincides with the distribution area of the superior mesenteric artery (SMA, see the section on “The branching pattern of the superior mesenteric artery”). The vitelline artery and duct, unambiguous landmarks for the apex of the midgut, were located inside the “periductal” mesenchyme that surrounded the connection of the intestine with the yolk sac (Fig. 1b,c). The vitelline duct became interrupted at CS15 (35–37 days) and the vitelline artery no longer extended as a patent vessel into the periductal mesenchyme at CS16 (37–40 days). We, therefore, designate its remaining proximal part as the SMA from CS16 onwards. Another conspicuous vessel in the periductal mesenchyme that is rarely described in literature was the right vitelline vein, which drained blood from the yolk sac. The right vitelline vein passed the midgut apex and proximal midgut limb cranially. At CS14, the vessel was attached to, but not embedded in the connective tissue surrounding the intestinal tube (Fig. 2a,b), but in subsequent stages, the vein became disconnected from the intestinal mesenchyme, so that it appeared as a “free” vessel in the abdominal cavity (Fig. 2d-f). The left vitelline vein drained the midgut and was found inside the mesentery between the proximal and distal limbs of the primary loop. Just caudal to the pancreas, both veins merged. The periductal mesenchyme and the right vitelline vein continued to mark the apex of the midgut loop until shortly after the return of the herniated intestine into the abdominal cavity.
The herniation period
The herniation of the primary midgut loop (week 6)
Starting in the 5th week and continuing during the 6th week, the root of the SMA descended from the level of segment 13 to that of segment 19 (corresponding to Th6 and Th12, respectively). The position of the esophagogastric junction, pylorus, pancreatic ducts and confluence of both vitelline veins descended concomitantly, but over 8–9 segments (Fig. 3a). The descent was initiated when the body axis is still helical (Fig. 3b), so that a cranial midline structure that shifted caudally, also shifted to the right of the midline (Fig. 3c). As a result of the descent, the cranial limb of the midgut acquired a position to the right of and at same transverse level as the caudal limb (Fig. 3d,e). During the 6th week, the helical appearance of the embryonic body axis resolved, concomitant with the straightening of the trunk (Fig. 3b,c). From this stage onwards, the umbilicus and the associated structures exited the embryo at its ventral side. The midgut loop increased further in length, so that its apex herniated into the umbilical coelom (Fig. 3d,e). The proximal midgut segment (red) did not develop a thin mesentery. The dorsal mesentery of the remaining part of the midgut transformed into a rod-shaped mesenchymal mass. At its ventral tip the rod remained connected with the periductal mesenchyme. The right vitelline vein and mesenteric rod formed the central axis of the primary loop (Figs. 2e-h, 3d,e and 3D-PDF CS16).
The appearance of four secondary loops (week 7)
In the course of the late 6th and 7th weeks of development, the midgut increased ~1.4-fold in length and formed 4 secondary loops (Fig. 4). The 1st secondary loop (coded red and orange) developed intra-abdominally at CS16 (Fig. 3d,e) between the duct of the ventral pancreas and the passage of the midgut through the umbilical orifice. Initially, this 1st secondary loop expanded rightward and caudally on the right side of the SMA (Figs. 3d,e and 4). The other three secondary loops developed extra-abdominally during CS17 and CS18 (39–45 days; Figs. 3d,e and 4). The 2nd and 3rd loop (coded yellow and green, respectively) developed from the remaining part of the cranial limb of the midgut and expanded caudally and then leftward on the right side of the axis formed by the SMA, right vitelline vein, and mesenteric rod (Fig. 4). The distal end of this axis, i.e., the periductal mesenchyme and right vitelline vein, still marked the apex of the intestine. The 4th loop (coded blue) developed from the caudal limb of the midgut between the apex and the cecum, and expanded cranially on the left side of the axis. Thin sideward extensions of the mesentery connected the intestinal tube with the mesenteric rod (Fig. 5a). The mesenteric leaf on the right side of the mesenteric rod connected with loops 2 and 3, while the leaf on the left side connected with loop 4 and the proximal colon (Fig. 5a,b and 3D-PDF CS20).
