CaltechAUTHORS
  A Caltech Library Service

A Hypothesis for the Color Diversity of the Kuiper Belt

Brown, M. E. and Schaller, E. L. and Fraser, W. C. (2011) A Hypothesis for the Color Diversity of the Kuiper Belt. Astrophysical Journal Letters, 739 (2). Art. No. L60. ISSN 2041-8205. https://resolver.caltech.edu/CaltechAUTHORS:20111011-074859547

[img]
Preview
PDF - Published Version
See Usage Policy.

195Kb
[img] PDF - Submitted Version
See Usage Policy.

158Kb

Use this Persistent URL to link to this item: https://resolver.caltech.edu/CaltechAUTHORS:20111011-074859547

Abstract

We propose a chemical and dynamical process to explain the surface colors of the Kuiper belt. In our hypothesis, the initial bulk compositions of the bodies themselves can be quite diverse—as is seen in comets—but the early surface compositions are set by volatile evaporation after the objects are formed. Strong gradients in surface composition, coupled with UV and particle irradiation, lead to the surface colors that are seen today. The objects formed in the inner part of the primordial belt retain only H_2O and CO_2 as the major ice species on their surfaces. Irradiation of these species plausibly results in the dark neutrally colored centaurs and Kuiper belt objects (KBOs). Object formed further in the disk retain CH_3OH, which has been shown to lead to brighter redder surfaces after irradiation, as seen in the brighter redder centaurs and KBOs. Objects formed at the current location of the cold classical Kuiper belt uniquely retain NH_3, which has been shown to affect irradiation chemistry and could plausibly lead to the unique colors of these objects. We propose observational and experimental tests of this hypothesis.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1088/2041-8205/739/2/L60DOIArticle
http://iopscience.iop.org/2041-8205/739/2/L60PublisherArticle
https://arxiv.org/abs/1109.0298arXivDiscussion Paper
Additional Information:© 2011 The American Astronomical Society. Received 2011 May 24; accepted 2011 August 19; published 2011 September 12. This research has been supported by grant NNX09AB49G from the NASA Planetary Astronomy program. We thank Hal Levison, Rosario Brunetto, and Konstantin Batygin for enlightening conversations.
Funders:
Funding AgencyGrant Number
NASANNX09AB49G
Subject Keywords:astrochemistry; Kuiper belt: general; planets and satellites: formation
Issue or Number:2
Classification Code:PACS: 96.30.Xa; 96.10.+i; 96.12.Ma
Record Number:CaltechAUTHORS:20111011-074859547
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20111011-074859547
Official Citation:A Hypothesis for the Color Diversity of the Kuiper Belt M. E. Brown et al. 2011 ApJ 739 L60
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:27149
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:11 Oct 2011 14:59
Last Modified:03 Oct 2019 03:21

Repository Staff Only: item control page