Logo do repositório

Apophis: May a meteor activity happen on Earth after the 2029 closest approach?

dc.contributor.authorValvano, G. [UNESP]
dc.contributor.authorSfair, R. [UNESP]
dc.contributor.authorWinter, O. C. [UNESP]
dc.contributor.authorMachado-Oliveira, R. [UNESP]
dc.contributor.authorBorderes-Motta, G.
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)
dc.contributor.institutionEberhard Karls Universitat Tubingen
dc.contributor.institutionUC3M
dc.contributor.institutionIRF
dc.date.accessioned2025-04-29T19:15:04Z
dc.date.issued2024-06-01
dc.description.abstractThe potentially hazardous asteroid 99942 Apophis will have a very close approach to the Earth in 2029. The encounter on its own may provide measurements of Earth's effects on Apophis' surface and also contribute to the improvement of some physical characteristics of the asteroid. In a previous work, we assumed the existence of a hypothetical disc of particles around Apophis before the 2029 encounter, and identified the particles that would escape from the gravity domain of Apophis due to the Earth's gravitational perturbation during the close encounter. In the current work, we investigate the possibility of a meteor activity originating from this event. We study the orbital evolution of these particles computing the MOIDs of the particles with respect to the Earth for the following 200 yr. Our results are not favourable for a meteor activity on Earth. However, a meteoroid activity on the Moon might happen during the encircling period after 88 yr of the 2029 encounter.en
dc.description.affiliationGrupo de Dinamica Orbital e Planetologia Sao Paulo State University UNESP, Guaratingueta, CEP 12516-410
dc.description.affiliationInstitut fur Astronomie und Astrophysik Eberhard Karls Universitat Tubingen
dc.description.affiliationBioengineering and Aerospace Engineering Department Universidad Carlos III de Madrid UC3M, Leganes
dc.description.affiliationSolar Terrestrial and Atmospheric Research (STAR) Swedish Institute of Space Physics IRF, Kiruna
dc.description.affiliationUnespGrupo de Dinamica Orbital e Planetologia Sao Paulo State University UNESP, Guaratingueta, CEP 12516-410
dc.format.extent1585-1591
dc.identifierhttp://dx.doi.org/10.1093/mnras/stae1181
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, v. 531, n. 1, p. 1585-1591, 2024.
dc.identifier.doi10.1093/mnras/stae1181
dc.identifier.issn1365-2966
dc.identifier.issn0035-8711
dc.identifier.scopus2-s2.0-85194183849
dc.identifier.urihttps://hdl.handle.net/11449/302612
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.sourceScopus
dc.subjectcelestial mechanics
dc.subjectminor planets, asteroids: general
dc.subjectplanetary systems
dc.subjectplanets and satellites: dynamical evolution and stability
dc.titleApophis: May a meteor activity happen on Earth after the 2029 closest approach?en
dc.typeArtigopt
dspace.entity.typePublication
relation.isOrgUnitOfPublicationa4071986-4355-47c3-a5a3-bd4d1a966e4f
relation.isOrgUnitOfPublication.latestForDiscoverya4071986-4355-47c3-a5a3-bd4d1a966e4f
unesp.author.orcid0000-0002-7905-1788[1]
unesp.author.orcid0000-0002-4939-013X 0000-0002-4939-013X[2]
unesp.author.orcid0000-0002-4901-3289[3]
unesp.author.orcid0000-0002-6875-0508[4]
unesp.author.orcid0000-0002-4680-8414 0000-0002-4680-8414[5]
unesp.campusUniversidade Estadual Paulista (UNESP), Faculdade de Engenharia e Ciências, Guaratinguetápt

Arquivos