The appearance of tertiary loops (week 8)
The length of the small intestine increased ~6-fold during CS20-23 (Fig. 6) with all secondary loops lengthening evenly. In addition, the radial length of the mesenteric leaves of the secondary loops increased, so that each secondary loop now clearly had its own leaf (3D-PDF CS23; compare Fig. 5b,c). The 3rd and 4th loops remained separated by the central axis, formed by the mesenteric rod, right vitelline vein, SMA, and periductal mesenchyme. The mesenteric leaves associated with the secondary loops remained recognizable during subsequent development and, thus, formed landmarks for these loops. The continued longitudinal growth was further accompanied by the appearance of tertiary loops within the secondary loops (Fig. 6a-d). The tertiary loops differed from the secondary loops in that their deposition varied between different embryos of similar stage (Fig. 6e-g). Of note, tertiary loops only developed within secondary loops with a mesentery. Accordingly, the proximal (future duodenal) part of the 1st secondary loop (coded red) did not develop tertiary loops. Interestingly, the 2nd secondary loop (coded yellow) assumed a left-sided position inside the hernia during the formation of tertiary loops (Fig. 6e-g). Although this change in position is obviously important for its future position in the abdomen (see: “Resolution of the hernia”), we have not identified any external cause for it.
The branching pattern of the superior mesenteric artery
The SMA, which was reconstructed in five specimens from 8 to 10 weeks of development, showed a consistent branching pattern, with 10–13 small-intestinal branches originating from the caudal side of the artery and 1–3 smaller colonic branches from its cranial side (Fig. 7a,b). The 7–8 caudal branches with an intra-abdominal origin at CS23 supplied the 1st and 2nd secondary loops. The 3rd caudal branch was of particular interest, because it supplied both intra- (distal part of the 1st secondary loop; coded orange) and extra-abdominal (2nd secondary loop; coded yellow) portions of the small intestine (Fig. 7a,b). The portion of the SMA passing the umbilical ring did not give off caudal branches, which probably explains the short gap between the intra- and extra-abdominal branches of the SMA. Distances between extra-abdominal branches were larger than those between intra-abdominal branches. Extra-abdominal branches 10–12 supplied the 3rd secondary loop (coded green) and the terminal branches the 4th secondary loop (coded blue). The periductal mesenchyme was still present as the landmark defining the apex of the midgut. A colic branch consistently arose on the cranial side of the SMA between the 7th and 9th caudal SMA branches. Because of the constant branching pattern of the SMA, these branches were suitable landmarks to follow the fate of the intestinal coils during and after the return of the herniated intestinal loops in the 9th week of development.
Resolution of the hernia (week 9)
While the crown-rump length (CRL) of the embryo and the length of the small intestine increased ~4- and >10-fold, respectively, between 5 and 9 weeks of development (Fig. 8a), the diameters of the intestinal tube and the umbilical orifice both increased only ~1.5-fold (Fig. 8b). Since the diameter of the umbilical orifice is ~4-fold larger than the outer diameter of the gut tube throughout the period of study, ~8 gut loops would be able to pass at once if the mesentery is not included, indicating that the umbilical orifice remained large enough to allow passage of intestinal coils, even shortly after intestinal return. Intestinal return from the hernial sac could also be triggered by an increase in free abdominal space. However, the length of the intestine increased 1.5 fold more rapidly than the abdominal width. Furthermore, the liver continued to occupy a large portion of the abdominal volume, as its right inferior border continued to reach the level of the lumbar vertebrae L3–4. In addition, the ratio of the volume of the left and right liver lobes did not change between 5 and 10 weeks development. Finally, as Fig. 8c shows, we observed that the dorso-ventral “depth” of the abdomen (measured as the distance between the aorta and the umbilical orifice) increased ~2-fold between 8.0 and 9.5 weeks of development, while the mesenteric rod became shorter in the same period. This differential increase in the depth of the abdomen and the length of mesenteric rod should facilitate and may even initiate intestinal return from the hernial sac.
