Exigências nutricionais e crescimento de plantas de mogno (Swietenia macrophylla King.) Nutritional requirements and growth of mahogany (Swietenia macrophylla King.) plants

A necessidade de desenvolver pesquisas referentes aos requerimentos nutricionais das espécies florestais, principalmente as essências florestais nativas da Amazônia, como o mogno, é inadiável, visto que as constantes explorações de espécies de alto valor econômico são cada vez maiores. Com o objetivo de avaliar o crescimento e o requerimento nutricional de mudas de mogno, foi realizado um experimento em casa de vegetação com 14 tratamentos. O delineamento experimental foi de blocos casualisados, com 5 repetições. As características de crescimento avaliadas foram: altura da parte aérea, diâmetro de colo, matéria seca da parte aérea, da raiz e total, relação raiz e parte aérea e conteúdo de nutrientes da matéria seca da parte aérea. Os resultados obtidos permitem concluir que: é necessária a correção conjunta da acidez e da fertilidade do solo para solos ácidos e de baixa fertilidade natural, mesmo que o teor de matéria orgânica seja considerado alto; dos nutrientes, P é o que mais limita o desenvolvimento da planta, bem como a absorção dos outros nutrientes; não há necessidade de adição de K para o desenvolvimento das plantas quando se realiza calagem; na ausência de calagem a adição de K deve ser recomendada e o requerimento nutricional do mogno em macronutrientes obedece à ordem decrescente de: P>S>K>N.<br>The need for developing research related principally to the nutritional requirements of essential native Amazonian forest species, such as mahogany, is urgent, since the exploration of highly valuable species is continually more frequent. With the objective of evaluating the growth and the nutritional requirement of mahogany plants, an experiment in a vegetation house with 14 treatments was undertaken. The experiment outline was of occasional blocks with 5 repetitions. The growth characteristics evaluated were: height of the aerial part, diameter of the bottom, dry material of the aerial part, root and total, relationship of root and aerial part, relationship and nutrient content of dry material of the aerial part. The results lead to the conclusion that: the conjoint correction of acidity and the fertility of the soil for acid soils and low natural fertility is necessary even if the content of the organic material is considered high; of the nutrients, P is the one which limits most the development of the plant, as well as the absorption of other nutrients; there is no need to add K for developing the plants when liming occurs.; addition of K is recommended when liming does not occur; and the nutritional requirement of mahogany in macronutrients obeys the decreasing order of P>S>K.N

Multi-messenger Observations of a Binary Neutron Star Merger

International audienceOn 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 $\sim 1.7\,{\rm{s}}$ with respect to the merger time. From the gravitational-wave signal, the source was initially localized to a sky region of 31 deg(2) 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 $\,{M}_{\odot }$. 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 $\sim 40\,{\rm{Mpc}}$) 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 $\sim 9$ and $\sim 16$ 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 NGC 4993 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