Academic literature on the topic 'Maya astronomy'

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Journal articles on the topic "Maya astronomy"

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Aveni, Anthony, John Justeson, and Victoria Bricker. "Maya astronomy and the precession of the equinoxes." Journal for the History of Astronomy 56, no. 2 (2025): 125–41. https://doi.org/10.1177/00218286241307930.

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The presence of very large time intervals in Maya hieroglyphic inscriptions has prompted a proposal that the period of the roughly 25,770-year precession of the equinoxes is among those in the historical record, by showing that some very long recorded intervals are near whole multiples of the sidereal year. Analysis of Maya long numbers shows the arguments for such a proposal to be invalid and the claims implausible. It argues methodologically for the effectiveness of basic, shorter-term calendrical intervals, and substantively for Maya daykeepers focusing on the solstices rather than equinoxe
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Šprajc, Ivan, and Pedro Francisco Sánchez Nava. "Astronomy and Architecture in the Maya Lowlands." Journal of Skyscape Archaeology 2, no. 2 (2017): 189–215. http://dx.doi.org/10.1558/jsa.30050.

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This article summarises recent systematic research into the use and significance of astronomical orientations in ancient Maya architecture, and shows how by applying a more rigorous methodology to a large number of orientations we were able to detect alignment patterns that shed light on the validity of former hypotheses and provide a basis for novel interpretations. Our measurements and analysis confirm that orientations to the Sun’s position on the horizon, which largely prevail, allowed the use of observational calendars composed of multiples of 13 and 20 days and were also intended to faci
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MacPherson, H. G. "The Maya lunar season." Antiquity 61, no. 233 (1987): 440–49. http://dx.doi.org/10.1017/s0003598x00072999.

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Archaeoastronomy in Europe, when it comes to megalithic sites, is still at the perhaps stage: perhaps there was some systematic understanding of the heavens that can be called astronomy, perhaps there was not. In the Americas matters are different, with the ‘long-count’ and other systems showing a clear interest in calendars, and in the timely movements of the heavens. Here the lunar order of the Maya scheme of things is set out.
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Sullivan, Lauren A. "Maya Political Science: Time, Astronomy, and the Cosmos." History: Reviews of New Books 33, no. 3 (2005): 106–7. http://dx.doi.org/10.1080/03612759.2005.10526568.

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Šprajc, Ivan. "Maya and Aztec astronomy: Skywatching in prehispanic Mesoamerica." Journal of Physics: Conference Series 2877, no. 1 (2024): 012032. http://dx.doi.org/10.1088/1742-6596/2877/1/012032.

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Abstract The Aztecs, Maya and other Mesoamerican peoples achieved advanced knowledge of the regularities of the apparent motion of the Sun, Moon and various planets visible with the naked eye, particularly Venus. Much of this knowledge enabled orientation in space and time and was particularly useful for scheduling agricultural activities. However, since the celestial order is apparently superior to that on Earth, the phenomena observed in the sky were believed to exert influence on earthly affairs. Therefore, the exact astronomical knowledge was intertwined with religious beliefs and ritual p
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Hammond, Norman. "Star Gods of the Maya: Astronomy in Art, Folklore, and Calendars:Star Gods of the Maya: Astronomy in Art, Folklore, and Calendars." American Anthropologist 103, no. 2 (2001): 549–50. http://dx.doi.org/10.1525/aa.2001.103.2.549.

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Peck, Douglas T. "Development of Celestial Navigation by the Ancient Maya." Journal of Navigation 54, no. 1 (2001): 145–49. http://dx.doi.org/10.1017/s0373463300001168.

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This paper discusses the knowledge and culture of astronomy possessed by the Maya civilisation and how this might have been used for marine navigation in the 8th Century. Comparison is made with the European view and use of celestial positioning.
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Carlson, John B., and Mark Van Stone. "The 2012 phenomenon: Maya calendar, astronomy, and apocalypticism in the worlds of scholarship and global popular culture." Proceedings of the International Astronomical Union 7, S278 (2011): 178–85. http://dx.doi.org/10.1017/s1743921311012609.

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AbstractThis essay introduces the papers from the specially organized session on the theme ‘The 2012 phenomenon: Maya calendar, astronomy, and apocalypticism in the worlds of scholarship and popular culture’. The papers that follow address this topical theme in the contexts of Maya and Western cultures as well as academic and popular cultures.
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Aimers, James J., and Prudence M. Rice. "ASTRONOMY, RITUAL, AND THE INTERPRETATION OF MAYA “E-GROUP” ARCHITECTURAL ASSEMBLAGES." Ancient Mesoamerica 17, no. 1 (2006): 79–96. http://dx.doi.org/10.1017/s0956536106060056.

