論文

本文へのリンクあり
2020年10月

Solar system physics for exoplanet research

Publications of the Astronomical Society of the Pacific
  • J. Horner
  • S. R. Kane
  • J. P. Marshall
  • P. A. Dalba
  • T. R. Holt
  • J. Wood
  • H. E. Maynard-Casely
  • R. Wittenmyer
  • P. S. Lykawka
  • M. Hill
  • R. Salmeron
  • J. Bailey
  • T. Löhne
  • M. Agnew
  • B. D. Carter
  • C. C.E. Tylor
  • 全て表示

132
1016
開始ページ
1
終了ページ
115
記述言語
英語
掲載種別
研究論文(学術雑誌)
DOI
10.1088/1538-3873/ab8eb9
出版者・発行元
IOP PUBLISHING LTD

© 2020. The Astronomical Society of the Pacific. Printed in the U.S.A. Over the past three decades, we have witnessed one of the great revolutions in our understanding of the cosmos— the dawn of the Exoplanet Era. Where once we knew of just one planetary system (the solar system), we now know of thousands, with new systems being announced on a weekly basis. Of the thousands of planetary systems we have found to date, however, there is only one that we can study up-close and personal—the solar system. In this review, we describe our current understanding of the solar system for the exoplanetary science community—with a focus on the processes thought to have shaped the system we see today. In section one, we introduce the solar system as a single well studied example of the many planetary systems now observed. In section two, we describe the solar systemʼs small body populations as we know them today—from the two hundred and five known planetary satellites to the various populations of small bodies that serve as a reminder of the systemʼs formation and early evolution. In section three, we consider our current knowledge of the solar systemʼs planets, as physical bodies. In section four we discuss the research that has been carried out into the solar systemʼs formation and evolution, with a focus on the information gleaned as a result of detailed studies of the systemʼs small body populations. In section five, we discuss our current knowledge of planetary systems beyond our own—both in terms of the planets they host, and in terms of the debris that we observe orbiting their host stars. As we learn ever more about the diversity and ubiquity of other planetary systems, our solar system will remain the key touchstone that facilitates our understanding and modeling of those newly found systems, and we finish section five with a discussion of the future surveys that will further expand that knowledge.

リンク情報
DOI
https://doi.org/10.1088/1538-3873/ab8eb9
arXiv
http://arxiv.org/abs/arXiv:2004.13209
Web of Science
https://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=JSTA_CEL&SrcApp=J_Gate_JST&DestLinkType=FullRecord&KeyUT=WOS:000569631300001&DestApp=WOS_CPL
Scopus
https://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=85093963806&origin=inward 本文へのリンクあり
Scopus Citedby
https://www.scopus.com/inward/citedby.uri?partnerID=HzOxMe3b&scp=85093963806&origin=inward
URL
http://arxiv.org/abs/2004.13209v1
URL
http://arxiv.org/pdf/2004.13209v1 本文へのリンクあり
ID情報
  • DOI : 10.1088/1538-3873/ab8eb9
  • ISSN : 0004-6280
  • eISSN : 1538-3873
  • arXiv ID : arXiv:2004.13209
  • SCOPUS ID : 85093963806
  • Web of Science ID : WOS:000569631300001

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