Electron-cyclotron maser emission from Earth-like planets around degenerate stars

Details Electron-cyclotron maser emission from Earth-like planets around degenerate stars Electron-cyclotron maser emission from Earth-like planets around degenerate stars

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003eaeja.....4873w&link_type=abstract

EGS - AGU - EUG Joint Assembly, Abstracts from the meeting held in Nice, France, 6 - 11 April 2003, abstract #4873

Physics

Scientific paper

By analogy to Jovian radio emissions produced by the electrodynamic interaction between Jupiter and its moons Io, Ganymede and Callisto, we predict that terrestrial planets around magnetic white dwarf stars can produce an observable radio signature. We discuss formation scenarios of white-dwarf planetary systems and present a simple model to predict radio flux densities and planetary system lifespans. Particular emphasis is placed here on constraints on the detectability of white-dwarf planetary systems using LOFAR.

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