To quantify shape changes, we measured the length of each rubble pile's axes
after encounter (
), calculated the axis ratios (
and
), and defined a single-value
measure of the remnant's ``ellipticity'' (
). For reference, our progenitor has
and Geographos has a value of
.
Sampling a broad set of parameters to map tidal disruption outcomes,
Richardson et al. (1998) identified 195 S, B, or M-class events produced with
a
rubble pile. Fig. 2 shows this set with
ellipticity plotted against the fraction of mass shed by the progenitor during
tidal disruption.
fig2
We find that, in general, S-class events tend to yield lower ellipticity
values; only 2 of the 79 outcomes are likely to have a Geographos-like
elongations (
). The mean value of
for the S-class events is 0.22 with standard
deviation
= 0.14. The near-spherical shapes produced by S-class
events are a by-product of gravitational instabilities in the fragment chain
which readily agglomerate scattered particles as they recede from the planet.
B-class events do not show a simple trend with respect to ellipticity, though
these values tend to increase as the degree of mass shedding decreases. We
find that 5 of 40 outcomes have Geographos-like
values. The mean value of
for all 40 B-class events
is 0.45 (
), very close to the starting ellipticity of 0.43.
M-class events are most effective at increasing
and
creating Geographos-like shapes, probably because tidal torques must first
stretch and/or spin-up the rubble pile before particles or clumps can be
ejected near the ends of the body. Fig. 2 shows 23 of 76 M-class events with
Geographos-like
values. Overall, the 76 outcomes
have a mean
with
.
Thus,
getting a Geographos-like ellipticity from a M-class disruption is less than a
1
event, decent odds if such disruptions (and
progenitors) are common.