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• W3100420188 endingPage "63" @default.
• W3100420188 startingPage "63" @default.
• W3100420188 abstract "We investigate whether coagulation models of planet formation can explain the observed size distributions of trans-Neptunian objects (TNOs). Analyzing published and new calculations, we demonstrate robust relations between the size of the largest object and the slope of the size distribution for sizes 0.1 km and larger. These relations yield clear, testable predictions for TNOs and other icy objects throughout the solar system. Applying our results to existing observations, we show that a broad range of initial disk masses, planetesimal sizes, and fragmentation parameters can explain the data. Adding dynamical constraints on the initial semimajor axis of hot Kuiper Belt objects along with probable TNO formation times of 10–700 Myr restricts the viable models to those with a massive disk composed of relatively small (1–10 km) planetesimals." @default.
• W3100420188 created "2020-11-23" @default.
• W3100420188 creator A5015993983 @default.
• W3100420188 creator A5061772707 @default.
• W3100420188 date "2012-02-08" @default.
• W3100420188 modified "2023-10-12" @default.
• W3100420188 title "COAGULATION CALCULATIONS OF ICY PLANET FORMATION AT 15-150 AU: A CORRELATION BETWEEN THE MAXIMUM RADIUS AND THE SLOPE OF THE SIZE DISTRIBUTION FOR TRANS-NEPTUNIAN OBJECTS" @default.
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