Indirect inguinal hernia

Last revised by Craig Hacking on 21 Feb 2024

Indirect inguinal hernias (alternative plural: herniae), a type of groin herniation, are the most common type of abdominal hernia.

It is five times more common than a direct inguinal hernia, and is seven times more frequent in males, due to the persistence of the processus vaginalis during testicular descent. 

In children, the vast majority of inguinal hernias are indirect. 

Many are longstanding and asymptomatic, although the sheer size can become burdensome.

Indirect inguinal hernias arise lateral and superior to the course of the inferior epigastric vessels, lateral to Hesselbach's triangle, and then protrude through the deep (internal) inguinal ring into the inguinal canal. The hernial sac and content often pass inferomedially within the canal to emerge via the superficial inguinal ring.

Contents may include mesenteric fat (most common), peritoneal fluid, small bowel loops, mobile colon segments (sigmoid, cecum, appendix).

On imaging, consider:

  • direct inguinal hernia

    • emerges medially to the inferior epigastric vessels and above the inguinal ligament

    • the inguinal canal is usually compressed/displaced ("lateral crescent sign")

  • femoral hernia

    • exit below the inguinal ligament and caudal to the emergence of the inferior epigastric vessels

On testicular ultrasound, one could consider spermatic cord lipoma on the differential if an inguinal hernia contains only omental fat. Movement of the fat with the Valsalva maneuver is more likely an indirect hernia.

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