Volcanism and tectonism across the inner solar system: an overview
Volcanism and tectonism across the inner solar system: an overview
复制标题
DOI:
10.1144/sp401.22
复制
发表时间:
2014-09
期刊:
影响因子:
--
通讯作者:
T. Platz;T. Platz;Paul K. Byrne;Paul K. Byrne;Matteo Massironi;Harald Hiesinger
中科院分区:
文献类型:
--
作者:
T. Platz;T. Platz;Paul K. Byrne;Paul K. Byrne;Matteo Massironi;Harald Hiesinger
Abstract Volcanism and tectonism are the dominant endogenic means by which planetary surfaces change. This book, in general, and this overview, in particular, aim to encompass the broad range in character of volcanism, tectonism, faulting and associated interactions observed on planetary bodies across the inner solar system – a region that includes Mercury, Venus, Earth, the Moon, Mars and asteroids. The diversity and breadth of landforms produced by volcanic and tectonic processes are enormous, and vary across the inventory of inner solar system bodies. As a result, the selection of prevailing landforms and their underlying formational processes that are described and highlighted in this review are but a primer to the expansive field of planetary volcanism and tectonism. In addition to this extended introductory contribution, this Special Publication features 21 dedicated research articles about volcanic and tectonic processes manifest across the inner solar system. Those articles are summarized at the end of this review.