O calendário babilónico, que adopta o calendário standard de Nippur, é luni-solar e está profundamente ligado ao culto, estruturando a vida dos mesopotâmios. Procura-se compreender o modo como os mesopotâmios, e particularmente os babilónios, estruturavam a sua noção de tempo, articulando o mês lunar com um ano solar. Por outro lado, eram várias as formas de datar os acontecimentos e essas tradições coexistiram ao longo do tempo. O calendário era determinado com grande precisão, uma vez que era fundamental (...) não apenas para orientar a vida económica e social dos mesopotâmios como o era também para enquadrar com precisão e rigor o culto. (shrink)

A partir de la “mitodología” y la fenomenología de las religiones, analizo el cuento “Blancanieves y los siete enanos” e identifico ele- mentos que sugieren un origen lunar e iniciático de él; además, encuentro semejanzas entre Blancanieves y algunas otras sacerdotisas de la luna.

La presente investigación pretende hacer un análisis histórico sobre la figura de San José y sus diferentes manifestaciones en la cultura y sociedad hondureña, como consecuencia de su culto, creación artística y devoción popular. Este culto tiene su origen en la época colonial, específicamente en el s. XVI, con los Concilios de Trento (1545 – 1563), Nueva España (1555, 1565, 1585) y Lima, Perú (1556 y 1561), los cuales contribuyeron a expandir el evangelio desde la iconografía hasta la (...) fundación de poblados que adoptaron esta imagen como Santo Patrón. También, se analiza esta imagen en el imaginario hondureño durante la secularización del Estado, su adopción y creación como un ideal de paternidad que simboliza protección, sustento y responsabilidad en la construcción de la organización familiar, finalizando con la vinculación de San José como patrono de la clase obrera en el siglo XX. (shrink)

Summary Tycho Brahe's lunar theory, mostly the work of his assistant Christian Longomontanus, published in the Progymnasmata (1602), was the most advanced and accurate lunar theory yet developed. Its principal innovations are: the introduction of equant motion for the first inequality in order to separate the determination of direction and distance; a more accurate limit for the second inequality although requiring a more complex calculation; additional inequalities of the variation and, in place of the annual inequality in Tycho's (...) earlier theory, a reduction in the equation of time; in the latitude theory a variation of the inclination of the orbital plane and an inequality of the motion of the nodes; a reduction in the range of variation of distance, parallax, and apparent diameter. Some of these were already present in Tycho's earlier lunar theory (1599), but all were changed in notable ways. Twenty years later Longomontanus published a modified version of the lunar theory in Astronomia Danica (1622), for the purpose of facilitating the calculation through new correction tables, and also explained his reasons for parts of the theory in the Progymnasmata. This paper is a technical study of both lunar theories. (shrink)

David Farrell Krell reflects on nine writers and philosophers, including Heidegger, Derrida, Blanchot, and Holderlin, in a personal exploration of the meaning of sensual love, language, tragedy, and death. The moon provides a unifying image that guides Krell's development of a new poetics in which literature and philosophy become one. Krell pursues important philosophical motifs such as time, rhythm, and desire, through texts by Nietzsche, Trakl, Empedocles, Kafka, and Garcia Marquez. He surveys instances in which poets or novelists explicitly address (...) philosophical questions, and philosophers confront literary texts--Heidegger's and Derrida's appropriations of Georg Trakl's poetry, Blanchot's obsession with Kafka's tortuous love affairs, and Garcia Marquez's use of Nietzsche's idea of the Eternal Return--all linked by the tragic hero Empedocles. In his search to understand the insatiable desire for completeness that patterns so much art and philosophy, Krell investigates the identification of the lunar voice with woman in various roles--lover, friend, sister, shadow, and narrative voice. (shrink)

A brief scholion allusion to a “Selenite” community in Arcadia raises a question concerning this epithet and its meaning on the background of similar expressions denoting extreme antiquity. The better known term associated with the Arcadians is Proselēnoi, namely, pre-lunar, people who preceded the moon. This term is examined through several options of understanding. At the core of this analysis stands the Classical tendency to highly appreciate early periods of time and early peoples. This opens up a discussion of (...) autochthony and the concept of extreme antiquity, particularly associated with Arcadia. The result is an etymologically based mythographic study centred on the Arcadians’ existence in relation to the first appearance of the moon. The conclusion offers a new interpretation of a neglected term. (shrink)

El propósito de este artículo es volver la mirada a un oficio intelectual y a un producto literario del que se podría decir que no ha enfrentado aún los desafíos que plantea la crítica literaria. El culto y el cultivo del haikú en escritores colombianos reclama hoy horizontes de comprensión propiamente literarios, ya que ante todo son, como cualquier otra expresión literaria, palabra, lenguaje, comunicación y sentido; hay en ellos campos semánticos y visiones de mundo, como hay epistemología, fenomenología (...) e ideología. Poder involucrar todo este andamiaje de reflexión y análisis no desapropiará el haikú de los escritores colombianos de su vínculo con la experiencia sensible e intuitiva recogida de la tradición japonesa. (shrink)

