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Jupiter's decisive role in the inner Solar System's early evolution

Batygin, Konstantin and Laughlin, Greg (2015) Jupiter's decisive role in the inner Solar System's early evolution. Proceedings of the National Academy of Sciences of the United States of America, 112 (14). pp. 4214-4217. ISSN 0027-8424. PMCID PMC4394287. http://resolver.caltech.edu/CaltechAUTHORS:20150323-125531277

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Abstract

The statistics of extrasolar planetary systems indicate that the default mode of planet formation generates planets with orbital periods shorter than 100 days and masses substantially exceeding that of the Earth. When viewed in this context, the Solar System is unusual. Here, we present simulations which show that a popular formation scenario for Jupiter and Saturn, in which Jupiter migrates inward from a > 5 astronomical units (AU) to a ≈ 1.5 AU before reversing direction, can explain the low overall mass of the Solar System’s terrestrial planets, as well as the absence of planets with a < 0.4 AU. Jupiter’s inward migration entrained s ≳ 10−100 km planetesimals into low-order mean motion resonances, shepherding and exciting their orbits. The resulting collisional cascade generated a planetesimal disk that, evolving under gas drag, would have driven any preexisting short-period planets into the Sun. In this scenario, the Solar System’s terrestrial planets formed from gas-starved mass-depleted debris that remained after the primary period of dynamical evolution.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1073/pnas.1423252112DOIArticle
http://www.pnas.org/content/112/14/4214PublisherArticle
http://www.pnas.org/lookup/suppl/doi:10.1073/pnas.1423252112/-/DCSupplementalPublisherSupporting Information
http://www.ncbi.nlm.nih.gov/pmc/articles/PMC4394287/PubMed CentralArticle
ORCID:
AuthorORCID
Laughlin, Greg0000-0002-3253-2621
Additional Information:Copyright © 2015 National Academy of Sciences. Edited by Neta A. Bahcall, Princeton University, Princeton, NJ, and approved February 11, 2015 (received for review December 5, 2014. Published online before print March 23, 2015. We thank Dave Stevenson, Peter Goldreich, Mike Brown, Geoff Blake, and Christopher Spalding for enlightening conversations. Author contributions: K.B. and G.L. designed research, performed research, and wrote the paper. The authors declare no conflict of interest. This article is a PNAS Direct Submission. See Commentary on page 4189. This article contains supporting information online at www.pnas.org/lookup/suppl/doi:10.1073/pnas.1423252112/-/DCSupplemental.
Subject Keywords:Solar System formation; planetary dynamics; extrasolar planets
PubMed Central ID:PMC4394287
Record Number:CaltechAUTHORS:20150323-125531277
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20150323-125531277
Official Citation:Konstantin Batygin and Greg Laughlin Jupiter’s decisive role in the inner Solar System’s early evolution PNAS 2015 112 (14) 4214-4217; published ahead of print March 23, 2015, doi:10.1073/pnas.1423252112
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:55970
Collection:CaltechAUTHORS
Deposited By: Joy Painter
Deposited On:23 Mar 2015 20:51
Last Modified:19 Aug 2017 21:02

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