Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/1182
DC FieldValueLanguage
dc.contributor.authorHsieh, Henry H.en_US
dc.contributor.authorFitzsimmons, Alanen_US
dc.contributor.authorNovaković, Bojanen_US
dc.contributor.authorDenneau, Larryen_US
dc.contributor.authorHeinze, Aren N.en_US
dc.date.accessioned2022-09-23T17:57:47Z-
dc.date.available2022-09-23T17:57:47Z-
dc.date.issued2021-
dc.identifier.issn00191035en
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/1182-
dc.description.abstractComet P/2019 LD2 has orbital elements currently resembling those of a Jupiter Trojan, and therefore superficially appears to represent a unique opportunity to study the volatile content and active behavior of a member of this population for the first time. However, numerical integrations show that it was previously a Centaur before reaching its current Jupiter Trojan-like orbit in 2018 July, and is expected to return to being a Centaur in 2028 February, before eventually becoming a Jupiter-family comet in 2063 February. The case of P/2019 LD2 highlights the need for mechanisms to quickly and reliably dynamically classify small solar system bodies discovered in current and upcoming wide-field surveys.en_US
dc.relation.ispartofIcarusen
dc.subjectCentaursen_US
dc.subjectCometsen_US
dc.subjectDynamicsen_US
dc.subjectTrojan asteroidsen_US
dc.titleThe transient Jupiter Trojan-like orbit of P/2019 LD<inf>2</inf> (ATLAS)en_US
dc.typeArticleen_US
dc.identifier.doi10.1016/j.icarus.2020.114019-
dc.identifier.scopus2-s2.0-85089539317-
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/85089539317-
dc.contributor.affiliationAstronomyen_US
dc.description.rankM22en_US
dc.relation.volume354en
item.fulltextNo Fulltext-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.cerifentitytypePublications-
item.grantfulltextnone-
item.openairetypeArticle-
crisitem.author.deptAstronomy-
crisitem.author.orcid0000-0001-6349-6881-
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