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Singer et al. Europa Graben Data for JGR Planets Publication Titled "Thin Ice Lithospheres and High Heat Flows on Europa from Large Impact Structure Ring-graben"

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DataCite Commons2025-08-11 更新2024-09-03 收录
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https://figshare.com/articles/dataset/Singer_et_al_Europa_Graben_Data_for_JGR_Planets_Publication_Titled_Thin_Ice_Lithospheres_and_High_Heat_Flows_on_Europa_from_Large_Impact_Structure_Ring-graben_/22336048
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These are the data associated with a Singer et al. manuscript submitted to the Journal of Geophysical Research - Planets. The title is "Thin Ice Lithospheres and High Heat Flows on Europa from Large Impact Structure Ring-graben". Publication information, including a DOI, will be updated upon completion of the peer review process.<b>Abstract: </b>Craters are probes of planetary surface and interior properties. Here we measure depths, widths, and spacing of circumferential ring-graben surrounding the two largest multiring impact structures on Europa, Tyre and Callanish. We estimate formation conditions including the ice shell structure. The radial extension necessary to form these graben is thought to be caused by asthenospheric drag of warmer, more ductile ice and/or water flowing towards the excavated center of the crater, under a brittle-elastic lithospheric lid. Measurements of graben depths from stereo-photoclinometric digital elevation models result in estimates of displacement, strain, and stress experienced by the ice shell. Graben widths are used to estimate the intersection depth of the bounding normal faults, a quantity related to the brittle-ductile transition depth that approximates elastic shell thickness during crater collapse. Heat flows at the time of crater formation as well as ice lithosphere and total shell thickness are thus also constrained. Average widths and depths tend to decrease with increasing distance from the structure center, while inter-graben spacing generally increases. Varied assumptions yield plausible total conductive ice shell thickness estimates between 4–8 and 2.5–5 km for Tyre and Callanish, respectively, and heat flows of ~70-115 (±30) mW m<sup>-2</sup> for realistic thermal conductivities, consistent with other geophysical estimates for Europa. Higher heat flows are consistent with thin (≲10 km), conductive ice shells and impact breaching, or penetration of the stagnant lid for a convecting ice shell. Callanish, geologically younger, formed in a time or region of greater heat flow than Tyre.
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figshare
创建时间:
2023-03-25
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