A globally fragmented and mobile lithosphere on Venus. [PDF]
Proc Natl Acad Sci U S A, 2021 Byrne PK +5 more
europepmc +1 more source
Distribution of water phase near the poles of the Moon from gravity aspects. [PDF]
Sci Rep, 2022 Kletetschka G +5 more
europepmc +1 more source
Monte Carlo computer simulations of Venus equilibrium and global resurfacing models [PDF]
Two models have been proposed for the resurfacing history of Venus: (1) equilibrium resurfacing and (2) global resurfacing. The equilibrium model consists of two cases: in case 1, areas less than or equal to 0.03 percent of the planet are spatially ...
Dawson, D. D. +2 more
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Geochemistry and mineral chemistry of pelitic gneiss of Ikare area, southwestern Nigeria. [PDF]
Heliyon, 2021 Oziegbe EJ +3 more
europepmc +1 more source
Elemental abundances of major elements in the solar wind as measured in Genesis targets and implications on solar wind fractionation. [PDF]
Astrophys J, 2021 Heber VS +7 more
europepmc +1 more source
Reconstructing landscape evolution in the Lower Khuzestan plain (SW Iran): integrating imagery, historical and sedimentary archives [PDF]
, 2010 During the late Holocene, an avulsion-controlled Karun megafan developed in the Lower Khuzestan plain. Based on the interpretation of satellite data, at least three different Karun channels were detected.
Heyvaert, Vanessa +2 more
core +1 more source
Enriched Basaltic Andesites from Mid-crustal Fractional Crystallization, Recharge, and Assimilation (Pilavo Volcano, Western Cordillera of Ecuador) [PDF]
, 2017 The origin of andesite is an important issue in petrology because andesite is the main eruptive product at convergent margins, corresponds to the average crustal composition and is often associated with major Cu-Au mineralization.
Beate, Bernardo +2 more
core
Compositions and Interior Structures of the Large Moons of Uranus and Implications for Future Spacecraft Observations. [PDF]
J Geophys Res Planets, 2023 Castillo-Rogez J +7 more
europepmc +1 more source
The Case against Mercury as the Angrite Parent Body (APB) [PDF]
, 2007 Angrites are not plausibly from Mercury based on their high FeO contents and ancient ages (e.g., [1]). Rather, the early crystallization ages of angrites argues for a small asteroidal-sized parent body for these meteorites (e.g., [2]).
Hutson, M. L. +2 more
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The thermosphere and ionosphere of Venus [PDF]
Our knowledge of the upper atmosphere and ionosphere of Venus and its interaction with the solar wind has advanced dramatically over the last decade, largely due to the data obtained during the Pioneer Venus mission and to the theoretical work that was ...
Cravens, T. E.
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