Could Earth's Early Magnetic Field Have Trapped Hydrogen in the Atmosphere?

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SUMMARY

The discussion centers on the hypothesis that Earth's early magnetic field may have been strong enough to trap hydrogen in the atmosphere, influencing conditions for abiogenesis. It highlights the role of the Lorentz force in deflecting charged hydrogen ions, or protons, within the magnetic field, potentially allowing them to collide with atmospheric ions and become trapped. The conversation also touches on the significance of early mantle convection in creating local redox environments necessary for life, suggesting that a near-neutral atmosphere could facilitate organic production. The upper limit for hydrogen excess in the atmosphere is estimated to be around 0.5 billion years, influenced by hydrodynamic escape mechanisms.

PREREQUISITES
  • Understanding of Lorentz force and its effects on charged particles.
  • Knowledge of Earth's magnetic field and its historical strength.
  • Familiarity with abiogenesis and the conditions required for life emergence.
  • Concepts of mantle convection and redox reactions in geological processes.
NEXT STEPS
  • Research the role of the Lorentz force in plasma physics.
  • Explore the historical variations in Earth's magnetic field strength.
  • Investigate the relationship between mantle convection and atmospheric chemistry.
  • Study the conditions for abiogenesis in various planetary environments.
USEFUL FOR

Geophysicists, astrobiologists, and researchers interested in planetary atmospheres and the origins of life will benefit from this discussion.

daniel dahl
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could Earth's early magnetic field have been strong enough to trap hydrogen within the atmosphere?
 
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How would a magnetic field trap neutral hydrogen atoms?
 
if they were hydrogen ions emitted as solar wind
 
Hydrogen ions, let's just call them protons, have a charge and a mass. When they encounter a magnetic field they will be deflected onto a different trajectory by a Lorentz_force. http://en.wikipedia.org/wiki/Lorentz_force
As a proton spirals down the converging magnetic field lines toward a magnetic pole, it may collide with ions in the upper atmosphere and so could be slowed and trapped.There is significant coupling between the solar wind and the Earth's magnetic field.
 
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Interesting question, Daniel. Are you wondering if this could have given the early atmosphere reducing properties, a condition often thought necessary for abiogenesis?
 
Ophiolite said:
Interesting question, Daniel. Are you wondering if this could have given the early atmosphere reducing properties, a condition often thought necessary for abiogenesis?

Not any longer, since early mantle convection is now known to give local environments with the necessary redox differences. (Often around hydrothermal vents as they pass the differentiated and serpentinized minerals.) Instead a near neutral atmosphere would be conducive for life emergence, since the CO2 generates a slightly acidic ocean that contrasts to the mantle convection alkaline conditions and makes (local) organic production effective. Such conditions may seem constraining (less global organic production), but in fact increase the likelihood for life elsewhere since especially ice moons with oceans but also early cold, wet bodies like Mars have them.

Perhaps there were a slightly reducing excess due to hydrogen escape from the hot planet (and perhaps remaining and, yes, captured hydrogen). But too much of an excess and the upper atmosphere goes into hydrodynamic escape, hydrogen vents preferably. (But can remove some somewhat more massive molecules with the outflow.) I think the upper limit of hydrogen excess has been limited to 0.5 billion years from such considerations.
 

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