You are in: eMedicine Specialties > Radiology > GASTROINTESTINAL Hiatal HerniaArticle Last Updated: Sep 8, 2005AUTHOR AND EDITOR INFORMATIONAuthor: Ali Nawaz Khan, MBBS, FRCS, FRCP, FRCR, LRCP, Chairman of Medical Imaging, Professor of Radiology, NGHA, King Fahad National Guard Hospital, King Abdulaziz Medical City, Riyadh, Saudi Arabia Ali Nawaz Khan is a member of the following medical societies: American Institute of Ultrasound in Medicine, Radiological Society of North America, Royal College of Physicians, Royal College of Physicians and Surgeons of the United States, Royal College of Radiologists, and Royal College of Surgeons of England Coauthor(s): Muthusamy Chandramohan, MBBS, DMRD, FRCR, Special Registrar, Department of Radiology, Manchester Radiology; Sumaira MacDonald, MBChB, PhD, MRCP, FRCR, Lecturer, Sheffield University Medical School; Endovascular Fellow, Sheffield Vascular Institute Editors: Neela Lamki, MD, Professor, Department of Radiology, Sultan Qaboos University, Oman; Adjunct Professor, Department of Radiology, Baylor College of Medicine; Bernard D Coombs, MB, ChB, PhD, Consulting Staff, Department of Specialist Rehabilitation Services, Hutt Valley District Health Board, New Zealand; David Andrew Nicholson, BM, BS, FRCR, Honorary Lecturer, Department of Radiology, University of Manchester; Consultant Gastrointestinal Radiologist, Department of Radiology, Hope Hospital, Salford Royal Hospital NHS Trust; Robert M Krasny, MD, Consulting Staff, Department of Radiology, The Angeles Clinic and Research Institute; Eugene C Lin, MD, Consulting Staff, Department of Radiology, Virginia Mason Medical Center Author and Editor Disclosure Synonyms and related keywords: sliding hiatal hernia, axial hernia, concentric hernia, paraesophageal hernia, rolling hiatal hernia, parahiatal hernia, congenital hernia, hiatus hernia, acquired hernia, congenital hernia, gastroesophageal reflux, volvulus, diaphragmatic hernia, Barrett esophagus INTRODUCTIONBackgroundEmbryologic development of the diaphragm is complex, and a number of defects allow a variety of congenital hernias through the diaphragm. A hernia may occur through a congenitally large esophageal hiatus; however, acquired hernias through the esophageal hiatus are more common. These hernias are classified either as sliding or paraesophageal. Approximately 99% of hiatal hernias are sliding, and the remaining 1% are paraesophageal. Although paraesophageal hernias are uncommon, they are potentially life threatening because of the risk of volvulus and incarceration. Incidence of a hiatal hernia increases with age. When the lower esophageal sphincter is located within the thorax, its reinforcement of the diaphragmatic crus is loosened and allows gastroesophageal reflux of acid contents; such reflux may be symptomatic in one quarter of patients because of reflux esophagitis. For excellent patient education resources, visit eMedicine's Esophagus, Stomach, and Intestine Center. Also, see eMedicine's patient education article Hiatal Hernia. PathophysiologyThe phrenicoesophageal membrane normally surrounds the lower esophagus and fixes it to the diaphragm, thereby preventing gastric herniation through the esophageal hiatus into the thorax. When the phrenicoesophageal membrane is deficient, an axial gastric herniation may develop in the thoracic cavity. The stomach may be totally intrathoracic. This condition is usually related to a defect in the central tendon of the diaphragm rather than to herniation through the esophageal hiatus. The stomach acquires a position behind the heart as a result of a slight volvulus in its transverse axis. The cardia of the stomach is usually within the thorax, but occasionally, it may lie below the diaphragm. The gastric curvature may lie on the right or the left. With a paraesophageal hernia, part of the stomach herniates through a defect in the phrenicoesophageal membrane into the thorax, while the gastric cardia remains in the normal intra-abdominal position. The herniated portion of the stomach is usually anterior to the esophagus; the hernia is frequently nonreducible. In such cases, epigastric discomfort and, occasionally, dysphagia may occur; however, no reflux symptoms are evident because the cardiac mechanism is not disturbed. Occasionally, a gastric ulcer on the lesser curve may be associated at the level of the diaphragmatic hiatus. A distinct subgroup of paraesophageal hernias occurs in a younger age group and appears to be secondary to a congenital defect. These hernias are characteristically situated to the right of the lower thoracic esophagus where a part of the gastric fundus herniates into the thorax. A congenitally short esophagus, which is not a true hernia and is exceptionally rare, may mimic a hiatal hernia. Gastric ectopy is responsible for this condition, in which the esophagus is short and straight and a segment of the stomach is intrathoracic; the segment