Ultra wide Trans Neptunian Binaries

This book PDF is perfect for those who love Electronic Books genre, written by Alex Harrison Parker and published by Unknown which was released on 19 May 2024 with total hardcover pages null. You could read this book directly on your devices with pdf, epub and kindle format, check detail and related Ultra wide Trans Neptunian Binaries books below.

Ultra wide Trans Neptunian Binaries
Author : Alex Harrison Parker
File Size : 46,6 Mb
Publisher : Unknown
Language : English
Release Date : 19 May 2024
ISBN : OCLC:858830706
Pages : null pages
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Ultra wide Trans Neptunian Binaries by Alex Harrison Parker Book PDF Summary

Ultra-wide Trans-Neptunian Binaries (TNBs) are extremely sensitive to perturbation, and therefore make excellent probes of the past and present dynamical environment of the outer Solar System. Using data gathered from a host of facilities we have determined the mutual orbits for a sample of seven wide TNBs whose periods exceed one year. This characterized sample provides us with new information about the probable formation scenarios of TNBs, and has significant implications for the early dynamical and collisional history of the Kuiper Belt. We show that these wide binaries have short collisional lifetimes, and use them to produce a new estimate of the number of small (~1 km) objects in the Kuiper Belt. Additionally, these systems are susceptible to tidal disruption, and we show that it is unlikely that they were ever subjected to a period of close encounters with the giant planets. We find that the current properties of these ultra-wide Trans-Neptunian Binaries suggest that planetesimal growth in the Cold Classical Kuiper Belt did not occur through slow hierarchical accretion, but rather through rapid gravitational collapse.

Ultra wide Trans Neptunian Binaries

Ultra-wide Trans-Neptunian Binaries (TNBs) are extremely sensitive to perturbation, and therefore make excellent probes of the past and present dynamical environment of the outer Solar System. Using data gathered from a host of facilities we have determined the mutual orbits for a sample of seven wide TNBs whose periods exceed

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