Development, Health and Disease Research Program, University of California, Irvine, CA, USA.
Department of Biomedical Engineering, University of California, Irvine, CA, USA.
Int J Obes (Lond). 2017 Sep;41(9):1434-1439. doi: 10.1038/ijo.2017.114. Epub 2017 May 10.
The importance of energy homeostasis brain circuitry in the context of obesity is well established, however, the developmental ontogeny of this circuitry in humans is currently unknown. Here, we investigate the prospective association between newborn gray matter (GM) volume in the insula, a key brain region underlying energy homeostasis, and change in percent body fat accrual over the first six months of postnatal life, an outcome that represents among the most reliable infant predictors of childhood obesity risk.
A total of 52 infants (29 male, 23 female, gestational age at birth=39(1.5) weeks) were assessed using structural MRI shortly after birth (postnatal age at MRI scan=25.9(12.2) days), and serial Dual X-Ray Absorptiometry shortly after birth (postnatal age at DXA scan 1=24.6(11.4) days) and at six months of age (postnatal age at DXA scan 2=26.7(3.3) weeks).
Insula GM volume was inversely associated with change in percent body fat from birth to six-months postnatal age and accounted for 19% of its variance (β=-3.6%/S.D., P=0.001). This association was driven by the central-posterior portion of the insula, a region of particular importance for gustation and interoception. The direction of this effect is in concordance with observations in adults, and the results remained statistically significant after adjusting for relevant covariates and potential confounding variables.
Altogether, these findings suggest an underlying neural basis of childhood obesity that precedes the influence of the postnatal environment. The identification of plausible brain-related biomarkers of childhood obesity risk that predate the influence of the postnatal obesogenic environment may contribute to an improved understanding of propensity for obesity, early identification of at-risk individuals, and intervention targets for primary prevention.
能量平衡脑回路在肥胖中的重要性已得到充分证实,然而,人类这种回路的发育发生尚不清楚。在这里,我们研究了新生儿大脑岛状体内灰质量(GM)体积与出生后前六个月体脂肪百分比变化之间的前瞻性关联,这是代表儿童肥胖风险的最可靠婴儿预测因素之一。
共有 52 名婴儿(29 名男性,23 名女性,出生时的胎龄=39(1.5)周)在出生后不久(MRI 扫描时的出生后年龄=25.9(12.2)天)接受了结构 MRI 评估,并在出生后不久(DXA 扫描 1 时的出生后年龄=24.6(11.4)天)和六个月大时(DXA 扫描 2 时的出生后年龄=26.7(3.3)周)进行了连续双能 X 射线吸收法测量。
岛状体内 GM 体积与出生至六个月大时体脂肪百分比的变化呈负相关,占其方差的 19%(β=-3.6%/S.D.,P=0.001)。这种关联是由岛状体内的中央后部分驱动的,该部分对于味觉和内脏感觉尤为重要。这种效应的方向与成年人的观察结果一致,并且在调整了相关协变量和潜在混杂变量后,结果仍然具有统计学意义。
总之,这些发现表明了儿童肥胖的潜在神经基础,这先于出生后环境的影响。识别出可能与儿童肥胖风险相关的脑生物标志物,这些标志物先于出生后肥胖环境的影响,可能有助于更好地理解肥胖倾向、早期识别高危个体以及为一级预防确定干预靶点。