The post-herniation position of the secondary loops
The 1st secondary loop increased substantially in length and continued to expand in a leftward direction caudally of the mesenteric rod. The 2nd and 3rd secondary loops moved back into the abdominal cavity between 8.5 and 9.0 weeks of development to occupy left-sided and mostly median positions, respectively (Fig. 9a; 3D-PDF 9.0 WKS). The colon co-migrated with these loops as demonstrated by the finding that the cecum had moved inward before the 4th secondary loop of the small intestine and the appendix (Figs. 9a and 10c). The 4th secondary loop and cecum returned to a ventral midline position in the abdominal cavity at 9.5 weeks (Fig. 9b). Between 9.5 and 10.0 weeks, the 4th secondary loop, cecum and appendix moved rightward and only slightly caudal to their definitive positions near the iliac crest (corresponding to lumbar vertebra L4; Figs. 9c and 11a; 3D-PDF 9.5 WKS). After the complete return of the herniated intestine, the empty hernial sac persisted for at least a week, indicating that the newly attained intra-abdominal position of the intestines was not metastable. The described deposition of the small intestine and its mesentery from the upper left to the lower right part of the abdominal cavity was reflected in the winding staircase appearance of the approximately 10 (caudal) branches of the SMA (Fig. 11d) and represents its definitive position.
Development of the colon
The colon did not develop secondary loops. In agreement, the relative contribution of the colon to the total intestinal length declined with age (from ~50 % of small intestinal length at CS14 to ~15 % at 10 weeks). The cecum was located close to the dorsal body wall at CS14 (Fig. 1a,b), herniated at CS16 (Fig. 3e), and occupied a left-sided position during the entire herniation phase, but remained close to the midline (Fig. 4). The mesentery of the proximal colon connected to the mesenteric rod (Fig. 10e1, f1 and f3), whereas that of the distal colon attached in the midline to the dorsal body wall from the kidneys (Th12) downward (Fig. 10e2, f1 and f2). The transition of the proximal colon into the distal colon was located where the mesocolon passed as a “roof” over the vitelline vein, SMA, and duodenojejunal junction (Fig. 10a-d). It was marked by the boundary of the vascular territories of the superior and inferior mesenteric arteries, which were identifiable from CS15 onwards. After CS23, when the branches of the IMA become unambiguously identifiable the left colic bend can be clearly distinguished. The descending colon and its mesentery moved leftward between 8 and 10 weeks of development, concomitant with the leftward increase in length of the 1st secondary loop (Fig. 4). The proximal colon and its mesentery followed the course of the central mesenteric rod and the SMA from a still medial position and dorsoventral orientation at 9.5 weeks (Fig. 10d) to a diagonal and coronal position at 10.0 weeks (Fig. 11a-c). In the 10th week, the proximal colon did not have separate ascending and transverse portions yet, and accordingly a hepatic flexure was not yet identifiable. Figure 11e shows, for comparison, the position of the colonic mesentery in the adult, with the parts of the mesocolon of the ascending and descending colon that still have to merge with the posterior body wall shown in light and dark purple, respectively.
We studied the midgut during its looping and herniation phases of development and distinguished 3 generations of midgut loops. The topography of the primary and secondary loops was constant, but that of tertiary loops not. The primary loop changed from a sagittal to a transverse orientation due to the descent of ventral structures over at least 8 segments when the body axis was still helical. The 4 secondary loops determined the definitive topography of the intestine. The 1st secondary loop (duodenum and proximal jejunum) assumed its left-sided position during herniation. The 2nd secondary loop (distal jejunum) assumed a left-sided position inside the hernia just prior to return, while the 3rd and 4th secondary loops retained near-midline positions. Intestinal return into the abdomen resembled a backward sliding movement. Only after its return into the abdominal cavity, the 4th secondary loop (distal ileum and cecum) descended to the right lower abdomen. Our description shows that the “en-bloc rotation” model of midgut development is a fallacy of schematic drawings.
