File:Eccentric and True Anomaly.svg

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t ) {\displaystyle y(t)=b\sin(t)} The parameter t : is called the eccentric anomaly in astronomy is not the angle of ( x ( t ) , y ( t ) ) {\displaystyle

motion such that its revolution would be completed in its actual time. Eccentric anomaly is defined thus:—Draw the circumscribing circle of the elliptic orbit

t ) {\displaystyle y(t)=b\sin(t)} The parameter t : is called the eccentric anomaly in astronomy is not the angle of ( x ( t ) , y ( t ) ) {\displaystyle