Mapping the biosphere: exploring species to understand the origin, organization and sustainability of biodiversity

The time is ripe for a comprehensive mission to explore and document Earth's species. This calls for a campaign to educate and inspire the next generation of professional and citizen species explorers, investments in cyber-infrastructure and collections to meet the unique needs of the producers and consumers of taxonomic information, and the formation and coordination of a multi-institutional, international, transdisciplinary community of researchers, scholars and engineers with the shared objective of creating a comprehensive inventory of species and detailed map of the biosphere. We conclude that an ambitious goal to describe 10 million species in less than 50 years is attainable based on the strength of 250 years of progress, worldwide collections, existing experts, technological innovation and collaborative teamwork. Existing digitization projects are overcoming obstacles of the past, facilitating collaboration and mobilizing literature, data, images and specimens through cyber technologies. Charting the biosphere is enormously complex, yet necessary expertise can be found through partnerships with engineers, information scientists, sociologists, ecologists, climate scientists, conservation biologists, industrial project managers and taxon specialists, from agrostologists to zoophytologists. Benefits to society of the proposed mission would be profound, immediate and enduring, from detection of early responses of flora and fauna to climate change to opening access to evolutionary designs for solutions to countless practical problems. The impacts on the biodiversity, environmental and evolutionary sciences would be transformative, from ecosystem models calibrated in detail to comprehensive understanding of the origin and evolution of life over its 3.8 billion year history. The resultant cyber-enabled taxonomy, or cybertaxonomy, would open access to biodiversity data to developing nations, assure access to reliable data about species, and change how scientists and citizens alike access, use and think about biological diversity information.

High precision astrometry mission for the detection and characterization of nearby habitable planetary systems with the Nearby Earth Astrometric Telescope (NEAT)

A complete census of planetary systems around a volume-limited sample of solar-type stars (FGK dwarfs) in the Solar neighborhood (d a parts per thousand currency signaEuro parts per thousand 15 pc) with uniform sensitivity down to Earth-mass planets within their Habitable Zones out to several AUs would be a major milestone in extrasolar planets astrophysics. This fundamental goal can be achieved with a mission concept such as NEAT-the Nearby Earth Astrometric Telescope. NEAT is designed to carry out space-borne extremely-high-precision astrometric measurements at the 0.05 mu as (1 sigma) accuracy level, sufficient to detect dynamical effects due to orbiting planets of mass even lower than Earth's around the nearest stars. Such a survey mission would provide the actual planetary masses and the full orbital geometry for all the components of the detected planetary systems down to the Earth-mass limit. The NEAT performance limits can be achieved by carrying out differential astrometry between the targets and a set of suitable reference stars in the field. The NEAT instrument design consists of an off-axis parabola single-mirror telescope (D = 1 m), a detector with a large field of view located 40 m away from the telescope and made of 8 small movable CCDs located around a fixed central CCD, and an interferometric calibration system monitoring dynamical Young's fringes originating from metrology fibers located at the primary mirror. The mission profile is driven by the fact that the two main modules of the payload, the telescope and the focal plane, must be located 40 m away leading to the choice of a formation flying option as the reference mission, and of a deployable boom option as an alternative choice. The proposed mission architecture relies on the use of two satellites, of about 700 kg each, operating at L2 for 5 years, flying in formation and offering a capability of more than 20,000 reconfigurations. The two satellites will be launched in a stacked configuration using a Soyuz ST launch vehicle. The NEAT primary science program will encompass an astrometric survey of our 200 closest F-, G- and K-type stellar neighbors, with an average of 50 visits each distributed over the nominal mission duration. The main survey operation will use approximately 70% of the mission lifetime. The remaining 30% of NEAT observing time might be allocated, for example, to improve the characterization of the architecture of selected planetary systems around nearby targets of specific interest (low-mass stars, young stars, etc.) discovered by Gaia, ground-based high-precision radial-velocity surveys, and other programs. With its exquisite, surgical astrometric precision, NEAT holds the promise to provide the first thorough census for Earth-mass planets around stars in the immediate vicinity of our Sun.

Reflexões sobre a formação do acervo da Academia de Direito do Largo de São Francisco: do século XIX aos nossos dias

O trabalho apresenta algumas reflexões sobre a história da formação do acervo acadêmico dos cursos jurídicos do Brasil criados no século XIX, especificamente da Faculdade de Direito da Universidade de São Paulo. A primeira Biblioteca Pública de São Paulo, fundada em 1825, exerceu forte influência para que o Convento dos frades franciscanos recebesse a escola de direito criada por Decreto Imperial, em razão de seu fundo bibliográfico de 5.000 mil livros, preponderantemente de cunho eclesiástico, e considerável para os padrões culturais do Brasil à época. Atualmente configura-se como uma importante biblioteca jurídica acadêmica da América Latina e, ao longo da sua história tem sido uma instituição de depósito moral, isto é, recebe doações das mais diversas localidades do país, encaminhadas espontaneamente pelos autores para ter sua obra disponibilizada no acervo do primeiro e um dos mais tradicionais cursos de Direito do Brasil. Atualmente, este acervo está estimado em aproximadamente 400 mil itens, com doações de personalidades brasileiras. Outro ponto estudado refere-se ao estabelecimento de critérios para seleção de material – corpo editorial, autores de renome, relevância nos temas abordados etc. – em razão do boom editorial ocorrido na década de 1990, concomitante com o aumento de escolas de Direito no país. Chama-se à reflexão de quem atua na seara jurídica para atentar a pontos relevantes no momento da seleção para não incorrer no erro de avaliar com preconceito, modernidade, ideológico, interesse de estudo pessoal ou embasado apenas na data de publicação da obra. As ciências humanas, diferentemente de outras áreas, têm sua obsolescência mais lenta ou inexistente, decorrendo em grave erro para o Direito julgar exclusivamente pela data de publicação, o que torna premente aos profissionais bibliotecários dominarem conceitos básicos na área de atuação para que as bibliotecas sejam depositárias de material bibliográfico de qualidade.