The midgut as a structural entity
The midgut is usually defined as the portion of the gut that is perfused by the SMA and that shows the characteristic features of herniation and rotation . Earlier definitions described the midgut as the intestinal loop between the duodenojejunal flexure cranially and the colic bend (or angle or flexure) caudally [6, 16]. These definitions leave space for arguments about the proximal and distal boundaries. If the boundary of the perfusion areas of the celiac trunk and SMA is taken as criterion for the junction of the foregut and midgut, the proximal boundary is positioned in the perfusion area of the pancreaticoduodenal arteries [17, 18]. Furthermore, the ventral mesentery and the glands that penetrate the muscularis muscle (liver, dorsal and ventral pancreas, Brunner’s glands) end where the duct of the common bile duct and ventral pancreas enter the duodenum. Vascular supply, caudal end of the ventral mesentery, and intestinal architecture appear strong arguments to locate the junction between the caudal foregut and midgut at the ventral pancreatic duct, that is, midway along the descending part of the definitive duodenum. If the remainder of the duodenum represents, by consequence, the most cranial portion of the midgut, it never acquires the thin dorsal mesentery that develops more caudally from CS14 onwards. We hypothesize that a relatively thin dorsal mesentery identifies parts of the gut with rapid longitudinal growth. Interestingly, we did not observe tertiary looping in the distal duodenum, suggesting that tertiary looping reflects rapid longitudinal growth and requires the presence of a thin mesentery. The (left) colic bend as caudal boundary of the midgut is present as the gradual transition of the horizontal into the vertical portion of the colon during herniation, but can be unambiguously identified after the main branches of the superior and inferior mesenteric arteries become identifiable at CS23 and even more so after the bend has become acute after week 13.
The developmental origin of the convoluted small intestine
Frazer and Robbins stated that the midgut developed between fixed proximal and distal boundaries: the duodenojejunal junction was fixed by the ligament of Treitz (LOT) and the colic angle by a “retention band” . Snyder and Chaffin considered both bends as growth zones instead . We and others observed a rapid longitudinal growth of the entire small-intestinal part of the midgut and the coincident thinning of the mesentery . The midgut formed 3 generations of loops, each with their own characteristics.
The primary loop encompasses the entire midgut. Its asymmetric growth has been ascribed to laterality in gene expression , and asymmetric outgrowth of the mesentery due to extracellular-matrix and cytoskeletal remodeling [22–25]. The correlation between heterotaxia syndromes and malrotation also suggests a genetic component in intestinal looping . However, the chirality of heart looping in chicks was recently shown to depend on the turning of the head , that is, upon a biophysical factor . When the primary loop was still a midline structure at CS14, its limbs followed the helical shape of the body axis. Concomitant with the descent of the ventral thoracic and upper abdominal structures after CS13 (also reported by [10, 29–31], more cranial midline structures acquired a right-sided position and more caudal structures a left-sided position relative to the midline. These findings imply that the change in the position of the primary loop, like the heart loop, depends on the chiral growth of the body. We found no evidence for an effect of an asymmetric expansion of the liver and associated positional changes of the vasculature [16, 32], because the liver already has an asymmetric shape prior to the rightward shift of the proximal limb of the primary loop .
The small intestinal portion of the primary loop was further divided into secondary loops according to a strict spatiotemporal pattern during the late 6th and early 7th week. This second generation of intestinal loops and their very constant distribution were already described two centuries ago [10–12], but have since disappeared from descriptions, probably because their presence did not accommodate the prevailing theories of intestinal malrotation (see: “Implications for malformations”). The secondary loops probably develop, like the primary loop, as a result of the rapid growth of the intestinal tube, but the exact number (four) and predictable growth pattern of the secondary loops suggests a genetic regulation.
