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
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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
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Czech description
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Classification
Type
D - Article in proceedings
CEP classification
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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
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e-ISSN
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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
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