Membranes by the Numbers

Many of the most important processes in cells take place on and across membranes. With the rise of an impressive array of powerful quantitative methods for characterizing these membranes, it is an opportune time to reflect on the structure and function of membranes from the point of view of biological numeracy. To that end, in this article, I review the quantitative parameters that characterize the mechanical, electrical and transport properties of membranes and carry out a number of corresponding order of magnitude estimates that help us understand the values of those parameters.Comment: 27 pages, 12 figure

Multi-messenger observations of a binary neutron star merger

On 2017 August 17 a binary neutron star coalescence candidate (later designated GW170817) with merger time 12:41:04 UTC was observed through gravitational waves by the Advanced LIGO and Advanced Virgo detectors. The Fermi Gamma-ray Burst Monitor independently detected a gamma-ray burst (GRB 170817A) with a time delay of ~1.7 s with respect to the merger time. From the gravitational-wave signal, the source was initially localized to a sky region of 31 deg2 at a luminosity distance of 40+8-8 Mpc and with component masses consistent with neutron stars. The component masses were later measured to be in the range 0.86 to 2.26 Mo. An extensive observing campaign was launched across the electromagnetic spectrum leading to the discovery of a bright optical transient (SSS17a, now with the IAU identification of AT 2017gfo) in NGC 4993 (at ~40 Mpc) less than 11 hours after the merger by the One- Meter, Two Hemisphere (1M2H) team using the 1 m Swope Telescope. The optical transient was independently detected by multiple teams within an hour. Subsequent observations targeted the object and its environment. Early ultraviolet observations revealed a blue transient that faded within 48 hours. Optical and infrared observations showed a redward evolution over ~10 days. Following early non-detections, X-ray and radio emission were discovered at the transient’s position ~9 and ~16 days, respectively, after the merger. Both the X-ray and radio emission likely arise from a physical process that is distinct from the one that generates the UV/optical/near-infrared emission. No ultra-high-energy gamma-rays and no neutrino candidates consistent with the source were found in follow-up searches. These observations support the hypothesis that GW170817 was produced by the merger of two neutron stars in NGC4993 followed by a short gamma-ray burst (GRB 170817A) and a kilonova/macronova powered by the radioactive decay of r-process nuclei synthesized in the ejecta

Vibrio cholerae interactions with the gastrointestinal tract: lessons from animal studies.

Vibrio cholerae is a curved Gram-negative rod that causes the diarrheal disease cholera. One hundred and twenty five years of study of V. cholerae microbiology have made this lethal pathogen arguably the most well-understood non-invasive mucosal pathogen. Over the past 25 years, modern molecular techniques have permitted the identification of many genes and cellular processes that are critical for V. cholerae colonization of the gastrointestinal tract. Review of the literature reveals that there are two classes of genes that influence V. cholerae colonization of the suckling mouse intestine, the most commonly used animal model to study V. cholerae pathogenesis. Inactivation of one class of genes results in profound attenuation of V. cholerae intestinal colonization, whereas inactivation of the other class of genes results in only moderate colonization defects. The latter class of genes suggests that V. cholerae may colonize several intestinal niches that impose distinct requirements and biological challenges, thus raising the possibility that there is physiologic heterogeneity among the infecting population. Efficient V. cholerae intestinal colonization and subsequent dissemination to the environment appears to require temporally ordered expression of sets of genes during the course of infection. Key challenges for future investigations of V. cholerae pathogenicity will be to assess the degree of heterogeneity in the infecting population, whether such heterogeneity has functional significance, and if stochastic processes contribute to generation of heterogeneity in vivo