Foraging for Meaning: Harvesting Wild Plants as the Basis for an Ecological Worldview

Redeveloping a meaningful connection between people and the Earth may serve to heighten our ecological awareness, foster environmental values, and promote a more sustainable cultural worldview. Various environmental literatures, such as Deep Ecology, have suggested this, but seldom provide specific strategies for practical application. The present study seeks to address this gap by providing a concrete strategy for fostering an improved relationship between people and planet. Foraging, the collection and harvest of wild plant foods, was explored as one potential avenue for establishing a meaningful reconnection to nature, which could serve to shift our cultural values toward preservation rather than destruction of the biosphere. The modern era is characterized not only by ecological disconnection, but social and psychological rifts as well. In our individualistic, deracinated society, we strive to find meaning through wealth, status, and consumer culture; this phenomenon serves to undermine our planetary support system by promoting unsustainable levels of energy and resource throughput. In order to maintain the planet as a suitable home for ourselves, future generations, and other life forms, we must strive to enact a new worldview based upon ecological values which are equally capable of meeting our psychological needs for meaning. However, mainstream environmental messages have failed to promote the necessary paradigmatic societal shifts. Renewable energy and hybrid vehicles, for example, cannot substantially alter the course of our society; instead, we must address the problematic aspects of our core cultural values, particularly the dualistic notion of humans as separate from nature, which is considered a root of modern environmental problems. Interviews and surveys were conducted with foragers at two wild food weekend events in the United States, in order to characterize this understudied population and to determine how foraging might promote a heightened ecological conscience. The data analysis revealed that foragers experience a sense of connection with the Earth, which is built through deep observation and direct interaction with surrounding ecosystems; consuming food produced by nature provides the ultimate connection between people and land. An awareness of and connection to the natural world, built upon direct experience, contributes to a sense of ecological belonging; by re-envisioning humanity’s role in nature, foragers are able to reject and move beyond the modern dualism which typically prevents a fully embedded conception of people as part of nature. By redefining this relationship, foraging allows for an understanding of the value of land and our complete dependence upon it, encouraging values of care and protection. Foragers also described this connection with the Earth as having spiritual qualities; finding meaning within nature indicates the possibility for meeting psychological needs in an ecologically benign manner, and provides hope for an ecological worldview. Based on these findings, further research is recommended to determine how involvement in foraging might impact those who are ambivalent toward nature and lack ecological values. If foraging is found to be impactful for the general population, then it seems likely that promoting this activity on a larger scale could contribute to a positive shift toward a collective ecological conscience and should be encouraged, in a sustainable manner, as a new form of environmental message

Use of Ultrasound Measurements to Direct Laparoscopic Pyloromyotomy in Infants

Preoperative ultrasound measurement of pyloric length to determine laparoscopic pyloromyotomy appears to minimize the risk of incomplete pyloromyotomy

The chlorine isotopic composition of the Moon: Insights from melt inclusions

The Moon exhibits a heavier chlorine (Cl) isotopic composition compared to the Earth. Several hypotheses have been put forward to explain this difference, based mostly on analyses of apatite in lunar samples complemented by bulk-rock data. The earliest hypothesis argued for Cl isotope fractionation during the degassing of anhydrous basaltic magmas on the Moon. Subsequently, other hypotheses emerged linking Cl isotope fractionation on the Moon with the degassing during the crystallization of the Lunar Magma Ocean (LMO). Currently, a variant of the LMO degassing model involving mixing between two end-member components, defined by early-formed cumulates, from which mare magmas were subsequently derived, and a KREEP component, which formed towards the end of the LMO crystallization, seems to reconcile some existing Cl isotope data on lunar samples. To further ascertain the history of Cl in the Moon and to investigate any evolution of Cl during magma crystallization and emplacement events, which could help resolve the chlorine isotopic variation between the Earth and the Moon, we analysed the Cl abundance and its isotopic composition in 36 olivine- and pyroxene-hosted melt inclusions (MI) in five Apollo basalts (10020, 12004, 12040, 14072 and 15016). Olivine-hosted MI have an average of 3.3 ± 1.4 ppm Cl. Higher Cl abundances (11.9 ppm on average) are measured for pyroxene-hosted MI, consistent with their formation at later stages in the crystallization of their parental melt compared to olivines. Chlorine isotopic composition (δ37) of MI in the five Apollo basalts have weighted averages of +12 ± 2.4‰ and +10.1 ± 3.2‰ for olivine- and pyroxene-hosted MI, respectively, which are statistically indistinguishable. These isotopic compositions are also similar to those measured in apatite in these lunar basalts, with the exception of sample 14072, which is known to have a distinct petrogenetic history compared to other mare basalts. Based on our dataset, we conclude that, post-MI-entrapment, no significant Cl isotopic fractionation occurred during the crystallization and subsequent eruption of the parent magma and that Cl isotopic composition of MI and apatite primarily reflect the signature of the source region of these lunar basalts. Our findings are compatible with the hypothesis that in the majority of the cases the heavy Cl isotopic signature of the Moon was acquired during the earliest stages of LMO evolution. Interestingly, MI data from 14072 suggests that Apollo 14 lunar basalts might be an exception and may have experienced post-crystallization processes, possibly metasomatism, resulting in additional Cl isotopic fractionation recorded by apatite but not melt inclusions

