Clarification about Earth's Precession

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Discussion Overview

The discussion revolves around the concept of Earth's precession, specifically addressing the calculations and relationships between various angular momentum vectors and torques. Participants explore the mathematical formulation of precession, the angles involved, and the implications of their assumptions.

Discussion Character

  • Technical explanation
  • Debate/contested
  • Mathematical reasoning

Main Points Raised

  • One participant presents a calculation involving torques and angular momentum, questioning the correctness of their approach and the resulting expressions for precession frequency.
  • Another participant suggests that the angle between the angular momentum vector (L) and the precession vector (Ω_p) may be 90 degrees, rather than the angle θ, proposing that a visual representation could clarify the situation.
  • A different participant clarifies that θ is the angle between the Earth's rotation axis and the direction it would have if it were not tilted, contributing to the discussion on the angles involved.
  • Another participant agrees that Ω_p is likely perpendicular to the rotation vector (ω_rot), but emphasizes that the direction of Ω_p varies while its magnitude remains constant, suggesting that the sine function should be retained in calculations.
  • One participant expresses confusion about the perpendicularity of Ω_p to ω_rot and references an external image to support their inquiry.
  • A later reply acknowledges a potential error in their previous understanding, referencing an external source that aligns with the original formula presented, which indicates that the frequency of precession depends on cos(θ) rather than sin(2θ).

Areas of Agreement / Disagreement

Participants express differing views on the relationships between the vectors involved in precession, particularly regarding the angles and the correctness of the formulas. The discussion remains unresolved as participants explore various interpretations and calculations.

Contextual Notes

Participants note potential mistakes in their calculations and assumptions, particularly regarding the angles and the relationships between the vectors involved in precession. Some mathematical steps and definitions remain unclear or contested.

bznm
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I haven't a textbook where I can study Earth Precession and I'm not sure to have correctly understood... Could you tell me if I do mistakes?

I consider two points P and Q on the equatorial bulge. The torques of the gravitation forces between P-sun and Q-sun (calculated wrt the Earth center) are not equal and opposite, so I have a ##\tau_{tot} \neq 0## that generates ##\Delta L## (##\tau=dL/dt##).

##\vec{\tau_{tot}}=\vec{\tau_p}-\vec{\tau_q}=\vec{R}\times\vec{F_p}-\vec{R}\times\vec{F_q}=\vec{R}\times\vec{\Delta F}##

##\Delta F=\displaystyle \frac{4G mMR^2 cos \theta}{a^3}##

so ##\tau_{tot}=\displaystyle \frac{4G mMR^2 cos \theta}{a^3} Rsin \theta##

but ##\tau_{tot}=\displaystyle\vec{\Omega_p}\times{L}=\Omega_p L sin \theta## . From this last relations, I obtain:

##\displaystyle \frac{4G mMR^2 cos \theta}{a^3} Rsin \theta=\Omega_p L sin \theta## -> ##\Omega_p=\displaystyle\frac{4GmMR^2 cos \theta}{a^3 I \omega_{rot} }##

Is it correct? My colleague wrote on his blocknotes ##|\Omega_p||L|=|\tau_{tot}|## so ##\Omega_p=\frac{2GmMR^2 sin2 \theta}{a^3 I \omega_{rot} }##
 
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Hello

I'm not sure, but maybe it's that the angle between L and Ω_p is 90deg, and not θ. Drawing the vectors may help.

Greetings
 
Mmmmh. ##\theta## is the angle between the Earth rotation axis and the Earth direction axis that we would have if the Earth wasn't "crooked"...
 
Hello

I'm not completely sure, but if nobody answers... I think that the Ω_p is always perpendicular to the ω_{rot}; the tricky point here is to see that the direction of Ω_p is not constant, but its module is (ie, the frequency of precession is constant).

So the angle between Ω_p and L would be 90deg, and not theta, and you will keep the sin(theta) in the cross product, in order to get 2sin(theta)cos(theta) = sin(2theta), as your classmate. I still think that a drawing is useful (I'm not native English speaker, and it would be easier also for me ;) ).

Another point: I think there is another mistake in the second equation; maybe it's just R not R squared (magically it desappears in the next steps ;) ).

Greetings! :D
 
The setting should be this:
XkJeU7U.jpg


I can't understand the reason why ##\Omega_p## should be perpendicular to ##w_r##.. see also

http://oceanworld.tamu.edu/students/iceage/images/precession_1.jpg
 
Hello

After thinking carefully, it's pretty probable I were wrong.

I found a very complete explanation about this problem:

http://astro.cornell.edu/academics/courses/astro6570/Precession_Free_and_Forced.pdf

In the page 7/19 it's shown the same formula that you proposed, the frequency of precession depends on cos(theta), and not on sin(2*theta).

Thank you for making me think in this issue ;)

Greetings
 

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