Strong Ursid shower predicted for 2007 December 22

International audience The imminent return of comet 8P/Tuttle is expected to cause Ursid shower outbursts on December 22. There are occasional visual and forward meteor scatter observations of such outbursts from the previous perihelion return of 1994, and the one before that in 1980. In this paper,...

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Main Authors: Jenniskens, Peter, Lyytinen, Esko, Nissinen, Markku, Yrjola, I., Vaubaillon, Jérémie
Other Authors: Carl Sagan Center, SETI Institute, Kehaekukantie 3 B, 00720 Helsinki, Finland, MilliLab, VTT Technical Research Centre of Finland, Spitzer Science Center, California Institute of Technology (SSC), Institut de Mécanique Céleste et de Calcul des Ephémérides (IMCCE), Université Pierre et Marie Curie - Paris 6 (UPMC)-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-Centre National de la Recherche Scientifique (CNRS)
Format: Article in Journal/Newspaper
Language:English
Published: HAL CCSD 2007
Subjects:
Online Access:https://hal.science/hal-03732915
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spelling ftccsdartic:oai:HAL:hal-03732915v1 2024-02-27T08:38:17+00:00 Strong Ursid shower predicted for 2007 December 22 Jenniskens, Peter Lyytinen, Esko Nissinen, Markku Yrjola, I. Vaubaillon, Jérémie Carl Sagan Center, SETI Institute Kehaekukantie 3 B, 00720 Helsinki, Finland MilliLab, VTT Technical Research Centre of Finland Spitzer Science Center, California Institute of Technology (SSC) Institut de Mécanique Céleste et de Calcul des Ephémérides (IMCCE) Université Pierre et Marie Curie - Paris 6 (UPMC)-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-Centre National de la Recherche Scientifique (CNRS) 2007 https://hal.science/hal-03732915 en eng HAL CCSD International Meteor Organization hal-03732915 https://hal.science/hal-03732915 BIBCODE: 2007JIMO.35.125J ISSN: 1016-3115 WGN, Journal of the International Meteor Organization https://hal.science/hal-03732915 WGN, Journal of the International Meteor Organization, 2007, 35, pp.125-133 [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] info:eu-repo/semantics/article Journal articles 2007 ftccsdartic 2024-01-28T01:16:09Z International audience The imminent return of comet 8P/Tuttle is expected to cause Ursid shower outbursts on December 22. There are occasional visual and forward meteor scatter observations of such outbursts from the previous perihelion return of 1994, and the one before that in 1980. In this paper, we investigated what may cause these outbursts and make predictions on what to expect from dust trails ejected in the period AD 300 - 1400. Younger trails do not contribute to these Filament-type outbursts. Our knowledge of the position of older trails suffers progressively from an uncertain position of the comet in its orbit. The comet passed close to Jupiter's orbit 15 000 years ago, at which time it may have been captured. We find that Jupiter's influence at the ascending node causes some meteoroids to evolve into resonant orbits that move into Earth's path. For 2007, we expect a strong shower with a peak ZHR = 40 - 80 per hour and a duration of FWHM = 2 - 8.5 hours, centered on December 22 at 20.0 h - 22.2 h UT (most likely 21.4 h - 22.2 h UT). Peak rates in 2008 - 2012 will be less. The exact peak time and duration, as well as structure in the shower profile, can identify the age of the stream. To find out, an airborne observing campaign is being prepared that would deploy from NASA Ames Research Center in California and would observe the 2007 December 22 Ursid shower over the Canadian arctic. Article in Journal/Newspaper Arctic Archive ouverte HAL (Hyper Article en Ligne, CCSD - Centre pour la Communication Scientifique Directe) Arctic
institution Open Polar
collection Archive ouverte HAL (Hyper Article en Ligne, CCSD - Centre pour la Communication Scientifique Directe)
op_collection_id ftccsdartic
language English
topic [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
spellingShingle [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Jenniskens, Peter
Lyytinen, Esko
Nissinen, Markku
Yrjola, I.
Vaubaillon, Jérémie
Strong Ursid shower predicted for 2007 December 22
topic_facet [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
description International audience The imminent return of comet 8P/Tuttle is expected to cause Ursid shower outbursts on December 22. There are occasional visual and forward meteor scatter observations of such outbursts from the previous perihelion return of 1994, and the one before that in 1980. In this paper, we investigated what may cause these outbursts and make predictions on what to expect from dust trails ejected in the period AD 300 - 1400. Younger trails do not contribute to these Filament-type outbursts. Our knowledge of the position of older trails suffers progressively from an uncertain position of the comet in its orbit. The comet passed close to Jupiter's orbit 15 000 years ago, at which time it may have been captured. We find that Jupiter's influence at the ascending node causes some meteoroids to evolve into resonant orbits that move into Earth's path. For 2007, we expect a strong shower with a peak ZHR = 40 - 80 per hour and a duration of FWHM = 2 - 8.5 hours, centered on December 22 at 20.0 h - 22.2 h UT (most likely 21.4 h - 22.2 h UT). Peak rates in 2008 - 2012 will be less. The exact peak time and duration, as well as structure in the shower profile, can identify the age of the stream. To find out, an airborne observing campaign is being prepared that would deploy from NASA Ames Research Center in California and would observe the 2007 December 22 Ursid shower over the Canadian arctic.
author2 Carl Sagan Center, SETI Institute
Kehaekukantie 3 B, 00720 Helsinki, Finland
MilliLab, VTT Technical Research Centre of Finland
Spitzer Science Center, California Institute of Technology (SSC)
Institut de Mécanique Céleste et de Calcul des Ephémérides (IMCCE)
Université Pierre et Marie Curie - Paris 6 (UPMC)-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-Centre National de la Recherche Scientifique (CNRS)
format Article in Journal/Newspaper
author Jenniskens, Peter
Lyytinen, Esko
Nissinen, Markku
Yrjola, I.
Vaubaillon, Jérémie
author_facet Jenniskens, Peter
Lyytinen, Esko
Nissinen, Markku
Yrjola, I.
Vaubaillon, Jérémie
author_sort Jenniskens, Peter
title Strong Ursid shower predicted for 2007 December 22
title_short Strong Ursid shower predicted for 2007 December 22
title_full Strong Ursid shower predicted for 2007 December 22
title_fullStr Strong Ursid shower predicted for 2007 December 22
title_full_unstemmed Strong Ursid shower predicted for 2007 December 22
title_sort strong ursid shower predicted for 2007 december 22
publisher HAL CCSD
publishDate 2007
url https://hal.science/hal-03732915
geographic Arctic
geographic_facet Arctic
genre Arctic
genre_facet Arctic
op_source ISSN: 1016-3115
WGN, Journal of the International Meteor Organization
https://hal.science/hal-03732915
WGN, Journal of the International Meteor Organization, 2007, 35, pp.125-133
op_relation hal-03732915
https://hal.science/hal-03732915
BIBCODE: 2007JIMO.35.125J
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