The secondary loops formed additional, tertiary loops after the second half of the 8th week of development. Tertiary loops did not have a predictable constant distribution pattern and their formation coincided with an acceleration of the longitudinal growth of the small intestine. In a recently proposed model of gut development, regular loops emerged when the relative growth rates and elasticity of the gut tube and its mesentery differed . Even though both the length of the gut and that of the mesentery increased, the individual domains of the four secondary loops remained identifiable since the mesenteric leaves were shorter in the transition areas between these domains. Mall already showed that the 4 domains of the secondary loops could still be identified in ~50 % of adult cadavers . We could confirm his findings in a smaller number of cadavers. If not all domains could be identified, there were fewer or one was of smaller size.
What triggers intestinal return?
Prior to return into the abdominal cavity, the longitudinal growth of the intestine was much more rapid than that of the embryo, but its diameter increased at the same rate as that of the hernial connection with the abdominal cavity and allowed the passage of several intestinal loops at once. We and others showed in rare intermediate stage embryos (9.5 weeks) that the intestine returned in a proximodistal fashion, with the distal jejunal loop (yellow) first , then the proximal ileal loop (green) and cecum, and the distal ileal loop (blue) and appendix last (Fig. 9a). The deep incisures between the mesenteries of the secondary loops further suggested that the secondary loops could move independently of each other. This architecture could facilitate phased return of the loops through the umbilical orifice. These size considerations imply that, even if tertiary loops can only partially uncoil, the width of the hernia neck does not appear to determine the time window for intestinal return, as is often hypothesized . Although we are not aware of experiments to explore the return mechanism, we hypothesize that the decrease of the length of the mesenteric rod relative to the dorso-ventral depth of the abdomen is responsible for the proximodistal sequence in the return of the intestinal segments to the abdominal cavity. This mechanism was first proposed by Pernkopf in 1925 [11, 12].
Does the midgut rotate?
We have, of course, asked ourselves the question whether the change in position of the duodenojejunal junction and the cecum relative to the axis of the SMA represented a 270° rotation. Rotation is usually described to occur in 2 phases, that is, during formation of the primary loop and upon intestinal return into the abdominal cavity [6, 16], but sometimes an intermediate stage that represents the growth of the secondary loops is included . We also mapped the positions of the 4 secondary loops relative to the SMA as degrees of rotation when they first develop (5.5 weeks), during intrahernial growth (between 5.5 and 8 weeks), and after return (>9.0 weeks). Figure 12 shows that the rotation of the primary loop is experienced by all parts of the midgut. Although the outcome of our model does not differ from the “en-bloc” rotation model in this phase of development, it proposes for the first time a potential mechanism for the initiation of asymmetric gut development, namely the descent of the distal foregut and its derivatives in embryos with a still helical body axis. The subsequent topographical changes of the intestine relative to the SMA during late herniation are most pronounced in the proximal duodeno-jejunal loop (orange) which extends caudal to the SMA in a leftward direction over a 3-week period, suggesting it represents a period of local growth. Thereafter, the position of this segment hardly changes in position. In contrast, the distal ileal loop (blue) hardly changes in position relative to the SMA during late herniation, but does so within a few days after return in the abdominal cavity. As Fig. 9 shows, this latter change in position is due to a movement of this part of the gut from midsagittal and ventral to right-lateral and more dorsal. Even though the rotational change of this part of the intestine after intestinal return appears extensive, the linear change in position is only minor. If one insists on using the term rotation for this movement, it would be largely around a craniocaudal axis (in the transverse plane) rather than a dorsoventral axis (frontal plane). In view of the brief time window and orientation of the apparent rotational axis, we conclude that the distal ileum and cecum “slide” rather than “rotate” as from the umbilical orifice to the lower-right abdominal cavity. “En-bloc rotation” is a conceptually simple and, therefore, attractive model of intestinal development, but the very different degrees, rates, and developmental timing of the apparent rotation of different parts of the midgut shows that this model cannot be upheld. Our present study shows that hierarchical looping is a viable new model to describe key morphogenetic events in intestinal development (for a comparison of both models, see Fig. 13).
