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Related Experiment Videos

Extrasolar planets.

J J Lissauer1, G W Marcy, S Ida

  • 1Space Science Division, National Aeronautics and Space Administration, Ames Research Center, Moffett Field, CA 94035, USA. lissauer@ringside.arc.nasa.gov

Proceedings of the National Academy of Sciences of the United States of America
|October 18, 2000
PubMed
Summary

The discovery of extrasolar planets reveals massive gas giants orbiting close to their stars, challenging current planet formation theories. These findings necessitate modifications to existing models to explain observed exoplanetary system properties.

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The seventh inner moon of Neptune.

Nature·2019

Area of Science:

  • Astronomy
  • Astrophysics
  • Exoplanetary Science

Background:

  • The first extrasolar planet orbiting a Sun-like star was detected in 1995.
  • Over two dozen extrasolar planets have since been identified using Doppler spectroscopy.

Purpose of the Study:

  • To analyze the characteristics of detected extrasolar planets.
  • To evaluate prevailing theories of star and planet formation against observational data.

Main Methods:

  • Detection of extrasolar planets via periodic variations in stellar Doppler shift.
  • Characterization of planet mass, orbital distance, and orbital path.

Main Results:

  • All detected extrasolar planets are more massive than Saturn, with most exceeding Jupiter's mass.

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  • Many planets orbit closer to their stars than Mercury orbits the Sun.
  • Several planets exhibit highly elliptical orbits.
  • Conclusions:

    • Current planet formation models, based on Solar System observations, require adjustments.
    • The properties of observed extrasolar planetary systems present a challenge to existing theories.