The power of synthetic biology for bioproduction, remediation and pollution control

The agenda of the UN's Sustainable Development Goals (SDGs) 1 challenges the synthetic biology community—and the life sciences as a whole—to develop transformative technologies that help to protect, even expand our planet's habitability. While modern tools for genome editing already benefit applications in health and agriculture, sustainability also asks for a dramatic transformation of our use of natural resources. The challenge is not just to limit and, wherever possible revert emissions of pollutants and greenhouse gases, but also to replace environmentally costly processes based on fossil fuels with bio‐based sustainable alternatives. This task is not exclusively a scientific and technical one but will also require guidelines and regulations for the development and large‐scale deployment of this new type of bio‐based production. Some recent advances that can (or soon could) enable us to make progress in these areas—and several possible governance principles—need to be addressed

Latest Miocene restriction of the Mediterranean Outflow Water:a perspective from the Gulf of Cádiz

The Mediterranean-Atlantic water mass exchange provides the ideal setting for deciphering the role of gateway evolution in ocean circulation. However, the dynamics of Mediterranean Outflow Water (MOW) during the closure of the Late Miocene Mediterranean-Atlantic gateways are poorly understood. Here, we define the sedimentary evolution of Neogene basins from the Gulf of Cádiz to the West Iberian margin to investigate MOW circulation during the latest Miocene. Seismic interpretation highlights a middle to upper Messinian seismic unit of transparent facies, whose base predates the onset of the Messinian salinity crisis (MSC). Its facies and distribution imply a predominantly hemipelagic environment along the Atlantic margins, suggesting an absence or intermittence of MOW preceding evaporite precipitation in the Mediterranean, simultaneous to progressive gateway restriction. The removal of MOW from the Mediterranean-Atlantic water mass exchange reorganized the Atlantic water masses and is correlated to a severe weakening of the Atlantic Meridional Overturning Circulation (AMOC) and a period of further cooling in the North Atlantic during the latest Miocene

Short-Lived Trace Gases in the Surface Ocean and the Atmosphere

The two-way exchange of trace gases between the ocean and the atmosphere is important for both the chemistry and physics of the atmosphere and the biogeochemistry of the oceans, including the global cycling of elements. Here we review these exchanges and their importance for a range of gases whose lifetimes are generally short compared to the main greenhouse gases and which are, in most cases, more reactive than them. Gases considered include sulphur and related compounds, organohalogens, non-methane hydrocarbons, ozone, ammonia and related compounds, hydrogen and carbon monoxide. Finally, we stress the interactivity of the system, the importance of process understanding for modeling, the need for more extensive field measurements and their better seasonal coverage, the importance of inter-calibration exercises and finally the need to show the importance of air-sea exchanges for global cycling and how the field fits into the broader context of Earth System Science

First M87 Event Horizon Telescope results: VIII. Magnetic field structure near the Event Horizon

Instrumentatio

Polarimetric Properties of Event Horizon Telescope Targets from ALMA

We present the results from a full polarization study carried out with the Atacama Large Millimeter/submillimeter Array (ALMA) during the first Very Long Baseline Interferometry (VLBI) campaign, which was conducted in 2017 April in the lambda 3 mm and lambda 1.3 mm bands, in concert with the Global mm-VLBI Array (GMVA) and the Event Horizon Telescope (EHT), respectively. We determine the polarization and Faraday properties of all VLBI targets, including Sgr A*, M87, and a dozen radio-loud active galactic nuclei (AGNs), in the two bands at several epochs in a time window of 10 days. We detect high linear polarization fractions (2%-15%) and large rotation measures (RM > 10(3.3)-10(5.5) rad m(-2)), confirming the trends of previous AGN studies at millimeter wavelengths. We find that blazars are more strongly polarized than other AGNs in the sample, while exhibiting (on average) order-of-magnitude lower RM values, consistent with the AGN viewing angle unification scheme. For Sgr A* we report a mean RM of (-4.2 0.3) x 10(5) rad m(-2) at 1.3 mm, consistent with measurements over the past decade and, for the first time, an RM of (-2.1 0.1) x 10(5) rad m(-2) at 3 mm, suggesting that about half of the Faraday rotation at 1.3 mm may occur between the 3 mm photosphere and the 1.3 mm source. We also report the first unambiguous measurement of RM toward the M87 nucleus at millimeter wavelengths, which undergoes significant changes in magnitude and sign reversals on a one year timescale, spanning the range from -1.2 to 0.3 x 10(5) rad m(-2) at 3 mm and -4.1 to 1.5 x 10(5) rad m(-2) at 1.3 mm. Given this time variability, we argue that, unlike the case of Sgr A*, the RM in M87 does not provide an accurate estimate of the mass accretion rate onto the black hole. We put forward a two-component model, comprised of a variable compact region and a static extended region, that can simultaneously explain the polarimetric properties observed by both the EHT (on horizon scales) and ALMA (which observes the combined emission from both components). These measurements provide critical constraints for the calibration, analysis, and interpretation of simultaneously obtained VLBI data with the EHT and GMVA

