Origin of the 2006 Orionid Outburst
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- Sato Mikiya
- National Astronomical Observatory of Japan
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- Watanabe Jun-Ichi
- National Astronomical Observatory of Japan
Bibliographic Information
- Other Title
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- オリオン座流星群の2006年突発出現の起源
Abstract
The Orionid outburst observed in 2006 resulted in strong activity, continuing for about four days. We have found that this activity was caused by the dust trails formed by meteoroids ejected from 1P/Halley in -1265, -1197 and -910. The orbital period of these meteoroids had six times the Jovian orbital period. Therefore, the mean motion resonance with Jupiter is thought to have forced these meteoroids move close to intersect the Earth's orbit.
Journal
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- Abstracts for fall meeting of the Japanese Society for Planetary Science
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Abstracts for fall meeting of the Japanese Society for Planetary Science 2007f (0), 4-4, 2007
THE JAPANESE SOCIETY FOR PLANETARY SCIENCES
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Details 詳細情報について
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- CRID
- 1390282680534682112
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- NII Article ID
- 130004636236
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- Data Source
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- JaLC
- CiNii Articles
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- Abstract License Flag
- Disallowed