Archaeoastronomy/Cultural Astronomy

DOI
10.1093/acrefore/9780190647926.013.215
Belmonte, J. A.
Referencia bibliográfica

Oxford Research Encyclopedias on Planetary Science

Fecha de publicación:
2021
Número de autores
1
Número de autores del IAC
1
Número de citas referidas
0
Descripción
Archaeoastronomy and cultural astronomy are often considered synonyms, but they actually express different concepts, the former being a sub-discipline of the latter. Cultural astronomy is a fascinating but controversial discipline, which serves as an auxiliary subject to social sciences such as history, archaeology, anthropology, and ethnography, among others. The tools and methodology of astronomy play a relevant role in the discipline, but it should be inserted within social sciences epistemology. Keywords SubjectsHistory of Ideas about Planets and Planetary Systems
Proyectos relacionados
Puesta de sol en el equinoccio de primavera en los Obeliscos del Jabal Madbah, en la antigua Petra
Arqueoastronomía
Este Proyecto tiene como objetivo fundamental determinar la importancia de la astronomía como parte integrante de la cultura y de la civilización desde el Paleolítico a nuestros días. El interés del grupo se centra, en especial, en los pueblos del antiguo ámbito Mediterráneo desde el Atlántico al Oriente Medio, con una dedicación especial a España
Juan Antonio
Belmonte Avilés
En ejecución
Tipo
Con árbitro
Sistema Solar y Sistemas Planetarios (SEYSS)

Te puede interesar

  • Con árbitro
    Characterisation at Cryogenic Temperatures of an Attenuator for an Application of Astrophysical Instrumentation with MKIDs
    The use of non-cryogenic certified commercial electronics for cryogenic applications may be attractive due to their cost and availability, but it also carries risks related to reliability, performance and thermal compatibility. The decision to use commercial components that are not certified for cryogenics instead of components specifically
    Rodríguez Ramos L.F. et al.

    Fecha de publicación:

    12
    2024
  • Con árbitro
    Non-local thermodynamic equilibrium inversions of the Si I 10827 Å spectral line
    Inferring the coupling of different atmospheric layers requires observing spectral lines sensitive to the atmospheric parameters, particularly the magnetic field vector, at various heights. The best way to tackle this goal is to perform multi-line observations simultaneously. For instance, the new version of the Gregor Infrared Spectrograph
    Quintero Noda, C. et al.

    Fecha de publicación:

    12
    2024
    Bibcode
    2024A&A...692A.169Q
    Número de citas
    0
  • Con árbitro
    The Pristine survey: XXIII. Data Release 1 and an all-sky metallicity catalogue based on Gaia DR3 BP/RP spectro-photometry
    We used the spectro-photometric information of ∼219 million stars from Gaia's Data Release 3 (DR3) to calculate synthetic, narrowband, metallicity-sensitive CaHK magnitudes that mimic the observations of the Pristine survey, a survey of photometric metallicities of Milky Way stars that has been mapping more than 6500 deg 2 of the northern sky with
    Martin, Nicolas F. et al.

    Fecha de publicación:

    12
    2024
    Bibcode
    2024A&A...692A.115M
    Número de citas
    0