Introduction: The surface of Europa consists of an intensely
fractured ice shell that is floating on a subsurface ocean of liquid water [1].
Compelling evidence for a floating ice shell comes from the presence of arcuate
tensile cracks (or cycloids) [2]. Cycloids consist of curved segments linked
together at cusps (Fig. 1). Individual cycloid chains of 100s - 1000s km in
length are observed at a variety of orientations in nearly every imaged region
of Europa.

Fig. 1. (a) Image of
a cycloid in the E15RegMap01 area. (b) Trace of the cycloid with cusp and
segment labels. The different cusp types (simple and complex) are also
indicated.
Crack growth is
strongly controlled by rotating diurnal stresses in the ice shell that result
from oscillating tidal bulges in the subsurface ocean [2, 3, 4]. However, the
long-term stress component due to nonsynchronous rotation (NSR) of the ice
shell also likely affects the overall distribution and patterns of cycloidal
features observed on the surface [5]. While geologic mapping has revealed
cycloids are geologically recent, relative age sequences documenting multiple
episodes of cycloid formation are needed to study changes in cycloid
characteristics (i.e., orientation, morphology) over time. Using age sequences determined
through cross-cutting relationships, and conventional means of interpreting NSR
based on a consistent rotation of fracture orientations through time, we have
estimated the amount of NSR that occurred purely since the onset of cycloid
development in the E15RegMap01 area.
Cycloids in the
E15RegMap01 Area: The E15RegMap01
mosaic (Fig. 2a), located in the northern trailing hemisphere, spans latitudes
19 to 62°N and longitudes 212 to 234°W. Twenty-two cycloids have been
identified in the mosaic [4], 14 of which (Fig. 2b) could be fitted into a
relative age sequence based on cross-cutting relationships of both cycloids and
other lineaments. The remaining 8 cycloids had an insufficient number of
cross-cutting features to fit them into the age sequence.
In the northern
hemisphere, the diurnal stress field rotates in a counterclockwise sense. This
allows cycloid chain growth directions to be predicted based on the direction
cusps point [2]. As indicated in Fig. 2b, there are two predominant cycloid
growth directions in the E15RegMap01 area: ~ N-S oriented cycloid chains that
grow from N to S and ENE-WSW oriented cycloid chains that grow from ENE to WSW.
Cycloids are, in
general, some of the youngest features in the E15RegMap01 area. However, each
of the 22 cycloids identified is cross-cut at least once by younger features.
These younger features include other lineaments (cycloids, ridges, troughs, or
bands) and, to a lesser extent, chaos, pits, or craters. The oldest cycloids
studied are predominantly cut by non-cycloidal features but the youngest
cycloids are predominantly cut by other cycloids and are only occasionally cut
by non-cycloidal features. Therefore, the onset of cycloid development in this
area does not indicate the end of the formation of non-cycloidal fractures.
Most cycloid segments
are defined by double ridges but there are a few band and trough cycloids
observed in the mosaic. All of the 14 cycloid chains fitted into the age
sequence have predominantly double ridge morphologies. Cycloid cusps are either
simple (one splay) or complex (multiple splays) (Fig. 1b). Neither segment nor
cusp morphologies appear to show a preferential pattern through time.
Nonsynchronous
Rotation Implications: Cycloid chain
orientations have rotated in a clockwise sense through time which is consistent
with previous NSR studies in the northern hemisphere (e.g., [6, 7, 8]).
Relative age sequences determined through cross-cutting relationships of 14
cycloid chains in the E15RegMap01 area have been used to estimate the amount of
NSR that occurred between the formation of the oldest and youngest cycloids
studied. Based purely on average cycloid chain orientations, there has been at
least 600° of NSR during cycloid development in this area (Fig. 3).

Fig. 2. (a)
E15RegMap01 image mosaic. (b) Traces of the 14 cycloid chains fitted into the
age sequence. The colors grade from darkest blue (oldest cycloid) to red
(youngest cycloid) and the arrows indicate growth direction.
Previous NSR studies
based on detailed fracture maps of the leading hemisphere [7] and the Bright
Plains region [8] reported NSR amounts of 360-720° and 720-900° respectively.
The minimum of 600° of NSR found in this study is based purely on average
cycloid chain orientations. If the orientations of other non-cycloidal
lineaments that cross-cut the 14 cycloids studied are taken into account, the
minimum amount of NSR would be much greater. Therefore, this study suggests
that the amount of NSR may be significantly higher than previously reported.
Fig. 3 shows the
amount of NSR that has occurred between time steps in cycloid formation. Older
time steps tend to have larger amounts of NSR between each other than younger
time steps. Therefore, the amount of NSR between periods of cycloid growth is
temporally variable and there are potentially long time intervals between
episodes of cycloid formation. An average of 8.4 cycloids grow per NSR period
based on the minimum of 600° of NSR that occurred during the development of the
14 cycloids studied.
Two previous studies
have constrained 1 NSR period to be between 12,000 [9] and 240,000 [3] years.
Using those estimates and our 600° minimum amount of NSR and assuming a
consistent rotation of fracture orientations through time, the minimum duration
of cycloid development in this region has been constrained to between 20,000
and 400,000 years. However, recent work [10] suggests NSR does not occur at a
constant rate through time due to thickening of the ice shell. This implies that
the constraint on the minimum duration of cycloid development may not be
representative of the actual duration.

Fig. 3. Rose diagram
showing average cycloid chain orientations through time. Each ring represents a
time step in the age sequence with the first ring being the oldest. Colors also
represent time steps with blue being older and red being younger (as in Fig.
2b).
References: [1] Pappalardo, R.T. et al. (1999) JGR 104, 24,015-24,055. [2] Hoppa, G.V. et al. (1999) Science
285, 1899-1902. [3] Hoppa, G.V. et
al. (2001) Icarus 153, 208-213.
[4] Marshall & Kattenhorn (2005) Icarus 177, 341-366. [5] Gleeson et al. (2005) LPSC XXXVI,
Abstract #2364. [6] Geissler, P.E. et al. (1998) Icarus 135, 107-126. [7] Figueredo, P.H. & Greeley, R. (2000)
JGR 105, 22,629-22,646. [8]
Kattenhorn, S.A. (2002) Icarus 157,
490-506. [9] Hoppa, G. et al. (1999) Icarus 137, 341-347. [10] Nimmo, F. et al. (2005) Eos Trans.
AGU 86, Abstract #P22A-05.