Science and Society: The Case of Acceptance of Newtonian Optics in the Eighteenth Century

The present paper presents a historical study on the acceptance of Newton's corpuscular theory of light in the early eighteenth century. Isaac Newton first published his famous book Opticks in 1704. After its publication, it became quite popular and was an almost mandatory presence in cultural life of Enlightenment societies. However, Newton's optics did not become popular only via his own words and hands, but also via public lectures and short books with scientific contents devoted to general public (including women) that emerged in the period as a sort of entertainment business. Lectures and writers stressed the inductivist approach to the study of nature and presented Newton's ideas about optics as they were consensual among natural philosophers in the period. The historical case study presented in this paper illustrates relevant aspects of nature of science, which can be explored by students of physics on undergraduate level or in physics teacher training programs.

A new dwarf species of Proceratophrys Miranda-Ribeiro, 1920 (Anura, Cycloramphidae) from the highlands of Chapada Diamantina, Bahia, Brazil

A new species of Proceratophrys is described from the highlands of northeastern Brazil. Molecular and morphological data suggests that Proceratophrys redacta sp. nov. is sister to P. minuta, and related to P. schirchi and P. cristiceps. The new species is diagnosed by its small size, absence of rostral and palpebral appendages, sagittal ridges interrupted, absence of postocular swellings, snout vertical in profile and dorsal coloration lacking distinct ocelli. The new species represents another example of endemism for the genus Proceratophrys in Chapada Diamantina region, and of another appendageless small-sized species associated with highlands. The phylogenetic results indicate that current morphological groupings in Proceratophrys may not represent natural groups.

XMM-Newton EPIC and OM observation of Nova Centauri 1986 (V842 Cen)

We report the results from the temporal and spectral analysis of an XMMNewton observation of Nova Centauri 1986 (V842 Cen). We detect a period at 3.51 +/- 0.4 h in the EPIC data and at 4.0 +/- 0.8 h in the Optical Monitor (OM) data. The X-ray spectrum is consistent with the emission from an absorbed thin thermal plasma with a temperature distribution given by an isobaric cooling flow. The maximum temperature of the cooling flow model is keV. Such a high temperature can be reached in a shocked region and, given the periodicity detected, most likely arises in a magnetically channelled accretion flow characteristic of intermediate polars. The pulsed fraction of the 3.51-h modulation decreases with energy as observed in the X-ray light curves of magnetic cataclysmic variables, possibly due either to occultation of the accretion column by the white dwarf body or phase-dependent to absorption. We do not find the 57-s white dwarf spin period, with a pulse amplitude of 4 mmag, reported by Woudt et al. in either the OM data, which are sensitive to pulse amplitudes ?0.03 mag, or the EPIC data, sensitive to pulse fractions p? 14 +/- 2 per cent.

The objectives of the US Exploring Expedition's circumnavigation (1838-1842): longitude, nautical charting and the establishment of modern geographic coordinates

This article analyzes the main objectives of the scientific voyage to circumnavigate the earth, undertaken by the United States from 1838 to 1842. Charting was one of the most important of the scientific and strategic goals of the exploratory voyage. The initiative for the undertaking was the search for exact positioning on the high seas after the establishment of the longitude system, when nautical charts and maps from various countries were compared, and other, new ones were drawn. The United States participated in this international effort, leading to the creation of its own cartographic system.

The peculiar isolated neutron star in the Carina Nebula Deep XMM-Newton and ESO-VLT observations of 2XMM J104608.7-594306

While fewer in number than the dominant rotation-powered radio pulsar population, peculiar classes of isolated neutron stars (INSs) which include magnetars, the ROSAT-discovered "Magnificent Seven" (M7), rotating radio transients (RRATs), and central compact objects in supernova remnants (CCOs) - represent a key element in understanding the neutron star phenomenology. We report the results of an observational campaign to study the properties of the source 2XMM J104608.7-594306, a newly discovered thermally emitting INS. The evolutionary state of the neutron star is investigated by means of deep dedicated observations obtained with the XMM-Newton Observatory, the ESO Very Large Telescope, as well as publicly available gamma-ray data from the Fermi Space Telescope and the AGILE Mission. The observations confirm previous expectations and reveal a unique type of object. The source, which is likely within the Carina Nebula (N-H = 2.6x10(21) cm(-2)), has a spectrum that is both thermal and soft, with kT(infinity) = 135 eV. Non-thermal (magnetospheric) emission is not detected down to 1% (3 sigma, 0.1-12 keV) of the source luminosity. Significant deviations (absorption features) from a simple blackbody model are identified in the spectrum of the source around energies 0.6 keV and 1.35 keV. While the former deviation is likely related to a local oxygen overabundance in the Carina Nebula, the latter can only be accounted for by an additional spectral component, which is modelled as a Gaussian line in absorption with EW = 91 eV and sigma = 0.14 keV (1 sigma). Furthermore, the optical counterpart is fainter than m(V) = 27 (2 sigma) and no gamma-ray emission is significantly detected by either the Fermi or AGILE missions. Very interestingly, while these characteristics are remarkably similar to those of the M7 or the only RRAT so far detected in X-rays, which all have spin periods of a few seconds, we found intriguing evidence of very rapid rotation, P = 18.6ms, at the 4 sigma confidence level. We interpret these new results in the light of the observed properties of the currently known neutron star population, in particular those of standard rotation-powered pulsars, recycled objects, and CCOs. We find that none of these scenarios can satisfactorily explain the collective properties of 2XMM J104608.7-594306, although it may be related to the still poorly known class of Galactic anti-magnetars. Future XMM-Newton data, granted for the next cycle of observations (AO11), will help us to improve our current observational interpretation of the source, enabling us to significantly constrain the rate of pulsar spin down.

