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rotating star
setâre-ye carxân, ~ carxandé
Fr.: étoile en rotation
A star that has a non-zero → angular velocity.
In a rotating star, the → centrifugal forces reduce the
→ effective gravity according to the latitude and also
introduce deviations from sphericity. In a rotating star, the equations of stellar
structure need to be modified. The usual spherical coordinates must be replaced
by new coordinates characterizing the → equipotentials. |