Planets in Mean-Motion Resonances and the System Around HD45364

In some planetary systems, the orbital periods of two of its members present a commensurability, usually known by mean-motion resonance. These resonances greatly enhance the mutual gravitational influence of the planets. As a consequence, these systems present uncommon behaviors, and their motions need to be studied with specific methods. Some features are unique and allow us a better understanding and characterization of these systems. Moreover, mean-motion resonances are a result of an early migration of the orbits in an accretion disk, so it is possible to derive constraints on their formation. Here we review the dynamics of a pair of resonant planets and explain how their orbits evolve in time. We apply our results to the HD 45365 planetary system.Comment: invited review, 17 pages, 6 figure

The consequences of niche and physiological differentiation of archaeal and bacterial ammonia oxidisers for nitrous oxide emissions

The authors are members of the Nitrous Oxide Research Alliance (NORA), a Marie Skłodowska-Curie ITN and research project under the EU's seventh framework program (FP7). GN is funded by the AXA Research Fund and CGR by a Royal Society University Research Fellowship (UF150571) and a Natural Environment Research Council (NERC) Standard Grant (NE/K016342/1). The authors would like to thank Dr Robin Walker and the SRUC Craibstone Estate (Aberdeen) for access to the agricultural plots, Dr Alex Douglas for statistical advice and Philipp Schleusner for assisting microcosm construction and sampling.Peer reviewedPublisher PD

Alternative Splicing Regulation During C. elegans Development: Splicing Factors as Regulated Targets

Alternative splicing generates protein diversity and allows for post-transcriptional gene regulation. Estimates suggest that 10% of the genes in Caenorhabditis elegans undergo alternative splicing. We constructed a splicing-sensitive microarray to detect alternative splicing for 352 cassette exons and tested for changes in alternative splicing of these genes during development. We found that the microarray data predicted that 62/352 (∼18%) of the alternative splicing events studied show a strong change in the relative levels of the spliced isoforms (>4-fold) during development. Confirmation of the microarray data by RT-PCR was obtained for 70% of randomly selected genes tested. Among the genes with the most developmentally regulated alternatively splicing was the hnRNP F/H splicing factor homolog, W02D3.11 – now named hrpf-1. For the cassette exon of hrpf-1, the inclusion isoform comprises 65% of hrpf-1 steady state messages in embryos but only 0.1% in the first larval stage. This dramatic change in the alternative splicing of an alternative splicing factor suggests a complex cascade of splicing regulation during development. We analyzed splicing in embryos from a strain with a mutation in the splicing factor sym-2, another hnRNP F/H homolog. We found that approximately half of the genes with large alternative splicing changes between the embryo and L1 stages are regulated by sym-2 in embryos. An analysis of the role of nonsense-mediated decay in regulating steady-state alternative mRNA isoforms was performed. We found that 8% of the 352 events studied have alternative isoforms whose relative steady-state levels in embryos change more than 4-fold in a nonsense-mediated decay mutant, including hrpf-1. Strikingly, 53% of these alternative splicing events that are affected by NMD in our experiment are not obvious substrates for NMD based on the presence of premature termination codons. This suggests that the targeting of splicing factors by NMD may have downstream effects on alternative splicing regulation

Cryptomare magmatism 4.35 Gyr ago recorded in lunar meteorite Kalahari 009

The origin and evolution of the Moon remain controversial 1,2, with one of the most important questions for lunar evolution being the timing and duration of basaltic (mare) magmatism1,3–8. 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 4.3560.15 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 type10–12, we conclude that Kalahari 009 is our first sample of a very-low-Ti cryptomare from the Moon

Analysis of Transcription Complexes and Effects of Ligands by Microelectrospray Ionization Mass Spectrometry

The human vitamin D receptor (VDR) and retinoid X receptor-alpha (RXRalpha) modulate gene activity by forming homodimeric or heterodimeric complexes with specific DNA sequences and interaction with other elements of the transcriptional apparatus in the presence of their known endogenous ligands 1alpha,25-dihydroxyvitamin D3 (1, 25-[OH]2D3) and 9-cis-retinoic acid (9-c-RA). We used rapid buffer exchange gel filtration in conjunction with microelectrospray ionization mass spectrometry (microESI-MS) to study the binding of these receptors to the osteopontin vitamin D response element (OP VDRE). In the absence of DNA, both VDR and RXRalpha existed primarily as monomers, but in the presence of OP VDRE, homodimeric RXRalpha and heterodimeric RXRalpha-VDR complexes were shown to bind OP VDRE. Addition of 9-c-RA increased RXRalpha homodimer-OP VDRE complexes, and addition of 1,25-(OH) 2D3 resulted in formation of 1, 25-(OH)2D 3-VDR-RXRalpha-OP VDRE complexes. Addition of low-affinity binding ligands had no detectable effect on the VDR-RXRalpha-OP VDRE transcription complex. These results demonstrate the utility of microESI-MS in analyzing multimeric, high-molecular-weight protein-protein and protein-DNA complexes, and the effects of ligands on these transcriptional complexes

Planets in mean-motion resonances and the system around HD45364

In some planetary systems, the orbital periods of two of its members present a commensurability, usually known by mean-motion resonance. These resonances greatly enhance the mutual gravitational influence of the planets. As a consequence, these systems present uncommon behaviors, and their motions need to be studied with specific methods. Some features are unique and allow us a better understanding and characterization of these systems. Moreover, mean-motion resonances are a result of an early migration of the orbits in an accretion disk, so it is possible to derive constraints on their formation. Here we review the dynamics of a pair of resonant planets and explain how their orbits evolve in time. We apply our results to the HD 45365 planetary system.publishe