may be round or cylindrical with large sinuous folds. The gastric intrathoracic segment is nonreducible and remains in the thorax with the patient in both the erect and the supine positions. Often, a circular narrowing occurs at the intrathoracic junction; this finding is commonly associated with gastroesophageal ulcer. When the lower esophageal sphincter is located within the thorax, its reinforcement of the diaphragmatic crus is loosened. On its own, the lower esophageal sphincter is not sufficiently strong to prevent the reflux of gastric contents into the lower esophagus. Gastroesophageal reflux disease is a common finding in patients with hiatal hernia; however, most patients with hiatal hernia do not have gastroesophageal disease. Occasionally, differentiating a normal ampulla of the distal esophagus from a small hiatal hernia may be difficult. The most ideal way of localizing the lower esophageal sphincter is by manometry, which is performed by monitoring pressure changes between the abdominal and thoracic cavities during breathing. Hiatal hernia is associated with esophagitis in 20% of patients; duodenal ulcer, in another 20%; diverticulosis, in 25%; and gallstones, in 18%. In a small series, an association between asplenia syndrome and a hiatal hernia has been described. Symptoms in patients with hiatal hernia may be multifactorial. Barrett esophagus consists of columnar epithelium lining the esophagus. It is an acquired condition related to chronic gastroesophageal reflux. These patients can develop an ulcer, stricture, or malignancy. An associated hiatal hernia is common. Adenocarcinoma represents the most serious complication of Barrett esophagus. In patients with Barrett esophagus, the risk of esophageal carcinoma is 30-40 times higher than that of the general population. FrequencyUnited StatesThe incidence of hiatal hernia increases significantly with age, and it occurs in 10% of the adult population. Sliding hiatal hernias are common. Paraesophageal hernias are rare. InternationalThe international frequency is the same as found in the United States. Mortality/Morbidity
RaceNo racial predilection is recognized. SexWomen are affected more frequently than men. AgeMost hiatal hernias occur in patients older than 40 years. The incidence increases with age. AnatomyThe diaphragm is a dome-shaped septum dividing the thoracic from the abdominal cavity. The diaphragm is composed of 2 parts: a peripheral muscular part and the central fibrous tendinous aponeurosis to which it attaches. The central aponeurosis is trefoil shaped and is partially attached to the undersurface of the pericardium. The peripheral muscular part is arranged into 3 groups of muscle fibers: (1) the vertebral fibers arising from the crura and arcuate ligaments, (2) the costal fibers arising from the inner aspects of the lower 6 ribs and the costal cartilages, and (3) the sternal fibers arising from the deep surface of the sternum. The right crus of the diaphragm arises from the anterior aspects of the bodies of the first 3 lumbar vertebral bodies and the associated intervertebral discs. The left crus is attached to the first 2 lumbar vertebral bodies and the intervertebral disks. The arcuate ligaments comprise a series of fibrous arches. The medial arch is formed by thickening of the fascia covering the major psoas muscle, while the lateral arch represents the fascia covering the quadratus lumborum muscle. The median arcuate ligament is formed by the medial fibrous borders of the 2 crura and is placed on the anterior surface of the aorta. In the diaphragm, 3 main openings are identified as follows: The aortic opening transmits the aorta, the thoracic duct and, often, the azygos vein. The esophageal opening is located between the muscular fibers of the right diaphragmatic crus and transmits the esophagus, the vagi, and branches of the left gastric artery and vein. The opening of the inferior vena cava (IVC) is located within the central aponeurosis, which transmits the IVC and the right phrenic nerve. Embryologic development of the diaphragm is complex, and as a result, several defects may occur, giving rise to a variety of congenital hernias. These hernias include the following: (1) herniation of upper abdominal contents through the canal of Morgagni, which is positioned anteriorly between the xiphoid and the costal margins; (2) herniation through the posteriorly located pleuroperitoneal canal (Bochdalek foramen); (3) herniation through a deficient central tendon; and (4) herniation through a congenitally large esophageal hiatus. Herniation through the central tendon may occasionally be traumatic. In particular, it may be caused by steering-column injuries sustained in motor vehicle accidents. Clinical DetailsMost hiatal hernias are found incidentally and usually are discovered on routine chest radiographs or CT scans performed for unrelated symptoms. When symptomatic, patients