In vivo modulation of Hmgic reduces obesity

The HMGI family of proteins consists of three members, HMGIC, HMGI and HMGI(Y), that function as architectural factors and are essential components of the enhancesome. HMGIC is predominantly expressed in proliferating, undifferentiated mesenchymal cells and is not detected in adult tissues. It is disrupted and misexpressed in a number of mesenchymal tumour cell types, including fat-cell tumours (lipomas). In addition Hmgic-/- mice have a deficiency in fat tissue. To study its role in adipogenesis and obesity, we examined Hmgic expression in the adipose tissue of adult, obese mice. Mice with a partial or complete deficiency of Hmgic resisted diet-induced obesity. Disruption of Hmgic caused a reduction in the obesity induced by leptin deficiency (Lepob/Lepob) in a gene-dose-dependent manner. Our studies implicate a role for HMGIC in fat-cell proliferation, indicating that it may be an adipose-specific target for the treatment of obesity.     

Cryptomare magmatism 4.35 Gyr ago recorded in lunar meteorite Kalahari 009

The origin and evolution of the Moon remain controversial, with one of the most important questions for lunar evolution being the timing and duration of basaltic (mare) magmatism. Here we report the result of ion microprobe U-Pb dating of phosphates in a lunar meteorite, Kalahari 009, which is classified as a very-low-Ti mare-basalt breccia. In situ analyses of five phosphate grains, associated with basaltic clasts, give an age of 4.35 +/- 0.15 billion years. These ancient phosphate ages are thought to represent the crystallization ages of parental basalt magma, making Kalahari 009 one of the oldest known mare basalts. We suggest that mare basalt volcanism on the Moon started as early as 4.35 Gyr ago, relatively soon after its formation and differentiation, and preceding the bulk of lunar volcanism which ensued after the late heavy bombardment around 3.8-3.9 Gyr (refs 7 and 8). Considering the extremely low abundances of incompatible elements such as thorium and the rare earth elements in Kalahari 009 (ref. 9) and recent remote-sensing observations illustrating that the cryptomaria tend to be of very-low-Ti basalt type, we conclude that Kalahari 009 is our first sample of a very-low-Ti cryptomare from the Moon.