2019
DOI: 10.1029/2019gl085903
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Is Airy Isostasy Applicable to Icy Moons?

Abstract: Airy isostasy is commonly used in planetary science to explain the relationship between crustal thickness variations and topography. Recently, several researchers have questioned the validity of this concept and proposed alternative approaches. Here we examine the accuracy of these approaches by comparing their results with those obtained from the numerical solution of the equations governing the flow in the crust of a small icy moon with a subsurface ocean. We find that the traditional approach based on appli… Show more

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Cited by 19 publications
(10 citation statements)
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“…Their model shows that the distribution of heat flux along the seafloor is dominated by radially advecting water that varies laterally in temperature. These narrow upwellings are characterized as powerful hotspots, from 1 to 5 GW, with temperatures in excess of 363 K. For a core radius of ~190 km 45 and assuming that heat flux at the surface is confined to an area comparable in size to the modeled hotspots in ref. 24 approximately 10% of the polar area-we estimate a heat flux of ~3 GW, which fits well into this 1-5 GW range.…”
Section: Resultsmentioning
confidence: 99%
See 1 more Smart Citation
“…Their model shows that the distribution of heat flux along the seafloor is dominated by radially advecting water that varies laterally in temperature. These narrow upwellings are characterized as powerful hotspots, from 1 to 5 GW, with temperatures in excess of 363 K. For a core radius of ~190 km 45 and assuming that heat flux at the surface is confined to an area comparable in size to the modeled hotspots in ref. 24 approximately 10% of the polar area-we estimate a heat flux of ~3 GW, which fits well into this 1-5 GW range.…”
Section: Resultsmentioning
confidence: 99%
“…3c. Varying the ocean thicknesses H at 20 km, 40 km, and 60 km to accommodate the distribution of ice shell thickness variations 9,16,45,46 leads to turbulent length scales on the order of 100's of meters to a few kilometers. Figure 3d shows free-fall velocity versus heat flux.…”
Section: Resultsmentioning
confidence: 99%
“…The basin topography is thus only used to (a) evaluate the gravity anomaly (see Equation 11in Supporting Information S1) and to (b) estimate the initial ocean/shell boundary uplift. For this, we employ the assumption of Airy isostasy (Airy, 1855;Bursa & Pec, 2013;Cadek et al, 2019) using the findings by Johnson et al (2016) that a positive gravity anomaly can only be obtained if the ocean density is higher than ∼1,100 kg ⋅ m −3 . This value, which we adopt in our study, can be the result of 5%-10% MgSO 4 dissolved in Pluto's ocean (Vance et al, 2018).…”
Section: Boundary and Initial Conditionsmentioning
confidence: 99%
“…In addition, this paradigm of fast hydrothermal plume transport is also the basis of models explaining various surface geological features or surface shell thickness variations on icy satellites (e.g. Čadek et al, 2019;Kvorka et al, 2018) using model results from solid core processes. Finally, an efficient transport from seafloor to ice shell (and potentially to the surface through jets or other cryovolcanism) is a key motivator for future space missions to these bodies seeking extraterrestrial life, especially mission concepts arguing for landing on the ice shell and scooping surface material deposited by the plumes (Choblet et al, 2021;MacKenzie et al, 2022).…”
Section: Introductionmentioning
confidence: 99%