Internal hernia

Last revised by Konrad Schultz on 7 May 2023

Internal hernias (alternative plural: herniae) are protrusions of the viscera through the peritoneum or mesentery but remaining within the abdominal cavity.

Internal hernias have a low incidence of <1% and represent a relatively small proportion, up to 5.8%, of presentations with small bowel obstruction 1.

The most common presentation is an acute obstruction of small bowel loops that develops through normal or abnormal apertures.

Internal hernias not infrequently self-resolve, making imaging at the time of symptomatology vital.

The orifice that the small bowel herniates through is usually a pre-existing anatomic structure, such as foramina, recesses, and fossae (e.g. fossa of Landzert).

Pathologic defects of the mesentery and visceral peritoneum, such as from congenital maldevelopment of the mesenteries, and surgery also create potential internal herniation orifices. 

In contemporary practice, virtually all patients undergo CT, which is the gold standard imaging modality for assessment of bowel obstruction and suspected internal hernias. Traditionally barium studies were performed and may still on occasion be used in niche circumstances.

The appearance depends on the particular internal hernia. Common features include:

  • encapsulation of distended bowel loops within an abnormal location

  • arrangement or crowding of small bowel loops within a hernial sac

  • evidence of obstruction with segmental dilatation and stasis

  • mesenteric vessel abnormalities

    • engorgement, crowding, twisting, stretching of mesenteric vessels

The appearances on barium studies vary depending on the type and site of the internal hernia:

  • clustering of small bowel loops

  • distended bowel proximal to the site of obstruction

  • abnormal site or displacement of normal parts of the gastrointestinal tract

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