FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2004427377> ?p ?o ?g. }

• W2004427377 endingPage "77" @default.
• W2004427377 startingPage "70" @default.
• W2004427377 abstract "The interiors of the lunar south circumpolar craters Haworth, Shoemaker, Faustini, and Shackleton contain permanently shadowed regions (PSRs) and have been interpreted to contain sequestered volatiles including water ice. Altimetry data from the Lunar Orbiter Laser Altimeter (LOLA) onboard the Lunar Reconnaissance Orbiter provide a new means of examining the permanently shadowed interiors of these craters in unprecedented detail. In this study, we used extremely high-resolution gridded LOLA data of Haworth, Shoemaker, Faustini, and Shackleton to determine the size–frequency distributions and the spatial density of craters superposing their rims, inner slopes, and floors. Based on their population of superposed D ⩾ 2 km craters, Haworth, Shoemaker, and Faustini have pre-Nectarian formation ages. Shackleton is interpreted as having a Late Imbrian age on the basis of craters with diameter D ⩾ 0.5 km superposed on its rim. The local density of craters with sub-km diameters across our study area is strongly dependent on slope; because of its steep interior slopes, the lifetime of craters on the interior of Shackleton is limited. The slope-dependence of the small crater population implies that the population in this size range is controlled primarily by the rate at which craters are destroyed. This is consistent with the hypothesis that crater removal and resurfacing is a result of slope-dependent processes such as diffusive mass wasting and seismic shaking, linked to micrometeorite and meteorite bombardment. Epithermal neutron flux data and UV albedo data show that these circumpolar PSRs, particularly Shoemaker, may have ∼1–2% water ice by mass in their highly porous surface regolith, and that Shoemaker may have ∼5% or more water ice by mass in the near subsurface. The ancient formation ages of Shoemaker, Faustini and Haworth, and the Late Imbrian (∼3.5 Ga) crater retention ages of their floors suggests that any water ice that might have been deposited in their permanently shadowed areas was insufficient to modify the superposed crater population since that time." @default.
• W2004427377 created "2016-06-24" @default.
• W2004427377 creator A5018571347 @default.
• W2004427377 creator A5023264421 @default.
• W2004427377 creator A5047333821 @default.
• W2004427377 creator A5068314771 @default.
• W2004427377 creator A5073881201 @default.
• W2004427377 creator A5075400563 @default.
• W2004427377 creator A5077690822 @default.
• W2004427377 creator A5089257012 @default.
• W2004427377 date "2015-07-01" @default.
• W2004427377 modified "2023-10-17" @default.
• W2004427377 title "The age of lunar south circumpolar craters Haworth, Shoemaker, Faustini, and Shackleton: Implications for regional geology, surface processes, and volatile sequestration" @default.
• W2004427377 cites W1655452824 @default.
• W2004427377 cites W1841347802 @default.
• W2004427377 cites W1891287366 @default.
• W2004427377 cites W1915441942 @default.
• W2004427377 cites W1975640118 @default.
• W2004427377 cites W1979129737 @default.
• W2004427377 cites W1998899726 @default.
• W2004427377 cites W2008515095 @default.
• W2004427377 cites W2009777753 @default.
• W2004427377 cites W2017380441 @default.
• W2004427377 cites W2018463199 @default.
• W2004427377 cites W2037460055 @default.
• W2004427377 cites W2066776771 @default.
• W2004427377 cites W2085741319 @default.
• W2004427377 cites W2087807155 @default.
• W2004427377 cites W2148345729 @default.
• W2004427377 cites W2161264942 @default.
• W2004427377 cites W2163101776 @default.
• W2004427377 cites W2171032696 @default.
• W2004427377 cites W4230969046 @default.
• W2004427377 doi "https://doi.org/10.1016/j.icarus.2015.03.016" @default.
• W2004427377 hasPublicationYear "2015" @default.
• W2004427377 type Work @default.
