Building on the Legacy of Astronomical Standards

Autores
Kaplan, G. H.
Año de publicación
2025
Idioma
inglés
Tipo de recurso
documento de conferencia
Estado
versión publicada
Descripción
International cooperation and collaboration on astronomical projects of various kinds followed the improvements in communication and travel that rapidly advanced during the late 19th and early 20th centuries. The history of international astronomical standards probably dates to the International Meridian Conference in 1884 in Washington and the Paris Conference of 1896. The formation of the IAU in 1919 institutionalized international cooperation in astronomy. Before the midpoint of the 20th century, only a few organizations worldwide, mostly the national observatories, had the capabilities to compute and distribute the data for fundamental astronomy, such as the celestial coordinates of the Sun, Moon, and planets; sidereal time; eclipse circumstances; apparent places of stars; the data needed for celestial navigation; and precise time. The situation changed after World War II as electronic computers became available at scientific institutions and more precise observational techniques were invented, some involving spaced-based instruments. As many common astronomical computations became more "democratized” in the latter part of the 20th century, IAU standards, as well as those from other institutions, such as the IUGG and IERS, of necessity became more comprehensive and detailed, covering time scales, constants, reference systems, Earth orientation models, and the implementation of relativity in various astronomical computations. Thus, the evolution of astronomical standards traces the major advances in observational technology, theoretical sophistication, and computing power that have defined our science for the last century.
Facultad de Ciencias Astronómicas y Geofísicas
Materia
Ciencias Astronómicas
Astronomical standards
International Astronomical Union (IAU)
Reference systems
Nivel de accesibilidad
acceso abierto
Condiciones de uso
http://creativecommons.org/licenses/by-nc-nd/4.0/
Repositorio
SEDICI (UNLP)
Institución
Universidad Nacional de La Plata
OAI Identificador
oai:sedici.unlp.edu.ar:10915/192036

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spelling Building on the Legacy of Astronomical StandardsKaplan, G. H.Ciencias AstronómicasAstronomical standardsInternational Astronomical Union (IAU)Reference systemsInternational cooperation and collaboration on astronomical projects of various kinds followed the improvements in communication and travel that rapidly advanced during the late 19th and early 20th centuries. The history of international astronomical standards probably dates to the International Meridian Conference in 1884 in Washington and the Paris Conference of 1896. The formation of the IAU in 1919 institutionalized international cooperation in astronomy. Before the midpoint of the 20th century, only a few organizations worldwide, mostly the national observatories, had the capabilities to compute and distribute the data for fundamental astronomy, such as the celestial coordinates of the Sun, Moon, and planets; sidereal time; eclipse circumstances; apparent places of stars; the data needed for celestial navigation; and precise time. The situation changed after World War II as electronic computers became available at scientific institutions and more precise observational techniques were invented, some involving spaced-based instruments. As many common astronomical computations became more "democratized” in the latter part of the 20th century, IAU standards, as well as those from other institutions, such as the IUGG and IERS, of necessity became more comprehensive and detailed, covering time scales, constants, reference systems, Earth orientation models, and the implementation of relativity in various astronomical computations. Thus, the evolution of astronomical standards traces the major advances in observational technology, theoretical sophistication, and computing power that have defined our science for the last century.Facultad de Ciencias Astronómicas y Geofísicas2025-08info:eu-repo/semantics/conferenceObjectinfo:eu-repo/semantics/publishedVersionResumenhttp://purl.org/coar/resource_type/c_5794info:ar-repo/semantics/documentoDeConferenciaapplication/pdfhttp://sedici.unlp.edu.ar/handle/10915/192036enginfo:eu-repo/semantics/reference/url/https://sedici.unlp.edu.ar/handle/10915/190232info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-nd/4.0/Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2026-03-31T12:41:57Zoai:sedici.unlp.edu.ar:10915/192036Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292026-03-31 12:41:57.993SEDICI (UNLP) - Universidad Nacional de La Platafalse
dc.title.none.fl_str_mv Building on the Legacy of Astronomical Standards
title Building on the Legacy of Astronomical Standards
spellingShingle Building on the Legacy of Astronomical Standards
Kaplan, G. H.
Ciencias Astronómicas
Astronomical standards
International Astronomical Union (IAU)
Reference systems
title_short Building on the Legacy of Astronomical Standards
title_full Building on the Legacy of Astronomical Standards
title_fullStr Building on the Legacy of Astronomical Standards
title_full_unstemmed Building on the Legacy of Astronomical Standards
title_sort Building on the Legacy of Astronomical Standards
dc.creator.none.fl_str_mv Kaplan, G. H.
author Kaplan, G. H.
author_facet Kaplan, G. H.
author_role author
dc.subject.none.fl_str_mv Ciencias Astronómicas
Astronomical standards
International Astronomical Union (IAU)
Reference systems
topic Ciencias Astronómicas
Astronomical standards
International Astronomical Union (IAU)
Reference systems
dc.description.none.fl_txt_mv International cooperation and collaboration on astronomical projects of various kinds followed the improvements in communication and travel that rapidly advanced during the late 19th and early 20th centuries. The history of international astronomical standards probably dates to the International Meridian Conference in 1884 in Washington and the Paris Conference of 1896. The formation of the IAU in 1919 institutionalized international cooperation in astronomy. Before the midpoint of the 20th century, only a few organizations worldwide, mostly the national observatories, had the capabilities to compute and distribute the data for fundamental astronomy, such as the celestial coordinates of the Sun, Moon, and planets; sidereal time; eclipse circumstances; apparent places of stars; the data needed for celestial navigation; and precise time. The situation changed after World War II as electronic computers became available at scientific institutions and more precise observational techniques were invented, some involving spaced-based instruments. As many common astronomical computations became more "democratized” in the latter part of the 20th century, IAU standards, as well as those from other institutions, such as the IUGG and IERS, of necessity became more comprehensive and detailed, covering time scales, constants, reference systems, Earth orientation models, and the implementation of relativity in various astronomical computations. Thus, the evolution of astronomical standards traces the major advances in observational technology, theoretical sophistication, and computing power that have defined our science for the last century.
Facultad de Ciencias Astronómicas y Geofísicas
description International cooperation and collaboration on astronomical projects of various kinds followed the improvements in communication and travel that rapidly advanced during the late 19th and early 20th centuries. The history of international astronomical standards probably dates to the International Meridian Conference in 1884 in Washington and the Paris Conference of 1896. The formation of the IAU in 1919 institutionalized international cooperation in astronomy. Before the midpoint of the 20th century, only a few organizations worldwide, mostly the national observatories, had the capabilities to compute and distribute the data for fundamental astronomy, such as the celestial coordinates of the Sun, Moon, and planets; sidereal time; eclipse circumstances; apparent places of stars; the data needed for celestial navigation; and precise time. The situation changed after World War II as electronic computers became available at scientific institutions and more precise observational techniques were invented, some involving spaced-based instruments. As many common astronomical computations became more "democratized” in the latter part of the 20th century, IAU standards, as well as those from other institutions, such as the IUGG and IERS, of necessity became more comprehensive and detailed, covering time scales, constants, reference systems, Earth orientation models, and the implementation of relativity in various astronomical computations. Thus, the evolution of astronomical standards traces the major advances in observational technology, theoretical sophistication, and computing power that have defined our science for the last century.
publishDate 2025
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Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0)
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