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Radiants and orbits of Geminids observed by the European Fireball Network

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F23%3A00604840" target="_blank" >RIV/67985815:_____/23:00604840 - isvavai.cz</a>

  • Result on the web

    <a href="http://ftp.dutch-meteor-society.nl/Publications-General/Radiants%20and%20orbits%20of%20Geminids%20observed%20by%20the%20European%20Network.pdf" target="_blank" >http://ftp.dutch-meteor-society.nl/Publications-General/Radiants%20and%20orbits%20of%20Geminids%20observed%20by%20the%20European%20Network.pdf</a>

  • DOI - Digital Object Identifier

Alternative languages

  • Result language

    angličtina

  • Original language name

    Radiants and orbits of Geminids observed by the European Fireball Network

  • Original language description

    Precise radiants and orbits of bright Geminid meteors observed by the digital cameras of the European Fireball Network in the recent years are presented. When corrected for the radiant motion, most individual radiants fall within an area of a diameter of one degree. The radiants in the east-south-eastern part of that area belong to meteoroids with smaller semimajor axes and larger arguments of perihelia. We can distinguish a core of the stream with semimajor axes between 1.25 AU and 1.30 AU and a wing with semimajor axes up to 1.39 AU. The core is more concentrated in eccentricities and perihelion distances than the wing. Both core and wing meteoroids are encountered during the whole duration of the shower. The wing contains smaller meteoroids on average. Therefore, an opposite trend than expected from the action of the Poynting–Robertson effect, which decreases semimajor axes of small meteoroids, is present in Geminids, as noted already by (Spurný 1993). We hope that our new observations together with a modeling effort will shed light on the formation and evolution of the stream.

  • Czech name

  • Czech description

Classification

  • Type

    D - Article in proceedings

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

    <a href="/en/project/GX19-26232X" target="_blank" >GX19-26232X: Compositional and orbital mapping of meteoroid sources in the Solar System</a><br>

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2023

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Article name in the collection

    Proceedings of the International Meteor Conference

  • ISBN

    978-2-87355-035-6

  • ISSN

  • e-ISSN

  • Number of pages

    4

  • Pages from-to

    34-37

  • Publisher name

    International Meteor Organization

  • Place of publication

    Mechelen

  • Event location

    Poroszlo

  • Event date

    Sep 29, 2022

  • Type of event by nationality

    WRD - Celosvětová akce

  • UT code for WoS article