The trans-Neptunian object size distribution at small sizes
- Autores
- Gil Hutton, Ricardo Alfredo; Licandro, J.; Pinilla Alonso, N.; Brunetto, R.
- Año de publicación
- 2009
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- Aims. The aim. of this work, is to estimate the size distribution of small Trans-Neptunian objects. Methods. We simulate the irradiation and collisional processes affecting the surface of a Trans-Neptunian object for the first time using as a constraint the peculiar crystalline to amorphous water ice ratio observed on (136108) 2003 ELa. Results. We find that the size distribution changes its exponent from q0 = 4.2 at larger sizes to q1 = 2.40 ± 0.3 at the smaller ones, with a break, radius of r1 = 35 ± 15 km. If this size distribution is applied to studying the collisional surface evolution of (1361.08) 2003 EL61, we find that the object must be covered by a thin ice crust of ≈0.12 cm, while the original, composition of the object is still present at 1.61 cm or more below the surface. This result is not affected by a collision with a large projectile that occurred by chance more than 109 yr ago since after a short time the mean value obtained for the crystalline to amorphous water ice ratio is indistinguishable from the one obtained without a collision with a large projectile. Since the simulations are not sensitive to the effects of very small projectiles (rp < 10-30 m), it is possible that the exponent of the size distribution for these very small, objects changes again, approaching a Donhanyi's size distribution.
Fil: Gil Hutton, Ricardo Alfredo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Complejo Astronómico "El Leoncito". Universidad Nacional de Córdoba. Complejo Astronómico "El Leoncito". Universidad Nacional de la Plata. Complejo Astronómico "El Leoncito". Universidad Nacional de San Juan. Complejo Astronómico "El Leoncito"; Argentina
Fil: Licandro, J.. Instituto de Astrofísica de Canarias; España
Fil: Pinilla Alonso, N.. Fundación Galileo Galilei & Telescopio Nazionale Galileo; España
Fil: Brunetto, R.. Université Paris-Sud; Francia - Materia
-
ASTROCHEMISTRY -
KUIPER BELT -
METHODS, NUMERICAL
SOLAR SYSTEM, FORMATION - - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/213848
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The trans-Neptunian object size distribution at small sizesGil Hutton, Ricardo AlfredoLicandro, J.Pinilla Alonso, N.Brunetto, R.ASTROCHEMISTRY -KUIPER BELT -METHODS, NUMERICALSOLAR SYSTEM, FORMATION -https://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Aims. The aim. of this work, is to estimate the size distribution of small Trans-Neptunian objects. Methods. We simulate the irradiation and collisional processes affecting the surface of a Trans-Neptunian object for the first time using as a constraint the peculiar crystalline to amorphous water ice ratio observed on (136108) 2003 ELa. Results. We find that the size distribution changes its exponent from q0 = 4.2 at larger sizes to q1 = 2.40 ± 0.3 at the smaller ones, with a break, radius of r1 = 35 ± 15 km. If this size distribution is applied to studying the collisional surface evolution of (1361.08) 2003 EL61, we find that the object must be covered by a thin ice crust of ≈0.12 cm, while the original, composition of the object is still present at 1.61 cm or more below the surface. This result is not affected by a collision with a large projectile that occurred by chance more than 109 yr ago since after a short time the mean value obtained for the crystalline to amorphous water ice ratio is indistinguishable from the one obtained without a collision with a large projectile. Since the simulations are not sensitive to the effects of very small projectiles (rp < 10-30 m), it is possible that the exponent of the size distribution for these very small, objects changes again, approaching a Donhanyi's size distribution.Fil: Gil Hutton, Ricardo Alfredo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Complejo Astronómico "El Leoncito". Universidad Nacional de Córdoba. Complejo Astronómico "El Leoncito". Universidad Nacional de la Plata. Complejo Astronómico "El Leoncito". Universidad Nacional de San Juan. Complejo Astronómico "El Leoncito"; ArgentinaFil: Licandro, J.. Instituto de Astrofísica de Canarias; EspañaFil: Pinilla Alonso, N.. Fundación Galileo Galilei & Telescopio Nazionale Galileo; EspañaFil: Brunetto, R.. Université Paris-Sud; FranciaEDP Sciences2009-06info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/213848Gil Hutton, Ricardo Alfredo; Licandro, J.; Pinilla Alonso, N.; Brunetto, R.; The trans-Neptunian object size distribution at small sizes; EDP Sciences; Astronomy and Astrophysics; 500; 2; 6-2009; 909-9160004-6361CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/200811301info:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/abs/2009/23/aa11301-08/aa11301-08.htmlinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:06:50Zoai:ri.conicet.gov.ar:11336/213848instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 10:06:50.412CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
The trans-Neptunian object size distribution at small sizes |
title |
The trans-Neptunian object size distribution at small sizes |
spellingShingle |
The trans-Neptunian object size distribution at small sizes Gil Hutton, Ricardo Alfredo ASTROCHEMISTRY - KUIPER BELT - METHODS, NUMERICAL SOLAR SYSTEM, FORMATION - |
title_short |
The trans-Neptunian object size distribution at small sizes |
title_full |
The trans-Neptunian object size distribution at small sizes |
title_fullStr |
The trans-Neptunian object size distribution at small sizes |
