Introduction: Ridges
are the most common linear and tectonic surface features on Europa [1,2,3,4]
and apparent lateral offsets are often observed along them [4,5]. Ridges have
formed throughout Europa's geologic history, creating identifiable crosscutting
relationships [3,4]. These crosscutting relationships offer us an opportunity
to determine the mechanisms responsible for ridge formation [6,7]. Recent ridge
formation models characterize them as shearing-related [8]. We show evidence
for both lateral shearing and ridge-orthogonal motion along ridges, indicating
that apparent lateral offsets are not purely the result of strike-slip motions. First, apparent offsets along a ridge (or band) of interest
must be large enough to overcome Galileo's image resolution constraints.
Therefore, our analysis required us to perform a search of high resolution Galileo
images to focus on ridges with these characteristics. Second, in order for our
analysis to accurately determine the displacement ratio (DR) of strike-slip
offset motion to ridge-orthogonal motion, a ridge must have offset features
along its length with both low and high-angle orientations, a, relative to the ridge. At both small and large orientations (0° to
30° and 160° to 180°), apparent offsets due to convergence across the ridge may
become relatively large compared to where these angles are closer to 90° (for
which pure-ridge orthogonal motion gives an apparent offset of zero). Finally,
using ISIS software, each image chosen for our analysis was photometrically
corrected and reprojected to preserve local angular relationships and line
lengths using a transverse mercator or an orthographic projection, respectively
[9]. A technique developed by [6] uses simple geometric
measurements to provide a clear mode of fracture development and allows us to
create a verifiable model for ridge (and band) evolution. We present an
analysis of an unnamed band as a test for our method for determining
displacement ratios, and to quantify the deformation mechanisms of both a band
and a ridge. Analytical
Technique: The technique uses three
parameters that we can measure from each crosscut feature across a ridge or
band of interest. Separation (sep) is the perpendicular distance between a
displaced feature and its corresponding projection from the opposing side of
the ridge or band. Strike-slip offset (w) is the measurable distance along a
ridge between two parts of a displaced feature and alpha (a) is defined as the clockwise angle between the ridge or band of interest
and the displaced feature. Fault-orthogonal motion is defined by dilation (+d) or
contraction (-d). The measured separation and alpha angles are normalized and
corrected to account for the limited range of alpha angles found along the
ridge of interest (as detailed in [6]). These data sets are then compared to
unique analytical curves of various displacement ratios (DR). Figure 1 illustrates
several examples of right-lateral motion plus contraction displacement ratios,
and shows that each DR's curve is unique. Analogous curves have been produced
for left-lateral motions and for oblique dilations. Figure 1. Plots of various analytical solutions have been created to compare
against measured results to best determine the DR (strike-slip
offset:orthogonal motion) for each ridge or band investigated. Using a square correlation ratio (SCR)
we are able to determine goodness of fit of the data set to a specific type
curve. An SCR of 0 indicates that a correlation between the analytical solution
and the data set is no better than would be produced by a straight line plotted
through the average of the corrected normalized separations. An SCR of 1 would
be a perfect correlation between the data set and the analytical solution type
curve and all the data points would fall on the curve. Analysis
of an unnamed band: We analyze a simple linear band as a
simple test for the effectiveness of our technique (Figure 2). This image shows
an unnamed band in Europa's northern trailing hemisphere that both crosscuts
numerous lineaments and shows apparent offset of these lineaments along its
length. Using the technique described above, an SCR can be determined for the
fit of the data to our analytical Figure 2. An unnamed band in Galileo image s0449961865r
(23.1° N, 221.6° W). Crosscut features are shown in blue, projected features
(blue dashed lines), offsets are shown in red and separations are shown in
green. Resolution is ~220 m/pix. Figure
3. This graph illustrates a good
correlation (SCR of 0.976) between the normalized data set and the analytical
solution of a DR of 1:1. curves and a best fit can be found (Figure 3). The displacement
ratio (DR) of offset to dilation (opening) is approximately 1:1 indicating
right-lateral oblique dilation of this unnamed band. The SCR is high at 0.976
for the 1:1 DR. This high correlation is a reassurance that this method can be
used to determine formation mechanisms for linear features of interest that do
not have complex geologic histories. Argadnel Regio Ridge analysis: We analyze a portion of an unnamed ridge in Argadnel Regio (Figure 4)
in Europa's southern trailing hemisphere using our technique described above. The
SCR is relatively high, at 0.65, for a 2.5:1.1 DR (Figure 5). In other words,
this unnamed ridge underwent both right-lateral offset and dilation in the
ratio of ~ 2.5:1.1. Discussion: Our test of the analytical technique indicates that explicit deformation
mechanisms can be determined. Numerous linear ridges will need to be examined
to better determine deformation mechanisms of ridges that display lateral
offsets, especially considering that some ridges appear to show evidence for
concomitant offset and contraction [6,10,11]. Favorable ridge characteristics
for this analysis will include Figure
4. An unnamed ridge is shown here in
the Argadnel Regio region (Galileo image number s0426273839r). Features are
labeled using the same color scheme as in Fig. 2. Image resolution is ~50
m/pix. Figure
5. This graph illustrates a
relatively good correlation (SCR of 0.65) between the normalized data set and
the analytical solution of a DR of 2.5:1.1. linearity, numerous crosscut features with apparent
offsets large enough to overcome image resolutions, a variety of alpha angles
along the length of the ridge, and a high resolution to capture the apparent offsets
along the ridge. References: [1] Greenberg R et al. (1998) Icarus, 135, 64-78. [2] Figueredo P H
& Greeley R (2000) JGR, 105,
22,629-22,646. [3] Kattenhorn S A (2002) Icarus, 157, 490-506. [4] Spaun N A et al.
(2003) JGR, 108, E6, 1-21. [5] Kattenhorn S A (2004) Icarus, 172, 582-602. [6]
Vetter J C (2005) MS Thesis University of Idaho, Moscow, ID, U.S.A., 1-46. [7] McBee J H et al. (2003) LPSC
XXXIV, Abstract #1783. [8] Nimmo F & Gaidos E (2002) JGR, 107, 1-8. [9] Snyder J P & Voxland P M (1994) USGS Prof. Paper #1453, 1-249. [10]
Bader C E & Kattenhorn S A (2007) AGU Abstract P53B-1243. [11] Aydin, A (2006) JSG 28, 2222-2236.
Acknowledgements: This work is supported by the NASA-Idaho Space
Grant Consortium and NASA Grant #NNX06AC12G.Bader, C.E., Kattenhorn, S.A. (2008)
Formation mechanisms of Europan ridges with apparent lateral offsets
Lunar and Planetary Science Conference Abstracts XXXIX, #2036.





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