A new orbit for comet C/1861 J1 (Great comet of 1861)

Autores
Branham, Richard Lacy
Año de publicación
2014
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
A new orbit is calculated for Comet C/1861 J1 (Great comet of 1861) to replace Kreutz?s orbit of 1880. The orbit is based upon 2,362 observations, 1,198 in right ascension and 1,164 in declination, made between May of 1861 and March of 1862. The comet?s period of 364.96 ± 0.51 yr differs significantly from Kreutz?s period of 409 yr. This orbit is linked with one calculated from 5 observations made in the Far East in 1500, possibly of the Great comet, by imposing boundary conditions on the differential equations of motion. The linked orbit indicates a period of 361.3 yr. This increases the probability that the Great comet is indeed the comet observed in 1500. Although the residuals are relatively random (16.0% probability of randomness), post-perihelion residuals are less random indicating possible deviations from Keplerian motion such as systematics error or nongravitational forces.
Fil: Branham, Richard Lacy. Consejo Nacional de Investigaciones Científicas y Técnicas. Científico Tecnológico Mendoza. Instituto Argentino de Nivología, Glaciología y Ciencias Ambientales; Argentina
Materia
CELESTIAL MECHANICS
COMETS: INDIVIDUAL (C/1861 J1)
METHODS: DATA ANLYSIS
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/9410
Acceder
id CONICETDig_04580c7ca0274f6378ac5e881c4ea04b
oai_identifier_str oai:ri.conicet.gov.ar:11336/9410
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling A new orbit for comet C/1861 J1 (Great comet of 1861)Branham, Richard LacyCELESTIAL MECHANICSCOMETS: INDIVIDUAL (C/1861 J1)METHODS: DATA ANLYSIShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1A new orbit is calculated for Comet C/1861 J1 (Great comet of 1861) to replace Kreutz?s orbit of 1880. The orbit is based upon 2,362 observations, 1,198 in right ascension and 1,164 in declination, made between May of 1861 and March of 1862. The comet?s period of 364.96 ± 0.51 yr differs significantly from Kreutz?s period of 409 yr. This orbit is linked with one calculated from 5 observations made in the Far East in 1500, possibly of the Great comet, by imposing boundary conditions on the differential equations of motion. The linked orbit indicates a period of 361.3 yr. This increases the probability that the Great comet is indeed the comet observed in 1500. Although the residuals are relatively random (16.0% probability of randomness), post-perihelion residuals are less random indicating possible deviations from Keplerian motion such as systematics error or nongravitational forces.Fil: Branham, Richard Lacy. Consejo Nacional de Investigaciones Científicas y Técnicas. Científico Tecnológico Mendoza. Instituto Argentino de Nivología, Glaciología y Ciencias Ambientales; ArgentinaUniversidad Nacional Autónoma de México. Instituto de Astronomía2014-04info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/9410Branham, Richard Lacy; A new orbit for comet C/1861 J1 (Great comet of 1861); Universidad Nacional Autónoma de México. Instituto de Astronomía; Revista Mexicana de Astronomía y Astrofísica; 50; 4-2014; 109-1180185-1101enginfo:eu-repo/semantics/altIdentifier/url/http://www.astroscu.unam.mx/rmaa/RMxAA..50-1/PDF/RMxAA..50-1_rbranham.pdfinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-22T11:20:24Zoai:ri.conicet.gov.ar:11336/9410instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-10-22 11:20:25.011CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv A new orbit for comet C/1861 J1 (Great comet of 1861)
title A new orbit for comet C/1861 J1 (Great comet of 1861)
spellingShingle A new orbit for comet C/1861 J1 (Great comet of 1861)
Branham, Richard Lacy
CELESTIAL MECHANICS
COMETS: INDIVIDUAL (C/1861 J1)
METHODS: DATA ANLYSIS
title_short A new orbit for comet C/1861 J1 (Great comet of 1861)
title_full A new orbit for comet C/1861 J1 (Great comet of 1861)
title_fullStr A new orbit for comet C/1861 J1 (Great comet of 1861)
title_full_unstemmed A new orbit for comet C/1861 J1 (Great comet of 1861)
title_sort A new orbit for comet C/1861 J1 (Great comet of 1861)
dc.creator.none.fl_str_mv Branham, Richard Lacy
author Branham, Richard Lacy
author_facet Branham, Richard Lacy
author_role author
dc.subject.none.fl_str_mv CELESTIAL MECHANICS
COMETS: INDIVIDUAL (C/1861 J1)
METHODS: DATA ANLYSIS
topic CELESTIAL MECHANICS
COMETS: INDIVIDUAL (C/1861 J1)
METHODS: DATA ANLYSIS
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv A new orbit is calculated for Comet C/1861 J1 (Great comet of 1861) to replace Kreutz?s orbit of 1880. The orbit is based upon 2,362 observations, 1,198 in right ascension and 1,164 in declination, made between May of 1861 and March of 1862. The comet?s period of 364.96 ± 0.51 yr differs significantly from Kreutz?s period of 409 yr. This orbit is linked with one calculated from 5 observations made in the Far East in 1500, possibly of the Great comet, by imposing boundary conditions on the differential equations of motion. The linked orbit indicates a period of 361.3 yr. This increases the probability that the Great comet is indeed the comet observed in 1500. Although the residuals are relatively random (16.0% probability of randomness), post-perihelion residuals are less random indicating possible deviations from Keplerian motion such as systematics error or nongravitational forces.
Fil: Branham, Richard Lacy. Consejo Nacional de Investigaciones Científicas y Técnicas. Científico Tecnológico Mendoza. Instituto Argentino de Nivología, Glaciología y Ciencias Ambientales; Argentina
description A new orbit is calculated for Comet C/1861 J1 (Great comet of 1861) to replace Kreutz?s orbit of 1880. The orbit is based upon 2,362 observations, 1,198 in right ascension and 1,164 in declination, made between May of 1861 and March of 1862. The comet?s period of 364.96 ± 0.51 yr differs significantly from Kreutz?s period of 409 yr. This orbit is linked with one calculated from 5 observations made in the Far East in 1500, possibly of the Great comet, by imposing boundary conditions on the differential equations of motion. The linked orbit indicates a period of 361.3 yr. This increases the probability that the Great comet is indeed the comet observed in 1500. Although the residuals are relatively random (16.0% probability of randomness), post-perihelion residuals are less random indicating possible deviations from Keplerian motion such as systematics error or nongravitational forces.
publishDate 2014
dc.date.none.fl_str_mv 2014-04
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/9410
Branham, Richard Lacy; A new orbit for comet C/1861 J1 (Great comet of 1861); Universidad Nacional Autónoma de México. Instituto de Astronomía; Revista Mexicana de Astronomía y Astrofísica; 50; 4-2014; 109-118
0185-1101
url http://hdl.handle.net/11336/9410
identifier_str_mv Branham, Richard Lacy; A new orbit for comet C/1861 J1 (Great comet of 1861); Universidad Nacional Autónoma de México. Instituto de Astronomía; Revista Mexicana de Astronomía y Astrofísica; 50; 4-2014; 109-118
0185-1101
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/http://www.astroscu.unam.mx/rmaa/RMxAA..50-1/PDF/RMxAA..50-1_rbranham.pdf
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
dc.publisher.none.fl_str_mv Universidad Nacional Autónoma de México. Instituto de Astronomía
publisher.none.fl_str_mv Universidad Nacional Autónoma de México. Instituto de Astronomía
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
_version_ 1846781694755995648
score 12.982451

Publicaciones similares