title_full_unstemmed |
The trans-Neptunian object size distribution at small sizes |
title_sort |
The trans-Neptunian object size distribution at small sizes |
dc.creator.none.fl_str_mv |
Gil Hutton, Ricardo Alfredo Licandro, J. Pinilla Alonso, N. Brunetto, R. |
author |
Gil Hutton, Ricardo Alfredo |
author_facet |
Gil Hutton, Ricardo Alfredo Licandro, J. Pinilla Alonso, N. Brunetto, R. |
author_role |
author |
author2 |
Licandro, J. Pinilla Alonso, N. Brunetto, R. |
author2_role |
author author author |
dc.subject.none.fl_str_mv |
ASTROCHEMISTRY - KUIPER BELT - METHODS, NUMERICAL SOLAR SYSTEM, FORMATION - |
topic |
ASTROCHEMISTRY - KUIPER BELT - METHODS, NUMERICAL SOLAR SYSTEM, FORMATION - |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
Aims. The aim. of this work, is to estimate the size distribution of small Trans-Neptunian objects. Methods. We simulate the irradiation and collisional processes affecting the surface of a Trans-Neptunian object for the first time using as a constraint the peculiar crystalline to amorphous water ice ratio observed on (136108) 2003 ELa. Results. We find that the size distribution changes its exponent from q0 = 4.2 at larger sizes to q1 = 2.40 ± 0.3 at the smaller ones, with a break, radius of r1 = 35 ± 15 km. If this size distribution is applied to studying the collisional surface evolution of (1361.08) 2003 EL61, we find that the object must be covered by a thin ice crust of ≈0.12 cm, while the original, composition of the object is still present at 1.61 cm or more below the surface. This result is not affected by a collision with a large projectile that occurred by chance more than 109 yr ago since after a short time the mean value obtained for the crystalline to amorphous water ice ratio is indistinguishable from the one obtained without a collision with a large projectile. Since the simulations are not sensitive to the effects of very small projectiles (rp < 10-30 m), it is possible that the exponent of the size distribution for these very small, objects changes again, approaching a Donhanyi's size distribution. Fil: Gil Hutton, Ricardo Alfredo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Complejo Astronómico "El Leoncito". Universidad Nacional de Córdoba. Complejo Astronómico "El Leoncito". Universidad Nacional de la Plata. Complejo Astronómico "El Leoncito". Universidad Nacional de San Juan. Complejo Astronómico "El Leoncito"; Argentina Fil: Licandro, J.. Instituto de Astrofísica de Canarias; España Fil: Pinilla Alonso, N.. Fundación Galileo Galilei & Telescopio Nazionale Galileo; España Fil: Brunetto, R.. Université Paris-Sud; Francia |
description |
Aims. The aim. of this work, is to estimate the size distribution of small Trans-Neptunian objects. Methods. We simulate the irradiation and collisional processes affecting the surface of a Trans-Neptunian object for the first time using as a constraint the peculiar crystalline to amorphous water ice ratio observed on (136108) 2003 ELa. Results. We find that the size distribution changes its exponent from q0 = 4.2 at larger sizes to q1 = 2.40 ± 0.3 at the smaller ones, with a break, radius of r1 = 35 ± 15 km. If this size distribution is applied to studying the collisional surface evolution of (1361.08) 2003 EL61, we find that the object must be covered by a thin ice crust of ≈0.12 cm, while the original, composition of the object is still present at 1.61 cm or more below the surface. This result is not affected by a collision with a large projectile that occurred by chance more than 109 yr ago since after a short time the mean value obtained for the crystalline to amorphous water ice ratio is indistinguishable from the one obtained without a collision with a large projectile. Since the simulations are not sensitive to the effects of very small projectiles (rp < 10-30 m), it is possible that the exponent of the size distribution for these very small, objects changes again, approaching a Donhanyi's size distribution. |
publishDate |
2009 |
dc.date.none.fl_str_mv |
2009-06 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
format |
article |
status_str |
publishedVersion |
dc.identifier.none.fl_str_mv |
http://hdl.handle.net/11336/213848 Gil Hutton, Ricardo Alfredo; Licandro, J.; Pinilla Alonso, N.; Brunetto, R.; The trans-Neptunian object size distribution at small sizes; EDP Sciences; Astronomy and Astrophysics; 500; 2; 6-2009; 909-916 0004-6361 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/213848 |
identifier_str_mv |
Gil Hutton, Ricardo Alfredo; Licandro, J.; Pinilla Alonso, N.; Brunetto, R.; The trans-Neptunian object size distribution at small sizes; EDP Sciences; Astronomy and Astrophysics; 500; 2; 6-2009; 909-916 0004-6361 CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/200811301 info:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/abs/2009/23/aa11301-08/aa11301-08.html |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
dc.format.none.fl_str_mv |
application/pdf application/pdf |
dc.publisher.none.fl_str_mv |
EDP Sciences |
publisher.none.fl_str_mv |
EDP Sciences |
dc.source.none.fl_str_mv |
reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas |
reponame_str |
CONICET Digital (CONICET) |
collection |
CONICET Digital (CONICET) |
instname_str |
Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.name.fl_str_mv |
CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.mail.fl_str_mv |
dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
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1844613921192804352 |
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13.070432 |