Implications for malformations
By far the best-known malformation of the intestine is malrotation. If problems with intestinal rotation are taken as the underlying mechanism, reversed rotation and complete nonrotation are the extreme conditions of the spectrum of malrotations . Reversed rotation is a rare anomaly in which colon and duodenum rotate clockwise instead of counterclockwise in relation to the SMA, so that the transverse colon ends up posterior to the superior mesenteric vessels . We hypothesize that the early helical growth of the embryo is reversed in these cases. If nonrotation is diagnosed, the cecum and ascending colon have a left-sided instead of the normal right-sided position, while the position of the ligament of Treitz (LOT) is unaffected. This intestinal configuration resembles the configuration before the “slide” of ileum and proximal colon from the umbilical orifice to the lower-right abdominal cavity. The remaining malrotations are classified as either typical or atypical . A typical malrotation is defined by a right-sided position of the LOT, whereas an atypical malrotation has a left-sided LOT relative to the vertebral column [3, 35]. The position of the cecum is subhepatic in the vast majority (~85 %) of both typical and atypical malrotations [35, 37], that is, the ascending colon is too short. The position of the LOT can be regarded as the marker for the development of the 1st secondary loop and the position of the cecum as marker for the 4th secondary loop . Abnormal positions of the LOT and cecum are not necessarily linked [3, 19].
Based on our study, we hypothesize that growth restriction of secondary loops underlies the development of malrotations. A right-sided position of the LOT implies that the growth of the 1st secondary loop is impaired. Similarly, we hypothesize that a cranial position of the cecum and short ascending colon imply impaired development of the 4th secondary loop and proximal colon. The cecal position in malrotations resembles that at 9.5 weeks of development, so just after intestinal return, when it occupies a subhepatic position and the proximal colon is still relatively short. It is not surprising that underdevelopment of the 1st and 4th secondary loops produces a more pronounced phenotype than of the 2nd or 3rd secondary loops, because underdevelopment of the latter loops would “only” present as short bowel syndrome. In agreement, short bowel syndrome occurs in combination with intestinal malrotation as a genetic disease [38–40]. Variation in the degree of development of the respective secondary loops would also explain the variance in the size of the domains of the small intestine in adults .
What could cause growth retardation of the intestine? Although we can only speculate about the cause(s), vascular incidents are an appealing option. A rare but instructive congenital malformation is the “apple peel” small bowel. This malformation is characterized by jejunal or ileal atresia and absence of the dorsal mesentery [41, 42]. In some cases of jejunal or ileal atresia, squamous epithelial cells, lanugo hair, or bile droplets were reportedly found distal to the atresia and even between atretic segments [43, 44], suggesting the atresia developed after bile production started. These congenital malformations were plausibly attributed to intestinal injuries after e.g., vascular accidents. We hypothesize that similar accidents can cause insufficient growth of the secondary loops during herniation or shortly after return. This hypothesis may also explain the presence of Ladd’s bands: after the injury, tissue repair entails the development of scar tissue.
Intestinal morphogenesis is characterized by 3 phases of looping, each with a distinct underlying mechanism. The secondary loops of the small intestine develop according to a highly predictable pattern. We hypothesize, based on published accounts of malrotations, that the pathology associated with these malformations results from incomplete development of the secondary loops.
This study was undertaken in accordance with the Dutch regulation for the proper use of human tissue for medical research purposes. We included anonymized specimens from the historical collections of embryos and fetuses of the Departments of Anatomy and Embryology, Leiden University Medical Center, Leiden, and the Academic Medical Center, Amsterdam, The Netherlands, and the Carnegie Collection, Washington D.C., USA (obtained via the Digitally Reproduced Embryonic Morphology (DREM) project) that were donated for scientific research. Only specimens with an intact umbilicus were selected for reconstruction. The criteria of O’Rahilly  were used to determine the Carnegie stage of development. In total, 19 embryos representing a gradual progression of intestinal development were reconstructed (Table 1). In addition, we studied other serially sectioned embryos of the LUMC and AMC collections that were not reconstructed. Finally, we compared our reconstructions with the reconstructions in the historic reports of Mall , Frazer & Robins , and Pernkopf [11, 12, 31]. Brain development , and the return of the physiological hernia between 9.0 and 9.5 weeks of development [46, 47] were used to estimate the age of the embryos after Carnegie stage 23. Specimens of 8–10 weeks development will also be referred to as embryos.