La narración de la experiencia visionaria del culto celestial en Ap 4-5 desvela dramá- ticamente el culto celestial. Los seres celestiales tributan el culto al que está sentado en el trono y al Cordero. Ambos, el Sentado y el Cordero, son los únicos dignos destinatarios de este culto. Todas las criaturas los reconocen como seres divinos. El hecho de dar culto a ambos supone una modificación innovadora del monoteísmo judío del segundo templo. Así, en su (...) visión, Juan participó en el culto celestial reconociendo la divinidad del Cordero que compartió los mismos honores con el Creador del universo. (shrink)

Este artigo tem como objetivo refletir sobre o racismo institucional que é perpetuado na manutenção da cobrança do Imposto sobre a Propriedade Territorial Urbana (IPTU) aos terreiros no município de Poções, na Bahia, bem como sobre a necessidade da implementação de políticas públicas e de uma hermenêutica jurídica decolonial que valorizem a cultura afrodiaspórica. O estudo se ancorou à luz da Constituição Federal de 1988, trazendo destaque para a discussão do racismo dentro das políticas públicas, os conceitos de tributo e (...) de imunidade tributária como um processo político e de decolonialidade. O percurso metodológico trilhou por uma abordagem qualitativa, de cunho bibliográfico, com base na legislação brasileira e em artigos científicos, dissertações e livros disponibilizados pela Internet. O recorte temporal corresponde aos dois últimos exercícios 2021 e 2022 para cobrança do IPTU dos imóveis urbanos do município de Poções. Por fim, considera-se que a insistente cobrança do IPTU em espaços de culto religioso de matriz africana, contrariando o cumprimento da Constituição federal de 1988 repercute os fortes resquícios patriarcais e racistas em que a sociedade brasileira ainda perpetua em suas práticas cotidianas. (shrink)

In this paper, three problems that have hardly been noticed or even gone unnoticed in the available literature in the cosmology of Philolaus are addressed. They have to do with the interrelationships of the orbits of the Earth, the Sun, and the Moon around the Central Fire and all three of them constitute potentially insurmountable obstacles within the context of the Philolaic system. The first difficulty is Werner Ekschmitt’s claim that the Philolaic system cannot account for the length of the (...) day (νυχϑήμερον). It is shown that this problem can be solved with the help of the distinction between the synodic day and the sidereal day. The other two problems discussed in this paper are concerned with two hitherto unnoticed deficiencies in the explanation of lunar eclipses in the Philolaic system. The Philolaic system cannot account for long-lasting lunar eclipses and according to the internal logic of the system, during lunar eclipses the Moon enters the shadow of the Earth from the wrong side. It is almost unbelievable that nobody, from the Pythagoreans themselves up to recent authors, has noticed these two serious deficiencies, and especially the latter, in the cosmology of Philolaus the Pythagorean. (shrink)

O presente artigo apresenta uma pesquisa sobre o que a instituição católica entende por piedade popular, tendo como base o Diretório de Piedade Popular e Liturgia, para em seguida, abordar o tema piedade popular mariana, com suas características próprias, como sentimento via cordis, exuberância, expressividade, vitalidade e caráter maravilhoso, e analisar a postura do catolicismo oficial, diante dessa maneira de vivenciar a fé. Posto isso, pesquisou-se o culto mariano, tendo como horizonte a exortação apostólica Marialis Cultus, de Paulo VI, (...) que contém orientações, como bíblica, litúrgica, sensibilidade ecumênica e antropológica, para promover uma genuína reforma da veneração a Maria. (shrink)

From the early ninth century until about eight centuries later, the Middle East witnessed a series of both simple and systematic astronomical observations for the purpose of testing contemporary astronomical tables and deriving the fundamental solar, lunar, and planetary parameters. Of them, the extensive observations of lunar eclipses available before 1000 AD for testing the ephemeredes computed from the astronomical tables are in a relatively sharp contrast to the twelve lunar observations that are pertained to the four (...) extant accounts of the measurements of the basic parameters of Ptolemaic lunar model. The last of them are Taqī al-Dīn Muḥammad b. Ma‘rūf’s trio of lunar eclipses observed from Istanbul, Cairo, and Thessalonica in 1576–1577 and documented in chapter 2 of book 5 of his famous work, Sidrat muntaha al-afkar fī malakūt al-falak al-dawwār. In this article, we provide a detailed analysis of the accuracy of his solar and lunar observations. (shrink)

