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Solar System Physics for Exoplanet Research

TLDR
In this paper, the authors present a review of the 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.
Abstract
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.

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Citations
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Journal ArticleDOI

Theoretical constraints imposed by gradient detection and dispersal on microbial size in astrobiological environments

TL;DR: The connections between information acquisition, motility, and microbial size are explored from an explicitly astrobiological standpoint and the constraints on organism size imposed by gradient detection and motility are elucidated in the form of simple heuristic scaling relations.
Journal ArticleDOI

Astrocladistics of the Jovian Trojan Swarms

TL;DR: The Jovian Trojans are two swarms of small objects that share Jupiter's orbit, clustered around the leading and trailing Lagrange points, L4 and L5 as mentioned in this paper.
Journal ArticleDOI

HD 83443c: A Highly Eccentric Giant Planet on a 22 yr Orbit

TL;DR: In this paper , the authors reported the discovery of a highly eccentric long-period Jovian planet orbiting the hot-Jupiter host HD 83443, which is a rare example of a system hosting a hot Jupiter and an exterior planetary companion.
Journal ArticleDOI

HD 183579b: a warm sub-Neptune transiting a solar twin detected by TESS

Tianjun Gan, +58 more
TL;DR: In this article, the authors reported the discovery and characterization of a transiting warm sub-Neptune planet around the nearby bright solar twin HD 183579, delivered by the Transiting Exoplanet Survey Satellite (TESS).
References
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Journal ArticleDOI

Gaia Data Release 2. Summary of the contents and survey properties

Anthony G. A. Brown, +452 more
TL;DR: The second Gaia data release, Gaia DR2 as mentioned in this paper, is a major advance with respect to Gaia DR1 in terms of completeness, performance, and richness of the data products.
Journal ArticleDOI

The Gaia mission

T. Prusti, +624 more
TL;DR: Gaia as discussed by the authors is a cornerstone mission in the science programme of the European Space Agency (ESA). The spacecraft construction was approved in 2006, following a study in which the original interferometric concept was changed to a direct-imaging approach.
Journal ArticleDOI

A Jupiter-Mass Companion to a Solar-Type Star

Michel Mayor, +1 more
- 23 Nov 1995 - 
TL;DR: The presence of a Jupiter-mass companion to the star 51 Pegasi is inferred from observations of periodic variations in the star's radial velocity as discussed by the authors, which would be well inside the orbit of Mercury in our Solar System.
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