subject predicate object context
44535 Creator 1c5c32b11b5ad1bd9c846a77784abc38
44535 Creator 5f42b242ffdb697d629c938841756fa1
44535 Creator 949c668bc3ce6d8779d2003a89cbb493
44535 Creator d0e13faff99f34ededfccfae0494fc52
44535 Date 2015-12-01
44535 Is Part Of repository
44535 Is Part Of p580c713c60793f14842d2873adb1a57a
44535 abstract Vents and deposits attributed to explosive volcanism occur within numerous impact craters on both the Moon and Mercury. Given the similarities between the two bodies it is probable that similar processes control this spatial association on both. However, the precise morphology and localization of the activity differs on the two bodies, indicating that the nature of structures beneath impact craters and/or volcanic activity may also be different. To explore this, we analyze sites of explosive volcanism within complex impact craters on the Moon and Mercury, comparing the scale and localization of volcanic activity and evidence for post-formation modification of the host crater. We show that the scale of vents and deposits is consistently greater on Mercury than on the Moon, indicating greater eruption energy, powered by a higher concentration of volatiles. Additionally, while the floors of lunar craters hosting explosive volcanism are commonly fractured, those on Mercury are not. The most probable explanation for these differences is that the state of regional compression acting on Mercury's crust through most of the planet's history results in deeper magma storage beneath craters on Mercury than on the Moon. The probable role of the regional stress regime in dictating the depth of intrusion on Mercury suggests that it may also play a role in the depth of sub-crater intrusion on the Moon and on other planetary bodies. Examples on the Moon (and also on Mars) commonly occur at locations where flexural extension may facilitate shallower intrusion than would be driven by the buoyancy of the magma alone.
44535 authorList authors
44535 status peerReviewed
44535 uri http://data.open.ac.uk/oro/document/358490
44535 uri http://data.open.ac.uk/oro/document/358495
44535 uri http://data.open.ac.uk/oro/document/358496
44535 uri http://data.open.ac.uk/oro/document/358497
44535 uri http://data.open.ac.uk/oro/document/358498
44535 uri http://data.open.ac.uk/oro/document/358499
44535 uri http://data.open.ac.uk/oro/document/358890
44535 volume 431
44535 type AcademicArticle
44535 type Article
44535 label Thomas, Rebecca J. ; Rothery, David A. ; Conway, Susan J. and Anand, Mahesh (2015). Explosive volcanism in complex impact craters on Mercury and the Moon: influence of tectonic regime on depth of magmatic intrusion. Earth and Planetary Science Letters, 431 pp. 164–172.
44535 label Thomas, Rebecca J. ; Rothery, David A. ; Conway, Susan J. and Anand, Mahesh (2015). Explosive volcanism in complex impact craters on Mercury and the Moon: influence of tectonic regime on depth of magmatic intrusion. Earth and Planetary Science Letters, 431 pp. 164–172.
44535 Title Explosive volcanism in complex impact craters on Mercury and the Moon: influence of tectonic regime on depth of magmatic intrusion
44535 in dataset oro