Resolving the Inner Parsec of the Blazar J1924-2914 with the Event Horizon Telescope

The blazar J1924-2914 is a primary Event Horizon Telescope (EHT) calibrator for the Galactic center's black hole Sagittarius A*. Here we present the first total and linearly polarized intensity images of this source obtained with the unprecedented 20 mu as resolution of the EHT. J1924-2914 is a very compact flat-spectrum radio source with strong optical variability and polarization. In April 2017 the source was observed quasi-simultaneously with the EHT (April 5-11), the Global Millimeter VLBI Array (April 3), and the Very Long Baseline Array (April 28), giving a novel view of the source at four observing frequencies, 230, 86, 8.7, and 2.3 GHz. These observations probe jet properties from the subparsec to 100 pc scales. We combine the multifrequency images of J1924-2914 to study the source morphology. We find that the jet exhibits a characteristic bending, with a gradual clockwise rotation of the jet projected position angle of about 90 degrees between 2.3 and 230 GHz. Linearly polarized intensity images of J1924-2914 with the extremely fine resolution of the EHT provide evidence for ordered toroidal magnetic fields in the blazar compact core

Coupling carboxylic acid reductase to inorganic pyrophosphatase enhances cell-free in vitro aldehyde biosynthesis

© 2015 Elsevier B.V. Carboxylic acid reductases (CARs) have been harnessed in metabolic pathways to produce aldehydes in engineered organisms. However, desired aldehyde products inhibit cell growth and limit product titers currently achievable from fermentative processes. Aldehyde toxicity can be entirely circumvented by performing aldehyde biosynthesis in non-cellular systems. Use of purified CARs for preparative-scale aldehyde synthesis has been limited by in vitro turnover of model CARs, such as Car. Ni from Nocardia iowensis, despite robust conversion of substrates associated with expression in heterologous hosts such as E. coli and yeast. In this study, we report that in vitro activity of Car. Ni is inhibited by formation of the co-product pyrophosphate, and that pairing of an inorganic pyrophosphatase (Ppa. Ec) with Car. Ni substantially improves the rate and yield of aldehyde biosynthesis. We demonstrate that, in the presence of Ppa. Ec, Michaelis-Menten kinetic models based on initial rate measurements accurately predict Car. Ni kinetics within an in vitro pathway over longer timescales. We rationalize our novel observations for Car. Ni by examining previously posed arguments for pyrophosphate hydrolysis made in the context of other adenylate-forming enzymes. Overall, our findings may aid in increasing adoption of CARs for cell-free in vitro aldehyde biosynthetic processes

A Robust CRISPR Interference Gene Repression System in Pseudomonas

© 2018 American Society for Microbiology. Pseudomonas spp. are widely used model organisms in different areas of research. Despite the relevance of Pseudomonas in many applications, the use of protein depletion tools in this host remains limited. Here, we developed the CRISPR interference system for gene repression in Pseudomonas spp. using a nuclease-null Streptococcus pasteurianus Cas9 variant (dead Cas9, or dCas9). We demonstrate a robust and titratable gene depletion system with up to 100-fold repression in β-galactosidase activity in P. aeruginosa and 300-fold repression in pyoverdine production in Pseudomonas putida. This inducible system enables the study of essential genes, as shown by ftsZ depletions in P. aeruginosa, P. putida, and Pseudomonas fluorescens that led to phenotypic changes consistent with depletion of the targeted gene. Additionally, we performed the first in vivo characterization of protospacer adjacent motif (PAM) site preferences of S. pasteurianus dCas9 and identified NNGCGA as a functional PAM site that resulted in repression efficiencies comparable to the consensus NNGTGA sequence. This discovery significantly expands the potential genomic targets of S. pasteurianus dCas9, especially in GC-rich organisms