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1. Identity statement
Reference TypeBook Section
Sitemtc-m16.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Repositorysid.inpe.br/marciana/2004/09.14.09.26
Last Update2004:09.16.03.00.00 (UTC) administrator
Metadata Repositorysid.inpe.br/marciana/2004/09.14.09.26.48
Metadata Last Update2018:06.05.01.21.02 (UTC) administrator
Secondary KeyINPE--/
ISBN/ISSN85-17-00012-9
Citation KeyOliveiraNetoMaiaCarn:2004:TyDiEq
TitleA description of extra-solar planetary orbits through a schrödinger - type diffusion equation.
Year2004
Access Date2024, Dec. 26
Secondary TypePRE LI
Number of Files1
Size406 KiB
2. Context
Author1 Oliveira Neto, Marçal de
2 Maia, Liliane de Almeida
3 Carneiro, Saulo
Affiliation1 Universidade de Brasília, Instituto de Química (UNB)
2 Universidade de Brasília, Departamento de Matemática (UNB)
3 Universidade Federal da Bahia. Instituto de Física (UFBA)
EditorKuga, Hélio Koiti
e-Mail Addressmarcal@unb.br
Book TitleAdvances in space dynamics 4: celestial mechanics and astronautics
PublisherINPE
CitySão José dos Campos
Pages113-121
History (UTC)2005-07-25 16:47:03 :: jefferson -> administrator ::
2018-06-05 01:21:02 :: administrator -> marciana :: 2004
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
KeywordsSPACE MECHANICS AND CONTROL
Planetary orbits
Schrodinger equation
MECÂNICA ESPACIAL E CONTROLE
Órbitas planetárias
Equação de Schrodinger
AbstractThe planetary orbits in our solar system have been successfully described by an approach similar to the Bohr atomic model [1-3]. A Schrödinger-type diffusion equation has shown that quantum states associated to the asteroid belt are in very good agreement with the observed mean radii of the asteroids which perform the internal and external orbits in the belt. According to these results, a model of quantum states condensation was proposed in order to infer the orbits of the planets in our solar system [4]. In this paper, the use of the Schrödinger-type diffusion equation reproduces the observed mean distances for the 101 extra-solar planets discovered up to now. A considerable number of these planets were found at the planetary mean distance of 0.05 AU from their stars, which is the fundamental radius obtained by this approach. Planets with mean distances of 2.0 AU were also predicted by the model.
AreaETES
doc Directory Contentaccess
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4. Conditions of access and use
data URLhttp://urlib.net/ibi/sid.inpe.br/marciana/2004/09.14.09.26
zipped data URLhttp://urlib.net/zip/sid.inpe.br/marciana/2004/09.14.09.26
Languageen
Target FileA description of extra-solar.pdf
User Groupjefferson
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Visibilityshown
5. Allied materials
DisseminationNTRSNASA, BNDEPOSITOLEGAL.
Host Collectionsid.inpe.br/banon/2003/08.15.17.40
6. Notes
Empty Fieldsarchivingpolicy archivist callnumber contenttype copyholder copyright creatorhistory descriptionlevel documentstage doi edition electronicmailaddress format group identifier isbn issn label lineage mark mirrorrepository nextedition nexthigherunit notes numberofvolumes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup readpermission resumeid rightsholder schedulinginformation secondarydate secondarymark serieseditor seriestitle session shorttitle sponsor subject tertiarymark tertiarytype translator url versiontype volume
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