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The Chant Meteor Procession of 1913 – Towards a Descriptive Model

Received: 5 April 2018     Accepted: 19 May 2018     Published: 28 June 2018
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Abstract

From an observational standpoint the Chant Meteor Procession of 9 February, 1913 is particularly remarkable, being especially noted for its long ground track of at least 15,000 km, and for the slow motion and near parallel to the horizon paths adopted by the meteors. The circumstances surrounding the Procession are re-considered here in terms of the successive entry of multiple meteoroid clusters. These clusters are in turn considered to be derived from a temporarily captured Earth orbiting object that has undergone disaggregation. It is suggested that the general observational accounts of the Procession can be explained through the sequential entry of multiple meteoroid clusters that moved through the Earth’s atmosphere on grazing-incident trajectories. It is further suggested that the parent object to the Procession, prior to its breakup, may have been no more than 3 to 4-m across.

Published in American Journal of Astronomy and Astrophysics (Volume 6, Issue 2)
DOI 10.11648/j.ajaa.20180602.11
Page(s) 31-38
Creative Commons

This is an Open Access article, distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted use, distribution and reproduction in any medium or format, provided the original work is properly cited.

Copyright

Copyright © The Author(s), 2018. Published by Science Publishing Group

Keywords

Natural Earth Satellites, Meteoroid Ablation, Grazing Atmospheric Flight

References
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Cite This Article
  • APA Style

    Martin Beech, Mark Comte. (2018). The Chant Meteor Procession of 1913 – Towards a Descriptive Model. American Journal of Astronomy and Astrophysics, 6(2), 31-38. https://doi.org/10.11648/j.ajaa.20180602.11

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    ACS Style

    Martin Beech; Mark Comte. The Chant Meteor Procession of 1913 – Towards a Descriptive Model. Am. J. Astron. Astrophys. 2018, 6(2), 31-38. doi: 10.11648/j.ajaa.20180602.11

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    AMA Style

    Martin Beech, Mark Comte. The Chant Meteor Procession of 1913 – Towards a Descriptive Model. Am J Astron Astrophys. 2018;6(2):31-38. doi: 10.11648/j.ajaa.20180602.11

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  • @article{10.11648/j.ajaa.20180602.11,
      author = {Martin Beech and Mark Comte},
      title = {The Chant Meteor Procession of 1913 – Towards a Descriptive Model},
      journal = {American Journal of Astronomy and Astrophysics},
      volume = {6},
      number = {2},
      pages = {31-38},
      doi = {10.11648/j.ajaa.20180602.11},
      url = {https://doi.org/10.11648/j.ajaa.20180602.11},
      eprint = {https://article.sciencepublishinggroup.com/pdf/10.11648.j.ajaa.20180602.11},
      abstract = {From an observational standpoint the Chant Meteor Procession of 9 February, 1913 is particularly remarkable, being especially noted for its long ground track of at least 15,000 km, and for the slow motion and near parallel to the horizon paths adopted by the meteors. The circumstances surrounding the Procession are re-considered here in terms of the successive entry of multiple meteoroid clusters. These clusters are in turn considered to be derived from a temporarily captured Earth orbiting object that has undergone disaggregation. It is suggested that the general observational accounts of the Procession can be explained through the sequential entry of multiple meteoroid clusters that moved through the Earth’s atmosphere on grazing-incident trajectories. It is further suggested that the parent object to the Procession, prior to its breakup, may have been no more than 3 to 4-m across.},
     year = {2018}
    }
    

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    JF  - American Journal of Astronomy and Astrophysics
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    AB  - From an observational standpoint the Chant Meteor Procession of 9 February, 1913 is particularly remarkable, being especially noted for its long ground track of at least 15,000 km, and for the slow motion and near parallel to the horizon paths adopted by the meteors. The circumstances surrounding the Procession are re-considered here in terms of the successive entry of multiple meteoroid clusters. These clusters are in turn considered to be derived from a temporarily captured Earth orbiting object that has undergone disaggregation. It is suggested that the general observational accounts of the Procession can be explained through the sequential entry of multiple meteoroid clusters that moved through the Earth’s atmosphere on grazing-incident trajectories. It is further suggested that the parent object to the Procession, prior to its breakup, may have been no more than 3 to 4-m across.
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Author Information
  • Campion College at the University of Regina, Saskatchewan, Canada

  • Department of Physics, The University of Regina, Saskatchewan, Canada

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