Mitochondrial leucine tRNA level and PTCD1 are regulated in response to leucine starvation

Pentatricopeptide repeat domain protein 1 (PTCD1) is a novel human protein that was recently shown to decrease the levels of mitochondrial leucine tRNAs. The physiological role of this regulation, however, remains unclear. Here we show that amino acid starvation by leucine deprivation significantly increased the mRNA steady-state levels of PTCD1 in human hepatocarcinoma (HepG2) cells. Amino acid starvation also increased the mitochondrially encoded leucine tRNA (tRNA(Leu(CUN))) and the mRNA for the mitochondrial leucyl-tRNA synthetase (LARS2). Despite increased PTCD1 mRNA steady-state levels, amino acid starvation decreased PTCD1 on the protein level. Decreasing PTCD1 protein concentration increases the stability of the mitochondrial leucine tRNAs, tRNA(Leu(CUN)) and tRNA(Leu(UUR)) as could be shown by RNAi experiments against PTCD1. Therefore, it is likely that decreased PTCD1 protein contributes to the increased tRNA(Leu(CUN)) levels in amino acid-starved cells. The stabilisation of the mitochondrial leucine tRNAs and the upregulation of the mitochondrial leucyl-tRNA synthetase LARS2 might play a role in adaptation of mitochondria to amino acid starvation.

Local Interstellar Medium: Six Years of Direct Sampling by IBEX

The Interstellar Boundary Explorer (IBEX) has been directly observing neutral atoms from the local interstellar medium for the last six years (2009–2014). This paper ties together the 14 studies in this Astrophysical Journal Supplement Series Special Issue, which collectively describe the IBEX interstellar neutral results from this epoch and provide a number of other relevant theoretical and observational results. Interstellar neutrals interact with each other and with the ionized portion of the interstellar population in the “pristine” interstellar medium ahead of the heliosphere. Then, in the heliosphereʼs close vicinity, the interstellar medium begins to interact with escaping heliospheric neutrals. In this study, we compare the results from two major analysis approaches led by IBEX groups in New Hampshire and Warsaw. We also directly address the question of the distance upstream to the pristine interstellar medium and adjust both sets of results to a common distance of ~1000 AU. The two analysis approaches are quite different, but yield fully consistent measurements of the interstellar He flow properties, further validating our findings. While detailed error bars are given for both approaches, we recommend that for most purposes, the community use “working values” of ~25.4 km s⁻¹, ~75°7 ecliptic inflow longitude, ~−5°1 ecliptic inflow latitude, and ~7500 K temperature at ~1000 AU upstream. Finally, we briefly address future opportunities for even better interstellar neutral observations to be provided by the Interstellar Mapping and Acceleration Probe mission, which was recommended as the next major Heliophysics mission by the NRCʼs 2013 Decadal Survey.