ABSTRACT
Studies1,2 have shown that the remnants of destroyed planets and debris-disk planetesimals can survive the volatile evolution of their host stars into white dwarfs3,4, but few intact planetary bodies around white dwarfs have been detected5-8. Simulations predict9-11 that planets in Jupiter-like orbits around stars of â²8 Mâ (solar mass) avoid being destroyed by the strong tidal forces of their stellar host, but as yet, there has been no observational confirmation of such a survivor. Here we report the non-detection of a main-sequence lens star in the microlensing event MOA-2010-BLG-477Lb12 using near-infrared observations from the Keck Observatory. We determine that this system contains a 0.53 ± 0.11 Mâ white-dwarf host orbited by a 1.4 ± 0.3 Jupiter-mass planet with a separation on the plane of the sky of 2.8 ± 0.5 astronomical units, which implies a semi-major axis larger than this. This system is evidence that planets around white dwarfs can survive the giant and asymptotic giant phases of their host's evolution, and supports the prediction that more than half of white dwarfs have Jovian planetary companions13. Located at approximately 2.0 kiloparsecs towards the centre of our Galaxy, it is likely to represent an analogue to the end stages of the Sun and Jupiter in our own Solar System.
ABSTRACT
Growth retardation induced by dietary restriction in the lamb results in a low GnRH pulse frequency, and thus, puberty is delayed. In our experimental model, in which ovariectomized lambs are maintained at weaning weight (approximately 20 kg BW), hypothalamic GnRH is present and releasable, suggesting that central mechanisms limit the release of GnRH during chronic growth restriction. Our study compared the number and distribution of GnRH-containing neurons in growth-restricted (n = 5) and rapidly growing (n = 5) ovariectomized prepubertal female lambs at 24 weeks of age (normal age of puberty is about 30 weeks). Immunoreactive cells were labeled using LR-1 antiserum (R. Benoit) and an avidin-biotin-immunoperoxidase procedure. GnRH neurons were localized in 60-micron coronal sections from the level of the diagonal band of Broca to the mammillary bodies. The estimated total number of GnRH neurons in the growth-restricted and rapidly growing lambs was similar (3364.8 +/- 513.8 vs. 3151.2 +/- 279.8, respectively). In addition, the percent distributions of GnRH neurons in the diagonal band of Broca, the anterior hypothalamus, the lateral hypothalamus, and the posterior hypothalamus were not different. A trend (P = 0.07) toward a smaller percent distribution in the preoptic area was noted in growth-restricted lambs (30.6 +/- 3.6) compared to rapidly growing lambs (44.0 +/- 5.2). By contrast, the percent distribution of GnRH neurons in the medial basal hypothalamus was significantly greater in the growth-restricted lambs compared with the rapidly growing lambs (17.7 +/- 2.2 vs. 6.7 +/- 1.4, respectively; P < 0.005). It is of interest that the percent distribution of GnRH-containing neurons in the medial basal hypothalamus of the hypogonadotropic growth-restricted lamb is similar to that observed in the fetal lamb, whereas the eugonadotropic rapidly growing lamb is more similar to the adult female. In this context, decreased GnRH secretion and delayed puberty during diet-induced growth restriction may arise from alterations in the GnRH neurosecretory system.
