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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34T/47A5SAL
Repositorysid.inpe.br/mtc-m21d/2022/07.18.12.57
Last Update2022:07.18.12.57.03 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21d/2022/07.18.12.57.03
Metadata Last Update2023:01.03.16.46.10 (UTC) administrator
DOI10.1093/mnras/stac1699
ISSN0035-8711
1365-2966
Citation KeyCarrubaAljDomHuaMar:2022:IdPoSt
TitleIdentifying the population of stable nu(6) resonant asteroids using large data bases
Year2022
MonthJuly
Access Date2024, May 14
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size5020 KiB
2. Context
Author1 Carruba, Valerio
2 Aljbaae, Safwan
3 Domingos, R. C.
4 Huaman, M.
5 Martins, B.
Group1
2 DIMEC-CGCE-INPE-MCTI-GOV-BR
Affiliation1 Universidade Estadual Paulista (UNESP)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Universidade Estadual Paulista (UNESP)
4 Universidad Tecnoloóica del Perú (UTP)
5 Universidade Estadual Paulista (UNESP)
Author e-Mail Address1 valerio.carruba@unesp.br
2 safwan.aljbaae@gmail.com
JournalMonthly Notices of the Royal Astronomical Society
Volume514
Number4
Pages4803-4815
Secondary MarkA1_QUÍMICA A1_INTERDISCIPLINAR A1_GEOCIÊNCIAS A1_ENGENHARIAS_III A2_MATEMÁTICA_/_PROBABILIDADE_E_ESTATÍSTICA A2_ASTRONOMIA_/_FÍSICA B2_ENSINO B5_ENGENHARIAS_IV
History (UTC)2022-07-18 12:57:03 :: simone -> administrator ::
2022-07-18 12:57:04 :: administrator -> simone :: 2022
2022-07-18 12:58:05 :: simone -> administrator :: 2022
2023-01-03 16:46:10 :: administrator -> simone :: 2022
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
Keywordsmethods: data analysis
methods: statistical
minor planets
asteroids: general
AbstractLarge observational surveys, like those that will be conducted at the Vera C. Rubin Observatory, are expected to discover up to one million new asteroids in the first year of operation. This will more than double the data base of known asteroids. New methods will be needed to handle the large influx of data. Here, we tested some of these new approaches by studying the population of asteroids on stable orbits inside the.6 secular resonance. This resonance is one of the strongest mechanisms for destabilizing the orbits of main-belt bodies and producing Near-Earth Asteroids. Yet, stable orbital configurations where the asteroid pericenter is either aligned or anti-aligned with that of Saturn exist inside the resonance. The population of stable nu(6) resonators is now the largest population of asteroids in stable orbits inside a secular resonance. Here, we obtained the largest sample of asteroids' proper elements ever used. Clustering methods and the use of machine learning algorithms permitted the identification of the known asteroid families crossed by the.6 resonance and of two entirely new groups: the Tiffanykapler and the 138605 QW177 families. The Tiffanykapler family is the first young asteroid family ever found in a linear secular resonance, with an age of 3.0 +/- 1.2 My and an ejection velocity field parameter of V-EJ = 15(-3)(+6) m s(-1). We identify a population of high-eccentricity objects around the Tina family that may be the first example of an asteroid family 'resonant halo'.
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4. Conditions of access and use
data URLhttp://mtc-m21d.sid.inpe.br/ibi/8JMKD3MGP3W34T/47A5SAL
zipped data URLhttp://mtc-m21d.sid.inpe.br/zip/8JMKD3MGP3W34T/47A5SAL
Languageen
User Groupsimone
Reader Groupadministrator
simone
Visibilityshown
Archiving Policyallowpublisher allowfinaldraft
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/46KTFK8
DisseminationWEBSCI; PORTALCAPES; MGA; COMPENDEX.
Host Collectionurlib.net/www/2021/06.04.03.40
6. Notes
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