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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34T/4527D58
Repositorysid.inpe.br/mtc-m21d/2021/07.02.12.37
Last Update2021:07.02.12.37.47 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21d/2021/07.02.12.37.47
Metadata Last Update2022:04.03.23.14.01 (UTC) administrator
DOI10.1093/mnras/stab1165
ISSN0035-8711
1365-2966
Citation KeyBarbosaWintAmarMaca:2021:FoEaPl
TitleFormation of Earth-sized planets within the Kepler-1647 system habitable zone
Year2021
MonthJuly
Access Date2024, May 09
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size3246 KiB
2. Context
Author1 Barbosa, Gerson de Oliveira
2 Winter, O. C.
3 Amarante, A.
4 Macau, Elbert Einstein Nehrer
Resume Identifier1
2
3
4 8JMKD3MGP5W/3C9JGUT
ORCID1 0000-0002-1147-2519
2 0000-0002-4901-3289
3 0000-0002-9448-141X
4 0000-0002-6337-8081
Group1 COPDT-CGIP-INPE-MCTI-GOV-BR
2
3
4 COPDT-CGIP-INPE-MCTI-GOV-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Universidade Estadual Paulista (UNESP)
3 Universidade Estadual Paulista (UNESP)
4 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1 gerson.barbosa@inpe.br
2
3
4 elbert.macau@gmail.com
JournalMonthly Notices of the Royal Astronomical Society
Volume504
Number4
Pages6144-6156
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)2021-07-02 12:37:47 :: simone -> administrator ::
2021-07-02 12:37:48 :: administrator -> simone :: 2021
2021-07-02 12:38:17 :: simone -> administrator :: 2021
2022-04-03 23:14:01 :: administrator -> simone :: 2021
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsBinaries: close
Planets and satellites: formation
AbstractThe Kepler-1647 is a binary system with two Sun-type stars (≈1.22 and ≈0.97 M⊙). It has the most massive circumbinary planet (≈1.52 MJup) with the longest orbital period (≈1107.6 d) detected by the Kepler probe and is located within the habitable zone (HZ) of the system. In this work, we investigated the ability to form and house an Earth-sized planet within its HZ. First, we computed the limits of its HZ and performed numerical stability tests within that region. We found that HZ has three subregions that show stability, one internal, one co-orbital, and external to the host planet Kepler-1647b. Within the limits of these three regions, we performed numerical simulations of planetary formation. In the regions inner and outer to the planet, we used two different density profiles to explore different conditions of formation. In the co-orbital region, we used eight different values of total disc mass. We showed that many resonances are located within regions causing much of the disc material to be ejected before a planet is formed. Thus, the system might have two asteroid belts with Kirkwood gaps, similar to the Solar system's main belt of asteroids. The co-orbital region proved to be extremely sensitive, not allowing the planet formation, but showing that this binary system has the capacity to have Trojan bodies. Finally, we looked for regions of stability for an Earth-sized moon. We found that there is stability for a moon with this mass up to 0.4 Hill's radius from the host planet.
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Arrangementurlib.net > CGIP > Formation of Earth-sized...
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4. Conditions of access and use
data URLhttp://urlib.net/ibi/8JMKD3MGP3W34T/4527D58
zipped data URLhttp://urlib.net/zip/8JMKD3MGP3W34T/4527D58
Languageen
Target Filebarbosa-formation.pdf
User Groupsimone
Reader Groupadministrator
simone
Visibilityshown
Archiving Policyallowpublisher allowfinaldraft
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/46KUES5
Citing Item Listsid.inpe.br/bibdigital/2022/04.03.23.11 3
sid.inpe.br/mtc-m21/2012/07.13.14.45.07 1
DisseminationWEBSCI; PORTALCAPES; MGA; COMPENDEX.
Host Collectionurlib.net/www/2021/06.04.03.40
6. Notes
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