Introduction: Voyager and Galileo showed that the surface of Europa
has undergone significant re-working at some point during the moon's
history. The surface is covered in
lineaments, which likely formed from the tides generated from Europa's eccentric
orbit around Jupiter [1]. There is also a relative paucity of visible impact
craters, suggesting a surface age of about 80 million years [2]. Therefore, all
of the visible surface features have formed within that time frame. This yields
a maximum age of the surface, but the search for a minimum age for tectonic
activity is more challenging. Ridgeless surface fractures [3] (also called troughs)
are the youngest tectonic features on the surface, cross cutting all other
fractures and occasionally regions of endogenic disruption (chaos). There have
been several mechanisms to explain the formation of these fractures [1, 4-5],
but the most likely of them seems to be formation by tectonic processes in the
ice shell. The tectonic activity
is likely caused by the tidal stress induced at the surface [1], but could also
be a result of stresses induced by nonsynchronous rotation (NSR) of the ice
shell, polar wander, or ice shell thickening. Europa is a good candidate to be currently under-going
active tectonics. Searching for the evidence of recent tectonic activity
logically starts with the geologically young, ridgeless surface fractures. This
project will develop comprehensive fracture maps of the re-cent surface
fractures using the program Arc GIS. Fractures have been mapped onto
spatially-referenced images with each fracture having a unique identifier and
embedded information about the length and orientation, the fracture
classification (described below), and the crosscutting relationship (older or
younger) between young fractures that intersect. Preliminary mapping has identified at least six
separate types of recent fractures that have distinct formation mechanisms: (1)
tectonic fractures; (2) cycloidal fractures; (3) tailcracks; (4) endogenic
process fractures; (5) flexure fractures; and (6) fold hinge fractures. Fracture
classification: Tectonic
Fractures: These fractures formed in
response to a global stress (tidal or otherwise). Tectonic fractures have also
been called regional fractures [6].
They can be >10 to 100s of km in length. Some of these fractures show
segmentation along their lengths, or may show evidence of having formed by the
coalescence of numerous segments. The temporal relationship of these features
relative to the other surface fractures could yield a clear answer to recent
tectonics on the moon through comparisons to theoretical stress patterns. Cycloidal
Fractures: A type of tectonic
fracture comprised of chains of arcuate lineaments that are individually up to
100s of km long and form in response to diurnal tidal stresses [7]. Their
shapes potentially record the location of their formation (relative to the
direction of Jupiter) due to the explicit, longitude-dependent stress field
needed to account for their formation.
Previous work has identified young cycloidal fractures [8] which could
provide the most likely indicator of whether or not cycloid development has continued
to the present day. Tailcracks: Similar to terrestrial tailcracks, these cracks
propagate from the tips of strike-slip faults and result from brittle failure
from fault motion in the tensile quadrant at a fault tip. Tailcracks are
secondary fractures that form in response to the locally perturbed stress
field, and may not a good indicator of the global stress field at the time of
formation, although they could conceivably indicate active strike-slip
faulting. Endogenic
Process Fractures: These fractures
are most commonly associated with a narrow strip of terrain around the rough
edges of chaos regions. Endogenic process fractures appear to be the secondary cracks
that form as a result of warping or disaggregation of the chaos region. Chaos
regions result from local processes likely driven by thermal upwelling and
diapirism in a convecting ice shell.
This process disrupts the brittle volume above a diapir [9-10], forming
regions of chaos or perhaps less developed lenticulae. Flexure
Fractures: These fractures are
primarily found along the flanks of large ridges, the large weight of which
impinges on the ice shell, causing elastic flexing that affects the local
stress field. Billings and
Kattenhorn (2005) showed that the tensile strength of ice could be exceeded by
bending stresses from the flexing of the elastic portion of the ice shell [11]. Fold Hinge
Fractures: Prockter and Pappalardo
(2000) examined Astypalaea Linea and found a region of undulating folds across
the surface of smooth band material in the fault zone [12]. They believed that the folding
was due to contraction of the ice shell, causing tension cracks to form along
the fold hinge. Discussion: The fractures described above each formed as a result
of different loading conditions. Therefore the presence of each type of
fracture and their relationship to the other fractures can begin to build a
temporal relationship of the stresses at the time of fracture formation. The interpreted stresses at the time of
formation of the fractures can be compared to the theoretical stress fields due
to diurnal tidal effects and any contributions by nonsynchronous rotation. Not all of the fracture types are good
indicators of the presence of active tectonics, however, due to the distinctly
local nature of their formation mechanisms and because they are not relatable
to a theoretical global stress state. Tectonic fractures are likely to be the best indicator
of recent tectonic activity. These are occasionally disrupted by chaos regions
or lenticulae. In the analysis of fracture maps, determining whether there is evidence that tectonic fractures
postdate chaos or lenticulae will be fundamental to making a case for active
tectonics, especially if the orientations of these fractures can be reconciled
with contemporary global stress fields. Cycloids should form with specific orientations that
are a function of the current stress field. A comparison of the most recent
cycloids to the current stress field could be a litmus test for active
tectonics of this type. Tailcracks indicate the sense of motion (right-lateral
or left-lateral) along the causal strike-slip fault. Therefore, if the sense of
motion is compatible with the current stress field, this could be an indicator
of active faulting. It is nonetheless
possible that the tailcracks formed in an older stress state that is similar to
the current state of stress, thereby providing a false positive test. Endogenic fractures are not tectonic in origin;
however, they form around geologically young regions of crustal
disruption and thus provide some age constraints on any other fractures that
crosscut them.Flexure fractures may provide clues to whether ridge development
continues to the present, if crosscutting relationships exist with other
fracture types; however, they are unlikely to a good indicator of active
tectonics. Fold hinge fractures are rare and typically short.
They are therefore of limited use in addressing the issue of active tectonics. By understanding the formation mechanics behind the
youngest fractures on the surface of Europa, it may ultimately be possible to
address whether or not there is active tectonics on the moon. References: [1] Greenberg, R., et al. (1998) Icarus 135, 64–78. [2] Zahnle, K., et al. (2003) Icarus 163 263-289. [3] Kattenhorn, S.A.
(2002) Icarus 157, 490-506. [4] Lucchita,
B. L., Soderblom L.A. (1982) In:
Satellites of Jupiter (D. Morrison, ed.), p.521. [5] Pappalardo, R.T. et
al., (1999) JGR 104, 24015–24055.
[6] Figueredo, P.H., Greeley, R. (2004) Icarus
167, 287-312. [7] Hoppa et al. (1999) Science
285, 1899-1902. [8] Marshall, S.T., Kattenhorn, S.A. (2005) Icarus 177, 341–366. [9] Collins, G.C et al. (1998) GRL 25, 233-236. [10] Schenk, P. M.,
Pappalardo, R.T. (2004) GRL 31
L16703, doi:10.1029/ 2004GL019978. [11] Billings, S.E., Kattenhorn S. A. (2005)
Icarus 177, 397-412. [12] Prockter,
L. M., Pappalardo, R.T. (2000) Science. 289, 941–943.Kay, J.P., Kattenhorn, S.A. (2009)
Searching for evidence of active tectonics on Europa
Lunar and Planetary Science Conference Abstracts XL, #2454.
Entire document in original PDF format (requires Adobe Acrobat Reader)
Citations:
This abstract has been cited in the following works:
None at present.