Discussion Overview
The discussion revolves around the potential effects of Faraday braking due to the solar wind on Earth's orbit around the Sun. Participants explore the implications of conductive plasma ejected by the Sun and its interaction with Earth's magnetic field, as well as various forces acting on Earth in its orbital dynamics.
Discussion Character
- Exploratory
- Technical explanation
- Debate/contested
- Mathematical reasoning
Main Points Raised
- One participant suggests that the braking effect observed when a magnet falls through a conductive tube could similarly apply to Earth as it orbits the Sun, potentially causing it to fall closer to the Sun due to the conductive plasma ejected by the Sun.
- Another participant questions the comparison of the conductivity of solar plasma to copper, implying that this comparison is crucial to understanding the braking effect.
- A participant outlines various forces affecting Earth's orbit, including gravitational wave resistance, tidal forces due to the Sun's rotation, and the impact of solar wind drag, suggesting these forces could influence Earth's orbital dynamics.
- One participant reiterates the request for numeric estimates of the small drag components mentioned in the previous post.
- Another participant acknowledges the conductivity of solar wind, suggesting it could have a significant effect on Earth's orbit, but notes that the mass of the solar wind would need to be considerably greater for it to have a substantial influence.
- A later reply encourages estimating the effect of solar wind on Earth's orbit by calculating the force exerted on Earth's magnetic field based on the solar wind's charge density and velocity.
Areas of Agreement / Disagreement
Participants express differing views on the significance of solar wind and its conductivity, as well as the various forces acting on Earth. There is no consensus on the overall impact of these factors on Earth's orbit.
Contextual Notes
Participants have not reached a consensus on the numerical estimates of the forces discussed, and assumptions regarding the conductivity of solar plasma compared to copper remain unaddressed.