Geodynamo, solar wind, and magnetopause 3.4 to 3.45 billion years ago

  • John A. Tarduno
  • , Rory D. Cottrell
  • , Michael K. Watkeys
  • , Axel Hofmann
  • , Pavel V. Doubrovine
  • , Eric E. Mamajek
  • , Dunji Liu
  • , David G. Sibeck
  • , Levi P. Neukirch
  • , Yoichi Usui

Research output: Contribution to journalArticlepeer-review

285 Citations (Scopus)

Abstract

Stellar wind standoff by a planetary magnetic field prevents atmospheric erosion and water loss. Although the early Earth retained its water and atmosphere, and thus evolved as a habitable planet, little is known about Earth's magnetic field strength during that time. We report paleointensity results from single silicate crystals bearing magnetic inclusions that record a geodynamo 3.4 to 3.45 billion years ago. The measured field strength is -50 to 70% that of the present-day field. When combined with a greater Paleoarchean solar wind pressure, the paleofield strength data suggest steady-state magnetopause standoff distances of ≤5 Earth radii, similar to values observed during recent coronal mass ejection events. The data also suggest lower-latitude aurora and increases in polar cap area, as well as heating, expansion, and volatile loss from the exosphere that would have affected long-term atmospheric composition.

Original languageEnglish
Pages (from-to)1238-1240
Number of pages3
JournalScience
Volume327
Issue number5970
DOIs
Publication statusPublished - 5 Mar 2010
Externally publishedYes

ASJC Scopus subject areas

  • Multidisciplinary

Fingerprint

Dive into the research topics of 'Geodynamo, solar wind, and magnetopause 3.4 to 3.45 billion years ago'. Together they form a unique fingerprint.

Cite this