An Etymological Dictionary of Astronomy and Astrophysics
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The point where the → stellar wind makes a transition from → subsonic to → supersonic flow. In the particular case of a spherically symmetric wind (thus with no magnetic field), the distance from star, at which the sonic point occurs, is given by: r_s = (GM_*)/2c_s², where G is the → gravitational constant, M_* is the stellar mass, and c_s the → sound speed at the sonic point.

→ sonic; → point.