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Estimation of the flux density of galactic comets in the Orion-Cygnus branch based on number of shield volcanoes on Venus, craters on Mars and marine basins on the Moon

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dc.contributor.author Barenbaum A.A.
dc.contributor.author Shpekin M.I.
dc.date.accessioned 2022-02-09T20:39:13Z
dc.date.available 2022-02-09T20:39:13Z
dc.date.issued 2021
dc.identifier.issn 1742-6588
dc.identifier.uri https://dspace.kpfu.ru/xmlui/handle/net/169561
dc.description.abstract Based on data on shield volcanoes of Venus and the distribution of craters on Mars and sea basins on the Moon, the flux density of galactic comets in the Orion-Cygnus branch was calculated. The comets flux density is 5 × 10-10 year-1 km-2. This value was used to estimate the number, energy and fallings frequency of galactic comets on terrestrial planets in the period from ˜ 5 to 1 million years ago. The article shows, that the falls of such comets can explain the phenomena of newest uplifts of Earth's crust and young volcanism on Earth, the appearance of shield volcanoes on Venus, the asymmetric structure of Mars, as well as origin of large craters, seas and mascons on the Moon, Mars and Mercury. A hypothesis of formation on the Moon of the South Pole-Aitken basin by galactic comets is proposed.
dc.relation.ispartofseries Journal of Physics: Conference Series
dc.title Estimation of the flux density of galactic comets in the Orion-Cygnus branch based on number of shield volcanoes on Venus, craters on Mars and marine basins on the Moon
dc.type Conference Proceeding
dc.relation.ispartofseries-issue 1
dc.relation.ispartofseries-volume 1787
dc.collection Публикации сотрудников КФУ
dc.source.id SCOPUS17426588-2021-1787-1-SID85102347478


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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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