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E-group architectural assemblages, constructed and used for more than a millennium in the Maya Lowlands, are among the most distinctive and enduring forms in Mesoamerican monumental architecture. Since the 1920s, E-groups have been thought to mark the solstices and equinoxes, but more recent investigations have shown that these alignments were rarely accurate. We argue that accurate solar alignment was probably only a minor element, and primarily an early one, of a larger set of metaphorically linked design considerations that included concepts of sacred geography, ritual performance in refere
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Aveni, Anthony F., and Lorren D. Hotaling. "Monumental Inscriptions and the Observational Basis of Maya Planetary Astronomy." Journal for the History of Astronomy 25, no. 19 (1994): S21—S54. http://dx.doi.org/10.1177/002182869402501903.

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Dissertations / Theses on the topic "Maya astronomy"

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Beck, William Earl. "Maya Eclipses: Modern Data, the Triple Tritos and The Double Tzolkin." Master's thesis, University of Central Florida, 2007. http://digital.library.ucf.edu/cdm/ref/collection/ETD/id/3407.

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The Eclipse Table, on pages 51-58, of the Dresden Codex has long fascinated Maya scholars. Researchers use the mean-value method of 173.3 days to determine nodal passage that is the place where eclipses can occur. These studies rely on Oppolzer's Eclipse Canon and Schram's Moon Phase Tables to verify eclipse occurrences. The newer canons of Jean Meeus and Bao-Lin Liu use decimal accuracy. What would be the effect of modern astronomical data on the previous studies and the Maya Eclipse Table? The study utilizes a general view of eclipses that includes eclipses not visible to the Maya. Lunar ecl
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May, Castillo Manuel. "Análisis, estudio y conservación de los edificios astronómicos mayas. Arquitectura maya y urbanismo, una aproximación desde la astronomía y el paisaje." Doctoral thesis, Universitat Politècnica de València, 2014. http://hdl.handle.net/10251/43218.

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El presente trabajo representa el resultado final de seis años de investigación en la región maya y versa sobre las relaciones entre la arquitectura y el urbanismo con el paisaje y la astronomía. En una primera parte se presentan los fundamentos metódicos para el estudio de la arquitectura y el urbanismo maya, a partir de la lectura de los datos del paisaje circundante y las orientaciones arquitectónicas. A lo anterior se le suman los datos provistos por las fuentes pre-coloniales, coloniales y contemporáneas. Los aspectos teóricos sustentan la postura del autor, quien plantea un
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Krause, Maya [Verfasser], and Jürgen [Akademischer Betreuer] Blum. "Wärmeleitfähigkeit von Planetesimalen / Maya Krause ; Betreuer: Jürgen Blum." Braunschweig : Technische Universität Braunschweig, 2019. http://d-nb.info/1175387428/34.

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Cerda, Escobar Francisca. "Wenu Kimun: el saber del cielo: mapa interactivo sobre astronomía y cosmología mapuche para dispositivos móviles." Tesis, Universidad de Chile, 2016. http://repositorio.uchile.cl/handle/2250/143254.

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Memoria para optar al título de Diseñadora Gráfica<br>Wenu Kimün consiste en un proyecto de carácter profesional, que propone una visualización informativa e interactiva para acceder al planisferio astronómico cultural mapuche. De esta manera, el proyecto se enfoca en la difusión de los conocimientos y las creencias del pueblo mapuche. La oportunidad que da origen a la propuesta, se basa en la relación de las personas con el “cielo”. En esta relación, los cuerpos y fenómenos astronómicos visibles se configuran como elementos visuales que entregan información cultural y de la vida cotidiana, e
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Mana, Annalisa [Verfasser], and Jochen [Akademischer Betreuer] Weller. "Optically selected galaxy clusters as a cosmological probe / Annalisa Mana. Betreuer: Jochen Weller." München : Universitätsbibliothek der Ludwig-Maximilians-Universität, 2013. http://d-nb.info/1045153087/34.

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Kierdorf, Maja [Verfasser]. "Probing the Magnetized Medium of Galaxies and AGNs using Wideband Radio Polarimetry / Maja Kierdorf." Bonn : Universitäts- und Landesbibliothek Bonn, 2019. http://d-nb.info/119446484X/34.

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Lorenzo, Espinosa Javier. "Binarias espectroscópicas de alta masa como laboratorios astrofísicos." Doctoral thesis, Universidad de Alicante, 2013. http://hdl.handle.net/10045/36040.

