How does the period and angular velocity of the planet change with the distance from the central celestial body?

How does the period and angular velocity of the planet change with the distance from the central celestial body?

GMm/R^2 =m(2∏/T)^2*R=mV^2/R=mω^2R=ma
The farther away R is, the larger R is. If we deform the above formula, we can get that t becomes larger
V, W, a are all smaller