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Pituitary volume in children with growth hormone deficiency, idiopathic short stature and controls
Insights
Pediatric patients with isolated growth hormone deficiency (IGHD) show reduced pituitary volume (PV). Idiopathic short stature (ISS) patients have intermediate PV, suggesting potential chronic growth hormone secretion issues. MRI-based PV measurement aids diagnosis.
Area of Science:
- Pediatric Endocrinology
- Radiology
- Growth Disorders
Background:
- Pituitary volume (PV) assessment is crucial for diagnosing growth disorders in children.
- Distinguishing between isolated growth hormone deficiency (IGHD) and idiopathic short stature (ISS) can be challenging.
Purpose of the Study:
- To characterize and compare pituitary volume (PV) in pediatric patients with IGHD, ISS, and healthy controls.
- To evaluate the utility of PV measurements in diagnosing growth hormone-related conditions.
Main Methods:
- Three-dimensional (3D) contrast-enhanced magnetic resonance imaging (MRI) was used to measure pituitary volume.
- Study included 69 IGHD patients, 29 ISS patients, and 66 age-matched controls.
Main Results:
- Significant differences in mean PV were observed across the three groups (p<0.001).
- IGHD patients exhibited the smallest mean PV (230.8 mm³), followed by ISS patients (286.8 mm³), and controls (343.7 mm³).
- PV increased with age in ISS patients and controls, but showed minimal increase in IGHD patients.
Conclusions:
- Reduced pituitary volume is characteristic of IGHD and intermediate in ISS.
- Diminished chronic growth hormone secretion may contribute to short stature in some ISS patients.
- MRI-determined PV can aid in the diagnostic evaluation of children with growth problems.
Background:
The objective of the study was to describe the pituitary volume (PV) in pediatric patients with isolated growth hormone deficiency (IGHD), idiopathic short stature (ISS) and normal controls.
Methods:
Sixty-nine patients (57 male, 12 female), with a mean age of 11.9 (±2.0), were determined to have IGHD. ISS was identified in 29 patients (20 male, 9 female), with a mean age of 12.7 (±3.7). Sixty-six controls (28 female, 38 male), mean age 9.8 (±4.7) were also included. Three-dimensional (3D) magnetic resonance images with contrast were obtained to accurately measure PV.
Results:
There was a significant difference in the mean PV among the three groups. The IGHD patients had a mean PV 230.8 (±89.6), for ISS patients it was 286.8 (±108.2) and for controls it was 343.7 (±145.9) (p<0.001). There was a normal increase in PV with age in the ISS patients and controls, but a minimal increase in the IGHD patients.
Conclusions:
Those patients with isolated GHD have the greatest reduction in PV compared to controls and the patients with ISS fall in between. We speculate that a possible cause for the slowed growth in some ISS patients might be related to diminished chronic secretion of growth hormone over time, albeit having adequate pituitary reserves to respond acutely to GH stimulation. Thus, what was called neurosecretory GHD in the past, might, in some patients, be relative pituitary hypoplasia and resultant diminished growth hormone secretion. Thus, PV determinations by magnetic resonance imaging (MRI) could assist in the diagnostic evaluation of the slowly growing child.
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