Magnetic Fields of Extrasolar Planets: Planetary Interiors and Habitability
J. Lazio (JPL, CIT), G. Hallinan (Caltech), V. Airapetian, (NASA/GSFC), D. A. Brain (Univ. Colorado, Boulder), C. F. Dong, (Princeton), P. E. Driscoll (Carnegie), J.-M. Griessmeier, (LPC2E-Universit\`e d'Orl\`eans/CNRS, Station de Radioastronomie de, Nan\c{c}ay

TL;DR
This paper discusses how magnetic fields of extrasolar planets, detectable via radio emissions, can reveal interior properties and assess planetary habitability, building on recent research and observational strategies.
Contribution
It synthesizes current knowledge on planetary magnetic fields, emphasizing their role in habitability and proposing methods for detecting extrasolar magnetic fields through radio emissions.
Findings
Magnetic fields are key to understanding planetary interiors.
Radio emissions can be used to measure extrasolar planetary magnetic fields.
Magnetic fields may influence planetary habitability.
Abstract
Jupiter's radio emission has been linked to its planetary-scale magnetic field, and spacecraft investigations have revealed that most planets, and some moons, have or had a global magnetic field. Generated by internal dynamos, magnetic fields are one of the few remote sensing means of constraining the properties of planetary interiors. For the Earth, its magnetic field has been speculated to be partially responsible for its habitability, and knowledge of an extrasolar planet's magnetic field may be necessary to assess its habitability. The radio emission from Jupiter and other solar system planets is produced by an electron cyclotron maser, and detections of extrasolar planetary electron cyclotron masers will enable measurements of extrasolar planetary magnetic fields. This white paper draws heavily on the W. M. Keck Institute for Space Studies report Planetary Magnetic Fields:…
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Taxonomy
TopicsAstro and Planetary Science · Stellar, planetary, and galactic studies · Astrophysics and Star Formation Studies
