Microplastics Alter the Properties and Sinking Rates of Zooplankton Faecal Pellets

Plastic debris is a widespread contaminant, prevalent in aquatic ecosystems across the globe. Zooplankton readily ingest microscopic plastic (microplastic, < 1 mm), which are later egested within their faecal pellets. These pellets are a source of food for marine organisms, and contribute to the oceanic vertical flux of particulate organic matter as part of the biological pump. The effects of microplastics on faecal pellet properties are currently unknown. Here we test the hypotheses that (1) faecal pellets are a vector for transport of microplastics, (2) polystyrene microplastics can alter the properties and sinking rates of zooplankton egests and, (3) faecal pellets can facilitate the transfer of plastics to coprophagous biota. Following exposure to 20.6 μm polystyrene microplastics (1000 microplastics mL–1) and natural prey (∼1650 algae mL–1) the copepod Calanus helgolandicus egested faecal pellets with significantly (P < 0.001) reduced densities, a 2.25-fold reduction in sinking rates, and a higher propensity for fragmentation. We further show that microplastics, encapsulated within egests of the copepod Centropages typicus, could be transferred to C. helgolandicus via coprophagy. Our results support the proposal that sinking faecal matter represents a mechanism by which floating plastics can be vertically transported away from surface waters.

COVALENT LIPOPROTEIN(A) ASSEMBLY: Characterization of Oxidase Activity Responsible for Catalyzing Covalent Lipoprotein(a) Assembly

Lipoprotein(a) (Lp(a)) has been identified as an emerging risk factor for the development of vascular diseases. The Lp(a) particle is assembled in a 2-step process upon secretion of the LDL and apo(a) components from hepatocytes. Work done by the Koschinsky group has identified an oxidase-like activity present in the conditioned medium (CM) harvested from human hepatoma (HepG2), as well as HEK 293 (human endothelian kidney) cells that catalyzes the rate of covalent Lp(a) formation. We have taken a candidate enzyme approach to identifying this oxidase activity. Specifically, we have proposed that the QSOX (Quiescin/sulfhydryl oxidase) is responsible for catalysis of covalent Lp(a) assembly. An oxidase activity assay developed by Dr. Thorpe (University of Delaware) was used to detect QSOX1 in CM harvested from cultured cell lines that catalyze covalent Lp(a) assembly. In addition, the QSOX1 transcript was identified in each cell line and quantified with the use of Real-Time RT-PCR. Quantitative assays of covalent Lp(a) assembly were performed to study some characteristics of the unkwown oxidase activity. First, conditioned medium was dialyzed through a 5 kDa cutoff, as this has previously been shown to reduce the aforementioned oxidase activity. Purified QSOX was then added back to the reaction and the rate of catalysis was observed. The addition of QSOX appeared to enhance the rate of covalent Lp(a) assembly in a dose-dependent manner. Additional covalent Lp(a) assembly assays were performed where various chemicals were added to determine whether Lp(a) assembly was affected. The addition of EDTA did not affect covalent assembly, suggesting that the oxidase activity may not be metallo-dependent. Moreover, dose-dependent addition of Calcium, DTT, Copper and glutathione to dialyzed medium also did not affect the rate of Lp(a) assembly. Taken together, these studies will aid in identifying the nature of the oxidase activity that catalyzes covalent Lp(a) assembly. This will provide us with valuable information on how Lp(a) particles are assembled, and may lead to the development of drugs inhibiting Lp(a) formation.

Chemical abundances and winds of massive stars in M31: a B-type supergiant and a WC star in OB 10

We present high quality spectroscopic data for two massive stars in the OB 10 association of M31, OB 10-64 (B0 la) and OB 10-WRI (WC6). Medium resolution spectra of both stars were obtained using the ISIS spectrograph on the William Herschel Telescope. This is supplemented with Hubble Space Telescope STIS UV spectroscopy and Keck I HIRES data for OB 10-64. A non- local thermodynamic equilibrium (LTE) model atmosphere and abundance analysis for OB 10-64 is presented, indicating that this star has similar photospheric CNO, Mg and Si abundances to solar neighbourhood massive stars. A wind analysis of this early B-type supergiant reveals a mass-loss rate of (M)over dot = 1.6 x 10(-6) M-circle dot yr(-1), and v(infinity) = 1650 km s(-1). The corresponding wind momentum is in good agreement with the wind momentum-luminosity relationship found for Galactic early-B supergiants. Observations of OB 10-WRI are analysed using a non-LTE, line-blanketed code, to reveal approximate stellar parameters of log L/L-circle dot similar to 5.7, T-* - 75 kK, v(infinity) similar to 3000 km s(-1), (M)over dot/(M-circle dot yr(-1)) similar to 10(-4.3) adopting a clumped wind with a filling factor of 10 per cent. Quantitative comparisons are made with the Galactic WC6 star HD 92809 (WR23) revealing that OB 10-WR1 is 0.4 dex more luminous, though it has a much lower C/He ratio (similar to0.1 versus 0.3 for HD 92809). Our study represents the first detailed, chemical model atmosphere analysis for either a B-type supergiant or a Wolf- Rayet (WR) star in Andromeda, and shows the potential of how such studies can provide new information on the chemical evolution of galaxies and the evolution of massive stars in the local Universe.

Behavior of the heterogeneous electron-transfer rate constants of arenes and substituted anthracenes in room-temperature ionic liquids

We report the anodic oxidation of several arenes and anthracenes within room-temperature ionic liquids (RTILs). In particular, the heterogeneous electron-transfer rates (k(0)) for substituted anthracenes and arenes are also investigated in 1-ethyl-3-methylimidazolium bis(trifluoromethylsulfonyl)imide ([C(2)mim][NTf2]) and found not to obey the outer-sphere Marcus-type behavior of these compounds in contrast to the behavior in traditional organic solvents,in particular the predictions for k(0) with molecular size and solvent static dielectric constant. To obtain the electron-transfer rate for 9-phenylanthracene, the dimerization and heterogeneous electron-transfer kinetics of its electrogenerated radical cations is studied in [C(2)mim][NTf2] and eight other RTILs and are both found to be largely independent of the solution viscosity.