We analyze the trajectory perturbations that result in phugoid oscilla
tions during the grazing planetary entry of space vehicles starting wi
th near-circular speed, in ballistic and equilibrium glide modes. The
equations for planar entry are transformed into a dimensionless system
appropriate for an analytical integration that provides accurate resu
lts in comparison with those obtained from a numerical integration of
the original system. For ballistic entry, the small perturbation in th
e flight-path angle is a lightly damped oscillation with long period,
while the perturbation in the density (altitude) increases as the spee
d decreases. Nevertheless, the relative change in the density is decre
asing, and the phugoid in ballistic entry is termed stable in both the
Right-path angle and the altitude. For glide entry, in the reference
solution where there is equilibrium of forces along the normal to the
flight path, both the flight-path angle and the altitude have a steady
decrease along the Right path. With a slight perturbation in either t
he initial speed or the initial Right-path angle, or both, the traject
ory variables undergo a damped oscillation about the reference traject
ory, Both the damping and the frequency are obtained explicitly, and t
hey correctly predict the phugoid motion as seen in the numerical solu
tion.