Col-OSSOS: Evidence for a compositional gradient inherited from the protoplanetary disk? Article Swipe
Michael Marsset
,
Wesley C. Fraser
,
Megan E. Schwamb
,
Laura E. Buchanan
,
Rosemary E. Pike
,
N. Peixinho
,
Susan Benecchi
,
Michele T. Bannister
,
Nicole J. Tan
,
J. J. Kavelaars
·
YOU?
·
· 2022
· Open Access
·
· DOI: https://doi.org/10.48550/arxiv.2206.04096
YOU?
·
· 2022
· Open Access
·
· DOI: https://doi.org/10.48550/arxiv.2206.04096
In the present-day Kuiper Belt, the number of compositional classes and the orbital distributions of these classes hold important cosmogonic implications for the Solar System. In a companion paper by Fraser et al., we demonstrate that the observed color distribution of small (H>6) Trans-Neptunian Objects (TNOs) can be accounted for by the existence of only two composition classes, named brightIR and faintIR, where the range of colors in each class is governed by a mixture of two material end members. Here, we investigate the orbital distribution of the two color classes identified by Fraser et al. and find that the orbital inclinations of the brightIR class objects are correlated with their optical colors. Using the output of numerical simulations investigating the orbital evolution of TNOs during their scattering phase with Neptune, we show that this correlation could reflect a composition gradient in the early protoplanetary disk, in the range of heliocentric distances over which TNOs from the brightIR class accreted. However, tensions between this interpretation and the existence of blue contaminants among cold classical TNOs, and possible alternative origins for the detected correlation, currently bear uncertainty on our proposed interpretation.
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- Type
- preprint
- Language
- en
- Landing Page
- http://arxiv.org/abs/2206.04096
- https://arxiv.org/pdf/2206.04096
- OA Status
- green
- Related Works
- 10
- OpenAlex ID
- https://openalex.org/W4281752443
All OpenAlex metadata
Raw OpenAlex JSON
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https://openalex.org/W4281752443Canonical identifier for this work in OpenAlex
- DOI
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https://doi.org/10.48550/arxiv.2206.04096Digital Object Identifier
- Title
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Col-OSSOS: Evidence for a compositional gradient inherited from the protoplanetary disk?Work title
- Type
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preprintOpenAlex work type
- Language
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enPrimary language
- Publication year
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2022Year of publication
- Publication date
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2022-06-08Full publication date if available
- Authors
-
Michael Marsset, Wesley C. Fraser, Megan E. Schwamb, Laura E. Buchanan, Rosemary E. Pike, N. Peixinho, Susan Benecchi, Michele T. Bannister, Nicole J. Tan, J. J. KavelaarsList of authors in order
- Landing page
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https://arxiv.org/abs/2206.04096Publisher landing page
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https://arxiv.org/pdf/2206.04096Direct link to full text PDF
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YesWhether a free full text is available
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greenOpen access status per OpenAlex
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https://arxiv.org/pdf/2206.04096Direct OA link when available
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Neptune, Physics, Astrophysics, Solar System, Protoplanetary disk, Range (aeronautics), Interpretation (philosophy), Astronomy, Planet, Programming language, Materials science, Composite material, Computer scienceTop concepts (fields/topics) attached by OpenAlex
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| abstract_inverted_index.material | 77 |
| abstract_inverted_index.members. | 79 |
| abstract_inverted_index.observed | 37 |
| abstract_inverted_index.possible | 176 |
| abstract_inverted_index.proposed | 188 |
| abstract_inverted_index.tensions | 161 |
| abstract_inverted_index.accounted | 48 |
| abstract_inverted_index.accreted. | 159 |
| abstract_inverted_index.classical | 173 |
| abstract_inverted_index.companion | 27 |
| abstract_inverted_index.currently | 183 |
| abstract_inverted_index.distances | 151 |
| abstract_inverted_index.evolution | 122 |
| abstract_inverted_index.existence | 52, 167 |
| abstract_inverted_index.important | 18 |
| abstract_inverted_index.numerical | 117 |
| abstract_inverted_index.correlated | 108 |
| abstract_inverted_index.cosmogonic | 19 |
| abstract_inverted_index.identified | 91 |
| abstract_inverted_index.scattering | 127 |
| abstract_inverted_index.alternative | 177 |
| abstract_inverted_index.composition | 56, 139 |
| abstract_inverted_index.correlation | 135 |
| abstract_inverted_index.demonstrate | 34 |
| abstract_inverted_index.investigate | 82 |
| abstract_inverted_index.present-day | 2 |
| abstract_inverted_index.simulations | 118 |
| abstract_inverted_index.uncertainty | 185 |
| abstract_inverted_index.contaminants | 170 |
| abstract_inverted_index.correlation, | 182 |
| abstract_inverted_index.distribution | 39, 85 |
| abstract_inverted_index.heliocentric | 150 |
| abstract_inverted_index.implications | 20 |
| abstract_inverted_index.inclinations | 101 |
| abstract_inverted_index.compositional | 8 |
| abstract_inverted_index.distributions | 13 |
| abstract_inverted_index.investigating | 119 |
| abstract_inverted_index.interpretation | 164 |
| abstract_inverted_index.protoplanetary | 144 |
| abstract_inverted_index.Trans-Neptunian | 43 |
| abstract_inverted_index.interpretation. | 189 |
| cited_by_percentile_year | |
| countries_distinct_count | 0 |
| institutions_distinct_count | 10 |
| citation_normalized_percentile |