Dynamics of Asteroid 3200 Phaethon Under Overlap of Different Resonances
The paper is focused on studying the motion of asteroid 3200 Phaethon which approached the Earth in December 2017. We consider the dynamics of asteroid 3200 Phaethon, reveal its encounters with planets, mean motion and secular resonances, and estimate the predictability time and the causes of chaoti...
Gespeichert in:
Veröffentlicht in: | Solar system research 2019-05, Vol.53 (3), p.215-223 |
---|---|
Hauptverfasser: | , |
Format: | Artikel |
Sprache: | eng |
Schlagworte: | |
Online-Zugang: | Volltext |
Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
container_end_page | 223 |
---|---|
container_issue | 3 |
container_start_page | 215 |
container_title | Solar system research |
container_volume | 53 |
creator | Galushina, T. Yu Sambarov, G. E. |
description | The paper is focused on studying the motion of asteroid 3200 Phaethon which approached the Earth in December 2017. We consider the dynamics of asteroid 3200 Phaethon, reveal its encounters with planets, mean motion and secular resonances, and estimate the predictability time and the causes of chaoticity. A peculiar feature in the dynamics of the object is that it passes through the unstable orbital resonance 3/7 with Venus and exhibits a gamut of apsidal-nodal resonances with Mercury, Venus, Earth, Mars, and Jupiter, as well as a large number of close encounters with terrestrial planets. These properties result in a chaotic character of the motion beyond a time interval between the years 1780 and 2350. |
doi_str_mv | 10.1134/S0038094619030018 |
format | Article |
fullrecord | <record><control><sourceid>crossref_sprin</sourceid><recordid>TN_cdi_crossref_primary_10_1134_S0038094619030018</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>10_1134_S0038094619030018</sourcerecordid><originalsourceid>FETCH-LOGICAL-c288t-6d5cbc9edb81858c0cb536dec94114e2f2c38ceb87f42c6b72da62d9e6bc9bea3</originalsourceid><addsrcrecordid>eNp9kM1KAzEUhYMoOFYfwF1eYPTmZzKZZWnVCoWK2vWQSW7slDZTklHo2ztDuxNc3cX5vsPlEHLP4IExIR8_AISGSipWgQBg-oJkTIHOheTikmRjnI_5NblJaTsQAKXKyGJ-DGbf2kQ7T6epx9i1jgoOQN82BvtNF-g6OIx09YNxZw4jN2-9x4ihp--YumCCxXRLrrzZJbw73wlZPz99zhb5cvXyOpsuc8u17nPlCtvYCl2jmS60BdsUQjm0lWRMIvfcCm2x0aWX3Kqm5M4o7ipUg9WgERPCTr02dilF9PUhtnsTjzWDepyi_jPF4PCTkwY2fGGst913DMOb_0i_OUFgVg</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>Dynamics of Asteroid 3200 Phaethon Under Overlap of Different Resonances</title><source>SpringerNature Journals</source><creator>Galushina, T. Yu ; Sambarov, G. E.</creator><creatorcontrib>Galushina, T. Yu ; Sambarov, G. E.</creatorcontrib><description>The paper is focused on studying the motion of asteroid 3200 Phaethon which approached the Earth in December 2017. We consider the dynamics of asteroid 3200 Phaethon, reveal its encounters with planets, mean motion and secular resonances, and estimate the predictability time and the causes of chaoticity. A peculiar feature in the dynamics of the object is that it passes through the unstable orbital resonance 3/7 with Venus and exhibits a gamut of apsidal-nodal resonances with Mercury, Venus, Earth, Mars, and Jupiter, as well as a large number of close encounters with terrestrial planets. These properties result in a chaotic character of the motion beyond a time interval between the years 1780 and 2350.</description><identifier>ISSN: 0038-0946</identifier><identifier>EISSN: 1608-3423</identifier><identifier>DOI: 10.1134/S0038094619030018</identifier><language>eng</language><publisher>Moscow: Pleiades Publishing</publisher><subject>Astronomy ; Astrophysics and Astroparticles ; Astrophysics and Cosmology ; Observations and Techniques ; Physics ; Physics and Astronomy ; Planetology</subject><ispartof>Solar system research, 2019-05, Vol.53 (3), p.215-223</ispartof><rights>Pleiades Publishing, Inc. 2019</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c288t-6d5cbc9edb81858c0cb536dec94114e2f2c38ceb87f42c6b72da62d9e6bc9bea3</citedby><cites>FETCH-LOGICAL-c288t-6d5cbc9edb81858c0cb536dec94114e2f2c38ceb87f42c6b72da62d9e6bc9bea3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.1134/S0038094619030018$$EPDF$$P50$$Gspringer$$H</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.1134/S0038094619030018$$EHTML$$P50$$Gspringer$$H</linktohtml><link.rule.ids>314,780,784,27924,27925,41488,42557,51319</link.rule.ids></links><search><creatorcontrib>Galushina, T. Yu</creatorcontrib><creatorcontrib>Sambarov, G. E.