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Exoplanet orbital eccentricity: multiplicity relation and the Solar System.

Mary Anne Limbach1, Edwin L Turner2

  • 1Departments of Astrophysical Sciences and Mechanical and Aerospace Engineering, Princeton University, Princeton, NJ 08544; and.

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Summary
This summary is machine-generated.

The Solar System is not unusual among exoplanetary systems. A new study reveals orbital eccentricity decreases with more planets, fitting our Solar System into the broader cosmic context.

Keywords:
Solar Systemdynamical evolutionorbital eccentricitiesradial velocity

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Area of Science:

  • Exoplanetary Science
  • Astronomy
  • Astrophysics

Background:

  • Exoplanetary systems often display higher orbital eccentricities compared to our Solar System.
  • This has led to the prevailing view that the Solar System is atypical.

Purpose of the Study:

  • To investigate the relationship between orbital eccentricity and system multiplicity in exoplanetary systems.
  • To re-evaluate the Solar System's typicality within the broader population of planetary systems.

Main Methods:

  • Analysis of cataloged radial velocity (RV) exoplanetary systems.
  • Statistical examination of orbital eccentricity and the number of planets per system.
  • Extrapolation of observed trends to compare with the Solar System's configuration.

Main Results:

  • A strong anticorrelation was found between orbital eccentricity and system multiplicity.
  • The Solar System's eccentricity distribution aligns with this anticorrelation when its eight-planet multiplicity is considered.
  • Even as a single or double-planet system, the Solar System occupies a common region in eccentricity-multiplicity space.

Conclusions:

  • The Solar System is not anomalous regarding orbital eccentricities when system multiplicity is accounted for.
  • Orbital eccentricity decreases as a power law with increasing system multiplicity (index -1.20).
  • Low eccentricities may favor higher planet multiplicities, potentially increasing the prevalence of habitable systems.