may experience heartburn, dyspepsia, or epigastric pain. Rarely, the patient may present with recurrent chest infections due to aspiration of gastric contents. A paraesophageal or, rarely, a sliding hiatal hernia may present acutely due to a volvulus or strangulation. Paraesophageal hernias are particularly likely to incarcerate and cause symptoms of intermittent epigastric pain. Barrett esophagus is commonly associated with hiatal hernia and may present with reflux symptoms or dysphagia. Sliding hiatal hernias are common. The clinical significance of a sliding hiatal hernia is uncertain. Most patients with a sliding hiatal hernia do not have gastroesophageal reflux, but reflux esophagitis is found more commonly in patients who have a hiatal hernia than in those who do not. Paraesophageal hernias are rare but can be potentially life threatening because of the risk of volvulus and incarceration. Strangulation of the stomach may occur but is rare. Symptoms associated with a hiatal hernia may be multifactorial and may be related to gallstone disease; peptic ulcer disease; esophagitis; or, rarely, a carcinoma developing within a hiatal hernia. Recurrent chest infections may be due to aspiration of gastric contents from esophageal reflux; this rarely occurs in elderly patients. Preferred ExaminationPlain chest radiographs may demonstrate a retrocardiac gas-filled structure. An upper GI barium series is the preferred examination in the investigation of suggested hiatal hernia and its sequelae. CT scans are useful when more precise cross-sectional anatomic localization is desired. The use of MRI and radionuclide studies is anecdotal. Ultrasonography is a sensitive means of diagnosis of gastroesophageal reflux and is particularly attractive in young patients because it is noninvasive and does not require the use of ionizing radiation. Limitations of TechniquesFindings in an upper GI barium series may be specific, although images may fail to demonstrate a small sliding hiatal hernia. Since gastroesophageal reflux may be intermittent, its presence may be overlooked. When no gas is present within the hernia, differentiating hernias from other retrocardiac masses may be difficult at times. Diagnosis of a hiatal hernia is not always straightforward by using sonography, and an intermittent hernia is likely to be missed, although some regard sonography as the examination of choice in infants because the findings may differentiate duodenal causes of vomiting from esophageal causes. DIFFERENTIALSGanglioglioma
| |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Media file 1: Diagram shows the 3 major orifices at the inferior aspect of the diaphragm (inferior vena cava [IVC], esophagus, aorta). | |
![]() | View Full Size Image | Media type: Image |
| Media file 2: Diagram shows a sliding hiatal hernia. The gastroesophageal junction (Jn) is located above the diaphragmatic hiatus. | |
![]() | View Full Size Image | Media type: Image |
| Media file 3: Diagram of a paraesophageal hiatal hernia shows the normal infradiaphragmatic location of the gastroesophageal junction. | |
![]() | View Full Size Image | Media type: Image |
| Media file 4: Plain chest radiograph shows a well-defined, rounded, soft-tissue mass in the retrocardiac region consistent with a sliding hiatal hernia. | |
![]() | View Full Size Image | Media type: Image |
| Media file 5: Frontal chest radiograph in a patient with a large hiatal hernia demonstrates a retrocardiac opacity with radiolucent gas, which shifts the mediastinum to the right. | |
![]() | View Full Size Image | Media type: X-RAY |
| Media file 6: Lateral chest radiograph shows a hiatal hernia (same patient as in Image 5). Note the absence of fundal gas below the left hemidiaphragm. | |
![]() | View Full Size Image | Media type: X-RAY |
| Media file 7: Barium-meal examination in a patient with a sliding hiatal hernia demonstrates the supradiaphragmatic location of the gastroesophageal junction. | |
![]() | View Full Size Image | Media type: X-RAY |
| Media file 8: Frontal chest radiograph in a 75-year-old woman with a hiatal hernia demonstrates an air-fluid level. | |
![]() | View Full Size Image | Media type: X-RAY |
| Media file 9: Axial CT scan of the thorax in a 75-year-old woman shows a retrocardiac mediastinal mass with a fluid level due to a hiatal hernia (same patient as in Image 8). | |
![]() | View Full Size Image | Media type: CT |
| Media file 10: Chest radiograph in a patient with a huge air-filled hiatal hernia, which appears as a mediastinal mass. | |
![]() | View Full Size Image | Media type: X-RAY |
| Media file 11: Abdominal radiograph in a patient with a huge air-filled hiatal hernia (same patient as in Image 10). Radiograph obtained on the day after Image 10 was obtained shows acute gastric dilatation due to incarcerated hiatal hernia. | |
![]() | View Full Size Image | Media type: X-RAY |
Article Last Updated: Sep 8, 2005