Ultra High Resolution Transmission Electron Microscopy of Matrix Mineral Grains in CM Chondrites: Preaccretionary or Parent Body Aqueous Processing?

CM chondrites are highly hydrated meteorites associated with a parent asteroid that has experienced significant aqueous processing. The meteoritic evidence indicates that these non-differentiated asteroids are formed by fine-grained minerals embedded in a nanometric matrix that preserves chemical clues of the forming environment. So far there are two hypothesis to explain the presence of hydrated minerals in the content of CM chondrites: one is based on textural features in chondrule-rim boundaries [1-3], and the other ‘preaccretionary’ hypothesis proposes the incorporation of hydrated phases from the protoplanetary disk [4-6]. The highly porous structure of these chondrites is inherited from the diverse materials present in the protoplanetary disk environment. These bodies were presumably formed by low relative velocity encounters that led to the accretion of silicate-rich chondrules, refractory Ca- and Al-rich inclusions (CAIs), metal grains, and the fine-grained materials forming the matrix. Owing to the presence of significant terrestrial water in meteorite finds [7], here we have focused on two CM chondrite falls with minimal terrestrial processing: Murchison and Cold Bokkeveld. Anhydrous carbonaceous chondrite matrices are usually represented by highly chemically unequilibrated samples that contain distinguishable stellar grains. Other chondrites have experienced hydration and chemical homogeneization that reveal parent body processes. We have studied CM chondrites because these meteorites have experienced variable hydration levels [8-10]. It is important to study the textural effects of aqueous alteration in the main minerals to decipher which steps and environments promote bulk chemistry changes, and create the distinctive alteration products. It is thought that aqueous alteration has particularly played a key role in modifying primordial bulk chemistry, and homogenizing the isotopic content of fine-grained matrix materials [7, 11, 12]. Fortunately, the mineralogy produced by parent-body and terrestrial aqueous alteration processes is distinctive [5, 11]

Ancient Martian Floods in a Plausible Variable Climatic Environment as Revealed from the Sequential Growth of Allan Hills 84001 Carbonate Globules

No abstract available

THE KNOWLEDGE BASED BIO-ECONOMY AT WORK: FROM LARGE SCALE EXPERIENCES TO INSTRUMENTS FOR RURAL AND LOCAL DEVELOPMENT

N° ISBN - 978-2-7380-1284-5International audienceThe new bio-economy is increasingly seen as a workable alternative to move today's economies in the direction of more sustainable natural resource use and economic growth. Most of existing experiences, both from science as well as from implementation of the Knowledge Based Bio-Economy (KBBE) concepts, refer to relatively strong science basis and relatively large scales of application. This paper proposes to review existing advances in the implementation of the KBBE in small scale situations and identify what the key research, institutional and policy issues that need to be taken into account to further promote KBBE approaches to rural and local development. As such, the analytical approach used includes an extensive literature review in the form of a desk study, followed by a comparative analysis and the formulation of recommendations regarding S&T and policy agendas

The 2011 October Draconids Outburst. II. Meteoroid Chemical Abundances from Fireball Spectroscopy

On October 8, 2011 the Earth crossed dust trails ejected from comet 21P/Giacobini-Zinner in the late 19th and early 20th Century. This gave rise to an outburst in the activity of the October Draconid meteor shower, and an international team was organized to analyze this event. The SPanish Meteor Network (SPMN) joined this initiative and recorded the October Draconids by means of low light level CCD cameras. In addition, spectroscopic observations were carried out. Tens of multi-station meteor trails were recorded, including an extraordinarily bright October Draconid fireball (absolute mag. -10.5) that was simultaneously imaged from three SPMN meteor ob-serving stations located in Andalusia. Its spectrum was obtained, showing a clear evolution in the relative intensity of emission lines as the fireball penetrated deeper into the atmosphere. Here we focus on the analysis of this remarkable spectrum, but also discuss the atmospheric trajectory, atmospheric penetration, and orbital data computed for this bolide which was probably released during 21P/Giacobini-Zinner return to perihelion in 1907. The spectrum is discussed together with the tensile strength for the October Draconid meteoroids. The chemical profile evolution of the main rocky elements for this extremely bright bolide is compared with the elemental abundances obtained for 5 October Draconid fireballs also recorded during our spectroscopic campaign but observed only at a single station. Significant chemical heterogeneity between the small meteoroids is found as we should expect for cometary aggregates being formed by diverse dust components.Comment: Manuscript in press in Monthly Notices of the Royal Astronomical Society. Accepted for publication in MNRAS on April 28th, 2013 Manuscript Pages: 28 Tables: 5 Figures: 12. Manuscript associated: "The 2011 October Draconids outburst. I. Orbital elements, meteoroid fluxes and 21P/Giacobini-Zinner delivered mass to Earth" by Trigo-Rodriguez et al. is also in press in the same journa

Cardiac Arrest in the Pediatric Population

Apresenta-se o caso clínico de uma criança de 10 anos com paragem cardíaca em repouso que foi reanimada, com sucesso. A investigação etiológica do acidente mostrou uma Cardiomiopatia Hipertrófica (CMH). Foi colocado um Cardiodesfibrilhador Implantável (CDI) para profilaxia secundária da Morte Súbita (MS). A Morte Súbita em idade pediátrica é uma situação rara, de muito mau prognóstico (sobrevida sem sequelas inferior a 5%) e com um impacto social significativo. A Cardiomiopatia Hipertrófica é uma causa conhecida de Morte Súbita, com possibilidade de prevenção. O caso apresentado serve para levantar questões sobre a necessidade e forma de estratégias para prevenir a MS de etiologica cardíaca em idade pediátrica