The closest point in the path of a sound wave to the center of a star, as studied in
→ asteroseismology. Starting from the surface, the sound wave
first moves into the star almost straight toward the center. Its path then deflects,
because of the increasing → sound speed, so that it misses
the center of the star. After the turning point, the wave moves out again until it
reaches the surface, where it is reflected.
If exactly an integer number of wavelengths fits
between two reflections at the surface, the sound wave
corresponds to a → standing wave with a specific pattern of
→ node lines on the surface.
See also: → turn; → point.