Key topics of this session are the recent developments in the study of non-thermal radio emissions from the Sun, the five radio planets, and potential radio emissions from exoplanets. Special emphasis is put on current missions like Cassini and STEREO, but new findings from data of ground radio-telescopes and older missions like Voyager, Galileo, Wind or Ulysses are also welcome. Presentations should focus on physical properties of radio emissions like rotational modulation, fine structures in dynamic spectra, polarization as well as source direction, and theorectical modeling and simulation of plasma and magnetic processes leading to their generation. Key questions for future missions like Juno, Solar Orbiter or JUICE can also be addressed. New developments in ground-based radio telescopes (e.g. LOFAR) will be matters of discussion, that should lead to a better coordination of ground- and space-based observations.