The Promoter Region of the Adiponectin Gene Is a Determinant in Modulating Insulin Sensitivity in Childhood Obesity
We investigated the association of the −11,391G>A, −11,377G>C, +45T>G, and +276G>T adiponectin single‐nucleotide polymorphisms (SNPs) and expected haplotypes with the insulin resistance (IR) state in overweight/obese children; by using the haplotype background analysis, we also assessed...
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Veröffentlicht in: | Obesity (Silver Spring, Md.) Md.), 2006-09, Vol.14 (9), p.1498-1504 |
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Zusammenfassung: | We investigated the association of the −11,391G>A, −11,377G>C, +45T>G, and +276G>T adiponectin single‐nucleotide polymorphisms (SNPs) and expected haplotypes with the insulin resistance (IR) state in overweight/obese children; by using the haplotype background analysis, we also assessed the effect of each SNP independently. GG genotype at the −11,391 locus was associated with higher fasting insulin levels and homeostasis model assessment‐IR index and lower adiponectin levels compared with GA + AA genotypes (p = 0.01, 0.002, and 0.03, respectively). Those heterozygous and homozygous for G allele at the −11,377 locus showed higher fasting glucose (p = 0.001 for both), fasting insulin (p = 0.001 for both), homeostasis model assessment‐IR index (p < 0.001 for both), and triglyceride levels (p = 0.02 and 0.03, respectively) and lower adiponectin levels (p = 0.002 and 0.02, respectively) compared with C homozygotes. The +45G carriers showed higher fasting and 2‐hour glucose levels (p = 0.01 for both) and lower adiponectin levels (p = 0.02) compared with non‐carriers. Haplotype analysis suggested that, considering the same haplotypic background, each of the three polymorphisms exerted an independent effect on investigated parameters. The −11,391G>A, −11,377C>G, and +45T>G SNPs are associated with IR syndrome in overweight/obese children; they independently influence the investigated variables. The effect of +45T>G SNP seems to be marginal compared with the promoter SNPs. The GGT haplotype is associated with the highest degree of IR. |
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ISSN: | 1930-7381 1930-739X |
DOI: | 10.1038/oby.2006.172 |