| Literature DB >> 25953822 |
Catherine L Johnson1, Roger J Phillips2, Michael E Purucker3, Brian J Anderson4, Paul K Byrne5, Brett W Denevi4, Joshua M Feinberg6, Steven A Hauck7, James W Head8, Haje Korth4, Peter B James9, Erwan Mazarico3, Gregory A Neumann3, Lydia C Philpott10, Matthew A Siegler11, Nikolai A Tsyganenko12, Sean C Solomon13.
Abstract
Magnetized rocks can record the history of the magnetic field of a planet, a key constraint for understanding its evolution. From orbital vector magnetic field measurements of Mercury taken by the MErcury Surface, Space ENvironment, GEochemistry, and Ranging (MESSENGER) spacecraft at altitudes below 150 kilometers, we have detected remanent magnetization in Mercury's crust. We infer a lower bound on the average age of magnetization of 3.7 to 3.9 billion years. Our findings indicate that a global magnetic field driven by dynamo processes in the fluid outer core operated early in Mercury's history. Ancient field strengths that range from those similar to Mercury's present dipole field to Earth-like values are consistent with the magnetic field observations and with the low iron content of Mercury's crust inferred from MESSENGER elemental composition data.Entities:
Year: 2015 PMID: 25953822 DOI: 10.1126/science.aaa8720
Source DB: PubMed Journal: Science ISSN: 0036-8075 Impact factor: 47.728