Image acquisition and processing
The embryos that were reconstructed are shown in Table 1. Digitized images of serial sections of DREM embryos are directly available via the Virtual Human Embryo project [48, 49]. Serial sections of the embryos from the AMC and LUMC collections were digitized at high resolution with an Olympus BX51 scanning microscope and dotSlide software (Olympus, Zoeterwoude, the Netherlands). Resized JPEG images were converted to grey-scale images with Photoshop CS5. The image resizing factor was kept minimal to preserve detail and correlated with embryo size (Table 1).
The 3D reconstructions were generated with Amira™ (version 5.5; base package; FEI Visualization Sciences Group Europe, Mérignac Cédex, France). Serial sections were first aligned automatically with the least-squares method and then manually adjusted to account for curvature and rotation of the body axis with the help of photographic, MRI and ultrasound images of age-matched embryos ; Aligned slices were resampled into the Amira mesh-file format. The intestine, mesentery, vessels and reference structures were segmented manually based on histologically identifiable contours. The outer muscular layer was used to delineate the esophagus and stomach, and the serosal layer of the intestine was used to delineate the intestinal tract to the transition of the hindgut from an intra- to a retroperitoneal position. Somites, intersegmental arteries, spinal ganglia, and vertebral bodies were used as landmarks for segmental levels.
To describe the precise topographic position of structures, landmarks such as somites, vertebrae, spinal ganglia, and intersegmental arteries were identified. The exact somite level was deduced from the position of the 7th intersegmental artery (future subclavian artery) located between somites 10 and 11 [51–53]. Once vertebral development begins, the 7th intersegmental artery is found in the loose zone of somite 11 and no longer between somites. As such, segments 1–7 correspond to C1-7, segments 8–19 to Th1-12, and segments 20–24 to L1-5.
Polygon meshes were created from the segmented labels and exported to Cinema 4D (MAXON Computer GmbH, Friedrichsdorf, Germany). The meshes for the mesentery were optimized using deformers and sculpting, whereas the intestine and vessels were modeled with Bezier curves. All structures were modeled proportionally and scaled as indicated. Intestinal length was measured in Cinema4D by assessment of the spline length of the Bezier curves. The Cinema 4D files formed the basis for three-dimensional interactive PDFs .
The data set(s) supporting the results of this article is (are) included within the article (and its Additional file 1).
Crown Rump Length
Inferior mesenteric artery
Superior mesenteric artery
Superior mesenteric artery
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The authors wish to thank Maurice van den Hoff (AMC), Marco de Ruiter (LUMC) and John Cork (DREM project) for allowing us to use their institutional series of human embryos. Special thanks go to Jaco Hagoort (University of Amsterdam), Els Terwindt and Jack Cleutjens (Maastricht University) for their technical assistance. The financial support of ‘Stichting Rijp’ is gratefully acknowledged.
The authors declare that they have no competing interests.
JHMS performed data acquisition, generated the 3D models and drafted the manuscript. JPJMH and HKM created additional reconstructions to substantiate the description of landmark structures. WHL and LK conceived of the study, and participated in its design and coordination and helped to draft the manuscript. All authors read and approved the final manuscript.
Supplemental Figures. 3D PDF CS14, CS16, CS20, CS23, and 9.0 and 9.5 WKS. Interactive 3D PDFs are provided for CS14, CS16, CS20, CS23, and 9.0 and 9.5 WKS. See the supplement “3D PDF operation manual” for instructions how to use the interactive PDF tools. The color codes correspond to those used in the Figures (Legend Table). (PDF 394 kb)
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Soffers, J.H., Hikspoors, J.P., Mekonen, H.K. et al. The growth pattern of the human intestine and its mesentery. BMC Dev Biol 15, 31 (2015). https://doi.org/10.1186/s12861-015-0081-x
- Short Bowel Syndrome
- Primary Loop
- Secondary Loop
- Intestinal Development
- Intestinal Tube