Ferrovolcanism: Iron Volcanism on Metallic Asteroids. Issue 10 (16th May 2019)

• Record Type: Journal Article
• Authors: Abrahams, Jacob N. H.; Nimmo, Francis
• Is Part Of: Geophysical research letters. Volume 46:Issue 10(2019)
• Page Start: 5055
• Page End: 5064
• Publication Date: 2019-05-16
• Subjects: iron volcanism -- ferrovolcanism -- metallic asteroid -- Psyche; Geophysics -- Periodicals; Planets -- Periodicals; Lunar geology -- Periodicals; 550
• DOI: 10.1029/2019GL082542
• Languages: English
• ISSNs: 0094-8276

Abstract

Abstract: Metallic asteroids, the exposed cores of disrupted planetesimals, are expected to have been exposed while still molten. Some would have cooled from the outside in, crystallizing a surface crust which would then grow inward. Because the growing crust is expected to be more dense than the underlying melt, this melt will tend to migrate toward the surface whenever it is able. Compressional stresses produced in the crust while it cools will be relieved locally by thrust faulting, which will also provide potential conduits for melt to reach the surface. We predict iron volcanism to have occurred on metallic asteroids as they cooled and discuss the implications of this process for both the evolution and the modern appearance of these bodies. Key Points: Metallic asteroids begin fully molten, and as they solidify, their remaining melt is buoyant The primary stress state of metallic asteroid crust is compression, limiting the ability of melt at depth to reach the surface Local stress changes likely allow this compression to be overcome, and we predict metallic asteroids should host volcanic activity