</creatorcontrib><title>Dynamics of Asteroid 3200 Phaethon Under Overlap of Different Resonances</title><title>Solar system research</title><addtitle>Sol Syst Res</addtitle><description>The paper is focused on studying the motion of asteroid 3200 Phaethon which approached the Earth in December 2017. We consider the dynamics of asteroid 3200 Phaethon, reveal its encounters with planets, mean motion and secular resonances, and estimate the predictability time and the causes of chaoticity. A peculiar feature in the dynamics of the object is that it passes through the unstable orbital resonance 3/7 with Venus and exhibits a gamut of apsidal-nodal resonances with Mercury, Venus, Earth, Mars, and Jupiter, as well as a large number of close encounters with terrestrial planets. These properties result in a chaotic character of the motion beyond a time interval between the years 1780 and 2350.</description><subject>Astronomy</subject><subject>Astrophysics and Astroparticles</subject><subject>Astrophysics and Cosmology</subject><subject>Observations and Techniques</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Planetology</subject><issn>0038-0946</issn><issn>1608-3423</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2019</creationdate><recordtype>article</recordtype><recordid>eNp9kM1KAzEUhYMoOFYfwF1eYPTmZzKZZWnVCoWK2vWQSW7slDZTklHo2ztDuxNc3cX5vsPlEHLP4IExIR8_AISGSipWgQBg-oJkTIHOheTikmRjnI_5NblJaTsQAKXKyGJ-DGbf2kQ7T6epx9i1jgoOQN82BvtNF-g6OIx09YNxZw4jN2-9x4ihp--YumCCxXRLrrzZJbw73wlZPz99zhb5cvXyOpsuc8u17nPlCtvYCl2jmS60BdsUQjm0lWRMIvfcCm2x0aWX3Kqm5M4o7ipUg9WgERPCTr02dilF9PUhtnsTjzWDepyi_jPF4PCTkwY2fGGst913DMOb_0i_OUFgVg</recordid><startdate>20190501</startdate><enddate>20190501</enddate><creator>Galushina, T. Yu</creator><creator>Sambarov, G. E.</creator><general>Pleiades Publishing</general><scope>AAYXX</scope><scope>CITATION</scope></search><sort><creationdate>20190501</creationdate><title>Dynamics of Asteroid 3200 Phaethon Under Overlap of Different Resonances</title><author>Galushina, T. Yu ; Sambarov, G. E.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c288t-6d5cbc9edb81858c0cb536dec94114e2f2c38ceb87f42c6b72da62d9e6bc9bea3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2019</creationdate><topic>Astronomy</topic><topic>Astrophysics and Astroparticles</topic><topic>Astrophysics and Cosmology</topic><topic>Observations and Techniques</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Planetology</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Galushina, T. Yu</creatorcontrib><creatorcontrib>Sambarov, G. E.</creatorcontrib><collection>CrossRef</collection><jtitle>Solar system research</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Galushina, T. Yu</au><au>Sambarov, G. E.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Dynamics of Asteroid 3200 Phaethon Under Overlap of Different Resonances</atitle><jtitle>Solar system research</jtitle><stitle>Sol Syst Res</stitle><date>2019-05-01</date><risdate>2019</risdate><volume>53</volume><issue>3</issue><spage>215</spage><epage>223</epage><pages>215-223</pages><issn>0038-0946</issn><eissn>1608-3423</eissn><abstract>The paper is focused on studying the motion of asteroid 3200 Phaethon which approached the Earth in December 2017. We consider the dynamics of asteroid 3200 Phaethon, reveal its encounters with planets, mean motion and secular resonances, and estimate the predictability time and the causes of chaoticity. A peculiar feature in the dynamics of the object is that it passes through the unstable orbital resonance 3/7 with Venus and exhibits a gamut of apsidal-nodal resonances with Mercury, Venus, Earth, Mars, and Jupiter, as well as a large number of close encounters with terrestrial planets. These properties result in a chaotic character of the motion beyond a time interval between the years 1780 and 2350.</abstract><cop>Moscow</cop><pub>Pleiades Publishing</pub><doi>10.1134/S0038094619030018</doi><tpages>9</tpages></addata></record> |
fulltext | fulltext |
identifier | ISSN: 0038-0946 |
ispartof | Solar system research, 2019-05, Vol.53 (3), p.215-223 |
issn | 0038-0946 1608-3423 |
language | eng |
recordid | cdi_crossref_primary_10_1134_S0038094619030018 |
source | SpringerNature Journals |
subjects | Astronomy Astrophysics and Astroparticles Astrophysics and Cosmology Observations and Techniques Physics Physics and Astronomy Planetology |
title | Dynamics of Asteroid 3200 Phaethon Under Overlap of Different Resonances |
url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-21T11%3A39%3A43IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-crossref_sprin&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Dynamics%20of%20Asteroid%203200%20Phaethon%20Under%20Overlap%20of%20Different%20Resonances&rft.jtitle=Solar%20system%20research&rft.au=Galushina,%20T.%20Yu&rft.date=2019-05-01&rft.volume=53&rft.issue=3&rft.spage=215&rft.epage=223&rft.pages=215-223&rft.issn=0038-0946&rft.eissn=1608-3423&rft_id=info:doi/10.1134/S0038094619030018&rft_dat=%3Ccrossref_sprin%3E10_1134_S0038094619030018%3C/crossref_sprin%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_id=info:pmid/&rfr_iscdi=true |