Measuring Rotational Speed of Io w/Doppler & Relative Velocity to Jupiter

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SUMMARY

This discussion focuses on measuring the rotational speed of Io, one of Jupiter's moons, using a spectrograph and the Doppler formula. The key method involves calculating the relative velocity of Io to Jupiter by taking the dot product of Io's velocity vector with the unit observation vector. The resulting radial velocity (v_r) is then used to determine the red or blueshift in the observed spectrum, expressed by the formula Δλ/λ = v_r/c. Proper alignment of Io's motion with the observation vector is crucial for maximizing the detected radial velocity.

PREREQUISITES
  • Understanding of the Doppler effect in spectroscopy
  • Familiarity with vector mathematics and dot products
  • Knowledge of astronomical observation techniques using spectrographs
  • Basic principles of celestial mechanics, particularly orbital dynamics
NEXT STEPS
  • Research the application of the Doppler formula in astrophysics
  • Study vector mathematics, specifically dot products and their applications
  • Explore advanced spectroscopic techniques for measuring celestial object velocities
  • Investigate the orbital dynamics of Io and its motion relative to Jupiter
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Astronomers, astrophysicists, and students studying celestial mechanics or spectroscopy who are interested in measuring the rotational dynamics of celestial bodies.

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I want to measure the rotational speed of Io using a spectrograph, using the doppler formula. Since it is rotating around Jupiter, i have to take the velocity relative to jupiter, but I wonder tough how this is possible when Io is not rotating at an right angle to my observation point. Is there some mathematical way to solve this?
 
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I want to measure the rotational speed of Io using a spectrograph, using the doppler formula. Since it is rotating around Jupiter, i have to take the velocity relative to jupiter, but I wonder tough how this is possible when Io is not rotating at an right angle to my observation point. Is there some mathematical way to solve this?

You'll want to take the dot product of Io's velocity vector with your unit observation vector (a magnitude 1 vector pointing towards Io):

[tex]v_r = \vec{v}_{total} \cdot \hat{u}[/tex]

This translates into red or blueshift in the usual way:

[tex]\frac{\Delta \lambda}{\lambda}=\frac{v_r}{c}[/tex]

Note that you'll want it to be moving parallel to your observation vector if you want a large radial velocity.
 

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