| 1. Identity statement | |
| Reference Type | Book Section |
| Site | mtc-m16.sid.inpe.br |
| Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
| Repository | sid.inpe.br/marciana/2004/09.14.09.21 |
| Last Update | 2004:09.16.03.00.00 (UTC) administrator |
| Metadata Repository | sid.inpe.br/marciana/2004/09.14.09.21.53 |
| Metadata Last Update | 2018:06.05.01.21.02 (UTC) administrator |
| Secondary Key | INPE--/ |
| ISBN/ISSN | 85-17-00012-9 |
| Citation Key | ParisiBrun:2004:MoGiIm |
| Title | Model of a giant impact on saturn.  |
| Year | 2004 |
| Access Date | 2025, July 03 |
| Secondary Type | PRE LI |
| Number of Files | 1 |
| Size | 795 KiB |
| 2. Context | |
| Author | 1 Parisi, Mirta Gabriela 2 Brunini, Adrián |
| Affiliation | 1 Universidad Nacional de La Plata and CONICET. Facultad de Ciencias Astronómicas y Geofísicas |
| Editor | Kuga, Hélio Koiti |
| Book Title | Advances in space dynamics 4: celestial mechanics and astronautics |
| Publisher | INPE |
| City | São José dos Campos |
| Pages | 103-112 |
| History (UTC) | 2005-07-25 16:41:27 :: 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 Stage | completed |
| Transferable | 1 |
| Keywords | SPACE MECHANICS AND CONTROL Cosmology Saturn MECÂNICA ESPACIAL E CONTROLE Cosmologia Saturno |
| Abstract | The origin of the obliquities of the giant planets is one of the fundamental questions of cosmogony. Large stochastic impacts are believed to play a key role during the last stage of the formation of the planets and have been considered as a possible explanation to account for the planetary spin obliquities. We assume that the obliquity of Saturn (26'.7) is due to a giant off-center impact with another protoplanet. We obtain that the impactor mass required to tilt Saturn is 6-7.2 mE). This range of masses set a constraint for the mass of the planetary embryos in the outer Solar System. In order to get dynamical constraints, we study the possible scenarios taking into account the mechanisms of satellite formation and the physical and dynamical characterisitcs of the saturnian moons. |
| Area | ETES |
| doc Directory Content | access |
| source Directory Content | there are no files |
| agreement Directory Content | there are no files |
| 4. Conditions of access and use | |
| data URL | http://urlib.net/ibi/sid.inpe.br/marciana/2004/09.14.09.21 |
| zipped data URL | http://urlib.net/zip/sid.inpe.br/marciana/2004/09.14.09.21 |
| Language | en |
| Target File | Model of a giant.pdf |
| User Group | jefferson administrator |
| Visibility | shown |
| 5. Allied materials | |
| Dissemination | NTRSNASA, BNDEPOSITOLEGAL. |
| Host Collection | sid.inpe.br/banon/2003/08.15.17.40 |
| 6. Notes | |
| Empty Fields | archivingpolicy archivist callnumber contenttype copyholder copyright creatorhistory descriptionlevel documentstage doi e-mailaddress 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 |
| 7. Description control | |
| e-Mail (login) | marciana |
| update | |