FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W4381800208> ?p ?o ?g. }

• W4381800208 endingPage "118270" @default.
• W4381800208 startingPage "118270" @default.
• W4381800208 abstract "Planets and moons reorient in space due to mass redistribution associated with various types of internal and external processes. While the equilibrium orientation of a tidally locked body is well understood, much less explored are the dynamics of the reorientation process (or true polar wander, TPW, used here for the motion of either the rotation or the tidal pole). TPW dynamics can be non-trivial and are important for predicting the patterns of TPW-induced surface fractures, as well as for assessing whether enough time has passed for the equilibrium orientation to be reached. The only existing and relatively complex numerical method for an accurate evaluation of the reorientation dynamics of a tidally locked body was described in a series of papers by Hu et al., 2017a, Hu et al., 2017b, Hu et al., 2019. Here we demonstrate that an identical solution can be obtained with a simpler approach, denoted as oω||mMIA, because during TPW the tidal and the rotation axes closely follow respectively the minor and the major axes of the total, time-evolving inertia tensor of the body. Motivated by the presumed reorientation of Pluto, the use of the oω||mMIA method is illustrated on several test examples. In particular, we vary the load sign and the mass of the host body and analyze whether TPW paths are curved or straight. When tidal forcing is relatively small, the paths of negative anomalies (e.g. basins) towards the rotation pole are highly curved, while positive loads may reach the sub- or anti-host point straightforwardly. The obtained behavior is explained by the relative timing of longitudinal and latitudinal reorientation. Our results suggest that the Sputnik Planitia basin cannot be a negative anomaly at present day, and that the remnant figure of Pluto must have formed prior to the reorientation. Finally, the presented method is complemented with an energy balance that can be used to test the numerical solution and to quantify the changes in orbital distance due to TPW. A new release of the custom written code LIOUSHELL that is used to perform the simulations is made freely available on GitHub." @default.
• W4381800208 created "2023-06-24" @default.
• W4381800208 creator A5050800567 @default.
• W4381800208 creator A5068791144 @default.
• W4381800208 date "2023-09-01" @default.
• W4381800208 modified "2023-10-18" @default.
• W4381800208 title "Dynamic reorientation of tidally locked bodies: Application to Pluto" @default.
• W4381800208 cites W1914353419 @default.
• W4381800208 cites W1965621013 @default.
• W4381800208 cites W1993044327 @default.
• W4381800208 cites W2007106925 @default.
• W4381800208 cites W2045456018 @default.
• W4381800208 cites W2054794276 @default.
• W4381800208 cites W2060034575 @default.
• W4381800208 cites W2062226426 @default.
• W4381800208 cites W2077499895 @default.
• W4381800208 cites W2135661768 @default.
• W4381800208 cites W2289749624 @default.
• W4381800208 cites W2521629938 @default.
• W4381800208 cites W2552239989 @default.
• W4381800208 cites W2556142403 @default.
• W4381800208 cites W2558484839 @default.
• W4381800208 cites W2571160522 @default.
• W4381800208 cites W2609739496 @default.
• W4381800208 cites W2766153166 @default.
• W4381800208 cites W2790743130 @default.
• W4381800208 cites W2797346771 @default.
• W4381800208 cites W2887914971 @default.
• W4381800208 cites W2946196644 @default.
• W4381800208 cites W3045618861 @default.
• W4381800208 cites W3103049736 @default.
• W4381800208 cites W3105034819 @default.
• W4381800208 cites W3135370368 @default.
• W4381800208 cites W3200573582 @default.
• W4381800208 cites W3210051068 @default.
• W4381800208 cites W4237781224 @default.
• W4381800208 cites W4280601117 @default.
• W4381800208 doi "https://doi.org/10.1016/j.epsl.2023.118270" @default.
• W4381800208 hasPublicationYear "2023" @default.
• W4381800208 type Work @default.
• W4381800208 citedByCount "0" @default.
• W4381800208 crossrefType "journal-article" @default.
• W4381800208 hasAuthorship W4381800208A5050800567 @default.
• W4381800208 hasAuthorship W4381800208A5068791144 @default.
• W4381800208 hasBestOaLocation W43818002082 @default.
• W4381800208 hasConcept C121332964 @default.
• W4381800208 hasConcept C127313418 @default.
• W4381800208 hasConcept C13280743 @default.
• W4381800208 hasConcept C142670403 @default.
• W4381800208 hasConcept C16345878 @default.
• W4381800208 hasConcept C2524010 @default.
• W4381800208 hasConcept C2780263841 @default.
• W4381800208 hasConcept C33923547 @default.
• W4381800208 hasConcept C36293798 @default.
• W4381800208 hasConcept C46668750 @default.
• W4381800208 hasConcept C74050887 @default.
• W4381800208 hasConcept C87355193 @default.
• W4381800208 hasConceptScore W4381800208C121332964 @default.
• W4381800208 hasConceptScore W4381800208C127313418 @default.
• W4381800208 hasConceptScore W4381800208C13280743 @default.
• W4381800208 hasConceptScore W4381800208C142670403 @default.
• W4381800208 hasConceptScore W4381800208C16345878 @default.
• W4381800208 hasConceptScore W4381800208C2524010 @default.
• W4381800208 hasConceptScore W4381800208C2780263841 @default.
• W4381800208 hasConceptScore W4381800208C33923547 @default.
• W4381800208 hasConceptScore W4381800208C36293798 @default.
• W4381800208 hasConceptScore W4381800208C46668750 @default.
• W4381800208 hasConceptScore W4381800208C74050887 @default.
• W4381800208 hasConceptScore W4381800208C87355193 @default.
• W4381800208 hasFunder F4320321006 @default.
• W4381800208 hasLocation W43818002081 @default.
• W4381800208 hasLocation W43818002082 @default.
• W4381800208 hasLocation W43818002083 @default.
• W4381800208 hasOpenAccess W4381800208 @default.
• W4381800208 hasPrimaryLocation W43818002081 @default.
• W4381800208 hasRelatedWork W1495970509 @default.
• W4381800208 hasRelatedWork W1846807394 @default.
• W4381800208 hasRelatedWork W1856072836 @default.
• W4381800208 hasRelatedWork W1973379844 @default.
• W4381800208 hasRelatedWork W2024499421 @default.
• W4381800208 hasRelatedWork W2090833431 @default.
• W4381800208 hasRelatedWork W2162377856 @default.
• W4381800208 hasRelatedWork W2244279624 @default.
• W4381800208 hasRelatedWork W2334095446 @default.
• W4381800208 hasRelatedWork W3112673879 @default.
• W4381800208 hasVolume "617" @default.
• W4381800208 isParatext "false" @default.
• W4381800208 isRetracted "false" @default.
• W4381800208 workType "article" @default.