KFU. Card publication. Genetic analysis of parameters of Near Earth Asteroids for determining parent bodies of meteoroid streams

KAZAN
FEDERAL UNIVERSITY

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GENETIC ANALYSIS OF PARAMETERS OF NEAR EARTH ASTEROIDS FOR DETERMINING PARENT BODIES OF METEOROID STREAMS

Form of presentation

Articles in international journals and collections

Year of publication

2017

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Authors, employees of KFU

Nefedev Yuriy Anatolevich, author

Authors, postgraduates KFU

Andreev Aleksey Olegovich, postgraduate kfu

Bibliographic description in the original language

M. Sokolova M. Sergienko Y. Nefedyev A. Andreev L. Nefediev. Genetic analysis of parameters of Near Earth Asteroids for determining parent bodies of meteoroid streams. Advances in Space Research https://doi.org/10.1016/j.asr. Indexed Thursday, November 23 2017 | Published Wednesday, November 1 2017

Annotation

The present paper is focusing on determining genetic connections between small bodies of the Solar system and their parent bodies (PB) on the basis of analysis of Near Earth Asteroids (NEAs) parameters. In order to search for parent bodies of meteoroid streams, the asteroid groups, including Atira, Apollo, Amor and Aten, have been investigated. Currently, it is considered that surface of asteroids with elongated orbit is exposed to temperature fall: in perihelion it is heated and in aphelion it is cooled. At small orbital periods around the Sun (about 2-4 years) this may lead to formation of meteoroid clusters. On the basis of comparative analysis of orbit, size and chemical and mineralogical composition of NEAs, it is found that asteroids from Apollo group are most likely to be parent bodies of the studied meteoroid streams.

Keywords

small bodies of the Solar system , Near Earth Asteroids

The name of the journal

ADVANCES IN SPACE RESEARCH

Please use this ID to quote from or refer to the card

https://repository.kpfu.ru/eng/?p_id=168290&p_lang=2

Full metadata record

Field DC	Value	Language
dc.contributor.author	Nefedev Yuriy Anatolevich	ru_RU
dc.contributor.author	Andreev Aleksey Olegovich	ru_RU
dc.date.accessioned	2017-01-01T00:00:00Z	ru_RU
dc.date.available	2017-01-01T00:00:00Z	ru_RU
dc.date.issued	2017	ru_RU
dc.identifier.citation	M. Sokolova M. Sergienko Y. Nefedyev A. Andreev L. Nefediev. Genetic analysis of parameters of Near Earth Asteroids for determining parent bodies of meteoroid streams. Advances in Space Research https://doi.org/10.1016/j.asr. Indexed Thursday, November 23 2017 \| Published Wednesday, November 1 2017	ru_RU
dc.identifier.uri	https://repository.kpfu.ru/eng/?p_id=168290&p_lang=2	ru_RU
dc.description.abstract	ADVANCES IN SPACE RESEARCH	ru_RU
dc.description.abstract	The present paper is focusing on determining genetic connections between small bodies of the Solar system and their parent bodies (PB) on the basis of analysis of Near Earth Asteroids (NEAs) parameters. In order to search for parent bodies of meteoroid streams, the asteroid groups, including Atira, Apollo, Amor and Aten, have been investigated. Currently, it is considered that surface of asteroids with elongated orbit is exposed to temperature fall: in perihelion it is heated and in aphelion it is cooled. At small orbital periods around the Sun (about 2-4 years) this may lead to formation of meteoroid clusters. On the basis of comparative analysis of orbit, size and chemical and mineralogical composition of NEAs, it is found that asteroids from Apollo group are most likely to be parent bodies of the studied meteoroid streams.	ru_RU
dc.language.iso	ru	ru_RU
dc.subject	small bodies of the Solar system	ru_RU
dc.subject	Near Earth Asteroids	ru_RU
dc.title	Genetic analysis of parameters of Near Earth Asteroids for determining parent bodies of meteoroid streams	ru_RU
dc.type	Articles in international journals and collections	ru_RU