Effects of selection for ethanol preference on gene expression in the nucleus accumbens of HS‐CC mice

Previous studies on changes in murine brain gene expression associated with the selection for ethanol preference have used F₂ intercross or heterogeneous stock (HS) founders, derived from standard laboratory strains. However, these populations represent only a small proportion of the genetic variance available in Mus musculus. To investigate a wider range of genetic diversity, we selected mice for ethanol preference using an HS derived from the eight strains of the collaborative cross. These HS mice were selectively bred (four generations) for high and low ethanol preference. The nucleus accumbens shell of naive S₄ mice was interrogated using RNA sequencing (RNA‐Seq). Gene networks were constructed using the weighted gene coexpression network analysis assessing both coexpression and cosplicing. Selection targeted one of the network coexpression modules (greenyellow) that was significantly enriched in genes associated with receptor signaling activity including Chrna7, Grin2a, Htr2a and Oprd1. Connectivity in the module as measured by changes in the hub nodes was significantly reduced in the low preference line. Of particular interest was the observation that selection had marked effects on a large number of cell adhesion molecules, including cadherins and protocadherins. In addition, the coexpression data showed that selection had marked effects on long non‐coding RNA hub nodes. Analysis of the cosplicing network data showed a significant effect of selection on a large cluster of Ras GTPase‐binding genes including Cdkl5, Cyfip1, Ndrg1, Sod1 and Stxbp5. These data in part support the earlier observation that preference is linked to Ras/Mapk pathways.     

Localization of Pyrophosphatase and V-ATPase in Chlamydomonas reinhardtii

Microsomal membranes of Chlamydomonas reinhardtii possess PPase and V-ATPase activities. By immunogold labelling we have shown that H⁺-pyrophosphatase (PPase) is localized to membranes of lytic and contractile vacuoles of Chlamydomonas, in which the density of antigen in the latter is much higher. In addition, PPase is conspicuously present in trans cisternae and transpole elements of the Colgi apparatus. Such a distribution for PPase has hitherto not been reported. A positive in situ identification for PPase at the plasma membrane, including the flagellar membrane, was also made, and has also been confirmed by Western blotting and activity measurements on isolated plasma membranes. V-ATPase antisera which cross react with polypeptides of this transport complex from maize roots failed to recognize anything in Western blots of Chlamydomonas microsomal membranes. Thus immunogold labelling for V-ATPase was not possible with Chlamydomonas. On the other hand, surfaces of contractile vacuole membranes as revealed by deepetching were covered by conspicuous 9 ? 11.5 nm diameter smooth particles which had a central hole. These were very similar to those previously identified by Heuser et al., (1993) as the V,-head of V-ATPase in Dictyostelium contractile vacuoles. Another type of membrane image, designated “intermediate-sized vesicle”, was found associated with the contractile vacuole. It was characterized by densely-packed 6 ? 7.5nm diameter polygonal particles, which upon rotation analysis showed both 5- and 6-fold symmetries, also with a central hole. These particles are interpreted as representing either PPase complexes or the V₀ body of the V-ATPase in etched fractured membrane surfaces. We have incorporated these findings into a model of contractile vacuole function.     

The role of cometary particle Coalescence in chemical evolution

Important prebiotic organic compounds might have been transported to Earth in dust or produced in vapor clouds resulting from atmospheric explosions or impacts of comets. These compounds coalesced in the upper atmosphere with particles ejected from craters formed by impacts of large objects. Coalescence during exposure to UV radiation concentrated organic monomers and enhanced formation of oligomers. Continuing coalescence added material to the growing particles and shielded prebiotic compounds from prolonged UV radiation. These particles settled into the lower atmosphere where they were scavenged by rain. Aqueous chemistry and evaporation of raindrops containing nomomers in high temperature regions near the Earth's surface also promoted continued formation of oligomers. Finally, these oligomers were deposited in the oceans where continued prebiotic evolution led to the most primitive cell. Results of our studies suggest that prebiotic chemical evolution may be an inevitable consequence of impacting comets during the late accretion of planets anywhere in the universe if oceans remained on those planetary surfaces.     

Thinking of biology: asteroid impacts, microbes, and the cooling of the atmosphere

The authors examine the cooling of the Earth's surface from 3.75 to 1 billion years ago. Three effects of the bombardment of Earth by asteroids and comets that may have delayed surface cooling include time to form continents, volatilization of carbonate rocks which released carbon dioxide into the atmosphere, and inability of microbes to inhabit land masses during large impact events. Continental microbes may have helped reduce high temperatures from 3.75 to 3.5 billion years ago. If so, the evolutionary sequence of microbes is proposed to be anaerobic heterotrophs, chemoautotrophs, and then photoautotrophs.     

Crystal Structure of Ripk4 Reveals Dimerization-Dependent Kinase Activity

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Estimates of the maximum time required to originate life

Fossils of the oldest microorganisms exist in 3.5 billion year old rocks and there is indirect evidence that life may have existed 3.8 billion years ago (3.8 Ga). Impacts able to destroy life or interrupt prebiotic chemistry may have occurred after 3.5 Ga. If large impactors vaporized the oceans, sterilized the planets, and interfered with the origination of life, life must have originated in the time interval between these impacts which increased with geologic time. Therefore, the maximum time required for the origination of life is the time that occurred between sterilizing impacts just before 3.8 Ga or 3.5 Ga, depending upon when life first appeared on Earth. If life first originated 3.5 Ga, and impacts with kinetic energies between 2×10³⁴ and 2×10³⁵ were able to vaporize the oceans, using the most probable impact flux, we find that the maximum time required to originate life would have been 67 to 133 million years (My). If life first originated 3.8 Ga, the maximum time to originate life was 2.5 to 11 My. Using a more conservative estimate for the flux of impacting objects before 3.8 Ga, we find a maximum time of 25 My for the same range of impactor kinetic energies. The impact model suggests that it is possible that life may have originated more than once.     

Comet impacts and chemical evolution on the bombarded Earth

Amino acids yields for previously published shock tube experiments are used with minimum Cretaceous-Tertiary (K/T) impactor mass and comet composition to predict AIB amino acid K/T boundary sediment column density. The inferred initial concentration of all amino acids in the K/T sea and in similar primordial seas just after 10 km comet impacts would have been at least 10^–7 M. However, sinks for amino acids must also be considered in calculating amino acid concentrations after comet impacts and in assessing the contribution of comets to the origin of life. The changing concentration of cometary amino acids due to ultraviolet light is compared with the equilibrium concentration of amino acids produced in the sea from corona discharge in the atmosphere, deposition in water, and degradation by ultraviolet light. Comets could have been more important than endogenous agents for initial evolution of amino acids. Sites favorable for chemical evolution of amino acids are examined and it is concluded that chemical evolution could have occurred at or above the surface even during periods of intense bombardment of Earth before 3.8 billion years ago.