Meteor shower output caused by comet 15P/Finlay

International audience Theoretical work on the meteoroid stream ejected by comet 15P/Finlay predicts multiple outbursts in 2021 in agreement with previous authors. This work predicts the first outburst to happen around 2021-09-29T08:35 UT, for a radiant located at α = 260.8 deg δ = −57.4 deg and wil...

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Main Authors: Vaubaillon, J, Egal, A, Desmars, J, Baillie, Kevin
Other Authors: Institut de Mécanique Céleste et de Calcul des Ephémérides (IMCCE), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université de Lille-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)
Format: Article in Journal/Newspaper
Language:English
Published: HAL CCSD 2020
Subjects:
Online Access:https://hal.science/hal-03017579
https://hal.science/hal-03017579/document
https://hal.science/hal-03017579/file/Vaubaillon_2020_15PFinlayMeteors.pdf
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spelling ftunivparis:oai:HAL:hal-03017579v1 2023-06-11T04:06:57+02:00 Meteor shower output caused by comet 15P/Finlay Vaubaillon, J Egal, A Desmars, J Baillie, Kevin Institut de Mécanique Céleste et de Calcul des Ephémérides (IMCCE) Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université de Lille-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS) 2020 https://hal.science/hal-03017579 https://hal.science/hal-03017579/document https://hal.science/hal-03017579/file/Vaubaillon_2020_15PFinlayMeteors.pdf en eng HAL CCSD International Meteor Organization hal-03017579 https://hal.science/hal-03017579 https://hal.science/hal-03017579/document https://hal.science/hal-03017579/file/Vaubaillon_2020_15PFinlayMeteors.pdf info:eu-repo/semantics/OpenAccess ISSN: 1016-3115 WGN, Journal of the International Meteor Organization https://hal.science/hal-03017579 WGN, Journal of the International Meteor Organization, 2020 [SDU.ASTR.EP]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP] info:eu-repo/semantics/article Journal articles 2020 ftunivparis 2023-05-03T16:24:14Z International audience Theoretical work on the meteoroid stream ejected by comet 15P/Finlay predicts multiple outbursts in 2021 in agreement with previous authors. This work predicts the first outburst to happen around 2021-09-29T08:35 UT, for a radiant located at α = 260.8 deg δ = −57.4 deg and will be best visible from New-Zealand. The second will happen on 2021-10-07T 00:35 UT, followed by a third on 2021-10-07T03:55 UT. They will be best visible from the tip of Antarctica or Tierra Del Fuego (Argentina). The level of each outburst is evaluated based on the photometry of the comet, which is known to have experienced some outbursts, but is less certain than the timing of each event. Article in Journal/Newspaper Antarc* Antarctica Tierra del Fuego Université de Paris: Portail HAL Argentina New Zealand
institution Open Polar
collection Université de Paris: Portail HAL
op_collection_id ftunivparis
language English
topic [SDU.ASTR.EP]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP]
spellingShingle [SDU.ASTR.EP]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP]
Vaubaillon, J
Egal, A
Desmars, J
Baillie, Kevin
Meteor shower output caused by comet 15P/Finlay
topic_facet [SDU.ASTR.EP]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP]
description International audience Theoretical work on the meteoroid stream ejected by comet 15P/Finlay predicts multiple outbursts in 2021 in agreement with previous authors. This work predicts the first outburst to happen around 2021-09-29T08:35 UT, for a radiant located at α = 260.8 deg δ = −57.4 deg and will be best visible from New-Zealand. The second will happen on 2021-10-07T 00:35 UT, followed by a third on 2021-10-07T03:55 UT. They will be best visible from the tip of Antarctica or Tierra Del Fuego (Argentina). The level of each outburst is evaluated based on the photometry of the comet, which is known to have experienced some outbursts, but is less certain than the timing of each event.
author2 Institut de Mécanique Céleste et de Calcul des Ephémérides (IMCCE)
Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université de Lille-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)
format Article in Journal/Newspaper
author Vaubaillon, J
Egal, A
Desmars, J
Baillie, Kevin
author_facet Vaubaillon, J
Egal, A
Desmars, J
Baillie, Kevin
author_sort Vaubaillon, J
title Meteor shower output caused by comet 15P/Finlay
title_short Meteor shower output caused by comet 15P/Finlay
title_full Meteor shower output caused by comet 15P/Finlay
title_fullStr Meteor shower output caused by comet 15P/Finlay
title_full_unstemmed Meteor shower output caused by comet 15P/Finlay
title_sort meteor shower output caused by comet 15p/finlay
publisher HAL CCSD
publishDate 2020
url https://hal.science/hal-03017579
https://hal.science/hal-03017579/document
https://hal.science/hal-03017579/file/Vaubaillon_2020_15PFinlayMeteors.pdf
geographic Argentina
New Zealand
geographic_facet Argentina
New Zealand
genre Antarc*
Antarctica
Tierra del Fuego
genre_facet Antarc*
Antarctica
Tierra del Fuego
op_source ISSN: 1016-3115
WGN, Journal of the International Meteor Organization
https://hal.science/hal-03017579
WGN, Journal of the International Meteor Organization, 2020
op_relation hal-03017579
https://hal.science/hal-03017579
https://hal.science/hal-03017579/document
https://hal.science/hal-03017579/file/Vaubaillon_2020_15PFinlayMeteors.pdf
op_rights info:eu-repo/semantics/OpenAccess
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