An Investigation on the Origin of Centaurs’ Color-Inclination Relation

碩士 === 國立中央大學 === 天文研究所 === 106 === Since its discovery, there has been a debate on the origin of the bimodal color distribution of Centaurs in the past few decades. In principle, two theories have been proposed to explain this bimodal color distribution: (1) evolutionary processes resulting in chan...

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Main Authors: Po-Yen Liu, 劉柏彥
Other Authors: Wing-Huen Ip
Format: Others
Language:en_US
Published: 2018
Online Access:http://ndltd.ncl.edu.tw/handle/jqzwer
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spelling ndltd-TW-106NCU051990082019-10-24T05:19:40Z http://ndltd.ncl.edu.tw/handle/jqzwer An Investigation on the Origin of Centaurs’ Color-Inclination Relation Po-Yen Liu 劉柏彥 碩士 國立中央大學 天文研究所 106 Since its discovery, there has been a debate on the origin of the bimodal color distribution of Centaurs in the past few decades. In principle, two theories have been proposed to explain this bimodal color distribution: (1) evolutionary processes resulting in changes of the surface properties of Centaurs, and, (2) compositional differences inherited from the primordial origin of Centaurs. What might be more intriguing is that Centaurs also show a correlation between their orbital inclinations and colors that the blue (B-R≤1.4) and red (B-R>1.4) Centaurs tend to be characterized by high and low inclination distributions, respectively. In this study, we consider two hypotheses to explain the color-inclination relation based on the two major theories of explaining the bimodal color distribution mentioned above. Namely, we consider: (1) Initially, the scattering Kuiper Belt objects (SKBOs) have no color-inclination relation. When they evolve into Centaurs with perihelion distances within Saturn’s orbit, the gravitational effect of Saturn or Jupiter becomes strong enough to greatly change the inclinations of Centaurs. At the same time, the thermal radiation is also strong enough to trigger cometary activities to produce the blue surface colors; (2) Assuming that the SKBOs also have color-inclination relation (which is unclear yet), and this relation is statistically preserved when they evolved into Centaurs. We perform numerical simulations on 158 observed Centaurs (58 of them have color information) and 82 observed SKBOs to investigate their dynamical evolution. Our results show that the color-inclination relation of Centaurs is more likely to inherit from SKBOs. We find that our hypothesis (2) is more likely to explain the color-inclination relation of Centaurs. Wing-Huen Ip 葉永烜 2018 學位論文 ; thesis 63 en_US
collection NDLTD
language en_US
format Others
sources NDLTD
description 碩士 === 國立中央大學 === 天文研究所 === 106 === Since its discovery, there has been a debate on the origin of the bimodal color distribution of Centaurs in the past few decades. In principle, two theories have been proposed to explain this bimodal color distribution: (1) evolutionary processes resulting in changes of the surface properties of Centaurs, and, (2) compositional differences inherited from the primordial origin of Centaurs. What might be more intriguing is that Centaurs also show a correlation between their orbital inclinations and colors that the blue (B-R≤1.4) and red (B-R>1.4) Centaurs tend to be characterized by high and low inclination distributions, respectively. In this study, we consider two hypotheses to explain the color-inclination relation based on the two major theories of explaining the bimodal color distribution mentioned above. Namely, we consider: (1) Initially, the scattering Kuiper Belt objects (SKBOs) have no color-inclination relation. When they evolve into Centaurs with perihelion distances within Saturn’s orbit, the gravitational effect of Saturn or Jupiter becomes strong enough to greatly change the inclinations of Centaurs. At the same time, the thermal radiation is also strong enough to trigger cometary activities to produce the blue surface colors; (2) Assuming that the SKBOs also have color-inclination relation (which is unclear yet), and this relation is statistically preserved when they evolved into Centaurs. We perform numerical simulations on 158 observed Centaurs (58 of them have color information) and 82 observed SKBOs to investigate their dynamical evolution. Our results show that the color-inclination relation of Centaurs is more likely to inherit from SKBOs. We find that our hypothesis (2) is more likely to explain the color-inclination relation of Centaurs.
author2 Wing-Huen Ip
author_facet Wing-Huen Ip
Po-Yen Liu
劉柏彥
author Po-Yen Liu
劉柏彥
spellingShingle Po-Yen Liu
劉柏彥
An Investigation on the Origin of Centaurs’ Color-Inclination Relation
author_sort Po-Yen Liu
title An Investigation on the Origin of Centaurs’ Color-Inclination Relation
title_short An Investigation on the Origin of Centaurs’ Color-Inclination Relation
title_full An Investigation on the Origin of Centaurs’ Color-Inclination Relation
title_fullStr An Investigation on the Origin of Centaurs’ Color-Inclination Relation
title_full_unstemmed An Investigation on the Origin of Centaurs’ Color-Inclination Relation
title_sort investigation on the origin of centaurs’ color-inclination relation
publishDate 2018
url http://ndltd.ncl.edu.tw/handle/jqzwer
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