Features:
It should be quasi-infinite compared to the Earth---but that is undrawable.
v = r * (2πf) ,
where r is radius perpendicular to the rotation axis and f is the frequency of rotation. For the at-rest Earth reference frame, f=1/( 86164.1 s) where 86164.1 s = 1 sidereal day. We have the special cases:
v = 0.4651 km/s = 1.551*10**(-6) * c for r = 6378.1 km/s = Earth equatorial radius, v = 1.091*10**5 km/s = 0.03639 * c for r= 1.495978707*10**8 km = 1 astronomical unit, v = 7506 * c for r= 3.0856775814671900*10**13 km = 1 parsec.