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The κ-Cygnid Meteor Shower and Its Relationship with Near-Earth Asteroids

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dc.contributor.author Sergienko M.V.
dc.contributor.author Sokolova M.G.
dc.contributor.author Nefedyev Y.A.
dc.contributor.author Andreev A.O.
dc.date.accessioned 2021-02-25T20:37:14Z
dc.date.available 2021-02-25T20:37:14Z
dc.date.issued 2020
dc.identifier.issn 1063-7729
dc.identifier.uri https://dspace.kpfu.ru/xmlui/handle/net/162057
dc.description.abstract © 2020, Pleiades Publishing, Ltd. Abstract—: This study is focused on the relationships between the κ-Cygnid meteor shower and different groups of asteroids crossing the Earth’s orbit (the so-called near-Earth objects (NEOs)). The analysis is based on the visible structure of the meteor shower and a comprehensive strategy for estimating the proximity of orbits of two bodies. The κ-Cygnid meteor shower (abbreviated as KCG) is observed from August 3 to August 25 every year; it is classified as a minor shower, and the size of its mean orbit is around 3.2 AU, while the geocentric velocity is 20.9 km/s. No parent body (PB) of the shower has been found among comets so far. Relationships between the shower and asteroids, as potential PBs of the shower, are under active examination; some hypotheses on this subject can be found on the website of the Meteor Data Center (MDC) of the International Astronomical Union (IAU).
dc.relation.ispartofseries Astronomy Reports
dc.title The κ-Cygnid Meteor Shower and Its Relationship with Near-Earth Asteroids
dc.type Article
dc.relation.ispartofseries-issue 12
dc.relation.ispartofseries-volume 64
dc.collection Публикации сотрудников КФУ
dc.relation.startpage 1087
dc.source.id SCOPUS10637729-2020-64-12-SID85098503430


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  • Публикации сотрудников КФУ Scopus [24551]
    Коллекция содержит публикации сотрудников Казанского федерального (до 2010 года Казанского государственного) университета, проиндексированные в БД Scopus, начиная с 1970г.

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