SummaryThe celebrated Swedish natural philosopher and visionary theologian Emanuel Swedenborg (1688–1772) devoted major efforts to the establishment of a reliable method for the determination of longitude at sea. He first formulated a method, based on the astronomical observation of lunar position, while in London in 1710–12. He issued various versions of the method, both in Latin and in Swedish, throughout his career. In 1766, at the age of 78, he presented his scheme for judgment by the Board of Longitude (...) in London. The rich archive of Swedenborg's career allows an unusually detailed historical analysis of his longitude project, an analysis rather better documented than that available for the host of contemporary projectors who launched longitude schemes, submitted their proposals to the Board of Longitude, and have too often been ignored or dismissed by historians. This analysis uses the longitude work to illuminate key aspects of Swedenborg's wider enterprises, including his scheme to set up an astronomical observatory in southern Sweden to be devoted to lunar and stellar observation, his complex attitude to astronomical and magnetic cosmology, and his attempt to fit the notion of longitude into his visionary world-view. Swedenborg's programme also helps make better sense of the metropolitan and international networks of diplomatic and natural philosophical communication in which the longitude schemes were developed and judged. It emerges that his longitude method owed much to the established principles of earlier Baroque and Jesuit natural philosophy while his mature cosmology sought a rational and enlightened model of the universe. (shrink)

Nevil Maskelyne, the Cambridge-trained mathematician and later Astronomer Royal, was appointed by the Royal Society to observe the 1761 transit of Venus from the Atlantic island of St Helena, assisted by the mathematical practitioner Robert Waddington. Both had experience of measurement and computation within astronomy and they decided to put their outward and return voyages to a further use by trying out the method of finding longitude at sea by lunar distances. The manuscript and printed records they generated in (...) this activity are complemented by the traditional logs and journals kept by the ships’ officers. Together these records show how the mathematicians came to engage with the navigational practices that were already part of shipboard routine and how their experience affected the development of the methods that Maskelyne and Waddington would separately promote on their return. The expedition to St Helena, in particular the part played by Maskelyne, has long been regarded as pivotal to the introduction of the lunar method to British seamen and to the establishment of theNautical Almanac. This study enriches our understanding of the episode by pointing to the significant role played by the established navigational competence among officers of the East India Company. (shrink)

This paper is the third of a multi-part examination of the Babylonian mathematical lunar theories known as Systems A and B. Part I (Britton, AHES 61:83–145, 2007) addressed the development of the empirical elements needed to separate the effects of lunar and solar anomaly on the intervals between syzygies, accomplished in the construction of the System A lunar theory early in the fourth century B.C. Part II (Britton, AHES 63:357–431, 2009) examines the accomplishment of this separation by (...) the construction of a successful theory depicting the variations due to lunar anomaly in System A and its subsequent adaptation in System B. The present paper examines the introduction of the uniform zodiac, necessary for any theory depicting variations depending on the position of syzygy. It addresses three questions: (1) In light of all available evidence, what is the magnitude of the constant term in the expression Δλ* = C − 1.3828°Y, describing the difference between the Babylonian sidereal longitudes and modern tropical longitudes? (2) What considerations governed the placement of the Babylonian sidereal zodiac relative to the fixed stars? (3) When was the uniform zodiac introduced? To the first question it finds C = 3.20° ± 0.1°, scarcely different from Huber’s (Centaurus 5:192–208, 1958) estimate of 3.08°, essentially confirming Huber’s result obtained from much less data. For the second it shows that accommodating the three asterisms comprising Taurus limited the placement of the zodiac to within 3°, while the prominence of half sign multiples among the measured intervals between prominent Normal Stars led irresistibly to the choice adopted. Finally, it finds that the zodiac was introduced between −408 and −397 and probably within a very few years of −400. (shrink)

This paper is the second of a multi-part examination of the creation of the Babylonian mathematical lunar theories known as Systems A and B. Part I (Britton 2007) addressed the development of the empirical elements needed to separate the effects of lunar and solar anomaly on the intervals between syzygies. This was accomplished in the construction of the System A lunar theory by an unknown author, almost certainly in the city of Babylon and probably early in the (...) 4th century B.C. The present paper focuses mainly on System A and the likely process of its construction. The first three sections are largely descriptive – first of the basic concepts which underlie the theory; then of the component schemes comprising the theory; and finally of two distinctive texts which suggest how the theory was constructed. The crux of the paper is Sect. 4, which describes how the theory seems likely to have been constructed. Here the crucial insight in separating the effects of lunar and solar anomaly appears to have been recognizing that – of all the measurable intervals bounded by eclipses – only 235 months exhibits a variation due solely to lunar anomaly, and that by means of an elegant mathematical model the amplitudes of 223 and 12 months could be deduced from its amplitude. The rest of the section describes the likely details of the derivation of the Φ ~ Λ scheme, and the extension of the methodology to the other components of the theory. It concludes with a demonstration that Φ and its dependent schemes were anchored through the Φ ~ W scheme to the syzygy on –403 Aug 18 (GN 7391) which concluded the shortest 6-month interval in the first 24 saros cycles since –746 (and in fact in the 900 years separating Nabonassar and Ptolemy). The next three sections address a number of largely technical details and amplifications of the theory, beginning with the schemes describing the variation of lunar velocity (column F) in Sect. 5. Section 6 addresses issues concerning the interpretation of Φ and the so-call Saros Text (BM 36705), while Sect. 7 discusses System B’s corresponding treatment of the effects of lunar anomaly, illustrating both its derivative nature and mathematically less rigorous structure. Section 8 examines the accuracy of the two theories, showing that the System A theory was both remarkably accurate and superior to System B. The final section offers some brief remarks on the power and elegance of the mathematical treatment of the problem by the author of System A. (shrink)

