2012
DOI: 10.2322/tastj.10.tk_41
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Structure of the South Pole-Aitken Basin from KAGUYA Selenodesy Data

Abstract: The South Pole-Aitken basin (SPA) is the largest (2500km in diameter), deepest and presumably oldest impact basin in the solar system. SPA was characterized by an ellipse with axes 2400 by 2050 km, but more precise topography and gravity data are necessary to discuss the structure of large basin like SPA. We use localized representation of gravity potential where Slepian functions were used to estimate the gravity field over certain areas of the Moon and a spherical cap area with a radius of 40 degree from the… Show more

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Cited by 2 publications
(5 citation statements)
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“…This depression could correspond to the “possible fourth ring” described by Hiesinger and Head [] for the SPA basin; however, in their study it was tracked only partially. The central depression is smaller than the previously suggested area (1250 × 1150 km) [ Sasaki et al , ], based on its lower elevation and thinner crust, and it is shifted slightly northward compared to the lowest elevation (Figures a and ). However, the current lowest elevation may not need to correspond completely to a geologic structure, because the topography changes with relaxation and melt cooling after basin formation.…”
Section: Mineralogy Of the Spa Interior And Its Correlation With Toposupporting
confidence: 67%
“…This depression could correspond to the “possible fourth ring” described by Hiesinger and Head [] for the SPA basin; however, in their study it was tracked only partially. The central depression is smaller than the previously suggested area (1250 × 1150 km) [ Sasaki et al , ], based on its lower elevation and thinner crust, and it is shifted slightly northward compared to the lowest elevation (Figures a and ). However, the current lowest elevation may not need to correspond completely to a geologic structure, because the topography changes with relaxation and melt cooling after basin formation.…”
Section: Mineralogy Of the Spa Interior And Its Correlation With Toposupporting
confidence: 67%
“…Because the melt sheet has no strength, the basin center should have a relatively flat floor with little topographic relief. This is seen in Kaguya data where the central region of the basin is at a depth of about 5 km relative to the Moon's mean radius (Sasaki et al, 2010). Beyond about half of the basin radius, the effect of impact heating is minor and would not affect the strength of the crust near the basin rim.…”
Section: Crustal Thickness and Topographymentioning
confidence: 91%
“…The gravity-derived profiles suggest the crust beneath the center of SPA has a thickness of $30-55 km, gradually thickening towards $60 km nearer the basin's edge (radial distance of $1200 km). Unlike the majority of gravity-derived crustal profiles for smaller lunar basins, SPA does not appear to possess a thickened annulus of crust around its basin rim (see Wieczorek and Phillips, 1999;Hikida and Wieczorek, 2007;Sasaki et al, 2010Sasaki et al, , 2011. By comparison to the gravity-derived profiles, our steepest LTG (50 K/km) therefore appears to best fit the gravity data, as the other, shallower, LTGs all produced a prominent thickened annulus.…”
Section: Final Crater Structurementioning
confidence: 95%
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