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Las estrellas masivas desempeñan un papel fundamental en la evolución de las Galaxias, siendo la fuente primordial de generación y dispersión de elementos como el oxígeno, silicio, etc., en el medio interestelar. La masa de la estrella es el parámetro más determinante en los procesos de evolución de la estrella, pero su determinación no siempre es posible sin el uso de calibraciones externas. Afortunadamente, la naturaleza nos ofrece las estrellas binarias como laboratorios astrofísicos, donde es posible la determinación de las masas de sus componentes a partir del movimiento orbital de las mi
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García, Fuentes Pablo Fernando. "Giant Molecular Clouds in the Southern Milky Way." Tesis, Universidad de Chile, 2007. http://www.repositorio.uchile.cl/handle/2250/104575.

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Guzmán, Fernández Andrés Ernesto. "Ionized Jets and Molecular Outflows in High-Mass Young Stellar Objects." Tesis, Universidad de Chile, 2012. http://repositorio.uchile.cl/handle/2250/102759.

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Uno de los problemas claves en el estudio de la formación de estrellas es determinar si acaso el paradigma de formación de estrellas de baja masa, específicamente, contracción gravitacional y la posterior presencia de un disco de acreción y chorros altamente colimados, se extiende a las estrellas de alta masa. En esta tesis se lleva a cabo una búsqueda sistemática de chorros ionizados hacia objetos estelares jóvenes de alta masa. La presencia de estos chorros entrega evidencia que sostiene dos importantes nociones astrofísicas: que las estrellas de alta masa pasan por una fase de eyección chor
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Miller, Bertolami Marcelo Miguel. "Procesos de mezcla en estrellas de masa intermedia." Tesis, 2004. http://hdl.handle.net/10915/1972.

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El objetivo de esta tesis es el estudio de la formación de estrellas deficientes en H por medio de flashes del He de diferentes tipos que ocurren en situaciones diferentes a las usuales y producen la dilución o quema del H remanente de la estrella, dando como resultado abundancias superficiales deficientes en H. El trabajo está orientado tanto al estudio de los eventos y mecanismos por medio de los cuales la estrella adquiere la composición deficiente en H, como así también al estudio de su evolución posterior como estrella deficiente en H.
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Books on the topic "Maya astronomy"

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Guatemala), ESEDIR (School :. Ciencia y tecnología maya: Maya' no'jb'äl. Escuela Superior de Educación Integral Rural, 2001.

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Cabrera, Edgar. La cosmogonía maya. Liga Maya Internacional, 1992.

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Romano, Giuliano. Introduzione alla matematica precolombiana: Con esercizi e applicazioni alla calendaristica e all'astronomia dei popoli precolombiani. CLEUP, 2000.

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Conde, Paulino Romero. La milpa y el origen del calendario maya. Gobierno del Estado de Yucatán, 1994.

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Cabrera, Edgar. El calendario maya: Su orígen y su filosofía. Ediciones Liga Maya, 1995.

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Sotelo, Laura. Las ideas cosmológicas mayas en el siglo XVI. Universidad Nacional Autónoma de México, Instituto de Investigaciones Filológicas, Centro de Estudios Mayas, 1988.

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Arturo Ospina de la Roche. El legado maya: Los aportes de un Pueblo sorprendente a las matemáticas y la astronomía. Editorial Planeta Colombiana, 2001.

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1940-, Bricker Victoria Reifler, ed. Astronomy in the Maya codices. American Philosophical Society, 2011.

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1938, Aveni Anthony F., ed. The Sky in Mayan Literature. Oxford University Press, 1993.

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F, Aveni Anthony, ed. The Sky in Mayan literature. Oxford University Press, 1992.

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Book chapters on the topic "Maya astronomy"

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Dolan, Marion. "Maya Astronomy and Architecture." In Decoding Astronomy in Maya Art and Architecture. Springer Nature Switzerland, 2024. http://dx.doi.org/10.1007/978-3-031-61092-9_4.

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Dolan, Marion. "The Maya and Astronomy." In Decoding Astronomy in Maya Art and Architecture. Springer Nature Switzerland, 2024. http://dx.doi.org/10.1007/978-3-031-61092-9_5.

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Dolan, Marion. "Maya Society." In Decoding Astronomy in Maya Art and Architecture. Springer Nature Switzerland, 2024. http://dx.doi.org/10.1007/978-3-031-61092-9_3.