In Asian countries, there is a tradition that a rabbit, known as the Moon rabbit, lives on the Moon. Typically, two reasons are mentioned for the origin of this tradition. The first reason is that the color pattern of the lunar surface resembles the shape of a rabbit. The second reason is that both the Moon and rabbits are symbols of fertility, as the Moon appears and disappears (i.e., waxing and waning) cyclically and rabbits are known for their high (...) fertility. Considering the latter reason, is the color pattern of the lunar surface not similar to a rabbit? Here, the similarity between rabbit and the lunar surface pattern was evaluated using seven AI architectures. In the test conducted with Contrastive Language-Image Pre-Training (CLIP), which can classify images based on given words, it was assumed that people frequently observe the Moon in the early evening. Under this condition, the lunar surface pattern was found to be more similar to a rabbit than a face in low-latitude regions, while it could also be classified as a face as the latitude increases. This result is consistent with that the oldest literatures about the Moon rabbit were written in India and that a tradition of seeing a human face in the Moon exists in Europe. In a 1000-class test using seven AI architectures, ConvNeXt and CLIP sometimes classified the lunar surface pattern as a rabbit with relatively high probabilities. Cultures are generated by our attitude to the environment. Both dynamic and static similarities may be essential to induce our imagination. (shrink)

Name der Zeitschrift: Apeiron Jahrgang: 50 Heft: 4 Seiten: 483-510.

Leonhard Euler (1707–1783) published two lunar theories in 1753 and 1772. He also published lunar tables in 1745, 1746, and—anonymously—in 1750. There are notebook records, unpublished manuscripts, and manuscript fragments by Euler reflecting the development of his lunar theories between about 1725 until about 1752. These documents might be used to reconstruct Euler’s theory on which he based his calculations of those lunar tables and to analyze the development of his lunar theories within this time (...) span. The results of this analysis will be published here in three parts representing three stages of Euler’s research on this topic: First approaches (about 1725–1730), developing the methods (about 1730–1744), and the breakthrough (about 1744–1752). In this part, I analyze Euler’s manuscripts and, predominantly, Euler’s records of his first two notebooks written between 1725 and 1730. I found that his early theoretical approach is coined by his development of analytical (rational) mechanics of punctiform bodies moved by central forces. He tried to describe the Moon’s motion in terms of two simultaneously acting centripetal forces, Huygens’ centrifugal theorem, and associated osculating radii. (shrink)

Quanto ao processo de tradução de um texto, neste caso traduzido do alemão para o português, é importante ressaltar o conhecimento do tema abordado, bem como a figura do autor e a teoria ou o pensamento desenvolvido para a sua época, uma vez que muitos vocábulos utilizados em uma determinada língua não possuem tradução real sobre o seu significado na língua portuguesa. Logo, o tradutor tem como artifícios a seu favor no trabalho de tradução, não apenas o conhecimento da língua, (...) mas a importância que o autor e sua obra teve na época que foi redigido o texto ou postumamente. Algumas palavras deixam de ser utilizada ou substituídas por outras com o decorrer de anos, décadas e séculos. Isso é perceptível, por exemplo, quando nos deparamos com textos antigos, no caso de Hanslick, importante escritor e crítico de estética pertencente ao século XIX. As alterações não são apenas por questões de revisões ortográficas, mas também por tópicos relacionados à própria cultura que a língua amalgama conforme a prática e a vivência do cotidiano dessa mesma cultura. Outro exemplo para melhor compreensão se dá em pensamentos e teorias filosóficas, a saber, termos específicos de uma determinada filosofia, pois um mesmo vocábulos possui outro conceito quando é desenvolvido em uma concepção filosófica e teoria discrepante de um pensador para outro pensador. Estes são apenas alguns dos impasses que o tradutor convive durante o trabalho de tradução. (shrink)