Space weathering and the color-color diagram of Plutinos and Jupiter Trojans

The Jupiter Trojan asteroids and the Plutinos are two peculiar populations. They are dynamically resonant, therefore with heliocentric distances relatively bounded for long timescales, as a farely general rule. As a consequence, some correlation with the surface color properties of their respective...

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Detalles Bibliográficos
Publicado: 2015
Materias:
Collisional physics
Trans-neptunian objects
Trojan asteroids
Acceso en línea:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00191035_v248_n_p222_Melita
http://hdl.handle.net/20.500.12110/paper_00191035_v248_n_p222_Melita
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires
id paper:paper_00191035_v248_n_p222_Melita
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spelling paper:paper_00191035_v248_n_p222_Melita2023-06-08T14:40:15Z Space weathering and the color-color diagram of Plutinos and Jupiter Trojans Collisional physics Trans-neptunian objects Trojan asteroids The Jupiter Trojan asteroids and the Plutinos are two peculiar populations. They are dynamically resonant, therefore with heliocentric distances relatively bounded for long timescales, as a farely general rule. As a consequence, some correlation with the surface color properties of their respective members is expected. Indeed, there are apparent differences in the B- V vs. V- R color-color diagram of the two populations. Using a simple model based on the surface color due to the contribution of two components, one pristine and one altered, we find as plausible that the difference is due to the interplay of space weathering by energetic cosmic-radiation and collisional effects. © 2014 Elsevier Inc. 2015 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00191035_v248_n_p222_Melita http://hdl.handle.net/20.500.12110/paper_00191035_v248_n_p222_Melita
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
topic Collisional physics
Trans-neptunian objects
Trojan asteroids
spellingShingle Collisional physics
Trans-neptunian objects
Trojan asteroids
Space weathering and the color-color diagram of Plutinos and Jupiter Trojans
topic_facet Collisional physics
Trans-neptunian objects
Trojan asteroids
description The Jupiter Trojan asteroids and the Plutinos are two peculiar populations. They are dynamically resonant, therefore with heliocentric distances relatively bounded for long timescales, as a farely general rule. As a consequence, some correlation with the surface color properties of their respective members is expected. Indeed, there are apparent differences in the B- V vs. V- R color-color diagram of the two populations. Using a simple model based on the surface color due to the contribution of two components, one pristine and one altered, we find as plausible that the difference is due to the interplay of space weathering by energetic cosmic-radiation and collisional effects. © 2014 Elsevier Inc.
title Space weathering and the color-color diagram of Plutinos and Jupiter Trojans
title_short Space weathering and the color-color diagram of Plutinos and Jupiter Trojans
title_full Space weathering and the color-color diagram of Plutinos and Jupiter Trojans
title_fullStr Space weathering and the color-color diagram of Plutinos and Jupiter Trojans
title_full_unstemmed Space weathering and the color-color diagram of Plutinos and Jupiter Trojans
title_sort space weathering and the color-color diagram of plutinos and jupiter trojans
publishDate 2015
url https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00191035_v248_n_p222_Melita
http://hdl.handle.net/20.500.12110/paper_00191035_v248_n_p222_Melita
_version_ 1768546659937026048

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