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Dolan, Marion. "Maya City of Copan." In Decoding Astronomy in Maya Art and Architecture. Springer Nature Switzerland, 2024. http://dx.doi.org/10.1007/978-3-031-61092-9_11.

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Dolan, Marion. "Deities of the Maya." In Decoding Astronomy in Maya Art and Architecture. Springer Nature Switzerland, 2024. http://dx.doi.org/10.1007/978-3-031-61092-9_6.

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Dolan, Marion. "Maya City of Palenque." In Decoding Astronomy in Maya Art and Architecture. Springer Nature Switzerland, 2024. http://dx.doi.org/10.1007/978-3-031-61092-9_10.

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Dolan, Marion. "Maya Mythology, Cosmology and Art." In Decoding Astronomy in Maya Art and Architecture. Springer Nature Switzerland, 2024. http://dx.doi.org/10.1007/978-3-031-61092-9_7.

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Dolan, Marion. "Introduction to the Ancient Maya." In Decoding Astronomy in Maya Art and Architecture. Springer Nature Switzerland, 2024. http://dx.doi.org/10.1007/978-3-031-61092-9_2.

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Dolan, Marion. "Maya City of Chichen Itza." In Decoding Astronomy in Maya Art and Architecture. Springer Nature Switzerland, 2024. http://dx.doi.org/10.1007/978-3-031-61092-9_14.

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Dolan, Marion. "Early Classic Cities of the Maya." In Decoding Astronomy in Maya Art and Architecture. Springer Nature Switzerland, 2024. http://dx.doi.org/10.1007/978-3-031-61092-9_9.

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Conference papers on the topic "Maya astronomy"

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Morgan, Jeffrey S., J. Gethyn Timothy, Andrew M. Smith, Robert J. Hill, and David B. Kasle. "High time-resolution imaging with the MAMA detector systems." In Astronomy '90, Tucson AZ, 11-16 Feb 90, edited by David L. Crawford. SPIE, 1990. http://dx.doi.org/10.1117/12.19077.

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Romaniuk, Ryszard S. "Astronomy and Space Technologies, Photonics Applications and Web Engineering, Wilga, May 2012." In Photonics Applications in Astronomy, Communications, Industry, and High-Energy Physics Experiments 2012, edited by Ryszard S. Romaniuk. SPIE, 2012. http://dx.doi.org/10.1117/12.2005972.

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Todorović, Nataša. "MALA PLANETA 1675 SIMONIDA." In Kralj Milutin i doba Paleologa: istorija, književnost, kulturno nasleđe. Publishing House of the Eparchy of Šumadija of the Serbian Orthodox Church - "Kalenić", 2023. http://dx.doi.org/10.46793/6008-065-5.833t.

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Minor planets (also called asteroids or planetoids) are small celestial bodies orbiting the Sun. In this work, we present one asteroid named after the Serbian and Byzantine princess Simonida Nemanjić (1294–1345), the wife of King Milutin. The asteroid was discovered from the Belgrade observatory on March 20, 1938, by Serbian astronomer Milorad B. Protić. It was provisionally designated with 1938 FB and after three decades of observations numbered 1675. In the early 1970s, following the suggestion of Ms Zora Sučić-Protić, who was the Minister of Education at the time, the asteroid was named SIM
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"The complex VHE and multiwavelength flaring activity of the FSRQ PKS 1510-089 in May 2015." In HIGH ENERGY GAMMA-RAY ASTRONOMY: 6th International Meeting on High Energy Gamma-Ray Astronomy. Author(s), 2017. http://dx.doi.org/10.1063/1.4968969.

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Romaniuk, Ryszard S. "Photonics applications and web engineering: WILGA May 2013." In Photonics Applications in Astronomy, Communications, Industry, and High-Energy Physics Experiments 2013, edited by Ryszard S. Romaniuk. SPIE, 2013. http://dx.doi.org/10.1117/12.2035420.

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Moiseev, Yu, and O. Sazhina. "A strategy for wormhole search using observational astronomy." In Modern astronomy: from the Early Universe to exoplanets and black holes. Special Astrophysical Observatory of the Russian Academy of Sciences, 2024. https://doi.org/10.26119/vak2024.035.

