1998
DOI: 10.1029/97je02815
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The lunar mascons revisited

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Cited by 60 publications
(54 citation statements)
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“…Units in Mare Serenitatis estimated to be younger than 3.0 byr have been identified (Boyce, 1976) and some may be as young as 2.44 byr (Hiesinger et al:, 2001). The total thickness of the basalt sequence in Serenitatis and other mascon maria is estimated to be 2 4 km or as much as 3-6 km (Sjogren et al, 1974;Head, 1979, 1980;Arkani-Hamed, 1998;Williams and Zuber, 1998). Thus, the present surface of Mare Serenitatis reflects a long period of volcanism, subsidence, and deformation.…”
Section: Discussionmentioning
confidence: 96%
“…Units in Mare Serenitatis estimated to be younger than 3.0 byr have been identified (Boyce, 1976) and some may be as young as 2.44 byr (Hiesinger et al:, 2001). The total thickness of the basalt sequence in Serenitatis and other mascon maria is estimated to be 2 4 km or as much as 3-6 km (Sjogren et al, 1974;Head, 1979, 1980;Arkani-Hamed, 1998;Williams and Zuber, 1998). Thus, the present surface of Mare Serenitatis reflects a long period of volcanism, subsidence, and deformation.…”
Section: Discussionmentioning
confidence: 96%
“…Several processes have been proposed to explain the formation and support mechanism of lunar mascons (10,15). After a giant impact, according to one scenario, the extensive excavation of lunar material resulted in crater relaxation, a strong thermal anomaly, and high amounts of stress within the crust (16 ).…”
mentioning
confidence: 99%
“…The spatial agreement between two data sets can be evaluated using spherical harmonic coefficients by computing the degree correlation measure (Arkani-Hamed, 1998;Tapley et al, 2004a) following Eq. (5):…”
Section: Evaluating Spatial Agreement In the Spherical Harmonics Of Tmentioning
confidence: 99%