Os objetivos da circunavegação da U.S. Exploring Expedition (1838-1842): longitude, mapeamento náutico e instituição das coordenadas geográficas modernas

Analisa o principal objetivo da viagem científica de circunavegação realizada pelos EUA entre 1838 e 1842. A tarefa de mapeamento destaca-se entre outras metas científico-estratégicas da viagem exploratória. A iniciativa da empreitada foi movida pela busca da exata localização em alto-mar após a instituição do sistema de longitudes, quando cartas náuticas e mapas de vários países foram conferidos, e outros, novos, desenhados. Os EUA participaram desse esforço internacional, dando início à constituição de um sistema cartográfico próprio.

A sala de aula foi o meu mundo: a carreira do magistério em São Paulo (1920-1950)

Nas primeiras décadas do século XX, dá-se a implantação, a expansão e a estruturação do sistema público de ensino paulista republicano. A criação de uma rede de escolas impulsiona a organização da carreira docente pela necessidade de formação de professores capazes de tornar tal expansão mais eficiente. Nesse período, foi estabelecido um conjunto de leis que normatizavam o exercício da profissão, fazendo dos professores funcionários do Estado. Ao lado da organização do sistema educativo, portanto, foi-se organizando também a profissão docente. Objetiva-se, aqui, problematizar a carreira e o trabalho docente em São Paulo a partir da experiência e da trajetória da professora paulista Botyra Camorim, tomando seu itinerário como representativo, pois a identidade de uma classe, de uma profissão, não pode ser considerada evidente independentemente das trajetórias dos membros que a compõem. Nesse movimento, acompanhar os fios de tal itinerário particular, inserido em meadas de relações, permitiu perceber a multiplicidade das experiências docentes, a pluralidade dos contextos de referência e as tensões que configuram limites e possibilidades ao fazer cotidiano. O confronto de fontes primárias - autobiografias, romances e contos escritos por Botyra Camorim - com a legislação, textos de educadores e pesquisas evidenciou que não se deve perseguir apenas a uniformidade e a homogeneização dos professores, pois os significados atribuídos ao trabalho docente e os modos de vivenciá-lo ou executá-lo não são perenes, mas estão intimamente relacionados com as condições espaço-temporais de exercício da profissão.

Entre antropologia e medicina: uma análise dos estudos antropológicos de Álvaro Fróes da Fonseca nas décadas de 1920 e 1930

O médico e antropólogo Álvaro Fróes da Fonseca percorreu várias cidades do Brasil durante sua trajetória profissional, na primeira metade do século XX. Atuou no magistério na cadeira de Anatomia Médico-Cirúrgica, nas Faculdades de Medicina de Porto Alegre, da Bahia e do Rio de Janeiro. Como antropólogo, exerceu atividades no Museu Nacional do Rio de Janeiro e, já nos anos 1960, no Instituto de Antropologia Tropical da Faculdade de Medicina do Recife. Pretendo, neste artigo, resgatar a contribuição do estudioso no campo antropológico, analisando algumas de suas pesquisas desenvolvidas no Laboratório de Antropologia do Museu Nacional e outras publicadas no periódico dessa instituição entre os anos 1920 e 1930. Neste período, ele congregou cientistas, desenvolveu e orientou vários trabalhos no âmbito da antropologia física e dos 'tipos antropológicos', voltando-se para o desenvolvimento de métodos e índices de classificação racial, ou seja, para a produção de conceitos e técnicas que orientavam a prática antropológica. Refutou o racismo científico do período, motivo pelo qual as investigações desenvolvidas por Fróes da Fonseca refletiram sobre o 'problema da raça' e a questão da mestiçagem em prol do futuro do Brasil.