Spatial distribution of ice blocks on Enceladus and implications for their origin and emplacement
We have mapped the locations of over 100,000 ice blocks across the south polar region of Saturn's moon Enceladus, thus generating the first quantitative estimates of ice-block number density distribution in relation to major geological features. Ice blocks were manually identified and mapped fr...
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ftcaltechauth:oai:authors.library.caltech.edu:p0vkm-4dr47 2024-10-13T14:10:51+00:00 Spatial distribution of ice blocks on Enceladus and implications for their origin and emplacement Martens, Hilary R. Ingersoll, Andrew P. Ewald, Shawn P. Helfenstein, Paul Giese, Bernd 2015-01-01 https://doi.org/10.1016/j.icarus.2014.09.035 unknown Elsevier https://doi.org/10.1016/j.icarus.2014.09.035 eprintid:53171 info:eu-repo/semantics/openAccess Other Icarus, 245, 162-176, (2015-01-01) Enceladus Satellites surfaces Geological processes Ices info:eu-repo/semantics/article 2015 ftcaltechauth https://doi.org/10.1016/j.icarus.2014.09.035 2024-09-25T18:46:43Z We have mapped the locations of over 100,000 ice blocks across the south polar region of Saturn's moon Enceladus, thus generating the first quantitative estimates of ice-block number density distribution in relation to major geological features. Ice blocks were manually identified and mapped from twenty of the highest resolution (4–25 m per pixel) Cassini Imaging Science Subsystem (ISS) narrow-angle images using ArcGIS software. The 10–100 m-diameter positive-relief features are marginally visible at the resolution of the images, making ice-block identifications difficult but not impossible. Our preliminary results reveal that ice blocks in the southern hemisphere are systematically most concentrated within the geologically active South Polar Terrain (SPT) and exhibit peak concentrations within 20 km of the tiger-stripe fractures as well as close to the south pole. We find that ice blocks are concentrated just as heavily between tiger-stripe fractures as on the directly adjacent margins; although significant local fluctuations in ice-block number density do occur, we observe no clear pattern with respect to the tiger stripes or jet sources. We examine possible roles of several mechanisms for ice-block origin, emplacement, and evolution: impact cratering, ejection from fissures during cryovolcanic eruptions, tectonic disruption of lithospheric ice, mass wasting, seismic disturbance, and vapor condensation around icy fumeroles. We conclude that impact cratering as well as mass wasting, perhaps triggered by seismic events, cannot account for a majority of ice-block features within the inner SPT. The pervasiveness of fracturing at many size scales, the ubiquity of ice blocks in the inner SPT, as well as the occurrence of linear block arrangements that parallel through-cutting crack networks along the flanks of tiger stripes indicate that tectonic deformation is an important source of blocky-ice features in the SPT. Ejection during catastrophic cryovolcanic eruptions and condensation around surface vents, ... Article in Journal/Newspaper South pole Caltech Authors (California Institute of Technology) South Pole Stripe ENVELOPE(9.914,9.914,63.019,63.019) Icarus 245 162 176 |
institution |
Open Polar |
collection |
Caltech Authors (California Institute of Technology) |
op_collection_id |
ftcaltechauth |
language |
unknown |
topic |
Enceladus Satellites surfaces Geological processes Ices |
spellingShingle |
Enceladus Satellites surfaces Geological processes Ices Martens, Hilary R. Ingersoll, Andrew P. Ewald, Shawn P. Helfenstein, Paul Giese, Bernd Spatial distribution of ice blocks on Enceladus and implications for their origin and emplacement |
topic_facet |
Enceladus Satellites surfaces Geological processes Ices |
description |
We have mapped the locations of over 100,000 ice blocks across the south polar region of Saturn's moon Enceladus, thus generating the first quantitative estimates of ice-block number density distribution in relation to major geological features. Ice blocks were manually identified and mapped from twenty of the highest resolution (4–25 m per pixel) Cassini Imaging Science Subsystem (ISS) narrow-angle images using ArcGIS software. The 10–100 m-diameter positive-relief features are marginally visible at the resolution of the images, making ice-block identifications difficult but not impossible. Our preliminary results reveal that ice blocks in the southern hemisphere are systematically most concentrated within the geologically active South Polar Terrain (SPT) and exhibit peak concentrations within 20 km of the tiger-stripe fractures as well as close to the south pole. We find that ice blocks are concentrated just as heavily between tiger-stripe fractures as on the directly adjacent margins; although significant local fluctuations in ice-block number density do occur, we observe no clear pattern with respect to the tiger stripes or jet sources. We examine possible roles of several mechanisms for ice-block origin, emplacement, and evolution: impact cratering, ejection from fissures during cryovolcanic eruptions, tectonic disruption of lithospheric ice, mass wasting, seismic disturbance, and vapor condensation around icy fumeroles. We conclude that impact cratering as well as mass wasting, perhaps triggered by seismic events, cannot account for a majority of ice-block features within the inner SPT. The pervasiveness of fracturing at many size scales, the ubiquity of ice blocks in the inner SPT, as well as the occurrence of linear block arrangements that parallel through-cutting crack networks along the flanks of tiger stripes indicate that tectonic deformation is an important source of blocky-ice features in the SPT. Ejection during catastrophic cryovolcanic eruptions and condensation around surface vents, ... |
format |
Article in Journal/Newspaper |
author |
Martens, Hilary R. Ingersoll, Andrew P. Ewald, Shawn P. Helfenstein, Paul Giese, Bernd |
author_facet |
Martens, Hilary R. Ingersoll, Andrew P. Ewald, Shawn P. Helfenstein, Paul Giese, Bernd |
author_sort |
Martens, Hilary R. |
title |
Spatial distribution of ice blocks on Enceladus and implications for their origin and emplacement |
title_short |
Spatial distribution of ice blocks on Enceladus and implications for their origin and emplacement |
title_full |
Spatial distribution of ice blocks on Enceladus and implications for their origin and emplacement |
title_fullStr |
Spatial distribution of ice blocks on Enceladus and implications for their origin and emplacement |
title_full_unstemmed |
Spatial distribution of ice blocks on Enceladus and implications for their origin and emplacement |
title_sort |
spatial distribution of ice blocks on enceladus and implications for their origin and emplacement |
publisher |
Elsevier |
publishDate |
2015 |
url |
https://doi.org/10.1016/j.icarus.2014.09.035 |
long_lat |
ENVELOPE(9.914,9.914,63.019,63.019) |
geographic |
South Pole Stripe |
geographic_facet |
South Pole Stripe |
genre |
South pole |
genre_facet |
South pole |
op_source |
Icarus, 245, 162-176, (2015-01-01) |
op_relation |
https://doi.org/10.1016/j.icarus.2014.09.035 eprintid:53171 |
op_rights |
info:eu-repo/semantics/openAccess Other |
op_doi |
https://doi.org/10.1016/j.icarus.2014.09.035 |
container_title |
Icarus |
container_volume |
245 |
container_start_page |
162 |
op_container_end_page |
176 |
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1812818379155701760 |