These orbitals all have some angular momentum , and in the planetary model , they correspond to particles in orbit with eccentricity less than 1.0 .
Orbitals do not pass straight through the center of the primary body .
These orbitals all have some angular momentum , and in the planetary model , they correspond to particles in orbit with eccentricity less than 1.0 , so that they do not pass straight through the center of the primary body .