Detecting the oldest geodynamo and attendant shielding from the solar wind: Implications for habitability
John A. Tarduno, Eric G. Blackman, Eric E. Mamajek

TL;DR
This paper reviews evidence of Earth's earliest magnetic field, its implications for atmospheric retention and habitability, and discusses methods to constrain ancient geomagnetic and solar wind conditions, focusing on the Paleoarchean era.
Contribution
It proposes new pathways to estimate early solar wind pressure and geomagnetic field strength, enhancing understanding of Earth's early interior and atmospheric evolution.
Findings
Geodynamo existed during Paleoarchean (3.4-3.45 billion years ago).
Solar wind pressure was similar to modern extreme solar storms.
Magnetic shielding influenced atmospheric retention and habitability.
Abstract
The onset and nature of the earliest geomagnetic field is important for understanding the evolution of the core, atmosphere and life on Earth. A record of the early geodynamo is preserved in ancient silicate crystals containing minute magnetic inclusions. These data indicate the presence of a geodynamo during the Paleoarchean, between 3.4 and 3.45 billion years ago. While the magnetic field sheltered Earth's atmosphere from erosion at this time, standoff of the solar wind was greatly reduced, and similar to that during modern extreme solar storms. These conditions suggest that intense radiation from the young Sun may have modified the atmosphere of the young Earth by promoting loss of volatiles, including water. Such effects would have been more pronounced if the field were absent or very weak prior to 3.45 billion years ago, as suggested by some models of lower mantle evolution. The…
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