• W2004427377 sameAs 2004427377 @default.
• W2004427377 citedByCount "30" @default.
• W2004427377 countsByYear W20044273772016 @default.
• W2004427377 countsByYear W20044273772017 @default.
• W2004427377 countsByYear W20044273772018 @default.
• W2004427377 countsByYear W20044273772019 @default.
• W2004427377 countsByYear W20044273772020 @default.
• W2004427377 countsByYear W20044273772021 @default.
• W2004427377 countsByYear W20044273772022 @default.
• W2004427377 countsByYear W20044273772023 @default.
• W2004427377 crossrefType "journal-article" @default.
• W2004427377 hasAuthorship W2004427377A5018571347 @default.
• W2004427377 hasAuthorship W2004427377A5023264421 @default.
• W2004427377 hasAuthorship W2004427377A5047333821 @default.
• W2004427377 hasAuthorship W2004427377A5068314771 @default.
• W2004427377 hasAuthorship W2004427377A5073881201 @default.
• W2004427377 hasAuthorship W2004427377A5075400563 @default.
• W2004427377 hasAuthorship W2004427377A5077690822 @default.
• W2004427377 hasAuthorship W2004427377A5089257012 @default.
• W2004427377 hasConcept C111368507 @default.
• W2004427377 hasConcept C114793014 @default.
• W2004427377 hasConcept C121332964 @default.
• W2004427377 hasConcept C127313418 @default.
• W2004427377 hasConcept C1276947 @default.
• W2004427377 hasConcept C13280743 @default.
• W2004427377 hasConcept C142362112 @default.
• W2004427377 hasConcept C144024400 @default.
• W2004427377 hasConcept C149923435 @default.
• W2004427377 hasConcept C17534553 @default.
• W2004427377 hasConcept C179537507 @default.
• W2004427377 hasConcept C186295008 @default.
• W2004427377 hasConcept C195886398 @default.
• W2004427377 hasConcept C2776481522 @default.
• W2004427377 hasConcept C2908647359 @default.
• W2004427377 hasConcept C38458734 @default.
• W2004427377 hasConcept C38935664 @default.
• W2004427377 hasConcept C52119013 @default.
• W2004427377 hasConcept C554144382 @default.
• W2004427377 hasConcept C87355193 @default.
• W2004427377 hasConceptScore W2004427377C111368507 @default.
• W2004427377 hasConceptScore W2004427377C114793014 @default.
• W2004427377 hasConceptScore W2004427377C121332964 @default.
• W2004427377 hasConceptScore W2004427377C127313418 @default.
• W2004427377 hasConceptScore W2004427377C1276947 @default.
• W2004427377 hasConceptScore W2004427377C13280743 @default.
• W2004427377 hasConceptScore W2004427377C142362112 @default.
• W2004427377 hasConceptScore W2004427377C144024400 @default.
• W2004427377 hasConceptScore W2004427377C149923435 @default.
• W2004427377 hasConceptScore W2004427377C17534553 @default.
• W2004427377 hasConceptScore W2004427377C179537507 @default.
• W2004427377 hasConceptScore W2004427377C186295008 @default.
• W2004427377 hasConceptScore W2004427377C195886398 @default.
• W2004427377 hasConceptScore W2004427377C2776481522 @default.
• W2004427377 hasConceptScore W2004427377C2908647359 @default.
• W2004427377 hasConceptScore W2004427377C38458734 @default.
• W2004427377 hasConceptScore W2004427377C38935664 @default.
• W2004427377 hasConceptScore W2004427377C52119013 @default.
• W2004427377 hasConceptScore W2004427377C554144382 @default.
• W2004427377 hasConceptScore W2004427377C87355193 @default.
• W2004427377 hasLocation W20044273771 @default.
• W2004427377 hasOpenAccess W2004427377 @default.
• W2004427377 hasPrimaryLocation W20044273771 @default.

• next