English   español  
Por favor, use este identificador para citar o enlazar a este item: http://hdl.handle.net/10261/17822
Compartir / Impacto:
Add this article to your Mendeley library MendeleyBASE
Visualizar otros formatos: MARC | Dublin Core | RDF | ORE | MODS | METS | DIDL

The History of the Solar System's Debris Disc: Observable Properties of the Kuiper Belt.

AutorBooth, Mark; Wyatt, Mark C.; Morbidelli, Alessandro; Moro-Martín, Amaya ; Levison, Harold F.
Palabras claveKuiper Belt
Solar system: general
Circumstellar matter
Planetary systems
Fecha de publicación19-ago-2009
EditorRoyal Astronomical Society
Blackwell Publishing
CitaciónMonthly Notices of the Royal Astronomical Society (MNRAS) 399(1): 385-398 (2009)
ResumenThe Nice model of Gomes et al. suggests that the migration of the giant planets caused a planetesimal clearing event, which led to the late heavy bombardment (LHB) at 880 Myr. Here, we investigate the infrared emission from the Kuiper belt during the history of the Solar system as described by the Nice model. We describe a method for easily converting the results of N-body planetesimal simulations into observational properties (assuming blackbody grains and a single size distribution) and further modify this method to improve its realism (using realistic grain properties and a three-phase size distribution). We compare our results with observed debris discs and evaluate the plausibility of detecting an LHB-like process in extrasolar systems. Recent surveys have shown that 4 per cent of stars exhibit 24 μm excess and 16 per cent exhibit 70 μm excess. We show that the Solar system would have been amongst the brightest of these systems before the LHB at both 24 and 70 μm. We find a significant increase in 24 μm emission during the LHB, which rapidly drops off and becomes undetectable within 30 Myr, whereas the 70 μm emission remains detectable until 360 Myr after the LHB. Comparison with the statistics of debris disc evolution shows that such depletion events must be rare occurring around less than 12 per cent of Sun-like stars and with this level of incidence we would expect approximately one of the 413 Sun-like field stars so far detected to have a 24 μm excess to be currently going through an LHB. We also find that collisional processes are important in the Solar system before the LHB and that parameters for weak Kuiper belt objects are inconsistent with the Nice model interpretation of the LHB.
Descripción14 pages, 13 figures.-- Printed version published Oct 2009.
ArXiv pre-print available at: http://arxiv.org/abs/0906.3755
Versión del editorhttp://dx.doi.org/10.1111/j.1365-2966.2009.15286.x
Aparece en las colecciones: (CAB) Artículos
Ficheros en este ítem:
Fichero Descripción Tamaño Formato  
0906.3755v1.pdf685,55 kBAdobe PDFVista previa
Mostrar el registro completo

Artículos relacionados:

NOTA: Los ítems de Digital.CSIC están protegidos por copyright, con todos los derechos reservados, a menos que se indique lo contrario.