The Scattered Disk Population and the Oort Cloud
- Autores
- Fernández, Julio A.; Gallardo, Tabaré; Brunini, Adrián; Davies, John K.; Barrera, Luis H.
- Año de publicación
- 2004
- Idioma
- inglés
- Tipo de recurso
- parte de libro
- Estado
- versión publicada
- Descripción
- The trans-Neptunian belt has been subject to a strong depletion that has reduced its primordial population by a factor of one hundred over the solar system’s age. One by-product of such a depletion process is the existence of a scattered disk population in transit from the belt to other places, such as the Jupiter zone, the Oort cloud or interstellar space. We have integrated the orbits of the scattered disk objects (SDOs) so far discovered by 2500 Myr to study their dynamical time scales and the probability of falling in each of the end states mentioned above, paying special attention to their contribution to the Oort cloud. We found that their dynamical half-time is close to 2.5 Gyr and that about one third of the SDOs end up in the Oort cloud.
Facultad de Ciencias Astronómicas y Geofísicas - Materia
- Ciencias Astronómicas
- Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by-nc-sa/4.0/
- Repositorio
.jpg)
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/138927
Ver los metadatos del registro completo
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The Scattered Disk Population and the Oort CloudFernández, Julio A.Gallardo, TabaréBrunini, AdriánDavies, John K.Barrera, Luis H.Ciencias AstronómicasThe trans-Neptunian belt has been subject to a strong depletion that has reduced its primordial population by a factor of one hundred over the solar system’s age. One by-product of such a depletion process is the existence of a scattered disk population in transit from the belt to other places, such as the Jupiter zone, the Oort cloud or interstellar space. We have integrated the orbits of the scattered disk objects (SDOs) so far discovered by 2500 Myr to study their dynamical time scales and the probability of falling in each of the end states mentioned above, paying special attention to their contribution to the Oort cloud. We found that their dynamical half-time is close to 2.5 Gyr and that about one third of the SDOs end up in the Oort cloud.Facultad de Ciencias Astronómicas y GeofísicasSpringer2004info:eu-repo/semantics/bookPartinfo:eu-repo/semantics/publishedVersionCapitulo de librohttp://purl.org/coar/resource_type/c_3248info:ar-repo/semantics/parteDeLibroapplication/pdf43-48http://sedici.unlp.edu.ar/handle/10915/138927enginfo:eu-repo/semantics/altIdentifier/isbn/978-94-017-3321-2info:eu-repo/semantics/altIdentifier/doi/10.1007/978-94-017-3321-2_3info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-sa/4.0/Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-10-22T17:13:07Zoai:sedici.unlp.edu.ar:10915/138927Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-10-22 17:13:07.334SEDICI (UNLP) - Universidad Nacional de La Platafalse |
| dc.title.none.fl_str_mv |
The Scattered Disk Population and the Oort Cloud |
| title |
The Scattered Disk Population and the Oort Cloud |
| spellingShingle |
The Scattered Disk Population and the Oort Cloud Fernández, Julio A. Ciencias Astronómicas |
| title_short |
The Scattered Disk Population and the Oort Cloud |
| title_full |
The Scattered Disk Population and the Oort Cloud |
| title_fullStr |
The Scattered Disk Population and the Oort Cloud |
| title_full_unstemmed |
The Scattered Disk Population and the Oort Cloud |
| title_sort |
The Scattered Disk Population and the Oort Cloud |
| dc.creator.none.fl_str_mv |
Fernández, Julio A. Gallardo, Tabaré Brunini, Adrián Davies, John K. Barrera, Luis H. |
| author |
Fernández, Julio A. |
| author_facet |
Fernández, Julio A. Gallardo, Tabaré Brunini, Adrián Davies, John K. Barrera, Luis H. |
| author_role |
author |
| author2 |
Gallardo, Tabaré Brunini, Adrián Davies, John K. Barrera, Luis H. |
| author2_role |
author author author author |
| dc.subject.none.fl_str_mv |
Ciencias Astronómicas |
| topic |
Ciencias Astronómicas |
| dc.description.none.fl_txt_mv |
The trans-Neptunian belt has been subject to a strong depletion that has reduced its primordial population by a factor of one hundred over the solar system’s age. One by-product of such a depletion process is the existence of a scattered disk population in transit from the belt to other places, such as the Jupiter zone, the Oort cloud or interstellar space. We have integrated the orbits of the scattered disk objects (SDOs) so far discovered by 2500 Myr to study their dynamical time scales and the probability of falling in each of the end states mentioned above, paying special attention to their contribution to the Oort cloud. We found that their dynamical half-time is close to 2.5 Gyr and that about one third of the SDOs end up in the Oort cloud. Facultad de Ciencias Astronómicas y Geofísicas |
| description |
The trans-Neptunian belt has been subject to a strong depletion that has reduced its primordial population by a factor of one hundred over the solar system’s age. One by-product of such a depletion process is the existence of a scattered disk population in transit from the belt to other places, such as the Jupiter zone, the Oort cloud or interstellar space. We have integrated the orbits of the scattered disk objects (SDOs) so far discovered by 2500 Myr to study their dynamical time scales and the probability of falling in each of the end states mentioned above, paying special attention to their contribution to the Oort cloud. We found that their dynamical half-time is close to 2.5 Gyr and that about one third of the SDOs end up in the Oort cloud. |
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2004 |
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2004 |
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eng |
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Springer |
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