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We present a promising strategy for wormhole (WH) search using astronomical observations. By identifying a net effect of anomalous gravitational acceleration may allow for assumptions regarding the hidden WH nature of a black hole (BH). We provide an upper estimate of this effect for several stars in known BH systems such as S2 and S62 orbiting around Sgr A*; along with modeling a synthetic system consisting of a traversable WH, a star on our side and a perturbing object on the other side of a WH. We also consider recently discovered objects from GAIA catalogue data – GAIA BH1, BH2 and BH3. We
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Garcia Burillo, Santiago. "The formation and evolution of galaxies: what we may learn with the SKA." In 2nd MCCT-SKADS Training School. Radio Astronomy: fundamentals and the new instruments. Sissa Medialab, 2009. http://dx.doi.org/10.22323/1.065.0007.

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Romaniuk, Ryszard S. "Photon Physics and Plasma Research, Photonics Applications and Web Engineering, Wilga, May 2012." In Photonics Applications in Astronomy, Communications, Industry, and High-Energy Physics Experiments 2012, edited by Ryszard S. Romaniuk. SPIE, 2012. http://dx.doi.org/10.1117/12.2005976.

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Sharykin, I., and I. Zimovets. "Photospheric disturbances and acoustic sources of the helioseismic ``circular'' X1.5 flare of May 10, 2022." In Modern astronomy: from the Early Universe to exoplanets and black holes. Special Astrophysical Observatory of the Russian Academy of Sciences, 2024. https://doi.org/10.26119/vak2024.116.

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This paper is devoted to the analysis of the energy release of the X1.5-class solar flare that occurred on May 10, 2022, during which the powerful helioseismic response (``sunquake'') was observed. An additional feature is the fact that this powerful sunquake was generated in the NOAA active region 13006 of Hale class $\beta\delta$, whereas earlier it was shown that the strongest helioseismic disturbances are generated in the sunspot groups with the most complex Hale class of $\beta\gamma\delta$. We analyze magnetic fields and photospheric perturbations basing on the Helioseismic and Magnetic
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Romaniuk, Ryszard S. "Optoelectronic Devices, Sensors, Communication and Multimedia, Photonics Applications and Web Engineering, Wilga, May 2012." In Photonics Applications in Astronomy, Communications, Industry, and High-Energy Physics Experiments 2012, edited by Ryszard S. Romaniuk. SPIE, 2012. http://dx.doi.org/10.1117/12.2005977.

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Reports on the topic "Maya astronomy"

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Francesco, Petruccione,, Gastrow, Michael, Hadzic, Senka, et al. Evaluation of Alternative Telecommunication Technologies for the Karoo Central Astronomy Advantage Area. Academy of Science of South Africa (ASSAf), 2021. http://dx.doi.org/10.17159/assaf.2021/0073.

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The National Research Foundation (NRF) requested the Academy of Science of South Africa (ASSAf), on behalf of South African Radio Astronomy Observatory (SARAO) and the Square Kilometre Array (SKA), to undertake an independent and objective evaluation of potential alternative telecommunication technologies for the areas of the Karoo Central Astronomy Advantage Areas (KCAAA). The study encompasses regulatory, public sphere, and technical dimensions to explore options for maintaining the functionality of the telescope while, at the same time, delivering appropriate connectivity solutions for loca
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Durik, Amanda, Steven McGee, Linda Huber, and Jennifer Duck. The Cat is Alive and Well: Curiosity Motivates Exploration for High Interest Learners. The Learning Partnership, 2015. http://dx.doi.org/10.51420/conf.2015.1.

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Two studies were conducted to examine how individual interest predicts interactions with domain content and subsequent free-choice exploration. Particular focus was on learners’ acquisition of knowledge and identification of content that triggered curiosity. College student participants reported their individual interest, learned about a topic in ecology (Study 1, N = 85) and astronomy (Study 2, N = 184), responded to prompts for memory of the learning content and curiosity questions, and then had the opportunity to explore additional content related to the topic. In both studies individual in
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Weekes, T. C. The application of two-dimensional imaging to very high energy gamma ray astronomy. Annual report, 1 May 1991--30 April 1992. Office of Scientific and Technical Information (OSTI), 1992. http://dx.doi.org/10.2172/10142618.

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Zilberman, Mark. Methods to Test the “Dimming Effect” Produced by a Decrease in the Number of Photons Received from Receding Light Sources. Intellectual Archive, 2020. http://dx.doi.org/10.32370/iaj.2437.

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The hypothetical “Dimming Effect” describes the change of the number of photons arriving from a moving light source per unit of time. In non-relativistic systems, the “Dimming effect” may occur due to the growing distance of light sources moving away from the receiver. This means that due to the growing distance, the photons continuously require more time to reach the receiver, which reduces the number of received photons per time unit compared to the number of emitted photons. Understandably, the proposed “Dimming effect” must be tested (confirmed or rejected) through observations. a. This ar
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