Effects of shock and Martian alteration on Tissint hydrogen isotope ratios and water content

publisher: Elsevier articletitle: Effects of shock and Martian alteration on Tissint hydrogen isotope ratios and water content journaltitle: Geochimica et Cosmochimica Acta articlelink: http://dx.doi.org/10.1016/j.gca.2016.12.035 content_type: article copyright: © 2017 The Authors. Published by Elsevier Ltd.© 2017 The Authors. Published by Elsevier Ltd. This is an open access article, available to all readers online, published under a creative commons licensing (https://creativecommons.org/licenses/by/4.0/). The attached file is the published version of the article

CO2 wettability of seal and reservoir rocks and the implications for carbon geo-sequestration

We review the literature data published on the topic of CO2 wettability of storage and seal rocks. We first introduce the concept of wettability and explain why it is important in the context of carbon geo-sequestration (CGS) projects, and review how it is measured. This is done to raise awareness of this parameter in the CGS community, which, as we show later on in this text, may have a dramatic impact on structural and residual trapping of CO2. These two trapping mechanisms would be severely and negatively affected in case of CO2-wet storage and/or seal rock. Overall, at the current state of the art, a substantial amount of work has been completed, and we find that: 1. Sandstone and limestone, plus pure minerals such as quartz, calcite, feldspar, and mica are strongly water wet in a CO2-water system. 2. Oil-wet limestone, oil-wet quartz, or coal is intermediate wet or CO2 wet in a CO2-water system. 3. The contact angle alone is insufficient for predicting capillary pressures in reservoir or seal rocks. 4. The current contact angle data have a large uncertainty. 5. Solid theoretical understanding on a molecular level of rock-CO2-brine interactions is currently limited. 6. In an ideal scenario, all seal and storage rocks in CGS formations are tested for their CO2 wettability. 7. Achieving representative subsurface conditions (especially in terms of the rock surface) in the laboratory is of key importance but also very challenging

Amphibole and apatite insights into the evolution and mass balance of Cl and S in magmas associated with porphyry copper deposits

Chlorine and sulfur are of paramount importance for supporting the transport and deposition of ore metals at magmatic–hydrothermal systems such as the Coroccohuayco Fe–Cu–Au porphyry–skarn deposit, Peru. Here, we used recent partitioning models to determine the Cl and S concentration of the melts from the Coroccohuayco magmatic suite using apatite and amphibole chemical analyses. The pre-mineralization gabbrodiorite complex hosts S-poor apatite, while the syn- and post-ore dacitic porphyries host S-rich apatite. Our apatite data on the Coroccohuayco magmatic suite are consistent with an increasing oxygen fugacity (from the gabbrodiorite complex to the porphyries) causing the dominant sulfur species to shift from S2− to S6+ at upper crustal pressure where the magmas were emplaced. We suggest that this change in sulfur speciation could have favored S degassing, rather than its sequestration in magmatic sulfides. Using available partitioning models for apatite from the porphyries, pre-degassing S melt concentration was 20–200 ppm. Estimates of absolute magmatic Cl concentrations using amphibole and apatite gave highly contrasting results. Cl melt concentrations obtained from apatite (0.60 wt% for the gabbrodiorite complex; 0.2–0.3 wt% for the porphyries) seems much more reasonable than those obtained from amphibole which are very low (0.37 wt% for the gabbrodiorite complex; 0.10 wt% for the porphyries). In turn, relative variations of the Cl melt concentrations obtained from amphibole during magma cooling are compatible with previous petrological constraints on the Coroccohuayco magmatic suite. This confirms that the gabbrodioritic magma was initially fluid undersaturated upon emplacement, and that magmatic fluid exsolution of the gabbrodiorite and the pluton rooting the porphyry stocks and dikes were emplaced and degassed at 100–200 MPa. Finally, mass balance constraints on S, Cu and Cl were used to estimate the minimum volume of magma required to form the Coroccohuayco deposit. These three estimates are remarkably consistent among each other (ca. 100 km3) and suggest that the Cl melt concentration is at least as critical as that of Cu and S to form an economic mineralization